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711.4208 | Noel Malod-Dognin | Rumen Andonov (IRISA), Nicola Yanev, No\"el Malod-Dognin (IRISA) | Towards Structural Classification of Proteins based on Contact Map
Overlap | null | null | null | null | q-bio.QM | null | A multitude of measures have been proposed to quantify the similarity between
protein 3-D structure. Among these measures, contact map overlap (CMO)
maximization deserved sustained attention during past decade because it offers
a fine estimation of the natural homology relation between proteins. Despite
this large involvement of the bioinformatics and computer science community,
the performance of known algorithms remains modest. Due to the complexity of
the problem, they got stuck on relatively small instances and are not
applicable for large scale comparison. This paper offers a clear improvement
over past methods in this respect. We present a new integer programming model
for CMO and propose an exact B &B algorithm with bounds computed by solving
Lagrangian relaxation. The efficiency of the approach is demonstrated on a
popular small benchmark (Skolnick set, 40 domains). On this set our algorithm
significantly outperforms the best existing exact algorithms, and yet provides
lower and upper bounds of better quality. Some hard CMO instances have been
solved for the first time and within reasonable time limits. From the values of
the running time and the relative gap (relative difference between upper and
lower bounds), we obtained the right classification for this test. These
encouraging result led us to design a harder benchmark to better assess the
classification capability of our approach. We constructed a large scale set of
300 protein domains (a subset of ASTRAL database) that we have called Proteus
300. Using the relative gap of any of the 44850 couples as a similarity
measure, we obtained a classification in very good agreement with SCOP. Our
algorithm provides thus a powerful classification tool for large structure
databases.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:36:32 GMT"
}
] | 2009-04-20T00:00:00 | [
[
"Andonov",
"Rumen",
"",
"IRISA"
],
[
"Yanev",
"Nicola",
"",
"IRISA"
],
[
"Malod-Dognin",
"Noël",
"",
"IRISA"
]
] | [
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711.4209 | Yakov Itin | Yakov Itin (Institute of Mathematics, Hebrew University of Jerusalem,
and Jerusalem College of Technology) | Coframe geometry and gravity | to be published in "Classical and Quantum Gravity Research Progress",
Nova Science Publishers, Inc | null | null | null | gr-qc | null | The possible extensions of GR for description of fermions on a curved space,
for supergravity and for loop quantum gravity require a richer set of 16
independent variables. These variables can be assembled in a coframe field,
i.e., a local set of four linearly independent 1-forms. In the ordinary
formulation, the coframe gravity does not have any connection to a specific
geometry even being constructed from the geometrical meaningful objects. A
geometrization of the coframe gravity is an aim of this paper. We construct a
complete class of the coframe connections which are linear in the first order
derivatives of the coframe field on an $n$ dimensional manifolds with and
without a metric. The subclasses of the torsion-free, metric-compatible and
flat connections are derived. We also study the behavior of the geometrical
structures under local transformations of the coframe. The remarkable fact is
an existence of a subclass of connections which are invariant when the
infinitesimal transformations satisfy the Maxwell-like system of equations. In
the framework of the coframe geometry construction, we propose a geometrical
action for the coframe gravity. It is similar to the Einstein-Hilbert action of
GR, but the scalar curvature is constructed from the general coframe
connection. We show that this geometric Lagrangian is equivalent to the coframe
Lagrangian up to a total derivative term. Moreover there is a family of coframe
connections which Lagrangian does not include the higher order terms at all. In
this case, the equivalence is complete.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:07:24 GMT"
}
] | 2019-08-12T00:00:00 | [
[
"Itin",
"Yakov",
"",
"Institute of Mathematics, Hebrew University of Jerusalem,\n and Jerusalem College of Technology"
]
] | [
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711.421 | Jeffrey Burdges | Jeffrey Burdges | Signalizers and balance in groups of finite Morley rank | null | null | null | null | math.LO math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that a minimal counter example to the Cherlin-Zilber Algebraicity
Conjecture for simple groups of finite Morley rank has Prufer 2-rank at most
two. This article covers the signalizer functor theory and identifies the
groups of Lie rank at least three; leaving the uniqueness case analysis to
previous articles. This result signifies the end of the general methods used to
handle large groups; hereafter each individual group PSL$_2$, PSL$_3$, PSp$_4$,
and G$_2$ will require its own identification theorem.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 09:59:07 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Nov 2008 18:58:57 GMT"
}
] | 2008-11-28T00:00:00 | [
[
"Burdges",
"Jeffrey",
""
]
] | [
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711.4211 | Alexandre Losev | A. Losev | The Penrose Lattice revisited | 6 pages 2 figures | null | null | null | cond-mat.other | null | A recursive scheme relying on decagons is used to generate Penrose-like
sublattices or tilings. Its relevance for understanding structures with
non-crystallographic symmetry is discussed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:00:00 GMT"
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] | 2007-11-28T00:00:00 | [
[
"Losev",
"A.",
""
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711.4212 | Jaromir Fiurasek | Jaromir Fiurasek, Nicolas J. Cerf | Quantum cloning a pair of orthogonally polarized photons with linear
optics | 6 pages, 2 figures, RevTeX4 | Phys. Rev. A 77, 052308 (2008). | 10.1103/PhysRevA.77.052308 | null | quant-ph | null | A linear optical probabilistic scheme for the optimal cloning of a pair of
orthogonally-polarized photons is devised, based on single- and two-photon
interferences. It consists in a partial symmetrization device, realized with a
modified unbalanced Mach-Zehnder interferometer, followed by two independent
Hong-Ou-Mandel interferometers. This scheme has the advantage that it enables
quantum cloning without the need for stimulated amplification in a nonlinear
medium. It can also be modified so to make an optical two-qubit partial SWAP
gate, thereby providing a potentially useful tool to linear optics quantum
computing.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:00:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fiurasek",
"Jaromir",
""
],
[
"Cerf",
"Nicolas J.",
""
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711.4213 | Yoichi Ando | Yoichi Ando (Osaka University) | Implication of the Mott-limit violation in high-Tc cuprates | 5 pages, 5 figures; manuscript for the Proceedings of SNS2007 to be
published as a Special Issue of the Journal of Physics and Chemistry of
Solids | null | 10.1016/j.jpcs.2008.06.074 | null | cond-mat.supr-con cond-mat.str-el | null | The Fermi arc is a striking manifestation of the strong-correlation physics
in high-T_c cuprates. In this paper, implications of the metallic transport in
the lightly hole-doped regime of the cuprates, where the Fermi arcs are found,
are examined in conjunction with competing interpretations of the Fermi arcs in
terms of small hole pockets or a large underlying Fermi surface. It is
discussed that the latter picture provides a more natural understanding of the
metallic transport in view of the Mott-limit argument. Furthermore, it is shown
that a suitable modeling of the Fermi arcs in the framework of the Boltzmann
theory allows us to intuitively understand why the transport properties are
apparently determined by a "small" carrier density even when the underlying
Fermi surface, and hence k_F, is large.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:10:39 GMT"
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] | 2009-11-13T00:00:00 | [
[
"Ando",
"Yoichi",
"",
"Osaka University"
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] |
711.4214 | Yoichi Ando | Yoichi Ando (Osaka Univ.), X. F. Sun (USTC), and Kouji Segawa (Osaka
Univ.) | Pitfalls in the analysis of low-temperature thermal conductivity of
high-Tc cuprates | 4 pages, 1 figure; manuscript for the Proceedings of LEHTSC2007 to be
published in Journal of Physics: Conference Series | J. Phys.: Conference Series 108, 012001 (2008) | 10.1088/1742-6596/108/1/012001 | null | cond-mat.supr-con cond-mat.str-el | null | Recently, it was proposed that phonons are specularly reflected below about
0.5 K in ordinary single-crystal samples of high-T_c cuprates, and that the
low-temperature thermal conductivity should be analyzed by fitting the data up
to 0.5 K using an arbitrary power law. Such an analysis yields a result
different from that obtained from the conventional analysis, in which the
fitting is usually restricted to a region below 0.15 K. Here we show that the
proposed new analysis is most likely flawed, because the specular phonon
reflection means that the phonon mean free path \ell gets LONGER than the mean
sample width, while the estimated \ell is actually much SHORTER than the mean
sample width above 0.15 K.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:10:57 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Ando",
"Yoichi",
"",
"Osaka Univ."
],
[
"Sun",
"X. F.",
"",
"USTC"
],
[
"Segawa",
"Kouji",
"",
"Osaka\n Univ."
]
] | [
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] |
711.4215 | Lukas Jelinek | J. D. Baena, L. Jelinek, R. Marques, M. Silveirinha | Unified Homogenization Theory for Magnetoinductive and Electromagnetic
Waves in Split Ring Metamaterials | 4 pages, 3 figures | Phys. Rev. A 78, 013842, 2008 | 10.1103/PhysRevA.78.013842 | null | physics.optics | null | A unified homogenization procedure for split ring metamaterials taking into
account time and spatial dispersion is introduced. The procedure is based on
two coupled systems of equations. The first one comes from an approximation of
the metamaterial as a cubic arrangement of coupled LC circuits, giving the
relation between currents and local magnetic field. The second equation comes
from macroscopic Maxwell equations, and gives the relation between the
macroscopic magnetic field and the average magnetization of the metamaterial.
It is shown that electromagnetic and magnetoinductive waves propagating in the
metamaterial are obtained from this analysis. Therefore, the proposed time and
spatially dispersive permeability accounts for the characterization of the
complete spectrum of waves of the metamaterial. Finally, it is shown that the
proposed theory is in good quantitative and qualitative agreement with full
wave simulations.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:12:42 GMT"
}
] | 2014-09-10T00:00:00 | [
[
"Baena",
"J. D.",
""
],
[
"Jelinek",
"L.",
""
],
[
"Marques",
"R.",
""
],
[
"Silveirinha",
"M.",
""
]
] | [
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] |
711.4216 | Francesco Fontani | F. Fontani, P. Caselli, T.L. Bourke, R. Cesaroni, J. Brand | Highly deuterated pre-stellar cores in a high-mass star formation region | 4 pages, 2 figures, accepted for publication in Astronomy and
Astrophysics | null | 10.1051/0004-6361:20078973 | null | astro-ph | null | We have observed the deuterated gas in the high-mass star formation region
IRAS 05345+3157 at high-angular resolution, in order to determine the
morphology and the nature of such gas. We have mapped the N2H+ (1-0) line with
the Plateau de Bure Interferometer, and the N2D+ (3-2) and N2H+ (3-2) lines
with the Submillimeter Array. The N2D+ (3-2) integrated emission is
concentrated in two condensations, with masses of 2-3 and 9 M_sun and diameters
of 0.05 and 0.09 pc, respectively. The high deuterium fractionation (0.1) and
the line parameters in the N2D+ condensations indicate that they are likely
low- to intermediate-mass pre-stellar cores, even though other scenarios are
possible.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:17:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fontani",
"F.",
""
],
[
"Caselli",
"P.",
""
],
[
"Bourke",
"T. L.",
""
],
[
"Cesaroni",
"R.",
""
],
[
"Brand",
"J.",
""
]
] | [
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] |
711.4217 | Kees Middelburg | J. A. Bergstra, C. A. Middelburg | Instruction sequences with dynamically instantiated instructions | 25 pages; phrasing improved | Fundamenta Informaticae, 96(1--2):27--48, 2009 | 10.3233/FI-2009-165 | PRG0710 | cs.PL | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study sequential programs that are instruction sequences with dynamically
instantiated instructions. We define the meaning of such programs in two
different ways. In either case, we give a translation by which each program
with dynamically instantiated instructions is turned into a program without
them that exhibits on execution the same behaviour by interaction with some
service. The complexity of the translations differ considerably, whereas the
services concerned are equally simple. However, the service concerned in the
case of the simpler translation is far more powerful than the service concerned
in the other case.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:24:34 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 08:06:27 GMT"
},
{
"version": "v3",
"created": "Wed, 2 Jul 2008 08:08:28 GMT"
},
{
"version": "v4",
"created": "Tue, 4 Aug 2009 06:37:50 GMT"
}
] | 2010-01-12T00:00:00 | [
[
"Bergstra",
"J. A.",
""
],
[
"Middelburg",
"C. A.",
""
]
] | [
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711.4218 | Ingrid Van Keilegom | Ingrid Van Keilegom, C\'esar S\'anchez Sellero, Wenceslao Gonz\'alez
Manteiga | Empirical likelihood based testing for regression | Published in at http://dx.doi.org/10.1214/07-EJS152 the Electronic
Journal of Statistics (http://www.i-journals.org/ejs/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Electronic Journal of Statistics 2008, Vol. 2, 581-604 | 10.1214/07-EJS152 | IMS-EJS-EJS_2007_152 | math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Consider a random vector $(X,Y)$ and let $m(x)=E(Y|X=x)$. We are interested
in testing $H_0:m\in {\cal M}_{\Theta,{\cal G}}=\{\gamma(\cdot,\theta,g):\theta
\in \Theta,g\in {\cal G}\}$ for some known function $\gamma$, some compact set
$\Theta \subset $IR$^p$ and some function set ${\cal G}$ of real valued
functions. Specific examples of this general hypothesis include testing for a
parametric regression model, a generalized linear model, a partial linear
model, a single index model, but also the selection of explanatory variables
can be considered as a special case of this hypothesis. To test this null
hypothesis, we make use of the so-called marked empirical process introduced by
\citeD and studied by \citeSt for the particular case of parametric regression,
in combination with the modern technique of empirical likelihood theory in
order to obtain a powerful testing procedure. The asymptotic validity of the
proposed test is established, and its finite sample performance is compared
with other existing tests by means of a simulation study.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:34:14 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jul 2008 14:14:09 GMT"
}
] | 2008-07-16T00:00:00 | [
[
"Van Keilegom",
"Ingrid",
""
],
[
"Sellero",
"César Sánchez",
""
],
[
"Manteiga",
"Wenceslao González",
""
]
] | [
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711.4219 | Kluson Josef | J. Kluson | Fundamental String and D1-brane in I-brane Background | 16 pages, reference added | JHEP0801:045,2008 | 10.1088/1126-6708/2008/01/045 | null | hep-th | null | This paper is devoted to the study of dynamics of fundamental string and
D1-brane in I-brane background. We consider configurations where string and
D1-brane uniformly wrap transverse spheres. We explicitly determine
corresponding conserved charges and find relations between them.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:51:17 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Dec 2007 13:25:07 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kluson",
"J.",
""
]
] | [
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] |
711.422 | David Gruenewald | David Gruenewald | Computing Humbert Surfaces | 7 pages | null | null | null | math.NT math.AG | null | We describe an algorithm which computes components of Humbert surfaces in
terms of Rosenhain invariants, based on Runge's method
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:06:38 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Gruenewald",
"David",
""
]
] | [
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] |
711.4221 | Matteo Cirillo Prof. | F. Stella, M. Casalboni, M. Cirillo, V. Merlo, C. Palazzesi, G. P.
Pepe, P. Prosposito, and M. Salvato | Integrating Superconductive and Optical Circuits | Document composed of 7 pages of text and 3 figures | null | 10.1063/1.2931700 | null | cond-mat.supr-con cond-mat.mtrl-sci | null | We have integrated on oxidized silicon wafers superconductive films and
Josephson junctions along with sol-gel optical channel waveguides. The
fabrication process is carried out in two steps that result to be solid and
non-invasive. It is demonstrated that 660 nm light, coupled from an optical
fibre into the channel sol-gel waveguide, can be directed toward
superconducting tunnel junctions whose current-voltage characteristics are
affected by the presence of the radiation. The dependence of the change in the
superconducting energy gap under optical pumping is discussed in terms of a
non-equilibrium superconductivity model.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 10:56:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Stella",
"F.",
""
],
[
"Casalboni",
"M.",
""
],
[
"Cirillo",
"M.",
""
],
[
"Merlo",
"V.",
""
],
[
"Palazzesi",
"C.",
""
],
[
"Pepe",
"G. P.",
""
],
[
"Prosposito",
"P.",
""
],
[
"Salvato",
"M.",
""
]
] | [
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] |
711.4222 | Carlo Giunti | Mario A. Acero, Carlo Giunti, Marco Laveder | Limits on nu_e and anti-nu_e disappearance from Gallium and reactor
experiments | 21 pages. Final version to be published in Phys. Rev. D | Phys.Rev.D78:073009,2008 | 10.1103/PhysRevD.78.073009 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The deficit observed in the Gallium radioactive source experiments is
interpreted as a possible indication of the disappearance of electron
neutrinos. In the effective framework of two-neutrino mixing we obtain
$\sin^{2}2\vartheta \gtrsim 0.03$ and $\Delta{m}^{2} \gtrsim 0.1
\text{eV}^{2}$. The compatibility of this result with the data of the Bugey and
Chooz reactor short-baseline antineutrino disappearance experiments is studied.
It is found that the Bugey data present a hint of neutrino oscillations with
$0.02 \lesssim \sin^{2}2\vartheta \lesssim 0.08$ and $\Delta{m}^{2} \approx 1.8
\text{eV}^{2}$, which is compatible with the Gallium allowed region of the
mixing parameters. This hint persists in the combined analyses of Bugey and
Chooz data, of Gallium and Bugey data, and of Gallium, Bugey, and Chooz data.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:11:33 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 10:03:40 GMT"
},
{
"version": "v3",
"created": "Wed, 17 Sep 2008 09:32:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Acero",
"Mario A.",
""
],
[
"Giunti",
"Carlo",
""
],
[
"Laveder",
"Marco",
""
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711.4223 | Pelaez | J.R. Pel\'aez and G. R\'ios | Scalar mesons from Unitarized Chiral Perturbation Theory: N_c and quark
mass dependences | Invited talk to the 11th International Conference on Meson-Nucleon
Physics and the Structure of the Nucleon, Sept. 10th-14th 2007 (MENU 2007),
Juelich, Germany. 10 pages, 3 figures | ECONFC070910:157,2007 | null | null | hep-ph | null | We review recent studies of light scalar meson properties by means of
unitarization techniques, obtained from dispersion theory, and applied to the
Chiral Perturbation Theory expansion. In particular, light scalars do not
follow the N_c dependence of $\bar q q$ states although a subdominant
quark-antiquark component may be observed to arise for the f_0(600) around 1
GeV, where another quark-antiquark multiplet is believed to exist. Finally, we
present our preliminary results on the quark mass dependence of the f_0(600)
and rho(770) resonances.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:32:22 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Peláez",
"J. R.",
""
],
[
"Ríos",
"G.",
""
]
] | [
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711.4224 | Pop Adrian | Pop Adrian Alin | Perturbations for the Coulomb - Kepler problem on de Sitter space-time | 6 pages | null | null | null | gr-qc | null | In the Schrodinger picture of the Dirac quantum mechanics, defined in charts
with spatially flat Robertson-Walker metrics and Cartesian coordinates the
perturbation theory is applied to the interacting part of the Hamiltonian
operator produced by the minimal coupling with the gravitational field. First
and second order perturbations are computed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:12:10 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Alin",
"Pop Adrian",
""
]
] | [
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711.4225 | Tom Fischer | Tom Fischer | Consumption processes and positively homogeneous projection properties | 24 pages, 2 figures | Fischer, T., 2008. Consumption processes and positively
homogeneous projection properties. Finance & Stochastics 12 (3), 357-380 | 10.1007/s00780-008-0064-x | null | q-fin.GN math.OC | null | We constructively prove the existence of time-discrete consumption processes
for stochastic money accounts that fulfill a pre-specified positively
homogeneous projection property (PHPP) and let the account always be positive
and exactly zero at the end. One possible example is consumption rates forming
a martingale under the above restrictions. For finite spaces, it is shown that
any strictly positive consumption strategy with restrictions as above possesses
at least one corresponding PHPP and could be constructed from it. We also
consider numeric examples under time-discrete and -continuous account
processes, cases with infinite time horizons and applications to income
drawdown and bonus theory.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:20:59 GMT"
}
] | 2012-06-21T00:00:00 | [
[
"Fischer",
"Tom",
""
]
] | [
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] |
711.4226 | Bertrand Patureau-Mirand | Nathan Geer, Bertrand Patureau-Mirand | On the Colored HOMFLY-PT, Multivariable and Kashaev Link Invariants | 16 pages | null | null | null | math.GT math.QA | null | We study various specializations of the colored HOMFLY-PT polynomial. These
specializations are used to show that the multivariable link invariants arising
from a complex family of sl(m|n) super-modules previously defined by the
authors contains both the multivariable Alexander polynomial and Kashaev's
invariants. We conjecture these multivariable link invariants also specialize
to the generalized multivariable Alexander invariants defined by Y. Akutsu, T.
Deguchi, and T. Ohtsuki.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:21:04 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Geer",
"Nathan",
""
],
[
"Patureau-Mirand",
"Bertrand",
""
]
] | [
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-0.0065462091,
-0.0617532283,
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-0.1192078441,
-0.077165328,
-0.0840326175,
-0.0483069606,
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-0.0211129989,
0.1015416011,
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-0.0287010968,
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] |
711.4227 | Le Bolloc'h David | D. Le Bolloc'h, V.L.R. Jacques, N. Kirova, J. Dumas, S. Ravy, J.
Marcus, F. Livet | Observation of correlations up to the micrometer scale in sliding
charge-density waves | 4 pages, 3 figures Typos added, references removed | null | 10.1103/PhysRevLett.100.096403 | null | cond-mat.str-el | null | High-resolution coherent x-ray diffraction experiment has been performed on
the charge density wave (CDW) system K$_{0.3}$MoO$_3$. The $2k_F$ satellite
reflection associated with the CDW has been measured with respect to external
dc currents. In the sliding regime, the $2k_F$ satellite reflection displays
secondary satellites along the chain axis which corresponds to correlations up
to the micrometer scale. This super long range order is 1500 times larger than
the CDW period itself. This new type of electronic correlation seems inherent
to the collective dynamics of electrons in charge density wave systems. Several
scenarios are discussed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:24:22 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Dec 2007 13:11:07 GMT"
},
{
"version": "v3",
"created": "Tue, 8 Jan 2008 14:03:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bolloc'h",
"D. Le",
""
],
[
"Jacques",
"V. L. R.",
""
],
[
"Kirova",
"N.",
""
],
[
"Dumas",
"J.",
""
],
[
"Ravy",
"S.",
""
],
[
"Marcus",
"J.",
""
],
[
"Livet",
"F.",
""
]
] | [
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] |
711.4228 | Frank Morgan | Frank Morgan | Existence of Least-perimeter Partitions | 5 pages; for submission to Fortes memorial isue of Philosphical
Magazine Letters | null | 10.1080/09500830801992849 | null | math.MG math.DG | null | We prove the existence of a perimeter-minimizing partition of R^n into
regions of unit volume. We conclude with a short tribute to the late Manuel A.
Fortes.
| [
{
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"created": "Tue, 27 Nov 2007 11:26:05 GMT"
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{
"version": "v2",
"created": "Tue, 19 Feb 2008 02:26:18 GMT"
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] | 2009-11-13T00:00:00 | [
[
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711.4229 | Bertrand Patureau-Mirand | Nathan Geer, Bertrand Patureau-Mirand, Vladimir Turaev | Modified quantum dimensions and re-normalized link invariants | 16 pages | Compositio Mathematica, volume 145 (2009), issue 01, pp. 196-212 | 10.1112/S0010437X08003795 | null | math.QA math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we give a re-normalization of the Reshetikhin-Turaev quantum
invariants of links, by modified quantum dimensions. In the case of simple Lie
algebras these modified quantum dimensions are proportional to the usual
quantum dimensions. More interestingly we will give two examples where the
usual quantum dimensions vanish but the modified quantum dimensions are
non-zero and lead to non-trivial link invariants. The first of these examples
is a class of invariants arising from Lie superalgebras previously defined by
the first two authors. These link invariants are multivariable and generalize
the multivariable Alexander polynomial. The second example, is a hierarchy of
link invariants arising from nilpotent representations of quantized sl(2) at a
root of unity. These invariants contain Kashaev's quantum dilogarithm
invariants of knots.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:34:17 GMT"
},
{
"version": "v2",
"created": "Wed, 25 Sep 2013 08:08:00 GMT"
}
] | 2013-09-26T00:00:00 | [
[
"Geer",
"Nathan",
""
],
[
"Patureau-Mirand",
"Bertrand",
""
],
[
"Turaev",
"Vladimir",
""
]
] | [
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711.423 | S\'ebastien Comer\'on | S. Comer\'on (1), J. H. Knapen (1), J. E. Beckman (1, 2), I. Shlosman
(3) ((1) Instituto de Astrofisica de Canarias, (2) Consejo Superior de
Investigaciones Cientificas, (3) University of Kentucky) | Discovery of ultra-compact nuclear rings in three spiral galaxies | 6 pages, 2 Figures, Accepted for publication in Astronomy &
Astrophysics | null | 10.1051/0004-6361:20078845 | null | astro-ph | null | Ring-shaped morphologies of nuclear star-forming regions within the central
40-200 pc of disk galaxies have been barely resolved so far in three composite
Sy2 nuclei, the Sy2 Circinus galaxy and in three non-AGN galaxies. Such
morphologies resemble those of the standard 1 kpc-size nuclear rings that lie
in the inner Lindblad resonance regions of disk galaxies and, if they have a
similar origin, represent recent radial gas inflows tantalisingly close to the
central supermassive black holes. We aim to identify the population of such
ultra-compact nuclear rings (UCNRs) and study their properties in relation to
those of the host galaxies. From archival Hubble Space Telescope UV and Halpha
images and from dust structure maps of the circumnuclear regions in nearby
galaxies, we analyse the morphology of the star formation and dust,
specifically searching for ring structures on the smallest observable scales.
In a sample of 38 galaxies studied, we have detected a total of four new UCNRs,
30-130 pc in radius, in three different galaxies. Including our confirmation of
a previous UCNR detection, this yields a UCNR fraction of roughly 10%, although
our sample is neither complete nor unbiased. For the first time we resolve
UCNRs in two LINERs. Overall the UCNR phenomenon appears widespread and limited
neither to late-type galaxies nor exclusively to AGN hosts.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:02:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Comerón",
"S.",
""
],
[
"Knapen",
"J. H.",
""
],
[
"Beckman",
"J. E.",
""
],
[
"Shlosman",
"I.",
""
]
] | [
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] |
711.4231 | Bertrand Patureau-Mirand | Nathan Geer, Bertrand Patureau-Mirand | An invariant supertrace for the category of representations of Lie
superalgebras | 19 pages | null | null | null | math.RT math.QA | null | In this paper we give a re-normalization of the supertrace on the category of
representations of Lie superalgebras of type I, by a kind of modified
superdimension. The genuine superdimensions and supertraces are generically
zero. However, these modified superdimensions are non-zero and lead to a kind
of supertrace which is non-trivial and invariant. As an application we show
that this new supertrace gives rise to a non-zero bilinear form on a space of
invariant tensors of a Lie superalgebra of type I. The results of this paper
are completely classical results in the theory of Lie superalgebras but
surprisingly we can not prove them without using quantum algebra and
low-dimensional topology.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:44:15 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Geer",
"Nathan",
""
],
[
"Patureau-Mirand",
"Bertrand",
""
]
] | [
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711.4232 | Golden Gadzirayi Nyambuya Mr. | G. G. Nyambuya | Lepton Generation Problem, Some Properties and Implications of the
Curved Spacetime Dirac Equation -- (II) | I figure added, Improvements to the arguments made | null | null | null | physics.gen-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This reading is a continuation of the earlier reading Nyambuya (2008); where
three new Curved Spacetime Dirac Equations have been derived mainly to try and
account in a natural way for the observed anomalous gyromagnetic ratio of
fermions and the suggestions is that particles including the Electron, which is
thought to be a point particle, do have a finite spatial size and this is one
of the reasons for the observed anomalous gyromagnetic ratio. Combining the
idea in Nyambuya (2008) which lead to the derivation of the three new Curved
Spacetime Dirac Equations, and the proposed Unified Field Theory (Nyambuya
2007), a total of 12 equations each with 16 sub-components are generated thus
leading to a total of 192 equations for the Curved Spacetime Dirac Equation.
Some symmetries of these equations are investigated, i.e., the Lorentz
symmetry, charge conjugation symmetry (C), time reversal symmetry (T), Space
reversal (P) and a combination of the C, P and T - symmetries. It is shown that
these equations are Lorentz invariant, obey C-symmetry and that some violate T
and P-symmetry while others do not and that they all obey PT-symmetry. These
symmetries show (or modestly said -- seem to suggest) that anti-particles have
positive mass and energy but a negative rest-mass and the opposite sign in
electronic charge. Through the inspection of these symmetries, a suggestion is
(here) made to the effect that the rest-mass of a particle must be related to
the electronic charge of that particle thus leading us to a possible resolution
of whether or not Neutrinos do have a none-zero rest-mass. Additionally, we
demonstrate that these equations have the potency to explain naturally the
observed lepton generation phenomena.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:45:16 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 19:25:23 GMT"
},
{
"version": "v3",
"created": "Mon, 7 Jan 2008 09:27:39 GMT"
},
{
"version": "v4",
"created": "Fri, 27 Jun 2008 12:15:29 GMT"
},
{
"version": "v5",
"created": "Sat, 6 Sep 2008 08:05:23 GMT"
},
{
"version": "v6",
"created": "Fri, 22 Jan 2010 00:54:09 GMT"
}
] | 2010-01-22T00:00:00 | [
[
"Nyambuya",
"G. G.",
""
]
] | [
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711.4233 | K. Shizuya | K. Shizuya | Static structure factor for graphene in a magnetic field | 7 pages, 3 figures, revtex | Phys. Rev. B 77, 075419 (2008) | 10.1103/PhysRevB.77.075419 | YITP-07-80 | cond-mat.mes-hall | null | A close study is made of the static structure factor for graphene in a
magnetic field at integer filling factors nu, with focus on revealing possible
signatures of "relativistic" quantum field theory in the low-energy physics of
graphene. It is pointed out, in particular, that for graphene even the vacuum
state has a nonzero density spectral weight, which, together with the structure
factor for all nu, grows significantly with increasing wave vector; such
unusual features of density correlations are a "relativistic" effect deriving
from massless Dirac quasiparticles in graphene. Remarkably it turns out that
the zero-energy Landau levels of electrons or holes, characteristic to
graphene, remain indistinguishable in density response from the vacuum state,
although they are distinct in Hall conductance.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:45:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shizuya",
"K.",
""
]
] | [
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] |
711.4234 | Ivan Dmitriev | I.A. Dmitriev, F. Evers, I.V. Gornyi, A.D. Mirlin, D.G. Polyakov, and
P. W\"olfle | Magnetotransport of electrons in quantum Hall systems | Mini-review for Proceedings of the DFG Priority Progamme "Quantum
Hall Systems"; to be published in a special issue of Physica Status Solidi
(b); 27 pages, 22 figures | physica status solidi (b), 245, 239 (2008) | 10.1002/pssb.200743278 | null | cond-mat.dis-nn cond-mat.mes-hall | null | Recent theoretical results on magnetotransport of electrons in a 2D system in
the range of moderately strong transverse magnetic fields are reviewed. The
phenomena discussed include: quasiclassical memory effects in systems with
various types of disorder, transport in lateral superlattices,
interaction-induced quantum magnetoresistance, quantum magnetooscillations in
dc and ac transport, and oscillatory microwave photoconductivity.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:05:30 GMT"
}
] | 2008-02-01T00:00:00 | [
[
"Dmitriev",
"I. A.",
""
],
[
"Evers",
"F.",
""
],
[
"Gornyi",
"I. V.",
""
],
[
"Mirlin",
"A. D.",
""
],
[
"Polyakov",
"D. G.",
""
],
[
"Wölfle",
"P.",
""
]
] | [
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] |
711.4235 | Asato Tsuchiya | Takaaki Ishii, Goro Ishiki, Kazutoshi Ohta, Shinji Shimasaki, Asato
Tsuchiya | On relationships among Chern-Simons theory, BF theory and matrix model | 20 pages, references added, typos corrected | Prog.Theor.Phys.119:863-882,2008 | 10.1143/PTP.119.863 | OU-HET 592, TU-786 | hep-th | null | Chern-Simons theory on a U(1) bundle over a Riemann surface \Sigma_g of genus
g is dimensionally reduced to BF theory with a mass term, which is equivalent
to the two-dimensional Yang-Mills on \Sigma_g. We show that the former is
inversely obtained from the latter by the extended matrix T-duality developed
in hep-th/0703021. For the case of g=0 (i.e. S^2), the U(1) bundle represents
the lens space S^3/Z_p. We find that in this case both the Chern-Simons theory
and the BF theory with the mass term are realized in a matrix model. We also
construct Wilson loops in the matrix model that correspond to those in the
Chern-Simons theory on S^3.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 11:58:04 GMT"
},
{
"version": "v2",
"created": "Fri, 30 May 2008 04:00:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ishii",
"Takaaki",
""
],
[
"Ishiki",
"Goro",
""
],
[
"Ohta",
"Kazutoshi",
""
],
[
"Shimasaki",
"Shinji",
""
],
[
"Tsuchiya",
"Asato",
""
]
] | [
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] |
711.4236 | Aad Dijksma | D. Alpay, A. Dijksma, H. Langer | The Schur transformation for Nevanlinna functions: operator
representations, resolvent matrices, and orthogonal polynomials | 37 pages | null | null | null | math.FA math.CV | null | A Nevanlinna function is a function which is analytic in the open upper half
plane and has a non-negative imaginary part there. In this paper we study a
fractional linear transformation for a Nevanlinna function $n$ with a suitable
asymptotic expansion at $\infty$, that is an analogue of the Schur
transformation for contractive analytic functions in the unit disc. Applying
the transformation $p$ times we find a Nevanlinna function $n_p$ which is a
fractional linear transformation of the given function $n$. The main results
concern the effect of this transformation to the realizations of $n$ and $n_p$,
by which we mean their representations through resolvents of self-adjoint
operators in Hilbert space. Our tools are block operator matrix
representations, $u$--resolvent matrices, and reproducing kernel Hilbert
spaces.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:03:22 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Alpay",
"D.",
""
],
[
"Dijksma",
"A.",
""
],
[
"Langer",
"H.",
""
]
] | [
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] |
711.4237 | Henning Bostelmann | Henning Bostelmann, Claudio D'Antoni, Gerardo Morsella | Scaling algebras and pointlike fields: A nonperturbative approach to
renormalization | minor changes and clarifications; as to appear in Commun. Math.
Phys.; 37 pages | Commun.Math.Phys.285:763-798,2009 | 10.1007/s00220-008-0613-3 | ESI-1985 | math-ph hep-th math.MP math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a method of short-distance analysis in quantum field theory that
does not require choosing a renormalization prescription a priori. We set out
from a local net of algebras with associated pointlike quantum fields. The net
has a naturally defined scaling limit in the sense of Buchholz and Verch; we
investigate the effect of this limit on the pointlike fields. Both for the
fields and their operator product expansions, a well-defined limit procedure
can be established. This can always be interpreted in the usual sense of
multiplicative renormalization, where the renormalization factors are
determined by our analysis. We also consider the limits of symmetry actions. In
particular, for suitable limit states, the group of scaling transformations
induces a dilation symmetry in the limit theory.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:10:48 GMT"
},
{
"version": "v2",
"created": "Tue, 14 Oct 2008 09:58:40 GMT"
}
] | 2009-01-01T00:00:00 | [
[
"Bostelmann",
"Henning",
""
],
[
"D'Antoni",
"Claudio",
""
],
[
"Morsella",
"Gerardo",
""
]
] | [
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] |
711.4238 | Goulnara N. Arzhantseva | G. Arzhantseva, M.R. Bridson, T. Januszkiewicz, I. J. Leary, A.
Minasyan, J. Swiatkowski | Infinite groups with fixed point properties | Version 2: 29 pages. This is the final published version of the
article | Geom. Topol. 13 (2009) 1229-1263 | 10.2140/gt.2009.13.1229 | null | math.GR math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We construct finitely generated groups with strong fixed point properties.
Let $\mathcal{X}_{ac}$ be the class of Hausdorff spaces of finite covering
dimension which are mod-$p$ acyclic for at least one prime $p$. We produce the
first examples of infinite finitely generated groups $Q$ with the property that
for any action of $Q$ on any $X\in \mathcal{X}_{ac}$, there is a global fixed
point. Moreover, $Q$ may be chosen to be simple and to have Kazhdan's property
(T). We construct a finitely presented infinite group $P$ that admits no
non-trivial action by diffeomorphisms on any smooth manifold in
$\mathcal{X}_{ac}$. In building $Q$, we exhibit new families of hyperbolic
groups: for each $n\geq 1$ and each prime $p$, we construct a non-elementary
hyperbolic group $G_{n,p}$ which has a generating set of size $n+2$, any proper
subset of which generates a finite $p$-group.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:27:39 GMT"
},
{
"version": "v2",
"created": "Mon, 20 Apr 2009 10:25:31 GMT"
}
] | 2014-11-11T00:00:00 | [
[
"Arzhantseva",
"G.",
""
],
[
"Bridson",
"M. R.",
""
],
[
"Januszkiewicz",
"T.",
""
],
[
"Leary",
"I. J.",
""
],
[
"Minasyan",
"A.",
""
],
[
"Swiatkowski",
"J.",
""
]
] | [
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] |
711.4239 | Emiliano Di Gennaro Dr. | E. Di Gennaro, D. Morello, C. Miletto, S. Savo, A. Andreone, G.
Castaldi, V. Galdi, V. Pierro | A parametric study of the lensing properties of dodecagonal photonic
quasicrystals | 12 pages, 8 figures, to be pubblished in Photonics and Nanostructures
- Fundamentals and Applications | null | 10.1016/j.photonics.2007.12.001 | null | physics.optics | null | We present a study of the lensing properties of two-dimensional (2-D)
photonic quasicrystal (PQC) slabs made of dielectric cylinders arranged
according to a 12-fold-symmetric square-triangle aperiodic tiling. Our
full-wave numerical analysis confirms the results recently emerged in the
technical literature and, in particular, the possibility of achieving focusing
effects within several frequency regions. However, contrary to the original
interpretation, such focusing effects turn out to be critically associated to
local symmetry points in the PQC slab, and strongly dependent on its thickness
and termination. Nevertheless, our study reveals the presence of some peculiar
properties, like the ability to focus the light even for slabs with a reduced
lateral width, or beaming effects, which render PQC slabs potentially
interesting and worth of deeper investigation. Key words: Photonic
quasicrystals; negative refraction; superlensing.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:39:24 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Dec 2007 13:57:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Di Gennaro",
"E.",
""
],
[
"Morello",
"D.",
""
],
[
"Miletto",
"C.",
""
],
[
"Savo",
"S.",
""
],
[
"Andreone",
"A.",
""
],
[
"Castaldi",
"G.",
""
],
[
"Galdi",
"V.",
""
],
[
"Pierro",
"V.",
""
]
] | [
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] |
711.424 | Yuri Pogorelov | J.M. Teixeira, J. Ventura, Yu.G. Pogorelov, and J.B. Sousa | Quantum effects in atomically perfect specular spin valve structures | 5 pages, 5 figures | null | 10.1088/0953-8984/20/36/365205 | null | cond-mat.mtrl-sci | null | A simple tight-binding theoretical model is proposed for spin dependent,
current-in-plane transport in highly coherent spin valve structures under
specularity conditions. Using quantum-mechanically coherent and spatially
quantized Fermi states in the considered multilayered system, a system of
partial Boltzmann kinetic equations is built for relevant subbands to yield the
expressions for conductance in parallel or antiparallel spin valve states and
thus for the magneto-conductance. It is shown that specularity favors the
magnetoresistance to reach its theoretical maximum for this structure close to
100%. This result is practically independent of the model parameters, in
particular it does not even need that lifetimes of majority and minority
carriers be different (as necessary for the quasiclassical regimes). The main
MR effect in the considered limit is due to the transformation of coherent
quantum states, induced by the relative rotation of magnetization in the FM
layers. Numerical calculation based on the specific Boltzmann equation with an
account of spin-dependent specular reflection at the interfaces is also
performed for a typical choice of material parameters.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:44:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Teixeira",
"J. M.",
""
],
[
"Ventura",
"J.",
""
],
[
"Pogorelov",
"Yu. G.",
""
],
[
"Sousa",
"J. B.",
""
]
] | [
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] |
711.4241 | Bojan Arbutina | Dusan Onic, Bojan Arbutina and Dejan Urosevic | Radial Dependence of Extinction in Parent Galaxies of Supernovae | Accepted for publication in RevMexAA, 10 pages, 6 figures, 6 tables | Revista Mexicana de Astronomia y Astrofisica Vol. 44, pp. 103-110
(2008) | null | null | astro-ph | null | The problem of extinction is the most important issue to be dealt with in the
process of obtaining true absolute magnitudes of core-collapse (including
stripped-envelope) supernovae (SNe). The plane-parallel model, widely used in
the past, was shown not to describe extinction adequately. We try to apply an
alternative model which introduces radial dependance of extinction in parent
galaxies of supernovae. For calculating extinction in our Galaxy we use two
different methods and compare the results obtained. Our analysis is primarily
focused on a chosen sample of stripped-envelope SNe (Ib/c) for which we find
intrinsic peak absolute magnitude $\mathrm{M}_{\mathrm{B}}^{0}=-17.80\pm 0.43$.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:47:16 GMT"
}
] | 2008-03-12T00:00:00 | [
[
"Onic",
"Dusan",
""
],
[
"Arbutina",
"Bojan",
""
],
[
"Urosevic",
"Dejan",
""
]
] | [
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] |
711.4242 | Oliver Piattella | V. Gorini, A. Y. Kamenshchik, U. Moschella, O. F. Piattella and A. A.
Starobinsky | Gauge-invariant analysis of perturbations in Chaplygin gas unified
models of dark matter and dark energy | References added, discussion expanded, matches the published version | JCAP 0802:016,2008 | 10.1088/1475-7516/2008/02/016 | null | astro-ph gr-qc hep-th | null | We exploit the gauge-invariant formalism to analyse the perturbative
behaviour of two cosmological models based on the generalized Chaplygin gas
describing both dark matter and dark energy in the present Universe. In the
first model we consider the generalized Chaplygin gas alone, while in the
second one we add a baryon component to it. We extend our analysis also into
the parameter range $\alpha > 1$, where the generalized Chaplygin gas sound
velocity can be larger than that of light. In the first model we find that the
matter power spectrum is compatible with the observed one only for $\alpha <
10^{-5}$, which makes the generalized Chaplygin gas practically
indistinguishable from $\Lambda$CDM. In the second model we study the evolution
of inhomogeneities of the baryon component. The theoretical power spectrum is
in good agreement with the observed one for almost all values of $\alpha$.
However, the growth of inhomogeneities seems to be particularly favoured either
for sufficiently small values of $\alpha$ or for $\alpha \gtrsim 3$. Thus, it
appears that the viability of the generalized Chaplygin gas as a cosmological
model is stronger when its sound velocity is superluminal. We show that in this
case the generalized Chaplygin gas equation of state can be changed in an
unobservable region in such a way that its equivalent $k$-essence microscopical
model has no problems with causality.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 12:53:18 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Feb 2008 14:04:26 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Gorini",
"V.",
""
],
[
"Kamenshchik",
"A. Y.",
""
],
[
"Moschella",
"U.",
""
],
[
"Piattella",
"O. F.",
""
],
[
"Starobinsky",
"A. A.",
""
]
] | [
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] |
711.4243 | Chay Goldenberg | C. Goldenberg and I. Goldhirsch | Effects of Friction and Disorder on the Quasi-Static Response of
Granular Solids to a Localized Force | 21 pages (PDFLaTeX), 24 figures (some of them bitmapped to save
space); submitted to Phys. Rev. E | null | 10.1103/PhysRevE.77.041303 | null | cond-mat.soft cond-mat.dis-nn cond-mat.mtrl-sci | null | The response to a localized force provides a sensitive test for different
models of stress transmission in granular solids. The elasto-plastic models
traditionally used by engineers have been challenged by theoretical and
experimental results which suggest a wave-like (hyperbolic) propagation of the
stress, as opposed to the elliptic equations of static elasticity. Numerical
simulations of two-dimensional granular systems subject to a localized external
force are employed to examine the nature of stress transmission in these
systems as a function of the magnitude of the applied force, the frictional
parameters and the disorder (polydispersity). The results indicate that in
large systems (typically considered by engineers), the response is close to
that predicted by isotropic elasticity whereas the response of small systems
(or when sufficiently large forces are applied) is strongly anisotropic. In the
latter case the applied force induces changes in the contact network
accompanied by frictional sliding. The larger the coefficient of static
friction, the more extended is the range of forces for which the response is
elastic and the smaller the anisotropy. Increasing the degree of polydispersity
(for the range studied, up to 25%) decreases the range of elastic response.
This article is an extension of a previously published letter [1].
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:02:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Goldenberg",
"C.",
""
],
[
"Goldhirsch",
"I.",
""
]
] | [
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] |
711.4244 | Archana Bora | Archana Bora, Ranjan Gupta, Harinder P. Singh, Jayant Murthy, Rekhesh
Mohan and Kalpana Duorah | A 3D Automated Classification Scheme for the TAUVEX data pipeline | 8 pages, 12 figures, Accepted for publication in MNRAS; High
resolution figures available from the authors on request | Mon. Not. R. Astron. Soc. 384, 827-833 (2008) | 10.1111/j.1365-2966.2007.12764.x | null | astro-ph | null | In order to develop a pipeline for automated classification of stars to be
observed by the TAUVEX ultraviolet space Telescope, we employ an artificial
neural network (ANN) technique for classifying stars by using synthetic spectra
in the UV region from 1250\AA to 3220\AA as the training set and International
Ultraviolet Explorer (IUE) low resolution spectra as the test set. Both the
data sets have been pre-processed to mimic the observations of the TAUVEX
ultraviolet imager. We have successfully classified 229 stars from the IUE low
resolution catalog to within 3-4 spectral sub-class using two different
simulated training spectra, the TAUVEX spectra of 286 spectral types and UVBLUE
spectra of 277 spectral types. Further, we have also been able to obtain the
colour excess (i.e. E(B-V) in magnitude units) or the interstellar reddening
for those IUE spectra which have known reddening to an accuracy of better than
0.1 magnitudes. It has been shown that even with the limitation of data from
just photometric bands, ANNs have not only classified the stars, but also
provided satisfactory estimates for interstellar extinction. The ANN based
classification scheme has been successfully tested on the simulated TAUVEX data
pipeline. It is expected that the same technique can be employed for data
validation in the ultraviolet from the virtual observatories. Finally, the
interstellar extinction estimated by applying the ANNs on the TAUVEX data base
would provide an extensive extinction map for our galaxy and which could in
turn be modeled for the dust distribution in the galaxy.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:28:09 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Dec 2007 08:00:44 GMT"
}
] | 2009-11-09T00:00:00 | [
[
"Bora",
"Archana",
""
],
[
"Gupta",
"Ranjan",
""
],
[
"Singh",
"Harinder P.",
""
],
[
"Murthy",
"Jayant",
""
],
[
"Mohan",
"Rekhesh",
""
],
[
"Duorah",
"Kalpana",
""
]
] | [
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] |
711.4245 | Gerardo Cristofano | Gerardo Cristofano, Vincenzo Marotta, Adele Naddeo, Giuliano Niccoli | Fully frustrated Josephson junction ladders with Mobius boundary
conditions as topologically protected qubits | 21 pages, 2 figures, in print in Phys. Lett. A | Phys. Lett. A 372 (2008) 2464 | 10.1016/j.physleta.2007.11.048 | Napoli DSF-T-16/2007, INFN-NA-16/2007 | quant-ph cond-mat.stat-mech hep-th | null | We show how to realize a ``protected'' qubit by using a fully frustrated
Josephson Junction ladder (JJL) with Mobius boundary conditions. Such a system
has been recently studied within a twisted conformal field theory (CFT)
approach (Mod. Phys. Lett. A 15 (2000) 1679; Nucl. Phys. B 641 (2002) 547) and
shown to develop the phenomenon of flux fractionalization (Eur. Phys. J. B 49
(2006) 83). The relevance of a ``closed'' geometry has been fully exploited in
relating the topological properties of the ground state of the system to the
presence of half flux quanta and the emergence of a topological order has been
predicted (JSTAT (2005) P03006). In this letter the stability and
transformation properties of the ground states under adiabatic magnetic flux
change are analyzed and the deep consequences on the realization of a solid
state qubit, protected from decoherence, are presented.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:06:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cristofano",
"Gerardo",
""
],
[
"Marotta",
"Vincenzo",
""
],
[
"Naddeo",
"Adele",
""
],
[
"Niccoli",
"Giuliano",
""
]
] | [
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] |
711.4246 | Francesco Mainardi | Gianni Pagnini and Francesco Mainardi | Evolution equations of the probabilistic generalization of the Voigt
profile function | 9 pages. 2 Figures Conference ``Special Functions, Information Theory
and Mathematical Physics'',Granada, Spain, September 17-19 2007. Journal of
Computational and Applied Mathematics, in press (2008) | null | null | null | math-ph cond-mat.stat-mech math.MP math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The spectrum profile that emerges in molecular spectroscopy and atmospheric
radiative transfer as the combined effect of Doppler and pressure broadenings
is known as the Voigt profile function. Because of its convolution integral
representation, the Voigt profile can be interpreted as the probability density
function of the sum of two independent random variables with Gaussian density
(due to the Doppler effect) and Lorentzian density (due to the pressure
effect). Since these densities belong to the class of symmetric L\'evy stable
distributions, a probabilistic generalization is proposed as the convolution of
two arbitrary symmetric L\'evy densities. We study the case when the widths of
the considered distributions depend on a scale-factor $\tau$ that is
representative of spatial inhomogeneity or temporal non-stationarity. The
evolution equations for this probabilistic generalization of the Voigt function
are here introduced and interpreted as generalized diffusion equations
containing two Riesz space-fractional derivatives, thus classified as
space-fractional diffusion equations of double order.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:36:12 GMT"
},
{
"version": "v2",
"created": "Thu, 12 Jun 2008 13:03:44 GMT"
}
] | 2008-06-12T00:00:00 | [
[
"Pagnini",
"Gianni",
""
],
[
"Mainardi",
"Francesco",
""
]
] | [
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] |
711.4247 | Pavel Exner | Pavel Exner and Andrea Mantile | On the optimization of the principal eigenvalue for single-centre
point-interaction operators in a bounded region | LaTeX, 15 pages | J. Phys. A: Math. Theor. 41 (2008), 065305 (15pp) | 10.1088/1751-8113/41/6/065305 | null | math-ph math.MP math.SP quant-ph | null | We investigate relations between spectral properties of a single-centre
point-interaction Hamiltonian describing a particle confined to a bounded
domain $\Omega\subset\mathbb{R}^{d},\: d=2,3$, with Dirichlet boundary, and the
geometry of $\Omega$. For this class of operators Krein's formula yields an
explicit representation of the resolvent in terms of the integral kernel of the
unperturbed one, $(-\Delta_{\Omega}^{D}+z) ^{-1}$. We use a moving plane
analysis to characterize the behaviour of the ground-state energy of the
Hamiltonian with respect to the point-interaction position and the shape of
$\Omega$, in particular, we establish some conditions showing how to place the
interaction to optimize the principal eigenvalue.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:15:31 GMT"
}
] | 2019-12-10T00:00:00 | [
[
"Exner",
"Pavel",
""
],
[
"Mantile",
"Andrea",
""
]
] | [
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] |
711.4248 | Ayman Kachmar | Ayman Kachmar | Magnetic vortices for a Ginzburg-Landau type energy with discontinuous
constraint | 34 pages | null | null | null | math.AP math-ph math.MP | null | This paper is devoted to an analysis of vortex-nucleation for a
Ginzburg-Landau functional with discontinuous constraint. This functional has
been proposed as a model for vortex-pinning, and usually accounts for the
energy resulting from the interface of two superconductors. The critical
applied magnetic field for vortex nucleation is estimated in the London
singular limit, and as a by-product, results concerning vortex-pinning and
boundary conditions on the interface are obtained.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:25:11 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 19:19:09 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Kachmar",
"Ayman",
""
]
] | [
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711.4249 | Ivan Dmitriev | I.A. Dmitriev, A.D. Mirlin, and D.G. Polyakov | Fractional microwave-induced resistance oscillations | 3 pages, 2 figures; Proceedings of EP2DS17 to be published in Physica
E; less technical version of arXiv:0707.0990 | null | 10.1016/j.physe.2007.09.003 | null | cond-mat.mes-hall cond-mat.dis-nn | null | We develop a systematic theory of microwave-induced oscillations in
magnetoresistivity of a 2D electron gas in the vicinity of fractional harmonics
of the cyclotron resonance, observed in recent experiments. We show that in the
limit of well-separated Landau levels the effect is dominated by the
multiphoton inelastic mechanism. At moderate magnetic field, two single-photon
mechanisms become important. One of them is due to resonant series of multiple
single-photon transitions, while the other originates from microwave-induced
sidebands in the density of states of disorder-broadened Landau levels.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:49:09 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Dmitriev",
"I. A.",
""
],
[
"Mirlin",
"A. D.",
""
],
[
"Polyakov",
"D. G.",
""
]
] | [
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] |
711.425 | Mairan Teodoro | A. Damineli (1), M. F. Corcoran (3 and 4), D. J. Hillier (2), O. Stahl
(5), R. S. Levenhagen (1), N. V. Leister (1), J. H. Groh (1), M. Teodoro (1),
J. F. Albacete Colombo (6), F. Gonzalez (7), J. Arias (8), H. Levato (7), M.
Grosso (7), N. Morrell (9), R. Gamen (7), G. Wallerstein (10), V. Niemela
(11) ((1) Instituto de Astronomia, Geof\'isica e Ci\^encias Atmosf\'ericas,
Universidade de S\~ao Paulo, Brazil (2) Department of Physics and Astronomy,
University of Pittsburgh, USA (3) CRESST and X-ray Astrophysics Laboratory,
NASA/GSFC, USA (4) Universities Space Research Association, USA (5) ZAH,
Landessternwarte, Germany (6) Facultad de Ciencias Astronomicas y Geofisicas
de La Plata (FCAGLP) (7) Complejo Astronomico El Leoncito, Argentina (8)
Departamento de F\'isica, Universidad de La Serena, Chile (9) Las Campanas
Observatory, Carnegie Observatories, Chile (10) Department of Astronomy,
University of Washington, USA (11) In memoriam) | The periodicity of the eta Carinae events | 9 pages, 4 EPS figures, submitted to MNRAS | null | 10.1111/j.1365-2966.2007.12815.x | null | astro-ph | null | Extensive spectral observations of eta Carinae over the last cycle, and
particularly around the 2003.5 low excitation event, have been obtained. The
variability of both narrow and broad lines, when combined with data taken from
two earlier cycles, reveal a common and well defined period. We have combined
the cycle lengths derived from the many lines in the optical spectrum with
those from broad-band X-rays, optical and near-infrared observations, and
obtained a period length of 2022.7+-1.3 d.
Spectroscopic data collected during the last 60 years yield an average period
of 2020+-4 d, consistent with the present day period. The period cannot have
changed by more than $\Delta$P/P=0.0007 since 1948. This confirms the previous
claims of a true, stable periodicity, and gives strong support to the binary
scenario. We have used the disappearance of the narrow component of HeI 6678 to
define the epoch of the Cycle 11 minimum, T_0=JD 2,452,819.8. The next event is
predicted to occur on 2009 January 11 (+-2 days). The dates for the start of
the minimum in other spectral features and broad-bands is very close to this
date, and have well determined time delays from the HeI epoch.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:14:18 GMT"
}
] | 2016-08-14T00:00:00 | [
[
"Damineli",
"A.",
"",
"3 and 4"
],
[
"Corcoran",
"M. F.",
"",
"3 and 4"
],
[
"Hillier",
"D. J.",
""
],
[
"Stahl",
"O.",
""
],
[
"Levenhagen",
"R. S.",
""
],
[
"Leister",
"N. V.",
""
],
[
"Groh",
"J. H.",
""
],
[
"Teodoro",
"M.",
""
],
[
"Colombo",
"J. F. Albacete",
""
],
[
"Gonzalez",
"F.",
""
],
[
"Arias",
"J.",
""
],
[
"Levato",
"H.",
""
],
[
"Grosso",
"M.",
""
],
[
"Morrell",
"N.",
""
],
[
"Gamen",
"R.",
""
],
[
"Wallerstein",
"G.",
""
],
[
"Niemela",
"V.",
""
]
] | [
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711.4251 | Andr\'e Chailloux | Andr\'e Chailloux and Iordanis Kerenidis | The role of help in Classical and Quantum Zero-Knowledge | 22 pages, 0 figures, This paper will be be superseded by joint work
with Dragos Florin Ciocan and Salil Vadhan and will be presented at TCC'08 | null | null | null | quant-ph | null | We study the role of help in Non-Interactive Zero-Knowledge protocols and its
relation to the standard interactive model. In the classical case, we show that
help and interaction are equivalent, answering an open question of Ben-Or and
Gutfreund. This implies a new complete problem for the class SZK, the Image
Intersection Density. For this problem, we also prove a polarization lemma
which is stronger than the previously known one.
In the quantum setting, we define the notion of quantum help and show in a
more direct way that help and interaction are again equivalent. Moreover, we
define quantum Non-Interactive Zero-Knowledge with classical help and prove
that it is equal to the class of languages that have classical honest-Verifier
Zero Knowledge protocols secure against quantum Verifiers. Last, we provide new
complete problems for all these quantum classes.
Similar results were independently discovered by Dragos Florin Ciocan and
Salil Vadhan.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:48:51 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 14:47:49 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Chailloux",
"André",
""
],
[
"Kerenidis",
"Iordanis",
""
]
] | [
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] |
711.4252 | Eric Jurgenson | E.D. Jurgenson, S.K. Bogner, R.J. Furnstahl, R.J. Perry | Decoupling in the Similarity Renormalization Group for Nucleon-Nucleon
Forces | 13 pages, 14 figures | Phys.Rev.C78:014003,2008 | 10.1103/PhysRevC.78.014003 | null | nucl-th cond-mat.str-el hep-ph | null | Decoupling via the Similarity Renormalization Group (SRG) of low-energy
nuclear physics from high-energy details of the nucleon-nucleon interaction is
examined for two-body observables and few-body binding energies. The universal
nature of this decoupling is illustrated and errors from suppressing
high-momentum modes above the decoupling scale are shown to be perturbatively
small.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:32:07 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Jurgenson",
"E. D.",
""
],
[
"Bogner",
"S. K.",
""
],
[
"Furnstahl",
"R. J.",
""
],
[
"Perry",
"R. J.",
""
]
] | [
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] |
711.4253 | Eduard Simioni | Eduard Simioni | Production and Testing of the LHCb Outer Tracker Front End Readout
Electronics | 5 pages | TWEPP 2007 proceedings | null | null | physics.ins-det | null | The LHCb Outer Tracker is a straw drift detector with a modular design and a
total of 53760 readout channels distributed over a sensitive area of 12 double
layers of 6x5 m2 each. The main electronics readout requirement is the precise
(0.5 ns) drift time measurement at an occupancy of 4% and 1 MHz readout. A
total of 128 channels are read out by one Front-End box. About half of the
FE-Boxes have been built. Quality Assurance during the production has been
performed on single FE-Box components. The assembled FE-Box is finally
commissioned using a special FE-Tester. The FE-Tester is a programmable pulser
with a time resolution of 150 ps capable to simulate all the functionality of
the readout mimicking the real detector. Consequently, problems have been found
and solved resulting in good overall performance.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:58:10 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Simioni",
"Eduard",
""
]
] | [
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] |
711.4254 | Tian-Jun Li | Tian-Jun Li, Yongbin Ruan | Uniruled symplectic divisors | 45 pages | null | null | null | math.SG math.AG | null | This is a paper devoted to the symplectic birational geometry program where
many basic notions are defined in terms of genus 0 GW invariants. We show that
the existence of a positive uniruled symplectic divisor often implies that the
ambient manifold has a nonzero uniruled genus 0 GW invariant, hence is uniruled
as well. This confirms a part of the dichotomy on uniruled symplectic divisors.
In addition, it gives a rather general construction of uniruled symplectic
manifolds, generalizing some beautiful results of McDuff.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 13:59:01 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Li",
"Tian-Jun",
""
],
[
"Ruan",
"Yongbin",
""
]
] | [
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] |
711.4255 | K. Werner | K. Werner, J. Barnstedt, W. Gringel, N. Kappelmann, H. Becker-Ross, S.
Florek, R. Graue, D. Kampf, A. Reutlinger, C. Neumann, B. Shustov, A.
Moisheev, E. Skripunov | HIRDES - The High-Resolution Double-Echelle Spectrograph for the World
Space Observatory Ultraviolet (WSO/UV) | Accepted for publication in Advances in Space Research | Adv.Space Res.41:1992-1997,2008 | 10.1016/j.asr.2007.11.029 | TUE 01/2007 | astro-ph | null | The World Space Observatory Ultraviolet (WSO/UV) is a multi-national project
grown out of the needs of the astronomical community to have future access to
the UV range. WSO/UV consists of a single UV telescope with a primary mirror of
1.7m diameter feeding the UV spectrometer and UV imagers. The spectrometer
comprises three different spectrographs, two high-resolution echelle
spectrographs (the High-Resolution Double-Echelle Spectrograph, HIRDES) and a
low-dispersion long-slit instrument. Within HIRDES the 102-310nm spectral band
is split to feed two echelle spectrographs covering the UV range 174-310nm and
the vacuum-UV range 102-176nm with high spectral resolution (R>50,000). The
technical concept is based on the heritage of two previous ORFEUS SPAS
missions. The phase-B1 development activities are described in this paper
considering performance aspects, design drivers, related trade-offs (mechanical
concepts, material selection etc.) and a critical functional and environmental
test verification approach. The current state of other WSO/UV scientific
instruments (imagers) is also described.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:00:12 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Werner",
"K.",
""
],
[
"Barnstedt",
"J.",
""
],
[
"Gringel",
"W.",
""
],
[
"Kappelmann",
"N.",
""
],
[
"Becker-Ross",
"H.",
""
],
[
"Florek",
"S.",
""
],
[
"Graue",
"R.",
""
],
[
"Kampf",
"D.",
""
],
[
"Reutlinger",
"A.",
""
],
[
"Neumann",
"C.",
""
],
[
"Shustov",
"B.",
""
],
[
"Moisheev",
"A.",
""
],
[
"Skripunov",
"E.",
""
]
] | [
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] |
711.4256 | Kaspar von Braun | Kaspar von Braun, David R. Ciardi (Caltech) | Observational Window Functions in Planet Transit Searches | 8 pages, 6 figures; to appear in the Proceedings of the 249th IAU
Meeting: "Exoplanets: Detection, Formation and Dynamics" (Suzhou, China);
added referee's comments | null | 10.1017/S1743921308016451 | null | astro-ph | null | Window functions describe, as a function of orbital period, the probability
that an existing planetary transit is detectable in one's data for a given
observing strategy. We show the dependence of this probability upon several
strategy and astrophysical parameters, such as length of observing run,
observing cadence, length of night, and transit duration. The ability to detect
a transit is directly related to the intrinsic noise of the observations. In
our simulations of the window function, we explicitly address non-correlated
(gaussian or white) noise and correlated (red) noise and discuss how these two
different noise components affect window functions in different manners.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 01:58:23 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Jan 2008 00:17:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"von Braun",
"Kaspar",
"",
"Caltech"
],
[
"Ciardi",
"David R.",
"",
"Caltech"
]
] | [
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] |
711.4257 | Ralf Hofmann | Jochen Keller, Ralf Hofmann, and Francesco Giacosa | Correlation of energy density in deconfining SU(2) Yang-Mills
thermodynamics | 22 pages, 8 figures, v6: formulas (6), (7), (11), (12), (18), (20)
altered, figures (2), (6), (7), (8) altered, figures (1), (4), (5) exchanged,
no qualitative changes in the results and no change of our conclusions | Int.J.Mod.Phys.A23:5181-5200,2008 | 10.1142/S0217751X08042535 | KA-TP-34-2007 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We compute the two-point correlation of the energy density for the massless
mode in deconfining SU(2) Yang-Mills thermodynamics and point towards a
possible application for the physics of cold, dilute, and stable clouds of
atomic hydrogen within the Milky Way.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:04:48 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 11:00:18 GMT"
},
{
"version": "v3",
"created": "Thu, 21 Feb 2008 10:28:41 GMT"
},
{
"version": "v4",
"created": "Thu, 15 May 2008 14:01:06 GMT"
},
{
"version": "v5",
"created": "Mon, 22 Sep 2008 08:08:53 GMT"
},
{
"version": "v6",
"created": "Wed, 29 Oct 2008 19:47:28 GMT"
}
] | 2009-02-11T00:00:00 | [
[
"Keller",
"Jochen",
""
],
[
"Hofmann",
"Ralf",
""
],
[
"Giacosa",
"Francesco",
""
]
] | [
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] |
711.4258 | Ulrich Kuhl | R. Hoehmann, U. Kuhl, H.-J. Stoeckmann | Algebraic fidelity decay for local perturbations | 4 pages, 5 figures | PRL 100, 124101 (2008) | 10.1103/PhysRevLett.100.124101 | null | quant-ph cond-mat.mes-hall | null | From a reflection measurement in a rectangular microwave billiard with
randomly distributed scatterers the scattering and the ordinary fidelity was
studied. The position of one of the scatterers is the perturbation parameter.
Such perturbations can be considered as {\em local} since wave functions are
influenced only locally, in contrast to, e. g., the situation where the
fidelity decay is caused by the shift of one billiard wall. Using the
random-plane-wave conjecture, an analytic expression for the fidelity decay due
to the shift of one scatterer has been obtained, yielding an algebraic $1/t$
decay for long times. A perfect agreement between experiment and theory has
been found, including a predicted scaling behavior concerning the dependence of
the fidelity decay on the shift distance. The only free parameter has been
determined independently from the variance of the level velocities.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:04:55 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Apr 2008 12:00:08 GMT"
}
] | 2010-06-07T00:00:00 | [
[
"Hoehmann",
"R.",
""
],
[
"Kuhl",
"U.",
""
],
[
"Stoeckmann",
"H. -J.",
""
]
] | [
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] |
711.4259 | Guihua Chen | YongYao Li, HuaRong Zhang, YongZhu Chen, JianYing Zhou | Coherent control of light field with electromagnetically induced
transparency in a dark state Raman coherent tripod system | null | null | null | null | quant-ph | null | The coherent superposition of two-atomic levels induced by coherent
population trapping is employed in a standard $\Lambda$ type scheme to form a
tripod-like system. A weak probe pulse scanning across the system is shown to
experience a crossover from absorption to transparent and then to
amplification. Consequently the group velocity of the probe pulse can be
controlled to propagate either as a subluminal, a standard, a superluminal or
even a negative speed. It is shown that the propagation behavior of the light
field is entirely determined and controlled by the initial states of the
coherent superposition.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:05:14 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Jan 2008 06:19:46 GMT"
}
] | 2008-01-02T00:00:00 | [
[
"Li",
"YongYao",
""
],
[
"Zhang",
"HuaRong",
""
],
[
"Chen",
"YongZhu",
""
],
[
"Zhou",
"JianYing",
""
]
] | [
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] |
711.426 | Roland Donninger | Roland Donninger | Spectral Properties and Stability of Self-Similar Wave Maps | PhD thesis University of Vienna, 143 pages, some typos corrected | null | null | null | math-ph math.MP | null | In this thesis the Cauchy problem and in particular the question of
singularity formation for co--rotational wave maps from 3+1 Minkowski space to
the three--sphere $S^3$ is studied. Numerics indicate that self--similar
solutions of this model play a crucial role in dynamical time evolution. In
particular, it is conjectured that a certain solution $f_0$ defines a universal
blow up pattern in the sense that the future development of a large set of
generic blow up initial data approaches $f_0$. Thus, singularity formation is
closely related to stability properties of self--similar solutions.
In this work, the problem of linear stability is studied by functional
analytic methods. In particular, a complete spectral analysis of the
perturbation operators is given and well--posedness of the linearized Cauchy
problem is proved by means of semigroup theory and, alternatively, the
functional calculus for self--adjoint operators. These results lead to growth
estimates which provide information on the stability of self--similar wave
maps. Finally, convergence properties of $f_n$ for large $n$ and the spectra of
the corresponding perturbation operators are investigated.
The thesis is intended to be self--contained as far as possible, i.e. all the
mathematical requirements are carefully introduced, including proofs for many
results which could be found elsewhere.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:06:02 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Donninger",
"Roland",
""
]
] | [
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] |
711.4261 | Francesco Mainardi | Francesco Mainardi, Gianni Pagnini, Rudolf Gorenflo | Some aspects of fractional diffusion equations of single and distributed
order | 14 pages. International Symposium on "Analytic Function Theory,
Fractional Calculus and Their Applications", University of Victoria (British
Columbia, Canada), 22-27 August 2005 | Applied Mathematics and Computation, Vol. 187, No 1, pp. 295-305
(2007) | 10.1016/j.amc.2006.08.126 | null | math-ph cond-mat.dis-nn cond-mat.stat-mech math.MP | null | The time fractional diffusion equation is obtained from the standard
diffusion equation by replacing the first-order time derivative with a
fractional derivative of order $\beta \in (0,1)$. The fundamental solution for
the Cauchy problem is interpreted as a probability density of a self-similar
non-Markovian stochastic process related to a phenomenon of sub-diffusion (the
variance grows in time sub-linearly). A further generalization is obtained by
considering a continuous or discrete distribution of fractional time
derivatives of order less than one.
Then the fundamental solution is still a probability density of a
non-Markovian process that, however, is no longer self-similar but exhibits a
corresponding distribution of time-scales.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:17:55 GMT"
}
] | 2008-05-27T00:00:00 | [
[
"Mainardi",
"Francesco",
""
],
[
"Pagnini",
"Gianni",
""
],
[
"Gorenflo",
"Rudolf",
""
]
] | [
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] |
711.4262 | Thibault Lagache | T. Lagache, E. Dauty, D. Holcman | Toward a quantitative analysis of virus and plasmid trafficking in cells | 10 pages, 6 figures | null | null | null | q-bio.QM q-bio.SC | null | Intracellular transport of DNA carriers is a fundamental step of gene
delivery. We present here a theoretical approach to study generically a single
virus or DNA particle trafficking in a cell cytoplasm. Cellular trafficking has
been studied experimentally mostly at the macroscopic level, but very little
has been done so far at the microscopic level. We present here a physical model
to account for certain aspects of cellular organization, starting with the
observation that a viral particle trajectory consists of epochs of pure
diffusion and epochs of active transport along microtubules. We define a
general degradation rate to describe the limitations of the delivery of plasmid
or viral particles to the nucleus imposed by various types of direct and
indirect hydrolysis activity inside the cytoplasm. Following a homogenization
procedure, which consists of replacing the switching dynamics by a single
steady state stochastic description, not only can we study the spatio-temporal
dynamics of moving objects in the cytosol, but also estimate the probability
and the mean time to go from the cell membrane to a nuclear pore. Computational
simulations confirm that our model can be used to analyze and interpret viral
trajectories and estimate quantitatively the success of nuclear delivery.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:22:35 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Lagache",
"T.",
""
],
[
"Dauty",
"E.",
""
],
[
"Holcman",
"D.",
""
]
] | [
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] |
711.4263 | Nicola Bartolo | N. Bartolo (1 and 2), S. Matarrese (1 and 2), M. Pietroni (2), A.
Riotto (2 and 3), D. Seery (4) ((1) Physics Dept. Padova, Italy; (2) INFN,
Padova, Italy; (3) CERN, Switzerland; (4) Centre for Theoretical Cosmology,
Cambridge, UK) | On the Physical Significance of Infra-red Corrections to Inflationary
Observables | 11 pages; LateX file; 5 figures. Some coefficients in Eq.(A6)
corrected; References added | JCAP 0801:015,2008 | 10.1088/1475-7516/2008/01/015 | null | astro-ph gr-qc hep-ph hep-th | null | Inflationary observables, like the power spectrum, computed at one- and
higher-order loop level seem to be plagued by large infra-red corrections. In
this short note, we point out that these large infra-red corrections appear
only in quantities which are not directly observable. This is in agreement with
general expectations concerning infra-red effects.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:26:48 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 18:38:45 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Bartolo",
"N.",
"",
"1 and 2"
],
[
"Matarrese",
"S.",
"",
"1 and 2"
],
[
"Pietroni",
"M.",
"",
"2 and 3"
],
[
"Riotto",
"A.",
"",
"2 and 3"
],
[
"Seery",
"D.",
""
]
] | [
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] |
711.4264 | Teppo Mattsson | Teppo Mattsson | Dark energy as a mirage | 33 pages, 2 figs; v2: minor clarifications, results unchanged; v3:
matches the version published in General Relativity and Gravitation | Gen.Rel.Grav.42:567-599,2010 | 10.1007/s10714-009-0873-z | HIP-2007-64/TH | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Motivated by the observed cosmic matter distribution, we present the
following conjecture: due to the formation of voids and opaque structures, the
average matter density on the path of the light from the well-observed objects
changes from Omega_M ~ 1 in the homogeneous early universe to Omega_M ~ 0 in
the clumpy late universe, so that the average expansion rate increases along
our line of sight from EdS expansion Ht ~ 2/3 at high redshifts to free
expansion Ht ~ 1 at low redshifts. To calculate the modified observable
distance-redshift relations, we introduce a generalized Dyer-Roeder method that
allows for two crucial physical properties of the universe: inhomogeneities in
the expansion rate and the growth of the nonlinear structures. By treating the
transition redshift to the void-dominated era as a free parameter, we find a
phenomenological fit to the observations from the CMB anisotropy, the position
of the baryon oscillation peak, the magnitude-redshift relations of type Ia
supernovae, the local Hubble flow and the nucleosynthesis, resulting in a
concordant model of the universe with 90% dark matter, 10% baryons, no dark
energy, 15 Gyr as the age of the universe and a natural value for the
transition redshift z_0=0.35. Unlike a large local void, the model respects the
cosmological principle, further offering an explanation for the late onset of
the perceived acceleration as a consequence of the forming nonlinear
structures. Additional tests, such as quantitative predictions for angular
deviations due to an anisotropic void distribution and a theoretical derivation
of the model, can vindicate or falsify the interpretation that light
propagation in voids is responsible for the perceived acceleration.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 20:47:32 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Dec 2007 09:45:53 GMT"
},
{
"version": "v3",
"created": "Wed, 16 Sep 2009 15:19:53 GMT"
}
] | 2010-02-23T00:00:00 | [
[
"Mattsson",
"Teppo",
""
]
] | [
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711.4265 | Timo Anguita | T. Anguita (1), R.W. Schmidt (1), E.L. Turner (2), J. Wambsganss (1),
R.L. Webster (3), K.A. Loomis (4), D. Long (4), R. McMillan (4) ((1)
ARI/Zentrum fuer Astronomie, University of Heidelberg, (2) Princeton
University, (3) University of Melbourne, (4) Apache Point Observatory) | The multiple quasar Q2237+0305 under a microlensing caustic | Accepted for publication in A&A, 8 pages, 4 figures. Slightly
modified compared to the original version: qualitative results unchanged,
constraints on the r'/g' source size ratio now tighter due to correction of
an error in the numerical treatment of the simulated light curves | null | 10.1051/0004-6361:20078221 | null | astro-ph | null | We use the high magnification event seen in the 1999 OGLE campaign light
curve of image C of the quadruply imaged gravitational lens Q2237+0305 to study
the structure of the quasar engine. We have obtained g'- and r'-band photometry
at the Apache Point Observatory 3.5m telescope where we find that the event has
a smaller amplitude in the r'-band than in the g'- and OGLE V-bands. By
comparing the light curves with microlensing simulations we obtain constraints
on the sizes of the quasar regions contributing to the g'- and r'-band flux.
Assuming that most of the surface mass density in the central kiloparsec of the
lensing galaxy is due to stars and by modeling the source with a Gaussian
profile, we obtain for the Gaussian width 1.20 x 10^15 sqrt(M/0.1M_sun)cm <
sigma_g' < 7.96 x 10^15 sqrt(M/0.1Msun) cm, where M is the mean microlensing
mass, and a ratio sigma_r'/sigma_g'=1.25^{+0.45}_{-0.15}. With the limits on
the velocity of the lensing galaxy from Gil-Merino et al. (2005) as our only
prior, we obtain 0.60 x 10^15 sqrt(M/0.1Msun) cm < sigma_g' < 1.57 x 10^15
sqrt(M/0.1Msun) cm and a ratio sigma_r'/sigma_g'=1.45^{+0.90}_{-0.25} (all
values at 68 percent confidence). Additionally, from our microlensing
simulations we find that, during the chromatic microlensing event observed, the
continuum emitting region of the quasar crossed a caustic at >72 percent
confidence.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:57:04 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jan 2008 17:19:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Anguita",
"T.",
""
],
[
"Schmidt",
"R. W.",
""
],
[
"Turner",
"E. L.",
""
],
[
"Wambsganss",
"J.",
""
],
[
"Webster",
"R. L.",
""
],
[
"Loomis",
"K. A.",
""
],
[
"Long",
"D.",
""
],
[
"McMillan",
"R.",
""
]
] | [
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] |
711.4266 | Parimal Kar | Parimal Kar, Max Seel, Ulrich H.E. Hansmann, Siegfried Hoefinger | Dispersion Terms and Analysis of Size- Charge Dependence in an Enhanced
Poisson Boltzmann Approach | null | J. Phys. Chem. B, 111 (30), 8910 -8918, 2007 | null | null | physics.bio-ph physics.chem-ph | null | We implement a well-established concept to consider dispersion effects within
a Poisson-Boltzmann approach of continuum solvation of proteins. The
theoretical framework is particularly suited for boundary element methods. Free
parameters are determined by comparison to experimental data as well as
high-level quantum mechanical reference calculations. The method is general and
can be easily extended in several directions. The model is tested on various
chemical substances and found to yield good-quality estimates of the solvation
free energy without obvious indication of any introduced bias. Once optimized,
the model is applied to a series of proteins, and factors such as protein size
or partial charge assignments are studied.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:32:32 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Kar",
"Parimal",
""
],
[
"Seel",
"Max",
""
],
[
"Hansmann",
"Ulrich H. E.",
""
],
[
"Hoefinger",
"Siegfried",
""
]
] | [
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] |
711.4267 | Linda \"Ostman | Linda Ostman, Ariel Goobar and Edvard Mortsell | Extinction properties of lensing galaxies | 14 pages, 9 figures. Matches version accepted by A&A | Astron.Astrophys.485:403-415,2008 | 10.1051/0004-6361:20079187 | null | astro-ph | null | Context. Observations of quasars shining through foreground galaxies, offer a
way to probe the dust extinction curves of distant galaxies. Interesting
objects for this study are found in strong gravitational lensing systems, where
the foreground galaxies generate multiple images.
Aims. The reddening law of lensing galaxies is investigated by studying the
colours of gravitationally-lensed quasars, and a handful of other quasars where
a foreground galaxy is detected.
Methods. We compare the observed colours of quasars reported in the
literature, with spectral templates reddened by different extinction laws and
dust properties. The data consists of 21 quasar-galaxy systems, with a total of
48 images. The galaxies, which are both early- and late-type, have redshifts in
the interval z=0.04-1.51.
Results. We measure a difference in rest-frame B-V between the quasar images
we study, and quasars without resolved foreground galaxies. This difference in
colour is indicative of significant dust extinction in the intervening galaxy.
Good fits to standard extinction laws were found for 22 of the images,
corresponding to 13 different galaxies. Our fits imply a wide range of possible
values for the total-to-selective extinction ratio, Rv. The distribution was
found to be broad with a weighted mode of Rv=2.4 and a FWHM of 2.7 (sigma =
1.1). Thus the bulk of the galaxies for which good reddening fits could be
derived, have dust properties compatible with the Milky Way value (Rv=3.1).
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:38:05 GMT"
},
{
"version": "v2",
"created": "Fri, 2 May 2008 08:12:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ostman",
"Linda",
""
],
[
"Goobar",
"Ariel",
""
],
[
"Mortsell",
"Edvard",
""
]
] | [
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] |
711.4268 | Dan Roozemond | Arjeh M. Cohen, Gabor Ivanyos, Dan A. Roozemond | Simple Lie Algebras having Extremal Elements | 11 pages | null | 10.1016/S0019-3577(09)00003-2 | null | math.RA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let L be a simple finite-dimensional Lie algebra of characteristic distinct
from 2 and from 3. Suppose that L contains an extremal element that is not a
sandwich, that is, an element x such that [x, [x, L]] is equal to the linear
span of x in L. In this paper we prove that, with a single exception, L is
generated by extremal elements. The result is known, at least for most
characteristics, but the proofs in the literature are involved. The current
proof closes a gap in a geometric proof that every simple Lie algebra
containing no sandwiches (that is, ad-nilpotent elements of order 2) is in fact
of classical type.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:43:21 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 08:23:46 GMT"
},
{
"version": "v3",
"created": "Wed, 17 Dec 2008 09:30:33 GMT"
}
] | 2011-06-17T00:00:00 | [
[
"Cohen",
"Arjeh M.",
""
],
[
"Ivanyos",
"Gabor",
""
],
[
"Roozemond",
"Dan A.",
""
]
] | [
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] |
711.4269 | Smarajit Karmakar | Pinaki Chaudhuri, Smarajit Karmakar and Chandan Dasgupta | Signatures of Dynamical Heterogeneity in the Structure of Glassy
Free-energy Minima | 5 pages, 5 figures | Phys. Rev. Lett. 100, 125701 (2008) | 10.1103/PhysRevLett.100.125701 | null | cond-mat.stat-mech cond-mat.soft | null | From numerical minimization of a model free energy functional for a system of
hard spheres, we show that the width of the local peaks of the time-averaged
density field at a glassy free-energy minimum exhibits large spatial variation,
similar to that of the ``local Debye-Waller factor'' in simulations of
dynamical heterogeneity. Molecular dynamics simulations starting from a
particle configuration generated from the density distribution at a glassy
free-energy minimum show similar spatial heterogeneity in the degree of
localization, implying a direct connection between dynamical heterogeneity and
the structure of glassy free energy minima.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:53:34 GMT"
}
] | 2008-12-23T00:00:00 | [
[
"Chaudhuri",
"Pinaki",
""
],
[
"Karmakar",
"Smarajit",
""
],
[
"Dasgupta",
"Chandan",
""
]
] | [
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] |
711.427 | Davide Sarchi | D. Sarchi, I. Carusotto, M. Wouters and V. Savona | Dynamics of coherent polaritons in double-well systems | null | null | null | null | cond-mat.other | null | We investigate the physics of coherent polaritons in a double-well
configuration under a resonant pumping. For a continuous wave pump, bistability
and self-pulsing regimes are identified as a function of the pump energy and
intensity. The response to an additional probe pulse is characterized in the
different cases and related to the Bogoliubov modes around the stationary
state. Under a pulsed pump, a crossover from Josephson-like oscillations to
self-trapping is predicted for increasing pump intensity. The accurateness of
the effective two-mode model is assessed by comparing its predictions to a full
solution of the non-equilibrium Gross-Pitaevskii equation.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:55:00 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Sarchi",
"D.",
""
],
[
"Carusotto",
"I.",
""
],
[
"Wouters",
"M.",
""
],
[
"Savona",
"V.",
""
]
] | [
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] |
711.4271 | Okan Ozer Dr | R. Koc, O. Ozer, H. Tutunculer, R. G. Yildirim | Solution of spin-boson systems in one and two-dimensional geometry via
the asymptotic iteration method | 13 pages, 5 figures. Please check "http://www1.gantep.edu.tr/~ozer/"
for other studies of Nuclear Physics Group at University of Gaziantep | Eur. Phys. J. B 59, 375-383 (2007) | 10.1140/epjb/e2007-00294-0 | null | quant-ph | null | We consider solutions of the $2\times 2$ matrix Hamiltonian of physical
systems within the context of the asymptotic iteration method. Our technique is
based on transformation of the associated Hamiltonian in the form of the first
order coupled differential equations. We construct a general matrix Hamiltonian
which includes a wide class of physical models. The systematic study presented
here reproduces a number of earlier results in a natural way as well as leading
to new findings. Possible generalizations of the method are also suggested.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 14:57:38 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 06:01:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Koc",
"R.",
""
],
[
"Ozer",
"O.",
""
],
[
"Tutunculer",
"H.",
""
],
[
"Yildirim",
"R. G.",
""
]
] | [
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0.0127845705,
-0.0142528266,
-0.0071562557,
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] |
711.4272 | Gustavo Moreno A. | C. D. Fosco, G. A. Moreno | Casimir effect in 2+1 dimensional noncommutative theories | 12 pages, 3 figures | Phys.Lett.B659:901-905,2008 | 10.1016/j.physletb.2007.12.015 | null | hep-th | null | We study the Dirichlet Casimir effect for a complex scalar field on two
noncommutative spatial coordinates plus a commutative time. To that end, we
introduce Dirichlet-like boundary conditions on a curve contained in the
spatial plane, in such a way that the correct commutative limit can be reached.
We evaluate the resulting Casimir energy for two different curves: (a) Two
parallel lines separated by a distance $L$, and (b) a circle of radius $R$. In
the first case, the resulting Casimir energy agrees exactly with the one
corresponding to the commutative case, regardless of the values of $L$ and of
the noncommutativity scale $\theta$, while for the latter the commutative
behaviour is only recovered when $R >> \sqrt{\theta}$. Outside of that regime,
the dependence of the energy with $R$ is substantially changed due to
noncommutative corrections, becoming regular for $R \to 0$.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:03:00 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Fosco",
"C. D.",
""
],
[
"Moreno",
"G. A.",
""
]
] | [
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711.4273 | Jacob Sonnenschein | Victoria Mazo and Jacob Sonnenschein | Non critical holographic models of the thermal phases of QCD | 11 figure minor corrections | JHEP0806:091,2008 | 10.1088/1126-6708/2008/06/091 | null | hep-th | null | We analyze the thermal phases of a non critical holographic model of QCD. The
model is based on a six dimensional background of $N_c$ non extremal D4 branes
wrapping a spacial circle of radius $R$ and the compactified Euclidean time
direction of radius $\beta=1/T$. We place in this background stacks of $N_f$ D4
and anti-D4 flavor probe branes with a separation distance $L$ at large radial
direction. %The dual theory is a 4+1 dimensional $SU(N_c)$ gauge theory
%compactified on a radius $R$ with anti-periodic boundary conditions for the
fermions. The analysis of the DBI effective action yields the following phase
diagram: At low temperature the system is in a confining phase with broken
chiral symmetry. In the high temperature deconfining phase chiral symmetry can
be either restored for $L>L_c=1.06 R$ or broken for $L<L_c$. All of these phase
transitions are of first order. We analyze the spectrum of the low-spin and
high-spin mesons. High spin mesons above certain critical angular momentum
``melt''. We detect (no) drag for (mesons) quarks moving in hot quark-gluon
fluid. The results resemble the structure and properties of the thermal
Sakai-Sugimoto model derived in hep-th/0604161.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:07:23 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 14:37:39 GMT"
},
{
"version": "v3",
"created": "Wed, 16 Jan 2008 14:34:52 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mazo",
"Victoria",
""
],
[
"Sonnenschein",
"Jacob",
""
]
] | [
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] |
711.4274 | Egor Muljarov | E. A. Muljarov, R. Zimmermann | Exciton dephasing in quantum dots: Coupling to LO phonons via excited
states | OECS10 contribution paper | phys. stat. sol. (b) 245, 1106 (2008) | 10.1002/pssb.200777613 | null | cond-mat.mes-hall | null | We have found a novel mechanism of spectral broadening and dephasing in
quantum dots (QDs) due to the coupling to longitudinal-optical (LO) phonons. In
theory, this mechanism comes into play only if the complete manifold of exciton
levels (including those in the wetting-layer continuum) is taken into account.
We demonstrate this nontrivial dephasing in different types of QDs, using the
exactly solvable quadratic coupling model, here generalized to an arbitrary
number of excitonic states.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:09:10 GMT"
}
] | 2012-05-16T00:00:00 | [
[
"Muljarov",
"E. A.",
""
],
[
"Zimmermann",
"R.",
""
]
] | [
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] |
711.4275 | J. Scott Berg | Robert B. Palmer, J. Scott Berg, Richard C. Fernow, Juan Carlos
Gallardo, Harold G. Kirk, Yuri Alexahin, David Neuffer, Stephen Alan Kahn,
Don Summers | A Complete Scheme of Ionization Cooling for a Muon Collider | 3 pages, 6 figures | Conf.Proc.C070625:3193,2007 | 10.2172/921988 | BNL-78088-2007-CP | physics.acc-ph | null | A complete scheme for production and cooling a muon beam for three specified
muon colliders is presented. Parameters for these muon colliders are given. The
scheme starts with the front end of a proposed neutrino factory that yields
bunch trains of both muon signs. Emittance exchange cooling in slow helical
lattices reduces the longitudinal emittance until it becomes possible to merge
the trains into single bunches, one of each sign. Further cooling in all
dimensions is applied to the single bunches in further slow helical lattices.
Final transverse cooling to the required parameters is achieved in 50 T
solenoids using high Tc superconductor at 4 K. Preliminary simulations of each
element are presented.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:34:49 GMT"
}
] | 2011-03-18T00:00:00 | [
[
"Palmer",
"Robert B.",
""
],
[
"Berg",
"J. Scott",
""
],
[
"Fernow",
"Richard C.",
""
],
[
"Gallardo",
"Juan Carlos",
""
],
[
"Kirk",
"Harold G.",
""
],
[
"Alexahin",
"Yuri",
""
],
[
"Neuffer",
"David",
""
],
[
"Kahn",
"Stephen Alan",
""
],
[
"Summers",
"Don",
""
]
] | [
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] |
711.4276 | George E. A. Matsas | George E. A. Matsas, Vicente Pleitez, Alberto Saa, Daniel A. T.
Vanzella | The number of dimensional fundamental constants | 7 pages, 2 figures, v2: Only changes in authors affiliations | null | null | null | physics.class-ph gr-qc hep-th physics.gen-ph | null | We revisit, qualify, and objectively resolve the seemingly controversial
question about what is the number of dimensional fundamental constants in
Nature. For this purpose, we only assume that all we can directly measure are
space and time intervals, and that this is enough to evaluate any physical
observable. We conclude that the number of dimensional fundamental constants is
two. We emphasize that this is an objective result rather than a "philosophical
opinion", and we let it clear how it could be refuted in order to prove us
wrong. Our conclusion coincides with Veneziano's string-theoretical one but our
arguments are not based on any particular theory. As a result, this implies
that one of the three usually considered fundamental constants "G", "c" or "h"
can be eliminated and we show explicitly how this can be accomplished.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:13:37 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 20:09:29 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Matsas",
"George E. A.",
""
],
[
"Pleitez",
"Vicente",
""
],
[
"Saa",
"Alberto",
""
],
[
"Vanzella",
"Daniel A. T.",
""
]
] | [
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] |
711.4277 | Bjoern Trauzettel | A. Komnik, B. Trauzettel, U. Weiss | Statistics of charge transfer through impurities in strongly correlated
1D metals | 11 pages, review article | Ann. Phys. (Leipzig) 16, 661 (2007) | 10.1002/andp.200710258 | null | cond-mat.mes-hall cond-mat.str-el | null | We review recent advances in the field of full counting statistics (FCS) of
charge transfer through impurities imbedded into strongly correlated
one-dimensional metallic systems, modelled by Tomonaga-Luttinger liquids
(TLLs). We concentrate on the exact analytic solutions for the cumulant
generating function (CGF), which became available recently and apply these
methods in order to obtain the FCS of a non-trivial contact between two crossed
TLL.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:15:58 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Komnik",
"A.",
""
],
[
"Trauzettel",
"B.",
""
],
[
"Weiss",
"U.",
""
]
] | [
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] |
711.4278 | David J. Thompson | D. J. Thompson | Gamma-Ray Pulsar Studies with GLAST | 8 pages, 5 figures. To appear in the proceedings of "40 Years of
Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007,
McGill University, Montreal, Canada | AIP Conf.Proc.983:56-63,2008 | 10.1063/1.2900301 | null | astro-ph | null | Some pulsars have their maximum observable energy output in the gamma-ray
band, offering the possibility of using these high-energy photons as probes of
the particle acceleration and interaction processes in pulsar magnetospheres.
After an extended hiatus between satellite missions, the recently-launched
AGILE mission and the upcoming Gamma-ray Large Area Space Telescope (GLAST)
Large Area Telescope (LAT) will allow gamma-ray tests of the theoretical models
developed based on past discoveries. With its greatly improved sensitivity,
better angular resolution, and larger energy reach than older instruments,
GLAST LAT should detect dozens to hundreds of new gamma-ray pulsars and measure
luminosities, light curves, and phase-resolved spectra with unprecedented
resolution. It will also have the potential to find radio-quiet pulsars like
Geminga, using blind search techniques. Cooperation with radio and X-ray pulsar
astronomers is an important aspect of the LAT team's planning for pulsar
studies.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:16:08 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Thompson",
"D. J.",
""
]
] | [
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] |
711.4279 | Patrizia Michetti | J. Franz, F.A. Gianturco, K.L. Baluja, J. Tennyson, R. Carey, R.
Montuoro, R.R. Lucchese, T. Stoecklin | Correlation-Polarization Effects in Electron/Positron Scattering from
Acetylene: A Comparison of Computational Models | null | null | 10.1016/j.nimb.2007.12.019 | null | physics.chem-ph | null | Different computational methods are employed to evaluate elastic
(rotationally summed) integral and differential cross sections for low energy
(below about 10 eV) positron scattering off gas-phase C$_2$H$_2$ molecules. The
computations are carried out at the static and static-plus-polarization levels
for describing the interaction forces and the correlation-polarization
contributions are found to be an essential component for the correct
description of low-energy cross section behavior. The local model potentials
derived from density functional theory (DFT) and from the distributed positron
model (DPM) are found to produce very high-quality agreement with existing
measurements. On the other hand, the less satisfactory agreement between the
R-matrix (RM) results and measured data shows the effects of the slow
convergence rate of configuration-interaction (CI) expansion methods with
respect to the size of the CI-expansion. To contrast the positron scattering
findings, results for electron-C$_2$H$_2$ integral and differential cross
sections, calculated with both a DFT model potential and the R-matrix method,
are compared and analysed around the shape resonance energy region and found to
produce better internal agreement.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:21:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Franz",
"J.",
""
],
[
"Gianturco",
"F. A.",
""
],
[
"Baluja",
"K. L.",
""
],
[
"Tennyson",
"J.",
""
],
[
"Carey",
"R.",
""
],
[
"Montuoro",
"R.",
""
],
[
"Lucchese",
"R. R.",
""
],
[
"Stoecklin",
"T.",
""
]
] | [
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] |
711.428 | Saverio Pascazio | Paolo Facchi, Giuseppe Marmo and Saverio Pascazio | Quantum Zeno dynamics and quantum Zeno subspaces | 20 pages, 9 figures. Dedicated to George Sudarshan on the occasion of
his 75th birthday. Review of the quantum Zeno dynamics in its three different
formulations. Proposal of a novel experiment in Section 10 | J.Phys.Conf.Ser.196:012017,2009 | 10.1088/1742-6596/196/1/012017 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A quantum Zeno dynamics can be obtained by means of frequent measurements,
frequent unitary kicks or a strong continuous coupling and yields a partition
of the total Hilbert space into quantum Zeno subspaces, among which any
transition is hindered. We focus on the "continuous" version of the quantum
Zeno effect and look at several interesting examples. We first analyze these
examples in practical terms, towards applications, then propose a novel
experiment.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:22:20 GMT"
},
{
"version": "v2",
"created": "Fri, 20 Mar 2009 09:45:01 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Facchi",
"Paolo",
""
],
[
"Marmo",
"Giuseppe",
""
],
[
"Pascazio",
"Saverio",
""
]
] | [
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711.4281 | Yvonne C. Pachmayer | HADES Collaboration: G. Agakishiev, C. Agodi, H. Alvarez Pol, A.
Balanda, R. Bassini, G. Bellia, D. Belver, A. Belyaev, A. Blanco, M. Boehmer,
A. Bortolotti, J. L. Boyard, P. Braun-Munzinger, P. Cabanelas, E. Castro, T.
Christ, M. Destefanis, J. Diaz, F. Dohrmann, A. Dybczak, T. Eberl, L.
Fabbietti, P. Finocchiaro, P. Fonte, J. Friese, I. Froehlich, T. Galatyuk, J.
A. Garzon, R. Gernhaeuser, A. Gil, C. Gilardi, M. Golubeva, D. Gonzalez Diaz,
E. Grosse, F. Guber, M. Heilmann, T. Hennino, R. Holzmann, A. Ierusalimov, I.
Iori, A. Ivashkin, M. Jurkovic, B. Kaempfer, K. Kanaki, T. Karavicheva, D.
Kirschner, I. Koenig, W. Koenig, B. W. Kolb, R. Kotte, A. Kozuch, A. Krasa,
F. Krizek, R. Kruecken, W. Kuehn, A. Kugler, A. Kurepin, J. Lamas Valverde,
S. Lang, J. S. Lange, K. Lapidus, L. Lopes, L. Maier, A. Mangiarotti, J.
Marin, J. Markert, V. Metag, B. Michalska, D. Mishra, E. Moriniere, J. Mousa,
M. Muench, C. Muentz, L. Naumann, R. Novotny, J. Otwinowski, Y. C. Pachmayer,
M. Palka, Y. Parpottas, V. Pechenov, O. Pechenova, T. Perez, J. Pietraszko,
R. Pleskac, W. Przygoda, B. Ramstein, A. Reshetin, M. Roy Stephan, A.
Rustamov, A. Sadovsky, B. Sailer, P. Salabura, A. Schmah, R. Simon, Y.
Sobolev, S. Spataro, B. Spruck, H. Stroebele, J. Stroth, C. Sturm, M. Sudol,
A. Tarantola, K. Teilab, P. Tlusty, A. Toia, M. Traxler, R. Trebacz, H.
Tsertos, I. Veretenkin, V. Wagner, M. Weber, H. Wen, M. Wisniowski, T.
Wojcik, J. Wuestenfeld, S. Yurevich, Y. Zanevsky, P. Zhou, P. Zumbruch | Study of dielectron production in C+C collisions at 1 AGeV | submitted to Physics Letters B | Phys.Lett.B663:43-48,2008 | 10.1016/j.physletb.2008.03.062 | null | nucl-ex | null | The emission of e+e- pairs from C+C collisions at an incident energy of 1 GeV
per nucleon has been investigated. The measured production probabilities,
spanning from the pi0-Dalitz to the rho/omega! invariant-mass region, display a
strong excess above the cocktail of standard hadronic sources. The
bombarding-energy dependence of this excess is found to scale like pion
production, rather than like eta production. The data are in good agreement
with results obtained in the former DLS experiment.
| [
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711.4282 | Wieslaw Laskowski | P. Badziag, C. Brukner, W. Laskowski, T. Paterek, M. Zukowski | Experimentally friendly geometrical criteria for entanglement | 4 pages, journal version | Phys. Rev. Lett. 100, 140403 (2008) | 10.1103/PhysRevLett.100.140403 | null | quant-ph | null | We present an intuitive geometrical entanglement criterion. It allows
formulation of simple and experimentally friendly sufficient conditions for
entanglement. The conditions are illustrated with several examples. Moreover, a
generalization of our approach is a necessary and sufficient separability
condition. It can be associated with a family of entanglement identifiers,
which is strictly richer than the family of entanglement witnesses.
| [
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"created": "Tue, 27 Nov 2007 18:51:55 GMT"
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{
"version": "v2",
"created": "Tue, 29 Apr 2008 16:01:43 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Badziag",
"P.",
""
],
[
"Brukner",
"C.",
""
],
[
"Laskowski",
"W.",
""
],
[
"Paterek",
"T.",
""
],
[
"Zukowski",
"M.",
""
]
] | [
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711.4283 | Dmitry Matyushov V | Vitaliy Kapko, Dmitry V. Matyushov, and C. Austen Angell | Thermodynamics and Dynamics of a Monoatomic Glass-Former. Constant
Pressure and Constant Volume Behavior | 14 pages, 14 figures | null | 10.1063/1.2883693 | null | cond-mat.soft cond-mat.stat-mech | null | We report constant-volume and constant-pressure simulations of the
thermodynamic and dynamic properties of the low-temperature liquid and
crystalline phases of the modified Stillinger-Weber (mSW) model. We have found
an approximately linear increase of the effective Gaussian width of the
distribution of inherent structures. This effect comes from non-Gaussianity of
the landscape and is consistent with the predictions of the Gaussian
excitations model representing the thermodynamics of the configurational
manifold as an ensemble of excitations, each carrying an excitation entropy.
The mSW model provides us with both the configurational and excess entropies,
with the difference mostly attributed to vibrational anharmonicity. We
therefore can address the distinction between the excess thermodynamic
quantities often used in the Adam-Gibbs (AG) equation. We find a new break in
the slope of the constant pressure AG plot when the excess entropy is used in
the AG equation. The simulation diffusivity data are equally well fitted by
applying a new equation, derived within the Gaussian excitations model, that
emphasizes enthalpy over entropy as the thermodynamic control variable for
transport in viscous liquids.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:36:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kapko",
"Vitaliy",
""
],
[
"Matyushov",
"Dmitry V.",
""
],
[
"Angell",
"C. Austen",
""
]
] | [
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] |
711.4284 | Ruth Britto | Ruth Britto, Bo Feng | Integral Coefficients for One-Loop Amplitudes | 32 pages, 1 figure | JHEP0802:095,2008 | 10.1088/1126-6708/2008/02/095 | ITFA-2007-53 | hep-ph hep-th | null | We present a set of algebraic functions for evaluating the coefficients of
the scalar integral basis of a general one-loop amplitude. The functions are
derived from unitarity cuts, but the complete cut-integral procedure has been
carried out in generality so that it never needs to be repeated. Where the
master integrals are known explicitly, the results here can be used as a black
box with tree-level amplitudes as input and one-loop amplitudes as output.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:27:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Britto",
"Ruth",
""
],
[
"Feng",
"Bo",
""
]
] | [
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-0.0829803497,
0.0133734057,
-0.0166613068,
-0.082719408,
-0.0026844665,
-0.029982524,
0.0058255862,
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] |
711.4285 | Roman Khymyn S | B. A. Ivanov, A. Yu. Galkin, R. S. Khymyn, A. Yu. Merkulov | Non-linear dynamics and two-dimensional solitons for spin $ S=1$
ferromagnets with biquadratic exchange | 11 pages, 7 figures, MikTEX | null | 10.1103/PhysRevB.77.064402 | null | cond-mat.other | null | We develop a consistent semiclassical theory of spin dynamics for an
isotropic ferromagnet with a spin $ S=1$ taking into consideration both
bilinear and biquadratic over spin operators exchange interaction. For such
non-Heisenberg magnets, a peculiar class of spin oscillations and waves, for
which the quantum spin expectation value $ {\rm {\bf m}}=<{\rm {\bf S}}>$ does
not change it direction, but changes in length, is presented. Such
``longitudinal'' excitations do not exist in regular magnets, dynamics of which
are described in terms of the Landau-Lifshitz equation or by means of the spin
Heisenberg Hamiltonian. We demonstrate the presence of non-linear uniform
oscillations and waves, as well as self-localized dynamical excitations
(solitons) with finite energy. A possibility of excitation of such oscillations
by ultrafast laser pulse is discussed.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:41:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ivanov",
"B. A.",
""
],
[
"Galkin",
"A. Yu.",
""
],
[
"Khymyn",
"R. S.",
""
],
[
"Merkulov",
"A. Yu.",
""
]
] | [
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711.4286 | Jaros{\l}aw Miszczak | D. Markham, J.A. Miszczak, Z. Puchala, K. Zyczkowski | Quantum state discrimination: a geometric approach | 12 pages, 2 figures | Phys. Rev. A 77, 042111 (2008) | 10.1103/PhysRevA.77.042111 | null | quant-ph | null | We analyse the problem of finding sets of quantum states that can be
deterministically discriminated. From a geometric point of view this problem is
equivalent to that of embedding a simplex of points whose distances are maximal
with respect to the Bures distance (or trace distance). We derive upper and
lower bounds for the trace distance and for the fidelity between two quantum
states, which imply bounds for the Bures distance between the unitary orbits of
both states. We thus show that when analysing minimal and maximal distances
between states of fixed spectra it is sufficient to consider diagonal states
only. Hence considering optimal discrimination, given freedom up to unitary
orbits, it is sufficient to consider diagonal states. This is illustrated
geometrically in terms of Weyl chambers.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:41:26 GMT"
}
] | 2008-06-09T00:00:00 | [
[
"Markham",
"D.",
""
],
[
"Miszczak",
"J. A.",
""
],
[
"Puchala",
"Z.",
""
],
[
"Zyczkowski",
"K.",
""
]
] | [
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] |
711.4287 | George Lusztig | G. Lusztig | Unipotent classes and special Weyl group representations | 31 pages | null | null | null | math.RT | null | We show that various invariants of a unipotent conjugacy class in a connected
semisimple group can be recovered purely in terms of data involving the Weyl
group.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:49:18 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Lusztig",
"G.",
""
]
] | [
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] |
711.4288 | Pedro Pina Avelino | P. P. Avelino, L.M.G. be\c{c}a, C.J.A.P. Martins | Linear and non-Linear Instabilities in Unified Dark Energy Models | 6 pages, accepted for publication in Physical Review D | Phys. Rev. D77:063515,2008 | 10.1103/PhysRevD.77.063515 | null | astro-ph | null | We revisit the paradigm of unified dark energy discussing in detail the
averaging problem in this type of scenarios, highlighting the need for a full
non-linear treatment. We also address the question of if and how models with
one or several dark fluids can be observationally distinguished. Simpler and
physically clearer derivations of some key results, most notably on the
relation between the generalized Chaplygin gas and the standard ($\Lambda$CDM)
`concordance' model and on a Jeans-type small-scale instability of some coupled
dark energy/dark matter models are presented.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:10:55 GMT"
},
{
"version": "v2",
"created": "Fri, 1 Feb 2008 15:47:44 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Avelino",
"P. P.",
""
],
[
"beça",
"L. M. G.",
""
],
[
"Martins",
"C. J. A. P.",
""
]
] | [
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711.4289 | Martha Evonuk | M. Evonuk | The role of density stratification in generating zonal flow structures
in a rotating fluid | 15 pages, 5 figures, accepted to ApJ | null | 10.1086/524938 | null | astro-ph | null | Local generation of vorticity occurs in rotating density-stratified fluids as
fluid parcels move radially, expanding or contracting with respect to the
background density stratification. Thermal convection in rotating 2D equatorial
simulations demonstrates this mechanism. The convergence of the vorticity into
zonal flow structures as a function of radius depends on the shape of the
density profile, with the prograde jet forming in the region of the disk where
the greatest number of density scale heights occurs. The number of stable jets
that form in the fluid increases with decreasing Ekman number and decreases
with increasing thermal driving. This local form of vorticity generation via
the density stratification is likely to be of great importance in bodies that
are quickly rotating, highly turbulent, and have large density changes, such as
Jovian planets. However, it is likely to be of lesser importance in the
interiors of planets such as the Earth, which have smaller density
stratifications and are less turbulent.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:54:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Evonuk",
"M.",
""
]
] | [
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711.429 | Roland Hoffmann | Thomas DeGrand, Roland Hoffmann, Johannes Najjar | More about QCD on compact spaces | 9 pages, 8 figures, JHEP style | JHEP0801:032,2008 | 10.1088/1126-6708/2008/01/032 | null | hep-lat | null | We present some results about spontaneous breaking of global symmetries for
four-flavor, three color QCD on compact spaces with two short directions. When
the two short directions have equal length and identical boundary conditions,
there is a single transition. When the two short directions have boundary
conditions of opposite parity and are of roughly equal extent, the C-breaking
and deconfinement transitions separate. When the two short dimensions are of
different length, the transitions are modified in qualitative agreement with
expectations from dimensional reduction. These features resemble the situation
in pure gauge simulations at small and large number of colors.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 15:58:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"DeGrand",
"Thomas",
""
],
[
"Hoffmann",
"Roland",
""
],
[
"Najjar",
"Johannes",
""
]
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] |
711.4291 | Artur Avila | Artur Avila and David Damanik | Absolute Continuity of the Integrated Density of States for the Almost
Mathieu Operator with Non-Critical Coupling | 13 pages, to appear in Inv. Math | Invent. Math. 172 (2008), 439-453 | 10.1007/s00222-007-0105-7 | null | math.DS math-ph math.MP math.SP | null | We show that the integrated density of states of the almost Mathieu operator
is absolutely continuous if and only if the coupling is non-critical. We deduce
for subcritical coupling that the spectrum is purely absolutely continuous for
almost every phase, settling the measure-theoretical case of Problem 6 of Barry
Simon's list of Schr\"odinger operator problems for the twenty-first century.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:08:40 GMT"
}
] | 2015-02-24T00:00:00 | [
[
"Avila",
"Artur",
""
],
[
"Damanik",
"David",
""
]
] | [
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] |
711.4292 | Christophe Le Poncin-Lafitte | Christophe Le Poncin-Lafitte and Pierre Teyssandier | Influence of mass multipole moments on the deflection of a light ray by
an isolated axisymmetric body | 9 pages. Submitted to Physical Review D | Phys.Rev.D77:044029,2008; Erratum-ibid.D77:069901,2008 | 10.1103/PhysRevD.77.044029 10.1103/PhysRevD.77.069901 | null | astro-ph gr-qc | null | Future space astrometry missions are planned to measure positions and/or
parallaxes of celestial objects with an accuracy of the order of the
microarcsecond. At such a level of accuracy, it will be indispensable to take
into account the influence of the mass multipole structure of the giant planets
on the bending of light rays. Within the parametrized post-Newtonian formalism,
we present an algorithmic procedure enabling to determine explicitly this
influence on a light ray connecting two points located at a finite distance.
Then we specialize our formulae in the cases where 1) the light source is
located at space infinity, 2) both the light source and the observer are
located at space infinity. We examine in detail the cases where the unperturbed
ray is in the equatorial plane or in a meridian plane.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:18:27 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Poncin-Lafitte",
"Christophe Le",
""
],
[
"Teyssandier",
"Pierre",
""
]
] | [
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711.4293 | Sarika Jalan | Fatihcan Atay, Sarika Jalan, J\"urgen Jost | Randomness, chaos, and structure | null | Complexity, 15 (1) pp. 29-35 (2009) | null | null | nlin.CD | null | We show how a simple scheme of symbolic dynamics distinguishes a chaotic from
a random time series and how it can be used to detect structural relationships
in coupled dynamics. This is relevant for the question at which scale in
complex dynamics regularities and patterns emerge.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:25:27 GMT"
}
] | 2009-10-26T00:00:00 | [
[
"Atay",
"Fatihcan",
""
],
[
"Jalan",
"Sarika",
""
],
[
"Jost",
"Jürgen",
""
]
] | [
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] |
711.4294 | Ivan Dmitriev | I.A. Dmitriev and R.A. Suris | Quantum dot cascade laser: Arguments in favor | 4 pages, 2 figures; Proceedings of MSS13 to be published in Physica E | null | 10.1016/j.physe.2007.09.055 | null | cond-mat.other | null | Quantum cascade lasers are recognized as propitious candidates for future
terahertz optoelectronics. Here we demonstrate several definite advantages of
quantum dot cascade structures over quantum well devices, which suffer
fundamental performance limitations owing to continuous carrier spectrum. The
discrete spectrum of quantum dots opens an opportunity to control the
non-radiative relaxation and optical loss and also provides for more
flexibility in the choice of an optical and electrical design of the laser.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:34:41 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Dmitriev",
"I. A.",
""
],
[
"Suris",
"R. A.",
""
]
] | [
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] |
711.4295 | Junegone Chay | Junegone Chay | Transverse-momentum-dependent parton distribution function in
soft-collinear effective theory | 25 pages, 6 figures, added references | null | null | MIT-CTP 3904 | hep-ph | null | Transverse-momentum-dependent parton distribution functions are analyzed in
semi-inclusive deep inelastic scattering at low transverse momentum using
soft-collinear effective theory. The transverse-momentum-dependent parton
distribution functions are defined on the lightcone without distorting the
lightcone path nor adding additional soft Wilson lines. In this approach, the
comparison between the integrated and unintegrated parton distribution
functions becomes transparent. The procedure of computing radiative corrections
in dimensional regularization is explained in detail, and the divergence, which
is a product of infrared and ultraviolet divergence, is cancelled. The
renormalization group equation for the transverse-momentum-dependent parton
distribution functions is derived. It depends only on the relevant physical
quantities and exhibits a nontrivial scaling behavior because the longitudinal
momentum fraction and the transverse momentum are coupled in the
renormalization group equation.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:30:02 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 19:30:48 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Chay",
"Junegone",
""
]
] | [
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] |
711.4296 | L\'aszl\'o Demk\'o | L. Demk\'o, I. K\'ezsm\'arki, G. Mih\'aly, N. Takeshita, Y. Tomioka,
Y. Tokura | Multicritical end-point of the first-order ferromagnetic transition in
colossal magnetoresistive manganites | 4 pages, 4 figures | null | 10.1103/PhysRevLett.101.037206 | null | cond-mat.str-el | null | We have studied the bandwidth-temperature-magnetic field phase diagram of
RE(0.55)Sr(0.45)MnO(3) colossal magnetoresistance manganites with ferromagnetic
metallic (FM) ground state. The bandwidth (or equivalently the double exchange
interaction) was controlled both via chemical substitution and hydrostatic
pressure with a focus on the vicinity of the critical pressure p* where the
character of the zero-field FM transition changes from first to second order.
Below p* the first-order FM transition extends up to a critical magnetic field,
H_cr. It is suppressed by pressure and approaches zero on the larger bandwidth
side where the surface of the first-order FM phase boundary is terminated by a
multicritical end-point (p*~32 kbar, T*~188 K, H*=0). The change in the
character of the transition and the decrease of the CMR effect is attributed to
the reduced CO/OO fluctuations.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:33:34 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 15:02:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Demkó",
"L.",
""
],
[
"Kézsmárki",
"I.",
""
],
[
"Mihály",
"G.",
""
],
[
"Takeshita",
"N.",
""
],
[
"Tomioka",
"Y.",
""
],
[
"Tokura",
"Y.",
""
]
] | [
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] |
711.4297 | Mairan Teodoro | A. Damineli (1), D. J. Hillier (2), M. F. Corcoran (3 and 4), O. Stahl
(5), J. H. Groh (1), J. Arias (8), M. Teodoro (1), N. Morrell (9), R. Gamen
(7), F. Gonzalez (7), N. V. Leister (1), H. Levato (7), R. S. Levenhagen (1),
M. Grosso (7), J. F. Albacete Colombo (6), G. Wallerstein (10) ((1) Instituto
de Astronomia, Geof\'isica e Ci\^encias Atmosf\'ericas, Universidade de S\~ao
Paulo, Brazil (2) Department of Physics and Astronomy, University of
Pittsburgh, USA (3) CRESST and X-ray Astrophysics Laboratory, NASA/GSFC, USA
(4) Universities Space Research Association, USA (5) ZAH, Landessternwarte,
Germany (6) Facultad de Ciencias Astronomicas y Geofisicas de La Plata
(FCAGLP) (7) Complejo Astronomico El Leoncito, Argentina (8) Departamento de
F\'isica, Universidad de La Serena, Chile (9) Las Campanas Observatory,
Carnegie Observatories, Chile (10) Department of Astronomy, University of
Washington, USA) | A multispectral view of the periodic events in eta Carinae | 16 pages, 7 EPS figures, accepted for publication on MNRAS | null | 10.1111/j.1365-2966.2008.13214.x | null | astro-ph | null | A full description of the 5.5-yr low excitation events in Eta Carinae is
presented. We show that they are not as simple and brief as previously thought,
but a combination of two components. The first, the 'slow variation' component,
is revealed by slow changes in the ionization level of circumstellar matter
across the whole cycle and is caused by gradual changes in the wind-wind
collision shock-cone orientation, angular opening and gaseous content. The
second, the 'collapse' component, is restricted to around the minimum, and is
due to a temporary global collapse of the wind-wind collision shock. High
energy photons (E > 16 eV) from the companion star are strongly shielded,
leaving the Weigelt objects at low ionization state for >6 months. High energy
phenomena are sensitive only to the 'collapse', low energy only to the 'slow
variation' and intermediate energies to both components. Simple eclipses and
mechanisms effective only near periastron (e.g., shell ejection or accretion
onto the secondary star) cannot account for the whole 5.5-yr cycle.
We find anti-correlated changes in the intensity and the radial velocity of P
Cygni absorption profiles in FeII 6455 and HeI 7065 lines, indicating that the
former is associated to the primary and the latter to the secondary star. We
present a set of light curves representative of the whole spectrum, useful for
monitoring the next event (2009 January 11).
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:33:48 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Mar 2008 15:09:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Damineli",
"A.",
"",
"3 and 4"
],
[
"Hillier",
"D. J.",
"",
"3 and 4"
],
[
"Corcoran",
"M. F.",
"",
"3 and 4"
],
[
"Stahl",
"O.",
""
],
[
"Groh",
"J. H.",
""
],
[
"Arias",
"J.",
""
],
[
"Teodoro",
"M.",
""
],
[
"Morrell",
"N.",
""
],
[
"Gamen",
"R.",
""
],
[
"Gonzalez",
"F.",
""
],
[
"Leister",
"N. V.",
""
],
[
"Levato",
"H.",
""
],
[
"Levenhagen",
"R. S.",
""
],
[
"Grosso",
"M.",
""
],
[
"Colombo",
"J. F. Albacete",
""
],
[
"Wallerstein",
"G.",
""
]
] | [
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] |
711.4298 | Svetoslav Ivanov | S. S. Ivanov, N. V. Vitanov | Steering quantum transitions between three crossing energy levels | 10 pages, 6 figures | null | 10.1103/PhysRevA.77.023406 | null | quant-ph | null | We calculate the propagator and the transition probabilities for a coherently
driven three-state quantum system. The energies of the three states change
linearly in time, whereas the interactions between them are pulse-shaped. We
derive a highly accurate analytic approximation by assuming independent
pairwise Landau-Zener transitions occurring instantly at the relevant avoided
crossings, and adiabatic evolution elsewhere. Quantum interferences are
identified, which occur due to different possible evolution paths in Hilbert
space between an initial and a final state. A detailed comparison with
numerical results for Gaussian-shaped pulses demonstrates a remarkable accuracy
of the analytic approximation. We use the analytic results to derive estimates
for the half-width of the excitation profile, and for the parameters required
for creation of a maximally coherent superposition of the three states. These
results are of potential interest in ladder climbing in alkali atoms by chirped
laser pulses, in quantum rotors, in transitions between Zeeman sublevels of a
J=1 level in a magnetic field, and in control of entanglement of a pair of
spin-1/2 particles. The results for the three-state system can be generalized,
without essential difficulties, to higher dimensions.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:34:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ivanov",
"S. S.",
""
],
[
"Vitanov",
"N. V.",
""
]
] | [
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] |
711.4299 | Avatar Tulsi | Avatar Tulsi | Quantum computers can search rapidly by using almost any selective
transformations | 8 pages, Accepted for publication in PRA | null | 10.1103/PhysRevA.78.022332 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The search problem is to find a state satisfying certain properties out of a
given set. Grover's algorithm drives a quantum computer from a prepared initial
state to the target state and solves the problem quadratically faster than a
classical computer. The algorithm uses selective transformations to distinguish
the initial state and target state from other states. It does not succeed
unless the selective transformations are very close to phase-inversions. Here
we show a way to go beyond this limitation. An important application lies in
quantum error-correction, where the errors can cause the selective
transformations to deviate from phase-inversions. The algorithms presented here
are robust to errors as long as the errors are reproducible and reversible.
This particular class of systematic errors arise often from imperfections in
apparatus setup. Hence our algorithms offer a significant flexibility in the
physical implementation of quantum search.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:39:39 GMT"
},
{
"version": "v2",
"created": "Thu, 12 Jun 2008 12:22:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tulsi",
"Avatar",
""
]
] | [
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] |
711.43 | Alexander Kamenshchik | Alexander A. Andrianov, Francesco Cannata, Alexander Y. Kamenshchik
and Daniele Regoli | Reconstruction of scalar potentials in two-field cosmological models | final version, to appear in JCAP | JCAP0802:015,2008 | 10.1088/1475-7516/2008/02/015 | null | gr-qc astro-ph hep-th | null | We study the procedure of the reconstruction of phantom-scalar field
potentials in two-field cosmological models. It is shown that while in the
one-field case the chosen cosmological evolution defines uniquely the form of
the scalar potential, in the two-field case one has an infinite number of
possibilities. The classification of a large class of possible potentials is
presented and the dependence of cosmological dynamics on the choice of initial
conditions is investigated qualitatively and numerically for two particular
models.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:42:15 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Feb 2008 17:59:43 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Andrianov",
"Alexander A.",
""
],
[
"Cannata",
"Francesco",
""
],
[
"Kamenshchik",
"Alexander Y.",
""
],
[
"Regoli",
"Daniele",
""
]
] | [
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] |
711.4301 | E.G. van Putten | E.G. van Putten, I.M. Vellekoop, and A.P. Mosk | Spatial amplitude and phase modulation using commercial twisted nematic
LCDs | 10 pages, 6 figures | null | 10.1364/AO.47.002076 | null | physics.optics | null | We present a method for full spatial phase and amplitude control of a laser
beam using a twisted nematic liquid crystal display combined with a spatial
filter. By spatial filtering we combine four neighboring pixels into one
superpixel. At each superpixel we are able to independently modulate the phase
and the amplitude of light. We demonstrate experimentally the independent phase
and amplitude modulation using this novel technique. Our technique does not
impose special requirements on the spatial light modulator and allows precise
control of fields even with imperfect modulators.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:44:01 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Feb 2008 16:23:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"van Putten",
"E. G.",
""
],
[
"Vellekoop",
"I. M.",
""
],
[
"Mosk",
"A. P.",
""
]
] | [
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] |
711.4302 | Sergey Neshveyev | Sergey Neshveyev, Lars Tuset | Notes on the Kazhdan-Lusztig theorem on equivalence of the Drinfeld
category and the category of Uq(g)-modules | 40 pages | null | null | null | math.QA math.OA | null | We discuss the proof of Kazhdan and Lusztig of the equivalence of the
Drinfeld category D(g,h) of g-modules and the category of finite dimensional
Uq(g)-modules, q=exp(\pi ih), for h\in C\Q*. Aiming at operator algebraists the
result is formulated as the existence for each h\in iR of a normalized unitary
2-cochain F on the dual \hat G of a compact simple Lie group G such that the
convolution algebra of G with the coproduct twisted by F is *-isomorphic to the
convolution algebra of the q-deformation G_q of G, while the coboundary of
F^{-1} coincides with Drinfeld's KZ-associator defined via monodromy of the
Knizhnik-Zamolodchikov equations.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 16:48:20 GMT"
}
] | 2007-11-28T00:00:00 | [
[
"Neshveyev",
"Sergey",
""
],
[
"Tuset",
"Lars",
""
]
] | [
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711.4303 | Hiroaki Sugiyama | Hiroaki Sugiyama | More on Non-standard Interaction at MINOS | Talk given at 9th International Workshop on Neutrino Factories,
Superbeams and Betabeams (NuFact07), Okayama, Japan, 6-11 Aug 2007 | AIPConf.Proc.981:216-218,2008 | 10.1063/1.2898938 | SISSA 88/2007/EP | hep-ph | null | We discuss about effects of the non-standard interaction of neutrinos with
matter on the nu_e appearance search in the MINOS experiment. We consider the
effects of the complex phase of the interaction and of the uncertainty on
theta_23 also. We show that the oscillation probability can be so large that
can not be explained by the ordinary oscillation. We show also how much
constraints on the non-standard effects can be improved if the experiment does
not observe nu_e appearance signal.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:09:44 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Sugiyama",
"Hiroaki",
""
]
] | [
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711.4304 | Thorsten Feldmann | M. Diehl (DESY Hamburg), Th. Feldmann (Univ. Siegen), P. Kroll (Univ.
Wuppertal) | Form factors and other measures of strangeness in the nucleon | (22 pages, 19 figures, minor corrections, matches journal version) | Phys.Rev.D77:033006,2008 | 10.1103/PhysRevD.77.033006 | DESY 07-209, SI-HEP-2007-18, WUB 07-11 | hep-ph | null | We discuss the phenomenology of strange-quark dynamics in the nucleon, based
on experimental and theoretical results for electroweak form factors and for
parton densities. In particular, we construct a model for the generalized
parton distribution that relates the asymmetry s(x)-sbar(x) between the
longitudinal momentum distributions of strange quarks and antiquarks with the
form factor F1^s(t), which describes the distribution of strangeness in
transverse position space.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:10:17 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Feb 2008 14:24:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Diehl",
"M.",
"",
"DESY Hamburg"
],
[
"Feldmann",
"Th.",
"",
"Univ. Siegen"
],
[
"Kroll",
"P.",
"",
"Univ.\n Wuppertal"
]
] | [
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] |
711.4305 | Karen Masters | Karen L. Masters (CfA), Christopher M. Springob (Washington
State/NRL), John P. Huchra (CfA) | 2MTF I. The Tully-Fisher Relation in the 2MASS J, H and K Bands | 13 pages, 5 figures. AJ, accepted (scheduled for June 2008). v2 is as
accepted by AJ and includes only minor textual changes from v1. v3 includes a
3 page erratum published as Masters et al. 2014. A coding error was
discovered and corrected, resulting in small changes in the slope and offsets
offsets of the TF relation. All qualitative results still hold. We apologise
for the inconvenience | null | 10.1088/0004-6256/135/5/1738 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The 2 Micron All-Sky Survey (2MASS) Tully-Fisher Survey (2MTF) aims to
measure Tully-Fisher (TF) distances to all bright inclined spirals in the 2MASS
Redshift Survey (2MRS). Essential to this project is a universal calibration of
the TF relation in the 2MASS J (1.2 um), H (1.6 um) and K (2.2 um) bands. We
present the first bias corrected or universal TF template in these bands. We
find that the slope of the TF relation becomes steeper as the wavelength
increases being close to L \propto v^4 in K-band and L \propto v^3.6 in J and
H-bands. We also investigate the dependence on galaxy morphology showing that
in all three bands the relation is steeper for later type spirals which also
have a dimmer TF zeropoint than earlier type spirals. We correct the final
relation to that for Sc galaxies. Finally we study the scatter from the TF
relation fitting for a width dependent intrinsic scatter which is not found to
vary significantly with wavelength.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:20:29 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Mar 2008 19:54:58 GMT"
},
{
"version": "v3",
"created": "Thu, 10 Apr 2014 19:59:57 GMT"
}
] | 2014-04-11T00:00:00 | [
[
"Masters",
"Karen L.",
"",
"CfA"
],
[
"Springob",
"Christopher M.",
"",
"Washington\n State/NRL"
],
[
"Huchra",
"John P.",
"",
"CfA"
]
] | [
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] |
711.4306 | Romain Danneau | R. Danneau, F. Wu, M.F. Craciun, S. Russo, M.Y. Tomi, J. Salmilehto,
A.F. Morpurgo, and P.J. Hakonen | Shot Noise in Ballistic Graphene | Phys. Rev. Lett. 100, 196802 (2008) | null | 10.1103/PhysRevLett.100.196802 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We have investigated shot noise in graphene field effect devices in the
temperature range of 4.2--30 K at low frequency ($f$ = 600--850 MHz). We find
that for our graphene samples with large width over length ratio $W/L$, the
Fano factor $\mathfrak{F}$ reaches a maximum $\mathfrak{F} \sim$ 1/3 at the
Dirac point and that it decreases strongly with increasing charge density. For
smaller $W/L$, the Fano factor at Dirac point is significantly lower. Our
results are in good agreement with the theory describing that transport at the
Dirac point in clean graphene arises from evanescent electronic states.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:42:32 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Jul 2008 19:21:08 GMT"
}
] | 2008-07-01T00:00:00 | [
[
"Danneau",
"R.",
""
],
[
"Wu",
"F.",
""
],
[
"Craciun",
"M. F.",
""
],
[
"Russo",
"S.",
""
],
[
"Tomi",
"M. Y.",
""
],
[
"Salmilehto",
"J.",
""
],
[
"Morpurgo",
"A. F.",
""
],
[
"Hakonen",
"P. J.",
""
]
] | [
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] |
711.4307 | Jerome Martin | Jerome Martin and Jun'ichi Yokoyama | Generation of Large-Scale Magnetic Fields in Single-Field Inflation | 33 pages, 5 figures | JCAP 0801:025,2008 | 10.1088/1475-7516/2008/01/025 | null | astro-ph gr-qc hep-ph hep-th | null | We consider the generation of large-scale magnetic fields in slow-roll
inflation. The inflaton field is described in a supergravity framework where
the conformal invariance of the electromagnetic field is generically and
naturally broken. For each class of inflationary scenarios, we determine the
functional dependence of the gauge coupling that is consistent with the
observations on the magnetic field strength at various astrophysical scales
and, at the same time, avoid a back-reaction problem. Then, we study whether
the required coupling functions can naturally emerge in well-motivated,
possibly string-inspired, models. We argue that this is non trivial and can be
realized only for a restricted class of scenarios. This includes power-law
inflation where the inflaton field is interpreted as a modulus. However, this
scenario seems to be consistent only if the energy scale of inflation is low
and the reheating stage prolonged. Another reasonable possibility appears to be
small field models since no back-reaction problem is present in this case but,
unfortunately, the corresponding scenario cannot be justified in a stringy
framework. Finally, large field models do not lead to sensible model building.
| [
{
"version": "v1",
"created": "Tue, 27 Nov 2007 17:22:35 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Martin",
"Jerome",
""
],
[
"Yokoyama",
"Jun'ichi",
""
]
] | [
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