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711.2108 | Kallosh Renata | Renata Kallosh | The Effective Action of N=8 Supergravity | 17 pages | null | null | null | hep-th | null | We present a simple form of the on-shell gauge-invariant 1-loop effective
action of N=8 supergravity which is manifestly N=8 supersymmetric at the linear
level. By generalizing the dimensional arguments in superspace to non-local
invariants, we show that the 1-loop effective action does not contain any
contributions from bubble and triangle diagrams. The absence of bubbles implies
the absence of conformal and axial anomalies. We also show that the 1-loop
effective action of N=8 supergravity features a "dual" conformal symmetry in
the momentum space.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:22:54 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Kallosh",
"Renata",
""
]
] | [
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] |
711.2109 | Floris van der Tak | Floris van der Tak (SRON Groningen), Susanne Aalto (Onsala), Rowin
Meijerink (Berkeley) | Detection of extragalactic H3O+ | Accepted by A&A Letters; 4-5 pages depending on paper format; two b/w
figures | null | 10.1051/0004-6361:20078824 | null | astro-ph | null | The H3O+ molecule probes the oxygen chemistry and the ionization rate of
dense circumnuclear gas in galaxies. In particular, recent H3O+ observations
show variations in the cosmic-ray ionization rate by factors of $>$10 within
our Galaxy. Using the JCMT, we have observed the 364 GHz line of p-H3O+ in the
centers of M82 and Arp 220. In Arp 220, the line profile suggests that the
emission originates in the Western nucleus. In M82, both the eastern molecular
peak and the circumnuclear region contribute to the emission. The derived
column densities, abundances, and H3O+ / H2O ratios indicate ionization rates
similar to or even exceeding that in the Galactic Center. Model calculations of
the chemistry of irradiated molecular gas indicate a likely origin of this high
ionization rate in the extended, evolved starburst of M82. In contrast,
irradiation by X-rays from the AGN disk is the most likely model for Arp 220.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 15:48:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"van der Tak",
"Floris",
"",
"SRON Groningen"
],
[
"Aalto",
"Susanne",
"",
"Onsala"
],
[
"Meijerink",
"Rowin",
"",
"Berkeley"
]
] | [
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711.211 | Fumiko Yamada | Fumiko Yamada, Toshio Ono, Hidekazu Tanaka, Gregoire Misguich, Masaki
Oshikawa and Toshiro Sakakibara | Magnetic-Field Induced Bose-Einstein Condensation of Magnons and
Critical Behavior in Interacting Spin Dimer System TlCuCl$_3$ | 5 pages, 6 figures, to appear in J. Phys. Soc. Jpn. Vol.77 No.1 | null | 10.1143/JPSJ.77.013701 | null | cond-mat.str-el | null | Magnetization measurements were performed to investigate the critical
behavior of the field-induced magnetic ordering in gapped spin system
TlCuCl$_3$. The critical density of the magnons was obtained as a function of
temperature and the magnon-magnon interaction constant was evaluated. The
experimental phase boundary for $T < 5$ K agrees almost perfectly with the
magnon BEC theory based on the Hartree-Fock approximation with realistic
dispersion relations. The phase boundary can be described by the power law
$[H_{N}(T)-H_{c}] propto T^{phi}$. With decreasing fitting temperature range,
the critical exponent ${phi}$ decreases and converges at $phi_{BEC} =3/2$
predicted by the magnon BEC theory.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 05:44:27 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Yamada",
"Fumiko",
""
],
[
"Ono",
"Toshio",
""
],
[
"Tanaka",
"Hidekazu",
""
],
[
"Misguich",
"Gregoire",
""
],
[
"Oshikawa",
"Masaki",
""
],
[
"Sakakibara",
"Toshiro",
""
]
] | [
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] |
711.2111 | Joseph Rhee | Joseph H. Rhee, Inseok Song, B. Zuckerman | Warm dust in the terrestrial planet zone of a sun-like Pleiad:
collisions between planetary embryos? | ApJ in press, 19 pages including 3 figures and 2 tables, minor
changes to the tables and figures | null | 10.1086/524935 | null | astro-ph | null | Only a few solar-type main sequence stars are known to be orbited by warm
dust particles; the most extreme is the G0 field star BD+20 307 that emits ~4%
of its energy at mid-infrared wavelengths. We report the identification of a
similarly dusty star HD 23514, an F6-type member of the Pleiades cluster. A
strong mid-IR silicate emission feature indicates the presence of small warm
dust particles, but with the primary flux density peak at the non-standard
wavelength of ~9 micron. The existence of so much dust within an AU or so of
these stars is not easily accounted for given the very brief lifetime in orbit
of small particles. The apparent absence of very hot (>~1000 K) dust at both
stars suggests the possible presence of a planet closer to the stars than the
dust. The observed frequency of the BD+20 307/HD 23514 phenomenon indicates
that the mass equivalent of Earth's Moon must be converted, via collisions of
massive bodies, to tiny dust particles that find their way to the terrestrial
planet zone during the first few hundred million years of the life of many
(most?) sun-like stars. Identification of these two dusty systems among
youthful nearby solar-type stars suggests that terrestrial planet formation is
common.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 05:58:52 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 18:59:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rhee",
"Joseph H.",
""
],
[
"Song",
"Inseok",
""
],
[
"Zuckerman",
"B.",
""
]
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711.2112 | Michel Grabisch | Michel Grabisch (CES), Christophe Labreuche (TRT) | Bi-capacities -- Part II: the Choquet integral | null | Fuzzy Sets and Systems (2005) 237-259 | null | null | cs.DM cs.GT | null | Bi-capacities arise as a natural generalization of capacities (or fuzzy
measures) in a context of decision making where underlying scales are bipolar.
They are able to capture a wide variety of decision behaviours, encompassing
models such as Cumulative Prospect Theory (CPT). The aim of this paper in two
parts is to present the machinery behind bi-capacities, and thus remains on a
rather theoretical level, although some parts are firmly rooted in decision
theory, notably cooperative game theory. The present second part focuses on the
definition of Choquet integral. We give several expressions of it, including an
expression w.r.t. the M\"obius transform. This permits to express the Choquet
integral for 2-additive bi-capacities w.r.t. the interaction index.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:11:57 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Grabisch",
"Michel",
"",
"CES"
],
[
"Labreuche",
"Christophe",
"",
"TRT"
]
] | [
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711.2113 | Martin Gaskell | C. Martin Gaskell | Accretion Disks and the Nature and Origin of AGN Continuum Variability | Invited talk given at "The Nuclear Region, Host Galaxy, and
Environment of Active Galaxies", Huatulco, Mexico, April 2007. To appear in
Rev. Mex. A&A Conf. Ser. 11 pages, 7 figures | null | null | null | astro-ph | null | Theory and observations of the dominant thermal continuum emission in AGNs
are examined. After correction for reddening, the steady state AGN optical--UV
spectral energy distributions (SEDs) are very similar. The SEDs are dominated
energetically by the big blue bump (BBB), but this bump never shows the
nu^{+1/3} spectrum predicted for a standard thin accretion disk with a
r^{-0.75} radial temperature gradient. Instead, the observed optical-UV SED
implies a temperature gradient of r^{-0.57} independent of the thickness of the
disk. This means that there is some flow of heat outwards in the disk. The disk
is large and the region emitting the optical continuum is as large as the inner
broad-line region (BLR). Because optical variability is seen in all AGNs on the
light-crossing time of the BLR, variations must propagate at close to the speed
of light, rather than on dynamical timescales. This argues that the
energy-generation mechanism is electromagnetic rather that hydrodynamic. Since
the velocities are near the speed of light, there can be significant local
anisotropy in the emission. The large rapid variations of the BBB imply that
the magnetohydrodynamic energy generation is fundamentally unstable. Because of
the inevitable radial temperature gradient in the accreting material, different
spectral regions come predominantly from different radii, and variations in
different spectral regions correspond to variability at different radii. This
explains the frequently observed independence of X-ray and optical variations,
cases of variability at lower energies leading variability at higher energies,
and rapid changes in emission-line reverberation lags. Some observational tests
of the local variability hypothesis are proposed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:12:27 GMT"
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] | 2007-11-15T00:00:00 | [
[
"Gaskell",
"C. Martin",
""
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] |
711.2114 | Michel Grabisch | Michel Grabisch (CES), Christophe Labreuche (TRT) | Bi-capacities -- Part I: definition, M\"obius transform and interaction | null | Fuzzy Sets and Systems (2005) 211-236 | null | null | cs.DM cs.GT | null | Bi-capacities arise as a natural generalization of capacities (or fuzzy
measures) in a context of decision making where underlying scales are bipolar.
They are able to capture a wide variety of decision behaviours, encompassing
models such as Cumulative Prospect Theory (CPT). The aim of this paper in two
parts is to present the machinery behind bi-capacities, and thus remains on a
rather theoretical level, although some parts are firmly rooted in decision
theory, notably cooperative game theory. The present first part is devoted to
the introduction of bi-capacities and the structure on which they are defined.
We define the M\"obius transform of bi-capacities, by just applying the well
known theory of M\" obius functions as established by Rota to the particular
case of bi-capacities. Then, we introduce derivatives of bi-capacities, by
analogy with what was done for pseudo-Boolean functions (another view of
capacities and set functions), and this is the key point to introduce the
Shapley value and the interaction index for bi-capacities. This is done in a
cooperative game theoretic perspective. In summary, all familiar notions used
for fuzzy measures are available in this more general framework.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:15:05 GMT"
}
] | 2007-11-15T00:00:00 | [
[
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711.2115 | Michel Grabisch | Michel Grabisch (CES), Christophe Labreuche (TRT) | Derivative of functions over lattices as a basis for the notion of
interaction between attributes | null | Annals of Mathematics and Artificial Intelligence 49 (2007)
151-170 | null | null | cs.DM cs.GT | null | The paper proposes a general notion of interaction between attributes, which
can be applied to many fields in decision making and data analysis. It
generalizes the notion of interaction defined for criteria modelled by
capacities, by considering functions defined on lattices. For a given problem,
the lattice contains for each attribute the partially ordered set of remarkable
points or levels. The interaction is based on the notion of derivative of a
function defined on a lattice, and appears as a generalization of the Shapley
value or other probabilistic values.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:15:49 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Grabisch",
"Michel",
"",
"CES"
],
[
"Labreuche",
"Christophe",
"",
"TRT"
]
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] |
711.2116 | Frederic Vignat | Fr\'ed\'eric Vignat (LGS), Fran\c{c}ois Villeneuve (LGS) | A numerical approach for 3D manufacturing tolerances synthesis | null | Dans Proceedings of the 10th CIRP International Seminar on
Computer Aided Tolerancing - 10th CIRP International Seminar on Computer
Aided Tolerancing, Erlangen : Allemagne (2007) | null | null | cs.CE | null | Making a product conform to the functional requirements indicated by the
customer suppose to be able to manage the manufacturing process chosen to
realise the parts. A simulation step is generally performed to verify that the
expected generated deviations fit with these requirements. It is then necessary
to assess the actual deviations of the process in progress. This is usually
done by the verification of the conformity of the workpiece to manufacturing
tolerances at the end of each set-up. It is thus necessary to determine these
manufacturing tolerances. This step is called "manufacturing tolerance
synthesis". In this paper, a numerical method is proposed to perform 3D
manufacturing tolerances synthesis. This method uses the result of the
numerical analysis of tolerances to determine influent mall displacement of
surfaces. These displacements are described by small displacements torsors. An
algorithm is then proposed to determine suitable ISO manufacturing tolerances.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:21:17 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Vignat",
"Frédéric",
"",
"LGS"
],
[
"Villeneuve",
"François",
"",
"LGS"
]
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711.2117 | Vasily E. Tarasov | Vasily E. Tarasov | Fractional Stability | 5 pages, LaTeX | null | null | null | physics.class-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A fractional generalization of variations is used to define a stability of
non-integer order. Fractional variational derivatives are suggested to describe
the properties of dynamical systems at fractional perturbations. We formulate
stability with respect to motion changes at fractional changes of variables.
Note that dynamical systems, which are unstable "in sense of Lyapunov", can be
stable with respect to fractional variations.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:37:17 GMT"
},
{
"version": "v2",
"created": "Wed, 20 Jul 2011 08:47:20 GMT"
},
{
"version": "v3",
"created": "Sat, 23 Jul 2011 11:39:31 GMT"
}
] | 2011-07-26T00:00:00 | [
[
"Tarasov",
"Vasily E.",
""
]
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711.2118 | Alberica Toia Dr | Alberica Toia (for the PHENIX Collaboration) | Measurements of dilepton continuum at the PHENIX experiment at RHIC | 14 pages, 9 figures, proceedings of CPOD conference | PoS CPOD07:037,2007 | null | null | nucl-ex | null | PHENIX has measured the dielectron continuum in sqrt(s_(NN))=200 GeV Au+Au
and p+p collisions. In minimum bias Au+Au collisions the dielectron yield in
the mass range between 150 and 750 MeV/c^2 is enhanced by a factor of 3.4 +/-
0.2(stat.) +/- 1.3(syst.) +/- 0.7(model) compared to the expectation from our
model of hadron decays that well reproduces the mass spectrum in p+p
collisions. The integrated yield increases faster with the centrality of the
collisions than the number of participating nucleons, suggesting emission from
scattering processes in the dense medium. The continuum yield between the
masses of the phi and the J/psi meson is consistent with expectations from
correlated ccbar production, though other mechanisms are not ruled out.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 07:16:04 GMT"
},
{
"version": "v2",
"created": "Wed, 21 Nov 2007 16:48:12 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Toia",
"Alberica",
"",
"for the PHENIX Collaboration"
]
] | [
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711.2119 | Nicolas Verzelen | Nicolas Verzelen (INRIA Futurs), Fanny Villers (MIA) | Goodness-of-fit Tests for high-dimensional Gaussian linear models | null | null | null | RR-6354 | math.ST stat.TH | null | Let $(Y,(X_i)_{i\in\mathcal{I}})$ be a zero mean Gaussian vector and $V$ be a
subset of $\mathcal{I}$. Suppose we are given $n$ i.i.d. replications of the
vector $(Y,X)$. We propose a new test for testing that $Y$ is independent of
$(X_i)_{i\in \mathcal{I}\backslash V}$ conditionally to $(X_i)_{i\in V}$
against the general alternative that it is not. This procedure does not depend
on any prior information on the covariance of $X$ or the variance of $Y$ and
applies in a high-dimensional setting. It straightforwardly extends to test the
neighbourhood of a Gaussian graphical model. The procedure is based on a model
of Gaussian regression with random Gaussian covariates. We give non asymptotic
properties of the test and we prove that it is rate optimal (up to a possible
$\log(n)$ factor) over various classes of alternatives under some additional
assumptions. Besides, it allows us to derive non asymptotic minimax rates of
testing in this setting. Finally, we carry out a simulation study in order to
evaluate the performance of our procedure.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:53:15 GMT"
},
{
"version": "v2",
"created": "Thu, 15 Nov 2007 13:01:20 GMT"
},
{
"version": "v3",
"created": "Wed, 5 Dec 2007 16:03:49 GMT"
},
{
"version": "v4",
"created": "Fri, 23 May 2008 11:21:40 GMT"
}
] | 2008-05-23T00:00:00 | [
[
"Verzelen",
"Nicolas",
"",
"INRIA Futurs"
],
[
"Villers",
"Fanny",
"",
"MIA"
]
] | [
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] |
711.212 | Takashi Fujita | S. G. Tan, M. B. A. Jalil, X. -J. Liu, T. Fujita | Non-Abelian gauge field effects and its relevance to spinning particle
dynamics in the technology of spintronics | 11 pages, 1 figure | null | null | null | quant-ph cond-mat.mes-hall | null | We describe formally the precession of spin vector about the k-space
effective magnetic field in condensed matter system with spin orbital effects
as constituting a local transformation of the electron wavefunction which
necessarily invokes the SU(2) transformation rule to ensure covariance. We
showed a "no-precession" condition as pre-requisite for the spin gauge field to
exert its influence on spin particle motion. The effects of the spin gauge
field on spin particle motion were shown to be consistent in both classical and
quantum pictures, which hence should underpin theoretical explanations for
important effects in anomalous Hall, spin Hall, spin torque, optical Magnus,
geometric quantum computation.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 06:59:00 GMT"
}
] | 2013-04-04T00:00:00 | [
[
"Tan",
"S. G.",
""
],
[
"Jalil",
"M. B. A.",
""
],
[
"Liu",
"X. -J.",
""
],
[
"Fujita",
"T.",
""
]
] | [
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] |
711.2121 | Rahul Basu | Rahul Basu (IMSc), P. N. Pandita (NEHU) and Chandradew Sharma (IMSc) | Radiative Neutralino Production in Low Energy Supersymmetric Models | LaTeX, 21 pages, 19 figures, figures and text added, version to
appear in Phys. Rev. D | Phys.Rev.D77:115009,2008 | 10.1103/PhysRevD.77.115009 | IMSc/2007/11/14 | hep-ph | null | We study the production of the lightest neutralinos in the radiative process
$e^+e^- \to \tilde\chi^0_1 \tilde\chi^0_1\gamma$ in low energy supersymmetric
models for the International Linear Collider energies. This includes the
minimal supersymmetric standard model as well as its extension with an
additional chiral Higgs singlet superfield, the nonminimal supersymmetric
standard model. We compare and contrast the dependence of the signal cross
section on the parameters of the neutralino sector of the minimal and
nonminimal supersymmetric standard model. We also consider the background to
this process coming from the Standard Model process $e^+e^- \to \nu \bar\nu
\gamma$, as well as from the radiative production of the scalar partners of the
neutrinos (sneutrinos) $e^+e^- \to \tilde\nu \tilde\nu^\ast \gamma$, which can
be a background to the radiative neutralino production when the sneutrinos
decay invisibly. In low energy supersymmetric models radiative production of
the lightest neutralinos may be the only channel to study supersymmetric
partners of the Standard Model particles at the first stage of a linear
collider, since heavier neutralinos, charginos and sleptons may be too heavy to
be pair-produced at a $e^+ e^-$ machine with $\sqrt{s} =500\GeV$.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 07:09:56 GMT"
},
{
"version": "v2",
"created": "Fri, 23 Nov 2007 14:51:32 GMT"
},
{
"version": "v3",
"created": "Tue, 1 Apr 2008 11:05:28 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Basu",
"Rahul",
"",
"IMSc"
],
[
"Pandita",
"P. N.",
"",
"NEHU"
],
[
"Sharma",
"Chandradew",
"",
"IMSc"
]
] | [
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-0.087008968,
-0.0612828769,
0.0667117685,
-0.0018784082,
-0.0160421263,
0.0258728191,
0.0289540812,
-0.0009644228,
-0.0638750494,
-0.0813844427,
-0.0517945476,
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] |
711.2122 | Mohammad Sami | R. Chingangbam, M. Sami, P. V. Tretyakov, A.V. Toporensky | A Note on the Viability of Gauss-Bonnet Cosmology | 6 latex pages, 4 eps figures, typos corrected and references added,
final version to appear in Phys. Lett. B | Phys.Lett.B661:162-166,2008 | 10.1016/j.physletb.2008.01.070 | null | hep-th astro-ph gr-qc hep-ph | null | In this paper, we analyze the viability of a vacuum Gauss-Bonnet cosmology by
examining the dynamics of the homogeneous and anisotropic background in 4+1
dimensions. The trajectories of the system either originate from the standard
singularity or from non-standard type, the later is characterized by the
divergence of time derivative of the Hubble parameters for its finite value. At
the onset, the system should relax to Einstein phase at late times as the
effect of Gauss-Bonnet term becomes negligible in the low energy regime.
However, we find that most of the trajectories emerging from the standard
big-bang singularity lead to future re-collapse whereas the system beginning
its evolution from the non-standard singularity enters the Kasner regime at
late times. This leads to the conclusion that the measure of trajectories
giving rise to a smooth evolution from a standard singularity to the Einstein
phase is negligibly small for generic initial conditions.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 07:34:11 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 08:50:37 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chingangbam",
"R.",
""
],
[
"Sami",
"M.",
""
],
[
"Tretyakov",
"P. V.",
""
],
[
"Toporensky",
"A. V.",
""
]
] | [
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] |
711.2123 | Volker Mayer | Volker Mayer and Mariusz Urba\'nski | Ergodic properties of sub-hyperbolic functions with polynomial
Schwarzian derivative | 25 pages | null | null | null | math.DS | null | The ergodic theory and geometry of the Julia set of meromorphic functions on
the complex plane with polynomial Schwarzian derivative is investigated under
the condition that the forward trajectory of asymptotic values in the Julia set
is bounded and the map $f$ restricted to its closure is expanding, the property
refered to as sub-expanding. We first show the existence, uniqueness,
conservativity and ergodicity of a conformal measure $m$ with minimal exponent
$h$; furthermore, we show weak metrical exactness of this measure. Then we
prove the existence of a $\sg$--finite invariant measure $\mu$ absolutely
continuous with respect to $m$. Our main result states that $\mu$ is finite if
and only if the order $\rho$ of the function $f$ satisfies the condition
$h>3\frac{\rho}{\rho +1}$. When finite, this measure is shown to be metrically
exact. We also establish a version of Bowen's formula showing that the exponent
$h$ equals the Hausdorff dimension of the Julia set of $f$.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 07:36:10 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Mayer",
"Volker",
""
],
[
"Urbański",
"Mariusz",
""
]
] | [
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] |
711.2124 | Kohei Hamaya | K. Hamaya, M. Kitabatake, K. Shibata, M. Jung, M. Kawamura, K.
Hirakawa, T. Machida, T. Taniyama, S. Ishida, and Y. Arakawa | Kondo effect in a semiconductor quantum dot coupled to ferromagnetic
electrodes | 4 pages, 3 figures | null | 10.1063/1.2820445 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | Using a laterally-fabricated quantum-dot (QD) spin-valve device, we
experimentally study the Kondo effect in the electron transport through a
semiconductor QD with an odd number of electrons (N). In a parallel magnetic
configuration of the ferromagnetic electrodes, the Kondo resonance at N = 3
splits clearly without external magnetic fields. With applying magnetic fields
(B), the splitting is gradually reduced, and then the Kondo effect is almost
restored at B = 1.2 T. This means that, in the Kondo regime, an inverse
effective magnetic field of B ~ 1.2 T can be applied to the QD in the parallel
magnetic configuration of the ferromagnetic electrodes.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:07:02 GMT"
},
{
"version": "v2",
"created": "Sun, 16 Dec 2007 02:48:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hamaya",
"K.",
""
],
[
"Kitabatake",
"M.",
""
],
[
"Shibata",
"K.",
""
],
[
"Jung",
"M.",
""
],
[
"Kawamura",
"M.",
""
],
[
"Hirakawa",
"K.",
""
],
[
"Machida",
"T.",
""
],
[
"Taniyama",
"T.",
""
],
[
"Ishida",
"S.",
""
],
[
"Arakawa",
"Y.",
""
]
] | [
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] |
711.2125 | Jose Antonio Oller | J.A. Oller, L. Roca, C. Schat | Scalar radius of the pion and two photons into two pions. Strong S-wave
final state interactions | 10 pages, 1 figure. Invited talk at the 11th International Conference
on Meson-Nucleon Physics and the Structure of the Nucleon (MENU 2007),
September 10-14, 2007, IKP, Forschungzentrum J\"ulich, Germany | ECONFC070910:156,2007 | null | null | hep-ph | null | The quadratic pion scalar radius, <r^2>^\pi_s, plays an important role for
present precise determinations of \pi\pi scattering. The solution of the
Muskhelishvili-Omn\`es equations for the non-strange null isospin (I) pion
scalar form factor determines that <r^2>^\pi_s=(0.61\pm 0.04) fm^2. However, by
using an Omn\`es representation of this form factor, Yndur\'ain recently
obtains <r^2>^\pi_s=(0.75\pm 0.07) fm^2. A large discrepancy between both
values, given the precision, then results. We show that Yndur\'ain's method is
indeed compatible with the determinations from the Muskhelishvili-Omn\`es
equations once a zero in the scalar form factor for some S-wave I=0 T-matrices
is considered. Once this is accounted for, the resulting value is
<r^2>^\pi=(0.63\pm 0.05) fm^2.
On the other hand, we perform a theoretical study of the reaction
\gamma\gamma\to \pi^0\pi^0 based on dispersion relations. The large source of
uncertainty for \sqrt{s}\gtrsim 0.5 GeV, due to variations in the phase used in
the Omn\`es function above the K\bar{K} threshold, is removed by taking one
more subtraction in the dispersion relation. This allows us to make sharper
predictions for the cross section so that one could use this reaction to
distinguish between different low energy \pi\pi parameterizations, once
independent experiments are available. We also study the role played by the
\sigma or f_0(600) meson in this reaction and determine its width to two
photons.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 07:59:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Oller",
"J. A.",
""
],
[
"Roca",
"L.",
""
],
[
"Schat",
"C.",
""
]
] | [
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] |
711.2126 | Ray-Kuang Lee | Tsin-Dong Lee, Chih-Yao Chen, YuanYao Lin, Chia-Yu Chang, Ming-Chiu
Chou, Hung-Pin D. Yang, Te-ho Wu, and Ray-Kuang Lee | Direct observation of higher-order whispering-gallery modes in VCSELs at
room temperature by embedding a defect-free surface micro-structure | null | null | null | null | physics.optics | null | We propose and demonstrate a direct method to observe higher-order
whispering-gallery modes in vertical cavity surface emitting lasers (VCSELs) at
room temperature. Instead of introducing any defect mode, we show that
suppression of lower-order cavity modes can be achieved by destroying vertical
reflectors with a surface micro-structure. Up to the 23rd azimuthal order
whispering-gallery mode confined laterally by the native oxide layers is
observed in experiments through collecting near-field radiation patterns.
Various vertical emission transverse modes are identified by the spectrum in
experiments as well as numerical simulations.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:25:56 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Lee",
"Tsin-Dong",
""
],
[
"Chen",
"Chih-Yao",
""
],
[
"Lin",
"YuanYao",
""
],
[
"Chang",
"Chia-Yu",
""
],
[
"Chou",
"Ming-Chiu",
""
],
[
"Yang",
"Hung-Pin D.",
""
],
[
"Wu",
"Te-ho",
""
],
[
"Lee",
"Ray-Kuang",
""
]
] | [
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] |
711.2127 | Pascu Catalin Moca | C. P. Moca and D. C. Marinescu | Spin-Hall conductivity of a spin-polarized two-dimensional electron gas
with Rashba spin-orbit interaction and magnetic impurities | 13 pages, 5 figures | New Journal of Physics 9, 343 (2007) | 10.1088/1367-2630/9/9/343 | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | The Kubo formula is used to calculate the spin-Hall conductivity in a
spin-polarized two-dimensional electron system with Rashba-type spin-orbit
interaction. As in the case of the unpolarized electron system, spin Hall
conductivity is entirely determined by states at the Fermi level, a property
that persists in the presence of magnetic impurities. In the clean limit, the
spin-Hall conductivity decreases monotonically with the Zeeman splitting, a
result of the ordering effect on the electron spins produced by the magnetic
field. In the presence of magnetic impurities, the spin-dependent scattering
determines a finite renormalization of the static part of the fully dressed
vertex correction of the velocity operator that leads to an enhancement of the
\sigma_{sH}, an opposite behaviour to that registered in the presence of
spin-independent disorder. The variation of \sigma_{sH} with the strength of
the Rashba coupling and the Zeeman splitting is studied.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:33:00 GMT"
},
{
"version": "v2",
"created": "Thu, 15 Nov 2007 10:02:44 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Moca",
"C. P.",
""
],
[
"Marinescu",
"D. C.",
""
]
] | [
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] |
711.2128 | Alexander Premet | Alexander Premet | Support varieties of non-restricted modules over Lie algebras of
reductive groups: corrigenda and addenda | 6 pages | null | null | null | math.RT math.RA | null | This paper fixes a gap in my article "Support varieties of non-restricted
modules over Lie algebras of reductive groups" pointed out to me by J.C.
Jantzen. It was written several years ago, but never widely circulated.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:39:01 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Premet",
"Alexander",
""
]
] | [
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] |
711.2129 | Frank Pollmann | P. Fulde, F. Pollmann | Strings in strongly correlated electron systems | 6 | AnnalenPhys.17:441-449,1997 | 10.1002/andp.200810309 | null | cond-mat.str-el | null | It is shown that strongly correlated electrons on frustrated lattices like
pyrochlore, checkerboard or kagome lattice can lead to the appearance of closed
and open strings. They are resulting from nonlocal subsidiary conditions which
propagating strongly correlated electrons require. The dynamics of the strings
is discussed and a number of their properties are pointed out. Some of them are
reminiscent of particle physics.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:40:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Fulde",
"P.",
""
],
[
"Pollmann",
"F.",
""
]
] | [
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] |
711.213 | Artem Sabourov | S.P. Knurenko, A.V. Sabourov, and I.Ye. Sleptsov | Behavior of some characteristics of EAS in the region of knee and ankle
of spectrum | 6 pages, 9 figures | null | null | null | astro-ph | null | The energy dependence of such characteristics as a ratio of the total number
of charged particles to the total flux of EAS Cherenkov radiation, a ratio of
E(thr)>=1GeV muon flux density at the distance of 600m from a shower core to
charged particle flux density, a ratio of the energy transferred to the
electromagnetic component of EAS to the primary particle energy is presented.
Their comparison with two-component mass composition of cosmic rays (p-Fe) in
the framework of calculations by a QGSJET model is given.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:45:18 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Knurenko",
"S. P.",
""
],
[
"Sabourov",
"A. V.",
""
],
[
"Sleptsov",
"I. Ye.",
""
]
] | [
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] |
711.2131 | Ting-Wai Chiu | TWQCD Collaboration: Ting-Wai Chiu, Tung-Han Hsieh, Chao-Hsi Huang,
Kenji Ogawa | Dirac b quark on the lattice | 7 pages, 1 figure, Proceedings of Lattice 2007, Regensburg, Germany,
July 30 - August 4, 2007 | PoS LAT2007:105,2007 | null | NTUTH-07-505F | hep-lat hep-ex hep-ph | null | We perform the first study of treating b, c, and s quarks as Dirac fermions
in lattice QCD with exact chiral symmetry. On a 32^3 60 lattice with 1/a ~ 7.68
GeV, we compute point-to-point quark propagators, and measure the
time-correlation functions for mesons with quark contents b_bbar, c_bbar,
s_bbar, and c_cbar. The lowest-lying meson mass spectra, the pseudoscalar decay
constants, and the b and c quark masses are determined.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:42:48 GMT"
}
] | 2011-02-16T00:00:00 | [
[
"TWQCD Collaboration",
"",
""
],
[
"Chiu",
"Ting-Wai",
""
],
[
"Hsieh",
"Tung-Han",
""
],
[
"Huang",
"Chao-Hsi",
""
],
[
"Ogawa",
"Kenji",
""
]
] | [
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] |
711.2132 | Hiroshi Suzuki | Issaku Kanamori, Fumihiko Sugino and Hiroshi Suzuki | Observing dynamical supersymmetry breaking with euclidean lattice
simulations | 35 pages, 9 figures, the final version to appear in Prog. Theor. Phys | Prog.Theor.Phys.119:797-827,2008 | 10.1143/PTP.119.797 | RIKEN-TH-122, OIQP-07-16 | hep-lat hep-th | null | A strict positivity of the ground-state energy is a necessary and sufficient
condition for spontaneous supersymmetry breaking. This ground-state energy may
be directly determined from the expectation value of the Hamiltonian in the
functional integral, defined with an \emph{antiperiodic} temporal boundary
condition for all fermionic variables. We propose to use this fact to observe
the dynamical spontaneous supersymmetry breaking in Euclidean lattice
simulations. If a lattice formulation possesses a manifestly preserved
fermionic symmetry, there exists a natural choice of a Hamiltonian operator
that is consistent with a topological nature of the Witten index. We
numerically confirm the validity of our idea in models of supersymmetric
quantum mechanics. We further examine the possibility of dynamical
supersymmetry breaking in the two-dimensional $\mathcal{N}=(2,2)$ super
Yang-Mills theory with the gauge group SU(2), for which the Witten index is
unknown. Although statistical errors are still large, we do not observe
positive ground-state energy, at least within one standard deviation. This
prompts us to draw a different conclusion from a recent conjectural claim that
supersymmetry is dynamically broken in this system.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 08:57:11 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 00:55:33 GMT"
},
{
"version": "v3",
"created": "Fri, 23 May 2008 00:32:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kanamori",
"Issaku",
""
],
[
"Sugino",
"Fumihiko",
""
],
[
"Suzuki",
"Hiroshi",
""
]
] | [
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] |
711.2133 | A. K. Chaudhuri | A. K. Chaudhuri | $J/\psi$ suppression in the threshold model at RHIC and LHC energy | 9 pages, 9 figures | J.Phys.G35:065105,2008 | 10.1088/0954-3899/35/6/065105 | null | nucl-th | null | In the QGP based threshold model \cite{Blaizot:2000ev,Blaizot:1996nq}, in
addition to the normal nuclear absorption, $J/\psi$'s are subjected to an
'anomalous' suppression such that above a threshold density $n_{J/\psi}$, all
the $J/\psi$'s are melted. In the threshold model we have analysed the recent
PHENIX data on the centrality dependence of $J/\psi$ suppression in Au+Au
collisions at RHIC. Feedback from decay of the state $\chi$ is accounted for.
$J/\psi$'s are anomalously suppressed above a threshold density,
$n_{J/\psi}=3.57\pm 0.17$ $fm^{-2}$. Threshold density for anomalous
suppression of the state $\chi$ is uncertain to a large extent, $n_\chi=0.32
\pm 0.32$ $fm^{-2}$. The fraction $F$ of the state $\chi$ can not be determined
unambiguously, depending on the nuclear absorption, it can vary from 20% to
40%. We have also predicted for the suppression in Pb+Pb collisions at LHC
energy. In central Pb+Pb collisions, $J/\psi$'s are suppressed by a factor of
3-4. Suppression pattern is rather similar to that in Au+Au collisions, if not
slighty less in central collisions. Using the PHENIX data on the participant
number dependence of the Bjorken energy density, we have also estimated the QGP
formation time. For critical temperature $T_c$=192 MeV, estimated QGP formation
time ranges between 0.07-0.09 fm/c.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:00:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chaudhuri",
"A. K.",
""
]
] | [
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711.2134 | Tetsu Mizumachi | Tetsu Mizumachi | Asymptotic stability of lattice solitons in the energy space | 19pages | null | null | null | math.AP math-ph math.MP | null | Orbital and asymptotic stability for 1-soliton solutions to the Toda lattice
equations as well as small solitary waves to the FPU lattice equations are
established in the energy space. Unlike analogous Hamiltonian PDEs, the lattice
equations do not conserve momentum. Furthermore, the Toda lattice equation is a
bidirectional model that does not fit in with existing theory for Hamiltonian
system by Grillakis, Shatah and Strauss.
To prove stability of 1-soliton solutions, we split a solution around a
1-soliton into a small solution that moves more slowly than the main solitary
wave, and an exponentially localized part. We apply a decay estimate for
solutions to a linearized Toda equation which has been recently proved by
Mizumachi and Pego to estimate the localized part. We improve the asymptotic
stability results for FPU lattices in a weighted space obtained by Friesecke
and Pego.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:01:57 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Mizumachi",
"Tetsu",
""
]
] | [
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] |
711.2135 | Masanori Hino | Masanori Hino | Martingale dimensions for fractals | 22 pages, 1 figure | Annals of Probability, Vol. 36, No. 3 (2008), 971-991 | 10.1214/07-AOP349 | null | math.PR | null | We prove that the martingale dimensions for canonical diffusion processes on
a class of self-similar sets including nested fractals are always one. This
provides an affirmative answer to the conjecture of S. Kusuoka [Publ. Res.
Inst. Math. Sci. 25 (1989) 659--680].
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:18:29 GMT"
}
] | 2008-04-22T00:00:00 | [
[
"Hino",
"Masanori",
""
]
] | [
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-0.0125952279,
-0.059227135,
0.0640050471
] |
711.2136 | Jeremy Shears | Jeremy Shears, Steve Brady, Jerry Foote, Donn Starkey, Tonny
Vanmunster | The orbital and superhump periods of the deeply eclipsing dwarf nova
SDSS J122740.83+513925.9 | Accepted for publication in the Journal of the British Astronomical
Association. 12 pages, 9 figures | null | null | null | astro-ph | null | During June 2007 the first confirmed superoutburst of the eclipsing dwarf
nova SDSS J122740.83+513925.9 was observed using CCD photometry. The outburst
amplitude was at least 4.7 magnitudes. The orbital period was measured as
0.06296(5) d from times of the 31 observed eclipses. Time series photometry
also revealed superhumps with a period of 0.0653(3) d, thereby establishing it
to be a UGSU-type system. The superhump period excess was 3.7% and the maximum
peak-to-peak amplitude of the superhumps was 0.35 magnitudes. The eclipse
duration declined from a maximum of 23 min at the peak of the outburst to about
12 mins towards the end. The depth of the eclipses was correlated with the beat
period between the orbital and superhump periods.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:24:40 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Shears",
"Jeremy",
""
],
[
"Brady",
"Steve",
""
],
[
"Foote",
"Jerry",
""
],
[
"Starkey",
"Donn",
""
],
[
"Vanmunster",
"Tonny",
""
]
] | [
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] |
711.2137 | Gerasimos Dousmanis | Gerasimos Dousmanis | Rank two filtered $(\phi, N)$-modules with Galois descent data and
coefficients | Final version. To appear in Trans. A.M.S | null | null | null | math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $K$ be any finite extension of $Q_{p}$, $L$ any finite Galois extension
of $K$ and $E$ any finite large enough coefficient field containing $L$. We
classify two-dimensional, F-semistable $E$-representations of $G_{K}$, by
listing the isomorphism classes of rank two weakly admissible filtered
$(\phi,N,L/K,E)$-modules.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:28:55 GMT"
},
{
"version": "v2",
"created": "Mon, 20 Oct 2008 15:36:38 GMT"
},
{
"version": "v3",
"created": "Tue, 19 May 2009 07:12:52 GMT"
}
] | 2009-05-19T00:00:00 | [
[
"Dousmanis",
"Gerasimos",
""
]
] | [
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] |
711.2138 | Michael Ruzhansky | Michael Ruzhansky and James Smith | Dispersive and Strichartz estimates for hyperbolic equations with
constant coefficients | 119 pages | MSJ Memoirs, 22, Mathematical Society of Japan, Tokyo, 2010. | null | null | math.AP math.FA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Dispersive and Strichartz estimates for solutions to general strictly
hyperbolic partial differential equations with constant coefficients are
considered. The global time decay estimates of $L^p-L^q$ norms of propagators
are obtained, and it is shown how the time decay rates depend on the geometry
of the problem. The frequency space is separated in several zones each giving a
certain decay rate. Geometric conditions on characteristics responsible for the
particular decay are identified and investigated. Thus, a comprehensive
analysis is carried out for strictly hyperbolic equations of high orders with
lower order terms of a general form. Results are applied to establish time
decay estimates for the Fokker-Planck equation and for semilinear hyperbolic
equations.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:31:41 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Dec 2009 20:29:51 GMT"
}
] | 2010-04-27T00:00:00 | [
[
"Ruzhansky",
"Michael",
""
],
[
"Smith",
"James",
""
]
] | [
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] |
711.2139 | Damien Dornic | J. Carr, D. Dornic, F. Jouvenot, G. Maurin (for the KM3NeT consortium) | Configuration studies for a cubic-kilometre deep-sea neutrino telescope
- KM3NeT - with NESSY, a fast and flexible approach | 4 pages, 5 figures, contribution for the 30th International Cosmic
Ray conference | null | null | null | astro-ph | null | Theoretical predictions for neutrino fluxes indicate that km$^{3}$ scale
detectors are needed to detect certain astrophysical sources. The three
Mediterranean experiments, ANTARES, NEMO and NESTOR are working together on a
design study, KM3NeT, for a large deep-sea neutrino telescope. A detector
placed in the Mediterranean Sea will survey a large part of the Galactic disc,
including the Galactic Centre. It will complement the IceCube telescope
currently under construction at the South Pole. Furthermore, the improved
optical properties of sea water, compared to Antarctic ice, will allow a better
angular resolution and hence better background rejection.
The main work presented in this paper is to evaluate different km$^{3}$ scale
detector geometries in order to optimize the muon neutrino sensitivity between
1 and 100 TeV. For this purpose, we have developed a detailed simulation based
on the {\it Mathematica} software - for the muon track production, the light
transmission in water, the environmental background and the detector response.
To compare different geometries, we have mainly used the effective neutrino
area obtained after the full standard reconstruction chain.}
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:41:30 GMT"
}
] | 2019-08-14T00:00:00 | [
[
"Carr",
"J.",
"",
"for the KM3NeT consortium"
],
[
"Dornic",
"D.",
"",
"for the KM3NeT consortium"
],
[
"Jouvenot",
"F.",
"",
"for the KM3NeT consortium"
],
[
"Maurin",
"G.",
"",
"for the KM3NeT consortium"
]
] | [
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] |
711.214 | Erik Sjoqvist | David Kult, Johan {\AA}berg, Erik Sj\"oqvist | Holonomy for Quantum Channels | Minor changes, journal reference added | Phys. Rev. A 77, 012114 (2008) | 10.1103/PhysRevA.77.012114 | null | quant-ph | null | A quantum holonomy reflects the curvature of some underlying structure of
quantum mechanical systems, such as that associated with quantum states. Here,
we extend the notion of holonomy to families of quantum channels, i.e., trace
preserving completely positive maps. By the use of the Jamio{\l}kowski
isomorphism, we show that the proposed channel holonomy is related to the
Uhlmann holonomy. The general theory is illustrated for specific examples. We
put forward a physical realization of the channel holonomy in terms of
interferometry. This enables us to identify a gauge invariant physical object
that directly relates to the channel holonomy. Parallel transport condition and
concomitant gauge structure are delineated in the case of smoothly parametrized
families of channels. Finally, we point out that interferometer tests that have
been carried out in the past to confirm the $4\pi$ rotation symmetry of the
neutron spin, can be viewed as early experimental realizations of the channel
holonomy.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:53:54 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jan 2008 08:18:44 GMT"
}
] | 2016-03-28T00:00:00 | [
[
"Kult",
"David",
""
],
[
"Åberg",
"Johan",
""
],
[
"Sjöqvist",
"Erik",
""
]
] | [
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] |
711.2141 | Nicola Manini | L. Salasnich, N. Manini and F. Toigo | Macroscopic Periodic Tunneling of Fermi Atoms in the BCS-BEC Crossover | 6 pages 3 figures revtex | Phys. Rev. A 77, 043609 (2008) | 10.1103/PhysRevA.77.043609 | null | cond-mat.stat-mech cond-mat.soft cond-mat.supr-con | null | We study the macroscopic quantum tunneling of two weakly-linked superfluids
made of interacting fermionic atoms. We derive atomic Josephson junction
equations and find that zero-mode and pi-mode frequencies of coherent atomic
oscillations depend on the tunneling coefficient and the sound velocity of the
superfluid. By considering a superfluid of ^40K atoms, we calculate these
oscillation frequencies in the crossover from the Bardeen-Cooper-Schrieffer
state of weakly-bound Cooper pairs to the Bose-Einstein Condensate of
strongly-bound molecular dimers.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 09:59:14 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Dec 2007 16:13:25 GMT"
},
{
"version": "v3",
"created": "Mon, 17 Mar 2008 10:52:12 GMT"
}
] | 2008-04-09T00:00:00 | [
[
"Salasnich",
"L.",
""
],
[
"Manini",
"N.",
""
],
[
"Toigo",
"F.",
""
]
] | [
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] |
711.2142 | Jean-Philippe Beaulieu | J.P. Beaulieu, S. Carey, I. Ribas, G. Tinetti | Primary transit of the planet HD189733b at 3.6 and 5.8 microns | 6 pages, 4 figures, Astrophysical Journal 675. Accepted Nov 21,
20007, to appear on March 10, 2008 | Astrophys.J.677:1343-1347,2008 | 10.1086/527045 | null | astro-ph | null | The hot Jupiter HD 189733b was observed during its primary transit using the
Infrared Array Camera on the Spitzer Space Telescope. The transit depths were
measured simultaneously at 3.6 and 5.8 microns. Our analysis yields values of
2.356 +- 0.019 % and 2.436 +- 0.020$ % at 3.6 and 5.8 microns respectively, for
a uniform source. We estimated the contribution of the limb-darkening and
star-spot effects on the final results. We concluded that although the limb
darkening increases by ~0.02-0.03 % the transit depths, and the differential
effects between the two IRAC bands is even smaller, 0.01 %. Furthermore, the
host star is known to be an active spotted K star with observed photometric
modulation. If we adopt an extreme model of 20 % coverage with spots 1000K
cooler of the star surface, it will make the observed transits shallower by
0.19 and 0.18 %. The difference between the two bands will be only of 0.01 %,
in the opposite direction to the limb darkening correction. If the transit
depth is affected by limb darkening and spots, the differential effects between
the 3.6 and 5.8 microns bands are very small. The differential transit depths
at 3.6 and 5.8 microns and the recent one published by Knutson et al.(2007) at
8 microns are in agreement with the presence of water vapour in the upper
atmosphere of the planet. This is the companion paper to Tinetti et al.
(2007b), where the detailed atmosphere models are presented.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:02:48 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 11:47:30 GMT"
}
] | 2010-03-01T00:00:00 | [
[
"Beaulieu",
"J. P.",
""
],
[
"Carey",
"S.",
""
],
[
"Ribas",
"I.",
""
],
[
"Tinetti",
"G.",
""
]
] | [
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] |
711.2143 | Timothy Johnson | Andrew J. F. Jack, Timothy C. Johnson, Mihail Zervos | A Singular Control Model with Application to the Goodwill Problem | null | null | null | null | math.PR math.OC | null | We consider a stochastic system whose uncontrolled state dynamics are
modelled by a general one-dimensional It\^{o} diffusion. The control effort
that can be applied to this system takes the form that is associated with the
so-called monotone follower problem of singular stochastic control. The control
problem that we address aims at maximising a performance criterion that rewards
high values of the utility derived from the system's controlled state but
penalises any expenditure of control effort. This problem has been motivated by
applications such as the so-called goodwill problem in which the system's state
is used to represent the image that a product has in a market, while control
expenditure is associated with raising the product's image, e.g., through
advertising. We obtain the solution to the optimisation problem that we
consider in a closed analytic form under rather general assumptions. Also, our
analysis establishes a number of results that are concerned with analytic as
well as probabilistic expressions for the first derivative of the solution to a
second order linear non-homogeneous ordinary differential equation. These
results have independent interest and can potentially be of use to the solution
of other one-dimensional stochastic control problems.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 20:46:06 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Jack",
"Andrew J. F.",
""
],
[
"Johnson",
"Timothy C.",
""
],
[
"Zervos",
"Mihail",
""
]
] | [
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] |
711.2144 | Masanori Hino | Masanori Hino and Hiroto Uchida | Reflecting Ornstein-Uhlenbeck processes on pinned path spaces | 19 pages | Proceedings of RIMS Workshop on Stochastic Analysis and
Applications, 111-128, RIMS Kokyuroku Bessatsu, B6, Res. Inst. Math. Sci.
(RIMS), Kyoto, 2008 | null | null | math.PR | null | Consider a set of continuous maps from the interval $[0,1]$ to a domain in
${\mathbb R}^d$. Although the topological boundary of this set in the path
space is not smooth in general, by using the theory of functions of bounded
variation (BV functions) on the Wiener space and the theory of Dirichlet forms,
we can discuss the existence of the surface measure and the Skorokhod
representation of the reflecting Ornstein-Uhlenbeck process associated with the
canonical Dirichlet form on this set.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:08:20 GMT"
}
] | 2008-04-22T00:00:00 | [
[
"Hino",
"Masanori",
""
],
[
"Uchida",
"Hiroto",
""
]
] | [
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] |
711.2145 | Damien Dornic | J. Carr, D. Dornic, F. Jouvenot, U.F. Katz, S. Kuch, G. Maurin, R.
Shanidze (for the KM3NeT consortium) | Sensitivity studies for the cubic-kilometre deep-sea neutrino telescope
KM3NeT | 4 pages, 1 figure, contribution of the 30th International Cosmic Ray
conference | null | null | null | astro-ph | null | The observation of high-energy neutrinos from astrophysical sources would
substantially improve our knowledge and understanding of the non-thermal
processes in these sources, and would in particular pinpoint the accelerators
of cosmic rays. The sensitivity of different design options for a future
cubic-kilometre scale neutrino telescope in the Mediterranean Sea is
investigated for generic point sources and in particular for some of the
galactic objects from which TeV gamma emmission has recently been observed by
the H.E.S.S. atmospheric Cherenkov telescope. The effect of atmospheric
background on the source detection probabilities has been taken into account
through full simulation. The estimated event rates are compared to previous
results and limits from present neutrino telescopes.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:09:00 GMT"
}
] | 2019-08-14T00:00:00 | [
[
"Carr",
"J.",
"",
"for the KM3NeT consortium"
],
[
"Dornic",
"D.",
"",
"for the KM3NeT consortium"
],
[
"Jouvenot",
"F.",
"",
"for the KM3NeT consortium"
],
[
"Katz",
"U. F.",
"",
"for the KM3NeT consortium"
],
[
"Kuch",
"S.",
"",
"for the KM3NeT consortium"
],
[
"Maurin",
"G.",
"",
"for the KM3NeT consortium"
],
[
"Shanidze",
"R.",
"",
"for the KM3NeT consortium"
]
] | [
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] |
711.2146 | Fethi Mahmoudi | Mouhamed Moustapha Fall and Fethi Mahmoudi | Hypersurfaces with free boundary and large constant mean curvature:
concentration along submanifolds | 28 pages | null | null | null | math.AP math.DG | null | Given a domain $\Omega$ of $\mathbb{R}^{m+1}$ and a $k$-dimensional
non-degenerate minimal submanifold $K$ of $\pa \Omega$ with $1\le k\le m-1$, we
prove the existence of a family of embedded constant mean curvature
hypersurfaces which as their mean curvature tends to infinity concentrate along
$K$ and intersecting $\partial \Omega$ perpendicularly.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:13:38 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Fall",
"Mouhamed Moustapha",
""
],
[
"Mahmoudi",
"Fethi",
""
]
] | [
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] |
711.2147 | Gilles Maurin | G. Maurin, A. Djannati-Atai, P. Espigat | A Deconvolution technique for VHE Gamma-ray Astronomy, and its
application to the morphological study of shell-type supernova remnants | 4 pages, 3 figures, contribution for the 30th International Cosmic
Ray Conference | null | null | null | astro-ph | null | Deconvolution algorithms have been used successfully for
optimization/restoration/deblurring of astronomical images in a variety of
wavelengths, especially in the optical band (e.g., for HST). We present here an
iterative Richardson-Lucy type method designed for treatment of images obtained
with the H.E.S.S. array of ground-based gamma-ray telescopes. Its application
to shell-type supernova remnant images yields refined details relevant for the
study of correlations with other wavelengths, and hence for interpretation in
terms either of hadronic or leptonic origin of the observed VHE gamma-ray
emission.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:21:54 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Maurin",
"G.",
""
],
[
"Djannati-Atai",
"A.",
""
],
[
"Espigat",
"P.",
""
]
] | [
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] |
711.2148 | J\"urgen Blum | Doreen Langkowski, Jens Teiser, J\"urgen Blum | The Physics of Protoplanetesimal Dust Agglomerates II. Low Velocity
Collision Properties | 46 pages, 1 table, 16 figures | null | 10.1086/525841 | null | astro-ph | null | For the investigation of collisions among protoplanetesimal dust aggregates,
we performed microgravity experiments in which the impacts of high-porosity
mm-sized dust aggregates into 2.5 cm-sized high-porosity dust aggregates can be
studied. The dust aggregates consisted of micrometer-sized dust grains and were
produced by random ballistic deposition with porosities between 85% and 93%.
Impact velocities ranged from ~0.1 m/s to ~3 m/s and impact angles were almost
randomly distributed. We also used "molded" target aggregates such that the
radii of the local surface curvatures corresponded to the projectile radii. The
experiments showed that impacts into the highest-porosity targets almost always
led to sticking, whereas for the less porous dust aggregates, the collisions
with intermediate velocities and high impact angles resulted in the bouncing of
the projectile with a mass transfer from the target to the projectile
aggregate. Sticking probabilities for the impacts into the "molded" target
aggregates were considerably decreased. For the impacts into smooth targets, we
measured the depth of intrusion and the crater volume and could derive some
interesting dynamical properties which can help to derive a collision model for
protoplanetesimal dust aggregates. Future models of the aggregate growth in
protoplanetary disks should take into account non-central impacts, impact
compression, the influence of the local radius of curvature on the collisional
outcome and the possible mass transfer between target and projectile
agglomerates in non-sticking collisions.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:48:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Langkowski",
"Doreen",
""
],
[
"Teiser",
"Jens",
""
],
[
"Blum",
"Jürgen",
""
]
] | [
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] |
711.2149 | Jan Pomplun | Jan Pomplun, Sven Burger, Lin Zschiedrich, Frank Schmidt | Adaptive Finite Element Method for Simulation of Optical Nano Structures | null | phys. stat. sol. (b), 244, No. 10, 3419-3434 (2007) | 10.1002/pssb.200743192 | null | physics.optics | null | We discuss realization, properties and performance of the adaptive finite
element approach to the design of nano-photonic components. Central issues are
the construction of vectorial finite elements and the embedding of bounded
components into the unbounded and possibly heterogeneous exterior. We apply the
finite element method to the optimization of the design of a hollow core
photonic crystal fiber. Thereby we look at the convergence of the method and
discuss automatic and adaptive grid refinement and the performance of higher
order elements.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:39:56 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Pomplun",
"Jan",
""
],
[
"Burger",
"Sven",
""
],
[
"Zschiedrich",
"Lin",
""
],
[
"Schmidt",
"Frank",
""
]
] | [
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] |
711.215 | Jean-Christophe Aval | Jean-Christophe Aval (LaBRI) | Keys and alternating sign matrices | null | Seminaire Lotharingien de Combinatoire 59 (2008) B59f | null | null | math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Lascoux and Sch\"utzenberger introduced a notion of key associated to any
Young tableau. More recently Lascoux defined the key of an alternating sign
matrix by recursively removing all -1's in such matrices. But alternating sign
matrices are in bijection with monotone triangles, which form a subclass of
Young tableaux. We show that in this case these two notions of keys coincide.
Moreover we obtain an elegant and direct way to compute the key of any Young
tableau, and discuss consequences of our result.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:29:09 GMT"
},
{
"version": "v2",
"created": "Mon, 18 May 2009 08:21:18 GMT"
}
] | 2009-05-18T00:00:00 | [
[
"Aval",
"Jean-Christophe",
"",
"LaBRI"
]
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711.2151 | Sinya Aoki | Sinya Aoki | Hadron interactions from lattice QCD | 15 pages, 10 figures, Plenary talk presented at the XXVth
International Symposium on Lattice Field Theory, July 30 - August 4, 2007,
Regensburg, Germany | PoSLAT2007:002,2007 | null | null | hep-lat nucl-th | null | Studies on hadron interactions from lattice QCD are reviewed. The $S$-wave
$\pi\pi$ scattering lengths of the I=0 and I=2 channels are extracted from
various lattice determinations of low energy constants in $N_f=2$ chiral
perturbation theory. The results agree with each other and agree also with
other non-lattice estimates. Recently the $P$-wave $\pi\pi$ scattering phase
shift for the I=1 channel has been calculated. A preliminary estimate of the
$\rho$ meson decay width from the phase shift is consistent with the
experimental value. Two approaches to potentials between hadrons are discussed.
One is a method using static quarks to define the distance between two hadrons.
The other is a method to define a potential from a wave function of two
hadrons. An application of the latter to the nucleon-nucleon ($NN$) potential
turns out to reproduce qualitative features of the phenomenological $NN$
potential such as attraction at long distance and repulsion at short distance.
Theoretical issues of this approach are also discussed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:34:13 GMT"
}
] | 2009-04-14T00:00:00 | [
[
"Aoki",
"Sinya",
""
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711.2152 | Paul David Mitchener | Paul D. Mitchener | $KK$-theory spectra for $C^\ast$-categories and discrete groupoid
$C^\ast$-algebras | null | null | null | null | math.KT math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we refine a version of bivariant $K$-theory developed by Cuntz
to define symmetric spectra representing the $KK$-theory of $C^\ast$-categories
and discrete groupoid $C^\ast$-algebras. In both cases, the Kasparov product
can be expressed as a smash product of spectra.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:39:43 GMT"
},
{
"version": "v2",
"created": "Fri, 6 Jun 2008 12:30:22 GMT"
}
] | 2008-06-06T00:00:00 | [
[
"Mitchener",
"Paul D.",
""
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] |
711.2153 | Ayesha Begum Dr | Jayaram N. Chengalur, Ayesha Begum, I. D. Karachentsev, Margarita
Sharina, S. S. Kaisin | Gas rich galaxies from the FIGGS survey | 5 Pages, 4 Figures. To be published in the proceedings of "Galaxies
in the Local Volume", ed. B. Koribalski, H. Jerjen | null | 10.1007/978-1-4020-6933-8_13 | null | astro-ph | null | The FIGGS (Faint Irregular Galaxy GMRT Survey) is aimed at creating a
multi-wavelength observational data base for a volume limited sample of the
faintest gas rich galaxies. In this paper we discuss two very gas rich galaxies
that were observed as part of the FIGGS survey, viz. NGC 3741 and And IV. These
galaxies are unusual in that they have extremely extended gas disks and very
high ratios of dark to luminous matter. The very extended HI disks provide an
unique opportunity to trace the extended distribution of dark matter around
faint galaxies. We compare the baryon fraction of these galaxies with a sample
of galaxies with well measured rotation curves and discuss whether extremely
gas rich dwarf galaxies have abnormally small baryon fractions.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:44:38 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Chengalur",
"Jayaram N.",
""
],
[
"Begum",
"Ayesha",
""
],
[
"Karachentsev",
"I. D.",
""
],
[
"Sharina",
"Margarita",
""
],
[
"Kaisin",
"S. S.",
""
]
] | [
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] |
711.2154 | Rainer Rolffs | Rainer Rolffs, Peter Schilke, Claudia Comito, Carolin Hieret,
Friedrich Wyrowski | Hot Cores in the submm - obscured by dust? | 4 pages, 3 figures, to appear in "Science with ALMA: a new era for
Astrophysics" Conference Proceedings (to be published by Springer
"Astrophysics and Space Science (ApSS)") | null | null | null | astro-ph | null | We present APEX observations of HCN (9-8) and (4-3) lines toward a sample of
hot cores. The spectral shapes of the main transitions are asymmetric and
self-absorbed, as expected for high optical depth in a possibly infalling
envelope. For spherical symmetry, the large column densities of these sources
would mean that the central region is obscured by dust above a certain
frequency. However, we detected the vibrationally excited satellite lines
(v_2=1; J=9-8) at 797 GHz, which originate from the inner regions. This
indicates that high-frequency ALMA observations of hot core centers will be
feasible.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:54:02 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Rolffs",
"Rainer",
""
],
[
"Schilke",
"Peter",
""
],
[
"Comito",
"Claudia",
""
],
[
"Hieret",
"Carolin",
""
],
[
"Wyrowski",
"Friedrich",
""
]
] | [
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] |
711.2155 | Stijn Heymans | Stijn Heymans, Jos de Bruijn, Livia Predoiu, Cristina Feier, Davy Van
Nieuwenborgh | Guarded Hybrid Knowledge Bases | 18 pages | null | null | null | cs.LO | null | Recently, there has been a lot of interest in the integration of Description
Logics and rules on the Semantic Web.We define guarded hybrid knowledge bases
(or g-hybrid knowledge bases) as knowledge bases that consist of a Description
Logic knowledge base and a guarded logic program, similar to the DL+log
knowledge bases from (Rosati 2006). G-hybrid knowledge bases enable an
integration of Description Logics and Logic Programming where, unlike in other
approaches, variables in the rules of a guarded program do not need to appear
in positive non-DL atoms of the body, i.e. DL atoms can act as guards as well.
Decidability of satisfiability checking of g-hybrid knowledge bases is shown
for the particular DL DLRO, which is close to OWL DL, by a reduction to guarded
programs under the open answer set semantics. Moreover, we show
2-EXPTIME-completeness for satisfiability checking of such g-hybrid knowledge
bases. Finally, we discuss advantages and disadvantages of our approach
compared with DL+log knowledge bases.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:49:56 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Heymans",
"Stijn",
""
],
[
"de Bruijn",
"Jos",
""
],
[
"Predoiu",
"Livia",
""
],
[
"Feier",
"Cristina",
""
],
[
"Van Nieuwenborgh",
"Davy",
""
]
] | [
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] |
711.2156 | Yu Xin | Y. Xin, L. Deng, R. de Grijs, A. D. Mackey, and Z. Han | Simple Stellar Population Models as probed by the Large Magellanic Cloud
Star Cluster ESO 121-SC03 | 11 pages, 7 figures, 2 tables, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2007.12720.x | null | astro-ph | null | The presence of blue straggler stars (BSs) in star clusters has proven a
challenge to conventional simple stellar population (SSP) models. Conventional
SSP models are based on the evolution theory of single stars. Meanwhile, the
typical locations of BSs in the colour-magnitude diagram of a cluster are
brighter and bluer than the main sequence turn-off point. Such loci cannot be
predicted by single-star evolution theory. However, stars with such properties
contribute significantly to the integrated light of the cluster. In this paper,
we reconstruct the integrated properties of the Large Magellanic Cloud cluster
ESO 121-SC03, based on a detailed exploration of the individual cluster stars,
and with particular emphasis on the cluster's BSs. We find that the integrated
light properties of ESO 121-SC03 are dramatically modified by its BS component.
The integrated spectral energy distribution (ISED) flux level is significantly
enhanced toward shorter wavelengths, and all broad-band colours become bluer.
When fitting the fully integrated ISED of this cluster based on conventional
SSP models, the best-fitting values of age and metallicity are significantly
underestimated compared to the true cluster parameters. The age underestimate
is $\sim40$ per cent if we only include the BSs within the cluster's half-light
radius and $\sim60$ per cent if all BSs are included. The corresponding
underestimates of the cluster's metallicity are $\sim30$ and $\sim60$ per cent,
respectively. The populous star clusters in the Magellanic Clouds are ideal
objects to explore the potential importance of BSs for the integrated light
properties of more distant unresolved star clusters in a statistically robust
manner, since they cover a large range in age and metallicity.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:50:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Xin",
"Y.",
""
],
[
"Deng",
"L.",
""
],
[
"de Grijs",
"R.",
""
],
[
"Mackey",
"A. D.",
""
],
[
"Han",
"Z.",
""
]
] | [
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] |
711.2157 | Bodo Manthey | Bodo Manthey | On Approximating Multi-Criteria TSP | Preliminary version at STACS 2009. This paper is a revised full
version, where some proofs are simplified | null | null | null | cs.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present approximation algorithms for almost all variants of the
multi-criteria traveling salesman problem (TSP).
First, we devise randomized approximation algorithms for multi-criteria
maximum traveling salesman problems (Max-TSP). For multi-criteria Max-STSP,
where the edge weights have to be symmetric, we devise an algorithm with an
approximation ratio of 2/3 - eps. For multi-criteria Max-ATSP, where the edge
weights may be asymmetric, we present an algorithm with a ratio of 1/2 - eps.
Our algorithms work for any fixed number k of objectives. Furthermore, we
present a deterministic algorithm for bi-criteria Max-STSP that achieves an
approximation ratio of 7/27.
Finally, we present a randomized approximation algorithm for the asymmetric
multi-criteria minimum TSP with triangle inequality Min-ATSP. This algorithm
achieves a ratio of log n + eps.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:53:49 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Nov 2008 09:20:10 GMT"
},
{
"version": "v3",
"created": "Wed, 13 Jul 2011 12:29:45 GMT"
}
] | 2011-07-14T00:00:00 | [
[
"Manthey",
"Bodo",
""
]
] | [
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] |
711.2158 | Grigori Rozenblum | Grigori Rozenblum, Alexander V. Sobolev | Discrete spectrum distribution of the Landau Operator Perturbed by an
Expanding Electric Potential | 22 pages, AMSLaTEX | null | null | null | math.SP math-ph math.MP | null | Under a perturbation by a decaying electric potential, the Landau Hamiltonian
acquires some discrete eigenvalues between the Landau levels. We study the
perturbation by an "expanding" electric potential $V(t^{-1}x)$, $t>0$, and
derive a quasi-classical formula for the counting function of the discrete
spectrum as $t\to \infty$.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:55:57 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Rozenblum",
"Grigori",
""
],
[
"Sobolev",
"Alexander V.",
""
]
] | [
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] |
711.2159 | Slava Khruschev | V. V. Khruschov | Fundamental interactions in quantum phase space specified by extra
dimensional constants | 5 pages, reference added, style corrected | Grav.Cosmol.13:259-261,2007 | null | null | hep-th | null | A generalized algebra of quantum observables, depending on extra dimensional
constants, is considered. Some limiting forms of the algebra are investigated
and their possible applications to the descriptions of interactions of
fundamental particles are proposed. A relation between current and constituent
quark masses is found using a modified quark equation of Dirac-Gursey-Lee type
and restrictions on the results of simultaneous measurements of momentum
components are pointed out.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 10:57:23 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Dec 2007 16:45:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Khruschov",
"V. V.",
""
]
] | [
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] |
711.216 | Akira Sekiyama | M. Uruma, A. Sekiyama, H. Fujiwara, M. Yano, H. Fujita, S. Imada, T.
Muro, I. A. Nekrasov, Y. Maeno, S. Suga | Three-Dimensional Bulk Electronic Structures of Ca1.5Sr0.5RuO4 Studied
by Soft X-ray Angle-Resolved Photoemission | 4 pages, 3 figures | null | null | null | cond-mat.str-el cond-mat.supr-con | null | We report on experimental data of the three-dimensional bulk Fermi surfaces
of the layered strongly correlated Ca1.5Sr0.5RuO4 system. The measurements have
been performed by means of hn-depndent bulk-sensitive soft x-ray angle-resolved
photoemission technique. Our experimental data evinces the bulk Fermi surface
topology at kz~0 to be qualitatively different from the one observed by
surface-sensitive low-energy ARPES. Furthermore, stronger kz dispersion of the
circle-like gamma Fermi surface sheet is observed compared with Sr2RuO4. Thus
in the paramagnetic metal phase, Ca1.5Sr0.5RuO4 compound is found to have
rather three-dimensional electronic structure.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:16:13 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Uruma",
"M.",
""
],
[
"Sekiyama",
"A.",
""
],
[
"Fujiwara",
"H.",
""
],
[
"Yano",
"M.",
""
],
[
"Fujita",
"H.",
""
],
[
"Imada",
"S.",
""
],
[
"Muro",
"T.",
""
],
[
"Nekrasov",
"I. A.",
""
],
[
"Maeno",
"Y.",
""
],
[
"Suga",
"S.",
""
]
] | [
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] |
711.2161 | H. Suderow | I. Guillamon, H. Suderow, F. Guinea, S. Vieira | Intrinsic atomic scale modulations of the superconducting gap of
2H-NbSe2 | 9 pages, 5 figures. Discussion extended, references added, one more
figure | Phys. Rev. B 77, 134505 (2008) | 10.1103/PhysRevB.77.134505 | null | cond-mat.supr-con cond-mat.str-el | null | We present scanning tunneling microscopy and spectroscopy measurements at
100mK in the superconducting material 2H-NbSe2 that show well defined features
in the superconducting density of states changing in a pattern closely
following atomic periodicity. Our experiment demonstrates that the intrinsic
superconducting density of states can show atomic size modulations, which
reflect the reciprocal space structure of the superconducting gap. In
particular we obtain that the superconducting gap of 2H-NbSe2 has six fold
modulated components at 0.75 mV and 1.2 mV.Moreover, we also find related
atomic size modulations inside vortices, demonstrating that the much discussed
star shape vortex structure produced by localized states inside the vortex
cores, has a, hitherto undetected, superposed atomic size modulation. The tip
substrate interaction in an anisotropic superconductor has been calculated,
giving position dependent changes related to the observed gap anisotropy.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:09:02 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 06:08:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Guillamon",
"I.",
""
],
[
"Suderow",
"H.",
""
],
[
"Guinea",
"F.",
""
],
[
"Vieira",
"S.",
""
]
] | [
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] |
711.2162 | Juan Li | Rainer Buckdahn, Boualem Djehiche, Juan Li, Shige Peng | Mean-field backward stochastic differential equations: A limit approach | Published in at http://dx.doi.org/10.1214/08-AOP442 the Annals of
Probability (http://www.imstat.org/aop/) by the Institute of Mathematical
Statistics (http://www.imstat.org) | Annals of Probability 2009, Vol. 37, No. 4, 1524-1565 | 10.1214/08-AOP442 | IMS-AOP-AOP442 | math.PR math.SG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Mathematical mean-field approaches play an important role in different fields
of Physics and Chemistry, but have found in recent works also their application
in Economics, Finance and Game Theory. The objective of our paper is to
investigate a special mean-field problem in a purely stochastic approach: for
the solution $(Y,Z)$ of a mean-field backward stochastic differential equation
driven by a forward stochastic differential of McKean--Vlasov type with
solution $X$ we study a special approximation by the solution $(X^N,Y^N,Z^N)$
of some decoupled forward--backward equation which coefficients are governed by
$N$ independent copies of $(X^N,Y^N,Z^N)$. We show that the convergence speed
of this approximation is of order $1/\sqrt{N}$. Moreover, our special choice of
the approximation allows to characterize the limit behavior of
$\sqrt{N}(X^N-X,Y^N-Y,Z^N-Z)$. We prove that this triplet converges in law to
the solution of some forward--backward stochastic differential equation of
mean-field type, which is not only governed by a Brownian motion but also by an
independent Gaussian field.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:13:27 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Feb 2008 05:27:04 GMT"
},
{
"version": "v3",
"created": "Fri, 28 Aug 2009 08:13:52 GMT"
}
] | 2009-08-28T00:00:00 | [
[
"Buckdahn",
"Rainer",
""
],
[
"Djehiche",
"Boualem",
""
],
[
"Li",
"Juan",
""
],
[
"Peng",
"Shige",
""
]
] | [
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] |
711.2163 | Filipe Abdalla B. | F. B. Abdalla, A. Mateus, W. A. Santos, L. Sodre Jr, I. Ferreras, O.
Lahav | Predicting spectral features in galaxy spectra from broad-band
photometry | 10 pages 7 figures summitted to MNRAS | null | 10.1111/j.1365-2966.2008.12881.x | null | astro-ph | null | We explore the prospects of predicting emission line features present in
galaxy spectra given broad-band photometry alone. There is a general consent
that colours, and spectral features, most notably the 4000 A break, can predict
many properties of galaxies, including star formation rates and hence they
could infer some of the line properties. We argue that these techniques have
great prospects in helping us understand line emission in extragalactic objects
and might speed up future galaxy redshift surveys if they are to target
emission line objects only. We use two independent methods, Artifical Neural
Neworks (based on the ANNz code) and Locally Weighted Regression (LWR), to
retrieve correlations present in the colour N-dimensional space and to predict
the equivalent widths present in the corresponding spectra. We also investigate
how well it is possible to separate galaxies with and without lines from broad
band photometry only. We find, unsurprisingly, that recombination lines can be
well predicted by galaxy colours. However, among collisional lines some can and
some cannot be predicted well from galaxy colours alone, without any further
redshift information. We also use our techniques to estimate how much
information contained in spectral diagnostic diagrams can be recovered from
broad-band photometry alone. We find that it is possible to classify AGN and
star formation objects relatively well using colours only. We suggest that this
technique could be used to considerably improve redshift surveys such as the
upcoming FMOS survey and the planned WFMOS survey.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:14:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Abdalla",
"F. B.",
""
],
[
"Mateus",
"A.",
""
],
[
"Santos",
"W. A.",
""
],
[
"Sodre",
"L.",
"Jr"
],
[
"Ferreras",
"I.",
""
],
[
"Lahav",
"O.",
""
]
] | [
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] |
711.2164 | Murach Aleksandr | Vladimir A. Mikhailets, Alexandr A. Murach | Elliptic systems of pseudodifferential equations in a refined scale on a
closed manifold | null | Extended variant is published in: Bull. Pol. Acad. Sci. Math., 56
(2008), no. 3 -- 4, 213 -- 224. | null | null | math.AP | null | We study a system of pseudodifferential equations that is elliptic in the
sense of Petrovskii on a closed compact smooth manifold. We prove that the
operator generated by the system is Fredholm one on a refined two-sided scale
of the functional Hilbert spaces. Elements of this scale are the special
isotropic spaces of H\"{o}rmander--Volevich--Paneah.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:22:11 GMT"
}
] | 2009-03-30T00:00:00 | [
[
"Mikhailets",
"Vladimir A.",
""
],
[
"Murach",
"Alexandr A.",
""
]
] | [
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] |
711.2165 | Marcelo Kuperman | M.N. Kuperman, S. Risau Gusman | The effect of the topology on the spatial ultimatum game | 6 pages, 5 figures | null | 10.1140/epjb/e2008-00133-x | null | nlin.AO nlin.CG | null | In this work we present an analysis of a spatially non homogeneous ultimatum
game. By considering different underlying topologies as substrates on top of
which the game takes place we obtain nontrivial behaviors for the evolution of
the strategies of the players. We analyze separately the effect of the size of
the neighborhood and the spatial structure. Whereas this last effect is the
most significant one, we show that even for disordered networks and provided
the neighborhood of each site is small, the results can be significantly
different from those obtained in the case of fully connected networks.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:22:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kuperman",
"M. N.",
""
],
[
"Gusman",
"S. Risau",
""
]
] | [
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] |
711.2166 | Nikola Vitas | N. Vitas (1 and 2), I. Vince (2 and 3), M. Lugaro (1 and 4), O.
Andriyenko (5 and 6), M. Gosic (2) and R. J. Rutten (1 and 7) ((1)
Sterrekundig Instituut, Utrecht University, The Netherlands, (2) Department
of Astronomy, University of Belgrade, Serbia, (3) Astronomical Observatory,
Belgrade, Serbia, (4) Center for Stellar Planetary Astrophysics, Monash
University, Australia, (5) ICAMER, NASU, Kyiv, Ukraine, (6) Main Astronomical
Observatory, NASU, Kyiv, Ukraine, (7) Institutt for Teoretisk Astrofysikk,
University of Oslo, Norway) | On the solar abundance of indium | 7 pages, 9 figures, accepted for publication in MNRAS Main Journal | null | 10.1111/j.1365-2966.2007.12708.x | null | astro-ph | null | The generally adopted value for the solar abundance of indium is over six
times higher than the meteoritic value. We address this discrepancy through
numerical synthesis of the 451.13 nm line on which all indium abundance studies
are based, both for the quiet-sun and the sunspot umbra spectrum, employing
standard atmosphere models and accounting for hyperfine structure and Zeeman
splitting in detail. The results, as well as a re-appraisal of indium
nucleosynthesis, suggest that the solar indium abundance is close to the
meteoritic value, and that some unidentified ion line causes the 451.13 nm
feature in the quiet-sun spectrum.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:24:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vitas",
"N.",
"",
"1 and 2"
],
[
"Vince",
"I.",
"",
"2 and 3"
],
[
"Lugaro",
"M.",
"",
"1 and 4"
],
[
"Andriyenko",
"O.",
"",
"5 and 6"
],
[
"Gosic",
"M.",
"",
"1 and 7"
],
[
"Rutten",
"R. J.",
"",
"1 and 7"
]
] | [
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] |
711.2167 | Juan Li | Rainer Buckdahn, Juan Li, Shige Peng | Mean-Field Backward Stochastic Differential Equations and Related
Partial Differential Equations | The results were presented by Rainer Buckdahn at the Mittag-Leffler
Institute (Stockholm, Sweden) in November 8th, 2007. The paper was submitted | null | null | null | math.PR math.SG | null | In [5] the authors obtained Mean-Field backward stochastic differential
equations (BSDE) associated with a Mean-field stochastic differential equation
(SDE) in a natural way as limit of some highly dimensional system of forward
and backward SDEs, corresponding to a large number of ``particles'' (or
``agents''). The objective of the present paper is to deepen the investigation
of such Mean-Field BSDEs by studying them in a more general framework, with
general driver, and to discuss comparison results for them. In a second step we
are interested in partial differential equations (PDE) whose solutions can be
stochastically interpreted in terms of Mean-Field BSDEs. For this we study a
Mean-Field BSDE in a Markovian framework, associated with a Mean-Field forward
equation. By combining classical BSDE methods, in particular that of ``backward
semigroups" introduced by Peng [14], with specific arguments for Mean-Field
BSDEs we prove that this Mean-Field BSDE describes the viscosity solution of a
nonlocal PDE. The uniqueness of this viscosity solution is obtained for the
space of continuous functions with polynomial growth. With the help of an
example it is shown that for the nonlocal PDEs associated to Mean-Field BSDEs
one cannot expect to have uniqueness in a larger space of continuous functions.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:34:11 GMT"
}
] | 2007-11-21T00:00:00 | [
[
"Buckdahn",
"Rainer",
""
],
[
"Li",
"Juan",
""
],
[
"Peng",
"Shige",
""
]
] | [
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711.2168 | Frithjof Anders | Frithjof B. Anders, David E. Logan, Martin R. Galpin, Gleb Finkelstein | Zero-bias conductance in carbon nanotube quantum dots | 4 pages, 5 figures | Phys. Rev. Lett. 100, 086809 (2008) | 10.1103/PhysRevLett.100.086809 | null | cond-mat.mes-hall cond-mat.str-el | null | We present numerical renormalization group calculations for the zero-bias
conductance of quantum dots made from semiconducting carbon nanotubes. These
explain and reproduce the thermal evolution of the conductance for different
groups of orbitals, as the dot-lead tunnel coupling is varied and the system
evolves from correlated Kondo behavior to more weakly correlated regimes. For
integer fillings $N=1,2,3$ of an SU(4) model, we find universal scaling
behavior of the conductance that is distinct from the standard SU(2) universal
conductance, and concurs quantitatively with experiment. Our results also agree
qualitatively with experimental differential conductance maps.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:36:44 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Mar 2008 15:50:01 GMT"
}
] | 2008-03-15T00:00:00 | [
[
"Anders",
"Frithjof B.",
""
],
[
"Logan",
"David E.",
""
],
[
"Galpin",
"Martin R.",
""
],
[
"Finkelstein",
"Gleb",
""
]
] | [
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] |
711.2169 | Dmitry Korshunov A. | Dmitry Korshunov | The Key Renewal Theorem for a Transient Markov Chain | 12 pages | null | null | null | math.PR | null | We consider a time-homogeneous Markov chain $X_n$, $n\ge0$, valued in ${\bf
R}$. Suppose that this chain is transient, that is, $X_n$ generates a
$\sigma$-finite renewal measure. We prove the key renewal theorem under
condition that this chain has asymptotically homogeneous at infinity jumps and
asymptotically positive drift.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:42:16 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Korshunov",
"Dmitry",
""
]
] | [
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] |
711.217 | Carsten Gundlach | Carsten Gundlach | Summary of GR18 Numerical Relativity parallel sessions (B1/B2 and B2),
Sydney, 8-13 July 2007 | References updated, to be published in CQG | Class.Quant.Grav.25:114019,2008 | 10.1088/0264-9381/25/11/114019 | null | gr-qc | null | The numerical relativity session at GR18 was dominated by physics results on
binary black hole mergers. Several groups can now simulate these from a time
when the post-Newtonian equations of motion are still applicable, through
several orbits and the merger to the ringdown phase, obtaining plausible
gravitational waves at infinity, and showing some evidence of convergence with
resolution. The results of different groups roughly agree. This new-won
confidence has been used by these groups to begin mapping out the
(finite-dimensional) initial data space of the problem, with a particular focus
on the effect of black hole spins, and the acceleration by gravitational wave
recoil to hundreds of km/s of the final merged black hole. Other work was
presented on a variety of topics, such as evolutions with matter, extreme mass
ratio inspirals, and technical issues such as gauge choices.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:42:51 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 10:46:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Gundlach",
"Carsten",
""
]
] | [
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711.2171 | Angela Bragaglia | Angela Bragaglia (INAF - Osservatorio Astronomico di Bologna) | The Bologna Open Clusters Chemical Evolution project (in short: BOCCE) | 5 pages, proceedings of "XXI Century challenges for stellar
evolution" (Cefalu', Italy), eds. S. Cassisi and M. Salaris, to be published
in MemSAIt, 79, 2 | null | null | null | astro-ph | null | I present here our project, the Bologna Open Clusters Chemical Evolution
(BOCCE) project, aimed at using Open Clusters as tracers of the disk properties
and their evolution with time. We are collecting and homogeneously analyzing
data, both photometric and spectroscopic, on a large sample of open clusters,
representative of the old cluster population, and I show here results obtained
on a subset of our clusters.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:47:42 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Bragaglia",
"Angela",
"",
"INAF - Osservatorio Astronomico di Bologna"
]
] | [
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711.2172 | Jan Pomplun | Jan Pomplun, Lin Zschiedrich, Roland Klose, Frank Schmidt, Sven Burger | Finite Element simulation of radiation losses in photonic crystal fibers | null | phys. stat. sol. (a) 204, No. 11, 3822-3837 (2007) | 10.1002/pssa.200776414 | null | physics.optics | null | In our work we focus on the accurate computation of light propagation in
finite size photonic crystal structures with the finite element method (FEM).
We discuss how we utilize numerical concepts like high-order finite elements,
transparent boundary conditions and goal-oriented error estimators for adaptive
grid refinement in order to compute radiation leakage in photonic crystal
fibers and waveguides. Due to the fast convergence of our method we can use it
e.g. to optimize the design of photonic crystal structures with respect to
geometrical parameters, to minimize radiation losses and to compute
attenutation spectra for different geometries.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:51:16 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Pomplun",
"Jan",
""
],
[
"Zschiedrich",
"Lin",
""
],
[
"Klose",
"Roland",
""
],
[
"Schmidt",
"Frank",
""
],
[
"Burger",
"Sven",
""
]
] | [
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] |
711.2173 | Ludwik Turko | Ludwik Turko | Statistical ensemble equivalence problem | 5 pages, Talk given at the conference ''New Trends in High Energy
Physics'', Crimea 2007, Yalta, 15-22 September 2007 | null | null | null | hep-th cond-mat.stat-mech | null | A problem of the equivalence of statistical ensembles is critically analyzed.
It is shown, that although different probability distributions of statistical
physics have the same behavior in the thermodynamic limit, there are physical
observables -- semi-intensive variables -- which keep memory of the underlying
ensembles. This property is an universal one and can be observed even in the
simplest case of the grand canonical and canonical ensembles of the classical
statistical physics.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 11:55:27 GMT"
}
] | 2007-11-17T00:00:00 | [
[
"Turko",
"Ludwik",
""
]
] | [
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] |
711.2174 | Roger Horsley | V.M. Braun, D. Br\"ommel, M. G\"ockeler, R. Horsley, Y. Nakamura, H.
Perlt, D. Pleiter, P.E.L. Rakow, A. Sch\"afer, G. Schierholz, A. Schiller, W.
Schroers, T. Streuer, H. St\"uben, J.M. Zanotti | Distribution Amplitudes of Vector Mesons | 7 pages, 5 figures, Contribution to Lattice 2007, Regensburg,
Germany, 30 July - 4 August 2007 | PoSLAT2007:144,2007 | null | DESY 07-177, Edinburgh 2007/28, Liverpool LTH 776 | hep-lat | null | Results are presented for the lowest moment of the distribution amplitude for
the K-star vector meson. Both longitudinal and transverse moments are
investigated. We use two flavours of O(a) improved Wilson fermions, together
with a non-perturbative renormalisation of the matrix element.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:02:27 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Braun",
"V. M.",
""
],
[
"Brömmel",
"D.",
""
],
[
"Göckeler",
"M.",
""
],
[
"Horsley",
"R.",
""
],
[
"Nakamura",
"Y.",
""
],
[
"Perlt",
"H.",
""
],
[
"Pleiter",
"D.",
""
],
[
"Rakow",
"P. E. L.",
""
],
[
"Schäfer",
"A.",
""
],
[
"Schierholz",
"G.",
""
],
[
"Schiller",
"A.",
""
],
[
"Schroers",
"W.",
""
],
[
"Streuer",
"T.",
""
],
[
"Stüben",
"H.",
""
],
[
"Zanotti",
"J. M.",
""
]
] | [
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] |
711.2175 | Ashley Willis | Yohann Duguet, Ashley P. Willis and Rich R. Kerswell | Transition in pipe flow: the saddle structure on the boundary of
turbulence | 24 pages, 14 figures. Accepted, Jou. Fluid Mech | null | 10.1017/S0022112008003248 | null | physics.flu-dyn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The laminar-turbulent boundary S is the set separating initial conditions
which relaminarise uneventfully from those which become turbulent. Phase space
trajectories on this hypersurface in cylindrical pipe flow look to be chaotic
and show recurring evidence of coherent structures. A general numerical
technique is developed for recognising approaches to these structures and then
for identifying the exact coherent solutions themselves. Numerical evidence is
presented which suggests that trajectories on S are organised around only a few
travelling waves and their heteroclinic connections. If the flow is suitably
constrained to a subspace with a discrete rotational symmetry, it is possible
to find locally-attracting travelling waves embedded within S. Four new types
of travelling waves were found using this approach.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:09:11 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Jul 2008 12:10:34 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Duguet",
"Yohann",
""
],
[
"Willis",
"Ashley P.",
""
],
[
"Kerswell",
"Rich R.",
""
]
] | [
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] |
711.2176 | Dmitri Volchenkov | Philippe Blanchard, Dimitry Volchenkov | Modelling Complex Networks: Cameo Graphs And Transport Processes | 24 pages, 7 figures, a contribution for the book of servey papers,
Stochastic Networks and Internet Technology, edited by Scuola Normale
Superiore, Pisa (Italy) | null | null | null | physics.soc-ph physics.data-an | null | We discuss a model accounting for the creation and development of transport
networks based on the Cameo principle which refers to the idea of distribution
of resources, including land, water, minerals, fuel and wealth. We also give an
outlook of the use of random walks as an effective tool for the investigation
of network structures and its functional segmentation. In particular, we have
studied the complex transport network of Venetian canals by means of random
walks.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:12:20 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Blanchard",
"Philippe",
""
],
[
"Volchenkov",
"Dimitry",
""
]
] | [
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] |
711.2177 | Cesare Tronci | Darryl D. Holm, Lennon O. Naraigh, Cesare Tronci | Emergent singular solutions of non-local density-magnetization equations
in one dimension | 19 pages, 13 figures. Submitted to Phys. Rev. E | null | 10.1103/PhysRevE.77.036211 | null | nlin.AO | null | We investigate the emergence of singular solutions in a non-local model for a
magnetic system. We study a modified Gilbert-type equation for the
magnetization vector and find that the evolution depends strongly on the length
scales of the non-local effects. We pass to a coupled density-magnetization
model and perform a linear stability analysis, noting the effect of the length
scales of non-locality on the system's stability properties. We carry out
numerical simulations of the coupled system and find that singular solutions
emerge from smooth initial data. The singular solutions represent a collection
of interacting particles (clumpons). By restricting ourselves to the
two-clumpon case, we are reduced to a two-dimensional dynamical system that is
readily analyzed, and thus we classify the different clumpon interactions
possible.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:18:28 GMT"
}
] | 2008-04-25T00:00:00 | [
[
"Holm",
"Darryl D.",
""
],
[
"Naraigh",
"Lennon O.",
""
],
[
"Tronci",
"Cesare",
""
]
] | [
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] |
711.2178 | Brett Hayes | Brett Hayes, Robert Brunner, Volodymyr Kindratenko | Angular Power Spectrum Estimation using High Performance Reconfigurable
Computing | 2 pages, In Proc. 3rd Annual Reconfigurable Systems Summer Institute
- RSSI'07, 2007 | null | null | null | astro-ph | null | Angular power spectra are an important measure of the angular clustering of a
given distribution. In Cosmology, they are applied to such vastly different
observations as galaxy surveys that cover a fraction of the sky and the Cosmic
Microwave Background that covers the entire sky, to obtain fundamental
parameters that determine the structure and evolution of the universe. The
calculation of an angular power spectrum, however, is complex and the
optimization of these calculations is a necessary consideration for current and
forthcoming observational surveys. In this work, we present preliminary results
of implementing angular power spectrum estimation scheme on a high-performance
reconfigurable computing platform.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:18:50 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Hayes",
"Brett",
""
],
[
"Brunner",
"Robert",
""
],
[
"Kindratenko",
"Volodymyr",
""
]
] | [
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] |
711.2179 | Peter Klimek | Rudolf Hanel, Peter Klimek, and Stefan Thurner | Studies in the physics of evolution: creation, formation, destruction | 11 pages, 10 figures, to be published in SPIE proceedings | null | 10.1117/12.771146 | null | q-bio.PE | null | The concept of (auto)catalytic systems has become a cornerstone in
understanding evolutionary processes in various fields. The common ground is
the observation that for the production of new species/goods/ideas/elements
etc. the pre-existence of specific other elements is a necessary condition. In
previous work some of us showed that the dynamics of the catalytic network
equation can be understood in terms of topological recurrence relations paving
a path towards the analytic tractability of notoriously high dimensional
evolution equations. We apply this philosophy to studies in socio-physics,
bio-diversity and massive events of creation and destruction in technological
and biological networks. Cascading events, triggered by small exogenous
fluctuations, lead to dynamics strongly resembling the qualitative picture of
Schumpeterian economic evolution. Further we show that this new methodology
allows to mathematically treat a variant of the threshold voter-model of
opinion formation on networks. For fixed topology we find distinct phases of
mixed opinions and consensus.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:22:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hanel",
"Rudolf",
""
],
[
"Klimek",
"Peter",
""
],
[
"Thurner",
"Stefan",
""
]
] | [
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] |
711.218 | Dean McLaughlin | Dean E. McLaughlin, Pauline Barmby, William E. Harris, Duncan A.
Forbes, and Gretchen L. H. Harris | Structural parameters for globular clusters in NGC 5128. III. ACS
surface-brightness profiles and model fits | MNRAS, in press. 28 pages. Full data tables available at
http://www.astro.keele.ac.uk/~dem/clusters.html | null | 10.1111/j.1365-2966.2007.12566.x | null | astro-ph | null | We present internal surface-brightness profiles, based on HST/ACS imaging in
the F606W bandpass, for 131 globular cluster (GC) candidates with luminosities
10^4 - 3 x 10^6 solar, in the giant elliptical galaxy NGC 5128. Several
structural models are fit to the profile of each cluster and combined with
mass-to-light ratios from population-synthesis models, to derive a catalogue of
fundamental structural and dynamical parameters parallel in form to the
catalogues recently produced by McLaughlin & van der Marel and Barmby et al.
for GCs and massive young star clusters in Local Group galaxies. As part of
this, we provide corrected and extended parameter estimates for another 18
clusters in NGC 5128, which we observed previously. We show that, like GCs in
the Milky Way and some of its satellites, the majority of globulars in NGC 5128
are well fit by isotropic Wilson models, which have intrinsically more
distended envelope structures than the standard King lowered isothermal
spheres. We use our models to predict internal velocity dispersions for every
cluster in our sample. These predictions agree well in general with the
observed dispersions in a small number of clusters for which spectroscopic data
are available. In a subsequent paper, we use these results to investigate
scaling relations for GCs in NGC 5128.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:58:44 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"McLaughlin",
"Dean E.",
""
],
[
"Barmby",
"Pauline",
""
],
[
"Harris",
"William E.",
""
],
[
"Forbes",
"Duncan A.",
""
],
[
"Harris",
"Gretchen L. H.",
""
]
] | [
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711.2181 | Paul David Mitchener | Paul D. Mitchener | The $KH$-Isomorphism Conjecture and Algebraic $KK$-theory | null | null | null | null | math.KT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this article we prove that the $KH$-asembly map, as defined by Bartels and
L{\"u}ck, can be described in terms of the algebraic $KK$-theory of Cortinas
and Thom. The $KK$-theory description of the $KH$-assembly map is similar to
that of the Baum-Connes assembly map. In very elementary cases, methods used to
prove the Baum-Connes conjecture also apply to the $KH$-isomorphism conjecture.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:24:10 GMT"
},
{
"version": "v2",
"created": "Wed, 14 Jan 2009 13:12:54 GMT"
}
] | 2009-01-14T00:00:00 | [
[
"Mitchener",
"Paul D.",
""
]
] | [
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711.2182 | Paul David Mitchener | Paul D. Mitchener | Algebraic $K$-theory Spectra and Factorisations of Analytic Assembly
Maps | null | null | null | null | math.KT | null | In this article we use existing machinery to define connective $K$-theory
spectra associated to topological ringoids. Algebraic $K$-theory of discrete
ringoids, and the analytic $K$-theory of Banach categories are obtained as
special cases.
As an application, we show how the analytic assembly maps featuring in the
Novikov and Baum-Connes conjectures can be factorised into composites of
assembly maps resembling those appearing in algebraic $K$-theory and maps
coming from completions of certain topological ringoids into Banach categories.
These factorisations are proved by using existing characterisations of assembly
maps along with our unified picture of algebraic and analytic $K$-theory.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:31:43 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Mitchener",
"Paul D.",
""
]
] | [
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711.2183 | Hung The Diep | Miron Kaufman and H. T. Diep | Potts-Percolation-Gauss Model of a Solid | 10 pages, 12 figures | null | 10.1088/0953-8984/20/7/075222 | null | cond-mat.stat-mech | null | We study a statistical mechanics model of a solid. Neighboring atoms are
connected by Hookian springs. If the energy is larger than a threshold the
"spring" is more likely to fail, while if the energy is lower than the
threshold the spring is more likely to be alive. The phase diagram and
thermodynamic quantities, such as free energy, numbers of bonds and clusters,
and their fluctuations, are determined using renormalization-group and
Monte-Carlo techniques.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:37:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kaufman",
"Miron",
""
],
[
"Diep",
"H. T.",
""
]
] | [
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0.0391160287,
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-0.0112701319,
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-0.0533753447,
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] |
711.2184 | Markus Diehl | Markus Diehl and Wolfgang Kugler | Some numerical studies of the evolution of generalized parton
distributions | 12 pages, 12 figures. v2: added comments on power-law behavior | Phys.Lett.B660:202-211,2008 | 10.1016/j.physletb.2007.12.047 | DESY 07-195 | hep-ph | null | We study the evolution behavior of generalized parton distributions at small
longitudinal momentum fraction. Particular attention is paid to the ratio of a
generalized parton distribution and its forward limit, to the mixing between
quarks and gluons, and to the dependence on the squared momentum transfer t.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:06:42 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Jan 2008 15:24:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Diehl",
"Markus",
""
],
[
"Kugler",
"Wolfgang",
""
]
] | [
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] |
711.2185 | Adam Shwartz | Arie Leizarowitz and Adam Shwartz | Exact finite approximations of average-cost countable Markov Decision
Processes | Submitted to Automatica | null | null | null | math.PR math.OC | null | For a countable-state Markov decision process we introduce an embedding which
produces a finite-state Markov decision process. The finite-state embedded
process has the same optimal cost, and moreover, it has the same dynamics as
the original process when restricting to the approximating set. The embedded
process can be used as an approximation which, being finite, is more convenient
for computation and implementation.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:45:11 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Leizarowitz",
"Arie",
""
],
[
"Shwartz",
"Adam",
""
]
] | [
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] |
711.2186 | Anne-Sophie Kaloghiros | Anne-Sophie Kaloghiros | The defect of Fano 3-folds | 24 pages, minor changes in exposition, final version | null | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper studies the defect of terminal Gorenstein Fano 3 folds. I
determine a bound on the defect of terminal Gorenstein Fano 3-folds of Picard
rank 1 that do not contain a plane. I give a general bound for quartic 3-folds
and indicate how to study the defect of terminal Gorenstein Fano 3-folds with
Picard rank 1 that contain a plane.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:42:43 GMT"
},
{
"version": "v2",
"created": "Thu, 31 Jul 2008 14:14:16 GMT"
},
{
"version": "v3",
"created": "Mon, 24 Aug 2009 11:12:33 GMT"
}
] | 2009-08-24T00:00:00 | [
[
"Kaloghiros",
"Anne-Sophie",
""
]
] | [
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0.0361908674,
0.0058585079,
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-0.015559284,
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0.1093588099
] |
711.2187 | Yi-Fu Cai | Yi-Fu Cai, Taotao Qiu, Robert Brandenberger, Yun-Song Piao, Xinmin
Zhang | On Perturbations of Quintom Bounce | 24 pages, 9 figures | JCAP0803:013,2008 | 10.1088/1475-7516/2008/03/013 | null | hep-th astro-ph gr-qc hep-ph | null | A Quintom universe with an equation-of-state crossing the cosmological
constant boundary can provide a bouncing solution dubbed the Quintom Bounce and
thus resolve the Big Bang singularity. In this paper, we investigate the
cosmological perturbations of the Quintom Bounce both analytically and
numerically. We find that the fluctuations in the dominant mode in the
post-bounce expanding phase couple to the growing mode of the perturbations in
the pre-bounce contracting phase.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 17:57:48 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Mar 2008 18:04:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cai",
"Yi-Fu",
""
],
[
"Qiu",
"Taotao",
""
],
[
"Brandenberger",
"Robert",
""
],
[
"Piao",
"Yun-Song",
""
],
[
"Zhang",
"Xinmin",
""
]
] | [
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711.2188 | Adam Shwartz | Rami Atar and Adam Shwartz | Efficient routing in heavy traffic under partial sampling of service
times | null | null | null | null | math.PR math.OC | null | We consider a queue with renewal arrivals and n exponential servers in the
Halfin-Whitt heavy traffic regime, where n and the arrival rate increase
without bound, so that a critical loading condition holds. Server k serves at
rate $\mu_k $, and the empirical distribution of the $\mu_k $ is assumed to
converge weakly. We show that very little information on the service rates is
required for a routing mechanism to perform well. More precisely, we construct
a routing mechanism that has access to a single sample from the service time
distribution of each of $n$ to the power of $1/2 + \epsilon $ randomly selected
servers, but not to the actual values of the service rates, the performance of
which is asymptotically as good as the best among mechanisms that have the
complete information on $ \mu_k $.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 12:59:20 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Atar",
"Rami",
""
],
[
"Shwartz",
"Adam",
""
]
] | [
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] |
711.2189 | Yoshiyuki Miyazaki | Y.Miyazaki, et al (Belle Collaboration) | Search for Lepton Flavor Violating tau Decays into Three Leptons | 11 pages, 4 figures, submitted to Phys. Lett. B | Phys.Lett.B660:154-160,2008 | 10.1016/j.physletb.2007.12.046 | Belle Preprint 2007-45, KEK Preprint 2007-57 | hep-ex | null | We search for lepton-flavor-violating tau decays into three leptons (electron
or muon) using 535 fb-1 of data collected with the Belle detector at the KEKB
asymmetric-energy e+e- collider. No evidence for these decays is observed, and
we set 90% confidence level upper limits on the branching fractions of
(2.0-4.1)x10^-8. These results improve upon our previously published upper
limits by factors of 4.9 to 10.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:01:31 GMT"
},
{
"version": "v2",
"created": "Mon, 19 Nov 2007 07:24:30 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Miyazaki",
"Y.",
""
]
] | [
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] |
711.219 | Andreas Berthold Thom | Andreas Thom | Integer operators in finite von Neumann algebras | 17 pages, no figures | null | null | null | math.FA math.NT | null | Motivated by the study of spectral properties of self-adjoint operators in
the integral group ring of a sofic group, we define and study integer
operators. We establish a relation with classical potential theory and in
particular the circle of results obtained by M. Fekete and G. Szeg"o. More
concretely, we use results by R. Rumely on equidistribution of algebraic
integers to obtain a description of those integer operator which have spectrum
of logarithmic capacity less or equal to one.
Finally, we relate the study of integer operators to a recent construction by
B. and L. Petracovici and A. Zaharescu.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:16:49 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Thom",
"Andreas",
""
]
] | [
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] |
711.2191 | Adam Shwartz | Adam Shwartz and Alan Weiss | Uniqueness of a constrained variational problem and large deviations of
buffer size | null | null | null | null | math.PR math.OC | null | We show global uniqueness of the solution to a class of constrained
variational problems, using scaling properties. This is used to establish the
essential uniqueness of solutions of a large deviations problem in multiple
dimensions. The result is motivated by models of buffers, and in particular the
probability of, and typical path to overflow in the limit of small buffers,
which we analyze.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:17:17 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Shwartz",
"Adam",
""
],
[
"Weiss",
"Alan",
""
]
] | [
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] |
711.2192 | Frithjof Brauer | F. Brauer, C.P. Dullemond, Th. Henning | Coagulation, fragmentation and radial motion of solid particles in
protoplanetary disks | accepted for publication in A&A | null | 10.1051/0004-6361:20077759 | null | astro-ph | null | The growth of solid particles towards meter sizes in protoplanetary disks has
to circumvent at least two hurdles, namely the rapid loss of material due to
radial drift and particle fragmentation due to destructive collisions. In this
paper, we present the results of numerical simulations with more and more
realistic physics involved. Step by step, we include various effects, such as
particle growth, radial/vertical particle motion and dust particle
fragmentation in our simulations. We demonstrate that the initial dust-to-gas
ratio is essential for the particles to overcome the radial drift barrier. If
this value is increased by a factor of 2 compared with the canonical value for
the interstellar medium, km-sized bodies can form in the inner disk <2 AU
within 10 thousand years. However, we find that solid particles get destroyed
through collisional fragmentation. Only with the unrealistically high-threshold
velocities needed for fragmentation to occur (>30 m/s), particles are able to
grow to larger sizes in low turbulent disks. We also find that less than 5% of
the small dust grains remain in the disk after 1 Myrs due to radial drift, no
matter whether fragmentation is included in the simulations or not. In this
paper, we also present considerable improvements to existing algorithms for
dust-particle coagulation, which speed up the coagulation scheme by a factor of
10 thousand.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:40:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Brauer",
"F.",
""
],
[
"Dullemond",
"C. P.",
""
],
[
"Henning",
"Th.",
""
]
] | [
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] |
711.2193 | Tsung-Shung Harry Lee | T.-S. H. Lee | Dynamical Coupled-Channels Analysis at EBAC | null | null | 10.1088/1742-6596/69/1/012013 | JLAB-THY-07-750 | nucl-th | null | The status of dynamical coupled-channel analysis at Excited Baryon Analysis
Center (EBAC) of Jefferson Laboratory is reported.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:24:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lee",
"T. -S. H.",
""
]
] | [
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711.2194 | Jun-Bao Wu | Bin Chen, Chang-Yong Liu, Jun-Bao Wu | Operator Product Expansion of Wilson surfaces from M5-branes | 27 pages, no figures; typos corrected, references added, minor
changes, 29 pages; typos fixed, JHEP published version | JHEP0801:007,2008 | 10.1088/1126-6708/2008/01/007 | CAS-KITPC/ITP-018, SISSA-83/2007/EP | hep-th | null | The operator product expansion (OPE) of the Wilson surface operators in
six-dimensional (2, 0) superconformal field theory is studied from AdS/CFT
correspondence in this paper. We compute the OPE coefficients of the chiral
primary operators using the M5-brane description for spherical Wilson surface
operators in higher dimensional representations. We use the non-chiral M5-brane
action in our calculation. We also discuss their membrane limit, and compare
our results with the ones obtained from membrane description.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:26:12 GMT"
},
{
"version": "v2",
"created": "Sun, 2 Dec 2007 12:06:41 GMT"
},
{
"version": "v3",
"created": "Sat, 5 Jan 2008 09:57:56 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chen",
"Bin",
""
],
[
"Liu",
"Chang-Yong",
""
],
[
"Wu",
"Jun-Bao",
""
]
] | [
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711.2195 | Jan Christian Rohde | Jan Christian Rohde | Cyclic coverings, Calabi-Yau manifolds and Complex multiplication | 151 pages, one reference added | null | null | null | math.AG | null | We construct families of Calabi-Yau manifolds with dense set of complex
multiplication fibers in an arbitrary dimension. We will also give explicite
examples of complex multiplication fibers. For this construction we use
families of curves with dense set of complex multiplication fibers. In
addition, we give examples of such families for each genus less or equal 7 and
we study the generic Hodge groups of families of cyclic covers of the
projective line.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:57:42 GMT"
},
{
"version": "v2",
"created": "Fri, 23 Nov 2007 16:01:39 GMT"
},
{
"version": "v3",
"created": "Fri, 22 Feb 2008 14:58:38 GMT"
},
{
"version": "v4",
"created": "Mon, 3 Mar 2008 14:02:21 GMT"
}
] | 2008-03-03T00:00:00 | [
[
"Rohde",
"Jan Christian",
""
]
] | [
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] |
711.2196 | Leszek Motyka | J. Bartels and L. Motyka | Baryon scattering at high energies: wave function, impact factor, and
gluon radiation | 36 pages, 16 figures | Eur.Phys.J.C55:65-83,2008 | 10.1140/epjc/s10052-008-0572-z | DESY 07-198 | hep-ph | null | The scattering of a baryon consisting of three massive quarks is investigated
in the high energy limit of perturbative QCD. A model of a relativistic
proton-like wave function, dependent on valence quark longitudinal and
transverse momenta and on quark helicities, is proposed, and we derive the
baryon impact factors for two, three and four t-channel gluons. We find that
the baryonic impact factor can be written as a sum of three pieces: in the
first one a subsystem consisting of two of the three quarks behaves very much
like the quark-antiquark pair in gamma* scattering, whereas the third quark
acts as a spectator. The second term belongs to the odderon, whereas in the
third (C-even) piece all three quarks participate in the scattering. This term
is new and has no analogue in gamma* scattering. We also study the small x
evolution of gluon radiation for each of these three terms. The first term
follows the same pattern of gluon radiation as the gamma*-initiated
quark-antiquark dipole, and, in particular, it contains the BFKL evolution
followed by the 2-->4 transition vertex (triple Pomeron vertex). The
odderon-term is described by the standard BKP evolution, and the baryon couples
to both known odderon solutions, the Janik-Wosiek solution and the BLV
solution. Finally, the t-channel evolution of the third term starts with a
three reggeized gluon state which then, via a new 3-->4 transition vertex,
couples to the four gluon (two-Pomeron) state. We briefly discuss a few
consequences of these findings, in particular the pattern of unitarization of
high energy baryon scattering amplitudes.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:42:07 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Bartels",
"J.",
""
],
[
"Motyka",
"L.",
""
]
] | [
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] |
711.2197 | Su-Chan Park | Su-Chan Park and Hyunggyu Park | Nonequilibrium Phase Transitions into Absorbing States: Focused around
the pair contact process with diffusion | Proceedings of STATPHY23. Submitted to EPJB | Eur. Phys. J. B 64, 415 (2008) | 10.1140/epjb/e2008-00022-4 | null | cond-mat.stat-mech | null | Systems with absorbing (trapped) states may exhibit a nonequilibrium phase
transition from a noise-free inactive phase into an ever-lasting active phase.
We briefly review the absorbing critical phenomena and universality classes,
and discuss over the controversial issues on the pair contact process with
diffusion (PCPD). Two different approaches are proposed to clarify its
universality issue, which unveil strong evidences that the PCPD belongs to a
new universality class other than the directed percolation class.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:38:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Park",
"Su-Chan",
""
],
[
"Park",
"Hyunggyu",
""
]
] | [
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711.2198 | Stefano Ansoldi | Stefano Ansoldi, Eduardo I. Guendelman and Idan Shilon | Stability, Singularities and Mass Thresholds in Child Universe
Production: a concise survey including some recent results and prospects | 19 pages LaTeX, including 68 references; to appear in the Proceedings
of "BH2, Dynamics and Thermodynamics of Blackholes and Naked Singularities",
May 10-12 2007, Milano, Italy; conference website:
http://www.mate.polimi.it/bh2 | null | null | KUNS-2109 | gr-qc hep-th | null | We present a review of selected topics concerning the creation and evolution
of child universes, together with a concise account of some recent progress in
the field.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:40:12 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Ansoldi",
"Stefano",
""
],
[
"Guendelman",
"Eduardo I.",
""
],
[
"Shilon",
"Idan",
""
]
] | [
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] |
711.2199 | Kim Nilsson | Kim K. Nilsson (Dark Cosmology Centre, DK, ESO - Garching) | The Lyman-alpha Emission Line as a Cosmological Tool | 138 pages, 39 figures, 28 tables, PhD thesis defended at Copenhagen
University on 21 September 2007 | null | null | null | astro-ph | null | This thesis deals with different aspects of a special kind of high redshift
galaxy, namely Ly-alpha emitters. Ly-alpha emitters are galaxies found through
their Ly-alpha emission, at redshifts larger than z >~ 2 where the emission
line has been redshifted into the optical or near-infrared regime. The thesis
has two main parts; a lower redshift, observational part (z ~ 3) and a more
technical/theoretical very high redshift part (z ~ 9).
In the first, lower redshift part I present the analysis of a narrow-band
image taken in the GOODS-S field, focused on a redshift for Ly-alpha of z =
3.15. The image, covering a central part of the GOODS-S field revealed 25
Ly-alpha emitting candidates, of which one turned out to be a so-called
Ly-alpha blob. In the second part, I discuss future, very high redshift
narrow-band surveys for Ly-alpha emitters. Finally, in a project unrelated to
the other two parts of the thesis, I present a search for a 'Fundamental plane'
of Ly-alpha emitters in the colour space produced by large-scale
multi-wavelength surveys such as GOODS or COSMOS. [Abridged]
| [
{
"version": "v1",
"created": "Tue, 13 Nov 2007 21:23:47 GMT"
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] | 2007-11-15T00:00:00 | [
[
"Nilsson",
"Kim K.",
"",
"Dark Cosmology Centre, DK, ESO - Garching"
]
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711.22 | Kunji Nakayama | Kunji Nakayama | Topos-Theoretic Extension of a Modal Interpretation of Quantum Mechanics | LaTeX2e | Int.J.Theor.Phys.47:2065-2094,2008 | 10.1007/s10773-008-9649-6 | null | quant-ph gr-qc | null | This paper deals with topos-theoretic truth-value valuations of quantum
propositions. Concretely, a mathematical framework of a specific type of modal
approach is extended to the topos theory, and further, structures of the
obtained truth-value valuations are investigated. What is taken up is the modal
approach based on a determinate lattice $\Dcal(e,R)$, which is a sublattice of
the lattice $\Lcal$ of all quantum propositions and is determined by a quantum
state $e$ and a preferred determinate observable $R$. Topos-theoretic extension
is made in the functor category $\Sets^{\CcalR}$ of which base category
$\CcalR$ is determined by $R$. Each true atom, which determines truth values,
true or false, of all propositions in $\Dcal(e,R)$, generates also a
multi-valued valuation function of which domain and range are $\Lcal$ and a
Heyting algebra given by the subobject classifier in $\Sets^{\CcalR}$,
respectively. All true propositions in $\Dcal(e,R)$ are assigned the top
element of the Heyting algebra by the valuation function. False propositions
including the null proposition are, however, assigned values larger than the
bottom element. This defect can be removed by use of a subobject
semi-classifier. Furthermore, in order to treat all possible determinate
observables in a unified framework, another valuations are constructed in the
functor category $\Sets^{\Ccal}$. Here, the base category $\Ccal$ includes all
$\CcalR$'s as subcategories. Although $\Sets^{\Ccal}$ has a structure
apparently different from $\Sets^{\CcalR}$, a subobject semi-classifier of
$\Sets^{\Ccal}$ gives valuations completely equivalent to those in
$\Sets^{\CcalR}$'s.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:47:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Nakayama",
"Kunji",
""
]
] | [
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711.2201 | Narit Pidokrajt | Jan E. Aman, Narit Pidokrajt, John Ward | On Geometro-thermodynamics of Dilaton Black Holes | Talk given at 30th Spanish Relativity Meeting (ERE 2007):
Relativistic Astrophysics And Cosmology, 10-14 Sep 2007, Puerto de La Cruz,
Tenerife, Spain. Typos corrected | EAS Publ.Ser.30:279,2008 | 10.1051/eas:0830044 | USITP 07-02 | hep-th gr-qc | null | In this talk we present the latest results from our ongoing project on
geometro-thermodynamics (also known as information geometry of thermodynamics
or Ruppeiner geometry) of dilaton BHs in 4D in both Einstein and string frames
and a dyonic dilaton BH and at the end we report very briefly results from this
approach to the 2D dilaton BHs.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 13:57:42 GMT"
},
{
"version": "v2",
"created": "Sun, 18 Nov 2007 10:17:29 GMT"
}
] | 2009-01-14T00:00:00 | [
[
"Aman",
"Jan E.",
""
],
[
"Pidokrajt",
"Narit",
""
],
[
"Ward",
"John",
""
]
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] |
711.2202 | Hans-Christoph Grunau | Alberto Ferrero, Hans-Christoph Grunau, Paschalis Karageorgis | Supercritical biharmonic equations with power-type nonlinearity | null | Ann. Mat. Pura Appl. 188, 171 - 185 (2009). | 10.1007/s10231-008-0070-9 | null | math.AP math.CA | null | The biharmonic supercritical equation $\Delta^2u=|u|^{p-1}u$, where $n>4$ and
$p>(n+4)/(n-4)$, is studied in the whole space $\mathbb{R}^n$ as well as in a
modified form with $\lambda(1+u)^p$ as right-hand-side with an additional
eigenvalue parameter $\lambda>0$ in the unit ball, in the latter case together
with Dirichlet boundary conditions. As for entire regular radial solutions we
prove oscillatory behaviour around the explicitly known radial {\it singular}
solution, provided $p\in((n+4)/(n-4),p_c)$, where $p_c\in ((n+4)/(n-4),\infty]$
is a further critical exponent, which was introduced in a recent work by
Gazzola and the second author. The third author proved already that these
oscillations do not occur in the complementing case, where $p\ge p_c$.
Concerning the Dirichlet problem we prove existence of at least one singular
solution with corresponding eigenvalue parameter. Moreover, for the extremal
solution in the bifurcation diagram for this nonlinear biharmonic eigenvalue
problem, we prove smoothness as long as $p\in((n+4)/(n-4),p_c)$.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:05:26 GMT"
}
] | 2009-02-27T00:00:00 | [
[
"Ferrero",
"Alberto",
""
],
[
"Grunau",
"Hans-Christoph",
""
],
[
"Karageorgis",
"Paschalis",
""
]
] | [
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] |
711.2203 | Masafumi Seriu | Masafumi Seriu and Chun-Hsien Wu | Switching effect upon the quantum Brownian motion near a reflecting
boundary | 12 pages, 2 figures This version is just to correct the author-list | Physical Review A77, 022107 (2008) | 10.1103/PhysRevA.77.022107 | null | quant-ph gr-qc | null | The quantum Brownian motion of a charged particle in the electromagnetic
vacuum fluctuations is investigated near a perfectly reflecting flat boundary,
taking into account the smooth switching process in the measurement.
Constructing a smooth switching function by gluing together a plateau and the
Lorentzian switching tails, it is shown that the switching tails have a great
influence on the measurement of the Brownian motion in the quantum vacuum.
Indeed, it turns out that the result with a smooth switching function and the
one with a sudden switching function are qualitatively quite different. It is
also shown that anti-correlations between the switching tails and the main
measuring part plays an essential role in this switching effect. The switching
function can also be interpreted as a prototype of an non-equilibrium process
in a realistic measurement, so that the switching effect found here is expected
to be significant in actual applications in vacuum physics.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:06:24 GMT"
},
{
"version": "v2",
"created": "Fri, 16 Nov 2007 01:43:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Seriu",
"Masafumi",
""
],
[
"Wu",
"Chun-Hsien",
""
]
] | [
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] |
711.2204 | Alexandre Kisselev | A.V. Kisselev | RS model with the small curvature and Bhabha scattering at the ILC | 13 pages, 5 figures, talk at the International School-Seminar
``Actual Problems of Microworld Physics'', Gomel, Belarus, July 23 - August
3, 2007 | null | null | null | hep-ph | null | The Randall-Sundrum (RS) model with the small curvature is studied. In such a
scheme the mass spectrum of Kaluza-Klein (KK) gravitons is similar to that in a
model with one extra flat dimension. The gravity effects in the Bhabha
scattering at the energy 1 TeV are estimated. The calculations are based on the
analytical formula which describes virtual graviton contributions. It takes
into account both a discrete character of the mass spectrum and nonzero widths
of the KK gravitons.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:08:04 GMT"
}
] | 2007-11-15T00:00:00 | [
[
"Kisselev",
"A. V.",
""
]
] | [
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711.2205 | Heinrichs Jean | J. Heinrichs | Enhancement of Persistent Current in Metal Rings by Correlated Disorder | 18 | J.Phys.:Condens.Matter 20 (2008) 345232 (9pp) | 10.1088/0953-8984/20/34/345232 | null | cond-mat.mes-hall cond-mat.dis-nn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study analytically the effect of a correlated random potential on the
persistent current in a one-dimensional ring threaded by a magnetic flux
$\phi$, using an Anderson tight-binding model. In our model, the system of
$N=2M$ atomic sites of the ring is assumed to be partitioned into $M$ pairs of
identical nearest-neighbour sites (dimers). The site energies for different
dimers are taken to be uncorrelated gaussian variables. For this system we
obtain the exact flux-dependent energy levels to second order in the random
site energies, using an earlier exact transfer matrix perturbation theory.
These results are used to study the mean persistent current generated by
$N_e\leq N$ spinless electrons occupying the $N_e$ lowest levels of the
flux-dependent energy band at zero temperature. Detailed analyses are carried
out in the limit $1\ll N_e\ll N$ and for a half-filled band ($N_e=N/2$), for
magnetic fluxes $-1/2 <\phi/\phi_0<1/2$. While the uncorrelated disorder leads
to a reduction of the persistent current, the disorder correlation acts to
enhance it. In particular, in the half-filled band case the correlated disorder
leads to a global flux-dependent enhancement of persistent current which has
the same form for even and odd $N_e$. At low filling of the energy band the
effect of the disorder on the persistent current is found to depend on the
parity of $N_e$: the correlated disorder yields a reduction of the current for
odd $N_e$ and an enhancement of the current for even $N_e$.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:10:12 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Feb 2008 15:17:52 GMT"
},
{
"version": "v3",
"created": "Fri, 22 Aug 2008 13:35:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Heinrichs",
"J.",
""
]
] | [
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711.2206 | Charles Young | C. A. S. Young, R. Zegers | Covariant particle statistics and intertwiners of the kappa-deformed
Poincare algebra | 16 pages, latex; v2, references added | Nucl.Phys.B797:537-549,2008 | 10.1016/j.nuclphysb.2007.12.021 | DCPT-07/59 | hep-th | null | To speak about identical particles - bosons or fermions - in quantum field
theories with kappa-deformed Poincare symmetry, one must have a kappa-covariant
notion of particle exchange. This means constructing intertwiners of the
relevant representations of kappa-Poincare. We show, in the simple case of
spinless particles, that intertwiners exist, and, supported by a perturbative
calculation to third order in 1/kappa, make a conjecture about the existence
and uniqueness of a certain preferred intertwiner defining particle exchange in
kappa-deformed theories.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:10:21 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 10:53:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Young",
"C. A. S.",
""
],
[
"Zegers",
"R.",
""
]
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] |
711.2207 | Francesco Petruccione | Alessandro Sergi and Francesco Petruccione | Nos\'e-Hoover Dynamics in Quantum Phase Space | 4 pages, no figures | null | 10.1088/1751-8113/41/35/355304 | null | quant-ph | null | Thermal fluctuations in time-dependent quantum processes are treated by a
constant-temperature generalization of Wigner's formulation of quantum
mechanics in phase space. To this end, quantum Nos\`e-Hoover dynamics is
defined by generalizing the Moyal bracket. Computational applications of the
formalism, together with further theoretical developments, are discussed.
| [
{
"version": "v1",
"created": "Wed, 14 Nov 2007 14:15:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sergi",
"Alessandro",
""
],
[
"Petruccione",
"Francesco",
""
]
] | [
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