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712.1379 | Masako Yamada | Masako Yamada | Three Dimensional Molecular Line Transfer Study of Extragalactic ISM :
AGN/Starburst Connection | 4 pages, 2 figures. Contribution to FIR Workshop 2007 "Far-Infrared
and Submillimeter Emission of the Interstellar Medium: Models meet
extragalactic and Galactic Observations" | null | 10.1051/eas:0831020 | null | astro-ph | null | Molecular gas in external galaxies is a subject of crucial importance for
observational and theoretical studies of galaxy formation. Compact molecular
gas around an active galactic nuclei (AGN) is expected to be an energy budget
of AGN and/or nuclear starburst. Recent observational studies suggest that line
ratios in millimeter and submillimeter band may be a good tool to reveal the
long-standing question on the origin of activity -- AGN or nuclear starburst.
We have constructed a powerful "telescope" of theory, three-dimensional nonLTE
line transfer code, preceding the high resolution and sensitivity observations
such as ALMA.
| [
{
"version": "v1",
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] | 2009-11-13T00:00:00 | [
[
"Yamada",
"Masako",
""
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712.138 | Daniel T Schmitt | Daniel T. Schmitt, Plamen Ch. Ivanov | Fractal scale-invariant and nonlinear properties of cardiac dynamics
remain stable with advanced age: A new mechanistic picture of cardiac control
in healthy elderly | 19 pages, 14 figures | The American Journal of Physiology - Regulatory, Integrative and
Comparative Physiology, vol 293, R1923-R1937, 2007 | 10.1152/ajpregu.00372.2007 | null | physics.data-an cond-mat.soft physics.bio-ph physics.med-ph q-bio.OT | null | We analyze heartbeat interval recordings from two independent databases: (a)
19 healthy young (avg. age 25.7 years) and 16 healthy elderly subjects (avg.
age 73.8 years) during 2h under resting conditions from the Fantasia database;
and (b) 29 healthy elderly subjects (avg. age 75.9 years) during $\approx{}8$h
of sleep from the SHHS database, and the same subjects recorded 5 years later.
We quantify: (1) The average heart rate <RR>; (2) the SD $\sigma_{RR}$ and
$\sigma_{\Delta{}RR}$ of the heartbeat intervals RR and their increments
$\Delta{}RR$; (3) the long-range correlations in RR as measured by the scaling
exponent $\alpha_{RR}$ using the Detrended Fluctuation Analysis; (4) fractal
linear and nonlinear properties as represented by the scaling exponents
$\alpha^{sign}$ and $\alpha^{mag}$ for the time series of the sign and
magnitude of $\Delta{}RR$; (5) the nonlinear fractal dimension $D(k)$ of $RR$
using the Fractal Dimension Analysis. We find: (1) No significant difference in
$\left<RR\right>$ (P>0.05); (2) a significant difference in $\sigma_{RR}$ and
$\sigma_{\Delta{}RR}$ for the Fantasia groups (P<10^{-4}) but no significant
change with age between the elderly SHHS groups (P>0.5); (3) no significant
change in the fractal measures $\alpha_{RR}$ (P>0.15), $\alpha^{sign}$ (P>0.2),
$\alpha^{mag}$ (P>0.3), and D(k) with age. Our findings do not support the
hypothesis that fractal linear and nonlinear characteristics of heartbeat
dynamics break down with advanced age in healthy subjects. While our results
indeed show a reduced SD of heartbeat fluctuations with advanced age, the
inherent temporal fractal and nonlinear organization of these fluctuations
remains stable.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 00:42:44 GMT"
}
] | 2016-09-08T00:00:00 | [
[
"Schmitt",
"Daniel T.",
""
],
[
"Ivanov",
"Plamen Ch.",
""
]
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712.1381 | Bin Zhu | Yu Zhou and Bin Zhu | Cluster combinatorics of d-cluster categories | correted many typos according to the referee's comments, final
version to appear in J. Algebra | null | null | null | math.RT math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the cluster combinatorics of $d-$cluster tilting objects in
$d-$cluster categories. By using mutations of maximal rigid objects in
$d-$cluster categories which are defined similarly for $d-$cluster tilting
objects, we prove the equivalences between $d-$cluster tilting objects, maximal
rigid objects and complete rigid objects. Using the chain of $d+1$ triangles of
$d-$cluster tilting objects in [IY], we prove that any almost complete
$d-$cluster tilting object has exactly $d+1$ complements, compute the extension
groups between these complements, and study the middle terms of these $d+1$
triangles. All results are the extensions of corresponding results on cluster
tilting objects in cluster categories established in [BMRRT] to $d-$cluster
categories. They are applied to the Fomin-Reading's generalized cluster
complexes of finite root systems defined and studied in [FR2] [Th] [BaM1-2],
and to that of infinite root systems [Zh3].
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 00:56:14 GMT"
},
{
"version": "v2",
"created": "Sat, 14 Feb 2009 04:38:21 GMT"
}
] | 2009-02-14T00:00:00 | [
[
"Zhou",
"Yu",
""
],
[
"Zhu",
"Bin",
""
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712.1382 | Lee Spitler | Lee R. Spitler, Duncan A. Forbes, Jay Strader, Jean P. Brodie and Jay
S. Gallagher III | The connection between globular cluster systems and their host galaxy
and environment: a case study of the isolated elliptical NGC 821 | Published in MNRAS. This version matches the published article | MNRAS Vol. 385 2008 p361 | 10.1111/j.1365-2966.2007.12823.x | null | astro-ph | null | In an effort to probe the globular cluster (GC) system of an isolated
elliptical galaxy, a comprehensive analysis of the NGC 821 GC system was
performed. New imaging from the WIYN Mini-Mosaic imager, supplemented with
Hubbl e Space Telescope (HST) WFPC2 images reveals a GC system similar to those
found in counterpart ellipticals located in high-density environments. To put
these results into the context of galaxy formation, a robustly-determined
census of GC systems is presented and analysed for galaxies spanning a wide
range of masses (> M_star), morphologies and environments.
Results from this meta-study: (1) confirm previous findings that the number
of GCs normalized by host galaxy stellar mass increases with host stellar mass.
Spiral galaxies in the sample show smaller relative GC numbers than those of
massive ellipticals, suggesting the GC systems of massive ellipticals were not
formed from major spiral-spiral mergers; (2) indicate that GC system numbers
per unit galaxy baryon mass increases with host baryon mass and that GC
formation efficiency may not be universal as previously thought; (3) suggest
previously reported trends with environment may be incorrect due to sample bias
or the use of galaxy stellar masses to normalize GC numbers. Thus claims for
environmentally dependent GC formation efficiencies should be revisited; (4) in
combination with weak-lensing halo mass estimates, suggest that GCs formed in
direct proportion to the halo mass; (5) are consistent with theoretical
predictions whereby the local epoch of re-ionization did not vary significantly
with environment or host galaxy type.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 00:57:34 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Apr 2008 23:28:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Spitler",
"Lee R.",
""
],
[
"Forbes",
"Duncan A.",
""
],
[
"Strader",
"Jay",
""
],
[
"Brodie",
"Jean P.",
""
],
[
"Gallagher",
"Jay S.",
"III"
]
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712.1383 | David Jacob | David Jacob | Spin transport in nanocontacts and nanowires | PhD thesis (2007), Universidad de Alicante, Spain; 134 pages, 47
figures | null | null | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | In this thesis we study electron transport through magnetic nanocontacts and
nanowires with ab initio quantum transport calculations. The aim is to gain a
thorough understanding of the interplay between electrical conduction and
magnetism in atomic-size conductors and how it is affected by different aspects
as e.g. the atomic structure and the chemical composition of the conductor. To
this end our ab initio quantum transport program ALACANT which combines the
non-equilibrium Green's function formalism (NEGF) with density functional
theory (DFT) calculations has been extended to describe spin-polarized systems.
We present calculations on nanocontacts made of Ni as a prototypical magnetic
material. We find that atomic disorder in the contact region strongly reduces
the a priori high spin-polarization of the conductance leading to rather
moderate values of the so-called ballistic magnetoresistance (BMR). On the
other hand, we show that the adsorption of oxygen in the contact region could
strongly enhance the spin-polarization of the conduction electrons and thus BMR
by eliminating the spin-unpolarized s-channel. Finally, we show that short
atomic Pt chains suspended between the tips of a nanocontact are magnetic in
contrast to bulk Pt. However, this emergent nanoscale magnetism barely affects
the overall conductance of the nanocontact making it thus difficult to
demonstrate by simple conductance measurements. In conclusion, we find that
spin-transport through atomic-scale conductors is quite sensitive to the actual
atomic structure as well as to the chemical composition of the conductor. This
presents both, opportunities and challenges for the realization of future
nanoscale spintronics devices.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 01:48:38 GMT"
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] | 2007-12-11T00:00:00 | [
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712.1384 | Xian-Hui Ge | Xian-Hui Ge, Fu-Wen Shu | Generalized entropy function for Schwarzschild and non-extremal black
holes in string theory | This paper has been withdrawn | null | null | null | hep-th | null | This paper has been withdrawn by the author due to a crucial error
| [
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{
"version": "v2",
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] |
712.1385 | Benoit Dherin | Alberto S. Cattaneo, Benoit Dherin, Alan Weinstein | Cotangent Microbundle Category, I | 32 pages, 5 figures | null | null | null | math-ph math.MP math.SG | null | We define a local version of the extended symplectic category, the cotangent
microbundle category, MiC, which turns out to be a true monoidal category. We
show that a monoid in this category induces a Poisson manifold together with
the local symplectic groupoid integrating it. Moreover, we prove that monoid
morphisms produce Poisson maps between the induced Poisson manifolds in a
functorial way. This gives a functor between the category of monoids in MiC and
the category of Poisson manifolds and Poisson maps. Conversely, the
semi-classical part of the Kontsevich star-product associated to a
real-analytic Poisson structure on an open subset of R^n produces a monoid in
MiC.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 02:46:01 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Cattaneo",
"Alberto S.",
""
],
[
"Dherin",
"Benoit",
""
],
[
"Weinstein",
"Alan",
""
]
] | [
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] |
712.1386 | Adam Nepomuk Otte | A. Nepomuk Otte (for the MAGIC collaboration) | Observation of the Crab Nebula with the MAGIC telescope | 4 pages, 5 figures, to appear in the proceedings of the 30th
International Cosmic Ray Conference, Merida, July 2007 | null | null | MPP-2007-185 | astro-ph | null | We report about very high energy (VHE) gamma-ray observations of the Crab
Nebula with the MAGIC telescope. The gamma-ray flux from the nebula was
measured between 60 GeV and 9 TeV. The energy spectrum can be described with a
curved power law dF/dE=f_0 (E/300GeV)^(a+b log10(E/300GeV)) with a flux
normalization f_0 of (6.0+-0.2stat)*10^-10 cm^-2 s^-1 TeV^-1, a=-2.31+-0.06stat
and b=-0.26+-0.07stat. The position of the IC-peak is determined at 77+-47 GeV.
Within the observation time and the experimental resolution of the telescope,
the gamma-ray emission is steady and pointlike. The emission's center of
gravity coincides with the position of the pulsar. Pulsed gamma-ray emission
from the pulsar could not be detected. We constrain the cutoff energy of the
spectrum to be less than ~30 GeV, assuming that the differential energy
spectrum has an exponential cutoff. For a super-exponential shape, the cutoff
energy can be as high as ~60GeV.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 03:02:12 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Otte",
"A. Nepomuk",
"",
"for the MAGIC collaboration"
]
] | [
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712.1387 | Manabu Machida | Manabu Machida, Jun Goryo, and Naomichi Hatano | Transient Oscillation of Currents in Quantum Hall Effect of Bloch
Electrons | 16 pages and 8 figures | J. Phys. Soc. Jpn. 77 (2008) 024713 | 10.1143/JPSJ.77.024713 | null | cond-mat.mes-hall | null | We consider the quantum Hall effect of two-dimensional electrons with a
periodic potential and study the time dependence of the Hall and longitudinal
currents when the electric field is applied abruptly. We find that the currents
oscillate in time with very large frequencies because of quantum fluctuation
and the oscillations eventually vanish, for their amplitudes decay as 1/t.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 03:15:07 GMT"
}
] | 2008-12-16T00:00:00 | [
[
"Machida",
"Manabu",
""
],
[
"Goryo",
"Jun",
""
],
[
"Hatano",
"Naomichi",
""
]
] | [
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] |
712.1388 | Yi-Kai Liu | Yi-Kai Liu | The Local Consistency Problem for Stoquastic and 1-D Quantum Systems | 18 pages, submitted to IEEE Conference on Computational Complexity
(CCC). v2: slightly revised introduction | null | null | null | quant-ph | null | The Local Hamiltonian problem (finding the ground state energy of a quantum
system) is known to be QMA-complete. The Local Consistency problem (deciding
whether descriptions of small pieces of a quantum system are consistent) is
also known to be QMA-complete. Here we consider special cases of Local
Hamiltonian, for ``stoquastic'' and 1-dimensional systems, that seem to be
strictly easier than QMA. We show that there exist analogous special cases of
Local Consistency, that have equivalent complexity (up to poly-time oracle
reductions). Our main technical tool is a new reduction from Local Consistency
to Local Hamiltonian, using SDP duality.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 03:15:22 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 03:12:17 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Liu",
"Yi-Kai",
""
]
] | [
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712.1389 | Hiromi Okada Dr. | H. Okada, I. Alekseev, A. Bravar, G. Bunce, S. Dhawan, K.O. Eyser, R.
Gill, W. Haeberli, H. Huang, O. Jinnouchi, Y. Makdisi, I. Nakagawa, A. Nass,
N. Saito, E. Stephenson, D. Sviridia, T. Wise, J. Wood, A. Zelenski | Absolute polarimetry at RHIC | 10 pages, PSTP07 proceedings contribution | AIPConf.Proc.980:370-379,2008 | 10.1063/1.2888110 | null | nucl-ex | null | Precise and absolute beam polarization measurements are critical for the RHIC
spin physics program. Because all experimental spin-dependent results are
normalized by beam polarization, the normalization uncertainty contributes
directly to final physics uncertainties. We aimed to perform the beam
polarization measurement to an accuracy of $\Delta P_{beam}/P_{beam} < 5%$.
The absolute polarimeter consists of Polarized Atomic Hydrogen Gas Jet Target
and left-right pairs of silicon strip detectors and was installed in the
RHIC-ring in 2004. This system features \textit{proton-proton} elastic
scattering in the Coulomb nuclear interference (CNI) region. Precise
measurements of the analyzing power $A_N$ of this process has allowed us to
achieve $\Delta P_{beam}/P_{beam} =4.2%$ in 2005 for the first long
spin-physics run.
In this report, we describe the entire set up and performance of the system.
The procedure of beam polarization measurement and analysis results from
2004-2005 are described. Physics topics of $A_N$ in the CNI region
(four-momentum transfer squared $0.001 < -t < 0.032 ~ ({\rm GeV}/c)^2$) are
also discussed. We point out the current issues and expected optimum accuracy
in 2006 and the future.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 03:26:52 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 20:07:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Okada",
"H.",
""
],
[
"Alekseev",
"I.",
""
],
[
"Bravar",
"A.",
""
],
[
"Bunce",
"G.",
""
],
[
"Dhawan",
"S.",
""
],
[
"Eyser",
"K. O.",
""
],
[
"Gill",
"R.",
""
],
[
"Haeberli",
"W.",
""
],
[
"Huang",
"H.",
""
],
[
"Jinnouchi",
"O.",
""
],
[
"Makdisi",
"Y.",
""
],
[
"Nakagawa",
"I.",
""
],
[
"Nass",
"A.",
""
],
[
"Saito",
"N.",
""
],
[
"Stephenson",
"E.",
""
],
[
"Sviridia",
"D.",
""
],
[
"Wise",
"T.",
""
],
[
"Wood",
"J.",
""
],
[
"Zelenski",
"A.",
""
]
] | [
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-0.0715361685,
-0.0337089412,
-0.0279128328
] |
712.139 | Naoyuki Sugimoto | Naoyuki Sugimoto, Shigeki Onoda, Naoto Nagaosa | Field-induced metal-insulator transition and switching phenomenon in
correlated insulators | 5 pages, 3 figures. A study on the metal-insulator transition in
correlated insulators was added | null | 10.1103/PhysRevB.78.155104 | null | cond-mat.other cond-mat.stat-mech | null | We study the nonequilibrium switching phenomenon associated with the
metal-insulator transition under electric field E in correlated insulator by a
gauge-covariant Keldysh formalism. Due to the feedback effect of the resistive
current I, this occurs as a first-order transition with a hysteresis of I-V
characteristics having a lower threshold electric field (\sim 10^4 Vcm^{-1})
much weaker than that for the Zener breakdown. It is also found that the
localized mid-gap states introduced by impurities and defects act as hot spots
across which the resonant tunneling occurs selectively, which leads to the
conductive filamentary paths and reduces the energy cost of the switching
function.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 03:35:51 GMT"
},
{
"version": "v2",
"created": "Fri, 30 May 2008 02:29:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sugimoto",
"Naoyuki",
""
],
[
"Onoda",
"Shigeki",
""
],
[
"Nagaosa",
"Naoto",
""
]
] | [
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712.1391 | Alex Kontorovich | Alex V. Kontorovich | The Hyperbolic Lattice Point Count in Infinite Volume with Applications
to Sieves | 33 pages, 1 figure, minor corrections. To appear, Duke Math J | Duke Math. J. 149, no. 1 (2009), 1-36 | 10.1215/00127094-2009-035 | null | math.NT math.SP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We develop novel techniques using abstract operator theory to obtain
asymptotic formulae for lattice counting problems on infinite-volume hyperbolic
manifolds, with error terms which are uniform as the lattice moves through
"congruence" subgroups.
We give the following application to the theory of affine linear sieves. In
the spirit of Fermat, consider the problem of primes in the sum of two squares,
f(c,d)=c^2+d^2, but restrict (c,d) to the orbit O = (0,1).Gamma, where Gamma is
an infinite-index non-elementary finitely-generated subgroup of SL(2,Z). Assume
that the Reimann surface Gamma\H^2 has a cusp at infinity. We show that the set
of values f(O) contains infinitely many integers having at most R prime factors
for any R>4/(delta-theta), where theta>1/2 is the spectral gap and delta<1 is
the Hausdorff dimension of the limit set of Gamma. If delta>149/150, then we
can take theta=5/6, giving R=25. The limit of this method is R=9 for
delta-theta>4/9. This is the same number of prime factors as attained in Brun's
original attack on the twin prime conjecture.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 03:58:37 GMT"
},
{
"version": "v2",
"created": "Fri, 20 Feb 2009 16:26:42 GMT"
}
] | 2019-12-19T00:00:00 | [
[
"Kontorovich",
"Alex V.",
""
]
] | [
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] |
712.1392 | Savel'ev Sergey | E.G. Galkina, B.A. Ivanov, Sergey Savel'ev, Franco Nori | Chirality tunneling and quantum dynamics for domain walls in mesoscopic
ferromagnets | 27 pages, 9 figures | null | 10.1103/PhysRevB.77.134425 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | We studied the quantum dynamics of ferromagnetic domain walls (topological
kink-type solitons) in one dimensional ferromagnetic spin chains. We show that
the tunneling probability does not depend on the number of spins in a domain
wall; thus, this probability can be large even for a domain wall containing a
large number of spins. We also predict that there is a strong interplay between
the tunneling of a wall from one lattice site to another (tunneling of the kink
coordinate) and the tunneling of the kink topological charge (so-called
chirality). Both of these elementary processes are suppressed for kinks in
one-dimensional ferromagnets with half-integer spin. The dispersion law (i.e.,
the domain wall energy versus momentum) is essentially different for chains
with either integer or half-integer spins. The predicted quantum effects could
be observed for mesoscopic magnetic structures, e.g., chains of magnetic
clusters, large-spin molecules, or nanosize magnetic dots.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 04:37:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Galkina",
"E. G.",
""
],
[
"Ivanov",
"B. A.",
""
],
[
"Savel'ev",
"Sergey",
""
],
[
"Nori",
"Franco",
""
]
] | [
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] |
712.1393 | Magdalena Czubak | Magdalena Czubak | Local wellposedness for the 2+1 dimensional monopole equation | 23 pages; Added some remarks, and rewrote parts of Sections 4 and 5;
Submitted | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The space-time monopole equation on $\R^{2+1}$ can be derived by a
dimensional reduction of the anti-self-dual Yang Mills equations on $\R^{2+2}$.
It can be also viewed as the hyperbolic analog of Bogomolny equations. We
uncover null forms in the nonlinearities and employ optimal bilinear estimates
in the framework of Wave-Sobolev spaces. As a result, we show the equation is
locally wellposed in the Coulomb gauge for initial data sufficiently small in
$H^s$ for $s>{1/4}$.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 04:39:11 GMT"
},
{
"version": "v2",
"created": "Tue, 10 Feb 2009 20:52:11 GMT"
}
] | 2009-02-10T00:00:00 | [
[
"Czubak",
"Magdalena",
""
]
] | [
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712.1394 | Gao Changjun | Changjun Gao, Fengquan Wu, Xuelei Chen and You-Gen Shen | A Holographic Dark Energy Model from Ricci Scalar Curvature | 7 pages, 8 figures. The discussions on structure formation and
k-essence reconstruction are added. To appear in Phys. Rev. D | Phys.Rev.D79:043511,2009 | 10.1103/PhysRevD.79.043511 | null | astro-ph gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Motivated by the holographic principle, it has been suggested that the dark
energy density may be inversely proportional to the area of the event horizon
of the Universe. However, such a model would have a causality problem. In this
paper, we propose to replace the future event horizon area with the inverse of
the Ricci scalar curvature. We show that this model does not only avoid the
causality problem and is phenomenologically viable, but also naturally solves
the coincidence problem of dark energy. Our analysis of the evolution of
density perturbations show that the matter power spectra and CMB temperature
anisotropy is only slightly affected by such modification.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 04:58:08 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Dec 2007 04:18:06 GMT"
},
{
"version": "v3",
"created": "Mon, 21 Jan 2008 05:10:30 GMT"
},
{
"version": "v4",
"created": "Thu, 25 Dec 2008 08:20:31 GMT"
}
] | 2009-09-02T00:00:00 | [
[
"Gao",
"Changjun",
""
],
[
"Wu",
"Fengquan",
""
],
[
"Chen",
"Xuelei",
""
],
[
"Shen",
"You-Gen",
""
]
] | [
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] |
712.1395 | Savel'ev Sergey | V.A. Yampol'skii, Sergey Savel'ev, Z. A. Mayselis, S. S. Apostolov,
Franco Nori | Anomalous temperature dependence of the Casimir force for thin metal
films | 4 pages, 2 figures | null | 10.1103/PhysRevLett.101.096803 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | Within the framework of the Drude dispersive model, we predict an unusual
non-monotonous temperature dependence of the Casimir force for thin metal
films. For certain conditions, this force decreases with temperature due to the
decrease of the metallic conductivity, whereas the force increases at high
temperatures due to the increase of the thermal radiation pressure. We consider
the attraction of a film to: either (i) a bulk ideal metal with a planar
boundary, or (ii) a bulk metal sphere (lens). The experimental observation of
the predicted non-monotonous temperature dependence of the Casimir force can
put an end to the long-standing discussion on the role of the electron
relaxation in the Casimir effect.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 05:03:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Yampol'skii",
"V. A.",
""
],
[
"Savel'ev",
"Sergey",
""
],
[
"Mayselis",
"Z. A.",
""
],
[
"Apostolov",
"S. S.",
""
],
[
"Nori",
"Franco",
""
]
] | [
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712.1396 | Alessandro Tomasiello | Alessandro Tomasiello | New string vacua from twistor spaces | 19 pages. v3: published version, further minor corrections | Phys.Rev.D78:046007,2008 | 10.1103/PhysRevD.78.046007 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We find a new family of AdS_4 vacua in IIA string theory. The internal space
is topologically either the complex projective space CP^3 or the "flag
manifold" SU(3)/(U(1)xU(1)), but the metric is in general neither Einstein nor
Kaehler. All known moduli are stabilized by fluxes, without using quantum
effects or orientifold planes. The analysis is completely ten--dimensional and
does not rely on assumptions about Kaluza--Klein reduction.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 05:13:04 GMT"
},
{
"version": "v2",
"created": "Mon, 24 Dec 2007 21:24:55 GMT"
},
{
"version": "v3",
"created": "Sun, 17 Aug 2008 15:28:03 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Tomasiello",
"Alessandro",
""
]
] | [
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712.1397 | Guido Festuccia | Michael Dine, Guido Festuccia, Alexander Morisse and Korneel van den
Broek | Metastable Domains of the Landscape | 20 pages | JHEP0806:014,2008 | 10.1088/1126-6708/2008/06/014 | SCIPP 07/17, RUNHETC-2007-24 | hep-th | null | We argue that the vast majority of flux vacua with small cosmological
constant are unstable to rapid decay to a big crunch. Exceptions are states
with large compactification volume and supersymmetric and approximately
supersymmetric states. Neither weak string coupling, warping, or the existence
of very light particles are, by themselves, enough to render states reasonably
metastable. We speculate, as well, about states which might be cosmological
attractors.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 05:59:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Dine",
"Michael",
""
],
[
"Festuccia",
"Guido",
""
],
[
"Morisse",
"Alexander",
""
],
[
"Broek",
"Korneel van den",
""
]
] | [
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712.1398 | Paul Andi Nagy | Paul-Andi Nagy | Prolongations of Lie algebras and applications | New version. Proofs shortened, one section added on flat connections
with 3-form torsion | Journal of Lie Theory 23 (2013), No. 1, 1-33 | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the skew-symmetric prolongation of a Lie subalgebra $\g \subseteq
\mathfrak{so}(n)$, in other words the intersection $\Lambda^3 \cap (\Lambda^1
\otimes \g)$.We compute this space in full generality. Applications include
uniqueness results for connections with skew-symmetric torsion and also the
proof of the Euclidean version of a conjecture posed in \cite{ofarill}
concerning a class of Pl\"ucker-type embeddings. We also derive a
classification of the metric k-Lie algebras (or Filipov algebras), in positive
signature and finite dimension. Prolongations of Lie algebras can also be used
to finish the classification, started in \cite{datri}, of manifolds admitting
Killing frames, or equivalently flat connections with 3-form torsion. Next we
study specific properties of invariant 4-forms of a given metric representation
and apply these considerations to classify the holonomy representation of
metric connections with vectorial torsion, that is with torsion contained in
$\Lambda^1 \subseteq \Lambda^1 \otimes \Lambda^2$.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:12:26 GMT"
},
{
"version": "v2",
"created": "Thu, 5 Jun 2008 15:10:11 GMT"
}
] | 2012-08-08T00:00:00 | [
[
"Nagy",
"Paul-Andi",
""
]
] | [
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712.1399 | Kohei Motegi | Kohei Motegi, Kazumitsu Sakai | Correlation functions of an interacting spinless fermion model at finite
temperature | 21 pages, v2: typos corrected, published version | J. Stat. Mech. (2008) P02005 | 10.1088/1742-5468/2008/02/P02005 | null | cond-mat.stat-mech math-ph math.MP nlin.SI | null | We formulate correlation functions for a one-dimensional interacting spinless
fermion model at finite temperature. By combination of a lattice path integral
formulation for thermodynamics with the algebraic Bethe ansatz for fermion
systems, the equal-time one-particle Green's function at arbitrary particle
density is expressed as a multiple integral form. Our formula reproduces
previously known results in the following three limits: the zero-temperature,
the infinite-temperature and the free fermion limits.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:24:40 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 07:09:26 GMT"
}
] | 2008-02-21T00:00:00 | [
[
"Motegi",
"Kohei",
""
],
[
"Sakai",
"Kazumitsu",
""
]
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] |
712.14 | An-Ping Li | An-Ping Li | Birthday attack to discrete logarithm | 4 pages | null | null | null | cs.CR | null | The discrete logarithm in a finite group of large order has been widely
applied in public key cryptosystem. In this paper, we will present a
probabilistic algorithm for discrete logarithm.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:15:49 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 01:57:48 GMT"
}
] | 2009-03-21T00:00:00 | [
[
"Li",
"An-Ping",
""
]
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712.1401 | Dmitri Finkelshtein L | D.L. Finkelshtein | Measures on two-component configuration spaces | null | Condensed Matter Physics, 2009, 12(1), p. 5-18 | null | null | math-ph math.MP math.PR | null | We study measures on the configuration spaces of two type particles. Gibbs
measures on the such spaces are described. Main properties of corresponding
relative energies densities and correlation functions are considered. In
particular, we show that a support set for the such Gibbs measure is the set of
pairs of non-intersected configurations.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:40:51 GMT"
}
] | 2015-01-27T00:00:00 | [
[
"Finkelshtein",
"D. L.",
""
]
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] |
712.1402 | Allan Sly | Guy Bresler, Elchanan Mossel, Allan Sly | Reconstruction of Markov Random Fields from Samples: Some Easy
Observations and Algorithms | 14 pages, 0 figures | null | null | null | cs.CC cs.LG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Markov random fields are used to model high dimensional distributions in a
number of applied areas. Much recent interest has been devoted to the
reconstruction of the dependency structure from independent samples from the
Markov random fields. We analyze a simple algorithm for reconstructing the
underlying graph defining a Markov random field on $n$ nodes and maximum degree
$d$ given observations. We show that under mild non-degeneracy conditions it
reconstructs the generating graph with high probability using $\Theta(d
\epsilon^{-2}\delta^{-4} \log n)$ samples where $\epsilon,\delta$ depend on the
local interactions. For most local interaction $\eps,\delta$ are of order
$\exp(-O(d))$.
Our results are optimal as a function of $n$ up to a multiplicative constant
depending on $d$ and the strength of the local interactions. Our results seem
to be the first results for general models that guarantee that {\em the}
generating model is reconstructed. Furthermore, we provide explicit $O(n^{d+2}
\epsilon^{-2}\delta^{-4} \log n)$ running time bound. In cases where the
measure on the graph has correlation decay, the running time is $O(n^2 \log n)$
for all fixed $d$. We also discuss the effect of observing noisy samples and
show that as long as the noise level is low, our algorithm is effective. On the
other hand, we construct an example where large noise implies
non-identifiability even for generic noise and interactions. Finally, we
briefly show that in some simple cases, models with hidden nodes can also be
recovered.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:50:36 GMT"
},
{
"version": "v2",
"created": "Mon, 8 Mar 2010 19:30:26 GMT"
}
] | 2010-03-09T00:00:00 | [
[
"Bresler",
"Guy",
""
],
[
"Mossel",
"Elchanan",
""
],
[
"Sly",
"Allan",
""
]
] | [
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] |
712.1403 | Kenji Ishida | Tetsuya Ohta, Yusuke Nakai, Yoshihiko Ihara, Kenji Ishida, Kazuhiko
Deguchi, Noriaki K. Sato and Isamu Satoh | Ferromagnetic Quantum Critical Fluctuations and Anomalous Coexistence of
Ferromagnetism and Superconductivity in UCoGe Revealed by Co-NMR and NQR
Studies | 5 pages, 7 figures. submitted to J. Phys. Soc. Jpn. To appear in J.
Phys. Soc. Jpn | null | 10.1143/JPSJ.77.023707 | null | cond-mat.supr-con cond-mat.str-el | null | Co nuclear magnetic resonance (NMR) and nuclear quadrupole resonance (NQR)
studies were performed in the recently discovered UCoGe, in which the
ferromagnetic and superconducting (SC) transitions were reported to occur at
$T_{\rm Curie} \sim 3$ K and $T_S \sim 0.8$ K (N. T. Huy {\it et al.}, Phys.
Rev. Lett. {\bf 99} (2007) 067006), in order to investigate the coexistence of
ferromagnetism and superconductivity as well as the normal-state and SC
properties from a microscopic point of view. From the nuclear spin-lattice
relaxation rate $1/T_1$ and Knight-shift measurements, we confirmed that
ferromagnetic fluctuations which possess a quantum critical character are
present above $T_{\rm Curie}$ and the occurrence of ferromagnetic transition at
2.5 K in our polycrystalline sample. The magnetic fluctuations in the normal
state show that UCoGe is an itinerant ferromagnet similar to ZrZn$_2$ and
YCo$_2$. The onset SC transition was identified at $T_S \sim 0.7$ K, below
which $1/T_1$ of 30 % of the volume fraction starts to decrease due to the
opening of the SC gap. This component of $1/T_1$, which follows a $T^3$
dependence in the temperature range of $0.3 - 0.1$ K, coexists with the
magnetic components of $1/T_1$ showing a $\sqrt{T}$ dependence below $T_S$.
From the NQR measurements in the SC state, we suggest that the self-induced
vortex state is realized in UCoGe.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:51:35 GMT"
},
{
"version": "v2",
"created": "Mon, 31 Dec 2007 05:11:27 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Ohta",
"Tetsuya",
""
],
[
"Nakai",
"Yusuke",
""
],
[
"Ihara",
"Yoshihiko",
""
],
[
"Ishida",
"Kenji",
""
],
[
"Deguchi",
"Kazuhiko",
""
],
[
"Sato",
"Noriaki K.",
""
],
[
"Satoh",
"Isamu",
""
]
] | [
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] |
712.1404 | Satyabrata Adhikari | S.Adhikari, N.Ganguly, Indranil Chakrabarty and B.S.Choudhury | Quantum Cloning, Bell's Inequality and Teleportation | 7 pages and no figures, Accepted in Journal of Physics A | J. Phys. A: Math. Theor. 41 415302 (2008) | 10.1088/1751-8113/41/41/415302 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We analyze a possibility of using the two qubit output state from
Buzek-Hillery quantum copying machine (not necessarily universal quantum
cloning machine) as a teleportation channel. We show that there is a range of
values of the machine parameter $\xi$ for which the two qubit output state is
entangled and violates Bell-CHSH inequality and for a different range it
remains entangled but does not violate Bell-CHSH inequality. Further we observe
that for certain values of the machine parameter the two-qubit mixed state can
be used as a teleportation channel. The use of the output state from the
Buzek-Hillery cloning machine as a teleportation channel provides an additional
appeal to the cloning machine and motivation of our present work.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 07:01:36 GMT"
},
{
"version": "v2",
"created": "Mon, 1 Sep 2008 07:24:53 GMT"
}
] | 2008-10-01T00:00:00 | [
[
"Adhikari",
"S.",
""
],
[
"Ganguly",
"N.",
""
],
[
"Chakrabarty",
"Indranil",
""
],
[
"Choudhury",
"B. S.",
""
]
] | [
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712.1405 | Aiichi Iwazaki | Aiichi Iwazaki | Thermalization of Color Gauge Fields in High Energy Heavy Ion Collisions | 6 pages | Phys.Rev.C77:034907,2008 | 10.1103/PhysRevC.77.034907 | Nisho-07/2 | hep-ph | null | We discuss quantum mechanical decay of color magnetic field generated
initially at high energy heavy ion collisions. It is caused by Nielsen-Olesen
unstable modes and is accomplished possibly in a period $<1$fm/c. We show that
the decay products, i.e. incoherent gluons may be thermalized in a sufficiently
short period ($< 1$fm/c). The precise determination of the period is made by
calculating two point function of the color magnetic field in a model of color
glass condensate.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 07:07:53 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 01:44:26 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Iwazaki",
"Aiichi",
""
]
] | [
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712.1406 | Yunori Nisikawa | Yunori Nisikawa, Muneharu Ibuki and Manabu Usuda | Momentum-dependent resonant inelastic X-ray scattering at the Si K edge
of 3C-SiC: A theoretical study on a relation between spectra and valence band
dispersion | 8 pages, 8 figures. submitted to Physical Review B. Please also see
following related paper: arXiv:cond-mat/0311008 and arXiv:cond-mat/0405009 | null | null | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We theoretically demonstrate that a resonant inelastic x-ray scattering
(RIXS) with a sizable momentum transfer can be utilized to study valence band
dispersion for broad band materials. We take RIXS at the Si K edge of 3C-SiC as
a typical example. The RIXS spectra are calculated by systematically changing
the transferred momentum, an incident photon polarization and an incident
photon energy, on the basis of an ab initio calculation. We find that the
spectra depend heavily on both the transferred momentum and the incident photon
polarization, and the peaks in the spectra correspond to the energies of the
valence bands. We conclude that the information on the energy dispersion of
valence bands can be extracted from the transferred momentum dependence of the
RIXS spectra. These findings lead to further application for RIXS when
investigating the band structure of broad band materials.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 08:32:25 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Sep 2009 13:28:13 GMT"
}
] | 2009-09-21T00:00:00 | [
[
"Nisikawa",
"Yunori",
""
],
[
"Ibuki",
"Muneharu",
""
],
[
"Usuda",
"Manabu",
""
]
] | [
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] |
712.1407 | Savel'ev Sergey | V.A. Yampol'skii, S.E. Savel'ev, and Franco Nori | Voltage-driven quantum oscillations in graphene | 4 pages, 4 figures | null | null | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | We predict unusual (for non-relativistic quantum mechanics) electron states
in graphene, which are localized within a finite-width potential barrier. The
density of localized states in the sufficiently high and/or wide graphene
barrier exhibits a number of singularities at certain values of the energy.
Such singularities provide quantum oscillations of both the transport (e.g.,
conductivity) and thermodynamic properties of graphene - when increasing the
barrier height and/or width, similarly to the well-known Shubnikov-de-Haas
(SdH) oscillations of conductivity in pure metals. However, here the SdH-like
oscillations are driven by an electric field instead of the usual
magnetically-driven SdH-oscillations.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 07:47:06 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Yampol'skii",
"V. A.",
""
],
[
"Savel'ev",
"S. E.",
""
],
[
"Nori",
"Franco",
""
]
] | [
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] |
712.1408 | Mikhail Kalenkov | Mikhail S. Kalenkov, Andrei D. Zaikin | Non-local electron transport and cross-resistance peak in NSN
heterostructures | 4 pages, 3 figures | JETP Lett. vol. 87, 140 (2008) [Pis'ma v ZhETF, vol. 87, 166
(2008)] | 10.1134/S0021364008030053 | null | cond-mat.supr-con | null | We develop a microscopic theory describing the peak in the temperature
dependence of the non-local resistance of three-terminal NSN devices. This peak
emerges at sufficiently high temperatures as a result of a competition between
quasiparticle/charge imbalance and subgap (Andreev) contributions to the
conductance matrix. Both the height and the shape of this peak demonstrate the
power law dependence on the superconductor thickness $L$ in contrast to the
zero-temperature non-local resistance which decays (roughly) exponentially with
increasing $L$. A similar behavior was observed in recent experiments.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 07:49:58 GMT"
}
] | 2011-02-08T00:00:00 | [
[
"Kalenkov",
"Mikhail S.",
""
],
[
"Zaikin",
"Andrei D.",
""
]
] | [
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] |
712.1409 | Enno Middelberg | Enno Middelberg, Ray P. Norris, Tim J. Cornwell, Maxim A. Voronkov,
Brian D. Siana, Brian J. Boyle, Paolo Ciliegi, Carole A. Jackson, Minh T.
Huynh, Stefano Berta, Stefano Rubele, Carol J. Lonsdale, Rob J. Ivison, Ian
Smail, Seb J. Oliver | Deep ATLAS Radio Observations of the ELAIS-S1/Spitzer Wide-Area Infrared
Extragalctic field | Accepted for publication in the Astronomical Journal, needs
aastex.cls | null | null | null | astro-ph | null | We have conducted sensitive (1 sigma<30 uJy) 1.4 GHz radio observations with
the Australia Telescope Compact Array of a field largely coincident with
infrared observations of the Spitzer Wide-Area Extragalactic Survey. The field
is centred on the European Large Area ISO Survey S1 region and has a total area
of 3.9 deg. We describe the observations and calibration, source extraction,
and cross-matching to infrared sources. Two catalogues are presented; one of
the radio components found in the image and one of radio sources with
counterparts in the infrared and extracted from the literature. 1366 radio
components were grouped into 1276 sources, 1183 of which were matched to
infrared sources. We discover 31 radio sources with no infrared counterpart at
all, adding to the class of Infrared-Faint Radio Sources.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 08:32:12 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Middelberg",
"Enno",
""
],
[
"Norris",
"Ray P.",
""
],
[
"Cornwell",
"Tim J.",
""
],
[
"Voronkov",
"Maxim A.",
""
],
[
"Siana",
"Brian D.",
""
],
[
"Boyle",
"Brian J.",
""
],
[
"Ciliegi",
"Paolo",
""
],
[
"Jackson",
"Carole A.",
""
],
[
"Huynh",
"Minh T.",
""
],
[
"Berta",
"Stefano",
""
],
[
"Rubele",
"Stefano",
""
],
[
"Lonsdale",
"Carol J.",
""
],
[
"Ivison",
"Rob J.",
""
],
[
"Smail",
"Ian",
""
],
[
"Oliver",
"Seb J.",
""
]
] | [
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] |
712.141 | Andrea Quadri | Daniele Bettinelli, Ruggero Ferrari, Andrea Quadri (Milan U. and INFN,
Milan) | Gauge Dependence in the Nonlinearly Realized Massive SU(2) Gauge Theory | 5 pages. Prepared for AGMF2007 - Algebra, Geometry, and Mathematical
Physics Baltic-Nordic Workshop, Goeteborg, 11-13 October, 2007 | J.General.Lie Theor.Appl.2:122-126,2008 | null | IFUM-908-FT | hep-th | null | The implementation of the 't Hooft alpha-gauge in the symmetrically
subtracted massive gauge theory based on the nonlinearly realized SU(2) gauge
group is discussed. The gauge independence of the self-mass of the gauge bosons
is proven by cohomological techniques.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 08:53:50 GMT"
}
] | 2009-02-24T00:00:00 | [
[
"Bettinelli",
"Daniele",
"",
"Milan U. and INFN,\n Milan"
],
[
"Ferrari",
"Ruggero",
"",
"Milan U. and INFN,\n Milan"
],
[
"Quadri",
"Andrea",
"",
"Milan U. and INFN,\n Milan"
]
] | [
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] |
712.1411 | Fang Liu | BES Collaboration | Measurements of J/\psi decays into \omega K \bar{K} \pi and \phi K
\bar{K} \pi | 18 pages, 10 figures | Phys.Rev.D77:032005,2008 | 10.1103/PhysRevD.77.032005 | null | hep-ex | null | The decays of $J/\psi \to \omega K\bar{K}\pi$ and $J/\psi \to \phi
K\bar{K}\pi$ are studied using $5.8 \times 10^{7}$ $J/\psi$ events collected
with the Beijing Spectrometer (BESII) at the Beijing Electron-Positron Collider
(BEPC). The $K^{0}_{S}K^{\pm}\pi^{\mp}$ and $K^{+}K^{-}\pi^{0}$ systems,
produced in $J/\psi \to \omega K\bar{K}\pi$, have enhancements in the invariant
mass distributions at around 1.44 GeV/$c^{2}$. However, there is no evidence
for mass enhancements in the $K\bar{K}\pi$ system in $J/\psi \to \phi
K\bar{K}\pi$. The branching fractions of $J/\psi \to \omega
K^{0}_{S}K^{\pm}\pi^{\mp}$, $\phi K^{0}_{S}K^{\pm}\pi^{\mp}$, $\omega
K^{*}\bar{K}+c.c.$, and $\phi K^{*}\bar{K}+c.c.$ are obtained, and the $J/\psi
\to \eta K^{0}_{S}K^{\pm}\pi^{\mp}$ branching fraction is measured for the
first time.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 09:03:15 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 03:30:19 GMT"
}
] | 2012-08-27T00:00:00 | [
[
"BES Collaboration",
"",
""
]
] | [
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] |
712.1412 | Raffaella Margutti | R. Margutti, A. Moretti, F. Pasotti, S. Campana, G. Chincarini, S.
Covino, C. Guidorzi, P. Romano, G. Tagliaferri | Anomalous X-Ray emission in GRB060904B: a Nickel line? | Accepted by A&A | null | 10.1051/0004-6361:20078799 | null | astro-ph | null | The detection of an extra component in GRB060904B X-ray spectra in addition
to the standard single power-law behaviour has recently been reported in the
literature. This component can be fit with different models; in particular the
addition of a spectral line provides the best representation.In this paper we
investigate the physical properties that the surrounding medium must have in
order to produce a spectral feature that can explain the detected emission. We
analyse and discuss how and if the detected spectral excess fits in different
theoretical models developed to explain the nature of line emission during the
afterglow phase of Gamma-Ray Bursts (GRBs). Trasmission and reflection models
have been considered. Given the high value (>>1) of the Thomson optical depth,
the emission is likely to arise in a reflection scenario. Within reflection
models, the external reflection geometry fails to predict the observed
luminosity. On the contrary, the detected feature can be explained in a funnel
scenario with typical opening angle theta of 5 degrees, Nickel mass of the
order of 0.1 M_o and T=10^6 K. For theta=20 degrees, assuming the reprocessing
material to be the SN shell, the detected emission implies a Nickel mass of 0.4
M_o at T=10^7 K and a metallicity 10 times the solar value. If the giant X-ray
flare that dominates the early XRT light curve is identified with the ionizing
source, the SN expansion began 3000 s before the GRB event.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:31:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Margutti",
"R.",
""
],
[
"Moretti",
"A.",
""
],
[
"Pasotti",
"F.",
""
],
[
"Campana",
"S.",
""
],
[
"Chincarini",
"G.",
""
],
[
"Covino",
"S.",
""
],
[
"Guidorzi",
"C.",
""
],
[
"Romano",
"P.",
""
],
[
"Tagliaferri",
"G.",
""
]
] | [
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] |
712.1413 | Rakesh Tibrewala | Rakesh Tibrewala, Sashideep Gutti, T.P. Singh, Cenalo Vaz | Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime I.
Classical Solutions | 19 pages, sections on surface gravity removed, section on self
similar solution expanded, appendix removed, references added. To appear in
Phys. Rev.D | Phys.Rev.D77:064012,2008 | 10.1103/PhysRevD.77.064012 | null | gr-qc astro-ph hep-th | null | We study the collapse of a spherically symmetric dust distribution in
$d$-dimensional AdS spacetime. We investigate the role of dimensionality, and
the presence of a negative cosmological constant, in determining the formation
of trapped surfaces and the end state of gravitational collapse. We obtain the
self-similar solution for the case of zero cosmological constant, and show that
one cannot construct a self-similar solution when a cosmological constant is
included.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 09:25:15 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Feb 2008 09:53:47 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Tibrewala",
"Rakesh",
""
],
[
"Gutti",
"Sashideep",
""
],
[
"Singh",
"T. P.",
""
],
[
"Vaz",
"Cenalo",
""
]
] | [
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] |
712.1414 | Irina Rezvyakova S. | Irina Rezvyakova | One metric result about analytic continuation of some Dirichlet series | 4 pages | null | null | null | math.CV math.NT | null | In this paper we consider certain 1-parametric family of Dirichlet series.
For a particular value of the parameter the series turns into the Dirichlet
series for the Riemann zeta function. We prove that almost every series of the
family has analytic continuation to the half plane Re s > 1/2 where it doesn't
vanish. The result was obtained before by different authors. We give its simple
proof in terms of estimates of some trigonometric sums.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 14:08:47 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Rezvyakova",
"Irina",
""
]
] | [
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] |
712.1415 | Agur Sevink | G.J.A. Sevink and A.V. Zvelindovsky | Block copolymers confined in a nanopore: Pathfinding in a curving and
frustrating flatland | The following article has been accepted by JCP. After it is
published, it will be found at http://jcp.aip.org/ | null | 10.1063/1.2829406 | null | cond-mat.soft | null | We have studied structure formation in a confined block copolymer melt by
means of dynamic density functional theory (DDFT). The confinement is
two-dimensional, and the confined geometry is that of a cylindrical nanopore.
Although the results of this study are general, our coarse-grained molecular
model is inspired by an experimental lamellae-forming PS-PBD diblock copolymer
system (Shin et al, Science, 306, 76 (2004)), in which an exotic toroidal
structure was observed upon confinement in alumina nanopores. Our computational
study shows that a zoo of exotic structures can be formed, although the
majority, including the catenoid, helix and double helix that were also found
in Monte Carlo (MC) nanopore studies, are metastable states. We introduce a
general classification scheme and consider the role of kinetics and
elongational pressure on stability and formation pathway of both equilibrium
and metastable structures in detail. We find that helicity and three-fold
connections mediate structural transitions on a larger scale. Moreover, by
matching the remaining parameter in our mesoscopic method, the Flory-Huggins
parameter, to the experimental system, we obtain a structure that resembles the
experimental toroidal structure in great detail. Here, the most important
factor seems to be the roughness of the pore, i.e. small variations of the pore
radius on a scale that is larger than the characteristic size in the system.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 09:57:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sevink",
"G. J. A.",
""
],
[
"Zvelindovsky",
"A. V.",
""
]
] | [
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712.1416 | Anastasia Doikou | Jean Avan, Anastasia Doikou | Systematic derivation of boundary Lax pairs | 13 pages, Latex. Proceedings contribution RAQIS'07, September 2007,
Annecy, France. References added, minor typos corrected | null | null | null | hep-th math-ph math.MP nlin.SI | null | We systematically derive the Lax pair formulation for both discrete and
continuum integrable classical theories with consistent boundary conditions.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 09:58:04 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Dec 2007 16:39:36 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Avan",
"Jean",
""
],
[
"Doikou",
"Anastasia",
""
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712.1417 | Martin Schumacher | Martin Schumacher | Properties of the $\pi^0$, $\eta$, $\eta'$, $\sigma$, $f_0(980)$ and
$a_0(980)$ mesons and their relevance for the polarizabilities of the nucleon | null | Eur.Phys.J.A34:293-301,2007 | 10.1140/epja/i2007-10506-3 | null | hep-ph | null | The signs and values of the two-photon couplings $F_{M\gamma\gamma}$ of
mesons $(M)$ and their couplings $g_{MNN}$ to the nucleon as entering into the
$t$-channel parts of the difference of the electromagnetic polarizabilities
$(\alpha-\beta)$ and the backward angle spin polarizabilities $\gamma_\pi$ are
determined. The excellent agreement achieved with the experimental
polarizabilities of the proton makes it possible to make reliable predictions
for the neutron. The results obtained are $\alpha_n=13.4\pm 1.0$,
$\beta_n=1.8\mp 1.0$ ($10^{-4}$ fm$^3$), and $\gamma^{(n)}_\pi=57.6\pm 1.8$
($10^{-4}$ fm$^4$). New empirical information on the flavor wave functions of
the $f_0(980)$ and the $a_0(980)$ meson is obtained.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:00:42 GMT"
}
] | 2013-06-26T00:00:00 | [
[
"Schumacher",
"Martin",
""
]
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712.1418 | Giovanni Vladilo | Juan Vladilo | Pathways through interstellar matter: - From the closest stars to the
most distant quasars | Invited talk presented at the Conference "Pathways through an
Eclectic Universe" (23rd-27th April 2007, Tenerife, Spain). To appear in ASP
Conf. Ser., eds. J. Knapen, T. Maloney, & A. Vazdekis | null | null | null | astro-ph | null | Observations of quasar absorption systems relevant for studies of star
formation at redshift 2 </= z </= 4 are briefly reviewed. Emphasis is given on
the role played by dust in our understanding of the star formation history of
galaxies detected as absorption systems. Local interstellar studies are used as
a reference for understanding the properties of high redshift interstellar
media. An example is shown of the potential effects of dust extinction on the
metallicity-N(HI) distribution obtained from magnitude-limited surveys of
damped lyman alpha absorbers.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:05:32 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Vladilo",
"Juan",
""
]
] | [
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712.1419 | Zhang He | Zhi-zhong Xing, He Zhang, Shun Zhou | Updated Values of Running Quark and Lepton Masses | 23 pages, 6 tables, 2 figures; version published in PRD | Phys.Rev.D77:113016,2008 | 10.1103/PhysRevD.77.113016 | null | hep-ph astro-ph hep-ex hep-th nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Reliable values of quark and lepton masses are important for model building
at a fundamental energy scale, such as the Fermi scale M_Z \approx 91.2 GeV and
the would-be GUT scale \Lambda_GUT \sim 2 \times 10^16 GeV. Using the latest
data given by the Particle Data Group, we update the running quark and
charged-lepton masses at a number of interesting energy scales below and above
M_Z. In particular, we take into account the possible new physics scale (\mu
\sim 1 TeV) to be explored by the LHC and the typical seesaw scales (\mu \sim
10^9 GeV and \mu \sim 10^12 GeV) which might be relevant to the generation of
neutrino masses. For illustration, the running masses of three light Majorana
neutrinos are also calculated. Our up-to-date table of running fermion masses
are expected to be very useful for the study of flavor dynamics at various
energy scales.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:15:57 GMT"
},
{
"version": "v2",
"created": "Tue, 20 May 2008 12:07:31 GMT"
},
{
"version": "v3",
"created": "Fri, 27 Jun 2008 09:09:43 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Xing",
"Zhi-zhong",
""
],
[
"Zhang",
"He",
""
],
[
"Zhou",
"Shun",
""
]
] | [
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712.142 | Narae Hwang | Narae Hwang, Myung Gyoon Lee (Seoul National University, Korea) | A Catalog of Bright Star Clusters in the Interacting Galaxy M51 | 40 pages, 17 figures, accepted for publication in AJ | The Astronomical Journal 135 (2008) 1567-1579 | 10.1088/0004-6256/135/4/1567 | null | astro-ph | null | We present a catalog of star clusters with V_{F555W}<23 mag detected in the
interacting spiral galaxy M51 system based on the mosaic images taken with HST
ACS by the Hubble Heritage Team. We have selected about 3,600 clusters based on
their morphological information through the visual inspection. The final star
cluster catalog includes 2,224 clusters that are relatively well isolated and
have a circular shape. The star clusters in M51 are mostly distributed around
the spiral arms of NGC 5194. The color-magnitude diagrams show that most of the
star clusters in M51 are bluer than (B_{F435W}-V_{F555W}) = 0.5 and
(V_{F555W}-I_{F814W}) = 0.8. There are also some red star clusters with
(B_{F435W}-V_{F555W}) > 0.7, uniformly distributed over the M51 field. Some of
these red clusters are suspected to be a part of the halo or old disk
population based on their old ages (t >= 10^9 yrs) and their spatial
distribution. The luminosity function of the star clusters is fit well by a
single power law with \alpha = -2.59 \pm 0.03 for the range -10.0 <M_V < -8.0
mag. We find that the size distribution of the star clusters can be fit with
three Gaussian components with peaks at effective radii of 2.27, 4.80 and 7.51
pc. Some large star clusters with red color are faint fuzzy clusters, and they
are distributed not only around NGC 5195 but also around NGC 5194. These faint
fuzzies are found to display an elongated spatial distribution, while the
normal compact red clusters show a relatively uniform distribution around NGC
5194.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:21:52 GMT"
}
] | 2008-03-18T00:00:00 | [
[
"Hwang",
"Narae",
"",
"Seoul National University, Korea"
],
[
"Lee",
"Myung Gyoon",
"",
"Seoul National University, Korea"
]
] | [
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] |
712.1421 | Eduardo J.S. Villase\~nor | Daniel G\'omez Vergel, Eduardo J. S. Villase\~nor | Unitary evolution of free massless fields in de Sitter space-time | 20 pages. Comments and references added | Class.Quant.Grav.25:145008,2008 | 10.1088/0264-9381/25/14/145008 | null | gr-qc | null | We consider the quantum dynamics of a massless scalar field in de Sitter
space-time. The classical evolution is represented by a canonical
transformation on the phase space for the field theory. By studying the
corresponding Bogoliubov transformations, we show that the symplectic map that
encodes the evolution between two instants of time cannot be unitarily
implemented on any Fock space built from a SO(4)-symmetric complex structure.
We will show also that, in contrast with some effectively lower dimensional
examples arising from Quantum General Relativity such as Gowdy models, it is
impossible to find a time dependent conformal redefinition of the massless
scalar field leading to a quantum unitary dynamics.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:22:00 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Feb 2008 20:52:10 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Vergel",
"Daniel Gómez",
""
],
[
"Villaseñor",
"Eduardo J. S.",
""
]
] | [
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] |
712.1422 | Bartlomiej Szafran | S.Bednarek, B.Szafran, R.Dudek, K.Lis | Induced quantum dots and wires: electron storage and delivery | null | Phys. Rev. Lett 100, 126805 (2008) | 10.1103/PhysRevLett.100.126805 | null | cond-mat.mes-hall | null | We show that quantum dots and quantum wires are formed underneath metal
electrodes deposited on a planar semiconductor heterostructure containing a
quantum well. The confinement is due to the self-focusing mechanism of an
electron wave packet interacting with the charge induced on the metal surface.
Induced quantum wires guide the transfer of electrons along metal paths and
induced quantum dots store the electrons in specific locations of the
nanostructure. Induced dots and wires can be useful for devices operating on
the electron spin.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:24:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bednarek",
"S.",
""
],
[
"Szafran",
"B.",
""
],
[
"Dudek",
"R.",
""
],
[
"Lis",
"K.",
""
]
] | [
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] |
712.1423 | Denise Hagnier | Hadj-Ali Gueniche (DCPR), Pierre-Alexandre Glaude (DCPR), Ren\'e
Fournet (DCPR), Fr\'ed\'erique Battin-Leclerc (DCPR) | Rich methane laminar flames doped with light unsaturated hydrocarbons.
Part III : cyclopentene | null | Combustion and Flame 152 (2008) 245261 | 10.1016/j.combustflame.2007.07.012 | null | physics.chem-ph | null | In line with the studies presented in the parts I and II of this paper, the
structure of a laminar rich premixed methane flame doped with cyclopentene has
been investigated. The gases of this flame contains 15.3% (molar) of methane,
26.7% of oxygen and 2.4% cyclopentene corresponding to an equivalence ratio of
1.79 and a ratio C5H8 / CH4 of 16 %. The flame has been stabilized on a burner
at a pressure of 6.7 kPa using argon as dilutant, with a gas velocity at the
burner of 36 cm/s at 333 K. The temperature ranged from 627 K close to the
burner up to 2027 K. Quantified species included usual methane C0-C2 combustion
products, but also propyne, allene, propene, propane, 1-butene, 1,3-butadiene,
1,2-butadiene, vinylacetylene, diacetylene, cyclopentadiene, 1,3-pentadiene,
benzene and toluene. A new mechanism for the oxidation of cyclopentene has been
proposed. The main reaction pathways of consumption of cyclopentene and of
formation of benzene and toluene have been derived from flow rate analyses.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:24:54 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Gueniche",
"Hadj-Ali",
"",
"DCPR"
],
[
"Glaude",
"Pierre-Alexandre",
"",
"DCPR"
],
[
"Fournet",
"René",
"",
"DCPR"
],
[
"Battin-Leclerc",
"Frédérique",
"",
"DCPR"
]
] | [
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] |
712.1424 | Giovanni Di Santo | Giovanni Di Santo, Susana Tobenas, Jozef Adamcik and Giovanni Dietler | Force spectroscopy on DNA by FM-AFM | 3 pages, 2 figures, short communication under submission | null | null | null | physics.bio-ph physics.gen-ph | null | We present imaging and force spectroscopy measurements of DNA molecules
adsorbed on functionalized mica. By means of Non-Contact mode AFM (NC-AFM) in
Ultra High Vacuum (UHV), the frequency shift (\Delta f) versus separation (z)
curves were measured providing a quantitative measurement of both force and
energy of the tip-DNA interaction. Similarly, topographic images of the
adsorbed DNA molecules in constant frequency shift mode were collected. The
high resolution force measurements confirm the imaging contrast difference
between the substrate and DNA. The force curves measured along the DNA molecule
can be divided into two classes showing marked differences in the minimum of
the interaction force and energy, indicating that NC-AFM could deliver chemical
contrast along the DNA molecule.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:37:41 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Di Santo",
"Giovanni",
""
],
[
"Tobenas",
"Susana",
""
],
[
"Adamcik",
"Jozef",
""
],
[
"Dietler",
"Giovanni",
""
]
] | [
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] |
712.1425 | Gareth M. James | Gareth M. James | Curve alignment by moments | Published in at http://dx.doi.org/10.1214/07-AOAS127 the Annals of
Applied Statistics (http://www.imstat.org/aoas/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Statistics 2007, Vol. 1, No. 2, 480-501 | 10.1214/07-AOAS127 | IMS-AOAS-AOAS127 | stat.AP | null | A significant problem with most functional data analyses is that of
misaligned curves. Without adjustment, even an analysis as simple as estimation
of the mean will fail. One common method to synchronize a set of curves
involves equating ``landmarks'' such as peaks or troughs. The landmarks method
can work well but will fail if marker events can not be identified or are
missing from some curves. An alternative approach, the ``continuous monotone
registration'' method, works by transforming the curves so that they are as
close as possible to a target function. This method can also perform well but
is highly dependent on identifying an accurate target function. We develop an
alignment method based on equating the ``moments'' of a given set of curves.
These moments are intended to capture the locations of important features which
may represent local behavior, such as maximums and minimums, or more global
characteristics, such as the slope of the curve averaged over time. Our method
works by equating the moments of the curves while also shrinking toward a
common shape. This allows us to capture the advantages of both the landmark and
continuous monotone registration approaches. The method is illustrated on
several data sets and a simulation study is performed.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:37:58 GMT"
}
] | 2007-12-18T00:00:00 | [
[
"James",
"Gareth M.",
""
]
] | [
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712.1426 | Ralf Meyer | Ralf Meyer and Ryszard Nest | C*-Algebras over Topological Spaces: The Bootstrap Class | Final version, very minor changes | Munster J. Math. 2 (2009), pp. 215-252 | null | null | math.KT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We carefully define and study C*-algebras over topological spaces, possibly
non-Hausdorff, and review some relevant results from point-set topology along
the way. We explain the triangulated category structure on the bivariant
Kasparov theory over a topological space. We introduce and describe an analogue
of the bootstrap class for C*-algebras over a finite topological space.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:39:45 GMT"
},
{
"version": "v2",
"created": "Fri, 30 May 2008 11:03:58 GMT"
},
{
"version": "v3",
"created": "Thu, 11 Dec 2008 18:39:25 GMT"
}
] | 2015-10-23T00:00:00 | [
[
"Meyer",
"Ralf",
""
],
[
"Nest",
"Ryszard",
""
]
] | [
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712.1427 | Piotr Su{\l}kowski | Robbert Dijkgraaf and Piotr Su{\l}kowski | Instantons on ALE spaces and orbifold partitions | 28 pages, 10 figures; reference added | JHEP 0803:013,2008 | 10.1088/1126-6708/2008/03/013 | ITFA-2007-26, IFT-UW-2007-5, BONN-TH-2007-12 | hep-th math.AG math.CO | null | We consider N=4 theories on ALE spaces of $A_{k-1}$ type. As is well known,
their partition functions coincide with $A_{k-1}$ affine characters. We show
that these partition functions are equal to the generating functions of some
peculiar classes of partitions which we introduce under the name 'orbifold
partitions'. These orbifold partitions turn out to be related to the
generalized Frobenius partitions introduced by G. E. Andrews some years ago. We
relate the orbifold partitions to the blended partitions and interpret
explicitly in terms of a free fermion system.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:39:52 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Mar 2008 04:30:31 GMT"
}
] | 2010-02-03T00:00:00 | [
[
"Dijkgraaf",
"Robbert",
""
],
[
"Sułkowski",
"Piotr",
""
]
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] |
712.1428 | Jose M. M. Senovilla | Jos\'e M. M. Senovilla | A New Type of Singularity Theorem | 6 pages, no figures. Contribution to appear in the Proceedings of the
Spanish Relativity Meeting ERE-07, "Relativistic Astrophysics and Cosmology" | null | 10.1051/eas:0830009 | null | gr-qc | null | A new type of singularity theorem, based on spatial averages of physical
quantities, is presented and discussed. Alternatively, the results inform us of
when a spacetime can be singularity-free. This theorem provides a decisive
observational difference between singular and non-singular, globally
hyperbolic, open cosmological models.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 16:39:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Senovilla",
"José M. M.",
""
]
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712.1429 | Ralf Schutzhold | Ralf Sch\"utzhold | Quantum back-reaction problems | 5 pages RevTeX, Proceedings to the workshop From Quantum to Emergent
Gravity: Theory and Phenomenology, June 11-15 2007, Trieste, Italy, published
in Proceedings of Science | PoSQG-Ph:036,2007 | null | null | gr-qc | null | The macroscopic behavior of many physical systems can be approximately
described by classical quantities. However, quantum theory demands the
existence of omnipresent quantum fluctuations on top of this classical
background -- which, albeit small, should have some impact onto its dynamics.
The correct treatment of this quantum back-reaction is one of the main problems
in quantum gravity and related to fundamental questions such as the initial
(big bang) singularity or the cosmological constant. By means of the
qualitative analogy between gravity and fluid dynamics, we try to shed some
light onto these problems and show some of the difficulties associated with the
calculation of the quantum back-reaction starting from the classical
(macroscopic) equation of motion.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:46:46 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Schützhold",
"Ralf",
""
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] |
712.143 | Grigoris Panotopoulos | Grigoris Panotopoulos | Non-thermal leptogenesis and gravitino problem in inflaton decay | 11 pages, 1 figure | JHEP 0712:016,2007 | 10.1088/1126-6708/2007/12/016 | null | hep-ph | null | In the present work we discuss baryon asymmetry in the non-thermal
leptogenesis scenario and gravitino cosmology for an unstable gravitino with
inflaton decay. We take into account two production mechanisms for gravitino,
namely thermal production and inflaton decay. We wish to show in plots the
allowed parameter space so that the BBN constraint and the requirement for the
right baryon asymmetry are satisfied at the same time. However our analysis
shows that it is impossible to achieve both goals simultaneously.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:52:40 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Panotopoulos",
"Grigoris",
""
]
] | [
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] |
712.1431 | Claudio Giberti | Pierluigi Contucci, Cristian Giardin\`a, Claudio Giberti, Giorgio
Parisi, Cecilia Vernia | Answer to Comment on "Ultrametricity in the Edwards-Anderson Model"
arXiv:0709.0894 | 2 pages, 1 figure; abstract replaced, typos corrected | null | 10.1103/PhysRevLett.100.159701 | null | cond-mat.dis-nn cond-mat.stat-mech | null | This reply shows that the argument presented in the comment by Jorg and
Krzakala (cond mat 0709.0894) cannot be used to weaken the results presented in
our paper on ultrametricity evidence in the 3d Edwards Anderson model (PRL 99,
057206, 2007; cond-mat/0607376). Our work in fact was mainly based on
identifying the scaling law that governs the large volume approach to
ultrametricity while NO asymptotic analysis has been done in (cond mat
0709.0894). We show here that the same method we used in our paper, when
properly applied to the 2d case, reveals the expected lack of RSB picture at
positive temperature, despite the fact that for a fixed finite volume some
ultrametric features might still be seen in the joint overlap probability
distribution. Those features disappear for increasing volume or when the system
is away from the critical curve in the (T,d) plane.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 10:52:44 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 18:19:57 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"Contucci",
"Pierluigi",
""
],
[
"Giardinà",
"Cristian",
""
],
[
"Giberti",
"Claudio",
""
],
[
"Parisi",
"Giorgio",
""
],
[
"Vernia",
"Cecilia",
""
]
] | [
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712.1432 | Rajendra Prasad | Nitya Nath Shukla, A. Sen, and R. Prasad | Quantum well states in Fe/Nb(001) multilayers: First principles study | 9 pages, 8 figures | Phys. Rev. B 76, 174417 (2007) | 10.1103/PhysRevB.76.174417 | null | cond-mat.mes-hall | null | We present a first-principles study to understand the phenomena of interlayer
exchange coupling in Fe/Nb multilayers using the linearized-muffin-tin-orbitals
method within the generalized gradient approximation. We find that the exchange
coupling oscillates with both short and long periodicities, which have been
examined in terms of the Ruderman-Kittel-Kasuya-Yosida (RKKY) model as well as
the quantum well (QW) model. We have investigated the behavior of the exchange
coupling by artificially varying moments of Fe atoms in ferromagnetic layers.
For a small moment of Fe, the coupling shows bilinearity in the magnetic
moments, implying its RKKY character. However, at higher moments close to that
of bulk Fe, the saturation of long-period oscillations is in accordance with
the QW model. Quantum well dispersions around the Fermi level demonstrate that
the majority-spin bands contribute largely to the formation of quantum well
states, which we analyze quantitatively by making use of the phase accumulation
model. Our analysis indicates that the quantum well model gives a better
description of the oscillatory behavior of the exchange coupling in Fe/Nb
multilayers.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:00:15 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Shukla",
"Nitya Nath",
""
],
[
"Sen",
"A.",
""
],
[
"Prasad",
"R.",
""
]
] | [
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] |
712.1433 | Denise Hagnier | Mohammed Yahyaoui (DCPR), Hichem Hakka (DCPR), Pierre-Alexandre Glaude
(DCPR), Fr\'ed\'erique Battin-Leclerc (DCPR) | Experimental and modeling study of the autoignition of cyclopentane | null | International Journal of Chemical Kinetics 40 (2008) 25-33 | 10.1002/kin.20290 | null | physics.chem-ph | null | Ignition delay times of cyclopentene-oxygen-argon mixtures were measured
behind reflected shock waves. Mixtures contained 0.5 or 1 % of hydrocarbons for
equivalence ratios ranging from 0.5 to 1.5. Reflected shock waves conditions
were: temperatures from 1300 to 1700 K and pressures from 7 to 9 atm. When
comparing to previous results obtained under similar conditions, it can be
observed that the reactivity of cyclopentene is much lower than that of
cyclohexene, but very close to that of cyclopentane. A kinetic mechanism
recently proposed for the combustion of cyclopentene in a flame has been used
to model these results and a satisfactory agreement has been obtained. The main
reaction pathways have been derived from flow rate, simulated temporal profiles
of products and sensitivity analyses.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:00:25 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Yahyaoui",
"Mohammed",
"",
"DCPR"
],
[
"Hakka",
"Hichem",
"",
"DCPR"
],
[
"Glaude",
"Pierre-Alexandre",
"",
"DCPR"
],
[
"Battin-Leclerc",
"Frédérique",
"",
"DCPR"
]
] | [
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] |
712.1434 | Branislav Cvetkovi\'c | B. Cvetkovi\'c and M. Blagojevi\'c | Stability of 3D black hole with torsion | LATEX, 9 pages | Mod.Phys.Lett.A22:3047-3055,2007 | 10.1142/S0217732307026126 | null | gr-qc | null | Using $N=1+1$ supersymmetric extension of the three-dimensional gravity with
torsion, we show that a generic black hole has no exact supersymmetries, the
extremal black hole has only one, while the zero-energy black hole has two.
Combining these results with the asymptotic supersymmetry algebra, we are
naturally led to interpret the zero-energy black hole as the ground state of
the Ramond sector, and analogously, the anti-de Sitter solution as the ground
state of the Neveau-Schwartz sector.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:09:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cvetković",
"B.",
""
],
[
"Blagojević",
"M.",
""
]
] | [
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] |
712.1435 | M\'at\'e Csan\'ad | M. Csanad (for the PHENIX Collaboration) | Milestones of the PHENIX experiment at RHIC | 10 pages, 5 figures. For the proceedings of M. Csanad's talk at the
XII International Conference on Hadron Spectroscopy - Hadron07 | Frascati Phys.Ser.46:123-132,2007 | null | null | nucl-ex | null | The latest PHENIX results for particle production are presented in this
paper. A suppression of the yield of high p_t (transverse momentum) hadrons in
central Au+Au collisions is found. In contrast, direct photons are not
suppressed in central Au+Au collisions and no suppression of high p_t particles
can be seen in d+Au collisions. This leads to the conclusion that the dense
medium formed in central Au+Au collisions is responsible for the suppression.
It is as well found, that the properties of this medium are similar to the one
of a liquid. Further measurements provide information about the chiral dynamics
of the system.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:11:46 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Csanad",
"M.",
"",
"for the PHENIX Collaboration"
]
] | [
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712.1436 | Igor M. Sokolov | F. Sagues, V.P. Shkilev and I.M. Sokolov | Reaction-Subdiffusion Equations for the A <--> B Reaction | null | null | 10.1103/PhysRevE.77.032102 | null | cond-mat.stat-mech cond-mat.dis-nn | null | We consider a simple linear reversible isomerization reaction A <--> B under
subdiffusion described by continuous time random walks (CTRW). The reactants'
transformations take place independently on the motion and are described by
constant rates. We show that the form of the ensuing system of mesoscopic
reaction-subdiffusion is somewhat unusual: the equation giving the time
derivative of one reactant concentration, say A(x,t), contains the terms
depending not only on Laplacian A, but also on Laplacian B, i.e. depends also
on the transport operator of another reactant. Physically this is due to the
fact that several transitions from A to B and back may take place at one site
before the particle jumps.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:18:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sagues",
"F.",
""
],
[
"Shkilev",
"V. P.",
""
],
[
"Sokolov",
"I. M.",
""
]
] | [
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] |
712.1437 | Peter Van | P. V\'an | Internal energy in dissipative relativistic fluids | 8 pages | Journal of Mechanics of Materials and Structures, 3/6 (2008)
1161-1169. | null | null | nucl-th | null | Liu procedure is applied to a first order weakly nonlocal special
relativistic fluid. It is shown, that a reasonable relativistic theory is and
extended one, where the basic state space contains the momentum density. This
property follows from the structure of the energy-momentum balance and the
Second Law of thermodynamics. Moreover, the entropy depends on the energy
density and the momentum density on a given specific way, indicating that the
local rest frame energy density cannot be interpreted as the internal energy,
the local rest frame momentum density should be considered, too. The
corresponding constitutive relations for the stress and the energy flux are
derived.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:20:06 GMT"
}
] | 2008-08-01T00:00:00 | [
[
"Ván",
"P.",
""
]
] | [
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] |
712.1438 | Miriam Giorgini | M.Giorgini (Bologna University and INFN) | Search for massive rare particles with the SLIM experiment | 4 pages, 5 EPS figures. Talk given at the 10th ICATPP Conference on
Astroparticle, Particle, Space Physics, Detectors and Medical Physics
Applications, Como, Italy, 8-12 October 2007 | null | 10.1142/9789812819093_0035 | null | hep-ex | null | The SLIM experiment is a large array of nuclear track detectors located at
the Chacaltaya High Altitude Laboratory (5260 m a.s.l.). The preliminary
results from the analysis of ~383 m^2 exposed for 4.07 y are here reported. The
detector is sensitive to Intermediate Mass Magnetic Monopoles, 10^5 < M_M <
10^12 GeV, and to SQM nuggets and Q-balls, which are possible Dark Matter
candidates.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:21:10 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Giorgini",
"M.",
"",
"Bologna University and INFN"
]
] | [
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712.1439 | Eugene Terentjev | K.K. Hon, D. Corbett and E.M. Terentjev | Thermal diffusion and bending kinetics in nematic elastomer cantilever | null | null | 10.1140/epje/i2007-10266-4 | null | cond-mat.soft cond-mat.mtrl-sci | null | Vertically aligned mono-domain nematic liquid crystal elastomers contract
when heated. If a temperature gradient is applied across the width of such a
cantilever, inhomogeneous strain distribution leads to bending motion. We
modelled the kinetics of thermally-induced bending in the limit of a long thin
strip and the predicted time-variation of curvature agreed quantitatively with
experimental data from samples with a range of critical indices and
nematic-isotropic transition temperatures. We also deduced a value for the
thermal diffusion coefficient of the elastomer.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:21:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hon",
"K. K.",
""
],
[
"Corbett",
"D.",
""
],
[
"Terentjev",
"E. M.",
""
]
] | [
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712.144 | Ganna Ivashchenko | Amjad Al-Sawad | Multi Eruption Solar Energetic Particle Events Observed with SOHO/ERNE | Published in Proceedings of the 14th Young Scientists Conference on
Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007 | YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A.
Golovin), Kyiv, Kyivskyi Universytet, pp. 5-14, 2007 | null | null | astro-ph | null | A combination of many Solar energetic particle (SEP) events, each one of
which is associated with a single eruption, can create one complex
intensity-time profile, that will result in masking the observation of the
first injected particles detected near Earth for each participated eruption. We
defined such SEP events as Multi Eruption Solar Energetic Particle (MESEP)
events. We have investigated the intensity-time profile of 333 solar energetic
particle events during the operation time of SOHO mission and studied the
associative solar eruptions (CMEs and solar flare) from the starting time of
each event till the end. We found that most of the events have multi eruption
phenomena which might or might not affect the intensity-time profile. We found
that it is possible to know the real effect of some of the eruptions during the
whole duration of the event, even if their effect as masked by the first
eruption, by studying the widest possible energy range, the $^4He/P$ ratio and
the anisotropy.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:28:41 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Al-Sawad",
"Amjad",
""
]
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] |
712.1441 | Andrea Lapi | A. Cavaliere (1) and A. Lapi (1,2) ((1) Univ. "Tor Vergata", Roma,
Italy; (2) SISSA/ISAS, Trieste, Italy) | Missing Baryons, from Clusters to Groups of Galaxies | 5 pages, 3 figures, uses REVTeX4 + emulateapj.cls and apjfonts.sty.
Accepted on ApJL | Astrophys.J. 673 (2008) L5 | 10.1086/527435 | null | astro-ph | null | From clusters to groups of galaxies, the powerful bremsstrahlung radiation
L_X emitted in X rays by the intracluster plasma is observed to decline sharply
with lowering virial temperatures T (i.e., at shallower depths of the
gravitational wells) after a steep local L_X-T correlation; this implies
increasing scarcity of diffuse baryons relative to dark matter, well under the
cosmic fraction. We show how the widely debated issue concerning these `missing
baryons' is solved in terms of the thermal and/or dynamical effects of the
kinetic (at low redshifts z) and radiative (at high z) energy inputs from
central active galactic nuclei, of which independent evidence is being
observed. From these inputs we compute shape and z-evolution expected for L_X-T
correlation which agree with the existing data, and provide a predictive
pattern for future observations.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:30:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cavaliere",
"A.",
""
],
[
"Lapi",
"A.",
""
]
] | [
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] |
712.1442 | J\'anos K\"orner | J\'anos K\"orner, G\'abor Simonyi, Blerina Sinaimeri | On types of growth for graph-different permutations | 14 pages+title page | null | null | null | math.CO cs.IT math.IT | null | We consider an infinite graph G whose vertex set is the set of natural
numbers and adjacency depends solely on the difference between vertices. We
study the largest cardinality of a set of permutations of [n] any pair of which
differ somewhere in a pair of adjacent vertices of G and determine it
completely in an interesting special case. We give estimates for other cases
and compare the results in case of complementary graphs. We also explore the
close relationship between our problem and the concept of Shannon capacity
"within a given type".
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:32:39 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Körner",
"János",
""
],
[
"Simonyi",
"Gábor",
""
],
[
"Sinaimeri",
"Blerina",
""
]
] | [
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712.1443 | Ganna Ivashchenko | K. Baczek, B. Wszolek | The Jagiellonians and the Stars | Published in Proceedings of the 14th Young Scientists Conference on
Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007 | YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A.
Golovin), Kyiv, Kyivskyi Universytet, pp. 15-17, 2007 | null | null | astro-ph | null | The largest centre for astronomical and astrological study in the fifteenth
century was the University of Cracow, which always was under special care of
Jagiellonians. The use of astronomy and astrology at Jagiellonian courts in the
fifteenth and sixteenth centuries were very common. We try to convince the
reader about this, exposing very limited historical sources.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:35:03 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Baczek",
"K.",
""
],
[
"Wszolek",
"B.",
""
]
] | [
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] |
712.1444 | Detlef Klimm | D. Klimm, S. Ganschow, D. Schulz, R. Fornari | The growth of ZnO crystals from the melt | 6 pages, 6 figures, accepted for J. Crystal Growth | null | 10.1016/j.jcrysgro.2008.02.027 | null | cond-mat.mtrl-sci cond-mat.other physics.chem-ph | null | The peculiar properties of zinc oxide (ZnO) make this material interesting
for very different applications like light emitting diodes, lasers, and
piezoelectric transducers. Most of these applications are based on epitaxial
ZnO layers grown on suitable substrates, preferably bulk ZnO. Unfortunately the
thermochemical properties of ZnO make the growth of single crystals difficult:
the triple point 1975 deg C., 1.06 bar and the high oxygen fugacity at the
melting point p_O2 = 0.35 bar lead to the prevailing opinion that ZnO crystals
for technical applications can only be grown either by a hydrothermal method or
from "cold crucibles" of solid ZnO. Both methods are known to have significant
drawbacks. Our thermodynamic calculations and crystal growth experiments show,
that in contrast to widely accepted assumptions, ZnO can be molten in metallic
crucibles, if an atmosphere with "self adjusting" p_O2 is used. This new result
is believed to offer new perspectives for ZnO crystal growth by established
standard techniques like the Bridgman method.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:39:22 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 15:36:16 GMT"
},
{
"version": "v3",
"created": "Tue, 26 Feb 2008 07:21:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Klimm",
"D.",
""
],
[
"Ganschow",
"S.",
""
],
[
"Schulz",
"D.",
""
],
[
"Fornari",
"R.",
""
]
] | [
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] |
712.1445 | Takashi Mukaiyama Dr. | Yasuhisa Inada, Munekazu Horikoshi, Shuta Nakajima, Makoto
Kuwata-Gonokami, Masahito Ueda and Takashi Mukaiyama | Critical Temperature and Condensate Fraction of a Fermion Pair
Condensate | null | null | 10.1103/PhysRevLett.101.180406 | null | cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report on measurements of the critical temperature and the temperature
dependence of the condensate fraction for a fermion pair condensate of 6Li
atoms. The Bragg spectroscopy is employed to determine the critical temperature
and the condensate fraction after a fast magnetic field ramp to the molecular
side of the Feshbach resonance. Our measurements reveal the level-off of the
critical temperature and the limiting behavior of condensate fraction near the
unitarity limit.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:08:54 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Dec 2007 23:53:16 GMT"
},
{
"version": "v3",
"created": "Mon, 28 Jan 2008 07:21:30 GMT"
},
{
"version": "v4",
"created": "Wed, 16 Jul 2008 06:05:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Inada",
"Yasuhisa",
""
],
[
"Horikoshi",
"Munekazu",
""
],
[
"Nakajima",
"Shuta",
""
],
[
"Kuwata-Gonokami",
"Makoto",
""
],
[
"Ueda",
"Masahito",
""
],
[
"Mukaiyama",
"Takashi",
""
]
] | [
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] |
712.1446 | Ashley Montanaro | Ashley Montanaro, Harumichi Nishimura and Rudy Raymond | Unbounded Error Quantum Query Complexity | 14 pages | Theoretical Computer Science vol. 412 no. 35, pp. 4619-4628, 2011 | 10.1016/j.tcs.2011.04.043 | null | quant-ph | null | This work studies the quantum query complexity of Boolean functions in a
scenario where it is only required that the query algorithm succeeds with a
probability strictly greater than 1/2. We show that, just as in the
communication complexity model, the unbounded error quantum query complexity is
exactly half of its classical counterpart for any (partial or total) Boolean
function. Moreover, we show that the "black-box" approach to convert quantum
query algorithms into communication protocols by Buhrman-Cleve-Wigderson
[STOC'98] is optimal even in the unbounded error setting.
We also study a setting related to the unbounded error model, called the
weakly unbounded error setting, where the cost of a query algorithm is given by
q+log(1/2(p-1/2)), where q is the number of queries made and p>1/2 is the
success probability of the algorithm. In contrast to the case of communication
complexity, we show a tight Theta(log n) separation between quantum and
classical query complexity in the weakly unbounded error setting for a partial
Boolean function. We also show the asymptotic equivalence between them for some
well-studied total Boolean functions.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:42:07 GMT"
}
] | 2016-05-25T00:00:00 | [
[
"Montanaro",
"Ashley",
""
],
[
"Nishimura",
"Harumichi",
""
],
[
"Raymond",
"Rudy",
""
]
] | [
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] |
712.1447 | Ganna Ivashchenko | L.A. Berdina, A.A. Minakov | Microlensing Effects in Atmospheres of Substars | Published in Proceedings of the 14th Young Scientists Conference on
Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007 | YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A.
Golovin), Kyiv, Kyivskyi Universytet, pp. 18-21, 2007 | null | null | astro-ph | null | The purpose of the present work is the study of focusing properties of
atmospheres of substars that is necessary for adequate interpreting of
observational data and for solving the inverse problem consisting in recovery
parameters of 'microlenses' (substars) and sources (quasars). Amplification
factor for a quasar image as projected onto the field of microlenses-substars
was computed for optical and radio wavelengths.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:42:21 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Berdina",
"L. A.",
""
],
[
"Minakov",
"A. A.",
""
]
] | [
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] |
712.1448 | Ulrich Schollwoeck | Adrian Kleine, Corinna Kollath, Ian P. McCulloch, Thierry Giamarchi,
Ulrich Schollwoeck | Excitations in two-component Bose-gases | null | null | 10.1088/1367-2630/10/4/045025 | null | cond-mat.stat-mech | null | In this paper, we study a strongly correlated quantum system that has become
amenable to experiment by the advent of ultracold bosonic atoms in optical
lattices, a chain of two different bosonic constituents. Excitations in this
system are first considered within the framework of bosonization and Luttinger
liquid theory which are applicable if the Luttinger liquid parameters are
determined numerically. The occurrence of a bosonic counterpart of fermionic
spin-charge separation is signalled by a characteristic two-peak structure in
the spectral functions found by dynamical DMRG in good agreement with
analytical predictions. Experimentally, single-particle excitations as probed
by spectral functions are currently not accessible in cold atoms. We therefore
consider the modifications needed for current experiments, namely the
investigation of the real-time evolution of density perturbations instead of
single particle excitations, a slight inequivalence between the two
intraspecies interactions in actual experiments, and the presence of a
confining trap potential. Using time-dependent DMRG we show that only
quantitative modifications occur. With an eye to the simulation of strongly
correlated quantum systems far from equilibrium we detect a strong dependence
of the time-evolution of entanglement entropy on the initial perturbation,
signalling limitations to current reasonings on entanglement growth in
many-body systems.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:46:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kleine",
"Adrian",
""
],
[
"Kollath",
"Corinna",
""
],
[
"McCulloch",
"Ian P.",
""
],
[
"Giamarchi",
"Thierry",
""
],
[
"Schollwoeck",
"Ulrich",
""
]
] | [
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] |
712.1449 | Ganna Ivashchenko | K. Bryndal, B. Wszolek | Spectroscopic Families Among Diffuse Interstellar Bands | Published in Proceedings of the 14th Young Scientists Conference on
Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007 | YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A.
Golovin), Kyiv, Kyivskyi Universytet, pp. 22-24, 2007 | null | null | astro-ph | null | Looking for spectroscopic families in the whole set of discovered diffuse
interstellar bands (DIBs) is an indirect trial of solving the problem of DIBs'
carriers. Basing on optical high resolution spectra, covering the range from
5655 to 7020 \AA, we found few relatively strong DIBs which are not well
correlated one with another and therefore they may play a role of
representatives of separate spectroscopic families. In the next step we
indicated DIBs which tend to follow the behaviour of their representatives. As
a result of our analysis we propose few, probably not complete yet,
spectroscopic families of DIBs.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:50:53 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Bryndal",
"K.",
""
],
[
"Wszolek",
"B.",
""
]
] | [
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712.145 | Nobuyuki Sakai | Nobuyuki Sakai (Yamagata U), Misao Sasaki (YITP) | Stability of Q-balls and Catastrophe | 9 pages, 4 figures, some discussions and references added, to apear
in Prog. Theor. Phys | Prog.Theor.Phys.119:929-937,2008 | 10.1143/PTP.119.929 | YITP-07-84 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We propose a practical method for analyzing stability of Q-balls for the
whole parameter space, which includes the intermediate region between the
thin-wall limit and thick-wall limit as well as Q-bubbles (Q-balls in false
vacuum), using the catastrophe theory. We apply our method to the two concrete
models, $V_3=m^2\phi^2/2-\mu\phi^3+\lambda\phi^4$ and
$V_4=m^2\phi^2/2-\lambda\phi^4+\phi^6/M^2$. We find that $V_3$ and $V_4$ Models
fall into {\it fold catastrophe} and {\it cusp catastrophe}, respectively, and
their stability structures are quite different from each other.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:52:34 GMT"
},
{
"version": "v2",
"created": "Thu, 5 Jun 2008 12:05:03 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Sakai",
"Nobuyuki",
"",
"Yamagata U"
],
[
"Sasaki",
"Misao",
"",
"YITP"
]
] | [
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712.1451 | Ganna Ivashchenko | A. Martin-Carrillo, M. Kirsch, E. Kendziorra, R. Staubert | X-ray Timing Analysis of Six Pulsars Using ESA's XMM-Newton Observatory | Published in Proceedings of the 14th Young Scientists Conference on
Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007 | YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A.
Golovin), Kyiv, Kyivskyi Universytet, pp. 25-29, 2007 | null | null | astro-ph | null | We present results of a timing analysis of various isolated pulsars using
ESA's \emph{XMM-Newton} observatory. Isolated pulsars are useful for
calibration purposes because of their stable emission. We have analyzed six
pulsars with different pulse profiles in a range of periods between 15 and 200
ms. All observations were made using the \emph{EPIC-pn camera} in its faster
modes (Small window, Timing and Burst modes). We investigate the relative
timing accuracy of the camera by comparing the pulse periods determined from
the \emph{EPIC-pn camera} observations with those from radio observations. As a
result of our analysis we conclude that the relative timing accuracy of the
\emph{EPIC-pn camera} is of the order of $1\times 10^{-8}$.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:54:15 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Martin-Carrillo",
"A.",
""
],
[
"Kirsch",
"M.",
""
],
[
"Kendziorra",
"E.",
""
],
[
"Staubert",
"R.",
""
]
] | [
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] |
712.1452 | Ganna Ivashchenko | M. Dyrka, B. Wszolek | Interstellar C_2 Molecule Detected in UV Spectra of Reddened Stars | Published in Proceedings of the 14th Young Scientists Conference on
Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007 | YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A.
Golovin), Kyiv, Kyivskyi Universytet, pp. 30-33, 2007 | null | null | astro-ph | null | $C_2$ molecule is sometimes considered as a crucial component of carriers of
some diffuse interstellar bands. Using UV data achieved by spectrometer STIS
fed with HST we detected interstellar $C_2$ lines for few reddened target
stars. We tried to verify the idea that intensity of $C_2$ lines around 2313
\AA is correlated with some diffuse interstellar bands.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 11:57:20 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Dyrka",
"M.",
""
],
[
"Wszolek",
"B.",
""
]
] | [
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712.1453 | Julia Garayoa | Julia Garayoa (Valencia U. and Valencia U.-IFIC), Thomas Schwetz
(CERN) | Neutrino mass hierarchy and Majorana CP phases within the Higgs triplet
model at the LHC | 22 pages, 6 figures. Version to be published at JHEP | JHEP 0803:009,2008 | 10.1088/1126-6708/2008/03/009 | CERN-PH-TH/2007-255, IFIC/07-75, FTUV-07-1210 | hep-ph | null | Neutrino masses may be generated by the VEV of an $SU(2)_L$ Higgs triplet. We
assume that the doubly charged component of such a triplet has a mass in the
range of several 100 GeV, such that it is accessible at LHC. Its decay into
like-sign leptons provides a clean experimental signature, which allows for a
direct test of the neutrino mass matrix. By exploring the branching ratios of
this decay into leptons of various flavours, we show that within this model the
type of the neutrino mass spectrum (normal, inverted or quasi-degenerate) might
actually be resolved at the LHC. Furthermore, we show that within the Higgs
triplet model for neutrino mass the decays of the doubly charged scalar into
like-sign lepton pairs at the LHC provide a possibility to determine the
Majorana CP phases of the lepton mixing matrix.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:59:54 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Feb 2008 14:04:11 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Garayoa",
"Julia",
"",
"Valencia U. and Valencia U.-IFIC"
],
[
"Schwetz",
"Thomas",
"",
"CERN"
]
] | [
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712.1454 | Carlos Carrasco-Gonz\'alez | Carlos Carrasco-Gonzalez (1), Guillem Anglada (1), Luis F. Rodriguez
(2), Jose M. Torrelles (3), Mayra Osorio (1) and Jose M. Girart (3) (1.
Instituto de Astrofisica de Andalucia, CSIC; 2. Centro de Radioastronomia y
Astrofisica, UNAM; 3. Instituto de Ciencias del Espacio (CSIC) and Institut
d'Estudis Espacials de Catalunya) | A Multiple System of Radio Sources at the Core of the L723 Multipolar
Outflow | Accepted for publication in The Astrophysical Journal (2007 December
6) | null | 10.1086/527550 | null | astro-ph | null | We present high angular resolution Very Large Array multi-epoch continuum
observations at 3.6 cm and 7 mm towards the core of the L723 multipolar outflow
revealing a multiple system of four radio sources suspected to be YSOs in a
region of only ~4 arcsecs (1200 AU) in extent. The 3.6 cm observations show
that the previously detected source VLA 2 contains a close (separation ~0.29
arcsecs or ~90 AU) radio binary, with components (A and B) along a position
angle of ~150 degrees. The northern component (VLA 2A) of this binary system is
also detected in the 7 mm observations, with a positive spectral index between
3.6 cm and 7 mm. In addition, the source VLA 2A is associated with extended
emission along a position angle of ~115 degrees, that we interpret as
outflowing shock-ionized gas that is exciting a system of HH objects with the
same position angle. A third, weak 3.6 cm source, VLA 2C, that is detected also
at 7 mm, is located ~0.7 arcsecs northeast of VLA 2A, and is possibly
associated with the water maser emission in the region. The 7 mm observations
reveal the presence of an additional source, VLA 2D, located ~3.5 arcsecs
southeast of VLA 2A, and with a 1.35 mm counterpart. All these radio continuum
sources have a positive spectral index, compatible with them being YSOs. We
also propose that the high velocity CO emission observed in the region could be
the superposition of multiple outflows (at least three independent bipolar
outflows) excited by the YSOs located at the core, instead of the previous
interpretations in terms of only one or two outflows.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:16:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Carrasco-Gonzalez",
"Carlos",
""
],
[
"Anglada",
"Guillem",
""
],
[
"Rodriguez",
"Luis F.",
""
],
[
"Torrelles",
"Jose M.",
""
],
[
"Osorio",
"Mayra",
""
],
[
"Girart",
"Jose M.",
""
]
] | [
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] |
712.1455 | Wojciech Kry\'nski | Wojciech Kry\'nski | On contact equivalence of systems of ordinary differential equations | null | null | null | null | math.CA math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider a problem of equivalence of generic pairs $(X,V)$ on a manifold
$M$, where $V$ is a distribution of rank $m$ and $X$ is a distribution of rank
one. We construct a canonical bundle with a canonical frame. We prove that two
pairs are equivalent if and only if the corresponding frames are diffeomorphic.
As a particular case, with $V$ integrable, we provide a new solution to the
problem of contact equivalence of systems of $m$ ordinary differential
equations: $x^{(k+1)}=F(t,x,x',...,x^{(k)})$, where $k>2$ or $k=2$ and $m>1$.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:17:34 GMT"
},
{
"version": "v2",
"created": "Wed, 27 May 2009 15:11:37 GMT"
}
] | 2009-05-27T00:00:00 | [
[
"Kryński",
"Wojciech",
""
]
] | [
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] |
712.1456 | Imen Kammoun | Jean-Marc Bardet (SAMOS, Ces), Imen Kammoun (SAMOS, Ces) | Detecting abrupt changes of the long-range dependence or the
self-similarity of a Gaussian process | null | null | null | null | math.ST stat.TH | null | In this paper, an estimator of $m$ instants ($m$ is known) of abrupt changes
of the parameter of long-range dependence or self-similarity is proved to
satisfy a limit theorem with an explicit convergence rate for a sample of a
Gaussian process. In each estimated zone where the parameter is supposed not to
change, a central limit theorem is established for the parameter's (of
long-range dependence, self-similarity) estimator and a goodness-of-fit test is
also built. {\it To cite this article: J.M. Bardet, I. Kammoun, C. R. Acad.
Sci. Paris, Ser. I 340 (2007).}
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:27:16 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Apr 2008 06:12:36 GMT"
}
] | 2008-04-28T00:00:00 | [
[
"Bardet",
"Jean-Marc",
"",
"SAMOS, Ces"
],
[
"Kammoun",
"Imen",
"",
"SAMOS, Ces"
]
] | [
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] |
712.1457 | Eduardo Esteves | Lucia Caporaso, Juliana Coelho and Eduardo Esteves | Abel maps of Gorenstein curves | null | null | null | null | math.AG | null | For a Gorenstein curve X and a nonsingular point P of X, we construct Abel
maps A from X to J_X^1 and A_P from X to J_X^0, where J_X^i is the moduli
scheme for simple, torsion-free, rank-1 sheaves on X of degree i. The image
curves of A and A_P are shown to have the same arithmetic genus of X. Also, A
and A_P are shown to be embeddings away from rational subcurves L of X meeting
the closure of X-L in separating nodes. Finally, we establish a connection with
Seshadri's moduli scheme U_X(1) for semistable, torsion-free, rank-1 sheaves on
X, obtaining an embedding of A(X) into U_X(1).
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:29:18 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Caporaso",
"Lucia",
""
],
[
"Coelho",
"Juliana",
""
],
[
"Esteves",
"Eduardo",
""
]
] | [
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] |
712.1458 | Ji Meng Loh | Ji Meng Loh, Zhengyuan Zhu | Accounting for spatial correlation in the scan statistic | Published in at http://dx.doi.org/10.1214/07-AOAS129 the Annals of
Applied Statistics (http://www.imstat.org/aoas/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Statistics 2007, Vol. 1, No. 2, 560-584 | 10.1214/07-AOAS129 | IMS-AOAS-AOAS129 | stat.AP | null | The spatial scan statistic is widely used in epidemiology and medical studies
as a tool to identify hotspots of diseases. The classical spatial scan
statistic assumes the number of disease cases in different locations have
independent Poisson distributions, while in practice the data may exhibit
overdispersion and spatial correlation. In this work, we examine the behavior
of the spatial scan statistic when overdispersion and spatial correlation are
present, and propose a modified spatial scan statistic to account for that.
Some theoretical results are provided to demonstrate that ignoring the
overdispersion and spatial correlation leads to an increased rate of false
positives, which is verified through a simulation study. Simulation studies
also show that our modified procedure can substantially reduce the rate of
false alarms. Two data examples involving brain cancer cases in New Mexico and
chickenpox incidence data in France are used to illustrate the practical
relevance of the modified procedure.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:30:09 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Loh",
"Ji Meng",
""
],
[
"Zhu",
"Zhengyuan",
""
]
] | [
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712.1459 | Olivier Tiret | O. Tiret, F. Combes (LERMA, Observatoire de Paris) | Interacting Galaxies with MOND | 4 pages, 2 figures. To appear in the proceedings of "Formation and
Evolution of Galaxy Disks" (J. G. Funes, and E. M. Corsini eds) | null | null | null | astro-ph | null | We compare N-body simulations performed in MOND with analogs in Newtonian
gravity with dark matter (DM). We have developed a code which solves the
Poisson equation in both gravity models. It is a grid solver using adaptive
mesh refinement techniques, allowing us to study isolated galaxies as well as
interacting galaxies. Galaxies in MOND are found to form bars faster and
stronger than in the DM model. In Newton dynamics, it is difficult to reproduce
the observed high frequency of strong bars, while MOND appears to fit better
the observations. Galaxy interactions and mergers, such as the Antennae, are
also simulated with Newton and MOND dynamics. In the latter, dynamical friction
is much weaker, and merging time-scales are longer. The formation of tidal
dwarf galaxies in tidal tails are also compared in MOND and Newton+DM models.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:30:41 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Tiret",
"O.",
"",
"LERMA, Observatoire de Paris"
],
[
"Combes",
"F.",
"",
"LERMA, Observatoire de Paris"
]
] | [
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] |
712.146 | Christian Berg | Christian Berg (University of Copenhagen), Ryszard Szwarc (University
of Wroclaw) | Bounds on Tur{\'a}n determinants | null | null | null | null | math.CA | null | Let \mu denote a symmetric probability measure on
[-1,1] and let (p_n) be the corresponding orthogonal polynomials normalized
such that p_n(1)=1. We prove that the normalized Tur{\'a}n determinant
\Delta_n(x)/(1-x^2), where \Delta_n=p_n^2-p_{n-1}p_{n+1}, is a Tur{\'a}n
determinant of order n-1 for orthogonal polynomials with respect to
(1-x^2)d\mu(x). We use this to prove lower and upper bounds for the normalized
Tur{\'a}n determinant in the interval -1<x<1.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:50:55 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Berg",
"Christian",
"",
"University of Copenhagen"
],
[
"Szwarc",
"Ryszard",
"",
"University\n of Wroclaw"
]
] | [
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] |
712.1461 | Xin Wan | Zi-Xiang Hu, Xin Wan, Peter Schmitteckert | Trapping Abelian anyons in fractional quantum Hall droplets | 8 pages, 8 figures | Phys. Rev. B 77, 075331 (2008) | 10.1103/PhysRevB.77.075331 | null | cond-mat.mes-hall cond-mat.str-el | null | We study the trapping of Abelian anyons (quasiholes and quasiparticles) by a
local potential (e.g., induced by an AFM tip) in a microscopic model of
fractional quantum Hall liquids with long-range Coulomb interaction and edge
confining potential. We find, in particular, at Laughlin filling fraction $\nu
= 1/3$, both quasihole and quasiparticle states can emerge as the ground state
of the system in the presence of the trapping potential. As expected, we find
the presence of an Abelian quasihole has no effect on the edge spectrum of the
quantum liquid, unlike in the non-Abelian case [Phys. Rev. Lett. {\bf 97},
256804 (2006)]. Although quasiholes and quasiparticles can emerge generically
in the system, their stability depends on the strength of the confining
potential, the strength and the range of the trapping potential. We discuss the
relevance of the calculation to the high-accuracy generation and control of
individual anyons in potential experiments, in particular, in the context of
topological quantum computing.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:52:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hu",
"Zi-Xiang",
""
],
[
"Wan",
"Xin",
""
],
[
"Schmitteckert",
"Peter",
""
]
] | [
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] |
712.1462 | Raul Vera | Marc Mars, Jos\'e M. M. Senovilla and Ra\"ul Vera | Accelerating expansion and change of signature | LaTeX, 4 pages. Uses the eas.cls class. To appear in the proceedings
of the Spanish Relativity Meeting ERE'07 | null | 10.1051/eas:0830050 | null | gr-qc | null | We show that some types of sudden singularities admit a natural explanation
in terms of regular changes of signature on brane-worlds in AdS$_{5}$. The
present accelerated expansion of the Universe and its possible ending at a
sudden singularity may therefore simply be an indication that our braneworld is
about to change its Lorentzian signature to an Euclidean one, while remaining
fully regular. An explicit example of this behaviour satisfying the weak and
strong energy conditions is presented.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 16:31:47 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mars",
"Marc",
""
],
[
"Senovilla",
"José M. M.",
""
],
[
"Vera",
"Raül",
""
]
] | [
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] |
712.1463 | Salvino Ciccariello | Salvino Ciccariello | Strongly localized quantum crystalline states of the jellium model | 28 pages, 3 figures | null | null | DFPD/07/TH/16 | cond-mat.str-el | null | We consider a system made up of N electrons interacting with a neutralizing
positive background within a cubic box of volume V. After dividing the box into
N (or N/2) cubic cells for the polarized (unpolarized) case, we average the
creation field operator over each cell with a suitable weight function and we
consider the quantum crystalline states obtained by letting all the average
operators act on the vacuum state. These states exclude the possibility that
each cell may momentarily contain more than one or two electrons in the
polarized or unpolarized case. The expectation value of the Hamiltonian over
this class of states is evaluated in the thermodynamic limit and the weight
function is chosen in such a way to minimize the expectation value. The
involved numerical analysis is explicitly performed with a weight function
having a generalized Gaussian shape depending on a parameter. It turns out that
the unpolarized and polarized quantum crystalline states yield an energy per
particle smaller than the homogeneous Hartree-Fock ones for r_s>90 and r_s>28,
respectively. Moreover, for the polarized case, the energy per particle at
r_s=100 is -0.01448ryd close {to -0.0153530(8)ryd, the best quantum Monte Carlo
value [Drummond et al., Phys. Rev.B {\bf 69}, 085116, (2004)] and this
discrepancy measures the correlation contribution neglected in our
approximation.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 16:02:04 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Ciccariello",
"Salvino",
""
]
] | [
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712.1464 | Constantin Vernicos | Constantin Vernicos | Spectral Radius and Amenability in Hilbert Geometries | 24 pages, 3 figures | Houston Journal of Math, 35(4):1143-1169 (2009) | null | null | math.DG math.GM | null | We study the bottom of the spectrum in Hilbert geometries, we show that it is
zero if and only if the geometry is amenable, in other words if and only if it
admits a F\"olner sequence. We also show that the bottom of the spectrum admits
an upper bound, which depends only on the dimension and which is the bottom of
the spectrum of the Hyperbolic geometry of the same dimension. Horoballs, from
a purely metric point of view, and their relation with the bottom of the
spectrum in Hilbert geometries are briefly studied.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:57:29 GMT"
}
] | 2010-05-11T00:00:00 | [
[
"Vernicos",
"Constantin",
""
]
] | [
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] |
712.1465 | Tsonka Baicheva | Tsonka Baicheva, Iliya Bouyukliev, Stefan Dodunekov, and Veerle Fack | Binary and Ternary Quasi-perfect Codes with Small Dimensions | 4 pages | IEEE Transactions on Information Theory, vol. 54, issue 9, pp.
4335-4339, 2008 | 10.1109/TIT.2008.928277 | null | math.CO | null | The aim of this work is a systematic investigation of the possible parameters
of quasi-perfect (QP) binary and ternary linear codes of small dimensions and
preparing a complete classification of all such codes. First we give a list of
infinite families of QP codes which includes all binary, ternary and quaternary
codes known to is. We continue further with a list of sporadic examples of
binary and ternary QP codes. Later we present the results of our investigation
where binary QP codes of dimensions up to 14 and ternary QP codes of dimensions
up to 13 are classified.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:09:08 GMT"
},
{
"version": "v2",
"created": "Sat, 10 May 2008 09:16:41 GMT"
}
] | 2016-11-18T00:00:00 | [
[
"Baicheva",
"Tsonka",
""
],
[
"Bouyukliev",
"Iliya",
""
],
[
"Dodunekov",
"Stefan",
""
],
[
"Fack",
"Veerle",
""
]
] | [
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] |
712.1466 | Jomel Imperio | J. C. Imperio, Mikhail P. Solon, A. Laganapan, J. P. H. Esguerra, A.
Muriel | Theoretical Criteria for the Occurrence of Turbulence in Burger's
Equation | 7 pages; PACS numbers added | null | null | null | physics.flu-dyn | null | Throughout the history of the study of turbulence in fluid dynamics, there
has yet to arise a unique definition or theoretical criterion for this
important phenomenon. There have been interesting conjectures made by Ruelle
[2], Muriel [3], and Getreuer, Albano and Muriel [6], however, attempting to
provide the sufficient criteria for the onset of turbulence. In this paper, a
classic equation in fluid dynamics, Burger's equation, is solved in one and two
dimensions, and these conjectures are illustrated. This illustration supports
these conjectures by showing that the proposed criteria do arise mathematically
from the solutions of an equation modelling fluid flows.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 12:58:49 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Dec 2007 03:19:41 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Imperio",
"J. C.",
""
],
[
"Solon",
"Mikhail P.",
""
],
[
"Laganapan",
"A.",
""
],
[
"Esguerra",
"J. P. H.",
""
],
[
"Muriel",
"A.",
""
]
] | [
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] |
712.1467 | Michel Gross | Michael Atlan (LKB - Lhomond), Michel Gross (LKB - Lhomond), Pierre
Desbiolles (LKB - Lhomond), Emilie Absil (LPEM), Gilles Tessier (LPEM),
Mait\'e Coppey-Moisan (IJM) | Heterodyne holographic microscopy of gold particles | null | Optics Letters 33, 5 (2008) 500-502 | 10.1364/OL.33.000500 | null | physics.optics physics.bio-ph | null | We report experimental results on heterodyne holographic microscopy of
subwavelength-sized gold particles. The apparatus uses continuous green laser
illumination of the metal beads in a total internal reflection configuration
for dark-field operation. Detection of the scattered light at the illumination
wavelength on a charge-coupled device array detector enables 3D localization of
brownian particles in water
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:00:15 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 18:45:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Atlan",
"Michael",
"",
"LKB - Lhomond"
],
[
"Gross",
"Michel",
"",
"LKB - Lhomond"
],
[
"Desbiolles",
"Pierre",
"",
"LKB - Lhomond"
],
[
"Absil",
"Emilie",
"",
"LPEM"
],
[
"Tessier",
"Gilles",
"",
"LPEM"
],
[
"Coppey-Moisan",
"Maité",
"",
"IJM"
]
] | [
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] |
712.1468 | Evgeny Lakshtanov L | A. I. Aleksenko, J. P. Cruz, E. L. Lakshtanov | High frequency limit of the Transport Cross Section and boundedness of
the Total Cross Section in scattering by an obstacle with impedance boundary
conditions | null | J. Phys. A: Math. Theor., 41(1), 255203 (5pp), 2008 | 10.1088/1751-8113/41/25/255203 | null | math-ph math.MP | null | The scalar scattering of the plane wave by a strictly convex obstacle with
impedance boundary conditions is considered. The uniform boundedness of the
Total Cross Section for all values of frequencies is proved. The high frequency
limit of the Transport Cross Section is founded and presented as a classical
functional of the variational theory.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:25:31 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 10:27:04 GMT"
}
] | 2010-09-13T00:00:00 | [
[
"Aleksenko",
"A. I.",
""
],
[
"Cruz",
"J. P.",
""
],
[
"Lakshtanov",
"E. L.",
""
]
] | [
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] |
712.1469 | Shinji Takeda | Shinji Takeda | Perturbative analysis of the Neuberger-Dirac operator in the
Schr\"odinger functional | 22 pages 5 figures | Nucl.Phys.B796:402-421,2008 | 10.1016/j.nuclphysb.2007.12.020 | HU-EP-07/61, SFB/CPP-07-84 | hep-lat | null | We investigate the spectrum of the free Neuberger-Dirac operator $\Dov$ on
the Schr\"odinger functional (SF). We check that the lowest few eigen-values of
the Hermitian operator $\Dov^{\dag}\Dov$ in unit of $L^{-2}$ converge to the
continuum limit properly. We also perform a one-loop calculation of the SF
coupling, and then check the universality and investigate lattice artifacts of
the step scaling function. It turns out that the lattice artifacts for the
Neuberger-Dirac operator are comparable in those of the clover action.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:27:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Takeda",
"Shinji",
""
]
] | [
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] |
712.147 | Famaey Benoit | Benoit Famaey, Arnaud Siebert, Alain Jorissen | On the age heterogeneity of the Pleiades, Hyades and Sirius moving
groups | 8 pages, 8 figures, accepted for publication in A&A | null | 10.1051/0004-6361:20078979 | null | astro-ph | null | We investigate the nature of the classical low-velocity structures in the
local velocity field, i.e. the Pleiades, Hyades and Sirius moving groups. After
using a wavelet transform to locate them in velocity space, we study their
relation with the open clusters kinematically associated with them. By directly
comparing the location of moving group stars in parallax space to the
isochrones of the embedded clusters, we check whether, within the observational
errors on the parallax, all moving group stars could originate from the
on-going evaporation of the associated cluster. We conclude that, in each
moving group, the fraction of stars making up the velocity-space overdensity
superimposed on the background is higher than the fraction of stars compatible
with the isochrone of the associated cluster. These observations thus favour a
dynamical (resonant) origin for the Pleiades, Hyades and Sirius moving groups.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:47:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Famaey",
"Benoit",
""
],
[
"Siebert",
"Arnaud",
""
],
[
"Jorissen",
"Alain",
""
]
] | [
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] |
712.1471 | Carsten Denker | C. Denker (1) and K. G. Strassmeier (1)((1)Astrophysikalisches
Institut Potsdam, Germany) | Solar Physics and the Solar-Stellar Connection at Dome C | 8 pages, 2 b/w figures, submitted to 2nd ARENA Conference on "The
Astrophysical Science Cases at Dome C'', H. Zinnecker, H. Rauer, and N.
Epchtein (eds.), EAS Publications Series | null | 10.1051/eas:0833014 | null | astro-ph | null | Solar magnetic fields evolve on many time-scales, e.g., the generation,
migration, and dissipation of magnetic flux during the 22-year magnetic cycle
of the Sun. Active regions develop and decay over periods of weeks. The
build-up of magnetic shear in active regions can occur within less than a day.
At the shortest time-scales, the magnetic field topology can change rapidly
within a few minutes as the result of eruptive events such as flares, filament
eruptions, and coronal mass ejections. The unique daytime seeing
characteristics at Dome C, i.e., continuous periods of very good to excellent
seeing during almost the entire Antarctic summer, allow us to address many of
the top science cases related to the evolution of solar magnetic fields. We
introduce the Advanced Solar Photometric Imager and Radiation Experiment and
present the science cases for synoptic solar observations at Dome C.
Furthermore, common science cases concerning the solar-stellar connection are
discussed in the context of the proposed International Concordia Explorer
Telescope.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:33:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Denker",
"C.",
""
],
[
"Strassmeier",
"K. G.",
""
]
] | [
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] |
712.1472 | Rolf Dyre Svegstrup | Ryszard Nest, Rolf Dyre Svegstrup | Classification of Connections on Higher-Dimensional Non-Commutative Tori | 13 pages | null | null | null | math.OA math.DG math.QA | null | If X is a full, finitely generated, projective module over a non-commutative
torus, the Yang-Mills functional attains its minimum exactly on the flat
connections on X. We classify the flat connections on modules admitting
integrable connections.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:58:50 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Nest",
"Ryszard",
""
],
[
"Svegstrup",
"Rolf Dyre",
""
]
] | [
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712.1473 | Peter Erwin | Peter Erwin, Michael Pohlen, Leonel Gutierrez, and John E. Beckman | Trends for Outer Disk Profiles | LaTeX, 2 pages, 1 EPS figure, uses modified newpasp.sty (included).
To appear in Formation and Evlution of Galaxy Disks, eds. J.G. Funes and E.M.
Corsini | null | null | null | astro-ph | null | The surface-brightness profiles of galaxy disks fall into three main classes,
based on whether they are simple exponentials (Type I), bend down at large
radii (Type II, "truncations") or bend up at large radii (Type III,
"antitruncations"). Here, we discuss how the frequency of these different
profiles depends on Hubble type, environment, and the presence or absence of
bars; these trends may herald important new tests for disk formation models.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:40:16 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Erwin",
"Peter",
""
],
[
"Pohlen",
"Michael",
""
],
[
"Gutierrez",
"Leonel",
""
],
[
"Beckman",
"John E.",
""
]
] | [
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712.1474 | Johann Summhammer | Johann Summhammer and Gustav Bernroider | Quantum entanglement in the voltage dependent sodium channel can
reproduce the salient features of neuronal action potential initiation | 2 Figures | null | null | null | physics.bio-ph | null | We investigate the effects of a quantum entanglement regime within an ion
conducting molecule (ion channel) of the neuronal plasma membrane on the onset
dynamics of propagating nerve pulses (action potentials). In particular, we
model the onset parameters of the sodium current in the Hodgkin Huxley equation
as three similar but independent probabilistic mechanisms which become quantum
entangled. The underlying physics is general and can involve entanglement
between various degrees of freedom underlaying ion transition states or 'gating
states' during conduction, e.g. Na$^+$ ions in different channel locations, or
different 'affinity' states of ions with atoms lining the sub-regions of the
channel protein ('filter-states'). We find that the 'quantum corrected' Hodgkin
Huxley equation incorporating entangled systems states can reproduce action
potential pulses with the critical onset dynamics observed recently in
neocortical neurons in vivo by Naundorf et al. [Nature {\bf 440}, 1060 (20
April 2006)]. Interestingly, the suggested entanglement term can also slow down
action potential initiation.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:43:19 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Summhammer",
"Johann",
""
],
[
"Bernroider",
"Gustav",
""
]
] | [
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] |
712.1475 | V Braguta | V.V. Braguta | The study of double vector charmonium mesons production at B-factories
within light cone formalism | 9 pages, 3 figures. Published version. References and new discussions
added. Some errors fixed, results changed only slightly | Phys.Rev.D78:054025,2008 | 10.1103/PhysRevD.78.054025 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper the processes $e^+ e^- \to J/\Psi J/\Psi, J/\Psi \psi', \psi'
\psi'$ are considered in the framework of light cone formalism. An important
distinction of this approach in comparison to the approaches used in other
papers is that relativistic and leading logarithmic radiative corrections to
the cross section can be easily resummed within light cone formalism. In this
paper the effect of this resummation is studied. It is shown that this effect
is important especially for the production of higher charmonium mesons. The
predicted cross sections are in agreement with the upper bounds set by Belle
collaboration.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:53:07 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Nov 2008 07:25:07 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Braguta",
"V. V.",
""
]
] | [
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712.1476 | Carlo Giocoli | Carlo Giocoli (1), Lidia Pieri (2,3), Giuseppe Tormen (1) ((1)
Dipartimento di Astronomia, Universita' degli Studi di Padova; (2) INAF; (3)
OaPD) | Analytical Approach to Subhaloes Population in Dark Matter Haloes | 10 pages, 7 figures - submitted to MNRAS | null | 10.1111/j.1365-2966.2008.13283.x | null | astro-ph | null | In the standard model of cosmic structure formation, dark matter haloes form
by gravitational instability. The process is hierarchical: smaller systems
collapse earlier, and later merge to form larger haloes. The galaxy clusters,
hosted by the largest dark matter haloes, are at the top of this hierarchy
representing the largest as well as the last structures formed in the universe,
while the smaller and first haloes are those Earth-sized dark subhaloes which
have been both predicted by theoretical considerations and found in numerical
simulations, though it does not exist any observational hints of their
existence. The probability that a halo of mass $m$ at redshift $z$ will be part
of a larger halo of mass $M$ at the present time can be described in the frame
of the extended Press & Schecter theory making use of the progenitor
(conditional) mass function. Using the progenitor mass function we calculate
analytically, at redshift zero, the distribution of subhaloes in mass,
formation epoch and rarity of the peak of the density field at the formation
epoch. That is done for a Milky Way-size system, assuming both a spherical and
an ellipsoidal collapse model. Our calculation assumes that small progenitors
do not lose mass due to dynamical processes after entering the parent halo, and
that they do not interact with other subhaloes. For a $\mathrm{\Lambda}$CDM
power spectrum we obtain a subhalo mass function $\mathrm{d}n/\mathrm{d}m$
proportional to $m^{- \alpha}$ with a model-independent $\alpha \sim 2$.
Assuming the dark matter is a weakly interacting massive particle, the inferred
distributions is used to test the feasibility of an indirect detection in the
$\gamma$-rays energy band of such a population of subhaloes with a GLAST-like
satellite.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:53:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Giocoli",
"Carlo",
""
],
[
"Pieri",
"Lidia",
""
],
[
"Tormen",
"Giuseppe",
""
]
] | [
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712.1477 | Marc Artzrouni | Marc Artzrouni (LMA - Pau) | Crossing paths in 2D Random Walks | null | null | null | null | stat.AP | null | We investigate crossing path probabilities for two agents that move randomly
in a bounded region of the plane or on a sphere (denoted $R$). At each discrete
time-step the agents move, independently, fixed distances $d_1$ and $d_2$ at
angles that are uniformly distributed in $(0,2\pi)$. If $R$ is large enough and
the initial positions of the agents are uniformly distributed in $R$, then the
probability of paths crossing at the first time-step is close to $ 2d_1d_2/(\pi
A[R])$, where $A[R]$ is the area of $R$. Simulations suggest that the long-run
rate at which paths cross is also close to $2d_1d_2/(\pi A[R])$ (despite marked
departures from uniformity and independence conditions needed for such a
conclusion).
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:55:15 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Artzrouni",
"Marc",
"",
"LMA - Pau"
]
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] |
712.1478 | Stanislaw D. Glazek | Stanislaw D. Glazek | Heavy Quarkonia in Light-Front QCD | 9 pages, latex, uses frascatiphys.sty, talk at HADRON07: XII Int.
Conf. on Hadron Spectroscopy, Frascati, October 8-13, 2007 | null | null | IFT/07/15 | hep-ph | null | This talk is based on results obtained for masses and wave functions of heavy
quarkonia in a light-front Hamiltonian formulation of QCD with just one flavor
of quarks using an ansatz for the mass-gap for gluons. Since the calculated
spectra compare reasonably well with data, some further steps one can make are
discussed.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 13:56:05 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Glazek",
"Stanislaw D.",
""
]
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