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802.0303 | Matthew Lehner | M. J. Lehner, C.-Y. Wen, J.-H. Wang, S. L. Marshall, M. E. Schwamb,
Z.-W. Zhang, F. B. Bianco, J. Giammarco, R. Porrata, C. Alcock, T. Axelrod,
Y.-I. Byun, W. P. Chen, K. H. Cook, R. Dave, S.-K. King, T. Lee, H.-C. Lin
and S.-Y. Wang | The Taiwanese-American Occultation Survey: The Multi-Telescope Robotic
Observatory | 11 pages, 11 figures | PASP 121 (2009) 138-152 | 10.1086/597516 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Taiwanese-American Occultation Survey (TAOS) operates four fully
automatic telescopes to search for occultations of stars by Kuiper Belt
Objects. It is a versatile facility that is also useful for the study of
initial optical GRB afterglows. This paper provides a detailed description of
the TAOS multi-telescope system, control software, and high-speed imaging.
| [
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{
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] | 2009-11-13T00:00:00 | [
[
"Lehner",
"M. J.",
""
],
[
"Wen",
"C. -Y.",
""
],
[
"Wang",
"J. -H.",
""
],
[
"Marshall",
"S. L.",
""
],
[
"Schwamb",
"M. E.",
""
],
[
"Zhang",
"Z. -W.",
""
],
[
"Bianco",
"F. B.",
""
],
[
"Giammarco",
"J.",
""
],
[
"Porrata",
"R.",
""
],
[
"Alcock",
"C.",
""
],
[
"Axelrod",
"T.",
""
],
[
"Byun",
"Y. -I.",
""
],
[
"Chen",
"W. P.",
""
],
[
"Cook",
"K. H.",
""
],
[
"Dave",
"R.",
""
],
[
"King",
"S. -K.",
""
],
[
"Lee",
"T.",
""
],
[
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""
],
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""
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802.0304 | Michael Marthaler | M. Marthaler, Gerd Sch\"on, Alexander Shnirman | Photon-Number Squeezing in Circuit Quantum Electrodynamics | 5 pages, 5 figures | Phys. Rev. Lett. 101, 147001 (2008). | 10.1103/PhysRevLett.101.147001 | null | cond-mat.other cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A superconducting single-electron transistor (SSET) coupled to an anharmonic
oscillator, e.g., a Josephson junction-L-C circuit, can drive the latter to a
nonequilibrium photon number state. By biasing the SSET in a regime where the
current is carried by a combination of inelastic quasiparticle tunneling and
coherent Cooper-pair tunneling (Josephson quasiparticle cycle), cooling of the
oscillator as well as a laser like enhancement of the photon number can be
achieved. Here we show, that the cut-off in the quasiparticle tunneling rate
due to the superconducting gap, in combination with the anharmonicity of the
oscillator, may create strongly squeezed photon number distributions. For low
dissipation in the oscillator nearly pure Fock states can be produced.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 21:21:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Marthaler",
"M.",
""
],
[
"Schön",
"Gerd",
""
],
[
"Shnirman",
"Alexander",
""
]
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802.0305 | David Delphenich | David Delphenich | Generalized Madelung transformations for quantum wave equations I:
generalized spherical coordinates for field spaces | 42 pages | null | null | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Madelung transformation of the space in which a quantum wave function
takes its values is generalized from complex numbers to include field spaces
that contain orbits of groups that are diffeomorphic to spheres. The general
form for the resulting real wave equations then involves structure constants
for the matrix algebra that is associated with the group action. The particular
cases of the algebras of complex numbers, quaternions, and complex quaternions,
which pertain to the Klein-Gordon equation, the relativistic Pauli equation,
and the bi-Dirac equation, resp., are then discussed.
| [
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"version": "v1",
"created": "Sun, 3 Feb 2008 21:48:37 GMT"
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[
"Delphenich",
"David",
""
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802.0306 | Alastair Craw | Emiko Dupont | A Symplectic Isotopy of a Dehn Twist on CP^n x CP^{n+1} | 20 pages, 6 figures | null | 10.1112/jlms/jdp020 | null | math.SG math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The complex manifold CP^n x CP^{n+1} with symplectic form
\sigma_\mu=\sigma_{CP^n}+\mu\sigma_{CP^{n+1}}, where \sigma_{CP^n} and
\sigma_{CP^{n+1}} are normalized Fubini-Study forms, n a natural number and
\mu>1 a real number, contains a natural Lagrangian sphere L^{\mu}. We prove
that the Dehn twist along L^{\mu} is symplectically isotopic to the identity
for all \mu>1. This isotopy can be chosen so that it pointwise fixes a complex
hypersurface in CP^n x CP^{n+1} and lifts to the blow-up of CP^n x CP^{n+1}
along a complex n-dimensional submanifold.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 21:51:07 GMT"
}
] | 2014-02-26T00:00:00 | [
[
"Dupont",
"Emiko",
""
]
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802.0307 | Ovidiu Munteanu | Ovidiu Munteanu | On a characterization of the complex hyperbolic space | null | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Consider a compact K\"{a}hler manifold $M^m$ with Ricci curvature lower bound
$Ric_M\geq -2(m+1) .$ Assume that its universal cover $% \widetilde{M}$ has
maximal bottom of spectrum $\lambda_1(\widetilde{M}%) =m^2.$ Then we prove that
$\widetilde{M}$ is isometric to the complex hyperbolic space $\Bbb{CH}^m.$
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 22:05:08 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Munteanu",
"Ovidiu",
""
]
] | [
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802.0308 | Bob Eisenberg | Bob Eisenberg | Bubble Gating Currents in Ionic Channels | Typo corrected | null | null | null | q-bio.BM q-bio.QM | null | Bubbles in ion channel proteins have been proposed to be the bistable gates
that control current flow. Gating currents associated with channel gating would
then be an electrical signature of bubble breaking and formation, arising from
the change in dielectric coefficient as the bubble breaks or forms. A bubble
would have a dielectric coefficient of 1. A filled bubble would have a
dielectric coefficient (say) between 30 and 80. Transporters, pumps, and
channels would be expected to have gating currents.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 22:19:22 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Feb 2008 11:06:35 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Eisenberg",
"Bob",
""
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] |
802.0309 | Fredy Ochoa | R. Martinez and F. Ochoa | Mass-matrix ansatz and constraints on $B_{s}^{0}-\bar{B}_{s}^{0}$ mixing
in 331 models | To be published at Physical Revew D | Phys.Rev.D77:065012,2008 | 10.1103/PhysRevD.77.065012 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Comparing the theoretically predicted and measured values of the mass
difference of the $B^{0}_{s}$ system, we estimate the lower bound on the mass
of the $Z^{\prime}$ boson of models based on the $SU(3)_{c} \otimes SU(3)_{L}
\otimes U(1)_X$ gauge group. By assuming zero-texture approaches of the quark
mass matrices, we find the ratio of the measured value to the theoretical
prediction from the Standard Model and the $Z^{\prime}$ contribution from the
331 models of the mass difference of the $B^{0}_{s}$ system. We find lower
bounds on the $Z^{\prime}$ mass ranging between 1 TeV and 30 TeV for the two
most popular 331 models, and four different zero-textures ans\"atze. The above
results are expressed as a function of the weak angle associated to the
$b-s-Z^{\prime}$ couplings.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 22:21:45 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Martinez",
"R.",
""
],
[
"Ochoa",
"F.",
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802.031 | Fredy Ochoa | N. Gutierrez, R. Martinez, F. Ochoa | $Z^{\prime}$ boson signal at Tevatron and LHC in a 331 model | null | null | null | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We analyse the possibilities to detect a new $Z^{\prime}$ boson in
di-electron events at Tevatron and LHC in the framework of the 331 model with
right-handed neutrinos. Using $p\bar{p}$ collision data collected by the CDF II
detector at Fermilab Tevatron, we find that the 331 $Z^{\prime}$ boson is
excluded with masses below 920 GeV. For an integrated luminosity of $100
fb^{-1}$ at LHC, and considering a central value $M_{Z^{\prime}}=1500$ GeV, we
obtain the invariant mass distribution in the process $pp\to Z^{\prime}\to
e^{+}e^{-}$, where a huge peak, corresponding to 800 signal events, is found
above the SM background. The number of di-electron events vary from 10000 to 1
in the mass range of $M_{Z^{\prime}}=1000-5000$ GeV.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 22:36:18 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Gutierrez",
"N.",
""
],
[
"Martinez",
"R.",
""
],
[
"Ochoa",
"F.",
""
]
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802.0311 | Guendelman Eduardo I | E.I. Guendelman | Photon and Axion Splitting in an Inhomogeneous Magnetic Field | 9 pages, latex | Phys.Lett.B662:445-448,2008 | 10.1016/j.physletb.2008.03.050 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The axion photon system in an external magnetic field, when the direction of
propagation of axions and photons is orthogonal to the direction of the
external magnetic field, displays a continuous axion-photon duality symmetry in
the limit the axion mass is neglected. The conservation law that follow in this
effective 2+1 dimensional theory from this symmetry is obtained. The magnetic
field interaction is seen to be equivalent to first order to the interaction of
a complex charged field with an external electric potential, where this
ficticious "electric potential" is proportional to the external magnetic field.
This allows one to solve for the scattering amplitudes using already known
scalar QED results. From the scalar QED analog the axion and the photon are
symmetric and antisymmetric combinations of particle and antiparticle. If one
considers therefore scattering experiments in which the two spatial dimensions
of the effective theory are involved non trivially, one observes that both
particle and antiparticle components of photons and axions are preferentially
scattered in different directions, thus producing the splitting or
decomposition of the photon and axion into their particle and antiparticle
components in an inhomogeneous magnetic field. This observable in principle
effect is of first order in the axion photon coupling, unlike the "light
shining through a wall phenomena ", which is second order.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 22:39:24 GMT"
}
] | 2010-10-27T00:00:00 | [
[
"Guendelman",
"E. I.",
""
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802.0312 | Jaroslaw Zalesny | Jaroslaw Zalesny | The simple complex numbers | LateX, 4 figures | null | null | null | physics.ed-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A new simple geometrical interpretation of complex numbers is presented. It
differs from their usual interpretation as points in the complex plane. From
the new point of view the complex numbers are rather operations on vectors than
points. Moreover, in this approach the real, imaginary and complex numbers have
similar interpretation. They are simply some operations on vectors. The
presented interpretation is simpler, more natural, and better adjusted to
possible applications in geometry and physics than the usual one, especially
for describing rotations in a plane. The relation of the new approach to the
usual interpretation and especially to the notion of complex plane is also
clarified in the paper. The new interpretation of complex numbers gives new
insight into their applications in physics, which is demonstrated by some
elementary examples in mechanics and optics
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 23:26:25 GMT"
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] | 2008-02-05T00:00:00 | [
[
"Zalesny",
"Jaroslaw",
""
]
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802.0313 | Damien James Martin | Jamison Galloway, Damien Martin and David Stancato | Comments on "Gauge Fields and Unparticles" | 7 pages, comment on arXiv:0801.0892; references added | null | null | null | hep-th hep-ph | null | The derivation of Feynman rules for unparticles carrying standard model
quantum numbers is discussed. In particular, this note demonstrates that an
application of Mandelstam's approach to constructing a gauge-invariant action
reproduces for unparticles the vertices one obtains through the usual minimal
coupling scheme; other non-trivial requirements are satisfied as well. This
approach is compared to an alternative method 0801.0892 that has recently been
constructed by A. L. Licht.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 23:33:04 GMT"
},
{
"version": "v2",
"created": "Sat, 9 Feb 2008 00:26:25 GMT"
}
] | 2008-03-02T00:00:00 | [
[
"Galloway",
"Jamison",
""
],
[
"Martin",
"Damien",
""
],
[
"Stancato",
"David",
""
]
] | [
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802.0314 | Fran\c{c}ois Nicolas | Morris Michael and Francois Nicolas and Esko Ukkonen | On the complexity of finding gapped motifs | Published in Journal of Discrete Algorithms | null | 10.1016/j.jda.2009.12.001 | null | cs.CC cs.DM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper has been withdrawn by the corresponding author because the newest
version is now published in Journal of Discrete Algorithms.
| [
{
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"created": "Mon, 4 Feb 2008 00:08:40 GMT"
},
{
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{
"version": "v3",
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{
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"created": "Wed, 18 Aug 2010 01:00:49 GMT"
},
{
"version": "v6",
"created": "Wed, 1 Sep 2010 13:21:53 GMT"
}
] | 2010-09-02T00:00:00 | [
[
"Michael",
"Morris",
""
],
[
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"Francois",
""
],
[
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"Esko",
""
]
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] |
802.0315 | Alexander Bolonkin | Alexander Bolonkin, Joseph Friedlander | Protection of Cities from Small Rockets, Missiles, Projectiles and
Mortar Shells | 21 pages, 10 figures, 2 tables | null | null | null | physics.gen-ph physics.soc-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The authors suggest a low cost closed AB-Dome, which may protect small cities
such as Sederot from rockets, mortar shells, chemical and biological weapons.
The offered AB-Dome is also very useful in peacetime because it protects the
city from outside weather (violent storms, hail) and creates a fine climate
within the Dome. The roughly hemispherical AB-Dome is a gigantic inflated thin
transparent film, located at altitude up to 1 - 5 kilometers, which converts
the city into a closed-loop air system. The film may be armored with a basalt
or steel grille or cloth pocket-retained stones that destroy (by collision or
detonation) incoming rockets, shells and other projectiles. Such an AB-Dome
would even protect the city in case of a third-party nuclear war involving
temporary poisoning of the Earth atmosphere by radioactive dust. The building
of the offered dome is easy; the film spreads on the ground, the fan engines
turn on and the cover rises to the needed altitude and is supported there by a
small internal overpressure.
The offered method is cheaper by thousands of times than protection of a city
by current anti-rocket systems. The AB-Dome may be also used (height is up to
1-5 and more kilometers) for TV, communication, long distance location,
tourism, suspended high speed and altitude windmills (energy), illumination and
entertainment (projected messages and pictures).
The authors developed the theory of AB-Dome, made estimations, computations
and computed a typical project. Discussion and results are at the end of the
article.
| [
{
"version": "v1",
"created": "Sun, 3 Feb 2008 23:57:58 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Bolonkin",
"Alexander",
""
],
[
"Friedlander",
"Joseph",
""
]
] | [
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] |
802.0316 | Yuan Xu | Yuan Xu | Fourier series and approximation on hexagonal and triangular domains | 19 pages, 2 figures | null | null | null | math.CA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Several problems on Fourier series and trigonometric approximation on a
hexagon and a triangle are studied. The results include Abel and Ces\`aro
summability of Fourier series, degree of approximation and best approximation
by trigonometric functions, both direct and inverse theorems. One of the
objective of this study is to demonstrate that Fourier series on spectral sets
enjoy a rich structure that allow an extensive theory for Fourier expansions
and approximation.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 00:04:44 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Xu",
"Yuan",
""
]
] | [
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] |
802.0317 | Adam Rennie | A. L. Carey, A. Rennie, K. Tong | Spectral flow invariants and twisted cyclic theory from the Haar state
on SU_q(2) | 25 pages, 1 figure | null | 10.1016/j.geomphys.2009.07.005 | null | math.OA math.QA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In [CPR2], we presented a K-theoretic approach to finding invariants of
algebras with no non-trivial traces. This paper presents a new example that is
more typical of the generic situation. This is the case of an algebra that
admits only non-faithful traces, namely SU_q(2), and also KMS states. Our main
results are index theorems (which calculate spectral flow), one using ordinary
cyclic cohomology and the other using twisted cyclic cohomology, where the
twisting comes from the generator of the modular group of the Haar state. In
contrast to the Cuntz algebras studied in [CPR2], the computations are
considerably more complex and interesting, because there are nontrivial `eta'
contributions to this index.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 00:15:53 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Carey",
"A. L.",
""
],
[
"Rennie",
"A.",
""
],
[
"Tong",
"K.",
""
]
] | [
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] |
802.0318 | Janka Petravic | Janka Petravic | Force autocorrelation function in linear response theory and the origin
of friction | 24 pages text and figures | null | 10.1063/1.2972977 | null | physics.chem-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Vanishing of the equilibrium Green-Kubo fluctuation expression for the
friction coefficient of a massive particle moving in a finite-volume liquid is
usually interpreted as an unphysical consequence of the finite volume. Here I
show that it is a physical consequence of the finite mass of the rest of the
system, which allows it to be dragged by the moving particle. As a consequence,
it is sufficient to have two infinite masses in the liquid for the friction
coefficient to be finite. In addition, I give the physical interpretation of
different friction coefficients for two infinite-mass particles moving in the
liquid.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 00:16:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Petravic",
"Janka",
""
]
] | [
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] |
802.0319 | Cheng-Wei Chiang | Abdesslam Arhrib, Rachid Benbrik, and Cheng-Wei Chiang | Probing triple Higgs couplings of the Two Higgs Doublet Model at Linear
Collider | 21 pages and 9 figures; one figure and some discussions added,
version to appear in PRD | Phys.Rev.D77:115013,2008 | 10.1103/PhysRevD.77.115013 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study double Higgs production at the future Linear Collider in the
framework of the Two Higgs Doublet Models through the following channels:
$e^+e^- \to \Phi_i \Phi_j Z$, $\Phi_i=h^0, H^0, A^0, H^\pm$. All these
processes are sensitive to triple Higgs couplings. Hence observations of them
provide information on the triple Higgs couplings that help reconstructing the
scalar potential. We also discuss the double Higgs-strahlung $e^+e^- \to h^0
h^0 Z$ in the decoupling limit where $h^0$ mimics the SM Higgs boson. The
processes $e^+e^- \to h^0 h^0 Z$ and $e^+e^- \to h^0 H^0 Z$ are also discussed
in the fermiophobic limit where distinctive signatures such as $4\gamma +X$,
$2\gamma +X$ and $6\gamma +X$ are expected in the Type-I Two Higgs Doublet
Model.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 00:49:31 GMT"
},
{
"version": "v2",
"created": "Wed, 7 May 2008 10:16:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Arhrib",
"Abdesslam",
""
],
[
"Benbrik",
"Rachid",
""
],
[
"Chiang",
"Cheng-Wei",
""
]
] | [
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] |
802.032 | Dennis DeTurck | Dennis DeTurck and Herman Gluck | Linking integrals in the n-sphere | 14 pages, 2 figures | null | null | null | math.GT math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let K and L be disjoint closed oriented submanifolds of the n-sphere, with
dimensions adding up to n-1. We define a map from their join K*L to the
n-sphere whose degree up to sign equals their linking number, and then use this
to find the desired linking integral.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 01:25:44 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"DeTurck",
"Dennis",
""
],
[
"Gluck",
"Herman",
""
]
] | [
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802.0321 | Cristina Manuel | Massimo Mannarelli and Cristina Manuel | Transport theory for cold relativistic superfluids from an analogue
model of gravity | 14 pages | Phys.Rev.D77:103014,2008 | 10.1103/PhysRevD.77.103014 | null | hep-ph astro-ph gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We write a covariant transport equation for the phonon excitations of a
relativistic superfluid valid at small temperatures. The hydrodynamical
equations for this system are derived from the effective field theory
associated to the superfluid phonons. We describe how to construct the kinetic
theory for the phonon quasiparticles using a relativistic generalization of the
analogue model of gravity developed by Unruh. This gravity analogy relies on
the equivalence between the action of a phonon field moving in a superfluid
background with that of a boson propagating in a given curved space-time.
Exploiting this analogy we obtain continuity equations for the phonon current,
entropy and energy-momentum tensor in a covariant form, valid in any reference
frame. Our aim is to shed light on some aspects of transport phenomena of
relativistic superfluidity. In particular, we are interested in the low
temperature regime of the color flavor locked phase, which is a color
superconducting and superfluid phase of high density QCD that may be realized
in the core of neutron stars.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 14:41:50 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mannarelli",
"Massimo",
""
],
[
"Manuel",
"Cristina",
""
]
] | [
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802.0322 | David Kubiznak | Valeri P. Frolov, David Kubiznak | Higher-Dimensional Black Holes: Hidden Symmetries and Separation of
Variables | 33 pages, no figures, updated references and corrected typos | Class.Quant.Grav.25:154005,2008 | 10.1088/0264-9381/25/15/154005 | Alberta-Thy-02-08 | hep-th gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, we discuss hidden symmetries in rotating black hole
spacetimes. We start with an extended introduction which mainly summarizes
results on hidden symmetries in four dimensions and introduces Killing and
Killing-Yano tensors, objects responsible for hidden symmetries. We also
demonstrate how starting with a principal CKY tensor (that is a closed
non-degenerate conformal Killing-Yano 2-form) in 4D flat spacetime one can
"generate" 4D Kerr-NUT-(A)dS solution and its hidden symmetries. After this we
consider higher-dimensional Kerr-NUT-(A)dS metrics and demonstrate that they
possess a principal CKY tensor which allows one to generate the whole tower of
Killing-Yano and Killing tensors. These symmetries imply complete integrability
of geodesic equations and complete separation of variables for the
Hamilton-Jacobi, Klein-Gordon, and Dirac equations in the general
Kerr-NUT-(A)dS metrics.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 01:54:00 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Mar 2008 01:56:19 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Frolov",
"Valeri P.",
""
],
[
"Kubiznak",
"David",
""
]
] | [
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] |
802.0323 | Marina Chugunova | Marina Chugunova, Vladimir Strauss | Factorization of the Indefinite Convection-Diffusion Operator | 8 pages | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that some non-self-adjoint differential operator admits
factorization and apply this new representation of the operator to construct
explicitly its domain. We also show that this operator is J-self-adjoint in
some Krein space.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 01:56:10 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Chugunova",
"Marina",
""
],
[
"Strauss",
"Vladimir",
""
]
] | [
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] |
802.0324 | C.Clare Worley | C.C.Worley, P.L.Cottrell and E.C.Wylie de Boer | s- and r-process element abundances in the CMD of 47 Tucanae using the
Robert Stobie Spectrograph on SALT | 7 pages, 11 figures | null | 10.1071/AS07031 | null | astro-ph | null | A recent study by Wylie et al 2006 has revealed that s-process element
abundances are enhanced relative to iron in both red giant branch and
asymptotic giant branch stars of 47 Tucanae. A more detailed investigation into
s-process element abundances throughout the colour-magnitude diagram of 47
Tucanae is vital in order to determine whether the observed enhancements are
intrinsic to the cluster. This paper explores this possibility through
observational and theoretical means. The visibility of s- and r-process element
lines in synthetic spectra of giant and dwarf stars throughout the colour
magnitude diagram of 47 Tucanae has been explored. It was determined that a
resolving power of 10 000 was sufficient to observe s-process element abundance
variations in globular cluster giant branch stars. These synthetic results were
compared with the spectra of eleven 47 Tucanae giant branch stars observed
during the performance verification of the Robert Stobie Spectrograph on the
Southern African Large Telescope. Three s-process elements, Zr, Ba, Nd, and one
r-process element, Eu, were investigated. No abundance variations were found
such that [X/Fe] = 0.0 +/- 0.5 dex. It was concluded that this resolving power,
R ~ 5000, was not sufficient to obtain exact abundances but upper limits on the
s-process element abundances could be determined.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 02:34:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Worley",
"C. C.",
""
],
[
"Cottrell",
"P. L.",
""
],
[
"de Boer",
"E. C. Wylie",
""
]
] | [
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] |
802.0325 | Yue Chongxing | Chong-Xing Yue, Li Ding, Wei Ma | The new charged gauge boson $W'$ and the subprocess $eq\to\nu q'$ at
$e^{+}e^{-}$ and $ep$ colliders | 18 pages, 6 figures, typos corrected, references added | Eur.Phys.J.C55:615-622,2008 | 10.1140/epjc/s10052-008-0618-2 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In the framework of the little Higgs models and the three-site Higgsless
model, we discuss the contributions of the new charged gauge boson $W'$ to the
process $eq\to\nu q'$ and the possibility of detecting $W'$ via this process in
future high energy linear $e^{+}e^{-}$ collider $(ILC)$ and $ep$ collider
$(THERA)$ experiments. Our numerical results show that the process $eq\to\nu
q'$ is rather sensitive to the coupling $W'ff'$ and one can use this process to
distinguish different new physics models in future $ILC$ and $THERA$
experiments.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 02:01:51 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Mar 2008 11:36:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Yue",
"Chong-Xing",
""
],
[
"Ding",
"Li",
""
],
[
"Ma",
"Wei",
""
]
] | [
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] |
802.0326 | David Garcia-Alvarez | D.Garcia-Alvarez (Imperial College London), J.J.Drake (SAO),
V.L.Kashyap (SAO), L.Lin (SAO), B.Ball (SAO) | Coronal Structure and Abundances in Young Fast Rotators | 22 pages, 8 figures, 6 tables. Accepted by ApJ | null | 10.1086/587611 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | AB Dor, Speedy Mic and Rst137B are in their early post-T Tauri evolutionary
phase (<100Myr), at the age of fastest rotation in the life of late-type stars.
They straddle the coronal saturation-supersaturation boundary first defined by
young stars in open clusters. High resolution Chandra X-ray spectra have been
analysed to study their coronal properties as a function of coronal activity
parameters Rossby number, $L_X/L_{bol}$ and a coronal temperature index. Plasma
emission measure distributions as a function of temperature show broad peaks at
T~10e7K. Differences between stars suggest that as supersaturation is reached
the DEM slope below the temperature of peak DEM becomes shallower, while the
DEM drop-off above this temperature becomes more pronounced. A larger sample
comprising our three targets and 22 active stars studied in the recent
literature reveals a general increase of plasma at T>10e7 toward the
saturated-supersaturated boundary but a decline beyond this among
supersaturated stars. All three of the stars studied in detail here show lower
coronal abundances of the low FIP elements Mg, Si and Fe, relative to the high
FIP elements S, O and Ne, as compared to the solar mixture. The coronal Fe
abundances of the stellar sample are inversely correlated with Lx/Lbol,
declining slowly with rising Lx/Lbol, but with a much more sharp decline at
Lx/Lbol>3x10e-4. For dwarfs the Fe abundance is also well-correlated with
Rossby number. The coronal O/Fe ratios for dwarfs show a clear increase with
decreasing Rossby number, apparently reaching saturation at [O/Fe]=0.5 at the
coronal supersaturation boundary. Similar increases in O/Fe with increasing
coronal temperature and $L_X/L_{bol}$ are seen.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 02:11:36 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Garcia-Alvarez",
"D.",
"",
"Imperial College London"
],
[
"Drake",
"J. J.",
"",
"SAO"
],
[
"Kashyap",
"V. L.",
"",
"SAO"
],
[
"Lin",
"L.",
"",
"SAO"
],
[
"Ball",
"B.",
"",
"SAO"
]
] | [
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] |
802.0327 | Adam Showman | Adam P. Showman, Curtis S. Cooper, Jonathan J. Fortney, and Mark S.
Marley | Atmospheric Circulation of Hot Jupiters: Three-dimensional circulation
models of HD 209458b and HD 189733b with Simplified Forcing | 17 pages, 14 figures, submitted for publication in ApJ | null | 10.1086/589325 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present global, three-dimensional numerical simulations of the atmospheric
circulation on HD 209458b and HD 189733b and calculate the infrared spectra and
light curves predicted by these simulations, which we compare with available
observations. Radiative heating/cooling is parameterized with a simplified
Newtonian relaxation scheme. Our simulations develop day-night temperature
contrasts that vary strongly with pressure. At low pressure (<10 mbar), air
flows from the substellar point toward the antistellar point, both along the
equator and over the poles. At deeper levels, the flow develops an eastward
equatorial jet with speeds of 3-4 km/sec, with weaker westward flows at high
latitudes. This basic flow pattern is robust to variations in model resolution,
gravity, radiative time constant, and initial temperature structure. Nightside
spectra show deep absorption bands of H2O, CO, and/or CH4, whereas on the
dayside these absorption bands flatten out or even flip into emission. This
results from the strong effect of dynamics on the vertical temperature-pressure
structure; the temperature decreases strongly with altitude on the nightside
but becomes almost isothermal on the dayside. In Spitzer bandpasses, our
predicted planet-to-star flux ratios vary by a factor of 2-10 with orbital
phase, depending on the wavelength and chemistry. For HD 189733b, where a
detailed 8-micron light curve has been obtained, we correctly produce the
observed phase offset of the flux maximum, but we do not explain the flux
minimum and we overpredict the total flux variation. This discrepancy likely
results from the simplifications inherent in the Newtonian relaxation scheme
and provides motivation for incorporating realistic radiative transfer in
future studies.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 02:28:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Showman",
"Adam P.",
""
],
[
"Cooper",
"Curtis S.",
""
],
[
"Fortney",
"Jonathan J.",
""
],
[
"Marley",
"Mark S.",
""
]
] | [
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802.0328 | Yunkyu Bang | Yunkyu Bang | Effects of phonon interaction on the pairing in the high-T$c$
superconductors | 9 pages, 10 figures | Phys. Rev. B 78, 075116 (2008) | 10.1103/PhysRevB.78.075116 | null | cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the effects of phonon interaction on the superconducting pairing in
the background of a d-wave gap, mediated by antiferromagnetic (AFM) spin
fluctuations, using coupled BCS gap equations. We found that phonon interaction
can induce a s-wave component to the d-wave gap in the (D+S) form with an
interaction anisotropy and in the (D+$i$S) form without anisotropy,
respectively. In either case, however, T$_c$ is not enhanced compared to the
pure d-wave pairing without phonon interaction. On the other hand, anisotropic
phonon interaction can dramatically enhance the d-wave pairing itself and
therefore T$_c$, together with the AFM spin fluctuation interaction. This
(D$_{AFM}$ + D$_{ph}$) type pairing exhibits strongly reduced isotope
coefficient despite the large enhancement of T$_c$ by phonon interaction.
Finally, we study the combined type of (D$_{AFM}$ + D$_{ph}$ +$i$S)) gap and
calculate the penetration depth and specific heat to be compared with the
experiments.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 03:00:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bang",
"Yunkyu",
""
]
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] |
802.0329 | Tohya Hiroshima | Tohya Hiroshima | Bound entangled states with non-positive partial transpose exist | This paper has been withdrawn by the author, due a crucial error in
the optimization. For the last one month I have been trying to remove the
error, but it seems to take a lot of time so I decided to withdraw this paper
for the moment | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper has been withdrawn by the author, due a crucial error in the
optimization. For the last one month I have been trying to remove the error,
but it seems to take a lot of time so I decided to withdraw this paper for the
moment.
| [
{
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},
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},
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"created": "Mon, 31 Mar 2008 03:27:28 GMT"
},
{
"version": "v5",
"created": "Wed, 7 May 2008 08:02:38 GMT"
}
] | 2008-05-07T00:00:00 | [
[
"Hiroshima",
"Tohya",
""
]
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802.033 | Stefano Ansoldi | Stefano Ansoldi | Spherical black holes with regular center: a review of existing models
including a recent realization with Gaussian sources | LaTeX, 36 pages, 10 figures. 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-2108 | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We review, in a historical perspective, some results about black hole
spacetimes with a regular center. We then see how their properties are realized
in a specific solution that recently appeared; in particular we analyze in
detail the (necessary) violation of the strong energy condition.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 03:13:00 GMT"
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] | 2008-02-05T00:00:00 | [
[
"Ansoldi",
"Stefano",
""
]
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802.0331 | George Lowther | George Lowther | Nondifferentiable functions of one-dimensional semimartingales | Published in at http://dx.doi.org/10.1214/09-AOP476 the Annals of
Probability (http://www.imstat.org/aop/) by the Institute of Mathematical
Statistics (http://www.imstat.org) | Annals of Probability 2010, Vol. 38, No. 1, 76-101 | 10.1214/09-AOP476 | IMS-AOP-AOP476 | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider decompositions of processes of the form $Y=f(t,X_t)$ where $X$ is
a semimartingale. The function $f$ is not required to be differentiable, so
It\^{o}'s lemma does not apply. In the case where $f(t,x)$ is independent of
$t$, it is shown that requiring $f$ to be locally Lipschitz continuous in $x$
is enough for an It\^{o}-style decomposition to exist. In particular, $Y$ will
be a Dirichlet process. We also look at the case where $f(t,x)$ can depend on
$t$, possibly discontinuously. It is shown, under some additional mild
constraints on $f$, that the same decomposition still holds. Both these results
follow as special cases of a more general decomposition which we prove, and
which applies to nondifferentiable functions of Dirichlet processes. Possible
applications of these results to the theory of one-dimensional diffusions are
briefly discussed.
| [
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{
"version": "v3",
"created": "Tue, 26 Jan 2010 09:15:56 GMT"
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] | 2010-01-26T00:00:00 | [
[
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""
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] |
802.0332 | Boldizsar Kalmar | Boldizsar Kalmar | Cobordisms of fold maps of 4-manifolds into the space | 11 pages, revised version | null | null | null | math.GT math.AT | null | We compute the oriented cobordism group of fold maps of 4-manifolds into the
space with all the possible restrictions (and also with no restriction) to the
singular fibers. We also give geometric invariants which describe completely
the cobordism group of fold maps.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 15:45:24 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Mar 2008 14:02:01 GMT"
},
{
"version": "v3",
"created": "Mon, 12 May 2008 16:12:53 GMT"
}
] | 2008-05-12T00:00:00 | [
[
"Kalmar",
"Boldizsar",
""
]
] | [
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] |
802.0333 | Lan Zhou | Yu Guo, Lan Zhou, Le-Man Kuang, C.P. Sun | Magneto-Optical Stern-Gerlach Effect in Atomic Ensemble | 7 pages, 5 figures | Phys. Rev. A 78, 013833 (2008) | 10.1103/PhysRevA.78.013833 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the birefringence of the quantized polarized light in a
magneto-optically manipulated atomic ensemble as a generalized Stern-Gerlach
Effect of light. To explain this engineered birefringence microscopically, we
derive an effective Shr\"odinger equation for the spatial motion of two
orthogonally polarized components, which behave as a spin with an effective
magnetic moment leading to a Stern-Gerlach split in an nonuniform magnetic
field. We show that electromagnetic induced transparency (EIT) mechanism can
enhance the magneto-optical Stern-Gerlach effect of light in the presence of a
control field with a transverse spatial profile and a inhomogeneous magnetic
field.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 05:11:34 GMT"
},
{
"version": "v2",
"created": "Mon, 26 May 2008 03:47:30 GMT"
},
{
"version": "v3",
"created": "Wed, 20 Aug 2008 14:18:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Guo",
"Yu",
""
],
[
"Zhou",
"Lan",
""
],
[
"Kuang",
"Le-Man",
""
],
[
"Sun",
"C. P.",
""
]
] | [
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] |
802.0334 | Masashi Shiraishi | Ryo Nouchi, Haruo Tomita, Akio Ogura, Masashi Shiraishi, Hiromichi
Kataura | Logic Ciucuits Using Solution-processed Single-walled Carbon Nanotue
Transistors | 12 PAGES, 3 FIGURES | Applied Physics Letters 92, 253507 (2008). | 10.1063/1.2949686 | null | cond-mat.mtrl-sci cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This letter reports on the realization of logic circuits employing
solution-processed networks of single-walled carbon nanotubes. We constructed
basic logic gates (inverter, NAND and NOR) with n- and p-type field-effect
transistors fabricated by solution-based chemical doping. Complementary
metal-oxide-semiconductor inverters exhibited voltage gains of up to 20, which
illustrates the great potential of carbon nanotube networks for printable
flexible electronics.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 05:13:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nouchi",
"Ryo",
""
],
[
"Tomita",
"Haruo",
""
],
[
"Ogura",
"Akio",
""
],
[
"Shiraishi",
"Masashi",
""
],
[
"Kataura",
"Hiromichi",
""
]
] | [
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802.0335 | Motoki Kino | M. Kino (ISAS/Jaxa), F. Takahara (Osaka Univ.) | Invisible Plasma Content in Blazars? The Case of Markarian 421 | 4 pages, 2 figure for the proceedings of 'Approaching Micro-Arcsecond
Resolution with VSOP-2: Astrophysics and Technology' (3-7 December 2007,
ISAS/JAXA, Sagamihara, Japan) | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Invisible plasma content in blazar jets such as protons and/or thermal
electron-positron ($e^{\pm}$) pairs is explored through combined arguments of
dynamical and radiative processes. By comparing physical quantities required by
the internal shock model with those obtained through the observed
radio-to-gamma-ray spectra for Mrk 421, we find the existence of a copious
amount of invisible plasma in the jet. We speculate that the blazar sequence
could arise from variations of total amount and/or blending ratio of $e^{\pm}$
pair and electron-proton plasma.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 05:34:47 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Kino",
"M.",
"",
"ISAS/Jaxa"
],
[
"Takahara",
"F.",
"",
"Osaka Univ."
]
] | [
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] |
802.0336 | Minzu Wang | The Belle Collaboration: J. H. Chen, M.-Z. Wang, et al | Observation of B0 to p pbar K*0 with a large K*0 polarization | 11 pages, 4 figures (8 figure files), submitted to Phys.Rev.Lett | Phys.Rev.Lett.100:251801,2008 | 10.1103/PhysRevLett.100.251801 | Belle Preprint 2008-5; KEK Preprint 2007-77 | hep-ex | null | We observe the decay B0 to p pbar K*0 with a branching fraction of
(1.18^{+0.29}_{-0.25} (stat.) \pm 0.11 (syst.)) \times 10^{-6}. The statistical
significance is 7.2 sigma for the signal in the low ppbar mass region. We study
the decay dynamics of B0 to p pbar K*0 and compare it with B+ to p pbar K*+.
The K*0 meson is found to be almost 100% polarized (with a fraction of (101 \pm
13 \pm 3)% in the helicity zero state), while the K*+ meson has a (32 \pm 17
\pm 9)% fraction in the helicity zero state. The direct CP asymmetries for B0
to p pbar K*0 and B+ to p pbar K*+ are measured to be -0.08\pm 0.20\pm 0.02 and
-0.01\pm 0.19\pm 0.02, respectively. We also study the characteristics of the
low mass ppbar enhancements near threshold and the associated angular
distributions. In addition, we report improved measurements of the branching
fractions BF(B+ to p pbar K*+) = (3.38^{+0.73}_{-0.60} \pm 0.39) \times 10^{-6}
and BF(B0 to p pbar K0) = (2.51^{+0.35}_{-0.29} \pm 0.21) \times 10^{-6}, which
supersede our previous measurements. These results are obtained from a 492
fb^{-1} data sample collected near the Upsilon(4S) resonance with the Belle
detector at the KEKB asymmetric-energy e^+ e^- collider.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 06:27:24 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Apr 2008 03:34:37 GMT"
},
{
"version": "v3",
"created": "Fri, 30 May 2008 07:46:19 GMT"
}
] | 2009-02-19T00:00:00 | [
[
"The Belle Collaboration",
"",
""
],
[
"Chen",
"J. H.",
""
],
[
"Wang",
"M. -Z.",
""
]
] | [
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] |
802.0337 | Tatsuhiko Yagasaki | Taras Banakh, Kotaro Mine, Katsuro Sakai and Tatsuhiko Yagasaki | Homeomorphism and diffeomorphism groups of non-compact manifolds with
the Whitney topology | 21 pages, Sections 3, 5.2, 5.3, 6, 7 in the previous version (arXiv:
0802.0337v1) will be included in another paper cited as Ref. [6] | null | null | null | math.GT math.GN | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For a non-compact n-manifold M let H(M) denote the group of homeomorphisms of
M endowed with the Whitney topology and H_c(M) the subgroup of H(M) consisting
of homeomorphisms with compact support. It is shown that the group H_c(M) is
locally contractible and the identity component H_0(M) of H(M) is an open
normal subgroup in H_c(M). This induces the topological factorization H_c(M)
\approx H_0(M) \times \M_c(M) for the mapping class group \M_c(M) =
H_c(M)/H_0(M) with the discrete topology. Furthermore, for any non-compact
surface M, the pair (H(M), H_c(M)) is locally homeomorphic to (\square^w
l_2,\cbox^w l_2) at the identity id_M of M. Thus the group H_c(M) is an (l_2
\times R^\infty)-manifold. We also study topological properties of the group
D(M) of diffeomorphisms of a non-compact smooth n-manifold M endowed with the
Whitney C^\infty-topology and the subgroup D_c(M) of D(M) consisting of all
diffeomorphisms with compact support. It is shown that the pair (D(M),D_c(M))
is locally homeomorphic to (\square^w l_2, \cbox^w l_2) at the identity id_M of
M.
Hence the group D_c(M) is a topological (l_2 \times R^\infty)-manifold for
any dimension n.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 06:29:49 GMT"
},
{
"version": "v2",
"created": "Wed, 24 Feb 2010 03:48:25 GMT"
}
] | 2010-02-24T00:00:00 | [
[
"Banakh",
"Taras",
""
],
[
"Mine",
"Kotaro",
""
],
[
"Sakai",
"Katsuro",
""
],
[
"Yagasaki",
"Tatsuhiko",
""
]
] | [
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] |
802.0338 | Motomu Tsuda | Kazunari Shima and Motomu Tsuda | On N = 2 superfield for N = 2 vector supermultiplet in two dimensional
spacetime | 8 pages, some discussions changed, references added | Mod.Phys.Lett.A23:1167-1173,2008 | 10.1142/S0217732308027096 | null | hep-th | null | We focus on the superfield formulation for a N = 2 vector supermultiplet in
two dimensional spacetime and explicitly show that the Wess-Zumino gauge
condition for a N = 2 superfield is compatible with familiar SUSY (plus U(1)
gauge) transformations for the vector supermultiplet. N = 2 SUSY invariant mass
and Yukawa interaction terms for the vector supermultiplet are also constructed
from the superfield explicitly in addition to a free (kinetic) action.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 06:34:03 GMT"
},
{
"version": "v2",
"created": "Sat, 16 Feb 2008 04:27:55 GMT"
},
{
"version": "v3",
"created": "Mon, 3 Mar 2008 05:41:39 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Shima",
"Kazunari",
""
],
[
"Tsuda",
"Motomu",
""
]
] | [
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] |
802.0339 | Ben Morris | Ben Morris | Improved mixing time bounds for the Thorp shuffle and L-reversal chain | 20 pages | null | null | null | math.PR | null | We prove a theorem that reduces bounding the mixing time of a card shuffle to
verifying a condition that involves only pairs of cards, then we use it to
obtain improved bounds for two previously studied models.
E. Thorp introduced the following card shuffling model in 1973. Suppose the
number of cards n is even. Cut the deck into two equal piles. Drop the first
card from the left pile or from the right pile according to the outcome of a
fair coin flip. Then drop from the other pile. Continue this way until both
piles are empty. We obtain a mixing time bound of O(log^4 n). Previously, the
best known bound was O(log^{29} n) and previous proofs were only valid for n a
power of 2.
We also analyze the following model, called the L-reversal chain, introduced
by Durrett. There are n cards arrayed in a circle. Each step, an interval of
cards of length at most L is chosen uniformly at random and its order is
reversed. Durrett has conjectured that the mixing time is O(max(n, n^3/L^3) log
n). We obtain a bound that is within a factor O(log^2 n) of this,the first
bound within a poly log factor of the conjecture.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 06:44:31 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Morris",
"Ben",
""
]
] | [
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] |
802.034 | Redouane Mecheri | R. Mecheri, E. Marsch (Max Planck Institute for Solar System Research) | Drift instabilities in the solar corona within the multi-fluid
description | 9 pages, 7 figures, accepted for publication in Astronomy &
Astrophysics | null | 10.1051/0004-6361:20079221 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Recent observations revealed that the solar atmosphere is highly structured
in density, temperature and magnetic field. The presence of these gradients may
lead to the appearance of currents in the plasma, which in the weakly
collisional corona can constitute sources of free energy for driving
micro-instabilities. Such instabilities are very important since they represent
a possible source of ion-cyclotron waves which have been conjectured to play a
prominent role in coronal heating, but whose solar origin remains unclear.
Considering a density stratification transverse to the magnetic field, this
paper aims at studying the possible occurrence of gradient-induced plasma
micro-instabilities under typical conditions of coronal holes. Taking into
account the WKB (Wentzel-Kramers-Brillouin) approximation, we perform a Fourier
plane waves analysis using the collisionless multi-fluid model. By neglecting
the electron inertia, this model allows us to take into account ion-cyclotron
wave effects that are absent from the one-fluid model of magnetohydrodynamics
(MHD). Realistic models of density and temperature, as well as a 2-D analytical
magnetic-field model, are used to define the background plasma in the
open-field funnel in a polar coronal hole. The ray-tracing theory is used to
compute the ray path of the unstable waves, as well as the evolution of their
growth rates during the propagation. We demonstrate that in typical coronal
hole conditions, and when assuming typical transverse density length scales
taken from radio observations, the current generated by a relative electron-ion
drift provides enough free energy for driving the mode unstable. This
instability results from a coupling between oppositely propagating slow-mode
waves.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 16:00:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mecheri",
"R.",
"",
"Max Planck Institute for Solar System Research"
],
[
"Marsch",
"E.",
"",
"Max Planck Institute for Solar System Research"
]
] | [
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802.0341 | Christian Schunck H. | Christian H. Schunck, Yong-il Shin, Andre Schirotzek, and Wolfgang
Ketterle | Determination of the Fermion Pair Size in a Resonantly Interacting
Superfluid | 8 pages, 7 figures; Figures updated; New Figures added; Updated
discussion of fit functions | Nature 454, 739-743 (2008) | 10.1038/nature07176 | null | cond-mat.supr-con cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Fermionic superfluidity requires the formation of pairs. The actual size of
these fermion pairs varies by orders of magnitude from the femtometer scale in
neutron stars and nuclei to the micrometer range in conventional
superconductors. Many properties of the superfluid depend on the pair size
relative to the interparticle spacing. This is expressed in BCS-BEC crossover
theories, describing the crossover from a Bardeen-Cooper-Schrieffer (BCS) type
superfluid of loosely bound and large Cooper pairs to Bose-Einstein
condensation (BEC) of tightly bound molecules. Such a crossover superfluid has
been realized in ultracold atomic gases where high temperature superfluidity
has been observed. The microscopic properties of the fermion pairs can be
probed with radio-frequency (rf) spectroscopy. Previous work was difficult to
interpret due to strong and not well understood final state interactions. Here
we realize a new superfluid spin mixture where such interactions have
negligible influence and present fermion-pair dissociation spectra that reveal
the underlying pairing correlations. This allows us to determine the
spectroscopic pair size in the resonantly interacting gas to be 2.6(2)/kF (kF
is the Fermi wave number). The pairs are therefore smaller than the
interparticle spacing and the smallest pairs observed in fermionic superfluids.
This finding highlights the importance of small fermion pairs for superfluidity
at high critical temperatures. We have also identified transitions from fermion
pairs into bound molecular states and into many-body bound states in the case
of strong final state interactions.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 07:51:01 GMT"
},
{
"version": "v2",
"created": "Fri, 13 Jun 2008 17:55:27 GMT"
}
] | 2008-08-14T00:00:00 | [
[
"Schunck",
"Christian H.",
""
],
[
"Shin",
"Yong-il",
""
],
[
"Schirotzek",
"Andre",
""
],
[
"Ketterle",
"Wolfgang",
""
]
] | [
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] |
802.0342 | Bobak Nazer | Bobak Nazer and Michael Gastpar | The Case for Structured Random Codes in Network Capacity Theorems | 23 pages, 7 figures, To appear in European Transactions on
Telecommunication: Special Issue on New Directions in Information Theory | null | null | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Random coding arguments are the backbone of most channel capacity
achievability proofs. In this paper, we show that in their standard form, such
arguments are insufficient for proving some network capacity theorems:
structured coding arguments, such as random linear or lattice codes, attain
higher rates. Historically, structured codes have been studied as a stepping
stone to practical constructions. However, K\"{o}rner and Marton demonstrated
their usefulness for capacity theorems through the derivation of the optimal
rate region of a distributed functional source coding problem. Here, we use
multicasting over finite field and Gaussian multiple-access networks as
canonical examples to demonstrate that even if we want to send bits over a
network, structured codes succeed where simple random codes fail. Beyond
network coding, we also consider distributed computation over noisy channels
and a special relay-type problem.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 07:14:40 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Nazer",
"Bobak",
""
],
[
"Gastpar",
"Michael",
""
]
] | [
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] |
802.0343 | D.N. Triantafyllopoulos | E. Iancu, M.S. Kugeratski, D.N. Triantafyllopoulos | Geometric Scaling in Mueller-Navelet Jets | 24 pages | Nucl.Phys.A808:95-116,2008 | 10.1016/j.nuclphysa.2008.05.003 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We argue that the production of Mueller-Navelet jets at the LHC represents a
convenient environment to study gluon saturation and high energy scattering in
the presence of unitarity corrections. We show that, in a suitable range of
transverse momenta for the produced jets, the cross section for the partonic
subprocess should exhibit geometric scaling. We point out that, in the presence
of a running coupling, the cross section for producing hard jets cannot be
fully computed in perturbation theory, not even after taking into account the
saturation effects: the non-perturbative physics affects the overall
normalization of the cross section, but not also its geometric scaling
behavior.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 07:17:11 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Iancu",
"E.",
""
],
[
"Kugeratski",
"M. S.",
""
],
[
"Triantafyllopoulos",
"D. N.",
""
]
] | [
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] |
802.0344 | Toshihiko Masuda | Toshihiko Masuda, Reiji Tomatsu | Approximate innerness and central triviality of endomorphisms | 57 pages | null | null | null | math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce the notions of approximate innerness and central triviality for
endomorphisms on separable von Neumann factors, and we characterize them for
hyperfinite factors by Connes-Takesaki modules of endomorphisms and modular
endomorphisms which are introduced by Izumi. Our result is a generalization of
the corresponding result obtained by Kawahigashi-Sutherland-Takesaki in
automorphism case.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 07:28:59 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Masuda",
"Toshihiko",
""
],
[
"Tomatsu",
"Reiji",
""
]
] | [
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] |
802.0345 | A. M. Kamchatnov | E.G. Khamis, A. Gammal, G.A. El, Yu.G. Gladush, A.M. Kamchatnov | Nonlinear diffraction of light beams propagating in photorefractive
media with embedded reflecting wire | 18 pages | null | 10.1103/PhysRevA.78.013829 | null | nlin.PS | null | The theory of nonlinear diffraction of intensive light beams propagating
through photorefractive media is developed. Diffraction occurs on a reflecting
wire embedded in the nonlinear medium at relatively small angle with respect to
the direction of the beam propagation. It is shown that this process is
analogous to the generation of waves by a flow of a superfluid past an
obstacle. The ``equation of state'' of such a superfluid is determined by the
nonlinear properties of the medium. On the basis of this hydrodynamic analogy,
the notion of the ``Mach number'' is introduced where the transverse component
of the wave vector plays the role of the fluid velocity. It is found that the
Mach cone separates two regions of the diffraction pattern: inside the Mach
cone oblique dark solitons are generated and outside the Mach cone the region
of ``ship waves'' is situated. Analytical theory of ``ship waves'' is developed
and two-dimensional dark soliton solutions of the equation describing the beam
propagation are found. Stability of dark solitons with respect to their decay
into vortices is studied and it is shown that they are stable for large enough
values of the Mach number.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:27:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Khamis",
"E. G.",
""
],
[
"Gammal",
"A.",
""
],
[
"El",
"G. A.",
""
],
[
"Gladush",
"Yu. G.",
""
],
[
"Kamchatnov",
"A. M.",
""
]
] | [
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] |
802.0346 | Marco Genovese | G.Brida, M.Chekhova, M.Genovese, M.L.Rastello and I.Ruo-Berchera | Absolute calibration of Analog Detectors using Stimulated Parametric
Down Conversion | null | Journal of Modern Optics 56 (2009) 401. | 10.1080/09500340802318317 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Spontaneous parametric down conversion has been largely exploited as a tool
for absolute calibration of photon counting detectors, photomultiplier tubes or
avalanche photodiodes working in Geiger regime. In this work we investigate the
extension of this technique from very low photon flux of photon counting regime
to the absolute calibration of analog photodetectors at higher photon flux.
Moving toward higher photon rate, i.e. at high gain regime, with the
spontaneous parametric down conversion shows intrinsic limitations of the
method, while the stimulated parametric down conversion process, where a seed
beam properly injected into the crystal in order to increase the photon
generation rate in the conjugate arm, allows us to work around this problem. A
preliminary uncertainty budget is discussed.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 16:48:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Brida",
"G.",
""
],
[
"Chekhova",
"M.",
""
],
[
"Genovese",
"M.",
""
],
[
"Rastello",
"M. L.",
""
],
[
"Ruo-Berchera",
"I.",
""
]
] | [
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] |
802.0347 | Dr. Peter S"ule | P. S\"ule | Self-organized transient facilitated atomic transport in Pt/Al(111) | 12 pages, 8 figures, full paper at:
http://www.mfa.kfki.hu/~sule/papers/ptonal.pdf . J. Chem. Phys. (2008), in
press | null | 10.1063/1.2841452 | null | cond-mat.mtrl-sci cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | During the course of atomic transport in a host material, impurity atoms need
to surmount an energy barrier driven by thermodynamic bias or at ultra-low
temperatures by quantum tunneling. In the present article we demonstrate using
atomistic simulations that at ultra-low temperature transient inter-layer
atomic transport is also possible without tunneling when the Pt/Al(111)
impurity/host system self-organizes itself spontaneously into an intermixed
configuration. No such extremely fast athermal concerted process has been
reported before at ultra low temperatures. The outlined novel transient atomic
exchange mechanism could be of general validity. We find that the source of
ultra-low temperature heavy particle barrier crossing is intrinsic and no
external bias is necessary for atomic intermixing and surface alloying in Pt/Al
although the dynamic barrier height is few eV. The mechanism is driven by the
local thermalization of the Al(111) surface in a self-organized manner arranged
spontaneously by the system without any external stimulus. The core of the
short lived thermalized region reaches the local temperature of $\sim 1000$ K
(including few tens of Al atoms) while the average temperature of the
simulation cell is $\sim 3$ K. The transient facilitated intermixing process
also takes place with repulsive impurity-host interaction potential leading to
negative atomic mobility hence the atomic injection is largely independent of
the strength of the impurity-surface interaction. We predict that similar
exotic behaviour is possible in other materials as well.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:12:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Süle",
"P.",
""
]
] | [
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802.0348 | Zhongshui Ma | Zhongshui Ma | Thermospin Hall effect generated by thermal influence and thermoelectric
effect | 16 pages | null | null | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, we present the theoretical predication of a thermospin Hall
effect, in which a transverse spin current can be generated in semiconductors
in the presence of spin-orbit coupling by a frequency-dependent longitudinal
temperature gradient. Because of the thermoelectric effect, there is no net
charge current but there is a heat flow from the hot side to the cold side. We
perform the theoretical calculation of dynamical thermospin Hall conductivity
in a two-dimensional Rashba spintronic system. It has been shown that the
direct interband optical transition dominates the ordering and manipulation of
spin in the generation of a transverse intrinsic spin current. In view of the
role of the thermoelectric effect, the contributions to the thermospin Hall
effect are classified as that originating from a direct contribution of thermal
electronic diffusion and that from the compensatory electron flow in balance
with the thermal diffusion. For a finite system, the analysis yields evidence
that the spin accumulation around the edges of a plate determines the
magnetization. In equilibrium, a field created by a magnetization gradient
emerges in the direction perpendicular to the temperature gradient. The
experimental observation of the thermospin Hall effect is proposed by measuring
the longitudinal temperature difference with the injection of a transverse spin
current and by analyzing the Hall angle. In addition, in order to achieve pure
spin accumulation in the spin Hall effect, an extension of the thermospin Hall
effect for exciting electron-hole pairs in semiconductors is proposed.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:15:20 GMT"
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] | 2008-02-05T00:00:00 | [
[
"Ma",
"Zhongshui",
""
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] |
802.0349 | Elijah Liflyand | E. Ostrovsky, E. Rogover | Exact exponential bounds for the random field maximum distribution via
the majoring measures (generic chaining) | 18 pages | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper non-asymptotic exact exponential estimates are derived for the
tail of maximum distribution of random field in the terms of majoring measures
or, equally, generic chaining.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:39:00 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Ostrovsky",
"E.",
""
],
[
"Rogover",
"E.",
""
]
] | [
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802.035 | Paolo Esposito | A. Pellizzoni (1), A. Tiengo (1), A. De Luca (1,2,3), P. Esposito
(1,3,4), S. Mereghetti (1) ((1) INAF-IASF Milano, Italy, (2) IUSS Pavia,
Italy, (3) Universit\`a di Pavia, DFNT, Italy, (4) INFN-Pavia, Italy) | PSR J0737-3039: Interacting Pulsars in X-Rays | Revised to match the final version. Typos corrected | The Astrophysical Journal, Volume 679, Issue 1, pp. 664-674 (2008) | 10.1086/587053 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present the results of a ~230 ks long X-ray observation of the
relativistic double-pulsar system PSR J0737-3039 obtained with the XMM-Newton
satellite in 2006 October. We confirm the detection in X-rays of pulsed
emission from PSR J0737-3039A (PSR A), mostly ascribed to a soft non-thermal
power-law component (photon index ~ 3.3) with a 0.2-3 keV luminosity of
~1.9E+30 erg/s (assuming a distance of 500 pc). For the first time, pulsed
X-ray emission from PSR J0737-3039B (PSR B) is also detected in part of the
orbit. This emission, consistent with thermal radiation with temperature kT=30
eV and a bolometric luminosity of ~1E+32 erg/s, is likely powered by heating of
PSR B's surface caused by PSR A's wind. A hotter (~130 eV) and fainter (~5E+29
erg/s) thermal component, probably originating from back-falling particles
heating polar caps of either PSR A or PSR B is also required by the data. No
signs of X-ray emission from a bow-shock between PSR A's wind and the
interstellar medium or PSR B's magnetosphere are present. The upper limit on
the luminosity of such a shock component (~1E+29 erg/s) constrains the wind
magnetization parameter sigma of PSR A to values greater than 1.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:39:46 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Mar 2008 23:53:58 GMT"
}
] | 2009-02-23T00:00:00 | [
[
"Pellizzoni",
"A.",
""
],
[
"Tiengo",
"A.",
""
],
[
"De Luca",
"A.",
""
],
[
"Esposito",
"P.",
""
],
[
"Mereghetti",
"S.",
""
]
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] |
802.0351 | Sunil Srinivasa | Sunil Srinivasa and Martin Haenggi | Path Loss Exponent Estimation in a Large Field of Interferers | Work underway | null | null | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In wireless channels, the path loss exponent (PLE) has a strong impact on the
quality of links, and hence, it needs to be accurately estimated for the
efficient design and operation of wireless networks. In this paper, we address
the problem of PLE estimation in large wireless networks, which is relevant to
several important issues in networked communications such as localization,
energy-efficient routing, and channel access. We consider a large ad hoc
network where nodes are distributed as a homogeneous Poisson point process on
the plane and the channels are subject to Nakagami-m fading. We propose and
discuss three distributed algorithms for estimating the PLE under these
settings which explicitly take into account the interference in the network. In
addition, we provide simulation results to demonstrate the performance of the
algorithms and quantify the estimation errors. We also describe how to estimate
the PLE accurately even in networks with spatially varying PLEs and more
general node distributions.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 17:04:15 GMT"
},
{
"version": "v2",
"created": "Sat, 7 Nov 2009 06:16:41 GMT"
},
{
"version": "v3",
"created": "Mon, 23 Jan 2012 01:46:49 GMT"
}
] | 2012-01-24T00:00:00 | [
[
"Srinivasa",
"Sunil",
""
],
[
"Haenggi",
"Martin",
""
]
] | [
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] |
802.0352 | Sergei Zvyagin | S. A. Zvyagin, J. Wosnitza, A. K. Kolezhuk, V. S. Zapf, M. Jaime, A.
Paduan-Filho, V. N. Glazkov, S. S. Sosin, A. I. Smirnov | Spin Dynamics of $Ni Cl_2-4SC(NH_2)_2$ in the Field-Induced Ordered
Phase | 4 pages, 3 figures | null | 10.1103/PhysRevB.77.092413 | null | cond-mat.str-el cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | $Ni Cl_2$-$4SC(NH_2)_2$ (known as DTN) is a spin-1 material with a strong
single-ion anisotropy that is regarded as a new candidate for Bose-Einstein
condensation (BEC) of spin degrees of freedom. We present a systematic study of
the low-energy excitation spectrum of DTN in the field-induced magnetically
ordered phase by means of high-field electron spin resonance measurements at
temperatures down to 0.45 K. We argue that two gapped modes observed in the
experiment can be consistently interpreted within a four-sublattice
antiferromagnet model with a finite interaction between two tetragonal
subsystems and unbroken axial symmetry. The latter is crucial for the
interpretation of the field-induced ordering in DTN in terms of BEC.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:41:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zvyagin",
"S. A.",
""
],
[
"Wosnitza",
"J.",
""
],
[
"Kolezhuk",
"A. K.",
""
],
[
"Zapf",
"V. S.",
""
],
[
"Jaime",
"M.",
""
],
[
"Paduan-Filho",
"A.",
""
],
[
"Glazkov",
"V. N.",
""
],
[
"Sosin",
"S. S.",
""
],
[
"Smirnov",
"A. I.",
""
]
] | [
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] |
802.0353 | Tsuyoshi Yamamoto | T. Yamamoto, M. Watanabe, J. Q. You, Yu. A. Pashkin, O. Astafiev, Y.
Nakamura, F. Nori, and J. S. Tsai | Spectroscopy of superconducting charge qubits coupled by a Josephson
inductance | Accepted for publication in PRB. 11 pages, 7 figures | Phys. Rev. B 77, 064505 (2008) | 10.1103/PhysRevB.77.064505 | null | cond-mat.mes-hall cond-mat.supr-con | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have designed and experimentally implemented a circuit of
inductively-coupled superconducting charge qubits, where a Josephson junction
is used as an inductance, and the coupling between the qubits is controlled by
an applied magnetic flux. Spectroscopic measurements on the circuit are in good
agreement with theoretical calculations. We observed anticrossings which
originate from the coupling between the qubit and the plasma mode of the
Josephson junction. Moreover, the size of the anticrossing depends on the
external magnetic flux, which demonstrates the controllability of the coupling.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:42:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Yamamoto",
"T.",
""
],
[
"Watanabe",
"M.",
""
],
[
"You",
"J. Q.",
""
],
[
"Pashkin",
"Yu. A.",
""
],
[
"Astafiev",
"O.",
""
],
[
"Nakamura",
"Y.",
""
],
[
"Nori",
"F.",
""
],
[
"Tsai",
"J. S.",
""
]
] | [
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802.0354 | M. B. Paranjape | Garnik Alexanian, R. MacKenzie, M. B. Paranjape, Jonathan Ruel | Path integration and perturbation theory with complex Euclidean actions | 11 pages, no figures, version to be published in PRD | Phys.Rev.D77:105014,2008 | 10.1103/PhysRevD.77.105014 | UdeM-GPP-TH-08-165 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Euclidean path integral quite often involves an action that is not
completely real {\it i.e.} a complex action. This occurs when the Minkowski
action contains $t$-odd CP-violating terms. Analytic continuation to Euclidean
time yields an imaginary term in the Euclidean action. In the presence of
imaginary terms in the Euclidean action, the usual method of perturbative
quantization can fail. Here the action is expanded about its critical points,
the quadratic part serving to define the Gaussian free theory and the higher
order terms defining the perturbative interactions. For a complex action, the
critical points are generically obtained at complex field configurations. Hence
the contour of path integration does not pass through the critical points and
the perturbative paradigm cannot be directly implemented. The contour of path
integration has to be deformed to pass through the complex critical point using
a generalized method of steepest descent, in order to do so. Typically, what is
done is that only the real part of the Euclidean action is considered, and its
critical points are used to define the perturbation theory. In this article we
present a simple 0+1-dimensional example, of $N$ scalar fields interacting with
a U(1) gauge field, in the presence of a Chern-Simons term, where
alternatively, the path integral can be done exactly, the procedure of
deformation of the contour of path integration can be done explicitly and the
standard method of only taking into account the real part of the action can be
followed. We show explicitly that the standard method does not give a correct
perturbative expansion.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:47:20 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Apr 2008 04:44:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Alexanian",
"Garnik",
""
],
[
"MacKenzie",
"R.",
""
],
[
"Paranjape",
"M. B.",
""
],
[
"Ruel",
"Jonathan",
""
]
] | [
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802.0355 | Seoktae Koh | Seoktae Koh | Trans-Planckian Physics and Non-Commutative Inflation | 11pages, 1 figure, To appear in the Proceedings of the CospA 2007,
Taiwan | Mod.Phys.Lett.A23:1598-1605,2008 | 10.1142/S0217732308027990 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Non-commutativity of spacetime at the Planck scale may deform the usual
dispersion relations. And these deformed dispersion relations could lead to the
accelerating phase without a scalar field. In this paper, we have calculated
the spectral index and the running of spectral index in a non-commutative
inflation model. Non-commutative inflation with thermal radiation gives a scale
invariant spectrum in the limit $w \to -1$ and negative running spectral index
which are consistent with the WMAP 3-year results.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 08:50:48 GMT"
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] | 2008-11-26T00:00:00 | [
[
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"Seoktae",
""
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] |
802.0356 | Hu Chen | Hu Chen, Jie Yan | Effects of kink and flexible hinge defects on mechanical responses of
short double stranded DNA molecules | 9 pages with 9 figures. Theoretical calculation based on transfer
matrix. Minor updates, a new figure and more discussions are added | PHYSICAL REVIEW E 77, 041907 (2008) | 10.1103/PhysRevE.77.041907 | null | q-bio.BM q-bio.QM | null | We predict various detectable mechanical responses to the presence of local
DNA defects which are defined as short DNA segments exhibiting mechanical
properties obviously different from the 50 nm persistence length based
semiflexible polymer model. The defects discussed are kinks and flexible hinges
either permanently fixed on DNA or thermally excited. Their effects on
extension shift, the effective persistence length, the end-to-end distance
distribution, and the cyclization probability are computed using a
transfer-matrix method. Our predictions will be useful in future experimental
designs to study DNA nicks or mismatch base pairs, mechanics of specific DNA
sequences, and specific DNA-protein interaction using magnetic tweezer,
fluorescence resonance energy transfer or plasmon resonance technique, and the
traditional biochemistry cyclization probability measurements.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:09:18 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Mar 2008 10:46:14 GMT"
}
] | 2009-05-04T00:00:00 | [
[
"Chen",
"Hu",
""
],
[
"Yan",
"Jie",
""
]
] | [
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802.0357 | Mohamed Boucetta | Mohamed Boucetta-Alberto Medina | Polynomial Poisson structures on affine solvmanifolds | 17 pages | null | null | null | math.SG math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A $n$-dimensional Lie group $G$ equipped with a left invariant symplectic
form $\om^+$ is called a symplectic Lie group. It is well-known that $\om^+$
induces a left invariant affine structure on $G$. Relatively to this affine
structure we show that the left invariant Poisson tensor $\pi^+$ corresponding
to $\om^+$ is polynomial of degree 1 and any right invariant $k$-multivector
field on $G$ is polynomial of degree at most $k$. If $G$ is unimodular, the
symplectic form $\om^+$ is also polynomial and the volume form
$\wedge^{\frac{n}2}\om^+$ is parallel. We show also that any left invariant
tensor field on a nilpotent symplectic Lie group is polynomial, in particular,
any left invariant Poisson structure on a nilpotent symplectic Lie group is
polynomial. Because many symplectic Lie groups admit uniform lattices, we get a
large class of polynomial Poisson structures on compact affine solvmanifolds.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:00:45 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Medina",
"Mohamed Boucetta-Alberto",
""
]
] | [
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0.0334701873,
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] |
802.0358 | Qing-Yu Cai | Yong-gang Tan and Qing-yu Cai | Classical Correlation in Quantum Dialogue | Here we point out the erroneous use of classical communication
results in the insecurity of quantum dialogue protocols. Int. J. Quant. Inf.
(In press) | Int. J. Quant. Inf. 6, 325-329 (2008) | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Classical communications are used in the post-processing procedure of quantum
key distribution. Since the security of quantum key distribution is based on
the principles of quantum mechanics, intuitively the secret key can only be
derived from the quantum states. We find that classical communications are
incorrectly used in the so-called quantum dialogue type protocols. In these
protocols, public communications are used to transmit secret messages. Our
calculations show that half of Alice's and Bob's secret message is leaked
through classical channel. By applying Holevo bound, we can see that the
quantum efficiency claimed in the quantum dialogue type of protocols is not
achievable.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:10:42 GMT"
}
] | 2008-05-05T00:00:00 | [
[
"Tan",
"Yong-gang",
""
],
[
"Cai",
"Qing-yu",
""
]
] | [
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802.0359 | Yng-Ing Lee | Yng-Ing Lee and Mu-Tao Wang | Hamiltonian stationary cones and self-similar solutions in higher
dimension | 18 pages | null | null | null | math.DG math.AP | null | In [LW], we construct examples of two-dimensional Hamiltonian stationary
self-shrinkers and self-expanders for Lagrangian mean curvature flows, which
are asymptotic to the union of two Schoen-Wolfson cones. These self-shrinkers
and self-expanders can be glued together to yield solutions of the Brakke flow
- a weak formulation of the mean curvature flow. Moreover, there is no mass
loss along the Brakke flow. In this paper, we generalize these results to
higher dimension. We construct new higher dimensional Hamiltonian stationary
cones of different topology as generalizations of the Schoen-Wolfson cones.
Hamiltonian stationary self-shrinkers and self-expanders that are asymptotic to
these Hamiltonian stationary cones are also constructed. They can also be glued
together to produce eternal solutions of the Brakke flow without mass loss.
Finally, we show the same conclusion holds for those Lagrangian self-similar
examples recently found by Joyce, Tsui and the first author in [JLT].
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:40:16 GMT"
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] | 2008-02-05T00:00:00 | [
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802.036 | Anne Decourchelle | Anne Decourchelle (SAp/AIM, CEA Saclay) | Supernova remnants, planetary nebulae and superbubbles: prospects for
new XMM-Newton observations | 4 pages, 1 figure, invited review for "XMM-Newton: The next decade",
AN in press | Astron.Nachr.329:178-181,2008 | 10.1002/asna.200710907 | null | astro-ph | null | Important results achieved over the last years on supernova remnants,
planetary nebulae and superbubbles are briefly reviewed in the context of X-ray
observations. I intend to review the important open scientific questions in
these fields, and the specific contributions that can be made by XMM-Newton.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:53:46 GMT"
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] | 2009-06-23T00:00:00 | [
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802.0361 | Anton Deitmar | Anton Deitmar, Nikolaos Diamantis | Automorphic forms of higher order | LaTeX, 24 pages | Journal of the London Mathematical Society. 80, 18-34 (2009) | 10.1112/jlms/jdp015 | null | math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper a theory of Hecke operators for higher order modular forms is
established. The definition of cusp forms and attached L-functions is extended
beyond the realm of parabolic invariants. The role of representation theoretic
methods is clarified and, motivated by higher order forms, new convolution
products of L-functions are introduced.
| [
{
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{
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"created": "Sun, 12 Oct 2008 09:35:49 GMT"
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{
"version": "v4",
"created": "Fri, 1 Sep 2017 08:29:44 GMT"
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] |
802.0362 | Jan-Joris van Es | J. J. P. van Es, S. Whitlock, T. Fernholz, A. H. van Amerongen, N. J.
van Druten | Three-dimensional character of atom-chip-based rf-dressed potentials | 9 pages, 7 figures | Phys. Rev. A 77, 063623 (2008) | 10.1103/PhysRevA.77.063623 | null | cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We experimentally investigate the properties of radio-frequency-dressed
potentials for Bose-Einstein condensates on atom chips. The three-dimensional
potential forms a connected pair of parallel waveguides. We show that
rf-dressed potentials are robust against the effect of small magnetic-field
variations on the trap potential. Long-lived dipole oscillations of condensates
induced in the rf-dressed potentials can be tuned to a remarkably low damping
rate. We study a beam-splitter for Bose-Einstein condensates and show that a
propagating condensate can be dynamically split in two vertically separated
parts and guided along two paths. The effect of gravity on the potential can be
tuned and compensated for using a rf-field gradient.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:42:28 GMT"
}
] | 2010-10-08T00:00:00 | [
[
"van Es",
"J. J. P.",
""
],
[
"Whitlock",
"S.",
""
],
[
"Fernholz",
"T.",
""
],
[
"van Amerongen",
"A. H.",
""
],
[
"van Druten",
"N. J.",
""
]
] | [
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] |
802.0363 | Stefan Schramm | A. Mishra, S. Schramm, W. Greiner | Kaons and antikaons in asymmetric nuclear matter | null | Phys.Rev.C78:024901,2008 | 10.1103/PhysRevC.78.024901 | null | nucl-th hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The properties of kaons and antikaons and their modification in isospin
asymmetric nuclear matter are investigated using a chiral SU(3) model. These
isospin dependent medium effects are important for asymmetric heavy ion
collision experiments. In the present work, the medium modifications of the
energies of the kaons and antikaons, within the asymmetric nuclear matter,
arise due to the interactions of kaons and antikaons with the nucleons and
scalar mesons. The values of the parameters in the model are obtained by
fitting the saturation properties of nuclear matter and kaon-nucleon scattering
lengths. The pion-nucleon scattering lengths are also calculated within the
chiral effective model and compared with earlier results from the literature.
The density dependence of the isospin asymmetry is seen to be appreciable for
the kaon and antikaon optical potentials. This can be particularly relevant for
the future accelerator facility FAIR at GSI, where experiments using neutron
rich beams are planned to be used in the study of compressed baryonic matter.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:45:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mishra",
"A.",
""
],
[
"Schramm",
"S.",
""
],
[
"Greiner",
"W.",
""
]
] | [
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] |
802.0364 | Christian Kramberger | C. Kramberger, R. Hambach, C. Giorgetti, M. H. Rummeli, M. Knupfer, J.
Fink, B. Buchner, L. Reining, E. Einarsson, S. Maruyama, F. Sottile, K.
Hannewald, V. Olevano, A.G. Marinopoulos, T. Pichler | Linear plasmon dispersion in single-wall carbon nanotubes and the
collective excitation spectrum of graphene | null | Phys. Rev. Lett. 100, 196803 (2008) | 10.1103/PhysRevLett.100.196803 | null | cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have measured a strictly linear pi-plasmon dispersion along the axis of
individualized single wall carbon nanotubes, which is completely different from
plasmon dispersions of graphite or bundled single wall carbon nanotubes.
Comparative ab initio studies on graphene based systems allow us to reproduce
the different dispersions. This suggests that individualized nanotubes provide
viable experimental access to collective electronic excitations of graphene,
and it validates the use of graphene to understand electronic excitations of
carbon nanotubes. In particular, the calculations reveal that local field
effects (LFE) cause a mixing of electronic transitions, including the 'Dirac
cone', resulting in the observed linear dispersion.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:50:33 GMT"
}
] | 2010-09-08T00:00:00 | [
[
"Kramberger",
"C.",
""
],
[
"Hambach",
"R.",
""
],
[
"Giorgetti",
"C.",
""
],
[
"Rummeli",
"M. H.",
""
],
[
"Knupfer",
"M.",
""
],
[
"Fink",
"J.",
""
],
[
"Buchner",
"B.",
""
],
[
"Reining",
"L.",
""
],
[
"Einarsson",
"E.",
""
],
[
"Maruyama",
"S.",
""
],
[
"Sottile",
"F.",
""
],
[
"Hannewald",
"K.",
""
],
[
"Olevano",
"V.",
""
],
[
"Marinopoulos",
"A. G.",
""
],
[
"Pichler",
"T.",
""
]
] | [
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] |
802.0365 | Marco Koschorreck | M. Koschorreck and M. W. Mitchell | Non-ideal atom-light interfaces: modeling real-world effects | null | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a model which describes coherent and incoherent processes in
continuous-variable atom-light interfaces. We assume Gaussian states for light
and atoms and formulate the system dynamics in terms of first and second
moments of the angular momentum operators. Spatial and temporal inhomogeneities
in light and atom variables are incorporated by partitioning the system into
small homogeneous segments. Furthermore, other experimental imperfections as
for instance limited detector time-resolution and atomic motion are simulated.
The model is capable of describing many experimental situations ranging from
room temperature vapor cells to sub-mK atomic clouds. To illustrate the method,
we calculate the effect of detector time-resolution, spatial inhomogeneities
and atomic motion on the spin squeezing dynamics of rubidium 87 on the D2
transition.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 09:56:34 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 15:07:10 GMT"
}
] | 2008-02-22T00:00:00 | [
[
"Koschorreck",
"M.",
""
],
[
"Mitchell",
"M. W.",
""
]
] | [
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] |
802.0366 | Ming-Hao Liu | Ming-Hao Liu, Son-Hsien Chen, Ching-Ray Chang | Current-induced spin polarization in spin-orbit-coupled two-dimensional
electron systems | 7 pages, 6 figures, 1 table, Phys. Rev. B, in press | Phys. Rev. B 78, 165316 (2008) | 10.1103/PhysRevB.78.165316 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Current-induced spin polarization (CISP) is rederived in ballistic
spin-orbit-coupled electron systems, based on equilibrium statistical
mechanics. A simple and useful picture is correspondingly proposed to help
understand the CISP and predict the polarization direction. Nonequilibrium
Landauer-Keldysh formalism is applied to demonstrate the validity of the
statistical picture, taking the linear Rashba-Dresselhaus [001] two-dimensional
system as a specific example. Spin densities induced by the CISP in
semiconductor heterostructures and in metallic surface states are compared,
showing that the CISP increases with the spin splitting strength and hence
suggesting that the CISP should be more observable on metal and semimetal
surfaces due to the discovered strong Rashba splitting. An application of the
CISP designed to generate a spin-Hall pattern in the inplane, instead of the
out-of-plane, component is also proposed.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:02:41 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 08:43:42 GMT"
},
{
"version": "v3",
"created": "Sun, 19 Oct 2008 07:30:37 GMT"
}
] | 2008-10-24T00:00:00 | [
[
"Liu",
"Ming-Hao",
""
],
[
"Chen",
"Son-Hsien",
""
],
[
"Chang",
"Ching-Ray",
""
]
] | [
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0.0406390727,
0.0196732413,
0.0043204869,
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] |
802.0367 | Faruk Gungor | P. Basarab-Horwath, F. Gungor, V. Lahno | Symmetry classification of third-order nonlinear evolution equations | The authors withdraw this article due to substantial revisions to the
content | null | null | null | nlin.SI | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a Lie-algebraic classification of third order quasilinear equations
which admit non-trivial Lie point symmetries.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:05:10 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Oct 2010 13:16:24 GMT"
},
{
"version": "v3",
"created": "Wed, 6 Oct 2010 10:56:26 GMT"
}
] | 2010-10-07T00:00:00 | [
[
"Basarab-Horwath",
"P.",
""
],
[
"Gungor",
"F.",
""
],
[
"Lahno",
"V.",
""
]
] | [
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802.0368 | Surajit Sen | Mihir Ranjan Nath, Surajit Sen, Asoke Kumar Sen and Gautam
Gangopadhyay | Dynamical symmetry breaking of lambda and vee-type three-level systems
on quantization of the field modes | 27 pages, 9 Figures | Pramana - Journal of Physics, Vol. 71, (2008) 77-97 | null | null | quant-ph | http://creativecommons.org/licenses/publicdomain/ | We develop a scheme to construct the Hamiltonians of the lambda, vee and
cascade type of three-level configurations using the generators of SU(3) group.
It turns out that this approach provides a well defined selection rule to give
different Hamitonians for each configurations. The lambda and vee type
configurations are exactly solved with different initial conditions while
taking the two-mode classical and quantized fields . For the classical field,
it is shown that the Rabi oscillation of the lambda model is similar to that of
the vee model and the dynamics of the vee model can be recovered from lambda
model and vice versa simply by inversion. We then proceed to solve the
quantized version of both models introducing a novel Euler matrix formalism. It
is shown that this dynamical symmetry exhibited in the Rabi oscillation of two
configurations for the semiclassical models is completely destroyed on
quantization of the field modes. The symmetry can be restored within the
quantized models when the field modes are both in the coherent states with
large average photon number which is depicted through the collapse and revival
of the Rabi oscillations.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:06:16 GMT"
}
] | 2008-09-12T00:00:00 | [
[
"Nath",
"Mihir Ranjan",
""
],
[
"Sen",
"Surajit",
""
],
[
"Sen",
"Asoke Kumar",
""
],
[
"Gangopadhyay",
"Gautam",
""
]
] | [
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802.0369 | Alice Garbagnati | Alice Garbagnati | Symplectic Automorphisms on Kummer Surfaces | 13 pages | null | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Nikulin proved that the isometries induced on the second cohomology group of
a K3 surface $X$ by a finite abelian group $G$ of symplectic automorphisms are
essentially unique. Moreover he computed the discriminant of the sublattice of
$H^2(X, \Z)$ which is fixed by the isometries induced by $G$. However for
certain groups these discriminants are not the same of those found for explicit
examples. Here we describe Kummer surfaces for which this phenomena happens and
we explain the difference.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:18:25 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Garbagnati",
"Alice",
""
]
] | [
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] |
802.037 | Timo Anguita | T. Anguita (1), C. Faure (1), A. Yonehara (1,2), J. Wambsganss (1),
J.-P. Kneib (3), G. Covone (4) and D. Alloin (5) ((1) ARI/Zentrum fuer
Astronomie, University of Heidelberg, (2) JSPS Fellowships for Research
Abroad, (3) Laboratoire d'Astrophysique de Marseille, (4) INAF, Naples, (5)
AIM, CEA/DSM-CNRS-Universite Paris 7) | Integral field spectroscopy of four lensed quasars: analysis of their
neighborhood and evidence for microlensing | 13 pages, 18 figures. Accepted for publication in A&A: January 7,
2008 | null | 10.1051/0004-6361:20077306 | null | astro-ph | null | CONTEXT: Gravitationally lensed quasars constitute an independent tool to
derive H0 through time-delays; they offer as well the opportunity to study the
mass distribution and interstellar medium of their lensing galaxies and,
through microlensing they also allow one to study details of the emitting
source. AIMS: For such studies, one needs to have an excellent knowledge of the
close environment of the lensed images in order to model the lensing potential:
this means observational data over a large field-of-view and spectroscopy at
high spatial resolution. METHODS: We present VIMOS integral field observations
around four lensed quasars: HE 0230-2130, RX J0911.4+0551, H 1413+117 and B
1359+154. Using the low, medium and high resolution modes, we study the quasar
images and the quasar environments, as well as provide a detailed report of the
data reduction. RESULTS: Comparison between the quasar spectra of the different
images reveals differences for HE 0230-2130, RX J0911.4+0551 and H 1413+117:
flux ratios between the images of the same quasar are different when measured
in the emission lines and in the continuum. We have also measured the redshifts
of galaxies in the neighborhood of HE 0230-2130 and RX J0911.4+0551 which
possibly contribute to the total lensing potential. CONCLUSIONS: A careful
analysis reveals that microlensing is the most natural explanation for the
(de)magnification of the continuum emitting region of the background sources.
In HE 0230-2130, image D is likely to be affected by microlensing
magnification; in RX J0911.4+0551, images A1 and A3 are likely to be modified
by microlensing de-magnification and in H 1413+117, at least image D is
affected by microlensing.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:31:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Anguita",
"T.",
""
],
[
"Faure",
"C.",
""
],
[
"Yonehara",
"A.",
""
],
[
"Wambsganss",
"J.",
""
],
[
"Kneib",
"J. -P.",
""
],
[
"Covone",
"G.",
""
],
[
"Alloin",
"D.",
""
]
] | [
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] |
802.0371 | Frithjof Anders | Frithjof B. Anders | On steady-state currents through nano-devices: a scattering-states
numerical renormalization group approach to open quantum systems | 4 pages, 6 figures | Phys. Rev. Lett. 101, 066804 (2008) | 10.1103/PhysRevLett.101.066804 | null | cond-mat.mes-hall cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We propose a numerical renormalization group (NRG) approach to steady-state
currents through nano-devices. A discretization of the scattering-states
continuum ensures the correct boundary condition for an open quantum system. We
introduce two degenerate Wilson chains for current carrying left and
right-moving electrons reflecting time-reversal symmetry in the absence of a
finite bias $V$. We employ the time-dependent NRG to evolve the known
steady-state density operator for a non-interacting junction into the density
operator of the fully interacting nano-device at finite bias. We calculate the
temperature dependent current as function of $V$ and applied external magnetic
field using a recently developed algorithm for non-equilibrium spectral
functions.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:22:18 GMT"
},
{
"version": "v2",
"created": "Thu, 15 Jan 2009 12:57:33 GMT"
}
] | 2009-01-15T00:00:00 | [
[
"Anders",
"Frithjof B.",
""
]
] | [
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] |
802.0372 | Anne Decourchelle | Anne Decourchelle (SAp/AIM, CEA Saclay) | Non-thermal acceleration mechanisms in supernova remnant shells | 6 pages, 3 figures, invited talk at 'Simbol-X: the hard X-ray
universe in focus', Bologna (Italy), 14-16 May, 2007. To appear in Memorie
della SAIt | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A review of the main issues in the field of particle acceleration in
Supernova Remnants is provided in the context of future X-ray observations with
Simbol-X. After a summary of the nonthermal acceleration mechanisms at work, I
briefly review the observations of supernova remnants in hard X-rays and in
gamma rays. Open issues are discussed in this framework.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:44:39 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Decourchelle",
"Anne",
"",
"SAp/AIM, CEA Saclay"
]
] | [
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] |
802.0373 | Guangyan Jia | Guangyan Jia and Shige Peng | Jensen's Inequality for g-Convex Function under g-Expectation | 21 pages | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A real valued function defined on}$\mathbb{R}$ {\small is called}$g${\small
--convex if it satisfies the following \textquotedblleft generalized Jensen's
inequality\textquotedblright under a given}$g${\small -expectation, i.e.,
}$h(\mathbb{E}^{g}[X])\leq \mathbb{E}% ^{g}[h(X)]${\small, for all random
variables}$X$ {\small such that both sides of the inequality are meaningful. In
this paper we will give a necessary and sufficient conditions for a
}$C^{2}${\small -function being}$% g ${\small -convex. We also studied some
more general situations. We also studied}$g${\small -concave and}$g${\small
-affine functions.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:58:27 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Jia",
"Guangyan",
""
],
[
"Peng",
"Shige",
""
]
] | [
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] |
802.0374 | Itskovsky Matvey A. | M. A. Itskovsky, H. Cohen and T. Maniv | Far-field interaction of focused relativistic electron beams in electron
energy loss spectroscopy of nanoscopic platelets | 11 pages, 6 figures | null | 10.1103/PhysRevB.78.045419 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A quantum mechanical scattering theory for relativistic, highly focused
electron beams near nanoscopic platelets is presented, revealing a new
excitation mechanism due to the electron wave scattering from the platelet
edges. Radiative electromagnetic excitations within the light cone are shown to
arise, allowed by the breakdown of momentum conservation along the beam axis in
the inelastic scattering process. Calculated for metallic (silver and gold) and
insulating (SiO2 and MgO) nanoplatelets, new radiative features are revealed
above the main surface plasmon-polariton peak, and dramatic enhancements in the
electron energy loss probability at gaps of the 'classical' spectra, are found.
The corresponding radiation should be detectable in the vacuum far-field zone,
with e-beams exploited as sensitive 'tip-detectors' of electronically excited
nanostructures.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:58:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Itskovsky",
"M. A.",
""
],
[
"Cohen",
"H.",
""
],
[
"Maniv",
"T.",
""
]
] | [
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] |
802.0375 | Mladen Mitic Mr | M. Mitic, K. D. Petersson, M. C. Cassidy, R. P. Starrett, E. Gauja, A.
J. Ferguson, C. Yang, D. N. Jamieson, R. G. Clark and A. S. Dzurak | Bias spectroscopy and simultaneous SET charge state detection of Si:P
double dots | 7 pages, 6 figures | null | 10.1088/0957-4484/19/26/265201 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report a detailed study of low-temperature (mK) transport properties of a
silicon double-dot system fabricated by phosphorous ion implantation. The
device under study consists of two phosphorous nanoscale islands doped to above
the metal-insulator transition, separated from each other and the source and
drain reservoirs by nominally undoped (intrinsic) silicon tunnel barriers.
Metallic control gates, together with an Al-AlOx single-electron transistor,
were positioned on the substrate surface, capacitively coupled to the buried
dots. The individual double-dot charge states were probed using source-drain
bias spectroscopy combined with non-invasive SET charge sensing. The system was
measured in linear (VSD = 0) and non-linear (VSD <> 0) regimes allowing
calculations of the relevant capacitances. Simultaneous detection using both
SET sensing and source-drain current measurements was demonstrated, providing a
valuable combination for the analysis of the system. Evolution of the triple
points with applied bias was observed using both charge and current sensing.
Coulomb diamonds, showing the interplay between the Coulomb charging effects of
the two dots, were measured using simultaneous detection and compared with
numerical simulations.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 10:59:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mitic",
"M.",
""
],
[
"Petersson",
"K. D.",
""
],
[
"Cassidy",
"M. C.",
""
],
[
"Starrett",
"R. P.",
""
],
[
"Gauja",
"E.",
""
],
[
"Ferguson",
"A. J.",
""
],
[
"Yang",
"C.",
""
],
[
"Jamieson",
"D. N.",
""
],
[
"Clark",
"R. G.",
""
],
[
"Dzurak",
"A. S.",
""
]
] | [
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] |
802.0376 | Tomaso Belloni | Tomaso M. Belloni (INAF - Osservatorio Astronomico di Brera) | Noise components from black-hole binaries in our galaxy | Proc. SPIE Conference Fluctuations and Noise, Florence May 2-24, 2007
- 14 pages, 10 figures | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Accreting binaries containing a black hole are stellar systems composed of a
normal star and a black hole. Because of the strong gravitational pull of the
black hole, matter is removed from the companion star and falls into the
compact ob ject. In falling, it forms an accretion disk of gas that spirals
towards the center, heating up and emitting in X rays. The physics of such a
structure is extremely complex and can be studied through observations with
X-ray satellites. The time series derived from X-ray observations of bright
black-hole binaries in the Galaxy show a complex phenomenology. Broad noise
components with a variability of up to 40% are observed, as well as
quasi-periodic features on time scales from 100 seconds down to a few
milliseconds. The characteristic frequencies of the different components can
change on very short time scales. However, some of these signals are elusive as
they are very weak and are drowned in intrinsic and instrumental noise. The
physical nature of these signals is still largely unknown, but it is clear that
they originate from gas orbiting a few kilometers from the central black hole
and accreting onto it. In addition of being important for the study of the
accretion of matter onto a black hole, these observational properties
constitute a unique probe for testing General Relativity in the strong field
regime. I review the current observational status as well as the techniques
used to study these signals.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 13:47:27 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Belloni",
"Tomaso M.",
"",
"INAF - Osservatorio Astronomico di Brera"
]
] | [
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802.0377 | Maria Colonna | J.Rizzo, Ph.Chomaz, M.Colonna | A new approach to solve the Boltzmann-Langevin equation for fermionic
systems | submitted to Nucl. Phys. A | Nucl.Phys.A806:40-64,2008 | 10.1016/j.nuclphysa.2008.02.304 | null | nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a new method to introduce phase-space fluctuations in transport
theories, corresponding to a full implementation of the Boltzmann-Langevin
equation for fermionic systems. It is based on the procedure originally
developed by Bauer et al. for transport codes employing the test particle
method. In the new procedure, the Pauli principle is carefully checked, leading
to a good reproduction of the correct fluctuations in the ``continuum limit''
($h \to 0$). Accurate tests are carried out in one and two dimensional
idealized systems, and finally results for a full 3D application are shown. We
stress the reliability of this method, which can be easily plugged into
existing tranport codes using test particles, and its general applicability to
systems characterized by instabilities, like for instance multifragmentation
processes.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:01:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Rizzo",
"J.",
""
],
[
"Chomaz",
"Ph.",
""
],
[
"Colonna",
"M.",
""
]
] | [
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] |
802.0378 | Jos\'e Miguel Urbano | Jos\'e Francisco Rodrigues, Manel Sanch\'on and Jos\'e Miguel Urbano | The obstacle problem for nonlinear elliptic equations with variable
growth and L^1-data | null | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The aim of this paper is twofold: to prove, for L^1-data, the existence and
uniqueness of an entropy solution to the obstacle problem for nonlinear
elliptic equations with variable growth, and to show some convergence and
stability properties of the corresponding coincidence set. The latter follow
from extending the Lewy--Stampacchia inequalities to the general framework of
L^1.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:08:06 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Rodrigues",
"José Francisco",
""
],
[
"Sanchón",
"Manel",
""
],
[
"Urbano",
"José Miguel",
""
]
] | [
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] |
802.0379 | Julien Vidal | S. Dusuel, K. P. Schmidt, J. Vidal | Creation and Manipulation of Anyons in the Kitaev Model | 4 pages, 3 figures, published version | Phys. Rev. Lett. 100, 177204 (2008) | 10.1103/PhysRevLett.100.177204 | null | cond-mat.other quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We analyze the effect of local spin operators in the Kitaev model on the
honeycomb lattice. We show, in perturbation around the isolated-dimer limit,
that they create Abelian anyons together with fermionic excitations which are
likely to play a role in experiments. We derive the explicit form of the
operators creating and moving Abelian anyons without creating fermions and show
that it involves multi-spin operations. Finally, the important experimental
constraints stemming from our results are discussed.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:09:15 GMT"
},
{
"version": "v2",
"created": "Tue, 6 May 2008 08:54:18 GMT"
}
] | 2008-05-06T00:00:00 | [
[
"Dusuel",
"S.",
""
],
[
"Schmidt",
"K. P.",
""
],
[
"Vidal",
"J.",
""
]
] | [
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802.038 | Ute Ebert | T.M.P. Briels, E.M. van Veldhuizen, Ute Ebert | Positive streamers in ambient air and a N2:O2-mixture (99.8 : 0.2) | 2 pages, 4 figures, paper is accepted for IEEE Trans. Plasma Sci. and
scheduled to appear in June 2008 | IEEE Transactions on Plasma Science 36, 906 (2008) | 10.1109/TPS.2008.924510 | null | physics.plasm-ph physics.geo-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Photographs show distinct differences between positive streamers in air or in
a nitrogen-oxygen mixture (0.2% O2). The streamers in the mixture branch more
frequently, but the branches also extinguish more easily. Probably related to
that, the streamers in the mixture propagate more in a zigzag manner while they
are straighter in air. Furthermore, streamers in the mixture can become longer;
they are thinner and more intense.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:17:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Briels",
"T. M. P.",
""
],
[
"van Veldhuizen",
"E. M.",
""
],
[
"Ebert",
"Ute",
""
]
] | [
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802.0381 | Tamas Biro S | T.S.Biro, K.Urmossy and G.G.Barnafoldi | Pion and Kaon Spectra from Distributed Mass Quark Matter | Talk given at SQM 2007 | J.Phys.G35:044012,2008 | 10.1088/0954-3899/35/4/044012 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | After discussing some hints for possible masses of quasiparticles in quark
matter on the basis of lattice equation of state, we present pion and kaon
transverse spectra obtained by recombining quarks with distributed mass and
thermal cut power-law momenta as well as fragmenting by NLO pQCD with intrinsic
$k_T$ {and nuclear} broadening.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:20:14 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Biro",
"T. S.",
""
],
[
"Urmossy",
"K.",
""
],
[
"Barnafoldi",
"G. G.",
""
]
] | [
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802.0382 | Alcides Buss | Alcides Buss | A generalized Fourier inversion theorem | 15 pages; some typos corrected | Bulletin Braz. Math. Soc. 39(4), 2008, 555-571 | 10.1007/s00574-008-0004-6 | null | math.FA math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this work we define operator-valued Fourier transforms for suitable
integrable elements with respect to the Plancherel weight of a (not necessarily
Abelian) locally compact group. Our main result is a generalized version of the
Fourier inversion Theorem for strictly-unconditionally integrable Fourier
transforms. Our results generalize and improve those previously obtained by Ruy
Exel in the case of Abelian groups.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:22:10 GMT"
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{
"version": "v2",
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] | 2009-03-26T00:00:00 | [
[
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802.0383 | Dmitry Talalaev | D. Talalaev | Bethe ansatz and Isomonodromic deformations | 14 pages, extended version of the talk given at CQIS-2008, the
hypothesis proved | null | 10.1007/s11232-009-0051-1 | ITEP-TH-03/08 | math-ph math.MP nlin.SI | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study symmetries of the Bethe equations for the Gaudin model appeared
naturally in the framework of the geometric Langlands correspondence under the
name of Hecke operators and under the name of Schlesinger transformations in
the theory of isomonodromic deformations, and particularly in the theory of
Painlev\'e transcendents.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 13:26:02 GMT"
},
{
"version": "v2",
"created": "Sat, 22 Nov 2008 08:53:36 GMT"
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] | 2015-05-13T00:00:00 | [
[
"Talalaev",
"D.",
""
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802.0384 | Constantinos Simserides Dr. | Constantinos Simserides | Purely orbital diamagnetic to paramagnetic fluctuation of quasi
two-dimensional carriers under in-plane magnetic field | 4 pages, 6 figures | EXTENDED VERSION in J. Phys.: Condens. Matter 21 (2009) 015304
(6pp) | 10.1088/0953-8984/21/1/015304 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | An external magnetic field, $H$, applied parallel to a quasi two-dimensional
system modifies quantitatively and qualitatively the density of states. Using a
self-consistent numerical approach, we study how this affects the entropy, $S$,
the free energy, $F$, and the magnetization, $M$, for different sheet carrier
concentrations, $N_s$. As a prototype system we employ III-V double quantum
wells. We find that although $M$ is mainly in the opposite direction of $H$,
the system is not linear. Surprisingly $\partial M / \partial H$ swings between
negative and positive values, i.e., we predict an entirely orbital diamagnetic
to paramagnetic fluctuation. This phenomenon is important compared to the ideal
de Haas-van Alphen effect i.e. the corresponding phenomenon under perpendicular
magnetic field.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:28:25 GMT"
}
] | 2008-12-05T00:00:00 | [
[
"Simserides",
"Constantinos",
""
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] |
802.0385 | Saak Gabriyelyan S. | S.S. Gabriyelyan | Absolute continuity and singularity of two probability measures on a
filtered space | 18 pages, no figures | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $\mu$ and $\nu$ be fixed probability measures on a filtered space
$(\Omega, {\cal F}, ({\cal F}_t)_{t\in {\bf R}^{+}})$. Denote by $\mu_T $ and
$\nu_T $ (respectively, $\mu_{T-} $ and $\nu_{T-} $) the restrictions of the
measures $\mu$ and $\nu$ on ${\cal F}_T $ (respectively, on ${\cal F}_{T-} $)
for a stopping time $T$. We find the Hahn decomposition of $\mu_T $ and $\nu_T
$ using the Hahn decomposition of the measures $\mu$, $\nu$, and the Hellinger
process $h_t$ in the strict sense of order 1/2. The norm of the absolutely
continuous component of $\mu_{T-} $ with respect to $\nu_{T-} $ is computed in
terms of density processes and Hellinger integrals.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:29:44 GMT"
},
{
"version": "v2",
"created": "Sun, 16 Mar 2008 11:40:53 GMT"
},
{
"version": "v3",
"created": "Tue, 5 Apr 2011 19:13:18 GMT"
},
{
"version": "v4",
"created": "Wed, 6 Apr 2011 08:44:04 GMT"
}
] | 2011-04-07T00:00:00 | [
[
"Gabriyelyan",
"S. S.",
""
]
] | [
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] |
802.0386 | Schmiedmayer Joerg | S. Aigner, L. Della Pietra, Y. Japha, O. Entin-Wohlman, T. David, R.
Salem, R. Folman, J. Schmiedmayer | Long-Range Order in Electronic Transport through Disordered Metal Films | null | Science 319, 1226 - 1229, (2008) | 10.1126/science.1152458 | null | cond-mat.mtrl-sci cond-mat.other quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Ultracold atom magnetic field microscopy enables the probing of current flow
patterns in planar structures with unprecedented sensitivity. In
polycrystalline metal (gold) films we observe long-range correlations forming
organized patterns oriented at +/- 45 deg relative to the mean current flow,
even at room temperature and at length scales orders of magnitude larger than
the diffusion length or the grain size. The preference to form patterns at
these angles is a direct consequence of universal scattering properties at
defects. The observed amplitude of the current direction fluctuations scales
inversely to that expected from the relative thickness variations, the grain
size and the defect concentration, all determined independently by standard
methods. This indicates that ultracold atom magnetometry enables new insight
into the interplay between disorder and transport.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:32:54 GMT"
}
] | 2008-03-08T00:00:00 | [
[
"Aigner",
"S.",
""
],
[
"Della Pietra",
"L.",
""
],
[
"Japha",
"Y.",
""
],
[
"Entin-Wohlman",
"O.",
""
],
[
"David",
"T.",
""
],
[
"Salem",
"R.",
""
],
[
"Folman",
"R.",
""
],
[
"Schmiedmayer",
"J.",
""
]
] | [
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0.0952752233,
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] |
802.0387 | Jos\'e Gaite | Jose Gaite | Geometry and scaling of cosmic voids | 18 pages, A&A format, 11 EPS figure files | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | CONTEXT: Cosmic voids are observed in the distribution of galaxies and, to
some extent, in the dark matter distribution. If these distributions have
fractal geometry, it must be reflected in the geometry of voids; in particular,
we expect scaling sizes of voids. However, this scaling is not well
demonstrated in galaxy surveys yet. AIMS: Our objective is to understand the
geometry of cosmic voids in relation to a fractal structure of matter. We
intend to distinguish monofractal voids from multifractal voids, regarding
their scaling properties. We plan to analyse voids in the distributions of mass
concentrations (halos) in a multifractal and their relation to galaxy voids.
METHODS: We make a statistical analysis of point distributions based on the
void probability function and correlation functions. We assume that voids are
spherical and devise a simple spherical void finder. For continuous mass
distributions, we employ the methods of fractal geometry. We confirm the
analytical predictions with numerical simulations. Smoothed mass distributions
are suitable for the method of excursion sets. RESULTS: Voids are very
nonlinear and non-perturbative structures. Voids reflect the fractal geometry
of the matter distribution but not always directly: scaling sizes of voids
imply fractal geometry, but fractal voids may have a complicated geometry and
may not have scaling sizes. Proper multifractal voids are of this type. A
natural multifractal biasing model implies that the voids in the galaxy
distribution inherit the same complicated geometry. CONCLUSIONS: Current galaxy
surveys as well as cosmological N-body simulations indicate that cosmic voids
are proper multifractal voids. This implies the presence in the voids of
galaxies or, at least, small dark matter halos.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:34:22 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Gaite",
"Jose",
""
]
] | [
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] |
802.0388 | I. A. B. Strachan | Ian A. B. Strachan | Weyl groups and Elliptic Solutions of the WDVV equations | Typographical errors corrected. One result weakened (though with
changing the main result). Main theorem rewritten | Advances in Mathematics Volume 224, Issue 5, 1 August 2010, Pages
1801-1838 | 10.1016/j.aim.2010.01.013 | null | math-ph math.DG math.MP nlin.SI | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A functional ansatz is developed which gives certain elliptic solutions of
the Witten-Dijkgraaf-Verlinde-Verlinde (or WDVV) equation. This is based on the
elliptic trilogarithm function introduced by Beilinson and Levin. For this to
be a solution results in a number of purely algebraic conditions on the set of
vectors that appear in the ansatz, this providing an elliptic version of the
idea, introduced by Veselov, of a V-system.
Rational and trigonometric limits are studied together with examples of
elliptic V-systems based on various Weyl groups. Jacobi group orbit spaces are
studied: these carry the structure of a Frobenius manifold. The corresponding
almost dual structure is shown, in the A_N and B_N and conjecturally for an
arbitrary Weyl group, to correspond to the elliptic solutions of the WDVV
equations.
Transformation properties, under the Jacobi group, of the elliptic
trilogarithm are derived together with various functional identities which
generalize the classical Frobenius-Stickelburger relations.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:39:16 GMT"
},
{
"version": "v2",
"created": "Wed, 4 Nov 2009 11:07:40 GMT"
}
] | 2020-12-15T00:00:00 | [
[
"Strachan",
"Ian A. B.",
""
]
] | [
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802.0389 | Oleg Derzhko | Taras Verkholyak, Oleg Derzhko, Taras Krokhmalskii, and Joachim Stolze | Dynamic properties of quantum spin chains: Simple route to complex
behavior | null | Phys. Rev. B 76, 144418 (2007) (11 pages) | 10.1103/PhysRevB.76.144418 | null | cond-mat.str-el cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We examine dynamic structure factors of spin-1/2 chains with nearest-neighbor
interactions of XX and Dzyaloshinskii-Moriya type, and with periodic and random
changes in the sign of these interactions. This special kind of inhomogeneity
can be eliminated from the Hamiltonian by suitable transformation of the spin
variables. As a result, the dynamic structure factors of periodic or random
chains can be computed from those of the uniform chains. Using the exact
analytical and precise numerical results available for the uniform systems we
illustrate the effects of regular alternation or random disorder on dynamic
structure factors of quantum spin chains.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:42:31 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Verkholyak",
"Taras",
""
],
[
"Derzhko",
"Oleg",
""
],
[
"Krokhmalskii",
"Taras",
""
],
[
"Stolze",
"Joachim",
""
]
] | [
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] |
802.039 | P. B. Jones | P. B. Jones | Constraints on fall-back disks in radio pulsars and anomalous X-ray
pulsars | To be published in Monthly Notices of the Royal Astronomical Society | null | 10.1111/j.1365-2966.2008.13057.x | null | astro-ph | null | Calculations have been made of fall-back disk heating by the pulsar wind as
distinct from the soft X-rays emitted by the neutron-star surface. The relation
between these heating rates and measured near-infrared fluxes in the K and Ks
bands places severe constraints on the inner radii of any fall-back disks that
may be present in radio pulsars and in some anomalous X-ray pulsars. The lower
limits found are so large that the disks concerned can have no significant
effect on pulsar spin-down.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 11:58:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jones",
"P. B.",
""
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] |
802.0391 | Simon Vaughan | S. Vaughan (1), P. Uttley (2) ((1) University of Leicester, (2)
University of Southampton) | Studying accreting black holes and neutron stars with time series:
beyond the power spectrum | 13 pages, 6 figures, in "Noise and Fluctuations" Proc. SPIE vol. 6603 | null | null | null | astro-ph | null | The fluctuating brightness of cosmic X-ray sources, particularly accreting
black holes and neutron star systems, has enabled enormous progress in
understanding the physics of turbulent accretion flows, the behaviour of matter
on the surfaces of neutron stars and improving the evidence for black holes.
Most of this progress has been made by analysing and modelling time series data
in terms of their power and cross spectra, as will be discussed in other
articles in this volume. Recently, attempts have been made to make use of other
aspects of the data, by testing for non-linearity, non-Gaussianity, time
asymmetry and by examination of higher order Fourier spectra. These projects,
which have been made possible by the vast increase in data quality and quantity
over the past decade, are the subject of this article.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:14:24 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Vaughan",
"S.",
""
],
[
"Uttley",
"P.",
""
]
] | [
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] |
802.0392 | Emilio Santos Corchero | E. S. Corchero | Gravitational vacuum polarization as an alternative to dark matter | 9 pages, no figures | null | null | null | gr-qc astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | It is assumed that the quantum vacuum may be studied as consisting of two
contributions, with positive and negative energy respectively, which interact
but slightly and may be displaced from each other. Then it is proposed that
dark matter may be just an increase of the quantum vacuum energy, with respect
to the normal dark energy level, induced by the gravitational field of galaxies
or clusters. A simple model is worked out able to reproduce astronomical
observations.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 16:51:12 GMT"
}
] | 2008-02-08T00:00:00 | [
[
"Corchero",
"E. S.",
""
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] |
802.0393 | Alexander Dietz | Alexander Dietz (for the LIGO Scientific Collaboration) | GRB-triggered searches for gravitational waves in LIGO data | 5 pages, 3 figures, contributed talk, submitted to the proceedings of
Gamma Ray Bursts 2007, Santa Fe, New Mexico, November 5-9 2007 | AIP Conf.Proc.1000:284-288,2008 | 10.1063/1.2943464 | null | gr-qc astro-ph | null | The LIGO gravitational wave detectors have recently reached their design
sensitivity and finished a two-year science run. During this period one year of
data with unprecedented sensitivity has been collected. I will briefly describe
the status of the LIGO detectors and the overall quality of the most recent
science run. I also will present results of a search for inspiral waveforms in
gravitational wave data coincident with the short gamma ray burst detected on
1st February 2007, with its sky location error box overlapping a spiral arms of
M31. No gravitational wave signals were detected and a binary merger in M31 can
be excluded at the 99% confidence level.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:21:14 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Dietz",
"Alexander",
"",
"for the LIGO Scientific Collaboration"
]
] | [
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802.0394 | Stefan Weigert | Stefan Weigert and Michael Wilkinson | Mutually Unbiased Bases for Continuous Variables | 5 pages, no figures, revised to be identical to published text | Phys. Rev. A 78, 020303(R) (2008) | 10.1103/PhysRevA.78.020303 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The concept of mutually unbiased bases is studied for N pairs of continuous
variables. To find mutually unbiased bases reduces, for specific states related
to the Heisenberg-Weyl group, to a problem of symplectic geometry. Given a
single pair of continuous variables, three mutually unbiased bases are
identified while five such bases are exhibited for two pairs of continuous
variables. For N = 2, the golden ratio occurs in the definition of these
mutually unbiased bases suggesting the relevance of number theory not only in
the finite-dimensional setting.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:20:18 GMT"
},
{
"version": "v2",
"created": "Sun, 9 Nov 2008 14:58:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Weigert",
"Stefan",
""
],
[
"Wilkinson",
"Michael",
""
]
] | [
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] |
802.0395 | Enqvist Kari | K. Enqvist, S. Nurmi, D. Podolsky, G.I. Rigopoulos (University of
Helsinki and Helsinki Institute of Physics) | On the divergences of inflationary superhorizon perturbations | 12 pages | JCAP 0804:025,2008 | 10.1088/1475-7516/2008/04/025 | HIP-2008-05/TH | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss the infrared divergences that appear to plague cosmological
perturbation theory. We show that within the stochastic framework they are
regulated by eternal inflation so that the theory predicts finite fluctuations.
Using the $\Delta N$ formalism to one loop, we demonstrate that the infrared
modes can be absorbed into additive constants and the coefficients of the
diagrammatic expansion for the connected parts of two and three-point functions
of the curvature perturbation. As a result, the use of any infrared cutoff
below the scale of eternal inflation is permitted, provided that the background
fields are appropriately redefined. The natural choice for the infrared cutoff
would of course be the present horizon; other choices manifest themselves in
the running of the correlators. We also demonstrate that it is possible to
define observables that are renormalization group invariant. As an example, we
derive a non-perturbative, infrared finite and renormalization point
independent relation between the two-point correlators of the curvature
perturbation for the case of the free single field.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:29:31 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Enqvist",
"K.",
"",
"University of\n Helsinki and Helsinki Institute of Physics"
],
[
"Nurmi",
"S.",
"",
"University of\n Helsinki and Helsinki Institute of Physics"
],
[
"Podolsky",
"D.",
"",
"University of\n Helsinki and Helsinki Institute of Physics"
],
[
"Rigopoulos",
"G. I.",
"",
"University of\n Helsinki and Helsinki Institute of Physics"
]
] | [
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802.0396 | Tapan Mishra | Meetu Sethi Luthra, Tapan Mishra, Ramesh V. Pai, B. P. Das | Phase diagram of a bosonic ladder with two coupled chains | 6 pages, 10 figures | null | null | null | cond-mat.stat-mech cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study a bosonic ladder with two coupled chains using the finite size
density matrix renormalisation group method. We show that in a commensurate
bosonic ladder the critical on-site interaction ($U_C$) for the superfluid to
Mott insulator transition becomes larger as the inter-chain hopping
($t_\bot$)increases. We analyze this quantum phase transition and obtain the
phase diagram in the $t_\bot -U$ plane.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:38:58 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Luthra",
"Meetu Sethi",
""
],
[
"Mishra",
"Tapan",
""
],
[
"Pai",
"Ramesh V.",
""
],
[
"Das",
"B. P.",
""
]
] | [
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] |
802.0397 | Janusz Morawiec | Janusz Morawiec | On bounded solutions of a problem of R. Schilling | 6 pages | Ann. Math. Sil. 8 (1994), 97-101 | null | null | math.CA | null | The paper deals with locally bounded solutions of a Schilling's problem.
| [
{
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"created": "Mon, 4 Feb 2008 12:43:37 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Feb 2008 08:17:25 GMT"
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] | 2008-02-05T00:00:00 | [
[
"Morawiec",
"Janusz",
""
]
] | [
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802.0398 | Ian Huston | Ian Huston, James E. Lidsey, Steven Thomas, John Ward | Gravitational Wave Constraints on Multi-Brane Inflation | 18 pages, uses iopart.sty; v2: added references, version as published
in JCAP | JCAP0805:016,2008 | 10.1088/1475-7516/2008/05/016 | null | hep-th astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A class of non-canonical inflationary models is identified, where the
leading-order contribution to the non-Gaussianity of the curvature perturbation
is determined by the sound speed of the fluctuations in the inflaton field.
Included in this class of models is the effective action for multiple
coincident branes in the finite n limit. The action for this configuration is
determined using a powerful iterative technique, based upon the fundamental
representation of SU(2). In principle the upper bounds on the tensor-scalar
ratio that arise in the standard, single-brane DBI inflationary scenario can be
relaxed in such multi-brane configurations if a large and detectable
non-Gaussianity is generated. Moreover models with a small number of coincident
branes could generate a gravitational wave background that will be observable
to future experiments.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:46:04 GMT"
},
{
"version": "v2",
"created": "Mon, 19 May 2008 12:04:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Huston",
"Ian",
""
],
[
"Lidsey",
"James E.",
""
],
[
"Thomas",
"Steven",
""
],
[
"Ward",
"John",
""
]
] | [
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] |
802.0399 | S. V. Troitsky | Sergey Troitsky | Spectral energy distributions and high-energy emission of BL Lac type
objects | v.2: selection effects quantified, discussion of Auger results on BL
Lac correlations extended. 5 pages, 4 figures, mn2e.cls style. The definitive
version is available at http://www.blackwellsynergy.com | Mon. Not. Roy. Astron. Soc. Lett., 388 (2008) L79 | 10.1111/j.1745-3933.2008.00503.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Based on identifications from the Veron and Quasars.org catalogs, we
determine the optical-to-X-ray spectral indices for a sample of 201 BL Lac type
objects (BLLs) and search for trends in the distribution of these indices of
the sources detected in high-energy bands. We find that EGRET-detected sources
are low-energy peaked and that the positional correlation with the arrival
directions of ultra-high-energy cosmic rays from the previously studied AGASA,
Yakutsk and High Resolution Fly's Eye samples is dominated by low-energy-peaked
BLLs.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:49:42 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jul 2008 05:01:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Troitsky",
"Sergey",
""
]
] | [
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] |
802.04 | Paola Andreani | Robertio Vio (Chip Computers Consulting) and Paola Andreani (ESO,
INAF-OAT) | A Modified ICA Approach for Signal Separation in CMB Maps | 12 pages, 6 Encapsulated Postscript figures | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | AIMS: One of the most challenging and important problem of digital signal
processing in Cosmology is the separation of foreground contamination from
cosmic microwave background (CMB). This problem becomes even more difficult in
situations, as the CMB polarization observations, where the amount of available
"a priori" information is limited. In this case, it is necessary to resort to
the "blind separation" methods. One important member of this class is
represented by the "Independent Components Analysis" (ICA). In its original
formulation, this method has various interesting characteristics, but also some
limits. One of the most serious is the difficulty to take into account any
information available in advance. In particular, ICA is not able to exploit the
fact that emission of CMB is the same at all the frequencies of observations.
Here, we show how to deal with this question. The connection of the proposed
methodology with the "Internal Linear Composition" (ILC) technique is also
illustrated.
METHODS: A modification of the classic ICA approach is presented and its
characteristics are analyzed both analytically and by means of numerical
experiments.
RESULTS: The modified version of ICA appears to provide more stable results
and of better quality.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 12:54:03 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Vio",
"Robertio",
"",
"Chip Computers Consulting"
],
[
"Andreani",
"Paola",
"",
"ESO,\n INAF-OAT"
]
] | [
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] |
802.0401 | Khikmat Muminov | D. A. Abdushukurov, D.V.Bondarenko, Kh.Kh.Muminov, D.Yu.Chistyakov | Contribution of nano-scale effects to the total efficiency of converters
of thermal neutrons on the basis of gadolinium foils | 9 pages, 3 figures | null | null | null | physics.ins-det nucl-ex nucl-th | http://creativecommons.org/licenses/publicdomain/ | We study the influence of nano-scale layers of converters made from natural
gadolinium and its 157 isotope into the total efficiency of registration of
thermal neutrons. Our estimations show that contribution of low-energy Auger
electrons with the runs about nanometers in gadolinium, to the total efficiency
of neutron converters in this case is essential and results in growth of the
total efficiency of converters. The received results are in good consent to the
experimental data.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 16:45:01 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Abdushukurov",
"D. A.",
""
],
[
"Bondarenko",
"D. V.",
""
],
[
"Muminov",
"Kh. Kh.",
""
],
[
"Chistyakov",
"D. Yu.",
""
]
] | [
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] |
802.0402 | Monika Winklmeier | Monika Winklmeier, Osanobu Yamada | On the local energy decay of solutions of the Dirac equation in the
non-extreme Kerr-Newman metric, I | null | J. Phys. A: Math. Theor. 42 (2009) 295204 | null | null | math-ph math.MP | null | We investigate the local energy decay of solutions of the Dirac equation in
the non-extreme Kerr-Newman metric. First, we write the Dirac equation as a
Cauchy problem and define the Dirac operator. It is shown that the Dirac
operator is selfadjoint in a suitable Hilbert space. With the RAGE theorem, we
show that for each particle its energy located in any compact region outside of
the event horizon of the Kerr-Newman black hole decays in the time mean.
| [
{
"version": "v1",
"created": "Mon, 4 Feb 2008 13:36:15 GMT"
}
] | 2009-07-20T00:00:00 | [
[
"Winklmeier",
"Monika",
""
],
[
"Yamada",
"Osanobu",
""
]
] | [
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