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801.1373 | Christian Iniotakis | C. Iniotakis, S. Fujimoto, and M. Sigrist | Fractional flux quanta at intrinsic metallic interfaces of
noncentrosymmetric superconductors | 4 pages, 3 figures | J. Phys. Soc. Jpn. 77, 083701 (2008) | 10.1143/JPSJ.77.083701 | null | cond-mat.supr-con | null | We examine intrinsic interfaces separating crystalline twin domains of
opposite spin-orbit coupling in a noncentrosymmetric superconductor such as
CePt3Si. At these interfaces, low-energy Andreev bound states occur as a
consequence of parity-mixed Cooper pairing, and a superconducting phase which
violates time reversal symmetry can be realized. This provides an environment
allowing flux lines with fractional flux quanta to be formed at the interface.
Their presence could have strong implications on the flux creep behavior in
such superconductors.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:13:57 GMT"
}
] | 2008-07-25T00:00:00 | [
[
"Iniotakis",
"C.",
""
],
[
"Fujimoto",
"S.",
""
],
[
"Sigrist",
"M.",
""
]
] | [
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801.1374 | Byung-Yoon Park | Byung-Yoon Park, Mannque Rho, Vicente Vento | The Role of the Dilaton in Dense Skyrmion Matter | null | Nucl.Phys.A807:28-37,2008 | 10.1016/j.nuclphysa.2008.03.015 | null | hep-ph nucl-th | null | In this note, we report on a remarkable and surprising interplay between the
omega meson and the dilaton chi in the structure of a single skyrmion as well
as in the phase structure of dense skyrmion matter which may have a potentially
important consequence on the properties of compact stars. In our continuing
effort to understand hadronic matter at high density, we have developed a
unified field theoretic formalism for dense skyrmion matter using a single
Lagrangian to describe simultaneously both matter and meson fluctuations and
studied in-medium properties of hadrons. The effective theory used is the
Skyrme model Lagrangian gauged with the vector mesons rho and omega,
implemented with the dilaton field that describes the spontaneously broken
scale symmetry of QCD, in a form consistent with the symmetries of QCD and our
expectations regarding the high density limit. We analyze the restoration of
scale invariance and chiral symmetry as the density of the system increases. In
order to preserve the restoration of scale symmetry and chiral symmetry,
signalled in our case by the vanishing of the expectation value of the dilaton,
and to be consistent with the vector manifestation of hidden local symmetry, a
density dependent omega coupling is introduced. We uncover the crucial role
played by both the dilaton and the omega meson in the phase structure of dense
medium and discover how two different phase transition regimes arise as we dial
the dilaton mass.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:06:30 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Park",
"Byung-Yoon",
""
],
[
"Rho",
"Mannque",
""
],
[
"Vento",
"Vicente",
""
]
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801.1375 | Francisco Lobo | Christian G. Boehmer, Tiberiu Harko, Francisco S.N. Lobo | Solar system tests of brane world models | 14 pages, to appear in Classical and Quantum Gravity. V2, minor
corrections and references added | Class.Quant.Grav.25:045015,2008 | 10.1088/0264-9381/25/4/045015 | null | gr-qc astro-ph hep-th | null | The classical tests of general relativity (perihelion precession, deflection
of light, and the radar echo delay) are considered for the Dadhich, Maartens,
Papadopoulos and Rezania (DMPR) solution of the spherically symmetric static
vacuum field equations in brane world models. For this solution the metric in
the vacuum exterior to a brane world star is similar to the Reissner-Nordstrom
form of classical general relativity, with the role of the charge played by the
tidal effects arising from projections of the fifth dimension. The existing
observational solar system data on the perihelion shift of Mercury, on the
light bending around the Sun (obtained using long-baseline radio
interferometry), and ranging to Mars using the Viking lander, constrain the
numerical values of the bulk tidal parameter and of the brane tension.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:04:20 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Feb 2008 15:37:24 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Boehmer",
"Christian G.",
""
],
[
"Harko",
"Tiberiu",
""
],
[
"Lobo",
"Francisco S. N.",
""
]
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] |
801.1376 | Carsten Schubert | Daniel Lenz, Carsten Schubert and Peter Stollmann | Eigenfunction expansion for Schrodinger operators on metric graphs | 11 pages, submitted to Jounal of Integral Equations and Operator
Theory | null | null | null | math-ph math.MP | null | We construct an expansion in generalized eigenfunctions for Schrodinger
operators on metric graphs. We require rather minimal assumptions concerning
the graph structure and the boundary conditions at the vertices.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:18:42 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Lenz",
"Daniel",
""
],
[
"Schubert",
"Carsten",
""
],
[
"Stollmann",
"Peter",
""
]
] | [
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] |
801.1377 | Shankar Prasad Das | Madhu Priya and Shankar P. Das | Fragility and elastic behavior of a supercooled liquid | 20 pages, 9 figures (.eps) | Physical Review E 76, 061501 (2007) | 10.1103/PhysRevE.76.061501 | null | cond-mat.soft | null | A model for the supercooled liquid is considered by taking into account its
solid like properties. We focus on how the long time dynamics is affected due
to the coupling between the slowly decaying density fluctuations and the local
displacement variables in the frozen liquid. Results from our model agree with
the recent observation of Novikov and Sokolov [Nature (London) {\bf 431}, 961
(2004)] that the fragility index $m$ of a glass forming material is linearly
related to the corresponding ratio $K/G$ of the bulk and the shear moduli.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:10:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Priya",
"Madhu",
""
],
[
"Das",
"Shankar P.",
""
]
] | [
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] |
801.1378 | Andr\'e Eckardt | Andre Eckardt and Martin Holthaus | Dressed matter waves | 9 pages, 4 figures, to be published in: J. Phys.: Conference Series | J. Phys.: Conf. Ser. 99, 012007 (2008) | 10.1088/1742-6596/99/1/012007 | null | cond-mat.other | null | We suggest to view ultracold atoms in a time-periodically shifted optical
lattice as a "dressed matter wave", analogous to a dressed atom in an
electromagnetic field. A possible effect lending support to this concept is a
transition of ultracold bosonic atoms from a superfluid to a Mott-insulating
state in response to appropriate "dressing" achieved through time-periodic
lattice modulation. In order to observe this effect in a laboratory experiment,
one has to identify conditions allowing for effectively adiabatic motion of a
many-body Floquet state.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:25:32 GMT"
}
] | 2008-03-25T00:00:00 | [
[
"Eckardt",
"Andre",
""
],
[
"Holthaus",
"Martin",
""
]
] | [
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] |
801.1379 | Sixia Yu | Ying Dong, Xiuhao Deng, Mingming Jiang, Qing Chen, and Sixia Yu | Quantum Error-Correcting Codes with Preexisting Protected Qubits | 4 pages 2 figures | null | null | null | quant-ph | null | We provide a systematic way of constructing entanglement-assisted quantum
error-correcting codes via graph states in the scenario of preexisting
perfectly protected qubits. It turns out that the preexisting entanglement can
help beat the quantum Hamming bound and can enhance (not only behave as an
assistance) the performance of the quantum error correction. Furthermore we
generalize the error models to the case of not-so-perfectly-protected qubits
and introduce the quantity infidelity as a figure of merit and show that our
code outperforms also the ordinary quantum error-correcting codes.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:30:09 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Dong",
"Ying",
""
],
[
"Deng",
"Xiuhao",
""
],
[
"Jiang",
"Mingming",
""
],
[
"Chen",
"Qing",
""
],
[
"Yu",
"Sixia",
""
]
] | [
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] |
801.138 | Krzysztof Rogacki | K. Rogacki, G. Schuck, Z. Bukowski, N.D. Zhigadlo, and J. Karpinski | Structural and Superconducting Properties of RbOs2O6 Single Crystals | 20 pages, 8 figures, 3 tables | Phys. Rev. B 77, 134514 (2008) | 10.1103/PhysRevB.77.134514 | null | cond-mat.supr-con cond-mat.str-el | null | Single crystals of RbOs2O6 have been grown from Rb2O and Os in sealed quartz
ampoules. The crystal structure has been identified at room temperature as
cubic with the lattice constant a = 10.1242(12) A. The anisotropy of the
tetrahedral and octahedral networks is lower and the displacement parameters of
alkali metal atoms are smaller than for KOs2O6, so the "rattling" of the alkali
atoms in RbOs2O6 is less pronounced. Superconducting properties of RbOs2O6 in
the mixed state have been well described within the London approach and the
Ginzburg-Landau parameter kappa(0) = 31 has been derived from the reversible
magnetization. This parameter is field dependent and changes at low
temperatures from kappa = 22 (low fields) to kappa = 31 at H_{c2}. The
thermodynamic critical field H_{c}(0) = 1.3 kOe and the superconducting gap
2delta/k_{B}T_{c} = 3.2 have been estimated. These results together with
slightly different H_{c2}(T) dependence obtained for crystals and
polycrystalline RbOs2O6 proof evidently that this compound is a weak-coupling
BCS-type superconductor close to the dirty limit.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:33:23 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Apr 2008 12:44:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rogacki",
"K.",
""
],
[
"Schuck",
"G.",
""
],
[
"Bukowski",
"Z.",
""
],
[
"Zhigadlo",
"N. D.",
""
],
[
"Karpinski",
"J.",
""
]
] | [
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] |
801.1381 | Alessia Annibale | Alessia Annibale, Peter Sollich | Fluctuation-dissipation relations in critical coarsening: crossover from
unmagnetized to magnetized initial states | 34 pages, 10 figures | null | 10.1088/1751-8113/41/13/135001 | null | cond-mat.dis-nn | null | We study the non-equilibrium dynamics of the spherical ferromagnet quenched
to its critical temperature, as a function of the magnetization of the initial
state. The two limits of unmagnetized and fully magnetized initial conditions
can be understood as corresponding to times that are respectively much shorter
and much longer than a magnetization timescale, as in a recent field
theoretical analysis of the $n$-vector model. We calculate exactly the
crossover functions interpolating between these two limits, for the
magnetization correlator and response and the resulting fluctuation-dissipation
ratio (FDR). For $d>4$ our results match those obtained recently from a
Gaussian field theory. For $d<4$, non-Gaussian fuctuations arising from the
spherical constraint need to be accounted for. We extend our framework from the
fully magnetized case to achieve this, providing an exact solution for the
relevant integral kernel. The resulting crossover behaviour is very rich, with
the asymptotic FDR $X^\infty$ depending non-monotonically on the scaled age of
the system. This is traced back to non-monotonicities of the two-time
correlator, themselves the consequence of large magnetization fluctuations on
the crossover timescale. We correct a trivial error in our earlier calculation
for fully magnetized initial states; the corrected FDR is {\em consistent} with
renormalization group expansions to first order in $4-d$ for the longitudinal
fluctuations of the O(n) model in the limit $n\to\infty$.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:36:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Annibale",
"Alessia",
""
],
[
"Sollich",
"Peter",
""
]
] | [
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] |
801.1382 | Takuma Akimoto | Takuma Akimoto | Generalized Arcsine Law and Stable Law in an Infinite Measure Dynamical
System | 8 pages, 8 figures | J. Stat. Phys. 132 (2008) 171-186 | 10.1007/s10955-008-9544-9 | null | cond-mat.stat-mech | null | Limit theorems for the time average of some observation functions in an
infinite measure dynamical system are studied. It is known that intermittent
phenomena, such as the Rayleigh-Benard convection and Belousov-Zhabotinsky
reaction, are described by infinite measure dynamical systems.We show that the
time average of the observation function which is not the $L^1(m)$ function,
whose average with respect to the invariant measure $m$ is finite, converges to
the generalized arcsine distribution. This result leads to the novel view that
the correlation function is intrinsically random and does not decay. Moreover,
it is also numerically shown that the time average of the observation function
converges to the stable distribution when the observation function has the
infinite mean.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:46:01 GMT"
}
] | 2010-05-14T00:00:00 | [
[
"Akimoto",
"Takuma",
""
]
] | [
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] |
801.1383 | Thomas Jordan | Anders Johansson, Thomas Jordan, Anders \"Oberg and Mark Pollicott | Multifractal analysis of non-uniformly hyperbolic systems | 19 pages. We have corrected some typographical errors and clarified a
few points | null | null | null | math.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove a multifractal formalism for Birkhoff averages of continuous
functions in the case of some non-uniformly hyperbolic maps, which includes
interval examples such as the Manneville--Pomeau map.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 09:58:08 GMT"
},
{
"version": "v2",
"created": "Tue, 23 Sep 2008 13:40:15 GMT"
}
] | 2008-09-23T00:00:00 | [
[
"Johansson",
"Anders",
""
],
[
"Jordan",
"Thomas",
""
],
[
"Öberg",
"Anders",
""
],
[
"Pollicott",
"Mark",
""
]
] | [
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] |
801.1384 | Vitaly Svetovoy | V. B. Svetovoy, P. J. van Zwol, G. Palasantzas, and J. Th. M. De
Hosson | Optical properties of gold films and the Casimir force | 18 pages, 14 figures, accepted for publication in Phys. Rev. B | Phys. Rev. B 77, 035439 (2008) | 10.1103/PhysRevB.77.035439 | null | cond-mat.other quant-ph | null | Precise optical properties of metals are very important for accurate
prediction of the Casimir force acting between two metallic plates. Therefore
we measured ellipsometrically the optical responses of Au films in a wide range
of wavelengths from 0.14 mum to 33 mum. The films at various thickness were
deposited at different conditions on silicon or mica substrates. Considerable
variation of the frequency dependent dielectric function from sample to sample
was found. Detailed analysis of the dielectric functions was performed to check
the Kramers-Kronig consistency, and extract the Drude parameters of the films.
It was found that the plasma frequency varies in the range from 6.8 eV to 8.4
eV. It is suggested that this variation is related with the film density. X-ray
reflectivity measurements support qualitatively this conclusion. The Casimir
force is evaluated for the dielectric functions corresponding to our samples,
and for that typically used in the precise prediction of the force. The force
for our films was found to be 5-14% smaller at a distance of 100 nm between the
plates. Noise in the optical data is responsible for the force variation within
1%. It is concluded that prediction of the Casimir force between metals with a
precision better than 10% must be based on the material optical response
measured from visible to mid-infrared range.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:09:24 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Svetovoy",
"V. B.",
""
],
[
"van Zwol",
"P. J.",
""
],
[
"Palasantzas",
"G.",
""
],
[
"De Hosson",
"J. Th. M.",
""
]
] | [
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] |
801.1385 | Alessandro Pastore | A. Pastore, F. Barranco, R. A. Broglia and E. Vigezzi | Microscopic calculation and LDA of the spatial dependence of the pairing
field with bare and induced interactions | null | Phys.Rev.C78:024315,2008 | 10.1103/PhysRevC.78.024315 | null | nucl-th | null | The bare nucleon-nucleon interaction is essential for the production of pair
correlations in nuclei, but an important contribution also arises from the
induced interaction resulting from the exchange of collective vibrations
between nucleons moving in time reversal states close to the Fermi energy. The
pairing field resulting from the summed interaction is strongly peaked at the
nuclear surface. It is possible to reproduce the detailed spatial dependence of
this field using a Local Density Approximation (LDA) and a contact interaction,
with parameters which are quite different from those commonly used in more
phenomenological approaches.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:11:09 GMT"
},
{
"version": "v2",
"created": "Wed, 4 Jun 2008 07:42:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Pastore",
"A.",
""
],
[
"Barranco",
"F.",
""
],
[
"Broglia",
"R. A.",
""
],
[
"Vigezzi",
"E.",
""
]
] | [
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] |
801.1386 | Ralf Blossey | Ralf Blossey, Helmut Schiessel | Kinetic proofreading of gene activation by chromatin remodeling | 8 pages, 2 Figures; application added | null | 10.2976/1.2909080 | null | q-bio.MN q-bio.BM | null | Gene activation in eukaryotes involves the concerted action of histone tail
modifiers, chromatin remodellers and transcription factors, whose precise
coordination is currently unknown. We demonstrate that the experimentally
observed interactions of the molecules are in accord with a kinetic
proofreading scheme. Our finding could provide a basis for the development of
quantitative models for gene regulation in eukaryotes based on the
combinatorical interactions of chromatin modifiers.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:13:08 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Apr 2008 15:45:17 GMT"
}
] | 2008-04-28T00:00:00 | [
[
"Blossey",
"Ralf",
""
],
[
"Schiessel",
"Helmut",
""
]
] | [
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] |
801.1387 | Abdulla Rakhimov | Abdulla Rakhimov, Chul Koo Kim, Sang-Hoon Kim, and Jae Hyung Yee | Stability of the homogeneous Bose-Einstein condensate at large gas
parameter | 9 pages, 3 figures, Revtex | null | 10.1103/PhysRevA.77.033626 | null | cond-mat.stat-mech nucl-th physics.atom-ph | null | The properties of the uniform Bose gas is studied within the optimized
variational perturbation theory (Gaussian approximation) in a self-consistent
way. It is shown that the atomic BEC with a repulsive interaction becomes
unstable when the gas parameter gamma=rho a^3 exceeds a critical value
gamma_{crit} ~ 0.01. The quantum corrections beyond the Bogoliubov-Popov
approximation to the energy density, chemical potential and pressure in powers
of gamma expansions are presented.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:23:50 GMT"
},
{
"version": "v2",
"created": "Sat, 12 Jan 2008 13:27:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rakhimov",
"Abdulla",
""
],
[
"Kim",
"Chul Koo",
""
],
[
"Kim",
"Sang-Hoon",
""
],
[
"Yee",
"Jae Hyung",
""
]
] | [
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] |
801.1388 | Arup Banerjee | Arup Banerjee and Jochen Autschbach | Time dependent density functional theory calculation of van der Waals
coefficient C$_{6}$ of alkali-metal atoms Li, Na, K, alkali dimers Li$_{2}$,
Na$_{2}$, K$_{2}$ and sodium clusters Na$_{n}$ | 14 pages of text and 4 figures | null | 10.1103/PhysRevA.78.032704 | null | physics.atm-clus physics.chem-ph | null | In this paper we employ all-electron time dependent density functional theory
(TDDFT) to calculate the long range dipole-dipole dispersion coefficient (van
der Waals coefficient) $C_{6}$ of alkali-metal atoms Li, Na, K, alkali-metal
atom dimers Li$_{2}$, Na$_{2}$, K$_{2}$ and sodium clusters containing even
number of atoms ranging from 2 to 20 atoms. The dispersion coefficients are
obtained via Casimir-Polder expression which relates it to the frequency
dependent linear polarizabilty at imaginary frequencies. The frequency
dependent polarizabilities are calculated by employing TDDFT--based complete
sum-over-states expressions for the atoms, and direct TDDFT linear response
theory for the closed shell dimers and clusters.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:26:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Banerjee",
"Arup",
""
],
[
"Autschbach",
"Jochen",
""
]
] | [
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] |
801.1389 | Tao Zhou | Tao Zhou, Xiaopu Han, and Binghong Wang | Towards the understanding of human dynamics | 28 pages, 16 figures | pp. 207-233, in M. Burguete and L. Lam (eds.), Science Matters:
Humanities as Complex Systems, World Scientific Publishing, Singapore 2008. | null | null | physics.soc-ph physics.data-an | null | Quantitative understanding of human behaviors provides elementary
comprehension of the complexity of many human-initiated systems. A basic
assumption embedded in the previous analyses on human dynamics is that its
temporal statistics are uniform and stationary, which can be properly described
by a Poisson process. Accordingly, the interevent time distribution should have
an exponential tail. However, recently, this assumption is challenged by the
extensive evidence, ranging from communication to entertainment and work
patterns, that the human dynamics obeys non-Poisson statistics with
heavy-tailed interevent time distribution. This review article summarizes the
recent empirical explorations on human activity pattern, as well as the
corresponding theoretical models for both task-driven and interest-driven
systems. Finally, we outline some future open questions in the studies of the
statistical mechanics of human dynamics.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:33:45 GMT"
}
] | 2009-07-31T00:00:00 | [
[
"Zhou",
"Tao",
""
],
[
"Han",
"Xiaopu",
""
],
[
"Wang",
"Binghong",
""
]
] | [
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] |
801.139 | Matteo Silimbani | Marilena Barnabei, Flavio Bonetti, Matteo Silimbani | The Eulerian distribution on self evacuated involutions | 18 pages | null | null | null | math.CO | null | We present an extensive study of the Eulerian distribution on the set of self
evacuated involutions, namely, involutions corresponding to standard Young
tableaux that are fixed under the Sch$\ddot{\textrm{u}}$tzenberger map. We find
some combinatorial properties for the generating polynomial of such
distribution, together with an explicit formula for its coefficients.
Afterwards, we carry out an analogous study for the subset of self evacuated
involutions without fixed points.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:39:46 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Barnabei",
"Marilena",
""
],
[
"Bonetti",
"Flavio",
""
],
[
"Silimbani",
"Matteo",
""
]
] | [
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] |
801.1391 | Kozlov Gleb Gennadievich | G. G. Kozlov | The limiting nuclear polarization in a quantum dot under optical
electron-spin orientation and applicability of the box-model of the
electron-nuclear dynamics | no figures | null | null | null | cond-mat.mes-hall | null | For the model Hamiltonian describing the electron-nuclear dynamics of a
quantum dot, we obtained an exact expression for the limiting nuclear
polarization as a function of the number of groups of equivalent nuclei. It is
shown that the refinement of the model Hamiltonian by increasing the number of
the groups results in a slow growth of the limiting nuclear polarization. This
allowed us to put forward arguments in favor of applicability of the box-model
(with all the nuclei being equivalent) for description of the electron-nuclear
spin dynamics within the time intervals of around hundreds of periods of the
optical orientation.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:43:00 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Kozlov",
"G. G.",
""
]
] | [
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801.1392 | Masatoshi Nishikawa | Masatoshi Nishikawa, Hiroaki Takagi, Atsuko H. Iwane, Toshio Yanagida | Fluctuation analysis of mechanochemical coupling depending on the type
of bio-molecular motor | null | null | 10.1103/PhysRevLett.101.128103 | null | q-bio.SC | null | Mechanochemical coupling was studied for two different types of myosin motors
in cells: myosin V, which carries cargo over long distances by as a single
molecule; and myosin II, which generates a contracting force in cooperation
with other myosin II molecules. Both mean and variance of myosin V velocity at
various [ATP] obeyed Michaelis-Menten mechanics, consistent with tight
mechanochemical coupling. Myosin II, working in an ensemble, however, was
explained by a loose coupling mechanism, generating variable step sizes
depending on the ATP concentration and realizing a much larger step (200 nm)
per ATP hydrolysis than myosin V through its cooperative nature at zero load.
These different mechanics are ideal for the respective myosin's physiological
functions.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:00:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nishikawa",
"Masatoshi",
""
],
[
"Takagi",
"Hiroaki",
""
],
[
"Iwane",
"Atsuko H.",
""
],
[
"Yanagida",
"Toshio",
""
]
] | [
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] |
801.1393 | Stefano Baroni | Dario Rocca, Ralph Gebauer, Yousef Saad, and Stefano Baroni | Turbo charging time-dependent density-functional theory with Lanczos
chains | 15 pages, 7 figures, to be pdflatex + bibtex | null | 10.1063/1.2899649 | null | cond-mat.mtrl-sci | null | We introduce a new implementation of time-dependent density-functional theory
which allows the \emph{entire} spectrum of a molecule or extended system to be
computed with a numerical effort comparable to that of a \emph{single} standard
ground-state calculation. This method is particularly well suited for large
systems and/or large basis sets, such as plane waves or real-space grids. By
using a super-operator formulation of linearized time-dependent
density-functional theory, we first represent the dynamical polarizability of
an interacting-electron system as an off-diagonal matrix element of the
resolvent of the Liouvillian super-operator. One-electron operators and density
matrices are treated using a representation borrowed from time-independent
density-functional perturbation theory, which permits to avoid the calculation
of unoccupied Kohn-Sham orbitals. The resolvent of the Liouvillian is evaluated
through a newly developed algorithm based on the non-symmetric Lanczos method.
Each step of the Lanczos recursion essentially requires twice as many
operations as a single step of the iterative diagonalization of the unperturbed
Kohn-Sham Hamiltonian. Suitable extrapolation of the Lanczos coefficients
allows for a dramatic reduction of the number of Lanczos steps necessary to
obtain well converged spectra, bringing such number down to hundreds (or a few
thousands, at worst) in typical plane-wave pseudopotential applications. The
resulting numerical workload is only a few times larger than that needed by a
ground-state Kohn-Sham calculation for a same system. Our method is
demonstrated with the calculation of the spectra of benzene, C$_{60}$
fullerene, and of chlorofyll a.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:50:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rocca",
"Dario",
""
],
[
"Gebauer",
"Ralph",
""
],
[
"Saad",
"Yousef",
""
],
[
"Baroni",
"Stefano",
""
]
] | [
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] |
801.1394 | Antonella De Pasquale Dr | A. De Pasquale, G. Costantini, P. Facchi, G. Florio, S. Pascazio, K.
Yuasa | XX model on the circle | 12 pages, 11 figures | Eur. Phys. J. Special Topics 160, 127 (2008) | 10.1140/epjst/e2008-00716-9 | null | quant-ph cond-mat.stat-mech | null | We diagonalize the XX model with a finite number of spins and periodic
boundary conditions. We solve for the ground state, focus on the rapidity of
the convergence to the thermodynamic limit and study the features of
multipartite entanglement.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:51:03 GMT"
}
] | 2012-05-28T00:00:00 | [
[
"De Pasquale",
"A.",
""
],
[
"Costantini",
"G.",
""
],
[
"Facchi",
"P.",
""
],
[
"Florio",
"G.",
""
],
[
"Pascazio",
"S.",
""
],
[
"Yuasa",
"K.",
""
]
] | [
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] |
801.1395 | Liang Tian | Liang Tian and Da-Ning Shi | Scaling of disordered recursive networks | 5 pages, 5 figures | null | 10.1209/0295-5075/84/58001 | null | cond-mat.dis-nn | null | In this brief report, we present a disordered version of recursive networks.
Depending on the structural parameters $u$ and $v$, the networks are either
fractals with a finite fractal dimension $d_{f}$ or transfinite fractals
(transfractal) with a infinite fractal dimension. The scaling behavior of
degree and dimensionality are studied analytically and by simulations, which
are found to be different from those in ordered recursive networks. The
transfractal dimension $\tilde{d}_f$, which is recently introduced to
distinguish the differences between networks with infinite fractal dimension,
scales as $\tilde{d}_f\sim \frac{1}{u+v-1}$ for transfractal networks.
Interestingly, the fractal dimension for fractal networks with $u=v$ is found
to approach 3 in large limit of $u$, which is thought to be the effect of
disorder. We also investigate the diffusion process on this family of networks,
and the scaling behavior of diffusion time is observed numercally as $\tau\sim
N^{(d_{f}+1)/d_{f}}$ for fractal networks and $\tau\sim \frac{1}{\tilde{d}_f}N$
for transfractal ons. We think that the later relation will give a further
understanding of transfractal dimension.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:57:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tian",
"Liang",
""
],
[
"Shi",
"Da-Ning",
""
]
] | [
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] |
801.1396 | Claire Voisin | Claire Voisin (IMJ, Ihes) | Rationally connected $3$-folds and symplectic geometry | New final version. The statement is improved, thanks to the help of
Jason Starr. Indeed, the result holds now for general syplectic equivalence,
and not the restricted notion of symplectic equivalence we used before | null | null | null | math.AG math.SG | null | We study the following question, asked to us By Pandharipande and Starr: Let
$X$ be a rationally connected $3$-fold, and $Y$ be a compact Kaehler $3$-fold
symplectically equivalent to it. Is $Y$ rationally connected? We show that the
answer is positive if $X$ is Fano or $b_2(X)\leq2$.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:58:36 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 08:06:42 GMT"
},
{
"version": "v3",
"created": "Sat, 2 Feb 2008 10:28:18 GMT"
},
{
"version": "v4",
"created": "Thu, 21 Feb 2008 11:01:20 GMT"
},
{
"version": "v5",
"created": "Thu, 27 Mar 2008 07:56:52 GMT"
}
] | 2008-03-27T00:00:00 | [
[
"Voisin",
"Claire",
"",
"IMJ, Ihes"
]
] | [
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] |
801.1397 | Martin Lind\'en | Martin Lind\'en | Decay times in turnover statistics of single enzymes | 4 pages, 1 figure v2: Published version, minor corrections in
response to referee comments | Phys. Rev. E 78, 010901(R), 2008 | 10.1103/PhysRevE.78.010901 | null | physics.bio-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The first passage times for enzymatic turnovers in non-equilibrium steady
state display a statistical symmetry property related to non-equilibrium
fluctuation theorems, that makes it possible to extract the chemical driving
force from single molecule trajectories in non-equilibrium steady state. Below,
we show that this system violates the general expectation that the number of
decay constants needed to fit a first passage time distribution reflects the
number of states in the escape problem. In fact, the structure of the kinetic
mechanism makes half of the decay times vanish identically from the turnover
time distribution. The terms that cancel out correspond to the eigenvalues of a
certain sub-matrix of the master equation matrix for the first exit time
problem. We discuss how these results make modeling and data analysis easier
for such systems, and how the turnovers can be measured.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:07:30 GMT"
},
{
"version": "v2",
"created": "Wed, 10 Dec 2008 17:13:24 GMT"
}
] | 2008-12-10T00:00:00 | [
[
"Lindén",
"Martin",
""
]
] | [
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801.1398 | Hamid Reza Sepangi | K. Atazadeh, M. Farhoudi and H. R. Sepangi | Accelerating universe in $f({\cal R})$ brane gravity | 9 pages, 1 figure, to appear in PLB | Phys.Lett.B660:275-281,2008 | 10.1016/j.physletb.2007.12.057 | null | gr-qc astro-ph hep-th | null | We study a 5-dimensional $f({\cal R})$ brane gravity within the framework of
scalar-tensor type theories. We show that such a model predicts, for a certain
choice of $f({\cal R})$ and a spatially flat universe, an exponential
potential, leading to an accelerated expanding universe driven solely by the
curvature of the bulk space. This result is consistent with the observational
data in the cosmological scale.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:09:47 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Atazadeh",
"K.",
""
],
[
"Farhoudi",
"M.",
""
],
[
"Sepangi",
"H. R.",
""
]
] | [
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] |
801.1399 | Jan Lorenz | Jan Lorenz | Heterogeneous bounds of confidence: Meet, Discuss and Find Consensus! | 14 pages, 12 figures, large parts rewritten and improved | Complexity (2010), 15(4), 43-52 | 10.1002/cplx.20295 | null | physics.soc-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Models of continuous opinion dynamics under bounded confidence show a sharp
transition between a consensus and a polarization phase at a critical global
bound of confidence. In this paper, heterogeneous bounds of confidence are
studied. The surprising result is that a society of agents with two different
bounds of confidence (open-minded and closed-minded agents) can find consensus
even when both bounds of confidence are significantly below the critical bound
of confidence of a homogeneous society.
The phenomenon is shown by examples of agent-based simulation and by
numerical computation of the time evolution of the agents density. The result
holds for the bounded confidence model of Deffuant, Weisbuch and others
(Weisbuch, G. et al; Meet, discuss, and segregate!, Complexity, 2002, 7,
55--63), as well as for the model of Hegselmann and Krause (Hegselmann, R.,
Krause, U.; Opinion Dynamics and Bounded Confidence, Models, Analysis and
Simulation, Journal of Artificial Societies and Social Simulation, 2002, 5, 2).
Thus, given an average level of confidence, diversity of bounds of confidence
enhances the chances for consensus. The drawback of this enhancement is that
opinion dynamics becomes suspect to severe drifts of clusters, where
open-minded agents can pull closed-minded agents towards another cluster of
closed-minded agents. A final consensus might thus not lie in the center of the
opinion interval as it happens for uniform initial opinion distributions under
homogeneous bounds of confidence. It can be located at extremal locations. This
is demonstrated by example.
This also show that the extension to heterogeneous bounds of confidence
enriches the complexity of the dynamics tremendously.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:10:38 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Aug 2009 11:17:39 GMT"
}
] | 2010-12-07T00:00:00 | [
[
"Lorenz",
"Jan",
""
]
] | [
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801.14 | Ping Wang | Zhe Chang and Ping Wang | Topology Changes and Quantum Phase Transition in Spin-Chain System | 5 pages | null | null | null | quant-ph | null | The standard Landau-Ginzburg scenario of phase transition is broken down for
quantum phase transition. It is difficult to find an order parameter to
indicate different phases for quantum fluctuations. Here, we suggest a
topological description of the quantum phase transition for the XY model. The
ground states are identified as a specialized U(1) principal bundle on the base
manifold $S^2$. And then different first Chern numbers of U(1) principal bundle
on the base manifold $S^2$ are associated to each phase of quantum
fluctuations. The particle-hole picture is used to parameterized the ground
states of the XY system. We show that a singularity of the Chern number of the
ground states occurs simultaneously with a quantum phase transition. The Chern
number is a suitable topological order of the quantum phase transition.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:16:12 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Chang",
"Zhe",
""
],
[
"Wang",
"Ping",
""
]
] | [
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] |
801.1401 | Saumyadip Samui | Saumyadip Samui, Kandaswamy Subramanian, Raghunathan Srianand | Constrained semi-analytical models of Galactic outflows | 27 pages, 31 figures, 2 tables, pdflatex. Accepted for publication in
MNRAS | null | 10.1111/j.1365-2966.2008.12932.x | null | astro-ph | null | We present semi-analytic models of galactic outflows, constrained by
available observations on high redshift star formation and reionization.
Galactic outflows are modeled in a manner akin to models of stellar wind blown
bubbles. Large scale outflows can generically escape from low mass halos
(M<10^9 M_sun) for a wide range of model parameters but not from high mass
halos (M> 10^{11} M_sun). The gas phase metallicity of the outflow and within
the galaxy are computed. Ionization states of different metal species are
calculated and used to examine the detectability of metal lines from the
outflows. The global influence of galactic outflows is also investigated.
Models with only atomic cooled halos significantly fill the IGM at z~3 with
metals (with -2.5>[Z/Z_sun]>-3.7), the actual extent depending on the
efficiency of winds, the IMF, the fractional mass that goes through star
formation and the reionization history of the universe. In these models, a
large fraction of outflows at z~3 are supersonic, hot (T> 10^5 K) and have low
density, making metal lines difficult to detect. They may also result in
significant perturbations in the IGM gas on scales probed by the Lyman-alpha
forest. On the contrary, models including molecular cooled halos with a normal
mode of star formation can potentially volume fill the universe at z> 8 without
drastic dynamic effects on the IGM, thereby setting up a possible metallicity
floor (-4.0<[Z/Z_sun]<-3.6). Interestingly, molecular cooled halos with a
``top-heavy'' mode of star formation are not very successful in establishing
the metallicity floor because of the additional radiative feedback, that they
induce. (Abridged)
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:48:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Samui",
"Saumyadip",
""
],
[
"Subramanian",
"Kandaswamy",
""
],
[
"Srianand",
"Raghunathan",
""
]
] | [
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] |
801.1402 | Hideaki Mouri | H. Mouri, A. Hori, M. Takaoka | Fluctuations of statistics among subregions of a turbulence velocity
field | 7 pages, accepted by Physics of Fluids (see http://pof.aip.org/) | PoF, 20, 035108 [2008] | 10.1063/1.2890499 | null | physics.flu-dyn | null | To study subregions of a turbulence velocity field, a long record of velocity
data of grid turbulence is divided into smaller segments. For each segment, we
calculate statistics such as the mean rate of energy dissipation and the mean
energy at each scale. Their values significantly fluctuate, in lognormal
distributions at least as a good approximation. Each segment is not under
equilibrium between the mean rate of energy dissipation and the mean rate of
energy transfer that determines the mean energy. These two rates still
correlate among segments when their length exceeds the correlation length. Also
between the mean rate of energy dissipation and the mean total energy, there is
a correlation characterized by the Reynolds number for the whole record,
implying that the large-scale flow affects each of the segments.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:19:15 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Mar 2008 09:21:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mouri",
"H.",
""
],
[
"Hori",
"A.",
""
],
[
"Takaoka",
"M.",
""
]
] | [
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] |
801.1403 | Salvatore Orlando | S. Orlando, F. Bocchino, F. Reale, G. Peres, P. Pagano | The importance of magnetic-field-oriented thermal conduction in the
interaction of SNR shocks with interstellar clouds | 14 pages, 7 Figures; paper accepted for publication in ApJ; the paper
with high-resolution figures can be downloaded at
http://www.astropa.unipa.it/~orlando/PAPERS/sorlando_clmhd.pdf | null | 10.1086/529420 | null | astro-ph | null | We explore the importance of magnetic-field-oriented thermal conduction in
the interaction of supernova remnant (SNR) shocks with radiative gas clouds and
in determining the mass and energy exchange between the clouds and the hot
surrounding medium. We perform 2.5D MHD simulations of a shock impacting on an
isolated gas cloud, including anisotropic thermal conduction and radiative
cooling; we consider the representative case of a Mach 50 shock impacting on a
cloud ten-fold denser than the ambient medium. We consider different
configurations of the ambient magnetic field and compare MHD models with or
without the thermal conduction. The efficiency of the thermal conduction in the
presence of magnetic field is, in general, reduced with respect to the
unmagnetized case. The reduction factor strongly depends on the initial
magnetic field orientation, and it is minimum when the magnetic field is
initially aligned with the direction of shock propagation. The thermal
conduction contributes to suppress hydrodynamic instabilities, reducing the
mass mixing of the cloud and preserving the cloud from complete fragmentation.
Depending on the magnetic field orientation, the heat conduction may determine
a significant energy exchange between the cloud and the hot surrounding medium
which, while remaining always at levels less than those in the unmagnetized
case, leads to a progressive heating and evaporation of the cloud. This
additional heating may contrast the radiative cooling of some parts of the
cloud, preventing the onset of thermal instabilities.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:19:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Orlando",
"S.",
""
],
[
"Bocchino",
"F.",
""
],
[
"Reale",
"F.",
""
],
[
"Peres",
"G.",
""
],
[
"Pagano",
"P.",
""
]
] | [
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0.0904469937,
0.0343359075,
-0.0029461957,
-0.0238969196,
-0.0356453285,
-0.0449810103
] |
801.1404 | Takeshi Okuda | T. Okuda, S. Iguchi | Performance Measurements of 8-Gsps 1-bit ADCs Developed for Wideband
Radio Astronomical Observations | Accepted for publication in PASJ. 19 pages, 15 figures | null | 10.1093/pasj/60.2.315 | null | astro-ph | null | 8-Gsps 1-bit Analog-to-Digital Converters (ADCs) were newly developed toward
the realization of the wideband observation. The development of the wideband
ADCs is one of the most essential developments for the radio interferometer. To
evaluate its performance in interferometric observations, the time (phase)
stability and frequency response were measured with a noise source and a signal
generator. The results of these measurements show that the developed ADCs can
achieve the jitter time less than 0.05 psec at the time interval of 1 sec, the
passband frequency response with the slope less than 0.73 dB/GHz and the ripple
less than 1.8 dB, and the aperture time less than 20 psec. The details of the
developed ADC design, the measurement methods, and the results of these
measurements are presented in this paper.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 11:19:57 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Okuda",
"T.",
""
],
[
"Iguchi",
"S.",
""
]
] | [
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801.1405 | Sung Myung | Sung Myung | On multilinearity and skew-symmetry of certain symbols in motivic
cohomology of fields | We acknowledge that mutilinearity does not hold for arbitrary symbols
in H^{l-1} (Spec k, Z(l)) as claimed in the 1st version and this mistake has
been corrected in the 2nd version | Math. Res. Lett. 16 (2009): 303-322 | null | null | math.KT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The purpose of the present article is to show the multilinearity for symbols
in Goodwillie-Lichtenbaum complex in two cases.
The first case shown is where the degree is equal to the weight. In this
case, the motivic cohomology groups of a field are isomorphic to the Milnor's
K-groups as shown by Nesterenko-Suslin, Totaro and Suslin-Voevodsky for various
motivic complexes, but we give an explicit isomorphism for
Goodwillie-Lichtenbaum complex in a form which visibly carries multilinearity
of Milnor's symbols to our multilinearity of motivic symbols. Next, we
establish multilinearity and skew-symmetry for irreducible
Goodwillie-Lichtenbaum symbols in H^{l-1} (Spec k, Z(l)). These properties have
been expected to hold from the author's construction of a bilinear form of
dilogarithm in case k is a subfield of the field of complex numbers and l=2.
Next, we establish multilinearity and skew-symmetry for
Goodwillie-Lichtenbaum symbols in H^{l-1} (Spec k, Z(l)). These properties have
been expected to hold from the author's construction of a bilinear form of
dilogarithm in case k is a subfield of the field of complex numbers and l=2.
The multilinearity of symbols may be viewed as a generalization of the
well-known formula det(AB) = det(A) det(B) for tuples of commuting matrices.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:07:45 GMT"
},
{
"version": "v2",
"created": "Mon, 15 Sep 2008 09:03:22 GMT"
}
] | 2009-05-15T00:00:00 | [
[
"Myung",
"Sung",
""
]
] | [
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801.1406 | Nikolai Voshchinnikov | N.V. Voshchinnikov, H.K. Das | Modelling interstellar extinction and polarization with spheroidal
grains | 13 pages, 9 figures, aacepted for publication in Journal of
Quantitative Spectroscopy & Radiative Transfer (special issue, X Conference
on Electromagnetic & Light Scattering) | null | 10.1016/j.jqsrt.2008.01.003 | null | astro-ph | null | We calculate the wavelength dependence of the ratio of the linear
polarization degree to extinction (polarizing efficiency)
$P(\lambda)/A(\lambda)$ from the ultraviolet to near-infrared. The prolate and
oblate particles with aspect ratios from $a/b=1.1$ up to 10 are assumed to be
rotating and partially aligned with the mechanism of paramagnetic relaxation
(Davis--Greenstein). Size/shape/orientation effects are analyzed. It is found
that the wavelength dependence of $P(\lambda)/A(\lambda)$ is mainly determined
by the particle composition and size whereas the values of
$P(\lambda)/A(\lambda)$ depend on the particle shape, degree and direction of
alignment.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:33:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Voshchinnikov",
"N. V.",
""
],
[
"Das",
"H. K.",
""
]
] | [
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] |
801.1407 | Chunshan Lin | Miao Li, Chunshan Lin, Yi Wang | Some Issues Concerning Holographic Dark Energy | 19 pages, 6 figures. final version published in JCAP | JCAP 0805:023,2008 | 10.1088/1475-7516/2008/05/023 | USTC-ICTS-0726 | astro-ph gr-qc hep-th | null | We study perturbation of holographic dark energy and find it be stable. We
study the fate of the universe when interacting holographic dark energy is
present, and discuss a simple phenomenological classification of the
interacting holographic dark energy models. We also discuss the cosmic
coincidence problem in the context of holographic dark energy. We find that the
coincidence problem can not be completely solved by adding an interacting term.
Inflation may provide a better solution of the coincidence problem.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:06:06 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jan 2008 05:32:30 GMT"
},
{
"version": "v3",
"created": "Thu, 29 May 2008 02:05:20 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Li",
"Miao",
""
],
[
"Lin",
"Chunshan",
""
],
[
"Wang",
"Yi",
""
]
] | [
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] |
801.1408 | Michael Duetsch | Ferdinand Brennecke and Michael Duetsch | The Quantum Action Principle in the framework of Causal Perturbation
Theory | 20 pages. Contribution to the Conference on 'Recent Developments in
Quantum Field Theory' held from July 20 to July 22, 2007 at the Max Planck
Institute for Mathematics in the Sciences, Leipzig/Germany | null | 10.1007/978-3-7643-8736-5_11 | null | hep-th | null | In perturbative quantum field theory the maintenance of classical symmetries
is quite often investigated by means of algebraic renormalization, which is
based on the Quantum Action Principle. We formulate and prove this principle in
a new framework, in causal perturbation theory with localized interactions.
Throughout this work a universal formulation of symmetries is used: the Master
Ward Identity.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:06:39 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Brennecke",
"Ferdinand",
""
],
[
"Duetsch",
"Michael",
""
]
] | [
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] |
801.1409 | Arnaud Bodin | Arnaud Bodin | Integral points on generic fibers | 12 pages | null | 10.1112/jlms/jdp084 | null | math.AG math.NT | null | Let P(x,y) be a rational polynomial and k in Q be a generic value. If the
curve (P(x,y)=k) is irreducible and admits an infinite number of points whose
coordinates are integers then there exist algebraic automorphisms that send
P(x,y) to the polynomial x or to x^2-dy^2. Moreover for such curves (and
others) we give a sharp bound for the number of integral points (x,y) with x
and y bounded.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:23:25 GMT"
}
] | 2014-02-26T00:00:00 | [
[
"Bodin",
"Arnaud",
""
]
] | [
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-0.104846932,
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] |
801.141 | Shmuel Onn | Shmuel Onn | Two graph isomorphism polytopes | null | Discrete Mathematics, 309:2934--2936, 2009 | null | null | cs.CC cs.DM math.CO math.OC | null | The convex hull $\psi_{n,n}$ of certain $(n!)^2$ tensors was considered
recently in connection with graph isomorphism. We consider the convex hull
$\psi_n$ of the $n!$ diagonals among these tensors. We show: 1. The polytope
$\psi_n$ is a face of $\psi_{n,n}$. 2. Deciding if a graph $G$ has a subgraph
isomorphic to $H$ reduces to optimization over $\psi_n$. 3. Optimization over
$\psi_n$ reduces to optimization over $\psi_{n,n}$. In particular, this implies
that the subgraph isomorphism problem reduces to optimization over
$\psi_{n,n}$.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:34:26 GMT"
},
{
"version": "v2",
"created": "Sat, 12 Jan 2008 11:25:35 GMT"
}
] | 2009-08-22T00:00:00 | [
[
"Onn",
"Shmuel",
""
]
] | [
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] |
801.1411 | Ramazan Sever | Ramazan Sever, Cevdet Tezcan, Ozlem Yesiltas, Mahmut Bucurgat | Exact solution of Effective mass Schrodinger Equation for the Hulthen
potential | 9 pages | Int. J. Theo. Phys. 47, 2243(2008) | 10.1007/s10773-008-9656-7 | null | quant-ph | null | A general form of the effective mass Schrodinger equation is solved exactly
for Hulthen potential. Nikiforov-Uvarov method is used to obtain energy
eigenvalues and the corresponding wave functions. A free parameter is used in
the transformation of the wave function.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:24:15 GMT"
}
] | 2010-05-04T00:00:00 | [
[
"Sever",
"Ramazan",
""
],
[
"Tezcan",
"Cevdet",
""
],
[
"Yesiltas",
"Ozlem",
""
],
[
"Bucurgat",
"Mahmut",
""
]
] | [
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-0.0049468102,
0.0290337242,
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-0.0523773059,
0.030106457,
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-0.1331120431,
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] |
801.1412 | Peter Akhmetiev | Petr M. Akhmet'ev | Geometric approach towards stable homotopy groups of spheres. The
Steenrod-Hopf invariant I | null | null | null | null | math.GT math.AT | null | In this paper a geometric approach toward stable homotopy groups of spheres,
based on the Pontrjagin-Thom construction is proposed. From this approach a new
proof of Hopf Invariant One Theorem by J.F.Adams for all dimensions except
$15,31,63,127$ is obtained.
It is proved that for $n>127$ in the stable homotopy group of spheres $\Pi_n$
there is no elements with Hopf invariant one. The new proof is based on
geometric topology methods. The Pontrjagin-Thom Theorem (in the form proposed
by R.Wells) about the representation of stable homotopy groups of the real
projective infinite-dimensional space (this groups is mapped onto 2-components
of stable homotopy groups of spheres by the Khan-Priddy Theorem) by cobordism
classes of immersions of codimension 1 of closed manifolds (generally speaking,
non-orientable) is considered. The Hopf Invariant is expressed as a
characteristic number of the dihedral group for the self-intersection manifold
of an immersed codimension 1 manifold that represents the given element in the
stable homotopy group. In the new proof the Geometric Control Principle (by
M.Gromov) for immersions in a given regular homotopy classes based on
Smale-Hirsch Immersion Theorem is required.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:26:26 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Akhmet'ev",
"Petr M.",
""
]
] | [
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] |
801.1413 | Andrij Rovenchak | Andrij Rovenchak | Fractional statistics and finite bosonic system: A one-dimensional case | 10 pages | Fiz. Nizk. Temp. 35, No. 5, 510-513 (2009); Low Temp. Phys. 35,
400-403 (2009) | 10.1063/1.3132748 | null | math-ph math.MP | null | The equivalence is established between the one-dimensional (1D) Bose-system
with a finite number of particles and the system obeying the fractional
(intermediate) Gentile statistics, in which the maximum occupation of
single-particle energy levels is limited. The system of 1D harmonic oscillators
is considered providing the model of harmonically trapped Bose-gas. The results
are generalized for the system with power energy spectrum.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:28:07 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Rovenchak",
"Andrij",
""
]
] | [
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] |
801.1414 | Giuliano Benenti | Giuseppe Gennaro, Giuliano Benenti, Massimo Palma | Entanglement dynamics and relaxation in a few qubit system interacting
with random collisions | 5 pages, 4 figures | Europhys. Lett. 82, 20006 (2008) | 10.1209/0295-5075/82/20006 | null | quant-ph | null | The dynamics of a single qubit interacting by a sequence of pairwise
collisions with an environment consisting of just two more qubits is analyzed.
Each collision is modeled in terms of a random unitary operator with a uniform
probability distribution described by the uniform Haar measure. We show that
the purity of the system qubit as well as the bipartite and the tripartite
entanglement reach time averaged equilibrium values characterized by large
instantaneous fluctuations.These equilibrium values are independent of the
order of collision among the qubits. The relaxation to equilibrium is analyzed
also in terms of an ensemble average of random collision histories. Such
average allows for a quantitative evaluation and interpretation of the decay
constants. Furthermore a dependence of the transient dynamics on the initial
degree of entanglement between the environment qubits is shown to exist.
Finally the statistical properties of bipartite and tripartite entanglement are
analyzed.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:29:23 GMT"
}
] | 2008-04-16T00:00:00 | [
[
"Gennaro",
"Giuseppe",
""
],
[
"Benenti",
"Giuliano",
""
],
[
"Palma",
"Massimo",
""
]
] | [
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801.1415 | Dietrich Stauffer | S. Wichmann | The emerging field of language dynamics | null | null | null | null | cs.CL physics.soc-ph | null | A simple review by a linguist, citing many articles by physicists:
Quantitative methods, agent-based computer simulations, language dynamics,
language typology, historical linguistics
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:34:40 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Wichmann",
"S.",
""
]
] | [
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] |
801.1416 | Piyush Kurur | Anindya De, Piyush P Kurur, Chandan Saha and Ramprasad Saptharishi | Fast Integer Multiplication using Modular Arithmetic | fixed some typos and references | null | null | null | cs.SC cs.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give an $O(N\cdot \log N\cdot 2^{O(\log^*N)})$ algorithm for multiplying
two $N$-bit integers that improves the $O(N\cdot \log N\cdot \log\log N)$
algorithm by Sch\"{o}nhage-Strassen. Both these algorithms use modular
arithmetic. Recently, F\"{u}rer gave an $O(N\cdot \log N\cdot 2^{O(\log^*N)})$
algorithm which however uses arithmetic over complex numbers as opposed to
modular arithmetic. In this paper, we use multivariate polynomial
multiplication along with ideas from F\"{u}rer's algorithm to achieve this
improvement in the modular setting. Our algorithm can also be viewed as a
$p$-adic version of F\"{u}rer's algorithm. Thus, we show that the two seemingly
different approaches to integer multiplication, modular and complex arithmetic,
are similar.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:44:55 GMT"
},
{
"version": "v2",
"created": "Tue, 6 May 2008 07:05:09 GMT"
},
{
"version": "v3",
"created": "Fri, 19 Sep 2008 06:45:16 GMT"
}
] | 2008-09-19T00:00:00 | [
[
"De",
"Anindya",
""
],
[
"Kurur",
"Piyush P",
""
],
[
"Saha",
"Chandan",
""
],
[
"Saptharishi",
"Ramprasad",
""
]
] | [
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] |
801.1417 | Peter Akhmetiev | Petr M. Akhmet'ev | Geometric approach towards stable homotopy groups of spheres. The
Kervaire invariant II | null | null | null | null | math.GT math.AT | null | The notion of the geometrical $\Z/2 \oplus \Z/2$--control of
self-intersection of a skew-framed immersion and the notion of the $\Z/2 \oplus
\Z/4$-structure (the cyclic structure) on the self-intersection manifold of a
$\D_4$-framed immersion are introduced. It is shown that a skew-framed
immersion $f:M^{\frac{3n+q}{4}} \looparrowright \R^n$, $0 < q <<n$ (in the
$\frac{3n}{4}+\epsilon$-range) admits a geometrical $\Z/2 \oplus \Z/2$--control
if the characteristic class of the skew-framing of this immersion admits a
retraction of the order $q$, i.e. there exists a mapping $\kappa_0:
M^{\frac{3n+q}{4}} \to \RP^{\frac{3(n-q)}{4}}$, such that this composition $I
\circ \kappa_0: M^{\frac{3n+q}{4}} \to \RP^{\frac{3(n-q)}{4}} \to \RP^{\infty}$
is the characteristic class of the skew-framing of $f$. Using the notion of
$\Z/2 \oplus \Z/2$-control we prove that for a sufficiently great $n$,
$n=2^l-2$, an arbitrary immersed $\D_4$-framed manifold admits in the regular
cobordism class (modulo odd torsion) an immersion with a $\Z/2 \oplus
\Z/4$-structure. In the last section we present an approach toward the Kervaire
Invariant One Problem.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:35:28 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Akhmet'ev",
"Petr M.",
""
]
] | [
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] |
801.1418 | Stefan Wewers | Irene I. Bouw, Stefan Wewers, Leonardo Zapponi | Deformation data, Belyi maps, and the local lifting problem | null | null | null | null | math.NT math.AG | null | We prove existence and nonexistence results for certain differential forms in
positive characteristic, called {\em good deformation data}. Some of these
results are obtained by reduction modulo $p$ of Belyi maps. As an application,
we solve the local lifting problem for groups with Sylow $p$-subgroup of order
$p$.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:41:07 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Bouw",
"Irene I.",
""
],
[
"Wewers",
"Stefan",
""
],
[
"Zapponi",
"Leonardo",
""
]
] | [
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] |
801.1419 | Vincent Gramoli | Vincent Gramoli (IRISA), Anne-Marie Kermarrec (IRISA), Achour
Mostefaoui (IRISA), Michel Raynal (IRISA), Bruno Sericola (IRISA) | Core Persistence in Peer-to-Peer Systems: Relating Size to Lifetime | null | Dans Proceedings of the Workshop on Reliability in Decentralized
Distributed Systems 4278 (2006) 1470--1479 | null | null | cs.DC | null | Distributed systems are now both very large and highly dynamic. Peer to peer
overlay networks have been proved efficient to cope with this new deal that
traditional approaches can no longer accommodate. While the challenge of
organizing peers in an overlay network has generated a lot of interest leading
to a large number of solutions, maintaining critical data in such a network
remains an open issue. In this paper, we are interested in defining the portion
of nodes and frequency one has to probe, given the churn observed in the
system, in order to achieve a given probability of maintaining the persistence
of some critical data. More specifically, we provide a clear result relating
the size and the frequency of the probing set along with its proof as well as
an analysis of the way of leveraging such an information in a large scale
dynamic distributed system.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:41:15 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Gramoli",
"Vincent",
"",
"IRISA"
],
[
"Kermarrec",
"Anne-Marie",
"",
"IRISA"
],
[
"Mostefaoui",
"Achour",
"",
"IRISA"
],
[
"Raynal",
"Michel",
"",
"IRISA"
],
[
"Sericola",
"Bruno",
"",
"IRISA"
]
] | [
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] |
801.142 | Przemyslaw Piekarz | P. Piekarz, K. Parlinski, and A. M. Oles | Order parameters in the Verwey phase transition | 4 pages, 1 figure | Journal of Physics: Conference Series 92 (2007) 012164 | 10.1088/1742-6596/92/1/012164 | null | cond-mat.stat-mech cond-mat.str-el | null | The Verwey phase transition in magnetite is analyzed on the basis of the
Landau theory. The free energy functional is expanded in a series of components
belonging to the primary and secondary order parameters. A low-temperature
phase with the monoclinic P2/c symmetry is a result of condensation of two
order parameters X_3 and \Delta_5 . The temperature dependence of the shear
elastic constant C_44 is derived and the mechanism of its softening is
discussed.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:45:58 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Piekarz",
"P.",
""
],
[
"Parlinski",
"K.",
""
],
[
"Oles",
"A. M.",
""
]
] | [
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] |
801.1421 | Sergei Popov B. | S.B. Popov (Sternberg Astronomical Institute) | Soft gamma repeaters activity in time | 5 pages, no figures | Astron.Nachr.329:15-19,2008 | 10.1002/asna.200710851 | null | astro-ph | null | In this short note I discuss the hypothesis that bursting activity of
magnetars evolves in time analogously to the glitching activity of normal radio
pulsars (i.e. sources are more active at smaller ages), and that the increase
of the burst rate follows one of the laws established for glitching radio
pulsars. If the activity of soft gamma repeaters decreases in time in the way
similar to the evolution of core-quake glitches ($\propto t^{5/2}$), then it is
more probable to find the youngest soft gamma repeaters, but the energy of
giant flares from these sources should be smaller than observed $10^{44}$
--$10^{46}$ ergs as the total energy stored in a magnetar's magnetic field is
not enough to support thousands of bursts similar to the prototype 5 March 1979
flare.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:46:14 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Popov",
"S. B.",
"",
"Sternberg Astronomical Institute"
]
] | [
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] |
801.1422 | Sebastian Wolf | S. Wolf, A. Schegerer, H. Beuther, D.L. Padgett, K.R. Stapelfeldt | Submillimeter Structure of the Disk of the Butterfly Star | 6 pages, emulatepaj, Accepted to ApJL | null | 10.1086/529188 | null | astro-ph | null | We present a spatially resolved 894 micron map of the circumstellar disk of
the Butterfly star in Taurus (IRAS 04302+2247), obtained with the Submillimeter
Array (SMA). The predicted and observed radial brightness profile agree well in
the outer disk region, but differ in the inner region with an outer radius of
~80-120 AU. In particular, we find a local minimum of the radial brightness
distribution at the center, which can be explained by an increasing density /
optical depth combined with the decreasing vertical extent of the disk towards
the center. Our finding indicates that young circumstellar disks can be
optically thick at wavelengths as long as 894 micron. While earlier modeling
lead to general conclusions about the global disk structure and, most
importantly, evidence for grain growth in the disk (Wolf, Padgett, &
Stapelfeldt 2003), the presented SMA observations provide more detailed
constraints for the disk structure and dust grain properties in the inner,
potentially planet-forming region (inside ~80-120 AU) vs. the outer disk region
(~120-300 AU).
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 12:55:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wolf",
"S.",
""
],
[
"Schegerer",
"A.",
""
],
[
"Beuther",
"H.",
""
],
[
"Padgett",
"D. L.",
""
],
[
"Stapelfeldt",
"K. R.",
""
]
] | [
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] |
801.1423 | Felix Finster | Felix Finster, Niky Kamran, Joel Smoller and Shing-Tung Yau | Linear Waves in the Kerr Geometry: A Mathematical Voyage to Black Hole
Physics | 25 pages, LaTeX, 2 figures, minor changes (published version) | Bull. Amer. Math. Soc. 46 (2009) 635-659 | 10.1090/S0273-0979-09-01258-0 | null | math-ph gr-qc math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper gives a survey of wave dynamics in the Kerr space-time geometry,
the mathematical model of a rotating black hole in equilibrium. After a brief
introduction to the Kerr metric, we review the separability properties of
linear wave equations for fields of general spin $s=0, 1/2, 1, 2$,
corresponding to scalar, Dirac, electromagnetic fields and linearized
gravitational waves. We give results on the long-time dynamics of Dirac and
scalar waves, including decay rates for massive Dirac fields. For scalar waves,
we give a rigorous treatment of superradiance and describe rigorously a
mechanism of energy extraction from a rotating black hole. Finally, we discuss
the open problem of linear stability of the Kerr metric and present partial
results.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:56:44 GMT"
},
{
"version": "v2",
"created": "Mon, 4 Feb 2008 08:27:37 GMT"
},
{
"version": "v3",
"created": "Wed, 22 Apr 2009 15:37:09 GMT"
},
{
"version": "v4",
"created": "Sat, 25 Jul 2009 06:22:25 GMT"
}
] | 2009-07-25T00:00:00 | [
[
"Finster",
"Felix",
""
],
[
"Kamran",
"Niky",
""
],
[
"Smoller",
"Joel",
""
],
[
"Yau",
"Shing-Tung",
""
]
] | [
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] |
801.1424 | Arup Banerjee | Arup Banerjee and Manoj K. Harbola | Comparison of van der Waals coefficient C$_{6}$ of sodium clusters
obtained via spherical jellium background model and all-electron ab-initio
method | 15 pages including 2 figures. To be published in Journal of
Computational Methods in Science and Engineering | null | null | null | physics.atm-clus physics.chem-ph | null | In this paper we employ two distinct approaches - all-electron \textit{ab
initio} method and the spherical jellium background model- within time
dependent density functional theory to calculate the long range dipole-dipole
dispersion coefficient (van der Waals coefficient) $C_{6}$ of sodium atom
clusters containing even number of atoms ranging from 2 to 20 atoms. The
dispersion coefficients are obtained via Casimir-Polder relation. All the
calculations are carried out with local density approximation for
exchange-correlation energy functional. These two sets of results are compared
to assess the accuracy of jellium based results and to ascertain the effect of
detail ionic structure of the clusters on the van der Waals coefficient.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:17:50 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Banerjee",
"Arup",
""
],
[
"Harbola",
"Manoj K.",
""
]
] | [
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] |
801.1425 | Sergey Kiselev | S. M. Kiselev | Direct Photons in Nuclear Collisions at FAIR Energies | 9 pages, 5 figures, Talk at the session of Russian Academy of
Sciences, ITEP, Moscow, 26 - 30 November 2007 | null | 10.1134/S1063778809030168 | null | hep-ph | null | Using the extrapolation of existing data estimations of prompt photon
production at FAIR energies have been made. At $y=y_{c.m.}$ the rapidity
density of prompt photons with $p_{t}>$ 1.5 GeV/c per central Au+Au event at 25
AGeV is estimated as $\sim 10^{-4}$ . With the planed beam intensity $10^{9}$
per second and 1% interaction probability, for 10% of most central events one
can expect the prompt photon rate $\sim 10^{2}$ photons per second.
Direct photons from the hadron scenario of ion collisions generated by the
Hadron-String-Dynamics (HSD) transport approach with implemented meson
scatterings $\pi\rho\to\pi\gamma, \pi\pi\to\rho\gamma$ have been analyzed.
Photons from short-living resonances (e.g. $\omega \to \pi^{0} \gamma$)
decaying during the dense phase of the collision should be considered as direct
photons. They contribute significantly in the direct photon spectrum at
$p_{t}=0.5 - 1$ GeV/c. At the FAIR energy 25 AGeV in Au+Au central collisions
the HSD generator predicts, as a lower estimate,
$\gamma_{direct}/\gamma_{\pi^{0}} \simeq$ 0.5% in the region $p_{t}=0.5 - 1$
GeV/c. At $p_{t}=1.5 - 2$ GeV/c $\gamma_{prompt}/\gamma_{\pi^{0}} \simeq$ 2%.
Thermal direct photons have been evaluated with the Bjorken Hydro-Dynamics
(BHD) model. The BHD spectra differ strongly from the HSD predictions. The
direct photon spectrum is very sensitive to the initial temperature parameter
$T_{0}$ of the model. The 10 MeV increase in the $T_{0}$ value leads to $\sim$
2 times higher photon yield.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:33:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kiselev",
"S. M.",
""
]
] | [
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] |
801.1426 | Michael R. Shirts | Michael R. Shirts (Department of Chemistry, Columbia University) and
John D. Chodera (Department of Chemistry, Stanford University) | Statistically optimal analysis of samples from multiple equilibrium
states | 13 pages (including appendices), 1 figure, LaTeX | J. Chem. Phys. 129, 124105 (2008) | 10.1063/1.2978177 | null | physics.comp-ph physics.chem-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a new estimator for computing free energy differences and
thermodynamic expectations as well as their uncertainties from samples obtained
from multiple equilibrium states via either simulation or experiment. The
estimator, which we term the multistate Bennett acceptance ratio (MBAR)
estimator because it reduces to the Bennett acceptance ratio when only two
states are considered, has significant advantages over multiple histogram
reweighting methods for combining data from multiple states. It does not
require the sampled energy range to be discretized to produce histograms,
eliminating bias due to energy binning and significantly reducing the time
complexity of computing a solution to the estimating equations in many cases.
Additionally, an estimate of the statistical uncertainty is provided for all
estimated quantities. In the large sample limit, MBAR is unbiased and has the
lowest variance of any known estimator for making use of equilibrium data
collected from multiple states. We illustrate this method by producing a highly
precise estimate of the potential of mean force for a DNA hairpin system,
combining data from multiple optical tweezer measurements under constant force
bias.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:56:48 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Mar 2008 04:05:19 GMT"
},
{
"version": "v3",
"created": "Tue, 17 Jun 2008 21:25:58 GMT"
}
] | 2011-12-06T00:00:00 | [
[
"Shirts",
"Michael R.",
"",
"Department of Chemistry, Columbia University"
],
[
"Chodera",
"John D.",
"",
"Department of Chemistry, Stanford University"
]
] | [
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] |
801.1427 | Yuri Djikaev | Yuri S. Djikaev | Effect of the surface-stimulated mode on the kinetics of homogeneous
crystal nucleation in droplets | 33 pages, 3 figures | null | 10.1021/jp8008942 | null | cond-mat.mtrl-sci cond-mat.stat-mech | null | A kinetic theory of homogeneous crystal nucleation in unary droplets is
presented taking into account that a crystal nucleus can form not only in the
volume-based mode (with all its facets within the droplet) but also in the
surface-stimulated one (with one of its facets at the droplet surface). The
previously developed thermodynamics of surface-stimulated crystal nucleation
rigorously showed that if at least one of the facets of the crystal is only
partially wettable by its melt, then it is thermodynamically more favorable for
the nucleus to form with that facet at the droplet surface rather than within
the droplet. So far, however, the kinetic aspects of this phenomenon had not
been studied at all. The theory proposed in the present paper advocates that
even in the surface-stimulated mode crystal nuclei initially emerge (as
sub-critical clusters) homogeneously in the sub-surface layer, not
"pseudo-heterogeneously" at the surface. A homogeneously emerged sub-critical
crystal can become a surface-stimulated nucleus due to density and structure
fluctuations. This effect contributes to the total rate of crystal nucleation
(as the volume-based mode does). An explicit expression for the total
per-particle rate of crystal nucleation is derived. Numerical evaluations for
water droplets suggest that the surface-stimulated mode can significantly
enhance the per-particle rate of crystal nucleation in droplets as large as 10
microns in radius. Possible experimental verification of the proposed theory is
discussed.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:49:24 GMT"
}
] | 2016-09-28T00:00:00 | [
[
"Djikaev",
"Yuri S.",
""
]
] | [
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] |
801.1428 | Martin Cederwall | Martin Cederwall and Bengt E.W. Nilsson | Pure Spinors and D=6 Super-Yang-Mills | 11 pp, 3 figs, plain tex | null | null | null | hep-th | null | Pure spinor cohomology has been used to describe maximally supersymmetric
theories, like D=10 super-Yang-Mills and D=11 supergravity. Supersymmetry
closes on-shell in such theories, and the fields in the cohomology
automatically satisfy the equations of motion. In this paper, we investigate
the corresponding structure in a model with off-shell supersymmetry, N=1
super-Yang-Mills theory in D=6. Here, fields and antifields are obtained as
cohomologies in different complexes with respect to the BRST operator Q. It
turns out to be natural to enlarge the pure spinor space with additional
bosonic variables, subject to some constraints generalising the pure spinor
condition, in order to accommodate the different supermultiplets in the same
generalised pure spinor wave-function. We construct another BRST operator, s,
acting in the cohomology of Q, whose cohomology implies the equations of
motion. We comment on the possible use of similar approaches in other models.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:50:36 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Cederwall",
"Martin",
""
],
[
"Nilsson",
"Bengt E. W.",
""
]
] | [
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] |
801.1429 | Marco Miranda | M. Miranda (Univ. of Zurich), M. Sereno (Univ. of Zurich), E. De
Filippis (INAF, INFN, Univ. of Naples), M. Paolillo (INFN, Univ. of Naples) | The dynamical state of RX J1347.5-1145 from a combined strong lensing
and X-ray analysis | 9 pages, 7 figures, accepted for publication in MNRAS. High
resolution version at
http://www-theorie.physik.unizh.ch/~solar/papers/RXJ1347.pdf | null | 10.1111/j.1365-2966.2008.12855.x | null | astro-ph | null | We perform a combined X-ray and strong lensing analysis of RX J1347.5-1145,
one of the most luminous galaxy clusters at X-ray wavelengths. We show that
evidence from strong lensing alone, based on published VLT and new HST data,
strongly argues in favor of a complex structure. The analysis takes into
account arc positions, shapes and orientations and is done thoroughly in the
image plane. The cluster inner regions are well fitted by a bimodal mass
distribution, with a total projected mass of $M_{tot} = (9.9 \pm 0.3)\times
10^{14} M_\odot/h$ within a radius of $360 \mathrm{kpc}/h$ ($1.5'$). Such a
complex structure could be a signature of a recent major merger as further
supported by X-ray data. A temperature map of the cluster, based on deep
Chandra observations, reveals a hot front located between the first main
component and an X-ray emitting South Eastern sub-clump. The map also unveils a
filament of cold gas in the innermost regions of the cluster, most probably a
cooling wake caused by the motion of the cD inside the cool core region. A
merger scenario in the plane of the sky between two dark matter sub-clumps is
consistent with both our lensing and X-ray analyses, and can explain previous
discrepancies with mass estimates based on the virial theorem.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 13:53:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Miranda",
"M.",
"",
"Univ. of Zurich"
],
[
"Sereno",
"M.",
"",
"Univ. of Zurich"
],
[
"De Filippis",
"E.",
"",
"INAF, INFN, Univ. of Naples"
],
[
"Paolillo",
"M.",
"",
"INFN, Univ. of Naples"
]
] | [
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] |
801.143 | Raphaele Herbin | Robert Eymard (LETEM), Thierry Gallou\"et (LATP), Raphaele Herbin
(LATP) | Discretisation of heterogeneous and anisotropic diffusion problems on
general non-conforming meshes. SUSHI: a scheme using stabilisation and hybrid
interfaces | null | null | null | null | math.NA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A discretisation scheme for heterogeneous anisotropic diffusion problems on
general meshes is developed and studied. The unknowns of this scheme are the
values at the centre of the control volumes and at some internal interfaces
which may for instance be chosen at the diffusion tensor discontinuities. The
scheme is therefore completely cell centred if no edge unknown is kept. It is
shown to be accurate on several numerical examples. Mathematical convergence of
the approximate solution to the continuous solution is obtained for general
(possibly discontinuous) tensors, general (possibly non-conforming) meshes, and
with no regularity assumption on the solution. An error estimate is then drawn
under sufficient regularity assumptions on the solution.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:01:20 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 08:33:50 GMT"
},
{
"version": "v3",
"created": "Tue, 22 Jan 2008 07:08:49 GMT"
},
{
"version": "v4",
"created": "Fri, 19 Sep 2008 07:08:17 GMT"
},
{
"version": "v5",
"created": "Tue, 9 Dec 2008 10:41:17 GMT"
}
] | 2008-12-09T00:00:00 | [
[
"Eymard",
"Robert",
"",
"LETEM"
],
[
"Gallouët",
"Thierry",
"",
"LATP"
],
[
"Herbin",
"Raphaele",
"",
"LATP"
]
] | [
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] |
801.1431 | William Chaplin | W. J. Chaplin, S. J. Jimenez-Reyes, A. Eff-Darwich, Y. Elsworth, R.
New | A devil in the detail: parameter cross-talk from the solar cycle and
estimation of solar p-mode frequencies | 9 pages; accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12942.x | null | astro-ph | null | Frequencies, powers and damping rates of the solar p modes are all observed
to vary over the 11-yr solar activity cycle. Here, we show that simultaneous
variations of these parameters give rise to a subtle cross-talk effect, which
we call the ``devil in the detail'', that biases p-mode frequencies estimated
from analysis of long power frequency spectra. We also show that the resonant
peaks observed in the power frequency spectra show small distortions due to the
effect. Most of our paper is devoted to a study of the effect for Sun-as-a-star
observations of the low-l p modes. We show that for these data the significance
of the effect is marginal. We also touch briefly on the likely l dependence of
the effect, and discuss the implications of these results for solar structure
inversions.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:03:01 GMT"
},
{
"version": "v2",
"created": "Tue, 12 Feb 2008 08:39:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chaplin",
"W. J.",
""
],
[
"Jimenez-Reyes",
"S. J.",
""
],
[
"Eff-Darwich",
"A.",
""
],
[
"Elsworth",
"Y.",
""
],
[
"New",
"R.",
""
]
] | [
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] |
801.1432 | Bertrand Reulet | Julien Gabelli and Bertrand Reulet | The Noise Susceptibility of a Photo-excited Coherent Conductor | abstract rewritten. minor corrections | null | null | null | cond-mat.mes-hall | null | We report the theory of the \emph{dynamical response of current fluctuations}
of a photo-excited conductor. We have performed the calculation for a coherent
conductor described by arbitrary energy-dependent transmissions and for
arbitrary frequencies. We consider two experimental setups that correspond to
different ways of symmetrizing the current operators, leading to different
predictions. Our results are in very good, quantitative agreement with a recent
measurement. We demonstrate that the dynamical response of noise that we have
calculated is the key concept that relates Dynamical Coulomb Blockade, i.e. the
electron-electron correction to the conductance due to the presence of an
external impedance, to quantum noise.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:06:20 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Jan 2008 14:22:03 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Gabelli",
"Julien",
""
],
[
"Reulet",
"Bertrand",
""
]
] | [
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] |
801.1433 | DaeKil Park | Eylee Jung, Mi-Ra Hwang, You Hwan Ju, Min-Soo Kim, Sahng-Kyoon Yoo,
Hungsoo Kim, D. K. Park, Jin-Woo Son, S. Tamaryan, Seong-Keuck Cha | GHZ versus W : Quantum Teleportation through Noisy Channels | 19 pages, 7 figure are included, 4 figures are not included due to
file size, These 4 figures can be downloaded from http://rose.kyungnam.ac.kr
V2: 23 pages, will appear in PRA | Physical Review A 78, (2008) 012312 | 10.1103/PhysRevA.78.012312 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Which state does lose less quantum information between GHZ and W states when
they are prepared for two-party quantum teleportation through noisy channel? We
address this issue by solving analytically a master equation in the Lindbald
form with introducing the noisy channels which makes the quantum channels to be
mixed states. It is found that the answer of the question is dependent on the
type of the noisy channel. If, for example, the noisy channel is ($L_{2,x}$,
$L_{3,x}$, $L_{4,x}$)-type where $L's$ denote the Lindbald operators, GHZ state
is always more robust than W state, i.e. GHZ state preserves more quantum
information. In, however, ($L_{2,y}$, $L_{3,y}$, $L_{4,y}$)-type channel the
situation becomes completely reversed. In ($L_{2,z}$, $L_{3,z}$,
$L_{4,z}$)-type channel W state is more robust than GHZ state when the noisy
paramter ($\kappa$) is comparatively small while GHZ state becomes more robust
when $\kappa$ is large. In isotropic noisy channel we found that both states
preserve equal amount of quantum information. A relation between the average
fidelity and entanglement for the mixed state quantum channels are discussed.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:06:39 GMT"
},
{
"version": "v2",
"created": "Fri, 13 Jun 2008 14:48:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jung",
"Eylee",
""
],
[
"Hwang",
"Mi-Ra",
""
],
[
"Ju",
"You Hwan",
""
],
[
"Kim",
"Min-Soo",
""
],
[
"Yoo",
"Sahng-Kyoon",
""
],
[
"Kim",
"Hungsoo",
""
],
[
"Park",
"D. K.",
""
],
[
"Son",
"Jin-Woo",
""
],
[
"Tamaryan",
"S.",
""
],
[
"Cha",
"Seong-Keuck",
""
]
] | [
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] |
801.1434 | Alexander Tsirlin | Alexander A. Tsirlin, Alexei A. Belik, Roman V. Shpanchenko, Evgeny V.
Antipov, Eiji Takayama-Muromachi, Helge Rosner | Frustrated spin-1/2 square lattice in the layered perovskite PbVO(3) | 4 pages, 4 figures, 2 tables | Phys. Rev. B, 77, 092402 (2008) | 10.1103/PhysRevB.77.092402 | null | cond-mat.str-el cond-mat.mtrl-sci | null | We report on the magnetic properties of the layered perovskite PbVO(3). The
results of magnetic susceptibility and specific heat measurements as well as
band structure calculations consistently suggest that the S=1/2 square lattice
of vanadium atoms in PbVO(3) is strongly frustrated due to
next-nearest-neighbor antiferromagnetic interactions. The ratio of
next-nearest-neighbor (J(2)) to nearest-neighbor (J(1)) exchange integrals is
estimated to be J(2)/J(1)\approx 0.2-0.4. Thus, PbVO(3) is within or close to
the critical region of the J(1)-J(2) frustrated square lattice. Supporting
this, no sign of long-range magnetic ordering was found down to 1.8 K.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:26:59 GMT"
}
] | 2008-03-06T00:00:00 | [
[
"Tsirlin",
"Alexander A.",
""
],
[
"Belik",
"Alexei A.",
""
],
[
"Shpanchenko",
"Roman V.",
""
],
[
"Antipov",
"Evgeny V.",
""
],
[
"Takayama-Muromachi",
"Eiji",
""
],
[
"Rosner",
"Helge",
""
]
] | [
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] |
801.1435 | Jyotirmoy Bhattacharya | Jyotirmoy Bhattacharya, Sayantani Bhattacharyya, Shiraz Minwalla and
Suvrat Raju | Indices for Superconformal Field Theories in 3,5 and 6 Dimensions | a small typo corrected, 46 pages | JHEP 0802:064,2008 | 10.1088/1126-6708/2008/02/064 | TIFR/TH/08-01, HUTP-08/A0001 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a trace formula for a Witten type Index for superconformal field
theories in d=3,5 and 6 dimensions, generalizing a similar recent construction
in d=4. We perform a detailed study of the decomposition of long
representations into sums of short representations at the unitarity bound to
demonstrate that our trace formula yields the most general index (i.e. quantity
that is guaranteed to be protected by superconformal symmetry alone) for the
corresponding superalgebras. Using the dual gravitational description, we
compute our index for the theory on the world volume of N M2 and M5 branes in
the large N limit. We also compute our index for recently constructed Chern
Simons theories in three dimensions in the large N limit, and find that, in
certain cases, this index undergoes a large N phase transition as a function of
chemical potentials.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:28:14 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Nov 2008 07:08:28 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Bhattacharya",
"Jyotirmoy",
""
],
[
"Bhattacharyya",
"Sayantani",
""
],
[
"Minwalla",
"Shiraz",
""
],
[
"Raju",
"Suvrat",
""
]
] | [
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] |
801.1436 | Kai O. Schweda | K. Schweda | Bulk Properties of QCD-matter at Highest Collider Energies | Proceedings of the ISMD07 conference, Berkeley, CA. 5 pages, 3
figures | Acta Phys.Polon.Supp.1:561-565,2008 | null | null | nucl-ex hep-ex | null | The Large Hadron Collider at CERN will provide Pb-Pb collisions at energies
up to $\sqrt{s_{NN}}$ = 5.5 TeV. We speculate on global observables, i.e. the
charged particle density at mid-rapidity, chemical freeze-out conditions and
collective parameters for transverse radial an elliptic flow. Finally, we
present an idea how to address the important issue of thermalization by
measuring the correlated production of heavy-quark hadrons.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:17:08 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Schweda",
"K.",
""
]
] | [
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] |
801.1437 | Juan Belmonte | J. Belmonte-Beitia, V. M. Perez-Garcia, V. Vekslerchik, P. J. Torres | Lie Symmetries, qualitative analysis and exact solutions of nonlinear
Schr\"odinger equations with inhomogeneous nonlinearities | 11 pages, 6 figures, 1 table | null | null | null | nlin.PS nlin.SI | null | Using Lie group theory and canonical transformations, we construct explicit
solutions of nonlinear Schrodinger equations with spatially inhomogeneous
nonlinearities. We present the general theory, use it to study different
examples and use the qualitative theory of dynamical systems to obtain some
properties of these solutions.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 10:12:34 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Belmonte-Beitia",
"J.",
""
],
[
"Perez-Garcia",
"V. M.",
""
],
[
"Vekslerchik",
"V.",
""
],
[
"Torres",
"P. J.",
""
]
] | [
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] |
801.1438 | Jean-S\'ebastien Sereni | Frantisek Kardos, Daniel Kr\'al', Jozef Miskuf, Jean-S\'ebastien
Sereni | Fullerene graphs have exponentially many perfect matchings | 7 pages, 3 figures | Journal of Mathematical Chemistry 46(2):443--447, 2009 | 10.1007/s10910-008-9471-7 | KAM-DIMATIA Series 2007-839 and ITI-Series 2008-368 | math.CO math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A fullerene graph is a planar cubic 3-connected graph with only pentagonal
and hexagonal faces. We show that fullerene graphs have exponentially many
perfect matchings.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:25:10 GMT"
},
{
"version": "v2",
"created": "Thu, 27 May 2010 16:14:44 GMT"
}
] | 2010-05-28T00:00:00 | [
[
"Kardos",
"Frantisek",
""
],
[
"Král'",
"Daniel",
""
],
[
"Miskuf",
"Jozef",
""
],
[
"Sereni",
"Jean-Sébastien",
""
]
] | [
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] |
801.1439 | Edwin J. Son | Wontae Kim, Edwin J. Son, Myungseok Yoon | Thermodynamics of (2+1)-dimensional acoustic black hole based on the
generalized uncertainty principle | 11 pages, 4 figures | null | null | null | gr-qc | null | We study thermodynamic quantities of an acoustic black hole and its
thermodynamic stability in a cavity based on the generalized uncertainty
principle. It can be shown that there is a minimal black hole which can be a
stable remnant after black hole evaporation. Moreover, the behavior of the free
energy shows that the large black hole is stable too. Therefore, the acoustic
black hole can decay into the remnant or the large black hole.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:25:38 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Kim",
"Wontae",
""
],
[
"Son",
"Edwin J.",
""
],
[
"Yoon",
"Myungseok",
""
]
] | [
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] |
801.144 | Monia Lupparelli | Monia Lupparelli, Giovanni M. Marchetti and Wicher P. Bergsma | Parameterizations and fitting of bi-directed graph models to categorical
data | null | null | null | null | stat.ML math.ST stat.TH | null | We discuss two parameterizations of models for marginal independencies for
discrete distributions which are representable by bi-directed graph models,
under the global Markov property. Such models are useful data analytic tools
especially if used in combination with other graphical models. The first
parameterization, in the saturated case, is also known as the multivariate
logistic transformation, the second is a variant that allows, in some (but not
all) cases, variation independent parameters. An algorithm for maximum
likelihood fitting is proposed, based on an extension of the Aitchison and
Silvey method.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:29:17 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Lupparelli",
"Monia",
""
],
[
"Marchetti",
"Giovanni M.",
""
],
[
"Bergsma",
"Wicher P.",
""
]
] | [
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801.1441 | Harry K. Hahn | Harry K. Hahn, Robert Sachs | The distribution of prime numbers on the square root spiral | 44 pages, 26 figures, 7 tables, minor change on text on page 1 | null | null | null | math.GM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Prime Numbers clearly accumulate on defined spiral graphs,which run through
the Square Root Spiral. These spiral graphs can be assigned to different
spiral-systems, in which all spiral-graphs have the same direction of rotation
and the same -- second difference -- between the numbers, which lie on these
spiral-graphs. A mathematical analysis shows, that these spiral graphs are
caused exclusively by quadratic polynomials. For example the well known Euler
Polynomial x2+x+41 appears on the Square Root Spiral in the form of three
spiral-graphs, which are defined by three different quadratic polynomials. All
natural numbers,divisible by a certain prime factor, also lie on defined spiral
graphs on the Square Root Spiral (or Spiral of Theodorus, or Wurzelspirale).
And the Square Numbers 4, 9, 16, 25, 36 even form a highly three-symmetrical
system of three spiral graphs, which divides the square root spiral into three
equal areas. Fibonacci number sequences also play a part in the structure of
the Square Root Spiral. With the help of the Number-Spiral, described by Mr.
Robert Sachs, a comparison can be drawn between the Square Root Spiral and the
Ulam Spiral. The shown sections of his study of the number spiral contain
diagrams, which are related to my analysis results, especially in regards to
the distribution of prime numbers.
| [
{
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"created": "Wed, 9 Jan 2008 12:08:23 GMT"
},
{
"version": "v2",
"created": "Wed, 17 Jul 2019 19:33:19 GMT"
}
] | 2019-07-19T00:00:00 | [
[
"Hahn",
"Harry K.",
""
],
[
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"Robert",
""
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801.1442 | Jaeweon Lee Dr. | Jae-Weon Lee | Is dark matter a BEC or scalar field? | published version | J.Korean Phys.Soc. 54 (2009) 2622 | 10.3938/jkps.54.2622 | null | astro-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This is a brief review on the history of the Bose-Einstein condensate (BEC)
or boson star model of galactic dark matter halos, where ultra-light scalar
dark matter particles condense in a single BEC quantum state. The halos can be
described as a self-gravitating, possibly self-interacting, coherent scalar
field.
On a scale larger than galaxies, dark matter behaves like cold dark matter
while below that scale the quantum mechanical nature suppresses the dark matter
structure formation due to the minimum length scale determined by the mass
$m\st{>}{\sim}10^{-24} eV$ and the self-interaction of the particles. This
property could alleviate the cusp problem and missing satellite problems of the
$\Lambda$CDM model. Furthermore, this model well reproduces the observed
rotation curves of spiral and dwarf galaxies, which makes the model promising.
| [
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"version": "v2",
"created": "Wed, 23 Apr 2008 13:54:39 GMT"
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"created": "Tue, 23 Dec 2008 14:22:11 GMT"
},
{
"version": "v4",
"created": "Wed, 30 Sep 2009 17:49:56 GMT"
}
] | 2013-08-22T00:00:00 | [
[
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""
]
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801.1443 | Wei Liu | Wei Liu | Large Deviations for Stochastic Evolution Equations with Small
Multiplicative Noise | 31 pages, published in Appl. Math. Optim | Appl. Math. Optim. 61 (2010), 27-56 | 10.1007/s00245-009-9072-2 | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Freidlin-Wentzell large deviation principle is established for the
distributions of stochastic evolution equations with general monotone drift and
small multiplicative noise. As examples, the main results are applied to derive
the large deviation principle for different types of SPDE such as stochastic
reaction-diffusion equations, stochastic porous media equations and fast
diffusion equations, and the stochastic p-Laplace equation in Hilbert space.
The weak convergence approach is employed in the proof to establish the Laplace
principle, which is equivalent to the large deviation principle in our
framework.
| [
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"version": "v3",
"created": "Fri, 1 Feb 2008 23:42:09 GMT"
},
{
"version": "v4",
"created": "Thu, 10 Sep 2009 11:00:08 GMT"
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] | 2010-05-06T00:00:00 | [
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] |
801.1444 | Elena Cordero | Elena Cordero, Fabio Nicola and Luigi Rodino | Boundedness of Fourier Integral Operators on $\mathcal{F} L^p$ spaces | 26 pages | Trans. Amer. Math. Soc., 361(11):6049--6071, 2009 | null | null | math.AP | null | We study the action of Fourier Integral Operators (FIOs) of H{\"o}rmander's
type on ${\mathcal{F}} L^p({\mathbb {R}}^d_{comp}$, $1\leq p\leq\infty$. We
see, from the Beurling-Helson theorem, that generally FIOs of order zero fail
to be bounded on these spaces when $p\not=2$, the counterexample being given by
any smooth non-linear change of variable. Here we show that FIOs of order
$m=-d|1/2-1/p|$ are instead bounded. Moreover, this loss of derivatives is
proved to be sharp in every dimension $d\geq1$, even for phases which are
linear in the dual variables. The proofs make use of tools from time-frequency
analysis such as the theory of modulation spaces.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:34:50 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 09:13:35 GMT"
},
{
"version": "v3",
"created": "Thu, 24 Apr 2008 10:49:25 GMT"
}
] | 2016-06-28T00:00:00 | [
[
"Cordero",
"Elena",
""
],
[
"Nicola",
"Fabio",
""
],
[
"Rodino",
"Luigi",
""
]
] | [
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] |
801.1445 | Frank Thuillier | Enore Guadagnini (df), Frank Thuillier (LAPTH) | Deligne-Beilinson cohomology and abelian links invariants | null | SIGMA 4 (2008), 078 | 10.3842/SIGMA.2008.078 | LAPTH-1191/07 | math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For the abelian Chern-Simons field theory, we consider the quantum functional
integration over the Deligne-Beilinson cohomology classes and we derive the
main properties of the observables in a generic closed orientable 3-manifold.
We present an explicit path-integral non-perturbative computation of the
Chern-Simons links invariants in the case of the torsion-free 3-manifolds
$S^3$, $S^1 \times S^2$ and $S^1 \times \Sigma_g$.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:39:24 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Nov 2008 19:56:02 GMT"
}
] | 2015-05-29T00:00:00 | [
[
"Guadagnini",
"Enore",
"",
"df"
],
[
"Thuillier",
"Frank",
"",
"LAPTH"
]
] | [
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] |
801.1446 | Abhijit Majumder | A. Majumder | The study of dense matter through jet modification | 5 pages, 2 figures, Presented at ISMD 2007, LBNL, Berkeley,
California, USA; Aug. 4-9 2007 | Acta Phys.Polon.Supp.1:619-623,2008 | null | null | nucl-th | null | The use of jet modification to study the properties of dense matter is
reviewed. Different sets of jet correlations measurements which may be used to
obtain both the space-time and momentum space structure of the produced matter
are outlined.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 19:42:56 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Majumder",
"A.",
""
]
] | [
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] |
801.1447 | Janyska Josef | Josef Jany\v{s}ka and Marco Modugno | Generalized geometrical structures of odd dimensional manifolds | null | null | null | null | math.DG math-ph math.MP | null | We define an almost--cosymplectic--contact structure which generalizes
cosymplectic and contact structures of an odd dimensional manifold.
Analogously, we define an almost--coPoisson--Jacobi structure which generalizes
a Jacobi structure. Moreover, we study relations between these structures and
analyse the associated algebras of functions. As examples of the above
structures, we present geometrical dynamical structures of the phase space of a
general relativistic particle, regarded as the 1st jet space of motions in a
spacetime. We describe geometric conditions by which a metric and a connection
of the phase space yield cosymplectic and dual coPoisson structures, in case of
a spacetime with absolute time (a Galilei spacetime), or
almost--cosymplectic--contact and dual almost--coPoisson--Jacobi structures, in
case of a spacetime without absolute time (an Einstein spacetime).
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 14:56:00 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Janyška",
"Josef",
""
],
[
"Modugno",
"Marco",
""
]
] | [
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] |
801.1448 | Jari Hyv\"aluoma | Jari Hyv\"aluoma and Jens Harting | Slip flow over structured surfaces with entrapped microbubbles | 4 pages, 4 figures. v2: revised version, to appear in Phys. Rev. Lett | Phys. Rev. Lett. 100, 246001 (2008) | 10.1103/PhysRevLett.100.246001 | null | cond-mat.soft | null | On hydrophobic surfaces, roughness may lead to a transition to a
superhydrophobic state, where gas bubbles at the surface can have a strong
impact on a detected slip. We present two-phase lattice Boltzmann simulations
of a Couette flow over structured surfaces with attached gas bubbles. Even
though the bubbles add slippery surfaces to the channel, they can cause
negative slip to appear due to the increased roughness. The simulation method
used allows the bubbles to deform due to viscous stresses. We find a decrease
of the detected slip with increasing shear rate which is in contrast to some
recent experimental results implicating that bubble deformation cannot account
for these experiments. Possible applications of bubble surfaces in microfluidic
devices are discussed.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:16:39 GMT"
},
{
"version": "v2",
"created": "Mon, 26 May 2008 05:50:56 GMT"
}
] | 2008-06-17T00:00:00 | [
[
"Hyväluoma",
"Jari",
""
],
[
"Harting",
"Jens",
""
]
] | [
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] |
801.1449 | Peter Curran | P.A. Curran (1), A.J. van der Horst (1,2), R.A.M.J. Wijers (1), R.L.C.
Starling (3) ((1) University of Amsterdam, (2) University of Alabama at
Huntsville, (3) University of Leicester) | The hidden X-ray breaks in afterglow light curves | 4 pages, contributed talk, submitted to the proceedings of Gamma Ray
Bursts 2007, Santa Fe, New Mexico, November 5-9 2007 | AIP Conf.Proc.1000:208-211,2008 | 10.1063/1.2943445 | null | astro-ph | null | Gamma-Ray Burst (GRB) afterglow observations in the Swift era have a
perceived lack of achromatic jet breaks compared to the BeppoSAX, or pre-Swift
era. Specifically, relatively few breaks, consistent with jet breaks, are
observed in the X-ray light curves of these bursts. If these breaks are truly
missing, it has serious consequences for the interpretation of GRB jet
collimation and energy requirements, and the use of GRBs as standard candles.
Here we address the issue of X-ray breaks which are possibly 'hidden' and
hence the light curves are misinterpreted as being single power-laws. We show
how a number of precedents, including GRB 990510 & GRB 060206, exist for such
hidden breaks and how, even with the well sampled light curves of the Swift
era, these breaks may be left misidentified. We do so by synthesising X-ray
light curves and finding general trends via Monte Carlo analysis. Furthermore,
in light of these simulations, we discuss how to best identify achromatic
breaks in afterglow light curves via multi-wavelength analysis.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:27:30 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Curran",
"P. A.",
""
],
[
"van der Horst",
"A. J.",
""
],
[
"Wijers",
"R. A. M. J.",
""
],
[
"Starling",
"R. L. C.",
""
]
] | [
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801.145 | Martin Lemoine | Kumiko Kotera, Martin Lemoine (IAP) | The optical depth of the Universe to ultrahigh energy cosmic ray
scattering in the magnetized large scale structure | version to appear in PRD; substantial improvements: extended
introduction, sections added on angular images and on direction dependent
effects with sky maps of optical depth, enlarged discussion of Auger results
(conclusions unchanged); 27 pages, 9 figures | Phys.Rev.D77:123003,2008 | 10.1103/PhysRevD.77.123003 | null | astro-ph | null | This paper provides an analytical description of the transport of ultrahigh
energy cosmic rays in an inhomogeneously magnetized intergalactic medium. This
latter is modeled as a collection of magnetized scattering centers such as
radio cocoons, magnetized galactic winds, clusters or magnetized filaments of
large scale structure, with negligible magnetic fields in between. Magnetic
deflection is no longer a continuous process, it is rather dominated by
scattering events. We study the interaction between high energy cosmic rays and
the scattering agents. We then compute the optical depth of the Universe to
cosmic ray scattering and discuss the phenomological consequences for various
source scenarios. For typical parameters of the scattering centers, the optical
depth is greater than unity at 5x10^{19}eV, but the total angular deflection is
smaller than unity. One important consequence of this scenario is the
possibility that the last scattering center encountered by a cosmic ray be
mistaken with the source of this cosmic ray. In particular, we suggest that
part of the correlation recently reported by the Pierre Auger Observatory may
be affected by such delusion: this experiment may be observing in part the last
scattering surface of ultrahigh energy cosmic rays rather than their source
population. Since the optical depth falls rapidly with increasing energy, one
should probe the arrival directions of the highest energy events beyond
10^{20}eV on an event by event basis to circumvent this effect.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:37:19 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Apr 2008 08:29:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kotera",
"Kumiko",
"",
"IAP"
],
[
"Lemoine",
"Martin",
"",
"IAP"
]
] | [
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] |
801.1451 | Pieter Moree | Andreas Decker and Pieter Moree | Counting RSA-integers | to appear in Results in Mathematics, 5 pages, with the view of
possible interest by cryptographers we aimed for a very short paper, rather
than a more extensive technical one with stronger results | Result. Math. 52 (2008), 35-39 | null | null | math.NT | null | In the RSA cryptosystem integers of the form n=p.q with p and q primes of
comparable size (`RSA-integers') play an important role. It is a folklore
result of cryptographers that C_r(x), the number of integers n<=x that are of
the form n=pq with p and q primes such that p<q<rp, is for fixed r>1
asymptotically equal to c_r*x*log^{-2}x for some constant c_r>0. Here we prove
this and show that c_r=2log r.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:36:28 GMT"
}
] | 2012-07-30T00:00:00 | [
[
"Decker",
"Andreas",
""
],
[
"Moree",
"Pieter",
""
]
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] |
801.1452 | Mohamed Saidi | Mohamed Saidi and Akio Tamagawa | A prime-to-p version of the Grothendieck anabelian conjecture for
hyperbolic curves over finite fields of characteristic p>0 | null | null | null | null | math.AG math.NT | null | In this paper, we prove a prime-to-p version of Grothendieck's anabelian
conjecture for hyperbolic curves over finite fields of characteristic p>0,
whose original (full profinite) version was proved by Tamagawa in the affine
case and by Mochizuki in the proper case.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:52:53 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 11:53:43 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Saidi",
"Mohamed",
""
],
[
"Tamagawa",
"Akio",
""
]
] | [
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] |
801.1453 | Ren\'e Messina | Lahcen Assoud, Rene Messina, Hartmut Loewen | Binary crystals in two-dimensional two-component Yukawa mixtures | RevTeX 4 - 17 pages - 6 main figures | null | 10.1063/1.2996515 | null | cond-mat.soft cond-mat.mtrl-sci | null | The zero-temperature phase diagram of binary mixtures of particles
interacting via a screened Coulomb pair potential is calculated as a function
of composition and charge ratio. The potential energy obtained by a Lekner
summation is minimized among a variety of candidate two-dimensional crystals. A
wealth of different stable crystal structures is identified including
$A,B,AB_2, A_2B, AB_4$ structures [$A$ $(B)$ particles correspond to large
(small) charge.] Their elementary cells consist of triangular, square or
rhombic lattices of the $A$ particles with a basis comprising various
structures of $A$ and $B$ particles. For small charge asymmetry there are no
intermediate crystals besides the pure $A$ and $B$ triangular crystals.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 15:57:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Assoud",
"Lahcen",
""
],
[
"Messina",
"Rene",
""
],
[
"Loewen",
"Hartmut",
""
]
] | [
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-0.0370274037,
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-0.0527209826,
-0.0372869968,
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] |
801.1454 | Isabel P\'erez-Arjona | Isabel Perez-Arjona, Victor J. Sanchez-Morcillo and German de
Valcarcel | Derivation of the spatio-temporal model equations for the thermoacoustic
resonator | null | null | null | null | nlin.PS | null | We derive the model equations describing the thermoacoustic resonator, that
is, an acoustical resonator containing a viscous medium inside. Previous
studies on this system have addressed this sytem in the frame of the plane-wave
approximation, we extend the previous model to by considering spatial effects
in a large aperture resonator. This model exhibits pattern formation and
localized structures scenario.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:02:35 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Perez-Arjona",
"Isabel",
""
],
[
"Sanchez-Morcillo",
"Victor J.",
""
],
[
"de Valcarcel",
"German",
""
]
] | [
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] |
801.1455 | J\"org Hennig | J\"org Hennig and Marcus Ansorg | A Fully Pseudospectral Scheme for Solving Singular Hyperbolic Equations | 24 pages, 12 figures | J.Hyperbol.Diff.Equat.6:161,2009 | 10.1142/S0219891609001769 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | With the example of the spherically symmetric scalar wave equation on
Minkowski space-time we demonstrate that a fully pseudospectral scheme (i.e.
spectral with respect to both spatial and time directions) can be applied for
solving hyperbolic equations. The calculations are carried out within the
framework of conformally compactified space-times. In our formulation, the
equation becomes singular at null infinity and yields regular boundary
conditions there. In this manner it becomes possible to avoid "artificial"
conditions at some numerical outer boundary at a finite distance. We obtain
highly accurate numerical solutions possessing exponential spectral
convergence, a feature known from solving elliptic PDEs with spectral methods.
Our investigations are meant as a first step towards the goal of treating time
evolution problems in General Relativity with spectral methods in space and
time.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:13:19 GMT"
},
{
"version": "v2",
"created": "Thu, 26 Mar 2009 12:41:44 GMT"
}
] | 2010-11-05T00:00:00 | [
[
"Hennig",
"Jörg",
""
],
[
"Ansorg",
"Marcus",
""
]
] | [
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] |
801.1456 | Guo Hongchen | H. C. Guo, Y. Q. Qin, G. J. You, W. M. Liu, S. H. Tang | A Diffractive Study of Parametric Process in Nonlinear Photonic Crystals | null | null | 10.1007/s00340-009-3828-x | null | physics.optics | null | We report a general description of quasi-phase-matched parametric process in
nonlinear photonic crystals (NLPC) by extending the conventional X-ray
diffraction theory in solids. Under the virtual wave approximation,
phase-matching resonance is equivalent to the diffraction of the scattered
virtual wave. Hence a modified NLPC Ewald construction can be built up, which
illustrates the nature of the accident for the diffraction of the virtual wave
in NLPC and further reveals the complete set of diffractions of the virtual
wave for both of the air-dielectric and dielectric-dielectric contacts. We show
the two basic linear sequences, the anti-stacking and para-stacking linear
sequences, in one-dimension (1D) NLPC and present a general rule for multiple
phase-matching resonances in 1D NLPC. The parameters affecting the NLPC
structure factor are investigated, which indicate that not only the Ewald
construction but also the relative NLPC atom size together determine whether a
diffraction of the virtual wave can occur in 2D NLPC. The results also show
that 1D NLPC is a better choice than 2D NLPC for a single parametric process.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:08:46 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Guo",
"H. C.",
""
],
[
"Qin",
"Y. Q.",
""
],
[
"You",
"G. J.",
""
],
[
"Liu",
"W. M.",
""
],
[
"Tang",
"S. H.",
""
]
] | [
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-0.1004416123,
-0.0446098261,
-0.0550988242,
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] |
801.1457 | Frederick Bernardot | B. Eble, C. Testelin, F. Bernardot, M. Chamarro, and G. Karczewski | Inversion of the spin polarization of localized electrons driven by dark
excitons | 3 figures | null | null | null | cond-mat.other | null | The creation of free excitons by absorption of circularly polarized photons,
and their subsequent fast capture by donors, is at the origin of the spin
polarization of donor-bound electrons. The sign of the electronic spin
polarization at low density of excitation is, as expected, fixed by the
helicity of the exciting light; but at high density of excitation we show that
the spin polarization is of the opposite sign. This striking inversion is
explained, here, by the contribution of dark excitons to mechanisms of spin
polarization of localized electrons.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:15:01 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Eble",
"B.",
""
],
[
"Testelin",
"C.",
""
],
[
"Bernardot",
"F.",
""
],
[
"Chamarro",
"M.",
""
],
[
"Karczewski",
"G.",
""
]
] | [
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] |
801.1458 | Miguel Orszag | Maritza Hernandez, Miguel Orszag | Decoherence versus disentanglement for two qubits in a squeezed bath | 9 pages, 13 figures | null | 10.1103/PhysRevA.78.042114 | null | quant-ph | null | We study the relation between the sudden death and revival of the
entanglement of two qubits in a common squeezed reservoir, and the normal
decoherence, by getting closer to the Decoherence Free Subspace and calculating
the effect on the death and revival times.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:17:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hernandez",
"Maritza",
""
],
[
"Orszag",
"Miguel",
""
]
] | [
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] |
801.1459 | Eilam Gross | Eilam Gross and Ofer Vitells | A Method for Deriving Transverse Masses Using Lagrange Multipliers | 4 pages, 2 figures | null | null | null | physics.data-an hep-ex | null | We use Lagrange multipliers to extend the traditional definition of
Transverse Mass used in experimental high energy physics. We demonstrate the
method by implementing it to derive a new Transverse Mass that can be used as a
discriminator to distinguish between top decays via a charged W or a charged
Higgs Boson.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:20:04 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Gross",
"Eilam",
""
],
[
"Vitells",
"Ofer",
""
]
] | [
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] |
801.146 | Jean-Marc Luck | Y. Avishai, J.M. Luck | Tight-binding electronic spectra on graphs with spherical topology. I.
The effect of a magnetic charge | 28 pages, 22 figures, 6 tables. Various kinds of minor improvements | J. Stat. Mech. (2008) P06007 | 10.1088/1742-5468/2008/06/P06007 | null | cond-mat.mes-hall | null | This is the first of two papers devoted to tight-binding electronic spectra
on graphs with the topology of the sphere. In this work the one-electron
spectrum is investigated as a function of the radial magnetic field produced by
a magnetic charge sitting at the center of the sphere. The latter is an integer
multiple of the quantized magnetic charge of the Dirac monopole, that integer
defining the gauge sector. An analysis of the spectrum is carried out for the
five Platonic solids (tetrahedron, cube, octahedron, dodecahedron and
icosahedron), the C$_{60}$ fullerene, and two families of polyhedra, the
diamonds and the prisms. Except for the fullerene, all the spectra are obtained
in closed form. They exhibit a rich pattern of degeneracies. The total energy
at half filling is also evaluated in all the examples as a function of the
magnetic charge.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:29:48 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 14:43:50 GMT"
}
] | 2008-06-13T00:00:00 | [
[
"Avishai",
"Y.",
""
],
[
"Luck",
"J. M.",
""
]
] | [
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] |
801.1461 | Adam-Christiaan van Roosmalen | Carl Fredrik Berg, Adam-Christiaan van Roosmalen | The Quiver of Projectives in Hereditary Categories with Serre Duality | 16 pages, as accepted by Journal of Pure and Applied Algebra | null | null | null | math.RT math.CT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let k be an algebraically closed field and A a k-linear hereditary category
satisfying Serre duality with no infinite radicals between the preprojective
objects. If A is generated by the preprojective objects, then we show that A is
derived equivalent to rep_k Q for a so called strongly locally finite quiver Q.
To this end, we introduce light cone distances and round trip distances on
quivers which will be used to investigate sections in stable translation
quivers of the form \mathbb{Z} Q.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:51:17 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Sep 2009 15:03:09 GMT"
}
] | 2009-09-23T00:00:00 | [
[
"Berg",
"Carl Fredrik",
""
],
[
"van Roosmalen",
"Adam-Christiaan",
""
]
] | [
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] |
801.1462 | Alberto Tonolo | Francesca Mantese, Alberto Tonolo | On classes defining a homological dimension | to appear in Contribution to Module Theory, de Gruyter 2007 | null | null | null | math.RA math.CT | null | A class $\mathcal F$ of objects of an abelian category $\mathcal A$ is said
to define a \emph{homological dimension} if for any object in $\mathcal A$ the
length of any $\mathcal F$-resolution is uniquely determined. In the present
paper we investigate classes satisfying this property.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:39:04 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Mantese",
"Francesca",
""
],
[
"Tonolo",
"Alberto",
""
]
] | [
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] |
801.1463 | Dmitry Semenov | D. Semenov (1), Ya. Pavlyuchenkov (1), Th. Henning (1), S. Wolf (1),
and R. Launhardt (1) ((1) Max Planck Institute for Astronomy, Heidelberg,
Germany) | Chemical and thermal structure of protoplanetary disks as observed with
ALMA | 4 pages, 3 figures, 1 table, accepted for publication to ApJ Letters | null | 10.1086/528795 | null | astro-ph | null | We predict how protoplanetary disks around low-mass young stars would appear
in molecular lines observed with the ALMA interferometer. Our goal is to
identify those molecules and transitions that can be used to probe and
distinguish between chemical and physical disk structure and to define
necessary requirements for ALMA observations. Disk models with and without
vertical temperature gradient as well as with uniform abundances and those from
a chemical network are considered. As an example, we show the channel maps of
HCO$^+$(4-3) synthesized with a non-LTE line radiative transfer code and used
as an input to the GILDAS ALMA simulator to produce noise-added realistic
images. The channel maps reveal complex asymmetric patterns even for the model
with uniform abundances and no vertical thermal gradient. We find that a
spatial resolution of $0.2-0.5\arcsec$ and 0.5--10 hours of integration time
will be needed to disentangle large-scale temperature gradients and the
chemical stratification in disks in lines of abundant molecules.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:43:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Semenov",
"D.",
""
],
[
"Pavlyuchenkov",
"Ya.",
""
],
[
"Henning",
"Th.",
""
],
[
"Wolf",
"S.",
""
],
[
"Launhardt",
"R.",
""
]
] | [
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] |
801.1464 | G. Mihaly | A. Geresdi, A. Halbritter, M. Csontos, Sz. Csonka, G. Mihaly, T.
Wojtowicz, X. Liu, B. Janko, J.K. Furdyna | Nanoscale spin-polarization in dilute magnetic semiconductor (In,Mn)Sb | 4 pages | null | 10.1103/PhysRevB.77.233304 | null | cond-mat.other | null | Results of point contact Andreev reflection (PCAR) experiments on (In,Mn)Sb
are presented and analyzed in terms of current models of charge conversion at a
superconductor-ferromagnet interface. We investigate the influence of surface
transparency, and study the crossover from ballistic to diffusive transport
regime as contact size is varied. Application of a Nb tip to a (In,Mn)Sb sample
with Curie temperature Tc of 5.4 K allowed the determination of
spin-polarization when the ferromagnetic phase transition temperature is
crossed. We find a striking difference between the temperature dependence of
the local spin polarization and of the macroscopic magnetization, and
demonstrate that nanoscale clusters with magnetization close to the saturated
value are present even well above the magnetic phase transition temperature.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:46:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Geresdi",
"A.",
""
],
[
"Halbritter",
"A.",
""
],
[
"Csontos",
"M.",
""
],
[
"Csonka",
"Sz.",
""
],
[
"Mihaly",
"G.",
""
],
[
"Wojtowicz",
"T.",
""
],
[
"Liu",
"X.",
""
],
[
"Janko",
"B.",
""
],
[
"Furdyna",
"J. K.",
""
]
] | [
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] |
801.1465 | Harry Lipkin J | Harry J. Lipkin | New method for studying neutrino mixing and mass differences | 12 pages -Revised in view of announcement of new experiment on
K-capture | null | null | null | hep-ph | null | Neutrino masses and mixing can be investigated by studying the behavior of a
radioactive bare nucleus which decays by emitting an electron into the open
atomic K shell BEFORE and DURING its weak decay by neutrino emission. The
initial nuclear state has a momentum spread required by Heisenberg. The wave
packet contains pairs of components with different momenta which can produce
neutrinos in two mass eigenstates with exactly the same energy and different
momenta. These neutrino amplitudes mix to produce a single electron-neutrino
state with the same energy. Since there is no information on which mass
eigenstates produced the neutrino this is a typical quantum mechanics
"two-slit" or "which path" experiment. A transition between the same initial
and a final states can go via two paths with a phase difference producing
interference and oscillations. Here the two paths are in momentum space
A new oscillation phenomenon providing information about neutrino mixing is
obtained by following the nucleus before and during the decay. The analysis
starts with Stodolsky's proof that interference between states having different
energies cannot be observed in realistic experiments. Results then follow from
simple rigorous quantum mechanics without the hand waving and loopholes which
have confused many previous neutrino oscillation investigations.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 16:49:06 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Mar 2008 19:53:34 GMT"
}
] | 2008-03-06T00:00:00 | [
[
"Lipkin",
"Harry J.",
""
]
] | [
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] |
801.1466 | Lei-Han Tang | Lei-Han Tang and Qing-Hu Chen | Phase glass and zero-temperature phase transition in a randomly
frustrated two-dimensional quantum rotor model | 14 pages, 4 figures, to appear in JSTAT | null | 10.1088/1742-5468/2008/04/P04003 | null | cond-mat.supr-con cond-mat.dis-nn | null | The ground state of the quantum rotor model in two dimensions with random
phase frustration is investigated. Extensive Monte Carlo simulations are
performed on the corresponding (2+1)-dimensional classical model under the
entropic sampling scheme. For weak quantum fluctuation, the system is found to
be in a phase glass phase characterized by a finite compressibility and a
finite value for the Edwards-Anderson order parameter, signifying long-ranged
phase rigidity in both spatial and imaginary time directions. Scaling
properties of the model near the transition to the gapped, Mott insulator state
with vanishing compressibility are analyzed. At the quantum critical point, the
dynamic exponent $z_{\rm dyn}\simeq 1.17$ is greater than one. Correlation
length exponents in the spatial and imaginary time directions are given by
$\nu\simeq 0.73$ and $\nu_z\simeq 0.85$, respectively, both assume values
greater than 0.6723 of the pure case. We speculate that the phase glass phase
is superconducting rather than metallic in the zero current limit.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:00:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tang",
"Lei-Han",
""
],
[
"Chen",
"Qing-Hu",
""
]
] | [
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] |
801.1467 | Tobias Gail | Wolfram Weise and Rainer Hartle | Chiral SU(3) Dynamics and Antikaon-Nuclear quasibound States | null | Nucl.Phys.A804:173-185,2008 | 10.1016/j.nuclphysa.2008.01.003 | TUM/T39-08-01 | nucl-th | null | Recent developments are summarised concerning low-energy KbarN interactions
as they relate to the possible existence of antikaon-nuclear quasibound states.
An exploratory study of antikaons bound to finite nuclei is performed, with
emphasis on the evolution of such states from light to heavy nuclei (A = 16 -
208). The energy dependent, driving attractive KbarN interactions are
constructed using the s-wave coupled-channel amplitudes involving the
Lambda(1405) and resulting from chiral SU(3) dynamics, plus p-wave amplitudes
dominated by the Sigma(1385). Effects of Pauli and short-range correlations are
discussed. The decay width induced by K^-NN two-body absorption is estimated
and found to be substantial. It is concluded that Kbar-nuclear quasibound
states can possibly exist with binding energies ranging from 60 to 100 MeV, but
with short life times corresponding to decay widths of the similar magnitudes.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:10:13 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Weise",
"Wolfram",
""
],
[
"Hartle",
"Rainer",
""
]
] | [
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] |
801.1468 | Ingo Krug | I. P. Krug, F. U. Hillebrecht, H. Gomonaj, M. Haverkort, A. Tanaka, L.
H. Tjeng and C. M. Schneider | Magnetic coupling in highly-ordered NiO/Fe3O4(110): Ultrasharp magnetic
interfaces vs. long-range magnetoelastic interactions | null | Europhysics Letters 81 (2008) 17005 | 10.1209/0295-5075/81/17005 | null | cond-mat.mtrl-sci | null | We present a laterally resolved X-ray magnetic dichroism study of the
magnetic proximity effect in a highly ordered oxide system, i.e. NiO films on
Fe3O4(110). We found that the magnetic interface shows an ultrasharp
electronic, magnetic and structural transition from the ferrimagnet to the
antiferromagnet. The monolayer which forms the interface reconstructs to
NiFe2O4 and exhibits an enhanced Fe and Ni orbital moment, possibly caused by
bonding anisotropy or electronic interaction between Fe and Ni cations. The
absence of spin-flop coupling for this crystallographic orientation can be
explained by a structurally uncompensated interface and additional
magnetoelastic effects.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:10:35 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Krug",
"I. P.",
""
],
[
"Hillebrecht",
"F. U.",
""
],
[
"Gomonaj",
"H.",
""
],
[
"Haverkort",
"M.",
""
],
[
"Tanaka",
"A.",
""
],
[
"Tjeng",
"L. H.",
""
],
[
"Schneider",
"C. M.",
""
]
] | [
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] |
801.1469 | Vadim Asnin | Vadim Asnin | Analyticity Properties of Graham-Witten Anomalies | 2 typos corrected | Class. Quantum Grav. 25 (2008) 145013 | 10.1088/0264-9381/25/14/145013 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Analytic properties of Graham-Witten anomalies are considered. Weyl anomalies
according to their analytic properties are of type A (coming from
$\delta$-singularities in correlators of several energy-momentum tensors) or of
type B (originating in counterterms which depend logarithmically on a mass
scale). It is argued that all Graham-Witten anomalies can be divided into 2
groups: internal and external, and that all external anomalies are of type B,
whereas among internal anomalies there is one term of type A and all the rest
are of type B. This argument is checked explicitly for the case of a free
scalar field in a 6-dimensional space with a 2-dimensional submanifold.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:20:02 GMT"
},
{
"version": "v2",
"created": "Thu, 3 Jul 2008 12:56:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Asnin",
"Vadim",
""
]
] | [
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] |
801.147 | Dorodnitsyn Anton | A. Dorodnitsyn, T. Kallman, and D. Proga | An axisymmetric, hydrodynamical model for the torus wind in AGN | ApJ Letters, accepted for publication | null | 10.1086/529374 | null | astro-ph | null | We report on time-dependent axisymmetric simulations of an X-ray excited flow
from a parsec-scale, rotating, cold torus around an active galactic nucleus.
Our simulations account for radiative heating and cooling and radiation
pressure force. The simulations follow the development of a broad bi-conical
outflow induced mainly by X-ray heating. We compute synthetic spectra predicted
by our simulations. The wind characteristics and the spectra support the
hypothesis that a rotationally supported torus can serve as the source of a
wind which is responsible for the warm absorber gas observed in the X-ray
spectra of many Seyfert galaxies.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:28:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dorodnitsyn",
"A.",
""
],
[
"Kallman",
"T.",
""
],
[
"Proga",
"D.",
""
]
] | [
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] |
801.1471 | Witold Maciejewski | Witold Maciejewski (Liverpool John Moores University) | Orbits in corotating and counterrotating double bars | 2 pages, 1 figure; to appear in "Formation and Evolution of Galaxy
Disks", ASP Conf. Ser., eds. J.G. Funes & E.M. Corsini | null | null | null | astro-ph | null | The backbone of double bars is made out of double-frequency orbits, and
loops, their maps, indicate the bars' extent, morphology and dynamics.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 18:00:02 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Maciejewski",
"Witold",
"",
"Liverpool John Moores University"
]
] | [
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] |
801.1472 | Witold Maciejewski | Witold Maciejewski (Liverpool John Moores University) and Hannah Singh
(University of Oxford) | Tremaine-Weinberg integrals for gas flows in double bars | 4 pages, 2 figures; to appear in "Formation and Evolution of Galaxy
Disks", ASP Conf. Ser., eds. J.G. Funes & E.M. Corsini | null | null | null | astro-ph | null | We report on our attempts to achieve a nearly steady-state gas flow in
hydrodynamical simulations of doubly barred galaxies. After exploring the
parameter space, we construct two models, for which we evaluate the photometric
and the kinematic integrals, present in the Tremaine-Weinberg method, in search
of observational signatures of two rotating patterns. We show that such
signatures are often present, but a direct fit to data points is likely to
return incorrect pattern speeds. However, for a particular distribution of the
tracer, presented here, the values of the pattern speeds can be retrieved
reliably even with the direct fit.
| [
{
"version": "v1",
"created": "Wed, 9 Jan 2008 17:51:57 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Maciejewski",
"Witold",
"",
"Liverpool John Moores University"
],
[
"Singh",
"Hannah",
"",
"University of Oxford"
]
] | [
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