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712.2279 | Kenny Easwaran | Kenny Easwaran | A Cheerful Introduction to Forcing and the Continuum Hypothesis | null | null | null | null | math.LO math.GM | null | This is an introduction to the set-theoretic method of forcing, including its
application in proving the independence of the Continuum Hypothesis from the
Zermelo-Fraenkel axioms of set theory. I presuppose no particular mathematical
background beyond some familiarity with set theory and mathematical logic - in
particular, no algebra is presupposed, though it can be useful. The goal is to
have a document that makes this material accessible to mathematics graduate
students in all fields, and to philosophers with an interest in set theory and
mathematical logic but no other mathematical background.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 03:37:42 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Easwaran",
"Kenny",
""
]
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712.228 | Raul Angulo | R. E. Angulo, C. M. Baugh, C. G. Lacey | The assembly bias of dark matter haloes to higher orders | 13 pages, 6 figures. Published version | 2008MNRAS.387..921A | 10.1111/j.1365-2966.2008.13304.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We use an extremely large volume ($2.4h^{-3}{\rm Gpc}^{3}$), high resolution
N-body simulation to measure the higher order clustering of dark matter haloes
as a function of mass and internal structure. As a result of the large
simulation volume and the use of a novel ``cross-moment'' counts-in-cells
technique which suppresses discreteness noise, we are able to measure the
clustering of haloes corresponding to rarer peaks than was possible in previous
studies; the rarest haloes for which we measure the variance are 100 times more
clustered than the dark matter. We are able to extract, for the first time,
halo bias parameters from linear up to fourth order. For all orders measured,
we find that the bias parameters are a strong function of mass for haloes more
massive than the characteristic mass $M_{*}$. Currently, no theoretical model
is able to reproduce this mass dependence closely. We find that the bias
parameters also depend on the internal structure of the halo up to fourth
order. For haloes more massive than $M_{*}$, we find that the more concentrated
haloes are more weakly clustered than the less concentrated ones. We see no
dependence of clustering on concentration for haloes with masses $M<M_{*}$;
this is contrary to the trend reported in the literature when segregating
haloes by their formation time. Our results are insensitive to whether haloes
are labelled by the total mass returned by the friends-of-friends group finder
or by the mass of the most massive substructure. This implies that our
conclusions are not an artefact of the particular choice of group finding
algorithm. Our results will provide important input to theoretical models of
galaxy clustering.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 20:56:49 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Dec 2007 21:02:30 GMT"
},
{
"version": "v3",
"created": "Thu, 31 Jul 2008 14:29:35 GMT"
}
] | 2008-07-31T00:00:00 | [
[
"Angulo",
"R. E.",
""
],
[
"Baugh",
"C. M.",
""
],
[
"Lacey",
"C. G.",
""
]
] | [
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712.2281 | Kei-Jiro Takahashi | Tetsuji Kimura, Mitsuhisa Ohta and Kei-Jiro Takahashi | Type IIA orientifolds and orbifolds on non-factorizable tori | 42 pages, 3 figures, v2: typos corrected, references added, version
to appear in Nucl. Phys. B | Nucl.Phys.B798:89-123,2008 | 10.1016/j.nuclphysb.2008.01.030 | KUNS-2100, YITP-07-82 | hep-th | null | We investigate Type II orientifolds on non-factorizable torus with and
without its oribifolding. We explicitly calculate the Ramond-Ramond tadpole
from string one-loop amplitudes, and confirm that the consistent number of
orientifold planes is directly derived from the Lefschetz fixed point theorem.
We furthermore classify orientifolds on non-factorizable Z_N x Z_M orbifolds,
and construct new supersymmetric Type IIA orientifold models on them.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 20:11:21 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Mar 2008 03:22:15 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kimura",
"Tetsuji",
""
],
[
"Ohta",
"Mitsuhisa",
""
],
[
"Takahashi",
"Kei-Jiro",
""
]
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] |
712.2282 | Albert Roura | Guillem Perez-Nadal, Albert Roura, Enric Verdaguer | Stability of de Sitter spacetime under isotropic perturbations in
semiclassical gravity | 19 pages, REVTeX4 | Phys.Rev.D77:124033,2008 | 10.1103/PhysRevD.77.124033 | LA-UR-07-7066 | gr-qc | null | A spatially flat Robertson-Walker spacetime driven by a cosmological constant
is non-conformally coupled to a massless scalar field. The equations of
semiclassical gravity are explicitly solved for this case, and a
self-consistent de Sitter solution associated with the Bunch-Davies vacuum
state is found (the effect of the quantum field is to shift slightly the
effective cosmological constant). Furthermore, it is shown that the corrected
de Sitter spacetime is stable under spatially-isotropic perturbations of the
metric and the quantum state. These results are independent of the free
renormalization parameters.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 05:14:45 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Perez-Nadal",
"Guillem",
""
],
[
"Roura",
"Albert",
""
],
[
"Verdaguer",
"Enric",
""
]
] | [
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] |
712.2283 | Bruno Julia Diaz | B. Julia-Diaz, T.-S. H. Lee, A. Matsuyama, T. Sato, L.C. Smith | Dynamical Coupled-Channels Effects on Pion Photoproduction | Corrected version. 14 pages, 10 figures | Phys.Rev.C77:045205,2008 | 10.1103/PhysRevC.77.045205 | null | nucl-th | null | The electromagnetic pion production reactions are investigated within the
dynamical coupled-channels model developed in {\bf Physics Reports, 439, 193
(2007)}. The meson-baryon channels included in this study are $\gamma N$, $\pi
N$, $\eta N$, and the $\pi\Delta$, $\rho N$ and $\sigma N$ resonant components
of the $\pi\pi N$ channel. With the hadronic parameters of the model determined
in a recent study of $\pi N$ scattering, we show that the pion photoproduction
data up to the second resonance region can be described to a very large extent
by only adjusting the bare $\gamma N \to N^*$ helicity amplitudes, while the
non-resonant electromagnetic couplings are taken from previous works. It is
found that the coupled-channels effects can contribute about 10 - 20 % of the
production cross sections in the $\Delta$ (1232) resonance region, and can
drastically change the magnitude and shape of the cross sections in the second
resonance region. The importance of the off-shell effects in a dynamical
approach is also demonstrated. The meson cloud effects as well as the
coupled-channels contributions to the $\gamma N \to N^*$ form factors are found
to be mainly in the low $Q^2$ region. For the magnetic M1 $\gamma N \to \Delta$
(1232) form factor, the results are close to that of the Sato-Lee Model.
Necessary improvements to the model and future developments are discussed.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 05:20:22 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 16:16:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Julia-Diaz",
"B.",
""
],
[
"Lee",
"T. -S. H.",
""
],
[
"Matsuyama",
"A.",
""
],
[
"Sato",
"T.",
""
],
[
"Smith",
"L. C.",
""
]
] | [
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] |
712.2284 | Andrzej Niedzielski | Andrzej Niedzielski and Aleksander Wolszczan | The PennState/Toru\'n Center for Astronomy Search for Planets around
Evolved Stars | 5 pages, to appear in ,,Extreme Solar Systems'', 2007 ASP Conference
Series, eds. Debra Fischer, Fred Rasio, Steve Thorsett and Alex Wolszczan | null | null | null | astro-ph | null | We present the motivation for and the first results from a large radial
velocity search for planets around red giants with the 9.2-m Hobby-Eberly
Telescope.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 05:28:38 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Niedzielski",
"Andrzej",
""
],
[
"Wolszczan",
"Aleksander",
""
]
] | [
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] |
712.2285 | Andrzej Niedzielski | Grzegorz Nowak and Andrzej Niedzielski | The PSU/TCfA Search for Planets Around Evolved Stars: Bisector Analysis
of Activity of a Sample of Red Giants | 2 pages, to appear in "Extreme Solar Systems", 2007 ASP Conference
Series, eds. Debra Fischer, Fred Rasio, Steve Thorsett and Alex Wolszczan | null | null | null | astro-ph | null | Searches for planets around evolved G-K subgiant and giant stars are
essential for developing general understanding of planet formation and
evolution of the planetary systems. Precise radial velocity (RV) measurements
of giants have lead to the discovery of ten planets around such star. However,
the long period radial velocity variations of red giants may also have other
than planetary nature. Non-radial oscillations or rotational modulation due to
starspots can also induce RV variations, thereby mimicking the gravitational
influence of low-mass companions. In this work we present bisector analysis of
five carefully selected lines for two stars from our survey.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 05:38:40 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Nowak",
"Grzegorz",
""
],
[
"Niedzielski",
"Andrzej",
""
]
] | [
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712.2286 | Andrzej Niedzielski | Grzegorz Nowak and Andrzej Niedzielski | The PSU/TCfA Search for Planets Around Evolved Stars: Vsin(i)
Measurements for Slow Rotating F-K Giants | 2 pages, to appear in "Extreme Solar Systems", 2007 ASP Conference
Series, eds. Debra Fischer, Fred Rasio, Steve Thorsett and Alex Wolszczan | null | null | null | astro-ph | null | We present results of our projected rotational velocities (Vsin(i))
measurements of F, G and K giants obtained from the cross-correlation function
(CCF) constructed from high signal to noise spectra. We also present the
calibration of the HET/HRS cross-correlation function to determine accurate
projected rotational velocities Vsin(i) for slowly-rotating F-K giants.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:45:21 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Nowak",
"Grzegorz",
""
],
[
"Niedzielski",
"Andrzej",
""
]
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712.2287 | Andrzej Niedzielski | Pawel Zielinski and Andrzej Niedzielski | The PennState/Toru\'n Center for Astronomy Search for Planets Around
Evolved Stars. Basic parameters of a sample of evolved stars | 2 pages, to appear in "Extreme Solar Systems", 2007 ASP Conference
Series, eds. Debra Fischer, Fred Rasio, Steve Thorsett and Alex Wolszczan | null | 10.1016/j.actao.2008.03.008 | null | astro-ph | null | The objective of the PSU/TCfA Search for Planets Around Evolved Stars is to
study evolution of planetary systems in the stellar evolution timescale. For
such an analysis precise physical parameters of the hosts of the planetary
systems are essential. In this paper we present an attempt to obtain basic
physical parameters for a sample of evolved stars observed within our survey
with the High Resolution Spectrograph of the Hobby-Eberly Telescope.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 05:56:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zielinski",
"Pawel",
""
],
[
"Niedzielski",
"Andrzej",
""
]
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712.2288 | Yu Shi | Yu Shi, Yue-Liang Wu | CP Measurement in Quantum Teleportation of Neutral Mesons | 7 pages | Eur.Phys.J.C55:477-482,2008 | 10.1140/epjc/s10052-008-0593-7 | null | hep-ph quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Quantum teleportation using neutral pseudoscalar mesons shows novel
connections between particle physics and quantum information. The projection
basis, which is crucial in the teleportation process, is determined by the
conservation laws of particle physics, and is different from the Bell basis, as
in the usual case. Here we show that one can verify the teleportation process
by CP measurement. This method significantly simplifies the high energy quantum
teleportation protocol. Especially, it is rigorous, and is independent of
whether CP is violated in weak decays. This method can also be applied to
general verification of Einstein-Podolsky-Rosen correlations in particle
physics.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 06:20:49 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Jul 2008 08:33:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Shi",
"Yu",
""
],
[
"Wu",
"Yue-Liang",
""
]
] | [
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712.2289 | Mitsutoshi Fujita | Mitsutoshi Fujita | Non-equilibrium thermodynamics near the horizon and holography | 15 pages; v2, v3: typos (in eq. (32) etc.) corrected, v4:refs. added,
minor corrections, sections enlarged, v5, v6:explanation clarified | JHEP 0810:031,2008 | 10.1088/1126-6708/2008/10/031 | KUNS-2115 | hep-th gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Small perturbations of a black brane are interpreted as small deviations from
thermodynamic equilibrium in a dual theory with the AdS/CFT correspondence. In
this paper, we calculate hydrodynamics of the dual Yang-Mills theory in the
gravity side using membrane paradigm. This method is different from the usual
AdS/CFT correspondence and evaluate classical solutions not at boundaries but
at the place slightly away from a horizon. There are sound modes or shear modes
for gravity perturbation. For sound modes, such calculation at the horizon has
not yet been done. Then, we find that boundary stress tensor at the horizon
satisfies conservation law in flat space and can represent dissipative parts of
stress tensor in the dual theory by holography. Using them, we can read off
directly shear and bulk viscosity of the dual theory. Quasinormal modes are
solutions to linearized equations obeyed by classical fluctuations of a
gravitational background subject to specific boundary conditions and are also
gauge-invariant quantities. We use solutions for each fluctuation that compose
such quantities and show that quasinormal modes are consistent with the
membrane paradigm.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 06:34:15 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 05:34:01 GMT"
},
{
"version": "v3",
"created": "Sun, 23 Dec 2007 14:42:50 GMT"
},
{
"version": "v4",
"created": "Sun, 20 Jan 2008 10:52:45 GMT"
},
{
"version": "v5",
"created": "Sun, 30 Mar 2008 13:15:16 GMT"
},
{
"version": "v6",
"created": "Tue, 2 Sep 2008 13:33:47 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Fujita",
"Mitsutoshi",
""
]
] | [
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712.229 | Alex Degtyarev | Alex Degtyarev | Irreducible plane sextics with large fundamental groups | A revised version: a few proofs added/clarified | J. Math. Soc. Japan, 61:4 (2009), 1131--1169 | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We compute the fundamental group of the complement of each irreducible sextic
of weight eight or nine (in a sense, the largest groups for irreducible
sextics), as well as of 169 of their derivatives (both of and not of torus
type). We also give a detailed geometric description of sextics of weight eight
and nine and of their moduli spaces and compute their Alexander modules; the
latter are shown to be free over an appropriate ring.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 06:35:24 GMT"
},
{
"version": "v2",
"created": "Wed, 10 Sep 2008 10:53:52 GMT"
}
] | 2010-01-25T00:00:00 | [
[
"Degtyarev",
"Alex",
""
]
] | [
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712.2291 | Ikuo Ichinose | T.Ono, S.Doi, Y.Hori, I.Ichinose, and T.Matsui | Phase Structure and Critical Behavior of Multi-Higgs U(1) Lattice Gauge
Theory in Three Dimensions | Long version of arXiv:0704.1323, New results added | Annals of Physics 324(2009)2453 | null | null | hep-lat astro-ph cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the three-dimensional (3D) compact U(1) lattice gauge theory coupled
with $N$-flavor Higgs fields by means of the Monte Carlo simulations. This
model is relevant to multi-component superconductors, antiferromagnetic spin
systems in easy plane, inflational cosmology, etc. It is known that there is no
phase transition in the N=1 model. For N=2, we found that the system has a
second-order phase transition line $\tilde{c}_1(c_2)$ in the $c_2$(gauge
coupling)$-c_1$(Higgs coupling) plane, which separates the confinement phase
and the Higgs phase. Numerical results suggest that the phase transition
belongs to the universality class of the 3D XY model as the previous works by
Babaev et al. and Smiseth et al. suggested. For N=3, we found that there exists
a critical line similar to that in the N=2 model, but the critical line is
separated into two parts; one for $c_2 < c_{2{\rm tc}}=2.4\pm 0.1$ with
first-order transitions, and the other for $ c_{2{\rm tc}} < c_2$ with
second-order transitions, indicating the existence of a tricritical point. We
verified that similar phase diagram appears for the N=4 and N=5 systems. We
also studied the case of anistropic Higgs coupling in the N=3 model and found
that there appear two second-order phase transitions or a single second-order
transition and a crossover depending on the values of the anisotropic Higgs
couplings. This result indicates that an "enhancement" of phase transition
occurs when multiple phase transitions coincide at a certain point in the
parameter space.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:58:06 GMT"
},
{
"version": "v2",
"created": "Wed, 29 Apr 2009 06:28:42 GMT"
}
] | 2009-10-26T00:00:00 | [
[
"Ono",
"T.",
""
],
[
"Doi",
"S.",
""
],
[
"Hori",
"Y.",
""
],
[
"Ichinose",
"I.",
""
],
[
"Matsui",
"T.",
""
]
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712.2292 | Tsung-Wen Yeh | Tsung-Wen Yeh | QCD factorization at twist-3: the two parton contributions | 67 pages, 7 figures, typos corrected, six references added; | null | null | null | hep-ph | null | In this paper, the twist-3 two parton corrections in charmless $B\to PP$
decays are shown to be factorizable under the QCD factorization approach. The
factorizability of the twist-3 two parton corrections is constructed on the
following findings. Under the energetic meson limit, the pseudoscalar
distribution amplitude for a light pseudoscalar meson is allowed to be
non-constant by the equations of motion for the quark. The non-constant
pseudoscalar distribution amplitude is then used to regularize the end-point
divergences in the hard spectator corrections at twist-3 order. By retaining
the momentum fraction variable of the spectator quark of the $B$ meson in the
propagators, the end-point divergence in the weak annihilation corrections at
twist-3 order is resolved. The factorization of the $O(\alpha_s)$ corrections
under the two parton approximation is shown valid up-to $O(1/m_b)$ . The hard
scattering kernels of order $O(\alpha_s)$ and $O(\Lambda_{QCD}/m_b)$ are
explicitly given and found to be infrared finite. The results are applied for
making predictions for the branching ratios of $B\to \pi K $ decays.
| [
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"created": "Fri, 14 Dec 2007 06:42:15 GMT"
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"created": "Thu, 3 Jan 2008 08:24:35 GMT"
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{
"version": "v3",
"created": "Thu, 6 Mar 2008 12:28:27 GMT"
}
] | 2008-03-06T00:00:00 | [
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] |
712.2293 | Kazufumi Kimoto | Kazufumi Kimoto | Representation theory of the $\alpha$-determinant and zonal spherical
functions | 9 pages | null | null | null | math.RT | null | We prove that the multiplicity of each irreducible component in the
$\mathcal{U}(\mathfrak{gl}_n)$-cyclic module generated by the $l$-th power
$\det^{(\alpha)}(X)^l$ of the $\alpha$-determinant is given by the rank of a
matrix whose entries are given by a variation of the spherical Fourier
transformation for $(\mathfrak{S}_{nl},\mathfrak{S}_l^n)$. Further, we
calculate the matrix explicitly when $n=2$. This gives not only another proof
of the result by Kimoto-Matsumoto-Wakayama (2007) but also a new aspect of the
representation theory of the $\alpha$-determinants.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 06:48:53 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Kimoto",
"Kazufumi",
""
]
] | [
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] |
712.2294 | Amaya Moro-Martin | Amaya Moro-Martin | On the Solar System-Debris Disk Connecction | 8 pages, Exoplanets: Detection, Formation and Dynamics Proceedings
IAU Symposium No. 249 2008 | null | 10.1017/S1743921308016803 | null | astro-ph | null | This paper emphasizes the connection between solar and extra-solar debris
disks: how models and observations of the Solar System are helping us
understand the debris disk phenomenon, and vice versa, how debris disks are
helping us place our Solar System into context.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 06:49:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Moro-Martin",
"Amaya",
""
]
] | [
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] |
712.2295 | Wei Huang | Wei Huang, Zhaohui Wei | Efficient One-way Quantum Computations for Quantum Error Correction | null | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show how to explicitly construct an $O(nd)$ size and constant quantum
depth circuit which encodes any given $n$-qubit stabilizer code with $d$
generators. Our construction is derived using the graphic description for
stabilizer codes and the one-way quantum computation model. Our result
demonstrates how to use cluster states as scalable resources for many
multi-qubit entangled states and how to use the one-way quantum computation
model to improve design of quantum algorithms.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:12:17 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Aug 2008 18:53:25 GMT"
}
] | 2008-08-18T00:00:00 | [
[
"Huang",
"Wei",
""
],
[
"Wei",
"Zhaohui",
""
]
] | [
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] |
712.2296 | Toshiaki Shoji | Toshiaki Shoji | Lusztig's conjecture for finite classical groups with even
characteristic | 30 pages | null | null | null | math.RT | null | The determination of scalars involved in Lusztig's conjecture for finite
reductive groups $G(F_q)$ was achieved by Waldspurger in the case of symplectic
groups or orthogonal groups, under the condition that $p,q$ are large enough.
Here $p$ is the characteristic of the finite field $F_q$. In this paper, we
determine the scalars in the case of symplectic groups with $p = 2$, by
applying the theory of symmetric spaces over a finite field due to Kawanaka and
Lusztig. We also obtain a partial result in the case of special orthogonal
groups with $p = 2$.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:13:31 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Shoji",
"Toshiaki",
""
]
] | [
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712.2297 | Andrzej Niedzielski | Andrzej Niedzielski, Alex Wolszczan | A HET search for planets around evolved stars | 6 pages, to appear in ,,Exoplanets. Detection, Formation & Dynamics''
IAU Symposium 249, Cambridge University Press, 2007 | null | 10.1017/S1743921308016347 | null | astro-ph | null | We present our ongoing survey of ~1000 GK-giants with the 9.2-m Hobby-Eberly
Telescope in search for planets around evolved stars. The stars selected for
this survey are brighter than 11 mag and are located in the section of the
HR-diagram, which is approximately delimited by the main sequence, the
instability strip, and the coronal dividing line. We use the High Resolution
Spectrograph to obtain stellar spectra for radial velocity measurements with a
4-6 m/s precision. So far, the survey has discovered a planetary-mass companion
to the K0-giant HD 17092, and it has produced a number of plausible planet
candidates around other stars. Together with other similar efforts, our program
provides information on planet formation around intermediate mass main
sequence-progenitors and it will create the experimental basis with which to
study dynamics of planetary systems around evolving stars.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:24:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Niedzielski",
"Andrzej",
""
],
[
"Wolszczan",
"Alex",
""
]
] | [
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712.2298 | Andrzej Niedzielski | Andrzej Niedzielski, Grzegorz Nowak and Pawel Zielinski | The PSU/TCfA Search for Planets around Evolved Stars. Stellar parameters
and activity indicators of targets | 5 pages, to appear in ,,Exoplanets. Detection, Formation & Dynamics''
IAU Symposium 249, Cambridge University Press, 2007 | null | 10.1017/S1743921308016359 | null | astro-ph | null | The main objective of the Penn State/Torun Centre for Astronomy Search for
Planets around Evolved Stars is the detection of planetary systems around
massive, evolved stars. We are also interested in the evolution of these
systems on stellar evolution timescales. In this paper we present our approach
to determine the basic physical parameters of our targets GK-giants. We also
discuss the stellar activity indicators used in our survey: line bisector and
curvature, and Halpha variability.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:32:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Niedzielski",
"Andrzej",
""
],
[
"Nowak",
"Grzegorz",
""
],
[
"Zielinski",
"Pawel",
""
]
] | [
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] |
712.2299 | Dave Witte Morris | Dave Witte Morris | What is a superrigid subgroup? | 18 pages, 7 figures | null | null | null | math.HO math.MG | null | This is an expository paper. It is well known that a linear transformation
can be defined to have any desired action on a basis. From this fact, one can
show that every group homomorphism from Z^k to R^d extends to a homomorphism
from R^k to R^d, and we will see other examples of discrete subgroups H of
connected groups G, such that the homomorphisms defined on $H$ can ("almost")
be extended to homomorphisms defined on all of G. This is related to a very
classical topic in geometry, the study of linkages.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:39:03 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Morris",
"Dave Witte",
""
]
] | [
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712.23 | P. F. Chen | D. H. Gao, P. F. Chen, M. D. Ding, and X. D. Li | Simulations of the periodic flaring rate on YY Gem | 9 pages, 9 figures, accepted by MNRAS | null | 10.1111/j.1365-2966.2007.12830.x | null | astro-ph | null | The binary YY Gem shows many interesting properties, one of which is the
periodicity in its flaring rate. The period, which is about $48 \pm 3$ min, was
ever interpreted in terms of the oscillation of a filament. In this paper, we
propose a new model to explain this phenomenon by means of 2.5-dimensional MHD
numerical simulations. It is found that magnetic reconnection is induced as the
coronal loops rooted on both stars inflate and approach each other, which is
driven by the differential stellar rotation. The magnetic reconnection is
modulated by fast-mode magnetoacoustic waves which are trapped between the
surfaces of the two stars, so that the reconnection rate presents a periodic
behaviour. With the typical parameters for the binary system, the observed
period can be reproduced. We also derive an empirical formula to relate the
period of the flaring rate to the coronal temperature and density, as well as
the magnetic field.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 07:51:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gao",
"D. H.",
""
],
[
"Chen",
"P. F.",
""
],
[
"Ding",
"M. D.",
""
],
[
"Li",
"X. D.",
""
]
] | [
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712.2301 | Ho Seong Hwang | Ho Seong Hwang (Seoul National Univ, Korea Institute for Advanced
Study), Myung Gyoon Lee (Seoul National Univ.) | Galaxy Orbits for Galaxy Clusters in Sloan Digital Sky Survey and 2dF
Galaxy Redshift Survey | 59 pages, 21 figures. To appear in ApJ. Paper with high resolution
figures are available at http://astro.kias.re.kr/~hshwang/papers/orbit.pdf | Astrophys.J.676:218-247,2008 | 10.1086/528733 | null | astro-ph | null | We present the results of a study for galaxy orbits in galaxy clusters using
a spectroscopic sample of galaxies in Sloan Digital Sky Survey (SDSS) and 2dF
Galaxy Redshift Survey (2dFGRS). We have determined the member galaxies of
Abell clusters covered by these surveys using the galaxies' redshift and
positional data. We have selected 10 clusters using three criteria: the number
of member galaxies is greater than or equal to 40, the spatial coverage is
complete, and X-ray mass profile is available in the literature. We derive the
radial profile of the galaxy number density and velocity dispersion using all,
early-type, and late-type galaxies for each cluster. We have investigated the
galaxy orbits for our sample clusters with constant and variable velocity
anisotropies over the clustercentric distance using Jeans equation. Using all
member galaxies, the galaxy orbits are found to be isotropic within the
uncertainty for most of sample clusters, although it is difficult to conclude
strongly for some clusters due the large errors and the variation as a function
of the clustercentric distance in the calculated velocity anisotropies. We
investigated the orbital difference between early-type and late-type galaxies
for four sample clusters, and found no significant difference between them.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 08:11:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hwang",
"Ho Seong",
"",
"Seoul National Univ, Korea Institute for Advanced\n Study"
],
[
"Lee",
"Myung Gyoon",
"",
"Seoul National Univ."
]
] | [
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] |
712.2302 | Georg Hager | Georg Hager, Thomas Zeiser, Gerhard Wellein | Data access optimizations for highly threaded multi-core CPUs with
multiple memory controllers | 12 pages, 7 figures. Accepted for Workshop on Large-Scale Parallel
Processing 2008. Revised and extended version | null | null | null | cs.DC cs.PF | null | Processor and system architectures that feature multiple memory controllers
are prone to show bottlenecks and erratic performance numbers on codes with
regular access patterns. Although such effects are well known in the form of
cache thrashing and aliasing conflicts, they become more severe when memory
access is involved. Using the new Sun UltraSPARC T2 processor as a prototypical
multi-core design, we analyze performance patterns in low-level and application
benchmarks and show ways to circumvent bottlenecks by careful data layout and
padding.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 08:14:20 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Jan 2008 16:18:50 GMT"
}
] | 2008-01-28T00:00:00 | [
[
"Hager",
"Georg",
""
],
[
"Zeiser",
"Thomas",
""
],
[
"Wellein",
"Gerhard",
""
]
] | [
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712.2303 | Attila Popping | Attila Popping and Robert Braun | The Standing Wave Phenomenon in Radio Telescopes; Frequency Modulation
of the WSRT Primary Beam | 12 pages, 11 figures, Accepted for publication in A&A, figures
compressed to low resolution; high-resolution version available at:
http://www.astro.rug.nl/~popping/wsrtbeam.pdf | null | 10.1051/0004-6361:20079122 | null | astro-ph | null | Inadequacies in the knowledge of the primary beam response of current
interferometric arrays often form a limitation to the image fidelity. We hope
to overcome these limitations by constructing a frequency-resolved,
full-polarization empirical model for the primary beam of the Westerbork
Synthesis Radio Telescope (WSRT). Holographic observations, sampling angular
scales between about 5 arcmin and 11 degrees, were obtained of a bright compact
source (3C147). These permitted measurement of voltage response patterns for
seven of the fourteen telescopes in the array and allowed calculation of the
mean cross-correlated power beam. Good sampling of the main-lobe, near-in, and
far-side-lobes out to a radius of more than 5 degrees was obtained. A robust
empirical beam model was detemined in all polarization products and at
frequencies between 1322 and 1457 MHz with 1 MHz resolution. Substantial
departures from axi-symmetry are apparent in the main-lobe as well as
systematic differences between the polarization properties. Surprisingly, many
beam properties are modulated at the 5 to 10% level with changing frequency.
These include: (1) the main beam area, (2) the side-lobe to main-lobe power
ratio, and (3) the effective telescope aperture. These semi-sinusoidsal
modulations have a basic period of about 17 MHz, consistent with the natural
'standing wave' period of a 8.75 m focal distance. The deduced frequency
modulations of the beam pattern were verified in an independent long duration
observation using compact continuum sources at very large off-axis distances.
Application of our frequency-resolved beam model should enable higher dynamic
range and improved image fidelity for interferometric observations in complex
fields. (abridged)
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:24:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Popping",
"Attila",
""
],
[
"Braun",
"Robert",
""
]
] | [
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] |
712.2304 | Damien Roy | Damien Roy | On simultaneous rational approximations to a real number, its square,
and its cube | 12 pages | Acta Arithmetica, vol.133 (2008), 185-197 | 10.4064/aa133-2-6 | null | math.NT | null | We provide an upper bound on the uniform exponent of approximation to a
triple (xi, xi^2, xi^3) by rational numbers with the same denominator, valid
for any transcendental real number xi. This upper bound refines a previous
result of Davenport and Schmidt. As a consequence, we get a sharper lower bound
on the exponent of approximation of such a number xi by algebraic integers of
degree at most 4.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 18:42:26 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 19:47:41 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Roy",
"Damien",
""
]
] | [
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] |
712.2305 | Eugene Kamenetskii | M. Sigalov, E.O. Kamenetskii, and R. Shavit | Electric self inductance of quasi-2D magnetic-dipolar-mode ferrite disks | null | J. Appl. Phys. 104, 053901 (2008) | 10.1063/1.2973676 | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | An electric current flowing around a loop produces a magnetic field and hence
a magnetic flux through the loop. The ratio of the magnetic flux to the
electric current is called the (magnetic) self inductance. Can there be a dual
situation with a magnetic current flowing around a loop and producing an
electric field and hence an electric flux through the loop? Following the
classical electrodynamics laws an answer to this question should be negative.
Nevertheless special spectral properties of magnetic dipolar modes in a
quasi-2D ferrite disk show there are the double-valued-function loop magnetic
currents which may produce eigen electric fields and hence eigen electric
fluxes through the loop. In this case one can definitely introduce the notion
of the electric self inductance as the ratio of the electric flux to the
magnetic current. In this paper we show experimentally that in the
magnetic-dipolar-mode ferrite disks there exist eigen electric fluxes. These
fluxes are very sensitive to permittivity parameters of materials abutting to
the ferrite disk. Dielectric samples above a ferrite disk with a higher
permittivity than air confine the electric field closely outside the ferrite,
thereby changing the loop magnetic currents and thus transforming the
magnetic-dipolar-mode oscillating spectrum.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 08:56:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sigalov",
"M.",
""
],
[
"Kamenetskii",
"E. O.",
""
],
[
"Shavit",
"R.",
""
]
] | [
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] |
712.2306 | Phuong Mai Dinh | J. Messud, P. M. Dinh, P.-G. Reinhard, and E. Suraud | Time-dependent density-functional theory with self-interaction
correction | 4 pages, 1 figure | Phys. Rev. Lett. 101 (2008) 096404 | 10.1103/PhysRevLett.101.096404 | null | cond-mat.other | null | We discuss an extension of time-dependent density-functional theory by a
self-interaction correction (SIC). A strictly variational formulation is given
taking care of the necessary constraints. A manageable and transparent
propagation scheme using two sets of wavefunctions is proposed and applied to
laser excitation with subsequent ionization of a dimer molecule.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:05:26 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Apr 2008 10:01:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Messud",
"J.",
""
],
[
"Dinh",
"P. M.",
""
],
[
"Reinhard",
"P. -G.",
""
],
[
"Suraud",
"E.",
""
]
] | [
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] |
712.2307 | Valerio Scarani | Valerio Scarani (CQT Singapore) | On the local and non-local content of bipartite qubit and qutrit
correlations | Accepted version. Previous title "The Elitzur-Popescu-Rohrlich
approach to quantum non-locality" changed for editorial reasons | Phys. Rev. A 77, 042112 (2008) | 10.1103/PhysRevA.77.042112 | null | quant-ph | null | The local and non-local contents of non-local probability distributions are
studied using the approach of Elitzur, Popescu and Rohrlich [Phys. Lett. A
\textbf{162}, 25 (1992)]. This work focuses on distributions that can be
obtained by single-copy von Neumann measurements on bipartite quantum systems.
For pure two-qubit states Psi(theta)=cos(theta)|00>+sin(theta)|11>, with
cos(theta)>=sin(theta), the local content of the corresponding probability
distribution is found to lie between 1-sin(2*theta) and cos(2*theta). For the
family Psi(gamma)= (|00>+|11>+gamma*|22>)/sqrt(2+gamma^2) of two-qutrit states,
non-zero local content is found for gamma>2.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:11:30 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 03:30:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Scarani",
"Valerio",
"",
"CQT Singapore"
]
] | [
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] |
712.2308 | Xinxian Zheng | J\"urgen Herzog, Marius Vladoiu and Xinxian Zheng | How to compute the Stanley depth of a monomial ideal | null | null | null | null | math.AC | null | Let $J\subset I$ be monomial ideals. We show that the Stanley depth of $I/J$
can be computed in a finite number of steps. We also introduce the $\fdepth$ of
a monomial ideal which is defined in terms of prime filtrations and show that
it can also be computed in a finite number of steps. In both cases it is shown
that these invariants can be determined by considering partitions of suitable
finite posets into intervals.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:11:39 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Herzog",
"Jürgen",
""
],
[
"Vladoiu",
"Marius",
""
],
[
"Zheng",
"Xinxian",
""
]
] | [
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] |
712.2309 | Shrisha Rao | Jeremiah Barr, Shrisha Rao | The $n$-Queens Problem in Higher Dimensions | null | Elemente der Mathematik 61 (4), 2006, pp. 133--137 | null | null | math.CO | null | A well-known chessboard problem is that of placing eight queens on the
chessboard so that no two queens are able to attack each other. (Recall that a
queen can attack anything on the same row, column, or diagonal as itself.) This
problem is known to have been studied by Gauss, and can be generalized to an (n
\times n) board, where (n \geq 4). We consider this problem in $d$-dimensional
chess spaces, where (d \geq 3), and obtain the result that in higher
dimensions, $n$ queens do not always suffice (in any arrangement) to attack all
board positions. Our methods allow us to obtain the first lower bound on the
number of queens that are necessary to attack all positions in a
$d$-dimensional chess space of size $n$, and further to show that for any $k$,
there are higher-dimensional chess spaces in which not all positions can be
attacked by (n^k) queens.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:17:04 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Barr",
"Jeremiah",
""
],
[
"Rao",
"Shrisha",
""
]
] | [
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] |
712.231 | Thomas Oikonomou | Thomas Oikonomou | From Boltzmann-Gibbs ensemble to generalized ensembles | This paper has been withdrawn by the author | null | null | null | cond-mat.stat-mech | null | We reconsider the Boltzmann-Gibbs statistical ensemble in thermodynamics
using the multinomial coefficient approach. We show that an ensemble is defined
by the determination of four statistical quantities, the element probabilities
$p_i$, the configuration probabilities $P_j$, the entropy $S$ and the extremum
constraints (EC). This distinction is of central importance for the
understanding of the conditions under which a microcanonical, canonical and
macrocanonical ensemble is defined. These three ensembles are characterized by
the conservation of their sizes. A variation of the ensemble size creates
difficulties in the definitions of the quadruplet $\{p_i, P_j, S, \mt{EC}\}$,
giving rise for a generalization of the Boltzmann-Gibbs formalism, such one as
introduced by Tsallis. We demonstrate that generalized thermodynamics represent
a transformation of ordinary thermodynamics in such a way that the energy of
the system remains conserved.
From our results it becomes evident that Tsallis's formalism is a very
specific generalization, however, not the only one. We also revisit the
Jaynes's Maximum Entropy Principle, showing that in general it can lead to
incorrect results and consider the appropriate corrections.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:18:24 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Jan 2008 10:42:36 GMT"
},
{
"version": "v3",
"created": "Sat, 27 Aug 2011 11:54:56 GMT"
}
] | 2011-08-30T00:00:00 | [
[
"Oikonomou",
"Thomas",
""
]
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712.2311 | Christoph Bohle | C. Bohle, K. Leschke, F. Pedit, U. Pinkall | Conformal maps from a 2-torus to the 4-sphere | 27 pages, 5 figures | J. Reine Angew. Math. 671 (2012), 1-30 | 10.1515/CRELLE.2011.156 | null | math.DG | null | We study the space of conformal immersions of a 2-torus into the 4-sphere.
The moduli space of generalized Darboux transforms of such an immersed torus
has the structure of a Riemann surface, the spectral curve. This Riemann
surface arises as the zero locus of the determinant of a holomorphic family of
Dirac type operators parameterized over the complexified dual torus. The kernel
line bundle of this family over the spectral curve describes the generalized
Darboux transforms of the conformally immersed torus. If the spectral curve has
finite genus the kernel bundle can be extended to the compactification of the
spectral curve and we obtain a linear 2-torus worth of algebraic curves in
projective 3-space. The original conformal immersion of the 2-torus is
recovered as the orbit under this family of the point at infinity on the
spectral curve projected to the 4-sphere via the twistor fibration.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:46:54 GMT"
}
] | 2012-12-21T00:00:00 | [
[
"Bohle",
"C.",
""
],
[
"Leschke",
"K.",
""
],
[
"Pedit",
"F.",
""
],
[
"Pinkall",
"U.",
""
]
] | [
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] |
712.2312 | Roberto Lineros | T. Delahaye (1), R. Lineros (2), F. Donato (2), N. Fornengo (2), P.
Salati (1) ((1) LAPTH/Annecy, CNRS-SPM and Universite' de Savoie 9, (2)
University of Torino and INFN/Torino) | Positrons from dark matter annihilation in the galactic halo:
theoretical uncertainties | 22 pages, 15 figures. A few comments and references added | Phys.Rev.D77:063527,2008 | 10.1103/PhysRevD.77.063527 | DFTT 7/2007, LAPTH-1187/07 | astro-ph hep-ph | null | Indirect detection signals from dark matter annihilation are studied in the
positron channel. We discuss in detail the positron propagation inside the
galactic medium: we present novel solutions of the diffusion and propagation
equations and we focus on the determination of the astrophysical uncertainties
which affect the positron dark matter signal. We find dark matter scenarios and
propagation models that nicely fit existing data on the positron fraction.
Finally, we present predictions both on the positron fraction and on the flux
for already running or planned space experiments, concluding that they have the
potential to discriminate a possible signal from the background and, in some
cases, to distinguish among different astrophysical propagation models.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:34:10 GMT"
},
{
"version": "v2",
"created": "Sat, 9 Feb 2008 16:35:42 GMT"
}
] | 2010-04-06T00:00:00 | [
[
"Delahaye",
"T.",
""
],
[
"Lineros",
"R.",
""
],
[
"Donato",
"F.",
""
],
[
"Fornengo",
"N.",
""
],
[
"Salati",
"P.",
""
]
] | [
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-0.0173977334,
0.0351273045,
-0.0645659789,
-0.008005565,
-0.1295111924,
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] |
712.2313 | Felix H\"ofling | Felix H\"ofling, Tobias Munk, Erwin Frey, and Thomas Franosch | Critical dynamics of ballistic and Brownian particles in a heterogeneous
environment | 14 pages | J. Chem. Phys. 128, 164517 (2008) | 10.1063/1.2901170 | LMU-ASC 77/07 | cond-mat.soft cond-mat.stat-mech | null | The dynamic properties of a classical tracer particle in a random, disordered
medium are investigated close to the localization transition. For Lorentz
models obeying Newtonian and diffusive motion at the microscale, we have
performed large-scale computer simulations, demonstrating that universality
holds at long times in the immediate vicinity of the transition. The scaling
function describing the crossover from anomalous transport to diffusive motion
is found to vary extremely slowly and spans at least 5 decades in time. To
extract the scaling function, one has to allow for the leading universal
corrections to scaling. Our findings suggest that apparent power laws with
varying exponents generically occur and dominate experimentally accessible time
windows as soon as the heterogeneities cover a decade in length scale. We
extract the divergent length scales, quantify the spatial heterogeneities in
terms of the non-Gaussian parameter, and corroborate our results by a thorough
finite-size analysis.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:58:23 GMT"
}
] | 2008-04-29T00:00:00 | [
[
"Höfling",
"Felix",
""
],
[
"Munk",
"Tobias",
""
],
[
"Frey",
"Erwin",
""
],
[
"Franosch",
"Thomas",
""
]
] | [
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] |
712.2314 | Erik Dujardin | Jean-Francois Dayen, Ather Mahmood, Dmitry S. Golubev, Isabelle
Roch-Jeune, Philippe Salles and Erik Dujardin | Side-gated transport in FIB-fabricated multilayered graphene nanoribbons | Revised version: more detailed description of control experiments. 5
pages, 4 figures, submitted to Small (Wiley-VCH). Added supporting
information (Figs S1 to S8) | Small, 2008, 4, 716-720 | 10.1002/smll.200700913 | null | cond-mat.mtrl-sci | null | In this Letter, we present the patterning, exfoliation and micromanipulation
of thin graphitic discs which are subsequently connected and patterned into
sub-100nm wide ribbons with a resist-free process using Focused Ion Beam (FIB)
lithography and deposition. The electronic transport properties of the double
side-gated nanoribbons are then investigated down to 40 K and interpreted with
a simple model of 1D array of tunnelling junctions.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:47:13 GMT"
},
{
"version": "v2",
"created": "Sat, 26 Jan 2008 23:47:07 GMT"
}
] | 2010-11-22T00:00:00 | [
[
"Dayen",
"Jean-Francois",
""
],
[
"Mahmood",
"Ather",
""
],
[
"Golubev",
"Dmitry S.",
""
],
[
"Roch-Jeune",
"Isabelle",
""
],
[
"Salles",
"Philippe",
""
],
[
"Dujardin",
"Erik",
""
]
] | [
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] |
712.2315 | Vadim Puller | Vadim I. Puller, Yigal Meir | Phase switching in a voltage-biased Aharonov-Bohm interferometer | 12 pages, 9 figures | null | 10.1103/PhysRevB.77.165421 | null | cond-mat.mes-hall | null | Recent experiment [Sigrist et al., Phys. Rev. Lett. {\bf 98}, 036805 (2007)]
reported switches between 0 and $\pi$ in the phase of Aharonov-Bohm
oscillations of the two-terminal differential conductance through a two-dot
ring with increasing voltage bias. Using a simple model, where one of the dots
contains multiple interacting levels, these findings are explained as a result
of transport through the interferometer being dominated at different biases by
quantum dot levels of different "parity" (i.e. the sign of the overlap integral
between the dot state and the states in the leads). The redistribution of
electron population between different levels with bias leads to the fact that
the number of switching events is not necessarily equal to the number of dot
levels, in agreement with experiment. For the same reason switching does not
always imply that the parity of levels is strictly alternating. Lastly, it is
demonstrated that the correlation between the first switching of the phase and
the onset of the inelastic cotunneling, as well as the sharp (rather than
gradual) change of phase when switching occurs, give reason to think that the
present interpretation of the experiment is preferable to the one based on
electrostatic AB effect.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 09:49:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Puller",
"Vadim I.",
""
],
[
"Meir",
"Yigal",
""
]
] | [
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] |
712.2316 | Hiroshi Itoyama | H.Itoyama and A.Morozov | Boundary Ring or a Way to Construct Approximate NG Solutions with
Polygon Boundary Conditions. II. Polygons which admit an inscribed circle | 45 pages | Prog.Theor.Phys.120:231-287,2008 | 10.1143/PTP.120.231 | OCU-PHYS 284, ITEP/TH-58/07 | hep-th | null | We further develop the formalism of arXiv:0712.0159 for approximate solution
of Nambu-Goto (NG) equations with polygon conditions in AdS backgrounds, needed
in modern studies of the string/gauge duality. Inscribed circle condition is
preserved, which leaves only one unknown function y_0(y_1,y_2) to solve for,
what considerably simplifies our presentation. The problem is to find a
delicate balance -- if not exact match -- between two different structures: NG
equation -- a non-linear deformation of Laplace equation with solutions
non-linearly deviating from holomorphic functions, -- and the boundary ring,
associated with polygons made from null segments in Minkovski space. We provide
more details about the theory of these structures and suggest an extended class
of functions to be used at the next stage of Alday-Maldacena program:
evaluation of regularized NG actions.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 10:15:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Itoyama",
"H.",
""
],
[
"Morozov",
"A.",
""
]
] | [
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] |
712.2317 | Laurent Duval | Caroline Chaux, Laurent Duval, Amel Benazza-Benyahia and
Jean-Christophe Pesquet | A nonlinear Stein based estimator for multichannel image denoising | null | null | 10.1109/TSP.2008.921757 | null | physics.data-an stat.AP | null | The use of multicomponent images has become widespread with the improvement
of multisensor systems having increased spatial and spectral resolutions.
However, the observed images are often corrupted by an additive Gaussian noise.
In this paper, we are interested in multichannel image denoising based on a
multiscale representation of the images. A multivariate statistical approach is
adopted to take into account both the spatial and the inter-component
correlations existing between the different wavelet subbands. More precisely,
we propose a new parametric nonlinear estimator which generalizes many reported
denoising methods. The derivation of the optimal parameters is achieved by
applying Stein's principle in the multivariate case. Experiments performed on
multispectral remote sensing images clearly indicate that our method
outperforms conventional wavelet denoising techniques
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 10:27:16 GMT"
}
] | 2023-01-19T00:00:00 | [
[
"Chaux",
"Caroline",
""
],
[
"Duval",
"Laurent",
""
],
[
"Benazza-Benyahia",
"Amel",
""
],
[
"Pesquet",
"Jean-Christophe",
""
]
] | [
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] |
712.2318 | Makoto Sakurai | Makoto Sakurai | Mixed anomalies of chiral algebras compactified to smooth
quasi-projective surfaces | Ph.D. dissertation at the University of Tokyo, 2007, v2. changed the
arXiv address of reference, v3. eliminated some typos and references, v4.
introduced AMS format of LaTeX, v5. cleaned signs, fonts, and formats with
polite calculations | null | null | UT-07-39 | hep-th math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Some time ago, the chiral algebra theory of Beilinson-Drinfeld was expected
to play a central role in the convergence of divergence in mathematical physics
of superstring theory for quantization of gauge theory and gravity. Naively,
this algebra plays an important role in a holomorphic conformal field theory
with a non-negative integer graded conformal dimension, whose target space does
not necessarily have the vanishing first Chern class. This algebra has two
definitions until now: one is that by Malikov-Schechtman-Vaintrob by gluing
affine patches, and the other is that of Kapranov-Vasserot by gluing the formal
loop spaces. I will use the new definition of Nekrasov by simplifying
Malikov-Schechtman-Vaintrob in order to compute the obstruction classes of
gerbes of chiral differential operators.
In this paper, I will examine the two independent Ans$\"{a}$tze (or working
hypotheses) of Witten's $\mathcal{N}=(0,2)$ heterotic strings and Nekrasov's
generalized complex geometry, after Hitchin and Gualtieri, are consistent in
the case of $\mathbb{CP}^2$, which has $3$ affine patches and is expected to
have the "first Pontryagin anomaly".
I also scrutinized the physical meanings of $2$ dimensional toric Fano
manifolds, or rather toric del Pezzo surfaces, obtained by blowing up the
non-colinear $1, 2, 3$ points of $\mathbb{CP}^2$. The obstruction classes of
gerbes of them coincide with the second Chern characters obtained by the
Riemann-Roch theorem and in particular vanishes for $1$ point blowup, which
means that one of the gravitational anomalies vanishes for a non-Calabi-Yau
manifold compactification.
The future direction towards the geometric Langlands program is also
discussed in the last section.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:45:58 GMT"
},
{
"version": "v2",
"created": "Sun, 16 Dec 2007 08:21:41 GMT"
},
{
"version": "v3",
"created": "Wed, 19 Sep 2012 00:31:55 GMT"
},
{
"version": "v4",
"created": "Thu, 13 Dec 2012 07:11:35 GMT"
},
{
"version": "v5",
"created": "Wed, 25 Feb 2015 04:49:50 GMT"
}
] | 2015-02-26T00:00:00 | [
[
"Sakurai",
"Makoto",
""
]
] | [
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] |
712.2319 | Jens Mueller | Jens Mueller, Steffen Wirth, Stephan von Molnar | Room-temperature magnetoresistance switching of Py thin films induced by
Fe-nanoparticles grown by STM-assisted CVD | null | null | null | null | cond-mat.other | null | Arrays of Fe-nanoparticles grown by STM-assited CVD have been placed on top
of a narrow stripe of Py. The magnetic coupling between the nanoparticles and
the underlying Py film results in distinct negative jumps of the Py
magnetoresistance. The switching of the magnetization orientation of individual
particles is clearly reflected in the Py magnetoresistance as a consequence of
AMR and DWMR, with a homogeneous particle magnetization orientation yielding
the highest resistances.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 10:38:08 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 10:37:29 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Mueller",
"Jens",
""
],
[
"Wirth",
"Steffen",
""
],
[
"von Molnar",
"Stephan",
""
]
] | [
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] |
712.232 | Ernst Heintze | Ernst Heintze (Augsburg) | Real forms and finite order automorphisms of affine Kac-Moody algebras -
an outline of a new approach | 13 pages. To appear in RIMS Kokyuroku | null | null | null | math.RA math.MG | null | We outline a new approach to classify real forms and automorphisms of finite
order of affine Kac-Moody algebras.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 10:25:40 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Heintze",
"Ernst",
"",
"Augsburg"
]
] | [
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] |
712.2321 | Euro Spallucci | Patricio Gaete, Euro Spallucci | Remarks on confinement driven by axion-like particles in Yang-Mills
theories | 8 pages, Latex; typos corrected; presentation improved; 2 references
added | J.Phys.A41:185401,2008 | 10.1088/1751-8113/41/18/185401 | USM-TH-233 | hep-th | null | Features of screening and confinement are studied for a non-Abelian gauge
theory with a mixture of pseudoscalar and scalar coupling, in the case where a
constant chromo-electric, or chromo-magnetic, strength expectation value is
present. Our discussion is carried out using the gauge-invariant but
path-dependent variables formalism. We explicitly show that the static
potential profile is the sum of a Yukawa and a linear potential, leading to the
confinement of static probe charges. Interestingly, similar results have been
obtained in the context of gluodynamics in curved space-time. For only
pseudoscalar coupling, the results are radically different.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 10:46:33 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Mar 2008 09:33:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Gaete",
"Patricio",
""
],
[
"Spallucci",
"Euro",
""
]
] | [
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] |
712.2322 | Faustino Palmero | F. Palmero, R. Carretero-Gonz\'alez, J. Cuevas, P.G. Kevrekidis and W.
Kr\'olikowski | Solitons in one-dimensional nonlinear Schr\"{o}dinger lattices with a
local inhomogeneity | 12 pages, 10 figures | null | 10.1103/PhysRevE.77.036614 | null | nlin.PS | null | In this paper we analyze the existence, stability, dynamical formation and
mobility properties of localized solutions in a one-dimensional system
described by the discrete nonlinear Schr\"{o}dinger equation with a linear
point defect. We consider both attractive and repulsive defects in a focusing
lattice. Among our main findings are: a) the destabilization of the on--site
mode centered at the defect in the repulsive case; b) the disappearance of
localized modes in the vicinity of the defect due to saddle-node bifurcations
for sufficiently strong defects of either type; c) the decrease of the
amplitude formation threshold for attractive and its increase for repulsive
defects; and d) the detailed elucidation as a function of initial speed and
defect strength of the different regimes (trapping, trapping and reflection,
pure reflection and pure transmission) of interaction of a moving localized
mode with the defect.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:27:20 GMT"
}
] | 2008-03-31T00:00:00 | [
[
"Palmero",
"F.",
""
],
[
"Carretero-González",
"R.",
""
],
[
"Cuevas",
"J.",
""
],
[
"Kevrekidis",
"P. G.",
""
],
[
"Królikowski",
"W.",
""
]
] | [
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] |
712.2323 | Gerald Teschl | Michael Schmied, Robert Sims, and Gerald Teschl | On the Absolutely Continuous Spectrum of Sturm-Liouville Operators with
Applications to Radial Quantum Trees | 16 pages | Oper. Matrices 2:3, 417-434 (2008) | 10.7153/oam-02-25 | null | math.SP math-ph math.MP | null | We consider standard subordinacy theory for general Sturm--Liouville
operators and give criteria when boundedness of solutions implies that no
subordinate solutions exist. As applications, we prove a Weidmann-type result
for general Sturm--Liouville operators and investigate the absolutely
continuous spectrum of radially symmetric quantum trees.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:32:08 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Mar 2008 10:01:56 GMT"
}
] | 2013-11-28T00:00:00 | [
[
"Schmied",
"Michael",
""
],
[
"Sims",
"Robert",
""
],
[
"Teschl",
"Gerald",
""
]
] | [
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] |
712.2324 | Andrej Vilfan | Andrej Vilfan | Myosin V passing over Arp2/3 junctions: branching ratio calculated from
the elastic lever arm model | 9 pages, 7 figures, to appear in Biophysical Journal | Biophys. J. 94, 3405-3412 (2008) | 10.1529/biophysj.107.120568 | null | physics.bio-ph cond-mat.soft q-bio.BM | null | Myosin V is a two-headed processive motor protein that walks in a
hand-over-hand fashion along actin filaments. When it encounters a filament
branch, formed by the Arp2/3 complex, it can either stay on the straight mother
filament, or switch to the daughter filament. We study both probabilities using
the elastic lever arm model for myosin V. We calculate the shapes and bending
energies of all relevant configurations in which the trail head is bound to the
actin filament before Arp2/3 and the lead head is bound either to the mother or
to the daughter filament. Based on the assumption that the probability for a
head to bind to a certain actin subunit is proportional to the Boltzmann factor
obtained from the elastic energy, we calculate the mother/daughter filament
branching ratio. Our model predicts a value of 27% for the daughter and 73% for
the mother filament. This result is in good agreement with recent experimental
data.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:32:20 GMT"
}
] | 2008-04-03T00:00:00 | [
[
"Vilfan",
"Andrej",
""
]
] | [
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] |
712.2325 | Cosima Schuster | U. Schwingenschloegl and C. Schuster | Confined Ge-Pt states in self-organized Pt nanowire arrays on Ge(001) | 3 pages, 3 figures, accepted by Eur. Phys. J. B | The European Physical Journal B 60, 409-411 (2007) | 10.1140/epjb/e2008-00019-y | null | cond-mat.mes-hall | null | By means of band structure calculations within the density functional theory
and the generalized gradient approximation, we investigate the electronic
structure of self-organized Pt nanowires on the Ge(001) surface. In particular,
we deal with a novel one-dimensional surface state confined in the nanowire
array and clarify its origin. Due to large Pt contributions, the novel state is
rather a mixed Ge-Pt hybrid state than a confined Ge surface state. Moreover,
we compare our results to data from scanning tunneling microscopy.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:39:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schwingenschloegl",
"U.",
""
],
[
"Schuster",
"C.",
""
]
] | [
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] |
712.2326 | Dominique Eckert M. | D. Eckert, N. Produit, S. Paltani, A. Neronov, T. J.-L. Courvoisier | INTEGRAL discovery of non-thermal hard X-ray emission from the Ophiuchus
cluster | 8 pages, 9 figures, accepted by A&A | null | 10.1051/0004-6361:20078853 | null | astro-ph | null | We present the results of deep observations of the Ophiuchus cluster of
galaxies with INTEGRAL in the 3-80 keV band. We analyse 3 Ms of INTEGRAL data
on the Ophiuchus cluster with the IBIS/ISGRI hard X-ray imager and the JEM-X
X-ray monitor. In the X-ray band using JEM-X, we show that the source is
extended, and that the morphology is compatible with the results found by
previous missions. Above 20 keV, we show that the size of the source is
slightly larger than the PSF of the instrument, and is consistent with the soft
X-ray morphology found with JEM-X and ASCA. Thanks to the constraints on the
temperature provided by JEM-X, we show that the spectrum of the cluster is not
well fitted by a single-temperature thermal Bremsstrahlung model, and that
another spectral component is needed to explain the high energy data. We detect
the high energy tail with a higher detection significance (6.4 sigma) than the
BeppoSAX claim (2 sigma). Because of the imaging capabilities of JEM-X and
ISGRI, we are able to exclude the possibility that the excess emission comes
from very hot regions or absorbed AGN, which proves that the excess emission is
indeed of non-thermal origin. Using the available radio data together with the
non-thermal hard X-ray flux, we estimate a magnetic field B ~ 0.1-0.2 mu G.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:41:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Eckert",
"D.",
""
],
[
"Produit",
"N.",
""
],
[
"Paltani",
"S.",
""
],
[
"Neronov",
"A.",
""
],
[
"Courvoisier",
"T. J. -L.",
""
]
] | [
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-0.0725604221,
-0.1004458144,
-0.0690078288,
-0.0255007781
] |
712.2327 | Lothar Tiator | B. Pasquini (Pavia), D. Drechsel, L. Tiator (Mainz) | Invariant Amplitudes for Pion Electroproduction | 18 pages, 8 figures | Eur.Phys.J.A34:387-403,2007 | 10.1140/epja/i2007-10510-7 | null | hep-ph nucl-th | null | The invariant amplitudes for pion electroproduction on the nucleon are
evaluated by dispersion relations at constant t with MAID as input for the
imaginary parts of these amplitudes. In the threshold region these amplitudes
are confronted with the predictions of several low-energy theorems derived in
the soft-pion limit. In general agreement with Chiral Perturbation Theory, the
dispersive approach yields large corrections to these theorems because of the
finite pion mass.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 11:58:00 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Pasquini",
"B.",
"",
"Pavia"
],
[
"Drechsel",
"D.",
"",
"Mainz"
],
[
"Tiator",
"L.",
"",
"Mainz"
]
] | [
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712.2328 | Erwan Deriaz M | Erwan Deriaz | $L^2$-stability of explicit schemes for incompressible Euler equations | 6 pages | null | null | null | math.NA | null | We present an original study on the numerical stabiliy of explicit schemes
solving the incompressible Euler equations on an open domain with slipping
boundary conditions. Relying on the skewness property of the non-linear term,
we demonstrate that some explicit schemes are numerically stable for small
perturbations under the condition $\delta t\leq C \delta x^{2r/(2r-1)}$ where
$r$ is an integer, $\delta t$ the time step and $\delta x$ the space step.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:01:32 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Deriaz",
"Erwan",
""
]
] | [
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712.2329 | Mahender Singh | Mahender Singh | Fixed points of circle actions on spaces with rational cohomology of
$S^n V S^{2n} V S^{3n}$ or $P^2(n) V S^{3n}$ | 10 pages, appeared in Archiv der Mathematik | Archiv der Mathematik, 92 (2009), 174-183 | 10.1007/s00013-009-2792-3 | null | math.AT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $X$ be a finitistic space with its rational cohomology isomorphic to that
of the wedge sum $P^2(n)\vee S^{3n} $ or $S^{n} \vee S^{2n}\vee S^{3n}$. We
study continuous $\mathbb{S}^1$ actions on $X$ and determine the possible fixed
point sets up to rational cohomology depending on whether or not $X$ is totally
non-homologous to zero in $X_{\mathbb{S}^1}$ in the Borel fibration
$X\hookrightarrow X_{\mathbb{S}^1} \longrightarrow B_{\mathbb{S}^1}$. We also
give examples realizing the possible cases.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:02:12 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Dec 2007 09:18:21 GMT"
},
{
"version": "v3",
"created": "Fri, 27 Mar 2009 08:44:35 GMT"
},
{
"version": "v4",
"created": "Tue, 28 Sep 2010 04:22:44 GMT"
}
] | 2010-09-29T00:00:00 | [
[
"Singh",
"Mahender",
""
]
] | [
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0.083311893,
0.0890521929,
-0.0188757554,
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] |
712.233 | Alessandro Giuliani | Alessandro Giuliani, Joel L. Lebowitz, Elliott H. Lieb | Periodic minimizers in 1D local mean field theory | 20 pages, 2 figures | Comm. Math. Phys. 286, 163-177 (2009) | 10.1007/s00220-008-0589-z | null | math-ph cond-mat.stat-mech math.MP | null | Using reflection positivity techniques we prove the existence of minimizers
for a class of mesoscopic free-energies representing 1D systems with competing
interactions. All minimizers are either periodic, with zero average, or of
constant sign. If the local term in the free energy satisfies a convexity
condition, then all minimizers are either periodic or constant. Examples of
both phenomena are given. This extends our previous work where such results
were proved for the ground states of lattice systems with ferromagnetic nearest
neighbor interactions and dipolar type antiferromagnetic long range
interactions.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:03:09 GMT"
}
] | 2011-09-09T00:00:00 | [
[
"Giuliani",
"Alessandro",
""
],
[
"Lebowitz",
"Joel L.",
""
],
[
"Lieb",
"Elliott H.",
""
]
] | [
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] |
712.2331 | Andrey Milchev | D. I. Dimitrov, A. Milchev, and K. Binder | Forced Imbibition - a Tool for Determining Laplace Pressure, Drag Force
and Slip Length in Capillary Filling Experiments | 4 pages, 5 figures | null | 10.1039/b719248g | null | physics.flu-dyn physics.comp-ph | null | When a very thin capillary is inserted into a liquid, the liquid is sucked
into it: this imbibition process is controlled by a balance of capillary and
drag forces, which are hard to quantify experimentally, in particularly
considering flow on the nanoscale. By computer experiments using a generic
coarse-grained model, it is shown that an analysis of imbibition forced by a
controllable external pressure quantifies relevant physical parameter such as
the Laplace pressure, Darcy's permeability, effective pore radius, effective
viscosity, dynamic contact angle and slip length of the fluid flowing into the
pore. In determining all these parameters independently, the consistency of our
analysis of such forced imbibition processes is demonstrated.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:11:00 GMT"
}
] | 2019-02-20T00:00:00 | [
[
"Dimitrov",
"D. I.",
""
],
[
"Milchev",
"A.",
""
],
[
"Binder",
"K.",
""
]
] | [
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] |
712.2332 | Jose Luis Jaramillo | J.L. Jaramillo, J.A. Valiente Kroon and E. Gourgoulhon | From Geometry to Numerics: interdisciplinary aspects in mathematical and
numerical relativity | Topical review commissioned by Classical and Quantum Gravity.
Discussion inspired by the workshop "From Geometry to Numerics" (Paris, 20-24
November, 2006), part of the "General Relativity Trimester" at the Institut
Henri Poincare (Fall 2006). Comments and references added. Typos corrected.
Submitted to Classical and Quantum Gravity | Class.Quant.Grav.25:093001,2008 | 10.1088/0264-9381/25/9/093001 | null | gr-qc | null | This article reviews some aspects in the current relationship between
mathematical and numerical General Relativity. Focus is placed on the
description of isolated systems, with a particular emphasis on recent
developments in the study of black holes. Ideas concerning asymptotic flatness,
the initial value problem, the constraint equations, evolution formalisms,
geometric inequalities and quasi-local black hole horizons are discussed on the
light of the interaction between numerical and mathematical relativists.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:20:54 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jan 2008 17:38:11 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Jaramillo",
"J. L.",
""
],
[
"Kroon",
"J. A. Valiente",
""
],
[
"Gourgoulhon",
"E.",
""
]
] | [
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] |
712.2333 | Mayra Osorio | Mayra Osorio | Models for Dust and Molecular Emission of High-Mass Protostars | 8 pages, 5 figures. Conference: "Massive Star Formation: Observations
confront Theory" 2007, Heidelberg Germany. To appear in Astronomical Society
of the Pacific | null | null | null | astro-ph | null | We present the results of a detailed modeling aimed to reproduce the spectral
energy distribution (SED) of dust and molecular line emission of massive
protostars under the hypothesis that they form via an accretion process. We
model the emission originated in the infalling envelopes at scales smaller than
0.1 pc from the central protostar. To do that, we compared our model results
with observational data covering a wide range of wavelengths, paying special
attention to the high angular resolution mid-infrared data obtained with the
Gemini Observatory and the ammonia line emission observed with the VLA at
centimeter wavelengths. We have explored two kind of model envelopes. In the
first kind of models, spherical symmetry is assumed and the SED as well as the
ammonia emission of the infalling envelope are calculated. In this way, the
temperature, density, velocity, velocity dispersion, and ammonia abundance
variations along the core can be obtained. The second approach takes into
account deviations from the spherical symmetry, and parameters such as the
rotation, degree of elongation of the core, or inclination of the system can be
constrained through the SED fitting. Using these two approaches we have been
able to model the formation of massive stars with a degree of detail similar to
that reached for the low mass stars.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:22:42 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Osorio",
"Mayra",
""
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712.2334 | Daniel Sevcovic | M. Benes, M. Kimura, P. Paus, D. Sevcovic, T. Tsujikawa, S. Yazaki | Application of a curvature adjusted method in image segmentation | submitted to: Bulltetin of Inst. of Mathematics, Academia Sinica at
Taipei | null | null | null | math.NA | null | This article deals with flow of plane curves driven by the curvature and
external force. We make use of such a geometric flow for the purpose of image
segmentation. A parametric model for evolving curves with uniform and curvature
adjusted redistribution of grid points will be described and compared.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:24:30 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Benes",
"M.",
""
],
[
"Kimura",
"M.",
""
],
[
"Paus",
"P.",
""
],
[
"Sevcovic",
"D.",
""
],
[
"Tsujikawa",
"T.",
""
],
[
"Yazaki",
"S.",
""
]
] | [
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712.2335 | Didier Sornette | D. Sornette, S. Utkin and A. Saichev | Nonlinear theory and tests of earthquake recurrence times | 31 pages including 11 figures | null | 10.1103/PhysRevE.77.066109 | null | physics.data-an physics.geo-ph | null | We develop an efficient numerical scheme to solve accurately the set of
nonlinear integral equations derived previously in (Saichev and Sornette,
2007), which describes the distribution of inter-event times in the framework
of a general model of earthquake clustering with long memory. Detailed
comparisons between the linear and nonlinear versions of the theory and direct
synthetic catalogs show that the nonlinear theory provides an excellent fit to
the synthetic catalogs, while there are significant biases resulting from the
use of the linear approximation. We then address the suggestions proposed by
some authors to use the empirical distribution of inter-event times to obtain a
better determination of the so-called clustering parameter. Our theory and
tests against synthetic and empirical catalogs find a rather dramatic lack of
power for the distribution of inter-event times to distinguish between quite
different sets of parameters, casting doubt on the usefulness of this
statistics for the specific purpose of identifying the clustering parameter.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:29:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sornette",
"D.",
""
],
[
"Utkin",
"S.",
""
],
[
"Saichev",
"A.",
""
]
] | [
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] |
712.2336 | Andreas Schaelicke | Andreas Sch\"alicke, Karim Laihem and Pavel Starovoitov | Polarised Geant4 - Applications at the ILC | Proceedings to the International Conference on Linear Colliders
(ILC07/LCWS07), Hamburg 2007 | ECONF C0705302:POL04,2007 | null | DESY-07-202 | physics.ins-det | null | Geant4 is a Monte Carlo simulation framework for the description of
interactions of particles and matter. Starting with version 8.2 a new package
of QED physics processes is available, allowing for the studies of interactions
of polarised particles with polarised media dedicated to beam applications. In
this contribution some details about the implementation are presented and
applications to the linear collider are discussed.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:38:20 GMT"
}
] | 2009-02-16T00:00:00 | [
[
"Schälicke",
"Andreas",
""
],
[
"Laihem",
"Karim",
""
],
[
"Starovoitov",
"Pavel",
""
]
] | [
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] |
712.2337 | David Sauzin | David Sauzin (IMCCE) | Mould expansions for the saddle-node and resurgence monomials | 78 pages | null | null | null | math.DS | null | This article is an introduction to some aspects of \'Ecalle's mould calculus,
a powerful combinatorial tool which yields surprisingly explicit formulas for
the normalising series attached to an analytic germ of singular vector field or
of map. This is illustrated on the case of the saddle-node, a two-dimensional
vector field which is formally conjugate to Euler's vector field
$x^2\frac{\pa}{\pa x}+(x+y)\frac{\pa}{\pa y}$, and for which the formal
normalisation is shown to be resurgent in $1/x$. Resurgence monomials adapted
to alien calculus are also described as another application of mould calculus.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:35:59 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Sauzin",
"David",
"",
"IMCCE"
]
] | [
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712.2338 | Louis-Pierre Arguin | Louis-Pierre Arguin | Competing Particle Systems and the Ghirlanda-Guerra Identities | 17 pages | Electr. Jour. Prob. 13 (2008) 2101-2117 | null | null | math.PR cond-mat.dis-nn math-ph math.MP | null | We study point processes on the real line whose configurations X can be
ordered decreasingly and evolve by increments which are functions of correlated
gaussian variables. The correlations are intrinsic to the points and quantified
by a matrix Q={q_ij}. Quasi-stationary systems are those for which the law of
(X,Q) is invariant under the evolution up to translation of X. It was
conjectured by Aizenman and co-authors that the matrix Q of robustly
quasi-stationary systems must exhibit a hierarchal structure. This was
established recently, up to a natural decomposition of the system, whenever the
set S_Q of values assumed by q_ij is finite. In this paper, we study the
general case where S_Q may be infinite. Using the past increments of the
evolution, we show that the law of robustly quasi-stationary systems must obey
the Ghirlanda-Guerra identities, which first appear in the study of spin glass
models. This provides strong evidence that the above conjecture also holds in
the general case.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:37:31 GMT"
}
] | 2010-11-09T00:00:00 | [
[
"Arguin",
"Louis-Pierre",
""
]
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712.2339 | Serge Richard | Johannes Kellendonk, Serge Richard | The topological meaning of Levinson's theorem, half-bound states
included | 4 pages | null | 10.1088/1751-8113/41/29/295207 | null | math-ph math.MP | null | We propose to interpret Levinson's theorem as an index theorem. This exhibits
its topological nature. It furthermore leads to a more coherent explanation of
the corrections due to resonances at thresholds.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:39:04 GMT"
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] | 2009-11-13T00:00:00 | [
[
"Kellendonk",
"Johannes",
""
],
[
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"Serge",
""
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712.234 | Andreas Schaelicke | Andreas Sch\"alicke | Polarised Positrons for the ILC | Presented at the XXXI International Conference of Theoretical
Physics, "Matter to the Deepest", Ustron, Poland, September 5--11, 2007 | ActaPhys.Polon.B38:3589,2007 | null | DESY-07-203 | hep-ex | null | For the planned International Linear Collider it is intended to have both --
electron and positron -- beams polarised. This offers a great benefit for many
physics studies, but also provides a challenge for the engineering of the
machine. A polarised positron source that meets the machine parameters is topic
of current design studies and prototype experiments.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:50:37 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Schälicke",
"Andreas",
""
]
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712.2341 | Lars Brink | Lars Brink | From the Nambu-Goto the Sigma-Model Action, Memoirs from Long Ago | Contribution to the volume "The Birth of StringTheory" 12 pages | null | null | null | hep-th | null | In this article I describe my own stumblings in the first string era. This
was a time when most of the active people were very young, not very
knowledgeable and the field was completely new. Many of us had little training
for what we came to work on, and it took quite some time to accomplish the new
conceptual discoveries.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 12:56:47 GMT"
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] | 2007-12-17T00:00:00 | [
[
"Brink",
"Lars",
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] |
712.2342 | Klaus Capelle | Mariana M. Odashima and K. Capelle | Empirical analysis of the Lieb-Oxford bound in ions and molecules | 8 pages, 3 color figures | Int. J. Quantum Chem. 108, p. 2428 (2008) | 10.1002/qua.21677 | null | physics.chem-ph cond-mat.mtrl-sci physics.atom-ph | null | Universal properties of the Coulomb interaction energy apply to all
many-electron systems. Bounds on the exchange-correlation energy, inparticular,
are important for the construction of improved density functionals. Here we
investigate one such universal property -- the Lieb-Oxford lower bound -- for
ionic and molecular systems. In recent work [J. Chem. Phys. 127, 054106
(2007)], we observed that for atoms and electron liquids this bound may be
substantially tightened. Calculations for a few ions and molecules suggested
the same tendency, but were not conclusive due to the small number of systems
considered. Here we extend that analysis to many different families of ions and
molecules, and find that for these, too, the bound can be empirically tightened
by a similar margin as for atoms and electron liquids. Tightening the
Lieb-Oxford bound will have consequences for the performance of various
approximate exchange-correlation functionals.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:00:41 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Odashima",
"Mariana M.",
""
],
[
"Capelle",
"K.",
""
]
] | [
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] |
712.2343 | Andriy Ushakov | Andriy Ushakov and Sabine Riemann | Radiation damage of the ILC positron source target | to appear in the proceedings of the Linear Collider Workshop 2007 and
the International Linear Collider meeting 2007, DESY, Hamburg, 30 May - 3
June 2007 | ECONF C0705302:SRC10,2007 | null | DESY 07-204 | physics.acc-ph | null | The radiation damage of the positron source target for the International
Linear Collider (ILC) has been studied. The displacement damage in target
material due to multi-MeV photons has been calculated by combining FLUKA
simulations for secondary particle production, SPECTER data for neutron
displacement cross-sections and the Lindhard model for estimations of
displacement damage by ions. The radiation damage of a stationary Ti6Al4V
target in units of displacements per atom (dpa) has been estimated for photons
from an undulator with strength 0.92 and period 1.15 cm. The calculated damage
is 7 dpa. Approximately 12.5% of displacement damage result from neutrons.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:12:48 GMT"
}
] | 2009-02-16T00:00:00 | [
[
"Ushakov",
"Andriy",
""
],
[
"Riemann",
"Sabine",
""
]
] | [
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] |
712.2344 | Par M. Kurlberg | Robert L. Benedetto, Dragos Ghioca, Par Kurlberg, and Thomas J. Tucker | The Dynamical Mordell-Lang Conjecture | 25 pages. Results strengthened to include the case of indecomposable
polynomials with complex coefficients (using some recent results of Medvedev
and Scanlon.) | null | null | null | math.NT math.AG math.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove a special case of a dynamical analogue of the classical Mordell-Lang
conjecture. In particular, let $\phi$ be a rational function with no
superattracting periodic points other than exceptional points. If the
coefficients of $\phi$ are algebraic, we show that the orbit of a point outside
the union of proper preperiodic subvarieties of $(\bP^1)^g$ has only finite
intersection with any curve contained in $(\bP^1)^g$. We also show that our
result holds for indecomposable polynomials $\phi$ with coefficients in $\bC$.
Our proof uses results from $p$-adic dynamics together with an integrality
argument. The extension to polynomials defined over $\bC$ uses the method of
specializations coupled with some new results of Medvedev and Scanlon for
describing the periodic plane curves under the action of $(\phi,\phi)$ on
$\bA^2$.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:06:51 GMT"
},
{
"version": "v2",
"created": "Fri, 6 Feb 2009 16:13:22 GMT"
}
] | 2009-02-06T00:00:00 | [
[
"Benedetto",
"Robert L.",
""
],
[
"Ghioca",
"Dragos",
""
],
[
"Kurlberg",
"Par",
""
],
[
"Tucker",
"Thomas J.",
""
]
] | [
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] |
712.2345 | Yi Wang | Bin Chen, Yi Wang, Wei Xue | Inflationary NonGaussianity from Thermal Fluctuations | 20 pages, 1 figure. v2, v3: references and acknowledgments updated | JCAP 0805:014,2008 | 10.1088/1475-7516/2008/05/014 | CAS-KITPC/ITP-017 | hep-th astro-ph gr-qc | null | We calculate the contribution of the fluctuations with the thermal origin to
the inflationary nonGaussianity. We find that even a small component of
radiation can lead to a large nonGaussianity. We show that this thermal
nonGaussianity always has positive $f_{\rm NL}$. We illustrate our result in
the chain inflation model and the very weakly dissipative warm inflation model.
We show that $f_{NL}\sim {\cal O}(1)$ is general in such models. If we allow
modified equation of state, or some decoupling effects, the large thermal
nonGaussianity of order $f_{\rm NL}>5$ or even $f_{\rm NL}\sim 100$ can be
produced. We also show that the power spectrum of chain inflation should have a
thermal origin. In the Appendix A, we made a clarification on the different
conventions used in the literature related to the calculation of $f_{\rm NL}$.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:13:37 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 02:10:09 GMT"
},
{
"version": "v3",
"created": "Tue, 18 Dec 2007 12:27:15 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Chen",
"Bin",
""
],
[
"Wang",
"Yi",
""
],
[
"Xue",
"Wei",
""
]
] | [
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] |
712.2346 | Bernd Reindl | G.A. Tammann (1), A. Sandage (2), B. Reindl (1) ((1) Astr. Inst. Univ.
Basel, (2) Obs. Carnegie Inst. Washington) | Comparison of Distances from RR Lyrae Stars, the Tip of the Red-Giant
Branch and Classical Cepheids | 55 pages, 9 figures, 9 tables, accepted for publication in the
Astrophysical Journal | null | 10.1086/529508 | null | astro-ph | null | The extragalactic distance scale relies heavily on Cepheids. However, it has
become clear from observations and pulsation models that the slope and zero
point of their P-L relations differ from galaxy to galaxy. This makes the
determination of Cepheid distances complex and calls for an independent test of
their differences. The test is provided by RR Lyrae star distances of 24
galaxies which calibrate the tip of the red-giant branch (TRGB; M_I = -4.05),
which in turn confirms the adopted Cepheids distances on our 2006 distance
scale in 18 cases to within 0.1 mag on average. Relative SN Ia and velocity
distances deny a remaining significant metallicity effect of the adopted
distances. The new support for these Cepheid distances increases the weight of
our previous calibration of the SN Ia luminosity and of the 21cm line width -
luminosity (TF) relation. The value of H_0 = 62.3 (+/-5) is confirmed on all
scales.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:57:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tammann",
"G. A.",
""
],
[
"Sandage",
"A.",
""
],
[
"Reindl",
"B.",
""
]
] | [
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] |
712.2347 | Vladimir Chernov (Tchernov) | Evarist Byberi and Vladimir Chernov (Tchernov) | Virtual Bridge Number One Knots | 8 pages, 7 figures | Commun. Contemp. Math. 10 (2008), suppl. 1, 1013-1021 | null | null | math.GT | null | We define the virtual bridge number $vb(K)$ and the virtual unknotting number
$vu(K)$ invariants for virtual knots. For ordinary knots $K$ they are closely
related to the bridge number $b(K)$ and the unknotting number $u(K)$ and we
have $vu(K)\leq u(K), vb(K)\leq b(K).$
There are no ordinary knots $K$ with $b(K)=1.$ We show there are infinitely
many homotopy classes of virtual knots each of which contains infinitely many
isotopy classes of $K$ with $vb(K)=1.$ In fact for each $i\in \N$ there exists
$K$ virtually homotopic (but not virtually isotopic) to the unknot with
$vb(K)=1$ and $vu(K)=i.$
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:29:07 GMT"
}
] | 2014-04-24T00:00:00 | [
[
"Byberi",
"Evarist",
"",
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],
[
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"Vladimir",
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712.2348 | Thomas Kuhr | CDF collaboration: T. Aaltonen, et al | Measurement of Lifetime and Decay-Width Difference in B0s -> J/psi phi
Decays | null | Phys.Rev.Lett.100:121803,2008 | 10.1103/PhysRevLett.100.121803 | FERMILAB-PUB-07-655-E | hep-ex | null | We measure the mean lifetime, tau=2/(Gamma_L+Gamma_H), and the width
difference, DeltaGamma=Gamma_L-Gamma_H, of the light and heavy mass eigenstates
of the B0s meson, B0sL and B0sH, in B0s -> J/psi phi decays using 1.7 fb^-1 of
data collected with the CDF II detector at the Fermilab Tevatron ppbar
collider. Assuming CP conservation, a good approximation for the B0s system in
the Standard Model, we obtain DeltaGamma = 0.076^+0.059_-0.063 (stat.) +- 0.006
(syst.) ps^-1 and tau = 1.52 +- 0.04 (stat.) +- 0.02 (syst.) ps, the most
precise measurements to date. Our constraints on the weak phase and DeltaGamma
are consistent with CP conservation.
Dedicated to the memory of our dear friend and colleague, Michael P. Schmidt
| [
{
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"created": "Fri, 14 Dec 2007 20:05:51 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Apr 2008 19:01:20 GMT"
}
] | 2010-05-12T00:00:00 | [
[
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"",
""
],
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"T.",
""
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712.2349 | Sebastian Bernhardsson | Petter Minnhagen and Sebastian Bernhardsson | Optimization and Scale-freeness for Complex Networks | 8 pages, 4 figures | Chaos 17, 2 (2007) | 10.1063/1.2720101 | null | cond-mat.stat-mech | null | Complex networks are mapped to a model of boxes and balls where the balls are
distinguishable. It is shown that the scale-free size distribution of boxes
maximizes the information associated with the boxes provided configurations
including boxes containing a finite fraction of the total amount of balls are
excluded. It is conjectured that for a connected network with only links
between different nodes, the nodes with a finite fraction of links are
effectively suppressed. It is hence suggested that for such networks the
scale-free node-size distribution maximizes the information encoded on the
nodes. The noise associated with the size distributions is also obtained from a
maximum entropy principle. Finally explicit predictions from our least bias
approach are found to be born out by metabolic networks.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:55:45 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Minnhagen",
"Petter",
""
],
[
"Bernhardsson",
"Sebastian",
""
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] |
712.235 | Klaus Capelle | J. M. Morbec and K. Capelle | Orbital-polarization terms: from a phenomenological to a
first-principles description of orbital magnetism in density-functional
theory | null | Int. J. Quantum Chem. 108, p. 2433 (2008) | 10.1002/qua.21784 | null | cond-mat.mtrl-sci physics.chem-ph | null | Phenomenological orbital-polarization (OP) terms have been repeatedly
introduced in the single-particle equations of spin-density-functional theory,
in order to improve the description of orbital magnetic moments in systems
containing transition metal ions. Here we show that these ad hoc corrections
can be interpreted as approximations to the exchange-correlation vector
potential A_xc of current-density-functional theory (CDFT). This connection
provides additional information on both approaches: Phenomenological OP terms
are connected to first-principles theory, leading to a rationale for their
empirical success and a reassessment of their limitations and the
approximations made in their derivation. Conversely, the connection of OP terms
with CDFT leads to a set of simple approximations to the CDFT potential A_xc,
with a number of desirable features that are absent from electron-gas-based
functionals.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 13:48:08 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Morbec",
"J. M.",
""
],
[
"Capelle",
"K.",
""
]
] | [
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712.2351 | Teruhiko Kawano | Teruhiko Kawano | Chaotic D-Term Inflation | 3 pages, lanlmac | Prog. Theor. Phys. 120 (2008), 793 | 10.1143/PTP.120.793 | UT-07-40 | hep-th astro-ph gr-qc hep-ph | null | A simple model for chaotic inflation in supergravity is proposed. The model
is N=1 supersymmetric massive U(1) gauge theory via the Stuckelberg superfield
and gives rise to D-term inflation with a quadratic term of inflaton in the
potential. The Fayet-Iliopoulos field plays a role of the inflaton.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:05:09 GMT"
}
] | 2008-12-23T00:00:00 | [
[
"Kawano",
"Teruhiko",
""
]
] | [
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] |
712.2352 | Guido Nolte | Guido Nolte, Andreas Ziehe, Vadim V. Nikulin, Alois Schl\"ogl, Nicole
Kr\"amer, Tom Brismar, Klaus-Robert M\"uller | Robustly estimating the flow direction of information in complex
physical systems | 5 pages, 4 figures | null | 10.1103/PhysRevLett.100.234101 | null | stat.ME stat.AP | null | We propose a new measure to estimate the direction of information flux in
multivariate time series from complex systems. This measure, based on the slope
of the phase spectrum (Phase Slope Index) has invariance properties that are
important for applications in real physical or biological systems: (a) it is
strictly insensitive to mixtures of arbitrary independent sources, (b) it gives
meaningful results even if the phase spectrum is not linear, and (c) it
properly weights contributions from different frequencies. Simulations of a
class of coupled multivariate random data show that for truly unidirectional
information flow without additional noise contamination our measure detects the
correct direction as good as the standard Granger causality. For random
mixtures of independent sources Granger Causality erroneously yields highly
significant results whereas our measure correctly becomes non-significant. An
application of our novel method to EEG data (88 subjects in eyes-closed
condition) reveals a strikingly clear front-to-back information flow in the
vast majority of subjects and thus contributes to a better understanding of
information processing in the brain.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 16:10:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nolte",
"Guido",
""
],
[
"Ziehe",
"Andreas",
""
],
[
"Nikulin",
"Vadim V.",
""
],
[
"Schlögl",
"Alois",
""
],
[
"Krämer",
"Nicole",
""
],
[
"Brismar",
"Tom",
""
],
[
"Müller",
"Klaus-Robert",
""
]
] | [
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] |
712.2353 | Stephen L. Olsen | Stephen L. Olsen (for the Belle Collaboration) | Recent Belle results on CP violation | 5 pages, 5 figures to be published in the Proceedings of the 4th
International Conference on Flavor Physics (ICFP 2007), Beijing, China, 24-28
Sept. 2007 | Int.J.Mod.Phys.A23:3277-3281,2008 | 10.1142/S0217751X08041979 | null | hep-ex | null | The Belle experiment's recent results on CP violation in B meson decays are
summarized.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 08:05:11 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Olsen",
"Stephen L.",
"",
"for the Belle Collaboration"
]
] | [
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] |
712.2354 | Victor Malyshev | Joost A. Klugkist, Victor A. Malyshev, Jasper Knoester | Intrinsic optical bistability of thin films of linear molecular
aggregates: The two-exciton approximation | 11 two-column pages, 6 figures, to appear in the Journal of Chemical
Physics | J. Chem. Phys. 128, 084706 (2008) | 10.1063/1.2832312 | null | cond-mat.dis-nn cond-mat.mtrl-sci | null | We generalize our recent work on the optical bistability of thin films of
molecular aggregates [J. Chem. Phys. 127, 164705 (2007); arXiv:0707.1264v1
[cond-mat.dis-nn]] by accounting for the optical transitions from the
one-exciton manifold to the two-exciton manifold as well as the exciton-exciton
annihilation of the two-exciton states via a high-lying molecular vibronic
term. We also include the relaxation from the vibronic level back to both the
one-exciton manifold and the ground state. By selecting the dominant optical
transitions between the ground state, the one-exciton manifold, and the
two-exciton manifold, we reduce the problem to four levels, enabling us to
describe the nonlinear optical response of the film. The one- and two-exciton
states are obtained by diagonalizing a Frenkel Hamiltonian with an uncorrelated
on-site (diagonal) disorder. The optical dynamics is described by means of the
density matrix equations coupled to the electromagnetic field in the film. We
show that the one-to-two exciton transitions followed by a fast exciton-exciton
annihilation promote the occurrence of bistability and reduce the switching
intensity. We provide estimates of pertinent parameters for actual materials
and conclude that the effect can be realized.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:17:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Klugkist",
"Joost A.",
""
],
[
"Malyshev",
"Victor A.",
""
],
[
"Knoester",
"Jasper",
""
]
] | [
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] |
712.2355 | Rikkert Frederix | R. Frederix, F. Maltoni | Top pair invariant mass distribution: a window on new physics | 32 pages, 18 figures; Improvements on the section about the top quark
mass dependence, including one more figure | JHEP 0901:047,2009 | 10.1088/1126-6708/2009/01/047 | CP3-07-29 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We explore in detail the physics potential of a measurement of the ttbar
invariant mass distribution. First, we assess the accuracy of the best
available predictions for this observable and find that in the low invariant
mass region, the shape is very well predicted and could be used to perform a
top mass measurement. Second, we study the effects of a heavy s-channel
resonance on the ttbar invariant mass distribution, in a model independent way.
We provide the necessary Monte Carlo tools to perform the search and outline a
simple three-step analysis.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:26:04 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jul 2008 12:34:28 GMT"
},
{
"version": "v3",
"created": "Wed, 21 Jan 2009 09:11:45 GMT"
}
] | 2009-01-27T00:00:00 | [
[
"Frederix",
"R.",
""
],
[
"Maltoni",
"F.",
""
]
] | [
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] |
712.2356 | Klaus Moenig | Ties Behnke, Chris Damerell, John Jaros, Akya Myamoto, et al | ILC Reference Design Report Volume 4 - Detectors | A version with high resolution pictures can be found at
http://www.linearcollider.org/cms/?pid=1000437 The full authorlist is inside
the report | null | null | null | physics.ins-det | null | This report, Volume IV of the International Linear Collider Reference Design
Report, describes the detectors which will record and measure the charged and
neutral particles produced in the ILC's high energy e+e- collisions. The
physics of the ILC, and the environment of the machine-detector interface, pose
new challenges for detector design. Several conceptual designs for the detector
promise the needed performance, and ongoing detector R&D is addressing the
outstanding technological issues. Two such detectors, operating in push-pull
mode, perfectly instrument the ILC interaction region, and access the full
potential of ILC physics.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 10:36:45 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Behnke",
"Ties",
""
],
[
"Damerell",
"Chris",
""
],
[
"Jaros",
"John",
""
],
[
"Myamoto",
"Akya",
""
]
] | [
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712.2357 | Ansgar Reiners | Ansgar Reiners | At the Bottom of the Main Sequence: Activity and magnetic fields beyond
the threshold to complete convection | 25 pages, 7 figures, Ludwig Biermann Lecture given at the annual
meeting of the German Astronomical Society, 2007, v2 | null | 10.1002/9783527622993.ch3 | null | astro-ph | null | The bottom of the main sequence hosts objects with fundamentally different
properties. At masses of about 0.3 M$_{\odot}$, stars become fully convective
and at about 0.08 M$_{\odot}$ the hydrogen-burning main sequence ends; less
massive objects are brown dwarfs. While stars and brown dwarfs experience very
different evolutions, their inner structure has relatively little impact on the
atmospheres. The generation of magnetic fields and activity is obviously
connected to the threshold between partial and complete convection, because
dynamo mechanisms involving a layer of shear like the solar
$\alpha\Omega$-dynamo must cease. Hence a change in stellar activity can be
expected there. Observations of stellar activity do not confirm a rapid break
in activity at the convection boundary, but the fraction of active stars and
rapid rotators is higher on the fully convective side. I summarize the current
picture of stellar activity and magnetic field measurements at the bottom of
the main sequence and present recent results on rotational braking beyond.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:21:59 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Dec 2007 13:49:17 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Reiners",
"Ansgar",
""
]
] | [
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712.2358 | Richard W. Robinett | R. W. Robinett | Using Physics to Learn Mathematica to Do Physics: From Homework Problems
to Research Examples | 27 pages, 3 figures | null | null | null | physics.ed-ph physics.comp-ph | null | We describe the development of a junior-senior level course for Physics
majors designed to teach Mathematica skills in support of their undergraduate
coursework, but also to introduce students to modern research level results.
Standard introductory and intermediate level Physics homework-style problems
are used to teach Mathematica commands and programming methods, which are then
applied, in turn, to more sophisticated problems in some of the core
undergraduate subjects, along with making contact with recent research papers
in a variety of fields.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:22:39 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Robinett",
"R. W.",
""
]
] | [
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] |
712.2359 | Katarzyna Ostasiewicz | A. Radosz, A. T. Augousti, K. Ostasiewicz | Decoupling of kinematical time dilation and gravitational time dilation
in particular geometries | 4 pages | ActaPhys.Polon.B39:1357-1362,2008 | null | null | gr-qc | null | Two different forms of time dilation, namely, the kinematical time dilation
of special relativity and gravitational red shift are coupled during
observations of systems moving through a gravitational field. In the particular
situation of free fall in a Schwarzschild geometry these two effects are
decoupled and in consequence the time dilation, as observed by a distant
observer, factorises. Such a factorization is not a universal feature. We
define here a necessary and sufficient criterion for time dilation and
gravitational red-shift decoupling. This property is manifested in a particular
form of the Doppler shift in Schwarzschild geometry.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:27:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Radosz",
"A.",
""
],
[
"Augousti",
"A. T.",
""
],
[
"Ostasiewicz",
"K.",
""
]
] | [
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] |
712.236 | John Ellis | J.S. Lee, M. Carena, J. Ellis, A. Pilaftsis and C.E.M. Wagner | CPsuperH2.0: an Improved Computational Tool for Higgs Phenomenology in
the MSSM with Explicit CP Violation | 35 pages, 11 figures, references added, to appear in Comput. Phys.
Commun | Comput.Phys.Commun.180:312-331,2009 | 10.1016/j.cpc.2008.09.003 | KEK-TH-1203 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We describe the Fortran code CPsuperH2.}, which contains several improvements
and extensions of its predecessor CPsuperH. It implements improved calculations
of the Higgs-boson pole masses, notably a full treatment of the 4 times 4
neutral Higgs propagator matrix including the Goldstone boson and a more
complete treatment of threshold effects in self-energies and Yukawa couplings,
improved treatments of two-body Higgs decays, some important three-body decays,
and two-loop Higgs-mediated contributions to electric dipole moments.
CPsuperH2.0 also implements an integrated treatment of several B-meson
observables, including the branching ratios of B_s to mu^+ mu^-, B_d to tau^+
tau^-, B_u to tau nu, B to X_s gamma and the latter's CP-violating asymmetry
A_CP, and the supersymmetric contributions to the B^0_{s,d} - \bar B^0_{s,d}
mass differences. These additions make CPsuperH2.0 an attractive integrated
tool for analyzing supersymmetric CP and flavour physics as well as searches
for new physics at high-energy colliders such as the Tevatron, LHC and linear
colliders. The program may be obtained from
http://www.hep.man.ac.uk/u/jslee/CPsuperH.html
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:28:05 GMT"
},
{
"version": "v2",
"created": "Wed, 3 Sep 2008 11:44:49 GMT"
}
] | 2009-02-02T00:00:00 | [
[
"Lee",
"J. S.",
""
],
[
"Carena",
"M.",
""
],
[
"Ellis",
"J.",
""
],
[
"Pilaftsis",
"A.",
""
],
[
"Wagner",
"C. E. M.",
""
]
] | [
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] |
712.2361 | Klaus Moenig | Nan Phinney, Nobukasu Toge, Nicholas Walker, et al | ILC Reference Design Report Volume 3 - Accelerator | A version with high resolution pictures can be found at
http://www.linearcollider.org/cms/?pid=1000437 The full authorlist is inside
the report | null | null | null | physics.acc-ph | null | The International Linear Collider (ILC) is a 200-500 GeV center-of-mass
high-luminosity linear electron-positron collider, based on 1.3 GHz
superconducting radio-frequency (SCRF) accelerating cavities. The ILC has a
total footprint of about 31 km and is designed for a peak luminosity of 2x10^34
cm^-2 s^-1. The complex includes a polarized electron source, an
undulator-based positron source, two 6.7 km circumference damping rings,
two-stage bunch compressors, two 11 km long main linacs and a 4.5 km long beam
delivery system. This report is Volume III (Accelerator) of the four volume
Reference Design Report, which describes the design and cost of the ILC.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:40:46 GMT"
}
] | 2007-12-18T00:00:00 | [
[
"Phinney",
"Nan",
""
],
[
"Toge",
"Nobukasu",
""
],
[
"Walker",
"Nicholas",
""
]
] | [
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] |
712.2362 | Boris Kostenko F. | B.F. Kostenko, J. Pribish, M.Z. Yuriev | Quantum Elastic Net and the Traveling Salesman Problem | Reported at Quantum Physics and Communication, Dubna, October 15-19,
2007 | Physics of Particles and Nuclei Lett. 2009, V.6, P. 599 | null | null | quant-ph | null | Theory of computer calculations strongly depends on the nature of elements
the computer is made of. Quantum interference allows to formulate the Shor
factorization algorithm turned out to be more effective than any one written
for classical computers. Similarly, quantum wave packet reduction allows to
devise the Grover search algorithm which outperforms any classical one. In the
present paper we argue that the quantum incoherent tunneling can be used for
elaboration of new algorithms able to solve some NP-hard problems, such as the
Traveling Salesman Problem, considered to be intractable in the classical
theory of computer computations.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:44:45 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 15:56:08 GMT"
},
{
"version": "v3",
"created": "Wed, 30 Jan 2008 16:52:43 GMT"
}
] | 2009-11-23T00:00:00 | [
[
"Kostenko",
"B. F.",
""
],
[
"Pribish",
"J.",
""
],
[
"Yuriev",
"M. Z.",
""
]
] | [
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] |
712.2363 | Jason Steffen | Jason H. Steffen (Fermilab) Octavio Valenzuela (UNAM, Mexico) | Constraints on the angular distribution of satellite galaxies about
spiral hosts | MNRAS in press. Version 2 has some sections reordered and additional
discussion included | Mon.Not.Roy.Astron.Soc.387:1199-1205,2008 | 10.1111/j.1365-2966.2008.13314.x | FERMILAB-PUB-07-654-A-CD | astro-ph | null | We present, using a novel technique, a study of the angular distribution of
satellite galaxies around a sample of isolated, blue host galaxies selected
from the sixth data release of the Sloan Digital Sky Survey. As a complement to
previous studies we subdivide the sample of galaxies into bins of differing
inclination and use the systematic differences that would exist between the
different bins as the basis for our approach. We parameterize the cumulative
distribution function of satellite galaxies and apply a maximum likelihood,
Monte-Carlo technique to determine allowable distributions, which we show as an
exclusion plot. We find that the allowed distributions of the satellites of
spiral hosts are very nearly isotropic. We outline our formalism and our
analysis and discuss how this technique may be refined for future studies and
future surveys.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:26:18 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Apr 2008 15:34:38 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Steffen",
"Jason H.",
"",
"Fermilab"
],
[
"Valenzuela",
"Octavio",
"",
"UNAM, Mexico"
]
] | [
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] |
712.2364 | Peter Vermeire | Pete Vermeire | Singularities of the Secant Variety | 6 pages | null | null | null | math.AG math.AC | null | We give positivity conditions on the embedding of a smooth variety which
guarantee the normality of the secant variety, generalizing earlier results of
the author and others. We also give classes of secant varieties satisfying the
Hodge conjecture as well as a result on the singular locus of degenerate secant
varieties.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 14:55:14 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Vermeire",
"Pete",
""
]
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] |
712.2365 | Pieter Moree | Yves Gallot and Pieter Moree | Ternary cyclotomic polynomials having a large coefficient | 19 pages, 6 tables, to appear in Crelle's Journal. Revised version
with many small changes | J. Reine Angew. Math. 632 (2009), 105-125 | null | MPIM2007-141 | math.NT | null | Let $\Phi_n(x)$ denote the $n$th cyclotomic polynomial. In 1968 Sister Marion
Beiter conjectured that $a_n(k)$, the coefficient of $x^k$ in $\Phi_n(x)$,
satisfies $|a_n(k)|\le (p+1)/2$ in case $n=pqr$ with $p<q<r$ primes (in this
case $\Phi_n(x)$ is said to be ternary). Since then several results towards
establishing her conjecture have been proved (for example $|a_n(k)|\le 3p/4$).
Here we show that, nevertheless, Beiter's conjecture is false for every $p\ge
11$. We also prove that given any $\epsilon>0$ there exist infinitely many
triples $(p_j,q_j,r_j)$ with $p_1<p_2<... $ consecutive primes such that
$|a_{p_jq_jr_j}(n_j)|>(2/3-\epsilon)p_j$ for $j\ge 1$.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:05:49 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Apr 2008 14:49:54 GMT"
}
] | 2012-07-30T00:00:00 | [
[
"Gallot",
"Yves",
""
],
[
"Moree",
"Pieter",
""
]
] | [
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712.2366 | Paolo Sibani | Paolo Sibani and Simon Christiansen | Thermal shifts and intermittent linear response of aging systems | 10 pages, 17 figures, RevTeX style | Phys. Rev. E 77,041106 (2008) | 10.1103/PhysRevE.77.041106 | null | cond-mat.stat-mech cond-mat.dis-nn cond-mat.soft | null | At time $t$ after an initial quench, an aging system responds to a
perturbation turned on at time $ t_{\rm w} < t$ in a way mainly depending on
the number of intermittent energy fluctuations, so-called quakes, which fall
within the observation interval $(t_{\rm w},t]$ [Sibani et al. Phys. Rev. B,
74, 224407 and Eur. J. of Physics B, 58,483-491, 2007]. The temporal
distribution of the quakes implies a functional dependence of the average
response on the ratio $t/t_{\rm w}$. Further insight is obtained imposing small
temperature steps, so-called $T$-shifts. The average response as a function of
$t/t_{\rm w,eff}$, where $t_{\rm w,eff}$ is the effective age, is similar to
the response of a system aged isothermally at the final temperature. Using an
Ising model with plaquette interactions, the applicability of analytic formulae
for the average isothermal magnetization is confirmed. The $T$-shifted aging
behavior of the model is described using effective ages. Large positive shifts
nearly reset the effective age. Negative $T$-shifts offer a more detailed probe
of the dynamics. Assuming the marginal stability of the `current' attractor
against thermal noise fluctuations, the scaling form $t_{\rm w,eff} = t_{\rm
w}^x$, and the dependence of the exponent $x$ on the aging temperatures before
and after the shift are theoretically available. The predicted form of $x$ has
no adjustable parameters. Both the algebraic scaling of the effective age and
the form of the exponent agree with the data. The simulations thus confirm the
crucial r\^{o}le of marginal stability in glassy relaxation.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:37:12 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Sibani",
"Paolo",
""
],
[
"Christiansen",
"Simon",
""
]
] | [
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] |
712.2367 | Montserrat Teixidor i Bigas | Montserrat Teixidor i Bigas | Petri map for rank two bundles with canonical determinant | To appear in Compositio Mathematica | null | 10.1112/S0010437X07003442 | null | math.AG | null | We prove the Bertram-Feinberg-Mukai conjecture for a generic curve $C$ of
genus $g$ and a semistable vector bundle $E$ of rank two and determinant $K$ on
$C$, namely we prove the injectivity of the Petri-canonical map $S^2(H^0(E))\to
H^0(S^2(E))$.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 19:17:48 GMT"
}
] | 2014-01-14T00:00:00 | [
[
"Bigas",
"Montserrat Teixidor i",
""
]
] | [
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712.2368 | Ewa L. Lokas | Ewa L. Lokas, Radoslaw Wojtak, Gary A. Mamon and Stefan Gottloeber | Mass modelling of galaxy clusters via velocity moments | 6 pages, 5 figures, contribution to the proceedings of XIX Rencontres
de Blois | null | null | null | astro-ph | null | We summarize the method of mass modelling of galaxy clusters based on
reproducing the dispersion and kurtosis of the projected velocity distribution
of galaxies. The models are parametrized within the framework of the NFW
density profile, characterized by the virial mass and concentration, together
with the constant anisotropy of galaxy orbits. The use of velocity dispersion
alone does not allow to constrain all the three parameters from kinematic data
due to the mass-anisotropy degeneracy. The degeneracy is broken by introducing
the fourth velocity moment, the kurtosis. We tested the method based on fitting
both moments on mock data sets drawn from simulated dark matter haloes and
showed it to reproduce reliably the properties of the haloes. The method has
been applied to estimate the mass, concentration and anisotropy of more than 20
clusters which allowed us to confirm, for the first time using kinematic data,
the mass-concentration relation found in N-body simulations.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:16:58 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Lokas",
"Ewa L.",
""
],
[
"Wojtak",
"Radoslaw",
""
],
[
"Mamon",
"Gary A.",
""
],
[
"Gottloeber",
"Stefan",
""
]
] | [
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] |
712.2369 | Jason Nordhaus | J. Nordhaus (Univ. of Rochester), E. G. Blackman (Univ. of Rochester) | Dynamos and Chemical Mixing in Evolved Stars | 7 pages, 3 figures. To appear in AIP Proceedings of the IXth Torino
Workshop on AGB Nucleosynthesis | AIPConf.Proc.1001:306-312,2008 | 10.1063/1.2916979 | null | astro-ph | null | In low-mass Red Giant Branch (RGB) and Asymptotic Giant Branch (AGB) stars,
anomalous mixing must transport material near the hydrogen-burning shell to the
convective envelope. Recently, it was suggested that buoyant magnetic flux
tubes could supply the necessary transport rate (Busso et al. 2007). The fields
are assumed to originate from a dynamo operating in the stellar interior. Here,
we show what is required of an $\alpha-\Omega$ dynamo in the envelope of an AGB
star to maintain these fields. Differential rotation and rotation drain via
turbulent dissipation and Poynting flux, so if shear can be resupplied by
convection, then large-scale toroidal field strengths of
$\left<B_\phi\right>\simeq3\times10^4$ G can be sustained at the base of the
convection zone.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:26:10 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Nordhaus",
"J.",
"",
"Univ. of Rochester"
],
[
"Blackman",
"E. G.",
"",
"Univ. of Rochester"
]
] | [
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] |
712.237 | Pin Liu | Changjian Fu, Pin Liu | Lifting to cluster-tilting objects in 2-Calabi-Yau triangulated
categories | 7 pages; typos corrected; reference added; a gap filled | null | null | null | math.RT math.RA | null | We show that a tilting module over the endomorphism algebra of a
cluster-tilting object in a 2-Calabi-Yau triangulated category lifts to a
cluster-tilting object in this 2-Calabi-Yau triangulated category. This
generalizes a recent work of D. Smith for cluster categories.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:24:24 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 02:21:51 GMT"
},
{
"version": "v3",
"created": "Sat, 29 Dec 2007 15:23:54 GMT"
}
] | 2007-12-29T00:00:00 | [
[
"Fu",
"Changjian",
""
],
[
"Liu",
"Pin",
""
]
] | [
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] |
712.2371 | B.Sundar Rajan | Sanjay Karmakar and B. Sundar Rajan | Maximum-rate, Minimum-Decoding-Complexity STBCs from Clifford Algebras | Under consideration for possible publication in IEEE Transactions on
Information Theory | null | null | null | cs.IT math.IT | null | It is well known that Space-Time Block Codes (STBCs) from orthogonal designs
(ODs) are single-symbol decodable/symbol-by-symbol decodable (SSD) and are
obtainable from unitary matrix representations of Clifford algebras. However,
SSD codes are obtainable from designs that are not orthogonal also. Recently,
two such classes of SSD codes have been studied: (i) Coordinate Interleaved
Orthogonal Designs (CIODs) and (ii) Minimum-Decoding-Complexity (MDC) STBCs
from Quasi-ODs (QODs). Codes from ODs, CIODs and MDC-QODs are mutually
non-intersecting classes of codes. The class of CIODs have {\it non-unitary
weight matrices} when written as a Linear Dispersion Code (LDC) proposed by
Hassibi and Hochwald, whereas several known SSD codes including CODs have {\it
unitary weight matrices}. In this paper, we obtain SSD codes with unitary
weight matrices (that are not CODs) called Clifford Unitary Weight SSDs
(CUW-SSDs) from matrix representations of Clifford algebras. A main result of
this paper is the derivation of an achievable upper bound on the rate of any
unitary weight SSD code as $\frac{a}{2^{a-1}}$ for $2^a$ antennas which is
larger than that of the CODs which is $\frac{a+1}{2^a}$. It is shown that
several known classes of SSD codes are CUW-SSD codes and CUW-SSD codes meet
this upper bound. Also, for the codes of this paper conditions on the signal
sets which ensure full-diversity and expressions for the coding gain are
presented. A large class of SSD codes with non-unitary weight matrices are
obtained which include CIODs as a proper subclass.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:24:29 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Karmakar",
"Sanjay",
""
],
[
"Rajan",
"B. Sundar",
""
]
] | [
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] |
712.2372 | Ewa L. Lokas | Ewa L. Lokas, Jaroslaw Klimentowski and Radoslaw Wojtak | The effect of unbound stars on the mass modelling of the Fornax dwarf | 7 pages, 5 figures, contribution to the proceedings of XIX Rencontres
de Blois | null | null | null | astro-ph | null | We discuss how different approaches to selecting member stars in kinematic
samples of dwarf spheroidal galaxies affect the estimates of their mass and
anisotropy of stellar orbits. We demonstrate that the selection of members is
an additional source of error compared to the usual uncertainties due to the
sampling of velocity moments. As an example we use the kinematic data set for
202 stars in the Fornax dwarf galaxy for which we model the velocity dispersion
profile and estimate the mass-to-light ratio and anisotropy assuming that mass
follows light. We also show that stronger constraints on these parameters can
be obtained if kurtosis of the velocity distribution is included in the
analysis. Using the Besancon model of the Milky Way we demonstrate that the
majority of contamination in Fornax probably comes from the Milky Way stars.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:29:06 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Lokas",
"Ewa L.",
""
],
[
"Klimentowski",
"Jaroslaw",
""
],
[
"Wojtak",
"Radoslaw",
""
]
] | [
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] |
712.2373 | Shahin Atashbar Tehrani | Ali N. Khorramian and S. Atashbar Tehrani | Simple model for QCD analysis of the proton helicity structure | 4 pages and 1 figure, submission for the Proceedings of the
International Conference on Hadron Physics, 30 Aug - 3 Sep 2007, Canakkale,
Turkey | null | null | null | hep-ph | null | In this paper we use the experimental data to obtain the polarized parton
distribution functions (PPDFs) in the LO and NLO approximations. The analysis
is based on the Jacobi polynomials expansion of the polarized structure
function (PSF). Our calculations for polarized parton distribution functions
based on the Jacobi polynomials method are in good agreement with the other
theoretical models.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:33:24 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 13:30:15 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Khorramian",
"Ali N.",
""
],
[
"Tehrani",
"S. Atashbar",
""
]
] | [
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] |
712.2374 | Jae Dong Noh | Sang-Woo Kim and Jae Dong Noh (UOS) | Instability in a Network Coevolving with a Particle System | 4 pages and 5 figures | Phys. Rev. Lett. 100, 118702 (2008) | 10.1103/PhysRevLett.100.118702 | null | cond-mat.stat-mech | null | We study a coupled dynamics of a network and a particle system. Particles of
density $\rho$ diffuse freely along edges, each of which is rewired at a rate
given by a decreasing function of particle flux. We find that the coupled
dynamics leads to an instability toward the formation of hubs and that there is
a dynamic phase transition at a threshold particle density $\rho_c$. In the low
density phase, the network evolves into a star-shaped one with the maximum
degree growing linearly in time. In the high density phase, the network
exhibits a fat-tailed degree distribution and an interesting dynamic scaling
behavior. We present an analytic theory explaining mechanism for the
instability and a scaling theory for the dynamic scaling behavior.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:33:56 GMT"
}
] | 2008-03-24T00:00:00 | [
[
"Kim",
"Sang-Woo",
"",
"UOS"
],
[
"Noh",
"Jae Dong",
"",
"UOS"
]
] | [
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] |
712.2375 | Fabrizio Nicastro | F. Nicastro (1,2), Smita Mathur (3), Martin Elvis (2) | Missing Baryons and the Warm-Hot Intergalactic Medium | 14 pages, accepted for publication in Science (to appear as a
Perspective Article in a Januray 2008 special issue of Science) | null | 10.1126/science.1151400 | null | astro-ph | null | Stars and gas in galaxies, hot intracluster medium, and intergalactic
photo-ionized gas make up at most half of the baryons that are expected to be
present in the universe. The majority of baryons are still missing and are
expected to be hidden in a web of warm-hot intergalactic medium. This matter
was shock-heated during the collapse of density perturbations that led to the
formation of the relaxed structures that we see today. Finding the missing
baryons and thereby producing a complete inventory of possibly the only
detectable component of the energy-mass budget of the universe is crucial to
validate or invalidate our standard cosmological model.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:47:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nicastro",
"F.",
""
],
[
"Mathur",
"Smita",
""
],
[
"Elvis",
"Martin",
""
]
] | [
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] |
712.2376 | Johannes Voss | Johannes Voss and Daniela Pfannkuche | Electron spin relaxation in GaAs quantum dot systems - The role of the
hyperfine interaction | 14 pages, 10 figures | null | null | null | cond-mat.mes-hall cond-mat.other | null | We present numerical results for electron spin relaxation rates for single
and laterally coupled double GaAs quantum dots in a perpendicular magnetic
field. As source of spin relaxation we consider hyperfine interaction with the
nuclear spins in the GaAs substrate. Due to the differences in the energy
scales of the nuclear and electronic Zeeman energies, the phonon bath system
has to be taken into account for energy dissipation. The corresponding
transition rates of second order show strong dependencies on correlations
between the electrons and the electronic energy differences, and hence on the
magnetic field. For a highly asymmetric double dot we have found a relatively
low second order electron spin relaxation rate for a wide range of magnetic
fields.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:48:30 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Voss",
"Johannes",
""
],
[
"Pfannkuche",
"Daniela",
""
]
] | [
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712.2377 | Ettore Vicari | Andrea Pelissetto, Ettore Vicari | High-order perturbative expansions of multi-parameter Phi^4 quantum
field theories | 12 pages | null | null | null | hep-th cond-mat.stat-mech | null | We present high-order pertubative expansions of multi-parameter Phi^4 quantum
field theories with an N-component fundamental field, containing up to
4th-order polynomials of the field. Multi-parameter Phi^4 theories generalize
the simplest O(N)-symmetric Phi^4 theories, and describe more complicated
symmetry breaking patterns. These notes collect several high-order perturbative
series of physically interesting multi-parameter Phi^4 theories, to five or six
loops. We consider the O(M)XO(N)-symmetric Phi^4 model, the so-called MN model,
and a spin-density-wave Phi^4 model containing five quartic terms.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:48:32 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Pelissetto",
"Andrea",
""
],
[
"Vicari",
"Ettore",
""
]
] | [
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] |
712.2378 | Alexander Gutman | A. E. Gutman, A. G. Kusraev, S. S. Kutateladze | The Wickstead Problem | 44 pages; copyright statements are changed; some typos are corrected;
item A3.9 is subdivided into two items and some remarks are added therein;
the references section is corrected and slightly extended; a footnote on a
foundation support is added | Siberian Electronic Math. Reports, 2008, V.5, 293-333 | null | null | math.FA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In 1977 Anthony Wickstead raised the question of the conditions for all band
preserving linear operators to be order bounded in a vector lattice. This
article overviews the main ideas and results on the Wickstead problem and its
variations, focusing primarily on the case of band preserving operators in a
universally complete vector lattice.
| [
{
"version": "v1",
"created": "Fri, 14 Dec 2007 15:49:55 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 09:24:12 GMT"
},
{
"version": "v3",
"created": "Wed, 2 Jul 2008 08:24:24 GMT"
},
{
"version": "v4",
"created": "Sat, 13 Dec 2008 16:03:29 GMT"
}
] | 2011-05-31T00:00:00 | [
[
"Gutman",
"A. E.",
""
],
[
"Kusraev",
"A. G.",
""
],
[
"Kutateladze",
"S. S.",
""
]
] | [
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