INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1666, 'Nino Panagia', 'Nino Panagia', 'Ultraviolet Observations of Supernovae', '10 pages, 5 figures - Invited talk at the \"Supernova 1987A: 20 Years\n  after: Supernovae and Gamma-Ray Bursters\" Conference, February 19-23, 2007,\n  Aspen, CO, (AIP Conf. Proc.), eds. S. Immler, R. McCray and K.W. Weiler, in\n  press. Slightly revised version that clarifies some confusing statements', 'AIP Conf.Proc.937:236-245,2007', '10.1063/1.2803569', '', 'astro-ph', '', '  The motivations to make ultraviolet (UV) studies of supernovae (SNe) are\nreviewed and discussed in the light of the results obtained so far by means of\nIUE and HST observations. It appears that UV studies of SNe can, and do lead to\nfundamental results not only for our understanding of the SN phenomenon, such\nas the kinematics and the metallicity of the ejecta, but also for exciting new\nfindings in Cosmology, such as the tantalizing evidence for \"dark energy\" that\nseems to pervade the Universe and to dominate its energetics. The need for\nadditional and more detailed UV observations is also considered and discussed.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 21:17:06 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 1 May 2007 20:38:57 GMT\"}]', '2009-06-23', '[[\"Panagia\",\"Nino\",\"\"]]'),
(704.1667, 'Erel Levine', 'Erel Levine and Terence Hwa', 'Stochastic fluctuations in metabolic pathways', '', 'PNAS 2007', '10.1073/pnas.0610987104', '', 'q-bio.MN cond-mat.stat-mech', '', '  Fluctuations in the abundance of molecules in the living cell may affect its\ngrowth and well being. For regulatory molecules (e.g., signaling proteins or\ntranscription factors), fluctuations in their expression can affect the levels\nof downstream targets in a network. Here, we develop an analytic framework to\ninvestigate the phenomenon of noise correlation in molecular networks.\nSpecifically, we focus on the metabolic network, which is highly inter-linked,\nand noise properties may constrain its structure and function. Motivated by the\nanalogy between the dynamics of a linear metabolic pathway and that of the\nexactly soluable linear queueing network or, alternatively, a mass transfer\nsystem, we derive a plethora of results concerning fluctuations in the\nabundance of intermediate metabolites in various common motifs of the metabolic\nnetwork. For all but one case examined, we find the steady-state fluctuation in\ndifferent nodes of the pathways to be effectively uncorrelated. Consequently,\nfluctuations in enzyme levels only affect local properties and do not propagate\nelsewhere into metabolic networks, and intermediate metabolites can be freely\nshared by different reactions. Our approach may be applicable to study\nmetabolic networks with more complex topologies, or protein signaling networks\nwhich are governed by similar biochemical reactions. Possible implications for\nbioinformatic analysis of metabolimic data are discussed.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 00:19:21 GMT\"}]', '2009-11-13', '[[\"Levine\",\"Erel\",\"\"],[\"Hwa\",\"Terence\",\"\"]]'),
(704.1668, 'Marco Montalto', 'M. Montalto (1), G. Piotto (1), S. Desidera (2), F. De Marchi (1), H.\n  Bruntt (3,4), P. B. Stetson (5), A. Arellano Ferro (6), Y. Momany (1,2), R.\n  G. Gratton (2), E. Poretti (7), A. Aparicio (8), M. Barbieri (2,9), R. U.\n  Claudi (2), G. Grundahl (3), A. Rosenberg (8) ((1) Dipartimento di\n  Astronomia, Universit\\`a di Padova, Italy, (2) INAF - Osservatorio\n  Astronomico di Padova, Italy, (3) Department of Physics and Astronomy,\n  Denmark, (4) University of Sydney, School of Physics, Australia, (5) Herzberg\n  Institute of Astrophysics, Canada, (6) Instituto de Astronom\\\'ia, Universidad\n  Nacional Auton\\\'oma de M\\\'exico, (7) INAF - Osservatorio Astronomico di\n  Brera, Italy, (8) Instituto de Astrofisica de Canarias, Canary Islands,\n  Spain, (9) Dipartimento di Fisica, Universit\\`a di Padova, Italy)', 'A new search for planet transits in NGC 6791', '23 pages, 23 figures, A&A accepted', '', '10.1051/0004-6361:20066199', '', 'astro-ph', '', '  Context. Searching for planets in open clusters allows us to study the\neffects of dynamical environment on planet formation and evolution.\n  Aims. Considering the strong dependence of planet frequency on stellar\nmetallicity, we studied the metal rich old open cluster NGC 6791 and searched\nfor close-in planets using the transit technique.\n  Methods. A ten-night observational campaign was performed using the\nCanada-France-Hawaii Telescope (3.6m), the San Pedro M\\\'artir telescope (2.1m),\nand the Loiano telescope (1.5m). To increase the transit detection probability\nwe also made use of the Bruntt et al. (2003) eight-nights observational\ncampaign. Adequate photometric precision for the detection of planetary\ntransits was achieved.\n  Results. Should the frequency and properties of close-in planets in NGC 6791\nbe similar to those orbiting field stars of similar metallicity, then detailed\nsimulations foresee the presence of 2-3 transiting planets. Instead, we do not\nconfirm the transit candidates proposed by Bruntt et al. (2003). The\nprobability that the null detection is simply due to chance coincidence is\nestimated to be 3%-10%, depending on the metallicity assumed for the cluster.\n  Conclusions. Possible explanations of the null-detection of transits include:\n(i) a lower frequency of close-in planets in star clusters; (ii) a smaller\nplanetary radius for planets orbiting super metal rich stars; or (iii)\nlimitations in the basic assumptions. More extensive photometry with 3-4m class\ntelescopes is required to allow conclusive inferences about the frequency of\nplanets in NGC 6791.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 23:07:59 GMT\"}]', '2009-11-13', '[[\"Montalto\",\"M.\",\"\"],[\"Piotto\",\"G.\",\"\"],[\"Desidera\",\"S.\",\"\"],[\"De Marchi\",\"F.\",\"\"],[\"Bruntt\",\"H.\",\"\"],[\"Stetson\",\"P. B.\",\"\"],[\"Ferro\",\"A. Arellano\",\"\"],[\"Momany\",\"Y.\",\"\"],[\"Gratton\",\"R. G.\",\"\"],[\"Poretti\",\"E.\",\"\"],[\"Aparicio\",\"A.\",\"\"],[\"Barbieri\",\"M.\",\"\"],[\"Claudi\",\"R. U.\",\"\"],[\"Grundahl\",\"G.\",\"\"],[\"Rosenberg\",\"A.\",\"\"]]'),
(704.1669, 'D. V. Ahluwalia-Khalilova', 'D. V. Ahluwalia-Khalilova, N. G. Gresnigt, Alex B. Nielsen, D.\n  Schritt, T. F. Watson (University of Canterbury, New Zealand)', 'Possible polarisation and spin dependent aspects of quantum gravity', 'Awarded an \"honourable mention\" in the 2007 Gravity Research\n  Foundation Essay Competition', 'Int.J.Mod.Phys.D17:495-504,2008', '10.1142/S0218271808012164', '', 'gr-qc astro-ph hep-ph', '', '  We argue that quantum gravity theories that carry a Lie algebraic\nmodification of the Poincare\' and Heisenberg algebras inevitably provide\ninhomogeneities that may serve as seeds for cosmological structure formation.\nFurthermore, in this class of theories one must expect a strong polarisation\nand spin dependence of various quantum-gravity effects.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 22:14:44 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 8 Jun 2007 03:00:27 GMT\"}]', '2008-11-26', '[[\"Ahluwalia-Khalilova\",\"D. V.\",\"\",\"University of Canterbury, New Zealand\"],[\"Gresnigt\",\"N. G.\",\"\",\"University of Canterbury, New Zealand\"],[\"Nielsen\",\"Alex B.\",\"\",\"University of Canterbury, New Zealand\"],[\"Schritt\",\"D.\",\"\",\"University of Canterbury, New Zealand\"],[\"Watson\",\"T. F.\",\"\",\"University of Canterbury, New Zealand\"]]'),
(704.1670, 'Mehmet Firat Arikan', 'Mehmet Firat Arikan', 'On the support genus of a contact structure', '20 pages, 13 figures, title shorthened, minor corrections', 'J. Gokova Geom. Topol. GGT 1 (2007)', '', '', 'math.GT math.SG', '', '  The algorithm given by Akbulut-Ozbagci constructs an explicit open book\ndecomposition on a contact three-manifold described by a contact surgery on a\nlink in the three-sphere. In this article, we will improve this algorithm by\nusing Giroux\'s contact cell decomposition process. Our algorithm is more\neconomical on choosing the supporting genus of the open book; in particular it\ngives a good upper bound for the recently defined ``minimal supporting genus\ninvariant\'\' of contact structures.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 22:20:54 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 14 Apr 2007 22:59:31 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 29 May 2007 19:27:28 GMT\"},{\"version\":\"v4\",\"created\":\"Thu, 8 Nov 2007 18:57:20 GMT\"}]', '2018-03-23', '[[\"Arikan\",\"Mehmet Firat\",\"\"]]'),
(704.1671, 'Mark Dijkstra', 'Mark Dijkstra, Stuart Wyithe (Melbourne)', 'Very Massive Stars in High-Redshift Galaxies', '11 pages, 7 figures, MNRAS in press, comments by referee included,\n  references added+updated', 'Mon.Not.Roy.Astron.Soc.379:1589-1598,2007', '10.1111/j.1365-2966.2007.12039.x', '', 'astro-ph', '', '  A significant fraction of Lyman Alpha (Lya) emitting galaxies (LAEs) at z>\n5.7 have rest-frame equivalent widths (EW) greater than ~100 Angstrom. However\nonly a small fraction of the Lya flux produced by a galaxy is transmitted\nthrough the IGM, which implies intrinsic Lya EWs that are in excess of the\nmaximum allowed for a population-II stellar population having a Salpeter mass\nfunction. In this paper we study characteristics of the sources powering Lya\nemission in high redshift galaxies. We propose a simple model for Lya emitters\nin which galaxies undergo a burst of very massive star formation that results\nin a large intrinsic EW, followed by a phase of population-II star formation\nwith a lower EW. We confront this model with a range of high redshift\nobservations and find that the model is able to simultaneously describe the\nfollowing eight properties of the high redshift galaxy population with\nplausible values for parameters like the efficiency and duration of star\nformation: i-iv) the UV and Lya luminosity functions of LAEs at z=5.7 and 6.5,\nv-vi) the mean and variance of the EW distribution of Lya selected galaxies at\nz=5.7, vii) the EW distribution of i-drop galaxies at z~6, and viii) the\nobserved correlation of stellar age with EW. Our modeling suggests that the\nobserved anomalously large intrinsic equivalent widths require a burst of very\nmassive star formation lasting no more than a few to ten percent of the\ngalaxies star forming lifetime. This very massive star formation may indicate\nthe presence of population-III star formation in a few per cent of i-drop\ngalaxies, and in about half of the Lya selected galaxies.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 22:43:30 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 27 Jun 2007 11:02:38 GMT\"}]', '2009-06-23', '[[\"Dijkstra\",\"Mark\",\"\",\"Melbourne\"],[\"Wyithe\",\"Stuart\",\"\",\"Melbourne\"]]'),
(704.1672, 'Ilia Solov\'yov', 'Ilia A. Solov\'yov, Alexander V. Yakubovich, Andrey V. Solov\'yov and\n  Walter Greiner', 'Two center multipole expansion method: application to macromolecular\n  systems', '23 pages, 7 figures, 1 table', '', '10.1103/PhysRevE.75.051912', '', 'physics.bio-ph physics.comp-ph', '', '  We propose a new theoretical method for the calculation of the interaction\nenergy between macromolecular systems at large distances. The method provides a\nlinear scaling of the computing time with the system size and is considered as\nan alternative to the well known fast multipole method. Its efficiency,\naccuracy and applicability to macromolecular systems is analyzed and discussed\nin detail.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 22:07:56 GMT\"}]', '2009-11-13', '[[\"Solov\'yov\",\"Ilia A.\",\"\"],[\"Yakubovich\",\"Alexander V.\",\"\"],[\"Solov\'yov\",\"Andrey V.\",\"\"],[\"Greiner\",\"Walter\",\"\"]]'),
(704.1673, 'C. Robin Graham', 'C. Robin Graham and Andreas Juhl', 'Holographic formula for Q-curvature', '13 pages', '', '', '', 'math.DG', '', '  This paper derives an explicit formula for Branson\'s Q-curvature in\neven-dimensional conformal geometry. The ingredients in the formula come from\nthe Poincare metric in one higher dimension; hence the formula is called\nholographic. When specialized to the conformally flat case, the holographic\nformula expresses Q-curvature as a multiple of the Pfaffian and the divergence\nof a natural one-form. The paper also outlines the relation between holographic\nformulae for Q-curvature and a new theory of conformally covariant families of\ndifferential operators due to the second author.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:06:19 GMT\"}]', '2007-05-23', '[[\"Graham\",\"C. Robin\",\"\"],[\"Juhl\",\"Andreas\",\"\"]]'),
(704.1674, 'Thomas A. Trainor', 'Thomas A. Trainor and David T. Kettler', 'The azimuth structure of nuclear collisions -- I', '27 pages, 12 figures', 'Int.J.Mod.Phys.E17:1219-1272,2008', '10.1142/S0218301308010465', '', 'hep-ph', '', '  We describe azimuth structure commonly associated with elliptic and directed\nflow in the context of 2D angular autocorrelations for the purpose of precise\nseparation of so-called nonflow (mainly minijets) from flow. We extend the\nFourier-transform description of azimuth structure to include power spectra and\nautocorrelations related by the Wiener-Khintchine theorem. We analyze several\nexamples of conventional flow analysis in that context and question the\nrelevance of reaction plane estimation to flow analysis. We introduce the 2D\nangular autocorrelation with examples from data analysis and describe a\nsimulation exercise which demonstrates precise separation of flow and nonflow\nusing the 2D autocorrelation method. We show that an alternative correlation\nmeasure based on Pearson\'s normalized covariance provides a more intuitive\nmeasure of azimuth structure.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 23:08:44 GMT\"}]', '2008-11-26', '[[\"Trainor\",\"Thomas A.\",\"\"],[\"Kettler\",\"David T.\",\"\"]]'),
(704.1675, 'Kristina Lerman', 'Anon Plangprasopchok and Kristina Lerman', 'Exploiting Social Annotation for Automatic Resource Discovery', '6 pages, submitted to AAAI07 workshop on Information Integration on\n  the Web', '', '', '', 'cs.AI cs.CY cs.DL', '', '  Information integration applications, such as mediators or mashups, that\nrequire access to information resources currently rely on users manually\ndiscovering and integrating them in the application. Manual resource discovery\nis a slow process, requiring the user to sift through results obtained via\nkeyword-based search. Although search methods have advanced to include evidence\nfrom document contents, its metadata and the contents and link structure of the\nreferring pages, they still do not adequately cover information sources --\noften called ``the hidden Web\'\'-- that dynamically generate documents in\nresponse to a query. The recently popular social bookmarking sites, which allow\nusers to annotate and share metadata about various information sources, provide\nrich evidence for resource discovery. In this paper, we describe a\nprobabilistic model of the user annotation process in a social bookmarking\nsystem del.icio.us. We then use the model to automatically find resources\nrelevant to a particular information domain. Our experimental results on data\nobtained from \\emph{del.icio.us} show this approach as a promising method for\nhelping automate the resource discovery task.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 23:24:19 GMT\"}]', '2016-09-08', '[[\"Plangprasopchok\",\"Anon\",\"\"],[\"Lerman\",\"Kristina\",\"\"]]'),
(704.1676, 'Kristina Lerman', 'Kristina Lerman, Anon Plangprasopchok and Chio Wong', 'Personalizing Image Search Results on Flickr', '12 pages, submitted to AAAI07 workshop on Intelligent Information\n  Personalization', '', '', '', 'cs.IR cs.AI cs.CY cs.DL cs.HC', '', '  The social media site Flickr allows users to upload their photos, annotate\nthem with tags, submit them to groups, and also to form social networks by\nadding other users as contacts. Flickr offers multiple ways of browsing or\nsearching it. One option is tag search, which returns all images tagged with a\nspecific keyword. If the keyword is ambiguous, e.g., ``beetle\'\' could mean an\ninsect or a car, tag search results will include many images that are not\nrelevant to the sense the user had in mind when executing the query. We claim\nthat users express their photography interests through the metadata they add in\nthe form of contacts and image annotations. We show how to exploit this\nmetadata to personalize search results for the user, thereby improving search\nperformance. First, we show that we can significantly improve search precision\nby filtering tag search results by user\'s contacts or a larger social network\nthat includes those contact\'s contacts. Secondly, we describe a probabilistic\nmodel that takes advantage of tag information to discover latent topics\ncontained in the search results. The users\' interests can similarly be\ndescribed by the tags they used for annotating their images. The latent topics\nfound by the model are then used to personalize search results by finding\nimages on topics that are of interest to the user.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 23:31:04 GMT\"}]', '2007-05-23', '[[\"Lerman\",\"Kristina\",\"\"],[\"Plangprasopchok\",\"Anon\",\"\"],[\"Wong\",\"Chio\",\"\"]]'),
(704.1677, 'Daniel de Florian', 'Daniel de Florian and Werner Vogelsang', 'Resummed Cross Section for Jet Production at Hadron Colliders', '10 figures included', 'Phys.Rev.D76:074031,2007', '10.1103/PhysRevD.76.074031', 'BNL-NT-07/17', 'hep-ph', '', '  We study the resummation of large logarithmic perturbative corrections to the\nsingle-inclusive jet cross section at hadron colliders. The corrections we\naddress arise near the threshold for the partonic reaction, when the incoming\npartons have just enough energy to produce the high-transverse-momentum final\nstate. The structure of the resulting logarithmic corrections is known to\ndepend crucially on the treatment of the invariant mass of the produced jet at\nthreshold. We allow the jet to have a non-vanishing mass at threshold, which\nmost closely corresponds to the situation in experiment. Matching our results\nto available semi-analytical next-to-leading-order calculations, we derive\nresummed results valid to next-to-leading logarithmic accuracy. We present\nnumerical results for the resummation effects at Tevatron and RHIC energies.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 23:40:21 GMT\"}]', '2008-11-26', '[[\"de Florian\",\"Daniel\",\"\"],[\"Vogelsang\",\"Werner\",\"\"]]'),
(704.1678, 'Shanghua Teng', 'Xi Chen, Xiaotie Deng, Shang-Hua Teng', 'Settling the Complexity of Computing Two-Player Nash Equilibria', '53 pages 2 figures', '', '', '', 'cs.GT cs.CC', '', '  We settle a long-standing open question in algorithmic game theory. We prove\nthat Bimatrix, the problem of finding a Nash equilibrium in a two-player game,\nis complete for the complexity class PPAD Polynomial Parity Argument, Directed\nversion) introduced by Papadimitriou in 1991.\n  This is the first of a series of results concerning the complexity of Nash\nequilibria. In particular, we prove the following theorems:\n  Bimatrix does not have a fully polynomial-time approximation scheme unless\nevery problem in PPAD is solvable in polynomial time. The smoothed complexity\nof the classic Lemke-Howson algorithm and, in fact, of any algorithm for\nBimatrix is not polynomial unless every problem in PPAD is solvable in\nrandomized polynomial time. Our results demonstrate that, even in the simplest\nform of non-cooperative games, equilibrium computation and approximation are\npolynomial-time equivalent to fixed point computation. Our results also have\ntwo broad complexity implications in mathematical economics and operations\nresearch: Arrow-Debreu market equilibria are PPAD-hard to compute. The P-Matrix\nLinear Complementary Problem is computationally harder than convex programming\nunless every problem in PPAD is solvable in polynomial time.\n', '[{\"version\":\"v1\",\"created\":\"Thu, 12 Apr 2007 23:54:30 GMT\"}]', '2007-05-23', '[[\"Chen\",\"Xi\",\"\"],[\"Deng\",\"Xiaotie\",\"\"],[\"Teng\",\"Shang-Hua\",\"\"]]'),
(704.1679, 'Andrea Mignone', 'A. Mignone and Jonathan C. McKinney', 'Equation of State in Relativistic Magnetohydrodynamics: variable versus\n  constant adiabatic index', '14 pages, 14 figures', 'Mon.Not.Roy.Astron.Soc.378:1118-1130,2007', '10.1111/j.1365-2966.2007.11849.x', '', 'astro-ph', '', '  The role of the equation of state for a perfectly conducting, relativistic\nmagnetized fluid is the main subject of this work. The ideal constant\n$\\Gamma$-law equation of state, commonly adopted in a wide range of\nastrophysical applications, is compared with a more realistic equation of state\nthat better approximates the single-specie relativistic gas. The paper focus on\nthree different topics. First, the influence of a more realistic equation of\nstate on the propagation of fast magneto-sonic shocks is investigated. This\ncalls into question the validity of the constant $\\Gamma$-law equation of state\nin problems where the temperature of the gas substantially changes across\nhydromagnetic waves. Second, we present a new inversion scheme to recover\nprimitive variables (such as rest-mass density and pressure) from conservative\nones that allows for a general equation of state and avoids catastrophic\nnumerical cancellations in the non-relativistic and ultrarelativistic limits.\nFinally, selected numerical tests of astrophysical relevance (including\nmagnetized accretion flows around Kerr black holes) are compared using\ndifferent equations of state. Our main conclusion is that the choice of a\nrealistic equation of state can considerably bear upon the solution when\ntransitions from cold to hot gas (or viceversa) are present. Under these\ncircumstances, a polytropic equation of state can significantly endanger the\nsolution.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 00:33:18 GMT\"}]', '2009-06-23', '[[\"Mignone\",\"A.\",\"\"],[\"McKinney\",\"Jonathan C.\",\"\"]]'),
(704.1680, 'Roderick Melnik', 'N. Sinha, D. Roy Mahapatra, J.T.W. Yeow, R.V.N. Melnik, D.A. Jaffray', 'Carbon Nanotube Thin Film Field Emitting Diode: Understanding the System\n  Response Based on Multiphysics Modeling', '40 pages, 13 figures; keywords: field emission, carbon nanotubes,\n  degradation, electrodynamics, self-assembly', 'Carbon nanotube thin film fSinha, N., Mahapatra, D.R., Yeow,\n  J.T.W., Melnik, R.V.N. and Jaffray, D.A., Journal of Computational and\n  Theoretical Nanoscience, 4, 1--15, 2007', '', '', 'cond-mat.mtrl-sci cond-mat.mes-hall', '', '  In this paper, we model the evolution and self-assembly of randomly oriented\ncarbon nanotubes (CNTs), grown on a metallic substrate in the form of a thin\nfilm for field emission under diode configuration. Despite high output, the\ncurrent in such a thin film device often decays drastically. The present paper\nis focused on understanding this problem. A systematic, multiphysics based\nmodelling approach is proposed. First, a nucleation coupled model for\ndegradation of the CNT thin film is derived, where the CNTs are assumed to\ndecay by fragmentation and formation of clusters. The random orientation of the\nCNTs and the electromechanical interaction are then modeled to explain the\nself-assembly. The degraded state of the CNTs and the electromechanical force\nare employed to update the orientation of the CNTs. Field emission current at\nthe device scale is finally obtained by using the Fowler-Nordheim equation and\nintegration over the computational cell surfaces on the anode side. The\nsimulated results are in close agreement with the experimental results. Based\non the developed model, numerical simulations aimed at understanding the\neffects of various geometric parameters and their statistical features on the\ndevice current history are reported.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 00:55:09 GMT\"}]', '2010-04-14', '[[\"Sinha\",\"N.\",\"\"],[\"Mahapatra\",\"D. Roy\",\"\"],[\"Yeow\",\"J. T. W.\",\"\"],[\"Melnik\",\"R. V. N.\",\"\"],[\"Jaffray\",\"D. A.\",\"\"]]'),
(704.1681, 'Joan Najita', 'Joan R. Najita, Stephen E. Strom, and James Muzerolle', 'Demographics of Transition Objects', '11 pages, 4 figures, to appear in MNRAS', 'Mon.Not.Roy.Astron.Soc.378:369-378,2007', '10.1111/j.1365-2966.2007.11793.x', '', 'astro-ph', '', '  The unusual properties of transition objects (young stars with an optically\nthin inner disc surrounded by an optically thick outer disc) suggest that\nsignificant disc evolution has occured in these systems. We explore the nature\nof these systems by examining their demographics, specifically their stellar\naccretion rates (Mdot) and disc masses (Mdisc) compared to those of accreting T\nTauri stars of comparable age. We find that transition objects in Taurus occupy\na restricted region of the Mdot vs. Mdisc plane. Compared to non-transition\nsingle stars in Taurus, they have stellar accretion rates that are typically\n~10 times lower at the same disc mass and median disc masses ~4 times larger.\nThese properties are anticipated by several proposed planet formation theories\nand suggest that the formation of Jovian mass planets may play a significant\nrole in explaining the origin of at least some transition objects. Considering\ntransition objects as a distinct demographic group among accreting T Tauri\nstars leads to a tighter relationship between disc masses and stellar accretion\nrates, with a slope between the two quantities that is close to the value of\nunity expected in simple theories of disc accretion.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 01:06:43 GMT\"}]', '2009-06-23', '[[\"Najita\",\"Joan R.\",\"\"],[\"Strom\",\"Stephen E.\",\"\"],[\"Muzerolle\",\"James\",\"\"]]'),
(704.1682, 'Roderick Melnik', 'N. Sinha, D. Roy Mahapatra, J.T.W. Yeow, R.V.N. Melnik', 'Modeling the Field Emission Current Fluctuation in Carbon Nanotube Thin\n  Films', '4 pages, 5 figures', '', '', '', 'cond-mat.mtrl-sci cond-mat.mes-hall', '', '  Owing to their distinct properties, carbon nanotubes (CNTs) have emerged as\npromising candidate for field emission devices. It has been found\nexperimentally that the results related to the field emission performance show\nvariability. The design of an efficient field emitting device requires the\nanalysis of the variabilities with a systematic and multiphysics based modeling\napproach. In this paper, we develop a model of randomly oriented CNTs in a thin\nfilm by coupling the field emission phenomena, the electron-phonon transport\nand the mechanics of single isolated CNT. A computational scheme is developed\nby which the states of CNTs are updated in time incremental manner. The device\ncurrent is calculated by using Fowler-Nordheim equation for field emission to\nstudy the performance at the device scale.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 01:09:19 GMT\"}]', '2009-09-29', '[[\"Sinha\",\"N.\",\"\"],[\"Mahapatra\",\"D. Roy\",\"\"],[\"Yeow\",\"J. T. W.\",\"\"],[\"Melnik\",\"R. V. N.\",\"\"]]'),
(704.1683, 'Nurulla Azamov', 'Nurulla Azamov, Fyodor Sukochev', 'Spectral averaging for trace compatible operators', '10 pages, LaTeX; a gap in the proof of Proposition 2.4 has been fixed', '', '', '', 'math.FA math.SP', '', '  In this note the notions of trace compatible operators and infinitesimal\nspectral flow are introduced. We define the spectral shift function as the\nintegral of infinitesimal spectral flow. It is proved that the spectral shift\nfunction thus defined is absolutely continuous and Krein\'s formula is\nestablished. Some examples of trace compatible affine spaces of operators are\ngiven.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 01:20:10 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 25 May 2007 02:36:18 GMT\"}]', '2007-06-13', '[[\"Azamov\",\"Nurulla\",\"\"],[\"Sukochev\",\"Fyodor\",\"\"]]'),
(704.1684, 'Steven Longmore N', 'S. N. Longmore (1 and 2), M. G. Burton (1), P. J. Barnes (3 and 1), T.\n  Wong (1 and 2 and 5), C. R. Purcell (1 and 4), J. Ott (2 and 6) ((1) UNSW,\n  (2) ATNF, (3) University of Sydney, (4) Jodrell Bank Observatory,\n  (5)University of Illinois, (6) NRAO)', 'The molecular environment of massive star forming cores associated with\n  Class II methanol maser emission', '5 pages, 1 figure, IAU Symposium 242 Conference Proceedings', '', '10.1017/S1743921307012677', '', 'astro-ph', '', '  Methanol maser emission has proven to be an excellent signpost of regions\nundergoing massive star formation (MSF). To investigate their role as an\nevolutionary tracer, we have recently completed a large observing program with\nthe ATCA to derive the dynamical and physical properties of molecular/ionised\ngas towards a sample of MSF regions traced by 6.7 GHz methanol maser emission.\nWe find that the molecular gas in many of these regions breaks up into multiple\nsub-clumps which we separate into groups based on their association\nwith/without methanol maser and cm continuum emission. The temperature and\ndynamic state of the molecular gas is markedly different between the groups.\nBased on these differences, we attempt to assess the evolutionary state of the\ncores in the groups and thus investigate the role of class II methanol masers\nas a tracer of MSF.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 01:26:29 GMT\"}]', '2009-11-13', '[[\"Longmore\",\"S. N.\",\"\",\"1 and 2\"],[\"Burton\",\"M. G.\",\"\",\"3 and 1\"],[\"Barnes\",\"P. J.\",\"\",\"3 and 1\"],[\"Wong\",\"T.\",\"\",\"1 and 2 and 5\"],[\"Purcell\",\"C. R.\",\"\",\"1 and 4\"],[\"Ott\",\"J.\",\"\",\"2 and 6\"]]'),
(704.1685, 'Xin-Zhou Li', 'Xing-hua Jin, Xin-zhou Li and Dao-jun Liu', 'Gravitating Global k-monopole', '9 pages, 2 figures, references added, typos corrected, accepted by\n  Class. Quantum Grav', 'Class.Quant.Grav.24:2773-2780,2007', '10.1088/0264-9381/24/11/001', '', 'gr-qc', '', '  A gravitating global k-monopole produces a tiny gravitational field outside\nthe core in addition to a solid angular deficit in the k-field theory. As a new\nfeature, the gravitational field can be attractive or repulsive depending on\nthe non-canonical kinetic term.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 01:48:38 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 18 Apr 2007 03:18:19 GMT\"}]', '2008-11-26', '[[\"Jin\",\"Xing-hua\",\"\"],[\"Li\",\"Xin-zhou\",\"\"],[\"Liu\",\"Dao-jun\",\"\"]]'),
(704.1686, 'Levente Horvath Dr', 'L. Horvath and H. J. Carmichael', 'Effect of atomic beam alignment on photon correlation measurements in\n  cavity QED', '15 pages and 13 figures', 'Phys. Rev. A 76, 043821 (2007)', '10.1103/PhysRevA.76.043821', '', 'quant-ph', '', '  Quantum trajectory simulations of a cavity QED system comprising an atomic\nbeam traversing a standing-wave cavity are carried out. The delayed photon\ncoincident rate for forwards scattering is computed and compared with the\nmeasurements of Rempe et al. [Phys. Rev. Lett. 67, 1727 (1991)] and Foster et\nal. [Phys. Rev. A 61, 053821 (2000)]. It is shown that a moderate atomic beam\nmisalignment can account for the degradation of the predicted correlation. Fits\nto the experimental data are made in the weak-field limit with a single\nadjustable parameter--the atomic beam tilt from perpendicular to the cavity\naxis. Departures of the measurement conditions from the weak-field limit are\ndiscussed.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 02:54:37 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 8 Nov 2007 00:38:38 GMT\"}]', '2007-11-08', '[[\"Horvath\",\"L.\",\"\"],[\"Carmichael\",\"H. J.\",\"\"]]'),
(704.1687, 'Juefei Zhou', 'Juefei Zhou, Urszula B. Szafruga, David S. Watkins and Mark G. Kuzyk', 'Studies on optimizing potential energy functions for maximal intrinsic\n  hyperpolarizability', '9 pages, 9 figures', '', '10.1103/PhysRevA.76.053831', '', 'physics.optics physics.chem-ph', '', '  We use numerical optimization to study the properties of (1) the class of\none-dimensional potential energy functions and (2) systems of point charges in\ntwo-dimensions that yield the largest hyperpolarizabilities, which we find to\nbe within 30% of the fundamental limit. We investigate the character of the\npotential energy functions and resulting wavefunctions and find that a broad\nrange of potentials yield the same intrinsic hyperpolarizability ceiling of\n0.709.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 03:01:54 GMT\"}]', '2009-11-13', '[[\"Zhou\",\"Juefei\",\"\"],[\"Szafruga\",\"Urszula B.\",\"\"],[\"Watkins\",\"David S.\",\"\"],[\"Kuzyk\",\"Mark G.\",\"\"]]'),
(704.1688, 'Masaki Kobayashi', 'M. Kobayashi, K. Tanaka, A. Fujimori, Sugata Ray, D. D. Sarma', 'Critical test for Altshuler-Aronov theory: Evolution of the density of\n  states singularity in double perovskite Sr$_2$FeMoO$_6$ with controlled\n  disorder', '5 pages, 4 figures', 'Phys. Rev. Lett. 98, 246401 (2007)', '10.1103/PhysRevLett.98.246401', '', 'cond-mat.mtrl-sci cond-mat.str-el', '', '  With high-resolution photoemission spectroscopy measurements, the density of\nstates (DOS) near the Fermi level ($E_\\mathrm{F}$) of double perovskite\nSr$_2$FeMoO$_6$ having different degrees of Fe/Mo antisite disorder has been\ninvestigated with varying temperature. The DOS near $E_\\mathrm{F}$ showed a\nsystematic depletion with increasing degree of disorder, and recovered with\nincreasing temperature. Altshuler-Aronov (AA) theory of disordered metals well\nexplains the dependences of the experimental results. Scaling analysis of the\nspectra provides experimental indication for the functional form of the AA DOS\nsingularity.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 03:10:20 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Apr 2007 01:41:11 GMT\"}]', '2007-07-07', '[[\"Kobayashi\",\"M.\",\"\"],[\"Tanaka\",\"K.\",\"\"],[\"Fujimori\",\"A.\",\"\"],[\"Ray\",\"Sugata\",\"\"],[\"Sarma\",\"D. D.\",\"\"]]'),
(704.1689, 'Wenhua Zhao', 'Wenhua Zhao', 'Some Properties of and Open Problems on Hessian Nilpotent Polynomials', 'Latex, 33 pages. Some misprints have been corrected; English and also\n  terminology for some newly defined notion have been improved. To appear in\n  Annales Polonici Mathematici', 'Ann. Polon. Math. 93 (2008), no. 2, 135--162.', '', '', 'math.CV math.AG', '', '  In the recent progress [BE1], [M], [Z1] and [Z2], the well-known Jacobian\nconjecture ([BCW], [E]) has been reduced to a problem on HN (Hessian nilpotent)\npolynomials (the polynomials whose Hessian matrix are nilpotent) and their\n(deformed) inversion pairs. In this paper, we prove several results on HN\npolynomials, their (deformed) inversion pairs as well as the associated\nsymmetric polynomial or formal maps. We also propose some open problems for\nfurther study of these objects.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 04:02:09 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 25 Feb 2008 02:27:36 GMT\"}]', '2009-02-02', '[[\"Zhao\",\"Wenhua\",\"\"]]'),
(704.1690, 'Wenhua Zhao', 'Arno van den Essen and Wenhua Zhao', 'Two Results on Homogeneous Hessian Nilpotent Polynomials', 'Latex, 7 pages', 'J. Pure Appl. Algebra, 212 (2008), no. 10, 2190--2193.', '', '', 'math.AG math.CV', '', '  Let $z=(z_1, ..., z_n)$ and $\\Delta=\\sum_{i=1}^n \\frac {\\partial^2}{\\partial\nz^2_i}$ the Laplace operator. A formal power series $P(z)$ is said to be {\\it\nHessian Nilpotent}(HN) if its Hessian matrix $\\Hes P(z)=(\\frac {\\partial^2\nP}{\\partial z_i\\partial z_j})$ is nilpotent. In recent developments in [BE1],\n[M] and [Z], the Jacobian conjecture has been reduced to the following\nso-called {\\it vanishing conjecture}(VC) of HN polynomials: {\\it for any\nhomogeneous HN polynomial $P(z)$ $($of degree $d=4$$)$, we have $\\Delta^m\nP^{m+1}(z)=0$ for any $m>>0$.} In this paper, we first show that, the VC holds\nfor any homogeneous HN polynomial $P(z)$ provided that the projective\nsubvarieties ${\\mathcal Z}_P$ and ${\\mathcal Z}_{\\sigma_2}$ of $\\mathbb C\nP^{n-1}$ determined by the principal ideals generated by $P(z)$ and\n$\\sigma_2(z):=\\sum_{i=1}^n z_i^2$, respectively, intersect only at regular\npoints of ${\\mathcal Z}_P$. Consequently, the Jacobian conjecture holds for the\nsymmetric polynomial maps $F=z-\\nabla P$ with $P(z)$ HN if $F$ has no non-zero\nfixed point $w\\in \\mathbb C^n$ with $\\sum_{i=1}^n w_i^2=0$. Secondly, we show\nthat the VC holds for a HN formal power series $P(z)$ if and only if, for any\npolynomial $f(z)$, $\\Delta^m (f(z)P(z)^m)=0$ when $m>>0$.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 03:15:59 GMT\"}]', '2009-02-02', '[[\"Essen\",\"Arno van den\",\"\"],[\"Zhao\",\"Wenhua\",\"\"]]'),
(704.1691, 'Wenhua Zhao', 'Wenhua Zhao', 'A Vanishing Conjecture on Differential Operators with Constant\n  Coefficients', 'Latex, 32 pages. Following the referee, some minor improvements have\n  been done. Appeared in the proceeding of the joint international conference\n  \"Polynomial Automorphisms and related topics\" (Hanoi, Vietnam, 2006) of the\n  Institute of Mathematics, Hanoi, Vietnam, and the Adus Salam International\n  Centreof Theoretical Physics (ICTP), Trieste, Italy', 'Acta Mathematica Vietnamica, vol 32 (2007), no. 3, 107--134.', '', '', 'math.CV math.AG', '', '  In the recent progress [BE1], [Me] and [Z2], the well-known JC (Jacobian\nconjecture) ([BCW], [E]) has been reduced to a VC (vanishing conjecture) on the\nLaplace operators and HN (Hessian nilpotent) polynomials (the polynomials whose\nHessian matrix are nilpotent). In this paper, we first show that the vanishing\nconjecture above, hence also the JC, is equivalent to a vanishing conjecture\nfor all 2nd order homogeneous differential operators $\\Lambda$ and\n$\\Lambda$-nilpotent polynomials $P$ (the polynomials $P(z)$ satisfying\n$\\Lambda^m P^m=0$ for all $m\\ge 1$). We then transform some results in the\nliterature on the JC, HN polynomials and the VC of the Laplace operators to\ncertain results on $\\Lambda$-nilpotent polynomials and the associated VC for\n2nd order homogeneous differential operators $\\Lambda$. This part of the paper\ncan also be read as a short survey on HN polynomials and the associated VC in\nthe more general setting. Finally, we discuss a still-to-be-understood\nconnection of $\\Lambda$-nilpotent polynomials in general with the classical\northogonal polynomials in one or more variables. This connection provides a\nconceptual understanding for the isotropic properties of homogeneous\n$\\Lambda$-nilpotent polynomials for the 2nd order homogeneous full rank\ndifferential operators $\\Lambda$ with constant coefficients.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 04:08:11 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 28 Oct 2007 22:57:26 GMT\"}]', '2009-02-02', '[[\"Zhao\",\"Wenhua\",\"\"]]'),
(704.1692, 'Lujun Fang', 'Zhongzhi Zhang, Lujun Fang, Shuigeng Zhou, and Jihong Guan', 'Effects of accelerating growth on the evolution of weighted complex\n  networks', 'Final version accepted for publication in Physica A', 'Physica A, 2009, 388:225-232.', '10.1016/j.physa.2008.10.008', '', 'physics.soc-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Many real systems possess accelerating statistics where the total number of\nedges grows faster than the network size. In this paper, we propose a simple\nweighted network model with accelerating growth. We derive analytical\nexpressions for the evolutions and distributions for strength, degree, and\nweight, which are relevant to accelerating growth. We also find that\naccelerating growth determines the clustering coefficient of the networks.\nInterestingly, the distributions for strength, degree, and weight display a\ntransition from scale-free to exponential form when the parameter with respect\nto accelerating growth increases from a small to large value. All the\ntheoretical predictions are successfully contrasted with extensive numerical\nsimulations.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:54:19 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 1 Oct 2008 13:08:06 GMT\"}]', '2008-11-20', '[[\"Zhang\",\"Zhongzhi\",\"\"],[\"Fang\",\"Lujun\",\"\"],[\"Zhou\",\"Shuigeng\",\"\"],[\"Guan\",\"Jihong\",\"\"]]'),
(704.1693, 'Dongwoo Cha', 'Jin-Hee Yoon, Eunja Ha, and Dongwoo Cha', 'N_p N_n Scheme Based on New Empirical Formula for Excitation Energy', '11 pages, 7 figures', 'J.Phys.G34:2545-2552,2007', '10.1088/0954-3899/34/12/002', '', 'nucl-th', '', '  We examine the $N_p N_n$ scheme based on a recently proposed simple empirical\nformula which is highly valid for the excitation energy of the first excited\nnatural parity even multipole states in even-even nuclei. We demonstrate\nexplicitly that the $N_p N_n$ scheme for the excitation energy emerges from the\nseparate exponential dependence of the excitation energy on the valence nucleon\nnumbers $N_p$ and $N_n$ together with the fact that only a limited set of\nnumbers is allowed for the $N_p$ and $N_n$ of the existing nuclei.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 03:26:41 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 12 Sep 2007 15:11:09 GMT\"}]', '2008-11-26', '[[\"Yoon\",\"Jin-Hee\",\"\"],[\"Ha\",\"Eunja\",\"\"],[\"Cha\",\"Dongwoo\",\"\"]]'),
(704.1694, 'Sergey Yekhanin', 'Kiran S. Kedlaya, Sergey Yekhanin', 'Locally Decodable Codes From Nice Subsets of Finite Fields and Prime\n  Factors of Mersenne Numbers', '18 pages', '', '', '', 'cs.CC math.NT', '', '  A k-query Locally Decodable Code (LDC) encodes an n-bit message x as an N-bit\ncodeword C(x), such that one can probabilistically recover any bit x_i of the\nmessage by querying only k bits of the codeword C(x), even after some constant\nfraction of codeword bits has been corrupted. The major goal of LDC related\nresearch is to establish the optimal trade-off between length and query\ncomplexity of such codes.\n  Recently [Y] introduced a novel technique for constructing locally decodable\ncodes and vastly improved the upper bounds for code length. The technique is\nbased on Mersenne primes. In this paper we extend the work of [Y] and argue\nthat further progress via these methods is tied to progress on an old number\ntheory question regarding the size of the largest prime factors of Mersenne\nnumbers.\n  Specifically, we show that every Mersenne number m=2^t-1 that has a prime\nfactor p>m^\\gamma yields a family of k(\\gamma)-query locally decodable codes of\nlength Exp(n^{1/t}). Conversely, if for some fixed k and all \\epsilon > 0 one\ncan use the technique of [Y] to obtain a family of k-query LDCs of length\nExp(n^\\epsilon); then infinitely many Mersenne numbers have prime factors arger\nthan known currently.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 04:18:19 GMT\"}]', '2007-05-23', '[[\"Kedlaya\",\"Kiran S.\",\"\"],[\"Yekhanin\",\"Sergey\",\"\"]]'),
(704.1695, 'Todd M. Tinsley', 'Duane A. Dicus, Wayne W. Repko, and Todd M. Tinsley', 'Pair production with neutrinos in an intense background magnetic field', '20 pages, 12 figures', 'Phys.Rev.D76:025005,2007; Erratum-ibid.D76:089903,2007', '10.1103/PhysRevD.76.025005 10.1103/PhysRevD.76.089903', '', 'hep-ph astro-ph', '', '  We present a detailed calculation of the electron-positron production rate\nusing neutrinos in an intense background magnetic field. The computation is\ndone for the process nu -> nu e- e+ (where nu can be nu_e, nu_mu, or nu_tau)\nwithin the framework of the Standard Model. Results are given for various\ncombinations of Landau-levels over a range of possible incoming neutrino\nenergies and magnetic field strengths.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 13:54:38 GMT\"}]', '2014-11-18', '[[\"Dicus\",\"Duane A.\",\"\"],[\"Repko\",\"Wayne W.\",\"\"],[\"Tinsley\",\"Todd M.\",\"\"]]'),
(704.1696, 'Marie Cottrell', 'Marie Cottrell (SAMOS, Matisse), Jean-Claude Fort (SAMOS, Matisse,\n  Iecn), Gilles Pag\\`es (PMA)', 'Theoretical Aspects of the SOM Algorithm', '', 'Neurocomputing 21 (1998) 119-138', '', '', 'math.ST stat.TH', '', '  The SOM algorithm is very astonishing. On the one hand, it is very simple to\nwrite down and to simulate, its practical properties are clear and easy to\nobserve. But, on the other hand, its theoretical properties still remain\nwithout proof in the general case, despite the great efforts of several\nauthors. In this paper, we pass in review the last results and provide some\nconjectures for the future work.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 04:52:39 GMT\"}]', '2007-05-23', '[[\"Cottrell\",\"Marie\",\"\",\"SAMOS, Matisse\"],[\"Fort\",\"Jean-Claude\",\"\",\"SAMOS, Matisse,\\n  Iecn\"],[\"Pagès\",\"Gilles\",\"\",\"PMA\"]]'),
(704.1697, 'Stanislav Pavlov', 'L. I. Korovin, I. G. Lang, S. T. Pavlov', 'Effect of the Spatial Dispersion on the Shape of a Light Pulse in a\n  Quantum Well', '7 pages, 5 figures', '', '10.1134/S1063783407100290', '', 'cond-mat.mes-hall', '', '  Reflectance, transmittance and absorbance of a symmetric light pulse, the\ncarrying frequency of which is close to the frequency of interband transitions\nin a quantum well, are calculated. Energy levels of the quantum well are\nassumed discrete, and two closely located excited levels are taken into\naccount. A wide quantum well (the width of which is comparable to the length of\nthe light wave, corresponding to the pulse carrying frequency) is considered,\nand the dependance of the interband matrix element of the momentum operator on\nthe light wave vector is taken into account. Refractive indices of barriers and\nquantum well are assumed equal each other. The problem is solved for an\narbitrary ratio of radiative and nonradiative lifetimes of electronic\nexcitations. It is shown that the spatial dispersion essentially affects the\nshapes of reflected and transmitted pulses. The largest changes occur when the\nradiative broadening is close to the difference of frequencies of interband\ntransitions taken into account.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 04:59:02 GMT\"}]', '2009-11-13', '[[\"Korovin\",\"L. I.\",\"\"],[\"Lang\",\"I. G.\",\"\"],[\"Pavlov\",\"S. T.\",\"\"]]'),
(704.1698, 'Yoshinori Okada', 'Y. Okada, T. Takeuchi, T. Baba, S. Shin, H. Ikuta', 'The origin of the anomalously strong influence of out-of-plane disorder\n  on high-Tc superconductivity', '4 pages, 4 figures', 'Jounal of Phys. Soc. Japan 77 074714 (2008)', '10.1143/JPSJ.77.074714', '', 'cond-mat.supr-con cond-mat.str-el', '', '  The electronic structure of Bi2Sr2-xRxCuOy(R=La, Eu) near the (pi,0) point of\nthe first Brillouin zone was studied by means of angle-resolved photoemission\nspectroscopy (ARPES). The temperature T* above which the pseudogap structure in\nthe ARPES spectrum disappears was found to have an R dependence that is\nopposite to that ofthe superconducting transition temperature Tc. This\nindicates that the pseudogap state is competing with high-Tc superconductivity,\nand the large Tc suppression observed with increasing the out-of-plane disorder\nis due to the stabilization of the pseudogap state.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:04:40 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 20 Dec 2007 09:39:13 GMT\"}]', '2011-05-27', '[[\"Okada\",\"Y.\",\"\"],[\"Takeuchi\",\"T.\",\"\"],[\"Baba\",\"T.\",\"\"],[\"Shin\",\"S.\",\"\"],[\"Ikuta\",\"H.\",\"\"]]'),
(704.1699, 'Tetsufumi Hirano', 'Tetsufumi Hirano', 'Relativistic Hydrodynamics at RHIC and LHC', '8 pages, 7 figures, talk given at YKIS Seminar on New Frontiers in\n  QCD', 'Prog.Theor.Phys.Suppl.168:347-354,2007', '10.1143/PTPS.168.347', 'TKYNT-07-09', 'nucl-th hep-ph nucl-ex', '', '  Recent development of a hydrodynamic model is discussed by putting an\nemphasis on realistic treatment of the early and late stages in relativistic\nheavy ion collisions. The model, which incorporates a hydrodynamic description\nof the quark-gluon plasma with a kinetic approach of hadron cascades, is\napplied to analysis of elliptic flow data at the Relativistic Heavy Ion\nCollider energy. It is predicted that the elliptic flow parameter based on the\nhybrid model increases with the collision energy up to the Large Hadron\nCollider energy.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 05:13:32 GMT\"}]', '2008-11-26', '[[\"Hirano\",\"Tetsufumi\",\"\"]]'),
(704.1700, 'Ming-chang Kang Professor', 'Ming-chang Kang', 'Retract rationality and Noether\'s problem', '', '', '', '', 'math.AC math.RA', '', '  Let K be any field and G be a finite group. We will prove that, if K is any\nfield, p an odd prime number, and G is a non-abelian group of exponent p with\n|G|=p^3 or p^4 satisfying [K(\\zeta_p):K] <= 2, then K(G) is rational over K. We\nwill also show that K(G) is retract rational if G belongs to a much larger\nclass of p-groups. In particular, generic G-polynomials of G-Galois extensions\nexist for these groups.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 05:30:01 GMT\"}]', '2007-05-23', '[[\"Kang\",\"Ming-chang\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1701, 'Ming-chang Kang Professor', 'Ming-chang Kang and Shou-Jen Hu', 'Noether\'s problem for some p-groups', '', '', '', '', 'math.AC math.RA', '', '  Let K be any field and G be a finite group. Noether\'s problem asks whether\nthe fixed field is rational (=purely transcendental) over K. We will prove that\nif G is a non-abelian p-group of order p^n containing a cyclic subgroup of\nindex p and K is any field containing a primitive p^{n-2}-th root of unity,\nthen K(G) is rational over K.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 05:39:45 GMT\"}]', '2007-05-23', '[[\"Kang\",\"Ming-chang\",\"\"],[\"Hu\",\"Shou-Jen\",\"\"]]'),
(704.1702, 'Meng Chen', 'Jungkai A. Chen, Meng Chen', 'The canonical volume of threefolds of general type with $\\chi<1$', '16 pages, Updated version, To appear in Journal of LMS', '', '', '', 'math.AG', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We prove that the canonical volume $K^3\\geq {1/30}$ for all projective\n3-folds of general type with $\\chi(\\mathcal{O})\\leq 0$. This bound is sharp.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 06:36:15 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 26 Jun 2008 12:48:11 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 27 Jun 2008 04:46:33 GMT\"}]', '2008-06-27', '[[\"Chen\",\"Jungkai A.\",\"\"],[\"Chen\",\"Meng\",\"\"]]'),
(704.1703, 'Troy Porter', 'T. A. Porter, I. V. Moskalenko, and A. W. Strong', 'Very High Energy Gamma Rays from Supernova Remnants and Constraints on\n  the Galactic Interstellar Radiation Field', 'To appear in the proceedings of the 1st GLAST Symposium', 'AIPConf.Proc.921:411-412,2007', '10.1063/1.2757377', 'SLAC-PUB-12466', 'astro-ph', '', '  The large-scale Galactic interstellar radiation field (ISRF) is the result of\nstellar emission and dust re-processing of starlight. Where the energy density\nof the ISRF is high (e.g., the Galactic Centre), the dominant gamma-ray\nemission in individual supernova remnants (SNRs), such as G0.9+0.1, may come\nfrom inverse Compton (IC) scattering of the ISRF. Several models of the ISRF\nexist. The most recent one, which has been calculated by us, predicts a\nsignificantly higher ISRF than the well-used model of Mathis, Mezger, and\nPanagia. However,comparison with data is limited to local observations. Based\non our current estimate of the ISRF we predict the gamma-ray emission in the\nSNRs G0.9+0.1 and RXJ1713, and pair-production absorption features above 20 TeV\nin the spectra of G0.9+0.1, J1713-381, and J1634-472. We discuss how GLAST,\nalong with current and future very high energy instruments, may be able to\nprovide upper bounds on the large-scale ISRF.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:30:50 GMT\"}]', '2008-11-26', '[[\"Porter\",\"T. A.\",\"\"],[\"Moskalenko\",\"I. V.\",\"\"],[\"Strong\",\"A. W.\",\"\"]]'),
(704.1704, 'Tigran Sedrakyan', 'T. A. Sedrakyan and M. E. Raikh', 'Magneto-oscillations due to electron-electron interactions in the ac\n  conductivity of a 2D electron gas', '4+ pages, 3 figures', 'Phys. Rev. Lett. 100, 086808 (2008)', '10.1103/PhysRevLett.100.086808', '', 'cond-mat.mes-hall', '', '  Electron-electron interactions give rise to the correction,\n\\delta\\sigma^{int}(\\omega), to the ac magnetoconductivity, \\sigma(\\omega), of a\nclean 2D electron gas that is periodic in \\omega_c^{-1}, where \\omega_c is the\ncyclotron frequency. Unlike conventional harmonics of the cyclotron resonance,\nwhich are periodic with \\omega, this correction is periodic with \\omega^{3/2}.\nOscillations in \\delta\\sigma^{int}(\\omega) develop at low magnetic fields,\n\\omega_c\\ll\\omega, when the conventional harmonics are suppressed by the\ndisorder. Their origin is a {\\em double} backscattering of an electron from the\nimpurity-induced Friedel oscillations. During the time \\sim\\omega^{-1} between\nthe two backscattering events the electron travels only a {\\em small portion}\nof the Larmour circle.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:20:20 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 4 Mar 2008 23:20:04 GMT\"}]', '2008-03-05', '[[\"Sedrakyan\",\"T. A.\",\"\"],[\"Raikh\",\"M. E.\",\"\"]]'),
(704.1705, 'S. E. Korshunov', 'I.V. Kolokolov and S.E. Korshunov', 'Optimal fluctuation approach to a directed polymer in a random medium', '4 pages, no figures', 'Phys. Rev. B 75, 140201 (2007)', '10.1103/PhysRevB.75.140201', '', 'cond-mat.dis-nn cond-mat.stat-mech', '', '  A modification of the optimal fluctuation approach is applied to study the\ntails of the free energy distribution function P(F) for an elastic string in\nquenched disorder both in the regions of the universal behavior of P(F) and in\nthe regions of large fluctuations, where the behavior of P(F) is non-universal.\nThe difference between the two regimes is shown to consist in whether it is\nnecessary or not to take into account the renormalization of parameters by the\nfluctuations of disorder in the vicinity of the optimal fluctuation.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:24:51 GMT\"}]', '2009-11-13', '[[\"Kolokolov\",\"I. V.\",\"\"],[\"Korshunov\",\"S. E.\",\"\"]]'),
(704.1706, 'Nick van Eijndhoven', 'N. van Eijndhoven, O. Fadiran and G. Japaridze', 'Implementation of a Gauss convoluted Pandel PDF for track reconstruction\n  in Neutrino Telescopes', '9 pages, 4 figures Revision 1 : extended content 12 pages, 4 figures\n  Accepted for publication in Astroparticle Physics', 'Astropart.Phys.28:456-462,2007', '10.1016/j.astropartphys.2007.09.001', '', 'astro-ph', '', '  A probability distribution function is presented which provides a realistic\ndescription of the detection of scattered photons. The resulting probabilities\ncan be described analytically by means of a superposition of several special\nfunctions. These exact expressions can be evaluated numerically only for small\ndistances and limited time residuals, due to computer accuracy limitations. In\nthis report we provide approximations for the exact expressions in different\nregions of the distance-time residual space, defined by the detector geometry\nand the space-time scale of an event. These approximations can be evaluated\nnumerically with a relative error with respect to the exact expression at the\nboundaries of less than 0.001.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:26:14 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 5 Sep 2007 09:20:16 GMT\"}]', '2009-06-23', '[[\"van Eijndhoven\",\"N.\",\"\"],[\"Fadiran\",\"O.\",\"\"],[\"Japaridze\",\"G.\",\"\"]]'),
(704.1707, 'Linda Buisman', 'Linda Buisman and Rajeev Gor\\\'e', 'A Cut-free Sequent Calculus for Bi-Intuitionistic Logic: Extended\n  Version', '', '', '', '', 'cs.LO', '', '  Bi-intuitionistic logic is the extension of intuitionistic logic with a\nconnective dual to implication. Bi-intuitionistic logic was introduced by\nRauszer as a Hilbert calculus with algebraic and Kripke semantics. But her\nsubsequent ``cut-free\'\' sequent calculus for BiInt has recently been shown by\nUustalu to fail cut-elimination. We present a new cut-free sequent calculus for\nBiInt, and prove it sound and complete with respect to its Kripke semantics.\nEnsuring completeness is complicated by the interaction between implication and\nits dual, similarly to future and past modalities in tense logic. Our calculus\nhandles this interaction using extended sequents which pass information from\npremises to conclusions using variables instantiated at the leaves of failed\nderivation trees. Our simple termination argument allows our calculus to be\nused for automated deduction, although this is not its main purpose.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:29:31 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Apr 2007 03:11:16 GMT\"}]', '2007-05-23', '[[\"Buisman\",\"Linda\",\"\"],[\"Goré\",\"Rajeev\",\"\"]]'),
(704.1708, 'Qiuping A. Wang', 'Qiuping A. Wang (ISMANS)', 'From virtual work principle to least action principle for stochastic\n  dynamics', '13 pages', '', '', '', 'cond-mat.stat-mech', '', '  After the justification of the maximum entropy principle for equilibrium\nmechanical system from the principle of virtual work, i.e., the virtual work of\nmicroscopic forces on the elements of a mechanical system vanishes in\nthermodynamic equilibrium, we present in this paper an application of the same\nprinciple to dynamical systems out of equilibrium. The aim of this work is to\njustify a least action principle and the concurrent maximum path entropy\nprinciple for nonequilibrium thermodynamic systems.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:30:52 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 16 Apr 2007 10:36:27 GMT\"},{\"version\":\"v3\",\"created\":\"Sun, 9 Dec 2007 08:30:44 GMT\"}]', '2007-12-09', '[[\"Wang\",\"Qiuping A.\",\"\",\"ISMANS\"]]'),
(704.1709, 'Marie Cottrell', 'Marie Cottrell (SAMOS, Matisse), Smail Ibbou (SAMOS, Matisse), Patrick\n  Letr\\\'emy (SAMOS, Matisse)', 'Traitement Des Donnees Manquantes Au Moyen De L\'Algorithme De Kohonen', '', 'Actes de la dixi\\`eme conf\\\'erence ACSEG 2003 (Nantes) (2003)\n  201-217', '', '', 'stat.AP cs.NE', '', '  Nous montrons comment il est possible d\'utiliser l\'algorithme d\'auto\norganisation de Kohonen pour traiter des donn\\\'ees avec valeurs manquantes et\nestimer ces derni\\`eres. Apr\\`es un rappel m\\\'ethodologique, nous illustrons\nnotre propos \\`a partir de trois applications \\`a des donn\\\'ees r\\\'eelles.\n  -----\n  We show how it is possible to use the Kohonen self-organizing algorithm to\ndeal with data which contain missing values and to estimate them. After a\nmethodological recall, we illustrate our purpose from three real databases\napplications.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:33:15 GMT\"}]', '2007-05-23', '[[\"Cottrell\",\"Marie\",\"\",\"SAMOS, Matisse\"],[\"Ibbou\",\"Smail\",\"\",\"SAMOS, Matisse\"],[\"Letrémy\",\"Patrick\",\"\",\"SAMOS, Matisse\"]]'),
(704.1710, 'Kazuya Mitsutani', 'Kazuya Mitsutani, Masakiyo Kitazawa, Teiji Kunihiro, Yukio Nemoto', 'Further Analysis of Excitations of Quarks at Finite Temperature -- Mass\n  Effect and Pole Structure --', '6pages, 5 figures. Poster presentation at the 19th International\n  Conference on Ultra-Relativistic Nucleus-Nucleus Collisions (QM2006) held in\n  Shanghai, China on November 14-20, 2006', 'Int.J.Mod.Phys.E16:2263-2268,2007', '10.1142/S0218301307007787', 'YITP-07-19', 'hep-ph', '', '  We calculate the spectral function of the massive quark at finite temperature\n(T) using a Yukawa model and show that the peak in the negative energy region\namong the three-peaks found in a previous work for the massless quark is\nlargely suppressed. To explore the underlying mechanism of this behavior, we\nalso investigate the pole structure of the retarded Green function of the\nquark. We will show the result only for the massless quark. We find the\nresidues of the poles corresponding the three-peaks are all comparable at\n$T\\sim m_b$. We also show that the multi-peak structure of the quark spectra is\nwell described in the pole approximation which indicates that the quasi-paricle\npicture is valid in this $T$ region.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:43:05 GMT\"}]', '2010-11-26', '[[\"Mitsutani\",\"Kazuya\",\"\"],[\"Kitazawa\",\"Masakiyo\",\"\"],[\"Kunihiro\",\"Teiji\",\"\"],[\"Nemoto\",\"Yukio\",\"\"]]'),
(704.1711, 'Marie Cottrell', 'Patrick Letr\\\'emy (SAMOS, CES), Marie Cottrell (SAMOS, CES), Patrice\n  Gaubert (SAMOS, CES), Joseph Rynkiewicz (SAMOS, CES)', 'Dynamical Equilibrium, trajectories study in an economical system. The\n  case of the labor market', 'accepted to the WSOM 2007 Conference (Bielefield)', '', '', '', 'stat.AP', '', '  The paper deals with the study of labor market dynamics, and aims to\ncharacterize its equilibriums and possible trajectories. The theoretical\nbackground is the theory of the segmented labor market. The main idea is that\nthis theory is well adapted to interpret the observed trajectories, due to the\nheterogeneity of the work situations.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:49:11 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 9 Jul 2007 10:23:34 GMT\"}]', '2007-07-09', '[[\"Letrémy\",\"Patrick\",\"\",\"SAMOS, CES\"],[\"Cottrell\",\"Marie\",\"\",\"SAMOS, CES\"],[\"Gaubert\",\"Patrice\",\"\",\"SAMOS, CES\"],[\"Rynkiewicz\",\"Joseph\",\"\",\"SAMOS, CES\"]]'),
(704.1712, 'Ayumu Sugita', 'Ayumu Sugita', 'Borromean Entanglement Revisited', 'Proceedings of the International Workshop on \"Knot Theory for\n  Scientic Objects\" held in Osaka (Japan), March 8-10, 2006. 10 pages, 5\n  figures', '', '', '', 'quant-ph', '', '  An interesting analogy between quantum entangled states and topological links\nwas suggested by Aravind. In particular, he emphasized a connection between the\nGreenberger-Horne-Zeilinger (GHZ) state and the Borromean rings. However, he\nmade the connection in a way that depends on the choice of measurement basis.\nWe reconsider it in a basis-independent way by using the reduced density\nmatrix.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:53:54 GMT\"}]', '2007-05-23', '[[\"Sugita\",\"Ayumu\",\"\"]]'),
(704.1713, 'Shuji Deguchi', 'S. Deguchi, T. Fujii, Y. Ita, H. Imai, H. Izumiura, O. Kameya, N.\n  Matsunaga, A. Miyazaki, A. Mizutani, Y. Nakada, J. Nakashima, A. Winnberg', 'An SiO Maser Search off the Galactic Plane', 'PASJ No.3 (June 25, 2007 issue in press)', '', '10.1093/pasj/59.3.559', 'NRO report No.651', 'astro-ph', '', '  We have searched for the SiO J=1--0 v= 1 and 2 maser lines at ~ 43 GHz in 277\n2MASS/MSX/IRAS sources off the Galactic plane (|b|> 3 deg), which resulted in\n119 (112 new) detections. Among the new detections, are two very faint objects\nwith MSX 12 micron flux densities below 2 Jy. These are likely to be O-rich\nAGB-stars associated with dwarf-galaxy tidal tails. The sample also includes\nmedium bright MSX objects at moderately high Galactic latitudes (3 deg<|b|<5\ndeg) and in the IRAS gap at higher latitudes. A signature of a warp of the\ninner Galactic disk is found for a disk subsample. This warp appears relatively\nstrongly in the area of 0<l<45 deg and 3<|b|<5 deg. We also found a group of\nstars that does not follow to the Galactic rotation. This feature appears in\nthe Galactic disk at l~ 27 deg, and extends more than 15 deg in Galactic\nlatitude, like a stream of tidal debris from a dwarf galaxy.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:57:04 GMT\"}]', '2015-05-13', '[[\"Deguchi\",\"S.\",\"\"],[\"Fujii\",\"T.\",\"\"],[\"Ita\",\"Y.\",\"\"],[\"Imai\",\"H.\",\"\"],[\"Izumiura\",\"H.\",\"\"],[\"Kameya\",\"O.\",\"\"],[\"Matsunaga\",\"N.\",\"\"],[\"Miyazaki\",\"A.\",\"\"],[\"Mizutani\",\"A.\",\"\"],[\"Nakada\",\"Y.\",\"\"],[\"Nakashima\",\"J.\",\"\"],[\"Winnberg\",\"A.\",\"\"]]'),
(704.1714, 'Boris Petukhov', 'B. V. Petukhov', 'Dislocation Dynamics in a Crystal Lattice (Peierls-Nabarro) Relief', '39 pages, 15 figures', '', '', '', 'nlin.PS', '', '  The theory of the dislocation motion in the periodic potential relief of the\ncrystal lattice (the Peierls-Nabarro barriers) is reviewed. On the basis of the\nkink mechanism the temperature dependence of the flow stress is described for a\nwide class of materials. The theory of quantum mechanical dislocation\ntunnelling through the Peierls-Nabarro barriers is extended and compared with\nexperimental data on the plasticity of alkali halides, BCC and HCP metals at\nlow temperatures. The behavior of the flow stress at the range of athermic\nanomalies is modeled by changing the mechanism of the dislocation motion from\nthe thermally activated hopping over the barriers to the quantum tunnelling\nthrough them. Some results of previous calculations are represented in a more\nexplicit convenient for applications form. The pronounced effect of the\nswitching between the normal and the superconducting states on the flow stress\nof metals is explained on the basis of the change in the dissipative properties\nof the electron subsystem affecting the dislocation motion.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 07:58:58 GMT\"}]', '2007-05-23', '[[\"Petukhov\",\"B. V.\",\"\"]]'),
(704.1715, 'Leonid Ksenofontov', 'E.G.Berezhko, H.J.Voelk', 'Spectrum of cosmic rays, produced in supernova remnants', '4 pages with emulateapj, 3 figures, accepted for publication in the\n  Astrophysical Journal Letters', '', '10.1086/518737', '', 'astro-ph', '', '  Nonlinear kinetic theory of cosmic ray (CR) acceleration in supernova\nremnants is employed to calculate CR spectra. The magnetic field in SNRs is\nassumed to be significantly amplified by the efficiently accelerating nuclear\nCR component. It is shown that the calculated CR spectra agree in a\nsatisfactory way with the existing measurements up to the energy $10^{17}$ eV.\nThe power law spectrum of protons extends up to the energy $3\\times 10^{15}$ eV\nwith a subsequent exponential cutoff. It gives a natural explanation for the\nobserved knee in the Galactic CR spectrum. The maximum energy of the\naccelerated nuclei is proportional to their charge number $Z$. Therefore the\nbreak in the Galactic CR spectrum is the result of the contribution of\nprogressively heavier species in the overall CR spectrum so that at $10^{17}$\neV the CR spectrum is dominated by iron group nuclei. It is shown that this\ncomponent plus a suitably chosen extragalactic CR component can give a\nconsistent description for the entire Galactic CR spectrum.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:26:46 GMT\"}]', '2009-11-13', '[[\"Berezhko\",\"E. G.\",\"\"],[\"Voelk\",\"H. J.\",\"\"]]'),
(704.1716, 'Paluba  Waldemar', 'Waldemar Paluba', 'One-parameter families of functions in the Pick class', '', '', '', '', 'math.DS', '', '  In the one-parameter family of power-law maps of the form\n$f_a(x)=-|x|^{\\alpha}+a,$ $\\alpha >1,$ we give examples of mutually related\ndynamically determined quantities, depending on the parameter $a$, such that\none is a Pick function of the following one. These Pick functions are\nextendable by reflection through the $(1,+\\infty)$ half-axis and have\ncompletely monotone derivatives there.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:23:48 GMT\"}]', '2007-05-23', '[[\"Paluba\",\"Waldemar\",\"\"]]'),
(704.1717, 'Gerhard Roehrle', 'J. Matthew Douglass and Gerhard Roehrle', 'The homology of the Steinberg variety and Weyl group coinvariants', '17 pages, to appear in Documenta Math', '', '', '', 'math.RT math.AT', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Let G be a complex, connected, reductive algebraic group with Weyl group W\nand Steinberg variety Z. We show that the graded Borel-Moore homology of Z is\nisomorphic to the smash product of the coinvariant algebra of W and the group\nalgebra of W.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:31:09 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 1 Sep 2008 10:43:19 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 31 Jul 2009 17:01:51 GMT\"}]', '2009-07-31', '[[\"Douglass\",\"J. Matthew\",\"\"],[\"Roehrle\",\"Gerhard\",\"\"]]'),
(704.1718, 'Anjan Kumar Chandra', 'Anjan Kumar Chandra, Subinay Dasgupta', 'Spin-spin Correlation in Some Excited States of Transverse Ising Model', '5 pages, 1 figure', 'J. Phys. A: Math. Theor. 40 (2007) 5231-5239', '10.1088/1751-8113/40/20/001', '', 'cond-mat.stat-mech', '', '  We consider the transverse Ising model in one dimension with\nnearest-neighbour interaction and calculate exactly the longitudinal spin-spin\ncorrelation for a class of excited states. These states are known to play an\nimportant role in the perturbative treatment of one-dimensional transverse\nIsing model with frustrated second-neighbour interaction. To calculate the\ncorrelation, we follow the earlier procedure of Wu, use Szego\'s theorem and\nalso use Fisher-Hartwig conjecture. The result is that the correlation decays\nalgebraically with distance ($n$) as $1/\\surd n$ and is oscillatory or\nnon-oscillatory depending on the magnitude of the transverse field.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:38:46 GMT\"}]', '2007-05-23', '[[\"Chandra\",\"Anjan Kumar\",\"\"],[\"Dasgupta\",\"Subinay\",\"\"]]'),
(704.1719, 'Paolo Nason', 'Michelangelo L. Mangano and Paolo Nason', 'Radiative quarkonium decays and the NMSSM Higgs interpretation of the\n  HyperCP Sigma+ --> p mu+mu- events', '6 pages, no figures', 'Mod.Phys.Lett.A22:1373-1380,2007', '10.1142/S0217732307023729', 'Bicocca-FT-07-6, CERN-PH-TH/2007-062', 'hep-ph', '', '  We study the potential of radiative decays of the Upsilon(1S) and of the phi\nmesons to search for a light pseudoscalar Higgs boson, proposed as a possible\ninterpretation of Sigma+ --> p mu+mu- events observed by the HyperCP\ncollaboration at Fermilab. We conclude that the detection of this signal should\ncertainly be possible with the current CLEO Upsilon(1S) data, and is within the\nreach of KLOE in at least part of the range of couplings suggested by the\nHyperCP findings.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:48:52 GMT\"}]', '2008-11-26', '[[\"Mangano\",\"Michelangelo L.\",\"\"],[\"Nason\",\"Paolo\",\"\"]]'),
(704.1720, 'Mikko Laine', 'M. Laine', 'A resummed perturbative estimate for the quarkonium spectral function in\n  hot QCD', '16 pages. v2: misprint fixed, minor additions', 'JHEP 0705:028,2007', '10.1088/1126-6708/2007/05/028', '', 'hep-ph hep-lat', '', '  By making use of the finite-temperature real-time static potential that was\nintroduced and computed to leading non-trivial order in Hard Thermal Loop\nresummed perturbation theory in recent work, and solving numerically a\nSchr\\\"odinger-type equation, we estimate the quarkonium (in practice,\nbottomonium) contribution to the spectral function of the electromagnetic\ncurrent in hot QCD. The spectral function shows a single resonance peak which\nbecomes wider and then disappears as the temperature is increased beyond 450\nMeV or so. This behaviour can be compared with recently attempted lattice\nreconstructions of the same quantity, based on the ``maximum entropy method\'\',\nwhich generically show several peaks. We also specify the dependence of our\nresults on the spatial momentum of the electromagnetic current, as well as on\nthe baryon chemical potential characterising the hot QCD plasma.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 18:26:59 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 12 Jun 2007 13:24:22 GMT\"}]', '2009-11-13', '[[\"Laine\",\"M.\",\"\"]]'),
(704.1721, 'Terunuma Sachiko', 'Masako Bando, Yoko Fukase, Jonathan Shock, Akio Sugamoto, Sachiko\n  Terunuma', 'An Exotic Approach to Hadron Physics', '8 pages, 5 figures, to appear in the proceedings for YKIS06', 'Prog.Theor.Phys.Suppl.168:223-230,2007', '10.1143/PTPS.168.223', '', 'hep-ph', '', '  An exotic approach to hadrons is discussed. It is based on the recently\ndeveloped open-closed string duality explicitly conjectured as the AdS/CFT\ncorrespondence. Mesons as well as pentaquarks are studied in this approach.\nSpins are introduced as distribution functions over the string, and a second\nquantization method of string theory is examined and used to estimate the mass\nand decay width of various hadrons. This approach provides a way to understand\nthe structure of flavor by a configuration of probe branes.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:46:59 GMT\"}]', '2008-11-26', '[[\"Bando\",\"Masako\",\"\"],[\"Fukase\",\"Yoko\",\"\"],[\"Shock\",\"Jonathan\",\"\"],[\"Sugamoto\",\"Akio\",\"\"],[\"Terunuma\",\"Sachiko\",\"\"]]'),
(704.1722, 'Hiroshi Watanabe', 'Hiroshi Watanabe and Masao Ogata', 'Fermi Surface Reconstruction without Breakdown of Kondo Screening at\n  Quantum Critical Point', '4 pages, 3 figures, submitted to Physical Review Letters', 'Phys. Rev. Lett. 99, 136401 (2007)', '10.1103/PhysRevLett.99.136401', '', 'cond-mat.str-el', '', '  Motivated by recent Hall-effect experiment in YbRh$_2$Si$_2$, we study ground\nstate properties of a Kondo lattice model in a two-dimensional square lattice\nusing variational Monte Carlo method. We show that there are two types of phase\ntransition, antiferromagnetic transition and topological one (Fermi surface\nreconstruction). In a wide region of parameters, these two transitions occur\nsimultaneously without the breakdown of Kondo screening, accompanied by a\ndiscontinuous change of the Hall coefficient. This result is consistent with\nthe experiment and gives a novel theoretical picture for the quantum critical\npoint in heavy fermion systems.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 08:59:39 GMT\"}]', '2007-09-26', '[[\"Watanabe\",\"Hiroshi\",\"\"],[\"Ogata\",\"Masao\",\"\"]]'),
(704.1723, 'Andres Asensio Ramos', 'A. Asensio Ramos (1), J. Trujillo Bueno (1,2) ((1) IAC, (2) CSIC)', 'A User-Friendly Code to Diagnose Chromospheric Plasmas', '8 pages, 3 figures, proceedings of \"Physics of Chromospheric Plasmas\"\n  (Coimbra), ASP 368, 163 (2007)', '', '', '', 'astro-ph', '', '  The physical interpretation of spectropolarimetric observations of lines of\nneutral helium, such as those of the 10830 A multiplet, represents an excellent\nopportunity for investigating the magnetism of plasma structures in the solar\nchromosphere. Here we present a powerful forward modeling and inversion code\nthat permits either to calculate the emergent intensity and polarization for\nany given magnetic field vector or to infer the dynamical and magnetic\nproperties from the observed Stokes profiles. This diagnostic tool is based on\nthe quantum theory of spectral line polarization, which self-consistently\naccounts for the Hanle and Zeeman effects in the most general case of the\nincomplete Paschen-Back effect regime. We also take into account radiative\ntransfer effects. An efficient numerical scheme based on global optimization\nmethods has been applied. Our Stokes inversion code permits a fast and reliable\ndetermination of the global minimum.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:21:58 GMT\"}]', '2007-05-23', '[[\"Ramos\",\"A. Asensio\",\"\",\"IAC\"],[\"Bueno\",\"J. Trujillo\",\"\",\"IAC\",\"CSIC\"]]'),
(704.1724, 'Marco Ruggieri', 'M. Ruggieri', 'Inhomogeneous color superconductivity and the cooling of compact stars', '4 pages, 1 figure, uses aiproc style. Talk given at \"Quark\n  confinement and the hadron spectrum\", Ponta Delgada, Acores, Portugal, 2-7\n  September 2006', 'AIPConf.Proc.892:495-498,2007', '10.1063/1.2714452', '', 'hep-ph', '', '  In this talk I discuss the inhomogeneous (LOFF) color superconductive phases\nof Quantum Chromodynamics (QCD). In particular, I show the effect of a core of\nLOFF phase on the cooling of a compact star.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:28:14 GMT\"}]', '2008-11-26', '[[\"Ruggieri\",\"M.\",\"\"]]'),
(704.1725, 'Pulak Ranjan Giri', 'Pulak Ranjan Giri', 'Scaling anomaly in cosmic string background', '4 pages,1 figure', 'Eur.Phys.J.C56:147-151,2008', '10.1140/epjc/s10052-008-0635-1', 'SINP/TNP/2007/05', 'hep-th gr-qc', '', '  We show that the classical scale symmetry of a particle moving in cosmic\nstring background is broken upon inequivalent quantization of the classical\nsystem, leading to anomaly. The consequence of this anomaly is the formation of\nsingle bound state in the coupling interval \\gamma\\in(-1,1). The inequivalent\nquantization is characterized by a 1-parameter family of self-adjoint extension\nparameter \\omega. It has been conjectured that the formation of loosely bound\nstate in cosmic string background may lead to the so called anomalous\nscattering cross section for the particles, which is usually seen in molecular\nphysics.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:38:06 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 14 Apr 2007 08:33:04 GMT\"}]', '2008-11-26', '[[\"Giri\",\"Pulak Ranjan\",\"\"]]'),
(704.1726, 'Agung Budiyono', 'Agung Budiyono', 'On de Broglie\'s quantum particle as the soliton solution of linear\n  Schr\\\"odinger equation', '14 pages, content changed', '', '', '', 'physics.gen-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We develop a class of soliton solution of {\\it linear} Schr\\\"odinger equation\nwithout external potential. The quantum probability density generates its own\nboundary inside which there is internal vibration whose wave number is\ndetermined by the velocity of the particle as firstly conjectured by de\nBroglie. Assuming resonance of the internal vibration will lead to quantization\nof particle\'s momentum in term of wave number of the envelope quantum\nprobability density. We further show that the linearity of the Schr\\\"odinger\nequation allows us to have non-interacting many solitons solution through\nsuperposition, each describing a particle with equal mass.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:43:46 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 19 Aug 2009 05:56:55 GMT\"}]', '2009-08-19', '[[\"Budiyono\",\"Agung\",\"\"]]'),
(704.1727, 'Gustavo Niz', 'Gustavo Niz and Neil Turok', 'Stringy corrections to a time-dependent background solution of string\n  and M-Theory', '22 pages, 4 figures', 'Phys.Rev.D75:126004,2007', '10.1103/PhysRevD.75.126004', 'Phys.Rev.D75:126004,2007.', 'hep-th', '', '  We consider one of the simplest time-dependent backgrounds in M-theory,\ndescribing the shrinking away of the M-theory dimension with the other spatial\ndimensions static. As the M-theory dimension becomes small, the situation\nbecomes well-described by string theory in a singular cosmological background\nwhere the string coupling tends to zero but the $\\alpha\'$-corrections become\nlarge, near the cosmic singularity. We compute these $\\alpha\'$-corrections,\nboth for the background and for linearized perturbations, in heterotic string\ntheory, and show they may be reproduced by a map from eleven-dimensional\nM-theory.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:46:25 GMT\"}]', '2008-11-26', '[[\"Niz\",\"Gustavo\",\"\"],[\"Turok\",\"Neil\",\"\"]]'),
(704.1728, 'S. Mignemi', 'S. Mignemi', 'Doubly Special Relativity and Finsler geometry', '8 pages, plain TeX', 'Phys.Rev.D76:047702,2007', '10.1103/PhysRevD.76.047702', '', 'gr-qc', '', '  We discuss the recent proposal of implementing Doubly Special Relativity in\nconfiguration space by means of Finsler geometry. Although this formalism leads\nto a consistent description of the dynamics of a particle, it does not seem to\ngive a complete description of the physics. In particular, the Finsler line\nelement is not invariant under the deformed Lorentz transformations of Doubly\nSpecial Relativity. We study in detail some simple applications of the\nformalism.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 09:51:02 GMT\"}]', '2008-11-26', '[[\"Mignemi\",\"S.\",\"\"]]'),
(704.1729, 'Silvia Piranomonte Miss', 'S. Piranomonte, M. Perri, P. Giommi, H. Landt, P. Padovani', 'The Sedentary Survey of Extreme High Energy Peaked BL Lacs III. Results\n  from Optical Spectroscopy', '23 pages, accepted by A&A', '', '10.1051/0004-6361:20077086', '', 'astro-ph', '', '  The multi-frequency Sedentary Survey is a flux limited, statistically\nwell-defined sample of highly X-ray dominated BL Lacertae objects (HBLs) which\nincludes 150 sources. In this paper, the third of the series, we report the\nresults of a dedicated optical spectroscopy campaign that, together with\nresults from other independent optical follow up programs, led to the\nspectroscopic identification of all sources in the sample. We carried out a\nsystematic spectroscopic campaign for the observation of all unidentified\nobjects of the sample using the ESO 3.6m, the KPNO 4m, and the TNG optical\ntelescopes. We present new identifications and optical spectra for 76 sources,\n50 of which are new BL Lac objects, 18 are sources previously referred as BL\nLacs but for which no redshift information was available, and 8 are broad\nemission lines AGNs. We find that the multi-frequency selection technique used\nto build the survey is highly efficient (about 90%) in selecting BL Lacs\nobjects. We present positional and spectroscopic information for all confirmed\nBL Lac objects. Our data allowed us to determined 36 redshifts out of the 50\nnew BL Lacs and 5 new redshifts for the previously known objects. The redshift\ndistribution of the complete sample is presented and compared with that of\nother BL Lacs samples. For 26 sources without recognizable absorption features,\nwe calculated lower limits to the redshift using a method based on simulated\noptical spectra with different ratios between jet and galaxy emission. For a\nsubsample of 38 object with high-quality spectra, we find a correlation between\nthe optical spectral slope, the 1.4 GHz radio luminosity, and the Ca H&K break\nvalue, indicating that for powerful/beamed sources the optical light is\ndominated by the non-thermal emission from the jet.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 10:36:26 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 18 Apr 2007 15:56:26 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 4 May 2007 15:25:12 GMT\"}]', '2009-11-13', '[[\"Piranomonte\",\"S.\",\"\"],[\"Perri\",\"M.\",\"\"],[\"Giommi\",\"P.\",\"\"],[\"Landt\",\"H.\",\"\"],[\"Padovani\",\"P.\",\"\"]]'),
(704.1730, 'Carlo H\\\"am\\\"al\\\"ainen', 'Nicholas J. Cavenagh, Ales Drapal, and Carlo Hamalainen', 'Latin bitrades derived from groups', '23 pages', '', '', '', 'math.CO', '', '  A latin bitrade is a pair of partial latin squares which are disjoint, occupy\nthe same set of non-empty cells, and whose corresponding rows and columns\ncontain the same set of entries. Dr\\\'apal (\\cite{Dr9}) showed that a latin\nbitrade is equivalent to three derangements whose product is the identity and\nwhose cycles pairwise have at most one point in common. By letting a group act\non itself by right translation, we show how some latin bitrades may be derived\nfrom groups without specifying an independent group action. Properties of latin\ntrades such as homogeneousness, minimality (via thinness) and orthogonality may\nalso be encoded succinctly within the group structure. We apply the\nconstruction to some well-known groups, constructing previously unknown latin\nbitrades. In particular, we show the existence of minimal, $k$-homogeneous\nlatin trades for each odd $k\\geq 3$. In some cases these are the smallest known\nsuch examples.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 10:36:30 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 8 Mar 2008 10:09:24 GMT\"}]', '2008-03-08', '[[\"Cavenagh\",\"Nicholas J.\",\"\"],[\"Drapal\",\"Ales\",\"\"],[\"Hamalainen\",\"Carlo\",\"\"]]'),
(704.1731, 'Pedro Gonzalez-Diaz', 'Pedro F Gonzalez-Diaz and Prado Martin-Moruno (IMAFF, CSIC)', 'Wormholes in the accelerating universe', '2 pages, LaTex, to appear in the Proceedings of the 11th Marcel\n  Grossmann Conference, 2006', '', '10.1142/9789812834300_0358', 'IMAFF-RCA-05-07', 'astro-ph', '', '  We discuss different arguments that have been raised against the viability of\nthe big trip process, reaching the conclusions that this process can actually\noccur by accretion of phantom energy onto the wormholes and that it is stable\nand might occur in the global context of a multiverse model. We finally argue\nthat the big trip does not contradict any holographic bounds on entropy and\ninformation.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 10:38:21 GMT\"}]', '2016-11-15', '[[\"Gonzalez-Diaz\",\"Pedro F\",\"\",\"IMAFF, CSIC\"],[\"Martin-Moruno\",\"Prado\",\"\",\"IMAFF, CSIC\"]]'),
(704.1732, 'Sergey Bastrukov', 'S. Bastrukov, H-K. Chang, S. Misicu, I. Molodtsova, D. Podgainy', 'Spheroidal and torsional modes of quasistatic shear oscillations in the\n  solid globe models of nuclear physics and pulsar astrophysics', '34 pages; 6 figures; Int.J.Mod.Phys.A.2007.Vol.22.N19.pp3261-3291', 'Int.J.Mod.Phys.A22:3261-3291,2007', '10.1142/S0217751X07036634', '', 'astro-ph', '', '  The past three decades of investigation on nuclear physics and pulsar\nastrophysics have seen gradual recognition that elastodynamic approach to the\ncontinuum mechanics of nuclear matter provides proper account of macroscopic\nmotions of degenerate Fermi-matter constituting interior of the nuclear\nmaterial objects, the densest of all known today. This paper focuses on one\ntheoretical issue of this development which is concerned with oscillatory\nbehavior of a viscoelastic solid globe in the regime of quasistatic,\nforce-free, non-compressional oscillations less investigated in the literature\ncompared to oscillations in the regime of standing shear waves. We show that in\nthis case the problem of computing frequency and lifetime of spheroidal and\ntorsional modes of non-radial shear vibrations damped by viscosity can be\nunambiguously resolved by working from the energy balance equation and taking\nadvantage of the Rayleigh\'s variational method. The efficiency of this method\nis demonstrated by solid globe models of nuclear physics and pulsar\nastrophysics dealing with oscillations of a spherical mass of a viscoelastic\nFermi-solid with homogeneous and non-homogeneous profiles of the bulk density,\nthe shear modulus, and the shear viscosity.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:12:11 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 15 Apr 2007 02:32:15 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 27 Apr 2007 04:51:09 GMT\"},{\"version\":\"v4\",\"created\":\"Mon, 16 Jul 2007 13:15:32 GMT\"},{\"version\":\"v5\",\"created\":\"Wed, 15 Aug 2007 08:02:46 GMT\"}]', '2009-06-23', '[[\"Bastrukov\",\"S.\",\"\"],[\"Chang\",\"H-K.\",\"\"],[\"Misicu\",\"S.\",\"\"],[\"Molodtsova\",\"I.\",\"\"],[\"Podgainy\",\"D.\",\"\"]]'),
(704.1733, 'Orfeu Bertolami', 'Orfeu Bertolami, Christian G. Boehmer, Tiberiu Harko, Francisco S.N.\n  Lobo', 'Extra force in $f(R)$ modified theories of gravity', 'Revtex4 file, 5 pages. Version to appear in Physical Review D', 'Phys.Rev.D75:104016,2007', '10.1103/PhysRevD.75.104016', '', 'gr-qc astro-ph hep-th', '', '  The equation of motion for test particles in $f(R)$ modified theories of\ngravity is derived. By considering an explicit coupling between an arbitrary\nfunction of the scalar curvature, $R$, and the Lagrangian density of matter, it\nis shown that an extra force arises. This extra force is orthogonal to the\nfour-velocity and the corresponding acceleration law is obtained in the weak\nfield limit. Connections with MOND and with the Pioneer anomaly are further\ndiscussed.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:49:59 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 24 May 2007 12:03:50 GMT\"}]', '2008-11-26', '[[\"Bertolami\",\"Orfeu\",\"\"],[\"Boehmer\",\"Christian G.\",\"\"],[\"Harko\",\"Tiberiu\",\"\"],[\"Lobo\",\"Francisco S. N.\",\"\"]]'),
(704.1734, 'Alan Coley', 'A.A. Coley', 'Averaging and Cosmological Observations', '9 pages', '', '', '', 'gr-qc astro-ph hep-th', '', '  The gravitational field equations on cosmological scales are obtained by\naveraging the Einstein field equations of general relativity. By assuming\nspatial homogeneity and isotropy on the largest scales, the local\ninhomogeneities affect the dynamics though correction (backreaction) terms,\nwhich can lead to behaviour qualitatively and quantitatively different from the\nFriedmann-Lema\\^{i}tre-Robertson-Walker models. The effects of averaging on\ncosmological observations are discussed. It is argued that, based on estimates\nfrom observational data, the backreaction (and, in particular, the averaged\nspatial curvature) can have a very significant dynamical effect on the\nevolution of the Universe and must be taken into account in observational\ncosmology.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:36:29 GMT\"}]', '2007-05-23', '[[\"Coley\",\"A. A.\",\"\"]]'),
(704.1735, 'Peter Blair Blakie', 'P. B. Blakie, E. Toth, M. J. Davis', 'Calorimetry of Bose-Einstein condensates', '6 pages, 1 figure. Updated to published version', 'J. Phys. B: At. Mol. Opt. Phys. 40, 3273 (2007)', '10.1088/0953-4075/40/16/008', '', 'cond-mat.other', '', '  We outline a practical scheme for measuring the thermodynamic properties of a\nBose-Einstein condensate as a function of internal energy. We propose using\nBragg scattering and controlled trap manipulations to impart a precise amount\nof energy to a near zero temperature condensate. After thermalisation the\ntemperature can be measured using standard techniques to determine the state\nequation $T(U,N,\\omega)$. Our analysis accounts for interaction effects and the\nexcitation of constants of motion which restrict the energy available for\nthermalisation.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:25:00 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 6 Aug 2007 23:14:11 GMT\"}]', '2009-11-13', '[[\"Blakie\",\"P. B.\",\"\"],[\"Toth\",\"E.\",\"\"],[\"Davis\",\"M. J.\",\"\"]]'),
(704.1736, 'Elham Kashefi', 'Anne Broadbent and Elham Kashefi', 'Parallelizing Quantum Circuits', '34 pages, 14 figures; depth complexity, measurement-based quantum\n  computing and parallel computing', 'Theoretical Computer Science, Volume 410, Issue 26, 2009', '10.1016/j.tcs.2008.12.046', '', 'quant-ph', '', '  We present a novel automated technique for parallelizing quantum circuits via\nforward and backward translation to measurement-based quantum computing\npatterns and analyze the trade off in terms of depth and space complexity. As a\nresult we distinguish a class of polynomial depth circuits that can be\nparallelized to logarithmic depth while adding only polynomial many auxiliary\nqubits. In particular, we provide for the first time a full characterization of\npatterns with flow of arbitrary depth, based on the notion of influencing paths\nand a simple rewriting system on the angles of the measurement. Our method\nleads to insightful knowledge for constructing parallel circuits and as\napplications, we demonstrate several constant and logarithmic depth circuits.\nFurthermore, we prove a logarithmic separation in terms of quantum depth\nbetween the quantum circuit model and the measurement-based model.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 18:39:53 GMT\"}]', '2012-02-22', '[[\"Broadbent\",\"Anne\",\"\"],[\"Kashefi\",\"Elham\",\"\"]]'),
(704.1737, 'Denis Vasilyev', 'Denis V. Vasilyev, Ivan V. Sokolov, and Eugene S. Polzik', 'Quantum memory for images - a quantum hologram', '5 pages, 3 figures', 'Phys. Rev. A 77, 020302(R) (2008)', '10.1103/PhysRevA.77.020302', '', 'quant-ph', '', '  Matter-light quantum interface and quantum memory for light are important\ningredients of quantum information protocols, such as quantum networks,\ndistributed quantum computation, etc. In this Letter we present a spatially\nmultimode scheme for quantum memory for light, which we call a quantum\nhologram. Our approach uses a multi-atom ensemble which has been shown to be\nefficient for a single spatial mode quantum memory. Due to the multi-atom\nnature of the ensemble it is capable of storing many spatial modes, a feature\ncritical for the present proposal. A quantum hologram has a higher storage\ncapacity compared to a classical hologram, and is capable of storing quantum\nfeatures of an image, such as multimode superposition and entangled quantum\nstates, something that a standard hologram is unable to achieve. Due to optical\nparallelism, the information capacity of the quantum hologram will obviously\nexceed that of a single-mode scheme.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:33:16 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 17 Sep 2007 10:43:26 GMT\"}]', '2009-11-13', '[[\"Vasilyev\",\"Denis V.\",\"\"],[\"Sokolov\",\"Ivan V.\",\"\"],[\"Polzik\",\"Eugene S.\",\"\"]]'),
(704.1738, 'Marco Patriarca', 'A. Chakraborti, M. Patriarca, and M.S. Santhanam', 'Financial time-series analysis: A brief overview', '16 pages, 7 figures, submitted for publication in the Proceedings\n  Volume of the International Workshop \"Econophys-Kolkata III\", Saha Institute\n  of Nuclear Physics, March 12-15, 2007', '', '10.1007/978-88-470-0665-2_4', '', 'q-fin.ST physics.soc-ph', '', '  Prices of commodities or assets produce what is called time-series. Different\nkinds of financial time-series have been recorded and studied for decades.\nNowadays, all transactions on a financial market are recorded, leading to a\nhuge amount of data available, either for free in the Internet or commercially.\nFinancial time-series analysis is of great interest to practitioners as well as\nto theoreticians, for making inferences and predictions. Furthermore, the\nstochastic uncertainties inherent in financial time-series and the theory\nneeded to deal with them make the subject especially interesting not only to\neconomists, but also to statisticians and physicists. While it would be a\nformidable task to make an exhaustive review on the topic, with this review we\ntry to give a flavor of some of its aspects.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:34:10 GMT\"}]', '2015-05-13', '[[\"Chakraborti\",\"A.\",\"\"],[\"Patriarca\",\"M.\",\"\"],[\"Santhanam\",\"M. S.\",\"\"]]'),
(704.1739, 'Celine Roucairol', 'Marco Hien, Celine Roucairol', 'Integral representations for solutions of exponential Gauss-Manin\n  systems', '16 pages', '', '', '', 'math.AG', '', '  Let f,g be two algebraically independent regular functions from the smooth\naffine complex variety U to the affine line. The associated exponential\nGauss-Manin systems on the affine line are defined to be the cohomology sheaves\nof the direct image of the exponential differential system $\\mathcal{O}_U e^g $\nwith respect to f. We prove that its holomorphic solutions admit\nrepresentations in terms of period integrals over topological chains with\npossibly closed support and with rapid decay condition.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:36:16 GMT\"}]', '2007-05-23', '[[\"Hien\",\"Marco\",\"\"],[\"Roucairol\",\"Celine\",\"\"]]'),
(704.1740, 'Mikhail Rogal', 'S. Moch and M. Rogal', 'Charged current deep-inelastic scattering at three loops', '29 pages, 6 figures', 'Nucl.Phys.B782:51-78,2007', '10.1016/j.nuclphysb.2007.05.008', 'DESY 07-002, SFB/CPP-07-01', 'hep-ph', '', '  We derive for deep-inelastic neutrino-proton scattering in the combination nu\nP - nubar P the perturbative QCD corrections to three loops for the charged\ncurrent structure functions F_2, F_L and F_3. In leading twist approximation we\ncalculate the first five odd-integer Mellin moments in the case of F_2 and F_L\nand the first five even-integer moments in the case of F_3. As a new result we\nobtain the coefficient functions to O(alpha_s^3) while the corresponding\nanomalous dimensions agree with known results in the literature.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:11:07 GMT\"}]', '2008-11-26', '[[\"Moch\",\"S.\",\"\"],[\"Rogal\",\"M.\",\"\"]]'),
(704.1741, 'Peter Jonker', 'P.G. Jonker, J.J.M. in \'t Zand, M. Mendez, M. van der Klis', 'Detection of a 1258 Hz high-amplitude kilohertz quasi-periodic\n  oscillation in the ultra-compact X-ray binary 1A 1246-588', '4 pages, 3 figures, accepted for publication in MNRAS', 'Mon.Not.Roy.Astron.Soc.378:1187-1190,2007', '10.1111/j.1365-2966.2007.11854.x', '', 'astro-ph', '', '  We have observed the ultra-compact low-mass X-ray binary (LMXB) 1A 1246-588\nwith the Rossi X-ray Timing Explorer (RXTE). In this manuscript we report the\ndiscovery of a kilohertz quasi-periodic oscillation (QPO) in 1A 1246-588. The\nkilohertz QPO was only detected when the source was in a soft high-flux state\nreminiscent of the lower banana branch in atoll sources. Only one kilohertz QPO\npeak is detected at a relatively high frequency of 1258+-2 Hz and at a single\ntrial significance of more than 7 sigma. Kilohertz QPOs with a higher frequency\nhave only been found on two occasions in 4U 0614+09. Furthermore, the frequency\nis higher than that found for the lower kilohertz QPO in any source, strongly\nsuggesting that the QPO is the upper of the kilohertz QPO pair often found in\nLMXBs. The full-width at half maximum is 25+-4 Hz, making the coherence the\nhighest found for an upper kilohertz QPO. From a distance estimate of ~6 kpc\nfrom a radius expansion burst we derive that 1A 1246-588 is at a persistent\nflux of ~0.2-0.3 per cent of the Eddington flux, hence 1A 1246-588 is one of\nthe weakest LMXBs for which a kilohertz QPO has been detected. The\nroot-mean-square (rms) amplitude in the 5-60 keV band is 27+-3 per cent, this\nis the highest for any kilohertz QPO source so far, in line with the general\nanti-correlation between source luminosity and rms amplitude of the kilohertz\nQPO peak identified before. Using the X-ray spectral information we produce a\ncolour-colour diagram. The source behaviour in this diagram provides further\nevidence for the atoll nature of the source.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:42:31 GMT\"}]', '2009-06-23', '[[\"Jonker\",\"P. G.\",\"\"],[\"Zand\",\"J. J. M. in \'t\",\"\"],[\"Mendez\",\"M.\",\"\"],[\"van der Klis\",\"M.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1742, 'Tomas Dohnal', 'Tomas Dohnal and Dmitry Pelinovsky', 'Surface gap solitons at a nonlinearity interface', '23 pages, 6 figures, 3 tables corrections in v.2: sign error in the\n  energy functional on p.3; discussion of the symmetries of Bloch functions on\n  p. 5-6 corrected; derivative symbol missing in (3.5) and in the formula for\n  \\mu below (3.6)', '', '10.1137/060676751', '', 'nlin.PS physics.optics', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We demonstrate existence of waves localized at the interface of two nonlinear\nperiodic media with different coefficients of the cubic nonlinearity via the\none-dimensional Gross--Pitaevsky equation. We call these waves the surface gap\nsolitons (SGS). In the case of smooth symmetric periodic potentials, we study\nanalytically bifurcations of SGS\'s from standard gap solitons and determine\nnumerically the maximal jump of the nonlinearity coefficient allowing for the\nSGS existence. We show that the maximal jump vanishes near the thresholds of\nbifurcations of gap solitons. In the case of continuous potentials with a jump\nin the first derivative at the interface, we develop a homotopy method of\ncontinuation of SGS families from the solution obtained via gluing of parts of\nthe standard gap solitons and study existence of SGS\'s in the photonic band\ngaps. We explain the termination of the SGS families in the interior points of\nthe band gaps from the bifurcation of linear bound states in the continuous\nnon-smooth potentials.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:55:45 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 1 Apr 2009 16:29:54 GMT\"}]', '2009-11-13', '[[\"Dohnal\",\"Tomas\",\"\"],[\"Pelinovsky\",\"Dmitry\",\"\"]]'),
(704.1743, 'Osamu Nakamura', 'Masataka Fukugita, Osamu Nakamura, Sadanori Okamura, Naoki Yasuda,\n  John C. Barentine, Jon Brinkmann, James E. Gunn, Mike Harvanek, Takashi\n  Ichikawa, Robert H. Lupton, Donald P. Schneider, Michael A. Strauss, Donald\n  G. York', 'A Catalogue of Morphologically Classified Galaxies from the Sloan\n  Digital Sky Survey: North Equatorial Region', 'Accepted for publication in Astronomical Journal. Table 2 available\n  at http://www.icrr.u-tokyo.ac.jp/~fukugita/MCGpaper/table2.txt', 'Astron.J.134:579-593,2007', '10.1086/518962', '', 'astro-ph', '', '  We present a catalogue of morphologically classified bright galaxies in the\nnorth equatorial stripe (230 deg$^2$) derived from the Third Data Release of\nthe Sloan Digital Sky Survey (SDSS). Morphological classification is performed\nby visual inspection of images in the $g$ band. The catalogue contains 2253\ngalaxies complete to a magnitude limit of $r=16$ after Galactic extinction\ncorrection, selected from 2658 objects that are judged as extended in the\nphotometric catalogue in the same magnitude limit. 1866 galaxies in our\ncatalogue have spectroscopic information. A brief statistical analysis is\npresented for the frequency of morphological types and mean colours in the\ncatalogue. A visual inspection of the images reveals that the rate of\ninteracting galaxies in the local Universe is approximately 1.5% in the\n$r\\le16$ sample. A verification is made for the photometric catalogue generated\nby the SDSS, especially as to its bright end completeness.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:45:55 GMT\"}]', '2008-11-26', '[[\"Fukugita\",\"Masataka\",\"\"],[\"Nakamura\",\"Osamu\",\"\"],[\"Okamura\",\"Sadanori\",\"\"],[\"Yasuda\",\"Naoki\",\"\"],[\"Barentine\",\"John C.\",\"\"],[\"Brinkmann\",\"Jon\",\"\"],[\"Gunn\",\"James E.\",\"\"],[\"Harvanek\",\"Mike\",\"\"],[\"Ichikawa\",\"Takashi\",\"\"],[\"Lupton\",\"Robert H.\",\"\"],[\"Schneider\",\"Donald P.\",\"\"],[\"Strauss\",\"Michael A.\",\"\"],[\"York\",\"Donald G.\",\"\"]]'),
(704.1744, 'Sergio Colafrancesco', 'P. Giommi, M. Capalbi, E. Cavazzuti, S. Colafrancesco, S. Cutini, D.\n  Gasparrini, E. Massaro, P. Padovani, M. Perri, S. Puccetti', 'Blazar surveys with WMAP and Swift', '3 pages, 3 figures, to appear in Proc. of the 1st GLAST Symposium,\n  Feb 5-8, 2007, Stanford, AIP, Eds. S. Ritz, P. F. Michelson, and C. Meegan', 'AIP Conf.Proc.921:32-36,2007', '10.1063/1.2757262', '', 'astro-ph', '', '  We present the preliminary results from two new surveys of blazars that have\ndirect implications on the GLAST detection of extragalactic sources from two\ndifferent perspectives: microwave selection and a combined deep X-ray/radio\nselection. The first one is a 41 GHz flux-limited sample extracted from the\nWMAP 3-yr catalog of microwave point sources. This is a statistically well\ndefined sample of about 200 blazars and radio galaxies, most of which are\nexpected to be detected by GLAST. The second one is a new deep survey of\nBlazars selected among the radio sources that are spatially coincident with\nserendipitous sources detected in deep X-ray images (0.3-10 keV) centered on\nthe Gamma Ray Bursts (GRB) discovered by the Swift satellite. This sample is\nparticularly interesting from a statistical viewpoint since a) it is unbiased\nas GRBs explode at random positions in the sky, b) it is very deep in the X-ray\nband (\\fx \\simgt $10^{-15}$ \\ergs) with a position accuracy of a few\narc-seconds, c) it will cover a fairly large (20-30 square deg.) area of sky,\nd) it includes all blazars with radio flux (1.4 GHz) larger than 10 mJy, making\nit approximately two orders of magnitude deeper than the WMAP sample and about\none order of magnitude deeper than the deepest existing complete samples of\nradio selected blazars, and e) it can be used to estimate the amount of\nunresolved GLAST high latitude gamma-ray background and its anisotropy\nspectrum.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 11:57:14 GMT\"}]', '2009-06-23', '[[\"Giommi\",\"P.\",\"\"],[\"Capalbi\",\"M.\",\"\"],[\"Cavazzuti\",\"E.\",\"\"],[\"Colafrancesco\",\"S.\",\"\"],[\"Cutini\",\"S.\",\"\"],[\"Gasparrini\",\"D.\",\"\"],[\"Massaro\",\"E.\",\"\"],[\"Padovani\",\"P.\",\"\"],[\"Perri\",\"M.\",\"\"],[\"Puccetti\",\"S.\",\"\"]]'),
(704.1745, 'V. Gogohia', 'V. Gogokhia', 'I. The mass gap and solution of the quark confinement problem in QCD', 'no tables, no figures, 14 pages', '', '', '', 'hep-ph hep-th', '', '  Using the previously derived confining gluon propagator, the corresponding\nsystem of equations determining the quark propagator is derived. The system of\nequations consists of the Schwinger-Dyson equation for the quark propagator\nitself, which includes the zero momentum transfer quark-gluon vertex. It is\ncomplemented by the Slavnov-Taylor identity for this vertex. The quark equation\ndepends explicitly on the mass gap, determining the scale of the truly\nnonperturbative dynamics in the QCD ground state. The obtained system of\nequations is manifestly gauge-invariant, i.e., does not depend explicitly on\nthe gauge-fixing parameter. It is also free from all the types of the\nperturbative contributions (\"contaminations\"), which may appear at the\nfundamental quark-gluon level.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:01:19 GMT\"}]', '2007-05-23', '[[\"Gogokhia\",\"V.\",\"\"]]'),
(704.1746, 'Parthasarathi Mitra', 'Bhramar Chatterjee, A. Ghosh and P. Mitra', 'Tunnelling from black holes and tunnelling into white holes', 'REVTeX, 6 pages; changed interpretation for white hole spacetimes; to\n  appear in PLB', 'Phys.Lett.B661:307-311,2008', '10.1016/j.physletb.2008.02.034', '', 'hep-th gr-qc', '', '  Hawking radiation is nowadays being understood as tunnelling through black\nhole horizons. Here, the extension of the Hamilton-Jacobi approach to\ntunnelling for non-rotating and rotating black holes in different non-singular\ncoordinate systems not only confirms this quantum emission from black holes but\nalso reveals the new phenomenon of absorption into white holes by quantum\nmechanical tunnelling. The role of a boundary condition of total absorption or\nemission is also clarified.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:06:44 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 26 Apr 2007 11:45:19 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 17 May 2007 09:07:14 GMT\"},{\"version\":\"v4\",\"created\":\"Wed, 20 Feb 2008 05:02:07 GMT\"}]', '2010-04-29', '[[\"Chatterjee\",\"Bhramar\",\"\"],[\"Ghosh\",\"A.\",\"\"],[\"Mitra\",\"P.\",\"\"]]'),
(704.1747, 'Iskander Aliev', 'Iskander Aliev and Chris Smyth', 'Solving algebraic equations in roots of unity', 'Since the last submission we became aware of several important\n  results in the area. The paper is now changed according to the current state\n  of the art', '', '', '', 'math.NT math.AG', '', '  This paper is devoted to finding solutions of polynomial equations in roots\nof unity. It was conjectured by S. Lang and proved by M. Laurent that all such\nsolutions can be described in terms of a finite number of parametric families\ncalled maximal torsion cosets. We obtain new explicit upper bounds for the\nnumber of maximal torsion cosets on an algebraic subvariety of the complex\nalgebraic $n$-torus ${\\mathbb G}_{\\rm m}^n$. In contrast to earlier works that\ngive the bounds of polynomial growth in the maximum total degree of defining\npolynomials, the proofs of our results are constructive. This allows us to\nobtain a new algorithm for determining maximal torsion cosets on an algebraic\nsubvariety of ${\\mathbb G}_{\\rm m}^n$.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:22:43 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 16 Apr 2007 14:30:54 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 1 Feb 2008 13:21:30 GMT\"}]', '2008-02-01', '[[\"Aliev\",\"Iskander\",\"\"],[\"Smyth\",\"Chris\",\"\"]]'),
(704.1748, 'Frank Schweitzer', 'Markus M. Geipel', 'Self-Organization applied to Dynamic Network Layout', 'Text revision and figures improved in v.2. See http://www.sg.ethz.ch\n  for more info and examples', 'International Journal of Modern Physics C vol. 18, no. 10 (2007),\n  pp. 1537-1549', '10.1142/S0129183107011558', '', 'physics.comp-ph cs.DS nlin.AO', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  As networks and their structure have become a major field of research, a\nstrong demand for network visualization has emerged. We address this challenge\nby formalizing the well established spring layout in terms of dynamic\nequations. We thus open up the design space for new algorithms. Drawing from\nthe knowledge of systems design, we derive a layout algorithm that remedies\nseveral drawbacks of the original spring layout. This new algorithm relies on\nthe balancing of two antagonistic forces. We thus call it {\\em arf} for\n\"attractive and repulsive forces\". It is, as we claim, particularly suited for\na dynamic layout of smaller networks ($n < 10^3$). We back this claim with\nseveral application examples from on going complex systems research.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:45:28 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 19 Apr 2007 13:21:55 GMT\"},{\"version\":\"v3\",\"created\":\"Sun, 7 Sep 2008 12:46:19 GMT\"},{\"version\":\"v4\",\"created\":\"Mon, 24 Nov 2008 18:35:59 GMT\"},{\"version\":\"v5\",\"created\":\"Tue, 20 Jan 2009 14:58:35 GMT\"}]', '2009-11-13', '[[\"Geipel\",\"Markus M.\",\"\"]]'),
(704.1749, 'Steffen Mieske', 'S. Mieske, M. Rejkuba, S. Bagnulo, C. Izzo, G. Marconi', 'VIMOS total transmission profiles for broad-band filters', '5 pages, 3 figures, to appear in the proceedings of the ESO\n  instrument calibration workshop 2007, Springer Verlag series \"ESO\n  Astrophysics Symposia\", eds. F. Kerber & A. Kaufer', '', '10.1007/978-3-540-76963-7_7', '', 'astro-ph', '', '  VIMOS is a wide-field imager and spectrograph mounted on UT3 at the\n  VLT, whose FOV consists of four 7\'x8\' quadrants. Here we present the\nmeasurements of total transmission profiles -- i.e. the throughput of telescope\n+ instrument -- for the broad band filters U, B, V, R, I, and z for each of its\nfour quadrants. Those measurements can also be downloaded from the public VIMOS\nweb-page. The transmission profiles are compared with previous estimates from\nthe VIMOS consortium.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:36:42 GMT\"}]', '2015-05-13', '[[\"Mieske\",\"S.\",\"\"],[\"Rejkuba\",\"M.\",\"\"],[\"Bagnulo\",\"S.\",\"\"],[\"Izzo\",\"C.\",\"\"],[\"Marconi\",\"G.\",\"\"]]'),
(704.1750, 'Ekaterina Evstigneeva', 'E.A. Evstigneeva, M.J. Drinkwater, R. Jurek, P. Firth, J.B. Jones,\n  M.D. Gregg, S. Phillipps', 'Searches for Ultra-Compact Dwarf Galaxies in Galaxy Groups', '8 pages, 2 figures, accepted for publication in MNRAS', 'Mon.Not.Roy.Astron.Soc.378:1036-1042,2007', '10.1111/j.1365-2966.2007.11856.x', '', 'astro-ph', '', '  We present the results of a search for ultra-compact dwarf galaxies (UCDs) in\nsix different galaxy groups: Dorado, NGC1400, NGC0681, NGC4038, NGC4697 and\nNGC5084. We searched in the apparent magnitude range 17.5 < b_j < 20.5 (except\nNGC5084: 19.2 < b_j < 21.0). We found 1 definite plus 2 possible UCD candidates\nin the Dorado group and 2 possible UCD candidates in the NGC1400 group. No UCDs\nwere found in the other groups. We compared these results with predicted\nluminosities of UCDs in the groups according to the hypothesis that UCDs are\nglobular clusters formed in galaxies. The theoretical predictions broadly agree\nwith the observational results, but deeper surveys are needed to fully test the\npredictions.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:38:45 GMT\"}]', '2009-06-23', '[[\"Evstigneeva\",\"E. A.\",\"\"],[\"Drinkwater\",\"M. J.\",\"\"],[\"Jurek\",\"R.\",\"\"],[\"Firth\",\"P.\",\"\"],[\"Jones\",\"J. B.\",\"\"],[\"Gregg\",\"M. D.\",\"\"],[\"Phillipps\",\"S.\",\"\"]]'),
(704.1751, 'Olivier Rioul', 'Olivier Rioul', 'Information Theoretic Proofs of Entropy Power Inequalities', 'submitted for publication in the IEEE Transactions on Information\n  Theory, revised version', '', '10.1109/TIT.2010.2090193', '', 'cs.IT math.IT', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  While most useful information theoretic inequalities can be deduced from the\nbasic properties of entropy or mutual information, up to now Shannon\'s entropy\npower inequality (EPI) is an exception: Existing information theoretic proofs\nof the EPI hinge on representations of differential entropy using either Fisher\ninformation or minimum mean-square error (MMSE), which are derived from de\nBruijn\'s identity. In this paper, we first present an unified view of these\nproofs, showing that they share two essential ingredients: 1) a data processing\nargument applied to a covariance-preserving linear transformation; 2) an\nintegration over a path of a continuous Gaussian perturbation. Using these\ningredients, we develop a new and brief proof of the EPI through a mutual\ninformation inequality, which replaces Stam and Blachman\'s Fisher information\ninequality (FII) and an inequality for MMSE by Guo, Shamai and Verd\\\'u used in\nearlier proofs. The result has the advantage of being very simple in that it\nrelies only on the basic properties of mutual information. These ideas are then\ngeneralized to various extended versions of the EPI: Zamir and Feder\'s\ngeneralized EPI for linear transformations of the random variables, Takano and\nJohnson\'s EPI for dependent variables, Liu and Viswanath\'s\ncovariance-constrained EPI, and Costa\'s concavity inequality for the entropy\npower.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:42:07 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Aug 2010 10:41:34 GMT\"}]', '2016-11-17', '[[\"Rioul\",\"Olivier\",\"\"]]'),
(704.1752, 'Galina L. Klimchitskaya', 'E.V. Blagov, G.L. Klimchitskaya, V.M. Mostepanenko', 'Van der Waals interaction between a microparticle and a single-wall\n  carbon nanotube', '16 pages, 5 figures, to appear in Physical Review B', 'Phys. Rev. B, v.75, N23, 235413-(1-8), 2007', '10.1103/PhysRevB.75.235413', '', 'cond-mat.mtrl-sci quant-ph', '', '  The Lifshitz-type formulas describing the free energy and the force of the\nvan der Waals interaction between an atom (molecule) and a single-wall carbon\nnanotube are obtained. The single-wall nanotube is considered as a cylindrical\nsheet carrying a two-dimensional free electron gas with appropriate boundary\nconditions on the electromagnetic field. The obtained formulas are used to\ncalculate the van der Waals free energy and force between a hydrogen atom\n(molecule) and single-wall carbon nanotubes of different radia. Comparison\nstudies of the van der Waals interaction of hydrogen atoms with single- and\nmulti-wall carbon nanotubes show that depending on atom-nanotube separation\ndistance the idealization of graphite dielectric permittivity is already\napplicable to nanotubes with only two or three walls.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:54:50 GMT\"}]', '2009-11-13', '[[\"Blagov\",\"E. V.\",\"\"],[\"Klimchitskaya\",\"G. L.\",\"\"],[\"Mostepanenko\",\"V. M.\",\"\"]]'),
(704.1753, 'Buisseret Fabien Mr', 'F. Buisseret, C. Semay', 'Relativistic corrections for two- and three-body flux tube model', '10 pages; v2 accepted for publication (minor changes)', 'Phys.Rev.D76:017501,2007', '10.1103/PhysRevD.76.017501', '', 'hep-ph', '', '  We generalize the relativistic flux tube model for arbitrary two- or\nthree-body systems. The spin-independent and spin-dependent contributions of\nthe flux tube to the total Hamiltonian are computed in perturbation. In\nparticular, we show that the spin-dependent part exhibits a universal\nspin-orbit form: It does not depend on the nature of the confined particles.\nThe general equations we present, being well-defined for light particles, can\nthus be applied to usual as well as exotic hadrons such as hybrid mesons and\nglueballs.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:56:52 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 9 Jul 2007 14:41:41 GMT\"}]', '2008-11-26', '[[\"Buisseret\",\"F.\",\"\"],[\"Semay\",\"C.\",\"\"]]'),
(704.1754, 'Amir Kalev', 'A. Kalev and I. Hen', 'The No-Broadcasting Theorem and its Classical Counterpart', '4 pages', '', '10.1103/PhysRevLett.100.210502', '', 'quant-ph', '', '  Although it is widely accepted that `no-broadcasting\' -- the nonclonability\nof quantum information -- is a fundamental principle of quantum mechanics, an\nimpossibility theorem for the broadcasting of general density matrices has not\nyet been formulated. In this paper, we present a general proof for the\nno-broadcasting theorem, which applies to arbitrary density matrices. The proof\nrelies on entropic considerations, and as such can also be directly linked to\nits classical counterpart, which applies to probabilistic distributions of\nstatistical ensembles.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 12:59:53 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 26 Nov 2007 15:14:25 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 2 May 2008 15:49:00 GMT\"}]', '2009-11-13', '[[\"Kalev\",\"A.\",\"\"],[\"Hen\",\"I.\",\"\"]]'),
(704.1755, 'Lingaraj Sahu', 'Debashish Goswami and Lingaraj Sahu', 'Quantum random walks and vanishing of the second Hochschild cohomology', '', '', '10.1007/s11005-008-0233-z', '', 'math.OA', '', '  Given a conditionally completely positive map $\\mathcal L$ on a unital\n$\\ast$-algebra $\\A$, we find an interesting connection between the second\nHochschild cohomology of $\\A$ with coefficients in the bimodule $E_{\\mathcal\nL}=\\B^a(\\A \\oplus M)$ of adjointable maps, where $M$ is the GNS bimodule of\n$\\mathcal L$, and the possibility of constructing a quantum random walk (in the\nsense of \\cite{AP,LP,L,KBS}) corresponding to $\\mathcal L$.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 13:00:56 GMT\"}]', '2009-11-13', '[[\"Goswami\",\"Debashish\",\"\"],[\"Sahu\",\"Lingaraj\",\"\"]]'),
(704.1756, 'Jose M. Martin-Garcia', 'Jose M. Martin-Garcia, Renato Portugal, Leon R. U. Manssur', 'The Invar Tensor Package', 'Accepted in Computer Physics Communications. Package can be\n  downloaded from http://metric.iem.csic.es/Martin-Garcia/xAct/Invar/\n  (Mathematica version) or http://www.lncc.br/~portugal/Invar.html (Maple\n  version)', 'Comp. Phys. Commun. 177 (2007) 640-648', '10.1016/j.cpc.2007.05.015', '', 'cs.SC gr-qc hep-th', '', '  The Invar package is introduced, a fast manipulator of generic scalar\npolynomial expressions formed from the Riemann tensor of a four-dimensional\nmetric-compatible connection. The package can maximally simplify any polynomial\ncontaining tensor products of up to seven Riemann tensors within seconds. It\nhas been implemented both in Mathematica and Maple algebraic systems.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 13:03:59 GMT\"}]', '2015-05-13', '[[\"Martin-Garcia\",\"Jose M.\",\"\"],[\"Portugal\",\"Renato\",\"\"],[\"Manssur\",\"Leon R. U.\",\"\"]]'),
(704.1757, 'Andrea Macrina', 'Andrea Macrina', 'Towards a Gauge Invariant Scattering Theory of Cylindrical Gravitational\n  Waves', 'MSc Thesis, University of Bern (2002)', '', '', '', 'gr-qc', '', '  In this account we investigate an asymptotically flat space-time geometry. In\nparticular, we focus on a pure gravity model with cylindrical symmetry where no\nmatter fields are included. The Einstein-Rosen metric is introduced and the\ncorresponding Einstein equations are solved. By use of the ADM formalism, we\nderive the observables of the cylindrical gravitational waves. We conclude with\nan analysis of the algebra of the observables of the Einstein-Rosen waves.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 13:25:31 GMT\"}]', '2007-05-23', '[[\"Macrina\",\"Andrea\",\"\"]]'),
(704.1758, 'George Poulipoulis', 'G. N. Throumoulopoulos, H. Tasso and G. Poulipoulis', 'On axisymmetric MHD equilibria with incompressible flows under side\n  conditions', '19 pages, 1 table, 6 figures', '', '', '', 'physics.plasm-ph', '', '  Axisymmetric equilibria with incompressible flows of arbitrary direction are\nstudied in the framework of magnetohydrodynamics under a variety of physically\nrelevant side conditions. To this end a set of pertinent non-linear ODEs are\ntransformed to quasilinear ones and the respective initial value problem is\nsolved numerically with appropriately determined initial values near the\nmagnetic axis. Several equilibria are then constructed surface by surface. The\nnon field aligned flow results in novel configurations with a single magnetic\naxis, toroidal shell configurations in which the plasma is confined within a\ncouple of magnetic surfaces and double shell-like configurations. In addition,\nthe flow affects the elongation and triangularity of the magnetic surfaces.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 13:25:33 GMT\"}]', '2007-05-23', '[[\"Throumoulopoulos\",\"G. N.\",\"\"],[\"Tasso\",\"H.\",\"\"],[\"Poulipoulis\",\"G.\",\"\"]]'),
(704.1759, 'Corina Calinescu', 'Corina Calinescu, James Lepowsky, Antun Milas', 'Vertex-algebraic structure of the principal subspaces of certain\n  A_1^(1)-modules, I: level one case', '20 pages. To appear in International J. of Math', 'Int.J.Math.19:71-92,2008', '10.1142/S0129167X08004571', '', 'math.QA hep-th math.RT', '', '  This is the first in a series of papers in which we study vertex-algebraic\nstructure of Feigin-Stoyanovsky\'s principal subspaces associated to standard\nmodules for both untwisted and twisted affine Lie algebras. A key idea is to\nprove suitable presentations of principal subspaces, without using bases or\neven ``small\'\' spanning sets of these spaces. In this paper we prove\npresentations of the principal subspaces of the basic A_1^(1)-modules. These\nconvenient presentations were previously used in work of\nCapparelli-Lepowsky-Milas for the purpose of obtaining the classical\nRogers-Ramanujan recursion for the graded dimensions of the principal\nsubspaces.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 13:30:40 GMT\"}]', '2008-11-26', '[[\"Calinescu\",\"Corina\",\"\"],[\"Lepowsky\",\"James\",\"\"],[\"Milas\",\"Antun\",\"\"]]'),
(704.1760, 'Pieter van Dokkum', 'Pieter van Dokkum, Ryan Quadri', 'Galaxy Evolution and Environment', 'To appear in the proceedings of the Cosmic Frontiers conference\n  (Durham, UK). 8 pages, 5 figures', '', '', '', 'astro-ph', '', '  The properties of galaxies are strongly correlated with their environment,\nwith red galaxies dominating galaxy clusters and blue galaxies dominating the\ngeneral field. However, not all field galaxies are young: studies of the\ncolors, line strengths, and M/L ratios of massive early-type galaxies at\n0<z<1.3 show that the most massive galaxies do not seem to care about their\nsurroundings, and have very similar ages irrespective of their environment.\nThere is good evidence that the growth of these galaxies does continue longer\nin the field than in clusters, via (nearly) dissipationless mergers of already\nold galaxies. These results are consistent with predictions of recent galaxy\nformation models, which incorporate AGN feedback to suppress star formation in\nthe most massive halos. Systematic studies of the relation of galaxies with\ntheir environment beyond z=1 are difficult, and still somewhat contradictory.\nIntriguingly both the DEEP2 and VVDS surveys find that the color-density\nrelation disappears at z~1.3, unfortunately just at the point where both\nsurveys become highly incomplete. On the other hand, clustering studies at\nz~2.5 have shown that red galaxies cluster more strongly than blue galaxies,\nimplying that the color-density relation was already in place at that redshift.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:44:07 GMT\"}]', '2007-05-23', '[[\"van Dokkum\",\"Pieter\",\"\"],[\"Quadri\",\"Ryan\",\"\"]]'),
(704.1761, 'Eric R. Sharpe', 'R. Donagi, E. Sharpe', 'GLSM\'s for partial flag manifolds', '57 pp, LaTeX; v3: refs added, material on weighted Grassmannians\n  added', 'J.Geom.Phys.58:1662-1692,2008', '10.1016/j.geomphys.2008.07.010', '', 'hep-th', '', '  In this paper we outline some aspects of nonabelian gauged linear sigma\nmodels. First, we review how partial flag manifolds (generalizing\nGrassmannians) are described physically by nonabelian gauged linear sigma\nmodels, paying attention to realizations of tangent bundles and other aspects\npertinent to (0,2) models. Second, we review constructions of Calabi-Yau\ncomplete intersections within such flag manifolds, and properties of the gauged\nlinear sigma models. We discuss a number of examples of nonabelian GLSM\'s in\nwhich the Kahler phases are not birational, and in which at least one phase is\nrealized in some fashion other than as a complete intersection, extending\nprevious work of Hori-Tong. We also review an example of an abelian GLSM\nexhibiting the same phenomenon. We tentatively identify the mathematical\nrelationship between such non-birational phases, as examples of Kuznetsov\'s\nhomological projective duality. Finally, we discuss linear sigma model moduli\nspaces in these gauged linear sigma models. We argue that the moduli spaces\nbeing realized physically by these GLSM\'s are precisely Quot and hyperquot\nschemes, as one would expect mathematically.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:06:31 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 14 Apr 2007 02:15:29 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 30 Aug 2007 23:56:18 GMT\"}]', '2008-11-26', '[[\"Donagi\",\"R.\",\"\"],[\"Sharpe\",\"E.\",\"\"]]'),
(704.1762, 'Sean Brittain', 'E. L. Gibb (1), K. A. Van Brunt (1), S. D. Brittain (2), T. W. Rettig\n  (3) ((1) University of Missouri - St. Louis, (2) Clemson University, (3)\n  University of Notre Dame)', 'Warm HCN, C2H2, and CO in the disk of GV Tau', '23 pages, 6 figures, accepted by ApJ', 'Astrophys.J.660:1572-1579,2007', '10.1086/513502', '', 'astro-ph', '', '  We present the first high-resolution, ground-based observations of HCN and\nC2H2 toward the T Tauri binary star system GV Tau. We detected strong\nabsorption due to HCN nu_3 and weak C2H2 (nu_3 and nu_2 + (nu_4 + nu_5)^0_+)\nabsorption toward the primary (GV Tau S) but not the infrared companion. We\nalso report CO column densities and rotational temperatures, and present\nabundances relative to CO of HCN/CO ~0.6% and C2H2/CO ~1.2% and an upper limit\nfor CH4/CO < 0.37% toward GV Tau S. Neither HCN nor C2H2 were detected toward\nthe infrared companion and results suggest that abundances may differ between\nthe two sources.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:14:52 GMT\"}]', '2009-06-23', '[[\"Gibb\",\"E. L.\",\"\"],[\"Van Brunt\",\"K. A.\",\"\"],[\"Brittain\",\"S. D.\",\"\"],[\"Rettig\",\"T. W.\",\"\"]]'),
(704.1763, 'Ilia Solov\'yov', 'Ilia A. Solov\'yov, Walter Greiner', 'Towards understanding of birds magnetoreceptor mechanism', '10 pages, 4 figures', '', '', '', 'physics.bio-ph', '', '  In the present letter we suggest a new theoretical model for a quantitative\ndescription of the magnetoreception mechanism in birds. The considered\nmechanism involves two types of iron minerals (magnetite and maghemite) which\nwere found in subcellular compartments within sensory dendrites of the upper\nbeak of several bird species. The analysis of forces acting between the iron\nparticles shows that the orientation of the external geomagnetic field can\nsignificantly change the probability of the mechanosensitive ion channels\nopening and closing. The performed theoretical analysis shows that the\nsuggested magnetoreceptor system might be a sensitive biological magnetometer\nproviding an essential part of the magnetic map for navigation.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:21:55 GMT\"}]', '2007-05-23', '[[\"Solov\'yov\",\"Ilia A.\",\"\"],[\"Greiner\",\"Walter\",\"\"]]'),
(704.1764, 'Scott Guthery Dr.', 'Scott B. Guthery', 'Another Riemann-Farey Computation', '6 pages, 2 figures', '', '', '', 'math.GM', '', '  Another approach to constructing an upper bound for the Riemann-Farey sum is\ndescribed.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:28:42 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 15 May 2007 19:53:23 GMT\"}]', '2007-05-23', '[[\"Guthery\",\"Scott B.\",\"\"]]'),
(704.1765, 'Anna Sajina', 'Anna Sajina (1), Lin Yan (1), Lee Armus (1), Phil Choi (2), Dario\n  Fadda (3), George Helou (1), Henrik Spoon (4)((1)Spitzer Science Center, (2)\n  Pomona College, (3) Herschel Science Center, (4) Cornell)', 'Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2\n  II: Diagnostics', '60 pages, 15 figures, accepted for publication in ApJ', 'Astrophys.J.664:713-737,2007', '10.1086/519446', '', 'astro-ph', '', '  We present mid-IR spectral decomposition of a sample of 48 Spitzer-selected\nULIRGs spanning z~1-3 and likely L_IR~10^12-10^13Lsun. Our study aims at\nquantifying the star-formation and AGN processes in these sources which recent\nresults suggest have evolved strongly between the observed epoch and today. To\ndo this, we study the mid-IR contribution of PAH emission, continuum, and\nextinction. About 3/4 of our sample are continuum- (i.e. AGN) dominated\nsources, but ~60% of these show PAH emission, suggesting the presence of\nstar-formation activity. These sources have redder mid-IR colors than typical\noptically-selected quasars. About 25% of our sample have strong PAH emission,\nbut none are likely to be pure starbursts as reflected in their relatively high\n5um hot dust continua. However, their steep 30um-to-14um slopes suggest that\nstar-formation might dominate the total infrared luminosity. Six of our z~2\nsources have EW6.2>~0.3um and L_14um>~10^12Lsun (implying L_IR>~10^13Lsun). At\nthese luminosities, such high EW6.2 ULIRGs do not exist in the local Universe.\nWe find a median optical depth at 9.7um of <tau_9.7>=1.4. This is consistent\nwith local IRAS-selected ULIRGs, but differs from early results on\nSCUBA-selected z~2 ULIRGs. Similar to local ULIRGs about 25% of our sample show\nextreme obscuration (tau_9.7>~3) suggesting buried nuclei. In general, we find\nthat our sources are similar to local ULIRGs, but are an order of magnitude\nmore luminous. It is not clear whether our z~2 ULIRGs are simply scaled-up\nversions of local ULIRGs, or subject to fundamentally different physical\nprocesses.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:36:12 GMT\"}]', '2009-06-23', '[[\"Sajina\",\"Anna\",\"\"],[\"Yan\",\"Lin\",\"\"],[\"Armus\",\"Lee\",\"\"],[\"Choi\",\"Phil\",\"\"],[\"Fadda\",\"Dario\",\"\"],[\"Helou\",\"George\",\"\"],[\"Spoon\",\"Henrik\",\"\"]]'),
(704.1766, 'Oscar Esquivel', 'O. Esquivel, B. Fuchs', 'Jeans instability of a galactic disk embedded in a live dark halo', '3 pages, 1 figure, accepted by Astron. Astrophys', '', '10.1051/0004-6361:20077372', '', 'astro-ph', '', '  We investigate the Jeans instability of a galactic disk embedded in a\ndynamically responsive dark halo. It is shown that the disk-halo system becomes\nnominally Jeans unstable. On small scales the instability is suppressed, if the\nToomre stability index Q_T is higher than a certain threshold, but on large\nscales the Jeans instability sets invariably in. However, using a simple\nself-consistent disk-halo model it is demonstrated that this occurs on scales\nwhich are much larger than the system so that this is indeed only a nominal\neffect. From a practical point of view the Jeans instability of galactic disks\nis not affected by a live dark halo.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:37:31 GMT\"}]', '2009-11-13', '[[\"Esquivel\",\"O.\",\"\"],[\"Fuchs\",\"B.\",\"\"]]'),
(704.1767, 'Markus Mugrauer', 'M. Mugrauer, A. Seifahrt, R. Neuhaeuser', 'The multiplicity of planet host stars - New low-mass companions to\n  planet host stars', 'MNRAS accepted, 8 pages, 6 figures, and 1 table', 'Mon.Not.Roy.Astron.Soc.378:1328-1334,2007', '10.1111/j.1365-2966.2007.11858.x', '', 'astro-ph', '', '  We present new results from our ongoing multiplicity study of exoplanet host\nstars, carried out with the infrared camera SofI at ESO-NTT. We have identified\nnew low mass companions to the planet host stars HD101930 and HD65216.\nHD101930AB is a wide binary systems composed of the planet host star HD101930A\nand its companion HD101930B which is a M0 to M1 dwarf with a mass of about\n0.7Msun separated from the primary by ~73arcsec (2200AU projected separation).\nHD65216 forms a hierarchical triple system, with a projected separation of\n253AU (angular separation of about 7arcsec) between the planet host star\nHD65216A and its close binary companion HD65216BC, whose two components are\nseparated by only ~0.17arcsec (6AU of projected separation). Two VLT-NACO\nimages separated by 3 years confirm that this system is co-moving to the planet\nhost star. The infrared photometry of HD65216B and C is consistent with a M7 to\nM8 (0.089Msun), and a L2 to L3 dwarf (0.078Msun), respectively, both close to\nthe sub-stellar limit. An infrared spectrum with VLT-ISAAC of the pair\nHD65216BC, even though not resolved spatially, confirms this late spectral\ntype. Furthermore, we present H- and K-band ISAAC infrared spectra of HD16141B,\nthe recently detected co-moving companion of the planet host star HD16141A. The\ninfrared spectroscopy as well as the apparent infrared photometry of HD16141B\nare both fully consistent with a M2 to M3 dwarf located at the distance of the\nplanet host star.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:19:57 GMT\"}]', '2009-06-23', '[[\"Mugrauer\",\"M.\",\"\"],[\"Seifahrt\",\"A.\",\"\"],[\"Neuhaeuser\",\"R.\",\"\"]]'),
(704.1768, 'Enrique ter Horst A', 'Henryk Gzyl, German Molina, Enrique ter Horst', 'Assessment and Propagation of Input Uncertainty in Tree-based Option\n  Pricing Models', '39 pages, 21 figures', '', '', '', 'cs.CE cs.GT', '', '  This paper aims to provide a practical example on the assessment and\npropagation of input uncertainty for option pricing when using tree-based\nmethods. Input uncertainty is propagated into output uncertainty, reflecting\nthat option prices are as unknown as the inputs they are based on. Option\npricing formulas are tools whose validity is conditional not only on how close\nthe model represents reality, but also on the quality of the inputs they use,\nand those inputs are usually not observable. We provide three alternative\nframeworks to calibrate option pricing tree models, propagating parameter\nuncertainty into the resulting option prices. We finally compare our methods\nwith classical calibration-based results assuming that there is no options\nmarket established. These methods can be applied to pricing of instruments for\nwhich there is not an options market, as well as a methodological tool to\naccount for parameter and model uncertainty in theoretical option pricing.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:48:41 GMT\"}]', '2007-05-23', '[[\"Gzyl\",\"Henryk\",\"\"],[\"Molina\",\"German\",\"\"],[\"ter Horst\",\"Enrique\",\"\"]]'),
(704.1769, 'Ralf Metzler', 'Michael A. Lomholt, Irwin M. Zaid, Ralf Metzler', 'Subdiffusion and weak ergodicity breaking in the presence of a reactive\n  boundary', '4 pages, 1 figure, REVTeX4, accepted to Phys Rev Lett, some typos\n  corrected', 'Phys. Rev. Lett. 98, 200603 (2007)', '10.1103/PhysRevLett.98.200603', '', 'cond-mat.stat-mech cond-mat.soft', '', '  We derive the boundary condition for a subdiffusive particle interacting with\na reactive boundary with finite reaction rate. Molecular crowding conditions,\nthat are found to cause subdiffusion of larger molecules in biological cells,\nare shown to effect long-tailed distributions with identical exponent for both\nthe unbinding times from the boundary to the bulk and the rebinding times from\nthe bulk. This causes a weak ergodicity breaking: typically, an individual\nparticle either stays bound or remains in the bulk for very long times. We\ndiscuss why this may be beneficial for in vivo gene regulation by DNA-binding\nproteins, whose typical concentrations are nanomolar\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:56:57 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 10 May 2007 13:27:03 GMT\"}]', '2008-06-02', '[[\"Lomholt\",\"Michael A.\",\"\"],[\"Zaid\",\"Irwin M.\",\"\"],[\"Metzler\",\"Ralf\",\"\"]]'),
(704.1770, 'Laura V. Sales', 'L. V. Sales, J. F. Navarro, M. G. Abadi and M. Steinmetz', 'Satellites of Simulated Galaxies: survival, merging, and their relation\n  to the dark and stellar halos', '13 pages, 11 figures, MNRAS in press. Accepted version with minor\n  changes. Version with high resolution figures available at:\n  http://www.astro.uvic.ca/~lsales/SatPapers/SatPapers.html', 'Mon.Not.Roy.Astron.Soc.379:1464-1474,2007', '10.1111/j.1365-2966.2007.12024.x', '', 'astro-ph', '', '  We study the population of satellite galaxies formed in a suite of\nN-body/gasdynamical simulations of galaxy formation in a LCDM universe. We find\nlittle spatial or kinematic bias between the dark matter and the satellite\npopulation. The velocity dispersion of the satellites is a good indicator of\nthe virial velocity of the halo: \\sigma_{sat}/V_{vir}=0.9 +/- 0.2. Applied to\nthe Milky Way and M31 this gives V_{vir}^{MW}=109 +/- 22$ km/s and\nV_{vir}^{M31} = 138 +/- 35 km/s, respectively, substantially lower than the\nrotation speed of their disk components. The detailed kinematics of simulated\nsatellites and dark matter are also in good agreement. By contrast, the stellar\nhalo of the simulated galaxies is kinematically and spatially distinct from the\npopulation of surviving satellites. This is because the survival of a satellite\ndepends on mass and on time of accretion; surviving satellites are biased\ntoward low-mass systems that have been recently accreted by the galaxy. Our\nresults support recent proposals for the origin of the systematic differences\nbetween stars in the Galactic halo and in Galactic satellites: the elusive\n``building blocks\'\' of the Milky Way stellar halo were on average more massive,\nand were accreted (and disrupted) earlier than the population of dwarfs that\nhas survived self-bound until the present.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:56:44 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 24 May 2007 16:02:05 GMT\"}]', '2009-06-23', '[[\"Sales\",\"L. V.\",\"\"],[\"Navarro\",\"J. F.\",\"\"],[\"Abadi\",\"M. G.\",\"\"],[\"Steinmetz\",\"M.\",\"\"]]'),
(704.1771, 'Vasily E. Tarasov', 'Vasily E. Tarasov, George M. Zaslavsky', 'Fractional Generalization of Kac Integral', '16 pages, LaTeX', 'Communications in Nonlinear Science and Numerical Simulation.\n  Vol.13. No.2. (2008) 248-258', '10.1016/j.cnsns.2007.04.020', '', 'math-ph cond-mat.other math.MP nlin.CD physics.class-ph', '', '  Generalization of the Kac integral and Kac method for paths measure based on\nthe Levy distribution has been used to derive fractional diffusion equation.\nApplication to nonlinear fractional Ginzburg-Landau equation is discussed.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 14:58:46 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 7 May 2007 14:32:36 GMT\"}]', '2015-03-12', '[[\"Tarasov\",\"Vasily E.\",\"\"],[\"Zaslavsky\",\"George M.\",\"\"]]'),
(704.1772, 'Anisa Bajkova', 'Vadim V. Bobylev, and Anisa T. Bajkova', 'Analysis of the Velocity Field of F and G Dwarfs in the Solar\n  Neighborhood as a Function of Age', '13 pages, 6 figures, 3 tables', 'Astron.Rep.51:327-381,2007', '10.1134/S1063772907050034', '', 'astro-ph', '', '  The space velocities from the catalog of Nordstrom et al. (2004) are used to\ntrace variations of a number of kinematic parameters of single F and G dwarfs\nas a function of their age. The vertex deviation of disk stars increases from\n7+- 1 to 15+-2 degrees as the mean age decreases from 4.3 to 1.5 Gyr. The\ntwo-dimensional velocity distributions in the UV, UW, and VW planes are\nanalyzed. The evolution of the main peaks in the velocity distributions can be\nfollowed to an average age of approximately 9 Gyr. We find that: (1) in the\ndistributions of the UV velocity components, stars of different types are\nconcentrated toward several stable peaks (the Hyades, Pleiades, and Sirius\nCluster), suggesting that the stars belonging to these formations did not form\nsimultaneously; (2) the peak associated with the Hyades Cluster dominates in\nall age intervals; and (3) the Hyades peak is strongest for stars with an\naverage age of 1.5 Gyr, suggesting that this peak contains a considerable\nfraction of stars from the Hyades cluster. The age dependences of the kinematic\nparameters exhibit a break near 4.5 Gyr, which can be explained as an effect of\nthe different contributions of stars of the thin and thick disks. The Stromberg\nrelation yields a solar LSR velocity of V_{\\odot LSR} = (8.7, 6.2, 7.2)+- (0.5,\n2.2, 0.8) km/s.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:03:23 GMT\"}]', '2009-06-23', '[[\"Bobylev\",\"Vadim V.\",\"\"],[\"Bajkova\",\"Anisa T.\",\"\"]]'),
(704.1773, 'Laura V. Sales', 'L. V. Sales, J. F. Navarro, M. G. Abadi and M. Steinmetz', 'Cosmic M\\\'enage \\`a Trois: The Origin of Satellite Galaxies On Extreme\n  Orbits', '10 pages, 6 figures, MNRAS in press. Accepted version with minor\n  changes. Version with high resolution figures available at:\n  http://www.astro.uvic.ca/~lsales/SatPapers/SatPapers.html', 'Mon.Not.Roy.Astron.Soc.379:1475-1483,2007', '10.1111/j.1365-2966.2007.12026.x', '', 'astro-ph', '', '  We examine the orbits of satellite galaxies identified in a suite of\nN-body/gasdynamical simulations of the formation of $L_*$ galaxies in a LCDM\nuniverse. Most satellites follow conventional orbits; after turning around,\nthey accrete into their host halo and settle on orbits whose apocentric radii\nare steadily eroded by dynamical friction. However, a number of outliers are\nalso present, we find that ~1/3 of satellites identified at $z=0$ are on\nunorthodox orbits, with apocenters that exceed their turnaround radii. This\npopulation of satellites on extreme orbits consists typically of the faint\nmember of a satellite pair that has been ejected onto a highly-energetic orbit\nduring its first approach to the primary. Since the concurrent accretion of\nmultiple satellite systems is a defining feature of hierarchical models of\ngalaxy formation, we speculate that this three-body ejection mechanism may be\nthe origin of (i) some of the newly discovered high-speed satellites around M31\n(such as Andromeda XIV); (ii) some of the distant fast-receding Local Group\nmembers, such as Leo I; and (iii) the oddly isolated dwarf spheroidals Cetus\nand Tucana in the outskirts of the Local Group. Our results suggest that care\nmust be exercised when using the orbits of the most weakly bound satellites to\nplace constraints on the total mass of the Local Group.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:06:16 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 24 May 2007 15:07:52 GMT\"}]', '2009-06-23', '[[\"Sales\",\"L. V.\",\"\"],[\"Navarro\",\"J. F.\",\"\"],[\"Abadi\",\"M. G.\",\"\"],[\"Steinmetz\",\"M.\",\"\"]]'),
(704.1774, 'Francesco Pederiva', 'S. Gandolfi, F. Pederiva, S. Fantoni, K.E. Schmidt', 'Auxiliary Field Diffusion Monte Carlo calculation of nuclei with A<40\n  with tensor interactions', '4 pages, no figures', 'Phys.Rev.Lett.99:022507,2007', '10.1103/PhysRevLett.99.022507', '', 'nucl-th', '', '  We calculate the ground-state energy of 4He, 8He, 16O, and 40Ca using the\nauxiliary field diffusion Monte Carlo method in the fixed phase approximation\nand the Argonne v6\' interaction which includes a tensor force. Comparison of\nour light nuclei results to those of Green\'s function Monte Carlo calculations\nshows the accuracy of our method for both open and closed shell nuclei. We also\napply it to 16O and 40Ca to show that quantum Monte Carlo methods are now\napplicable to larger nuclei.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:06:29 GMT\"}]', '2008-11-26', '[[\"Gandolfi\",\"S.\",\"\"],[\"Pederiva\",\"F.\",\"\"],[\"Fantoni\",\"S.\",\"\"],[\"Schmidt\",\"K. E.\",\"\"]]'),
(704.1775, 'Lam Yu', 'Lam H. Yu, Christopher D. Zangmeister, James G. Kushmerick', 'Origin of Discrepancies in Inelastic Electron Tunneling Spectra of\n  Molecular Junctions', '4 pages, 4 figures accepted for publication in Physical Review\n  Letters', '', '10.1103/PhysRevLett.98.206803', '', 'cond-mat.mes-hall cond-mat.other', '', '  We report inelastic electron tunneling spectroscopy (IETS) of multilayer\nmolecular junctions with and without incorporated metal nano-particles. The\nincorporation of metal nanoparticles into our devices leads to enhanced IET\nintensity and a modified line-shape for some vibrational modes. The enhancement\nand line-shape modification are both the result of a low lying hybrid metal\nnanoparticle-molecule electronic level. These observations explain the apparent\ndiscrepancy between earlier IETS measurements of alkane thiolate junctions by\nKushmerick \\emph{et al.} [Nano Lett. \\textbf{4}, 639 (2004)] and Wang \\emph{et\nal.} [Nano Lett. \\textbf{4}, 643 (2004)].\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:11:18 GMT\"}]', '2009-11-13', '[[\"Yu\",\"Lam H.\",\"\"],[\"Zangmeister\",\"Christopher D.\",\"\"],[\"Kushmerick\",\"James G.\",\"\"]]'),
(704.1776, 'Joerg Junkersfeld', 'H. van Pee, O. Bartholomy, V. Crede (for the CB-ELSA Collaboration)', 'Photoproduction of pi0-mesons off protons from the Delta(1232) region to\n  E(gamma) = 3 GeV', '17 pages, 17 figures', 'Eur.Phys.J.A31:61-77,2007', '10.1140/epja/i2006-10160-3', '', 'nucl-ex', '', '  Photoproduction of pi0 mesons was studied with the Crystal-Barrel detector at\nELSA for incident energies from 300 MeV to 3 GeV. Differential cross sections d\nsigma /d Omega, d sigma/d t, and the total cross section are presented. For\nE(gamma) < 3 GeV, the angular distributions agree well with the SAID\nparametrization. At photon energies above 1.5 GeV, a strong forward peaking\nindicates t-channel exchange to be the dominant process. The rapid variations\nof the cross section with energy and angle indicate production of resonances.\nAn interpretation of the data within the Bonn-Gatchina partial wave analysis is\nbriefly discussed.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:12:37 GMT\"}]', '2019-08-14', '[[\"van Pee\",\"H.\",\"\",\"for the CB-ELSA Collaboration\"],[\"Bartholomy\",\"O.\",\"\",\"for the CB-ELSA Collaboration\"],[\"Crede\",\"V.\",\"\",\"for the CB-ELSA Collaboration\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1777, 'Hyun-Chul Kim', 'H.-Ch. Kim, Gh.-S. Yang, and K. Goeke', 'Magnetic and axial-vector transitions of the baryon antidecuplet', '8 pages, 5 figures, Talk given at the Yukawa International Seminar\n  (YKIS) 2006, \"New frontiers in QCD\", Kyoto, Japan, 20 Nov. - 8 Dec. 2006', 'Prog.Theor.Phys.Suppl.168:62-69,2007', '10.1143/PTPS.168.62', 'PNU-NTG-03/2007', 'hep-ph', '', '  We report the recent results of the magnetic transitions and axial-vector\ntransitions of the baryon antidecuplet within the framework of the chiral\nquark-soliton model. The dynamical model parameters are fixed by experimental\ndata for the magnetic moments of the baryon octet, for the hyperon semileptonic\ndecay constants, and for the singlet axial-vector constant. The transition\nmagnetic moments $\\mu_{\\Lambda\\Sigma}$ and $\\mu_{N\\Delta}$ are well reproduced\nand other octet-decuplet and octet-antidecuplet transitions are predicted. In\nparticular, the present calculation of $\\mu_{\\Sigma\\Sigma^*}$ is found to be\nbelow the upper bound $0.82\\mu_N$ that the SELEX collaboration measured very\nrecently. The results explains consistently the recent findings of a new $N^*$\nresonance from the GRAAL and Tohoku LNS group. We also obtain the transition\naxial-vector constants for the $\\Theta^+\\to KN$ from which the decay width of\nthe $\\Theta^{+}$ pentaquark baryon is determined as a function of the\npion-nucleon sigma term $\\Sigma_{\\pi N}$. We investigate the dependence of the\ndecay width of the $\\Theta^{+}$ on the $g_{A}^{(0)}$, with the $g_{A}^{(0)}$\nvaried within the range of the experimental uncertainty. We show that a small\ndecay width of the $\\Theta^{+}\\to KN$, i.e. $\\Gamma_{\\Theta KN} \\leq 1$ MeV, is\ncompatible with the values of all known semileptonic decays with the generally\naccepted value of $g_{A}^{(0)} \\approx 0.3$ for the proton.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:12:39 GMT\"}]', '2008-11-26', '[[\"Kim\",\"H. -Ch.\",\"\"],[\"Yang\",\"Gh. -S.\",\"\"],[\"Goeke\",\"K.\",\"\"]]'),
(704.1778, 'Jonathon Peterson', 'Jonathon Peterson, Ofer Zeitouni', 'Quenched limits for transient, zero speed one-dimensional random walk in\n  random environment', 'Published in at http://dx.doi.org/10.1214/08-AOP399 the Annals of\n  Probability (http://www.imstat.org/aop/) by the Institute of Mathematical\n  Statistics (http://www.imstat.org)', 'Annals of Probability 2009, Vol. 37, No. 1, 143-188', '10.1214/08-AOP399', 'IMS-AOP-AOP399', 'math.PR', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We consider a nearest-neighbor, one dimensional random walk\n$\\{X_n\\}_{n\\geq0}$ in a random i.i.d. environment, in the regime where the walk\nis transient but with zero speed, so that $X_n$ is of order $n^s$ for some\n$s<1$. Under the quenched law (i.e., conditioned on the environment), we show\nthat no limit laws are possible: There exist sequences $\\{n_k\\}$ and $\\{x_k\\}$\ndepending on the environment only, such that $X_{n_k}-x_k=o(\\log n_k)^2$ (a\nlocalized regime). On the other hand, there exist sequences $\\{t_m\\}$ and\n$\\{s_m\\}$ depending on the environment only, such that $\\log s_m/\\log t_m\\to\ns<1$ and $P_{\\omega}(X_{t_m}/s_m\\leq x)\\to1/2$ for all $x>0$ and $\\to0$ for\n$x\\leq0$ (a spread out regime).\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:12:46 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 23 Feb 2011 12:02:32 GMT\"}]', '2011-02-24', '[[\"Peterson\",\"Jonathon\",\"\"],[\"Zeitouni\",\"Ofer\",\"\"]]'),
(704.1779, 'Simonetta Abenda', 'S. Abenda, T. Grava', 'Reciprocal transformations and flat metrics on Hurwitz spaces', '25 pages', 'J. Phys. A: Math. Theor. 40 (2007) 10769-10790', '10.1088/1751-8113/40/35/004', '', 'nlin.SI math-ph math.MP', '', '  We consider hydrodynamic systems which possess a local Hamiltonian structure\nof Dubrovin-Novikov type. To such a system there are also associated an\ninfinite number of nonlocal Hamiltonian structures. We give necessary and\nsufficient conditions so that, after a nonlinear transformation of the\nindependent variables, the reciprocal system still possesses a local\nHamiltonian structure of Dubrovin-Novikov type. We show that, under our\nhypotheses, bi-hamiltonicity is preserved by the reciprocal transformation.\nFinally we apply such results to reciprocal systems of genus g Whitham-KdV\nmodulation equations.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:15:01 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 9 Jul 2007 18:13:02 GMT\"}]', '2009-02-26', '[[\"Abenda\",\"S.\",\"\"],[\"Grava\",\"T.\",\"\"]]'),
(704.1780, 'Amornrat Aungwerojwit', 'A. Aungwerojwit, B. T. Gaensicke, P. Rodriguez-Gil, H.-J. Hagen, O.\n  Giannakis, C. Papadimitriou, C. Allende Prieto and D. Engels', 'HS1857+5144: A hot and young pre-cataclysmic variable', 'accepted for publication in A&A, 10 pages, 9 figures', '', '10.1051/0004-6361:20077276', '', 'astro-ph', '', '  We report the discovery of a new white dwarf/M dwarf binary, HS1857+5144,\nidentified in the Hamburg Quasar Survey (HQS). Time-resolved optical\nspectroscopy and photometry were carried out to determine the properties of\nthis new cataclysmic variable progenitor pre-CV). The light curves of\nHS1857+5144 display a sinusoidal variation with a period of Porb=383.52 min and\npeak-to-peak amplitudes of 0.7 mag and 1.1 mag in the B-band and R-band,\nrespectively. The large amplitude of the brightness variation results from a\nreflection effect on the heated inner hemisphere of the companion star,\nsuggesting a very high temperature of the white dwarf. Our radial velocity\nstudy confirms the photometric period as the orbital period of the system. A\nmodel atmosphere fit to the spectrum of the white dwarf obtained at minimum\nlight provides limits to its mass and temperature of Mwd=~0.6-1.0 Msun and\nTwd=~70000-100000 K, respectively. The detection of HeII 4686 absorption\nclassifies the primary star of HS1857+5144 as a DAO white dwarf. Combining the\nresults from our spectroscopy and photometry, we estimate the mass of the\ncompanion star and the binary inclination to be Msec=~0.15-0.30 Msun and\ni=~45-55 deg, respectively. We classify HS1857+5144 as one of the youngest\npre-CV known to date. The cooling age of the white dwarf suggests that the\npresent system has just emerged from a common envelope phase ~10^5 yr ago.\nHS1857+5144 will start mass transfer within or below the 2-3h period gap.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:17:00 GMT\"}]', '2009-11-13', '[[\"Aungwerojwit\",\"A.\",\"\"],[\"Gaensicke\",\"B. T.\",\"\"],[\"Rodriguez-Gil\",\"P.\",\"\"],[\"Hagen\",\"H. -J.\",\"\"],[\"Giannakis\",\"O.\",\"\"],[\"Papadimitriou\",\"C.\",\"\"],[\"Prieto\",\"C. Allende\",\"\"],[\"Engels\",\"D.\",\"\"]]'),
(704.1781, 'Angela Bonaccorso', 'G. Blanchon (INFN and Physics Department, Pisa), A. Bonaccorso (INFN\n  and Physics Department, Pisa), D.M. Brink (Oxford University), N. Vinh Mau\n  (IPN, Orsay)', '$^{10}$Li spectrum from $^{11}$Li fragmentation', '15 pages, 4 figures, 3 tables. Accepted for publication in\n  Nucl.Phys.A', 'Nucl.Phys.A791:303-312,2007', '10.1016/j.nuclphysa.2007.04.014', '', 'nucl-th nucl-ex', '', '  A recently developed time dependent model for the excitation of a nucleon\nfrom a bound state to a continuum resonant state in the system n+core is\napplied to the study of the population of the low energy continuum of the\nunbound $^{10}$Li system obtained from $^{11}$Li fragmentation. Comparison of\nthe model results to new data from the GSI laboratory suggests that the\nreaction mechanism is dominated by final state effects rather than by the\nsudden process, but for the population of the l=0 virtual state, in which case\nthe two mechanisms give almost identical results. There is also, for the first\ntime, a clear evidence for the population of a d$_{5/2}$ resonance in\n$^{10}$Li.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:31:32 GMT\"}]', '2008-11-26', '[[\"Blanchon\",\"G.\",\"\",\"INFN and Physics Department, Pisa\"],[\"Bonaccorso\",\"A.\",\"\",\"INFN\\n  and Physics Department, Pisa\"],[\"Brink\",\"D. M.\",\"\",\"Oxford University\"],[\"Mau\",\"N. Vinh\",\"\",\"IPN, Orsay\"]]'),
(704.1782, 'Yossi Farjoun', 'Richard Ehrenborg and Yossi Farjoun', 'Asymptotics of the Euler number of bipartite graphs', '13 pages, 6 figure, submitted to JCTB', 'Advances in Applied Mathematics 44 (2010) 155--167', '10.1016/j.aam.2009.05.002', '', 'math.CO math.NA', '', '  We define the Euler number of a bipartite graph on $n$ vertices to be the\nnumber of labelings of the vertices with $1,2,...,n$ such that the vertices\nalternate in being local maxima and local minima. We reformulate the problem of\ncomputing the Euler number of certain subgraphs of the Cartesian product of a\ngraph $G$ with the path $P_m$ in terms of self adjoint operators. The\nasymptotic expansion of the Euler number is given in terms of the eigenvalues\nof the associated operator. For two classes of graphs, the comb graphs and the\nCartesian product $P_2 \\Box P_m$, we numerically solve the eigenvalue problem.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:34:43 GMT\"}]', '2010-02-22', '[[\"Ehrenborg\",\"Richard\",\"\"],[\"Farjoun\",\"Yossi\",\"\"]]'),
(704.1783, 'Francesco Santini', 'Stefano Bistarelli, Ugo Montanari, Francesca Rossi, Francesco Santini', 'Unicast and Multicast Qos Routing with Soft Constraint Logic Programming', '45 pages', '', '', '', 'cs.LO cs.AI cs.NI', '', '  We present a formal model to represent and solve the unicast/multicast\nrouting problem in networks with Quality of Service (QoS) requirements. To\nattain this, first we translate the network adapting it to a weighted graph\n(unicast) or and-or graph (multicast), where the weight on a connector\ncorresponds to the multidimensional cost of sending a packet on the related\nnetwork link: each component of the weights vector represents a different QoS\nmetric value (e.g. bandwidth, cost, delay, packet loss). The second step\nconsists in writing this graph as a program in Soft Constraint Logic\nProgramming (SCLP): the engine of this framework is then able to find the best\npaths/trees by optimizing their costs and solving the constraints imposed on\nthem (e.g. delay < 40msec), thus finding a solution to QoS routing problems.\nMoreover, c-semiring structures are a convenient tool to model QoS metrics. At\nlast, we provide an implementation of the framework over scale-free networks\nand we suggest how the performance can be improved.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:53:44 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 29 Apr 2007 15:40:10 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 21 Apr 2008 17:25:06 GMT\"}]', '2009-09-29', '[[\"Bistarelli\",\"Stefano\",\"\"],[\"Montanari\",\"Ugo\",\"\"],[\"Rossi\",\"Francesca\",\"\"],[\"Santini\",\"Francesco\",\"\"]]'),
(704.1784, 'Sergio Fabi', 'S.Fabi, B.Harms, G.Karatheodoris', 'Zero point energy on extra dimension: Noncommutative Torus', 'RevTeX4', 'Phys.Rev.D76:065010,2007', '10.1103/PhysRevD.76.065010', '', 'hep-th', '', '  In this paper we calculate the zero point energy density experienced by\nobservers on M^4 due to a massless scalar field defined throughout M^4 x T^2_F,\nwhere T^2_F are fuzzy extra dimensions. Using the Green\'s function approach we\ncalculate the energy density for the commutative torus and the fuzzy torus. We\ncalculate then the energy density for the fuzzy torus using the Hamiltonian\napproach. Agreement is shown between Green\'s function and Hamiltonian\napproaches.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:45:03 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 16 Apr 2007 14:51:36 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 25 Apr 2007 16:40:47 GMT\"}]', '2008-11-26', '[[\"Fabi\",\"S.\",\"\"],[\"Harms\",\"B.\",\"\"],[\"Karatheodoris\",\"G.\",\"\"]]'),
(704.1785, 'Alexei Larionov', 'A.B. Larionov, O. Buss, K. Gallmeister and U. Mosel', 'Three-body collisions in Boltzmann-Uehling-Uhlenbeck theory', '26 pages, 9 figures, figures added, discussion extended, results not\n  changed, version accepted in Phys. Rev. C', 'Phys.Rev.C76:044909,2007', '10.1103/PhysRevC.76.044909', '', 'nucl-th', '', '  Aiming at a microscopic description of heavy ion collisions in the beam\nenergy region of about 10 A GeV, we extend the Giessen\nBoltzmann-Uehling-Uhlenbeck (GiBUU) transport model by including a relativistic\nmean field, in-medium baryon-baryon cross sections and three-body collisions.\nThe model is then compared with experimental data for central Au+Au collisions\nat 2-10 A GeV and central Pb+Pb collisions at 30 and 40 A GeV on the proton\nrapidity spectra, the midrapidity yields of $\\pi^+$, $K^\\pm$ and\n$(\\Lambda+\\Sigma^0)$, and the transverse mass spectra of $\\pi^\\pm$ and $K^\\pm$.\nThe three-body collisions increase the inverse slope parameters of the hadron\n$m_\\perp$-spectra to a good agreement with the data.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:51:33 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 24 Sep 2007 08:11:21 GMT\"}]', '2008-11-26', '[[\"Larionov\",\"A. B.\",\"\"],[\"Buss\",\"O.\",\"\"],[\"Gallmeister\",\"K.\",\"\"],[\"Mosel\",\"U.\",\"\"]]'),
(704.1786, 'Stefan Popescu', 'Stefan Popescu and Bernhard Rothenstein', 'Learning more from the Lorentz transformations', 'very interesting new approach to Lorenz transformations', '', '', '', 'physics.gen-ph', '', '  Admitting the validity of Lorentz transformations for the space as time\ncoordinates of the same event we derive their differential form in order to\nunderline the correct prerequisites for the application of time and length\ncontraction or dilation effects. Furthermore we quantify the simultaneity error\noccurring in the relativity theory. Having done this, we analyse the root cause\nof these effects and identify it with a finite phase velocity associated with\nthe moving frame. We define this phase velocity by analogy to the de Broglie\nwave associated with a moving particle. Based on this construct we demonstrate\nthat the phase of the de Broglie waves further extended for stationary\nparticles is a relativistic invariant being the same for all corresponding\nobservers. Also the phase of the electromagnetic waves transporting energy at\nlight speed is a relativistic invariant. Therefore the universe and its matter\n/ energy may be seen as a superposition of waves propagating such that their\nphase is the same for all corresponding observers. The wave phase may replace\nthe time as an invariant and universal reference.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 15:56:39 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 7 May 2007 15:20:29 GMT\"}]', '2008-12-02', '[[\"Popescu\",\"Stefan\",\"\"],[\"Rothenstein\",\"Bernhard\",\"\"]]'),
(704.1787, 'Roi Baer', 'Roi Baer', 'On the Mapping of Time-Dependent Densities onto Potentials in Quantum\n  Mechanics', '', '', '10.1063/1.2822124', '', 'cond-mat.other cond-mat.dis-nn', '', '  The mapping of time-dependent densities on potentials in quantum mechanics is\ncritically examined. The issue is of significance ever since Runge and Gross\n(Phys. Rev. Lett. 52, 997 (1984)) established the uniqueness of the mapping,\nforming a theoretical basis for time-dependent density functional theory. We\nargue that besides existence (so called v-representability) and uniqueness\nthere is an important question of stability and chaos. Studying a 2-level\nsystem we find innocent, almost constant densities that cannot be constructed\nfrom any potential (non-existence). We further show via a Lyapunov analysis\nthat the mapping of densities on potentials has chaotic regions in this case.\nIn real space the situation is more subtle. V-representability is formally\nassured but the mapping is often chaotic making the actual construction of the\npotential almost impossible. The chaotic nature of the mapping, studied for the\nfirst time here, has serious consequences regarding the possibility of using\nTDDFT in real-time settings.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:56:09 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 28 Apr 2007 08:01:22 GMT\"}]', '2009-11-13', '[[\"Baer\",\"Roi\",\"\"]]'),
(704.1788, 'Bipin singh Koranga', 'Bipin Singh Koranga and S. Uma Sankar (Indian Institute of Technology\n  Bombay)', 'New Jarlskog determinant from Physics above the GUT Scal', '11 pages and 2 figures', 'Electron.J.Theor.Phys.6:229,2009', '', '', 'hep-ph', '', '  We study the Planck scale effects on Jarlskog determinant. Quantum\ngravitational (Planck scale) effects lead to an effective SU(2)_{L}\\times U(1)\ninvariant dimension-5 Lagrangian involving neutrino and Higgs fields, which\ngives rise to additional terms in neutrino mass matrix on electroweak symmetry\nbreaking. We assume that gravitational interaction is flavor blind and compute\nthe Jarlskog determinant due to the Planck scale effects. In the case of\nneutrino sector, the strength of CP violation is measured by Jarlskog\ndeterminant. In this paper, we assume CP violation arise from Planck scale\neffects. We applied our approach to study Jarlskog determinant due to the\nPlanck scale effects.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:03:45 GMT\"}]', '2009-06-25', '[[\"Koranga\",\"Bipin Singh\",\"\",\"Indian Institute of Technology\\n  Bombay\"],[\"Sankar\",\"S. Uma\",\"\",\"Indian Institute of Technology\\n  Bombay\"]]'),
(704.1789, 'Kevin Ford', 'Kevin Ford', 'Generalized Smirnov statistics and the distribution of prime factors', '10 pages. Minor corrections; increase in the range of variables in\n  the theorems and corollary. To appear in Functiones et Approximatio\n  Commentarii Mathematici', 'Funct. Approx. Comm. Math. XXXVII.I (2007), 119-129.', '', '', 'math.NT math.PR', '', '  We apply recent bounds of the author (math.PR/0609224) for generalized\nSmirnov statistics to the distribution of integers whose prime factors satisfy\ncertain systems of inequalities.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:10:30 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 27 Jun 2007 07:16:12 GMT\"}]', '2008-01-09', '[[\"Ford\",\"Kevin\",\"\"]]'),
(704.1790, 'Nino Boccara', 'Nino Boccara', 'Models of Opinion Formation: Influence of Opinion Leaders', '20 pages, 9 figures', '', '10.1142/S0129183108011954', '', 'nlin.AO', '', '  This paper studies the evolution of the distribution of opinions in a\npopulation of individuals in which there exist two distinct subgroups of\nhighly-committed, well-connected opinion leaders endowed with a strong\nconvincing power. Each individual, located at a vertex of a directed graph, is\ncharacterized by her name, the list of people she is interacting with, her\nlevel of awareness, and her opinion. Various temporal evolutions according to\ndifferent local rules are compared in order to find under which conditions the\nformation of strongly polarized subgroups, each adopting the opinion of one of\nthe two groups of opinion leaders, is favored.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:06:03 GMT\"}]', '2009-11-13', '[[\"Boccara\",\"Nino\",\"\"]]'),
(704.1791, 'Dennis Sivers Dr.', 'Dennis Sivers', 'Chiral Mechanisms Leading to Orbital Quantum Structures in the Nucleon', '28 pages, no figures', '', '', '', 'hep-ph', '', '  Color confinement and chiral symmetry specify some important territory for\nthe study of hadronic physics. Any hadron can be defined as a color-singlet\ncomposite system of qurks and gluons, the fundamental fields of qcd, while the\nlandscape of the hadronic spectrum is dominated by the fact that two quark\nflavors, u and d, are characterized by masses small compared to the fundamental\nscale of this theory. Measurements sensitive to the orbital angular momenta of\nthe color constituents of the nucleon display the interplay of chiral dynamics\nand confinement in a unique manner. This pageant can be explored by an\nevaluation, within the context of the Georgi-Manohar chiral quark model, of the\nnormalization of the orbital structure functions and the normalization of the\nBoer-Mulders functions for different quark flavors. The resolution structures\nin the chiral quark model represent an evaluation of Collins functions for a\nconfined system defined by the quantum numbers of the nucleon in the\nconstituent quark model. The orbital structure functions for antiquarks can\nalso be specified within the basic framework of this approach while the\nnormalization of the gluon orbital structure function requires some additional\nassumptions.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:10:48 GMT\"}]', '2007-05-23', '[[\"Sivers\",\"Dennis\",\"\"]]'),
(704.1792, 'Charles Creffield', 'C.E. Creffield', 'Quantum control and entanglement using periodic driving fields', '4 pages, 4 eps figures. V2: minor changes, this version to be\n  published in PRL', 'Phys. Rev. Lett. 99, 110501 (2007).', '10.1103/PhysRevLett.99.110501', '', 'cond-mat.other', '', '  We propose a scheme for producing directed motion in a lattice system by\napplying a periodic driving potential. By controlling the dynamics by means of\nthe effect known as coherent destruction of tunneling, we demonstrate a novel\nratchet-like effect that enables particles to be coherently manipulated and\nsteered without requiring local control. Entanglement between particles can\nalso be controllably generated, which points to the attractive possibility of\nusing these technique for quantum information processing.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:33:50 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 29 Aug 2007 13:43:54 GMT\"}]', '2007-09-13', '[[\"Creffield\",\"C. E.\",\"\"]]'),
(704.1793, 'Misha Katsnelson', 'A. Fasolino, J. H. Los and M. I. Katsnelson', 'Intrinsic ripples in graphene', '14 pages, 6 figures', 'Nature Materials 6, 858-861 (2007)', '10.1038/nmat2011', '', 'cond-mat.mtrl-sci cond-mat.mes-hall', '', '  The stability of two-dimensional (2D) layers and membranes is subject of a\nlong standing theoretical debate. According to the so called Mermin-Wagner\ntheorem, long wavelength fluctuations destroy the long-range order for 2D\ncrystals. Similarly, 2D membranes embedded in a 3D space have a tendency to be\ncrumpled. These dangerous fluctuations can, however, be suppressed by\nanharmonic coupling between bending and stretching modes making that a\ntwo-dimensional membrane can exist but should present strong height\nfluctuations. The discovery of graphene, the first truly 2D crystal and the\nrecent experimental observation of ripples in freely hanging graphene makes\nthese issues especially important. Beside the academic interest, understanding\nthe mechanisms of stability of graphene is crucial for understanding electronic\ntransport in this material that is attracting so much interest for its unusual\nDirac spectrum and electronic properties. Here we address the nature of these\nheight fluctuations by means of straightforward atomistic Monte Carlo\nsimulations based on a very accurate many-body interatomic potential for\ncarbon. We find that ripples spontaneously appear due to thermal fluctuations\nwith a size distribution peaked around 70 \\AA which is compatible with\nexperimental findings (50-100 \\AA) but not with the current understanding of\nstability of flexible membranes. This unexpected result seems to be due to the\nmultiplicity of chemical bonding in carbon.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:38:30 GMT\"}]', '2011-01-14', '[[\"Fasolino\",\"A.\",\"\"],[\"Los\",\"J. H.\",\"\"],[\"Katsnelson\",\"M. I.\",\"\"]]'),
(704.1794, 'Bachtold', 'An. Gruneis, M.J. Esplandiu, D. Garcia-Sanchez, and A. Bachtold', 'Counting and manipulating single electrons using a carbon nanotube\n  transistor', '4 figures', 'Nano Lett. 7, 3766 (2007)', '', '', 'cond-mat.mes-hall cond-mat.mtrl-sci', '', '  We report on the electric measurements of an individual Au nanoparticle with\nan ultra-high contact resistance of about $10^{19} \\Omega$. The high-impedance\nmeasurements have been carried out by counting the electrons that are\ntransferred onto the particle. In order to do this, a carbon nanotube is used\nas the electrode for the supply of electrons but also as the detector of the\ncharge transfer. Measurements using single-electron detection allow us to\ndetermine the separation between the electron states in the Au nanoparticle,\nwhich is about 4 meV, consistent with the charging energy of the particle.\nSingle-electron detection with nanotubes offers great promise for the study of\nelectron transfer in highly resistive molecular systems.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:40:25 GMT\"}]', '2008-03-12', '[[\"Gruneis\",\"An.\",\"\"],[\"Esplandiu\",\"M. J.\",\"\"],[\"Garcia-Sanchez\",\"D.\",\"\"],[\"Bachtold\",\"A.\",\"\"]]'),
(704.1795, 'Frederic Chapoton', 'Fr\\\'ed\\\'eric Chapoton (ICJ)', 'Le module dendriforme sur le groupe cyclique', '12 pages', '', '', '', 'math.QA', '', '  The structure of anticyclic operad on the Dendriform operad defines in\nparticular a matrix of finite order acting on the vector space spanned by\nplanar binary trees. We compute its characteristic polynomial and propose a\n(compatible) conjecture for the characteristic polynomial of the Coxeter\ntransformation for the Tamari lattice, which is mostly a square root of this\nmatrix.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 16:58:28 GMT\"}]', '2007-05-23', '[[\"Chapoton\",\"Frédéric\",\"\",\"ICJ\"]]'),
(704.1796, 'Ying Hu', 'Ying Hu (IRMAR), Jin Ma (Department of Mathematics), Shige Peng\n  (Institute of Mathematics), Song Yao (Department of Mathematics)', 'Representation Theorems for Quadratic ${\\cal F}$-Consistent Nonlinear\n  Expectations', '', '', '', '', 'math.PR', '', '  In this paper we extend the notion of ``filtration-consistent nonlinear\nexpectation\" (or \"${\\cal F}$-consistent nonlinear expectation\") to the case\nwhen it is allowed to be dominated by a $g$-expectation that may have a\nquadratic growth. We show that for such a nonlinear expectation many\nfundamental properties of a martingale can still make sense, including the\nDoob-Meyer type decomposition theorem and the optional sampling theorem. More\nimportantly, we show that any quadratic ${\\cal F}$-consistent nonlinear\nexpectation with a certain domination property must be a quadratic\n$g$-expectation. The main contribution of this paper is the finding of the\ndomination condition to replace the one used in all the previous works, which\nis no longer valid in the quadratic case. We also show that the representation\ngenerator must be deterministic, continuous, and actually must be of the simple\nform.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:03:19 GMT\"}]', '2007-05-23', '[[\"Hu\",\"Ying\",\"\",\"IRMAR\"],[\"Ma\",\"Jin\",\"\",\"Department of Mathematics\"],[\"Peng\",\"Shige\",\"\",\"Institute of Mathematics\"],[\"Yao\",\"Song\",\"\",\"Department of Mathematics\"]]'),
(704.1797, 'Philippe Vergne', 'Kazuyuki Yagi (LaMCoS), Philippe Vergne (LaMCoS)', 'Film Thickness Changes in EHD Sliding Contacts Lubricated by a Fatty\n  Alcohol', '', 'Tribology Online 1, 1 (31/08/2006) 5-8', '', '', 'physics.class-ph', '', '  This paper describes the appearance of abnormal film thickness features\nformed in elastohydrodynamic contacts lubricated by a fatty alcohol.\nExperiments were conducted by varying the slide to roll ratio between a steel\nball and a glass disk in a ball-on-disk type device. Lauric alcohol was used as\nlubricant and film thickness was measured in the contact area by optical\ninterferometry. Experimental results showed that the film thickness\ndistributions under pure rolling conditions remained classical whereas the film\nshape changed when the slide to roll ratio was increased. The thickness in the\ncentral contact area increased and in the same time inlet and exit film\nthicknesses were modified. In addition, the film shapes observed when the ball\nsurface was moving faster than the disk one and those obtained in the opposite\ncase were different, i.e. when opposite signs but equal absolute values of the\nslide to roll ratio were applied.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:04:33 GMT\"}]', '2007-05-23', '[[\"Yagi\",\"Kazuyuki\",\"\",\"LaMCoS\"],[\"Vergne\",\"Philippe\",\"\",\"LaMCoS\"]]'),
(704.1798, 'Philippe Vergne', 'Scott Bair, Philippe Vergne (LaMCoS), Michel Querry (LaMCoS)', 'A unified shear-thinning treatment of both film thickness and traction\n  in EHD', '', 'Tribology Letters 18, 2 (01/02/2005) 145-152', '', '', 'physics.class-ph', '', '  A conclusive demonstration has been provided that the nature of the\nshear-thinning, that affects both film thickness and traction in EHL contacts,\nfollows the ordinary power-law rule that has been described by many empirical\nmodels of which Carreau is but one example. This was accomplished by accurate\nmeasurements in viscometers of the shear response of a PAO that possesses a\nvery low critical stress for shear-thinning and accurate measurements\nin-contact of film thickness and traction under conditions which accentuate the\nshear-thinning effect. The in-contact central film thickness and traction were\nentirely predictable from the rheological properties obtained from viscometers\nusing simple calculations. These data should be invaluable to researchers\nendeavoring to accurately simulate Hertz zone behavior since the shear-thinning\nrheology is extensively characterized and accurate in-contact data are\navailable to test. In addition, a new model has been introduced that may be\nuseful for the rheological characterization of mixtures.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:04:56 GMT\"}]', '2007-05-23', '[[\"Bair\",\"Scott\",\"\",\"LaMCoS\"],[\"Vergne\",\"Philippe\",\"\",\"LaMCoS\"],[\"Querry\",\"Michel\",\"\",\"LaMCoS\"]]'),
(704.1799, 'Philippe Vergne', 'Philippe Vergne (LaMCoS)', 'Super Low Traction under EHD and Mixed Lubrication Regimes', '', 'Superlubricity, Elsevier BV (Ed.) (31/03/2007) 429-445', '', '', 'physics.class-ph', '', '  After the pioneered experimental works on superlubricity by Martin et al. on\nMoS2 [1], Hirano et al. on tungsten and silicon [2] and the further\nconfirmation by Dienwiebel et al. on graphite [3], many groups around the word\ninvestigated the occurrence of near frictionless sliding contacts. This large\nmobilization of tribologists, material sciences specialists and physicists has\nlead to emerging solutions involving new materials and coatings, the most\npromising being carbon based like graphite, diamond, carbon composites or\ndiamond-like-carbons. Some of them are currently used in practical\napplications. The situation is different especially in EHL: the highest\nfriction coefficients are close to 10% when traction fluids are involved, i.e.\nfluids that have especially designed to transmit the highest friction, and they\nvary within 3-6% for the rest of lubricants. The range of variation is\nconsequently very narrow and these typical values are really low compared to\nthose obtained in dry contacts: as a consequence the gain expected from a super\nlow traction regime in lubrication will be probably more limited, especially in\nthe case of experiments conducted at the meso or macro scales. This weak\nperspective could be one explanation on the relatively low number of articles\nin recent literature dealing with lubricated superlubricity in the above\nconditions.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:05:21 GMT\"}]', '2007-05-23', '[[\"Vergne\",\"Philippe\",\"\",\"LaMCoS\"]]'),
(704.1800, 'MariaConcepcion Gonzalez-Garcia', 'M.C. Gonzalez-Garcia and Michele Maltoni', 'Phenomenology with Massive Neutrinos', '204 pages, 57 figures. All results updated with the new MINOS,\n  KamLAND and Borexino data. Three new sections added: nu magnetic moment, nu\n  decay, two sterile nu\'s. Many sections and bibliography expanded. Analysis\n  fully updated as of Fall 2007; for more recent results check\n  http://dark.ft.uam.es/~maltoni/neutrino/', 'Phys.Rept.460:1-129,2008', '10.1016/j.physrep.2007.12.004', 'YITP-SB-07-14, UB-ECM-PF 07/08, IFT-UAM/CSIC-07-51', 'hep-ph astro-ph hep-ex', '', '  The current status and some perspectives of the phenomenology of massive\nneutrinos is reviewed. We start with the phenomenology of neutrino oscillations\nin vacuum and in matter. We summarize the results of neutrino experiments using\nsolar, atmospheric, reactor and accelerator neutrino beams. We update the\nleptonic parameters derived from the three-neutrino oscillation interpretation\nof this data. We describe the method and present results on our understanding\nof the solar and atmospheric neutrino fluxes by direct extraction from the\ncorresponding neutrino event rates. We present some tests of different forms of\nnew physics which induce new sources of leptonic flavor transitions in vacuum\nand in matter which can be performed with the present neutrino data. The aim\nand potential of future neutrino experiments and facilities to further advance\nin these fronts is also briefly summarized. Last, the implications of the LSND\nobservations are discussed, and the status of extended models which could\naccommodate all flavor-mixing signals is presented in the light of the recent\nresults from MiniBooNE.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:09:13 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 16 Oct 2007 13:11:59 GMT\"}]', '2008-11-26', '[[\"Gonzalez-Garcia\",\"M. C.\",\"\"],[\"Maltoni\",\"Michele\",\"\"]]'),
(704.1801, 'Harvey B. Meyer', 'Harvey B. Meyer', 'A calculation of the shear viscosity in SU(3) gluodynamics', '4 pages, 3 figures', 'Phys.Rev.D76:101701,2007', '10.1103/PhysRevD.76.101701', 'MIT-CTP 3830', 'hep-lat hep-ph', '', '  We perform a lattice Monte-Carlo calculation of the two-point functions of\nthe energy-momentum tensor at finite temperature in the SU(3) gauge theory.\nUnprecedented precision is obtained thanks to a multi-level algorithm. The\nlattice operators are renormalized non-perturbatively and the classical\ndiscretization errors affecting the correlators are corrected for. A robust\nupper bound for the shear viscosity to entropy density ratio is derived, eta/s\n< 1.0, and our best estimate is eta/s = 0.134(33) at T=1.65Tc under the\nassumption of smoothness of the spectral function in the low-frequency region.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:17:51 GMT\"}]', '2010-04-06', '[[\"Meyer\",\"Harvey B.\",\"\"]]'),
(704.1802, 'Comelli Denis', 'Denis Comelli', 'A Way to Dynamically Overcome the Cosmological Constant Problem', '5 pages', 'Int.J.Mod.Phys.A23:4133-4143,2008', '10.1142/S0217751X08041359', '', 'gr-qc astro-ph', '', '  The Cosmological Constant problem can be solved once we require that the full\nstandard Einstein Hilbert lagrangian, gravity plus matter, is multiplied by a\ntotal derivative. We analyze such a picture writing the total derivative as the\ncovariant gradient of a new vector field (b_mu). The dynamics of this b_mu\nfield can play a key role in the explanation of the present cosmological\nacceleration of the Universe.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:29:06 GMT\"}]', '2009-01-06', '[[\"Comelli\",\"Denis\",\"\"]]'),
(704.1803, 'Andrew Toms', 'George A. Elliott, Andrew S. Toms', 'Regularity properties in the classification program for separable\n  amenable C*-algebras', '19 pages, to appear in Bull. AMS, April 2008', '', '', '', 'math.OA math.FA', '', '  We report on recent progress in the program to classify separable amenable\nC*-algebras. Our emphasis is on the newly apparent role of regularity\nproperties such as finite decomposition rank, strict comparison of positive\nelements, and Z-stability, and on the importance of the Cuntz semigroup. We\ninclude a brief history of the program\'s successes since 1989, a more detailed\nlook at the Villadsen-type algebras which have so dramatically changed the\nlandscape, and a collection of announcements on the structure and properties of\nthe Cuntz semigroup.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 17:45:01 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 15 Apr 2007 14:56:01 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 22 Aug 2007 20:32:23 GMT\"}]', '2007-08-22', '[[\"Elliott\",\"George A.\",\"\"],[\"Toms\",\"Andrew S.\",\"\"]]'),
(704.1804, 'Ryan Kalas', 'Ryan M. Kalas, D. Blume', 'Equation of state of atomic systems beyond s-wave determined by the\n  lowest order constrained variational method: Large scattering length limit', '10 pages, 7 figures', '', '', '', 'cond-mat.other', '', '  Dilute Fermi systems with large s-wave scattering length a_s exhibit\nuniversal properties if the interparticle spacing r_o greatly exceeds the range\nof the underlying two-body interaction potential. In this regime, r_o is the\nonly relevant length scale and observables such as the energy per particle\ndepend only on r_o (or, equivalently, the energy E_{FG} of the free Fermi gas).\nThis paper investigates Bose and Fermi systems with non-vanishing angular\nmomentum l using the lowest order constrained variational method. We focus on\nthe regime where the generalized scattering length becomes large and determine\nthe relevant length scales. For Bose gases with large generalized scattering\nlengths, we obtain simple expressions for the energy per particle in terms of a\nl-dependent length scale \\xi_l, which depends on the range of the underlying\ntwo-body potential and the average interparticle spacing. We discuss possible\nimplications for dilute two-component Fermi systems with finite l. Furthermore,\nwe determine the equation of state of liquid and gaseous bosonic helium.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 18:09:58 GMT\"}]', '2007-05-23', '[[\"Kalas\",\"Ryan M.\",\"\"],[\"Blume\",\"D.\",\"\"]]'),
(704.1805, 'Youngone Lee', 'Youngone Lee', 'On Charge Conservation and The Equivalence Principle in the\n  Noncommutative Spacetime', 'typos corrected, references added, accepted for publication in Phys.\n  Rev. D', 'Phys.Rev.D76:025022,2007', '10.1103/PhysRevD.76.025022', '', 'hep-th', '', '  We investigate one of the consequences of the twisted Poincare symmetry. We\nderive the charge conservation law and show that the equivalence principle is\nsatisfied in the canonical noncommutative spacetime. We applied the twisted\nPoincare symmetry to the Weinberg\'s analysis. To this end, we generalize our\nearlier construction of the twisted S matrix \\cite{Bu}, which apply the\nnoncommutativity to the fourier modes, to the massless fields of integer spins.\nThe transformation formula for the twisted S matrix for the massless fields of\ninteger spin has been obtained. For massless fields of spin 1, we obtain the\nconservation of charge, and the universality of coupling constant for massless\nfields of spin 2, which can be interpreted as the equality of gravitational\nmass and inertial mass, i.e., the equivalence principle.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 18:19:07 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 22 Apr 2007 09:00:23 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 20 Jun 2007 01:07:56 GMT\"}]', '2008-11-26', '[[\"Lee\",\"Youngone\",\"\"]]'),
(704.1806, 'Stephen Teitel', 'Peter Olsson and S. Teitel', 'Critical Scaling of Shear Viscosity at the Jamming Transition', 'replaced with published version; new references added', 'Phys. Rev. Lett. 99, 178001 (2007)', '10.1103/PhysRevLett.99.178001', '', 'cond-mat.soft cond-mat.stat-mech', '', '  We carry out numerical simulations to study transport behavior about the\njamming transition of a model granular material in two dimensions at zero\ntemperature. Shear viscosity \\eta is computed as a function of particle volume\ndensity \\rho and applied shear stress \\sigma, for diffusively moving particles\nwith a soft core interaction. We find an excellent scaling collapse of our data\nas a function of the scaling variable \\sigma/|\\rho_c-\\rho|^\\Delta, where \\rho_c\nis the critical density at \\sigma=0 (\"point J\"), and \\Delta is the crossover\nscaling critical exponent. Our results show that jamming is a true critical\nphenomenon, extending to driven steady states along the non-equilibrium \\sigma\naxis of the \\rho-\\sigma phase diagram.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:10:26 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 26 Oct 2007 20:04:40 GMT\"}]', '2011-11-09', '[[\"Olsson\",\"Peter\",\"\"],[\"Teitel\",\"S.\",\"\"]]'),
(704.1807, 'Ruy Tojeiro', 'Ion Moutinho and Ruy Tojeiro', 'Polar actions on compact Euclidean hypersurfaces', '17 pages', '', '', '', 'math.DG', '', '  Given an isometric immersion $f\\colon M^n\\to \\R^{n+1}$ of a compact\nRiemannian manifold of dimension $n\\geq 3$ into Euclidean space of dimension\n$n+1$, we prove that the identity component $Iso^0(M^n)$ of the isometry group\n$Iso(M^n)$ of $M^n$ admits an orthogonal representation $\\Phi\\colon\nIso^0(M^n)\\to SO(n+1)$ such that $f\\circ g=\\Phi(g)\\circ f$ for every $g\\in\nIso^0(M^n)$. If $G$ is a closed connected subgroup of $Iso(M^n)$ acting locally\npolarly on $M^n$, we prove that $\\Phi(G)$ acts polarly on $\\R^{n+1}$, and we\nobtain that $f(M^n)$ is given as $\\Phi(G)(L)$, where $L$ is a hypersurface of a\nsection which is invariant under the Weyl group of the $\\Phi(G)$-action. We\nalso find several sufficient conditions for such an $f$ to be a rotation\nhypersurface. Finally, we show that compact Euclidean rotation hypersurfaces of\ndimension $n\\geq 3$ are characterized by their underlying warped product\nstructure.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:45:57 GMT\"}]', '2007-05-23', '[[\"Moutinho\",\"Ion\",\"\"],[\"Tojeiro\",\"Ruy\",\"\"]]'),
(704.1808, 'Neil J. Cornish', 'Neil J. Cornish and Tyson B. Littenberg', 'Tests of Bayesian Model Selection Techniques for Gravitational Wave\n  Astronomy', '11 pages, 6 figures', 'Phys.Rev.D76:083006,2007', '10.1103/PhysRevD.76.083006', '', 'gr-qc', '', '  The analysis of gravitational wave data involves many model selection\nproblems. The most important example is the detection problem of selecting\nbetween the data being consistent with instrument noise alone, or instrument\nnoise and a gravitational wave signal. The analysis of data from ground based\ngravitational wave detectors is mostly conducted using classical statistics,\nand methods such as the Neyman-Pearson criteria are used for model selection.\nFuture space based detectors, such as the \\emph{Laser Interferometer Space\nAntenna} (LISA), are expected to produced rich data streams containing the\nsignals from many millions of sources. Determining the number of sources that\nare resolvable, and the most appropriate description of each source poses a\nchallenging model selection problem that may best be addressed in a Bayesian\nframework. An important class of LISA sources are the millions of low-mass\nbinary systems within our own galaxy, tens of thousands of which will be\ndetectable. Not only are the number of sources unknown, but so are the number\nof parameters required to model the waveforms. For example, a significant\nsubset of the resolvable galactic binaries will exhibit orbital frequency\nevolution, while a smaller number will have measurable eccentricity. In the\nBayesian approach to model selection one needs to compute the Bayes factor\nbetween competing models. Here we explore various methods for computing Bayes\nfactors in the context of determining which galactic binaries have measurable\nfrequency evolution. The methods explored include a Reverse Jump Markov Chain\nMonte Carlo (RJMCMC) algorithm, Savage-Dickie density ratios, the Schwarz-Bayes\nInformation Criterion (BIC), and the Laplace approximation to the model\nevidence. We find good agreement between all of the approaches.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:47:48 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 15 Apr 2007 05:54:09 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 8 Nov 2007 18:41:40 GMT\"}]', '2008-11-26', '[[\"Cornish\",\"Neil J.\",\"\"],[\"Littenberg\",\"Tyson B.\",\"\"]]'),
(704.1809, 'Marek Zukowski', 'Piotr Badziag and Marek Zukowski', 'All tight multipartite Bell correlation inequalities for an arbitrary\n  number of dichotomic observables per observer', 'there is a mistake in the proof, and even worse... one can find a\n  counterexample', '', '', '', 'quant-ph', '', '  Derivation of the full set of Bell inequalities involving correlation\nfunctions, for two parties, with binary observables, and N possible local\nsettings is not as easy as it seemed. The proof of v1 is wrong. Additionaly one\ncan find a counterexample, which will be presented soon. Thus our thesis is\ndead. Still the series of Bell inequalities discussed in the manuscript (v1)\nform a necessary condition for local realism, and are tight. They are tight and\ncomplete (sufficient) only for N=3 settings per observer (as shown in\nquant-ph/0611086, fortunately using an entirely different approach).\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:49:17 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 26 May 2007 17:04:32 GMT\"}]', '2007-06-13', '[[\"Badziag\",\"Piotr\",\"\"],[\"Zukowski\",\"Marek\",\"\"]]'),
(704.1810, 'Jeffrey N. Cuzzi', 'Robert C. Hogan and Jeffrey N. Cuzzi', 'A Cascade Model for Particle Concentration and Enstrophy in Fully\n  Developed Turbulence with Mass Loading Feedback', 'Accepted by Phys. Rev. E; in press; 9 pages, 8 figures; the research\n  is relevant to turbulent concentration of chondrules and other small\n  particles in protoplanetary nebulae. Solid/gas mass ratios as large as 100\n  are possible before turbulence is damped, for particles in this size range', 'Phys.Rev.E75:056305,2007', '10.1103/PhysRevE.75.056305', '', 'astro-ph', '', '  A cascade model is described based on multiplier distributions determined\nfrom 3D direct numerical simulations (DNS) of turbulent particle laden flows,\nwhich include two-way coupling between the phases at global mass loadings equal\nto unity. The governing Eulerian equations are solved using pseudo-spectral\nmethods on up to 512**3 computional grid points. DNS results for particle\nconcentration and enstrophy at Taylor microscale Reynolds numbers in the range\n34 - 170 were used to directly determine multiplier distributions (PDFs) on\nspatial scales 3 times the Kolmogorov length scale. The width of the PDFs,\nwhich is a measure of intermittency, decreases with increasing mass loading\nwithin the local region where the multipliers are measured. The functional form\nof this dependence is not sensitive to Reynolds numbers in the range\nconsidered. A partition correlation probability is included in the cascade\nmodel to account for the observed spatial anticorrelation between particle\nconcentration and enstrophy. Joint probability distribution functions of\nconcentration and enstrophy generated using the cascade model are shown to be\nin excellent agreement with those derived directly from our 3D simulations.\nProbabilities predicted by the cascade model are presented at Reynolds numbers\nwell beyond what is achievable by direct simulation. These results clearly\nindicate that particle mass loading significantly reduces the probabilities of\nhigh particle concentration and enstrophy relative to those resulting from\nunloaded runs. Particle mass density appears to reach a limit at around 100\ntimes the gas density. This approach has promise for significant computational\nsavings in certain applications.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:51:16 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 13 Apr 2007 20:02:05 GMT\"}]', '2015-06-30', '[[\"Hogan\",\"Robert C.\",\"\"],[\"Cuzzi\",\"Jeffrey N.\",\"\"]]'),
(704.1811, 'Samarth Swarup', 'Samarth Swarup and Les Gasser', 'Unifying Evolutionary and Network Dynamics', '11 pages, 12 figures, Accepted for publication in Physical Review E', '', '10.1103/PhysRevE.75.066114', '', 'q-bio.QM q-bio.PE', '', '  Many important real-world networks manifest \"small-world\" properties such as\nscale-free degree distributions, small diameters, and clustering. The most\ncommon model of growth for these networks is \"preferential attachment\", where\nnodes acquire new links with probability proportional to the number of links\nthey already have. We show that preferential attachment is a special case of\nthe process of molecular evolution. We present a new single-parameter model of\nnetwork growth that unifies varieties of preferential attachment with the\nquasispecies equation (which models molecular evolution), and also with the\nErdos-Renyi random graph model. We suggest some properties of evolutionary\nmodels that might be applied to the study of networks. We also derive the form\nof the degree distribution resulting from our algorithm, and we show through\nsimulations that the process also models aspects of network growth. The\nunification allows mathematical machinery developed for evolutionary dynamics\nto be applied in the study of network dynamics, and vice versa.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 19:56:37 GMT\"}]', '2009-11-13', '[[\"Swarup\",\"Samarth\",\"\"],[\"Gasser\",\"Les\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1812, 'Nicholas Law', 'N.M. Law (1 and 2), S.T. Hodgkin (2), C.D. Mackay (2) ((1) Caltech,\n  (2) IOA, Cambridge)', 'The LuckyCam Survey for Very Low Mass Binaries II: 13 new M4.5-M6.0\n  Binaries', '11 pages, 8 figures. Submitted to MNRAS', '', '10.1111/j.1365-2966.2007.12675.x', '', 'astro-ph', '', '  We present results from a high-angular-resolution survey of 78 very low mass\n(VLM) binary systems with 6.0 <= V-K colour <= 7.5 and proper motion >= 0.15\narcsec/yr. 21 VLM binaries were detected, 13 of them new discoveries. The new\nbinary systems range in separation between 0.18 arcsec and 1.3 arcsec. The\ndistance-corrected binary fraction is 13.5% (+6.5%/-4%), in agreement with\nprevious results. 9 of the new binary systems have orbital radii > 10 AU,\nincluding a new wide VLM binary with 27 AU projected orbital separation. One of\nthe new systems forms two components of a 2300 AU separation triple system. We\nfind that the orbital radius distribution of the binaries with V-K < 6.5 in\nthis survey appears to be different from that of redder (lower-mass) objects,\nsuggesting a possible rapid change in the orbital radius distribution at around\nthe M5 spectral type. The target sample was also selected to investigate X-ray\nactivity among VLM binaries. There is no detectable correlation between excess\nX-Ray emission and the frequency and binary properties of the VLM systems.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 05:09:45 GMT\"}]', '2009-11-13', '[[\"Law\",\"N. M.\",\"\",\"1 and 2\"],[\"Hodgkin\",\"S. T.\",\"\"],[\"Mackay\",\"C. D.\",\"\"]]'),
(704.1813, 'Mukremin Kilic', 'Mukremin Kilic, Warren R. Brown, Carlos Allende Prieto, M. H.\n  Pinsonneault, and S. J. Kenyon', 'The Discovery of a Companion to the Lowest Mass White Dwarf', 'ApJ, in press. See the Press Release at\n  http://www.cfa.harvard.edu/press/2007/pr200708.html', 'Astrophys.J.664:1088-1092,2007', '10.1086/518735', '', 'astro-ph', '', '  We report the detection of a radial velocity companion to SDSS\nJ091709.55+463821.8, the lowest mass white dwarf currently known with\nM~0.17Msun. The radial velocity of the white dwarf shows variations with a\nsemi-amplitude of 148.8 km/s and a period of 7.5936 hours, which implies a\ncompanion mass of M > 0.28Msun. The lack of evidence of a companion in the\noptical photometry forces any main-sequence companion to be smaller than\n0.1Msun, hence a low mass main sequence star companion is ruled out for this\nsystem. The companion is most likely another white dwarf, and we present\ntentative evidence for an evolutionary scenario which could have produced it.\nHowever, a neutron star companion cannot be ruled out and follow-up radio\nobservations are required to search for a pulsar companion.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:06:53 GMT\"}]', '2009-06-23', '[[\"Kilic\",\"Mukremin\",\"\"],[\"Brown\",\"Warren R.\",\"\"],[\"Prieto\",\"Carlos Allende\",\"\"],[\"Pinsonneault\",\"M. H.\",\"\"],[\"Kenyon\",\"S. J.\",\"\"]]'),
(704.1814, 'Giovanni Villadoro', 'Nima Arkani-Hamed, Sergei Dubovsky, Alberto Nicolis, Enrico\n  Trincherini, Giovanni Villadoro', 'A Measure of de Sitter Entropy and Eternal Inflation', '33 pages, 8 figures', 'JHEP 0705:055,2007', '10.1088/1126-6708/2007/05/055', '', 'hep-th', '', '  We show that in any model of non-eternal inflation satisfying the null energy\ncondition, the area of the de Sitter horizon increases by at least one Planck\nunit in each inflationary e-folding. This observation gives an operational\nmeaning to the finiteness of the entropy S_dS of an inflationary de Sitter\nspace eventually exiting into an asymptotically flat region: the asymptotic\nobserver is never able to measure more than e^(S_dS) independent inflationary\nmodes. This suggests a limitation on the amount of de Sitter space outside the\nhorizon that can be consistently described at the semiclassical level, fitting\nwell with other examples of the breakdown of locality in quantum gravity, such\nas in black hole evaporation. The bound does not hold in models of inflation\nthat violate the null energy condition, such as ghost inflation. This\nstrengthens the case for the thermodynamical interpretation of the bound as\nconventional black hole thermodynamics also fails in these models, strongly\nsuggesting that these theories are incompatible with basic gravitational\nprinciples.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:08:20 GMT\"}]', '2009-11-13', '[[\"Arkani-Hamed\",\"Nima\",\"\"],[\"Dubovsky\",\"Sergei\",\"\"],[\"Nicolis\",\"Alberto\",\"\"],[\"Trincherini\",\"Enrico\",\"\"],[\"Villadoro\",\"Giovanni\",\"\"]]'),
(704.1815, 'Daniel E. Sheehy', 'Daniel E. Sheehy (Louisiana State University) and Joerg Schmalian\n  (Iowa State University)', 'Kondo-lattice screening in a d-wave superconductor', '11 pages, 6 figures, revised version to appear in Physical Review B', 'Phys. Rev. B 77, 125129 (2008).', '10.1103/PhysRevB.77.125129', '', 'cond-mat.str-el', '', '  We show that local moment screening in a Kondo lattice with d-wave\nsuperconducting conduction electrons is qualitatively different from the\ncorresponding single Kondo impurity case. Despite the conduction-electron\npseudogap, Kondo-lattice screening is stable if the gap amplitude obeys $\\Delta\n<\\sqrt{\\tk D}$, in contrast to the single impurity condition $\\Delta <\\tk$\n(where $\\tk$ is the Kondo temperature for $\\Delta = 0$ and D is the bandwidth).\nOur theory explains the heavy electron behavior in the d-wave superconductor\nNd_{2-x}Ce_{x}CuO_{4}.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:54:39 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 27 Jul 2007 17:21:19 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 31 Jan 2008 23:18:57 GMT\"}]', '2009-11-13', '[[\"Sheehy\",\"Daniel E.\",\"\",\"Louisiana State University\"],[\"Schmalian\",\"Joerg\",\"\",\"Iowa State University\"]]'),
(704.1816, 'Sara L. Ellison', 'Sara L. Ellison, Joseph F. Hennawi, Crystal L. Martin, Jesper\n  Sommer-Larsen', 'Coincident, 100 kpc-scale damped Lyman alpha absorption towards a binary\n  QSO: how large are galaxies at z ~ 3?', 'Accepted for publication in MNRAS. Full resolution simulation images\n  available in pdf copy of the manuscript at\n  http://www.astro.uvic.ca/~sara/1116.pdf', 'Mon.Not.Roy.Astron.Soc.378:801-818,2007', '10.1111/j.1365-2966.2007.11847.x', '', 'astro-ph', '', '  We report coincident damped Lyman alpha (DLA) and sub-DLA absorption at z =\n2.66 and z = 2.94 towards the z ~ 3 13.8 arcsecond separation binary quasar\nSDSS 1116+4118 AB. At the redshifts of the absorbers, this angular separation\ncorresponds to a proper transverse separation of ~ 110 kpc. A third absorber, a\nsub-DLA at z = 2.47, is detected towards SDSS 1116+4118 B, but no corresponding\nhigh column density absorber is present towards SDSS 1116+4118 A. We use high\nresolution galaxy simulations and a clustering analysis to interpret the\ncoincident absorption and its implications for galaxy structure at z ~ 3. We\nconclude that the common absorption in the two lines of sight is unlikely to\narise from a single galaxy, or a galaxy plus satellite system, and is more\nfeasibly explained by a group of two or more galaxies with separations ~ 100\nkpc. The impact of these findings on single line of sight observations is also\ndiscussed; we show that abundances of DLAs may be affected by up to a few\ntenths of a dex by line of sight DLA blending. From a Keck ESI spectrum of the\ntwo quasars, we measure metal column densities for all five absorbers and\ndetermine abundances for the three absorbers with log N(HI) > 20. For the two\nhighest N(HI) absorbers, we determine high levels of metal enrichment,\ncorresponding to 1/3 and 1/5 solar. These metallicities are amongst the highest\nmeasured for DLAs at any redshift and are consistent with values measured in\nLyman break galaxies at 2 < z < 3. For the DLA at z = 2.94 we also infer an\napproximately solar ratio of alpha-to-Fe peak elements from [S/Zn] = +0.05, and\nmeasure an upper limit for the molecular fraction in this particular line of\nsight of log f(H_2)< -5.5.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:15:36 GMT\"}]', '2009-06-23', '[[\"Ellison\",\"Sara L.\",\"\"],[\"Hennawi\",\"Joseph F.\",\"\"],[\"Martin\",\"Crystal L.\",\"\"],[\"Sommer-Larsen\",\"Jesper\",\"\"]]'),
(704.1817, 'Louis Strigari', 'Louis E. Strigari, James S. Bullock, Manoj Kaplinghat, Juerg Diemand,\n  Michael Kuhlen, Piero Madau', 'Redefining the Missing Satellites Problem', '8 pages, 6 figures', 'Astrophys.J.669:676-683,2007', '10.1086/521914', '', 'astro-ph', '', '  Numerical simulations of Milky-Way size Cold Dark Matter (CDM) halos predict\na steeply rising mass function of small dark matter subhalos and a substructure\ncount that greatly outnumbers the observed satellites of the Milky Way. Several\nproposed explanations exist, but detailed comparison between theory and\nobservation in terms of the maximum circular velocity (Vmax) of the subhalos is\nhampered by the fact that Vmax for satellite halos is poorly constrained. We\npresent comprehensive mass models for the well-known Milky Way dwarf\nsatellites, and derive likelihood functions to show that their masses within\n0.6 kpc (M_0.6) are strongly constrained by the present data. We show that the\nM_0.6 mass function of luminous satellite halos is flat between ~ 10^7 and 10^8\nM_\\odot. We use the ``Via Lactea\'\' N-body simulation to show that the M_0.6\nmass function of CDM subhalos is steeply rising over this range. We rule out\nthe hypothesis that the 11 well-known satellites of the Milky Way are hosted by\nthe 11 most massive subhalos. We show that models where the brightest\nsatellites correspond to the earliest forming subhalos or the most massive\naccreted objects both reproduce the observed mass function. A similar analysis\nwith the newly-discovered dwarf satellites will further test these scenarios\nand provide powerful constraints on the CDM small-scale power spectrum and warm\ndark matter models.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:24:31 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 24 Oct 2007 18:46:30 GMT\"}]', '2010-11-11', '[[\"Strigari\",\"Louis E.\",\"\"],[\"Bullock\",\"James S.\",\"\"],[\"Kaplinghat\",\"Manoj\",\"\"],[\"Diemand\",\"Juerg\",\"\"],[\"Kuhlen\",\"Michael\",\"\"],[\"Madau\",\"Piero\",\"\"]]'),
(704.1818, 'Martin Wainwright', 'Martin J. Wainwright, Emin Martinian', 'Low-density graph codes that are optimal for source/channel coding and\n  binning', 'Appeared as technical report 730, Dept. of Statistics, UC Berkeley.\n  Portions previously published in conference form (DCC 2006; ISIT 2006)', '', '', 'Technical report 730', 'cs.IT math.IT', '', '  We describe and analyze the joint source/channel coding properties of a class\nof sparse graphical codes based on compounding a low-density generator matrix\n(LDGM) code with a low-density parity check (LDPC) code. Our first pair of\ntheorems establish that there exist codes from this ensemble, with all degrees\nremaining bounded independently of block length, that are simultaneously\noptimal as both source and channel codes when encoding and decoding are\nperformed optimally. More precisely, in the context of lossy compression, we\nprove that finite degree constructions can achieve any pair $(R, D)$ on the\nrate-distortion curve of the binary symmetric source. In the context of channel\ncoding, we prove that finite degree codes can achieve any pair $(C, p)$ on the\ncapacity-noise curve of the binary symmetric channel. Next, we show that our\ncompound construction has a nested structure that can be exploited to achieve\nthe Wyner-Ziv bound for source coding with side information (SCSI), as well as\nthe Gelfand-Pinsker bound for channel coding with side information (CCSI).\nAlthough the current results are based on optimal encoding and decoding, the\nproposed graphical codes have sparse structure and high girth that renders them\nwell-suited to message-passing and other efficient decoding procedures.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:33:43 GMT\"}]', '2007-07-13', '[[\"Wainwright\",\"Martin J.\",\"\"],[\"Martinian\",\"Emin\",\"\"]]'),
(704.1819, 'Yuji Tachikawa', 'Kentaro Hanaki, Keisuke Ohashi and Yuji Tachikawa', 'Comments on Charges and Near-Horizon Data of Black Rings', '30 pages, 1 figure; v2: additional references; v3: published version', 'JHEP0712:057,2007', '10.1088/1126-6708/2007/12/057', 'TIT/HEP-570', 'hep-th', '', '  We study how the charges of the black rings measured at the asymptotic\ninfinity are encoded in the near-horizon metric and gauge potentials,\nindependent of the detailed structure of the connecting region. Our analysis\nclarifies how different sets of four-dimensional charges can be assigned to a\nsingle five-dimensional object under the Kaluza-Klein reduction. Possible\nchoices are related by the Witten effect on dyons and by the large gauge\ntransformation in four and five dimensions, respectively.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 13:59:57 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 30 Apr 2007 20:37:19 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 17 Dec 2007 16:16:52 GMT\"}]', '2008-11-26', '[[\"Hanaki\",\"Kentaro\",\"\"],[\"Ohashi\",\"Keisuke\",\"\"],[\"Tachikawa\",\"Yuji\",\"\"]]'),
(704.1820, 'Oriol T. Valls', 'Klaus Halterman, Paul H. Barsic, and Oriol T. Valls', 'Odd Triplet Pairing in clean Superconductor/Ferromagnet heterostructures', 'Four pages, including four figures', 'Phys. Rev Lett. 99, 127002 (2007)', '10.1103/PhysRevLett.99.127002', '', 'cond-mat.supr-con', '', '  We study triplet pairing correlations in clean Ferromagnet (F)/Superconductor\n(S) nanojunctions, via fully self consistent solution of the Bogoliubov-de\nGennes equations. We consider FSF trilayers, with S being an s-wave\nsuperconductor, and an arbitrary angle $\\alpha$ between the magnetizations of\nthe two F layers. We find that contrary to some previous expectations, triplet\ncorrelations, odd in time, are induced in both the S and F layers in the clean\nlimit. We investigate their behavior as a function of time, position, and\n$\\alpha$. The triplet amplitudes are largest at times on the order of the\ninverse ``Debye\'\' frequency, and at that time scale they are long ranged in\nboth S and F. The zero temperature condensation energy is found to be lowest\nwhen the magnetizations are antiparallel.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 21:47:43 GMT\"}]', '2009-11-13', '[[\"Halterman\",\"Klaus\",\"\"],[\"Barsic\",\"Paul H.\",\"\"],[\"Valls\",\"Oriol T.\",\"\"]]'),
(704.1821, 'Matthew Reece', 'Kaustubh Agashe, Csaba Csaki, Christophe Grojean, Matthew Reece', 'The S-parameter in Holographic Technicolor Models', '21 pages, 2 figures. v2: references added', 'JHEP 0712:003,2007', '10.1088/1126-6708/2007/12/003', '', 'hep-ph', '', '  We study the S parameter, considering especially its sign, in models of\nelectroweak symmetry breaking (EWSB) in extra dimensions, with fermions\nlocalized near the UV brane. Such models are conjectured to be dual to 4D\nstrong dynamics triggering EWSB. The motivation for such a study is that a\nnegative value of S can significantly ameliorate the constraints from\nelectroweak precision data on these models, allowing lower mass scales (TeV or\nbelow) for the new particles and leading to easier discovery at the LHC. We\nfirst extend an earlier proof of S>0 for EWSB by boundary conditions in\narbitrary metric to the case of general kinetic functions for the gauge fields\nor arbitrary kinetic mixing. We then consider EWSB in the bulk by a Higgs VEV\nshowing that S is positive for arbitrary metric and Higgs profile, assuming\nthat the effects from higher-dimensional operators in the 5D theory are\nsub-leading and can therefore be neglected. For the specific case of AdS_5 with\na power law Higgs profile, we also show that S ~ + O(1), including effects of\npossible kinetic mixing from higher-dimensional operator (of NDA size) in the\n$5D$ theory. Therefore, our work strongly suggests that S is positive in\ncalculable models in extra dimensions.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 15:43:51 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Jul 2007 10:15:21 GMT\"}]', '2009-01-06', '[[\"Agashe\",\"Kaustubh\",\"\"],[\"Csaki\",\"Csaba\",\"\"],[\"Grojean\",\"Christophe\",\"\"],[\"Reece\",\"Matthew\",\"\"]]'),
(704.1822, 'Zuoliang Hou', 'Zuoliang Hou and Qi Li', 'Energy Functionals for the Parabolic Monge-Ampere Equation', '12 pages', '', '', '', 'math.AP math.DG', '', '  We introduce certain energy functionals to the complex Monge-Ampere equation\nover a bounded domain with inhomogeneous boundary condition, and use these\nfunctionals to show the convergence of the solution to the parabolic\nMonge-Ampere equation.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:39:33 GMT\"}]', '2007-05-23', '[[\"Hou\",\"Zuoliang\",\"\"],[\"Li\",\"Qi\",\"\"]]'),
(704.1823, 'Alejandro Adem', 'Alejandro Adem, Jianquan Ge, Jianzhong Pan and Nansen Petrosyan', 'Compatible Actions and Cohomology of Crystallographic Groups', '', '', '', '', 'math.AT math.GR', '', '  We compute the cohomology of crystallographic groups with holonomy of prime\norder. As an application we compute the group of gerbes associated to many\nsix--dimensional toroidal orbifolds arising in string theory.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:41:10 GMT\"}]', '2007-05-23', '[[\"Adem\",\"Alejandro\",\"\"],[\"Ge\",\"Jianquan\",\"\"],[\"Pan\",\"Jianzhong\",\"\"],[\"Petrosyan\",\"Nansen\",\"\"]]'),
(704.1824, 'Yaozhong Hu', 'Yaozhong Hu, David Nualart', 'Stochastic Heat Equation Driven by Fractional Noise and Local Time', '', '', '', '', 'math.PR math.AP', '', '  The aim of this paper is to study the $d$-dimensional stochastic heat\nequation with a multiplicative Gaussian noise which is white in space and it\nhas the covariance of a fractional Brownian motion with Hurst parameter $% H\\in\n(0,1)$ in time. Two types of equations are considered. First we consider the\nequation in the It\\^{o}-Skorohod sense, and later in the Stratonovich sense. An\nexplicit chaos development for the solution is obtained. On the other hand, the\nmoments of the solution are expressed in terms of the exponential moments of\nsome weighted intersection local time of the Brownian motion.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 20:48:34 GMT\"}]', '2007-05-23', '[[\"Hu\",\"Yaozhong\",\"\"],[\"Nualart\",\"David\",\"\"]]'),
(704.1825, 'Antoine Merand', 'A. M\\\'erand, J. Audenberg, P. Kervella, V. Coud\\\'e du Foresto, T. ten\n  Brummelaar, H. McAlister, et al', 'Extended envelopes around Galactic Cepheids III. Y Oph and alpha Per\n  from near-infrared interferometry with CHARA/FLUOR', 'accepted for publication in ApJ', 'Astrophys.J.664:1093-1101,2007', '10.1086/518597', '', 'astro-ph', '', '  Unbiased angular diameter measurements are required for accurate distances to\nCepheids using the interferometric Baade Wesselink method (IBWM). The precision\nof this technique is currently limited by interferometric measurements at the\n1.5% level. At this level, the center-to-limb darkening (CLD) and the presence\nof circumstellar envelopes (CSE) seem to be the two main sources of bias. The\nobservations we performed aim at improving our knowledge of the interferometric\nvisibility profile of Cepheids. In particular, we assess the systematic\npresence of CSE around Cepheids in order determine accurate distances with the\nIBWM free from CSE biased angular diameters. We observed a Cepheid (Y Oph) for\nwhich the pulsation is well resolved and a non-pulsating yellow supergiant\n(alpha Per) using long-baseline near-infrared interferometry. We interpreted\nthese data using a simple CSE model we previously developed. We found that our\nobservations of alpha Per do not provide evidence for a CSE. The measured CLD\nis explained by an hydrostatic photospheric model. Our observations of Y Oph,\nwhen compared to smaller baseline measurements, suggest that it is surrounded\nby a CSE with similar characteristics to CSE found previously around other\nCepheids. We have determined the distance to Y Oph to be d=491+/-18 pc.\nAdditional evidence points toward the conclusion that most Cepheids are\nsurrounded by faint CSE, detected by near infrared interferometry: after\nobserving four Cepheids, all show evidence for a CSE. Our CSE non-detection\naround a non-pulsating supergiant in the instability strip, alpha Per, provides\nconfidence in the detection technique and suggests a pulsation driven mass-loss\nmechanism for the Cepheids.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 21:39:59 GMT\"}]', '2009-06-23', '[[\"Mérand\",\"A.\",\"\"],[\"Audenberg\",\"J.\",\"\"],[\"Kervella\",\"P.\",\"\"],[\"Foresto\",\"V. Coudé du\",\"\"],[\"Brummelaar\",\"T. ten\",\"\"],[\"McAlister\",\"H.\",\"\"]]'),
(704.1826, 'Michael Klasen', 'G. Bozzi (ITP Karlsruhe), B. Fuks, B. Herrmann, M. Klasen (LPSC\n  Grenoble)', 'Squark and Gaugino Hadroproduction and Decays in Non-Minimal Flavour\n  Violating Supersymmetry', '35 pages, 29 (partly colour) figures. Some typos corrected, wording\n  of several paragraphs improved, version accepted by Nucl. Phys. B', 'Nucl.Phys.B787:1-54,2007', '10.1016/j.nuclphysb.2007.05.031', 'KA-TP-07-2007, LPSC 07-023, SFB/CPP-07-09', 'hep-ph', '', '  We present an extensive analysis of squark and gaugino hadroproduction and\ndecays in non-minimal flavour violating supersymmetry. We employ the so-called\nsuper-CKM basis to define the possible misalignment of quark and squark\nrotations, and we use generalized (possibly complex) charges to define the\nmutual couplings of (s)quarks and gauge bosons/gauginos. The cross sections for\nall squark-(anti-)squark/gaugino pair and squark-gaugino associated production\nprocesses as well as their decay widths are then given in compact analytic\nform. For four different constrained supersymmetry breaking models with\nnon-minimal flavour violation in the second/third generation squark sector\nonly, we establish the parameter space regions allowed/favoured by low-energy,\nelectroweak precision, and cosmological constraints and display the chirality\nand flavour decomposition of all up- and down-type squark mass eigenstates.\nFinally, we compute numerically the dependence of a representative sample of\nproduction cross sections at the LHC on the off-diagonal mass matrix elements\nin the experimentally allowed/favoured ranges.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 10 Apr 2007 11:39:10 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 1 Jun 2007 13:39:42 GMT\"}]', '2008-11-26', '[[\"Bozzi\",\"G.\",\"\",\"ITP Karlsruhe\"],[\"Fuks\",\"B.\",\"\",\"LPSC\\n  Grenoble\"],[\"Herrmann\",\"B.\",\"\",\"LPSC\\n  Grenoble\"],[\"Klasen\",\"M.\",\"\",\"LPSC\\n  Grenoble\"]]'),
(704.1827, 'Gerald Krafft', 'Gerald Krafft', 'Transaction-Oriented Simulation In Ad Hoc Grids', '101 pages (plus 131 appendix), 23 figures, 11 tables, MSc thesis for\n  degree in Advanced Computer Science at the Westminster University, London', '', '', '', 'cs.DC', '', '  This paper analyses the possibilities of performing parallel\ntransaction-oriented simulations with a special focus on the space-parallel\napproach and discrete event simulation synchronisation algorithms that are\nsuitable for transaction-oriented simulation and the target environment of Ad\nHoc Grids. To demonstrate the findings a Java-based parallel\ntransaction-oriented simulator for the simulation language GPSS/H is\nimplemented on the basis of the promising Shock Resistant Time Warp\nsynchronisation algorithm and using the Grid framework ProActive. The\nvalidation of this parallel simulator shows that the Shock Resistant Time Warp\nalgorithm can successfully reduce the number of rolled back Transaction moves\nbut it also reveals circumstances in which the Shock Resistant Time Warp\nalgorithm can be outperformed by the normal Time Warp algorithm. The conclusion\nof this paper suggests possible improvements to the Shock Resistant Time Warp\nalgorithm to avoid such problems.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 6 Apr 2007 15:59:27 GMT\"}]', '2007-05-23', '[[\"Krafft\",\"Gerald\",\"\"]]'),
(704.1828, 'Dennis D. Dietrich', 'Dennis D. Dietrich', 'Gauge invariance in gravity-like descriptions of massive gauge field\n  theories', '11 pages', '', '', '', 'hep-th', '', '  We discuss gravity-like formulations of massive Abelian and non-Abelian gauge\nfield theories in four space-time dimensions with particular emphasis on the\nissue of gauge invariance. Alternative descriptions in terms of antisymmetric\ntensor fields and geometric variables, respectively, are analysed. In both\napproaches St\\\"uckelberg degrees of freedom factor out. We also demonstrate, in\nthe Abelian case, that the massless limit for the gauge propagator, which does\nnot exist in the vector potential formulation, is well-defined for the\nantisymmetric tensor fields.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 21:51:21 GMT\"}]', '2007-05-23', '[[\"Dietrich\",\"Dennis D.\",\"\"]]'),
(704.1829, 'Kamil Kloch', 'Stefan Felsner, Kamil Kloch, Grzegorz Matecki, and Piotr Micek', 'On-line Chain Partitions of Up-growing Semi-orders', '', '', '', '', 'cs.DM', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  On-line chain partition is a two-player game between Spoiler and Algorithm.\nSpoiler presents a partially ordered set, point by point. Algorithm assigns\nincoming points (immediately and irrevocably) to the chains which constitute a\nchain partition of the order. The value of the game for orders of width $w$ is\na minimum number $\\fVal(w)$ such that Algorithm has a strategy using at most\n$\\fVal(w)$ chains on orders of width at most $w$. We analyze the chain\npartition game for up-growing semi-orders. Surprisingly, the golden ratio comes\ninto play and the value of the game is $\\lfloor\\frac{1+\\sqrt{5}}{2}\\; w\n\\rfloor$.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:41:21 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 20 Sep 2007 21:51:26 GMT\"},{\"version\":\"v3\",\"created\":\"Sat, 19 Feb 2011 21:18:10 GMT\"}]', '2011-02-22', '[[\"Felsner\",\"Stefan\",\"\"],[\"Kloch\",\"Kamil\",\"\"],[\"Matecki\",\"Grzegorz\",\"\"],[\"Micek\",\"Piotr\",\"\"]]'),
(704.1830, 'Bogdan Wojtsekhowski', 'D. J. Hamilton, A. Shahinyan, B. Wojtsekhowski, J. R. M. Annand, T.-H.\n  Chang, E. Chudakov, A. Danagoulian, P. Degtyarenko, K. Egiyan, R. Gilman, V.\n  Gorbenko, J. Hines, E. Hovhannisyan, C. E. Hyde-Wright, C.W. de Jager, A.\n  Ketikyan, V. H. Mamyan, R. Michaels, A. M. Nathan, V. Nelyubin, I. Rachek, M.\n  Roedelbrom, A. Petrosyan, R. Pomatsalyuk, V. Popov, J. Segal, Y. Shestakov,\n  J. Templon, H. Voskanyan', 'An Electromagnetic Calorimeter for the JLab Real Compton Scattering\n  Experiment', 'text updated according to published version', 'Nuclear Instruments and Methods A, Volume 643, Issue 1, 1 July\n  2011, Pages 17-28', '', 'JLAB-PHY-07-633', 'physics.ins-det nucl-ex', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  A lead-glass hodoscope calorimeter that was constructed for use in the\nJefferson Lab Real Compton Scattering experiment is described. The detector\nprovides a measurement of the coordinates and the energy of scattered photons\nin the GeV energy range with resolutions of 5 mm and 6%/\\sqrt(E{\\gamma} [GeV]).\nFeatures of both the detector design and its performance in the high luminosity\nenvironment during the experiment are presented.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 17:09:07 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 17 Mar 2011 15:11:26 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 25 Sep 2015 14:22:08 GMT\"}]', '2015-09-28', '[[\"Hamilton\",\"D. J.\",\"\"],[\"Shahinyan\",\"A.\",\"\"],[\"Wojtsekhowski\",\"B.\",\"\"],[\"Annand\",\"J. R. M.\",\"\"],[\"Chang\",\"T. -H.\",\"\"],[\"Chudakov\",\"E.\",\"\"],[\"Danagoulian\",\"A.\",\"\"],[\"Degtyarenko\",\"P.\",\"\"],[\"Egiyan\",\"K.\",\"\"],[\"Gilman\",\"R.\",\"\"],[\"Gorbenko\",\"V.\",\"\"],[\"Hines\",\"J.\",\"\"],[\"Hovhannisyan\",\"E.\",\"\"],[\"Hyde-Wright\",\"C. E.\",\"\"],[\"de Jager\",\"C. W.\",\"\"],[\"Ketikyan\",\"A.\",\"\"],[\"Mamyan\",\"V. H.\",\"\"],[\"Michaels\",\"R.\",\"\"],[\"Nathan\",\"A. M.\",\"\"],[\"Nelyubin\",\"V.\",\"\"],[\"Rachek\",\"I.\",\"\"],[\"Roedelbrom\",\"M.\",\"\"],[\"Petrosyan\",\"A.\",\"\"],[\"Pomatsalyuk\",\"R.\",\"\"],[\"Popov\",\"V.\",\"\"],[\"Segal\",\"J.\",\"\"],[\"Shestakov\",\"Y.\",\"\"],[\"Templon\",\"J.\",\"\"],[\"Voskanyan\",\"H.\",\"\"]]'),
(704.1831, 'Elena Bratkovskaya', 'V.P. Konchakovski, M.I. Gorenstein and E.L. Bratkovskaya', 'Multiplicity Fluctuations in Au+Au Collisions at RHIC', '7 pages, 3 figures, submitted to Phys. Rev. C (Rapid Communication)', 'Phys.Rev.C76:031901,2007', '10.1103/PhysRevC.76.031901', 'FIAS070413', 'nucl-th', '', '  The preliminary data of the PHENIX collaboration for the scaled variances of\ncharged hadron multiplicity fluctuations in Au+Au at $\\sqrt{s}=200$ GeV are\nanalyzed within the model of independent sources. We use the HSD transport\nmodel to calculate the participant number fluctuations and the number of\ncharged hadrons per nucleon participant in different centrality bins. This\ncombined picture leads to a good agreement with the PHENIX data and suggests\nthat the measured multiplicity fluctuations result dominantly from participant\nnumber fluctuations. The role of centrality selection and acceptance is\ndiscussed separately.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:09:47 GMT\"}]', '2008-11-26', '[[\"Konchakovski\",\"V. P.\",\"\"],[\"Gorenstein\",\"M. I.\",\"\"],[\"Bratkovskaya\",\"E. L.\",\"\"]]'),
(704.1832, 'Luisa Rebull', 'John R. Stauffer (SSC), Lee W. Hartmann (Univ Michigan), Giovanni G.\n  Fazio (CfA), Lori E. Allen (CfA), Brian M. Patten (CfA), Patrick J. Lowrance\n  (SSC), Robert L. Hurt (SSC), Luisa M. Rebull (SSC), Roc M. Cutri (IPAC),\n  Solange V. Ramirez (IPAC), Erick T. Young (Univ Arizona), George H. Rieke\n  (Univ Arizona), Nadya I. Gorlova (Univ Arizona), James C. Muzerolle (Univ\n  Arizona), Cathy L. Slesnick (Caltech), Michael F. Skrutskie (Univ Virginia)', 'Near and Mid-IR Photometry of the Pleiades, and a New List of Substellar\n  Candidate Members', 'Accepted to ApJS; data tables and embedded-figure version available\n  at http://spider.ipac.caltech.edu/staff/stauffer/pleiades07/', '', '10.1086/518961', '', 'astro-ph', '', '  We make use of new near and mid-IR photometry of the Pleiades cluster in\norder to help identify proposed cluster members. We also use the new photometry\nwith previously published photometry to define the single-star main sequence\nlocus at the age of the Pleiades in a variety of color-magnitude planes.\n  The new near and mid-IR photometry extend effectively two magnitudes deeper\nthan the 2MASS All-Sky Point Source catalog, and hence allow us to select a new\nset of candidate very low mass and sub-stellar mass members of the Pleiades in\nthe central square degree of the cluster. We identify 42 new candidate members\nfainter than Ks =14 (corresponding to 0.1 Mo). These candidate members should\neventually allow a better estimate of the cluster mass function to be made down\nto of order 0.04 solar masses.\n  We also use new IRAC data, in particular the images obtained at 8 um, in\norder to comment briefly on interstellar dust in and near the Pleiades. We\nconfirm, as expected, that -- with one exception -- a sample of low mass stars\nrecently identified as having 24 um excesses due to debris disks do not have\nsignificant excesses at IRAC wavelengths. However, evidence is also presented\nthat several of the Pleiades high mass stars are found to be impacting with\nlocal condensations of the molecular cloud that is passing through the Pleiades\nat the current epoch.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:19:23 GMT\"}]', '2009-11-13', '[[\"Stauffer\",\"John R.\",\"\",\"SSC\"],[\"Hartmann\",\"Lee W.\",\"\",\"Univ Michigan\"],[\"Fazio\",\"Giovanni G.\",\"\",\"CfA\"],[\"Allen\",\"Lori E.\",\"\",\"CfA\"],[\"Patten\",\"Brian M.\",\"\",\"CfA\"],[\"Lowrance\",\"Patrick J.\",\"\",\"SSC\"],[\"Hurt\",\"Robert L.\",\"\",\"SSC\"],[\"Rebull\",\"Luisa M.\",\"\",\"SSC\"],[\"Cutri\",\"Roc M.\",\"\",\"IPAC\"],[\"Ramirez\",\"Solange V.\",\"\",\"IPAC\"],[\"Young\",\"Erick T.\",\"\",\"Univ Arizona\"],[\"Rieke\",\"George H.\",\"\",\"Univ Arizona\"],[\"Gorlova\",\"Nadya I.\",\"\",\"Univ Arizona\"],[\"Muzerolle\",\"James C.\",\"\",\"Univ\\n  Arizona\"],[\"Slesnick\",\"Cathy L.\",\"\",\"Caltech\"],[\"Skrutskie\",\"Michael F.\",\"\",\"Univ Virginia\"]]'),
(704.1833, 'Inanc Inan', 'Inanc Inan, Feyza Keceli, Ender Ayanoglu', 'Analysis of the 802.11e Enhanced Distributed Channel Access Function', '', '', '', '', 'cs.NI', '', '  The IEEE 802.11e standard revises the Medium Access Control (MAC) layer of\nthe former IEEE 802.11 standard for Quality-of-Service (QoS) provision in the\nWireless Local Area Networks (WLANs). The Enhanced Distributed Channel Access\n(EDCA) function of 802.11e defines multiple Access Categories (AC) with\nAC-specific Contention Window (CW) sizes, Arbitration Interframe Space (AIFS)\nvalues, and Transmit Opportunity (TXOP) limits to support MAC-level QoS and\nprioritization. We propose an analytical model for the EDCA function which\nincorporates an accurate CW, AIFS, and TXOP differentiation at any traffic\nload. The proposed model is also shown to capture the effect of MAC layer\nbuffer size on the performance. Analytical and simulation results are compared\nto demonstrate the accuracy of the proposed approach for varying traffic loads,\nEDCA parameters, and MAC layer buffer space.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:40:05 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 26 Oct 2007 05:59:08 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 28 Mar 2008 05:21:34 GMT\"}]', '2008-03-28', '[[\"Inan\",\"Inanc\",\"\"],[\"Keceli\",\"Feyza\",\"\"],[\"Ayanoglu\",\"Ender\",\"\"]]'),
(704.1834, 'Dmitri Volja', 'Dmitri Volja, Wei-Guo Yin and Wei Ku', 'Charge Ordering in Half-Doped Manganites: Weak Charge Disproportion and\n  Leading Mechanisms', 'accepted by Europhysics Letters', 'Europhysics Letters 89, 27008 (2010)', '10.1209/0295-5075/89/27008', '', 'cond-mat.str-el', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  The apparent contradiction between the recently observed weak charge\ndisproportion and the traditional Mn$^{3+}$/Mn$^{4+}$ picture of the\ncharge-orbital orders in half-doped manganites is resolved by a novel Wannier\nstates analysis of the LDA$+U$ electronic structure. Strong electron itinerancy\nin this charge-transfer system significantly delocalizes the occupied\nlow-energy \"Mn$^{3+}$\" Wannier states such that charge leaks into the\n\"Mn$^{4+}$\"-sites. Furthermore, the leading mechanisms of the charge order are\nquantified via our first-principles derivation of the low-energy effective\nHamiltonian. The electron-electron interaction is found to play a role as\nimportant as the electron-lattice interaction. \\ignore{A general picture of\ndoped holes in strongly correlated charge-transfer systems is presented and\napplied to the study of charge order in half-doped manganites, using a novel\nWannier states analysis of the LDA$+U$ electronic structure. While residing\nprimarily in the oxygen atoms, the doped holes form additional effective $e_g$\norbitals at the low-energy scale, leading to an effective Mn$^{3+}$/Mn$^{4+}$\nvalence picture that enables weak charge disproportion, resolving the current\nserious contradictions between the recent experimental observations of charge\ndistribution and traditional models. Furthermore, the leading mechanisms of the\nobserved charge order are quantified via our first-principles derivation of the\nlow-energy effective Hamiltonian\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 19:10:58 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 7 Jan 2010 00:23:53 GMT\"}]', '2015-05-13', '[[\"Volja\",\"Dmitri\",\"\"],[\"Yin\",\"Wei-Guo\",\"\"],[\"Ku\",\"Wei\",\"\"]]'),
(704.1835, 'Darren Forde', 'Darren Forde', 'Direct extraction of one-loop integral coefficients', '42 pages, 7 figures', 'Phys.Rev.D75:125019,2007', '10.1103/PhysRevD.75.125019', 'SLAC-PUB-12455, UCLA/07/TEP/12', 'hep-ph', '', '  We present a general procedure for obtaining the coefficients of the scalar\nbubble and triangle integral functions of one-loop amplitudes. Coefficients are\nextracted by considering two-particle and triple unitarity cuts of the\ncorresponding bubble and triangle integral functions. After choosing a specific\nparameterisation of the cut loop momentum we can uniquely identify the\ncoefficients of the desired integral functions simply by examining the\nbehaviour of the cut integrand as the unconstrained parameters of the cut loop\nmomentum approach infinity. In this way we can produce compact forms for scalar\nintegral coefficients. Applications of this method are presented for both QCD\nand electroweak processes, including an alternative form for the recently\ncomputed three-mass triangle coefficient in the six-photon amplitude\n$A_6(1^-,2^+,3^-,4^+,5^-,6^+)$. The direct nature of this extraction procedure\nallows for a very straightforward automation of the procedure.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 01:13:11 GMT\"}]', '2008-11-26', '[[\"Forde\",\"Darren\",\"\"]]'),
(704.1836, 'Hitoshi Nishino', 'Hitoshi Nishino and Subhash Rajpoot', 'Comment on Electroweak Higgs as a Pseudo-Goldstone Boson of Broken Scale\n  Invariance', '2 pages, no figure', '', '', 'CSULB-PA-07-4', 'hep-ph hep-th', '', '  The first model of Foot, Kobakhidze and Volkas described in their work in\narXiv:0704.1165 [hep-ph] is a tailored version of our model on broken scale\ninvariance in the standard model presented in hep-th/0403039.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:53:47 GMT\"}]', '2007-05-23', '[[\"Nishino\",\"Hitoshi\",\"\"],[\"Rajpoot\",\"Subhash\",\"\"]]'),
(704.1837, 'Hiroki Wadati', 'H. Wadati, Y. Hotta, A. Fujimori, T. Susaki, H. Y. Hwang, Y. Takata,\n  K. Horiba, M. Matsunami, S. Shin, M. Yabashi, K. Tamasaku, Y. Nishino, and T.\n  Ishikawa', 'Hard x-ray photoemission study of LaAlO3/LaVO3 multilayers', '5 pages, 7 figures', 'Phys. Rev. B 77, 045122 (2008)', '10.1103/PhysRevB.77.045122', '', 'cond-mat.str-el cond-mat.mtrl-sci', '', '  We have studied the electronic structure of multilayers composed of a band\ninsulator LaAlO$_3$ (LAO) and a Mott insulator LaVO$_3$ (LVO) by means of hard\nx-ray photoemission spectroscopy, which has a probing depth as large as $\\sim\n60 {\\AA}$. The Mott-Hubbard gap of LVO remained open at the interface,\nindicating that the interface is insulating unlike the LaTiO$_3$/SrTiO$_3$\nmultilayers. We found that the valence of V in LVO were partially converted\nfrom V$^{3+}$ to V$^{4+}$ only at the interface on the top side of the LVO\nlayer and that the amount of V$^{4+}$ increased with LVO layer thickness. We\nsuggest that the electronic reconstruction to eliminate the polarity\ncatastrophe inherent in the polar heterostructure is the origin of the highly\nasymmetric valence change at the LVO/LAO interfaces.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 22:54:17 GMT\"}]', '2008-01-18', '[[\"Wadati\",\"H.\",\"\"],[\"Hotta\",\"Y.\",\"\"],[\"Fujimori\",\"A.\",\"\"],[\"Susaki\",\"T.\",\"\"],[\"Hwang\",\"H. Y.\",\"\"],[\"Takata\",\"Y.\",\"\"],[\"Horiba\",\"K.\",\"\"],[\"Matsunami\",\"M.\",\"\"],[\"Shin\",\"S.\",\"\"],[\"Yabashi\",\"M.\",\"\"],[\"Tamasaku\",\"K.\",\"\"],[\"Nishino\",\"Y.\",\"\"],[\"Ishikawa\",\"T.\",\"\"]]'),
(704.1838, 'Inanc Inan', 'Inanc Inan, Feyza Keceli, Ender Ayanoglu', 'Performance Analysis of the IEEE 802.11e Enhanced Distributed\n  Coordination Function using Cycle Time Approach', '', '', '', '', 'cs.OH', '', '  The recently ratified IEEE 802.11e standard defines the Enhanced Distributed\nChannel Access (EDCA) function for Quality-of-Service (QoS) provisioning in the\nWireless Local Area Networks (WLANs). The EDCA uses Carrier Sense Multiple\nAccess with Collision Avoidance (CSMA/CA) and slotted Binary Exponential\nBackoff (BEB) mechanism. We present a simple mathematical analysis framework\nfor the EDCA function. Our analysis considers the fact that the distributed\nrandom access systems exhibit cyclic behavior where each station successfully\ntransmits a packet in a cycle. Our analysis shows that an AC-specific cycle\ntime exists for the EDCA function. Validating the theoretical results via\nsimulations, we show that the proposed analysis accurately captures EDCA\nsaturation performance in terms of average throughput, medium access delay, and\npacket loss ratio. The cycle time analysis is a simple and insightful\nsubstitute for previously proposed more complex EDCA models.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 23:01:40 GMT\"}]', '2007-05-23', '[[\"Inan\",\"Inanc\",\"\"],[\"Keceli\",\"Feyza\",\"\"],[\"Ayanoglu\",\"Ender\",\"\"]]'),
(704.1839, 'Vladimir Makarenko', 'V. Makarenko', 'ALHEP symbolic algebra program for high-energy physics', '33 pages, 4 figures', '', '', '', 'hep-ph', '', '  ALHEP is the symbolic algebra program for high-energy physics. It deals with\namplitudes calculation, matrix element squaring, Wick theorem, dimensional\nregularization, tensor reduction of loop integrals and simplification of final\nexpressions. The program output includes: Fortran code for differential cross\nsection, Mathematica files to view results and intermediate steps and TeX\nsource for Feynman diagrams. The PYTHIA interface is available. The project\nwebsite http://www.hep.by/alhep contains up-to-date executables, manual and\nscript examples.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 23:02:17 GMT\"}]', '2007-05-23', '[[\"Makarenko\",\"V.\",\"\"]]'),
(704.1840, 'Mya Warren', 'Mya Warren and Joerg Rottler', 'Simulations of aging and plastic deformation in polymer glasses', '9 pages, 12 figures', '', '10.1103/PhysRevE.76.031802', '', 'cond-mat.soft cond-mat.mtrl-sci', '', '  We study the effect of physical aging on the mechanical properties of a model\npolymer glass using molecular dynamics simulations. The creep compliance is\ndetermined simultaneously with the structural relaxation under a constant\nuniaxial load below yield at constant temperature. The model successfully\ncaptures universal features found experimentally in polymer glasses, including\nsignatures of mechanical rejuvenation. We analyze microscopic relaxation\ntimescales and show that they exhibit the same aging characteristics as the\nmacroscopic creep compliance. In addition, our model indicates that the entire\ndistribution of relaxation times scales identically with age. Despite large\nchanges in mobility, we observe comparatively little structural change except\nfor a weak logarithmic increase in the degree of short-range order that may be\ncorrelated to an observed decrease in aging with increasing load.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 23:05:22 GMT\"}]', '2009-11-13', '[[\"Warren\",\"Mya\",\"\"],[\"Rottler\",\"Joerg\",\"\"]]'),
(704.1841, 'Joan Najita', 'Joan R. Najita, John S. Carr, Alfred E. Glassgold, and Jeff Valenti', 'Gaseous Inner Disks', '16 pages, 6 figures, a chapter in \"Protostars and Planets V\"', '', '', '', 'astro-ph', '', '  As the likely birthplaces of planets and an essential conduit for the buildup\nof stellar masses, inner disks are of fundamental interest in star and planet\nformation. Studies of the gaseous component of inner disks are of interest\nbecause of their ability to probe the dynamics, physical and chemical\nstructure, and gas content of this region. We review the observational and\ntheoretical developments in this field, highlighting the potential of such\nstudies to, e.g., measure inner disk truncation radii, probe the nature of the\ndisk accretion process, and chart the evolution in the gas content of disks.\nMeasurements of this kind have the potential to provide unique insights on the\nphysical processes governing star and planet formation.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 23:07:56 GMT\"}]', '2007-05-23', '[[\"Najita\",\"Joan R.\",\"\"],[\"Carr\",\"John S.\",\"\"],[\"Glassgold\",\"Alfred E.\",\"\"],[\"Valenti\",\"Jeff\",\"\"]]'),
(704.1842, 'Inanc Inan', 'Feyza Keceli, Inanc Inan, Ender Ayanoglu', 'Fairness Provision in the IEEE 802.11e Infrastructure Basic Service Set', '', '', '', '', 'cs.OH', '', '  Most of the deployed IEEE 802.11e Wireless Local Area Networks (WLANs) use\ninfrastructure Basic Service Set (BSS) in which an Access Point (AP) serves as\na gateway between wired and wireless domains. We present the unfairness problem\nbetween the uplink and the downlink flows of any Access Category (AC) in the\n802.11e Enhanced Distributed Channel Access (EDCA) when the default settings of\nthe EDCA parameters are used. We propose a simple analytical model to calculate\nthe EDCA parameter settings that achieve weighted fair resource allocation for\nall uplink and downlink flows. We also propose a simple model-assisted\nmeasurement-based dynamic EDCA parameter adaptation algorithm. Moreover, our\ndynamic solution addresses the differences in the transport layer and the\nMedium Access Control (MAC) layer interactions of User Datagram Protocol (UDP)\nand Transmission Control Protocol (TCP). We show that proposed Contention\nWindow (CW) and Transmit Opportunity (TXOP) limit adaptation at the AP provides\nfair UDP and TCP access between uplink and downlink flows of the same AC while\npreserving prioritization among ACs.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 23:11:27 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 13 Sep 2007 15:08:17 GMT\"}]', '2007-09-13', '[[\"Keceli\",\"Feyza\",\"\"],[\"Inan\",\"Inanc\",\"\"],[\"Ayanoglu\",\"Ender\",\"\"]]'),
(704.1843, 'Edison Liang', 'Edison Liang and Koichi Noguchi', 'Radiation from Kinetic Poynting Flux Acceleration', '25 pages, 11 figures, revised paper resubmitted to Astrophysical\n  Journal', '', '', '', 'astro-ph', '', '  We derive analytic formulas for the power output and critical frequency of\nradiation by electrons accelerated by relativistic kinetic Poynting flux, and\nvalidate these results with Particle-In-Cell plasma simulations. We find that\nthe in-situ radiation power output and critical frequency are much below those\npredicted by the classical synchrotron formulae. We discuss potential\nastrophysical applications of these results.\n', '[{\"version\":\"v1\",\"created\":\"Fri, 13 Apr 2007 23:20:54 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 18 Nov 2007 20:23:37 GMT\"}]', '2007-11-18', '[[\"Liang\",\"Edison\",\"\"],[\"Noguchi\",\"Koichi\",\"\"]]'),
(704.1844, 'Kazuyuki Fujii', 'Kazuyuki Fujii (Yokohama City University)', 'A New Algebraic Structure of Finite Quantum Systems and the Modified\n  Bessel Functions', 'Latex ; 14 pages ; no figure ; minor changes. To appear in\n  International Journal of Geometric Methods in Modern Physics, (Vo.4, No.7),\n  2007', 'Int.G.Geom.Meth.Mod.Phys. 4(2007) 1205-1215', '10.1142/S021988780700251X', '', 'quant-ph math-ph math.MP', '', '  In this paper we present a new algebraic structure (a super hyperbolic system\nin our terminology) for finite quantum systems, which is a generalization of\nthe usual one in the two-level system.\n  It fits into the so-called generalized Pauli matrices, so they play an\nimportant role in the theory. Some deep relation to the modified Bessel\nfunctions of integer order is pointed out.\n  By taking a skillful limit finite quantum systems become quantum mechanics on\nthe circle developed by Ohnuki and Kitakado.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 00:20:40 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Jul 2007 00:08:48 GMT\"}]', '2015-05-13', '[[\"Fujii\",\"Kazuyuki\",\"\",\"Yokohama City University\"]]'),
(704.1845, 'Donal O\'Connell', 'Benjamin Grinstein, Donal O\'Connell and Mark B. Wise', 'The Lee-Wick Standard Model', '20 pages, 4 figures. Improved discussion and reference added. Contour\n  prescription clarified', 'Phys.Rev.D77:025012,2008', '10.1103/PhysRevD.77.025012', 'CALT 68-2643, UCSD/PTH 07-04', 'hep-ph hep-th', '', '  We construct a modification of the standard model which stabilizes the Higgs\nmass against quadratically divergent radiative corrections, using ideas\noriginally discussed by Lee and Wick in the context of a finite theory of\nquantum electrodynamics. The Lagrangian includes new higher derivative\noperators. We show that the higher derivative terms can be eliminated by\nintroducing a set of auxiliary fields; this allows for convenient computation\nand makes the physical interpretation more transparent. Although the theory is\nunitary, it does not satisfy the usual analyticity conditions.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 01:25:57 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 1 May 2007 08:32:51 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 24 Jul 2007 13:15:12 GMT\"}]', '2008-11-26', '[[\"Grinstein\",\"Benjamin\",\"\"],[\"O\'Connell\",\"Donal\",\"\"],[\"Wise\",\"Mark B.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1846, 'Meinolf Geck', 'Meinolf Geck, Lacrimioara Iancu and Christos Pallikaros', 'Specht modules and Kazhdan--Lusztig cells in type $B_n$', 'the revised version corrects some minor errors', '', '', '', 'math.RT', '', '  Dipper, James and Murphy generalized the classical Specht module theory to\nHecke algebras of type $B_n$. On the other hand, for any choice of a monomial\norder on the parameters in type $B_n$, we obtain corresponding Kazhdan--Lusztig\ncell modules. In this paper, we show that the Specht modules are naturally\nequivalent to the Kazhdan--Lusztig cell modules {\\em if} we choose the\ndominance order on the parameters, as in the ``asymptotic case\'\' studied by\nBonnaf\\\'e and the second named author. We also give examples which show that\nsuch an equivalence does not hold for other choices of monomial orders.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 19:52:02 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 13 Jun 2007 12:36:43 GMT\"}]', '2007-06-13', '[[\"Geck\",\"Meinolf\",\"\"],[\"Iancu\",\"Lacrimioara\",\"\"],[\"Pallikaros\",\"Christos\",\"\"]]'),
(704.1847, 'Daniel Fraiman', 'Daniel Fraiman', 'Growing Networks: Limit in-degree distribution for arbitrary out-degree\n  one', '12 pages, 6 figures, v2 adds a section on descriptive statistics, an\n  analisis on www network, typos added', 'The European Physical Journal B 61 3 (2008) 377-388', '10.1140/epjb/e2008-00075-3', '', 'physics.soc-ph physics.data-an', '', '  We compute the stationary in-degree probability, $P_{in}(k)$, for a growing\nnetwork model with directed edges and arbitrary out-degree probability. In\nparticular, under preferential linking, we find that if the nodes have a light\ntail (finite variance) out-degree distribution, then the corresponding\nin-degree one behaves as $k^{-3}$. Moreover, for an out-degree distribution\nwith a scale invariant tail, $P_{out}(k)\\sim k^{-\\alpha}$, the corresponding\nin-degree distribution has exactly the same asymptotic behavior only if\n$2<\\alpha<3$ (infinite variance). Similar results are obtained when\nattractiveness is included. We also present some results on descriptive\nstatistics measures %descriptive statistics such as the correlation between the\nnumber of in-going links, $D_{in}$, and outgoing links, $D_{out}$, and the\nconditional expectation of $D_{in}$ given $D_{out}$, and we calculate these\nmeasures for the WWW network. Finally, we present an application to the\nscientific publications network. The results presented here can explain the\ntail behavior of in/out-degree distribution observed in many real networks.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 01:29:04 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 12 Oct 2007 12:23:26 GMT\"}]', '2008-10-21', '[[\"Fraiman\",\"Daniel\",\"\"]]'),
(704.1848, 'Shinji Tsujikawa', 'Maxim Libanov, Eleftherios Papantonopoulos, Valery Rubakov, M. Sami,\n  Shinji Tsujikawa', 'UV stable, Lorentz-violating dark energy with transient phantom era', '22 pages, 7 figures; Presentation modified substantially, results and\n  conclusions unchanged. Journal version', 'JCAP0708:010,2007', '10.1088/1475-7516/2007/08/010', '', 'hep-th astro-ph gr-qc hep-ph', '', '  Phantom fields with negative kinetic energy are often plagued by the vacuum\nquantum instability in the ultraviolet region. We present a Lorentz-violating\ndark energy model free from this problem and show that the crossing of the\ncosmological constant boundary w=-1 to the phantom equation of state is\nrealized before reaching a de Sitter attractor. Another interesting feature is\na peculiar time-dependence of the effective Newton\'s constant; the magnitude of\nthis effect is naturally small but may be close to experimental limits. We also\nderive momentum scales of instabilities at which tachyons or ghosts appear in\nthe infrared region around the present Hubble scale and clarify the conditions\nunder which tachyonic instabilities do not spoil homogeneity of the\npresent/future Universe.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 02:58:52 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 19 Jul 2007 00:46:31 GMT\"}]', '2008-11-26', '[[\"Libanov\",\"Maxim\",\"\"],[\"Papantonopoulos\",\"Eleftherios\",\"\"],[\"Rubakov\",\"Valery\",\"\"],[\"Sami\",\"M.\",\"\"],[\"Tsujikawa\",\"Shinji\",\"\"]]'),
(704.1849, 'Sheng-Jun Wang', 'Sheng-Jun Wang, An-Cai Wu, Zhi-Xi Wu, Xin-Jian Xu, Ying-Hai Wang', 'Response of degree-correlated scale-free networks to stimuli', '5 pages, 5 figures', 'Physical Review E 75, 046113 (2007)', '10.1103/PhysRevE.75.046113', '', 'cond-mat.dis-nn', '', '  The response of degree-correlated scale-free attractor networks to stimuli is\nstudied. We show that degree-correlated scale-free networks are robust to\nrandom stimuli as well as the uncorrelated scale-free networks, while\nassortative (disassortative) scale-free networks are more (less) sensitive to\ndirected stimuli than uncorrelated networks. We find that the\ndegree-correlation of scale-free networks makes the dynamics of attractor\nsystems different from uncorrelated ones. The dynamics of correlated scale-free\nattractor networks result in the effects of degree correlation on the response\nto stimuli.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 03:19:46 GMT\"}]', '2007-07-05', '[[\"Wang\",\"Sheng-Jun\",\"\"],[\"Wu\",\"An-Cai\",\"\"],[\"Wu\",\"Zhi-Xi\",\"\"],[\"Xu\",\"Xin-Jian\",\"\"],[\"Wang\",\"Ying-Hai\",\"\"]]'),
(704.1850, 'Damian Swift', 'Damian C. Swift, Achim Seifter, David B. Holtkamp, David A. Clark', 'Shock and Release Temperatures in Molybdenum', '', 'Physical Review B, vol 76, 054122 (2007)', '10.1103/PhysRevB.76.054122', 'LA-UR-07-1660', 'cond-mat.mtrl-sci', '', '  Shock and release temperatures in Mo were calculated, taking account of\nheating from plastic flow predicted using the Steinberg-Guinan model. Plastic\nflow was calculated self-consistently with the shock jump conditions: this is\nnecessary for a rigorous estimate of the locus of shock states accessible. The\ntemperatures obtained were significantly higher than predicted assuming ideal\nhydrodynamic loading. The temperatures were compared with surface emission\nspectrometry measurements for Mo shocked to around 60GPa and then released into\nvacuum or into a LiF window. Shock loading was induced by the impact of a\nplanar projectile, accelerated by high explosive or in a gas gun. Surface\nvelocimetry showed an elastic wave at the start of release from the shocked\nstate; the amplitude of the elastic wave matched the prediction to around 10%,\nindicating that the predicted flow stress in the shocked state was reasonable.\nThe measured temperatures were consistent with the simulations, indicating that\nthe fraction of plastic work converted to heat was in the range 70-100% for\nthese loading conditions.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 03:28:22 GMT\"}]', '2009-11-13', '[[\"Swift\",\"Damian C.\",\"\"],[\"Seifter\",\"Achim\",\"\"],[\"Holtkamp\",\"David B.\",\"\"],[\"Clark\",\"David A.\",\"\"]]'),
(704.1851, 'Shengli Kong', 'Shengli Kong, Peter Li and Detang Zhou', 'Spectrum of the Laplacian on Quaternionic Kahler Manifolds', '46 pages', 'J. Differential Geom. 78 (2008), 295-332', '', '', 'math.DG', '', '  Let $M^{4n}$ be a complete quaternionic K\\\"ahler manifold with scalar\ncurvature bounded below by $-16n(n+2)$. We get a sharp estimate for the first\neigenvalue $\\lambda_1(M)$ of the Laplacian which is $\\lambda_1(M)\\le (2n+1)^2$.\nIf the equality holds, then either $M$ has only one end, or $M$ is\ndiffeomorphic to $\\mathbb{R}\\times N$ with N given by a compact manifold.\nMoreover, if $M$ is of bounded curvature, $M$ is covered by the quaterionic\nhyperbolic space $\\mathbb{QH}^n$ and $N$ is a compact quotient of the\ngeneralized Heisenberg group. When $\\lambda_1(M)\\ge \\frac{8(n+2)}3$, we also\nprove that $M$ must have only one end with infinite volume.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 03:40:22 GMT\"}]', '2011-03-14', '[[\"Kong\",\"Shengli\",\"\"],[\"Li\",\"Peter\",\"\"],[\"Zhou\",\"Detang\",\"\"]]'),
(704.1852, 'Ellen Williams', 'O. Bondarchuk, W.G. Cullen, M. Degawa and Ellen D. Williams', 'Biased Structural Fluctuations due to Electron Wind Force', '15 pages', '', '', '', 'cond-mat.mtrl-sci cond-mat.stat-mech', '', '  Direct correlation between temporal structural fluctuations and electron wind\nforce is demonstrated, for the first time, by STM imaging and analysis of\natomically-resolved motion on a thin film surface under large applied current\n(10e5 Amp/sqare cm). The magnitude of the momentum transfer between current\ncarriers and atoms in the fluctuating structure is at least five to fifteen\ntimes (plus or minus one sigma range) larger than for freely diffusing adatoms.\nThe corresponding changes in surface resistivity will contribute significant\nfluctuation signature to nanoscale electronic properties.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 04:08:56 GMT\"}]', '2007-05-23', '[[\"Bondarchuk\",\"O.\",\"\"],[\"Cullen\",\"W. G.\",\"\"],[\"Degawa\",\"M.\",\"\"],[\"Williams\",\"Ellen D.\",\"\"]]'),
(704.1853, 'Hajime Susa', 'Hideki Maki and Hajime Susa', 'Dissipation of Magnetic Flux in Primordial Star Formation: From Run-away\n  Phase to Mass Accretion Phase', '12 pages, 7 figures, PASJ accepted', '', '10.1093/pasj/59.4.787', '', 'astro-ph', '', '  We investigate the dissipation of magnetic flux in primordial star-forming\nclouds throughout their collapse including the run-away collapse phase as well\nas the accretion phase. We solve the energy equation and the non-equilibrium\nchemical reactions in the collapsing gas, in order to obtain the radial\ndistribution of the ionized fraction during the collapse. As a result, we find\nthe ionized fraction is high enough for the magnetic field to couple with the\ngas throughout the evolution of the cloud. This result suggests that the jet\nformation from protostars as well as the activation of magneto-rotational\ninstability in the accretion disk are enabled in the presence of the\ncosmological seed magnetic flux proposed by Langer et al.(2003).\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 04:37:57 GMT\"}]', '2019-08-19', '[[\"Maki\",\"Hideki\",\"\"],[\"Susa\",\"Hajime\",\"\"]]'),
(704.1854, 'Sanjoy Mahajan', 'Sanjoy Mahajan', 'Teaching for transfer', '3 pages, 3 figures, ConTeXt, GPL free-software license; from a\n  workshop on curriculum integration at MIT (2006-09-25)', '', '', '', 'physics.ed-ph', '', '  Students, after they leave our care, are called to solve the diverse problems\nof the world, so we should teach to increase transfer: the ability to apply\nfundamental principles to new problems and contexts. This ability is rare. The\nfollowing pages are from a workshop for faculty on designing courses that\npromote transfer. I discuss two design principles: to name the transferable\nideas and to illustrate them with examples from diverse subjects. The\ndiscussion uses dimensional reasoning as the example of a valuable transferable\nidea, illustrating it with three diverse examples.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 05:15:31 GMT\"}]', '2007-05-23', '[[\"Mahajan\",\"Sanjoy\",\"\"]]'),
(704.1855, 'Tianjun Li', 'Ching-Ming Chen, Tianjun Li, V. E. Mayes, Dimitri V. Nanopoulos', 'Variations of the Hidden Sector in a Realistic Intersecting Brane Model', 'RevTex4, 15 pages, 10 tables', 'J.Phys.G35:095008,2008', '10.1088/0954-3899/35/9/095008', 'ACT-02-07, MIFP-07-11', 'hep-th', '', '  Recently, we discussed the first example of a phenomenologically realistic\nintersecting D6-brane model. In this model, the gauge symmetry in the hidden\nsector is USp(2)_1 x USp(2)_2 x USp(2)_3 x USp(2)_4. However, we find that the\nUSp(2)_1 x USp(2)_2 gauge symmetry can be replaced by an U(2)_{12} gauge\nsymmetry, and/or the USp(2)_3 x USp(2)_4 gauge symmetry can be replaced by an\nU(2)_{34} gauge symmetry since the USp(2)^2 stacks of D6-branes contribute to\nthe same Ramond-Ramond tadpoles as those of the U(2) stacks. Thus, there are\nthree non-equivalent variations of the hidden sector, and the corresponding\ngauge symmetries are U(2)_{12} x USp(2)_3 x USp(2)_4, U(2)_{34} x USp(2)_1 x\nUSp(2)_2, and U(2)_{12} x U(2)_{34}, respectively. Moreover, we study the\nhidden sector gauge symmetry breaking, discuss how to decouple the additional\nexotic particles, and briefly comment on the phenomenological consequences.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 00:17:36 GMT\"}]', '2008-11-26', '[[\"Chen\",\"Ching-Ming\",\"\"],[\"Li\",\"Tianjun\",\"\"],[\"Mayes\",\"V. E.\",\"\"],[\"Nanopoulos\",\"Dimitri V.\",\"\"]]'),
(704.1856, 'Yoshiko Kanada-En\'yo', 'Yoshiko Kanada-En\'yo, Osamu Morimatsu and Tetsuo Nishikawa', 'Axial Vector Tetraquark with Two s-quarks', 'prepared for Yukawa International Seminars \"New Frontiers in QCD\"\n  (YKIS2006), Nov. 20-Dec. 8, 2006, Kyoto, Japan, to appear in Prog. Theor.\n  Phys. Suppl', 'Prog.Theor.Phys.Suppl.168:194-197,2007', '10.1143/PTPS.168.194', '', 'nucl-th', '', '  Possibility of an axial vector isoscalar tetraquark $ud\\bar{s}\\bar{s}$ is\ndiscussed. If a $f_1$ meson in the mass region $1.4-1.5$ GeV consists of four\nquarks $ns\\bar{n}\\bar{s}$, the mass of the isoscalar\n$ud\\bar{s}\\bar{s}$($\\vartheta^+$-meson) state with $J^P=1^+$ is expected to be\nlower than that of the $f_1$ meson. Within a flux-tube quark model, a possible\nresonant state of $ud\\bar{s}\\bar{s}(J^{P}=1^{+})$ is suggested to appear at\n$\\sim$ 1.4 GeV with the width ${\\cal{O}}(20\\sim 50)$ MeV. We propose that the\n$\\vartheta^+$-meson is the good candidate for the tetraquark search, which\nwould be observed in the $K^+K^+\\pi^-$ decay channel.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 08:31:30 GMT\"}]', '2008-11-26', '[[\"Kanada-En\'yo\",\"Yoshiko\",\"\"],[\"Morimatsu\",\"Osamu\",\"\"],[\"Nishikawa\",\"Tetsuo\",\"\"]]'),
(704.1857, 'Hsiao-Ping Hsu', 'Hsiao-Ping Hsu, Kurt Binder, Leonid I. Klushin, and Alexander M.\n  Skvortsov', 'What is the order of 2D polymer escape transition?', '16 pages, 21 figures, and 4 tables. Edited for typos', 'Phys. Rev. E 76, 021108 (2007)', '10.1103/PhysRevE.76.021108', '', 'cond-mat.stat-mech cond-mat.soft', '', '  An end-grafted flexible polymer chain in 3d space between two pistons\nundergoes an abrupt transition from a confined coil to a flower-like\nconformation when the number of monomers in the chain, N, reaches a critical\nvalue. In 2d geometry, excluded volume interactions between monomers of a chain\nconfined inside a strip of finite length 2L transform the coil conformation\ninto a linear string of blobs. However, the blob picture raises questions on\nthe nature of this escape transition. To check the theoretical predictions\nbased on the blob picture we study 2d single polymer chains with excluded\nvolume interactions and with one end grafted in the middle of a strip of length\n  2L and width H by simulating self-avoiding walks on a square lattice with the\npruned-enriched-Rosenbluth method (PERM). We estimate the free energy, the\nend-to-end distance, the number of imprisoned monomers, the order parameter,\nand its distribution. It is shown that in the thermodynamic limit of large N\nand L but finite L/N, there is a small but finite jump in several average\ncharacteristics, including the order parameter. We also present a theoretical\ndescription based on the Landau free energy approach, which is in good\nagreement with the simulation results. Both simulation results and the\nanalytical theory indicate that the 2d escape transition is a weak first-order\nphase transition.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 09:45:33 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 10 Sep 2007 12:00:16 GMT\"}]', '2009-11-13', '[[\"Hsu\",\"Hsiao-Ping\",\"\"],[\"Binder\",\"Kurt\",\"\"],[\"Klushin\",\"Leonid I.\",\"\"],[\"Skvortsov\",\"Alexander M.\",\"\"]]'),
(704.1858, 'Fabian Walter', 'Fabian Walter and Chris Carilli', 'Detecting the Most Distant (z>7) Objects with ALMA', 'to appear in Astrophysics and Space Science, \"Science with ALMA: a\n  new era for Astrophysics\", ed. R. Bachiller', 'Astrophys.Space Sci.313:313-316,2008', '10.1007/s10509-007-9634-1', '', 'astro-ph', '', '  Detecting and studying objects at the highest redshifts, out to the end of\nCosmic Reionization at z>7, is clearly a key science goal of ALMA. ALMA will in\nprinciple be able to detect objects in this redshift range both from high-J\n(J>7) CO transitions and emission from ionized carbon, [CII], which is one of\nthe main cooling lines of the ISM. ALMA will even be able to resolve this\nemission for individual targets, which will be one of the few ways to determine\ndynamical masses for systems in the Epoch of Reionization. We discuss some of\nthe current problems regarding the detection and characterization of objects at\nhigh redshifts and how ALMA will eliminate most (but not all) of them.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 10:00:18 GMT\"}]', '2009-06-23', '[[\"Walter\",\"Fabian\",\"\"],[\"Carilli\",\"Chris\",\"\"]]'),
(704.1859, 'Ryszard Szwarc', 'T. Pytlik, R. Szwarc', 'Weak type radial convolution operators on free group', '', '', '', '', 'math.FA', '', '  Radial convolution operators on free groups with nonnegative kernel of weak\ntype $(2,2)$ and of restricted weak type $(2,2)$ are characterized. Estimates\nof weak type $(p,p)$ are obtained as well for $1<p<2.$\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 10:53:15 GMT\"}]', '2007-05-23', '[[\"Pytlik\",\"T.\",\"\"],[\"Szwarc\",\"R.\",\"\"]]'),
(704.1860, 'Chien Peng', 'Chien Y. Peng (STScI)', 'How Mergers May Affect The Mass Scaling Relations Between Black Holes,\n  Galaxies, and Other Gravitationally Bound Systems', '10 pages, 8 figures, ApJ in press, includes ApJ corrections', '', '10.1086/522774', '', 'astro-ph', '', '  Supermassive black hole (BH) masses (MBH) are strongly correlated with galaxy\nstellar bulge masses (Mbulge) and there are several ideas to explain the origin\nof this relationship. This study isolates the role of galaxy mergers from\nconsiderations of other detailed physics to more clearly show how a linear\nBH-galaxy mass relation (MBH-Mgal) can naturally emerge regardless of how\nprimordial BHs were seeded inside galaxies, if the galaxy mass function\ndeclines with increasing mass. Under this circumstance, the MBH-Mgal relation\nis a passive attractor that eventually converges to a tight linear relation\nbecause of two basic statistical effects: a central limit-like tendency for\ngalaxy mergers which is much stronger for major mergers than minor mergers, and\na convergence toward a linear relation that is due mainly to minor mergers. A\ncurious consequence of this thought experiment is that, if galaxy bulges are\nformed by major mergers, then merging statistics naturally show that MBH would\ncorrelate more strongly with bulge dominated galaxies, because of stronger\ncentral-seeking tendencies, than with disk dominated galaxies. Even if some\nother physics is ultimately responsible for causing a linear MBH-Mbulge\nrelationship, this thought experiment shows that, counter to intuition, random\nmerging of galaxies that harbor random BH masses tends to strengthen rather\nthan weaken a pre-existing, linear, correlation. This idea may be generalized\nto other gravitationally bound systems (dark matter halo, compact nuclear\nobjects) that retain their physical identities after experiencing mergers.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 18:56:32 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 20 Apr 2007 17:37:32 GMT\"},{\"version\":\"v3\",\"created\":\"Sat, 21 Apr 2007 16:51:01 GMT\"},{\"version\":\"v4\",\"created\":\"Fri, 10 Aug 2007 18:20:45 GMT\"},{\"version\":\"v5\",\"created\":\"Wed, 24 Oct 2007 04:48:03 GMT\"}]', '2009-11-13', '[[\"Peng\",\"Chien Y.\",\"\",\"STScI\"]]'),
(704.1861, 'Mauricio Sepulveda', 'Mauricio Sepulveda (GI2MA), Octavio Vera', 'Analycity and smoothing effect for the coupled system of equations of\n  Korteweg - de Vries type with a single point singularity', '', 'Acta Applicandae Mathematicae. vol 113, 1 (2011)', '10.1007/s10440-010-9586-2', '', 'math.AP', '', '  We study that a solution of the initial value problem associated for the\ncoupled system of equations of Korteweg - de Vries type which appears as a\nmodel to describe the strong interaction of weakly nonlinear long waves, has\nanalyticity in time and smoothing effect up to real analyticity if the initial\ndata only has a single point singularity at $x=0.$\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 11:13:42 GMT\"}]', '2013-10-30', '[[\"Sepulveda\",\"Mauricio\",\"\",\"GI2MA\"],[\"Vera\",\"Octavio\",\"\"]]'),
(704.1862, 'Mauricio Sepulveda', 'Mauricio Sepulveda (GI2MA), Octavio Vera', 'Smoothing properties for the higher order nonlinear Schr\\\"{o}dinger\n  equation with constant coefficients', '', 'Nonlinear Analysis, TMA, Vol 71 (2009) 948-966', '10.1016/j.na.2008.11.010', '', 'math.AP', '', '  We study local and global existence and smoothing properties for the initial\nvalue problem associated to a higher order nonlinear Schr\\\"odinger equation\nwith constant coefficients which appears as a model for propagation of pulse in\noptical fiber.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 11:15:03 GMT\"}]', '2013-10-30', '[[\"Sepulveda\",\"Mauricio\",\"\",\"GI2MA\"],[\"Vera\",\"Octavio\",\"\"]]'),
(704.1863, 'Gerhard Mallot', 'COMPASS Collaboration, M. Alekseev, et al', 'Double spin asymmetry in exclusive rho^0 muoproduction at COMPASS', '6 Figures, 15 pages, version 2 with updated author list, technical\n  latex problem fixed', 'Eur.Phys.J.C52:255-265,2007', '10.1140/epjc/s10052-007-0376-6', 'CERN-PH-EP_2007-009', 'hep-ex', '', '  The longitudinal double spin asymmetry A_1^rho for exclusive leptoproduction\nof rho^0 mesons, mu + N -> mu + N + rho, is studied using the COMPASS 2002 and\n2003 data. The measured reaction is incoherent exclusive rho^0 production on\npolarised deuterons. The Q^2 and x dependence of A_1^rho is presented in a wide\nkinematical range: 3x10^-3 < Q^2 < 7 (GeV/c)^2 and 5x10^-5 < x < 0.05. The\npresented results are the first measurements of A_1^rho at small Q2 (Q2 < 0.1\n(GeV/c)^2) and small x (x < 3x10^-3). The asymmetry is in general compatible\nwith zero in the whole kinematical range.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 12:25:50 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 10 Jul 2007 15:36:37 GMT\"}]', '2008-11-26', '[[\"COMPASS Collaboration\",\"\",\"\"],[\"Alekseev\",\"M.\",\"\"]]'),
(704.1864, 'Jonas Schou Neergaard-Nielsen', 'J. S. Neergaard-Nielsen, B. Melholt Nielsen, H. Takahashi, A. I.\n  Vistnes, and E. S. Polzik', 'High purity bright single photon source', '9 pages, 4 figures; minor changes, added reference', 'Opt. Express 15, 7940-7949 (2007)', '10.1364/OE.15.007940', '', 'quant-ph', '', '  Using cavity-enhanced non-degenerate parametric downconversion, we have built\na frequency tunable source of heralded single photons with a narrow bandwidth\nof 8 MHz, making it compatible with atomic quantum memories. The photon state\nis 70% pure single photon as characterized by a tomographic measurement and\nreconstruction of the quantum state, revealing a clearly negative Wigner\nfunction. Furthermore, it has a spectral brightness of ~1,500 photons/s per MHz\nbandwidth, making it one of the brightest single photon sources available. We\nalso investigate the correlation function of the down-converted fields using a\ncombination of two very distinct detection methods; photon counting and\nhomodyne measurement.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 12:18:28 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 5 Jun 2007 06:30:10 GMT\"}]', '2009-11-13', '[[\"Neergaard-Nielsen\",\"J. S.\",\"\"],[\"Nielsen\",\"B. Melholt\",\"\"],[\"Takahashi\",\"H.\",\"\"],[\"Vistnes\",\"A. I.\",\"\"],[\"Polzik\",\"E. S.\",\"\"]]'),
(704.1865, 'SongPing Zhou', 'Dan Sheng Yu, Ping Zhou and Song Ping Zhou', 'On $L^{1}$-Convergence of Fourier Series Under $MVBV$ Condition', '13 Pages, Accepted by Canad. Math. Bull', '', '', '', 'math.CA', '', '  Let $f\\in L_{2\\pi}$ be a real-valued even function with its Fourier series $\n\\frac{a_{0}}{2}+\\sum_{n=1}^{\\infty}a_{n}\\cos nx,$ and let $S_{n}(f,x), n\\geq\n1,$ be the $n$-th partial sum of the Fourier series. It is well-known that if\nthe nonnegative sequence $\\{a_{n}\\}$ is decreasing and $\\lim\\limits_{n\\to\n\\infty}a_{n}=0$, then $$ \\lim\\limits_{n\\to \\infty}\\Vert f-S_{n}(f)\\Vert_{L}=0\n{if and only if} \\lim\\limits_{n\\to \\infty}a_{n}\\log n=0. $$ We weaken the\nmonotone condition in this classical result to the so-called mean value bounded\nvariation ($MVBV$) condition. The generalization of the above classical result\nin real-valued function space is presented as a special case of the main result\nin this paper which gives the $L^{1}$% -convergence of a function $f\\in\nL_{2\\pi}$ in complex space. We also give results on $L^{1}$-approximation of a\nfunction $f\\in L_{2\\pi}$ under the $% MVBV$ condition.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 12:50:22 GMT\"}]', '2007-05-23', '[[\"Yu\",\"Dan Sheng\",\"\"],[\"Zhou\",\"Ping\",\"\"],[\"Zhou\",\"Song Ping\",\"\"]]'),
(704.1866, 'Changxing Miao', 'Changxing Miao, Junyong Zhang', 'On global solution to the Klein-Gordon-Hartree equation below energy\n  space', '31 pages', 'J. Differential Equations, 250 (2011) 3418-3447', '10.1016/j.jde.2010.12.010', '', 'math.AP math-ph math.MP', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  In this paper, we consider the Cauchy problem for Klein-Gordon equation with\na cubic convolution nonlinearity in $\\R^3$. By making use of Bourgain\'s method\nin conjunction with a precise Strichartz estimate of S.Klainerman and D.Tataru,\nwe establish the $H^s (s<1)$ global well-posedness of the Cauchy problem for\nthe cubic convolution defocusing Klein-Gordon-Hartree equation. Before arriving\nat the previously discussed conclusion, we obtain global solution for this\nnon-scaling equation with small initial data in $H^{s_0}\\times H^{s_0-1}$ where\n$s_0=\\frac\\gamma 6$ but not $\\frac\\gamma2-1$, for this equation that we\nconsider is a subconformal equation in some sense. In doing so a number of\nnonlinear prior estimates are already established by using Bony\'s\ndecomposition, flexibility of Klein-Gordon admissible pairs which are slightly\ndifferent from that of wave equation and a commutator estimate. We establish\nthis commutator estimate by exploiting cancellation property and utilizing\nCoifman and Meyer multilinear multiplier theorem. As far as we know, it seems\nthat this is the first result on low regularity for this Klein-Gordon-Hartree\nequation.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 13:16:38 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 5 May 2007 13:41:41 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 28 May 2007 01:43:08 GMT\"},{\"version\":\"v4\",\"created\":\"Sat, 6 Jun 2009 01:33:30 GMT\"}]', '2011-02-22', '[[\"Miao\",\"Changxing\",\"\"],[\"Zhang\",\"Junyong\",\"\"]]'),
(704.1867, 'Heiko Bauke', 'Heiko Bauke', 'Parameter estimation for power-law distributions by maximum likelihood\n  methods', 'Supplementary software:\n  http://www.physics.ox.ac.uk/users/bauke/Publications/index.html#powerlaws', 'The European Physical Journal B, vol. 58, no. 2, pp. 167-173\n  (2007)', '10.1140/epjb/e2007-00219-y', '', 'cond-mat.other physics.data-an', '', '  Distributions following a power-law are an ubiquitous phenomenon. Methods for\ndetermining the exponent of a power-law tail by graphical means are often used\nin practice but are intrinsically unreliable. Maximum likelihood estimators for\nthe exponent are a mathematically sound alternative to graphical methods.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 14:29:00 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 11 Aug 2007 11:36:30 GMT\"}]', '2007-08-11', '[[\"Bauke\",\"Heiko\",\"\"]]'),
(704.1868, 'Jan H. Bruinier', 'Jan H. Bruinier and Oliver Stein', 'The Weil representation and Hecke operators for vector valued modular\n  forms', '23 pages', '', '', '', 'math.NT', '', '  We define Hecke operators on vector valued modular forms transforming with\nthe Weil representation associated to a discriminant form. We describe the\nproperties of the corresponding algebra of Hecke operators and study the action\non modular forms.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 13:46:52 GMT\"}]', '2007-05-23', '[[\"Bruinier\",\"Jan H.\",\"\"],[\"Stein\",\"Oliver\",\"\"]]'),
(704.1869, 'Nagalakshmi Rao A', 'Nagalakshmi A Rao and B. A. Kagali', 'On the energy spectrum of the one-dimensional Klein-Gordon Oscillator', 'Latex, 9 Pages, 1 Table, Added Reference', 'Physica Scripta Phys.Scr 77(2008) 015003 (4pp)', '', '', 'quant-ph', '', '  In the present article, we describe a method of introducing the harmonic\npotential into the Klein-Gordon equation, leading to genuine bound states. The\neigenfunctions and eigenenergies are worked out explicitly.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 13:54:31 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Apr 2007 17:17:06 GMT\"}]', '2008-11-06', '[[\"Rao\",\"Nagalakshmi A\",\"\"],[\"Kagali\",\"B. A.\",\"\"]]'),
(704.1870, 'Rochal Serguei', 'A.E.Myasnikova, E.N. Myasnikov', 'Band in ARPES caused by photodissociation of Landau-Pekar polarons', '8 pages, 6 figures', '', '', '', 'cond-mat.supr-con cond-mat.other', '', '  We consider decay of phonon condensate into phonons at photodissociation of\nthe strong coupling large polaron (SCLP), when the charge carrier becomes free.\nExpression to calculate the band in ARPES caused by photodissociation of SCLP\nis obtained. The band in ARPES caused by photodissociation of strong-coupling\nlarge-radius polarons is a broad band with the shape determined by Poisson\ndistribution. It can be structured or unstructured depending on the phonon\ndispersion since a distance between neighbouring lines comprising the band is\nthe phonon energy. Half-width of the band is in the interval 1.3 - 1.7Ep,\ndepending on the phonon energy. The band maximum is situated approximately at\nthe electron energy Ephot-W-3.2Ep (where Ephot is the photon energy, W is work\nfunction), and its position does not depend on the electron wave vector\ndirection.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 14:02:37 GMT\"}]', '2007-05-23', '[[\"Myasnikova\",\"A. E.\",\"\"],[\"Myasnikov\",\"E. N.\",\"\"]]'),
(704.1871, 'Andres Balaguera', 'A. Balaguera-Antolinez, M. Nowakowski', 'From Global to Local Dynamics: Effects of the Expansion on Astrophysical\n  Structures', 'References added To be published in CQG', 'Class.Quant.Grav.24:2677-2688,2007', '10.1088/0264-9381/24/10/013', '', 'gr-qc', '', '  We explore the effects of background cosmology on large scale structures with\nnon-spherical symmetry by using the concept of quasi-equilibrium which allows\ncertain internal properties (e.g. angular velocity) of the bodies to change\nwith time. In accordance with the discovery of the accelerated phase of the\nuniverse we model the cosmological background by two representative models: the\n$\\Lambda$CDM Model and the Chaplygin Gas Model. We compare the effects of the\ntwo models on various properties of large astrophysical objects. Different\nequations of state are also invoked in the investigation.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 16:49:41 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Apr 2007 16:37:47 GMT\"}]', '2008-11-26', '[[\"Balaguera-Antolinez\",\"A.\",\"\"],[\"Nowakowski\",\"M.\",\"\"]]'),
(704.1872, 'Vladimir Kozhevnikov', 'V.F. Kozhevnikov, C.V. Giuraniuc, M.J. Van Bael, K. Temst, C. Van\n  Haesendonck, T.M. Mishonov, T. Charlton, R.M. Dalgliesh, Yu.N. Khaidukov,\n  Yu.V. Nikitenko, V.L. Aksenov, V.N. Gladilin, V.M. Fomin, J.T. Devreese, and\n  J.O. Indekeu', 'Evidence for nonmonotonic magnetic field penetration in a type-I\n  superconductor', '5 pages, 4 figures, LaTex, corrected typos and figures', '', '10.1103/PhysRevB.78.012502', '', 'cond-mat.supr-con', '', '  Polarized neutron reflectometry (PNR) provides evidence that nonlocal\nelectrodynamics governs the magnetic field penetration in an extreme low-k\nsuperconductor. The sample is an indium film with a large elastic mean free\npath (11 mkm) deposited on a silicon oxide wafer. It is shown that PNR can\nresolve the difference between the reflected neutron spin asymmetries predicted\nby the local and nonlocal theories of superconductivity. The experimental data\nsupport the nonlocal theory, which predicts a nonmonotonic decay of the\nmagnetic field.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 15:18:59 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 6 Dec 2007 02:23:27 GMT\"}]', '2009-11-13', '[[\"Kozhevnikov\",\"V. F.\",\"\"],[\"Giuraniuc\",\"C. V.\",\"\"],[\"Van Bael\",\"M. J.\",\"\"],[\"Temst\",\"K.\",\"\"],[\"Van Haesendonck\",\"C.\",\"\"],[\"Mishonov\",\"T. M.\",\"\"],[\"Charlton\",\"T.\",\"\"],[\"Dalgliesh\",\"R. M.\",\"\"],[\"Khaidukov\",\"Yu. N.\",\"\"],[\"Nikitenko\",\"Yu. V.\",\"\"],[\"Aksenov\",\"V. L.\",\"\"],[\"Gladilin\",\"V. N.\",\"\"],[\"Fomin\",\"V. M.\",\"\"],[\"Devreese\",\"J. T.\",\"\"],[\"Indekeu\",\"J. O.\",\"\"]]'),
(704.1873, 'Yi Cao', 'Yi Cao and Biao Chen', 'An Achievable Rate Region for Interference Channels with Conferencing', '5 pages, 2 figures, accepted by ISIT\'07', '', '', '', 'cs.IT math.IT', '', '  In this paper, we propose an achievable rate region for discrete memoryless\ninterference channels with conferencing at the transmitter side. We employ\nsuperposition block Markov encoding, combined with simultaneous superposition\ncoding, dirty paper coding, and random binning to obtain the achievable rate\nregion. We show that, under respective conditions, the proposed achievable\nregion reduces to Han and Kobayashi achievable region for interference\nchannels, the capacity region for degraded relay channels, and the capacity\nregion for the Gaussian vector broadcast channel. Numerical examples for the\nGaussian case are given.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 15:42:44 GMT\"}]', '2007-07-13', '[[\"Cao\",\"Yi\",\"\"],[\"Chen\",\"Biao\",\"\"]]'),
(704.1874, 'Alexei Popov', 'Alexei V. Popov and Vladimir V. Kopeikin', 'Electromagnetic Pulse Propagation over Nonuniform Earth Surface:\n  Numerical Simulation', '', '', '', '', 'math.NA math-ph math.MP', '', '  We simulate EM pulse propagation along the nonuniform earth surface using so\ncalled time-domain parabolic equation. To solve it by finite differences, we\nintroduce a time-domain analog of the impedance boundary condition and a\nnonlocal BC of transparency reducing open computational domain to a strip of\nfinite width. Numerical examples demonstrate influence of soil conductivity on\nthe wide-band pulse waveform. For a high-frequency modulated EM pulse, we\ndevelop an asymptotic approach based on the ray structure of the monochromatic\nwave field at carrier frequency. This radically diminishes the computation\ncosts and allows for pulsed wave field calculation in vast domains measured by\ntens of thousands wavelengths.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 15:50:54 GMT\"}]', '2007-05-23', '[[\"Popov\",\"Alexei V.\",\"\"],[\"Kopeikin\",\"Vladimir V.\",\"\"]]'),
(704.1875, 'Gianluca Fiori', 'G. Fiori and G. Iannaccone', 'Simulation of Graphene Nanoribbon Field Effect Transistors', '', 'IEEE Electron Device Letters, Vol. 28, Issue 8, pp. 760 - 762,\n  2007', '10.1109/LED.2007.901680', '', 'cond-mat.mes-hall', '', '  We present an atomistic three-dimensional simulation of graphene nanoribbon\nfield effect transistors (GNR-FETs), based on the self-consistent solution of\nthe 3D Poisson and Schroedinger equation with open boundary conditions within\nthe non-equilibrium Green\'s Function formalism and a tight-binding hamiltonian.\nWith respect to carbon nanotube FETs, GNR-FETs exhibit comparable performance,\nreduced sensitivity on the variability of channel chirality, and similar\nleakage problems due to band-to-band tunneling. Acceptable transistor\nperformance requires effective nanoribbon width of 1-2 nm, that could be\nobtained with periodic etching patterns or stress patterns.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 16:07:49 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 7 Jan 2008 11:43:30 GMT\"}]', '2009-11-13', '[[\"Fiori\",\"G.\",\"\"],[\"Iannaccone\",\"G.\",\"\"]]'),
(704.1876, 'Scott Funkhouser', 'Scott Funkhouser', 'Stars and the holographic upper bound on gravitational action', '2 pages', '', '', '', 'physics.gen-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  The holographic upper bound on entropy is applied to the gravitational action\nassociated with the non-relativistic contraction of a nebula. A critical radius\nis identified, as a function of the initial radius and mass, for which the\nnumber of bits associated with the action would equal the maximum number of\nbits allowed to the body. The gravitational action of a typical star\napproximately saturates the holographic bound, perhaps suggesting a physical\nlink between holographic principles and astrophysical processes.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 16:23:57 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 21 Apr 2007 20:02:46 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 22 Dec 2008 18:34:16 GMT\"}]', '2008-12-22', '[[\"Funkhouser\",\"Scott\",\"\"]]'),
(704.1877, 'Stephen Doty', 'Stephen Doty', 'New versions of Schur-Weyl duality', 'Preprint from 2003', '', '', '', 'math.RT', '', '  After reviewing classical Schur-Weyl duality, we present some other contexts\nwhich enjoy similar features, relating to Brauer algebras and classical groups.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 16:29:41 GMT\"}]', '2007-05-23', '[[\"Doty\",\"Stephen\",\"\"]]'),
(704.1878, 'John D. Weeks', 'Jeng-Da Chai and John D Weeks', 'Orbital-Free Density Functional Theory: Kinetic Potentials and Ab-Initio\n  Local Pseudopotentials', 'To be published in Phys. Rev. B', '', '10.1103/PhysRevB.75.205122', '', 'cond-mat.str-el cond-mat.mtrl-sci', '', '  In the density functional (DF) theory of Kohn and Sham, the kinetic energy of\nthe ground state of a system of noninteracting electrons in a general external\nfield is calculated using a set of orbitals. Orbital free methods attempt to\ncalculate this directly from the electron density by approximating the\nuniversal but unknown kinetic energy density functional. However simple local\napproximations are inaccurate and it has proved very difficult to devise\ngenerally accurate nonlocal approximations. We focus instead on the kinetic\npotential, the functional derivative of the kinetic energy DF, which appears in\nthe Euler equation for the electron density. We argue that the kinetic\npotential is more local and more amenable to simple physically motivated\napproximations in many relevant cases, and describe two pathways by which the\nvalue of the kinetic energy can be efficiently calculated. We propose two\nnonlocal orbital free kinetic potentials that reduce to known exact forms for\nboth slowly varying and rapidly varying perturbations and also reproduce exact\nresults for the linear response of the density of the homogeneous system to\nsmall perturbations. A simple and systematic approach for generating accurate\nand weak ab-initio local pseudopotentials which produce a smooth slowly varying\nvalence component of the electron density is proposed for use in orbital free\nDF calculations of molecules and solids. The use of these local\npseudopotentials further minimizes the possible errors from the kinetic\npotentials. Our theory yields results for the total energies and ionization\nenergies of atoms, and for the shell structure in the atomic radial density\nprofiles that are in very good agreement with calculations using the full\nKohn-Sham theory.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 16:31:36 GMT\"}]', '2009-11-13', '[[\"Chai\",\"Jeng-Da\",\"\"],[\"Weeks\",\"John D\",\"\"]]'),
(704.1879, 'Johan Andersson', 'Johan Andersson', 'Lower bounds in some power sum problems', '9 pages', '', '', '', 'math.NT', '', '  We study the power sum problem max_{v=1,...,m} | sum_{k=1}^n z_k^v | and by\nusing features of Fejer kernels we give new lower bounds in the case of\nunimodular complex numbers z_k and m cn^2 for constants c>1.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 09:36:09 GMT\"}]', '2007-05-23', '[[\"Andersson\",\"Johan\",\"\"]]'),
(704.1880, 'Pasquale Calabrese', 'Pasquale Calabrese, John Cardy', 'Quantum Quenches in Extended Systems', '24 Pages, 4 figures', 'J.Stat.Mech.0706:P06008,2007', '10.1088/1742-5468/2007/06/P06008', '', 'cond-mat.stat-mech hep-th', '', '  We study in general the time-evolution of correlation functions in a extended\nquantum system after the quench of a parameter in the hamiltonian. We show that\ncorrelation functions in d dimensions can be extracted using methods of\nboundary critical phenomena in d+1 dimensions. For d=1 this allows to use the\npowerful tools of conformal field theory in the case of critical evolution.\nSeveral results are obtained in generic dimension in the gaussian (mean-field)\napproximation. These predictions are checked against the real-time evolution of\nsome solvable models that allows also to understand which features are valid\nbeyond the critical evolution.\n  All our findings may be explained in terms of a picture generally valid,\nwhereby quasiparticles, entangled over regions of the order of the correlation\nlength in the initial state, then propagate with a finite speed through the\nsystem. Furthermore we show that the long-time results can be interpreted in\nterms of a generalized Gibbs ensemble. We discuss some open questions and\npossible future developments.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 15:34:49 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 19 Apr 2007 13:36:26 GMT\"}]', '2011-02-16', '[[\"Calabrese\",\"Pasquale\",\"\"],[\"Cardy\",\"John\",\"\"]]'),
(704.1881, 'Brian Landry', 'Eric J. Heller and Brian R. Landry', 'Statistical Properties of Many Particle Eigenfunctions', '13 pages, 4 figures', '', '10.1088/1751-8113/40/31/006', '', 'quant-ph', '', '  Wavefunction correlations and density matrices for few or many particles are\nderived from the properties of semiclassical energy Green functions. Universal\nfeatures of fixed energy (microcanonical) random wavefunction correlation\nfunctions appear which reflect the emergence of the canonical ensemble as the\nnumber of particles approaches infinity. This arises through a little known\nasymptotic limit of Bessel functions. Constraints due to symmetries,\nboundaries, and collisions between particles can be included.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 16:43:25 GMT\"}]', '2009-11-13', '[[\"Heller\",\"Eric J.\",\"\"],[\"Landry\",\"Brian R.\",\"\"]]'),
(704.1882, 'Raissa M. D\'Souza', 'Raissa M. D\'Souza, Paul L. Krapivsky, Cristopher Moore', 'The power of choice in network growth', '9 pages, 4 figures', '', '10.1140/epjb/e2007-00310-5', '', 'cond-mat.stat-mech', '', '  The \"power of choice\" has been shown to radically alter the behavior of a\nnumber of randomized algorithms. Here we explore the effects of choice on\nmodels of tree and network growth. In our models each new node has k randomly\nchosen contacts, where k > 1 is a constant. It then attaches to whichever one\nof these contacts is most desirable in some sense, such as its distance from\nthe root or its degree. Even when the new node has just two choices, i.e., when\nk=2, the resulting network can be very different from a random graph or tree.\nFor instance, if the new node attaches to the contact which is closest to the\nroot of the tree, the distribution of depths changes from Poisson to a\ntraveling wave solution. If the new node attaches to the contact with the\nsmallest degree, the degree distribution is closer to uniform than in a random\ngraph, so that with high probability there are no nodes in the network with\ndegree greater than O(log log N). Finally, if the new node attaches to the\ncontact with the largest degree, we find that the degree distribution is a\npower law with exponent -1 up to degrees roughly equal to k, with an\nexponential cutoff beyond that; thus, in this case, we need k >> 1 to see a\npower law over a wide range of degrees.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 17:23:05 GMT\"}]', '2009-11-13', '[[\"D\'Souza\",\"Raissa M.\",\"\"],[\"Krapivsky\",\"Paul L.\",\"\"],[\"Moore\",\"Cristopher\",\"\"]]'),
(704.1883, 'Junichiro Kono', 'X. Wang, D. J. Hilton, L. Ren, D. M. Mittleman, J. Kono, J. L. Reno', 'Terahertz Time-Domain Magnetospectroscopy of a High-Mobility\n  Two-Dimensional Electron Gas', '4 pages, 3 figures', 'Optics Letters 32, 13 (2007)', '10.1364/OL.32.001845', '', 'cond-mat.mes-hall cond-mat.mtrl-sci', '', '  We have observed cyclotron resonance in a high-mobility GaAs/AlGaAs\ntwo-dimensional electron gas by using the techniques of terahertz time-domain\nspectroscopy combined with magnetic fields. From this, we calculate the real\nand imaginary parts of the diagonal elements of the magnetoconductivity tensor,\nwhich in turn allows us to extract the concentration, effective mass, and\nscattering time of the electrons in the sample. We demonstrate the utility of\nultrafast terahertz spectroscopy, which can recover the true linewidth of\ncyclotron resonance in a high-mobility ($>{10}^{6} \\mathrm{cm^{2} V^{-1}\ns^{-1}}$) sample without being affected by the saturation effect.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 18:21:01 GMT\"}]', '2009-11-13', '[[\"Wang\",\"X.\",\"\"],[\"Hilton\",\"D. J.\",\"\"],[\"Ren\",\"L.\",\"\"],[\"Mittleman\",\"D. M.\",\"\"],[\"Kono\",\"J.\",\"\"],[\"Reno\",\"J. L.\",\"\"]]'),
(704.1884, 'Saka\\\'e Fuchino', 'J\\\"org Brendle and Saka\\\'e Fuchino', 'Coloring ordinals by reals', '', '', '', '', 'math.LO', '', '  We study combinatorial principles we call Homogeneity Principle HP(\\kappa)\nand Injectivity Principle IP(\\kappa,\\lambda) for regular \\kappa>\\aleph_1 and\n\\lambda\\leq\\kappa which are formulated in terms of coloring the ordinals\n<\\kappa by reals.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 18:41:56 GMT\"}]', '2007-05-23', '[[\"Brendle\",\"Jörg\",\"\"],[\"Fuchino\",\"Sakaé\",\"\"]]'),
(704.1885, 'Jesse Bloom', 'Jesse D. Bloom, Zhongyi Lu, David Chen, Alpan Raval, Ophelia S.\n  Venturelli, and Frances H. Arnold', 'Evolution favors protein mutational robustness in sufficiently large\n  populations', '', 'BMC Biology 5:29 (2007)', '10.1186/1741-7007-5-29', '', 'q-bio.PE q-bio.BM', '', '  BACKGROUND: An important question is whether evolution favors properties such\nas mutational robustness or evolvability that do not directly benefit any\nindividual, but can influence the course of future evolution. Functionally\nsimilar proteins can differ substantially in their robustness to mutations and\ncapacity to evolve new functions, but it has remained unclear whether any of\nthese differences might be due to evolutionary selection for these properties.\n  RESULTS: Here we use laboratory experiments to demonstrate that evolution\nfavors protein mutational robustness if the evolving population is sufficiently\nlarge. We neutrally evolve cytochrome P450 proteins under identical selection\npressures and mutation rates in populations of different sizes, and show that\nproteins from the larger and thus more polymorphic population tend towards\nhigher mutational robustness. Proteins from the larger population also evolve\ngreater stability, a biophysical property that is known to enhance both\nmutational robustness and evolvability. The excess mutational robustness and\nstability is well described by existing mathematical theories, and can be\nquantitatively related to the way that the proteins occupy their neutral\nnetwork.\n  CONCLUSIONS: Our work is the first experimental demonstration of the general\ntendency of evolution to favor mutational robustness and protein stability in\nhighly polymorphic populations. We suggest that this phenomenon may contribute\nto the mutational robustness and evolvability of viruses and bacteria that\nexist in large populations.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 19:42:13 GMT\"}]', '2009-04-16', '[[\"Bloom\",\"Jesse D.\",\"\"],[\"Lu\",\"Zhongyi\",\"\"],[\"Chen\",\"David\",\"\"],[\"Raval\",\"Alpan\",\"\"],[\"Venturelli\",\"Ophelia S.\",\"\"],[\"Arnold\",\"Frances H.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1886, 'Pedro Resende', 'S\\\'ergio Marcelino and Pedro Resende', 'An algebraic generalization of Kripke structures', '39 pages', 'Math. Proc. Cambridge Philos. Soc. 145 (2008) 549-577', '10.1017/S0305004108001667', '', 'math.LO cs.LO math.RA', '', '  The Kripke semantics of classical propositional normal modal logic is made\nalgebraic via an embedding of Kripke structures into the larger class of\npointed stably supported quantales. This algebraic semantics subsumes the\ntraditional algebraic semantics based on lattices with unary operators, and it\nsuggests natural interpretations of modal logic, of possible interest in the\napplications, in structures that arise in geometry and analysis, such as\nfoliated manifolds and operator algebras, via topological groupoids and inverse\nsemigroups. We study completeness properties of the quantale based semantics\nfor the systems K, T, K4, S4, and S5, in particular obtaining an axiomatization\nfor S5 which does not use negation or the modal necessity operator. As\nadditional examples we describe intuitionistic propositional modal logic, the\nlogic of programs PDL, and the ramified temporal logic CTL.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 19:59:18 GMT\"}]', '2009-11-13', '[[\"Marcelino\",\"Sérgio\",\"\"],[\"Resende\",\"Pedro\",\"\"]]'),
(704.1887, 'Vladimir Matic Milan', 'V. M. Matic and N. Dj. Lazarov', 'Origin of the 60K plateau in YBa_2Cu_3O_6+x', '5 pages of text, 3 figures, corrected two typing errors: in paragraph\n  1 of page 2 \"p(x)=0.94 - replaced by p(x)=0.094\", in paragraph 2 of page 5\n  \"2/3 - replaced by 2/5\". Accepted for publication in Journal of Physics\n  Condensed Matter in a revised form (one page added to provide some more\n  informations on length distributions of CuO chains and some references added)', 'J. Phys.: Condens. Matter 19 (2007) 346230', '10.1088/0953-8984/19/34/346230', '', 'cond-mat.supr-con', '', '  A model for charge transfer mechanism in YBa2Cu3O6+x high-Tc cuprate based on\ncritical chain length concept is proposed to account for 60K and 90K plateaus\nin Tc(x) dependence. It has been shown, when the statistics of CuO chain\nformation was described in terms of two dimensional asymmetric next-to-nearest\nneighbor Ising (ASYNNNI) model, that at any constant temperature below the top\nof OII phase there exists a uniquely defined value of critical chain length\nlcr(T) that yields a constant doping p(x)=const over the regime of OII phase\n(related to 60K plateau of Tc(x)), while 90K plateau coincides with the\nmonotonously increasing p(x) over optimal doping level p=0.16 in the regime of\nOI phase. Short length chains (l<lcr(T)), together with the first lcr(T)-2\nholes in longer chains (l>lcr(T)), are taken as not capable of attracting\nelectrons from CuO2 planes.. It is shown that only a part (41%) of the\nremaining l-lcr(T)+1 holes in the long chains can capture electrons. The\nresults obtained indicate that the ASYNNNI model and two-plateaus-like behavior\nof Tc(x) in YBa2Cu3O6+x are closely connected.\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 20:17:27 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 20 Apr 2007 09:22:12 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 27 Apr 2007 11:11:56 GMT\"},{\"version\":\"v4\",\"created\":\"Thu, 5 Jul 2007 23:34:56 GMT\"}]', '2007-08-15', '[[\"Matic\",\"V. M.\",\"\"],[\"Lazarov\",\"N. Dj.\",\"\"]]'),
(704.1888, 'Martin Lorenz', 'Phung Ho Hai, Benoit Kriegk and Martin Lorenz', 'N-homogeneous superalgebras', '42 pages, LaTeX; typos corrected, several references added,\n  introduction slightly expanded', '', '', '', 'math.QA math.CO', '', '  We develop the theory of N-homogeneous algebras in a super setting, with\nparticular emphasis on the Koszul property. To any Hecke operator on a vector\nsuperspace, we associate certain superalgebras and generalizing the ordinary\nsymmetric and Grassmann algebra, respectively. We prove that these algebras are\nN-Koszul. For the special case where the Hecke operator is the ordinary\nsupersymmetry, we derive an $N$-generalized super-version of MacMahon\'s\nclassical \"master theorem\".\n', '[{\"version\":\"v1\",\"created\":\"Sat, 14 Apr 2007 22:58:58 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 4 Jun 2007 21:16:31 GMT\"}]', '2007-06-13', '[[\"Hai\",\"Phung Ho\",\"\"],[\"Kriegk\",\"Benoit\",\"\"],[\"Lorenz\",\"Martin\",\"\"]]'),
(704.1889, 'Qijin Chen', 'Yan He, Qijin Chen, Chih-Chun Chien, and K. Levin', 'First and second sound modes at finite temperature in trapped Fermi\n  gases from BCS to BEC', '4 pages, 3 figures, replaced with revised version', 'Phys. Rev. A 76, 051602(R) (2007)', '10.1103/PhysRevA.76.051602', '', 'cond-mat.str-el cond-mat.quant-gas cond-mat.supr-con', '', '  We determine the temperature $T$ dependence of first and second sound mode\nfrequencies for trapped Fermi gases undergoing BCS to Bose Einstein\ncondensation (BEC) crossover. Our results are based on the two fluid equations\nin conjunction with a microscopic calculation of thermodynamical variables. As\nin experiment and at unitarity, we show that the lowest radial breathing mode\nis $T$ independent. At finite $T$, higher order breathing modes strongly mix\nwith second sound. Their complex $T$ dependence should provide an alternative\nway of measuring the transition temperature, $T_c$.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 00:02:39 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 16 Jul 2007 07:25:49 GMT\"}]', '2011-09-13', '[[\"He\",\"Yan\",\"\"],[\"Chen\",\"Qijin\",\"\"],[\"Chien\",\"Chih-Chun\",\"\"],[\"Levin\",\"K.\",\"\"]]'),
(704.1890, 'Alejandro Rodriguez', 'Alejandro Rodriguez, Mihai Ibanescu, Davide Iannuzzi, Federico\n  Capasso, John D. Joannopoulos, and Steven G. Johnson', 'Computation and visualization of Casimir forces in arbitrary geometries:\n  non-monotonic lateral forces and failure of proximity-force approximations', 'Accepted for publication in Physical Review Letters. (Expected\n  publication: Vol. 99 (8) 2007)', 'Physical Review Letters, Vol. 99, No. 8, 80401 (2007)', '10.1103/PhysRevLett.99.080401', '', 'physics.comp-ph physics.optics quant-ph', '', '  We present a method of computing Casimir forces for arbitrary geometries,\nwith any desired accuracy, that can directly exploit the efficiency of standard\nnumerical-electromagnetism techniques. Using the simplest possible\nfinite-difference implementation of this approach, we obtain both agreement\nwith past results for cylinder-plate geometries, and also present results for\nnew geometries. In particular, we examine a piston-like problem involving two\ndielectric and metallic squares sliding between two metallic walls, in two and\nthree dimensions, respectively, and demonstrate non-additive and non-monotonic\nchanges in the force due to these lateral walls.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 00:49:15 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 18 Apr 2007 02:19:28 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 8 Aug 2007 03:35:09 GMT\"},{\"version\":\"v4\",\"created\":\"Thu, 9 Aug 2007 05:43:32 GMT\"}]', '2011-01-25', '[[\"Rodriguez\",\"Alejandro\",\"\"],[\"Ibanescu\",\"Mihai\",\"\"],[\"Iannuzzi\",\"Davide\",\"\"],[\"Capasso\",\"Federico\",\"\"],[\"Joannopoulos\",\"John D.\",\"\"],[\"Johnson\",\"Steven G.\",\"\"]]'),
(704.1891, 'P. Christopher Staecker', 'P. Christopher Staecker', 'Axioms for a local Reidemeister trace in fixed point and coincidence\n  theory on differentiable manifolds', 'minor changes, synchronized with publication version', 'Journal of Fixed Point Theory and Applications 5, 2009, p. 237-247', '10.1007/s11784-008-0055-8', '', 'math.GT math.GN', '', '  We give axioms which characterize the local Reidemeister trace for orientable\ndifferentiable manifolds. The local Reidemeister trace in fixed point theory is\nalready known, and we provide both uniqueness and existence results for the\nlocal Reidemeister trace in coincidence theory.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 01:04:09 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 9 May 2008 18:59:26 GMT\"}]', '2010-06-03', '[[\"Staecker\",\"P. Christopher\",\"\"]]'),
(704.1892, 'Donald Barnes', 'Donald W. Barnes', 'On (n+2)-dimensional n-Lie algebras', '2 pages', '', '', '', 'math.RA', '', '  I show that an (n+2)-dimensional n-Lie algebra over an algebraically closed\nfield must have a subalgeba of codimension 1.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 01:41:47 GMT\"}]', '2007-05-23', '[[\"Barnes\",\"Donald W.\",\"\"]]'),
(704.1893, 'Elnikova Liliya V', 'L. V. Elnikova', 'Elastic properties of vanadium pentoxide aggregates and topological\n  defects', 'original title was \"The junction of tactoids in lyotropic inorganic\n  liquid crystals\" final form', '', '', '', 'cond-mat.soft', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We study the aqueous solution of vanadium pentoxide by using topology\nmethods. The experiments by Zocher, Kaznacheev, and Dogic exhibited, that in\nthe sol phases of $V_2O_5-H_2O$, the tactoid droplets of $V_2O_5$ can coalesce.\nIn the magnetic field, this effect is associated with a gauge field action,\nviz. we consider coalescence (in the topologically more convenient term,\n\"junction\") of droplets as annihilation of topological defects, concerning with\nthe tactoid geometry. We have shown, that in the magnetic field, the tactoid\njunction is mainly caused by non-Abelian monopoles (vortons), whereas the\nAbelian defects almost do not annihilate. Taking into account this annihilation\nmechanism, the estimations of time-aging of the $V_2O_5-H_2O$ sols may be\nspecified\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 05:20:32 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 1 May 2007 13:51:59 GMT\"},{\"version\":\"v3\",\"created\":\"Sat, 14 Jul 2007 18:22:58 GMT\"},{\"version\":\"v4\",\"created\":\"Fri, 6 Jun 2008 15:09:19 GMT\"},{\"version\":\"v5\",\"created\":\"Wed, 13 Aug 2008 21:07:18 GMT\"},{\"version\":\"v6\",\"created\":\"Sat, 20 Sep 2008 14:57:16 GMT\"},{\"version\":\"v7\",\"created\":\"Fri, 7 Nov 2008 21:01:02 GMT\"}]', '2008-11-07', '[[\"Elnikova\",\"L. V.\",\"\"]]'),
(704.1894, 'Mushfiq Ahmad Mr.', 'Mushfiq Ahmad and M. Shah Alam', 'Non-Associativity of Lorentz Transformation and Associative Reflection\n  Symmetric Transformation', '4 pages, 1 figure', '', '', '', 'math-ph math.MP', '', '  Each of the two moving observers observes the relative velocity of the other.\nThe two velocities should be equal and opposite. We have shown that this\nrelativistic requirement is not fulfilled by Lorentz transformation. We have\nalso shown that the reason is that Lorentz transformation is not associative.\nReciprocal symmetric transformation is associative and fulfills relativistic\nrequirements.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 05:48:05 GMT\"}]', '2007-05-23', '[[\"Ahmad\",\"Mushfiq\",\"\"],[\"Alam\",\"M. Shah\",\"\"]]'),
(704.1895, 'Supurna Sinha', 'Supurna Sinha', 'Jamming dynamics in grain mixtures : An extended hydrodynamic approach', 'To appear in ``Fluctuation and Noise Letters\'\'', 'Fluctuation and Noise Letters, Vol. 7, No. 2 (2007), L163-L167', '', '', 'cond-mat.soft', '', '  We study jamming in granular mixtures from the novel point of view of\nextended hydrodynamics. Using a hard sphere binary mixture model we predict\nthat a few large grains are expected to get caged more effectively in a matrix\nof small grains compared to a few small grains in a matrix of larger ones. A\nsimilar effect has been experimentally seen in the context of colloidal\nmixtures.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 07:06:12 GMT\"}]', '2011-11-09', '[[\"Sinha\",\"Supurna\",\"\"]]'),
(704.1896, 'Berthold-Georg Englert', 'Christian Miniatura, Cord A. M\\\"uller, Yin Lu, Guangquan Wang,\n  Berthold-Georg Englert', 'Path Distinguishability in Double Scattering of Light by Atoms', '4 pages, 1 figure; version 2: address correction', 'Physical Review A 76 (2007) 022101 (4 pages)', '10.1103/PhysRevA.76.022101', '', 'quant-ph', '', '  Wave-particle duality finds a natural application for electrons or light\npropagating in disordered media where coherent corrections to transport are\ngiven by two-wave interference. For scatterers with internal degrees of\nfreedom, these corrections are observed to be much smaller than would be\nexpected for structureless scatterers. By examining the basic example of the\nscattering of one photon by two spin-1/2 atoms--a case-study for coherent\nbackscattering--we demonstrate that the loss of interference strength is\nassociated with which-path information stored by the scattering atoms.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 07:26:51 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Apr 2007 23:43:32 GMT\"}]', '2011-03-15', '[[\"Miniatura\",\"Christian\",\"\"],[\"Müller\",\"Cord A.\",\"\"],[\"Lu\",\"Yin\",\"\"],[\"Wang\",\"Guangquan\",\"\"],[\"Englert\",\"Berthold-Georg\",\"\"]]'),
(704.1897, 'Sergei Zhukovsky', 'S. V. Zhukovsky, S. V. Gaponenko', 'Constraints on transmission, dispersion, and density of states in\n  dielectric multilayers and stepwise potential barriers with arbitrary layer\n  arrangement', '10 pages, 5 figures, to be submitted to PRE', 'Phys. Rev. E 77, 046602 (2008)', '10.1103/PhysRevE.77.046602', '', 'cond-mat.mes-hall physics.optics', '', '  Normal-incidence transmission and dispersion properties of optical\nmultilayers and one-dimensional stepwise potential barriers in the\nnon-tunneling regime are analytically investigated. The optical paths of every\nconstituent layer in a multilayer structure, as well as the parameters of every\nstep of the stepwise potential barrier, are constrained by a generalized\nquarter-wave condition. No other restrictions on the structure geometry is\nimposed, i.e., the layers are arranged arbitrarily. We show that the density of\nstates (DOS) spectra of the multilayer or barrier in question are subject to\nintegral conservation rules similar to the Barnett-Loudon sum rule but ocurring\nwithin a finite frequency or energy interval. In the optical case, these\nfrequency intervals are regular. For the potential barriers, only non-periodic\nenergy intervals can be present in the spectrum of any given structure, and\nonly if the parameters of constituent potential steps are properly chosen.\n  Abstract The integral conservation relations derived analytically have also\nbeen verified numerically. The relations can be used in dispersion-engineered\nmultilayer-based devices, e.g., ultrashort pulse compressors or ultracompact\noptical delay lines, as well as to design multiple-quantum-well electronic\nheterostructures with engineered DOS.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 17:16:07 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 14 Mar 2008 15:10:07 GMT\"}]', '2008-04-13', '[[\"Zhukovsky\",\"S. V.\",\"\"],[\"Gaponenko\",\"S. V.\",\"\"]]'),
(704.1898, 'Saharian', 'A.A. Saharian', 'Electromagnetic Casimir densities for a wedge with a coaxial cylindrical\n  shell', '21 pages, 7 figures', 'Eur.Phys.J.C52:721-733,2007', '10.1140/epjc/s10052-007-0409-1', '', 'hep-th quant-ph', '', '  Vacuum expectation values of the field square and the energy-momentum tensor\nfor the electromagnetic field are investigated for the geometry of a wedge with\na coaxal cylindrical boundary. All boundaries are assumed to be perfectly\nconducting and both regions inside and outside the shell are considered. By\nusing the generalized Abel-Plana formula, the vacuum expectation values are\npresented in the form of the sum of two terms. The first one corresponds to the\ngeometry of the wedge without the cylindrical shell and the second term is\ninduced by the presence of the shell. The vacuum energy density induced by the\nshell is negative for the interior region and is positive for the exterior\nregion. The asymptotic behavior of the vacuum expectation values are\ninvestigated in various limiting cases. It is shown that the vacuum forces\nacting on the wedge sides due to the presence of the cylindrical boundary are\nalways attractive.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 10:53:31 GMT\"}]', '2008-11-26', '[[\"Saharian\",\"A. A.\",\"\"]]'),
(704.1899, 'Andrew Levan', 'Melvyn B. Davies, Andrew J. Levan, Josefin Larsson, Andrew R. King,\n  Andrew S. Fruchter', 'Progenitors of Long Gamma-ray Bursts', 'To appear in \"Gamma-ray bursts: Prospects for GLAST\", AIP Conference\n  proceedings 906, Editors M. Axelsson and F Ryde', 'AIP Conf.Proc.906:69-78,2007', '10.1063/1.2737408', '', 'astro-ph', '', '  Pinpointing the progenitors of long duration gamma-ray bursts (LGRBs) remains\nan extremely important question, although it is now clear that at least a\nfraction of LGRBs originate in the core collapse of massive stars in type Ic\nsupernovae, the pathways to the production of these stars, and their initial\nmasses, remain uncertain. Rotation is thought to be vital in the creation of\nLGRBs, and it is likely that black hole creation is also necessary. We suggest\nthat these two constraints can be met if the GRB progenitors are very massive\nstars (>20 solar masses) and are formed in tight binary systems. Using simple\nmodels we compare the predictions of this scenario with observations and find\nthat the location of GRBs on their host galaxies are suggestive of\nmain-sequence masses in excess of 20 solar masses, while 50% of the known\ncompact binary systems may have been sufficiently close to have had the\nnecessary rotation rates for GRB creation. Thus, massive stars in compact\nbinaries are a likely channel for at least some fraction of LGRBs.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 11:54:27 GMT\"}]', '2009-06-23', '[[\"Davies\",\"Melvyn B.\",\"\"],[\"Levan\",\"Andrew J.\",\"\"],[\"Larsson\",\"Josefin\",\"\"],[\"King\",\"Andrew R.\",\"\"],[\"Fruchter\",\"Andrew S.\",\"\"]]'),
(704.1900, 'Luca Vecchi', 'Luca Vecchi', 'Causal vs. Analytic constraints on anomalous quartic gauge couplings', '4 pages, non forward scattering included, references added', 'JHEP 0711:054,2007', '10.1088/1126-6708/2007/11/054', '', 'hep-ph', '', '  We derive one loop constraints on the anomalous quartic gauge couplings using\na general non-forward dispersion relation for the elastic scattering amplitude\nof two longitudinally polarized vector bosons. We compare this result with\nanother one derived by the assumption that the underlying theory satisfies the\ncausality principle of Special Relativity and show that this latter is more\nconstraining.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 14:23:13 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 29 Jun 2007 11:43:47 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 15 Nov 2007 14:52:46 GMT\"}]', '2009-04-21', '[[\"Vecchi\",\"Luca\",\"\"]]'),
(704.1901, 'Saikat Guha', 'Saikat Guha, Jeffrey H. Shapiro', 'Classical Information Capacity of the Bosonic Broadcast Channel', '5 pages, 4 figures, to appear in Proceedings of ISIT 2007', '', '', '', 'quant-ph', '', '  We show that when coherent-state encoding is employed in conjunction with\ncoherent detection, the Bosonic broadcast channel is equivalent to a classical\ndegraded Gaussian broadcast channel whose capacity region is dual to that of\nthe classical Gaussian multiple-access channel. We further show that if a\nminimum output-entropy conjecture holds true, then the ultimate classical\ninformation capacity of the Bosonic broadcast channel can be achieved by a\ncoherent-state encoding. We provide some evidence in support of the conjecture.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 13:17:32 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Apr 2007 23:17:04 GMT\"}]', '2007-05-23', '[[\"Guha\",\"Saikat\",\"\"],[\"Shapiro\",\"Jeffrey H.\",\"\"]]'),
(704.1902, 'Haim Beidenkopf', 'H. Beidenkopf, T. Verdene, Y. Myasoedov, H. Shtrikman, E. Zeldov, B.\n  Rosenstein, D. Li, T. Tamegai', 'Interplay of Anisotropy and Disorder in the Doping-Dependent Melting and\n  Glass Transitions of Vortices in Bi$_2$Sr$_2$CaCu$_2$O$_{8+\\delta}$', '4 pages, 4 figures', '', '10.1103/PhysRevLett.98.167004', '', 'cond-mat.supr-con cond-mat.stat-mech', '', '  We study the oxygen doping dependence of the equilibrium first-order melting\nand second-order glass transitions of vortices in\nBi$_2$Sr$_2$CaCu$_2$O$_{8+\\delta}$. Doping affects both anisotropy and\ndisorder. Anisotropy scaling is shown to collapse the melting lines only where\nthermal fluctuations are dominant. Yet, in the region where disorder breaks\nthat scaling, the glass lines are still collapsed. A quantitative fit to\nmelting and replica symmetry breaking lines of a 2D Ginzburg-Landau model\nfurther reveals that disorder amplitude weakens with doping, but to a lesser\ndegree than thermal fluctuations, enhancing the relative role of disorder.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 13:23:27 GMT\"}]', '2015-05-13', '[[\"Beidenkopf\",\"H.\",\"\"],[\"Verdene\",\"T.\",\"\"],[\"Myasoedov\",\"Y.\",\"\"],[\"Shtrikman\",\"H.\",\"\"],[\"Zeldov\",\"E.\",\"\"],[\"Rosenstein\",\"B.\",\"\"],[\"Li\",\"D.\",\"\"],[\"Tamegai\",\"T.\",\"\"]]'),
(704.1903, 'Shigeo Maruyama', 'Kei Hasegawa, Suguru Noda, Hisashi Sugime, Kazunori Kakehi, Shigeo\n  Maruyama, Yukio Yamaguchi', 'Growth window and possible mechanism of millimeter-thick single-walled\n  carbon nanotube forests', '6 pages, 6 figures. Submitted to J. Nanosci. Nanotech', '', '', '', 'cond-mat.mtrl-sci', '', '  Our group recently reproduced the water-assisted growth method, so-called\n\"super growth\", of millimeter-thick single-walled carbon nanotube (SWNT)\nforests by using C2H4/ H2/ H2O/ Ar reactant gas and Fe/ Al2O3 catalyst. In this\ncurrent work, a parametric study was carried out on both reaction and catalyst\nconditions. Results revealed that a thin Fe catalyst layer (about 0.5 nm)\nyielded rapid growth of SWNTs only when supported on Al2O3, and that Al2O3\nsupport enhanced the activity of Fe, Co, and Ni catalysts. The growth window\nfor the rapid SWNT growth was narrow, however. Optimum amount of added H2O\nincreased the SWNT growth rate but further addition of H2O degraded both the\nSWNT growth rate and quality. Addition of H2 was also essential for rapid SWNT\ngrowth, but again, further addition decreased both the SWNT growth rate and\nquality. Because Al2O3 catalyzes hydrocarbon reforming, Al2O3 support possibly\nenhances the SWNT growth rate by supplying the carbon source to the catalyst\nnanoparticles. The origin of the narrow window for rapid SWNT growth will also\nbe discussed.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 14:27:59 GMT\"}]', '2007-05-23', '[[\"Hasegawa\",\"Kei\",\"\"],[\"Noda\",\"Suguru\",\"\"],[\"Sugime\",\"Hisashi\",\"\"],[\"Kakehi\",\"Kazunori\",\"\"],[\"Maruyama\",\"Shigeo\",\"\"],[\"Yamaguchi\",\"Yukio\",\"\"]]'),
(704.1904, 'Alexander Bershadskii', 'A. Bershadskii', 'Nonlocal interactions versus viscosity in turbulence', '', 'Phys.Fluids.20:085103,2008', '10.1063/1.2969473', '', 'nlin.CD astro-ph cond-mat.stat-mech', '', '  It is shown that nonlocal interactions determine energy spectrum in isotropic\nturbulence at small Reynolds numbers. It is also shown that for moderate\nReynolds numbers the bottleneck effect is determined by the same nonlocal\ninteractions. Role of the large and small scales covariance at the nonlocal\ninteractions and in energy balance has been investigated. A possible\nhydrodynamic mechanism of the nonlocal solution instability at large scales has\nbeen briefly discussed. A quantitative relationship between effective strain of\nthe nonlocal interactions and viscosity has been found. All results are\nsupported by comparison with the data of experiments and numerical simulations.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 15:27:50 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 22 Apr 2007 18:23:08 GMT\"},{\"version\":\"v3\",\"created\":\"Sun, 6 May 2007 14:51:20 GMT\"},{\"version\":\"v4\",\"created\":\"Sun, 20 May 2007 16:20:49 GMT\"}]', '2008-11-07', '[[\"Bershadskii\",\"A.\",\"\"]]'),
(704.1905, 'Tomislav Prokopec', 'Ante Bilandzic (Nikhef) and Tomislav Prokopec (Utrecht University)', 'Quantum radiative corrections to slow-roll inflation', '31 pages, 2 eps figures, references added and an improved\n  introduction', 'Phys.Rev.D76:103507,2007', '10.1103/PhysRevD.76.103507', 'NIKHEF-2007-09, SPIN-07-11, ITP-UU-07-18', 'astro-ph', '', '  We consider the nonminimally coupled lambda phi^4 scalar field theory in de\nSitter space and construct the renormalization group improved renormalized\neffective theory at the one-loop level. Based on the corresponding quantum\nFriedmann equation and the scalar field equation of motion, we calculate the\nquantum radiative corrections to the scalar spectral index n_s, gravitational\nwave spectral index n_g and the ratio r of tensor to scalar perturbations. When\ncompared with the standard (tree-level) values, we find that the quantum\ncontributions are suppressed by lambda N^2 where N denotes the number of\ne-foldings. Hence there is an N^2 enhancement with respect to the naive\nexpectation, which is due to the infrared enhancement of scalar vacuum\nfluctuations characterising de Sitter space. Since observations constrain\nlambda to be very small lambda ~ 10^(-12) and N ~ 50-60, the quantum\ncorrections in this inflationary model are unobservably small.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 16:12:16 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 17 May 2007 17:44:13 GMT\"}]', '2008-11-26', '[[\"Bilandzic\",\"Ante\",\"\",\"Nikhef\"],[\"Prokopec\",\"Tomislav\",\"\",\"Utrecht University\"]]'),
(704.1906, 'Liviu Hozoi', 'L. Hozoi, U. Birkenheuer, P. Fulde, A. Mitrushchenkov, and H. Stoll', 'Ab initio wavefunction based methods for excited states in solids:\n  correlation corrections to the band structure of ionic oxides', '', 'Phys. Rev. B 76, 085109 (2007)', '10.1103/PhysRevB.76.085109', '', 'cond-mat.mtrl-sci cond-mat.other', '', '  Ab initio wavefunction based methods are applied to the study of electron\ncorrelation effects on the band structure of oxide systems. We choose MgO as a\nprototype closed-shell ionic oxide. Our analysis is based on a local\nHamiltonian approach and performed on finite fragments cut from the infinite\nsolid. Localized Wannier functions and embedding potentials are obtained from\nprior periodic Hartree-Fock (HF) calculations. We investigate the role of\nvarious electron correlation effects in reducing the HF band gap and modifying\nthe band widths. On-site and nearest-neighbor charge relaxation as well as\nlong-range polarization effects are calculated. Whereas correlation effects are\nessential for computing accurate band gaps, we found that they produce smaller\nchanges on the HF band widths, at least for this material. Surprisingly, a\nbroadening effect is obtained for the O 2p valence bands. The ab initio data\nare in good agreement with the energy gap and band width derived from\nthermoreflectance and x-ray photoemission experiments. The results show that\nthe wavefunction based approach applied here allows for well controlled\napproximations and a transparent identification of the microscopic processes\nwhich determine the electronic band structure.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 16:32:37 GMT\"}]', '2007-08-13', '[[\"Hozoi\",\"L.\",\"\"],[\"Birkenheuer\",\"U.\",\"\"],[\"Fulde\",\"P.\",\"\"],[\"Mitrushchenkov\",\"A.\",\"\"],[\"Stoll\",\"H.\",\"\"]]'),
(704.1907, 'Peter Robert Wood', 'J. A. McSaveney, P. R. Wood, M. Scholz, J. C. Lattanzio and K. H.\n  Hinkle', 'Abundances in intermediate-mass AGB stars undergoing third dredge-up and\n  hot-bottom burning', 'Accepted for publication in MNRAS', '', '10.1111/j.1365-2966.2007.11845.x', '', 'astro-ph', '', '  High dispersion near-infrared spectra have been taken of seven\nhighly-evolved, variable, intermediate-mass (4-6 Msun) AGB stars in the LMC and\nSMC in order to look for C, N and O variations that are expected to arise from\nthird dredge-up and hot-bottom burning. The pulsation of the objects has been\nmodelled, yielding stellar masses, and spectral synthesis calculations have\nbeen performed in order to derive abundances from the observed spectra. For two\nstars, abundances of C, N, O, Na, Al, Ti, Sc and Fe were derived and compared\nwith the abundances predicted by detailed AGB models. Both stars show very\nlarge N enhancements and C deficiencies. These results provide the first\nobservational confirmation of the long-predicted production of primary nitrogen\nby the combination of third dredge-up and hot-bottom burning in\nintermediate-mass AGB stars. It was not possible to derive abundances for the\nremaining five stars: three were too cool to model, while another two had\nstrong shocks in their atmospheres which caused strong emission to fill the\nline cores and made abundance determination impossible. The latter occurrence\nallows us to predict the pulsation phase interval during which observations\nshould be made if successful abundance analysis is to be possible.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 17:18:01 GMT\"}]', '2009-11-13', '[[\"McSaveney\",\"J. A.\",\"\"],[\"Wood\",\"P. R.\",\"\"],[\"Scholz\",\"M.\",\"\"],[\"Lattanzio\",\"J. C.\",\"\"],[\"Hinkle\",\"K. H.\",\"\"]]'),
(704.1908, 'Radek Erban', 'Radek Erban, Jonathan Chapman and Philip Maini', 'A practical guide to stochastic simulations of reaction-diffusion\n  processes', '35 pages', '', '', '', 'q-bio.SC physics.ed-ph q-bio.QM', '', '  A practical introduction to stochastic modelling of reaction-diffusion\nprocesses is presented. No prior knowledge of stochastic simulations is\nassumed. The methods are explained using illustrative examples. The article\nstarts with the classical Gillespie algorithm for the stochastic modelling of\nchemical reactions. Then stochastic algorithms for modelling molecular\ndiffusion are given. Finally, basic stochastic reaction-diffusion methods are\npresented. The connections between stochastic simulations and deterministic\nmodels are explained and basic mathematical tools (e.g. chemical master\nequation) are presented. The article concludes with an overview of more\nadvanced methods and problems.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 17:50:38 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 19 Nov 2007 03:47:24 GMT\"}]', '2007-11-19', '[[\"Erban\",\"Radek\",\"\"],[\"Chapman\",\"Jonathan\",\"\"],[\"Maini\",\"Philip\",\"\"]]'),
(704.1909, 'Sergey Mikhailov', 'S. A. Mikhailov', 'Non-linear electromagnetic response of graphene', '5 pages, 3 figures', 'Europhys. Lett. 79, 27002 (2007)', '10.1209/0295-5075/79/27002', '', 'cond-mat.mes-hall', '', '  It is shown that the massless energy spectrum of electrons and holes in\ngraphene leads to the strongly non-linear electromagnetic response of this\nsystem. We predict that the graphene layer, irradiated by electromagnetic\nwaves, emits radiation at higher frequency harmonics and can work as a\nfrequency multiplier. The operating frequency of the graphene frequency\nmultiplier can lie in a broad range from microwaves to the infrared.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 17:56:19 GMT\"}]', '2007-07-24', '[[\"Mikhailov\",\"S. A.\",\"\"]]'),
(704.1910, 'Eric Pfahl', 'Eric Pfahl (KITP), Phil Arras (UVa), Bill Paxton (KITP)', 'Ellipsoidal Oscillations Induced by Substellar Companions: A Prospect\n  for the Kepler Mission', '13 pages (emulateapj), 9 figures, 3 tables, submitted to ApJ', 'Astrophys.J.679:783-796,2008', '10.1086/586878', '', 'astro-ph', '', '  Hundreds of substellar companions to solar-type stars will be discovered with\nthe Kepler satellite. Kepler\'s extreme photometric precision gives access to\nlow-amplitude stellar variability contributed by a variety of physical\nprocesses. We discuss in detail the periodic flux modulations arising from the\ntidal force on the star due to a substellar companion. An analytic expression\nfor the variability is derived in the equilibrium-tide approximation. We\ndemonstrate analytically and through numerical solutions of the linear,\nnonadiabatic stellar oscillation equations that the equilibrium-tide formula\nworks extremely well for stars of mass <1.4 Msun with thick surface convection\nzones. More massive stars with largely radiative envelopes do not conform to\nthe equilibrium-tide approximation and can exhibit flux variations $\\ga$10\ntimes larger than naive estimates. Over the full range of stellar masses\nconsidered, we treat the oscillatory response of the convection zone by\nadapting a prescription that A. J. Brickhill developed for pulsating white\ndwarfs. Compared to other sources of periodic variability, the ellipsoidal\nlightcurve has a distinct dependence on time and system parameters. We suggest\nthat ellipsoidal oscillations induced by giant planets may be detectable from\nas many as ~100 of the 10^5 Kepler target stars. (Abridged)\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 18:00:07 GMT\"}]', '2011-02-07', '[[\"Pfahl\",\"Eric\",\"\",\"KITP\"],[\"Arras\",\"Phil\",\"\",\"UVa\"],[\"Paxton\",\"Bill\",\"\",\"KITP\"]]'),
(704.1911, 'Igor Kulic', 'Herve Mohrbach and Igor M. Kulic', 'Motor driven microtubule shape fluctuations - force from within the\n  lattice', '', '', '10.1103/PhysRevLett.99.218102', '', 'cond-mat.soft', '', '  We develop a general theory of microtubule (MT) deformations by molecular\nmotors generating internal force doublets within the MT lattice. We describe\ntwo basic internal excitations, the S and V shape, and compare them with\nexperimental observations from literature. We explain the special role of\ntubulin vacancies and the dramatic deformation amplifying effect observed for\nkatanin acting at positions of defects. Experimentally observed shapes are used\nto determine the ratio of MT shear and stretch moduli ($\\approx\n6\\times10^{-5}$) and to estimate the forces induced in the MT lattice by\nkatanin (10\'s of pN). For many motors acting on a single MT we derive\nexpressions for the end-to-end distance reduction and provide criteria for\ndominance of this new effect over thermal fluctuations. We conclude that\nmolecular motors if acting cooperatively can \'\'animate\'\' MTs from within the\nlattice and induce slack even without cross-bridging to other structures, a\nscenario very much reminiscent of the motor driven axoneme.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:04:09 GMT\"}]', '2009-11-13', '[[\"Mohrbach\",\"Herve\",\"\"],[\"Kulic\",\"Igor M.\",\"\"]]'),
(704.1912, 'Adrian Melott', 'L.C. Natarajan, A.L. Melott, B.M. Rothschild, and L.D. Martin\n  (University of Kansas)', 'Bone Cancer Rates in Dinosaurs Compared with Modern Vertebrates', 'As published in Transactions of the Kansas Academy of Science', 'TKAS 110, 155-158 (2007)', '', '', 'q-bio.PE astro-ph physics.geo-ph', '', '  Data on the prevalence of bone cancer in dinosaurs is available from past\nradiological examination of preserved bones. We statistically test this data\nfor consistency with rates extrapolated from information on bone cancer in\nmodern vertebrates, and find that there is no evidence of a different rate.\nThus, this test provides no support for a possible role of ionizing radiation\nin the K-T extinction event.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:08:16 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 10 Sep 2007 16:28:09 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 11 Sep 2007 14:19:34 GMT\"},{\"version\":\"v4\",\"created\":\"Tue, 16 Oct 2007 18:17:26 GMT\"}]', '2007-10-16', '[[\"Natarajan\",\"L. C.\",\"\",\"University of Kansas\"],[\"Melott\",\"A. L.\",\"\",\"University of Kansas\"],[\"Rothschild\",\"B. M.\",\"\",\"University of Kansas\"],[\"Martin\",\"L. D.\",\"\",\"University of Kansas\"]]'),
(704.1913, 'Pran Nath', 'Tarek Ibrahim', 'Effective Lagrangian for the $\\chi^{+}_j \\chi^{-}_kH^{0}_l$ interaction\n  in the minimal supersymmetric standard model and neutral Higgs decays', '36 pages, 14 figues, revised version was published in Phys. Rev. D', 'Phys.Rev.D76:075012,2007', '10.1103/PhysRevD.76.075012', '', 'hep-ph', '', '  We extend previous analyses of the supersymmetric loop correction to the\nneutral Higgs couplings to include the coupling $\\chi^{+}_j \\chi^{-}_kH^{0}_l$.\nThe analysis completes the previous analyses where similar corrections were\ncomputed for the $\\bar{\\tau} \\tau H^{0}_l$, $\\bar{b} b H^{0}_l$, $\\bar{c} c\nH^{0}_l$ and for $\\bar{t} t H^{0}_l$ couplings within the minimal\nsupersymmetric standard model. The effective one loop Lagrangian is then\napplied to the computation of the neutral Higgs decays. The sizes of the\nsupersymmetric loop corrections of the neutral Higgs decay widths into\n$\\chi^{+}_i \\chi^{-}_j$ ($i=1,2$; $j=1,2$) are investigated and the\nsupersymmetric loop correction is found to be in the range of $7\\sim15%$ in\nsignificant regions of the parameter space. By including the loop corrections\nof the other decay channels $\\bar{b} b$, $\\bar{t} t$, $\\bar{\\tau} \\tau$,\n$\\bar{c} c$, and $\\chi^0_i \\chi^0_j$ ($i=1-4$; $j=1-4$), the corrections to\nbranching ratios for $H^{0}_l\\to \\chi^{+}_i \\chi^{-}_j$ can reach as high as\n40%.\n  The effects of CP phases on the branching ratio are also investigated.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:11:53 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 5 Jul 2007 20:02:35 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 31 Oct 2007 22:22:58 GMT\"}]', '2008-11-26', '[[\"Ibrahim\",\"Tarek\",\"\"]]'),
(704.1914, 'Abdelouahab Arouche', 'Abdelouahab Arouche (LATN)', 'Finite Representations of the braid group commutator subgroup', '', '', '', '', 'math.DS', '', '  We study the representations of the commutator subgroup K_{n} of the braid\ngroup B_{n} into a finite group . This is done through a symbolic dynamical\nsystem. Some experimental results enable us to compute the number of subgroups\nof K_{n} of a given (finite) index, and, as a by-product, to recover the well\nknown fact that every representation of K_{n} into S_{r}, with n > r, must be\ntrivial.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:17:21 GMT\"}]', '2007-05-23', '[[\"Arouche\",\"Abdelouahab\",\"\",\"LATN\"]]'),
(704.1915, 'Marco Delbo', 'Marco Delbo (INAF-Osservatorio Astronomico Di Torino, Oca), Aldo\n  Dell\'oro (INAF-Osservatorio Astronomico Di Torino), Alan W. Harris (DLR\n  Institute of Planetary Research), Stefano Mottola (DLR Institute of Planetary\n  Research), Michael Mueller (DLR Institute of Planetary Research)', 'Thermal inertia of near-Earth asteroids and implications for the\n  magnitude of the Yarkovsky effect', 'Icarus (30/03/2007) in press', '', '10.1016/j.icarus.2007.03.007', '', 'astro-ph', '', '  Thermal inertia determines the temperature distribution over the surface of\nan asteroid and therefore governs the magnitude the Yarkovsky effect. The\nlatter causes gradual drifting of the orbits of km-sized asteroids and plays an\nimportant role in the delivery of near-Earth asteroids (NEAs) from the main\nbelt and in the dynamical spreading of asteroid families. At present, very\nlittle is known about the thermal inertia of asteroids in the km size range.\nHere we show that the average thermal inertia of a sample of NEAs in the\nkm-size range is 200 $\\pm$ 40 J m&#8722;2 s&#8722;0.5 K&#8722;1. Furthermore,\nwe identify a trend of increasing thermal inertia with decreasing asteroid\ndiameter, D. This indicates that the dependence of the drift rate of the\norbital semimajor axis on the size of asteroids due to the Yarkovsky effect is\na more complex function than the generally adopted D^(&#8722;1) dependence, and\nthat the size distribution of objects injected by Yarkovsky-driven orbital\nmobility into the NEA source regions is less skewed to smaller sizes than\ngenerally assumed. We discuss how this fact may help to explain the small\ndifference in the slope of the size distribution of km-sized NEAs and main-belt\nasteroids.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:20:24 GMT\"}]', '2007-05-23', '[[\"Delbo\",\"Marco\",\"\",\"INAF-Osservatorio Astronomico Di Torino, Oca\"],[\"Dell\'oro\",\"Aldo\",\"\",\"INAF-Osservatorio Astronomico Di Torino\"],[\"Harris\",\"Alan W.\",\"\",\"DLR\\n  Institute of Planetary Research\"],[\"Mottola\",\"Stefano\",\"\",\"DLR Institute of Planetary\\n  Research\"],[\"Mueller\",\"Michael\",\"\",\"DLR Institute of Planetary Research\"]]'),
(704.1916, 'Hans J. Haubold', 'R.K. Saxena, A.M. Mathai, H.J. Haubold', 'Solutions of certain fractional kinetic equations and a fractional\n  diffusion equation', '10 pages, LaTeX,corrected typos', 'Journal of Mathematical Physics 51(2010)103506', '10.1063/1.3496829', '', 'math.CA', '', '  In view of the usefulness and importance of the kinetic equation in certain\nphysical problems, the authors derive the explicit solution of a fractional\nkinetic equation of general character, that unifies and extends earlier\nresults. Further, an alternative shorter method based on a result developed by\nthe authors is given to derive the solution of a fractional diffusion equation.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:20:52 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 7 Aug 2007 16:15:22 GMT\"}]', '2015-05-13', '[[\"Saxena\",\"R. K.\",\"\"],[\"Mathai\",\"A. M.\",\"\"],[\"Haubold\",\"H. J.\",\"\"]]'),
(704.1917, 'Dan Bohr', 'Dan Bohr and Peter Schmitteckert', 'Strong enhancement of transport by interaction on contact links', 'Published version -- references corrected', 'Phys. Rev. B 75, 241103(R) (2007)', '10.1103/PhysRevB.75.241103', '', 'cond-mat.str-el', '', '  Strong repulsive interactions within a one dimensional Fermi system in a\ntwo-probe configuration normally lead to a reduced off-resonance conductance.\nWe show that if the repulsive interaction extends to the contact regions, a\nstrong increase of the conductance may occur, even for systems where one would\nexpect to find a reduced conductance. An essential ingredient in our\ncalculations is a momentum-space representation of the leads, which allows a\nhigh energy resolution. Further, we demonstrate that these results are\nindependent of the high-energy cutoff and that the relevant scale is set by the\nFermi velocity.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:21:27 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 14 Jun 2007 09:10:24 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 18 Jun 2007 07:00:11 GMT\"}]', '2007-06-18', '[[\"Bohr\",\"Dan\",\"\"],[\"Schmitteckert\",\"Peter\",\"\"]]'),
(704.1918, 'Christoffer Wittmann', 'C. Wittmann, D. Elser, U. L. Andersen, R. Filip, P. Marek, G. Leuchs', 'Quantum Filtering of Optical Coherent States', '6 pages, 5 figures', '', '10.1103/PhysRevA.78.032315', '', 'quant-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We propose and experimentally demonstrate non-destructive and noiseless\nremoval (filtering) of vacuum states from an arbitrary set of coherent states\nof continuous variable systems. Errors i.e. vacuum states in the quantum\ninformation are diagnosed through a weak measurement, and on that basis,\nprobabilistically filtered out. We consider three different filters based on\non/off detection phase stabilized and phase randomized homodyne detection. We\nfind that on/off etection, optimal in the ideal theoretical setting, is\nsuperior to the homodyne strategy in a practical setting.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 15:55:42 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 13 Aug 2007 16:41:28 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 29 Sep 2008 13:53:29 GMT\"}]', '2009-11-13', '[[\"Wittmann\",\"C.\",\"\"],[\"Elser\",\"D.\",\"\"],[\"Andersen\",\"U. L.\",\"\"],[\"Filip\",\"R.\",\"\"],[\"Marek\",\"P.\",\"\"],[\"Leuchs\",\"G.\",\"\"]]'),
(704.1919, 'Francois Fressin', 'Francois Fressin (LG), Tristan Guillot (OCA), Vincent Morello (OCA),\n  Fr\\\'ed\\\'eric Pont', 'Interpreting and predicting the yield of transit surveys: Giant planets\n  in the OGLE fields', 'article in press in A&A, 21 pages, 18 figures', 'Astron.Astrophys.475:729-746,2007', '10.1051/0004-6361:20077138', '', 'astro-ph', '', '  Transiting extrasolar planets are now discovered jointly by photometric\nsurveys and by radial velocimetry. We want to determine whether the different\ndata sets are compatible between themselves and with models of the evolution of\nextrasolar planets. We simulate directly a population of stars corresponding to\nthe OGLE transit survey and assign them planetary companions based on radial\nvelocimetry discoveries. We use a model of the evolution and structure of giant\nplanets assuming a variable fraction of heavy elements. The output list of\ndetectable planets of the simulations is compared to the real detections. We\nconfirm that the radial velocimetry and photometric survey data sets are\ncompatible within the statistical errors, assuming that planets with periods\nbetween 1 and 2 days are approximately 5 times less frequent than planets with\nperiods between 2 and 5 days. We show that evolution models fitting present\nobservational constraints predict a lack of small giant planets with large\nmasses. We also identify distinct populations of planets: those with short\nperiods (P < 10d) are only found in orbit around metal-rich stars with [Fe/H] >\n-0.07. We further confirm the relative absence of low-mass giant planets at\nsmall orbital distances.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 19:25:16 GMT\"}]', '2011-08-04', '[[\"Fressin\",\"Francois\",\"\",\"LG\"],[\"Guillot\",\"Tristan\",\"\",\"OCA\"],[\"Morello\",\"Vincent\",\"\",\"OCA\"],[\"Pont\",\"Frédéric\",\"\"]]'),
(704.1920, 'Manuel Ortega-Rodr\\\'iguez', 'Manuel Ortega-Rodriguez, Robert V. Wagoner', 'Global Disk Oscillation Modes in Cataclysmic Variables and Other\n  Newtonian Accretors', '1 figure', 'Astrophys.J.668:1158-1164,2007', '10.1086/521419', '', 'astro-ph', '', '  Diskoseismology, the theoretical study of small adiabatic hydrodynamical\nglobal perturbations of geometrically thin, optically thick accretion disks\naround black holes (and other compact objects), is a potentially powerful probe\nof the gravitational field. For instance, the frequencies of the normal mode\noscillations can be used to determine the elusive angular momentum parameter of\nthe black hole. The general formalism developed by diskoseismologists for\nrelativistic systems can be readily applied to the Newtonian case of\ncataclysmic variables (CVs). Some of these systems (e.g., the dwarf nova SS\nCygni) show rapid oscillations in the UV with periods of tens of seconds and\nhigh coherence. In this paper, we assess the possibility that these dwarf nova\noscillations (DNOs) are diskoseismic modes. Besides its importance in\ninvestigating the physical origin of DNOs, the present work could help us to\nanswer the following question. To what extent are the similarities in the\noscillation phenomenology of CVs and X-ray binaries (XRBs) indicative of a\ncommon physical mechanism?\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 20:33:38 GMT\"}]', '2009-11-16', '[[\"Ortega-Rodriguez\",\"Manuel\",\"\"],[\"Wagoner\",\"Robert V.\",\"\"]]'),
(704.1921, 'Isabelle Herbauts', 'I.M.Herbauts and D.J.Dunstan', 'Quantum molecular dynamics study of the pressure dependence of the\n  ammonia inversion transition', 'pdf format, 10 pages, 4 figures', 'Physical Review A (Vol.76, No.6, December 2007)', '10.1103/PhysRevA.76.062506', '', 'quant-ph cond-mat.other', '', '  The mechanism of the shift, broadening and quenching of the ammonia inversion\nfrequency with gas pressure has been a problem of lively interest for over\nseventy years. A simple quantum model of the ammonia molecule perturbed by\ncollisions with ideal gas molecules displays the essential features of the\nexperimental data for NH3 and for ND3. The model does not display the behaviour\nexpected from theories of quantum localisation such as quantum state diffusion\nand decoherence. On the other hand, models of perturbed classical oscillators\ndo display similar behaviour to our model. The quenching of the ammonia\ninversion transition cannot therefore be interpreted as spatial localisation of\nthe wavefunction.\n', '[{\"version\":\"v1\",\"created\":\"Sun, 15 Apr 2007 20:36:58 GMT\"}]', '2008-01-08', '[[\"Herbauts\",\"I. M.\",\"\"],[\"Dunstan\",\"D. J.\",\"\"]]');

INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.1958, 'Fausto Vagnetti', 'D.Trevese, D.Paris, G. M. Stirpe, F.Vagnetti, V. Zitelli', 'Line and continuum variability of two intermediate-redshift,\n  high-luminosity quasars', '6 pages, 5 figures, A&A in press', '', '10.1051/0004-6361:20077237', '', 'astro-ph', '', '  It has been shown that the luminosity of AGNs and the size of their broad\nline region obey a simple relation of the type R=a L^g, from faint Seyfert\nnuclei to bright quasars, allowing single-epoch determination of the central\nblack hole mass M=b L^g D^2 from their luminosity L and width of H_beta\nemission line. Adopting this mass determination for cosmological studies\nrequires the extrapolation to high z and L of a relation whose calibration\nrelies so far on reverberation mapping measurements performed for L<10^46 erg/s\nand z<0.4. We initiated a campaign for the monitoring of a few luminous,\nintermediate z quasars whose apparent magnitude V<15.7 allows observations with\na 1.8m telescope, aimed at proving that emission lines vary and respond to\ncontinuum variations even for luminosities >10^47 erg/s, and determining\neventually their M_BH from reverberation mapping. We have repeatedly performed\nsimultaneous observations of quasars and reference stars to determine relative\nvariability of continuum and emission lines. We describe the observations and\nmethods of analysis. For the quasars PG1634+706 and PG1247+268 we obtain\nlight-curves respectively for CIII], MgII and for CIV, CIII] emission lines\nwith the relevant continua. During 3.2 years of observation, in the former case\nno continuum variability has been detected and the evidence for line\nvariability is marginal, while in the latter case both continuum and line\nvariability are detected with high significance and the line variations appear\ncorrelated with continuum variations. The detection of the emission line\nvariability in a quasar with L~10^47 erg/s encourages the prosecution of the\ncampaign which should provide a black hole mass estimate in other 5-6 years,\nconstraining the M_BH-L relation in a poorly explored range of luminosity.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:25:25 GMT\"}]', '2009-11-13', '[[\"Trevese\",\"D.\",\"\"],[\"Paris\",\"D.\",\"\"],[\"Stirpe\",\"G. M.\",\"\"],[\"Vagnetti\",\"F.\",\"\"],[\"Zitelli\",\"V.\",\"\"]]'),
(704.1959, 'Boris Fainberg', 'B.D. Fainberg and V.A. Gorbunov', 'Adiabatic passage in a three-state system with non-Markovian relaxation:\n  The role of excited-state absorption and two-exciton processes', '38 pages, 7 figures; submitted to JPC', 'J. Phys. Chem. A, v.111, pp9560-9569 (2007)', '10.1021/jp0728611', '', 'physics.chem-ph physics.optics', '', '  The influence of excited-state absorption (ESA) and two-exciton processes on\na coherent population transfer with intense ultrashort chirped pulses in\nmolecular systems in solution has been studied. An unified treatment of\nadiabatic rapid passage (ARP) in such systems has been developed using a\nthree-state electronic system with relaxation treated as a diffusion on\nelectronic potential energy surfaces. We have shown that ESA has a profound\neffect on coherent population transfer in large molecules that necessitates a\nmore accurate interpretation of experimental data. A simple and physically\nclear model for ARP in molecules with three electronic states in solution has\nbeen developed by extending the Landau-Zener calculations putting in a third\nlevel to random crossing of levels. A method for quantum control of two-exciton\nstates in molecular complexes has been proposed.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:29:14 GMT\"}]', '2016-09-28', '[[\"Fainberg\",\"B. D.\",\"\"],[\"Gorbunov\",\"V. A.\",\"\"]]'),
(704.1960, 'Karl-Henning Rehren', 'Nikolay M. Nikolov, Karl-Henning Rehren, Ivan Todorov', 'Harmonic bilocal fields generated by globally conformal invariant scalar\n  fields', '29 pages. v2: corrected an argument, v4: final version as to be\n  published in CMP', 'Commun.Math.Phys.279:225-250,2008', '10.1007/s00220-007-0394-0', 'ICTP Trieste IC/2007021, ESI Vienna ESI 1907 (2007)', 'hep-th math-ph math.MP', '', '  The twist two contribution in the operator product expansion of phi_1(x_1)\nphi_2(x_2) for a pair of globally conformal invariant, scalar fields of equal\nscaling dimension d in four space-time dimensions is a field V_1(x_1,x_2) which\nis harmonic in both variables. It is demonstrated that the Huygens bilocality\nof V_1 can be equivalently characterized by a \"single-pole property\" concerning\nthe pole structure of the (rational) correlation functions involving the\nproduct phi_1(x_1) phi_2(x_2). This property is established for the dimension\nd=2 of phi_1, phi_2. As an application we prove that any system of GCI scalar\nfields of conformal dimension 2 (in four space-time dimensions) can be\npresented as a (possibly infinite) superposition of products of free massless\nfields.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:36:03 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 14 May 2007 10:13:07 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 5 Jun 2007 10:32:54 GMT\"},{\"version\":\"v4\",\"created\":\"Wed, 16 Jan 2008 13:34:30 GMT\"}]', '2008-11-26', '[[\"Nikolov\",\"Nikolay M.\",\"\"],[\"Rehren\",\"Karl-Henning\",\"\"],[\"Todorov\",\"Ivan\",\"\"]]'),
(704.1961, 'Yi Liao', 'Yi Liao (Nankai U.)', 'Impact of spin-zero particle-photon interactions on light polarization\n  in external magnetic fields', 'To appear in PLB, 10 pp, 0 figs; thanks to the anonymous referee for\n  useful comments/suggestions. Main changes: (1)English hopefully improved.\n  (2)The word `interference\' deleted. (3)Results unchanged but discussions\n  extended. (4)Quote Ref [26] where spin-zero particles with mixed parity\n  appear. (5)Acknowledgements added', 'Phys.Lett.B650:257-261,2007', '10.1016/j.physletb.2007.05.020', '', 'hep-ph hep-ex', '', '  If the recent PVLAS results on polarization changes of a linearly polarized\nlaser beam passing through a magnetic field are interpreted by an axion-like\nparticle, it is almost certain that it is not a standard QCD axion. Considering\nthis, we study the general effective interactions of photons with spin-zero\nparticles without restricting the latter to be a pseudo-scalar or a scalar,\ni.e., a parity eigenstate. At the lowest order in effective field theory, there\nare two dimension-5 interactions, each of which has previously been treated\nseparately for a pseudo-scalar or a scalar particle. By following the evolution\nin an external magnetic field of the system of spin-zero particles and photons,\nwe compute the changes in light polarization and the transition probability for\ntwo experimental set-ups: one-way propagation and round-trip propagation. While\nthe first may be relevant for astrophysical sources of spin-zero particles, the\nsecond applies to laboratory optical experiments like PVLAS. In the one-way\npropagation, interesting phenomena can occur for special configurations of\npolarization where, for instance, transition occurs but light polarization does\nnot change. For the round-trip propagation, however, the standard results of\npolarization changes for a pseudoscalar or a scalar are only modified by a\nfactor that depends on the relative strength of the two interactions.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:38:32 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 17 May 2007 03:15:12 GMT\"}]', '2008-11-26', '[[\"Liao\",\"Yi\",\"\",\"Nankai U.\"]]'),
(704.1962, 'Robert Alicki', 'Robert Alicki and Nicholas Van Ryn', 'A simple test of quantumness for a single system', '3 pages, no figures, corrected typos, text essentially amended', 'J. Phys. A: Math. Theor. 41 (2008) 062001', '10.1088/1751-8113/41/6/062001', '', 'quant-ph', '', '  We propose a simple test of quantumness which can decide whether for the\ngiven set of accessible experimental data the classical model is insufficient.\nTake two observables $ A,B$ such that for any state $\\psi$ their mean values\nsatisfy $0\\leq <\\psi|A|\\psi>\\leq <\\psi|B|\\psi>\\leq 1$. If there exists a state\n$\\phi$ such that the second moments fulfill the inequality $<\\phi|A^2|\\phi>\n><\\phi|B^2|\\phi>$ then the system cannot be described by the classical\nprobabilistic scheme. An example of an optimal triple $(A,B,\\phi)$ in the case\nof a qubit is given.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:39:33 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 8 May 2007 17:33:10 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 2 Jul 2007 11:10:55 GMT\"}]', '2012-10-26', '[[\"Alicki\",\"Robert\",\"\"],[\"Van Ryn\",\"Nicholas\",\"\"]]'),
(704.1963, 'David Barrado y Navascues', 'D. Barrado y Navascues, J. R. Stauffer, M. Morales-Calderon, A. Bayo,\n  G. Fazzio, T. Megeath, L. Allen, L. W. Hartmann, N. Calvet', 'SPITZER: Accretion in Low Mass Stars and Brown Dwarfs in the Lambda\n  Orionis Cluster', 'ApJ, in press', 'Astrophys.J.664:481-500,2007', '10.1086/518816', '', 'astro-ph', '', '  We present multi-wavelength optical and infrared photometry of 170 previously\nknown low mass stars and brown dwarfs of the 5 Myr Collinder 69 cluster (Lambda\nOrionis). The new photometry supports cluster membership for most of them, with\nless than 15% of the previous candidates identified as probable non-members.\nThe near infrared photometry allows us to identify stars with IR excesses, and\nwe find that the Class II population is very large, around 25% for stars (in\nthe spectral range M0 - M6.5) and 40% for brown dwarfs, down to 0.04 Msun,\ndespite the fact that the H(alpha) equivalent width is low for a significant\nfraction of them. In addition, there are a number of substellar objects,\nclassified as Class III, that have optically thin disks. The Class II members\nare distributed in an inhomogeneous way, lying preferentially in a filament\nrunning toward the south-east. The IR excesses for the Collinder 69 members\nrange from pure Class II (flat or nearly flat spectra longward of 1 micron), to\ntransition disks with no near-IR excess but excesses beginning within the IRAC\nwavelength range, to two stars with excess only detected at 24 micron.\nCollinder 69 thus appears to be at an age where it provides a natural\nlaboratory for the study of primordial disks and their dissipation.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:41:29 GMT\"}]', '2009-06-23', '[[\"Navascues\",\"D. Barrado y\",\"\"],[\"Stauffer\",\"J. R.\",\"\"],[\"Morales-Calderon\",\"M.\",\"\"],[\"Bayo\",\"A.\",\"\"],[\"Fazzio\",\"G.\",\"\"],[\"Megeath\",\"T.\",\"\"],[\"Allen\",\"L.\",\"\"],[\"Hartmann\",\"L. W.\",\"\"],[\"Calvet\",\"N.\",\"\"]]'),
(704.1964, 'Yi Pan', 'Yi Pan, Alessandra Buonanno, John G. Baker, Joan Centrella, Bernard J.\n  Kelly, Sean T. McWilliams, Frans Pretorius and James R. van Meter', 'A data-analysis driven comparison of analytic and numerical coalescing\n  binary waveforms: nonspinning case', '19 pages, 17 figures, added references, corrected typos, changed\n  figure 16', 'Phys.Rev.D77:024014,2008', '10.1103/PhysRevD.77.024014', '', 'gr-qc', '', '  We compare waveforms obtained by numerically evolving nonspinning binary\nblack holes to post-Newtonian (PN) template families currently used in the\nsearch for gravitational waves by ground-based detectors. We find that the\ntime-domain 3.5PN template family, which includes the inspiral phase, has\nfitting factors (FFs) >= 0.96 for binary systems with total mass M = 10 ~ 20\nMsun. The time-domain 3.5PN effective-one-body template family, which includes\nthe inspiral, merger and ring-down phases, gives satisfactory signal-matching\nperformance with FFs >= 0.96 for binary systems with total mass M = 10 ~ 120\nMsun. If we introduce a cutoff frequency properly adjusted to the final\nblack-hole ring-down frequency, we find that the frequency-domain\nstationary-phase-approximated template family at 3.5PN order has FFs >= 0.96\nfor binary systems with total mass M = 10 ~ 20 Msun. However, to obtain high\nmatching performances for larger binary masses, we need to either extend this\nfamily to unphysical regions of the parameter space or introduce a 4PN order\ncoefficient in the frequency-domain GW phase. Finally, we find that the\nphenomenological Buonanno-Chen-Vallisneri family has FFs >= 0.97 with total\nmass M=10 ~ 120Msun. The main analyses use the noise spectral-density of LIGO,\nbut several tests are extended to VIRGO and advanced LIGO noise-spectral\ndensities.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:16:41 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 25 Aug 2007 20:39:11 GMT\"}]', '2008-11-26', '[[\"Pan\",\"Yi\",\"\"],[\"Buonanno\",\"Alessandra\",\"\"],[\"Baker\",\"John G.\",\"\"],[\"Centrella\",\"Joan\",\"\"],[\"Kelly\",\"Bernard J.\",\"\"],[\"McWilliams\",\"Sean T.\",\"\"],[\"Pretorius\",\"Frans\",\"\"],[\"van Meter\",\"James R.\",\"\"]]'),
(704.1965, 'Phoenix S. Y. Poon', 'Phoenix S. Y. Poon and C. K. Law', 'Quantum entanglement of decohered two-mode squeezed states in absorbing\n  and amplifying environment', '9 pages, 7 figures', 'Phys. Rev. A 76, 012333 (2007)', '10.1103/PhysRevA.76.012333', '', 'quant-ph', '', '  We investigate the properties of quantum entanglement of two-mode squeezed\nstates interacting with linear baths with general gain and loss parameters. By\nexplicitly solving for \\rho from the master equation, we determine analytical\nexpressions of eigenvalues and eigenvectors of \\rho^{T_A} (the partial\ntransposition of density matrix \\rho). In Fock space, \\rho^{T_A} is shown to\nmaintain a block diagonal structure as the system evolves. In addition, we\ndiscover that the decoherence induced by the baths would break the degeneracy\nof \\rho^{T_A}, and leads to a novel set of eigenvectors for the construction of\nentanglement witness operators. Such eigenvectors are shown to be\ntime-independent, which is a signature of robust entanglement of two-mode\nsqueezed states in the presence of noise.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:44:29 GMT\"}]', '2009-11-13', '[[\"Poon\",\"Phoenix S. Y.\",\"\"],[\"Law\",\"C. K.\",\"\"]]'),
(704.1966, 'Gautam Bharali', 'Gautam Bharali', 'Some new observations on interpolation in the spectral unit ball', 'Added a definition (Def.1.1); 2 of the 4 results herein are minor\n  refinements of those in the author\'s preprint math.CV/0608177; to appear in\n  Integral Eqns. Operator Theory', 'Integral Equations Operator Theory 59 (2007) no. 3, 329-343', '10.1007/s00020-007-1534-9', '', 'math.CV math.OA', '', '  We present several results associated to a holomorphic-interpolation problem\nfor the spectral unit ball \\Omega_n, n\\geq 2. We begin by showing that a known\nnecessary condition for the existence of a\n$\\mathcal{O}(D;\\Omega_n)$-interpolant (D here being the unit disc in the\ncomplex plane), given that the matricial data are non-derogatory, is not\nsufficient. We provide next a new necessary condition for the solvability of\nthe two-point interpolation problem -- one which is not restricted only to\nnon-derogatory data, and which incorporates the Jordan structure of the\nprescribed data. We then use some of the ideas used in deducing the latter\nresult to prove a Schwarz-type lemma for holomorphic self-maps of \\Omega_n,\nn\\geq 2.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:49:01 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 17 Sep 2007 16:36:57 GMT\"}]', '2008-02-14', '[[\"Bharali\",\"Gautam\",\"\"]]'),
(704.1967, 'Francesco Becattini', 'F. Becattini, L. Ferroni (University of Florence and INFN Florence)', 'The microcanonical ensemble of the ideal relativistic quantum gas', '31 pages; published version with minor corrections', 'Eur.Phys.J.C51:899-912,2007', '10.1140/epjc/s10052-007-0340-5', '', 'nucl-th cond-mat.stat-mech quant-ph', '', '  We derive the microcanonical partition function of the ideal relativistic\nquantum gas of spinless bosons in a quantum field framework as an expansion\nover fixed multiplicities. Our calculation generalizes well known expressions\nin literature in that it does not introduce any large volume approximation and\nit is valid at any volume. We discuss the issues concerned with the definition\nof the microcanonical ensemble for a free quantum field at volumes comparable\nwith the Compton wavelength and provide a consistent prescription of\ncalculating the microcanonical partition function, which is finite at finite\nvolume and yielding the correct thermodynamic limit. Besides an immaterial\noverall factor, the obtained expression turns out to be the same as in the\nnon-relativistic multi-particle approach. This work is introductory to derive\nthe most general expression of the microcanonical partition function fixing the\nmaximal set of observables of the Poincare\' group.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:54:22 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 9 Oct 2007 10:58:49 GMT\"}]', '2008-11-26', '[[\"Becattini\",\"F.\",\"\",\"University of Florence and INFN Florence\"],[\"Ferroni\",\"L.\",\"\",\"University of Florence and INFN Florence\"]]'),
(704.1968, 'L\\\'aszl\\\'o \\\'A Gergely', 'L\\\'aszl\\\'o \\\'A. Gergely, Peter L. Biermann', 'The spin-flip phenomenon in supermassive black hole binary mergers', 'v3: 36 pages, 1 figure; discussion on the validity of the model and\n  estimates for the angular value of the spin-flip added to Section 5; v4:\n  minor changes, 2 new references, published version', 'Astrophys.J.697:1621-1633,2009', '10.1088/0004-637X/697/2/1621', '', 'astro-ph gr-qc', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Massive merging black holes will be the primary sources of powerful\ngravitational waves at low frequency, and will permit to test general\nrelativity with candidate galaxies close to a binary black hole merger. In this\npaper we identify the typical mass ratio of the two black holes but then show\nthat the distance when gravitational radiation becomes the dominant dissipative\neffect (over dynamical friction) does not depend on the mass ratio. However the\ndynamical evolution in the gravitational wave emission regime does. For the\ntypical range of mass ratios the final stage of the merger is preceded by a\nrapid precession and a subsequent spin-flip of the main black hole. This\nalready occurs in the inspiral phase, therefore can be described analytically\nby post-Newtonian techniques. We then identify the radio galaxies with a\nsuper-disk as those in which the rapidly precessing jet produces effectively a\npowerful wind, entraining the environmental gas to produce the appearance of a\nthick disk. These specific galaxies are thus candidates for a merger of two\nblack holes to happen in the astronomically near future.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:06:41 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 23 Jun 2008 15:32:05 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 21 Apr 2009 12:36:11 GMT\"},{\"version\":\"v4\",\"created\":\"Fri, 15 May 2009 22:13:05 GMT\"}]', '2009-06-23', '[[\"Gergely\",\"László Á.\",\"\"],[\"Biermann\",\"Peter L.\",\"\"]]'),
(704.1969, 'Janvier Nzeutchap', 'Janvier Nzeutchap', 'On the Young-Fibonacci insertion algorithm', '19 pages, to appear in the Proceedings of FPSAC\'07', '', '', '', 'math.CO', '', '  This work is concerned with some properties of the Young-Fibonacci insertion\nalgorithm and its relation with Fomin\'s growth diagrams. It also investigates a\nrelation between the combinatorics of Young-Fibonacci tableaux and the study of\nOkada\'s algebra associated to the Young-Fibonacci lattice. The original\nalgorithm was introduced by Roby and we redefine it in such a way that both the\ninsertion and recording tableaux of any permutation are \\emph{conveniently}\ninterpreted as chains in the Young-Fibonacci lattice. A property of\nKillpatrick\'s evacuation is given a simpler proof, but this evacuation is no\nlonger needed in making Roby\'s and Fomin\'s constructions coincide. We provide\nthe set of Young-Fibonacci tableaux of size $n$ with a structure of graded\nposet, induced by the weak order on permutations of the symmetric group, and\nrealized by transitive closure of elementary transformations on tableaux. We\nshow that this poset gives a combinatorial interpretation of the coefficients\nin the transition matrix from the analogue of complete symmetric functions to\nanalogue of the Schur functions in Okada\'s algebra. We end with a quite similar\nobservation for four posets on Young-tableaux studied by Taskin.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 09:57:53 GMT\"}]', '2007-05-23', '[[\"Nzeutchap\",\"Janvier\",\"\"]]'),
(704.1970, 'Koichi Izawa', 'K. Izawa, K. Behnia, Y. Matsuda, H. Shishido, R.Settai, Y. Onuki and\n  J. Flouquet', 'Thermoelectric response near a quantum critical point: the case of\n  CeCoIn5', '4 pages, 4 figures,final published version', 'Phys. Rev. Lett. 99, 147005 (2007)', '10.1103/PhysRevLett.99.147005', '', 'cond-mat.str-el cond-mat.supr-con', '', '  We present a study of thermoelectric coefficients in CeCoIn_5 down to 0.1 K\nand up to 16 T in order to probe the thermoelectric signatures of quantum\ncriticality. In the vicinity of the field-induced quantum critical point, the\nNernst coefficient nu exhibits a dramatic enhancement without saturation down\nto lowest measured temperature. The dimensionless ratio of Seebeck coefficient\nto electronic specific heat shows a minimum at a temperature close to threshold\nof the quasiparticle formation. Close to T_c(H), in the vortex-liquid state,\nthe Nernst coefficient behaves anomalously in puzzling contrast with other\nsuperconductors and standard vortex dynamics.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:00:58 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 9 Oct 2007 10:34:40 GMT\"}]', '2009-11-13', '[[\"Izawa\",\"K.\",\"\"],[\"Behnia\",\"K.\",\"\"],[\"Matsuda\",\"Y.\",\"\"],[\"Shishido\",\"H.\",\"\"],[\"Settai\",\"R.\",\"\"],[\"Onuki\",\"Y.\",\"\"],[\"Flouquet\",\"J.\",\"\"]]'),
(704.1971, 'Natalia Berloff', 'Natalia G. Berloff and Anthony J. Youd', 'Dissipative dynamics of superfluid vortices at non-zero temperatures', '4 pages, 3 figures', '', '10.1103/PhysRevLett.99.145301', '', 'cond-mat.soft', '', '  We consider the evolution and dissipation of vortex rings in a condensate at\nnon-zero temperature, in the context of the classical field approximation,\nbased on the defocusing nonlinear Schr\\\"odinger equation. The temperature in\nsuch a system is fully determined by the total number density and the number\ndensity of the condensate. A vortex ring is introduced into a condensate in a\nstate of thermal equilibrium, and interacts with non-condensed particles. These\ninteractions lead to a gradual decrease in the vortex line density, until the\nvortex ring completely disappears. We show that the square of the vortex line\nlength changes linearly with time, and obtain the corresponding universal decay\nlaw. We relate this to mutual friction coefficients in the fundamental equation\nof vortex motion in superfluids.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:05:11 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 21 Jun 2007 17:15:23 GMT\"}]', '2009-11-13', '[[\"Berloff\",\"Natalia G.\",\"\"],[\"Youd\",\"Anthony J.\",\"\"]]'),
(704.1972, 'Arno Kuijlaars', 'A.R. Its, A.B.J. Kuijlaars, and J. Ostensson', 'Critical edge behavior in unitary random matrix ensembles and the thirty\n  fourth Painleve transcendent', '51 pages, 6 figures', 'International Mathematics Research Notices 2008, article ID rnn017', '', '', 'math.CA math-ph math.MP', '', '  We describe a new universality class for unitary invariant random matrix\nensembles. It arises in the double scaling limit of ensembles of random $n\n\\times n$ Hermitian matrices $Z_{n,N}^{-1} |\\det M|^{2\\alpha} e^{-N \\Tr V(M)}\ndM$ with $\\alpha > -1/2$, where the factor $|\\det M|^{2\\alpha}$ induces\ncritical eigenvalue behavior near the origin. Under the assumption that the\nlimiting mean eigenvalue density associated with $V$ is regular, and that the\norigin is a right endpoint of its support, we compute the limiting eigenvalue\ncorrelation kernel in the double scaling limit as $n, N \\to \\infty$ such that\n$n^{2/3}(n/N-1) = O(1)$. We use the Deift-Zhou steepest descent method for the\nRiemann-Hilbert problem for polynomials on the line orthogonal with respect to\nthe weight $|x|^{2\\alpha} e^{-NV(x)}$. Our main attention is on the\nconstruction of a local parametrix near the origin by means of the\n$\\psi$-functions associated with a distinguished solution of the Painleve XXXIV\nequation. This solution is related to a particular solution of the Painleve II\nequation, which however is different from the usual Hastings-McLeod solution.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:22:20 GMT\"}]', '2010-07-30', '[[\"Its\",\"A. R.\",\"\"],[\"Kuijlaars\",\"A. B. J.\",\"\"],[\"Ostensson\",\"J.\",\"\"]]'),
(704.1973, 'Jernej Mravlje', 'Jernej Mravlje, Anton Ramsak, Rok Zitko', 'Vibrational effects on low-temperature properties of molecular\n  conductors', '2 pages, 3 figures, to be presented on \"The International Conference\n  on Strongly Correlated Electron Systems\" SCES\'07, May 13-18, Houston, USA', 'Physica B 403, 1484 (2008)', '10.1016/j.physb.2007.10.170', '', 'cond-mat.mes-hall cond-mat.str-el', '', '  We calculate characteristic correlation functions for the Anderson model with\nadditional phonon-assisted coupling to the odd conduction channel. This model\ndescribes, for example, the behavior of a molecule embedded between two\nelectrodes in linear transport experiments where the position of the molecule\nwith respect to the leads affects the tunneling amplitudes. We use variational\nprojection-operator method and numerical renormalization group (NRG) method.\nThe spin is Kondo screened either by even or odd conduction channel depending\non the gate voltage and electron-phonon coupling. However, in all regimes the\ngate-voltage dependence of the zero temperature conductance is found to be\nqualitatively the same as in the model with no coupling to the vibrational\nmode.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:45:05 GMT\"}]', '2008-03-05', '[[\"Mravlje\",\"Jernej\",\"\"],[\"Ramsak\",\"Anton\",\"\"],[\"Zitko\",\"Rok\",\"\"]]'),
(704.1974, 'Helene Perrin', 'Olivier Morizot (LPL), Julien De Lapeyre De Bellair (LPL), Fabrice\n  Wiotte (LPL), Olivier Lopez (LPL), Paul-Eric Pottie (LPL), H\\\'el\\`ene Perrin\n  (LPL)', 'Agile low phase noise radio-frequency sine wave generator applied to\n  experiments on ultracold atoms', '10 pages, 6 figures', '', '', '', 'physics.atom-ph', '', '  We report on the frequency performance of a low cost (~500$) radio-frequency\nsine wave generator, using direct digital synthesis (DDS) and a\nfield-programmable gate array (FPGA). The output frequency of the device may be\nchanged dynamically to any arbitrary value ranging from DC to 10 MHz without\nany phase slip. Sampling effects are substantially reduced by a high sample\nrate, up to 1 MHz, and by a large memory length, more than 2.10^5 samples. By\nusing a low noise external oscillator to clock the DDS, we demonstrate a phase\nnoise as low as that of the master clock, that is at the level of -113\ndB.rad^2/Hz at 1 Hz from the carrier for an output frequency of 3.75 MHz. The\ndevice is successfully used to confine an ultracold atomic cloud of rubidium 87\nin a RF-based trap, and there is no extra heating from the RF source.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:36:55 GMT\"}]', '2007-05-23', '[[\"Morizot\",\"Olivier\",\"\",\"LPL\"],[\"De Bellair\",\"Julien De Lapeyre\",\"\",\"LPL\"],[\"Wiotte\",\"Fabrice\",\"\",\"LPL\"],[\"Lopez\",\"Olivier\",\"\",\"LPL\"],[\"Pottie\",\"Paul-Eric\",\"\",\"LPL\"],[\"Perrin\",\"Hélène\",\"\",\"LPL\"]]'),
(704.1975, 'Eugene Gutkin', 'Eugene Gutkin, Michal Rams', 'Growth rates for geometric complexities and counting functions in\n  polygonal billiards', '25 pages, 2 figures', 'Ergodic Theory & Dynamical Systems 29 (2009), 1163 -- 1183', '10.1017/S0143385708080620', '', 'math.DS math.DG', '', '  We introduce a new method for estimating the growth of various quantities\narising in dynamical systems. We apply our method to polygonal billiards on\nsurfaces of constant curvature. For instance, we obtain power bounds of degree\ntwo plus epsilon in length for the number of billiard orbits between almost all\npairs of points in a planar polygon.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:24:36 GMT\"}]', '2010-12-14', '[[\"Gutkin\",\"Eugene\",\"\"],[\"Rams\",\"Michal\",\"\"]]'),
(704.1976, 'Dorje C. Brody', 'Dorje C. Brody, Lane P. Hughston, Andrea Macrina', 'Information-Based Asset Pricing', '32 pages. No figure', 'International Journal of Theoretical and Applied Finance 11,\n  107-142 (2008)', '', '', 'q-fin.PR math.PR math.ST stat.TH', '', '  A new framework for asset price dynamics is introduced in which the concept\nof noisy information about future cash flows is used to derive the price\nprocesses. In this framework an asset is defined by its cash-flow structure.\nEach cash flow is modelled by a random variable that can be expressed as a\nfunction of a collection of independent random variables called market factors.\nWith each such \"X-factor\" we associate a market information process, the values\nof which are accessible to market agents. Each information process is a sum of\ntwo terms; one contains true information about the value of the market factor;\nthe other represents \"noise\". The noise term is modelled by an independent\nBrownian bridge. The market filtration is assumed to be that generated by the\naggregate of the independent information processes. The price of an asset is\ngiven by the expectation of the discounted cash flows in the risk-neutral\nmeasure, conditional on the information provided by the market filtration. When\nthe cash flows are the dividend payments associated with equities, an explicit\nmodel is obtained for the share-price, and the prices of options on\ndividend-paying assets are derived. Remarkably, the resulting formula for the\nprice of a European call option is of the Black-Scholes-Merton type. The\ninformation-based framework also generates a natural explanation for the origin\nof stochastic volatility.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:50:48 GMT\"}]', '2013-01-31', '[[\"Brody\",\"Dorje C.\",\"\"],[\"Hughston\",\"Lane P.\",\"\"],[\"Macrina\",\"Andrea\",\"\"]]'),
(704.1977, 'Xuanming Ye', 'Xuanming Ye', 'The Jumping Phenomenon of Hodge Numbers', '', '', '', '', 'math.AG math.DG', '', '  Let $X$ be a compact complex manifold, consider a small deformation $\\phi:\n\\mathcal{X} \\to B$ of $X$, the dimension of the Dolbeault cohomology groups\n$H^q(X_t,\\Omega_{X_t}^p)$ may vary under this defromation. This paper will\nstudy such phenomenons by studying the obstructions to deform a class in\n$H^q(X,\\Omega_X^p)$ with the parameter $t$ and get the formula for the\nobstructions.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 15:27:45 GMT\"}]', '2007-05-23', '[[\"Ye\",\"Xuanming\",\"\"]]'),
(704.1978, 'Yoichi Ikeda', 'Y. Ikeda and T. Sato', 'Strange dibaryon resonance in the anti-KNN--piYN system', '22 pages, 10 figures; added extended KNN-piYN calculation, Appendix', 'Phys.Rev.C76:035203,2007', '10.1103/PhysRevC.76.035203', '', 'nucl-th', '', '  Three-body resonances in the \\bar{K}NN system have been studied within a\nframework of the \\bar{K}NN-\\pi YN coupled hannel Faddeev equation. By solving\nthe three-body equation the energy dependence of the resonant \\bar{K}N\namplitude is fully taken into account. The S-matrix pole has been investigated\nfrom the eigenvalue of the kernel with the analytic continuation of the\nscattering amplitude on the unphysical Riemann sheet. The \\barKN interaction is\nconstructed from the leading order term of the chiral Lagrangian using\nrelativistic kinematics. The \\Lambda(1405) resonance is dynamically generated\nin this model, where the \\bar{K}N interaction parameters are fitted to the data\nof scattering length. As a result we find a three-body resonance of the strange\ndibaryon system with binding energy, B~79 MeV, and width, \\Gamma~74 MeV. The\nenergy of the three-body resonance is found to be sensitive to the model of the\nI=0 \\barKN interaction.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 10:58:24 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 7 Sep 2007 10:58:22 GMT\"}]', '2008-11-26', '[[\"Ikeda\",\"Y.\",\"\"],[\"Sato\",\"T.\",\"\"]]'),
(704.1979, 'Jernej Mravlje', 'Jernej Mravlje, Anton Ramsak, Tomaz Rejec', 'SU(2) and SU(4) Kondo effect in double quantum dots', '5 pages, 2 figures, presented on \"XI Training Course in the Physics\n  of Strongly Correlated Systems\", Vietri sul Mare, Salerno, Italy', 'AIP Conference Proceedings 918, 312 (2006)', '10.1063/1.2752001', '', 'cond-mat.mes-hall cond-mat.str-el', '', '  We investigate serial double quantum dot systems with on-site and inter-site\ninteraction by means of Sch\\\"onhammer-Gunnarsson projection-operator method.\nThe ground state is established by the competition between extended Kondo\nphases and localized singlet phases in spi$ degrees of freedom. We present and\ndiscuss different phases, as discerned by characteristic correlation functions.\nWe discuss also how different phases would be seen in linear transport\nmeasurements.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:00:24 GMT\"}]', '2007-12-20', '[[\"Mravlje\",\"Jernej\",\"\"],[\"Ramsak\",\"Anton\",\"\"],[\"Rejec\",\"Tomaz\",\"\"]]'),
(704.1980, 'Cristina Tablino Possio', 'C. Tablino Possio', 'V-cycle optimal convergence for DCT-III matrices', '19 pages', '', '', '', 'math.NA', '', '  The paper analyzes a two-grid and a multigrid method for matrices belonging\nto the DCT-III algebra and generated by a polynomial symbol. The aim is to\nprove that the convergence rate of the considered multigrid method (V-cycle) is\nconstant independent of the size of the given matrix. Numerical examples from\ndifferential and integral equations are considered to illustrate the claimed\nconvergence properties.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:07:30 GMT\"}]', '2007-05-23', '[[\"Possio\",\"C. Tablino\",\"\"]]'),
(704.1981, 'David W. Hertzog', 'MuLan Collaboration: D.B. Chitwood, T.I. Banks, M.J. Barnes, S. Battu,\n  R.M. Carey, S. Cheekatmalla, S.M. Clayton, J. Crnkovic, K.M. Crowe, P.T.\n  Debevec, S. Dhamija, W. Earle, A. Gafarov, K. Giovanetti, T.P. Gorringe, F.E.\n  Gray, M. Hance, D.W. Hertzog, M.F. Hare, P. Kammel, B. Kiburg, J. Kunkle, B.\n  Lauss, I. Logashenko, K.R. Lynch, R. McNabb, J.P. Miller, F. Mulhauser,\n  C.J.G. Onderwater, C.S. Ozben, Q. Peng, C.C. Polly, S. Rath, B.L. Roberts, V.\n  Tishchenko, G.D. Wait, J. Wasserman, D.M. Webber, P. Winter, P.A. Zolnierczuk', 'Improved Measurement of the Positive Muon Lifetime and Determination of\n  the Fermi Constant', 'As published version (PRL, July 2007)', 'Phys.Rev.Lett.99:032001,2007', '10.1103/PhysRevLett.99.032001', '', 'hep-ex nucl-ex', '', '  The mean life of the positive muon has been measured to a precision of 11 ppm\nusing a low-energy, pulsed muon beam stopped in a ferromagnetic target, which\nwas surrounded by a scintillator detector array. The result, tau_mu =\n2.197013(24) us, is in excellent agreement with the previous world average. The\nnew world average tau_mu = 2.197019(21) us determines the Fermi constant G_F =\n1.166371(6) x 10^-5 GeV^-2 (5 ppm). Additionally, the precision measurement of\nthe positive muon lifetime is needed to determine the nucleon pseudoscalar\ncoupling g_P.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 17:07:24 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 8 Feb 2008 16:02:11 GMT\"}]', '2008-11-26', '[[\"MuLan Collaboration\",\"\",\"\"],[\"Chitwood\",\"D. B.\",\"\"],[\"Banks\",\"T. I.\",\"\"],[\"Barnes\",\"M. J.\",\"\"],[\"Battu\",\"S.\",\"\"],[\"Carey\",\"R. M.\",\"\"],[\"Cheekatmalla\",\"S.\",\"\"],[\"Clayton\",\"S. M.\",\"\"],[\"Crnkovic\",\"J.\",\"\"],[\"Crowe\",\"K. M.\",\"\"],[\"Debevec\",\"P. T.\",\"\"],[\"Dhamija\",\"S.\",\"\"],[\"Earle\",\"W.\",\"\"],[\"Gafarov\",\"A.\",\"\"],[\"Giovanetti\",\"K.\",\"\"],[\"Gorringe\",\"T. P.\",\"\"],[\"Gray\",\"F. E.\",\"\"],[\"Hance\",\"M.\",\"\"],[\"Hertzog\",\"D. W.\",\"\"],[\"Hare\",\"M. F.\",\"\"],[\"Kammel\",\"P.\",\"\"],[\"Kiburg\",\"B.\",\"\"],[\"Kunkle\",\"J.\",\"\"],[\"Lauss\",\"B.\",\"\"],[\"Logashenko\",\"I.\",\"\"],[\"Lynch\",\"K. R.\",\"\"],[\"McNabb\",\"R.\",\"\"],[\"Miller\",\"J. P.\",\"\"],[\"Mulhauser\",\"F.\",\"\"],[\"Onderwater\",\"C. J. G.\",\"\"],[\"Ozben\",\"C. S.\",\"\"],[\"Peng\",\"Q.\",\"\"],[\"Polly\",\"C. C.\",\"\"],[\"Rath\",\"S.\",\"\"],[\"Roberts\",\"B. L.\",\"\"],[\"Tishchenko\",\"V.\",\"\"],[\"Wait\",\"G. D.\",\"\"],[\"Wasserman\",\"J.\",\"\"],[\"Webber\",\"D. M.\",\"\"],[\"Winter\",\"P.\",\"\"],[\"Zolnierczuk\",\"P. A.\",\"\"]]'),
(704.1982, 'Neil Seshadri', 'Neil Seshadri', 'Some notes on analytic torsion of the Rumin complex on contact manifolds', 'This paper has been withdrawn by the author, due a crucial error on\n  page 8. A corrected and extended version of this paper appears at\n  arXiv:0802.0123', '', '', '', 'math.DG', '', '  We propose a definition for analytic torsion of the Rumin complex on contact\nmanifolds. This is given by the derivative at zero of a well-chosen combination\nof zeta functions of a fourth-order modified Rumin Laplacian. The regular value\nat zero (before differentiation) of this well-chosen combination of zeta\nfunctions is shown to be a contact invariant. The variation of our analytic\ntorsion is given as the integral of local terms, together with a global term\ncoming from the null-space of the Laplacian.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:19:55 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 4 Feb 2008 01:38:27 GMT\"}]', '2008-02-04', '[[\"Seshadri\",\"Neil\",\"\"]]'),
(704.1983, 'Yi-Fang Chang', 'Yi-Fang Chang', 'Universal 2+1-Dimensional Plane Equations in General Relativity and\n  Evolutions of Disk Nebula', '7 pages', '', '', '', 'physics.gen-ph', '', '  The general relativity is the base for any exact evolutionary theory of large\nscale structures. We calculate the universal 2+1-dimensional plane equations of\ngravitational field in general relativity. Based on the equations, the\nevolutions of disk nebula are discussed. A system of nebula can form binary\nstars or single star for different conditions. While any simplified linear\ntheory forms only a single star system. It is proved that the nonlinear\ninteractions are very general, so the binary stars are also common.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:21:57 GMT\"}]', '2007-05-23', '[[\"Chang\",\"Yi-Fang\",\"\"]]'),
(704.1984, 'Herbert Muther', 'P. G\\\"ogelein and H. M\\\"uther, (Universit\\\"at T\\\"ubingen, Germany)', 'Nuclear matter in the crust of neutron stars', '23 pages, 8 figures', 'Phys.Rev.C76:024312,2007', '10.1103/PhysRevC.76.024312', '', 'nucl-th', '', '  The properties of inhomogeneous nuclear matter are investigated considering\nthe self-consistent Skyrme Hartree-Fock approach with inclusion of pairing\ncorrelations. For a comparison we also consider a relativistic mean field\napproach. The inhomogeneous infinite matter is described in terms of cubic\nWigner-Seitz cells, which leads to a smooth transition to the limit of\nhomogeneous nuclear matter. The possible existence of various structures in the\nso-called pasta phase is investigated within this self-consistent approach and\na comparison is made to results obtained within the Thomas-Fermi approximation.\nResults for the proton abundances and the pairing properties are discussed for\ndensities for which clustering phenomena are obtained.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:25:47 GMT\"}]', '2008-11-26', '[[\"Gögelein\",\"P.\",\"\"],[\"Müther\",\"H.\",\"\"]]'),
(704.1985, 'Jeremy Miller', 'J. S. Miller', 'Electromagnetic Higgs production', '23 pages, 5 figures', '', '', '', 'hep-ph', '', '  The cross section for central diffractive Higgs production is calculated, for\nthe LHC range of energies. The graphs for the possible mechanisms for Higgs\nproduction, through pomeron fusion and photon fusions are calculated for all\npossibilities allowed by the standard model. The cross section for central\ndiffractive Higgs production through pomeron fusion, must be multiplied by a\nfactor for the survival probability, to isolate the Higgs signal and reduce the\nbackground. Due to the small value of the survival probability $\\Lb 4 \\times\n10^{-3}\\Rb $, the cross sections for central diffractive Higgs production, in\nthe two cases for pomeron fusion and photon fusion, are competitive.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:34:18 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 13 Nov 2007 10:10:06 GMT\"}]', '2007-11-13', '[[\"Miller\",\"J. S.\",\"\"]]'),
(704.1986, 'Nabil Youssef L', 'Nabil L. Youssef', 'Characterization of Closed Vector Fields in Finsler Geometry', '10 pages, LaTeX file, Presented in \"The International Conference on\n  Finsler Extensions of Relativity Theory\" held at Cairo, Egypt, November 4-10,\n  2006', 'Hadronic J., 30,2 (2007), 193-207.', '', '', 'math.DG', '', '  The $\\pi$-exterior derivative ${\\o}d$, which is the Finslerian generalization\nof the (usual) exterior derivative $d$ of Riemannian geometry, is defined. The\nnotion of a ${\\o}d$-closed vector field is introduced and investigated. Various\ncharacterizations of ${\\o}d$-closed vector fields are established. Some results\nconcerning ${\\o}d$-closed vector fields in relation to certain special Finsler\nspaces are obtained.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:45:44 GMT\"}]', '2007-09-07', '[[\"Youssef\",\"Nabil L.\",\"\"]]'),
(704.1987, 'Anilesh Mohari', 'Anilesh Mohari', 'Pure inductive limit state and Kolmogorov\'s property', '', '', '', '', 'math.OA math.PR', '', '  Let $(\\clb,\\lambda_t,\\psi)$ be a $C^*$-dynamical system where $(\\lambda_t: t\n\\in \\IT_+)$ be a semigroup of injective endomorphism and $\\psi$ be an\n$(\\lambda_t)$ invariant state on the $C^*$ subalgebra $\\clb$ and $\\IT_+$ is\neither non-negative integers or real numbers. The central aim of this\nexposition is to find a useful criteria for the inductive limit state $\\clb\n\\raro^{\\lambda_t} \\clb$ canonically associated with $\\psi$ to be pure. We\nachieve this by exploring the minimal weak forward and backward Markov\nprocesses associated with the Markov semigroup on the corner von-Neumann\nalgebra of the support projection of the state $\\psi$ to prove that\nKolmogorov\'s property [Mo2] of the Markov semigroup is a sufficient condition\nfor the inductive state to be pure. As an application of this criteria we find\na sufficient condition for a translation invariant factor state on a one\ndimensional quantum spin chain to be pure. This criteria in a sense complements\ncriteria obtained in [BJKW,Mo2] as we could go beyond lattice symmetric states.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:46:36 GMT\"}]', '2007-05-23', '[[\"Mohari\",\"Anilesh\",\"\"]]'),
(704.1988, 'Emmanuel Clouet', 'Emmanuel Clouet (SRMP), Maylise Nastar (SRMP)', 'Classical nucleation theory in ordering alloys precipitating with L12\n  structure', '', 'Physical Review B 75, 13 (12/04/2007) 132102', '10.1103/PhysRevB.75.132102', '', 'cond-mat.mtrl-sci', '', '  By means of low-temperature expansions (LTEs), the nucleation free energy and\nthe precipitate interface free energy are expressed as functions of the\nsolubility limit for alloys which lead to the precipitation of a stoichiometric\nL12 compound such as Al-Sc or Al-Zr alloys. Classical nucleation theory is then\nused to obtain a simple expression of the nucleation rate whose validity is\ndemonstrated by a comparison with atomic simulations. LTEs also explain why\nsimple mean-field approximation like the Bragg-Williams approximation fails to\npredict correct nucleation rates in such an ordering alloy.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:51:44 GMT\"}]', '2007-05-23', '[[\"Clouet\",\"Emmanuel\",\"\",\"SRMP\"],[\"Nastar\",\"Maylise\",\"\",\"SRMP\"]]'),
(704.1989, 'Anilesh Mohari', 'Anilesh Mohari', 'Jones index of a quantum dynamical semigroup', '', '', '', '', 'math.OA math.PR', '', '  In this paper we consider a semigroup of completely positive maps\n$\\tau=(\\tau_t,t \\ge 0)$ with a faithful normal invariant state $\\phi$ on a\ntype-$II_1$ factor $\\cla_0$ and propose an index theory. We :achieve this via a\nmore general Kolmogorov\'s type of construction for stationary Markov processes\nwhich naturally associate a nested isomorphic von-Neumann algebras. In\nparticular this construction generalizes well known Jones construction\nassociated with a sub-factor of type-II$_1$ factor.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 11:58:56 GMT\"}]', '2007-05-23', '[[\"Mohari\",\"Anilesh\",\"\"]]'),
(704.1990, 'Eugenio R. Bezerra de Mello', 'J. Spinelly and E. R. Bezerra de Mello', 'Vacuum Polarization by a Magnetic Flux Tube at Finite Temperature in the\n  Cosmic String Spacetime', '16 pages, 1 figure', 'Int.J.Mod.Phys.D18:53-70,2009', '10.1142/S0218271809014273', '', 'hep-th gr-qc', '', '  In this paper we analyse the effect produced by the temperature in the vacuum\npolarization associated with charged massless scalar field in the presence of\nmagnetic flux tube in the cosmic string spacetime. Three different\nconfigurations of magnetic fields are taken into account: $(i)$ a homogeneous\nfield inside the tube, $(ii)$ a field proportional to $1/r$ and $(iii)$ a\ncylindrical shell with $\\delta$-function. In these three cases, the axis of the\ninfinitely long tube of radius $R$ coincides with the cosmic string. Because\nthe complexity of this analysis in the region inside the tube, we consider the\nthermal effect in the region outside. In order to develop this analysis, we\nconstruct the thermal Green function associated with this system for the three\nabove mentioned situations considering points in the region outside the tube.\nWe explicitly calculate in the high-temperature limit, the thermal average of\nthe field square and the energy-momentum tensor.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 12:02:57 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 3 Apr 2008 17:37:47 GMT\"}]', '2009-03-24', '[[\"Spinelly\",\"J.\",\"\"],[\"de Mello\",\"E. R. Bezerra\",\"\"]]'),
(704.1991, 'Ingo Schienbein', 'E. A. Paschos, I. Schienbein, J.-Y. Yu', 'Single pion electro-- and neutrinoproduction on heavy targets', '21 pages, 8 figures', '', '', 'DO-TH-07-05,LPSC-07-29,SMU-HEP-07-07', 'hep-ph', '', '  We present a calculation of single pion electroproduction cross sections on\nheavy targets in the kinematic region of the Delta(1232) resonance. Final state\ninteractions of the pions are taken into account using the pion multiple\nscattering model of Adler, Nussinov and Paschos (ANP model). For\nelectroproduction and neutral current reactions we obtain results for carbon,\noxygen, argon and iron targets and find a significant reduction of the\nW-spectra for pi^0 as compared to the free nucleon case. On the other hand, the\ncharged pion spectra are only little affected by final state interactions.\nMeasurements of such cross sections with the CLAS detector at JLAB could help\nto improve our understanding of pion rescattering effects and serve as\nimportant/valuable input for calculations of single pion neutrinoproduction on\nheavy targets relevant for current and future long baseline neutrino\nexperiments. Two ratios, in Eq. (3.8) and (3.10), will test important\nproperties of the model.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 12:35:04 GMT\"}]', '2007-05-23', '[[\"Paschos\",\"E. A.\",\"\"],[\"Schienbein\",\"I.\",\"\"],[\"Yu\",\"J. -Y.\",\"\"]]'),
(704.1992, 'Massimiliano Procura', 'Wolfram Weise', 'Yukawa\'s Pion, Low-Energy QCD and Nuclear Chiral Dynamics', '21 pages, 13 figures. Proc. Yukawa-Tomonaga Symposium, Kyoto, Dec.06;\n  to be publ. in Progr. Theor. Phys. Suppl. (Kyoto)', 'Prog.Theor.Phys.Suppl.170:161-184,2007', '10.1143/PTPS.170.161', '', 'nucl-th', '', '  A survey is given of the evolution from Yukawa\'s early work, via the\nunderstanding of the pion as a Nambu-Goldstone boson of spontaneously broken\nchiral symmetry in QCD, to modern developments in the theory of the nucleus\nbased on the chiral effective field theory representing QCD in its low-energy\nlimit.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 16 Apr 2007 12:11:48 GMT\"}]', '2008-11-26', '[[\"Weise\",\"Wolfram\",\"\"]]');
