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711.2208 | Jacob Bock Axelsen | Jacob Bock Axelsen, Sebastian Bernhardsson, Kim Sneppen | One Hub-One Process: A Tool Based View on Regulatory Network Topology | 18 pages, 3 figures, 5 supplementary figures | BMC Systems Biology 2008, 2:25 | 10.1186/1752-0509-2-25 | null | q-bio.MN cond-mat.soft | null | The relationship between the regulatory design and the functionality of
molecular networks is a key issue in biology. Modules and motifs have been
associated to various cellular processes, thereby providing anecdotal evidence
for performance based localization on molecular networks. To quantify
structure-function relationship we investigate similarities of proteins which
are close in the regulatory network of the yeast Saccharomyces Cerevisiae. We
find that the topology of the regulatory network show weak remnants of its
history of network reorganizations, but strong features of co-regulated
proteins associated to similar tasks. This suggests that local topological
features of regulatory networks, including broad degree distributions, emerge
as an implicit result of matching a number of needed processes to a finite
toolbox of proteins.
| [
{
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"created": "Wed, 14 Nov 2007 14:16:39 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 15:02:23 GMT"
}
] | 2008-03-04T00:00:00 | [
[
"Axelsen",
"Jacob Bock",
""
],
[
"Bernhardsson",
"Sebastian",
""
],
[
"Sneppen",
"Kim",
""
]
] | [
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711.2209 | Daniel Brown | D. Brown, M. Salaris, S. Cassisi, A. Pietrinferni | Impact of Rotation on the Evolution of Low-Mass Stars | 5 pages, 4 figures. Oral contrubution. Proceedings of the workshop
"XXI Century challenges for stellar evolution", held in Cefalu' (Sicily,
Italy), August 29 - September 2, 2007; S. Cassisi and M. Salaris Eds. To be
published in Mem. SAIt Vol. 79 No. 2 | null | null | null | astro-ph | null | High precision photometry and spectroscopy of low-mass stars reveal a variety
of properties standard stellar evolution cannot predict. Rotation, an essential
ingredient of stellar evolution, is a step towards resolving the discrepancy
between model predictions and observations. The first rotating stellar model,
continuously tracing a low-mass star from the pre-main sequence onto the
horizontal branch, is presented. The predicted luminosity functions of stars of
globular clusters and surface rotation velocities on the horizontal branch are
discussed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:17:32 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Brown",
"D.",
""
],
[
"Salaris",
"M.",
""
],
[
"Cassisi",
"S.",
""
],
[
"Pietrinferni",
"A.",
""
]
] | [
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711.221 | Urmila Mitra-Kraev | U. Mitra-Kraev, A.G. Kosovichev, T. Sekii | Properties of high-degree oscillation modes of the Sun observed with
Hinode/SOT | 4 pages, 3 figures (6 plots), accepted by A&A Letters for Hinode
special issue. v2 includes minor changes suggested by the referee (incl.
math. definitions) as well as edited language | null | 10.1051/0004-6361:20079042 | null | astro-ph | null | Aims. With the Solar Optical Telescope on Hinode, we investigate the basic
properties of high-degree solar oscillations observed at two levels in the
solar atmosphere, in the G-band (formed in the photosphere) and in the Ca II H
line (chromospheric emission).
Methods. We analyzed the data by calculating the individual power spectra as
well as the cross-spectral properties, i.e., coherence and phase shift. The
observational properties are compared with a simple theoretical model, which
includes the effects of correlated noise.
Results. The results reveal significant frequency shifts between the Ca II H
and G-band spectra, in particular above the acoustic cut-off frequency for
pseudo-modes. The cross-spectrum phase shows peaks associated with the acoustic
oscillation (p-mode) lines, and begins to increase with frequency around the
acoustic cut-off. However, we find no phase shift for the (surface gravity
wave) f-mode. The observed properties for the p-modes are qualitatively
reproduced in a simple model with a correlated background if the correlated
noise level in the Ca II H data is higher than in the G-band data. These
results suggest that multi-wavelength observations of solar oscillations, in
combination with the traditional intensity-velocity observations, may help to
determine the level of the correlated background noise and to determine the
type of wave excitation sources on the Sun.
| [
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"version": "v1",
"created": "Wed, 14 Nov 2007 14:34:33 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 12:10:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mitra-Kraev",
"U.",
""
],
[
"Kosovichev",
"A. G.",
""
],
[
"Sekii",
"T.",
""
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] |
711.2211 | Xiaoli Han | Xiaoli Han, Jiayu Li | Symplectic critical surfaces in K\"ahler surfaces | null | null | null | null | math.DG math.SG | null | Let $M$ be a K\"ahler surface and $\Sigma$ be a closed symplectic surface
which is smoothly immersed in $M$. Let $\alpha$ be the K\"ahler angle of
$\Sigma$ in $M$. We first deduce the Euler-Lagrange equation of the functional
$L=\int_{\Sigma}\frac{1}{\cos\alpha}d\mu$ in the class of symplectic surfaces.
It is $\cos^3\alpha H=(J(J\nabla\cos\alpha)^\top)^\bot$, where $H$ is the mean
curvature vector of $\Sigma$ in $M$, $J$ is the complex structure compatible
with the K\"ahler form $\omega$ in $M$, which is an elliptic equation. We then
study the properties of the equation.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:39:32 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Han",
"Xiaoli",
""
],
[
"Li",
"Jiayu",
""
]
] | [
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] |
711.2212 | Abhinav Singh | Abhinav Singh, Dmitri Vainchtein, Howard Weiss | Schelling's Segregation Model: Parameters, Scaling, and Aggregation | null | null | null | null | nlin.AO nlin.CG | null | Thomas Schelling proposed an influential simple spatial model to illustrate
how, even with relatively mild assumptions on each individual's nearest
neighbor preferences, an integrated city would likely unravel to a segregated
city, even if all individuals prefer integration. Aggregation relates to
individuals coming together to form groups and global aggregation corresponds
to segregation. Many authors assumed that the segregation which Schelling
observed in simulations on very small cities persists for larger, realistic
size cities. We devise new measures to quantify the segregation and unlock its
dependence on city size, disparate neighbor comfortability threshold, and
population density. We identify distinct scales of global aggregation, and show
that the striking global aggregation Schelling observed is strictly a small
city phenomenon. We also discover several scaling laws for the aggregation
measures.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:33:36 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Singh",
"Abhinav",
""
],
[
"Vainchtein",
"Dmitri",
""
],
[
"Weiss",
"Howard",
""
]
] | [
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] |
711.2213 | Leonardo Castaneda | Mauricio Duque, Leonardo Castaneda, Carlos Duque | Radiative Transfer in Special Relativity: Covariance | 11 pages, 8 figures. Submitted to "Revista Mexicana de Fisica". Minor
changes added by the referee. Spanish | Rev. Mex. Fis. E 54 (2008) 037. | null | null | astro-ph | null | The purpose is to introduce in a clear and direct way the students of
undergraduate courses in physics and/or astronomy to the subject of radiative
transfer. A pedagogical revision is made in order to obtain the radiative
transfer equation, its restrictions and the different types of interactions
present between the radiation and the matter. Because in the classical
literature about radiative transfer the covariance is not fully developed, we
show in an explicit manner detail calculations and then we discuss the
relativistic effects.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:48:48 GMT"
}
] | 2008-07-04T00:00:00 | [
[
"Duque",
"Mauricio",
""
],
[
"Castaneda",
"Leonardo",
""
],
[
"Duque",
"Carlos",
""
]
] | [
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] |
711.2214 | Chi-Yong Lin | Bin Wang, Chi-Yong Lin, Diego Pavon, Elcio Abdalla | Thermodynamical description of the interaction between holographic dark
energy and dark matter | 14 pages, 4 figures, to be published in Phys. Lett. B | Phys.Lett.B662:1-6,2008 | 10.1016/j.physletb.2008.01.074 | null | hep-th astro-ph gr-qc | null | We present a thermodynamical description of the interaction between
holographic dark energy and dark matter. If holographic dark energy and dark
matter evolve separately, each of them remains in thermodynamic equilibrium. A
small interaction between them may be viewed as a stable thermal fluctuation
that brings a logarithmic correction to the equilibrium entropy. From this
correction we obtain a physical expression for the interaction which is
consistent with phenomenological descriptions and passes reasonably well the
observational tests.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:51:16 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 02:11:38 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Wang",
"Bin",
""
],
[
"Lin",
"Chi-Yong",
""
],
[
"Pavon",
"Diego",
""
],
[
"Abdalla",
"Elcio",
""
]
] | [
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] |
711.2215 | Guiyun Liang | G.Y. Liang, G. Zhao | Soft X-ray emissions of highly charged Si VII--Si XII in cool
star--Procyon | 9 pages, 3 figures, Accepted by MNRAS | null | 10.1111/j.1365-2966.2007.12696.x | null | astro-ph | null | Different observation data for cool star--Procyon (Obs\_IDs of 63, 1461 and
1224) available from {\it Chandra Data Public Archive} were co-added and
analyzed. Emissivities of emission lines of highly charged silicon ions (Si
VII--Si XII) were calculated over temperatures by adopting the published data
of Liang et al. (2007, {\it Atom. Data and Nucl. Data Tables}, {\bf 93}, 375).
Using the emission measure derived by Raassen et al. (2002, A&A, {\bf 389},
228), the theoretical line fluxes are predicted, and the theoretical spectra
are constructed by assuming the Gaussian profile with instrumental broadening
(0.06 \AA). By detailed comparison between observation and predictions, several
emissions lines are identified firstly such as emissions at 43.663 \AA (Si XI),
45.550 \AA (Si XII), 46.179 \AA (Si VIII), 50.874 \AA (Si X), 64.668 \AA (Si
IX), and 73.189 \AA (Si VII) etc. Several emission lines are re-assigned in
this work, such as the emission line at 52.594 \AA to Si X (52.612 \AA), at
69.641 \AA to the blending of Si VII (69.632 \AA) and Si VIII (69.664 \AA)
lines, as well as at 70.050 \AA to Si VII (70.027 \AA). The prediction reveals
the large discrepancies between the $3s$--$2p$ line (63.715 \AA) {\it versus}
3d--$2p$ line (61.012 \AA) again for lower charge stage Si VIII. Solar flare
observation is also added for the assessment of present calculation. Different
assignments for some lines between Procyon and solar flare, have been found to
be due to the hotter emitter in Sun than in Procyon coronae.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:58:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Liang",
"G. Y.",
""
],
[
"Zhao",
"G.",
""
]
] | [
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] |
711.2216 | Joerg Wotschack | V. Ammosov, et al | Comments on TPC and RPC calibrations reported by the HARP Collaboration | 17 pages, 13 figures | JINST3:P01002,2008 | 10.1088/1748-0221/3/01/P01002 | null | hep-ex | null | The HARP Collaboration recently published calibrations of their TPC and RPC
detectors, and differential cross-sections of large-angle pion production in
proton-nucleus collisions. We argue that these calibrations are biased and
cross-sections based on them should not be trusted.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:00:47 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ammosov",
"V.",
""
]
] | [
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] |
711.2217 | J\"org Main | T. Fabcic, J. Main, G. Wunner | Time propagation of constrained coupled Gaussian wave packets | 8 pages, 3 figures, accepted for publication in J. Chem. Phys | J. Chem. Phys. 128 (2008) 044116 | 10.1063/1.2821751 | null | quant-ph | null | The dynamics of quantum systems can be approximated by the time propagation
of Gaussian wave packets. Applying a time dependent variational principle, the
time evolution of the parameters of the coupled Gaussian wave packets can be
calculated from a set of ordinary differential equations. Unfortunately, the
set of equations is ill-behaved in most practical applications, depending on
the number of propagated Gaussian wave packets, and methods for regularization
are needed. We present a general method for regularization based on applying
adequate nonholonomic inequality constraints to the evolution of the
parameters, keeping the equations of motion well-behaved. The power of the
method is demonstrated for a non-integrable system with two degrees of freedom.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:16:27 GMT"
}
] | 2008-02-01T00:00:00 | [
[
"Fabcic",
"T.",
""
],
[
"Main",
"J.",
""
],
[
"Wunner",
"G.",
""
]
] | [
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] |
711.2218 | Olaf Post | Olaf Post | First order operators and boundary triples | 14 pages, new version due to paper size problems | null | 10.1134/S1061920807040139 | null | math.SP math-ph math.AP math.FA math.MP | null | The aim of the present paper is to introduce a first order approach to the
abstract concept of boundary triples for Laplace operators. Our main
application is the Laplace operator on a manifold with boundary; a case in
which the ordinary concept of boundary triples does not apply directly. In our
first order approach, we show that we can use the usual boundary operators also
in the abstract Green's formula. Another motivation for the first order
approach is to give an intrinsic definition of the Dirichlet-to-Neumann map and
intrinsic norms on the corresponding boundary spaces. We also show how the
first order boundary triples can be used to define a usual boundary triple
leading to a Dirac operator.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:18:22 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Dec 2007 18:26:58 GMT"
},
{
"version": "v3",
"created": "Thu, 6 Dec 2007 13:18:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Post",
"Olaf",
""
]
] | [
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] |
711.2219 | Michael Joyce | Thierry Baertschiger, Michael Joyce, Francesco Sylos Labini and Bruno
Marcos | Gravitational dynamics of an infinite shuffled lattice: early time
evolution and universality of non-linear correlations | 11 pages, 11 figures, shortened introductory sections and other minor
modifications, version to appear in Phys. Rev. E | null | 10.1103/PhysRevE.77.051114 | null | cond-mat.stat-mech astro-ph | null | In two recent articles a detailed study has been presented of the out of
equilibrium dynamics of an infinite system of self-gravitating points initially
located on a randomly perturbed lattice. In this article we extend the
treatment of the early time phase during which strong non-linear correlations
first develop, prior to the onset of ``self-similar'' scaling in the two point
correlation function. We establish more directly, using appropriate
modifications of the numerical integration, that the development of these
correlations can be well described by an approximation of the evolution in two
phases: a first perturbative phase in which particles' displacements are small
compared to the lattice spacing, and a subsequent phase in which particles
interact only with their nearest neighbor. For the range of initial amplitudes
considered we show that the first phase can be well approximated as a
transformation of the perturbed lattice configuration into a Poisson
distribution at the relevant scales. This appears to explain the
``universality'' of the spatial dependence of the asymptotic non-linear
clustering observed from both shuffled lattice and Poisson initial conditions.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:18:26 GMT"
},
{
"version": "v2",
"created": "Thu, 15 Nov 2007 13:10:17 GMT"
},
{
"version": "v3",
"created": "Fri, 9 May 2008 14:53:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Baertschiger",
"Thierry",
""
],
[
"Joyce",
"Michael",
""
],
[
"Labini",
"Francesco Sylos",
""
],
[
"Marcos",
"Bruno",
""
]
] | [
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] |
711.222 | Francesco Sciortino | Francesco Sciortino | Gel-forming patchy colloids and network glass formers: Thermodynamic and
Dynamic analogies | Proceeding of Stat-Phys 2007. EPJB in press | null | 10.1140/epjb/e2008-00034-0 | null | cond-mat.soft cond-mat.stat-mech | null | This article discusses recent attempts to provide a deeper understanding of
the thermoreversible "gel" state of colloidal matter and to unravel the
analogies between gels at the colloidal level and gels at the molecular level,
commonly known as network-forming strong liquids. The connection between
gel-forming patchy colloids and strong liquids is provided by the limited
valence of the inter-particle interactions, i.e. by the presence of a limit in
the number of bonded nearest neighbors.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:19:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sciortino",
"Francesco",
""
]
] | [
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] |
711.2221 | Chris Lodewijk | T. Zijlstra, C. F. J. Lodewijk, N. Vercruyssen, F. D. Tichelaar, D. N.
Loudkov, and T. M. Klapwijk | Epitaxial aluminium-nitride tunnel barriers grown by nitridation with a
plasma source | 3 pages, 3 figures, accepted for publication in APL | Appl. Phys. Lett. 91, 233102 (2007) | 10.1063/1.2819532 | null | cond-mat.mes-hall cond-mat.supr-con | null | High critical current-density (10 to 420 kA/cm^2)
superconductor-insulator-superconductor tunnel junctions with aluminium nitride
barriers have been realized using a remote nitrogen plasma from an inductively
coupled plasma source operated in a pressure range of 10^{-3} to 10^{-1} mbar.
We find a much better reproducibility and control compared to previous work.
From the current-voltage characteristics and cross-sectional TEM images it is
inferred that, compared to the commonly used AlO_x barriers, the
poly-crystalline AlN barriers are much more uniform in transmissivity, leading
to a better quality at high critical current-densities.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:00:11 GMT"
}
] | 2008-06-03T00:00:00 | [
[
"Zijlstra",
"T.",
""
],
[
"Lodewijk",
"C. F. J.",
""
],
[
"Vercruyssen",
"N.",
""
],
[
"Tichelaar",
"F. D.",
""
],
[
"Loudkov",
"D. N.",
""
],
[
"Klapwijk",
"T. M.",
""
]
] | [
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711.2222 | Bruce Gendre | B. Gendre (1, 2, 5), A. Galli (1, 3), M. Boer (4) ((1) IASF-Roma,
Roma, Italy; (2) Bicocca University, Milano, Italy; (3) INFN-Trieste,
Trieste, Italy; (4) Observatoire de Haute Provence (CNRS), Saint Michel
l'Observatoire, France; (5) LAM/CNRS/universite de Provence) | X-ray afterglow light curves : toward standard candle ? | 17 pages, 10 color figures, 1 b&w figure. Accepted for publication by
ApJ | AIPConf.Proc.1000:72-75,2008 | 10.1063/1.2943553 | null | astro-ph | null | We investigate the clustering of afterglow light curves observed at X-ray and
optical wavelengths. We have constructed a sample of 61 bursts with known dis
tance and X-ray afterglow. This sample includes bursts observed by BeppoSAX,
XMM-Newton, Chandra, and SWIFT. We correct the light curves for cosmological ef
fects and compare the observed X-ray fluxes one day after the burst. We check
for correlations between the observed flux and the burst spectral and temporal
properties. We confirm the previous result of Boer and Gendre (2000) that X-ray
afterglow light curves cluster in luminosity, even when we consider the l ast
SWIFT data. We observe this clustering only for the afterglow light curves; the
inclusion of prompt-related data broaden the distribution. A similar clu
stering is observed for the optical light curves; GRB sources can be divided in
three classes, namely optical and X-ray bright afterglows, optical and X-ray
dim ones, and optically bright -X-ray dim ones. We argue that this clustering
is related to the fireball total energy, the external medium density, the
fraction of fireball energy going in relativistic electrons and magnetic
fields. These parameters can be either fixed to a standard va lue, or
correlated. We finally propose a method for the estimation of the GRB source
redshift based on the observed X-ray flux one day after the burst and optical
properties. Using this method, we compute a redshift of 1.4 +/- 0.2 for GRB
980519 and of 1.9 \+/- 0.3 for GRB 040827. We tested this method on three
recently detected SWIFT GRBs with known redshift, and found it in good
agreement with the reported distance from optical spectroscopy .
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:26:38 GMT"
},
{
"version": "v2",
"created": "Mon, 5 May 2008 16:28:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Gendre",
"B.",
""
],
[
"Galli",
"A.",
""
],
[
"Boer",
"M.",
""
]
] | [
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711.2223 | Kathrin Vorwerk | Axel Hultman and Kathrin Vorwerk | Pattern avoidance and the Bruhat order on involutions | 14 pages, 5 figures | J. Algebraic Combin. 30 (2009), no. 1, 87--102 | null | null | math.CO | null | We show that the principal order ideal below an element w in the Bruhat order
on involutions in a symmetric group is a Boolean lattice if and only if w
avoids the patterns 4321, 45312 and 456123. Similar criteria for signed
permutations are also stated. Involutions with this property are enumerated
with respect to natural statistics. In this context, a bijective correspondence
with certain Motzkin paths is demonstrated.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:33:57 GMT"
}
] | 2012-07-24T00:00:00 | [
[
"Hultman",
"Axel",
""
],
[
"Vorwerk",
"Kathrin",
""
]
] | [
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] |
711.2224 | Graham Smith Dr | Graham Smith | A smooth foliation of convex hypersurfaces for quasi-hyper-Fuchsian
manifolds | This submission has been withdrawn by the author and superseded by
arXiv:0804.0744 | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This submission has been withdrawn by the author and superseded by
arXiv:0804.0744.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:28:28 GMT"
},
{
"version": "v2",
"created": "Mon, 19 Nov 2007 16:22:12 GMT"
},
{
"version": "v3",
"created": "Wed, 16 Jul 2008 19:01:17 GMT"
}
] | 2008-07-16T00:00:00 | [
[
"Smith",
"Graham",
""
]
] | [
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] |
711.2225 | Andrey Tsiganov | A. V. Tsiganov | On maximally superintegrable systems | 12 pages, LaTeX with AmsFonts | Regular and Chaotic Dynamics, v.13, n.3, 178-190, 2008 | 10.1134/S1560354708030040 | null | nlin.SI | null | Locally any completely integrable system is maximally superintegrable system
such as we have the necessary number of the action-angle variables. The main
problem is the construction of the single-valued additional integrals of motion
on the whole phase space by using these multi-valued action-angle variables.
Some constructions of the additional integrals of motion for the St\"ackel
systems and for the integrable systems related with two different quadratic
$r$-matrix algebras are discussed. Among these system there are the open
Heisenberg magnet and the open Toda lattices associated with the different root
systems.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:31:50 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Apr 2008 11:14:51 GMT"
}
] | 2010-06-22T00:00:00 | [
[
"Tsiganov",
"A. V.",
""
]
] | [
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711.2226 | Nikolaos Tetradis | N. Brouzakis, N. Tetradis and C. Wetterich | Neutrino Lumps in Quintessence Cosmology | 9 pages, 4 figures, references and discussion of formation added | Phys.Lett.B665:131-134,2008 | 10.1016/j.physletb.2008.05.068 | null | astro-ph hep-ph hep-th | null | Neutrinos interacting with the quintessence field can trigger the accelerated
expansion of the Universe. In such models with a growing neutrino mass the
homogeneous cosmological solution is often unstable to perturbations. We
present static, spherically symmetric solutions of the Einstein equations in
the same models. They describe astophysical objects composed of neutrinos, held
together by gravity and the attractive force mediated by the quintessence
field. We discuss their characteristics as a function of the present neutrino
mass. We suggest that these objects are the likely outcome of the growth of
cosmological perturbations.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:32:29 GMT"
},
{
"version": "v2",
"created": "Tue, 12 Feb 2008 14:43:03 GMT"
},
{
"version": "v3",
"created": "Sun, 1 Jun 2008 09:34:44 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Brouzakis",
"N.",
""
],
[
"Tetradis",
"N.",
""
],
[
"Wetterich",
"C.",
""
]
] | [
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711.2227 | Christian Korn | C. B. Korn and U. S. Schwarz (University of Heidelberg, Bioquant) | Dynamic states of cells adhering in shear flow: from slipping to rolling | Reftex, postscript figures included, typos corrected, accepted for
publication in PRE | Phys. Rev. E, 77:041904, 2008 | 10.1103/PhysRevE.77.041904 | null | q-bio.CB q-bio.SC | null | Motivated by rolling adhesion of white blood cells in the vasculature, we
study how cells move in linear shear flow above a wall to which they can adhere
via specific receptor-ligand bonds. Our computer simulations are based on a
Langevin equation accounting for hydrodynamic interactions, thermal
fluctuations and adhesive interactions. In contrast to earlier approaches, our
model not only includes stochastic rules for the formation and rupture of
bonds, but also fully resolves both receptor and ligand positions. We identify
five different dynamic states of motion in regard to the translational and
angular velocities of the cell. The transitions between the different states
are mapped out in a dynamic state diagram as a function of the rates for bond
formation and rupture. For example, as the cell starts to adhere under the
action of bonds, its translational and angular velocities become synchronized
and the dynamic state changes from slipping to rolling. We also investigate the
effect of non-molecular parameters. In particular, we find that an increase in
viscosity of the medium leads to a characteristic expansion of the region of
stable rolling to the expense of the region of firm adhesion, but not to the
expense of the regions of free or transient motion. Our results can be used in
an inverse approach to determine single bond parameters from flow chamber data
on rolling adhesion.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:33:07 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 09:44:37 GMT"
}
] | 2008-04-30T00:00:00 | [
[
"Korn",
"C. B.",
"",
"University of Heidelberg, Bioquant"
],
[
"Schwarz",
"U. S.",
"",
"University of Heidelberg, Bioquant"
]
] | [
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] |
711.2228 | Stephen Hogan | D. Tak\'acs, G. St\'ep\'an. S. J. Hogan | Isolated large amplitude periodic motions of towed rigid wheels | Appeared online in Nonlinear Dynamics Thursday, April 26, 2007 | null | 10.1007/s11071-007-9253-y | null | nlin.CD | null | This study investigates a low degree-of-freedom (DoF) mechanical model of
shimmying wheels. The model is studied using bifurcation theory and numerical
continuation. Self-excited vibrations, that is, stable and unstable periodic
motions of the wheel, are detected with the help of Hopf bifurcation
calculations. These oscillations are then followed over a large parameter range
for different damping values by means of the software package AUTO97. For
certain parameter regions, the branches representing large amplitude stable and
unstable periodic motions become isolated following an isola birth. These
regions are extremely dangerous from an engineering view-point if they are not
identified and avoided at the design stage.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:38:27 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Takács",
"D.",
""
],
[
"Hogan",
"G. Stépán. S. J.",
""
]
] | [
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] |
711.2229 | Poilblanc | Didier Poilblanc | Properties of holons in the Quantum Dimer Model | 4 pages, 5 figures, extensive revision, important new data included
in Fig.4(a) | Phys. Rev. Lett. 100, 157206 (2008) | 10.1103/PhysRevLett.100.157206 | null | cond-mat.str-el cond-mat.supr-con | null | I introduce a doped two-dimensional quantum dimer model describing a doped
Mott insulator and retaining the original Fermi statistics of the electrons.
This model shows a rich phase diagram including a d-wave hole-pair
unconventional superconductor at small enough doping and a bosonic superfluid
at large doping. The hole kinetic energy is shown to favor binding of
topological defects to the bare fermionic holons turning them into bosons, in
agreement with arguments based on RVB wave-functions. Results are discussed in
the context of cuprates superconductors.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:41:10 GMT"
},
{
"version": "v2",
"created": "Wed, 21 Nov 2007 10:15:32 GMT"
},
{
"version": "v3",
"created": "Tue, 22 Jan 2008 18:18:37 GMT"
}
] | 2008-04-24T00:00:00 | [
[
"Poilblanc",
"Didier",
""
]
] | [
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] |
711.223 | Alessandro Teta | Gianfausto Dell'Antonio, Rodolfo Figari, Alessandro Teta | Joint excitation probability for two harmonic oscillators in dimension
one and the Mott problem | 26 pages | null | null | null | quant-ph math-ph math.MP | null | We analyze a one dimensional quantum system consisting of a test particle
interacting with two harmonic oscillators placed at the positions $a_1$, $a_2$,
with $a_1 >0$, $|a_2|>a_1$, in the two possible situations: $a_2>0$ and $a_2
<0$. At time zero the harmonic oscillators are in their ground state and the
test particle is in a superposition state of two wave packets centered in the
origin with opposite mean momentum. %$\pm M v_0$. Under suitable assumptions on
the physical parameters of the model, we consider the time evolution of the
wave function and we compute the probability $\mathcal{P}^{-}_{n_1 n_2} (t)$
(resp. $\mathcal{P}^{+}_{n_1 n_2} (t)$) that both oscillators are in the
excited states labelled by $n_1$, $n_2 >0$ at time $t > |a_2| v_0^{-1}$ when
$a_2 <0$ (resp. $a_2 >0$). We prove that $\mathcal{P}_{n_1 n_2}^- (t)$ is
negligible with respect to $\mathcal{P}_{n_1 n_2}^+ (t)$, up to second order in
time dependent perturbation theory. The system we consider is a simplified, one
dimensional version of the original model of a cloud chamber introduced by Mott
in \cite{m}, where the result was argued using euristic arguments in the
framework of the time independent perturbation theory for the stationary
Schr\"{o}dinger equation. The method of the proof is entirely elementary and it
is essentially based on a stationary phase argument. We also remark that all
the computations refer to the Schr\"{o}dinger equation for the three-particle
system, with no reference to the wave packet collapse postulate.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:44:49 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Dell'Antonio",
"Gianfausto",
""
],
[
"Figari",
"Rodolfo",
""
],
[
"Teta",
"Alessandro",
""
]
] | [
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] |
711.2231 | Vitaly Okorokov A | V.A. Okorokov (1), S.B. Nurushev (2) ((1) Moscow Engineering Physics
Institute (State University), (2) Institute for High Energy Physics,
Protvino) | Elastic proton-proton and proton-antiproton scattering: analysis of
complete set of helicity amplitudes | 4 pages, XII Workshop on high energy spin physics, DSPIN-2007,
September 3-7, 2007, Dubna, Russia | null | null | null | hep-ph | null | The differential cross-sections are calculated for proton-proton and
proton-antiproton elastic scattering using the phenomenological model based on
the analytic parameterizations for global scattering parameters (total
cross-section and $\rho$ - parameter), crossing symmetry and derivative
relations. We confront our model predictions with experimental data in wide
range of energy and momentum transfer. The suggested method may be useful for
PAX Program (GSI) as well as for high-energy experiments at RHIC and LHC.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:50:10 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Okorokov",
"V. A.",
""
],
[
"Nurushev",
"S. B.",
""
]
] | [
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] |
711.2232 | S. M. Iftiquar | S. M. Iftiquar | Electromagnetically induced transparency in two channels of a $\Lambda$
system | 5 pages, 6 figures | null | null | null | physics.optics physics.atom-ph | null | We show two channel electromagnetically induced transparency (EIT) spectra at
various optical power. The two channels are coupling field and probe field
absorption. It is shown that EIT width and intensity increases linearly with
pump power. A density matrix calculation is used to determine nature of EIT
spectra induced by optical field. It has been observed that EIT occurs in cases
when coupling laser is at fixed frequency while probe laser frequency is
scanned, when coupling laser is frequency scanned and probe is at fixed
frequency.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:06:30 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Iftiquar",
"S. M.",
""
]
] | [
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] |
711.2233 | Norbert Kaiser | N. Kaiser | Parity-violating two-pion exchange nucleon-nucleon interaction | 7 pages, 3 figures, 1 table, published in: Phys. Rev. C76. 047001
(2007) | Phys.Rev.C76:047001,2007 | 10.1103/PhysRevC.76.047001 | null | nucl-th | null | We calculate in chiral perturbation theory the parity-violating two-pion
exchange nucleon-nucleon potentials at leading one-loop order. At a distance of
$r= m_\pi^{-1} \simeq 1.4 $fm they amount to about $\pm 16%$ of the
parity-violating $1\pi$-exchange potential. We evaluate also the
parity-violating effects arising from $2\pi$-exchange with excitation of
virtual $\Delta(1232)$-isobars. These come out to be relatively small in
comparison to those from diagrams with only nucleon intermediate states. The
reason for this opposite behavior to the parity-conserving case is the blocking
of the dominant isoscalar central channel by CP-invariance. Furthermore, we
calculate the T-matrix related to the iteration of the parity-violating
$1\pi$-exchange with the parity-conserving one. The analytical results
presented in this work can be easily implemented into calculations of
parity-violating nuclear observables.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:56:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kaiser",
"N.",
""
]
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] |
711.2234 | Anne Green | Anne M. Green, Ben Morgan | Consequences of statistical sense determination for WIMP directional
detection | 5 pages, 3 figures, version to appear in PRD, minor changes | Phys.Rev.D77:027303,2008 | 10.1103/PhysRevD.77.027303 | null | astro-ph hep-ex hep-ph | null | We study the consequences of limited recoil sense reconstruction on the
number of events required to reject isotropy and detect a WIMP signal using a
directional detector. For a constant probability of determining the sense
correctly, 3-d read-out and zero background, we find that as the probability is
decreased from 1.0 to 0.75 the number of events required to reject isotropy
using the mean angle statistic is increased by a factor of a few. As the
probability is decreased further the number of events required using this
statistic increases sharply, and in fact isotropy can be rejected more easily
by discarding the sense information and using axial statistics. This however
requires an order of magnitude more events than vectorial data with perfect
sense determination. We also consider energy dependent probabilities of
correctly measuring the sense, 2-d read-out and non-zero background. Our main
conclusion regarding the sense determination is that correctly determining the
sense of the abundant, but less anisotropic, low energy recoils is most
important for minimising the number of events required.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:00:01 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Dec 2007 09:41:52 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Green",
"Anne M.",
""
],
[
"Morgan",
"Ben",
""
]
] | [
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] |
711.2235 | Lee Martin | L. C. Martin and F. F. Assaad | Evolution of the Fermi Surface across a Magnetic Order-Disorder
Transition in the Two-Dimensional Kondo Lattice Model: A Dynamical Cluster
Approach | 5 pages, 5 figures, v3 text restructured and results clarified | null | 10.1103/PhysRevLett.101.066404 | null | cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We use the dynamical cluster approximation, with a quantum Monte Carlo
cluster solver on clusters of up to 16 orbitals, to investigate the evolution
of the Fermi surface across the magnetic order-disorder transition in the
two-dimensional doped Kondo lattice model. In the paramagnetic phase we observe
the generic hybridized heavy fermion band structure with large Luttinger
volume. In the antiferromagnetic phase, the heavy fermion band drops below the
Fermi surface giving way to hole pockets centered around k=(pi/2,pi/2) and
equivalent points. In this phase Kondo screening does not break down but the
topology of the resulting Fermi surface is that of a spin-density wave
approximation in which the localized spins are frozen.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:01:30 GMT"
},
{
"version": "v2",
"created": "Thu, 22 Nov 2007 15:38:20 GMT"
},
{
"version": "v3",
"created": "Thu, 3 Jul 2008 09:32:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Martin",
"L. C.",
""
],
[
"Assaad",
"F. F.",
""
]
] | [
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711.2236 | Alexander Chervov | Alexander Chervov, Gregorio Falqui | Manin matrices and Talalaev's formula | 40 pages, V2: exposition reorganized, some proofs added, misprints
e.g. in Newton id-s fixed, normal ordering convention turned to standard one,
refs. added | J.Phys.A41:194006,2008 | 10.1088/1751-8113/41/19/194006 | ITEP-TH-45/07 | math.QA hep-th math.RA math.RT nlin.SI | null | We study special class of matrices with noncommutative entries and
demonstrate their various applications in integrable systems theory. They
appeared in Yu. Manin's works in 87-92 as linear homomorphisms between
polynomial rings; more explicitly they read: 1) elements in the same column
commute; 2) commutators of the cross terms are equal: $[M_{ij},
M_{kl}]=[M_{kj}, M_{il}]$ (e.g. $[M_{11}, M_{22}]=[M_{21}, M_{12}]$). We claim
that such matrices behave almost as well as matrices with commutative elements.
Namely theorems of linear algebra (e.g., a natural definition of the
determinant, the Cayley-Hamilton theorem, the Newton identities and so on and
so forth) holds true for them.
On the other hand, we remark that such matrices are somewhat ubiquitous in
the theory of quantum integrability. For instance, Manin matrices (and their
q-analogs) include matrices satisfying the Yang-Baxter relation "RTT=TTR" and
the so--called Cartier-Foata matrices. Also, they enter Talalaev's
hep-th/0404153 remarkable formulas: $det(\partial_z-L_{Gaudin}(z))$,
$det(1-e^{-\p}T_{Yangian}(z))$ for the "quantum spectral curve", etc. We show
that theorems of linear algebra, after being established for such matrices,
have various applications to quantum integrable systems and Lie algebras, e.g
in the construction of new generators in $Z(U(\hat{gl_n}))$ (and, in general,
in the construction of quantum conservation laws), in the
Knizhnik-Zamolodchikov equation, and in the problem of Wick ordering. We also
discuss applications to the separation of variables problem, new Capelli
identities and the Langlands correspondence.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:03:13 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Feb 2008 18:48:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chervov",
"Alexander",
""
],
[
"Falqui",
"Gregorio",
""
]
] | [
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] |
711.2237 | Norbert Kaiser | N. Kaiser | $\Sigma$-nuclear spin-orbit coupling from two-pion exchange | 7 pages, 2 figures, submitted to Phys. Rev. C | Phys.Rev.C76:068201,2007 | 10.1103/PhysRevC.76.068201 | null | nucl-th | null | Using SU(3) chiral perturbation theory we calculate the density-dependent
complex-valued spin-orbit coupling strength $U_{\Sigma ls}(k_f)+ i W_{\Sigma
ls}(k_f)$ of a $\Sigma$ hyperon in the nuclear medium. The leading long-range
$\Sigma N$ interaction arises from iterated one-pion exchange with a $\Lambda$
or a $\Sigma$ hyperon in the intermediate state. We find from this unique
long-range dynamics a sizeable ``wrong-sign'' spin-orbit coupling strength of
$U_{\Sigma ls}(k_{f0}) \simeq -20$ MeVfm$^2$ at normal nuclear matter density
$\rho_0 = 0.16 $fm$^{-3}$. The strong $\Sigma N\to \Lambda N$ conversion
process contributes at the same time an imaginary part of $W_{\Sigma
ls}(k_{f0}) \simeq -12$ MeVfm$^2$. When combined with estimates of the
short-range contribution the total $\Sigma$-nuclear spin-orbit coupling becomes
rather weak.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:07:42 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kaiser",
"N.",
""
]
] | [
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] |
711.2238 | Martin G. Gulbrandsen | Martin G. Gulbrandsen | Fourier-Mukai transforms of line bundles on derived equivalent abelian
varieties | null | Le Matematiche, Vol. 63, no. 1, 123--137 (2008) | null | null | math.AG | null | We study the Fourier-Mukai functor D(Y) -> D(X) induced by the universal
family on a fine moduli space Y for simple semihomogeneous vector bundles on an
abelian variety X. The main result is that the Fourier-Mukai transform of a
very negative line bundle on Y is ample if and only if the bundles parametrized
by Y are nef.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:37:54 GMT"
}
] | 2011-11-07T00:00:00 | [
[
"Gulbrandsen",
"Martin G.",
""
]
] | [
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] |
711.2239 | Guillaume Thomann | Guillaume Thomann (LGS), Jean Caelen (LIG), Morgan Verdier (LGS),
Brigitte Meillon (LIG) | Mise en place de sc\'enarios pour la conception d'outils en Chirurgie
Minimalement Invasive | null | Les Syst\`emes de Production, Lavoisier (Ed.) (2007) 93-107 | null | null | cs.HC | null | Nowadays, more and more surgical interventions are carried out in Minimally
Invasive Surgery, to make the post-operative constraints less painful for the
patient. Actually, new surgical tools or medical products are designed after
informal discussions between surgeons and designers. The user requirements
documents are the main document used by the mechanical designers to design and
improve the product. Medical terms, often used by surgeons and employed to
explain their needs, don't allow for an instantaneous understanding by
designers. Unfortunately, this relation causes a dysfunction in the definition
cycle of the product. Our aim is to work on the design process, its assistance
thanks to methods and tools and on its organisation for better understandings
and more complementarities between surgeons and designers. We propose on this
article a design method already tested in the informatics domain: User Centred
Design which takes the user into account more effectively in the process
design. We already propose a scenario oriented design method centred on the
user and represented as a scenario (Scenario-Based Design). We start in this
article by clarifying these concepts before detailing their implementation for
the design of a new surgical tool.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:18:42 GMT"
}
] | 2007-11-19T00:00:00 | [
[
"Thomann",
"Guillaume",
"",
"LGS"
],
[
"Caelen",
"Jean",
"",
"LIG"
],
[
"Verdier",
"Morgan",
"",
"LGS"
],
[
"Meillon",
"Brigitte",
"",
"LIG"
]
] | [
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711.224 | Moubariz Garaev Z. | M. Z. Garaev | A note on the least totient of a residue class | Improved version | null | null | null | math.NT | null | Let $q$ be a large prime number, $a$ be any integer, $\epsilon$ be a fixed
small positive quantity. Friedlander and Shparlinksi \cite{FSh} have shown that
there exists a positive integer $n\ll q^{5/2+\epsilon}$ such that $\phi(n)$
falls into the residue class $a \pmod q.$ Here, $\phi(n)$ denotes Euler's
function. In the present paper we improve this bound to $n\ll q^{2+\epsilon}.$
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:19:48 GMT"
},
{
"version": "v2",
"created": "Mon, 19 Nov 2007 19:57:45 GMT"
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] | 2007-11-19T00:00:00 | [
[
"Garaev",
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""
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711.2241 | Kerry Soileau | Kerry M. Soileau | Bounds on the cardinality of partition | I'm no longer satisfied with my treatment of this topic | null | null | null | math.GM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | If A is infinite and well-ordered, then |2^A|<=|Part(A)|<=|A^A|.
| [
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] |
711.2242 | Marco Tarzia | M. M\'ezard, M.Tarzia, C. Toninelli | Group testing with Random Pools: Phase Transitions and Optimal Strategy | null | null | 10.1007/s10955-008-9528-9 | null | cond-mat.stat-mech | null | The problem of Group Testing is to identify defective items out of a set of
objects by means of pool queries of the form "Does the pool contain at least a
defective?". The aim is of course to perform detection with the fewest possible
queries, a problem which has relevant practical applications in different
fields including molecular biology and computer science. Here we study GT in
the probabilistic setting focusing on the regime of small defective probability
and large number of objects, $p \to 0$ and $N \to \infty$. We construct and
analyze one-stage algorithms for which we establish the occurrence of a
non-detection/detection phase transition resulting in a sharp threshold, $\bar
M$, for the number of tests. By optimizing the pool design we construct
algorithms whose detection threshold follows the optimal scaling $\bar M\propto
Np|\log p|$. Then we consider two-stages algorithms and analyze their
performance for different choices of the first stage pools. In particular, via
a proper random choice of the pools, we construct algorithms which attain the
optimal value (previously determined in Ref. [16]) for the mean number of tests
required for complete detection. We finally discuss the optimal pool design in
the case of finite $p$.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 16:52:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mézard",
"M.",
""
],
[
"Tarzia",
"M.",
""
],
[
"Toninelli",
"C.",
""
]
] | [
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] |
711.2243 | Bernard Jancovici | Bernard Jancovici and Ladislav \v{S}amaj | Guest Charge and Potential Fluctuations in Two-Dimensional Classical
Coulomb Systems | 21 pages. Latex. Appendix moved, with changes, to new subsection 2.3.
Description of the Appendix at the end of the Introduction, from an earlier
version, deleted | J.Stat.Phys. 131, 613 (2008) | 10.1007/s10955-008-9515-1 | LPT-07-116 | cond-mat.stat-mech | null | A known generalization of the Stillinger-Lovett sum rule for a guest charge
immersed in a two-dimensional one-component plasma (the second moment of the
screening cloud around this guest charge) is more simply retrieved, just by
using the BGY hierarchy for a mixture of several species; the zeroth moment of
the excess density around a guest charge immersed in a two-component plasma is
also obtained. The moments of the electric potential are related to the excess
chemical potential of a guest charge; explicit results are obtained in several
special cases.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:00:39 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 08:48:54 GMT"
},
{
"version": "v3",
"created": "Tue, 8 Apr 2008 13:40:51 GMT"
}
] | 2008-04-08T00:00:00 | [
[
"Jancovici",
"Bernard",
""
],
[
"Šamaj",
"Ladislav",
""
]
] | [
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] |
711.2244 | Jos\'e Eduardo S. Costa | J. E. S. Costa, S. O. Kepler, D. E. Winget, M. S. O'Brien, S. D.
Kawaler, A. F. M. Costa, O. Giovannini, A. Kanaan, A. S. Mukadam, F.
Mullally, A. Nitta, J. L. Proven\c{c}al, H. Shipman, M. A. Wood, T. J.
Ahrens, A. Grauer, M. Kilic, P. A. Bradley, K. Sekiguchi, R. Crowe, X. J.
Jiang, D. Sullivan, T. Sullivan, R. Rosen, J. C. Clemens, R. Janulis, D.
O'Donoghue, W. Ogloza, A. Baran, R. Silvotti, S. Marinoni,, G. Vauclair, N.
Dolez, M. Chevreton, S. Dreizler, S. Schuh, J. Deetjen, T. Nagel, J.-E.
Solheim, J. M. Gonzalez Perez, A. Ulla, Martin Barstow, M. Burleigh, S. Good,
T.S. Metcalfe, S.-L. Kim, H. Lee, A. Sergeev, M.C. Akan, \"O. \c{C}akirli, M.
Paparo, G. Viraghalmy, B. N. Ashoka, G. Handler, \"Ozlem H\"urkal, F.
Johannessen, S. J. Kleinman, R. Kalytis, J. Krzesinski, E. Klumpe, J.
Larrison, T. Lawrence, E. Mei\v{s}tas, P. Martinez, R. E. Nather, J.-N. Fu,
E. Pak\v{s}tien\.e, R. Rosen, E. Romero-Colmenero, R. Riddle, S. Seetha, N.
M. Silvestri, M. Vu\v{c}kovi\'c, B. Warner, S. Zola, L. G. Althaus, A. H.
C\'orsico and M. H. Montgomery | The pulsation modes of the pre-white dwarf PG 1159-035 | 25 pages, 11 figures, appendix with 6 long tables. The resolution of
some of the figures were changed and some of them can appear with a bit lower
quality | 2008A&A...477..627 | 10.1051/0004-6361:20053470 | null | astro-ph | null | PG 1159-035, a pre-white dwarf with T_eff=140,000 K, is the prototype of both
two classes: the PG1159 spectroscopic class and the DOV pulsating class.
Previous studies of PG 1159-035 photometric data obtained with the Whole Earth
Telescope (WET) showed a rich frequency spectrum allowing the identification of
122 pulsation modes. In this work, we used all available WET photometric data
from 1983, 1985, 1989, 1993 and 2002 to identify the pulsation periods and
identified 76 additional pulsation modes, increasing to 198 the number of known
pulsation modes in PG 1159-035, the largest number of modes detected in any
star besides the Sun. From the period spacing we estimated a mass M = 0.59 +/-
0.02 solar masses for PG 1159-035, with the uncertainty dominated by the
models, not the observation. Deviations in the regular period spacing suggest
that some of the pulsation modes are trapped, even though the star is a
pre-white dwarf and the gravitational settling is ongoing. The position of the
transition zone that causes the mode trapping was calculated at r_c = 0.83 +/-
0.05 stellar radius. From the multiplet splitting, we calculated the rotational
period P_rot = 1.3920 +/- 0.0008 days and an upper limit for the magnetic
field, B < 2000 G. The total power of the pulsation modes at the stellar
surface changed less than 30% for l=1 modes and less than 50% for l=2 modes. We
find no evidence of linear combinations between the 198 pulsation mode
frequencies. PG 1159-035 models have not significative convection zones,
supporting the hypothesis that nonlinearity arises in the convection zones in
cooler pulsating white dwarf stars.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:19:21 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Dec 2007 12:43:29 GMT"
}
] | 2007-12-18T00:00:00 | [
[
"Costa",
"J. E. S.",
""
],
[
"Kepler",
"S. O.",
""
],
[
"Winget",
"D. E.",
""
],
[
"O'Brien",
"M. S.",
""
],
[
"Kawaler",
"S. D.",
""
],
[
"Costa",
"A. F. M.",
""
],
[
"Giovannini",
"O.",
""
],
[
"Kanaan",
"A.",
""
],
[
"Mukadam",
"A. S.",
""
],
[
"Mullally",
"F.",
""
],
[
"Nitta",
"A.",
""
],
[
"Provençal",
"J. L.",
""
],
[
"Shipman",
"H.",
""
],
[
"Wood",
"M. A.",
""
],
[
"Ahrens",
"T. J.",
""
],
[
"Grauer",
"A.",
""
],
[
"Kilic",
"M.",
""
],
[
"Bradley",
"P. A.",
""
],
[
"Sekiguchi",
"K.",
""
],
[
"Crowe",
"R.",
""
],
[
"Jiang",
"X. J.",
""
],
[
"Sullivan",
"D.",
""
],
[
"Sullivan",
"T.",
""
],
[
"Rosen",
"R.",
""
],
[
"Clemens",
"J. C.",
""
],
[
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"Martin",
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"M.",
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"S.",
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"S. -L.",
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"A.",
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[
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"Ö.",
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"M.",
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"G.",
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"B. N.",
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"G.",
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"Özlem",
""
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"F.",
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"S. J.",
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"R.",
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"J.",
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"E.",
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"J.",
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"T.",
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"E.",
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"P.",
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"R. E.",
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"E.",
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"E.",
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"M.",
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"M. H.",
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711.2245 | Maxim Shirokov Evgenyevich | M.E.Shirokov, A.S.Holevo | On approximation of quantum channels | 26 pages | Problems of Information Transmission, Vol. 44, No. 2, (2008), 3-22 | null | null | quant-ph | null | We develop an approximation approach to infinite dimensional quantum channels
based on detailed investigation of the continuity properties of entropic
characteristics of quantum channels and operations (trace-nonincreasing
completely positive maps) as functions of a pair ``channel, input state''. The
obtained results are then applied to the following problems: continuity of the
$\chi$-capacity as function of a channel; strong additivity of the
$\chi$-capacity for infinite dimensional channels; the analytical expression
for the convex closure of the output entropy of arbitrary quantum channel.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:05:34 GMT"
}
] | 2008-12-17T00:00:00 | [
[
"Shirokov",
"M. E.",
""
],
[
"Holevo",
"A. S.",
""
]
] | [
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] |
711.2246 | Dmitri Nikonov | Dmitri E. Nikonov, George I. Bourianoff, Paolo A. Gargini | Simulation of highly idealized, atomic scale MQCA logic circuits | 34 pages, 12 figures | null | null | null | cond-mat.mes-hall cond-mat.str-el | null | Spintronics logic devices based on majority gates formed by atomic-level
arrangements of spins in the crystal lattice is considered. The dynamics of
switching is modeled by time-dependent solution of the density-matrix equation
with relaxation. The devices are shown to satisfy requirements for logic.
Switching speed and dissipated energy are calculated and compared with
electronic transistors. The simulations show that for the highly idealized case
assumed here, it is possible to trade off size for speed and achieve lower
power operation than ultimately scaled CMOS devices.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:10:04 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Nikonov",
"Dmitri E.",
""
],
[
"Bourianoff",
"George I.",
""
],
[
"Gargini",
"Paolo A.",
""
]
] | [
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] |
711.2247 | Jouravlev Mikhail | M.V.Jouravlev | Power thresholds of morphology dependent induced thermal scattering in
silica microresonators | 4 papers, 6 figures | null | null | null | physics.optics physics.chem-ph | null | Induced thermal scattering power thresholds have been calculated as a
function of size and laser pump frequency. The thermal coupling coefficients of
morphology dependent resonances were estimated by asymptotic methods. The
resulting power threshold is comparable with experimental observations of
thresholds of Raman lasing and thermal instability in spherical silica
resonators. Applications may include the remote measurement of the temperature
of aerosol droplets and the stabilization of microcavity lasers against thermal
oscillations and temperature deviations on microcavity. A silica resonator can
be used as an IR sensor, as well as an additional tool for precisely measuring
the thermal conductivity and heat capacity of a target in a microsphere by
calculating of the thermal shifts of eigenfrequencies in spectra of nonlinear
scattering.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:12:02 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Jouravlev",
"M. V.",
""
]
] | [
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] |
711.2248 | Mattia Cafasso | Mattia Cafasso | Block Toeplitz determinants, constrained KP and Gelfand-Dickey
hierarchies | 35 pages. Typos corrected, some changes in the introduction | Mathematical Physics, Analysis and Geometry. February 2008, Volume
11, Issue 1, pp 11-51 | 10.1007/s11040-008-9038-7 | null | math.FA math-ph math.MP nlin.SI | null | We propose a method for computing any Gelfand-Dickey tau function living in
Segal-Wilson Grassmannian as the asymptotics of block Toeplitz determinant
associated to a certain class of symbols. Also truncated block Toeplitz
determinants associated to the same symbols are shown to be tau function for
rational reductions of KP. Connection with Riemann-Hilbert problems is
investigated both from the point of view of integrable systems and block
Toeplitz operator theory. Examples of applications to algebro-geometric
solutions are given.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:16:24 GMT"
},
{
"version": "v2",
"created": "Sun, 25 Nov 2007 16:50:47 GMT"
}
] | 2013-06-06T00:00:00 | [
[
"Cafasso",
"Mattia",
""
]
] | [
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] |
711.2249 | Soeren S. Larsen | S. S. Larsen (Astronomical Institute, Utrecht University) | A peculiar planetary nebula candidate in a globular cluster in the
Fornax dwarf spheroidal galaxy | 4 pages, 4 figures. Accepted for publication in A&A Letters | null | 10.1051/0004-6361:20078950 | null | astro-ph | null | CONTEXT: Until now, only one planetary nebula (PN) has been known in the
Fornax dwarf spheroidal galaxy. AIMS: The discovery of a second PN candidate,
associated with one of the 5 globular clusters in the Fornax dwarf, is
reported. METHODS: Spectra of the globular cluster H5, obtained with the UVES
echelle spectrograph on the ESO Very Large Telescope, show [O III] line
emission at a radial velocity consistent with membership of the Fornax dwarf. A
possible counterpart of the [O III] emission is identified in archival images
from the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. The
source of the emission is located about 1.5" (less than one core radius)
southwest of the centre of the cluster. RESULTS: The emission line source is
identified as a likely PN, albeit with several peculiar properties. No Hbeta,
He I, or He II line emission is detected and the [O III]/Hbeta ratio is >25 (2
sigma). The expansion velocity inferred from the [O III] 5007 AA line is about
55 km/s, which is large for a PN. The diameter measured on the HST images is
about 0.23" or 0.15 pc at the distance of the Fornax dSph. CONCLUSIONS: This
object doubles the number of known PNe in Fornax, and is only the 5th PN
associated with an old GC for which direct imaging is available. It may be a
member of the rare class of extremely H-deficient PNe, the second such case
found in a GC.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:21:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Larsen",
"S. S.",
"",
"Astronomical Institute, Utrecht University"
]
] | [
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] |
711.225 | Jeffrey Weiss | Jeffrey B. Weiss | Fluctuation Properties of Steady-State Langevin Systems | 8 pages, to be published in Physical Review E | null | 10.1103/PhysRevE.76.061128 | null | cond-mat.stat-mech physics.ao-ph | null | Motivated by stochastic models of climate phenomena, the steady-state of a
linear stochastic model with additive Gaussian white noise is studied.
Fluctuation theorems for nonequilibrium steady-states provide a constraint on
the character of these fluctuations. The properties of the fluctuations which
are unconstrained by the fluctuation theorem are investigated and related to
the model parameters. The irreversibility of trajectory segments, which
satisfies a fluctuation theorem, is used as a measure of nonequilibrium
fluctuations. The moments of the irreversibility probability density function
(pdf) are found and the pdf is seen to be non-Gaussian. The average
irreversibility goes to zero for short and long trajectory segments and has a
maximum for some finite segment length, which defines a characteristic
timescale of the fluctuations. The initial average irreversibility growth rate
is equal to the average entropy production and is related to
noise-amplification. For systems with a separation of deterministic timescales,
modes with timescales much shorter than the trajectory timespan and whose noise
amplitudes are not asymptotically large, do not, to first order, contribute to
the irreversibility statistics, providing a potential basis for dimensional
reduction.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:22:58 GMT"
}
] | 2008-01-04T00:00:00 | [
[
"Weiss",
"Jeffrey B.",
""
]
] | [
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711.2251 | Olaf Kaczmarek | Sourendu Gupta, Kay Hubner, Olaf Kaczmarek | Renormalized Polyakov loops in many representations | 17 pages, 24 figures, revtex4 | Phys.Rev.D77:034503,2008 | 10.1103/PhysRevD.77.034503 | BI-TP 2007/30, BNL-NT-07/45, TIFR/TH/07-30 | hep-lat hep-ph | null | We present a renormalization procedure for Polyakov loops which explicitly
implements the fact that the renormalization constant depends only on the
ultraviolet cutoff. Using this we study the renormalized Polyakov loops in all
representations upto the {\bf 27} of the gauge group SU(3). We find good
evidence for Casimir scaling of the Polyakov loops and for approximate large-N
factorization. By studying many loops together, we are able to show that there
is a matrix model with a single coupling which can describe the high
temperature phase of QCD, although it is hard to construct explicitly. We
present the first results for the non-vanishing renormalized octet loop in the
thermodynamic limit below the SU(3) phase transition, and estimate the
associated string breaking distance and the gluelump binding energy. By
studying the connection of the direct renormalization procedure with a
generalization of an earlier suggestion which goes by the name of the $Q\bar Q$
renormalization procedure, we find that they are functionally equivalent.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:24:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Gupta",
"Sourendu",
""
],
[
"Hubner",
"Kay",
""
],
[
"Kaczmarek",
"Olaf",
""
]
] | [
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] |
711.2252 | Jouravlev Mikhail | M.V. Jouravlev | Asymptotic estimations of power thresholds and anti-Stokes frequency of
laser induced thermal scattering in microresonators | 6 pages, 3 figures | null | null | null | physics.optics physics.chem-ph | null | A derivation of the asymptotic expressions for the threshold intensity of
laser induced thermal scattering in silica microresonator when illuminated with
a plane wave is present. The calculation of anti-Stokes thermal combination
frequencies are made for the spherical high Q-factor microresonators. The three
modes regime of nonlinear interaction is considered. One pump-driven, two
signal modes, and one mode of temperature relaxation are taken into account,
satisfying morphology-dependent input and output resonances. There are low
power thresholds for laser induced thermal scattering at morphology dependent
resonances.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:27:01 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Jouravlev",
"M. V.",
""
]
] | [
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] |
711.2253 | Federico von der Pahlen | Herbi K. Dreiner, Olaf Kittel, and Federico von der Pahlen | Disentangling CP phases in nearly degenerate resonances: neutralino
production via Higgs at a muon collider | 36 pages, 10 figures, minor typos corrected, to appear in JHEP | JHEP 0801:017,2008 | 10.1088/1126-6708/2008/01/017 | BONN-TH-2007-13 | hep-ph | null | In the CP-violating Minimal Supersymmetric Standard Model, we study the pair
production of neutralinos at center-of-mass energies around the heavy neutral
Higgs boson resonances. For longitudinally polarized muon beams, we analyze CP
asymmetries which are sensitive to the interference of the two heavy neutral
Higgs bosons. Due to radiatively induced scalar-pseudoscalar transitions, the
CP asymmetries can be strongly enhanced when the resonances are nearly
degenerate, as in the Higgs decoupling limit. The Higgs couplings to the
neutralino sector can then be analyzed in the presence of CP violating phases.
We present a detailed numerical analysis of the cross sections, neutralino
branching ratios, and the CP observables. We find that radiatively induced CP
violation in the Higgs sector leads to sizable CP-asymmetries, which are
accessible in future measurements at a muon collider. However, we expect that
our proposed method should be applicable to other processes with nearly
degenerate scalar resonances, even at hadron colliders.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:57:42 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 17:18:09 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Dreiner",
"Herbi K.",
""
],
[
"Kittel",
"Olaf",
""
],
[
"von der Pahlen",
"Federico",
""
]
] | [
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] |
711.2254 | Felix Fehr | Felix Fehr (for the ANTARES Collaboration) | Calibration systems and methods for the ANTARES neutrino telescope | 4 pages, 3 figures, to appear in the proceedings of 30th
International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico,
3-11 Jul 2007 | null | null | FAU-ECAP-07-01 | astro-ph | null | The ANTARES neutrino telescope is currently being constructed in the
Mediterranean Sea. The complete detector will consist of 12 strings,
supplemented by an additional instrumentation line. Nine strings are at present
deployed of which five are already connected to the shore and operating. Each
string is equipped with 75 Optical Modules (OMs) housing the photomultipliers
to detect the Cherenkov light induced by the charged particles produced in
neutrino reactions. An accurate measurement of the Cherenkov photon arrival
times as well as the positions and orientations of the OMs is required for a
precise reconstruction of the direction of the detected neutrinos. For this
purpose the ANTARES detector is provided with several system s to facilitate
the calibration of the detector. The time calibration is performed using light
pulses emitted from LED and laser devices. The positioning is done via acoustic
triangulation using hydrophones. Additionally, local tilt angles and the
orientations of the modules are measured with a set of tiltmeters and
compasses. In this paper, it is demonstrated that the ANTARES time and
alignment calibration systems operate successfully in situ. In particular, it
is shown that the ANTARES read-out electronics is capable of reaching a
sub-nanosecond time resolution.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:47:28 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Fehr",
"Felix",
"",
"for the ANTARES Collaboration"
]
] | [
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] |
711.2255 | Xiang Liu | I. Abt, A. Caldwell, K. Kroeninger, J. Liu, X. Liu, B. Majorovits | Neutron Interactions as Seen by A Segmented Germanium Detector | 17 pages, 10 figures, submitted to EPJC | Eur.Phys.J.A36:139-149,2008 | 10.1140/epja/i2007-10553-8 | null | nucl-ex | null | The GERmanium Detector Array, GERDA, is designed for the search for
``neutrinoless double beta decay'' (0-nu-2-beta) with germanium detectors
enriched in Ge76. An 18-fold segmented prototype detector for GERDA Phase II
was exposed to an AmBe neutron source to improve the understanding of neutron
induced backgrounds. Neutron interactions with the germanium isotopes
themselves and in the surrounding materials were studied. Segment information
is used to identify neutron induced peaks in the recorded energy spectra. The
Geant4 based simulation package MaGe is used to simulate the experiment. Though
many photon peaks from germanium isotopes excited by neutrons are correctly
described by Geant4, some physics processes were identified as being
incorrectly treated or even missing.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:55:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Abt",
"I.",
""
],
[
"Caldwell",
"A.",
""
],
[
"Kroeninger",
"K.",
""
],
[
"Liu",
"J.",
""
],
[
"Liu",
"X.",
""
],
[
"Majorovits",
"B.",
""
]
] | [
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] |
711.2256 | Antoine Letessier-Selvon | The Pierre Auger Collaboration | Correlation of the highest energy cosmic rays with nearby extragalactic
objects | 22 pages, 2 figures | Science 318:938-943,2007 | 10.1126/science.1151124 | null | astro-ph | null | Using data collected at the Pierre Auger Observatory during the past 3.7
years, we demonstrated a correlation between the arrival directions of cosmic
rays with energy above ~ 6x10^{19} electron volts and the positions of active
galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis
of an isotropic distribution of these cosmic rays with at least a 99%
confidence level from a prescribed a priori test. The correlation we observed
is compatible with the hypothesis that the highest energy particles originate
from nearby extragalactic sources whose flux has not been substantially reduced
by interaction with the cosmic background radiation. AGN or objects having a
similar spatial distribution are possible sources.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:35:38 GMT"
}
] | 2012-08-27T00:00:00 | [
[
"The Pierre Auger Collaboration",
"",
""
]
] | [
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] |
711.2257 | Rustem Khasanov | R. Khasanov, A. Shengelaya, D.Di Castro, E. Morenzoni, A. Maisuradze,
I.M. Savi\'c, K. Conder, E. Pomjakushina, and H. Keller | Oxygen isotope effect on superconductivity and magnetism in
Y_1-xPr_xBa_2Cu_3O_7-\delta | 5 pages, 3 figures, 1 table | Phys. Rev. Lett. 101, 077001 (2008) | 10.1103/PhysRevLett.101.077001 | null | cond-mat.supr-con | null | Oxygen isotope (^{16}O/^{18}O) effects (OIE's) on the superconducting
transition (T_c), the spin-glass ordering (T_g), and the antiferromagnetic
ordering (T_N) temperatures were studied for Y_1-xPr_xBa_2Cu_3O_7-\delta as a
function of Pr content (0.0\leq x \leq 1.0). The OIE on T_c increases with
increasing x up to x\approx0.55, where superconductivity disappears. For
decreasing x the OIE's on T_N and T_g increase down to x\approx 0.7 where
antiferromagnetic order and down to x\approx0.3 where spin-glass behavior
vanish, respectively. The OIE's on T_g and T_N are found to have {\it opposite
signs} as compared to the OIE on T_c. All OIE's are suggested to arise from the
isotope dependent mobility (kinetic energy) of the charge carriers.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:47:10 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Khasanov",
"R.",
""
],
[
"Shengelaya",
"A.",
""
],
[
"Di Castro",
"D.",
""
],
[
"Morenzoni",
"E.",
""
],
[
"Maisuradze",
"A.",
""
],
[
"Savić",
"I. M.",
""
],
[
"Conder",
"K.",
""
],
[
"Pomjakushina",
"E.",
""
],
[
"Keller",
"H.",
""
]
] | [
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711.2258 | Pawel Urbanski | Wlodzimierz M. Tulczyjew | Density operators and selective measurements | 5 pages | null | null | null | math-ph math.MP | null | It is widely believed that statistical interpretation of quantum mechanics
requires that density operators representing quantum states be normalized. We
present a description of selective measurements in terms of density operators.
The description is inspired by Schwinger's Algebra of Microscopic Measurements.
Density operators used are not normalized. We do not know applications of
density operators requiring normalization.
| [
{
"version": "v1",
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711.2259 | Anthony Thomas Prof | A. W. Thomas | The Pion Cloud: Insights into Hadron Structure | Invited talk at Yukawa Institute Kyoto | Prog.Theor.Phys.168:614,2007 | 10.1143/PTPS.168.614 | null | nucl-th | null | Modern nuclear theory presents a fascinating study in contrasting approaches
to the structure of hadrons and nuclei. Nowhere is this more apparent than in
the treatment of the pion cloud. As this discussion really begins with Yukawa,
it is entirely appropriate that this invited lecture at the Yukawa Institute in
Kyoto should deal with the issue.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:48:22 GMT"
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] | 2009-11-13T00:00:00 | [
[
"Thomas",
"A. W.",
""
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711.226 | Elio Conte | Elio Conte | A Quantum Like Interpretation and Solution of Einstein, Podolsky, and
Rosen Paradox in Quantum Mechanics | 9 pages | Proceedings Fundamental problems of Sciences,271-304,S.Petersburg
2002 | null | null | quant-ph | null | We discuss the Einstein, Podolsky, and Rosen paradox as it was formulated by
Asher Peres in 1992 [4]. On this basis we realize an algebraic quantum like
elaboration showing that in this formulation the paradox may be still
interpreted and solved.
| [
{
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"created": "Wed, 14 Nov 2007 17:51:53 GMT"
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] |
711.2261 | T. K. Sridharan | F. M. Fazal, T. K. Sridharan, K. Qiu, T. P. Robitaille, B. A. Whitney,
Q. Zhang | Spectral Energy Distributions of High Mass Proto Stellar Objects -
Evidence for High Accretion Rates | 10 pages; 3 figures; 3 tables | null | 10.1086/593975 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The spectral energy distributions (SEDs), spanning the mid-infrared to
millimeter wavelengths, of a sample of 13 high-mass protostellar objects
(HMPOs) were studied using a large archive of 2-D axisymmetric radiative
transfer models. Measurements from the Spitzer GLIMPSE and MIPSGAL surveys and
the MSX survey were used in addition to our own surveys at millimeter and
submillimeter wavelengths to construct the SEDs, which were then fit to the
archive of models. These models assumed that stars of all masses form via
accretion and allowed us to make estimates for the masses, luminosities and
envelope accretion rates for the HMPOs. The models fit the observed SEDs well.
The implied envelope accretion rates are high, $\approx 10^{-2.5} \msun/yr$,
consistent with the accretion-based scenario of massive star formation. With
the fitted accretion rates and with mass estimates of up to $\sim 20 \msun$ for
these objects, it appears plausible that stars with stellar masses $M_{\ast} >
20 \msun$ can form via accretion.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:36:44 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Apr 2008 21:22:12 GMT"
},
{
"version": "v3",
"created": "Wed, 24 Sep 2008 18:58:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fazal",
"F. M.",
""
],
[
"Sridharan",
"T. K.",
""
],
[
"Qiu",
"K.",
""
],
[
"Robitaille",
"T. P.",
""
],
[
"Whitney",
"B. A.",
""
],
[
"Zhang",
"Q.",
""
]
] | [
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] |
711.2262 | Mustapha Bentaiba | S.-A. Yahiaoui, M. Bentaiba | Weak-Pseudo-Hermiticity of Non-Hermitian Hamiltonians with
Position-Dependent Mass | 17 pages | null | null | null | math-ph math.MP | null | We extend the definition of eta-weak-pseudo-Hermiticity to the class of
potentials endowed with position-dependent mass. The construction of
non-Hermitian Hamiltonians through some generating function are obtained.
Special cases of potentials are thus deduced.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:03:20 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Yahiaoui",
"S. -A.",
""
],
[
"Bentaiba",
"M.",
""
]
] | [
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] |
711.2263 | Benjamin Zwickl | B. M. Zwickl, W. E. Shanks, A. M. Jayich, C. Yang, A. C. Bleszynski
Jayich, J. D. Thompson, and J. G. E. Harris | High quality mechanical and optical properties of commercial silicon
nitride membranes | 4 pages, 4 figures | null | 10.1063/1.2884191 | null | quant-ph | null | We have measured the optical and mechanical loss of commercial silicon
nitride membranes. We find that 50 nm-thick, 1 mm^2 membranes have mechanical Q
> 10^6 at 293 K, and Q > 10^7 at 300 mK, well above what has been observed in
devices with comparable dimensions. The near-IR optical loss at 293 K is less
than 2E-4. This combination of properties make these membranes attractive
candidates for studying quantum effects in optomechanical systems.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:07:29 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zwickl",
"B. M.",
""
],
[
"Shanks",
"W. E.",
""
],
[
"Jayich",
"A. M.",
""
],
[
"Yang",
"C.",
""
],
[
"Jayich",
"A. C. Bleszynski",
""
],
[
"Thompson",
"J. D.",
""
],
[
"Harris",
"J. G. E.",
""
]
] | [
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] |
711.2264 | Ian Hunter | I. Hunter, D.J. Lennon, P.L. Dufton, C. Trundle, S. Simon-Diaz, S.J.
Smartt, R.S.I. Ryans, C.J. Evans | The VLT-FLAMES survey of massive stars: atmospheric parameters and
rotational velocity distributions for B-type stars in the Magellanic Clouds | 25 pages with tables. 11 figures. Submitted to A&A and corrected for
referee's comments | null | 10.1051/0004-6361:20078511 | null | astro-ph | null | We provide atmospheric parameters and rotational velocities of a large sample
(~400) of O- and early B-type stars, analysed in a homogeneous and consistent
manner, for use in constraining theoretical models. Comparison of the
rotational velocities with evolutionary tracks suggest that the end of core
hydrogen burning occurs later than currently predicted. We also show that the
large number of the luminous blue supergiants observed in the fields are
unlikely to have directly evolved from main-sequence massive O-type stars as
neither their low rotational velocities or position on the H-R diagram are
predicted. We suggest that blue-loops or mass-transfer binary systems may
populate the blue supergiant regime. By comparing the rotational velocity
distributions of the Magellanic Cloud stars to a similar Galactic sample we
find that (at 3sigma confidence level) massive stars (above 8Msun) in the SMC
rotate faster than those in the solar neighbourhood. However there appears to
be no significant difference between the rotational velocity distributions in
the Galaxy and the LMC. We find that the vsini distributions in the SMC and LMC
can modelled with an intrinsic rotational velocity distribution which is a
Gaussian peaking at 175km/s (SMC) and 100km/s (LMC). We find that in NGC346 in
the SMC, the 10-25Msun main-sequence stars appear to rotate faster than their
higher mass counterparts. Recently Yoon et al. (2006) have determined rates of
GRBs by modelling rapidly rotating massive star progenitors. Our measured
rotational velocity distribution for the 10-25Msun stars is peaked at slightly
higher velocities than they assume, supporting the idea that GRBs could come
from rapid rotators with initial masses as low as 14Msun at low metallicities.
(abridged).
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:11:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hunter",
"I.",
""
],
[
"Lennon",
"D. J.",
""
],
[
"Dufton",
"P. L.",
""
],
[
"Trundle",
"C.",
""
],
[
"Simon-Diaz",
"S.",
""
],
[
"Smartt",
"S. J.",
""
],
[
"Ryans",
"R. S. I.",
""
],
[
"Evans",
"C. J.",
""
]
] | [
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] |
711.2265 | Mustapha Bentaiba | S.-A. Yahiaoui, M. Bentaiba | Exactly Solvable Potentials by SO(2,2) Dynamical Algebra | 22 pages | null | null | null | math-ph math.MP | null | The differential realization of the potential group SO(2,2) is used. The
spectrum-generating algebra for a kind of exactly solvable potentials endowed
with position-dependent mass is constructed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:13:35 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Yahiaoui",
"S. -A.",
""
],
[
"Bentaiba",
"M.",
""
]
] | [
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] |
711.2266 | Antoine Mellet | L. A. Caffarelli and A. Mellet | Random Homogenization of Fractional Obstacle Problems | null | null | null | null | math.AP | null | We use a characterization of the fractional Laplacian as a Dirichlet to
Neumann operator for an appropriate differential equation to study its obstacle
problem in perforated domains.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:18:20 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Caffarelli",
"L. A.",
""
],
[
"Mellet",
"A.",
""
]
] | [
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] |
711.2267 | Ian Hunter | I. Hunter, I. Brott, D.J. Lennon, N. Langer, P.L. Dufton, C. Trundle,
S.J. Smartt, A. de Koter, C.J. Evans and R.S.I. Ryans | The VLT-FLAMES survey of massive stars: rotation and nitrogen enrichment
as the key to understanding massive star evolution | ApJL. 10 pages, 1 figure. Updated to match accepted version | null | 10.1086/587436 | null | astro-ph | null | Rotation has become an important element in evolutionary models of massive
stars, specifically via the prediction of rotational mixing. Here, we study a
sample of stars, including rapid rotators, to constrain such models and use
nitrogen enrichments as a probe of the mixing process. Chemical compositions
(C, N, O, Mg and Si) have been estimated for 135 early B-type stars in the
Large Magellanic Cloud with projected rotational velocities up to ~300km/s
using a non-LTE TLUSTY model atmosphere grid. Evolutionary models, including
rotational mixing, have been generated attempting to reproduce these
observations by adjusting the overshooting and rotational mixing parameters and
produce reasonable agreement with 60% of our core hydrogen burning sample. We
find (excluding known binaries) a significant population of highly nitrogen
enriched intrinsic slow rotators vsini less than 50km/s incompatible with our
models ~20% of the sample). Furthermore, while we find fast rotators with
enrichments in agreement with the models, the observation of evolved (log g
less than 3.7dex) fast rotators that are relatively unenriched (a further ~20%
of the sample) challenges the concept of rotational mixing. We also find that
70% of our blue supergiant sample cannot have evolved directly from the
hydrogen burning main-sequence. We are left with a picture where invoking
binarity and perhaps fossil magnetic fields are required to understand the
surface properties of a population of massive main sequence stars.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:23:47 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 18:55:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hunter",
"I.",
""
],
[
"Brott",
"I.",
""
],
[
"Lennon",
"D. J.",
""
],
[
"Langer",
"N.",
""
],
[
"Dufton",
"P. L.",
""
],
[
"Trundle",
"C.",
""
],
[
"Smartt",
"S. J.",
""
],
[
"de Koter",
"A.",
""
],
[
"Evans",
"C. J.",
""
],
[
"Ryans",
"R. S. I.",
""
]
] | [
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] |
711.2268 | Fabrizio Illuminati | M. Blasone, F. Dell'Anno, S. De Siena, M. Di Mauro, F. Illuminati | Multipartite entangled states in particle mixing | 18 pages, 7 figures | Phys. Rev. D 77, 096002 (2008) | 10.1103/PhysRevD.77.096002 | null | quant-ph hep-ph hep-th | null | In the physics of flavor mixing, the flavor states are given by
superpositions of mass eigenstates. By using the occupation number to define a
multiqubit space, the flavor states can be interpreted as multipartite
mode-entangled states. By exploiting a suitable global measure of entanglement,
based on the entropies related to all possible bipartitions of the system, we
analyze the correlation properties of such states in the instances of three-
and four-flavor mixing. Depending on the mixing parameters, and, in particular,
on the values taken by the free phases, responsible for the CP-violation,
entanglement concentrates in preferred bipartitions. We quantify in detail the
amount and the distribution of entanglement in the physically relevant cases of
flavor mixing in quark and neutrino systems. By using the wave packet
description for localized particles, we use the global measure of entanglement,
suitably adapted for the instance of multipartite mixed states, to analyze the
decoherence induced by the free evolution dynamics on the quantum correlations
of stationary neutrino beams. We define a decoherence length as the distance
associated with the vanishing of the coherent interference effects among
massive neutrino states. We investigate the role of the CP-violating phase in
the decoherence process.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:24:56 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Mar 2008 22:11:56 GMT"
}
] | 2009-07-02T00:00:00 | [
[
"Blasone",
"M.",
""
],
[
"Dell'Anno",
"F.",
""
],
[
"De Siena",
"S.",
""
],
[
"Di Mauro",
"M.",
""
],
[
"Illuminati",
"F.",
""
]
] | [
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] |
711.2269 | Luke Rogers | Jessica L. DeGrado, Luke G. Rogers, Robert S. Strichartz | Gradients of Laplacian Eigenfunctions on the Sierpinski Gasket | LaTex, 8 pages, 4 figures | null | null | null | math.CA math.FA | null | We use spectral decimation to provide formulae for computing the harmonic
gradients of Laplacian eigenfunctions on the Sierpinski Gasket. These formulae
are given in terms of special functions that are defined as infinite products.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:28:12 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"DeGrado",
"Jessica L.",
""
],
[
"Rogers",
"Luke G.",
""
],
[
"Strichartz",
"Robert S.",
""
]
] | [
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] |
711.227 | Igor M. Suslov | I. M. Suslov (P.L.Kapitza Institute for Physical Problems, Moscow,
Russia) | Can a Computer Laugh ? | English translation of the paper in Russian; 18 pages, 6 figures
included | Computer Chronicle (Moscow), 1994, issue 1, p.1 | null | null | cs.CL cs.AI q-bio.NC | null | A computer model of "a sense of humour" suggested previously
[arXiv:0711.2058,0711.2061], relating the humorous effect with a specific
malfunction in information processing, is given in somewhat different
exposition. Psychological aspects of humour are elaborated more thoroughly. The
mechanism of laughter is formulated on the more general level. Detailed
discussion is presented for the higher levels of information processing, which
are responsible for a perception of complex samples of humour. Development of a
sense of humour in the process of evolution is discussed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:32:09 GMT"
}
] | 2007-11-27T00:00:00 | [
[
"Suslov",
"I. M.",
"",
"P.L.Kapitza Institute for Physical Problems, Moscow,\n Russia"
]
] | [
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] |
711.2271 | Roger Francis Picken | J. E. Nelson and R. F. Picken | A quantum Goldman bracket in 2+1 quantum gravity | 9 pages, 4 figures, dedication added, very minor corrections | J.Phys.A41:304011,2008 | 10.1088/1751-8113/41/30/304011 | null | math-ph gr-qc hep-th math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In the context of quantum gravity for spacetimes of dimension 2+1, we
describe progress in the construction of a quantum Goldman bracket for
intersecting loops on surfaces. Using piecewise linear paths in R^2
(representing loops on the spatial manifold, i.e. the torus) and a quantum
connection with noncommuting components, we review how holonomies and Wilson
loops for two homotopic paths are related by phases in terms of the signed area
between them. Paths rerouted at intersection points with other paths occur on
the r.h.s. of the Goldman bracket. To better understand their nature we
introduce the concept of integer points inside the parallelogram spanned by two
intersecting paths, and show that the rerouted paths must necessarily pass
through these integer points.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:41:57 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Jul 2008 17:05:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Nelson",
"J. E.",
""
],
[
"Picken",
"R. F.",
""
]
] | [
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] |
711.2272 | Dmitry V. Belyaev | Dmitry V. Belyaev, Peter van Nieuwenhuizen | Tensor calculus for supergravity on a manifold with boundary | 20 pages, JHEP format; published version | JHEP0802:047,2008 | 10.1088/1126-6708/2008/02/047 | DESY-07-208, YITP-SB-07-33 | hep-th hep-ph | null | Using the simple setting of 3D N=1 supergravity, we show how the tensor
calculus of supergravity can be extended to manifolds with boundary. We present
an extension of the standard F-density formula which yields supersymmetric
bulk-plus-boundary actions. To construct additional separately supersymmetric
boundary actions, we decompose bulk supergravity and bulk matter multiplets
into co-dimension one submultiplets. As an illustration we obtain the
supersymmetric extension of the York-Gibbons-Hawking extrinsic curvature
boundary term. We emphasize that our construction does not require any boundary
conditions on off-shell fields. This gives a significant improvement over the
existing orbifold supergravity tensor calculus.
| [
{
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"created": "Wed, 14 Nov 2007 20:51:59 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 15:01:59 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Belyaev",
"Dmitry V.",
""
],
[
"van Nieuwenhuizen",
"Peter",
""
]
] | [
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711.2273 | Jun Takahashi | Jun Takahashi (for the STAR collaboration) | Energy and System Size Dependence of Strangeness Production from SPS to
RHIC | 6 pages, SQM2007 conference proceedings, to be published in Jornal of
Phys. G | J.Phys.G35:044007,2008 | 10.1088/0954-3899/35/4/044007 | null | nucl-ex | null | Strange particle production is an important experimental observable that
allows the study of the strongly interacting matter created in relativistic
heavy-ion collisions. The STAR experiment at RHIC has a unique capability of
measuring identified strange particles over a wide range of acceptance
providing a rich set of data to perform a systematic study. In addition to the
data from Au+Au collisions, strange particles from p+p and d+Au collisions are
also available for comparison and normalization. A new set of data from Cu+Cu
reactions at 62 GeV and 200 GeV provides the chance to compare the system size
dependence observed in Au+Au collisions with this smaller system size. In
addition to the comparison of the yields, a statistical thermal model was used
to extract freeze-out characteristics for the different system sizes and
collision energies.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 18:54:23 GMT"
},
{
"version": "v2",
"created": "Fri, 16 Nov 2007 12:32:22 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Takahashi",
"Jun",
"",
"for the STAR collaboration"
]
] | [
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] |
711.2274 | Jose Geraldo Pereira | R. Aldrovandi, J. G. Pereira | de Sitter Relativity: a New Road to Quantum Gravity? | 18 pages, no figures. v3: Important presentation changes intended to
clarify some points of the previous version; title slightly changed and
references added. Version to be published in Foundations of Physics | Found.Phys.39:1-19,2009 | 10.1007/s10701-008-9258-5 | null | gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Poincare' group generalizes the Galilei group for high-velocity
kinematics. The de Sitter group is assumed to go one step further, generalizing
Poincare' as the group governing high-energy kinematics. In other words,
ordinary special relativity is here replaced by de Sitter relativity. In this
theory, the cosmological constant is no longer a free parameter, and can be
determined in terms of other quantities. When applied to the whole universe, it
is able to predict the value of the cosmological constant and to explain the
cosmic coincidence. When applied to the propagation of ultra-high energy
photons, it gives a good estimate of the time delay observed in extragalactic
gamma-ray flares. It can, for this reason, be considered a new paradigm to
approach the quantum gravity problem.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:35:41 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 14:17:55 GMT"
},
{
"version": "v3",
"created": "Wed, 12 Nov 2008 11:08:54 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Aldrovandi",
"R.",
""
],
[
"Pereira",
"J. G.",
""
]
] | [
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] |
711.2275 | Joseph Schechter | Amir H. Fariborz, Renata Jora, Joseph Schechter | Scalar mesons from an effective Lagrangian approach | 10 pages, 5 figures, menu 2007 talk | ECONFC070910:107,2007 | null | null | hep-ph | null | A brief discussion of the recent interest in light scalar mesons motivates
the study of a generalized linear sigma model. In an SU(3) flavor invariant
version of the model there is a prediction that the the lighter scalars have
sizeable "four quark" content. It is further predicted that one of the singlet
scalars should be exceptionally light. Due to the presence of scalar mesons,
the model gives "controlled" corrections to the current algebra formula for
threshold pion pion scattering. These corections act in the direction to
improve agreement with current experiments.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:13:08 GMT"
},
{
"version": "v2",
"created": "Fri, 16 Nov 2007 17:08:59 GMT"
},
{
"version": "v3",
"created": "Wed, 16 Jan 2008 20:14:59 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Fariborz",
"Amir H.",
""
],
[
"Jora",
"Renata",
""
],
[
"Schechter",
"Joseph",
""
]
] | [
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] |
711.2276 | Valeri Dvoeglazov | Valeri V. Dvoeglazov (Universidad de Zacatecas) | Fermion-fermion and boson-boson amplitudes: surprising similarities | 7 pages, no figures, talks given at the 5th International Symposium
on "Quantum Theory and Symmetries", July 22-28, 2007, Valladolid, Spain and
the 10th Workshop "What comes beyond the Standard Model?", July 17-27, 2007,
Bled, Slovenia | J.Phys.Conf.Ser.128:012002,2008 | 10.1088/1742-6596/128/1/012002 | null | math-ph hep-ph hep-th math.MP | null | Amplitudes for fermion-fermion, boson-boson and fermion-boson interactions
are calculated in the second order of perturbation theory in the Lobachevsky
space. An essential ingredient of the model is the Weinberg's 2(2j+1)-component
formalism for describing a particle of spin j. The boson-boson amplitude is
then compared with the two-fermion amplitude obtained long ago by Skachkov on
the basis of the Hamiltonian formulation of quantum field theory on the mass
hyperboloid, p_0^2 - p^2=M^2, proposed by Kadyshevsky. The parametrization of
the amplitudes by means of the momentum transfer in the Lobachevsky space leads
to same spin structures in the expressions of T-matrices for the fermion case
and the boson case. However, certain differences are found. Possible physical
applications are discussed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:15:01 GMT"
}
] | 2011-09-02T00:00:00 | [
[
"Dvoeglazov",
"Valeri V.",
"",
"Universidad de Zacatecas"
]
] | [
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] |
711.2277 | Ignacio Taboada | Ignacio Taboada and Michelangelo V. D'Agostino | Correlating prompt GRB photons with neutrinos | null | null | null | null | astro-ph | null | It is standard in theoretical neutrino astrophysics to use a broken power law
approximation, based on the Band function, to describe the average photon flux
of the prompt emission of Gamma-Ray Bursts. We will show that this
approximation overestimates the contribution of high energy gamma-rays (and
underestimates low energy gamma-rays). As a consequence models that rely on
this approximation overestimate neutrino event rate by a factor of approx 2
depending on Earth's column density in the direction of the GRB. Furthermore
the characteristic energy of neutrinos that trigger a km^3 detector is
typically 10^{16} eV, higher than previously predicted. We also provide a new
broken power law approximation to the Band function and show that it properly
represents the photon spectra.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:24:45 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Taboada",
"Ignacio",
""
],
[
"D'Agostino",
"Michelangelo V.",
""
]
] | [
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711.2278 | Valeri Dvoeglazov | Valeri V. Dvoeglazov (Universidad de Zacatecas) | Antisymmetric Tensor Fields, 4-Vector Fields, Indefinite Metrics and
Normalization | 9 pages, no figures, talks given at the VII Mexican School on
Gravitation and Mathematical Physics "Relativistic Astrophysics and Numerical
Relativity", November 26 -- December 1, 2006, Playa del Carmen, QR, Mexico;
and the 10th Workshop "What comes beyond the Standard Model?", July 17-27,
2007, Bled, Slovenia | J.Phys.Conf.Ser.91:012009,2007 | null | null | math-ph gr-qc hep-th math.MP | null | On the basis of our recent modifications of the Dirac formalism we generalize
the Bargmann-Wigner formalism for higher spins to be compatible with other
formalisms for bosons. Relations with dual electrodynamics, with the
Ogievetskii-Polubarinov notoph and the Weinberg 2(2J+1) theory are found. Next,
we introduce the dual analogues of the Riemann tensor and derive corresponding
dynamical equations in the Minkowski space. Relations with the Marques-Spehler
chiral gravity theory are discussed. The problem of indefinite metrics,
particularly, in quantization of 4-vector fields is clarified.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:22:19 GMT"
}
] | 2011-09-15T00:00:00 | [
[
"Dvoeglazov",
"Valeri V.",
"",
"Universidad de Zacatecas"
]
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711.2279 | Andrew DeBenedictis | A. DeBenedictis | Developments in Black Hole Research: Classical, Semi-classical, and
Quantum | 59 pages, 17 figures (some are quality reduced due to file size
restrictions). Version 2 has extra references and minor changes to match
version for publication. Invited chapter to appear in an edited collection
'Classical and Quantum Gravity Research', Nova Science Publishers | Classical and Quantum Gravity Research, 371-426, (2008), Nova Sci.
Pub. ISBN 978-1-60456-366-5 | null | null | gr-qc | null | The possible existence of black holes has fascinated scientists at least
since Michell and Laplace's proposal that a gravitating object could exist from
which light could not escape. In the 20th century, in light of the general
theory of relativity, it became apparent that, were such objects to exist,
their structure would be far richer than originally imagined. Today,
astronomical observations strongly suggest that either black holes, or objects
with similar properties, not only exist but may well be abundant in our
universe. In light of this, black hole research is now not only motivated by
the fascinating theoretical properties such objects must possess but also as an
attempt to better understand the universe around us. We review here some
selected developments in black hole research, from a review of its early
history to current topics in black hole physics research. Black holes have been
studied at all levels; classically, semi-classically, and more recently, as an
arena to test predictions of candidate theories of quantum gravity. We will
review here progress and current research at all these levels as well as
discuss some proposed alternatives to black holes.
| [
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"version": "v1",
"created": "Wed, 14 Nov 2007 19:25:27 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 01:01:53 GMT"
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] | 2008-11-15T00:00:00 | [
[
"DeBenedictis",
"A.",
""
]
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711.228 | Peter Petreczky | Peter Petreczky | Properties of quark gluon plasma from lattice calculations | Invited talk at Zimanyi 75 Memorial workshop, 8 pages, uses
svjour.cls | Eur.Phys.J.ST155:123-130,2008 | 10.1140/epjst/e2008-00596-y | null | hep-lat | null | I discuss lattice QCD calculations of the properties of strongly interacting
matter at finite temperature, including the determination of the transition
temperature Tc, equation of state, different static screening lengths and
quarkonium spectral functions. The lattice data suggest that at temperatures
above 2Tc many properties of the quark gluon plasma can be understood using
weak coupling approach, although non-perturbative effects due to static
magnetic fields are significant in some quantities.
| [
{
"version": "v1",
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[
"Petreczky",
"Peter",
""
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] |
711.2281 | Eduardo Gonz\'alez-Alfonso | Eduardo Gonz\'alez-Alfonso, Howard A. Smith, Matthew L. N. Ashby,
Jacqueline Fischer, Luigi Spinoglio, Timothy W. Grundy | High-excitation OH and H_2O lines in Markarian 231: the molecular
signatures of compact far-infrared continuum sources | 16 pages, 6 figures, accepted for publication in The Astrophysical
Journal | null | 10.1086/527292 | null | astro-ph | null | The ISO/LWS far-infrared spectrum of the ultraluminous galaxy Mkn 231 shows
OH and H_2O lines in absorption from energy levels up to 300 K above the ground
state, and emission in the [O I] 63 micron and [C II] 158 micron lines. Our
analysis shows that OH and H_2O are radiatively pumped by the far-infrared
continuum emission of the galaxy. The absorptions in the high-excitation lines
require high far-infrared radiation densities, allowing us to constrain the
properties of the underlying continuum source. The bulk of the far-infrared
continuum arises from a warm (T_dust=70-100 K), optically thick
(tau_100micron=1-2) medium of effective diameter 200-400 pc. In our best-fit
model of total luminosity L_IR, the observed OH and H2O high-lying lines arise
from a luminous (L/L_IR~0.56) region with radius ~100 pc. The high surface
brightness of this component suggests that its infrared emission is dominated
by the AGN. The derived column densities N(OH)>~10^{17} cm^{-2} and
N(H_2O)>~6x10^{16} cm^{-2} may indicate XDR chemistry, although significant
starburst chemistry cannot be ruled out. The lower-lying OH, [C II] 158 micron,
and [O I] 63 micron lines arise from a more extended (~350 pc) starburst
region. We show that the [C II] deficit in Mkn 231 is compatible with a high
average abundance of C+ because of an extreme overall luminosity to gas mass
ratio. Therefore, a [C II] deficit may indicate a significant contribution to
the luminosity by an AGN, and/or by extremely efficient star formation.
| [
{
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"version": "v4",
"created": "Tue, 20 Nov 2007 18:57:27 GMT"
},
{
"version": "v5",
"created": "Mon, 24 Dec 2007 09:18:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"González-Alfonso",
"Eduardo",
""
],
[
"Smith",
"Howard A.",
""
],
[
"Ashby",
"Matthew L. N.",
""
],
[
"Fischer",
"Jacqueline",
""
],
[
"Spinoglio",
"Luigi",
""
],
[
"Grundy",
"Timothy W.",
""
]
] | [
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] |
711.2282 | Todor Stanev | Todor Stanev (Bartol Research Institute, Department of Physics and
Astronomy, University of Delaware) | Ultra High Energy Cosmic Rays: origin and propagation | LaTeX, 15 pages, 13 postscript figures, Invited talk at the 30th
International Conference of Cosmic Rays, July 2007, Merida, Mexico | null | 10.1142/9789812790156_0008 | null | astro-ph | null | We discuss the basic difficulties in understanding the origin of the highest
energy particles in the Universe - the ultrahigh energy cosmic rays (UHECR). It
is difficult to imagine the sources they are accelerated in. Because of the
strong attenuation of UHECR on their propagation from the sources to us these
sources should be at cosmologically short distance from us but are currently
not identified. We also give information of the most recent experimental
results including the ones reported at this conference and compare them to
models of the UHECR origin.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:37:25 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Stanev",
"Todor",
"",
"Bartol Research Institute, Department of Physics and\n Astronomy, University of Delaware"
]
] | [
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] |
711.2283 | Mohamed Assad Abdel-Raouf | Mohamed Assad Abdel-Raouf | Possible Coexistence of Antihydrogen with Hydrogen, Deuterium and
Tritium Atoms | 29 pages, 3 Figures and 4 Tables | null | null | null | physics.atm-clus physics.plasm-ph | null | Recent productions of large numbers of cold antiprotons as well as the
formation of antihydrogens at CERN and Fermilab have raised basic questions
about possible coexistence of matter and antimatter in nature. In the present
work, previous mathematical considerations are revisited which support the
possible coexistence of Antihydrogen with Hydrogen, Deuterium and Tritium
atoms. In particular, the main objective of the present work is to present
computational treatments which confirm the possible formation of these quasi
molecules in laboratory. These treatments are based on a nonadiabatic picture
of the system in which generalized basis functions are adjusted within the
framework of Rayleigh-Ritz' variational method. Thus, it is ruled out in the
present work the Born-Oppenheimer adiabatic picture of the system, which
demands the existence of bound states composed of fixed quasi heavy atoms
(containing at least two baryons, e.g. protonium (Pn), with mean lifetime
1.0x10^^-6 s) and quasi light atoms (composed of two leptons, e.g. positronium
(Ps), with mean lifetime 125x10^^-12 s for para-Ps and 142.05x10^^-9 s for
ortho-Ps). Our calculations of the binding energies and internal structure of
Antihydrogen-Hydrogen, Antihydrogen-Deuterium and Antihydrogen-Tritium show
that these quasi molecules are bound and could be formed in nature. On the
other hand, having in mind the adiabatic picture of the systems, our results
suggest the possible formation of these molecules as resonant states in
Antihydrogen-Atom interaction. Nevertheless, several arguments are accumulated
in the conclusion as consequences of the proposed bound states.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:38:39 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 11:21:22 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Abdel-Raouf",
"Mohamed Assad",
""
]
] | [
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] |
711.2284 | Rainer Grauer | Tobias Grafke, Holger Homann, Juergen Dreher, and Rainer Grauer | Numerical simulations of possible finite time singularities in the
incompressible Euler equations: comparison of numerical methods | Euler equations: 250 years on | null | 10.1016/j.physd.2007.11.006 | null | physics.flu-dyn physics.comp-ph | null | The numerical simulation of the 3D incompressible Euler equation is analyzed
with respect to different integration methods. The numerical schemes we
considered include spectral methods with different strategies for dealiasing
and two variants of finite difference methods. Based on this comparison, a
Kida-Pelz like initial condition is integrated using adaptive mesh refinement
and estimates on the necessary numerical resolution are given. This estimate is
based on analyzing the scaling behavior similar to the procedure in critical
phenomena and present simulations are put into perspective.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:40:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Grafke",
"Tobias",
""
],
[
"Homann",
"Holger",
""
],
[
"Dreher",
"Juergen",
""
],
[
"Grauer",
"Rainer",
""
]
] | [
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] |
711.2285 | Eric White | Eric White and Qing He | Impact on $\gamma\phi_3$ from CLEO-c Using CP-tagged $D\toK_{S,L}\pi\pi$
Decays | 5 pages, 5 figures, submitted to Charm 2007 Workshop Conference
proceedings | ECONF C070805:26,2007 | null | null | hep-ex | null | Precision determination of the CKM angle $\gamma/\phi_3$ depends upon
constraints on charm mixing amplitudes, measurements of doubly-Cabibbo
suppressed amplitudes and relative phases, and studies of charm Dalitz plots
tagged by flavor or CP eigenstates. In this note we describe the technique used
at CLEO-c to constrain the $K_{S,L}\pi\pi$ model uncertainty, and its impact on
$\gamma/\phi_3$ measurements at B-factories presented at the Charm 2007
Workshop.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:46:04 GMT"
}
] | 2010-01-05T00:00:00 | [
[
"White",
"Eric",
""
],
[
"He",
"Qing",
""
]
] | [
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] |
711.2286 | Anton Klimovsky | Anton Bovier, Anton Klimovsky | The Aizenman-Sims-Starr scheme for the SK model with multidimensional
spins | 29 pages, presented on Frankfurter Stochastik-Tage 2006, Frankfurt,
14-17.03.2006 and on The 5th Prague Summer School on Mathematical Statistical
Mechanics, September 10-23, Prague, 2006 This paper has been temporarily
withdrawn for revision by the authors | null | null | null | math.PR math-ph math.MP | null | This paper has been temporarily withdrawn for revision by the authors.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:23:42 GMT"
},
{
"version": "v2",
"created": "Thu, 15 Nov 2007 14:48:56 GMT"
},
{
"version": "v3",
"created": "Sat, 24 Nov 2007 17:35:50 GMT"
}
] | 2007-11-24T00:00:00 | [
[
"Bovier",
"Anton",
""
],
[
"Klimovsky",
"Anton",
""
]
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] |
711.2287 | Nicolas Douguet | Nicolas Douguet, Juan Blandon, Viatcheslav Kokoouline | Correlation diagrams in collisions of three identical particles | 14 pages,4 figures | null | 10.1088/0953-4075/41/4/045202 | null | physics.atom-ph | null | We discuss collision of three identical particles and derive scattering
selection rules from initial to final states of the particles. We use either
laboratory-frame, hyperspherical, or Jacobian coordinates depending on which
one is best suited to describe three different configurations of the particles:
(1) three free particles, (2) a quasi-bound trimer, or (3) a dimer and a free
particle. We summarize quantum numbers conserved during the collision as well
as quantum numbers that are appropriate for a given configuration but may
change during the scattering process. The total symmetry of the system depends
on these quantum numbers. Based on the selection rules, we construct
correlation diagrams between different configurations before and after a
collision. In particular, we describe a possible recombination of the system
into one free particle and a dimer, which can be used, for example, to identify
possible decay products of quasi-stationary three-body states
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:53:07 GMT"
},
{
"version": "v2",
"created": "Tue, 20 Nov 2007 20:59:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Douguet",
"Nicolas",
""
],
[
"Blandon",
"Juan",
""
],
[
"Kokoouline",
"Viatcheslav",
""
]
] | [
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] |
711.2288 | Pedro Lacerda | Pedro Lacerda | Detection of Contact Binaries Using Sparse High Phase Angle Lightcurves | 4 pages, 4 figures, 1 table. Accepted for publication in ApJL | null | 10.1086/526454 | null | astro-ph | null | We show that candidate contact binary asteroids can be efficiently identified
from sparsely sampled photometry taken at phase angles >60deg. At high phase
angle, close/contact binary systems produce distinctive lightcurves that spend
most of the time at maximum or minimum (typically >1mag apart) brightness with
relatively fast transitions between the two. This means that a few (~5) sparse
observations will suffice to measure the large range of variation and identify
candidate contact binary systems. This finding can be used in the context of
all-sky surveys to constrain the fraction of contact binary near-Earth objects.
High phase angle lightcurve data can also reveal the absolute sense of the
spin.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:56:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lacerda",
"Pedro",
""
]
] | [
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711.2289 | Francisco Fernandez Dr. | Francisco M. Fernandez | Accurate calculation of resonances in multiple-well oscillators | null | null | 10.1088/1751-8113/41/6/065202 | null | math-ph math.MP | null | Quantum--mechanical multiple--well oscillators exhibit curious complex
eigenvalues that resemble resonances in models with continuum spectra. We
discuss a method for the accurate calculation of their real and imaginary
parts.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:57:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fernandez",
"Francisco M.",
""
]
] | [
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] |
711.229 | Zhongxiang Wang | Z. Wang, C. Bassa, V. M. Kaspi, J. B. Bryant, and N. Morrell | Optical/Infrared Observations of the Anomalous X-ray Pulsar 1E
1048.1-5937 During Its 2007 X-Ray Flare | 5 pages, 1 figure, accepted by ApJ | null | 10.1086/587505 | null | astro-ph | null | We report on optical and infrared observations of the anomalous X-ray pulsar
(AXP) 1E 1048.1-5937, made during its ongoing X-ray flare which started in 2007
March. We detected the source in the optical I and near-infrared Ks bands in
two ground-based observations and obtained deep flux upper limits from four
observations, including one with the Spitzer Space Telescope at 4.5 and 8.0
microns. The detections indicate that the source was approximately 1.3--1.6
magnitudes brighter than in 2003--2006, when it was at the tail of a previous
similar X-ray flare. Similar related flux variations have been seen in two
other AXPs during their X-ray outbursts, suggesting common behavior for large
X-ray flux variation events in AXPs. The Spitzer flux 1E 1048.1-5937 limits are
sufficiently deep that we can exclude mid-infrared emission similar to that
from the AXP 4U 0142+61, which has been interpreted as arising from a dust disk
around the AXP. The optical/near-infrared emission from probably has a
magnetospheric origin. The similarity in the flux spectra of 4U 0142+61 and 1E
1048.1-5937 challenges the dust disk model proposed for the latter.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:09:06 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 18:18:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wang",
"Z.",
""
],
[
"Bassa",
"C.",
""
],
[
"Kaspi",
"V. M.",
""
],
[
"Bryant",
"J. B.",
""
],
[
"Morrell",
"N.",
""
]
] | [
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711.2291 | Brett Kotschwar | Brett Kotschwar and Lei Ni | Local gradient estimates of p-harmonic functions, 1/H-flow, and an
entropy formula | 31 pages | null | null | null | math.AP math.DG | null | In the first part of this paper, we prove local interior and boundary
gradient estimates for p-harmonic functions on general Riemannian manifolds.
With these estimates, following the strategy in recent work of R. Moser, we
prove an existence theorem for weak solutions to the level set formulation of
the 1/H (inverse mean curvature) flow for hypersurfaces in ambient manifolds
satisfying a sharp volume growth assumption. In the second part of this paper,
we consider two parabolic analogues of the p-Laplace equation and prove sharp
Li-Yau type gradient estimates for positive solutions to these equations on
manifolds of nonnegative Ricci curvature. For one of these equations, we also
prove an entropy monotonicity formula generalizing an earlier such formula of
the second author for the linear heat equation. As an application of this
formula, we show that a complete Riemannian manifold with non-negative Ricci
curvature and sharp L^p-logarithmic Sobolev inequality must be isometric to
Euclidean space.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 19:59:21 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Kotschwar",
"Brett",
""
],
[
"Ni",
"Lei",
""
]
] | [
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711.2292 | Arbab Ibrahim Arbab | Arbab I. Arbab | Viscous Dark Energy Models with Variable G and Lambda | 6 Latex pages | Chin.Phys.Lett.25:3834-3838,2008 | 10.1088/0256-307X/25/10/086 | null | hep-th | null | We consider a cosmological model with bulk viscosity ($\eta$) and variable
cosmological $(\Lambda\propto \rho^{-\alpha}, \alpha=\rm const.$) and
gravitational ($G$) constants. The model exhibits many interesting cosmological
features. Inflation proceeds du to the presence of bulk viscosity and dark
energy without requiring the equation of state $p=-\rho$. During the
inflationary era the energy density ($\rho$) does not remain constant, as in
the de-Sitter type. Moreover, the cosmological and gravitational constants
increase exponentially with time, whereas the energy density and viscosity
decrease exponentially with time. The rate of mass creation during inflation is
found to be very huge suggesting that all matter in the universe was created
during inflation.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:03:37 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Arbab",
"Arbab I.",
""
]
] | [
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711.2293 | Simon Portegies Zwart | Simon Portegies Zwart (UvA) Edward P.J. van den Heuvel (UvA) | A runaway collision in a young star cluster as the origin of the
brightest supernova | null | Nature450:388-389,2007 | 10.1038/nature06276 | null | astro-ph | null | Supernova 2006gy in the galaxy NGC 1260 is the most luminous one recorded
\cite{2006CBET..644....1Q, 2006CBET..647....1H, 2006CBET..648....1P,
2006CBET..695....1F}. Its progenitor might have been a very massive ($>100$
\msun) star \cite{2006astro.ph.12617S}, but that is incompatible with hydrogen
in the spectrum of the supernova, because stars $>40$ \msun are believed to
have shed their hydrogen envelopes several hundred thousand years before the
explosion \cite{2005A&A...429..581M}. Alternatively, the progenitor might have
arisen from the merger of two massive stars \cite{2007ApJ...659L..13O}. Here we
show that the collision frequency of massive stars in a dense and young cluster
(of the kind to be expected near the center of a galaxy) is sufficient to
provide a reasonable chance that SN 2006gy resulted from such a bombardment. If
this is the correct explanation, then we predict that when the supernova fades
(in a year or so) a dense cluster of massive stars becomes visible at the site
of the explosion.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:12:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Zwart",
"Simon Portegies",
"",
"UvA"
],
[
"Heuvel",
"Edward P. J. van den",
"",
"UvA"
]
] | [
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711.2294 | Brian M. Andersen | Brian M. Andersen, P. J. Hirschfeld | Breakdown of universal transport in correlated d-wave superconductors | 5 pages, 2 figures | Phys. Rev. Lett. 100, 257003 (2008) | 10.1103/PhysRevLett.100.257003 | null | cond-mat.supr-con cond-mat.str-el | null | The prediction and observation of low-temperature universal thermal
conductivity in cuprates has served as a keystone of theoretical approaches to
the superconducting state, but recent measurements on underdoped samples show
strong violations of this apparently fundamental property of d-wave nodal
quasiparticles. Here, we show that the breakdown of universality may be
understood as the consequence of disorder-induced magnetic states in the
presence of increasing antiferromagnetic correlations in the underdoped state,
even as these same correlations protect the nodal low-energy density of states
in agreement with recent scanning tunneling experiments.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:15:13 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Dec 2007 08:12:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Andersen",
"Brian M.",
""
],
[
"Hirschfeld",
"P. J.",
""
]
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] |
711.2295 | Dinshaw Balsara | D.S. Balsara, A.J. Bendinelli, D.A. Tilley, A.R. Massari, J.C. Howk | Simulating Anisotropic Thermal Conduction in Supernova Remnants,
Implications for the Interstellar Medium | null | null | 10.1111/j.1365-2966.2008.13121.x | null | astro-ph | null | We present a large number of two and a half dimensional simulations of
supernova remnants expanding into interstellar media having a range of
densities, temperatures and magnetic field strengths. The volume of hot gas
produced is strongly dependent on the inclusion of thermal conduction and
magnetic fields. The four-volumes and three-areas of hot gas have been
catalogued and their dependence on interstellar parameters documented.
Simulated line widths of radioactive species ejected by supernovae have also
been catalogued.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:15:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Balsara",
"D. S.",
""
],
[
"Bendinelli",
"A. J.",
""
],
[
"Tilley",
"D. A.",
""
],
[
"Massari",
"A. R.",
""
],
[
"Howk",
"J. C.",
""
]
] | [
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] |
711.2296 | Victor Kac | Victor G. Kac and Minoru Wakimoto | On rationality of W-algebras | 41 pages | Transformation Groups 13 (2008), 671-713 | null | null | math-ph math.MP | null | We study the problem of classification of triples ($\mathfrak{g}, f, k$),
where $\mathfrak{g}$ is a simple Lie algebra, $f$ its nilpotent element and $k
\in \CC$, for which the simple $W$-algebra $W_k (\mathfrak{g}, f)$ is rational.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:27:56 GMT"
}
] | 2014-01-17T00:00:00 | [
[
"Kac",
"Victor G.",
""
],
[
"Wakimoto",
"Minoru",
""
]
] | [
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] |
711.2297 | Claudio Simeone | Martin Richarte and Claudio Simeone | Traversable wormholes in a string cloud | 21 pages, 10 figures; accepted for publication in Int. J. Mod. Phys.
D | Int.J.Mod.Phys.D17:1179-1196,2008 | 10.1142/S0218271808012759 | null | gr-qc astro-ph | null | We study spherically symmetric thin-shell wormholes in a string cloud
background in (3+1)-dimensional spacetime. The amount of exotic matter required
for the construction, the traversability and the stability under radial
perturbations, are analyzed as functions of the parameters of the model.
Besides, in the Appendices a non perturbative approach to the dynamics and a
possible extension of the analysis to a related model are briefly discussed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:41:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Richarte",
"Martin",
""
],
[
"Simeone",
"Claudio",
""
]
] | [
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] |
711.2298 | Valery Nesvizhevsky | V.V. Nesvizhevsky, G. Pignol, K.V. Protasov | Neutron scattering and extra short range interactions | null | Phys.Rev.D77:034020,2008 | 10.1103/PhysRevD.77.034020 | null | hep-ph | null | The available data on neutron scattering were analyzed to constrain a
hypothetical new short-range interaction. We show that these constraints are
several orders of magnitude better than those usually cited in the range
between 1 pm and 5 nm. This distance range occupies an intermediate space
between collider searches for strongly coupled heavy bosons and searches for
new weak macroscopic forces. We emphasise the reliability of the neutron
constraints in so far as they provide several independent strategies. We have
identified the most promising way to improve them.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:42:49 GMT"
},
{
"version": "v2",
"created": "Wed, 14 Nov 2007 21:57:00 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Nesvizhevsky",
"V. V.",
""
],
[
"Pignol",
"G.",
""
],
[
"Protasov",
"K. V.",
""
]
] | [
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] |
711.2299 | Vesna Borka Jovanovi\'c | Vesna Borka Jovanovi\'c | Masses and Mixing of $c q \bar{q} \bar{q}$ Tetraquarks Using
Glozman-Riska Hyperfine Interaction | 10 pages, 6 tables, 6 figures. Accepted for publication in Phys. Rev.
D | Phys.Rev.D76:105011,2007 | 10.1103/PhysRevD.76.105011 | null | hep-ph | null | In this paper we perform a detailed study of the masses and mixing of the
single charmed scalar tetraquarks: $c q \bar{q} \bar{q}$. We also give a
systematic analysis of these tetraquark states by weight diagrams, quantum
numbers and flavor wave functions. Tetraquark masses are calculated using four
different fits. The following SU(3)$_\mathrm{F}$ representations are discussed:
$\bar{15}_\mathrm{S}$, $\bar{3}_\mathrm{S}$, $6_\mathrm{A}$ and
$\bar{3}_\mathrm{A}$. We use the flavor-spin Glozman-Riska interaction
Hamiltonian with SU(3) flavor symmetry breaking. There are 27 different
tetraquarks composed of a charm quark $c$ and of the three light flavors $u, d,
s$: 11 cryptoexotic (3 D$_\mathrm{s}^{+}$, 4 D$^{+}$, 4 D$^{0}$) and 16
explicit exotic states. We discuss D$_\mathrm{s}$ and its isospin partners in
the same multiplet, as well as all the other four-quark states. Some explicit
exotic states appear in the spectrum with the same masses as
D$_\mathrm{s}^{+}$(2632) in $\bar{15}_\mathrm{S}$ and with the same masses as
D$_\mathrm{s}^{+}$(2317) in $6_\mathrm{A}$ representation, which confirm the
tetraquark nature of these states.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:45:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Jovanović",
"Vesna Borka",
""
]
] | [
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] |
711.23 | David Kubiznak | David Kubiznak and Valeri P. Frolov | Stationary strings and branes in the higher-dimensional Kerr-NUT-(A)dS
spacetimes | 8 pages, no figures | JHEP0802:007,2008 | 10.1088/1126-6708/2008/02/007 | Alberta-Thy-16-07 | hep-th gr-qc | null | We demonstrate complete integrability of the Nambu-Goto equations for a
stationary string in the general Kerr-NUT-(A)dS spacetime describing the
higher-dimensional rotating black hole. The stationary string in D dimensions
is generated by a 1-parameter family of Killing trajectories and the problem of
finding a string configuration reduces to a problem of finding a geodesic line
in an effective (D-1)-dimensional space. Resulting integrability of this
geodesic problem is connected with the existence of hidden symmetries which are
inherited from the black hole background. In a spacetime with p mutually
commuting Killing vectors it is possible to introduce a concept of a
$\xi$-brane, that is a p-brane with the worldvolume generated by these fields
and a 1-dimensional curve. We discuss integrability of such $\xi$-branes in the
Kerr-NUT-(A)dS spacetime.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 22:04:10 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kubiznak",
"David",
""
],
[
"Frolov",
"Valeri P.",
""
]
] | [
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] |
711.2301 | Le Hur Karyn | Karyn Le Hur | Entanglement Entropy, decoherence, and quantum phase transition of a
dissipative two-level system | 38 pages, 8 figures, related to cond-mat/0612095 and arXiv:0705.0957;
final version to appear in Annals of Physics | Annals of Physics 323, 2208-2240 (2008) | 10.1016/j.aop.2007.12.003 | null | cond-mat.mes-hall cond-mat.other | null | The concept of entanglement entropy appears in multiple contexts, from black
hole physics to quantum information theory, where it measures the entanglement
of quantum states. We investigate the entanglement entropy in a simple model,
the spin-boson model, which describes a qubit (two-level system) interacting
with a collection of harmonic oscillators that models the environment
responsible for decoherence and dissipation. The entanglement entropy allows to
make a precise unification between entanglement of the spin with its
environment, decoherence, and quantum phase transitions. We derive exact
analytical results which are confirmed by Numerical Renormalization Group
arguments both for an ohmic and a subohmic bosonic bath. Those demonstrate that
the entanglement entropy obeys universal scalings. We make comparisons with
entanglement properties in the quantum Ising model and in the Dicke model. We
also emphasize the possibility of measuring this entanglement entropy using
charge qubits subject to electromagnetic noise; such measurements would provide
an empirical proof of the existence of entanglement entropy.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 23:12:55 GMT"
},
{
"version": "v2",
"created": "Fri, 23 Nov 2007 23:14:35 GMT"
},
{
"version": "v3",
"created": "Mon, 24 Mar 2008 14:26:54 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Hur",
"Karyn Le",
""
]
] | [
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711.2302 | Priya Natarajan | Priyamvada Natarajan (Yale), Darren Croton (Berkeley) and Gianfranco
Bertone (IAP) | Consequences of dark matter self-annihilation for galaxy formation | 16 pages, 8 figures, MNRAS, in press | null | 10.1111/j.1365-2966.2008.13306.x | null | astro-ph | null | Galaxy formation requires a process that continually heats gas and quenches
star formation in order to reproduce the observed shape of the luminosity
function of bright galaxies. To accomplish this, current models invoke heating
from supernovae, and energy injection from active galactic nuclei. However,
observations of radio-loud active galactic nuclei suggest that their feedback
is likely to not be as efficient as required, signaling the need for additional
heating processes. We propose the self-annihilation of weakly interacting
massive particles that constitute dark matter as a steady source of heating. In
this paper, we explore the circumstances under which this process may provide
the required energy input. To do so, dark matter annihilations are incorporated
into a galaxy formation model within the Millennium cosmological simulation.
Energy input from self-annihilation can compensate for all the required gas
cooling and reproduce the observed galaxy luminosity function only for what
appear to be extreme values of the relevant key parameters. The key parameters
are: the slope of the inner density profile of dark matter haloes and the outer
spike radius. The inner density profile needs to be steepened to slopes of -1.5
or more and the outer spike radius needs to extend to a few tens of parsecs on
galaxy scales and a kpc or so on cluster scales. If neutralinos or any thermal
relic WIMP with s-wave annihilation constitute dark matter, their
self-annihilation is inevitable and could provide enough power to modulate
galaxy formation. Energy from self-annihilating WIMPs could be yet another
piece of the feedback puzzle along with supernovae and active galactic nuclei.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:00:04 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Apr 2008 02:50:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Natarajan",
"Priyamvada",
"",
"Yale"
],
[
"Croton",
"Darren",
"",
"Berkeley"
],
[
"Bertone",
"Gianfranco",
"",
"IAP"
]
] | [
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711.2303 | Andres Jordan | Andres Jordan, Gregory R. Sivakoff, Dean E. McLaughlin, John P.
Blakeslee, Daniel A. Evans, Ralph P. Kraft, Martin J. Hardcastle, Eric W.
Peng, Patrick Cote, Judith H. Croston, Adrienne M. Juett, Dante Minniti,
Somak Raychaudhury, Craig L. Sarazin, Diana M. Worrall, William E. Harris,
Kristin A. Woodley, Mark Birkinshaw, Nicola J. Brassington, William R.
Forman, Christine Jones, Stephen S. Murray | Low-Mass X-ray Binaries and Globular Clusters in Centaurus A | 4 pages, 2 figures. Accepted for publication in ApJ Letters | null | 10.1086/525524 | null | astro-ph | null | We present results of Hubble Space Telescope and Chandra X-ray Observatory
observations of globular clusters (GCs) and low-mass X-ray binaries (LMXBs) in
the central regions of Centaurus A. Out of 440 GC candidates we find that 41
host X-ray point sources that are most likely LMXBs. We fit King models to our
GC candidates in order to measure their structural parameters. We find that GCs
that host LMXBs are denser and more compact, and have higher encounter rates
and concentrations than the GC population as a whole. We show that the higher
concentrations and masses are a consequence of the dependence of LMXB incidence
on central density and size plus the general trend for denser GCs to have
higher masses and concentrations. We conclude that neither concentration nor
mass are fundamental variables in determining the presence of LMXBs in GCs, and
that the more fundamental parameters relate to central density and size.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:01:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jordan",
"Andres",
""
],
[
"Sivakoff",
"Gregory R.",
""
],
[
"McLaughlin",
"Dean E.",
""
],
[
"Blakeslee",
"John P.",
""
],
[
"Evans",
"Daniel A.",
""
],
[
"Kraft",
"Ralph P.",
""
],
[
"Hardcastle",
"Martin J.",
""
],
[
"Peng",
"Eric W.",
""
],
[
"Cote",
"Patrick",
""
],
[
"Croston",
"Judith H.",
""
],
[
"Juett",
"Adrienne M.",
""
],
[
"Minniti",
"Dante",
""
],
[
"Raychaudhury",
"Somak",
""
],
[
"Sarazin",
"Craig L.",
""
],
[
"Worrall",
"Diana M.",
""
],
[
"Harris",
"William E.",
""
],
[
"Woodley",
"Kristin A.",
""
],
[
"Birkinshaw",
"Mark",
""
],
[
"Brassington",
"Nicola J.",
""
],
[
"Forman",
"William R.",
""
],
[
"Jones",
"Christine",
""
],
[
"Murray",
"Stephen S.",
""
]
] | [
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] |
711.2304 | Xin Liu | Xin Liu, Edwin L. Turner, Norio Narita, Yasushi Suto, Joshua N. Winn,
Toru Yamada, Bun'ei Sato, Wako Aoki, Motohide Tamura | A Technique for Detecting Starlight Scattered from Transiting Extrasolar
Planets with Application to HD 209458b | 8 pages, 4 figures; Submitted to ApJ | null | null | null | astro-ph | null | We present a new technique for detecting scattered starlight from transiting,
close-orbiting extrasolar giant planets (CEGPs) that has the virtues of
simplicity, robustness, linearity, and model-independence. Given a series of
stellar spectra obtained over various phases of the planetary orbit, the goal
is to measure the strength of the component scattered by the planet relative to
the component coming directly from the star. We use two complementary
strategies, both of which rely on the predictable Doppler shifts of both
components and on combining the results from many spectral lines and many
exposures. In the first strategy, we identify segments of the stellar spectrum
that are free of direct absorption lines and add them after Doppler-shifting
into the planetary frame. In the second strategy, we compare the distribution
of equivalent-width ratios of the scattered and direct components. Both
strategies are calibrated with a ``null test'' in which scrambled Doppler
shifts are applied to the spectral segments. As an illustrative test case, we
apply our technique to spectra of HD 209458 taken when the planet was near
opposition (with orbital phases ranging from 11 to 34$\arcdeg$, where
0$\arcdeg$ is at opposition), finding that the planet-to-star flux ratio is
$(1.4 \pm 2.9)\times10^{-4}$ in the wavelength range 554$-$681 nm. This
corresponds to a geometric albedo of $0.8 \pm 1.6$, assuming the phase function
of a Lambert sphere. Although the result is not statistically significant, the
achieved sensitivity and relatively small volume of data upon which it is based
are very encouraging for future ground-based spectroscopic studies of scattered
light from transiting CEGP systems.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:02:51 GMT"
}
] | 2007-11-16T00:00:00 | [
[
"Liu",
"Xin",
""
],
[
"Turner",
"Edwin L.",
""
],
[
"Narita",
"Norio",
""
],
[
"Suto",
"Yasushi",
""
],
[
"Winn",
"Joshua N.",
""
],
[
"Yamada",
"Toru",
""
],
[
"Sato",
"Bun'ei",
""
],
[
"Aoki",
"Wako",
""
],
[
"Tamura",
"Motohide",
""
]
] | [
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] |
711.2305 | Yanbin Yang | Y.Yang (1), H.Flores (1), F.Hammer (1), B.Neichel (1), M.Puech (2),
N.Nesvadba (1), A.Rawat (1 and 3), C.Cesarsky (2), M.Lehnert (1), L.Pozzetti
(4), I.Fuentes-Carrera (1), P.Amram (5), C.Balkowski (1), H.Dannerbauer (6),
S.diSeregoAlighieri (7), B.Guiderdoni (8), A.Kembhavi (3), Y.C.Liang (9), G.
\"Ostlin (10), C.D.Ravikumar (11), D.Vergani (12), J.Vernet (2), H.Wozniak
(8)((1) GEPI, Observatoire de Paris (2) ESO (3) Inter-University Centre for
Astronomy and Astrophysics (4) INAF, Osservatorio Astronomico di Bologna (5)
LAM (6) MPIA (7) INAF, Osservatorio Astrofisico di Arcetri (8) Centre de
Recherche Astronomique de Lyon (9) NAOC (10) Stockholm Observatory (11)
Department of Physics, University of Calicut (12) IASF-INAF) | IMAGES I. Strong evolution of galaxy kinematics since z=1 | 17 pages, 6 figures, Accepted by A&A | null | 10.1051/0004-6361:20078219 | null | astro-ph | null | (abbreviated) We present the first results of the ESO large program,
``IMAGES'' which aims at obtaining robust measurements of the kinematics of
distant galaxies using the multi-IFU mode of GIRAFFE on the VLT. 3D
spectroscopy is essential to robustly measure the often distorted kinematics of
distant galaxies (e.g., Flores et al. 2006). We derive the velocity fields and
$\sigma$-maps of 36 galaxies at 0.4<z<0.75 from the kinematics of the [OII]
emission line doublet, and generate a robust technique to identify the nature
of the velocity fields based on the pixels of the highest signal-to-noise
ratios (S/N). We have gathered a unique sample of 63 velocity fields of
emission line galaxies (W0([OII]) > 15 A) at z=0.4-0.75, which are a
representative subsample of the population of M_stellar>1.5x10^{10} M_sun
emission line galaxies in this redshift range, and are largely unaffected by
cosmic variance. Taking into account all galaxies -with or without emission
lines- in that redshift range, we find that at least 41+/-7% of them have
anomalous kinematics, i.e., they are not dynamically relaxed. This includes
26+/-7% of distant galaxies with complex kinematics, i.e., they are not simply
pressure or rotationally supported. Our result implies that galaxy kinematics
are among the most rapidly evolving properties, because locally, only a few
percent of the galaxies in this mass range have complex kinematics.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:11:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Yang",
"Y.",
"",
"1 and 3"
],
[
"Flores",
"H.",
"",
"1 and 3"
],
[
"Hammer",
"F.",
"",
"1 and 3"
],
[
"Neichel",
"B.",
"",
"1 and 3"
],
[
"Puech",
"M.",
"",
"1 and 3"
],
[
"Nesvadba",
"N.",
"",
"1 and 3"
],
[
"Rawat",
"A.",
"",
"1 and 3"
],
[
"Cesarsky",
"C.",
""
],
[
"Lehnert",
"M.",
""
],
[
"Pozzetti",
"L.",
""
],
[
"Fuentes-Carrera",
"I.",
""
],
[
"Amram",
"P.",
""
],
[
"Balkowski",
"C.",
""
],
[
"Dannerbauer",
"H.",
""
],
[
"diSeregoAlighieri",
"S.",
""
],
[
"Guiderdoni",
"B.",
""
],
[
"Kembhavi",
"A.",
""
],
[
"Liang",
"Y. C.",
""
],
[
"Östlin",
"G.",
""
],
[
"Ravikumar",
"C. D.",
""
],
[
"Vergani",
"D.",
""
],
[
"Vernet",
"J.",
""
],
[
"Wozniak",
"H.",
""
]
] | [
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] |
711.2306 | Xavier Calmet | Xavier Calmet and Stephen D. H. Hsu | TeV gravity in four dimensions? | 5 pages | Phys.Lett.B663:95-98,2008 | 10.1016/j.physletb.2008.04.002 | null | hep-ph hep-th | null | We describe a model in which the fundamental scale M_\star of the theory
which unifies gravity and quantum mechanics is in the TeV range, but without
requiring additional spacetime dimensions. The weakness of gravity at low
energies is due to a large vacuum expectation of a dilaton like field. The
model requires a small dimensionless parameter (the self-coupling of the
dilaton) but no fine-tuning. We discuss in detail the dynamical assumptions
about nonperturbative quantum gravity required within the model. We observe
that M_\star could be quite small, less than a TeV, and that the model could
lead to copious strong coupling effects at the LHC. However, semiclassical
black holes will not be produced.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:25:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Calmet",
"Xavier",
""
],
[
"Hsu",
"Stephen D. H.",
""
]
] | [
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] |
711.2307 | Matilde Mart\'iAnez | Matilde Mart\'inez, Shigenori Matsumoto and Alberto Verjovsky | Horocycle flows for laminations by hyperbolic Riemann surfaces and
Hedlund's theorem | Corrected version of previous paper "Hedlund's theorem for compact
minimal laminations" | null | null | null | math.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the dynamics of the geodesic and horocycle flows of the unit tangent
bundle $(\hat M, T^1\mathcal{F})$ of a compact minimal lamination $(M,\mathcal
F)$ by negatively curved surfaces. We give conditions under which the action of
the affine group generated by the joint action of these flows is minimal, and
examples where this action is not minimal. In the first case, we prove that if
$\mathcal F$ has a leaf which is not simply connected, the horocyle flow is
topologically transitive.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 21:45:22 GMT"
},
{
"version": "v2",
"created": "Tue, 27 May 2008 19:50:59 GMT"
},
{
"version": "v3",
"created": "Wed, 21 Nov 2012 21:54:46 GMT"
},
{
"version": "v4",
"created": "Wed, 15 Apr 2015 17:23:43 GMT"
}
] | 2016-02-01T00:00:00 | [
[
"Martínez",
"Matilde",
""
],
[
"Matsumoto",
"Shigenori",
""
],
[
"Verjovsky",
"Alberto",
""
]
] | [
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