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801.1973 | Michael Ivanov A | Michael A. Ivanov | A non-universal transition to asymptotic freedom in low-energy quantum
gravity | 8 pages, 6 figures, Latex | Journal of Gravitational Physics, 2008, vol.2, No.2, pp. 26-31 | null | null | hep-th gr-qc quant-ph | null | The model of low-energy quantum gravity by the author has the property of
asymptotic freedom at very short distances. The character of transition to
asymptotic freedom is studied here. It is shown that this transition is not
universal, but the one obeys the scaling rule: the range of this transition in
units of $r/E^{1/2}$, where $r$ is a distance between particles and $E$ is an
energy of the screening particle, is the same for any micro-particle. This
range for a proton is between $10^{-11} - 10^{-13}$ meter, while for an
electron it is approximately between $10^{-13} - 10^{-15}$ meter.
| [
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"version": "v1",
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801.1974 | Georg Weiglein | S. Heinemeyer, V.A. Khoze, M. Ryskin, W. Stirling, M. Tasevsky and G.
Weiglein | Central Exclusive Diffractive MSSM Higgs-Boson Production at the LHC | 5 pages, to appear in the proceedings of EPS07 | J.Phys.Conf.Ser.110:072016,2008 | 10.1088/1742-6596/110/7/072016 | IPPP/07/86, DCPT/07/172 | hep-ph | null | The prospects for central exclusive diffractive (CED) production of MSSM
Higgs bosons at the LHC are reviewed. It is shown that the CED channels, making
use of forward proton detectors at the LHC installed at 220 m and 420 m
distance around ATLAS and / or CMS, can provide important information on the
Higgs sector of the MSSM. In particular, CED production of the neutral CP-even
Higgs bosons h and H and their decays into bottom quarks has the potential to
probe interesting regions of the M_A--tan_beta parameter plane of the MSSM and
may give access to the bottom Yukawa couplings of the Higgs bosons up to masses
of M_H \approx 250 GeV.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 18:05:26 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Heinemeyer",
"S.",
""
],
[
"Khoze",
"V. A.",
""
],
[
"Ryskin",
"M.",
""
],
[
"Stirling",
"W.",
""
],
[
"Tasevsky",
"M.",
""
],
[
"Weiglein",
"G.",
""
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801.1975 | Alexander Moskvin | A.S. Moskvin, Yu.D. Panov, and S.-L. Drechsler | Nonrelativistic Multiferroicity in the Nonstoichiometric Spin s=1/2
Spiral Chain Cuprate LiCu2O2 | 4 pages, 4 figures | null | 10.1103/PhysRevB.79.104112 | null | cond-mat.str-el cond-mat.mtrl-sci | null | We argue for a recently observed puzzling multiferroic behavior in s=1/2 1D
chain cuprate LiCu2O2 with edge-shared arrangement of CuO4 plaquettes and
incommensurate spiral spin ordering can be consistently explained if one takes
into account the nonrelativistic exchange-induced electric polarization on the
Cu2+ centers substituting for the positions native for the Cu1+ ions. These
substituent centers are proved to be an effective probe of the spin
incommensurability and magnetic field effects.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 18:17:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Moskvin",
"A. S.",
""
],
[
"Panov",
"Yu. D.",
""
],
[
"Drechsler",
"S. -L.",
""
]
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] |
801.1976 | Milan Janjic | Milan Janjic | An Enumerative Function | null | null | null | null | math.CO | null | We define an enumerative function F(n,k,P,m) which is a generalization of
binomial coefficients. Special cases of this function are also power function,
factorials, rising factorials and falling factorials.
The first section of the paper is an introduction.
In the second section we derive an explicit formula for F. From the
expression for the power function we obtain a number theory result.
Then we derive a formula which shows that the case of arbitrary m may be
reduced to the case m=0. This formula extends Vandermonde convolution.
In the second section we describe F by the series of recurrence relations
with respect to each of arguments k, n, and P. As a special case of the first
recurrence relation we state a binomial identity. As a consequence of the
second recurrence relation we obtain relation for coefficients of Chebyshev
polynomial of both kind. This means that these polynomials might be defined in
pure combinatorial way.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 18:43:46 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jan 2008 16:52:46 GMT"
}
] | 2008-01-19T00:00:00 | [
[
"Janjic",
"Milan",
""
]
] | [
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] |
801.1977 | Grzegorz Michalek | G. Michalek, N. Gopalswamy, S. Yashiro | Space Weather Application Using Projected Velocity Asymmetry of Halo
CMEs | accepted for [publication in Solar Physics | null | 10.1007/s11207-008-9126-7 | null | astro-ph | null | Halo coronal mass ejections (HCMEs) originating from regions close to the
center of the Sun are likely to be responsible for severe geomagnetic storms.
It is important to predict geo-effectiveness of HCMEs using observations when
they are still near the Sun. Unfortunately, coronagraphic observations do not
provide true speeds of CMEs due to the projection effects. In the present
paper, we present a new technique allowing estimate the space speed and
approximate source location using projected speeds measured at different
position angles for a given HCME (velocity asymmetry). We apply this technique
to HCMEs observed during 2001-2002 and find that the improved speeds are better
correlated with the travel times of HCMEs to Earth and with the magnitudes
ensuing geomagnetic storms.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 18:45:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Michalek",
"G.",
""
],
[
"Gopalswamy",
"N.",
""
],
[
"Yashiro",
"S.",
""
]
] | [
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] |
801.1978 | Galina L. Klimchitskaya | G. L. Klimchitskaya, V. M. Mostepanenko | Conductivity of dielectric and thermal atom-wall interaction | 4 pages, 2 figures; page size is corrected | J. Phys. A: Math. Theor. v.41, 312002(F), 2008. | 10.1088/1751-8113/41/31/312002 | null | quant-ph cond-mat.stat-mech physics.optics | null | We compare the experimental data of the first measurement of a temperature
dependence of the Casimir-Polder force by Obrecht et al. [Phys. Rev. Lett. {\bf
98}, 063201 (2007)] with the theory taking into account small, but physically
real, static conductivity of the dielectric substrate. The theory is found to
be inconsistent with the data. The conclusion is drawn that the conductivity of
dielectric materials should not be included in the model of the dielectric
response in the Lifshitz theory. This conclusion obtained from the long
separation measurement is consistent with related but different results
obtained for semiconductors and metals at short separations.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 18:48:14 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jan 2008 21:57:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Klimchitskaya",
"G. L.",
""
],
[
"Mostepanenko",
"V. M.",
""
]
] | [
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] |
801.1979 | Gregory Gutin | G. Gutin, I. Razgon, E.J. Kim | Minimum Leaf Out-branching and Related Problems | The main change is a quadratic kernel derivation | null | null | null | cs.DS cs.DM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Given a digraph $D$, the Minimum Leaf Out-Branching problem (MinLOB) is the
problem of finding in $D$ an out-branching with the minimum possible number of
leaves, i.e., vertices of out-degree 0. We prove that MinLOB is polynomial-time
solvable for acyclic digraphs. In general, MinLOB is NP-hard and we consider
three parameterizations of MinLOB. We prove that two of them are NP-complete
for every value of the parameter, but the third one is fixed-parameter
tractable (FPT). The FPT parametrization is as follows: given a digraph $D$ of
order $n$ and a positive integral parameter $k$, check whether $D$ contains an
out-branching with at most $n-k$ leaves (and find such an out-branching if it
exists). We find a problem kernel of order $O(k^2)$ and construct an algorithm
of running time $O(2^{O(k\log k)}+n^6),$ which is an `additive' FPT algorithm.
We also consider transformations from two related problems, the minimum path
covering and the maximum internal out-tree problems into MinLOB, which imply
that some parameterizations of the two problems are FPT as well.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 19:33:29 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Jan 2008 17:41:09 GMT"
},
{
"version": "v3",
"created": "Tue, 14 Oct 2008 20:51:12 GMT"
}
] | 2008-10-14T00:00:00 | [
[
"Gutin",
"G.",
""
],
[
"Razgon",
"I.",
""
],
[
"Kim",
"E. J.",
""
]
] | [
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801.198 | Michael Trusov | I.M.Narodetskii, M.A.Trusov, A.I.Veselov | Charm and bottom baryons in nonperturbative quark dynamics | Contributed talk at the session of Russian Academy of Sciences
"Physics of Fundamental Interactions", ITEP, Moscow, November 26-30, 2007 | Phys.Atom.Nucl.72:536-540,2009 | 10.1134/S1063778809030193 | null | hep-ph | null | We use the Field Correlator Method in QCD to calculate the masses of
$\Sigma_c$, $\Xi_c$ and recently observed $\Sigma_b$, $\Xi_b$ baryons and their
orbital excitations.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 19:47:02 GMT"
}
] | 2009-04-17T00:00:00 | [
[
"Narodetskii",
"I. M.",
""
],
[
"Trusov",
"M. A.",
""
],
[
"Veselov",
"A. I.",
""
]
] | [
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] |
801.1981 | Andrey O. Matveev | Andrey O. Matveev | Neighboring Fractions in Farey Subsequences | 14 pages; v.2,3 - misprints in Corollary 2.3(ii) and Remark 4.1(iii)
corrected; v.4 - minor improvements; v.5 - new Section 2 and references
added. | null | null | null | math.NT math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present explicit formulas for the computation of the neighbors of several
elements of Farey subsequences.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 20:02:36 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jan 2008 22:23:09 GMT"
},
{
"version": "v3",
"created": "Sat, 23 Feb 2008 19:07:40 GMT"
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{
"version": "v4",
"created": "Sun, 30 Nov 2008 12:14:36 GMT"
},
{
"version": "v5",
"created": "Mon, 10 May 2010 16:25:45 GMT"
}
] | 2010-05-11T00:00:00 | [
[
"Matveev",
"Andrey O.",
""
]
] | [
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] |
801.1982 | Luciano da Fontoura Costa | Luciano da Fontoura Costa | Inward and Outward Node Accessibility in Complex Networks as Revealed by
Non-Linear Dynamics | null | null | null | null | physics.soc-ph cond-mat.dis-nn | null | In this work, the outward and inward accessibilities of individual nodes are
defined and their potential for application is illustrated with respect to the
investigation of 6 different types of networks. The outward accessibility
quantifies the potential of an individual node for accessing other nodes
through random walks. The inward accessibility measures the potential of a
given node of being accessed by other nodes. Both the inward and outward
accessibilities are measured with respect to successive time steps along the
walks, providing an interesting means for the characterization of the transient
non-linear dynamics of accessibility. Self-avoiding walks are considered here
because they are more purposive and necessarily finite (unlike traditional
random walks). The results include the identification of the fact that the
inward values tend to be much smaller than the outward values, the tendency of
the inward accessibility to be highly correlated with the node degree while the
outward values are mostly uncorrelated with that measurements, the distinct
behavior of the accessibility in geographical networks, the dominance of hubs
in scale free networks, as well as the enhanced uniformity of the
accessibilities for the path-regular model. Also investigated was the
possibility to predict the accessibility of a given node in terms of its
respective degree. The concepts of inward and outward accessibility, as well as
the several obtained results, have several implications and potential for
applications to several real-time problems including disease spreading, WWW
surfing, protein interaction, cortical networks and network attacks, among
others.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 20:46:44 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Costa",
"Luciano da Fontoura",
""
]
] | [
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] |
801.1983 | Tien-Cuong Dinh | Tien-Cuong Dinh, Viet-Anh Nguyen and Nessim Sibony | Exponential estimates for plurisubharmonic functions and stochastic
dynamics | 24 pages, theorem and references added | null | null | null | math.CV math.DS | null | We prove exponential estimates for plurisubharmonic functions with respect to
Monge-Ampere measures with Holder continuous potential. As an application, we
obtain several stochastic properties for the equilibrium measures associated to
holomorphic maps on projective spaces. More precisely, we prove the exponential
decay of correlations, the central limit theorem for general d.s.h.
observables, and the large deviations theorem for bounded d.s.h. observables
and Holder continuous observables.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 20:55:50 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Mar 2008 20:51:46 GMT"
}
] | 2008-03-04T00:00:00 | [
[
"Dinh",
"Tien-Cuong",
""
],
[
"Nguyen",
"Viet-Anh",
""
],
[
"Sibony",
"Nessim",
""
]
] | [
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] |
801.1984 | Emre Kahya Mr. | E. O. Kahya | A Decisive test to confirm or rule out the existence of dark matter
emulators using gravitational wave observations | 4 Pages, no figures, Contributed to 12th Annual Gravitational Wave
Data Analysis Workshop (GWDAW-12 2007): Connecting Gravitational Waves with
Observational Astrophysics, Cambridge, Massachusetts, 13-16 Dec 2007 | Class.Quant.Grav.25:184008,2008 | 10.1088/0264-9381/25/18/184008 | UFIFT-QG-08-01 | gr-qc astro-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider stable modified theories of gravity that reproduce galactic
rotation curves and the observed amount of weak lensing without dark matter. In
any such model gravity waves follow a different geodesic from that of other
massless particles. For a specific class of models which we call "dark matter
emulators," over cosmological distances this results in an easily detectable
and difference between the arrival times of the pulse of gravity waves from
some cosmic event and those of photons or neutrinos. For a repeat of SN 1987a
(which took place in the Large Magellanic Cloud) the time lag is in the range
of days. For the recent gamma ray burst, GRB 070201 (which seems to have taken
place on the edge of the Andromeda galaxy) the time lag would be in the range
of about two years.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 21:00:08 GMT"
},
{
"version": "v2",
"created": "Sun, 19 Oct 2008 15:04:33 GMT"
}
] | 2008-11-07T00:00:00 | [
[
"Kahya",
"E. O.",
""
]
] | [
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801.1985 | Constantinos Skordis | Constantinos Skordis | Generalizing TeVeS Cosmology | 12 pages | Phys.Rev.D77:123502,2008 | 10.1103/PhysRevD.77.123502 | pi-cosmo-70 | astro-ph | null | I consider an extented version of Bekenstein's Tensor-Vector-Scalar theory
where the action of the vector field is of a general Einstein-Ether form. This
work presents the cosmological equations of this theory, both at the background
and perturbed level, for scalar, vector and tensor perturbation modes. By
solving the background equations in the radiation era analytically, to an
excellent approximation, I construct the primordial adiabatic perturbation for
a general family of scalar field kinetic functions.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 21:11:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Skordis",
"Constantinos",
""
]
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] |
801.1986 | Karl-Heinz Kampert | Karl-Heinz Kampert | Ultra High-Energy Cosmic Ray Observations | 9 pages, 8 figures, Invited paper presented at TAUP 2007 (Sendai,
Japan), to appear in Journal of Physics | J.Phys.Conf.Ser.120:062002,2008 | 10.1088/1742-6596/120/6/062002 | null | astro-ph | null | The year 2007 has furnished us with outstanding results about the origin of
the most energetic cosmic rays: a flux suppression as expected from the
GZK-effect has been observed in the data of the HiRes and Auger experiments and
correlations between the positions of nearby AGN and the arrival directions of
trans-GZK events have been observed by the Pierre Auger Observatory. The latter
finding marks the beginning of ultra high-energy cosmic ray astronomy and is
considered a major breakthrough starting to shed first light onto the sources
of the most extreme particles in nature. This report summarizes those
observations and includes other major advances of the field, mostly presented
at the 30th International Cosmic Ray Conference held in Merida, Mexico, in July
2007. With increasing statistics becoming available from current and even
terminated experiments, systematic differences amongst different experiments
and techniques can be studied in detail which is hoped to improve our
understanding of experimental techniques and their limitations.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 21:46:40 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Kampert",
"Karl-Heinz",
""
]
] | [
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] |
801.1987 | Neal E. Young | Christos Koufogiannakis and Neal E. Young | A Nearly Linear-Time PTAS for Explicit Fractional Packing and Covering
Linear Programs | corrected version of FOCS 2007 paper: 10.1109/FOCS.2007.62. Accepted
to Algorithmica, 2013 | Algorithmica 70(4):648-674(2014) | 10.1007/s00453-013-9771-6 | null | cs.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give an approximation algorithm for packing and covering linear programs
(linear programs with non-negative coefficients). Given a constraint matrix
with n non-zeros, r rows, and c columns, the algorithm computes feasible primal
and dual solutions whose costs are within a factor of 1+eps of the optimal cost
in time O((r+c)log(n)/eps^2 + n).
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 22:04:49 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Mar 2013 16:03:10 GMT"
}
] | 2015-06-02T00:00:00 | [
[
"Koufogiannakis",
"Christos",
""
],
[
"Young",
"Neal E.",
""
]
] | [
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] |
801.1988 | Andras Lorincz | Istvan Szita and Andras Lorincz | Online variants of the cross-entropy method | 8 pages | null | null | null | cs.LG | null | The cross-entropy method is a simple but efficient method for global
optimization. In this paper we provide two online variants of the basic CEM,
together with a proof of convergence.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 06:56:42 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Szita",
"Istvan",
""
],
[
"Lorincz",
"Andras",
""
]
] | [
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] |
801.1989 | Chiu Fan Lee | Chiu Fan Lee | Density functional methods for polymers: a coil-globule transition case
study | null | null | null | null | cond-mat.soft cond-mat.stat-mech | null | We consider a free energy functional on the monomer density function that is
suitable for the study of coil-globule transition. We demonstrate, with
explicitly stated assumptions, why the entropic contribution is in the form of
the Kullback-Leibler distance, and that the energy contribution is given by
two-body and three-body terms. We then solve for the free energy analytically
on a set of trial density functions, and reproduce de Gennes' classical theory
on polymer coil-globule transition. We then discuss how our formalism can be
applied to study polymer dynamics from the perspective of dynamical density
function theory.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 23:42:44 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 22:23:35 GMT"
},
{
"version": "v3",
"created": "Fri, 18 Jan 2008 17:46:51 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Lee",
"Chiu Fan",
""
]
] | [
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] |
801.199 | Daniel Valdez-Balderas | Daniel Valdez-Balderas and David Stroud | Effects of inhomogeneities and thermal fluctuations on the spectral
function of a model d-wave superconductor | Accepted for publication in Phys. Rev. B. Scheduled Issue: 01 Jan
2008. 26 Pages and 10 figures | null | 10.1103/PhysRevB.77.014515 | null | cond-mat.supr-con cond-mat.mes-hall | null | We compute the spectral function $A({\bf k}, \omega)$ of a model
two-dimensional high-temperature superconductor, at both zero and finite
temperatures $T$. We assume that an areal fraction $c_{\beta}$ of the
superconductor has a large gap $\Delta$ ($\beta$ regions), while the rest has a
smaller $\Delta$ ($\alpha$ regions), both of which are randomly distributed in
space. We find that $A({\bf k}, \omega)$ is most strongly affected by
inhomogeneity near the point $\mathbf k = (\pi, 0)$ (and the symmetry-related
points). For $c_\beta\simeq 0.5$, $A({\bf k}, \omega)$ exhibits two double
peaks (at positive and negative energy) near this k-point if the difference
between $\Delta_\alpha$ and $\Delta_\beta$ is sufficiently large in comparison
to the hopping integral. The strength of the inhomogeneity required to produce
a split spectral function peak suggests that inhomogeneity is unlikely to be
the cause of a second branch in the dispersion relation. Thermal fluctuations
also affect $A({\bf k}, \omega)$ most strongly near $\mathbf k = (\pi,0)$.
Typically, peaks that are sharp at $T = 0$ become reduced in height, broadened,
and shifted toward lower energies with increasing $T$; the spectral weight near
$\mathbf k = (\pi, 0)$ becomes substantial at zero energy for $T$ greater than
the phase-ordering temperature.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 23:13:29 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Valdez-Balderas",
"Daniel",
""
],
[
"Stroud",
"David",
""
]
] | [
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] |
801.1991 | Bhagawan Sahu | Bhagawan Sahu, Hongki Min, Allan. H. MacDonald, Sanjay K. Banerjee | Energy gaps, magnetism, and electric field effects in bilayer graphene
nanoribbons | 8 pages, 8 figures (contents and figures changed) | Phys. Rev. B 78, 045404 (2008) | 10.1103/PhysRevB.78.045404 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using a first principles density functional electronic structure method, we
study the energy gaps and magnetism in bilayer graphene nanoribbons as a
function of the ribbon width and the strength of an external electric field
between the layers. We assume AB (Bernal) stacking and consider both armchair
and zigzag edges and two edge alignments distinguished by a 60$^o$ rotation of
one layer with respect to the other. Armchair ribbons exhibit three classes of
bilayer gaps which decrease with increasing ribbon width. An external electric
field between the layers increases the gap in narrow ribbons and decreases the
gap for wide ribbons, a property which can be understood semi-analytically
using a $\pi$-band tight-binding model and perturbation theory. The magnetic
properties of zigzag edge ribbons are different for the two different edge
alignments, and not robust for all exchange-correlation approximations
considered. Bilayer ribbon gaps are sensitive to the presence or absence of
magnetism.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 23:14:19 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 21:32:30 GMT"
},
{
"version": "v3",
"created": "Wed, 2 Jul 2008 17:20:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sahu",
"Bhagawan",
""
],
[
"Min",
"Hongki",
""
],
[
"MacDonald",
"Allan. H.",
""
],
[
"Banerjee",
"Sanjay K.",
""
]
] | [
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] |
801.1992 | David Pask | T. Bates and D. A. Pask | C*-algebras of labelled graphs II - Simplicity results | 18 pages, 4 figures | null | null | null | math.OA math.DS | null | We prove simplicity and pure infiniteness results for a certain class of
labelled graph $C^*$-algebras. We show, by example, that this class of unital
labelled graph $C^*$-algebras is strictly larger than the class of unital graph
$C^*$-algebras.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 23:32:37 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Bates",
"T.",
""
],
[
"Pask",
"D. A.",
""
]
] | [
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] |
801.1993 | Boris Solomyak | Richard Kenyon, Boris Solomyak | On the characterization of expansion maps for self-affine tilings | Revised version. A typo corrected (after publication!) in the
definition of the set $\Omega$ at the bottom of p.13 | Discrete Comput. Geom. (2010) 43: 577-593 | null | null | math.MG math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider self-affine tilings in $\R^n$ with expansion matrix $\phi$ and
address the question which matrices $\phi$ can arise this way. In one
dimension, $\lambda$ is an expansion factor of a self-affine tiling if and only
if $|\lambda|$ is a Perron number, by a result of Lind. In two dimensions, when
$\phi$ is a similarity, we can speak of a complex expansion factor, and there
is an analogous necessary condition, due to Thurston: if a complex $\lambda$ is
an expansion factor of a self-similar tiling, then it is a complex Perron
number. We establish a necessary condition for $\phi$ to be an expansion matrix
for any $n$, assuming only that $\phi$ is diagonalizable over the complex
numbers. We conjecture that this condition on $\phi$ is also sufficient for the
existence of a self-affine tiling.
| [
{
"version": "v1",
"created": "Sun, 13 Jan 2008 23:56:34 GMT"
},
{
"version": "v2",
"created": "Sun, 4 Apr 2010 20:44:35 GMT"
}
] | 2011-07-20T00:00:00 | [
[
"Kenyon",
"Richard",
""
],
[
"Solomyak",
"Boris",
""
]
] | [
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801.1994 | Victor Flambaum | V.V. Flambaum | Variation of fundamental constants in space and time: theory and
observations | Proceeding of ACFC, BadHonnef, 2007: to be published in EPJ | Eur.Phys.J.ST 163:159-171,2008 | 10.1140/epjst/e2008-00817-5 | null | nucl-th | null | Review of recent works devoted to the temporal and spatial variation of the
fundamental constants and dependence of the fundamental constants on the
gravitational potential (violation of local position invariance) is presented.
We discuss the variation of the fine structure constant $\alpha=e^2/\hbar c$,
strong interaction and fundamental masses (Higgs vacuum), e.g. the
electron-to-proton mass ratio $\mu=m_e/M_p$ or $X_e=m_e/\Lambda_{QCD}$ and
$X_q=m_q/\Lambda_{QCD}$. We also present new results from Big Bang
nucleosynthesis and Oklo natural nuclear reactor data and propose new
measurements of enhanced effects in atoms, nuclei and molecules, both in quasar
and laboratory spectra.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 00:17:46 GMT"
}
] | 2009-08-18T00:00:00 | [
[
"Flambaum",
"V. V.",
""
]
] | [
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801.1995 | Arjen van der Wel | Arjen van der Wel | The Dependence of Galaxy Morphology and Structure on Environment and
Stellar Mass | Accepted for publication in ApJ Letters, 5 pages, 5 figures. Minor
changes made to match published version | null | 10.1086/529432 | null | astro-ph | null | From the Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5), we extract a
sample of 4594 galaxies at redshifts 0.02<z<0.03, complete down to a stellar
mass of M=10^10 Msol. We quantify their structure (Sersic index), morphology
(Sersic index + ``Bumpiness''), and local environment. We show that morphology
and structure are intrinsically different galaxy properties, and we demonstrate
that this is a physically relevant distinction by showing that these properties
depend differently on galaxy mass and environment. Structure mainly depends on
galaxy mass whereas morphology mainly depends on environment. This is driven by
variations in star formation activity, as traced by color, which only weakly
affects the structure of a galaxy but strongly affects its morphological
appearance. The implication of our results is that the existence of the
morphology-density relation is intrinsic and not just due to a combination of
more fundamental, underlying relations. Our findings have consequences for
high-redshift studies, which often use some measure of structure as a proxy for
morphology. A direct comparison with local samples selected through visually
classified morphologies may lead to biases in the inferred evolution of the
morphological mix of the galaxy population, and misinterpretations in terms of
how galaxy evolution depends on mass and environment.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 00:20:42 GMT"
},
{
"version": "v2",
"created": "Thu, 31 Jan 2008 20:45:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"van der Wel",
"Arjen",
""
]
] | [
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] |
801.1996 | Yue Shen | Yue Shen, B. T. Draine, Eric T. Johnson (Princeton) | Modeling Porous Dust Grains with Ballistic Aggregates I: Geometry and
Optical Properties | Updated calculations and references; conclusions unchanged; ApJ in
press | Astrophys.J. 689 (2008) 260-275 | 10.1086/592765 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the scattering and absorption of light by random ballistic
aggregates of spherical monomers. We present a general measure for the porosity
of an irregular particle. Three different classes of ballistic aggregates are
considered, with different degrees of porosity. Scattering and absorption cross
sections are calculated, using the discrete dipole approximation (DDA), for
grains of three compositions (50% silicate and 50% graphite; 50% silicate and
50% amorphous carbon; and 100% silicate), for wavelengths from 0.1 micron to 4
micron. For fixed particle mass, increased porosity increases the extinction at
short wavelengths, but decreases the extinction at wavelengths long compared to
the overall aggregate size. Scattering and absorption cross sections are
insensitive to monomer size as long as the constituent monomers are small
compared with the incident wavelength. We compare our accurate DDA results with
two other approximations: the analytical multi-layer sphere (MLS) model and
effective medium theory (EMT). For high porosity and/or absorptive materials,
the MLS model does not provide a good approximation for scattering and
absorption by ballistic aggregates. The EMT method provides a much better
approximation than the MLS model for these aggregates, with a typical
difference less than 20% in extinction and scattering cross sections compared
with DDA results, for all types, compositions and wavelengths probed in this
study.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 01:15:01 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Aug 2008 03:27:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shen",
"Yue",
"",
"Princeton"
],
[
"Draine",
"B. T.",
"",
"Princeton"
],
[
"Johnson",
"Eric T.",
"",
"Princeton"
]
] | [
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] |
801.1997 | Galyna Dobrovolska | G. Dobrovolska, P. Etingof | An upper bound for the lower central series quotients of a free
associative algebra | 7 pages; introduction expanded | null | null | null | math.RA math.RT | null | Feigin and Shoikhet conjectured in math/0610410 that successive quotients
$B_m(A_n)$ of the lower central series filtration of a free associative algebra
$A_n$ have polynomial growth. In this paper we give a proof of this conjecture,
using the structure of $W_n$-representation on $B_m(A_n)$ which was defined in
math/0610410 . We also prove that the number of squares in a Young diagram $D$
corresponding to an irreducible $W_n$-module in the Jordan-Holder series of
$B_m(A_n)$ is bounded above by the integer $(m-1)^2+2[(n-2)/2](m-1)$. This
bound combined with MAGMA computations by Rains in math/0610410 allows us to
confirm the $W_n$-module structure of $B_3(A_3)$ conjectured in math/0610410 .
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 01:14:02 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Mar 2008 18:17:44 GMT"
}
] | 2008-03-27T00:00:00 | [
[
"Dobrovolska",
"G.",
""
],
[
"Etingof",
"P.",
""
]
] | [
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] |
801.1998 | James Atkinson | James Atkinson | Backlund transformations for integrable lattice equations | 9 pages | null | 10.1088/1751-8113/41/13/135202 | null | nlin.SI | null | We give new Backlund transformations (BTs) for some known integrable (in the
sense of being multidimensionally consistent) quadrilateral lattice equations.
As opposed to the natural auto-BT inherent in every such equation, these BTs
are of two other kinds. Specifically, it is found that some equations admit
additional auto-BTs (with Backlund parameter), whilst some pairs of apparently
distinct equations admit a BT which connects them.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 01:25:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Atkinson",
"James",
""
]
] | [
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] |
801.1999 | Wolfgang Staubach | Wilhelm Schlag, Avy Soffer, Wolfgang Staubach | Decay for the wave and Schroedinger evolutions on manifolds with conical
ends, Part I | 32 pages, This paper differs in terms of both generalizations and
improvement of the exposition from the paper "Decay estimates for the
Schroedinger evolution on asymptotically conic surfaces of revolution, Part
I", and is therefore posted as a new paper | null | null | null | math.AP math-ph math.MP | null | Global in time dispersive estimates for the Schroedinger and wave evolutions
are obtained on manifolds with conical ends whose Hamiltonian flow exhibits
trapping. This paper deals with the case of initial data with "zero angular
momentum".
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 01:36:45 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Schlag",
"Wilhelm",
""
],
[
"Soffer",
"Avy",
""
],
[
"Staubach",
"Wolfgang",
""
]
] | [
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] |
801.2 | Qingjun Liu | Qing-Jun Liu and Wei-Qin Zhao | Elastic parton scattering and non-statistical event-by-event mean-pt
fluctuations in Au + Au collisions at RHIC | 6 pages, 3 figures | Phys.Rev.C77:034902,2008 | 10.1103/PhysRevC.77.034902 | null | nucl-th | null | Non-statistical event-by-event mean-pt fluctuations in Au + Au collisions at
sqrt(s_NN) = 130 and 200 GeV are analyzed in AMPT with string-melting, and the
results are compared with STAR data. The analysis suggests that in-medium
elastic parton scattering may contribute greatly to the mean-p_t fluctuations
in relativistic heavy-ion collisions. Furthermore, it is demonstrated that
non-statistical event-by-event mean-pt fluctuations can be used to probe the
initial partonic dynamics in these collisions. The comparison shows that with
an in-medium elastic parton scattering cross section sigma_p=10 mb, AMPT with
string-melting can well reproduce sqrt(s_NN) = 130 GeV data on the centrality
dependence of non-statistical event-by-event mean-pt fluctuations. The
comparison also shows that the fluctuation data for sqrt(s_NN) = 200 GeV Au +
Au collisions can be well reproduced with sigma_p between 6 and 10 mb.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 01:58:19 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Liu",
"Qing-Jun",
""
],
[
"Zhao",
"Wei-Qin",
""
]
] | [
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] |
801.2001 | Wolfgang Staubach | Wilhelm Schlag, Avy Soffer, Wolfgang Staubach | Decay for the wave and Schroedinger evolutions on manifolds with conical
ends, Part II | 28 pages | null | null | null | math.AP math-ph math.MP | null | Global in time dispersive estimates for the Schroedinger and wave evolutions
are obtained on manifolds with conical ends whose Hamiltonian flow exhibits
trapping. This paper deals with the case of initial data with fixed "nonzero
angular momentum".
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 01:40:33 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Schlag",
"Wilhelm",
""
],
[
"Soffer",
"Avy",
""
],
[
"Staubach",
"Wolfgang",
""
]
] | [
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] |
801.2002 | Nirav Mehta | N. P. Mehta, Seth T. Rittenhouse, J. P. D'Incao, Chris H. Greene | Efimov states embedded in the three-body continuum | 4 pages 3 figures | Phys. Rev. A 78, 020701 (2008) | 10.1103/PhysRevA.78.020701 | null | cond-mat.other | null | We consider a multichannel generalization of the Fermi pseudopotential to
model low-energy atom-atom interactions near a magnetically tunable Feshbach
resonance, and calculate the adiabatic hyperspherical potential curves for a
system of three such interacting atoms. In particular, our model suggests the
existence of a series of quasi-bound Efimov states attached to excited
three-body thresholds, far above open channel collision energies. We discuss
the conditions under which such states may be supported, and identify which
interaction parameters limit the lifetime of these states. We speculate that it
may be possible to observe these states using spectroscopic methods, perhaps
allowing for the measurement of multiple Efimov resonances for the first time.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 02:25:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mehta",
"N. P.",
""
],
[
"Rittenhouse",
"Seth T.",
""
],
[
"D'Incao",
"J. P.",
""
],
[
"Greene",
"Chris H.",
""
]
] | [
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] |
801.2003 | Max Spolaor | Max Spolaor (1), Duncan A. Forbes (1), George K. T. Hau (1,2), Robert
N. Proctor (1), Sarah Brough (1) ((1) Centre for Astrophysics and
Supercomputing, Swinburne University of Technology, (2) Department of
Physics, University of Durham) | The early-type galaxies NGC 1407 and NGC 1400 - I: spatially resolved
radial kinematics and surface photometry | 11 pages, 6 tables, 6 figures, Accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12891.x | null | astro-ph | null | This is the first paper of a series focused on investigating the star
formation and evolutionary history of the two early-type galaxies NGC 1407 and
NGC 1400. They are the two brightest galaxies of the NGC 1407 (or Eridanus-A)
group, one of the 60 groups studied as part of the Group Evolution
Multi-wavelength Study (GEMS). Here we present new high signal-to-noise
long-slit spectroscopic data obtained at the ESO 3.6m telescope and
high-resolution multi-band imaging data from the HST/ACS and wide-field imaging
from Subaru Suprime-Cam. We spatially resolved integrated spectra out to 0.6
(NGC 1407) and 1.3 (NGC 1400) effective radii. The radial profiles of the
kinematic parameters v(rot), sigma, h3 and h4 are measured. The surface
brightness profiles are fitted to different galaxy light models and the colour
distributions analysed. The multi-band images are modelled to derive isophotal
shape parameters and residual galaxy images. The parameters from the surface
brightness profile fitting are used to estimate the mass of the possible
central supermassive black hole in NGC 1407. The galaxies are found to be
rotationally supported and to have a flat core in the surface brightness
profiles. Elliptical isophotes are observed at all radii and no fine structures
are detected in the residual galaxy images. From our results we can also
discard a possible interaction between NGC 1400, NGC 1407 and the group
intergalactic medium. We estimate a mass of 1.03x10^9 M(sun) for the
supermassive black hole in NGC 1407 galaxy.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 03:44:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Spolaor",
"Max",
""
],
[
"Forbes",
"Duncan A.",
""
],
[
"Hau",
"George K. T.",
""
],
[
"Proctor",
"Robert N.",
""
],
[
"Brough",
"Sarah",
""
]
] | [
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] |
801.2004 | Yanxia Zhang | Dan Gao, Yanxia Zhang and Yongheng Zhao | The Application of kd-tree in Astronomy | 4 pages, 3 tables, ADASS XVII conference | null | null | null | astro-ph | null | The basic idea of the kd-tree algorithm is to recursively partition a point
set P by hyperplanes, and to store the obtained partitioning in a binary tree.
Due to its immense popularity, many applications in astronomy have been
implemented. The algorithm can been used to solve a near neighbor problem for
cross-identification of huge catalogs and realize the classification of
astronomical objects. Since kd-tree can speed up query and partition spaces,
some approaches based on it have been applied for photometric redshift
measurement. We give the case studies of kd-tree in astronomy to show its
importance and performance.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 03:21:32 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Gao",
"Dan",
""
],
[
"Zhang",
"Yanxia",
""
],
[
"Zhao",
"Yongheng",
""
]
] | [
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] |
801.2005 | Max Spolaor | Max Spolaor (1), Duncan A. Forbes (1), Robert N. Proctor (1), George
K. T. Hau (1,2), Sarah Brough (1)((1) Centre for Astrophysics and
Supercomputing, Swinburne University, (2) Department of Physics, University
of Durham) | The early-type galaxies NGC 1407 and NGC 1400 - II: star formation and
chemical evolutionary history | 14 pages, 9 tables, 6 figures, Accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12892.x | null | astro-ph | null | We present a possible star formation and chemical evolutionary history for
two early-type galaxies NGC 1407 and NGC 1400. They are the two brightest
galaxies of the NGC 1407 (or Eridanus-A) group, one of the 60 groups studied as
part of the Group Evolution Multi-wavelength Study (GEMS). Our analysis is
based on new high signal-to-noise spatially resolved integrated spectra
obtained at the ESO 3.6m telescope, out to 0.6 (NGC 1407) and 1.3 (NGC 1400)
effective radii. Using Lick/IDS indices we estimate luminosity-weighted ages,
metallicities and $\alpha$-element abundance ratios. Colour radial
distributions from HST/ACS and Subaru Suprime-Cam multi-band wide-field imaging
are compared to colours predicted from spectroscopically determinated ages and
metallicities using single stellar population models. The galaxies formed over
half of their mass in a single short-lived burst of star formation (> 100
M(sun)/year) at redshift z>5. This likely involved an outside-in mechanism with
supernova-driven galactic winds, as suggested by the flatness of the
alpha-element radial profiles and the strong negative metallicity gradients.
Our results support the predictions of the revised version of the monolithic
collapse model for galaxy formation and evolution. We speculate that, since
formation the galaxies have evolved quiescently and that we are witnessing the
first infall of NGC 1400 in the group.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 03:49:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Spolaor",
"Max",
""
],
[
"Forbes",
"Duncan A.",
""
],
[
"Proctor",
"Robert N.",
""
],
[
"Hau",
"George K. T.",
""
],
[
"Brough",
"Sarah",
""
]
] | [
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] |
801.2006 | Jason Behrstock | Jason Behrstock, Bruce Kleiner, Yair Minsky, Lee Mosher | Geometry and rigidity of mapping class groups | Version 4, 98 pages. Cleaned up some notation involving the partial
order on subsurfaces (at the end of section 4). | null | null | null | math.GT math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the large scale geometry of mapping class groups MCG(S), using
hyperbolicity properties of curve complexes. We show that any self
quasi-isometry of MCG(S) (outside a few sporadic cases) is a bounded distance
away from a left-multiplication, and as a consequence obtain quasi-isometric
rigidity for MCG(S), namely that groups quasi-isometric to MCG(S) are virtually
equal to it. (The latter theorem was proved by Hamenstadt using different
methods). As part of our approach we obtain several other structural results: a
description of the tree-graded structure on the asymptotic cone of MCG(S); a
characterization of the image of the curve-complex projection map from MCG(S)
to the product of the curve complexes of essential subsurfaces of S; and a
construction of Sigma-hulls in MCG(S), an analogue of convex hulls.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 03:48:14 GMT"
},
{
"version": "v2",
"created": "Sat, 3 May 2008 18:19:08 GMT"
},
{
"version": "v3",
"created": "Mon, 23 Feb 2009 17:07:52 GMT"
},
{
"version": "v4",
"created": "Fri, 9 Apr 2010 18:09:43 GMT"
}
] | 2010-04-12T00:00:00 | [
[
"Behrstock",
"Jason",
""
],
[
"Kleiner",
"Bruce",
""
],
[
"Minsky",
"Yair",
""
],
[
"Mosher",
"Lee",
""
]
] | [
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0.010942338,
-0.0066069392,
-0.0314640887,
0.0083073499,
0.0065258127,
-0.0250518527,
-0.0747661516,
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0.0668741688,
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] |
801.2007 | Qiang Yuan | Qiang Yuan, Tong-Jie Zhang, Bao-Quan Wang | Reconstruction of Gas Temperature and Density Profiles of the Galaxy
Cluster RX J1347.5-1145 | 6 pages, 1 figure. The published version, 2008, Chin. J. Astron.
Astrophys., 8, 671 | Chin.J.Astron.Astrophys.8:671-676, 2008 | 10.1088/1009-9271/8/6/05 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We use observations of Sunyaev-Zel'dovich effect and X-ray surface brightness
to reconstruct the radial profiles of gas temperature and density under the
assumption of a spherically symmetric distribution of the gas. The method of
reconstruction, first raised by Silk & White, depends directly on the
observations of the Sunyaev-Zel'dovich effect and the X-ray surface brightness,
without involving additional assumptions such as the equation of state of the
gas or the conditions of hydrostatic equilibrium. We applied this method to the
cluster RX J1347.5-1145, which has both the Sunyaev-Zel'dovich effect and X-ray
observations with relative high precision. It is shown that it will be an
effective method to obtain the gas distribution in galaxy clusters. Statistical
errors of the derived temperature and density profiles of gas were estimated
according to the observational uncertainties.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 03:42:23 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Mar 2008 11:39:17 GMT"
},
{
"version": "v3",
"created": "Sun, 14 Dec 2008 04:03:50 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Yuan",
"Qiang",
""
],
[
"Zhang",
"Tong-Jie",
""
],
[
"Wang",
"Bao-Quan",
""
]
] | [
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] |
801.2008 | Tiberiu Harko | C. S. J. Pun, L. \'A. Gergely, M. K. Mak, Z. Kov\'acs, G. M. Szab\'o,
T. Harko | Viscous dissipative Chaplygin gas dominated homogenous and isotropic
cosmological models | 14 pages, 9 figures, to appear in PRD | Phys.Rev.D77:063528,2008 | 10.1103/PhysRevD.77.063528 | null | gr-qc astro-ph hep-th | null | The generalized Chaplygin gas, which interpolates between a high density
relativistic era and a non-relativistic matter phase, is a popular dark energy
candidate. We consider a generalization of the Chaplygin gas model, by assuming
the presence of a bulk viscous type dissipative term in the effective
thermodynamic pressure of the gas. The dissipative effects are described by
using the truncated Israel-Stewart model, with the bulk viscosity coefficient
and the relaxation time functions of the energy density only. The corresponding
cosmological dynamics of the bulk viscous Chaplygin gas dominated universe is
considered in detail for a flat homogeneous isotropic
Friedmann-Robertson-Walker geometry. For different values of the model
parameters we consider the evolution of the cosmological parameters (scale
factor, energy density, Hubble function, deceleration parameter and luminosity
distance, respectively), by using both analytical and numerical methods. In the
large time limit the model describes an accelerating universe, with the
effective negative pressure induced by the Chaplygin gas and the bulk viscous
pressure driving the acceleration. The theoretical predictions of the
luminosity distance of our model are compared with the observations of the type
Ia supernovae. The model fits well the recent supernova data. From the fitting
we determine both the equation of state of the Chaplygin gas, and the
parameters characterizing the bulk viscosity. The evolution of the scalar field
associated to the viscous Chaplygin fluid is also considered, and the
corresponding potential is obtained. Hence the viscous Chaplygin gas model
offers an effective dynamical possibility for replacing the cosmological
constant, and to explain the recent acceleration of the universe.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 03:52:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Pun",
"C. S. J.",
""
],
[
"Gergely",
"L. Á.",
""
],
[
"Mak",
"M. K.",
""
],
[
"Kovács",
"Z.",
""
],
[
"Szabó",
"G. M.",
""
],
[
"Harko",
"T.",
""
]
] | [
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] |
801.2009 | Athanasios Gentimis | Thanos Gentimis | On Limit Aperiodic G-Sets | 9 pages,0 figures | null | null | null | math.GN math.GR | null | We prove that the property to be limit aperiodic is preserved by the standard
construction with groups like extension, HNN extension and free product. We
also construct a non-limit aperiodic G-space.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 04:38:33 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Gentimis",
"Thanos",
""
]
] | [
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] |
801.201 | Dillon Mayhew | Rhiannon Hall and Dillon Mayhew | Contracting an element from a cocircuit | 23 pages, 1 figure. Minor changes to introduction | null | null | null | math.CO | null | We consider the situation that M and N are 3-connected matroids such that
|E(N)| > 3 and C* is a cocircuit of M with the property that M/y has an N-minor
for some y in C*. We show that either there is an element x in C* such that
si(M/x) or co(si(M/x)) is 3-connected with an N-minor, or there is a
four-element fan of M that contains two elements of C* and an element x such
that si(M/x) is 3-connected with an N-minor.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 04:48:59 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Apr 2008 05:44:11 GMT"
}
] | 2008-04-14T00:00:00 | [
[
"Hall",
"Rhiannon",
""
],
[
"Mayhew",
"Dillon",
""
]
] | [
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] |
801.2011 | C. Q. Geng | Chian-Shu Chen, Chao-Qiang Geng and Dmitry V. Zhuridov | Same-sign single dilepton productions at the LHC | 10 pages, 5 figures | Phys.Lett.B666:340-343,2008 | 10.1016/j.physletb.2008.07.088 | null | hep-ph | null | We examine the same-sign single dilepton productions of
$\ell_i^{\pm}\ell_j^{\pm} (\ell_{i,j}=e,\mu)$ in high-energy proton-proton
collisions at the Large Hadron Collider (LHC) in models with doubly charged
Higgs scalars as well as heavy Majorana neutrinos. We demonstrate that these
spectacular productions can be detected at the LHC for a class model in which
the doubly charged Higgs scalars couple only to the right-handed charged
leptons. The ranges of the possible doubly charged Higgs masses and mixings to
observe the processes at the LHC are discussed.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 04:50:15 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chen",
"Chian-Shu",
""
],
[
"Geng",
"Chao-Qiang",
""
],
[
"Zhuridov",
"Dmitry V.",
""
]
] | [
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] |
801.2012 | Taejung Kim | Taejung Kim | The linear flows in the space of Krichever-Lax matrices over an
algebraic curve | null | null | null | null | math.DS math.AG | null | In \cite{kri02}, I. M. Krichever invented the space of matrices parametrizing
the cotangent bundle of moduli space of stable vector bundles over a compact
Riemann surface, which is named as the Hitchin system after the investigation
\cite{hit87}. We study a necessary and sufficient condition for the linearity
of flows on the space of Krichever-Lax matrices in a Lax representation in
terms of cohomological classes using the similar technique and analysis from
the work \cite{grif85} by P. A. Griffiths.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 04:58:57 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Kim",
"Taejung",
""
]
] | [
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] |
801.2013 | Piotr Bizon | Piotr Bizo\'n | Huygens' principle and anomalously small radiation tails | 9 pages, for the proceedings of the Mathisson conference held in
Warsaw, 2007 | Acta Phys.Polon.Supp.1:77,2008 | null | null | math-ph gr-qc math.MP | null | This is a short account of recent joint work with T. Chmaj and A.
Rostworowski on asymptotic behavior of linear and nonlinear waves, as presented
at the conference devoted to Myron Mathisson held at the Banach Center, Warsaw
2007.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 05:17:25 GMT"
}
] | 2011-03-28T00:00:00 | [
[
"Bizoń",
"Piotr",
""
]
] | [
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] |
801.2014 | Matthew Ballard | Matthew Robert Ballard | Meet homological mirror symmetry | 34 pages. Published version. Comments still very welcome | Modular forms and string duality, 191--224, Fields Inst. Commun.,
54, Amer. Math. Soc., Providence, RI, 2008 | null | null | math.AG math.CT math.SG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, we introduce the interested reader to homological mirror
symmetry. After recalling a little background knowledge, we tackle the simplest
cases of homological mirror symmetry: curves of genus zero and one. We close by
outlining the current state of the field and mentioning what homo- logical
mirror symmetry has to say about other aspects of mirror symmetry.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 05:24:51 GMT"
},
{
"version": "v2",
"created": "Tue, 19 May 2009 17:42:24 GMT"
}
] | 2009-05-19T00:00:00 | [
[
"Ballard",
"Matthew Robert",
""
]
] | [
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] |
801.2015 | Takaya Nozawa | T. Nozawa, T. Kozasa, N. Tominaga, I. Sakon, M. Tanaka, T. Suzuki, K.
Nomoto, K. Maeda, H. Umeda, M. Limongi, T. Onaka | Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and
Temperature and Mass of the Dust | 25 pages including 6 figures and 1 table. Accepted for publication in
ApJ | null | 10.1086/589961 | null | astro-ph | null | SN 2006jc is a peculiar supernova (SN), in which the formation of dust has
been confirmed at an early epoch of ~50 days after the explosion. We
investigate the possibility of such an earlier formation of dust grains in the
expanding ejecta of SN 2006jc, applying the Type Ib SN model that is developed
to reproduce the observed light curve. We find that the rapid decrease of the
gas temperature in SN 2006jc enables the condensation of C grains in the C-rich
layer at 40-60 days after the explosion, which is followed by the condensation
of silicate and oxide grains until ~200 days. The average radius of each grain
species is confined to be less than 0.01 micron due to the low gas density at
the condensation time. The calculated total dust mass reaches ~1.5 Msun, of
which C dust shares 0.7 Msun. On the other hand, based on the calculated dust
temperature, we show that the dust species and mass evaluated to reproduce the
spectral energy distribution observed by AKARI and MAGNUM at day 200 are
different from those obtained by the dust formation calculations; the dust
species contributing to the observed flux are hot C and FeS grains with masses
of $5.6 \times 10^{-4}$ Msun and $2.0 \times 10^{-3}$ Msun, respectively,
though we cannot defy the presence of a large amount of cold dust such as
silicate and oxide grains up to 0.5 Msun. One of the physical processes
responsible for the difference between calculated and evaluated masses of C and
FeS grains could be considered to be the destruction of small-sized clusters by
energetic photons and electrons prevailing within the ejecta at the earlier
epoch.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 05:34:37 GMT"
},
{
"version": "v2",
"created": "Tue, 20 May 2008 08:05:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nozawa",
"T.",
""
],
[
"Kozasa",
"T.",
""
],
[
"Tominaga",
"N.",
""
],
[
"Sakon",
"I.",
""
],
[
"Tanaka",
"M.",
""
],
[
"Suzuki",
"T.",
""
],
[
"Nomoto",
"K.",
""
],
[
"Maeda",
"K.",
""
],
[
"Umeda",
"H.",
""
],
[
"Limongi",
"M.",
""
],
[
"Onaka",
"T.",
""
]
] | [
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] |
801.2016 | Peter Moran | Peter J. Moran and Derek B. Leinweber | Impact of Dynamical Fermions on QCD Vacuum Structure | 9 pages, 8 figures | Phys.Rev.D78:054506,2008 | 10.1103/PhysRevD.78.054506 | ADP-08-02/T661 | hep-lat | null | We examine how dynamical fermions affect both the UV and infrared structure
of the QCD vacuum. We consider large $28^3 \times 96$ lattices from the MILC
collaboration, using a gluonic definition of the topological charge density,
founded on a new over-improved stout-link smearing algorithm. The algorithm
reproduces established results from the overlap formalism and is designed to
preserve nontrivial topological objects including instantons. At short
distances we focus on the topological charge correlator, $<q(x) q(0) >$, where
negative values at small $x$ reveal a sign-alternating layered structure to the
topological-charge density of the QCD vacuum. We find that the magnitudes of
the negative dip in the $<q(x)q(0)>$ correlator and the positive $<q(0)^2>$
contact term are both increased with the introduction of dynamical fermion
degrees of freedom. This is in accord with expectations based on charge
renormalization and the vanishing of the topological susceptibility in the
chiral limit. At large distances we examine the extent to which instanton-like
objects are found on the lattice, and how their distributions vary between
quenched and dynamical gauge fields. We show that dynamical gauge fields
contain more instanton-like objects with an average size greater than in the
quenched vacuum. Finally, we directly visualize the topological charge density
in order to investigate the effects of dynamical sea-quark degrees of freedom
on topology.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 05:41:24 GMT"
}
] | 2009-01-09T00:00:00 | [
[
"Moran",
"Peter J.",
""
],
[
"Leinweber",
"Derek B.",
""
]
] | [
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] |
801.2017 | Sanil Unnikrishnan | Sanil Unnikrishnan, H. K. Jassal, T. R. Seshadri | Scalar Field Dark Energy Perturbations and their Scale Dependence | 12 pages, 13 figures, added new section, accepted for publication in
Phys. Rev. D | Phys.Rev.D78:123504,2008 | 10.1103/PhysRevD.78.123504 | null | astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We estimate the amplitude of perturbation in dark energy at different length
scales for a quintessence model with an exponential potential. It is shown that
on length scales much smaller than hubble radius, perturbation in dark energy
is negligible in comparison to that in in dark matter. However, on scales
comparable to the hubble radius ($\lambda_{p}>1000\mathrm{Mpc}$) the
perturbation in dark energy in general cannot be neglected. As compared to the
$\Lambda$CDM model, large scale matter power spectrum is suppressed in a
generic quintessence dark energy model. We show that on scales $\lambda_{p} <
1000\mathrm{Mpc}$, this suppression is primarily due to different background
evolution compared to $\Lambda$CDM model. However, on much larger scales
perturbation in dark energy can effect matter power spectrum significantly.
Hence this analysis can act as a discriminator between $\Lambda$CDM model and
other generic dark energy models with $w_{de} \neq -1$.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 06:48:34 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Apr 2008 08:19:46 GMT"
},
{
"version": "v3",
"created": "Thu, 6 Nov 2008 17:22:10 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Unnikrishnan",
"Sanil",
""
],
[
"Jassal",
"H. K.",
""
],
[
"Seshadri",
"T. R.",
""
]
] | [
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] |
801.2018 | S Dev Sharma | S. Dev and Sanjeev Kumar | Two-Zero Symmetric Neutrino Mass Matrices in Minimal Supersymmetric
SO(10) | 12 pages, two tables | null | null | null | hep-ph | null | The phenomenological neutrino mass matrix for two-zero symmetric texture has
been obtained and used to rule out all possible two-zero symmetric neutrino
mass matrices obtained from Yukawa couplings to $\mathbf{10}$ and
$\mathbf{126}$ Higgs representations within the framework of minimal
supersymmetric SO(10).
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 07:26:12 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Dev",
"S.",
""
],
[
"Kumar",
"Sanjeev",
""
]
] | [
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] |
801.2019 | Yveline Lebreton | Pierre Morel, Yveline Lebreton | CESAM: a free code for stellar evolution calculations | 13 pages, 1 figure, accepted for publication in Astrophysics & Space
Science, ESTA/CoRoT Volume | Astrophys.Space Sci.316:61-73,2008 | 10.1007/s10509-007-9663-9 | null | astro-ph | null | The Cesam code is a consistent set of programs and routines which perform
calculations of 1D quasi-hydrostatic stellar evolution including microscopic
diffusion of chemical species and diffusion of angular momentum. The solution
of the quasi-static equilibrium is performed by a collocation method based on
piecewise polynomials approximations projected on a B-spline basis; that allows
stable and robust calculations, and the exact restitution of the solution, not
only at grid points, even for the discontinuous variables. Other advantages are
the monitoring by only one parameter of the accuracy and its improvement by
super-convergence. An automatic mesh refinement has been designed for adjusting
the localisations of grid points according to the changes of unknowns. For
standard models, the evolution of the chemical composition is solved by stiffly
stable schemes of orders up to four; in the convection zones mixing and
evolution of chemical are simultaneous. The solution of the diffusion equation
employs the Galerkin finite elements scheme; the mixing of chemicals is then
performed by a strong turbulent diffusion. A precise restoration of the
atmosphere is allowed for.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 07:21:02 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Morel",
"Pierre",
""
],
[
"Lebreton",
"Yveline",
""
]
] | [
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] |
801.202 | Kiyoshi Shiraishi | Nahomi Kan (Yamaguchi Junior College) and Kiyoshi Shiraishi (Yamaguchi
University) | Induced Gravity in Deconstructed Space at Finite Temperature --
Self-consistent Einstein Universe | 4 pages, 2 figures. A presentation given at JGRG17 (Nagoya, Japan),
to appear in the proceedings | null | null | null | gr-qc hep-th math-ph math.MP | null | We study self-consistent cosmological solutions for an Einstein Universe in a
graph-based induced gravity model. The graph-based field theory has been
proposed by the present authors to generalize dimensional deconstruction. In
this paper, we consider self-consistent Einstein equations for a ``graph theory
space''. Especially, we demonstrate specific results for cycle graphs.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 07:25:00 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Kan",
"Nahomi",
"",
"Yamaguchi Junior College"
],
[
"Shiraishi",
"Kiyoshi",
"",
"Yamaguchi\n University"
]
] | [
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] |
801.2021 | Alexey Glibichuk Anatolyevich | Alexey Glibichuk | Additive properties of product sets in an arbitrary finite field | 11 pages | null | null | null | math.NT math.CO | null | It is proved that for any two subsets $A$ and $B$ of an arbitrary finite
field $\Fq$ such that $|A||B|>q$ the identity $16AB=\Fq$ holds. Moreover, it is
established that for every subsets $X, Y\subset \Fq$ with the property
$|X||Y|\geqslant 2q$ the equality $8XY=\Fq$ holds.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 07:26:01 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Glibichuk",
"Alexey",
""
]
] | [
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801.2022 | Yveline Lebreton | Y. Lebreton | Stars in the age of micro-arc-second astrometry | 7 pages; to appear in the proceedings of "IAU Symposium 248 - A Giant
Step: from Milli- to Micro-arcsecond Astrometry", held in Shanghai, China,
15-19 Oct. 2007 | null | 10.1017/S1743921308019728 | null | astro-ph | null | The understanding and modeling of the structure and evolution of stars is
based on statistical physics as well as on hydrodynamics. Today, a precise
identification and proper description of the physical processes at work in
stellar interiors are still lacking (one key point being that of transport
processes) while the comparison of real stars to model predictions, which
implies conversions from the theoretical space to the observational one,
suffers from uncertainties in model atmospheres. That results in uncertainties
on the prediction of stellar properties needed for galactic studies or
cosmology (as stellar ages and masses). In the next decade, progress is
expected from the theoretical, experimental and observational sides. I
illustrate some of the problems we are faced with when modeling stars and the
possible tracks towards their solutions. I discuss how future observational
ground-based or spatial programs (in particular those dedicated to
micro-arc-second astrometry, asteroseismology and interferometry) will provide
precise determinations of the stellar parameters and contribute to a better
knowledge of stellar interiors and atmospheres in a wide range of stellar
masses, chemical compositions and evolution stages.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 07:34:32 GMT"
}
] | 2018-10-31T00:00:00 | [
[
"Lebreton",
"Y.",
""
]
] | [
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] |
801.2023 | Balasubramanian Ananthanarayan | B. Ananthanarayan, S. Ramanan | Constraining the low energy pion electromagnetic form factor with
space-like data | 11 pages in EPJ journal style, to appear in European Physical Journal
C | Eur.Phys.J.C54:461-470,2008 | 10.1140/epjc/s10052-008-0533-6 | null | hep-ph | null | The pionic contribution to the g-2 of the muon involves a certain integral
over the the modulus squared of F_\pi(t), the pion electromagnetic form factor.
We extend techniques that use cut-plane analyticity properties of F_\pi(t) in
order to account for present day estimates of the pionic contribution and
experimental information at a finite number of points in the space-like region.
Using data from several experiments over a large kinematic range for |t|, we
find bounds on the expansion coefficients of F_\pi(t), sub-leading to the
charge radius. The value of one of these coefficients in chiral perturbation
theory respects these bounds. Furthermore, we present a sensitivity analysis to
the inputs. A brief comparison with results in the literature that use
observables other than the g-2 and timelike data is presented.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 07:45:56 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ananthanarayan",
"B.",
""
],
[
"Ramanan",
"S.",
""
]
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] |
801.2024 | Sisir Roy | Sisir Roy and Malabika Roy | Dark Matter and Supersolidity | 5 pages | null | null | null | physics.gen-ph | null | The origin of collisionless cold dark matter has been traced back to its
origin to the supersolid model of quantum vacuum.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 08:00:59 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Roy",
"Sisir",
""
],
[
"Roy",
"Malabika",
""
]
] | [
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801.2025 | Andrew King | A. R. King | Accretion Rates and Beaming in Ultraluminous X-ray Sources | MNRAS Letters, in press | null | 10.1111/j.1745-3933.2008.00444.x | null | astro-ph | null | I show that extreme beaming factors $b$ are not needed to explain ULXs as
stellar--mass binaries. For neutron star accretors one typically requires $b
\sim 0.13$, and for black holes almost no beaming ($b \sim 0.8$). The main
reason for the high apparent luminosity is the logarithmic increase in the
limiting luminosity for super--Eddington accretion. The required accretion
rates are explicable in terms of thermal--timescale mass transfer from donor
stars of mass $6 - 10\msun$, or possibly transient outbursts. Beaming factors
$\la 0.1$ would be needed to explain luminosities significantly above
$10^{40}L_{40}$ erg s$^{-1}$, but these requirements are relaxed somewhat if
the accreting matter has low hydrogen content.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 08:40:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"King",
"A. R.",
""
]
] | [
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801.2026 | Inge S. Helland | Inge S. Helland | Quantum Mechanics from Focusing and Symmetry | This article is outdated | Found.Phys.38:818-842,2008 | 10.1007/s10701-008-9239-8 | null | quant-ph | null | A foundation of quantum mechanics based on the concepts of focusing and
symmetry is proposed. Focusing is connected to c-variables - inaccessible
conceptually derived variables; several examples of such variables are given.
The focus is then on a maximal accessible parameter, a function of the common
c-variable. Symmetry is introduced via a group acting on the c-variable. From
this, the Hilbert space is constructed and state vectors and operators are
given a clear interpretation. The Born formula is proved from weak assumptions,
and from this the usual rules of quantum mechanics are derived. Several
paradoxes and other issues of quantum theory are discussed.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 08:44:06 GMT"
},
{
"version": "v2",
"created": "Fri, 27 Oct 2023 06:27:34 GMT"
}
] | 2023-10-30T00:00:00 | [
[
"Helland",
"Inge S.",
""
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-0.0159815475,
-0.004973161,
0.0059453156,
0.0458991826,
0.0387737975,
-0.0426399373,
0.0105419774,
0.1392709762,
-0.0525525436,
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0.0080244904,
0.0053299922
] |
801.2027 | Yu-Min Zhao | J. J. Shen, A. Arima, Y. M. Zhao, N. Yoshinaga | Strong Linear Correlation Between Eigenvalues and Diagonal Matrix
Elements | 4 pages | Phys.Rev.C78:044305,2008 | 10.1103/PhysRevC.78.044305 | null | nucl-th | null | We investigate eigenvalues of many-body systems interacting by two-body
forces as well as those of random matrices. We find a strong linear correlation
between eigenvalues and diagonal matrix elements if both of them are sorted
from the smaller values to larger ones. By using this linear correlation we are
able to predict reasonably all eigenvalues of given shell model Hamiltonian
without complicated iterations.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 08:49:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Shen",
"J. J.",
""
],
[
"Arima",
"A.",
""
],
[
"Zhao",
"Y. M.",
""
],
[
"Yoshinaga",
"N.",
""
]
] | [
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] |
801.2028 | Alexander E. Dorokhov | A. E. Dorokhov, E. A. Kuraev, Yu. M. Bystritskiy and M. Secansk\'y | QED radiative corrections to the decay pi^0 to e^+e^- | 12 pages, 3 figures | Eur.Phys.J.C55:193-198,2008 | 10.1140/epjc/s10052-008-0590-x | null | hep-ph | null | We reconsider QED radiative corrections (RC) to the $\pi^{0}\to e^{+}e^{-}$
decay width. One kind of RC investigated earlier has a renormalization group
origin and can be associated with the final state interaction of electron and
positron. It determines the distribution of lepton pair invariant masses in the
whole kinematic region. The other type of RC has a double-logarithmic character
and is related to almost on-mass-shell behavior of the lepton form factors. The
total effect of RC for the $\pi^{0}\to e^{+}e^{-}$ decay is estimated to be
3.2% and for the decay $\eta \to e^{+}e^{-}$ is 4.3%.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:14:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Dorokhov",
"A. E.",
""
],
[
"Kuraev",
"E. A.",
""
],
[
"Bystritskiy",
"Yu. M.",
""
],
[
"Secanský",
"M.",
""
]
] | [
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] |
801.2029 | Asli Sabanci | A. Sabanci, A. Hayreter, L. Solmaz | Higgs Boson Masses Of The MSSM With General Soft Breaking | 9 pages, 2 figures; added new references | Phys.Lett.B661:154-157,2008 | 10.1016/j.physletb.2008.01.071 | 661/2-3 pp. 154-157 | hep-ph | null | The operators that break supersymmetry can be holomorphic or non-holomorphic
in structure. The latter do not pose any problem for gauge hierarchy and are
soft provided that the particle spectrum does not contain any gauge singlets.
In minimal supersymmetric model (MSSM) we discuss the impact of non-holomorphic
soft-breaking terms on the Higgs sector. We find that non-holomorphic operators
can cause significant changes as are best exhibited by the correlation between
the masses of the charginos and Higgs bosons.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:29:32 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Jan 2008 12:17:22 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Sabanci",
"A.",
""
],
[
"Hayreter",
"A.",
""
],
[
"Solmaz",
"L.",
""
]
] | [
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] |
801.203 | Olivier Merlo | L. Benet, O. Merlo | Phase-Space Volume of Regions of Trapped Motion: Multiple Ring
Components and Arcs | 19 pages, 17 figures | Luis Benet and Olivier Merlo, Cel. Mech. Dyn. Astron. 103 (2009),
209-225 | 10.1007/s10569-008-9182-1 | null | nlin.CD | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The phase--space volume of regions of regular or trapped motion, for bounded
or scattering systems with two degrees of freedom respectively, displays
universal properties. In particular, sudden reductions in the phase-space
volume or gaps are observed at specific values of the parameter which tunes the
dynamics; these locations are approximated by the stability resonances. The
latter are defined by a resonant condition on the stability exponents of a
central linearly stable periodic orbit. We show that, for more than two degrees
of freedom, these resonances can be excited opening up gaps, which effectively
separate and reduce the regions of trapped motion in phase space. Using the
scattering approach to narrow rings and a billiard system as example, we
demonstrate that this mechanism yields rings with two or more components. Arcs
are also obtained, specifically when an additional (mean-motion) resonance
condition is met. We obtain a complete representation of the phase-space volume
occupied by the regions of trapped motion.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:36:19 GMT"
},
{
"version": "v2",
"created": "Thu, 30 Oct 2008 19:32:28 GMT"
}
] | 2010-10-28T00:00:00 | [
[
"Benet",
"L.",
""
],
[
"Merlo",
"O.",
""
]
] | [
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] |
801.2031 | Yu-Min Zhao | J. J. Shen, Y. M. Zhao, A. Arima, N. Yoshinaga | Lowest Eigenvalues of Random Hamiltonians | null | Phys.Rev.C77:054312,2008 | 10.1103/PhysRevC.77.054312 | null | nucl-th | null | In this paper we present results of the lowest eigenvalues of random
Hamiltonians for both fermion and boson systems. We show that an empirical
formula of evaluating the lowest eigenvalues of random Hamiltonians in terms of
energy centroids and widths of eigenvalues are applicable to many different
systems (except for $d$ boson systems). We improve the accuracy of the formula
by adding moments higher than two. We suggest another new formula to evaluate
the lowest eigenvalues for random matrices with large dimensions (20-5000).
These empirical formulas are shown to be applicable not only to the evaluation
of the lowest energy but also to the evaluation of excited energies of systems
under random two-body interactions.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:40:43 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Shen",
"J. J.",
""
],
[
"Zhao",
"Y. M.",
""
],
[
"Arima",
"A.",
""
],
[
"Yoshinaga",
"N.",
""
]
] | [
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] |
801.2032 | Ali Massih R. | Karl Forsberg and Ali R. Massih | Diffusion of particles in an expanding sphere with an absorbing boundary | 12 pages. To appear in J. Phys. A: Math. Theor. 41 (2008) | null | 10.1088/1751-8113/41/6/065001 | null | cond-mat.stat-mech | null | We study the problem of particles undergoing Brownian motion in an expanding
sphere whose surface is an absorbing boundary for the particles. The problem is
akin to that of the diffusion of impurities in a grain of polycrystalline
material undergoing grain growth. We solve the time dependent diffusion
equation for particles in a d-dimensional expanding sphere to obtain the
particle density function (function of space and time). The survival rate or
the total number of particles per unit volume as a function of time is
evaluated. We have obtained particular solutions exactly for the case where d=3
and a parabolic growth of the sphere. Asymptotic solutions for the particle
density when the sphere growth rate is small relative to particle diffusivity
and vice versa are derived.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:42:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Forsberg",
"Karl",
""
],
[
"Massih",
"Ali R.",
""
]
] | [
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] |
801.2033 | Tom Michoel | Anagha Joshi, Yves Van de Peer, Tom Michoel | Analysis of a Gibbs sampler method for model based clustering of gene
expression data | 8 pages, 7 figures | Bioinformatics 2008 24(2):176-183 | 10.1093/bioinformatics/btm562 | null | q-bio.QM | null | Over the last decade, a large variety of clustering algorithms have been
developed to detect coregulatory relationships among genes from microarray gene
expression data. Model based clustering approaches have emerged as
statistically well grounded methods, but the properties of these algorithms
when applied to large-scale data sets are not always well understood. An
in-depth analysis can reveal important insights about the performance of the
algorithm, the expected quality of the output clusters, and the possibilities
for extracting more relevant information out of a particular data set. We have
extended an existing algorithm for model based clustering of genes to
simultaneously cluster genes and conditions, and used three large compendia of
gene expression data for S. cerevisiae to analyze its properties. The algorithm
uses a Bayesian approach and a Gibbs sampling procedure to iteratively update
the cluster assignment of each gene and condition. For large-scale data sets,
the posterior distribution is strongly peaked on a limited number of
equiprobable clusterings. A GO annotation analysis shows that these local
maxima are all biologically equally significant, and that simultaneously
clustering genes and conditions performs better than only clustering genes and
assuming independent conditions. A collection of distinct equivalent
clusterings can be summarized as a weighted graph on the set of genes, from
which we extract fuzzy, overlapping clusters using a graph spectral method. The
cores of these fuzzy clusters contain tight sets of strongly coexpressed genes,
while the overlaps exhibit relations between genes showing only partial
coexpression.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:49:57 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Joshi",
"Anagha",
""
],
[
"Van de Peer",
"Yves",
""
],
[
"Michoel",
"Tom",
""
]
] | [
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] |
801.2034 | Jochen Sommerfeld | Jochen Sommerfeld, Igor Bjelakovic and Holger Boche | On the Boundedness of the Support of Optimal Input Measures for Rayleigh
Fading Channels | 5 pages, submitted to ISIT 2008 | null | null | null | cs.IT math.IT | null | We consider transmission over a wireless multiple antenna communication
system operating in a Rayleigh flat fading environment with no channel state
information at the receiver and the transmitter with coherence time T=1. We
show that, subject to the average power constraint, the support of the capacity
achieving input distribution is bounded. Moreover, we show by a simple example
concerning the identity theorem (or uniqueness theorem) from the complex
analysis in several variables that some of the existing results in the field
are not rigorous.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 09:58:26 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Sommerfeld",
"Jochen",
""
],
[
"Bjelakovic",
"Igor",
""
],
[
"Boche",
"Holger",
""
]
] | [
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] |
801.2035 | Larisa Tatarinova | Larisa L. Tatarinova and Martin E. Garcia | Exact description of self-focusing in highly nonlinear geometrical
optics | 3 figures | null | null | null | physics.optics | null | We demonstrate that laser beam collapse in highly nonlinear media can be
described, for a large number of experimental conditions, by the geometrical
optics approximation within high accuracy. Taking into account this fact we
succeed in constructing analytical solutions of the eikonal equation, which are
exact on the beam axis and provide: i) a first-principles determination of the
self-focusing position, thus replacing the widely used empirical Marburger
formula, ii) a benchmark solution for numerical simulations, and iii) a tool
for the experimental determination of the high-order nonlinear susceptibility.
Successful comparison with several experiments is presented.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:11:40 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Tatarinova",
"Larisa L.",
""
],
[
"Garcia",
"Martin E.",
""
]
] | [
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] |
801.2036 | Alexei Nefediev | Yu.S.Kalashnikova, A.V.Nefediev (ITEP, Moscow) | Spectra and decays of hybrid charmonia | RevTeX4, 19 pages, introduction extended, version to appear in
Phys.Rev.D | Phys.Rev.D77:054025,2008 | 10.1103/PhysRevD.77.054025 | null | hep-ph | null | QCD string model is employed to calculate the masses and spin splittings of
lowest charmonium hybrid states with a magnetic gluon. Relative decay rates
into various S- and P-wave D-meson pairs are calculated for these hybrids.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:36:46 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Feb 2008 12:54:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kalashnikova",
"Yu. S.",
"",
"ITEP, Moscow"
],
[
"Nefediev",
"A. V.",
"",
"ITEP, Moscow"
]
] | [
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] |
801.2037 | Ian Heywood | Ian Heywood, Hans-Rainer Kloeckner, Steve Rawlings | Equatorial Imaging with e-MERLIN Including the Chilbolton Antenna | 4 pages, 5 figures, to appear in the proceedings of 'Cosmology,
Galaxy Formation and Astroparticle Physics on the Pathway to the SKA' (H.R.
Kloeckner, S. Rawlings, M.J. Jarvis & A. Taylor, eds.) 10-12 April 2006,
Oxford, UK | null | null | null | astro-ph | null | We discuss the equatorial imaging benefits that arise from the addition of
the 25-metre dish at Chilbolton to the e-MERLIN array. Its inclusion
considerably enhances the capabilities of e-MERLIN on and below the equator.
This will become particularly important in the era of ALMA and other upcoming
southern hemisphere facilities. We present simulated observations of point
sources in the equatorial region of the sky which is the target area for many
existing sky surveys. We find that the additional baselines created by the
inclusion of the Chilbolton dish favourably adjust the beam shape of e-MERLIN
to a more compact and circular shape, with significantly reduced sidelobe
structure. Putting aside the benefits of increased collecting area, the
modified beam shape has implications for more rapidly reaching a given
completeness limit for equatorial surveys.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:38:59 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Heywood",
"Ian",
""
],
[
"Kloeckner",
"Hans-Rainer",
""
],
[
"Rawlings",
"Steve",
""
]
] | [
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] |
801.2038 | Giuseppe Longo | Francis Bailly, Giuseppe Longo | Biological Organization and Negative Entropy: Based on Schroedinger's
reflections | 28 pages | null | null | null | q-bio.OT | null | This paper proposes a systemic perspective for some aspects of both
phylogenesis and ontogenesis, in the light of the notion of biological
organization as negative entropy, following some hints by Schroedinger. To this
purpose, we introduce two extra principles to the thermodynamic ones, which are
(mathematically) compatible with the traditional principles, but have no
meaning in inert matter. A traditional balance equation for metabolism will be
then extended to the new notion as specified by these principles. We consider
far from equilibrium systems and we focus in particular on the production of
global entropy associated to the irreversible character of the processes. A
close analysis of this term will be carried on, both in terms of a diffusion
equation of biomass over complexity and, as a complementary approach and as a
tool for specifying a source term, in connection to Schroedinger's method for
his equation in Quantum Mechanics. We borrow from this equation just the
operatorial approach and, this, in a classical frame, as we use real
coefficients instead of complex ones, away thus from the mathematical frame of
quantum theories. The first application of our proposal is a simple
mathematical reconstruction of Gould's complexity curve of biomass over
complexity, as for evolution. We then elaborate, from the existence of
different time scales, a partition of ontogenetic time, in reference to entropy
and negative entropy variation. On the grounds of this approach, we analyze
metabolism and scaling laws. This allows to compare various relevant
coefficients appearing in these scaling laws, which seem to fit empirical data.
Finally, a tentative and quantitative evaluation of complexity is proposed,
also in relation to some empirical data (caenorhabditis elegans).
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:39:10 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Bailly",
"Francis",
""
],
[
"Longo",
"Giuseppe",
""
]
] | [
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] |
801.2039 | Isabella Pagano | I. Pagano, M. Sachkov, A.I. Gomez de Castro, M. Huang, N. Kappelmann,
S. Scuderi, B. Shustov, K. Werner, and G. Zhao | The focal-plane instruments on board WSO-UV | in Astrophysics and Space Science Proceedings series, M. Chavez, E.
Bertone, D. Rosa-Gonzalez & L. H. Rodriguez-Merino (eds.), invited paper, in
press | null | 10.1007/978-0-387-87621-4_41 | null | astro-ph | null | Dedicated to spectroscopic and imaging observations of the ultraviolet sky,
the World Space Observatory for Ultraviolet Project is a Russia led
international collaboration presently involving also China, Germany, Italy,
Spain and Ukraine. The mission consists of a 1.7m telescope able to perform: a)
high resolution (R greater than 60000) spectroscopy by means of two echelle
spectrographs covering the 103-310 nm range; b) long slit (1x75 arcsec) low
resolution (R about 1500-2500) spectroscopy using a near-UV channel and a
far-UV channel to cover the 102-310nm range; c) deep UV and diffraction limited
UV and optical imaging (from 115 to 700 nm). Overall information on the project
and on its science objectives are given by other two papers in these
proceedings. Here we present the WSO-UV focal plane instruments, their status
of implementation, and the expected performances.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 15:03:03 GMT"
}
] | 2020-08-05T00:00:00 | [
[
"Pagano",
"I.",
""
],
[
"Sachkov",
"M.",
""
],
[
"de Castro",
"A. I. Gomez",
""
],
[
"Huang",
"M.",
""
],
[
"Kappelmann",
"N.",
""
],
[
"Scuderi",
"S.",
""
],
[
"Shustov",
"B.",
""
],
[
"Werner",
"K.",
""
],
[
"Zhao",
"G.",
""
]
] | [
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] |
801.204 | Harikumar E | K. M. Ajith, E. Harikumar, Victor O. Rivelles, M. Sivakumar | Aspects of Noncommutative Scalar/Tensor Duality | 7 pages, typos corrected, a footnote removed and a sentence added in
the text | Phys.Rev.D77:085010,2008 | 10.1103/PhysRevD.77.085010 | null | hep-th | null | We study the noncommutative massless Kalb-Ramond gauge field coupled to a
dynamical U(1) gauge field in the adjoint representation together with a
compensating vector field. We derive the Seiberg-Witten map and obtain the
corresponding mapped action to first order in $\theta$. The (emergent) gravity
structure found in other situations is not present here. The off-shell dual
scalar theory is derived and it does not coincide with the Seiberg-Witten
mapped scalar theory. Dispersion relations are also discussed. The p-form
generalization of the Seiberg-Witten map to order $\theta $ is also derived.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:55:48 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 05:58:23 GMT"
},
{
"version": "v3",
"created": "Wed, 5 Mar 2008 04:21:29 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ajith",
"K. M.",
""
],
[
"Harikumar",
"E.",
""
],
[
"Rivelles",
"Victor O.",
""
],
[
"Sivakumar",
"M.",
""
]
] | [
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] |
801.2041 | Pankaj Jain | Pankaj Jain, Subhadip Mitra and Naveen K. Singh | Cosmological Implications of a Scale Invariant Standard Model | 12 pages, no figures | JCAP 0803:011,2008 | 10.1088/1475-7516/2008/03/011 | null | astro-ph gr-qc hep-ph hep-th | null | We generalize the standard model of particle physics such it displays global
scale invariance. The gravitational action is also suitably modified such that
it respects this symmetry. This model is interesting since the cosmological
constant term is absent in the action. We find that the scale symmetry is
broken by the recently introduced cosmological symmetry breaking mechanism.
This simultaneously generates all the dimensionful parameters such as the
Newton's gravitational constant, the particle masses and the vacuum or dark
energy. We find that in its simplest version the model predicts the Higgs mass
to be very small, which is ruled out experimentally. We further generalize the
model such that it displays local scale invariance. In this case the Higgs
particle disappears from the particle spectrum and instead we find a very
massive vector boson. Hence the model gives a consistent description of
particle physics phenomenology as well as fits the cosmological dark energy.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:47:52 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Jain",
"Pankaj",
""
],
[
"Mitra",
"Subhadip",
""
],
[
"Singh",
"Naveen K.",
""
]
] | [
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] |
801.2042 | Dong Ruan | Dexin Lu (NJU), Dong Ruan (THU), Wang Xu (NJU), Nianle Wu (THU),
Minwen Xiao (NJU), Yu an (THU) | An Experiment of Research-Oriented Teaching/Learning | 31 pages, 4 figures | null | null | null | physics.ed-ph | null | We introduce our experiment of research-oriented teaching mainly in Nanjing
University and Tsinghua University, China. The great population and enrollment
in China makes it worth to concern. It lasts 20 years and involves thousands of
students and hundreds of instructors, consultant experts. We tried many
characteristic styles such as integrated teaching and case analysis, open
resources, interactive mode, course paper program, elite solutions and so on.
The research on the contents is also placed on the agenda. Many students joined
research works that lead to PRL, APL, Nature, Science, and Cell papers. To
impart colleagues the essence we offered some examples in every session. We
declare the accomplishment of the experiment through this paper and new project
is programming.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:49:28 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Lu",
"Dexin",
"",
"NJU"
],
[
"Ruan",
"Dong",
"",
"THU"
],
[
"Xu",
"Wang",
"",
"NJU"
],
[
"Wu",
"Nianle",
"",
"THU"
],
[
"Xiao",
"Minwen",
"",
"NJU"
],
[
"an",
"Yu",
"",
"THU"
]
] | [
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] |
801.2043 | Joakim Nystrand | Joakim Nystrand | Photoproduction in Ultra-Peripheral Heavy-Ion Collisions | 6 pages, 1 figure. Presented at the International Conference on the
Structure and Interactions of the Photon (Photon 2007), Paris, France, 9-13
July 2007. To be published in Nucl. Phys. B. v2 one reference corrected | Nucl.Phys.Proc.Suppl.184:146-151,2008 | 10.1016/j.nuclphysbps.2008.09.153 | 2007.12 | hep-ph | null | The strong electromagnetic fields present in ultra-peripheral collisions of
heavy-ions offer a possibility to study two-photon and photonuclear collisions
complementary to similar studies with lepton beams but over an increased photon
energy range. This presentation will give an overview of photoproduction at
hadron colliders.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 10:54:31 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 10:12:11 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Nystrand",
"Joakim",
""
]
] | [
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] |
801.2044 | Masakatsu Kenmoku | M. Kenmoku, M. Kuwata and K. Shigemoto | Normal Modes and No Zero Mode Theorem of Scalar Fields in BTZ Black Hole
Spacetime | 11 pages,v2 typos corrected | Class.Quant.Grav.25:145016,2008 | 10.1088/0264-9381/25/14/145016 | null | gr-qc | null | Eigenfunctions for normal modes of scalar fields in BTZ black hole spacetime
are studied. Orthonormal relations among them are derived. Quantization for
scalar fields is done and particle number, energy and angular momentum are
expressed by the creation and annihilation operators. Allowed physical normal
mode region is studied on the basis of the no zero mode theorem. Its
implication to the statistical mechanics is also studied.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:21:35 GMT"
},
{
"version": "v2",
"created": "Sun, 17 Feb 2008 06:00:53 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kenmoku",
"M.",
""
],
[
"Kuwata",
"M.",
""
],
[
"Shigemoto",
"K.",
""
]
] | [
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] |
801.2045 | Kirrily Rule | K.C. Rule, M.J. Lewis, H.A. Dabkowska, D.R. Taylor and B.D. Gaulin | Critical X-ray Scattering Studies of Jahn-Teller Phase Transitions in
TbV$_{1-x}$As$_{x}$O$_{4}$ | 8 pages, 6 figures | null | 10.1103/PhysRevB.77.134116 | null | cond-mat.str-el | null | The critical behaviour associated with cooperative Jahn-Teller phase
transitions in TbV$_{1-x}$As$_{x}$O$_{4}$ (where \textit{x} = 0, 0.17, 1)
single crystals have been studied using high resolution x-ray scattering. These
materials undergo continuous tetragonal $\to$ orthorhombic structural phase
transitions driven by Jahn-Teller physics at T$_C$ = 33.26(2) K, 30.32(2) K and
27.30(2) K for \textit{x} = 0, 0.17 and 1 respectively. The orthorhombic strain
was measured close to the phase transition and is shown to display mean field
behavior in all three samples. Pronounced fluctuation effects are manifest in
the longitudinal width of the Bragg scattering, which diverges as a power law,
with an exponent given by $x=0.45 \pm 0.04$, on approaching the transition from
either above or below. All samples exhibited twinning; however the disordered x
= 0.17 sample showed a broad distribution of twins which were stable to
relatively low temperatures, well below T$_C$. This indicates that while the
orthorhombic strain continues to develop in a conventional mean field manner in
the presence of disorder, twin domains are easily pinned by the quenched
impurities and their associated random strains.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:02:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rule",
"K. C.",
""
],
[
"Lewis",
"M. J.",
""
],
[
"Dabkowska",
"H. A.",
""
],
[
"Taylor",
"D. R.",
""
],
[
"Gaulin",
"B. D.",
""
]
] | [
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] |
801.2046 | Deepak Mathur | Deepak Mathur, Aditya K. Dharmadhikari, Firoz A. Rajgara, and
Jayashree A. Dharmadhikari | Molecular symmetry effects in the ionization of CS$_2$ by intense,
few-cycle laser pulses | Submitted to Physical Review Lottery | null | 10.1103/PhysRevA.78.013405 | null | physics.optics physics.atom-ph | null | Few-cycle pulses of intense 800 nm light are used to probe ionization and
dissociation of carbon disulfide in the intensity and temporal regime where
rescattering is expected to dominate the laser-molecule interaction. The
wavepacket of the rescattered electron destructively interferes with the
anti-bonding $\pi$-orbital of CS$_2^+$ such that rescattering is effectively
"switched off". Direct signature of enhanced ionization being "switched off" in
the ultrashort domain is also obtained. Consequently, dissociation becomes an
almost non-existent channel when few-cycle pulses are used, with only
long-lived singly-, doubly-, and triply-charged molecular ions dominating the
mass spectrum. Few-cycle optical pulses help reveal that quantum-mechanically
determined molecular symmetry contributes to strong field molecular ionization.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:03:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mathur",
"Deepak",
""
],
[
"Dharmadhikari",
"Aditya K.",
""
],
[
"Rajgara",
"Firoz A.",
""
],
[
"Dharmadhikari",
"Jayashree A.",
""
]
] | [
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] |
801.2047 | Jerome Boudet | J\'er\^ome Boudet (LMFA), Jo\"elle Caro (LMFA), L. Shao (LMFA),
Emmanuel L\'ev\^eque (Phys-ENS) | Numerical studies towards practical large-eddy simulation | null | Journal of Thermal Science 16, 4 (2007) 328-336 | 10.1007/s11630-007-0328-3 | null | physics.flu-dyn | null | Large-eddy simulation developments and validations are presented for an
improved simulation of turbulent internal flows. Numerical methods are proposed
according to two competing criteria: numerical qualities (precision and
spectral characteristics), and adaptability to complex configurations. First,
methods are tested on academic test-cases, in order to abridge with fundamental
studies. Consistent results are obtained using adaptable finite volume method,
with higher order advection fluxes, implicit grid filtering and "low-cost"
shear-improved Smagorinsky model. This analysis particularly focuses on mean
flow, fluctuations, two-point correlations and spectra. Moreover, it is shown
that exponential averaging is a promising tool for LES implementation in
complex geometry with deterministic unsteadiness. Finally, adaptability of the
method is demonstrated by application to a configuration representative of
blade-tip clearance flow in a turbomachine.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:04:10 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Boudet",
"Jérôme",
"",
"LMFA"
],
[
"Caro",
"Joëlle",
"",
"LMFA"
],
[
"Shao",
"L.",
"",
"LMFA"
],
[
"Lévêque",
"Emmanuel",
"",
"Phys-ENS"
]
] | [
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] |
801.2048 | Petros Draggiotis | Petros Draggiotis | Numerical Implementation of Generalized Unitarity | 10 pages, 1 figure | null | null | null | hep-ph | null | We present a numerical implementation of generalized unitarity. We will show
that we are able to obtain the box coefficients of any 1 loop gluonic
amplitude, for an arbitrary helicity configuration and for any number of
external particles.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 15:14:19 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Draggiotis",
"Petros",
""
]
] | [
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] |
801.2049 | Andrzej Trzesowski | Andrzej Trzesowski | Nanothermomechanics | 29 pages. Keywords: affinely-rigid body, constraints, graphenes,
fullerenes, insensibility group, liquid-like response, nanocluster,
nanothermodynamics, nanothermomechanics, quasi-solid state, solid state,
structural stability, size effect, shape effect, viscosity effect | Journal of Technical Physics, vol. 50, 3-4, pp. 151-172, 2009. | null | null | cond-mat.mtrl-sci math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The paper concerns the dependence of thermomechanical properties of
three-dimensional solid nanoclusters on the cluster size as well as on its
shape. Investigations are restricted to the class of so-called homogeneous
thermodynamic processes with kinematics based on affine group and referred to
the one whole body, not an infinite system of subbodies. It is shown that then
the thermodynamics of nanoclusters is consistent with dynamics of
affinely-rigid bodies (constrained or not and elastic as well as admitting
viscosity effects). The main discussed top-ics are: (i) a group-theoretical
description of structurally stable solid nanoclusters; (ii) a phe-nomenological
model of mechanical properties of nanoclusters revealing the coexistence of
solid and liquid states in a finite interval of absolute temperature.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:23:09 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 12:27:49 GMT"
},
{
"version": "v3",
"created": "Wed, 7 May 2008 10:02:28 GMT"
},
{
"version": "v4",
"created": "Thu, 19 Jun 2008 10:14:18 GMT"
},
{
"version": "v5",
"created": "Fri, 5 Dec 2008 10:54:53 GMT"
},
{
"version": "v6",
"created": "Tue, 16 Mar 2010 11:08:19 GMT"
}
] | 2010-03-17T00:00:00 | [
[
"Trzesowski",
"Andrzej",
""
]
] | [
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] |
801.205 | Alessandro Siria | A. Siria, M. S. Rodrigues, O. Dhez, W. Schwartz, G. Torricelli, S. Le
Denmat, N. Rochat, G. Auvert, O. Bikondoa, T. H. Metzger, D. Wermeille, R.
Felici, F. Comin and J. Chevrier | X-ray pushing of a mechanical microswing | 5 pages, 4 figure | null | 10.1088/0957-4484/19/44/445501 | null | physics.ins-det | null | Nanoelectromechanical Systems (NEMS) are among the best candidates to measure
interactions at nanoscale [1-6], especially when resonating oscillators are
used with high quality factor [7, 8]. Despite many efforts [9, 10], efficient
and easy actuation in NEMS remains an issue [11]. The mechanism that we
propose, thermally mediated Center Of Mass (COM) displacements, represents a
new actuation scheme for NEMS and MEMS. To demonstrate this scheme efficiency
we show how mechanical nanodis- placements of a MEMS is triggered using
modulated X-ray microbeams. The MEMS is a microswing constituted by a Ge
microcrystal attached to a Si microcantilever. The interaction is mediated by
the Ge absorption of the intensity modulated X-ray microbeam impinging on the
microcrystal. The small but finite thermal expansion of the Ge microcrystal is
large enough to force a nanodisplacement of the Ge microcrystal COM glued on a
Si microlever. The inverse mechanism can be envisaged: MEMS can be used to
shape X-ray beams. A Si microlever can be a high frequency X-ray beam chopper
for time studies in biology and chemistry.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:25:26 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 22:16:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Siria",
"A.",
""
],
[
"Rodrigues",
"M. S.",
""
],
[
"Dhez",
"O.",
""
],
[
"Schwartz",
"W.",
""
],
[
"Torricelli",
"G.",
""
],
[
"Denmat",
"S. Le",
""
],
[
"Rochat",
"N.",
""
],
[
"Auvert",
"G.",
""
],
[
"Bikondoa",
"O.",
""
],
[
"Metzger",
"T. H.",
""
],
[
"Wermeille",
"D.",
""
],
[
"Felici",
"R.",
""
],
[
"Comin",
"F.",
""
],
[
"Chevrier",
"J.",
""
]
] | [
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] |
801.2051 | Daniel M. Pellegrino | Geraldo Botelho and Daniel Pellegrino | Absolutely summing linear operators into spaces with no finite cotype | 7 pages | Bulletin of the Belgian Mathematical Society Simon Stevin, v. 16,
p. 373-378, 2009 | null | null | math.FA | null | Given an infinite-dimensional Banach space $X$ and a Banach space $Y$ with no
finite cotype, we determine whether or not every continuous linear operator
from $X$ to $Y$ is absolutely $(q;p)$-summing for almost all choices of $p$ and
$q$, including the case $p=q$. If $X$ assumes its cotype, the problem is solved
for all choices of $p$ and $q$. Applications to the theory of dominated
multilinear mappings are also provided.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:34:45 GMT"
}
] | 2015-10-06T00:00:00 | [
[
"Botelho",
"Geraldo",
""
],
[
"Pellegrino",
"Daniel",
""
]
] | [
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-0.0922598094,
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0.0383023806,
0.0317396671,
0.0556995347,
-0.0381353274,
0.0465356,
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] |
801.2052 | Peter Jorgensen | Peter Jorgensen | Calabi-Yau categories and Poincare duality spaces | 33 pages; minor changes. To appear in the ICRA XII volume "Trends in
Representation Theory of Algebras and Related Topics" | null | null | null | math.RT math.AT math.RA | null | The singular cochain complex of a topological space is a classical object. It
is a Differential Graded algebra which has been studied intensively with a
range of methods, not least within rational homotopy theory.
More recently, the tools of Auslander-Reiten theory have also been applied to
the singular cochain complex. One of the highlights is that by these methods,
each Poincare duality space gives rise to a Calabi-Yau category. This paper is
a review of the theory.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:36:46 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Apr 2008 13:03:07 GMT"
}
] | 2008-04-14T00:00:00 | [
[
"Jorgensen",
"Peter",
""
]
] | [
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] |
801.2053 | Chen Songbai | Songbai Chen, Bin Wang, Rukeng Su | Hawking radiation in a $d$-dimensional static spherically-symmetric
black Hole surrounded by quintessence | 16 pages, Accepted for publication in Phys. Rev. D | Phys.Rev.D77:124011,2008 | 10.1103/PhysRevD.77.124011 | null | gr-qc | null | We present a solution of Einstein equations with quintessential matter
surrounding a $d$-dimensional black hole, whose asymptotic structures are
determined by the state of the quintessential matter. We examine the
thermodynamics of this black hole and find that the mass of the black hole
depends on the equation of state of the quintessence, while the first law is
universal. Investigating the Hawking radiation in this black hole background,
we observe that the Hawking radiation dominates on the brane in the low-energy
regime. For different asymptotic structures caused by the equation of state of
the quintessential matter surrounding the black hole, we learn that the
influences by the state parameter of the quintessence on Hawking radiation are
different.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:40:22 GMT"
},
{
"version": "v2",
"created": "Sun, 20 Apr 2008 02:21:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chen",
"Songbai",
""
],
[
"Wang",
"Bin",
""
],
[
"Su",
"Rukeng",
""
]
] | [
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] |
801.2054 | Pinaki Majumdar | Anamitra Mukherjee, Kalpataru Pradhan and Pinaki Majumdar | Conductance Switching and Inhomogeneous Field Melting in the Charge
Ordered Manganites | 5 pages, pdflatex, 5 png figures To appear in Europhys. Lett | null | 10.1209/0295-5075/86/27003 | null | cond-mat.str-el cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The field induced switching of conductance in the charge ordered half-doped
manganites is controlled by the combination of metastability, an inhomogeneous
high field state, and cation disorder. We study this non-equilibrium problem
via real space Monte Carlo on a disordered strong coupling model appropriate to
the manganites. We reproduce the variation of the switching fields with the
mean ionic radius r_A and cation disorder \sigma_A, and demonstrate how the
experimental features arise from the proximity of several phases in the Landau
free energy landscape. Our prediction for the field melted state is consistent
with a growing body of experimental evidence.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 11:44:42 GMT"
},
{
"version": "v2",
"created": "Fri, 20 Mar 2009 11:03:00 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Mukherjee",
"Anamitra",
""
],
[
"Pradhan",
"Kalpataru",
""
],
[
"Majumdar",
"Pinaki",
""
]
] | [
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] |
801.2055 | Florin Panaite | Florin Panaite, Mihai D. Staic, Freddy Van Oystaeyen | Pseudosymmetric braidings, twines and twisted algebras | 29 pages | null | null | null | math.QA math.CT | null | A laycle is the categorical analogue of a lazy cocycle. Twines (as introduced
by Bruguieres) and strong twines (as introduced by the authors) are laycles
satisfying some extra conditions. If $c$ is a braiding, the double braiding
$c^2$ is always a twine; we prove that it is a strong twine if and only if $c$
satisfies a sort of modified braid relation (we call such $c$ pseudosymmetric,
as any symmetric braiding satisfies this relation). It is known that symmetric
Yetter-Drinfeld categories are trivial; we prove that the Yetter-Drinfeld
category $_H{\cal YD}^H$ over a Hopf algebra $H$ is pseudosymmetric if and only
if $H$ is commutative and cocommutative. We introduce as well the Hopf
algebraic counterpart of pseudosymmetric braidings under the name
pseudotriangular structures and prove that all quasitriangular structures on
the $2^{n+1}$-dimensional pointed Hopf algebras E(n) are pseudotriangular. We
observe that a laycle on a monoidal category induces a so-called pseudotwistor
on every algebra in the category, and we obtain some general results (and give
some examples) concerning pseudotwistors, inspired by properties of laycles and
twines.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:03:28 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Panaite",
"Florin",
""
],
[
"Staic",
"Mihai D.",
""
],
[
"Van Oystaeyen",
"Freddy",
""
]
] | [
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] |
801.2056 | Julius Ruseckas | Gediminas Juzeliunas, Julius Ruseckas, Andreas Jacob, Luis Santos,
Patrik Ohberg | Double and negative reflection of cold atoms in non-Abelian gauge
potentials | 5 figures corrected references | Phys. Rev. Lett. 100, 200405 (2008) | 10.1103/PhysRevLett.100.200405 | null | cond-mat.other physics.atom-ph quant-ph | null | Atom reflection is studied in the presence of a non-Abelian vector potential
proportional to a spin-1/2 operator. The potential is produced by a relatively
simple laser configuration for atoms with a tripod level scheme. We show that
the atomic motion is described by two different dispersion branches with
positive or negative chirality. As a consequence of that, atom reflection shows
unusual features, since an incident wave may split into two reflected ones at a
barrier, an ordinary specular reflection, and an additional non-specular one.
Remarkably, the latter wave can exhibit negative reflection and may become
evanescent if the angle of incidence exceeds a critical value. These reflection
properties are crucial for future designs in non-Abelian atom optics.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:06:09 GMT"
},
{
"version": "v2",
"created": "Tue, 27 May 2008 09:12:52 GMT"
}
] | 2008-05-27T00:00:00 | [
[
"Juzeliunas",
"Gediminas",
""
],
[
"Ruseckas",
"Julius",
""
],
[
"Jacob",
"Andreas",
""
],
[
"Santos",
"Luis",
""
],
[
"Ohberg",
"Patrik",
""
]
] | [
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] |
801.2057 | Chenchang Zhu | Chenchang Zhu | n-Groupoids and Stacky Groupoids | 45 pages, include other categories than a previous paper--
arXiv:math/0609420 [math.DG], edited version, typos removed, more details on
axioms of stacky groupoids. to appear in IMRN | International Mathematics Research Notices (2009) 2009:4087-4141 | 10.1093/imrn/rnp080 | null | math.DG math.CT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss two generalizations of Lie groupoids. One consists of Lie
$n$-groupoids defined as simplicial manifolds with trivial $\pi_{k\geq n+1}$.
The other consists of stacky Lie groupoids $\cG\rra M$ with $\cG$ a
differentiable stack. We build a 1-1 correspondence between Lie 2-groupoids and
stacky Lie groupoids up to a certain Morita equivalence. We prove this in a
general set-up so that the statement is valid in both differential and
topological categories. \Equivalences of higher groupoids in various categories
are also described.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:12:04 GMT"
},
{
"version": "v2",
"created": "Mon, 29 Jun 2009 10:04:24 GMT"
}
] | 2009-12-04T00:00:00 | [
[
"Zhu",
"Chenchang",
""
]
] | [
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] |
801.2058 | Shoulan Gao | Shoulan Gao, Cuipo Jiang and Yufeng Pei | Structure of the extended Schrodinger-Virasoro Lie algebra | 24 pages, to appear in Algrbra Colloquium | null | null | null | math.RA math.GM | null | In this paper, we study the derivations, the central extensions and the
automorphism group of the extended Schrodinger-Virasoro Lie algebra, introduced
by J. Unterberger in the context of two-dimensional conformal field theory and
statistical physics. Moreover, we show that the extended Schrodinger-Virasoro
Lie algebra is an infinite-dimensional complete Lie algebra and the universal
central extension of the extended Schrodinger-Virasoro Lie algebra in the
category of Leibniz algebras is the same as that in the category of Lie
algebras.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:13:48 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Gao",
"Shoulan",
""
],
[
"Jiang",
"Cuipo",
""
],
[
"Pei",
"Yufeng",
""
]
] | [
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] |
801.2059 | Michael B\"orsch | N. Zarrabi, T. Heitkamp, J. C. Greie, M. Boersch | Monitoring the conformational dynamics of a single potassium transporter
by ALEX-FRET | 10 pages, 4 figures | null | 10.1117/12.768262 | null | physics.bio-ph physics.data-an | null | Conformational changes of single proteins are monitored in real time by
Forster-type resonance energy transfer, FRET. Two different fluorophores have
to be attached to those protein domains, which move during function. The
distance between the fluorophores is measured by relative fluorescence
intensity changes of FRET donor and acceptor fluorophore, or by fluorescence
lifetime changes of the FRET donor. The fluorescence spectrum of a single FRET
donor fluorophore is influenced by local protein environment dynamics causing
apparent fluorescence intensity changes on the FRET donor and acceptor detector
channels. To discriminate between those spectral fluctuations and
distance-dependent FRET, alternating pulsed excitation schemes (ALEX) have
recently been introduced which simultaneously probe the existence of a FRET
acceptor fluorophore. Here we employ single-molecule FRET measurements to a
membrane protein. The membrane-embedded KdpFABC complex transports potassium
ions across a lipid bilayer using ATP hydrolysis. Our study aims at the
observation of conformational fluctuations within a single P-type ATPase
functionally reconstituted into liposomes by single-molecule FRET and analysis
by Hidden-Markov-Models.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:14:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zarrabi",
"N.",
""
],
[
"Heitkamp",
"T.",
""
],
[
"Greie",
"J. C.",
""
],
[
"Boersch",
"M.",
""
]
] | [
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] |
801.206 | Wei Lin | Qing Ding, Wei Lin | The Transmission Property of the Discrete Heisenberg Ferromagnetic Spin
Chain | 16 pages, 7 figures | null | 10.1063/1.2976036 | null | nlin.CD nlin.SI | null | We present a mechanism for displaying the transmission property of the
discrete Heisenberg ferromagnetic spin chain (DHF) via a geometric approach. By
the aid of a discrete nonlinear Schr\"odinger-like equation which is the
discrete gauge equivalent to the DHF, we show that the determination of
transmitting coefficients in the transmission problem is always bistable. Thus
a definite algorithm and general stochastic algorithms are presented. A new
invariant periodic phenomenon of the non-transmitting behavior for the DHF,
with a large probability, is revealed by an adoption of various stochastic
algorithms.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:19:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ding",
"Qing",
""
],
[
"Lin",
"Wei",
""
]
] | [
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] |
801.2061 | Robert de Mello Koch | Rajsekhar Bhattacharyya, Storm Collins and Robert de Mello Koch | Exact Multi-Matrix Correlators | 13+1 pages; v1:minor improvements in presentation and refs added; v2:
additional comments in finite N counting; v3: Final JHEP version | JHEP 0803:044,2008 | 10.1088/1126-6708/2008/03/044 | WITS-CTP-036 | hep-th | null | We argue that restricted Schur polynomials provide a useful parameterization
of the complete set of gauge invariant variables of multi-matrix models. The
two point functions of restricted Schur polynomials are evaluated exactly in
the free field theory limit. They have diagonal two point functions.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:25:01 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 06:49:50 GMT"
},
{
"version": "v3",
"created": "Wed, 5 Mar 2008 18:36:00 GMT"
},
{
"version": "v4",
"created": "Mon, 10 Mar 2008 04:21:31 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Bhattacharyya",
"Rajsekhar",
""
],
[
"Collins",
"Storm",
""
],
[
"Koch",
"Robert de Mello",
""
]
] | [
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] |
801.2062 | Michael Bordag | M. Bordag, N. Khusnutdinov | On the vacuum energy of a spherical plasma shell | 16 pages, 3 figures, submitted to Phys.Rev.D | Phys.Rev.D77:085026,2008 | 10.1103/PhysRevD.77.085026 | null | hep-th quant-ph | null | We consider the vacuum energy of the electromagnetic field interacting with a
spherical plasma shell together with a model for the classical motion of the
shell. We calculate the heat kernel coefficients, especially that for the TM
mode, and carry out the renormalization by redefining the parameters of the
classical model. It turns out that this is possible and results in a model,
which in the limit of the plasma shell becoming an ideal conductor reproduces
the vacuum energy found by Boyer in 1968.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:31:41 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bordag",
"M.",
""
],
[
"Khusnutdinov",
"N.",
""
]
] | [
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] |
801.2063 | Andrei Barvinsky | A.O.Barvinsky, C.Deffayet, A.Yu.Kamenshchik | Anomaly Driven Cosmology: Big Boost Scenario and AdS/CFT Correspondence | LaTeX, 14 pages, 1 figure | JCAP 0805:020,2008 | 10.1088/1475-7516/2008/05/020 | null | hep-th | null | We consider the cosmological evolution in a recently suggested new model of
quantum initial conditions for the Universe. The effective Friedmann equation
incorporates the effect of the conformal anomaly of quantum fields and,
interestingly, shows that their vacuum Casimir energy is completely screened
and does not gravitate. The cosmological evolution also features a new
mechanism for a cosmological acceleration stage. This stage is followed by a
big boost singularity -- a rapid growth up to infinity of the scale factor
acceleration parameter. We also briefly discuss the relation between our model,
the AdS/CFT correspondence and RS and DGP braneworlds.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:25:16 GMT"
}
] | 2009-03-19T00:00:00 | [
[
"Barvinsky",
"A. O.",
""
],
[
"Deffayet",
"C.",
""
],
[
"Kamenshchik",
"A. Yu.",
""
]
] | [
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] |
801.2064 | Joseph A. Minahan | J. A. Minahan, O. Ohlsson Sax | Finite size effects for giant magnons on physical strings | 24 pages, 7 figures; v2 typos fixed | Nucl.Phys.B801:97-117,2008 | 10.1016/j.nuclphysb.2008.04.018 | UUITP-20/07 | hep-th | null | Using finite gap methods, we find the leading order finite size corrections
for an arbitrary number of giant magnons on physical strings, where the sum of
the momenta is a multiple of 2\pi. Our results are valid for the
Hofman-Maldacena fundamental giant magnons as well as their dyonic
generalizations. The energy corrections turn out to be surprisingly simple,
especially if all the magnons are fundamental, and at leading order are
independent of the magnon flavors. We also show how to use the Bethe ansatz to
find finite size corrections for dyonic giant magnons with large R-charges.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 20:20:20 GMT"
},
{
"version": "v2",
"created": "Fri, 1 Feb 2008 03:30:42 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Minahan",
"J. A.",
""
],
[
"Sax",
"O. Ohlsson",
""
]
] | [
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] |
801.2065 | Christian Schr\"oder | Christian Schr\"oder, Ruslan Prozorov, Paul K\"ogerler, Matthew D.
Vannette, Xikui Fang, Marshall Luban, Akira Matsuo, Koichi Kindo, Achim
M\"uller, Ana Maria Todea | Multiple nearest-neighbor exchange model for the frustrated magnetic
molecules Mo72Fe30 and Mo72Cr30 | 8 pages, 5 figures | null | 10.1103/PhysRevB.77.224409 | null | physics.atm-clus | null | Our measurements of the differential susceptibility dM/dH of the frustrated
magnetic molecules Mo72Fe30 and Mo72Cr30 reveal a pronounced dependence on
magnetic field (H) and temperature (T) in the low H - low T regime, contrary to
the predictions of existing models. Excellent agreement with experiment is
achieved upon formulating a nearest-neighbor classical Heisenberg model where
the 60 nearest-neighbor exchange interactions in each molecule, rather than
being identical as has been assumed heretofore, are described by a
two-parameter probability distribution of values of the exchange constant. We
suggest that the probability distribution provides a convenient
phenomenological platform for summarizing the combined effects of multiple
microscopic mechanisms that disrupt the idealized picture of a Heisenberg model
based on a single value of the nearest-neighbor exchange constant.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:44:51 GMT"
},
{
"version": "v2",
"created": "Fri, 9 May 2008 10:34:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schröder",
"Christian",
""
],
[
"Prozorov",
"Ruslan",
""
],
[
"Kögerler",
"Paul",
""
],
[
"Vannette",
"Matthew D.",
""
],
[
"Fang",
"Xikui",
""
],
[
"Luban",
"Marshall",
""
],
[
"Matsuo",
"Akira",
""
],
[
"Kindo",
"Koichi",
""
],
[
"Müller",
"Achim",
""
],
[
"Todea",
"Ana Maria",
""
]
] | [
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] |
801.2066 | Misak Sargsian | Misak M. Sargsian | High Energy Break-Up of Few-Nucleon Systems | To appear in the proceedings of Workshop on Exclusive Reactions at
High Momentum Transfer, Newport News, Virgina, 21-24 May 2007 | null | 10.1142/9789812796950_0027 | null | nucl-th | null | We discus recent developments in theory of high energy two-body break-up
reactions of few-nucleon systems. The characteristics of these reactions are
such that the hard two-body quasielastic subprocess can be clearly separated
from the accompanying soft subprocesses. We discuss in details the hard
rescattering model (HRM) in which hard photodisintegration develops in two
stages. At first, photon knocks-out an energetic quark which rescatters
subsequently with a quark of the other nucleon. The latter provides a mechanism
of sharing the initial high momentum of the photon by the outgoing two
nucleons. Within HRM we discuss hard break-up reactions involving $^2D$ and
$^3He$ targets. Another development of HRM is the prediction of new helicity
selection mechanism for hard two-body reactions, which was apparently confirmed
in the recent JLab experiment.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 12:44:54 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Sargsian",
"Misak M.",
""
]
] | [
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] |
801.2067 | Mahdou Najib | D. Bennis and N. Mahdou | On n-Perfect Rings and Cotorsion Dimension | null | null | null | null | math.AC math.RA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A ring is called $n$-perfect ($n\geq 0$), if every flat module has projective
dimension less or equal than $n$. In this paper, we show that the
$n$-perfectness relate, via homological approach, some homological dimension of
rings. We study $n$-perfectness in some known ring constructions. Finally,
several examples of $n$-perfect rings satisfying special conditions are given.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 13:02:13 GMT"
},
{
"version": "v2",
"created": "Wed, 10 Sep 2008 23:54:18 GMT"
}
] | 2008-09-11T00:00:00 | [
[
"Bennis",
"D.",
""
],
[
"Mahdou",
"N.",
""
]
] | [
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] |
801.2068 | Christine Weber | C. Weber, G. Audi, D. Beck, K. Blaum, G. Bollen, F. Herfurth, A.
Kellerbauer, H.-J. Kluge, D. Lunney, and S. Schwarz | Atomic mass measurements of short-lived nuclides around the doubly-magic
208Pb | 40 pages, 20 figures, accept. for publication in Nucl. Phys. A | Nucl.Phys.A803:1-29,2008 | 10.1016/j.nuclphysa.2007.12.014 | null | nucl-ex | null | Accurate atomic mass measurements of neutron-deficient and neutron-rich
nuclides around the doubly-magic 208Pb and of neutron-rich cesium isotopes were
performed with the Penning trap mass spectrometer ISOLTRAP at ISOLDE/CERN. The
masses of 145,147Cs, 181,183Tl, 186Tlm, 187Tl, 196Tlm, 205Tl, 197Pbm, 208Pb,
190 to 197Bi, 209,215,216Bi, 203,205,229Fr, and 214,229,230Ra were determined.
The obtained relative mass uncertainty in the range of $2 \cdot 10^{-7}$ to $2
\cdot 10^{-8}$ is not only required for safe identification of isomeric states
but also allows mapping the detailed structure of the mass surface. A mass
adjustment procedure was carried out and the results included into the Atomic
Mass Evaluation. The resulting separation energies are discussed and the mass
spectrometric and laser spectroscopic data are examined for possible
correlations.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 13:03:22 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Weber",
"C.",
""
],
[
"Audi",
"G.",
""
],
[
"Beck",
"D.",
""
],
[
"Blaum",
"K.",
""
],
[
"Bollen",
"G.",
""
],
[
"Herfurth",
"F.",
""
],
[
"Kellerbauer",
"A.",
""
],
[
"Kluge",
"H. -J.",
""
],
[
"Lunney",
"D.",
""
],
[
"Schwarz",
"S.",
""
]
] | [
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] |
801.2069 | Istvan Szita | Istvan Szita and Andras Lorincz | Factored Value Iteration Converges | 17 pages, 1 figure | null | null | null | cs.AI cs.LG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we propose a novel algorithm, factored value iteration (FVI),
for the approximate solution of factored Markov decision processes (fMDPs). The
traditional approximate value iteration algorithm is modified in two ways. For
one, the least-squares projection operator is modified so that it does not
increase max-norm, and thus preserves convergence. The other modification is
that we uniformly sample polynomially many samples from the (exponentially
large) state space. This way, the complexity of our algorithm becomes
polynomial in the size of the fMDP description length. We prove that the
algorithm is convergent. We also derive an upper bound on the difference
between our approximate solution and the optimal one, and also on the error
introduced by sampling. We analyze various projection operators with respect to
their computation complexity and their convergence when combined with
approximate value iteration.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 13:09:06 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Aug 2008 15:07:08 GMT"
}
] | 2008-08-13T00:00:00 | [
[
"Szita",
"Istvan",
""
],
[
"Lorincz",
"Andras",
""
]
] | [
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] |
801.207 | Baba Thiam | Abdelkader Mokkadem (LM-Versailles), Mariane Pelletier
(LM-Versailles), Baba Thiam (LM-Versailles) | Joint behaviour of semirecursive kernel estimators of the location and
of the size of the mode of a probability density function | 26 pages | null | null | null | math.ST stat.TH | null | Let $\theta$ and $\mu$ denote the location and the size of the mode of a
probability density. We study the joint convergence rates of semirecursive
kernel estimators of $\theta$ and $\mu$. We show how the estimation of the size
of the mode allows to measure the relevance of the estimation of its location.
We also enlighten that, beyond their computational advantage on nonrecursive
estimators, the semirecursive estimators are preferable to use for the
construction on confidence regions.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 13:11:34 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Mokkadem",
"Abdelkader",
"",
"LM-Versailles"
],
[
"Pelletier",
"Mariane",
"",
"LM-Versailles"
],
[
"Thiam",
"Baba",
"",
"LM-Versailles"
]
] | [
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] |
801.2071 | Evelina Viada | Viada Evelina | The optimality of the Boundedness Height Conjecture | 12 pages | Journal de Theorie des nombres de bordeaux, 21 (2009), 769-784 | null | null | math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that the Boundedness Height Conjecture is optimal; all varieties in a
power of an elliptic curve which do not satisfy the hypothesis neither satisfy
the thesis. The Bounded Height Conjecture is known to hold for varieties in a
power of an elliptic curve. We also present some examples and remarks.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 13:14:19 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 12:36:53 GMT"
},
{
"version": "v3",
"created": "Mon, 10 Nov 2008 12:45:34 GMT"
}
] | 2010-03-29T00:00:00 | [
[
"Evelina",
"Viada",
""
]
] | [
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] |
801.2072 | Gennady Kozlov | G.A. Kozlov | Bose-Einstein correlations and the stochastic scale of light hadrons
emitter source | 16 pages | null | 10.1142/9789812834959_0010 | null | hep-ph | null | Based on quantum field theory at finite temperature we carried out new
results for two-particle Bose-Einstein correlation (BEC) function ${C_2}(Q)$ in
case of light hadrons. The important parameters of BEC function related to the
size of the emitting source, mean multiplicity, stochastic forces range with
the particle energy and mass dependence, and the temperature of the source are
obtained for the first time. Not only the correlation between identical hadrons
are explored but even the off-correlation between non-identical particles are
proposed. The correlations of two bosons in 4-momentum space presented in this
paper offer useful and instructive complimentary viewpoints to theoretical and
experimental works in multiparticle femtoscopy and interferometry measurements
at hadron colliders. This paper is the first one to the next opening series of
works concerning the searching of BEC with experimental data where the
parameters above mentioned will be retrieved.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 13:16:01 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Kozlov",
"G. A.",
""
]
] | [
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