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801.2673 | Silke Weinfurtner | Silke Weinfurtner, Piyush Jain, Matt Visser, C.W. Gardiner | Cosmological particle production in emergent rainbow spacetimes | null | Class.Quant.Grav.26:065012,2009 | 10.1088/0264-9381/26/6/065012 | null | gr-qc | null | We investigate cosmological particle production in spacetimes where Lorentz
invariance emerges in the infrared limit, but is explicitly broken in the
ultraviolet regime. Our specific model focuses on the boost subgroup that
supports CPT invariance and results in a momentum-dependent dispersion
relation. Motivated by previous studies on spacetimes emerging from a
microscopic substrate, we show how these modifications naturally lead to
momentum-dependent rainbow metrics. Firstly, we investigate the possibility of
reproducing cosmological particle production in spacetimes emerging from real
Bose gases. We have studied the influence of non-perturbative ultraviolet
corrections in time-dependent analogue spacetimes, leading to
momentum-dependent emergent rainbow spacetimes. Within certain limits the
analogy is sufficiently good to simulate relativistic quantum field theory in
time-dependent classical backgrounds, and the quantum effects are approximately
robust against the model-dependent modifications. Secondly, we analyze how
significantly the particle production process deviates from the common picture.
While very low-energy modes do not see the difference at all, some modes
"re-enter the Hubble horizon" during the inflationary epoch, and extreme
ultraviolet modes are completely insensitive to the expansion.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 02:40:21 GMT"
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] | 2009-03-27T00:00:00 | [
[
"Weinfurtner",
"Silke",
""
],
[
"Jain",
"Piyush",
""
],
[
"Visser",
"Matt",
""
],
[
"Gardiner",
"C. W.",
""
]
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801.2674 | Dany Vanbeveren | D. Vanbeveren, H. Belkus, J. Van Bever, N. Mennekens | Binary populations and stellar dynamics in young clusters | Contributed paper IAU 250: Massive Stars as Cosmic Engines | null | 10.1017/S1743921308020619 | null | astro-ph | null | We first summarize work that has been done on the effects of binaries on
theoretical population synthesis of stars and stellar phenomena. Next, we
highlight the influence of stellar dynamics in young clusters by discussing a
few candidate UFOs (unconventionally formed objects) like intermediate mass
black holes, Eta Carinae, Zeta Puppis, Gamma Velorum and WR 140.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 13:55:47 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vanbeveren",
"D.",
""
],
[
"Belkus",
"H.",
""
],
[
"Van Bever",
"J.",
""
],
[
"Mennekens",
"N.",
""
]
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801.2675 | Alexey Okulov Yu | A.Yu.Okulov | Angular Momentum of a Photon and Phase Conjugation | 12 pages, 5 figures | J.Phys.B, v.41, 101001(2008). | 10.1088/0953-4075/41/10/101001 | null | nlin.PS cond-mat.soft physics.flu-dyn physics.optics quant-ph | null | Using the concept of an ideal phase-conjugating mirror we demonstrate that
regardless of internal physical mechanism the phase-conjugation of a singular
laser beam is accompanied by excitation within the mirror of internal waves
which carry doubled angular momentum in order to match angular momentum
conservation. For a Brillouin hypersound wavefront-reversal mirror this means
that each elementary optical vortex belonging to a speckle pattern emits an
acoustical vortex wave with doubled topological charge. The exact spatial
profiles of light intensity and the intensity of hypersound in the vicinity of
the phase singularity are obtained. These spiral profiles have a form of double
helix which rotates with the frequency of sound. An optoacoustic experiment is
proposed for visualization of the wavefront reversal of twisted optical beams
and tunable twisted sound generation.
| [
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] | 2015-05-13T00:00:00 | [
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] |
801.2676 | Mark Gieles | M. Gieles (ESO/Santiago) | What determines the mass of the most massive star cluster in a galaxy:
statistics, physics or disruption? | 6 pages, 3 figures, to appear in ``Young Massive Star Clusters -
Initial Conditions and Environments'', 2008, Astrophysics & Space Science,
eds. E. Perez, R. de Grijs, R. M. Gonzalez Delgado | Astrophys.Space Sci.324:299-304,2009 | 10.1007/s10509-009-0102-y | null | astro-ph | null | In many different galactic environments the cluster initial mass function
(CIMF) is well described by a power-law with index -2. This implies a linear
relation between the mass of the most massive cluster (M_max) and the number of
clusters. Assuming a constant cluster formation rate and no disruption of the
most massive clusters it also means that M_max increases linearly with age when
determining M_max in logarithmic age bins. We observe this increase in five out
of the seven galaxies in our sample, suggesting that M_max is determined by the
size of the sample. It also means that massive clusters are very stable against
disruption, in disagreement with the mass independent disruption (MID) model
presented at this conference. For the clusters in M51 and the Antennae galaxies
the size-of-sample prediction breaks down around 10^6 M_sun, suggesting that
this is a physical upper limit to the masses of star clusters in these
galaxies. In this method there is a degeneracy between MID and a CIMF
truncation. We show how the cluster luminosity function can serve as a tool to
distinguish between the two.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 13:57:36 GMT"
},
{
"version": "v2",
"created": "Tue, 26 Feb 2008 14:39:18 GMT"
}
] | 2009-12-04T00:00:00 | [
[
"Gieles",
"M.",
"",
"ESO/Santiago"
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801.2677 | Dr. W. B. Vasantha Kandasamy | W.B.Vasantha Kandasamy, Florentin Smarandache, K. Amal | Super Fuzzy Matrices and Super Fuzzy Models for Social Scientists | 280 pages | Published by InfoLearnQuest, Ann Arbor, United States in 2008 | null | null | math.GM | null | This book introduces the concept of fuzzy super matrices and operations on
them. This book will be highly useful to social scientists who wish to work
with multi-expert models. Super fuzzy models using Fuzzy Cognitive Maps, Fuzzy
Relational Maps, Bidirectional Associative Memories and Fuzzy Associative
Memories are defined here. The authors introduce 13 multi-expert models using
the notion of fuzzy supermatrices. These models are described with illustrative
examples. This book has three chapters. In the first chaper, the basic concepts
about super matrices and fuzzy super matrices are recalled. Chapter two
introduces the notion of fuzzy super matrices adn their properties. The final
chapter introduces many super fuzzy multi expert models.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 13:59:03 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Kandasamy",
"W. B. Vasantha",
""
],
[
"Smarandache",
"Florentin",
""
],
[
"Amal",
"K.",
""
]
] | [
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-0.0271766447,
-0.13585563,
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] |
801.2678 | Scipio Cuccagna | Scipio Cuccagna | On asymptotic stability in 3D of kinks for the $\phi ^4$ model | To appear on Transactions of the American Mathematical Society | null | null | null | math.AP | null | We add to a kink, which is a 1 dimensional structure, two transversal
directions. We then check its asymptotic stability with respect to compactly
supported perturbations in 3D and a time evolution under a Nonlinear Wave
Equation (NLW). The problem is inspired by work by Jack Xin on asymptotic
stability in dimension larger than 1 of fronts for reaction diffusion
equations. The proof involves a separation of variables. The transversal
variables are treated as in work on Nonlinear Klein Gordon Equation (NLKG)
originating from Klainerman and from Shatah in a particular elaboration due to
Delort and others. The longitudinal variable is treated by means of a result by
Weder on dispersion for Schroedinger operators in 1D.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:00:38 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Cuccagna",
"Scipio",
""
]
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] |
801.2679 | Riccardo Faccini | Riccardo Faccini | Heavy Quarkonium Spectroscopy | 7 pages, 9 postscript figures, contributed to the Proceedings of
Lepton-Photon 2007 | null | null | BaBar-CONF-07/35 | hep-ex | null | This paper reviews the experimental status of the Heavy Quarkonium
Spectroscopy and highlights the measurements that hint at the existence of a
new form of quark and gluon aggregation beyond the mesons and the baryons.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:04:37 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Faccini",
"Riccardo",
""
]
] | [
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] |
801.268 | Thomas Gehrmann | A. Gehrmann-De Ridder, T. Gehrmann, E.W.N. Glover, G. Heinrich | Event shapes in $e^+e^-$ annhilation at NNLO | 6 pages, contribution to the Proceedings of RADCOR07, Florence | PoS RADCOR2007:048,2007 | null | ZU-TH 02/08, IPPP/08/02 | hep-ph | null | We report first results on the calculation of NNLO corrections to event shape
distributions in electron-positron annhilation. The corrections are sizeable
for all variables, however their magnitude is substantially different for
different observables. We observe that inclusion of the NNLO corrections yields
a considerably better agreement between theory and experimental data both in
shape and normalisation of the event shape distributions.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:05:14 GMT"
}
] | 2008-12-30T00:00:00 | [
[
"Ridder",
"A. Gehrmann-De",
""
],
[
"Gehrmann",
"T.",
""
],
[
"Glover",
"E. W. N.",
""
],
[
"Heinrich",
"G.",
""
]
] | [
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] |
801.2681 | Dr. W. B. Vasantha Kandasamy | W.B. Vasantha Kandasamy, Florentin Smarandache | New Classes of Codes for Cryptologists and Computer Scientists | 206 pages | Published by InfoLearnQuest, Ann Arbor, United States in 2008 | null | null | math.GM | null | In this book, we have introduced several new classes of codes to aid
cryptologists and computer scientists. We have explained these codes very
non-technically so that a strong mathematical foundation is not needed to
understand them. This book also provides an easy method to detect and correct
errors that occur during transmission. Further, some of the codes are
constructed so as to mislead an intruder/ hacker. False n-codes, whole n-codes
can serve this pupose. These codes can be used to ensure security in networks
and safe transmission of identity. We have named a few new classes of codes
after Periyar, the south-Indian social leader, to mark his services to
humanity. This book is divided into three chapters. Chapter one is introductory
in nature. The notion of bicodes and their generalization, and n-codes are
introduced in the second chapter. Periyar linear codes are introduced in the
third chapter. We have used two methods, viz. pseudo best n-approximations and
n-coset leader properties to detect and correct errors.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:14:21 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Kandasamy",
"W. B. Vasantha",
""
],
[
"Smarandache",
"Florentin",
""
]
] | [
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] |
801.2682 | Fabian Stoeckli | Charalampos Anastasiou, Guenther Dissertori, Fabian Stoeckli, Bryan R.
Webber | QCD radiation effects on the H->WW->l nu l nu signal at the LHC | 16 pages, 14 figures, added references, results update | JHEP0803:017,2008 | 10.1088/1126-6708/2008/03/017 | null | hep-ph | null | The discovery of a Standard Model Higgs boson is possible when experimental
cuts are applied which increase the ratio of signal and background
cross-sections. In this paper we study the pp->H->WW signal cross-section at
the LHC which requires a selection of Higgs bosons with small transverse
momentum. We compare predictions for the efficiency of the experimental cuts
from a NNLO QCD calculation, a calculation of the resummation of logarithms in
the transverse momentum of the Higgs boson at NNLL, and the event generator
MC@NLO. We also investigate the impact of various jet-algorithms, the
underlying event and hadronization on the signal cross-section.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:31:59 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 11:10:43 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Anastasiou",
"Charalampos",
""
],
[
"Dissertori",
"Guenther",
""
],
[
"Stoeckli",
"Fabian",
""
],
[
"Webber",
"Bryan R.",
""
]
] | [
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] |
801.2683 | Adrian Staicu | A. Staicu, G. Manukyan, and F. Mugele | Microscopic structure of electrowetting-driven transitions on
superhydrophobic surfaces | 9 pages, 5 figures | null | null | null | physics.flu-dyn | null | We investigate directly at the microscale the morphology of the
electrowetting induced transition between the Cassie-Baxter and Wenzel states
for a water droplet on a superhydrophobic surface. Our experiments demonstrate
that the transition originates in a very narrow annular region near the
macroscopic contact line, which is first invaded by water and causes a thin
film of air to be entrapped below. At high applied voltages, a growing fraction
of microscopic air-pockets collapse, resulting in a partialWenzel state.
Modulations in the intensity of the light reflected from individual
micro-menisci clarify that the local contact angles near the filling transition
are close to the usual advancing values for contact lines on smooth surfaces.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:35:24 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Staicu",
"A.",
""
],
[
"Manukyan",
"G.",
""
],
[
"Mugele",
"F.",
""
]
] | [
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] |
801.2684 | Paolo Tanga | P. Tanga (OCA), M. Delbo (OCA, Inaf-Osservatorio Astronomico Di
Torino) | Asteroid occultations today and tomorrow: toward the GAIA era | null | Astron.Astrophys.474:1015-1022,2007 | 10.1051/0004-6361:20077470 | null | astro-ph | null | Context: Observation of star occultations is a powerful tool to determine
shapes and sizes of asteroids. This is key information necessary for studying
the evolution of the asteroid belt and to calibrate indirect methods of size
determination, such as the models used to analyze thermal infrared
observations. Up to now, the observation of asteroid occultations is an
activity essentially secured by amateur astronomers equipped with small,
portable equipments. However, the accuracy of the available ephemeris prevents
accurate predictions of the occultation events for objects smaller than ~100
km. Aims: We investigate current limits in predictability and observability of
asteroid occultations, and we study their possible evolution in the future,
when high accuracy asteroid orbits and star positions (such as those expected
from the mission Gaia of the European Space Agency) will be available. Methods:
We use a simple model for asteroid ephemeris uncertainties and numerical
algorithms for estimating the limits imposed by the instruments, assuming
realistic CCD performances and asteroid size distribution, to estimate the
expected occultation rate under different conditions. Results: We show that
high accuracy ephemerides which will be available in the future will extend
toward much smaller asteroids the possibility of observing asteroid
occultations, greatly increasing the number of events and objects involved. A
complete set of size measurements down to ~10 km main belt asteroids could be
obtained in a few years, provided that a small network of ground-based 1m
telescopes are devoted to occultation studies.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:38:49 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Tanga",
"P.",
"",
"OCA"
],
[
"Delbo",
"M.",
"",
"OCA, Inaf-Osservatorio Astronomico Di\n Torino"
]
] | [
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] |
801.2685 | Paolo Tanga | Jean-Fran\c{c}ois Consigli (OCA), Paolo Tanga (OCA), Carlo Comito
(OCA), Daniel Hestroffer (IMCCE), Derek C. Richardson | Formes d'ast\'ero\"ides et formation de satellites : r\^ole de la
r\'eaccumulation gravitationnelle | null | Comptes Rendus Physique 8:469-480, 2007 | 10.1016/j.crhy.2007.02.006 | null | astro-ph physics.geo-ph | null | Asteroid shapes and satellites: role of gravitational reaccumulation.
Following current evidences, it is widely accepted that many asteroids would be
"gravitational aggregates", i.e. bodies lacking internal cohesion. They could
mainly be originated during the catastrophic disruption of some parent bodies,
through the gravitational reaccumulation of the resulting fragments. The same
events produced the dynamical families that we observe. In this work we address
the problem of the origin of shapes of gravitational aggregates, that could
contain signatures of their origin. We use a N-body code to simulate the
collapse of a cloud of fragments, with a variety of initial velocity
distributions and total angular momentum. The fragments are treated as
inhelastic spheres, that rapidly accumulate to form rotating aggregates. The
resulting shapes and rotational properties are compared with theoretical
predictions. The results show that only a precise category of shapes (flattened
spheroids) are created via this mechanism. This may provide interesting
constraints on the evolution of asteroid shapes, in particular for those with
one or more satellites.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:42:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Consigli",
"Jean-François",
"",
"OCA"
],
[
"Tanga",
"Paolo",
"",
"OCA"
],
[
"Comito",
"Carlo",
"",
"OCA"
],
[
"Hestroffer",
"Daniel",
"",
"IMCCE"
],
[
"Richardson",
"Derek C.",
""
]
] | [
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] |
801.2686 | Andrei Smilga | A.V. Smilga | Crypto-Hermiticity of nonanticommutative theories | 9 pages, 1 figure. Invited contribution to the Proceedings of the
International Workshop on Supersymmetry and Quantum Symmetries, Dubna, July
30 - August 4, 2007. SQS07 | null | null | null | hep-th | null | We note that, though nonanticommutative deformations of Minkowski
supersymmetric theories do not respect the reality condition and seem to lead
to non-Hermitian Hamiltonians H, the latter belong to the class of
crypto-Hermitian (or quasi-Hermitian) Hamiltonians having attracted recently a
considerable attention.
They can be made manifestly Hermitian via the similarity transformation H ->
e^R H e^{-R} with a properly chosen R. The deformed model enjoys the same
supersymmetry algebra as the undeformed one though it is difficult in some
cases to write explicit expressions for a half of supercharges. The deformed
SQM models make perfect sense. It is not clear whether it is also the case for
NAC Minkowski field theories -- the conventionally defined S--matrix is not
unitary there.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:45:38 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Smilga",
"A. V.",
""
]
] | [
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] |
801.2687 | Denis Dujmic | D. Dujmic, S. Ahlen, P. Fisher, S. Henderson, A. Kaboth, G. Kohse, R.
Lanza, M. Lewandowska, J. Monroe, A. Roccaro, G. Sciolla, N. Skvorodnev, H.
Tomita, R. Vanderspek, H. Wellenstein, R. Yamamoto | Improved measurement of the head-tail effect in nuclear recoils | Contributed to the International Conference on Topics in
Astroparticle and Underground Physics (TAUP) 2007, Sendai, Japan (3 pages, 4
figures) | J.Phys.Conf.Ser.120:042030,2008 | 10.1088/1742-6596/120/4/042030 | null | astro-ph | null | We present new results with a prototype detector that is being developed by
the DMTPC collaboration for the measurement of the direction tag (head-tail) of
dark matter wind. We use neutrons from a Cf-252 source to create low-momentum
nuclear recoils in elastic scattering with the residual gas nuclei. The recoil
track is imaged in low-pressure time-projection chamber with optical readout.
We measure the ionization rate along the recoil trajectory, which allows us to
determine the direction tag of the incoming neutrons.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:46:57 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Dujmic",
"D.",
""
],
[
"Ahlen",
"S.",
""
],
[
"Fisher",
"P.",
""
],
[
"Henderson",
"S.",
""
],
[
"Kaboth",
"A.",
""
],
[
"Kohse",
"G.",
""
],
[
"Lanza",
"R.",
""
],
[
"Lewandowska",
"M.",
""
],
[
"Monroe",
"J.",
""
],
[
"Roccaro",
"A.",
""
],
[
"Sciolla",
"G.",
""
],
[
"Skvorodnev",
"N.",
""
],
[
"Tomita",
"H.",
""
],
[
"Vanderspek",
"R.",
""
],
[
"Wellenstein",
"H.",
""
],
[
"Yamamoto",
"R.",
""
]
] | [
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801.2688 | Shao-Feng Wu | Shao-Feng Wu, Bin Wang, Guo-Hong Yang, Peng-Ming Zhang | The generalized second law of thermodynamics in generalized gravity
theories | 19 pages, no figure, mistakes corrected, references added, to appear
in Class. Quantum Grav | Class.Quant.Grav.25:235018,2008 | 10.1088/0264-9381/25/23/235018 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the generalized second law of thermodynamics (GSL) in
generalized theories of gravity. We examine the total entropy evolution with
time including the horizon entropy, the non-equilibrium entropy production, and
the entropy of all matter, field and energy components. We derive a universal
condition to protect the generalized second law and study its validity in
different gravity theories. In Einstein gravity, (even in the phantom-dominated
universe with a Schwarzschild black hole), Lovelock gravity, and braneworld
gravity, we show that the condition to keep the GSL can always be satisfied. In
$f(R)$ gravity and scalar-tensor gravity, the condition to protect the GSL can
also hold because the gravity is always attractive and the effective Newton
constant should be approximate constant satisfying the experimental bounds.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:49:25 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Apr 2008 09:04:06 GMT"
},
{
"version": "v3",
"created": "Tue, 13 May 2008 00:52:55 GMT"
},
{
"version": "v4",
"created": "Tue, 7 Oct 2008 05:49:36 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Wu",
"Shao-Feng",
""
],
[
"Wang",
"Bin",
""
],
[
"Yang",
"Guo-Hong",
""
],
[
"Zhang",
"Peng-Ming",
""
]
] | [
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] |
801.2689 | Diego Paz\'o | Diego Paz\'o and Ernesto M. Nicola | Breaking chirality in nonequilibrium systems on the lattice | null | Europhys. Lett. 81, 10009 (2008) | 10.1209/0295-5075/81/10009 | null | nlin.PS | null | We study the dynamics of fronts in parametrically forced oscillating
lattices. Using as a prototypical example the discrete Ginzburg-Landau
equation, we show that much information about front bifurcations can be
extracted by projecting onto a cylindrical phase space. Starting from a normal
form that describes the nonequilibrium Ising-Bloch bifurcation in the continuum
and using symmetry arguments, we derive a simple dynamical system that captures
the dynamics of fronts in the lattice. We can expect our approach to be
extended to other pattern-forming problems on lattices.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:53:11 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Pazó",
"Diego",
""
],
[
"Nicola",
"Ernesto M.",
""
]
] | [
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] |
801.269 | Ki-Seng Tan | Ki-Seng Tan | Control Theorems for Abelian Varieties over Function Fields | 13 pages | null | null | null | math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove control theorems for abelian varieties over function fields.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:55:14 GMT"
},
{
"version": "v2",
"created": "Fri, 12 Dec 2008 00:16:51 GMT"
}
] | 2008-12-12T00:00:00 | [
[
"Tan",
"Ki-Seng",
""
]
] | [
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801.2691 | Remy Reche | R\'emy Reche (LAOG), Herv\'e Beust (LAOG), J. C. Augereau (LAOG),
Olivier Absil (LAOG) | On the observability of resonant structures in planetesimal disks due to
planetary migration | 16 pages, 13 figures. Accepted for publication in A&A | null | 10.1051/0004-6361:20077934 | null | astro-ph | null | We present a thorough study of the impact of a migrating planet on a
planetesimal disk, by exploring a broad range of masses and eccentricities for
the planet. We discuss the sensitivity of the structures generated in debris
disks to the basic planet parameters. We perform many N-body numerical
simulations, using the symplectic integrator SWIFT, taking into account the
gravitational influence of the star and the planet on massless test particles.
A constant migration rate is assumed for the planet. The effect of planetary
migration on the trapping of particles in mean motion resonances is found to be
very sensitive to the initial eccentricity of the planet and of the
planetesimals. A planetary eccentricity as low as 0.05 is enough to smear out
all the resonant structures, except for the most massive planets. The
planetesimals also initially have to be on orbits with a mean eccentricity of
less than than 0.1 in order to keep the resonant clumps visible. This numerical
work extends previous analytical studies and provides a collection of disk
images that may help in interpreting the observations of structures in debris
disks. Overall, it shows that stringent conditions must be fulfilled to obtain
observable resonant structures in debris disks. Theoretical models of the
origin of planetary migration will therefore have to explain how planetary
systems remain in a suitable configuration to reproduce the observed
structures.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:57:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Reche",
"Rémy",
"",
"LAOG"
],
[
"Beust",
"Hervé",
"",
"LAOG"
],
[
"Augereau",
"J. C.",
"",
"LAOG"
],
[
"Absil",
"Olivier",
"",
"LAOG"
]
] | [
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] |
801.2692 | Syksy Rasanen | Syksy Rasanen | Evaluating backreaction with the peak model of structure formation | 49 pages, 6 figures. v2: Added clarifications and references. v3:
Published version. Corrected typos | JCAP 0804:026,2008 | 10.1088/1475-7516/2008/04/026 | null | astro-ph gr-qc | null | We evaluate the average expansion rate of a universe which contains a
realistic evolving ensemble of non-linear structures. We use the peak model of
structure formation to obtain the number density of structures, and take the
individual structures to be spherical. The expansion rate increases relative to
the FRW value on a timescale of 10-100 billion years, because the universe
becomes dominated by fast-expanding voids. However, the increase is not rapid
enough to correspond to acceleration. We discuss how to improve our treatment.
We also consider various qualitative issues related to backreaction.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:18:22 GMT"
},
{
"version": "v2",
"created": "Thu, 31 Jan 2008 19:23:53 GMT"
},
{
"version": "v3",
"created": "Fri, 18 Apr 2008 14:21:41 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Rasanen",
"Syksy",
""
]
] | [
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] |
801.2693 | Hagen Neidhardt Dr | Horia Cornean, Kurt Hoke, Hagen Neidhardt, Paul N. Racec, Joachim
Rehberg | A Kohn-Sham system at zero temperature | 27 pages | J. Phys. A: Math. Theor. 41 385304 (2008) | 10.1088/1751-8113/41/38/385304 | WIAS Preprint 1293 | math-ph math.MP | null | An one-dimensional Kohn-Sham system for spin particles is considered which
effectively describes semiconductor {nano}structures and which is investigated
at zero temperature. We prove the existence of solutions and derive a priori
estimates. For this purpose we find estimates for eigenvalues of the
Schr\"odinger operator with effective Kohn-Sham potential and obtain
$W^{1,2}$-bounds of the associated particle density operator. Afterwards,
compactness and continuity results allow to apply Schauder's fixed point
theorem. In case of vanishing exchange-correlation potential uniqueness is
shown by monotonicity arguments. Finally, we investigate the behavior of the
system if the temperature approaches zero.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 14:59:12 GMT"
}
] | 2009-01-13T00:00:00 | [
[
"Cornean",
"Horia",
""
],
[
"Hoke",
"Kurt",
""
],
[
"Neidhardt",
"Hagen",
""
],
[
"Racec",
"Paul N.",
""
],
[
"Rehberg",
"Joachim",
""
]
] | [
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801.2694 | Fabien Malbet | F. Malbet (LAOG), D. Buscher (MRAO), G. Weigelt, P. Garcia (CAUP), M.
Gai (OATo), D. Lorenzetti (OAR), J. Surdej (IAGL), J. Hron (IfAW), R.
Neuh\"auser (AIU), P. Kern (LAOG), L. Jocou (LAOG), J.-P. Berger (LAOG), O.
Absil (LAOG), U. Beckmann, L. Corcione (OATo), G. Duvert (LAOG, JMMC), M.
Filho (CAUP), P. Labeye (LETI), E. Le Coarer (LAOG), G. Li Causi (OAR), J.
Lima (FCUL), K. Perraut (LAOG), E. Tatulli (LAOG, JMMC, Oaa), E. Thi\'ebaut
(CRAL), J. Young (MRAO), G. Zins (LAOG), A. Amorim (FCUL), B. Aringer (IfAW),
T. Beckert, M. Benisty (LAOG), X. Bonfils (FCUL), A. Chelli (LAOG, JMMC), O.
Chesneau (LG), A. Chiavassa (GRAAL), R. Corradi (IAC), M. De Becker (IAGL),
A. Delboulb\'e (LAOG), G. Duch\^ene (LAOG), T. Forveille (LAOG), C. Haniff
(MRAO), E. Herwats (LAOG, Iagl), J.-B. Le Bouquin (ESO), S. Ligori (OATo), D.
Loreggia (OAR), A. Marconi (OAA), A. Moitinho (FCUL), B. Nisini (OAR), P.-O.
Petrucci (LAOG), J. Rebordao (INETI), R. Speziali (OAR), L. Testi (OAA, ESO),
F. Vitali (OAR) | Milli-arcsecond astrophysics with VSI, the VLTI spectro-imager in the
ELT era | 8 pages. To be published in the proceedings of the ESO workshop
"Science with the VLT in the ELT Era", held in Garching (Germany) on 8-12
October 2007, A. Moorwood editor | null | 10.1007/978-1-4020-9190-2_57 | null | astro-ph | null | Nowadays, compact sources like surfaces of nearby stars, circumstellar
environments of stars from early stages to the most evolved ones and
surroundings of active galactic nuclei can be investigated at milli-arcsecond
scales only with the VLT in its interferometric mode. We propose a
spectro-imager, named VSI (VLTI spectro-imager), which is capable to probe
these sources both over spatial and spectral scales in the near-infrared
domain. This instrument will provide information complementary to what is
obtained at the same time with ALMA at different wavelengths and the extreme
large telescopes.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:01:50 GMT"
}
] | 2009-11-13T00:00:00 | [
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"",
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[
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"P.",
"",
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"M.",
"",
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[
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"D.",
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[
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"J.",
"",
"IAGL"
],
[
"Hron",
"J.",
"",
"IfAW"
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[
"Neuhäuser",
"R.",
"",
"AIU"
],
[
"Kern",
"P.",
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"Jocou",
"L.",
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[
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] |
801.2695 | Levente Molnar | D. Di Bari, A. Mastroserio, L. Molnar, E. Nappi, D. Perrino, G. Volpe | Contribution of the HMPID detector to the high-pT physics at LHC | 6 pages, 7 figures, Contribution to QCD @ Work 2007: International
Workshop on Quantum Chromodynamics Theory and Experiment, Martina Franca,
Italy, 16-20 June 2007 | AIPConf.Proc.964:218-223,2007 | 10.1063/1.2823853 | null | nucl-ex | null | The LHC will deliver unexplored energy regimes for proton-proton and
heavy-ion collisions. As shown by the RHIC experiments, particle identification
over a large momentum range is essential to disentangle physics processes,
especially in the intermediate p$_T$ (1 $<p_{T}<5$ GeV/c) region. The novel
design of the High-Momentum Particle Identification Detector (HMPID), based on
large surface CsI photocathodes, is able to identify $\pi^{\pm}$, $K^{\pm}$,
$p$ and $\bar{p}$ in the momentum region where bulk medium properties and hard
scatterings interplay. Furthermore, measurement of resonance particles such as
the $\phi \to K^+K^-$ could provide information on the system evolution. The
HMPID layout and segmentation are optimized to study particle correlations at
high momenta describing the early phase and the dynamical evolution of the
collision. At LHC, the increased hard cross section will significantly be
enhanced compared to RHIC. Jet reconstruction via Deterministic Annealing can
address jet quenching and detailed measurements of jet properties. In this
paper, we present these selected topics from the possible HMPID contributions
to the physics goals of LHC.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:15:43 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Di Bari",
"D.",
""
],
[
"Mastroserio",
"A.",
""
],
[
"Molnar",
"L.",
""
],
[
"Nappi",
"E.",
""
],
[
"Perrino",
"D.",
""
],
[
"Volpe",
"G.",
""
]
] | [
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] |
801.2696 | Mark V. Kartsovnik | D. Andres, M. V. Kartsovnik, W. Biberacher, K. Neumaier, I. Sheikin,
and H. Mueller | Field-induced charge-density-wave transitions in the organic metal
$\alpha$-(BEDT-TTF)$_2$KHg(SCN)$_4$ under hydrostatic pressure | 18 pages, 13 figures | Low Temp. Phys. 37, 959 (2011) | null | null | cond-mat.str-el | null | Successive magnetic-field-induced charge-density-wave transitions in the
molecular conductor $\alpha$-(BEDT-TTF)$_2$KHg(SCN)$_4$ are studied in the
hydrostatic pressure regime, in which the zero field charge-density wave
(CDW)state is completely suppressed. The orbital effect of the magnetic field
is demonstrated to restore the density wave, while the orbital quantization
induces different CDW states in different field intervals. In particular, we
have found that at certain field orientations the hysteretic first order
transitions between field-induced CDW subphases become visible at much higher
temperatures. This observation is very well in line with the existing theories
of field-induced CDW transitions.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:03:38 GMT"
}
] | 2018-01-09T00:00:00 | [
[
"Andres",
"D.",
""
],
[
"Kartsovnik",
"M. V.",
""
],
[
"Biberacher",
"W.",
""
],
[
"Neumaier",
"K.",
""
],
[
"Sheikin",
"I.",
""
],
[
"Mueller",
"H.",
""
]
] | [
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] |
801.2697 | Christian Fischer | Christian Kellermann and Christian S. Fischer | The running coupling from the four-gluon vertex in Landau gauge
Yang-Mills theory | 25 pages, 4 figures; v2: minor clarifications added and typos
corrected, version accepted by PRD | Phys.Rev.D78:025015,2008 | 10.1103/PhysRevD.78.025015 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider the running coupling from the four-gluon vertex in Landau gauge,
SU($N_c$) Yang-Mills theory as given by a combination of dressing functions of
the vertex and the gluon propagator. We determine these functions numerically
from a coupled set of Dyson-Schwinger equations. We reproduce asymptotic
freedom in the ultraviolet momentum region and find a coupling of order one at
mid-momenta. In the infrared we find a nontrivial (i.e. nonzero) fixed point
which is three orders of magnitude smaller than the corresponding fixed point
in the coupling of the ghost-gluon vertex. This result explains why the
Dyson-Schwinger and the functional renormalization group equations for the two
point functions can agree in the infrared, although their structure is quite
different. Our findings also support Zwanziger's notion of an infrared
effective theory driven by the Faddeev-Popov determinant.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:17:48 GMT"
},
{
"version": "v2",
"created": "Wed, 25 Jun 2008 15:08:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kellermann",
"Christian",
""
],
[
"Fischer",
"Christian S.",
""
]
] | [
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] |
801.2698 | Dominique Sluse | D. Sluse (1), J.-F. Claeskens (2), D. Hutsem\'ekers (2) and J. Surdej
(2) (1- Ecole Polytechnique F\'ed\'erale de Lausanne EPFL, Switzerland; 2-
Liege University, Belgium) | Microlensing probes the AGN structure of the lensed quasar J1131-1231 | 3 pages, To appear in "The Nuclear Region, Host Galaxy and
Environment of Active Galaxies" (RevMexAA - Conference Series) | null | null | null | astro-ph | null | We present the analysis of single epoch long slit spectra of the three
brightest images of the gravitationally lensed system J1131-1231. These spectra
provide one of the clearest observational evidence for differential
micro-lensing of broad emission lines (BELs) in a gravitationally lensed
quasar. The micro-lensing effect enables us: (1) to confirm that the width of
the emission lines is anti-correlated to the size of the emitting region; (2)
to show that the bulk of FeII is emitted in the outer parts of the Broad Line
Region (BLR) while another fraction of FeII is produced in a compact region;
(3) to derive interesting informations on the origin of the narrow intrinsic
MgII absorption doublet observed in that system.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:10:53 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Sluse",
"D.",
""
],
[
"Claeskens",
"J. -F.",
""
],
[
"Hutsemékers",
"D.",
""
],
[
"Surdej",
"J.",
""
]
] | [
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] |
801.2699 | Erik Koop | E.J. Koop, B.J. van Wees, D. Reuter, A.D. Wieck, C.H. van der Wal | Spin Accumulation and Spin Relaxation in a Large Open Quantum Dot | 4 pages, 4 figures | Phys. Rev. Lett 101, 056602 (2008) | 10.1103/PhysRevLett.101.056602 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report electronic control and measurement of an imbalance between spin-up
and spin-down electrons in micron-scale open quantum dots. Spin injection and
detection was achieved with quantum point contacts tuned to have spin-selective
transport, with four contacts per dot for realizing a non-local spin-valve
circuit. This provides an interesting system for studies of spintronic effects
since the contacts to reservoirs can be controlled and characterized with high
accuracy. We show how this can be used to extract in a single measurement the
relaxation time for electron spins inside the dot ~ 300 ps and the degree of
spin polarization of the contacts P ~ 0.8.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:05:32 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Aug 2008 17:24:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Koop",
"E. J.",
""
],
[
"van Wees",
"B. J.",
""
],
[
"Reuter",
"D.",
""
],
[
"Wieck",
"A. D.",
""
],
[
"van der Wal",
"C. H.",
""
]
] | [
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] |
801.27 | Amelia Sparavigna | Amelia Sparavigna | Labels discover physics: the development of new labelling methods as a
promising research field for applied physics | 16 pages, 9 fihures | null | null | null | physics.pop-ph physics.soc-ph | null | Labels and tags are accompanying us in almost each moment of our life and
everywhere we are going, in the form of electronic keys or money, or simply as
labels on products we are buying in shops and markets. The label diffusion,
rapidly increasing for logistic reasons in the actual global market, carries
huge amount of information but it is demanding security and anti-fraud systems.
The first crucial point, for the consumer and producer safety, is to ensure the
authenticity of the labelled products with systems against counterfeiting and
piracy. Recent anti-fraud techniques are based on a sophisticated use of
physical effects, from holograms till magnetic resonance or tunnel transitions
between atomic sublevels. In this paper we will discuss labels and anti-fraud
technologies as a new and very promising research field for applied physics.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:12:37 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Sparavigna",
"Amelia",
""
]
] | [
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] |
801.2701 | Yadin Y. Goldschmidt | Yadin Y. Goldschmidt and Jin-Tao Liu | Observing the Inverse melting of the vortex lattice in
Bi$_2$Sr$_2$CaCu$_2$O$_8$ with point defects using Langevin simulations with
vortex shaking | RevTex 4, 5 figures | null | null | null | cond-mat.supr-con cond-mat.dis-nn | null | Langevin dynamics simulations of the vortex matter in the highly-anisotropic
high-temperature superconductor Bi$_2$Sr$_2$CaCu$_2$O$_8$ were performed. We
introduced point defects as a smoothened distribution of a random potential.
Both the electromagnetic and Josephson interactions among pancake vortices were
included. A special shaking and annealing process was introduced to let the
system approach the equilibrium configuration. We are able to see the inverse
melting transition from the Bragg-glass to the amorphous vortex glass state, in
agreement with recent experiments.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:13:22 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Goldschmidt",
"Yadin Y.",
""
],
[
"Liu",
"Jin-Tao",
""
]
] | [
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] |
801.2702 | Roberto Casalbuoni Prof | Roberto Casalbuoni (Department of Physics, University of Florence,
INFN-Florence and Galileo Galilei Institute, Florence, Italy), Joaquim Gomis
(PH-TH Division, CERN, Geneva, Switzerland, Departament d'Estructura i
Constituents de la Mat\`eria and Institut de Ciencies del Cosmos, Universitat
de Barcelona, Diagonal, Barcelona, Spain), Kiyoshi Kamimura (Department of
Physics, Toho University, Funabashi, Japan) and Giorgio Longhi (Department of
Physics, University of Florence, and INFN-Florence, Italy) | Space-time Vector Supersymmetry and Massive Spinning Particle | 14 pages. Few references and two comments added | JHEP 0802:094,2008 | 10.1088/1126-6708/2008/02/094 | null | hep-th | null | We construct the action of a relativistic spinning particle from a non-linear
realization of a space-time odd vector extension of the Poincar\'e group. For
particular values of the parameters appearing in the lagrangian the model has a
gauge world-line supersymmetry.{As a consequence of this local symmetry there
are BPS solutions in the model preserving 1/5 of the supersymmetries.} A
supersymmetric invariant quantization produces two decoupled 4d Dirac
equations.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:35:25 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Jan 2008 15:51:06 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Casalbuoni",
"Roberto",
"",
"Department of Physics, University of Florence,\n INFN-Florence and Galileo Galilei Institute, Florence, Italy"
],
[
"Gomis",
"Joaquim",
"",
"PH-TH Division, CERN, Geneva, Switzerland, Departament d'Estructura i\n Constituents de la Matèria and Institut de Ciencies del Cosmos, Universitat\n de Barcelona, Diagonal, Barcelona, Spain"
],
[
"Kamimura",
"Kiyoshi",
"",
"Department of\n Physics, Toho University, Funabashi, Japan"
],
[
"Longhi",
"Giorgio",
"",
"Department of\n Physics, University of Florence, and INFN-Florence, Italy"
]
] | [
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] |
801.2703 | Antonio Paulo Baeta Scarpelli | E. W. Dias, A. P. Baeta Scarpelli, L. C. T. Brito, Marcos Sampaio, M.
C. Nemes | Implicit regularization beyond one loop order: gauge field theories | 18 pages, 5 figures, accepted for publication in European Physical
Journal | Eur.Phys.J.C55:667-681,2008 | 10.1140/epjc/s10052-008-0614-6 | null | hep-th | null | We extend a constrained version of Implicit Regularization (CIR) beyond one
loop order for gauge field theories. In this framework, the ultraviolet content
of the model is displayed in terms of momentum loop integrals order by order in
perturbation theory for any Feynman diagram, while the Ward-Slavnov-Taylor
identities are controlled by finite surface terms. To illustrate, we apply CIR
to massless abelian Gauge Field Theories (scalar and spinorial QED) to two loop
order and calculate the two-loop beta-function of the spinorial QED.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:26:19 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Apr 2008 17:54:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Dias",
"E. W.",
""
],
[
"Scarpelli",
"A. P. Baeta",
""
],
[
"Brito",
"L. C. T.",
""
],
[
"Sampaio",
"Marcos",
""
],
[
"Nemes",
"M. C.",
""
]
] | [
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] |
801.2704 | Yuri Janssen | Y. Janssen, K. W. Dennis, R. Prozorov, P. C. Canfield, R. W. McCallum | Exotic (anti)ferromagnetism in single crystals of Pr6Ni2Si3 | 9 pages, 13 figures, submitted to PRB | null | 10.1103/PhysRevB.77.214407 | null | cond-mat.mtrl-sci | null | The ternary intermetallic compound Pr6Ni2Si3, is a member of a structure
series of compounds based on a triangular structure where the number of Pr
atoms in the prism cross section can be systematically varied. Pr6Ni2Si3
contains two distinct Pr lattice sites which result in complex interactions
between the magnetic ions. Extensive measurements of specific heat and
magnetization on single crystal samples indicate that Pr6Ni2Si3 orders with
both a ferromagnet and an antiferromagnet component, with ordering temperatures
of 39.6 K and ~ 32 K, respectively. The ferromagnetic component // c-axis is
accompanied by a large hysteresis, and the antiferromagnetic component,_|_
c-axis is accompanied by a spin-flop-type transition. More detailed
measurements, of the vector magnetization, indicate that the ferromagnetic and
the antiferromagnetic order appear independent of each other. These results not
only clarify the behavior of Pr6Ni2Si3 itself, but also of the other members of
the structure series, Pr5Ni2Si3 and Pr15Ni7Si10.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:30:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Janssen",
"Y.",
""
],
[
"Dennis",
"K. W.",
""
],
[
"Prozorov",
"R.",
""
],
[
"Canfield",
"P. C.",
""
],
[
"McCallum",
"R. W.",
""
]
] | [
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] |
801.2705 | Paolo Pagano | P. Pagano, J.C. Raymond, F. Reale, S. Orlando | Modeling magnetohydrodynamics and non equilibrium SoHO/UVCS line
emission of CME shocks | 11 pages, 12 figures, 2 appendixes | null | 10.1051/0004-6361:20079088 | null | astro-ph | null | We provide a guideline to interpret the UVCS emission lines (in particular O
VI and Si XII) during shock wave propagation in the outer solar corona. We use
a numerical MHD model performing a set of simulations of shock waves generated
in the corona and from the result we compute the plasma emission for the O VI
and Si XII including the effects of NEI. We analyze the radiative and spectral
properties of our model with the support of a detailed radiation model
including Doppler dimming and an analytical model for shocks, and, finally, we
synthesize the expected O VI 1032A line profile. We explain several spectral
features of the observations like the absence of discontinuities in the O VI
emission during the shock passage, the brightening of Si XII emission and the
width of the lines. We use our model also to give very simple and general
predictions for the strength of the line wings due to the ions shock heating
and on the line shape for Limb CMEs or Halo CMEs. The emission coming from
post-shock region in the solar corona roughly agrees with the emission from a
simple planar and adiabatic shock, but the effect of thermal conduction and the
magnetic field may be important depending on the event parameters. Doppler
dimming significantly influences the O VI emission while Si XII line brightens
mainly because of the shock compression. Significant shock heating is
responsible for the wide and faint component of the O VI line usually observed
which may be taken as a shock signature in the solar corona.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:31:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Pagano",
"P.",
""
],
[
"Raymond",
"J. C.",
""
],
[
"Reale",
"F.",
""
],
[
"Orlando",
"S.",
""
]
] | [
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] |
801.2706 | Alessandro Villar | Katiuscia N. Cassemiro and Alessandro S. Villar | Scalable continuous-variable entanglement of light beams produced by
optical parametric oscillators | null | Phys. Rev. A 77, 022311 (2008) | 10.1103/PhysRevA.77.022311 | null | quant-ph | null | We show that scalable multipartite entanglement among light fields may be
generated by optical parametric oscillators (OPO). The tripartite entanglement
existent among the three bright beams produced by a single OPO -- pump, signal,
and idler -- is scalable to a system of many OPOs by pumping them in cascade
with the same optical field. This latter serves as an entanglement distributor.
The special case of two OPOs is studied, as it is shown that the resulting five
bright beams share genuine multipartite entanglement. In addition, the
structure of entanglement distribution among the fields can be manipulated to
some degree by tuning the incident pump power. The scalability to many fields
is straightforward, allowing an alternative implementation of a multipartite
quantum information network with continuous variables.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:34:26 GMT"
},
{
"version": "v2",
"created": "Tue, 12 Feb 2008 09:34:55 GMT"
}
] | 2008-02-12T00:00:00 | [
[
"Cassemiro",
"Katiuscia N.",
""
],
[
"Villar",
"Alessandro S.",
""
]
] | [
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] |
801.2707 | Thomas Wiegelmann | T. Wiegelmann, J. K. Thalmann, C. J. Schrijver, M. L. Derosa, T. R.
Metcalf | Can We Improve the Preprocessing of Photospheric Vector Magnetograms by
the Inclusion of Chromospheric Observations? | 22 pages, 6 Figure | Bibliographic Code: 2008SoPh..247..249W | 10.1007/s11207-008-9130-y | null | astro-ph | null | The solar magnetic field is key to understanding the physical processes in
the solar atmosphere. Nonlinear force-free codes have been shown to be useful
in extrapolating the coronal field upward from underlying vector boundary data.
However, we can only measure the magnetic field vector routinely with high
accuracy in the photosphere, and unfortunately these data do not fulfill the
force-free condition. We must therefore apply some transformations to these
data before nonlinear force-free extrapolation codes can be self-consistently
applied. To this end, we have developed a minimization procedure that yields a
more chromosphere-like field, using the measured photospheric field vectors as
input. The procedure includes force-free consistency integrals, spatial
smoothing, and -- newly included in the version presented here -- an improved
match to the field direction as inferred from fibrils as can be observed in,
e.g., chromospheric H$\alpha$ images. We test the procedure using a model
active-region field that included buoyancy forces at the photospheric level.
The proposed preprocessing method allows us to approximate the chromospheric
vector field to within a few degrees and the free energy in the coronal field
to within one percent.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:57:31 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Feb 2008 12:28:34 GMT"
}
] | 2008-02-29T00:00:00 | [
[
"Wiegelmann",
"T.",
""
],
[
"Thalmann",
"J. K.",
""
],
[
"Schrijver",
"C. J.",
""
],
[
"Derosa",
"M. L.",
""
],
[
"Metcalf",
"T. R.",
""
]
] | [
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] |
801.2708 | Ioana Bena Dr. | Ioana Bena, Michel Droz, Janusz Szwabinski, Andrzej Pekalski | How bad is to be slow-reacting ? On the effect of the delay in response
to a changing environment on a population's survival | 7 pages, 4 figures | null | null | null | q-bio.PE cond-mat.stat-mech physics.bio-ph | null | We consider a simple-model population, whose individuals react with a certain
delay to temporal variations of their habitat. We investigate the impact of
such a delayed-answer on the survival chances of the population, both in a
periodically changing environment, and in the case of an abrupt change of it.
It is found that for population with low degree of mutation-induced
variability, being "slow-reacting" decreases the extinction risk face to
environmental changes. On the contrary, for populations with high mutation
amplitude, the delayed reaction reduces the survival chances.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:50:41 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Bena",
"Ioana",
""
],
[
"Droz",
"Michel",
""
],
[
"Szwabinski",
"Janusz",
""
],
[
"Pekalski",
"Andrzej",
""
]
] | [
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] |
801.2709 | Yuri Yermolaev | Yu. I. Yermolaev | Comment on "Geoeffectiveness of halo coronal mass ejections" by N.
Gopalswamy, S. Yashiro, and S. Akiyama | null | Cosmic Research, 2008, Vol. 46, No. 6, pp. 540-541. | 10.1134/S0010952508060099 | null | physics.space-ph physics.geo-ph | null | Comment on paper: Gopalswamy, N., S. Yashiro, and S. Akiyama (2007),
Geoeffectiveness of halo coronal mass ejections, J. Geophys. Res., 112, A06112,
doi:10.1029/2006JA012149
Gopalswamy et al. [2007] studied the geoeffectiveness of halo coronal mass
ejections (CMEs) on the basis of solar observations during 1996-2005 and found
that the geoeffectiveness of 229 frontside halo CMEs was 71%. Recently for
observations of 305 frontside halo CMEs during 1997-2003 the geoeffectiveness
was found to be 40% [Kim et al., 2005]. Complex analysis of both solar and
interplanetary measurements showed that the geoeffectiveness of frontside halo
CMEs is likely to be about 50% [Yermolaev et al., 2005; Yermolaev and
Yermolaev, 2006]. Gopalswamy et al. [2007] did not discuss possible causes of
this difference and were limited only to the general words: "The reason for the
conflicting results (geoeffectiveness of CMEs ranging from 35% to more than
80%) may be attributed to the different definition of halo CMEs and
geoeffectiveness." So, here we shall present our point of view on high
geoeffectivenees of CME obtained in paper by Gopalswamy et al. [2007].
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 15:59:16 GMT"
}
] | 2009-04-01T00:00:00 | [
[
"Yermolaev",
"Yu. I.",
""
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] |
801.271 | Sushant Ghosh | S. G.Ghosh and D. W. Deshkar | Horizons of radiating black holes in Einstein gauss-bonnet gravity | 4 pages, RevTeX, Accepted in Physical Review D | Phys.Rev.D77:047504,2008 | 10.1103/PhysRevD.77.047504 | null | gr-qc | null | A Vaidya-based model of a radiating black-hole is studied in a 5-dimensional
Einstein gravity with Gauss-Bonnet contribution of quadratic curvature terms.
The structure and locations of the apparent and event horizons of the radiating
black hole are determined.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:00:27 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ghosh",
"S. G.",
""
],
[
"Deshkar",
"D. W.",
""
]
] | [
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] |
801.2711 | Hendrik Adorf | Hendrik Adorf and Michael Flohr | On Factorization Constraints for Branes in the H3+ Model | v2: version published in IJMPA; remark on possible pitfalls when
doing the analytic continuations added; discussion of AdS2 vs. S2 branes
changed; remarks on the brane spectrum and on the regular branes added; some
typos corrected; Ref. Exton: Publisher added; 50 pages | Int.J.Mod.Phys.A23:3963-4010,2008 | 10.1142/S0217751X08041311 | ITP-UH-02/08 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We comment on the brane solutions for the boundary H3+ model that have been
proposed so far and point out that they should be distinguished according to
the patterns regular/irregular and discrete/continuous. In the literature,
mostly irregular branes have been studied, while results on the regular ones
are rare. For all types of branes, there are questions about how a second
factorization constraint in the form of a b^{-2}/2-shift equation can be
derived. Here, we assume analyticity of the boundary two point function, which
means that the Cardy-Lewellen constraints remain unweakened. This enables us to
derive unambiguously the desired b^{-2}/2-shift equations. They serve as
important additional consistency conditions. For some regular branes, we also
derive 1/2-shift equations that were not known previously. Case by case, we
discuss possible solutions to the enlarged system of constraints. We find that
the well-known irregular continuous AdS_2 branes are consistent with our new
factorization constraint. Furthermore, we establish the existence of a new type
of brane: The shift equations in a certain regular discrete case possess a
non-trivial solution that we write down explicitly. All other types are found
to be inconsistent when using our second constraint. We discuss these results
in view of the Hosomichi-Ribault proposal and some of our earlier results on
the derivation of b^{-2}/2-shift equations.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:10:52 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Nov 2008 15:50:44 GMT"
}
] | 2010-10-27T00:00:00 | [
[
"Adorf",
"Hendrik",
""
],
[
"Flohr",
"Michael",
""
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] |
801.2712 | Daniel Reitzner | Teiko Heinosaari, Peter Stano, Daniel Reitzner | Approximate Joint Measurability of Spin Along Two Directions | 6 pages, 4 figures | International Journal of Quantum Information 6 (2008) 975-980 | 10.1142/S0219749908004365 | null | quant-ph | null | We study the existence of jointly measurable POVM approximations to two
non-commuting sharp spin observables. We compare two different ways to specify
optimal approximations.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:01:01 GMT"
}
] | 2008-11-16T00:00:00 | [
[
"Heinosaari",
"Teiko",
""
],
[
"Stano",
"Peter",
""
],
[
"Reitzner",
"Daniel",
""
]
] | [
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] |
801.2713 | Giuliana Fiorentino | G. Fiorentino, R. Contreras, G. Clementini, K. Glatt, E. Sabbi, M.
Sirianni, E. Grebel, and J. Ghallager | Detection of new variable stars in the SMC cluster NGC 121 | 3 pages, 3 figures | Mem.Soc.Ast.It.79:3,2008 | null | null | astro-ph | null | New candidate variable stars have been identified in the Small Magellanic
Cloud cluster NGC121, by applying both the image subtraction technique (ISIS,
Alard 2000) and the Welch & Stetson (1993) detection method to HST WFPC2
archive and ACS proprietary images of the cluster. The new candidate variable
stars are located from the cluster's Main Sequence up to Red Giant Branch.
Twenty-seven of them fall on the cluster Horizontal Branch and are very likely
RR Lyrae stars. They include the few RR Lyrae stars already discussed by Walker
& Mack (1988). We also detected 20 Dwarf Cepheid candidates in the central
region of NGC121. Our results confirm the "true" globular cluster nature of
NGC121, a cluster that is at the young end of the Galactic globulars' age
range.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:05:37 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 09:44:31 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Fiorentino",
"G.",
""
],
[
"Contreras",
"R.",
""
],
[
"Clementini",
"G.",
""
],
[
"Glatt",
"K.",
""
],
[
"Sabbi",
"E.",
""
],
[
"Sirianni",
"M.",
""
],
[
"Grebel",
"E.",
""
],
[
"Ghallager",
"J.",
""
]
] | [
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] |
801.2714 | Grigory Volovik | G.E. Volovik | On spectrum of vacuum energy | 10 pages, 2 figures, JPCS style, prepared for proceedings of
DICE-2008 | Journal of Physics: Conference Series 174, 012007 (2009) | 10.1088/1742-6596/174/1/012007 | null | gr-qc cond-mat.stat-mech hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss the problem of the spectral function of vacuum energy. In
traditional approach the ultraviolet divergencies of the vacuum energy are
cancelled by imposing relations between different quantum fields and their
masses. The emergent theories suggest that the microscopic degrees of the
underlying quantum vacuum add to the spectral function and their contribution
cancels the diverging zero point energy of quantum fields. Examples of the
spectral function of the vacuum energy in the condensed-matter systems with
relativity emerging at low energy are presented. In the Sakharov induced
gravity situation may be even more dramatic: only microscopic (Planck scale)
constituent fields contribute to the vacuum energy, while the diverging
zero-point energy of emergent quantum field (gravitational field) is missing.
On the other hand consideration of the fermionic condensed matter systems
suggests that emergent relativistic fermionic quasiparticles contribute in
conventional way as Dirac vacuum.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:06:44 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jan 2008 19:20:29 GMT"
},
{
"version": "v3",
"created": "Wed, 14 Jan 2009 19:58:53 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Volovik",
"G. E.",
""
]
] | [
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] |
801.2715 | Levente Molnar | L. Molnar | Prospects for identified leading particle correlation at LHC and in
ALICE | 9 pages, 8 figures, Talk given at Workshop on High P(T) Physics at
LHC (LHC07), Jyvaskyla, Finland, 23-27 Mar 2007 | PoSLHC07:027,2007 | null | null | nucl-ex | null | Azimuthal di-hadron correlations play important role in the characterization
of the medium created in heavy-ion collisions at RHIC. Moreover, as a novel
phenomenon, strong modification of the away-side correlation is observed in
Au+Au with respect to p+p collisions. Below the exclusive jet reconstruction
threshold at LHC, leading particle correlations will provide access to the
regime where hard scatterings and bulk medium properties can be simultaneously
studied. Leading particle correlations can be extended to very low transverse
momenta via the tracking and particle identification capabilities of ALICE, to
the coalescence and hydrodynamic domains. In preparation for the first p+p and
Pb+Pb collisions of LHC, we present prospects on leading particle correlations
with identified particles in ALICE.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:15:23 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Molnar",
"L.",
""
]
] | [
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] |
801.2716 | Gregory MacDougall | G. J. MacDougall, A. A. Aczel, J.P. Carlo, T. Ito, J. Rodriguez, P. L.
Russo, Y. J. Uemura, S. Wakimoto, and G. M. Luke | Absence of time reversal symmetry breaking in La_{2-x}Sr_{x}CuO_{4} | Submitted to Phys. Rev. Lett. (2008) | Physical Review Letters 101, 017001 (2008). | 10.1103/PhysRevLett.101.017001 | null | cond-mat.supr-con | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have performed zero-field muon spin rotation measurements on single
crystals of La_{2-x}Sr_{x}CuO_{4} to search for spontaneous currents in the
pseudo-gap state. By comparing measurements on materials across the phase
diagram, we put strict upper limits on any possible time-reversal symmetry
breaking fields that could be associated with the pseudo-gap. Comparison
between experimental limits and proposed circulating current states effectively
eliminates the possibility that such states exist in this family of materials.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:02:05 GMT"
},
{
"version": "v2",
"created": "Fri, 6 Jun 2008 15:09:03 GMT"
},
{
"version": "v3",
"created": "Tue, 1 Jul 2008 15:29:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"MacDougall",
"G. J.",
""
],
[
"Aczel",
"A. A.",
""
],
[
"Carlo",
"J. P.",
""
],
[
"Ito",
"T.",
""
],
[
"Rodriguez",
"J.",
""
],
[
"Russo",
"P. L.",
""
],
[
"Uemura",
"Y. J.",
""
],
[
"Wakimoto",
"S.",
""
],
[
"Luke",
"G. M.",
""
]
] | [
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0.0456056893,
-0.0561030321,
0.0429687947,
-0.0975901484,
0.0351334587
] |
801.2717 | Charalampos Moustakidis | Ch.C. Moustakidis | Temperature and momentum dependence of single-particle properties in hot
asymmetric nuclear matter | 22 pages, 14 figures | Phys.Rev.C78:054323,2008 | 10.1103/PhysRevC.78.054323 | null | nucl-th nucl-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have studied the effects of momentum dependent interactions on the
single-particle properties of hot asymmetric nuclear matter. In particular, the
single-particle potential of protons and neutrons as well as the symmetry
potential have been studied within a self-consistent model using a momentum
dependent effective interaction. In addition, the isospin splitting of the
effective mass has been derived from the above model. In each case temperature
effects have been included and analyzed. The role of the specific
parametrization of the effective interaction used in the present work has been
investigated. It has been concluded that the behavior of the symmetry potential
depends strongly on the parametrization of the interaction part of the energy
density and the momentum dependence of the regulator function. The effects of
the parametrization have been found to be less pronounced on the isospin mass
splitting.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:25:56 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Nov 2008 06:34:28 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Moustakidis",
"Ch. C.",
""
]
] | [
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801.2718 | F. de los Santos | Elvira Romera, Francisco de los Santos, Omar Al Hammal, and Miguel A.
Munoz | Critical wetting of a class of nonequilibrium interfaces: A computer
simulation study | 7 pages, 8 figures | Physical Review E 77, 011116 (2008) | 10.1103/PhysRevE.77.011116 | null | cond-mat.stat-mech | null | Critical wetting transitions under nonequilibrium conditions are studied
numerically and analytically by means of an interface-displacement model
defined by a Kardar-Parisi-Zhang equation, plus some extra terms representing a
limiting, short-ranged attractive wall. Its critical behavior is characterized
in detail by providing a set of exponents for both the average height and the
surface order-parameter in one dimension. The emerging picture is qualitatively
and quantitatively different from recently reported mean-field predictions for
the same problem. Evidence is shown that the presence of the attractive wall
induces an anomalous scaling of the interface local slopes.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:41:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Romera",
"Elvira",
""
],
[
"Santos",
"Francisco de los",
""
],
[
"Hammal",
"Omar Al",
""
],
[
"Munoz",
"Miguel A.",
""
]
] | [
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-0.0607121587,
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] |
801.2719 | Paolo Butera | Lev N. Shchur (LITP), Bertrand Berche (LPM), and Paolo Butera (INFN) | High-precision determination of universal amplitude ratios for the q=3
Potts model in 2d | LaTeX, 20 pages with 6 figures | Phys. Rev. B 77 (2008) 144410 | 10.1103/PhysRevB.77.144410 | null | cond-mat.stat-mech hep-lat | null | Monte Carlo simulations and series expansion data for the energy, specific
heat, magnetization and susceptibility of the 3-state Potts model on the square
lattice are analyzed in the vicinity of the critical point in order to estimate
universal combinations of critical amplitudes.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:16:04 GMT"
}
] | 2008-06-30T00:00:00 | [
[
"Shchur",
"Lev N.",
"",
"LITP"
],
[
"Berche",
"Bertrand",
"",
"LPM"
],
[
"Butera",
"Paolo",
"",
"INFN"
]
] | [
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] |
801.272 | David Craven | David A. Craven | Algebraic Modules and the Auslander--Reiten Quiver | 10 pages | null | null | null | math.RT | null | Recall that an algebraic module is a KG-module that satisfies a polynomial
with integer coefficients, with addition and multiplication given by direct sum
and tensor product. In this article we prove that non-periodic algebraic
modules are very rare, and that if the complexity of an algebraic module is at
least 3, then it is the only algebraic module on its component of the (stable)
Auslander--Reiten quiver. We include a strong conjecture on the relationship
between periodicity and algebraicity.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:52:10 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Craven",
"David A.",
""
]
] | [
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] |
801.2721 | Alain Le-Yaouanc | Ph. Boucaud, J-P. Leroy, A. Le Yaouanc, J. Micheli, O. Pene, J.
Rodriguez--Quintero | IR finiteness of the ghost dressing function from numerical resolution
of the ghost SD equation | 17 pages, 3 figures (one new figure and a short paragraph added) | JHEP 0806:012,2008 | 10.1088/1126-6708/2008/06/012 | LPT-Orsay/08-44, UHU-FT/0803 | hep-ph hep-lat | null | We solve numerically the Schwinger-Dyson (SD hereafter) ghost equation in the
Landau gauge for a given gluon propagator finite at k=0 (alpha_gluon=1) and
with the usual assumption of constancy of the ghost-gluon vertex ; we show that
there exist two possible types of ghost dressing function solutions, as we have
previously inferred from analytical considerations : one singular at zero
momentum, satisfying the familiar relation alpha_gluon+2 alpha_ghost=0 between
the infrared exponents of the gluon and ghost dressing functions(in short,
respectively alpha_G and alpha_F) and having therefore alpha_ghost=-1/2, and
another which is finite at the origin (alpha_ghost=0), which violates the
relation. It is most important that the type of solution which is realized
depends on the value of the coupling constant. There are regular ones for any
coupling below some value, while there is only one singular solution, obtained
only at a critical value of the coupling. For all momenta k<1.5 GeV where they
can be trusted, our lattice data exclude neatly the singular one, and agree
very well with the regular solution we obtain at a coupling constant compatible
with the bare lattice value.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 16:53:30 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Mar 2008 16:29:15 GMT"
}
] | 2010-03-19T00:00:00 | [
[
"Boucaud",
"Ph.",
""
],
[
"Leroy",
"J-P.",
""
],
[
"Yaouanc",
"A. Le",
""
],
[
"Micheli",
"J.",
""
],
[
"Pene",
"O.",
""
],
[
"Rodriguez--Quintero",
"J.",
""
]
] | [
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] |
801.2722 | Manuela Capello | Manuela Capello, Marcin Raczkowski, and Didier Poilblanc | Stability of RVB hole stripes in high-temperature superconductors | 8 pages, 9 figures. Enlarged version | Phys. Rev. B 77, 224502 (2008) | 10.1103/PhysRevB.77.224502 | null | cond-mat.str-el | null | Indications of density-wave states in underdoped cuprates, coming from recent
STM (scanning tunneling microscopy) and Hall-resistance measurements, have
raised new concerns whether stripes could be stabilized in the superconducting
phase of cuprate materials, even in the absence of antiferromagnetism. Here, we
investigate this issue using state-of-the-art quantum Monte Carlo calculations
of a $t-J$ model. In particular we consider the stability of unidirectional
hole domains in a modulated superconducting background, by taking into account
the effect of tetragonal-lattice distortions, next-nearest neighbor hopping and
long-range Coulomb repulsion.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:05:48 GMT"
},
{
"version": "v2",
"created": "Thu, 15 May 2008 16:19:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Capello",
"Manuela",
""
],
[
"Raczkowski",
"Marcin",
""
],
[
"Poilblanc",
"Didier",
""
]
] | [
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] |
801.2723 | David Craven | David A. Craven | On the Tensor Products of Modules for Dihedral 2-Groups | 11 pages | null | null | null | math.RT | null | Recall that an algebraic module is a KG-module that satisfies a polynomial
with integer coefficients, with addition and multiplication given by direct sum
and tensor product. In this article we prove that if L is a component of the
(stable) Auslander-Reiten quiver for a dihedral 2-group consisting of
non-periodic modules, then there is at most one algebraic module on L.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:19:15 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Craven",
"David A.",
""
]
] | [
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801.2724 | Juerg Froehlich | Juerg Froehlich | Spin - or, actually: Spin and Quantum Statistics | 50 pages, no figures, seminar on "spin" | null | 10.1007/978-3-7643-8799-0_1 | null | math-ph math.MP | null | The history of the discovery of electron spin and the Pauli principle and the
mathematics of spin and quantum statistics are reviewed. Pauli's theory of the
spinning electron and some of its many applications in mathematics and physics
are considered in more detail. The role of the fact that the tree-level
gyromagnetic factor of the electron has the value g = 2 in an analysis of
stability (and instability) of matter in arbitrary external magnetic fields is
highlighted. Radiative corrections and precision measurements of g are
reviewed. The general connection between spin and statistics, the CPT theorem
and the theory of braid statistics are described.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:15:39 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 11:25:31 GMT"
},
{
"version": "v3",
"created": "Fri, 29 Feb 2008 16:46:49 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Froehlich",
"Juerg",
""
]
] | [
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] |
801.2725 | Eric D. Chisolm | Thomas F. Jordan and Eric D. Chisolm | Probability sum rules and consistent quantum histories | 14 pages, 2 figures, added discussion of tensor-product histories in
response to Physics Letters A referee, corrected typo | Physics Letters A 373, 3016 (2009) | 10.1016/j.physleta.2009.06.064 | LA-UR 09-03687 | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | An example shows that weak decoherence is more restrictive than the minimal
logical decoherence structure that allows probabilities to be used consistently
for quantum histories. The probabilities in the sum rules that define minimal
decoherence are all calculated by using a projection operator to describe each
possibility for the state at each time. Weak decoherence requires more sum
rules. They bring in additional variables, that require different measurements
and a different way to calculate probabilities, and raise questions of
operational meaning. The example shows that extending the linearly positive
probability formula from weak to minimal decoherence gives probabilities that
are different from those calculated in the usual way using the Born and von
Neumann rules and a projection operator at each time.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:21:53 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Mar 2008 15:01:07 GMT"
},
{
"version": "v3",
"created": "Wed, 11 Jun 2008 21:32:05 GMT"
},
{
"version": "v4",
"created": "Thu, 12 Jun 2008 20:24:11 GMT"
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{
"version": "v5",
"created": "Thu, 11 Jun 2009 22:37:58 GMT"
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{
"version": "v6",
"created": "Mon, 6 Jul 2009 22:58:22 GMT"
},
{
"version": "v7",
"created": "Tue, 21 Jul 2009 21:06:26 GMT"
}
] | 2010-10-11T00:00:00 | [
[
"Jordan",
"Thomas F.",
""
],
[
"Chisolm",
"Eric D.",
""
]
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] |
801.2726 | Mohammad Sal Moslehian | O. Hirzallah, F. Kittaneh, M. S. Moslehian | Schatten p-norm inequalities related to a characterization of inner
product spaces | Minor revision, to appear in Math. Inequal. Appl. (MIA) | Math. Inequal. Appl. 13 (2010), no. 2, 235-241 | 10.7153/mia-13-19 | null | math.FA math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $A_1, ... A_n$ be operators acting on a separable complex Hilbert space
such that $\sum_{i=1}^n A_i=0$. It is shown that if $A_1, ... A_n$ belong to a
Schatten $p$-class, for some $p>0$, then 2^{p/2}n^{p-1} \sum_{i=1}^n
\|A_i\|^p_p \leq \sum_{i,j=1}^n\|A_i\pm A_j\|^p_p for $0<p\leq 2$, and the
reverse inequality holds for $2\leq p<\infty$. Moreover, \sum_{i,j=1}^n\|A_i\pm
A_j\|^2_p \leq 2n^{2/p} \sum_{i=1}^n \|A_i\|^2_p for $0<p\leq 2$, and the
reverse inequality holds for $2\leq p<\infty$. These inequalities are related
to a characterization of inner product spaces due to E.R. Lorch.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:50:05 GMT"
},
{
"version": "v2",
"created": "Thu, 4 Dec 2008 09:48:02 GMT"
}
] | 2021-07-23T00:00:00 | [
[
"Hirzallah",
"O.",
""
],
[
"Kittaneh",
"F.",
""
],
[
"Moslehian",
"M. S.",
""
]
] | [
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] |
801.2727 | Andrieux David | D. Andrieux and P. Gaspard | Dynamical randomness, information, and Landauer's principle | null | Europhys. Lett. 81, 28004 (2008) | 10.1209/0295-5075/81/28004 | null | cond-mat.stat-mech | null | New concepts from nonequilibrium thermodynamics are used to show that
Landauer's principle can be understood in terms of time asymmetry in the
dynamical randomness generated by the physical process of the erasure of
digital information. In this way, Landauer's principle is generalized, showing
that the dissipation associated with the erasure of a sequence of bits produces
entropy at the rate $k_{{\rm B}}I$ per erased bit, where $I$ is Shannon's
information per bit.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:23:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Andrieux",
"D.",
""
],
[
"Gaspard",
"P.",
""
]
] | [
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] |
801.2728 | Paolo Visco | P. Visco, F. van Wijland, E. Trizac | Non Poissonian statistics in a low density fluid | 4 pages, 2 figures | J. Phys. Chem. B 112 (17), 5412 (2008) | 10.1021/jp800333h | null | cond-mat.stat-mech cond-mat.soft | null | Our interest goes to the collisional statistics in an arbitrary interacting
fluid. We show that even in the low density limit and contrary to naive
expectation, the number of collisions experienced by a tagged particle in a
given time does not obey Poisson law, and that conversely, the free flight time
distribution is not a simple exponential. As an illustration, the hard sphere
fluid case is worked out in detail. For this model, we quantify analytically
those deviations and successfully compare our predictions against molecular
dynamics simulations.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:40:06 GMT"
}
] | 2008-04-30T00:00:00 | [
[
"Visco",
"P.",
""
],
[
"van Wijland",
"F.",
""
],
[
"Trizac",
"E.",
""
]
] | [
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] |
801.2729 | Luca Martinazzi | Luca Martinazzi | Classification of solutions to the higher order Liouville's equation on
R^{2m} | null | Math. Z. 263 (2009), 307-329 | 10.1007/s00209-008-0419-1 | null | math.AP math.DG | null | We classify the solutions to the equation (- \Delta)^m u=(2m-1)!e^{2mu} on
R^{2m} giving rise to a metric g=e^{2u}g_{R^{2m}} with finite total
$Q$-curvature in terms of analytic and geometric properties. The analytic
conditions involve the growth rate of u and the asymptotic behaviour of \Delta
u(x) as |x|\to \infty. As a consequence we give a geometric characterization in
terms of the scalar curvature of the metric e^{2u}g_{R^{2m}} at infinity, and
we observe that the pull-back of this metric to $S^{2m}$ via the stereographic
projection can be extended to a smooth Riemannian metric if and only if it is
round.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:35:53 GMT"
}
] | 2015-07-29T00:00:00 | [
[
"Martinazzi",
"Luca",
""
]
] | [
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] |
801.273 | Mario Nicodemi | M. Nicodemi and A. Prisco | A Symmetry Breaking Model for X Chromosome Inactivation | See also Nature Physics N&V April 2007 | Phys. Rev. Lett. 98, 108104 (2007) | 10.1103/PhysRevLett.98.108104 | null | q-bio.SC | null | In mammals, dosage compensation of X linked genes in female cells is achieved
by inactivation of one of their two X chromosomes which is randomly chosen. The
earliest steps in X-inactivation (XCI), namely the mechanism whereby cells
count their X chromosomes and choose between two equivalent X, remain
mysterious. Starting from the recent discovery of X chromosome colocalization
at the onset of X-inactivation, we propose a Statistical Mechanics model of
XCI, which is investigated by computer simulations and checked against
experimental data. Our model describes how a `blocking factor' complex is
self-assembled and why only one is formed out of many diffusible molecules,
resulting in a spontaneous symmetry breaking (SB) in the binding to two
identical chromosomes. These results are used to derive a scenario of
biological implications describing all current experimental evidences, e.g.,
the importance of colocalization.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:36:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nicodemi",
"M.",
""
],
[
"Prisco",
"A.",
""
]
] | [
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] |
801.2731 | Jose Luis Toca-Herrera | Miguel J.A. Lainez, Luis-Millan Gonzalez, Jose E. Gallach, Gerard
Moras, Daniel Ranz, and Jose L. Toca-Herrera | Strength stimuli on the quadriceps femoris influences the physiological
tremor of the index finger | 22 pages, 5 figures, 1 table | null | null | null | physics.med-ph | null | The influence of fatiguing stimuli applied to the quadriceps femoris on the
tremor of the index finger on sixteen healthy subjects has been investigated,
by measuring the acceleration and the electromyography activity of the extensor
digitorum at two different speeds. No significant changes in the basal
condition could be measured at 0.52 rad/s. However, at 1.05 rad/s the tremor
amplitude (12.23%, p<0.05) and the electromyography activity (20.19%, p<0.05)
increased in the time domain. In the frequential domain, the peak associated to
the acceleration increased in 26.30% (p<0.05), while the electromiography
activity experienced an increase of 81.34% (p<0.05). The largest change in
frequency took place in the range 7-17 Hz. The discussion of the results leads
to the conclusion that the supraespinal mechanism is responsible for the
measured effect.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:46:51 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Lainez",
"Miguel J. A.",
""
],
[
"Gonzalez",
"Luis-Millan",
""
],
[
"Gallach",
"Jose E.",
""
],
[
"Moras",
"Gerard",
""
],
[
"Ranz",
"Daniel",
""
],
[
"Toca-Herrera",
"Jose L.",
""
]
] | [
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] |
801.2732 | Blanca Biel | Blanca Biel, F.J. Garcia-Vidal, Angel Rubio and Fernando Flores | Ab initio study of transport properties in defected carbon nanotubes: an
O(N) approach | 15 pages, 12 figures (submitted to J. Phys: Condens. Matter) | J. Phys.: Condens. Matter 20, 294214 (2008) | 10.1088/0953-8984/20/29/294214 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | A combination of ab initio simulations and linear-scaling Green's functions
techniques is used to analyze the transport properties of long (up to one
micron) carbon nanotubes with realistic disorder. The energetics and the
influence of single defects (mono- and di-vacancies) on the electronic and
transport properties of single-walled armchair carbon nanotubes are analyzed as
a function of the tube diameter by means of the local orbital first-principles
Fireball code. Efficient O(N) Green's functions techniques framed within the
Landauer-Buttiker formalism allow a statistical study of the nanotube
conductance averaged over a large sample of defected tubes and thus extraction
of the nanotubes localization length. Both the cases of zero and room
temperature are addressed.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:40:43 GMT"
}
] | 2009-03-03T00:00:00 | [
[
"Biel",
"Blanca",
""
],
[
"Garcia-Vidal",
"F. J.",
""
],
[
"Rubio",
"Angel",
""
],
[
"Flores",
"Fernando",
""
]
] | [
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] |
801.2733 | Nicola Fabiano | Nicola Fabiano | On the cross-section peaks for a heavy quark bound state | 8 pages, latex2e. Accepted for publication in EPJC. Revised version
has an added paragraph about J/psi | Eur.Phys.J.C58:395-398,2008 | 10.1140/epjc/s10052-008-0789-x | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss the values of resonance peaks of the cross-section of a heavy
quark bound state obtained by means of a Green function method applied to a
Coulombic model and compare the result to the Upsilon and J/psi data.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:46:13 GMT"
},
{
"version": "v2",
"created": "Fri, 24 Oct 2008 20:01:14 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Fabiano",
"Nicola",
""
]
] | [
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801.2734 | Fabio Franchini | Fabio Franchini | On Hydrodynamic Correlations in Low-Dimensional Interacting Systems | Ph.D. Graduation Thesis, University of Stony Brook, New York (U.S.A)
211 Pages, 21 Figures, 1 Table | null | null | null | cond-mat.str-el cond-mat.other | null | Low-dimensional systems are an important field of current theoretical and
experimental research. Recent technological developments provide many possible
realizations of effectively one-dimensional systems. These devices promise to
give us access to a new range of phenomena. It is therefore very interesting to
develop theoretical methods specific for such systems to model their behavior
and calculate the correlators of the resulting theory. Incidentally, one such
method exists and is known as Bosonization. It can be applied to
one-dimensional systems and effectively describes low energy excitations in a
universal way. We use the example of a correlator known as the Emptiness
Formation Probability to show that Bosonization fails to describe some long
range correlators corresponding to large disturbances (the EFP measures the
probability for the ground state of the system to develop a region without
particles). We trace this failure to the fact that Bosonization is constructed
as a linear approximation of the full theory and we set up to develop a
collective description with the required non-linearity. The resulting scheme is
essentially a Hydrodynamic paradigm for quantum systems. We show how to
construct such a hydrodynamic description for a variety of exactly integrable
models and illustrate how it can be used to make new predictions. For the
special case of the spin-1/2 XY model we take advantage of the structure of the
model to express the EFP as a determinant of a very special type of matrix,
known as Toeplitz Matrix. We use the theory of Toeplitz determinants to
calculate the asymptotic behavior of the EFP in the XY model and discuss its
relation with the criticality of the theory.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 17:54:57 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Franchini",
"Fabio",
""
]
] | [
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] |
801.2735 | Rajiv Singh | Rajiv R. P. Singh and David A. Huse | Triplet and Singlet Excitations in the Valence Bond Crystal Phase of
Kagome Lattice Heisenberg Model | 8 pages, 2 figures | Phys. Rev. B 77, 144415 (2008) | 10.1103/PhysRevB.77.144415 | null | cond-mat.str-el | null | A proposed ground state for the Kagome Lattice Heisenberg Model (KLHM)
consists of a Valence Bond Crystal (VBC) with a 36-site unit cell. We calculate
the low-lying triplet and singlet excitations in the VBC phase for the
infinite-lattice model and for the 36-site cluster. For the infinite lattice,
the lowest triplet excitation is found to have a spin gap of approximately
$0.08 \pm 0.02 J$ and a bandwidth of only about $0.01 J$. For the 36-site
cluster, consisting of a single unit cell with periodic boundary conditions,
there are substantial finite-size effects: the spin gap there is estimated to
be approximately $0.2 J$, close to the exact diagonalization result of $0.164
J$. The triplet excitations attract one another and form many bound states in
the spin-singlet channel. We find a large number of such bound states for the
36-site cluster, many of which appear to lie below the spin gap, again in
agreement with the results from exact diagonalization.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:02:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Singh",
"Rajiv R. P.",
""
],
[
"Huse",
"David A.",
""
]
] | [
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-0.0732516199,
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] |
801.2736 | Neil Drummond | A. Ma, N. D. Drummond, M. D. Towler, and R. J. Needs | All-electron quantum Monte Carlo calculations for the noble gas atoms He
to Xe | null | A. Ma et al., Phys. Rev. E 71, 066704 (2005) | 10.1103/PhysRevE.71.066704 | null | cond-mat.mtrl-sci | null | We report all-electron variational and diffusion quantum Monte Carlo (VMC and
DMC) calculations for the noble gas atoms He, Ne, Ar, Kr, and Xe. The
calculations were performed using Slater-Jastrow wave functions with
Hartree-Fock single-particle orbitals. The quality of both the optimized
Jastrow factors and the nodal surfaces of the wave functions declines with
increasing atomic number Z, but the DMC calculations are tractable and well
behaved in all cases. We discuss the scaling of the computational cost of DMC
calculations with Z.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:05:20 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Ma",
"A.",
""
],
[
"Drummond",
"N. D.",
""
],
[
"Towler",
"M. D.",
""
],
[
"Needs",
"R. J.",
""
]
] | [
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] |
801.2737 | Sergio Colafrancesco | S. Colafrancesco, P. Marchegiani | Warming rays in cluster cool cores | 19 pages, 17 figures, A&A in press | null | 10.1051/0004-6361:20078428 | null | astro-ph | null | We present a model of cosmic ray heating of clusters' cores that reproduces
the observed temperature distribution in clusters by using an energy balance
condition in which the emitted X-ray energy is supplied by the hadronic cosmic
rays, which act as warming rays (WRs). The temperature profile of the IC gas is
correlated with the WR pressure distribution and, consequently, with the
non-thermal emission (radio, hard X-ray and gamma-ray) induced by the
interaction of the WRs with the IC gas and magnetic field. The temperature
distribution of the IC gas in both cool-core and non cool-core clusters is
successfully predicted from the measured IC gas density distribution. Under
this contraint, the WR model is also able to reproduce the thermal and
non-thermal pressure distribution in clusters, as well as their radial entropy
distribution. The WR model provides other observable features: a correlation of
the pressure ratio (WRs to thermal IC gas) with the inner cluster temperature
T_{inner}, a correlation of the gamma-ray luminosity with T_{inner}, a
substantial number of cool-core clusters observable with the GLAST-LAT
experiment, a surface brightness of radio halos in cool-core clusters that
recovers the observed one, a hard X-ray emission from cool-core clusters that
is systematically lower than the observed limits and yet observable with the
next generation HXR experiments like Simbol-X. The specific theoretical
properties and the multi-frequency distribution of the e.m. signals predicted
in the WR model render it quite different from the other models proposed for
the heating of clusters' cool-cores. Such differences make it possible to prove
or disprove our model as an explanation of the cooling-flow problems on the
basis of multi-frequency observations of galaxy clusters.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:05:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Colafrancesco",
"S.",
""
],
[
"Marchegiani",
"P.",
""
]
] | [
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801.2738 | Francesco Leone | M. J. Stift, F. Leone | Paschen is Partially Back | 6 pages, 3 figures | Contrib.Astron.Obs.Skalnate Pleso 38:185-190,2008 | null | null | astro-ph | null | We present a discussion of the partial Paschen-Back (PB) effect in magnetic
Ap stars. An overview of the theory is illustrated with examples of how
splittings deviate non-linearly from the simple Zeeman picture; normally
forbidden ``ghost lines'' appear in strong fields. Resulting asymmetric stellar
Stokes profiles for a dipolar magnetic geometry are shown for the FeII 6149
line and it is established that PB lines may be subject to wavelength shifts.
Modelling of Stokes profiles in the PB regime opens exciting new diagnostics.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:08:32 GMT"
}
] | 2010-11-26T00:00:00 | [
[
"Stift",
"M. J.",
""
],
[
"Leone",
"F.",
""
]
] | [
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] |
801.2739 | David Berenstein | David Berenstein, Randel Cotta, Rodrigo Leonardi | Numerical tests of AdS/CFT at strong coupling | 23 pages, 7 figures, revtex. v2: minor corrections | Phys.Rev.D78:025008,2008 | 10.1103/PhysRevD.78.025008 | NI07082 | hep-th | null | We study various correlation functions (two and three point functions) in a
large $N$ matrix model of six commuting matrices with a numerical Monte Carlo
algorithm. This is equivalent to a model of a gas of particles in six
dimensions with a confining quadratic potential and logarithmic repulsions at
finite temperature, where we are measuring the leading order non-gaussianities
in the thermal fluctuations.
This is a simplified model of the low energy dynamics of N=4 SYM at strong
coupling. We find strong evidence that the simplified matrix model matches with
the dual gravitational description of three point functions in the AdS/CFT
correspondence.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:09:20 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 18:46:18 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Berenstein",
"David",
""
],
[
"Cotta",
"Randel",
""
],
[
"Leonardi",
"Rodrigo",
""
]
] | [
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] |
801.274 | Francesco Leone | M.J. Stift, F. Leone and E. Landi Degl'Innocenti | Modelling the incomplete Paschen-Back effect in the spectra of magnetic
Ap stars | 8 pages, 10 figures, to appear in MNRAS | null | 10.1111/j.1365-2966.2008.12981.x | null | astro-ph | null | We present first results of a systematic investigation of the incomplete
Paschen-Back effect in magnetic Ap stars. A short overview of the theory is
followed by a demonstration of how level splittings and component strengths
change with magnetic field strength for some lines of special astrophysical
interest. Requirements are set out for a code which allows the calculation of
full Stokes spectra in the Paschen-Back regime and the behaviour of Stokes I
and V profiles of transitions in the multiplet 74 of FeII is discussed in some
detail. It is shown that the incomplete Paschen-Back effect can lead to
noticeable line shifts which strongly depend on total multiplet strength,
magnetic field strength and field direction. Ghost components (which violate
the normal selection rule on J) show up in strong magnetic fields but are
probably unobservable. Finally it is shown that measurements of the integrated
magnetic field modulus $H_s$ are not adversely affected by the Paschen-Back
effect, and that there is a potential problem in (magnetic) Doppler mapping if
lines in the Paschen-Back regime are treated in the Zeeman approximation.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:15:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Stift",
"M. J.",
""
],
[
"Leone",
"F.",
""
],
[
"Degl'Innocenti",
"E. Landi",
""
]
] | [
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] |
801.2741 | Walter Simon | Walter Simon | Static perfect fluids with Pant-Sah equations of state | 32 p., Latex, minor changes and corrections | Gen.Rel.Grav.40:2591-2618,2008 | 10.1007/s10714-008-0641-5 | null | gr-qc | null | We analyze the 3-parameter family of exact, regular, static, spherically
symmetric perfect fluid solutions of Einstein's equations (corresponding to a
2-parameter family of equations of state) due to Pant and Sah and
"rediscovered" by Rosquist and the present author. Except for the Buchdahl
solutions which are contained as a limiting case, the fluids have finite radius
and are physically realistic for suitable parameter ranges. The equations of
state can be characterized geometrically by the property that the 3-metric on
the static slices, rescaled conformally with the fourth power of any linear
function of the norm of the static Killing vector, has constant scalar
curvature. This local property does not require spherical symmetry; in fact it
simplifies the the proof of spherical symmetry of asymptotically flat solutions
which we recall here for the Pant-Sah equations of state. We also consider a
model in Newtonian theory with analogous geometric and physical properties,
together with a proof of spherical symmetry of the asymptotically flat
solutions.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:18:36 GMT"
},
{
"version": "v2",
"created": "Mon, 31 Mar 2008 18:00:40 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Simon",
"Walter",
""
]
] | [
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] |
801.2742 | Neil Drummond | A. Ma, M. D. Towler, N. D. Drummond, and R. J. Needs | Scheme for adding electron-nucleus cusps to Gaussian orbitals | null | A. Ma et al., J. Chem. Phys. 122, 224322 (2005) | 10.1063/1.1940588 | null | physics.comp-ph | null | A simple scheme is described for introducing the correct cusps at nuclei into
orbitals obtained from Gaussian basis set electronic structure calculations.
The scheme is tested with all-electron variational quantum Monte Carlo (VMC)
and diffusion quantum Monte Carlo (DMC) methods for the Ne atom, the H2
molecule, and 55 molecules from a standard benchmark set. It greatly reduces
the variance of the local energy in all cases and slightly improves the
variational energy. This scheme yields a general improvement in the efficiency
of all-electron VMC and DMC calculations using Gaussian basis sets.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:18:55 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Ma",
"A.",
""
],
[
"Towler",
"M. D.",
""
],
[
"Drummond",
"N. D.",
""
],
[
"Needs",
"R. J.",
""
]
] | [
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] |
801.2743 | Arnoldas Deltuva | A. Deltuva, A.C. Fonseca, P.U. Sauer | Four-nucleon system with $\Delta$-isobar excitation | 11 figures, to be published in Phys. Lett. B | Phys.Lett.B660:471-477,2008 | 10.1016/j.physletb.2007.12.058 | null | nucl-th | null | The four-nucleon bound state and scattering below three-body breakup
threshold are described based on the realistic coupled-channel potential CD
Bonn + $\Delta$ which allows the excitation of a single nucleon to a $\Delta$
isobar. The Coulomb repulsion between protons is included. In the four-nucleon
system the two-baryon coupled-channel potential yields effective two-, three-
and four-nucleon forces, mediated by the $\Delta$ isobar and consistent with
each other and with the underlying two-nucleon force. The effect of the
four-nucleon force on the studied observables is much smaller than the effect
of the three-nucleon force. The inclusion of the $\Delta$ isobar is unable to
resolve the existing discrepancies with the experimental data.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:21:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Deltuva",
"A.",
""
],
[
"Fonseca",
"A. C.",
""
],
[
"Sauer",
"P. U.",
""
]
] | [
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] |
801.2744 | Claire Berger | Jakub Kedzierski, Pei-Lan Hsu, Paul Healey, Peter Wyatt, Craig Keast,
Mike Sprinkle, Claire Berger, Walt de Heer | Epitaxial graphene transistors on SiC substrates | null | IEEE /Transactions on Electron Devices 55, 2078 (2008). | 10.1109/TED.2008.926593 | null | cond-mat.mtrl-sci | null | This paper describes the behavior of top gated transistors fabricated using
carbon, particularly epitaxial graphene on SiC, as the active material. In the
past decade research has identified carbon-based electronics as a possible
alternative to silicon-based electronics. This enthusiasm was spurred by high
carbon nanotube carrier mobilities. However, nanotube production, placement,
and control are all serious issues. Graphene, a thin sheet of graphitic carbon,
can overcome some of these problems and therefore is a promising new electronic
material. Although graphene devices have been built before, in this work we
provide the first demonstration and systematic evaluation of arrays of a large
number of transistors entirely produced using standard microelectronics
methods. Graphene devices presented feature high-k dielectric, mobilities up to
5000 cm2/Vs and, Ion/Ioff ratios of up to 7, and are methodically analyzed to
provide insight into the substrate properties. Typical of graphene, these
micron-scale devices have negligible band gaps and therefore large leakage
currents.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:26:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kedzierski",
"Jakub",
""
],
[
"Hsu",
"Pei-Lan",
""
],
[
"Healey",
"Paul",
""
],
[
"Wyatt",
"Peter",
""
],
[
"Keast",
"Craig",
""
],
[
"Sprinkle",
"Mike",
""
],
[
"Berger",
"Claire",
""
],
[
"de Heer",
"Walt",
""
]
] | [
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] |
801.2745 | Gabriel Zarnauskas | M. R. Robilotta and G. R. S. Zarnauskas | Scalar form factors and nuclear interactions | Talk given at the 20EFB, Pisa, Italy, September 2007. 3 pages and 4
figures | Few Body Syst.44:121-124,2008 | 10.1007/s00601-008-0271-1 | null | nucl-th | null | The scalar-isoscalar term in the two-pion exchange $NN$ potential is
abnormally large and does not respect the hierarchy of effects predicted by
chiral perturbation theory. We argue that this anomaly is associated with
non-perturbative effects, which are also present in the $\pi N$ scalar form
factor.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:27:19 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Robilotta",
"M. R.",
""
],
[
"Zarnauskas",
"G. R. S.",
""
]
] | [
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] |
801.2746 | Serge Koutchmy | Serge Koutchmy, Vladimir Slemzin, Boris Filippov, Jacques-Clair Noens,
David Romeuf and Leon Golub | Analysis and interpretation of a fast limb CME with eruptive prominence,
C-flare and EUV dimming | 11 pages, 9 figures | null | 10.1051/0004-6361:20078311 | null | astro-ph | null | Coronal Mass ejections or CMEs are large dynamical solar-corona events. The
mass balance and kinematics of a fast limb CME, including its prominence
progenitor and the associated flare, will be compared with computed magnetic
structures to look for their origin and effect.
Multi-wavelength ground-based and space-borne observations are used to study
a fast W-limb CME event of December 2, 2003, taking into account both on and
off disk observations. Its erupting prominence is measured at high cadence with
the Pic du Midi full H-alpha line-flux imaging coronagraph. EUV images from
space instruments are processed including difference imaging. SOHO/LASCO images
are used to study the mass excess and motions. A fast bright expanding coronal
loop is identified in the region recorded slightly later by GOES as a C7.2
flare, followed by a brightening and an acceleration phase of the erupting
material with both cool and hot components. The total coronal radiative flux
dropped by 5 percent in the EUV channels, revealing a large dimming effect at
and above the limb. The typical 3-part structure observed 1 hour later shows a
core shaped similarly to the eruptive filament/prominence. The total measured
mass of the escaping CME (1.5x10to16 g from C2 LASCO observations) definitely
exceeds the estimated mass of the escaping cool prominence material although
assumptions made to analyse the Ha erupting prominence, as well as the
corresponding EUV darkening of the filament observed several days before, made
this evaluation uncertain by a factor of 2. From the current free extrapolation
we discuss the shape of the magnetic neutral surface and a possible scenario
leading to an instability, including the small scale dynamics inside and around
the filament.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:30:29 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Koutchmy",
"Serge",
""
],
[
"Slemzin",
"Vladimir",
""
],
[
"Filippov",
"Boris",
""
],
[
"Noens",
"Jacques-Clair",
""
],
[
"Romeuf",
"David",
""
],
[
"Golub",
"Leon",
""
]
] | [
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] |
801.2747 | Javier von Stecher | J. von Stecher, Chris H. Greene, D. Blume | Energetics and Structural Properties of Trapped Two-Component Fermi
Gases | 22 pages, 21 figures | null | 10.1103/PhysRevA.77.043619 | null | cond-mat.other | null | Using two different numerical methods, we study the behavior of two-component
Fermi gases interacting through short-range s-wave interactions in a harmonic
trap. A correlated Gaussian basis-set expansion technique is used to determine
the energies and structural properties, i.e., the radial one-body densities and
pair distribution functions, for small systems with either even or odd $N$, as
functions of the s-wave scattering length and the mass ratio $\kappa$ of the
two species. Particular emphasis is put on a discussion of the angular momentum
of the system in the BEC-BCS crossover regime. At unitarity, the excitation
spectrum of the four-particle system with total angular momentum L=0 is
calculated as a function of the mass ratio $\kappa$. The results are analyzed
from a hyperspherical perspective, which offers new insights into the problem.
Additionally, fixed-node diffusion Monte Carlo calculations are performed for
equal-mass Fermi gases with up to N=30 atoms. We focus on the odd-even
oscillations of the ground state energy of the equal-mass unitary system having
up to N=30 particles, which are related to the excitation gap of the system.
Furthermore, we present a detailed analysis of the structural properties of
these systems.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:36:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"von Stecher",
"J.",
""
],
[
"Greene",
"Chris H.",
""
],
[
"Blume",
"D.",
""
]
] | [
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] |
801.2748 | Mark Kliger | Ami Wiesel, Mark Kliger and Alfred O. Hero III | A greedy approach to sparse canonical correlation analysis | 5 pages, 3 pages | null | null | null | stat.CO stat.ME | null | We consider the problem of sparse canonical correlation analysis (CCA), i.e.,
the search for two linear combinations, one for each multivariate, that yield
maximum correlation using a specified number of variables. We propose an
efficient numerical approximation based on a direct greedy approach which
bounds the correlation at each stage. The method is specifically designed to
cope with large data sets and its computational complexity depends only on the
sparsity levels. We analyze the algorithm's performance through the tradeoff
between correlation and parsimony. The results of numerical simulation suggest
that a significant portion of the correlation may be captured using a
relatively small number of variables. In addition, we examine the use of sparse
CCA as a regularization method when the number of available samples is small
compared to the dimensions of the multivariates.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 18:53:07 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Wiesel",
"Ami",
""
],
[
"Kliger",
"Mark",
""
],
[
"Hero",
"Alfred O.",
"III"
]
] | [
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] |
801.2749 | B. Glenn Piner | B. Glenn Piner, Niraj Pant, and Philip G. Edwards | The Parsec-Scale Jets of the TeV Blazars H 1426+428, 1ES 1959+650, and
PKS 2155-304: 2001-2004 | 16 pages, Astrophysical Journal, in press | null | 10.1086/533521 | null | astro-ph | null | We present Very Long Baseline Array (VLBA) observations of the TeV blazars H
1426+428, 1ES 1959+650, and PKS 2155-304 obtained during the years 2001 through
2004. We observed H 1426+428 at four epochs at 8 GHz, and found that its
parsec-scale structure consisted of a ~17 mJy core and a single ~3 mJy jet
component with an apparent speed of 2.09 +/- 0.53c. The blazar 1ES 1959+650 was
observed at three epochs at frequencies of 15 and 22 GHz. Spectral index
information from these dual-frequency observations was used to definitively
identify the core of the parsec-scale structure. PKS 2155-304 was observed at a
single epoch at 15 GHz with dual-circular polarization, and we present the
first VLBI polarimetry image of this source. For 1ES 1959+650 and PKS 2155-304,
the current observations are combined with the VLBA observations from our
earlier paper to yield improved apparent speed measurements for these sources
with greatly reduced measurement errors. The new apparent speed measured for
component C2 in 1ES 1959+650 is 0.00 +/- 0.04c (stationary), and the new
apparent speed measured for component C1 in PKS 2155-304 is 0.93 +/- 0.31c. We
combine the new apparent speed measurements from this paper with the apparent
speeds measured in TeV blazar jets from our earlier papers to form a current
set of apparent speed measurements in TeV HBLs. The mean peak apparent pattern
speed in the jets of the TeV HBLs is about 1c. We conclude the paper with a
detailed discussion of the interpretation of the collected VLBA data on TeV
blazars in the context of current theoretical models for the parsec-scale
structure of TeV blazar jets.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:34:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Piner",
"B. Glenn",
""
],
[
"Pant",
"Niraj",
""
],
[
"Edwards",
"Philip G.",
""
]
] | [
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] |
801.275 | Hiroyuki Nakano | Hiroyuki Nakano, Carlos O. Lousto (RIT) | New method to integrate 2+1 wave equations with Dirac's delta functions
as sources | 4 pages, 1 figure, prepared for the proceedings of the 17th workshop
on general relativity and gravitation, Nagoya, Japan, Dec.3 - Dec.7, 2007 | null | null | null | gr-qc | null | Gravitational perturbations in a Kerr black hole background can not be
decomposed into simple tensor harmonics in the time domain. Here, we make the
mode decomposition only in the azimuthal direction and discuss the resulting
(2+1)-dimensional Klein-Gordon differential equation for scalar perturbations
with a two dimensional Dirac's $\delta$-function as a source representing a
point particle orbiting a much larger black hole. To make this equation
amenable for numerical integrations we explicitly remove analytically the
singular behavior of the source and compute a global effective source for the
corresponding waveform.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:15:07 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Nakano",
"Hiroyuki",
"",
"RIT"
],
[
"Lousto",
"Carlos O.",
"",
"RIT"
]
] | [
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0.046741616,
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0.048430752,
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0.0274221003,
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0.0049618427,
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0.0114346724,
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] |
801.2751 | Joseph Najnudel | Joseph Najnudel | Construction of an Edwards' probability measure on
$\mathcal{C}(\mathbb{R}_+,\mathbb{R})$ | Published in at http://dx.doi.org/10.1214/10-AOP540 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. 6, 2295-2321 | 10.1214/10-AOP540 | IMS-AOP-AOP540 | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this article, we prove that the measures $\mathbb{Q}_T$ associated to the
one-dimensional Edwards' model on the interval $[0,T]$ converge to a limit
measure $\mathbb{Q}$ when $T$ goes to infinity, in the following sense: for all
$s\geq0$ and for all events $\Lambda_s$ depending on the canonical process only
up to time $s$, $\mathbb{Q}_T(\Lambda_s)\rightarrow\mathbb{Q}(\Lambda_s)$.
Moreover, we prove that, if $\mathbb{P}$ is Wiener measure, there exists a
martingale $(D_s)_{s\in\mathbb{R}_+}$ such that $\mathbb{Q}(\Lambda_s)
=\mathbb{E}_{\mathbb{P}}(\mathbh{1}_{\Lambda_s}D_s)$, and we give an explicit
expression for this martingale.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:27:53 GMT"
},
{
"version": "v2",
"created": "Sat, 20 Feb 2010 00:35:04 GMT"
},
{
"version": "v3",
"created": "Wed, 24 Nov 2010 06:34:07 GMT"
}
] | 2010-11-25T00:00:00 | [
[
"Najnudel",
"Joseph",
""
]
] | [
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801.2752 | Henri Lehn | Georges Lochak (AFBL) | The Equation of a Light Leptonic Magnetic Monopole and its Experimental
Aspects | null | Z.Naturforsch..A62:231-246,2007 | null | null | quant-ph | null | The present theory is closely related to Dirac's equation of the electron,
but not to his magnetic monopole theory, except for his relation between
electric and magnetic charge. The theory is based on the fact, that the
massless Dirac equation admits a second electromagnetic coupling, deduced from
a pseudo-scalar gauge invariance. The equation thus obtained has the symmetry
laws of a massless leptonic, magnetic monopole, able to interact weakly. We
give a more precise form of the Dirac relation between electric and magnetic
charges and a quantum form of the Poincare first integral. In the Weyl
representation our equation splits into P-conjugated monopole and antimonopole
equations with the correct electromagnetic coupling and opposite chiralities,
predicted by P. Curie. Charge-conjugated monopoles are symmetric in space and
not in time (contrary to the electric particles), an important fact for the
vacuum polarization. Our monopoles are magnetically excited neutrinos, which
leads to experimental consequences. These monopoles are assumed to be produced
by electromagnetic pulses or arcs, leading to nuclear transmutations and, for
beta radioactive elements, a shortening of the life time and the emission of
monopoles instead of neutrinos in a magnetic field. A corresponding discussion
is given.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:51:31 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Lochak",
"Georges",
"",
"AFBL"
]
] | [
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] |
801.2753 | Nadine Guillotin-Plantard | Cl\'ement Dombry (LMA), Nadine Guillotin-Plantard (ICJ) | Discrete approximation of a stable self-similar stationary increments
process | 31 pages | null | null | null | math.PR | null | The aim of this paper is to present a result of discrete approximation of
some class of stable self-similar stationary increments processes. The
properties of such processes were intensively investigated, but little is known
on the context in which such processes can arise. To our knowledge,
discretisation and convergence theorems are available only in the case of
stable L\'evy motions and fractional Brownian motions. This paper yields new
results in this direction. Our main result is the convergence of the random
rewards schema, which was firstly introduced by Cohen and Samorodnitsky, and
that we consider in a more general setting. Strong relationships with Kesten
and Spitzer's random walk in random sceneries are evidenced. Finally, we study
some path properties of the limit process.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:42:00 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Dombry",
"Clément",
"",
"LMA"
],
[
"Guillotin-Plantard",
"Nadine",
"",
"ICJ"
]
] | [
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] |
801.2754 | Patrice Bacchin | Benjamin Espinasse (LGC), Patrice Bacchin (LGC), Pierre Aimar (LGC) | Filtration method characterizing the reversibility of colloidal fouling
layers at a membrane surface: analysis through critical flux and osmotic
pressure | Journal of Colloid and Interface Science (2008) to be published | null | 10.1016/j.jcis.2008.01.023 | null | cond-mat.soft | null | A filtration procedure was developed to measure the reversibility of fouling
during cross-flow filtration based on the square wave of applied pressure. The
principle of this method, the apparatus required, and the associated
mathematical relationships are detailed. This method allows for differentiating
the reversible accumulation of matter on, and the irreversible fouling of, a
membrane surface. Distinguishing these two forms of attachment to a membrane
surface provides a means by which the critical flux may be determined. To
validate this method, experiments were performed with a latex suspension at
different degrees of destabilization (obtained by the addition of salt to the
suspension) and at different cross-flow velocities. The dependence of the
critical flux on these conditions is discussed and analysed through the osmotic
pressure of the colloidal dispersion.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:44:50 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Espinasse",
"Benjamin",
"",
"LGC"
],
[
"Bacchin",
"Patrice",
"",
"LGC"
],
[
"Aimar",
"Pierre",
"",
"LGC"
]
] | [
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] |
801.2755 | Ludovic Dan Lemle | Ludovic Dan Lemle (ICJ) | $L^\infty$-Uniqueness of Generalized SCHR\"Odinger Operators | null | null | null | null | math-ph math.MP | null | The main purpose of this paper is to show that the generalized Schr\"odinger
operator ${\cal A}^Vf={1/2}\Delta f+b\nabla f-Vf$, $f\in C_0^\infty(\R^d)$, is
a pre-generator for which we can prove its $L^\infty(\R^d,dx)$-uniqueness.
Moreover, we prove the $L^1(\R^d,dx)$-uniqueness of weak solutions for the
Fokker-Planck equation associated with this pre-generator.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:45:49 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Lemle",
"Ludovic Dan",
"",
"ICJ"
]
] | [
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] |
801.2756 | Giampaolo Cristadoro | Giampaolo Cristadoro, Roland Ketzmerick | On universality of algebraic decays in Hamiltonian systems | 4 pages, 3 figures | Phys. Rev. Lett. 100, 184101 (2008) | 10.1103/PhysRevLett.100.184101 | null | nlin.CD | null | Hamiltonian systems with a mixed phase space typically exhibit an algebraic
decay of correlations and of Poincare' recurrences, with numerical experiments
over finite times showing system-dependent power-law exponents. We conjecture
the existence of a universal asymptotic decay based on results for a Markov
tree model with random scaling factors for the transition probabilities.
Numerical simulations for different Hamiltonian systems support this conjecture
and permit the determination of the universal exponent.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:46:03 GMT"
}
] | 2008-10-06T00:00:00 | [
[
"Cristadoro",
"Giampaolo",
""
],
[
"Ketzmerick",
"Roland",
""
]
] | [
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] |
801.2757 | Martin Houde | Hua-bai Li (1) and Martin Houde (2) (1- Harvard-Smithsonian Center for
Astrophysics, 2- The University of Western Ontario) | Probing the Turbulence Dissipation Range and Magnetic Field Strengths in
Molecular Clouds | 15 pages, 3 figures, accepted for publication in The Astrophysical
Journal | null | 10.1086/529581 | null | astro-ph | null | We study the turbulent velocity dispersion spectra of the coexistent HCN and
HCO+ molecular species as a function of length scale in the M17 star-forming
molecular cloud. We show that the observed downward shift of the ion's spectrum
relative to that of the neutral is readily explained by the existence of an
ambipolar diffusion range within which ion and neutral turbulent energies
dissipate differently. We use these observations to evaluate this decoupling
scale and show how to estimate the strength of the plane-of-the-sky component
of the embedded magnetic field in a completely novel way.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 19:49:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Li",
"Hua-bai",
""
],
[
"Houde",
"Martin",
""
]
] | [
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] |
801.2758 | Werner Krauth | Markus Holzmann, Maguelonne Chevallier, Werner Krauth | Semiclassical theory of the quasi two-dimensional trapped Bose gas | 5 pages, 3 figures | Europhysics Letters 82, 30001 (2008) | 10.1209/0295-5075/82/30001 | null | cond-mat.stat-mech | null | We discuss the quasi two-dimensional trapped Bose gas where the thermal
occupation of excited states in the tightly confined direction is small but
remains finite in the thermodynamic limit. We show that the semiclassical
theory describes very accurately the density profile obtained by Quantum Monte
Carlo calculations in the normal phase above the Kosterlitz--Thouless
temperature T_KT, but differs strongly from the predictions of strictly
two-dimensional mean-field theory, even at relatively high temperature. We
discuss the relevance of our findings for analyzing ultra-cold-atom experiments
in quasi two-dimensional traps.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:20:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Holzmann",
"Markus",
""
],
[
"Chevallier",
"Maguelonne",
""
],
[
"Krauth",
"Werner",
""
]
] | [
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] |
801.2759 | Rachel Dudik Ms. | S. Satyapal, D. Vega, R. P. Dudik, N. P. Abel, T. Heckman | Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in 7
Late-type Galaxies | 8 figures, 17 pages, astro-ph\0801.2766 (Abel & Satyapal 2008; ApJ
accepted) and this posting designed to form a two-part investigation | null | 10.1086/529014 | null | astro-ph | null | We report the discovery using Spitzers high resolution spectrograph of 7
Active Galactic Nuclei (AGN) in a sample of 32 late-type galaxies that show no
definitive signatures of AGN in their optical spectra. Our observations suggest
that the AGN detection rate in late-type galaxies is possibly 4 times larger
than what optical spectroscopic observations alone suggest. We demonstrate
using photoionization models with an input AGN and an extreme EUV-bright
starburst ionizing radiation field that the observed mid-infrared line ratios
cannot be replicated unless an AGN contribution, in some cases as little as 10%
of the total galaxy luminosity, is included. These models show that when the
fraction of the total luminosity due to the AGN is low, optical diagnostics are
insensitive to the presence of the AGN. In this regime of parameter space, the
mid-infrared diagnostics offer a powerful tool for uncovering AGN missed by
optical spectroscopy. The AGN bolometric luminosities in our sample range from
~3 X 10^41 - ~2 X 10^43 ergs s^-1, which, based on the Eddington limit,
corresponds to a lower mass limit for the black hole that ranges from ~3 X
10^3Mdot to as high as ~1.5 X 10^5Mdot. These lower mass limits however do not
put a strain on the well-known relationship between the black hole mass and the
host galaxy's stellar velocity dispersion established in predominantly
early-type galaxies. Our findings add to the growing evidence that black holes
do form and grow in low-bulge environments and that they are significantly more
common than optical studies indicate.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:34:05 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 16:59:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Satyapal",
"S.",
""
],
[
"Vega",
"D.",
""
],
[
"Dudik",
"R. P.",
""
],
[
"Abel",
"N. P.",
""
],
[
"Heckman",
"T.",
""
]
] | [
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] |
801.276 | John Dudley | John. M. Dudley, Goery Genty and Benjamin J. Eggleton | Harnessing and control of optical rogue waves in supercontinuum
generation | Submitted for Publication (2008) | null | 10.1364/OE.16.003644 | null | physics.optics | null | We present a numerical study of the evolution dynamics of ``optical rogue
waves'', statistically-rare extreme red-shifted soliton pulses arising from
supercontinuum generation in photonic crystal fiber [D. R. Solli et al. Nature
Vol. 450, 1054-1058 (2007)]. Our specific aim is to use nonlinear Schrodinger
equation simulations to identify ways in which the rogue wave dynamics can be
actively controlled, and we demonstrate that rogue wave generation can be
enhanced by an order of magnitude through a small modulation across the input
pulse envelope and effectively suppressed through the use of a sliding
frequency filter.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:41:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dudley",
"John. M.",
""
],
[
"Genty",
"Goery",
""
],
[
"Eggleton",
"Benjamin J.",
""
]
] | [
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] |
801.2761 | Lev Vaidman | L. Vaidman | Protective Measurements | An entry in the Compendium of Quantum Physics: Concepts, Experiments,
History and Philosophy, ed. F. Weinert, K. Hentschel, D. Greenberger and B.
Falkenburg | null | null | null | quant-ph | null | A review of protective measurements. Protective measurement is a method for
measuring an expectation value of an observable on a single quantum system. The
quantum state of the system can be protected by a potential, when the state is
a nondegenerate energy eigenstate with a known gap to neighboring states, or
via Zeno effect by frequent projection measurements.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:41:37 GMT"
}
] | 2008-01-18T00:00:00 | [
[
"Vaidman",
"L.",
""
]
] | [
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801.2762 | Kai Schwenzer | Reinhard Alkofer, Markus Q. Huber and Kai Schwenzer | Infrared singularities in Landau gauge Yang-Mills theory | 29 pages, 25 figures; published version | Phys.Rev.D81:105010,2010 | 10.1103/PhysRevD.81.105010 | null | hep-th hep-lat hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a more detailed picture of the infrared regime of Landau gauge
Yang-Mills theory. This is done within a novel framework that allows one to
take into account the influence of finite scales within an infrared power
counting analysis. We find that there are two qualitatively different infrared
fixed points of the full system of Dyson-Schwinger equations. The first extends
the known scaling solution, where the ghost dynamics is dominant and gluon
propagation is strongly suppressed. It features in addition to the strong
divergences of gluonic vertex functions in the previously considered uniform
scaling limit, when all external momenta tend to zero, also weaker kinematic
divergences, when only some of the external momenta vanish. The second solution
represents the recently proposed decoupling scenario where the gluons become
massive and the ghosts remain bare. In this case we find that none of the
vertex functions is enhanced, so that the infrared dynamics is entirely
suppressed. Our analysis also provides a strict argument why the Landau gauge
gluon dressing function cannot be infrared divergent.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:49:22 GMT"
},
{
"version": "v2",
"created": "Fri, 24 Oct 2008 17:27:29 GMT"
},
{
"version": "v3",
"created": "Fri, 29 Jan 2010 22:46:03 GMT"
},
{
"version": "v4",
"created": "Tue, 11 May 2010 02:16:56 GMT"
}
] | 2010-05-19T00:00:00 | [
[
"Alkofer",
"Reinhard",
""
],
[
"Huber",
"Markus Q.",
""
],
[
"Schwenzer",
"Kai",
""
]
] | [
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] |
801.2763 | Fabio Riccioni | Fabio Riccioni, Antoine Van Proeyen and Peter West | Real forms of very extended Kac-Moody algebras and theories with eight
supersymmetries | 46 pages, 25 figures. Refs added, one appendix included, one figure
added | JHEP 0805:079,2008 | 10.1088/1126-6708/2008/05/079 | KCL-MTH-08-01, KUL-TF-08/02 | hep-th | null | We consider all theories with eight supersymmetries whose reduction to three
dimensions gives rise to scalars that parametrise symmetric manifolds. We
conjecture that these theories are non-linear realisations of very-extended
Kac-Moody algebras for suitable choices of real forms. We show for the most
interesting cases that the bosonic sector of the supersymmetric theory is
precisely reproduced by the corresponding non-linear realisation.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 20:50:07 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 16:51:40 GMT"
},
{
"version": "v3",
"created": "Tue, 19 Feb 2008 18:12:50 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Riccioni",
"Fabio",
""
],
[
"Van Proeyen",
"Antoine",
""
],
[
"West",
"Peter",
""
]
] | [
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] |
801.2764 | Joshua Younger | J. D. Younger, J. S. Dunlop, A. B. Peck, R. J. Ivison, A. D. Biggs, E.
L. Chapin, D. L. Clements, S. Dye, T. R. Greve, D. H. Hughes, D. Iono, I.
Smail, M. Krips, G. R. Petitpas, D. Wilner, A. M. Schael, and C. D. Wilson | Clarifying the nature of the brightest submillimetre sources:
interferometric imaging of LH850.02 | MNRAS, in press | null | 10.1111/j.1365-2966.2008.13241.x | null | astro-ph | null | We present high-resolution interferometric imaging of LH850.02, the brightest
850- and 1200-micron submillimetre (submm) galaxy in the Lockman Hole. Our
observations were made at 890 micron with the Submillimetre Array (SMA). Our
high-resolution submm imaging detects LH850.02 at >6-sigma as a single compact
(size < 1 arcsec or < 8 kpc) point source and yields its absolute position to
~0.2-arcsec accuracy. LH850.02 has two alternative radio counterparts within
the SCUBA beam (LH850.02N & S), both of which are statistically very unlikely
to be so close to the SCUBA source position by chance. However, the precise
astrometry from the SMA shows that the submm emission arises entirely from
LH850.02N, and is not associated with LH850.02S (by far the brighter of the two
alternative identifications at 24-micron). Fits to the optical-infrared
multi-colour photometry of LH850.02N & S indicate that both lie at z~3.3, and
are therefore likely to be physically associated. At these redshifts, the 24
micron--to--submm flux density ratios suggest that LH850.02N has an Arp220-type
starburst-dominated far-IR SED, while LH850.02S is more similar to Mrk231, with
less dust-enshrouded star-formation activity, but a significant contribution at
24-micron (rest-frame ~5-6 micron) from an active nucleus. This complex mix of
star-formation and AGN activity in multi-component sources may be common in the
high redshift ultraluminous galaxy population, and highlights the need for
precise astrometry from high resolution interferometric imaging for a more
complete understanding.
| [
{
"version": "v1",
"created": "Fri, 18 Jan 2008 20:21:31 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Apr 2008 17:59:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Younger",
"J. D.",
""
],
[
"Dunlop",
"J. S.",
""
],
[
"Peck",
"A. B.",
""
],
[
"Ivison",
"R. J.",
""
],
[
"Biggs",
"A. D.",
""
],
[
"Chapin",
"E. L.",
""
],
[
"Clements",
"D. L.",
""
],
[
"Dye",
"S.",
""
],
[
"Greve",
"T. R.",
""
],
[
"Hughes",
"D. H.",
""
],
[
"Iono",
"D.",
""
],
[
"Smail",
"I.",
""
],
[
"Krips",
"M.",
""
],
[
"Petitpas",
"G. R.",
""
],
[
"Wilner",
"D.",
""
],
[
"Schael",
"A. M.",
""
],
[
"Wilson",
"C. D.",
""
]
] | [
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] |
801.2765 | Jeffrey Bary | Jeffrey S. Bary, David A. Weintraub, Sonali J. Shukla, Jarron M.
Leisenring, and Joel H. Kastner | Quiescent H2 Emission From Pre-Main Sequence Stars in Chamaeleon I | 12 pages, emulateapj, Accepted by ApJ | null | 10.1086/529517 | null | astro-ph | null | We report the discovery of quiescent emission from molecular hydrogen gas
located in the circumstellar disks of six pre-main sequence stars, including
two weak-line T Tauri stars (TTS), and one Herbig AeBe star, in the Chamaeleon
I star forming region. For two of these stars, we also place upper limits on
the 2->1 S(1)/1->0 S(1) line ratios of 0.4 and 0.5. Of the 11 pre-main sequence
sources now known to be sources of quiescent near-infrared hydrogen emission,
four possess transitional disks, which suggests that detectable levels of H$_2$
emission and the presence of inner disk holes are correlated. These H$_2$
detections demonstrate that these inner holes are not completely devoid of gas,
in agreement with the presence of observable accretion signatures for all four
of these stars and the recent detections of [Ne II] emission from three of
them. The overlap in [Ne II] and H$_2$ detections hints at a possible
correlation between these two features and suggests a shared excitation
mechanism of high energy photons. Our models, combined with the kinematic
information from the H$_2$ lines, locate the bulk of the emitting gas at a few
tens of AU from the stars. We also find a correlation between H$_2$ detections
and those targets which possess the largest H$\alpha$ equivalent widths,
suggesting a link between accretion activity and quiescent H$_2$ emission. We
conclude that quiescent H$_2$ emission from relatively hot gas within the disks
of TTS is most likely related to on-going accretion activity, the production of
UV photons and/or X-rays, and the evolutionary status of the dust grain
populations in the inner disks.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 21:00:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bary",
"Jeffrey S.",
""
],
[
"Weintraub",
"David A.",
""
],
[
"Shukla",
"Sonali J.",
""
],
[
"Leisenring",
"Jarron M.",
""
],
[
"Kastner",
"Joel H.",
""
]
] | [
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] |
801.2766 | Nicholas Abel | N. P. Abel, S. Satyapal | [Ne V] Emission in Optically Classified Starbursts | 16 pages, 3 figures, accepted for publication in ApJ;
astro-ph\0801.2759 (Satyapal et al. 2008; ApJ accepted) and this posting
designed to form a two-part investigation | null | 10.1086/529013 | null | astro-ph | null | Detecting Active Galactic Nuclei (AGN) in galaxies dominated by powerful
nuclear star formation and extinction effects poses a unique challenge. Due to
the longer wavelength emission and the ionization potential of Ne^3+, infrared
[Ne V] emission lines are thought to be excellent AGN diagnostics. However,
stellar evolution models predict Wolf-Rayet stars in young stellar clusters
emit significant numbers of photons capable of creating Ne^4+. Recent
observations of [Ne V] emission in optically classified starburst galaxies
require us to investigate whether [Ne V] can arise from star-formation activity
and not an AGN. In this work, we calculate the optical and IR spectrum of gas
exposed to a young starburst and AGN SED. We find: 1) a range of parameters
where [Ne V] emission can be explained solely by star-formation and 2) a range
of relative AGN to starburst luminosities that reproduce the [Ne V]
observations, yet leaves the optical spectrum looking like a starburst. We also
find infrared emission-line diagnostics are much more sensitive to the AGN than
optical diagnostics, particularly for weak AGN. We apply our model to the
optically classified, yet [Ne V] emitting, starburst galaxy NGC 3621. We find,
when taking the IR and optical spectrum into account, about 30 - 50% of the
galaxy's total luminosity is due to an AGN. Our calculations show that [Ne V]
emission is almost always the result of AGN activity. The models presented in
this work can be used to determine the AGN contribution to a galaxy's power
output.
| [
{
"version": "v1",
"created": "Fri, 18 Jan 2008 02:37:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Abel",
"N. P.",
""
],
[
"Satyapal",
"S.",
""
]
] | [
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] |
801.2767 | Jeronimo Bernard-Salas | S.R. Pottasch, J. Bernard-Salas, T.L. Roellig | Abundances of Planetary Nebula NGC2392 | 9 pages, 7 tables, 3 figures. Accepted for publication in A&A | null | 10.1051/0004-6361:20079041 | null | astro-ph | null | The spectra of the planetary nebula NGC2392 is reanalysed using spectral
measurements made in the mid-infrared with the Spitzer Space Telescope. The aim
is to determine the chemical composition of this object. We also make use of
IUE and ground based spectra. Abundances determined from the mid-infrared
lines, which are insensitive to electron temperature, are used as the basis for
the determination of the composition, which are found to differ somewhat from
earlier results. The abundances found, especially the low value of helium and
oxygen, indicate that the central star was originally of rather low mass.
Abundances of phosphorus, iron, silicon and chlorine have been determined for
the first time in this nebula. The variation of electron temperature in this
nebula is very clear reaching quite high values close to the center. The
temperature of the central star is discussed in the light of the high observed
stages of ionization. The nebular information indicates the spectrum of the
star deviates considerably from a blackbody.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 21:01:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Pottasch",
"S. R.",
""
],
[
"Bernard-Salas",
"J.",
""
],
[
"Roellig",
"T. L.",
""
]
] | [
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] |
801.2768 | Ladislav Subr | L. Subr, P. Kroupa, H. Baumgardt | A new method to create initially mass segregated star clusters in virial
equilibrium | 9 pages, 8 figures, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12993.x | null | astro-ph | null | Mass segregation stands as one of the most robust features of the dynamical
evolution of self-gravitating star clusters. In this paper we formulate
parametrised models of mass segregated star clusters in virial equilibrium. To
this purpose we introduce mean inter-particle potentials for statistically
described unsegregated systems and suggest a single-parameter generalisation of
its form which gives a mass-segregated state. We describe an algorithm for
construction of appropriate star cluster models. Their stability over several
crossing-times is verified by following the evolution by means of direct N-body
integration.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 21:01:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Subr",
"L.",
""
],
[
"Kroupa",
"P.",
""
],
[
"Baumgardt",
"H.",
""
]
] | [
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] |
801.2769 | Darren Croton J | Antonio D. Montero-Dorta, Darren J. Croton, Renbin Yan, Michael C.
Cooper, Jeffery A. Newman, Antonis Georgakakis, Francisco Prada, Marc Davis,
Kirpal Nandra, Alison Coil | The DEEP2 Galaxy Redshift Survey: The Red Sequence AGN Fraction and its
Environment and Redshift Dependence | 11 pages, 7 figures, submitted to MNRAS | null | 10.1111/j.1365-2966.2008.13893.x | null | astro-ph | null | We measure the dependence of the AGN fraction on local environment at z~1,
using spectroscopic data taken from the DEEP2 Galaxy Redshift Survey, and
Chandra X-ray data from the All-Wavelength Extended Groth Strip International
Survey (AEGIS). To provide a clean sample of AGN we restrict our analysis to
the red sequence population; this also reduces additional colour-environment
correlations. We find evidence that high redshift LINERs in DEEP2 tend to
favour higher density environments relative to the red population from which
they are drawn. In contrast, Seyferts and X-ray selected AGN at z~1 show little
(or no) environmental dependencies within the same underlying population. We
compare these results with a sample of local AGN drawn from the SDSS. Contrary
to the high redshift behaviour, we find that both LINERs and Seyferts in the
SDSS show a slowly declining red sequence AGN fraction towards high density
environments. Interestingly, at z~1 red sequence Seyferts and LINERs are
approximately equally abundant. By z~0, however, the red Seyfert population has
declined relative to the LINER population by over a factor of 7. We speculate
on possible interpretations of our results.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 21:02:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Montero-Dorta",
"Antonio D.",
""
],
[
"Croton",
"Darren J.",
""
],
[
"Yan",
"Renbin",
""
],
[
"Cooper",
"Michael C.",
""
],
[
"Newman",
"Jeffery A.",
""
],
[
"Georgakakis",
"Antonis",
""
],
[
"Prada",
"Francisco",
""
],
[
"Davis",
"Marc",
""
],
[
"Nandra",
"Kirpal",
""
],
[
"Coil",
"Alison",
""
]
] | [
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] |
801.277 | Claudio Dalla Vecchia | Claudio Dalla Vecchia, Joop Schaye (Leiden Observatory) | Simulating galactic outflows with kinetic supernova feedback | 15 pages, 11 figures, accepted for publication in MNRAS. Added 4 new
figures and made minor textual changes. Simulation videos available at
http://www.strw.leidenuniv.nl/DS08/ | Mon.Not.Roy.Astron.Soc.387:1431,2008 | 10.1111/j.1365-2966.2008.13322.x | null | astro-ph | null | Feedback from star formation is thought to play a key role in the formation
and evolution of galaxies, but its implementation in cosmological simulations
is currently hampered by a lack of numerical resolution. We present and test a
sub-grid recipe to model feedback from massive stars in cosmological smoothed
particle hydrodynamics simulations. The energy is distributed in kinetic form
among the gas particles surrounding recently formed stars. The impact of the
feedback is studied using a suite of high-resolution simulations of isolated
disc galaxies embedded in dark halos with total mass 10^{10} and 10^{12}
Msol/h. We focus in particular on the effect of pressure forces on wind
particles within the disc, which we turn off temporarily in some of our runs to
mimic a recipe that has been widely used in the literature. We find that this
popular recipe gives dramatically different results because (ram) pressure
forces on expanding superbubbles determine both the structure of the disc and
the development of large-scale outflows. Pressure forces exerted by expanding
superbubbles puff up the disc, giving the dwarf galaxy an irregular morphology
and creating a galactic fountain in the massive galaxy. Hydrodynamic drag
within the disc results in a strong increase of the effective mass loading of
the wind for the dwarf galaxy, but quenches much of the outflow in the case of
the high-mass galaxy.
| [
{
"version": "v1",
"created": "Fri, 18 Jan 2008 10:45:05 GMT"
},
{
"version": "v2",
"created": "Wed, 7 May 2008 13:21:47 GMT"
}
] | 2011-06-29T00:00:00 | [
[
"Vecchia",
"Claudio Dalla",
"",
"Leiden Observatory"
],
[
"Schaye",
"Joop",
"",
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801.2771 | Darren Croton J | Darren J. Croton, Glennys R. Farrar | Where do "red and dead" early-type void galaxies come from? | 6 pages, 3 figures, accepted MNRAS | Mon.Not.Roy.Astron.Soc.386:2285-2289,2008 | 10.1111/j.1365-2966.2008.13204.x | null | astro-ph | null | Void regions of the Universe offer a special environment for studying
cosmology and galaxy formation, which may expose weaknesses in our
understanding of these phenomena. Although galaxies in voids are observed to be
predominately gas rich, star forming and blue, a sub-population of bright red
void galaxies can also be found, whose star formation was shut down long ago.
Are the same processes that quench star formation in denser regions of the
Universe also at work in voids?
We compare the luminosity function of void galaxies in the 2dF Galaxy
Redshift Survey, to those from a galaxy formation model built on the Millennium
Simulation. We show that a global star formation suppression mechanism in the
form of low luminosity "radio mode" AGN heating is sufficient to reproduce the
observed population of void early-types. Radio mode heating is environment
independent other than its dependence on dark matter halo mass, where, above a
critical mass threshold of approximately M_vir~10^12.5 M_sun, gas cooling onto
the galaxy is suppressed and star formation subsequently fades. In the
Millennium Simulation, the void halo mass function is shifted with respect to
denser environments, but still maintains a high mass tail above this critical
threshold. In such void halos, radio mode heating remains efficient and red
galaxies are found; collectively these galaxies match the observed space
density without any modification to the model. Consequently, galaxies living in
vastly different large-scale environments but hosted by halos of similar mass
are predicted to have similar properties, consistent with observations.
| [
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},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 22:24:22 GMT"
},
{
"version": "v3",
"created": "Fri, 30 May 2008 06:37:50 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Croton",
"Darren J.",
""
],
[
"Farrar",
"Glennys R.",
""
]
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801.2772 | Tanja Cuk | T. Cuk, V. Struzhkin, T.P. Devereaux, A. Goncharov, C. Kendziora, H.
Eisaki, H. Mao, and Z.-X. Shen | Uncovering a pressure-tuned electronic transition in BiSrYCu2O8 using
Raman scattering and x-ray diffraction | 5 pages, 4 figures, submitted to PRL | null | 10.1103/PhysRevLett.100.217003 | null | cond-mat.supr-con | null | We report pressure tuned Raman and x-ray diffraction data of
Bi1.98Sr2.06Y0.68Cu2O8 revealing a critical pressure at 21 GPa with anomalies
in six physical quantities: electronic Raman background, electron-phonon
coupling, spectral weight transfer from high to low frequency, density
dependent behaviour of phonon and magnon frequencies, and a compressibility
change in the c-axis. For the first time in a cuprate, mobile charge carriers,
lattice, and magnetism all show anomalies at a distinct critical pressure in
the same experimental setting. Furthermore, the Raman spectral changes are
similar to that seen traversing the superconducting dome with doping,
suggesting that the critical pressure at 21 GPa is related to the much
discussed critical point at optimal doping.
| [
{
"version": "v1",
"created": "Thu, 17 Jan 2008 21:27:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cuk",
"T.",
""
],
[
"Struzhkin",
"V.",
""
],
[
"Devereaux",
"T. P.",
""
],
[
"Goncharov",
"A.",
""
],
[
"Kendziora",
"C.",
""
],
[
"Eisaki",
"H.",
""
],
[
"Mao",
"H.",
""
],
[
"Shen",
"Z. -X.",
""
]
] | [
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