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711.4108 | Zurab Kakushadze | Zurab Kakushadze | Tachyon-Free Non-Supersymmetric Strings on Orbifolds | 17 pages | Int.J.Mod.Phys.A23:4371-4386,2008 | 10.1142/S0217751X08042304 | null | hep-th | null | We discuss tachyon-free examples of (Type IIB on) non-compact
non-supersymmetric orbifolds. Tachyons are projected out by discrete torsion
between orbifold twists, while supersymmetry is broken by a Scherk-Schwarz
phase (+1/-1 when acting on space-time bosons/fermions) accompanying some even
order twists. The absence of tachyons is encouraging for constructing
non-supersymmetric D3-brane gauge theories with stable infrared fixed points.
The D3-brane gauge theories in our orbifold backgrounds have chiral N = 1
supersymmetric spectra, but non-supersymmetric interactions.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:00:01 GMT"
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] | 2008-12-18T00:00:00 | [
[
"Kakushadze",
"Zurab",
""
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711.4109 | Martin White | Martin White, Paul Martini and J.D. Cohn | Constraints on the correlation between QSO luminosity and host halo mass
from high-redshift quasar clustering | 6 pages, 4 figures. Minor revisions to address questions from
referee. References updated | null | 10.1111/j.1365-2966.2008.13817.x | null | astro-ph | null | Recent measurements of high-redshift QSO clustering from the Sloan Digital
Sky Survey indicate that QSOs at z~4 have a bias b~14. We find that this
extremely high clustering amplitude, combined with the corresponding space
density, constrains the dispersion in the L-Mhalo relation to be less than 50%
at 99% confidence for the most conservative case of a 100% duty cycle. This
upper limit to the intrinsic dispersion provides as strong a constraint as
current upper limits to the intrinsic dispersion in the local M_BH-sigma
relation and the ratio of bolometric to Eddington luminosity of luminous QSOs.
| [
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"created": "Mon, 26 Nov 2007 21:00:07 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Apr 2008 20:17:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"White",
"Martin",
""
],
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"Martini",
"Paul",
""
],
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"Cohn",
"J. D.",
""
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711.411 | Paola Rebusco Dr | P. Rebusco, E. Churazov, R. A. Sunyaev, H. Boehringer, W. Forman | Width of X-ray lines in cooling flows | Accepted for publication on MNRAS | null | null | null | astro-ph | null | The dissipation of turbulent gas motions is one of the likely mechanisms that
has been proposed to heat the intracluster medium (ICM) in the cores of
clusters and groups of galaxies. We consider the impact of gas motions on the
width of the most prominent X-ray emission lines. For heavy elements (like
iron) the expected linewidth is much larger than the width due to pure thermal
broadening and the contribution due to turbulent gas motions should be easily
detected with the new generation of X-ray micro-calorimeters, such as the
Spektr-RG calorimeter (SXC). For instance in the Perseus cluster the turbulent
velocity required to balance radiative cooling (as derived by Rebusco et al.
2006), would imply a width of the 6.7 keV Fe line of 10-20 eV, while the pure
thermal broadening is ~4 eV. The radial dependence of the linewidth is
sensitive to i) the radial dependence of the velocity amplitude and ii) the
"directionality" of the stochastic motions (e.g. isotropic turbulence or
predominantly radial gas motions). If the width of several lines,
characteristic for different gas temperatures, can be measured, then it should
be possible to probe both the "directionality" and the amplitude of the gas
motions. Moreover a measurement of the width would put a lower limit on the
amount of the kinetic energy available for dissipation, giving a constraint on
the ICM models.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:14:40 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Rebusco",
"P.",
""
],
[
"Churazov",
"E.",
""
],
[
"Sunyaev",
"R. A.",
""
],
[
"Boehringer",
"H.",
""
],
[
"Forman",
"W.",
""
]
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] |
711.4111 | Jason F. Rowe | Jason F. Rowe, Jaymie M. Matthews, Sara Seager, Eliza Miller-Ricci,
Dimitar Sasselov, Rainer Kuschnig, David B. Guenther, Anthony F. J. Moffat,
Slavek M. Rucinski, Gordon A. H. Walker, and Werner W. Weiss | The Very Low Albedo of an Extrasolar Planet: MOST Spacebased Photometry
of HD 209458 | 23 pages, 8 figures, accepted to the ApJ. v2: minor changes to mirror
accepted ApJ version | null | 10.1086/591835 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Measuring the albedo of an extrasolar planet provides insights into its
atmospheric composition and its global thermal properties, including heat
dissipation and weather patterns. Such a measurement requires very precise
photometry of a transiting system sampling fully many phases of the secondary
eclipse. Spacebased optical photometry of the transiting system HD 209458 from
the MOST (Microvariablity and Oscillations of STars) satellite, spanning 14 and
44 days in 2004 and 2005 respectively, allows us to set a sensitive limit on
the optical eclipse of the hot exosolar giant planet in this system. Our best
fit to the observations yields a flux ratio of the planet and star of 7 $\pm$ 9
ppm (parts per million), which corresponds to a geometric albedo through the
MOST bandpass (400-700 nm) of $A_g$ = 0.038 $\pm$ 0.045. This gives a 1$\sigma$
upper limit of 0.08 for the geometric albedo and a 3$\sigma$ upper limit of
0.17. HD 209458b is significantly less reflective than Jupiter (for which $A_g$
would be about 0.5). This low geometric albedo rules out the presence of bright
reflective clouds in this exoplanet's atmosphere. We determine refined
parameters for the star and exoplanet in the HD 209458 system based on a model
fit to the MOST light curve.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:00:15 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jul 2008 20:43:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rowe",
"Jason F.",
""
],
[
"Matthews",
"Jaymie M.",
""
],
[
"Seager",
"Sara",
""
],
[
"Miller-Ricci",
"Eliza",
""
],
[
"Sasselov",
"Dimitar",
""
],
[
"Kuschnig",
"Rainer",
""
],
[
"Guenther",
"David B.",
""
],
[
"Moffat",
"Anthony F. J.",
""
],
[
"Rucinski",
"Slavek M.",
""
],
[
"Walker",
"Gordon A. H.",
""
],
[
"Weiss",
"Werner W.",
""
]
] | [
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] |
711.4112 | Gabriele Ghisellini | A. Celotti (SISSA, Trieste) and G. Ghisellini (Oss. Astron. di Brera) | The power of blazar jets | MNRAS, in press, changed Fig. 5, corrected typos | null | 10.1111/j.1365-2966.2007.12758.x | null | astro-ph | null | We estimate the power of relativistic, extragalactic jets by modelling the
spectral energy distribution of a large number of blazars. We adopt a simple
one-zone, homogeneous, leptonic synchrotron and inverse Compton model, taking
into account seed photons originating both locally in the jet and externally.
The blazars under study have an often dominant high energy component, which, if
interpreted as due to inverse Compton radiation, limits the value of the
magnetic field within the emission region. As a consequence, the corresponding
Poynting flux cannot be energetically dominant. Also the bulk kinetic power in
relativistic leptons is often smaller than the dissipated luminosity. This
suggests that the typical jet should comprise an energetically dominant proton
component. If there is one proton per relativistic electrons, jets radiate
around 2-10 per cent of their power in high power blazars and 3-30 per cent in
less powerful BL Lacs.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:00:26 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Feb 2008 11:16:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Celotti",
"A.",
"",
"SISSA, Trieste"
],
[
"Ghisellini",
"G.",
"",
"Oss. Astron. di Brera"
]
] | [
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] |
711.4113 | Charles C. Steidel | T. S. Goncalves, C. C. Steidel, and M. Pettini | Detection of the Transverse Proximity Effect: Radiative Feedback from
Bright QSOs | 19 pages, 17 figures, ApJ, in press | null | 10.1086/527313 | null | astro-ph | null | Measuring the response of the intergalactic medium to a blast of ionizing
radiation allows one to infer the physical properties of the medium and, in
principle, the lifetime and isotropy of the radiating source. The most
sensitive such measurements can be made if the source of radiation is near the
line of sight to a bright background QSO. We present results based on deep
Keck/HIRES observations of the QSO triplet KP76, KP77 and KP78 at z ~2.5, with
separations of 2-3 arcmin on the plane of the sky. Using accurate systemic
redshifts of the QSOs from near-IR spectroscopy, we quantify the state of the
IGM gas in the proximity regions where the expected ionizing flux from the
foreground QSOs exceeds that of the metagalactic background by factors of
10-200, assuming constant and isotropic emission. Based on the unusual
ionization properties of the absorption systems with detected HI, CIV, and OVI,
we conclude that the gas has been significantly affected by the UV radiation
from the nearby QSOs. Aided by observations of the galaxy density near the
foreground QSOs, we discuss several effects that may explain why the transverse
proximity effect has eluded most previous attempts to detect it. Our
observations suggest that the luminosities of KP76 and KP77 have remained
comparable to current values over timescales of, respectively, Delta t > 25 Myr
and 16 Myr < Delta t < 33 Myr - consistent with typical QSO lifetimes estimated
from independent, less-direct methods. There is no evidence that the UV
radiation from either QSO was significantly anisotropic during these intervals.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:00:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Goncalves",
"T. S.",
""
],
[
"Steidel",
"C. C.",
""
],
[
"Pettini",
"M.",
""
]
] | [
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] |
711.4114 | Carlos Mochon | Carlos Mochon (Perimeter Institute) | Quantum weak coin flipping with arbitrarily small bias | 80 pages. The main result has thus far only been checked by the
author, so it may yet be destined to join the other set of illustrious
bit-commitment/coin-flipping papers. For updates see
http://lightlike.com/zerocoin/ | null | null | null | quant-ph | null | "God does not play dice. He flips coins instead." And though for some reason
He has denied us quantum bit commitment. And though for some reason he has even
denied us strong coin flipping. He has, in His infinite mercy, granted us
quantum weak coin flipping so that we too may flip coins.
Instructions for the flipping of coins are contained herein. But be warned!
Only those who have mastered Kitaev's formalism relating coin flipping and
operator monotone functions may succeed. For those foolhardy enough to even
try, a complete tutorial is included.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:02:01 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Mochon",
"Carlos",
"",
"Perimeter Institute"
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711.4115 | Daniel Grumiller | Daniel Grumiller | Path integral for half-binding potentials as quantum mechanical analog
for black hole partition functions | 6 pages, proceedings contribution to "Path integrals - New Trends and
Perspectives", Dresden, September 2007 | null | 10.1142/9789812837271_0033 | MIT-CTP 3913 | quant-ph gr-qc hep-th | null | The semi-classical approximation to black hole partition functions is not
well-defined, because the classical action is unbounded and the first variation
of the uncorrected action does not vanish for all variations preserving the
boundary conditions. Both problems can be solved by adding a Hamilton-Jacobi
counterterm. I show that the same problem and solution arises in quantum
mechanics for half-binding potentials.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:23:50 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Grumiller",
"Daniel",
""
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711.4116 | Jonathan C. Tan | Jonathan C. Tan (1), Christopher F. McKee (2) ((1) Dept. of Astronomy,
University of Florida; (2) Depts. of Physics and Astronomy, UC Berkeley) | Star Formation at Zero and Very Low Metallicities | 16 pages, including 11 figures, Review paper to appear in "First
Stars III", eds. B. O'Shea, A. Heger and T. Abel | AIP Conf.Proc.990:47-62,2008 | 10.1063/1.2905668 | null | astro-ph | null | We describe how star formation is expected to proceed in the early metal-free
Universe, focusing on the very first generations of stars. We then discuss how
the star formation process may change as the effects of metallicity, external
radiative feedback, and magnetic and turbulent support of the gas become more
important. The very first stars (Pop III.1) have relatively simple initial
conditions set by cosmology and the cooling properties of primordial gas. We
describe the evolution of these stars as they grow in mass by accretion from
their surrounding gas cores and how the accretion process is affected and
eventually terminated by radiative feedback processes, especially HII region
expansion and disk photoevaporation. The ability of the protostar and its disk
to generate dynamically important magnetic fields is reviewed and their effects
discussed. Pop III.1 star formation is likely to produce massive (~100-200Msun)
stars that then influence their surroundings via ionization, stellar winds, and
supernovae. These processes heat, ionize and metal-enrich the gas, thus
altering the initial conditions for the next generation of star formation.
Stars formed from gas that has been altered significantly by radiative and/or
mechanical feedback, but not by metal enrichment (Pop III.2) are expected to
have significantly smaller masses than Pop III.1 stars because of more
efficient cooling from enhanced HD production. Stars formed from gas that is
metal-enriched to levels that affect the dynamics of the collapse (the first
Pop II stars) are also expected to have relatively low masses. We briefly
compare the above star formation scenarios to what is known about present-day
star formation.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:52:22 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Tan",
"Jonathan C.",
""
],
[
"McKee",
"Christopher F.",
""
]
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] |
711.4117 | Andrew Raich | Albert Boggess and Andrew Raich | A Simplified Calculation for the Fundamental Solution to the Heat
Equation on the Heisenberg Group | 8 pages | Proc. Amer. Math. Soc. 137 (2009), no. 3, 937--944 | null | null | math.AP | null | Let $L = -1/4 (\sum_{j=1}^n(X_j^2+Y_j^2)+i\gamma T)$ where $\gamma$ is a
complex number, $X_j$, $Y_j$, and $T$ are the left invariant vector fields of
the Heisenberg group structure for $R^n \times R^n \times R$. We explicitly
compute the Fourier transform (in the spatial variables) of the fundamental
solution of the Heat Equation $\partial_s\rho = -L\rho$. As a consequence, we
have a simplified computation of the Fourier transform of the fundamental
solution of the $\Box_b$-heat equation on the Heisenberg group and an explicit
kernel of the heat equation associated to the weighted dbar-operator in $C^n$
with weight $\exp(-\tau P(z_1,...,z_n))$ where $P(z_1,...,z_n) = 1/2(x_1^2 +
>... x_n^2)$, $z_j=x_j+iy_j$, and $\tau\in R$.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:03:40 GMT"
}
] | 2012-08-13T00:00:00 | [
[
"Boggess",
"Albert",
""
],
[
"Raich",
"Andrew",
""
]
] | [
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] |
711.4118 | Mukund Rangamani | Veronika E. Hubeny and Mukund Rangamani | Holographic entanglement entropy for disconnected regions | 3 eps figures, 17 pages. v2: minor changes | JHEP0803:006,2008 | 10.1088/1126-6708/2008/03/006 | null | hep-th cond-mat.stat-mech quant-ph | null | We present a simple derivation of the entanglement entropy for a region made
up of a union of disjoint intervals in 1+1 dimensional quantum field theories
using holographic techniques. This generalizes the results for 1+1 dimensional
conformal field theories derived previously by exploiting the uniformization
map. We further comment on the generalization of our result to higher
dimensional field theories.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:04:10 GMT"
},
{
"version": "v2",
"created": "Mon, 4 Feb 2008 14:59:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hubeny",
"Veronika E.",
""
],
[
"Rangamani",
"Mukund",
""
]
] | [
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] |
711.4119 | Pier Stefano Corasaniti | Pier Stefano Corasaniti (LUTH, Meudon) and Alessandro Melchiorri (Rome
U. & INFN, Rome) | Testing Cosmology with Cosmic Sound Waves | 9 pages, 6 figures. Additional discussion, matches PRD accepted
version | Phys.Rev.D77:103507,2008 | 10.1103/PhysRevD.77.103507 | null | astro-ph | null | WMAP observations have accurately determined the position of the first two
peaks and dips in the CMB temperature power spectrum. These encode information
on the ratio of the distance to the last scattering surface to the sound
horizon at decoupling. However pre-recombination processes can contaminate this
distance information. In order to assess the amplitude of these effects we use
the WMAP data and evaluate the relative differences of the CMB peaks and dips
multipoles. We find that the position of the first peak is largely displaced
with the respect to the expected position of the sound horizon scale at
decoupling. In contrast the relative spacings of the higher extrema are
statistically consistent with those expected from perfect harmonic
oscillations. This provides evidence for a scale dependent phase shift of the
CMB oscillations which is caused by gravitational driving forces affecting the
propagation of sound waves before recombination. By accounting for these
effects we have performed a MCMC likelihood analysis to constrain in
combination with recent BAO data a constant dark energy equation w. For a flat
universe we find at 95% upper limit w<-1.10, and including the HST prior
w<-1.14, which are only marginally consistent with limits derived from the
supernova SNLS sample. Larger limits are obtained for non-flat cosmologies.
From the full CMB likelihood analysis we also estimate the values of the
shift parameter R and the multipole l_a of the acoustic horizon at decoupling
for several cosmologies to test their dependence on model assumptions. Although
the analysis of the full CMB spectra should be always preferred, using the
position of the CMB peaks and dips provide a simple and consistent method for
combining CMB constraints with other datasets.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:20:33 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Mar 2008 11:19:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Corasaniti",
"Pier Stefano",
"",
"LUTH, Meudon"
],
[
"Melchiorri",
"Alessandro",
"",
"Rome\n U. & INFN, Rome"
]
] | [
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711.412 | Jens Gerlach Christensen | J. G. Christensen and G. \'Olafsson | Examples of Coorbit Spaces for Dual Pairs | null | null | null | null | math.FA math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we summarize and give examples of a generalization of the
coorbit space theory initiated in the 1980's by H.G. Feichtinger and K.H.
Gr\"ochenig. Coorbit theory has been a powerful tool in characterizing Banach
spaces of distributions with the use of integrable representations of locally
compact groups. Examples are a wavelet characterization of the Besov spaces and
a characterization of some Bergman spaces by the discrete series representation
of $\mathrm{SL}_2(\mathbb{R})$. We present examples of Banach spaces which
could not be covered by the previous theory, and we also provide atomic
decompositions for an example related to a non-integrable representation.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:06:23 GMT"
},
{
"version": "v2",
"created": "Thu, 11 Sep 2008 01:41:29 GMT"
}
] | 2008-09-11T00:00:00 | [
[
"Christensen",
"J. G.",
""
],
[
"Ólafsson",
"G.",
""
]
] | [
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] |
711.4121 | Jian-Xin Zhu Dr. | Yunong Qi, Jian-Xin Zhu, Shufeng Zhang, and C. S. Ting | Kondo Resonance in the Presence of Spin-Polarized Currents | 4+ pages, 4 eps figures | null | 10.1103/PhysRevB.78.045305 | null | cond-mat.str-el cond-mat.mes-hall | null | We propose an improved method of the equation of motion approach to study the
Kondo problem in spin-dependent non-equilibrium conditions. We find that the
previously introduced additional renormalization for non-equilibrium Kondo
effects is not required when we use a proper decoupling scheme. Our improved
formulation is then applied to address the spin-split Kondo peaks when a spin
current injects into a Kondo system.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:07:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Qi",
"Yunong",
""
],
[
"Zhu",
"Jian-Xin",
""
],
[
"Zhang",
"Shufeng",
""
],
[
"Ting",
"C. S.",
""
]
] | [
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] |
711.4122 | St\'ephane Vern\`ede | St\'ephane Vern\`ede and Michel Rappaz | A simple and efficient model for mesoscale solidification simulation of
globular grain structures | null | Acta Materialia, Volume 55, Issue 5, March 2007, Pages 1703-1710 | 10.1016/j.actamat.2006.10.031 | null | cond-mat.mtrl-sci | null | A simple model for the solidification of globular grains in metallic alloys
is presented. Based on the Voronoi diagram of the nuclei centers, it accounts
for the curvature of the grains near triple junctions. The predictions of this
model are close to those of more refined approaches such as the phase field
method, but with a computation cost decreased by several orders of magnitude.
Therefore, this model is ideally suited for granular simulations linking the
behavior of individual grains to macroscopic properties of the material.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:08:22 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Vernède",
"Stéphane",
""
],
[
"Rappaz",
"Michel",
""
]
] | [
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] |
711.4123 | St\'ephane Herbert-Fort | St\'ephane Herbert-Fort, Dennis Zaritsky, Yeun Jin Kim, Jeremy Bailin,
James E. Taylor | The Orbital Distribution of Satellite Galaxies | 14 pages, 13 figures; Accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2007.12756.x | null | astro-ph | null | We measure the distribution of velocities for prograde and retrograde
satellite galaxies using a combination of published data and new observations
for 78 satellites of 63 extremely isolated disc galaxies (169 satellites
total). We find that the velocity distribution is non-Gaussian (>99.9%
confidence), but that it can be described as the sum of two Gaussians, one of
which is broad (sigma = 176 \pm 15 km/s), has a mean prograde velocity of 86
\pm 30 km/s, and contains ~55% of the satellites, while the other is slightly
retrograde with a mean velocity of -21 \pm 22 km/s and sigma = 74 \pm 18 km/s
and contains ~45% of the satellites. Both of these components are present over
all projected radii and found in the sample regardless of cuts on primary
inclination or satellite disc angle. The double-Gaussian shape, however,
becomes more pronounced among satellites of more luminous primaries. We remove
the potential dependence of satellite velocity on primary luminosity using the
Tully-Fisher relation and still find the velocity distribution to be asymmetric
and even more significantly non-Gaussian. The asymmetric velocity distribution
demonstrates a connection between the inner, visible disc galaxy and the
kinematics of the outer, dark halo. The reach of this connection, extending
even beyond the virial radii, suggests that it is imprinted by the satellite
infall pattern and large-scale effects, rather than by higher-level dynamical
processes in the formation of the central galaxy or late-term evolution of the
satellites.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:35:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Herbert-Fort",
"Stéphane",
""
],
[
"Zaritsky",
"Dennis",
""
],
[
"Kim",
"Yeun Jin",
""
],
[
"Bailin",
"Jeremy",
""
],
[
"Taylor",
"James E.",
""
]
] | [
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711.4124 | Ayres Freitas | Ayres Freitas, Kyoungchul Kong | Two universal extra dimensions and spinless photons at the ILC | 21 pp; few minor modifications in text and references added; version
published in JHEP | JHEP 0802:068,2008 | 10.1088/1126-6708/2008/02/068 | ANL-HEP-PR-07-99, FERMILAB-PUB-07-619-T | hep-ph | null | We study the ILC phenomenology of (1,0) Kaluza-Klein (KK) modes along two
universal extra dimensions compactified on the chiral square. We compute
production cross sections of various (1,0) particles at the ILC with sqrt(s)=1
TeV, focusing on decays of KK-leptons and the KK partner of hypercharge gauge
boson down to the "spinless photon", which is the lightest KK particle. We
contrast this model to one universal extra dimension with KK-photon (spin-1)
and supersymmetry with neutralino (spin-1/2) or gravitino (spin-3/2) dark
matter. We also investigate the discovery potential for (1,1) KK bosons as
s-channel resonances.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:30:07 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Mar 2008 21:00:27 GMT"
}
] | 2009-09-17T00:00:00 | [
[
"Freitas",
"Ayres",
""
],
[
"Kong",
"Kyoungchul",
""
]
] | [
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] |
711.4125 | Jean-Luc Thiffeault | Jean-Luc Thiffeault and Khalid Kamhawi | Chaotic Geodesics | 13 pages, 27 figures. PDFLaTeX with RevTeX4-1 macros. Fixed some
typos and updated references. Published in proceedings of the conference on
"Chaos, Complexity, and Transport" (Le Pharo, Marseille, June 2007) | null | 10.1142/9789812818805_0003 | null | nlin.CD | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | When a shallow layer of inviscid fluid flows over a substrate, the fluid
particle trajectories are, to leading order in the layer thickness, geodesics
on the two-dimensional curved space of the substrate. Since the two-dimensional
geodesic equation is a two degree-of-freedom autonomous Hamiltonian system, it
can exhibit chaos, depending on the shape of the substrate. We find chaotic
behaviour for a range of substrates.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:25:57 GMT"
},
{
"version": "v2",
"created": "Thu, 5 Feb 2015 14:59:04 GMT"
}
] | 2015-02-06T00:00:00 | [
[
"Thiffeault",
"Jean-Luc",
""
],
[
"Kamhawi",
"Khalid",
""
]
] | [
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711.4126 | Sarah Shandera | Marilena LoVerde, Amber Miller, Sarah Shandera, Licia Verde | Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures | 43 pages, 9 figures; references added, submitted to JCAP; typo
corrected in Table 1, minor changes to the text | JCAP 0804:014,2008 | 10.1088/1475-7516/2008/04/014 | null | astro-ph | null | The detection of primordial non-Gaussianity could provide a powerful means to
test various inflationary scenarios. Although scale-invariant non-Gaussianity
(often described by the $f_{NL}$ formalism) is currently best constrained by
the CMB, single-field models with changing sound speed can have strongly
scale-dependent non-Gaussianity. Such models could evade the CMB constraints
but still have important effects at scales responsible for the formation of
cosmological objects such as clusters and galaxies. We compute the effect of
scale-dependent primordial non-Gaussianity on cluster number counts as a
function of redshift, using a simple ansatz to model scale-dependent features.
We forecast constraints on these models achievable with forthcoming data sets.
We also examine consequences for the galaxy bispectrum. Our results are
relevant for the Dirac-Born-Infeld model of brane inflation, where the
scale-dependence of the non-Gaussianity is directly related to the geometry of
the extra dimensions.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:38:46 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 13:48:29 GMT"
},
{
"version": "v3",
"created": "Thu, 13 Mar 2008 20:53:21 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"LoVerde",
"Marilena",
""
],
[
"Miller",
"Amber",
""
],
[
"Shandera",
"Sarah",
""
],
[
"Verde",
"Licia",
""
]
] | [
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711.4127 | Fabio Zucca | Fabio Zucca | An inequality for correlated measurable functions | 8 pages, corrected some misprints and simplified some proofs | J. Ineq. Pure and Appl. Math. 9 n.1 (2008), Art. 3 | null | null | math.CA math.PR | null | A classical inequality, which is known for families of monotone functions, is
generalized to a larger class of families of measurable functions. Moreover we
characterize all the families of functions for which the equality holds. We
apply this result to a problem arising from probability theory.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:09:20 GMT"
},
{
"version": "v2",
"created": "Fri, 30 Nov 2007 15:08:30 GMT"
}
] | 2011-01-25T00:00:00 | [
[
"Zucca",
"Fabio",
""
]
] | [
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] |
711.4128 | Zied Ammari | Ammari Zied (UCP-Cergy), Nier Francis (IRMAR-Rennes) | Mean field limit for bosons and infinite dimensional phase-space
analysis | 57 pages | null | null | null | math-ph math.AP math.MP | null | This article proposes the construction of Wigner measures in the infinite
dimensional bosonic quantum field theory, with applications to the derivation
of the mean field dynamics. Once these asymptotic objects are well defined, it
is shown how they can be used to make connections between different kinds of
results or to prove new ones.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:47:15 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Zied",
"Ammari",
"",
"UCP-Cergy"
],
[
"Francis",
"Nier",
"",
"IRMAR-Rennes"
]
] | [
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] |
711.4129 | Melanie Johnston-Hollitt Dr | M. Johnston-Hollitt, R.W. Hunstead and E. Corbett | The optical morphology of A3667 re-examined | 10 pages, 12 figures, accepted to Astronomy & Astrophysics | null | 10.1051/0004-6361:20042242 | null | astro-ph | null | The galaxy cluster A3667 was observed using the Two-degree Field (2dF)
multifibre spectroscopic system on the Anglo-Australian Telescope in a program
designed to examine the velocity structure in the region. Specifically, we
sought evidence from the optical data for the putative cluster merger believed
to be responsible for the observed radio and X-ray emission. We present 184 new
redshifts in the region, of which 143 correspond to member galaxies of A3667.
We find the cluster velocity distribution to be well modelled by a single
Gaussian in agreement with previous results. In addition, new redshift-selected
isodensity plots significantly reduce the prominence of the previously reported
subgroup to the north-west of the main cluster. Instead, we find the galaxy
distribution to be elongated and well mixed, with a high velocity dispersion
and no significant evidence for substructure. These results are consistent with
the axis of the proposed merger being close to the plane of the sky.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:58:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Johnston-Hollitt",
"M.",
""
],
[
"Hunstead",
"R. W.",
""
],
[
"Corbett",
"E.",
""
]
] | [
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] |
711.413 | John K. Cannizzo | J. Tueller, R. F. Mushotzky, S. Barthelmy, J. K. Cannizzo, N. Gehrels,
C. B. Markwardt, G. K. Skinner, L. M. Winter | Swift BAT Survey of AGN | 15 pages, 15 figures, 2 tables; to appear in the Astrophysical
Journal, July 10, 2008, v. 681 | null | 10.1086/588458 | null | astro-ph | null | We present the results of the analysis of the first 9 months of data of the
Swift BAT survey of AGN in the 14-195 keV band. Using archival X-ray data or
follow-up Swift XRT observations, we have identified 129 (103 AGN) of 130
objects detected at |b|> 15 deg and with significance >4.8 sigma. One source
remains unidentified. These same X-ray data have allowed measurement of the
X-ray properties of the objects. We fit a power law to the log N - log S
distribution, and find the slope to be 1.42+/-0.14. Characterizing the
differential luminosity function data as a broken power law, we find a break
luminosity log L_*(erg/s) = 43.85+/-0.26, a low luminosity power law slope
a=0.84^{+0.16}_{-0.22}, and a high luminosity power law slope
b=2.55^{+0.43}_{-0.30}, similar to the values that have been reported based on
INTEGRAL data. We obtain a mean photon index 1.98 in the 14-195 keV band, with
an rms spread of 0.27. Integration of our luminosity function gives a local
volume density of AGN above 10^{41} erg/s of 2.4x10^{-3}/Mpc^3, which is about
10% of the total luminous local galaxy density above M_*=-19.75. We have
obtained X-ray spectra from the literature and from Swift XRT follow-up
observations. These show that the distribution of log n_H is essentially flat
from n_H=10^{20}/cm^{2} to 10^{24}/cm^2, with 50% of the objects having column
densities of less than 10^{22}/cm^{2}. BAT Seyfert galaxies have a median
redshift of 0.03, a maximum log luminosity of 45.1, and approximately half have
log n_H > 22.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 21:55:58 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Mar 2008 17:37:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tueller",
"J.",
""
],
[
"Mushotzky",
"R. F.",
""
],
[
"Barthelmy",
"S.",
""
],
[
"Cannizzo",
"J. K.",
""
],
[
"Gehrels",
"N.",
""
],
[
"Markwardt",
"C. B.",
""
],
[
"Skinner",
"G. K.",
""
],
[
"Winter",
"L. M.",
""
]
] | [
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] |
711.4131 | Hua Feng | Hua Feng, Philip Kaaret (Univ. of Iowa) | Optical Counterpart of the Ultraluminous X-ray Source IC 342 X-1 | 10 pages, 8 figures, accepted for publication in ApJ | Astrophys. J. 675: 1067-1075, 2008 | 10.1086/527353 | null | astro-ph | null | We present Chandra and HST observations of the ultraluminous X-ray source
(ULX) IC 342 X-1. The Chandra and HST images are aligned using two X-ray
emitting foreground stars. The astrometry corrected position for X-1 is R.A. =
03h45m55.61s, Decl. = +68d04m55.3s (J2000) with an error circle of 0.2". One
extended optical source is found in the error circle, which could be the
optical counterpart of X-1. The source shows an extended feature in HST images
at long wavelengths, which is likely to be a superposition of two point
sources, although it is possible that the dimmer one could be a jet. Both
sources are much redder than typical for ULX optical counterparts. The brighter
one has an absolute magnitude M_V = -5.2 +/- 0.2 and (B-V)_0 = 0.66 +/- 0.13
and the dimmer star is not detected in B and has (B-V)_0 > 2.1. Their colors
are consistent with an F8 to G0 Ib supergiant or a carbon star, respectively.
However, it is likely that part or most of the optical emission may be due to
X-rays reprocessed by the companion star or the accretion disk. The stellar
neighborhood of IC 342 X-1 lacks O stars and has a minimum age of ~10 Myr. This
excludes the possibility that the surrounding nebula is powered by an energetic
explosion of a single massive star that formed a black hole. We suggest that
the nebula is most likely powered by an outflow from the X-ray source.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:16:22 GMT"
}
] | 2010-05-25T00:00:00 | [
[
"Feng",
"Hua",
"",
"Univ. of Iowa"
],
[
"Kaaret",
"Philip",
"",
"Univ. of Iowa"
]
] | [
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711.4132 | Frank Oertel | Frank Oertel | A Short Note on some open problems in the geometry of operator ideals | null | null | null | null | math.FA math.RA | null | We list and discuss the background of some open problems, regarding the
principle of local reflexivity for maximal Banach ideals.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:00:56 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Oertel",
"Frank",
""
]
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711.4133 | Alexey Isaev | V.G. Gorbounov, A.P. Isaev and O.V. Ogievetsky | BRST Operator for Quantum Lie Algebras: Relation to Bar Complex | 20 pages | Theor. Math. Phys. 139 No. 1 (2004) 473 | null | null | math.QA math-ph math.MP | null | Quantum Lie algebras (an important class of quadratic algebras arising in the
Woronowicz calculus on quantum groups) are generalizations of Lie (super)
algebras. Many notions from the theory of Lie (super)algebras admit ``quantum''
generalizations. In particular, there is a BRST operator Q (Q^2=0) which
generates the differential in the Woronowicz theory and gives information about
(co)homologies of quantum Lie algebras. In our previous papers a recurrence
relation for the operator Q for quantum Lie algebras was given and solved. Here
we consider the bar complex for q-Lie algebras and its subcomplex of
q-antisymmetric chains. We establish a chain map (which is an isomorphism) of
the standard complex for a q-Lie algebra to the subcomplex of the antisymmetric
chains. The construction requires a set of nontrivial identities in the group
algebra of the braid group. We discuss also a generalization of the standard
complex to the case when a q-Lie algebra is equipped with a grading operator.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:18:40 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Gorbounov",
"V. G.",
""
],
[
"Isaev",
"A. P.",
""
],
[
"Ogievetsky",
"O. V.",
""
]
] | [
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] |
711.4134 | Justin Oelgoetz | Justin Oelgoetz, Christopher J. Fontes, Hong Lin Zhang, Anil K.
Pradhan | A study of the breakdown of the quasi-static approximation at high
densities and its effect on the helium-like K ALPHA complex of nickel, iron,
and calcium | Accepted by Physical Review A (http://pra.aps.org/). 11 pages + LANL
cover, 5 figures. Will update citation information as it becomes available.
Abbreviated abstract is listed here | Phys.Rev.A76:062504,2007 | 10.1103/PhysRevA.76.062504 | LA-UR-07-6501 | physics.atom-ph astro-ph | null | The General Spectral Modeling (GSM) code employs the quasi-static
approximation, a standard, low-density methodology that assumes the ionization
balance is separable from a determination of the excited-state populations that
give rise to the spectra. GSM also allows for some states to be treated only as
contributions to effective rates. While these two approximations are known to
be valid at low densities, this work investigates using such methods to model
high-density, non-LTE emission spectra and determines at what point the
approximations break down by comparing to spectra produced by the LANL code
ATOMIC which makes no such approximations. As both approximations are used by
other astrophysical and low-density modeling codes, the results should be of
broad interest. He-like K$\alpha$ emission spectra are presented for Ni, Fe,
and Ca, in order to gauge the effect of both approximations employed in GSM.
This work confirms that at and above the temperature of maximum abundance of
the He-like ionization stage, the range of validity for both approximations is
sufficient for modeling the low- and moderate-density regimes one typically
finds in astrophysical and magnetically confined fusion plasmas. However, a
breakdown does occur for high densities; we obtain quantitative limits that are
significantly higher than previous works. This work demonstrates that, while
the range of validity for both approximations is sufficient to predict the
density-dependent quenching of the z line, the approximations break down at
higher densities. Thus these approximations should be used with greater care
when modeling high-density plasmas such as those found in inertial confinement
fusion and electromagnetic pinch devices.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 19:29:27 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Oelgoetz",
"Justin",
""
],
[
"Fontes",
"Christopher J.",
""
],
[
"Zhang",
"Hong Lin",
""
],
[
"Pradhan",
"Anil K.",
""
]
] | [
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] |
711.4135 | Thomas Antonsen | T. M. Antonsen Jr. (1), R. T. Faghih (1), M. Girvan (1), E. Ott (1)
and J. Platig (1) ((1) Institute for Research in Electronics and Applied
Physics, University of Maryland, College Park, MD) | External Periodic Driving of Large Systems of Globally Coupled Phase
Oscillators | null | null | 10.1063/1.2952447 | null | nlin.CD | null | Large systems of coupled oscillators subjected to a periodic external drive
occur in many situations in physics and biology. Here the simple, paradigmatic
case of equal-strength, all-to-all sine-coupling of phase oscillators subject
to a sinusoidal external drive is considered. The stationary states and their
stability are determined. Using the stability information and numerical
experiments, parameter space phase diagrams showing when different types of
system behavior apply are constructed, and the bifurcations marking transitions
between different types of behavior are delineated. The analysis is supported
by results of direct numerical simulation of an ensemble of oscillators.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:15:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Antonsen",
"T. M.",
"Jr."
],
[
"Faghih",
"R. T.",
""
],
[
"Girvan",
"M.",
""
],
[
"Ott",
"E.",
""
],
[
"Platig",
"J.",
""
]
] | [
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] |
711.4136 | Andrzej Adamczak | Andrzej Adamczak and Mark P. faifman | Monte Carlo simulations of muCF processes kinetics in deuterium gas | 8 pages, 10 figures | Eur. Phys. J. D 51, 341 (2009) | 10.1140/epjd/e2008-00287-7 | null | physics.atom-ph | null | The muon-catalyzed-fusion processes in D$_2$ gas for various temperatures and
densities have been studied by means of Monte Carlo simulations. In particular,
the role of the resonant and nonresonant $dd\mu$ formation and differences
between the neutron time spectra from the ortho-D$_2$ and para-D$_2$ targets at
low temperatures have been investigated.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:19:51 GMT"
}
] | 2018-03-09T00:00:00 | [
[
"Adamczak",
"Andrzej",
""
],
[
"faifman",
"Mark P.",
""
]
] | [
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] |
711.4137 | Gavin Lawes | P. Kharel, C. Sudakar, A.B. Harris, R. Naik, G. Lawes | Electric field control of magnetic phase transitions in Ni3V2O8 | 11 pages, 4 figures | null | null | null | cond-mat.mtrl-sci cond-mat.str-el | null | We report on the electric field control of magnetic phase transition
temperatures in multiferroic Ni3V2O8 thin films. Using magnetization
measurements, we find that the phase transition temperature to the canted
antiferromagnetic state is suppressed by 0.2 K in an electric field of 30 MV/m,
as compared to the unbiased sample. Dielectric measurements show that the
transition temperature into the magnetic state associated with ferroelectric
order increases by 0.2 K when the sample is biased at 25 MV/m. This electric
field control of the magnetic transitions can be qualitatively understood using
a mean field model incorporating a tri-linear coupling between the magnetic
order parameters and spontaneous polarization.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:47:15 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Kharel",
"P.",
""
],
[
"Sudakar",
"C.",
""
],
[
"Harris",
"A. B.",
""
],
[
"Naik",
"R.",
""
],
[
"Lawes",
"G.",
""
]
] | [
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711.4138 | Paul Kiel Mr | Paul Kiel, Jarrod Hurley, Matthew Bailes, James Murray | Furnishing the Galaxy with Pulsars | 3 pages, 3 figures, Conference: "40 years of pulsars: Millisecond
pulsars, magnetars and more", McGill University, Montreal, Canada, ed.
A.Cumming et al., AIP | AIP Conf.Proc.983:610-612,2008 | 10.1063/1.2900309 | null | astro-ph | null | The majority of pulsar population synthesis studies performed to date have
focused on isolated pulsar evolution. Those that have incorporated pulsar
evolution within binary systems have tended to either treat binary evolution
poorly of evolve the pulsar population in an ad-hoc manner. Here we present the
first model of the Galactic field pulsar population that includes a
comprehensive treatment of both binary and pulsar evolution. Synthetic
observational surveys mimicking a variety of radio telescopes are then
performed on this population. As such, a complete and direct comparison of
model data with observations of the pulsar population within the Galactic disk
is now possible. The tool used for completing this work is a code comprised of
three components: stellar/binary evolution, Galactic kinematics and survey
selection effects. Here we give a brief overview of the method and assumptions
involved with each component. Some preliminary results are also presented as
well as plans for future applications of the code.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:47:35 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Kiel",
"Paul",
""
],
[
"Hurley",
"Jarrod",
""
],
[
"Bailes",
"Matthew",
""
],
[
"Murray",
"James",
""
]
] | [
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] |
711.4139 | Michael Eichmair | Michael Eichmair | The Plateau problem for marginally outer trapped surfaces | To app. in J. Differential Geometry. New title, introduction
rewritten with motivation and several concise references to the literature
added. Former Section 3 and Appendix B are now subsumed in Section 2. Remark
3.2 and Lemma A.1 added. Sections 3 and 4 now include a well-known geometric
argument driving Serrin's classical construction of boundary barriers | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We solve the Plateau problem for marginally outer trapped surfaces in general
Cauchy data sets. We employ the Perron method and tools from geometric measure
theory to force and control a blow-up of Jang's equation. Substantial new
geometric insights regarding the lower order properties of marginally outer
trapped surfaces are gained in the process. The techniques developed in this
paper are flexible and can be adapted to other non-variational existence
problems.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 04:51:52 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Aug 2008 19:49:24 GMT"
},
{
"version": "v3",
"created": "Sun, 17 Jan 2010 13:23:01 GMT"
}
] | 2010-01-17T00:00:00 | [
[
"Eichmair",
"Michael",
""
]
] | [
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] |
711.414 | Vladislav Kondratiev | A. V. Bilous (ASC Lpi, Mipt), V. I. Kondratiev (ASC Lpi, Wvu), M. V.
Popov (ASC Lpi), V. A. Soglasnov (ASC Lpi) | Review of overall parameters of giant radio pulses from the Crab pulsar
and B1937+21 | 3 pages, 4 figures, to be published in the Proceedings of the
conference "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More"
held on August 12-17, 2007, McGill University, Montreal, Canada | AIP Conf.Proc.983:118-120,2008 | 10.1063/1.2900119 | null | astro-ph | null | We present a review of observed parameters of giant radio pulses, based on
the observations conducted by our group during recent years. The observations
cover a broad frequency range of about 3 octaves, concentrating between 600 and
4850 MHz. Giant pulses of both the Crab pulsar and the millisecond pulsar
B1937+21 were studied with the 70-m Tidbinbilla, the 100-m GBT, 64-m Kalyazin
and Westerbork radio telescopes. We discuss pulse energy distribution,
dependence of peak flux density from the pulse width, peculiarities of radio
spectra, and polarization properties of giant radio pulses.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:52:06 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Bilous",
"A. V.",
"",
"ASC Lpi, Mipt"
],
[
"Kondratiev",
"V. I.",
"",
"ASC Lpi, Wvu"
],
[
"Popov",
"M. V.",
"",
"ASC Lpi"
],
[
"Soglasnov",
"V. A.",
"",
"ASC Lpi"
]
] | [
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] |
711.4141 | Knut Waagan | Christian Klingenberg, Wolfram Schmidt, Knut Waagan | Numerical comparison of Riemann solvers for astrophysical hydrodynamics | 24 pages, 38 figures. To be published in Journal of Computational
Physics | null | 10.1016/j.jcp.2007.07.034 | null | astro-ph | null | The idea of this work is to compare a new positive and entropy stable
approximate Riemann solver by Francois Bouchut with a state-of the-art
algorithm for astrophysical fluid dynamics. We implemented the new Riemann
solver into an astrophysical PPM-code, the Prometheus code, and also made a
version with a different, more theoretically grounded higher order algorithm
than PPM. We present shock tube tests, two-dimensional instability tests and
forced turbulence simulations in three dimensions. We find subtle differences
between the codes in the shock tube tests, and in the statistics of the
turbulence simulations. The new Riemann solver increases the computational
speed without significant loss of accuracy.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 22:54:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Klingenberg",
"Christian",
""
],
[
"Schmidt",
"Wolfram",
""
],
[
"Waagan",
"Knut",
""
]
] | [
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] |
711.4142 | Elizeu Santos-Neto | Elizeu Santos-Neto, Matei Ripeanu, Adriana Iamnitchi | Content Reuse and Interest Sharing in Tagging Communities | 6 pages, 6 figures, AAAI Spring Symposium on Social Information
Processing | null | null | null | cs.DL cs.IR | null | Tagging communities represent a subclass of a broader class of user-generated
content-sharing online communities. In such communities users introduce and tag
content for later use. Although recent studies advocate and attempt to harness
social knowledge in this context by exploiting collaboration among users,
little research has been done to quantify the current level of user
collaboration in these communities. This paper introduces two metrics to
quantify the level of collaboration: content reuse and shared interest. Using
these two metrics, this paper shows that the current level of collaboration in
CiteULike and Connotea is consistently low, which significantly limits the
potential of harnessing the social knowledge in communities. This study also
discusses implications of these findings in the context of recommendation and
reputation systems.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:05:02 GMT"
},
{
"version": "v2",
"created": "Sat, 26 Jan 2008 01:05:50 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Santos-Neto",
"Elizeu",
""
],
[
"Ripeanu",
"Matei",
""
],
[
"Iamnitchi",
"Adriana",
""
]
] | [
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711.4143 | Ignat Fialkovsky Mr | M. V. Perel, I. V. Fialkovsky | Exponentially localized solutions of the Klein-Gordon equation | 9 pages, 1 figure. Translated from Zapiski Nauchnykh Seminarov POMI,
Vol. 275, 2001, pp. 187--198 (in Russian) | Journal of Mathematical Sciences, vol. 117, no. 2, 2003 | 10.1023/A:1024679111273 | null | hep-th math-ph math.MP nlin.SI | null | Exponentially localized solutions of the Klein-Gordon equation for two and
three space variables are presented. The solutions depend on four free
parameters. For some relations between the parameters, the solutions describe
wave packets filled with oscillations whose amplitudes decrease in the Gaussian
way with distance from a point running with group velocity along a straight
line. The solutions are constructed using exact complex solutions of the
eikonal equation and may be regarded as ray solutions with amplitudes involving
one term. It is also shown that the multidimensional nonlinear Klein-Gordon
equation can be reduced to an ordinary differential equation with respect to
the complex eikonal.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:01:48 GMT"
}
] | 2009-11-08T00:00:00 | [
[
"Perel",
"M. V.",
""
],
[
"Fialkovsky",
"I. V.",
""
]
] | [
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711.4144 | Marta Asaeda | Marta Asaeda (UC Riverside), Seidai Yasuda (RIMS, Kyoto) | On Haagerup's list of potential principal graphs of subfactors | 19 pages | null | 10.1007/s00220-008-0588-0 | null | math.OA math.QA | null | We show that any graph, in the sequence given by Haagerup in 1991 as that of
candidates of principal graphs of subfactors, is not realized as a principal
graph except for the smallest two. This settles the remaining case of a
previous work of the first author.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:53:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Asaeda",
"Marta",
"",
"UC Riverside"
],
[
"Yasuda",
"Seidai",
"",
"RIMS, Kyoto"
]
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] |
711.4145 | Torsten Dahms | Torsten Dahms (for the PHENIX Collaboration) | Measurement of photons via conversion pairs in Au+Au collisions at
sqrt(s_NN) = 200 GeV with the PHENIX experiment at RHIC | 8 pages, 4 figures. To appear in the proceedings of the 23rd Winter
Workshop on Nuclear Dynamics, Big Sky (Montana), USA, 11-18 February 2007 | null | null | null | nucl-ex | null | Thermal photons can provide information on the temperature of the new state
of matter created at RHIC. In the p_T region of 1--3 GeV/c thermal photons are
expected to be the dominant direct photon source. Therefore, a possible excess
compared to a pure decay photon signal due to a thermal photon contribution
should be seen in the double ratio
(gamma/gamma(pi^0))_{Measured}/(gamma/gamma(pi^0))_{Simulated}, if sufficient
accuracy can be reached. We present a method to reconstruct direct photons by
measuring e^+e^- pairs from external photon conversions.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:21:23 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Dahms",
"Torsten",
"",
"for the PHENIX Collaboration"
]
] | [
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711.4146 | Apostolos Pilaftsis | Apostolos Pilaftsis | Comments on Spontaneous Spin-Statistics Violation by Fermion Condensates | 7 pages, major revision w.r.t. earlier versions | null | null | MAN-HEP/2007-28 | hep-ph | null | Scalar condensation, the well-established Higgs phenomenon, is the standard
paradigm for building up renormalizable gauge-invariant theories of massive
gauge bosons. In this short note, we demonstrate the uniqueness of the Higgs
vacuum state under the possible presence of fermion condensates in a
renormalizable U(1) model. In the same context, we explain why spontaneous
spin-statistics violation is technically not admitted in conventional Quantum
Field Theory.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:31:22 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 14:31:51 GMT"
},
{
"version": "v3",
"created": "Fri, 25 Jan 2008 17:59:22 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Pilaftsis",
"Apostolos",
""
]
] | [
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711.4147 | Mauro Napsuciale | S. Gomez-Avila, M. Napsuciale, E. Oset | \phi K^{+}K^{-} production in electron-positron annihilation | 21 pages, 17 figures. Revised version to appear in Phys. Rev. D.
Contributions of intermediate X(2175) included. Extraction of form factors
updated | Phys.Rev.D79:034018,2009 | 10.1103/PhysRevD.79.034018 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this work we study the e^{+}e^{-}\to\phi K^{+}K^{-} reaction. The leading
order electromagnetic contributions to this process involve the \gamma*\phi\
K^{+}K^{-} vertex function with a highly virtual photon. We calculate this
function at low energies using R\chi PT supplemented with the anomalous term
for the VV'P interactions. Tree level contributions involve the kaon form
factors and the K*K transition form factors. We improve this result, valid for
low photon virtualities, replacing the lowest order terms in the kaon form
factors and K*K transition form factors by the form factors as obtained in
U\chi PT in the former case and the ones extracted from recent data on
e^{+}e^{-}\to KK* in the latter case. We calculate rescattering effects which
involve meson-meson amplitudes. The corresponding result is improved using the
unitarized meson-meson amplitudes containing the scalar poles instead of the
lowest order terms. Using the BABAR value for BR(X\to \phi f_{0})\Gamma (X\to
e^{+} e^{-}), we calculate the contribution from intermediate X(2175). A good
description of data is obtained in the case of destructive interference between
this contribution and the previous ones, but more accurate data on the
isovector K*K transition form factor is required in order to exclude
contributions from an intermediate isovector resonance to e^{+}e^{-}\to \phi\
K^{+}K^{-} around 2.2 GeV.
| [
{
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{
"version": "v2",
"created": "Sat, 7 Feb 2009 00:21:20 GMT"
}
] | 2009-11-06T00:00:00 | [
[
"Gomez-Avila",
"S.",
""
],
[
"Napsuciale",
"M.",
""
],
[
"Oset",
"E.",
""
]
] | [
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711.4148 | Jeffrey Burdges | Jeffrey Burdges | Sylow 0-unipotent subgroups in groups of finite Morley rank | null | J. Group Theory 9 (2006) 467 | null | null | math.LO math.GR | null | One of the central tools in the classification of simple algebraic groups is
the distinction between semisimple subgroups and unipotent subgroups. It is not
a priori clear how to make this distinction for torsion-free subgroups of a
group of finite Morley rank. We exploit the ``graded'' notion of 0-unipotence
to develop a Sylow theory for torsion-free subgroups of a solvable group of
finite Morley rank. This Sylow theory provides a robust alternative to the
usual theory of Carter subgroups, and will be used in the analysis of
intersections of Borel subgroups in minimal simple groups.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:34:06 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Burdges",
"Jeffrey",
""
]
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] |
711.4149 | Todd Brun | Todd A. Brun, Lajos Diosi and Walter T. Strunz | Test of weak measurement on a two- or three-qubit computer | To appear in Physical Review A. Title changed. 6 pages in RevTeX
format | Phys. Rev. A 77, 032101 (2008) | 10.1103/PhysRevA.77.032101 | null | quant-ph | null | Current quantum computer technology is sufficient to realize weak
measurements and the corresponding concept of weak values. We demonstrate how
the weak value anomaly can be tested, along with consistency and simultaneity
of weak values, using only discrete degrees of freedom. All you need is a
quantum computer with two--or better, three--qubits. We also give an
interpretation of the weak value as an effective field strength in a
postselected spin measurement.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:38:05 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Feb 2008 07:06:33 GMT"
}
] | 2010-02-20T00:00:00 | [
[
"Brun",
"Todd A.",
""
],
[
"Diosi",
"Lajos",
""
],
[
"Strunz",
"Walter T.",
""
]
] | [
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] |
711.415 | Markus Kindermann | M. Kindermann | Nonequilibrium effective vector potential due to pseudospin exchange in
graphene | 4 pages, 2 figures | Phys. Rev. Lett. 101, 226809 (2008) | 10.1103/PhysRevLett.101.226809 | null | cond-mat.mes-hall | null | We show that exchange interactions in two-dimensional electron gases out of
equilibrium can generate a fictitious vector potential with intriguing
signatures in interference and Hall measurements. Detailed predictions are made
for graphene, where the effect is enhanced by pseudospin exchange.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:04:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kindermann",
"M.",
""
]
] | [
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] |
711.4151 | Matthias Beck | Matthias Beck, Christian Haase, and Steven V. Sam | Grid graphs, Gorenstein polytopes, and domino stackings | 14 pages, 6 figures, uses graphs package | Graphs Combin. 25 (2009), 409-426 | 10.1007/s00373-005-0858-y | null | math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We examine domino tilings of rectangular boards, which are in natural
bijection with perfect matchings of grid graphs. This leads to the study of
their associated perfect matching polytopes, and we present some of their
properties, in particular, when these polytopes are Gorenstein. We also
introduce the notion of domino stackings and present some results and several
open questions. Our techniques use results from graph theory, polyhedral
geometry, and enumerative combinatorics.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 23:54:24 GMT"
},
{
"version": "v2",
"created": "Tue, 28 Apr 2009 18:04:33 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Beck",
"Matthias",
""
],
[
"Haase",
"Christian",
""
],
[
"Sam",
"Steven V.",
""
]
] | [
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711.4152 | Jeffrey Burdges | Jeffrey Burdges | The Bender method in groups of finite Morley rank | null | J. Algebra 307 (2007) 704--726 | null | null | math.GR math.LO | null | Jaligot's Lemma states that the Fitting subgroups of distinct Borel subgroups
do not intersect in a tame minimal simple groups of finite Morley. Such a
strong result appears hopeless without tameness. Here we use the 0-unipotence
theory to build a toolkit for the analysis of nonabelian intersections of Borel
subgroups. As a demonstration, we show that any connected nilpotent subgroup of
an intersection of Borel subgroups, in a nontame minimal simple group, must
actually be abelian.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:01:49 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Burdges",
"Jeffrey",
""
]
] | [
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0.116326347
] |
711.4153 | Abbas Kenan Ciftci | A. K. Ciftci, R. Ciftci, S. Sultansoy | Anomalous Single Production of the Fourth Generation Neutrino at Future
ep Colliders | 11 pages, 6 figures, 5 tables | Phys.Lett.B660:534-538,2008 | 10.1016/j.physletb.2008.01.039 | null | hep-ph | null | Possible single productions of the fourth standard model generation neutrino
via anomalous interactions at the future ep colliders are studied. Signatures
of such anomalous processes and backgrounds are discussed in detail. Discovery
limits for neutrino mass and achievable values of anomalous coupling strength
are determined.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:07:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ciftci",
"A. K.",
""
],
[
"Ciftci",
"R.",
""
],
[
"Sultansoy",
"S.",
""
]
] | [
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711.4154 | Dietrich Belitz | Qi Li, John Toner, and D. Belitz | Skyrmion versus vortex flux lattices in p-wave superconductors | 13pp, 8 eps figs | Phys. Rev. B 79, 014517 (2009) | 10.1103/PhysRevB.79.014517 | null | cond-mat.supr-con | null | p-wave superconductors allow for topological defects known as skyrmions, in
addition to the usual vortices that are possible in both s-wave and p-wave
materials. In strongly type-II superconductors in a magnetic field, a skyrmion
flux lattice yields a lower free energy than the Abrikosov flux lattice of
vortices, and should thus be realized in p-wave superconductors. We
analytically calculate the energy per skyrmion, which agrees very well with
numerical results. From this, we obtain the magnetic induction B as a function
of the external magnetic field H, and the elastic constants of the skyrmion
lattice, near the lower critical field H_c1. Together with the Lindemann
criterion, these results suffice to predict the melting curve of the skyrmion
lattice. We find a striking difference in the melting curves of vortex lattices
and skyrmion lattices: while the former is separated at all temperatures from
the Meissner phase by a vortex liquid phase, the skyrmion lattice phase shares
a direct boundary with the Meissner phase. That is, skyrmions lattices never
melt near Hc1, while vortex lattices always melt sufficiently close to Hc1.
This allows for a very simple test for the existence of a skyrmion lattice.
Possible muSR experiments to detect skyrmion lattices are also discussed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:18:12 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"Li",
"Qi",
""
],
[
"Toner",
"John",
""
],
[
"Belitz",
"D.",
""
]
] | [
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711.4155 | Stathis Livadas | Stathis Livadas | The Expressional Limits of Formal Languages in the Notion of Observation | 20 pages | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this article I deal with the notion of observation in the most fundamental
sense and its representation by means of formal languages serving as
expressional tools of formal-axiomatical theories. In doing so, I have taken
this notion in two diverse contexts. In the first as an epistemic notion that
refers to its interpretation in a formal mathematical environment and then to
its interpretation in a quantum mechanical environment. The second context in
which I tried to approach the notion of observation is that of a
phenomenological constitution basically as it is described in E. Husserl's
original works. Assuming that in phenomenological constitution mathematical
objects are special cases of perceptual objects including consequently objects
of a quantum mechanical measurement, the question is to inquire on the limits
of their description in the language of a formal-axiomatical theory. On one
hand, I derive an irreducibility on the level of observables as indecomposable
atoms without any further syntactical content in formal representation and on
the other a transcendence of a continuous substratum self-constituted as a kind
of impredicative synthetic unity on which to define an observational frame and
generate a predicative universe of discourse.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:48:48 GMT"
},
{
"version": "v2",
"created": "Tue, 10 Feb 2009 16:43:39 GMT"
}
] | 2009-02-10T00:00:00 | [
[
"Livadas",
"Stathis",
""
]
] | [
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] |
711.4156 | Masashi Wakamatsu | M. Wakamatsu | Comparative Analysis of Transversities and Longitudinally Polarized
Distributions of the Nucleon | 9 pages; talk given at the 12th Workshop on High Energy Spin Physics
(DSPIN-07), Dubna, Russia, September 3 - 7, 2007 | null | null | OU-HET-591 | hep-ph hep-ex nucl-ex | null | We carry out a comparative analysis of the transversities and the
longitudinally polarized parton distribution functions in light of the first
empirical extraction of the transversity distributions recently done by
Anselmino et al. It is shown that the precise determination of the isoscalar
tensor charge, which is defined as the 1st moment of the isoscalar combination
of the transversity distributions, is of fundamental importance for clarifying
the internal spin structure function of the nucleon.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 00:55:12 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Wakamatsu",
"M.",
""
]
] | [
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] |
711.4157 | Xiaolin Li | Xiaolin Li, Xiaomin Tu, Sasa Zaric, Kevin Welsher, Won Seok Seo, Wei
Zhao, Hongjie Dai | Selective Synthesis Combined with Chemical Separation of Single-Walled
Carbon Nanotubes for Chirality Selection | 3 pages, 5 figures; Journal of the American Chemical Society, in
press, 2007 | null | null | null | cond-mat.mtrl-sci | null | Single-walled carbon nanotubes (SWNTs) are potential materials for future
nanoelectronics. Since the electronic and optical properties of SWNTs strongly
depend on tube diameter and chirality, obtaining SWNTs with narrow (n,m)
chirality distribution by selective growth or chemical separation has been an
active area of research. Here, we demonstrate that a new, bimetallic FeRu
catalyst affords SWNT growth with narrow diameter and chirality distribution in
methane CVD. At 600C, methane CVD on FeRu catalyst produced predominantly (6,5)
SWNTs according to Uv-vis-NIR absorption and photoluminescence
excitation/emission (PLE) spectroscopic characterization. At 850C, the dominant
semiconducting species produced are (8,4), (7,6) and (7,5) SWNTs, with much
narrower distributions in diameter and chirality than materials grown by other
catalysts. Further, we show that narrow-diameter/chirality growth combined with
chemical separation by ion exchange chromatography (IEC) greatly facilitate
achieving single-(m,n) SWNT samples, as demonstrated by obtaining highly
enriched (8,4) SWNTs with near elimination of metallic SWNTs existing in the
as-grown material.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:19:24 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Li",
"Xiaolin",
""
],
[
"Tu",
"Xiaomin",
""
],
[
"Zaric",
"Sasa",
""
],
[
"Welsher",
"Kevin",
""
],
[
"Seo",
"Won Seok",
""
],
[
"Zhao",
"Wei",
""
],
[
"Dai",
"Hongjie",
""
]
] | [
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] |
711.4158 | Christopher S. Reynolds | Christopher S. Reynolds (Maryland), Andrew C. Fabian (Cambridge) | Broad iron K-alpha emission lines as a diagnostic of black hole spin | 23 pages, 5 figures. Accepted for publication in the Astrophysical
Journal | null | 10.1086/527344 | null | astro-ph | null | We address the ability of broad iron emission lines from black hole accretion
disks to diagnose the spin of the black hole. Using a high-resolution
3-dimensional MHD simulation of a geometrically-thin accretion disk in a
Pseudo-Newtonian potential, we show that both the midplane density and the
vertical column density of the accretion flow drop dramatically over a narrow
range of radii close to the innermost stable circular orbit (ISCO). We argue
that this drop of density is accompanied by a sharp increase in the ionization
parameter of the X-ray photosphere, and that the resulting imprint of the ISCO
on the X-ray reflection spectrum can be used to constrain spin. Motivated by
this simulation, we construct a simplified toy-model of the accretion flow
within the ISCO of a Kerr black hole, and use this model to estimate the
systematic error on inferred black hole spin that may result from slight
bleeding of the iron line emission to the region inside of the ISCO. We find
that these systematic errors can be significant for slowly spinning black holes
but become appreciably smaller as one considers more rapidly rotating black
holes.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:21:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Reynolds",
"Christopher S.",
"",
"Maryland"
],
[
"Fabian",
"Andrew C.",
"",
"Cambridge"
]
] | [
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] |
711.4159 | Manas Kulkarni | M. Kulkarni, N. Seshadri, V. S. C. Manga Rao, S. Dutta Gupta | Control of superluminal transit through a heterogeneous medium | 21 Pages,5 Figures (Published in Journal of Modern Optics) | Journal of Modern Optics, 10 March 2004, Vol 51, No. 4, 549-557 | 10.1080/09500340408238067 | null | physics.optics | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider pulse propagation through a two component composite medium (metal
inclusions in a dielectric host) with or without cavity mirrors. We show that a
very thin slab of such a medium, under conditions of localized plasmon
resonance, can lead to significant superluminality with detectable levels of
transmitted pulse. A cavity containing the heterogeneous medium is shown to
lead to subluminal-to-superluminal transmission depending on the volume
fraction of the metal inclusions. The predictions of phase time calculations
are verified by explicit calculations of the transmitted pulse shapes. We also
demonstrate the independence of the phase time on system width and the volume
fraction under specific conditions.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:29:30 GMT"
},
{
"version": "v2",
"created": "Wed, 6 May 2009 21:48:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kulkarni",
"M.",
""
],
[
"Seshadri",
"N.",
""
],
[
"Rao",
"V. S. C. Manga",
""
],
[
"Gupta",
"S. Dutta",
""
]
] | [
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] |
711.416 | Lun Lv | Lun Lv, Guoce Xin, and Yue Zhou | Two Coefficients of the Dyson Product | 11 pages | null | null | null | math.CO math.AC | null | In this paper, the closed-form expressions for the coefficients of
$\frac{x_r^2}{x_s^2}$ and $\frac{x_r^2}{x_sx_t}$ in the Dyson product are found
by applying an extension of Good's idea. As onsequences, we find several
interesting Dyson style constant term identities.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:31:47 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Lv",
"Lun",
""
],
[
"Xin",
"Guoce",
""
],
[
"Zhou",
"Yue",
""
]
] | [
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] |
711.4161 | Ruiming Zhang Dr. | Ruiming Zhang | Scaled Asymptotics For Some $q$-Series As $q$ Approaching Unit | 16 | null | null | null | math.CA | null | In this work we investigate Plancherel-Rotach type asymptotics for some
$q$-series as $q\to1$. These $q$-series generalize Ramanujan function
$A_{q}(z)$; Jackson's $q$-Bessel function $J_{\nu}^{(2)}$(z;q), Ismail-Masson
orthogonal polynomials($q^{-1}$-Hermite polynomials) $h_{n}(x|q)$,
Stieltjes-Wigert orthogonal polynomials $S_{n}(x;q)$, $q$-Laguerre orthogonal
polynomials $L_{n}^{(\alpha)}(x;q)$ and confluent basic hypergeometric series.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:32:31 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Zhang",
"Ruiming",
""
]
] | [
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] |
711.4162 | Mauro Napsuciale | M. Napsuciale, S. Rodriguez, E. G. Delgado-Acosta, M.Kirchbach | Electromagnetic couplings of elementary vector particles | 10 pages, 2 figures, contributed to the XI Mexican Workshop on
Particles and Fields. Accepted in Phys. Rev. D | Phys.Rev.D77:014009,2008 | 10.1103/PhysRevD.77.014009 | null | hep-ph | null | On the basis of the three fundamental principles of (i) Poincar\'{e} symmetry
of space time, (ii) electromagnetic gauge symmetry, and (iii) unitarity, we
construct an universal Lagrangian for the electromagnetic interactions of
elementary vector particles, i.e., massive spin-1 particles transforming in the
/1/2,1/2) representation space of the Homogeneous Lorentz Group (HLG). We make
the point that the first two symmetries alone do not fix the electromagnetic
couplings uniquely but solely prescribe a general Lagrangian depending on two
free parameters, here denoted by \xi and g. The first one defines the
electric-dipole and the magnetic-quadrupole moments of the vector particle,
while the second determines its magnetic-dipole and electric-quadrupole
moments. In order to fix the parameters one needs an additional physical input
suited for the implementation of the third principle. As such, one chooses
Compton scattering off a vector target and requires the cross section to
respect the unitarity bounds in the high energy limit. In result, we obtain the
universal g=2, and \xi=0 values which completely characterize the
electromagnetic couplings of the considered elementary vector field at tree
level. The nature of this vector particle, Abelian versus non-Abelian, does not
affect this structure. Merely, a partition of the g=2 value into non-Abelian,
g_{na}, and Abelian, g_{a}=2-g_{na}, contributions occurs for non-Abelian
fields with the size of g_{na} being determined by the specific non-Abelian
group appearing in the theory of interest, be it the Standard Model or any
other theory.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:51:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Napsuciale",
"M.",
""
],
[
"Rodriguez",
"S.",
""
],
[
"Delgado-Acosta",
"E. G.",
""
],
[
"Kirchbach",
"M.",
""
]
] | [
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] |
711.4163 | Zhi-Zhong Xing | Zhi-zhong Xing | Neutrino telescopes as a probe of active and sterile neutrino mixings | 6 pages. Plenary talk given at the XIV International Symposium on
Very High Energy Cosmic Ray Interactions, Weihai, China, August 15-22, 2006 | Nucl.Phys.Proc.Suppl.175-176:421-426,2008 | 10.1016/j.nuclphysbps.2007.11.043 | null | astro-ph | null | If the ultrahigh-energy (UHE) neutrino fluxes produced from a distant
astrophysical source can be measured at a km^3-size neutrino telescope, they
will provide a promising way to help determine the flavor mixing pattern of
three active neutrinos. Considering the conventional UHE neutrino source with
the flavor ratio \phi_e : \phi_\mu : \phi_\tau = 1 : 2 : 0, I show that
\phi^D_e : \phi^D_\mu : \phi^D_\tau = (1 -2 \Delta) : (1 +\Delta) : (1 +\Delta)
holds at the detector of a neutrino telescope, where \Delta characterizes the
effect of \mu-\tau symmetry breaking (i.e., \theta_13 \neq 0 and \theta_23 \neq
\pi/4). Current experimental data yield -0.1 \leq \Delta \leq +0.1. It is also
possible to probe \Delta by detecting the \bar{\nu}_e flux of E_\bar{\nu}_e
\approx 6.3 PeV via the Glashow resonance channel \bar{\nu}_e e \to W^- \to
anything. Finally, I give some brief comments on the possibility to constrain
the mixing between active and sterile neutrinos by using the UHE neutrino
telescopes.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:51:39 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Xing",
"Zhi-zhong",
""
]
] | [
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711.4164 | Jonathan Seale | Jonathan P. Seale, Leslie W. Looney | Morphological Evolution of Outflows from YSOs | Accepted to Astrophysical Journal | null | null | null | astro-ph | null | We present Spitzer IRAC images that indicate the presence of cavities cut
into the dense outer envelope surrounding very young pre-main sequence stars.
These young stellar objects (YSOs) characterized by an outflow represent the
earliest stages of star formation. Mid-infrared photons thermally created by
the central protostar/disk are scattered by dust particles within the outflow
cavity itself into the line of sight. We observed this scattered light from 27
nearby, cavity-resolved YSOs, and quantified the shape of the outflow cavities.
Using the grid models of Robitaille et al. (2006), we matched model spectral
energy distributions (SEDs) to the observed SEDs of the 27 cataloged YSOs using
photometry from IRAC, MIPS, and IRAS. This allows for the estimation of
geometric and physical properties such as inclination angle, cavity density,
and accretion rate. By using the relative parameter estimates determined by the
models, we are able to deduce an evolutionary picture for outflows. Our work
supports the concept that cavities widen with time, beginning as a thin
jet-like outflow that widens to reveal the central protostar and disk until the
protostellar envelope is completely dispersed by outflow and accretion.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 03:47:01 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Seale",
"Jonathan P.",
""
],
[
"Looney",
"Leslie W.",
""
]
] | [
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] |
711.4165 | Jeffrey Burdges | Jeffrey Burdges and Gregory Cherlin and Eric Jaligot | Minimal connected simple groups of finite Morley rank with strongly
embedded subgroups | null | J. Algebra 314 (2007) 581--612 | null | null | math.GR math.LO | null | We show that a minimal nonalgebraic simple groups of finite Morley rank has
Prufer rank at most 2, and eliminates tameness from Cherlin and Jaligot's past
work on minimal simple groups. The argument given here begins with the strongly
embedded minimal simple configuration of Borovik, Burdges and Nesin. The
0-unipotence machinery of Burdges's thesis is used to analyze configurations
involving nonabelian intersections of Borel subgroups. The number theoretic
punchline of Cherlin and Jaligot has been replaced with a new genericity
argument.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:49:33 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Burdges",
"Jeffrey",
""
],
[
"Cherlin",
"Gregory",
""
],
[
"Jaligot",
"Eric",
""
]
] | [
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] |
711.4166 | Jeffrey Burdges | Alexandre Borovik, Jeffrey Burdges and Gregory Cherlin | Involutions in groups of finite Morley rank of degenerate type | null | Selecta Methematica 13 (2007) 1-22 | null | null | math.LO | null | This article proves a version of the Feit-Thompson theorem for simple groups
of finite Morley rank: a connected groups of finite Morley rank with a finite
Sylow 2-subgroup has a trivial Sylow 2-subgroups.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 02:03:27 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Borovik",
"Alexandre",
""
],
[
"Burdges",
"Jeffrey",
""
],
[
"Cherlin",
"Gregory",
""
]
] | [
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] |
711.4167 | Jeffrey Burdges | Alexandre Borovik, Jeffrey Burdges and Ali Nesin | Uniqueness cases in odd type groups of finite Morley rank | null | null | 10.1112/jlms/jdm106 | null | math.GR math.LO | null | Here we analyze a proper 2-generated core in a minimal counter example to the
Cherlin-Zilber Algebraicity Conjecture for simple groups of finite Morley rank.
We ultimately show that such a group is strongly embedded and the ambiant group
is minimal connected simple.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 02:07:55 GMT"
}
] | 2014-02-26T00:00:00 | [
[
"Borovik",
"Alexandre",
""
],
[
"Burdges",
"Jeffrey",
""
],
[
"Nesin",
"Ali",
""
]
] | [
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] |
711.4168 | Tao Zhou | Tao Zhou, Hoang Anh Tuan Kiet, Beom Jun Kim, Bing-Hong Wang, and
Petter Holme | Role of Activity in Human Dynamics | 5 pages, 6 figures. Accepted by EPL | EPL 82 (2008) 28002 | 10.1209/0295-5075/82/28002 | null | physics.soc-ph physics.data-an | null | The human society is a very complex system; still, there are several
non-trivial, general features. One type of them is the presence of power-law
distributed quantities in temporal statistics. In this Letter, we focus on the
origin of power-laws in rating of movies. We present a systematic empirical
exploration of the time between two consecutive ratings of movies (the
interevent time). At an aggregate level, we find a monotonous relation between
the activity of individuals and the power-law exponent of the interevent-time
distribution. At an individual level, we observe a heavy-tailed distribution
for each user, as well as a negative correlation between the activity and the
width of the distribution. We support these findings by a similar data set from
mobile phone text-message communication. Our results demonstrate a significant
role of the activity of individuals on the society-level patterns of human
behavior. We believe this is a common character in the interest-driven human
dynamics, corresponding to (but different from) the universality classes of
task-driven dynamics.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 02:09:16 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 17:56:34 GMT"
},
{
"version": "v3",
"created": "Wed, 20 Feb 2008 05:41:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zhou",
"Tao",
""
],
[
"Kiet",
"Hoang Anh Tuan",
""
],
[
"Kim",
"Beom Jun",
""
],
[
"Wang",
"Bing-Hong",
""
],
[
"Holme",
"Petter",
""
]
] | [
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] |
711.4169 | Jeffrey Burdges | Alexandre Borovik and Jeffrey Burdges | A New Trichotomy Theorem | null | null | null | null | math.GR math.LO | null | We show that a minimal counter example to the Cherlin-Zilber Algebraicity
Conjecture for simple groups of finite Morley rank has normal 2-rank at most
two, which is a tameness free version of Borovik's original trichotomy theorem.
This result serves as a bridge by showing that there are no groups found
strictly between the generic and quasithin cases, i.e. between groups of Lie
rank at least three, and groups of Lie rank one and two. Again this result
depends upon previous work for the uniqueness case analysis.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 02:18:00 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Borovik",
"Alexandre",
""
],
[
"Burdges",
"Jeffrey",
""
]
] | [
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] |
711.417 | Paulo F. Farinas | Paulo F. Farinas | Nonequilibrium interacting electrons in a ferromagnet | 4 pages, no figures, revised version, accepted for publication in the
PRB's Rapid Communication section | null | 10.1103/PhysRevB.77.020410 | null | cond-mat.str-el | null | Dynamics of the magnetization in ferromagnets is examined in the presence of
transport electrons allowing the latter to interact. It is found that the
existence of inhomogeneities such as domain wall (DW) structures, leads to
changes that affect the dynamical structure of the equations of motion for the
magnetization. Only in the limit of uniform magnetizations or sufficiently wide
DW's, the equations of motion maintain the form they have in the noninteracting
case. In this limit, results like the spin torques, the Gilbert parameter, and
the DW velocities become renormalized. However the length scale that defines
such a limit depends on the strength of the interaction. It is shown that if
large ferromagnetic fluctuations exist in the metallic band then the range for
which conformity with the noninteracting case holds extends to the limit of
arbitrarily narrow DW's.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 02:19:10 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Dec 2007 16:52:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Farinas",
"Paulo F.",
""
]
] | [
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711.4171 | Zdenka Misanovic | Zdenka Misanovic, George Pavlov, and Gordon Garmire | Chandra observations of the pulsar PSR B1929+10 and its environment | 14 pages, 12 figures and 2 tables; accepted by ApJ; version with
low-resolution figures | Astrophys.J.685:1129-1142,2008 | 10.1086/590949 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report on two Chandra observations of the 3-Myr pulsar B1929+10, which
reveal a faint compact (~9"x5") nebula elongated in the direction perpendicular
to the pulsar's proper motion, two patchy wings, and a possible short (~3") jet
emerging from the pulsar. In addition, we detect a tail extending up to at
least 4' in the direction opposite to the pulsar's proper motion, aligned with
the 15'-long tail detected in ROSAT and XMM-Newton observations. The overall
morphology of the nebula suggests that the shocked pulsar wind is confined by
the ram pressure due to the pulsar's supersonic speed. The shape of the compact
nebula in the immediate vicinity of the pulsar seems to be consistent with the
current MHD models. However, since these models do not account yet for the
change of the flow velocity at larger distances from the pulsar, they are not
able to constrain the extent of the long pulsar tail. The luminosity of the
whole nebula as seen by Chandra is ~10^30 ergs/s in the 0.3-8 keV band, for the
distance of 361 pc. Using the Chandra and XMM-Newton data, we found that the
pulsar spectrum is comprised of non-thermal (magnetospheric) and thermal
components. The non-thermal component can be described by a power-law model
with photon index ~1.7 and luminosity 1.7x10^30 ergs/s in the 0.3-10 keV band.
The blackbody fit for the thermal component, which presumably emerges from hot
polar caps, gives the temperature kT~0.3 keV and projected emitting area 3x10^3
m^2, corresponding to the bolometric luminosity ~(1-2)x10^30 ergs/s.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 05:42:23 GMT"
},
{
"version": "v2",
"created": "Fri, 12 Sep 2008 05:51:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Misanovic",
"Zdenka",
""
],
[
"Pavlov",
"George",
""
],
[
"Garmire",
"Gordon",
""
]
] | [
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] |
711.4172 | Michael Vanner | M. R. Vanner, R. J. McLean, A. I. Sidorov, P. Hannaford and A. M.
Akulshin | Broadband optical delay with large dynamic range using atomic dispersion | 8 pages, 5 figures | J. Phys. B: At. Mol. Opt. Phys. 41 051004 (2008) | 10.1088/0953-4075/41/5/051004 | null | physics.optics | null | We report on a tunable all-optical delay line for pulses with optical
frequency within the Rb $D_2$ absorption line. Using frequency tuning between
absorption components from different isotopes, pulses of 10 ns duration are
delayed in a 10 cm hot vapour cell by up to 40 ns while the transmission
remains above 10%. The use of two isotopes allows the delay to be increased or
decreased by optical pumping with a second laser, producing rapid tuning over a
range of more than 40% of the initial delay at 110$^{\circ}$C. We investigate
the frequency and intensity ranges in which this delay line can be realised.
Our observations are in good agreement with a numerical model of the system.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 02:44:55 GMT"
},
{
"version": "v2",
"created": "Sat, 26 Apr 2008 13:47:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vanner",
"M. R.",
""
],
[
"McLean",
"R. J.",
""
],
[
"Sidorov",
"A. I.",
""
],
[
"Hannaford",
"P.",
""
],
[
"Akulshin",
"A. M.",
""
]
] | [
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] |
711.4173 | Jun Fang | Jun Fang, Li Zhang | Non-thermal emission from old supernova remnants | 11 pages, 7 figures, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2007.12766.x | null | astro-ph | null | We study the non-thermal emission from old shell-type supernova remnants
(SNRs) on the frame of a time-dependent model. In this model, the
time-dependent non-thermal spectra of both primary electrons and protons as
well as secondary electron/positron ($e^{\pm}$) pairs can be calculated
numerically by taking into account the evolution of the secondary $e^{\pm}$
pairs produced from proton-proton (p-p) interactions due to the accelerated
protons collide with the ambient matter in an SNR. The multi-wavelength photon
spectrum for a given SNR can be produced through leptonic processes such as
electron/positron synchrotron radiation, bremsstrahlung and inverse Compton
scattering as well as hadronic interaction. Our results indicate that the
non-thermal emission of the secondary $e^{\pm}$ pairs is becoming more and more
prominent when the SNR ages in the radiative phase because the source of the
primary electrons has been cut off and the electron synchrotron energy loss is
significant for a radiative SNR, whereas the secondary $e^{\pm}$ pairs can be
produced continuously for a long time in the phase due to the large energy loss
time for the p-p interaction. We apply the model to two old SNRs, G8.7$-$0.1
and G23.3$-$0.3, and the predicted results can explain the observed
multi-wavelength photon spectra for the two sources.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 04:17:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fang",
"Jun",
""
],
[
"Zhang",
"Li",
""
]
] | [
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711.4174 | Veer Awana Dr | Arpita Vajpayee, V.P.S. Awana*, H. Kishan (NPL, New Delhi, India),
A.V. Narlikar (IUC, India), G.L. Bhalla (Univ. Delhi, India), and X.L. Wang
(ISEM, UOW, Australia) | High Field Performance of Nano-Diamond Doped MgB2 Superconductor | 12 PAGES (TEXT+FIGS). ACCEPTED: J. APPL.PHYS. (MMM-2007 Proceedings) | null | 10.1063/1.2831778 | null | cond-mat.supr-con | null | Polycrystalline MgB2-nDx (x= 0 to 0.1) samples are synthesized by solid-state
route with ingredients of Mg, B and n-Diamond. The results from
magneto-transport and magnetization of nano-diamond doped MgB2-nDx are
reported. Superconducting transition temperature (Tc) is not affected
significantly by x up to x = 0.05 and latter decreases slightly for higher x >
0.05. R(T) vs H measurements show higher Tc values under same applied magnetic
fields for the nano-diamond added samples, resulting in higher estimated Hc2
values. From the magnetization measurements it was found that irreversibility
field value Hirr for the pristine sample is 7.5 Tesla at 4 K and the same is
increased to 13.5 Tesla for 3-wt% nD added sample at the same temperature. The
Jc(H) plots at all temperatures show that Jc value is lowest at all applied
fields for pristine MgB2 and the sample doped with 3-wt% nD gives the best Jc
values at all fields. For the pure sample the value of Jc is of the order of
105 A/cm2 at lower fields but it decreases very fast as the magnetic field is
applied and becomes negligible above 7 Tesla. The Jc is 40 times higher than
pure MgB2 at 10 K at 6 Tesla field in case of 3%nD doped sample and its value
is still of the order of 103 A/cm2 at 10 Tesla for the same sample. On the
other hand at 20K the 5%nD sample shows the best performance at higher fields.
These results are discussed in terms of extrinsic pinning due to dispersed
n-Diamond in the host MgB2 matrix along with the intrinsic pinning due to
possible substitution of C at Boron site and increased inter-band scattering
for highly doped samples resulting in extraordinary performance of the doped
system.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 03:23:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vajpayee",
"Arpita",
"",
"NPL, New Delhi, India"
],
[
"Awana*",
"V. P. S.",
"",
"NPL, New Delhi, India"
],
[
"Kishan",
"H.",
"",
"NPL, New Delhi, India"
],
[
"Narlikar",
"A. V.",
"",
"IUC, India"
],
[
"Bhalla",
"G. L.",
"",
"Univ. Delhi, India"
],
[
"Wang",
"X. L.",
"",
"ISEM, UOW, Australia"
]
] | [
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711.4175 | Soren Riis | Soren Riis | Graph Entropy, Network Coding and Guessing games | 30 pages, 3 figures | null | null | null | math.CO cs.IT math.IT | null | We introduce the (private) entropy of a directed graph (in a new network
coding sense) as well as a number of related concepts. We show that the entropy
of a directed graph is identical to its guessing number and can be bounded from
below with the number of vertices minus the size of the graph's shortest index
code. We show that the Network Coding solvability of each specific multiple
unicast network is completely determined by the entropy (as well as by the
shortest index code) of the directed graph that occur by identifying each
source node with each corresponding target node.
Shannon's information inequalities can be used to calculate upper bounds on a
graph's entropy as well as calculating the size of the minimal index code.
Recently, a number of new families of so-called non-shannon-type information
inequalities have been discovered. It has been shown that there exist
communication networks with a capacity strictly less than required for
solvability, but where this fact cannot be derived using Shannon's classical
information inequalities. Based on this result we show that there exist graphs
with an entropy that cannot be calculated using only Shannon's classical
information inequalities, and show that better estimate can be obtained by use
of certain non-shannon-type information inequalities.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 03:32:55 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Riis",
"Soren",
""
]
] | [
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] |
711.4176 | Daniel Kosov | M. F. Gelin and D. S. Kosov | A unified approach to the derivation of work theorems for equilibrium
and steady-state, classical and quantum Hamiltonian systems | null | Phys. Rev. E 78, 011116 (2008) | 10.1103/PhysRevE.78.011116 | null | cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a unified and simple method for deriving work theorems for
classical and quantum Hamiltonian systems, both under equilibrium conditions
and in a steady state. Throughout the paper, we adopt the partitioning of the
total Hamiltonian into the system part, the bath part, and their coupling. We
rederive many equalities which are available in the literature and obtain a
number of new equalities for nonequilibrium classical and quantum systems. Our
results can be useful for determining partition functions and (generalized)
free energies through simulations and/or measurements performed on
nonequilibrium systems.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 04:06:22 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jul 2008 02:34:45 GMT"
}
] | 2008-07-30T00:00:00 | [
[
"Gelin",
"M. F.",
""
],
[
"Kosov",
"D. S.",
""
]
] | [
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] |
711.4177 | Ryosuke Shimizu | Ryosuke Shimizu, Takashi Yamaguchi, Yasuyoshi Mitsumori, Hideo Kosaka,
Keiichi Edamatsu | Generation of polarization entanglement from spatially-correlated
photons in spontaneous parametric down-conversion | 4 pages, 4 figures | null | 10.1103/PhysRevA.77.032338 | null | quant-ph | null | We propose a novel scheme to generate polarization entanglement from
spatially-correlated photon pairs. We experimentally realized a scheme by means
of a spatial correlation effect in a spontaneous parametric down-conversion and
a modified Michelson interferometer. The scheme we propose in this paper can be
interpreted as a conversion process from spatial correlation to polarization
entanglement.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:39:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shimizu",
"Ryosuke",
""
],
[
"Yamaguchi",
"Takashi",
""
],
[
"Mitsumori",
"Yasuyoshi",
""
],
[
"Kosaka",
"Hideo",
""
],
[
"Edamatsu",
"Keiichi",
""
]
] | [
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] |
711.4178 | Nobuyuki Kanematsu Ph.D. | Nobuyuki Kanematsu, Shunsuke Yonai, Azusa Ishizaki, Masami Torikoshi | Computational modeling of beam-customization devices for
heavy-charged-particle radiotherapy | 16 pages, 5 figures | Phys Med Biol. 2008 May 21;53(12):3113-3127 | 10.1088/0031-9155/53/12/003 | PMID: 18495975 | physics.med-ph | null | A model for beam customization with collimators and a range-compensating
filter based on the phase-space theory for beam transport is presented for dose
distribution calculation in treatment planning of radiotherapy with protons and
heavier ions. Independent handling of pencil beams in conventional pencil-beam
algorithms causes unphysical collimator-height dependence in the middle of
large fields, which is resolved by the framework comprised of generation,
transport, collimation, regeneration, range-compensation, and edge-sharpening
processes with a matrix of pencil beams. The model was verified to be
consistent with measurement and analytic estimation at a submillimeter level in
penumbra of individual collimators with a combinational-collimated carbon-ion
beam. The model computation is fast, accurate, and readily applicable to
pencil-beam algorithms in treatment planning with capability of combinational
collimation to make best use of the beam-customization devices.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 04:46:58 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Apr 2008 02:49:29 GMT"
}
] | 2008-05-27T00:00:00 | [
[
"Kanematsu",
"Nobuyuki",
""
],
[
"Yonai",
"Shunsuke",
""
],
[
"Ishizaki",
"Azusa",
""
],
[
"Torikoshi",
"Masami",
""
]
] | [
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] |
711.4179 | Alexander Olshevsky | Angelia Nedi\'c, Alex Olshevsky, Asuman Ozdaglar, John Tsitsiklis | On Distributed Averaging Algorithms and Quantization Effects | null | null | null | null | math.OC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider distributed iterative algorithms for the averaging problem over
time-varying topologies. Our focus is on the convergence time of such
algorithms when complete (unquantized) information is available, and on the
degradation of performance when only quantized information is available. We
study a large and natural class of averaging algorithms, which includes the
vast majority of algorithms proposed to date, and provide tight polynomial
bounds on their convergence time. We also describe an algorithm within this
class whose convergence time is the best among currently available averaging
algorithms for time-varying topologies. We then propose and analyze distributed
averaging algorithms under the additional constraint that agents can only store
and communicate quantized information, so that they can only converge to the
average of the initial values of the agents within some error. We establish
bounds on the error and tight bounds on the convergence time, as a function of
the number of quantization levels.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 04:55:51 GMT"
},
{
"version": "v2",
"created": "Wed, 14 Jan 2009 21:56:08 GMT"
}
] | 2009-01-14T00:00:00 | [
[
"Nedić",
"Angelia",
""
],
[
"Olshevsky",
"Alex",
""
],
[
"Ozdaglar",
"Asuman",
""
],
[
"Tsitsiklis",
"John",
""
]
] | [
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] |
711.418 | G. S. Asanov | G.S. Asanov | Finsleroid-regular space developed. Berwald case | null | null | 10.1016/S0034-4877(08)80037-7 | null | math.DG math-ph math.MP | null | The Finsleroid--Finsler space becomes regular when the norm $||b||=c$ of the
input 1-form $b$ is taken to be an arbitrary positive scalar $c(x) < 1$. By
performing required direct evaluations, the respective spray coefficients have
been obtained in a simple and transparent form. The adequate continuation into
the regular pseudo-Finsleroid domain has been indicated. The Finsleroid-regular
Berwald space is found under the assumptions that the Finsleroid charge is a
constant and the 1-form $b$ is parallel.
Keywords: Finsler metrics, spray coefficients, curvature tensors.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 05:26:41 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Asanov",
"G. S.",
""
]
] | [
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711.4181 | Fulvio Melia | Fulvio Melia | The Cosmic Horizon | Accepted for publication in MNRAS | Mon.Not.Roy.Astron.Soc.382:1917-1921,2008 | 10.1111/j.1365-2966.2007.12499.x | null | astro-ph gr-qc hep-ph hep-th math-ph math.MP | null | The cosmological principle, promoting the view that the universe is
homogeneous and isotropic, is embodied within the mathematical structure of the
Robertson-Walker (RW) metric. The equations derived from an application of this
metric to the Einstein Field Equations describe the expansion of the universe
in terms of comoving coordinates, from which physical distances may be derived
using a time-dependent expansion factor. These coordinates, however, do not
explicitly reveal properties of the cosmic spacetime manifested in Birkhoff's
theorem and its corollary. In this paper, we compare two forms of the
metric--written in (the traditional) comoving coordinates, and a set of
observer-dependent coordinates--first for the well-known de Sitter universe
containing only dark energy, and then for a newly derived form of the RW
metric, for a universe with dark energy and matter. We show that Rindler's
event horizon--evident in the co-moving system--coincides with what one might
call the "curvature horizon" appearing in the observer-dependent frame. The
advantage of this dual prescription of the cosmic spacetime is that with the
latest WMAP results, we now have a much better determination of the universe's
mass-energy content, which permits us to calculate this curvature with
unprecedented accuracy. We use it here to demonstrate that our observations
have probed the limit beyond which the cosmic curvature prevents any signal
from having ever reached us. In the case of de Sitter, where the mass-energy
density is a constant, this limit is fixed for all time. For a universe with a
changing density, this horizon expands until de Sitter is reached
asymptotically, and then it too ceases to change.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 05:28:46 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Melia",
"Fulvio",
""
]
] | [
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] |
711.4182 | Sachindra Naik | Sachindra Naik (1), Tadayasu Dotani (1, 2, 3), Nobuyuki Kawai (3),
Motohide Kokubun (1), Takayasu Anada (1), Mikio Morii (4), Tatehiro Mihara
(5), Teruaki Enoto (6), Madoka Kawaharada (6), Toshio Murakami (7), Yujin E.
Nakagawa (8), Hiromitsu Takahashi (9), Yukikatsu Terada (5), Atsumasa Yoshida
(8) ((1) ISAS/JAXA, Japan, (2) Space and Astronautical Science, School of
Physical Sciences, The Graduate University for Advanced Studies, 3-1-1
Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan, (3) Department of Physics,
Tokyo Institute of Technology, Tokyo, Japan, (4) Rikkyo University, Tokyo,
Japan, (5) RIKEN, Japan, (6) University of Tokyo, Japan, (7) Kanazawa
University, Kanazawa, Japan, (8) Aoyama Gakuin University, Sagamihara,
Kanagawa, Japan, (9) Hiroshima University, Japan) | Suzaku Observation of the Anomalous X-ray Pulsar CXOU J164710.2--455216 | 16 pages, 9 figures, Accepted for publication in Publications of the
Astronomical Society of Japan (PASJ) | 2008, PASJ, 60, 237 | 10.1093/pasj/60.2.237 | null | astro-ph | null | Suzaku TOO observation of the anomalous X-ray pulsar CXOU J164710.2-455216
was performed on 2006 September 23--24 for a net exposure of 38.8 ks. During
the observation, the XIS was operated in 1/8 window option to achieve a time
resolution of 1 s. Pulsations are clearly detected in the XIS light curves with
a barycenter corrected pulse period of 10.61063(2) s. The XIS pulse profile
shows 3 peaks of different amplitudes with RMS fractional amplitude of ~11% in
0.2--6.0 keV energy band. Though the source was observed with the HXD of
Suzaku, the data is highly contaminated by the nearby bright X-ray source GX
340+0 which was in the HXD field of view. The 1-10 keV XIS spectra are well
fitted by two blackbody components. The temperatures of two blackbody
components are found to be 0.61+/-0.01 keV and 1.22+/-0.06 keV and the value of
the absorption column density is 1.73+/-0.03 x 10^{22} atoms cm^{-2}. The
observed source flux in 1-10 keV energy range is calculated to be 2.6 x
10^{-11} ergs cm^{-2} s^{-1} with significant contribution from the soft
blackbody component (kT = 0.61 keV). Pulse phase resolved spectroscopy of XIS
data shows that the flux of the soft blackbody component consists of three
narrow peaks, whereas the flux of the other component shows a single peak over
the pulse period of the AXP. The blackbody radii changes between 2.2-2.7 km and
0.28-0.38 km (assuming the source distance to be 5 kpc) over pulse phases for
the soft and hard components, respectively. The details of the results obtained
from the timing and spectral analysis is presented.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 06:14:26 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Naik",
"Sachindra",
""
],
[
"Dotani",
"Tadayasu",
""
],
[
"Kawai",
"Nobuyuki",
""
],
[
"Kokubun",
"Motohide",
""
],
[
"Anada",
"Takayasu",
""
],
[
"Morii",
"Mikio",
""
],
[
"Mihara",
"Tatehiro",
""
],
[
"Enoto",
"Teruaki",
""
],
[
"Kawaharada",
"Madoka",
""
],
[
"Murakami",
"Toshio",
""
],
[
"Nakagawa",
"Yujin E.",
""
],
[
"Takahashi",
"Hiromitsu",
""
],
[
"Terada",
"Yukikatsu",
""
],
[
"Yoshida",
"Atsumasa",
""
]
] | [
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] |
711.4183 | Clayton Bjorland | Clayton Bjorland and Maria E. Schonbek | Existence and Stability of Steady-State Solutions with Finite Energy for
the Navier-Stokes equation in the Whole Space | 22 pages, submitted | null | null | null | math.AP | null | We consider the steady-state Navier-Stokes equation in the whole space
$\mathbb{R}^3$ driven by a forcing function $f$. The class of source functions
$f$ under consideration yield the existence of at least one solution with
finite Dirichlet integral ($\|\nabla U\|_2<\infty$). Under the additional
assumptions that $f$ is absent of low modes and the ratio of $f$ to viscosity
is sufficiently small in a natural norm we construct solutions which have
finite energy (finite $L^2$ norm). These solutions are unique among all
solutions with finite energy and finite Dirichlet integral. The constructed
solutions are also shown to be stable in the following sense: If $U$ is such a
solution then any viscous, incompressible flow in the whole space, driven by
$f$ and starting with finite energy, will return to $U$.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 05:48:56 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 05:06:39 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Bjorland",
"Clayton",
""
],
[
"Schonbek",
"Maria E.",
""
]
] | [
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711.4184 | Hideo Kodama | Hideo Kodama (KEK) | Superradiance and Instability of Black Holes | References added. 13 pages, 3 figures. A talk given at ICGA8 to be
published in Prog. Theor. Phys. Supplement | Prog.Theor.Phys.Suppl.172:11-20,2008 | 10.1143/PTPS.172.11 | null | hep-th gr-qc | null | We discuss the relation between the superradiance phenomenon and the
instability of rotating black holes in higher dimensions. In particular, we
point out that the superradiant instability of a massless scalar field around a
simply rotating Kerr-adS black hole implies the gravitational instability of
that black hole for tensor-type perturbations.
| [
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{
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] | 2008-11-26T00:00:00 | [
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"Kodama",
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711.4185 | Reiho Sakamoto | Reiho Sakamoto | Kirillov--Schilling--Shimozono bijection as energy functions of crystals | 31 pages, final version, expositions much detailed | International Mathematics Research Notices (2009) 2009: 579-614 | 10.1093/imrn/rnn140 | null | math.QA math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Kirillov--Schilling--Shimozono (KSS) bijection appearing in theory of the
Fermionic formula gives an one to one correspondence between the set of
elements of tensor products of the Kirillov--Reshetikhin crystals (called
paths) and the set of rigged configurations. It is a generalization of
Kerov--Kirillov--Reshetikhin bijection and plays inverse scattering formalism
for the box-ball systems. In this paper, we give an algebraic reformulation of
the KSS map from the paths to rigged configurations, using the combinatorial R
and energy functions of crystals. It gives a characterization of the KSS
bijection as an intrinsic property of tensor products of crystals.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 06:06:11 GMT"
},
{
"version": "v2",
"created": "Thu, 30 Oct 2008 05:16:23 GMT"
}
] | 2009-02-23T00:00:00 | [
[
"Sakamoto",
"Reiho",
""
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711.4186 | Mu Qing-Xia | Qing-Xia Mu, Yong-Hong Ma and L. Zhou | Generating an entangled coherent state of two cavity modes in a
three-level \Lambda - type atomic system | 3 figures | null | 10.1088/0953-4075/40/16/005 | null | quant-ph | null | In this paper, we present a scheme to generate an entangled coherent state by
considering a three-level \Lambda - type atom interacting with a two-mode
cavity driven by classical fields. The two-mode entangled coherent state can be
obtained under large detuning conditions. Considering the cavity decay, an
analytical solution is deduced.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 06:06:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mu",
"Qing-Xia",
""
],
[
"Ma",
"Yong-Hong",
""
],
[
"Zhou",
"L.",
""
]
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] |
711.4187 | Ke Zhu | Yong-Geun Oh, Ke Zhu | Floer trajectories with immersed nodes and scale-dependent gluing | 122 pages, 6 figures. Submitted version. Quadratic estimates added,
presentation of error estimates improved | null | null | null | math.SG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We define an enhanced compactification of Floer trajectories under Morse
background using the adiabatic degeneration and the scale-dependent gluing
techniques. The compactification reflects the 1-jet datum of the smooth Floer
trajectories nearby the limiting nodal Floer trajectories arising from
adiabatic degeneration of the background Morse function. This paper studies the
gluing problem when the limiting gradient trajectories has length zero through
a renomalization process. The case with limiting gradient trajectories of
non-zero length will be treated elsewhere.
An immediate application of our result is a proof of the isomorphism property
of the PSS map : A proof of this isomorphism property was first outlined by
P\"unihikin-Salamon-Schwarz \cite{PSS} in a way somewhat different from the
current proof in its details. This kind of scale-dependent gluing techniques
was initiated in [FOOO07] in relation to the metamorphosis of holomorphic
polygons under Lagrangian surgery and is expected to appear in other gluing and
compactification problem of pseudo-holomorphic curves that involves `adiabatic'
parameters or rescales the targets.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 20:16:32 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Apr 2008 19:51:14 GMT"
},
{
"version": "v3",
"created": "Tue, 9 Feb 2010 03:34:34 GMT"
}
] | 2010-02-09T00:00:00 | [
[
"Oh",
"Yong-Geun",
""
],
[
"Zhu",
"Ke",
""
]
] | [
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] |
711.4188 | Subenoy Chakraborty | Asit Banerjee, Tanwi Bandyopadhyay and Subenoy Chakraborty | Emergent Universe in Brane World Scenario with Schwarzschild-de Sitter
Bulk | 4 pages, no figure, accepted for publication in Gen.Relt.Grav | Gen.Rel.Grav.40:1603-1607,2008 | 10.1007/s10714-007-0567-3 | null | gr-qc | null | A model of an emergent universe is obtained in brane world. Here the bulk
energy is in the form of cosmological constant, while the brane consists of a
fluid satisfying an equation of state of the form $p_{b}={1/3} \rho_{b}$, which
is effectively a radiation equation of state at high energies. It is shown that
with the positive bulk cosmological constant, one of our models represents an
emergent universe.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 06:51:13 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Banerjee",
"Asit",
""
],
[
"Bandyopadhyay",
"Tanwi",
""
],
[
"Chakraborty",
"Subenoy",
""
]
] | [
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] |
711.4189 | Jian Wang | Z.H. Qiao and J. Wang | A variant transfer matrix method suitable for transport through
multi-probe systems | null | Nanotech. Vol.18, 435402 (2007) | 10.1088/0957-4484/18/43/435402 | null | cond-mat.mes-hall | null | We have developed a variant transfer matrix method that is suitable for
transport through multi-probe systems. Using this method, we have numerically
studied the quantum spin Hall effect (QSHE) on 2D graphene with both intrinsic
(Vso) and Rashba (Vr) spin-orbit (SO) couplings. The integer QSHE arises in the
presence of intrinsic SO interaction and is gradually destroyed by the Rashba
SO interaction and disorder fluctuation. We have numerically determined the
phase boundaries separating integer QSHE and spin Hall liquid. We have found
that when Vso> 0.2t with t the hopping constant the energy gap needed for the
integer QSHE is the largest satisfying |E|<t. For smaller Vso the energy gap
decreases linearly. In the presence of Rashba SO interaction or disorders, the
energy gap diminishes. With Rashba SO interaction the integer QSHE is robust at
the largest energy within the energy gap while at the smallest energy within
the energy gap the integer QSHE is insensitive to the disorder.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 07:16:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Qiao",
"Z. H.",
""
],
[
"Wang",
"J.",
""
]
] | [
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711.419 | Scipio Cuccagna | Scipio Cuccagna | On dispersion for Klein Gordon equation with periodic potential in 1D | null | null | null | null | math.AP | null | By exploiting estimates on Bloch functions obtained in a previous paper, we
prove decay estimates for Klein Gordon equations with a time independent
potential periodic in space in 1D and with generic mass
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 07:41:24 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Cuccagna",
"Scipio",
""
]
] | [
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711.4191 | Ken-Ichi Katayama | Masafumi Fukuma, Ken-Ichi Katayama, Takao Suyama | Notes on the Hamiltonian formulation of 3D Yang-Mills theory | 26 pages, LaTeX; discussions on IR regulators and local counterterms
improved, references added | JHEP0804:095,2008 | 10.1088/1126-6708/2008/04/095 | KUNS-2104 | hep-th | null | Three-dimensional Yang-Mills theory is investigated in the Hamiltonian
formalism based on the Karabali-Nair variable. A new algorithm is developed to
obtain the renormalized Hamiltonian by identifying local counterterms in
Lagrangian with the use of fictitious holomorphic symmetry existing in the
framework with the KN variable. Our algorithm is totally algebraic and enables
one to calculate the ground state wave functional recursively in gauge
potentials. In particular, the Gaussian part thus calculated is shown to
coincide with that obtained by Leigh et al. Higher-order corrections to the
Gaussian part are also discussed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 07:45:32 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 15:26:49 GMT"
},
{
"version": "v3",
"created": "Tue, 18 Mar 2008 18:26:30 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Fukuma",
"Masafumi",
""
],
[
"Katayama",
"Ken-Ichi",
""
],
[
"Suyama",
"Takao",
""
]
] | [
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711.4192 | Scipio Cuccagna | Scipio Cuccagna | A revision of "On asymptotic stability in energy space of ground states
of NLS in 1D" | This is a revision of the author's paper "On asymptotic stability in
energy space of ground states of NLS in 1D" which appeared in
J.Diff.Equations 245 (2008) pp 653-691. We correct an error in Lemma 5.4 in
that paper and we simplify the smoothing argument | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We transpose work by T.Mizumachi to prove smoothing estimates for dispersive
solutions of the linearization at a ground state of a Nonlinear Schr\"odinger
equation (NLS) in 1D. As an application we extend to dimension 1D a result on
asymptotic stability of ground states of NLS proved by Cuccagna & Mizumachi for
dimensions $\ge 3$
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 07:46:07 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 13:10:41 GMT"
},
{
"version": "v3",
"created": "Mon, 15 Sep 2008 13:23:30 GMT"
}
] | 2008-09-15T00:00:00 | [
[
"Cuccagna",
"Scipio",
""
]
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] |
711.4193 | Xin-Zhou Li | Ping Xi and Xin-zhou Li | Object Picture of Quasinormal Modes for Stringy Black Holes | 4 pages, 5 figures | Chin.Phys.Lett.22:2763-2765,2005 | 10.1088/0256-307X/22/11/010 | null | hep-th | null | We study the quasinormal modes (QNMs) for stringy black holes. By using
numerical calculation, the relations between the QNMs and the parameters of
black holes are minutely shown. For (1+1)-dimensional stringy black hole, the
real part of the quasinormal frequency increases and the imaginary part of the
quasinormal frequency decreases as the mass of the black hole increases.
Furthermore, the dependence of the QNMs on the charge of the black hole and the
flatness parameter is also illustrated. For (1+3)-dimensional stringy black
hole, increasing either the event horizon or the multipole index, the real part
of the quasinormal frequency decreases. The imaginary part of the quasinormal
frequency increases no matter whether the event horizon is increased or the
multipole index is decreased.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 07:52:35 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 06:59:38 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Xi",
"Ping",
""
],
[
"Li",
"Xin-zhou",
""
]
] | [
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] |
711.4194 | Gerard van Belle | G. T. van Belle, G. van Belle, M.J. Creech-Eakman, J. Coyne, A. F.
Boden, R. L. Akeson, D. R. Ciardi, K. M. Rykoski, R. R. Thompson, B. F. Lane
(for the PTI Collaboration) | The Palomar Testbed Interferometer Calibrator Catalog | 100 pages, 7 figures, 7 tables; to appear in the May 2008ApJS, v176n1 | null | 10.1086/526548 | null | astro-ph | null | The Palomar Testbed Interferometer (PTI) archive of observations between 1998
and 2005 is examined for objects appropriate for calibration of optical
long-baseline interferometer observations - stars that are predictably
point-like and single. Approximately 1,400 nights of data on 1,800 objects were
examined for this investigation. We compare those observations to an
intensively studied object that is a suitable calibrator, HD217014, and
statistically compare each candidate calibrator to that object by computing
both a Mahalanobis distance and a Principal Component Analysis. Our hypothesis
is that the frequency distribution of visibility data associated with
calibrator stars differs from non-calibrator stars such as binary stars.
Spectroscopic binaries resolved by PTI, objects known to be unsuitable for
calibrator use, are similarly tested to establish detection limits of this
approach. From this investigation, we find more than 350 observed stars
suitable for use as calibrators (with an additional $\approx 140$ being
rejected), corresponding to $\gtrsim 95%$ sky coverage for PTI. This approach
is noteworthy in that it rigorously establishes calibration sources through a
traceable, empirical methodology, leveraging the predictions of spectral energy
distribution modeling but also verifying it with the rich body of PTI's on-sky
observations.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 08:04:16 GMT"
}
] | 2019-08-17T00:00:00 | [
[
"van Belle",
"G. T.",
"",
"for the PTI Collaboration"
],
[
"van Belle",
"G.",
"",
"for the PTI Collaboration"
],
[
"Creech-Eakman",
"M. J.",
"",
"for the PTI Collaboration"
],
[
"Coyne",
"J.",
"",
"for the PTI Collaboration"
],
[
"Boden",
"A. F.",
"",
"for the PTI Collaboration"
],
[
"Akeson",
"R. L.",
"",
"for the PTI Collaboration"
],
[
"Ciardi",
"D. R.",
"",
"for the PTI Collaboration"
],
[
"Rykoski",
"K. M.",
"",
"for the PTI Collaboration"
],
[
"Thompson",
"R. R.",
"",
"for the PTI Collaboration"
],
[
"Lane",
"B. F.",
"",
"for the PTI Collaboration"
]
] | [
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711.4195 | Scipio Cuccagna | Scipio Cuccagna and Tetsu Mizumachi | On asymptotic stability in energy space of ground states for Nonlinear
Schr\"odinger equations | null | null | 10.1007/s00220-008-0605-3 | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider nonlinear Schr\"odinger equations in dimension 3 or higher. We
prove that symmetric finite energy solutions close to orbitally stable ground
states converge asymptotically to a sum of a ground state and a dispersive wave
assuming the so called Fermi Golden Rule (FGR) hypothesis. We improve the sign
condition required in a recent paper by Gang Zhou and I.M.Sigal
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 08:06:15 GMT"
},
{
"version": "v2",
"created": "Mon, 9 Jun 2008 09:36:36 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Cuccagna",
"Scipio",
""
],
[
"Mizumachi",
"Tetsu",
""
]
] | [
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711.4196 | Christopher Gordon | Christopher Gordon (1), Kate Land (1), and Anze Slosar (1 and 2) ((1)
Oxford, (2) Berkeley) | Determining the motion of the solar system relative to the cosmic
microwave background using type Ia supernovae | 6 pages, 6 figures; fixed a typo; matches version to appear in MNRAS | null | 10.1111/j.1365-2966.2008.13239.x | null | astro-ph gr-qc hep-ph hep-th | null | We estimate the solar system motion relative to the cosmic microwave
background using type Ia supernovae (SNe) measurements. We take into account
the correlations in the error bars of the SNe measurements arising from
correlated peculiar velocities. Without accounting for correlations in the
peculiar velocities, the SNe data we use appear to detect the peculiar velocity
of the solar system at about the 3.5 sigma level. However, when the
correlations are correctly accounted for, the SNe data only detects the solar
system peculiar velocity at about the 2.5 sigma level. We forecast that the
solar system peculiar velocity will be detected at the 9 sigma level by GAIA
and the 11 sigma level by the LSST. For these surveys we find the correlations
are much less important as most of the signal comes from higher redshifts where
the number density of SNe is insufficient for the correlations to be important.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:05:01 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Mar 2008 15:21:41 GMT"
},
{
"version": "v3",
"created": "Fri, 4 Apr 2008 10:01:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gordon",
"Christopher",
"",
"1 and 2"
],
[
"Land",
"Kate",
"",
"1 and 2"
],
[
"Slosar",
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"",
"1 and 2"
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711.4197 | Hadi Jor\'ati | Hadi Jorati | On a class of curved flag multipliers | null | null | null | null | math.CA | null | We characterize a family of curved flag kernels in terms of their multipliers
and prove L^p boundedness.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 08:22:24 GMT"
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] | 2007-11-28T00:00:00 | [
[
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] |
711.4198 | Vincent Leon | Vincent Leon (CRMD), Yang Ren (ANL), Marie-Louise Saboungi (CRMD) | Effect of Nanoscale Confinement on the \beta-\alpha Phase Transition in
Ag2Se | null | Journal of Applied Physics 102, 12 (2005) 1 | 10.1063/1.2822135 | null | cond-mat.mtrl-sci | null | The confinement of silver selenide was investigated using mesoporous silica.
Results from x-ray diffraction and electron microscopy show that the confined
material still exhibits a \beta to \alpha transition similar to the one that
takes place in the bulk crystalline state but with a transition temperature
that depends significantly on the confinement conditions. Decreasing the pore
size leads to an increase of the transition temperature, opposite to the
behavior of the melting point observed in several metallic and organic
materials. In the free particles, on the other hand, no size dependence is
observed with particle sizes down to 4 nm.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 08:27:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Leon",
"Vincent",
"",
"CRMD"
],
[
"Ren",
"Yang",
"",
"ANL"
],
[
"Saboungi",
"Marie-Louise",
"",
"CRMD"
]
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711.4199 | Haibo Li | Yi-Fang Wang | The BES-III experiment at the high luminosity Tau-Charm factory | 4 pages, 5 figures, to be published in the proceedings of CHARM07,
Ithaca, NY, August 2007, eConf C070805 | ECONF C070805:38,2007 | null | null | hep-ex | null | Interesting results from BES-II and other experiments raised actually many
new questions which shall be answered by its upgrade program, BEPCII and
BES-III. The design and current status of BEPCII and BES-III are reported.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 08:39:50 GMT"
}
] | 2011-06-15T00:00:00 | [
[
"Wang",
"Yi-Fang",
""
]
] | [
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] |
711.42 | Liliana Arrachea | Liliana Arrachea, Alfredo Levy Yeyati and Alvaro Martin-Rodero | Non adiabatic features of electron pumping through a quantum dot in the
Kondo regime | 8 pages, 7 figures | Phys. Rev. B 77, 165326 (2008) | 10.1103/PhysRevB.77.165326 | null | cond-mat.mes-hall cond-mat.str-el | null | We investigate the behavior of the dc electronic current, Jdc, in an
interacting quantum dot driven by two ac local potentials oscillating with a
frequency, Omega0, and a phase-lag, phi. We provide analytical functions to
describe the fingerprints of the Coulomb interaction in an experimental Jdc vs
phi characteristic curve. We show that the Kondo resonance reduces at low
temperatures the frequency range for the linear behavior of Jdc in Omega0 to
take place and determines the evolution of the dc-current as the temperature
increases.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 08:59:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Arrachea",
"Liliana",
""
],
[
"Yeyati",
"Alfredo Levy",
""
],
[
"Martin-Rodero",
"Alvaro",
""
]
] | [
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] |
711.4201 | Javier Junquera | Javier Junquera and Philippe Ghosez | First-principles study of ferroelectric oxide epitaxial thin films and
superlattices: role of the mechanical and electrical boundary conditions | 40 pages, 195 references, 6 eps Figures, submitted to Journal of
Computational and Theoretical Nanoscience | null | null | null | cond-mat.mtrl-sci | null | In this review, we propose a summary of the most recent advances in the
first-principles study of ferroelectric oxide epitaxial thin films and
multilayers. We discuss in detail the key roles of mechanical and electrical
boundary conditions, providing to the reader the basic background for a simple
and intuitive understanding of the evolution of the ferroelectric properties in
many nanostructures. Going further we also highlight promising new avenues and
future challenges within this exciting field or researches.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:16:46 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Junquera",
"Javier",
""
],
[
"Ghosez",
"Philippe",
""
]
] | [
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] |
711.4202 | Elena Villa | Elena Villa | Mean density of inhomogeneous Boolean models with lower dimensional
typical grain | shortened version; some remarks added and some misprints corrected | null | null | null | math.PR | null | The mean density of a random closed set $\Theta$ in $\R^d$ with Hausdorff
dimension $n$ is the Radon-Nikodym derivative of the expected measure
$\E[\h^n(\Theta\cap\cdot)]$ induced by $\Theta$ with respect to the usual
$d$-dimensional Lebesgue measure. We consider here inhomogeneous Boolean models
with lower dimensional typical grain. Under general regularity assumptions on
the typical grain, related to the existence of its Minkowski content, and on
the intensity measure of the underlying Poisson point process, we prove an
explicit formula for the mean density. The proof of such formula provides as
by-product estimators for the mean density in terms of the empirical capacity
functional, which turns to be closely related to the well known random variable
density estimation by histograms in the extreme case $n=0$. Particular cases
and examples are also discussed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:21:55 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Mar 2008 14:45:32 GMT"
}
] | 2008-03-28T00:00:00 | [
[
"Villa",
"Elena",
""
]
] | [
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711.4203 | Nicolas Matagne SE | N. N. Scoccola, J. L. Goity, N. Matagne | Analysis of Negative Parity Baryon Photoproduction Amplitudes in the
$1/N_c$ Expansion | 7 pages, 5 tables | Phys.Lett.B663:222-227,2008 | 10.1016/j.physletb.2008.03.056 | null | hep-ph | null | We study the photoproduction helicity amplitudes of negative parity baryons
in the context of the $1/N_c$ expansion of QCD. A complete analysis to
next-to-leading order is carried out. The results show sub-leading effects to
be within the magnitude expected from the $1/N_c$ power counting. They also
show significant deviations from the quark model, in particular the need for
2-body effects.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:32:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Scoccola",
"N. N.",
""
],
[
"Goity",
"J. L.",
""
],
[
"Matagne",
"N.",
""
]
] | [
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] |
711.4204 | Henry Joy McCracken | H. J. McCracken, O. Ilbert, Y. Mellier, E. Bertin, L. Guzzo, S.
Arnouts, O. Le F\`evre and G. Zamorani | Clustering properties of a type-selected volume-limited sample of
galaxies in the CFHTLS | 16 pages, 18 figures, accepted for publication in Astronomy and
Astrophysics | null | 10.1051/0004-6361:20078636 | null | astro-ph | null | (abridged) We present an investigation of the clustering of i'AB<24.5
galaxies in the redshift interval 0.2<z<1.2. Using 100,000 precise photometric
redshifts in the four ultra-deep fields of the Canada-France Legacy Survey, we
construct a set of volume-limited galaxy catalogues. We study the dependence of
the amplitude and slope of the galaxy correlation function on absolute B-band
rest-frame luminosity, redshift and best-fitting spectral type. We find: 1. The
comoving correlation length for all galaxies decreases steadily from z~0.3 to
z~1. 2. At all redshifts and luminosities, galaxies with redder rest-frame
colours have clustering amplitudes between two and three times higher than
bluer ones. 3. For bright red and blue galaxies, the clustering amplitude is
invariant with redshift. 4. At z~0.5, less luminous galaxies have higher
clustering amplitudes of around 6 h-1 Mpc. 5. The relative bias between
galaxies with red and blue rest-frame colours increases gradually towards
fainter absolute magnitudes. One of the principal implications of these results
is that although the full galaxy population traces the underlying dark matter
distribution quite well (and is therefore quite weakly biased), redder, older
galaxies have clustering lengths which are almost invariant with redshift, and
by z~1 are quite strongly biased.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:37:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"McCracken",
"H. J.",
""
],
[
"Ilbert",
"O.",
""
],
[
"Mellier",
"Y.",
""
],
[
"Bertin",
"E.",
""
],
[
"Guzzo",
"L.",
""
],
[
"Arnouts",
"S.",
""
],
[
"Fèvre",
"O. Le",
""
],
[
"Zamorani",
"G.",
""
]
] | [
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] |
711.4205 | Gregor Jundt | Gregor Jundt, Lucio Robledo, Alexander H\"ogele, Stefan F\"alt, and
Atac Imamo\u{g}lu | Observation of dressed excitonic states in a single quantum dot | null | null | 10.1103/PhysRevLett.100.177401 | null | cond-mat.mes-hall | null | We report the observation of dressed states of a quantum dot. The optically
excited exciton and biexciton states of the quantum dot are coupled by a strong
laser field and the resulting spectral signatures are measured using
differential transmission of a probe field. We demonstrate that the anisotropic
electron-hole exchange interaction induced splitting between the x- and
y-polarized excitonic states can be completely erased by using the AC-Stark
effect induced by the coupling field, without causing any appreciable
broadening of the spectral lines. We also show that by varying the polarization
and strength of a resonant coupling field, we can effectively change the
polarization-axis of the quantum dot.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:43:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jundt",
"Gregor",
""
],
[
"Robledo",
"Lucio",
""
],
[
"Högele",
"Alexander",
""
],
[
"Fält",
"Stefan",
""
],
[
"Imamoğlu",
"Atac",
""
]
] | [
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] |
711.4206 | Leonard Choup Dr | Leonard N. Choup | Edgeworth Expansion of the Largest Eigenvalue Distribution Function of
GUE Revisited | null | null | 10.1063/1.2873345 | null | math-ph math.MP | null | We derive expansions of the resolvent
Rn(x;y;t)=(Qn(x;t)Pn(y;t)-Qn(y;t)Pn(x;t))/(x-y) of the Hermite kernel Kn at the
edge of the spectrum of the finite n Gaussian Unitary Ensemble (GUEn) and the
finite n expansion of Qn(x;t) and Pn(x;t). Using these large n expansions, we
give another proof of the derivation of an Edgeworth type theorem for the
largest eigenvalue distribution function of GUEn. We conclude with a brief
discussion on the derivation of the probability distribution function of the
corresponding largest eigenvalue in the Gaussian Orthogonal Ensemble (GOEn) and
Gaussian Symplectic Ensembles (GSEn).
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:50:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Choup",
"Leonard N.",
""
]
] | [
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] |
711.4207 | Laurens Keek | L.Keek, J. J. M. in 't Zand, E. Kuulkers, A. Cumming, E. F. Brown, M.
Suzuki | First superburst from a classical low-mass X-ray binary transient | 12 pages, 8 figures, accepted for publication in A&A | null | 10.1051/0004-6361:20078464 | null | astro-ph | null | We report the analysis of the first superburst from a transiently accreting
neutron star system with the All-Sky Monitor (ASM) on the Rossi X-ray Timing
Explorer. The superburst occurred 55 days after the onset of an accretion
outburst in 4U 1608-522. During that time interval, the accretion rate was at
least 7% of the Eddington limit. The peak flux of the superburst is 22 to 45%
of the Eddington limit, and its radiation energy output is between 4e41 and
9e41 erg for a distance of 3.2 kpc. Fits of cooling models to the superburst
light curve indicate an ignition column depth between 1.5e12 and 4.1e12 g/cm2.
Extrapolating the accretion history observed by the ASM, we derive that this
column was accreted over a period of 26 to 72 years. The superburst
characteristics are consistent with those seen in other superbursting low-mass
X-ray binaries. However, the transient nature of the hosting binary presents
significant challenges for superburst theory, requiring additional ingredients
for the models. The carbon that fuels the superburst is thought to be produced
mostly during the accretion outbursts and destroyed in the frequent type-I
X-ray bursts. Mixing and sedimentation of the elements in the neutron star
envelope may significantly influence the balance between the creation and
destruction of carbon. Furthermore, predictions for the temperature of the
neutron star crust fail to reach the values required for the ignition of carbon
at the inferred column depth.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:53:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Keek",
"L.",
""
],
[
"Zand",
"J. J. M. in 't",
""
],
[
"Kuulkers",
"E.",
""
],
[
"Cumming",
"A.",
""
],
[
"Brown",
"E. F.",
""
],
[
"Suzuki",
"M.",
""
]
] | [
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