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712.0679 | Jean-Marc Bardet | Jean-Marc Bardet (CES, Matisse, Samos), Olivier Wintenberger (CES,
Matisse, Samos) | Asymptotic normality of the Quasi Maximum Likelihood Estimator for
multidimensional causal processes | null | The Annals of Statistics (2009) 1-32 | null | null | math.ST stat.TH | null | Strong consistency and asymptotic normality of the Quasi-Maximum Likelihood
Estimator (QMLE) are given for a general class of multidimensional causal
processes. For particular cases already studied in the literature (for instance
univariate or multivariate GARCH, ARCH, ARMA-GARCH processes) the assumptions
required for establishing these results are often weaker than existing
conditions. The QMLE asymptotic behavior is also given for numerous new
examples of univariate or multivariate processes (for instance TARCH or NLARCH
processes).
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:21:16 GMT"
}
] | 2009-01-09T00:00:00 | [
[
"Bardet",
"Jean-Marc",
"",
"CES, Matisse, Samos"
],
[
"Wintenberger",
"Olivier",
"",
"CES,\n Matisse, Samos"
]
] | [
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] |
712.068 | Claudio Grillo | C. Grillo, R. Gobat, P. Rosati, and M. Lombardi | Stellar mass estimates in early-type galaxies from lensing+dynamical and
photometric measurements | 4 pages, 2 figures, accepted by Astronomy & Astrophysics | null | 10.1051/0004-6361:20078934 | null | astro-ph | null | In this paper we compare two different diagnostics for estimating stellar
masses in early-type galaxies and we establish their level of reliability. In
particular, we consider the well-studied sample of 15 field elliptical galaxies
selected from the Sloan Lens ACS (SLACS) Survey (z = 0.06-0.33). We examine
here the correlation between the stellar mass values, enclosed inside the
Einstein radius of each lens, based on analyses of lensing and stellar dynamics
combined and based on multiwavelength photometry spectral template fitting. The
lensing+dynamics stellar mass is obtained from the published SLACS Survey
results, assuming a two-component density distribution model and a prior from
the fundamental plane on the mass-to-light ratio for the lens galaxies. The
photometric stellar mass is measured by fitting the observed spectral energy
distribution of the galaxies (from the SDSS multi-band photometry over 354-913
nm) with composite stellar population templates, under the assumption that
light traces stellar mass. The two methods are completely independent. They
rely on several different assumptions, and so, in principle, both can have
significant biases. Based on our sample of massive galaxies, we find
consistency between the lensing+dynamics and the photometric mass estimates. We
obtain a Pearson linear correlation coefficient of 0.94 and a median value of
the ratio between the former and the latter mass measurements of 1.1+/-0.1.
This suggests that both methods can separately yield reliable stellar masses of
early-type galaxies, and confirms that photometric mass estimates are accurate,
as long as optical/near-IR rest frame photometry is available.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:34:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Grillo",
"C.",
""
],
[
"Gobat",
"R.",
""
],
[
"Rosati",
"P.",
""
],
[
"Lombardi",
"M.",
""
]
] | [
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712.0681 | Luca Guido Molinari | Luca G. Molinari | Determinants of Block Tridiagonal Matrices | 8 pages, final form. To appear on Linear Algebra and its Applications | Linear Algebra and its Applications 429 (2008) 2221-2226 | 10.1016/j.laa.2008.06.015 | null | math-ph math.MP math.NA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | An identity is proven that evaluates the determinant of a block tridiagonal
matrix with (or without) corners as the determinant of the associated transfer
matrix (or a submatrix of it).
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:23:40 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 15:33:13 GMT"
},
{
"version": "v3",
"created": "Mon, 16 Jun 2008 07:23:31 GMT"
}
] | 2008-09-03T00:00:00 | [
[
"Molinari",
"Luca G.",
""
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] |
712.0682 | Daniel Buchholz | D. Buchholz, P. Drouvelis and P. Schmelcher | Tunable transmission via quantum state evolution in oval quantum dots | 5 pages, 3 figures, accepted for publication in EPL | null | 10.1209/0295-5075/81/37001 | null | cond-mat.mes-hall | null | We explore the quantum transmission through open oval shaped quantum dots.
The transmission spectra show periodic resonances and, depending on the
geometry parameter, a strong suppression of the transmission for low energies.
Applying a weak perpendicular magnetic field changes this situation drastically
and introduces a large conductance. We identify the underlying mechanisms being
partially due to the specific shape of the oval that causes a systematic
decoupling of a substantial number of states from the leads. Importantly a
pairwise destructive interference of the transmitting states is encountered
thereby leading to the complete conductance suppression. Coupling properties
and interferences can be tuned via a weak magnetic field. These properties are
robust with respect to the presence of disorder in the quantum dot.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:35:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Buchholz",
"D.",
""
],
[
"Drouvelis",
"P.",
""
],
[
"Schmelcher",
"P.",
""
]
] | [
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] |
712.0683 | Ghanashyam Date | Kinjal Banerjee and Ghanashyam Date | Loop Quantization of Polarized Gowdy Model on $T^3$: Classical Theory | 20 pages, no figures. Final version; to appear in Classical and
Quantum Gravity. Additional References included | Class.Quant.Grav.25:105014,2008 | 10.1088/0264-9381/25/10/105014 | IMSc/2007/12/15 | gr-qc hep-th | null | The vacuum Gowdy models provide much studied, non-trivial midi-superspace
examples. Various technical issues within Loop Quantum Gravity can be studied
in these models as well as one can hope to understand singularities and their
resolution in the loop quantization. The first step in this program is to
reformulate the model in real connection variables in a manner that is amenable
to loop quantization. We begin with the unpolarized model and carry out a
consistent reduction to the polarized case. Carrying out complete gauge fixing,
the known solutions are recovered.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:53:38 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Apr 2008 12:31:03 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Banerjee",
"Kinjal",
""
],
[
"Date",
"Ghanashyam",
""
]
] | [
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712.0684 | Anton Baranov | Anton D. Baranov | Compact embeddings of model subspaces of the Hardy space | 26 pages | Izvestia Mathematics, 73 (2009), 6, 1077-1100 (revised version) | 10.1070/IM2009v073n06ABEH002473 | null | math.CV math.FA | null | We study embeddings of model (star-invariant) subspaces $K^p_{\Theta}$ of the
Hardy space $H^p$, associated with an inner function $\Theta$. We obtain a
criterion for the compactness of the embedding of $K^p_{\Theta}$ into
$L^p(\mu)$ analogous to the Volberg--Treil theorem on bounded embeddings and
answer a question posed by Cima and Matheson. The proof is based on Bernstein
inequalities for functions in $K^p_{\Theta}$. Also we study measures $\mu$ such
that the embedding operator belongs to a Schatten--von Neumann ideal.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:41:53 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Baranov",
"Anton D.",
""
]
] | [
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] |
712.0685 | Felix Finster | Felix Finster | From Discrete Space-Time to Minkowski Space: Basic Mechanisms, Methods
and Perspectives | 25 pages, LaTeX, 6 figures, minor improvements (published version) | "Quantum Field Theory," B. Fauser et al. (eds.), Birkh\"auser
(2009) 235-259 | 10.1007/978-3-7643-8736-5_14 | null | math-ph math.MP | null | This survey article reviews recent results on fermion system in discrete
space-time and corresponding systems in Minkowski space. After a basic
introduction to the discrete setting, we explain a mechanism of spontaneous
symmetry breaking which leads to the emergence of a discrete causal structure.
As methods to study the transition between discrete space-time and Minkowski
space, we describe a lattice model for a static and isotropic space-time,
outline the analysis of regularization tails of vacuum Dirac sea
configurations, and introduce a Lorentz invariant action for the masses of the
Dirac seas. We mention the method of the continuum limit, which allows to
analyze interacting systems. Open problems are discussed.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:46:01 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 14:28:37 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Finster",
"Felix",
""
]
] | [
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712.0686 | Koji Nagata | Koji Nagata and Jaewook Ahn | Violation of Rotational Invariance of Local Realistic Models with Two
Settings | 4 pages | J. Korean Phys. Soc. 53, 2216 (2008) | 10.3938/jkps.53.2216 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have considered a two-particle Bell experiment to visualize the conflict
between rotational invariance of physical laws and a specific local realistic
theory. The experiment is reproducible by using a local realistic theory
obtained in a two-setting Bell experiment. The generalized Bell inequality {[J.
Phys. A: Math. Theor. {\bf 40}, 13101 (2007)]}, which is derived under the
assumption that there exists a rotationally invariant local realistic theory,
turns out to disprove such a local realistic model existing with a two-setting
experiment. This implies that such a model is not rotationally invariant and
should, therefore, be ruled out in some situations.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:46:52 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 05:37:12 GMT"
},
{
"version": "v3",
"created": "Wed, 13 Aug 2008 07:11:35 GMT"
},
{
"version": "v4",
"created": "Sat, 22 Nov 2008 08:14:54 GMT"
}
] | 2018-02-14T00:00:00 | [
[
"Nagata",
"Koji",
""
],
[
"Ahn",
"Jaewook",
""
]
] | [
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] |
712.0687 | Ghanashyam Date | Kinjal Banerjee and Ghanashyam Date | Loop Quantization of Polarized Gowdy Model on $T^3$: Kinematical States
and Constraint Operators | 26 pages, no figures. Version 2 accepted for publication. This has
the sub-title changed, introduction modified for comments on references,
small errors corrected and references updated | Class.Quant.Grav.25:145004,2008 | 10.1088/0264-9381/25/14/145004 | IMSc/2007/12/16 | gr-qc hep-th | null | In this second paper on loop quantization of Gowdy model, we introduce the
kinematical Hilbert space on which appropriate holonomies and fluxes are well
represented. The quantization of the volume operator and the Gauss constraint
is straightforward. Imposition of the Gauss constraint can be done on the
kinematical Hilbert space to select subspace of gauge invariant states. We
carry out the quantization of the Hamiltonian constraint making specific
choices. Alternative choices are briefly discussed. It appears that to get
spatial correlations reflected in the Hamiltonian constraint, one may have to
adopt the so called `effective operator viewpoint'.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:47:23 GMT"
},
{
"version": "v2",
"created": "Mon, 2 Jun 2008 09:43:07 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Banerjee",
"Kinjal",
""
],
[
"Date",
"Ghanashyam",
""
]
] | [
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] |
712.0688 | Parthanil Roy | Parthanil Roy | Ergodic Theory, Abelian Groups, and Point Processes Induced by Stable
Random Fields | To appear in the Annals of Probability. Some typos are fixed and
Remark 4.3 (due to Jan Rosinski) is added in the second version | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider a point process sequence induced by a stationary symmetric
alpha-stable (0 < alpha < 2) discrete parameter random field. It is easy to
prove, following the arguments in the one-dimensional case in Resnick and
Samorodnitsky (2004), that if the random field is generated by a dissipative
group action then the point process sequence converges weakly to a cluster
Poisson process. For the conservative case, no general result is known even in
the one-dimensional case. We look at a specific class of stable random fields
generated by conservative actions whose effective dimensions can be computed
using the structure theorem of finitely generated abelian groups. The
corresponding point processes sequence is not tight and hence needs to be
properly normalized in order to ensure weak convergence. This weak limit is
computed using extreme value theory and some counting techniques.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:48:45 GMT"
},
{
"version": "v2",
"created": "Thu, 2 Jul 2009 00:03:59 GMT"
}
] | 2009-07-02T00:00:00 | [
[
"Roy",
"Parthanil",
""
]
] | [
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712.0689 | Horatiu Stefan Nastase | Horatiu Nastase | Introduction to AdS-CFT | 133 pages, 13 figures; typos corrected, references added | null | null | null | hep-th | null | These lectures present an introduction to AdS-CFT, and are intended both for
begining and more advanced graduate students, which are familiar with quantum
field theory and have a working knowledge of their basic methods. Familiarity
with supersymmetry, general relativity and string theory is helpful, but not
necessary, as the course intends to be as self-contained as possible. I will
introduce the needed elements of field and gauge theory, general relativity,
supersymmetry, supergravity, strings and conformal field theory. Then I
describe the basic AdS-CFT scenario, of ${\cal N}=4 $ Super Yang-Mills's
relation to string theory in $AdS_5\times S_5$, and applications that can be
derived from it: 3-point functions, quark-antiquark potential, finite
temperature and scattering processes, the pp wave correspondence and spin
chains. I also describe some general properties of gravity duals of gauge
theories.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:51:01 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 04:42:24 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Nastase",
"Horatiu",
""
]
] | [
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] |
712.069 | Mathieu Servillat | M. Servillat, N. A. Webb, D. Barret | XMM-Newton observations of the Galactic globular clusters NGC 2808 and
NGC 4372 | 11 pages, 3 pages of online material, 10 figures and 9 tables.
Accepted for publication in A&A | null | 10.1051/0004-6361:20078327 | null | astro-ph | null | Galactic globular clusters harbour binary systems that are detected as faint
X-ray sources. These close binaries are thought to play an important role in
the stability of the clusters by liberating energy and delaying the inevitable
core collapse of globular clusters. The inventory of close binaries and their
identification is therefore essential. We present XMM-Newton observations of
two Galactic globular clusters: NGC 2808 and NGC 4372. We use X-ray spectral
and variability analysis combined with ultra-violet observations made with the
XMM-Newton optical monitor and published data from the Hubble Space Telescope
to identify sources associated with the clusters. We compare the results of our
observations with estimates from population synthesis models. Five sources out
of 96 are likely to be related to NGC 2808. Nine sources are found in the field
of view of NGC 4372, none being located inside its half-mass radius. We find
one quiescent neutron star low mass X-ray binary candidate in the core of NGC
2808, and propose that the majority of the central sources in NGC 2808 are
cataclysmic variables. An estimation leads to ~20+/-10 cataclysmic variables
with luminosity above 4.25 x 10^31 erg s^-1. Millisecond pulsars could also be
present in the core of NGC 2808, and some sources outside of the half-mass
radius could possibly be linked to the cluster.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 10:53:55 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 13:31:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Servillat",
"M.",
""
],
[
"Webb",
"N. A.",
""
],
[
"Barret",
"D.",
""
]
] | [
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] |
712.0691 | Marcelo Buffoni | Marcelo Buffoni (INRIA Futurs), Haysam Telib (DIASP), Angelo Iollo
(INRIA Futurs) | Iterative Methods for Model Reduction by Domain Decomposition | null | null | null | null | physics.class-ph | null | We propose a method to reduce the computational effort to solve a partial
differential equation on a given domain. The main idea is to split the domain
of interest in two subdomains, and to use different approximation methods in
each of the two subdomains. In particular, in one subdomain we discretize the
governing equations by a canonical scheme, whereas in the other one we solve a
reduced order model of the original problem. Different approaches to couple the
low-order model to the usual discretization are presented. The effectiveness of
these approaches is tested on numerical examples pertinent to non-linear model
problems including the Laplace equation with non-linear boundary conditions and
the compressible Euler equations.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:04:46 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Buffoni",
"Marcelo",
"",
"INRIA Futurs"
],
[
"Telib",
"Haysam",
"",
"DIASP"
],
[
"Iollo",
"Angelo",
"",
"INRIA Futurs"
]
] | [
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] |
712.0692 | Jochen Heinloth | Jochen Heinloth | Bounds for Behrend's conjecture on the canonical reduction | Erroneous claim about orthogonal bundles in characteristic 2 removed | null | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove Behrend's conjecture on the rationality of the canonical reduction
of principal bundles and reductive group schemes for classical groups and give
new bounds for the conjecture for exceptional groups. However we find a
counterexample in the case of G_2-bundles in characteristic 2.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:09:30 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Nov 2008 21:41:22 GMT"
}
] | 2008-11-03T00:00:00 | [
[
"Heinloth",
"Jochen",
""
]
] | [
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] |
712.0693 | Chengqing Li | Chengqing Li, Dan Zhang, and Guanrong Chen | Cryptanalysis of an image encryption scheme based on the Hill cipher | 10 pages, three figures | null | 10.1631/jzus.A0720102 | null | cs.CR | null | This paper studies the security of an image encryption scheme based on the
Hill cipher and reports its following problems: 1) there is a simple necessary
and sufficient condition that makes a number of secret keys invalid; 2) it is
insensitive to the change of the secret key; 3) it is insensitive to the change
of the plain-image; 4) it can be broken with only one known/chosen-plaintext;
5) it has some other minor defects.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:11:16 GMT"
}
] | 2009-12-21T00:00:00 | [
[
"Li",
"Chengqing",
""
],
[
"Zhang",
"Dan",
""
],
[
"Chen",
"Guanrong",
""
]
] | [
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] |
712.0694 | Yijun He | Yijun He, Haizhong Li, Hui Ma, Jianquan Ge | Compact embedded hypersurfaces with constant higher order anisotropic
mean curvatures | 15 pages | null | null | null | math.DG | null | Given a positive function $F$ on $S^n$ which satisfies a convexity condition,
for $1\leq r\leq n$, we define the $r$-th anisotropic mean curvature function
$H^F_r$ for hypersurfaces in $\mathbb{R}^{n+1}$ which is a generalization of
the usual $r$-th mean curvature function. We prove that a compact embedded
hypersurface without boundary in $\R^{n+1}$ with $H^F_r={constant}$ is the
Wulff shape, up to translations and homotheties. In case $r=1$, our result is
the anisotropic version of Alexandrov Theorem, which gives an affirmative
answer to an open problem of F. Morgan.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:21:40 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 10:33:49 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"He",
"Yijun",
""
],
[
"Li",
"Haizhong",
""
],
[
"Ma",
"Hui",
""
],
[
"Ge",
"Jianquan",
""
]
] | [
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] |
712.0695 | S\'andor Borb\'ely | S. Borb\'ely, K. T\H{o}k\'esi, L. Nagy | Ionization of the hydrogen atom by intense ultrashort laser pulses | submited to PRA | null | 10.1103/PhysRevA.77.033412 | null | physics.atom-ph physics.comp-ph | null | The ionization of atomic hydrogen in intense laser fields is studied
theoretically. The calculations were performed applying both quantummechanical
and classical approaches. Treating the problem quantummechanically, the time
dependent Schr\"odinger equation (TDSE) of our system was first transformed
into a pseudo-momentum space and solved in this space iteratively. While
neglecting the Coulomb potential during the solution of the TDSE we got the
results in the Volkov approximation, in the first order solution we taken into
account the Coulomb potential as perturbation. The classical calculations were
performed within the framework of the classical trajectory Monte-Carlo (CTMC)
method.
The double differential ionization probabilities are calculated for different
laser pulses and a reasonable agreement was found between the theories. Major
differences can be observed in the angular distribution of electrons at low
electron energies between classical and the quantummechanical approaches. At
high electron energies the differences disappear, which indicates that the
generation of low energy electrons is of quantum type, and it is strongly
influenced by the Coulomb potential, while the production of high energy
electrons is of classical type and it is less influenced by the Coulomb
interaction. Our results are also compared with the Coulomb-Volkov (CV) model
calculations.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:31:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Borbély",
"S.",
""
],
[
"Tőkési",
"K.",
""
],
[
"Nagy",
"L.",
""
]
] | [
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] |
712.0696 | Alexander Schegerer | A. A. Schegerer, S. Wolf, Th. Ratzka, and Ch. Leinert | The T Tauri star RY Tau as a case study of the inner regions of
circumstellar dust disks | 19 pages, 23 figures; accepted by Astronomy & Astrophysics | null | 10.1051/0004-6361:20077049 | null | astro-ph | null | We study the inner region of the circumstellar disk around the TTauri star RY
Tau. Our aim is to find a physical description satisfying the available
interferometric data, obtained with the mid-infrared interferometric instrument
at the Very Large Telescope Interferometer, as well as the spectral energy
distribution. We also compare the findings with the results of similar studies,
including those of intermediate-mass stars. Our analysis is done within the
framework of a passive circumstellar disk, which is optionally supplemented by
the effects of accretion and an added envelope. To achieve a more consistent
and realistic model, we used our continuum transfer code MC3D. In addition, we
studied the shape of the 10um silicate emission feature in terms of the
underlying dust population, both for single-dish and for interferometric
measurements. We show that a modestly flaring disk model with accretion can
explain both the observed spectral energy distribution and the mid-infrared
visibilities obtained with the mid-infrared infrared instrument. We found an
interesting ambiguity: a circumstellar active disk model with an added
envelope, and a lower accretion rate than in the active disk model without
envelope, could represent the observations equally as well. This type of model
with the envelope should be considered a viable alternative in future models of
other TTauri stars. The approach of a disk with a puffed-up inner rim wall and
the influence of a stellar companion is also discussed. From the study of the
silicate emission feature we see evidence for dust evolution in a TTauri star,
with a decreasing fraction of small amorphous and an increasing fraction of
crystalline particles closer to the star.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:48:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schegerer",
"A. A.",
""
],
[
"Wolf",
"S.",
""
],
[
"Ratzka",
"Th.",
""
],
[
"Leinert",
"Ch.",
""
]
] | [
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712.0697 | Ambar Ghosal | Debasish Majumdar and Ambar Ghosal | Investigating Possible Neutrino Decay in Long Baseline Experiment Using
ICAL as Far end Detector | 7 pages LaTeX, 4 pdf figures | null | null | null | hep-ph | null | We investigate the effects of possible decay of neutrinos from a neutrino
factory in a long baseline experiment. We consider the neutrinos from a factory
at CERN and the detector to be the 50 kTon iron calorimeter (ICAL) detector
proposed for India-based Neutrino Observatory (INO). We found considerable
depletion of muon yield at INO for certain value of decay parameters.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:49:34 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Dec 2007 06:52:50 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Majumdar",
"Debasish",
""
],
[
"Ghosal",
"Ambar",
""
]
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] |
712.0698 | Carolina Romero-Redondo | C. Romero-Redondo, E. Garrido, D.V. Fedorov, A.S. Jensen | Isomeric 0- halo-states in 12Be and 11Li | to be published in Physics Letters B | Phys.Lett.B660:32-36,2008 | 10.1016/j.physletb.2007.12.014 | null | nucl-th | null | We predict the existence of an isomeric 0$^-$-state in $^{12}$Be at an
excitation energy of about 2.5 MeV, and a 0$^-$-resonance in $^{11}$Li with
both energy and width of about 1 MeV corresponding to two-neutron emission. The
structure of these halo-like states are like the 1$^-$-states which means
essentially a core surrounded by two neutrons in single-particle $s$ and
p-states. The life-time of the $^{12}$Be state is determined by $M1$ or
$M2$-emission, $\tau(M1) \approx 10^{-11}$ s or $\tau(M2) \approx 10^{-8}$ s
estimated for photon energies of 0.1 MeV and 0.6 MeV, respectively.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 11:58:10 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Romero-Redondo",
"C.",
""
],
[
"Garrido",
"E.",
""
],
[
"Fedorov",
"D. V.",
""
],
[
"Jensen",
"A. S.",
""
]
] | [
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] |
712.0699 | Vlad Avrigeanu | M. Avrigeanu (1), S. V. Chuvaev (2), A. A. Filatenkov (2), R. A.
Forrest (3), M. Herman (4), A.J. Koning (5), A. J. M. Plompen (6), F. L.
Roman (1), V. Avrigeanu (1) ((1) "Horia Hulubei" National Institute for
Physics and Nuclear Engineering, Bucharest, (2) V.G. Khlopin Radium
Institute, St. Petersburg, (3) EURATOM-UKAEA Fusion Association, Culham
Science Centre, Culham, (4) Brookhaven National Laboratory, Upton, (5)
Nuclear Research and Consultancy Group NRG, Petten, (6) European Commission,
Joint Research Center, Institute for Reference Materials and Measurements,
Geel) | Fast-neutron induced pre-equilibrium reactions on 55Mn and 63,65Cu at
energies up to 40 MeV | 39 pages, 12 figures | Nucl.Phys.A806:15-39,2008 | 10.1016/j.nuclphysa.2008.03.010 | null | nucl-ex | null | Excitation functions were measured for the $^{55}$Mn(n,2n)$^{54}$Mn,
$^{55}$Mn(n,$\alpha$)$^{52}$V, $^{63}$Cu(n,$\alpha$)$^{60}$Co,
$^{65}$Cu(n,2n)$^{64}$Cu, and $^{65}$Cu(n,p)$^{65}$Ni reactions from 13.47 to
14.83 MeV. The experimental cross sections are compared with the results of
calculations including all activation channels for the stable isotopes of Mn
and Cu, for neutron incident energies up to 50 MeV. Within the energy range up
to 20 MeV the model calculations are most sensitive to the parameters related
to nuclei in the early stages of the reaction, while the model assumptions are
better established by analysis of the data in the energy range 20-40 MeV. While
the present analysis has taken advantage of both a new set of accurate measured
cross sections around 14 MeV and the larger data basis fortunately available
between 20 and 40 MeV for the Mn and Cu isotopes, the need of additional
measurements below as well as above 40 MeV is pointed out. Keywords: 55Mn,
63,65Cu, E$\leq$40 MeV, Neutron activation cross section measurements, Nuclear
reactions, Model calculations, Manganese, Copper
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:02:26 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Avrigeanu",
"M.",
""
],
[
"Chuvaev",
"S. V.",
""
],
[
"Filatenkov",
"A. A.",
""
],
[
"Forrest",
"R. A.",
""
],
[
"Herman",
"M.",
""
],
[
"Koning",
"A. J.",
""
],
[
"Plompen",
"A. J. M.",
""
],
[
"Roman",
"F. L.",
""
],
[
"Avrigeanu",
"V.",
""
]
] | [
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712.07 | Yuta Kodama | Yuta Kodama, Kento Kokubu, and Nobuyuki Sawado | Localizing gravity on Maxwell gauged CP1 model in six dimensions | 23 pages, 7 figures; references added | Phys.Rev.D78:045001,2008 | 10.1103/PhysRevD.78.045001 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We shall consider about a 3-brane embedded in six-dimensional space-time with
a negative bulk cosmological constant. The 3-brane is constructed by a
topological soliton solution living in two-dimensional axially symmetric
transverse subspace. Similar to most previous works of six-dimensional soliton
models, our Maxwell gauged CP1 brane model can also achieve to localize gravity
around the 3-brane. The CP1 field is described by a scalar doublet and derived
from O(3) sigma model by projecting it onto two-dimensional complex space. In
that sense, our framework is more effective than other solitonic brane models
concerning with gauge theory. We shall also discuss about linear stability
analysis for our new model by fluctuating all fields.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:09:48 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jul 2008 11:10:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kodama",
"Yuta",
""
],
[
"Kokubu",
"Kento",
""
],
[
"Sawado",
"Nobuyuki",
""
]
] | [
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] |
712.0701 | Marcella Di Criscienzo Miss | M. Di Criscienzo, M. Marconi, F. Caputo, S. Cassisi | Pulsational models of BL Her stars | 3 pages, 2 greyscale figures. Proceedings of the workshop "XXI
Century challenges for stellar evolution", held in Cefalu' (Sicily, Italy),
August 29 - September 2, 2007; S. Cassisi and M. Salaris Eds. To be published
in Mem. SAIt Vol. 79 No. 2 | null | null | null | astro-ph | null | We present an updated and homogeneous pulsational scenario for a wide range
of stellar parameters typical of BL Her stars i.e., Population II Cepheids with
periods shorter than 8 days.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:26:13 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Di Criscienzo",
"M.",
""
],
[
"Marconi",
"M.",
""
],
[
"Caputo",
"F.",
""
],
[
"Cassisi",
"S.",
""
]
] | [
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] |
712.0702 | Jeffrey Giansiracusa | Johannes Ebert, Jeffrey Giansiracusa | Pontrjagin-Thom maps and the homology of the moduli stack of stable
curves | 30 pages, 3 figures - v2: expanded material on homotopy types of
stacks, extended Pontrjagin-Thom construction to all local quotient stacks,
added references | null | null | null | math.AT math.AG | null | We study the singular homology (with field coefficients) of the moduli stack
of stable n-pointed complex curves of genus g (the Deligne-Mumford
compactification). Each of its irreducible boundary components determines via
the Pontrjagin-Thom construction a map to a certain infinite loop space whose
homology is well understood. We show that these maps are surjective on homology
in a range of degrees proportional to the genus. This implies the existence of
many new torsion classes in the homology of the moduli stack.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:18:56 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Apr 2008 11:57:58 GMT"
}
] | 2008-04-23T00:00:00 | [
[
"Ebert",
"Johannes",
""
],
[
"Giansiracusa",
"Jeffrey",
""
]
] | [
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] |
712.0703 | Ol'ga Galazutdinova A. | E.N. Tikhonov, O.A. Galazutdinova | Stellar population of the interacting galaxies M51 | 12 pages,9 figures, The International Conference "Cosmic Physics",
Special Astrophysical Observatory of the Russian Academy of Science, Nizhnij
Arkhyz, Karachaevo-Cherkesia, Russia, May 27-31, 2007 | null | null | null | astro-ph | null | Stellar photometry of about one million stars in the system of the
interacting galaxies M51 (NGC5194/NGC5195) has been carried out on the basis of
the ACS/WFC images of the Hubble Space telescope. The distance to the system
has been determined by TRGB method and metallicity of red supergiants along the
NGC5194 radius has been measured. A comparison of the spacial distribution of
stars in the main galaxy NGC5194 with our empirical model of spiral galaxies
showed their similarity, in spite of interaction in system M51. It has been
discovered that the "feathers", arising as a result of the interaction of
galaxies, mainly consist of stars of intermediate age.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:26:24 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Tikhonov",
"E. N.",
""
],
[
"Galazutdinova",
"O. A.",
""
]
] | [
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] |
712.0704 | Xavier Artru | X. Artru (IPNL), K. Benhizia | The High-Z hydrogen-like atom: a model for polarized structure functions | null | Prob.AtomicSci.Technol.3:98-103,2007 | null | null | nucl-th | null | The Dirac equation offers a precise analytical description of relativistic
two-particle bound states, when one of the constituent is very heavy and
radiative corrections are neglected. Looking at the high-Z hydrogen-like atom
in the infinite momentum frame and treating the electron as a "parton", various
properties usually attributed to the quark distributions in the nucleon are
tested, in particular: Bj{\o}rken scaling; charge, helicity, transversity and
momentum sum rules; existence of the parton sea; Soffer inequality; correlation
between spin and transverse momentum (Sivers and Boer-Mulders effects);
transverse displacement of the center-of-charge and its connection with the
magnetic moment. Deep inelastic experiments with photon or positron beams at
MeV energies, analogous to DIS or Drell-Yan reactions, are considered.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:36:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Artru",
"X.",
"",
"IPNL"
],
[
"Benhizia",
"K.",
""
]
] | [
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712.0705 | German Sierra | German Sierra | A quantum mechanical model of the Riemann zeros | 42 pages, 12 figures | NewJ.Phys.10:033016,2008 | 10.1088/1367-2630/10/3/033016 | null | math-ph cond-mat.other hep-th math.MP math.NT quant-ph | null | In 1999 Berry and Keating showed that a regularization of the 1D classical
Hamiltonian H = xp gives semiclassically the smooth counting function of the
Riemann zeros. In this paper we first generalize this result by considering a
phase space delimited by two boundary functions in position and momenta, which
induce a fluctuation term in the counting of energy levels. We next quantize
the xp Hamiltonian, adding an interaction term that depends on two wave
functions associated to the classical boundaries in phase space. The general
model is solved exactly, obtaining a continuum spectrum with discrete bound
states embbeded in it. We find the boundary wave functions, associated to the
Berry-Keating regularization, for which the average Riemann zeros become
resonances. A spectral realization of the Riemann zeros is achieved exploiting
the symmetry of the model under the exchange of position and momenta which is
related to the duality symmetry of the zeta function. The boundary wave
functions, giving rise to the Riemann zeros, are found using the Riemann-Siegel
formula of the zeta function. Other Dirichlet L-functions are shown to find a
natural realization in the model.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:38:21 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Sierra",
"German",
""
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712.0706 | Armin Rainer | Armin Rainer | Orbit projections of proper Lie groupoids as fibrations | LaTeX, 3 pages | Czechoslovak Math. J. 59 (2009), No. 3, 591--594. | null | null | math.DG math.AT | null | Let $\mathcal{G} \rightrightarrows M$ be a source locally trivial proper Lie
groupoid such that each orbit is of finite type. The orbit projection $M \to
M/\mathcal{G}$ is a fibration if and only if $\mathcal{G} \rightrightarrows M$
is regular.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:50:04 GMT"
}
] | 2010-03-30T00:00:00 | [
[
"Rainer",
"Armin",
""
]
] | [
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712.0707 | Jean-Luc Marichal | Alexander Dukhovny, Jean-Luc Marichal | System reliability and weighted lattice polynomials | Revised version (minor changes) | Probability in the Engineering and Informational Sciences 22 (3)
(2008) 373-388 | 10.1017/S0269964808000223 | null | math.PR math.RA | null | The lifetime of a system of connected units under some natural assumptions
can be represented as a random variable Y defined as a weighted lattice
polynomial of random lifetimes of its components. As such, the concept of a
random variable Y defined by a weighted lattice polynomial of (lattice-valued)
random variables is considered in general and in some special cases. The
central object of interest is the cumulative distribution function of Y. In
particular, numerous results are obtained for lattice polynomials and weighted
lattice polynomials in case of independent arguments and in general. For the
general case, the technique consists in considering the joint probability
generating function of "indicator" variables. A connection is studied between Y
and order statistics of the set of arguments.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:54:03 GMT"
},
{
"version": "v2",
"created": "Wed, 28 May 2008 14:06:30 GMT"
}
] | 2008-05-28T00:00:00 | [
[
"Dukhovny",
"Alexander",
""
],
[
"Marichal",
"Jean-Luc",
""
]
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] |
712.0708 | Francois Loeser | R. Cluckers, T. Hales, F. Loeser | Transfer Principle for the Fundamental Lemma | 31 pages | On the stabilization of the trace formula, 309-347, Stab. Trace
Formula Shimura Var. Arith. Appl., 1, Int. Press, Somerville, MA, 2011 | null | null | math.RT math.AG math.LO | null | The purpose of this paper is to explain how the identities of various
fundamental lemmas fall within the scope of the transfer principle, a general
result that allows to transfer theorems about identities of p-adic integrals
from one collection of fields to others. In particular, once the fundamental
lemma has been established for one collection of fields (for example, fields of
positive characteristic), it is also valid for others (fields of characteristic
zero).
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:56:55 GMT"
}
] | 2012-09-18T00:00:00 | [
[
"Cluckers",
"R.",
""
],
[
"Hales",
"T.",
""
],
[
"Loeser",
"F.",
""
]
] | [
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] |
712.0709 | Paola Castangia | P. Castangia (1, 2), A. Tarchi (2, 3), C. Henkel (1), K.M. Menten (1)
((1) Max-Planck-Institut fuer Radioastronomie, Bonn, (2) INAF-Osservatorio
Astronomico di Cagliari, (3) INAF-Istituto di Radioastronomia, Bologna) | New water masers in Seyfert and FIR bright galaxies. II | 12 pages, 9 figures, accepted by Astronomy and Astrophysics | null | null | null | astro-ph | null | Recently, a relationship between the water maser detection rate and far
infrared (FIR) flux density has been found as a result of a 22 GHz maser survey
in a sample comprised of northern galaxies with 100 micron flux density > 50 Jy
and a declination >-30 degrees. The survey has been extended toward galaxies
with lower FIR flux densities in order to confirm this correlation and to
discover additional maser sources for relevant follow-up interferometric
studies. A sample of 41 galaxies with 30 Jy < S(100 micron) < 50 Jy and Dec. >
-30 degrees was observed with the 100-m telescope at Effelsberg in a search for
the 22 GHz water vapor line. The average 3-sigma noise level of the survey is
40 mJy for a 1 km/s channel, corresponding to a detection threshold for the
isotropic maser luminosity of about 0.5 solar luminosities at a distance of 25
Mpc. Two detections are reported: a megamaser with an isotropic luminosity of
approximately 35 solar luminosities in the Seyfert/HII galaxy NGC613 and a
kilomaser of approximately 1 solar luminosity in the merger system
NGC520.[abridged]
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:57:11 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Castangia",
"P.",
""
],
[
"Tarchi",
"A.",
""
],
[
"Henkel",
"C.",
""
],
[
"Menten",
"K. M.",
""
]
] | [
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] |
712.071 | Pedro Castelo Ferreira Dr. | P. Castelo Ferreira | Canonical Functional Quantization of Pseudo-Photons in Planar Systems | 5 pages; 1 figure; submitted to Proceedings of XVI International Fall
Workshop on Geometry and Physics;
http://www.math.ist.utl.pt/~xvi-iwgp/talks/PedroCasteloF.pdf; v2: derivatives
on equation (10) corrected | AIPConf.Proc.1023:143-147,2008 | 10.1063/1.2958165 | null | hep-th math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Extended $U_e(1)\times U_g(1)$ electromagnetism containing both a photon and
a pseudo-photon is introduced at variational level and is justified by the
violation of the Bianchi identities in conceptual systems, either in the
presence of magnetic monopoles or non-regular external fields, not being
accounted by the standard Maxwell Lagrangian. It is carried a dimensional
reduction that renders a $U_e(1)\times U_g(1)$ Maxwell-BF type theory and it is
considered canonical functional quantization in planar systems which may be
relevant in Hall systems.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 12:58:10 GMT"
},
{
"version": "v2",
"created": "Fri, 10 Apr 2009 17:50:00 GMT"
}
] | 2009-04-10T00:00:00 | [
[
"Ferreira",
"P. Castelo",
""
]
] | [
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712.0711 | Pedro Castelo Ferreira Dr. | P. Castelo Ferreira | Pseudo-Photon Radiative Corrections in Non-Regular Backgrounds | 5 pages; 3 figures; based in hep-th/0510063 and hep-ph/0609239;
Submitted to Proceedings of New Worlds in Astroparticle Physics 2007 | null | null | null | hep-th | null | Extended $U_e(1)\times U_g(1)$ electromagnetism containing both a photon and
a pseudo-photon is introduced at variational level and is justified by the
violation of the Bianchi identities in conceptual systems, either in the
presence of magnetic monopoles or non-regular external fields, not being
accounted by the standard Maxwell action. It is shown that in the perturbative
quantum field theory regimes there are observable consequences both for the
magnetic momenta and second order vacuum polarization radiative corrections in
the presence of non-regular strong electromagnetic fields (e.g. rotating
magnetic fields).
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:11:40 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Ferreira",
"P. Castelo",
""
]
] | [
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] |
712.0712 | Ol'ga Galazutdinova A. | N. A. Tikhonov and O. A. Galazutdinova | Stellar Subsystems of the Galaxy NGC 2366 | 16 pages, 4 figures, Astronomy Reports, 2008,v. 52, n.1, p. 19 | null | 10.1134/S1063772908010034 | null | astro-ph | null | Hubble Space Telescope archive data are used to perform photometry of stars
in seven fields at the center and periphery of the galaxy NGC2366. The
variation of the number density of stars of various ages with galactocentric
radius and along the minor axis of the galaxy are determined. The boundaries of
the thin and thick disks of the galaxy are found. The inferred sizes of the
subsystems of NGC2366 ($Z_{thin} = 4$ kpc and $Z_{thick} = 8$ kpc for the thin
and thick disks, respectively) are more typical for spiral galaxies. Evidence
for a stellar halo is found at the periphery of NGC2366 beyond the thick disk
of the galaxy.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:16:58 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Dec 2007 07:23:04 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Tikhonov",
"N. A.",
""
],
[
"Galazutdinova",
"O. A.",
""
]
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0.0385161452,
0.0790648088,
-0.1246947497,
-0.0010948583,
-0.0094448393
] |
712.0713 | Luis Herrera | L. Herrera, J. Ospino and A. Di Prisco | All static spherically symmetric anisotropic solutions of Einstein's
equations | 8 pages Latex. To appear in Phys. Rev. D. New reference added. Some
references corrected | Phys.Rev.D77:027502,2008 | 10.1103/PhysRevD.77.027502 | null | gr-qc astro-ph | null | An algorithm recently presented by Lake to obtain all static spherically
symmetric perfect fluid solutions, is extended to the case of locally
anisotropic fluids (principal stresses unequal). As expected, the new formalism
requires the knowledge of two functions (instead of one) to generate all
possible solutions. To illustrate the method some known cases are recovered.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:17:29 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Dec 2007 22:11:04 GMT"
},
{
"version": "v3",
"created": "Tue, 15 Jan 2008 14:57:32 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Herrera",
"L.",
""
],
[
"Ospino",
"J.",
""
],
[
"Di Prisco",
"A.",
""
]
] | [
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712.0714 | Qasem Exirifard | Qasem Exirifard | Word-sheet corrections to dyons in string theories: A laboratory for the
strong OSV conjecture | This paper has been withdrawn | null | null | null | hep-th | null | The explicit computation of arXiv:hep-th/0112157 and arXiv:hep-th/0108106
prove that all the cubic alpha-prime corrections to the backgrounds composed of
metric, NS two-form and dilaton can not be written in term of the modified
Riemann tensor where the field strength of the NS two form plays the role of
torsion. So the outcome of this writing has been trivial.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:53:49 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 08:26:20 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Exirifard",
"Qasem",
""
]
] | [
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] |
712.0715 | Iain Stewart | Iain Stewart (Dept. of Computing, Imperial College, London, U.K.) | An iterated search for influence from the future on the Large Hadron
Collider | 18 pages, minor changes (mainly tracking N&N's title/notation changes
etc. in their latest revision of arXiv:0707.1919) | null | null | null | hep-ph hep-th | null | We analyse an iterated version of Nielsen and Ninomiya (N&N)'s proposed card
game experiment to search for a specific type of backward causation on the
running of the Large Hadron Collider (LHC) at CERN. We distinguish "endogenous"
and "exogenous" potential causes of failure of LHC and we discover a curious
"cross-talk" between their respective probabilities and occurrence timescales
when N&N-style backward causation is in effect. Finally, we note a kind of
"statistical cosmic censorship" preventing the influence from the future from
showing up in a statistical analysis of the iterated runs.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 18:16:32 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 20:28:12 GMT"
}
] | 2007-12-16T00:00:00 | [
[
"Stewart",
"Iain",
"",
"Dept. of Computing, Imperial College, London, U.K."
]
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0.0201783925,
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0.0118421456,
0.0415721647,
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] |
712.0716 | Ivan Smirnov | I.L. Drichko, A.M. Dyakonov, I.Yu. Smirnov, A.V. Suslov, Y.M.
Galperin, V. Vinokur, M. Myronov, O.A. Mironov, and D.R. Leadley | Magnetotransport in low-density $p$-Si/SiGe heterostructures: From metal
through hopping insulator to Wigner glass | 11 pages, 14 figures | null | 10.1103/PhysRevB.77.085327 | null | cond-mat.mes-hall | null | We study DC and AC transport in low-density $p-$Si/SiGe heterostructures at
low temperatures and in a broad domain of magnetic fields up to 18 T. Complex
AC conductance is determined from simultaneous measurement of velocity and
attenuation of a surface acoustic wave propagating in close vicinity of the 2D
hole layer. The observed behaviors of DC and AC conductance are interpreted as
an evolution from metallic conductance at B=0 through hopping between localized
states in intermediate magnetic fields (close to the plateau of the integer
quantum Hall effect corresponding to the Landau-level filling factor $\nu$=1)
to formation of the Wigner glass in the extreme quantum limit ($B\gtrsim 14$,
$T \lesssim 0.8$ K).
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:32:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Drichko",
"I. L.",
""
],
[
"Dyakonov",
"A. M.",
""
],
[
"Smirnov",
"I. Yu.",
""
],
[
"Suslov",
"A. V.",
""
],
[
"Galperin",
"Y. M.",
""
],
[
"Vinokur",
"V.",
""
],
[
"Myronov",
"M.",
""
],
[
"Mironov",
"O. A.",
""
],
[
"Leadley",
"D. R.",
""
]
] | [
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] |
712.0717 | Noam Gross | Noam Gross and Lev Khaykovich | All-optical production of 7Li Bose-Einstein condensation using Feshbach
resonances | 5 pages, 5 figures | Phys. Rev. A 77 023604 (2008) | 10.1103/PhysRevA.77.023604 | null | physics.atom-ph | null | We show an all-optical method of making 7Li condensate using tunability of
the scattering length in the proximity of a Feshbach resonance. We report the
observation of two new Feshbach resonances on |F = 1;mF = 0> state. The narrow
(broad) resonance of 7 G (34 G) width is detected at 831 +- 4 G (884 +4 -13 G).
Position of the scattering length zero crossing between the resonances is found
at 836 +- 4 G. The broad resonance is shown to be favorable for run away
evaporation which we perform in a crossed-beam optical dipole trap. Starting
directly form the phase space density of a magneto-optical trap we observe a
Bose-Einstein condensation threshold in less than 3 s of forced evaporation.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:51:47 GMT"
}
] | 2010-09-07T00:00:00 | [
[
"Gross",
"Noam",
""
],
[
"Khaykovich",
"Lev",
""
]
] | [
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] |
712.0718 | Maria Massi | M. Massi, E. Ros, K. M. Menten, M. Kaufman Bernado', G.
Torricelli-Ciamponi, J. Neidhofer, A. Boden, D. Boboltz, A. Sargent, G.Torres | Interacting coronae of two T Tauri stars: first observational evidence
for solar-like helmet streamers | 7 pages, 3 figures, A&A in press | null | 10.1051/0004-6361:20078637 | null | astro-ph | null | Context {The young binary system V773 Tau A exhibits a persistent radio
flaring activity that gradually increases from a level of a few mJy at
apoastron to more than 100 mJy at periastron. Interbinary collisions between
very large (> 15 R) magnetic structures anchored on the two rotating stars of
the system have been proposed to be the origin of these periodic radio flares.
Magnetic structures extended over tens of stellar radii, that can also account
for the observed fast decay of the radio flares, seem to correspond to the
typical solar semi-open quite extended magnetic configurations called helmet
streamers.} Aims {We aim to find direct observational evidence for the
postulated, solar-like, coronal topologies.} Methods {We performed
seven-consecutive-day VLBI observations at 8.4 GHz using an array consisting of
the VLBA and the 100-m Effelsberg telescope.} Results {Two distintive
structures appear in the radio images here presented. They happen to be
associated with the primary and secondary stars of the V773 Tau A system. In
one image (Fig.2-B) the two features are extended up to 18 R each and are
nearly parallel revealing the presence of two interacting helmet streamers. One
image (Fig.2-E) taken a few hours after a flare monitored by the 100-m
Effelsberg telescope shows one elongated fading structure substantially rotated
with respect to those seen in the B run. The same decay scenario is seen in
Fig.2-G for the helmet streamer associated with the other star.} Conclusions
{This is the very first direct evidence revealing that even if the flare origin
is magnetic reconnection due to interbinary collision, both stars independently
emit in the radio range with structures of their own. These structures are
helmet streamers, observed for the first time in stars other than the Sun.}
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:42:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Massi",
"M.",
""
],
[
"Ros",
"E.",
""
],
[
"Menten",
"K. M.",
""
],
[
"Bernado'",
"M. Kaufman",
""
],
[
"Torricelli-Ciamponi",
"G.",
""
],
[
"Neidhofer",
"J.",
""
],
[
"Boden",
"A.",
""
],
[
"Boboltz",
"D.",
""
],
[
"Sargent",
"A.",
""
],
[
"Torres",
"G.",
""
]
] | [
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] |
712.0719 | Nikolaos Lazarides | N. Lazarides, G. P. Tsironis and M. Eleftheriou | Dissipative discrete breathers in rf SQUID metamaterials | 9 pages, 13 figures, submitted to Nonlinear Phenomena in Complex
Systems | Nonlinear Phenomena in Complex Systems 11 (2008) 250-258 | null | null | nlin.PS | null | The existence and stability of dissipative discrete breathers (DDBs) in rf
superconducting quantum interference device (SQUID) arrays in both one and two
dimensions is investigated numerically. In an rf SQUID array, the nonlinearity
which is intrinsic to each SQUID due to the presence of the Josephson junction
(on-site nonlinearity), along with the weak coupling of each SQUID to its
nearest neighbors through magnetic forces, result in the appearance of discrete
breathers. We analyze several discrete breather excitations, both in one and
two dimensions, which are subjected to unavoidable losses. These losses,
however, are counter-balanced by an external flux source leading to linearly
stable discrete breather structures up to relatively large coupling parameters.
We show that DDB excitations may locally alter the magnetic response of array
from paramagnetic to diamagnetic or vice versa, and that they are not destroyed
by increasing the dimensionality.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:46:14 GMT"
}
] | 2009-09-18T00:00:00 | [
[
"Lazarides",
"N.",
""
],
[
"Tsironis",
"G. P.",
""
],
[
"Eleftheriou",
"M.",
""
]
] | [
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] |
712.072 | Stuart Mangles | S. P. D. Mangles, A. G. R. Thomas, C. Bellei, A. E. Dangor, C.
Kamperidis, S. Kneip, S. R. Nagel, L. Willingale and Z. Najmudin | Self-guided wakefield experiments driven by petawatt class ultra-short
laser pulses | 15 pages, 8 figures | null | 10.1109/TPS.2008.2000961 | null | physics.plasm-ph physics.acc-ph | null | We investigate the extension of self-injecting laser wakefield experiments to
the regime that will be accessible with the next generation of petawatt class
ultra-short pulse laser systems. Using linear scalings, current experimental
trends and numerical simulations we determine the optimal laser and target
parameters, i.e. focusing geometry, plasma density and target length, that are
required to increase the electron beam energy (to > 1 GeV) without the use of
external guiding structures.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:46:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mangles",
"S. P. D.",
""
],
[
"Thomas",
"A. G. R.",
""
],
[
"Bellei",
"C.",
""
],
[
"Dangor",
"A. E.",
""
],
[
"Kamperidis",
"C.",
""
],
[
"Kneip",
"S.",
""
],
[
"Nagel",
"S. R.",
""
],
[
"Willingale",
"L.",
""
],
[
"Najmudin",
"Z.",
""
]
] | [
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] |
712.0721 | Jay Bartroff | Jay Bartroff | Asymptotically optimal multistage tests of simple hypotheses | Published in at http://dx.doi.org/10.1214/009053607000000235 the
Annals of Statistics (http://www.imstat.org/aos/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Statistics 2007, Vol. 35, No. 5, 2075-2105 | 10.1214/009053607000000235 | IMS-AOS-AOS0260 | math.ST stat.TH | null | A family of variable stage size multistage tests of simple hypotheses is
described, based on efficient multistage sampling procedures. Using a loss
function that is a linear combination of sampling costs and error
probabilities, these tests are shown to minimize the integrated risk to second
order as the costs per stage and per observation approach zero. A numerical
study shows significant improvement over group sequential tests in a binomial
testing problem.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:50:08 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Bartroff",
"Jay",
""
]
] | [
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712.0722 | Nilanjana Datta | Nilanjana Datta and Tony Dorlas | Classical capacity of quantum channels with general Markovian correlated
noise | null | Journal of Statistical Physics, vol. 134, nos. 5-6, pp. 1173-1195,
2009 | 10.1007/s10955-009-9726-0 | null | quant-ph | null | The classical capacity of a quantum channel with arbitrary Markovian
correlated noise is evaluated. For the general case of a channel with long-term
memory, which corresponds to a Markov chain which does not converge to
equilibrium, the capacity is expressed in terms of the communicating classes of
the Markov chain. For an irreducible and aperiodic Markov chain, the channel is
forgetful, and one retrieves the known expression for the capacity.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 13:56:33 GMT"
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] | 2015-05-13T00:00:00 | [
[
"Datta",
"Nilanjana",
""
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"Tony",
""
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712.0723 | Sukmoon Huh | Sukmoon Huh | Dominance of a Rational Map to the Coble Quartic | 11 pages, Remark 3.5 added, the title changed | null | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show the dominance of the restriction map from a moduli space of stable
sheaves on the projective plane to the Coble quartic. With the dominance and
the interpretation of a stable sheaf on the plane in terms of the hyperplane
arrangements, we expect to investigate the geometry of the Coble quartic.
| [
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{
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"created": "Wed, 5 Nov 2008 15:54:31 GMT"
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] | 2008-11-05T00:00:00 | [
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712.0724 | Richard Garner | Richard Garner | Understanding the small object argument | 42 pages; supersedes the earlier arXiv preprint math/0702290; v2:
final journal version, minor corrections only | Applied Categorical Structures 17 (2009), no. 3, pages 247-285 | 10.1007/s10485-008-9137-4 | null | math.CT math.AT | null | The small object argument is a transfinite construction which, starting from
a set of maps in a category, generates a weak factorisation system on that
category. As useful as it is, the small object argument has some problematic
aspects: it possesses no universal property; it does not converge; and it does
not seem to be related to other transfinite constructions occurring in
categorical algebra. In this paper, we give an "algebraic" refinement of the
small object argument, cast in terms of Grandis and Tholen's natural weak
factorisation systems, which rectifies each of these three deficiencies.
| [
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] |
712.0725 | Fernando Jorge Guti\'errez Pinheiro | F. J. G. Pinheiro (1) ((1) Centro de Astrof\'isica da Universidade do
Porto) | Seismic evolution of low/intermediate mass PMS stars | 4 pages, 5 figures, accepted for publication on A&A | null | 10.1051/0004-6361:20077136 | null | astro-ph | null | This article presents a study of the evolution of the internal structure and
seismic properties expected for low/intermediate mass Pre-Main Sequence (PMS)
stars. Seismic and non-seismic properties of PMS stars were analysed. This was
done using 0.8 to 4.4M$_\odot$ stellar models at stages ranging from the end of
the Hayashi track up to the Zero-Age Main-Sequence (ZAMS). This research
concludes that, for intermediate-mass stars (M$>$1.3M$_\odot$), diagrams
comparing the effective temperature ($T_{eff}$) against the small separation
can provide an alternative to Christensen-Dalsgaard (C-D) diagrams. The impact
of the metal abundance of intermediate mass stars (2.5-4.4M$_\odot$) has over
their seismic properties is also evaluated.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:11:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Pinheiro",
"F. J. G.",
""
]
] | [
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] |
712.0726 | Ruth Nicol | R. M. Nicol, S. C. Chapman, R. O. Dendy | The signature of evolving turbulence in quiet solar wind as seen by
ULYSSES | 16 pages, 12 figures, to be presented at Fall AGU 2007 in San
Fransisco | null | 10.1086/586732 | null | astro-ph | null | Solar wind fluctuations, such as magnetic field or velocity, show power law
power spectra suggestive both of an inertial range of intermittent turbulence
(with $\sim -5/3$ exponent) and at lower frequencies, of fluctuations of
coronal origin (with $\sim -1$ exponent). The ULYSSES spacecraft spent many
months in the quiet fast solar wind above the Sun's polar coronal holes in a
highly ordered magnetic field. We use statistical analysis methods such as the
generalized structure function (GSF) and extended self-similarity (ESS) to
quantify the scaling of the moments of the probability density function of
fluctuations in the magnetic field. The GSFs give power law scaling in the
``$f^{-1}$'' range of the form $<| y(t+\tau)-y(t)|^{m}>\sim\tau^{\zeta(m)}$,
but ESS is required to reveal scaling in the inertial range, which is of the
form $<| y(t+\tau)-y(t)|^{m}>\sim [g(\tau)]^{\zeta(m)}$. We find that $g(\tau)$
is independent of spacecraft position and
$g(\tau)\sim\tau^{-log_{10}(\tilde{\lambda}\tau)}$. The ``$f^{-1}$'' scaling
fluctuates with radial spacecraft position. This confirms that, whereas the
``$f^{-1}$'' fluctuations are directly influenced by the corona, the inertial
range fluctuations are consistent with locally evolving turbulence, but with an
``envelope'' $g(\tau)$, which captures the formation of the quiet fast solar
wind.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:38:09 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 15:55:47 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nicol",
"R. M.",
""
],
[
"Chapman",
"S. C.",
""
],
[
"Dendy",
"R. O.",
""
]
] | [
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] |
712.0727 | Norma Sanchez | Marina Ramon Medrano (1,2) and Norma G. Sanchez ((1) Observatoire de
Paris, LERMA, (2) Universidad Complutense de Madrid, Dept de Fisica Teorica) | Semiclassical and Quantum Black Holes and their Evaporation, de Sitter
and Anti-de Sitter Regimes, Gravitational and String Phase Transitions | review paper, no figures. to appear in Int Jour Mod Phys A | Int.J.Mod.Phys.A22:6089-6131,2007 | 10.1142/S0217751X07038669 | null | hep-th astro-ph gr-qc hep-ph | null | An effective string theory in physically relevant cosmological and black hole
space times is reviewed. Explicit computations of the quantum string entropy,
partition function and quantum string emission by black holes (Schwarzschild,
rotating, charged, asymptotically flat, de Sitter dS and AdS space times) in
the framework of effective string theory in curved backgrounds provide an
amount of new quantum gravity results as: (i) gravitational phase transitions
appear with a distinctive universal feature: a square root branch point
singularity in any space time dimensions. This is of the type of the de Vega -
Sanchez transition for the thermal self-gravitating gas of point particles.
(ii) There are no phase transitions in AdS alone. (iii) For $dS$ background,
upper bounds of the Hubble constant H are found, dictated by the quantum string
phase transition.(iv) The Hawking temperature and the Hagedorn temperature are
the same concept but in different (semiclassical and quantum) gravity regimes
respectively. (v) The last stage of black hole evaporation is a microscopic
string state with a finite string critical temperature which decays as usual
quantum strings do in non-thermal pure quantum radiation (no information
loss).(vi) New lower string bounds are given for the Kerr-Newman black hole
angular momentum and charge, which are entirely different from the upper
classical bounds. (vii) Semiclassical gravity states undergo a phase transition
into quantum string states of the same system, these states are duals of each
other in the precise sense of the usual classical-quantum (wave-particle)
duality, which is universal irrespective of any symmetry or isommetry of the
space-time and of the number or the kind of space-time dimensions.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:13:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Medrano",
"Marina Ramon",
""
],
[
"Sanchez",
"Norma G.",
""
]
] | [
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712.0728 | Denis Denisov | Denis Denisov, Vsevolod Shneer | Asymptotics for first-passage times of L\'evy processes and random walks | null | null | null | Eurandom research report 2006-017 | math.PR | null | We study the exact asymptotics for the distribution of the first time
$\tau_x$ a L\'evy process $X_t$ crosses a negative level $-x$. We prove that
$\mathbf P(\tau_x>t)\sim V(x)\mathbf P(X_t\ge 0)/t$ as $t\to\infty$ for a
certain function $V(x)$. Using known results for the large deviations of random
walks we obtain asymptotics for $\mathbf P(\tau_x>t)$ explicitly in both light
and heavy tailed cases. We also apply our results to find asymptotics for the
distribution of the busy period in an M/G/1 queue.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:13:52 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Denisov",
"Denis",
""
],
[
"Shneer",
"Vsevolod",
""
]
] | [
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] |
712.0729 | Marcella Di Criscienzo Miss | M. Di Criscienzo, C. Greco, M. Dall'Ora, V. Ripepi, G. Clementini, M.
Marconi, L. Federici, L. Di Fabrizio, I. Musella, L. Baldacci, M. Maio | NGC 2419: an "intergalactic wanderer" or a simple Galactic Globular
Cluster? | 3 pages, 2 greyscale figures. Proceedings of the workshop "XXI
Century challenges for stellar evolution", held in Cefalu' (Sicily, Italy),
August 29 - September 2, 2007; S. Cassisi and M. Salaris Eds. To be published
in Mem. SAIt Vol. 79 No. 2 | null | null | null | astro-ph | null | We have carried out a new photometric study of the remote Galactic globular
cluster NGC 2419, using proprietary and archive B,V,I time-series CCD
photometry of the cluster, that allowed us to discover a large number of new
variable stars and to obtain a new colour magnitude diagram that reaches V ~26
mag over a field of 50X43 square arcmin centered on NGC 2419. The new variables
include 39 RR Lyrae and 11 SX Phoenicis stars. The pulsation properties of the
new RR Lyrae stars confirm and strengthen the classification of NGC 2419 as an
Oosterhoff type II cluster.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:16:17 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Di Criscienzo",
"M.",
""
],
[
"Greco",
"C.",
""
],
[
"Dall'Ora",
"M.",
""
],
[
"Ripepi",
"V.",
""
],
[
"Clementini",
"G.",
""
],
[
"Marconi",
"M.",
""
],
[
"Federici",
"L.",
""
],
[
"Di Fabrizio",
"L.",
""
],
[
"Musella",
"I.",
""
],
[
"Baldacci",
"L.",
""
],
[
"Maio",
"M.",
""
]
] | [
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] |
712.073 | Mireille Calvet | Roland Omn\`es | Possible agreement of wave function reduction from the basic principles
of quantum mechanics | "A shorter and clearer version of the previous paper, with
improvements in the physical content" | null | null | LPT Orsay 08-25 | quant-ph | null | Reduction is shown to be a possible consequence of the basic principles of
quantum mechanics, involving no branching of the quantum state of the universe.
The key feature of a measurement is attributed to the creation of macroscopic
germs of ionized tracks, bubbles, sparks and so on, in a superposed quantum
state, the main mechanism being a breaking and a restoration of
``classicality'' in nearby macroscopic objects and their small patterns. A new
significance of quantum probabilities, involving no absolute randomness, is
also proposed.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:20:16 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 10:15:31 GMT"
}
] | 2008-02-19T00:00:00 | [
[
"Omnès",
"Roland",
""
]
] | [
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] |
712.0731 | Stefania Patrizi | Stefania Patrizi | The Neumann problem for singular fully nonlinear operators | null | null | null | null | math.AP | null | We consider the Neumann problem in $C^2$ bounded domains for fully nonlinear
second order operators which are elliptic, homogenous with lower order terms.
Inspired by \cite{bnv}, we define the concept of principal eigenvalue and we
characterize it through the maximum principle. Moreover, Lipschitz regularity,
uniqueness and existence results for solutions of the Neumann problem are
given.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:24:33 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Patrizi",
"Stefania",
""
]
] | [
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] |
712.0732 | Charles Gale | Simon Turbide, Charles Gale, Evan Frodermann, Ulrich Heinz | Electromagnetic radiation from nuclear collisions at RHIC energies | null | Phys.Rev.C77:024909,2008 | 10.1103/PhysRevC.77.024909 | CERN-PH-TH/2007-239 | hep-ph nucl-th | null | The hot and dense strongly interacting matter created in collisions of heavy
nuclei at RHIC energies is modeled with relativistic hydrodynamics, and the
spectra of real and virtual photons produced at mid-rapidity in these events
are calculated. Several different sources are considered, and their relative
importance is compared. Specifically, we include jet fragmentation, jet-plasma
interactions, the emission of radiation from the thermal medium and from
primordial hard collisions. Our calculations consistently take into account jet
energy loss, as evaluated in the AMY formalism. We obtain results for the
spectra, the nuclear modification factor (R_AA), and the azimuthal anisotropy
(v_2) that agree with the photon measurements performed by the PHENIX
collaboration at RHIC.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:08:18 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 20:45:45 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Turbide",
"Simon",
""
],
[
"Gale",
"Charles",
""
],
[
"Frodermann",
"Evan",
""
],
[
"Heinz",
"Ulrich",
""
]
] | [
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] |
712.0733 | Hiroki Matui | Hiroki Matui | An absorption theorem for minimal AF equivalence relations on Cantor
sets | 12 pages | null | null | null | math.DS math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that a `small' extension of a minimal AF equivalence relation on a
Cantor set is orbit equivalent to the AF relation. By a `small' extension we
mean an equivalence relation generated by the minimal AF equivalence relation
and another AF equivalence relation which is defined on a closed thin subset.
The result we obtain is a generalization of the main theorem in [GMPS2].
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:39:32 GMT"
},
{
"version": "v2",
"created": "Tue, 9 Sep 2008 04:07:50 GMT"
}
] | 2008-09-09T00:00:00 | [
[
"Matui",
"Hiroki",
""
]
] | [
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] |
712.0734 | Mario Antonelli | Mario Antonelli | Precision tests of Standard Model with leptonic and semileptonic kaon
decays | 23 pages, 11 figures, Proceeding of the 23rd International Symposium
on Lepton-Photon Interactions at High Energy (LP07), Daegu, Korea, 13-18 Aug
2007; typos and references addded | null | null | null | hep-ex | null | Till the middle of 2004 it appeared that the unitarity relation
Vud^2+Vus^2+Vub^2=1 might not hold at the 2.3sigma level. At that time,
however, Vus was inferred from old experimental data. Since then, a large
experimental and theoretical effort has been invested leading to a removal of
the problem. Thanks to the new and improved measurements by BNL-E865, KLOE,
KTeV, ISTRA+ and NA48, the Kl3 decay rate moved up so that Vus is now
consistent with unitarity. On the theory side, much progress has been made in
order to tame the systematic uncertainties related to the computation of the
Kl3 form factors.
This joint progress allowed to assess the validity of the CKM unitarity
relation at the level of less than $1%.
Recent measurements of kaon decays contributing to the determination of
Vus, Vus/Vud are summarized, and up-to-date evaluations of Vusf0 and Vus are
presented. In addition, we discuss the sensitivity of Kl3 and Kl2 decays to
various scenarios of physics beyond Standard Model.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:42:02 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 13:52:55 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Antonelli",
"Mario",
""
]
] | [
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712.0735 | Min-Young Choi | Min-Young Choi, Kyung Kiu Kim, Choonkyu Lee, Ki-Myeong Lee | Higgs Structures of Dyonic Instantons | 1+27 pages, 6 figures | JHEP0804:097,2008 | 10.1088/1126-6708/2008/04/097 | null | hep-th | null | We study Higgs field configurations of dyonic instantons in spontaneously
broken (4+1)-dimensional Yang-Mills theory. The adjoint scalar field solutions
to the covariant Laplace equation in the ADHM instanton background are
constructed in general noncanonical basis, and they are used to study
explicitly the Higgs field configurations of dyonic instantons when the gauge
fields are taken by Jackiw-Nohl-Rebbi instanton solutions. For these solutions
corresponding to small instanton number we then consider in some detail the
zero locus of the Higgs field, which describes the cross section of supertubes
connecting parallel D4-branes in string theory. Also the information on the
Higgs zeroes is used to discuss the residual gauge freedom concerning the
Jackiw-Nohl-Rebbi solutions.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:42:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Choi",
"Min-Young",
""
],
[
"Kim",
"Kyung Kiu",
""
],
[
"Lee",
"Choonkyu",
""
],
[
"Lee",
"Ki-Myeong",
""
]
] | [
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] |
712.0736 | Alexej Pashkin | A. Pashkin, K. Rabia, S. Frank, C. A. Kuntscher, R. Haumont, R.
Saint-Martin, and J. Kreisel | Pressure-induced phase transitions in the multiferroic perovskite BiFeO3
studied by far-infrared micro-spectroscopy | null | null | null | null | cond-mat.other | null | We present the results of pressure-dependent far-infrared reflectivity
measurements on the multiferroic perovskite BiFeO3 at room temperature. The
observed behavior of the infrared-active phonon modes as a funtion of pressure
clearly reveals two structural phase transitions around 3.0 and 7.5 GPa,
supporting the results of recent Raman and x-ray diffraction studies under
pressure. Based on the pressure-dependent frequency shifts of the
infrared-active phonon modes we discuss the possible character of the phase
transitions.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:50:15 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Pashkin",
"A.",
""
],
[
"Rabia",
"K.",
""
],
[
"Frank",
"S.",
""
],
[
"Kuntscher",
"C. A.",
""
],
[
"Haumont",
"R.",
""
],
[
"Saint-Martin",
"R.",
""
],
[
"Kreisel",
"J.",
""
]
] | [
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] |
712.0737 | Song-Ho Chong | Song-Ho Chong, Martin Aichele, Hendrik Meyer, Matthias Fuchs, and
J\"org Baschnagel | Structural and conformational dynamics of supercooled polymer melts:
Insights from first-principles theory and simulations | 54 pages, 10 figures | Phys. Rev. E 76, 051806 (2007) | 10.1103/PhysRevE.76.051806 | null | cond-mat.soft | null | We report on quantitative comparisons between simulation results of a
bead-spring model and mode-coupling theory calculations for the structural and
conformational dynamics of a supercooled, unentangled polymer melt. We find
semiquantitative agreement between simulation and theory, except for processes
that occur on intermediate length scales between the compressibility plateau
and the amorphous halo of the static structure factor. Our results suggest that
the onset of slow relaxation in a glass-forming melt can be described in terms
of monomer-caging supplemented by chain connectivity. Furthermore, a unified
atomistic description of glassy arrest and of conformational fluctuations that
(asymptotically) follow the Rouse model, emerges from our theory.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:46:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chong",
"Song-Ho",
""
],
[
"Aichele",
"Martin",
""
],
[
"Meyer",
"Hendrik",
""
],
[
"Fuchs",
"Matthias",
""
],
[
"Baschnagel",
"Jörg",
""
]
] | [
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] |
712.0738 | T. Roy Choudhury | T. Roy Choudhury, A. Ferrara and S. Gallerani | On the minimum mass of reionization sources | 6 pages, 2 figures | null | 10.1111/j.1745-3933.2008.00433.x | null | astro-ph | null | By means of carefully calibrated semi-analytical reionization models, we
estimate the minimum mass of star-forming haloes required to match the current
data. Models which do not include haloes of total mass M < 10^9 M_sun fail at
reproducing the Gunn-Peterson and electron scattering optical depths
simultaneously, as they contribute too few (many) photons at high (low, z
\approx 6) redshift. Marginally acceptable solutions require haloes with M
\approx 5 \times 10^7 M_sun at z \approx 10, corresponding to virial
temperatures (\sim 10^4K) for which cooling can be ensured by atomic
transitions. However, a much better match to the data is obtained if minihaloes
(M \sim 10^6 M_sun) are included in the analysis. We have critically examined
the assumptions made in our model and conclude that reionization in the
large-galaxies-only scenario can remain viable only if metal-free stars and/or
some other exotic sources at z > 6 are included.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:48:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Choudhury",
"T. Roy",
""
],
[
"Ferrara",
"A.",
""
],
[
"Gallerani",
"S.",
""
]
] | [
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] |
712.0739 | Sonja Schuh | S. Schuh, I. Traulsen, T. Nagel, E. Reiff, D. Homeier, H. Schwager,
D.-J. Kusterer, R. Lutz, M. R. Schreiber | A new period determination for the close PG1159 binary
SDSSJ212531.92-010745.9 | 3 pages, 2 figures, accepted for publication in Astronomical Notes | null | 10.1002/asna.200710920 | null | astro-ph | null | Methods to measure masses of PG1159 stars in order to test evolutionary
scenarios are currently based on spectroscopic masses or asteroseismological
mass determinations. One recently discovered PG1159 star in a close binary
system may finally allow the first dynamical mass determination, which has so
far been analysed on the basis of one SDSS spectrum and photometric monitoring.
In order to be able to phase future radial velocity measurements of the
system SDSSJ212531.92-010745.9, we follow up on the photometric monitoring of
this system to provide a solid observational basis for an improved orbital
ephemeris determination.
New white-light time series of the brightness variation of
SDSSJ212531.92-010745.9 with the Tuebingen 80cm and Goettingen 50cm telescopes
extend the monitoring into a second season (2006), tripling the length of
overall observational data available, and significantly increasing the time
base covered.
We give the ephemeris for the orbital motion of the system, based on a sine
fit which now results in a period of 6.95573(5)h, and discuss the associated
new amplitude determination in the context of the phased light curve variation
profile. The accuracy of the ephemeris has been improved by more than one order
of magnitude compared to that previously published for 2005 alone.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:10:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schuh",
"S.",
""
],
[
"Traulsen",
"I.",
""
],
[
"Nagel",
"T.",
""
],
[
"Reiff",
"E.",
""
],
[
"Homeier",
"D.",
""
],
[
"Schwager",
"H.",
""
],
[
"Kusterer",
"D. -J.",
""
],
[
"Lutz",
"R.",
""
],
[
"Schreiber",
"M. R.",
""
]
] | [
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] |
712.074 | Ji\v{r}\'i Min\'a\v{r} | Ji\v{r}\'i Min\'a\v{r}, Hugues de Riedmatten, Christoph Simon, Hugo
Zbinden, Nicolas Gisin | Phase noise measurements in long fiber interferometers for quantum
repeaters applications | 9 pages with 10 figures | J. Min\'a\v{r}, H. de Riedmatten, C. Simon, H. Zbinden, and N.
Gisin, Phys. Rev. A77, 052325 (2008) | 10.1103/PhysRevA.77.052325 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Many protocols for long distance quantum communication require
interferometric phase stability over long distances of optical fibers. In this
paper we investigate the phase noise in long optical fibers both in laboratory
environment and in installed commercial fibers in an urban environment over
short time scales (up to hundreds of us). We show that the phase fluctuations
during the travel time of optical pulses in long fiber loops are small enough
to obtain high visibility first order interference fringes in a Sagnac
interferometer configuration for fiber lengths up to 75 km. We also measure
phase fluctuations in a Mach-Zehnder interferometer in installed fibers with
arm length 36.5 km. We verify that the phase noise respects gaussian
distribution and measure the mean phase change as a function of time
difference. The typical time needed for a mean phase change of 0.1 rad is of
order of 100 us, which provides information about the time scale available for
active phase stabilization. Our results are relevant for future implementations
of quantum repeaters in installed optical fiber networks.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 14:49:34 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Aug 2008 15:36:08 GMT"
}
] | 2008-08-22T00:00:00 | [
[
"Minář",
"Jiří",
""
],
[
"de Riedmatten",
"Hugues",
""
],
[
"Simon",
"Christoph",
""
],
[
"Zbinden",
"Hugo",
""
],
[
"Gisin",
"Nicolas",
""
]
] | [
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0.1026459187,
-0.0381158143,
-0.0538323149,
-0.0623377152,
0.0100704469
] |
712.0741 | Elvira Ritz | Elvira Ritz and Martin Dressel | Analysis of broadband microwave conductivity and permittivity
measurements of semiconducting materials | 9 pages, 10 figures, accepted for publication in the Journal of
Applied Physics | J. Appl. Phys. 103, 084902 (2008), http://jap.aip.org/ | 10.1063/1.2906131 | null | cond-mat.mtrl-sci cond-mat.dis-nn | null | We perform broadband phase sensitive measurements of the reflection
coefficient from 45 MHz up to 20 GHz employing a vector network analyzer with a
2.4 mm coaxial sensor which is terminated by the sample under test. While the
material parameters (conductivity and permittivity) can be easily extracted
from the obtained impedance data if the sample is metallic, no direct solution
is possible if the material under investigation is an insulator. Focusing on
doped semiconductors with largely varying conductivity, here we present a
closed calibration and evaluation procedure for frequencies up to 5 GHz, based
on the rigorous solution for the electromagnetic field distribution inside the
sample combined with the variational principle; basically no limiting
assumptions are necessary. A simple static model based on the electric current
distribution proves to yield the same frequency dependence of the complex
conductivity up to 1 GHz. After a critical discussion we apply the developed
method to the hopping transport in Si:P at temperature down to 1 K.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:34:59 GMT"
},
{
"version": "v2",
"created": "Thu, 7 Feb 2008 17:46:18 GMT"
},
{
"version": "v3",
"created": "Sun, 2 Mar 2008 14:46:21 GMT"
}
] | 2008-05-12T00:00:00 | [
[
"Ritz",
"Elvira",
""
],
[
"Dressel",
"Martin",
""
]
] | [
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] |
712.0742 | Sonja Schuh | Sonja Schuh, Thorsten Nagel, Iris Traulsen, Benjamin Beeck | New Light Curves and Spectra of the close PG1159 Binary System
SDSSJ212531.92-010745.9 | 2 pages, to appear in "Hydrogen-Deficient Stars", ASP conference
series | null | null | null | astro-ph | null | Methods to measure masses of PG1159 stars in order to test evolutionary
scenarios are currently based on spectroscopic masses or asteroseismological
mass determinations. SDSSJ212531.92-010745.9, a recently discovered PG1159 star
in a close binary system, may finally allow the first dynamical mass
determination, and has so far been analysed on the basis of one SDSS spectrum
and photometric monitoring.
In order to be able to phase radial velocity measurements of the system
SDSSJ212531.92-010745.9, we have followed up the photometric monitoring of this
system. New white light time series of the brightness variation of
SDSSJ212531.92-010745.9 with the Tuebingen 80cm and Goettingen 50cm telescopes
extend the monitoring into a second season (2006). We give the improved
ephemeris for the orbital motion of the system, based on a sine fit which now
results in a period of 6.95573(5)h.
In 2007, we have obtained a series of phase-resolved medium-resolution
spectra with the TWIN spectrograph at the 3.5m telescope at Calar Alto, which
will allow us to derive the radial velocity curves for both components of the
system, and to perform spectral analyses of the irradiating and irradiated
components at different phases. We briefly describe the newly obtained spectra.
The light curve and radial velocities combined will allow us to carry out a
mass determination.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:03:10 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Schuh",
"Sonja",
""
],
[
"Nagel",
"Thorsten",
""
],
[
"Traulsen",
"Iris",
""
],
[
"Beeck",
"Benjamin",
""
]
] | [
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] |
712.0743 | Yevgeny Kats | Yevgeny Kats, Pavel Petrov | Effect of curvature squared corrections in AdS on the viscosity of the
dual gauge theory | 18 pages; v4: added note and references; published version | JHEP 0901:044,2009 | 10.1088/1126-6708/2009/01/044 | null | hep-th hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We use the real-time finite-temperature AdS/CFT correspondence to compute the
effect of general R^2 corrections to the gravitational action in AdS space on
the shear viscosity of the dual gauge theory. The R^2 terms in AdS_5 are
determined by the central charges of the CFT. We present an example of a
four-dimensional gauge theory in which the conjectured lower bound of 1/(4\pi)
on the viscosity-to-entropy ratio is violated for finite N.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 19:49:32 GMT"
},
{
"version": "v2",
"created": "Tue, 26 Feb 2008 22:24:34 GMT"
},
{
"version": "v3",
"created": "Wed, 9 Apr 2008 19:45:47 GMT"
},
{
"version": "v4",
"created": "Tue, 20 Jan 2009 20:31:26 GMT"
}
] | 2009-01-27T00:00:00 | [
[
"Kats",
"Yevgeny",
""
],
[
"Petrov",
"Pavel",
""
]
] | [
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] |
712.0744 | Vitorino Ramos Dr. | Vitorino Ramos, C. M. Fernandes, A. C. Rosa, A. Abraham | Computational Chemotaxis in Ants and Bacteria over Dynamic Environments | 8 pages, 6 figures, in CEC 07 - IEEE Congress on Evolutionary
Computation, ISBN 1-4244-1340-0, pp. 1009-1017, Sep. 2007 | null | 10.1109/CEC.2007.4424594 | null | cs.MA cs.AI q-bio.PE q-bio.QM | null | Chemotaxis can be defined as an innate behavioural response by an organism to
a directional stimulus, in which bacteria, and other single-cell or
multicellular organisms direct their movements according to certain chemicals
in their environment. This is important for bacteria to find food (e.g.,
glucose) by swimming towards the highest concentration of food molecules, or to
flee from poisons. Based on self-organized computational approaches and similar
stigmergic concepts we derive a novel swarm intelligent algorithm. What strikes
from these observations is that both eusocial insects as ant colonies and
bacteria have similar natural mechanisms based on stigmergy in order to emerge
coherent and sophisticated patterns of global collective behaviour. Keeping in
mind the above characteristics we will present a simple model to tackle the
collective adaptation of a social swarm based on real ant colony behaviors (SSA
algorithm) for tracking extrema in dynamic environments and highly multimodal
complex functions described in the well-know De Jong test suite. Later, for the
purpose of comparison, a recent model of artificial bacterial foraging (BFOA
algorithm) based on similar stigmergic features is described and analyzed.
Final results indicate that the SSA collective intelligence is able to cope and
quickly adapt to unforeseen situations even when over the same cooperative
foraging period, the community is requested to deal with two different and
contradictory purposes, while outperforming BFOA in adaptive speed. Results
indicate that the present approach deals well in severe Dynamic Optimization
problems.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:02:19 GMT"
}
] | 2016-11-18T00:00:00 | [
[
"Ramos",
"Vitorino",
""
],
[
"Fernandes",
"C. M.",
""
],
[
"Rosa",
"A. C.",
""
],
[
"Abraham",
"A.",
""
]
] | [
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712.0745 | Andriy Ganshyn | T. R. Charlton, R. M. Dalgliesh, A. Ganshin, O. Kirichek, S.
Langridge, P. V. E. McClintock | Neutron reflection from the surface of normal and superfluid 4He | to be published in Low Temperature Physics | null | null | null | cond-mat.soft cond-mat.other | null | The reflection of neutrons from a helium surface has been observed for the
first time. The 4He surface is smoother in the superfluid state at 1.54 K than
in the case of the normal liquid at 2.3 K. In the superfluid state we also
observe a surface layer ~200 Angstroms thick which has a subtly different
neutron scattering cross-section, which may be explained by an enhanced
Bose-Einstein condensate fraction close to the helium surface.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:10:38 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Charlton",
"T. R.",
""
],
[
"Dalgliesh",
"R. M.",
""
],
[
"Ganshin",
"A.",
""
],
[
"Kirichek",
"O.",
""
],
[
"Langridge",
"S.",
""
],
[
"McClintock",
"P. V. E.",
""
]
] | [
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712.0746 | Cyrille Marquet | Cyrille Marquet | Testing BFKL evolution with Mueller-Navelet jets | 4 pages, 1 figure, Proceedings of the XXXVIIth International
Symposium on Multiparticle Dynamics (ISMD07), Berkeley, USA, August 4-9 2007 | Acta Phys.Polon.Supp.1:463-467,2008 | null | null | hep-ph | null | We study the correlation in azimuthal angle between Mueller-Navelet jets
produced in hadron-hadron collisions. We argue that this observable would test
the BFKL approach at next-to-leading logarithmic accuracy. In order to motivate
such a measurement, we give predictions for jets separated by large rapidity
intervals within the Tevatron and LHC ranges.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:11:11 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Marquet",
"Cyrille",
""
]
] | [
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] |
712.0747 | Alon Faraggi | Alon E. Faraggi, Costas Kounnas, John Rizos | Spinor-Vector Duality in N=2 Heterotic String Vacua | 19 pages. 1 figure | Nucl.Phys.B799:19-33,2008 | 10.1016/j.nuclphysb.2008.02.009 | null | hep-th hep-ph | null | Classification of the N=1 space-time supersymmetric fermionic Z2XZ2
heterotic-string vacua with symmetric internal shifts, revealed a novel
spinor-vector duality symmetry over the entire space of vacua, where the S_t
<-> V duality interchanges the spinor plus anti-spinor representations with
vector representations. In this paper we demonstrate that the spinor--vector
duality exists also in fermionic Z2 heterotic string models, which preserve N=2
space-time supersymmetry. In this case the interchange is between spinorial and
vectorial representations of the unbroken SO(12) GUT symmetry. We provide a
general algebraic proof for the existence of the S_t <-> V duality map. We
present a novel basis to generate the free fermionic models in which the ten
dimensional gauge degrees of freedom are grouped into four groups of four, each
generating an SO(8) modular block. In the new basis the GUT symmetries are
produced by generators arising from the trivial and non--trivial sectors, and
due to the triality property of the SO(8) representations. Thus, while in the
new basis the appearance of GUT symmetries is more cumbersome, it may be more
instrumental in revealing the duality symmetries that underly the string vacua.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:16:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Faraggi",
"Alon E.",
""
],
[
"Kounnas",
"Costas",
""
],
[
"Rizos",
"John",
""
]
] | [
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] |
712.0748 | Francois Ducastelle | Hakim Amara (LPS, PCPM), Christophe Bichara (CRMCN), Fran\c{c}ois
Ducastelle (LEM) | Understanding the nucleation mechanisms of Carbon Nanotubes in catalytic
Chemical Vapor Deposition | null | null | 10.1103/PhysRevLett.100.056105 | null | cond-mat.mtrl-sci | null | The nucleation of carbon caps on small nickel clusters is studied using a
tight binding model coupled to grand canonical Monte Carlo simulations. It
takes place in a well defined carbon chemical potential range, when a critical
concentration of surface carbon atoms is reached. The solubility of carbon in
the outermost Ni layers, that depends on the initial, crystalline or
disordered, state of the catalyst and on the thermodynamic conditions, is
therefore a key quantity to control the nucleation.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:22:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Amara",
"Hakim",
"",
"LPS, PCPM"
],
[
"Bichara",
"Christophe",
"",
"CRMCN"
],
[
"Ducastelle",
"François",
"",
"LEM"
]
] | [
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] |
712.0749 | Bogdan Ranguelov | Bogdan Ranguelov, Stoyan Stoyanov | Instabilities at vicinal crystal surfaces - competition between the
electromigration of the adatoms and the kinetic memory effect | 15 pages, 6 figures | null | 10.1103/PhysRevB.77.205406 | null | physics.chem-ph | null | We studied the step dynamics during sublimation and growth in the presence of
electromigration force acting on the adatoms. In the limit of fast surface
diffusion and slow kinetics of atom attachment-detachment at the steps we
formulate a model free of the quasi-static approximation in the calculation of
the adatom concentration on the terraces. Numerical integration of the
equations for the time evolution of the adatom concentrations and the equations
of step motion reveals two different step bunching instabilities: 1) step
density waves (small bunches which do not manifest any coarsening) induced by
the kinetic memory effect and 2) step bunching with coarsening when the
dynamics is dominated by the electromigration. The model developed in this
paper also provides very instructive illustrations of the Popkov-Krug dynamical
phase transition during sublimation and growth of a vicinal crystal surface.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:32:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ranguelov",
"Bogdan",
""
],
[
"Stoyanov",
"Stoyan",
""
]
] | [
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] |
712.075 | Michael Thorwart | R. Egger, A. O. Gogolin | Vibration-induced correction to the current through a single molecule | 4 pages, no figures, to appear in PRB, published version | Phys. Rev. B 77, 113405 (2008) | 10.1103/PhysRevB.77.113405 | null | cond-mat.mes-hall | null | We provide analytical results for the perturbative correction to the
current-voltage relation through a vibrating molecule for weak electron-phonon
coupling. The nonlinear conductance exhibits a step-like feature at $eV=\hbar
\omega_0$, where $\omega_0$ is the vibration frequency. We establish criteria
for the sign change of the step in the conductance (up or down). This
transition turns out to be nonuniversal and is governed by essentially all
system parameters.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:46:50 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 15:19:25 GMT"
},
{
"version": "v3",
"created": "Wed, 6 Feb 2008 10:20:04 GMT"
}
] | 2008-03-14T00:00:00 | [
[
"Egger",
"R.",
""
],
[
"Gogolin",
"A. O.",
""
]
] | [
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] |
712.0751 | Efim Brener | Efim A. Brener and D.E. Temkin | Melting of alloys along grain boundaries | submitted to Acta Materialia | null | null | null | cond-mat.mtrl-sci | null | We discuss melting of alloys along grain boundaries as a free boundary
problem for two moving solid-liquid interfaces. One of them is the melting
front and the other is the solidification front. The presence of the triple
junction plays an important role in controlling the velocity of this process.
The interfaces strongly interact via the diffusion field in the thin liquid
layer between them. In the liquid film migration (LFM) mechanism the system
chooses a more efficient kinetic path, which is controlled by diffusion in the
liquid film on relatively short distances. However, only weak coherency strain
energy is the effective driving force for LFM in the case of melting of
one-phase alloys.
The process with only one melting front would be controlled by the very slow
diffusion in the mother solid phase on relatively large distances.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:37:53 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Brener",
"Efim A.",
""
],
[
"Temkin",
"D. E.",
""
]
] | [
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] |
712.0752 | Torben Swart | Torben Swart, Vidian Rousse | A Mathematical Justification for the Herman-Kluk Propagator | Typos corrected | null | null | null | math-ph math.MP | null | A class of Fourier Integral Operators which converge to the unitary group of
the Schroedinger equation in semiclassical limit $\eps\to 0$ is constructed.
The convergence is in the uniform operator norm and allows for an error bound
of order $O(\eps^{1-\rho})$ for Ehrenfest timescales, where $\rho$ can be made
arbitrary small. For the shorter times of order O(1), the error can be improved
to arbitrary order in $\eps$. In the chemical literature the approximation is
known as the Herman-Kluk propagator.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:24:53 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Dec 2007 10:56:41 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Swart",
"Torben",
""
],
[
"Rousse",
"Vidian",
""
]
] | [
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] |
712.0753 | Cesar Seoanez | C. Seoanez, F. Guinea and A. H. Castro Neto | Surface dissipation in nanoelectromechanical systems: Unified
description with the standard tunneling model and effects of metallic
electrodes | 17 pages, 7 figures | Phys. Rev. B 77, 125107 (2008) | 10.1103/PhysRevB.77.125107 | null | cond-mat.mes-hall | null | By modifying and extending recent ideas [C. Seoanez et al., Europhys. Lett.
78, 60002 (2007)], a theoretical framework to describe dissipation processes in
the surfaces of vibrating micro- and nanoelectromechanical devices, thought to
be the main source of friction at low temperatures, is presented. Quality
factors as well as frequency shifts of flexural and torsional modes in doubly
clamped beams and cantilevers are given, showing the scaling with dimensions,
temperature, and other relevant parameters of these systems. Full agreement
with experimental observations is not obtained, leading to a discussion of
limitations and possible modifications of the scheme to reach a quantitative
fitting to experiments. For nanoelectromechanical systems covered with metallic
electrodes, the friction due to electrostatic interaction between the flowing
electrons and static charges in the device and substrate is also studied.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:40:49 GMT"
},
{
"version": "v2",
"created": "Sat, 8 Mar 2008 11:54:29 GMT"
}
] | 2008-03-08T00:00:00 | [
[
"Seoanez",
"C.",
""
],
[
"Guinea",
"F.",
""
],
[
"Neto",
"A. H. Castro",
""
]
] | [
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] |
712.0754 | Natalia Babych | N. Babych and Yu. Golovaty | Asymptotic analysis of vibrating system containing stiff-heavy and
flexible-light parts | 16 pages | null | null | null | math.SP | null | A model of strongly inhomogeneous medium with simultaneous perturbation of
rigidity and mass density is studied. The medium has strongly contrasting
physical characteristics in two parts with the ratio of rigidities being
proportional to a small parameter $\epsilon$. Additionally, the ratio of mass
densities is of order $\epsilon^{-1}$. We investigate the asymptotic behaviour
of spectrum and eigensubspaces as $\epsilon\to 0$. Complete asymptotic
expansions of eigenvalues and eigenfunctions are constructed and justified.
We show that the limit operator is nonself-adjoint in general and possesses
two-dimensional Jordan cells in spite of the singular perturbed problem is
associated with a self-adjoint operator in appropriated Hilbert space
$L_\epsilon$. This may happen if the metric in which the problem is
self-adjoint depends on small parameter $\epsilon$ in a singular way. In
particular, it leads to a loss of completeness for the eigenfunction
collection. We describe how root spaces of the limit operator approximate
eigenspaces of the perturbed operator.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:47:56 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Babych",
"N.",
""
],
[
"Golovaty",
"Yu.",
""
]
] | [
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] |
712.0755 | Isabella Pagano | C. De Martino, L. Bianchi, I. Pagano, J. Herald, and D. Thilker | GALEX Ultraviolet photometry of NGC 2420: searching for WDs | null | null | null | null | astro-ph | null | We present color-magnitude diagrams of the open cluster NGC 2420, obtained
from Galaxy Evolution Explorer (GALEX) ultraviolet images in FUV and NUV bands
and Sloan Digital Sky Survey (SDSS) u,g,r,i,z photometry. Our goal is to search
for and characterize hot evolved stars and peculiar objects in this open
cluster, as part of a larger project aimed to study a number of open clusters
in the Milky Way with GALEX and ground-based data.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:49:18 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"De Martino",
"C.",
""
],
[
"Bianchi",
"L.",
""
],
[
"Pagano",
"I.",
""
],
[
"Herald",
"J.",
""
],
[
"Thilker",
"D.",
""
]
] | [
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] |
712.0756 | Amy Winebarger | A.R Winebarger, H.P. Warren, and D.A. Falconer | Modeling X-ray Loops and EUV "Moss" in an Active Region Core | 17 pages, 6 figurs, accepted to ApJ | null | 10.1086/527291 | null | astro-ph | null | The Soft X-ray intensity of loops in active region cores and corresponding
footpoint, or moss, intensity observed in the EUV remain steady for several
hours of observation. The steadiness of the emission has prompted many to
suggest that the heating in these loops must also be steady, though no direct
comparison between the observed X-ray and EUV intensities and the steady
heating solutions of the hydrodynamic equations has yet been made. In this
paper, we perform these simulations and simultaneously model the X-Ray and EUV
moss intensities in one active regioncore with steady uniform heating. To
perform this task, we introduce a new technique to constrain the model
parameters using the measured EUV footpoint intensity to infer a heating rate.
We find that a filling factor of 8% and loops that expand with height provides
the best agreement with the intensity in two X-ray filters, though the
simulated SXT Al12 intensity is 147% the observed intensity and the SXT AlMg
intensity is 80% the observed intensity. From this solution, we determine the
required heating rate scales as ${\bar{B}}^{0.29} L^{-0.95}$. Finally we
discuss the future potential of this type of modeling, such as the ability to
use density measurements to fully constrain filling factor, and its
shortcomings, such as the requirement to use potential field extrapolations to
approximate the coronal field.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:52:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Winebarger",
"A. R",
""
],
[
"Warren",
"H. P.",
""
],
[
"Falconer",
"D. A.",
""
]
] | [
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] |
712.0757 | Sonja Koller | Ralph Peter Hornberger, Sonja Koller, Georg Begemann, Andrea Donarini,
Milena Grifoni | Transport through a double quantum dot system with non-collinearly
polarized leads | 18 pages, 13 figures, 5 tables; revised published version | Phys. Rev. B 77, 245313 (2008) | 10.1103/PhysRevB.77.245313 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate linear and non-linear transport in a double quantum dot system
weakly coupled to spin-polarized leads.
In the linear regime, the conductance as well as the non-equilibrium spin
accumulation are evaluated in analytic form. The conductance as a function of
the gate voltage exhibits four peaks of different height, with mirror symmetry
with respect to the charge neutrality point. As the polarization angle is
varied, the position and shape of the peaks changes in a characteristic way
which preserves the electron-hole symmetry of the problem. In the nonlinear
regime negative differential conductance features occur for non collinear
magnetisations of the leads. In the considered sequential tunneling limit, the
tunneling magneto resistance (TMR) is always positive with a characteristic
gate voltage dependence for non-collinear magnetization. If a magnetic field is
added to the system, the TMR can become negative.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:14:46 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 10:08:22 GMT"
},
{
"version": "v3",
"created": "Tue, 1 Jul 2008 10:02:31 GMT"
}
] | 2008-07-01T00:00:00 | [
[
"Hornberger",
"Ralph Peter",
""
],
[
"Koller",
"Sonja",
""
],
[
"Begemann",
"Georg",
""
],
[
"Donarini",
"Andrea",
""
],
[
"Grifoni",
"Milena",
""
]
] | [
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] |
712.0758 | Sang-Koog Kim | Ki-Suk Lee, and Sang-Koog Kim | Two Circular-Rotational Eigenmodes in Vortex Gyrotropic Motions in Soft
Magnetic Nanodots | 30 pages, 7 figures | Phys. Rev. B 78, 014405 (2008) (6 pages) | 10.1103/PhysRevB.78.014405 | null | cond-mat.mtrl-sci cond-mat.other | null | We found, by micromagnetic numerical and analytical calculations, that the
clockwise (CW) and counterclockwise (CCW) circular-rotational motions of a
magnetic vortex core in a soft magnetic circular nanodot are the elementary
eigenmodes existing in the gyrotropic motion with respect to the corresponding
CW and CCW circular-rotational-field eigenbasis. Any steady-state vortex
gyrotropic motions driven by a linearly polarized oscillating in-plane magnetic
field in the linear regime can be perfectly understood according to the
superposition of the two circular eigenmodes, which show asymmetric resonance
characteristics reflecting the vortex polarization. The relative magnitudes in
the amplitude and phase between the CCW and CW eigenmodes determine the
elongation and orientation of the orbital trajectories of the vortex core
motions, respectively, which trajectories vary with the polarization and
chirality of the given vortex as well as the field frequency across the
resonance frequency.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:56:47 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jan 2008 11:57:07 GMT"
},
{
"version": "v3",
"created": "Fri, 1 Feb 2008 14:47:35 GMT"
}
] | 2008-07-05T00:00:00 | [
[
"Lee",
"Ki-Suk",
""
],
[
"Kim",
"Sang-Koog",
""
]
] | [
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] |
712.0759 | Luis L. Sanchez. Soto | A. B. Klimov, J. L. Romero, L. L. Sanchez-Soto, A. Messina and A.
Napoli | Quantum light depolarization: the phase-space perspective | 6 pages, no figures. Submitted for publication | Phys. Rev. A 77, 033853 (2008) | 10.1103/PhysRevA.77.033853 | null | quant-ph | null | Quantum light depolarization is handled through a master equation obtained by
coupling dispersively the field to a randomly distributed atomic reservoir.
This master equation is solved by transforming it into a quasiprobability
distribution in phase space and the quasiclassical limit is investigated.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 15:59:09 GMT"
}
] | 2008-07-25T00:00:00 | [
[
"Klimov",
"A. B.",
""
],
[
"Romero",
"J. L.",
""
],
[
"Sanchez-Soto",
"L. L.",
""
],
[
"Messina",
"A.",
""
],
[
"Napoli",
"A.",
""
]
] | [
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] |
712.076 | Verena Koerting | V. Koerting, J. Paaske, and P. W\"olfle | Electron transport in the four-lead two-impurity Kondo model:
Nonequilibrium perturbation theory with almost degenerate levels | 10 pages, 8 figures | Phys. Rev. B 77, 165122 (2008) (10 pages) | 10.1103/PhysRevB.77.165122 | null | cond-mat.str-el | null | The eigenstates of an isolated nanostructure may get mixed by the coupling to
external leads. This effect is the stronger, the smaller the level splitting on
the dot and the larger the broadening induced by the coupling to the leads. We
describe how to calculate the nondiagonal density matrix of the nanostructure
efficiently in the cotunneling regime. As an example, we consider a system of
two quantum dots in the Kondo regime, the two spins coupled by an
antiferromagnetic exchange interaction and each dot tunnel coupled to two
leads. Calculating the nonequilibrium density matrix and the corresponding
current, we demonstrate the importance of the off-diagonal terms in the
presence of an applied magnetic field and a finite bias voltage.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:25:39 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Dec 2007 14:28:06 GMT"
},
{
"version": "v3",
"created": "Tue, 22 Apr 2008 08:00:11 GMT"
}
] | 2008-04-22T00:00:00 | [
[
"Koerting",
"V.",
""
],
[
"Paaske",
"J.",
""
],
[
"Wölfle",
"P.",
""
]
] | [
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] |
712.0761 | Seth Redfield | Seth Redfield, Michael Endl, William D. Cochran and Lars Koesterke | Sodium Absorption From the Exoplanetary Atmosphere of HD189733b Detected
in the Optical Transmission Spectrum | 12 pages, 2 figures; Accepted for publication in ApJ Letters | null | 10.1086/527475 | null | astro-ph | null | We present the first ground-based detection of sodium absorption in the
transmission spectrum of an extrasolar planet. Absorption due to the atmosphere
of the extrasolar planet HD189733b is detected in both lines of the NaI
doublet. High spectral resolution observations were taken of eleven transits
with the High Resolution Spectrograph (HRS) on the 9.2 meter Hobby-Eberly
Telescope (HET). The NaI absorption in the transmission spectrum due to
HD189733b is (-67.2 +/- 20.7) x 10^-5 deeper in the ``narrow'' spectral band
that encompasses both lines relative to adjacent bands. The 1-sigma error
includes both random and systematic errors, and the detection is >3-sigma. This
amount of relative absorption in NaI for HD189733b is ~3x larger than detected
for HD209458b by Charbonneau et al. (2002), and indicates these two
hot-Jupiters may have significantly different atmospheric properties.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 20:21:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Redfield",
"Seth",
""
],
[
"Endl",
"Michael",
""
],
[
"Cochran",
"William D.",
""
],
[
"Koesterke",
"Lars",
""
]
] | [
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] |
712.0762 | Charles Bonatto | Eduardo Bica, Charles Bonatto and Denilso Camargo | Probing FSR star cluster candidates in bulge/disk directions with 2MASS
colour-magnitude diagrams | 13 pages; 10 figs. Accepted by MNRAS | MNRAS 2008 | 10.1111/j.1365-2966.2007.12812.x | null | astro-ph | null | We analyse 20 star cluster candidates projected mostly in the bulge direction
($|\ell|<60^\circ$). The sample contains all candidates in that sector
classified by \citet{FSRcat} with quality flags denoting high probability of
being star clusters. Bulge contamination in the colour-magnitude diagrams
(CMDs) is in general important, while at lower Galactic latitudes disk stars
contribute as well. Properties of the candidates are investigated with 2MASS
CMDs and stellar radial density profiles (RDPs) built with field star
decontaminated photometry. To uncover the nature of the structures we
decontaminate the CMDs from field stars using tools that we previously
developed to deal with objects in dense fields. We confirm in all cases
excesses in the RDPs with respect to the background level, as expected from the
method the candidates were originally selected. CMDs and RDPs taken together
revealed 6 open clusters, 5 uncertain cases that require deeper observations,
while 9 objects are possibly field density fluctuations.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:01:20 GMT"
}
] | 2012-04-02T00:00:00 | [
[
"Bica",
"Eduardo",
""
],
[
"Bonatto",
"Charles",
""
],
[
"Camargo",
"Denilso",
""
]
] | [
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] |
712.0763 | Lorenzo Marrucci | C. Manzo, D. Paparo, L. Marrucci, I. Janossy | Light-induced rotation of dye-doped liquid crystal droplets | null | Phys. Rev. E 73, 051707 (2006) | 10.1103/PhysRevE.73.051707 | null | physics.optics cond-mat.soft physics.flu-dyn | null | We investigate both theoretically and experimentally the rotational dynamics
of micrometric droplets of dye-doped and pure liquid crystal induced by
circularly and elliptically polarized laser light. The droplets are dispersed
in water and trapped in the focus of the laser beam. Since the optical torque
acting on the molecular director is known to be strongly enhanced in
light-absorbing dye-doped materials, the question arises whether a similar
enhancement takes place also for the overall optical torque acting on the whole
droplets. We searched for such enhancement by measuring and comparing the
rotation speed of dye-doped droplets induced by a laser beam having a
wavelength either inside or outside the dye absorption band, and also comparing
it with the rotation of pure liquid crystal droplets. No enhancement was found,
confirming that photoinduced dye effects are only associated with an internal
exchange of angular momentum between orientational and translational degrees of
freedom of matter. Our result provides also the first direct experimental proof
of the existence of a photoinduced stress tensor in the illuminated dye-doped
liquid crystal. Finally, peculiar photoinduced dynamical effects are predicted
to occur in droplets in which the molecular director is not rigidly locked to
the flow, but so far they could not be observed.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:01:21 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Manzo",
"C.",
""
],
[
"Paparo",
"D.",
""
],
[
"Marrucci",
"L.",
""
],
[
"Janossy",
"I.",
""
]
] | [
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712.0764 | Roopa Narayan | R. H. Narayan | The Conception of Atom in Greek and Indian Physics | 4 pages, Presented at the 17th International Conference on Vedanta,
Miami University, Oxford. September 2007 | null | null | null | physics.gen-ph | null | This paper contrasts the Greek and Indian conceptions of atom. It is shown
that these two are quite different in spirit.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:02:48 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Narayan",
"R. H.",
""
]
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712.0765 | Cristina Bena | Cristina Bena, Gilles Montambaux | Remarks on the tight-binding model of graphene | 15 pages, 4 figures | New J. Phys. 11, 095003 (2009) | 10.1088/1367-2630/11/9/095003 | null | cond-mat.mes-hall | null | We address a simple but fundamental issue arising in the study of graphene,
as well as of other systems that have a crystalline structure with more than
one atom per unit cell. For these systems, the choice of the tight-binding
basis is not unique. For monolayer graphene two bases are widely used in the
literature. While the expectation values of operators describing physical
quantities should be independent of basis, the form of the operators may depend
on the basis, especially in the presence of disorder or of an applied magnetic
field. Using the inappropriate form of certain operators may lead to erroneous
physical predictions. We discuss the two bases used to describe monolayer
graphene, as well as the form of the most commonly used operators in the two
bases. We repeat our analysis for the case of bilayer graphene.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:04:50 GMT"
}
] | 2010-04-15T00:00:00 | [
[
"Bena",
"Cristina",
""
],
[
"Montambaux",
"Gilles",
""
]
] | [
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712.0766 | Jean-Francois Gonzalez | Jean-Fran\c{c}ois Gonzalez (CRAL), Laure Fouchet (ETHZ), Sarah T.
Maddison, Guillaume Laibe (CRAL) | Dust evolution in protoplanetary disks | 6 pages, 5 figures, to appear in the Proceedings of IAU Symp. 249:
Exoplanets: Detection, Formation and Dynamics (Suzhou, China) | Dans Proceedings of IAU Symp. 249 - Exoplanets: Detection,
Formation and Dynamics, Suzhou : Chine (2007) | 10.1017/S1743921308016840 | null | astro-ph | null | We investigate the behaviour of dust in protoplanetary disks under the action
of gas drag using our 3D, two-fluid (gas+dust) SPH code. We present the
evolution of the dust spatial distribution in global simulations of planetless
disks as well as of disks containing an already formed planet. The resulting
dust structures vary strongly with particle size and planetary gaps are much
sharper than in the gas phase, making them easier to detect with ALMA than
anticipated. We also find that there is a range of masses where a planet can
open a gap in the dust layer whereas it doesn't in the gas disk. Our dust
distributions are fed to the radiative transfer code MCFOST to compute
synthetic images, in order to derive constraints on the settling and growth of
dust grains in observed disks.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:12:47 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 08:03:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gonzalez",
"Jean-François",
"",
"CRAL"
],
[
"Fouchet",
"Laure",
"",
"ETHZ"
],
[
"Maddison",
"Sarah T.",
"",
"CRAL"
],
[
"Laibe",
"Guillaume",
"",
"CRAL"
]
] | [
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] |
712.0767 | Tim Sluckin | V.O. Kubytskyi, V.Y. Reshetnyak, T.J. Sluckin, S.J. Cox | Surface-mediated non-linear optical effects in liquid crystals | 13 figures +latex file + bbl file in winzip file | null | null | null | cond-mat.soft | null | We make a phenomenological model of optical two-beam interaction in a model
planar liquid crystal cell. The liquid crystal is subject to homeotropic
anchoring at the cell walls, is surrounded by thin photosensitive layers, and
is subject to a variable potential across the cell. These systems are often
known as liquid crystal photorefractive systems. The interference between the
two obliquely incident beams causes a time-independent periodic modulation in
electric field intensity in the direction transverse to the cell normal. Our
model includes this field phenomenologically by affecting the potential at the
walls of the cell. The transverse periodic surface potential causes spatially
periodic departures from a pure homeotropic texture. The texture modulation
acts as a grating for the incident light. The incident light is both directly
transmitted and also subject to diffraction. The first diffracted beams result
in energy exchange between the beams. We find that the degree of energy
exchange can be strongly sensitive to the mean angle of incidence, the angle
between the beams, and the imposed potential across the cell. We use the model
to speculate about what factors optimize non-linear optical interaction in
liquid crystalline photorefractive systems.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:14:07 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Kubytskyi",
"V. O.",
""
],
[
"Reshetnyak",
"V. Y.",
""
],
[
"Sluckin",
"T. J.",
""
],
[
"Cox",
"S. J.",
""
]
] | [
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] |
712.0768 | C. A. Dominguez | Cesareo A. Dominguez, Nasrallah F. Nasrallah, Raoul R\"ontsch, Karl
Schilcher | Strange quark mass from Finite Energy QCD sum rules to five loops | Additional comments added at the end of the Conclusions, and one
extra reference is given. A note added in proof uses the most recent
determination of Lambda_QCD from ALEPH to narrow down the prediction | JHEP 0805:020,2008 | 10.1088/1126-6708/2008/05/020 | UCT-TP-270/07, MZ-TH/07-18 | hep-ph hep-lat | null | The strange quark mass is determined from a new QCD Finite Energy Sum Rule
(FESR) optimized to reduce considerably the systematic uncertainties arising
from the hadronic resonance sector. As a result, the main uncertainty in this
determination is due to the value of $\Lambda_{QCD}$. The correlator of
axial-vector divergences is used in perturbative QCD to five-loop order,
including quark and gluon condensate contributions, in the framework of both
Fixed Order (FOPT), and Contour Improved Perturbation Theory (CIPT). The latter
exhibits very good convergence, leading to a remarkably stable result in the
very wide range $s_0 = 1.0 - 4.0 {GeV}^2$, where $s_0$ is the radius of the
integration contour in the complex energy (squared) plane. The value of the
strange quark mass in this framework at a scale of 2 GeV is $m_s(2 {GeV}) = 95
\pm 5 (111 \pm 6) {MeV}$ for $\Lambda_{QCD} = 420
(330) {MeV}$, respectively.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:14:56 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Dec 2007 10:23:28 GMT"
},
{
"version": "v3",
"created": "Wed, 20 Feb 2008 10:49:46 GMT"
},
{
"version": "v4",
"created": "Tue, 6 May 2008 15:42:47 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Dominguez",
"Cesareo A.",
""
],
[
"Nasrallah",
"Nasrallah F.",
""
],
[
"Röntsch",
"Raoul",
""
],
[
"Schilcher",
"Karl",
""
]
] | [
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] |
712.0769 | Jocelyne Troccaz | Michael Baumann (TIMC), Pierre Mozer (TIMC), Vincent Daanen (TIMC),
Jocelyne Troccaz (TIMC) | Towards 3D ultrasound image based soft tissue tracking: a transrectal
ultrasound prostate image alignment system | null | Dans Proceedings of MICCAI 2007 - Medical Image Computing and
Computer Assisted Interventions 2007, Brisbane : Australie (2007) | null | null | cs.OH physics.med-ph | null | The emergence of real-time 3D ultrasound (US) makes it possible to consider
image-based tracking of subcutaneous soft tissue targets for computer guided
diagnosis and therapy. We propose a 3D transrectal US based tracking system for
precise prostate biopsy sample localisation. The aim is to improve sample
distribution, to enable targeting of unsampled regions for repeated biopsies,
and to make post-interventional quality controls possible. Since the patient is
not immobilized, since the prostate is mobile and due to the fact that probe
movements are only constrained by the rectum during biopsy acquisition, the
tracking system must be able to estimate rigid transformations that are beyond
the capture range of common image similarity measures. We propose a fast and
robust multi-resolution attribute-vector registration approach that combines
global and local optimization methods to solve this problem. Global
optimization is performed on a probe movement model that reduces the
dimensionality of the search space and thus renders optimization efficient. The
method was tested on 237 prostate volumes acquired from 14 different patients
for 3D to 3D and 3D to orthogonal 2D slices registration. The 3D-3D version of
the algorithm converged correctly in 96.7% of all cases in 6.5s with an
accuracy of 1.41mm (r.m.s.) and 3.84mm (max). The 3D to slices method yielded a
success rate of 88.9% in 2.3s with an accuracy of 1.37mm (r.m.s.) and 4.3mm
(max).
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:15:58 GMT"
}
] | 2008-01-17T00:00:00 | [
[
"Baumann",
"Michael",
"",
"TIMC"
],
[
"Mozer",
"Pierre",
"",
"TIMC"
],
[
"Daanen",
"Vincent",
"",
"TIMC"
],
[
"Troccaz",
"Jocelyne",
"",
"TIMC"
]
] | [
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712.077 | Chiara Camere | Chiara Camere | About the stability of the tangent bundle restricted to a curve | 5 pages | null | null | null | math.AG | null | Let C be a smooth projective curve with genus g>1 and Clifford index c(C) and
let L be a line bundle on C generated by its global sections. The morphism i:C
-->P(H^0(L))=P is well-defined and i*T is the restriction to C of the tangent
bundle T of the projective space P. Sharpening a theorem by Paranjape, we show
that if deg L>2g-c(C)-1 then i*T is semi-stable, specifying when it is also
stable. We then prove the existence on many curves of a line bundle L of degree
2g-c(C)-1 such that i*T is not semi-stable. Finally, we completely characterize
the (semi-)stability of i*T when C is hyperelliptic.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:31:59 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Camere",
"Chiara",
""
]
] | [
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] |
712.0771 | Colin Folsom | C. P. Folsom, G. A. Wade, O. Kochukhov, E. Alecian, C. Catala, S.
Bagnulo, J. D. Landstreet, D. A. Hanes | Magnetic, Chemical and Rotational Properties of the Herbig Ae/Be Binary
System HD 72106 | Proceedings of the CP#AP Workshop held in Vienna in September 2007 | Contrib.Astron.Obs.Skalnate Pleso 38:245-250,2008 | null | null | astro-ph | null | Recently, strong, globally-ordered magnetic fields have been detected in some
Herbig Ae and Be (HAeBe) stars, suggesting a possible evolutionary connection
to main sequence magnetic chemically peculiar Ap and Bp stars. We have
undertaken a detailed study of the binary system HD 72106, which contains a B9
magnetic primary and a HAeBe secondary, using the ESPaDOnS spectropolarimeter
mounted on the CFHT. A careful analysis of the very young primary reveals that
it has an approximately dipolar magnetic field geometry, strong chemical
peculiarities, and strong surface chemical abundance inhomogeneities. Thus the
primary is very similar to an Ap/Bp star despite having completed less then
1.5% of its main sequence life, and possibly still being on the pre-main
sequence. In contrast, a similar analysis of the secondary reveals solar
chemical abundances and no magnetic field.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:21:07 GMT"
}
] | 2010-11-26T00:00:00 | [
[
"Folsom",
"C. P.",
""
],
[
"Wade",
"G. A.",
""
],
[
"Kochukhov",
"O.",
""
],
[
"Alecian",
"E.",
""
],
[
"Catala",
"C.",
""
],
[
"Bagnulo",
"S.",
""
],
[
"Landstreet",
"J. D.",
""
],
[
"Hanes",
"D. A.",
""
]
] | [
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] |
712.0772 | Jean-Francois Gonzalez | Guillaume Laibe (CRAL), Jean-Fran\c{c}ois Gonzalez (CRAL), Laure
Fouchet (ETHZ), Sarah T. Maddison | 3D SPH simulations of grain growth in protoplanetary disks | 3 pages, 3 figures, to appear in the Proceedings of IAU Symp. 249:
Exoplanets: Detection, Formation and Dynamics (Suzhou, China) | Dans Proceedings of IAU Symp. 249 - Exoplanets: Detection,
Formation and Dynamics, Suzhou : Chine (2007) | 10.1017/S1743921308016864 | Suzhou-221007 | astro-ph | null | We present the first results of the treatment of grain growth in our 3D,
two-fluid (gas+dust) SPH code describing protoplanetary disks. We implement a
scheme able to reproduce the variation of grain sizes caused by a variety of
physical processes and test it with the analytical expression of grain growth
given by Stepinski & Valageas (1997) in simulations of a typical T Tauri disk
around a one solar mass star. The results are in agreement with a turbulent
growing process and validate the method. We are now able to simulate the grain
growth process in a protoplanetary disk given by a more realistic physical
description, currently under development. We discuss the implications of the
combined effect of grain growth and dust vertical settling and radial migration
on subsequent planetesimal formation.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:25:23 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 08:02:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Laibe",
"Guillaume",
"",
"CRAL"
],
[
"Gonzalez",
"Jean-François",
"",
"CRAL"
],
[
"Fouchet",
"Laure",
"",
"ETHZ"
],
[
"Maddison",
"Sarah T.",
""
]
] | [
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712.0773 | Neil Budko | Neil V. Budko | Influence of Absorbers on the Electromagnetic Radiation | 2 pages | null | null | null | quant-ph | null | The phenomenon of the electromagnetic absorption by arbitrarily distributed
discrete absorbers is analyzed from the photon point of view. It is shown that
apart from the decrease in the intensity of the signal the net effect of
absorption includes a relative increase in the photon bunching.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:31:13 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Budko",
"Neil V.",
""
]
] | [
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712.0774 | M. N. Rebelo | Gustavo C. Branco, David Emmanuel-Costa, M. N. Rebelo and Probir Roy | Four Zero Neutrino Yukawa Textures in the Minimal Seesaw Framework | 19 pages, no figures. To appear in Phys. Rev. D. One reference added,
minor changes, mainly typo corrections | Phys.Rev.D77:053011,2008 | 10.1103/PhysRevD.77.053011 | CERN-PH-TH/2007-217 | hep-ph | null | We investigate, within the Type I seesaw framework, the physical implications
of zero textures in the Yukawa couplings which generate the neutrino Dirac mass
matrix $m_D$. It is shown that four is the maximal number of texture zeroes
compatible with the observed leptonic mixing and the assumption that no
neutrino mass vanishes. We classify all allowed four-zero textures of $m_D$
into two categories with three classes each. We show that the different
classes, in general, admit CP violation both at low and high energies. We
further present the constraints obtained for low energy physics in each case.
The r\^ ole of these zero textures in establishing a connection between
leptogenesis and low energy data is analysed in detail. It is shown that it is
possible in all cases to completely specify the parameters relevant for
leptogenesis in terms of light neutrino masses and leptonic mixing together
with the unknown heavy neutrino masses.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:31:27 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Mar 2008 16:36:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Branco",
"Gustavo C.",
""
],
[
"Emmanuel-Costa",
"David",
""
],
[
"Rebelo",
"M. N.",
""
],
[
"Roy",
"Probir",
""
]
] | [
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] |
712.0775 | Sylvain Arlot | Sylvain Arlot, Gilles Blanchard, Etienne Roquain | Some nonasymptotic results on resampling in high dimension, I:
Confidence regions, II: Multiple tests | Published in at http://dx.doi.org/10.1214/08-AOS667;
http://dx.doi.org/10.1214/08-AOS668 the Annals of Statistics
(http://www.imstat.org/aos/) by the Institute of Mathematical Statistics
(http://www.imstat.org) | The Annals of Statistics 38, 1 (2010) 51-99 | 10.1214/08-AOS667; 10.1214/08-AOS668 | IMS-AOS-AOS667; IMS-AOS-AOS668 | math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study generalized bootstrap confidence regions for the mean of a random
vector whose coordinates have an unknown dependency structure. The random
vector is supposed to be either Gaussian or to have a symmetric and bounded
distribution. The dimensionality of the vector can possibly be much larger than
the number of observations and we focus on a nonasymptotic control of the
confidence level, following ideas inspired by recent results in learning
theory. We consider two approaches, the first based on a concentration
principle (valid for a large class of resampling weights) and the second on a
resampled quantile, specifically using Rademacher weights. Several intermediate
results established in the approach based on concentration principles are of
interest in their own right. We also discuss the question of accuracy when
using Monte Carlo approximations of the resampled quantities.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:38:59 GMT"
},
{
"version": "v2",
"created": "Mon, 6 Jul 2009 09:30:13 GMT"
},
{
"version": "v3",
"created": "Mon, 11 Jan 2010 10:31:49 GMT"
}
] | 2010-07-02T00:00:00 | [
[
"Arlot",
"Sylvain",
""
],
[
"Blanchard",
"Gilles",
""
],
[
"Roquain",
"Etienne",
""
]
] | [
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] |
712.0776 | Ronald Wilhelm Ph.D. | Ronald Wilhelm, W. Lee Powell Jr., Timothy C. Beers, Branimir Sesar,
Carlos Alende Prieto, Kenneth W. Carrell, Young Sun Lee, Brian Yanny,
Constance M. Rockosi, Nathan De Lee, Gwen Hansford Armstrong, Stephen J.
Torrence | Identification of RR Lyrae Variables in SDSS from Single-Epoch
Photometric and Spectroscopic Observations | 59 pages, 17 figures, 8 tables | null | null | null | astro-ph | null | We describe a new RR Lyrae identification technique based on out-of-phase
single-epoch photometric and spectroscopic observations contained in SDSS Data
Release 6 (DR-6). This technique detects variability by exploiting the large
disparity between the g-r color and the strength of the hydrogen Balmer lines
when the two observations are made at random phases. Comparison with a large
sample of known variables in the SDSS equatorial stripe (Stripe 82) shows that
the discovery efficiency for our technique is ~85%. Analysis of stars with
multiple spectroscopic observations suggests a similar efficiency throughout
the entire DR-6 sample. We also develop a technique to estimate the average g
apparent magnitude (over the pulsation cycle) for individual RR Lyrae stars,
using the <g-r> for the entire sample and measured colors for each star. The
resulting distances are found to have precisions of ~14%. Finally, we explore
the properties of our DR-6 sample of N = 1087 variables, and recover portions
of the Sagittarius Northern and Southern Stream. Analysis of the distance and
velocity for the Southern Stream are consistent with previously published data
for blue horizontal-branch stars. In a sample near the North Galactic Polar
Cap, we find evidence for the descending leading Northern arm, and a possible
detection of the trailing arm.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 17:32:50 GMT"
}
] | 2007-12-06T00:00:00 | [
[
"Wilhelm",
"Ronald",
""
],
[
"Powell",
"W. Lee",
"Jr."
],
[
"Beers",
"Timothy C.",
""
],
[
"Sesar",
"Branimir",
""
],
[
"Prieto",
"Carlos Alende",
""
],
[
"Carrell",
"Kenneth W.",
""
],
[
"Lee",
"Young Sun",
""
],
[
"Yanny",
"Brian",
""
],
[
"Rockosi",
"Constance M.",
""
],
[
"De Lee",
"Nathan",
""
],
[
"Armstrong",
"Gwen Hansford",
""
],
[
"Torrence",
"Stephen J.",
""
]
] | [
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] |
712.0777 | Cristian Pisano | D. Boer, P.J. Mulders, C. Pisano | T-odd effects in photon-jet production at the Tevatron | 9 pages, 3 figures; references and discussion added in Section II,
matches final version to be published in Phys. Lett. B | Phys.Lett.B660:360-368,2008 | 10.1016/j.physletb.2008.01.021 | null | hep-ph hep-ex | null | The angular distribution in photon-jet production in p \bar{p} -> \gamma jet
X is studied within a generalized factorization scheme taking into account the
transverse momentum of the partons in the initial hadrons. Within this scheme
an anomalously large cos(2\phi) asymmetry observed in the Drell-Yan process
could be attributed to the T-odd, spin and transverse momentum dependent parton
distribution function h_1^{\perp q}(x, p_{\perp}^2). This same function is
expected to produce a cos(2\phi) asymmetry in the photon-jet production cross
section. We give the expression for this particular azimuthal asymmetry, which
is estimated to be smaller than the Drell-Yan asymmetry but still of
considerable size for Tevatron kinematics. This offers a new possibility to
study T-odd effects at the Tevatron.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:58:48 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 16:02:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Boer",
"D.",
""
],
[
"Mulders",
"P. J.",
""
],
[
"Pisano",
"C.",
""
]
] | [
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] |
712.0778 | Lawrence M. Krauss | Katherine Jones-Smith, Lawrence M. Krauss, Harsh Mathur (Case Western
Reserve University) | A Nearly Scale Invariant Spectrum of Gravitational Radiation from Global
Phase Transitions | 4 pages, PRL published version | Phys.Rev.Lett.100:131302,2008 | 10.1103/PhysRevLett.100.131302 | null | astro-ph gr-qc hep-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using a large N sigma model approximation we explicitly calculate the power
spectrum of gravitational waves arising from a global phase transition in the
early universe and we confirm that it is scale invariant, implying an
observation of such a spectrum may not be a unique feature of inflation.
Moreover, the predicted amplitude can be over 3 orders of magnitude larger than
the naive dimensional estimate, implying that even a transition that occurs
after inflation may dominate in Cosmic Microwave Background polarization or
other gravity wave signals.
| [
{
"version": "v1",
"created": "Wed, 5 Dec 2007 16:53:41 GMT"
},
{
"version": "v2",
"created": "Tue, 24 Jun 2008 19:50:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Jones-Smith",
"Katherine",
"",
"Case Western\n Reserve University"
],
[
"Krauss",
"Lawrence M.",
"",
"Case Western\n Reserve University"
],
[
"Mathur",
"Harsh",
"",
"Case Western\n Reserve University"
]
] | [
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