INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3017, 'Thomas Schaepers', 'I. E. Batov, Th. Schapers, N. M. Chtchelkatchev, H. Hardtdegen, and A.\n  V. Ustinov', 'Andreev reflection and strongly enhanced magnetoresistance oscillations\n  in GaInAs/InP heterostructures with superconducting contacts', '5 pages, 5 figures', '', '10.1103/PhysRevB.76.115313', '', 'cond-mat.mes-hall', '', '  We study the magnetotransport in small hybrid junctions formed by\nhigh-mobility GaInAs/InP heterostructures coupled to superconducting (S) and\nnormal metal (N) terminals. Highly transmissive superconducting contacts to a\ntwo-dimensional electron gas (2DEG) located in a GaInAs/InP heterostructure are\nrealized by using a Au/NbN layer system. The magnetoresistance of the S/2DEG/N\nstructures is studied as a function of dc bias current and temperature. At bias\ncurrents below a critical value, the resistance of the S/2DEG/N structures\ndevelops a strong oscillatory dependence on the magnetic field, with an\namplitude of the oscillations considerably larger than that of the reference\nN/2DEG/N structures. The experimental results are qualitatively explained by\ntaking Andreev reflection in high magnetic fields into account.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 14:25:32 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Apr 2007 10:39:53 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 1 Aug 2007 06:25:41 GMT\"}]', '2009-11-13', '[[\"Batov\",\"I. E.\",\"\"],[\"Schapers\",\"Th.\",\"\"],[\"Chtchelkatchev\",\"N. M.\",\"\"],[\"Hardtdegen\",\"H.\",\"\"],[\"Ustinov\",\"A. V.\",\"\"]]'),
(704.3018, 'Bing Wang', 'Bing Wang', 'On the Conditions to Extend Ricci Flow', '', '', '', '', 'math.DG', '', '  Along a Ricci flow solution on a closed manifold, we show that if Ricci\ncurvature is uniformly bounded from below, then a scalar curvature integral\nbound is enough to extend flow. Moreover, this integral bound condition is\noptimal in some sense.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:52:15 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 23 Apr 2007 20:28:14 GMT\"}]', '2007-05-23', '[[\"Wang\",\"Bing\",\"\"]]'),
(704.3019, 'Oliver Henkel', 'Oliver Henkel', 'Arbitrary Rate Permutation Modulation for the Gaussian Channel', 'to appear in the Proceedings of the International Symposium of\n  Information Theory (ISIT 2007)', '', '', '', 'cs.IT math.IT', '', '  In this paper non-group permutation modulated sequences for the Gaussian\nchannel are considered. Without the restriction to group codes rather than\nsubsets of group codes, arbitrary rates are achievable. The code construction\nutilizes the known optimal group constellations to ensure at least the same\nperformance but exploit the Gray code ordering structure of multiset\npermutations as a selection criterion at the decoder. The decoder achieves near\nmaximum likelihood performance at low computational cost and low additional\nmemory requirements at the receiver.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 14:31:17 GMT\"}]', '2007-07-13', '[[\"Henkel\",\"Oliver\",\"\"]]'),
(704.3020, 'Alessandra Faggionato', 'A. Faggionato', 'Random walks and exclusion processes among random conductances on random\n  infinite clusters: homogenization and hydrodynamic limit', '24 pages. extensions and corrections. new title', '', '', '', 'math.PR math-ph math.MP', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We consider a stationary and ergodic random field {\\omega(b)} parameterized\nby the family of bonds b in Z^d, d>1. The random variable \\omega(b) is thought\nof as the conductance of bond b and it ranges in a finite interval [0,c_0].\nAssuming that the set of bonds with positive conductance has a unique infinite\ncluster C, we prove homogenization results for the random walk among random\nconductances on C. As a byproduct, applying the general criterion of \\cite{F}\nleading to the hydrodynamic limit of exclusion processes with bond-dependent\ntransition rates, for almost all realizations of the environment we prove the\nhydrodynamic limit of simple exclusion processes among random conductances on\nC. The hydrodynamic equation is given by a heat equation whose diffusion matrix\ndoes not depend on the environment. We do not require any ellipticity\ncondition. As special case, C can be the infinite cluster of supercritical\nBernoulli bond percolation.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 14:51:07 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 10 May 2007 07:38:00 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 16 Sep 2008 09:04:51 GMT\"}]', '2008-09-16', '[[\"Faggionato\",\"A.\",\"\"]]'),
(704.3021, 'Gerrit Verschuur Ph.D.', 'Gerrit L. Verschuur', 'On the Critical Ionization Velocity Effect in Interstellar Space and\n  Possible Detection of Related Continuum Emission', 'To be published in IEEE Trans. Plasma Sci. Aug 2007', '', '10.1109/TPS.2007.898037', '', 'astro-ph', '', '  Interstellar neutral hydrogen (HI) emission spectra manifest several families\nof linewidths whose numerical values (34, 13 & 6 km/s) appear to be related to\nthe critical ionization velocities (CIVs) of the most abundant interstellar\natomic species. Extended new analysis of HI emission profiles shows that the 34\nkm/s wide component, probably corresponding to the CIV for helium, is\npervasive. The 34 km/s wide linewidth family is found in low-velocity (local)\nneutral hydrogen (HI) profiles as well as in the so-called high-velocity\nclouds. In addition, published studies of HI linewidths found in the Magellanic\nStream, Very-High-Velocity Clouds, and Compact High-Velocity Clouds, all of\nwhich are believed to be intergalactic, have noted that typical values are of\nthe same order. If the critical ionization velocity effect does play a role in\ninterstellar space it may be expected to produce locally enhanced electron\ndensities where rapidly moving neutral gas masses interact with surrounding\nplasma. Evidence is presented that suggests that this phenomenon is occurring\nin interstellar space. It manifests as a spatial association between peaks in\nHI structure offset with respect to peaks in high-frequency radio continuum\ndata obtained with the Wilkinson Microwave Anisotropy Probe.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 14:59:46 GMT\"}]', '2009-11-13', '[[\"Verschuur\",\"Gerrit L.\",\"\"]]'),
(704.3022, 'Mark Pankov', 'Mark Pankov', 'Order preserving transformations of the Hilbert grassmannian: complex\n  case', '', '', '', '', 'math.FA math.OA', '', '  Let $H$ be a separable complex Hilbert space. Denote by ${\\mathcal\nG}_{\\infty}(H)$ the Grassmannian consisting of closed linear subspaces with\ninfinite dimension and codimension. This Grassmannian is partially ordered by\nthe inclusion relation. We show that every continuous order preserving\nbijective transformation of ${\\mathcal G}_{\\infty}(H)$ is induced by an\ninvertible bounded semi-linear operator.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:03:44 GMT\"}]', '2007-05-23', '[[\"Pankov\",\"Mark\",\"\"]]'),
(704.3023, 'Marc Wagner', 'Marc Wagner', 'Fermions in the pseudoparticle approach', '11 pages, 10 figures', 'Phys.Rev.D76:076002,2007', '10.1103/PhysRevD.76.076002', '', 'hep-lat hep-ph physics.comp-ph', '', '  The pseudoparticle approach is a numerical technique to compute path\nintegrals without discretizing spacetime. The basic idea is to integrate over\nthose field configurations, which can be represented by a sum of a fixed number\nof localized building blocks (pseudoparticles). In a couple of previous papers\nwe have successfully applied the pseudoparticle approach to pure SU(2)\nYang-Mills theory. In this work we discuss how to incorporate fermionic fields\nin the pseudoparticle approach. To test our method, we compute the phase\ndiagram of the 1+1-dimensional Gross-Neveu model in the large-N limit.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:03:48 GMT\"}]', '2007-10-04', '[[\"Wagner\",\"Marc\",\"\"]]'),
(704.3024, 'David Ehrenreich', 'David Ehrenreich (IAP), Arnaud Cassan (ARI)', 'Are extrasolar oceans common throughout the Galaxy?', 'Accepted in Astronomische Nachrichten (Astronomical Notes)', '', '10.1002/asna.200710798', '', 'astro-ph', '', '  Light and cold extrasolar planets such as OGLE 2005-BLG-390Lb, a 5.5\nEarth-mass planet detected via microlensing, could be frequent in the Galaxy\naccording to some preliminary results from microlensing experiments. These\nplanets can be frozen rocky- or ocean-planets, situated beyond the snow line\nand, therefore, beyond the habitable zone of their system. They can nonetheless\nhost a layer of liquid water, heated by radiogenic energy, underneath an ice\nshell surface for billions of years, before freezing completely. These results\nsuggest that oceans under ice, like those suspected to be present on icy moons\nin the Solar system, could be a common feature of cold low-mass extrasolar\nplanets.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:19:39 GMT\"}]', '2009-11-13', '[[\"Ehrenreich\",\"David\",\"\",\"IAP\"],[\"Cassan\",\"Arnaud\",\"\",\"ARI\"]]'),
(704.3025, 'Shintaro Ishiwata', 'S. Ishiwata, I. Terasaki, F. Ishii, N. Nagaosa, H. Mukuda, Y. Kitaoka,\n  T. Saito, and M. Takano', 'Two-Staged Magnetoresistance Driven by Ising-like Spin Sublattice in\n  SrCo6O11', '14 pages, 4 figures, accepted for publication in Phys. Rev. Lett', '', '10.1103/PhysRevLett.98.217201', '', 'cond-mat.str-el', '', '  A two-staged, uniaxial magnetoresistive effect has been discovered in\nSrCo6O11 having a layered hexagonal structure. Conduction electrons and\nlocalized Ising spins are in different sublattices but their interpenetration\nmakes the conduction electrons sensitively pick up the stepwise\nfield-dependence of magnetization. The stepwise field-dependence suggests two\ncompetitive interlayer interactions between ferromagnetic Ising-spin layers,\ni.e., a ferromagnetic nearest-layer interaction and an antiferromagnetic\nnext-nearest-layer interaction. This oxide offers a unique opportunity to study\nnontrivial interplay between conduction electrons and Ising spins, the coupling\nof which can be finely controlled by a magnetic field of a few Tesla.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:16:54 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Apr 2007 05:03:36 GMT\"}]', '2009-11-13', '[[\"Ishiwata\",\"S.\",\"\"],[\"Terasaki\",\"I.\",\"\"],[\"Ishii\",\"F.\",\"\"],[\"Nagaosa\",\"N.\",\"\"],[\"Mukuda\",\"H.\",\"\"],[\"Kitaoka\",\"Y.\",\"\"],[\"Saito\",\"T.\",\"\"],[\"Takano\",\"M.\",\"\"]]'),
(704.3026, 'Kristen McQuinn', 'K. B. W. McQuinn, Charles E. Woodward, S. P. Willner, E. F. Polomski,\n  R. D. Gehrz, Roberta M. Humphreys, Jacco Th. van Loon, M. L. N. Ashby, K.\n  Eicher, and G. G. Fazio', 'The M33 Variable Star Population Revealed by Spitzer', 'Accepted for publication in ApJ. See published article for full\n  resolution figures and electronic tables', 'Astrophys.J.664:850-861,2007', '10.1086/519068', '', 'astro-ph', '', '  We analyze five epochs of Spitzer Space Telescope/Infrared Array Camera\n(IRAC) observations of the nearby spiral galaxy M33. Each epoch covered nearly\na square degree at 3.6, 4.5, and 8.0 microns. The point source catalog from the\nfull dataset contains 37,650 stars. The stars have luminosities characteristic\nof the asymptotic giant branch and can be separated into oxygen-rich and\ncarbon-rich populations by their [3.6] - [4.5] colors. The [3.6] - [8.0] colors\nindicate that over 80% of the stars detected at 8.0 microns have dust shells.\nPhotometric comparison of epochs using conservative criteria yields a catalog\nof 2,923 variable stars. These variables are most likely long-period variables\namidst an evolved stellar population. At least one-third of the identified\ncarbon stars are variable.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:12:33 GMT\"}]', '2009-06-23', '[[\"McQuinn\",\"K. B. W.\",\"\"],[\"Woodward\",\"Charles E.\",\"\"],[\"Willner\",\"S. P.\",\"\"],[\"Polomski\",\"E. F.\",\"\"],[\"Gehrz\",\"R. D.\",\"\"],[\"Humphreys\",\"Roberta M.\",\"\"],[\"van Loon\",\"Jacco Th.\",\"\"],[\"Ashby\",\"M. L. N.\",\"\"],[\"Eicher\",\"K.\",\"\"],[\"Fazio\",\"G. G.\",\"\"]]'),
(704.3027, 'Daniel Burgarth', 'Daniel Burgarth and Vittorio Giovannetti', 'Full control by locally induced relaxation', '4 pages, 2 figures', 'Phys. Rev. Lett. 99, 100501 (2007)', '10.1103/PhysRevLett.99.100501', '', 'quant-ph', '', '  We demonstrate a scheme for controlling a large quantum system by acting on a\nsmall subsystem only. The local control is mediated to the larger system by\nsome fixed coupling Hamiltonian. The scheme allows to transfer arbitrary and\nunknown quantum states from a memory on the large system (``upload access\'\') as\nwell as the inverse (``download access\'\'). We study sufficient conditions of\nthe coupling Hamiltonian and give lower bounds on the fidelities for\ndownloading and uploading.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:17:25 GMT\"}]', '2007-09-05', '[[\"Burgarth\",\"Daniel\",\"\"],[\"Giovannetti\",\"Vittorio\",\"\"]]'),
(704.3028, 'Mario Bessa', 'Mario Bessa and Joao Lopes Dias', 'Generic dynamics of 4-dimensional C2 Hamiltonian systems', '', 'Communications in Mathematical Physics, Vol 281, n{\\deg} 1,\n  597-619, 2008', '10.1007/s00220-008-0500-y', '', 'math.DS', '', '  We study the dynamical behaviour of Hamiltonian flows defined on\n4-dimensional compact symplectic manifolds. We find the existence of a\nC2-residual set of Hamiltonians for which every regular energy surface is\neither Anosov or it is in the closure of energy surfaces with zero Lyapunov\nexponents a.e. This is in the spirit of the Bochi-Mane dichotomy for\narea-preserving diffeomorphisms on compact surfaces and its continuous-time\nversion for 3-dimensional volume-preserving flows.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:19:49 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 21 Jan 2008 19:25:08 GMT\"}]', '2010-10-05', '[[\"Bessa\",\"Mario\",\"\"],[\"Dias\",\"Joao Lopes\",\"\"]]'),
(704.3029, 'Mikhail Voloshin', 'M.B. Voloshin', 'Isospin properties of the X state near the D {\\bar D}^{*} threshold', '10 pages, 1 figure', 'Phys.Rev.D76:014007,2007', '10.1103/PhysRevD.76.014007', 'FTPI-MINN-07/14, UMN-TH-2601/07', 'hep-ph', '', '  The $D {\\bar D}^*$ scattering amplitude and the production of the final\nstates $\\pi^+ \\pi^- J/\\psi$ and $\\pi^+ \\pi^- \\pi^0 J/\\psi$ near the $D^0 {\\bar\nD}^{*0}$ threshold are discussed following the recent suggestion that the\nobserved peaks X(3872) and X(3875) in the decays $B \\to X K$ are due to a\nvirtual state $X$ in the $D^0 {\\bar D}^{*0}$ channel. The strong interaction is\ntreated using the small interaction radius approximation. It is shown that the\nmass difference between the charged and neutral $D^{(*)}$ mesons results in a\ndistinctive behavior of the relevant isotopic amplitudes. In particular, the\nshape of the peak in the $\\pi^+ \\pi^- J/\\psi$ channel should be significantly\nnarrower than in the $\\pi^+ \\pi^- \\pi^0 J/\\psi$ channel, which property can be\nused for an experimental test of the virtual state hypothesis.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:51:41 GMT\"}]', '2008-11-26', '[[\"Voloshin\",\"M. B.\",\"\"]]'),
(704.3030, 'James L. Clem', 'Arlo U. Landolt, Alan K. Uomoto', 'Optical Multicolor Photometry of Spectrophotometric Standard Stars', '76 pages, 48 figures - published version available here:\n  http://www.journals.uchicago.edu/AJ/journal/issues/v133n3/205588/205588.html\n  . Also see ERRATUM at:\n  http://www.journals.uchicago.edu/AJ/journal/issues/v133n5/205838/205838.html', 'Astron.J.133:768-790,2007', '10.1086/510485 10.1086/518002', '', 'astro-ph', '', '  Photoelectric data on the Johnson-Kron-Cousins UBVRI broadband photometric\nsystem are provided for a set of stars which have been used as\nspectrophotometric standard stars at the Hubble Space Telescope.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:26:43 GMT\"}]', '2010-11-05', '[[\"Landolt\",\"Arlo U.\",\"\"],[\"Uomoto\",\"Alan K.\",\"\"]]'),
(704.3031, 'Simon Radford', 'Simon J. E. Radford, Riccardo Giovanelli, Thomas A. Sebring, Jonas\n  Zmuidzinas', 'The Cornell Caltech Atacama Telescope', '18th International Symposium on Space Terahertz Technology', '', '', '', 'astro-ph', '', '  Cornell University, the California Institute for Technology, and the Jet\nPropulsion Laboratory are jointly studying the construction of a 25 m diameter\ntelescope for submillimeter astronomy on a high mountain in northern Chile.\nThis Cornell Caltech Atacama Telescope (CCAT) will combine high sensitivity, a\nwide field of view, and a broad wavelength range to provide an unprecedented\ncapability for deep, large area, multi-color submillimeter surveys to\ncomplement narrow field, high resolution studies with ALMA. CCAT observations\nwill address fundamental themes in contemporary astronomy, notably the\nformation and evolution of galaxies, the nature of the dark matter and dark\nenergy that comprise most of the content of the universe, the formation of\nstars and planets, the conditions in circumstellar disks, and the conditions\nduring the early history of the Solar system. The candidate CCAT site, at 5600\nm in northern Chile, enjoys superb observing conditions. To accommodate large\nformat bolometer cameras, CCAT is designed with a 20 arcmin field of view. CCAT\nwill incorporate closed loop active control of its segmented primary mirror to\nmaintain a half wavefront error of 10 mum rms or less. Instrumentation under\nconsideration includes both short (650 mum-200 mum) and long (2 mm-750 mum)\nwavelength bolometer cameras, direct detection spectrometers, and heterodyne\nreceiver arrays. The University of Colorado, a Canadian university consortium,\nand the UK Astronomy Technology Centre on behalf of the UK community are\npursuing participation in the CCAT consortium. When complete early in the next\ndecade, CCAT will be the largest and most sensitive facility of its class as\nwell as the highest altitude astronomical facility on Earth.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:48:03 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 23:40:02 GMT\"}]', '2007-05-23', '[[\"Radford\",\"Simon J. E.\",\"\"],[\"Giovanelli\",\"Riccardo\",\"\"],[\"Sebring\",\"Thomas A.\",\"\"],[\"Zmuidzinas\",\"Jonas\",\"\"]]'),
(704.3032, 'Zolt\\\'an Nagy', 'Nenad Manojlovic and Zoltan Nagy', 'Algebraic Bethe ansatz for the elliptic quantum group\n  $E_{\\tau,\\eta}(A_2^{(2)})$', '15 pages; v2: minor corrections. A reference is added, a more precise\n  abstract is written, a section title is changed and typos are corrected', 'Journal of Mathematical Physics 48, 123515 (2007)', '10.1063/1.2823974', '', 'math.QA math-ph math.MP nlin.SI', '', '  We implement the Bethe anstaz method for the elliptic quantum group\n$E_{\\tau,\\eta}(A_2^{(2)})$. The Bethe creation operators are constructed as\npolynomials of the Lax matrix elements expressed through a recurrence relation.\nWe also give the eigenvalues of the family of commuting transfer matrices\ndefined in the tensor product of fundamental representations.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:51:15 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 27 Apr 2007 15:28:01 GMT\"}]', '2009-11-13', '[[\"Manojlovic\",\"Nenad\",\"\"],[\"Nagy\",\"Zoltan\",\"\"]]'),
(704.3033, 'Satoshi Miyashita', 'Satoshi Miyashita and Kenji Yonemitsu', 'Charge ordering in \\theta-(BEDT-TTF)2RbZn(SCN)4: Cooperative effects of\n  electron correlations and lattice distortions', '7 peges, 7 figures, accepted for publication in Phys. Rev. B', '', '10.1103/PhysRevB.75.245112', '', 'cond-mat.str-el', '', '  Combined effects of electron correlations and lattice distortions are\ninvestigated on the charge ordering in \\theta-(BEDT-TTF)2RbZn(SCN)4\ntheoretically in a two-dimensional 3/4-filled extended Hubbard model with\nelectron-lattice couplings. It is known that this material undergoes a phase\ntransition from a high-symmetry metallic state to a low-symmetry insulating\nstate with a horizontal-stripe charge order (CO) by lowering temperature. By\nmeans of the exact-diagonalization method, we show that electron-phonon\ninteractions are crucial to stabilize the horizontal-stripe CO and to realize\nthe low-symmetry crystal structure.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:45:21 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 23 Apr 2007 20:11:09 GMT\"}]', '2009-11-13', '[[\"Miyashita\",\"Satoshi\",\"\"],[\"Yonemitsu\",\"Kenji\",\"\"]]'),
(704.3034, 'James L. Clem', 'Arlo U. Landolt', 'UBVRI Photometric Standard Stars Around the Sky at -50 Degrees\n  Declination', '80 pages, 57 figures - published version available here:\n  http://www.journals.uchicago.edu/AJ/journal/issues/v133n6/205795/205795.html', 'Astron.J.133:2502-2523,2007', '10.1086/518000', '', 'astro-ph', '', '  UBVRI photoelectric observations have been made of 109 stars around the sky,\ncentered more or less at -50 degrees declination. The majority of the stars\nfall in the magnitude range 10.4 < V < 15.5 and in the color index range -0.33\n< (B - V) < +1.66. These new broadband photometric standard stars average 16.4\nmeasurements each from data taken on 116 different nights over a period of 4\nyr. Similar data are tabulated for 19 stars of interest that were not observed\noften enough to make them well-defined standard stars.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:50:15 GMT\"}]', '2010-11-05', '[[\"Landolt\",\"Arlo U.\",\"\"]]'),
(704.3035, 'Ender Tekin', 'Ender Tekin, Aylin Yener', 'Achievable Rates for Two-Way Wire-Tap Channels', 'International Symposium on Information Theory (ISIT) 2007, June 24-29', '', '', '', 'cs.IT cs.CR math.IT', '', '  We consider two-way wire-tap channels, where two users are communicating with\neach other in the presence of an eavesdropper, who has access to the\ncommunications through a multiple-access channel. We find achievable rates for\ntwo different scenarios, the Gaussian two-way wire-tap channel, (GTW-WT), and\nthe binary additive two-way wire-tap channel, (BATW-WT). It is shown that the\ntwo-way channels inherently provide a unique advantage for wire-tapped\nscenarios, as the users know their own transmitted signals and in effect help\nencrypt the other user\'s messages, similar to a one-time pad. We compare the\nachievable rates to that of the Gaussian multiple-access wire-tap channel\n(GMAC-WT) to illustrate this advantage.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:26:59 GMT\"}]', '2007-07-13', '[[\"Tekin\",\"Ender\",\"\"],[\"Yener\",\"Aylin\",\"\"]]'),
(704.3036, 'Stefaan Caenepeel', 'D. Bulacu, S. Caenepeel, B. Torrecillas', 'Involutory quasi-Hopf algebras', '26 pages', '', '', '', 'math.QA', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We introduce and investigate the basic properties of an involutory (dual)\nquasi-Hopf algebra. We also study the representations of an involutory\nquasi-Hopf algebra and prove that an involutory dual quasi-Hopf algebra with\nnon-zero integral is cosemisimple.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:51:32 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 9 Dec 2008 13:52:26 GMT\"}]', '2008-12-09', '[[\"Bulacu\",\"D.\",\"\"],[\"Caenepeel\",\"S.\",\"\"],[\"Torrecillas\",\"B.\",\"\"]]'),
(704.3037, 'Cristobal Lopez', 'Stefano Berti, Cristobal Lopez, Davide Vergni and Angelo Vulpiani', 'Discreteness effects in a reacting system of particles with finite\n  interaction radius', '23 pages, 13 figures', '', '10.1103/PhysRevE.76.031139', '', 'cond-mat.stat-mech', '', '  An autocatalytic reacting system with particles interacting at a finite\ndistance is studied. We investigate the effects of the discrete-particle\ncharacter of the model on properties like reaction rate, quenching phenomenon\nand front propagation, focusing on differences with respect to the continuous\ncase. We introduce a renormalized reaction rate depending both on the\ninteraction radius and the particle density, and we relate it to macroscopic\nobservables (e.g., front speed and front thickness) of the system.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:52:15 GMT\"}]', '2009-11-13', '[[\"Berti\",\"Stefano\",\"\"],[\"Lopez\",\"Cristobal\",\"\"],[\"Vergni\",\"Davide\",\"\"],[\"Vulpiani\",\"Angelo\",\"\"]]'),
(704.3038, 'Claudia Wigger', 'C. Wigger, W. Hajdas, A. Zehnder, K. Hurley, E. Bellm, S. Boggs, M.\n  Bandstra, D.M. Smith', 'Spectral Analysis of GRBs Measured by RHESSI', '4 pages, 4 figures, conference proceedings, \'Swift and GRBs:\n  Unveiling the Relativistic Universe\', San Servolo, Venice, 5-9 June 2006, to\n  appear in Il Nouvo Cimento', 'Nuovo Cim.B121:1117-1121,2006', '10.1393/ncb/i2007-10072-9', '', 'astro-ph', '', '  The Ge spectrometer of the RHESSI satellite is sensitive to Gamma Ray Bursts\n(GRBs) from about 40 keV up to 17 MeV, thus ideally complementing the Swift/BAT\ninstrument whose sensitivity decreases above 150 keV. We present preliminary\nresults of spectral fits of RHESSI GRB data. After describing our method, the\nRHESSI results are discussed and compared with Swift and Konus.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 15:53:53 GMT\"}]', '2010-11-11', '[[\"Wigger\",\"C.\",\"\"],[\"Hajdas\",\"W.\",\"\"],[\"Zehnder\",\"A.\",\"\"],[\"Hurley\",\"K.\",\"\"],[\"Bellm\",\"E.\",\"\"],[\"Boggs\",\"S.\",\"\"],[\"Bandstra\",\"M.\",\"\"],[\"Smith\",\"D. M.\",\"\"]]'),
(704.3039, 'Alain Corfdir', 'Alain Corfdir (ENPC-Cermes)', 'Yield design for porous media subjected to unconfined flow: construction\n  of approximate pressure fields', '', 'Comptes Rendus M\\\'ecanique 334, 3 (2006) 183-189', '10.116/j.crme.2006.011', '', 'physics.class-ph', '', '  We consider the stability of a porous medium submitted to a steady-state flow\nwith free-boundary. Assuming some hypotheses, it is possible to implement the\nkinematic method by using an approximate pressure field bounding the true\npressure field from below. We are interested in finding such approximate\npressure fields and in proving that they bound the true pressure field from\nbelow without knowing the true pressure field. We use fields which are\nsolutions of a problem with relaxed conditions with regard to the real problem.\nUnder a uniqueness condition of the solution of a weak formulation of the\nproblem, such fields are lower bounds for the true pressure field. Finally, we\ngive the example of a vertical dam.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:01:28 GMT\"}]', '2007-05-23', '[[\"Corfdir\",\"Alain\",\"\",\"ENPC-Cermes\"]]'),
(704.3040, 'Ari Pakman', 'Ari Pakman and Amit Sever', 'Exact N=4 correlators of AdS(3)/CFT(2)', '3 pages. v2:minor changes', 'Phys.Lett.B652:60-62,2007', '10.1016/j.physletb.2007.06.041', 'YITP-SB-07-15, BRX-TH-587', 'hep-th', '', '  We extend to chiral N=4 operators the holographic agreement recently found\nbetween correlators of the symmetric orbifold of M^4 at large N and type IIB\nstrings propagating in AdS(3) x S^3 x M^4, where M^4=T^4 or K3. We also present\nexpressions for some bulk correlators not yet computed in the boundary.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:24:11 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Apr 2007 19:50:29 GMT\"}]', '2008-11-26', '[[\"Pakman\",\"Ari\",\"\"],[\"Sever\",\"Amit\",\"\"]]'),
(704.3041, 'Natalia Tristan', 'E.A. Popova, D.V. Volkov, A.N. Vasiliev, A.A. Demidov, N.P. Kolmakova,\n  I.A. Gudim, L.N. Bezmaternykh, N. Tristan, Yu. Skourski, B. B\\\"uchner, C.\n  Hess, R. Klingeler', 'Magnetization and specific heat of TbFe3(BO3)4: Experiment and crystal\n  field calculations', '10 pages, 10 figures, 20 references, accepted by Phys. Rev. B', '', '10.1103/PhysRevB.75.224413', '', 'cond-mat.other', '', '  We have studied the thermodynamic properties of single-crystalline\nTbFe3(BO3)4. Magnetization measurements have been carried out as a function of\nmagnetic field (up to 50 T) and temperature up to 350K with the magnetic field\nboth parallel and perpendicular to the trigonal c-axis of the crystal. The\nspecific heat has been measured in the temperature range 2-300K with a magnetic\nfield up to 9 T applied parallel to the c-axis. The data indicate a structural\nphase transition at 192 K and antiferromagnetic spin ordering at 40 K. A\nSchottky anomaly is present in the specific heat data around 20 K, arising due\nto two low-lying energy levels of the Tb3+ ions being split by f-d coupling.\nBelow TN magnetic fields parallel to the c-axis drive a spin-flop phase\ntransition, which is associated with a large magnetization jump. The highly\nanisotropic character of the magnetic susceptibility is ascribed mainly to the\nIsing-like behavior of the Tb3+ ions in the trigonal crystal field. We describe\nour results in the framework of an unified approach which is based on\nmean-field approximation and crystal-field calculations.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:05:27 GMT\"}]', '2009-11-13', '[[\"Popova\",\"E. A.\",\"\"],[\"Volkov\",\"D. V.\",\"\"],[\"Vasiliev\",\"A. N.\",\"\"],[\"Demidov\",\"A. A.\",\"\"],[\"Kolmakova\",\"N. P.\",\"\"],[\"Gudim\",\"I. A.\",\"\"],[\"Bezmaternykh\",\"L. N.\",\"\"],[\"Tristan\",\"N.\",\"\"],[\"Skourski\",\"Yu.\",\"\"],[\"Büchner\",\"B.\",\"\"],[\"Hess\",\"C.\",\"\"],[\"Klingeler\",\"R.\",\"\"]]'),
(704.3042, 'Yeongduk Kim', 'W.G. Kang, Y.D. Kim, J.I. Lee, I.S. Hahn, A.R. Kim, H.J. Kim', 'Measurement on the thermal neutron capture cross section of w-180', '10 pages, 4 figures', 'Phys.Rev.C76:067602,2007', '10.1103/PhysRevC.76.067602', '', 'nucl-ex', '', '  We have measured the thermal neutron capture cross section for w-180 nucleus.\nThere is only one previous data on this cross section with a value of 30\n$^{+300%}_{-100%}$ barn. To consider w-181 as a low energy neutrino source, the\nthermal neutron capture cross section should be measured more precisely to\nestimate the production rate of w-181 inside a nuclear reactor. We measured the\ncross section of w-180 with a natural tungsten foil and obtained a new value of\n21.9 $\\pm$ 2.5 barn\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:14:50 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Apr 2007 03:40:35 GMT\"}]', '2008-11-26', '[[\"Kang\",\"W. G.\",\"\"],[\"Kim\",\"Y. D.\",\"\"],[\"Lee\",\"J. I.\",\"\"],[\"Hahn\",\"I. S.\",\"\"],[\"Kim\",\"A. R.\",\"\"],[\"Kim\",\"H. J.\",\"\"]]'),
(704.3043, 'Jailson Alcaniz', 'F.C. Carvalho (on), J.S. Alcaniz (on), J.A.S. Lima (USP), R. Silva\n  (UERN)', 'CMB and LSS constraints on a single-field model of inflation', '5 pages, 4 figures, LaTeX', 'Europhys.Lett.83:29001,2008', '10.1209/0295-5075/83/29001', '', 'astro-ph gr-qc hep-th', '', '  A new inflationary scenario whose exponential potential $V(\\Phi)$ has a\nquadratic dependence on the field $\\Phi$ in addition to the standard linear\nterm is confronted with the tree-year observations of the Wilkinson-Microwave\nAnisotropy Probe and the Sloan Digital Sky Survey data. The number of e-folds\n($N$), the ratio of tensor-to-scalar perturbations ($r$), the spectral scalar\nindex of the primordial power spectrum ($n_s$) and its running ($dn_s/d\\ln k$)\ndepend on the dimensionless parameter $\\alpha$ multiplying the quadratic term\nin the potential. In the limit $\\alpha \\to 0$ all the results of the standard\nexponential potential are fully recovered. For values of $\\alpha \\neq 0$, we\nfind that the model predictions are in good agreement with the current\nobservations of the Cosmic Microwave Background (CMB) anisotropies and\nLarge-Scale Structure (LSS) in the Universe.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:15:21 GMT\"}]', '2009-06-23', '[[\"Carvalho\",\"F. C.\",\"\",\"on\"],[\"Alcaniz\",\"J. S.\",\"\",\"on\"],[\"Lima\",\"J. A. S.\",\"\",\"USP\"],[\"Silva\",\"R.\",\"\",\"UERN\"]]'),
(704.3044, 'Pasquale Dario Serpico', 'Alessandro Mirizzi, Georg G. Raffelt, and Pasquale D. Serpico', 'Signatures of axion-like particles in the spectra of TeV gamma-ray\n  sources', '8 pages, 1 eps figure; typos corrected, matches published version', 'Phys.Rev.D76:023001,2007', '10.1103/PhysRevD.76.023001', 'FERMILAB-PUB-07-082-A, MPP-2007-44', 'astro-ph hep-ph', '', '  One interpretation of the unexplained signature observed in the PVLAS\nexperiment invokes a new axion-like particle (ALP) with a two-photon vertex,\nallowing for photon-ALP oscillations in the presence of magnetic fields. In the\nrange of masses and couplings suggested by PVLAS, the same effect would lead to\na peculiar dimming of high-energy photon sources. For typical parameters of the\nturbulent magnetic field in the galaxy, the effect sets in at E_gamma >~ 10\nTeV, providing an ALP signature in the spectra of TeV gamma sources that can be\nprobed with Cherenkov telescopes. A dedicated search will be strongly motivated\nif the ongoing photon regeneration experiments confirm the PVLAS particle\ninterpretation.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:16:28 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 13 Jul 2007 15:32:04 GMT\"}]', '2008-11-26', '[[\"Mirizzi\",\"Alessandro\",\"\"],[\"Raffelt\",\"Georg G.\",\"\"],[\"Serpico\",\"Pasquale D.\",\"\"]]'),
(704.3045, 'Igor Strakovsky', 'Ya. Azimov (PNPI), K. Goeke (Ruhr-Universitaet), I. Strakovsky (GWU)', 'A possible explanation why the Theta+ is seen in some experiments and\n  not in others', '18 pages. Some changes in the text; experimental suggestions\n  collected in a special subsection, references added and refreshed', '', '10.1103/PhysRevD.76.074013', '', 'hep-ph hep-ex nucl-ex nucl-th', '', '  To understand the whole set of positive and null data on the\nTheta+(1530)-production, we suggest the hypothesis that multiquark hadrons are\nmainly generated from many-quark states, which emerge either as short-term\nhadron fluctuations, or as hadron remnants in hard processes. This approach\nallows us to describe both non-observation of the Theta+ in current null\nexperiments and peculiar features of its production in positive experiments.\nFurther, we are able to propose new experiments that might be decisive for the\nproblem of the Theta+ existence. Distributions of the Theta+ in such\nexperiments can give important information both on higher Fock components of\nconventional hadrons and about structure and hadronization properties of hadron\nremnants produced in hard processes. We also explain that description of\nmultiquark hadrons may require a modified form of the constituent quark model,\nwith quark masses and couplings being intermediate between their values for the\nfamiliar constituent quarks and the current ones.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:27:42 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 15 Jun 2007 20:25:34 GMT\"}]', '2013-05-29', '[[\"Azimov\",\"Ya.\",\"\",\"PNPI\"],[\"Goeke\",\"K.\",\"\",\"Ruhr-Universitaet\"],[\"Strakovsky\",\"I.\",\"\",\"GWU\"]]'),
(704.3046, 'Artemio Gonzalez-Lopez', 'A. Enciso, F. Finkel, A. Gonzalez-Lopez, M.A. Rodriguez', 'A novel quasi-exactly solvable spin chain with nearest-neighbors\n  interactions', '38 pages, 8 figures', 'Nucl.Phys.B789:452-482,2008', '10.1016/j.nuclphysb.2007.07.001', '', 'hep-th cond-mat.other math-ph math.MP', '', '  In this paper we study a novel spin chain with nearest-neighbors interactions\ndepending on the sites coordinates, which in some sense is intermediate between\nthe Heisenberg chain and the spin chains of Haldane-Shastry type. We show that\nwhen the number of spins is sufficiently large both the density of sites and\nthe strength of the interaction between consecutive spins follow the Gaussian\nlaw. We develop an extension of the standard freezing trick argument that\nenables us to exactly compute a certain number of eigenvalues and their\ncorresponding eigenfunctions. The eigenvalues thus computed are all integers,\nand in fact our numerical studies evidence that these are the only integer\neigenvalues of the chain under consideration. This fact suggests that this\nchain can be regarded as a finite-dimensional analog of the class of\nquasi-exactly solvable Schroedinger operators, which has been extensively\nstudied in the last two decades. We have applied the method of moments to study\nsome statistical properties of the chain\'s spectrum, showing in particular that\nthe density of eigenvalues follows a Wigner-like law. Finally, we emphasize\nthat, unlike the original freezing trick, the extension thereof developed in\nthis paper can be applied to spin chains whose associated dynamical spin model\nis only quasi-exactly solvable.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:37:14 GMT\"}]', '2008-11-26', '[[\"Enciso\",\"A.\",\"\"],[\"Finkel\",\"F.\",\"\"],[\"Gonzalez-Lopez\",\"A.\",\"\"],[\"Rodriguez\",\"M. A.\",\"\"]]'),
(704.3047, 'Aurelien Perrin', 'A. Perrin (LCFIO), H. Chang (LCFIO), V. Krachmalnicoff (LCFIO), M.\n  Schellekens (LCFIO), D. Boiron (LCFIO), A. Aspect (LCFIO), C. I. Westbrook\n  (LCFIO)', 'Observation of atom pairs in spontaneous four wave mixing of two\n  colliding Bose-Einstein Condensates', 'A few typos have been corrected', 'Physical Review Letters 99, 15 (2007) 150405', '10.1103/PhysRevLett.99.150405', '', 'quant-ph cond-mat.other', '', '  We study atom scattering from two colliding Bose-Einstein condensates using a\nposition sensitive, time resolved, single atom detector. In analogy to quantum\noptics, the process can also be thought of as spontaneous, degenerate four wave\nmixing of de Broglie waves. We find a clear correlation between atoms with\nopposite momenta, demonstrating pair production in the scattering process. We\nalso observe a Hanbury Brown and Twiss correlation for collinear momenta, which\npermits an independent measurement of the size of the pair production source\nand thus the size of the spatial mode. The back to back pairs occupy very\nnearly two oppositely directed spatial modes, a promising feature for future\nquantum optics experiments.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:31:05 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 1 Oct 2007 12:56:36 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 11 Oct 2007 08:28:37 GMT\"},{\"version\":\"v4\",\"created\":\"Mon, 12 May 2008 19:39:59 GMT\"}]', '2008-05-12', '[[\"Perrin\",\"A.\",\"\",\"LCFIO\"],[\"Chang\",\"H.\",\"\",\"LCFIO\"],[\"Krachmalnicoff\",\"V.\",\"\",\"LCFIO\"],[\"Schellekens\",\"M.\",\"\",\"LCFIO\"],[\"Boiron\",\"D.\",\"\",\"LCFIO\"],[\"Aspect\",\"A.\",\"\",\"LCFIO\"],[\"Westbrook\",\"C. I.\",\"\",\"LCFIO\"]]'),
(704.3048, 'V. Nefer \\c{S}eno\\u{g}uz', 'V. Nefer Senoguz', 'Non-thermal leptogenesis with strongly hierarchical right handed\n  neutrinos', '7 pages, 5 figures. v2: added some comments and references, v3: minor\n  corrections and additions, v4: a typo corrected, published version', 'Phys.Rev.D76:013005,2007', '10.1103/PhysRevD.76.013005', '', 'hep-ph', '', '  Assuming the Dirac-type neutrino masses m_D are related to quark or charged\nlepton masses, neutrino oscillation data indicate that right handed neutrino\nmasses are in general strongly hierarchical. In particular, if m_D is similar\nto the up-type quark masses, the mass of the lightest right handed neutrino\nM_1<~10^6 GeV. We show that non-thermal leptogenesis by inflaton decay can\nyield sufficient baryon asymmetry despite this constraint, and discuss how the\nasymmetry is correlated with the low energy neutrino masses and CP-violating\nphases.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 16:47:04 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 27 Apr 2007 20:33:20 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 19 Jun 2007 21:44:03 GMT\"},{\"version\":\"v4\",\"created\":\"Wed, 25 Jul 2007 15:57:31 GMT\"}]', '2008-11-26', '[[\"Senoguz\",\"V. Nefer\",\"\"]]'),
(704.3049, 'Ryan Gutenkunst', 'Ryan N. Gutenkunst, Fergal P. Casey, Joshua J. Waterfall, Christopher\n  R. Myers, James P. Sethna', 'Extracting falsifiable predictions from sloppy models', '4 pages, 2 figures. Submitted to the Annals of the New York Academy\n  of Sciences for publication in \"Reverse Engineering Biological Networks:\n  Opportunities and Challenges in Computational Methods for Pathway Inference\"', 'Annals of the New York Academy of Sciences 1115:203-211 (2007)', '10.1196/annals.1407.003', '', 'q-bio.QM', '', '  Successful predictions are among the most compelling validations of any\nmodel. Extracting falsifiable predictions from nonlinear multiparameter models\nis complicated by the fact that such models are commonly sloppy, possessing\nsensitivities to different parameter combinations that range over many decades.\nHere we discuss how sloppiness affects the sorts of data that best constrain\nmodel predictions, makes linear uncertainty approximations dangerous, and\nintroduces computational difficulties in Monte-Carlo uncertainty analysis. We\nalso present a useful test problem and suggest refinements to the standards by\nwhich models are communicated.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 17:00:09 GMT\"}]', '2007-11-24', '[[\"Gutenkunst\",\"Ryan N.\",\"\"],[\"Casey\",\"Fergal P.\",\"\"],[\"Waterfall\",\"Joshua J.\",\"\"],[\"Myers\",\"Christopher R.\",\"\"],[\"Sethna\",\"James P.\",\"\"]]'),
(704.3050, 'M. B. N. Kouwenhoven', 'M.B.N. Kouwenhoven (1,2,3), M. Bureau (4), S. Kim (5), P.T. de Zeeuw\n  (2) ((1) University of Sheffield (2) Leiden University (3) University of\n  Amsterdam (4) University of Oxford (5) Sejong University)', 'Optical BVI Imaging and HI Synthesis Observations of the Dwarf Irregular\n  Galaxy ESO 364-G 029', '10 pages, 11 figures, accepted by A&A', '', '10.1051/0004-6361:20077531', '', 'astro-ph', '', '  As part of an effort to enlarge the number of well-studied Magellanic-type\ngalaxies, we obtained broadband optical imaging and neutral hydrogen radio\nsynthesis observations of the dwarf irregular galaxy ESO 364-G 029. The optical\nmorphology characteristically shows a bar-like main body with a one-sided\nspiral arm, an approximately exponential light distribution, and offset\nphotometric and kinematic centers. The HI distribution is mildly asymmetric\nand, although slightly offset from the photometric center, roughly follows the\noptical brightness distribution, extending to over 1.2 Holmberg radii (where\nmu_B = 26.5 mag/arcsec^2). In particular, the highest HI column densities\nclosely follow the bar, one-arm spiral, and a third optical extension. The\nrotation is solid-body in the inner parts but flattens outside of the optical\nextent. The total HI flux F_HI = 23.1 pm 1.2 Jy km/s, yielding a total HI mass\nM_HI= (6.4 pm 1.7) x 10^8 Msun (for a distance D = 10.8 pm 1.4 Mpc) and a total\nHI mass-to-blue-luminosity ratio M_HI/L_B = (0.96 pm 0.14) Msun / Lsun,B\n(distance independent). The HI data suggest a very complex small-scale HI\nstructure, with evidence of large shells and/or holes, but deeper observations\nare required for a detailed study. Follow-up observations are also desirable\nfor a proper comparison with the Large Magellanic Cloud, where despite an\noptical morphology very similar to ESO 364-G 029 the HI bears little\nresemblance to the optical.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 17:36:57 GMT\"}]', '2009-11-13', '[[\"Kouwenhoven\",\"M. B. N.\",\"\"],[\"Bureau\",\"M.\",\"\"],[\"Kim\",\"S.\",\"\"],[\"de Zeeuw\",\"P. T.\",\"\"]]'),
(704.3051, 'Stephane Toulin', 'Jalil Ouazzani (ICMCB), Yves Garrabos (ICMCB)', 'A new numerical algorithm for Low Mach number supercritical fluids', '', '', '', '', 'physics.class-ph', '', '  A new algorithm has been developed to compute low Mach Numbers supercritical\nfluid flows. The algorithm is applied using a finite volume method based on the\nSIMPLER algorithm. Its main advantages are to decrease significantly the CPU\ntime, and the possibility for supercritical fluid flow modelisation to use\nother discretisation methods (such as spectral methods and/or finite\ndifferences) and other algorithms such as PISO or projection. It makes it\npossible to solve 3D problems within reasonable CPU time even when considering\ncomplex equations of state. The algorithm is given after first a brief\ndescription of the previously existing algorithm to solve for supercritical\nfluids. The side and bottom heated near critical carbon dioxide filled cavity\nproblems are respectively solved and compared to the previously obtained\nresults.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:14:40 GMT\"}]', '2007-08-21', '[[\"Ouazzani\",\"Jalil\",\"\",\"ICMCB\"],[\"Garrabos\",\"Yves\",\"\",\"ICMCB\"]]'),
(704.3052, 'Kerry Soileau', 'Kerry M. Soileau', 'Representation Of Level Paths Of An Analytic Function', '', '', '', '', 'math.GM', '', '  We find an arc-parameterization of the contour on which an given analytic\nfunction has constant modulus. This contour is seen to satisfy a differential\nequation which we explicitly give.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:15:07 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 27 Apr 2007 15:52:34 GMT\"}]', '2007-05-23', '[[\"Soileau\",\"Kerry M.\",\"\"]]'),
(704.3053, 'Braito Valentina', 'R. M. Sambruna (1), J. N. Reeves (1, 2), V. Braito (1,3) ((1) NASA\n  GSFC, (2) Astrophysics Group, School of Physical and Geographical Sciences,\n  Keele University, (3) JHU)', 'The remarkable X-ray spectrum of the Broad-Line Radio Galaxy 3C 445', '32 pages, 3 figures, 2 tables, accepted for publication in ApJ', 'Astrophys.J.665:1030-1037,2007', '10.1086/519306', '', 'astro-ph', '', '  We present the results of the analysis of an archival 15 ks XMM-Newton\nobservation of the nearby (z=0.057) radio-loud source 3C445, optically\nclassified as a Broad-Line Radio Galaxy. While the RGS data are of insufficient\nquality to allow a meaningful analysis, the EPIC data show a remarkable X-ray\nspectrum. The 2-10 keV continuum is described by a heavily absorbed (Nh~ 1e22 -\n1e23 cm-2) power law with photon index Gamma ~1.4, and strong (R~2) cold\nreflection. A narrow, unresolved Fe Kalpha emission line is detected,\nconfirming previous findings, with EW 120eV. A soft excess is present below 2\nkeV over the extrapolation of the hard X-ray power law, which we model with a\npower law with the same photon index as the hard power law, absorbed by a\ncolumn density Nh=6e20 cm-2 in excess to Galactic. A host of emission lines are\npresent below 2 keV, confirming previous indications from ASCA, due to H- and\nHe-like O, Mg, and Si. We attribute the origin of the lines to a photoionized\ngas, with properties very similar to radio-quiet obscured AGN. Two different\nionized media, or a single stratified medium, are required to fit the soft\nX-ray data satisfactorily. The similarity of the X-ray spectrum of 3C445 to\nSeyferts underscores that the central engines of radio-loud and radio-quiet AGN\nsimilarly host both cold and warm gas.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:17:56 GMT\"}]', '2009-06-23', '[[\"Sambruna\",\"R. M.\",\"\"],[\"Reeves\",\"J. N.\",\"\"],[\"Braito\",\"V.\",\"\"]]'),
(704.3054, 'Peter Parker', 'Peter A. Parker, Patrick Mitran, Daniel W. Bliss, and Vahid Tarokh', 'On bounds and algorithms for frequency synchronization for collaborative\n  communication systems', 'Submitted to IEEE Transaction on Signal Processing', '', '10.1109/TSP.2008.924799', '', 'stat.AP math.ST stat.TH', '', '  Cooperative diversity systems are wireless communication systems designed to\nexploit cooperation among users to mitigate the effects of multipath fading. In\nfairly general conditions, it has been shown that these systems can achieve the\ndiversity order of an equivalent MISO channel and, if the node geometry\npermits, virtually the same outage probability can be achieved as that of the\nequivalent MISO channel for a wide range of applicable SNR. However, much of\nthe prior analysis has been performed under the assumption of perfect timing\nand frequency offset synchronization. In this paper, we derive the estimation\nbounds and associated maximum likelihood estimators for frequency offset\nestimation in a cooperative communication system. We show the benefit of\nadaptively tuning the frequency of the relay node in order to reduce estimation\nerror at the destination. We also derive an efficient estimation algorithm,\nbased on the correlation sequence of the data, which has mean squared error\nclose to the Cramer-Rao Bound.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:08:46 GMT\"}]', '2009-11-13', '[[\"Parker\",\"Peter A.\",\"\"],[\"Mitran\",\"Patrick\",\"\"],[\"Bliss\",\"Daniel W.\",\"\"],[\"Tarokh\",\"Vahid\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3055, 'Maurice Kleman', 'Maurice Kleman, Jacques Friedel', 'Disclinations, dislocations and continuous defects: a reappraisal', '72 pages, 36 figures', 'Rev. Mod. Phys. January-March 2008, 80, 61-115', '10.1103/RevModPhys.80.61', '', 'cond-mat.soft', '', '  Disclinations, first observed in mesomorphic phases, are relevant to a number\nof ill-ordered condensed matter media, with continuous symmetries or frustrated\norder. They also appear in polycrystals at the edges of grain boundaries. They\nare of limited interest in solid single crystals, where, owing to their large\nelastic stresses, they mostly appear in close pairs of opposite signs. The\nrelaxation mechanisms associated with a disclination in its creation, motion,\nchange of shape, involve an interplay with continuous or quantized dislocations\nand/or continuous disclinations. These are attached to the disclinations or are\nakin to Nye\'s dislocation densities, well suited here. The notion of \'extended\nVolterra process\' takes these relaxation processes into account and covers\ndifferent situations where this interplay takes place. These concepts are\nillustrated by applications in amorphous solids, mesomorphic phases and\nfrustrated media in their curved habit space. The powerful topological theory\nof line defects only considers defects stable against relaxation processes\ncompatible with the structure considered. It can be seen as a simplified case\nof the approach considered here, well suited for media of high plasticity\nor/and complex structures. Topological stability cannot guarantee energetic\nstability and sometimes cannot distinguish finer details of structure of\ndefects.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:30:04 GMT\"}]', '2009-11-13', '[[\"Kleman\",\"Maurice\",\"\"],[\"Friedel\",\"Jacques\",\"\"]]'),
(704.3056, 'Michael Hartmann Mr', 'Michael J. Hartmann, Fernando G.S.L. Brandao and Martin B. Plenio', 'Effective spin systems in coupled micro-cavities', '5 pages, 4 figures', 'Phys. Rev. Lett. 99, 160501 (2007)', '10.1103/PhysRevLett.99.160501', '', 'quant-ph cond-mat.other', '', '  We show that atoms trapped in micro-cavities that interact via exchange of\nvirtual photons can model an anisotropic Heisenberg spin-1/2 chain in an\nexternal magnetic field. All parameters of the effective Hamiltonian can\nindividually be tuned via external lasers. Since the occupation of excited\natomic levels and photonic states are strongly suppressed, the effective model\nis robust against decoherence mechanisms, has a long lifetime and its\nimplementation is feasible with current experimental technology. The model\nprovides a feasible way to create cluster states in these devices.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:31:42 GMT\"}]', '2009-11-13', '[[\"Hartmann\",\"Michael J.\",\"\"],[\"Brandao\",\"Fernando G. S. L.\",\"\"],[\"Plenio\",\"Martin B.\",\"\"]]'),
(704.3057, 'Benjamin Safdi', 'Benjamin R. Safdi and Harvey Segur', 'Explosive instability due to 4-wave mixing', '', '', '10.1103/PhysRevLett.99.245004', '', 'nlin.SI', '', '  It is known that an explosive instability can occur when nonlinear waves\npropagate in certain media that admit 3-wave mixing. The purpose of this paper\nis to show that explosive instabilities can occur even in media that admit no\n3-wave mixing. Instead, the instability is caused by 4-wave mixing: four\nresonantly interacting wavetrains gain energy from a background, and all blow\nup in a finite time. Unlike singularities associated with self-focussing, these\nsingularities can occur with no spatial structure - the waves blow up\neverywhere in space, simultaneously.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:36:48 GMT\"}]', '2009-11-13', '[[\"Safdi\",\"Benjamin R.\",\"\"],[\"Segur\",\"Harvey\",\"\"]]'),
(704.3058, 'Milan Janjic', 'Milan Janji\\\'c', 'Some integer sequences based on derangements', '', '', '', '', 'math.CO', '', '  Sequences whose terms are equal to the number of functions with specified\nproperties are considered. Properties are based on the notion of derangements\nin a more general sense. Several sequences which generalize the standard notion\nof derangements are thus obtained. These sequences generate a number of integer\nsequences from the well-known Sloane\'s encyclopedia.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:58:43 GMT\"}]', '2007-05-23', '[[\"Janjić\",\"Milan\",\"\"]]'),
(704.3059, 'Rob P. Olling', 'Rob P. Olling', 'Finding Solar System Analogs With SIM and HIPPARCOS: A White Paper for\n  the ExoPlanet Task Force', 'A White Paper for the ExoPlanet Task Force: 7 pages', '', '', '', 'astro-ph', '', '  The astrometric signature imposed by a planet on its primary increases\nsubstantially towards longer periods (proportinal to P^2/3), so that\nlong-period planets can be more easily detected, in principle. For example, a\none Solar-mass (M_Sun) star would be pulled by roughly 1 mas by a one\nJupiter-mass (M_J) planet with a period of one-hundred years at a distance of\n20 pc. Such position accuracies can now be obtained with both ground-based and\nspace-based telescopes. The difficulty was that it often takes many decades\nbefore a detectable position shift will occur. However, by the time the next\ngeneration of astrometric missions such as SIM will be taking data, several\ndecades will have past since the first astrometric mission, HIPPARCOS. Here we\npropose to use a new astrometric method that employs a future, highly accurate\nSIM Quick-Look survey and HIPPARCOS data taken twenty years prior. Using\nposition errors for SIM of 4 muas, this method enables the detection and\ncharacterization of Solar-system analogs (SOSAs) with periods up to 240 (500)\nyears for 1 (10) M_J companions. Because many tens of thousands nearby stars\ncan be surveyed this way for a modest expenditure of SIM time and SOSAs may be\nquite abundant, we expect to find many hundreds of extra-solar planets with\nlong-period orbits. Such a data set would nicely complement the short-period\nsystems found by the radial-velocity method. Brown dwarfs and low-mass stellar\ncompanions can be found and characterized if their periods are shorter than\nabout 500 years. This data set will provide invaluable constraints on models of\nplanet formation, as well as a database for systems where the location of the\ngiant planets allow for the formation of low-mass planets in the habitable\nzone. [Abridged]\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:42:10 GMT\"}]', '2007-05-23', '[[\"Olling\",\"Rob P.\",\"\"]]'),
(704.3060, 'Klaus Hornberger', 'Klaus Hornberger', 'Open quantum dynamics via environmental monitoring', '11 pages, 3 figures. Talk at DICE 2006; to appear in J. Phys.: Conf.\n  Ser. (2007)', '', '10.1088/1742-6596/67/1/012002', '', 'quant-ph', '', '  A general method is discussed to obtain Markovian master equations which\ndescribe the interaction with the environment in a microscopic and\nnon-perturbative fashion. It is based on combining time-dependent scattering\ntheory with the concept of continuous quantum measurements. The applications to\nthe case of a Brownian point particle and to the case of a complex molecule,\nboth in the presence of a gaseous environment, are outlined.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:45:11 GMT\"}]', '2009-11-13', '[[\"Hornberger\",\"Klaus\",\"\"]]'),
(704.3061, 'Evgeny Smirnov', 'Evgeny Smirnov', 'Bruhat order for two subspaces and a flag', '30 pages, with figures', '', '', '', 'math.RT math.AG math.CO', '', '  The classical Ehresmann-Bruhat order describes the possible degenerations of\na pair of flags in a finite-dimensional vector space V; or, equivalently, the\nclosure of an orbit of the group GL(V) acting on the direct product of two full\nflag varieties.\n  We obtain a similar result for triples consisting of two subspaces and a\npartial flag in V; this is equivalent to describing the closure of a\nGL(V)-orbit in the product of two Grassmannians and one flag variety. We give a\nrank criterion to check whether such a triple can be degenerated to another\none, and we classify the minimal degenerations. Our methods involve only\nelementary linear algebra and combinatorics of graphs (originating in\nAuslander-Reiten quivers).\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:59:56 GMT\"}]', '2007-05-23', '[[\"Smirnov\",\"Evgeny\",\"\"]]'),
(704.3062, 'Dmitry Klochkov', 'D. Klochkov, R. Staubert, S. Tsygankov, A. Lutovinov, K. P. Postnov,\n  N. I. Shakura, S. A. Potanin, C. Ferrigno, I. Kreykenbohm, and J.Wilms', 'INTEGRAL observations of HER X-1', 'To be published in the proceedings of the 6th INTEGRAL Workshop \"The\n  Obscured Universe\" (3-7 July 2006, Moscow)', '', '', '', 'astro-ph', '', '  First results of observations of the low mass X-ray binary Her X-1/HZ Her\nperformed by the INTEGRAL satellite in July-August 2005 are presented. A\nsignificant part of one 35 day main-on state was covered. The cyclotron line in\nthe X-ray spectrum is well observed and its position and shape, as well as its\nvariability with time and phase of the 1.24 s pulsation are explored. X-ray\npulse profiles for different energy bands are studied throughout the\nobservation. The pulse period is found to vary on short time scales revealing a\ndynamical spin-up/spin-down behavior. Results of simultaneous optical\nobservations of HZ Her are also discussed.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 18:58:24 GMT\"}]', '2007-05-23', '[[\"Klochkov\",\"D.\",\"\"],[\"Staubert\",\"R.\",\"\"],[\"Tsygankov\",\"S.\",\"\"],[\"Lutovinov\",\"A.\",\"\"],[\"Postnov\",\"K. P.\",\"\"],[\"Shakura\",\"N. I.\",\"\"],[\"Potanin\",\"S. A.\",\"\"],[\"Ferrigno\",\"C.\",\"\"],[\"Kreykenbohm\",\"I.\",\"\"],[\"Wilms\",\"J.\",\"\"]]'),
(704.3063, 'Pamela Morehouse', 'S. B. Athar, et al, CLEO Collaboration', 'Search for Radiative Decays of Upsilon(1S) into eta and eta\'', '14 pages postscript,also available through\n  http://www.lns.cornell.edu/public/CLNS/2007/, Submitted to PRD', 'Phys.Rev.D76:072003,2007', '10.1103/PhysRevD.76.072003', 'CLNS 07/1995, CLEO 07-5', 'hep-ex', '', '  We report on a search for the radiative decay of Upsilon(1S) to the\npseudoscalar mesons eta and etaprime in 21.2 +/- 0.2 times 10^6 Upsilon(1S)\ndecays collected with the CLEO III detector at the Cornell Electron Storage\nRing (CESR). The eta meson was reconstructed in the three modes eta to\ngamma-gamma, eta to pi+pi-pi0 and eta to 3pi0. The etaprime meson was\nreconstructed in the mode etaprime to pi+ pi- eta with eta decaying through any\nof the above three modes, and also etaprime to gamma rho, where rho decays to\npi^+ pi^-.\n  Five out of the seven sub-modes are found to be virtually background-free. In\nfour of them we find no signal candidates and in one Upsilon(1S) to\ngamma-etaprime, etaprime to pi+ pi- eta, eta to pi+pi-pi0 there are two good\nsignal candidates, which is insufficient evidence to claim a signal. The other\ntwo sub-modes eta to gamma-gamma and etaprime to gamma rho are background\nlimited, and show no excess of events in their signal regions. We combine the\nresults from different channels and obtain upper limits at the 90% C.L. which\nare B(Upsilon(1S) to gamma eta) < 1.0 times 10^-6 and B(Upsilon(1S) to gamma\netaprime) < 1.9 times 10^-6. Our limits are an order of magnitude tighter than\nthe previous ones and below the predictions made by some theoretical models.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 19:04:42 GMT\"}]', '2010-04-08', '[[\"Athar\",\"S. B.\",\"\"],[\"Collaboration\",\"CLEO\",\"\"]]'),
(704.3064, 'Kyle Lawson', 'Kyle Lawson and Ariel R.Zhitnitsky', 'Diffuse cosmic gamma-rays at 1-20 MeV: A trace of the dark matter?', '13 pages, 1 figure', 'JCAP 0801:022,2008', '10.1088/1475-7516/2008/01/022', '', 'astro-ph hep-ph', '', '  Several independent observations of the galactic core suggest hitherto\nunexplained sources of energy. The most well known case is the 511 keV line\nwhich has proven very difficult to explain with conventional astrophysical\npositron sources. A similar, but less well known mystery is the excess of\ngamma-ray photons detected by COMPTEL across a broad energy range 1-20 MeV.\nSuch photons are found to be very difficult to produce via known astrophysical\nsources. We show in this work that dark matter in the form of dense antimatter\ndroplets provides a natural explanations for the observed flux of gamma-rays in\nthe 1-20 MeV range. We argue thatsuch photons must always accompany the 511 keV\nline as they produced by the same mechanism within our framework. We calculate\nthe spectrum and intensity of the 1-20 MeV gamma-rays, and find it to be\nconsistent with the COMPTEL data.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 21:37:41 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 2 Aug 2007 16:19:48 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 26 Nov 2007 16:35:05 GMT\"}]', '2009-06-23', '[[\"Lawson\",\"Kyle\",\"\"],[\"Zhitnitsky\",\"Ariel R.\",\"\"]]'),
(704.3065, 'Elena Jimenez-Bailon', 'E. Jimenez-Bailon, N. Loiseau, M. Guainazzi, G. Matt, D.\n  Rosa-Gonzalez, E. Piconcelli, and M. Santos-Lleo', 'XMM-Newton view of galaxy pairs: activation of quiescent black holes?', 'Accepted for publication in A&A', '', '10.1051/0004-6361:20066761', '', 'astro-ph', '', '  We report on XMM-Newton observations of three nearby galaxy pairs,\nAM0707-273, AM1211-465, and AM2040-674. All six galaxies were previously\nclassified as HII galaxies based on optical and IR spectroscopic analysis. All\ngalaxies were detected with XMM-Newton and each member was isolated and\nanalyzed independently. The X-ray spectra reveal strong evidence of AGN\nactivity in the NE member of AM1211-465 pair. We measured a luminosity of\n1.94(+0.11/-0.15)x10^42 erg/s in the 2-10 keV band and the presence of a\nneutral FeK_alpha line with a confidence level of 98.8%. The high nH value,\n2.2+/-0.2x10^22 cm^-2, would explain the misclassification of the source.\nMarginal evidence of AGN nature was found in the X-ray spectra of AM1211-465SW\nand AM0707-273E. The X-ray emission of the three remaining galaxies can be\nexplained by starburst activity.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:06:19 GMT\"}]', '2009-11-13', '[[\"Jimenez-Bailon\",\"E.\",\"\"],[\"Loiseau\",\"N.\",\"\"],[\"Guainazzi\",\"M.\",\"\"],[\"Matt\",\"G.\",\"\"],[\"Rosa-Gonzalez\",\"D.\",\"\"],[\"Piconcelli\",\"E.\",\"\"],[\"Santos-Lleo\",\"M.\",\"\"]]'),
(704.3066, 'Mark Lindeman', 'Mark. A. Lindeman, Kathleen A. Barger, Donald E. Brandl, S. Gwynne\n  Crowder, Lindsay Rocks, and Dan McCammon', 'Complex impedance measurements of calorimeters and bolometers:\n  correction for stray impedances', '5 pages, 6 figures', 'Rev.Sci.Instrum.78:043105,2007', '10.1063/1.2723066', '', 'astro-ph', '', '  Impedance measurements provide a useful probe of the physics of bolometers\nand calorimeters. We describe a method for measuring the complex impedance of\nthese devices. In previous work, stray impedances and readout electronics of\nthe measurement apparatus have resulted in artifacts in the impedance data. The\nnew technique allows experimenters to find an independent Thevenin or Norton\nequivalent circuit for each frequency. This method allows experimenters to\neasily isolate the device impedance from the effects of parasitic impedances\nand frequency dependent gains in amplifiers.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:00:10 GMT\"}]', '2009-06-23', '[[\"Lindeman\",\"Mark. A.\",\"\"],[\"Barger\",\"Kathleen A.\",\"\"],[\"Brandl\",\"Donald E.\",\"\"],[\"Crowder\",\"S. Gwynne\",\"\"],[\"Rocks\",\"Lindsay\",\"\"],[\"McCammon\",\"Dan\",\"\"]]'),
(704.3067, 'Brant Jones', 'Brant C. Jones', 'Kazhdan--Lusztig polynomials for maximally-clustered hexagon-avoiding\n  permutations', '18 pages', '', '', '', 'math.CO math.RT', '', '  We provide a non-recursive description for the bounded admissible sets of\nmasks used by Deodhar\'s algorithm to calculate the Kazhdan--Lusztig polynomials\n$P_{x,w}(q)$ of type $A$, in the case when $w$ is hexagon avoiding and\nmaximally clustered. This yields a combinatorial description of the\nKazhdan--Lusztig basis elements of the Hecke algebra associated to such\npermutations $w$. The maximally-clustered hexagon-avoiding elements are\ncharacterized by avoiding the seven classical permutation patterns $\\{3421,\n4312, 4321, 46718235, 46781235, 56718234, 56781234\\}$. We also briefly discuss\nthe application of heaps to permutation pattern characterization.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:06:24 GMT\"}]', '2007-05-23', '[[\"Jones\",\"Brant C.\",\"\"]]'),
(704.3068, 'Sydney A. Barnes', 'Sydney A. Barnes', 'Ages for illustrative field stars using gyrochronology: viability,\n  limitations and errors', '58 pages, 18 color figures, accepted for publication in The\n  Astrophysical Journal; Age uncertainties slightly modified upon correcting an\n  algebraic error in Section 4', 'Astrophys.J.669:1167-1189,2007', '10.1086/519295', '', 'astro-ph', '', '  We here develop an improved way of using a rotating star as a clock, set it\nusing the Sun, and demonstrate that it keeps time well. This technique, called\ngyrochronology, permits the derivation of ages for solar- and late-type main\nsequence stars using only their rotation periods and colors. The technique is\nclarified and developed here, and used to derive ages for illustrative groups\nof nearby, late-type field stars with measured rotation periods. We first\ndemonstrate the reality of the interface sequence, the unifying feature of the\nrotational observations of cluster and field stars that makes the technique\npossible, and extends it beyond the proposal of Skumanich by specifying the\nmass dependence of rotation for these stars. We delineate which stars it cannot\ncurrently be used on. We then calibrate the age dependence using the Sun. The\nerrors are propagated to understand their dependence on color and period.\nRepresentative age errors associated with the technique are estimated at ~15%\n(plus possible systematic errors) for late-F, G, K, & early-M stars. Ages\nderived via gyrochronology for the Mt. Wilson stars are shown to be in good\nagreement with chromospheric ages for all but the bluest stars, and probably\nsuperior. Gyro ages are then calculated for each of the active main sequence\nfield stars studied by Strassmeier and collaborators where other ages are not\navailable. These are shown to be mostly younger than 1Gyr, with a median age of\n365Myr. The sample of single, late-type main sequence field stars assembled by\nPizzolato and collaborators is then assessed, and shown to have gyro ages\nranging from under 100Myr to several Gyr, and a median age of 1.2Gyr. Finally,\nwe demonstrate that the individual components of the three wide binaries\nXiBooAB, 61CygAB, & AlphaCenAB yield substantially the same gyro ages.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 23:57:30 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 17 May 2007 22:17:18 GMT\"}]', '2011-03-28', '[[\"Barnes\",\"Sydney A.\",\"\"]]'),
(704.3069, 'Nestor Mirabal', 'N. Mirabal, J. P. Halpern, P. T. O\'Brien', 'GRB 050826: A Subluminous Event at z = 0.296 Finds its Place in the\n  Luminosity Distribution of Gamma-Ray Burst Afterglows', 'Accepted for publication in ApJ', '', '10.1086/519006', '', 'astro-ph', '', '  We present the optical identification and spectroscopy of the host galaxy of\nGRB 050826 at a redshift z = 0.296 +/- 0.001. Image subtraction among\nobservations obtained on three consecutive nights, reveals a fading object 5\nhours after the burst, confirming its identification as the optical afterglow\nof this event. Deep imaging shows that the optical afterglow is offset by 0.4\narcseconds (~1.76 kpc) from the center of its irregular host galaxy, which is\ntypical for long-duration gamma-ray bursts. Combining these results with X-ray\nmeasurements acquired by the Swift XRT instrument, we find that GRB 050826\nfalls entirely within the subluminous, subenergetic group of long gamma-ray\nbursts at low redshift (z < 0.3). The results are discussed in the context of\nmodels that possibly account for this trend, including the nature of the\ncentral engine, the evolution of progenitor properties as a function of\nredshift, and incompleteness in current gamma-ray burst samples.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:15:00 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 11 May 2007 15:11:35 GMT\"}]', '2009-11-13', '[[\"Mirabal\",\"N.\",\"\"],[\"Halpern\",\"J. P.\",\"\"],[\"O\'Brien\",\"P. T.\",\"\"]]'),
(704.3070, 'Ward Struyve', 'S. Goldstein, W. Struyve', 'On the Uniqueness of Quantum Equilibrium in Bohmian Mechanics', '15 pages, no figures, LaTex', 'J. Stat. Phys. 128, 1197-1209 (2007)', '10.1007/s10955-007-9354-5', '', 'quant-ph cond-mat.other', '', '  In Bohmian mechanics the distribution $|\\psi|^2$ is regarded as the\nequilibrium distribution. We consider its uniqueness, finding that it is the\nunique equivariant distribution that is also a local functional of the wave\nfunction $\\psi$.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:17:14 GMT\"}]', '2011-11-09', '[[\"Goldstein\",\"S.\",\"\"],[\"Struyve\",\"W.\",\"\"]]'),
(704.3071, 'Karina Mazzitello', 'K. I. Mazzitello, C. M. Arizmendi, and H. G. E. Hentschel', 'Converting genetic network oscillations into somite spatial pattern', '7 pages, 7 figures', '', '10.1103/PhysRevE.78.021906', '', 'q-bio.QM', '', '  In most vertebrate species, the body axis is generated by the formation of\nrepeated transient structures called somites. This spatial periodicity in\nsomitogenesis has been related to the temporally sustained oscillations in\ncertain mRNAs and their associated gene products in the cells forming the\npresomatic mesoderm. The mechanism underlying these oscillations have been\nidentified as due to the delays involved in the synthesis of mRNA and\ntranslation into protein molecules [J. Lewis, Current Biol. {\\bf 13}, 1398\n(2003)]. In addition, in the zebrafish embryo intercellular Notch signalling\ncouples these oscillators and a longitudinal positional information signal in\nthe form of an Fgf8 gradient exists that could be used to transform these\ncoupled temporal oscillations into the observed spatial periodicity of somites.\nHere we consider a simple model based on this known biology and study its\nconsequences for somitogenesis. Comparison is made with the known properties of\nsomite formation in the zebrafish embryo . We also study the effects of\nlocalized Fgf8 perturbations on somite patterning.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:20:53 GMT\"}]', '2009-11-13', '[[\"Mazzitello\",\"K. I.\",\"\"],[\"Arizmendi\",\"C. M.\",\"\"],[\"Hentschel\",\"H. G. E.\",\"\"]]'),
(704.3072, 'Rob P. Olling', 'Rob P. Olling', 'LEAVITT: A MIDEX-class Mission for Finding & Characterizing 10,000\n  Transiting Planets in the Solar Neighborhood', 'A White Paper for the ExoPlanet Task Force, 7 pages', '', '', '', 'astro-ph', '', '  We propose a MIDEX-class space mission with the goal to find and characterize\nroughly 10,000 transiting planets. When transits occur, a much more detailed\ncharacterization of the planet is possible and so a large data base of\ntransiting planets will provide planets with a large range in periods and radii\nfor follow-up studies. Our survey will be all-sky and focused on stars brighter\nthan V=14.8. Down to V=12, LEAVITT will be able to detect Neptune-sized\nobjects. Because of it\'s high cadence, LEAVITT is about 100 times more\nsensitive at detecting transits than GAIA, while it will find more than 20\ntimes as many transits as KEPLER. LEAVITT has multi-band photometric capability\nimplemented via a low-resolution dispersive element which can obtain 0.2% (2\nmmag) photometry down to V=14.8. LEAVITT\'s high multi-band photometric accuracy\nreduces the number of false-positives significantly.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 23:10:48 GMT\"}]', '2007-05-23', '[[\"Olling\",\"Rob P.\",\"\"]]'),
(704.3073, 'Roland Kothes', 'R. Kothes, S.M. Dougherty', 'The distance and neutral environment of the massive stellar cluster\n  Westerlund 1', '8 pages, accepted for publication in A&A', 'Astron.Astrophys.468:993-1000,2007', '10.1051/0004-6361:20077309', '', 'astro-ph', '', '  The goal of this study is to determine a distance to Westerlund 1 independent\nof the characteristics of the stellar population and to study its neutral\nenvironment, using observations of atomic hydrogen. The HI observations are\ntaken from the Southern Galactic Plane Survey to study HI absorption in the\ndirection of the HII region created by the members of Westerlund 1 and to\ninvestigate its environment as observed in the HI line emission. A Galactic\nrotation curve was derived using the recently revised values for the Galactic\ncentre distance of $R_\\odot = 7.6$ kpc, and the velocity of the Sun around the\nGalactic centre of $\\Theta_\\odot = 214$ km s$^{-1}$. The newly determined\nrotation model leads us to derive a distance of $3.9\\pm 0.7$ kpc to Westerlund\n1, consistent with a location in the Scutum-Crux Arm. Included in this estimate\nis a very careful investigation of possible sources of error for the Galactic\nrotation curve. We also report on small expanding HI features around the\ncluster with a maximum dynamic age of 600,000 years and a larger bubble which\nhas a minimum dynamic age of 2.5 million years. Additionally we re-calculated\nthe kinematic distances to nearby HII regions and supernova remnants based on\nour new Galaxic rotation curve. We propose that in the early stages of the\ndevelopment of Wd 1 a large interstellar bubble of diameter about 50 pc was\ncreated by the cluster members. This bubble has a dynamic age similar to the\nage of the cluster. Small expanding bubbles, with dynamical ages $\\sim 0.6$ Myr\nare found around Wd 1, which we suggest consist of recombined material lost by\ncluster members through their winds.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 23:33:33 GMT\"}]', '2009-06-23', '[[\"Kothes\",\"R.\",\"\"],[\"Dougherty\",\"S. M.\",\"\"]]'),
(704.3074, 'Florin Moldoveanu', 'Florin Moldoveanu', 'Quantum Mechanics and Closed Timelike Curves', '8 pages, 1 figure (removed LaTex command)', 'Quant. Biosys. 1, 66 (2007)', '', '', 'physics.gen-ph', '', '  General relativity allows solutions exhibiting closed timelike curves. Time\ntravel generates paradoxes and quantum mechanics generalizations were proposed\nto solve those paradoxes. The implications of self-consistent interactions on\nacausal region of space-time are investigated. If the correspondence principle\nis true, then all generalizations of quantum mechanics on acausal manifolds are\nnot renormalizable. Therefore quantum mechanics can only be defined on global\nhyperbolic manifolds and all general relativity solutions exhibiting time\ntravel are unphysical.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 23:50:55 GMT\"}]', '2009-01-05', '[[\"Moldoveanu\",\"Florin\",\"\"]]'),
(704.3075, 'James P. Crutchfield', 'Karoline Wiesner and James P. Crutchfield', 'Computation in Sofic Quantum Dynamical Systems', '10 pages, 4 figures;\n  http://cse.ucdavis.edu/~cmg/compmech/pubs.htm#StochasticComputation', '', '', '', 'quant-ph', '', '  We analyze how measured quantum dynamical systems store and process\ninformation, introducing sofic quantum dynamical systems. Using recently\nintroduced information-theoretic measures for quantum processes, we quantify\ntheir information storage and processing in terms of entropy rate and excess\nentropy, giving closed-form expressions where possible. To illustrate the\nimpact of measurement on information storage in quantum processes, we analyze\ntwo spin-1 sofic quantum systems that differ only in how they are measured.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:49:54 GMT\"}]', '2007-05-23', '[[\"Wiesner\",\"Karoline\",\"\"],[\"Crutchfield\",\"James P.\",\"\"]]'),
(704.3076, 'Martin Kunz', 'M. Kunz, N. Aghanim, A. Riazuelo and O. Forni', 'On the detectability of non-trivial topologies', '11 pages, 9 figures', 'Phys.Rev.D77:023525,2008', '10.1103/PhysRevD.77.023525', '', 'astro-ph', '', '  We explore the main physical processes which potentially affect the\ntopological signal in the Cosmic Microwave Background (CMB) for a range of\ntoroidal universes. We consider specifically reionisation, the integrated\nSachs-Wolfe (ISW) effect, the size of the causal horizon, topological defects\nand primordial gravitational waves. We use three estimators: the information\ncontent, the S/N statistic and the Bayesian evidence. While reionisation has\nnearly no effect on the estimators, we show that taking into account the ISW\nstrongly decreases our ability to detect the topological signal. We also study\nthe impact of varying the relevant cosmological parameters within the 2 sigma\nranges allowed by present data. We find that only Omega_Lambda, which\ninfluences both ISW and the size of the causal horizon, significantly alters\nthe detection for all three estimators considered here.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:00:12 GMT\"}]', '2008-12-18', '[[\"Kunz\",\"M.\",\"\"],[\"Aghanim\",\"N.\",\"\"],[\"Riazuelo\",\"A.\",\"\"],[\"Forni\",\"O.\",\"\"]]'),
(704.3077, 'Eric F. Bell', 'Eric F. Bell (1), Xian Zhong Zheng (1,2), Casey Papovich (3), Andrea\n  Borch (4), Christian Wolf (5), and Klaus Meisenheimer (1) ((1) MPIA,\n  Heidelberg, (2) Purple Mountain Observatory, (3) Steward Observatory, (4)\n  ARI, Heidelberg, (5) Oxford)', 'Star Formation and the Growth of Stellar Mass', '9 Pages; ApJ in press', 'Astrophys.J.663:834-843,2007', '10.1086/518594', '', 'astro-ph', '', '  Recent observations have demonstrated a significant growth in the integrated\nstellar mass of the red sequence since z=1, dominated by a steadily increasing\nnumber of galaxies with stellar masses M* < 10^11 M_sun. In this paper, we use\nthe COMBO-17 photometric redshift survey in conjunction with deep Spitzer 24\nmicron data to explore the relationship between star formation and the growth\nof stellar mass. We calculate `star formation rate functions\' in four different\nredshift slices, splitting also into contributions from the red sequence and\nblue cloud for the first time. We find that the growth of stellar mass since\nz=1 is consistent with the integrated star formation rate. Yet, most of the\nstars formed are in blue cloud galaxies. If the stellar mass already in, and\nformed in, z<1 blue cloud galaxies were to stay in the blue cloud the total\nstellar mass in blue galaxies would be dramatically overproduced. We explore\nthe expected evolution of stellar mass functions, finding that in this picture\nthe number of massive M* > 3x10^10 M_sun blue galaxies would also be\noverproduced; i.e., most of the new stars formed in blue cloud galaxies are in\nthe massive galaxies. We explore a simple truncation scenario in which these\n`extra\' blue galaxies have their star formation suppressed by an unspecified\nmechanism or mechanisms; simple cessation of star formation in these extra blue\ngalaxies is approximately sufficient to build up the red sequence at M*<10^11\nM_sun.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:00:13 GMT\"}]', '2009-06-23', '[[\"Bell\",\"Eric F.\",\"\"],[\"Zheng\",\"Xian Zhong\",\"\"],[\"Papovich\",\"Casey\",\"\"],[\"Borch\",\"Andrea\",\"\"],[\"Wolf\",\"Christian\",\"\"],[\"Meisenheimer\",\"Klaus\",\"\"]]'),
(704.3078, 'A. V. Maccio\'', 'Andrea V. Maccio\'(MPIA), Ioannis Sideris (Zurich), Marco Miranda\n  (Zurich), Ben Moore (Zurich), Roland Jesseit (Munich Obs.)', 'Influence of Orbital Behaviour and Chaos on the Shape of Dark Matter\n  Halos', '14 pages, 8 figures, MNRAS submitted, a preprint with high-resolution\n  figures is available at http://www-theorie.physik.unizh.ch/~andrea/Orbits/', '', '', '', 'astro-ph', '', '  It has been shown that the dissipative gas infall during galaxy formation has\nthe capability to modify the shape of dark matter halos. In this paper we\nperform the first detailed analysis of particle orbits in a cosmological dark\nmatter halos to understand {\\it how} and {\\it why} baryons alter its shape. We\nperform a series of numerical experiments where we grow a baryonic core inside\na live dark matter halo extracted from a cosmological simulation. We follow the\norbits of more than 300 particles with more that 50000 timesteps. Our results\nclearly show that the dissipational component is responsible for repeatedly\ndeflecting orbits which visit often the center of the system. Moreover the\ngravitational potential time dependence associated with the growth of the\nbaryonic mass, shifts the frequencies of the orbits, making them extremely\nchaotic. This randomization makes the orbits explore a large phase space. When\nthis effect takes place for a significant number of orbits it will be\nmanifested in the density distribution as an approach to a rounder\nconfiguration. As a consequence, the influence of the central mass on the shape\nof the phase space decreases with increasing distance from the center. We\ndiscuss the importance of future analysis of controlled experiments (i.e. using\nanalytic potentials instead of live DM halos) to better decipher the dynamics\nof this phenomenon.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:32:22 GMT\"}]', '2007-05-23', '[[\"Maccio\'\",\"Andrea V.\",\"\",\"MPIA\"],[\"Sideris\",\"Ioannis\",\"\",\"Zurich\"],[\"Miranda\",\"Marco\",\"\",\"Zurich\"],[\"Moore\",\"Ben\",\"\",\"Zurich\"],[\"Jesseit\",\"Roland\",\"\",\"Munich Obs.\"]]'),
(704.3079, 'Ilia Solov\'yov', 'Alexander V. Yakubovich, Ilia A. Solov\'yov, Andrey V. Solov\'yov and\n  Walter Greiner', 'Ab initio theory of helix-coil phase transition', '24 pages, 3 figures', '', '10.1140/epjd/e2007-00328-9', '', 'physics.bio-ph physics.chem-ph', '', '  In this paper we suggest a theoretical method based on the statistical\nmechanics for treating the alpha-helix-random coil transition in alanine\npolypeptides. We consider this process as a first-order phase transition and\ndevelop a theory which is free of model parameters and is based solely on\nfundamental physical principles. It describes essential thermodynamical\nproperties of the system such as heat capacity, the phase transition\ntemperature and others from the analysis of the polypeptide potential energy\nsurface calculated as a function of two dihedral angles, responsible for the\npolypeptide twisting. The suggested theory is general and with some\nmodification can be applied for the description of phase transitions in other\ncomplex molecular systems (e.g. proteins, DNA, nanotubes, atomic clusters,\nfullerenes).\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:10:04 GMT\"}]', '2009-11-13', '[[\"Yakubovich\",\"Alexander V.\",\"\"],[\"Solov\'yov\",\"Ilia A.\",\"\"],[\"Solov\'yov\",\"Andrey V.\",\"\"],[\"Greiner\",\"Walter\",\"\"]]'),
(704.3080, 'Takuya Okuda', 'Jaume Gomis and Takuya Okuda', 'D-branes as a Bubbling Calabi-Yau', '32 pages; v.2 reference added', 'JHEP0707:005,2007', '10.1088/1126-6708/2007/07/005', 'CPHT-RR022.0407, NSF-KITP-07-106', 'hep-th math.DG', '', '  We prove that the open topological string partition function on a D-brane\nconfiguration in a Calabi-Yau manifold X takes the form of a closed topological\nstring partition function on a different Calabi-Yau manifold X_b. This\nidentification shows that the physics of D-branes in an arbitrary background X\nof topological string theory can be described either by open+closed string\ntheory in X or by closed string theory in X_b. The physical interpretation of\nthe \'\'bubbling\'\' Calabi-Yau X_b is as the space obtained by letting the\nD-branes in X undergo a geometric transition. This implies, in particular, that\nthe partition function of closed topological string theory on certain bubbling\nCalabi-Yau manifolds are invariants of knots in the three-sphere.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:02:59 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 15 Jun 2007 20:31:42 GMT\"}]', '2008-11-26', '[[\"Gomis\",\"Jaume\",\"\"],[\"Okuda\",\"Takuya\",\"\"]]'),
(704.3081, 'Andrei Gruzinov', 'Andrei Gruzinov', 'Directed Relativistic Blast Wave', '9 pages', '', '', '', 'astro-ph', '', '  A spherically symmetrical ultra-relativistic blast wave is not an attractor\nof a generic asymmetric explosion. Spherical symmetry is reached only by the\ntime the blast wave slows down to non-relativistic velocities, when the\nSedov-Taylor-von Neumann attractor solution sets in. We show however, that a\ndirected relativistic explosion, with the explosion momentum close to the\nexplosion energy, produces a blast wave with a universal intermediate\nasymptotic -- a selfsimilar directed ultra-relativistic blast wave. This\nuniversality might be of interest for the astrophysics of gamma-ray burst\nafterglows.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:11:08 GMT\"}]', '2007-05-23', '[[\"Gruzinov\",\"Andrei\",\"\"]]'),
(704.3082, 'Plamen Bozhilov', 'P. Bozhilov', 'Neumann and Neumann-Rosochatius integrable systems from membranes on\n  AdS_4xS^7', 'LaTeX, 17 pages, no figures;v2: comments and citations added;v3: 20\n  pages, new subsection, explanations, comments and references added; v4: some\n  typos fixed, to appear in JHEP', 'JHEP0708:073,2007', '10.1088/1126-6708/2007/08/073', '', 'hep-th nlin.SI', '', '  It is known that large class of classical string solutions in the type IIB\nAdS_5xS^5 background is related to the Neumann and Neumann-Rosochatius\nintegrable systems, including spiky strings and giant magnons. It is also\ninteresting if these integrable systems can be associated with some membrane\nconfigurations in M-theory. We show here that this is indeed the case by\npresenting explicitly several types of membrane embedding in AdS_4xS^7 with the\nsearched properties.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:14:00 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 28 Apr 2007 08:25:36 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 17 Jul 2007 08:54:05 GMT\"},{\"version\":\"v4\",\"created\":\"Fri, 24 Aug 2007 20:09:17 GMT\"}]', '2008-11-26', '[[\"Bozhilov\",\"P.\",\"\"]]'),
(704.3083, 'Alberto Buzzoni', 'Alberto Buzzoni (INAF, Osservatorio Astronomico di Bologna, Italy)', 'Late stages of stellar evolution and their impact on spectrophotometric\n  properties of galaxies', '8 pages and 6 figures (macro asp2006.sty included). An invited\n  contribution to the intl. conference \"From Stars to Galaxies: Building the\n  pieces to build up the Universe\" (Venezia, Italy, 16-20/Oct/2006). ASP Conf.\n  Series, eds. A. Vallenari, R. Tantalo, L. Portinari and A. Moretti. Further\n  info at author\'s web site (see http://www.bo.astro.it/~eps/home.html)', '', '', '', 'astro-ph', '', '  The connection between AGB evolution of stellar populations and infrared vs.\nultraviolet properties of the parent galaxies is reviewed relying on the\nupdated lookout provided by population-synthesis theory. In particular,\nplanetary-nebula events and hot horizontal-branch evolution are assessed in a\nunitary view to outline a plain general picture of galaxy spectrophotometric\nevolution. This will include a brief discussion of relevant phenomena such as\nthe \"UV upturn\" in ellipticals and the stellar mass loss properties along the\ngalaxy morphological sequence.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:18:24 GMT\"}]', '2007-05-23', '[[\"Buzzoni\",\"Alberto\",\"\",\"INAF, Osservatorio Astronomico di Bologna, Italy\"]]'),
(704.3084, 'Joshua Erlich', 'Christopher D. Carone, Joshua Erlich, and Marc Sher', 'Holographic Electroweak Symmetry Breaking from D-branes', 'REVTeX, 25 pages, 8 eps figures, version published in PRD', 'Phys.Rev.D76:015015,2007', '10.1103/PhysRevD.76.015015', '', 'hep-th hep-ph', '', '  We observe several interesting phenomena in a technicolor-like model of\nelectroweak symmetry breaking based on the D4-D8-D8bar system of Sakai and\nSugimoto. The benefit of holographic models based on D-brane configurations is\nthat both sides of the holographic duality are well understood. We find that\nthe lightest technicolor resonances contribute negatively to the\nPeskin-Takeuchi S-parameter, but heavy resonances do not decouple and lead\ngenerically to large, positive values of S, consistent with standard estimates\nin QCD-like theories. We study how the S parameter and the masses and decay\nconstants of the vector and axial-vector techni-resonances vary over a\none-parameter family of D8-brane configurations. We discuss possibilities for\nthe consistent truncation of the theory to the first few resonances and suggest\nsome generic predictions of stringy holographic technicolor models.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:13:40 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 21 Jun 2007 15:08:29 GMT\"}]', '2008-11-26', '[[\"Carone\",\"Christopher D.\",\"\"],[\"Erlich\",\"Joshua\",\"\"],[\"Sher\",\"Marc\",\"\"]]'),
(704.3085, 'Ilia Solov\'yov', 'Ilia A. Solov\'yov, Alexander V. Yakubovich, Andrey V. Solov\'yov and\n  Walter Greiner', 'Alpha helix-coil phase transition: analysis of ab initio theory\n  predictions', '34 pages, 12 figures', '', '10.1140/epjd/e2007-00327-x', '', 'physics.bio-ph physics.chem-ph', '', '  In the present paper we present results of calculations obtained with the use\nof the theoretical method described in our preceding paper [1] and perform\ndetail analysis of alpha helix-random coil transition in alanine polypeptides\nof different length. We have calculated the potential energy surfaces of\npolypeptides with respect to their twisting degrees of freedom and construct a\nparameter-free partition function of the polypeptide using the suggested method\n[1]. From the build up partition function we derive various thermodynamical\ncharacteristics for alanine polypeptides of different length as a function of\ntemperature. Thus, we analyze the temperature dependence of the heat capacity,\nlatent heat and helicity for alanine polypeptides consisting of 21, 30, 40, 50\nand 100 amino acids. Alternatively, we have obtained same thermodynamical\ncharacteristics from the use of molecular dynamics simulations and compared\nthem with the results of the new statistical mechanics approach. The comparison\nproves the validity of the statistical mechanic approach and establishes its\naccuracy.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:28:38 GMT\"}]', '2009-11-13', '[[\"Solov\'yov\",\"Ilia A.\",\"\"],[\"Yakubovich\",\"Alexander V.\",\"\"],[\"Solov\'yov\",\"Andrey V.\",\"\"],[\"Greiner\",\"Walter\",\"\"]]'),
(704.3086, 'Marek Biskup', 'Marek Biskup, Herbert Spohn', 'Scaling limit for a class of gradient fields with nonconvex potentials', 'Published in at http://dx.doi.org/10.1214/10-AOP548 the Annals of\n  Probability (http://www.imstat.org/aop/) by the Institute of Mathematical\n  Statistics (http://www.imstat.org)', 'Annals of Probability 2011, Vol. 39, No. 1, 224-251', '10.1214/10-AOP548', 'IMS-AOP-AOP548', 'math.PR math-ph math.MP', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We consider gradient fields $(\\phi_x:x\\in \\mathbb{Z}^d)$ whose law takes the\nGibbs--Boltzmann form $Z^{-1}\\exp\\{-\\sum_{< x,y>}V(\\phi_y-\\phi_x)\\}$, where the\nsum runs over nearest neighbors. We assume that the potential $V$ admits the\nrepresentation \\[V(\\eta):=-\\log\\int\\varrho({d}\\kappa)\\exp\\biggl[-{1/2}\\kappa\\et\na^2\\biggr],\\] where $\\varrho$ is a positive measure with compact support in\n$(0,\\infty)$. Hence, the potential $V$ is symmetric, but nonconvex in general.\nWhile for strictly convex $V$\'s, the translation-invariant, ergodic gradient\nGibbs measures are completely characterized by their tilt, a nonconvex\npotential as above may lead to several ergodic gradient Gibbs measures with\nzero tilt. Still, every ergodic, zero-tilt gradient Gibbs measure for the\npotential $V$ above scales to a Gaussian free field.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:45:20 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 10 Sep 2009 20:20:03 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 8 Dec 2010 12:58:35 GMT\"}]', '2010-12-09', '[[\"Biskup\",\"Marek\",\"\"],[\"Spohn\",\"Herbert\",\"\"]]'),
(704.3087, 'Dierk Schleicher', 'Mihai Bailesteanu, Vlad Balan, Dierk Schleicher', 'Hausdorff Dimension of Exponential Parameter Rays and Their Endpoints', '10 pages', 'Nonlinearity 21 (2008), 113-120', '10.1088/0951-7715/21/1/006', '', 'math.DS', '', '  We investigate the set $I$ of parameters $\\kappa$ for which the singular\nvalue of $z\\mapsto e^z+\\kappa$ converges to $\\infty$. The set $I$ consists of\nuncountably many parameter rays, plus landing points of some of these rays. We\nshow that the parameter rays have Hausdorff dimension 1, while the ray\nendpoints in $I$ alone have dimension 2. Analogous results were known for\ndynamical planes of exponential maps; our result shows that this also holds in\nparameter space.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:58:35 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 16 Nov 2007 08:49:20 GMT\"}]', '2009-11-13', '[[\"Bailesteanu\",\"Mihai\",\"\"],[\"Balan\",\"Vlad\",\"\"],[\"Schleicher\",\"Dierk\",\"\"]]'),
(704.3088, 'Henrique R. Schmitt', 'N. E. Kassim, T. J. W. Lazio, W. C. Erickson, R. A. Perley, W. D.\n  Cotton, E. W. Greisen, A. S. Cohen, B. Hicks, H. R. Schmitt, D. Katz', 'The 74MHz System on the Very Large Array', '73 pages, 46 jpeg figures, to appear in ApJS', '', '10.1086/519022', '', 'astro-ph', '', '  The Naval Research Laboratory and the National Radio Astronomy Observatory\ncompleted implementation of a low frequency capability on the VLA at 73.8 MHz\nin 1998. This frequency band offers unprecedented sensitivity (~25 mJy/beam)\nand resolution (~25 arcsec) for low-frequency observations. We review the\nhardware, the calibration and imaging strategies, comparing them to those at\nhigher frequencies, including aspects of interference excision and wide-field\nimaging. Ionospheric phase fluctuations pose the major difficulty in\ncalibrating the array. Over restricted fields of view or at times of extremely\nquiescent ionospheric ``weather\'\', an angle-invariant calibration strategy can\nbe used. In this approach a single phase correction is devised for each\nantenna, typically via self-calibration. Over larger fields of view or at times\nof more normal ionospheric ``weather\'\' when the ionospheric isoplanatic patch\nsize is smaller than the field of view, we adopt a field-based strategy in\nwhich the phase correction depends upon location within the field of view. This\nsecond calibration strategy was implemented by modeling the ionosphere above\nthe array using Zernike polynomials. Images of 3C sources of moderate strength\nare provided as examples of routine, angle-invariant calibration and imaging.\nFlux density measurements indicate that the 74 MHz flux scale at the VLA is\nstable to a few percent, and tied to the Baars et al. value of Cygnus A at the\n5 percent level. We also present an example of a wide-field image, devoid of\nbright objects and containing hundreds of weaker sources, constructed from the\nfield-based calibration. We close with a summary of lessons the 74 MHz system\noffers as a model for new and developing low-frequency telescopes. (Abridged)\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 20:59:04 GMT\"}]', '2009-11-13', '[[\"Kassim\",\"N. E.\",\"\"],[\"Lazio\",\"T. J. W.\",\"\"],[\"Erickson\",\"W. C.\",\"\"],[\"Perley\",\"R. A.\",\"\"],[\"Cotton\",\"W. D.\",\"\"],[\"Greisen\",\"E. W.\",\"\"],[\"Cohen\",\"A. S.\",\"\"],[\"Hicks\",\"B.\",\"\"],[\"Schmitt\",\"H. R.\",\"\"],[\"Katz\",\"D.\",\"\"]]'),
(704.3089, 'H. A. Dye', 'H. A. Dye', 'Pure Virtual Braids Homotopic to the Identity Braid', '18 pages, 17 figures Final version, accepted by Fundamenta\n  Mathematicae', '', '', '', 'math.GT math.AT', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Two virtual link diagrams are homotopic if one may be transformed into the\nother by a sequence of virtual Reidemeister moves, classical Reidemeister\nmoves, and self crossing changes. We recall the pure virtual braid group. We\nthen describe the set of pure virtual braids that are homotopic to the identity\nbraid.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 21:10:16 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 21 Aug 2008 12:33:35 GMT\"}]', '2008-08-21', '[[\"Dye\",\"H. A.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3090, 'Benoit Fresse', 'Benoit Fresse', 'Modules over operads and functors', 'This book project has been withdrawn from arXiv. Final version to\n  appear as a Springer-Verlag Lecture Notes with significant additions and\n  corrections. The preprint on arXiv will not be updated', '', '', '', 'math.AT', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  In the theory of operads we consider functors of generalized symmetric powers\ndefined by sums of coinvariant modules under actions of symmetric groups. One\nobserves classically that the construction of symmetric functors provides an\nisomorphism from the category of symmetric modules to a subcategory of the\ncategory of functors on the base category. The purpose of this book is to\nobtain a similar relationship for functors on a category of algebras over an\noperad.\n  We observe that right modules over operads, symmetric modules equipped with a\nright operad action, give rise to functors on categories of algebras and we\nprove that this construction yields an embedding of categories. Then we check\nthat right modules over operads form a model category. In addition we prove\nthat weak-equivalences of right modules correspond to pointwise\nweak-equivalences at the functor level. As a conclusion, we obtain that right\nmodules over operads supply good models for the homotopy of associated functors\non algebras over operads.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:28:01 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 29 May 2007 15:31:57 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 8 Nov 2007 22:38:10 GMT\"},{\"version\":\"v4\",\"created\":\"Fri, 18 Jan 2008 10:45:08 GMT\"},{\"version\":\"v5\",\"created\":\"Wed, 25 Feb 2009 09:29:30 GMT\"}]', '2009-02-25', '[[\"Fresse\",\"Benoit\",\"\"]]'),
(704.3091, 'David Richter', 'David A. Richter', 'Triacontagonal coordinates for the E(8) root system', '4 pages, 2 figures', '', '', '', 'math.GM', '', '  This note gives an explicit formula for the elements of the E(8) root system.\nThe formula is triacontagonally symmetric in that one may clearly see an action\nby the cyclic group with 30 elements. The existence of such a formula is due to\nthe fact that the Coxeter number of E(8) is 30.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 19:35:29 GMT\"}]', '2007-05-23', '[[\"Richter\",\"David A.\",\"\"]]'),
(704.3092, 'David P. Blecher', 'David P. Blecher and Maureen K. Royce', 'Extensions of operator algebras I', '', '', '10.1016/j.jmaa.2007.07.065', '', 'math.OA math.FA', '', '  We transcribe a portion of the theory of extensions of C*-algebras to general\noperator algebras. We also include several new general facts about\napproximately unital ideals in operator algebras and the C*-algebras which they\ngenerate.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 21:21:43 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 1 Aug 2007 20:08:22 GMT\"}]', '2015-05-13', '[[\"Blecher\",\"David P.\",\"\"],[\"Royce\",\"Maureen K.\",\"\"]]'),
(704.3093, 'Jean-Baptiste Meilhan', 'Jean-Baptiste Meilhan and Akira Yasuhara', 'Whitehead double and Milnor invariants', '9 pages, 5 figures. Some minor modifications in this final version', 'Osaka J. Math. 48 No. 2 (2011), 371-381', '', '', 'math.GT', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We consider the operation of Whitehead double on a component of a link and\nstudy the behavior of Milnor invariants under this operation. We show that this\noperation turns a link whose Milnor invariants of length < k are all zero into\na link with vanishing Milnor invariants of length < 2k, and we provide formulas\nfor the first non-vanishing ones.\n  As a consequence, we obtain statements relating the notions of link-homotopy\nand self Delta-equivalence via the Whitehead double operation. By using our\nresult, we show that a Brunnian link L is link-homotopic to the unlink if and\nonly if a link L with a single component Whitehed doubled is self\nDelta-equivalent to the unlink.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 21:24:47 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 29 Feb 2012 10:57:47 GMT\"}]', '2012-03-01', '[[\"Meilhan\",\"Jean-Baptiste\",\"\"],[\"Yasuhara\",\"Akira\",\"\"]]'),
(704.3094, 'Olympia Hadjiliadis', 'Olympia Hadjiliadis and H.Vincent Poor', 'Detection of two-sided alternatives in a Brownian motion model', '4 pages, to appear in the Proceedings of the 56th Session of the\n  International Statistical Institute, Lisbon, Portugal, August 22- 29, 2007', '', '', '', 'cs.IT math.IT', '', '  This work examines the problem of sequential detection of a change in the\ndrift of a Brownian motion in the case of two-sided alternatives. Applications\nto real life situations in which two-sided changes can occur are discussed.\nTraditionally, 2-CUSUM stopping rules have been used for this problem due to\ntheir asymptotically optimal character as the mean time between false alarms\ntends to $\\infty$. In particular, attention has focused on 2-CUSUM harmonic\nmean rules due to the simplicity in calculating their first moments. In this\npaper, we derive closed-form expressions for the first moment of a general\n2-CUSUM stopping rule. We use these expressions to obtain explicit upper and\nlower bounds for it. Moreover, we derive an expression for the rate of change\nof this first moment as one of the threshold parameters changes. Based on these\nexpressions we obtain explicit upper and lower bounds to this rate of change.\nUsing these expressions we are able to find the best 2-CUSUM stopping rule with\nrespect to the extended Lorden criterion. In fact, we demonstrate not only the\nexistence but also the uniqueness of the best 2-CUSUM stopping both in the case\nof a symmetric change and in the case of a non-symmetric case. Furthermore, we\ndiscuss the existence of a modification of the 2-CUSUM stopping rule that has a\nstrictly better performance than its classical 2-CUSUM counterpart for small\nvalues of the mean time between false alarms. We conclude with a discussion on\nthe open problem of strict optimality in the case of two-sided alternatives.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 22:28:30 GMT\"}]', '2007-07-13', '[[\"Hadjiliadis\",\"Olympia\",\"\"],[\"Poor\",\"H. Vincent\",\"\"]]'),
(704.3095, 'David P. Blecher', 'David P. Blecher, Kay Kirkpatrick, Matthew Neal, Wend Werner', 'Ordered involutive operator spaces', '11 pages. To appear, Positivity', '', '', '', 'math.OA math.FA', '', '  This is a companion to recent papers of the authors; here we construct the\n`noncommutative\n  Shilov boundary\' of a (possibly nonunital) selfadjoint ordered space of\nHilbert space operators. The morphisms in the universal property of the\nboundary preserve order.\n  As an application, we consider `maximal\' and `minimal\' unitizations of such\nordered operator spaces.\n', '[{\"version\":\"v1\",\"created\":\"Mon, 23 Apr 2007 21:29:18 GMT\"}]', '2007-05-23', '[[\"Blecher\",\"David P.\",\"\"],[\"Kirkpatrick\",\"Kay\",\"\"],[\"Neal\",\"Matthew\",\"\"],[\"Werner\",\"Wend\",\"\"]]'),
(704.3096, 'Vincent Bouchard', 'Vincent Bouchard and Ron Donagi', 'On a class of non-simply connected Calabi-Yau threefolds', '50 pages; v3: version published in CNTP', 'Comm. Numb. Theor. Phys. 2 (2008) 1-61', '', '', 'math.AG hep-th', '', '  We obtain a detailed classification for a class of non-simply connected\nCalabi-Yau threefolds which are of potential interest for a wide range of\nproblems in string phenomenology. These threefolds arise as quotients of\nSchoen\'s Calabi-Yau threefolds, which are fiber products over P1 of two\nrational elliptic surfaces. The quotient is by a freely acting finite abelian\ngroup preserving the fibrations. Our work involves a classification of\nrestricted finite automorphism groups of rational elliptic surfaces.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:05:55 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 3 May 2007 18:42:49 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 14 Apr 2008 17:56:58 GMT\"}]', '2008-04-14', '[[\"Bouchard\",\"Vincent\",\"\"],[\"Donagi\",\"Ron\",\"\"]]'),
(704.3097, 'Sarah Brough', 'S. Brough (Swinburne University), R. Proctor (Swin), D. Forbes (Swin),\n  W. Couch (Swin), C. Collins (Liverpool John Moores), D. Burke (CfA), R. Mann\n  (ROE)', 'Spatially resolved kinematics and stellar populations of brightest\n  cluster and group galaxies', '21 pages plus appendices, accepted for publication in MNRAS', 'Mon.Not.Roy.Astron.Soc.378:1507-1530,2007', '10.1111/j.1365-2966.2007.11900.x', '', 'astro-ph', '', '  We present an examination of the kinematics and stellar populations of a\nsample of 3 Brightest Group Galaxies (BGGs) and 3 Brightest Cluster Galaxies\n(BCGs) in X-ray groups and clusters. We have obtained high signal-to-noise\nGemini/GMOS (Gemini South Multi-Object Spectrograph) long-slit spectra of these\ngalaxies and use Lick indices to determine ages, metallicities and\nalpha-element abundance ratios out to at least their effective radii. We find\nthat the BGGs and BCGs have very uniform masses, central ages and central\nmetallicities. Examining the radial dependence of their stellar populations, we\nfind no significant velocity dispersion, age, or alpha-enhancement gradients.\nHowever, we find a wide range of metallicity gradients, suggesting a variety of\nformation mechanisms. The range of metallicity gradients observed is surprising\ngiven the homogeneous environment these galaxies probe and their uniform\ncentral stellar populations. However, our results are inconsistent with any\nsingle model of galaxy formation and emphasize the need for more theoretical\nunderstanding of both the origins of metallicity gradients and galaxy formation\nitself. We postulate two possible physical causes for the different formation\nmechanisms.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 00:39:38 GMT\"}]', '2009-06-23', '[[\"Brough\",\"S.\",\"\",\"Swinburne University\"],[\"Proctor\",\"R.\",\"\",\"Swin\"],[\"Forbes\",\"D.\",\"\",\"Swin\"],[\"Couch\",\"W.\",\"\",\"Swin\"],[\"Collins\",\"C.\",\"\",\"Liverpool John Moores\"],[\"Burke\",\"D.\",\"\",\"CfA\"],[\"Mann\",\"R.\",\"\",\"ROE\"]]'),
(704.3098, 'Amaury Lambert', 'Amaury Lambert (PMA)', 'The contour of splitting trees is a L\\\'evy process', '', '', '', '', 'math.PR', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Splitting trees are those random trees where individuals give birth at\nconstant rate during a lifetime with general distribution, to i.i.d. copies of\nthemselves. The width process of a splitting tree is then a binary, homogeneous\nCrump--Mode--Jagers (CMJ) process, and is not Markovian unless the lifetime\ndistribution is exponential. Here, we allow the birth rate to be infinite, that\nis, pairs of birth times and lifespans of newborns form a Poisson point process\nalong the lifetime of their mother, with possibly infinite intensity measure. A\nsplitting tree is a random (so-called) chronological tree. Each element of a\nchronological tree is a (so-called) existence point $(v,\\tau)$ of some\nindividual $v$ (vertex) in a discrete tree, where $\\tau$ is a nonnegative real\nnumber called chronological level (time). We introduce a total order on\nexistence points, called linear order, and a mapping $\\varphi$ from the tree\ninto the real line which preserves this order. The inverse of $\\varphi$ is\ncalled the exploration process, and the projection of this inverse on\nchronological levels the contour process. For splitting trees truncated up to\nlevel $\\tau$, we prove that thus defined contour process is a L\\\'evy process\nreflected below $\\tau$ and killed upon hitting 0. This allows to derive\nproperties of (i) splitting trees: conceptual proof of Le Gall--Le Jan\'s\ntheorem in the finite variation case, exceptional points, coalescent point\nprocess, age distribution; (ii) CMJ processes: one-dimensional marginals,\nconditionings, limit theorems, asymptotic numbers of individuals with infinite\nvs finite descendances.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:34:17 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 9 Feb 2009 11:00:30 GMT\"}]', '2009-02-09', '[[\"Lambert\",\"Amaury\",\"\",\"PMA\"]]'),
(704.3099, 'Vyacheslav P. Spiridonov', 'V.P. Spiridonov', 'Elliptic hypergeometric functions', '27 pp., a complement to the book by G.E. Andrews, R. Askey, and R.\n  Roy, Special Functions, Encyclopedia of Math. Appl. 71, Cambridge Univ.\n  Press, Cambridge, 1999, written for its Russian edition: Moscow, MCCME, 2013,\n  pp. 577-606', '', '', '', 'math.CA', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  This is a brief overview of the status of the theory of elliptic\nhypergeometric functions to the end of 2012 written as a complementary chapter\nto the Russian edition of the book by G.E. Andrews, R. Askey, and R. Roy,\nSpecial Functions, Encycl. of Math. Appl. 71, Cambridge Univ. Press, 1999.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:25:31 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 28 Dec 2016 19:22:16 GMT\"}]', '2016-12-30', '[[\"Spiridonov\",\"V. P.\",\"\"]]'),
(704.3100, 'Kristian Finlator', 'K. Finlator, R. Dave', 'The Origin of the Galaxy Mass-Metallicity Relation and Implications for\n  Galactic Outflows', '28 pages, 15 figures, accepted by MNRAS with minor revisions. The\n  definitive version is available at www.blackell-synergy.com', '', '10.1111/j.1365-2966.2008.12991.x', '', 'astro-ph', '', '  (Abridged) Using cosmological hydrodynamic simulations in combination with\nanalytic modeling, we show that the galaxy stellar mass-metallicity relation\n(MZR) provides strong constraints on galactic outflows across cosmic time. We\ncompare three outflow models: No outflows, a \"constant wind\" (cw) model that\nemulates the popular Dekel & Silk (1986) scenario, and a ``momentum-driven\nwind\" (vzw) model. We find that only the vzw scaling reproduces the observed\nz~2 MZR\'s slope, amplitude, and scatter. Comparing our fully three-dimensional\nsimulations with a simple one-zone chemical evolution model, we find that the\nMZR can be understood in terms of three parameters: (1) The equilibrium\nmetallicity Z_eq=y*SFR/ACC (where y=true yield), reflecting the enrichment\nbalance between star formation rate SFR and gas accretion rate ACC; (2) the\ndilution time t_d=M_g/ACC, representing the timescale for a galaxy to return to\nZ_eq after a metallicity-perturbing interaction; and (3) the blowout mass\nM_blowout, which is the galaxy stellar mass above which winds can escape its\nhalo. When outflows with mass loading factor MLF are present, galaxies below\nM_blowout obey Z_eq = y/(1+MLF), while above M_blowout, Z_eq->y. Our cw model\nhas M_blowout ~ 10^10 M_sun, which yields a sharp upturn in the MZR above this\nscale and a flat MZR with large scatter below it, in strong disagreement with\nobservations. Our vzw model reproduces the observed Z_g \\propto M_*^0.3 because\nZ_eq \\propto MLF^-1 \\propto M_*^1/3 when MLF >> 1 (i.e. at low masses). The\nflattening of the MZR at M_* > 10^10.5 M_sun observed by Tremonti et al. (2004)\nreflects the mass scale where MLF~1, rather than a characteristic wind speed.\nThe tight observed MZR scatter is ensured when t_d<1 dynamical time, which is\nonly satisified at all masses and epochs in our momentum-driven wind model.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 01:11:35 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 22 Jan 2008 00:08:53 GMT\"}]', '2009-11-13', '[[\"Finlator\",\"K.\",\"\"],[\"Dave\",\"R.\",\"\"]]'),
(704.3101, 'Seung-il Nam', 'Seung-il Nam, Ki-Seok Choi, Atsushi Hosaka, Hyun-Chul Kim', 'A new candidate for non-strangeness pentaquarks: N*(1675)', '5 pages, 8 figures, Talk given at Yukawa International Seminar (YKIS)\n  2006 \"New frontiers in QCD\", 20 Nov. ~ 8 Dec. 2006, Yukawa Institute for\n  Theoretical Physics (YITP), Kyoto, Japan', 'Prog.Theor.Phys.Suppl.168:97-100,2007', '10.1143/PTPS.168.97', 'PNU-NTG-04/2007, PNU-NuRI-04/2007', 'hep-ph', '', '  We study a new nucleon resonance from eta photoproduction, which was observed\nat sqrt{s}=1675 MeV with a narrow decay width (~10 MeV) by the Tohoku LNS group\nas well as the GRAAL collaboration. Using an effective Lagrangian approach, we\ncompute differential cross sections for the eta photoproduction. In addition to\nN*(1675,1/2+-,3/2+-), we employ six other nucleon resonances, i.e.\nN*(1520,1535,1650,1675,1710,1720) and vector meson exchanges which are the most\nrelevant ones to this reaction process. As a result, we can reproduce the GRAAL\ndata qualitatively well and observe obvious isospin asymmetry between the\ntransition magnetic moments of N*(1675): mu_{gamma nn*} >> mu_{gamma pp*},\nwhich indicates that the newly found nucleon resonance may be identified as a\nnon-strange pentaquark state.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 01:33:54 GMT\"}]', '2008-11-26', '[[\"Nam\",\"Seung-il\",\"\"],[\"Choi\",\"Ki-Seok\",\"\"],[\"Hosaka\",\"Atsushi\",\"\"],[\"Kim\",\"Hyun-Chul\",\"\"]]'),
(704.3102, 'Hernando Quevedo', 'Hernando Quevedo', 'Geometrothermodynamics of black holes', 'Revised version, to be published in Gen.Rel.Grav.(Mashhoon\'s\n  Festschrift)', 'Gen.Rel.Grav.40:971-984,2008', '10.1007/s10714-007-0586-0', '', 'gr-qc', '', '  The thermodynamics of black holes is reformulated within the context of the\nrecently developed formalism of geometrothermodynamics. This reformulation is\nshown to be invariant with respect to Legendre transformations, and to allow\nseveral equivalent representations. Legendre invariance allows us to explain a\nseries of contradictory results known in the literature from the use of\nWeinhold\'s and Ruppeiner\'s thermodynamic metrics for black holes. For the\nReissner-Nordstr\\\"om black hole the geometry of the space of equilibrium states\nis curved, showing a non trivial thermodynamic interaction, and the curvature\ncontains information about critical points and phase transitions. On the\ncontrary, for the Kerr black hole the geometry is flat and does not explain its\nphase transition structure.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 01:37:35 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 2 Jul 2007 18:33:21 GMT\"}]', '2008-11-26', '[[\"Quevedo\",\"Hernando\",\"\"]]'),
(704.3103, 'Alexander O. Korotkevich', 'A.O. Korotkevich (1), A.C. Newell (2), and V.E. Zakharov (2,3,4,1)\n  ((1) Landau Institute for Theoretical Physics RAS, (2) Department of\n  Mathematics, University of Arizona, Tucson, (3) Lebedev Physical Institute\n  RAS, (4) Waves and Solitons LLC, Phoenix)', 'Communication through plasma sheaths', '30 pages, 18 figures', 'A.O. Korotkevich, A.C. Newell, and V.E. Zakharov, Communication\n  through plasma sheaths, J. Appl. Phys., vol. 102, issue 8, p. 083305 (2007)', '10.1063/1.2794856', '', 'physics.plasm-ph nlin.PS physics.space-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We wish to transmit messages to and from a hypersonic vehicle around which a\nplasma sheath has formed. For long distance transmission, the signal carrying\nthese messages must be necessarily low frequency, typically 2 GHz, to which the\nplasma sheath is opaque. The idea is to use the plasma properties to make the\nplasma sheath appear transparent.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 01:50:02 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 30 Dec 2010 14:53:39 GMT\"}]', '2011-01-04', '[[\"Korotkevich\",\"A. O.\",\"\"],[\"Newell\",\"A. C.\",\"\"],[\"Zakharov\",\"V. E.\",\"\"]]'),
(704.3104, 'Wako Aoki', 'Wako Aoki, Satoshi Honda, Kozo Sadakane, Nobuo Arimoto', 'The first determination of the actinide Th abundance for a red giant of\n  the Ursa Minor dwarf galaxy', '5 pages, 2 figures, 1 table, to appear in PASJ', '', '10.1093/pasj/59.3.L15', '', 'astro-ph', '', '  The Thorium abundance for the red giant COS82 in the Ursa Minor dwarf\nspheroidal galaxy is determined based on a high resolution spectrum. This is\nthe first detection of actinides in an extra Galactic object. A detailed\nabundance pattern is determined for 12 other neutron-capture elements from the\natomic number 39 to 68. These elements are significantly over-abundant with\nrespect to other metals like Fe (> 1 dex) and their abundance pattern agrees\nwell with those of the r-process-enhanced, very metal-poor stars known in the\nGalactic halo, while the metallicity of this object ([Fe/H] ~ -1.5) is much\nhigher than these field stars ([Fe/H] ~ -3.0). The results indicate that the\nmechanism and the astrophysical site that are responsible for neutron-capture\nelements in COS82 is similar to that for field r-process-enhanced stars, while\nthe condition of low mass star formation is quite different. An estimate of the\nage of this object based on the Th abundance ratio is discussed.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 01:52:22 GMT\"}]', '2015-05-13', '[[\"Aoki\",\"Wako\",\"\"],[\"Honda\",\"Satoshi\",\"\"],[\"Sadakane\",\"Kozo\",\"\"],[\"Arimoto\",\"Nobuo\",\"\"]]'),
(704.3105, 'Xing-Hua Wu', 'Xin-Heng Guo and Xing-Hua Wu', 'Studying the scalar bound states of the $K\\bar K$ system in the\n  Bethe-Salpeter formalism', '23 pages, LaTeX2e. Discussions on the legitimacy of the ladder\n  approximation and the instantaneous approximation are added. Recognized typos\n  have been corrected. Several references added', 'Phys.Rev.D76:056004,2007', '10.1103/PhysRevD.76.056004', '', 'hep-ph', '', '  We study the possible bound states of the $K\\bar K$ system in the\nBethe-Salpeter formalism in the ladder and instantaneous approximations. We\nfind that the bound states exist. However, these bound states have very small\ndecay widths. Therefore, besides the possible $K\\bar K$ component, there may be\nsome other structures in the observed $f_0(980)$ and $a_0(980)$ .\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 02:02:52 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Jul 2007 01:46:10 GMT\"}]', '2008-11-26', '[[\"Guo\",\"Xin-Heng\",\"\"],[\"Wu\",\"Xing-Hua\",\"\"]]'),
(704.3106, 'Keivan G. Stassun', 'Keivan G. Stassun, Robert D. Mathieu, Jeff A. Valenti', 'A Surprising Reversal of Temperatures in the Brown-Dwarf Eclipsing\n  Binary 2MASS J05352184-0546085', '31 pages, 7 figures, accepted by ApJ', 'Astrophys.J.664:1154-1166,2007', '10.1086/519231', '', 'astro-ph', '', '  The newly discovered brown-dwarf eclipsing binary 2MASS J05352184-0546085\nprovides a unique laboratory for testing the predictions of theoretical models\nof brown-dwarf formation and evolution. The finding that the lower-mass brown\ndwarf in this system is hotter than its higher-mass companion represents a\nchallenge to brown-dwarf evolutionary models, none of which predict this\nbehavior. Here we present updated determinations of the basic physical\nproperties of 2M0535-05, bolstering the surprising reversal of temperatures\nwith mass in this system. We compare these measurements with widely used\nbrown-dwarf evolutionary tracks, and find that the temperature reversal can be\nexplained by some models if the components of 2M0535-05 are mildly non-coeval,\npossibly consistent with dynamical simulations of brown-dwarf formation.\nAlternatively, a strong magnetic field on the higher-mass brown dwarf might\nexplain its anomalously low surface temperature, consistent with emerging\nevidence that convection is suppressed in magnetically active, low-mass stars.\nFinally, we discuss future observational and theoretical work needed to further\ncharacterize and understand this benchmark system.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 02:11:52 GMT\"}]', '2009-06-23', '[[\"Stassun\",\"Keivan G.\",\"\"],[\"Mathieu\",\"Robert D.\",\"\"],[\"Valenti\",\"Jeff A.\",\"\"]]'),
(704.3107, 'Guowu Meng', 'Guowu Meng', 'The Representation Aspect of the Generalized Hydrogen Atoms', '18 pages, simplified proof', 'Journal of Lie Theory 18 (2008), No. 3, 697-715', '', '', 'math-ph math.MP', '', '  Let $D\\ge 1$ be an integer. In the Enright-Howe-Wallach classification list\nof the unitary highest weight modules of $\\widetilde{\\mr{Spin}}(2, D+1)$, the\n(nontrivial) Wallach representations in Case II, Case III, and the mirror of\nCase III are special in the sense that they are precisely the ones that can be\nrealized by the Hilbert space of bound states for a generalized hydrogen atom\nin dimension D. It has been shown recently that each of these special Wallach\nrepresentations can be realized as the space of L^2-sections of a canonical\nhermitian bundle over the punctured ${\\bb R}^D$. Here a simple algebraic\ncharacterization of these special Wallach representations is found.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:08:01 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 05:58:13 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 26 Apr 2007 13:13:41 GMT\"},{\"version\":\"v4\",\"created\":\"Tue, 17 Jul 2007 06:05:03 GMT\"},{\"version\":\"v5\",\"created\":\"Thu, 9 Aug 2007 02:58:10 GMT\"},{\"version\":\"v6\",\"created\":\"Sat, 29 Dec 2007 06:46:41 GMT\"}]', '2008-11-29', '[[\"Meng\",\"Guowu\",\"\"]]'),
(704.3108, 'Tim Bastian', 'T. S. Bastian', 'Synchrotron Radio Emission from a Fast Halo Coronal Mass Ejection', '19 pages, 3 figures', 'Astrophys.J.665:805-812,2007', '10.1086/519246', '', 'astro-ph', '', '  An interplanetary (IP) type-II-like radio burst is analyzed. It occurred on\n2003 June 17-18 in association with a fast halo coronal mass ejection (CME), an\nM6.8 soft-X-ray (SXR) flare, and produced a solar proton event. Unlike coronal\ntype II bursts and the ma jority of IP type II radio emissions, the IP\ntype-II-like event associated with the fast halo CME on June 17-18 varies\nsmoothly in time and frequency and has a frequency bandwidth that is several\ntimes larger than is typical for coronal and IP type II emissions. Moreover,\nthe frequency change with time is inconsistent with that expected from plasma\nradiation associated with a CME-driven shock. I suggest that this IP\ntype-II-like event, referred to here as an IP type II-S event, is not due to\nplasma radiation but, rather, incoherent synchrotron radiation from\nnear-relativistic electrons entrained in the CME magnetic field, or in the\nsheath region between the shock and the CME driver. This event may be an\nexample of a new and distinct class of interplanetary radio phenomenon.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 02:19:24 GMT\"}]', '2009-06-23', '[[\"Bastian\",\"T. S.\",\"\"]]'),
(704.3109, 'Youichi Shibukawa', 'Youichi Shibukawa', 'Dynamical Yang-Baxter Maps with an Invariance Condition', '27 pages', '', '', '', 'math.QA math-ph math.MP', '', '  By means of left quasigroups L=(L, .) and ternary systems, we construct\ndynamical Yang-Baxter maps associated with L, L, and (.) satisfying an\ninvariance condition that the binary operation (.) of the left quasigroup L\ndefines. Conversely, this construction characterize such dynamical Yang-Baxter\nmaps. The unitary condition of the dynamical Yang-Baxter map is discussed.\nMoreover, we establish a correspondence between two dynamical Yang-Baxter maps\nconstructed in this paper. This correspondence produces a version of the\nvertex-IRF correspondence.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 02:55:08 GMT\"}]', '2007-05-23', '[[\"Shibukawa\",\"Youichi\",\"\"]]'),
(704.3110, 'Irene M. Gamba', 'Irene M. Gamba, Maria Pia Gualdani and Ping Zhang', 'On the blowing up of solutions to quantum hydrodynamic models on bounded\n  domains', '14 pages', '', '', '', 'math-ph math.AP math.MP', '', '  The blow-up in finite time for the solutions to the initial-boundary value\nproblem associated to the multi-dimensional quantum hydrodynamic model in a\nbounded domain is proved. The model consists on conservation of mass equation\nand a momentum balance equation equivalent to a compressible Euler equations\ncorrected by a dispersion term of the third order in the momentum balance. The\nproof is based on a-priori estimates for the energy functional for a new\nobservable constructed with an auxiliary function, and it is shown that, under\nsuitable boundary conditions and assumptions on the initial data, the solution\nblows up after a finite time.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 03:19:07 GMT\"}]', '2007-05-23', '[[\"Gamba\",\"Irene M.\",\"\"],[\"Gualdani\",\"Maria Pia\",\"\"],[\"Zhang\",\"Ping\",\"\"]]'),
(704.3111, 'M Zahid Hasan', 'Y.W. Li, D. Qian, L. Wray, D. Hsieh, Y. Kaga, T. Sasagawa, H. Takagi,\n  R.S. Markiewicz, A. Bansil, H. Eisaki, S. Uchida, M.Z. Hasan', 'Anisotropic softening of collective charge modes in the vicinity of\n  critical doping in a doped Mott insulator', '5 pages + 5 Figures', 'Phys. Rev. B 78, 073104 (2008)', '10.1103/PhysRevB.78.073104', '', 'cond-mat.str-el cond-mat.supr-con', '', '  Momentum resolved inelastic resonant x-ray scattering is used to map the\nevolution of charge excitations over a large range of energies, momenta and\ndoping levels in the electron doped Mott insulator class\nNd$_{2-x}$Ce$_x$CuO$_4$. As the doping induced AFM-SC\n(antiferromagnetic-superconducting) transition is approached, we observe an\nanisotropic softening of collective charge modes over a large energy scale\nalong the Gamma to (\\pi,\\pi)-direction, whereas the modes exhibit broadening\n($\\sim$ 1 eV) with relatively little softening along Gamma to (\\pi,0) with\nrespect to the parent Mott insulator (x=0). Our study indicates a systematic\ncollapse of the gap consistent with the scenario that the system dopes\nuniformly with electrons even though the softening of the modes involves an\nunusually large energy scale.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 03:20:53 GMT\"}]', '2008-12-11', '[[\"Li\",\"Y. W.\",\"\"],[\"Qian\",\"D.\",\"\"],[\"Wray\",\"L.\",\"\"],[\"Hsieh\",\"D.\",\"\"],[\"Kaga\",\"Y.\",\"\"],[\"Sasagawa\",\"T.\",\"\"],[\"Takagi\",\"H.\",\"\"],[\"Markiewicz\",\"R. S.\",\"\"],[\"Bansil\",\"A.\",\"\"],[\"Eisaki\",\"H.\",\"\"],[\"Uchida\",\"S.\",\"\"],[\"Hasan\",\"M. Z.\",\"\"]]'),
(704.3112, 'Mikko Karttunen', 'Emppu Salonen, Emma Terama, Ilpo Vattulainen, Mikko Karttunen', 'Enhanced dielectrophoresis of nanocolloids by dimer formation', '', '', '10.1209/0295-5075/78/48004', '', 'cond-mat.soft', '', '  We investigate the dielectrophoretic motion of charge-neutral, polarizable\nnanocolloids through molecular dynamics simulations. Comparison to analytical\nresults derived for continuum systems shows that the discrete charge\ndistributions on the nanocolloids have a significant impact on their coupling\nto the external field. Aggregation of nanocolloids leads to enhanced\ndielectrophoretic transport, provided that increase in the dipole moment upon\naggregation can overcome the related increase in friction. The dimer\norientation and the exact structure of the nanocolloid charge distribution are\nshown to be important in the enhanced transport.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 03:36:06 GMT\"}]', '2009-11-13', '[[\"Salonen\",\"Emppu\",\"\"],[\"Terama\",\"Emma\",\"\"],[\"Vattulainen\",\"Ilpo\",\"\"],[\"Karttunen\",\"Mikko\",\"\"]]'),
(704.3113, 'Rafe Mazzeo', 'Rafe Mazzeo, Mariel Saez', 'Self similar expanding solutions of the planar network flow', '14 pages', '', '', '', 'math.DG math.AP', '', '  We prove the existence of self-similar expanding solutions of the curvature\nflow on planar networks where the initial configuration is any number of\nhalf-lines meeting at the origin. This generalizes recent work by Schn\\\"urer\nand Schulze which treats the case of three half-lines. There are multiple\nsolutions, and these are parametrized by combinatorial objects, namely Steiner\ntrees with respect to a complete negatively curved metric on the unit ball\nwhich span $k$ specified points on the boundary at infinity. We also provide a\nsharp formulation of the regularity of these solutions at $t=0$.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 04:12:38 GMT\"}]', '2007-05-23', '[[\"Mazzeo\",\"Rafe\",\"\"],[\"Saez\",\"Mariel\",\"\"]]'),
(704.3114, 'Rina Kanamoto', 'Rina Kanamoto, Lincoln D. Carr, Masahito Ueda', 'Topological Winding and Unwinding in Metastable Bose-Einstein\n  Condensates', '4 pages, 3 figures', 'Phys. Rev. Lett. 100, 060401 (2008)', '10.1103/PhysRevLett.100.060401', '', 'cond-mat.other', '', '  Topological winding and unwinding in a quasi-one-dimensional metastable\n  Bose-Einstein condensate are shown to be manipulated by changing the strength\nof interaction or the frequency of rotation. Exact diagonalization analysis\nreveals that quasidegenerate states emerge spontaneously near the transition\npoint, allowing a smooth crossover between topologically distinct states. On a\nmean-field level, the transition is accompanied by formation of grey solitons,\nor density notches, which serve as an experimental signature of this\nphenomenon.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:32:09 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 6 Nov 2007 21:33:36 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 12 Feb 2008 19:38:07 GMT\"}]', '2009-11-13', '[[\"Kanamoto\",\"Rina\",\"\"],[\"Carr\",\"Lincoln D.\",\"\"],[\"Ueda\",\"Masahito\",\"\"]]'),
(704.3115, 'Tim Oliver Wehling', 'T. O. Wehling, H. P. Dahal, A. I. Lichtenstein, A. V. Balatsky', 'Local impurity effects in superconducting graphene', '4 pages, 4 figures', 'Phys. Rev. B 78, 035414 (2008)', '10.1103/PhysRevB.78.035414', '', 'cond-mat.mes-hall cond-mat.supr-con', '', '  We study the effect of impurities in superconducting graphene and discuss\ntheir influence on the local electronic properties. In particular, we consider\nthe case of magnetic and non-magnetic impurities being either strongly\nlocalized or acting as a potential averaged over one unit cell. The spin\ndependent local density of states is calculated and possibilities for\nvisualizing impurities by means of scanning tunneling experiments is pointed\nout. A possibility of identifying magnetic scatters even by non spin-polarized\nscanning tunneling spectroscopy is explained.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 04:45:36 GMT\"}]', '2008-09-17', '[[\"Wehling\",\"T. O.\",\"\"],[\"Dahal\",\"H. P.\",\"\"],[\"Lichtenstein\",\"A. I.\",\"\"],[\"Balatsky\",\"A. V.\",\"\"]]'),
(704.3116, 'Pawel Blasiak', 'P. Blasiak (1), A. Horzela (1), K. A. Penson (2), A. I. Solomon (2),\n  G. H. E. Duchamp (3), ((1) Polish Academy of Sciences, Krakow, Poland, (2)\n  LPTMC, University of Paris VI, France, (3) Institut Galilee, University of\n  Paris, France)', 'Combinatorics and Boson normal ordering: A gentle introduction', '8 pages, 1 figure', 'Am. J. Phys. 75, 639-646 (2007)', '10.1119/1.2723799', '', 'quant-ph math-ph math.CO math.MP', '', '  We discuss a general combinatorial framework for operator ordering problems\nby applying it to the normal ordering of the powers and exponential of the\nboson number operator. The solution of the problem is given in terms of Bell\nand Stirling numbers enumerating partitions of a set. This framework reveals\nseveral inherent relations between ordering problems and combinatorial objects,\nand displays the analytical background to Wick\'s theorem. The methodology can\nbe straightforwardly generalized from the simple example given herein to a wide\nclass of operators.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 04:46:59 GMT\"}]', '2009-11-13', '[[\"Blasiak\",\"P.\",\"\"],[\"Horzela\",\"A.\",\"\"],[\"Penson\",\"K. A.\",\"\"],[\"Solomon\",\"A. I.\",\"\"],[\"Duchamp\",\"G. H. E.\",\"\"]]'),
(704.3117, 'Michael Bromley', 'M.W.J. Bromley, J. Mitroy, K. Varga', 'Positronic complexes with unnatural parity', '10 pages RevTeX, 6 figures, in press Phys.Rev.A', 'Phys.Rev.A 75 062505 (2007)', '10.1103/PhysRevA.75.062505', 'CSRCR 2007-09', 'physics.atom-ph physics.chem-ph', '', '  The structure of the unnatural parity states of PsH, LiPs, NaPs and KPs are\ninvestigated with the configuration interaction and stochastic variational\nmethods. The binding energies (in hartree) are found to be 8.17x10-4,\n4.42x10-4, 15.14x10-4 and 21.80x10-4 respectively. These states are constructed\nby first coupling the two electrons into a configuration which is predominantly\n3Pe, and then adding a p-wave positron. All the active particles are in states\nin which the relative angular momentum between any pair of particles is at\nleast L = 1. The LiPs state is Borromean since there are no 3-body bound\nsubsystems (of the correct symmetry) of the (Li+, e-, e-, e+) particles that\nmake up the system. The dominant decay mode of these states will be radiative\ndecay into a configuration that autoionizes or undergoes positron annihilation.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 04:57:09 GMT\"}]', '2007-07-29', '[[\"Bromley\",\"M. W. J.\",\"\"],[\"Mitroy\",\"J.\",\"\"],[\"Varga\",\"K.\",\"\"]]'),
(704.3118, 'S. Ole Warnaar', 'S Ole Warnaar', 'Proof of the Flohr-Grabow-Koehn conjectures for characters of\n  logarithmic conformal field theory', '13 pages, 1 figure', 'J.Phys.A40:12243,2007', '10.1088/1751-8113/40/40/015', '', 'hep-th math-ph math.MP math.QA', '', '  In a recent paper Flohr, Grabow and Koehn conjectured that the characters of\nthe logarithmic conformal field theory c_{k,1}, of central charge\nc=1-6(k-1)^2/k, admit fermionic representations labelled by the Lie algebra\nD_k. In this note we provide a simple analytic proof of this conjecture.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 04:57:30 GMT\"}]', '2008-11-26', '[[\"Warnaar\",\"S Ole\",\"\"]]'),
(704.3119, 'Soumitra SenGupta', 'Saurya Das (U of Lethbridge), Anindya Dey (HRI, Allahabad), Soumitra\n  SenGupta (IACS, Kolkata)', 'Stability and hierarchy problems in string inspired braneworld scenarios', '5 Pages, Revtex. Minor changes. To appear in Europhysics Letters', 'Europhys.Lett.83:51002,2008', '10.1209/0295-5075/83/51002', '', 'hep-th gr-qc hep-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We generalise the RS braneworld model by taking into account a general\nstringy bulk containing the scalar dilaton field and the two-form Kalb-Ramond\nfield, apart from gravity. Assuming small fluctuations around a RS background,\nthe back-reacted warp factor is obtained. It is shown that the fine tuning\nproblem in connection with the Higgs mass reappears in a new guise and the\neffective modular potential fails to stabilise the braneworld.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 05:10:21 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 13 Aug 2008 00:11:36 GMT\"}]', '2008-11-26', '[[\"Das\",\"Saurya\",\"\",\"U of Lethbridge\"],[\"Dey\",\"Anindya\",\"\",\"HRI, Allahabad\"],[\"SenGupta\",\"Soumitra\",\"\",\"IACS, Kolkata\"]]'),
(704.3120, 'Oliver Henkel', 'Oliver Henkel', 'Space Time Codes from Permutation Codes', '', 'Proc. IEEE GlobeCom, San Francisco, California, Nov. 2006', '', '', 'cs.IT math.IT', '', '  A new class of space time codes with high performance is presented. The code\ndesign utilizes tailor-made permutation codes, which are known to have large\nminimal distances as spherical codes. A geometric connection between spherical\nand space time codes has been used to translate them into the final space time\ncodes. Simulations demonstrate that the performance increases with the block\nlengths, a result that has been conjectured already in previous work. Further,\nthe connection to permutation codes allows for moderate complex en-/decoding\nalgorithms.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 05:45:30 GMT\"}]', '2007-07-13', '[[\"Henkel\",\"Oliver\",\"\"]]'),
(704.3121, 'Hongsheng Zhang', 'Hongsheng Zhang, Zong-Hong Zhu and Lihua Yang', 'Hybrid Chaplygin gas and phantom divide crossing', '11 pages, 4 figures, V3: discussions on the perturbation growth\n  added, V4: minor corrections, to match the published version', 'Modern Physics Letters A, Vol. 24, No. 7 (2009) 541', '10.1142/S0217732309027303', 'BNU/0375-2007', 'astro-ph gr-qc hep-ph hep-th', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Hybrid Chaplygin gas model is put forward, in which the gases play the role\nof dark energy. For this model the coincidence problem is greatly alleviated.\nThe effective equation of state of the dark energy may cross the phantom divide\n$w=-1$. Furthermore, the crossing behaviour is decoupled from any gravity\ntheories. In the present model, $w<-1$ is only a transient behaviour. There is\na de Sitter attractor in the future infinity. Hence, the big rip singularity,\nwhich often afflicts the models with matter whose effective equation of state\nless than -1, is naturally disappear. There exist stable scaling solutions,\nboth at the early universe and the late universe. We discuss the perturbation\ngrowth of this model. We find that the index is consistent with observations.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:16:34 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 07:03:39 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 1 Apr 2009 06:29:10 GMT\"},{\"version\":\"v4\",\"created\":\"Wed, 17 Jun 2009 05:07:02 GMT\"}]', '2015-05-13', '[[\"Zhang\",\"Hongsheng\",\"\"],[\"Zhu\",\"Zong-Hong\",\"\"],[\"Yang\",\"Lihua\",\"\"]]'),
(704.3122, 'Jean Bertoin', 'Jean Bertoin (PMA, Dma)', 'Two-parameter Poisson-Dirichlet measures and reversible exchangeable\n  fragmentation-coalescence processes', '', '', '', '', 'math.PR', '', '  We show that for $0<\\alpha<1$ and $\\theta>-\\alpha$, the Poisson-Dirichlet\ndistribution with parameter $(\\alpha, \\theta)$ is the unique reversible\ndistribution of a rather natural fragmentation-coalescence process. This\ncompletes earlier results in the literature for certain split and merge\ntransformations and the parameter $\\alpha =0$.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:22:40 GMT\"}]', '2007-05-23', '[[\"Bertoin\",\"Jean\",\"\",\"PMA, Dma\"]]'),
(704.3123, 'Ivan Area', 'I. Area, M.K. Atakishiyeva, and J. Rodal', 'On factorization of $q$-difference equation for continuous\n  $q$-ultraspherical polynomials', '', '', '', '', 'math.CA math-ph math.MP', '', '  We prove that a customary Sturm-Liouville form of second-order $q$-difference\nequation for the continuous $q$-ultraspherical polynomials $C_n(x;\\beta| q)$ of\nRogers can be written in a factorized form in terms of some explicitly defined\n$q$-difference operator ${\\mathcal D}_x^{\\beta, q}$. This reveals the fact that\nthe continuous $q$-ultraspherical polynomials $C_n(x;\\beta| q)$ are actually\ngoverned by the $q$-difference equation ${\\mathcal D}_x^{\\beta, q} C_n(x;\\beta|\nq)= (q^{-n/2}+\\beta q^{n/2}) C_n(x;\\beta| q)$, which can be regarded as a\nsquare root of the equation, obtained from its original form.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:34:43 GMT\"}]', '2007-05-23', '[[\"Area\",\"I.\",\"\"],[\"Atakishiyeva\",\"M. K.\",\"\"],[\"Rodal\",\"J.\",\"\"]]'),
(704.3124, 'Massimiliano Morini', 'Filippo Cagnetti, Maria Giovanna Mora, Massimiliano Morini', 'A second order minimality condition for the Mumford-Shah functional', '30 pages', '', '', 'Preprint SISSA 82/2006/M', 'math.AP math.OC', '', '  A new necessary minimality condition for the Mumford-Shah functional is\nderived by means of second order variations. It is expressed in terms of a sign\ncondition for a nonlocal quadratic form on $H^1_0(\\Gamma)$, $\\Gamma$ being a\nsubmanifold of the regular part of the discontinuity set of the critical point.\nTwo equivalent formulations are provided: one in terms of the first eigenvalue\nof a suitable compact operator, the other involving a sort of nonlocal capacity\nof $\\Gamma$. A sufficient condition for minimality is also deduced. Finally, an\nexplicit example is discussed, where a complete characterization of the domains\nwhere the second variation is nonnegative can be given.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:39:26 GMT\"}]', '2007-05-23', '[[\"Cagnetti\",\"Filippo\",\"\"],[\"Mora\",\"Maria Giovanna\",\"\"],[\"Morini\",\"Massimiliano\",\"\"]]'),
(704.3125, 'Takehito Yokoyama', 'T. Yokoyama and Y. Tanaka', 'Theory of the tunneling spectroscopy of ferromagnetic superconductors', '4 pages, 2 figures', 'Phys. Rev. B 75, 132503 (2007)', '10.1103/PhysRevB.75.132503', '', 'cond-mat.supr-con', '', '  We study tunneling conductance in normal metal / insulator / ferromagnetic\nsuperconductor junctions. The tunneling spectra show a clear difference between\nspin-singlet s-wave pairing, spin-triplet opposite spin pairing and\nspin-triplet equal spin pairing: These pairings exhibit, respectively, gap\nstruture, double peak structure and zero bias peak in the spectra. The obtained\nresult may serve as a tool for determining the pairing symmetry of\nferromagnetic superconductors.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:41:38 GMT\"}]', '2015-05-13', '[[\"Yokoyama\",\"T.\",\"\"],[\"Tanaka\",\"Y.\",\"\"]]'),
(704.3126, 'Takehito Yokoyama', 'T. Yokoyama, Y. Sawa, Y. Tanaka, A. A. Golubov, A. Maeda and A.\n  Fujimaki', 'A quantitative model for IcR product in d-wave Josephson junctions', '4 pages, 6 figures', 'Phys. Rev. B 76, 052508 (2007)', '10.1103/PhysRevB.76.052508', '', 'cond-mat.supr-con', '', '  We study theoretically the Josephson effect in d-wave superconductor /\ndiffusive normal metal /insulator/ diffusive normal metal/ d-wave\nsuperconductor (D/DN/I/DN/D) junctions. This model is aimed to describe\npractical junctions in high-$T_C$ cuprate superconductors, in which the product\nof the critical Josephson current ($I_C$) and the normal state resistance ($R$)\n(the so-called $I_{\\rm C}R$ product) is very small compared to the prediction\nof the standard theory. We show that the $I_{\\rm C}R$ product in D/DN/I/DN/D\njunctions can be much smaller than that in d-wave superconductor / insulator /\nd-wave superconductor junctions and formulate the conditions necessary to\nachieve large $I_{\\rm C}R$ product in D/DN/I/DN/D junctions. The proposed\ntheory describes the behavior of $I_{\\rm C}R$ products quantitatively in\nhigh-$T_{\\rm C}$ cuprate junctions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 06:49:33 GMT\"}]', '2009-11-13', '[[\"Yokoyama\",\"T.\",\"\"],[\"Sawa\",\"Y.\",\"\"],[\"Tanaka\",\"Y.\",\"\"],[\"Golubov\",\"A. A.\",\"\"],[\"Maeda\",\"A.\",\"\"],[\"Fujimaki\",\"A.\",\"\"]]'),
(704.3127, 'Alberto Elduque', 'Alberto Elduque and Oliver Villa', 'The existence of superinvolutions', '21 pages', '', '', '', 'math.RA', '', '  Superinvolutions on graded associative algebras constitute a source of Lie\nand Jordan superalgebras. Graded versions of the classical Albert and\nAlbert-Riehm Theorems on the existence of superinvolutions are proven.\nSurprisingly, the existence of superinvolutions of the first kind is a rare\nphenomenon, as nontrivial central division superalgebras are never endowed with\nthis kind of superinvolutions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:07:50 GMT\"}]', '2007-05-23', '[[\"Elduque\",\"Alberto\",\"\"],[\"Villa\",\"Oliver\",\"\"]]'),
(704.3128, 'Li-Xin Li', 'Li-Xin Li (MPA)', 'Variation of the Amati Relation with the Cosmological Redshift: a\n  Selection Effect or an Evolution Effect?', '5 pages, including 5 figures. MNRAS Letters accepted', 'Mon.Not.Roy.Astron.Soc.Lett.379:L55-L59,2007', '10.1111/j.1745-3933.2007.00333.x', '', 'astro-ph', '', '  Because of the limit in the number of gamma-ray bursts (GRBs) with available\nredshifts and spectra, all current investigations on the correlation among GRB\nvariables use burst samples with redshifts that span a very large range. The\nevolution and selection effects have thus been ignored, which might have\nimportant influence on the results. In this Letter, we divide the 48\nlong-duration GRBs in Amati (2006, 2007) into four groups with redshift from\nlow to high, each group contains 12 GRBs. Then we fit each group with the Amati\nrelation $\\log E_\\iso = a + b \\log E_\\p$, and check if the parameters $a$ and\n$b$ evolve with the GRB redshift. We find that $a$ and $b$ vary with the mean\nredshift of the GRBs in each group systematically and significantly.\nMonte-Carlo simulations show that there is only $\\sim 4$ percent of chance that\nthe variation is caused by the selection effect arising from the fluence limit.\nHence, our results may indicate that GRBs evolve strongly with the cosmological\nredshift.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:25:53 GMT\"}]', '2009-06-23', '[[\"Li\",\"Li-Xin\",\"\",\"MPA\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3129, 'Vincent Sacksteder IV', 'Vincent E. Sacksteder IV', 'Sums over geometries and improvements on the mean field approximation', 'Accepted for publication in Physical Review D, probably in November\n  2007. At the reviewer\'s request, material was added which made the article\n  more assertive, confident, and clear. No changes in substance', 'Phys.Rev.D76:105032,2007', '10.1103/PhysRevD.76.105032', '', 'hep-th cond-mat.dis-nn cond-mat.stat-mech', '', '  The saddle points of a Lagrangian due to Efetov are analyzed. This Lagrangian\nwas originally proposed as a tool for calculating systematic corrections to the\nBethe approximation, a mean-field approximation which is important in\nstatistical mechanics, glasses, coding theory, and combinatorial optimization.\nDetailed analysis shows that the trivial saddle point generates a sum over\ngeometries reminiscent of dynamically triangulated quantum gravity, which\nsuggests new possibilities to design sums over geometries for the specific\npurpose of obtaining improved mean field approximations to $D$-dimensional\ntheories. In the case of the Efetov theory, the dominant geometries are locally\ntree-like, and the sum over geometries diverges in a way that is similar to\nquantum gravity\'s divergence when all topologies are included. Expertise from\nthe field of dynamically triangulated quantum gravity about sums over\ngeometries may be able to remedy these defects and fulfill the Efetov theory\'s\noriginal promise. The other saddle points of the Efetov Lagrangian are also\nanalyzed; the Hessian at these points is nonnormal and pseudo-Hermitian, which\nis unusual for bosonic theories. The standard formula for Gaussian integrals is\ngeneralized to nonnormal kernels.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:26:27 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 10 Nov 2007 12:58:54 GMT\"}]', '2012-12-13', '[[\"Sacksteder\",\"Vincent E.\",\"IV\"]]'),
(704.3130, 'Luigi Martina', 'Luigi Martina, Giulio Soliani', 'Hartree-Fock Approximation and Entanglement', '20 pages, 10 figures', '', '', '', 'quant-ph', '', '  The relation between the correlation energy and the entanglement is\nanalytically constructed for the Moshinsky\'s model of two coupled harmonic\noscillators. It turns out that the two quantities are far to be proportional,\neven at very small couplings. A comparison is made also with the 2-point Ising\nmodel.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:37:08 GMT\"}]', '2007-05-23', '[[\"Martina\",\"Luigi\",\"\"],[\"Soliani\",\"Giulio\",\"\"]]'),
(704.3131, 'Jose M. Diego Rodriguez', 'J.M. Diego, D. Herranz', 'Observing high redshift galaxy clusters through lensing of the\n  Ostriker-Vishniac effect', 'Submiteed to MNRAS', '', '10.1111/j.1365-2966.2007.12593.x', '', 'astro-ph', '', '  In this paper we study the possibility of detecting lensing signals in\nhigh-resolution and high-sensitivity CMB experiments. At scales below 1 arcmin,\nthe CMB background is dominated by the Sunyaev-Zel\'dovich effect in clusters\nand by Ostriker-Vishniac effect distortions elsewhere. Assuming the\nSunyaev-Zel\'dovich component in clusters can be removed, we focus on the\nOstriker-Vishniac effect and study the possibility of its detection while\npaying special attention to contaminants, such as instrumental noise and point\nsources. After designing an optimal filter for this particular lensing signal\nwe explore the signal-to-noise ratio for different scenarios varying the\nresolution of the experiment, its sensitivity, and the level of contamination\ndue to point sources. Our results show that the next generation of experiments\nshould be able to do new and exciting science through the lensing effect of the\nOstriker-Vishniac background.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:12:13 GMT\"}]', '2009-11-13', '[[\"Diego\",\"J. M.\",\"\"],[\"Herranz\",\"D.\",\"\"]]'),
(704.3132, 'Zhang Z.-H.', 'X.-H. Guo, Z.-H. Zhang', 'Direct CP violation in $\\bar{B}^0 \\to \\rho^0(\\omega)\\rho^0(\\omega) \\to\n  \\pi^+\\pi^-\\pi^+\\pi^-$', '26 pages,11figures', 'Phys.Rev.D75:074028,2007', '10.1103/PhysRevD.75.074028', '', 'hep-ph', '', '  We study the direct CP violation in $\\bar{B}^0 \\to\n\\rho^0(\\omega)\\rho^0(\\omega) \\to \\pi^+\\pi^-\\pi^+\\pi^-$ (with unpolarized\n$\\rho^0(\\omega)$) via the $\\rho-\\omega$ mixing mechanism which causes a large\nstrong phase difference and consequently a large CP violating asymmetry when\nthe masses of the $\\pi^+\\pi^-$ pairs are in the vicinity of the $\\omega$\nresonance. Since there are two $\\rho (\\omega)$ mesons in the intermediate state\n$\\rho-\\omega$ mixing contributes twice to the first order of isospin violation,\nleading to an even larger CP violating asymmetry (could be 30% -- 50% larger)\nthan in the case where only one $\\rho (\\omega)$ meson is involved. The CP\nviolating asymmetry depends on the Cabibbo-Kobayashi-Maskawa (CKM) matrix\nelements and the hadronic matrix elements. The factorization approach is\napplied in the calculation of the hadronic matrix elements with the\nnonfactorizable effects being included effectively in an effective parameter,\n$N_c$. We give the constraint on the range of $N_c$ from the latest\nexperimental data for the branching ratios for $\\bar{B}^0 \\to\\rho^0\\rho^0$ and\n$\\bar{B}^0 \\to\\rho^+\\rho^-$. We find that the CP violating asymmetry could be\nvery large (even more than 90% for some values of $N_c$). It is shown that the\nsensitivity of the CP violating asymmetry to $N_c$ is large compared with its\nsmaller sensitivity to the CKM matrix elements. We also discuss the possibility\nto remove the mod $(\\pi)$ ambiguity in the determination of the CP violating\nphase angle $\\alpha$ through the measurement of the CP violating asymmetry in\nthe decay $\\bar{B}^0\\to \\rho^0(\\omega)\\rho^0(\\omega) \\to \\pi^+\\pi^-\\pi^+\\pi^-$.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:42:57 GMT\"}]', '2011-03-15', '[[\"Guo\",\"X. -H.\",\"\"],[\"Zhang\",\"Z. -H.\",\"\"]]'),
(704.3133, 'James Stewart', 'The HERMES Collaboration: A. Airapetian, et al', 'Transverse Polarization of Lambda and Lambda-bar Hyperons in Quasireal\n  Photoproduction', '', 'Phys.Rev.D76:092008,2007', '10.1103/PhysRevD.76.092008', 'DESY 07-036', 'hep-ex', '', '  The HERMES experiment has measured the transverse polarization of Lambda and\nLambda-bar hyperons produced inclusively in quasireal photoproduction at a\npositron beam energy of 27.6 GeV. The transverse polarization of the Lambda\nhyperon is found to be positive while the observed Lambda-bar polarization is\ncompatible with zero. The transverse polarization values averaged over the\nkinematic acceptance of HERMES are 0.078 +/- 0.006(stat) +/- 0.012(syst) and\n-0.025 +/- 0.015(stat) +/- 0.018(syst) for Lambda and Lambda-bar hyperons,\nrespectively. The dependences of Lambda and Lambda-bar polarizations on the\nfraction $\\zeta$ of the beam\'s light-cone momentum carried by the hyperon and\non the hyperon\'s transverse momentum $p_T$ were investigated. The measured\nLambda polarization rises linearly with $p_T$ and exhibits a different behavior\nfor low and high values of $\\zeta$, which approximately correspond to the\nbackward and forward regions in the center-of-mass frame of the $\\gamma^*N$\nreaction.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:44:53 GMT\"}]', '2012-08-03', '[[\"The HERMES Collaboration\",\"\",\"\"],[\"Airapetian\",\"A.\",\"\"]]'),
(704.3134, 'Farook Rahaman', 'F. Rahaman, S.Mal and P. Ghosh', 'A study of global monopole in Lyra geometry', '6 pages, Published in Mod.Phys.Lett.A19:2785-2790,2004', '', '10.1142/S0217732304010862', '', 'gr-qc', '', '  A class of exact static solution around a global monopole resulting from the\nbreaking of a global S0(3) symmetry is obtained in the context of Lyra\ngeometry. Our solution is shown to possess an interesting feature like\nwormholes space-time. It has been shown that the global monopole exerts no\ngravitational force on surrounding non-relativistic matter.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:51:10 GMT\"}]', '2015-05-13', '[[\"Rahaman\",\"F.\",\"\"],[\"Mal\",\"S.\",\"\"],[\"Ghosh\",\"P.\",\"\"]]'),
(704.3135, 'Reza Rezaei', 'R. Rezaei, R. Schlichenmaier, W. Schmidt, and O. Steiner\n  (Kiepenheuer-Institut fuer Sonnenphysik, Freiburg, Germany)', 'Opposite magnetic polarity of two photospheric lines in single spectrum\n  of the quiet Sun', '4 pages, 5 figures, accepted in Astronomy & Astrophysics Letters', '', '10.1051/0004-6361:20077441', '', 'astro-ph', '', '  We study the structure of the photospheric magnetic field of the quiet Sun by\ninvestigating weak spectro-polarimetric signals. We took a sequence of Stokes\nspectra of the Fe I 630.15 nm and 630.25 nm lines in a region of quiet Sun near\nthe disk center, using the POLIS spectro-polarimeter at the German VTT on\nTenerife. The line cores of these two lines form at different heights in the\natmosphere. The 3$\\sigma$ noise level of the data is about 1.8 $\\times 10^{-3}\nI_{c}$. We present co-temporal and co-spatial Stokes-$V$ profiles of the Fe I\n630 nm line pair, where the two lines show opposite polarities in a single\nspectrum. We compute synthetic line profiles and reproduce these spectra with a\ntwo-component model atmosphere: a non-magnetic component and a magnetic\ncomponent. The magnetic component consists of two magnetic layers with opposite\npolarity: the upper one moves upwards while the lower one moves downward.\nIn-between, there is a region of enhanced temperature. The Stokes-$V$ line pair\nof opposite polarity in a single spectrum can be understood as a magnetic\nreconnection event in the solar photosphere. We demonstrate that such a\nscenario is realistic, but the solution may not be unique.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:38:51 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 16:27:08 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 9 May 2007 08:26:15 GMT\"}]', '2009-11-13', '[[\"Rezaei\",\"R.\",\"\",\"Kiepenheuer-Institut fuer Sonnenphysik, Freiburg, Germany\"],[\"Schlichenmaier\",\"R.\",\"\",\"Kiepenheuer-Institut fuer Sonnenphysik, Freiburg, Germany\"],[\"Schmidt\",\"W.\",\"\",\"Kiepenheuer-Institut fuer Sonnenphysik, Freiburg, Germany\"],[\"Steiner\",\"O.\",\"\",\"Kiepenheuer-Institut fuer Sonnenphysik, Freiburg, Germany\"]]'),
(704.3136, 'Hayk Sarkisyan A', 'E.M. Kazaryan, L.S. Petrosyan, H.A. Sarkisyan', 'Hidden Symmetry, Excitonic Transitions and Two-Dimensional Kane\'s\n  Exciton in the Quantum Well', '11 pages, grant number added', '', '', '', 'cond-mat.other cond-mat.mtrl-sci', '', '  In this article it is shown that, Sommerfeld\'s coefficients for excitonic\ntransitions in quantum wells are determined only with the principle quantum\nnumber within the framework of two-dimensional Coulomb potential. This is a\nconsequence of hidden symmetry of two-dimensional Coulomb problem, conditioned\nby the existence of two-dimensional analog of the Runge-Lentz vector. For the\nnarrow gap semiconductor quantum well with the non-parabolic dispersion law of\nelectron and hole in the two-band Kane model it is shown that two-dimensional\nexcitonic states are described in the frames of an analog of Klein-Gordon\nequation with the two-dimensional Coulomb potential. The non-stability of the\nground state of the two-dimensional Kane\'s exciton is show.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:55:48 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 29 May 2007 10:56:24 GMT\"}]', '2007-06-13', '[[\"Kazaryan\",\"E. M.\",\"\"],[\"Petrosyan\",\"L. S.\",\"\"],[\"Sarkisyan\",\"H. A.\",\"\"]]'),
(704.3137, 'Brenton Hall', 'M. Volk, S. Whitlock, B. V. Hall, A. I. Sidorov', 'Scanning magnetoresistance microscopy of atom chips', '6 pages, 6 figures', '', '10.1063/1.2839015', '', 'physics.atom-ph', '', '  Surface based geometries of microfabricated wires or patterned magnetic films\ncan be used to magnetically trap and manipulate ultracold neutral atoms or\nBose-Einstein condensates. We investigate the magnetic properties of such atom\nchips using a scanning magnetoresistive (MR) microscope with high spatial\nresolution and high field sensitivity. We show that MR sensors are ideally\nsuited to observe small variations of the magnetic field caused by\nimperfections in the wires or magnetic materials which ultimately lead to\nfragmentation of ultracold atom clouds. Measurements are also provided for the\nmagnetic field produced by a thin current-carrying wire with small geometric\nmodulations along the edge. Comparisons of our measurements with a full numeric\ncalculation of the current flow in the wire and the subsequent magnetic field\nshow excellent agreement. Our results highlight the use of scanning MR\nmicroscopy as a convenient and powerful technique for precisely characterizing\nthe magnetic fields produced near the surface of atom chips.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 07:58:46 GMT\"}]', '2009-11-13', '[[\"Volk\",\"M.\",\"\"],[\"Whitlock\",\"S.\",\"\"],[\"Hall\",\"B. V.\",\"\"],[\"Sidorov\",\"A. I.\",\"\"]]'),
(704.3138, 'Branislav Brutovsky', 'Branislav Brutovsky, Denis Horvath and Vladimir Lisy', 'Inverse Geometric Approach to the Simulation of the Circular Growth. The\n  Case of Multicellular Tumor Spheroids', '', '', '10.1016/j.physa.2007.10.036', '', 'q-bio.CB', '', '  We demonstrate the power of the genetic algorithms to construct the cellular\nautomata model simulating the growth of 2-dimensional close-to-circular\nclusters revealing the desired properties, such as the growth rate and, at the\nsame time, the fractal behavior of their contours. The possible application of\nthe approach in the field of tumor modeling is outlined.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:55:40 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 30 Jul 2007 11:05:50 GMT\"}]', '2009-11-13', '[[\"Brutovsky\",\"Branislav\",\"\"],[\"Horvath\",\"Denis\",\"\"],[\"Lisy\",\"Vladimir\",\"\"]]'),
(704.3139, 'Pietro Gambardella', 'G. Boero, S. Mouaziz, S. Rusponi, P. Bencok, F. Nolting, S. Stepanow,\n  and P. Gambardella', 'Element-resolved x-ray ferrimagnetic and ferromagnetic resonance\n  spectroscopy', '16 pages, 8 figures', 'New J. Phys. 10, 013011 (2008)', '10.1088/1367-2630/10/1/013011', '', 'cond-mat.mtrl-sci', '', '  We report on the measurement of element-specific magnetic resonance spectra\nat gigahertz frequencies using x-ray magnetic circular dichroism (XMCD). We\ninvestigate the ferrimagnetic precession of Gd and Fe ions in Gd-substituted\nYttrium Iron Garnet, showing that the resonant field and linewidth of Gd\nprecisely coincide with Fe up to the nonlinear regime of parametric\nexcitations. The opposite sign of the Gd x-ray magnetic resonance signal with\nrespect to Fe is consistent with dynamic antiferromagnetic alignment of the two\nionic species. Further, we investigate a bilayer metal film,\nNi$_{80}$Fe$_{20}$(5 nm)/Ni(50 nm), where the coupled resonance modes of Ni and\nNi$_{80}$Fe$_{20}$ are separately resolved, revealing shifts in the resonance\nfields of individual layers but no mutual driving effects. Energy-dependent\ndynamic XMCD measurements are introduced, combining x-ray absorption and\nmagnetic resonance spectroscopies.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:08:50 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 22 Jan 2008 12:55:16 GMT\"}]', '2008-01-22', '[[\"Boero\",\"G.\",\"\"],[\"Mouaziz\",\"S.\",\"\"],[\"Rusponi\",\"S.\",\"\"],[\"Bencok\",\"P.\",\"\"],[\"Nolting\",\"F.\",\"\"],[\"Stepanow\",\"S.\",\"\"],[\"Gambardella\",\"P.\",\"\"]]'),
(704.3140, 'Farook Rahaman', 'Farook Rahaman', 'Non static cosmic strings in Lyra geometry', '8 pages, Published in Nuovo Cim.118B:99-105,2003', '', '', '', 'gr-qc', '', '  The gravitational field of both local and global non static cosmic strings in\nthe context of Lyra geometry are investigated. Local strings are characterized\nby having an energy momentum tensor whose only non null components are $T_{tt}\n= T_{zz}$ . As linearized Einstein equations are formally analogous to the\nMaxwell equations, the exterior solution does not depend on the radial\ndistribution of the source and hence a Dirac d function was used to approximate\nthe radial distribution of the energy momentum tensor for a local cosmic string\nalong the z-axis: $T_{ab} = \\delta(x) \\delta(y)diag (\\sigma, 0, 0, \\sigma) $,\n$\\sigma $being the energy density of the string [A.Vilenkin.\nPhys.Rep.(1985)121,263]. For a global string, the energy momentum tensor\ncomponents are calculated from the action density for a complex scalar field y\nalong with a Maxican hat potential. The gravitational field of the global\nstring is shown to be attractive in nature.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:09:22 GMT\"}]', '2007-05-23', '[[\"Rahaman\",\"Farook\",\"\"]]'),
(704.3141, 'Evgueni Petrov', 'Evgueni Petrov', 'Algorithm for Evaluation of the Interval Power Function of Unconstrained\n  Arguments', '3 pages', '', '', '', 'cs.MS', '', '  We describe an algorithm for evaluation of the interval extension of the\npower function of variables x and y given by the expression x^y. Our algorithm\nreduces the general case to the case of non-negative bases.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:33:52 GMT\"}]', '2007-05-23', '[[\"Petrov\",\"Evgueni\",\"\"]]'),
(704.3142, 'Alastair Kay', 'Alastair Kay', 'A QMA-Complete Translationally Invariant Hamiltonian Problem and the\n  Complexity of Finding Ground State Energies in Physical Systems', '4 pages. v2: Significantly revised interpretation of results. v3:\n  updated references, added example class of Hamiltonians', 'Phys. Rev. A 76, 030307(R) (2007)', '10.1103/PhysRevA.76.030307', '', 'quant-ph cond-mat.str-el', '', '  Here we present a problem related to the local Hamiltonian problem\n(identifying whether the ground state energy falls within one of two ranges)\nwhich is restricted to being translationally invariant. We prove that for\nproblems with a fixed local dimension and O(\\log(N))-body local terms, or local\ndimension N and 2-body terms, there are instances of the problem which are\nQMA-complete. We discuss the implications for the computational complexity of\nfinding ground states of these systems, and hence for any classical\napproximation techniques that one could apply including DMRG, Matrix Product\nStates and MERA. One important example is a 1D lattice of bosons with\nnearest-neighbor hopping at constant filling fraction i.e. a generalization of\nthe Bose-Hubbard model.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:41:17 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 29 Apr 2007 14:10:03 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 29 May 2007 08:28:12 GMT\"}]', '2011-11-09', '[[\"Kay\",\"Alastair\",\"\"]]'),
(704.3143, 'Cosima Schuster', 'Udo Schwingenschloegl and Cosima Schuster', 'Charge redistribution at YBa2Cu3O7-metal interfaces', '3 pages, 2 figures, submitted to Appl. Phys. Lett', 'Appl. Phys. Lett., 192502 (2007)', '10.1063/1.2737397', '', 'cond-mat.supr-con', '', '  Charge redistribution at interfaces is crucial for electronic applications of\nhigh-Tc superconductors, since the band structure is modified on a local scale.\nWe address the normal-state electronic structure of YBa2Cu3O7 (YBCO) at an\nYBCO-metal contact by first principles calculations for prototypical interface\nconfigurations. We derive quantitative results for the intrinsic doping of the\nsuperconducting CuO2 planes due to the metal contact. Our findings can be\nexplained in terms of a band-bending mechanism, complemented by local screening\neffects. We determine a net charge transfer of 0.09 to 0.13 electrons in favour\nof the intraplane Cu sites, depending on the interface orientation.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:53:10 GMT\"}]', '2009-11-13', '[[\"Schwingenschloegl\",\"Udo\",\"\"],[\"Schuster\",\"Cosima\",\"\"]]'),
(704.3144, 'Yves Wiaux', 'Y. Wiaux, J. D. McEwen, P. Vielva', 'Complex data processing: fast wavelet analysis on the sphere', '20 pages, 5 figures, JFAA style, paper invited to J. Fourier Anal.\n  and Applic', 'J. Fourier Anal. and Applic. 13 (2007) 477', '10.1007/s00041-006-6917-9', '', 'astro-ph math-ph math.MP', '', '  In the general context of complex data processing, this paper reviews a\nrecent practical approach to the continuous wavelet formalism on the sphere.\nThis formalism notably yields a correspondence principle which relates wavelets\non the plane and on the sphere. Two fast algorithms are also presented for the\nanalysis of signals on the sphere with steerable wavelets.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 08:54:32 GMT\"}]', '2007-08-14', '[[\"Wiaux\",\"Y.\",\"\"],[\"McEwen\",\"J. D.\",\"\"],[\"Vielva\",\"P.\",\"\"]]'),
(704.3145, 'G\\\'abor Braun', 'Gabor Braun and Andras Nemethi', 'Surgery formula for Seiberg--Witten invariants of negative definite\n  plumbed 3-manifolds', '17 pages, 4 figures, accepted by Journal f\\\"ur die reine und\n  angewandte Mathematik. Minor improvements suggested by referee', '', '', '', 'math.GT math.AG', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We derive a cut-and-paste surgery formula of Seiberg--Witten invariants for\nnegative definite plumbed rational homology 3-spheres. It is similar to (and\nmotivated by) Okuma\'s recursion formula [arXiv:math.AG/0610464, 4.5] targeting\nanalytic invariants of splice quotient singularities. The two formulas combined\nprovide automatically a proof of the equivariant version\n[arXiv:math.AG/0310084, 5.2(b)] of the `Seiberg--Witten invariant conjecture\'\n[arXiv:math.AG/0111298] for these singularities.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 09:30:17 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 20 Nov 2008 13:29:10 GMT\"}]', '2008-11-20', '[[\"Braun\",\"Gabor\",\"\"],[\"Nemethi\",\"Andras\",\"\"]]'),
(704.3146, 'Thomas Schaepers', 'P. Lehnen, Th. Schapers, N. Kaluza, N. Thillosen, and H. Hardtdegen', 'Enhanced spin-orbit scattering length in narrow Al_xGa_{1-x}N/GaN wires', '6 pages, 5 figures', '', '10.1103/PhysRevB.76.205307', '', 'cond-mat.mes-hall', '', '  The magnetotransport in a set of identical parallel AlGaN/GaN quantum wire\nstructures was investigated. The width of the wires was ranging between 1110 nm\nand 340 nm. For all sets of wires clear Shubnikov--de Haas oscillations are\nobserved. We find that the electron concentration and mobility is approximately\nthe same for all wires, confirming that the electron gas in the AlGaN/GaN\nheterostructure is not deteriorated by the fabrication procedure of the wire\nstructures. For the wider quantum wires the weak antilocalization effect is\nclearly observed, indicating the presence of spin-orbit coupling. For narrow\nquantum wires with an effective electrical width below 250 nm the weak\nantilocalization effect is suppressed. By comparing the experimental data to a\ntheoretical model for quasi one-dimensional structures we come to the\nconclusion that the spin-orbit scattering length is enhanced in narrow wires.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 09:31:59 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 28 Jul 2007 11:57:09 GMT\"}]', '2009-11-13', '[[\"Lehnen\",\"P.\",\"\"],[\"Schapers\",\"Th.\",\"\"],[\"Kaluza\",\"N.\",\"\"],[\"Thillosen\",\"N.\",\"\"],[\"Hardtdegen\",\"H.\",\"\"]]'),
(704.3147, 'Boldizsar Kalmar', 'Boldizsar Kalmar', 'Fold cobordisms and stable homotopy groups', '10 pages', 'Stud. Scient. Math. Hung. 46 (2009), 437-447.', '', '', 'math.GT math.AT', '', '  We show that the cobordism groups of negative codimensional folds maps\ncontain direct sums of stable homotopy groups of Thom spaces of vector bundles\nlike the circle and the infinite dimensional projective space. We give\ngeometrical invariants which detect these direct summands.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 09:40:26 GMT\"}]', '2009-10-23', '[[\"Kalmar\",\"Boldizsar\",\"\"]]'),
(704.3148, 'Jose Luis Flores', 'V. Alana, J.L. Flores', 'The causal boundary of product spacetimes', '21 pages, 7 figures', 'Gen.Rel.Grav.39:1697-1718,2007', '10.1007/s10714-007-0492-5', '', 'gr-qc', '', '  The new formulation of the causal completion of spacetimes suggested in [1],\nand modified later in [2], is tested by computing the causal boundary for\nproduct spacetimes of a Lorentz interval and a Riemannian manifold. This is\nparticularized for two important families of spacetimes, conformal to the\nprevious ones: (standard) static spacetimes and Generalized Robertson-Walker\nspacetimes. As consequence, it is shown that this new approach essentially\nreproduces the structure of the conformal boundary for multiple classical\nspacetimes: Reissner-Nordstrom (including Schwarzschild), Anti-de Sitter, Taub\nand standard cosmological models as de Sitter and Einstein Universe.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 09:46:56 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 09:56:10 GMT\"}]', '2008-11-26', '[[\"Alana\",\"V.\",\"\"],[\"Flores\",\"J. L.\",\"\"]]'),
(704.3149, 'Pierre Lesaffre', 'P. Lesaffre, M. Gerin, P. Hennebelle', 'Effects of turbulent diffusion on the chemistry of diffuse clouds', '13 pages, 23 figures, A&A accepted', '', '10.1051/0004-6361:20066807', '', 'astro-ph', '', '  Aims. We probe the effect of turbulent diffusion on the chemistry at the\ninterface between a cold neutral medium (CNM) cloudlet and the warm neutral\nmedium (WNM). Methods. We perform moving grid, multifluid, 1D, hydrodynamical\nsimulations with chemistry including thermal and chemical diffusion. The\ndiffusion coefficients are enhanced to account for turbulent diffusion. We\npost-process the steady-states of our simulations with a crude model of\nradiative transfer to compute line profiles. Results. Turbulent diffusion\nspreads out the transition region between the CNM and the WNM. We find that the\nCNM slightly expands and heats up: its CH and H$_2$ content decreases due to\nthe lower density. The change of physical conditions and diffusive transport\nincrease the H$^+$ content in the CNM which results in increased OH and H$_2$O.\nDiffusion transports some CO out of the CNM. It also brings H$_2$ into contact\nwith the warm gas with enhanced production of CH$^+$, H$_3^+$, OH and H$_2$O at\nthe interface. O lines are sensitive to the spread of the thermal profile in\nthe intermediate region between the CNM and the WNM. Enhanced molecular content\nat the interface of the cloud broadens the molecular line profiles and helps\nexciting transitions of intermediate energy. The relative molecular yield are\nfound higher for bigger clouds. Conclusions. Turbulent diffusion can be the\nsource of additional molecular production and should be included in chemical\nmodels of the interstellar medium (ISM). It also is a good candidate for the\ninterpretation of observational problems such as warm H$_2$, CH$^+$ formation\nand presence of H$_3^+$.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 09:53:59 GMT\"}]', '2009-11-13', '[[\"Lesaffre\",\"P.\",\"\"],[\"Gerin\",\"M.\",\"\"],[\"Hennebelle\",\"P.\",\"\"]]'),
(704.3150, 'I. S. Glass', 'I. S. Glass, F. van Leeuwen', 'Semi-Regular Variables in the Solar Neighbourhood', 'MNRAS (accepted)', 'Mon.Not.Roy.Astron.Soc.378:1543-1549,2007', '10.1111/j.1365-2966.2007.11903.x', '', 'astro-ph', '', '  Period-luminosity sequences have been shown to exist among the Semi-Regular\nVariables (SRVs) in the Magellanic Clouds (Wood et al, 1999), the Bulge of the\nMilky Way galaxy (Glass & Schultheis, 2003) and elsewhere. Using modern period\nand revised Hipparcos parallax data, this paper demonstrates that they also\nappear among the M-giant SRVs of the Solar Neighbourhood. Their distribution in\nthe K, log P diagram resembles that of Bulge stars more closely than those in\nthe Magellanic Clouds. The prevalence of mass-loss among local M-type SRVs and\nits dependence on period and spectral sub-type are also discussed. K -- [12], a\nmeasure of circumstellar dust emission, increases clearly with V amplitude, M\ngiant sub-type and log P.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 09:57:42 GMT\"}]', '2009-06-23', '[[\"Glass\",\"I. S.\",\"\"],[\"van Leeuwen\",\"F.\",\"\"]]'),
(704.3151, 'Manuel Alonso-Moron', '\\\'Alvaro Mart\\\'inez P\\\'erez and M. A. Mor\\\'on', 'Uniformly continuous maps between ends of R-trees', '', '', '', '', 'math.GT math.MG', '', '  There is a well-known correspondence between infinite trees and ultrametric\nspaces which can be interpreted as an equivalence of categories and comes from\nconsidering the end space of the tree.\n  In this equivalence, uniformly continuous maps between the end spaces are\ntranslated to some classes of coarse maps (or even classes of metrically proper\nlipschitz maps) between the trees.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:02:10 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 18:15:31 GMT\"}]', '2007-05-23', '[[\"Pérez\",\"Álvaro Martínez\",\"\"],[\"Morón\",\"M. A.\",\"\"]]'),
(704.3152, 'Fabio Briscese', 'F. Briscese, A. Marciano', 'Cosmological Casimir effect with maximum planckian momentum and\n  accelerating universe', '9 pages', '', '', '', 'gr-qc astro-ph hep-th', '', '  We develop here a mechanism that, without making use of a cosmological\nconstant, reproduces an accelerating universe. This is done by taking into\naccount Casimir vacuum energy density, assuming that the underlying theory\nallows a maximum momentum, that turns out to be the leading contribution term\nto Einstein equations in a large expanding FRW universe. As stated in numerous\nquantum gravity studies, we postulate that maximum momentum is related to the\nexistence of the Planck length as a fundamental length. This insight, together\nwith the assumption of a Planck scale correction to the energy/momentum\ndispersion-relation on a FRW background, is used here to calculate Casimir\nvacuum energy. We show that, under these hypothesis, an accelerated universe\nexpansion is obtained. As last step we analyze the compatibility of the\nresulting model with experimental data, writing down the equation of state for\nCasimir energy and pressure and observing that this equation of state belongs\nto a class of models that naturally fits cosmological observations. We\nemphasize that our result relies, once a fundamental length is introduced in\nCasimir effect, just on general arguments thus it is independent on an explicit\nform of the energy-momentum dispersion relation.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:08:00 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 24 Apr 2007 23:20:13 GMT\"},{\"version\":\"v3\",\"created\":\"Sat, 5 May 2007 15:00:29 GMT\"}]', '2007-05-23', '[[\"Briscese\",\"F.\",\"\"],[\"Marciano\",\"A.\",\"\"]]'),
(704.3153, 'Zhi-Zhong Xing', 'Aik Hui Chan, Harald Fritzsch, Shu Luo, Zhi-zhong Xing', 'Deviations from Tri-bimaximal Neutrino Mixing in Type-II Seesaw and\n  Leptogenesis', 'RevTeX 14 pages, 2 figures. Title and authors changed, and\n  discussions on the minimal type-II seesaw and leptogenesis added. Accepted\n  for publication in Phys. Rev. D', 'Phys.Rev.D76:073009,2007', '10.1103/PhysRevD.76.073009', '', 'hep-ph', '', '  Current experimental data allow the zero value for one neutrino mass, either\nm_1 = 0 or m_3 = 0. This observation implies that a realistic neutrino mass\ntexture can be established by starting from the limit (a) m_1 = m_2 = 0 and m_3\n\\neq 0 or (b) m_1 = m_2 \\neq 0 and m_3 = 0. In both cases, we may introduce a\nparticular perturbation which ensures the resultant neutrino mixing matrix to\nbe the tri-bimaximal mixing pattern or its viable variations with all entries\nbeing formed from small integers and their square roots. We find that it is\nnatural to incorporate this kind of neutrino mass matrix in the minimal Type-II\nseesaw model with only one heavy right-handed Majorana neutrino N in addition\nto the SU(2)_L Higgs triplet \\Delta_L. We show that it is possible to account\nfor the cosmological baryon number asymmetry in the m_3 =0 case via thermal\nleptogenesis, in which the one-loop vertex correction to N decays is mediated\nby \\Delta_L and the CP-violating asymmetry of N decays is attributed to the\nelectron flavor.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:08:25 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 5 Sep 2007 10:28:03 GMT\"}]', '2008-11-26', '[[\"Chan\",\"Aik Hui\",\"\"],[\"Fritzsch\",\"Harald\",\"\"],[\"Luo\",\"Shu\",\"\"],[\"Xing\",\"Zhi-zhong\",\"\"]]'),
(704.3154, 'Andrea Ciardi Dr', 'D.J. Ampleford (1), S.V. Lebedev (2), A. Ciardi (3), S.N. Bland (2),\n  S.C. Bott (2), G.N. Hall (2), N. Naz (2), C.A. Jennings (1), M. Sherlock (2),\n  J.P. Chittenden (2), J.B.A.Palmer (2), A. Frank (4), E. Blackman (4) ((1)\n  Sandia National Laboratories, USA (2) Imperial College, UK (3) Observatoire\n  de Paris, France (4) Department of Physics and Astronomy, and Laboratory for\n  Laser Energetics, University of Rochester, USA)', 'Supersonic radiatively cooled rotating flows and jets in the laboratory', 'Accepted for publication in Physical Review Letters (16 pages, 5\n  figures)', '', '10.1103/PhysRevLett.100.035001', '', 'astro-ph', '', '  The first laboratory astrophysics experiments to produce a radiatively cooled\nplasma jet with dynamically significant angular momentum are discussed. A new\nconfiguration of wire array z-pinch, the twisted conical wire array, is used to\nproduce convergent plasma flows each rotating about the central axis. Collision\nof the flows produces a standing shock and jet that each have supersonic\nazimuthal velocities. By varying the twist angle of the array, the rotation\nvelocity of the system can be controlled, with jet rotation velocities reaching\n~20% of the propagation velocity.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:04:15 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 2 Jan 2008 10:07:26 GMT\"}]', '2009-11-13', '[[\"Ampleford\",\"D. J.\",\"\"],[\"Lebedev\",\"S. V.\",\"\"],[\"Ciardi\",\"A.\",\"\"],[\"Bland\",\"S. N.\",\"\"],[\"Bott\",\"S. C.\",\"\"],[\"Hall\",\"G. N.\",\"\"],[\"Naz\",\"N.\",\"\"],[\"Jennings\",\"C. A.\",\"\"],[\"Sherlock\",\"M.\",\"\"],[\"Chittenden\",\"J. P.\",\"\"],[\"Palmer\",\"J. B. A.\",\"\"],[\"Frank\",\"A.\",\"\"],[\"Blackman\",\"E.\",\"\"]]'),
(704.3155, 'Charalampos Skokos', 'Ch. Skokos, T.C. Bountis and Ch. Antonopoulos', 'Geometrical properties of local dynamics in Hamiltonian systems: the\n  Generalized Alignment Index (GALI) method', '45 pages, 10 figures, accepted for publication in Physica D', '', '10.1016/j.physd.2007.04.004', '', 'nlin.CD math-ph math.DS math.MP math.SG physics.acc-ph physics.class-ph physics.comp-ph', '', '  We investigate the detailed dynamics of multidimensional Hamiltonian systems\nby studying the evolution of volume elements formed by unit deviation vectors\nabout their orbits. The behavior of these volumes is strongly influenced by the\nregular or chaotic nature of the motion, the number of deviation vectors, their\nlinear (in)dependence and the spectrum of Lyapunov exponents. The different\ntime evolution of these volumes can be used to identify rapidly and efficiently\nthe nature of the dynamics, leading to the introduction of quantities that\nclearly distinguish between chaotic behavior and quasiperiodic motion on\n$N$-dimensional tori. More specifically we introduce the Generalized Alignment\nIndex of order $k$ (GALI$_k$) as the volume of a generalized parallelepiped,\nwhose edges are $k$ initially linearly independent unit deviation vectors from\nthe studied orbit whose magnitude is normalized to unity at every time step.\nThe GALI$_k$ is a generalization of the Smaller Alignment Index (SALI)\n(GALI$_2$ $\\propto$ SALI). However, GALI$_k$ provides significantly more\ndetailed information on the local dynamics, allows for a faster and clearer\ndistinction between order and chaos than SALI and works even in cases where the\nSALI method is inconclusive.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:53:04 GMT\"}]', '2019-08-19', '[[\"Skokos\",\"Ch.\",\"\"],[\"Bountis\",\"T. C.\",\"\"],[\"Antonopoulos\",\"Ch.\",\"\"]]'),
(704.3156, 'Alan Sokal', 'Thierry de la Rue, Roberto Fernandez, Alan D. Sokal', 'How to clean a dirty floor: Probabilistic potential theory and the\n  Dobrushin uniqueness theorem', 'LaTex2e, 80 pages including 4 figures', 'Markov Processes and Related Fields 14, 1--78 (2008)', '', '', 'math.PR math-ph math.MP', '', '  Motivated by the Dobrushin uniqueness theorem in statistical mechanics, we\nconsider the following situation: Let \\alpha be a nonnegative matrix over a\nfinite or countably infinite index set X, and define the \"cleaning operators\"\n\\beta_h = I_{1-h} + I_h \\alpha for h: X \\to [0,1] (here I_f denotes the\ndiagonal matrix with entries f). We ask: For which \"cleaning sequences\" h_1,\nh_2, ... do we have c \\beta_{h_1} ... \\beta_{h_n} \\to 0 for a suitable class of\n\"dirt vectors\" c? We show, under a modest condition on \\alpha, that this occurs\nwhenever \\sum_i h_i = \\infty everywhere on X. More generally, we analyze the\ncleaning of subsets \\Lambda \\subseteq X and the final distribution of dirt on\nthe complement of \\Lambda. We show that when supp(h_i) \\subseteq \\Lambda with\n\\sum_i h_i = \\infty everywhere on \\Lambda, the operators \\beta_{h_1} ...\n\\beta_{h_n} converge as n \\to \\infty to the \"balayage operator\" \\Pi_\\Lambda =\n\\sum_{k=0}^\\infty (I_\\Lambda \\alpha)^k I_{\\Lambda^c). These results are\nobtained in two ways: by a fairly simple matrix formalism, and by a more\npowerful tree formalism that corresponds to working with formal power series in\nwhich the matrix elements of \\alpha are treated as noncommuting indeterminates.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:43:28 GMT\"}]', '2008-07-25', '[[\"de la Rue\",\"Thierry\",\"\"],[\"Fernandez\",\"Roberto\",\"\"],[\"Sokal\",\"Alan D.\",\"\"]]'),
(704.3157, 'Giorgio Terracina', 'Giorgio Terracina, Nicola Leone, Vincenzino Lio, Claudio Panetta', 'Experimenting with recursive queries in database and logic programming\n  systems', 'To appear in Theory and Practice of Logic Programming (TPLP)', '', '', '', 'cs.AI cs.DB', '', '  This paper considers the problem of reasoning on massive amounts of (possibly\ndistributed) data. Presently, existing proposals show some limitations: {\\em\n(i)} the quantity of data that can be handled contemporarily is limited, due to\nthe fact that reasoning is generally carried out in main-memory; {\\em (ii)} the\ninteraction with external (and independent) DBMSs is not trivial and, in\nseveral cases, not allowed at all; {\\em (iii)} the efficiency of present\nimplementations is still not sufficient for their utilization in complex\nreasoning tasks involving massive amounts of data. This paper provides a\ncontribution in this setting; it presents a new system, called DLV$^{DB}$,\nwhich aims to solve these problems. Moreover, the paper reports the results of\na thorough experimental analysis we have carried out for comparing our system\nwith several state-of-the-art systems (both logic and databases) on some\nclassical deductive problems; the other tested systems are: LDL++, XSB, Smodels\nand three top-level commercial DBMSs. DLV$^{DB}$ significantly outperforms even\nthe commercial Database Systems on recursive queries. To appear in Theory and\nPractice of Logic Programming (TPLP)\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:58:40 GMT\"}]', '2007-05-23', '[[\"Terracina\",\"Giorgio\",\"\"],[\"Leone\",\"Nicola\",\"\"],[\"Lio\",\"Vincenzino\",\"\"],[\"Panetta\",\"Claudio\",\"\"]]'),
(704.3158, 'Jason McEwen', 'J. D. McEwen, P. Vielva, Y. Wiaux, R. B. Barreiro, L. Cayon, M. P.\n  Hobson, A. N. Lasenby, E. Martinez-Gonzalez, J. L. Sanz', 'Cosmological applications of a wavelet analysis on the sphere', '17 pages, 8 figures; JFAA invited review, in press', 'J. Fourier Anal. and Appl. 13 (2007) 495-510', '10.1007/s00041-006-6918-8', '', 'astro-ph math-ph math.MP', '', '  The cosmic microwave background (CMB) is a relic radiation of the Big Bang\nand as such it contains a wealth of cosmological information. Statistical\nanalyses of the CMB, in conjunction with other cosmological observables,\nrepresent some of the most powerful techniques available to cosmologists for\nplacing strong constraints on the cosmological parameters that describe the\norigin, content and evolution of the Universe. The last decade has witnessed\nthe introduction of wavelet analyses in cosmology and, in particular, their\napplication to the CMB. We review here spherical wavelet analyses of the CMB\nthat test the standard cosmological concordance model. The assumption that the\ntemperature anisotropies of the CMB are a realisation of a statistically\nisotropic Gaussian random field on the sphere is questioned. Deviations from\nboth statistical isotropy and Gaussianity are detected in the reviewed works,\nsuggesting more exotic cosmological models may be required to explain our\nUniverse. We also review spherical wavelet analyses that independently provide\nevidence for dark energy, an exotic component of our Universe of which we know\nvery little currently. The effectiveness of accounting correctly for the\ngeometry of the sphere in the wavelet analysis of full-sky CMB data is\ndemonstrated by the highly significant detections of physical processes and\neffects that are made in these reviewed works.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:45:37 GMT\"}]', '2007-08-17', '[[\"McEwen\",\"J. D.\",\"\"],[\"Vielva\",\"P.\",\"\"],[\"Wiaux\",\"Y.\",\"\"],[\"Barreiro\",\"R. B.\",\"\"],[\"Cayon\",\"L.\",\"\"],[\"Hobson\",\"M. P.\",\"\"],[\"Lasenby\",\"A. N.\",\"\"],[\"Martinez-Gonzalez\",\"E.\",\"\"],[\"Sanz\",\"J. L.\",\"\"]]'),
(704.3159, 'Henny Lamers', 'Henny J.G.L.M. Lamers', 'Mass Loss and Evolution of Stars and Star Clusters: a Personal\n  Historical Perspective', 'submitted to: Mass Loss from Stars and the Evolution of Stellar\n  Clusters, ASP Conf. Series, Eds. A. de Koter, L. Smith, R. Waters', '', '', '', 'astro-ph', '', '  The development and progress of the studies of winds and mass loss from hot\nstars, from about 1965 up to now, is discussed in a personal historical\nperspective. The present state of knowledge about stellar winds, based on\npapers presented at this workshop, is described. About ten years ago the\nmechanisms of the winds were reasonably well understood, the mass loss rates\nwere known, and the predictions of stellar evolution theory with mass loss\nagreed with observations. However, recent studies especially those based on\nFUSE observations, have resulted in a significant reduction of the mass loss\nrates, that disagrees with predictions from radiation driven wind models. The\nsituation is discussed and future studies that can clarify the situation are\nsuggested.\n  I also discuss what is known about the dissolution of star clusters in\ndifferent environments. The dissolution time can be derived from the mass and\nage distributions of cluster samples. The resulting dissolution times of\nclusters in the solar neighborhood (SN) and in interacting galaxies are shorter\nthan predicted by two-body relaxation of clusters in a tidal field. Encounters\nwith giant molecular clouds can explain the fate of clusters in the SN and are\nthe most likely cause of the short lifetime of clusters in interacting\ngalaxies.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 10:57:56 GMT\"}]', '2007-05-23', '[[\"Lamers\",\"Henny J. G. L. M.\",\"\"]]'),
(704.3160, 'Davoud Kamani', 'Davoud Kamani', 'New Form of the T-Duality Due to the Stability of a Compact Dimension', '12 pages, Latex, no figure', 'Int. J. Theor. Phys. 48, 611-620 (2009)', '10.1007/s10773-008-9834-7', '', 'hep-th', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We study behaviors of a compact dimension and the $T$-duality, in the\npresence of the wrapped closed bosonic strings. When the closed strings\ninteract and form another system of strings, the radius of compactification\nincreases. This modifies the $T$-duality, which we call it as $T$-duality-like.\nSome effects of the $T$-duality-like will be studied.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:00:15 GMT\"},{\"version\":\"v2\",\"created\":\"Sun, 31 Aug 2008 08:28:02 GMT\"}]', '2020-08-21', '[[\"Kamani\",\"Davoud\",\"\"]]'),
(704.3161, 'Baruch Meerson', 'Rui Liu, Yinchang Li, Meiying Hou, Baruch Meerson', 'van der Waals-like phase separation instability of a driven granular gas\n  in three dimensions', '7 pages, 7 figures, to appear in Phys. Rev. E', 'Phys. Rev. E 75 , 061304 (2007)', '', '', 'cond-mat.soft nlin.PS physics.flu-dyn', '', '  We show that the van der Waals-like phase separation instability of a driven\ngranular gas at zero gravity, previously investigated in two-dimensional\nsettings, persists in three dimensions. We consider a monodisperse granular gas\ndriven by a thermal wall of a three-dimensional rectangular container at zero\ngravity. The basic steady state of this system, as described by granular\nhydrodynamic equations, involves a denser and colder layer of granulate located\nat the wall opposite to the driving wall. When the inelastic energy loss is\nsufficiently high, the driven granular gas exhibits, in some range of average\ndensities, negative compressibility in the directions parallel to the driving\nwall. When the lateral dimensions of the container are sufficiently large, the\nnegative compressibility causes spontaneous symmetry breaking of the basic\nsteady state and a phase separation instability. Event-driven molecular\ndynamics simulations confirm and complement our theoretical predictions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:00:47 GMT\"}]', '2015-12-07', '[[\"Liu\",\"Rui\",\"\"],[\"Li\",\"Yinchang\",\"\"],[\"Hou\",\"Meiying\",\"\"],[\"Meerson\",\"Baruch\",\"\"]]'),
(704.3162, 'Urpin Vadim', 'V.Urpin', 'Neutrino transport and hydrodynamic stability of rotating proto-neutron\n  stars', '6 pages. Accepted for publication in A&A', '', '10.1051/0004-6361:20066258', '', 'astro-ph', '', '  We consider stability of differentially rotating non-magnetic proto-neutron\nstars. When neutrino transport is efficient, the star can be subject to a\ndiffusive instability that can occur even in the convectively stable region.\nThe instability arises on the time-scale comparable to the time-scale of\nthermal diffusion. Hydrodynamic motions driven by the instability can lead to\nanisotropy in the neutrino flux since the instability is suppressed near the\nequator and rotation axis.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:09:01 GMT\"}]', '2009-11-13', '[[\"Urpin\",\"V.\",\"\"]]'),
(704.3163, 'Thomas Dedieu', 'Thomas Dedieu', 'Severi varieties and self rational maps of K3 surfaces', '20 pages', 'Internat. J. Math., 20(12): 1455-1477, 2009', '', '', 'math.AG', '', '  Self-rational maps of generic algebraic K3 surfaces are conjectured to be\ntrivial. We relate this conjecture to a conjecture concerning the\nirreducibility of the universal Severi varieties parametrizing nodal curves of\ngiven genus and degree lying on some K3 surface. We also establish a number of\nnumerical constraints satisfied by such non trivial rational maps, that is of\ntopological degree >1.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:15:22 GMT\"}]', '2010-09-20', '[[\"Dedieu\",\"Thomas\",\"\"]]'),
(704.3164, 'George Savvidy K', 'Jessica K. Barrett and George Savvidy', 'A dual lagrangian for non-Abelian tensor gauge fields', '13 pages, LaTex file', 'Phys.Lett.B652:141-145,2007', '10.1016/j.physletb.2007.07.009', 'NRCPS-HE-54-07 and RH-02-2007', 'hep-th', '', '  For non-Abelian tensor gauge fields of the lower rank we have found an\nalternative expression for the field strength tensors, which transform\nhomogeneously with respect to the complementary gauge transformations and allow\nus to construct the dual Lagrangian.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:17:37 GMT\"}]', '2008-11-26', '[[\"Barrett\",\"Jessica K.\",\"\"],[\"Savvidy\",\"George\",\"\"]]'),
(704.3165, 'Peter Blake', 'E. W. Hill, A. K. Geim, K. Novoselov, F. Schedin and P. Blake', 'Graphene Spin Valve Devices', '3 pages, 6 figures', 'IEEE Trans. Magn. 42, 2694-2696 (2006)', '10.1109/TMAG.2006.878852', '', 'cond-mat.mes-hall', '', '  Graphene - a single atomic layer of graphite - is a recently-found\ntwo-dimensional form of carbon, which exhibits high crystal quality and\nballistic electron transport at room temperature. Soft magnetic NiFe electrodes\nhave been used to inject polarized spins into graphene and a 10% change in\nresistance has been observed as the electrodes switch from the parallel to the\nantiparallel state. This coupled with the fact that a field effect electrode\ncan modulate the conductivity of these graphene films makes them exciting\npotential candidates for spin electronic devices.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:21:34 GMT\"}]', '2019-08-19', '[[\"Hill\",\"E. W.\",\"\"],[\"Geim\",\"A. K.\",\"\"],[\"Novoselov\",\"K.\",\"\"],[\"Schedin\",\"F.\",\"\"],[\"Blake\",\"P.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3166, 'Margarida Hernanz', 'M. Hernanz (IEEC/Csic) and G. Sala (MPE)', 'XMM-Newton observations of Nova Sgr 1998', '18 pages, 3 figures. Accepted in Astrophysical Journal', 'Astrophys.J.664:467-473,2007', '10.1086/518780', '', 'astro-ph', '', '  We report on X-ray observations of Nova Sagittarius 1998 (V4633 Sgr),\nperformed with XMM-Newton at three different epochs, 934, 1083 and 1265 days\nafter discovery. The nova was detected with the EPIC cameras at all three\nepochs, with emission spanning the whole energy range from 0.2 to 10 keV.\n  The X-ray spectra do not change significantly at the different epochs, and\nare well fitted for the first and third observations with a multi-temperature\noptically thin thermal plasma, while lower statistics in the second\nobservations lead to a poorer fit. The thermal plasma emission is most probably\noriginated in the shock heated ejecta, with chemical composition similar to\nthat of a CO nova. However, we can not completely rule out reestablished\naccretion as the origin of the emission. We also obtain upper limits for the\ntemperature and luminosity of a potential white dwarf atmospheric component,\nand conclude that hydrogen burning had already turned-off by the time of our\nobservations.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:23:32 GMT\"}]', '2009-06-23', '[[\"Hernanz\",\"M.\",\"\",\"IEEC/Csic\"],[\"Sala\",\"G.\",\"\",\"MPE\"]]'),
(704.3167, 'Pekko Mets\\\"a', 'V.V. Abaev, P. Mets\\\"a, and M.E. Sainio', 'The Goldberger-Miyazawa-Oehme sum rule revisited', '4 pages, 1 figure. v2: Revised the second last paragraph of 5th\n  section and clarified the electromagnetic corrections (Tromborg vs.\n  $\\chi$PT). Also removed the KH80 slope from the fig. 1', 'Eur.Phys.J.A32:321-325,2007', '10.1140/epja/i2007-10377-6', 'HIP-2007-16/TH', 'hep-ph', '', '  The Goldberger-Miyazawa-Oehme sum rule is used to extract the pion-nucleon\ncoupling constant from experimental $\\pi$N information. Chiral perturbation\ntheory is exploited in relating the pionic hydrogen s-wave level shift and\nwidth results to the appropriate scattering lengths. The deduced value for the\ncoupling is $f^2 = 0.075 \\pm 0.002$, where the largest source of uncertainty is\nthe determination of the s-wave $\\pi^- p$ scattering length from the atomic\nlevel shift measurement.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:36:57 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 21 May 2007 11:44:44 GMT\"}]', '2008-11-26', '[[\"Abaev\",\"V. V.\",\"\"],[\"Metsä\",\"P.\",\"\"],[\"Sainio\",\"M. E.\",\"\"]]'),
(704.3168, 'Valerij Kozhevnikov', 'V. P. Kozhevnikov (Ural State University, Russia)', 'Detection of superhumps in the VY Scl-type nova-like variable KR Aur', '6 pages, 6 figures, will be published in MNRAS', 'Mon.Not.Roy.Astron.Soc.378:955-960,2007', '10.1111/j.1365-2966.2007.11819.x', '', 'astro-ph', '', '  We report on detection of negative superhumps in KR Aur which is the\nrepresentative member of the VY Scl stars. The observations were obtained with\nthe multi-channel photometer during 107 h. The analysis of the data clearly\nrevealed brightness variations with a period of 3.771 +/- 0.005 h. This is 3.5\nper cent less than the orbital period, suggesting it is a negative superhump.\nNegative superhumps in VY Scl stars are widely spread. The discovery of\npowerful soft X-rays from V751 Cyg demonstrates that VY Scl stars may contain\nwhite dwarfs, at which nuclear burning of the accreted material occur. If this\nsuspicion is correct, we then can suppose that the powerful radiation emerging\nfrom the white dwarf may cause the tilt of the accretion disk to the orbital\nplane, and its retrograde precession may produce negative superhumps in VY Scl\nstars.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:46:30 GMT\"}]', '2009-06-23', '[[\"Kozhevnikov\",\"V. P.\",\"\",\"Ural State University, Russia\"]]'),
(704.3169, 'Scott Wolpert', 'Kunio Obitsu and Scott A. Wolpert', 'Grafting hyperbolic metrics and Eisenstein series', 'Published in Mathematischen Annalen, 2008. The original publication\n  is available at http://www.springerlink.com', '', '', '', 'math.CV math.AG', '', '  The family hyperbolic metric for the plumbing variety $\\{zw=t\\}$ and the non\nholomorphic Eisenstein series $E(\\zeta;2)$ are combined to provide an explicit\nexpansion for the hyperbolic metrics for degenerating families of Riemann\nsurfaces. Applications include an asymptotic expansion for the Weil-Petersson\nmetric and a local form of symplectic reduction.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:51:33 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 2 Feb 2008 18:47:41 GMT\"}]', '2008-02-04', '[[\"Obitsu\",\"Kunio\",\"\"],[\"Wolpert\",\"Scott A.\",\"\"]]'),
(704.3170, 'Damian H. Zanette', 'Damian H. Zanette', 'Zipf\'s law and city sizes: A short tutorial review on multiplicative\n  processes in urban growth', 'To appear in Advances in Complex Systems', '', '', '', 'physics.soc-ph cond-mat.stat-mech physics.data-an', '', '  We address the role of multiplicative stochastic processes in modeling the\noccurrence of power-law city size distributions. As an explanation of the\nresult of Zipf\'s rank analysis, Simon\'s model is presented in a mathematically\nelementary way, with a thorough discussion of the involved hypotheses. Emphasis\nis put on the flexibility of the model, as to its possible extensions and the\nrelaxation of some strong assumptions. We point out some open problems\nregarding the prediction of the detailed shape of Zipf\'s rank plots, which may\nbe tackled by means of such extensions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 11:54:52 GMT\"}]', '2007-05-23', '[[\"Zanette\",\"Damian H.\",\"\"]]'),
(704.3171, 'Thomas Preibisch', 'Thomas Preibisch', 'The origin of X-ray emission from T Tauri stars', 'Review talk at the Conference \"Coronae of Stars and Accretion Disks\",\n  Bonn, Germany, December 2006. Conference proceedings to be published in\n  Memorie della Societa Astronomica Italiana', '', '', '', 'astro-ph', '', '  Several aspects concerning the origin of the very strong X-ray activity of T\nTauri Stars (TTS) are still not well understood. Important new insight came\nrecently from the Chandra Orion Ultradeep Project (COUP), a unique 10-day long\nChandra observation of the Orion Nebula Cluster, and the XMM-Newton Extended\nSurvey of the Taurus Molecular Cloud (XEST). Based mainly on the results of\nthese two large projects, I will discuss our current knowledge about the\nlocation of the X-ray emitting structures in TTS, the nature of their coronal\nmagnetic fields, inferences for pre-main-sequence magnetic dynamos, and the\nrelation between accretion processes and X-ray emission.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:02:49 GMT\"}]', '2007-05-23', '[[\"Preibisch\",\"Thomas\",\"\"]]'),
(704.3172, 'Debaprasad Giri', 'Sanjay Kumar and Debaprasad Giri', 'Force induced conformational transition in a system of interacting stiff\n  polymer: Application to unfolding', 'RevTeX v4, 9 pages with 6 eps figures', 'Phys. Rev. E 72, 052901 (2005)', '10.1103/PhysRevE.72.052901', 'BHU-PHY/CMPT/05-01', 'cond-mat.soft cond-mat.stat-mech physics.bio-ph', '', '  We consider a stiff polymer chain in poor solvent and apply a force at one\nend of the chain. We find that by varying the stiffness parameter, polymer\nundergoes a transition from the globule state to the folded like state. The\nconformation of folded state mimics the $\\beta$-sheet as seen in titin\nmolecule. Using exact enumeration technique, we study the extension-force and\nforce-temperature diagrams of such a system. Force-temperature diagram shows\nthe re-entrance behaviour for flexible chain. However, for stiff chain this\nre-entrance behaviour is absent and there is an enhancement in\n$\\theta$-temperature with the rise of stiffness. We further propose that the\ninternal information about the frozen structure of polymer can be read from the\ndistribution of end-to-end distance which shows saw-tooth like behaviour.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:14:46 GMT\"}]', '2015-05-13', '[[\"Kumar\",\"Sanjay\",\"\"],[\"Giri\",\"Debaprasad\",\"\"]]'),
(704.3173, 'Vyacheslav P. Spiridonov', 'Igor M. Loutsenko and Vyacheslav P. Spiridonov', 'A Critical Phenomenon in Solitonic Ising Chains', 'This is a contribution to the Vadim Kuznetsov Memorial Issue on\n  Integrable Systems and Related Topics, published in SIGMA (Symmetry,\n  Integrability and Geometry: Methods and Applications) at\n  http://www.emis.de/journals/SIGMA/', 'SIGMA 3 (2007), 059, 11 pages', '10.3842/SIGMA.2007.059', '', 'cond-mat.stat-mech math-ph math.MP nlin.SI', '', '  We discuss a phase transition of the second order taking place in non-local\n1D Ising chains generated by specific infinite soliton solutions of the KdV and\nBKP equations.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:17:31 GMT\"}]', '2008-04-24', '[[\"Loutsenko\",\"Igor M.\",\"\"],[\"Spiridonov\",\"Vyacheslav P.\",\"\"]]'),
(704.3174, 'Ma\\\'ira Aguiar', 'Ma\\\'ira Aguiar, Nico Stollenwerk', 'A new chaotic attractor in a basic multi-strain epidemiological model\n  with temporary cross-immunity', '16 pages, 15 figures', '', '', '', 'nlin.CD q-bio.PE', '', '  An epidemic multi-strain model with temporary cross-immunity shows chaos,\neven in a previously unexpected parameter region. Especially dengue fever\nmodels with strong enhanced infectivity on secondary infection have previously\nshown deterministic chaos motivated by experimental findings of\nantibody-dependent-enhancement (ADE). Including temporary cross-immunity in\nsuch models, which is common knowledge among field researchers in dengue, we\nfind a deterministically chaotic attractor in the more realistic parameter\nregion of reduced infectivity on secondary infection (\'\'inverse ADE\'\' parameter\nregion). This is realistic for dengue fever since on second infection people\nare more likely to be hospitalized, hence do not contribute to the force of\ninfection as much as people with first infection.\n  Our finding has wider implications beyond dengue in any multi-strain\nepidemiological systems with altered infectivity upon secondary infection,\nsince we can relax the condition of rather high infectivity on secondary\ninfection previously required for deterministic chaos. For dengue the finding\nof wide ranges of chaotic attractors open new ways to analysis of existing data\nsets.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:18:46 GMT\"}]', '2007-06-25', '[[\"Aguiar\",\"Maíra\",\"\"],[\"Stollenwerk\",\"Nico\",\"\"]]'),
(704.3175, 'Debaprasad Giri', 'Debaprasad Giri and Sanjay Kumar', 'Effects of Eye-phase in DNA unzipping', 'RevTeX v4, 9 pages with 7 eps figures', 'Phys. Rev. E 73, 050903(R) (2006)', '10.1103/PhysRevE.73.050903', 'BHU-PHY/CMPT/05-03', 'cond-mat.soft cond-mat.stat-mech physics.bio-ph', '', '  The onset of an \"eye-phase\" and its role during the DNA unzipping is studied\nwhen a force is applied to the interior of the chain. The directionality of the\nhydrogen bond introduced here shows oscillations in force-extension curve\nsimilar to a \"saw-tooth\" kind of oscillations seen in the protein unfolding\nexperiments. The effects of intermediates (hairpins) and stacking energies on\nthe melting profile have also been discussed.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:20:47 GMT\"}]', '2015-05-13', '[[\"Giri\",\"Debaprasad\",\"\"],[\"Kumar\",\"Sanjay\",\"\"]]'),
(704.3176, 'Sebastian Fallert', 'S.V. Fallert, Y.M. Kim, C.J. Neugebauer, S.N. Taraskin', 'The contact process in disordered and periodic binary two-dimensional\n  lattices', 'submitted to Physical Review E', '', '10.1103/PhysRevE.78.041117', '', 'cond-mat.stat-mech', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  The critical behavior of the contact process in disordered and periodic\nbinary 2d-lattices is investigated numerically by means of Monte Carlo\nsimulations as well as via an analytical approximation and standard mean field\ntheory. Phase-separation lines calculated numerically are found to agree well\nwith analytical predictions around the homogeneous point. For the disordered\ncase, values of static scaling exponents obtained via quasi-stationary\nsimulations are found to change with disorder strength. In particular, the\nfinite-size scaling exponent of the density of infected sites approaches a\nvalue consistent with the existence of an infinite-randomness fixed point as\nconjectured before for the 2d disordered CP. At the same time, both dynamical\nand static scaling exponents are found to coincide with the values established\nfor the homogeneous case thus confirming that the contact process in a\nheterogeneous environment belongs to the directed percolation universality\nclass.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:24:20 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 30 Jun 2008 21:21:19 GMT\"}]', '2009-11-13', '[[\"Fallert\",\"S. V.\",\"\"],[\"Kim\",\"Y. M.\",\"\"],[\"Neugebauer\",\"C. J.\",\"\"],[\"Taraskin\",\"S. N.\",\"\"]]'),
(704.3177, 'Andreas Enge', 'Andreas Enge (INRIA Futurs)', 'Computing modular polynomials in quasi-linear time', '', 'Mathematics of Computation 78, 267 (2009) 1809-1824', '', '', 'math.NT cs.CC', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We analyse and compare the complexity of several algorithms for computing\nmodular polynomials. We show that an algorithm relying on floating point\nevaluation of modular functions and on interpolation, which has received little\nattention in the literature, has a complexity that is essentially (up to\nlogarithmic factors) linear in the size of the computed polynomials. In\nparticular, it obtains the classical modular polynomials $\\Phi_\\ell$ of prime\nlevel $\\ell$ in time O (\\ell^3 \\log^4 \\ell \\log \\log \\ell). Besides treating\nmodular polynomials for $\\Gamma^0 (\\ell)$, which are an important ingredient in\nmany algorithms dealing with isogenies of elliptic curves, the algorithm is\neasily adapted to more general situations. Composite levels are handled just as\neasily as prime levels, as well as polynomials between a modular function and\nits transform of prime level, such as the Schl\\\"afli polynomials and their\ngeneralisations. Our distributed implementation of the algorithm confirms the\ntheoretical analysis by computing modular equations of record level around\n10000 in less than two weeks on ten processors.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:27:39 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 23 Jul 2008 12:33:49 GMT\"}]', '2009-05-08', '[[\"Enge\",\"Andreas\",\"\",\"INRIA Futurs\"]]'),
(704.3178, 'Adriana Elizabeth Nuncio Quiroz', 'A.E. Nuncio Quiroz (on behalf of the ZEUS Collaboration)', 'Beauty production using D* + mu and mu+ mu- correlations at ZEUS', '4 pages, 3 tables, 1 figure', '', '', '', 'hep-ex', '', '  Events with observed D* and/or muons in the final state were used to indicate\nthe presence of beauty quark production and to study the correlations between\nthe particles coming from the same or different B-hadrons. The Next-to-Leading\nOrder (NLO) theoretical predictions for such processes were often available\nonly at parton level. A method to calculate visible level cross sections at\nNLO, based on an interface of the FMNR program to PYTHIA 6.2, is applied. It\nuses the NLO description at b-quark level provided by FMNR applying a\nstatistical reduction procedure (REDSTAT) that allows the link to PYTHIA, from\nwhere the description of the B-hadron decay chain is obtained. Comparisons of\nthe data and NLO cross sections at visible and b-quark level were found to be\nconsistent and equivalent.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:38:20 GMT\"}]', '2007-05-23', '[[\"Quiroz\",\"A. E. Nuncio\",\"\",\"on behalf of the ZEUS Collaboration\"]]'),
(704.3179, 'Sabrina Maniscalco', 'S. Maniscalco, J. Piilo, and K.-A. Suominen', 'Measurement-induced manipulation of the quantum-classical border', '7 pages, 3 figures', '', '', '', 'quant-ph', '', '  We demonstrate the possibility of controlling the border between the quantum\nand the classical world by performing nonselective measurements on quantum\nsystems. We consider a quantum harmonic oscillator initially prepared in a\nSchroedinger cat state and interacting with its environment. We show that the\nenvironment induced decoherence transforming the cat state into a statistical\nmixture can be strongly inhibited by means of appropriate sequences of\nmeasurements.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:31:49 GMT\"}]', '2007-05-23', '[[\"Maniscalco\",\"S.\",\"\"],[\"Piilo\",\"J.\",\"\"],[\"Suominen\",\"K. -A.\",\"\"]]'),
(704.3180, 'Rahul Basu', 'Rahul Basu (IMSc), Eric Laenen (NIKHEF), Anuradha Misra (Mumbai U.),\n  Patrick Motylinski (NIKHEF)', 'Soft-collinear effects in prompt photon production', '14 pages, 12 figures, added comment on fragmentation contribution and\n  one more reference. Version to appear in Phys. Rev. D', 'Phys.Rev.D76:014010,2007', '10.1103/PhysRevD.76.014010', 'NIKHEF/2007-008, ITP-UU-07/23, IMSc-2007/04/5', 'hep-ph', '', '  We extend next-to-leading logarithmic threshold and joint resummation for\nprompt photon production to include leading collinear effects. The impact of\nthese effects is assessed for both fixed-target and collider kinematics. We\nfind them in general to be small, but noticeable.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:38:45 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 15 Jun 2007 08:18:30 GMT\"}]', '2008-11-26', '[[\"Basu\",\"Rahul\",\"\",\"IMSc\"],[\"Laenen\",\"Eric\",\"\",\"NIKHEF\"],[\"Misra\",\"Anuradha\",\"\",\"Mumbai U.\"],[\"Motylinski\",\"Patrick\",\"\",\"NIKHEF\"]]'),
(704.3181, 'Dmitri Diakonov', 'Dmitri Diakonov and Victor Petrov (St. Petersburg NPI)', 'Confining ensemble of dyons', '26 pp. Construction of general N-ality = k strings added. The title\n  changed', 'Phys.Rev.D76:056001,2007', '10.1103/PhysRevD.76.056001', '', 'hep-th hep-lat', '', '  We construct the integration measure over the moduli space of an arbitrary\nnumber of N kinds of dyons of the pure SU(N) gauge theory at finite\ntemperatures. The ensemble of dyons governed by the measure is mathematically\ndescribed by a (supersymmetric) quantum field theory that is exactly solvable\nand is remarkable for a number of striking features: 1) The free energy has the\nminimum corresponding to the zero average Polyakov line, as expected in the\nconfining phase; 2)The correlation function of two Polyakov lines exhibits a\nlinear potential between static quarks in any N-ality non-zero representation,\nwith a calculable string tension roughly independent of temperature; 3) The\naverage spatial Wilson loop falls off exponentially with its area and the same\nstring tension; 4) At a critical temperature the ensemble of dyons rearranges\nand de-confines; 5)The estimated ratio of the critical temperature to the\nsquare root of the string tension is in excellent agreement with the lattice\ndata.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:08:12 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 21 Jun 2007 14:45:08 GMT\"}]', '2008-11-26', '[[\"Diakonov\",\"Dmitri\",\"\",\"St. Petersburg NPI\"],[\"Petrov\",\"Victor\",\"\",\"St. Petersburg NPI\"]]'),
(704.3182, 'James P. Sethna', 'Christopher R. Myers and James. P. Sethna', 'Python for Education: Computational Methods for Nonlinear Systems', 'Submitted to special issue of CiSE', '', '', '', 'nlin.CD', '', '  We describe a novel, interdisciplinary, computational methods course that\nuses Python and associated numerical and visualization libraries to enable\nstudents to implement simulations for a number of different course modules.\nProblems in complex networks, biomechanics, pattern formation, and gene\nregulation are highlighted to illustrate the breadth and flexibility of\nPython-powered computational environments.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:55:17 GMT\"}]', '2007-05-23', '[[\"Myers\",\"Christopher R.\",\"\"],[\"Sethna\",\"James. P.\",\"\"]]'),
(704.3183, 'Shingo Takeuchi', 'Naoyuki Kawahara (KEK), Jun Nishimura (KEK, SOKENDAI), Shingo Takeuchi\n  (SOKENDAI)', 'Exact fuzzy sphere thermodynamics in matrix quantum mechanics', '22 pages, 14 figures, (v2) some typos corrected', 'JHEP 0705:091,2007', '10.1088/1126-6708/2007/05/091', 'KEK-TH-1145', 'hep-th astro-ph hep-lat', '', '  We study thermodynamical properties of a fuzzy sphere in matrix quantum\nmechanics of the BFSS type including the Chern-Simons term. Various quantities\nare calculated to all orders in perturbation theory exploiting the one-loop\nsaturation of the effective action in the large-N limit. The fuzzy sphere\nbecomes unstable at sufficiently strong coupling, and the critical point is\nobtained explicitly as a function of the temperature. The whole phase diagram\nis investigated by Monte Carlo simulation. Above the critical point, we obtain\nperfect agreement with the all order results. In the region below the critical\npoint, which is not accessible by perturbation theory, we observe the Hagedorn\ntransition. In the high temperature limit our model is equivalent to a totally\nreduced model, and the relationship to previously known results is clarified.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:13:59 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 31 May 2007 12:36:57 GMT\"}]', '2009-11-13', '[[\"Kawahara\",\"Naoyuki\",\"\",\"KEK\"],[\"Nishimura\",\"Jun\",\"\",\"KEK, SOKENDAI\"],[\"Takeuchi\",\"Shingo\",\"\",\"SOKENDAI\"]]'),
(704.3184, 'Alexander Burinskii', 'Alexander Burinskii', 'Kerr-Schild Photonlike Metric Solutions', '6 p, Revtex4', '', '', '', 'gr-qc hep-th', '', '  The charged and spinning lightlike solutions are obtained in the Kerr-Schild\nformalism. In particular, one of them may be considered as an ultrarelativistic\nboost of the Kerr-Newman solution along the direction of angular momentum. The\nKerr singular ring disappears, however, there remains a finite parameter $a$\nwhich determines spin by the Kerr relation $J=ma$. By $J=\\hbar$, the parameter\n$a$ is de Broglie wavelength of the corresponding photon. Electromagnetic field\nis aligned to the Kerr null congruence. Some of the presented solutions contain\nsingular beam pulse (pp-strings) like the considered recently `gyratons\'.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:01:59 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 11:18:01 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 20 Mar 2008 13:18:54 GMT\"}]', '2008-03-20', '[[\"Burinskii\",\"Alexander\",\"\"]]'),
(704.3185, 'Jonas Persson', 'Jonas R. Persson', 'Relativistic self-consistent-field calculations of the hyperfine\n  structure in the 4d-shell ions', '11 pages, 3 tables', '', '', '', 'physics.atom-ph', '', '  Relativistic self-consistent-field calculations of the radial hyperfine\nintegrals have been performed in the 4d-shell element ions. The comparison with\navailable experimental results gives an estimate of configuration interaction\neffects in the hyperfine interaction in these ions. The results can also be\nused to derive nuclear moments from laserspectroscopic measurements of\nradioactive isotopes.\n  PACS Numbers: 31.15.Ne, 31.30.Gs, 32.10.Fn\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:02:23 GMT\"}]', '2007-05-23', '[[\"Persson\",\"Jonas R.\",\"\"]]'),
(704.3186, 'Silvio Paolo Sorella', 'S.P. Sorella', 'On the dynamical mass generation in confining Yang-Mills theories', '11 pages', 'AnnalsPhys.321:1747-1761,2006', '10.1016/j.aop.2006.02.014', '', 'hep-th', '', '  The dynamical mass generation for gluons is discussed in Euclidean Yang-Mills\ntheories supplemented with a renormalizable mass term. The mass parameter is\nnot free, being determined in a self-consistent way through a gap equation\nwhich obeys the renormalization group. The example of the Landau gauge is\nworked out explicitly at one loop order. A few remarks on the issue of the\nunitarity are provided.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:57:42 GMT\"}]', '2008-11-26', '[[\"Sorella\",\"S. P.\",\"\"]]'),
(704.3187, 'Laura Magrini', 'Laura Magrini, Edvige Corbelli, Daniele Galli', 'The building up of the disk galaxy M33 and the evolution of the\n  metallicity gradient', '16 pages, 11 figures, A&A accepted', '', '10.1051/0004-6361:20077215', '', 'astro-ph', '', '  The evolution of radial gradients of metallicity in disk galaxies and its\nrelation with the disk formation are not well understood. Theoretical models of\ngalactic chemical evolution make contrasting predictions about the time\nevolution of metallicity gradients. To test chemical evolution models and trace\nthe star formation and accretion history of low luminosity disk galaxies we\nfocus on the Local Group galaxy M33. We analyze O/H and S/H abundances in\nplanetary nebulae, H{\\sc ii} regions, and young stars, together with known\n[Fe/H] abundances in the old stellar population of M33. With a theoretical\nmodel, we follow the time evolution of gas (diffuse and condensed in clouds),\nstars, and chemical abundances in the disk of M33, assuming that the galaxy is\naccreting gas from an external reservoir. Our model is able to reproduce the\navailable observational constraints on the distribution of gas and stars in M33\nand to predict the time evolution of several chemical abundances. In\nparticular, we find that a model characterized by a continuous infall of gas on\nthe disk, at a rate of $\\dot M_{\\rm inf}\\approx 1$ $M_\\odot$ yr$^{-1}$, almost\nconstant with time, can also account for the relatively high rate of star\nformation and for the shallow chemical gradients. Supported by a large sample\nof high resolution observations for this nearby galaxy, we conclude that the\nmetallicity in the disk of M33 has increased with time at all radii, with a\ncontinuous flattening of the gradient over the last $\\sim 8$ Gyr.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:40:09 GMT\"}]', '2009-11-13', '[[\"Magrini\",\"Laura\",\"\"],[\"Corbelli\",\"Edvige\",\"\"],[\"Galli\",\"Daniele\",\"\"]]'),
(704.3188, 'Sebastien Maret', 'Sebastien Maret and Edwin A. Bergin', 'The Ionization Fraction of Barnard 68: Implications for Star and Planet\n  Formation', 'To appear in the Astrophysical Journal', 'Astrophys.J.664:956-963,2007', '10.1086/519152', '', 'astro-ph', '', '  We present a detailed study of the ionization fraction of the Barnard 68\npre-stellar core, using millimeter H13CO+ and DCO+ lines observations. These\nobservations are compared to the predictions of a radiative transfer model\ncoupled to a chemical network that includes depletion on grains and gas phase\ndeuterium fractionation. Together with previous observations and modelling of\nCO and isotopologues, our H13CO+ and DCO+ observations and modelling allow to\nplace constraints on the metal abundance and the cosmic ionization rate. The\nH13CO+ emission is well reproduced for metals abundances lower than 3e-9 and a\nstandard cosmic ray ionization rate. However, the observations are also\nconsistent with a complete depletion of metals, i.e. with cosmic rays as the\nonly source of ionization at visual extinctions greater than a few Av . The\nDCO+ emission is found to be dependent of the ortho to para H2 ratio, and\nindicates a ratio of ~1e-2. The derived ionization fraction is about 5e-9 with\nrespect to H nuclei, which is about an order of magnitude lower than the one\nobserved in the L1544 core. The corresponding ambipolar diffusion timescale is\nfound to be an order of magnitude larger than the free fall timescale at the\ncenter of the core. The inferred metal abundance suggests that magnetically\ninactive regions (dead zones) are present in protostellar disks.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:07:51 GMT\"}]', '2009-06-23', '[[\"Maret\",\"Sebastien\",\"\"],[\"Bergin\",\"Edwin A.\",\"\"]]'),
(704.3189, 'V. Gogohia', 'V. Gogokhia', 'II. The mass gap and solution of the quark confinement problem in QCD', 'No tables and figures, 15 pages', '', '', '', 'hep-ph hep-th', '', '  We have investigated a closed system of equations for the quark propagator,\nobtained earlier within our general approach to QCD at low energies. It implies\nquark confinement (the quark propagator has no pole, indeed), as well as the\ndynamical breakdown of chiral symmetry (a chiral symmetry preserving solution\nis forbidded). This system can be solved exactly in the chiral limit. We have\nestablished the space of the smooth test functions (consisting of the Green\'s\nfunctions for the quark propagator and the corresponding quark-gluon vertex) in\nwhich our generalized function (the confining gluon propagator) becomes a\ncontinuous linear functional. It is a linear topological space $K(c)$ of the\ninfinitely differentiable functions (with respect to the dimensionless momentum\nvariable $x$), having compact support in the region $x \\leq c$. We develop an\nanalytical formalism, the so-called chiral perturbtion theory at the\nfundamental quark level, which allows one to find explicit solution for the\nquark propagator in powers of the light quark masses. We also develop an\nanalytical formalism, which allows one to find the solution for the quark\npropagator in the inverse powers of the heavy quark masses. It justifies the\nuse for the heavy quark propagator its free counterpart up to terms of the\norder $1/m_Q^3$, where $m_Q$ is the heavy quark mass. So this solution\nautomatically possesses the heavy quark spin-flavor symmetry.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:16:13 GMT\"}]', '2007-05-23', '[[\"Gogokhia\",\"V.\",\"\"]]'),
(704.3190, 'Karine Sartelet', 'Karine Sartelet (CEREA), Hiroshi Hayami (CRIEPI), Bruno Sportisse\n  (CEREA)', 'MICS Asia Phase II - Sensitivity to the aerosol module', 'Atmospheric Environment (2007) in press', '', '10.1016/j.atmosenv.2007.03.005', '', 'physics.ao-ph', '', '  In the framework of the model inter-comparison study - Asia Phase II (MICS2),\nwhere eight models are compared over East Asia, this paper studies the\ninfluence of different parameterizations used in the aerosol module on the\naerosol concentrations of sulfate and nitrate in PM10. An intracomparison of\naerosol concentrations is done for March 2001 using different configurations of\nthe aerosol module of one of the model used for the intercomparison. Single\nmodifications of a reference setup for model configurations are performed and\ncompared to a reference case. These modifications concern the size\ndistribution, i.e. the number of sections, and physical processes, i.e.\ncoagulation, condensation/evaporation, cloud chemistry, heterogeneous reactions\nand sea-salt emissions. Comparing monthly averaged concentrations at different\nstations, the importance of each parameterization is first assessed. It is\nfound that sulfate concentrations are little sensitive to sea-salt emissions\nand to whether condensation is computed dynamically or by assuming\nthermodynamic equilibrium. Nitrate concentrations are little sensitive to cloud\nchemistry. However, a very high sensitivity to heterogeneous reactions is\nobserved. Thereafter, the variability of the aerosol concentrations to the use\nof different chemistry transport models (CTMs) and the variability to the use\nof different parameterizations in the aerosol module are compared. For sulfate,\nthe variability to the use of different parameterizations in the aerosol module\nis lower than the variability to the use of different CTMs. However, for\nnitrate, for monthly averaged concentrations averaged over four stations, these\ntwo variabilities have the same order of magnitude.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:16:16 GMT\"}]', '2007-05-23', '[[\"Sartelet\",\"Karine\",\"\",\"CEREA\"],[\"Hayami\",\"Hiroshi\",\"\",\"CRIEPI\"],[\"Sportisse\",\"Bruno\",\"\",\"CEREA\"]]'),
(704.3191, 'Teresa Mineo', 'T.Mineo, V.Mangano, S.Covino, G.Cusumano, V.La Parola, E.Troja,\n  P.Roming, D.N.Burrows, S.Campana, M.Capalbi, G.Chincarini, N.Gehrels,\n  P.Giommi, J.E.Hill, F.Marshall, A.Moretti, P.O\'Brien, M.Page, M.Perri,\n  P.Romano, B.Sbarufatti, G.Sato, G.Tagliaferri', 'GRB 050410 and GRB 050412: are they really dark GRBs?', '6 figures, 9 pages, accepted for publication in A&A', '', '10.1051/0004-6361:20066594', '', 'astro-ph', '', '  We present a detailed analysis of the prompt and afterglow emission of GRB\n050410 and GRB 050412 detected by Swift for which no optical counterpart was\nobserved. The 15-150 keV energy distribution of the GRB 050410 prompt emission\nshows a peak energy at 53 keV. The XRT light curve of this GRB decays as a\npower law with a slope of alpha=1.06+/-0.04. The spectrum is well reproduced by\nan absorbed power law with a spectral index Gamma_x=2.4+/-0.4 and a low energy\nabsorption N_H=4(+3;-2)x10^21 cm^(-2) which is higher than the Galactic value.\nThe 15-150 keV prompt emission in GRB 050412 is modelled with a hard\n(Gamma=0.7+/-0.2) power law. The XRT light curve follows a broken power law\nwith the first slope alpha_1=0.7+/-0.4, the break time T_break=254(-41;+79) s\nand the second slope alpha_2=2.8(-0.8;+0.5). The spectrum is fitted by a power\nlaw with spectral index Gamma_x=1.3+/-0.2 which is absorbed at low energies by\nthe Galactic column. The GRB 050410 afterglow reveals the expected\ncharacteristics of the third component of the canonical Swift light curve.\nConversely, a complex phenomenology was detected in the GRB 050412 because of\nthe presence of the very early break. The light curve in this case can be\ninterpreted as being the last peak of the prompt emission. The two bursts\npresent tight upper limits for the optical emission, however, neither of them\ncan be clearly classified as dark. For GRB 050410, the suppression of the\noptical afterglow could be attributed to a low density interstellar medium\nsurrounding the burst. For GRB 050412, the evaluation of the darkness is more\ndifficult due to the ambiguity in the extrapolation of the X-ray afterglow\nlight curve.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:21:46 GMT\"}]', '2009-11-13', '[[\"Mineo\",\"T.\",\"\"],[\"Mangano\",\"V.\",\"\"],[\"Covino\",\"S.\",\"\"],[\"Cusumano\",\"G.\",\"\"],[\"La Parola\",\"V.\",\"\"],[\"Troja\",\"E.\",\"\"],[\"Roming\",\"P.\",\"\"],[\"Burrows\",\"D. N.\",\"\"],[\"Campana\",\"S.\",\"\"],[\"Capalbi\",\"M.\",\"\"],[\"Chincarini\",\"G.\",\"\"],[\"Gehrels\",\"N.\",\"\"],[\"Giommi\",\"P.\",\"\"],[\"Hill\",\"J. E.\",\"\"],[\"Marshall\",\"F.\",\"\"],[\"Moretti\",\"A.\",\"\"],[\"O\'Brien\",\"P.\",\"\"],[\"Page\",\"M.\",\"\"],[\"Perri\",\"M.\",\"\"],[\"Romano\",\"P.\",\"\"],[\"Sbarufatti\",\"B.\",\"\"],[\"Sato\",\"G.\",\"\"],[\"Tagliaferri\",\"G.\",\"\"]]'),
(704.3192, 'Katia Biazzo Dr', 'K. Biazzo (1,2), L. Pasquini (2), L. Girardi (3), A. Frasca (1), L. da\n  Silva (4), J. Setiawan (5), E. Marilli (1), A. P. Hatzes (6), S. Catalano\n  (1), ((1) INAF-OACt, (2) ESO-Garching, (3) INAF-OAPd, (4) ON/MCT, (5)\n  MPIA-Heidelberg, (6) TLS)', 'Deriving temperature, mass and age of evolved stars from high-resolution\n  spectra. Application to field stars and the open cluster IC 4651', '11 pages, 9 figures, version accepted for publication in A&A. Major\n  changes: revised paper, new discussion of results, references added, one\n  additional figure', '', '10.1051/0004-6361:20077374', '', 'astro-ph', '', '  We test our capability of deriving stellar physical parameters of giant stars\nby analysing a sample of field stars and the well studied open cluster IC 4651\nwith different spectroscopic methods. The use of a technique based on\nline-depth ratios (LDRs) allows us to determine with high precision the\neffective temperature of the stars and to compare the results with those\nobtained with a classical LTE abundance analysis. (i) For the field stars we\nfind that the temperatures derived by means of the LDR method are in excellent\nagreement with those found by the spectral synthesis. This result is extremely\nencouraging because it shows that spectra can be used to firmly derive\npopulation characteristics (e.g., mass and age) of the observed stars. (ii) For\nthe IC 4651 stars we use the determined effective temperature to derive the\nfollowing results. a) The reddening E(B-V) of the cluster is 0.12+/-0.02,\nlargely independent of the color-temperature calibration used. b) The age of\nthe cluster is 1.2+/-0.2 Gyr. c) The typical mass of the analysed giant stars\nis 2.0+/-0.2M_sun. Moreover, we find a systematic difference of about 0.2 dex\nin log g between spectroscopic and evolutionary values. We conclude that, in\nspite of known limitations, a classical spectroscopic analysis of giant stars\nmay indeed result in very reliable stellar parameters. We caution that the\nquality of the agreement, on the other hand, depends on the details of the\nadopted spectroscopic analysis.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:22:42 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 17 Sep 2007 08:37:24 GMT\"}]', '2009-11-13', '[[\"Biazzo\",\"K.\",\"\"],[\"Pasquini\",\"L.\",\"\"],[\"Girardi\",\"L.\",\"\"],[\"Frasca\",\"A.\",\"\"],[\"da Silva\",\"L.\",\"\"],[\"Setiawan\",\"J.\",\"\"],[\"Marilli\",\"E.\",\"\"],[\"Hatzes\",\"A. P.\",\"\"],[\"Catalano\",\"S.\",\"\"]]'),
(704.3193, 'Elsa Henriques S', 'Elsa S. Henriques, Andrey V. Solov\'yov', 'A Rational Method for Probing Macromolecules Dissociation: The\n  Antibody-Hapten System', '22 pages, 10 figures', '', '10.1140/epjd/e2008-00009-3', '', 'physics.bio-ph physics.chem-ph', '', '  The unbinding process of a protein-ligand complex of major biological\ninterest was investigated by means of a computational approach at atomistic\nclassical mechanical level. An energy minimisation-based technique was used to\ndetermine the dissociation paths of the system by probing only a relevant set\nof generalized coordinates. The complex problem was reduced to a\nlow-dimensional scanning along a selected distance between the protein and the\nligand. Orientational coordinates of the escaping fragment (the ligand) were\nalso assessed in order to further characterise the unbinding. Solvent effects\nwere accounted for by means of the Poisson--Boltzmann continuum model. The\ncorresponding dissociation time was derived from the calculated barrier height,\nin compliance with the experimentally reported Arrhenius-like behaviour. The\ncomputed results are in good agreement with the available experimental data.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 12:47:34 GMT\"}]', '2009-11-13', '[[\"Henriques\",\"Elsa S.\",\"\"],[\"Solov\'yov\",\"Andrey V.\",\"\"]]'),
(704.3194, 'Gilles Carron', 'Gilles Carron (LMJL)', 'L^2 harmonics forms on non compact manifolds', '', '', '', '', 'math.DG', '', '  The source of these notes is a series of lectures given at the CIMPA\'s summer\nschool \"Recent Topics in Geometric Analysis\".\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:32:34 GMT\"}]', '2007-05-23', '[[\"Carron\",\"Gilles\",\"\",\"LMJL\"]]'),
(704.3195, 'Andreas Ringwald', 'Andreas Ringwald (DESY)', 'Particle Interpretations of the PVLAS Data', '20 pages, 18 figures, pdproc.sty; talk presented at the XII\n  International Workshop on ``Neutrino Telescopes\'\', March 6-9, 2007, Venice,\n  Italy', '', '', 'DESY 07-054', 'hep-ph', '', '  Recently the PVLAS collaboration reported the observation of a rotation of\nlinearly polarized laser light induced by a transverse magnetic field -- a\nsignal being unexpected within standard QED. In this review, we emphasize two\nmechanisms which have been proposed to explain this result: production of a\nsingle light neutral spin-zero particle or pair production of light minicharged\nparticles. We discuss a class of models, involving, in addition to our familiar\n``visible\'\' photon, further light ``hidden paraphotons\'\', which mix\nkinematically with the visible one, and further light paracharged particles. In\nthese models, very strong astrophysical and cosmological bounds on the weakly\ninteracting light particles mentioned above can be evaded. In the upcoming\nyear, a number of decisive laboratory based tests of the particle\ninterpretation of the PVLAS anomaly will be done. More generally, such\nexperiments, exploiting high fluxes of low-energy photons and/or large\nelectromagnetic fields, will dig into previously unconstrained parameter space\nof the above mentioned models.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:55:48 GMT\"}]', '2007-05-23', '[[\"Ringwald\",\"Andreas\",\"\",\"DESY\"]]'),
(704.3196, 'Hasan Karabulut', 'Hasan Karabulut', 'Distributed Gaussian polynomials as q-oscillator eigenfunctions', '', 'Journal of Mathematical Physics 47, 013508 (2006)', '10.1063/1.2161022', '', 'math-ph math.MP', '', '  Karabulut and Sibert (\\textit{J. Math. Phys}. \\textbf{38} (9), 4815 (1997))\nhave constructed an orthogonal set of functions from linear combinations of\nequally spaced Gaussians. In this paper we show that they are actually\neigenfunctions of a q-oscillator in coordinate representation. We also\nreinterpret the coordinate representation example of q-oscillator given by\nMacfarlane as the functions orthogonal with respect to an unusual inner product\ndefinition. It is shown that the eigenfunctions in both q-oscillator examples\nare infinitely degenerate.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 13:57:06 GMT\"}]', '2007-05-23', '[[\"Karabulut\",\"Hasan\",\"\"]]'),
(704.3197, 'Reinhard Klette', 'Fajie Li and Reinhard Klette', 'Euclidean Shortest Paths in Simple Cube Curves at a Glance', '8 pages', '', '', 'CITR-TR-198', 'cs.CG cs.DM', '', '  This paper reports about the development of two provably correct approximate\nalgorithms which calculate the Euclidean shortest path (ESP) within a given\ncube-curve with arbitrary accuracy, defined by $\\epsilon >0$, and in time\ncomplexity $\\kappa(\\epsilon) \\cdot {\\cal O}(n)$, where $\\kappa(\\epsilon)$ is\nthe length difference between the path used for initialization and the\nminimum-length path, divided by $\\epsilon$. A run-time diagram also illustrates\nthis linear-time behavior of the implemented ESP algorithm.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 03:54:51 GMT\"}]', '2007-05-23', '[[\"Li\",\"Fajie\",\"\"],[\"Klette\",\"Reinhard\",\"\"]]'),
(704.3198, 'Jong E Han', 'J. E. Han, and R. J. Heary', 'Imaginary-time formulation of steady-state nonequilibrium: application\n  to strongly correlated transport', '5 pages 3 figures', 'Phys Rev Lett 99, 236808 (2007)', '10.1103/PhysRevLett.99.236808', '', 'cond-mat.str-el cond-mat.mes-hall', '', '  We extend the imaginary-time formulation of the equilibrium quantum many-body\ntheory to steady-state nonequilibrium with an application to strongly\ncorrelated transport. By introducing Matsubara voltage, we keep the finite\nchemical potential shifts in the Fermi-Dirac function, in agreement with the\nKeldysh formulation. The formulation is applied to strongly correlated\ntransport in the Kondo regime using the quantum Monte Carlo method.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:10:30 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 6 Oct 2007 21:51:42 GMT\"}]', '2009-11-13', '[[\"Han\",\"J. E.\",\"\"],[\"Heary\",\"R. J.\",\"\"]]'),
(704.3199, 'Enrico Paolini', 'E. Paolini, M. Fossorier, M. Chiani', 'Generalized Stability Condition for Generalized and Doubly-Generalized\n  LDPC Codes', '5 pages, 2 figures, to appear in Proc. of IEEE ISIT 2007', '', '10.1109/ISIT.2007.4557440', '', 'cs.IT math.IT', '', '  In this paper, the stability condition for low-density parity-check (LDPC)\ncodes on the binary erasure channel (BEC) is extended to generalized LDPC\n(GLDPC) codes and doublygeneralized LDPC (D-GLDPC) codes. It is proved that, in\nboth cases, the stability condition only involves the component codes with\nminimum distance 2. The stability condition for GLDPC codes is always expressed\nas an upper bound to the decoding threshold. This is not possible for D-GLDPC\ncodes, unless all the generalized variable nodes have minimum distance at least\n3. Furthermore, a condition called derivative matching is defined in the paper.\nThis condition is sufficient for a GLDPC or DGLDPC code to achieve the\nstability condition with equality. If this condition is satisfied, the\nthreshold of D-GLDPC codes (whose generalized variable nodes have all minimum\ndistance at least 3) and GLDPC codes can be expressed in closed form.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:11:58 GMT\"}]', '2016-11-15', '[[\"Paolini\",\"E.\",\"\"],[\"Fossorier\",\"M.\",\"\"],[\"Chiani\",\"M.\",\"\"]]'),
(704.3200, 'Samvel Ter-Antonyan', 'A. P. Garyaka, R. M. Martirosov, S. V. Ter-Antonyan, N. Nikolskaya, Y.\n  A. Gallant, L. Jones and J. Procureur', 'Rigidity-dependent cosmic ray energy spectra in the knee region obtained\n  with the GAMMA experiment', '28 pages, 18 figures, accepted for publication in Astroparticle\n  Physics', 'Astropart.Phys.28:169-181,2007', '10.1016/j.astropartphys.2007.04.004', '', 'astro-ph', '', '  On the basis of the extensive air shower (EAS) data obtained by the GAMMA\nexperiment, the energy spectra and elemental composition of the primary cosmic\nrays are derived in the 1-100 PeV energy range. The reconstruction of the\nprimary energy spectra is carried out using an EAS inverse approach in the\nframework of the SIBYLL2.1 and QGSJET01 interaction models and the hypothesis\nof power-law primary energy spectra with rigidity-dependent knees. The energy\nspectra of primary H, He, O-like and Fe-like nuclei obtained with the SIBYLL\ninteraction model agree with corresponding extrapolations of the balloon and\nsatellite data to ~1 PeV energies. The energy spectra obtained from the QGSJET\nmodel show a predominantly proton composition in the knee region. The\nrigidity-dependent knee feature of the primary energy spectra for each\ninteraction model is displayed at the following rigidities: ~2.5+/-0.2 PV\n(SIBYLL) and ~3.1-4.2 PV (QGSJET). All the results presented are derived taking\ninto account the detector response, the reconstruction uncertainties of the EAS\nparameters, and fluctuations in the EAS development.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:19:31 GMT\"}]', '2009-06-23', '[[\"Garyaka\",\"A. P.\",\"\"],[\"Martirosov\",\"R. M.\",\"\"],[\"Ter-Antonyan\",\"S. V.\",\"\"],[\"Nikolskaya\",\"N.\",\"\"],[\"Gallant\",\"Y. A.\",\"\"],[\"Jones\",\"L.\",\"\"],[\"Procureur\",\"J.\",\"\"]]'),
(704.3201, 'Grigoris Panotopoulos', 'Grigoris Panotopoulos', 'Assisted chaotic inflation in brane-world cosmology', 'Revtex, 4 pages, accepted for publication in Phys.Rev.D', 'Phys.Rev.D75:107302,2007', '10.1103/PhysRevD.75.107302', '', 'hep-ph', '', '  Assisted chaotic inflation in brane cosmology is discussed. We work in the\nframework of Randall-Sundrum (RS) II model, in which adopting the RS condition\nthe only parameter is the five-dimensional Planck mass. Using the scalar\nspectral index and the amplitude of scalar perturbations we determine both the\nmass of the scalar fields responsible for inflation and the fundamental Planck\nmass of the higher-dimensional theory. We find that the mass of the scalars has\nthe typical value of the inflaton mass in chaotic inflation ($M_I \\sim 10^{13}$\nGeV) and that the five-dimensional Planck mass is very close to the GUT (Grand\nUnified Theories) scale ($M_5 \\sim (10^{16}-10^{17})$ GeV). Furthermore, no\nmatter how many scalar fields we use it is not possible to have chaotic\ninflation with field values below the fundamental Planck mass.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:37:15 GMT\"}]', '2008-11-26', '[[\"Panotopoulos\",\"Grigoris\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3202, 'Mark Thompson', 'M.A. Thompson, S. Serjeant, T. Jenness, D. Scott, M. Ashdown, C.\n  Brunt, H. Butner, E. Chapin, A. C. Chrysostomou, J. S. Clark, D. Clements, J.\n  L. Collett, K. Coppin, I. M. Coulson, W. R. F. Dent, F. Economou, A. Evans,\n  P. Friberg, G. A. Fuller, A. G. Gibb, J. Greaves, J. Hatchell, W. S. Holland,\n  M. Hudson, R. J. Ivison, A. Jaffe, G. Joncas, H. R. A. Jones, J. H. Knapen,\n  J. Leech, R. Mann, H. E. Matthews, T. J. T. Moore, A. Mortier, M. Negrello,\n  D. Nutter, M. P. Pestalozzi, A. Pope, J. Richer, R. Shipman, J. S. Urquhart,\n  M. Vaccari, L. Van Waerbeke, S. Viti, B. Weferling, G. J. White, J.\n  Wouterloot, M. Zhu', 'The SCUBA-2 \"All-Sky\" Survey', '26 pages, 5 figures. In referee\'s format. Submitted to PASP. Figs 1-3\n  are missing due to file size constraints. A full version of the paper may be\n  found at http://star-www.herts.ac.uk/~mat/sassy_pasp.pdf Version 2 fixes\n  author list and link to full version of paper', '', '', '', 'astro-ph', '', '  The sub-millimetre wavelength regime is perhaps the most poorly explored over\nlarge areas of the sky, despite the considerable effort that has been expended\nin making deep maps over small regions. As a consequence the properties of the\nsub-millimetre sky as a whole, and of rare bright objects in particular,\nremains largely unknown. Here we describe a forthcoming survey (the SCUBA-2\n``All-Sky\'\' Survey, or SASSy) designed to address this issue by making a\nlarge-area map of approximately one-fifth of the sky visible from the JCMT\n(4800 square degrees) down to a 1 sigma noise level of 30 mJy/beam. This map\nforms the pilot for a much larger survey, which will potentially map the\nremaining sky visible from the JCMT, with the region also visible to ALMA as a\npriority. SASSy has been awarded 500 hours for the 4800 square degree pilot\nphase and will commence after the commissioning of SCUBA-2, expected in early\n2008.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:25:10 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 2 May 2007 22:01:26 GMT\"}]', '2007-05-23', '[[\"Thompson\",\"M. A.\",\"\"],[\"Serjeant\",\"S.\",\"\"],[\"Jenness\",\"T.\",\"\"],[\"Scott\",\"D.\",\"\"],[\"Ashdown\",\"M.\",\"\"],[\"Brunt\",\"C.\",\"\"],[\"Butner\",\"H.\",\"\"],[\"Chapin\",\"E.\",\"\"],[\"Chrysostomou\",\"A. C.\",\"\"],[\"Clark\",\"J. S.\",\"\"],[\"Clements\",\"D.\",\"\"],[\"Collett\",\"J. L.\",\"\"],[\"Coppin\",\"K.\",\"\"],[\"Coulson\",\"I. M.\",\"\"],[\"Dent\",\"W. R. F.\",\"\"],[\"Economou\",\"F.\",\"\"],[\"Evans\",\"A.\",\"\"],[\"Friberg\",\"P.\",\"\"],[\"Fuller\",\"G. A.\",\"\"],[\"Gibb\",\"A. G.\",\"\"],[\"Greaves\",\"J.\",\"\"],[\"Hatchell\",\"J.\",\"\"],[\"Holland\",\"W. S.\",\"\"],[\"Hudson\",\"M.\",\"\"],[\"Ivison\",\"R. J.\",\"\"],[\"Jaffe\",\"A.\",\"\"],[\"Joncas\",\"G.\",\"\"],[\"Jones\",\"H. R. A.\",\"\"],[\"Knapen\",\"J. H.\",\"\"],[\"Leech\",\"J.\",\"\"],[\"Mann\",\"R.\",\"\"],[\"Matthews\",\"H. E.\",\"\"],[\"Moore\",\"T. J. T.\",\"\"],[\"Mortier\",\"A.\",\"\"],[\"Negrello\",\"M.\",\"\"],[\"Nutter\",\"D.\",\"\"],[\"Pestalozzi\",\"M. P.\",\"\"],[\"Pope\",\"A.\",\"\"],[\"Richer\",\"J.\",\"\"],[\"Shipman\",\"R.\",\"\"],[\"Urquhart\",\"J. S.\",\"\"],[\"Vaccari\",\"M.\",\"\"],[\"Van Waerbeke\",\"L.\",\"\"],[\"Viti\",\"S.\",\"\"],[\"Weferling\",\"B.\",\"\"],[\"White\",\"G. J.\",\"\"],[\"Wouterloot\",\"J.\",\"\"],[\"Zhu\",\"M.\",\"\"]]'),
(704.3203, 'Carlos Rom\\\'an-Z\\\'u\\~niga', 'C. Rom\\\'an-Z\\\'u\\~niga, C. Lada, A. Muench, and J. Alves', 'The Infrared Extinction Law at Extreme Depth in a Dark Cloud Core', '22 pages manuscript, 4 figures (2 multipart), 1 table', '', '10.1086/518928', '', 'astro-ph', '', '  We combined sensitive near-infrared data obtained with ground-based imagers\non the ESO NTT and VLT telescopes with space mid-infrared data acquired with\nthe IRAC imager on the Spitzer Space Telescope to calculate the extinction law\nA_\\lambda/A_K as a function of \\lambda between 1.25 and 7.76 micron to an\nunprecedented depth in Barnard 59, a star forming, dense core located in the\nPipe Nebula. The ratios A_\\lambda/A_K were calculated from the slopes of the\ndistributions of sources in color-color diagrams \\lambda-K vs. H-K. The\ndistributions in the color-color diagrams are fit well with single slopes to\nextinction levels of A_K ~ 7 (A_V ~ 59 mag). Consequently, there appears to be\nno significant variation of the extinction law with depth through the B59 line\nof sight. However, when slopes are translated into the relative extinction\ncoefficients A_\\lambda/A_K, we find an extinction law which departs from the\nsimple extrapolation of the near-infrared power law extinction curve, and\nagrees more closely with a dust extinction model for a cloud with a total to\nselective absorption R_V=5.5 and a grain size distribution favoring larger\ngrains than those in the diffuse ISM. Thus, the difference we observe could be\npossibly due to the effect of grain growth in denser regions. Finally, the\nslopes in our diagrams are somewhat less steep than those from the study of\nIndebetouw et al. (2005) for clouds with lower column densities, and this\nindicates that the extinction law between 3 and 8 micron might vary slightly as\na function of environment.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:01:09 GMT\"}]', '2015-05-13', '[[\"Román-Zúñiga\",\"C.\",\"\"],[\"Lada\",\"C.\",\"\"],[\"Muench\",\"A.\",\"\"],[\"Alves\",\"J.\",\"\"]]'),
(704.3204, 'John Wisniewski', 'John P. Wisniewski (1), Karen S. Bjorkman (2), Antonio M. Magalhaes\n  (3), and Antonio Pereyra (3); ((1) NASA GSFC; (2) University of Toledo; (3)\n  University of Sao Paulo)', 'The Magnetic Field Structure of the LMC 2 Supershell: NGC 2100', '12 pages, accepted by ApJ, emulateapj5 format, full-resolution\n  figures available upon request (jwisnie@milkyway.gsfc.nasa.gov)', '', '10.1086/519155', '', 'astro-ph', '', '  We present U,B,V,R,I imaging polarimetry of NGC 2100 and its surrounding\nenvironment, which comprise a part of the LMC 2 supershell. The morphology of\nthe observed position angle distribution provides a tracer of the projected\nmagnetic field in this environment. Our polarization maps detail regions\nexhibiting similarly aligned polarization position angles, as well as more\ncomplex position angle patterns. We observe regions of coherent fields on\nspatial scales of 42 x 24 pc to 104 x 83 pc, and infer projected field\nstrengths of $\\sim14-30\\mu$G. We propose that the superposition of global\noutflows from the LMC 2 environment, as well as outflows created within NGC\n2100, produce the unique field geometry in the region.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:04:49 GMT\"}]', '2009-11-13', '[[\"Wisniewski\",\"John P.\",\"\"],[\"Bjorkman\",\"Karen S.\",\"\"],[\"Magalhaes\",\"Antonio M.\",\"\"],[\"Pereyra\",\"Antonio\",\"\"],[\";\",\"\",\"\"]]'),
(704.3205, 'Falk Neugebohrn', 'Falk Neugebohrn', 'Renormalization and Effective Actions for General Relativity', 'PhD thesis, 155 pages', '', '', '', 'hep-th', '', '  Quantum gravity is analyzed from the viewpoint of the renormalization group.\nThe analysis is based on methods introduced by J. Polchinski concerning the\nperturbative renormalization with flow equations. In the first part of this\nwork, the program of renormalization with flow equations is reviewed and then\nextended to effective field theories that have a finite UV cutoff. This is done\nfor a scalar field theory by imposing additional renormalization conditions for\nsome of the nonrenormalizable couplings. It turns out that one so obtains a\nstatement on the predictivity of the effective theory at scales far below the\nUV cutoff. In particular, nonrenormalizable theories can be treated without\nproblems in the proposed framework. In the second part, the standard covariant\nBRS quantization program for Euclidean Einstein gravity is applied. A momentum\ncutoff regularization is imposed and the resulting violation of the\nSlavnov-Taylor identities is discussed. Deriving Polchinski\'s renormalization\ngroup equation for Euclidean quantum gravity, the predictivity of effective\nquantum gravity at scales far below the Planck scale is investigated with flow\nequations. A fine-tuning procedure for restoring the violated Slavnov-Taylor\nidentities is proposed and it is argued that in the effective quantum gravity\ncontext, the restoration will only be accomplished with finite accuracy.\nFinally, the no-cutoff limit of Euclidean quantum gravity is analyzed from the\nviewpoint of the Polchinski method. It is speculated whether a limit with\nnonvanishing gravitational constant might exist where the latter would\nultimatively be determined by the cosmological constant and the masses of the\nelementary particles.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:49:11 GMT\"}]', '2007-05-23', '[[\"Neugebohrn\",\"Falk\",\"\"]]'),
(704.3206, 'Luca Del Zanna', 'L. Del Zanna, O. Zanotti, N. Bucciantini, P. Londrillo', 'ECHO: an Eulerian Conservative High Order scheme for general\n  relativistic magnetohydrodynamics and magnetodynamics', '20 pages, revised version submitted to A&A', '', '10.1051/0004-6361:20077093', '', 'astro-ph gr-qc', '', '  We present a new numerical code, ECHO, based on an Eulerian Conservative High\nOrder scheme for time dependent three-dimensional general relativistic\nmagnetohydrodynamics (GRMHD) and magnetodynamics (GRMD). ECHO is aimed at\nproviding a shock-capturing conservative method able to work at an arbitrary\nlevel of formal accuracy (for smooth flows), where the other existing GRMHD and\nGRMD schemes yield an overall second order at most. Moreover, our goal is to\npresent a general framework, based on the 3+1 Eulerian formalism, allowing for\ndifferent sets of equations, different algorithms, and working in a generic\nspace-time metric, so that ECHO may be easily coupled to any solver for\nEinstein\'s equations. Various high order reconstruction methods are implemented\nand a two-wave approximate Riemann solver is used. The induction equation is\ntreated by adopting the Upwind Constrained Transport (UCT) procedures,\nappropriate to preserve the divergence-free condition of the magnetic field in\nshock-capturing methods. The limiting case of magnetodynamics (also known as\nforce-free degenerate electrodynamics) is implemented by simply replacing the\nfluid velocity with the electromagnetic drift velocity and by neglecting the\nmatter contribution to the stress tensor. ECHO is particularly accurate,\nefficient, versatile, and robust. It has been tested against several\nastrophysical applications, including a novel test on the propagation of large\namplitude circularly polarized Alfven waves. In particular, we show that\nreconstruction based on a Monotonicity Preserving filter applied to a fixed\n5-point stencil gives highly accurate results for smooth solutions, both in\nflat and curved metric (up to the nominal fifth order), while at the same time\nproviding sharp profiles in tests involving discontinuities.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:51:49 GMT\"}]', '2009-11-13', '[[\"Del Zanna\",\"L.\",\"\"],[\"Zanotti\",\"O.\",\"\"],[\"Bucciantini\",\"N.\",\"\"],[\"Londrillo\",\"P.\",\"\"]]'),
(704.3207, 'Serguei Molodtsov', 'A.E. Dorokhov, S.V. Molodtsov, G.M. Zinovjev', 'Gluon condensate behaviour at filling the Fermi sphere up', '16 pages, 7 figures', '', '', '', 'hep-ph', '', '  The impact of filling up the Fermi sphere with the quarks, which dynamically\ngenerated their masses on the instanton liquid at finite temperature and\nbaryonic/quark number density, is investigated. It is demonstrated, in\nparticular, that the boundary of chiral symmetry restoration phase transition\nis shifted to the larger (about 100 MeV more) value of quark chemical potential\ncompared to the magnitude inherent in the Nambu-Jona-Lasinio model.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:55:03 GMT\"}]', '2007-05-23', '[[\"Dorokhov\",\"A. E.\",\"\"],[\"Molodtsov\",\"S. V.\",\"\"],[\"Zinovjev\",\"G. M.\",\"\"]]'),
(704.3208, 'Marcelo de Moura Leite', 'Paulo R. S. Carvalho and Marcelo M. Leite', 'Callan-Symanzik method for $m$-axial Lifshitz points', 'REVTeX 4, 22 pages', 'Annals Phys.324:178-204,2009; Erratum-ibid.324:2452,2009', '10.1016/j.aop.2008.05.006 10.1016/j.aop.2009.07.008', '', 'hep-th', '', '  We introduce the Callan-Symanzik method in the description of anisotropic as\nwell as isotropic Lifshitz critical behaviors. Renormalized perturbation\ntheories are defined by normalization conditions with nonvanishing masses and\nat zero external momenta. The orthogonal approximation is employed to obtain\nthe critical indices $\\eta_{L2}$, $\\nu_{L2}$, $\\eta_{L4}$ and $\\nu_{L4}$\ndiagramatically at least up to two-loop order in the anisotropic criticalities.\nThis approximation is also utilized to compute the exponents $\\eta_{L4}$ and\n$\\nu_{L4}$ in the isotropic case. Furthermore, we compute those exponents\nexactly for the isotropic behaviors at the same loop order. The results\nobtained for all exponents are in perfect agreement with those previously\nderived in the massless theories renormalized at nonzero external momenta.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 14:57:32 GMT\"}]', '2009-10-06', '[[\"Carvalho\",\"Paulo R. S.\",\"\"],[\"Leite\",\"Marcelo M.\",\"\"]]'),
(704.3209, 'Wang-Kong Tse', 'Wang-Kong Tse, Ben Yu-Kuang Hu, S. Das Sarma', 'Coulomb Drag in Graphene', '', 'Phys. Rev. B 76, 081401(R) (2007)', '10.1103/PhysRevB.76.081401', '', 'cond-mat.mes-hall', '', '  We study the Coulomb drag between two single graphene sheets in intrinsic and\nextrinsic graphene systems with no interlayer tunneling. The general expression\nfor the nonlinear susceptibility appropriate for single-layer graphene systems\nis derived using the diagrammatic perturbation theory, and the corresponding\nexact zero-temperature expression is obtained analytically. We find that,\ndespite the existence of a non-zero conductivity in an intrinsic graphene\nlayer, the Coulomb drag between intrinsic graphene layers vanishes at all\ntemperatures. In extrinsic systems, we obtain numerical results and an\napproximate analytical result for the drag resistivity $\\rho_{\\textrm{D}}$, and\nfind that $\\rho_{\\textrm{D}}$ goes as $T^2$ at low temperature $T$, as $1/d^4$\nfor large bilayer separation $d$ and $1/n^3$ for high carrier density $n$. We\nalso discuss qualitatively the effect of plasmon-induced enhancement on the\nCoulomb drag, which should occur at a temperature of the order of or higher\nthan the Fermi temperature.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:26:10 GMT\"}]', '2009-11-13', '[[\"Tse\",\"Wang-Kong\",\"\"],[\"Hu\",\"Ben Yu-Kuang\",\"\"],[\"Sarma\",\"S. Das\",\"\"]]'),
(704.3210, 'Ganpathy Murthy', 'Ganpathy Murthy, R. Shankar', 'Hamiltonian theory of the half-filled Landau level with disorder:\n  Application to recent NMR data', '21 pages, 6 figures', '', '10.1103/PhysRevB.76.075341', '', 'cond-mat.mes-hall', '', '  The Hamiltonian Theory of the fractional quantum Hall effect is an operator\ndescription that subsumes many properties of Composite Fermions, applies to\ngapped and gapless cases, and has been found to provide results in quantitative\naccord with data on gaps, relaxation rates and polarizations at temperatures of\n$300mK$ and above. The only free parameter is $\\lambda$, which is related to\nthe sample thickness and appears in the Zhang-Das Sarma potential $v(q) = {2\\pi\ne^2\\over \\kappa q} e^{-ql\\lambda}$ where $l$ and $\\kappa $ are the magnetic\nlength and dielectric constant. Here we examine the recent data of Tracy and\nEisenstein on the nuclear magnetic resonance relaxation rate at filling factor\n$\\nu=\\half$ deduced from resistivity measurements at temperatures as low as\n$45mK$. We find that their results can be satisfactorily described by this\ntheory, if in addition to a $v(q)$ with $\\lambda \\simeq 2$, a constant disorder\nwidth $\\Gamma\\simeq 100 mK$ is incorporated.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:02:50 GMT\"}]', '2009-11-13', '[[\"Murthy\",\"Ganpathy\",\"\"],[\"Shankar\",\"R.\",\"\"]]'),
(704.3211, 'Fabio Peano', 'F. Peano, G. Coppa, F. Peinetti, R. Mulas, and L. O. Silva', 'Ergodic model for the expansion of spherical nanoplasmas', 'To appear on Physical Review E', '', '10.1103/PhysRevE.75.066403', '', 'physics.plasm-ph', '', '  Recently, the collisionless expansion of spherical nanoplasmas has been\nanalyzed with a new ergodic model, clarifying the transition from\nhydrodynamic-like to Coulomb-explosion regimes, and providing accurate laws for\nthe relevant features of the phenomenon. A complete derivation of the model is\nhere presented. The important issue of the self-consistent initial conditions\nis addressed by analyzing the initial charging transient due to the electron\nexpansion, in the approximation of immobile ions. A comparison among different\nkinetic models for the expansion is presented, showing that the ergodic model\nprovides a simplified description, which retains the essential information on\nthe electron distribution, in particular, the energy spectrum. Results are\npresented for a wide range of initial conditions (determined from a single\ndimensionless parameter), in excellent agreement with calculations from the\nexact Vlasov-Poisson theory, thus providing a complete and detailed\ncharacterization of all the stages of the expansion.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:26:00 GMT\"}]', '2009-11-13', '[[\"Peano\",\"F.\",\"\"],[\"Coppa\",\"G.\",\"\"],[\"Peinetti\",\"F.\",\"\"],[\"Mulas\",\"R.\",\"\"],[\"Silva\",\"L. O.\",\"\"]]'),
(704.3212, 'Ryan Heary', 'R. J. Heary, J. E. Han and Lingyin Zhu', 'Spin-charge filtering through a spin-orbit coupled quantum dot\n  controlled via an Aharonov-Bohm interferometer', '8 pages, 10 figures', '', '10.1103/PhysRevB.77.115132', '', 'cond-mat.str-el cond-mat.mes-hall', '', '  We show that a strongly correlated quantum dot embedded in an Aharonov-Bohm\ninterferometer can be used to filter both charge and spin at zero voltage bias.\nThe magnitude with which the Aharonov-Bohm arm is coupled to the system\ncontrols the many-body effects on the quantum dot. When the quantum dot is in\nthe Kondo regime the flow of charge through the system can be tuned by the\nphase of the Aharonov-Bohm arm, $\\phi_{AB}$. Furthermore when a spin-orbit\ninteraction is present on a Kondo quantum dot we can control the flow of spin\nby the spin-orbit phase, $\\phi_{SO}$. The existence of the Kondo peak at the\nFermi energy makes it possible to control the flow of both charge and spin in\nthe zero voltage bias limit.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:25:34 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 11 Jul 2007 15:58:39 GMT\"},{\"version\":\"v3\",\"created\":\"Tue, 20 Nov 2007 16:19:52 GMT\"}]', '2009-11-13', '[[\"Heary\",\"R. J.\",\"\"],[\"Han\",\"J. E.\",\"\"],[\"Zhu\",\"Lingyin\",\"\"]]'),
(704.3213, 'Lasse Rempe', 'G\\\"unter Rottenfu{\\ss}er, Johannes R\\\"uckert, Lasse Rempe and Dierk\n  Schleicher', 'Dynamic rays of bounded-type entire functions', '42 pages, 9 figures. V2. General revisions and corrections.\n  Definition of the class \\B_{\\log} harmonized with other papers; some results\n  added/restated for future reference; details added in proofs of Theorem 6.3\n  and of Lemma A.3', 'Ann. of Math. 173 (2011), no. 1, 77-125', '10.4007/annals.2010.173.1.3', 'Stony Brook IMS Preprint #2007/05', 'math.DS math.CV math.GN', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We construct an entire function in the Eremenko-Lyubich class $\\B$ whose\nJulia set has only bounded path-components. This answers a question of Eremenko\nfrom 1989 in the negative.\n  On the other hand, we show that for many functions in $\\B$, in particular\nthose of finite order, every escaping point can be connected to $\\infty$ by a\ncurve of escaping points. This gives a partial positive answer to the\naforementioned question of Eremenko, and answers a question of Fatou from 1926.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:19:58 GMT\"},{\"version\":\"v2\",\"created\":\"Sat, 28 Feb 2009 22:56:29 GMT\"}]', '2011-01-07', '[[\"Rottenfußer\",\"Günter\",\"\"],[\"Rückert\",\"Johannes\",\"\"],[\"Rempe\",\"Lasse\",\"\"],[\"Schleicher\",\"Dierk\",\"\"]]'),
(704.3214, 'Dario Benedetti', 'D. Benedetti, R. Loll, F. Zamponi', '(2+1)-Dimensional Quantum Gravity as the Continuum Limit of Causal\n  Dynamical Triangulations', '38 pages, 13 figures', 'Phys.Rev.D76:104022,2007', '10.1103/PhysRevD.76.104022', '', 'hep-th gr-qc', '', '  We perform a non-perturbative sum over geometries in a (2+1)-dimensional\nquantum gravity model given in terms of Causal Dynamical Triangulations.\nInspired by the concept of triangulations of product type introduced\npreviously, we impose an additional notion of order on the discrete, causal\ngeometries. This simplifies the combinatorial problem of counting geometries\njust enough to enable us to calculate the transfer matrix between boundary\nstates labelled by the area of the spatial universe, as well as the\ncorresponding quantum Hamiltonian of the continuum theory. This is the first\ntime in dimension larger than two that a Hamiltonian has been derived from such\na model by mainly analytical means, and opens the way for a better\nunderstanding of scaling and renormalization issues.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:22:13 GMT\"}]', '2008-11-26', '[[\"Benedetti\",\"D.\",\"\"],[\"Loll\",\"R.\",\"\"],[\"Zamponi\",\"F.\",\"\"]]'),
(704.3215, 'Oleg Ruchayskiy', 'Oleg Ruchayskiy', 'Restrictions on sterile neutrino parameters from astrophysical\n  observations', '3 pages. Contribution to the Proceedings of 11 Marcel Grossmann\n  meeting', '', '10.1142/9789812834300_0052', '', 'astro-ph', '', '  Adding 3 right-handed (sterile) neutrino to the Standard Model (SM) can solve\nseveral \"beyond the Standard Model\" problems within one consistent framework:\nexplain neutrino oscillations and baryon asymmetry of the Universe and provide\na dark matter (DM) candidate. In this talk I will present current status of\nastrophysical searches for the DM sterile neutrino.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:32:41 GMT\"}]', '2016-11-15', '[[\"Ruchayskiy\",\"Oleg\",\"\"]]'),
(704.3216, 'Joel Merker', 'Joel Merker and Egmont Porten', 'The Hartogs extension theorem on (n-1)-complete complex spaces', '19 pages, 5 figures', '', '', '', 'math.CV math.DG', '', '  Employing Morse theory for the global control of monodromy and the method of\nanalytic discs for local extension, we establish a version of the global\nHartogs extension theorem in a singular setting: for every domain D of an\n(n-1)-complete normal complex space X of pure dimension n >= 2 and for every\ncompact set K in D such that D - K is connected, holomorphic or meromorphic\nfunctions in D - K extend holomorphically or meromorphically to D. Normality is\nan unvavoidable assumption for holomorphic extension, but we show that\nmeromorphic extension holds on a reduced globally irreducible (not necessarily\nnormal) X of pure dimension n >=2 provided that the regular part of D - K is\nconnected.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:22:33 GMT\"}]', '2007-05-23', '[[\"Merker\",\"Joel\",\"\"],[\"Porten\",\"Egmont\",\"\"]]'),
(704.3217, 'Dmitry Novikov', 'Dmitry Novikov', 'On limit cycles appearing by polynomial perturbation of Darbouxian\n  integrable systems', '21 pages, 2 figures, LaTeX', '', '', '', 'math.CA math.DS', '', '  We prove an existential finiteness Varchenko-Khovanskii type result for\nintegrals of rational 1-forms over the level curves of Darbouxian integrals.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:04:25 GMT\"}]', '2007-05-23', '[[\"Novikov\",\"Dmitry\",\"\"]]'),
(704.3218, 'Cornelius Krellner', 'C. Krellner, S. Haas, C. Goldmann, K. P. Pernstich, D. J. Gundlach, B.\n  Batlogg (Laboratory for Solid State Physics, ETH Zurich, Switzerland)', 'Density of bulk trap states in organic semiconductor crystals: discrete\n  levels induced by oxygen in rubrene', 'published in Phys. Rev. B, high quality figures:\n  http://www.cpfs.mpg.de/~krellner/', 'Phys. Rev. B 75, 245115 (2007)', '10.1103/PhysRevB.75.245115', '', 'cond-mat.mtrl-sci', '', '  The density of trap states in the bandgap of semiconducting organic single\ncrystals has been measured quantitatively and with high energy resolution by\nmeans of the experimental method of temperature-dependent\nspace-charge-limited-current spectroscopy (TD-SCLC). This spectroscopy has been\napplied to study bulk rubrene single crystals, which are shown by this\ntechnique to be of high chemical and structural quality. A density of deep trap\nstates as low as ~ 10^{15} cm^{-3} is measured in the purest crystals, and the\nexponentially varying shallow trap density near the band edge could be\nidentified (1 decade in the density of states per ~25 meV). Furthermore, we\nhave induced and spectroscopically identified an oxygen related sharp hole bulk\ntrap state at 0.27 eV above the valence band.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:39:37 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 19 Jun 2007 10:47:39 GMT\"}]', '2007-06-19', '[[\"Krellner\",\"C.\",\"\",\"Laboratory for Solid State Physics, ETH Zurich, Switzerland\"],[\"Haas\",\"S.\",\"\",\"Laboratory for Solid State Physics, ETH Zurich, Switzerland\"],[\"Goldmann\",\"C.\",\"\",\"Laboratory for Solid State Physics, ETH Zurich, Switzerland\"],[\"Pernstich\",\"K. P.\",\"\",\"Laboratory for Solid State Physics, ETH Zurich, Switzerland\"],[\"Gundlach\",\"D. J.\",\"\",\"Laboratory for Solid State Physics, ETH Zurich, Switzerland\"],[\"Batlogg\",\"B.\",\"\",\"Laboratory for Solid State Physics, ETH Zurich, Switzerland\"]]'),
(704.3219, 'Juan Manuel Borrero', 'J.M. Borrero', 'The structure of sunspot penumbrae IV. MHS equilibrium for penumbral\n  flux tubes and the origin of dark core penumbral filaments and penumbral\n  grains', 'Accepted for publication in Astronomy & Astrophysics. 10 pages, 7\n  figures (3 color figures)', '', '10.1051/0004-6361:20066776', '', 'astro-ph', '', '  We study the magnetohydrostatic equilibrium of magnetic flux tubes with\ncircular cross sections embedded in a magnetic surrounding atmosphere. We solve\nthe static momentum equation in 2.5D to obtain the thermodynamics that are\nconsistent with a prescribed velocity and magnetic fields. We show that force\nbalance is roughly satisfied if the flux tube\'s magnetic field is aligned with\nits axis. Equilibrium is guaranteed if this magnetic field possesses a\ntransverse component. Several forms of this transverse field are investigated.\nThe resulting magnetic field configurations are critically reviewed in terms of\nthe results from spectropolarimetric observations. The thermodynamic structure\nthat allows the flux tube to be in mechanical equilibrium is also calculated.\nWe show that the inferred pressure, density and temperature stratification\nreproduce intensity features similar to dark core penumbral filaments and\npenumbral grains.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:42:28 GMT\"}]', '2009-11-13', '[[\"Borrero\",\"J. M.\",\"\"]]'),
(704.3220, 'Peter Horvathy', 'P. A. Horvathy', 'Lectures on (abelian) Chern-Simons vortices', '51 pages, 9 figures. Lectures delivered at NIKHEF (Amsterdam), July\n  2006', '', '', '', 'hep-th', '', '  Various aspects including the construction and the symmetries of Abelian\nChern-Simons vortices are reviewed. Extended version of the Lectures delivered\nat NIKHEF (Amsterdam), July 2006. Typos corrected, some refernces added.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:43:22 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 9 May 2007 13:41:18 GMT\"}]', '2007-05-23', '[[\"Horvathy\",\"P. A.\",\"\"]]'),
(704.3221, 'Manuel Lladser', 'Manuel Lladser, M. D. Betterton, Rob Knight', 'Multiple pattern matching: A Markov chain approach', 'Final version to appear in the Journal of Mathematical Biology', '', '', '', 'math.PR math.CO math.ST q-bio.GN q-bio.QM stat.TH', '', '  RNA motifs typically consist of short, modular patterns that include base\npairs formed within and between modules. Estimating the abundance of these\npatterns is of fundamental importance for assessing the statistical\nsignificance of matches in genomewide searches, and for predicting whether a\ngiven function has evolved many times in different species or arose from a\nsingle common ancestor. In this manuscript, we review in an integrated and\nself-contained manner some basic concepts of automata theory, generating\nfunctions and transfer matrix methods that are relevant to pattern analysis in\nbiological sequences. We formalize, in a general framework, the concept of\nMarkov chain embedding to analyze patterns in random strings produced by a\nmemoryless source. This conceptualization, together with the capability of\nautomata to recognize complicated patterns, allows a systematic analysis of\nproblems related to the occurrence and frequency of patterns in random strings.\nThe applications we present focus on the concept of synchronization of\nautomata, as well as automata used to search for a finite number of keywords\n(including sets of patterns generated according to base pairing rules) in a\ngeneral text.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:12:45 GMT\"}]', '2007-05-23', '[[\"Lladser\",\"Manuel\",\"\"],[\"Betterton\",\"M. D.\",\"\"],[\"Knight\",\"Rob\",\"\"]]'),
(704.3222, 'Yves van Gennip', 'Yves van Gennip and Mark A. Peletier', 'Copolymer-homopolymer blends: global energy minimisation and global\n  energy bounds', '31 pages, 6 Postscript figures; to be published in Calc. Var. Partial\n  Differential Equations. Version history: Changes in v2 w.r.t v1 only concern\n  metadata. V3 contains some minor revisions and additions w.r.t. v2. V4\n  corrects a confusing typo in one of the formulas of the appendix. V5 is the\n  definitive version that will appear in print', '', '', '', 'math-ph math.MP', '', '  We study a variational model for a diblock-copolymer/homopolymer blend. The\nenergy functional is a sharp-interface limit of a generalisation of the\nOhta-Kawasaki energy. In one dimension, on the real line and on the torus, we\nprove existence of minimisers of this functional and we describe in complete\ndetail the structure and energy of stationary points. Furthermore we\ncharacterise the conditions under which the minimisers may be non-unique.\n  In higher dimensions we construct lower and upper bounds on the energy of\nminimisers, and explicitly compute the energy of spherically symmetric\nconfigurations.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:07:46 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 11:17:41 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 17 Sep 2007 09:45:28 GMT\"},{\"version\":\"v4\",\"created\":\"Tue, 18 Sep 2007 10:21:56 GMT\"},{\"version\":\"v5\",\"created\":\"Tue, 30 Oct 2007 09:21:36 GMT\"}]', '2007-10-30', '[[\"van Gennip\",\"Yves\",\"\"],[\"Peletier\",\"Mark A.\",\"\"]]'),
(704.3223, 'Benedikt Obermayer', 'Benedikt Obermayer and Oskar Hallatschek', 'Coupling of transverse and longitudinal response in stiff polymers', '4 pages, 3 figures, 1 table; final version', 'Phys. Rev. Lett. 99 (2007) 098302', '10.1103/PhysRevLett.99.098302', 'LMU-ASC 25/07', 'cond-mat.soft q-bio.BM', '', '  The time-dependent transverse response of stiff polymers, represented as\nweakly-bending wormlike chains (WLCs), is well-understood on the linear level,\nwhere transverse degrees of freedom evolve independently from the longitudinal\nones. We show that, beyond a characteristic time scale, the nonlinear coupling\nof transverse and longitudinal motion in an inextensible WLC significantly\nweakens the polymer response compared to the widely used linear response\npredictions. The corresponding feedback mechanism is rationalized by scaling\narguments and quantified by a multiple scale approach that exploits an inherent\nseparation of transverse and longitudinal correlation length scales. Crossover\nscaling laws and exact analytical and numerical solutions for characteristic\nresponse quantities are derived for different experimentally relevant setups.\nOur findings are applicable to cytoskeletal filaments as well as DNA under\ntension.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 15:57:03 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 3 Sep 2007 15:19:50 GMT\"}]', '2007-09-03', '[[\"Obermayer\",\"Benedikt\",\"\"],[\"Hallatschek\",\"Oskar\",\"\"]]'),
(704.3224, 'Ignacio Negueruela', 'Ignacio Negueruela (Universidad de Alicante), David M. Smith (UCSC),\n  Jose Miguel Torrejon (alicante), Pablo Reig (FORTH/University of Crete)', 'Supergiant Fast X-ray Transients: A common behaviour or a class of\n  objects?', 'To appear in \'\'Proceedings of the 6th Integral Workshop \"The obscured\n  Universe\", Moscow, July 3-7 2006\'\' (replaced with refereed version 10 May\n  07). Best viewed in PDF format', 'ESA SP-622, 255 (2008)', '', '', 'astro-ph', '', '  INTEGRAL monitoring of the Galactic Plane is revealing a growing number of\nrecurrent X-ray transients, characterised by short outbursts with very fast\nrise times (~ tens of minutes) and typical durations of a few hours. A\nsubstantial fraction of these sources are associated with OB supergiants and\nhence define a new class of massive X-ray binaries, which we call Supergiant\nFast X-ray Transients. Characterisation of the astrophysical parameters of\ntheir counterparts is underway. So far, we have found a number of late O and\nearly B supergiants of different luminosities at a large range of distances.\nNothing in their optical properties sets them apart from classical Supergiant\nX-ray Binaries. On the other hand, there is now rather concluding evidence that\npersistent supergiant X-ray binaries also show fast outbursts. This suggests a\ncontinuum of behaviours between typical persistent supergiant systems and\npurely transient systems, but offers very little information about the physical\ncauses of the outbursts.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:02:33 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 10 May 2007 15:28:38 GMT\"}]', '2008-01-28', '[[\"Negueruela\",\"Ignacio\",\"\",\"Universidad de Alicante\"],[\"Smith\",\"David M.\",\"\",\"UCSC\"],[\"Torrejon\",\"Jose Miguel\",\"\",\"alicante\"],[\"Reig\",\"Pablo\",\"\",\"FORTH/University of Crete\"]]'),
(704.3225, 'Alexey A. Kryukov', 'Alexey A. Kryukov', 'Linear algebra and differential geometry on abstract Hilbert space', '37 pages, 3 figures, see\n  http://www.uwc.edu/dept/math/faculty/kryukov/ for additional applications', 'Int. J. Math & Math. Sci. 14, 2241 (2005)', '', '', 'math-ph math.MP quant-ph', '', '  Isomorphisms of separable Hilbert spaces are analogous to isomorphisms of\nn-dimensional vector spaces. However, while n-dimensional spaces in\napplications are always realized as the Euclidean space R^n, Hilbert spaces\nadmit various useful realizations as spaces of functions. In the paper this\nsimple observation is used to construct a fruitful formalism of local\ncoordinates on Hilbert manifolds. Images of charts on manifolds in the\nformalism are allowed to belong to arbitrary Hilbert spaces of functions\nincluding spaces of generalized functions. Tensor equations then describe\nfamilies of functional equations on various spaces of functions. The formalism\nitself and its applications in linear algebra, differential equations and\ndifferential geometry are analyzed.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:03:01 GMT\"}]', '2007-05-23', '[[\"Kryukov\",\"Alexey A.\",\"\"]]'),
(704.3226, 'Radhakrishnan Nagarajan', 'Radhakrishnan Nagarajan', 'Delay estimation in a two-node acyclic network', '33 Pages, 6 Figures', 'Physica A: Volume 376, 15 March 2007, Pages 725-737', '10.1016/j.physa.2006.10.067', '', 'q-bio.QM q-bio.MN', '', '  Linear measures such as cross-correlation have been used successfully to\ndetermine time delays from the given processes. Such an analysis often precedes\nidentifying possible causal relationships between the observed processes. The\npresent study investigates the impact of a positively correlated driver whose\ncorrelation function decreases monotonically with lag on the delay estimation\nin a two-node acyclic network with one and two-delays. It is shown that\ncross-correlation analysis of the given processes can result in spurious\nidentification of multiple delays between the driver and the dependent\nprocesses. Subsequently, delay estimation of increment process as opposed to\nthe original process under certain implicit constraints is explored.\nShort-range and long-range correlated driver processes along with those of\ntheir coarse-grained counterparts are considered.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:07:15 GMT\"}]', '2015-05-13', '[[\"Nagarajan\",\"Radhakrishnan\",\"\"]]'),
(704.3227, 'O. Stenull', 'Olaf Stenull', 'Smectic elastomer membranes', '10 pages, 2 figures', 'Phys. Rev. E 75, 051702 (2007)', '10.1103/PhysRevE.75.051702', '', 'cond-mat.soft', '', '  We present a model for smectic elastomer membranes which includes elastic and\nliquid crystalline degrees of freedom. Based on our model, we determined the\nqualitative phase diagram of a smectic elastomer membrane using mean-field\ntheory. This phase diagram is found to comprise five phases, viz.\nsmectic-A--flat, smectic-A--crumpled, smectic-C--flat, smectic-C--crumpled and\nsmectic-C--tubule, where in the latter phase, the membrane is flat in the\ndirection of mesogenic tilt and crumpled in the perpendicular direction. The\ntransitions between adjacent phases are second order phase transitions. We\nstudy in some detail the elasticity of the smectic-C--flat and the\nsmectic-C--tubule phases which are associated with a spontaneous breaking of\nin-plane rotational symmetry. As a consequence of the Goldstone theorem, these\nphases exhibit soft elasticity characterized by the vanishing of in-plane shear\nmoduli.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:08:37 GMT\"}]', '2009-11-13', '[[\"Stenull\",\"Olaf\",\"\"]]'),
(704.3228, 'Thomas Silverston', 'Thomas Silverston, Olivier Fourmaux and Kave Salamatian', 'Characterization of P2P IPTV Traffic: Scaling Analysis', '27p, submitted to a conference', '', '', '', 'cs.NI cs.MM', '', '  P2P IPTV applications arise on the Internet and will be massively used in the\nfuture. It is expected that P2P IPTV will contribute to increase the overall\nInternet traffic. In this context, it is important to measure the impact of P2P\nIPTV on the networks and to characterize this traffic. Dur- ing the 2006 FIFA\nWorld Cup, we performed an extensive measurement campaign. We measured network\ntraffic generated by broadcasting soc- cer games by the most popular P2P IPTV\napplications, namely PPLive, PPStream, SOPCast and TVAnts. From the collected\ndata, we charac- terized the P2P IPTV traffic structure at different time\nscales by using wavelet based transform method. To the best of our knowledge,\nthis is the first work, which presents a complete multiscale analysis of the\nP2P IPTV traffic. Our results show that the scaling properties of the TCP\ntraffic present periodic behavior whereas the UDP traffic is stationary and\nlead to long- range depedency characteristics. For all the applications, the\ndownload traffic has different characteristics than the upload traffic. The\nsignaling traffic has a significant impact on the download traffic but it has\nnegligible impact on the upload. Both sides of the traffic and its granularity\nhas to be taken into account to design accurate P2P IPTV traffic models.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:18:13 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Jul 2007 14:26:05 GMT\"}]', '2007-07-17', '[[\"Silverston\",\"Thomas\",\"\"],[\"Fourmaux\",\"Olivier\",\"\"],[\"Salamatian\",\"Kave\",\"\"]]'),
(704.3229, 'Tabetha Boyajian', 'T. S. Boyajian, D. R. Gies, J. P. Dunn, C. D. Farrington, E. D.\n  Grundstrom, W. Huang, M. V. McSwain, S. J. Williams, D. W. Wingert, A. W.\n  Fullerton, C. T. Bolton', 'The Long Period, Massive Binaries HD 37366 and HD 54662: Potential\n  Targets for Long Baseline Optical Interferometry', '27 pages, 8 figures, Accepted for publication in ApJ', 'Astrophys.J.664:1121-1129,2007', '10.1086/519015', '', 'astro-ph', '', '  We present the results from an optical spectroscopic analysis of the massive\nstars HD 37366 and HD 54662. We find that HD 37366 is a double-lined\nspectroscopic binary with a period of 31.8187 +/- 0.0004 days, and HD 54662 is\nalso a double lined binary with a much longer period of 557.8 +/- 0.3 days. The\nprimary of HD 37366 is classified as O9.5 V, and it contributes approximately\ntwo-thirds of the optical flux. The less luminous secondary is a broad-lined,\nearly B-type main-sequence star. Tomographic reconstruction of the individual\nspectra of HD 37366 reveals absorption lines present in each component,\nenabling us to constrain the nature of the secondary and physical\ncharacteristics of both stars. Tomographic reconstruction was not possible for\nHD 54662; however, we do present mean spectra from our observations that show\nthat the secondary component is approximately half as bright as the primary.\nThe observed spectral energy distributions (SEDs) were fit with model SEDs and\ngalactic reddening curves to determine the angular sizes of the stars. By\nassuming radii appropriate for their classifications, we determine distance\nranges of 1.4 - 1.9 and 1.2 - 1.5 kpc for HD 37366 and HD 54662, respectively.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:11:15 GMT\"}]', '2009-11-13', '[[\"Boyajian\",\"T. S.\",\"\"],[\"Gies\",\"D. R.\",\"\"],[\"Dunn\",\"J. P.\",\"\"],[\"Farrington\",\"C. D.\",\"\"],[\"Grundstrom\",\"E. D.\",\"\"],[\"Huang\",\"W.\",\"\"],[\"McSwain\",\"M. V.\",\"\"],[\"Williams\",\"S. J.\",\"\"],[\"Wingert\",\"D. W.\",\"\"],[\"Fullerton\",\"A. W.\",\"\"],[\"Bolton\",\"C. T.\",\"\"]]'),
(704.3230, 'Axel Arnold', 'Axel Arnold and Suckjoon Jun', 'Time scale of entropic segregation of flexible polymers in confinement:\n  Implications for chromosome segregation in filamentous bacteria', 'Minor changes. Added some references, corrected the labels in figure\n  6 and reformatted in two columns. Also added reference to published version\n  in PRE', 'A. Arnold and S. Jun, Phys. Rev. E 76, 031901 (2007)', '10.1103/PhysRevE.76.031901', '', 'cond-mat.soft', '', '  We report molecular dynamics simulations of the segregation of two\noverlapping chains in cylindrical confinement. We find that the entropic\nrepulsion between the chains can be sufficiently strong to cause segregation on\na time scale that is short compared to the one for diffusion. This result\nimplies that entropic driving forces are sufficiently strong to cause rapid\nbacterial chromosome segregation.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:14:25 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 7 Sep 2007 14:02:09 GMT\"}]', '2011-11-09', '[[\"Arnold\",\"Axel\",\"\"],[\"Jun\",\"Suckjoon\",\"\"]]'),
(704.3231, 'Ravi Vakil', 'Robert W. Easton and Ravi Vakil', 'Absolute Galois acts faithfully on the components of the moduli space of\n  surfaces: A Belyi-type theorem in higher dimension', '7 pages', '', '', '', 'math.AG math.NT', '', '  Given an object over the algebraic closure Qbar of Q, there is often no\nreason for invariants of the corresponding holomorphic object to be preserved\nby the absolute Galois group Gal(Qbar/Q), and in general this is not true,\nalthough it is sometimes surprising to observe in practice. The case of covers\nof the projective line branched only over the points 0, 1, and infinity,\nthrough Belyi\'s theorem, leads to Grothendieck\'s dessins d\'enfants program for\nunderstanding the absolute Galois group through its faithful action on such\ncovers. This note is motivated by Catanese\'s question about a\nhigher-dimensional analogue: does the absolute Galois group act faithfully on\nthe deformation equivalence classes of smooth surfaces? (These equivalence\nclasses are of course by definition the strongest deformation invariants.) We\ngive a short proof of a weaker result: the absolute Galois group acts\nfaithfully on the irreducible components of the moduli space of smooth surfaces\n(of general type, canonically polarized). Bauer, Catanese, and Grunewald have\nrecently answered Catanese\'s original question using a different construction.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:22:27 GMT\"}]', '2007-05-23', '[[\"Easton\",\"Robert W.\",\"\"],[\"Vakil\",\"Ravi\",\"\"]]'),
(704.3232, 'S\\\'andor Szab\\\'o', 'V.E.S. Szabo', 'Characterization of polynomials', '5 pages', 'Analysis and Applications (Vol. 11, No. 02, March 2013)', '10.1142/S0219530513500152', '', 'math.AP math.FA', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  In 1954 it was proved if f is infinitely differentiable in the interval I and\nsome derivative (of order depending on x) vanishes at each x, then f is a\npolynomial. Later it was generalized for multi-variable case. In this paper we\ngive an extension for distributions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:22:40 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 22 Jul 2014 17:28:14 GMT\"}]', '2014-07-23', '[[\"Szabo\",\"V. E. S.\",\"\"]]'),
(704.3233, 'Marcelo Alloy', 'M. D. Alloy and D. P. Menezes', 'Slowly rotating pulsars', '', 'Int.J.Mod.Phys.E16:2826-2829,2007', '10.1142/S0218301307008501', '', 'astro-ph nucl-th', '', '  In the present work we investigate one possible variation on the usual static\npulsars: the inclusion of rotation. We use a formalism proposed by Hartle and\nThorne to calculate the properties of rotating pulsars with all possible\ncompositions. All calculations were performed for zero temperature and also for\nfixed entropy equations of state.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:30:12 GMT\"}]', '2009-06-23', '[[\"Alloy\",\"M. D.\",\"\"],[\"Menezes\",\"D. P.\",\"\"]]'),
(704.3234, 'Bernd-Jochen Schaefer', 'Bernd-Jochen Schaefer, Jan M. Pawlowski, Jochen Wambach', 'The Phase Structure of the Polyakov--Quark-Meson Model', '13 pages, 12 figures, RevTex4; discussion of mu-dependence extended,\n  references added, version to be published in PRD', 'Phys.Rev.D76:074023,2007', '10.1103/PhysRevD.76.074023', '', 'hep-ph hep-lat hep-th nucl-th', '', '  The relation between the deconfinement and chiral phase transition is\nexplored in the framework of an Polyakov-loop-extended two-flavor quark-meson\n(PQM) model. In this model the Polyakov loop dynamics is represented by a\nbackground temporal gauge field which also couples to the quarks. As a novelty\nan explicit quark chemical potential and N_f-dependence in the Polyakov loop\npotential is proposed by using renormalization group arguments. The behavior of\nthe Polyakov loop as well as the chiral condensate as function of temperature\nand quark chemical potential is obtained by minimizing the grand canonical\nthermodynamic potential of the system. The effect of the Polyakov loop dynamics\non the chiral phase diagram and on several thermodynamic bulk quantities is\npresented.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:59:18 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 24 Sep 2007 15:54:40 GMT\"}]', '2008-11-26', '[[\"Schaefer\",\"Bernd-Jochen\",\"\"],[\"Pawlowski\",\"Jan M.\",\"\"],[\"Wambach\",\"Jochen\",\"\"]]'),
(704.3235, 'Stephen Skinner', 'S.L. Skinner, S.A. Zhekov, M. Guedel, W. Schmutz', 'XMM-Newton X-ray Observations of the Wolf-Rayet Binary System WR 147', '8 pages, 7 figures', 'Mon.Not.Roy.Astron.Soc.378:1491-1498,2007', '10.1111/j.1365-2966.2007.11892.x', '', 'astro-ph', '', '  We present results of a 20 ksec X-ray observation of the Wolf-Rayet (WR)\nbinary system WR 147 obtained with XMM-Newton. Previous studies have shown that\nthis system consists of a nitrogen-type WN8 star plus an OB companion whose\nwinds are interacting to produce a colliding wind shock. X-ray spectra from the\npn and MOS detectors confirm the high extinction reported from IR studies and\nreveal hot plasma including the first detection of the Fe K-alpha line complex\nat 6.67 keV. Spectral fits with a constant-temperature plane-parallel shock\nmodel give a shock temperature kT(shock) = 2.7 keV [T(shock) ~ 31 MK], close to\nbut slightly hotter than the maximum temperature predicted for a colliding wind\nshock. Optically thin plasma models suggest even higher temperatures, which are\nnot yet ruled out. The X-ray spectra are harder than can be accounted for using\n2D numerical colliding wind shock models based on nominal mass-loss parameters.\nPossible explanations include: (i) underestimates of the terminal wind speeds\nor wind abundances, (ii) overly simplistic colliding wind models, or (iii) the\npresence of other X-ray emission mechanisms besides colliding wind shocks.\nFurther improvement of the numerical models to include potentially important\nphysics such as non-equilibrium ionization will be needed to rigorously test\nthe colliding wind interpretation.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:33:41 GMT\"}]', '2009-06-23', '[[\"Skinner\",\"S. L.\",\"\"],[\"Zhekov\",\"S. A.\",\"\"],[\"Guedel\",\"M.\",\"\"],[\"Schmutz\",\"W.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3236, 'Joao Yun', 'Joao L. Yun, Jose M. Torrelles, Nuno C. Santos', 'A \"diamond-ring\" star: the unusual morphologic structure of a young\n  (multiple?) object', '7 pages, 6 figures', '', '10.1051/0004-6361:20077248', '', 'astro-ph', '', '  We have observed IRAS06468-0325 obtaining optical and infrared images through\nIJHKs and L\' filters, K-band low-resolution spectroscopy, together with\nmillimetre line observations of CO and CS. IRAS06468-0325 has a very unusual\nand enigmatic morphology with two components: a bright, close to point-like\nsource (the diamond) and a sharp-edge ring-like structure (the ring). The\nsource is not detected in the optical, at wavelengths shorter than the I-band.\nThe diamond is seen in all the imaging bands observed. The ring-like structure\nin IRAS06468-0325 is clearly seen in the I, J, H, and Ks. It is not detected in\nthe L\'-band image. Infrared colours of the diamond are compatible with excess\ncircumstellar emission and a young stellar nature. A strongly non-gaussian and\nmoderately bright CO(1-0) and {13}CO(2-1) lines are seen towards\nIRAS06468-0325, at v_{LSR} of 30.5 km s{-1} (corresponding to a kinematic\ndistance of 3 kpc). Very weak C{18}O(2-1) and CS(2-1) lines were detected.\nK-band spectra of the diamond and of the ring are similar both in the slope of\nthe continuum and in the presence of lines supporting the idea that the ring is\nreflected light from the diamond. With the current data, a few different\nscenarios are possible to explain the morphology of this object. However, the\navailable data seem to favour that the morphology of IRAS06468-0325 correspond\nto a young stellar multiple system in a transient stage where a binary\nco-exists with a circumbinary disc, similar to the case of GG Tau. In this\ncase, the sharpness of the well-defined ring may be due to tidal truncation\nfrom dynamic interactions between components in a binary or multiple stellar\nsystem. IRAS06468-0325 may be an important rare case that illustrates a\nshort-lived stage of the process of binary or multiple star formation.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:34:30 GMT\"}]', '2009-11-13', '[[\"Yun\",\"Joao L.\",\"\"],[\"Torrelles\",\"Jose M.\",\"\"],[\"Santos\",\"Nuno C.\",\"\"]]'),
(704.3237, 'Jozsef Lorinczi', 'Massimiliano Gubinelli and Jozsef Lorinczi', 'Gibbs measures on Brownian currents', '51 pages', '', '', '', 'math-ph math.FA math.MP math.PR', '', '  Motivated by applications to quantum field theory we consider Gibbs measures\nfor which the reference measure is Wiener measure and the interaction is given\nby a double stochastic integral and a pinning external potential. In order\nproperly to characterize these measures through DLR equations, we are led to\nlift Wiener measure and other objects to a space of configurations where the\nbasic observables are not only the position of the particle at all times but\nalso the work done by test vector fields. We prove existence and basic\nproperties of such Gibbs measures in the small coupling regime by means of\ncluster expansion.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:35:08 GMT\"}]', '2007-05-23', '[[\"Gubinelli\",\"Massimiliano\",\"\"],[\"Lorinczi\",\"Jozsef\",\"\"]]'),
(704.3238, 'Nicolas Troquard', 'Philippe Balbiani, Andreas Herzig and Nicolas Troquard', 'Alternative axiomatics and complexity of deliberative STIT theories', 'Submitted to the Journal of Philosophical Logic; 13 pages excluding\n  annex', '', '10.1007/s10992-007-9078-7', '', 'cs.LO', '', '  We propose two alternatives to Xu\'s axiomatization of the Chellas STIT. The\nfirst one also provides an alternative axiomatization of the deliberative STIT.\nThe second one starts from the idea that the historic necessity operator can be\ndefined as an abbreviation of operators of agency, and can thus be eliminated\nfrom the logic of the Chellas STIT. The second axiomatization also allows us to\nestablish that the problem of deciding the satisfiability of a STIT formula\nwithout temporal operators is NP-complete in the single-agent case, and is\nNEXPTIME-complete in the multiagent case, both for the deliberative and the\nChellas\' STIT.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:36:13 GMT\"}]', '2011-04-29', '[[\"Balbiani\",\"Philippe\",\"\"],[\"Herzig\",\"Andreas\",\"\"],[\"Troquard\",\"Nicolas\",\"\"]]'),
(704.3239, 'Klaus Bartschat', 'X. Guan, O. Zatsarinny, K. Bartschat, B.I. Schneider, J. Feist, C.J.\n  Noble', 'A general approach to few-cycle intense laser interactions with complex\n  atoms', '7 pages (in the Phys. Rev. double column format) with 5 figures;\n  processed with REVTEX', 'Physical Review A 76 (2007), 053411', '10.1103/PhysRevA.76.053411', '', 'physics.atom-ph physics.comp-ph', '', '  A general {\\it ab-initio} and non-perturbative method to solve the\ntime-dependent Schr\\\"odinger equation (TDSE) for the interaction of a strong\nattosecond laser pulse with a general atom, i.e., beyond the models of\nquasi-one-electron or quasi-two-electron targets, is described. The field-free\nHamiltonian and the dipole matrices are generated using a flexible $B$-spline\n$R$-matrix method. This numerical implementation enables us to construct\nterm-dependent, non-orthogonal sets of one-electron orbitals for the bound and\ncontinuum electrons. The solution of the TDSE is propagated in time using the\nArnoldi-Lanczos method, which does not require the diagonalization of any large\nmatrices. The method is illustrated by an application to the multi-photon\nexcitation and ionization of Ne atoms. Good agreement with $R$-matrix Floquet\ncalculations for the generalized cross sections for two-photon ionization is\nachieved.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:39:59 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 13 Sep 2007 19:33:58 GMT\"}]', '2016-11-17', '[[\"Guan\",\"X.\",\"\"],[\"Zatsarinny\",\"O.\",\"\"],[\"Bartschat\",\"K.\",\"\"],[\"Schneider\",\"B. I.\",\"\"],[\"Feist\",\"J.\",\"\"],[\"Noble\",\"C. J.\",\"\"]]'),
(704.3240, 'Avtar Sehra', 'Avtar S. Sehra', 'Finite Element Analysis of the Schroedinger Equation', 'Computational Analysis of Schroedinger Equation', '', '', '', 'hep-lat', '', '  The purpose of this work is to test the application of the finite element\nmethod to quantum mechanical problems, in particular for solving the\nSchroedinger equation.\n  We begin with an overview of quantum mechanics, and standard numerical\ntechniques. We then give an introduction to finite element analysis using the\ndiffusion equation as an example. Three numerical time evolution methods are\nconsidered: the (tried and tested) Crank-Nicolson method, the continuous\nspace-time method, and the discontinuous space-time method.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 17 Apr 2007 12:37:35 GMT\"}]', '2009-09-29', '[[\"Sehra\",\"Avtar S.\",\"\"]]'),
(704.3241, 'Marco Lops', 'Daniele Angelosante, Ezio Biglieri, Marco Lops', 'Neighbor Discovery in Wireless Networks:A Multiuser-Detection Approach', '', '', '', '', 'cs.IT math.IT', '', '  We examine the problem of determining which nodes are neighbors of a given\none in a wireless network. We consider an unsupervised network operating on a\nfrequency-flat Gaussian channel, where $K+1$ nodes associate their identities\nto nonorthogonal signatures, transmitted at random times, synchronously, and\nindependently. A number of neighbor-discovery algorithms, based on different\noptimization criteria, are introduced and analyzed. Numerical results show how\nreduced-complexity algorithms can achieve a satisfactory performance.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:46:02 GMT\"}]', '2007-07-13', '[[\"Angelosante\",\"Daniele\",\"\"],[\"Biglieri\",\"Ezio\",\"\"],[\"Lops\",\"Marco\",\"\"]]'),
(704.3242, 'Louise Edwards', 'L. O. V. Edwards (1), Michael J. Hudson (2), Michael L. Balogh (2),\n  Russell J. Smith (3) ((1) Universit\\\'e Laval, (2) University of Waterloo, (3)\n  Durham University)', 'Line Emission in the Brightest Cluster Galaxies of the NOAO Fundamental\n  Plane and Sloan Digital Sky Surveys', 'Accepted for publication in MNRAS. 13 pages mn2e style with 7 figures\n  and 2 tables', 'Mon.Not.Roy.Astron.Soc.379:100-110,2007', '10.1111/j.1365-2966.2007.11910.x', '', 'astro-ph', '', '  We examine the optical emission line properties of Brightest Cluster Galaxies\n(BCGs) selected from two large, homogeneous datasets. The first is the X-ray\nselected National Optical Astronomy Observatory Fundamental Plane Survey\n(NFPS), and the second is the C4 catalogue of optically selected clusters built\nfrom the Sloan Digital Sky Survey Data Release ~3 (SDSS DR3). Our goal is to\nbetter understand the optical line emission in BCGs with respect to properties\nof the galaxy and the host cluster. Throughout the analysis we compare the line\nemission of the BCGs to that of a control sample made of the other bright\ngalaxies near the cluster centre. Overall, both the NFPS and SDSS show a modest\nfraction of BCGs with emission lines (~15%). No trend in the fraction of\nemitting BCGs as a function of galaxy mass or cluster velocity dispersion is\nfound. However we find that, for those BCGs found in cooling flow clusters,\n71^{+9}_{-14}% have optical emission. Furthermore, if we consider only BCGs\nwithin 50kpc of the X-ray centre of a cooling flow cluster, the emission-line\nfraction rises further to 100^{+0}_{-15}%. Excluding the cooling flow clusters,\nonly ~10% of BCGs are line emitting, comparable to the control sample of\ngalaxies. We show that the physical origin of the emission line activity\nvaries: in some cases it has LINER-like line ratios, whereas in others it is a\ncomposite of star-formation and LINER-like activity. We conclude that the\npresence of emission lines in BCGs is directly related to the cooling of X-ray\ngas at the cluster centre.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:53:20 GMT\"}]', '2008-11-26', '[[\"Edwards\",\"L. O. V.\",\"\"],[\"Hudson\",\"Michael J.\",\"\"],[\"Balogh\",\"Michael L.\",\"\"],[\"Smith\",\"Russell J.\",\"\"]]'),
(704.3243, 'Konstantinos Andriopoulos', 'K. Andriopoulos, P. G. L. Leach, A. Maharaj', 'On Differential Sequences', '29 pages, 2 tables', '', '', '', 'math-ph math.GR math.MP', '', '  We introduce the notion of Differential Sequences of ordinary differential\nequations. This is motivated by related studies based on evolution partial\ndifferential equations. We discuss the Riccati Sequence in terms of symmetry\nanalysis, singularity analysis and identification of the complete symmetry\ngroup for each member of the Sequence. The singularity analysis reveals\nconsiderable structure for the values of the coefficients of the leading-order\nterms and resonances of the different principal branches. Full proofs of the\nsymmetry properties are performed for differential equations defined by their\nrecursion properties and not given in explicit form.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:58:54 GMT\"}]', '2007-05-23', '[[\"Andriopoulos\",\"K.\",\"\"],[\"Leach\",\"P. G. L.\",\"\"],[\"Maharaj\",\"A.\",\"\"]]'),
(704.3244, 'Marcel Griesemer', 'M. Griesemer, D. Hasler', 'On the Smooth Feshbach-Schur Map', '8 pages', '', '', '', 'math-ph math.FA math.MP', '', '  A new variant of the Feshbach map, called smooth Feshbach map, has been\nintroduced recently by Bach et al., in connection with the renormalization\nanalysis of non-relativistic quantum electrodynamics. We analyze and clarify\nits algebraic and analytic properties, and we generalize it to non-selfadjoint\npartition operators $\\chi$ and $\\chib$.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 16:59:04 GMT\"}]', '2007-05-23', '[[\"Griesemer\",\"M.\",\"\"],[\"Hasler\",\"D.\",\"\"]]'),
(704.3245, 'Marcelo Alloy', 'M. D. Alloy and D. P. Menezes', 'Electrically charged pulsars', '', 'Braz.J.Phys.37:1183-1190,2007', '10.1590/S0103-97332007000800001', '', 'astro-ph', '', '  n the present work we investigate one possible variation on the usual\nelectrically neutral pulsars: the inclusion of electric charge. We study the\neffect of electric charge in pulsars assuming that the charge distribution is\nproportional to the energy density. All calculations were performed for zero\ntemperature and fixed entropy equations of state.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:00:09 GMT\"}]', '2011-08-04', '[[\"Alloy\",\"M. D.\",\"\"],[\"Menezes\",\"D. P.\",\"\"]]'),
(704.3246, 'Victor P. Ruban', 'V. P. Ruban', 'Nonlinear stage of the Benjamin-Feir instability: Three-dimensional\n  coherent structures and rogue waves', '11 pages, 7 figures, submitted to PRL', 'Phys. Rev. Lett. 99, 044502 (2007).', '10.1103/PhysRevLett.99.044502', '', 'physics.flu-dyn physics.ao-ph', '', '  A specific, genuinely three-dimensional mechanism of rogue wave formation, in\na late stage of the modulational instability of a perturbed Stokes deep-water\nwave, is recognized through numerical experiments. The simulations are based on\nfully nonlinear equations describing weakly three-dimensional potential flows\nof an ideal fluid with a free surface in terms of conformal variables.\nSpontaneous formation of zigzag patterns for wave amplitude is observed in a\nnonlinear stage of the instability. If initial wave steepness is sufficiently\nhigh ($ka>0.06$), these coherent structures produce rogue waves. The most tall\nwaves appear in ``turns\'\' of the zigzags. For $ka<0.06$, the structures decay\ntypically without formation of steep waves.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:04:14 GMT\"}]', '2007-08-01', '[[\"Ruban\",\"V. P.\",\"\"]]'),
(704.3247, 'Caina Hao', 'C.N. Hao, X.Y. Xia, S. Mao, Z.G. Deng, Hong Wu', 'The Growth of Black Holes and Their Host Spheroids in (Sub)mm-loud QSOs\n  at High Redshift', '19 pages,3 figures,submitted to Chin. J. Astron. Astrophys. This\n  paper was first prepared for publication on August 10th, 2005', 'Chin.J.Astron.Astrophys.8:12-24,2008', '10.1088/1009-9271/8/1/02', '', 'astro-ph', '', '  We study the growth of black holes and stellar population in spheroids at\nhigh redshift using several (sub)mm-loud QSO samples. Applying the same\ncriteria established in an earlier work, we find that, similar to IR QSOs at\nlow redshift, the far-infrared emission of these (sub)mm-loud QSOs mainly\noriginates from dust heated by starbursts. By combining low-z IR QSOs and\nhigh-z (sub)mm-loud QSOs, we find a trend that the star formation rate\n($\\Mstardot$) increases with the accretion rate ($\\Mdot$). We compare the\nvalues of $\\Mstardot/\\Mdot$ for submm emitting galaxies (SMGs), far-infrared\nultraluminous/hyperluminous QSOs and typical QSOs, and construct a likely\nevolution scenario for these objects. The (sub)mm-loud QSO transition phase has\nboth high $\\Mdot$ and $\\Mstardot$ and hence is important for establishing the\ncorrelation between the masses of black holes and spheroids.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:06:51 GMT\"}]', '2009-11-16', '[[\"Hao\",\"C. N.\",\"\"],[\"Xia\",\"X. Y.\",\"\"],[\"Mao\",\"S.\",\"\"],[\"Deng\",\"Z. G.\",\"\"],[\"Wu\",\"Hong\",\"\"]]'),
(704.3248, 'Brendan Guilfoyle', 'Brendan Guilfoyle and Wilhelm Klingenberg', 'On C$^2$-smooth Surfaces of Constant Width', '14 pages AMS-LATEX, 5 figures', 'Tbilisi Math. J. 2 (2009) 1-17', '10.32513/tbilisi/1528768838', '', 'math.DG', '', '  A number of results for C$^2$-smooth surfaces of constant width in Euclidean\n3-space ${\\mathbb{E}}^3$ are obtained. In particular, an integral inequality\nfor constant width surfaces is established. This is used to prove that the\nratio of volume to cubed width of a constant width surface is reduced by\nshrinking it along its normal lines. We also give a characterization of\nsurfaces of constant width that have rational support function.\n  Our techniques, which are complex differential geometric in nature, allow us\nto construct explicit smooth surfaces of constant width in ${\\mathbb{E}}^3$,\nand their focal sets. They also allow for easy construction of tetrahedrally\nsymmetric surfaces of constant width.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:13:16 GMT\"}]', '2021-11-15', '[[\"Guilfoyle\",\"Brendan\",\"\"],[\"Klingenberg\",\"Wilhelm\",\"\"]]'),
(704.3249, 'Andrea Mantile', 'Ph. Blanchard, R. Figari, A. Mantile', 'Point Interaction Hamiltonians in Bounded Domains', '18 pages, 3 figures, latex', '', '10.1063/1.2770672', '', 'math-ph math.MP math.SP', '', '  Making use of recent techniques in the theory of selfadjoint extensions of\nsymmetric operators, we characterize the class of point interaction\nHamiltonians in a 3-D bounded domain with regular boundary. In the particular\ncase of one point interaction acting in the center of a ball, we obtain an\nexplicit representation of the point spectrum of the operator togheter with the\ncorresponding related eigenfunctions. These operators are used to build up a\nmodel-system where the dynamics of a quantum particle depends on the state of a\nquantum bit.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:16:51 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 27 Apr 2007 16:09:37 GMT\"}]', '2009-11-13', '[[\"Blanchard\",\"Ph.\",\"\"],[\"Figari\",\"R.\",\"\"],[\"Mantile\",\"A.\",\"\"]]'),
(704.3250, 'Rui Dilao', 'Rui Dilao and Rui Alves-Pires', 'Chaos in the Stormer problem', '19 pages, 5 figures', '', '', '', 'nlin.CD nlin.SI', '', '  We survey the few exact results on the Stormer problem describing the\ndynamics of charged particles in the Earth magnetosphere. The analysis of this\nsystem leads to the the conclusion that charged particles are trapped in the\nEarth magnetosphere or escape to infinity, and the trapping region is bounded\nby a torus-like surface, the Van Allen inner radiation belt. In the trapping\nregion, the motion of the charged particles can be periodic, quasi-period or\nchaotic. The three main effects observed in the Earth magnetosphere, radiation\nbelts, radiation aurorae and South Atlantic anomaly, are described in the\nframework described here. We discuss some new mathematical problems suggested\nby the analysis of the Stormer problem.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:34:43 GMT\"}]', '2007-05-23', '[[\"Dilao\",\"Rui\",\"\"],[\"Alves-Pires\",\"Rui\",\"\"]]'),
(704.3251, 'Marcos Alexandrino', 'Marcos M. Alexandrino, Dirk Toeben', 'Equifocality of a singular riemannian foliation', '10 pages. This version contains some misprints corrections and\n  improvements of Corollary 1.6', 'Proceedings of the American Mathematical Society Proc. Amer. Math.\n  Soc. (136) (2008), 3271-3280', '', '', 'math.DG', '', '  A singular foliation on a complete riemannian manifold M is said to be\nriemannian if each geodesic that is perpendicular at one point to a leaf\nremains perpendicular to every leaf it meets. We prove that the regular leaves\nare equifocal, i.e., the end point map of a normal foliated vector field has\nconstant rank. This implies that we can reconstruct the singular foliation by\ntaking all parallel submanifolds of a regular leaf with trivial holonomy. In\naddition, the end point map of a normal foliated vector field on a leaf with\ntrivial holonomy is a covering map. These results generalize previous results\nof the authors on singular riemannian foliations with sections.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:38:58 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 24 May 2007 23:13:08 GMT\"}]', '2011-02-01', '[[\"Alexandrino\",\"Marcos M.\",\"\"],[\"Toeben\",\"Dirk\",\"\"]]'),
(704.3252, 'Zinovy Malkin', 'Zinovy Malkin, Natalia Miller', 'An analysis of celestial pole offset observations in the free core\n  nutation frequency band', '7 pages, 4 figures; Presented at the EGU 4th General Assembly,\n  Vienna, Austria, 15-20 April 2007', 'In: J. Boehm, A. Pany, H. Schuh (Eds.), Proc. 18th European VLBI\n  for Geodesy and Astrometry Working Meeting, Vienna, Austria, 12-13 Apr 2007,\n  Technische Universitaet Wien, 2007, 93-97', '', '', 'physics.geo-ph astro-ph.EP', '', '  In this study, three empirical Free Core Nutation (FCN) models developed to\nthe present time, MHB2000, Malkin\'s and Lambert\'s ones, are compared on the\nbasis of representation of variations of the FCN amplitude and phase predicted\nby these models. It is possible to conclude, that the model of the author\nprovides the most realistic representation of the FCN variations. However, the\nspecified models are based on representation about single FCN rotational mode.\nAt the same time, some results of processing of the VLBI observations made\nduring last years, specify possible presence of two close FCN periods. A\ntheoretical explanation to presence of a second FCN frequency FCN has been\ngiven by G. Krasinsky in his theory of rotation of the Earth with two-layer\nliquid core, ERA2005. In the present work, for more detailed studying this\nphenomenon, the IVS time series of celestial pole offset, and also those\npredicted by the ERA2005 theory, have been investigated by means of several\nstatistical methods which confidently show presence of two fluctuations in\nnutational movement of an Earth\'s rotation axis with the periods about -452 and\n-410 solar days.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:51:47 GMT\"}]', '2009-08-14', '[[\"Malkin\",\"Zinovy\",\"\"],[\"Miller\",\"Natalia\",\"\"]]'),
(704.3253, 'Yi Zhao', 'Yi Zhao, Chi-Hang Fred Fung, Bing Qi, Christine Chen, and Hoi-Kwong Lo', 'Quantum Hacking: Experimental demonstration of time-shift attack against\n  practical quantum key distribution systems', '5 pages, 3 figures. Substantially revised version', 'Physical Review A, 78, 042333 (2008)', '10.1103/PhysRevA.78.042333', '', 'quant-ph', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Quantum key distribution (QKD) systems can send signals over more than 100 km\nstandard optical fiber and are widely believed to be secure. Here, we show\nexperimentally for the first time a technologically feasible attack, namely the\ntime-shift attack, against a commercial QKD system. Our result shows that,\ncontrary to popular belief, an eavesdropper, Eve, has a non-negligible\nprobability (~4%) to break the security of the system. Eve\'s success is due to\nthe well-known detection efficiency loophole in the experimental testing of\nBell inequalities. Therefore, the detection efficiency loophole plays a key\nrole not only in fundamental physics, but also in technological applications\nsuch as QKD.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:06:00 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 17 Mar 2008 21:57:23 GMT\"},{\"version\":\"v3\",\"created\":\"Fri, 1 Apr 2011 21:01:36 GMT\"}]', '2011-04-05', '[[\"Zhao\",\"Yi\",\"\"],[\"Fung\",\"Chi-Hang Fred\",\"\"],[\"Qi\",\"Bing\",\"\"],[\"Chen\",\"Christine\",\"\"],[\"Lo\",\"Hoi-Kwong\",\"\"]]'),
(704.3254, 'Leonid Bedratyuk P.', 'Leonid Bedratyuk', 'Symmetrical invariants of some modular Lie algebras of Cartan type', '7 pages in Ukrainian', 'Mat. Stud. 30, No. 1, 3-8 (2008).', '', '', 'math.RA math.RT', '', '  Let $L$ be one of the finite dimensional Lie algebras $W_n({\\bf m}),$\n$S_n({\\bf m}),$ $ H_n({\\bf m})$ of Cartan type over an algebraically closed\nfield of prime characteristic $p>0.$ For an elements $F$ of the symmetrical\nalgebra $S(L)$ we found necessary and sufficient condition in order to the\nelement $ad(\\partial_1)^{p^{m_1}-1} ad(\\partial_2)^{p^{m_2}-1}...\nad(\\partial_n)^{p^{m_n}-1}(F)$ belongs to the symmetrical invariants algebra\n$S(L)^L.$ Also, for $p=3,5$ the algebra of symmetrical invariants\n$S(H_2)^{H_2}$ is calculated in explicit way.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:48:54 GMT\"}]', '2009-04-08', '[[\"Bedratyuk\",\"Leonid\",\"\"]]'),
(704.3255, 'Frans Klinkhamer', 'C. Kaufhold, F. R. Klinkhamer', 'Vacuum Cherenkov radiation in spacelike Maxwell-Chern-Simons theory', '24 pages with revtex4, v5: published version', 'Phys.Rev.D76:025024,2007', '10.1103/PhysRevD.76.025024', 'KA-TP-10-2007', 'hep-th astro-ph hep-ph', '', '  A detailed analysis of vacuum Cherenkov radiation in spacelike\nMaxwell-Chern-Simons (MCS) theory is presented. A semiclassical treatment\nreproduces the leading terms of the tree-level result from quantum field\ntheory. Moreover, certain quantum corrections turn out to be suppressed for\nlarge energies of the charged particle, for example, the quantum corrections to\nthe classical MCS Cherenkov angle. It is argued that MCS-theory Cherenkov\nradiation may, in principle, lead to anisotropy effects for ultra-high-energy\ncosmic rays (UHECRs). In addition, a qualitative discussion of vacuum Cherenkov\nradiation from a modified-Maxwell term in the action is given, together with\nUHECR bounds on some of its dimensionless \"coupling constants.\"\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:50:28 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 2 May 2007 17:30:12 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 28 May 2007 17:23:30 GMT\"},{\"version\":\"v4\",\"created\":\"Thu, 7 Jun 2007 18:09:42 GMT\"},{\"version\":\"v5\",\"created\":\"Mon, 23 Jul 2007 18:20:17 GMT\"}]', '2008-11-26', '[[\"Kaufhold\",\"C.\",\"\"],[\"Klinkhamer\",\"F. R.\",\"\"]]'),
(704.3256, 'Radu Laza', 'Radu Laza', 'The moduli space of cubic fourfolds', '28 pages, part I (the GIT compactification), the journal version', 'J. Algebraic Geom. 18 (2009), 511-545', '', '', 'math.AG', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We describe the GIT compactification of the moduli space of cubic fourfolds,\nwith a special emphasis on the role played by singularities. Our main result is\nthat a cubic fourfold with only isolated simple (A-D-E) singularities is GIT\nstable. Conversely, with some minor exceptions, the stability for cubic\nfourfolds is characterized by this condition.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 17:54:25 GMT\"},{\"version\":\"v2\",\"created\":\"Thu, 4 Sep 2008 16:56:52 GMT\"}]', '2011-09-28', '[[\"Laza\",\"Radu\",\"\"]]'),
(704.3257, 'Caroline Bot', 'C. Bot, F. Boulanger, M. Rubio and F. Rantakyro', 'Millimeter dust continuum emission unveiling the true mass of giant\n  molecular clouds in the Small Magellanic Cloud', '10 pages, 2 figures, Astronomy & Astrophysics accepted', '', '', '', 'astro-ph', '', '  CO observations have been so far the best way to trace molecular gas in\nexternal galaxies, but at low metallicity the gas mass deduced could be largely\nunderestimated. At present, the kinematic information of CO data cubes are used\nto estimate virial masses and trace the total mass of the molecular clouds.\nMillimeter dust emission can also be used as a dense gas tracer and could\nunveil H2 envelopes lacking CO. These different tracers must be compared in\ndifferent environments. This study compares virial masses to masses deduced\nfrom millimeter emission, in two GMC samples: the local molecular clouds in our\nGalaxy and their equivalents in the Small Magellanic Cloud (SMC), one of the\nnearest low metallicity dwarf galaxy. In our Galaxy, mass estimates deduced\nfrom millimeter emission are consistent with masses deduced from gamma ray\nanalysis and trace the total mass of the clouds. Virial masses are\nsystematically larger (twice on average) than mass estimates from millimeter\ndust emission. This difference decreases toward high masses and has already\nbeen reported in previous studies. In the SMC however, molecular cloud masses\ndeduced from SIMBA millimeter observations are systematically higher (twice on\naverage for conservative values of the dust to gas ratio and dust emissivity)\nthan the virial masses from SEST CO observations. The observed excess can not\nbe accounted for by any plausible change of dust properties. Taking a general\nform for the virial theorem, we show that a magnetic field strength of ~15\nmicro Gauss in SMC clouds could provide additional support to the clouds and\nexplain the difference observed. Masses of SMC molecular clouds have therefore\nbeen underestimated so far. Magnetic pressure may contribute significantly to\ntheir support.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:29:21 GMT\"}]', '2019-08-19', '[[\"Bot\",\"C.\",\"\"],[\"Boulanger\",\"F.\",\"\"],[\"Rubio\",\"M.\",\"\"],[\"Rantakyro\",\"F.\",\"\"]]'),
(704.3258, 'Rabindra N. Mohapatra', 'R. N. Mohapatra, N. Okada and Hai-Bo Yu', 'Natural Realizations of Seesaw in Mini-Warped Minimal SO(10)', '20 pages and one figure', 'Phys.Rev.D76:015013,2007', '10.1103/PhysRevD.76.015013', 'UMD-PP-07-003', 'hep-ph', '', '  The minimal SUSY SO(10) GUT models with {\\bf 10}, {\\bf 126} and {\\bf 210}\nHiggs and only renormalizable couplings has been shown to provide a simple way\nto understand the neutrino mixings as well as the ratio $\\Delta\nm^2_\\odot/\\Delta m^2_A$ in terms of quark mixing parameter $\\theta_{Cabibbo}$,\nprovided neutrino masses are described by type II seesaw formula. However, in\nthis minimal picture, it is impossible to realize type II dominance with\nrenormalizable couplings in 4-dimensions. We show that this problem can be\ncured by embedding this model into a warped 5-dimensional space time with\nwarping between the Planck and the GUT scale, where both type II as well as\nmixed seesaw formulae can be realized in a natural manner without expanding the\nHiggs sector. These models also avoid the possible problem of threshold effects\nassociated with large Higgs representations since the theory above the GUT\nscale is now strongly coupled.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:37:19 GMT\"}]', '2008-11-26', '[[\"Mohapatra\",\"R. N.\",\"\"],[\"Okada\",\"N.\",\"\"],[\"Yu\",\"Hai-Bo\",\"\"]]'),
(704.3259, 'James P. Sethna', 'Christopher R. Myers, Ryan N. Gutenkunst, and James. P. Sethna', 'Python Unleashed on Systems Biology', 'Submitted to special issue of CiSE', '', '', '', 'q-bio.QM q-bio.MN', '', '  We have built an open-source software system for the modeling of biomolecular\nreaction networks, SloppyCell, which is written in Python and makes substantial\nuse of third-party libraries for numerics, visualization, and parallel\nprogramming. We highlight here some of the powerful features that Python\nprovides that enable SloppyCell to do dynamic code synthesis, symbolic\nmanipulation, and parallel exploration of complex parameter spaces.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:48:18 GMT\"}]', '2007-05-23', '[[\"Myers\",\"Christopher R.\",\"\"],[\"Gutenkunst\",\"Ryan N.\",\"\"],[\"Sethna\",\"James. P.\",\"\"]]'),
(704.3260, 'Marco Frasca', 'Marco Frasca', 'Spectrum of Yang-Mills Theory in D=3+1', '6 pages, no figure. Updated references', '', '', '', 'hep-th hep-lat hep-ph math-ph math.MP', '', '  We give a comparison of the spectrum of Yang-Mills theory in $D=3+1$,\nrecently derived with a strong coupling expansion, with lattice data. We verify\nexcellent agreement also for 2$^{++}$ glueball. A deep analogy with the $D=2+1$\ncase is obtained and a full quantum theory of this approach is also given.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:57:19 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 18 May 2007 21:20:07 GMT\"},{\"version\":\"v3\",\"created\":\"Thu, 28 Jun 2007 06:13:01 GMT\"}]', '2007-06-28', '[[\"Frasca\",\"Marco\",\"\"]]'),
(704.3261, 'Gerard Le Caer', 'G. Le Caer, C. Male and R. Delannay', 'Nearest-neigbor spacing distributions of the beta-Hermite ensemble of\n  random matrices', 'Physica A (in press, 2007), 32 pages, 13 figures, corresponding\n  author:G. Le Caer', '', '10.1016/j.physa.2007.04.057', '', 'cond-mat.stat-mech cond-mat.dis-nn', '', '  The distributions of the spacing s between nearest-neighbor levels of\nunfolded spectra of random matrices from the beta-Hermite ensemble (beta-HE) is\ninvestigated by Monte Carlo simulations. The random matrices from the beta-HE\nare real-symmetric and tridiagonal where beta, which can take any positive\nvalue, is the reciprocal of the temperature in the classical electrostatic\ninterpretation of eigenvalues. Generalized gamma distributions are shown to be\nexcellent approximations of the nearest-neighbor spacing (NNS) distributions\nfor any beta while being still simple. They account both for the level\nrepulsion when s tends to zero and for the whole shape of the NNS distributions\nin the range of s which is accessible to experiment or to most numerical\nsimulations. The exact NNS distribution of the GOE (beta=1) is in particular\nsignificantly better described by a generalized gamma distribution than it is\nby the Wigner surmise while the best generalized gamma approximation coincides\nessentially with the Wigner surmise for beta larger than ~2. The distributions\nof the minimum NN spacing between eigenvalues of matrices from the beta-HE,\nobtained both from as-calculated eigenvalues and from unfolded eigenvalues are\nBrody distributions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 18:56:56 GMT\"}]', '2009-11-13', '[[\"Caer\",\"G. Le\",\"\"],[\"Male\",\"C.\",\"\"],[\"Delannay\",\"R.\",\"\"]]'),
(704.3262, 'Rainer Schmidt', 'Rainer Schmidt, Wilma Eerenstein, Thomas Winiecki, Finlay D. Morrison,\n  Paul A. Midgley', 'Impedance spectroscopy of epitaxial multiferroic thin films', '', 'Physical Review B 75, 245111 (2007)', '10.1103/PhysRevB.75.245111', '', 'cond-mat.str-el cond-mat.mtrl-sci', '', '  Temperature dependent impedance spectroscopy enables the many contributions\nto the dielectric and resistive properties of condensed matter to be\ndeconvoluted and characterized separately. We have achieved this for\nmultiferroic epitaxial thin films of BiFeO3 (BFO) and BiMnO3 (BMO), key\nexamples of materials with strong magneto-electric coupling. We demonstrate\nthat the true film capacitance of the epitaxial layers is similar to that of\nthe electrode interface, making analysis of capacitance as a function of film\nthickness necessary to achieve deconvolution. We modeled non-Debye impedance\nresponse using Gaussian distributions of relaxation times and reveal that\nconventional resistivity measurements on multiferroic layers may be dominated\nby interface effects. Thermally activated charge transport models yielded\nactivation energies of 0.60 eV +- 0.05 eV (BFO) and 0.25 eV +- 0.03 eV (BMO),\nwhich is consistent with conduction dominated by oxygen vacancies (BFO) and\nelectron hopping (BMO). The intrinsic film dielectric constants were determined\nto be 320 +- 75 (BFO) and 450 +- 100 (BMO).\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 19:13:19 GMT\"}]', '2007-06-20', '[[\"Schmidt\",\"Rainer\",\"\"],[\"Eerenstein\",\"Wilma\",\"\"],[\"Winiecki\",\"Thomas\",\"\"],[\"Morrison\",\"Finlay D.\",\"\"],[\"Midgley\",\"Paul A.\",\"\"]]'),
(704.3263, 'Dominique Jean-Marie Mornet', 'Karim Hnia, G\\\'erald Hugon, Ahmed Masmoudi, Jacques Mercier,\n  Fran\\c{c}ois Rivier, Dominique Jean-Marie Mornet', 'Effect of beta-Dystroglycan Processing on Utrophin / DP116 Anchorage in\n  Normal and MDX Mouse Schwann Cell Membrane', '', 'Neuroscience 141 (18/04/2006) 607-620', '10.1016/J.neuroscience.2006.04.043', '', 'q-bio.NC', '', '  In the peripheral nervous system, utrophin and the short dystrophin isoform\n(Dp116) are co-localized at the outermost layer of the myelin sheath of nerve\nfibers; together with the dystroglycan complex. In peripheral nerve, matrix\nmetalloproteinase (MMP) creates a 30 kDa fragment of beta-dystroglycan, leading\nto a disruption of the link between the extracellular matrix and the cell\nmembrane. Here we asked if the processing of the beta-dystroglycan could\ninfluence the anchorage of Dp116 or/and utrophin in normal and mdx Schwann cell\nmembrane. We showed that MMP-9 was more activated in mdx nerve than in\nwild-type one. This activation leads to an accumulation of the 30 kDa\nbeta-dystroglycan isoform and have an impact on the anchorage of Dp116 and\nutrophin isoforms in mdx Schwann cells membrane. Our results showed that Dp116\nhad greater affinity to the full length form of beta-dystroglycan than the 30\nkDa form. Moreover, we showed for the first time that the short isoform of\nutrophin (Up71) was over-expressed in mdx Schwann cells compared to wild-type.\nIn addition, this utrophin isoform (Up71) seems to have greater affinity to the\n30 kDa beta-dystroglycan which could explain a more stabilization of this 30\nkDa at the membrane compartment. Our results highlight the potential\nparticipation of the short utrophin isoform and the cleaved form of\nbeta-dystroglycan in mdx Schwann cell membrane architecture.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 19:17:45 GMT\"}]', '2007-05-23', '[[\"Hnia\",\"Karim\",\"\"],[\"Hugon\",\"Gérald\",\"\"],[\"Masmoudi\",\"Ahmed\",\"\"],[\"Mercier\",\"Jacques\",\"\"],[\"Rivier\",\"François\",\"\"],[\"Mornet\",\"Dominique Jean-Marie\",\"\"]]'),
(704.3264, 'Jose Vilar', 'Leonor Saiz and Jose M. G. Vilar', 'Efficiency and versatility of distal multisite transcription regulation', '', '', '', '', 'q-bio.SC q-bio.MN', '', '  Transcription regulation typically involves the binding of proteins over long\ndistances on multiple DNA sites that are brought close to each other by the\nformation of DNA loops. The inherent complexity of the assembly of regulatory\ncomplexes on looped DNA challenges the understanding of even the simplest\ngenetic systems, including the prototypical lac operon. Here we implement a\nscalable quantitative computational approach to analyze systems regulated\nthrough multiple DNA sites with looping. Our approach applied to the lac operon\naccurately predicts the transcription rate over five orders of magnitude for\nwild type and seven mutants accounting for all the combinations of deletions of\nthe three operators. A quantitative analysis of the model reveals that the\npresence of three operators provides a mechanism to combine robust repression\nwith sensitive induction, two seemingly mutually exclusive properties that are\nrequired for optimal functioning of metabolic switches.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 19:46:28 GMT\"}]', '2007-05-23', '[[\"Saiz\",\"Leonor\",\"\"],[\"Vilar\",\"Jose M. G.\",\"\"]]'),
(704.3265, 'Michael Ibison', 'M. Ibison', 'Static forms of the Robertson-Walker spacetimes', '', '', '', '', 'gr-qc', '', '  It is shown that only the maximally-symmetric spacetimes can be expressed in\nboth the Robertson-Walker form and in static form - there are no other static\nforms of the Robertson-Walker spacetimes. All possible static forms of the\nmetric of the maximally-symmetric spacetimes are presented as a table. The\nfindings are generalized to apply to functionally more general spacetimes: it\nis shown that the maximally symmetric spacetimes are also the only spacetimes\nthat can be written in both orthogonal-time isotropic form and in static form.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 19:55:14 GMT\"}]', '2007-05-23', '[[\"Ibison\",\"M.\",\"\"]]'),
(704.3266, 'Alexander Scholz', 'Aleks Scholz (SUPA, University of St. Andrews), Jaime Coffey\n  (University of British Columbia), Alexis Brandeker (Stockholm Observatory),\n  Ray Jayawardhana (University of Toronto)', 'Rotation and activity of pre-main-sequence stars', '40 pages, 8 figures, ApJ, in press', '', '10.1086/518361', '', 'astro-ph', '', '  We present a study of rotation (vsini) and chromospheric activity (Halpha EW)\nbased on an extensive set of high-resolution optical spectra obtained with MIKE\non the 6.5m Magellan Clay telescope. Our targets are 74 F-M dwarfs in the young\nstellar associations Eta Cha, TW Hydrae, Beta Pic, and Tuc-Hor, spanning ages\nfrom 6 to 30 Myr. While the Halpha EW for most F and G stars are consistent\nwith pure photospheric absorption, most K and M stars show chromospheric\nemission. By comparing Halpha EW in our sample to results in the literature, we\nsee a clear evolutionary sequence: Chromospheric activity declines steadily\nfrom the T Tauri phase to the main sequence. Using activity as an age\nindicator, we find a plausible age range for the Tuc-Hor association of 10-40\nMyr. Between 5 and 30 Myr, we do not see evidence for rotational braking in the\ntotal sample, thus angular momentum is conserved, in contrast to younger stars.\nThis difference indicates a change in the rotational regulation at 5-10 Myr,\npossibly because disk braking cannot operate longer than typical disk\nlifetimes, allowing the objects to spin up. The rotation-activity relation is\nflat in our sample; in contrast to main-sequence stars, there is no linear\ncorrelation for slow rotators. We argue that this is because young stars\ngenerate their magnetic fields in a fundamentally different way from\nmain-sequence stars, and not just the result of a saturated solar-type dynamo.\nBy comparing our rotational velocities with published rotation periods for a\nsubset of stars, we determine ages of 13 (7-20) Myr and 9 (7-17} Myr for the\nEta Cha and TWA associations, respectively, consistent with previous estimates.\nThus we conclude that stellar radii from evolutionary models by Baraffe et al.\n(1998) are in agreement with the observed radii within +-15%. (abridged)\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:09:31 GMT\"}]', '2009-11-13', '[[\"Scholz\",\"Aleks\",\"\",\"SUPA, University of St. Andrews\"],[\"Coffey\",\"Jaime\",\"\",\"University of British Columbia\"],[\"Brandeker\",\"Alexis\",\"\",\"Stockholm Observatory\"],[\"Jayawardhana\",\"Ray\",\"\",\"University of Toronto\"]]'),
(704.3267, 'Justin Read', 'J. I. Read, P. Saha, and A. V. Maccio', 'Radial density profiles of time-delay lensing galaxies', 'Replaced with final version accepted for publication in ApJ; very\n  minor changes to text; high resolution figures may be obtained at\n  justinread.net', '', '10.1086/520714', '', 'astro-ph', '', '  We present non-parametric radial mass profiles for ten QSO strong lensing\ngalaxies. Five of the galaxies have profiles close to $\\rho(r)\\propto r^{-2}$,\nwhile the rest are closer to r^{-1}, consistent with an NFW profile. The former\nare all relatively isolated early-types and dominated by their stellar light.\nThe latter --though the modeling code did not know this-- are either in\nclusters, or have very high mass-to-light, suggesting dark-matter dominant\nlenses (one is a actually pair of merging galaxies). The same models give\n$H_0^{-1} = 15.2_{-1.7}^{+2.5}\\Gyr$ ($H_0 = 64_{-9}^{+8} \\legacy$), consistent\nwith a previous determination. When tested on simulated lenses taken from a\ncosmological hydrodynamical simulation, our modeling pipeline recovers both H_0\nand $\\rho(r)$ within estimated uncertainties. Our result is contrary to some\nrecent claims that lensing time delays imply either a low H_0 or galaxy\nprofiles much steeper than r^{-2}. We diagnose these claims as resulting from\nan invalid modeling approximation: that small deviations from a power-law\nprofile have a small effect on lensing time-delays. In fact, as we show using\nusing both perturbation theory and numerical computation from a\ngalaxy-formation simulation, a first-order perturbation of an isothermal lens\ncan produce a zeroth-order change in the time delays.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:12:37 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 31 Jul 2007 13:44:06 GMT\"}]', '2009-11-13', '[[\"Read\",\"J. I.\",\"\"],[\"Saha\",\"P.\",\"\"],[\"Maccio\",\"A. V.\",\"\"]]'),
(704.3268, 'Koray Karahaliloglu', 'Koray Karahaliloglu', '2D Path Solutions from a Single Layer Excitable CNN Model', '24 pages, 9 figures', '', '', '', 'cs.RO cs.NE', '', '  An easily implementable path solution algorithm for 2D spatial problems,\nbased on excitable/programmable characteristics of a specific cellular\nnonlinear network (CNN) model is presented and numerically investigated. The\nnetwork is a single layer bioinspired model which was also implemented in CMOS\ntechnology. It exhibits excitable characteristics with regionally bistable\ncells. The related response realizes propagations of trigger autowaves, where\nthe excitable mode can be globally preset and reset. It is shown that, obstacle\ndistributions in 2D space can also be directly mapped onto the coupled cell\narray in the network. Combining these two features, the network model can serve\nas the main block in a 2D path computing processor. The related algorithm and\nconfigurations are numerically experimented with circuit level parameters and\nperformance estimations are also presented. The simplicity of the model also\nallows alternative technology and device level implementation, which may become\ncritical in autonomous processor design of related micro or nanoscale robotic\napplications.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:20:46 GMT\"}]', '2007-05-23', '[[\"Karahaliloglu\",\"Koray\",\"\"]]'),
(704.3269, 'Ian Dobbs-Dixon', 'Ian Dobbs-Dixon and D.N.C. Lin', 'Atmospheric Dynamics of Short-period Extra Solar Gas Giant Planets I:\n  Dependence of Night-Side Temperature on Opacity', '35 Pages, 13 Figures', '', '10.1086/523786', '', 'astro-ph', '', '  More than two dozen short-period Jupiter-mass gas giant planets have been\ndiscovered around nearby solar-type stars in recent years, several of which\nundergo transits, making them ideal for the detection and characterization of\ntheir atmospheres. Here we adopt a three-dimensional radiative hydrodynamical\nnumerical scheme to simulate atmospheric circulation on close-in gas giant\nplanets. In contrast to the conventional GCM and shallow water algorithms, this\nmethod does not assume quasi hydrostatic equilibrium and it approximates\nradiation transfer from optically thin to thick regions with flux-limited\ndiffusion. In the first paper of this series, we consider\nsynchronously-spinning gas giants. We show that a full three-dimensional\ntreatment, coupled with rotationally modified flows and an accurate treatment\nof radiation, yields a clear temperature transition at the terminator. Based on\na series of numerical simulations with varying opacities, we show that the\nnight-side temperature is a strong indicator of the opacity of the planetary\natmosphere. Planetary atmospheres that maintain large, interstellar opacities\nwill exhibit large day-night temperature differences, while planets with\nreduced atmospheric opacities due to extensive grain growth and sedimentation\nwill exhibit much more uniform temperatures throughout their photosphere\'s. In\naddition to numerical results, we present a four-zone analytic approximation to\nexplain this dependence.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:23:57 GMT\"}]', '2009-11-13', '[[\"Dobbs-Dixon\",\"Ian\",\"\"],[\"Lin\",\"D. N. C.\",\"\"]]'),
(704.3270, 'James Stewart', 'The HERMES Collaboration: A. Airapetian, et al', 'Hadronization in semi-inclusive deep-inelastic scattering on nuclei', '33 pages, 12 figures', 'Nucl.Phys.B780:1-27,2007', '10.1016/j.nuclphysb.2007.06.004', 'DESY 07-050', 'hep-ex', '', '  A series of semi-inclusive deep-inelastic scattering measurements on\ndeuterium, helium, neon, krypton, and xenon targets has been performed in order\nto study hadronization. The data were collected with the HERMES detector at the\nDESY laboratory using a 27.6 GeV positron or electron beam. Hadron\nmultiplicities on nucleus A relative to those on the deuteron, R_A^h, are\npresented for various hadrons (\\pi^+, \\pi^-, \\pi^0, K^+, K^-, p, and \\bar{p})\nas a function of the virtual-photon energy \\nu, the fraction z of this energy\ntransferred to the hadron, the photon virtuality Q^2, and the hadron transverse\nmomentum squared p_t^2. The data reveal a systematic decrease of R_A^h with the\nmass number A for each hadron type h. Furthermore, R_A^h increases (decreases)\nwith increasing values of \\nu (z), increases slightly with increasing Q^2, and\nis almost independent of p_t^2, except at large values of p_t^2. For pions\ntwo-dimensional distributions also are presented. These indicate that the\ndependences of R_A^{\\pi} on \\nu and z can largely be described as a dependence\non a single variable L_c, which is a combination of \\nu and z. The dependence\non L_c suggests in which kinematic conditions partonic and hadronic mechanisms\nmay be dominant. The behaviour of R_A^{\\pi} at large p_t^2 constitutes\ntentative evidence for a partonic energy-loss mechanism. The A-dependence of\nR_A^h is investigated as a function of \\nu, z, and of L_c. It approximately\nfollows an A^{\\alpha} form with \\alpha \\approx 0.5 - 0.6.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:29:31 GMT\"}]', '2012-08-03', '[[\"The HERMES Collaboration\",\"\",\"\"],[\"Airapetian\",\"A.\",\"\"]]');
INSERT INTO `xie_import_6000` (`id`, `submitter`, `authors`, `title`, `comments`, `journal-ref`, `doi`, `report-no`, `categories`, `license`, `abstract`, `versions`, `update_date`, `authors_parsed`) VALUES
(704.3271, 'Kathryn Zurek', 'Alexander Friedland, Kathryn M. Zurek, Sergei Bashinsky', 'Constraining Models of Neutrino Mass and Neutrino Interactions with the\n  Planck Satellite', '25 pages, 16 figures, revtex', '', '', '', 'astro-ph hep-ph', '', '  In several classes of particle physics models -- ranging from the classical\nMajoron models, to the more recent scenarios of late neutrino masses or\nMass-Varying Neutrinos -- one or more of the neutrinos are postulated to couple\nto a new light scalar field. As a result of this coupling, neutrinos in the\nearly universe instead of streaming freely could form a self-coupled fluid,\nwith potentially observable signatures in the Cosmic Microwave Background and\nthe large scale structure of the universe. We re-examine the constraints on\nthis scenario from the presently available cosmological data and investigate\nthe sensitivity expected from the Planck satellite. In the first case, we find\nthat the sensitivity strongly depends on which piece of data is used. The SDSS\nMain sample data, combined with WMAP and other data, disfavors the scenario of\nthree coupled neutrinos at about the 3.5$\\sigma$ confidence level, but also\nfavors a high number of freely streaming neutrinos, with the best fit at 5.2.\nIf the matter power spectrum is instead taken from the SDSS Large Red Galaxy\nsample, best fit point has 2.5 freely streaming neutrinos, but the scenario\nwith three coupled neutrinos becomes allowed at $2\\sigma$. In contrast, Planck\nalone will exclude even a single self-coupled neutrino at the $4.2\\sigma$\nconfidence level, and will determine the total radiation at CMB epoch to\n$\\Delta N_\\nu^{eff} = ^{+0.5}_{-0.3}$ ($1\\sigma$ errors). We investigate the\nrobustness of this result with respect to the details of Planck\'s detector.\nThis sensitivity to neutrino free-streaming implies that Planck will be capable\nof probing a large region of the Mass-Varying Neutrino parameter space. Planck\nmay also be sensitive to a scale of neutrino mass generation as high as 1 TeV.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 18:58:06 GMT\"}]', '2007-05-23', '[[\"Friedland\",\"Alexander\",\"\"],[\"Zurek\",\"Kathryn M.\",\"\"],[\"Bashinsky\",\"Sergei\",\"\"]]'),
(704.3272, 'Fernando Marchesano', 'Fernando Marchesano and Waldemar Schulgin', 'Non-geometric fluxes as supergravity backgrounds', '5 pages. Further typos corrected', 'Phys.Rev.D76:041901,2007', '10.1103/PhysRevD.76.041901', 'LMU-ASC 26/07, MPP-2007-49', 'hep-th', '', '  We consider examples of D=4 string theory vacua which, although globally\nnon-geometric, admit a local description in terms of D=10 supergravity\nbackgrounds. We analyze such backgrounds and find that the supersymmetry\nspinors vary non-trivially along the internal manifold, reproducing the\ninterpolating supergravity solutions found by Frey and Grana. Finally, we\npropose a simple, local expression for non-geometric fluxes in terms of the\ninternal spinors of the compactification.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 18:20:28 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 9 May 2007 16:43:15 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 19 Sep 2007 15:03:25 GMT\"}]', '2008-11-26', '[[\"Marchesano\",\"Fernando\",\"\"],[\"Schulgin\",\"Waldemar\",\"\"]]'),
(704.3273, 'Siu Chin', 'Siu A. Chin', 'Forward and non-forward symplectic integrators in solving classical\n  dynamics problems', '26 pages, 17 figures, to be published in a \"Special Issue on\n  Splitting Methods for Differential Equation\", Intl. J. of Comp. Math', '', '', '', 'physics.comp-ph physics.class-ph', '', '  Forward time step integrators are splitting algorithms with only positive\nsplitting coefficients. When used in solving physical evolution equations,\nthese positive coefficients correspond to positive time steps. Forward\nalgorithms are essential for solving time-irreversible equations that cannot be\nevolved using backward time steps. However, forward integrators are also better\nin solving time-reversible equations of classical dynamics by tracking as\nclosely as possible the physical trajectory. This work compares in detail\nvarious forward and non-forward fourth-order integrators using three, fourth,\nfive and six force evaluations. In the case of solving the 2D Kepler orbit, all\nnon-forward integrators are optimized by simply minimizing the size of their\nbackward time steps.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:42:25 GMT\"}]', '2007-05-23', '[[\"Chin\",\"Siu A.\",\"\"]]'),
(704.3274, 'Mladen Georgiev', 'Fabio DeMatteis and Mladen Georgiev', 'Nonradiative DKR processes: revisiting the theory. I. Unimode model', '17 pages including 1 table, 2 appendices and 1 figure, all pdf format', '', '', '', 'cond-mat.mtrl-sci', '', '  We are revisiting the efficiency problem of DKR nonradiative transitions at\nlocal electronic centers in polarizable solids. Following a brief survey, we\nformulate the general rate equations thereby defining the microscopic\nparameters controlling the nonradiative deexcitation. We also reproduce the\nquantum mechanical expressions for the energy conserving \"horizontal transfer\nrates\" to compare with the \"verical transition rates\" at various vibronic\nenergy levels.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 20:59:44 GMT\"}]', '2007-05-23', '[[\"DeMatteis\",\"Fabio\",\"\"],[\"Georgiev\",\"Mladen\",\"\"]]'),
(704.3275, 'Wei Zhang', 'Wei Zhang and C. A. R. Sa de Melo', 'Matter-wave interference in s-wave and p-wave Fermi condensates', '8 pages, 5 figures; Phys. Rev. A 76, 013627 (2007)', 'Phys. Rev. A 76, 013627 (2007)', '10.1103/PhysRevA.76.013627', '', 'cond-mat.str-el cond-mat.supr-con', '', '  We discuss the time evolution and matter-wave interference of Fermi\ncondensates on the BEC side of Feshbach resonances for s and p-wave\nsuperfluids, upon release from harmonic traps. In swave systems, where the\norder parameter is a complex scalar, we find that the interference patterns\ndepend on the relative phase of the order parameters of the condensates. In\np-wave systems involving the mixture of two-hyperfine states, we show that the\ninterference pattern exhibits a polarization effect depending on the relative\norientation of the two vector order parameters. Lastly, we also point out that\np-wave Fermi condensates exhibit an anisotropic expansion, reflecting the\nspatial anisotropy of the underlying interaction between fermions and the\norbital nature of the vector order parameter. Potential applications of our\nresults include systems of ultra-cold atoms that exhibit p-wave Feshbach\nresonances such as 6Li or 40K.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 21:20:57 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 21 May 2008 16:52:05 GMT\"}]', '2008-05-21', '[[\"Zhang\",\"Wei\",\"\"],[\"de Melo\",\"C. A. R. Sa\",\"\"]]'),
(704.3276, 'Frank Tipler', 'Frank J. Tipler', 'Feynman-Weinberg Quantum Gravity and the Extended Standard Model as a\n  Theory of Everything', '', 'Rept.Prog.PHys.68:897-964,2005', '10.1088/0034-4885/68/4/R04', '', 'hep-th', '', '  I argue that the (extended) Standard Model (SM) of particle physics and the\nrenormalizable Feynman-Weinberg theory of quantum gravity comprise a theory of\neverything. I show that imposing the appropriate cosmological boundary\nconditions make the theory finite. The infinities that are normally\nrenormalized away and the series divergence infinities are both eliminated by\nthe same mechanism. Furthermore, this theory can resolve the horizon, flatness,\nand isotropy problems of cosmology. Joint mathematical consistency naturally\nyields a scale-free, Gaussian, adiabatic perturbation spectrum, and more matter\nthan antimatter. I show that mathematical consistency of the theory requires\nthe universe to begin at an initial singularity with a pure $SU(2)_L$ gauge\nfield. I show that quantum mechanics requires this field to have a Planckian\nspectrum whatever its temperature. If this field has managed to survive\nthermalization to the present day, then it would be the CMBR. If so, then we\nwould have a natural explanation for the dark matter and the dark energy. I\nshow that isotropic ultrahigh energy (UHE) cosmic rays are explained if the\nCMBR is a pure $SU(2)_L$ gauge field. The $SU(2)_L$ nature of the CMBR may have\nbeen seen in the Sunyaev-Zel\'dovich effect. I propose several simple\nexperiments to test the hypothesis.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 21:44:28 GMT\"}]', '2008-11-26', '[[\"Tipler\",\"Frank J.\",\"\"]]'),
(704.3277, 'Michael Ibison', 'M. Ibison', 'Tachyons and superluminal boosts', 'Slightly revised from earlier publication with J. Em. P', '', '', '', 'physics.gen-ph physics.class-ph', '', '  Some arguments in favour of the existence of tachyons and extensions of the\nLorentz Group are presented. On the former, it is observed that with a slight\nmodification to standard electromagnetic theory a single superluminal charge\nwill bind to itself in a self-sustaining circular orbit, suggestive of a\n(modified) electromagnetic interpretation of the strong force. Symmetries in\nthat theory are used in the subsequent analysis as a starting point in the\nsearch for physically-motivated extensions of the Lorentz Group. There is some\ndiscussion of the validity of imaginary coordinates in superluminal\ntransformations of frame. The article concludes with some speculation on the\nimplications for faster-than light travel.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 22:02:13 GMT\"}]', '2007-05-23', '[[\"Ibison\",\"M.\",\"\"]]'),
(704.3278, 'Travis Schedler', 'Travis Schedler', 'Zeroth Hochschild homology of preprojective algebras over the integers', '69 pages, 2 figures; final pre-publication version; many corrections\n  and improvements throughout. Note though the first version has additional\n  results (for instance, it computes the higher Hochschild (co)homology and its\n  structures)', '', '', '', 'math.RT math.QA', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We determine the Z-module structure of the preprojective algebra and its\nzeroth Hochschild homology, for any non-Dynkin quiver (and hence the structure\nworking over any base commutative ring, of any characteristic). This answers\n(and generalizes) a conjecture of Hesselholt and Rains, producing new\n$p$-torsion classes in degrees 2p^l, l >= 1, We relate these classes by p-th\npower maps and interpret them in terms of the kernel of Verschiebung maps from\nnoncommutative Witt theory. An important tool is a generalization of the\nDiamond Lemma to modules over commutative rings, which we give in the appendix.\n  In the previous version, additional results are included, such as: the\nPoisson center of $\\text{Sym } HH_0(\\Pi)$ for all quivers, the BV algebra\nstructure on Hochschild cohomology, including how the Lie algebra structure\n$HH_0(\\Pi_Q)$ naturally arises from it, and the cyclic homology groups of\n$\\Pi_Q$.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 22:05:29 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 16 Feb 2016 11:37:10 GMT\"},{\"version\":\"v3\",\"created\":\"Sat, 28 May 2016 07:36:28 GMT\"}]', '2016-05-31', '[[\"Schedler\",\"Travis\",\"\"]]'),
(704.3279, 'Michael Ibison', 'M. Ibison', 'Un-renormalized Classical Electromagnetism', '', 'Annals of Physics 321 No. 2, pp. 261-305 (2006)', '10.1016/j.aop.2005.05.002', '', 'physics.gen-ph physics.class-ph', '', '  This paper follows in the tradition of direct-action versions of\nelectromagnetism having the aim of avoiding a balance of infinities wherein a\nmechanical mass offsets an infinite electromagnetic mass so as to arrive at a\nfinite observed value. Given that, in this respect the direct-action approached\nultimately failed because its initial exclusion of self-action was found to be\nuntenable in the relativistic domain, this paper continues the tradition\nconsidering instead a version of electromagnetism wherein mechanical action is\nexcluded and self-action is retained. It is shown that the resulting theory is\neffectively interacting due to the presence of infinite forces. A vehicle for\nthe investigation is a pair of classical point charges in a positronium-like\narrangement for which the orbits are found to be self-sustaining and naturally\nquantized.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 22:37:36 GMT\"}]', '2015-05-13', '[[\"Ibison\",\"M.\",\"\"]]'),
(704.3280, 'Jeng-Daw Yu', 'Jeng-Daw Yu', 'Local structure of the moduli space of K3 surfaces over finite\n  characteristic', '10 pages', '', '', '', 'math.AG', '', '  Let k be a perfect field of characteristic p > 2. In this note, we show that\nthe local moduli space of a non-supersingular K3 surface over k with trivial\ndeformation of the associated enlarged formal Brauer group admits a natural\np-divisible formal group structure.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 22:40:29 GMT\"}]', '2007-05-23', '[[\"Yu\",\"Jeng-Daw\",\"\"]]'),
(704.3281, 'Arthur Berg', 'Arthur Berg and Dimitris N Politis and Kagba Suaray and Hui Zeng', 'Reduced bias nonparametric lifetime density and hazard estimation', '21 pages, 4 figures', '', '', '', 'math.ST stat.TH', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  Kernel-based nonparametric hazard rate estimation is considered with a\nspecial class of infinite-order kernels that achieves favorable bias and mean\nsquare error properties. A fully automatic and adaptive implementation of a\ndensity and hazard rate estimator is proposed for randomly right censored data.\nCareful selection of the bandwidth in the proposed estimators yields estimates\nthat are more efficient in terms of overall mean squared error performance, and\nin some cases achieves a nearly parametric convergence rate. Additionally,\nrapidly converging bandwidth estimates are presented for use in second-order\nkernels to supplement such kernel-based methods in hazard rate estimation.\nSimulations illustrate the improved accuracy of the proposed estimator against\nother nonparametric estimators of the density and hazard function. A real data\napplication is also presented on survival data from 13,166 breast carcinoma\npatients.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 01:45:51 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 16 Oct 2018 14:22:00 GMT\"}]', '2018-10-17', '[[\"Berg\",\"Arthur\",\"\"],[\"Politis\",\"Dimitris N\",\"\"],[\"Suaray\",\"Kagba\",\"\"],[\"Zeng\",\"Hui\",\"\"]]'),
(704.3282, 'Andrii Neronov', 'A.Neronov, F.Aharonian', 'Production of TeV gamma-radiation in the vicinity of the supermassive\n  black hole in the giant radiogalaxy M87', '11 pages, ApJ, in print', '', '10.1086/522199', '', 'astro-ph', '', '  Although the giant radiogalaxy M 87 harbors many distinct regions of\nbroad-band nonthermal emission, the recently reported fast variability of TeV\ngamma rays from M 87 on a timescale of days strongly constrains the range of\nspeculations concerning the possible sites and scenarios of particle\nacceleration responsible for the observed TeV emission. A natural production\nsite of this radiation is the immediate vicinity of the central supermassive\nmass black hole (BH). Because of the low bolometric luminosity, the nucleus of\nM 87 is effectively transparent for gamma rays up to energy of 10 TeV, which\nmakes this source an ideal laboratory for study of particle acceleration\nprocesses close to the BH event horizon. We critically analyse different\npossible radiation mechanisms in this region, and argue that the observed very\nhigh-energy gamma ray emission can be explained by the inverse Compton emission\nof ultrarelativistic electron-positron pairs produced through the development\nof an electromagnetic cascade in the BH magnetosphere. We demonstrate, through\ndetailed numerical calculations of acceleration and radiation of electrons in\nthe magnetospheric vacuum gap, that this ``pulsar magnetosphere like\'\' scenario\ncan satisfactorily explain the main properties of TeV gamma-ray emission of M\n87.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 23:18:22 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 7 Aug 2007 11:41:42 GMT\"}]', '2009-11-13', '[[\"Neronov\",\"A.\",\"\"],[\"Aharonian\",\"F.\",\"\"]]'),
(704.3283, 'Uwe Nagel', 'Uwe Nagel, Tim Roemer', 'Glicci simplicial complexes', '', '', '', '', 'math.AC math.CO', '', '  One of the main open questions in liaison theory is whether every homogeneous\nCohen-Macaulay ideal in a polynomial ring is glicci, i.e. if it is in the\nG-liaison class of a complete intersection. We give an affirmative answer to\nthis question for Stanley-Reisner ideals defined by simplicial complexes that\nare weakly vertex-decomposable. This class of complexes includes matroid,\nshifted and Gorenstein complexes respectively. Moreover, we construct a\nsimplicial complex which shows that the property of being glicci depends on the\ncharacteristic of the base field. As an application of our methods we establish\nnew evidence for two conjectures of Stanley on partitionable complexes and on\nStanley decompositions.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 23:48:27 GMT\"}]', '2007-05-23', '[[\"Nagel\",\"Uwe\",\"\"],[\"Roemer\",\"Tim\",\"\"]]'),
(704.3284, 'Ricardo Carretero', 'G. Herring, P.G. Kevrekidis, B.A. Malomed, R. Carretero-Gonzalez, D.J.\n  Frantzeskakis', 'Symmetry Breaking in Linearly Coupled Dynamical Lattices', '9 pages, 9 figures, submitted to Phys. Rev. E, Apr, 2007', 'Phys. Rev. E 76 (2007) 066606', '10.1103/PhysRevE.76.066606', '', 'nlin.PS', '', '  We examine one- and two-dimensional (1D and 2D) models of linearly coupled\nlattices of the discrete-nonlinear-Schr{\\\"{o}}dinger type. Analyzing ground\nstates of the systems with equal powers in the two components, we find a\nsymmetry-breaking phenomenon beyond a critical value of the squared $l^2$-norm.\nAsymmetric states, with unequal powers in their components, emerge through a\nsubcritical pitchfork bifurcation, which, for very weakly coupled lattices,\nchanges into a supercritical one. We identify the stability of various solution\nbranches. Dynamical manifestations of the symmetry breaking are studied by\nsimulating the evolution of the unstable branches. The results present the\nfirst example of spontaneous symmetry breaking in 2D lattice solitons. This\nfeature has no counterpart in the continuum limit, because of the collapse\ninstability in the latter case.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 00:00:48 GMT\"}]', '2010-12-10', '[[\"Herring\",\"G.\",\"\"],[\"Kevrekidis\",\"P. G.\",\"\"],[\"Malomed\",\"B. A.\",\"\"],[\"Carretero-Gonzalez\",\"R.\",\"\"],[\"Frantzeskakis\",\"D. J.\",\"\"]]'),
(704.3285, 'Daniel J. H. Chung', 'Daniel J. H. Chung, Lisa L. Everett, and Konstantin T. Matchev', 'Inflationary Cosmology Connecting Dark Energy and Dark Matter', '16 pages, 3 figures', 'Phys.Rev.D76:103530,2007', '10.1103/PhysRevD.76.103530', 'MADPH-07-1487, UFIFT-HEP-07-5', 'hep-ph astro-ph hep-th', '', '  Kination dominated quintessence models of dark energy have the intriguing\nfeature that the relic abundance of thermal cold dark matter can be\nsignificantly enhanced compared to the predictions from standard cosmology.\nPrevious treatments of such models do not include a realistic embedding of\ninflationary initial conditions. We remedy this situation by constructing a\nviable inflationary model in which the inflaton and quintessence field are the\nsame scalar degree of freedom. Kination domination is achieved after inflation\nthrough a strong push or \"kick\" of the inflaton, and sufficient reheating can\nbe achieved depending on model parameters. This allows us to explore both\nmodel-dependent and model-independent cosmological predictions of this\nscenario. We find that measurements of the B-mode CMB polarization can rule out\nthis class of scenarios almost model independently. We also discuss other\nexperimentally accessible signatures for this class of models.\n', '[{\"version\":\"v1\",\"created\":\"Tue, 24 Apr 2007 23:54:54 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 9 Oct 2007 19:20:48 GMT\"}]', '2008-11-26', '[[\"Chung\",\"Daniel J. H.\",\"\"],[\"Everett\",\"Lisa L.\",\"\"],[\"Matchev\",\"Konstantin T.\",\"\"]]'),
(704.3286, 'Thomas Fleming', 'Thomas Fleming', 'Milnor Invariants for Spatial Graphs', '11 pages, 5 figures', '', '', '', 'math.GT', '', '  Link homotopy has been an active area of research for knot theorists since\nits introduction by Milnor in the 1950s. We introduce a new equivalence\nrelation on spatial graphs called component homotopy, which reduces to link\nhomotopy in the classical case. Unlike previous attempts at generalizing link\nhomotopy to spatial graphs, our new relation allows analogues of some standard\nlink homotopy results and invariants.\n  In particular we can define a type of Milnor group for a spatial graph under\ncomponent homotopy, and this group determines whether or not the spatial graph\nis splittable. More surprisingly, we will also show that whether the spatial\ngraph is splittable up to component homotopy depends only on the link homotopy\nclass of the links contained within it. Numerical invariants of the relation\nwill also be produced.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 00:43:34 GMT\"}]', '2009-09-29', '[[\"Fleming\",\"Thomas\",\"\"]]'),
(704.3287, 'N. Raj Rao', 'N. Raj Rao, Alan Edelman', 'Sample size cognizant detection of signals in white noise', 'To appear in the Proceedings of the 8th IEEE International Workshop\n  on Signal Processing Advances in Wireless Communications (SPAWC), Helsinki,\n  Finland, June 17-20, 2007', '', '', '', 'cs.IT math.IT', '', '  The detection and estimation of signals in noisy, limited data is a problem\nof interest to many scientific and engineering communities. We present a\ncomputationally simple, sample eigenvalue based procedure for estimating the\nnumber of high-dimensional signals in white noise when there are relatively few\nsamples. We highlight a fundamental asymptotic limit of sample eigenvalue based\ndetection of weak high-dimensional signals from a limited sample size and\ndiscuss its implication for the detection of two closely spaced signals.\n  This motivates our heuristic definition of the \'effective number of\nidentifiable signals.\' Numerical simulations are used to demonstrate the\nconsistency of the algorithm with respect to the effective number of signals\nand the superior performance of the algorithm with respect to Wax and Kailath\'s\n\"asymptotically consistent\" MDL based estimator.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 00:23:20 GMT\"}]', '2007-07-13', '[[\"Rao\",\"N. Raj\",\"\"],[\"Edelman\",\"Alan\",\"\"]]'),
(704.3288, 'Roland Kothes', 'P.P. Kronberg, R. Kothes, C.J. Salter, P. Perillat', 'Discovery of new faint radio emission on 8$\\arcdeg$ to 3$\\arcmin$ scales\n  in the Coma field, and some Galactic and extragalactic implications', '12 pages, published in ApJ', 'Astrophys.J.659:267-274,2007', '10.1086/511512', '', 'astro-ph', '', '  We present a deep, 8$\\degr$ diameter, 0.4 GHz radio image using a first time\ncombination of the NAIC Arecibo 305-m telescope in Puerto Rico, and the\nwide-angle interferometer at the Dominion Radio Astrophysical Observatory at\nPenticton, Canada. Our observations are centered on the Coma Cluster of\ngalaxies in the ``Great Wall\'\' of galaxies near the North Galactic Pole. The\ncomplementary nature of these two instruments enables us to produce a\ndistortion-free image that is sensitive to radiation on scales from 8$\\degr$\ndown to that of an individual galaxy halo at the 100 Mpc distance of the Great\nWall. Newly revealed patches of distributed radio ``glow\'\' are seen well above\nthe detection limit. One prominent such area coincides with groupings of radio\ngalaxies near the Coma cluster, and indicates intergalactic IGM magnetic fields\nin the range 0.2 to 0.4 $\\mu$G on scales of up to $\\sim$ 4 Mpc. Other patches\nof diffuse emission, not previously explored at these high latitudes on\narcminute scales, probably contain Galactic ``cirrus\'\'. A striking\nanticorrelation is found between low-level diffuse radio glow and some regions\nof enhanced optical galaxy surface density, suggesting that cosmological Large\nScale Structure (LSS), normally defined by the baryonic (or dark) matter\ndensity, is not {\\it uniquely} traced by faint continuum radio glow. Rather,\nintergalactic diffuse synchrotron radiation represents IGM magnetic and Cosmic\nray energy density, instead of matter density. The diffuse, arcminute-level\nstructures over a large region of sky are potentially important pathfinders to\nCMB foreground radiation on high multipole scales.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 00:20:09 GMT\"}]', '2010-11-05', '[[\"Kronberg\",\"P. P.\",\"\"],[\"Kothes\",\"R.\",\"\"],[\"Salter\",\"C. J.\",\"\"],[\"Perillat\",\"P.\",\"\"]]'),
(704.3289, 'Boris Gutkin', 'Boris Gutkin', 'Dynamical \"breaking\" of time reversal symmetry and converse quantum\n  ergodicity', '10 pages, 5 figures', '', '', '', 'nlin.CD', '', '  It is a common assumption that quantum systems with time reversal invariance\nand classically chaotic dynamics have energy spectra distributed according to\nGOE-type of statistics. Here we present a class of systems which fail to follow\nthis rule. We show that for convex billiards of constant width with time\nreversal symmetry and \"almost\" chaotic dynamics the energy level distribution\nis of GUE-type. The effect is due to the lack of ergodicity in the \"momentum\"\npart of the phase space and, as we argue, is generic in two dimensions.\nBesides, we show that certain billiards of constant width in multiply connected\ndomains are of interest in relation to the quantum ergodicity problem. These\nbilliards are quantum ergodic, but not classically ergodic.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 00:54:54 GMT\"}]', '2007-05-23', '[[\"Gutkin\",\"Boris\",\"\"]]'),
(704.3290, 'Konstantin Mikhailov R.', 'A. Stavinskiy, K. Mikhailov, B. Erazmus, R. Lednicky', 'Residual correlations between decay products of $\\pi^0\\pi^0$ and\n  $p\\Sigma^0$ systems', '10 pages, 5 figures', '', '', '', 'nucl-th hep-ph', '', '  Residual correlations between decay products due to a combination of both\ncorrelations between parents at small relative velocities and small decay\nmomenta are discussed. Residual correlations between photons from pion decays\nare considered as a new possible source of information on direct photon\nfraction. Residual correlations in $p\\gamma$ and $p\\Lambda$ systems due to\n$p\\Sigma^0$ interaction in final state are predicted based on the $p\\Sigma^0$\nlow energy scattering parameters deduced from the spin-flavour SU$_6$ model by\nFujiwara et al. including effective meson exchange potentials and explicit\nflavour symmetry breaking to reproduce the properties of the two-nucleon system\nand the low-energy hyperon-nucleon cross section data. The $p\\gamma_{\\Sigma^0}$\nresidual correlation is concentrated at $k^* \\approx 70$ Mev/$c$ and its shape\nand intensity appears to be sensitive to the scattering parameters and\nspace-time dimensions of the source. The $p\\Lambda_{\\Sigma^0}$ residual\ncorrelation recovers the negative parent $p\\Sigma^0$ correlation for $k^* > 70$\nMev/$c$. The neglect of this negative residual correlation would lead to the\nunderestimation of the parent $p\\Lambda$ correlation effect and to an\noverestimation of the source size.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 01:08:29 GMT\"}]', '2007-05-23', '[[\"Stavinskiy\",\"A.\",\"\"],[\"Mikhailov\",\"K.\",\"\"],[\"Erazmus\",\"B.\",\"\"],[\"Lednicky\",\"R.\",\"\"]]'),
(704.3291, 'Lukasz Fidkowski', 'Lukasz Fidkowski', 'Double Point Contact in the k=3 Read-Rezayi State', '7 pages, 3 figures', '', '', '', 'cond-mat.mes-hall cond-mat.str-el', '', '  We compute the dependence of the tunneling current in a double point contact\nin the k=3 Read-Rezayi state (which is conjectured to describe an\nincompressible quantum hall fluid at filling fraction nu=12/5) on voltage,\nseparation between the two contacts, and temperature. Using the tunneling\nhamiltonian of cond-mat/0607431, we show that the effect of quasiholes in the\nbulk region between the two contacts is simply an overall constant multiplying\nthe interference term. This is the same effect as found for the differential\nconductivity in cond-mat/0601242; the difference is that we do an actual edge\ntheory calculation and compute the full current-voltage curve at weak\ntunneling.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 01:17:30 GMT\"}]', '2007-05-23', '[[\"Fidkowski\",\"Lukasz\",\"\"]]'),
(704.3292, 'Zhu Han', 'Zhu Han and H. Vincent Poor', 'Coalition Games with Cooperative Transmission: A Cure for the Curse of\n  Boundary Nodes in Selfish Packet-Forwarding Wireless Networks', '', 'in the Proceedings of the 5th International Symposium on Modeling\n  and Optimization in Mobile Ad Hoc and Wireless Networks, WiOpt07, Limassol,\n  Cyprus, April 16-20, 2007', '', '', 'cs.IT math.IT', '', '  In wireless packet-forwarding networks with selfish nodes, applications of a\nrepeated game can induce the nodes to forward each others\' packets, so that the\nnetwork performance can be improved. However, the nodes on the boundary of such\nnetworks cannot benefit from this strategy, as the other nodes do not depend on\nthem. This problem is sometimes known as the curse of the boundary nodes. To\novercome this problem, an approach based on coalition games is proposed, in\nwhich the boundary nodes can use cooperative transmission to help the backbone\nnodes in the middle of the network. In return, the backbone nodes are willing\nto forward the boundary nodes\' packets. The stability of the coalitions is\nstudied using the concept of a core. Then two types of fairness, namely, the\nmin-max fairness using nucleolus and the average fairness using the Shapley\nfunction are investigated. Finally, a protocol is designed using both repeated\ngames and coalition games. Simulation results show how boundary nodes and\nbackbone nodes form coalitions together according to different fairness\ncriteria. The proposed protocol can improve the network connectivity by about\n50%, compared with pure repeated game schemes.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 15:37:22 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 21:15:48 GMT\"}]', '2007-07-13', '[[\"Han\",\"Zhu\",\"\"],[\"Poor\",\"H. Vincent\",\"\"]]'),
(704.3293, 'Andrea Montanari', 'Antoine Gerschenfeld and Andrea Montanari', 'Reconstruction for models on random graphs', '16 pages', '', '', '', 'math.PR cond-mat.stat-mech math.CO', '', '  Consider a collection of random variables attached to the vertices of a\ngraph. The reconstruction problem requires to estimate one of them given `far\naway\' observations. Several theoretical results (and simple algorithms) are\navailable when their joint probability distribution is Markov with respect to a\ntree. In this paper we consider the case of sequences of random graphs that\nconverge locally to trees. In particular, we develop a sufficient condition for\nthe tree and graph reconstruction problem to coincide. We apply such condition\nto colorings of random graphs.\n  Further, we characterize the behavior of Ising models on such graphs, both\nwith attractive and random interactions (respectively, `ferromagnetic\' and\n`spin glass\').\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 01:35:38 GMT\"},{\"version\":\"v2\",\"created\":\"Mon, 10 Sep 2007 05:14:58 GMT\"}]', '2007-09-10', '[[\"Gerschenfeld\",\"Antoine\",\"\"],[\"Montanari\",\"Andrea\",\"\"]]'),
(704.3294, 'Jonathan E. Grindlay', 'Jonathan E. Grindlay', 'AGN Variability Surveys: DASCH from BATSS to EXIST', '4 pages, 3 figures, Conference proceedings to appear in \"The Central\n  Engine of Active Galactic Nuclei\", eds. L. C. Ho and J.-M. Wang (San\n  Francisco: ASP)', '', '', '', 'astro-ph', '', '  Active galactic nuclei (AGN) are variable on a wide range of timescales,\nthough relatively few systematic variability surveys have been conducted.\nPrevious broad-band (both spectral and temporal) variability surveys of AGN are\nlimited in their temporal and spectral bandwidth, despite their promise for\nprobing the central engine and black hole mass. We outline optimal properties\nfor variability studies and provide a brief summary of three new variability\nsurveys, two (BATSS and DASCH) about to begin and the third (EXIST) possible\nwithin the next decade, which will open new windows on the physics and\nfundamental properties of AGN.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 01:53:25 GMT\"}]', '2007-05-23', '[[\"Grindlay\",\"Jonathan E.\",\"\"]]'),
(704.3295, 'Monica Guica', 'Monica Guica, Andrew Strominger', 'Cargese lectures on string theory with eight supercharges', '30 pp, 7 figures, based on lecture notes by A. Strominger at the 2006\n  Cargese summer school', 'Nucl.Phys.Proc.Suppl.171:39-68,2007', '10.1016/j.nuclphysbps.2007.06.007', '', 'hep-th', '', '  These lectures give an introduction to the interrelated topics of Calabi-Yau\ncompactification of the type II string, black hole attractors, the all-orders\nentropy formula, the dual (0,4) CFT, topological strings and the OSV\nconjecture. Based on notes by MG of lectures by AS at the 2006 Cargese summer\nschool.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 02:01:32 GMT\"}]', '2008-11-26', '[[\"Guica\",\"Monica\",\"\"],[\"Strominger\",\"Andrew\",\"\"]]'),
(704.3296, 'Anton Lipovka', 'J. Campos, A. Lipovka, J. Saucedo', 'Formation of C- by radiative association', '3 pages, 1 figure', '', '', '', 'astro-ph', '', '  In the present paper the problem of the radiative association of atoms of\ncarbon C with electrons $e^{-}$ for kinetic temperatures $T_{c}$ of $100 <\nT_{c} < 3000$ K is considered. The calculation of the rate rate constant of the\nradiative associations is made with principle of detailed balance. It is shown\nthat the rate has correct behavior (it increase with the temperature) and its\nbehavior is look-like that for the $H^{-}$ formation rate coefficient, which\nalso increase with the temperature.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 02:01:45 GMT\"}]', '2007-05-23', '[[\"Campos\",\"J.\",\"\"],[\"Lipovka\",\"A.\",\"\"],[\"Saucedo\",\"J.\",\"\"]]'),
(704.3297, 'Antia Lamas-Linares', 'Antia Lamas-Linares and Christian Kurtsiefer', 'Breaking a quantum key distribution system through a timing side channel', '6 pages, 4 figures. Added additional references and extended\n  analysis. Identical to published version', 'Opt. Express 15, 9388 (2007)', '10.1364/OE.15.009388', '', 'quant-ph', '', '  The security of quantum key distribution relies on the validity of quantum\nmechanics as a description of nature and on the non-existence of leaky degrees\nof freedom in the practical implementations. We experimentally demonstrate how,\nin some implementations, timing information revealed during public discussion\nbetween the communicating parties can be used by an eavesdropper to\nundetectably access a significant portion of the ``secret\'\' key.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 02:07:36 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 17 Jul 2007 09:45:55 GMT\"}]', '2009-11-13', '[[\"Lamas-Linares\",\"Antia\",\"\"],[\"Kurtsiefer\",\"Christian\",\"\"]]'),
(704.3298, 'Abdul Rahman', 'Abdul Rahman', 'A Perverse Sheaf Approach Toward a Cohomology Theory for String Theory', 'Added section 5 (an example)', '', '', '', 'math.AT hep-th math-ph math.MP', 'http://arxiv.org/licenses/nonexclusive-distrib/1.0/', '  We present the construction and properties of a self-dual perverse sheaf S_0\nwhose cohomology fulfills some of the requirements of String theory as outlined\nby T. Hubsch in hep-th/9612075. The construction of this S_0 utilizes\ntechniques that follow from MacPherson-Vilonen (Inv. Math. vol. 84, pp.\n403-435, 1986). Finally, we will discuss its properties as they relate to\nString theory.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 12:36:54 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 25 Apr 2007 22:10:58 GMT\"},{\"version\":\"v3\",\"created\":\"Mon, 30 Apr 2007 12:07:35 GMT\"},{\"version\":\"v4\",\"created\":\"Mon, 27 Aug 2007 01:45:58 GMT\"},{\"version\":\"v5\",\"created\":\"Wed, 20 May 2009 21:06:14 GMT\"}]', '2009-05-21', '[[\"Rahman\",\"Abdul\",\"\"]]'),
(704.3299, 'Kunihiko Terasaki', 'Kunihiko Terasaki', 'D_{s0}^+(2317) as an Iso-triplet Four-quark Meson and Production of Its\n  Neutral and Doubly Charged Partners', '6 pages, 3 figures, RevTeX', 'Prog.Theor.Phys.Suppl.168:211-218,2007', '10.1143/PTPS.168.211', 'YITP-07-22, KANAZAWA-07-02', 'hep-ph hep-ex nucl-th', '', '  By studying the decays D_{s0}^+(2317) --> D_s^+ pi^0 and D_s^{*+} gamma, It\nis shown that its assignment to the I_3=0 component of iso-triplet scalar\nfour-quark mesons is favored. Productions of its neutral and doubly charged\npartners are also studied. As the result, it is concluded that they could be\nobserved in B decays. Their iso-singlet partner might have been observed in the\nradiative channels of B decays by the BELLE Collaboration.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 03:01:02 GMT\"}]', '2008-11-26', '[[\"Terasaki\",\"Kunihiko\",\"\"]]'),
(704.3300, 'Kohkichi Konno', 'Kohkichi Konno, Munehiro Nishida, Satoshi Tanda, Noriyuki Hatakenaka', 'The effect of dissipation on quantum transmission resonance', '8 pages, 5 figures, Accepted for publication in Physics Letters A', 'Physics Letters A 368 (2007) 442-449', '10.1016/j.physleta.2007.04.055', '', 'quant-ph', '', '  Quantum transmissions of a free particle passing through a rectangular\npotential barrier with dissipation are studied using a path decomposition\ntechnique. Dissipative processes strongly suppress the transmission probability\nat resonance just above the barrier resulting in an unexpected reduction of the\nmean traversal time through the potential barrier.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 03:03:22 GMT\"}]', '2007-08-27', '[[\"Konno\",\"Kohkichi\",\"\"],[\"Nishida\",\"Munehiro\",\"\"],[\"Tanda\",\"Satoshi\",\"\"],[\"Hatakenaka\",\"Noriyuki\",\"\"]]'),
(704.3301, 'Alexander Vikman', 'Eugeny Babichev, Viatcheslav Mukhanov, Alexander Vikman', 'Looking beyond the horizon', 'To appear in the proceedings of 11th Marcel Grossmann Meeting on\n  Recent Developments in Theoretical and Experimental General Relativity,\n  Gravitation, and Relativistic Field Theories, Berlin, Germany, 23-29 Jul 2006', '', '10.1142/9789812834300_0171', 'LMU-ASC 27/07', 'hep-th astro-ph gr-qc', '', '  In this short talk we review our results from the paper hep-th/0604075 with\nthe main stress on the issues of causality and acoustic metric in eikonal\napproximation. In addition we correct the formula for the redshift of sound\nsignals from our original work. We show that, if there exists a special kind of\nBorn-Infeld type scalar field, then one can send information from inside a\nblack hole. This information is encoded in perturbations of the field\npropagating in non-trivial scalar field backgrounds, which serve as a \"new\nether\". Although the action of the theory is manifestly Lorentz-invariant the\nnon-trivial solutions break this symmetry spontaneously, allowing, the\nsuperluminal propagation of perturbations with respect to this \"new ether\". We\nfound the stationary solution for background, which describes the accretion of\nthe scalar field onto a black hole. Examining the propagation of small\nperturbations around this solution we show that the signals emitted inside the\nSchwarzschild horizon can reach an observer located outside the black hole.\nThus the accreting field forms a hydrodynamical analog of a black hole whose\nhorizon is inside of the gravitational black hole drawing in the scalar field.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 16:29:51 GMT\"}]', '2016-11-15', '[[\"Babichev\",\"Eugeny\",\"\"],[\"Mukhanov\",\"Viatcheslav\",\"\"],[\"Vikman\",\"Alexander\",\"\"]]'),
(704.3302, 'Vitali Nesterenko', 'E.B. Herbold, V.F. Nesterenko', 'Solitary and shock waves in discrete double power-law materials', '14 pages, 6 figures', '', '10.1063/1.2751592', '', 'cond-mat.soft cond-mat.mtrl-sci', '', '  A novel strongly nonlinear laminar metamaterial supporting new types of\nsolitary and shock waves with impact energy mitigating capabilities is\npresented. It consists of steel plates with intermittent polymer toroidal rings\nacting as strongly nonlinear springs with large allowable strain. Their\nforce-displacement relationship is described by the addition of two power-law\nrelationships resulting in a solitary wave speed and width depending on the\namplitude. This double nonlinearity allows splitting of an initial impulse into\ntwo separate strongly nonlinear solitary wave trains. Solitary and shock waves\nare observed experimentally and analyzed numerically in an assembly with Teflon\no-rings.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 03:08:03 GMT\"},{\"version\":\"v2\",\"created\":\"Fri, 24 Aug 2007 22:49:15 GMT\"}]', '2009-11-13', '[[\"Herbold\",\"E. B.\",\"\"],[\"Nesterenko\",\"V. F.\",\"\"]]'),
(704.3303, 'Gang Bao', 'Gang Bao, D N A Shaul, H M Araujo, Wei-Tou Ni, T J Sumner and Lei Liu', 'ASTROD I Charging Simulation and Disturbances', '17 pages, 11 figures, submitted to General Relativity and Gravitation', '', '', '', 'astro-ph', '', '  ASTROD I is planned as a single spacecraft mission. It will use\ninterferometric and pulse ranging techniques between the spacecraft and ground\nstations, to make high precision measurements of the parameters that describe\nthe solar system, and to test relativistic gravity with improved accuracy. At\nthe heart of the spacecraft is a test mass, which the spacecraft will follow\nusing a drag-free control system. The mission critically depends on maintaining\nthe geodesic motion of the test mass. Charging of the test mass due to cosmic\nrays and solar particles will disturb its geodesic motion. We have modelled the\ncharging process using the GEANT4 toolkit and a simplified, geometrical model\nand estimate that the ASTROD I test mass will charge positively, at a rate of\n24 +/-7 e+/s, due to cosmic ray protons and alpha particles (3He and 4He) at\nsolar minimum. We have used the results of this simulation to estimate the\nmagnitude of disturbances associated with test mass charging, for the\nworst-case scenario, taking into account uncertainties in the model and\npotential charging contributions from minor cosmic-ray components.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 03:08:29 GMT\"}]', '2007-05-23', '[[\"Bao\",\"Gang\",\"\"],[\"Shaul\",\"D N A\",\"\"],[\"Araujo\",\"H M\",\"\"],[\"Ni\",\"Wei-Tou\",\"\"],[\"Sumner\",\"T J\",\"\"],[\"Liu\",\"Lei\",\"\"]]'),
(704.3304, 'S. Satheesh', 'S Satheesh and E Sandhya', 'On the Marginal Distributions of Stationary AR(1) Sequences', '4 pages, in .pdf format, submitted', '', '', '', 'math.PR math.ST stat.TH', '', '  In this note we correct an omission in our paper (Satheesh and Sandhya, 2005)\nin defining semi-selfdecomposable laws and also show with examples that the\nmarginal distributions of a stationary AR(1) process need not even be\ninfinitely divisible.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 03:28:39 GMT\"}]', '2007-05-23', '[[\"Satheesh\",\"S\",\"\"],[\"Sandhya\",\"E\",\"\"]]'),
(704.3305, 'Ping Zhang', 'Zhigang Wang, Ping Zhang', 'Orbital magnetization and its effects in spin-chiral ferromagnetic\n  Kagome lattice', '9 pages, 7 figures', '', '10.1103/PhysRevB.76.064406', '', 'cond-mat.mes-hall cond-mat.str-el', '', '  Recently, Berry phase in the semiclassical dynamical of Bloch electrons has\nbeen found to make a correction to the phase-space density of states and a\ngeneral multi-band formula for finite-temperature orbital magnetization has\nbeen given [Phys. Rev. Lett. \\textbf{97}, 026603 (2006)], where the orbital\nmagnetization $\\mathcal{M}$ consists of two parts, i.e., the conventional part\n$M_{c}$ and the Berry-phase correction part $M_{\\Omega}$. Using this general\nformula, we theoretically investigate the orbital magnetization and its effects\non thermoelectric transport and magnetic susceptibility properties of the\ntwo-dimensional \\textit{kagom\\\'{e}} lattice with spin anisotropies included.\nThe study in this paper is highly interesting by the occurrence of nonzero\nChern number in the lattice. The spin chirality parameter $\\phi$ (see text)\nresults in profound effects on the orbital magnetization properties. It is\nfound that the two parts in orbital magnetization opposite each other. In\nparticular, we show that $M_{c}$ and $M_{\\Omega}$ yield the paramagnetic and\ndiamagnetic responses, respectively. It is further shown that the orbital\nmagnetization displays fully different behavior in the metallic and insulating\nregions, which is due to the different roles $M_{c}$ and $M_{\\Omega}$ play in\nthese two regions. The anomalous Nernst conductivity is also calculated, which\ndisplays a peak-valley structure as a function of the electron Fermi energy.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 03:34:10 GMT\"}]', '2009-11-13', '[[\"Wang\",\"Zhigang\",\"\"],[\"Zhang\",\"Ping\",\"\"]]'),
(704.3306, 'Alexey A. Kryukov', 'Alexey A. Kryukov', 'Quantum mechanics on Hilbert manifolds: The principle of functional\n  relativity', '45 pages, 9 figures, see arXiv:0704.3225v1 for mathematical\n  considerations and http://www.uwc.edu/dept/math/faculty/kryukov/ for related\n  papers', 'Found. Phys. 36, 175 (2006)', '10.1007/s10701-005-9012-1', '', 'quant-ph math-ph math.MP', '', '  Quantum mechanics is formulated as a geometric theory on a Hilbert manifold.\nImages of charts on the manifold are allowed to belong to arbitrary Hilbert\nspaces of functions including spaces of generalized functions. Tensor equations\nin this setting, also called functional tensor equations, describe families of\nfunctional equations on various Hilbert spaces of functions. The principle of\nfunctional relativity is introduced which states that quantum theory is indeed\na functional tensor theory, i.e., it can be described by functional tensor\nequations. The main equations of quantum theory are shown to be compatible with\nthe principle of functional relativity. By accepting the principle as a\nhypothesis, we then analyze the origin of physical dimensions, provide a\ngeometric interpretation of Planck\'s constant, and find a simple interpretation\nof the two-slit experiment and the process of measurement.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 04:03:37 GMT\"}]', '2015-05-13', '[[\"Kryukov\",\"Alexey A.\",\"\"]]'),
(704.3307, 'Takaki Muramatsu', 'Takaki Muramatsu, Taisuke Kanemasa, Ernst Bauer, Mauro Giiovannini,\n  Tomoko Kagayama, Katsuya Shimizu', 'Pressure induced magnetic ordering in Yb2Pd2Sn with two quantum critical\n  points', '4 pages, 4 figures', '', '', '', 'cond-mat.str-el', '', '  Pressure induced long range antiferromagnetic order is discovered in Yb2Pd2Sn\nby measuring the electrical resistivity under pressure up to 5.0 GPa. Magnetic\nordering is observed above about 1.0 GPa, being the lowest pressure in\nYb-intermetallics showing pressure induced magnetic ordering, Unexpectedly,\nordering disappears above about 4.0 GPa, giving rise to the first observation\nof the appearance of two quantum critical points persisting in a broad range of\npressure within a single material.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 04:07:54 GMT\"},{\"version\":\"v2\",\"created\":\"Wed, 30 May 2007 10:51:07 GMT\"}]', '2007-06-13', '[[\"Muramatsu\",\"Takaki\",\"\"],[\"Kanemasa\",\"Taisuke\",\"\"],[\"Bauer\",\"Ernst\",\"\"],[\"Giiovannini\",\"Mauro\",\"\"],[\"Kagayama\",\"Tomoko\",\"\"],[\"Shimizu\",\"Katsuya\",\"\"]]'),
(704.3308, 'Ilarion Melnikov', 'Nick Halmagyi, Ilarion V. Melnikov, and Savdeep Sethi', 'Instantons, Hypermultiplets and the Heterotic String', '52 pages, LaTeX; references, some corrections and clarifications\n  added to the published version', 'JHEP0707:086,2007', '10.1088/1126-6708/2007/07/086', 'EFI-07-11', 'hep-th', '', '  Hypermultiplet couplings in type IIA string theory on a Calabi-Yau space can\nbe quantum corrected by D2-brane instantons wrapping special Lagrangian cycles.\nOn the other hand, hypermultiplet couplings in the heterotic string on a K3\nsurface are corrected by world-sheet instantons wrapping curves. In a class of\nexamples, we relate these two sets of instanton corrections. We first present\nan analogue of the c-map for the heterotic string via a dual flux\ncompactification of M-theory. Using this duality, we propose two ways of\ncapturing quantum corrections to hypermultiplets. We then use the orientifold\nlimit of certain F-theory compactifications to relate curves in K3 to special\nLagrangians in dual type IIA compactifications. We conclude with some results\nfrom perturbative string theory for hypermultiplet F-terms and a conjecture\nabout the topology of brane instantons.\n', '[{\"version\":\"v1\",\"created\":\"Wed, 25 Apr 2007 05:09:34 GMT\"},{\"version\":\"v2\",\"created\":\"Tue, 8 May 2007 22:29:08 GMT\"},{\"version\":\"v3\",\"created\":\"Wed, 1 Aug 2007 16:28:15 GMT\"}]', '2008-11-26', '[[\"Halmagyi\",\"Nick\",\"\"],[\"Melnikov\",\"Ilarion V.\",\"\"],[\"Sethi\",\"Savdeep\",\"\"]]');
