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801.2173 | Simon Caron-Huot | Simon Caron-Huot, Guy D. Moore | Heavy quark diffusion in QCD and N=4 SYM at next-to-leading order | 40 pages, 14 figures | JHEP 0802:081,2008 | 10.1088/1126-6708/2008/02/081 | null | hep-ph | null | We present the full details of a calculation at next-to-leading order of the
momentum diffusion coefficient of a heavy quark in a hot, weakly coupled, QCD
plasma. Corrections arise at O(g_s); physically they represent interference
between overlapping scatterings, as well as soft, electric scale (p ~ gT) gauge
field physics, which we treat using the hard thermal loop (HTL) effective
theory. In 3-color, 3-flavor QCD, the momentum diffusion constant of a
fundamental representation heavy quark at NLO is kappa = (16\pi/3) alpha_s^2
T^3 (log(1/g) + 0.07428 + 1.9026 g). We extend the computation to a heavy
fundamental representation ``probe'' quark in large N_c, N=4 Super Yang-Mills
theory, where the result is kappa^{SYM}= (lambda^2 T^3)(6\pi)
(log(1/\sqrt{\lambda}) + 0.4304 + 0.8010 \sqrt{lambda}) (where lambda=g_s^2 N_c
is the t'Hooft coupling). In the absence of some resummation technique, the
convergence of perturbation theory is poor.
| [
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801.2174 | Ivan Gonzalez | I. Gonzalez, S. Okamoto, S. Yunoki, A. Moreo and E. Dagotto | Charge transfer in heterostructures of strongly correlated materials | 14 pages, 9 figures. Invited article for a special issue of JPCM on
Metal Oxide Thin Films; minor changes in the text | null | 10.1088/0953-8984/20/26/264002 | null | cond-mat.str-el | null | In this manuscript, recent theoretical investigations by the authors in the
area of oxide multilayers are briefly reviewed. The calculations were carried
out using model Hamiltonians and a variety of non-perturbative techniques.
Moreover, new results are also included here. They correspond to the generation
of a metallic state by mixing insulators in a multilayer geometry, using the
Hubbard and Double Exchange models. For the latter, the resulting metallic
state is also ferromagnetic. This illustrates how electron or hole doping via
transfer of charge in multilayers can lead to the study of phase diagrams of
transition metal oxides in the clean limit. Currently, these phase diagrams are
much affected by the disordering standard chemical doping procedure, which
introduces quenched disorder in the material.
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] | 2009-11-13T00:00:00 | [
[
"Gonzalez",
"I.",
""
],
[
"Okamoto",
"S.",
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801.2175 | Johannes Gro{\ss}e | Johannes Gro{\ss}e | MathPSfrag 2: Convenient LaTeX Labels in Mathematica | 9 pages, package can be found at
http://wwwth.mppmu.mpg.de/members/jgrosse/mathpsfrag/ | null | null | null | cs.GR | null | This article introduces the next version of MathPSfrag. MathPSfrag is a
Mathematica package that during export automatically replaces all expressions
in a plot by corresponding LaTeX commands. The new version can also produce
LaTeX independent images; e.g., PDF files for inclusion in pdfLaTeX. Moreover
from these files a preview is generated and shown within Mathematica.
| [
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"version": "v1",
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""
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801.2176 | Marcelo Loewe | Marcelo Loewe and Cristian Mart\'inez V | Thermal Corrections to $\pi$-$\pi$ Scattering Lengths in the Linear
Sigma Model | 8 pages. Keywords: Finite temperature field theory; scattering
lengths; linear sigma model. A new reference has been added. Written in
RevTex4. The paper is being accepted for publication in Phys. Rev. D. The
size of the manuscript was reduced considerably | Phys.Rev.D77:105006,2008; Erratum-ibid.D78:069902,2008 | 10.1103/PhysRevD.77.105006 10.1103/PhysRevD.78.069902 | null | hep-ph | null | In this article we explore the thermal evolution of the $\pi$-$\pi$
scattering lengths in the frame of the linear sigma model. We compute, using
thermofield dynamics, all the one loop diagrams that contribute to $\pi$-$\pi$
scattering. We restrict ourselves to temperature correction only in the pion
sector, due to the Boltzmann supression for the sigma meson. From this analysis
we obtain the thermal behavior of $a_0^0$ and $a_0^2$, s-waves scattering
lengths in the isospin channel I=0 and I=2 respectively. It turns out that
$a_0^0$ grows whereas $a_0^2$ diminishes as function of temperature. We compare
our results with other determinations of the thermal behavior of these
magnitudes.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 22:38:44 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 00:56:18 GMT"
},
{
"version": "v3",
"created": "Wed, 23 Jan 2008 21:57:46 GMT"
},
{
"version": "v4",
"created": "Thu, 27 Mar 2008 20:38:44 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Loewe",
"Marcelo",
""
],
[
"Martínez",
"Cristian",
"V"
]
] | [
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] |
801.2177 | N. J. Turner | N. J. Turner, K. Grogan and J. B. Breckinridge | Probing Interstellar Dust With Space-Based Coronagraphs | Accepted for publication in ApJ Supplements | null | 10.1086/587061 | null | astro-ph | null | We show that space-based telescopes such as the proposed Terrestrial Planet
Finder Coronagraph will be able to detect the light scattered by the
interstellar grains along lines of sight passing near stars in our Galaxy. The
relative flux of the scattered light within one arcsecond of a star at 100 pc
in a uniform interstellar medium of 0.1 H atoms cm^-3 is about 10^-7. The halo
increases in strength with the distance to the star and is unlikely to limit
the coronagraphic detection of planets around the nearest stars. Grains passing
within 100 AU of Sun-like stars are deflected by radiation, gravity and
magnetic forces, leading to features in the scattered light that can
potentially reveal the strength of the stellar wind, the orientation of the
stellar magnetic field and the relative motion between the star and the
surrounding interstellar medium.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 22:59:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Turner",
"N. J.",
""
],
[
"Grogan",
"K.",
""
],
[
"Breckinridge",
"J. B.",
""
]
] | [
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801.2178 | Elena Orlando | Elena Orlando, Andrew W. Strong | Gamma-ray emission from the solar halo and disk: a study with EGRET data | Corrected typos, added acknowledgements. A&A in press | Astron.Astrophys.480:847,2008 | 10.1051/0004-6361:20078817 | null | astro-ph | null | Context: The Sun has recently been predicted to be an extended source of
gamma-ray emission, produced by inverse-Compton (IC) scattering of cosmic-ray
(CR) electrons on the solar radiation field. The emission was predicted to be
extended and a confusing foreground for the diffuse extragalactic background
even at large angular distances from the Sun. The solar disk is also expected
to be a steady gamma-ray source. While these emissions are expected to be
readily detectable in the future by GLAST, the situation for available EGRET
data is more challenging. Aims: The theory of gamma-ray emission from IC
scattering on the solar radiation field by Galactic CR electrons is given in
detail. This is used as the basis for detection and model verification using
EGRET data. Methods: We present a detailed study of the solar emission using
the EGRET database, accounting for the effect of the emission from 3C 279, the
moon, and other sources, which interfere with the solar emission. The analysis
was performed for 2 energy ranges, above 300 MeV and for 100-300 MeV, as well
as for the combination to improve the detection statistics. The technique was
tested on the moon signal, with our results consistent with previous work.
Results: Analyzing the EGRET database, we find evidence of emission from the
solar disk and its halo. The observations are compared with our model for the
extended emission. The spectrum of the solar disk emission and the spectrum of
the extended emission have been obtained. The spectrum of the moon is also
given. Conclusions: The observed intensity distribution and the flux are
consistent with the predicted model of IC gamma-rays from the halo around the
Sun.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:07:31 GMT"
},
{
"version": "v2",
"created": "Sun, 10 Feb 2008 16:20:01 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Orlando",
"Elena",
""
],
[
"Strong",
"Andrew W.",
""
]
] | [
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] |
801.2179 | Terence C. Tao | Tim Austin, Terence Tao | On the testability and repair of hereditary hypergraph properties | 84 pages, 3 figures, to appear, Random Structures and Algorithms.
Referee recommendations incorporated (in particular, a longer introduction) | null | null | null | math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Recent works of Alon-Shapira and R\"odl-Schacht have demonstrated that every
hereditary property of undirected graphs or hypergraphs is testable with
one-sided error; informally, this means that if a graph or hypergraph satisfies
that property "locally" with sufficiently high probability, then it can be
perturbed (or "repaired") into a graph or hypergraph which satisfies that
property "globally".
In this paper we make some refinements to these results, some of which may be
surprising. In the positive direction, we strengthen the results to cover
hereditary properties of multiple directed polychromatic graphs and
hypergraphs. In the case of undirected graphs, we extend the result to
continuous graphs on probability spaces, and show that the repair algorithm is
"local" in the sense that it only depends on a bounded amount of data; in
particular, the graph can be repaired in a time linear in the number of edges.
We also show that local repairability also holds for monotone or partite
hypergraph properties (this latter result is also implicitly in work of
Ishigami). In the negative direction, we show that local repairability breaks
down for directed graphs, or for undirected 3-uniform hypergraphs. The reason
for this contrast in behavior stems from (the limitations of) Ramsey theory.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:07:48 GMT"
},
{
"version": "v2",
"created": "Tue, 12 May 2009 06:27:25 GMT"
}
] | 2009-05-12T00:00:00 | [
[
"Austin",
"Tim",
""
],
[
"Tao",
"Terence",
""
]
] | [
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801.218 | Mikhail Skvortsov | D. A. Ivanov and M. A. Skvortsov | Dyson-Maleev representation of nonlinear sigma-models | 16 pages, 1 figure | J.Phys.A41:215003,2008 | 10.1088/1751-8113/41/21/215003 | null | cond-mat.mes-hall cond-mat.dis-nn | null | For nonlinear sigma-models in the unitary symmetry class, the non-linear
target space can be parameterized with cubic polynomials. This choice of
coordinates has been known previously as the Dyson-Maleev parameterization for
spin systems, and we show that it can be applied to a wide range of
sigma-models. The practical use of this parameterization includes
simplification of diagrammatic calculations (in perturbative methods) and of
algebraic manipulations (in non-perturbative approaches). We illustrate the use
and specific issues of the Dyson-Maleev parameterization with three examples:
the Keldysh sigma-model for time-dependent random Hamiltonians, the
supersymmetric sigma-model for random matrices, and the supersymmetric
transfer-matrix technique for quasi-one-dimensional disordered wires. We
demonstrate that nonlinear sigma-models of unitary-like symmetry classes C and
B/D also admit the Dyson-Maleev parameterization.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:22:44 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ivanov",
"D. A.",
""
],
[
"Skvortsov",
"M. A.",
""
]
] | [
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] |
801.2181 | Daniel Silevitch | C. Ancona-Torres, D. M. Silevitch, G. Aeppli, T. F. Rosenbaum | Quantum and Classical Glass Transitions in $Li Ho_x Y_{1-x} F_4$ | 5 pages, 5 figures. Updated figure 3 with corrected calibration
information for thermometry | Phys. Rev. Lett. 101, 057201 (2008) | 10.1103/PhysRevLett.101.057201 | null | cond-mat.dis-nn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | When performed in the proper low field, low frequency limits, measurements of
the dynamics and the nonlinear susceptibility in the model Ising magnet in
transverse field, $\text{LiHo}_x\text{Y}_{1-x}\text{F}_4$, prove the existence
of a spin glass transition for $x$ = 0.167 and 0.198. The classical behavior
tracks for the two concentrations, but the behavior in the quantum regime at
large transverse fields differs because of the competing effects of quantum
entanglement and random fields.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 15:11:04 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 18:34:46 GMT"
},
{
"version": "v3",
"created": "Wed, 23 Jan 2008 14:28:57 GMT"
},
{
"version": "v4",
"created": "Mon, 26 Oct 2009 19:33:31 GMT"
}
] | 2009-10-26T00:00:00 | [
[
"Ancona-Torres",
"C.",
""
],
[
"Silevitch",
"D. M.",
""
],
[
"Aeppli",
"G.",
""
],
[
"Rosenbaum",
"T. F.",
""
]
] | [
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] |
801.2182 | Fabio D. A. Aarao Reis | R. B. Stinchcombe, F. D. A. Aar\~ao Reis | Modeling one-dimensional island growth with mass-dependent detachment
rates | 16 pages, 6 figures | Published in Phys. Rev. B 77, 035406 (2008) | 10.1103/PhysRevB.77.035406 | null | cond-mat.stat-mech cond-mat.mtrl-sci | null | We study one-dimensional models of particle diffusion and
attachment/detachment from islands where the detachment rates gamma(m) of
particles at the cluster edges increase with cluster mass m. They are expected
to mimic the effects of lattice mismatch with the substrate and/or long-range
repulsive interactions that work against the formation of long islands.
Short-range attraction is represented by an overall factor epsilon<<1 in the
detachment rates relatively to isolated particle hopping rates [epsilon ~
exp(-E/T), with binding energy E and temperature T]. We consider various
gamma(m), from rapidly increasing forms such as gamma(m) ~ m to slowly
increasing ones, such as gamma(m) ~ [m/(m+1)]^b. A mapping onto a column
problem shows that these systems are zero-range processes, whose steady states
properties are exactly calculated under the assumption of independent column
heights in the Master equation. Simulation provides island size distributions
which confirm analytic reductions and are useful whenever the analytical tools
cannot provide results in closed form. The shape of island size distributions
can be changed from monomodal to monotonically decreasing by tuning the
temperature or changing the particle density rho. Small values of the scaling
variable X=epsilon^{-1}rho/(1-rho) favour the monotonically decreasing ones.
However, for large X, rapidly increasing gamma(m) lead to distributions with
peaks very close to <m> and rapidly decreasing tails, while slowly increasing
gamma(m) provide peaks close to <m>/2$ and fat right tails.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:12:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Stinchcombe",
"R. B.",
""
],
[
"Reis",
"F. D. A. Aarão",
""
]
] | [
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] |
801.2183 | Rudolph C. Hwa | Charles B. Chiu, Rudolph C. Hwa and C. B. Yang | Azimuthal Anisotropy: Ridges, Recombination and Breaking of Quark Number
Scaling | 17 pages including 13 figures. This is a revised version with
additional material and author | null | 10.1103/PhysRevC.78.044903 | null | nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Azimuthal anisotropy is studied by taking into account the ridges created by
semi-hard scattering, which is sensitive to the initial spatial configuration
in non-central heavy-ion collisions. No rapid thermalization is required.
Although hydrodynamics is not used in this study, the validity of
hydrodynamical expansion is not excluded at later time after equilibration is
achieved. Phenomenological properties of the bulk and ridge behaviors are used
as inputs to determine the elliptic flow of pion and proton at low p_T. At
intermediate p_T the recombination of shower partons with thermal partons
becomes more important. The phi dependence arises from the variation of the
in-medium path length of the hard parton that generates the shower. The p_T
dependence of v_2 is therefore very different at intermediate p_T compared to
that at low p_T. Quark number scaling of v_2 is shown to be only approximately
valid at low p_T, but is broken at intermediate p_T, even though recombination
is the mechanism of hadronization in all p_T regions considered.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:27:39 GMT"
},
{
"version": "v2",
"created": "Fri, 10 Oct 2008 21:21:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chiu",
"Charles B.",
""
],
[
"Hwa",
"Rudolph C.",
""
],
[
"Yang",
"C. B.",
""
]
] | [
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-0.0628278479,
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] |
801.2184 | D. N. Matsukevich | D. N. Matsukevich, P. Maunz, D. L. Moehring, S. Olmschenk and C.
Monroe | Bell inequality violation with two remote atomic qubits | 4 pages, 4 figures | Phys. Rev. Lett. 100, 150404 (2008) | 10.1103/PhysRevLett.100.150404 | null | quant-ph | null | We observe violation of a Bell inequality between the quantum states of two
remote Yb ions separated by a distance of about one meter with the detection
loophole closed. The heralded entanglement of two ions is established via
interference and joint detection of two emitted photons, whose polarization is
entangled with each ion. The entanglement of remote qubits is also
characterized by full quantum state tomography.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:35:12 GMT"
}
] | 2008-05-20T00:00:00 | [
[
"Matsukevich",
"D. N.",
""
],
[
"Maunz",
"P.",
""
],
[
"Moehring",
"D. L.",
""
],
[
"Olmschenk",
"S.",
""
],
[
"Monroe",
"C.",
""
]
] | [
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] |
801.2185 | Xiaohu Shang | Xiaohu Shang, Gerhard Kramer, Biao Chen | New Outer Bounds on the Capacity Region of Gaussian Interference
Channels | 5 pages, 2 figures, submitted to ISIT 2008 | null | null | null | cs.IT math.IT | null | Recent outer bounds on the capacity region of Gaussian interference channels
are generalized to $m$-user channels with $m>2$ and asymmetric powers and
crosstalk coefficients. The bounds are again shown to give the sum-rate
capacity for Gaussian interference channels with low powers and crosstalk
coefficients. The capacity is achieved by using single-user detection at each
receiver, i.e., treating the interference as noise incurs no loss in
performance.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:48:05 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Shang",
"Xiaohu",
""
],
[
"Kramer",
"Gerhard",
""
],
[
"Chen",
"Biao",
""
]
] | [
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] |
801.2186 | Hans J. Deeg | H. J. Deeg (1), B. Oca\~na (1,2), V. P. Kozhevnikov (3), D.
Charbonneau (4), F. T. O'Donovan (5), L.R. Doyle (6) ((1) IAC, (2) IRAM, (3)
Ural State U., (4) Harvard U., (5) Caltech, (6) SETI) | Extrasolar planet detection by binary stellar eclipse timing: evidence
for a third body around CM Draconis | 10 pages, 5 figures, accepted by A&A. V2: fixed spelling of one of
the authors. V3: fixed error in distance to CM Dra, implying minor changes to
several derived numbers | null | 10.1051/0004-6361:20079000 | null | astro-ph | null | Context: New eclipse minimum timings of the M4.5/M4.5 binary CM Dra were
obtained between the years 2000 and 2007. In combination with published timings
going back to 1977, a clear non-linearity in observed-minus-calculated (O-C)
times has become apparent. Several models are applied to explain the observed
timing behavior.
Aims: Revealing the processes that cause the observed O-C behavior, and
testing the evidence for a third body around the CM Dra system.
Methods: The O-C times of the system were fitted against several functions,
representing different physical origins of the timing variations.
Results: An analysis using model-selection statistics gives about equal
weight to a parabolic and to a sinusoidal fitting function. Attraction from a
third body, either at large distance in a quasi-constant constellation across
the years of observations or from a body on a shorter orbit generating
periodicities in O-C times is the most likely source of the observed O-C times.
The white dwarf GJ 630.1B, a proper motion companion of CM Dra, can however be
rejected as the responsible third body. Also, no further evidence of the
short-periodic planet candidate described by Deeg et al. (2000) is found,
whereas other mechanisms, such as period changes from stellar winds or
Applegate's mechanism can be rejected.
Conclusions: A third body, being either a few-Jupiter-mass object with a
period of 18.5+-4.5 years or an object in the mass range of 1.5M_jup to
0.1M_sun with periods of hundreds to thousands of years is the most likely
origin of the observed minimum timing behavior.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:49:56 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 18:50:07 GMT"
},
{
"version": "v3",
"created": "Wed, 13 Feb 2008 15:49:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Deeg",
"H. J.",
""
],
[
"Ocaña",
"B.",
""
],
[
"Kozhevnikov",
"V. P.",
""
],
[
"Charbonneau",
"D.",
""
],
[
"O'Donovan",
"F. T.",
""
],
[
"Doyle",
"L. R.",
""
]
] | [
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801.2187 | Ephraim Feig | Ephraim Feig, Vivian Feig | A One-Way Function Based On The Extended Euclidean Algorithm | 2-page correspondence | null | null | null | cs.CR | null | A problem based on the Extended Euclidean Algorithm applied to a class of
polynomials with many factors is presented and believed to be hard. If so, it
is a one-way function well suited for applications in digital signicatures.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 23:58:01 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Feig",
"Ephraim",
""
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801.2188 | David Sherrington | David Sherrington | A Simple Spin Glass Perspective on Martensitic Shape-memory Alloys | This paper is dedicated to John Pendry in celebration of his 65th
birthday. It has been accepted for a special issue of J.Phys.CM. This version
corrects a typo, includes a new recent reference and indicates an alternative
formulation for 3D | J.Phys.: Condens.Matter 20, 304213 (2008) | 10.1088/0953-8984/20/30/304213 | null | cond-mat.dis-nn cond-mat.mtrl-sci | null | A brief qualitative mapping is given between austenite, tweed and twinned
phases of martensite alloys and corresponding paramagnetic, spin glass and
periodic phases in spin glass alloys.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 00:11:18 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Mar 2008 23:54:11 GMT"
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] | 2009-11-13T00:00:00 | [
[
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801.2189 | T. Goldman | T. Goldman and R.R. Silbar | The Effect of Pion Exchange in a Relativistic Quark Model of Baryons | 31 pp., 8 figs., submitted to Phys Rev C | Phys.Rev.C77:065203,2008 | 10.1103/PhysRevC.77.065203 | LA-UR-08-0168 | nucl-th | null | We examine the effect of adding pion exchange between quarks and pion
self-energy corrections to the Los Alamos Relativistic Quark model with a short
distance cutoff of the Bethe form. The contributions to the nucleon and the
Delta-baryon are small. We conclude that the model is stable under this change
in the sense that significant changes to the model parameters are not required.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 00:13:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Goldman",
"T.",
""
],
[
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"R. R.",
""
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] |
801.219 | Maciej Bzowski | M. Bzowski (Space Research Centre PAS, Warsaw, Poland) | Survival probability and energy modification of hydrogen Energetic
Neutral Atoms on their way from the termination shock to Earth orbit | final version, accepted by A&A, missing figure panels added | null | 10.1051/0004-6361:200809393 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Context: With the forthcoming launch of a NASA SMEX mission IBEX devoted to
imaging of heliospheric interface by in-situ detection of Energetic Neutral
Atoms (ENA) an important issue becomes recognizing of transport of these atoms
from the termination shock of the solar wind to Earth orbit.
Aims: Investigate modifications of energy and of survival probability of the
H ENA detectable by IBEX (0.01 -- 6 keV) between the termination shock and
Earth orbit taking into account the influence of the variable and anisotropic
solar wind and solar EUV radiation.
Methods: Energy change of the atoms is calculated by numerical simulations of
orbits of the H ENA atoms from ~100 AU from the Sun down to Earth orbit, taking
into account solar gravity and Lyman-$\alpha$ radiation pressure, which is
variable in time and depends on radial velocity of the atom. To calculate
survival probabilities of the atoms against onization, a detailed 3D and
time-dependent model of H ENA ionization based on observations of the solar
wind and EUV ionizing radiation is constructed, and wth the use of this model
probabilities of survival of the atoms are calculated by numerical integration
along the previously calculated orbits.
Results: Owing to the radiation pressure, H ENA reach the Earth orbit
practically without energy and direction change except the atoms with energy
lower than 0.1 keV during high solar activity. For a given energy at Earth
orbit one expects fluctuations of survival probability from ~20% at 0.01 keV
down to just a few percent at 6 keV and a modulation of survival probability as
a function of the location at Earth orbit, ecliptic latitude of the arrival
direction, and the phase of solar cycle with an amplitude of a few dozen
percent for 0.1 keV atoms at solar minimum to a few percent for 6 keV atoms at
solar maximum.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 01:04:49 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 11:41:56 GMT"
},
{
"version": "v3",
"created": "Tue, 3 Jun 2008 11:28:47 GMT"
},
{
"version": "v4",
"created": "Sat, 14 Jun 2008 08:39:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bzowski",
"M.",
"",
"Space Research Centre PAS, Warsaw, Poland"
]
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801.2191 | Mikhail Vasiliev a | O.A.Gelfond and M.A.Vasiliev | Higher Spin Fields in Siegel Space, Currents and Theta Functions | LaTeX, 38 pages, v.3: clarifications, acknowledgements and references
added, typos corrected, v.4: more comments and references added, typos
corrected, the version to appear in JHEP | JHEP 0903:125,2009 | 10.1088/1126-6708/2009/03/125 | FIAN/TD/12-08 | hep-th math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Dynamics of four-dimensional massless fields of all spins is formulated in
the Siegel space of complex $4\times 4$ symmetric matrices. It is shown that
the unfolded equations of free massless fields, that have a form of
multidimensional Schrodinger equations, naturally distinguish between positive-
and negative-frequency solutions of relativistic field equations, i.e.
particles and antiparticles. Multidimensional Riemann theta functions are shown
to solve massless field equations in the Siegel space. We establish the
correspondence between conserved higher-spin currents in four-dimensional
Minkowski space and those in the ten-dimensional matrix space. It is shown that
global symmetry parameters of the current in the matrix space should be
singular to reproduce a nonzero current in Minkowski space. The $\D$-function
integral evolution formulae for 4d massless fields in the Fock-Siegel space are
obtained. The generalization of the proposed scheme to higher dimensions and
systems of higher ranks is considered.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 01:27:25 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jan 2008 23:14:48 GMT"
},
{
"version": "v3",
"created": "Fri, 12 Dec 2008 21:45:07 GMT"
},
{
"version": "v4",
"created": "Sun, 29 Mar 2009 22:13:03 GMT"
}
] | 2009-10-21T00:00:00 | [
[
"Gelfond",
"O. A.",
""
],
[
"Vasiliev",
"M. A.",
""
]
] | [
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] |
801.2192 | Laurent Loinard | Laurent Loinard (CRyA-UNAM), Rosa M. Torres (CRyA-UNAM), Amy
Mioduszewski (AOC-NRAO), Luis F. Rodriguez (CRyA-UNAM) | A Preliminary VLBA Distance to the Core of Ophiuchus, with an Accuracy
of 4% | Changes to title to comply with ApJL style. Paper no published as ApJ
675, L29, 2008 | null | 10.1096/529548 | null | astro-ph | null | The non-thermal 3.6 cm radio continuum emission from the young stars
S1 and DoAr21 in the core of Ophiuchus, has been observed with the
Very Long Baseline Array (VLBA) at 6 and 7 epochs, respectively, between June
2005 and August 2006. The typical separation between successive observations
was 2 to 3 months. Thanks to the remarkably accurate astrometry delivered by
the VLBA, the trajectory described by both stars on the plane of the sky could
be traced very precisely, and modeled as the superposition of their
trigonometric parallax and a uniform proper motion. The best fits yield
distances to S1 and DoAr21 of 116.9$^{+7.2}_{-6.4}$ pc and
121.9$^{+5.8}_{-5.3}$ pc, respectively. Combining these results, we estimate
the mean distance to the Ophiuchus core to be 120.0$^{+4.5}_{-4.2}$ pc, a value
consistent with several recent indirect determinations, but with a
significantly improved accuracy of 4%. Both S1 and DoAr21 happen to be members
of tight binary systems, but our observations are not frequent enough to
properly derive the corresponding orbital parameters. This could be done with
additional data, however, and would result in a significantly improved accuracy
on the distance determination.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 01:32:32 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 15:01:09 GMT"
}
] | 2008-03-21T00:00:00 | [
[
"Loinard",
"Laurent",
"",
"CRyA-UNAM"
],
[
"Torres",
"Rosa M.",
"",
"CRyA-UNAM"
],
[
"Mioduszewski",
"Amy",
"",
"AOC-NRAO"
],
[
"Rodriguez",
"Luis F.",
"",
"CRyA-UNAM"
]
] | [
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] |
801.2193 | Arnab Das | Arnab Das and Bikas K. Chakrabarti | Quantum Annealing and Analog Quantum Computation | 22 pages, 7 figs (color online); new References Added. Reviews of
Modern Physics (in press) | Rev. Mod. Phys., 80, 1061 (2008) | 10.1103/RevModPhys.80.1061 | null | quant-ph cond-mat.stat-mech physics.comp-ph | null | We review here the recent success in quantum annealing, i.e., optimization of
the cost or energy functions of complex systems utilizing quantum fluctuations.
The concept is introduced in successive steps through the studies of mapping of
such computationally hard problems to the classical spin glass problems. The
quantum spin glass problems arise with the introduction of quantum
fluctuations, and the annealing behavior of the systems as these fluctuations
are reduced slowly to zero. This provides a general framework for realizing
analog quantum computation.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 01:32:58 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 15:06:41 GMT"
},
{
"version": "v3",
"created": "Mon, 24 Mar 2008 15:42:32 GMT"
}
] | 2010-09-21T00:00:00 | [
[
"Das",
"Arnab",
""
],
[
"Chakrabarti",
"Bikas K.",
""
]
] | [
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] |
801.2194 | Takeshi Oda | T. Oda, T. Totani, N. Yasuda, T. Sumi, T. Morokuma, M. Doi, G. Kosugi | Implications for Galaxy Evolution from the Cosmic Evolution of Supernova
Rate Density | 15 pages, 8 figures, accepted to PASJ | null | 10.1093/pasj/60.2.169 | null | astro-ph | null | We report a comprehensive statistical analysis of the observational data of
the cosmic evolution of supernova (SN) rate density, to derive constraints on
cosmic star formation history and the nature of type Ia supernova (SN Ia)
progenitor. We use all available information of magnitude, SN type, and
redshift information of both type Ia and core-collapse (CC) SNe in GOODS and
SDF, as well as SN Ia rate densities reported in the literature. Furthermore,
we also add 157 SN candidates in the past Subaru/Suprime-Cam data that are
newly reported here, to increase the statistics. We find that the current data
set of SN rate density evolution already gives a meaningful constraint on the
evolution of the cosmic star formation rate (SFR) at z <~ 1, though strong
constraints cannot be derived for the delay time distribution (DTD) of SNe Ia.
We derive a constraint of the evolutionary index of SFR density alpha ~ 3--4
[(1+z)^alpha at z <~ 1] with an evidence for a significant evolution of mean
extinction of CC SNe [E(B-V) ~ 0.5 at z ~ 0.5 compared with ~ 0.2 at z = 0],
which does not change significantly within a reasonable range of various DTD
models. This result is nicely consistent with the systematic trend of alpha
estimates based on galactic SFR indicators in different wavelengths
(ultraviolet, H_alpha, and infrared), indicating that there is a strong
evolution in mean extinction of star forming regions in galaxies at relatively
low redshift range of z <~ 0.5. These results are obtained by a method that is
completely independent of galaxy surveys, and especially, there is no detection
limit about the host galaxy luminosity in our analysis, giving a strong
constraint on the star formation activity in high-z dwarf galaxies or
intergalactic space.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 02:32:05 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Oda",
"T.",
""
],
[
"Totani",
"T.",
""
],
[
"Yasuda",
"N.",
""
],
[
"Sumi",
"T.",
""
],
[
"Morokuma",
"T.",
""
],
[
"Doi",
"M.",
""
],
[
"Kosugi",
"G.",
""
]
] | [
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] |
801.2195 | Chunbin Yang | L.L. Zhu, H. Zheng and C.B. Yang | Scaling Behavior of Transverse Kinetic Energy Distributions in Au+Au
Collisions at $\sqrt{s_{\rm NN}}=200$ GeV | 5 pages, 5 eps figures included, to be appeared in Nucl. Phys. A | Nucl.Phys.A802:122-130,2008 | 10.1016/j.nuclphysa.2008.01.006 | null | nucl-th | null | With the experimental data from STAR on the centrality dependence of
transverse momentum $p_T$ spectra of pions and protons in Au+Au collisions at
$\sqrt{s_{NN}}=200 {\rm GeV}$, we investigate the scaling properties of
transverse energy $E_T$ distributions at different centralities. In the
framework of cluster formation and decay mechanism for particle production, the
universal transverse energy distributions for pion and proton can be described
separately but not simultaneously.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 01:50:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Zhu",
"L. L.",
""
],
[
"Zheng",
"H.",
""
],
[
"Yang",
"C. B.",
""
]
] | [
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801.2196 | Rodolfo Baggio | Rodolfo Baggio | Tourism networks and computer networks | 10 pages, 3 figures, 2 tables | null | null | null | physics.soc-ph | null | The body of knowledge accumulated in recent years on the structure and the
dynamics of complex networks has offered useful insights on the behaviour of
many natural and artificial complex systems. The analysis of some of these,
namely those formed by companies and institutions, however, has proved
problematical mainly for the difficulties in collecting a reasonable amount of
data. This contribution argues that the World Wide Web can provide an efficient
and effective way to gather significant samples of networked socio-economic
systems to be used for network analyses and simulations. The case discussed
refers to a tourism destination, the fundamental subsystem of an industry which
can be considered one of the most important in today's World economy.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 02:03:33 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Baggio",
"Rodolfo",
""
]
] | [
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] |
801.2197 | Gerhard Kramm | Gerhard Kramm and Fritz Herbert | Heuristic Derivation of Blackbody Radiation Laws using Principles of
Dimensional Analysis | null | null | null | null | math-ph math.MP | null | A generalized form of Wien's displacement law and the blackbody radiation
laws of (a) Rayleigh and Jeans, (b) Rayleigh, (c) Wien and Paschen, (d) Thiesen
and (e) Planck are derived using principles of dimensional analysis. This kind
of scaling is expressed in a strictly mathematical manner employing dimensional
pi-invariants analysis sometimes called Buckingham's pi-theorem. It is shown
that in the case of the classical radiation law of Rayleigh and Jeans only one
pi number occurs that has to be considered as a non-dimensional universal
constant. This pi number may be determined theoretically or/and empirically. It
is also shown that dimensional pi-invariants analysis yields a generalized form
of Wien's displacement law. In this instance two pi numbers generally occur.
Consequently, a universal function is established that is indispensable to
avoid the so-called Rayleigh-Jeans catastrophe in the ultraviolet.
Unfortunately, such a universal function cannot be inferred from dimensional
arguments. It has to be derived theoretically or/and empirically, too. It is
shown that such a similarity function can be deduced on the basis of heuristic
principles, when criteria like the maximum condition regarding the generalized
form of Wien's displacement law, the requirement of the power law of Stefan and
Boltzmann, and Ehrenfest's arguments regarding the red and the violet
requirements are adopted.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 02:12:07 GMT"
},
{
"version": "v2",
"created": "Sat, 22 Mar 2008 01:57:15 GMT"
}
] | 2008-03-22T00:00:00 | [
[
"Kramm",
"Gerhard",
""
],
[
"Herbert",
"Fritz",
""
]
] | [
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] |
801.2198 | Osamu Fujino | Osamu Fujino | Theory of non-lc ideal sheaves -basic properties- | 21 pages; v2: mistakes were corrected, v3: the proof of the main
theorem was revised, v4: minor modifications, v5: minor revision following
referee's comments | Kyoto J. Math. 50, no. 2 (2010), 225-245 | 10.1215/0023608X-2009-011 | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce the notion of non-lc ideal sheaves. It is an analogue of the
notion of multiplier ideal sheaves. We establish the restriction theorem, which
seems to be the most important property of non-lc ideal sheaves.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 02:40:05 GMT"
},
{
"version": "v2",
"created": "Sun, 11 May 2008 01:25:58 GMT"
},
{
"version": "v3",
"created": "Wed, 11 Mar 2009 05:37:00 GMT"
},
{
"version": "v4",
"created": "Fri, 17 Jul 2009 10:52:33 GMT"
},
{
"version": "v5",
"created": "Sun, 25 Oct 2009 12:51:05 GMT"
}
] | 2015-01-14T00:00:00 | [
[
"Fujino",
"Osamu",
""
]
] | [
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] |
801.2199 | Yue-Liang Wu | Jian-Wei Cui and Yue-Liang Wu (KITPC/Itp-Cas) | One-Loop Renormalization of Non-Abelian Gauge Theory and \beta Function
Based on Loop Regularization Method | 32 pages, 7 figures, references added | Int.J.Mod.Phys.A23:2861-2913,2008 | 10.1142/S0217751X08040305 | null | hep-ph hep-th | null | All one-loop renormalization constants for Non-Abelian gauge theory are
computed in details by using the symmetry-preserving Loop Regularization method
proposed in\cite{LR1,LR2}. The resulting renormalization constants are
manifestly shown to satisfy Ward-Takahaski-Slavnov-Taylor identities, and lead
to the well-known one loop $\beta$ function for Non-Abelian gauge theory of
QCD\cite{GWP}. The loop regularization method is realized in the dimension of
original field theories, it maintains not only symmetries but also divergent
behaviors of original field theories with the introduction of two energy
scales. Such two scales play the roles of characterizing and sliding energy
scales as well as ultraviolet and infrared cutoff energy scales. An explicit
Check of those identities provides a clear demonstration how the
symmetry-preserving Loop Regularization method can consistently be applied to
non-Abelian gauge theories.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 03:00:08 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 02:16:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cui",
"Jian-Wei",
"",
"KITPC/Itp-Cas"
],
[
"Wu",
"Yue-Liang",
"",
"KITPC/Itp-Cas"
]
] | [
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] |
801.22 | Woonyoung So | W. Y. So, T. Udagawa, S. W. Hong, and B. T. Kim | Extended Optical Model Analyses of Elastic Scattering and Fusion Cross
Section Data for the $^{12}$C+$^{208}$Pb System at Near-Coulomb-Barrier
Energies by using a Folding Potential | 26 pages, 7 figures, submitted to Physical Review C | Phys.Rev.C77:024609,2008 | 10.1103/PhysRevC.77.024609 | null | nucl-th | null | Simultaneous $\chi^{2}$ analyses are performed for elastic scattering and
fusion cross section data for the $^{12}$C+$^{208}$Pb system at
near-Coulomb-barrier energies by using the extended optical model approach in
which the polarization potential is decomposed into direct reaction (DR) and
fusion parts. Use is made of the double folding potential as a bare potential.
It is found that the experimental elastic scattering and fusion data are well
reproduced without introducing any normalization factor for the double folding
potential and also that both DR and fusion parts of the polarization potential
determined from the $\chi^{2}$ analyses satisfy separately the dispersion
relation. Furthermore, it is shown that the imaginary parts of both DR and
fusion potentials at the strong absorption radius change very rapidly, which
results in a typical threshold anomaly in the total imaginary potential as
observed with tightly bound projectiles such as $\alpha$-particle and $^{16}$O.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 03:05:44 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"So",
"W. Y.",
""
],
[
"Udagawa",
"T.",
""
],
[
"Hong",
"S. W.",
""
],
[
"Kim",
"B. T.",
""
]
] | [
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] |
801.2201 | Ed Harcourt | Ed Harcourt | Policies of System Level Pipeline Modeling | null | null | null | null | cs.AR cs.PL | null | Pipelining is a well understood and often used implementation technique for
increasing the performance of a hardware system. We develop several SystemC/C++
modeling techniques that allow us to quickly model, simulate, and evaluate
pipelines. We employ a small domain specific language (DSL) based on resource
usage patterns that automates the drudgery of boilerplate code needed to
configure connectivity in simulation models. The DSL is embedded directly in
the host modeling language SystemC/C++. Additionally we develop several
techniques for parameterizing a pipeline's behavior based on policies of
function, communication, and timing (performance modeling).
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 15:44:28 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Harcourt",
"Ed",
""
]
] | [
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] |
801.2202 | Nour-Eddine Raouafi | N.-E. Raouafi, S.K. Solanki and T. Wiegelmann | Hanle Effect Diagnostics of the Coronal Magnetic Field - A Test Using
Realistic Magnetic Field Configurations | 6 pages, 5 figures, Solar Polarization Workshop 5 | null | null | null | astro-ph | null | Our understanding of coronal phenomena, such as coronal plasma
thermodynamics, faces a major handicap caused by missing coronal magnetic field
measurements. Several lines in the UV wavelength range present suitable
sensitivity to determine the coronal magnetic field via the Hanle effect. The
latter is a largely unexplored diagnostic of coronal magnetic fields with a
very high potential. Here we study the magnitude of the Hanle-effect signal to
be expected outside the solar limb due to the Hanle effect in polarized
radiation from the H {\sc{i}} Ly$\alpha$ and $\beta$ lines, which are among the
brightest lines in the off-limb coronal FUV spectrum. For this purpose we use a
magnetic field structure obtained by extrapolating the magnetic field starting
from photospheric magnetograms. The diagnostic potential of these lines for
determining the coronal magnetic field, as well as their limitations are
studied. We show that these lines, in particular H {\sc{i}} Ly$\beta$, are
useful for such measurements.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 03:16:22 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Raouafi",
"N. -E.",
""
],
[
"Solanki",
"S. K.",
""
],
[
"Wiegelmann",
"T.",
""
]
] | [
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] |
801.2203 | Akinobu Yamaguchi | A. Yamaguchi, K. Motoi, H. Miyajima, Y. Miyashita and Y. Sanada | Broadband ferromagnetic resonance of Ni81Fe19 wires using a rectifying
effect | 33pages, 8 figures. submitted | null | 10.1103/PhysRevB.78.104401 | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | The broadband ferromagnetic resonance measurement using the rectifying effect
of Ni81Fe19 wire has been investigated. One wire is deposited on the center
strip line of the coplanar waveguide (CPW) and the other one deposited between
two strip lines of CPW. The method is based on the detection of the
magnetoresistance oscillation due to the magnetization dynamics induced by the
radio frequency field. The magnetic field dependences of the resonance
frequency and the rectification spectrum are presented and analytically
interpreted on the standpoint of a uniform magnetization precession model.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 03:43:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Yamaguchi",
"A.",
""
],
[
"Motoi",
"K.",
""
],
[
"Miyajima",
"H.",
""
],
[
"Miyashita",
"Y.",
""
],
[
"Sanada",
"Y.",
""
]
] | [
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] |
801.2204 | Ken-iti Izawa | K. Hamaguchi, K.-I. Izawa, H. Nakajima | Supersymmetric Inflation of Dynamical Origin | 11 pages | Phys.Lett.B662:208-212,2008 | 10.1016/j.physletb.2008.03.001 | UT-07-42 | hep-ph | null | Dynamical models of inflation are given with composite inflatons by means of
massive supersymmetric gauge theory. Nearly flat directions and stable massive
ones in the potential are identified and slow-roll during inflation is
examined. This kind of dynamical inflations may be ubiquitous in fundamental
unified theory with supersymmetry, which should contain gauge theories for
interactions of elementary particles.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 03:58:15 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hamaguchi",
"K.",
""
],
[
"Izawa",
"K. -I.",
""
],
[
"Nakajima",
"H.",
""
]
] | [
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] |
801.2205 | Junbo Li | Junbo Li, Yucai Su | Classification of Irreducible Weight Modules with a Finite-dimensional
Weight Space over the Twisted Schr\"{o}dinger-Virasoro Lie algebra | 6 pages | null | null | null | math.RA math.RT | null | It is shown that the support of an irreducible weight module over the
Schr\"{o}dinger-Virasoro Lie algebra with an infinite-dimensional weight space,
coincides with the weight lattice and that all nontrivial weight spaces of such
a module are infinite-dimensional. As a side-product, it is obtained that every
simple weight module over the Schr\"{o}dinger-Virasoro Lie algebra with a
nontrivial finite-dimensional weight space, is a Harish-Chandra module.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:00:14 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Li",
"Junbo",
""
],
[
"Su",
"Yucai",
""
]
] | [
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] |
801.2206 | Lev I. Shekhtman | V. M. Aulchenko, O. V. Evdokov, L. I. Shekhtman, K. A. Ten, B. P.
Tolochko, I. L. Zhogin, V. V. Zhulanov | Detector for imaging of explosions: present status and future prospects
with higher energy X-rays | 14 pages, 15 figures. Submitted to JINST | JINST3:P05005,2008 | 10.1088/1748-0221/3/05/P05005 | null | physics.ins-det | null | The detector for imaging of explosions (DIMEX) is in operation at the
synchrotron radiation (SR) beam-line at VEPP-3 electron ring at Budker INP
since 2002. DIMEX is based on one-coordinate gas ionization chamber filled with
Xe-CO2(3:1) mixture at 7atm, and active Frisch-grid made of Gas Electron
Multiplier (GEM). The detector has spatial resolution of ~0.2mm and dynamic
range of ~100 that allows to realize the precision of signal measurement at a
percent level. The frame rate can be tuned up to 8 MHz (125 ns per image) and
up to 32 images can be stored in one shot. At present DIMEX is used with the
X-ray beam from 2T wiggler that has ~20 keV average energy. Future possibility
to install similar detector at the SR beam-line at VEPP-4 electron ring is
discussed.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 05:52:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Aulchenko",
"V. M.",
""
],
[
"Evdokov",
"O. V.",
""
],
[
"Shekhtman",
"L. I.",
""
],
[
"Ten",
"K. A.",
""
],
[
"Tolochko",
"B. P.",
""
],
[
"Zhogin",
"I. L.",
""
],
[
"Zhulanov",
"V. V.",
""
]
] | [
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] |
801.2207 | Junbo Li | Junbo Li, Yucai Su | The derivation algebra and automorphism group of the twisted
Schr\"{o}dinger-Virasoro algebra | 16 pages | null | null | null | math.RA | null | In this article, we determine the derivation algebra and the automorphism
group of the twisted Schr\"{o}dinger-Virasoro algebra.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:12:45 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Li",
"Junbo",
""
],
[
"Su",
"Yucai",
""
]
] | [
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] |
801.2208 | Luca Tessieri | J. C. Hern\'andez Herrej\'on, F. M. Izrailev, L. Tessieri | Anomalous properties of the Kronig-Penney model with compositional and
structural disorder | 11 pages, no figure | null | 10.1016/j.physe.2008.05.001 | null | cond-mat.dis-nn | null | We study the localization properties of the eigenstates in the Kronig-Penney
model with weak compositional and structural disorder. The main result is an
expression for the localization length that is valid for any kind of self- and
inter-correlations of the two types of disorder. We show that the interplay
between compositional and structural disorder can result in anomalous
localization.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:13:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Herrejón",
"J. C. Hernández",
""
],
[
"Izrailev",
"F. M.",
""
],
[
"Tessieri",
"L.",
""
]
] | [
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] |
801.2209 | Junbo Li | Junbo Li, Yucai Su | Representations of the Schr\"{o}dinger-Virasoro algebras | 15 pages | null | 10.1063/1.2924216 | null | math.RA | null | In this paper it is proved that an irreducible weight module with
finite-dimensional weight spaces over the Schr\"{o}dinger-Virasoro algebras is
a highest/lowest weight module or a uniformly bounded module. Furthermore,
indecomposable modules of the intermediate series over these algebras are
completely determined.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:18:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Li",
"Junbo",
""
],
[
"Su",
"Yucai",
""
]
] | [
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] |
801.221 | Junbo Li | Junbo Li, Yucai Su | 2-Cocycles of Deformative Schr\"{o}dinger-Virasoro Algebras | 18 pages | null | null | null | math.RA | null | In a series of papers by Henkel, Roger and Unterberger,
Schr\"{o}dinger-Virasoro algebras and their deformations were introduced and
investigated. In the present paper we determine the 2-cocycles of a class of
deformative Schr\"{o}dinger-Virasoro algebras.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:24:02 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Li",
"Junbo",
""
],
[
"Su",
"Yucai",
""
]
] | [
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] |
801.2211 | Junbo Li | Junbo Li, Linsheng Zhu | Leibniz Central Extension on the Twisted Schr\"{o}dinger-Virasoro
Algebra | 9 pages | null | null | null | math.RA | null | In this paper we present all the Leibniz 2-cocycles of the twisted
Schr\"{o}dinger-Virasoro algebra, which determine its second Leibniz cohomology
group.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:32:06 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Li",
"Junbo",
""
],
[
"Zhu",
"Linsheng",
""
]
] | [
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] |
801.2212 | Jia Wei | J. Wei, Y. Zhang, H. W. Ou, B. P. Xie, D. W. Shen, J. F. Zhao, L. X.
Yang, M. Arita, K. Shimada, H. Namatame, M. Taniguchi, Y. Yoshida, H. Eisaki,
and D. L. Feng | Superconducting coherence peak in the electronic excitations of a single
layer cuprate superconductor $Bi_2 Sr_{1.6} La_{0.4} Cu O_{6+\delta}$ | 5 pages, 4 figures | null | 10.1103/PhysRevLett.101.097005 | null | cond-mat.supr-con cond-mat.str-el | null | Angle resolved photoemission spectroscopy study is reported on a high quality
optimally doped Bi2Sr1.6La0.4CuO6+delta high Tc superconductor. In the
antinodal region with maximal d-wave gap, the symbolic superconducting
coherence peak, which has been widely observed in multi-CuO2-layer cuprate
superconductors, is unambiguously observed in a single layer system. The
associated peak-dip separation is just about 19 meV, which is much smaller than
its counterparts in multi-layered compounds, but correlates with the energy
scales of spin excitations in single layer cuprates.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:10:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wei",
"J.",
""
],
[
"Zhang",
"Y.",
""
],
[
"Ou",
"H. W.",
""
],
[
"Xie",
"B. P.",
""
],
[
"Shen",
"D. W.",
""
],
[
"Zhao",
"J. F.",
""
],
[
"Yang",
"L. X.",
""
],
[
"Arita",
"M.",
""
],
[
"Shimada",
"K.",
""
],
[
"Namatame",
"H.",
""
],
[
"Taniguchi",
"M.",
""
],
[
"Yoshida",
"Y.",
""
],
[
"Eisaki",
"H.",
""
],
[
"Feng",
"D. L.",
""
]
] | [
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] |
801.2213 | Matveev Alexei S. | V.E. Didenko, A.S. Matveev and M.A. Vasiliev | Unfolded Description of $AdS_4$ Kerr Black Hole | 18 pages | Phys.Lett.B665:284-293,2008 | 10.1016/j.physletb.2008.05.067 | null | gr-qc hep-th | null | It is shown that $AdS_4$ Kerr black hole is a solution of simple unfolded
differential equations that form a deformation of the zero-curvature
description of empty $AdS_4$ space-time. Our construction uses the Killing
symmetries of the Kerr solution. All known and some new algebraic properties of
the Kerr-Schild solution result from the obtained black hole unfolded system in
the coordinate-independent way. Kerr Schild type solutions of free equations in
$AdS_4$ for massless fields of any spin, associated to the proposed black hole
unfolded system, are found.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 05:01:34 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 00:20:39 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Didenko",
"V. E.",
""
],
[
"Matveev",
"A. S.",
""
],
[
"Vasiliev",
"M. A.",
""
]
] | [
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] |
801.2214 | Debashish Chowdhury | Debashish Chowdhury, Aakash Basu, Ashok Garai, Philip Greulich,
Katsuhiro Nishinari, Andreas Schadschneider and Tripti Tripathi | Intra-cellular traffic: bio-molecular motors on filamentary tracks | 9 pages, 11 figures; Based on the invited talk delivered by the first
author (DC) at the IUPAP International Conference STATPHYS23, Genoa (Italy),
July, 2007 | European Physical Journal B, vol. 64, p. 593 (2008). | 10.1140/epjb/e2008-00073-5 | null | physics.bio-ph cond-mat.stat-mech q-bio.SC | null | Molecular motors are macromolecular complexes which use some form of input
energy to perform mechanical work. The filamentary tracks, on which these
motors move, are made of either proteins (e.g., microtubules) or nucleic acids
(DNA or RNA). Often, many such motors move simultaneously on the same track and
their collective properties have superficial similarities with vehicular
traffic on highways. The models we have developed provide ``unified''
description: in the low-density limit, a model captures the transport
properties of a single motor while, at higher densities the same model accounts
for the collective spatio-temporal organization of interacting motors. By
drawing analogy with vehicular traffic, we have introduced novel quantities for
characterizing the nature of the spatio-temporal organization of molecular
motors on their tracks. We show how the traffic-like intracellular collective
phenomena depend on the mechano-chemistry of the corresponding individual
motors.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 04:57:26 GMT"
}
] | 2008-08-17T00:00:00 | [
[
"Chowdhury",
"Debashish",
""
],
[
"Basu",
"Aakash",
""
],
[
"Garai",
"Ashok",
""
],
[
"Greulich",
"Philip",
""
],
[
"Nishinari",
"Katsuhiro",
""
],
[
"Schadschneider",
"Andreas",
""
],
[
"Tripathi",
"Tripti",
""
]
] | [
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801.2215 | Ulrich Mohrhoff | U. Mohrhoff | The Utility of Time-Symmetric Quantum Counterfactuals: A Response to
Kastner | 17 pages | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Kastner's (Philosophy of Science 70, 2003, pp. 145--163) recent objections to
the counterfactual usage of the time-symmetric Aharonov-Bergmann-Lebowitz rule
by the author, especially her claims that the resulting time-symmetric quantum
counterfactuals are vacuous or invalid, are examined and shown to be unfounded
or beside the point.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 05:10:00 GMT"
},
{
"version": "v2",
"created": "Mon, 15 Dec 2008 01:11:24 GMT"
}
] | 2008-12-15T00:00:00 | [
[
"Mohrhoff",
"U.",
""
]
] | [
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801.2216 | Fuquan Fang | Fuquan Fang, S. Mendonca | Knots in Riemannian manifolds | 9 pages | null | null | null | math.DG math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we study submanifold with nonpositive extrinsic curvature in a
positively curved manifold. Among other things we prove that, if $K\subset
(S^n, g)$ is a totally geodesic submanifold in a Riemannian sphere with
positive sectional curvature where $n\ge 5$, then $K$ is homeomorphic to
$S^{n-2}$ and the fundamental group of the knot complement $\pi_1(S^n-K)\cong
\Bbb Z$.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 05:45:47 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Aug 2008 06:52:10 GMT"
}
] | 2008-08-25T00:00:00 | [
[
"Fang",
"Fuquan",
""
],
[
"Mendonca",
"S.",
""
]
] | [
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] |
801.2217 | Paul Michalski | P. J. Michalski and E. J. Mele | Carbon Nanotubes in Helically Modulated Potentials | 12 pages, 10 figures. Accepted for publication in Physical Review B.
Image quality reduced to comply with arxiv size limitations | null | 10.1103/PhysRevB.77.085429 | null | cond-mat.mes-hall | null | We calculate effects of an applied helically symmetric potential on the low
energy electronic spectrum of a carbon nanotube in the continuum approximation.
The spectrum depends on the strength of this potential and on a dimensionless
geometrical parameter, P, which is the ratio of the circumference of the
nanotube to the pitch of the helix. We find that the minimum band gap of a
semiconducting nanotube is reduced by an arbitrarily weak helical potential,
and for a given field strength there is an optimal P which produces the biggest
change in the band gap. For metallic nanotubes the Fermi velocity is reduced by
this potential and for strong fields two small gaps appear at the Fermi surface
in addition to the gapless Dirac point. A simple model is developed to estimate
the magnitude of the field strength and its effect on DNA-CNT complexes in an
aqueous solution. We find that under typical experimental conditions the
predicted effects of a helical potential are likely to be small and we discuss
several methods for increasing the size of these effects.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 05:47:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Michalski",
"P. J.",
""
],
[
"Mele",
"E. J.",
""
]
] | [
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] |
801.2218 | Renato Renner | Roger Colbeck and Renato Renner | Hidden variable models for quantum theory cannot have any local part | latex, 5 pages | Phys.Rev.Lett.101:050403,2008 | 10.1103/PhysRevLett.101.050403 | null | quant-ph | null | It was shown by Bell that no local hidden variable model is compatible with
quantum mechanics. If, instead, one permits the hidden variables to be entirely
non-local, then any quantum mechanical predictions can be recovered. In this
paper, we consider general hidden variable models which can have both local and
non-local parts. We then show the existence of (experimentally verifiable)
quantum correlations that are incompatible with any hidden variable model
having a non-trivial local part, such as the model proposed by Leggett.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 16:56:27 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 12:06:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Colbeck",
"Roger",
""
],
[
"Renner",
"Renato",
""
]
] | [
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] |
801.2219 | Atsushi Goto | Atsushi Goto, Kenjiro Hashi, Tadashi Shimizu, Shinobu Ohki | Dynamics of the electron-nuclear and heteronuclear polarization
transfers in optically-oriented semi-insulating InP:Fe | 7 pages, 4 figures, submitted to Physical Review B | Physical Review B 77, 115203 (2008). | 10.1103/PhysRevB.77.115203 | null | cond-mat.mtrl-sci | null | Dynamics of the electron-nuclear and heteronuclear polarization-transfer
processes in the optically oriented semi-insulating iron-doped indium phosphide
were investigated through the characteristic time scales of the processes. (1)
We find in the optical nuclear orientation process that the buildup times for
31P and 115In nuclear polarizations are of the same order. From the analysis of
the cross-relaxation process between photo-excited electrons and nuclei, it is
concluded that electron-nuclear dipolar-couplings are responsible for the
polarization transfer in this case. This example shows that the nuclear-site
dependence of the buildup time can be utilized to identify hyperfine couplings
responsible for the process. (2) We find in the heteronuclear polarization
transfer (cross polarization) process between optically oriented 31P and 115In
that the cross-relaxation time is rather short; it is an order of magnitude
shorter than that expected for nuclear dipolar couplings when a magnetic field
is applied parallel to the crystalline [100] axis. From the cross polarization
spectral density analysis, it is concluded that a large J-coupling of the order
of 2 kHz exists between these nuclei and that its angular dependence is not of
a simple pseudo-dipolar type.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 06:22:27 GMT"
}
] | 2008-03-11T00:00:00 | [
[
"Goto",
"Atsushi",
""
],
[
"Hashi",
"Kenjiro",
""
],
[
"Shimizu",
"Tadashi",
""
],
[
"Ohki",
"Shinobu",
""
]
] | [
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] |
801.222 | Christian Kurtsiefer | Alexander Ling, Antia Lamas-Linares, Christian Kurtsiefer | Absolute emission rates of Spontaneous Parametric Down Conversion into
single transverse Gaussian modes | RevTeX, 7 pages, 4 figures; this version has a short section
discussing ratios between pump and target waists | Phys. Rev. A 77, 043834 (2008) | 10.1103/PhysRevA.77.043834 | null | quant-ph | null | We provide an estimate on the absolute values of the emission rate of photon
pairs produced by spontaneous parametric down conversion in a bulk crystal when
all interacting fields are in single transverse Gaussian modes. Both collinear
and non-collinear configurations are covered, and we arrive at a fully
analytical expression for the collinear case. Our results agree reasonably well
with values found in typical experiments, which allows this model to be used
for understanding the dependency on the relevant experimental parameters.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 06:29:51 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Apr 2008 01:40:48 GMT"
}
] | 2008-04-29T00:00:00 | [
[
"Ling",
"Alexander",
""
],
[
"Lamas-Linares",
"Antia",
""
],
[
"Kurtsiefer",
"Christian",
""
]
] | [
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] |
801.2221 | Harish Seshadri | Siddartha Gadgil, Harish Seshadri | On the topology of manifolds with positive isotropic curvature | 5 Pages. To appear in Proc. of AMS | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that a closed orientable Riemannian $n$-manifold, $n \ge 5$, with
positive isotropic curvature and free fundamental group is homeomorphic to the
connected sum of copies of $S^{n-1} \times S^1$.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 06:40:58 GMT"
},
{
"version": "v2",
"created": "Tue, 10 Jun 2008 08:23:07 GMT"
},
{
"version": "v3",
"created": "Wed, 15 Oct 2008 06:11:07 GMT"
}
] | 2008-10-15T00:00:00 | [
[
"Gadgil",
"Siddartha",
""
],
[
"Seshadri",
"Harish",
""
]
] | [
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] |
801.2222 | Van An Dinh | Van An Dinh, Kazunori Sato and Hirosi Katayama-Yoshida | Structural and magnetic properties of half-heusler alloys NiCrZ (Z = Si,
P, Ge, As, Te): First principle study | 10 pages, 3 figures | null | 10.1016/j.commatsci.2011.08.037 | null | cond-mat.mtrl-sci cond-mat.str-el | null | We present a first principle study of new class of high-$T_c$ half-heusler
ferromagnets NiCrZ (Z = Si, P, Ge, As, Te). The structure and magnetic
properties are investigated through the calculation of the electronic
structure, equilibrium lattice constant, magnetic exchange interaction $J_{ij}$
and Curie temperature $T_c$. The role of $sp$-elements and the influence of
lattice expansion/compression are also studied. In alloys having 20 valence
electrons, a pseudo-gap of the majority band can be formed at Fermi level.
Otherwise, the half-metallicity and ferromagnetism at temperatures much higher
than room temperature are found to be stable in a wide range of lattice
expansion. Based on these results, NiCrZ can be expected to be promising
materials for spintronics.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 06:52:28 GMT"
}
] | 2011-10-26T00:00:00 | [
[
"Dinh",
"Van An",
""
],
[
"Sato",
"Kazunori",
""
],
[
"Katayama-Yoshida",
"Hirosi",
""
]
] | [
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] |
801.2223 | Shuang Zhang | Shuang Zhang, Dentcho A. Genov, Cheng Sun and Xiang Zhang | Cloaking of Matter Waves | 14 pages, 3 figs | null | 10.1103/PhysRevLett.100.123002 | null | physics.optics physics.gen-ph | null | Invariant transformation for quantum mechanical systems is proposed. A
cloaking of matter wave can be realized at given energy by designing the
potential and effective mass of the matter waves in the cloaking region. The
general conditions required for such a cloaking are determined and confirmed by
both the wave and particle (classical) approaches. We show that it may be
possible to construct such a cloaking system for cold atoms using optical
lattices.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 07:13:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zhang",
"Shuang",
""
],
[
"Genov",
"Dentcho A.",
""
],
[
"Sun",
"Cheng",
""
],
[
"Zhang",
"Xiang",
""
]
] | [
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] |
801.2224 | Dan J. Spitzner | Dan J. Spitzner | A powerful test based on tapering for use in functional data analysis | Published in at http://dx.doi.org/10.1214/08-EJS172 the Electronic
Journal of Statistics (http://www.i-journals.org/ejs/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Electronic Journal of Statistics 2008, Vol. 2, 939-962 | 10.1214/08-EJS172 | IMS-EJS-EJS_2008_172 | math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A test based on tapering is proposed for use in testing a global linear
hypothesis under a functional linear model. The test statistic is constructed
as a weighted sum of squared linear combinations of Fourier coefficients, a
tapered quadratic form, in which higher Fourier frequencies are down-weighted
so as to emphasize the smooth attributes of the model. A formula is
$Q_n^{OPT}=n\sum_{j=1}^{p_n}j^{-1/2}\|\boldsymbol{Y}_{n,j}\|^2$. Down-weighting
by $j^{-1/2}$ is selected to achieve adaptive optimality among tests based on
tapering with respect to its ``rates of testing,'' an asymptotic framework for
measuring a test's retention of power in high dimensions under smoothness
constraints. Existing tests based on truncation or thresholding are known to
have superior asymptotic power in comparison with any test based on tapering;
however, it is shown here that high-order effects can be substantial, and that
a test based on $Q_n^{OPT}$ exhibits better (non-asymptotic) power against the
sort of alternatives that would typically be of concern in functional data
analysis applications. The proposed test is developed for use in practice, and
demonstrated in an example application.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 07:36:08 GMT"
},
{
"version": "v2",
"created": "Thu, 9 Oct 2008 12:49:59 GMT"
}
] | 2008-10-09T00:00:00 | [
[
"Spitzner",
"Dan J.",
""
]
] | [
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801.2225 | Van An Dinh | Van An Dinh, Kazunori Sato and Hiroshi Katayama-Yoshida | New High-$T_c$ Half-Heusler Ferromagnets NiMnZ (Z = Si, P, Ge, As) | 6 pages, 6 figures | J. Phys. Soc. Jpn. 77 (2008) 014705 | 10.1143/JPSJ.77.014705 | null | cond-mat.mtrl-sci cond-mat.str-el | null | Based on the first principle calculation, we propose a new class of
high-$T_c$ half-heusler ferromagnets NiMnZ (Z = Si, P, Ge, As). The structural
and magnetic properties are investigated through the calculation of the
electronic structure, phase stability, equilibrium lattice constant, magnetic
exchange interaction $J_{ij}$ and Curie temperature $T_c$. It is found that all
alloys show half-metallicity and ferromagnetism at temperatures much higher
than room temperature in a wide range of lattice expansion (compression). At
the equilibrium lattice constant, $T_c$ of 715K, 840K, 875K and 1050K are
predicted by Monte Carlo simulation for NiMnP, NiMnAs, NiMnGe and NiMnSi,
respectively. Following these results, these alloys are strongly expected to be
promising candidates for spintronic applications.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 07:40:03 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Dinh",
"Van An",
""
],
[
"Sato",
"Kazunori",
""
],
[
"Katayama-Yoshida",
"Hiroshi",
""
]
] | [
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] |
801.2226 | Kees Middelburg | J. A. Bergstra, C. A. Middelburg | Programming an interpreter using molecular dynamics | 27 pages | Scientific Annals of Computer Science, 17:47--81, 2007.
http://www.infoiasi.ro/bin/download/Annals/XVII/XVII_2.pdf | null | PRG0801 | cs.PL | null | PGA (ProGram Algebra) is an algebra of programs which concerns programs in
their simplest form: sequences of instructions. Molecular dynamics is a simple
model of computation developed in the setting of PGA, which bears on the use of
dynamic data structures in programming. We consider the programming of an
interpreter for a program notation that is close to existing assembly languages
using PGA with the primitives of molecular dynamics as basic instructions. It
happens that, although primarily meant for explaining programming language
features relating to the use of dynamic data structures, the collection of
primitives of molecular dynamics in itself is suited to our programming wants.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 07:56:12 GMT"
}
] | 2008-04-08T00:00:00 | [
[
"Bergstra",
"J. A.",
""
],
[
"Middelburg",
"C. A.",
""
]
] | [
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] |
801.2227 | Remi Carles | Valeria Banica (DP), R\'emi Carles (I3M), Thomas Duyckaerts (AGM) | On scattering for NLS: from Euclidean to hyperbolic space | 13 pages. References updated; see Remark 1.1 | Discrete and Continuous Dynamical Systems: Series A 24, 4 (2009)
1113-1127 | 10.3934/dcds.2009.24.1113 | null | math.AP math-ph math.MP | null | We prove asymptotic completeness in the energy space for the nonlinear
Schrodinger equation posed on hyperbolic space in the radial case, in space
dimension at least 4, and for any energy-subcritical, defocusing, power
nonlinearity. The proof is based on simple Morawetz estimates and weighted
Strichartz estimates. We investigate the same question on spaces which kind of
interpolate between Euclidean space and hyperbolic space, showing that the
family of short range nonlinearities becomes larger and larger as the space
approaches the hyperbolic space. Finally, we describe the large time behavior
of radial solutions to the free dynamics.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 08:03:05 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 15:17:18 GMT"
}
] | 2009-06-18T00:00:00 | [
[
"Banica",
"Valeria",
"",
"DP"
],
[
"Carles",
"Rémi",
"",
"I3M"
],
[
"Duyckaerts",
"Thomas",
"",
"AGM"
]
] | [
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] |
801.2228 | Hans Brom | L. J. Huijbregts, H. B. Brom, J. C. M. Brokken-Zijp, W.E. Kleinjan,
and M. A. J. Michels | Dielectric quantification of conductivity limitations due to nanofiller
size in conductive powders and nanocomposites | 6 pages, 4 figures | null | 10.1103/PhysRevB.77.075322 | null | cond-mat.mtrl-sci cond-mat.dis-nn | null | Conducting submicron particles are well-suited as filler particles in
non-conducting polymer matrices to obtain a conducting composite with a low
percolation threshold. Going to nanometer-sized filler particles imposes a
restriction to the conductivity of the composite, due to the reduction of the
density of states involved in the hopping process between the particles,
compared to its value within the crystallites. We show how those microscopic
parameters that govern the charge-transport processes across many decades of
length scales, can accurately and consistently be determined by a range of
dielectric-spectroscopy techniques from a few Hz to infrared frequencies. The
method, which is suited for a variety of systems with restricted geometries, is
applied to densely packed 7-nm-sized tin-oxide crystalline particles with
various degree of antimony doping and the quantitative results unambiguously
show the role of the nanocrystal charging energy in limiting the hopping
process.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 08:27:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Huijbregts",
"L. J.",
""
],
[
"Brom",
"H. B.",
""
],
[
"Brokken-Zijp",
"J. C. M.",
""
],
[
"Kleinjan",
"W. E.",
""
],
[
"Michels",
"M. A. J.",
""
]
] | [
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] |
801.2229 | Rikkert Frederix | Rikkert Frederix and Massimiliano Grazzini | Higher-order QCD effects in the Higgs to ZZ search channel at the LHC | 12 pages, 8 figures. Discussion on scale uncertainties added | Phys.Lett.B662:353-359,2008 | 10.1016/j.physletb.2008.03.030 | CP3-08-01 | hep-ph | null | We present a consistent analysis of the signal as well as the irreducible
background for the search of the SM Higgs boson in the ZZ decay channel at the
LHC. Soft-gluons effects are resummed up to next-to-leading logarithmic
accuracy, and the results are compared to those obtained with fixed order
calculations and the MC@NLO event generator. The soft-gluon effects are
typically modest but should be taken into account when precise predictions are
demanded. Our results show that the signal over background ratio can be
significantly enhanced with a cut on the transverse momentum pt(ZZ) of the ZZ
pair. We also introduce a fully transverse angular variable that could give
information about the CP nature of the Higgs boson.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:00:17 GMT"
},
{
"version": "v2",
"created": "Tue, 27 May 2008 08:09:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Frederix",
"Rikkert",
""
],
[
"Grazzini",
"Massimiliano",
""
]
] | [
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801.223 | Ingrid Beltita | Ingrid Beltita, Anders Melin | Analysis of the quadratic term in the backscattering transformation | 14 pages | null | null | null | math.AP math-ph math.MP | null | The quadratic term in the Taylor expansion at the origin of the
backscattering transformation in odd dimensions $n\ge 3$ gives rise to a
symmetric bilinear operator $B_2$ on $C_0^\infty({\mathbb R}^n)\times
C_0^\infty({\mathbb R}^n)$. In this paper we prove that $B_2$ extends to
certain Sobolev spaces with weights and show that it improves both regularity
and decay.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:05:01 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Beltita",
"Ingrid",
""
],
[
"Melin",
"Anders",
""
]
] | [
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] |
801.2231 | Jian-feng Yao | C\'ecile Hardouin, Jian-Feng Yao | Spatial modelling for mixed-state observations | Published in at http://dx.doi.org/10.1214/08-EJS173 the Electronic
Journal of Statistics (http://www.i-journals.org/ejs/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Electronic Journal of Statistics 2008, Vol. 2, 213-233 | 10.1214/08-EJS173 | IMS-EJS-EJS_2008_173 | math.ST stat.TH | null | In several application fields like daily pluviometry data modelling, or
motion analysis from image sequences, observations contain two components of
different nature. A first part is made with discrete values accounting for some
symbolic information and a second part records a continuous (real-valued)
measurement. We call such type of observations "mixed-state observations". This
paper introduces spatial models suited for the analysis of these kinds of data.
We consider multi-parameter auto-models whose local conditional distributions
belong to a mixed state exponential family. Specific examples with exponential
distributions are detailed, and we present some experimental results for
modelling motion measurements from video sequences.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 15:04:51 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Mar 2008 08:13:32 GMT"
}
] | 2008-03-27T00:00:00 | [
[
"Hardouin",
"Cécile",
""
],
[
"Yao",
"Jian-Feng",
""
]
] | [
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801.2232 | Valery Lyubovitskij | Amand Faessler, Thomas Gutsche, Valery E. Lyubovitskij, Yong-Liang Ma | Molecular structure of the Bs0*(5725) and Bs1(5778) bottom-strange
mesons | 21 pages, 7 figures | Phys.Rev.D77:114013,2008 | 10.1103/PhysRevD.77.114013 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss a possible interpretation of the scalar Bs0*(5725) and axial
Bs1(5778) bottom-strange mesons as hadronic molecules - bound states of B K and
B* K mesons, respectively. Using a phenomenological Lagrangian approach we
analyze the strong Bs0* to Bs pi0, Bs1 to Bs* pi0 and the radiative Bs0* to Bs*
gamma, Bs1 to Bs gamma, Bs1 to Bs* gamma, Bs1 to Bs0* gamma decays. We give
predictions for the decay properties: effective couplings and decay widths.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:08:27 GMT"
},
{
"version": "v2",
"created": "Wed, 11 Jun 2008 14:25:58 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Faessler",
"Amand",
""
],
[
"Gutsche",
"Thomas",
""
],
[
"Lyubovitskij",
"Valery E.",
""
],
[
"Ma",
"Yong-Liang",
""
]
] | [
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] |
801.2233 | Lucile Sassatelli | Lucile Sassatelli and David Declercq | Analysis of Non-binary Hybrid LDPC Codes | in the proceedings of IEEE International Symposium on Information
Theory, June 2007, Nice, France | null | null | null | cs.IT math.IT | null | In this paper, we analyse asymptotically a new class of LDPC codes called
Non-binary Hybrid LDPC codes, which has been recently introduced. We use
density evolution techniques to derive a stability condition for hybrid LDPC
codes, and prove their threshold behavior. We study this stability condition to
conclude on asymptotic advantages of hybrid LDPC codes compared to their
non-hybrid counterparts.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:32:57 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Sassatelli",
"Lucile",
""
],
[
"Declercq",
"David",
""
]
] | [
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] |
801.2234 | M. K. Vemuri | M. K. Vemuri | Hermite expansions and Hardy's theorem | 11 pages | null | null | null | math.AP math-ph math.MP math.RT | null | Assuming that both a function and its Fourier transform are dominated by a
Gaussian of large variance, it is shown that the Hermite coefficients of the
function decay exponentially. A sharp estimate for the rate of exponential
decay is obtained in terms of the variance, and in the limiting case (when the
variance becomes so small that the Gaussian is its own Fourier transform),
Hardy's theorem on Fourier transform pairs is obtained. A quantitative result
on the confinement of particle-like states of a quantum harmonic oscillator is
obtained. A stronger form of the result is conjectured. Further, it is shown
how Hardy's theorem may be derived from a weak version of confinement without
using complex analysis.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 13:42:49 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Vemuri",
"M. K.",
""
]
] | [
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-0.0229455046
] |
801.2235 | Miryam Garcia-Fernandez | M. Garcia-Fernandez, U. Staub, Y. Bodenthin, S. M. Lawrence, A. M.
Mulders, C. E. Buckley, S. Weyeneth, E. Pomjakushina, and K. Conder | A Resonant soft x-ray powder diffraction study to determine the orbital
ordering in A-site ordered SmBaMn2O6 | null | null | 10.1103/PhysRevB.77.060402 | null | cond-mat.str-el | null | Soft X-ray resonant powder diffraction has been performed at the Mn L2,3
edges of A-site ordered SmBaMn2O6. The energy and polarization dependence of
the (1/2 1/2 0) reflection provide direct evidence for a (x2-z2)/(y2-z2) type
orbital ordering in contrast to the single layer manganite. The temperature
dependence of the reflection indicates an orbital reorientation transition at
210 K, below which the charge and orbital ordered MnO2 sheets show AAAA type of
stacking. The concurring reduction of the ferromagnetic super exchange
correlations leads to further charge localization.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:23:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Garcia-Fernandez",
"M.",
""
],
[
"Staub",
"U.",
""
],
[
"Bodenthin",
"Y.",
""
],
[
"Lawrence",
"S. M.",
""
],
[
"Mulders",
"A. M.",
""
],
[
"Buckley",
"C. E.",
""
],
[
"Weyeneth",
"S.",
""
],
[
"Pomjakushina",
"E.",
""
],
[
"Conder",
"K.",
""
]
] | [
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] |
801.2236 | Vladimir Grinin | L.V. Tambovtseva and V.P. Grinin | Dust in the disk winds from young stars as a source of the circumstellar
extinction | 12 pages, 5 figures. accepted by Astronomy Letters | null | 10.1007/s11443-008-4002-1 | null | astro-ph | null | We examine a problem of the dust grains survival in the disk wind in T Tauri
stars (TTSs). For consideration we choose the disk wind model described by
Garcia et al. (2001), where a gas component of the wind is heated by an
ambipolar diffusion up to the temperature of the order of 10$^4$ K. It is shown
that the dust grains heating due to collisions with the gas atoms and electrons
is inefficient in comparison with heating by the stellar radiation, and thus,
dust survives even in the hot wind component. Owing to this, the disk wind may
be opaque for the ultraviolet and optical radiation of the star and is capable
to absorb its noticeable fraction. Calculations show that at the accretion rate
$\dot{M_a} = 10^{-8}-10^{-6} M_\odot$ per year this fraction for TTSs may range
from 20% to 40% of a total luminosity of the star correspondingly. This means
that the disk wind in TTSs can play the same role as the puffed inner rim
considered in the modern models of accretion disks. In Herbig Ae stars (HAEs)
inner regions of the disk winds ($r \le 0.5$ AU) are free of dust since there
dust grains sublimate under the effect of the radiation of the star. Therefore,
in this case a fraction of the absorbed radiation by the disk wind is
significantly less, and may be compared with the effect of the "puffed-up inner
rim" only at $\dot{M_a} \geq 10^{-6} M_\odot$ yr$^{-1}$. Due to the structural
inhomogeneity of the disk wind its optical depth towards an observer may be
variable resulting in the photometric activity of the young stars. For the same
reason, one can observe moving shadows from the gas and dust streams with the
spiral-like structure on the highly resolved circumstellar disk images.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:26:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tambovtseva",
"L. V.",
""
],
[
"Grinin",
"V. P.",
""
]
] | [
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] |
801.2237 | Kirill Melnikov | Walter T. Giele, Zoltan Kunszt, Kirill Melnikov | Full one-loop amplitudes from tree amplitudes | 27 pages, revtex | JHEP 0804:049,2008 | 10.1088/1126-6708/2008/04/049 | null | hep-ph | null | We establish an efficient polynomial-complexity algorithm for one-loop
calculations, based on generalized $D$-dimensional unitarity. It allows
automated computations of both cut-constructible {\it and} rational parts of
one-loop scattering amplitudes from on-shell tree amplitudes. We illustrate the
method by (re)-computing all four-, five- and six-gluon scattering amplitudes
in QCD at one-loop.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:33:20 GMT"
}
] | 2009-09-17T00:00:00 | [
[
"Giele",
"Walter T.",
""
],
[
"Kunszt",
"Zoltan",
""
],
[
"Melnikov",
"Kirill",
""
]
] | [
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] |
801.2238 | Efremov Anatoly | A.V. Efremov, K.Goeke and P.Schweitzer | Sivers and Collins Single Spin Asymmetries | 9 pages, 23 eps figures. Talk at XII Workshop on High Energy Spin
Physics (DSPIN-07), Dubna, Sept. 3-7, 2007 and at ASI - SYMMETRIES AND SPIN
(SPIN-Praha-2007), Prague, July 8 - 14, 2007 | Eur.Phys.J.ST162:1-11,2008 | 10.1140/epjst/e2008-00768-9 | null | hep-ph | null | The Sivers and Collins asymmetries are the most prominent Single Spin
Asymmetries (SSA)in Semi-Inclusive Deeply Inelastic Scattering (SIDIS)with
transverse target polarization. In this talk we present our understanding of
these phenomena.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:40:58 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 12:50:49 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Efremov",
"A. V.",
""
],
[
"Goeke",
"K.",
""
],
[
"Schweitzer",
"P.",
""
]
] | [
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] |
801.2239 | Tomoki Nakanishi | Wakako Nakai, Tomoki Nakanishi | On Frenkel-Mukhin algorithm for q-character of quantum affine algebras | 19 pages, minor corrections (Remark 3.1, Eq (3.11), etc); final
version to appear in Adv. Stud. in Pure Math., the proceedings volume for the
workshop "Exploration of New Structures and Natural Constructions in
Mathematical Physics", Nagoya, 2007 | Adv. Stud. Pure Math. 61 (2011) 327--347 | null | null | math.QA | null | The q-character is a strong tool to study finite-dimensional representations
of quantum affine algebras. However, the explicit formula of the q-character of
a given representation has not been known so far. Frenkel and Mukhin proposed
the iterative algorithm which generates the q-character of a given irreducible
representation starting from its highest weight monomial. The algorithm is
known to work for various classes of representations. In this note, however, we
give an example in which the algorithm fails to generate the q-character.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:43:44 GMT"
},
{
"version": "v2",
"created": "Sun, 11 May 2008 05:56:56 GMT"
}
] | 2012-03-21T00:00:00 | [
[
"Nakai",
"Wakako",
""
],
[
"Nakanishi",
"Tomoki",
""
]
] | [
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801.224 | Rui Guo | Rui Guo, Xiaoji Zhou, Xuzong Chen | High momentum entanglement of cold atoms generated by a single photon
scattering | 4 pages, 5 figures | null | null | null | quant-ph | null | With the mechanism of pairwise scattering of photons between two atoms, we
propose a novel scheme to highly entangle the motional state between two
ultracold neutral atoms by a single photon scattering and detection. Under
certain conditions, it is shown that an arbitrary amount of entanglement can be
obtained with this scheme.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:50:12 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Guo",
"Rui",
""
],
[
"Zhou",
"Xiaoji",
""
],
[
"Chen",
"Xuzong",
""
]
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] |
801.2241 | Cyril Branciard | Cyril Branciard, Nicolas Brunner, Nicolas Gisin, Christian Kurtsiefer,
Antia Lamas-Linares, Alexander Ling, and Valerio Scarani | Testing quantum correlations versus single-particle properties within
Leggett's model and beyond | 9 pages, 5 figures | Nature Physics 4, 681 - 685 (2008) | 10.1038/nphys1020 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Quantum theory predicts and experiments confirm that nature can produce
correlations between distant events that are nonlocal in the sense of violating
a Bell inequality. Nevertheless, Bell's strong sentence {\it Correlations cry
out for explanations} remains relevant. The maturing of quantum information
science and the discovery of the power of nonlocal correlations, e.g. for
cryptographic key distribution beyond the standard Quantum Key Distribution
schemes, strengthen Bell's wish and make it even more timely.
In 2003, Leggett proposed an alternative model for nonlocal correlations
[Found. Phys. 33, 1469 (2003)], that he proved to be incompatible with quantum
predictions. We present here a new approach to this model, along with new
inequalities for testing it. Remarkably these inequalities can be derived in a
very simple way, assuming only the non-negativity of probability distributions;
they are also stronger than previously published Leggett-type inequalities. The
simplest of these inequalities is experimentally violated. Then we go beyond
Leggett's model, and show that one cannot ascribe even partially defined
individual properties to the components of a maximally entangled pair.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 09:53:25 GMT"
},
{
"version": "v2",
"created": "Tue, 14 Apr 2009 10:48:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Branciard",
"Cyril",
""
],
[
"Brunner",
"Nicolas",
""
],
[
"Gisin",
"Nicolas",
""
],
[
"Kurtsiefer",
"Christian",
""
],
[
"Lamas-Linares",
"Antia",
""
],
[
"Ling",
"Alexander",
""
],
[
"Scarani",
"Valerio",
""
]
] | [
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] |
801.2242 | Masahito Hayashi | Masahito Hayashi | Information Spectrum Approach to Second-Order Coding Rate in Channel
Coding | null | IEEE Transactions on Information Theory Volume 55, Issue 11, 4947
- 4966 (2009) | 10.1109/TIT.2009.2030478 | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Second-order coding rate of channel coding is discussed for general sequence
of channels. The optimum second-order transmission rate with a constant error
constraint $\epsilon$ is obtained by using the information spectrum method. We
apply this result to the discrete memoryless case, the discrete memoryless case
with a cost constraint, the additive Markovian case, and the Gaussian channel
case with an energy constraint. We also clarify that the Gallager bound does
not give the optimum evaluation in the second-order coding rate.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:00:46 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Aug 2008 06:34:05 GMT"
}
] | 2016-11-15T00:00:00 | [
[
"Hayashi",
"Masahito",
""
]
] | [
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] |
801.2243 | Eric Jaligot | Eric Jaligot (ICJ) | Cosets, genericity, and the Weyl group | null | null | null | null | math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove a non-generosity theorem for proper cosets in groups of finite
Morley rank and elaborate on the theory of Weyl groups in this context.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:01:00 GMT"
},
{
"version": "v2",
"created": "Mon, 19 May 2008 15:40:50 GMT"
},
{
"version": "v3",
"created": "Fri, 12 Sep 2008 18:53:44 GMT"
}
] | 2008-09-12T00:00:00 | [
[
"Jaligot",
"Eric",
"",
"ICJ"
]
] | [
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] |
801.2244 | Pranav Saxena | N.K. Sharma, Pranav Saxena (Rajasthan University), Prachi Parashar
(Oklahoma University), Ashok K. Nagawat, Sardar Singh (Rajasthan University) | Low energy theorems and the unitarity bounds in the extra U(1)
superstring inspired E6 models | 57 Pages, 13 Tables, 7 Figs.; PACS: 12.10.Dm, 12.60.Cn;
http://link.aps.org/abstract/PRD/v72/e095016 | Phys.Rev.D72:095016,2005 | 10.1103/PhysRevD.72.095016 | null | hep-ph | null | The conventional method using low energy theorems [3] does not seem to lead
to an explicit unitarity limit in the scattering processes of longitudinally
polarized gauge bosons for the high energy case in the extra U(1) superstring
inspired models, commonly known as eta model, emanating from E6 group of
superstring theory. We have made use of an alternative procedure given in [14],
which is applicable to SUSY GUT. Explicit unitarity bounds on the Yukawa
couplings are obtained from both using unitarity constraints as well as using
RGE analysis at one-loop level utilizing critical couplings concepts implying
divergence of scalar coupling at MG. These are found to be consistent with
finiteness over the entire range MZ<=sqrt(s)<=MG. For completeness, the similar
approach has been made use of in other models, i.e., chi, psi, and nu models
emanating from E6 and it has been noticed that at weak scale, the unitarity
bounds on Yukawa couplings do not differ among E6 extra U(1) models
significantly except for the case of chi model in 16 representations.
Theoretically we have obtained the upper bounds on top quark and lightest
neutral higgs boson mass using the unitarity constrained superpotential
couplings and also obtained the D-quark mass as a function of MZ2 is O(3 TeV)
for MZ2 is O(1 TeV). The obtained bounds on these physical parameters are found
consistent with the present day experimental precision measurements.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:01:19 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Sharma",
"N. K.",
"",
"Rajasthan University"
],
[
"Saxena",
"Pranav",
"",
"Rajasthan University"
],
[
"Parashar",
"Prachi",
"",
"Oklahoma University"
],
[
"Nagawat",
"Ashok K.",
"",
"Rajasthan University"
],
[
"Singh",
"Sardar",
"",
"Rajasthan University"
]
] | [
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801.2245 | Oleg Kochukhov | T. Ryabchikova, O. Kochukhov, S. Bagnulo | Isotopic anomaly and stratification of Ca in magnetic Ap stars | 13 pages, 10 figures; accepted for publication in Astronomy &
Astrophysics | null | 10.1051/0004-6361:20077834 | null | astro-ph | null | We have carried out an accurate investigation of the Ca isotopic composition
and stratification in the atmospheres of 23 magnetic chemically peculiar (Ap)
stars of different temperature and magnetic field strength. With the UVES
spectrograph at the 8m ESO VLT, we have obtained high-resolution spectra of Ap
stars in the wavelength range 3000-10000 A. Using a detailed spectrum synthesis
calculations, we have reproduced a variety of Ca lines in the optical and
ultraviolet spectral regions, inferring the overall vertical distribution of Ca
abundance, then we have deduced the relative isotopic composition and its
dependence on height using the profile of the the IR-triplet Ca II line at
lambda 8498 A. In 22 out of 23 studied stars, we found that Ca is strongly
stratified, being usually overabundant by 1.0-1.5 dex below log tau_5000 ~ -1,
and strongly depleted above log tau_5000 = -1.5. The IR-triplet Ca II line at
lambda 8498 A reveals a significant contribution of the heavy isotopes 46Ca and
48Ca, which represent less than 1% of the terrestrial Ca isotopic mixture. We
confirm our previous finding that the presence of heavy Ca isotopes is
generally anticorrelated with the magnetic field strength. Moreover, we
discover that in Ap stars with relatively small surface magnetic fields (<=4-5
kG), the light isotope 40Ca is concentrated close to the photosphere, while the
heavy isotopes are dominant in the outer atmospheric layers. This vertical
isotopic separation, observed for the first time for any metal in a stellar
atmosphere, disappears in stars with magnetic field strength above 6-7 kG. We
suggest that the overall Ca stratification and depth-dependent isotopic anomaly
observed in Ap stars may be attributed to a combined action of the
radiatively-driven diffusion and light-induced drift.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:02:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ryabchikova",
"T.",
""
],
[
"Kochukhov",
"O.",
""
],
[
"Bagnulo",
"S.",
""
]
] | [
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801.2246 | X.R. Wang | X. R. Wang | Light emitting diodes of inverse spin valves | null | null | 10.1155/2008/434936 | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | We propose making light emitting diodes out of inverse spin valves. The
proposed diodes rely on the spin-dependent electron transport of inverse spin
valves that are layered structures of a ferromagnetic half-metal sandwiched
between two non-magnetic metals. Under a bias, a giant spin-dependent chemical
potential difference between spin-up and spin-down electrons is created. Thus,
the inverse spin valves are possible to emit light when electrons in higher
chemical potential go to the lower chemical potential. The advantages of this
type of light emitting diodes include tunableness and less demand on materials.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:03:23 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Wang",
"X. R.",
""
]
] | [
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] |
801.2247 | Gemma Colom\'e-Nin | Gemma Colom\'e-Nin and Juan Elias | Cohomological properties of non-standard multigraded modules | null | null | null | null | math.AC | null | In this paper we study some cohomological properties of non-standard
multigraded modules and Veronese transforms of them. Among others numerical
characters, we study the generalized depth of a module and we see that it is
invariant by taking a Veronese transform. We prove some vanishing theorems for
the local cohomology modules of a multigraded module; as a corollary of these
results we get that the depth of a Veronese module is asymptotically constant.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:03:32 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Colomé-Nin",
"Gemma",
""
],
[
"Elias",
"Juan",
""
]
] | [
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] |
801.2248 | Sebastien Boyaval | S\'ebastien Boyaval (INRIA Rocquencourt, CERMICS), Tony Leli\`evre
(INRIA Rocquencourt, CERMICS), Claude Mangoubi (INRIA Rocquencourt, CERMICS) | Free-energy-dissipative schemes for the Oldroyd-B model | null | null | null | null | math.NA | null | In this article, we analyze the stability of various numerical schemes for
differential models of viscoelastic fluids. More precisely, we consider the
prototypical Oldroyd-B model, for which a free energy dissipation holds, and we
show under which assumptions such a dissipation is also satisfied for the
numerical scheme. Among the numerical schemes we analyze, we consider some
discretizations based on the log-formulation of the Oldroyd-B system proposed
by Fattal and Kupferman, which have been reported to be numerically more stable
than discretizations of the usual formulation in some benchmark problems. Our
analysis gives some tracks to understand these numerical observations.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 12:58:46 GMT"
}
] | 2009-04-20T00:00:00 | [
[
"Boyaval",
"Sébastien",
"",
"INRIA Rocquencourt, CERMICS"
],
[
"Lelièvre",
"Tony",
"",
"INRIA Rocquencourt, CERMICS"
],
[
"Mangoubi",
"Claude",
"",
"INRIA Rocquencourt, CERMICS"
]
] | [
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] |
801.2249 | Van An Dinh | Van An Dinh, Masayuki Toyoda, Kazunori Sato and Hiroshi
Katayama-Yoshida | Exchange Interaction and $T_c$ in Alkaline-earth-metal-oxide-based DMS
without Magnetic Impurities: First Principle Pseudo-SIC and Monte Carlo
Calculation | 5 pages, 5 figures | J. Phys. Soc. Jpn. 75 (2006) 093705 | 10.1143/JPSJ.75.093705 | null | cond-mat.mtrl-sci cond-mat.dis-nn | null | The prospects of half-metallic ferromagnetism being induced by the
incorporation of C atoms into alkaline-earth-metal-oxides are investigated by
the first principle calculation. The origin of the ferromagnetism is discussed
through the calculation of the electronic structure and exchange coupling
constant by using the pseudo-potential-like self-interaction-corrected local
spin density method. The Curie temperature ($T_c$) is also predicted by
employing the Monte Carlo simulation. It is shown that by taking the electron
self-interaction into account, the half-metallic ferromagnetism induced by C in
the host materials is more stabilized in comparison with the standard LDA case,
and the C's $2p$ electron states in the bandgap become more localized resulting
in the predominance of the short-ranged exchange interaction. While the
ferromagnetism in MgO$_{1-x}$C$_x$ is stabilized due to the exchange
interaction of the $1st$-nearest neighbor pairs and might be suppressed by the
anti-ferromagnetic super-exchange interaction at higher $x$, the ferromagnetism
in CaO$_{1-x}$C$_x$, SrO$_{1-x}$C$_x$, and BaO$_{1-x}$C$_x$ is stabilized by
both the $1st$- and $2nd$-nearest neighbor pairs, and $T_c$ monotonously
increases with the C concentration.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:07:55 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Dinh",
"Van An",
""
],
[
"Toyoda",
"Masayuki",
""
],
[
"Sato",
"Kazunori",
""
],
[
"Katayama-Yoshida",
"Hiroshi",
""
]
] | [
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] |
801.225 | Asuka Takatsu | Asuka Takatsu | On Wasserstein geometry of the space of Gaussian measures | 15pages, 1figures | null | null | null | math.DG math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The space of Gaussian measures on a Euclidean space is geodesically convex in
the $L^2$-Wasserstein space. This space is a finite dimensional manifold since
Gaussian measures are parameterized by means and covariance matrices. By
restricting to the space of Gaussian measures inside the $L^2$-Wasserstein
space, we manage to provide detailed descriptions of the $L^2$-Wasserstein
geometry from a Riemannian geometric viewpoint. We first construct a Riemannian
metric which induces the $L^2$-Wasserstein distance. Then we obtain a formula
for the sectional curvatures of the space of Gaussian measures, which is
written out in terms of the eigenvalues of the covariance matrix.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:32:17 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Feb 2008 15:41:39 GMT"
},
{
"version": "v3",
"created": "Wed, 11 Feb 2009 09:50:31 GMT"
}
] | 2009-02-11T00:00:00 | [
[
"Takatsu",
"Asuka",
""
]
] | [
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] |
801.2251 | Evgeny Komarov | E.V.Komarov, Yu.A.Simonov | Theory of Quark-Gluon Plasma and Phase Transition | 6 pages,5 figures; talk given at "13th Lomonosov Conference on
Elementary Particle Physics", Moscow, August 23 -- 29, 2007; new reference
added | null | 10.1142/9789812837592_0054 | null | hep-ph | null | Nonperturbative picture of strong interacting quark-gluon plasma is given
based on the systematic Field Correlator Method. Equation of state, phase
transition in density-temperature plane is derived and compared to lattice data
as well as subsequent thermodynamical quantities of QGP.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:18:50 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 12:32:52 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Komarov",
"E. V.",
""
],
[
"Simonov",
"Yu. A.",
""
]
] | [
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] |
801.2252 | Iosif Galanakis | K. Ozdogan, E. Sasioglu and I. Galanakis | Fundamentals of half-metallic Full-Heusler alloys | Submitted for a book entitled "Spintronics: Materials, Applications
and Devices" to be published by Nova Publishers | null | null | null | cond-mat.mtrl-sci | null | Intermetallic Heusler alloys are amongst the most attractive half-metallic
systems due to the high Curie temperatures and the structural similarity to the
binary semiconductors. In this review we present an overview of the basic
electronic and magnetic properties of the half-metallic full-Heusler alloys
like Co$_2$MnGe. Ab-initio results suggest that the electronic and magnetic
properties in these compounds are intrinsically related to the appearance of
the minority-spin gap. The total spin magnetic moment in the unit cell, $M_t$,
scales linearly with the number of the valence electrons, $Z_t$, such that
$M_t=Z_t-24$ for the full-Heusler alloys opening the way to engineer new
half-metallic alloys with the desired magnetic properties. Moreover we present
analytical results on the disorder in Co$_2$Cr(Mn)Al(Si) alloys, which is
susceptible to destroy the perfect half-metallicity of the bulk compounds and
thus degrade the performance of devices. Finally we discuss the appearance of
the half-metallic ferrimagnetism due to the creation of Cr(Mn) antisites in
these compounds and the Co-doping in Mn$_2$VAl(Si) alloys which leads to the
fully-compensated half-metallic ferrimagnetism.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:03:46 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Ozdogan",
"K.",
""
],
[
"Sasioglu",
"E.",
""
],
[
"Galanakis",
"I.",
""
]
] | [
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801.2253 | Rachid Ahl Laamara | T. Lhallabi and A. Moujib | Integrability and Generalized Monodromy Matrix | 13 pages, No figures | Phys.Rev.D76:064036,2007 | 10.1103/PhysRevD.76.064036 | null | hep-th | null | We construct the Generalized Monodromy matrix $\mathcal{\hat{M}}(\omega)$ of
two dimensional string effective action by introducing the T-duality group
properties.The integrability conditions with general solutions depending on
spectral parameter are given. This construction is investigated for the exactly
solvable Wess, Zumino, Novikov and Witten (WZNW) model in pp-wave Limit when
B=0.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:47:05 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Lhallabi",
"T.",
""
],
[
"Moujib",
"A.",
""
]
] | [
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] |
801.2254 | Masaaki Matsuda | M. Matsuda, M. Fujita, S. Wakimoto, J. A. Fernandez-Baca, J. M.
Tranquada and K. Yamada | Magnetic Excitations of the Diagonal Incommensurate Phase in
Lightly-Doped La2-xSrxCuO4 | 4 pages, 5 figures | null | 10.1103/PhysRevLett.101.197001 | null | cond-mat.str-el cond-mat.mtrl-sci | null | We present inelastic neutron scattering experiments on a single-domain
crystal of lightly-doped La1.96Sr0.04CuO4. We find that the magnetic excitation
spectrum in this insulating phase with a diagonal incommensurate spin
modulation is remarkably similar to that in the superconducting regime, where
the spin modulation is bond parallel. In particular, we find that the
dispersion slope at low energy is essentially independent of doping and
temperature over a significant range. The energy at which the excitations cross
the commensurate antiferromagnetic wave vector increases roughly linearly with
doping through the underdoped regime.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:47:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Matsuda",
"M.",
""
],
[
"Fujita",
"M.",
""
],
[
"Wakimoto",
"S.",
""
],
[
"Fernandez-Baca",
"J. A.",
""
],
[
"Tranquada",
"J. M.",
""
],
[
"Yamada",
"K.",
""
]
] | [
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] |
801.2255 | Armando Gil de Paz | A. Gil de Paz, D. A. Thilker, L. Bianchi, A. Aragon-Salamanca, S.
Boissier, B. F. Madore, C. Diaz-Lopez, I. Trujillo, M. Pohlen, P. Erwin, J.
Zamorano, J. Gallego, J. Iglesias-Paramo, J. M. Vilchez, M. Molla, J. C.
Munoz-Mateos, P. G. Perez-Gonzalez, S. Pedraz, K. Sheth, R. C. Kennicutt Jr,
R. Swaters, and the GALEX Science Team | Extended UV (XUV) Emission in Nearby Galaxy Disks | 4 pages, 2 figures, to appear in the proceedings of "The Formation
and Evolution of Galaxy Disks", Rome 2007, organized by the Vatican
Observatory, editors J. G. Funes, S.J. and E. M. Corsini | null | null | null | astro-ph | null | We summarize the main properties of the extended UV (XUV) emission found in
roughly 30% of the nearby spiral galaxies observed by the GALEX satellite. Two
different classes of XUV disks are identified, the Type 1 XUV disks where
significant, structured UV-bright features are found beyond the "classical"
azimuthally-averaged star-formation threshold, and the Type 2 XUV disks, which
are characterized by very extended (seven times the area where most of the
stellar mass is found), blue [(FUV-K)<5mag] outer disks. These latter disks are
extreme examples of galaxies growing inside-out. The few XUV disks studied in
detail to date are rich in HI but relatively poor in molecular gas, have
stellar populations with luminosity-weighted ages of ~1 Gyr, and ionized-gas
metal abundances of ~Zsun/10. As part of the CAHA-XUV project we are in the
process of obtaining deep multi-wavelength imaging and spectroscopy of 65
XUV-disk galaxies so to determine whether or not these properties are common
among XUV disks.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:03:16 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"de Paz",
"A. Gil",
""
],
[
"Thilker",
"D. A.",
""
],
[
"Bianchi",
"L.",
""
],
[
"Aragon-Salamanca",
"A.",
""
],
[
"Boissier",
"S.",
""
],
[
"Madore",
"B. F.",
""
],
[
"Diaz-Lopez",
"C.",
""
],
[
"Trujillo",
"I.",
""
],
[
"Pohlen",
"M.",
""
],
[
"Erwin",
"P.",
""
],
[
"Zamorano",
"J.",
""
],
[
"Gallego",
"J.",
""
],
[
"Iglesias-Paramo",
"J.",
""
],
[
"Vilchez",
"J. M.",
""
],
[
"Molla",
"M.",
""
],
[
"Munoz-Mateos",
"J. C.",
""
],
[
"Perez-Gonzalez",
"P. G.",
""
],
[
"Pedraz",
"S.",
""
],
[
"Sheth",
"K.",
""
],
[
"Kennicutt",
"R. C.",
"Jr"
],
[
"Swaters",
"R.",
""
],
[
"Team",
"the GALEX Science",
""
]
] | [
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] |
801.2256 | Shmuel Friedland | S. Friedland, E. Krop and K. Markstr\"om | On the Number of Matchings in Regular Graphs | 26 pages, 4 figures | null | null | null | math.CO | null | For the set of graphs with a given degree sequence, consisting of any number
of $2's$ and $1's$, and its subset of bipartite graphs, we characterize the
optimal graphs who maximize and minimize the number of $m$-matchings. We find
the expected value of the number of $m$-matchings of $r$-regular bipartite
graphs on $2n$ vertices with respect to the two standard measures. We state and
discuss the conjectured upper and lower bounds for $m$-matchings in $r$-regular
bipartite graphs on $2n$ vertices, and their asymptotic versions for infinite
$r$-regular bipartite graphs. We prove these conjectures for 2-regular
bipartite graphs and for $m$-matchings with $m\le 4$.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:50:51 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Friedland",
"S.",
""
],
[
"Krop",
"E.",
""
],
[
"Markström",
"K.",
""
]
] | [
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] |
801.2257 | Sami Dib | Sami Dib (1,2,4), Axel Brandenburg (3), Jongsoo Kim (4), Maheswar
Gopinathan (4,5), Philippe Andre (2) ((1) CEA Saclay, (2) Lebanese U., (3)
NORDITA, (4) KASI, (5) ARIES) | Core Mass Function: The Role of Gravity | 13 pages, 4 figures, accepted to ApJ Letters. An additional
simulation has been added. The sign of the beta values in Fig. 1 changed to
fit their definition in the text. The main conclusions, however unchanged,
are better clarified | null | 10.1086/588608 | null | astro-ph | null | We analyze the mass distribution of cores formed in an isothermal,
magnetized, turbulent, and self-gravitating nearly critical molecular cloud
model. Cores are identified at two density threshold levels. Our main results
are that the presence of self-gravity modifies the slopes of the core mass
function (CMF) at the high mass end. At low thresholds, the slope is shallower
than the one predicted by pure turbulent fragmentation. The shallowness of the
slope is due to the effects of core coalescence and gas accretion. Most
importantly, the slope of the CMF at the high mass end steepens when cores are
selected at higher density thresholds, or alternatively, if the CMF is fitted
with a log-normal function, the width of the lognormal distribution decreases
with increasing threshold. This is due to the fact that gravity plays a more
important role in denser structures selected at higher density threshold and
leads to the conclusion that the role of gravity is essential in generating a
CMF that bears more resemblance with the IMF when cores are selected with an
increasing density threshold in the observations.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:51:48 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 07:08:33 GMT"
},
{
"version": "v3",
"created": "Wed, 26 Mar 2008 14:25:36 GMT"
},
{
"version": "v4",
"created": "Wed, 2 Apr 2008 19:15:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dib",
"Sami",
""
],
[
"Brandenburg",
"Axel",
""
],
[
"Kim",
"Jongsoo",
""
],
[
"Gopinathan",
"Maheswar",
""
],
[
"Andre",
"Philippe",
""
]
] | [
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] |
801.2258 | N. W. Evans | E.M. Shin (Cambridge), N.W. Evans (Cambridge) | The Effect of Satellite Galaxies on Gravitational Lensing Flux Ratios | 10 pages, 14 figures, MNRAS, in press | null | 10.1111/j.1365-2966.2008.12971.x | null | astro-ph | null | Gravitational lenses with anomalous flux ratios are often cited as possible
evidence for dark matter satellites predicted by simulations of hierarchical
merging in cold dark matter cosmogonies. We show that the fraction of quads
with anomalous flux ratios depends primarily on the total mass and spatial
extent of the satellites, and the characteristic lengthscale R of their
distribution. If R is 100 kpc, then for a moderately elliptical galaxy with a
line-of-sight velocity dispersion of 250 km/s, a mass of 3 x 10^9 solar masses
in highly-concentrated (Plummer model) satellites is needed for 20% of
quadruplets to show anomalous flux ratios, rising to 1.25 x 10^10 solar masses
for 50%. Several times these masses are required if the satellites have more
extended Hernquist profiles. Compared to a typical elliptical, the flux ratios
of quads formed by typical edge-on disc galaxies with maximum discs are
significantly less susceptible to changes through substructure -- three times
the mass in satellite galaxies is needed to affect 50% of the systems. In many
of the lens systems with anomalous flux ratios, there is evidence for visible
satellites (e.g., B2045+265 or MG0414+0534). We show that optically identified
substructure should not be preponderant among lens systems with anomalies.
There are two possible resolutions of this difficulty. First, in some cases,
visible substructure may be projected within or close to the Einstein radius
and wrongly ascribed as the culprit, whereas dark matter substructure is
causing the flux anomaly. Second, bright satellites, in which baryon cooling
and condensation has taken place, may have higher central densities than dark
satellites, rendering them more efficient at causing flux anomalies.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 10:58:54 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 12:41:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shin",
"E. M.",
"",
"Cambridge"
],
[
"Evans",
"N. W.",
"",
"Cambridge"
]
] | [
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801.2259 | Wilhelm Winter | Mikael Rordam and Wilhelm Winter | The Jiang-Su algebra revisited | 22 pages | null | null | null | math.OA math.KT | null | We give a number of new characterizations of the Jiang-Su algebra Z, both
intrinsic and extrinsic, in terms of C*-algebraic, dynamical, topological and
K-theoretic conditions. Along the way we study divisibility properties of
C*-algebras, we give a precise characterization of those unital C*-algebras of
stable rank one that admit a unital embedding of the dimension-drop C*-algebra
Z_{n,n+1}, and we prove a cancellation theorem for the Cuntz semigroup of
C*-algebras of stable rank one.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:01:40 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Rordam",
"Mikael",
""
],
[
"Winter",
"Wilhelm",
""
]
] | [
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] |
801.226 | Marcello Rosini | Angelo Guida, Lino Reggiani and Marcello Rosini | High-field transport in semiconductor superlattices for interacting
Wannier-Stark levels | null | null | 10.1016/j.spmi.2008.05.003 | null | cond-mat.other | null | We develop a microscopic theory of electron transport in superlattices within
the Wannier-Stark approach by including the interaction associated with Zener
tuneling among the energy levels pertaining to adjacent quantum wells. By using
a Monte Carlo technique we have simulated the hopping motion associated with
absorption and emission of polar optical phonons and determined the main
transport parameters for the case of a GaAs/GaAlAs structure at room
temperature. The interaction among the levels is found to be responsible for a
systematic increase of the level energy with respect to the bottom of the
quantum well at electric fields above about 20 kV/cm. When compared with the
non-interacting case, at the highest fields the average carrier energy
evidences a consistent increase which leads to a significant softening of the
negative differential value of both the drift velocity and diffusivity.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:01:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Guida",
"Angelo",
""
],
[
"Reggiani",
"Lino",
""
],
[
"Rosini",
"Marcello",
""
]
] | [
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] |
801.2261 | Vittoria Colizza | Vittoria Colizza, Alain Barrat, Marc Barthelemy, Alessandro Vespignani | Predictability and epidemic pathways in global outbreaks of infectious
diseases: the SARS case study | 21 pages, 2 tables, 7 figures | BMC Medicine 5, 34 (2007) | 10.1186/1741-7015-5-34 | null | q-bio.OT | null | Background: The global spread of the severe acute respiratory syndrome (SARS)
epidemic has clearly shown the importance of considering the long-range
transportation networks in the understanding of emerging diseases outbreaks.
The introduction of extensive transportation data sets is therefore an
important step in order to develop epidemic models endowed with realism.
Methods: We develop a general stochastic meta-population model that
incorporates actual travel and census data among 3 100 urban areas in 220
countries. The model allows probabilistic predictions on the likelihood of
country outbreaks and their magnitude. The level of predictability offered by
the model can be quantitatively analyzed and related to the appearance of
robust epidemic pathways that represent the most probable routes for the spread
of the disease. Results: In order to assess the predictive power of the model,
the case study of the global spread of SARS is considered. The disease
parameter values and initial conditions used in the model are evaluated from
empirical data for Hong Kong. The outbreak likelihood for specific countries is
evaluated along with the emerging epidemic pathways. Simulation results are in
agreement with the empirical data of the SARS worldwide epidemic. Conclusions:
The presented computational approach shows that the integration of long-range
mobility and demographic data provides epidemic models with a predictive power
that can be consistently tested and theoretically motivated. This computational
strategy can be therefore considered as a general tool in the analysis and
forecast of the global spreading of emerging diseases and in the definition of
containment policies aimed at reducing the effects of potentially catastrophic
outbreaks.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:02:37 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Colizza",
"Vittoria",
""
],
[
"Barrat",
"Alain",
""
],
[
"Barthelemy",
"Marc",
""
],
[
"Vespignani",
"Alessandro",
""
]
] | [
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] |
801.2262 | Robin Zegers | Robin Zegers | Self-gravitating branes of codimension 4 in Lovelock gravity | 22 pages | JHEP 0803:066,2008 | 10.1088/1126-6708/2008/03/066 | DCPT-07/71 | gr-qc hep-th | null | We construct a familly of exact solutions of Lovelock equations describing
codimension four branes with discrete symmetry in the transverse space. Unlike
what is known from pure Einstein gravity, where such brane solutions of higher
codimension are singular, the solutions we find, for the complete Lovelock
theory, only present removable singularities. The latter account for a
localised tension-like energy-momentum tensor on the brane, in analogy with the
case of a codimension two self-gravitating cosmic string in pure Einstein
gravity. However, the solutions we discuss present two main distinctive
features : the tension of the brane receives corrections from the induced
curvature of the brane's worldsheet and, in a given Lovelock theory, the
spectrum of possible values of the tension is discrete. These solutions provide
a new framework for the study of higher codimension braneworlds.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:05:42 GMT"
}
] | 2010-01-15T00:00:00 | [
[
"Zegers",
"Robin",
""
]
] | [
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] |
801.2263 | Maillard Gregory | G. Maillard and S. Sch\"opfer | A functional central limit theorem for regenerative chains | 14 pages | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using the regenerative scheme of Comets, Fern\'andez and Ferrari (2002), we
establish a functional central limit theorem (FCLT) for discrete time
stochastic processes (chains) with summable memory decay. Furthermore, under
stronger assumptions on the memory decay, we identify the limiting variance in
terms of the process only. As applications, we define classes of binary
autoregressive processes and power-law Ising chains for which the FCLT is
fulfilled.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:10:28 GMT"
},
{
"version": "v2",
"created": "Wed, 24 Sep 2008 16:44:32 GMT"
}
] | 2008-09-24T00:00:00 | [
[
"Maillard",
"G.",
""
],
[
"Schöpfer",
"S.",
""
]
] | [
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] |
801.2264 | Bogus{\l}aw Kamys | P. Rosenthal (1), H. Freiesleben (1 and 2), B. Gehrmann (1), I.
Gotzhein (1), K. W. Potthast (1), B. Kamys (3), Z. Rudy (3) ((1) Institut
fuer Experimentalphysik I, Ruhr-Universitaet-Bochum, Germany (2) Present
address: Institut fuer Kern- und Teilchenphysik, Technische Universitaet
Dresden, Germany, (3) Institute of Physics, Jagellonian University, Cracow,
Poland) | Direct Nuclear Reactions in Lithium-Lithium Systems: 7Li+7Li at Elab = 2
- 16 MeV | PDF-LaTeX, 21 pages with 22 figures | Acta Phys.Polon.B41:845-874,2010 | null | null | nucl-ex | null | Angular distributions of 7Li(7Li,t), (7Li,alpha) and (7Li,6He) reactions were
measured for laboratory energies from 2 - 16 MeV. Exact finite range DWBA
analyses were performed with the aim to identify contributions of direct
processes and to investigate the applicability of DWBA to such few nucleon
systems. It turned out that DWBA can be successfully applied to estimate
differential and total cross sections of direct transfer processes in 7Li+7Li
interaction. The direct mechanism was found to play a dominant role in most of
these reactions but significant contributions of other, strongly energy
dependent processes were also established. It is suggested that these processes
might be due to isolated resonances superimposed on the backround of
statistical fluctuations arising from interference of compound nucleus and
direct transfer contributions.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 19:24:54 GMT"
}
] | 2011-09-15T00:00:00 | [
[
"Rosenthal",
"P.",
"",
"1 and 2"
],
[
"Freiesleben",
"H.",
"",
"1 and 2"
],
[
"Gehrmann",
"B.",
""
],
[
"Gotzhein",
"I.",
""
],
[
"Potthast",
"K. W.",
""
],
[
"Kamys",
"B.",
""
],
[
"Rudy",
"Z.",
""
]
] | [
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] |
801.2265 | Jinhui Chen | J.H. Chen, F. Jin, D. Gangadharan, X.Z. Cai, H.Z. Huang, Y.G. Ma | Parton Distributions at Hadronization from Bulk Dense Matter Produced at
RHIC | 5 pages, 3 figures, two more paragraph added to address the referee's
comment, figure updated to include the KET scale. Accepted version to appear
in Phys. Rev. C | Phys.Rev.C78:034907,2008 | 10.1103/PhysRevC.78.034907 | null | nucl-th nucl-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present an analysis of $\Omega$, $\Xi$, $\Lambda$ and $\phi$ spectra from
Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV in terms of distributions of
effective constituent quarks at hadronization. Consistency in quark ratios
derived from various hadron spectra provides clear evidence for hadron
formation dynamics as suggested by quark coalescence or recombination models.
We argue that the constituent quark distribution reflects properties of the
effective partonic degrees of freedom at hadronization. Experimental data
indicate that strange quarks have a transverse momentum distribution flatter
than that of up/down quarks consistent with hydrodynamic expansion in partonic
phase prior to hadronization. After the AMPT model is tuned to reproduce the
strange and up/down quark distributions, the model can describe the measured
spectra of hyperons and $\phi$ mesons very well where hadrons are formed
through dynamical coalescence.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:49:56 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Aug 2008 02:04:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chen",
"J. H.",
""
],
[
"Jin",
"F.",
""
],
[
"Gangadharan",
"D.",
""
],
[
"Cai",
"X. Z.",
""
],
[
"Huang",
"H. Z.",
""
],
[
"Ma",
"Y. G.",
""
]
] | [
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801.2266 | Claudiu Genes | C. Genes, D. Vitali and P. Tombesi | Emergence of atom-light-mirror entanglement inside an optical cavity | null | Phys. Rev. A 77, 050307 (2008) | 10.1103/PhysRevA.77.050307 | null | quant-ph | null | We propose a scheme for the realization of a hybrid, strongly
quantum-correlated system formed of an atomic ensemble surrounded by a
high-finesse optical cavity with a vibrating mirror. We show that the steady
state of the system shows tripartite and bipartite continuous variable
entanglement in experimentally accessible parameter regimes, which is robust
against temperature.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:39:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Genes",
"C.",
""
],
[
"Vitali",
"D.",
""
],
[
"Tombesi",
"P.",
""
]
] | [
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] |
801.2267 | F. de los Santos | E. Romera and F. de los Santos | Identifying wave packet fractional revivals by means of information
entropy | null | Physical Review Letters 99, 263601 (2007) | 10.1103/PhysRevLett.99.263601 | null | quant-ph physics.atom-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Wave packet fractional revivals is a relevant feature in the long time scale
evolution of a wide range of physical systems, including atoms, molecules and
nonlinear systems. We show that the sum of information entropies in both
position and momentum conjugate spaces is an indicator of fractional revivals
by analyzing three different model systems: $(i)$ the infinite square well,
$(ii)$ a particle bouncing vertically against a wall in a gravitational field,
and $(iii)$ the vibrational dynamics of hydrogen iodide molecules. This
description in terms of information entropies complements the usual one in
terms of the autocorrelation function.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:47:35 GMT"
},
{
"version": "v2",
"created": "Fri, 19 Sep 2014 09:53:06 GMT"
}
] | 2014-09-22T00:00:00 | [
[
"Romera",
"E.",
""
],
[
"Santos",
"F. de los",
""
]
] | [
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801.2268 | Evgeny Skvortsov D | E.D. Skvortsov | Mixed-Symmetry Massless Fields in Minkowski space Unfolded | 59 pages; PDOF counting added; typos corrected | JHEP 0807:004,2008 | 10.1088/1126-6708/2008/07/004 | null | hep-th | null | The unfolded formulation for arbitrary massless mixed-symmetry bosonic and
fermionic fields in Minkowski space is constructed. The unfolded form is proved
to be uniquely determined by the requirement that all gauge symmetries are
manifest. The unfolded equations have the form of a covariant constancy
condition. The gauge fields and gauge parameters are differential forms with
values in certain irreducible Lorentz tensors. The unfolded equations for
bosons determine completely those for fermions. The proposed unfolded
formulation also contains dual formulations for massless mixed-symmetry fields.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 17:28:46 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jan 2008 21:29:04 GMT"
},
{
"version": "v3",
"created": "Wed, 26 Mar 2008 09:59:48 GMT"
},
{
"version": "v4",
"created": "Thu, 29 May 2008 14:27:10 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Skvortsov",
"E. D.",
""
]
] | [
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] |
801.2269 | Paolo Saracco | P. Saracco, M. Longhetti, S. Andreon, A. Mignano (INAF - Osservatorio
Astronomico di Brera) | The evolution of the morphological scale of early-type galaxies since
z=2 | 4 pages, 2 figures. To appear in the proceedings of `A Century of
Cosmology', S. Servolo, August 2007, to be published in Il Nuovo Cimento | Nuovo Cim.B122:1301-1305,2007 | 10.1393/ncb/i2008-10478-9 | null | astro-ph | null | We present the morphological analysis based on HST-NICMOS observations in the
F160W filter of a sample of 30 early-type galaxies spectroscopically confirmed
at 1.2<z<2. We derive the effective radius R_e and the mean surface brightness
mu_e of galaxies in the rest-frame R-band. We find that early-types at z~1.5
are characterized by a surface brightness (SB) much higher then their local
counterparts with comparable R_e. In particular, we find that the mean SB of
these early-types should get fainter by ~2.5 mag from z~1.5 to z=0 to match the
SB of the local early-types with comparable R_e. This evolution exceeds by a
factor two the luminosity evolution expected for early-types in this redshift
range and more than a factor three the one derived from the observed luminosity
function of galaxies. Consequently, an evolution of the effective radius R_e
from the epoch of their formation towards z=0 has to be invoked and the
hypothesis of fixed size rejected.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 12:31:55 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Saracco",
"P.",
"",
"INAF - Osservatorio\n Astronomico di Brera"
],
[
"Longhetti",
"M.",
"",
"INAF - Osservatorio\n Astronomico di Brera"
],
[
"Andreon",
"S.",
"",
"INAF - Osservatorio\n Astronomico di Brera"
],
[
"Mignano",
"A.",
"",
"INAF - Osservatorio\n Astronomico di Brera"
]
] | [
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801.227 | Ferdinando Patat | F. Patat | The Dancing Sky: 6 years of night sky observations at Cerro Paranal | 19 pages, 27 figures, accepted for publication in Astronomy &
Astrophysics. Full resolution version at
http://www.hq.eso.org/~fpatat/science/skybright/paperIII.pdf | null | 10.1051/0004-6361:20079279 | null | astro-ph | null | The present work provides the results of the first six years of operation of
the systematic night-sky monitoring at ESO-Paranal (Chile). The UBVRI night-sky
brightness was estimated on about 10,000 VLT-FORS1 archival images, obtained on
more than 650 separate nights, distributed over 6 years and covering the
descent from maximum to minimum of sunspot cycle n.23. Additionally, a set of
about 1,000 low resolution, optical night-sky spectra have been extracted and
analyzed. The unprecedented database discussed in this paper has led to the
detection of a clear seasonal variation of the broad band night sky brightness
in the VRI passbands, similar to the well known semi-annual oscillation of the
NaI D doublet. The spectroscopic data demonstrate that this seasonality is
common to all spectral features, with the remarkable exception of the OH
rotational-vibrational bands. A clear dependency on the solar activity is
detected in all passbands and it is particularly pronounced in the U band,
where the sky brightness decreased by about 0.6 mag arcsec-2 from maximum to
minimum of solar cycle n.23. No correlation is found between solar activity and
the intensity of the NaI D doublet and the OH bands. A strong correlation
between the intensity of NI 5200A and [OI]6300,6364A is reported here for the
first time. The paper addresses also the determination of the correlation
timescales with solar activity and the possible connection with the flux of
charged particles emitted by the Sun.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 11:58:14 GMT"
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] | 2009-11-13T00:00:00 | [
[
"Patat",
"F.",
""
]
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801.2271 | Iraklis S. Konstantopoulos | I. S. Konstantopoulos (1), N. Bastian (1), L. J. Smith (2,1), G.
Trancho (3,4), M. S. Westmoquette (1), J. S. Gallagher III (5) ((1)
University College London, (2) STScI and ESA, (3) Universidad de La Laguna,
(4) Gemini Observatory, (5) University of Wisconsin-Madison) | New Results on the Ages of Star Clusters in Region B of M82 | To appear in Perez, de Grijs and Gonzalez Delgado (eds.), `Young
Massive Star Clusters: Initial Conditions and Environments', 2008,
Astrophysics & Space Science | Astrophys.Space Sci.324:343-346,2009 | 10.1007/s10509-009-0092-9 | null | astro-ph | null | The post-starburst region B in M82 and its massive star cluster component
have been the focus of multiple studies, with reports that there is a large
population of coeval clusters of age ~1 Gyr, which were created with a Gaussian
initial mass distribution. This is in disagreement with other studies of young
star clusters, which invariably find a featureless power-law mass distribution.
Here, we present Gemini-North optical spectra of seven star clusters in M82-B
and show that their ages are all between 10 and 300 Myr (a factor of 3-100
younger than previous photometric results) and that their extinctions range
between near-zero and 4 mag (Av). Using new HST ACS-HRC U-band observations we
age date an additional ~30 clusters whose ages/extinctions agree well with
those determined from spectroscopy. Completeness tests show that the reported
`turn-over' in the luminosity/mass distributions is most likely an artefact,
due to the resolved nature of the clusters. We also show that the radial
velocities of the clusters are inconsistent with them belonging to a bound
region.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 12:02:22 GMT"
}
] | 2009-12-04T00:00:00 | [
[
"Konstantopoulos",
"I. S.",
""
],
[
"Bastian",
"N.",
""
],
[
"Smith",
"L. J.",
""
],
[
"Trancho",
"G.",
""
],
[
"Westmoquette",
"M. S.",
""
],
[
"Gallagher",
"J. S.",
"III"
]
] | [
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801.2272 | Henri Johnston | Cornelius Greither and Henri Johnston | Non-existence and splitting theorems for normal integral bases | 17 pages, 4 figures, uses xypic, minor revisions following referee's
report. To appear in Annales de L'Institut Fourier | null | null | null | math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We establish new conditions that prevent the existence of (weak) normal
integral bases in tame Galois extensions of number fields. This leads to the
following result: under appropriate technical hypotheses, the existence of a
normal integral basis in the upper layer of an abelian tower Q \subset K
\subset L forces the tower to be split in a very strong sense.
| [
{
"version": "v1",
"created": "Tue, 15 Jan 2008 12:16:00 GMT"
},
{
"version": "v2",
"created": "Thu, 26 Feb 2009 12:38:19 GMT"
}
] | 2009-02-26T00:00:00 | [
[
"Greither",
"Cornelius",
""
],
[
"Johnston",
"Henri",
""
]
] | [
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