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802.0603 | Julien Bringer | Julien Bringer and Herve Chabanne | Trusted-HB: a low-cost version of HB+ secure against Man-in-The-Middle
attacks | submitted to IEEE Transactions on Information Theory | IEEE Trans. IT. 54:9 (2008) 4339-4342 | 10.1109/TIT.2008.928290 | null | cs.CR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Since the introduction at Crypto'05 by Juels and Weis of the protocol HB+, a
lightweight protocol secure against active attacks but only in a detection
based-model, many works have tried to enhance its security. We propose here a
new approach to achieve resistance against Man-in-The-Middle attacks. Our
requirements - in terms of extra communications and hardware - are surprisingly
low.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 20:39:03 GMT"
}
] | 2009-01-08T00:00:00 | [
[
"Bringer",
"Julien",
""
],
[
"Chabanne",
"Herve",
""
]
] | [
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802.0604 | Amnon Aharony | A. B. Harris, Amnon Aharony and Ora Entin-Wohlman | Order Parameters and Phase Diagram of Multiferroic RMn$_2$O$_5$ | null | Phys. Rev. Lett. 100, 217202 (2008) | 10.1103/PhysRevLett.100.217202 | null | cond-mat.mtrl-sci cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The generic magnetic phase diagram of multiferroic RMn$_2$O$_5$ (with R=Y,
Ho, Tb, Er, Tm), which allows different sequences of ordered magnetic
structures for different R's and different control parameters, is described
using order parameters which explicitly incorporate the magnetic symmetry. A
phenomenological magneto-electric coupling is used to explain why some of these
magnetic phases are also ferroelectric. Several new experiments, which can test
this theory, are proposed.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 12:34:47 GMT"
},
{
"version": "v2",
"created": "Fri, 6 Jun 2008 06:54:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Harris",
"A. B.",
""
],
[
"Aharony",
"Amnon",
""
],
[
"Entin-Wohlman",
"Ora",
""
]
] | [
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802.0605 | Fleurov Victor | O.V. Farberovich, A. Yaresko, K. Kikoin and V. Fleurov | Electronic structure of noble metal impurities in semiconductors: Cu in
GaP | 6 figures | null | 10.1103/PhysRevB.78.085206 | null | cond-mat.other cond-mat.str-el | null | A numerical method for calculation of the electronic structure of transition
metal impurities in semiconductors based on the Green function technique is
developed. The electronic structure of 3d impurity is calculated within the
LDA+U version of density functional method, whereas the host electron Green
function is calculated by using the linearized augmented plane wave expansion.
The method is applied to the Cu impurity in GaP. The results of calculations
are compared with those obtained within the supercell LDA procedure. It is
shown that in the Green function approach Cu impurity has an unfilled 3d shell.
This result paves a way to explanation of the magnetic order in dilute
Ga_{1-x}Cu_xP alloys.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:28:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Farberovich",
"O. V.",
""
],
[
"Yaresko",
"A.",
""
],
[
"Kikoin",
"K.",
""
],
[
"Fleurov",
"V.",
""
]
] | [
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] |
802.0606 | Michael J. W. Hall | Michael J. W. Hall | Complete positivity for time-dependent qubit master equations | Additional example and ref; to appear in J. Phys. A | J. Phys. A: Math. Theor. 41 (2008) 205302 | 10.1088/1751-8121/41/26/269801 | null | quant-ph | null | It is shown that if the decoherence matrix corresponding to a qubit master
equation has a block-diagonal real part, then the evolution is determined by a
one-dimensional oscillator equation. Further, when the full decoherence matrix
is block-diagonal, then the necessary and sufficient conditions for completely
positive evolution may be formulated in terms of the oscillator Hamiltonian or
Lagrangian. When the solution of the oscillator equation is not known, an
explicit sufficient condition for complete positivity can still be obtained,
based on a Hamiltonian/Lagrangian inequality. A rotational form-invariance
property is used to characterise the evolution via a single first-order
nonlinear differential equation, enabling some further exact results to be
obtained. A class of master equations is identified for which complete
positivity reduces to the simpler condition of positivity.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 19:17:44 GMT"
},
{
"version": "v2",
"created": "Sat, 29 Mar 2008 02:40:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hall",
"Michael J. W.",
""
]
] | [
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] |
802.0607 | Enrico Calzavarini | Enrico Calzavarini, Massimo Cencini, Detlef Lohse, and Federico Toschi | Quantifying turbulence induced segregation of inertial particles | 4 pages, 5 figures | Phys. Rev. Lett. 101, 084504 (2008) | 10.1103/PhysRevLett.101.084504 | null | nlin.CD physics.flu-dyn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Particles with density different from that of the advecting turbulent fluid
cluster due to the different response of light/heavy particles to turbulent
fluctuations. This study focuses on the quantitative characterization of the
segregation of dilute poly-disperse inertial particles evolving in turbulent
flow, as obtained from Direct Numerical Simulation of the Navier-Stokes
equations. We introduce an indicator of segregation amongst particles of
different inertia and/or size, from which a length scale r_{seg} quantifying
the degree of segregation of two different types of particles is deduced.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:01:55 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Aug 2008 09:00:26 GMT"
}
] | 2008-08-28T00:00:00 | [
[
"Calzavarini",
"Enrico",
""
],
[
"Cencini",
"Massimo",
""
],
[
"Lohse",
"Detlef",
""
],
[
"Toschi",
"Federico",
""
]
] | [
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] |
802.0608 | Jerzy Blawzdziewicz | S. Bhattacharya (Texas Tech University), J. Blawzdziewicz (Yale
University) | Effect of small particles on the near-wall dynamics of a large particle
in a highly bidisperse colloidal solution | 11 pages, 5 figures | null | 10.1063/1.2917339 | null | cond-mat.soft | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider the hydrodynamic effect of small particles on the dynamics of a
much larger particle moving normal to a planar wall in a highly bidisperse
dilute colloidal suspension of spheres. The gap $h_0$ between the large
particle and the wall is assumed to be comparable to the diameter $2a$ of the
smaller particles so there is a length-scale separation between the gap width
$h_0$ and the radius of the large particle $b<<h_0$. We use this length-scale
separation to develop a new lubrication theory which takes into account the
presence of the smaller particles in the space between the larger particle and
the wall. The hydrodynamic effect of the small particles on the motion of the
large particle is characterized by the short time (or high frequency)
resistance coefficient. We find that for small particle-wall separations $h_0$,
the resistance coefficient tends to the asymptotic value corresponding to the
large particle moving in a clear suspending fluid. For $h_0<<a$, the resistance
coefficient approaches the lubrication value corresponding to a particle moving
in a fluid with the effective viscosity given by the Einstein formula.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:03:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bhattacharya",
"S.",
"",
"Texas Tech University"
],
[
"Blawzdziewicz",
"J.",
"",
"Yale\n University"
]
] | [
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] |
802.0609 | Henri Gouin | Sergey Gavrilyuk, Henri Gouin (MSNMGP, LMMT), Yurii Perepechko | A variational principle for two-fluid models | 7 pages | Comptes Rendus de l Acad\'emie des Sciences - Series IIB -
Mechanics-Physics-Astronomy 324, 8 (1997) 483-490 | 10.1016/S1251-8069(97)80186-8 | null | physics.class-ph math-ph math.MP | null | A variational principle for two-fluid mixtures is proposed. The Lagrangian is
constructed as the difference between the kinetic energy of the mixture and a
thermodynamic potential conjugated to the internal energy with respect to the
relative velocity of phases. The equations of motion and a set of
Rankine-Hugoniot conditions are obtained. It is proved also that the convexity
of the internal energy guarantees the hyperbolicity of the one-dimensional
equations of motion linearized at rest.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:12:43 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Gavrilyuk",
"Sergey",
"",
"MSNMGP, LMMT"
],
[
"Gouin",
"Henri",
"",
"MSNMGP, LMMT"
],
[
"Perepechko",
"Yurii",
""
]
] | [
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] |
802.061 | Lorenzo Morelli | L. Morelli (1), E. Pompei (2), A. Pizzella (1), J. M\'endez-Abreu
(1),(3), E. M. Corsini (1), L. Coccato (4), R. P. Saglia (4), M. Sarzi (5)
and F. Bertola (1) ((1) Dipartimento di Astronomia, Universit\`a di Padova,
(2) European Southern Observatory, (3) INAF-Osservatorio Astronomico di
Padova, (4) Max-Planck Institut f\"ur extraterrestrische Physik, (6) Centre
for Astrophysics Research, University of Hertfordshire) | The pseudobulge of NGC 1292 | 2 pages, 1 figure to appear in the proceedings of "Formation and
Evolution of Galaxy Disks", Rome, October 2007, Eds. J. Funes and E. M.
Corsini | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The photometric and kinematic properties of Sb NGC 1292 suggest it hosts a
pseudobulge. The properties of the stellar population of such a pseudobulge are
consistent with a slow buildup within a scenario of secular evolution.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:14:14 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Morelli",
"L.",
""
],
[
"Pompei",
"E.",
""
],
[
"Pizzella",
"A.",
""
],
[
"Méndez-Abreu",
"J.",
""
],
[
"Corsini",
"E. M.",
""
],
[
"Coccato",
"L.",
""
],
[
"Saglia",
"R. P.",
""
],
[
"Sarzi",
"M.",
""
],
[
"Bertola",
"F.",
""
]
] | [
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] |
802.0611 | Denis Burgarella | D. Burgarella, B. Le Roux, M. Langlois, G. Moretto, T. Fusco, M.
Ferrari | The Wide-field High-resolution Infrared TElescope (WHITE) | Invited talk to the 2nd ARENA Conference : "The Astrophysical Science
Cases at Dome C" Potsdam 17-21 September, 2007 | null | 10.1117/12.789077 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Wide-field High-resolution Infrared TElescope (WHITE) will be dedicated
in the first years of its life to carrying out a few (well focused in terms of
science objectives and time) legacy surveys.
WHITE would have an angular resolution of ~0.3'' homogeneous over ~0.7 sq.
deg. in the wavelength range 1 - 5 um, which means that we will very
efficiently use all the available observational time during night time and day
time. Moreover, the deepest observations will be performed by summing up
shorter individual frames. We will have a temporal information that can be used
to study variable objects.
The three key science objectives of WHITE are : 1) A complete survey of the
Magellanic Clouds to make a complete census of young stellar objects in the
clouds and in the bridge and to study their star formation history and the link
with the Milky Way. The interaction of the two clouds with our Galaxy might the
closest example of a minor merging event that could be the main driver of
galaxy evolution in the last 5 Gyrs. 2) The building of the first sample of
dusty supernovae at z<1.2 in the near infrared range (1-5 um) to constrain the
equation of state from these obscured objects, study the formation of dust in
galaxies and build the first high resolution sample of high redshift galaxies
observed in their optical frame 3) A very wide weak lensing survey over that
would allow to estimate the equation of state in a way that would favourably
compete with space projects.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:19:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Burgarella",
"D.",
""
],
[
"Roux",
"B. Le",
""
],
[
"Langlois",
"M.",
""
],
[
"Moretto",
"G.",
""
],
[
"Fusco",
"T.",
""
],
[
"Ferrari",
"M.",
""
]
] | [
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802.0612 | Boris Pasquier | Boris Pasquier | The pseudo-index of horospherical Fano varieties | 9 pages | null | null | null | math.AG | null | We prove a conjecture of L.Bonavero, C. Casagrande, O. Debarre and S. Druel,
on the pseudo-index of smooth Fano varieties, in the special case of
horospherical varieties.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:02:21 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Pasquier",
"Boris",
""
]
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] |
802.0613 | Alexandre Matzkin | A. Matzkin | Is Bell's theorem relevant to quantum mechanics? On locality and
non-commuting observables | Extended with new material | AIP Conf Proc 1101, 339 (2009) | 10.1063/1.3109959 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Bell's theorem is a statement by which averages obtained from specific types
of statistical distributions must conform to a family of inequalities. These
models, in accordance with the EPR argument, provide for the simultaneous
existence of quantum mechanically incompatible quantities. We first recall
several contradictions arising between the assumption of a joint distribution
for incompatible observables and the probability structure of
quantum-mechanics, and conclude that Bell's theorem is not expected to be
relevant to quantum phenomena described by non-commuting observables,
irrespective of the issue of locality. Then, we try to disentangle the locality
issue from the existence of joint distributions by introducing two models
accounting for the EPR correlations but denying the existence of joint
distributions. We will see that these models do not need to resort explicitly
to non-locality: the first model relies on conservation laws for ensembles, and
the second model on an equivalence class by which different configurations lead
to the same physical predictions.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:28:02 GMT"
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{
"version": "v2",
"created": "Thu, 6 Mar 2008 09:44:05 GMT"
},
{
"version": "v3",
"created": "Mon, 12 Jan 2009 15:12:50 GMT"
}
] | 2009-04-13T00:00:00 | [
[
"Matzkin",
"A.",
""
]
] | [
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802.0614 | Ivan Melo | M. Gintner, I. Melo, B. Trpisova | Signatures of Strong Electroweak Symmetry Breaking in pp -> b \bar{b} t
\bar{t} + X at LHC | 3 pages, 3 figures, submitted to the Proceedings of the 16th
Conference of the Slovak Physicists, Sep 10-13, 2007, Zilina, Slovakia. (The
reason for the replacement: In the original submission the year of the
Conference was mistyped.) | null | null | null | hep-ph | null | We study the possible production of the $\rho$-resonance from the Strong
Electroweak Symmetry Breaking sector at LHC. Due to possibly enhanced couplings
of $\rho$ to the top and bottom quarks we focus on the process pp -> b \bar{b}
t \bar{t} where either b \bar{b} or t \bar{t} are the products of the $\rho$
decay.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:14:22 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Feb 2008 11:03:38 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Gintner",
"M.",
""
],
[
"Melo",
"I.",
""
],
[
"Trpisova",
"B.",
""
]
] | [
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] |
802.0615 | Elvan Ceyhan | E. Ceyhan, C. E. Priebe, D. J. Marchette | A New Family of Random Graphs for Testing Spatial Segregation | 31 pages, 15 figures | Canadian Journal of Statistics (2007), 35(1):27-50 | null | null | stat.ME math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss a graph-based approach for testing spatial point patterns. This
approach falls under the category of data-random graphs, which have been
introduced and used for statistical pattern recognition in recent years. Our
goal is to test complete spatial randomness against segregation and association
between two or more classes of points. To attain this goal, we use a particular
type of parametrized random digraph called proximity catch digraph (PCD) which
is based based on relative positions of the data points from various classes.
The statistic we employ is the relative density of the PCD. When scaled
properly, the relative density of the PCD is a $U$-statistic. We derive the
asymptotic distribution of the relative density, using the standard central
limit theory of $U$-statistics. The finite sample performance of the test
statistic is evaluated by Monte Carlo simulations, and the asymptotic
performance is assessed via Pitman's asymptotic efficiency, thereby yielding
the optimal parameters for testing. Furthermore, the methodology discussed in
this article is also valid for data in multiple dimensions.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:34:46 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Ceyhan",
"E.",
""
],
[
"Priebe",
"C. E.",
""
],
[
"Marchette",
"D. J.",
""
]
] | [
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] |
802.0616 | Guangyan Jia | Guangyan Jia | A uniqueness theorem for solution of BSDEs | null | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this note, we prove that if $g$ is uniformly continuous in $z$, uniformly
with respect to $(\oo,t)$ and independent of $y$, the solution to the backward
stochastic differential equation (BSDE) with generator $g$ is unique.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:44:14 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Jia",
"Guangyan",
""
]
] | [
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] |
802.0617 | Elvan Ceyhan | E. Ceyhan, C. E. Priebe | On the Distribution of the Domination Number of a New Family of
Parametrized Random Digraphs | 24 pages, 14 figures | Model Assisted Statistics and Applications (2007), 1(4):231-255 | null | null | math.CO math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We derive the asymptotic distribution of the domination number of a new
family of random digraph called proximity catch digraph (PCD), which has
application to statistical testing of spatial point patterns and to pattern
recognition. The PCD we use is a parametrized digraph based on two sets of
points on the plane, where sample size and locations of the elements of one is
held fixed, while the sample size of the other whose elements are randomly
distributed over a region of interest goes to infinity. PCDs are constructed
based on the relative allocation of the random set of points with respect to
the Delaunay triangulation of the other set whose size and locations are fixed.
We introduce various auxiliary tools and concepts for the derivation of the
asymptotic distribution. We investigate these concepts in one Delaunay triangle
on the plane, and then extend them to the multiple triangle case. The methods
are illustrated for planar data, but are applicable in higher dimensions also.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:50:56 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Ceyhan",
"E.",
""
],
[
"Priebe",
"C. E.",
""
]
] | [
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] |
802.0618 | Massimiliano Rinaldi | Massimiliano Rinaldi | Superluminal dispersion relations and the Unruh effect | Final discussion expanded, references added. Version accepted for
publication in Phys Rev D | Phys.Rev.D77:124029,2008 | 10.1103/PhysRevD.77.124029 | null | gr-qc hep-th | null | In the context of quantum gravity phenomenology, we study the Unruh effect in
the presence of superluminal dispersion relations. In particular, we estimate
the response function and the probability rate for an accelerated detector
coupled to a massless scalar field, whose dispersion relation becomes
essentially quadratic beyond a threshold momentum $k_p$. By means of
perturbative analysis, we show that superluminal dispersion induces a
correction to the Planckian spectrum, which tends to vanish as $k_p$ increases.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:52:38 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 15:57:22 GMT"
},
{
"version": "v3",
"created": "Mon, 26 May 2008 16:11:42 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Rinaldi",
"Massimiliano",
""
]
] | [
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] |
802.0619 | Leonid Fel | Leonid G. Fel | On Summatory Totient Functions | 9 pages | null | null | null | math.NT | null | The lower and upper bounds are found for the leading term of summatory
totient function $\sum_{k\leq N}k^u\phi^v(k)$ in various ranges of
$u\in{\mathbb R}$ and $v\in{\mathbb Z}$.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 13:59:00 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Feb 2008 17:53:01 GMT"
}
] | 2008-02-11T00:00:00 | [
[
"Fel",
"Leonid G.",
""
]
] | [
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] |
802.062 | Mami Hamasaki | Mami Hamasaki | Formalism of Nonequilibrium Perturbation Theory and Kondo Effect | Extended version of cond-mat/0506752 | null | null | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The formalism of nonequilibrium perturbation theory was constructed by
Schwinger and Keldysh and then was developed with the diagrammatical technique
by Lifshitz and Pitaevskii. Until now there has been widespread application to
various researches in physics, condensed matter, plasmas, atoms and molecules,
nuclear matter etc.. In spite of this, the formalism has not been established
as perturbation theory. For example, there is no perturbative method to derive
arbitrary self-energy properly. In addition, the connection with other
formalism, e.g., the Matsubara imaginary-time perturbative formalism is
uncertain. Although there must be the relationship between self-energies in the
perturbative formalism, such basic problems remain to be solved. The solution
is given by the present work. The real-time perturbative expansion is performed
on the basis of the adiabatic theorem. As the results, the requirements of
self-energies as functions in time are demonstrated and the formulated
self-energies meet the known relations. Besides, it gives exact agreement with
functions derived by perturbative expansion in imaginary-time and analytical
continuity. As a consequence, it implies that the present formalism can be
generalized.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:09:27 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Hamasaki",
"Mami",
""
]
] | [
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802.0621 | Jana Ka\v{s}parov\'a | J. C. Brown, J. Kasparova, A. M. Massone, M. Piana | Fast Spectral Fitting of Hard X-Ray Bremsstrahlung from Truncated
Power-Law Electron Spectra | 7 pages, 4 figures, submitted to Astronomy and Astrophysics | Astron.Astrophys.486:1023-1029,2008 | 10.1051/0004-6361:200809496 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Hard X-Ray bremsstrahlung continuum spectra, such as from solar flares, are
commonly described in terms of power-law fits, either to the photon spectra
themselves or to the electron spectra responsible for them. In applications
various approximate relations between electron and photon spectral indices are
often used for energies both above and below electron low-energy cutoffs. We
examine the form of the exact relationships in various situations, and for
various cross-sections, showing that empirical relations sometimes used can be
highly misleading and consider how to improve fitting procedures. We obtain
expressions for photon spectra from single, double and truncated power-law
electron spectra for a variety of cross-sections and for the thin and thick
target models and simple analytic expressions for the Bethe-Heitler cases. We
show that above a low-energy cutoff the Kramers and Bethe-Heitler results match
reasonably well with results for exact cross-sections up to energies around 100
keV; that below the low-energy cutoff, Kramers and other constant spectral
index forms commonly used are very poor approximations to accurate results; but
that our analytical forms are a very good match. Analytical forms of the
Bethe-Heitler photon spectra from general power-law electron spectra are an
excellent match to exact results for both thin and thick targets and they
enable much faster spectral fitting than evaluation of the full spectral
integrations.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:17:12 GMT"
}
] | 2009-02-20T00:00:00 | [
[
"Brown",
"J. C.",
""
],
[
"Kasparova",
"J.",
""
],
[
"Massone",
"A. M.",
""
],
[
"Piana",
"M.",
""
]
] | [
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] |
802.0622 | Elvan Ceyhan | E. Ceyhan, C. E. Priebe, J. C.Wierman | Relative Density of the Random $r$-Factor Proximity Catch Digraph for
Testing Spatial Patterns of Segregation and Association | 29 pages, 21 figures | Computational Statistics & Data Analysis (2006), 50(8):1925-1964 | null | null | stat.ME math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Statistical pattern classification methods based on data-random graphs were
introduced recently. In this approach, a random directed graph is constructed
from the data using the relative positions of the data points from various
classes. Different random graphs result from different definitions of the
proximity region associated with each data point and different graph statistics
can be employed for data reduction. The approach used in this article is based
on a parameterized family of proximity maps determining an associated family of
data-random digraphs. The relative arc density of the digraph is used as the
summary statistic, providing an alternative to the domination number employed
previously. An important advantage of the relative arc density is that,
properly re-scaled, it is a $U$-statistic, facilitating analytic study of its
asymptotic distribution using standard $U$-statistic central limit theory. The
approach is illustrated with an application to the testing of spatial patterns
of segregation and association. Knowledge of the asymptotic distribution allows
evaluation of the Pitman and Hodges-Lehmann asymptotic efficacies, and
selection of the proximity map parameter to optimize efficiency. Furthermore
the approach presented here also has the advantage of validity for data in any
dimension.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:17:29 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Ceyhan",
"E.",
""
],
[
"Priebe",
"C. E.",
""
],
[
"Wierman",
"J. C.",
""
]
] | [
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] |
802.0623 | Daniel Wohns | Daniel Wohns | Hawking-Moss Tunneling with a Dirac-Born-Infeld Action | 4 pages, version accepted in Phys. Rev. D., additional references and
example application | Phys.Rev.D78:107702,2008 | 10.1103/PhysRevD.78.107702 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Hawking-Moss tunneling rate for a field described by the
Dirac-Born-Infeld action is calculated using a stochastic approach. We find
that the effect of the non-trivial kinetic term is to enhance the tunneling
rate, which can be exponentially significant. This result should be compared to
the DBI enhancement found in the Coleman-de Luccia case.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:20:02 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Nov 2008 21:40:52 GMT"
}
] | 2009-02-23T00:00:00 | [
[
"Wohns",
"Daniel",
""
]
] | [
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802.0624 | Andreas Fring | Andreas Fring and Miloslav Znojil | PT-symmetric deformations of Calogero models | 19 pages, 2 figures, version acepted for publication | J.Phys.A41:194010,2008 | 10.1088/1751-8113/41/19/194010 | CMS 01/08 | quant-ph hep-th math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We demonstrate that Coxeter groups allow for complex PT-symmetric
deformations across the boundaries of all Weyl chambers. We compute the
explicit deformations for the A_2 and G_2-Coxeter group and apply these
constructions to Calogero-Moser-Sutherland models invariant under the extended
Coxeter groups. The eigenspecta for the deformed models are real and contain
the spectra of the undeformed case as subsystem.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 20:18:17 GMT"
},
{
"version": "v2",
"created": "Fri, 9 May 2008 16:19:55 GMT"
}
] | 2009-10-02T00:00:00 | [
[
"Fring",
"Andreas",
""
],
[
"Znojil",
"Miloslav",
""
]
] | [
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802.0625 | Aleksey Zakharenko | Aleksey A. Zakharenko, S. Karthikyan, K.S. Kim | Ab Initio Study of Different Acid Molecules Interacting with H2O | 22 pages, 2 figs, 2 tables, 90 references | null | null | null | physics.chem-ph physics.atm-clus physics.bio-ph physics.comp-ph physics.med-ph physics.space-ph | http://creativecommons.org/licenses/publicdomain/ | Using the Gaussian-03 for ab initio calculations, we have studied interaction
of different acid molecules with a single water molecule. The molecular and
supermolecular optimized structures were found with the Becke-3-Lee-Yang-Parr
(B3LYP-hybrid potential) calculations of density-functional theory (DFT)
methods as well as the Moeller-Plesset second-order perturbation theory, using
the basis set of Aug-cc-pVDZ quality and the CRENBL ECP effective core
potential for molecules containing heavy iodine atom. Possible isomers of
studied acids and supermolecules, consisting of acid molecules coupled with a
single water molecule, are shown. Energies, zero-point energies (ZPEs), thermal
enthalpies and free energies, as well as the corresponding binding energies for
the theoretical methods were calculated. It was found that optimized structures
of supermolecular isomers with lowest energies corresponding to the global
minimum on the potential energy surfaces can be different for both theories.
The simplest structure acids H2S and H2Se, forming acid-water supermolecules,
can give clear evidence of disagreement of the two theoretical methods
concerning optimization of lowest energy structures, because the B3LYP-DFT
method gives the lowest-energy structure for the first supermolecular isomer,
but the MP2 method for the second possible isomer. A dramatic difference
between potential energy surfaces for both theories applying to the optimized
structure finding of the H2SO3-H2O supermolecular isomers was found, because
MP2 supermolecular geometries cannot exist for the corresponding B3LYP-DFT
ones, for which the frequency characteristics of the supermolecular isomers
were also calculated. In general, the binding energies and ZPE ones for the MP2
method are 10-15% larger than those for the B3LYP-DFT method.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 02:42:25 GMT"
}
] | 2016-09-08T00:00:00 | [
[
"Zakharenko",
"Aleksey A.",
""
],
[
"Karthikyan",
"S.",
""
],
[
"Kim",
"K. S.",
""
]
] | [
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] |
802.0626 | Stephen Spratlin Bullock | Stephen S. Bullock and Dianne P. O'Leary | Bounds on Effective Hamiltonians for Stabilizer Codes | 12 pages, two algorithms, one figure, to be submitted to QIC | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This manuscript introduces various notions of k-locality of stabilizer codes
inherited from the associated stabilizer groups. A choice of generators for the
group leads to a Hamiltonian with the code in its groundspace, while a
Hamiltonian holding the code in its groundspace might be called effective if
its locality is less than that of a natural choice of generators (or any
choice). This paper establishes some conditions under which effective
Hamiltonians for stabilizer codes do not exist. Our results simplify in the
cases of Calderbank-Shor-Steane stabilizer codes and topologically-ordered
stabilizer codes arising from surface cellulations.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:24:56 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Bullock",
"Stephen S.",
""
],
[
"O'Leary",
"Dianne P.",
""
]
] | [
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] |
802.0627 | Friedrich Konrad Roepke | F. K. Roepke (MPA Garching) | Numerical simulations of multi-scale astrophysical problems: The example
of Type Ia supernovae | 10 pages, 1 figure; in "Modelling and Simulation in Science",
Proceedings of the 6th International Workshop on Data Analysis in Astronomy
"Livio Scarsi", Erice, Italy 15 - 22 April 2007 (World Scientific, 2008) | null | null | null | astro-ph | null | Vastly different time and length scales are a common problem in numerical
simulations of astrophysical phenomena. Here, we present an approach to
numerical modeling of such objects on the example of Type Ia supernova
simulations. The evolution towards the explosion proceeds on much longer time
scales than the explosion process itself. The physical length scales relevant
in the explosion process cover 11 orders of magnitude and turbulent effects
dominate the physical mechanism. Despite these challenges, three-dimensional
simulations of Type Ia supernova explosions have recently become possible and
pave the way to a better understanding of these important astrophysical
objects.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:36:35 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Roepke",
"F. K.",
"",
"MPA Garching"
]
] | [
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] |
802.0628 | Andras I. Stipsicz | Paolo Lisca, Peter Ozsv\'ath, Andr\'as I. Stipsicz and Zolt\'an
Szab\'o | Heegaard Floer invariants of Legendrian knots in contact
three--manifolds | 70 pages, 30 figures | null | null | null | math.SG math.GT | http://creativecommons.org/licenses/publicdomain/ | We define invariants of null--homologous Legendrian and transverse knots in
contact 3--manifolds. The invariants are determined by elements of the knot
Floer homology of the underlying smooth knot. We compute these invariants, and
show that they do not vanish for certain non--loose knots in overtwisted
3--spheres. Moreover, we apply the invariants to find transversely non--simple
knot types in many overtwisted contact 3--manifolds.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:33:04 GMT"
},
{
"version": "v2",
"created": "Tue, 21 Apr 2009 11:12:44 GMT"
}
] | 2009-04-21T00:00:00 | [
[
"Lisca",
"Paolo",
""
],
[
"Ozsváth",
"Peter",
""
],
[
"Stipsicz",
"András I.",
""
],
[
"Szabó",
"Zoltán",
""
]
] | [
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] |
802.0629 | Christian Martin | C. A. Martin, D. Ding, H. S. J. van der Zant, J. M. van Ruitenbeek | Lithographic mechanical break junctions for single-molecule measurements
in vacuum: possibilities and limitations | 19 pages, 6 figures; v2: changed wrongly given HDA peak position in
abstract to correct value, removed typing mistakes; v3: added three plots,
improved discussion, removed typos | New J. Phys. 10 (2008) 065008 | 10.1088/1367-2630/10/6/065008 | null | cond-mat.mes-hall cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have investigated electrical transport through the molecular model systems
benzenedithiol, benzenediamine, hexanedithiol and hexanediamine. Conductance
histograms under different experimental conditions indicate that measurements
using mechanically controllable break junctions in vacuum are limited by the
surface density of molecules at the contact. Hexanedithiol histograms typically
exhibit a broad peak around 7 * 10^{-4} G_0. In contrast to recent results on
STM-based break junctions in solution we find that the spread in
single-molecule conductance is not reduced by amino anchoring groups.
Histograms of hexanediamine exhibit a very wide peak around 4 * 10^{-4} G_0.
For both benzenedithiol and benzenediamine we observe a large variability in
low-bias conductance. We attribute these features to the slow breaking of the
lithographic mechanically controllable break junctions and the absence of a
solvent that may enable molecular readsorption after bond breaking.
Nevertheless, we have been able to acquire reproducible current-voltage
characteristics of benzenediamine and benzenedithiol using a statistical
measurement approach. Benzenedithiol measurements yield a conductance gap of
about 0.9 V at room temperature and 0.6 V at 77 K. In contrast, the
current-voltage characteristics of benzenediamine-junctions typically display
conductance gaps of about 0.9 V at both temperatures.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:07:56 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Feb 2008 10:21:09 GMT"
},
{
"version": "v3",
"created": "Tue, 1 Jul 2008 12:19:24 GMT"
}
] | 2008-07-01T00:00:00 | [
[
"Martin",
"C. A.",
""
],
[
"Ding",
"D.",
""
],
[
"van der Zant",
"H. S. J.",
""
],
[
"van Ruitenbeek",
"J. M.",
""
]
] | [
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] |
802.063 | Stefan Maubach | Stefan Maubach | A problem on polynomial maps over finite fields | 6 pages; | null | null | null | math.CO math.AC math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This is a short note that explains a problem on polynomial maps over finite
fields for non-experts. The problem is: Do there exist odd polynomial
automorphisms over the finite fields with 4,8,16,32,64,... elements? The
explanation is very, very basic. Also, the background of the problem is given,
and why it is of such importance. This all with the idea that the problem
enters the world of discrete mathematics, and can be approached from completely
different angles than normally used by people working in Affine Algebraic
Geometry.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:42:31 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Maubach",
"Stefan",
""
]
] | [
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] |
802.0631 | Spalek | J. Spa{\l}ek, A. Koz{\l}owski, Z. Tarnawski, Z. K\c{a}kol, Y. Fukami,
F. Ono, R. Zach, L. J. Spalek | Verwey transition in Fe$_{3}$O$_{4}$ at high pressure: quantum critical
behavior at the onset of metallization | 5 pages, 5 figures | null | 10.1103/PhysRevB.78.100401 | null | cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We provide evidence for the existence of a {\em quantum critical point} at
the metallization of magnetite Fe$_{3}$O$_{4}$ at an applied pressure of $p_{c}
\approx 8$ GPa. We show that the present ac magnetic susceptibility data
support earlier resistivity data. The Verwey temperature scales with pressure
$T_{V}\sim (1-p/p_{c})^{\nu}$, with $\nu\sim 1/3$. The resistivity data shows a
temperature dependence $\rho(T)=\rho_{0}+AT^{n}$, with $n\simeq 3$ above and
2.5 at the critical pressure, respectively. This difference in $n$ with
pressure is a sign of critical behavior at $p_{c}$. The magnetic susceptibility
is smooth near the critical pressure, both at the Verwey transition and near
the ferroelectric anomaly. A comparison with the critical behavior observed in
the Mott-Hubbard and related systems is made.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:42:49 GMT"
}
] | 2016-08-17T00:00:00 | [
[
"Spałek",
"J.",
""
],
[
"Kozłowski",
"A.",
""
],
[
"Tarnawski",
"Z.",
""
],
[
"Kcakol",
"Z.",
""
],
[
"Fukami",
"Y.",
""
],
[
"Ono",
"F.",
""
],
[
"Zach",
"R.",
""
],
[
"Spalek",
"L. J.",
""
]
] | [
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802.0632 | Vasudevarao Allu | S. Ponnusamy (IIT Madras, India), A. Vasudevarao (IIT Madras, India)
and M. Vuorinen (University of Turku, Finland) | Region of variability for certain classes of univalent functions
satisfying differential inequalities | 24 pages, 5 figures | null | null | null | math.CV | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we determine the region of variability for certain subclasses
of univalent functions satisfying differential inequalities. In the final
section we graphically illustrate the region of variability for several sets of
parameters.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 14:49:52 GMT"
},
{
"version": "v2",
"created": "Fri, 5 Dec 2008 16:32:01 GMT"
},
{
"version": "v3",
"created": "Thu, 30 Jul 2009 17:30:54 GMT"
}
] | 2009-07-30T00:00:00 | [
[
"Ponnusamy",
"S.",
"",
"IIT Madras, India"
],
[
"Vasudevarao",
"A.",
"",
"IIT Madras, India"
],
[
"Vuorinen",
"M.",
"",
"University of Turku, Finland"
]
] | [
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] |
802.0633 | Pablo Groisman | Juli\'an Fern\'andez Bonder, Pablo Groisman | Time--space white noise eliminates global solutions in reaction
diffusion equations | New results included. To be published in Physica D | null | 10.1016/j.physd.2008.09.005 | null | math.AP math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that perturbing the reaction--diffusion equation $u_t=u_{xx} +
(u_+)^p$ ($p>1$), with time--space white noise produces that solutions explodes
with probability one for every initial datum, opposite to the deterministic
model where a positive stationary solution exists.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:25:42 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Nov 2008 16:46:22 GMT"
}
] | 2008-11-10T00:00:00 | [
[
"Bonder",
"Julián Fernández",
""
],
[
"Groisman",
"Pablo",
""
]
] | [
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802.0634 | Adel Bilal | Adel Bilal | Lectures on Anomalies | 108 pages, 10 figures | null | null | LPTENS-08/05 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | These lectures on anomalies are relatively self-contained and intended for
graduate students who are familiar with the basics of quantum field theory. We
begin with several derivations of the abelian anomaly: anomalous transformation
of the measure, explicit computation of the triangle Feynman diagram, relation
to the index of the Euclidean Dirac operator. The chiral (non-abelian) gauge
anomaly is derived by evaluating the anomalous triangle diagram with three
non-abelian gauge fields coupled to a chiral fermion. We discuss in detail the
relation between anomaly, current non-conservation and non-invariance of the
effective action, with special emphasis on the derivation of the anomalous
Slavnov-Taylor/Ward identities. We show why anomalies always are finite and
local. A general characterization is given of gauge groups and fermion
representations which may lead to anomalies in four dimensions, and the issue
of anomaly cancellation is discussed, in particular the classical example of
the standard model.
Then, we move to more formal developments and arbitrary even dimensions.
After introducing a few basic notions of differential geometry, in particular
characteristic classes, we derive the descent equations. We prove the
Wess-Zumino consistency condition and show that relevant anomalies correspond
to BRST cohomologies at ghost number one. We discuss why and how anomalies are
related to characteristic classes in two more dimensions and outline their
computation in terms of the index of an appropriate Dirac operator. Finally we
derive the gauge and gravitational anomalies in arbitrary even dimensions from
the appropriate index and explain the anomaly cancellations in ten-dimensional
IIB supergravity and in type I and heterotic superstrings.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:00:20 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Bilal",
"Adel",
""
]
] | [
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802.0635 | Filippo Viviani | Sergey Gorchinskiy and Filippo Viviani | A note on families of hyperelliptic curves | 8 pages; final version, to appear on Arch. Math | Arch. Math. 92 (2009), 119-128 | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a stack-theoretic proof for some results on families of hyperelliptic
curves.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:05:00 GMT"
},
{
"version": "v2",
"created": "Fri, 19 Sep 2008 20:41:26 GMT"
}
] | 2009-04-15T00:00:00 | [
[
"Gorchinskiy",
"Sergey",
""
],
[
"Viviani",
"Filippo",
""
]
] | [
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] |
802.0636 | Bernard Segard | Bruno Macke (PhLAM), Bernard S\'egard (PhLAM) | Slow light in saturable absorbers | null | Physical Review A: Atomic, Molecular and Optical Physics 78, 1
(2008) 013817 | 10.1103/PhysRevA.78.013817 | null | physics.optics | null | In connection with the experiments recently achieved on doped crystals,
biological samples, doped optical fibers and semiconductor heterostructures, we
revisit the theory of the propagation of a pulse-modulated light in a saturable
absorber. Explicit analytical expressions of the transmitted pulse are
obtained, enabling us to determine the parameters optimizing the time-delay of
the transmitted pulse with respect to the incident pulse. We finally compare
the maximum fractional delay or figure of merit so attainable to those which
have been actually demonstrated in the experiments.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:12:09 GMT"
},
{
"version": "v2",
"created": "Wed, 18 Jun 2008 13:18:02 GMT"
}
] | 2008-07-11T00:00:00 | [
[
"Macke",
"Bruno",
"",
"PhLAM"
],
[
"Ségard",
"Bernard",
"",
"PhLAM"
]
] | [
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] |
802.0637 | Plyatsko Roman | Roman Plyatsko | Highly Relativistic Motions of Spinning Particles According to Mathisson
Equations | 6 pages, invited paper presented at the Mathisson Conference (17-20
October2007, Warsaw), to appear in Acta Phys. Pol. B | Acta Phys.Polon.Supp.1:173-178,2008 | null | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The physical effects following from the Mathisson equations at the highly
relativistic motions of a spinning test particle relative to a Schwarzschild
mass are discussed. The corresponding numerical estimates are presented.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:21:55 GMT"
}
] | 2009-02-10T00:00:00 | [
[
"Plyatsko",
"Roman",
""
]
] | [
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] |
802.0638 | Elvan Ceyhan | E. Ceyhan, C. E. Priebe | The Use of Domination Number of a Random Proximity Catch Digraph for
Testing Spatial Patterns of Segregation and Association | 13 pages, 7 figures | Statistics & Probability Letters (2005), 73, 37-50 | null | null | stat.ME math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Priebe et al. (2001) introduced the class cover catch digraphs and computed
the distribution of the domination number of such digraphs for one dimensional
data. In higher dimensions these calculations are extremely difficult due to
the geometry of the proximity regions; and only upper-bounds are available. In
this article, we introduce a new type of data-random proximity map and the
associated (di)graph in $\mathbb R^d$. We find the asymptotic distribution of
the domination number and use it for testing spatial point patterns of
segregation and association.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:22:56 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Ceyhan",
"E.",
""
],
[
"Priebe",
"C. E.",
""
]
] | [
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802.0639 | Fatemeh Sadat Tabatabaei Asl | F. S. Tabatabaei, R. Beck, M. Krause, E. M. Berkhuijsen, R. Gehrz, K.
D. Gordon, J. L. Hinz, and G. H. Rieke | A Multi-Scale Study of IR and Radio Emission from M33 | 2 pages, 1 figure, to appear in the proceedings of "Formation and
Evolution of Galaxy Disks",eds: Jose G. Funes, S.J. & Enrico M. Corsini (ASP
conference series) | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The origin of the tight radio--IR correlation in galaxies has not been fully
understood. One reason is the uncertainty about which heating sources (stars or
diffuse interstellar radiation field)provide the energy that is absorbed by
dust and re-radiated in IR. Another problem is caused by comparing the IR
emission with the thermal and nonthermal components of the radio continuum
emission separated by simplistically assuming a constant nonthermal spectral
index. We use the data at the $Spitzer$ MIPS wavelengths of 24, 70, and 160
$\mu$m, as well as recent radio continuum map at 3.6 cm observed with the
100--m Effelsberg telescope. Using the wavelet transformation, we separate
diffuse emission components from compact sources and study the radio-IR
correlation at various scales. We also investigate the IR correlations with the
thermal and nonthermal radio emissions separated by our developed method. A
H$\alpha$ map serves as a tracer of star forming regions.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:28:16 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Tabatabaei",
"F. S.",
""
],
[
"Beck",
"R.",
""
],
[
"Krause",
"M.",
""
],
[
"Berkhuijsen",
"E. M.",
""
],
[
"Gehrz",
"R.",
""
],
[
"Gordon",
"K. D.",
""
],
[
"Hinz",
"J. L.",
""
],
[
"Rieke",
"G. H.",
""
]
] | [
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] |
802.064 | Rami Barends | R. Barends, J. J. A. Baselmans, S. J. C. Yates, J. R. Gao, J. N.
Hovenier, and T. M. Klapwijk | Quasiparticle relaxation in optically excited high-Q superconducting
resonators | 4 pages, 3 figures | Phys. Rev. Lett. 100, 257002 (2008) | 10.1103/PhysRevLett.100.257002 | null | cond-mat.supr-con cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The quasiparticle relaxation time in superconducting films has been measured
as a function of temperature using the response of the complex conductivity to
photon flux. For tantalum and aluminium, chosen for their difference in
electron-phonon coupling strength, we find that at high temperatures the
relaxation time increases with decreasing temperature, as expected for
electron-phonon interaction. At low temperatures we find in both
superconducting materials a saturation of the relaxation time, suggesting the
presence of a second relaxation channel not due to electron-phonon interaction.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:32:29 GMT"
},
{
"version": "v2",
"created": "Thu, 5 Jun 2008 17:10:07 GMT"
}
] | 2008-06-25T00:00:00 | [
[
"Barends",
"R.",
""
],
[
"Baselmans",
"J. J. A.",
""
],
[
"Yates",
"S. J. C.",
""
],
[
"Gao",
"J. R.",
""
],
[
"Hovenier",
"J. N.",
""
],
[
"Klapwijk",
"T. M.",
""
]
] | [
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] |
802.0641 | Nicholas J. Proudfoot | Tom Braden, Nicholas J. Proudfoot | The hypertoric intersection cohomology ring | Significant revisions in Section 5, with several corrected proofs | null | 10.1007/s00222-009-0181-y | null | math.AG math.AT math.SG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a functorial computation of the equivariant intersection
cohomology of a hypertoric variety, and endow it with a natural ring structure.
When the hyperplane arrangement associated with the hypertoric variety is
unimodular, we show that this ring structure is induced by a ring structure on
the equivariant intersection cohomology sheaf in the equivariant derived
category. The computation is given in terms of a localization functor which
takes equivariant sheaves on a sufficiently nice stratified space to sheaves on
a poset.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:36:18 GMT"
},
{
"version": "v2",
"created": "Sun, 10 Feb 2008 07:06:32 GMT"
},
{
"version": "v3",
"created": "Sat, 4 Oct 2008 18:29:32 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Braden",
"Tom",
""
],
[
"Proudfoot",
"Nicholas J.",
""
]
] | [
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] |
802.0642 | Fatemeh Sadat Tabatabaei Asl | F. S. Tabatabaei, R. Beck, E. Kr\"ugel, M. Krause, E. M. Berkhuijsen,
K. D. Gordon, K. M. Menten | Variations of the Radio Synchrotron Spectral Index in M33 | 2 pages, 1 figure, to appear in the Proceeding "Formation and
Evolution of Galaxy Disks", eds: Jose G. Funes, S.J. & Enrico M. Corsini (ASP
conference series) | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We determine the variation in the nonthermal radio spectral index in the
nearby spiral galaxy M33. We separate the thermal and nonthermal components of
the radio continuum emission without the assumption of a constant nonthermal
spectral index. Using the Spitzer FIR data at 70 and 160 $\mu$m and a standard
dust model, we de-redden the H$\alpha$ emission. The extinction-corrected
H$\alpha$ emission serves as a template for the thermal free-free radio
emission. Subtracting from the observed 3.6 and 20cm emission (Effelsberg and
the VLA) this free-free emission, we obtain maps of the nonthermal intensity
and spectral index.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:42:09 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Tabatabaei",
"F. S.",
""
],
[
"Beck",
"R.",
""
],
[
"Krügel",
"E.",
""
],
[
"Krause",
"M.",
""
],
[
"Berkhuijsen",
"E. M.",
""
],
[
"Gordon",
"K. D.",
""
],
[
"Menten",
"K. M.",
""
]
] | [
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] |
802.0643 | Julian Grond | J. Grond, W. P\"otz, A. Imamoglu | Spin entanglement using coherent light and cavity-QED | 17 pages, 13 figures, typos corrected, reference updated | Phys. Rev. B 77, 165307 (2008) | 10.1103/PhysRevB.77.165307 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A scheme for probabilistic entanglement generation between two distant single
electron doped quantum dots, each placed in a high-Q microcavity, by detecting
strong coherent light which has interacted dispersively with both subsystems
and experienced Faraday rotation due to the spin selective trion transitions is
discussed. In order to assess the applicability of the scheme for distant
entanglement generation between atomic qubits proposed by T.D. Ladd et al. [New
J. Phys. 8, 184 (2006)] to two distant quantum dots, one needs to understand
the limitations imposed by hyperfine interactions of the quantum dot spin with
the nuclear spins of the material and by non-identical quantum dots.
Feasibility is displayed by calculating the fidelity for Bell state generation
analytically within an approximate framework. The fidelity is evaluated for a
wide range of parameters and different pulse lengths, yielding a trade-off
between signal and decoherence, as well as a set of optimal parameters.
Strategies to overcome the effect of non-identical quantum dots on the fidelity
are examined and the timescales imposed by the nuclear spins are discussed,
showing that efficient entanglement generation is possible with distant quantum
dots. In this context, effects due to light hole transitions become important
and have to be included. The scheme is discussed for one- as well as for
two-sided cavities, where one must be careful with reflected light which
carries spin information. The validity of the approximate method is checked by
a more elaborate semiclassical simulation which includes trion formation.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:44:00 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 09:26:14 GMT"
}
] | 2015-03-13T00:00:00 | [
[
"Grond",
"J.",
""
],
[
"Pötz",
"W.",
""
],
[
"Imamoglu",
"A.",
""
]
] | [
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802.0644 | Laurent Michel | Gilles Lebeau, Laurent Michel | Semi-classical analysis of a random walk on a manifold | Published in at http://dx.doi.org/10.1214/09-AOP483 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, 277-315 | 10.1214/09-AOP483 | IMS-AOP-AOP483 | math.SP math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove a sharp rate of convergence to stationarity for a natural random
walk on a compact Riemannian manifold $(M,g)$. The proof includes a detailed
study of the spectral theory of the associated operator.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:49:13 GMT"
},
{
"version": "v2",
"created": "Tue, 16 Dec 2008 17:57:25 GMT"
},
{
"version": "v3",
"created": "Fri, 6 Nov 2009 16:40:45 GMT"
},
{
"version": "v4",
"created": "Tue, 2 Feb 2010 13:57:48 GMT"
}
] | 2010-02-02T00:00:00 | [
[
"Lebeau",
"Gilles",
""
],
[
"Michel",
"Laurent",
""
]
] | [
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] |
802.0645 | Kenneth Falconer | K.J. Falconer and J. Levy Vehel | Multifractional, multistable, and other processes with prescribed local
form | 32 pages | null | 10.1007/s10959-008-0147-9 | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a general method for constructing stochastic processes with
prescribed local form. Such processes include variable amplitude
multifractional Brownian motion, multifractional $\alpha$-stable processes, and
multistable processes, that is processes that are locally $\alpha(t)$-stable
but where the stability index $\alpha(t)$ varies with $t$. In particular we
construct multifractional multistable processes where both the local
self-similarity and stability indices vary.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:51:32 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Falconer",
"K. J.",
""
],
[
"Vehel",
"J. Levy",
""
]
] | [
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] |
802.0646 | Gabriel Maresch | Mathias Beiglb\"ock, Martin Goldstern, Gabriel Maresch, Walter
Schachermayer | Optimal and better transport plans | 25 pages | null | null | null | math.OC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider the Monge-Kantorovich transport problem in a purely measure
theoretic setting, i.e. without imposing continuity assumptions on the cost
function. It is known that transport plans which are concentrated on c-monotone
sets are optimal, provided the cost function c is either lower semi-continuous
and finite, or continuous and may possibly attain the value infty. We show that
this is true in a more general setting, in particular for merely Borel
measurable cost functions provided that {c=infty} is the union of a closed set
and a negligible set. In a previous paper Schachermayer and Teichmann
considered strongly c-monotone transport plans and proved that every strongly
c-monotone transport plan is optimal. We establish that transport plans are
strongly c-monotone if and only if they satisfy a "better" notion of optimality
called robust optimality.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:52:20 GMT"
},
{
"version": "v2",
"created": "Mon, 19 Jan 2009 08:29:12 GMT"
}
] | 2009-01-19T00:00:00 | [
[
"Beiglböck",
"Mathias",
""
],
[
"Goldstern",
"Martin",
""
],
[
"Maresch",
"Gabriel",
""
],
[
"Schachermayer",
"Walter",
""
]
] | [
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] |
802.0647 | Joseph Yukich | T. Schreiber and J. E. Yukich | Stabilization and limit theorems for geometric functionals of Gibbs
point processes | null | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Given a Gibbs point process $\P^{\Psi}$ on $\R^d$ having a weak enough
potential $\Psi$, we consider the random measures $\mu_\la := \sum_{x \in
\P^{\Psi} \cap Q_\la} \xi(x, \P^{\Psi} \cap Q_\la) \delta_{x/\la^{1/d}}$, where
$Q_{\la} := [-\la^{1/d}/2,\la^{1/d}/2]^d$ is the volume $\la$ cube and where
$\xi(\cdot,\cdot)$ is a translation invariant stabilizing functional. Subject
to $\Psi$ satisfying a localization property and translation invariance, we
establish weak laws of large numbers for $\la^{-1} \mu_\la(f)$, $f$ a bounded
test function on $\R^d$, and weak convergence of $\la^{-1/2} \mu_\la(f),$
suitably centered, to a Gaussian field acting on bounded test functions. The
result yields limit laws for geometric functionals on Gibbs point processes
including the Strauss and area interaction point processes as well as more
general point processes defined by the Widom-Rowlinson and hard-core model. We
provide applications to random sequential packing on Gibbsian input, to
functionals of Euclidean graphs, networks, and percolation models on Gibbsian
input, and to quantization via Gibbsian input.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:52:33 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Schreiber",
"T.",
""
],
[
"Yukich",
"J. E.",
""
]
] | [
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] |
802.0648 | Renxin Xu | Renxin Xu (PKU) | Astro-quark matter: a challenge facing astroparticle physics | 14 pages, 4 figures and 1 table; talk presented at CosPA2007
(International Symposium on Cosmology and Particle Astrophysics, Taipei, Nov.
13-15, 2007) | Mod.Phys.Lett.A23:1629-1642,2008 | 10.1142/S021773230802803X | null | astro-ph hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Quark matter both in terrestrial experiment and in astrophysics is briefly
reviewed. Astrophysical quark matter could appear in the early Universe, in
compact stars, and as cosmic rays. Emphasis is put on quark star as the nature
of pulsars. Possible astrophysical implications of experiment-discovered sQGP
are also concisely discussed.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:52:39 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Xu",
"Renxin",
"",
"PKU"
]
] | [
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802.0649 | Marek Karliner | Marek Karliner and Harry J. Lipkin | Possibility of Exotic States in the Upsilon system | LaTex, 5 pages | null | null | null | hep-ph hep-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Recent data from Belle show unusually large partial widths Upsilon(5S) -->
Upsilon(1S) pi^+pi^- and \Upsilon(5S) --> \Upsilon(2S) pi^+ pi^-. The Z(4430)
narrow resonance also reported by Belle in psi' pi^+ spectrum has the
properties expected of a (cbar c u dbar) charged isovector tetraquark T^{+-}_cc
The analogous state T^{+-} in the bottom sector might mediate anomalously large
cascade decays in the Upsilon system, Upsilon(mS) --> T^{+-}_bb pi^{-+} -->
Upsilon(nS) pi^+ \pi^-, with a tetraquark-pion intermediate state. We suggest
looking for the (bbar b u dbar) tetraquark in these decays as peaks in the
invariant mass of Upsilon(1S) pi or Upsilon(2S) pi systems. The (bbar b u sbar)
tetraquark can appear in the observed decays Upsilon(5S) --> Upsilon(1S) K^+
K^- as a peak in the invariant mass of Upsilon(1S) K system. We review the
model showing that these tetraquarks are below the two heavy meson threshold,
but respectively above the Upsilon pi pi and Upsilon K Kbar thresholds.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:52:43 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Mar 2008 14:28:37 GMT"
}
] | 2008-03-04T00:00:00 | [
[
"Karliner",
"Marek",
""
],
[
"Lipkin",
"Harry J.",
""
]
] | [
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802.065 | Luca Guido Molinari | Carlo Alberto Mantica and Luca Guido Molinari | A second-order identity for the Riemann tensor and applications | 16 pages | Colloq. Math. 122 (2011) 69 - 82 | 10.4064/cm122-1-7 | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A second-order differential identity for the Riemann tensor is obtained, on a
manifold with symmetric connection. Several old and some new differential
identities for the Riemann and Ricci tensors descend from it. Applications to
manifolds with Recurrent or Symmetric structures are discussed. The new
structure of K-recurrency naturally emerges from an invariance property of an
old identity by Lovelock.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 15:57:03 GMT"
},
{
"version": "v2",
"created": "Thu, 9 Jul 2009 14:33:01 GMT"
}
] | 2012-02-16T00:00:00 | [
[
"Mantica",
"Carlo Alberto",
""
],
[
"Molinari",
"Luca Guido",
""
]
] | [
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] |
802.0651 | Sergey K. Nemirovskii | Sergey K. Nemirovskii | Kinetics of a Network of Vortex Loops in He II and a Theory of
Superfluid Turbulence | 34 pages, 9 Postscript figures, [aps,preprint,12pt]{revtex4} | null | 10.1103/PhysRevB.77.214509 | null | cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A theory is developed to describe the superfluid turbulence on the base of
kinetics of the merging and splitting vortex loops. Because of very frequent
reconnections the vortex loops (as a whole) do not live long enough to perform
any essential evolution due to the deterministic motion. On the contrary, they
rapidly merge and split, and these random recombination processes prevail over
other slower dynamic processes. To develop quantitative description we take the
vortex loops to have a Brownian structure with the only degree of freedom,
which is the length $l$ of the loop. We perform investigation on the base of
the Boltzmann type kinetic equation for the distribution function $n(l)$ of
number of loops with length $l$. By use of the special ansatz in the collision
integral we have found the exact power-like solution to kinetic equation in the
stationary case. This solution is not (thermodynamically) equilibrium, but on
the contrary, it describes the state with two mutual fluxes of the length (or
energy) in space of sizes of the vortex loops. The term flux means just
redistribution of length (or energy) among the loops of different sizes due to
reconnections. Analyzing this solution we drew several results on the structure
and dynamics of the vortex tangle in the turbulent superfluid helium. In
particular, we evaluated the mean radius of the curvature and the full rate of
the reconnection events. We also studied the evolution of the full length of
vortex loops per unit volume-the so-called vortex line density. It is shown
this evolution to obey the famous Vinen equation. The properties of the Vinen
equation from the point of view of the developed approach had been discussed.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:00:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nemirovskii",
"Sergey K.",
""
]
] | [
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802.0652 | Plyatsko Roman | Roman Plyatsko, Oleksandr Stefanyshyn | Mathisson Equations: Non-Oscillatory Solutions in a Schwarzschild Field | 11 pages, 3 figures | ActaPhys.Polon.B39:23,2008 | null | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Mathisson equations under the Frenkel-Mathisson supplementary condition
are studied in a Schwarzschild field. The choice of solutions, which describe
the motions of the proper center of mass of a spinning test particle, is
discussed, and the calculation procedure for highly relativistic motions is
proposed. The very motions are important for astrophysics while investigating
possible effects of the gravitational spin-orbit interaction on the particle's
world line and trajectory.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:01:09 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Plyatsko",
"Roman",
""
],
[
"Stefanyshyn",
"Oleksandr",
""
]
] | [
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802.0653 | Jeroen Vandenbrink | Gianluca Giovannetti and Jeroen van den Brink | Electronic correlations decimate the ferroelectric polarization of
multiferroic HoMn2O5 | 4 pages, 4 figures | Phys. Rev. Lett. 100, 227603 (2008) | 10.1103/PhysRevLett.100.227603 | null | cond-mat.mtrl-sci cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that electronic correlations decimate the intrinsic ferroelectric
polarization of the recently discovered class of multiferroic manganites
RMn$_2$O$_5$, where R is a rare earth element. Such is manifest from {\it ab
initio} bandstructure computations that account for the strong local Coulomb
interactions between the manganese 3d electrons --the root of magnetism in
these materials. When including these the computed electronic, magnetic and
lattice structure of multiferroic HoMn$_2$O$_5$ results in an amplitude and
direction of polarization that is in accordance with experiment. The
microscopic mechanism behind the decimation is a near cancellation of the ionic
polarization induced by ferroelectric lattice displacements and the electronic
one caused by valence charge redistributions.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:02:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Giovannetti",
"Gianluca",
""
],
[
"Brink",
"Jeroen van den",
""
]
] | [
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] |
802.0654 | Juan Elias | Juan Elias and Giuseppe Valla | A family of local rings with rational Poincar\'e Series | null | null | null | null | math.AC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this note we compute the Poincare Series of almost stretched Gorenstein
local rings. It turns out that it is rational
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:06:37 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Elias",
"Juan",
""
],
[
"Valla",
"Giuseppe",
""
]
] | [
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] |
802.0655 | Alexander Zhidenko | Hideki Ishihara, Masashi Kimura, Roman A. Konoplya, Keiju Murata, Jiro
Soda, Alexander Zhidenko | Evolution of perturbations of squashed Kaluza-Klein black holes: escape
from instability | 12 pages, 6 figures | Phys.Rev.D77:084019,2008 | 10.1103/PhysRevD.77.084019 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The squashed Kaluza-Klien (KK) black holes differ from the Schwarzschild
black holes with asymptotic flatness or the black strings even at energies for
which the KK modes are not excited yet, so that squashed KK black holes open a
window in higher dimensions. Another important feature is that the squashed KK
black holes are apparently stable and, thereby, let us avoid the
Gregory-Laflamme instability. In the present paper, the evolution of scalar and
gravitational perturbations in time and frequency domains is considered for
these squashed KK black holes. The scalar field perturbations are analyzed for
general rotating squashed KK black holes. Gravitational perturbations for the
so called zero mode are shown to be decayed for non-rotating black holes, in
concordance with the stability of the squashed KK black holes. The correlation
of quasinormal frequencies with the size of extra dimension is discussed.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:07:25 GMT"
},
{
"version": "v2",
"created": "Sun, 9 Mar 2008 20:09:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ishihara",
"Hideki",
""
],
[
"Kimura",
"Masashi",
""
],
[
"Konoplya",
"Roman A.",
""
],
[
"Murata",
"Keiju",
""
],
[
"Soda",
"Jiro",
""
],
[
"Zhidenko",
"Alexander",
""
]
] | [
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] |
802.0656 | Stefano Pirandola | Stefano Pirandola, Samuel L. Braunstein, Stefano Mancini and Seth
Lloyd | Quantum Direct Communication with Continuous Variables | 6 pages, 5 figures, REVTeX | Europhys. Lett. 84, 20013 (2008) | 10.1209/0295-5075/84/20013 | null | quant-ph physics.optics | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show how continuous variable systems can allow the direct communication of
messages with an acceptable degree of privacy. This is possible by combining a
suitable phase-space encoding of the plain message with real-time checks of the
quantum communication channel. The resulting protocol works properly when a
small amount of noise affects the quantum channel. If this noise is
non-tolerable, the protocol stops leaving a limited amount of information to a
potential eavesdropper.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:18:37 GMT"
},
{
"version": "v2",
"created": "Wed, 20 Feb 2008 21:49:53 GMT"
},
{
"version": "v3",
"created": "Tue, 2 Dec 2008 23:10:40 GMT"
}
] | 2008-12-03T00:00:00 | [
[
"Pirandola",
"Stefano",
""
],
[
"Braunstein",
"Samuel L.",
""
],
[
"Mancini",
"Stefano",
""
],
[
"Lloyd",
"Seth",
""
]
] | [
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] |
802.0657 | Boris A. Popov | HARP Collaboration | Measurement of the production cross-sections of $\pi^\pm$ in p-C and
$\pi^\pm$-C interactions at 12 GeV/c | accepted for publication in Astroparticle Physics | null | 10.1016/j.astropartphys.2008.02.002 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The results of the measurements of the double-differential production
cross-sections of pions in p-C and $\pi^\pm$-C interactions using the forward
spectrometer of the HARP experiment are presented. The incident particles are
12 GeV/c protons and charged pions directed onto a carbon target with a
thickness of 5% of a nuclear interaction length. For p-C interactions the
analysis is performed using 100035 reconstructed secondary tracks, while the
corresponding numbers of tracks for $\pi^-$-C and $\pi^+$-C analyses are 106534
and 10122 respectively. Cross-section results are presented in the kinematic
range 0.5 GeV/c $\leq p_{\pi} <$ 8 GeV/c and 30 mrad $\leq \theta_{\pi} <$ 240
mrad in the laboratory frame. The measured cross-sections have a direct impact
on the precise calculation of atmospheric neutrino fluxes and on the improved
reliability of extensive air shower simulations by reducing the uncertainties
of hadronic interaction models in the low energy range.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:22:07 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"HARP Collaboration",
"",
""
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802.0658 | Enric Verdaguer | B.L. Hu and E. Verdaguer | Stochastic Gravity: Theory and Applications | 100 pages, no figures; an update of the 2003 review in Living Reviews
in Relativity gr-qc/0307032 ; it includes new sections on the Validity of
Semiclassical Gravity, the Stability of Minkowski Spacetime, and the Metric
Fluctuations of an Evaporating Black Hole | Living Rev. Relativity, 11 (2008) 3 | 10.12942/lrr-2008-3 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Whereas semiclassical gravity is based on the semiclassical Einstein equation
with sources given by the expectation value of the stress-energy tensor of
quantum fields, stochastic semiclassical gravity is based on the
Einstein-Langevin equation, which has in addition sources due to the noise
kernel. In the first part, we describe the fundamentals of this new theory via
two approaches: the axiomatic and the functional. In the second part, we
describe three applications of stochastic gravity theory. First, we consider
metric perturbations in a Minkowski spacetime, compute the two-point
correlation functions of these perturbations and prove that Minkowski spacetime
is a stable solution of semiclassical gravity. Second, we discuss structure
formation from the stochastic gravity viewpoint. Third, we discuss the
backreaction of Hawking radiation in the gravitational background of a black
hole and describe the metric fluctuations near the event horizon of an
evaporating black hole
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:23:28 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Hu",
"B. L.",
""
],
[
"Verdaguer",
"E.",
""
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802.0659 | Pier Giorgio Bizzeti | P.G. Bizzeti and A.M. Bizzeti-Sona | Description of nuclear octupole and quadrupole deformation close to the
axial symmetry: Critical-point behavior of 224Ra and 224Th | 11 pages, 9 figures | Phys.Rev.C77:024320,2008 | 10.1103/PhysRevC.77.024320 | null | nucl-th nucl-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The model, introduced in a previous paper, for the description of the
octupole and quadrupole degrees of freedom in conditions close to the axial
symmetry, is applied to situations of shape phase transitions where the
quadrupole amplitude can reach zero. The transitional nuclei 224,226Ra and
224Th are discussed in the frame of this model. Their level schemes can be
reasonably accounted for assuming a square-well potential in two dimensions.
Electromagnetic transition amplitudes are also evaluated and compared with
existing experimental data.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:23:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bizzeti",
"P. G.",
""
],
[
"Bizzeti-Sona",
"A. M.",
""
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] |
802.066 | Niclas Wyllard | Mans Henningson, Niclas Wyllard | Zero-energy states of N = 4 SYM on T^3: S-duality and the mapping class
group | 17 pages | JHEP 0804:066,2008 | 10.1088/1126-6708/2008/04/066 | null | hep-th | null | We continue our studies of the low-energy spectrum of N=4 super-Yang-Mills
theory on a spatial three-torus. In two previous papers, we computed the
spectrum of normalizable zero-energy states for all choices of gauge group and
all values of the electric and magnetic 't Hooft fluxes, and checked its
invariance under the SL_2(Z) S-duality group. In this paper, we refine the
analysis by also decomposing the space of bound states into irreducible unitary
representations of the SL_3(Z) mapping class group of the three-torus. We
perform a detailed study of the S-dual pairs of theories with gauge groups
Spin(2n+1) and Sp(2n). The predictions of S-duality (which commutes with the
mapping class group) are fulfilled as expected, but the proof requires some
surprisingly intricate combinatorial infinite product identities.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:32:03 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Henningson",
"Mans",
""
],
[
"Wyllard",
"Niclas",
""
]
] | [
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] |
802.0661 | Ludkovsky Sergey Victor | S. V. Ludkovsky | Wrap groups of fiber bundles over quaternions and octonions | 27 pages, misprints are corrected | null | null | null | math.FA math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This article is devoted to the investigation of wrap groups of connected
fiber bundles over the fields of real $\bf R$, complex $\bf C$ numbers, the
quaternion skew field $\bf H$ and the octonion algebra $\bf O$. These groups
are constructed with mild conditions on fibers. Their examples are given. It is
shown, that these groups exist and for differentiable fibers have the infinite
dimensional Lie groups structure, that is, they are continuous or
differentiable manifolds and the composition $(f,g)\mapsto f^{-1}g$ is
continuous or differentiable depending on a class of smoothness of groups.
Moreover, it is demonstrated that in the cases of real, complex, quaternion and
octonion manifolds these groups have structures of real, complex, quaternion or
octonion manifolds respectively. Nevertheless, it is proved that these groups
does not necessarily satisfy the Campbell-Hausdorff formula even locally.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:33:16 GMT"
},
{
"version": "v2",
"created": "Mon, 22 Dec 2008 22:10:52 GMT"
}
] | 2008-12-23T00:00:00 | [
[
"Ludkovsky",
"S. V.",
""
]
] | [
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] |
802.0662 | Marco Panero | Falk Bruckmann, Stefan Keppeler, Marco Panero and Tilo Wettig | Polyakov loops and SU(2) staggered Dirac spectra | 7 pages, 4 figures, talk given by M. Panero at the XXV International
Symposium on Lattice Field Theory, Regensburg, Germany, 30 July - 4 August
2007 | PoS(LATTICE 2007)274 | null | null | hep-lat hep-th | null | We consider the spectrum of the staggered Dirac operator with SU(2) gauge
fields. Our study is motivated by the fact that the antiunitary symmetries of
this operator are different from those of the SU(2) continuum Dirac operator.
In this contribution, we investigate in some detail staggered eigenvalue
spectra close to the free limit. Numerical experiments in the quenched
approximation and at very large $\beta$-values show that the eigenvalues occur
in clusters consisting of eight eigenvalues each. We can predict the locations
of these clusters for a given configuration very accurately by an analytical
formula involving Polyakov loops and boundary conditions. The spacing
distribution of the eigenvalues within the clusters agrees with the chiral
symplectic ensemble of random matrix theory, in agreement with theoretical
expectations, whereas the spacing distribution between the clusters tends
towards Poisson behavior.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:21:43 GMT"
}
] | 2009-04-14T00:00:00 | [
[
"Bruckmann",
"Falk",
""
],
[
"Keppeler",
"Stefan",
""
],
[
"Panero",
"Marco",
""
],
[
"Wettig",
"Tilo",
""
]
] | [
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] |
802.0663 | Konrad Waldorf | Urs Schreiber and Konrad Waldorf | Smooth Functors vs. Differential Forms | 75 pages, 1 figure; v2 with only minor changes; v3 has a layout
improvement; v4 is the published version, with small improvements and a
better proof of Lemma 2.6 | Homology, Homotopy Appl., 13(1), 143-203 (2011) | null | null | math.DG math.CT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We establish a relation between smooth 2-functors defined on the path
2-groupoid of a smooth manifold and differential forms on this manifold. This
relation can be understood as a part of a dictionary between fundamental
notions from category theory and differential geometry. We show that smooth
2-functors appear in several fields, namely as connections on (non-abelian)
gerbes, as curvatures of smooth functors and as critical points in BF theory.
We demonstrate further that our dictionary provides a powerful tool to discuss
the transgression of geometric objects to loop spaces.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:48:51 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Aug 2008 19:31:13 GMT"
},
{
"version": "v3",
"created": "Thu, 11 Mar 2010 08:55:00 GMT"
},
{
"version": "v4",
"created": "Mon, 18 Jul 2011 22:19:44 GMT"
}
] | 2011-07-20T00:00:00 | [
[
"Schreiber",
"Urs",
""
],
[
"Waldorf",
"Konrad",
""
]
] | [
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] |
802.0664 | Dinesh Shetty | D.V. Shetty, G.A. Souliotis, S. Galanopoulos, Z. Kohley, S.N. Soisson,
B.C. Stein, S. Wuenschel, and S.J. Yennello | Nuclear expansion and symmetry energy of hot nuclei | 10 pages, 2 figures | J.Phys.G: Nucl. Part. Phys. 36 (2009) 075103 | 10.1088/0954-3899/36/7/075103 | null | nucl-ex nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The decrease in the symmetry energy of hot nuclei populated in $^{58}$Ni +
$^{58}$Ni, $^{58}$Fe + $^{58}$Ni and $^{58}$Fe + $^{58}$Fe reactions at beam
energies of 30, 40, and 47 MeV/nucleon, as a function of excitation energy is
studied. It is observed that this decrease is mainly a consequence of
increasing expansion or decreasing density rather than the increasing
temperature. The results are in good agreement with the recently reported
microscopic calculation based on the Thomas-Fermi approach. An empirical
relation to study the symmetry energy of finite nuclei in various mass region
is proposed.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:49:04 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Shetty",
"D. V.",
""
],
[
"Souliotis",
"G. A.",
""
],
[
"Galanopoulos",
"S.",
""
],
[
"Kohley",
"Z.",
""
],
[
"Soisson",
"S. N.",
""
],
[
"Stein",
"B. C.",
""
],
[
"Wuenschel",
"S.",
""
],
[
"Yennello",
"S. J.",
""
]
] | [
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802.0665 | Tanusree Pal | Tanusree Pal | Vogan Diagrams of Twisted Affine Kac-Moody Lie Algebras | Changed contents | null | null | null | math.RA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A Vogan diagram is a Dynkin diagram of a Kac-Moody Lie algebra of finite or
affine type overlayed with additional structures. This paper develops the
theory of Vogan diagrams for almost compact real forms of indecomposable
twisted affine Kac- Moody Lie algebras and shows that equivalence classes of
Vogan diagrams correspond to isomorphism classes of almost compact real forms
of twisted affine Kac-Moody Lie algebras as given by H. Ben Messaoud and G.
Rousseau.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:44:42 GMT"
},
{
"version": "v2",
"created": "Fri, 1 Aug 2008 07:13:17 GMT"
}
] | 2008-08-01T00:00:00 | [
[
"Pal",
"Tanusree",
""
]
] | [
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] |
802.0666 | Lasse Rempe | Lasse Rempe and Sebastian van Strien | Absence of line fields and Mane's theorem for non-recurrent
transcendental functions | 28 pages; V3. Proof of Theorem 7.4 corrected, as well as some other
minor corrections | Trans. Amer. Math. Soc. 363 (2011), 203-228 | 10.1090/S0002-9947-2010-05125-6 | null | math.DS math.CV | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let f be a transcendental meromorphic function. Suppose that the finite part
of the postsingular set of f is bounded, that f has no recurrent critical
points or wandering domains, and that the degree of pre-poles of f is uniformly
bounded. Then we show that f supports no invariant line fields on its Julia
set.
We prove this by generalizing two results about rational functions to the
transcendental setting: a theorem of Mane about the branching of iterated
preimages of disks, and a theorem of McMullen regarding absence of invariant
line fields for "measurably transitive" functions. Both our theorems extend
results previously obtained by Graczyk, Kotus and Swiatek.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 16:54:48 GMT"
},
{
"version": "v2",
"created": "Wed, 8 Oct 2008 12:16:09 GMT"
},
{
"version": "v3",
"created": "Fri, 6 Aug 2010 15:43:53 GMT"
}
] | 2014-11-14T00:00:00 | [
[
"Rempe",
"Lasse",
""
],
[
"van Strien",
"Sebastian",
""
]
] | [
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] |
802.0667 | Boris Malomed | Ze'ev Birnbaum and Boris A. Malomed (Department of Physical
Electronics, School of Electrical Engineering, Faculty of Engineering, Tel
Aviv University, Tel Aviv, Israel) | Families of spatial solitons in a two-channel waveguide with the
cubic-quintic nonlinearity | null | null | 10.1016/j.physd.2008.08.005 | null | nlin.PS physics.optics | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present eight types of spatial optical solitons which are possible in a
model of a planar waveguide that includes a dual-channel trapping structure and
competing (cubic-quintic) nonlinearity. Among the families of trapped beams are
symmetric and antisymmetric solitons of "broad" and "narrow" types, composite
states, built as combinations of broad and narrow beams with identical or
opposite signs ("unipolar" and "bipolar" states, respectively), and
"single-sided" broad and narrow beams trapped, essentially, in a single
channel. The stability of the families is investigated via eigenvalues of small
perturbations, and is verified in direct simulations. Three species - narrow
symmetric, broad antisymmetric, and unipolar composite states - are unstable to
perturbations with real eigenvalues, while the other five families are stable.
The unstable states do not decay, but, instead, spontaneously transform
themselves into persistent breathers, which, in some cases, demonstrate
dynamical symmetry breaking and chaotic internal oscillations. A noteworthy
feature is a stability exchange between the broad and narrow antisymmetric
states: in the limit when the two channels merge into one, the former species
becomes stable, while the latter one loses its stability. Different branches of
the stationary states are linked by four bifurcations, which take different
forms in the model with the strong and weak inter-channel coupling.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:03:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Birnbaum",
"Ze'ev",
"",
"Department of Physical\n Electronics, School of Electrical Engineering, Faculty of Engineering, Tel\n Aviv University, Tel Aviv, Israel"
],
[
"Malomed",
"Boris A.",
"",
"Department of Physical\n Electronics, School of Electrical Engineering, Faculty of Engineering, Tel\n Aviv University, Tel Aviv, Israel"
]
] | [
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] |
802.0668 | Francesco Marin | J. Belfi, F. Marin | Sensitivity below the standard quantum limit in gravitational wave
detectors with Michelson-Fabry-Perot readout | null | Phys.Rev.D77:122002,2008 | 10.1103/PhysRevD.77.122002 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We calculate the quantum noise limited displacement sensitivity of a
Michelson-Fabry-Perot (MFP) with detuned cavities, followed by phase-sensitive
homodyne detection. We show that the standard quantum limit can be surpassed
even with resonant cavities and without any signal-recycling mirror nor
additional cavities. Indeed, thanks to the homodyne detection, the output field
quadrature can be chosen in such a way to cancel the effect of input amplitude
fluctuations, i.e., eliminating the force noise. With detuned cavities, the
modified opto-mechanical susceptivity allows to reach unlimited sensitivity for
large enough (yet finite) optical power. Our expressions include mirror losses
and cavity delay effect, for a realistic comparison with experiments. Our study
is particularly devoted to gravitational wave detectors and we consider both an
interferometer with free-falling mirrors, and a MFP as readout for a massive
detector. In the latter case, the sensitivity curve of the recently conceived
'DUAL' detector, based on two acoustic modes, is obtained.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:11:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Belfi",
"J.",
""
],
[
"Marin",
"F.",
""
]
] | [
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] |
802.0669 | Vadim Guzey | K. Goeke (Ruhr U., Bochum), V. Guzey (Jefferson Lab), M. Siddikov
(Ruhr U., Bochum & Uzbekistan Natl. U.) | Deeply Virtual Compton Scattering on nucleons and nuclei in generalized
vector meson dominance model | 25 pages, 9 figures, 1 table | Eur.Phys.J.A36:49-60,2008 | 10.1140/epja/i2008-10549-x | JLAB-THY-08-774 | hep-ph hep-ex nucl-th | http://creativecommons.org/licenses/publicdomain/ | We consider Deeply Virtual Compton Scattering (DVCS) on nucleons and nuclei
in the framework of generalized vector meson dominance (GVMD) model. We
demonstrate that the GVMD model provides a good description of the HERA data on
the dependence of the proton DVCS cross section on Q^2, W (at Q^2=4 GeV^2) and
t. At Q^2 = 8 GeV^2, the soft W-behavior of the GVMD model somewhat
underestimates the W-dependence of the DVCS cross section due to the hard
contribution not present in the GVMD model. We estimate 1/Q^2 power-suppressed
corrections to the DVCS amplitude and the DVCS cross section and find them
large. We also make predictions for the nuclear DVCS amplitude and cross
section in the kinematics of the future Electron-Ion Collider. We predict
significant nuclear shadowing, which matches well predictions of the
leading-twist nuclear shadowing in DIS on nuclei.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:14:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Goeke",
"K.",
"",
"Ruhr U., Bochum"
],
[
"Guzey",
"V.",
"",
"Jefferson Lab"
],
[
"Siddikov",
"M.",
"",
"Ruhr U., Bochum & Uzbekistan Natl. U."
]
] | [
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] |
802.067 | Markus Lazar | Markus Lazar, Charalampos Anastassiadis | The gauge theory of dislocations: static solutions of screw and edge
dislocations | 33 pages, 17 figures | null | 10.1080/14786430802558551 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the T(3)-gauge theory of static dislocations in continuous
solids. We use the most general linear constitutive relations bilinear in the
elastic distortion tensor and dislocation density tensor for the force and
pseudomoment stresses of an isotropic solid. The constitutive relations contain
six material parameters. In this theory both the force and pseudomoment
stresses are asymmetric. The theory possesses four characteristic lengths l1,
l2, l3 and l4 which are given explicitely. We first derive the
three-dimensional Green tensor of the master equation for the force stresses in
the translational gauge theory of dislocations. We then investigate the
situation of generalized plane strain (anti-plane strain and plane strain).
Using the stress function method, we find modified stress functions for screw
and edge dislocations. The solution of the screw dislocation is given in terms
of one independent length l1=l4. For the problem of an edge dislocation, only
two characteristic lengths l2 and l3 arise with one of them being the same
l2=l1 as for the screw dislocation. Thus, this theory possesses only two
independent lengths for generalized plane strain. If the two lengths l2 and l3
of an edge dislocation are equal, we obtain an edge dislocation which is the
gauge theoretical version of a modified Volterra edge dislocation. In the case
of symmetric stresses we recover well known results obtained earlier.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:18:34 GMT"
},
{
"version": "v2",
"created": "Tue, 30 Sep 2008 13:02:12 GMT"
},
{
"version": "v3",
"created": "Thu, 2 Oct 2008 11:10:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lazar",
"Markus",
""
],
[
"Anastassiadis",
"Charalampos",
""
]
] | [
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] |
802.0671 | Daniel Dale | Daniel A. Dale, Rebecca J. Barlow, Seth A. Cohen, L. Clifton Johnson,
ShiAnne M. Kattner, Christine A. Lamanna, Carolynn A. Moore, Micah D.
Schuster and Jacob W. Thatcher | The Wyoming Survey for H-alpha. I. Initial Results at z ~ 0.16 and 0.24 | To appear in the Astronomical Journal | null | 10.1088/0004-6256/135/4/1412 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Wyoming Survey for H-alpha, or WySH, is a large-area, ground-based,
narrowband imaging survey for H-alpha-emitting galaxies over the latter half of
the age of the Universe. The survey spans several square degrees in a set of
fields of low Galactic cirrus emission. The observing program focuses on
multiple dz~0.02 epochs from z~0.16 to z~0.81 down to a uniform
(continuum+line) luminosity at each epoch of ~10^33 W uncorrected for
extinction (3sigma for a 3" diameter aperture). First results are presented
here for 98+208 galaxies observed over approximately 2 square degrees at
redshifts z~0.16 and 0.24, including preliminary luminosity functions at these
two epochs. These data clearly show an evolution with lookback time in the
volume-averaged cosmic star formation rate. Integrals of Schechter fits to the
extinction-corrected H-alpha luminosity functions indicate star formation rates
per co-moving volume of 0.009 and 0.014 h_70 M_sun/yr/Mpc^3 at z~0.16 and 0.24,
respectively. The formal uncertainties in the Schechter fits, based on this
initial subset of the survey, correspond to uncertainties in the cosmic star
formation rate density at the >~40% level; the tentative uncertainty due to
cosmic variance is 25%, estimated from separately carrying out the analysis on
data from the first two fields with substantial datasets.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:19:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dale",
"Daniel A.",
""
],
[
"Barlow",
"Rebecca J.",
""
],
[
"Cohen",
"Seth A.",
""
],
[
"Johnson",
"L. Clifton",
""
],
[
"Kattner",
"ShiAnne M.",
""
],
[
"Lamanna",
"Christine A.",
""
],
[
"Moore",
"Carolynn A.",
""
],
[
"Schuster",
"Micah D.",
""
],
[
"Thatcher",
"Jacob W.",
""
]
] | [
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] |
802.0672 | Horacio Ceva | Ines Caridi and Horacio Ceva | The underlying complex network of the Minority Game | null | null | null | null | physics.soc-ph cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the structure of the underlying network of connections in the
Minority Game. There is not an explicit interaction among the agents, but they
interact via global magnitudes of the model and mainly through their
strategies. We define a link between two agents by quantifying the similarity
among their strategies, and analyze the structure of the resulting underlying
complex networks as a function of the number of agents in the game and the
value of the agents' memory, in games with two strategies per player. We
characterize the different phases of this system with networks with different
properties, for this link definition. Thus, the Minority Game phase
characterized by the presence of crowds can be identified with a small world
network, while the phase with the same results as a random decision game as a
random network. Finally, we use the Full Strategy Minority Game model, to
explicitly calculate some properties of its networks, such as the degree
distribution, for the same link definition, and to estimate, from them, the
properties of the networks of the Minority Game, obtaining a very good
agreement with its measured properties.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:20:28 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Caridi",
"Ines",
""
],
[
"Ceva",
"Horacio",
""
]
] | [
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] |
802.0673 | Erkan Nane | Mark M. Meerschaert, Erkan Nane, P. Vellaisamy | Fractional Cauchy problems on bounded domains | Published in at http://dx.doi.org/10.1214/08-AOP426 the Annals of
Probability (http://www.imstat.org/aop/) by the Institute of Mathematical
Statistics (http://www.imstat.org) | Annals of Probability 2009, Vol. 37, No. 3, 979-1007 | 10.1214/08-AOP426 | IMS-AOP-AOP426 | math.PR math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Fractional Cauchy problems replace the usual first-order time derivative by a
fractional derivative. This paper develops classical solutions and stochastic
analogues for fractional Cauchy problems in a bounded domain
$D\subset\mathbb{R}^d$ with Dirichlet boundary conditions. Stochastic solutions
are constructed via an inverse stable subordinator whose scaling index
corresponds to the order of the fractional time derivative. Dirichlet problems
corresponding to iterated Brownian motion in a bounded domain are then solved
by establishing a correspondence with the case of a half-derivative in time.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:21:25 GMT"
},
{
"version": "v2",
"created": "Fri, 24 Jul 2009 14:14:49 GMT"
}
] | 2009-07-24T00:00:00 | [
[
"Meerschaert",
"Mark M.",
""
],
[
"Nane",
"Erkan",
""
],
[
"Vellaisamy",
"P.",
""
]
] | [
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] |
802.0674 | Uma P. Vijh | A. N. Witt (1), S. Mandel (2), P. H. Sell (3), T. Dixon (4) and U. P.
Vijh (1) ((1) University of Toledo, (2) Hidden Valley Observatory, (3)
University of Wisconsin, (4) University of Hawaii) | Extended Red Emission in High-Galactic Latitude Interstellar Clouds | Accepted for Publication in the ApJ | null | 10.1086/587131 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Nearby interstellar clouds at high Galactic latitudes are ideal objects in
which the interaction of interstellar dust with photons from the
well-characterized interstellar radiation field can be studied. Scattering and
UV-excited photoluminescence at optical wavelengths as well as thermal emission
at mid- and far-infrared wavelengths are observable manifestations of such
interactions. Here we report initial results from an optical imaging survey of
optically thin high-Galactic-latitude clouds, which is designed to study the
surface brightness, structure, and spectral energy distribution of these
objects. The primary aim of this paper is to study the extended red emission
(ERE) that has been reported at high Galactic latitudes in earlier
investigations and which is attributed to ultraviolet-excited photoluminescence
of an as yet unidentified component of interstellar dust. We find strong
evidence for dust emission in the form of a broad (>1000 A FWHM) ERE band with
peak emission near 600 nm wavelength and peak intensity of ~ 5x10^-9 (erg cm^-2
s^-1 A^-1 sr^-1) in optically-thin clouds. This amounts to about 30% of the
total optical surface brightness of these clouds, the remainder being
consistent with expectations for dust-scattered light. This supports claims for
the ubiquitous presence of the ERE carrier throughout the diffuse interstellar
medium of the Milky Way Galaxy. We suggest that the ERE carrier is involved in
the radiative processing of about 20% to 30% of the dust-absorbed UV/optical
luminosity of the Milky Way galaxy, with the bulk of this energy being emitted
in the near- to mid-infrared spectral regions.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:23:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Witt",
"A. N.",
""
],
[
"Mandel",
"S.",
""
],
[
"Sell",
"P. H.",
""
],
[
"Dixon",
"T.",
""
],
[
"Vijh",
"U. P.",
""
]
] | [
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802.0675 | Emil Johansson Bergholtz | Eddy Ardonne, Emil J. Bergholtz, Janik Kailasvuori, Emma Wikberg | Degeneracy of non-abelian quantum Hall states on the torus: domain walls
and conformal field theory | 15 pages | J.Stat.Mech.0804:P04016,2008 | 10.1088/1742-5468/2008/04/P04016 | NORDITA-2008-5 | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We analyze the non-abelian Read-Rezayi quantum Hall states on the torus,
where it is natural to employ a mapping of the many-body problem onto a
one-dimensional lattice model. On the thin torus--the Tao-Thouless (TT)
limit--the interacting many-body problem is exactly solvable. The Read-Rezayi
states at filling $\nu=\frac k {kM+2}$ are known to be exact ground states of a
local repulsive $k+1$-body interaction, and in the TT limit this is manifested
in that all states in the ground state manifold have exactly $k$ particles on
any $kM+2$ consecutive sites. For $M\neq 0$ the two-body correlations of these
states also imply that there is no more than one particle on $M$ adjacent
sites. The fractionally charged quasiparticles and quasiholes appear as domain
walls between the ground states, and we show that the number of distinct domain
wall patterns gives rise to the nontrivial degeneracies, required by the
non-abelian statistics of these states. In the second part of the paper we
consider the quasihole degeneracies from a conformal field theory (CFT)
perspective, and show that the counting of the domain wall patterns maps one to
one on the CFT counting via the fusion rules. Moreover we extend the CFT
analysis to topologies of higher genus.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:26:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ardonne",
"Eddy",
""
],
[
"Bergholtz",
"Emil J.",
""
],
[
"Kailasvuori",
"Janik",
""
],
[
"Wikberg",
"Emma",
""
]
] | [
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] |
802.0676 | Roald Guandalini | R. Guandalini (Department of Physics, University of Perugia) | MS, S and C Stars in the Infrared. Luminosities and Mass Loss Rates | 10 pages, 6 figures, contribution from the IX Torino Workshop, to be
published by AIP | AIP Conf.Proc.1001:339-348,2008 | 10.1063/1.2916983 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this note I present an outline of infrared (IR) photometric AGB
properties, based on two samples of Galactic Long Period Variables (C- and
S-type respectively). I show the various selection criteria used during the
choice of the sources and describe the motivations of observing them at near-
and mid-IR wavelengths. I discuss the problems encountered in estimating their
luminosity and distance and motivate the methods I choose for this purpose.
Properties of the luminosity functions and of the Hertzsprung-Russell (HR)
diagrams obtained from the analysis are discussed. Finally, the choices made
for estimating of the mass loss rates are described and preliminary results
concerning them are shown.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 20:04:08 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Guandalini",
"R.",
"",
"Department of Physics, University of Perugia"
]
] | [
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802.0677 | Andrei Vieru | Andrei Vieru | General definitions of chaos for continuous and discrete-time processes | 9 pages | null | null | null | math.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A precise definition of chaos for discrete processes based on iteration
already exists. We shall first reformulate it in a more general frame, taking
into account the fact that discrete chaotic behavior is neither necessarily
based on iteration nor strictly related to compact metric spaces or to bounded
functions. Then we shall apply the central idea of this definition to
continuous processes. We shall try to see what chaos is, regardless of the way
it is generated.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:32:07 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Mar 2008 17:48:21 GMT"
},
{
"version": "v3",
"created": "Sat, 31 May 2008 22:40:27 GMT"
}
] | 2008-06-01T00:00:00 | [
[
"Vieru",
"Andrei",
""
]
] | [
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802.0678 | Gabriele Cescutti | G. Cescutti (Astronomy Department, Trieste University) | An inhomogeneous model for the Galactic halo: a possible explanation for
the spread observed in s- and r-process elements | 10 pages, 14 figures, accepted for publication in A&A | null | 10.1051/0004-6361:20078571 | null | astro-ph | null | We propose an explanation for the considerable scatter of the abundances of
neutron capture elements observed in low-metallicity stars in the solar
vicinity, compared to the small star-to-star scatter observed for the
alpha-elements. We have developed a stochastic chemical evolution model in
which the main assumption is a random formation of new stars subject to the
condition that the cumulative mass distribution follows a given initial mass
function. With our model, we are able to reproduce the different spreads of
neutron capture elements and alpha-elements in low-metallicity stars. The
reason for different observed spread in neutron capture elements and
alpha-elements resides in the random birth of stars, coupled with different
stellar mass ranges, from which alpha-elements and neutron capture elements
originate. In particular, the site of production of alpha-elements is the whole
range of massive stars, from 10 to 80 Msun whereas the mass range of production
for neutron capture elements lies between 12 and 30 Msun.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:00:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cescutti",
"G.",
"",
"Astronomy Department, Trieste University"
]
] | [
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] |
802.0679 | Fatine Latif | Emmanuel Fricain (ICJ), Javad Mashreghi | Boundary behavior of functions in the de Branges--Rovnyak spaces | null | null | null | null | math.CV math.FA | null | This paper deals with the boundary behavior of functions in the de
Branges--Rovnyak spaces. First, we give a criterion for the existence of radial
limits for the derivatives of functions in the de Branges--Rovnyak spaces. This
criterion generalizes a result of Ahern-Clark. Then we prove that the
continuity of all functions in a de Branges--Rovnyak space on an open arc $I$
of the boundary is enough to ensure the analyticity of these functions on $I$.
We use this property in a question related to Bernstein's inequality.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:38:36 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Fricain",
"Emmanuel",
"",
"ICJ"
],
[
"Mashreghi",
"Javad",
""
]
] | [
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] |
802.068 | Roberto D. Mota Esteves | D Martinez and R D Mota | SUSY QM, symmetries and spectrum generating algebras for two-dimensional
systems | null | null | 10.1016/j.aop.2007.07.001 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show in a systematic and clear way how factorization methods can be used
to construct the generators for hidden and dynamical symmetries. This is shown
by studying the 2D problems of hydrogen atom, the isotropic harmonic oscillator
and the radial potential $A\rho^{2\zeta-2}-B\rho^{\zeta-2}$. We show that in
these cases the non-compact (compact) algebra corresponds to so(2,1) (su(2)).
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:45:51 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Martinez",
"D",
""
],
[
"Mota",
"R D",
""
]
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802.0681 | Christophe Real | Christophe Real | Numerical Correpondences between the physical Constants | null | null | null | null | physics.gen-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present here a note which synthesizes our previous ideas concerning some
problems in cosmology, and the numerical correspondences between the physical
constants that we could deduce.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:50:26 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Real",
"Christophe",
""
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] |
802.0682 | Davide Pini | Alberto Parola, Davide Pini, and Luciano Reatto | Liquid-vapor transition from a microscopic theory: Beyond the Maxwell
construction | 4 pages, 5 figures | null | 10.1103/PhysRevLett.100.165704 | null | cond-mat.stat-mech cond-mat.soft | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A smooth cut-off formulation of the Hierarchical Reference Theory (HRT) is
developed and applied to a Yukawa fluid. The HRT equations are derived and
numerically solved leading to: the expected renormalization group structure in
the critical region, non classical critical exponents and scaling laws, a
convex free energy in the whole phase diagram (including the two-phase region),
finite compressibility at coexistence, together with a fully satisfactory
comparison with available numerical simulations. This theory, which also
guarantees the correct short range behavior of two body correlations,
represents a major improvement over the existing liquid state theories.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 17:56:10 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Apr 2008 18:01:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Parola",
"Alberto",
""
],
[
"Pini",
"Davide",
""
],
[
"Reatto",
"Luciano",
""
]
] | [
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] |
802.0683 | Gabriel Price | Gabriel N. Price, S. Travis Bannerman, Kirsten Viering, Edvardas
Narevicius and Mark G. Raizen | Single-Photon Atomic Cooling | 4 pages and 3 figures | null | 10.1103/PhysRevLett.100.093004 | null | physics.atom-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report the cooling of an atomic ensemble with light, where each atom
scatters only a single photon on average. This is a general method that does
not require a cycling transition and can be applied to atoms or molecules which
are magnetically trapped. We discuss the application of this new approach to
the cooling of hydrogenic atoms for the purpose of precision spectroscopy and
fundamental tests.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:01:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Price",
"Gabriel N.",
""
],
[
"Bannerman",
"S. Travis",
""
],
[
"Viering",
"Kirsten",
""
],
[
"Narevicius",
"Edvardas",
""
],
[
"Raizen",
"Mark G.",
""
]
] | [
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] |
802.0684 | W. Desmond Ramsay | Willem T.H. van Oers | From Hadronic Parity Violation to Parity-Violating Electron Scattering
and Tests of the Standard Model | 12 pages, 8 figures, LaTeX. Invited talk at the International
Symposium on Cosmology and Particle Astrophysics (CosPA07), Taipei, Taiwan,
Nov 13-15, 2007 | null | 10.1142/S0217732308027643 | TRI-PP-07-46 | nucl-ex hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | After almost five decades of study of parity violation in hadronic systems,
the determination of the seven weak meson-nucleon couplings is still
incomplete. Whereas parity violation in nuclear systems is complicated by the
intricacies of QCD, measurements of parity violation in the much simpler
proton-proton system are more straightforward to interpret. We now have three
such precision pp experiments at 13.6, at 45, and 221 MeV. Today there are also
better possibilities for theoretical interpretation using effective field
theory. In electron-proton scattering, parity violating ep experiments such as
SAMPLE, G0, HAPPEX, and PVA4 have already shown that the strange quark
contributions to the charge and magnetization distributions of the nucleon are
tiny. When analyzed together, the results have also greatly improved knowledge
of the proton's "weak charge" (Q^p_weak = 1-4sin^2\theta_W at tree level). The
Q^p_weak experiment at JLab will further improve this, determining the proton's
weak charge to a precision of about 4%. Such a precision will either establish
conformity with the Standard Model of quarks and leptons or point to New
Physics. Following the upgrade of CEBAF at JLab to 12 GeV, a parity violating
electron-electron (Moller) scattering experiment similar to SLAC E158, will
measure the weak charge of the electron and hence sin^2\theta_W at low energy
with a precision comparable to the most precise individual measurements at the
Z0 pole (to about +/- 0.00025). This experiment will be complementary to
Q^p_weak in terms of sensitivity to New Physics.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:02:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"van Oers",
"Willem T. H.",
""
]
] | [
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] |
802.0685 | C\'edric B\'eny | C\'edric B\'eny | Unsharp pointer observables and the structure of decoherence | null | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The theory of decoherence attempts to explain the emergent classical
behaviour of a quantum system interacting with its quantum environment. In
order to formalize this mechanism we introduce the idea that the information
preserved in an open quantum evolution (or channel) can be characterized in
terms of observables of the initial system. We use this approach to show that
information which is broadcast into many parts of the environment can be
encoded in a single observable. This supports a model of decoherence where the
pointer observable can be an arbitrary positive operator-valued measure (POVM).
This generalization makes it possible to characterize the emergence of a
realistic classical phase-space. In addition, this model clarifies the
relationships among the information preserved in the system, the information
flowing from the system to the environment (measurement), and the establishment
of correlations between the system and the environment.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 20:39:37 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Bény",
"Cédric",
""
]
] | [
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802.0686 | Colin Torney Mr | Colin Torney, Zoltan Neufeld | Phototactic Clustering of Swimming Micro-organisms in a Turbulent
Velocity Field | null | null | 10.1103/PhysRevLett.101.078105 | null | math-ph math.MP | null | We study the distribution of swimming micro-organisms advected by a model
turbulent flow and attracted towards a localised light source through
phototaxis. It is shown that particles aggregate along a dynamical attractor
with fractal measure whose dimension depends on the strength of the phototaxis.
Using an effective diffusion approximation for the flow we derive an analytic
expression for the phototactic gain (increase in light exposure over the
aggregate) and by extension an accurate prediction for the fractal dimension
based on the properties of the advection dynamics and the statistics of the
attracting field. This shows that the fractal characteristics of the aggregate
are determined by the non-dimensional ratio of the kinetic energy of swimming
to that of the turbulent flow.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:12:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Torney",
"Colin",
""
],
[
"Neufeld",
"Zoltan",
""
]
] | [
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] |
802.0687 | Thomas Wiegelmann | T. Wiegelmann, B. Inhester | Magnetic modelling and tomography: First steps towards a consistent
reconstruction of the solar corona | 29 pages, 6 figures | Solar Phys.214:287,2003 | 10.1023/A:1024282131117 | null | astro-ph | null | We undertake a first attempt towards a consistent reconstruction of the
coronal magnetic field and the coronal density structure. We consider a
stationary solar corona which has to obey the equations of magnetohydrostatics.
We solve these equations with help of a newly developed optimization scheme. As
a first step we illustrate how tomographic information can be included into the
reconstruction of coronal magnetic fields. In a second step we use coronal
magnetic field information to improve the tomographic inversion process. As
input the scheme requires magnetic field measurements on the photosphere from
vector-magnetographs and the line-of-sight integrated density distribution from
coronagraphs. We test our codes with well known analytic magnetohydrostatic
equilibria and models. The program is planed for use within the STEREO mission.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:19:54 GMT"
}
] | 2009-06-25T00:00:00 | [
[
"Wiegelmann",
"T.",
""
],
[
"Inhester",
"B.",
""
]
] | [
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] |
802.0688 | Marco Valerio Battisti | Marco Valerio Battisti, Giovanni Montani | Quantum cosmology with a minimal length | 8 pages, 3 figures; to appear in the proceedings of the II
Stueckelberg Workshop, Int.J.Mod.Phys.A, references added | Int.J.Mod.Phys.A23:1257-1265,2008 | 10.1142/S0217751X08040184 | null | gr-qc hep-th | null | Quantum cosmology in the presence of a fundamental minimal length is analyzed
in the context of the flat isotropic and the Taub cosmological models. Such
minimal scale comes out from a generalized uncertainty principle and the
quantization is performed in the minisuperspace representation. Both the
quantum Universes are singularity-free and (i) in the isotropic model no
evidences for a Big-Bounce appear; (ii) in the Taub one a quasi-isotropic
configuration for the Universe is predicted by the model.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:08:29 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 13:46:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Battisti",
"Marco Valerio",
""
],
[
"Montani",
"Giovanni",
""
]
] | [
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] |
802.0689 | Fangwen Sun | F.W. Sun, B.H. Liu, C.W. Wong, G.C. Guo | Permutation asymmetry inducing entanglement between degrees of freedom
in multiphoton states | Final version | Phys. Rev. A 78, 015804 (2008) | 10.1103/PhysRevA.78.015804 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We describe and examine entanglement between different degrees of freedom in
multiphoton states based on the permutation properties. From the state
description, the entanglement comes from the permutation asymmetry. According
to the different permutation properties, the multiphoton states can be divided
into several parts. It will help to deal with the multiphoton interference,
which can be used as the measurement of the entanglement.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:17:11 GMT"
},
{
"version": "v2",
"created": "Thu, 31 Jul 2008 15:29:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sun",
"F. W.",
""
],
[
"Liu",
"B. H.",
""
],
[
"Wong",
"C. W.",
""
],
[
"Guo",
"G. C.",
""
]
] | [
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] |
802.069 | Pavel Bleher | Pavel Bleher and Karl Liechty | Exact solution of the six-vertex model with domain wall boundary
condition. Critical line between ferroelectric and disordered phases | 22 pages, 6 figures, to appear in the Journal of Statistical Physics | null | 10.1007/s10955-009-9688-2 | null | math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This is a continuation of the papers [4] of Bleher and Fokin and [5] of
Bleher and Liechty, in which the large $n$ asymptotics is obtained for the
partition function $Z_n$ of the six-vertex model with domain wall boundary
conditions in the disordered and ferroelectric phases, respectively. In the
present paper we obtain the large $n$ asymptotics of $Z_n$ on the critical line
between these two phases.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:31:07 GMT"
},
{
"version": "v2",
"created": "Thu, 26 Jun 2008 15:16:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bleher",
"Pavel",
""
],
[
"Liechty",
"Karl",
""
]
] | [
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] |
802.0691 | Betsabe Blas | Betsab\'e G. Blas Achic, M\^onica C. Sandoval and Olga Satomi Yoshida | Homoscedastic controlled calibration model | LaTex, 21 pages. Includes 13 tables. Version published in Journal of
Chemometrics, v. 21, p. 145-155, 2007 | Journal of Chemometrics, v. 21, p. 145-155, 2007 | null | null | stat.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In the context of the usual calibration model, we consider the case in which
the independent variable is unobservable, but a pre-fixed value on its
surrogate is available. Thus, considering controlled variables and assuming
that the measurement errors have equal variances we propose a new calibration
model. Likelihood based methodology is used to estimate the model parameters
and the Fisher information matrix is used to construct a confidence interval
for the unknown value of the regressor variable. A simulation study is carried
out to asses the effect of the measurement error on the estimation of the
parameter of interest. This new approach is illustrated with an example.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:44:45 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Achic",
"Betsabé G. Blas",
""
],
[
"Sandoval",
"Mônica C.",
""
],
[
"Yoshida",
"Olga Satomi",
""
]
] | [
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802.0692 | Gabriel Navarro | Pascual Jara, Luis Merino, Gabriel Navarro and Juan Francisco Ru\'iz | Prime path coalgebras | 14 pages | null | null | null | math.RA math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We use prime coalgebras as a generalization of simple coalgebras, and observe
that prime subcoalgebras represent the structure of the coalgebra in a more
efficient way than simple coalgebras. In particular, in this work we focus our
attention on the study and characterization of prime subcoalgebras of path
coalgebras of quivers and, by extension, of prime pointed coalgebras.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:53:51 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Jara",
"Pascual",
""
],
[
"Merino",
"Luis",
""
],
[
"Navarro",
"Gabriel",
""
],
[
"Ruíz",
"Juan Francisco",
""
]
] | [
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802.0693 | M. Polletta | M. Polletta (IAP, France & INAF-IASF Milano, Italy) | Black hole growth and stellar assembly at high-z | A&A Letters accepted | null | 10.1051/0004-6361:20079200 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Context. Observations indicate a strong link between star formation and black
hole (BH) growth, but some questions remain unanswered: whether both activities
are coeval or whether one precedes the other, what their characteristic
timescales are, and what kinds of physical processes are responsible for this
interplay.
Aims. We examine stellar and BH masses (M_star and M_BH) in z~2 active
systems at the peak of their AGN or star formation activity to investigate how
they are linked and whether AGN radiative or else radio power provides a
feedback mechanism that regulates the stellar growth in these systems.
Methods. We analyze the infrared (IR) spectral energy distributions of radio,
sub-millimeter and mid-IR selected AGNs at z~1-3 and constrain their stellar
and AGN luminosities using AGN and host-galaxy templates.
Results. We find evidence of increasing stellar light, thereby decreasing the
AGN mid-IR power going from mid-IR selected AGNs, to radio galaxies, and to
sub-millimeter AGNs. This trend can be explained by either decreasing Eddington
ratios or increasing offsets from the local M_BH-M_star relation. All systems
are characterized by high star formation rates regardless of their different
AGN powers, thus neither AGN radiative power nor AGN-driven radio activity
seems to influence the star formation rate in the selected AGNs. We discuss two
possible evolutionary scenarios that might link these three AGN classes.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:56:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Polletta",
"M.",
"",
"IAP, France & INAF-IASF Milano, Italy"
]
] | [
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] |
802.0694 | Ivan Savov | Ivan Savov | Distributed Compression and Squashed Entanglement | M.Sc thesis submitted to the Physics department of McGill University,
107 pages, 14 figures | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A single quantum state can be shared by many distant parties. In this thesis,
we try to characterize the information contents of such distributed states by
defining the multiparty information and the multiparty squashed entanglement,
two steps toward a general theory of multiparty quantum information. As a
further step in that direction, we partially solve the multiparty distributed
compression problem where multiple parties use quantum communication to
faithfully transfer their shares of a state to a common receiver. We build a
protocol for multiparty distributed compression based on the fully quantum
Slepian-Wolf protocol and prove both inner and outer bounds on the achievable
rate region. We relate our findings to previous results in information theory
and discuss some possible applications.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 18:59:45 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Savov",
"Ivan",
""
]
] | [
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802.0695 | Petr Jizba | Petr Jizba and Hagen Kleinert | Superpositions of Probability Distributions | 23 pages, RevTeX, minor changes, accepted to Phys. Rev. E | Phys. Rev. E 78 (2008) 031122 | 10.1103/PhysRevE.78.031122 | null | cond-mat.other cond-mat.stat-mech math-ph math.MP quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Probability distributions which can be obtained from superpositions of
Gaussian distributions of different variances v = \sigma ^2 play a favored role
in quantum theory and financial markets. Such superpositions need not
necessarily obey the Chapman-Kolmogorov semigroup relation for Markovian
processes because they may introduce memory effects. We derive the general form
of the smearing distributions in v which do not destroy the semigroup property.
The smearing technique has two immediate applications. It permits simplifying
the system of Kramers-Moyal equations for smeared and unsmeared conditional
probabilities, and can be conveniently implemented in the path integral
calculus. In many cases, the superposition of path integrals can be evaluated
much easier than the initial path integral. Three simple examples are
presented, and it is shown how the technique is extended to quantum mechanics.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 19:14:12 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Aug 2008 14:59:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jizba",
"Petr",
""
],
[
"Kleinert",
"Hagen",
""
]
] | [
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] |
802.0696 | Giorgio Sonnino | Giorgio Sonnino and Philippe Peeters | Nonlinear Transport Processes in Tokamak Plasmas. Part I: The
Collisional Regimes | 52 pages, 18 figures | null | 10.1063/1.2939377 | ULB-TH/08-02 | physics.plasm-ph physics.flu-dyn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | An application of the thermodynamic field theory (TFT) to transport processes
in L-mode tokamak plasmas is presented. The nonlinear corrections to the linear
(Onsager) transport coefficients in the collisional regimes are derived. A
quite encouraging result is the appearance of an asymmetry between the
Pfirsch-Schlueter (P-S) ion and electron transport coefficients: the latter
presents a nonlinear correction, which is absent for the ions, and makes the
radial electron coefficients much larger than the former. Explicit calculations
and comparisons between the neoclassical results and the TFT predictions for
JET plasmas are also reported. We found that the nonlinear electron P-S
transport coefficients exceed the values provided by neoclassical theory by a
factor, which may be of the order 100. The nonlinear classical coefficients
exceed the neoclassical ones by a factor, which may be of order 2. The
expressions of the ion transport coefficients, determined by the neoclassical
theory in these two regimes, remain unaltered. The low-collisional regimes
i.e., the plateau and the banana regimes, are analyzed in the second part of
this work.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 19:35:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sonnino",
"Giorgio",
""
],
[
"Peeters",
"Philippe",
""
]
] | [
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] |
802.0697 | Andreas Axelsson | Pascal Auscher, Andreas Axelsson, Alan McIntosh | A new approach to solvability of some elliptic pde's with square
integrable boundary data | null | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper has been withdrawn, and is replaced with paper "Solvability of
elliptic systems with square integrable boundary data" by the same authors.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 20:10:20 GMT"
},
{
"version": "v2",
"created": "Mon, 29 Sep 2008 13:31:39 GMT"
}
] | 2008-09-29T00:00:00 | [
[
"Auscher",
"Pascal",
""
],
[
"Axelsson",
"Andreas",
""
],
[
"McIntosh",
"Alan",
""
]
] | [
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] |
802.0698 | Annette Ferguson | Mike Irwin, Annette Ferguson, Avon Huxor, Nial Tanvir, Rodrigo Ibata,
Geraint Lewis | Andromeda XVII: A New Low Luminosity Satellite of M31 | 5 pages, ApJL acccepted | null | 10.1086/587100 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report the discovery of a new dwarf spheroidal galaxy near M31 based on
INT/WFC imaging. The system, Andromeda XVII (And XVII), is located at a
projected radius of ~44 kpc from M31 and has a line-of-sight distance of
794+/-40 kpc measured using the tip of the red giant branch, and therefore lies
well within the halo of M31. The colour of the red giant branch implies a
metallicity of [Fe/H]~-1.9 and we find an absolute magnitude of M_v~ -8.5.
Three globular clusters lie near the main body of And XVII, suggesting a
possible association; if any of these are confirmed, it would make And XVII
exceptionally unusual amongst the faint dSph population. The projected position
on the sky of And XVII strengthens an intriguing alignment apparent in the
satellite system of M31, although with a caveat about biases stemming from the
current area surveyed to significant depth.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 23:55:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Irwin",
"Mike",
""
],
[
"Ferguson",
"Annette",
""
],
[
"Huxor",
"Avon",
""
],
[
"Tanvir",
"Nial",
""
],
[
"Ibata",
"Rodrigo",
""
],
[
"Lewis",
"Geraint",
""
]
] | [
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] |
802.0699 | Massimiliano Esposito | Massimiliano Esposito and Katja Lindenberg | Continuous time random walk for open systems: Fluctuation theorems and
counting statistics | 1 figure ; v2: version accepted in Phys.Rev.E | Phys. Rev. E 77, 051119 (2008) | 10.1103/PhysRevE.77.051119 | null | cond-mat.stat-mech | null | We consider continuous time random walks (CTRW) for open systems that
exchange energy and matter with multiple reservoirs. Each waiting time
distribution (WTD) for times between steps is characterized by a positive
parameter a, which is set to a=1 if it decays at least as fast as t^{-2} at
long times and therefore has a finite first moment. A WTD with a<1 decays as
t^{-a-1}. A fluctuation theorem for the trajectory quantity R, defined as the
logarithm of the ratio of the probability of a trajectory and the probability
of the time reversed trajectory, holds for any CTRW. However, R can be
identified as a trajectory entropy change only if the WTDs have a=1 and satisfy
separability (also called "direction time independence"). For nonseparable WTDs
with a=1, R can only be identified as a trajectory entropy change at long
times, and a fluctuation theorem for the entropy change then only holds at long
times. For WTDs with 0<a<1 no meaningful fluctuation theorem can be derived. We
also show that the (experimentally accessible) n'th moments of the energy and
matter transfers between the system and a given reservoir grow as t^{n a} at
long times.
| [
{
"version": "v1",
"created": "Wed, 6 Feb 2008 00:52:51 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 21:05:20 GMT"
}
] | 2010-03-01T00:00:00 | [
[
"Esposito",
"Massimiliano",
""
],
[
"Lindenberg",
"Katja",
""
]
] | [
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] |
802.07 | Wei Zhang | G.-D. Lin, Wei Zhang, and L.-M. Duan | Characteristics of Bose-Einstein condensation in an optical lattice | 12 pages, 13 figures; Revised version with new figures; Phys. Rev. A
77, 043626 (2008) | Phys. Rev. A 77, 043626 (2008) | 10.1103/PhysRevA.77.043626 | null | cond-mat.supr-con cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss several possible experimental signatures of the Bose-Einstein
condensation (BEC) transition for an ultracold Bose gas in an inhomogeneous
optical lattice. Based on the commonly used time-of-flight imaging technique,
we show that the momentum-space density profile in the first Brillouin zone,
supplemented by the visibility of interference patterns, provides valuable
information about the system. In particular, by crossing the BEC transition
temperature, the appearance of a clear bimodal structure sets a qualitative and
universal signature of this phase transition. Furthermore, the momentum
distribution can also be applied to extract the condensate fraction, which may
serve as a promising thermometer in such a system.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 21:33:02 GMT"
},
{
"version": "v2",
"created": "Wed, 21 May 2008 17:15:53 GMT"
}
] | 2008-05-21T00:00:00 | [
[
"Lin",
"G. -D.",
""
],
[
"Zhang",
"Wei",
""
],
[
"Duan",
"L. -M.",
""
]
] | [
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] |
802.0701 | Andrew Norris | Andrew N. Norris | Acoustic cloaking in 2D and 3D using finite mass | 4 pages, 2 figures | null | null | null | physics.flu-dyn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Fundamental features of rotationally symmetric acoustic cloaks with
anisotropic inertia are derived. Two universal relations are found to connect
the radial and transverse phase speeds and the bulk modulus in the cloak.
Perfect cloaking occurs only if the radial component of the density becomes
infinite at the cloak inner boundary, requiring an infinitely massive cloak. A
practical cloak of finite mass is defined in terms of its effective visible
radius, which vanishes for perfect cloaking. Significant cloaking is obtained
when the effective visible radius is subwavelength, reducing the total
scattering cross section, and may be achieved even as the interior radius of
the cloak is large relative to the wavelength. Both 2D vs. 3D effects are
compared as we illustrate how the spatial dependence of the cloaking parameters
effect the total cross section.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 21:23:29 GMT"
}
] | 2008-02-07T00:00:00 | [
[
"Norris",
"Andrew N.",
""
]
] | [
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802.0702 | Dan Hooper | Dan Hooper and Edward A. Baltz | Strategies for Determining the Nature of Dark Matter | 25 pages, 5 figures, Review intended for the Annual Review of Nuclear
and Particle Science | Ann.Rev.Nucl.Part.Sci.58:293-314,2008 | 10.1146/annurev.nucl.58.110707.171217 | FERMILAB-PUB-08-026-A | hep-ph astro-ph | null | In this review, we discuss the role of the various experimental programs
taking part in the broader effort to identify the particle nature of dark
matter. In particular, we focus on electroweak scale dark matter particles and
discuss a wide range of search strategies being carried out and developed to
detect them. These efforts include direct detection experiments, which attempt
to observe the elastic scattering of dark matter particles with nuclei,
indirect detection experiments, which search for photons, antimatter and
neutrinos produced as a result of dark matter annihilations, and collider
searches for new TeV-scale physics. Each of these techniques could potentially
provide a different and complementary set of information related to the mass,
interactions and distribution of dark matter. Ultimately, it is hoped that
these many different tools will be used together to conclusively identify the
particle or particles that constitute the dark matter of our universe.
| [
{
"version": "v1",
"created": "Tue, 5 Feb 2008 21:27:40 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 17:46:39 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hooper",
"Dan",
""
],
[
"Baltz",
"Edward A.",
""
]
] | [
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