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712.0279 | Jorge Plazas | Jorge Plazas | Heisenberg modules over real multiplication noncommutative tori and
related algebraic structures | null | null | null | null | math.QA | null | We review some aspects of the theory of noncommutative two-tori with real
multiplication focusing on the role played by Heisenberg groups in the
definition of algebraic structures associated to these noncommutative spaces.
| [
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{
"version": "v2",
"created": "Fri, 7 Dec 2007 15:45:15 GMT"
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] | 2011-11-10T00:00:00 | [
[
"Plazas",
"Jorge",
""
]
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712.028 | Yoshiaki Hyodo | Yoshiaki Hyodo, Masahiro Tsujimoto, Katsuji Koyama, Shogo Nishiyama,
Tetsuya Nagata, Itsuki Sakon, Hiroshi Murakami, and Hironori Matsumoto | Suzaku X-Ray Spectroscopy of a Peculiar Hot Star in the Galactic Center
Region | Accepted for publication on PASJ Vol.60, SP-1, 2008 | null | 10.1093/pasj/60.sp1.S173 | null | astro-ph | null | We present the results of a Suzaku study of a bright point-like source in the
6.7 keV intensity map of the Galactic center region. We detected an intense
FeXXV 6.7 keV line with an equivalent width of ~1 keV as well as emission lines
of highly ionized Ar and Ca from a spectrum obtained by the X-ray Imaging
Spectrometer. The overall spectrum is described very well by a heavily absorbed
(~2x10^{23}cm^{-2}) thin thermal plasma model with a temperature of 3.8+/-0.6
keV and a luminosity of ~3x10^{34} erg s^{-1} (2.0--8.0 keV) at 8 kpc. The
absorption, temperature, luminosity, and the 6.7 keV line intensity were
confirmed with the archived XMM-Newton data. The source has a very red
(J-Ks=8.2 mag) infrared spectral energy distribution (SED), which was fitted by
a blackbody emission of ~1000 K attenuated by a visual extinction of ~31 mag.
The high plasma temperature and the large X-ray luminosity are consistent with
a wind-wind colliding Wolf-Rayet binary. The similarity of the SED to those of
the eponymous Quintuplet cluster members suggests that the source is a WC-type
source.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:10:43 GMT"
}
] | 2017-01-18T00:00:00 | [
[
"Hyodo",
"Yoshiaki",
""
],
[
"Tsujimoto",
"Masahiro",
""
],
[
"Koyama",
"Katsuji",
""
],
[
"Nishiyama",
"Shogo",
""
],
[
"Nagata",
"Tetsuya",
""
],
[
"Sakon",
"Itsuki",
""
],
[
"Murakami",
"Hiroshi",
""
],
[
"Matsumoto",
"Hironori",
""
]
] | [
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712.0281 | Salvatore Sciortino | S. Sciortino | Results and Perspectives of Young Stellar Object long look programs | Proceedings of the "XMM-Newton: the next decade", to appear in
Astronomische Nachrichten (4 pages and 5 figures) | null | 10.1002/asna.200710916 | null | astro-ph | null | Both Chandra and XMM-Newton have performed long look programs for studying
the YSO physics. I will discuss recent results on the controversial issue of
Class 0 YSO X-ray emission, the observational evidence of magnetic funnels
interconnecting the YSO with its circumstellar disk and the Fe 6.4 keV
fluorescent line emission and its origin. While recent results of the
XMM-Newton DROXO program challenge the ''standard'' interpretation of the Fe
6.4 line origin as due to photoionized fluorescing disk material, the discovery
of X-ray excited Ne 12.81 micron line is a clear evidence of the interaction
between X-rays and disk material. Future long look observations with XMM-Newton
are required to clarify the X-ray effects on YSO disk.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:12:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sciortino",
"S.",
""
]
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] |
712.0282 | St\'ephane Launois | S. Launois | On the automorphism groups of q-enveloping algebras of nilpotent Lie
algebras | 19p | Proc. workshop "From Lie Algebras to Quantum Groups", Ed. CIM,
vol. 28 (2007), 125-143 | null | null | math.RA math.QA math.RT | null | We investigate the automorphism group of the quantised enveloping algebra U
of the positive nilpotent part of certain simple complex Lie algebras g in the
case where the deformation parameter q \in \mathbb{C}^* is not a root of unity.
Studying its action on the set of minimal primitive ideals of U we compute this
group in the cases where g=sl_3 and g=so_5 confirming a Conjecture of
Andruskiewitsch and Dumas regarding the automorphism group of U. In the case
where g=sl_3, we retrieve the description of the automorphism group of the
quantum Heisenberg algebra that was obtained independently by Alev and Dumas,
and Caldero. In the case where g=so_5, the automorphism group of U was computed
in [16] by using previous results of Andruskiewitsch and Dumas. In this paper,
we give a new (simpler) proof of the Conjecture of Andruskiewitsch and Dumas in
the case where g=so_5 based both on the original proof and on graded arguments
developed in [17] and [18].
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:13:27 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Launois",
"S.",
""
]
] | [
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712.0283 | Anestis Antoniadis | Anestis Antoniadis | Wavelet methods in statistics: Some recent developments and their
applications | Published in at http://dx.doi.org/10.1214/07-SS014 the Statistics
Surveys (http://www.i-journals.org/ss/) by the Institute of Mathematical
Statistics (http://www.imstat.org) | Statistics Surveys 2007, Vol. 1, 16-55 | 10.1214/07-SS014 | IMS-SS-SS_2007_14 | stat.ME | null | The development of wavelet theory has in recent years spawned applications in
signal processing, in fast algorithms for integral transforms, and in image and
function representation methods. This last application has stimulated interest
in wavelet applications to statistics and to the analysis of experimental data,
with many successes in the efficient analysis, processing, and compression of
noisy signals and images. This is a selective review article that attempts to
synthesize some recent work on ``nonlinear'' wavelet methods in nonparametric
curve estimation and their role on a variety of applications. After a short
introduction to wavelet theory, we discuss in detail several wavelet shrinkage
and wavelet thresholding estimators, scattered in the literature and developed,
under more or less standard settings, for density estimation from i.i.d.
observations or to denoise data modeled as observations of a signal with
additive noise. Most of these methods are fitted into the general concept of
regularization with appropriately chosen penalty functions. A narrow range of
applications in major areas of statistics is also discussed such as partial
linear regression models and functional index models. The usefulness of all
these methods are illustrated by means of simulations and practical examples.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:15:09 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Antoniadis",
"Anestis",
""
]
] | [
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] |
712.0284 | Nikolai Gippius | A. A. Demenev, A. A. Shchekin, A. V. Larionov, S. S. Gavrilov, V. D.
Kulakovskii, N. A. Gippius, and S. G. Tikhodeev | Kinetics of stimulated polariton scattering in planar microcavities:
Evidence for a dynamically self-organized optical parametric oscillator | 4 pages, 4 figures | null | 10.1103/PhysRevLett.101.136401 | null | cond-mat.other | null | We demonstrate for the first time the strong temporal hysteresis effects in
the kinetics of the pumped and scattered polariton populations in a planar
semiconductor microcavity under a nano-second-long pulsed resonant (by
frequency and angle) excitation above the lower polariton branch. The
hysteresis effects are explained in the model of multi-mode scattering when the
bistability of the nonlinear pumped polariton is accompanied by the explosive
growth of the scattered polaritons population. Subsequent self-organization
process in the nonlinear polariton system results in a new -- dynamically
self-organized -- type of optical parametric oscillator.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:37:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Demenev",
"A. A.",
""
],
[
"Shchekin",
"A. A.",
""
],
[
"Larionov",
"A. V.",
""
],
[
"Gavrilov",
"S. S.",
""
],
[
"Kulakovskii",
"V. D.",
""
],
[
"Gippius",
"N. A.",
""
],
[
"Tikhodeev",
"S. G.",
""
]
] | [
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] |
712.0285 | Eric Moulines | Randal Douc (SAMOVAR), Eric Moulines (LTCI), Ya'Acov Ritov | Forgetting of the initial condition for the filter in general
state-space hidden Markov chain: a coupling approach | 21 | null | null | null | math.ST stat.TH | null | We give simple conditions that ensure exponential forgetting of the initial
conditions of the filter for general state-space hidden Markov chain. The
proofs are based on the coupling argument applied to the posterior Markov
kernels. These results are useful both for filtering hidden Markov models using
approximation methods (e.g., particle filters) and for proving asymptotic
properties of estimators. The results are general enough to cover models like
the Gaussian state space model, without using the special structure that
permits the application of the Kalman filter.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:28:04 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Douc",
"Randal",
"",
"SAMOVAR"
],
[
"Moulines",
"Eric",
"",
"LTCI"
],
[
"Ritov",
"Ya'Acov",
""
]
] | [
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] |
712.0286 | Vladimir P. Mineev | V.P. Mineev | In-plane magnetic field phase diagram of superconducting Sr2RuO4 | 4 pages, no figures | null | 10.1103/PhysRevB.77.064519 | null | cond-mat.supr-con cond-mat.str-el | null | We develop the Ginzburg - Landau theory of the upper critical field in the
basal plane of a tetragonal multiband metal in two-component superconducting
state. It is shown that typical for the two component superconducting state the
upper critical field basal plane anisotropy and the phase transition splitting
still exist in a multiband case. However, the value of anisotropy can be
effectively smaller than in the single band case. The results are discussed in
the application to the superconducting Sr2RuO4.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:38:45 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Dec 2007 08:47:16 GMT"
},
{
"version": "v3",
"created": "Fri, 21 Dec 2007 14:06:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mineev",
"V. P.",
""
]
] | [
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] |
712.0287 | Monika Kollar | Wolfgang Hollik, Monika Kollar, and Maike K. Trenkel | Hadronic production of top-squark pairs with electroweak NLO
contributions | 27 pages, 17 figures, 2 tables | JHEP 0802:018,2008 | 10.1088/1126-6708/2008/02/018 | MPP-2007-149 | hep-ph | null | Presented are complete next-to-leading order electroweak (NLO EW) corrections
to top-squark pair production at the Large Hadron Collider (LHC) within the
Minimal Supersymmetric Standard Model (MSSM). At this order, also effects from
the interference of EW and QCD contributions have to be taken into account.
Moreover, photon-induced top-squark production is considered as an additional
partonic channel, which arises from the non-zero photon density in the proton.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 13:59:12 GMT"
}
] | 2009-02-18T00:00:00 | [
[
"Hollik",
"Wolfgang",
""
],
[
"Kollar",
"Monika",
""
],
[
"Trenkel",
"Maike K.",
""
]
] | [
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] |
712.0288 | Sebastian Lipari L. | S. Lipari, M. Bergmann, S. Sanchez, R. Terlevich, Y. Taniguchi, E.
Mediavilla, B. Punsly, B. Garcia, W. Zheng, D. Merlo | Gemini GMOS IFU Spectroscopy of IRAS 04505-2958: A New Exploding BAL +
IR + Fe II QSO | 4 pages, 2 figures, Annual Meeting Argentinian Society of Astronomy,
Malargue - P. Auger Observatory, September 2007 | null | null | null | astro-ph | null | New results of a Programme of study of BAL + IR + Fe II QSOs (at low and high
redshift) are presented. Which are based mainly on deep Gemini GMOS integral
field unit (IFU/3D) spectroscopy. We have performed a detailed study of the
kinematics, morphological, and physical conditions, in the BAL + IR + Fe II
QSO: IRAS 04505-2958. From this study, some selected results are presented,
mainly for the 3 expanding giant shells (observed with Gemini). In particular,
the GMOS data suggest that the outflow (OF) process -in this IR QSO- generated
multiple expanding hypergiant shells (from 10, to 100 kpc), in several extreme
explosive events. These new Gemini GMOS data are in good agreement with our
evolutionary, explosive and composite Model: where part of the ISM of the host
galaxy is ejected in the form of multiple giant shells, mainly by HyN
explosions. This process could generate satellite/companion galaxies, and even
could expel a high fraction -or all- the host galaxy. In addition, this Model
for AGN could give important clue about the physical processes that could
explain the origin -in AGNs- of very energetic cosmic rays, detected by the P.
Auger Observatory.
| [
{
"version": "v1",
"created": "Sat, 1 Dec 2007 08:09:30 GMT"
},
{
"version": "v2",
"created": "Mon, 26 May 2008 15:09:48 GMT"
}
] | 2008-05-26T00:00:00 | [
[
"Lipari",
"S.",
""
],
[
"Bergmann",
"M.",
""
],
[
"Sanchez",
"S.",
""
],
[
"Terlevich",
"R.",
""
],
[
"Taniguchi",
"Y.",
""
],
[
"Mediavilla",
"E.",
""
],
[
"Punsly",
"B.",
""
],
[
"Garcia",
"B.",
""
],
[
"Zheng",
"W.",
""
],
[
"Merlo",
"D.",
""
]
] | [
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712.0289 | Frederic Bournaud | Marie Martig, Frederic Bournaud (CEA-Saclay, DSM/Dapnia/SAP) | Triggering of merger-induced starbursts by the tidal field of galaxy
groups and clusters | MNRAS Letters, in press | null | 10.1111/j.1745-3933.2008.00429.x | null | astro-ph | null | Star formation in galaxies is for a part driven by galaxy mergers. At low
redshift, star formation activity is low in high-density environments like
groups and clusters, and the star formation activity of galaxies increases with
their isolation. This star formation-density relation is observed to be
reversed at z~1, which is not explained by theoretical models so far. We study
the influence of the tidal field of a galaxy group or cluster on the star
formation activity of merging galaxies, using N-body simulations including gas
dynamics and star formation. We find that the merger-driven star formation is
significantly more active in the vicinity of such cosmological structures
compared to mergers in the field. The large-scale tidal field can thus enhance
the activity of galaxies in dense cosmic structures, and should be particularly
efficient at high redshift before quenching processes take effect in the
densest regions.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:38:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Martig",
"Marie",
"",
"CEA-Saclay, DSM/Dapnia/SAP"
],
[
"Bournaud",
"Frederic",
"",
"CEA-Saclay, DSM/Dapnia/SAP"
]
] | [
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] |
712.029 | Viswanath Balakrishnan | B. Viswanath, Paromita Kundu, B. Mukherjee and N. Ravishankar | Predicting the Growth of Two-Dimensional Nanostructures | 31 pages, 10 figures | null | 10.1088/0957-4484/19/19/195603 | null | cond-mat.mtrl-sci | null | The ability to predict the morphology of crystals formed by chemical
reactions is of fundamental importance for the shape-controlled synthesis of
nanostructures. Based on the atomistic mechanism for crystal growth under
different driving forces, we have developed morphology diagrams to predict
regimes for the growth of two-dimensional crystals. By using controlled
reactions for crystal growth in the absence of surfactants/capping agents, we
demonstrate the validity of this approach for the formation of 2-D structures
of Au, Ag, Pt, Pd and hydroxyapatite.
| [
{
"version": "v1",
"created": "Sat, 1 Dec 2007 15:22:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Viswanath",
"B.",
""
],
[
"Kundu",
"Paromita",
""
],
[
"Mukherjee",
"B.",
""
],
[
"Ravishankar",
"N.",
""
]
] | [
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712.0291 | Pekka Lahti | J. Kiukas, P. Lahti, J.-P. Pellonpaa | A proof for the informational completeness of the rotated quadrature
observables | 11 pages | J. Phys. A: Math. Theor. 41 (2008) 175206 (11 pp) | 10.1088/1751-8113/41/17/175206 | null | quant-ph | null | We give a new mathematically rigorous proof for the fact that, when $S$ is a
dense subset of $[0,2\pi)$, the rotated quadrature operators $Q_\theta$,
$\theta\in S$, of a single mode electromagnetic field constitute an
informationally complete set of observables.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:09:56 GMT"
}
] | 2010-10-19T00:00:00 | [
[
"Kiukas",
"J.",
""
],
[
"Lahti",
"P.",
""
],
[
"Pellonpaa",
"J. -P.",
""
]
] | [
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712.0292 | Dimitri Karayannakis | D. Karayannakis | An algorithm for evaluating the Gamma function and ramifications | 12 pages | null | null | null | math.CA | null | We provide a new algorithm for evaluating the gamma function at any
(rational) point and a new infinite product representation free from the
presence of Euler and Mascheroni constant.Formulae and inequalities seemingly
new are obtained as byproducts of the method.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:12:50 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Karayannakis",
"D.",
""
]
] | [
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712.0293 | Francesco Sylos Labini fsl | Francesco Sylos Labini and Luciano Pietronero | Statistical physics for cosmic structures | 8 pages, 4 figures, European Physical Journal B - STATPHYS 23 topical
issue in the press (2007) | Eur. Phys. J. B, 64, 615-623 (2008) | 10.1140/epjb/e2008-00002-8 | null | cond-mat.stat-mech | null | The recent observations of galaxy and dark matter clumpy distributions have
provided new elements to the understating of the problem of cosmological
structure formation. The strong clumpiness characterizing galaxy structures
seems to be present in the overall mass distribution and its relation to the
highly isotropic Cosmic Microwave Background Radiation represents a fundamental
problem. The extension of structures, the formation of power-law correlations
characterizing the strongly clustered regime and the relation between dark and
visible matter are the key problems both from an observational and a
theoretical point of view. We discuss recent progresses in the studies of
structure formation by using concepts and methods of statistical physics.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:13:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Labini",
"Francesco Sylos",
""
],
[
"Pietronero",
"Luciano",
""
]
] | [
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712.0294 | Viviana Casasola | V. Casasola, F. Combes, S. Garcia-Burillo, L. K. Hunt, S. Leon, A.
Baker | The NUGA project: The Seyfert 2 galaxy NGC3147 | 2 pages, 2 figures. To appear in the proceedings of "Formation and
Evolution of Galaxy Disks" (J. G. Funes, and E. M. Corsini eds) | null | null | null | astro-ph | null | We present CO(1-0) and CO(2-1) maps of the Seyfert 2 galaxy NGC3147 of the
NUclei of GAlaxies (NUGA) sample at 1.8'' x 1.6'' and 1.4'' x 1.2'' resolution
respectively. Identifying the presence of a bar in NGC3147 we also compute the
gravity torques exerted from the stellar bar on the gas.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:19:23 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Casasola",
"V.",
""
],
[
"Combes",
"F.",
""
],
[
"Garcia-Burillo",
"S.",
""
],
[
"Hunt",
"L. K.",
""
],
[
"Leon",
"S.",
""
],
[
"Baker",
"A.",
""
]
] | [
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] |
712.0295 | Delia Ionescu | Delia Ionescu-Kruse | Liapunov's direct method for Birkhoffian systems: Applications to
electrical networks | 21 pages, 1 figure | Journal of Geometry and Physics, 57(2007), 2213-2228 | 10.1016/j.geomphys.2007.06.005 | null | math.DS math.DG | null | In this paper, the concepts and the direct theorems of stability in the sense
of Liapunov, within the framework of Birkhoffian dynamical systems on
manifolds, are considered. The Liapunov-type functions are constructed for
linear and nonlinear LC and RLC electrical networks, to prove stability under
certain conditions.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:21:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ionescu-Kruse",
"Delia",
""
]
] | [
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712.0296 | Bertalan Horv\'ath Mr. | Bertalan Horv\'ath, Bence Lazarovits, Olivier Sauret, Gergely Zar\'and | Failure of mean-field approach in out-of-equilibrium Anderson model | 5 pages, 5 figures | Phys. Rev. B 77, 113108 (2008) | 10.1103/PhysRevB.77.113108 | null | cond-mat.str-el | null | To explore the limitations of the mean field approximation, frequently used
in \textit{ab initio} molecular electronics calculations, we study an
out-of-equilibrium Anderson impurity model in a scattering formalism. We find
regions in the parameter space where both magnetic and non-magnetic solutions
are stable. We also observe a hysteresis in the non-equilibrium magnetization
and current as a function of the applied bias voltage. The mean field method
also predicts incorrectly local moment formation for large biases and a spin
polarized current, and unphysical kinks appear in various physical quantities.
The mean field approximation thus fails in every region where it predicts local
moment formation.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:21:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Horváth",
"Bertalan",
""
],
[
"Lazarovits",
"Bence",
""
],
[
"Sauret",
"Olivier",
""
],
[
"Zaránd",
"Gergely",
""
]
] | [
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] |
712.0297 | Song Wei | Wei Song | Lower bounds on the squashed entanglement for multi-party systems | 4 pages, 2 figures | Int. J. Theor. Phys, 48, 2191(2009) | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Squashed entanglement is a promising entanglement measure that can be
generalized to multipartite case, and it has all of the desirable properties
for a good entanglement measure. In this paper we present computable lower
bounds to evaluate the multipartite squashed entanglement. We also derive some
inequalities relating the squashed entanglement to the other entanglement
measure.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:21:39 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 14:26:32 GMT"
},
{
"version": "v3",
"created": "Sat, 8 Dec 2007 12:01:30 GMT"
},
{
"version": "v4",
"created": "Sat, 1 Aug 2009 13:27:00 GMT"
},
{
"version": "v5",
"created": "Tue, 4 Aug 2009 00:47:34 GMT"
}
] | 2009-08-04T00:00:00 | [
[
"Song",
"Wei",
""
]
] | [
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712.0298 | Marcello Lissia | G. Bellini, G. Fiorentini, A. Ianni, M. Lissia, F. Mantovani, and O.
Smirnov | Nuclear physics inputs needed for geo-neutrino studies | 6 pages, 3 figures. Proceedings of the International Conference on
Topics in Astroparticle and Underground Physics (TAUP) 2007, Sendai, Japan,
September 11-15, 2007. To appear in Journal of Physics: Conference Series | J.Phys.Conf.Ser.120:052007,2008 | 10.1088/1742-6596/120/5/052007 | null | hep-ph astro-ph nucl-ex physics.geo-ph | null | Geo-neutrino studies are based on theoretical estimates of geo-neutrino
spectra. We propose a method for a direct measurement of the energy
distribution of antineutrinos from decays of long-lived radioactive isotopes.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:23:39 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bellini",
"G.",
""
],
[
"Fiorentini",
"G.",
""
],
[
"Ianni",
"A.",
""
],
[
"Lissia",
"M.",
""
],
[
"Mantovani",
"F.",
""
],
[
"Smirnov",
"O.",
""
]
] | [
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] |
712.0299 | Yu-Gang Ma | G. H. Liu, Y. G. Ma, X. Z. Cai, D. Q. Fang, W. Q. Shen, W. D. Tian,
and K. Wang | Azimuthal asymmetry of direct photons in intermediate energy heavy-ion
collisions | 7 pages, 4 figures; accepted by Physics Letters B | Phys. Lett. B 663 (2008) 312 | 10.1016/j.physletb.2008.04.037 | null | nucl-ex hep-ph nucl-th | null | Hard photon emitted from energetic heavy ion collisions is of very
interesting since it does not experience the late-stage nuclear interaction,
therefore it is useful to explore the early-stage information of matter phase.
In this work, we have presented a first calculation of azimuthal asymmetry,
characterized by directed transverse flow parameter $F$ and elliptic asymmetry
coefficient $v_2$, for proton-neutron bremsstrahlung hard photons in
intermediate energy heavy-ion collisions. The positive $F$ and negative $v_2$
of direct photons are illustrated and they seem to be anti-correlated to the
corresponding free proton's flow.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:23:55 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Apr 2008 12:56:52 GMT"
}
] | 2008-07-25T00:00:00 | [
[
"Liu",
"G. H.",
""
],
[
"Ma",
"Y. G.",
""
],
[
"Cai",
"X. Z.",
""
],
[
"Fang",
"D. Q.",
""
],
[
"Shen",
"W. Q.",
""
],
[
"Tian",
"W. D.",
""
],
[
"Wang",
"K.",
""
]
] | [
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712.03 | Szabolcs Borsanyi | Szabolcs Borsanyi, Mark Hindmarsh | Semiclassical decay of topological defects | 10 pages revtex, 7 figures | Phys.Rev.D77:045022,2008 | 10.1103/PhysRevD.77.045022 | null | hep-ph | null | Perturbative estimates suggest that extended topological defects such as
cosmic strings emit few particles, but numerical simulations of the fields from
which they are constructed suggest the opposite. In this paper we study the
decay of the two-dimensional prototype of strings, domain walls in a simple
scalar theory, solving the underlying quantum field theory in the Hartree
approximation. We conclude that including the quantum effects makes the picture
clear: the defects do not directly transform into particles, but there is a
non-perturbative channel to microscopic classical structures in the form of
propagating waves and persistent localised oscillations, which operates over a
huge separation of scales. When quantum effects are included, the microscopic
classical structures can decay into particles.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:25:40 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Borsanyi",
"Szabolcs",
""
],
[
"Hindmarsh",
"Mark",
""
]
] | [
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] |
712.0301 | Arjan Bik | A. Bik (MPIA, Heidelberg), A. Lenorzer (IAC, Tenerife), W-.F. Thi
(ROE, Edinburgh), E. Puga-Antolin (Univ. Leuven), L.B.F.M. Waters (Univ.
Amsterdam, Univ Leuven), L. Kaper (Univ. Amsterdam), L.N. Martin-Hernandez
(IAC, Tenerife) | An infrared view of (candidate accretion) disks around massive young
stars | 8 pages, 5 figures, to appear in the proceedings for "Massive Star
Formation: Observations confront Theory 2007" edited by H. Beuther | null | null | null | astro-ph | null | Near-infrared surveys of high-mass star-forming regions start to shed light
onto their stellar content. A particular class of objects found in these
regions, the so-called massive Young Stellar Objects (YSOs) are surrounded by
dense circumstellar material. Several near- and mid-infrared diagnostic tools
are used to infer the physical characteristics and geometry of this
circumstellar matter. Near-infrared hydrogen emission lines provide evidence
for a disk-wind. The profiles of the first overtone of the CO band-heads,
originating in the inner 10 AU from the central star, are well fitted assuming
a keplerian rotating disk. The mid-infrared spectral energy distribution
requires the presence of a more extended envelope containing dust at a
temperature of about 200 K. CRIRES observations of CO fundamental absorption
lines confirm the presence of a cold envelope. We discuss the evolutionary
status of these objects.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:29:27 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Bik",
"A.",
"",
"MPIA, Heidelberg"
],
[
"Lenorzer",
"A.",
"",
"IAC, Tenerife"
],
[
"Thi",
"W-. F.",
"",
"ROE, Edinburgh"
],
[
"Puga-Antolin",
"E.",
"",
"Univ. Leuven"
],
[
"Waters",
"L. B. F. M.",
"",
"Univ.\n Amsterdam, Univ Leuven"
],
[
"Kaper",
"L.",
"",
"Univ. Amsterdam"
],
[
"Martin-Hernandez",
"L. N.",
"",
"IAC, Tenerife"
]
] | [
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] |
712.0302 | Lars S\"oderholm H | Lars H. Soderholm | Hilbert fluid dynamics equations expressed in Chapman-Enskog pressure
tensor and heat current | null | null | 10.1080/00411450802515692 | null | cond-mat.stat-mech | null | The connection between the Chapman-Enskog and Hilbert expansions is
investigated in detail. In particular the fluid dynamics equations of any order
in the Hilbert expansion are given in terms of the pressure tensor and heat
current of the Chapman-Enskog expansion
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:35:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Soderholm",
"Lars H.",
""
]
] | [
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] |
712.0303 | Yu-Gang Ma | F. Jin, Y. G. Ma, G. L. Ma, J. H. Chen, S. Zhang, X. Z. Cai, H. Z.
Huang, J. Tian, C. Zhong, J. X. Zuo | Baryon-Strangeness correlations in Parton/Hadron transport model for Au
+ Au collisions at \sqrt{s_{NN}} = 200 GeV | 6 pages, 5 figures; to appear in Proceeding of International
Conference on "Strangeness in Quark Matter", 24 - 29 June 2007, Levoca,
Slovakia (Journal of Physics G: Nuclear and Particle Physics) | J.Phys.G35:044070,2008 | 10.1088/0954-3899/35/4/044070 | null | nucl-th hep-ph nucl-ex | null | Baryon-strangeness correlation (C$_{BS}$) has been investigated with a
multi-phase transport model (AMPT) in $^{197}$Au + $^{197}$Au collisions at
$\sqrt{s_{NN}}$ = 200 GeV. The centrality dependence of C$_{BS}$ is presented
within the model, from partonic phase to hadronic matter. We find that the
system still reserve partial predicted signatures of C$_{BS}$ after parton
coalescence. But after hadronic rescattering, the predicted signatures will be
obliterated completely. So it seems that both coalescence hadronization process
and hadronic rescattering are responsible for the disappearance of the C$_{BS}$
signatures.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:40:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Jin",
"F.",
""
],
[
"Ma",
"Y. G.",
""
],
[
"Ma",
"G. L.",
""
],
[
"Chen",
"J. H.",
""
],
[
"Zhang",
"S.",
""
],
[
"Cai",
"X. Z.",
""
],
[
"Huang",
"H. Z.",
""
],
[
"Tian",
"J.",
""
],
[
"Zhong",
"C.",
""
],
[
"Zuo",
"J. X.",
""
]
] | [
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] |
712.0304 | Yury Bystritskiy | Yu. M. Bystritskiy, M. K. Volkov, E. A. Kuraev, E. Bartos, M. Secansky | The decay \phi -> f_0(980) \gamma and the process e^+e^- -> \phi
f_0(980) | 13 pages, 5 figures, some errors in formulae are corrected and a few
references to new papers added | Phys.Rev.D77:054008,2008 | 10.1103/PhysRevD.77.054008 | null | hep-ph | null | The decay \phi -> f_0(980) \gamma and process e^+e^- -> \phi f_0(980) are
considered within the local Nambu-Jona-Lasinio model. In the amplitudes of
these processes contributions of s-quark and kaon loops are taken into account.
The kaon loop gives a dominant contribution. Our estimation for the decay width
of \phi -> f_0 \gamma is in satisfactory agreement with recent experimental
data. This allows us to make some predictions for cross sections of the process
e^+e^- -> \gamma^* -> \phi f_0 which can be tested in the C-\tau factory. The
total and differential cross sections of this process are calculated and
presented in the figures.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:43:47 GMT"
},
{
"version": "v2",
"created": "Sun, 9 Dec 2007 15:27:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bystritskiy",
"Yu. M.",
""
],
[
"Volkov",
"M. K.",
""
],
[
"Kuraev",
"E. A.",
""
],
[
"Bartos",
"E.",
""
],
[
"Secansky",
"M.",
""
]
] | [
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] |
712.0305 | N. Raj Rao | N. Raj Rao | The analytic computability of the Shannon transform for a large class of
random matrix channels | Submitted to the IEEE Transactions on Communications (Letters) | null | null | null | cs.IT math.IT | null | We define a class of "algebraic" random matrix channels for which one can
generically compute the limiting Shannon transform using numerical techniques
and often enumerate the low SNR series expansion coefficients in closed form.
We describe this class, the coefficient enumeration techniques and compare
theory with simulations.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:07:23 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Rao",
"N. Raj",
""
]
] | [
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] |
712.0306 | Mingyu Xu | Shige Peng, Mingyu Xu | Constrained BSDE and Viscosity Solutions of Variation Inequalities | null | null | null | null | math.SG math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, we study the relation between the smallest $g$-supersolution
of constraint backward stochastic differential equation and viscosity solution
of constraint semilineare parabolic PDE, i.e. variation inequalities. And we
get an existence result of variation inequalities via constraint BSDE, and
prove a uniqueness result under certain condition.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 14:50:42 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jul 2008 12:56:41 GMT"
}
] | 2008-07-16T00:00:00 | [
[
"Peng",
"Shige",
""
],
[
"Xu",
"Mingyu",
""
]
] | [
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] |
712.0307 | Oriana Mansutti | Marco Roncadelli, L. S. Schulman | Quantum Hamilton-Jacobi Theory | 7 pages | Phys. Rev. Lett. 99, 170406 (2007) | 10.1103/PhysRevLett.99.170406 | null | quant-ph hep-th | null | Quantum canonical transformations have attracted interest since the beginning
of quantum theory. Based on their classical analogues, one would expect them to
provide a powerful quantum tool. However, the difficulty of solving a nonlinear
operator partial differential equation such as the quantum Hamilton-Jacobi
equation (QHJE) has hindered progress along this otherwise promising avenue. We
overcome this difficulty. We show that solutions to the QHJE can be constructed
by a simple prescription starting from the propagator of the associated
Schroedinger equation. Our result opens the possibility of practical use of
quantum Hamilton-Jacobi theory. As an application we develop a surprising
relation between operator ordering and the density of paths around a
semiclassical trajectory.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:00:15 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Roncadelli",
"Marco",
""
],
[
"Schulman",
"L. S.",
""
]
] | [
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] |
712.0308 | Luis Dinis | L. Dinis, E.M. Gonzalez, J.V. Anguita, J.M.R. Parrondo, and J.L.
Vicent | Current reversal in collective ratchets induced by lattice instability | 5 pages, 4 figures. Accepted for publication in Phys. Rev. B | Phys. Rev. B 76, 212507 (2007) | 10.1103/PhysRevB.76.212507 | null | cond-mat.stat-mech cond-mat.supr-con | null | A collective mechanism for current reversal in superconducting vortex
ratchets is proposed. The mechanism is based on a two-dimensional instability
of the ground state (T=0) of the system. We illustrate our results with
numerical simulations and experiments in Nb superconducting films fabricated on
top of Si substrates with artificially induced asymmetric pinning centers.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:24:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dinis",
"L.",
""
],
[
"Gonzalez",
"E. M.",
""
],
[
"Anguita",
"J. V.",
""
],
[
"Parrondo",
"J. M. R.",
""
],
[
"Vicent",
"J. L.",
""
]
] | [
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712.0309 | Glenn van de Ven | G. van de Ven (Institute for Advanced Study, Princeton University,
Leiden University), P.T. de Zeeuw (European Southern Observatory, Leiden
University), R.C.E. van den Bosch (Leiden University) | Recovery of the internal orbital structure of galaxies | 34 pages, 21 figures; companion paper at arXiv:0712.0113; accepted
for publication in MNRAS; PDF file with full resolution figures at
http://www.sns.ias.edu/~glenn/vdven_abel.pdf | null | 10.1111/j.1365-2966.2008.12873.x | null | astro-ph | null | We construct axisymmetric and triaxial galaxy models with a phase-space
distribution function that depends on linear combinations of the three exact
integrals of motion for a separable potential. These Abel models, first
introduced by Dejonghe & Laurent and subsequently extended by Mathieu &
Dejonghe, are the axisymmetric and triaxial generalisations of the well-known
spherical Osipkov-Merritt models. We show that the density and higher order
velocity moments, as well as the line-of-sight velocity distribution (LOSVD) of
these models can be calculated efficiently and that they capture much of the
rich internal dynamics of early-type galaxies. We build a triaxial and oblate
axisymmetric galaxy model with projected kinematics that mimic the
two-dimensional kinematic observations that are obtained with integral-field
spectrographs such as SAURON. We fit the simulated observations with
axisymmetric and triaxial dynamical models constructed with our numerical
implementation of Schwarzschild's orbit-superposition method. We find that
Schwarzschild's method is able to recover the internal dynamics and
three-integral distribution function of realistic models of early-type
galaxies.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:48:08 GMT"
},
{
"version": "v2",
"created": "Thu, 3 Jan 2008 19:51:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"van de Ven",
"G.",
"",
"Institute for Advanced Study, Princeton University,\n Leiden University"
],
[
"de Zeeuw",
"P. T.",
"",
"European Southern Observatory, Leiden\n University"
],
[
"Bosch",
"R. C. E. van den",
"",
"Leiden University"
]
] | [
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712.031 | Roman Mizuk | R. Mizuk | Heavy flavor baryons | 9 pages, 15 figures, prepared for XXIII International Symposium on
Lepton and Photon Interactions at High Energy (LP07), 13-18 Aug 2007, Daegu,
Korea | null | null | null | hep-ex | null | We review the new results on the heavy flavor baryons and on the pentaquarks.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:13:42 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Mizuk",
"R.",
""
]
] | [
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] |
712.0311 | Reinhold Walser | M. Eckart, R. Walser and W.P. Schleich | Exploring the growth of correlations in a quasi one-dimensional trapped
Bose gas | 36 pages, 21 color pdf/jpeg figures, submitted to NJP, corrected
references | null | 10.1088/1367-2630/10/4/045024 | null | cond-mat.mes-hall | null | Phase correlations, density fluctuations and three-body loss rates are
relevant for many experiments in quasi one-dimensional geometries. Extended
mean-field theory is used to evaluate correlation functions up to third order
for a quasi one-dimensional trapped Bose gas at zero and finite temperature. At
zero temperature and in the homogeneous limit, we also study the transition
from the weakly correlated Gross-Pitaevskii regime to the strongly correlated
Tonks-Girardeau regime analytically. We compare our results with the exact
Lieb-Liniger solution for the homogeneous case and find good agreement up to
the cross-over regime.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:14:09 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Dec 2007 13:52:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Eckart",
"M.",
""
],
[
"Walser",
"R.",
""
],
[
"Schleich",
"W. P.",
""
]
] | [
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] |
712.0312 | Markus Heydenreich | Markus Heydenreich, Remco van der Hofstad and Akira Sakai | Mean-field behavior for long- and finite range Ising model, percolation
and self-avoiding walk | 43 pages, many figures. Version v2 with various (minor) changes (in
particular in Sections 1.4 and A.1), and Sect. 4 is shortened. Journal of
Statistical Physics (to appear) | null | 10.1007/s10955-008-9580-5 | null | math.PR math-ph math.MP | null | We consider self-avoiding walk, percolation and the Ising model with long and
finite range. By means of the lace expansion we prove mean-field behavior for
these models if $d>2(\alpha\wedge2)$ for self-avoiding walk and the Ising
model, and $d>3(\alpha\wedge2)$ for percolation, where $d$ denotes the
dimension and $\alpha$ the power-law decay exponent of the coupling function.
We provide a simplified analysis of the lace expansion based on the
trigonometric approach in Borgs et al. (2007)
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 10:26:22 GMT"
},
{
"version": "v2",
"created": "Thu, 29 May 2008 13:53:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Heydenreich",
"Markus",
""
],
[
"van der Hofstad",
"Remco",
""
],
[
"Sakai",
"Akira",
""
]
] | [
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] |
712.0313 | Pavel Exner | Pavel Exner and Sylwia Kondej | Hiatus perturbation for a singular Schr\"odinger operator with an
interaction supported by a curve in \mathbb{R}^3 | LaTeX, 29 pages | J. Math. Phys. 49 (2008), 032111 (19pp) | 10.1063/1.2845419 | null | math-ph math.MP math.SP quant-ph | null | We consider Schr\"odinger operators in $L^2(\mathbb{R}^3)$ with a singular
interaction supported by a finite curve $\Gamma$. We present a proper
definition of the operators and study their properties, in particular, we show
that the discrete spectrum can be empty if $\Gamma$ is short enough. If it is
not the case, we investigate properties of the eigenvalues in the situation
when the curve has a hiatus of length $2\epsilon$. We derive an asymptotic
expansion with the leading term which a multiple of $\epsilon \ln\epsilon$.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:16:11 GMT"
}
] | 2019-12-10T00:00:00 | [
[
"Exner",
"Pavel",
""
],
[
"Kondej",
"Sylwia",
""
]
] | [
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] |
712.0314 | Detlef Klimm | I. M. Ranieri, S. L. Baldochi, D. Klimm | The Phase Diagram GdF3-LuF3 | 6 pages, 4 figs., accepted for J. Solid State Chem | null | 10.1016/j.jssc.2008.02.017 | null | cond-mat.mtrl-sci cond-mat.other physics.chem-ph | null | The phase diagram gadolinium fluoride - lutetium fluoride was determined by
differential scanning calorimetry (DSC) and X-ray powder diffraction analysis.
Both pure components undergo a reversible first order transformation to a high
temperature phase. The mutual solubility of both components is unlimited in the
orthorhombic room temperature phase. The maximum solubility of Lu in the high
temperature phase of GdF3 (tysonite type) is about 20% and the maximum
solubility of Gd in LuF3 ($\alpha$-YF3 type) is about 40%. Intermediate
compositions of the low temperature phase decompose upon heating in a
peritectoid reaction to a mixture of both high temperature phases.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:56:13 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 08:53:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ranieri",
"I. M.",
""
],
[
"Baldochi",
"S. L.",
""
],
[
"Klimm",
"D.",
""
]
] | [
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712.0315 | Alessandro de Angelis | Alessandro De Angelis, Oriana Mansutti, Massimo Persic | Very-High Energy Gamma Astrophysics | 60 pages, 52 figures, (on line abstract replacement) | Riv.Nuovo Cim.31:187,2008 | 10.1393/ncr/i2008-10032-2 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | High-energy photons are a powerful probe for astrophysics and for fundamental
physics under extreme conditions. During the recent years, our knowledge of the
most violent phenomena in the Universe has impressively progressed thanks to
the advent of new detectors for high-energy gamma-rays. Observation of
gamma-rays gives an exciting view of the high-energy universe thanks to
satellite-based telescopes (AGILE, GLAST) and to ground-based detectors like
the Cherenkov telescopes (H.E.S.S. and MAGIC in particular), which recently
discovered more than 60 new very-high-energy sources. The progress achieved
with the last generation of Cherenkov telescopes is comparable to the one drawn
by EGRET with respect to the previous gamma-ray satellite detectors. This
article reviews the present status of high-energy gamma astrophysics, with
emphasis on the recent results and on the experimental developments.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:01:19 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Dec 2007 01:58:40 GMT"
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{
"version": "v3",
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{
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"created": "Tue, 20 May 2008 14:51:04 GMT"
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"created": "Mon, 7 Jul 2008 13:50:16 GMT"
},
{
"version": "v6",
"created": "Wed, 9 Jul 2008 13:37:24 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"De Angelis",
"Alessandro",
""
],
[
"Mansutti",
"Oriana",
""
],
[
"Persic",
"Massimo",
""
]
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] |
712.0316 | Dr. Christoph Hartnack | C Hartnack, H Oeschler, J Aichelin | Kaon production at subthreshold energies - what do we learn about the
nuclear medium ? | contribution to strange Quark Matter 2007, accepted for publication
in J. Phys. G 6 pages, 4 figures | J.Phys.G35:044021,2008 | 10.1088/0954-3899/35/4/044021 | null | nucl-th | null | The Isospin Quantum Molecular Dynamics model is used to compare spectra and
elliptic flow of kaons produced at subthreshold energies with data taken at the
SIS accelerator at GSI. We find that temperatures of the spectra are dominated
by the rescattering of the kaons. The study of elliptic flow observables
indicates the influence of rescattering as well as of the optical potential of
the kaons with increasing dominance of the optical potential at lower incident
energies.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:30:52 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hartnack",
"C",
""
],
[
"Oeschler",
"H",
""
],
[
"Aichelin",
"J",
""
]
] | [
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] |
712.0317 | Anne Sickles | Anne Sickles | Identified Particle Correlations at RHIC: Medium Interactions & Modified
Fragmentation | Invited talk given at International Symposium on Multiparticle
Dynamics, August 2007, in Berkeley | Acta Phys.Polon.Supp.1:647-650,2008 | null | null | nucl-ex | null | Azimuthal angle two particle correlations have been shown to be a powerful
probe for extracting novel features of jet induced correlations produced in
Au+Au collisions at RHIC. At intermediate $p_T$, 2-5GeV/c, the jets have been
shown to be significantly modified in both their particle composition and their
angular distribution compared to p+p collisions. Two-particle angular
correlations with identified particles provide sensitive probes of both the
interactions between hard scattered partons and the medium. The systematics of
these correlations are essential to understanding the physics of intermediate
$p_T$ in heavy ion collisions.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:20:03 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Sickles",
"Anne",
""
]
] | [
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712.0318 | Pedro Sacramento | D. Bozi, J. M. P. Carmelo, K. Penc, P. D. Sacramento | The TTF finite-energy spectral features in photoemission of TTF-TCNQ:
The Hubbard-chain description | To appear in Journal of Physics: Condensed Matter | null | 10.1088/0953-8984/20/02/022205 | null | cond-mat.str-el | null | A dynamical theory which accounts for all microscopic one-electron processes
is used to study the spectral function of the 1D Hubbard model for the whole
$(k, \omega)$-plane, beyond previous studies which focused on the weight
distribution in the vicinity of the singular branch lines only. While our
predictions agree with those of the latter studies concerning the
tetracyanoquinodimethane (TCNQ) related singular features in photoemission of
the organic compound tetrathiafulvalene-tetracyanoquinodimethane (TTF-TCNQ)
metallic phase, the generalized theory also leads to quantitative agreement
concerning the tetrathiafulvalene (TTF) related finite-energy spectral
features, which are found to correspond to a value of the on-site repulsion $U$
larger than for TCNQ. Our study reveals the microscopic mechanisms behind the
unusual spectral features of TTF-TCNQ and provides a good overall description
of those features for the whole $(k, \omega)$-plane.
| [
{
"version": "v1",
"created": "Fri, 30 Nov 2007 17:09:12 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Bozi",
"D.",
""
],
[
"Carmelo",
"J. M. P.",
""
],
[
"Penc",
"K.",
""
],
[
"Sacramento",
"P. D.",
""
]
] | [
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] |
712.0319 | Melanie Krips | M. Krips, R. Neri, S. Garcia-Burillo, S. Martin, F. Combes, J.
Gracia-Carpio, and A. Eckart | A multi-transition HCN and HCO+ study of 12 nearby active galaxies: AGN
versus SB environments | accepted for publication in ApJ; 20 pages, 7 figures; in emulateApJ
format | null | 10.1086/527367 | null | astro-ph | null | Recent studies have indicated that the HCN-to-CO(J=1-0) and
HCO+-to-HCN(J=1-0) ratios are significantly different between galaxies with AGN
(active galactic nucleus) and SB (starburst) signatures. In order to study the
molecular gas properties in active galaxies and search for differences between
AGN and SB environments, we observed the HCN(J=1-0), (J=2-1), (J=3-2),
HCO+(J=1-0) and HCO+(J=3-2), emission with the IRAM 30m in the centre of 12
nearby active galaxies which either exhibit nuclear SB and/or AGN signatures.
Consistent with previous results, we find a significant difference of the
HCN(J=2-1)-to-HCN(J=1-0), HCN(J=3-2)-to-HCN(J=1-0), HCO+(J=3-2)-to-HCO+(J=3-2),
and HCO+-to-HCN intensity ratios between the sources dominated by an AGN and
those with an additional or pure central SB: the HCN, HCO+ and HCO+-to-HCN
intensity ratios tend to be higher in the galaxies of our sample with a central
SB as opposed to the pure AGN cases which show rather low intensity ratios.
Based on an LVG analysis of these data, i.e., assuming purely collisional
excitation, the (average) molecular gas densities in the SB dominated sources
of our sample seem to be systematically higher than in the AGN sources. The LVG
analysis seems to further support systematically higher HCN and/or lower HCO+
abundances as well as similar or higher gas temperatures in AGN compared to the
SB sources of our sample. Also, we find that the HCN-to-CO ratios decrease with
increasing rotational number J for the AGN while they stay mostly constant for
the SB sources.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:31:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Krips",
"M.",
""
],
[
"Neri",
"R.",
""
],
[
"Garcia-Burillo",
"S.",
""
],
[
"Martin",
"S.",
""
],
[
"Combes",
"F.",
""
],
[
"Gracia-Carpio",
"J.",
""
],
[
"Eckart",
"A.",
""
]
] | [
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] |
712.032 | Sandu Popescu | Y. Aharonov, S. Popescu, J. Tollaksen, L. Vaidman | Multiple-time states and multiple-time measurements in quantum mechanics | 17 pages, 8 figures | null | 10.1103/PhysRevA.79.052110 | null | quant-ph | null | We discuss experimental situations that consist of multiple preparation and
measurement stages. This leads us to a new approach to quantum mechanics. In
particular, we introduce the idea of multi-time quantum states which are the
appropriate tools for describing these experimental situations. We also
describe multi-time measurements and discuss their relation to multi-time
states. A consequence of our new formalism is to put states and operators on an
equal footing. Finally we discuss the implications of our new approach to
quantum mechanics for the problem of the flow of time.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:27:41 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"Aharonov",
"Y.",
""
],
[
"Popescu",
"S.",
""
],
[
"Tollaksen",
"J.",
""
],
[
"Vaidman",
"L.",
""
]
] | [
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] |
712.0321 | Wolfgang Bertram | Wolfgang Bertram (IECN) | Difference Problems and Differential Problems | null | null | null | null | math.GM | null | We state some elementary problems concerning the relation between difference
calculus and differential calculus, and we try to convince the reader that, in
spite of the simplicity of the statements, a solution of these problems would
be a significant contribution to the understanding of the foundations of
differential and integral calculus.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:34:16 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Bertram",
"Wolfgang",
"",
"IECN"
]
] | [
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] |
712.0322 | Leonardo de Assis | S.O. Vellozo, Jose A. Helayel-Neto, A.W. Smith, L. P. G. De Assis | Standstill Electric Charge Generates Magnetostatic Field Under
Born-Infeld Electrodynamics | 11 pages, 3 figures. In this version is update a permanent address of
the author L.P.G. De Assis and information on submission publication.
Submetted to International Journal of Theoretical Physics | Int.J.Theor.Phys.47:2934-2944,2008 | 10.1007/s10773-008-9727-9 | CBPF-NF-021/07 | hep-th | null | The Abelian Born-Infeld classical non-linear electrodynamic has been used to
investigate the electric and magnetostatic fields generated by a point-like
electrical charge at rest in an inertial frame. The results show a rich
internal structure for the charge. Analytical solutions have also been found.
Such findings have been interpreted in terms of vacuum polarization and
magnetic-like charges produced by the very high strengths of the electric field
considered. Apparently non-linearity is to be accounted for the emergence of an
anomalous magnetostatic field suggesting a possible connection to that created
by a magnetic dipole composed of two mognetic charges with opposite signals.
Consistently in situations where the Born-Infeld field strength parameter is
free to become infinite, Maxwell`s regime takes over, the magnetic sector
vanishes and the electric field assumes a Coulomb behavior with no trace of a
magnetic component. The connection to other monopole solutions, like Dirac`s,
t' Hooft`s or Poliakov`s types, are also discussed. Finally some speculative
remarks are presented in an attempt to explain such fields.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:34:55 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 18:06:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Vellozo",
"S. O.",
""
],
[
"Helayel-Neto",
"Jose A.",
""
],
[
"Smith",
"A. W.",
""
],
[
"De Assis",
"L. P. G.",
""
]
] | [
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712.0323 | Neelima Kelkar Dr | N. G. Kelkar, H. M. Castaneda | Critical view of WKB decay widths | 18 pages, Latex | Phys.Rev.C76:064605,2007 | 10.1103/PhysRevC.76.064605 | null | nucl-th | null | A detailed comparison of the expressions for the decay widths obtained within
the semiclassical WKB approximation using different approaches to the tunneling
problem is performed. The differences between the available improved formulae
for tunneling near the top and the bottom of the barrier are investigated.
Though the simple WKB method gives the right order of magnitude of the decay
widths, a small number of parameters are often fitted. The need to perform the
fitting procedure remaining consistently within the WKB framework is emphasized
in the context of the fission model based calculations. Calculations for the
decay widths of some recently found super heavy nuclei using microscopic
alpha-nucleus potentials are presented to demonstrate the importance of a
consistent WKB calculation. The half-lives are found to be sensitive to the
density dependence of the nucleon-nucleon interaction and the implementation of
the Bohr-Sommerfeld quantization condition inherent in the WKB approach.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:42:22 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kelkar",
"N. G.",
""
],
[
"Castaneda",
"H. M.",
""
]
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712.0324 | Nathan Berkovits | Nathan Berkovits (IFT-UNESP, Sao Paulo) | Explaining the Pure Spinor Formalism for the Superstring | Added two footnotes and references to Baulieu et al | JHEP0801:065,2008 | 10.1088/1126-6708/2008/01/065 | IFT-P.019/2007 | hep-th | null | After adding a pair of non-minimal fields and performing a similarity
transformation, the BRST operator in the pure spinor formalism is expressed as
a conventional-looking BRST operator involving the Virasoro constraint and
(b,c) ghosts, together with 12 fermionic constraints. This BRST operator can be
obtained by gauge-fixing the Green-Schwarz superstring where the 8 first-class
and 8 second-class Green-Schwarz constraints are combined into 12 first-class
constraints. Alternatively, the pure spinor BRST operator can be obtained from
the RNS formalism by twisting the ten spin-half RNS fermions into five spin-one
and five spin-zero fermions, and using the SO(10)/U(5) pure spinor variables to
parameterize the different ways of twisting. GSO(-) vertex operators in the
pure spinor formalism are constructed using spin fields and picture-changing
operators in a manner analogous to Ramond vertex operators in the RNS
formalism.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:03:32 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Dec 2007 21:57:54 GMT"
}
] | 2008-11-26T00:00:00 | [
[
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"Nathan",
"",
"IFT-UNESP, Sao Paulo"
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] |
712.0325 | Marcelo Ponce C. | Arturo C. Mart\'i, Marcelo Ponce, Cristina Masoller | Dynamics of delayed-coupled chaotic logistic maps: influence of network
topology, connectivity and delay times | 5 pages, 7 figures. Also submitted to Pramana: the journal of the
Indian Academy of Sciences. To appear in the Proceedings of "Perspectives on
Nonlinear Dynamics 2007" | Pramana - Journal of Physics, Vol. 70, No. 6, June 2008, pp.
1117-1125 | 10.1007/s12043-008-0116-y | null | nlin.CD | null | We review our recent work on the synchronization of a network of
delay-coupled maps, focusing on the interplay of the network topology and the
delay times that take into account the finite velocity of propagation of
interactions. We assume that the elements of the network are identical ($N$
logistic maps in the regime where the individual maps, without coupling, evolve
in a chaotic orbit) and that the coupling strengths are uniform throughout the
network. We show that if the delay times are sufficiently heterogeneous, for
adequate coupling strength the network synchronizes in a spatially homogeneous
steady-state, which is unstable for the individual maps without coupling. This
synchronization behavior is referred to as ``suppression of chaos by random
delays'' and is in contrast with the synchronization when all the interaction
delay times are homogeneous, because with homogeneous delays the network
synchronizes in a state where the elements display in-phase time-periodic or
chaotic oscillations. We analyze the influence of the network topology
considering four different types of networks: two regular (a ring-type and a
ring-type with a central node) and two random (free-scale Barabasi-Albert and
small-world Newman-Watts). We find that when the delay times are sufficiently
heterogeneous the synchronization behavior is largely independent of the
network topology but depends on the networks connectivity, i.e., on the average
number of neighbors per node.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:45:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Martí",
"Arturo C.",
""
],
[
"Ponce",
"Marcelo",
""
],
[
"Masoller",
"Cristina",
""
]
] | [
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] |
712.0326 | Bian Qian | Bian Qian, Thomas R. Powers, Kenneth S. Breuer (Division of
Engineering, Brown University) | Shape transition and propulsive force of an elastic rod rotating in a
viscous fluid | 4 pages, 5 figures | PRL 100, 078101 (2008) | 10.1103/PhysRevLett.100.078101 | null | cond-mat.soft | null | The deformation of thin rods in a viscous liquid is central to the mechanics
of motility in cells ranging from \textit{Escherichia coli} to sperm. Here we
use experiments and theory to study the shape transition of a flexible rod
rotating in a viscous fluid driven either by constant torque or at constant
speed. The rod is tilted relative to the rotation axis. At low applied torque,
the rod bends gently and generates small propulsive force. At a critical
torque, the rotation speed increases abruptly and the rod forms a helical shape
with much greater propulsive force. We find good agreement between theory and
experiment.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:47:09 GMT"
}
] | 2008-02-26T00:00:00 | [
[
"Qian",
"Bian",
"",
"Division of\n Engineering, Brown University"
],
[
"Powers",
"Thomas R.",
"",
"Division of\n Engineering, Brown University"
],
[
"Breuer",
"Kenneth S.",
"",
"Division of\n Engineering, Brown University"
]
] | [
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712.0327 | Thomas Gehrmann | G. Dissertori, A. Gehrmann-De Ridder, T. Gehrmann, E.W.N. Glover, G.
Heinrich, H. Stenzel | First determination of the strong coupling constant using NNLO
predictions for hadronic event shapes in e^+e^- annihilations | 25 pages, LaTeX, extended discussion of hadronization corrections,
typos corrected | JHEP 0802:040,2008 | 10.1088/1126-6708/2008/02/040 | ZU-TH 28/07, IPPP/07/91, Edinburgh 2007-48, ETHZ-IPP RP-2007-04 | hep-ph hep-ex | null | We present the first determination of the strong coupling constant from a fit
of next-to-next-to-leading order QCD predictions to event-shape variables,
measured in $e^+e^-$ annihilations at LEP. The data have been collected by the
ALEPH detector at centre-of-mass energies between 91 and 206 GeV. Compared to
results of next-to-leading order fits we observe that the central fit values
are lower by about 10%, with considerably reduced scatter among the results
obtained with different event-shape variables. The dominant systematic
uncertainty from renormalization scale variations is reduced by a factor of
two. By combining the results for several event-shape variables and
centre-of-mass energies, we find \alpha_s(M_Z^2) =
0.1240+-0.0008(stat)+-0.0010(exp)+-0.0011(had)+-0.0029(theo).
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:51:12 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Feb 2008 12:48:12 GMT"
}
] | 2008-12-30T00:00:00 | [
[
"Dissertori",
"G.",
""
],
[
"Ridder",
"A. Gehrmann-De",
""
],
[
"Gehrmann",
"T.",
""
],
[
"Glover",
"E. W. N.",
""
],
[
"Heinrich",
"G.",
""
],
[
"Stenzel",
"H.",
""
]
] | [
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712.0328 | Krzysztof Urbanowski | K. Urbanowski | Khalfin's Theorem and neutral mesons subsystem | 26 pages, 3 figures, talk given at "13th Lomonosov Conference on
Elementary Particle Physics", Moscow, August 23 -- 29, 2007 | null | null | null | hep-ph | null | We analyze the proof of the Khalfin Theorem for neutral meson complex. The
consequences of this Theorem are discussed: using this Theorem we find, eg.,
that diagonal matrix elements of the exact effective Hamiltonian for the
neutral meson complex can not be equal if CPT symmetry holds and CP symmetry is
violated. The Properties of time evolution governed by a time--independent
effective Hamiltonian acting in the neutral mesons subspace of states are
considered. By means of the Khalfin's Theorem we show that if such Hamiltonian
is time--independent then the evolution operator for the total system
containing neutral meson complex can not be a unitary operator. Within a given
specific model we examine numerically the Khalfin's Theorem. We show for this
model in a graphic form how the Khalfin's Theorem works. We also show for this
model how the difference of the mentioned diagonal matrix elements of the
effective Hamiltonian varies in time.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 15:52:30 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Urbanowski",
"K.",
""
]
] | [
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] |
712.0329 | Boris Kolev | Boris Kolev (LATP) | Point fixe li\'e \`a une orbite p\'eriodique d'un diff\'eomorphisme de
R2 | in French, 4 pages | Comptes Rendus de l'Academie des Sciences. Serie 1, Mathematique
310, 12 (1990) 831-833 | null | null | math.DS | null | Given a diffeomorphism of the plane, which has a periodic orbit, we show how
Nielsen fixed point theory can be used to establish the existence of a fixed
point which is linked with this periodic orbit.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 07:45:41 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Kolev",
"Boris",
"",
"LATP"
]
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712.033 | Leszek Prochniak | L. Prochniak | Collective excitations of transactinide nuclei in a self-consistent mean
field theory | 8 pages, 7 figures; presented at 14th Nuclear Physics Workshop
(Kazimierz Dolny, Poland, Sept. 2007) | Int.J.Mod.Phys.E17:160-167,2008 | 10.1142/S0218301308009653 | null | nucl-th | null | The ATDHFB approach has been applied for a study of properties of collective
quadrupole states in several transactinide nuclei: 238U, 240Pu, 242Pu, 246Cm,
248Cm, 250Cf and 252Cf. Calculated energies and B(E2) transition probabilities
are in a reasonable agreement with experimental data. Results concerning
superdeformed collective states in the 240Pu nucleus are also presented.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:08:07 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Prochniak",
"L.",
""
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712.0331 | Benjamin Girard | Benjamin Girard (CMLS-EcolePolytechnique) | A new upper bound for the cross number of finite Abelian groups | 21 pages, to appear in Israel Journal of Mathematics | Israel Journal of Mathematics 172 (2009) 253-278 | 10.1007/s11856-009-0072-3 | null | math.NT math.CO math.GR | null | In this paper, building among others on earlier works by U. Krause and C.
Zahlten (dealing with the case of cyclic groups), we obtain a new upper bound
for the little cross number valid in the general case of arbitrary finite
Abelian groups. Given a finite Abelian group, this upper bound appears to
depend only on the rank and on the number of distinct prime divisors of the
exponent. The main theorem of this paper allows us, among other consequences,
to prove that a classical conjecture concerning the cross and little cross
numbers of finite Abelian groups holds asymptotically in at least two different
directions.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:00:14 GMT"
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] | 2011-10-11T00:00:00 | [
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"Benjamin",
"",
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712.0332 | Dapeng Zhan | Dapeng Zhan | Duality of Chordal SLE | In this third version, the referee's suggestions are taken into
consideration. More details are added. Some typos are corrected. The paper
has been accepted by Inventiones Mathematicae | null | 10.1007/s00222-008-0132-z | null | math.PR | null | We derive some geometric properties of chordal SLE$(\kappa;\vec{\rho})$
processes. Using these results and the method of coupling two SLE processes, we
prove that the outer boundary of the final hull of a chordal
SLE$(\kappa;\vec{\rho})$ process has the same distribution as the image of a
chordal SLE$(\kappa';\vec{\rho'})$ trace, where $\kappa>4$,
$\kappa'=16/\kappa$, and the forces $\vec{\rho}$ and $\vec{\rho'}$ are suitably
chosen. We find that for $\kappa\ge 8$, the boundary of a standard chordal
SLE$(\kappa)$ hull stopped on swallowing a fixed $x\in\R\sem\{0\}$ is the image
of some SLE$(16/\kappa;\vec{\rho})$ trace started from $x$. Then we obtain a
new proof of the fact that chordal SLE$(\kappa)$ trace is not reversible for
$\kappa>8$. We also prove that the reversal of SLE$(4;\vec{\rho})$ trace has
the same distribution as the time-change of some SLE$(4;\vec{\rho'})$ trace for
certain values of $\vec{\rho}$ and $\vec{\rho'}$.
| [
{
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{
"version": "v3",
"created": "Fri, 14 Mar 2008 17:54:50 GMT"
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] |
712.0333 | Eric Adles | E. J. Adles, D. E. Aspnes | Application of the anisotropic bond model to second-harmonic generation
from amorphous media | 10 pages. Changed content in response to referee remarks. Expanded
discussion section. Added magnetic force term to force equation | Phys. Rev. B 77, 165102 (2008) | 10.1103/PhysRevB.77.165102 | null | physics.optics | null | As a step toward analyzing second-harmonic generation (SHG) from crystalline
Si nanospheres in glass, we develop an anisotropic bond model (ABM) that
expresses SHG in terms of physically meaningful parameters and provides a
detailed understanding of the basic physics of SHG on the atomic scale.
Nonlinear-optical (NLO) responses are calculated classically via the four
fundamental steps of optics: evaluate the local field at a given bond site,
solve the force equation for the acceleration of the charge, calculate the
resulting radiation, then superpose the radiation from all charges. The ABM
goes beyond previous bond models by including the complete set of underlying
contributions: retardation (RD), spatial-dispersion (SD), and magnetic (MG)
effects, in addition to the anharmonic restoring force acting on the bond
charge. We apply the ABM to obtain analytic expressions for SHG from amorphous
materials under Gaussian-beam excitation. These materials represent an
interesting test case not only because they are ubiquitous but also because the
anharmonic-force contribution that dominates the SHG response of crystalline
materials and ordered interfaces vanishes by symmetry. Using the paraxial-ray
approximation, we reduce the results to the isotropic case in two limits, that
where the linear restoring force dominates (glasses), and that where it is
absent (metals). Both forward- and backscattering geometries are discussed.
Estimated signal strengths and conversion efficiencies for fused silica appear
to be in general agreement with data, where available. Predictions are made
that allow additional critical tests of these results.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:06:54 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 21:44:40 GMT"
}
] | 2008-04-25T00:00:00 | [
[
"Adles",
"E. J.",
""
],
[
"Aspnes",
"D. E.",
""
]
] | [
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] |
712.0334 | Zhangjin Chen | XiaoXin Zhou, Zhangjin Chen, Toru Morishita, Anh-Thu Le, and C. D. Lin | Retrieval of electron-atom scattering cross sections from laser-induced
electron rescattering of atomic negative ions in intense laser fields | 6 papges, 5 figures | null | 10.1103/PhysRevA.77.053410 | null | physics.atom-ph | null | We investigated the two-dimensional electron momentum distributions of atomic
negative ions in an intense laser field by solving the time-dependent
Schrodinger equation (TDSE) and using the first- and 2nd-order strong-field
approximations (SFA). We showed that photoelectron energy distributions and
low-energy photoelectron momentum spectra predicted from SFA are in reasonable
agreement with the solutions from the TDSE. More importantly, we showed that
accurate electron-atom elastic scattering cross sections can be retrieved
directly from high-energy electron momentum spectra of atomic negative ions in
the laser field. This opens up the possibility of measuring electron-atom and
electron-molecule scattering cross sections from the photodetachment of atomic
and molecular negative ions by intense short lasers, respectively, with
temporal resolutions in the order of femtoseconds.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:08:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zhou",
"XiaoXin",
""
],
[
"Chen",
"Zhangjin",
""
],
[
"Morishita",
"Toru",
""
],
[
"Le",
"Anh-Thu",
""
],
[
"Lin",
"C. D.",
""
]
] | [
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] |
712.0335 | Andrey Pototsky | Andrey Pototsky and Natalia Janson | Excitable systems with noise and delay with applications to control:
renewal theory approach | null | null | 10.1103/PhysRevE.77.031113 | null | nlin.CD | null | We present an approach for the analytical treatment of excitable systems with
noise-induced dynamics in the presence of time delay. An excitable system is
modeled as a bistable system with a time delay, while another delay enters as a
control term taken after [Pyragas 1992] as a difference between the current
system state and its state "tau" time units before. This approach combines the
elements of renewal theory to estimate the essential features of the resulting
stochastic process as functions of the parameters of the controlling term.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:20:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Pototsky",
"Andrey",
""
],
[
"Janson",
"Natalia",
""
]
] | [
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] |
712.0336 | Daniel Andersson | Daniel Andersson, Boualem Djehiche | A maximum principle for relaxed stochastic control of linear SDE's with
application to bond portfolio optimization | 30 pages | null | null | null | math.OC | null | We study relaxed stochastic control problems where the state equation is a
one dimensional linear stochastic differential equation with random and
unbounded coefficients. The two main results are existence of an optimal
relaxed control and necessary conditions for optimality in the form of a
relaxed maximum principle. The main motivation is an optimal bond portfolio
problem in a market where there exists a continuum of bonds and the portfolio
weights are modeled as measure-valued processes on the set of times to
maturity.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:44:57 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 10:30:41 GMT"
}
] | 2008-02-15T00:00:00 | [
[
"Andersson",
"Daniel",
""
],
[
"Djehiche",
"Boualem",
""
]
] | [
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712.0337 | Tobias Galla | Tobias Galla, Andrea De Martino | On the transition to efficiency in Minority Games | 12 pages, 3 figures; contribution to the special issue "Viewing the
World through Spin Glasses" in honour of David Sherrington on the occasion of
his 65th birthday | null | 10.1088/1751-8113/41/32/324003 | null | physics.soc-ph cond-mat.dis-nn cond-mat.stat-mech q-fin.GN q-fin.TR | null | The existence of a phase transition with diverging susceptibility in batch
Minority Games (MGs) is the mark of informationally efficient regimes and is
linked to the specifics of the agents' learning rules. Here we study how the
standard scenario is affected in a mixed population game in which agents with
the `optimal' learning rule (i.e. the one leading to efficiency) coexist with
ones whose adaptive dynamics is sub-optimal. Our generic finding is that any
non-vanishing intensive fraction of optimal agents guarantees the existence of
an efficient phase. Specifically, we calculate the dependence of the critical
point on the fraction $q$ of `optimal' agents focusing our analysis on three
cases: MGs with market impact correction, grand-canonical MGs and MGs with
heterogeneous comfort levels.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:25:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Galla",
"Tobias",
""
],
[
"De Martino",
"Andrea",
""
]
] | [
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] |
712.0338 | Ettore Minguzzi | E. Minguzzi | Weak distinction and the optimal definition of causal continuity | 9 pages, 2 figures. v2: improved and expanded version. v3: a few
misprints have been corrected and a reference has been updated | Class.Quant.Grav.25:075015,2008 | 10.1088/0264-9381/25/7/075015 | null | gr-qc | null | Causal continuity is usually defined by imposing the conditions (i)
distinction and (ii) reflectivity. It is proved here that a new causality
property which stays between weak distinction and causality, called feeble
distinction, can actually replace distinction in the definition of causal
continuity. An intermediate proof shows that feeble distinction and future
(past) reflectivity implies past (resp. future) distinction. Some new
characterizations of weak distinction and reflectivity are given.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 16:41:13 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Dec 2007 20:12:38 GMT"
},
{
"version": "v3",
"created": "Thu, 20 Mar 2008 13:56:59 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Minguzzi",
"E.",
""
]
] | [
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712.0339 | Punyabrata Pradhan | Punyabrata Pradhan, Yariv Kafri, and Dov Levine | Non-equilibrium fluctuation theorems in the presence of local heating | 8 pages, 7 figures, revised and extended version, to appear in Phys.
Rev. E | Phys. Rev. E 77, 041129 (2008) | 10.1103/PhysRevE.77.041129 | null | cond-mat.stat-mech | null | We study two non-equilibrium work fluctuation theorems, the Crooks' theorem
and the Jarzynski equality, for a test system coupled to a spatially extended
heat reservoir whose degrees of freedom are explicitly modeled. The sufficient
conditions for the validity of the theorems are discussed in detail and
compared to the case of classical Hamiltonian dynamics. When the conditions are
met the fluctuation theorems are shown to hold despite the fact that the
immediate vicinity of the test system goes out of equilibrium during an
irreversible process. We also study the effect of the coupling to the heat
reservoir on the convergence of $<\exp(-\beta W)>$ to its theoretical mean
value, where $W$ is the work done on the test system and $\beta$ is the inverse
temperature. It is shown that the larger the local heating, the slower the
convergence.
| [
{
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{
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"created": "Thu, 3 Apr 2008 16:53:04 GMT"
}
] | 2010-02-22T00:00:00 | [
[
"Pradhan",
"Punyabrata",
""
],
[
"Kafri",
"Yariv",
""
],
[
"Levine",
"Dov",
""
]
] | [
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712.034 | Sean Dobbs | Kamal K. Seth | Challenges in Hadron Physics | 25 pages, 8 figures, summary talk for XII Conference on Hadron
Spectroscopy | null | null | null | hep-ex | null | The status of hadron physics at the end of the HADRON07 Conference is
reviewed. The latest results presented at the conference, as well as those
important developments in the field which were not represented, are included.
| [
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},
{
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] | 2007-12-05T00:00:00 | [
[
"Seth",
"Kamal K.",
""
]
] | [
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712.0341 | Jeremy Michelson | Steven G. Avery and Jeremy Michelson | Mechanics and Quantum Supermechanics of a Monopole Probe Including a
Coulomb Potential | 34 pages with 4 black&white eps figures. v2: Reference corrected and
a reference added. Figure files are significantly smaller; colour figures are
included with the source (use \colorfigtrue). v3: Reference added | Phys.Rev.D77:085001,2008 | 10.1103/PhysRevD.77.085001 | null | hep-th | null | A supersymmetric Lagrangian used to study D-particle probes in a D6-brane
background is exactly soluble. We present an analysis of the classical and
quantum mechanics of this theory, including classical trajectories in the
bosonic theory, and the exact quantum spectrum and wavefunctions, including
both bound and unbound states.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 18:57:36 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Dec 2007 20:57:01 GMT"
},
{
"version": "v3",
"created": "Fri, 4 Jan 2008 22:37:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Avery",
"Steven G.",
""
],
[
"Michelson",
"Jeremy",
""
]
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] |
712.0342 | C. Motch | C. Motch, A. M. Pires, F. Haberl, A. Schwope, V.E. Zavlin | Proper motions of ROSAT discovered isolated neutron stars measured with
Chandra: First X-ray measurement of the large proper motion of RX
J1308.6+2127/RBS 1223 | 3 pages, 2 figures, proceedings of the conference "40 Years of
Pulsars", 12-17 August 2007, Montreal, Canada | AIPConf.Proc.983:354-356,2008 | 10.1063/1.2900182 | null | astro-ph | null | The unprecedented spatial resolution of the Chandra observatory opens the
possibility to detect with relatively high accuracy proper motions at X-ray
wavelengths. We have conducted an astrometric study of three of the
"Magnificent Seven", the thermally emitting radio quiet isolated neutron stars
(INSs) discovered by ROSAT. These three INSs (RX J0420.0-5022, RX J0806.4-4123
and RX J1308.6+2127/RBS 1223) either lack an optical counterpart or have one
too faint to be used for astrometric purposes. We obtained ACIS observations 3
to 5 years apart to constrain or measure the displacement of the sources on the
X-ray sky using as reference the background of extragalactic or remote galactic
X-ray sources. Upper limits of 138 mas/yr and 76 mas/yr on the proper motion of
RX J0420.0-5022 and RX J0806.4-4123, respectively, have already been presented
in Motch et al. (2007). Here we report the very significant measurement (~ 10
sigma) of the proper motion of the third INS of our program, RX
J1308.6+2127/RBS1223. Comparing observations obtained in 2002 and 2007 reveals
a displacement of 1.1 arcsec implying a yearly proper motion of 223 mas, the
second fastest measured for the ROSAT discovered INSs. The source is rapidly
moving away from the galactic plane at a speed which precludes any significant
accretion of matter from the interstellar medium. Its transverse velocity of ~
740 (d/700pc) km/s might be the largest of the "Magnificent Seven" and among
the fastest recorded for neutron stars. RX J1308.6+2127/RBS1223 is thus a young
high velocity cooling neutron star. The source may have its origin in the
closest part of the Scutum OB2 association about 0.8 Myr ago, an age consistent
with that expected from cooling curves, but significantly younger than inferred
from pulse timing measurements (1.5 Myr).
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:46:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Motch",
"C.",
""
],
[
"Pires",
"A. M.",
""
],
[
"Haberl",
"F.",
""
],
[
"Schwope",
"A.",
""
],
[
"Zavlin",
"V. E.",
""
]
] | [
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712.0343 | P Ajith | P. Ajith | Gravitational-wave data analysis using binary black-hole waveforms | Minor modifications in the text, added table of phenomenological
coefficients | Class.Quant.Grav.25:114033,2008 | 10.1088/0264-9381/25/11/114033 | AEI-2007-169 | gr-qc astro-ph | null | Coalescing binary black-hole systems are among the most promising sources of
gravitational waves for ground-based interferometers. While the \emph{inspiral}
and \emph{ring-down} stages of the binary black-hole coalescence are
well-modelled by analytical approximation methods in general relativity, the
recent progress in numerical relativity has enabled us to compute accurate
waveforms from the \emph{merger} stage also. This has an important impact on
the search for gravitational waves from binary black holes. In particular,
while the current gravitational-wave searches look for each stage of the
coalescence separately, combining the results from analytical and numerical
relativity enables us to \emph{coherently} search for all three stages using a
single template family. `Complete' binary black-hole waveforms can now be
produced by matching post-Newtonian waveforms with those computed by numerical
relativity. These waveforms can be parametrised to produce analytical waveform
templates. The `complete' waveforms can also be used to estimate the efficiency
of different search methods aiming to detect signals from black-hole
coalescences. This paper summarises some recent efforts in this direction.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:01:35 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Mar 2008 20:54:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ajith",
"P.",
""
]
] | [
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] |
712.0344 | Sean Dobbs | Kamal K. Seth | Charm at CLEO-c | 4 pages, 2 pages, presented at XV International Workshop on
Deep-Inelastic Scattering and Related Subjects | null | null | null | hep-ex | null | A minireview of the recent results from CLEO-c is presented. It includes new
results in charmonium spectroscopy, charmonium-like exotics, and open-charm
decays.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:03:12 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Seth",
"Kamal K.",
""
]
] | [
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712.0345 | Lars Mattsson | Lars Mattsson, Brady Caldwell, Nils Bergvall | The Chemical Evolution of LSB Galaxies | 2 pages, 1 figure. To appear in the proceedings of "Formation and
Evolution of Galaxy Disks" (J. G. Funes, and E. M. Corsini eds) | null | null | null | astro-ph | null | We have derived oxygen and nitrogen abundances of a sample of late-type, low
surface brightness (LSB) galaxies found in the Sloan Digital Sky Survey (SDSS).
Furthermore, we have computed a large grid (5000 models) of chemical evolution
models (CEMs) testing various time-scales for infall, baryon densities and
several power-law initial mass functions (IMFs) as well. Because of the rather
stable N/O-trends found both in CEMs (for a given IMF) and in observations, we
find that the hypotheses that LSB galaxies have stellar populations dominated
by low-mass stars, i.e., very bottom-heavy IMFs (see Lee et al. 2004), can be
ruled out. Such models predict much too high N/O-ratios and generally too low
O/H-ratios. We also conclude that LSB galaxies probably have the same ages as
their high surface brightness counterparts, although the global rate of star
formation must be considerably lower in these galaxies.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:09:20 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Mattsson",
"Lars",
""
],
[
"Caldwell",
"Brady",
""
],
[
"Bergvall",
"Nils",
""
]
] | [
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] |
712.0346 | Beatrix Hiesmayr C. | Beatrix C. Hiesmayr and Marcus Huber | Multipartite entanglement measure for all discrete systems | Extended version including explicitly the 3 qubit case, 7 pages, 3
figures | Phys. Rev. A 78, 012342 (2008). | 10.1103/PhysRevA.78.012342 | null | quant-ph | null | Via a multidimensional complementarity relation we derive a novel operational
entanglement measure for any discrete quantum system, i.e. for any
multidimensional and multipartite system. This new measure admits a separation
into different classes of entanglement obtained by using a flip operator
2,3,...,n times, defining a m-flip concurrence. For mixed states bounds on this
m-flip concurrence can be obtained. Moreover, the information content of a n
partite multidimensional system admits an intuitive interpretation. Explicitly,
the three qubits system is analyzed and the physical difference in entanglement
of the W-state, the GHZ state or the bi-separable state is revealed.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:20:20 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Apr 2008 09:58:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hiesmayr",
"Beatrix C.",
""
],
[
"Huber",
"Marcus",
""
]
] | [
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] |
712.0347 | Zhi-Yong Wang | Zhi-Yong Wang, Cai-Dong Xiong, Bing He | Superluminal propagation of evanescent modes as a quantum effect | Also as a Reply to the Comment by H. G. Winful [Phys. Rev. A 76,
057803 (2007)], to be published in Annalen der Physik | Ann. Phys. (Berlin) 17, No. 5, 319-325 (2008) | 10.1002/andp.200710288 | null | quant-ph | null | Contrary to mechanical waves, the two-slit interference experiment of single
photons shows that the behavior of classical electromagnetic waves corresponds
to the quantum mechanical one of single photons, which is also different from
the quantum-field-theory behavior such as the creations and annihilations of
photons, the vacuum fluctuations, etc. Owing to a purely quantum effect,
quantum tunneling particles including tunneling photons (evanescent modes) can
propagate over a spacelike interval without destroying causality. With this
picture we conclude that the superluminality of evanescent modes is a quantum
mechanical rather than a classical phenomenon.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:12:06 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Dec 2007 05:05:47 GMT"
},
{
"version": "v3",
"created": "Mon, 25 Feb 2008 12:13:11 GMT"
},
{
"version": "v4",
"created": "Tue, 8 Apr 2008 07:45:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wang",
"Zhi-Yong",
""
],
[
"Xiong",
"Cai-Dong",
""
],
[
"He",
"Bing",
""
]
] | [
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712.0348 | Miguel Aguado | Miguel Aguado, Guifre Vidal | Entanglement renormalization and topological order | 6 pages, 17 eps files. v2: References updated, typos corrected.
Includes appendix not in published version | Phys. Rev. Lett. 100, 070404 (2008) | 10.1103/PhysRevLett.100.070404 | null | cond-mat.str-el quant-ph | null | The multi-scale entanglement renormalisation ansatz (MERA) is argued to
provide a natural description for topological states of matter. The case of
Kitaev's toric code is analyzed in detail and shown to possess a remarkably
simple MERA description leading to distillation of the topological degrees of
freedom at the top of the tensor network. Kitaev states on an infinite lattice
are also shown to be a fixed point of the RG flow associated with entanglement
renormalization. All these results generalize to arbitrary quantum double
models.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:12:06 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 22:52:05 GMT"
}
] | 2008-02-22T00:00:00 | [
[
"Aguado",
"Miguel",
""
],
[
"Vidal",
"Guifre",
""
]
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712.0349 | Mark Andrea de Cataldo | Mark Andrea de Cataldo, Luca Migliorini | The Decomposition Theorem and the topology of algebraic maps | 117 pages. New title. Major structure changes. Final version of a
survey to appear in the Bulletin of the AMS | null | null | null | math.AG math.AT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a motivated introduction to the theory of perverse sheaves,
culminating in the Decomposition Theorem of Beilinson, Bernstein, Deligne and
Gabber. A goal of this survey is to show how the theory develops naturally from
classical constructions used in the study of topological properties of
algebraic varieties. While most proofs are omitted, we discuss several
approaches to the Decomposition Theorem, indicate some important applications
and examples.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:15:01 GMT"
},
{
"version": "v2",
"created": "Thu, 16 Apr 2009 17:36:42 GMT"
}
] | 2009-04-16T00:00:00 | [
[
"de Cataldo",
"Mark Andrea",
""
],
[
"Migliorini",
"Luca",
""
]
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] |
712.035 | Jerzy Lukierski | Marcin Daszkiewicz, Jerzy Lukierski and Mariusz Woronowicz | Quantization of kappa-deformed free fields and kappa-deformed
oscillators | 9 pages. Talk presented at Supersymmetry and Quantum Supersymmetry
2007 (SQS'07) Conference (Dubna, 30.07-4.08.2007) and IV-th Central European
Seminar "Commutative and Noncommutative Quantum Fields" (Vienna,
30.11-2.12.2007). To be published in the proceedings of SQS'07 (2008) | null | null | null | hep-th | null | We describe the deformed E.T. quantization rules for kappa-deformed free
quantum fields, and relate these rules with the kappa-deformed algebra of field
oscillators.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:15:55 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Daszkiewicz",
"Marcin",
""
],
[
"Lukierski",
"Jerzy",
""
],
[
"Woronowicz",
"Mariusz",
""
]
] | [
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] |
712.0351 | Li-Ming Si | Li-Ming Si | Improved Time Domain Method to Measure Near-Field Distribution of
Buried-Object | 8 pages, 5 figures | null | null | null | physics.class-ph | null | The paper analyses the ground antenna echo using microwave frequency detector
and high speed sampling technology and a new method detecting buried object in
time domain near-field is presented. The method detecting particular reflection
echo frequency of microwave pulse via digital signal processing is to reduce
the false alarm rate. Simulation results show that this method has advantages
of easy identification and high precision.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 18:15:44 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Si",
"Li-Ming",
""
]
] | [
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] |
712.0352 | Xinwen Shu | X. W. Shu, J. X. Wang, P. Jiang (Center for Astrophysics, USTC) | Are Seyfert 2 Galaxies without Polarized Broad Emission Lines More
Obscured? | 9 pages with 3 figures, accepted by ChJAA | null | 10.1088/1009-9271/8/2/07 | null | astro-ph | null | The new $XMM-Newton$ data of seven Seyfert 2 galaxies with optical
spectropolarimetric observations are presented. The analysis of 0.5 -- 10 keV
spectra shows that all four Seyfert 2 galaxies with polarized broad lines
(PBLs) are absorbed with $N_{\rm H}<10^{24}$ cm$^{-2}$, while two of three
Seyfert 2 galaxies without PBLs have evidence suggesting Compton-thick
obscuration, supporting the conclusion that Seyfert 2 galaxies without PBLs are
more obscured than those with PBLs. Adding the measured obscuration indicators
($N_{\rm H}$, $T$ ratio, and Fe K$\alpha$ line EW) of six luminous AGNs to our
previous sample improves the significance level of the difference in absorption
from 92.3% to 96.3% for $N_{\rm H}$, 99.1% to 99.4% for $T$ ratio, and 95.3% to
97.4% for Fe K$\alpha$ line EW. The present results support and enhance the
suggestions that the absence of PBLs in Seyfert 2 galaxies can be explained by
larger viewing angle of line of sight to the putative dusty torus, which lead
to the obscuration of broad-line scattering screen, as expected by the
unification model.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:18:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shu",
"X. W.",
"",
"Center for Astrophysics, USTC"
],
[
"Wang",
"J. X.",
"",
"Center for Astrophysics, USTC"
],
[
"Jiang",
"P.",
"",
"Center for Astrophysics, USTC"
]
] | [
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] |
712.0353 | Burkhard Zink | Burkhard Zink, Erik Schnetter, Manuel Tiglio | Multi-patch methods in general relativistic astrophysics - I.
Hydrodynamical flows on fixed backgrounds | 26 pages, 20 figures. A high-resolution version is available at
http://www.cct.lsu.edu/~bzink/papers/multipatch_1.pdf | Phys.Rev.D77:103015,2008 | 10.1103/PhysRevD.77.103015 | null | astro-ph astro-ph.HE gr-qc | null | Many systems of interest in general relativistic astrophysics, including
neutron stars, accreting compact objects in X-ray binaries and active galactic
nuclei, core collapse, and collapsars, are assumed to be approximately
spherically symmetric or axisymmetric. In Newtonian or fixed-background
relativistic approximations it is common practice to use spherical polar
coordinates for computational grids; however, these coordinates have
singularities and are difficult to use in fully relativistic models. We
present, in this series of papers, a numerical technique which is able to use
effectively spherical grids by employing multiple patches. We provide detailed
instructions on how to implement such a scheme, and present a number of code
tests for the fixed background case, including an accretion torus around a
black hole.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:45:10 GMT"
}
] | 2010-11-16T00:00:00 | [
[
"Zink",
"Burkhard",
""
],
[
"Schnetter",
"Erik",
""
],
[
"Tiglio",
"Manuel",
""
]
] | [
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] |
712.0354 | Tanja Branz | Tanja Branz, Thomas Gutsche, Valery E. Lyubovitskij | f0(980) meson as a K bar K molecule in a phenomenological Lagrangian
approach | 21 pages, 11 figures, revised version accepted for publication in
Eur. Phys. J. A | Eur.Phys.J.A37:303-317,2008 | 10.1140/epja/i2008-10635-1 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss a possible interpretation of the f0(980) meson as a hadronic
molecule - a bound state of K and bar K mesons. Using a phenomenological
Lagrangian approach we calculate the strong f0(980) to pi pi and
electromagnetic f0(980) to gamma gamma decays. The compositeness condition
provides a self-consistent method to determine the coupling constant between f0
and its constituents, K and bar K. Form factors governing the decays of the
f0(980) are calculated by evaluating the kaon loop integrals. The predicted
f0(980) to pi pi and f0(980) to gamma gamma decay widths are in good agreement
with available data and results of other theoretical approaches.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:56:47 GMT"
},
{
"version": "v2",
"created": "Thu, 7 Aug 2008 11:01:35 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Branz",
"Tanja",
""
],
[
"Gutsche",
"Thomas",
""
],
[
"Lyubovitskij",
"Valery E.",
""
]
] | [
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] |
712.0355 | Marvin D. Girardeau | M.D. Girardeau, E.M. Wright | Bright and dark solitary waves in a one-dimensional spin-polarized gas
of fermionic atoms with p-wave interactions in a hard-wall trap | 4 pages+, 3 figures, revtex4. Submitted to PRL | null | 10.1103/PhysRevA.77.043612 | null | cond-mat.other | null | In this paper we elucidate the physics underlying the fact that both bright
and dark solitary waves can arise in a one-dimensional spin-polarized gas of
fermionic atoms with attractive three-dimensional p-wave interactions in a
hard-wall trap. This is possible since the one-dimensional fermion system can
be mapped to a system of bosons described by the Lieb-Liniger model with either
repulsive or attractive delta-function interactions which can support solitary
waves.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 18:08:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Girardeau",
"M. D.",
""
],
[
"Wright",
"E. M.",
""
]
] | [
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712.0356 | Sean Dobbs | Kamal K. Seth | Timelike Form Factors | 9 pages, 4 figures, presented at Exclusive Reactions at High Momentum
Transfer 2007 | null | 10.1142/9789812796950_0035 | null | hep-ex | null | Form factors of nucleons and mesons with timelike momentum transfers are
discussed. New experimental results for protons, pions, and kaons at large
momentum transfers are presented, and the inadequacy of existing theoretical
ideas about these is pointed out.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:34:10 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Seth",
"Kamal K.",
""
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712.0357 | Francesco Prino | F. Prino | Charged particle pseudorapidity distributions from SPS to LHC | Proceedings of XLIV Intern. Winter Meeting on Nucl. Phys., Bormio,
January 06 | null | null | null | nucl-ex | null | Pseudorapidity distributions of charged particles produced in heavy ion
collisions are a powerful tool to characterize the global properties of the
created system. They have been measured in a wide range of energies at the GSI,
AGS, SPS and RHIC accelerators and will be one of the first measurements at
ALICE at the LHC. The various analysis techniques developed by SPS and RHIC
experiments are reviewed and the presently available results from SPS and RHIC
are presented, focusing in particular on the scaling of charged particle yield
with centrality and with center-of-mass energy. Finally the perspectives for
the multiplicity measurement in the ALICE experiment at the LHC are discussed.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:35:08 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Prino",
"F.",
""
]
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712.0358 | Stephen Kane | Stephen R. Kane, Eric B. Ford, Jian Ge | Cadence Optimisation and Exoplanetary Parameter Sensitivity | 4 pages, 5 figures, corrected typo, to appear in the Proceedings of
the 249th IAU Meeting: "Exoplanets: Detection, Formation and Dynamics"
(Suzhou, China) | null | 10.1017/S1743921308016487 | null | astro-ph | null | To achieve maximum planet yield for a given radial velocity survey, the
observing strategy must be carefully considered. In particular, the adopted
cadence can greatly affect the sensitivity to exoplanetary parameters such as
period and eccentricity. Here we describe simulations which aim to maximise
detections based upon the target parameter space of the survey.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:43:34 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 19:29:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kane",
"Stephen R.",
""
],
[
"Ford",
"Eric B.",
""
],
[
"Ge",
"Jian",
""
]
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] |
712.0359 | Jaroslav Ilnytskyi Dr. | J.M.Ilnytskyi and Yu.Holovatch | How does the scaling for the polymer chain in the dissipative particle
dynamics hold? | 12 pages, 6 figs | Condens. Matter Phys., vol. 10 (2007) 539-552 | null | null | cond-mat.soft | null | We performed a series of simulations for a linear polymer chain in a solvent
using dissipative particle dynamics to check the scaling relations for the
end-to-end distance, radius of gyration and hydrodynamic radius in three
dimensions. The polymer chains of up to 80 beads in explicit solvent of various
quality are studied. To extract the scaling exponent \nu, the data are analyzed
using linear fits, correction-to-scaling forms and analytical fits to the
histograms of radius of gyration distribution. For certain combinations of the
polymer characteristics and solvent quality, the correction-to-scaling terms
are found to be essential while for the others these are negligibly small. In
each particular case the final value for the exponent \nu was chosen according
to the best least-squares fit. The values of \nu obtained in this way are found
within the interval \nu=0.55-0.61 but are concentrated mostly around 0.59,
which is very close to the best known theoretical result \nu=0.588. The
existence of this interval is attributed both to the peculiarities of the
method and to the moderate chain lengths being simulated. Within this
shortcoming, the polymer chain in this kind of modeling is found to satisfy the
scaling relations for all three radii being considered
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:51:56 GMT"
}
] | 2009-04-03T00:00:00 | [
[
"Ilnytskyi",
"J. M.",
""
],
[
"Holovatch",
"Yu.",
""
]
] | [
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] |
712.036 | Dmitri Vassilevich | R. A. Konoplya, D. V. Vassilevich | Quantum corrections to the noncommutative kink | 18 pages, v2: minor changes | JHEP0801:068,2008 | 10.1088/1126-6708/2008/01/068 | null | hep-th | null | We calculate quantum corrections to the mass of noncommutative phi^4 kink in
(1+1) dimensions for intermediate and large values of the noncommutativity
parameter theta. All one-loop divergences are removed by a mass renormalization
(which is different from the one required in the topologically trivial sector).
For large theta quantum corrections to the mass grow linearly with theta
signaling about possible break down of the perturbative expansion.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 17:56:07 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jan 2008 19:11:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Konoplya",
"R. A.",
""
],
[
"Vassilevich",
"D. V.",
""
]
] | [
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712.0361 | Ayres Freitas | F. Deppisch, A. Freitas, W. Porod, P.M. Zerwas | Determining Heavy Mass Parameters in Supersymmetric SO(10) Models | 26 pp LaTeX; version published in Phys. Rev. D | Phys.Rev.D77:075009,2008 | 10.1103/PhysRevD.77.075009 | ANL-HEP-PR-07-98, DESY 07-199, LPT-ORSAY 07-109, MAN/HEP/2007/26,
PITHA 07/15 | hep-ph | null | Extrapolations of soft scalar mass parameters in supersymmetric theories can
be used to explore elements of the physics scenario near the grand unification
scale. We investigate the potential of this method in the lepton sector of
SO(10) which incorporates right-handed neutrino superfields. The method is
exemplified in two models by exploring limits on the precision that can be
expected from coherent LHC and e+e- collider analyses in the reconstruction of
the fundamental scalar mass parameters at the unification scale and of the
D-terms related to the breaking of grand unification symmetries. In addition,
the mass of the third-generation right-handed neutrino can be estimated in
seesaw scenarios. Even though the models are simplified and not intended to
account for all aspects of a final comprehensive SO(10) theory, they provide
nevertheless a valid base for identifying essential elements that can be
inferred on the fundamental high-scale theory from high-energy experiments.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 18:02:03 GMT"
},
{
"version": "v2",
"created": "Thu, 1 May 2008 15:34:27 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Deppisch",
"F.",
""
],
[
"Freitas",
"A.",
""
],
[
"Porod",
"W.",
""
],
[
"Zerwas",
"P. M.",
""
]
] | [
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712.0362 | Abdelmalek Salem Dr | Kouachi Said, Abdelmalek Salem, and Rebiai Belgacem | A Mathematical Proof of Dodgson's Algorithm | 6 pages | null | null | null | math.CO | null | In this paper we give a mathematical proof of Dodgson algorithm [1]. Recently
Zeilberger [2] gave a bijective proof. Our techniques are based on determinant
properties and they are obtained by induction.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:30:11 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Said",
"Kouachi",
""
],
[
"Salem",
"Abdelmalek",
""
],
[
"Belgacem",
"Rebiai",
""
]
] | [
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] |
712.0363 | Peter Zeiner | M. Baake, P. Zeiner | Coincidences in 4 dimensions | 6 pages, conference "Quasicrystals - The Silver Jubilee" | Phil. Mag. 88 (2008), 2025-2032 | 10.1080/14786430701264186 | null | math.MG math.CO | null | The coincidence site lattices (CSLs) of prominent 4-dimensional lattices are
considered. CSLs in 3 dimensions have been used for decades to describe grain
boundaries in crystals. Quasicrystals suggest to also look at CSLs in
dimensions $d>3$. Here, we discuss the CSLs of the root lattice $A_4$ and the
hypercubic lattices, which are of particular interest both from the
mathematical and the crystallographic viewpoint. Quaternion algebras are used
to derive their coincidence rotations and the CSLs. We make use of the fact
that the CSLs can be linked to certain ideals and compute their indices, their
multiplicities and encapsulate all this in generating functions in terms of
Dirichlet series. In addition, we sketch how these results can be generalised
for 4--dimensional $\Z$--modules by discussing the icosian ring.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:36:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Baake",
"M.",
""
],
[
"Zeiner",
"P.",
""
]
] | [
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712.0364 | Sidney Redner | R. Lambiotte and S. Redner | Dynamics of Non-Conservative Voters | 4 pages, 4 figures, 2-column revtex4 format; a minor typo in Eq. (16)
fixed; current version is the final published manuscript that contains minor
changes in response to referee comments | Europhysics Letters 82, 18007 (2008) | 10.1209/0295-5075/82/18007 | null | physics.data-an cond-mat.stat-mech physics.ed-ph | null | We study a family of opinion formation models in one dimension where the
propensity for a voter to align with its local environment depends non-linearly
on the fraction of disagreeing neighbors. Depending on this non-linearity in
the voting rule, the population may exhibit a bias toward zero magnetization or
toward consensus, and the average magnetization is generally not conserved. We
use a decoupling approximation to truncate the equation hierarchy for
multi-point spin correlations and thereby derive the probability to reach a
final state of a given consensus as a function of the initial magnetization.
The case when voters are influenced by more distant voters is also considered
by investigating the Sznajd model.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:43:08 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Dec 2007 12:18:37 GMT"
},
{
"version": "v3",
"created": "Tue, 22 Apr 2008 23:45:53 GMT"
}
] | 2008-04-23T00:00:00 | [
[
"Lambiotte",
"R.",
""
],
[
"Redner",
"S.",
""
]
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712.0365 | J. Antonio Garcia Zenteno | Ignacio Cortese and J. Antonio Garcia | Comment on ''A path integral leading to higher-order Lagrangians,
arXiv:0708.4351 [hep-th]'' | Latex, 3 pages | null | null | null | hep-th | null | We show that the ``effective Lagrangian'' constructed in [1] is inconsistent
with the exact result for the complete Lagrangian presented in [2]. We trace
the origin of the inconsistence to the peculiar way in which the path integral
methods are used to eliminate variables that are not auxialiry.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:04:32 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Cortese",
"Ignacio",
""
],
[
"Garcia",
"J. Antonio",
""
]
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] |
712.0366 | Sudhakar Yarlagadda | Sudhakar Yarlagadda | Cooperative electron-phonon interaction in molecular chains | Added Jahn-Teller system | null | null | null | cond-mat.str-el cond-mat.mtrl-sci | null | Using a controlled analytic treatment, we derive a model that generically
describes cooperative strong electron-phonon interaction (EPI) in one-band and
two-band Jahn-Teller (JT) systems. The model involves a {\em
next-nearest-neighbor} hopping and a nearest-neighbor repulsion. Rings with odd
number of sites (o-rings) belong to a different universality class compared to
rings with even number (e-rings). The e-rings, upon tuning repulsion, undergo a
dramatic discontinuous transition to a {\em conducting commensurate} charge
density wave (CDW) state with a period independent of filling.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:53:41 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Mar 2008 23:46:29 GMT"
}
] | 2008-03-04T00:00:00 | [
[
"Yarlagadda",
"Sudhakar",
""
]
] | [
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712.0367 | Zhihui Wang | Zhihui Wang, Christina M. Birch, Thomas S. Deisboeck | Cross-Scale Sensitivity Analysis of a Non-Small Cell Lung Cancer Model:
Linking Molecular Signaling Properties to Cellular Behavior | 30 pages, 6 figures, 2 tables | null | null | null | q-bio.QM | null | Sensitivity analysis is an effective tool for systematically identifying
specific perturbations in parameters that have significant effects on the
behavior of a given biosystem, at the scale investigated. In this work, using a
two-dimensional, multiscale non-small cell lung cancer (NSCLC) model, we
examine the effects of perturbations in system parameters which span both
molecular and cellular levels, i.e. across scales of interest. This is achieved
by first linking molecular and cellular activities and then assessing the
influence of parameters at the molecular level on the tumor's spatio-temporal
expansion rate, which serves as the output behavior at the cellular level.
Overall, the algorithm operated reliably over relatively large variations of
most parameters, hence confirming the robustness of the model. However, three
pathway components (proteins PKC, MEK, and ERK) and eleven reaction steps were
determined to be of critical importance by employing a sensitivity coefficient
as an evaluation index. Each of these sensitive parameters exhibited a similar
changing pattern in that a relatively larger increase or decrease in its value
resulted in a lesser influence on the system's cellular performance. This study
provides a novel cross-scaled approach to analyzing sensitivities of
computational model parameters and proposes its application to
interdisciplinary biomarker studies.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:57:27 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Wang",
"Zhihui",
""
],
[
"Birch",
"Christina M.",
""
],
[
"Deisboeck",
"Thomas S.",
""
]
] | [
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712.0368 | Mariola Ramirez | Mariola O. Ramirez, M. Krishnamurthi, S. Denev, A. Kumar, Seung-Yeul
Yang, Ying-Hao Chu, Eduardo Saiz, Jan Seidel, A.P Pyatakov, A.Bush, D.
Viehland, J. Orenstein, R. Ramesh, Venkatraman Gopalan | Two-phonon coupling to the antiferromagnetic phase transition in
multiferroic BiFeO3 | 12 pages with figures | null | 10.1063/1.2829681 | null | cond-mat.other | null | A prominent band centered at around 1000-1300 cm-1 and associated with
resonant enhancement of two-phonon Raman scattering is reported in multiferroic
BiFeO3 thin films and single crystals. A strong anomaly in this band occurs at
the antiferromagnetic Neel temperature. This band is composed of three peaks,
assigned to 2A4, 2E8, and 2E9 Raman modes. While all three peaks were found to
be sensitive to the antiferromagnetic phase transition, the 2E8 mode, in
particular, nearly disappears at TN on heating, indicating a strong spin-two
phonon coupling in BiFeO3.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:58:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ramirez",
"Mariola O.",
""
],
[
"Krishnamurthi",
"M.",
""
],
[
"Denev",
"S.",
""
],
[
"Kumar",
"A.",
""
],
[
"Yang",
"Seung-Yeul",
""
],
[
"Chu",
"Ying-Hao",
""
],
[
"Saiz",
"Eduardo",
""
],
[
"Seidel",
"Jan",
""
],
[
"Pyatakov",
"A. P",
""
],
[
"Bush",
"A.",
""
],
[
"Viehland",
"D.",
""
],
[
"Orenstein",
"J.",
""
],
[
"Ramesh",
"R.",
""
],
[
"Gopalan",
"Venkatraman",
""
]
] | [
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] |
712.0369 | Iain Hannah | I. G. Hannah, S. Krucker, H. S. Hudson, S. Christe, R. P. Lin | An Intriguing Solar Microflare Observed with RHESSI, Hinode and TRACE | 4 pages, 5 figures, accepted by A&A | null | 10.1051/0004-6361:20079019 | null | astro-ph astro-ph.SR | null | Investigate particle acceleration and heating in a solar microflare. In a
microflare with non-thermal emission to remarkably high energies ($>50$ keV),
we investigate the hard X-rays with RHESSI imaging and spectroscopy and the
resulting thermal emission seen in soft X-rays with Hinode/XRT and in EUV with
TRACE. The non-thermal footpoints observed with RHESSI spatially and temporally
match bright footpoint emission in soft X-rays and EUV. There is the
possibility that the non-thermal spectrum extends down to 4 keV. The hard X-ray
burst clearly does not follow the expected Neupert effect, with the time
integrated hard X-rays not matching the soft X-ray time profile. So although
this is a simple microflare with good X-ray observation coverage it does not
fit the standard flare model.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 19:59:47 GMT"
}
] | 2010-09-17T00:00:00 | [
[
"Hannah",
"I. G.",
""
],
[
"Krucker",
"S.",
""
],
[
"Hudson",
"H. S.",
""
],
[
"Christe",
"S.",
""
],
[
"Lin",
"R. P.",
""
]
] | [
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] |
712.037 | Tirthabir Biswas | Stephon Alexander, Tirthabir Biswas, Alessio Notari and Deepak Vaid | Local Void vs Dark Energy: Confrontation with WMAP and Type Ia
Supernovae | Minor numerical errors and typos corrected, references added | JCAP 0909:025,2009 | 10.1088/1475-7516/2009/09/025 | IGPG-07/2-1 | astro-ph hep-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | It is now a known fact that if we happen to be living in the middle of a
large underdense region, then we will observe an "apparent acceleration", even
when any form of dark energy is absent. In this paper, we present a "Minimal
Void" scenario, i.e. a "void" with minimal underdensity contrast (of about
-0.4) and radius (~ 200-250 Mpc/h) that can, not only explain the supernovae
data, but also be consistent with the 3-yr WMAP data. We also discuss
consistency of our model with various other measurements such as Big Bang
Nucleosynthesis, Baryon Acoustic Oscillations and local measurements of the
Hubble parameter, and also point out possible observable signatures.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:05:43 GMT"
},
{
"version": "v2",
"created": "Sat, 1 Mar 2008 22:50:56 GMT"
},
{
"version": "v3",
"created": "Wed, 1 Apr 2009 00:07:49 GMT"
}
] | 2009-09-24T00:00:00 | [
[
"Alexander",
"Stephon",
""
],
[
"Biswas",
"Tirthabir",
""
],
[
"Notari",
"Alessio",
""
],
[
"Vaid",
"Deepak",
""
]
] | [
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] |
712.0371 | Bert Schroer | Bert Schroer | Jorge A. Swieca's contributions to quantum field theory in the 60s and
70s and their relevance in present research | 49 pages, expansion and actualization of text, improvement of
formulations and addition of many references to be published in EPJH -
Historical Perspectives on Contemporary Physics | Eur.Phys.J.H35:53-88,2010 | 10.1140/epjh/e2010-00004-1 | null | physics.hist-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | After revisiting some high points of particle physics and QFT of the two
decades from 1960 to 1980, I comment on the work by Jorge Andre Swieca. I
explain how it fits into the quantum field theory during these two decades and
draw attention to its relevance to the ongoing particle physics research. A
particular aim of this article is to direct thr readers mindfulness to the
relevance of what at the time of Swieca was called "the Schwinger Higgs
screening mechanism". which, together with recent ideas which generalize the
concept of gauge theories, has all the ingredients to revolutionize the issue
of gauge theories and the standard model.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:38:02 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 20:22:05 GMT"
},
{
"version": "v3",
"created": "Mon, 10 May 2010 12:50:38 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Schroer",
"Bert",
""
]
] | [
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] |
712.0372 | Choukrallah Reda | Reda Choukrallah | Functions with support in a lacunary system of intervals and cyclicity
for the semi-group of left translations | null | null | null | null | math.SP | null | We prove in the vector-valued spaces $L^2(\mathbb{R}_+, X)$ (where $X$ is a
finite dimensional Hilbert space) the cyclicity for the semi-group of left
translations of some particular functions with support included in a lacunary
system of intervals.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:18:58 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 14:22:38 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Choukrallah",
"Reda",
""
]
] | [
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] |
712.0373 | Rodrigo Alves Dias Dias R. A. | R.A. Dias, P. Z. Coura, M. Rapini, B.V. Costa | Velocity, temperature and normal force dependence on friction: An
analytical and molecular dynamic study | null | null | null | null | physics.comp-ph physics.class-ph | null | In this work we propose an extension to the analytical one-dimensional model
proposed by E. Gnecco (Phys. Rev. Lett. 84:1172) to describe friction. Our
model includes normal forces and the dependence with the angular direction of
movement in which the object is dragged over a surface. The presence of the
normal force in the model allow us to define judiciously the friction
coefficient, instead of introducing it as an {\sl a posteriori} concept. We
compare the analytical results with molecular dynamics simulations. The
simulated model corresponds to a tip sliding over a surface. The tip is
simulated as a single particle interacting with a surface through a
Lennard-Jones $(6-12)$ potential. The surface is considered as consisting of a
regular BCC(001) arrangement of particles interacting with each other through a
Lennard-Jones $(6-12)$ potential. We investigate the system under several
conditions of velocity, temperature and normal forces. Our analytical results
are in very good agreement with those obtained by the simulations and with
experimental results from E. Riedo (Phys. Rev. Lett. 91:084502) and Eui-Sung
Yoon (Wear 259:1424-1431) as well.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:26:13 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Dias",
"R. A.",
""
],
[
"Coura",
"P. Z.",
""
],
[
"Rapini",
"M.",
""
],
[
"Costa",
"B. V.",
""
]
] | [
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712.0374 | Jean Cortissoz | Jean Cortissoz | Global regular solutions for the Navier-stokes system with small initial
data in $\Phi(2)$: an elementary approach | 13 pages, title has been changed, some bugs have been corrected, and
new comments in the last section have been added | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show existence and regularity result for the Navier Stokes system for
small data in the space $\Phi(2)$, and we show relations with some classical
results.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:42:03 GMT"
},
{
"version": "v2",
"created": "Tue, 3 Mar 2009 13:02:03 GMT"
}
] | 2009-03-03T00:00:00 | [
[
"Cortissoz",
"Jean",
""
]
] | [
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712.0375 | Matvei Libine | Matvei Libine | Hyperbolic Cauchy Integral Formula for the Split Complex Numbers | null | null | null | null | math-ph math.MP | null | In our joint papers [FL1-FL2] we revive quaternionic analysis and show deep
relations between quaternionic analysis, representation theory and
four-dimensional physics. As a guiding principle we use representation theory
of various real forms of the conformal group. We demonstrate that the
requirement of unitarity of representations naturally leads us to the
extensions of the Cauchy-Fueter and Poisson formulas to the Minkowski space,
which can be viewed as another real form of quaternions. However, the Minkowski
space formulation also brings some technical difficulties related to the fact
that the singularities of the kernels in these integral formulas are now
concentrated on the light cone instead of just a single point in the initial
quaternionic picture. But the same phenomenon occurs when one passes from the
complex numbers to the split complex numbers (or hyperbolic algebra). So, as a
warm-up example we proved an analogue of the Cauchy integral formula for the
split complex numbers. On the other hand, there seems to be sufficient interest
in such formula among physicists. For example, see [KS] and the references
therein.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:37:43 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Libine",
"Matvei",
""
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] |
712.0376 | Esteban Calzetta | E. Calzetta | Analog cosmology with spinor Bose-Einstein condensates | 8 pages. Fixed typos and updated references | null | null | null | cond-mat.other | null | It is well known that both a particle with spin and a quantum field in a
Bianchi type IX Universe are both related to the quantum mechanical top. In
this paper we will combine these insights to show that the dynamics of a cold
gas of noninteracting atoms with total momentum F=1 may be used to explore the
behavior of quantum matter near a cosmological singularity.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:38:08 GMT"
},
{
"version": "v2",
"created": "Fri, 16 May 2008 18:34:12 GMT"
}
] | 2008-05-16T00:00:00 | [
[
"Calzetta",
"E.",
""
]
] | [
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712.0377 | Jeppe C. Dyre | S{\o}ren Toxvaerd, Thomas B. Schr{\o}der, and Jeppe C. Dyre | Crystallization of the Kob-Andersen binary Lennard-Jones liquid | null | J. Chem. Phys. 130, 224501 (2009) | 10.1063/1.3144049 | null | cond-mat.soft | null | At density 1.2 the Kob-Andersen binary Lennard-Jones liquid partly
crystallizes in the temperature interval [0.39, 0.44] after typically 10-100
microseconds (Argon units). The crystallization is initiated by a phase
separation where the large (A) particles cluster in a volume void of B
particles. We investigate a modification of the Kob-Andersen system where the
attraction between particles of the same type is removed, thus disfavoring
phase separation. We have not been able to crystallize this new system.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:48:43 GMT"
},
{
"version": "v2",
"created": "Sat, 9 Feb 2008 10:27:20 GMT"
}
] | 2013-01-29T00:00:00 | [
[
"Toxvaerd",
"Søren",
""
],
[
"Schrøder",
"Thomas B.",
""
],
[
"Dyre",
"Jeppe C.",
""
]
] | [
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] |
712.0378 | Paul Kalas | Paul Kalas, Gaspard Duchene, Michael P. Fitzgerald, James R. Graham | Discovery of an extended debris disk around the F2V star HD 15745 | 7 pages, 4 figures, ApJ Letters, in press | null | 10.1086/525252 | null | astro-ph | null | Using the Advanced Camera for Surveys aboard the Hubble Space Telescope, we
have discovered dust-scattered light from the debris disk surrounding the F2V
star HD 15745. The circumstellar disk is detected between 2.0" and 7.5" radius,
corresponding to 128 - 480 AU radius. The circumstellar disk morphology is
asymmetric about the star, resembling a fan, and consistent with forward
scattering grains in an optically thin disk with an inclination of ~67 degrees
to our line of sight. The spectral energy distribution and scattered light
morphology can be approximated with a model disk composed of silicate grains
between 60 and 450 AU radius, with a total dust mass of 10E-7 M_sun (0.03
M_earth) representing a narrow grain size distribution (1 - 10 micron).
Galactic space motions are similar to the Castor Moving Group with an age of
~10E+8 yr, although future work is required to determine the age of HD 15745
using other indicators.
| [
{
"version": "v1",
"created": "Mon, 3 Dec 2007 20:48:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kalas",
"Paul",
""
],
[
"Duchene",
"Gaspard",
""
],
[
"Fitzgerald",
"Michael P.",
""
],
[
"Graham",
"James R.",
""
]
] | [
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