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711.2908 | Shin'ichiro Ando | Shin'ichiro Ando (Caltech), John F. Beacom (Ohio State), Stefano
Profumo (UCSC/Caltech), David Rainwater (Rochester) | Probing new physics with long-lived charged particles produced by
atmospheric and astrophysical neutrinos | 27 pages, 6 figures; accepted for publication in JCAP | JCAP 0804:029,2008 | 10.1088/1475-7516/2008/04/029 | null | hep-ph astro-ph | null | As suggested by some extensions of the Standard Model of particle physics,
dark matter may be a super-weakly interacting lightest stable particle, while
the next-to-lightest particle (NLP) is charged and meta-stable. One could test
such a possibility with neutrino telescopes, by detecting the charged NLPs
produced in high-energy neutrino collisions with Earth matter. We study the
production of charged NLPs by both atmospheric and astrophysical neutrinos;
only the latter, which is largely uncertain and has not been detected yet, was
the focus of previous studies. We compute the resulting fluxes of the charged
NLPs, compare those of different origins, and analyze the dependence on the
underlying particle physics setup. We point out that even if the astrophysical
neutrino flux is very small, atmospheric neutrinos, especially those from the
prompt decay of charmed mesons, may provide a detectable flux of NLP pairs at
neutrino telescopes such as IceCube. We also comment on the flux of charged
NLPs expected from proton-nucleon collisions, and show that, for theoretically
motivated and phenomenologically viable models, it is typically sub-dominant
and below detectable rates.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 20:04:33 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Mar 2008 19:21:25 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Ando",
"Shin'ichiro",
"",
"Caltech"
],
[
"Beacom",
"John F.",
"",
"Ohio State"
],
[
"Profumo",
"Stefano",
"",
"UCSC/Caltech"
],
[
"Rainwater",
"David",
"",
"Rochester"
]
] | [
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711.2909 | Krzysztof R. Apt | Krzysztof R. Apt, Francesca Rossi, Kristen Brent Venable | Comparing the notions of optimality in CP-nets, strategic games and soft
constraints | 39 pages. To appear in Annals of Mathematics and Artificial
Intelligence | null | null | null | cs.AI cs.GT | null | The notion of optimality naturally arises in many areas of applied
mathematics and computer science concerned with decision making. Here we
consider this notion in the context of three formalisms used for different
purposes in reasoning about multi-agent systems: strategic games, CP-nets, and
soft constraints. To relate the notions of optimality in these formalisms we
introduce a natural qualitative modification of the notion of a strategic game.
We show then that the optimal outcomes of a CP-net are exactly the Nash
equilibria of such games. This allows us to use the techniques of game theory
to search for optimal outcomes of CP-nets and vice-versa, to use techniques
developed for CP-nets to search for Nash equilibria of the considered games.
Then, we relate the notion of optimality used in the area of soft constraints
to that used in a generalization of strategic games, called graphical games. In
particular we prove that for a natural class of soft constraints that includes
weighted constraints every optimal solution is both a Nash equilibrium and
Pareto efficient joint strategy. For a natural mapping in the other direction
we show that Pareto efficient joint strategies coincide with the optimal
solutions of soft constraints.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:14:27 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Apr 2008 10:47:41 GMT"
}
] | 2008-04-21T00:00:00 | [
[
"Apt",
"Krzysztof R.",
""
],
[
"Rossi",
"Francesca",
""
],
[
"Venable",
"Kristen Brent",
""
]
] | [
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711.291 | Sergey Storchak | S. N. Storchak | Path integral measure factorization in path integrals for diffusion of
Yang--Mills fields | 34 pages | null | null | null | hep-th | null | Factorization of the (formal) path integral measure in a Wiener path
integrals for Yang--Mills diffusion is studied. Using the nonlinear filtering
stochastic differential equation, we perform the transformation of the path
integral defined on a total space of the Yang--Mills principal fiber bundle and
come to the reduced path integral on a Coulomb gauge surface. Integral relation
between the path integral representing the "quantum" evolution given on the
original manifold of Yang--Mills fields and the path integral on the reduced
manifold defined by the Coulomb gauge is obtained.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:17:00 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Storchak",
"S. N.",
""
]
] | [
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711.2911 | Daniel Lawson | Daniel John Lawson and Henrik Jeldtoft Jensen | Understanding clustering in type space using field theoretic techniques | Accepted, Bulletin of Mathematical Biology | null | null | null | q-bio.PE q-bio.QM | null | The birth/death process with mutation describes the evolution of a
population, and displays rich dynamics including clustering and fluctuations.
We discuss an analytical `field-theoretical' approach to the birth/death
process, using a simple dimensional analysis argument to describe evolution as
a `Super-Brownian Motion' in the infinite population limit. The field theory
technique provides corrections to this for large but finite population, and an
exact description at arbitrary population size. This allows a characterisation
of the difference between the evolution of a phenotype, for which strong local
clustering is observed, and a genotype for which distributions are more
dispersed. We describe the approach with sufficient detail for non-specialists.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:17:54 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Lawson",
"Daniel John",
""
],
[
"Jensen",
"Henrik Jeldtoft",
""
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711.2912 | Viktor Begun | Viktor V. Begun | Multiplicity fluctuations in relativistic gases. From simple models to
experiment | To appear in the proceedings of The International Workshop
Relativistic Nuclear Physics: from Nuclotron to LHC energies, Bogolyubov
Institute for Theoretical Physics, Kiev, Ukraine, June 18-22, 2007 | Phys.Atom.Nucl.71:1813-1823,2008 | 10.1134/S1063778808100165 | null | nucl-th | null | The aim of this paper is to give a short overview for the set of publications
considering recently found effect of non-equivalence of multiplicity
fluctuations in relativistic gases with globally conserved charge and energy.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:20:59 GMT"
}
] | 2009-05-29T00:00:00 | [
[
"Begun",
"Viktor V.",
""
]
] | [
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711.2913 | Michael Tung M. | M.M. Tung, L. Soler, E. Defez, and A. Hervas | Cubic-matrix splines and second-order matrix models | 5 pages | Progress in Industrial Mathematics at ECMI 2006 (edited by L. L.
Bonilla, M. A. Moscoso, G. Platero, and J. M. Vega), vol. 12 of Mathematics
in Industry, pp. 949-953 (Springer, Berlin, 2007), ISBN 978-3-540-71991-5 | null | null | math.NA | null | We discuss the direct use of cubic-matrix splines to obtain continuous
approximations to the unique solution of matrix models of the type $Y''(x) =
f(x,Y(x))$. For numerical illustration, an estimation of the approximation
error, an algorithm for its implementation, and an example are given.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:22:18 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Tung",
"M. M.",
""
],
[
"Soler",
"L.",
""
],
[
"Defez",
"E.",
""
],
[
"Hervas",
"A.",
""
]
] | [
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] |
711.2914 | Tshilidzi Marwala | Gidudu Anthony, Hulley Gregg and Marwala Tshilidzi | Image Classification Using SVMs: One-against-One Vs One-against-All | Proccedings of the 28th Asian Conference on Remote Sensing, 2007 | null | null | null | cs.LG cs.AI cs.CV | null | Support Vector Machines (SVMs) are a relatively new supervised classification
technique to the land cover mapping community. They have their roots in
Statistical Learning Theory and have gained prominence because they are robust,
accurate and are effective even when using a small training sample. By their
nature SVMs are essentially binary classifiers, however, they can be adopted to
handle the multiple classification tasks common in remote sensing studies. The
two approaches commonly used are the One-Against-One (1A1) and One-Against-All
(1AA) techniques. In this paper, these approaches are evaluated in as far as
their impact and implication for land cover mapping. The main finding from this
research is that whereas the 1AA technique is more predisposed to yielding
unclassified and mixed pixels, the resulting classification accuracy is not
significantly different from 1A1 approach. It is the authors conclusion
therefore that ultimately the choice of technique adopted boils down to
personal preference and the uniqueness of the dataset at hand.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:25:00 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Anthony",
"Gidudu",
""
],
[
"Gregg",
"Hulley",
""
],
[
"Tshilidzi",
"Marwala",
""
]
] | [
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] |
711.2915 | John Chick | J. M. Chick | Carmichael number variable relations: three-prime Carmichael numbers up
to 10^24 | 37 pages; 5 tables; amended version contains a minor factual
correction on page 25 immediately before Challenge 4, an updated reference
and 6 very minor textual improvements | null | null | null | math.NT | null | Bounds and other relations involving variables connected with Carmichael
numbers are reviewed and extended. Families of numbers or individual numbers
attaining or approaching these bounds are given. A new algorithm for finding
three-prime Carmichael numbers is described, with its implementation up to
$10^{24}$. Statistics relevant to the distribution of three-prime Carmichael
numbers are given, with particular reference to the conjecture of Granville and
Pomerance in [A.Granville and C.Pomerance, Two contradictory conjectures
concerning Carmichael numbers, Math. Comp. 71 (2001), 883-908].
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:26:48 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Feb 2008 12:02:14 GMT"
}
] | 2008-02-27T00:00:00 | [
[
"Chick",
"J. M.",
""
]
] | [
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] |
711.2916 | Eric Wille | E. Wille, F.M. Spiegelhalder, G. Kerner, D. Naik, A. Trenkwalder, G.
Hendl, F. Schreck, R. Grimm, T.G. Tiecke, J.T.M. Walraven, S.J.J.M.F.
Kokkelmans, E. Tiesinga, P.S. Julienne | Exploring an ultracold Fermi-Fermi mixture: Interspecies Feshbach
resonances and scattering properties of 6Li and 40K | 4 pages, 4 figures, 1 table | Phys. Rev. Lett. 100, 053201 (2008) | 10.1103/PhysRevLett.100.053201 | null | cond-mat.other | null | We report on the observation of Feshbach resonances in an ultracold mixture
of two fermionic species, 6Li and 40K. The experimental data are interpreted
using a simple asymptotic bound state model and full coupled channels
calculations. This unambiguously assigns the observed resonances in terms of
various s- and p-wave molecular states and fully characterizes the ground-state
scattering properties in any combination of spin states.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 20:34:12 GMT"
},
{
"version": "v2",
"created": "Fri, 1 Feb 2008 13:05:49 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Wille",
"E.",
""
],
[
"Spiegelhalder",
"F. M.",
""
],
[
"Kerner",
"G.",
""
],
[
"Naik",
"D.",
""
],
[
"Trenkwalder",
"A.",
""
],
[
"Hendl",
"G.",
""
],
[
"Schreck",
"F.",
""
],
[
"Grimm",
"R.",
""
],
[
"Tiecke",
"T. G.",
""
],
[
"Walraven",
"J. T. M.",
""
],
[
"Kokkelmans",
"S. J. J. M. F.",
""
],
[
"Tiesinga",
"E.",
""
],
[
"Julienne",
"P. S.",
""
]
] | [
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] |
711.2917 | Anne-Marie Vercoustre | James A. Thom (RMIT), Jovan Pehcevski (INRIA Rocquencourt / INRIA
Sophia Antipolis), Anne-Marie Vercoustre (INRIA Rocquencourt / INRIA Sophia
Antipolis) | Use of Wikipedia Categories in Entity Ranking | null | Dans The 12th Australasian Document Computing Symposium (ADCS'07)
(2007) | null | null | cs.IR | null | Wikipedia is a useful source of knowledge that has many applications in
language processing and knowledge representation. The Wikipedia category graph
can be compared with the class hierarchy in an ontology; it has some
characteristics in common as well as some differences. In this paper, we
present our approach for answering entity ranking queries from the Wikipedia.
In particular, we explore how to make use of Wikipedia categories to improve
entity ranking effectiveness. Our experiments show that using categories of
example entities works significantly better than using loosely defined target
categories.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:35:48 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Thom",
"James A.",
"",
"RMIT"
],
[
"Pehcevski",
"Jovan",
"",
"INRIA Rocquencourt / INRIA\n Sophia Antipolis"
],
[
"Vercoustre",
"Anne-Marie",
"",
"INRIA Rocquencourt / INRIA Sophia\n Antipolis"
]
] | [
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] |
711.2918 | Yanyang Zhang | Yan-Yang Zhang, Jiang-Ping Hu, B.A. Bernevig, X. R. Wang, X. C. Xie
and W. M. Liu | Quantum Blockades and Loop Currents in Graphene with Topological Defects | 6 pages, 7 figures | Phys. Rev. B 78, 155413 (2008) | 10.1103/PhysRevB.78.155413 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the effect of topological defects on the transport properties
of a narrow ballistic ribbon of graphene with zigzag edges. Our results show
that the longitudinal conductance vanishes at several discrete Fermi energies
where the system develops loop orbital electric currents with certain
chirality. The chirality depends on the direction of the applied bias voltage
and the sign of the local curvature created by the topological defects. This
novel quantum blockade phenomenon provides a new way to generate a magnetic
moment by an external electric field, which can prove useful in carbon
electronics.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:37:36 GMT"
},
{
"version": "v2",
"created": "Tue, 20 Nov 2007 01:42:37 GMT"
},
{
"version": "v3",
"created": "Sat, 11 Oct 2008 03:32:52 GMT"
}
] | 2008-10-11T00:00:00 | [
[
"Zhang",
"Yan-Yang",
""
],
[
"Hu",
"Jiang-Ping",
""
],
[
"Bernevig",
"B. A.",
""
],
[
"Wang",
"X. R.",
""
],
[
"Xie",
"X. C.",
""
],
[
"Liu",
"W. M.",
""
]
] | [
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] |
711.2919 | Charles Bonatto | Charles Bonatto and Eduardo Bica | Structural parameters of star clusters: relations among light, mass and
star-count radial profiles and the dependence on photometric depth | 10 pages and 9 figures. Accepted by A&A | null | 10.1051/0004-6361:20078616 | null | astro-ph | null | Structural parameters of model star clusters are measured in radial profiles
built from number-density, mass-density and surface-brightness distributions,
assuming as well different photometric conditions. Star clusters of different
ages, structure and mass functions are modelled by assuming that the radial
distribution of stars follows a pre-defined analytical form. Near-infrared
surface brightness and mass-density profiles result from mass-luminosity
relations taken from a set of isochrones. Core, tidal and half-light, half-mass
and half-star count radii, together with the concentration parameter, are
measured in the three types of profiles, which are built under different
photometric depths. While surface-brightness profiles are almost insensitive to
photometric depth, radii measured in number-density and mass-density profiles
change significantly with it. Compared to radii derived with deep photometry,
shallow profiles result in lower values. This effect increases for younger
ages. Radial profiles of clusters with a spatially-uniform mass function
produce radii that do not depend on depth. With deep photometry, number-density
profiles yield radii systematically larger than those derived from
surface-brightness ones. In general, low-noise surface-brightness profiles
result in uniform structural parameters that are essentially independent of
photometric depth. For less-populous star clusters, those projected against
dense fields and/or distant ones, which result in noisy surface-brightness
profiles, this work provides a quantitative way to estimate the intrinsic radii
by means of number-density profiles built with depth-limited photometry.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:54:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bonatto",
"Charles",
""
],
[
"Bica",
"Eduardo",
""
]
] | [
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] |
711.292 | Shuichiro Yokoyama | Shuichiro Yokoyama, Teruaki Suyama, Takahiro Tanaka | Primordial Non-Gaussianity in Multi-Scalar Inflation | 11 pages, 6 figures, few typos fixed | null | null | KUNS-2110 | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a concise formula for the non-Gaussianity of the primordial curvature
perturbation generated on super-horizon scales in multi-scalar inflation model
without assuming slow-roll conditions. This is an extension of our previous
work. Using this formula, we study the generation of non-Gaussianity for the
double inflation models in which the slow-roll conditions are temporarily
violated after horizon exit, and we show that the non-linear parameter $f_{NL}$
for such models is suppressed by the slow-roll parameters evaluated at the time
of horizon exit.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:54:57 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Apr 2008 14:14:31 GMT"
},
{
"version": "v3",
"created": "Thu, 10 Jan 2013 03:35:08 GMT"
}
] | 2013-01-11T00:00:00 | [
[
"Yokoyama",
"Shuichiro",
""
],
[
"Suyama",
"Teruaki",
""
],
[
"Tanaka",
"Takahiro",
""
]
] | [
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] |
711.2921 | Zhi-Gang Wang | Zhi-Gang Wang, Zhi-Bin Wang | Electromagnetic form-factor of the $\pi$ meson with light-cone QCD sum
rules | 16 pages, 3 figures, 5 version | Int.J.Mod.Phys.A23:4621-4636,2008 | 10.1142/S0217751X08041499 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this article, we calculate the electromagnetic form-factor of the $\pi$
meson with the light-cone QCD sum rules. The numerical value $F_\pi^{p}(0)
=0.999\pm 0.001$ is in excellent agreement with the experimental data
(extrapolated to the limit of zero momentum transfer, or the normalization
condition $F_\pi(0)=1$). For large momentum transfers, the values from the two
sum rules are all comparable with the experimental data and theoretical
estimations.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 12:59:04 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 02:14:06 GMT"
},
{
"version": "v3",
"created": "Thu, 1 May 2008 07:47:59 GMT"
},
{
"version": "v4",
"created": "Tue, 13 May 2008 10:44:21 GMT"
},
{
"version": "v5",
"created": "Sat, 14 Jun 2008 03:20:27 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Wang",
"Zhi-Gang",
""
],
[
"Wang",
"Zhi-Bin",
""
]
] | [
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0.0131693045,
-0.0017520078,
0.0685873404,
0.1423443556,
-0.0975999236,
0.040800333,
0.1121284962,
0.0243331306,
0.0416916572,
-0.0920737162,
-0.0418476388
] |
711.2922 | Richard Pettigrew | J. P. Mayberry and Richard Pettigrew | Natural Number Arithmetic in the Theory of Finite Sets | 53 pages; second version; section 6 added; section 12 revised;
material added on connection with bounded arithmetic | null | null | null | math.LO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We describe a theory of finite sets, and investigate the analogue of
Dedekind's theory of natural number systems (simply infinite systems) in this
theory. Unlike the infinitary case, in our theory, natural number systems come
in differing lengths and with different closure properties. We give examples of
natural number systems incomparable in length; we define hierarchies of natural
number systems closed under increasingly powerful functions; and we describe a
method by which to construct natural number systems with given closure
properties. These natural number systems form natural models for various
systems of weak arithmetic.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:29:18 GMT"
},
{
"version": "v2",
"created": "Fri, 8 Aug 2008 10:47:06 GMT"
}
] | 2008-08-08T00:00:00 | [
[
"Mayberry",
"J. P.",
""
],
[
"Pettigrew",
"Richard",
""
]
] | [
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] |
711.2923 | Brent Miszalski | B. Miszalski, Q. A. Parker, A. Acker, J. L. Birkby, D. J. Frew and A.
Kovacevic | MASH-II: More Planetary Nebulae from the AAO/UKST H\alpha Survey | 10 pages, 8 figures. Accepted for publication in MNRAS. Catalogue
will be available from vizier | null | 10.1111/j.1365-2966.2007.12727.x | null | astro-ph | null | We present a supplement to the Macquarie/AAO/Strasbourg H$\alpha$ planetary
nebulae (PNe) catalogue (MASH), which we denote MASH-II. The supplement
consists of over 300 true, likely and possible new Galactic PNe found after
re-examination of the entire AAO/UKST H$\alpha$ survey of the southern Galactic
Plane in digital form. We have spectroscopically confirmed over 240 of these
new candidates as bona-fide PNe and we include other high quality candidates
awaiting spectroscopic confirmation as possible PNe. These latest discoveries
largely comprise two distinct groups: small, star-like or moderately resolved
PNe at one end and mostly large, extremely low surface brightness PNe at the
other. Neither group were easy to discover from simple visual scrutiny of the
original survey exposures as for MASH but were relatively straightforward to
uncover from the digital images via application of semi-automated discovery
techniques. We suspect the few PNe still hidden in the H$\alpha$ survey will
lie outside our search criteria or be difficult to find.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:19:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Miszalski",
"B.",
""
],
[
"Parker",
"Q. A.",
""
],
[
"Acker",
"A.",
""
],
[
"Birkby",
"J. L.",
""
],
[
"Frew",
"D. J.",
""
],
[
"Kovacevic",
"A.",
""
]
] | [
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] |
711.2924 | Hao Yanhong | Huihui Dai, Yanhong Hao, Zhen Chen | On Constructing the Analytical Solutions for Localizations in a Slender
Cylinder Composed of an Incompressible Hyperelastic Material | 27 pages 10 figures | null | null | null | physics.class-ph physics.comp-ph | null | In this paper, we study the localization phenomena in a slender cylinder
composed of an incompressible hyperelastic material subjected to axial tension.
We aim to construct the analytical solutions based on a three-dimensional
setting and use the analytical results to describe the key features observed in
the experiments by others. Using a novel approach of coupled series-asymptotic
expansions, we derive the normal form equation of the original governing
nonlinear partial differential equations. By writing the normal form equation
into a first-order dynamical system and with the help of the phase plane, we
manage to solve two boundary-value problems analytically. The explicit solution
expressions (in terms of integrals) are obtained. By analyzing the solutions,
we find that the width of the localization zone depends on the material
parameters but remains almost unchanged for the same material in the post-peak
region. Also, it is found that when the radius-length ratio is relatively small
there is a snap-back phenomenon. These results are well in agreement with the
experimental observations. Through an energy analysis, we also deduce the
preferred configuration and give a prediction when a snap-through can happen.
Finally, based on the maximum-energy-distortion theory, an analytical criterion
for the onset of material failure is provided.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:21:18 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Dai",
"Huihui",
""
],
[
"Hao",
"Yanhong",
""
],
[
"Chen",
"Zhen",
""
]
] | [
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711.2925 | Werner Mueller | Erez Lapid, Werner Mueller | Spectral asymptotics for arithmetic quotients of SL(n,R)/SO(n) | 31 pages | Duke Math. J. 149, no. 1 (2009), 117-155 | 10.1215/00127094-2009-037 | null | math.RT math.SP | null | In this paper we study the asymptotic distribution of the cuspidal spectrum
of arithmetic quotients of the symmetric space S=SL(n,R)/SO(n). In particular,
we obtain Weyl's law with an estimation on the remainder term. This extends
results of Duistermaat-Kolk-Varadarajan on spectral asymptotics for compact
locally symmetric spaces to this non-compact setting.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:21:53 GMT"
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] | 2019-12-19T00:00:00 | [
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711.2926 | I. Rotter | Ingrid Rotter | Non-Hermitian Hamilton operator in open quantum systems | 24 pages | null | null | null | quant-ph | null | In the Feshbach projection operator (FPO) formalism the whole function space
is divided into two subspaces. One of them contains the wave functions
localized in a certain finite region while the continuum of extended scattering
wave functions is involved in the other subspace. The Hamilton operator of the
whole system is Hermitian, that of the localized part is, however,
non-Hermitian. This non-Hermitian Hamilton operator $H_{\rm eff}$ represents
the core of the FPO method in present-day studies. It gives a unified
description of discrete and resonance states. Furthermore, it contains the time
operator. The eigenvalues $z_\lambda$ and eigenfunctions $\phi_\lambda$ of
$H_{\rm eff}$ are an important ingredient of the $S$ matrix. They are energy
dependent. The phases of the $\phi_\lambda$ are, generally, nonrigid. Most
interesting physical effects are caused by the branch points in the complex
plane. On the one hand, they cause the avoided level crossings that appear as
level repulsion or widths bifurcation in approaching the branch points under
different conditions. On the other hand, observable values are usually enhanced
and accelerated in the vicinity of the branch points. In most cases, the theory
is time asymmetric. An exception are the ${\cal PT}$ symmetric bound states in
the continuum appearing in space symmetric systems due to the avoided level
crossing phenomenon in the complex plane. In the paper, the peculiarities of
the FPO method are considered and three typical phenomena are sketched: (i) the
unified description of decay and scattering processes, (ii) the appearance of
bound states in the continuum and (iii) the spectroscopic reordering processes
characteristic of the regime with overlapping resonances.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:34:12 GMT"
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711.2927 | Thomas Larsson | T. A. Larsson | A BV subtlety | 8 pages | null | null | null | math-ph math.MP | null | The standard BV complex is never acyclic provided that the equations of
motion have solutions and the admissible class of functions is general enough,
unless one introduces second-order antifields. This phenomenon is explicitly
illustrated for the harmonic oscillator and the free electromagnetic field.
| [
{
"version": "v1",
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] |
711.2928 | Jonathan Bowden | Jonathan Bowden | The topology of symplectic circle bundles | null | Trans. Amer. Math. Soc. 361 (2009), no. 10, 5457--5468 | null | null | math.GT math.SG | null | We consider circle bundles over compact three-manifolds with symplectic total
spaces. We show that the base of such a space must be irreducible or the
product of the two-sphere with the circle. We then deduce that such a bundle
admits a symplectic form if and only if it admits one that is invariant under
the circle action in three special cases: namely if the base is Seifert
fibered, has vanishing Thurston norm, or if the total space admits a Lefschetz
fibration.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:45:26 GMT"
}
] | 2011-05-19T00:00:00 | [
[
"Bowden",
"Jonathan",
""
]
] | [
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] |
711.2929 | Matthias Liebendoerfer | M. Liebendoerfer, S. C. Whitehouse, T. Fischer | The isotropic diffusion source approximation for supernova neutrino
transport | revised version, 19 pages, 10 figures, submitted to ApJ | Astrophys.J.698:1174-1190,2009 | 10.1088/0004-637X/698/2/1174 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Astrophysical observations originate from matter that interacts with
radiation or transported particles. We develop a pragmatic approximation in
order to enable multi-dimensional simulations with basic spectral radiative
transfer when the computational resources are not sufficient to solve the
complete Boltzmann transport equation. The distribution function of the
transported particles is decomposed into trapped and streaming particle
components. Their separate evolution equations are coupled by a source term
that converts trapped particles into streaming particles. We determine this
source term by requiring the correct diffusion limit. For a smooth transition
to the free streaming regime, this 'diffusion source' is limited by the matter
emissivity. The resulting streaming particle emission rates are integrated over
space to obtain the streaming particle flux. A geometric estimate of the flux
factor is used to convert the particle flux to the streaming particle density.
The efficiency of the scheme results from the freedom to use different
approximations for each particle component. In supernovae, reactions with
trapped particles on fast time scales establish equilibria that reduce the
number of primitive variables required to evolve the trapped particle
component. On the other hand, a stationary-state approximation facilitates the
treatment of the streaming particle component. Different approximations may
apply in applications to stellar atmospheres, star formation, or cosmological
radiative transfer. We compare the isotropic diffusion source approximation
with Boltzmann neutrino transport of electron flavour neutrinos in spherically
symmetric supernova models and find good agreement. An extension of the scheme
to the multi-dimensional case is also discussed.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:45:53 GMT"
},
{
"version": "v2",
"created": "Wed, 21 Jan 2009 21:32:04 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Liebendoerfer",
"M.",
""
],
[
"Whitehouse",
"S. C.",
""
],
[
"Fischer",
"T.",
""
]
] | [
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] |
711.293 | Daniel Senff | D. Senff, P. Link, N. Aliouane, D. N. Argyriou, and M. Braden | Field dependence of magnetic correlations through the polarization flop
transition in multiferroic TbMnO3 : evidence for a magnetic memory effect | 4 pages, 4 figures | null | 10.1103/PhysRevB.77.174419 | null | cond-mat.str-el | null | The field-induced multiferroic transition in TbMnO3 has been studied by
neutron scattering. Apart strong hysteresis, the magnetic transition associated
with the flop of electronic polarization exhibits a memory effect: after a
field sweep, TbMnO3 does not exhibit the same phase as that obtained by
zero-field cooling. The strong changes in the magnetic excitations across the
transition perfectly agree with a rotation of the cycloidal spiral plane
indicating that the inverse Dzyaloshinski-Moriya coupling causes the giant
magnetoelectric effect at the field-induced transition. The analysis of the
zone-center magnetic excitations identifies the electromagnon of the
multiferroic high-field phase.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 13:47:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Senff",
"D.",
""
],
[
"Link",
"P.",
""
],
[
"Aliouane",
"N.",
""
],
[
"Argyriou",
"D. N.",
""
],
[
"Braden",
"M.",
""
]
] | [
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711.2931 | Francesco Knechtli | F. Knechtli, N. Irges and M. Luz | New Higgs mechanism from the lattice | 7 pages, 5 figures. Presented at International Europhysics Conference
on High Energy Physics (EPS-HEP2007), Manchester, England, 19-25 Jul 2007 | J.Phys.Conf.Ser.110:102006,2008 | 10.1088/1742-6596/110/10/102006 | WUB/07-10 | hep-ph hep-lat | null | Spontaneous symmetry breaking has been observed in lattice simulations of
five-dimensional gauge theories on an orbifold. This effect is reproduced by
perturbation theory if it is modified to account for a finite cut-off. We
present a comparison of lattice and analytic results for bulk gauge group
SU(2).
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711.2932 | Marco Castellani | M. Castellani | Galactic Globular Clusters Database: a progress report | 3 pages, proceedings of "XXI Century challenges for stellar
evolution" (Cefalu', Italy), eds. S. Cassisi and M. Salaris, to be published
in MemSAIt, 79, 2. See http://www.mporzio.astro.it/~marco/gc/papers/ for a
PDF version with encapsulated figures | null | null | null | astro-ph | null | The present status of Galactic Globular Clusters Database is briefly
reviewed. The features implemented at the time writing are described, as well
as plans for future improvements.
| [
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711.2933 | Zsolt Szep | G. Fejos, A. Patkos, Zs. Szep | Renormalisability of the 2PI-Hartree approximation of multicomponent
scalar models in the broken symmetry phase | 21 pages, no figures, version accepted for publication in Nucl. Phys.
A | Nucl.Phys.A803:115-135,2008 | 10.1016/j.nuclphysa.2008.01.028 | null | hep-ph | null | Non-perturbative renormalisation of a general class of scalar field theories
is performed at the Hartree level truncation of the 2PI effective action in the
broken symmetry regime. Renormalised equations are explicitly constructed for
the one- and two-point functions. The non-perturbative counterterms are deduced
from the conditions for the cancellation of the overall and the subdivergences
in the complete Hartree-Dyson-Schwinger equations, with a transparent method.
The procedure proposed in the present paper is shown to be equivalent to the
iterative renormalisation method of Blaizot et al., Nucl. Phys. A736 (2004)
149.
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] |
711.2934 | Davide Fioravanti | Diego Bombardelli, Davide Fioravanti and Marco Rossi | Non-linear integral equations in {\cal {N}}=4 SYM | RAQIS '07 Prooceedings Contribution with some new results | null | null | null | hep-th | null | We survey and discuss the applications of the non-linear integral equation in
the framework of the Bethe Ansatz type equations which are conjectured to give
the eigenvalues of the dilatation operator in ${\cal {N}}=4$ SYM. Moreover, an
original idea (different from that of \cite {FMQR}) to derive a non-linear
integral equation is briefly depicted in Section 4.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:00:23 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Bombardelli",
"Diego",
""
],
[
"Fioravanti",
"Davide",
""
],
[
"Rossi",
"Marco",
""
]
] | [
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] |
711.2935 | Toru Goto | Toru Goto (KEK), Yasuhiro Okada (KEK, Sokendai), Tetsuo Shindou (DESY)
and Minoru Tanaka (Osaka U) | Patterns of flavor signals in supersymmetric models | 52 pages, 17 figures, 5 tables | Phys.Rev.D77:095010,2008 | 10.1103/PhysRevD.77.095010 | KEK-TH-1198, DESY 07-201, OU-HET-590-2007 | hep-ph | null | Quark and lepton flavor signals are studied in four supersymmetric models,
namely the minimal supergravity model, the minimal supersymmetric standard
model with right-handed neutrinos, SU(5) supersymmetric grand unified theory
with right-handed neutrinos and the minimal supersymmetric standard model with
U(2) flavor symmetry. We calculate b --> s(d) transition observables in B_d and
B_s decays, taking the constraint from the B_s--B_s-bar mixing recently
observed at Tevatron into account. We also calculate lepton flavor violating
processes mu --> e gamma, tau --> mu gamma and tau --> e gamma for the models
with right-handed neutrinos. We investigate possibilities to distinguish the
flavor structure of the supersymmetry breaking sector with use of patterns of
various flavor signals which are expected to be measured in experiments such as
MEG, LHCb and a future Super B Factory.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:09:05 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 15:33:36 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Goto",
"Toru",
"",
"KEK"
],
[
"Okada",
"Yasuhiro",
"",
"KEK, Sokendai"
],
[
"Shindou",
"Tetsuo",
"",
"DESY"
],
[
"Tanaka",
"Minoru",
"",
"Osaka U"
]
] | [
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] |
711.2936 | G\'abor Kupi | G\'abor Kupi | Determination of the upper and lower bound of masslimit of degenerate
fermionic dark matter objects | null | Phys.Rev.D77:023001,2008 | 10.1103/PhysRevD.77.023001 | null | astro-ph | null | We give a gravitational upper limit for the mass of static degenerate
fermionic dark matter objects. The treatment we use includes fully relativistic
equations for describing the static solutions of these objects. We study the
influence of the annihilation of the particles on this mass limit. We give the
change of its value over the age of the Universe with annihilation cross
sections relevant for such fermions constituting the dark matter. Our
calculations take into account the possibility of Dirac as well Majorana
spinors.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:10:47 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Kupi",
"Gábor",
""
]
] | [
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] |
711.2937 | Marc Siegmund | Marc Siegmund, Markus Hofmann, Oleg Pankratov | Persistent current and Wigner crystallization in a one dimensional
quantum ring | 7 pages, 5 figures | null | null | null | cond-mat.mes-hall | null | We use Density Functional Theory to study interacting spinless electrons on a
one-dimensional quantum ring in the density range where the system undergoes
Wigner crystallization. The Wigner transition leads to a drastic ``collective''
electron localization due to the Wigner crystal pinning, provided a weak
impurity potential is applied. To reveal this localization we examine a
persistent current in a ring penetrated by a magnetic flux. Using the DFT-OEP
method we calculated the current as a function of the interaction parameter
r_S. We find that in the limit of vanishing impurity potential the persistent
current stays constant up to a critical value of r_S^c=2.05 but shows a drastic
exponential decay for larger r_S which reflects a formation of a pinned Wigner
crystal. Above r_S^c the amplitude of the electron density oscillations exactly
follows the (r_S-r_S^c)^{1/2} behaviour, confirming a second-order phase
transition as expected in the mean-field-type OEP approximation.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:15:18 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Siegmund",
"Marc",
""
],
[
"Hofmann",
"Markus",
""
],
[
"Pankratov",
"Oleg",
""
]
] | [
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] |
711.2938 | Hidefumi Ohsugi | Hidefumi Ohsugi, Takayuki Hibi | Two way subtable sum problems and quadratic Groebner bases | 3 pages | Proc. Amer. Math. Soc. 137 (2009), 1539-1542 | 10.1090/S0002-9939-08-09675-5 | null | math.AC math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Hara, Takemura and Yoshida discuss toric ideals arising from two way subtable
sum problems and shows that these toric ideals are generated by quadratic
binomials if and only if the subtables are either diagonal or triangular. In
the present paper, we show that if the subtables are either diagonal or
triangular, then their toric ideals possess quadratic Groebner bases.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:16:36 GMT"
},
{
"version": "v2",
"created": "Thu, 12 Jun 2008 18:12:45 GMT"
}
] | 2018-08-22T00:00:00 | [
[
"Ohsugi",
"Hidefumi",
""
],
[
"Hibi",
"Takayuki",
""
]
] | [
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711.2939 | S. A. Lamzin | S. A. Lamzin, M. M. Romanova, S. A. Kravtsova | On the origin of continuum and line emission in CTTSs | 9 pages, 5 figure, 1 table, to appear in the proceedings of IAU
Symposium 243 "Star-Disk Interaction in Young Stars" (Grenoble, France,
May/2007) | null | 10.1017/S1743921307009477 | null | astro-ph | null | We calculated profiles of CIV 1550, Si IV 1400, NV 1240 and OVI 1035 doublet
lines using results of 3D MHD simulations of disc accretion onto young stars
with dipole magnetic field. It appeared that our calculations can not reproduce
profiles of these lines observed (HST/GHRS-STIS and FUSE) in CTTSs's spectra.
We also found that the theory predicts much larger C IV 1550 line flux than
observed (up to two orders of magnitude in some cases) and argue that the main
portion of accretion energy in CTTSs is liberated outside accretion shock. We
conclude that the reason of disagreement between the theory and observation is
strongly non-dipole character of CTTS's magnetic field near its surface.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:18:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lamzin",
"S. A.",
""
],
[
"Romanova",
"M. M.",
""
],
[
"Kravtsova",
"S. A.",
""
]
] | [
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711.294 | Masaaki Nakamura | Masaaki Nakamura and Lila Hirasawa | Electric transport and magnetic properties in multilayer graphene | 11 pages, 11 figures | Phys. Rev. B, 77 (2008) 045429 | 10.1103/PhysRevB.77.045429 | null | cond-mat.mes-hall cond-mat.str-el | null | We discuss electric transport and orbital magnetism of multilayer graphenes
in a weak-magnetic field using the matrix decomposition technique. At zero
temperature, the minimum conductivity is given by that of the monolayer system
multiplied by the layer number $N$, independent of the interlayer hopping $t$.
When the interlayer hopping satisfies the condition $t\gg \hbar/\tau$ with
$\tau$ being collision time of impurity scattering, $[N/2]$ kinks and $[N/2]+1$
plateaux appear in the Fermi-energy (gate voltage) dependence of the
conductivity and the Hall conductivity, respectively. These behaviors are
interpreted as multiband effects. We also found that the Hall conductivity and
the magnetic susceptibility take minimum value as a function of temperature,
for certain value of the gate voltage. This behavior is explained by
Fermi-energy dependence of these functions at zero temperature.
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711.2941 | Patrick Popescu-Pampu | Patrick Popescu-Pampu | Holomorphic fillability and cohomology | This paper was withdrawn | null | null | null | math.CV math.SG | null | I have withdrawn the paper, after having incorporated it into the paper
arXiv:0712.3484. In the meantime I have discovered that the main theorem proved
in the paper had already been proved by Bungart.
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711.2942 | Jen-Tsung Hsiang | Tai-Hung Wu, Jen-Tsung Hsiang, Da-Shin Lee | Boundary effects of electromagnetic vacuum fluctuations on charged
particles | 8 pages, presented at 8th Workshop on Quantum Field Theory Under the
Influence of External Conditions (QFEXT'07), Leipzig, Germany, 16-21 Sep 2007 | AIPConf.Proc.1059:175-179,2008 | 10.1063/1.3012273 | null | hep-th | null | The effects of electromagnetic vacuum fluctuations with the boundary on
charged particles is investigated. They may be observed via an electron
interference experiment near the conducting plate, where boundary effects of
vacuum fluctuations are found significant on coherence reduction of the
electrons. The dynamics of the charge under the influence of quantized
electromagnetic fields with a conducting plate is also studied. The
corresponding stochastic equation of motion is derived in the semiclassical
approximation, and the behavior of the charge's velocity fluctuations is
discussed.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:30:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Wu",
"Tai-Hung",
""
],
[
"Hsiang",
"Jen-Tsung",
""
],
[
"Lee",
"Da-Shin",
""
]
] | [
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711.2943 | Joakim Arnlind | Joakim Arnlind | Representation theory of C-algebras for a higher order class of spheres
and tori | 14 pages | null | 10.1063/1.2913523 | null | math-ph hep-th math.MP math.RT | null | We construct C-algebras for a class of surfaces that are inverse images of
certain polynomials of arbitrary degree. By using the directed graph associated
to a matrix, the representation theory can be understood in terms of ``loop''
and ``string'' representations, which are closely related to the dynamics of an
iterated map in the plane. As a particular class of algebras we introduce the
``Henon algebras'', for which the dynamical map is a generalized Henon map, and
give an example where irreducible representations of all dimensions exist.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:31:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Arnlind",
"Joakim",
""
]
] | [
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711.2944 | Ilian Iliev | Ilian T. Iliev (1,2), Paul R. Shapiro (3), Patrick McDonald (2),
Garrelt Mellema (4), Ue-Li Pen (2) ((1) ITP, Zurich, (2) CITA, (3) UT Austin,
(4) Stockholm) | Effect of the intergalactic environment on the observability of Ly-alpha
emitters during reionization | 21 pages, most figures in color, MNRAS, in press, replaced to match
the published version | null | 10.1111/j.1365-2966.2008.13879.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Observations of high-redshift Ly-alpha sources are a major tool for studying
the high-redshift Universe. We discuss the effect of the reionizing
intergalactic medium on the observability of Ly-alpha sources based on large
simulations of early structure formation with radiative transfer. This takes
into account self-consistently the reionization history, density, velocity and
ionization structures and nonlinear source clustering. We find that all fields
are highly anisotropic and as a consequence there are very large variations in
opacity among the different lines-of-sight. The velocity effects, from both
infall and source peculiar velocity are most important for the luminous
sources, affecting the line profile and depressing the bright end of the
luminosity function. The line profiles are generally asymmetric and the line
centers of the luminous sources are always absorbed due to the high density of
the local IGM. For both luminous and average sources the damping wing effects
are of similar magnitude and remain significant until fairly late.
The ionizing flux in the ionized patch surrounding a high density peak is
generally strongly dominated, particularly at late times, by the cluster of
faint sources, rather than the central massive galaxy. The IGM absorption does
not change appreciably the correlation function of sources at high redshift.
Our derived luminosity function assuming constant mass-to-light ratio provides
an excellent match to the shape of the observed luminosity function at z=6.6
with faint-end slope of alpha=-1.5. The resulting mass-to-light ratio implies
that the majority of sources responsible for reionization are too faint to be
observed by the current surveys. (abridged)
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:35:52 GMT"
},
{
"version": "v2",
"created": "Sun, 28 Sep 2008 20:10:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Iliev",
"Ilian T.",
""
],
[
"Shapiro",
"Paul R.",
""
],
[
"McDonald",
"Patrick",
""
],
[
"Mellema",
"Garrelt",
""
],
[
"Pen",
"Ue-Li",
""
]
] | [
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] |
711.2945 | Vadim N. Biktashev | V. N.Biktashev, A. Arutunyan, N. A. Sarvazyan | Generation and escape of local waves from the boundary of uncoupled
cardiac tissue | 28 pages, 10 figures, submitted to Biophysical Journal | null | 10.1529/biophysj.107.117630 | null | q-bio.TO q-bio.CB | null | We aim to understand the formation of abnormal waves of activity from
myocardial regions with diminished cell-to-cell coupling. In route to this
goal, we studied the behavior of a heterogeneous myocyte network in which a
sharp coupling gradient was placed under conditions of increasing network
automaticity. Experiments were conducted in monolayers of neonatal rat
cardiomyocytes using heptanol and isoproterenol as means of altering
cell-to-cell coupling and automaticity respectively. Experimental findings were
explained and expanded using a modified Beeler-Reuter numerical model. The data
suggests that the combination of a heterogeneous substrate, a gradient of
coupling and an increase in oscillatory activity of individual cells creates a
rich set of behaviors associated with self-generated spiral waves and ectopic
sources. Spiral waves feature a flattened shape and a pin-unpin drift type of
tip motion. These intercellular waves are action-potential based and can be
visualized with either voltage or calcium transient measurements. A source/load
mismatch on the interface between the boundary and well-coupled layers can lock
wavefronts emanating from both ectopic sources and rotating waves within the
inner layers of the coupling gradient. A numerical approach allowed us to
explore how: i) the spatial distribution of cells, ii) the amplitude and
dispersion of cell automaticity, iii) and the speed at which the coupling
gradient moves in space, affects wave behavior, including its escape into
well-coupled tissue.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 08:06:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Biktashev",
"V. N.",
""
],
[
"Arutunyan",
"A.",
""
],
[
"Sarvazyan",
"N. A.",
""
]
] | [
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] |
711.2946 | Monica Orienti | M. Orienti (1,2,3), D. Dallacasa (2,3), ((1) IAC, (2) Dipartimento di
Astronomia, Bologna, (3) IRA-INAF, Bologna) | Radio spectrum evolution and magnetic field in extreme GPS radio
sources. The case of RXJ1459+3337 | 8 pages, 4 figures; accepted for publication in A&A | null | 10.1051/0004-6361:20078098 | null | astro-ph | null | Aims: The knowledge of the properties of the youngest radio sources is very
important in order to trace the earliest phase of the evolution of the radio
emission. RXJ1459+3337, with its high turnover frequency (~25 GHz) provides a
unique opportunity to study this class of extreme objects. Methods:
High-sensitivity multi-frequency VLA observations have been carried out to
measure the flux-density with high accuracy, while multi-frequency VLBA
observations were performed, aimed at determining the pc-scale structure.
Archival ROSAT data have been used to infer the X-ray luminosity. Results: The
comparison between our new VLA data and those available in the literature shows
a steady increment of the flux-density in the optically-thick part of the
spectrum and a decrement of the turnover frequency. In the optically-thin
regime, the source flux density has already started to decrease. Such a
variability can be explained in terms of an adiabatically-expanding homogeneous
radio component. The frequency range spanned by our VLBA observations, together
with the resolution achieved, allows us to determine the source size and the
turnover frequency, and then to derive the magnetic field directly from these
observable quantities. The value obtained in this way is in good agreement with
that computed assuming equipartition condition. A similar value is also
obtained by comparing the radio and X-ray luminosities.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:44:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Orienti",
"M.",
""
],
[
"Dallacasa",
"D.",
""
]
] | [
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] |
711.2947 | Gerhard Huber | G. Huber, T. Deuschle, W. Schnitzler, R. Reichle, K. Singer and F.
Schmidt-Kaler | Transport of ions in a segmented linear Paul trap in
printed-circuit-board technology | 16 pages | null | null | null | quant-ph | null | We describe the construction and operation of a segmented linear Paul trap,
fabricated in printed-circuit-board technology with an electrode segment width
of 500 microns. We prove the applicability of this technology to reliable ion
trapping and report the observation of Doppler cooled ion crystals of Ca-40
with this kind of traps. Measured trap frequencies agree with numerical
simulations at the level of a few percent from which we infer a high
fabrication accuracy of the segmented trap. To demonstrate its usefulness and
versatility for trapped ion experiments we study the fast transport of a single
ion. Our experimental results show a success rate of 99.0(1)% for a transport
distance of 2x2mm in a round-trip time of T=20us, which corresponds to 4 axial
oscillations only. We theoretically and experimentally investigate the
excitation of oscillations caused by fast ion transports with error-function
voltage ramps: For a slightly slower transport (a round-trip shuttle within
T=30us) we observe non-adiabatic motional excitation of 0.89(15)meV.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:51:55 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Huber",
"G.",
""
],
[
"Deuschle",
"T.",
""
],
[
"Schnitzler",
"W.",
""
],
[
"Reichle",
"R.",
""
],
[
"Singer",
"K.",
""
],
[
"Schmidt-Kaler",
"F.",
""
]
] | [
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] |
711.2948 | Yunchang Shin | Yunchang Shin, W. Mike Snow, Christopher M. Lavelle, David V. Baxter,
Xin Tong, Haiyang Yan, Mark Leuschner | The Neutron Energy Spectrum Study from the Phase II Solid Methane
Moderator at the LENS Neutron Source | 20 pages, 12 figures | null | null | null | nucl-ex | null | Neutron energy spectrum measurements from a solid methane moderator were
performed at the Low Energy Neutron Source (LENS) at Indiana University
Cyclotron Facility (IUCF) to verify our neutron scattering model of solid
methane. The time-of-flight method was used to measure the energy spectrum of
the moderator in the energy range of 0.1$meV\sim$ 1$eV$. Neutrons were counted
with a high efficiency $^{3}{He}$ detector. The solid methane moderator was
operated in phase II temperature and the energy spectra were measured at the
temperatures of 20K and 4K. We have also tested our newly-developed scattering
kernels for phase II solid methane by calculating the neutron spectral
intensity expected from the methane moderator at the LENS neutron source using
MCNP (Monte Carlo N-particle Transport Code). Within the expected accuracy of
our approximate approach, our model predicts both the neutron spectral
intensity and the optimal thickness of the moderator at both temperatures. The
predictions are compared to the measured energy spectra. The simulations agree
with the measurement data at both temperatures.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:54:22 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Shin",
"Yunchang",
""
],
[
"Snow",
"W. Mike",
""
],
[
"Lavelle",
"Christopher M.",
""
],
[
"Baxter",
"David V.",
""
],
[
"Tong",
"Xin",
""
],
[
"Yan",
"Haiyang",
""
],
[
"Leuschner",
"Mark",
""
]
] | [
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] |
711.2949 | Marco Laumanns | Marco Laumanns | Stochastic convergence of random search to fixed size Pareto set
approximations | Corrected typo in Definition 4 | null | null | null | math.OC | null | This paper presents the first convergence result for random search algorithms
to a subset of the Pareto set of given maximum size k with bounds on the
approximation quality. The core of the algorithm is a new selection criterion
based on a hypothetical multilevel grid on the objective space. It is shown
that, when using this criterion for accepting new search points, the sequence
of solution archives converges with probability one to a subset of the Pareto
set that epsilon-dominates the entire Pareto set. The obtained approximation
quality epsilon is equal to the size of the grid cells on the finest level of
resolution that allows an approximation with at most k points within the family
of grids considered. While the convergence result is of general theoretical
interest, the archiving algorithm might be of high practical value for any type
iterative multiobjective optimization method, such as evolutionary algorithms
or other metaheuristics, which all rely on the usage of a finite on-line memory
to store the best solutions found so far as the current approximation of the
Pareto set.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 14:58:25 GMT"
},
{
"version": "v2",
"created": "Fri, 23 Nov 2007 11:32:54 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Laumanns",
"Marco",
""
]
] | [
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] |
711.295 | Thomas Schwetz | Patrick Huber, Mauro Mezzetto, Thomas Schwetz | On the impact of systematical uncertainties for the CP violation
measurement in superbeam experiments | 30 pages, 10 figures, version accepted for publication in JHEP | JHEP 0803:021,2008 | 10.1088/1126-6708/2008/03/021 | CERN-PH-TH/2007-227, VPI-IPNAS-07-09 | hep-ph hep-ex | null | Superbeam experiments can, in principle, achieve impressive sensitivities for
CP violation in neutrino oscillations for large $\theta_{13}$. We study how
those sensitivities depend on assumptions about systematical uncertainties. We
focus on the second phase of T2K, the so-called T2HK experiment, and we
explicitly include a near detector in the analysis. Our main result is that
even an idealised near detector cannot remove the dependence on systematical
uncertainties completely. Thus additional information is required. We identify
certain combinations of uncertainties, which are the key to improve the
sensitivity to CP violation, for example the ratio of electron to muon neutrino
cross sections and efficiencies. For uncertainties on this ratio larger than
2%, T2HK is systematics dominated. We briefly discuss how our results apply to
a possible two far detector configuration, called T2KK. We do not find a
significant advantage with respect to the reduction of systematical errors for
the measurement of CP violation for this setup.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:00:08 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Feb 2008 10:14:45 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Huber",
"Patrick",
""
],
[
"Mezzetto",
"Mauro",
""
],
[
"Schwetz",
"Thomas",
""
]
] | [
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] |
711.2951 | Alexander Milner | Alexander A Milner, Kaiyin Zhang and Yehiam Prior (Weizmann Institute
of Science) | Floating Tip Nanolithography | Version 2: new data added; PDF, 12 pages, 12 figures | null | 10.1021/nl801203c | null | cond-mat.mtrl-sci | null | We demonstrate noncontact, high quality surface modification with spatial
resolution of ~20 nm. The nanowriting is based on the interaction between the
surface and the tip of an Atomic force microscope illuminated by a focused
laser beam and hovering 1-4 nanometers above the surface without touching it.
The floating tip nanowriting is compared to mechanical surface scratching, and
is found to be much more reproducible, and of higher quality. In an
Apertureless Scanning Near Field Optical Microscope geometry the tip is
illuminated by a focused femtosecond laser, leading to two different, clearly
identifiable mechanisms for removing material from the surface: when heated by
the laser beam, the hot-tip thermally patterns the surface of low melting
temperature soft materials, and when focused right at the apex of the sharp
tip, the enhanced electric field of the laser beam causes ablation in high
melting temperature metal films.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:14:07 GMT"
},
{
"version": "v2",
"created": "Thu, 3 Apr 2008 08:18:03 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Milner",
"Alexander A",
"",
"Weizmann Institute\n of Science"
],
[
"Zhang",
"Kaiyin",
"",
"Weizmann Institute\n of Science"
],
[
"Prior",
"Yehiam",
"",
"Weizmann Institute\n of Science"
]
] | [
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] |
711.2952 | Petr Zasche | Zasche Petr, Zejda Miloslav, Brat Lubos | Eclipsing Binaries with Possible Light-Time Effect | 4 pages, 1 figure, 2 tables, conference proceedings | Astrophys.Space Sci.304:177,2006 | 10.1007/s10509-006-9103-2 | null | astro-ph | null | The period changes of six eclipsing binaries have been studied with focus on
the light-time effect. With the least squares method we also calculated
parameters of such an effect and properties of the unresolved body in these
systems. With these results we discussed the probability of presence of such
bodies in the systems with respect to possible confirmation by another method.
In two systems we also suggested the hypothesis of fourth body or magnetic
activity for explanation of the "second-order variability" after subtraction of
the light-time effect of the third body.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:19:36 GMT"
}
] | 2009-06-25T00:00:00 | [
[
"Petr",
"Zasche",
""
],
[
"Miloslav",
"Zejda",
""
],
[
"Lubos",
"Brat",
""
]
] | [
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] |
711.2953 | Junegone Chay | Junegone Chay, Hsiang-nan Li and Satoshi Mishima | Possible complex annihilation and B -> K pi direct CP asymmetry | 8 pages, 1 figure, added references | Phys.Rev.D78:034037,2008 | 10.1103/PhysRevD.78.034037 | MIT-CTP-3902 | hep-ph | null | We point out that a sizable strong phase could be generated from the penguin
annihilation in the soft-collinear effective theory for B meson decays. Keeping
a small scale suppressed by O(Lambda/m_b), Lambda being a hadronic scale and
m_b the b quark mass, in the denominators of internal particle propagators
without expansion, the resultant strong phase can accommodate the data of the
B^0 -> K^-+ pi^+- direct CP asymmetry. Our study reconciles the opposite
conclusions on the real or complex penguin annihilation amplitude drawn in the
soft-collinear effective theory and in the perturbative QCD approach based on
k_T factorization theorem.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:23:27 GMT"
},
{
"version": "v2",
"created": "Mon, 26 Nov 2007 14:19:22 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chay",
"Junegone",
""
],
[
"Li",
"Hsiang-nan",
""
],
[
"Mishima",
"Satoshi",
""
]
] | [
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711.2954 | Takashi Hamazaki | Takashi Hamazaki | Long wavelength limit of evolution of cosmological perturbations in the
universe where scalar fields and fluids coexist | Page:46 | Nucl.Phys.B791:20-59,2008 | 10.1016/j.nuclphysb.2007.09.028 | null | astro-ph | null | We present the LWL formula which represents the long wavelengh limit of the
solutions of evolution equations of cosmological perturbations in terms of the
exactly homogeneous solutions in the most general case where multiple scalar
fields and multiple perfect fluids coexist. We find the conserved quantity
which has origin in the adiabatic decaying mode, and by regarding this quantity
as the source term we determine the correction term which corrects the
discrepancy between the exactly homogeneous perturbations and the $k \to 0$
limit of the evolutions of cosmological perturbations. This LWL formula is
useful for investigating the evolutions of cosmological perturbations in the
early stage of our universe such as reheating after inflation and the curvaton
decay in the curvaton scenario. When we extract the long wavelength limits of
evolutions of cosmological perturbations from the exactly homogeneos
perturbations by the LWL formula, it is more convenient to describe the
corresponding exactly homogeneous system with not the cosmological time but the
scale factor as the evolution parameter. By applying the LWL formula to the
reheating model and the curvaton model with multiple scalar fields and multiple
radiation fluids, we obtain the S formula representing the final amplitude of
the Bardeen parameter in terms of the initial adiabatic and isocurvature
perturbations
Keywords:cosmological perturbations,long wavelength limit,reheating,curvaton
PACS number(s):98.80.Cq
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:24:32 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Hamazaki",
"Takashi",
""
]
] | [
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] |
711.2955 | Petr Zasche | P.Zasche, M. Wolf, P. Svoboda | The BVRI Light Curves And Period Analysis Of The Beta Lyrae System XX
Leonis | 4 pages, 2 figures, 2 tables, conference proceedings | IAU Symp.240:127,2007 | null | null | astro-ph | null | The contact eclipsing binary system XX Leonis (P = 0.97 days, sp A8) has been
analysed using the PHOEBE programme, based on the Wilson Devinney code. The
BVRI light curves were obtained during spring 2006 using the 20-cm telescope
and ST-7 CCD detector. The effective temperature of the primary component
determined from the photometric analysis is T=(7889+/-61)K, the inclination of
the orbit is i=(89.98+/-2.45)deg and the photometric mass ratio
q=(0.41+/-0.01). Also the third body hypothesis was suggested, based on the
period analysis using 57 minimum times and resulting the period of the third
body p3= (52.96+/-0.01)yr, amplitude A=(0.057+/-0.029)d and eccentricity
e=(0.79+/-0.08) which gives the minimum mass m3,min=(3.6+/-0.8)M_sun.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:29:22 GMT"
}
] | 2009-06-25T00:00:00 | [
[
"Zasche",
"P.",
""
],
[
"Wolf",
"M.",
""
],
[
"Svoboda",
"P.",
""
]
] | [
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] |
711.2956 | Ronny Thomas | R. Thomas, T. Hilger, B. Kampfer | Role of Four-Quark Condensates in QCD Sum Rules | Invited talk at International School of Nuclear Physics, 29th Course,
Quarks in Hadrons and Nuclei, Erice, Sicily, 16 - 24 Sep 2007 | Prog.Part.Nucl.Phys.61:297-303,2008 | 10.1016/j.ppnp.2007.12.028 | null | hep-ph nucl-th | null | The QCD sum rule approach to the in-medium behavior of hadrons is discussed
for omega meson, nucleon and D meson. Emphasis is devoted to the impact of
four-quark condensates and to order parameters of spontaneous symmetry
breaking.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:33:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Thomas",
"R.",
""
],
[
"Hilger",
"T.",
""
],
[
"Kampfer",
"B.",
""
]
] | [
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711.2957 | Martine Pithioux | Didier Mokoko (LABM), Martine Pithioux (LABM), Patrick Chabrand (LABM) | Temporal evolution of mechanical properties of skeletal tissue
regeneration in rabbits. An experimental study | 7 | Medical & biological engineering & computing 45, 10 (2007) 989-995 | null | null | physics.med-ph | null | Various mathematical models represent the effects of local mechanical
environment on the regulation of skeletal regeneration. Their relevance relies
on an accurate description of the evolving mechanical properties of the
regenerating tissue. The object of this study was to develop an experimental
model which made it possible to characterize the temporal evolution of the
structural and mechanical properties during unloaded enchondral osteogenesis in
the New Zealand rabbit, a standard animal model for studies of osteogenesis and
chondrogenesis. A 25mm segment of tibial diaphysis was removed sub-periosteally
from rabbits. The defect was repaired by the preserved periosteum. An external
fixator was applied to prevent mechanical loading during osteogenesis. The
regenerated skeletal tissues were studied by CT scan, histology and mechanical
tests. The traction tests between 7 to 21 days post-surgery were done on
formaldehyde-fixated tissue allowing to obtain force/displacement curves. The
viscoelastic properties of the regenerating skeletal tissues were visualized
throughout the repair process.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:35:02 GMT"
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] | 2007-11-20T00:00:00 | [
[
"Mokoko",
"Didier",
"",
"LABM"
],
[
"Pithioux",
"Martine",
"",
"LABM"
],
[
"Chabrand",
"Patrick",
"",
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711.2958 | Panayotis Boumis | Ioanna Leonidaki (1,3), Andreas Zezas (2), Panayotis Boumis (1) ((1)
Institute of Astronomy and Astrophysics, National Observatory of Athens,
Athens, Greece, (2) Harvard-Smithsonian Center for Astrophysics, Cambridge,
MA, USA, (3) Department of Physics, University of Patras, Rio-Patras, Greece) | X-ray supernova remnants in nearby galaxies | 2 pages, 4 figures, Contributed paper to "X-rays from nearby
galaxies", ESAC, Madrid (Spain), September 2007, in press | null | null | null | astro-ph | null | We present the initial results from a study of the SNR population in a sample
of six nearby galaxies (NGC 2403, NGC 4214, NGC 4449, NGC 5204, NGC 3077, NGC
4395) based on Chandra archival data. We discuss the analysis of the Chandra
data and we present candidate SNR sources selected on the basis of their X-ray
colours. We also present deep [S II] 6716 & 6731 A and Halpha line images for
most of the galaxies in our sample, which provide optically selected samples of
SNRs. Comparison of the X-ray results with the complementary optical
observations provides a more complete picture of the SNR population and allows
us to address their X-ray emission. Our preliminary analysis of the [S
II]/Halpha images show that 48 X-ray sources are typically associated with
Halpha sources, 7 of which are SNR candidates based on their [S II]/Halpha
ratio and one is an already known radio SNR.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:40:00 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Leonidaki",
"Ioanna",
""
],
[
"Zezas",
"Andreas",
""
],
[
"Boumis",
"Panayotis",
""
]
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] |
711.2959 | Simon Goodwin | Simon M. Goodwin, Gerhard Roehrle | On conjugacy of unipotent elements in finite groups of Lie type | 9 pages, Minor changes and corrections | null | null | null | math.GR math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $\bfG$ be a connected reductive algebraic group defined over $\F_q$,
where $q$ is a power of a prime $p$ that is good for $\bfG$. Let $F$ be the
Frobenius morphism associated with the $\FF_q$-structure on $\bfG$ and set $G =
\bfG^F$, the fixed point subgroup of $F$. Let $\bfP$ be an $F$-stable parabolic
subgroup of $\bfG$ and let $\bfU$ be the unipotent radical of $\bfP$; set $P =
\bfP^F$ and $U = \bfU^F$. Let $G_\uni$ be the set of unipotent elements in $G$.
In this note we show that the number of conjugacy classes of $U$ in $G_\uni$ is
given by a polynomial in $q$ with integer coefficients.
| [
{
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},
{
"version": "v2",
"created": "Fri, 11 Jul 2008 14:17:13 GMT"
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] | 2008-07-11T00:00:00 | [
[
"Goodwin",
"Simon M.",
""
],
[
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"Gerhard",
""
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711.296 | G. Papini | G. Papini, G. Scarpetta, A. Feoli, G. Lambiase | Optics of spin-1 particles from gravity-induced phases | 16 pages, 2 figures | Int.J.Mod.Phys.D18:485-499,2009 | 10.1142/S0218271809014595 | null | gr-qc | null | The Maxwell and Maxwell-de Rham equations can be solved exactly to first
order in an external gravitational field. The gravitational background induces
phases in the wave functions of spin-1 particles. These phases yield the optics
of the particles without requiring any thin lens approximation.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:48:11 GMT"
}
] | 2009-05-12T00:00:00 | [
[
"Papini",
"G.",
""
],
[
"Scarpetta",
"G.",
""
],
[
"Feoli",
"A.",
""
],
[
"Lambiase",
"G.",
""
]
] | [
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711.2961 | Felix Brandt | Felix Brandt, Felix Fischer, Paul Harrenstein | Recognizing Members of the Tournament Equilibrium Set is NP-hard | 9 pages, 3 figures | Social Choice and Welfare 34(4), 2009 | 10.1007/s00355-009-0419-z | null | cs.CC cs.GT cs.MA | null | A recurring theme in the mathematical social sciences is how to select the
"most desirable" elements given a binary dominance relation on a set of
alternatives. Schwartz's tournament equilibrium set (TEQ) ranks among the most
intriguing, but also among the most enigmatic, tournament solutions that have
been proposed so far in this context. Due to its unwieldy recursive definition,
little is known about TEQ. In particular, its monotonicity remains an open
problem up to date. Yet, if TEQ were to satisfy monotonicity, it would be a
very attractive tournament solution concept refining both the Banks set and
Dutta's minimal covering set. We show that the problem of deciding whether a
given alternative is contained in TEQ is NP-hard.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:48:46 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 13:47:48 GMT"
}
] | 2015-02-06T00:00:00 | [
[
"Brandt",
"Felix",
""
],
[
"Fischer",
"Felix",
""
],
[
"Harrenstein",
"Paul",
""
]
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] |
711.2962 | Ken Ebisawa | Ken Ebisawa, Shigeo Yamauchi, Yasuo Tanaka, Katsuji Koyama, Yuichiro
Ezoe, Aya Bamba, Motohide Kokubun, Yoshiaki Hyodo, Masahiro Tsujimoto, and
Hiromitsu Takahashi | Spectral Study of the Galactic Ridge X-ray Emission with Suzaku | Accepted to PASJ second Suzaku Special issue | null | 10.1093/pasj/60.sp1.S223 | null | astro-ph | null | We have observed a typical Galactic plane field at (l,b) = (28.46d, -0.20d)
with Suzaku for 100 ksec to carry out a precise spectral study of the Galactic
Ridge X-ray Emission (GRXE). The field is known to be devoid of X-ray point
sources brighter than ~2 x 10^{-13} ergs s^{-1} cm^{-2} (2--10 keV), and
already deeply observed with Chandra. Thanks to the low and stable background
and high spectral resolution of Suzaku, we were able to resolve, for the first
time, three narrow iron K-emission lines from low-ionized (6.41 keV),
helium-like (6.67 keV), and hydrogenic ions (7.00 keV) in the GRXE spectrum.
These line features constrain the GRXE emission mechanisms: The cosmic-ray ion
charge exchange model or the non-equilibrium ionization plasma model are
unlikely, since they require either broad emission lines or lines at
intermediate ionization states. Collisional ionization equilibrium plasma is
the likely origin for the 6.67 keV and 7.00 keV lines, while origin of the 6.41
keV line, which is due to fluorescence from cold material, is not elucidated.
Low non-X-ray background and little stray-light contamination of Suzaku allowed
us to precisely measure the absolute X-ray surface brightness in the direction
of the Galactic plane. Excluding the point sources brighter than ~2 x 10^{-13}
ergs s^{-1} cm^{-2} (2--10 keV), the total surface brightness on the Galactic
plane is ~6.1 x 10^{-11} ergs s^{-1} cm^{-2} deg^{-2} (2--10 keV), including
the contribution of the cosmic X-ray background that is estimated to be ~1.3x
10^{-11} ergs s^{-1} cm^{-2} deg^{-2}.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:48:57 GMT"
}
] | 2017-01-18T00:00:00 | [
[
"Ebisawa",
"Ken",
""
],
[
"Yamauchi",
"Shigeo",
""
],
[
"Tanaka",
"Yasuo",
""
],
[
"Koyama",
"Katsuji",
""
],
[
"Ezoe",
"Yuichiro",
""
],
[
"Bamba",
"Aya",
""
],
[
"Kokubun",
"Motohide",
""
],
[
"Hyodo",
"Yoshiaki",
""
],
[
"Tsujimoto",
"Masahiro",
""
],
[
"Takahashi",
"Hiromitsu",
""
]
] | [
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] |
711.2963 | Koos Gubbels | K. B. Gubbels and H. T. C. Stoof | Renormalization Group Theory for the Imbalanced Fermi Gas | Replaced with published version | Phys. Rev. Lett. 100, 140407 (2008) | 10.1103/PhysRevLett.100.140407 | null | cond-mat.stat-mech cond-mat.supr-con | null | We formulate a wilsonian renormalization group theory for the imbalanced
Fermi gas. The theory is able to recover quantitatively well-established
results in both the weak-coupling and the strong-coupling (unitarity) limit. We
determine for the latter case the line of second-order phase transitions of the
imbalanced Fermi gas and in particular the location of the tricritical point.
We obtain good agreement with the recent experiments of Y. Shin {\it et al}.
[Nature {\bf 451}, 689 (2008)].
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:49:31 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 16:40:40 GMT"
},
{
"version": "v3",
"created": "Thu, 20 Dec 2007 18:24:36 GMT"
},
{
"version": "v4",
"created": "Wed, 30 Apr 2008 15:27:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gubbels",
"K. B.",
""
],
[
"Stoof",
"H. T. C.",
""
]
] | [
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] |
711.2964 | Yossi Weinstein | Yuval Elias, Jos\'e M. Fernandez, Tal Mor and Yossi Weinstein | Optimal Algorithmic Cooling of Spins | 20 pages, 5 figures | Lecture Notes in Comput. Sci. (LNCS), vol 4618, pp. 2-26,
Unconvetional Computation, Springer, 2007 | 10.1007/978-3-540-73554-0 | null | quant-ph | null | Algorithmic Cooling (AC) of Spins is potentially the first near-future
application of quantum computing devices. Straightforward quantum algorithms
combined with novel entropy manipulations can result in a method to improve the
identification of molecules. We introduce here several new exhaustive cooling
algorithms, such as the Tribonacci and k-bonacci algorithms. In particular, we
present the ``all-bonacci'' algorithm, which appears to reach the maximal
degree of cooling obtainable by the optimal AC approach.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:49:58 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Elias",
"Yuval",
""
],
[
"Fernandez",
"José M.",
""
],
[
"Mor",
"Tal",
""
],
[
"Weinstein",
"Yossi",
""
]
] | [
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] |
711.2965 | Stefan Waldmann | Martin Bordemann, Nikolai Neumaier, Stefan Waldmann, Stefan Weiss | Deformation Quantization of Surjective Submersions and Principal Fibre
Bundles | 32 pages, typos corrected | null | null | null | math.QA math-ph math.MP | null | In this paper we establish a notion of deformation quantization of a
surjective submersion which is specialized further to the case of a principal
fibre bundle: the functions on the total space are deformed into a right module
for the star product algebra of the functions on the base manifold. In case of
a principal fibre bundle we require in addition invariance under the principal
action. We prove existence and uniqueness of such deformations. The commutant
within all differential operators on the total space is computed and gives a
deformation of the algebra of vertical differential operators. Applications to
noncommutative gauge field theories and phase space reduction of star products
are discussed.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 15:51:23 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 10:52:53 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Bordemann",
"Martin",
""
],
[
"Neumaier",
"Nikolai",
""
],
[
"Waldmann",
"Stefan",
""
],
[
"Weiss",
"Stefan",
""
]
] | [
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711.2966 | Clare Burrage | C. Burrage | Supernova Brightening from Chameleon-Photon Mixing | 17 pages, 3 figures | Phys.Rev.D77:043009,2008 | 10.1103/PhysRevD.77.043009 | null | astro-ph hep-ph | null | Measurements of standard candles and measurements of standard rulers give an
inconsistent picture of the history of the universe. This discrepancy can be
explained if photon number is not conserved as computations of the luminosity
distance must be modified. I show that photon number is not conserved when
photons mix with chameleons in the presence of a magnetic field. The strong
magnetic fields in a supernova mean that the probability of a photon converting
into a chameleon in the interior of the supernova is high, this results in a
large flux of chameleons at the surface of the supernova. Chameleons and
photons also mix as a result of the intergalactic magnetic field. These two
effects combined cause the image of the supernova to be brightened resulting in
a model which fits both observations of standard candles and observations of
standard rulers.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:11:18 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Burrage",
"C.",
""
]
] | [
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] |
711.2967 | Eulogio Oset | E. Oset, M. D\"oring, D. Strottman, D. Jido, M. Napsuciale, K. Sasaki,
C. A. Vaquera-Araujo, M. Kaskulov, E. Hernandez, H. Nagahiro, S. Hirenzaki | Photo- and Electron-Production of Mesons on Nucleons and Nuclei | Lecture at the "International School of Nuclear Physics", 29th Course
Quarks in Hadrons and Nuclei, Erice, Italy, September 2007. Note added in
Proofs concerning the mixed events technique and other comments on omega
production | Prog.Part.Nucl.Phys.61:260-275,2008 | 10.1016/j.ppnp.2007.12.024 | FTUV-19-1107, IFIC-19-1107 | nucl-th | null | In these lectures I will show some results obtained with the chiral unitary
approach applied to the photo and electroproduction of mesons. The results for
photoproduction of $\eta \pi^0 p$ and $K^0 \pi^0 \Sigma^+$, together with
related reactions will be shown, having with common denominator the excitation
of the $\Delta(1700)$ resonance which is one of those dynamically generated in
the chiral unitary approach. Then I will show results obtained for the $e^+ e^-
\to \phi f_0(980)$ reaction which reproduce the bulk of the data except for a
pronounced peak, giving support to a new mesonic resonance, X(2175). Results
will also be shown for the electromagnetic form factors of the $N^*(1535)$
resonance, also dynamically generated in this approach. Finally, I will show
some results on the photoproduction of the $\omega$ in nuclei, showing that
present experimental results claiming a shift of the $\omega$ mass in the
medium are tied to a particular choice of background and are not conclusive.
One the other hand, the same experimental results show unambiguously a huge
increase of the $\omega$ width in the nuclear medium.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:48:28 GMT"
},
{
"version": "v2",
"created": "Fri, 1 Feb 2008 09:04:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Oset",
"E.",
""
],
[
"Döring",
"M.",
""
],
[
"Strottman",
"D.",
""
],
[
"Jido",
"D.",
""
],
[
"Napsuciale",
"M.",
""
],
[
"Sasaki",
"K.",
""
],
[
"Vaquera-Araujo",
"C. A.",
""
],
[
"Kaskulov",
"M.",
""
],
[
"Hernandez",
"E.",
""
],
[
"Nagahiro",
"H.",
""
],
[
"Hirenzaki",
"S.",
""
]
] | [
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] |
711.2968 | Claudio Cazorla | C. Cazorla and J. Boronat | Zero-temperature equation of state of solid 4He at low and high
pressures | 29 pages, 9 figures. To be published in Journal of Physics: Condensed
Matter | null | 10.1088/0953-8984/20/01/015223 | null | cond-mat.other cond-mat.mtrl-sci | null | We study the zero-temperature equation of state (EOS) of solid 4He in the
hexagonal closed packet (hcp) phase over the 0-57 GPa pressure range by means
of the Diffusion Monte Carlo (DMC) method and the semi-empirical Aziz pair
potential HFD-B(HE). In the low pressure regime (P ~ 0-1 GPa) we assess
excellent agreement with experiments and we give an accurate description of the
atomic kinetic energy, Lindemann ratio and Debye temperature over a wide range
of molar volumes (22-6 cm^{3}/mol). However, on moving to higher pressures our
calculated P-V curve presents an increasingly steeper slope which ultimately
provides differences within ~40 % with respect to measurements. In order to
account for many-body interactions arising in the crystal with compression
which are not reproduced by our model, we perform additional electronic
density-functional theory (DFT) calculations for correcting the computed DMC
energies in a perturbative way. We explore both generalized gradient and local
density approximations (GGA and LDA, respectively) for the electronic
exchange-correlation potential. By proceeding in this manner, we show that
discrepancies with respect to high pressure data are reduced to 5-10 % with few
computational extra cost. Further comparison between our calculated EOSs and ab
initio curves deduced for the perfect crystal and corrected for the zero-point
motion of the atoms enforces the reliability of our approach.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:05:15 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Cazorla",
"C.",
""
],
[
"Boronat",
"J.",
""
]
] | [
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] |
711.2969 | Ara Avetissian Karapet | A. K. Avetissian | Cosmological Bang within Matter Era. Is the Generation of Galactic-Scale
Mass Possible? | 10 pages, 2 figures, revtex4 (Int. Conf. Nuclear Astrophysics Beyond
the First 50 Years, 2007, Caltech, Pasadena, USA) | null | null | null | astro-ph | null | A heuristic hypothesis about domination of Bose-Einstein statistics in the
early Universe is suggested. The possibility of Bose-Einstein condensation
(BEC) of primordial baryon-antibaryon pairs is considered. In accordance with
this postulation enormous masses in the order of galactic mass may be
accumulated within the cosmic scales. At the certain threshold value of the
matter density the structural bosons decay into fermions and the sharp
breakdown of quantum-mechanical symmetry of the particles wave functions
occurs. Then, due to the Pauli principle of exclusion a large-scale phase
transition occurs because of enormous pressure jump of the matter. This
phenomenon might cause Cosmological Bang at the beginning stage of the Matter
Era. As a mechanism of accumulation of galactic mass much larger than the
configuration with structural bosons, a hypothetical BEC of elementary bosons
(gauge bosons $W^{\pm}$ and $Z^{0})$ is discussed as well.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:06:49 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Avetissian",
"A. K.",
""
]
] | [
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] |
711.297 | Gelu Popescu | Gelu Popescu | Free holomorphic functions and interpolation | 20 pages | Math. Ann. 342 (2008), 1-30 | null | null | math.FA math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we obtain a noncommutative multivariable analogue of the
classical Nevanlinna-Pick interpolation problem for analytic functions with
positive real parts on the open unit disc. As consequences, we deduce some
results concerning operator-valued analytic interpolation on the unit ball on
C^n.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:33:46 GMT"
},
{
"version": "v2",
"created": "Wed, 4 Feb 2009 16:42:00 GMT"
}
] | 2009-02-04T00:00:00 | [
[
"Popescu",
"Gelu",
""
]
] | [
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711.2971 | Annie Bouyer | Sylvain Kubicki (MAP / CRAI), Annie Guerri\'ero (MAP / CRAI), Damien
Hanser (MAP / CRAI), Gilles Halin (MAP / CRAI) | IT services design to support coordination practices in the
Luxembourguish AEC sector | null | null | null | null | cs.HC | null | In the Architecture Engineering and Construction sector (AEC) cooperation
between actors is essential for project success. The configuration of actors'
organization takes different forms like the associated coordination mechanisms.
Our approach consists in analyzing these coordination mechanisms through the
identification of the "base practices" realized by the actors of a construction
project to cooperate. We also try with practitioners to highlight the "best
practices" of cooperation. Then we suggest here two prototypes of IT services
aiming to demonstrate the value added of IT to support cooperation. These
prototype tools allow us to sensitize the actors through terrain experiments
and then to bring inch by inch the Luxembourgish AEC sector towards electronic
cooperation.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:36:02 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Kubicki",
"Sylvain",
"",
"MAP / CRAI"
],
[
"Guerriéro",
"Annie",
"",
"MAP / CRAI"
],
[
"Hanser",
"Damien",
"",
"MAP / CRAI"
],
[
"Halin",
"Gilles",
"",
"MAP / CRAI"
]
] | [
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711.2972 | Jorge Fiscina | Jorge E. Fiscina and Christian Wagner | Wet Sand flows better than dry sand | 5 pages and 5 figures | null | null | null | cond-mat.stat-mech cond-mat.soft | null | We investigated the yield stress and the apparent viscosity of sand with and
without small amounts of liquid. By pushing the sand through a tube with an
enforced Poiseuille like profile we minimize the effect of avalanches and shear
localization. We find that the system starts to flow when a critical shear of
the order of one particle diameter is exceeded. In contrast to common believe,
we observe that the resistance against the flow of wet sand is much smaller
than that of dry sand. For the dissipative flow we propose a non-equilibrium
state equation for granular fluids.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:38:34 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Fiscina",
"Jorge E.",
""
],
[
"Wagner",
"Christian",
""
]
] | [
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] |
711.2973 | Ignazio Licata | Ignazio Licata | Emergence and Computation at the Edge of Classical and Quantum Systems | 16 pages | null | 10.1142/9789812779953_0001 | null | physics.gen-ph quant-ph | null | The problem of emergence in physical theories makes necessary to build a
general theory of the relationships between the observed system and the
observing system. It can be shown that there exists a correspondence between
classical systems and computational dynamics according to the Shannon-Turing
model. A classical system is an informational closed system with respect to the
observer; this characterizes the emergent processes in classical physics as
phenomenological emergence. In quantum systems, the analysis based on the
computation theory fails. It is here shown that a quantum system is an
informational open system with respect to the observer and able to exhibit
processes of observational, radical emergence. Finally, we take into
consideration the role of computation in describing the physical world.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 16:47:58 GMT"
}
] | 2016-11-23T00:00:00 | [
[
"Licata",
"Ignazio",
""
]
] | [
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] |
711.2974 | Francois Loeser | G. Guibert, F. Loeser, M. Merle | Composition with a two variable function | 11 pages | Math. Research Letters 16, 439-448 (2009) | null | null | math.AG | null | We compute the motivic nearby cycles of functions obtained by composition of
two functions with distinct sets of variables with a two variable function
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:11:30 GMT"
}
] | 2011-02-25T00:00:00 | [
[
"Guibert",
"G.",
""
],
[
"Loeser",
"F.",
""
],
[
"Merle",
"M.",
""
]
] | [
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] |
711.2975 | Dirk-S\"oren L\"uhmann | Dirk-S\"oren L\"uhmann, Kai Bongs, Klaus Sengstock, Daniela Pfannkuche | Self-Trapping of Bosons and Fermions in Optical Lattices | 4 pages, 4 figures. Published version | Phys. Rev. Lett. 101, 050402 (2008) | 10.1103/PhysRevLett.101.050402 | null | cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We theoretically investigate the enhanced localization of bosonic atoms by
fermionic atoms in three-dimensional optical lattices and find a self-trapping
of the bosons for attractive boson-fermion interaction. Because of this mutual
interaction, the fermion orbitals are substantially squeezed, which results in
a strong deformation of the effective potential for bosons. This effect is
enhanced by an increasing bosonic filling factor leading to a large shift of
the transition between the superfluid and the Mott-insulator phase. We find a
nonlinear dependency of the critical potential depth on the boson-fermion
interaction strength. The results, in general, demonstrate the important role
of higher Bloch bands for the physics of attractively interacting quantum gas
mixtures in optical lattices and are of direct relevance to recent experiments
with 87Rb - 40K mixtures, where a large shift of the critical point has been
found.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:13:31 GMT"
},
{
"version": "v2",
"created": "Fri, 1 Aug 2008 06:52:51 GMT"
}
] | 2008-08-01T00:00:00 | [
[
"Lühmann",
"Dirk-Sören",
""
],
[
"Bongs",
"Kai",
""
],
[
"Sengstock",
"Klaus",
""
],
[
"Pfannkuche",
"Daniela",
""
]
] | [
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] |
711.2976 | A.C. Fabian | A.C. Fabian (Institute of Astronomy, University of Cambridge, UK) | XMM-Newton and Broad Iron Lines | 7 pages, 18 figures, accepted for publication in Astron. Nachr. (ESAC
Conference) | null | 10.1002/asna.200710902 | null | astro-ph | null | Iron line emission is common in the X-ray spectra of accreting black holes.
When the line emission is broad or variable then it is likely to originate from
close to the black hole. X-ray irradiation of the accretion flow by the
power-law X-ray continuum produces the X-ray 'reflection' spectrum which
includes the iron line. The shape and variability of the iron lines and
reflection can be used as a diagnostic of the radius, velocity and nature of
the flow. The inner radius of the dense flow corresponds to the innermost
stable circular orbit and thus can be used to determine the spin of the black
hole. Studies of broad iron lines and reflection spectra offer much promise for
understanding how the inner parts of accretion flows (and outflows) around
black holes operate. There remains great potential for XMM-Newton to continue
to make significant progress in this work. The need for high quality spectra
and thus for long exposure times is paramount.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:17:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fabian",
"A. C.",
"",
"Institute of Astronomy, University of Cambridge, UK"
]
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711.2977 | Brendan Casey | Brendan Casey | Rare D Decays | To be published in the proceedings of CHARM07, Ithaca, NY, August
2007, eConf C070805 | ECONF C070805:13,2007 | 10.2172/920724 | FERMILAB-CONF-07-615-E | hep-ex | null | We discuss several recent measurements of rare charmed hadron decays. Focus
is placed on radiative and annihilation topologies highlighting their
sensitivity to new physics and pointing out the strengths and weaknesses of
different channels. We compare the different measurement techniques employed at
fixed target and $e^+e^-$ dedicated charm experiments, B-factories, and the
Tevatron experiments. Comparisons are also made to similar topologies in the
beauty, strange, and top systems where appropriate.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:21:04 GMT"
}
] | 2011-03-18T00:00:00 | [
[
"Casey",
"Brendan",
""
]
] | [
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711.2978 | Claudio Albanese | Claudio Albanese | Stochastic Mechanics as a Gauge Theory | null | null | null | null | math.PR math-ph math.MP | null | We show that non-relativistic Quantum Mechanics can be faithfully represented
in terms of a classical diffusion process endowed with a gauge symmetry of
group Z_4. The representation is based on a quantization condition for the
realized action along paths. A lattice regularization is introduced to make
rigorous sense of the construction and then removed. Quantum mechanics is
recovered in the continuum limit and the full U(1) gauge group symmetry of
electro-magnetism appears. Anti-particle representations emerge naturally,
albeit the context is non-relativistic. Quantum density matrices are obtained
by averaging classical probability distributions over phase-action variables.
We find that quantum conditioning can be described in classical terms but not
through the standard notion of sub sigma-algebras. Delicate restrictions arise
by the constraint that we are only interested in the algebra of gauge invariant
random variables. We conclude that Quantum Mechanics is equivalent to a theory
of gauge invariant classical stochastic processes we call Stochastic Mechanics.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:26:35 GMT"
},
{
"version": "v2",
"created": "Tue, 20 Nov 2007 14:18:17 GMT"
},
{
"version": "v3",
"created": "Fri, 23 Nov 2007 00:41:29 GMT"
}
] | 2007-11-23T00:00:00 | [
[
"Albanese",
"Claudio",
""
]
] | [
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] |
711.2979 | Emma Ryan-Weber | Emma V. Ryan-Weber (1), Ayesha Begum (1), Tom Oosterloo (2,3),
Sabyasachi Pal (4) Michael J. Irwin (1), Vasily Belokurov (1), N. Wyn Evans
(1), and Daniel B. Zucker (1), ((1) IoA, Cambridge, (2) Astron, (3) Kapteyn
Institute, (4) NCRA) | The Local Group dwarf Leo T: HI on the brink of star formation | 6 pages, 7 figures, accepted for publication in MNRAS on November
15th 2007, full resolution version at:
http://www.ast.cam.ac.uk/~eryan/leot.pdf . Typographical error in sound speed
equation has led to a new Figure 6 and minor changes to the text | Mon.Not.Roy.Astron.Soc.384:53,2008 | 10.1111/j.1365-2966.2007.12734.x | null | astro-ph | null | We present Giant Meterwave Radio Telescope (GMRT) and Westerbork ynthesis
Radio Telescope (WSRT) observations of the recently discovered Local Group
dwarf galaxy, Leo T. The peak HI column density is measured to be 7x10^20
cm^-2, and the total HI mass is 2.8Xx10^5 Msun, based on a distance of 420 kpc.
Leo T has both cold (~ 500 K) and warm (~ 6000 K) HI at its core, with a global
velocity dispersion of 6.9 km/s, from which we derive a dynamical mass within
the HI radius of 3.3x10^6 Msun, and a mass-to-light ratio of greater than 50.
We calculate the Jeans mass from the radial profiles of the HI column density
and velocity dispersion, and predict that the gas should be globally stable
against star formation. This finding is inconsistent with the half light radius
of Leo T, which extends to 170 pc, and indicates that local conditions must
determine where star formation takes place. Leo T is not only the lowest
luminosity galaxy with on-going star formation discovered to date, it is also
the most dark matter dominated, gas-rich dwarf in the Local Group.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:32:48 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Dec 2007 12:24:11 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Ryan-Weber",
"Emma V.",
""
],
[
"Begum",
"Ayesha",
""
],
[
"Oosterloo",
"Tom",
""
],
[
"Pal",
"Sabyasachi",
""
],
[
"Irwin",
"Michael J.",
""
],
[
"Belokurov",
"Vasily",
""
],
[
"Evans",
"N. Wyn",
""
],
[
"Zucker",
"Daniel B.",
""
]
] | [
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711.298 | Claudio Albanese | Claudio Albanese | Stochastic Integrals and Abelian Processes | null | null | null | null | math.PR | null | We study triangulation schemes for the joint kernel of a diffusion process
with uniformly continuous coefficients and an adapted, non-resonant Abelian
process. The prototypical example of Abelian process to which our methods apply
is given by stochastic integrals with uniformly continuous coeffcients. The
range of applicability includes also a broader class of processes of practical
relevance, such as the sup process and certain discrete time summations we
discuss. We discretize the space coordinate in uniform steps and assume that
time is either continuous or finely discretized as in a fully explicit Euler
method and the Courant condition is satisfied. We show that the Fourier
transform of the joint kernel of a diffusion and a stochastic integral
converges in a uniform graph norm associated to the Markov generator.
Convergence also implies smoothness properties for the Fourier transform of the
joint kernel. Stochastic integrals are straightforward to define for finite
triangulations and the convergence result gives a new and entirely constructive
way of defining stochastic integrals in the continuum. The method relies on a
reinterpretation and extension of the classic theorems by Feynman-Kac,
Girsanov, Ito and Cameron-Martin, which are also re-obtained. We make use of a
path-wise analysis without relying on a probabilistic interpretation. The
Fourier representation is needed to regularize the hypo-elliptic character of
the joint process of a diffusion and an adapted stochastic integral. The
argument extends as long as the Fourier analysis framework can be generalized.
This condition leads to the notion of non-resonant Abelian process.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:38:20 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Albanese",
"Claudio",
""
]
] | [
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] |
711.2981 | Volodymyr Magas | V.K. Magas, L.P. Csernai | Bjorken model with Freeze Out | 7 pages, 5 figures, presented the International Conference "New
Trends in High-Energy Physics" (Crimea 2007), Yalta, Crimea, Ukraine,
September 15-22, 2007 | null | null | null | nucl-th | null | The freeze out of the expanding systems, created in relativistic heavy ion
collisions, is discussed. We combine Bjorken scenario with earlier developed
freeze out equations into a unified model. The important feature of the
proposed model is that physical freeze out is completely finished in a finite
time, which can be varied from 0 (freeze out hypersurface) to infinity. The
dependence of the post freeze out distribution function on this freeze out time
will be studied. As an example model is completely solved and analyzed for the
gas of pions.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:49:47 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Magas",
"V. K.",
""
],
[
"Csernai",
"L. P.",
""
]
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711.2982 | Remi Tailleux | Remi Tailleux | Thermodynamic inadmissibility of the incompressible hydrodynamics
description of turbulent stratified fluid flows at low Mach numbers | 9 pages, submitted to Physical Review Letters | null | null | null | physics.flu-dyn physics.ao-ph | null | The incompressible Navier-Stokes equations currently represent the primary
model for describing stratified turbulent fluid flows at low Mach number. The
validity of the incompressible assumption, however, has so far only been
rigorously established for adiabatic motions. Here, we show from first principl
es that the use of available energetics and thermodynamics considerations
applied to a turbulent mixing event associated with stratified shear flow
instability r efutes the widespread idea that the incompressible assumption is
also valid when diabatic irreversible effects are important. The main
consequence is that dynamics and thermodynamics are strongly coupled in
stratified turbulence. This departs strongly from the currently accepted
wisdom, and calls for a complete revisiting of the physical processes governing
stratified turbulence at low Mach numbers.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 17:53:28 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Tailleux",
"Remi",
""
]
] | [
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] |
711.2983 | Antoni Szczurek | Antoni Szczurek, Tomasz Pietrycki, Anna Rybarska and Gabriela Slipek | Dijet and photon-jet correlations in proton-proton collisions at RHIC | an invited talk at the Memorial Workshop on Hadronic and Quark Matter
devoted to J.Zimanyi, Budapest, July 2-4, 2007 | PoS LHC07:034,2007; Eur.Phys.J.ST 155:191-200,2008 | 10.1140/epjst/e2008-00601-7 | null | nucl-th astro-ph hep-ph | null | We discuss correlations in azimuthal angle as well as correlations in
two-dimensional space of transverse momenta of two jets as well as photon and
jet. Some $k_t$-factorization subprocesses are included for the first time in
the literature. Different unintegrated gluon/parton distributions are used in
the $k_t$-factorization approach. The results depend on UGDF/UPDF used. The
collinear NLO $2 \to 3$ contributions dominate over $k_t$-factorization cross
section at small relative azimuthal angles as well as for asymmetric transverse
momentum configurations.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:02:23 GMT"
}
] | 2011-07-19T00:00:00 | [
[
"Szczurek",
"Antoni",
""
],
[
"Pietrycki",
"Tomasz",
""
],
[
"Rybarska",
"Anna",
""
],
[
"Slipek",
"Gabriela",
""
]
] | [
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711.2984 | Guido Tiana | Guido Tiana | Estimation of microscopic averages from metadynamics | null | null | 10.1140/epjb/e2008-00232-8 | null | cond-mat.stat-mech cond-mat.soft | null | With the help of metadynamics it is possible to calculate efficiently the
free energy of systems displaying high energy barriers as a function of few
selected "collective variables". In doing this, the contribution of all the
other degrees of freedom ("microscopic" variables) is averaged out and, thus,
lost. In the following, it is shown that it is possible to calculate the
thermal average of these microscopic degrees of freedom during the
metadynamics, not loosing this piece of information.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:03:23 GMT"
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] | 2009-11-13T00:00:00 | [
[
"Tiana",
"Guido",
""
]
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711.2985 | Leo Radzihovsky | Leo Radzihovsky, Quan Zhang | Conical soliton escape into a third dimension of a surface vortex | 9 pages, 8 eps figures, accepted by PRE | Phys. Rev. E 79, 041702 (2009) | 10.1103/PhysRevE.79.041702 | null | cond-mat.soft | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present an exact three-dimensional solitonic solution to a
sine-Gordon-type Euler-Lagrange equation, that describes a configuration of a
three-dimensional vector field n constrained to a surface p-vortex, with a
prescribed polar tilt angle on a planar substrate and escaping into the third
dimension in the bulk. The solution is relevant to characterization of a
schlieren texture in nematic liquid-crystal films with tangential (in-plane)
substrate alignment. The solution is identical to a section of a point defect
discovered many years ago by Saupe [Mol. Cryst. Liq. Cryst. 21, 211 (1973)],
when latter is restricted to a surface.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:03:52 GMT"
},
{
"version": "v2",
"created": "Fri, 3 Apr 2009 23:49:20 GMT"
}
] | 2009-04-22T00:00:00 | [
[
"Radzihovsky",
"Leo",
""
],
[
"Zhang",
"Quan",
""
]
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] |
711.2986 | Robert Thorne S | R.S. Thorne | The role of uncertainties in parton distribution functions | 10 pages, 15 figures as .ps or .eps files, invited talk at
PHYSTAT-LHC Workshop on Statistical Issues for LHC Physics, June 2007 | null | null | null | hep-ph | null | I consider the uncertainties in parton distributions and the consequences for
hadronic cross-sections. There is ever-increasing sophistication in the
relationship between the uncertainties of the distributions and the errors on
the experimental data used to extract them. However, I demonstrate that this
uncertainty is frequently subsumed by that due to the choice of data used in
fits, and more surprisingly by the precise details of the theoretical framework
used. Variations in heavy flavour prescriptions provide striking examples.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:07:19 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Thorne",
"R. S.",
""
]
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] |
711.2987 | Martin Kerin | Jost-Hinrich Eschenburg (Universit\"at Augsburg), Martin Kerin
(University of Pennsylvania) | Almost positive curvature on the Gromoll-Meyer sphere | 8 pages, 1 figure, to appear in Proc. Amer. Math. Soc | null | null | null | math.DG | null | Gromoll and Meyer have represented a certain exotic 7-sphere $\Sigma^7$ as a
biquotient of the Lie group $G = Sp(2)$. We show for a 2-parameter family of
left invariant metrics on $G$ that the induced metric on $\Sigma^7$ has
strictly positive sectional curvature at all points outside four subvarieties
of codimension $\geq 1$ which we describe explicitly.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:08:36 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Eschenburg",
"Jost-Hinrich",
"",
"Universität Augsburg"
],
[
"Kerin",
"Martin",
"",
"University of Pennsylvania"
]
] | [
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] |
711.2988 | Steve Brice | Steve Brice | Neutrino Experiments: Status, Recent Progress, and Prospects | 14 pages, 10 figures, proceedings of plenary talk at EPS HEP 2007
Conference, Manchester, UK. Updated with citation added to Figure 10 | J.Phys.Conf.Ser.110:012008,2008 | 10.1088/1742-6596/110/1/012008 | FERMILAB-CONF-07-617-E | hep-ex | null | Neutrino physics has seen an explosion of activity and new results in the
last decade. In this report the current state of the field is summarized, with
a particular focus on progress in the last two years. Prospects for the near
term (roughly 5 years) are also described.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:14:10 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 04:13:03 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Brice",
"Steve",
""
]
] | [
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711.2989 | Alexander Shirokov V | Alexander Shirokov (CITA) | Gravitational Softening and Adaptive Mass Resolution | 27 pages, 6 figures; Minor additions; WSHAPE package available at
http://www.gracos.org/wshape; Submitted to the Journal of Computational
Physics | null | null | null | astro-ph | null | Pairwise forces between particles in cosmological N-body simulations are
generally softened to avoid hard collisions. Physically, this softening
corresponds to treating the particles as diffuse clouds rather than point
masses. For particles of unequal mass (and hence unequal softening length),
computing the softened force involves a nontrivial double integral over the
volumes of the two particles. We show that Plummer force softening is
consistent with this interpretation of softening while spline softening is not.
We provide closed-form expressions and numerical implementation for pairwise
gravitational force laws for pairs of particles of general softening scales
$\epsilon_1$ and $\epsilon_2$ assuming the commonly used cloud profiles: NGP,
CIC, TSC, and PQS. Similarly, we generalize Plummer force law into pairs of
particles of general softenings. We relate our expressions to the gaussian,
Plummer and spline force softenings known from literature. Our expressions
allow possible inclusions of pointlike particles such as stars or supermassive
black holes.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 20:55:04 GMT"
},
{
"version": "v2",
"created": "Sat, 24 Nov 2007 03:28:06 GMT"
},
{
"version": "v3",
"created": "Wed, 9 Apr 2008 20:19:08 GMT"
}
] | 2008-04-10T00:00:00 | [
[
"Shirokov",
"Alexander",
"",
"CITA"
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] |
711.299 | Dorin Ervin Dutkay | Dorin Ervin Dutkay and Palle E.T. Jorgensen | Quasiperiodic Spectra and Orthogonality for Iterated Function System
Measures | null | null | null | null | math.CA math.GM | null | We extend classical basis constructions from Fourier analysis to attractors
for affine iterated function systems (IFSs). This is of interest since these
attractors have fractal features, e.g., measures with fractal scaling
dimension. Moreover, the spectrum is then typically quasi-periodic, but
non-periodic, i.e., the spectrum is a ``small perturbation'' of a lattice. Due
to earlier research on IFSs, there are known results on certain classes of
spectral duality-pairs, also called spectral pairs or spectral measures. It is
known that some duality pairs are associated with complex Hadamard matrices.
However, not all IFSs $X$ admit spectral duality. When $X$ is given, we
identify geometric conditions on $X$ for the existence of a Fourier spectrum,
serving as the second part in a spectral pair. We show how these spectral pairs
compose, and we characterize the decompositions in terms of atoms. The
decompositions refer to tensor product factorizations for associated complex
Hadamard matrices.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:31:26 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 16:26:03 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Dutkay",
"Dorin Ervin",
""
],
[
"Jorgensen",
"Palle E. T.",
""
]
] | [
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] |
711.2991 | Fernando Ruiz | G. Horcajada, F. Ruiz Ruiz | Quantization of the open string on plane-wave limits of dS_n x S^n and
non-commutativity outside branes | 31 pages, 12pt | Nucl.Phys.B799:110-135,2008 | 10.1016/j.nuclphysb.2008.02.016 | null | hep-th | null | The open string on the plane-wave limit of $dS_n\times S^n $ with constant
$B_2$ and dilaton background fields is canonically quantized. This entails
solving the classical equations of motion for the string, computing the
symplectic form, and defining from its inverse the canonical commutation
relations. Canonical quantization is proved to be perfectly suited for this
task, since the symplectic form is unambiguously defined and non-singular. The
string position and the string momentum operators are shown to satisfy
equal-time canonical commutation relations. Noticeably the string position
operators define non-commutative spaces for all values of the string
world-sheet parameter $\sig$, thus extending non-commutativity outside the
branes on which the string endpoints may be assumed to move. The Minkowski
spacetime limit is smooth and reproduces the results in the literature, in
particular non-commutativity gets confined to the endpoints.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:36:15 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 13:43:37 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Horcajada",
"G.",
""
],
[
"Ruiz",
"F. Ruiz",
""
]
] | [
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] |
711.2992 | Steven Willison | C. Garraffo, G. Giribet, E. Gravanis, S. Willison | Gravitational solitons and $C^0$ vacuum metrics in five-dimensional
Lovelock gravity | 48 pages, LaTex, 16 figures. A slightly shorter version of this paper
is accepted for publication in J. Math. Phys | J.Math.Phys.49:042502,2008 | 10.1063/1.2890377 | CECS-PHY-07/22 | gr-qc hep-th | null | Junction conditions for vacuum solutions in five-dimensional
Einstein-Gauss-Bonnet gravity are studied. We focus on those cases where two
spherically symmetric regions of space-time are joined in such a way that the
induced stress tensor on the junction surface vanishes. So a spherical vacuum
shell, containing no matter, arises as a boundary between two regions of the
space-time. A general analysis is given of solutions that can be constructed by
this method of geometric surgery. Such solutions are a generalized kind of
spherically symmetric empty space solutions, described by metric functions of
the class $C^0$. New global structures arise with surprising features. In
particular, we show that vacuum spherically symmetric wormholes do exist in
this theory. These can be regarded as gravitational solitons, which connect two
asymptotically (Anti) de-Sitter spaces with different masses and/or different
effective cosmological constants. We prove the existence of both static and
dynamical solutions and discuss their (in)stability under perturbations that
preserve the symmetry. This leads us to discuss a new type of instability that
arises in five-dimensional Lovelock theory of gravity for certain values of the
coupling of the Gauss-Bonnet term. The issues of existence and uniqueness of
solutions and determinism in the dynamical evolution are also discussed.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:39:07 GMT"
},
{
"version": "v2",
"created": "Mon, 26 Nov 2007 23:46:49 GMT"
},
{
"version": "v3",
"created": "Tue, 15 Jan 2008 23:46:34 GMT"
},
{
"version": "v4",
"created": "Thu, 28 Feb 2008 02:38:56 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Garraffo",
"C.",
""
],
[
"Giribet",
"G.",
""
],
[
"Gravanis",
"E.",
""
],
[
"Willison",
"S.",
""
]
] | [
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] |
711.2993 | Humberto Carmona PhD | H. A. Carmona, F. K. Wittel, F. Kun and H. J. Herrmann | Fragmentation processes in impact of spheres | null | null | 10.1103/PhysRevE.77.051302 | null | cond-mat.stat-mech | null | We study the brittle fragmentation of spheres by using a three-dimensional
Discrete Element Model. Large scale computer simulations are performed with a
model that consists of agglomerates of many particles, interconnected by
beam-truss elements. We focus on the detailed development of the fragmentation
process and study several fragmentation mechanisms. The evolution of meridional
cracks is studied in detail. These cracks are found to initiate in the inside
of the specimen with quasi-periodic angular distribution. The fragments that
are formed when these cracks penetrate the specimen surface give a broad peak
in the fragment mass distribution for large fragments that can be fitted by a
two-parameter Weibull distribution. This mechanism can only be observed in 3D
models or experiments. The results prove to be independent of the degree of
disorder in the model. Our results significantly improve the understanding of
the fragmentation process for impact fracture since besides reproducing the
experimental observations of fragment shapes, impact energy dependence and mass
distribution, we also have full access to the failure conditions and evolution.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:45:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Carmona",
"H. A.",
""
],
[
"Wittel",
"F. K.",
""
],
[
"Kun",
"F.",
""
],
[
"Herrmann",
"H. J.",
""
]
] | [
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] |
711.2994 | Sumit Das | Adel Awad, Sumit R. Das, K. Narayan and Sandip P. Trivedi | Gauge Theory Duals of Cosmological Backgrounds and their Energy Momentum
Tensors | 17 pages, LaTeX, v2: minor modifications | Phys.Rev.D77:046008,2008 | 10.1103/PhysRevD.77.046008 | UK/07-11 | hep-th | null | We revisit Type IIB supergravity backgrounds with null and spacelike
singularities with natural gauge theory duals proposed in {\tt hep-th/0602107}
and {\tt hep-th/0610053}. We show that for these backgrounds there are always
choices of the boundaries of these deformed $AdS_5 \times S^5$ space-times,
such that the dual gauge theories live on {\it flat} metrics and have
space-time dependent couplings. We present a new time dependent solution of
this kind where the effective string coupling is always bounded and vanishes at
a spacelike singularity in the bulk, and the space-time becomes $AdS_5 \times
S^5$ at early and late times. The holographic energy momentum tensor calculated
with a choice of flat boundary is shown to vanish for null backgrounds and to
be generically non-zero for time dependent backgrounds.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:50:38 GMT"
},
{
"version": "v2",
"created": "Tue, 27 Nov 2007 15:05:11 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Awad",
"Adel",
""
],
[
"Das",
"Sumit R.",
""
],
[
"Narayan",
"K.",
""
],
[
"Trivedi",
"Sandip P.",
""
]
] | [
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] |
711.2995 | Joerg Aichelin | J. Aichelin, H. Petersen, S. Vogel, M. Bleicher | How can we explore the onset of deconfinement by experiment? | invited talk, workshop on Critical Point and Onset of Deconfinement
(CPOD), GSI(Darmstadt), July 9-13, 2007 | PoSCPOD07:004,2007 | null | null | nucl-th | null | There is little doubt that Quantumchromodynamics (QCD) is the theory which
describes strong interaction physics. Lattice gauge simulations of QCD predict
that in the $\mu,T$ plane there is a line where a transition from confined
hadronic matter to deconfined quarks takes place. The transition is either a
cross over (at low $\mu$) or of first order (at high $\mu$). It is the goal of
the present and future heavy ion experiment at RHIC and FAIR to study this
phase transition at different locations in the $\mu,T$ plane and to explore the
properties of the deconfined phase. It is the purpose of this contribution to
discuss some of the observables which are considered as useful for this
purpose.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:52:19 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Aichelin",
"J.",
""
],
[
"Petersen",
"H.",
""
],
[
"Vogel",
"S.",
""
],
[
"Bleicher",
"M.",
""
]
] | [
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711.2996 | Ryan Requist | Ryan Requist and Oleg Pankratov | The Kohn-Sham system in one-matrix functional theory | 17 pages, 6 figures | Phys. Rev. B, vol. 77, 235121 (2008) | 10.1103/PhysRevB.77.235121 | null | cond-mat.str-el | null | A system of electrons in a local or nonlocal external potential can be
studied with 1-matrix functional theory (1MFT), which is similar to density
functional theory (DFT) but takes the one-particle reduced density matrix
(1-matrix) instead of the density as its basic variable. Within 1MFT, Gilbert
derived [PRB 12, 2111 (1975)] effective single-particle equations analogous to
the Kohn-Sham (KS) equations in DFT. The self-consistent solution of these
1MFT-KS equations reproduces not only the density of the original electron
system but also its 1-matrix. While in DFT it is usually possible to reproduce
the density using KS orbitals with integer (0 or 1) occupancy, in 1MFT
reproducing the 1-matrix requires in general fractional occupancies. The
variational principle implies that the KS eigenvalues of all fractionally
occupied orbitals must collapse at self-consistency to a single level, equal to
the chemical potential. We show that as a consequence of the degeneracy the
iteration of the KS equations is intrinsically divergent. Fortunately, the
level shifting method, commonly introduced in Hartree-Fock calculations, is
always able to force convergence. We introduce an alternative derivation of the
1MFT-KS equations that allows control of the eigenvalue collapse by
constraining the occupancies. As an explicit example, we apply the 1MFT-KS
scheme to calculate the ground state 1-matrix of an exactly solvable two-site
Hubbard model.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:54:26 GMT"
}
] | 2008-07-23T00:00:00 | [
[
"Requist",
"Ryan",
""
],
[
"Pankratov",
"Oleg",
""
]
] | [
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] |
711.2997 | Peter Watson | P. Watson and H. Reinhardt | Completing Continuum Coulomb Gauge in the Functional Formalism | 4 pages, no figures | null | null | null | hep-th hep-lat hep-ph | null | It is argued that within the continuum functional formalism, there is no need
to supply a further (spatially independent) gauge constraint to complete the
Coulomb gauge of Yang-Mills theory. It is shown explicitly that a natural
completion of the gauge-fixing leads to a contradiction with the perturbative
renormalizability of the theory.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:57:21 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Watson",
"P.",
""
],
[
"Reinhardt",
"H.",
""
]
] | [
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711.2998 | Benjamin Leveque | Yannick Frein (LGS), Benjamin L\'ev\^eque (LGS), Andras Sebo (LGS) | Optimizing diversity | null | null | null | null | cs.DM | null | We consider the problem of minimizing the size of a family of sets G such
that every subset of 1,...,n can be written as a disjoint union of at most k
members of G, where k and n are given numbers. This problem originates in a
real-world application aiming at the diversity of industrial production. At the
same time, the minimum of G so that every subset of 1,...,n is the union of two
sets in G has been asked by Erdos and studied recently by Furedi and Katona
without requiring the disjointness of the sets. A simple construction providing
a feasible solution is conjectured to be optimal for this problem for all
values of n and k and regardless of the disjointness requirement; we prove this
conjecture in special cases including all (n,k) for which n <= 3k holds, and
some individual values of n and k.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 18:58:06 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Frein",
"Yannick",
"",
"LGS"
],
[
"Lévêque",
"Benjamin",
"",
"LGS"
],
[
"Sebo",
"Andras",
"",
"LGS"
]
] | [
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] |
711.2999 | Masayuki Hase Oka | M. O. Hase and J. F. F. Mendes | Solvable Metric Growing Networks | null | J. Stat. Mech. (2008) P12002 | 10.1088/1742-5468/2008/12/P12002 | null | cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Structure and dynamics of complex networks usually deal with degree
distributions, clustering, shortest path lengths and other graph properties.
Although these concepts have been analysed for graphs on abstract spaces, many
networks happen to be embedded in a metric arrangement, where the geographic
distance between vertices plays a crucial role. The present work proposes a
model for growing network that takes into account the geographic distance
between vertices: the probability that they are connected is higher if they are
located nearer than farther. In this framework, the mean degree of vertices,
degree distribution and shortest path length between two randomly chosen
vertices are analysed.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 20:53:47 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Nov 2008 18:02:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hase",
"M. O.",
""
],
[
"Mendes",
"J. F. F.",
""
]
] | [
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] |
711.3 | Bruno Galvan | Bruno Galvan | Quantum Mechanics and imprecise probability | 16 pages, 1 figure. To appear in Journal of Statistical Physics,
almost the published version | J. Stat. Phys. 131, 1155-1167 (2008) | 10.1007/s10955-008-9530-2 | null | quant-ph | null | An extension of the Born rule, the {\it quantum typicality rule}, has
recently been proposed [B. Galvan: Found. Phys. 37, 1540-1562 (2007)]. Roughly
speaking, this rule states that if the wave function of a particle is split
into non-overlapping wave packets, the particle stays approximately inside the
support of one of the wave packets, without jumping to the others.
In this paper a formal definition of this rule is given in terms of {\it
imprecise probability}. An imprecise probability space is a measurable space
$(\Omega, {\cal A})$ endowed with a {\it set} of probability measures $\cal P$.
The quantum formalism and the quantum typicality rule allow us to define a set
of probabilities ${\cal P}_\Psi$ on $(X^T, {\cal F})$, where $X$ is the
configuration space of a quantum system, $T$ is a time interval and ${\cal F}$
is the $\sigma$-algebra generated by the cylinder sets. Thus, it is proposed
that a quantum system can be represented as the {\it imprecise stochastic
process} $(X^T, {\cal F}, {\cal P}_\Psi)$, which is a canonical stochastic
process in which the single probability measure is replaced by a set of
measures. It is argued that this mathematical model, when used to represent
macroscopic systems, has sufficient predictive power to explain both the
results of the statistical experiments and the quasi-classical structure of the
macroscopic evolution.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 19:12:13 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 20:08:58 GMT"
}
] | 2008-06-08T00:00:00 | [
[
"Galvan",
"Bruno",
""
]
] | [
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] |
711.3001 | Natalia Ivanova | Natalia Ivanova, Craig O. Heinke, Frederic A. Rasio | Formation of Millisecond Pulsars in Globular Clusters | 6 pages, 3 figures, to appear in the proceedings of the 40 Years of
Pulsars conference held at McGill University in August 2007 | AIP Conf.Proc.983:442-447,2008 | 10.1063/1.2900271 | null | astro-ph | null | In this contribution we discuss how neutron stars are produced and retained
in globular clusters, outlining the most important dynamical channels and
evolutionary events that affect thepopulation of mass-transferring binaries
with neutron stars and result in the formation of recycled pulsars. We confirm
the importance of electron-capture supernovae in globular clusters as the major
supplier of retained neutron stars.By comparing the observed millisecond pulsar
population and the results obtained from simulations, we discuss several
constraints on the evolution of mass-transferring systems.In particular, we
find that in our cluster model the following mass-gaining events create
populations of MSPs that do not match the observations (with respect to binary
periods and companion masses or the number of produced systems) and therefore
likely do not lead to NSs spun up to millisecond periods: (i) accretion during
a common envelope event with a NS formed through accretion-induced collapse,
and (ii) mass transfer from a WD donor. By restricting ourselves to the
evolutionary and dynamical paths that most likely lead to neutron star
recycling, we obtain good agreement between our models and the numbers and
characteristics of observed millisecond pulsars in the clusters Terzan 5 and 47
Tuc.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 20:33:57 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Ivanova",
"Natalia",
""
],
[
"Heinke",
"Craig O.",
""
],
[
"Rasio",
"Frederic A.",
""
]
] | [
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] |
711.3002 | Gabriela Aurelio | G. Aurelio, J. Curiale, R.D. Sanchez and G.J. Cuello | Probing phase coexistence and stabilization of the spin-ordered
ferrimagnetic state by Calcium addition in the YBa_{1-x}Ca_{x}Co_{2}O_{5.5}
layered cobaltites using neutron diffraction | null | null | 10.1103/PhysRevB.76.214417 | null | cond-mat.str-el cond-mat.mtrl-sci | null | In this article we study the effects of a partial substitution of Ba with the
smaller cation Ca in the layered cobaltites YBaCo_2O_{5+\delta} for \delta
\approx 0.5. Neutron thermodiffractograms are reported for the compounds
YBa_{0.95}Ca_{0.05}Co_2O_{5.5} (x_{Ca}=0.05) and YBa_{0.90}Ca_{0.10}Co_2O_{5.5}
(x_{Ca}=0.10) in the temperature range 20 K \leq T \leq 300 K, as well as high
resolution neutron diffraction experiments at selected temperatures for the
samples x_{Ca}=0.05, x_{Ca}=0.10 and the parent compound x_{Ca}=0. We have
found the magnetic properties to be strongly affected by the cationic
substitution. Although the "122" perovskite structure seems unaffected by Ca
addition, the magnetic arrangements of Co ions are drastically modified: the
antiferromagnetic (AFM) long-range order is destroyed, and a ferrimagnetic
phase with spin state order is stabilized below T \sim 290 K. For the sample
with x_{Ca}=0.05 a fraction of AFM phase coexists with the ferrimagnetic one
below T \sim 190 K, whereas for x_{Ca}=0.10 the AFM order is completely lost.
The systematic refinement of the whole series has allowed for a better
understanding of the observed low-temperature diffraction patterns of the
parent compound, YBaCo_2O_{5.5}, which had not yet been clarified. A two-phase
scenario is proposed for the x_{Ca}=0 compound which is compatible with the
phase coexistence observed in the x_{Ca}=0.05 sample.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 19:23:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Aurelio",
"G.",
""
],
[
"Curiale",
"J.",
""
],
[
"Sanchez",
"R. D.",
""
],
[
"Cuello",
"G. J.",
""
]
] | [
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] |
711.3003 | Georg Weiglein | Georg Weiglein | Electroweak Physics at the ILC | 5 pages, contribution to the proceedings of EPS07 | J.Phys.Conf.Ser.110:042033,2008 | 10.1088/1742-6596/110/4/042033 | IPPP/07/85, DCPT/07/170 | hep-ph | null | Some aspects of electroweak physics at the International Linear Collider
(ILC) are reviewed. The importance of precision measurements in the Higgs
sector and in top-quark physics is emphasized, and the physics potential of the
GigaZ option of the ILC is discussed. It is shown in particular that even in a
scenario where the states of new physics are so heavy that they would be
outside of the reach of the LHC and the first phase of the ILC, the GigaZ
precision on the effective weak mixing angle may nevertheless allow the
detection of quantum effects of new physics.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 19:24:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Weiglein",
"Georg",
""
]
] | [
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] |
711.3004 | Kurt Langfeld | Kurt Langfeld | Computational Methods in Quantum Field Theory | 50 pages, 16 figures, notes based on a lecture presented at the XIX
Physics Graduate Days at the University of Heidelberg, 8th - 12th October
2007 | null | null | null | hep-lat | null | After a brief introduction to the statistical description of data, these
lecture notes focus on quantum field theories as they emerge from lattice
models in the critical limit. For the simulation of these lattice models,
Markov chain Monte-Carlo methods are widely used. We discuss the heat bath and,
more modern, cluster algorithms. The Ising model is used as a concrete
illustration of important concepts such as correspondence between a theory of
branes and quantum field theory or the duality map between strong and weak
couplings. The notes then discuss the inclusion of gauge symmetries in lattice
models and, in particular, the continuum limit in which quantum Yang-Mills
theories arise.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 19:44:49 GMT"
}
] | 2007-11-20T00:00:00 | [
[
"Langfeld",
"Kurt",
""
]
] | [
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711.3005 | Jan Staff | Jan Staff, Brian Niebergal, and Rachid Ouyed | Gamma Ray Burst engine activity within the quark nova scenario: Prompt
emission, X-ray Plateau, and sharp drop-off | 4 pages, submitted to ApJL | null | 10.1111/j.1365-2966.2008.13465.x | null | astro-ph | null | We present a three-stage model for a long GRB inner engine to explain the
prompt gamma ray emission, and interpret recent Swift satellite observations of
early X-ray afterglow plateaus followed by a sharp drop off or a shallow power
law decay. The three stages involves a neutron star phase, a quark star (QS)
and a black hole phase as described in Staff et al. (2007). We find that the QS
stage allows for more energy to be extracted from neutron star to QS conversion
as well as from ensuing accretion onto the QS. The QS accretion phase naturally
extends the engine activity and can account for both the prompt emission and
irregular early X-ray afterglow activity. Following the accretion phase, the QS
can spin-down by emission of a baryon-free outflow. The magnetar-like magnetic
field strengths resulting from the NS to QS transition provide enough spin-down
energy, for the correct amount of time, to account for the plateau in the X-ray
afterglow. In our model, a sharp drop-off following the plateau occurs when the
QS collapses to a BH during the spin-down, thus shutting-off the secondary
outflow. We applied our model to GRB 070110 and GRB 060607A and found that we
can consistently account for the energetics and duration during the prompt and
plateau phases.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 20:05:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Staff",
"Jan",
""
],
[
"Niebergal",
"Brian",
""
],
[
"Ouyed",
"Rachid",
""
]
] | [
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] |
711.3006 | Alexandros Gezerlis | Alexandros Gezerlis and J. Carlson | Strongly paired fermions: Cold atoms and neutron matter | 5 pages, 4 figures; 3 references added; v2 corresponds to the
published version | Phys.Rev.C77:032801,2008 | 10.1103/PhysRevC.77.032801 | LA-UR-07-7894 | nucl-th cond-mat.other | null | Experiments with cold Fermi atoms can be tuned to probe strongly interacting
fluids that are very similar to the low-density neutron matter found in the
crusts of neutron stars. In contrast to traditional superfluids and
superconductors, matter in this regime is very strongly paired, with gaps of
the order of the Fermi energy. We compute the T=0 equation of state and pairing
gap for cold atoms and low-density neutron matter as a function of the Fermi
momentum times the scattering length. Results of quantum Monte Carlo
calculations show that the equations of state are very similar. The neutron
matter pairing gap at low densities is found to be very large but, except at
the smallest densities, significantly suppressed relative to cold atoms because
of the finite effective range in the neutron-neutron interaction.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 19:59:16 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Mar 2008 20:56:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Gezerlis",
"Alexandros",
""
],
[
"Carlson",
"J.",
""
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] |
711.3007 | Yasushi Mino | Yasushi Mino | Modulation of the gravitational waveform by the effect of radiation
reaction | Expressions are corrected for easier reading | Phys.Rev.D77:044008,2008 | 10.1103/PhysRevD.77.044008 | null | gr-qc | null | When we calculate gravitational waveforms from extreme-mass-ratio inspirals
(EMRIs) by metric perturbation, it is a common strategy to use the adiabatic
approximation. Under that approximation, we first calculate the linear metric
perturbation induced by geodesics orbiting a black hole, then we calculate the
adiabatic evolution of the parameters of geodesics due to the radiation
reaction effect through the calculation of the self-force. This procedure is
considered to be reasonable, however, there is no direct proof that it can
actually produce the correct waveform we would observe. In this paper, we study
the formal expression of the second order metric perturbation and show that it
be expressed as the linear metric perturbation modulated by the adiabatic
evolution of the geodesic. This evidence supports the assumption that the
adiabatic approximation can produce the correct waveform, and that the
adiabatic expansion we propose in Ref.\cite{adi} is an appropriate perturbation
expansion for studying the radiation reaction effect on the gravitational
waveform.
| [
{
"version": "v1",
"created": "Mon, 19 Nov 2007 23:37:31 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Jan 2008 18:42:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mino",
"Yasushi",
""
]
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