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712.1679 | Remi Carles | R\'emi Carles (I3M), Satoshi Masaki (Kyoto) | Semiclassical Analysis for Hartree equation | 16 pages | null | null | null | math.AP math-ph math.MP | null | We justify WKB analysis for Hartree equation in space dimension at least
three, in a regime which is supercritical as far as semiclassical analysis is
concerned. The main technical remark is that the nonlinear Hartree term can be
considered as a semilinear perturbation. This is in contrast with the case of
the nonlinear Schrodinger equation with a local nonlinearity, where quasilinear
analysis is needed to treat the nonlinearity.
| [
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712.168 | Delfim F. M. Torres | Moulay Rchid Sidi Ammi, Rui A. C. Ferreira, Delfim F. M. Torres | Diamond-$\alpha$ Jensen's Inequality on Time Scales | This is a preprint of an article whose final and definitive form will
appear in the \emph{Journal of Inequalities and Applications},
http://www.hindawi.com/journals/jia/. Accepted 07/April/2008 | Journal of Inequalities and Applications, vol. 2008, Article ID
576876, 13 pages, 2008 | 10.1155/2008/576876 | null | math.CA | null | The theory and applications of dynamic derivatives on time scales has
recently received considerable attention. The primary purpose of this paper is
to give basic properties of diamond-$\alpha$ derivatives which are a linear
combination of delta and nabla dynamic derivatives on time scales. We prove a
generalized version of Jensen's inequality on time scales via the
diamond-$\alpha$ integral and present some corollaries, including H\"{o}lder's
and Minkowski's diamond-$\alpha$ integral inequalities.
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712.1681 | Dafa Li | D. Li, X. Li, H. Huang, X. Li | Reply to the comment on "Stochastic local operations and classical
communication invariant and the residual entanglement for n qubits" | 3 pages, no figures | Phys. Rev. A 77, 056302 (2008) | 10.1103/PhysRevA.77.056302 | null | quant-ph | null | We have reviewed the comment in [3], posted on arXiv.org concerning our
recent work in [1]. We reply to the comment in this paper.
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] |
712.1682 | Stanislav Dubrovskiy | Vladimir Gol'dshtein, Stanislav Dubrovskiy | Lemma Poincar\'e for L_infty,loc - forms | 6 pages | null | null | null | math.DG math.FA | null | We show that every closed L_infty,loc - form on R^n is exact. Differential is
understood in the sense of currents. The proof does not use any explicit
geometric constructions. De Rham theorem follows.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:06:19 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Gol'dshtein",
"Vladimir",
""
],
[
"Dubrovskiy",
"Stanislav",
""
]
] | [
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712.1683 | Daniel Duque | Daniel Duque, Pedro Tarazona, and Enrique Chac\'on | Diffusion at the liquid-vapor interface | 25 pages, 7 figures. Submitted to J. Chem. Phys | null | 10.1063/1.2841128 | null | cond-mat.soft cond-mat.mtrl-sci | null | Recently, the intrinsic sampling method has been developed in order to
obtain, from molecular simulations, the intrinsic structure of the liquid-vapor
interface that is presupposed in the classical capillary wave theory. Our
purpose here is to study dynamical processes at the liquid-vapor interface,
since this method allows tracking down and analyzing the movement of surface
molecules, thus providing, with great accuracy, dynamical information on
molecules that are "at" the interface. We present results for the coefficients
for diffusion parallel and perpendicular to the liquid-vapor interface of the
Lennard-Jones fluid, as well as other time and length parameters that
characterize the diffusion process in this system. We also obtain statistics of
permanence and residence time. The generality of our results is tested by
varying the system size and the temperature; for the later case, an existing
model for alkali metals is also considered. Our main conclusion is that, even
if diffusion coefficients can still be computed, the turnover processes, by
which molecules enter and leave the intrinsic surface, are as important as
diffusion. For example, the typical time required for a molecule to traverse a
molecular diameter is very similar to its residence time at the surface.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:09:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Duque",
"Daniel",
""
],
[
"Tarazona",
"Pedro",
""
],
[
"Chacón",
"Enrique",
""
]
] | [
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712.1684 | Kai Matzutt | Kai Matzutt | Random Cluster Tessellations | 14 pages, 13 figures | null | null | null | math.MG math.PR | null | This article describes, in elementary terms, a generic approach to produce
discrete random tilings and similar random structures by using point process
theory. The standard Voronoi and Delone tilings can be constructed in this way.
For this purpose, convex polytopes are replaced by their vertex sets. Three
explicit constructions are given to illustrate the concept.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:17:05 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Matzutt",
"Kai",
""
]
] | [
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] |
712.1685 | Basarab Nicolescu | Evgenij Martynov and Basarab Nicolescu | Unified Model for Small-t and High-t Scattering at High Energies:
Predictions at RHIC and LHC | 6 pages, 2 table, 7 figures. Misprints are corrected | Eur.Phys.J.C56:57-62,2008 | 10.1140/epjc/s10052-008-0629-z | null | hep-ph | null | The urgency of predictions in large-t region at LHC stimulated us to present
a unified model of small and high t scattering at high energies. Our model is
based upon a safe theoretical ground: analyticity, unitarity, Regge behavior,
gluon exchange and saturation of bounds established in axiomatic quantum field
theory. We make precise predictions for the behavior of the differential cross
sections at high t, the evolution of the dip-shoulder structure localized in
the region of -t between 0.5 and 0.8 GeV**2 and the radical violation of the
exponential behavior of the first diffraction cone at small t.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:29:08 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Dec 2007 15:31:14 GMT"
},
{
"version": "v3",
"created": "Wed, 19 Dec 2007 17:20:30 GMT"
}
] | 2016-08-25T00:00:00 | [
[
"Martynov",
"Evgenij",
""
],
[
"Nicolescu",
"Basarab",
""
]
] | [
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] |
712.1686 | G\'{a}bor Lugosi | Luc Devroye, G\'abor Lugosi | Local tail bounds for functions of independent random variables | Published in at http://dx.doi.org/10.1214/00911797000000088 the
Annals of Probability (http://www.imstat.org/aop/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Probability 2008, Vol. 36, No. 1, 143-159 | 10.1214/00911797000000088 | IMS-AOP-AOP322 | math.PR | null | It is shown that functions defined on $\{0,1,...,r-1\}^n$ satisfying certain
conditions of bounded differences that guarantee sub-Gaussian tail behavior
also satisfy a much stronger ``local'' sub-Gaussian property. For self-bounding
and configuration functions we derive analogous locally subexponential
behavior. The key tool is Talagrand's [Ann. Probab. 22 (1994) 1576--1587]
variance inequality for functions defined on the binary hypercube which we
extend to functions of uniformly distributed random variables defined on
$\{0,1,...,r-1\}^n$ for $r\ge2$.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:29:48 GMT"
}
] | 2008-01-03T00:00:00 | [
[
"Devroye",
"Luc",
""
],
[
"Lugosi",
"Gábor",
""
]
] | [
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] |
712.1687 | David Jimenez | David Jimenez | A current-voltage model for Schottky-barrier graphene based transistors | 8 pages, 4 figures | Nanotechnology 19 (2008) 345204 | 10.1088/0957-4484/19/34/345204 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A low complexity computational model of the current-voltage characteristics
for graphene nano-ribbon (GNR) field effect transistors (FET), able to simulate
a hundred of points in few seconds using a PC, is presented. For quantum
capacitance controlled devices, self-consistent calculations of the
electrostatic potential can be skipped. Instead, analytical closed-form
electrostatic potential from Laplace's equation yields accurate results
compared with that obtained by self-consistent Non-Equilibrium Green's
Functions (NEGF) method. The model includes both tunnelling current through the
Schottky barrier (SB) at the contact interfaces and thermionic current above
the barrier, properly capturing the effect of arbitrary physical and electrical
parameters.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:48:56 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jul 2008 15:42:48 GMT"
}
] | 2008-07-15T00:00:00 | [
[
"Jimenez",
"David",
""
]
] | [
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] |
712.1688 | Mikheeva Elena | E. Mikheeva, A. Doroshkevich, V. Lukash (Astro Space Centre of P.N.
Lebedev Physics Institute, Moscow, Russia) | A solution of the cusp problem in relaxed halos of dark matter | 6 pages, 1 figure, submitted to Il Nuovo Cimento, a talk presented at
the conference "A Century of Cosmology: Past, Present and Future" (August
27-31 2007, Venezia, Italy) | Nuovo Cim.B122:1393-1398,2007 | 10.1393/ncb/i2008-10503-1 | null | astro-ph | null | We propose a solution of the cusp problem in framework of the standard
$\Lambda$CDM cosmology. To do this we describe the linear and nonlinear periods
of halo formation by the entropy function of dark matter particles. This
approach allows us to take into account together the impact of both the
processes of nonlinear relaxation of compressed matter and the small scale
initial velocity perturbations in collapsed halos. We show that such random
velocities lead to the random variations of the density profile of relaxed
halos. As a rule, they suppress the formation of cusp--like halos and favor the
creation of core--like ones. This approach allows us to reproduce observed
rotation curves, to explain their random scatter and deviations from simulated
ones.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:49:41 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Mikheeva",
"E.",
"",
"Astro Space Centre of P.N.\n Lebedev Physics Institute, Moscow, Russia"
],
[
"Doroshkevich",
"A.",
"",
"Astro Space Centre of P.N.\n Lebedev Physics Institute, Moscow, Russia"
],
[
"Lukash",
"V.",
"",
"Astro Space Centre of P.N.\n Lebedev Physics Institute, Moscow, Russia"
]
] | [
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] |
712.1689 | Hermine Landt | Hermine Landt (1), Paolo Padovani (2), Paolo Giommi (3), Matteo Perri
(3), Chi C. Cheung (4) ((1) Harvard-Smithsonian CfA, (2) ESO, (3) ASI Science
Data Center, (4) Stanford University) | A Search for Synchrotron X-ray Emission in Radio Quasars | 27 pages, 6 figures, accepted by ApJ | Astrophys.J.676:87-100,2008 | 10.1086/527531 | null | astro-ph | null | This paper presents XMM-Newton and Chandra X-ray spectroscopy of ten
flat-spectrum radio quasars (FSRQ) which are candidates to have an X-ray
spectrum dominated by jet synchrotron emission. In all these FSRQ, which are
less strongly relativistically beamed than blazars, a considerable contribution
from a power-law component similar to that present in radio-quiet quasars is
required to explain the observed X-ray fluxes and X-ray spectral slopes. And as
in radio-quiet quasars, their relatively high optical/UV fluxes can be
accounted for by a significant contribution from thermal accretion disk
emission. The lack of success in finding radio quasars with synchrotron X-rays
is attributed to the adopted selection criteria, which were based on the
multiwavelength flux ratios of BL Lacertae (BL Lac) objects. A refined
selection technique, which additionally involves radio imaging, is proposed to
search for these important candidates for the Gamma Ray Large Area Space
Telescope (GLAST). On the other hand, the discovered FSRQ with their strong
accretion disk signatures are expected to be important probes for studies of
the poorly known accretion disk - jet connection.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:51:10 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Landt",
"Hermine",
""
],
[
"Padovani",
"Paolo",
""
],
[
"Giommi",
"Paolo",
""
],
[
"Perri",
"Matteo",
""
],
[
"Cheung",
"Chi C.",
""
]
] | [
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] |
712.169 | Hannu Reittu | Hannu Reittu and Ilkka Norros | Random graph models of communication network topologies | Presented in ICCS 07, Boston USA,October 28-November 2, 2007 | null | null | null | math.PR | null | We consider a variant of so called power-law random graph. A sequence of
expected degrees corresponds to a power-law degree distribution with finite
mean and infinite variance. In previous works the asymptotic picture with
number of nodes limiting to infinity has been considered. It was found that an
interesting structure appears. It has resemblance with such graphs like the
Internet graph. Some simulations have shown that a finite sized variant has
similar properties as well. Here we investigate this case in more analytical
fashion, and, with help of some simple lower bounds for large valued
expectations of relevant random variables, we can shed some light into this
issue. A new term, 'communication range random graph' is introduced to
emphasize that some further restrictions are needed to have a relevant random
graph model for a reasonable sized communication network, like the Internet. In
this case a pleasant model is obtained, giving the opportunity to understand
such networks on an intuitive level. This would be beneficial in order to
understand, say, how a particular routing works in such networks.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 11:55:59 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Reittu",
"Hannu",
""
],
[
"Norros",
"Ilkka",
""
]
] | [
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] |
712.1691 | A. D. Polosa | Ad Polosa | Hints of a New Spectroscopy | Proceedings of the CHARM 2007 Workshop, Ithaca, NY, August 5-8, 2007 | ECONF C070805:36,2007 | null | null | hep-ph | null | There are several reasons to believe that some of the new particles observed
at B-factories have no ordinary quark composition. We briefly illustrate the
diquark-antidiquark model and the recent experimental discoveries which confirm
some of its most striking predictions.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:31:36 GMT"
}
] | 2011-06-15T00:00:00 | [
[
"Polosa",
"Ad",
""
]
] | [
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] |
712.1692 | Monika Meise | P.L. Davies, M. Meise | Approximating Data with weighted smoothing Splines | null | Journal of Nonparametric Statistics, 20:3, (2008) 207-228 | null | null | stat.ME | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Given a data set (t_i, y_i), i=1,..., n with the t_i in [0,1] non-parametric
regression is concerned with the problem of specifying a suitable function
f_n:[0,1] -> R such that the data can be reasonably approximated by the points
(t_i, f_n(t_i)), i=1,..., n. If a data set exhibits large variations in local
behaviour, for example large peaks as in spectroscopy data, then the method
must be able to adapt to the local changes in smoothness. Whilst many methods
are able to accomplish this they are less successful at adapting derivatives.
In this paper we show how the goal of local adaptivity of the function and its
first and second derivatives can be attained in a simple manner using weighted
smoothing splines. A residual based concept of approximation is used which
forces local adaptivity of the regression function together with a global
regularization which makes the function as smooth as possible subject to the
approximation constraints.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:14:42 GMT"
},
{
"version": "v2",
"created": "Wed, 18 Mar 2009 15:48:24 GMT"
}
] | 2009-03-18T00:00:00 | [
[
"Davies",
"P. L.",
""
],
[
"Meise",
"M.",
""
]
] | [
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712.1693 | Evgeny Strahov | Alexei Borodin and Eugene Strahov | Correlation Kernels for Discrete Symplectic and Orthogonal Ensembles | 45 pages, added references | null | 10.1007/s00220-008-0629-8 | null | math-ph math.MP | null | H. Widom derived formulae expressing correlation functions of orthogonal and
symplectic ensembles of random matrices in terms of orthogonal polynomials (H.
Widom. J. Stat. Phys. 94, (1999) 347-363). We obtain similar results for
discrete ensembles whose weights have rational discrete logarithmic
derivatives, and compute explicitly correlation kernels associated to the
classical Meixner and Charlier orthogonal polynomials.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:49:06 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jan 2008 13:37:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Borodin",
"Alexei",
""
],
[
"Strahov",
"Eugene",
""
]
] | [
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] |
712.1694 | Wei Yan | Wei Yan, Min Yan, Zhichao Ruan, Min Qiu | Coordinate transformation makes perfect invisibility cloak with
arbitrary shape | 12 pages, 3 figures | New. J. Phys. 10, 043040(2008) | 10.1088/1367-2630/10/4/043040 | null | physics.optics | null | By investigating wave properties at cloak boundaries, invisibility cloaks
with arbitrary shape constructed by general coordinate transformations are
confirmed to be perfectly invisible to the external incident wave. The
differences between line transformed cloaks and point transformed cloaks are
discussed. The fields in the cloak medium are found analytically to be related
to the fields in the original space via coordinate transformation functions. At
the exterior boundary of the cloak, it is shown that no reflection is excited
even though the permittivity and permeability do not always have a perfect
matched layer form. While at the inner boundary, no reflection is excited
either, and in particular no field can penetrate into the cloaked region.
However, for the inner boundary of any line transformed cloak, the permittivity
and permeability in a specific tangential direction are always required to be
infinitely large. Furthermore, the field discontinuity at the inner boundary
always exists; the surface current is induced to make this discontinuity
self-consistent. For a point transformed cloak, it does not experience such
problems. The tangential fields at the inner boundary are all zero, implying no
field discontinuity exists
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:22:43 GMT"
},
{
"version": "v2",
"created": "Thu, 1 May 2008 14:15:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Yan",
"Wei",
""
],
[
"Yan",
"Min",
""
],
[
"Ruan",
"Zhichao",
""
],
[
"Qiu",
"Min",
""
]
] | [
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] |
712.1695 | Michael Carley | Michael Carley | Evaluation of Biot-Savart integrals on tetrahedral meshes | null | null | null | null | math.NA math-ph math.MP | null | An arithmetically simple method has been developed for the evaluation of
Biot--Savart integrals on tetrahedralized distributions of vorticity. In place
of the usual approach of analytical formulae for the velocity induced by a
linear distribution of vorticity on a tetrahedron, the integration is performed
using Gaussian quadrature and a ray tracing technique from computer graphics.
This eliminates completely the need for the evaluation of square roots,
logarithms and arc tangents, and almost completely eliminates the requirement
for trigonometric functions, with no operation more costly than a division
required during the main calculation loop. An assessment of the algorithm's
performance is presented, demonstrating its accuracy, second order convergence
and near-linear speedup on parallel systems.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:23:58 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Carley",
"Michael",
""
]
] | [
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] |
712.1696 | Bolun Chen | Bo-Lun Chen, Xiao-Bin Huang, Su-Peng Kou and Yunbo Zhang | Mott-Hubbard Transition of Bosons in Optical Lattices with Three-body
Interactions | 7 pages, 4 figures; to be appear in Phys. Rev. A | null | 10.1103/PhysRevA.78.043603 | null | cond-mat.mes-hall cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, the quantum phase transition between superfluid state and
Mott-insulator state is studied based on an extended Bose-Hubbard model with
two- and three-body on-site interactions. By employing the mean-field
approximation we find the extension of the insulating 'lobes' and the existence
of a fixed point in three dimensional phase space. We investigate the link
between experimental parameters and theoretical variables. The possibility to
obverse our results through some experimental effects in optically trapped
Bose-Einstein Condensates(BEC) is also discussed.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:27:06 GMT"
},
{
"version": "v2",
"created": "Mon, 15 Sep 2008 13:18:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chen",
"Bo-Lun",
""
],
[
"Huang",
"Xiao-Bin",
""
],
[
"Kou",
"Su-Peng",
""
],
[
"Zhang",
"Yunbo",
""
]
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712.1697 | Isa M. Brand\~ao | I. M. Brand\~ao, M. S. Cunha and J. F. Gameiro | Bolometric Correction of the roAp star $\alpha$ Cir | 2 pages, 1 figure, poster proceeding - Vienna, 2007 - CP/AP Workshop | null | null | null | astro-ph | null | For the first time, the bolometric correction of $\alpha$ Cir was determined.
Two values, both based on an estimation of the total integrated flux, were
obtained. For that purpose spectroscopic and photometric data of $\alpha$ Cir
available in the literature was used. The values derived were then used to
place $\alpha$ Cir in the HR diagram.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:37:42 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Brandão",
"I. M.",
""
],
[
"Cunha",
"M. S.",
""
],
[
"Gameiro",
"J. F.",
""
]
] | [
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] |
712.1698 | Pierre Alquier | Pierre Alquier (PMA, Crest) | PAC-Bayesian Bounds for Randomized Empirical Risk Minimizers | null | Mathematical Methods of Statistics 17, 4 (2008) 279-304 | 10.3103/S1066530708040017 | null | stat.ML math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The aim of this paper is to generalize the PAC-Bayesian theorems proved by
Catoni in the classification setting to more general problems of statistical
inference. We show how to control the deviations of the risk of randomized
estimators. A particular attention is paid to randomized estimators drawn in a
small neighborhood of classical estimators, whose study leads to control the
risk of the latter. These results allow to bound the risk of very general
estimation procedures, as well as to perform model selection.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:40:41 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Nov 2008 10:37:52 GMT"
},
{
"version": "v3",
"created": "Fri, 9 Jan 2009 15:13:19 GMT"
}
] | 2009-01-09T00:00:00 | [
[
"Alquier",
"Pierre",
"",
"PMA, Crest"
]
] | [
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] |
712.1699 | Michael Carley | Michael Carley | Numerical quadratures for near-singular and near-hypersingular integrals
in boundary element methods | null | null | 10.3318/PRIA.2008.109.1.49 | null | math.NA math-ph math.MP | null | A method of deriving quadrature rules has been developed which gives nodes
and weights for a Gaussian-type rule which integrates functions of the form:
f(x,y,t) = a(x,y,t)/((x-t)^2+y^2) + b(x,y,t)/([(x-t)^2+y^2]^{1/2}) +
c(x,y,t)\log[(x-t)^2+y^2]^{1/2} + d(x,y,t), without having to explicitly
analyze the singularities of $f(x,y,t)$ or separate it into its components. The
method extends previous work on a similar technique for the evaluation of
Cauchy principal value or Hadamard finite part integrals, in the case when
$y\equiv0$. The method is tested by evaluating standard reference integrals and
its error is found to be comparable to machine precision in the best case.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:43:16 GMT"
}
] | 2010-09-21T00:00:00 | [
[
"Carley",
"Michael",
""
]
] | [
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] |
712.17 | Oleksandr Fialko | O. Fialko and K. Ziegler | Light Scattering on Random Dielectric Layers | 14 pages, 11 figures | Journal of Quantitative Spectroscopy & Radiative Transfer 109,
2329-2337 (2008) | 10.1016/j.jqsrt.2008.04.006 | null | physics.optics physics.gen-ph | null | Scattering of light by a random stack of dielectric layers represents a
one-dimensional scattering problem, where the scattered field is a
three-dimensional vector field. We investigate the dependence of the scattering
properties (band gaps and Anderson localization) on the wavelength, strength of
randomness and relative angle of the incident wave. There is a characteristic
angular dependence of Anderson localization for wavelengths close to the
thickness of the layers. In particular, the localization length varies
non-monotonously with the angle. In contrast to Anderson localization,
absorptive layers do not have this characteristic angular dependence.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:45:25 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Apr 2008 08:57:57 GMT"
}
] | 2010-03-10T00:00:00 | [
[
"Fialko",
"O.",
""
],
[
"Ziegler",
"K.",
""
]
] | [
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] |
712.1701 | Fr\'ed\'eric Paletou | L. Leger, F. Paletou (U. Toulouse/OMP, Laboratoire d'Astrophysique de
Toulouse-Tarbes, CNRS, France) | 2D radiative modelling of He I spectral lines formed in solar
prominences | 4 pages, 2 figures (to appear in the Procs. of Solar Polarization
Workshop #5, eds. Berdyugina, Nagendra and Ramelli), revised +2 citations,
better figures | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present preliminary results of 2D radiative modelling of He I lines in
solar prominences, using a new numerical code developed by us (Leger,
Chevallier and Paletou 2007). It treats self-consistently the radiation
transfer and the non-LTE statistical equilibrium of H and, in a second stage,
the one of He using a detailed atomic model. Preliminary comparisons with new
visible plus near-infrared observations made at high spectral resolution with
THeMIS are very satisfactory.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:55:43 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jul 2008 16:53:12 GMT"
}
] | 2008-07-11T00:00:00 | [
[
"Leger",
"L.",
"",
"U. Toulouse/OMP, Laboratoire d'Astrophysique de\n Toulouse-Tarbes, CNRS, France"
],
[
"Paletou",
"F.",
"",
"U. Toulouse/OMP, Laboratoire d'Astrophysique de\n Toulouse-Tarbes, CNRS, France"
]
] | [
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712.1702 | Diego Rubiera-Garcia | Joaquin Diaz-Alonso, Diego Rubiera-Garcia | Soliton solutions in relativistic field theories and gravitation | Latex, 4 pages, 1 figure. Talk given at 30th Spanish Relativity
Meeting (ERE 2007): Relativistic Astrophysics and Cosmology, Puerto de la
Cruz, Tenerife, Spain, 10-14 Sep 2007 | EAS Publ.Ser.30:183-196,2008 | 10.1051/eas:0830024 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report on some recent results on a class of relativistic lagrangian field
theories supporting non-topological soliton solutions and their applications in
the contexts of Gravitation and Cosmology. We analyze one and many-components
scalar fields and gauge fields.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:56:16 GMT"
},
{
"version": "v2",
"created": "Sat, 26 Mar 2011 04:34:27 GMT"
}
] | 2011-03-29T00:00:00 | [
[
"Diaz-Alonso",
"Joaquin",
""
],
[
"Rubiera-Garcia",
"Diego",
""
]
] | [
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] |
712.1703 | S. H. Curnoe | S. H. Curnoe | Structural distortion and the spin liquid state in Tb2Ti2O7 | 5 pages | Phys. Rev. B 78, 094418 (2008) | 10.1103/PhysRevB.78.094418 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | It is shown that a k=0, A_{2u} distortion of the terbium tetrahedral network
in Tb2Ti2O7 accounts for the apparent isolation of single tetrahedra as seen in
neutron scattering studies. Single tetrahedron collective spin states, rather
than individual spins, account for the main features of the spin liquid state,
namely, fluctuating local moments and the absence of long range order. Singlet
and doublet collective spin ground states are considered. An effective
interaction between tetrahedra on the fcc lattice is derived and found to be
weak and anisotropic.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:56:52 GMT"
},
{
"version": "v2",
"created": "Wed, 20 Aug 2008 16:01:02 GMT"
}
] | 2008-10-16T00:00:00 | [
[
"Curnoe",
"S. H.",
""
]
] | [
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712.1704 | Sergey Ganichev | V.V. Bel'kov, P. Olbrich, S.A. Tarasenko, D. Schuh, W. Wegscheider, T.
Korn, Ch. Sch\"uller, D. Weiss, W. Prettl, and S.D. Ganichev | Symmetry and spin dephasing in (110)-grown quantum wells | 4 pages, 4 figures | null | 10.1103/PhysRevLett.100.176806 | null | cond-mat.mes-hall | null | Symmetry and spin dephasing of in (110)-grown GaAs quantum wells (QWs) are
investigated applying magnetic field induced photogalvanic effect (MPGE) and
time-resolved Kerr rotation. We show that MPGE provides a tool to probe the
symmetry of (110)-grown quantum wells. The photocurrent is only observed for
asymmetric structures but vanishes for symmetric QWs. Applying Kerr rotation we
prove that in the latter case the spin relaxation time is maximal, therefore
these structures set upper limit of spin dephasing in GaAs QWs. We also
demonstrate that structure inversion asymmetry can be controllably tuned to
zero by variation of delta-doping layer position.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:12:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bel'kov",
"V. V.",
""
],
[
"Olbrich",
"P.",
""
],
[
"Tarasenko",
"S. A.",
""
],
[
"Schuh",
"D.",
""
],
[
"Wegscheider",
"W.",
""
],
[
"Korn",
"T.",
""
],
[
"Schüller",
"Ch.",
""
],
[
"Weiss",
"D.",
""
],
[
"Prettl",
"W.",
""
],
[
"Ganichev",
"S. D.",
""
]
] | [
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0.0516672395,
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0.025189044,
0.0070397877,
0.0369051695,
-0.0144208223,
-0.037941549,
0.032405775,
0.017542595,
-0.1180965453,
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] |
712.1705 | Ivan Shorubalko | I. Shorubalko, R. Leturcq, A. Pfund, D. Tyndall, R. Krischek, S.
Schon, and K. Ensslin | Self-aligned charge read-out for InAs nanowire quantum dots | 11 pages, 3 figures | Nanoletters 8, 382 (2008) | 10.1021/nl072522j | null | cond-mat.mes-hall | null | A highly sensitive charge detector is realized for a quantum dot in an InAs
nanowire. We have developed a self-aligned etching process to fabricate in a
single step a quantum point contact in a two-dimensional electron gas and a
quantum dot in an InAs nanowire. The quantum dot is strongly coupled to the
underlying point contact which is used as a charge detector. The addition of
one electron to the quantum dot leads to a change of the conductance of the
charge detector by typically 20%. The charge sensitivity of the detector is
used to measure Coulomb diamonds as well as charging events outside the dot.
Charge stability diagrams measured by transport through the quantum dot and
charge detection merge perfectly.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:14:24 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Mar 2008 17:20:21 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Shorubalko",
"I.",
""
],
[
"Leturcq",
"R.",
""
],
[
"Pfund",
"A.",
""
],
[
"Tyndall",
"D.",
""
],
[
"Krischek",
"R.",
""
],
[
"Schon",
"S.",
""
],
[
"Ensslin",
"K.",
""
]
] | [
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] |
712.1706 | Esmerindo Bernardes | Esmerindo Bernardes | A direct Numerov sixth order numerical scheme to accurately solve the
unidimensional Poisson equation with Dirichlet boundary conditions | 6 pages, 2 figures | null | null | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | In this article, we present an analytical direct method, based on a Numerov
three-point scheme, which is sixth order accurate and has a linear execution
time on the grid dimension, to solve the discrete one-dimensional Poisson
equation with Dirichlet boundary conditions. Our results should improve
numerical codes used mainly in self-consistent calculations in solid state
physics.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:25:13 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Bernardes",
"Esmerindo",
""
]
] | [
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] |
712.1707 | Alexei Glutsyuk | Alexey Glutsyuk, Christophe Sabot | Stokes matrices of hypergeometric integrals | 2 figures | null | null | null | math.DS math.CV | null | In this work we compute the Stokes matrices of the ordinary differential
equation satisfied by the hypergeometric integrals associated to an arrangement
of hyperplanes in generic position. This generalizes the computation done by
Ramis and Duval for confluent hypergeometric functions, which correspond to the
arrangement of two points on the line. The proof is based on an explicit
description of a base of canonical solutions as integrals on the cones of the
arrangement, and combinatorial relations between integrals on cones and on
domains.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:40:32 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Glutsyuk",
"Alexey",
""
],
[
"Sabot",
"Christophe",
""
]
] | [
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] |
712.1708 | Matthew Herndon | CDF Collaboration: T. Aaltonen, et al | Search for Bs --> mu+mu- and Bd --> mu+mu- Decays with 2fb-1 of ppbar
Collisions | Published in Phys. Rev. Lett | Phys.Rev.Lett.100:101802,2008 | 10.1103/PhysRevLett.100.101802 | FERMILAB-PUB-07-649-E | hep-ex | null | We have performed a search for Bs-->mu+mu- and Bd-->mu+mu- decays in ppbar
collisions at sqrt(s) = 1.96TeV using 2fb-1 of integrated luminosity collected
by the CDF II detector at the Fermilab Tevatron Collider. The observed number
of Bs and Bd candidates is consistent with background expectations. The
resulting upper limits on the branching fractions are B(Bs-->mu+mu-) <
5.8X10^-8 and B(Bd-->mu+mu-) < 1.8X10^-8 at 95% C.L.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 19:51:08 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Mar 2008 20:46:00 GMT"
}
] | 2010-05-12T00:00:00 | [
[
"CDF Collaboration",
"",
""
],
[
"Aaltonen",
"T.",
""
]
] | [
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] |
712.1709 | Alexander Gaifullin | A. A. Gaifullin | Explicit construction of manifolds realizing the prescribed homology
classes | 3 pages | null | null | null | math.GT math.CO | null | We consider a classical N. Steenrod's problem on realization of homology
classes by images of the fundamental classes of manifolds. It is well-known
that each integral homology class can be realized with some multiplicity as an
image of the fundamental class of a manifold. Our main result is an explicit
purely combinatorial construction that for a given integral cycle provides a
combinatorial manifold realizing a multiple of the homology class of this
cycle. The construction is based on a local procedure for resolving
singularities of a pseudo-manifold. We give an application of our result to the
problem of constructing a combinatorial manifold with the prescribed set of
links of vertices.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:45:47 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Gaifullin",
"A. A.",
""
]
] | [
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712.171 | Gianluca Geloni | Gianluca Geloni, Evgeni Saldin, Evgeni Schneidmiller and Mikhail
Yurkov | A simple method for timing an XFEL source to high-power lasers | Version 2: Reference list updated; submitted for publication. 21
pages, 8 figures | null | 10.1016/j.optcom.2008.03.023 | DESY 07-221 | physics.acc-ph physics.optics | null | We propose a technique, to be used for time-resolved pump-probe experiments,
for timing an x-ray free electron laser (XFEL) to a high-power conventional
laser with femtosecond accuracy. Our method takes advantage of the same
electron bunch to produce both an XFEL pulse and an ultrashort optical pulse
with the help of an optical radiator downstream of the x-ray undulator. Since
both pulses are produced by the same electron bunch, they are perfectly
synchronized. Application of cross-correlation techniques will allow to
determine relative jitter between the optical pulse (and, thus, the XFEL pulse)
and a pulse from an external pump-laser with femtosecond resolution. Technical
realization of the proposed timing scheme uses an optical replica synthesizer
(ORS) setup to be installed after the final bunch-compression stage of the
XFEL. The electron bunch is modulated in the ORS setup by an external optical
laser. Subsequently, it travels through the main undulator, and produces the
XFEL pulse. Finally, a powerful optical pulse of coherent edge radiation is
generated as the bunch passes through a long straight section and a separation
magnet downstream of the main undulator. Our study shows that at a moderate
(about 10%) density modulation of the electron bunch at the location of the
optical radiator allows production of high power x-ray and optical pulses.
Relative synchronization of these pulses is preserved by using the same
mechanical support for both x-ray and optical elements transporting radiation
down to the experimental area, where single-shot cross-correlation between
optical pulse and pump-laser pulse is performed. We illustrate the potential of
the proposed timing technique with numerical examples referring to the European
XFEL facility.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:45:52 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 12:06:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Geloni",
"Gianluca",
""
],
[
"Saldin",
"Evgeni",
""
],
[
"Schneidmiller",
"Evgeni",
""
],
[
"Yurkov",
"Mikhail",
""
]
] | [
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] |
712.1711 | D. P. Roy | M. Hirsch, D. P. Roy and J. W. F. Valle | Probing a Supersymmetric Model for Neutrino Masses at Ultrahigh Energy
Neutrino Telescopes | 11 pages pdf including 2 figures. Discussion added. Final version to
appear in Physics Letters B | Phys.Lett.B662:185-189,2008 | 10.1016/j.physletb.2008.02.065 | IFIC/07-76 | hep-ph | null | A bilinear R-Parity breaking SUSY model for neutrino mass and mixing predicts
the lightest superparticle to decay mainly into a pair of tau leptons or b
quarks along with a neutrino for relatively light SUSY spectra. This leads to a
distinctive triple bang signature of SUSY events at ultrahigh energy neutrino
telescopes like IceCube or Antares. While the expected signal size is only
marginal at IceCube, it will be promising for a future multi-km^3 size neutrino
telescope.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:47:13 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Feb 2008 16:17:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hirsch",
"M.",
""
],
[
"Roy",
"D. P.",
""
],
[
"Valle",
"J. W. F.",
""
]
] | [
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712.1712 | Ting Li | Ting Li | The \'Etale Homology and The Cycle Maps in Adic Coefficients | 17 pages | null | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this article, we define the l-adic homology for a morphism of schemes
satisfying certain finiteness conditions. This homology has these functors
similar to the Chow groups: proper push-forward, flat pull-back, base change,
cap-product, etc. In particular on singular varieties, this kind of l-adic
homology behaves much better that the classical l-adic cohomology. As an
application, we give an much easier approach to construct the cycle maps for
arbitrary algebraic schemes over fields of finite cohomology dimension. And we
prove these cycle maps kill the algebraic equivalences and commute with the
Chern action of locally free sheaves.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:52:52 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Feb 2008 14:39:01 GMT"
},
{
"version": "v3",
"created": "Thu, 23 Oct 2008 12:40:04 GMT"
}
] | 2008-10-23T00:00:00 | [
[
"Li",
"Ting",
""
]
] | [
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712.1713 | Grigoris Panotopoulos | Grigoris Panotopoulos | Detectable primordial non-gaussianities and gravitational waves in
k-inflation | 4 pages, 1 figure, REVTEX, to appear in PRD | Phys.Rev.D76:127302,2007 | 10.1103/PhysRevD.76.127302 | null | astro-ph | null | An inflationary single field model with a non-trivial kinetic term for the
inflaton is discussed. It is shown that it is possible to have large primordial
non-gaussianities and large tensor-to-scalar ratio in a simple concrete model
with just a scalar field and a generalized kinetic term for the inflaton field.
This is potentially interesting in the prospect of new forthcoming
observations.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:54:01 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Panotopoulos",
"Grigoris",
""
]
] | [
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] |
712.1714 | Dinh-V.-Trung | Dinh-V-Trung, Jeremy Lim | Molecular shells in IRC+10216: Evidence for non-isotropic and episodic
mass loss enhancement | 16 pages, 5 figures, accepted for publication in ApJ | null | 10.1086/527669 | null | astro-ph | null | We report high angular-resolution VLA observations of cyanopolyyne molecules
HC$_3$N and HC$_5$N from the carbon rich circumstellar envelope of IRC+10216.
The observed low-lying rotational transitions trace a much more extended
emitting region than seen in previous observations at higher frequency
transitions. We resolve the hollow quasi-spherical distribution of the
molecular emissions into a number of clumpy shells. These molecular shells
coincide spatially with dust arcs seen in deep optical images of the IRC+10216
envelope, allowing us to study for the first time the kinematics of these
features. We find that the molecular and dust shells represent the same density
enhancements in the envelope separated in time by $\sim$120 to $\sim$360 yrs.
From the angular size and velocity spread of the shells, we estimate that each
shell typically covers about 10% of the stellar surface at the time of
ejection. The distribution of the shells seems to be random in space. The good
spatial correspondance between HC$_3$N and HC$_5$N emissions is in qualitative
agreement with a recent chemical model that takes into account the presence of
density-enhanced shells. The broad spatial distribution of the cyanopolyyne
molecules, however, would necessitate further study on their formation.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 13:57:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dinh-V-Trung",
"",
""
],
[
"Lim",
"Jeremy",
""
]
] | [
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] |
712.1715 | Luigi Coraggio | A. Covello, L. Coraggio, A. Gargano, and N.Itaco | Shell-model structure of exotic nuclei beyond 132Sn | 4 pages, 1 figure, 2 tables, talk given at 7th International
Conference on Radioactive Nuclear Beams, Cortina d'Ampezzo (Italy), July 3-7
2006 | Eur.Phys.J.ST149:93-96,2007 | 10.1140/epjst/e2007-00275-7 | null | nucl-th | null | We report on a study of exotic nuclei around doubly magic 132Sn in terms of
the shell model employing a realistic effective interaction derived from the
CD-Bonn nucleon-nucleon potential. The short-range repulsion of the bare
potential is renormalized by constructing a smooth low-momentum potential,
V-low-k, that is used directly as input for the calculation of the effective
interaction. In this paper we focus attention on the nuclei 134Sn and 135Sb
which, with an N/Z ratio of 1.68 and 1.65, respectively, are at present the
most exotic nuclei beyond 132Sn for which information exists on excited states.
Comparison shows that the calculated results for both nuclei are in very good
agreement with the experimental data. We present our predictions of the
hitherto unknown spectrum of 136Sn.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:03:39 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 14:12:50 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Covello",
"A.",
""
],
[
"Coraggio",
"L.",
""
],
[
"Gargano",
"A.",
""
],
[
"Itaco",
"N.",
""
]
] | [
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] |
712.1716 | Jan Steinhoff | Jan Steinhoff, Steven Hergt, Gerhard Sch\"afer | The next-to-leading order gravitational spin(1)-spin(2) dynamics in
Hamiltonian form | REVTeX4, 5 pages, published version | Phys.Rev.D77:081501,2008 | 10.1103/PhysRevD.77.081501 | null | gr-qc astro-ph.HE | null | Based on recent developments by the authors a next-to-leading order
spin(1)-spin(2) Hamiltonian is derived for the first time. The result is
obtained within the canonical formalism of Arnowitt, Deser, and Misner (ADM)
utilizing their generalized isotropic coordinates. A comparison with other
methods is given.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:06:14 GMT"
},
{
"version": "v2",
"created": "Tue, 20 May 2008 18:16:45 GMT"
}
] | 2010-02-16T00:00:00 | [
[
"Steinhoff",
"Jan",
""
],
[
"Hergt",
"Steven",
""
],
[
"Schäfer",
"Gerhard",
""
]
] | [
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712.1717 | Cyril Malyshev | C. Malyshev | The Einsteinian T(3)-Gauge Approach and the Stress Tensor of the Screw
Dislocation in the Second Order: Avoiding the Cut-off at the Core | 34 pages, LaTeX | J.Phys.A.40:10657-10684,2007 | 10.1088/1751-8113/40/34/019 | null | cond-mat.mtrl-sci astro-ph gr-qc | null | A translational gauge approach of the Einstein type is proposed for obtaining
the stresses that are due to non-singular screw dislocation. The stress
distribution of second order around the screw dislocation is classically known
for the hollow circular cylinder with traction-free external and internal
boundaries. The inner boundary surrounds the dislocation's core, which is not
captured by the conventional solution. The present gauge approach enables us to
continue the classically known quadratic stresses inside the core. The gauge
equation is chosen in the Hilbert--Einstein form, and it plays the role of
non-conventional incompatibility law. The stress function method is used, and
it leads to the modified stress potential given by two constituents: the
conventional one, say, the `background' and a short-ranged gauge contribution.
The latter just causes additional stresses, which are localized. The asymptotic
properties of the resulting stresses are studied. Since the gauge contributions
are short-ranged, the background stress field dominates sufficiently far from
the core. The outer cylinder's boundary is traction-free. At sufficiently
moderate distances, the second order stresses acquire regular continuation
within the core region, and the cut-off at the core does not occur. Expressions
for the asymptotically far stresses provide self-consistently new length scales
dependent on the elastic parameters. These lengths could characterize an
exteriority of the dislocation core region.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:45:38 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Malyshev",
"C.",
""
]
] | [
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712.1718 | George Bogoslovsky | George Bogoslovsky | Rapidities and Observable 3-Velocities in the Flat Finslerian Event
Space with Entirely Broken 3D Isotropy | This is a contribution to the Proc. of the Seventh International
Conference ''Symmetry in Nonlinear Mathematical Physics'' (June 24-30, 2007,
Kyiv, Ukraine), published in SIGMA (Symmetry, Integrability and Geometry:
Methods and Applications) at http://www.emis.de/journals/SIGMA/ | SIGMA 4 (2008), 045, 21 pages | 10.3842/SIGMA.2008.045 | null | hep-th | null | We study the geometric phase transitions that accompany the dynamic
rearrangement of vacuum under spontaneous violation of initial gauge symmetry.
The rearrangement may give rise to condensates of three types, namely the
scalar, axially symmetric, and entirely anisotropic condensates. The flat
space-time keeps being the Minkowski space in the only case of scalar
condensate. The anisotropic condensate having arisen, the respective anisotropy
occurs also in space-time. In this case the space-time filled with axially
symmetric condensate proves to be a flat relativistically invariant Finslerian
space with partially broken 3D isotropy, while the space-time filled with
entirely anisotropic condensate proves to be a flat relativistically invariant
Finslerian space with entirely broken 3D isotropy. The two Finslerian space
types are described briefly in the extended introduction to the work, while the
original part of the latter is devoted to determining observable 3-velocities
in the entirely anisotropic Finslerian event space. The main difficulties that
are overcome in solving that problem arose from the nonstandard form of the
light cone equation and from the necessity of correct introducing of a norm in
the linear vector space of rapidities.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:33:39 GMT"
},
{
"version": "v2",
"created": "Mon, 26 May 2008 05:19:19 GMT"
}
] | 2008-05-26T00:00:00 | [
[
"Bogoslovsky",
"George",
""
]
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] |
712.1719 | Sebastian Burciu M | S. Burciu | Coset decomposition for semisimple Hopf algebras | 15 pages | null | null | null | math.RA | null | The notion of double coset for semisimple finite dimensional Hopf algebras is
introduced. This is done by considering an equivalence relation on the set of
irreducible characters of the dual Hopf algebra. As an application formulae for
the restriction of the irreducible characters to normal Hopf subalgebras are
given.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:41:20 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Burciu",
"S.",
""
]
] | [
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] |
712.172 | Thanos Manos | T. Manos, Ch. Skokos and T. Bountis | Application of the Generalized Alignment Index (GALI) method to the
dynamics of multi--dimensional symplectic maps | 8 pages, 4 figures, to appear in the proceedings of the international
conference "Chaos, Complexity and Transport: Theory and Applications",
Marseille, France. (Minor typographical errors corrected) | null | 10.1142/9789812818805_0028 | null | nlin.CD | null | We study the phase space dynamics of multi--dimensional symplectic maps,
using the method of the Generalized Alignment Index (GALI). In particular, we
investigate the behavior of the GALI for a system of N=3 coupled standard maps
and show that it provides an efficient criterion for rapidly distinguishing
between regular and chaotic motion.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:01:12 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 11:26:54 GMT"
}
] | 2016-11-23T00:00:00 | [
[
"Manos",
"T.",
""
],
[
"Skokos",
"Ch.",
""
],
[
"Bountis",
"T.",
""
]
] | [
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712.1721 | Stepanyantz Konstantin | A.B.Pimenov, E.S.Shevtsova, A.A.Soloshenko, K.V.Stepanyantz | Higher derivative regularization and quantum corrections in N=1
supersymmetric theories | 39 pages, 13 figures, 5 references added | null | null | null | hep-th | null | We review some results of applying the higher covariant derivative
regularization to the investigation of quantum corrections structure in N=1
supersymmetric theories. In particular, we demonstrate that all integrals,
defining the Gell-Mann--Low function in supersymmetric theories, are integrals
of total derivatives. As a consequence, there is an identity for Green
functions, which does not follow from any known symmetry of the theory, in N=1
supersymmetric theories. We also discuss how to derive the exact
$\beta$-function by methods of the perturbation theory.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:53:11 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 09:55:33 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Pimenov",
"A. B.",
""
],
[
"Shevtsova",
"E. S.",
""
],
[
"Soloshenko",
"A. A.",
""
],
[
"Stepanyantz",
"K. V.",
""
]
] | [
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] |
712.1722 | Gregory Conner | G. Conner (BYU), M. Meilstrup (BYU), D. Repov\v{s} (Ljubljana), A.
Zastrow (Gdansk), and M. \v{Z}eljko (Ljubljana) | On small homotopies of loops | 12 pages, 5 figures | Topol. Appl. 155:10 (2008), 1089-1097 | 10.1016/j.topol.2008.01.009 | null | math.GT math.AT math.GR | null | Two natural questions are answered in the negative:
(1) If a space has the property that small nulhomotopic loops bound small
nulhomotopies, then are loops which are limits of nulhomotopic loops themselves
nulhomotopic?
(2) Can adding arcs to a space cause an essential curve to become
nulhomotopic?
The answer to the first question clarifies the relationship between the
notions of a space being homotopically Hausdorff and $\pi_1$-shape injective.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 14:58:24 GMT"
}
] | 2008-04-27T00:00:00 | [
[
"Conner",
"G.",
"",
"BYU"
],
[
"Meilstrup",
"M.",
"",
"BYU"
],
[
"Repovš",
"D.",
"",
"Ljubljana"
],
[
"Zastrow",
"A.",
"",
"Gdansk"
],
[
"Željko",
"M.",
"",
"Ljubljana"
]
] | [
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712.1723 | Adolfo Paolo Masucci apm | C. Bedogn\'e, A.P. Masucci, G.J. Rodgers | Diophantine Networks | null | Physica A vol.387, 2161 (2008). | 10.1016/j.physa.2007.11.038 | null | physics.soc-ph cond-mat.dis-nn physics.data-an | null | We introduce a new class of deterministic networks by associating networks
with Diophantine equations, thus relating network topology to algebraic
properties. The network is formed by representing integers as vertices and by
drawing cliques between M vertices every time that M distinct integers satisfy
the equation. We analyse the network generated by the Pythagorean equation
$x^{2}+y^{2}= z^{2}$ showing that its degree distribution is well approximated
by a power law with exponential cut-off. We also show that the properties of
this network differ considerably from the features of scale-free networks
generated through preferential attachment. Remarkably we also recover a power
law for the clustering coefficient.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 12:19:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bedogné",
"C.",
""
],
[
"Masucci",
"A. P.",
""
],
[
"Rodgers",
"G. J.",
""
]
] | [
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] |
712.1724 | Krzysztof Kowalski | K. Kowalski and J. Rembielinski | Coherent states for the quantum mechanics on a torus | 2 eps figures | K. Kowalski and J. Rembielinski, Phys. Rev. A, 75 (2007)
052102-1--052102-7 | 10.1103/PhysRevA.75.052102 | null | quant-ph | null | The coherent states for the quantum mechanics on a torus and their basic
properties are discussed.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:16:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kowalski",
"K.",
""
],
[
"Rembielinski",
"J.",
""
]
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] |
712.1725 | Paul Levy | Paul Levy | Vinberg's \theta-groups in positive characteristic and
Kostant-Weierstrass slices | 36 pages. Some proofs improved, one or two references added | null | null | null | math.AG | null | We generalize the basic results of Vinberg's \theta-groups, or periodically
graded reductive Lie algebras, to fields of good positive characteristic. To
this end we clarify the relationship between the little Weyl group and the
(standard) Weyl group. We deduce that the ring of invariants associated to the
grading is a polynomial ring. This approach allows us to prove the existence of
a KW-section for a classical graded Lie algebra (in zero or good
characteristic), confirming a conjecture of Popov in this case.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:16:33 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 17:22:47 GMT"
},
{
"version": "v3",
"created": "Tue, 15 Apr 2008 15:09:15 GMT"
}
] | 2008-04-15T00:00:00 | [
[
"Levy",
"Paul",
""
]
] | [
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] |
712.1726 | Marcel Mudrich Dr. | M. Mudrich, G. Droppelmann, P. Claas, C. P. Schulz, F. Stienkemeier | Quantum interference spectroscopy of RbHe exciplexes formed on helium
nanodroplets | null | Phys. Rev. Lett. 100, 023401 (2008) | 10.1103/PhysRevLett.100.023401 | null | physics.atom-ph physics.atm-clus | null | Femtosecond multiphoton pump-probe photoionization is applied to helium
nanodroplets doped with rubidium (Rb). The yield of Rb+ ions features
pronounced quantum interference (QI) fringes demonstrating the coherence of a
superposition of electronic states on a time scale of tens of picoseconds.
Furthermore, we observe QI in the yield of formed RbHe exciplex molecules. The
quantum interferogram allows to determine the vibrational structure of these
unstable molecules. From a sliced Fourier analysis one can not only extract the
population dynamics of vibrational states but also follow their energetic
evolution during the RbHe formation.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:08:59 GMT"
}
] | 2011-12-19T00:00:00 | [
[
"Mudrich",
"M.",
""
],
[
"Droppelmann",
"G.",
""
],
[
"Claas",
"P.",
""
],
[
"Schulz",
"C. P.",
""
],
[
"Stienkemeier",
"F.",
""
]
] | [
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] |
712.1727 | Sergey Sushkov | Sergey V. Sushkov and Yuan-Zhong Zhang | Scalar wormholes in cosmological setting and their instability | REVTeX4, 11 pages, submitted to PRD | Phys.Rev.D77:024042,2008 | 10.1103/PhysRevD.77.024042 | null | gr-qc | null | We construct exact nonstatic nonhomogeneous spherically symmetric solutions
in the theory of gravity with a scalar field possessing the exponential
potential. The solution of particular interest corresponds to the scalar field
with negative kinetic energy, i.e. a ghost, and represents two asymptotically
homogeneous spatially flat universes connected by a throat. We interpret this
solution as a wormhole in cosmological setting. Both the universes and the
wormhole throat are simultaneously expanding with acceleration. The character
of expansion qualitatively depends on the wormhole's mass $m$. For $m=0$ the
expansion goes exponentially, so that the corresponding spacetime configuration
represents two de Sitter universes joining by the throat. For $m>0$ the
expansion has the power character, so that one has the inflating wormhole
connecting two homogeneous spatially flat universes expanding according to the
power law into the final singularity. The stability analysis of the non-static
wormholes reveals their instability against linear spherically symmetric
perturbations.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:09:45 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Sushkov",
"Sergey V.",
""
],
[
"Zhang",
"Yuan-Zhong",
""
]
] | [
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] |
712.1728 | Boris Kerner | Boris S. Kerner | Features of Traffic Congestion caused by bad Weather Conditions or
Accident | null | null | null | null | physics.soc-ph | null | Spatiotemporal features and physics of vehicular traffic congestion occurring
due to heavy freeway bottlenecks caused by bad weather conditions or accidents
are found based on simulations in the framework of three-phase traffic theory.
A model of a heavy bottleneck is presented. Under a continuous non-limited
increase in bottleneck strength, i.e., when the average flow rate within a
congested pattern allowed by the heavy bottleneck decreases continuously up to
zero, the evolution of the traffic phases in congested traffic, synchronized
flow and wide moving jams, is studied.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:49:26 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Kerner",
"Boris S.",
""
]
] | [
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] |
712.1729 | Tadafumi Ohsaku | Tadafumi Ohsaku | Dynamical Symmetry Breaking of a Relativistic Model in
Quasi-(1+1)-Dimensions. I. Formulation | 16 pages | null | null | null | cond-mat.supr-con cond-mat.mes-hall cond-mat.mtrl-sci cond-mat.str-el hep-ph | null | The dynamical symmetry breaking in a quasi-(1+1)-dimensional relativistic
model is investigated. The motions of particles in intrachain are described as
a relativistic electron-hole gas, while the interchain hopping term is
introduced as a 0th-component of vector in (1+1)-dimensions, a kind of chemical
potential of the system. The gauge symmetry of the model is chosen as U(1)
suitable for a possible situation of a real substance in condensed matter
physics. We consider the BCS-type contact interactions for the s-wave
fermion-pair condensates, while employ the nonlocal interactions of the
generalized BCS framework to generate the $p$-, $d$- and $f$-wave condensations
in the system. Especially we examine the dynamical generation of a Dirac mass
term and superconductivity in the model. The phenomenon is interpreted as
metal-insulator/metal-superconductor phase transitions.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:10:45 GMT"
}
] | 2016-09-08T00:00:00 | [
[
"Ohsaku",
"Tadafumi",
""
]
] | [
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] |
712.173 | Jordi Boronat | I. Beslic, L. Vranjes Markic, and J. Boronat | Quantum Monte Carlo study of small pure and mixed spin-polarized tritium
clusters | 12 pages, 5 figures, accepted for publication in J. Chem. Phys | null | 10.1063/1.2827119 | null | cond-mat.other | null | We have investigated the stability limits of small spin-polarized clusters
consisting of up to ten spin-polarized tritium T$\downarrow$ atoms and the
mixtures of T$\downarrow$ with spin-polarized deuterium D$\downarrow$ and
hydrogen H$\downarrow$ atoms. All of our calculations have been performed using
the variational and diffusion Monte Carlo methods. For clusters with
D$\downarrow$ atoms, the released node procedure is used in cases where the
wave function has nodes. In addition to the energy, we have also calculated the
structure of small clusters using unbiased estimators. Results obtained for
pure T$\downarrow$ clusters are in good accordance with previous calculations,
confirming that the trimer is the smallest spin-polarized tritium cluster. Our
results show that mixed T$\downarrow$-H$\downarrow$ clusters having up to ten
atoms are unstable and that it takes at least three tritium atoms to bind one,
two or three D$\downarrow$ atoms. Among all the considered clusters, we have
found no other Borromean states except the ground state of the T$\downarrow$
trimer.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:14:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Beslic",
"I.",
""
],
[
"Markic",
"L. Vranjes",
""
],
[
"Boronat",
"J.",
""
]
] | [
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] |
712.1731 | James McLaughlin | J. A. McLaughlin, J. S. L. Ferguson, A. W. Hood | 3D MHD Coronal Oscillations About a Magnetic Null Point: Application of
WKB Theory | 26 pages, 12 figures | null | 10.1007/s11207-007-9107-2 | null | astro-ph | null | This paper is a demonstration of how the WKB approximation can be used to
help solve the linearised 3D MHD equations. Using Charpit's Method and a
Runge-Kutta numerical scheme, we have demonstrated this technique for a
potential 3D magnetic null point, ${\bf{B}}=(x,\epsilon y -(\epsilon +1)z)$.
Under our cold plasma assumption, we have considered two types of wave
propagation: fast magnetoacoustic and Alfv\'en waves. We find that the fast
magnetoacoustic wave experiences refraction towards the magnetic null point,
and that the effect of this refraction depends upon the Alfv\'en speed profile.
The wave, and thus the wave energy, accumulates at the null point. We have
found that current build up is exponential and the exponent is dependent upon
$\epsilon$. Thus, for the fast wave there is preferential heating at the null
point. For the Alfv\'en wave, we find that the wave propagates along the
fieldlines. For an Alfv\'en wave generated along the fan-plane, the wave
accumulates along the spine. For an Alfv\'en wave generated across the spine,
the value of $\epsilon$ determines where the wave accumulation will occur:
fan-plane ($\epsilon=1$), along the $x-$axis ($0<\epsilon <1$) or along the
$y-$axis ($\epsilon>1$). We have shown analytically that currents build up
exponentially, leading to preferential heating in these areas. The work
described here highlights the importance of understanding the magnetic topology
of the coronal magnetic field for the location of wave heating.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:14:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"McLaughlin",
"J. A.",
""
],
[
"Ferguson",
"J. S. L.",
""
],
[
"Hood",
"A. W.",
""
]
] | [
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] |
712.1732 | B. P. Datta | B. P. Datta | The Theory of Uncertainty for Derived Results: Properties of Equations
Representing Physicochemical Evaluation Systems | 39 pages (Edited version [no. 3] With clarifying appendix no. 1 on
notations): however, wrong file got uploaded yesterday | null | null | null | physics.data-an physics.chem-ph physics.comp-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Any physiochemical variable (Ym) is always determined from certain measured
variables {Xi}. The uncertainties {ui} of measuring {Xi} are generally a priori
ensured as acceptable. However, there is no general method for assessing
uncertainty (em) in the desired Ym, i.e. irrespective of whatever might be its
system-specific-relationship (SSR) with {Xi}, and/ or be the causes of {ui}. We
here therefore study the behaviors of different typical SSRs. The study shows
that any SSR is characterized by a set of parameters, which govern em. That is,
em is shown to represent a net SSR-driven (purely systematic) change in ui(s);
and it cannot vary for whether ui(s) be caused by either or both statistical
and systematic reasons. We thus present the general relationship of em with
ui(s), and discuss how it can be used to predict a priori the requirements for
an evaluated Ym to be representative, and hence to set the guidelines for
designing experiments and also really appropriate evaluation models. Say: Y_m=
f_m ({X_i}_(i=1)^N), then, although: e_m= g_m ({u_i}_(i=1)^N), "N" is not a key
factor in governing em. However, simply for varying "fm", the em is
demonstrated to be either equaling a ui, or >ui, or even <ui. Further, the
limiting error (d_m^(Lim.)) in determining an Ym is also shown to be decided by
"fm" (SSR). Thus, all SSRs are classified into two groups: (I) the SSRs that
can never lead "d_m^(Lim.)" to be zero; and (II) the SSRs that enable
"d_m^(Lim.)" to be zero. In fact, the theoretical-tool (SSR) is by pros and
cons no different from any discrete experimental-means of a study, and has
resemblance with chemical reactions as well.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:43:34 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Jan 2011 08:08:42 GMT"
},
{
"version": "v3",
"created": "Wed, 19 Oct 2011 11:41:58 GMT"
},
{
"version": "v4",
"created": "Thu, 20 Oct 2011 06:57:18 GMT"
}
] | 2011-10-21T00:00:00 | [
[
"Datta",
"B. P.",
""
]
] | [
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] |
712.1733 | Hua Xu | Hua Xu, Liangbing Hu, Shixiong Zhang, George Gruner and Steven M.
Anlage | Frequency- and electric-field-dependent conductivity of single-walled
carbon nanotube networks of varying density | 7 pages and 6 figures | Physical Review B 77, 075418 (2008) | 10.1103/PhysRevB.77.075418 | null | cond-mat.mtrl-sci cond-mat.dis-nn | null | We present measurements of the frequency and electric field dependent
conductivity of single walled carbon nanotube(SWCNT) networks of various
densities. The ac conductivity as a function of frequency is consistent with
the extended pair approximation model and increases with frequency above an
onset frequency $\omega_0$ which varies over seven decades with a range of film
thickness from sub-monolayer to 200 nm. The nonlinear electric field-dependent
DC conductivity shows strong dependence on film thickness as well. Measurement
of the electric field dependence of the resistance R(E) allows for the
determination of a length scale $L_{E}$ possibly characterizing the distance
between tube contacts, which is found to systematically decrease with
increasing film thickness. The onset frequency $\omega_0$ of ac conductivity
and the length scale $L_{E}$ of SWCNT networks are found to be correlated, and
a physically reasonable empirical formula relating them has been proposed. Such
studies will help the understanding of transport properties and benefit the
applications of this material system.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:22:21 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 16:00:17 GMT"
},
{
"version": "v3",
"created": "Fri, 22 Feb 2008 19:41:45 GMT"
}
] | 2008-02-22T00:00:00 | [
[
"Xu",
"Hua",
""
],
[
"Hu",
"Liangbing",
""
],
[
"Zhang",
"Shixiong",
""
],
[
"Gruner",
"George",
""
],
[
"Anlage",
"Steven M.",
""
]
] | [
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] |
712.1734 | Pelaez | J.R. Pelaez, C. Hanhart, G. Rios | Chiral Extrapolation of light resonances from Unitarized Chiral
Perturbation Theory | To appear in the proceedings of the XII Int. Conf. on Hadron
Spectroscopy. HADRON07. Frascati, October, 2007. 8 pages, 3 figures.
References added and updated, typos corrected | null | null | null | hep-ph hep-lat nucl-th | null | Both scalar and vector light resonances can be generated from the
unitarization of one-loop chiral perturbation theory. This amounts to using in
a dispersion relation the chiral expansion, which incorporates the correct QCD
quark mass dependence. We can thus predict the quark mass dependence of the
poles associated to those light resonances. Our results compare well with some
recent lattice results for the rho(770) mass and can be used as a benchmark for
future lattice results on the rho(770) or the f0(600) also known as the sigma.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:22:43 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 09:27:33 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Pelaez",
"J. R.",
""
],
[
"Hanhart",
"C.",
""
],
[
"Rios",
"G.",
""
]
] | [
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] |
712.1735 | Daniel Sanchez-Portal | Sampsa Riikonen and Daniel Sanchez-Portal | Systematic investigation of the structure of the Si(553)-Au surface from
first principles | Submitted to Phys. Rev. B on December 10, 2007 | null | 10.1103/PhysRevB.77.165418 | null | cond-mat.mtrl-sci | null | We present here a comprehensive search for the structure of the Si(553)-Au
reconstruction. More than two hundred different trial structures have been
studied using first-principles density-functional calculations with the SIESTA
code. An iterative procedure, with a step-by-step increase of the accuracy and
computational cost of the calculations, was used to allow for the study of this
large number of configurations. We have considered reconstructions restricted
to the topmost bilayer and studied two types: i) "flat" surface-bilayer models,
where atoms at the topmost bilayer present different coordinations and
registries with the underlying bulk, and ii) nine different models based on the
substitution of a silicon atom by a gold atom in different positions of a
$\pi$-bonded chain reconstruction of the Si(553) surface. We have developed a
compact notation that allows us to label and identify all these structures.
This is very useful for the automatic generation of trial geometries and
counting the number of inequivalent structures, i.e., structures having
different bonding topologies. The most stable models are those that exhibit a
honeycomb-chain structure at the step edge. One of our models (model f2)
reproduces the main features of the room temperature photoemission and
scanning-tunneling microscopy data. Thus we conclude that f2 structure is a
good candidate for the high temperature structure of the Si(553)-Au surface.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 19:10:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Riikonen",
"Sampsa",
""
],
[
"Sanchez-Portal",
"Daniel",
""
]
] | [
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-0.0253174007,
-0.0870134458,
0.0545806997,
0.0126014203,
0.0678185523,
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] |
712.1736 | Bartlomiej Szafran | S.Bednarek, K.Lis, B.Szafran | Quantum dot defined in two-dimensional electron gas at n-AlGaAs/GaAs
heterojunction: simulation of electrostatic potential and charging properties | null | Phys. Rev. B 77, 115320 (2008) | 10.1103/PhysRevB.77.115320 | null | cond-mat.mes-hall | null | We present a self-consistent Schroedinger-Poisson scheme for simulation of
electrostatic quantum dots defined in gated two-dimensional electron gas formed
at n-AlGaAs/GaAs heterojunction. The computational method is applied to a
quantitative description of transport properties studied experimentally by
Elzermann et al. [Appl. Phys. Lett. {\bf 84}, 4617 (2004)]. The
three-dimensional model describes the electrostatics of the entire device with
a quantum dot that changes shape and floats inside a gated region when the
applied voltages are varied. Our approach accounts for the metal electrodes of
arbitrary geometry and configuration, includes magnetic field applied
perpendicular to the growth direction, electron-electron correlation in the
confined electron system and its interaction with the electron reservoir
surrounding the quantum dot. We calculate the electric field, the space charge
distribution as well as energies and wave functions of confined electrons to
describe opening of two transport channels between the reservoir and the
confined charge puddle. We determine the voltages for charging the dot with up
to 4 electrons.
The results are in a qualitative and quantitative agreement with the
experimental data.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:27:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bednarek",
"S.",
""
],
[
"Lis",
"K.",
""
],
[
"Szafran",
"B.",
""
]
] | [
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] |
712.1737 | Andrii Neronov | A.Neronov, D.Semikoz, I.Tkachev | Ultra-High Energy Cosmic Ray production in the polar cap regions of
black hole magnetospheres | null | New Journal of Physics 11, 065015 (2009) | 10.1088/1367-2630/11/6/065015 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We develop a model of ultra-high energy cosmic ray (UHECR) production via
acceleration in a rotation-induced electric field in vacuum gaps in the
magnetospheres of supermassive black holes (BH). We show that if the poloidal
magnetic field near the BH horizon is misaligned with the BH rotation axis,
charged particles, which initially spiral into the BH hole along the equatorial
plane, penetrate into the regions above the BH "polar caps" and are ejected
with high energies to infinity. We show that in such a model acceleration of
protons near a BH of typical mass 3e8 solar masses is possible only if the
magnetic field is almost aligned with the BH rotation axis. We find that the
power of anisotropic electromagnetic emission from an UHECR source near a
supermassive BH should be at least 10-100 times larger then UHECR power of the
source. This implies that if the number of UHECR sources within the 100 Mpc
sphere is ~100, the power of electromagnetic emission which accompanies proton
acceleration in each source, $10^{42-43}$ erg/s, is comparable to the typical
luminosities of active galactic nuclei (AGN) in the local Universe. We also
explore the acceleration of heavy nuclei, for which the constraints on the
electromagnetic luminosity and on the alignment of magnetic field in the gap
are relaxed.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:28:12 GMT"
},
{
"version": "v2",
"created": "Tue, 17 Apr 2012 09:58:55 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Neronov",
"A.",
""
],
[
"Semikoz",
"D.",
""
],
[
"Tkachev",
"I.",
""
]
] | [
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] |
712.1738 | David G. Grier | Sang-Hyuk Lee, Yohai Roichman, Gi-Ra Yi, Shin-Hyun Kim, Seung-Man
Yang, Alfons van Blaaderen, Peter van Oostrum, and David G. Grier | Characterizing and tracking single colloidal particles with video
holographic microscopy | 6 pages, 3 figures | null | 10.1364/OE.15.018275 | null | physics.optics cond-mat.soft | null | We use digital holographic microscopy and Mie scattering theory to
simultaneously characterize and track individual colloidal particles. Each
holographic snapshot provides enough information to measure a colloidal
sphere's radius and refractive index to within 1%, and simultaneously to
measure its three-dimensional position with nanometer in-plane precision and 10
nanometer axial resolution.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:29:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lee",
"Sang-Hyuk",
""
],
[
"Roichman",
"Yohai",
""
],
[
"Yi",
"Gi-Ra",
""
],
[
"Kim",
"Shin-Hyun",
""
],
[
"Yang",
"Seung-Man",
""
],
[
"van Blaaderen",
"Alfons",
""
],
[
"van Oostrum",
"Peter",
""
],
[
"Grier",
"David G.",
""
]
] | [
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] |
712.1739 | Joachim Mathiesen | Joachim Mathiesen, Mogens H. Jensen, and Jan Oystein Haavig Bakke | Dimensions, Maximal Growth Sites and Optimization in the Dielectric
Breakdown Model | 5 pages, 7 figures; v2: extra figures and new data added | null | 10.1103/PhysRevE.77.066203 | null | cond-mat.stat-mech | null | We study the growth of fractal clusters in the Dielectric Breakdown Model
(DBM) by means of iterated conformal mappings. In particular we investigate the
fractal dimension and the maximal growth site (measured by the Hoelder exponent
$\alpha_{min}$) as a function of the growth exponent $\eta$ of the DBM model.
We do not find evidence for a phase transition from fractal to non-fractal
growth for a finite $\eta$-value. Simultaneously, we observe that the limit of
non-fractal growth ($D\to 1$) is consistent with $\alpha_{min} \to 1/2$.
Finally, using an optimization principle, we give a recipe on how to estimate
the effective value of $\eta$ from temporal growth data of fractal aggregates.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:38:24 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Apr 2008 07:03:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mathiesen",
"Joachim",
""
],
[
"Jensen",
"Mogens H.",
""
],
[
"Bakke",
"Jan Oystein Haavig",
""
]
] | [
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] |
712.174 | Michael J. Gruber | Michael J. Gruber, Daniel H. Lenz and Ivan Veseli\'c | Uniform existence of the integrated density of states for combinatorial
and metric graphs over Z^d | 22 pages; minor extensions and updates | Proc. Symp. Pure Math. vol. 77 (2008), 87-108 | null | Isaac Newton Institute preprint NI08009-AGA | math-ph math.FA math.MP math.SP | null | We give an overview and extension of recent results on ergodic random
Schr\"odinger operators for models on $\mathbb{Z}^d$. The operators we consider
are defined on combinatorial or metric graphs, with random potentials, random
boundary conditions and random metrics taking values in a finite set. We show
that normalized finite volume eigenvalue counting functions converge to a limit
uniformly in the energy variable, at least locally. This limit, the integrated
density of states (IDS), can be expressed by a closed Shubin-Pastur type trace
formula. The set of points of increase of the IDS supports the spectrum and its
points of discontinuity are characterized by existence of compactly supported
eigenfunctions. This applies to several examples, including various periodic
operators and percolation models.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:40:04 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Feb 2008 14:14:01 GMT"
}
] | 2011-01-25T00:00:00 | [
[
"Gruber",
"Michael J.",
""
],
[
"Lenz",
"Daniel H.",
""
],
[
"Veselić",
"Ivan",
""
]
] | [
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] |
712.1741 | Jose Luis Jaramillo | J.L. Jaramillo, N. Vasset and M. Ansorg | A numerical study of Penrose-like inequalities in a family of axially
symmetric initial data | Contribution to the "Encuentros Relativistas Espanoles - Spanish
Relativity Meeting ERE07" Proceedings, Tenerife, Spain (September 2007) | null | 10.1051/eas:0830039 | null | gr-qc | null | Our current picture of black hole gravitational collapse relies on two
assumptions: i) the resulting singularity is hidden behind an event horizon --
weak cosmic censorship conjecture -- and ii) spacetime eventually settles down
to a stationarity state. In this setting, it follows that the minimal area
containing an apparent horizon is bound by the square of the total ADM mass
(Penrose inequality conjecture). Following Dain et al. 2002, we construct
numerically a family of axisymmetric initial data with one or several
marginally trapped surfaces. Penrose and related geometric inequalities are
discused for these data. As a by-product, it is shown how Penrose inequality
can be used as a diagnosis for an apparent horizon finder numerical routine.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:43:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jaramillo",
"J. L.",
""
],
[
"Vasset",
"N.",
""
],
[
"Ansorg",
"M.",
""
]
] | [
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] |
712.1742 | James Silvester Mr | J. Silvester, G.A. Wade, O. Kochukhov, J.D. Landstreet, S. Bagnulo | Magnetic Doppler Imaging of Ap stars | In the proceedings of the "CP/AP workshop" held in Vienna, September
2007 | null | null | null | astro-ph | null | Historically, the magnetic field geometries of the chemically peculiar Ap
stars were modelled in the context of a simple dipole field. However, with the
acquisition of increasingly sophisticated diagnostic data, it has become clear
that the large-scale field topologies exhibit important departures from this
simple model. Recently, new high-resolution circular and linear polarisation
spectroscopy has even hinted at the presence of strong, small-scale field
structures, which were completely unexpected based on earlier modelling. This
project investigates the detailed structure of these strong fossil magnetic
fields, in particular the large-scale field geometry, as well as small scale
magnetic structures, by mapping the magnetic and chemical surface structure of
a selected sample of Ap stars. These maps will be used to investigate the
relationship between the local field vector and local surface chemistry,
looking for the influence the field may have on the various chemical transport
mechanisms (i.e., diffusion, convection and mass loss). This will lead to
better constraints on the origin and evolution, as well as refining the
magnetic field model for Ap stars. Mapping will be performed using high
resolution and signal-to-noise ratio time-series of spectra in both circular
and linear polarisation obtained using the new-generation ESPaDOnS and NARVAL
spectropolarimeters at the CFHT and Pic du Midi Observatory. With these data we
will perform tomographic inversion of Doppler-broadened Stokes IQUV Zeeman
profiles of a large variety of spectral lines using the INVERS10 magnetic
Doppler imaging code, simultaneously recovering the detailed surface maps of
the vector magnetic field and chemical abundances.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:05:00 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Silvester",
"J.",
""
],
[
"Wade",
"G. A.",
""
],
[
"Kochukhov",
"O.",
""
],
[
"Landstreet",
"J. D.",
""
],
[
"Bagnulo",
"S.",
""
]
] | [
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712.1743 | Joerg Fischera JF | Joerg Fischera and Michael A. Dopita | The Spectral Energy Distribution of Self-gravitating Interstellar Clouds
I. Spheres | accepted for publication in ApJS, May 2008, v176n1 issue | null | 10.1086/525280 | null | astro-ph | null | We derive the spectral energy distribution (SED) of dusty, isothermal, self
gravitating, stable and spherical clouds externally heated by the ambient
interstellar radiation field. For a given radiation field and dust properties,
the radiative transfer problem is determined by the pressure of the surrounding
medium and the cloud mass expressed as a fraction of the maximum stable cloud
mass above which the clouds become gravitational unstable.
To solve the radiative transfer problem a ray-tracing code is used to
accurately derive the light distribution inside the cloud. This code considers
both non isotropic scattering on dust grains and multiple scattering events.
The dust properties inside the clouds are assumed to be the same as in the
diffuse interstellar medium in our galaxy. We analyse the effect of the
pressure, the critical mass fraction, and the ISRF on the SED and present
brightness profiles in the visible, the IR/FIR and the submm/mm regime with the
focus on the scattered emission and the thermal emission from PAH-molecules and
dust grains.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:02:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fischera",
"Joerg",
""
],
[
"Dopita",
"Michael A.",
""
]
] | [
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] |
712.1744 | Matteo Martini | The KLOE collaboration | Measurement of the KS->gg branching ratio using a pure KS beam with the
KLOE detector | 13 pages, 9 figures | JHEP 0805:051,2008 | 10.1088/1126-6708/2008/05/051 | null | hep-ex | null | We have searched for the decay KS->gg in a sample of 2x10^9 phi->KS KL decays
collected at DAPHNE with an integrated luminosity of 1.9 fb^{-1}. KS are tagged
by the KL interaction in the calorimeter. Two prompt photons must also be
detected. Kinematic constraints reduce the initial 6x10^5 events to 2740
candidates, from which a signal of 711\pm 35 events is extracted. By
normalizing to the KS->2pi^0 decays counted in the same sample, we measure
BR(KS->gg)= (2.26\pm0.12_{stat}\pm0.06_{syst})x10^{-6}, in agreement with
O(p^4) Chiral Perturbation Theory predictions.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:00:11 GMT"
},
{
"version": "v2",
"created": "Thu, 8 May 2008 13:46:32 GMT"
}
] | 2012-08-27T00:00:00 | [
[
"The KLOE collaboration",
"",
""
]
] | [
0.0476248451,
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] |
712.1745 | Michele Sciacca | Michele Sciacca, David Jou and Maria Stella Mongiov\'i | Phenomenological description of the vortex density in rotating BEC
superfluids | 11 pages, 3 figures | null | null | null | cond-mat.other | null | We propose a phenomenological equation for the vortex line density in
rotating Bose-Einstein condensates as a function of the angular speed. This
equation provides a simple description of the gross features of the increase in
vortex number from the appearance of the first vortex to the theoretical
rigid-body result for high vortex density, and allows one to compare with
analogous situations in superfluid helium, after the suitable changes in the
relevant parameters are made.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:53:43 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Sciacca",
"Michele",
""
],
[
"Jou",
"David",
""
],
[
"Mongioví",
"Maria Stella",
""
]
] | [
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] |
712.1746 | Evelyne Alecian | E. Alecian (RMC), C. Catala (LESIA), G.A. Wade (RMC), J.-F. Donati
(LATT), P. Petit (LATT), J.D. Landstreet (UWO), S. Bagnulo (Armagh
Observatory), T. Boehm (LATT), J.-C. Bouret (LAM), C. Folsom (Armagh
Observatory), J. Grunhut (RMC), J. Silvester (RMC) | Characterisation of the magnetic field of the Herbig Be star HD 200775 | Accepted for publication in MNRAS, 14 pages, 10 figures | null | 10.1111/j.1365-2966.2008.12842.x | null | astro-ph | null | After our recent discovery of four magnetic Herbig stars, we have decided to
study in detail one of them, HD 200775, to determine if its magnetic topology
is similar to that of the main sequence magnetic stars. With this aim, we
monitored this star in Stokes I and V over more than two years, using the new
spectropolarimeters ESPaDOnS at CFHT, and Narval at TBL. Using our data, we
find that HD 200775 is a double-lined spectroscopic binary system, whose
secondary seems similar, in temperature, to the primary. We determine the
luminosity ratio of the system, and using the luminosity of the system found in
literature, we derive the luminosity of both stars. From our measurements of
the radial velocities of both stars we determine the ephemeris and the orbital
parameters of the system. We have fitted 30 Stokes V profiles simultaneously,
using a chi2 minimisation method, with a decentered-dipole model. The best-fit
model provides a rotation period of 4.3281 d an inclination angle of 60
degrees, and a magnetic obliquity angle of 125 degrees. The polar strength of
the magnetic dipole field is 1000 G, which is decentered by 0.05 R* from the
center of the star. The derived magnetic field model is qualitatively identical
to those commonly observed in the Ap/Bp stars, which bring strong argument in
favour of the fossil field hypothesis, to explain the origin of the magnetic
fields in the main sequence Ap/Bp stars. Our determination of the inclination
of the rotation axis leads to a radius of the primary which is smaller than
that derived from the HR diagram position. This can be explained by a larger
intrinsic luminosity of the secondary relative to the primary, due to a larger
circumstellar extinction of the secondary relative to the primary.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:55:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Alecian",
"E.",
"",
"RMC"
],
[
"Catala",
"C.",
"",
"LESIA"
],
[
"Wade",
"G. A.",
"",
"RMC"
],
[
"Donati",
"J. -F.",
"",
"LATT"
],
[
"Petit",
"P.",
"",
"LATT"
],
[
"Landstreet",
"J. D.",
"",
"UWO"
],
[
"Bagnulo",
"S.",
"",
"Armagh\n Observatory"
],
[
"Boehm",
"T.",
"",
"LATT"
],
[
"Bouret",
"J. -C.",
"",
"LAM"
],
[
"Folsom",
"C.",
"",
"Armagh\n Observatory"
],
[
"Grunhut",
"J.",
"",
"RMC"
],
[
"Silvester",
"J.",
"",
"RMC"
]
] | [
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] |
712.1747 | Cormac Toher | C. Toher and S. Sanvito | Effects of self-interaction corrections on the transport properties of
phenyl-based molecular junctions | 12 pages, 21 figures | null | 10.1103/PhysRevB.77.155402 | null | cond-mat.mes-hall | null | In transport calculations for molecular junctions based on density functional
theory the choice of exchange and correlation functional may dramatically
affect the results. In particular local and semi-local functionals tend to
over-delocalize the molecular levels thus artificially increasing their
broadening. In addition the same molecular levels are usually misplaced with
respect to the Fermi level of the electrodes. These shortfalls are reminiscent
of the inability of local functionals to describe Mott-Hubbard insulators, but
they can be corrected with a simple and computationally undemanding
self-interaction correction scheme. We apply such a scheme, as implemented in
our transport code Smeagol, to a variety of phenyl-based molecular junctions
attached to gold electrodes. In general the corrections reduce the current,
since the resonant Kohn-Sham states of the molecule are shifted away from the
contact Fermi level. In contrast, when the junction is already described as
insulating by local exchange and correlation potentials, the corrections are
minimal and the I-V is only weakly modified.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:55:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Toher",
"C.",
""
],
[
"Sanvito",
"S.",
""
]
] | [
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] |
712.1748 | M. B. N. Kouwenhoven | M.B.N. Kouwenhoven (1), R. de Grijs (1,2) ((1) University of
Sheffield, UK (2) National Astronomical Observatories, Chinese Academy of
Sciences, China) | The effect of binaries on the dynamical mass determination of star
clusters | 12 pages, 10 figures, accepted by A&A | null | 10.1051/0004-6361:20078897 | null | astro-ph | null | The total mass of distant star clusters is often derived from the virial
theorem, using line-of-sight velocity dispersion measurements and half-light
radii. Although most stars form in binary systems, this is mostly ignored when
interpreting the observations. The components of binary stars exhibit orbital
motion, which may increase the measured velocity dispersion, and may therefore
result in a dynamical mass overestimation. In this paper we quantify the effect
of neglecting the binary population on the derivation of the dynamical mass of
a star cluster. We simulate star clusters numerically, and study the dependence
of the derived dynamical mass on the properties of the binary population. We
find that the presence of binaries plays a crucial role for very sparse
clusters with a stellar density comparable to that of the field star population
(~0.1 stars/pc3), as the velocity dispersion is fully dominated by the binary
orbital motion. For such clusters, the dynamical mass may overestimate the true
mass by up to an order of magnitude. For very dense clusters (>10^7 stars/pc3),
binaries do not affect the dynamical mass estimation significantly. For
clusters of intermediate density (0.1-10^7 stars/pc3), the dynamical mass can
be overestimated by 10-100%, depending on the properties of the binary
population.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:56:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kouwenhoven",
"M. B. N.",
""
],
[
"de Grijs",
"R.",
""
]
] | [
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712.1749 | Joni Tammi (ne Virtanen) | Joni Tammi and Paul Dempsey | Particle acceleration by multiple parallel shocks | 4 pages, 6 figures. Proceedings of a talk in the ICRC 2007 | null | null | null | astro-ph | null | We present both numerical and semi-analytical results on test-particle
acceleration in multiple parallel shocks. We apply a kinetic Monte Carlo code
and an eigenfunction expansion method to calculate the distribution functions
for electron populations accelerated in subsequent parallel shocks with speeds
ranging from non- to fully-relativistic. We examine the levels of particle
anisotropy at the shocks and discuss the implications for AGN and microquasar
jets.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:58:29 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Tammi",
"Joni",
""
],
[
"Dempsey",
"Paul",
""
]
] | [
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] |
712.175 | Stephen King | S.F.King | Neutrino Mass | 30 pages, 14 figures, review article suitable for a general audience | null | 10.1080/00107510701770539 | null | physics.pop-ph physics.ed-ph | null | This is a review article about the most recent developments on the field of
neutrino mass. The first part of the review introduces the idea of neutrino
masses and mixing angles, summarizes the most recent experimental data then
discusses the experimental prospects and challenges in this area. The second
part of the review discusses the implications of these results for particle
physics and cosmology, including the origin of neutrino mass, the see-saw
mechanism and sequential dominance, and large extra dimensions and cosmology.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 15:43:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"King",
"S. F.",
""
]
] | [
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712.1751 | Joni Tammi (ne Virtanen) | Joni Tammi | Hard particle spectra from parallel shocks due to turbulence
transmission | 4 pages, 3 figures. Proceedings of a poster in the ICRC 2007 | null | null | null | astro-ph | null | If taken into account, the transmission of the particle-scattering turbulence
--in addition to just the particles-- through the shock front can change the
effective compression ratio felt by the accelerating particles significantly
from the compression of the underlying plasma. This can lead to significantly
harder energy spectra than what are traditionally predicted assuming frozen-in
turbulence. I consider the applicability and limitations of turbulence
transmission scenario in parallel shock waves of different thickness, its
consequences in AGN and microquasar environments, and discuss the possible
effects to the spectrum of the accelerated particles.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:06:29 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Tammi",
"Joni",
""
]
] | [
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712.1752 | Duccio Fanelli | Pierre-Henri Chavanis, Giovanni De Ninno, Duccio Fanelli, Stefano
Ruffo | Out of equilibrium phase transitions in mean field Hamiltonian dynamics | Proceedings of the conference "Chaos, Complexity and Transport"
(Marseille, 5-9 June 2007) | null | 10.1142/9789812818805_0001 | null | cond-mat.stat-mech | null | Systems with long-range interactions display a short-time relaxation towards
Quasi-Stationary States (QSSs), whose lifetime increases with system size. With
reference to the Hamiltonian Mean Field (HMF) model, we here review
Lynden-Bell's theory of ``violent relaxation''. The latter results in a maximum
entropy scheme for a water-bag initial profile which predicts the presence of
out-of-equilibrium phase transitions} separating homogeneous (zero
magnetization) from inhomogeneous (non-zero magnetization) QSSs. Two different
parametric representations of the initial condition are analyzed and the
features of the phase diagram are discussed. In both representations we find a
second order and a first order line of phase transitions that merge at a
tricritical point. Particular attention is payed to the condition of existence
and stability of the homogenous phase.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:08:18 GMT"
}
] | 2016-11-23T00:00:00 | [
[
"Chavanis",
"Pierre-Henri",
""
],
[
"De Ninno",
"Giovanni",
""
],
[
"Fanelli",
"Duccio",
""
],
[
"Ruffo",
"Stefano",
""
]
] | [
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] |
712.1753 | Erkko Lehtonen | Miguel Couceiro, Erkko Lehtonen | Generalizations of Swierczkowski's lemma and the arity gap of finite
functions | 11 pages, proofs simplified, contents reorganized | Discrete Math. 309 (2009) 5905-5912 | 10.1016/j.disc.2009.04.009 | null | math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Swierczkowski's Lemma - as it is usually formulated - asserts that if f is an
at least quaternary operation on a finite set A and every operation obtained
from f by identifying a pair of variables is a projection, then f is a
semiprojection. We generalize this lemma in various ways. First, it is extended
to B-valued functions on A instead of operations on A and to essentially at
most unary functions instead of projections. Then we characterize the arity gap
of functions of small arities in terms of quasi-arity, which in turn provides a
further generalization of Swierczkowski's Lemma. Moreover, we explicitly
classify all pseudo-Boolean functions according to their arity gap. Finally, we
present a general characterization of the arity gaps of B-valued functions on
arbitrary finite sets A.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:12:59 GMT"
},
{
"version": "v2",
"created": "Tue, 17 Mar 2009 20:33:10 GMT"
}
] | 2016-11-22T00:00:00 | [
[
"Couceiro",
"Miguel",
""
],
[
"Lehtonen",
"Erkko",
""
]
] | [
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] |
712.1754 | Jie Xiao | Cheikh Birahim Ndiaye and Jie Xiao | An Upper Bound of the Total Q-Curvature and Its Isoperimetric Deficit
for Higher-dimensional Conformal Euclidean Metrics | null | null | 10.1007/s00526-009-0276-8 | null | math.DG math.MG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The aim of this paper is to give not only an explicit upper bound of the
total Q-curvature but also an induced isoperimetric deficit formula for the
complete conformal metrics on $\mathbb R^n$, $n\ge 3$ with scalar curvature
being nonnegative near infinity and Q-curvature being absolutely convergent.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:13:44 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Aug 2009 18:15:46 GMT"
},
{
"version": "v3",
"created": "Fri, 9 Oct 2009 15:23:20 GMT"
}
] | 2009-10-09T00:00:00 | [
[
"Ndiaye",
"Cheikh Birahim",
""
],
[
"Xiao",
"Jie",
""
]
] | [
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] |
712.1755 | Jiang Zeng | Anisse Kasraoui, Jiang Zeng | Euler-Mahonian Statistics On Ordered Set Partitions (II) | 27 pages,8 figures | null | null | null | math.CO | null | We study statistics on ordered set partitions whose generating functions are
related to $p,q$-Stirling numbers of the second kind. The main purpose of this
paper is to provide bijective proofs of all the conjectures of \stein
(Arxiv:math.CO/0605670). Our basic idea is to encode ordered partitions by a
kind of path diagrams and explore the rich combinatorial properties of the
latter structure. We also give a partition version of MacMahon's theorem on the
equidistribution of the statistics inversion number and major index on words.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:20:07 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Kasraoui",
"Anisse",
""
],
[
"Zeng",
"Jiang",
""
]
] | [
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] |
712.1756 | Alexander Popov | Alexander D. Popov | Integrability of Vortex Equations on Riemann Surfaces | 16 pages; v2: typos fixed, clarifying comments added, published
version | Nucl.Phys.B821:452-466,2009 | 10.1016/j.nuclphysb.2009.05.003 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Abelian Higgs model on a compact Riemann surface \Sigma of genus g is
considered. We show that for g > 1 the Bogomolny equations for multi-vortices
at critical coupling can be obtained as compatibility conditions of two linear
equations (Lax pair) which are written down explicitly. These vortices
correspond precisely to SO(3)-symmetric Yang-Mills instantons on the
(conformal) gravitational instanton \Sigma\times S^2 with a scalar-flat Kahler
metric. Thus, the standard methods of constructing solutions and studying their
properties by using Lax pairs (twistor approach, dressing method etc.) can be
applied to the vortex equations on \Sigma. In the twistor description,
solutions of the integrable vortex equations correspond to rank-2 holomorphic
vector bundles over the complex 3-dimensional twistor space of \Sigma\times
S^2. We show that in the general (nonintegrable) case there is a bijection
between the moduli spaces of solutions to vortex equations on \Sigma and of
pseudo-holomorphic bundles over the almost complex twistor space.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:24:02 GMT"
},
{
"version": "v2",
"created": "Fri, 29 May 2009 14:52:56 GMT"
}
] | 2009-09-28T00:00:00 | [
[
"Popov",
"Alexander D.",
""
]
] | [
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712.1757 | Maria T. Beltran | M.T. Beltran (1), R. Estalella (1), J.M. Girart (2), P.T.P. Ho (3, 4),
and G. Anglada (5) ((1) Universitat de Barcelona; (2) Institut de Ciencies de
l'Espai; (3) Harvard-Smithsonian Center for Astrophysics; (4) Academia
Sinica, Institute of Astronomy and Astrophysics; (5) Instituto de Astrofisica
de Andalucia) | On the nature of outflows in intermediate-mass protostars: a case study
of IRAS 20050+2720 | 13 pages, 8 figures, 5 tables. Accepted for publication by A&A | null | 10.1051/0004-6361:20078045 | null | astro-ph | null | Context. This is the third of a series of papers devoted to study in detail
and with high-angular resolution intermediate-mass molecular outflows and their
powering sources. Aims. The aim of this paper is to study the intermediate-mass
YSO IRAS 20050+2720 and its molecular outflow, and put the results of this and
the previous studied sources in the context of intermediate-mass star
formation. Methods. We carried out VLA observations of the 7 mm continuum
emission, and OVRO observations of the 2.7 mm continuum emission, CO(1-0),
C18O(1-0), and HC3N(12-11) to map the core towards IRAS 20050+2720. The
high-angular resolution of the observations allowed us to derive the properties
of the dust emission, the molecular outflow, and the dense protostellar
envelope. By adding this source to the sample of intermediate-mass protostars
with outflows, we compare their properties and evolution with those of lower
mass counterparts. Results. The 2.7mm continuum emission has been resolved into
three sources, labeled OVRO 1, OVRO 2, and OVRO 3. Two of them, OVRO 1 and OVRO
2, have also been detected at 7 mm. OVRO 3, which is located close to the C18O
emission peak, could be associated with IRAS 20050+2720. The mass of the
sources, estimated from the dust continuum emission, is 6.5 Msun for OVRO 1,
1.8 Msun for OVRO 2, and 1.3 Msun for OVRO 3. The CO(1-0) emission traces two
bipolar outflows within the OVRO field of view, a roughly east-west bipolar
outflow, labeled A, driven by the intermediate-mass source OVRO 1, and a
northeast-southwest bipolar outflow, labeled B, probably powered by a YSO
engulfed in the circumstellar envelope surrounding OVRO 1.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:34:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Beltran",
"M. T.",
""
],
[
"Estalella",
"R.",
""
],
[
"Girart",
"J. M.",
""
],
[
"Ho",
"P. T. P.",
""
],
[
"Anglada",
"G.",
""
]
] | [
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712.1758 | Daniel Gamermann | D. Gamermann and E. Oset | Hidden charm dynamically generated resonances and the $e^+e^-\to J/\psi
D \bar D$, $J/\psi D\bar D^*$ reactions | 5 pages, 5 figures, 2 tables | Eur.Phys.J.A36:189-194,2008 | 10.1140/epja/i2007-10580-5 | null | hep-ph hep-ex | null | We analyze two recent reactions of Belle, producing $D\bar D$ and $D\bar D^*$
states that have an enhancement of the invariant $D\bar D$, $D\bar D^*$ mass
distribution close to threshold, from the point of view that they might be
indicative of the existence of a hidden charm scalar and an axial vector meson
states below $D\bar D$ or $D\bar D^*$ thresholds, respectively. We conclude
that the data is compatible with the existing prediction of a hidden charm
scalar meson with mass around 3700 MeV, though other possibilities cannot be
discarded. The peak seen in the $D\bar D^*$ spectrum above threshold is,
however, unlikely to be due to a threshold enhancement produced by the
presence, below threshold, of the hidden charm axial vector meson X(3872).
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:35:57 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Gamermann",
"D.",
""
],
[
"Oset",
"E.",
""
]
] | [
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] |
712.1759 | Sebastien George | Madeth May (LIESP), S\'ebastien George (LIESP), Patrick Pr\'ev\^ot
(LIESP) | A Web-based System for Observing and Analyzing Computer Mediated
Communications | null | Dans Proceedings of the IEEE/WIC/ACM International Conference on
Web Intelligence (WI 2006) - IEEE/WIC/ACM International Conference on Web
Intelligence (WI 2006, Hong Kong : Chine (2006) | null | null | cs.HC | null | Tracking data of user's activities resulting from Computer Mediated
Communication (CMC) tools (forum, chat, etc.) is often carried out in an ad-hoc
manner, which either confines the reusability of data in different purposes or
makes data exploitation difficult. Our research works are biased toward
methodological challenges involved in designing and developing a generic system
for tracking user's activities while interacting with asynchronous
communication tools like discussion forums. We present in this paper, an
approach for building a Web-based system for observing and analyzing user
activity on any type of discussion forums.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:47:54 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"May",
"Madeth",
"",
"LIESP"
],
[
"George",
"Sébastien",
"",
"LIESP"
],
[
"Prévôt",
"Patrick",
"",
"LIESP"
]
] | [
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] |
712.176 | Stefan Nemirovski | Stefan Nemirovski | Lagrangian Klein bottles in R^{2n} | V.2 - explicit formula for the Luttinger-type surgery; V.3 - section
3 corrected, section 6 expanded; 6 pages | Geom. Funct. Anal. 19 (2009), 902-909 | 10.1007/s00039-009-0014-6 | null | math.SG math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | It is shown that the n-dimensional Klein bottle admits a Lagrangian embedding
into R^{2n} if and only if n is odd.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:12:06 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Mar 2008 10:59:42 GMT"
},
{
"version": "v3",
"created": "Tue, 17 Jun 2008 13:00:49 GMT"
}
] | 2009-11-20T00:00:00 | [
[
"Nemirovski",
"Stefan",
""
]
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] |
712.1761 | Yue Zou | Yue Zou, Israel Klich, and Gil Refael | Effect of inhomogeneous coupling on superconductivity | 12 pages, 14 figures | Phys. Rev. B 77, 144523 (2008) | 10.1103/PhysRevB.77.144523 | null | cond-mat.supr-con | null | We investigate the influence of inhomogeneity in the pairing coupling
constant $U(\vec r)$ on dirty BCS superconductors, focusing on $T_c$, the order
parameter $\Delta(\vec r)$, and the energy gap $E_g(\vec r)$. Within mean-field
theory, we find that when the length-scale of the inhomogeneity is comparable
to, or larger than the coherence length, the ratio $2E_g/T_c$ is significantly
reduced from that of a homogeneous superconductor, while in the opposite limit
this ratio stays unmodified. In two dimensions, when strong phase fluctuations
are included, the Kosterlitz-Thouless temperature $T_{KT}$ is also studied. We
find that when the inhomogeneity length scale is much larger than the coherence
length, $2E_g/T_{KT}$ can be larger than the usual BCS value. We use our
results to qualitatively explain recent experimental observation of a
surprisingly low value of $2E_g/T_c$ in thin films.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:00:51 GMT"
}
] | 2008-05-10T00:00:00 | [
[
"Zou",
"Yue",
""
],
[
"Klich",
"Israel",
""
],
[
"Refael",
"Gil",
""
]
] | [
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712.1762 | Frederic Jouhet | Frederic Jouhet (ICJ), Elie Mosaki (ICJ) | Irrationalit\'e aux entiers impairs positifs d'un q-analogue de la
fonction zeta de Riemann | 33 pages | null | null | null | math.CO math.NT | null | In this paper, we focus on a q-analogue of the Riemann zeta function at
positive integers, which can be written for s\in\N^* by \zeta_q(s)=\sum_{k\geq
1}q^k\sum_{d|k}d^{s-1}. We give a new lower bound for the dimension of the
vector space over \Q spanned, for 1/q\in\Z\setminus\{-1;1\} and an even integer
A, by 1,\zeta_q(3),\zeta_q(5),...,\zeta_q(A-1). This improves a recent result
of Krattenthaler, Rivoal and Zudilin (\emph{S\'eries hyperg\'eom\'etriques
basiques, q-analogues des valeurs de la fonction zeta et s\'eries
d'Eisenstein}, J. Inst. Jussieu {\bf 5}.1 (2006), 53-79). In particular, a
consequence of our result is that for 1/q\in\Z\setminus\{-1;1\}, at least one
of the numbers \zeta_q(3),\zeta_q(5),\zeta_q(7),\zeta_q(9) is irrational.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:49:33 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Jouhet",
"Frederic",
"",
"ICJ"
],
[
"Mosaki",
"Elie",
"",
"ICJ"
]
] | [
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712.1763 | Manuel Guedel | M. Guedel | The Sun in Time: Activity and Environment | accepted by The Living Reviews in Solar Physics, 121 pages, 44
figures; many figures have been degraded; for a version with full-quality
figures, see http://www.astro.phys.ethz.ch/papers/guedel/papers.html | null | 10.12942/lrsp-2007-3 | null | astro-ph | null | (abridged) The Sun's magnetic activity has steadily declined during its
main-sequence life. While the solar photospheric luminosity was about 30% lower
4.6 Gyr ago when the Sun arrived on the main sequence compared to present-day
levels, its faster rotation generated enhanced magnetic activity; magnetic
heating processes in the chromosphere, the transition region, and the corona
induced ultraviolet, extreme-ultraviolet, and X-ray emission about 10, 100, and
1000 times, respectively, the present-day levels, as inferred from young
solar-analog stars. Also, the production rate of accelerated, high-energy
particles was orders of magnitude higher than in present-day solar flares, and
a much stronger wind escaped from the Sun, permeating the entire solar system.
The consequences of the enhanced radiation and particle fluxes from the young
Sun were potentially severe for the evolution of solar-system planets and
moons. Interactions of high-energy radiation and the solar wind with upper
planetary atmospheres may have led to the escape of important amounts of
atmospheric constituents. The present dry atmosphere of Venus and the thin
atmosphere of Mars may be a product of early irradiation and heating by solar
high-energy radiation. High levels of magnetic activity are also inferred for
the pre-main sequence Sun. At those stages, interactions of high-energy
radiation and particles with the circumsolar disk in which planets eventually
formed were important. Traces left in meteorites by energetic particles and
anomalous isotopic abundance ratios in meteoritic inclusions may provide
evidence for a highly active pre-main sequence Sun. The present article reviews
these various issues related to the magnetic activity of the young Sun and the
consequent interactions with its environment.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:37:06 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Guedel",
"M.",
""
]
] | [
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] |
712.1764 | Slawomir Piatek | S. Piatek, C. Pryor and E. W. Olszewski | Proper Motions of the LMC and SMC: Reanalysis of Hubble Space Telescope
Data | Accepted for publication in AJ; 38 manuscript pages, 14 figures (some
in color) | null | null | null | astro-ph | null | Kallivayalil et al. have used the \textit{Hubble Space Telescope} to measure
proper motions of the LMC and SMC using images in 21 and five fields,
respectively, all centered on known QSOs. These results are more precise than
previous measurements, but have surprising and important physical implications:
for example, the LMC and SMC may be approaching the Milky Way for the first
time; they might not have been in a binary system; and the origin of the
Magellanic Stream needs to be re-examined. Motivated by these implications, we
have reanalyzed the original data in order to check the validity of these
measurements. Our work has produced a proper motion for the LMC that is in
excellent agreement with that of Kallivayalil et al., and for the SMC that is
in acceptable agreement.
We have detected a dependence between the brightness of stars and their mean
measured motion in a majority of the fields in both our reduction and that of
Kallivayalil et al. Correcting for this systematic error and for the errors
caused by the decreasing charge transfer efficiency of the detector produces
better agreement between the measurements from different fields. With our
improved reduction, we do not need to exclude any fields from the final
averages and, for the first time using proper motions, we are able to detect
the rotation of the LMC. The best-fit amplitude of the rotation curve at a
radius of 275 arcmin in the disk plane is $120 \pm 15$ km s$^{-1}$. This value
is larger than the 60--70 km s$^{-1}$ derived from the radial velocities of HI
and carbon stars, but in agreement with the value of 107 km s$^{-1}$ derived
from the radial velocities of red supergiants.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:03:01 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Piatek",
"S.",
""
],
[
"Pryor",
"C.",
""
],
[
"Olszewski",
"E. W.",
""
]
] | [
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712.1765 | Hugo Gimbert | Hugo Gimbert (LaBRI), Florian Horn (LIAFA, Cwi) | Solving Simple Stochastic Games with Few Random Vertices | null | Logical Methods in Computer Science, Volume 5, Issue 2 (May 25,
2009) lmcs:1119 | 10.2168/LMCS-5(2:9)2009 | null | cs.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Simple stochastic games are two-player zero-sum stochastic games with
turn-based moves, perfect information, and reachability winning conditions. We
present two new algorithms computing the values of simple stochastic games.
Both of them rely on the existence of optimal permutation strategies, a class
of positional strategies derived from permutations of the random vertices. The
"permutation-enumeration" algorithm performs an exhaustive search among these
strategies, while the "permutation-improvement" algorithm is based on
successive improvements, \`a la Hoffman-Karp. Our algorithms improve previously
known algorithms in several aspects. First they run in polynomial time when the
number of random vertices is fixed, so the problem of solving simple stochastic
games is fixed-parameter tractable when the parameter is the number of random
vertices. Furthermore, our algorithms do not require the input game to be
transformed into a stopping game. Finally, the permutation-enumeration
algorithm does not use linear programming, while the permutation-improvement
algorithm may run in polynomial time.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:50:51 GMT"
},
{
"version": "v2",
"created": "Tue, 7 Apr 2009 19:06:58 GMT"
},
{
"version": "v3",
"created": "Wed, 8 Apr 2009 13:30:39 GMT"
},
{
"version": "v4",
"created": "Thu, 9 Apr 2009 08:42:12 GMT"
},
{
"version": "v5",
"created": "Mon, 11 May 2009 12:18:50 GMT"
},
{
"version": "v6",
"created": "Mon, 25 May 2009 11:44:26 GMT"
}
] | 2015-07-01T00:00:00 | [
[
"Gimbert",
"Hugo",
"",
"LaBRI"
],
[
"Horn",
"Florian",
"",
"LIAFA, Cwi"
]
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712.1766 | Marguerite Virotte-Ducharme | Marguerite Virotte-Ducharme (IMJ) | Sur le centralisateur d'une involution de 2E6(2) | null | null | null | null | math.GR | null | In this paper we prove that $2^{20+1}.U_6(2)$, known as the centralizer of an
involution in the group $2E_6(2)$ is a quotient of a Coxeter group. We obtain a
presentation of $2^{20+1}.U_6(2)$ as a $Q_{222}$-group, which now resolve a
long pending question.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:56:14 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Virotte-Ducharme",
"Marguerite",
"",
"IMJ"
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] |
712.1767 | Guillaume Jourdan | Guillaume Jourdan (LKB - Jussieu, NEEL), Astrid Lambrecht (LKB -
Jussieu), Fabio Comin (ESRF), Jo\"el Chevrier (NEEL) | Quantitative non contact dynamic Casimir force measurements | null | null | null | null | physics.gen-ph | null | We show that the Casimir force gradient can be quantitatively measured with
no contact involved. Results of the Casimir force measurement with systematic
uncertainty of 3% are presented for the distance range of 100-600 nm. The
statistical uncertainty is shown to be due to the thermal fluctuations of the
force probe. The corresponding signal to noise ratio equals unity at the
distance of 600 nm. Direct contact between surfaces used in most previous
studies to determine absolute distance separation is here precluded. Use of
direct contact to identify the origin of distances is a severe limitation for
studies of the Casimir forces on structured surfaces as it deteriorates
irreversibly the studied surface and the probe. This force machine uses a
dynamical method with an inserted gold sphere probe glued to a lever. The lever
is mechanically excited at resonant frequency in front of a chosen sample. The
absolute distance determination is achieved to be possible, without any direct
probe/sample contact, using an electrostatic method associated to a real time
correction of the mechanical drift. The positioning shift uncertainty is as low
as 2 nm.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:56:58 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Jourdan",
"Guillaume",
"",
"LKB - Jussieu, NEEL"
],
[
"Lambrecht",
"Astrid",
"",
"LKB -\n Jussieu"
],
[
"Comin",
"Fabio",
"",
"ESRF"
],
[
"Chevrier",
"Joël",
"",
"NEEL"
]
] | [
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] |
712.1768 | Sebastien George | S\'ebastien George (LIESP), Alain Derycke (TRIGONE) | Conceptions et usages des plates-formes de formation, Revue Sciences et
Technologies de l'Information et de la Communication pour l'\'Education et la
Formation | null | Sciences et Technologies de l'Information et de la Communication
pour l'Education et la Formation 12 (2006) 51-64 | null | null | cs.HC | null | Educative platforms are at the heart of the development of online education.
They can not only be reduced to technological aspects. Underlying models impact
teaching and learning from the preparing of lessons to the learning sessions.
Research related to these platforms are numerous and their stakes are
important. For these reasons, we launched a call to a special issue on "Designs
and uses of educative platforms" An educative platform is a computer system
designed to automate various functions relating to the organization of the
course, to the management of their content, to the monitoring of learners and
supervision of persons in charge of various formations (Office de la langue
fran\c{c}aise, 2005). So educative platforms are Learning Management Systems
(LMS) which are specific to education contexts.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 16:59:19 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"George",
"Sébastien",
"",
"LIESP"
],
[
"Derycke",
"Alain",
"",
"TRIGONE"
]
] | [
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712.1769 | Toshiyuki Kobayashi | Toshiyuki Kobayashi and Gen Mano | The Schrodinger model for the minimal representation of the indefinite
orthogonal group O(p, q) | Memoirs of the American Mathematical Society, vol. 212, no.1000,
(2011), vi+132 pp | null | 10.1090/S0065-9266-2011-00592-7 | RIMS-1588 | math.RT math-ph math.AP math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce the `Fourier transform' F_C on the isotropic cone C associated
to an indefinite quadratic form of signature (n_1,n_2) on R^n (n=n_1+n_2:
even). This transform is in some sense the unique and natural unitary operator
on L^2(C), as is the case with the Euclidean Fourier transform.
Inspired by recent developments of algebraic representation theory of
reductive groups, we shed new light on classical analysis on the one hand, and
give the global formulas for the L^2-model of the minimal representation of the
simple Lie group G=O(n_1+1,n_2+1) on the other hand.
The transform F_C expands functions on C into joint eigenfunctions of the n
commuting, self-adjoint, second order differential operators. We decompose F_C
into the singular Radon transform and the Mellin--Barnes integral, find its
distribution kernel, and establish the inversion and the Plancherel formula.
F_C reduces to the Hankel transform if G is O(n,2) or O(3,3).
The unitary operator F_C together with the simple action of the conformal
transformation group generates the minimal representation of the indefinite
orthogonal group G. Various different models of the same representation have
been constructed by Kazhdan, Kostant, Binegar-Zierau, Gross-Wallach, Zhu-Huang,
Torasso, Brylinski, and Kobayashi-Orsted, and others. Among them, our model
built on L^2(C) generalizes the classic Schrodinger model of the Weil
representation.
Yet another motif is special functions. Large group symmetries in the minimal
representation yield functional equations of various special functions. We find
explicit K-finite vectors on L^2(C), and give a new proof of the Plancherel
formula for Meijer's G-transforms.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 18:22:13 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jul 2008 11:31:00 GMT"
}
] | 2011-06-23T00:00:00 | [
[
"Kobayashi",
"Toshiyuki",
""
],
[
"Mano",
"Gen",
""
]
] | [
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712.177 | Claudio Dappiaggi | C. Dappiaggi, V. Moretti and N. Pinamonti | Cosmological horizons and reconstruction of quantum field theories | 32 pages, 1 figure, to appear on Comm. Math. Phys., dedicated to
Professor Klaus Fredenhagen on the occasion of his 60th birthday | Comm.Math.Phys.285:1129-1163,2009;
Commun.Math.Phys.285:1129-1163,2009 | 10.1007/s00220-008-0653-8 | Desy 07-218, UTM 718, ZMP-HH/07-12 | gr-qc hep-th math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | As a starting point, we state some relevant geometrical properties enjoyed by
the cosmological horizon of a certain class of Friedmann-Robertson-Walker
backgrounds. Those properties are generalised to a larger class of expanding
spacetimes $M$ admitting a geodesically complete cosmological horizon $\scrim$
common to all co-moving observers. This structure is later exploited in order
to recast, in a cosmological background, some recent results for a linear
scalar quantum field theory in spacetimes asymptotically flat at null infinity.
Under suitable hypotheses on $M$, encompassing both the cosmological de Sitter
background and a large class of other FRW spacetimes, the algebra of
observables for a Klein-Gordon field is mapped into a subalgebra of the algebra
of observables $\cW(\scrim)$ constructed on the cosmological horizon. There is
exactly one pure quasifree state $\lambda$ on $\cW(\scrim)$ which fulfils a
suitable energy-positivity condition with respect to a generator related with
the cosmological time displacements. Furthermore $\lambda$ induces a preferred
physically meaningful quantum state $\lambda_M$ for the quantum theory in the
bulk. If $M$ admits a timelike Killing generator preserving $\scrim$, then the
associated self-adjoint generator in the GNS representation of $\lambda_M$ has
positive spectrum (i.e. energy). Moreover $\lambda_M$ turns out to be invariant
under every symmetry of the bulk metric which preserves the cosmological
horizon. In the case of an expanding de Sitter spacetime, $\lambda_M$ coincides
with the Euclidean (Bunch-Davies) vacuum state, hence being Hadamard in this
case. Remarks on the validity of the Hadamard property for $\lambda_M$ in more
general spacetimes are presented.
| [
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"created": "Thu, 17 Jul 2008 16:42:43 GMT"
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] | 2009-01-19T00:00:00 | [
[
"Dappiaggi",
"C.",
""
],
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712.1771 | Eef van Beveren | Eef van Beveren and George Rupp | Deducing the string-breaking distance in strong production processes | plain LaTeX, 7 pages, 6 figures. Minor, but not unimportant changes.
In particular w.r.t. implications for Watson's theorem. Title changed
accordingly. The results in our paper are not affected | null | null | null | hep-ph | null | We show that the string-breaking distance can be read from meson-production
data, by employing a previously derived expression for the production
amplitude. Accordingly, we find that the radii of 0.67, 0.34 and 0.20 fm for
the creation of non-strange q-qbar pairs obtained in the
Resonance-Spectrum-Expansion model, for light-quark, c-cbar, and b-bbar
environments, respectively, are in perfect agreement with S-wave di-pion
production data, upon employing an ansatz with no additional free parameters.
| [
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{
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"created": "Fri, 23 May 2008 11:42:30 GMT"
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] | 2008-05-23T00:00:00 | [
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0.121817112,
0.0202255566,
-0.0395493358,
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] |
712.1772 | Daniel Corbett | D. Corbett, C.L. van Oosten and M. Warner | The dynamics of non-linear optical absorption | null | null | 10.1103/PhysRevA.78.013823 | null | cond-mat.soft cond-mat.other | null | On traversing materials with absorbing dyes, weak optical beams develop a
Beer (exponential) profile, while intense beams develop a spatially initially
linear and then finally an exponential profile. This anomalous, deep
penetration due to photo-bleaching of surface layers is important for heavy
dye-loading and intense beams, for instance in photo-actuation. We address the
problem of the evolution in time from initial Beer's Law to deeply penetrating
optical profiles in dyes. Our solution of the coupled, non-linear, partial
differential equations governing the spatio-temporal decay of the Poynting flux
and the non-linear dynamics of the \textit{trans-cis} conversion is applicable
to general systems of photo-active molecules under intense irradiation, for
instance in biology, in spectroscopy and in opto-mechanical devices.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:16:29 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Dec 2007 15:13:35 GMT"
},
{
"version": "v3",
"created": "Fri, 15 Feb 2008 16:31:17 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"Corbett",
"D.",
""
],
[
"van Oosten",
"C. L.",
""
],
[
"Warner",
"M.",
""
]
] | [
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] |
712.1773 | Mathias Perrin | J. Javaloyes, M. Perrin, A. Politi | Collective Atomic Recoil Laser as a synchronization transition | null | null | 10.1103/PhysRevE.78.011108 | null | physics.optics physics.gen-ph | null | We consider here a model previously introduced to describe the collective
behavior of an ensemble of cold atoms interacting with a coherent
electromagnetic field. The atomic motion along the self-generated
spatially-periodic force field can be interpreted as the rotation of a phase
oscillator. This suggests a relationship with synchronization transitions
occurring in globally coupled rotators. In fact, we show that whenever the
field dynamics can be adiabatically eliminated, the model reduces to a
self-consistent equation for the probability distribution of the atomic
"phases". In this limit, there exists a formal equivalence with the Kuramoto
model, though with important differences in the self-consistency conditions.
Depending on the field-cavity detuning, we show that the onset of synchronized
behavior may occur through either a first- or second-order phase transition.
Furthermore, we find a secondary threshold, above which a periodic self-pulsing
regime sets in, that is immediately followed by the unlocking of the
forward-field frequency. At yet higher, but still experimentally meaningful,
input intensities, irregular, chaotic oscillations may eventually appear.
Finally, we derive a simpler model, involving only five scalar variables, which
is able to reproduce the entire phenomenology exhibited by the original model.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:08:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Javaloyes",
"J.",
""
],
[
"Perrin",
"M.",
""
],
[
"Politi",
"A.",
""
]
] | [
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] |
712.1774 | Christian Di Fidio | C. Di Fidio, W. Vogel, M. Khanbekyan, D.-G. Welsch | Photon emission by an atom in a lossy cavity | null | Phys. Rev. A 77, 043822 (2008) | 10.1103/PhysRevA.77.043822 | null | quant-ph | null | The dynamics of an initially excited two-level atom in a lossy cavity is
studied by using the quantum trajectory method. Unwanted losses are included,
such as photon absorption and scattering by the cavity mirrors and spontaneous
emission of the atom. Based on the obtained analytical solutions, it is shown
that the shape of the extracted spatiotemporal radiation mode sensitively
depends on the atom-field interaction. In the case of a short-term atom-field
interaction we show how different pulse shapes for the field extracted from the
cavity can be controlled by the interaction time.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:14:46 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Apr 2008 16:13:31 GMT"
}
] | 2008-04-18T00:00:00 | [
[
"Di Fidio",
"C.",
""
],
[
"Vogel",
"W.",
""
],
[
"Khanbekyan",
"M.",
""
],
[
"Welsch",
"D. -G.",
""
]
] | [
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] |
712.1775 | Rachit Agarwal | Rachit Agarwal | On Computation of Error Locations and Values in Hermitian Codes | 10 pages, Submitted to ITW 2008 (with some minor modifications) | null | null | null | cs.IT math.IT | null | We obtain a technique to reduce the computational complexity associated with
decoding of Hermitian codes. In particular, we propose a method to compute the
error locations and values using an uni-variate error locator and an
uni-variate error evaluator polynomial. To achieve this, we introduce the
notion of Semi-Erasure Decoding of Hermitian codes and prove that decoding of
Hermitian codes can always be performed using semi-erasure decoding. The
central results are:
* Searching for error locations require evaluating an univariate error
locator polynomial over $q^2$ points as in Chien search for Reed-Solomon codes.
* Forney's formula for error value computation in Reed-Solomon codes can
directly be applied to compute the error values in Hermitian codes.
The approach develops from the idea that transmitting a modified form of the
information may be more efficient that the information itself.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:18:11 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Agarwal",
"Rachit",
""
]
] | [
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712.1776 | Yidong Chong | Zheng Wang, Y. D. Chong, John D. Joannopoulos, Marin Soljacic | Reflection-Free One-Way Edge Modes in a Gyromagnetic Photonic Crystal | 4 pages, 3 figures (Figs. 1 and 2 revised.) | Phys. Rev. Lett. 100, 013905 (2008) | 10.1103/PhysRevLett.100.013905 | null | physics.optics cond-mat.mes-hall | null | We point out that electromagnetic one-way edge modes analogous to quantum
Hall edge states, originally predicted by Raghu and Haldane in 2D gyroelectric
photonic crystals possessing Dirac point-derived bandgaps, can appear in more
general settings. In particular, we show that the TM modes in a gyromagnetic
photonic crystal can be formally mapped to electronic wavefunctions in a
periodic electromagnetic field, so that the only requirement for the existence
of one-way edge modes is that the Chern number for all bands below a gap is
non-zero. In a square-lattice gyromagnetic Yttrium-Iron-Garnet photonic crystal
operating at microwave frequencies, which lacks Dirac points, time-reversal
breaking is strong enough that the effect should be easily observable. For
realistic material parameters, the edge modes occupy a 10% band gap. Numerical
simulations of a one-way waveguide incorporating this crystal show 100%
transmission across strong defects, such as perfect conductors several lattice
constants wide, larger than the width of the waveguide.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:18:44 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 17:52:15 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Wang",
"Zheng",
""
],
[
"Chong",
"Y. D.",
""
],
[
"Joannopoulos",
"John D.",
""
],
[
"Soljacic",
"Marin",
""
]
] | [
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] |
712.1777 | Peng Gao | Peng Gao | Finite Sections of Weighted Hardy's Inequality | 14 pages | null | null | null | math.CA | null | We study finite sections of weighted Hardy's inequality following the
approach of De Bruijn. Similar to the unweighted case, we obtain an asymptotic
expression for the optimal constant.
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:20:36 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Gao",
"Peng",
""
]
] | [
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] |
712.1778 | Aram Mekjian | Aram Mekjian | Isospin and isospin/strangeness correlations in relativistic heavy ion
collisions | 11 pages | Eur.Phys.J.80:22002,2007 | 10.1209/0295-5075/80/22002 | null | nucl-th | null | A fundamental symmetry of nuclear and particle physics is isospin whose third
component is the Gell-Mann/Nishijima expression I(z)=Q-(B+S)/2 . The role of
isospin symmetry in relativistic heavy ion collisions is studied. An isospin
I(z), strangeness S correlation is shown to be a direct and simple measure of
flavor correlations, vanishing in a Qg phase of uncorrelated flavors in both
symmetric N=Z and asymmetric N not equal to Z systems. By contrast, in a hadron
phase, a I(z)/S correlation exists as long as the electrostatic charge chemical
potential mu(Q)does not equal 0 as in N not equal to Z asymmetric systems. A
parallel is drawn with a Zeeman effect which breaks a spin degeneracy
| [
{
"version": "v1",
"created": "Tue, 11 Dec 2007 17:25:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mekjian",
"Aram",
""
]
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