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801.0873 | Alan Stapledon | Alan Stapledon | Inequalities and Ehrhart $\delta$-Vectors | 11 pages. v2: minor changes, more detailed proof of Lemma 2.12. To
appear in Trans. Amer. Math. Soc | Trans. Amer. Math. Soc. 361 (2009), 5615-5626. | null | null | math.CO | null | For any lattice polytope $P$, we consider an associated polynomial
$\bar{\delta}_{P}(t)$ and describe its decomposition into a sum of two
polynomials satisfying certain symmetry conditions. As a consequence, we
improve upon known inequalities satisfied by the coefficients of the Ehrhart
$\delta$-vector of a lattice polytope. We also provide combinatorial proofs of
two results of Stanley that were previously established using techniques from
commutative algebra. Finally, we give a necessary numerical criterion for the
existence of a regular unimodular lattice triangulation of the boundary of a
lattice polytope.
| [
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] | 2009-09-24T00:00:00 | [
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801.0874 | Rosa Orellana | Andrew Mathas and Rosa C. Orellana | Cyclotomic Solomon Algebras | null | null | null | null | math.CO math.RA math.RT | null | This paper introduces an analogue of the Solomon descent algebra for the
complex reflection groups of type $G(r,1,n)$. As with the Solomon descent
algebra, our algebra has a basis given by sums of `distinguished' coset
representatives for certain `reflection subgroups'. We explicitly describe the
structure constants with respect to this basis and show that they are
polynomials in $r$. This allows us to define a deformation, or $q$-analogue, of
these algebras which depends on a parameter $q$. We determine the irreducible
representations of all of these algebras and give a basis for their radicals.
Finally, we show that the direct sum of cyclotomic Solomon algebras is
canonically isomorphic to a concatenation Hopf algebra.
| [
{
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},
{
"version": "v2",
"created": "Fri, 9 May 2008 15:29:35 GMT"
}
] | 2008-05-09T00:00:00 | [
[
"Mathas",
"Andrew",
""
],
[
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"Rosa C.",
""
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801.0875 | David M. Fisher | David Fisher and Lior Silberman | Groups not acting on manifolds | References added, minor changes | null | null | null | math.DS math.DG math.GR | null | In this article we collect a series of observations that constrain actions of
many groups on compact manifolds. In particular, we show that "generic"
finitely generated groups have no smooth volume preserving actions on compact
manifolds while also producing many finitely presented, torsion free groups
with the same property.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 16:55:28 GMT"
},
{
"version": "v2",
"created": "Sat, 26 Jan 2008 20:43:07 GMT"
},
{
"version": "v3",
"created": "Thu, 15 May 2008 00:37:44 GMT"
}
] | 2008-05-15T00:00:00 | [
[
"Fisher",
"David",
""
],
[
"Silberman",
"Lior",
""
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801.0876 | Mensur Omerbashich | M. Omerbashich | Scale invariability | 7 pages, 1 figure. Expanded | null | null | null | physics.gen-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | I recently demonstrated that the Earth is a mechanical oscillator in which
springtide induced magnification of all-masses resonance forces tectonics. I
here generalize this georesonator concept so to make it apply to any body,
anywhere in all the universes, and at all times. It turns out that there is no
distinction between physics at intergalactic, mechanist, quantum, and smaller
scales. Instead of being a constant (of proportionality of physics at all
scales), G is a parameter of most general form: G = s e^2, nonlinearly varying
amongst different scales s. The so called scale variability of physics but not
of G, imagined as such by Planck and Einstein, is due to springtide-induced
extreme resonance of Earth masses critically impeding terrestrial experiments
for estimating G, while providing artificial settings for quantum experiments
to all trivially "work". Thus the derived equation is that of levitation.
Reality is a system of near infinitely many magnifying oscillators, where
permanent energy decay of all oscillation forbids constancy of known "physical
constants". This hyperresonator concept explains the magnetism (as every forced
oscillator feature), as well as the gravitation (as forward propagation of
mechanical vibrations along the aether i.e. throughout the vacuum structure).
To test my claim I propose a Space mission to collect on site measurements of
eigenperiods of the Sun, its planets, and their satellites. The levitation
equitation enables propulsionless Space travel via gravity sailing: Space
vehicle hull ought to be engineered so as to automatically adjust its grave
mode, to the vehicle instant gravitational surroundings, akin to trout up
swimming.
| [
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},
{
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801.0877 | Arnd Meyer | D0 Collaboration, V. Abazov, et al | Search for excited electrons in ppbar collisions at sqrt(s) = 1.96 TeV | 8 pages, 5 figures, submitted to Phys.Rev.D Rap.Comm | Phys.Rev.D77:091102,2008 | 10.1103/PhysRevD.77.091102 | Fermilab-Pub-08-007-E | hep-ex | null | We present the results of a search for the production of an excited state of
the electron, e*, in proton-antiproton collisions at sqrt(s) = 1.96 TeV. The
data were collected with the D0 experiment at the Fermilab Tevatron Collider
and correspond to an integrated luminosity of approximately 1 fb^-1. We search
for e* in the process ppbar -> e* e, with the e* subsequently decaying to an
electron plus photon. No excess above the standard model background is
observed. Interpreting our data in the context of a model that describes e*
production by four-fermion contact interactions and e* decay via electroweak
processes, we set 95% C.L. upper limits on the production cross section ranging
from 8.9 fb to 27 fb, depending on the mass of the excited electron. Choosing
the scale for contact interactions to be Lambda = 1 TeV, excited electron
masses below 756 GeV are excluded at the 95% C.L.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 17:28:04 GMT"
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] | 2008-11-26T00:00:00 | [
[
"D0 Collaboration",
"",
""
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"V.",
""
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801.0878 | Mitesh Patel Mr | M. Patel, R.D. Oudmaijer, J.S. Vink, J.E. Bjorkman, B. Davies, M.A.T.
Groenewegen, A.S. Miroshnichenko, J. C. Mottram | Spectropolarimetry of the Massive Post-Red Supergiants IRC +10420 and HD
179821 | 13 pages, 6 figures, MNRAS accepted | null | 10.1111/j.1365-2966.2008.12889.x | null | astro-ph | null | We present medium resolution spectropolarimetry and long term
photo-polarimetry of two massive post-red supergiants, IRC +10420 and HD
179821. The data provide new information on their circumstellar material as
well as their evolution. In IRC +10420, the polarization of the Halpha line is
different to that of the continuum, which indicates that the
electron-scattering region is not spherically symmetric. The observed long term
changes in the polarimetry can be associated with an axi-symmetric structure,
along the short axis of the extended reflection nebulosity. Long term
photometry reveals that the star increased in temperature until the
mid-nineties, after which the photospheric flux in the optical levelled off. As
the photometric changes are mostly probed in the red, they do not trace high
stellar temperatures sensitively. And so, it is not obvious whether the star
has halted its increase in temperature or not. For HD 179821 we find no
polarization effects across any absorption or emission lines, but observe very
large polarization changes of order 5% over 15 years. Unexpectedly, during the
same period, the optical photometry displayed modest variability at the 0.2
magnitude level. Several explanations for this puzzling fact are discussed.
Most of which, involving asymmetries in the circumstellar material, seem to
fail as there is no evidence for the presence of hot, dusty material close to
the star. Alternatively, the variations can be explained by the presence of a
non-radially pulsating photosphere. Changes in the photometry hint at an
increase in temperature corresponding to a change through two spectral
subclasses over the past ten years.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 17:44:44 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Patel",
"M.",
""
],
[
"Oudmaijer",
"R. D.",
""
],
[
"Vink",
"J. S.",
""
],
[
"Bjorkman",
"J. E.",
""
],
[
"Davies",
"B.",
""
],
[
"Groenewegen",
"M. A. T.",
""
],
[
"Miroshnichenko",
"A. S.",
""
],
[
"Mottram",
"J. C.",
""
]
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] |
801.0879 | Francesca Sammarruca | Francesca Sammarruca | Predicting the Lambda binding energy in nuclear matter | LaTeX, 8 pages | null | null | null | nucl-th | null | The purpose of this note is to report predictions of the binding energy of
the $\Lambda$ hyperon in nuclear matter using the latest version of the Juelich
nucleon-nucleon meson-exchange potential. Results from a conventional Brueckner
calculation are compared with previously reported values. A calculation
including Dirac effects on the $\Lambda$ single-particle potential is also
presented. Issues encountered in Dirac calculations with nucleon-hyperon
potentials are discussed.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 17:42:13 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Sammarruca",
"Francesca",
""
]
] | [
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] |
801.088 | Dipanjan Basu | D. Basu, M. J. Gilbert, L. F. Register and S. K. Banerjee | An Efficient Method for Quantum Transport Calculations in Nanostructures
using Full Band Structure | Additional simulations are being carried on to add to the results
section, mainly to investigate band-to-band tunneling in low band gap
semiconductors. The pre-print draft is however, complete from the perspective
of the quantum transport method that we illustrate | null | null | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | Scaling of semiconductor devices has reached a stage where it has become
absolutely imperative to consider the quantum mechanical aspects of transport
in these ultra small devices. In these simulations, often one excludes a
rigorous band structure treatment, since it poses a huge computational
challenge. We have proposed here an efficient method for calculating full
three-dimensionally coupled quantum transport in nanowire transistors including
full band structure. We have shown the power of the method by simulating hole
transport in p-type Ge nanowire transistors. The hole band structure obtained
from our nearest neighbor sp3s* tight binding Hamiltonian agrees well
qualitatively with more complex and accurate calculations that take third
nearest neighbors into account. The calculated I-V results show how shifting of
the energy bands due to confinement can be accurately captured only in a full
band full quantum simulation.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 17:50:19 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Basu",
"D.",
""
],
[
"Gilbert",
"M. J.",
""
],
[
"Register",
"L. F.",
""
],
[
"Banerjee",
"S. K.",
""
]
] | [
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801.0881 | Maria Chekhova Dr | I. N. Agafonov, M. V. Chekhova, T. Sh. Iskhakov, A. N. Penin | High-visibility multi-photon interference of Hanbury Brown - Twiss type
for classical light | 11 pages, 9 figures | null | 10.1103/PhysRevA.77.053801 | null | quant-ph | null | Difference-phase (or Hanbury Brown - Twiss type) intensity interference of
classical light is considered in higher orders in the intensity. It is shown
that, while the visibility of sum-phase (NOON-type) interference for classical
sources drops with the order of interference, the visibility of
difference-phase interference has opposite behavior. For three-photon and
four-photon interference of two coherent sources, the visibility can be as high
as 81.8% and 94.4%, respectively. High-visibility three-photon and four-photon
interference of space-time and polarization types has been observed in
experiment, for both coherent and pseudo-thermal light.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 18:05:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Agafonov",
"I. N.",
""
],
[
"Chekhova",
"M. V.",
""
],
[
"Iskhakov",
"T. Sh.",
""
],
[
"Penin",
"A. N.",
""
]
] | [
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] |
801.0882 | Nina Bohr | Neil D. Jones and Nina Bohr | Call-by-value Termination in the Untyped lambda-calculus | null | Logical Methods in Computer Science, Volume 4, Issue 1 (March 17,
2008) lmcs:915 | 10.2168/LMCS-4(1:3)2008 | null | cs.PL | null | A fully-automated algorithm is developed able to show that evaluation of a
given untyped lambda-expression will terminate under CBV (call-by-value). The
``size-change principle'' from first-order programs is extended to arbitrary
untyped lambda-expressions in two steps. The first step suffices to show CBV
termination of a single, stand-alone lambda;-expression. The second suffices to
show CBV termination of any member of a regular set of lambda-expressions,
defined by a tree grammar. (A simple example is a minimum function, when
applied to arbitrary Church numerals.) The algorithm is sound and proven so in
this paper. The Halting Problem's undecidability implies that any sound
algorithm is necessarily incomplete: some lambda-expressions may in fact
terminate under CBV evaluation, but not be recognised as terminating.
The intensional power of the termination algorithm is reasonably high. It
certifies as terminating many interesting and useful general recursive
algorithms including programs with mutual recursion and parameter exchanges,
and Colson's ``minimum'' algorithm. Further, our type-free approach allows use
of the Y combinator, and so can identify as terminating a substantial subset of
PCF.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 19:01:02 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Mar 2008 12:55:44 GMT"
}
] | 2015-07-01T00:00:00 | [
[
"Jones",
"Neil D.",
""
],
[
"Bohr",
"Nina",
""
]
] | [
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801.0883 | James D. Meiss | J.D. Meiss | Visual Explorations of Dynamics: the Standard Map | Corrections in a couple of equations, and updated to the latest
version of StdMap | Pramana, Indian Academy of Sciences 70: 965-988 (2008) | 10.1007/s12043-008-0103-3 | null | nlin.CD | null | The Macintosh application \textit{StdMap} allows easy exploration of many of
the phenomena of area-preserving mappings. This tutorial explains some of these
phenomena and presents a number of simple experiments centered on the use of
this program.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 18:39:23 GMT"
},
{
"version": "v2",
"created": "Mon, 12 May 2008 22:05:07 GMT"
}
] | 2010-02-19T00:00:00 | [
[
"Meiss",
"J. D.",
""
]
] | [
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801.0884 | Vivek Rane V | Vivek V. Rane | Instant Evaluation and Demystification of $\zeta(n),L(n,\chi)$ that
Euler,Ramanujan Missed - I | 19 pages | null | null | null | math.NT | null | For Hurwitz Zeta function,we consider its Taylor series expansion about
various points as an analytic function of second variable in appropriate
discs.We show that these Taylor are all polynomials in second variable for a
non positive integral argument in first variable.On using functionalequations
this results in instant evaluation of Riemann Zeta function at positive even
integral values of its argument and of Dirichlet L series at positive integral
values of its argument,when the argument and the corresponding Dirichlet
character are both even or both odd.We also obtain finite sum expression for
any Dirichlet L series,when its argument is one.We also deal with Lerch's Zeta
function on similar lines.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 18:48:54 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Rane",
"Vivek V.",
""
]
] | [
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] |
801.0885 | Yury Eroshenko | V.I. Dokuchaev, Yu.N. Eroshenko, S.G. Rubin | Early formation of galaxies initiated by clusters of primordial black
holes | 13 pages, 5 figures, accepted for publication in Astron. Rep.
(Astronomicheskii Zhurnal) | Astron.Rep.52:779-789,2008 | 10.1134/S1063772908100016 | null | astro-ph | null | Model of supermassive black holes formation inside the clusters of primordial
black holes is developed. Namely, it is supposed, that some mass fraction of
the universe ~10^-3 is composed of the compact clusters of primordial (relic)
black holes, produced during phase transitions in the early universe. These
clusters are the centers of dark matter condensation. We model the formation of
protogalaxies with masses about 2*10^8M_sun at the redshift z=15. These induced
protogalaxies contain central black holes with mass ~10^5M_sun and look like
dwarf spheroidal galaxies with central density spike. The subsequent merging of
induced protogalaxies and ordinary dark matter haloes corresponds to the
standard hierarchical clustering scenario of large-scale structure formation.
The coalescence of primordial black holes results in formation of supermassive
black holes in the galactic centers. As a result, the observed correlation
between the masses of central black holes and velocity dispersion in the
galactic bulges is reproduced.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 19:01:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dokuchaev",
"V. I.",
""
],
[
"Eroshenko",
"Yu. N.",
""
],
[
"Rubin",
"S. G.",
""
]
] | [
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] |
801.0886 | Andrew Rushforth | A.W. Rushforth, E. De Ranieri, J. Zemen, J. Wunderlich, K.W. Edmonds,
C.S. King, E. Ahmad, R.P. Campion, C.T. Foxon, B.L. Gallagher, K. Vyborny, J.
Kucera, T. Jungwirth | Voltage control of magnetocrystalline anisotropy in ferromagnetic -
semiconductor/piezoelectric hybrid structures | Submitted to Physical Review Letters. Updates version 1 to include a
more detailed discussion of the effect of strain on the anisotropic
magnetoresistance | Physical Review B 78, 085314 (2008) | 10.1103/PhysRevB.78.085314 | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | We demonstrate dynamic voltage control of the magnetic anisotropy of a
(Ga,Mn)As device bonded to a piezoelectric transducer. The application of a
uniaxial strain leads to a large reorientation of the magnetic easy axis which
is detected by measuring longitudinal and transverse anisotropic
magnetoresistance coefficients. Calculations based on the mean-field
kinetic-exchange model of (Ga,Mn)As provide microscopic understanding of the
measured effect. Electrically induced magnetization switching and detection of
unconventional crystalline components of the anisotropic magnetoresistance are
presented, illustrating the generic utility of the piezo voltage control to
provide new device functionalities and in the research of micromagnetic and
magnetotransport phenomena in diluted magnetic semiconductors.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 19:19:35 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 14:25:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rushforth",
"A. W.",
""
],
[
"De Ranieri",
"E.",
""
],
[
"Zemen",
"J.",
""
],
[
"Wunderlich",
"J.",
""
],
[
"Edmonds",
"K. W.",
""
],
[
"King",
"C. S.",
""
],
[
"Ahmad",
"E.",
""
],
[
"Campion",
"R. P.",
""
],
[
"Foxon",
"C. T.",
""
],
[
"Gallagher",
"B. L.",
""
],
[
"Vyborny",
"K.",
""
],
[
"Kucera",
"J.",
""
],
[
"Jungwirth",
"T.",
""
]
] | [
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0.1009806991,
-0.0609058402,
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] |
801.0887 | Ignazio Licata | Ignazio Licata | A Dynamical Model for Information Retrieval and Emergence of Scale-Free
Clusters in a Long Term Memory Network | 8 pages, 11 figures, 2 tables. Submitted to Emergence: Complexity and
Organization | null | null | null | physics.gen-ph nlin.AO | null | The classical forms of knowledge representation fail when a strong dynamical
interconnection between system and environment comes into play. We propose here
a model of information retrieval derived from the Kintsch-Ericsson scheme,
based upon a long term memory (LTM) associative net whose structure changes in
time according to the textual content of the analyzed documents. Both the
theoretical analysis carried out by using simple statistical tools and the
tests show the appearing of typical power-laws and the net configuration as a
scale-free graph. The information retrieval from LTM shows that the entire
system can be considered to be an information amplifier which leads to the
emergence of new cognitive structures. It has to be underlined that the
expanding of the semantic domain regards the user-network as a whole system.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 19:31:10 GMT"
}
] | 2010-04-26T00:00:00 | [
[
"Licata",
"Ignazio",
""
]
] | [
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801.0888 | Congjun Wu | Congjun Wu | Orbital ordering and frustration of $p$-band Mott-insulators | accepted by Phys. Rev. Lett | Phys. Rev. Lett. 100, 200406 (2008) | 10.1103/PhysRevLett.100.200406 | null | cond-mat.str-el cond-mat.stat-mech | null | We investigate the general structure of orbital exchange physics in
Mott-insulating states of $p$-orbital systems in optical lattices. Orbital
orders occur in both the triangular and Kagome lattices. In contrast, orbital
exchange in the honeycomb lattice is frustrated as described by a novel quantum
120$^\circ$-model. Its classical ground states are mapped into configurations
of the fully-packed loop model with an extra U(1) rotation degree of freedom.
Quantum orbital fluctuations select a six-site plaquette ground state ordering
pattern in the semiclassical limit from the ``order from disorder'' mechanism.
This effect arises from the appearance of a zero energy flat-band of orbital
excitations.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 20:38:11 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 19:04:49 GMT"
},
{
"version": "v3",
"created": "Sun, 2 Mar 2008 22:54:39 GMT"
},
{
"version": "v4",
"created": "Wed, 30 Apr 2008 04:21:07 GMT"
}
] | 2008-06-07T00:00:00 | [
[
"Wu",
"Congjun",
""
]
] | [
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801.0889 | Kirill Bronnikov | K.A. Bronnikov, O.B. Zaslavskii | Black holes can have curly hair | 5 pages, no figures. Some discussion added, misprints corrected | Phys.Rev.D78:021501,2008 | 10.1103/PhysRevD.78.021501 | null | gr-qc astro-ph hep-th | null | We study equilibrium conditions between a static, spherically symmetric black
hole and classical matter in terms of the radial pressure to density ratio
p_r/\rho = w(u), where u is the radial coordinate. It is shown that such an
equilibrium is possible in two cases: (i) the well-known case w\to -1 as $u\to
u_h (the horizon), i.e., "vacuum" matter, for which \rho(u_h) can be nonzero;
(ii) w \to -1/(1+2k) and \rho \sim (u-u_h)^k as u\to u_h, where k>0 is a
positive integer (w=-1/3 in the generic case k=1). A non-interacting mixture of
these two kinds of matter can also exist. The whole reasoning is local, hence
the results do not depend on any global or asymptotic conditions. They mean, in
particular, that a static black hole cannot live inside a star with nonnegative
pressure and density. As an example, an exact solution for an isotropic fluid
with w = -1/3 (that is, a fluid of disordered cosmic strings), with or without
vacuum matter, is presented.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 21:43:27 GMT"
},
{
"version": "v2",
"created": "Thu, 29 May 2008 19:58:24 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bronnikov",
"K. A.",
""
],
[
"Zaslavskii",
"O. B.",
""
]
] | [
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] |
801.089 | Jose Carlos Bermejo-Barrera | Jose Carlos Bermejo-Barrera | A Narration is Not an Equation: Metaphysical Principals of Standard
Cosmology | 30 pages | null | null | null | physics.gen-ph | null | In this paper the author maintains that the Standard Cosmology is not a
Physical Theory. The Standard Cosmology is a narration similar to the
historical or mythical narratives constructed from the Physical Sciences data.
Also the author maintains that this theory is founded on Philosophical
principles which are aliens to the Physical Theory, as the Principle of
Sufficient Reason. The author porpoise a new cosmological model based more on
eventuality than in necessity.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 21:57:53 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Bermejo-Barrera",
"Jose Carlos",
""
]
] | [
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801.0891 | David Broadhurst | David H. Bailey, Jonathan M. Borwein, David Broadhurst and M. L.
Glasser | Elliptic integral evaluations of Bessel moments | 51 pages, 1 Postscript figure, uses amsmath.sty, added references | J. Phys. A: Math. Theor. 41 (2008) 205203 | 10.1088/1751-8113/41/20/205203 | null | hep-th hep-ph math-ph math.MP | null | We record what is known about the closed forms for various Bessel function
moments arising in quantum field theory, condensed matter theory and other
parts of mathematical physics. More generally, we develop formulae for
integrals of products of six or fewer Bessel functions. In consequence, we are
able to discover and prove closed forms for $c_{n,k}:=\int_0^\infty t^k
K_0^n(t) {\rm d}t$ with integers $n=1,2,3,4$ and $k\ge0$, obtaining new results
for the even moments $c_{3,2k}$ and $c_{4,2k}$. We also derive new closed forms
for the odd moments $s_{n,2k+1}:=\int_0^\infty t^{2k+1}I_0^{}(t) K_0^{n-1}(t)
{\rm d}t$ with $n=3,4$ and for $t_{n,2k+1}:=\int_0^\infty t^{2k+1}I_0^2(t)
K_0^{n-2}(t) {\rm d}t$ with $n=5$, relating the latter to Green functions on
hexagonal, diamond and cubic lattices. We conjecture the values of
$s_{5,2k+1}$, make substantial progress on the evaluation of $c_{5,2k+1}$,
$s_{6,2k+1}$ and $t_{6,2k+1}$ and report more limited progress regarding
$c_{5,2k}$, $c_{6,2k+1}$ and $c_{6,2k}$. In the process, we obtain 8
conjectural evaluations, each of which has been checked to 1200 decimal places.
One of these lies deep in 4- dimensional quantum field theory and two are
probably provable by delicate combinatorics. There remains a hard core of five
conjectures whose proofs would be most instructive, to mathematicians and
physicists alike.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 22:15:49 GMT"
},
{
"version": "v2",
"created": "Fri, 8 Feb 2008 01:17:55 GMT"
}
] | 2008-04-29T00:00:00 | [
[
"Bailey",
"David H.",
""
],
[
"Borwein",
"Jonathan M.",
""
],
[
"Broadhurst",
"David",
""
],
[
"Glasser",
"M. L.",
""
]
] | [
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801.0892 | A. Lewis Licht | A. Lewis Licht | Gauge Fields and Unparticles | 7 pages v2: Typographical error in Eq. (30) corrected | null | null | null | hep-th | null | We show that a rigorous path integral method of introducing gauge fields in
the UnParticle lagrangian leads to somewhat different and more complicated
vertexes than those currently used.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 23:52:14 GMT"
},
{
"version": "v2",
"created": "Sun, 3 Feb 2008 23:13:09 GMT"
}
] | 2008-02-04T00:00:00 | [
[
"Licht",
"A. Lewis",
""
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] |
801.0893 | Gwen Rudie | G. C. Rudie, R. A. Fesen, and T. Yamada | The Crab Nebula's Dynamical Age as Measured from its Northern
Filamentary Jet | 8 pages, 5 figures, Accepted to MNRAS | null | 10.1111/j.1365-2966.2007.12799.x | null | astro-ph | null | We present a deep [O III] 4959,5007 image of the northern filamentary jet in
the Crab Nebula taken with the 8.2m Subaru telescope. Using this image and an
image taken with the KPNO 4m in 1988 (Fesen & Staker 1993), we have computed
proper motions for 35 locations in the jet. The results suggest that when
compared to the main body of the remnant, the jet experienced less outward
acceleration from the central pulsar's rapidly expanding synchrotron nebula.
The jet's apparent expansion rate yields an undecelerated explosion date for
the Crab Nebula of 1055 plus or minus 24 C.E., a date much closer to the
appearance of the historic 1054 C.E. guest star than the 1120 - 1140 C.E. dates
estimated in previous studies using filaments located within the remnant's main
nebula. Our proper motion measurements suggest the jet likely formed during the
1054 supernova explosion and represents the remnant's highest velocity knots
possibly associated with a suspected N-S bipolar outflow from the supernova
explosion.
| [
{
"version": "v1",
"created": "Sun, 6 Jan 2008 23:58:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rudie",
"G. C.",
""
],
[
"Fesen",
"R. A.",
""
],
[
"Yamada",
"T.",
""
]
] | [
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] |
801.0894 | EDA Publishing Association | C. S. Yu, W. C. Wei, S. W. Kang | Investigation of Micro Porosity Sintered wick in Vapor Chamber for Fan
Less Design | Submitted on behalf of TIMA Editions
(http://irevues.inist.fr/tima-editions) | Dans 13th International Worshop on THERMal INvestigations of ICs
and Systems - THERMINIC 2007, Budapest : Hongrie (2007) | null | null | physics.gen-ph | null | Micro Porosity Sintered wick is made from metal injection molding processes,
which provides a wick density with micro scale. It can keep more than 53 %
working fluid inside the wick structure, and presents good pumping ability on
working fluid transmission by fine infiltrated effect. Capillary pumping
ability is the important factor in heat pipe design, and those general
applications on wick structure are manufactured with groove type or screen
type. Gravity affects capillary of these two types more than a sintered wick
structure does, and mass heat transfer through vaporized working fluid
determines the thermal performance of a vapor chamber. First of all, high
density of porous wick supports high transmission ability of working fluid. The
wick porosity is sintered in micro scale, which limits the bubble size while
working fluid vaporizing on vapor section. Maximum heat transfer capacity
increases dramatically as thermal resistance of wick decreases. This study on
permeability design of wick structure is 0.5 - 0.7, especially permeability (R)
= 0.5 can have the best performance, and its heat conductivity is 20 times to a
heat pipe with diameter (Phi) = 10mm. Test data of this vapor chamber shows
thermal performance increases over 33 %.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 16:41:09 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Yu",
"C. S.",
""
],
[
"Wei",
"W. C.",
""
],
[
"Kang",
"S. W.",
""
]
] | [
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] |
801.0895 | Yeo Woong Yoon | Chuan-Hung Chen, C. S. Kim, Yeo Woong Yoon | Investigation of $B_{u,d}\to (\pi, K) \pi$ decays within unparticle
physics | Analysis on mixing part is revised | Phys.Lett.B671:250-255,2009 | 10.1016/j.physletb.2008.12.007 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the implication of unparticle physics on the B_{u,d}\to (\pi,
K) \pi decays under the constraints of the B_{d,s}-\bar B_{d,s} mixing. We
found that not only the unparticle parameters that belong to the flavor
changing neutral current (FCNC) processes but also scaling dimension d_{\UP}
could be constrained by the B_{d,s}-\bar B_{d,s} mixing phenomenology.
Employing the minimum \chi^2 analysis to the B_{u,d}\to (\pi, K) \pi decays
with the constraints of B_{d,s} mixing, we find that the puzzle of large
branching ratio for B_{d}\to \pi^0 \pi^0 and the discrepancy between the
standard model estimation and data for the direct CP asymmetry of B^+ \to K^+
\pi^0 and B_d \to \pi^+\pi^- can be resolved well. However, the mixing induced
CP asymmetry of B_d\to K_S \pi^0 could not be well accommodated by the
unparticle contributions.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 01:07:18 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 08:44:29 GMT"
},
{
"version": "v3",
"created": "Mon, 15 Dec 2008 00:25:14 GMT"
}
] | 2009-01-14T00:00:00 | [
[
"Chen",
"Chuan-Hung",
""
],
[
"Kim",
"C. S.",
""
],
[
"Yoon",
"Yeo Woong",
""
]
] | [
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] |
801.0896 | Bobby Eka Gunara | Bobby E. Gunara and Freddy P. Zen (ITB and ICTMP) | Deformation of Curved BPS Domain Walls and Supersymmetric Flows on 2d
K\"ahler-Ricci Soliton | 19 pages, no figures. Typos corrected. Published version | Commun.Math.Phys.287:849-866,2009 | 10.1007/s00220-009-0744-1 | null | hep-th math-ph math.DG math.DS math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider some aspects of the curved BPS domain walls and their
supersymmetric Lorentz invariant vacua of the four dimensional N=1 supergravity
coupled to a chiral multiplet. In particular, the scalar manifold can be viewed
as a two dimensional K\"ahler-Ricci soliton generating a one-parameter family
of K\"ahler manifolds evolved with respect to a real parameter, $\tau$. This
implies that all quantities describing the walls and their vacua indeed evolve
with respect to $\tau$. Then, the analysis on the eigenvalues of the first
order expansion of BPS equations shows that in general the vacua related to the
field theory on a curved background do not always exist. In order to verify
their existence in the ultraviolet or infrared regions one has to perform the
renormalization group analysis. Finally, we discuss in detail a simple model
with a linear superpotential and the K\"ahler-Ricci soliton considered as the
Rosenau solution.
| [
{
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},
{
"version": "v4",
"created": "Fri, 13 Mar 2009 10:28:39 GMT"
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] | 2009-03-24T00:00:00 | [
[
"Gunara",
"Bobby E.",
"",
"ITB and ICTMP"
],
[
"Zen",
"Freddy P.",
"",
"ITB and ICTMP"
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801.0897 | Jordan Bell | Leonhard Euler | A more accurate treatment of the problem of drawing the shortest line on
a surface | 10 pages; E727 in the Enestrom index | null | null | null | math.HO math.CA | null | E727 in the Enestrom index. This is a translation from the Latin original
"Accuratior evolutio problematis de linea brevissima in superficie quacunque
ducenda" (1779). Given a surface $pdx+qdy+rdz=0$, Euler wants to develop
equations that give the geodesics on this surface. I am new to the calculus of
variations, so it is not clear to me what steps follow from results that are
previously known (like the Euler-Lagrange equation in the calculations) and
what steps follow from earlier in this paper. I would appreciate comments from
any readers who are familiar with calculus of variations.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 02:31:23 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Euler",
"Leonhard",
""
]
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801.0898 | Juan Carlos Martinez Oliveros JCMO | J.C. Martinez-Oliveros, H. Moradi, A-C. Donea | Seismic Emissions from a Highly Impulsive M6.7 Solar Flare | 16 pages, 7 figures, Solar Physics Topical Issue: SOHO 19/GONG 2007
"Seismology of Magnetic Activity", Accepted | null | 10.1007/s11207-008-9122-y | null | astro-ph | null | On 10 March 2001 the active region NOAA 9368 produced an unusually impulsive
solar flare in close proximity to the solar limb. This flare has previously
been studied in great detail, with observations classifying it as a type 1
white-light flare with a very hard spectrum in hard X-rays. The flare was also
associated with a type II radio burst and coronal mass ejection. The flare
emission characteristics appeared to closely correspond with previous instances
of seismic emission from acoustically active flares. Using standard local
helioseismic methods, we identified the seismic signatures produced by the
flare that, to date, is the least energetic (in soft X-rays) of the flares
known to have generated a detectable acoustic transient. Holographic analysis
of the flare shows a compact acoustic source strongly correlated with the
impulsive hard X-ray, visible continuum, and radio emission. Time-distance
diagrams of the seismic waves emanating from the flare region also show faint
signatures, mainly in the eastern sector of the active region. The strong
spatial coincidence between the seismic source and the impulsive visible
continuum emission reinforces the theory that a substantial component of the
seismic emission seen is a result of sudden heating of the low photosphere
associated with the observed visible continuum emission. Furthermore, the
low-altitude magnetic loop structure inferred from potential--field
extrapolations in the flaring region suggests that there is a significant
inverse correlation between the seismicity of a flare and the height of the
magnetic loops that conduct the particle beams from the corona.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 03:01:30 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 05:08:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Martinez-Oliveros",
"J. C.",
""
],
[
"Moradi",
"H.",
""
],
[
"Donea",
"A-C.",
""
]
] | [
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801.0899 | EDA Publishing Association | F. Stefani, P.E. Bagnoli, S. Luschi | Study of Water Speed Sensitivity in a Multifunctional Thick-film Sensor
by Analytical Thermal Simulations and Experiments | Submitted on behalf of TIMA Editions
(http://irevues.inist.fr/tima-editions) | Dans 13th International Worshop on THERMal INvestigations of ICs
and Systems - THERMINIC 2007, Budapest : Hongrie (2007) | null | null | physics.gen-ph | null | The present paper deals with an application of the analytical thermal
simulator DJOSER. It consist of the characterization of a water speed sensor
realized in hybrid technology. The capability of the thermal solver to manage
the convection heat exchange and the effects of the passivating layers make the
simulation work easy and fast.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 16:40:35 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Stefani",
"F.",
""
],
[
"Bagnoli",
"P. E.",
""
],
[
"Luschi",
"S.",
""
]
] | [
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] |
801.09 | Chad Galley | Chad R. Galley and B. L. Hu | Self-force on extreme mass ratio inspirals via curved spacetime
effective field theory | 22 pages, 5 figures; references added, revised Appendices B & C,
corrected typos, revisions throughout for clarification particularly in
Section IV.B; submitted to PRD | Phys.Rev.D79:064002,2009 | 10.1103/PhysRevD.79.064002 | null | gr-qc astro-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this series we construct an effective field theory (EFT) in curved
spacetime to study gravitational radiation and backreaction effects. We begin
in this paper with a derivation of the self-force on a compact object moving in
the background spacetime of a supermassive black hole. The EFT approach
utilizes the disparity between two length scales, which in this problem are the
size of the compact object and the radius of curvature of the background
spacetime, to treat the orbital dynamics of the compact object, described as an
effective point particle, separately from its tidal deformations. Ultraviolet
divergences are regularized using Hadamard's {\it partie finie} to isolate the
non-local finite part from the quasi-local divergent part. The latter is
constructed from a momentum space representation for the graviton retarded
propagator and is evaluated using dimensional regularization in which only
logarithmic divergences are relevant for renormalizing the parameters of the
theory. As a first important application of this framework we explicitly derive
the first order self-force given by Mino, Sasaki, Tanaka, Quinn and Wald. Going
beyond the point particle approximation, to account for the finite size of the
object, we demonstrate that for extreme mass ratio inspirals the motion of a
compact object is affected by tidally induced moments at $O(\epsilon^4)$, in
the form of an Effacement Principle. The relatively large radius-to-mass ratio
of a white dwarf star allows for these effects to be enhanced until the white
dwarf becomes tidally disrupted, a potentially $O(\epsilon^2)$ process, or
plunges into the supermassive black hole. This work provides a new foundation
for further exploration of higher order self force corrections, gravitational
radiation and spinning compact objects.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 04:39:26 GMT"
},
{
"version": "v2",
"created": "Thu, 5 Jun 2008 15:10:49 GMT"
}
] | 2009-03-12T00:00:00 | [
[
"Galley",
"Chad R.",
""
],
[
"Hu",
"B. L.",
""
]
] | [
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] |
801.0901 | Taylor Hughes | Markus Koenig, Hartmut Buhmann, Laurens W. Molenkamp, Taylor L.
Hughes, Chao-Xing Liu, Xiao-Liang Qi and Shou-Cheng Zhang | The Quantum Spin Hall Effect: Theory and Experiment | Invited review article for special issue of JPSJ, 32 pages. For
higher resolution figures see official online version when published | null | 10.1143/JPSJ.77.031007 | null | cond-mat.mes-hall | null | The search for topologically non-trivial states of matter has become an
important goal for condensed matter physics. Recently, a new class of
topological insulators has been proposed. These topological insulators have an
insulating gap in the bulk, but have topologically protected edge states due to
the time reversal symmetry. In two dimensions the helical edge states give rise
to the quantum spin Hall (QSH) effect, in the absence of any external magnetic
field. Here we review a recent theory which predicts that the QSH state can be
realized in HgTe/CdTe semiconductor quantum wells. By varying the thickness of
the quantum well, the band structure changes from a normal to an "inverted"
type at a critical thickness $d_c$. We present an analytical solution of the
helical edge states and explicitly demonstrate their topological stability. We
also review the recent experimental observation of the QSH state in
HgTe/(Hg,Cd)Te quantum wells. We review both the fabrication of the sample and
the experimental setup. For thin quantum wells with well width $d_{QW}< 6.3$
nm, the insulating regime shows the conventional behavior of vanishingly small
conductance at low temperature. However, for thicker quantum wells ($d_{QW}>
6.3$ nm), the nominally insulating regime shows a plateau of residual
conductance close to $2e^2/h$. The residual conductance is independent of the
sample width, indicating that it is caused by edge states. Furthermore, the
residual conductance is destroyed by a small external magnetic field. The
quantum phase transition at the critical thickness, $d_c= 6.3$ nm, is also
independently determined from the occurrence of a magnetic field induced
insulator to metal transition.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 05:35:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Koenig",
"Markus",
""
],
[
"Buhmann",
"Hartmut",
""
],
[
"Molenkamp",
"Laurens W.",
""
],
[
"Hughes",
"Taylor L.",
""
],
[
"Liu",
"Chao-Xing",
""
],
[
"Qi",
"Xiao-Liang",
""
],
[
"Zhang",
"Shou-Cheng",
""
]
] | [
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] |
801.0902 | Junichiro Yasuda | Junichiro Yasuda | An analytic study of the tricritical line in the U(Nf)xU(Nf) sigma model | 14 pages | null | null | UT-Komaba/08-1 | hep-ph nucl-th | null | The tricritical line of the first-order chiral phase transition is
investigated in the U(Nf)xU(Nf) sigma model by means of the ring improved
one-loop finite temperature effective potential. To locate the tricritical line
in the space of the coupling constants, we expand the effective potential up to
third order in the high temperature expansion, and up to sixth order in the
order parameter expansion. In this approximation, the tricritical line can be
evaluated to the lowest order of the coupling constants and it follows an
analytic relation between the tree-level masses of the scalar bosons. The
validity of the high temperature expansion, the order parameter expansion, and
the ring improved perturbation is critically examined. This result does not
alter if one includes the massless fermions with the small Yukawa couplings.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:39:33 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Mar 2008 11:35:34 GMT"
}
] | 2008-03-19T00:00:00 | [
[
"Yasuda",
"Junichiro",
""
]
] | [
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] |
801.0903 | Vyacheslav Futorny | Vyacheslav Futorny, Alexander Molev, Serge Ovsienko | Gelfand-Kirillov Conjecture and Harish-Chandra Modules for Finite
W-Algebras | null | null | null | null | math.RA math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We address two problems regarding the structure and representation theory of
finite W-algebras associated with the general linear Lie algebras. Finite
W-algebras can be defined either via the Whittaker model of Kostant or,
equivalently, by the quantum Hamiltonian reduction. Our first main result is a
proof of the Gelfand-Kirillov conjecture for the skew fields of fractions of
the finite W-algebras. The second main result is a parametrization of finite
families of irreducible Harish-Chandra modules by the characters of the
Gelfand-Tsetlin subalgebra. As a corollary, we obtain a complete classification
of generic irreducible Harish-Chandra modules for the finite W-algebras.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 05:26:56 GMT"
},
{
"version": "v2",
"created": "Sat, 12 Jan 2008 20:40:39 GMT"
},
{
"version": "v3",
"created": "Sat, 6 Jun 2009 00:09:45 GMT"
}
] | 2009-06-06T00:00:00 | [
[
"Futorny",
"Vyacheslav",
""
],
[
"Molev",
"Alexander",
""
],
[
"Ovsienko",
"Serge",
""
]
] | [
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] |
801.0904 | Hvedri Inassaridze | Alastair Hamilton and Andrey Lazarev | Characteristic classes of $\ai$-algebras | To be published in "Journal of Homotopy and Related Structures" | null | null | null | math.AT | null | Standard combinatorial construction, due to Kontsevich, associates to any
$\ai$-algebra with an invariant inner product, an inhomogeneous class in the
cohomology of the moduli spaces of Riemann surfaces with marked points. We
propose an alternative version of this construction based on noncommutative
geometry and use it to prove that homotopy equivalent algebras give rise to the
same cohomology classes. Along the way we re-prove Kontsevich's theorem
relating graph homology to the homology of certain infinite dimensional Lie
algebras. An application to topological conformal field theories is given.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 05:29:13 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Hamilton",
"Alastair",
""
],
[
"Lazarev",
"Andrey",
""
]
] | [
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] |
801.0905 | Haiqing Zhang | Chao-Guang Huang, Hai-Qing Zhang, Han-Ying Guo | Cosmological Solutions with Torsion in a Model of de Sitter Gauge Theory
of Gravity | 16 pages, 2 figures | JCAP 0810:010,2008 | 10.1088/1475-7516/2008/10/010 | null | gr-qc | null | The torsion is shown to be vitally important in the explanation of the
evolution of the universe in a large class of gravitational theories containing
quadratic terms of curvature and torsion. The cosmological solutions with
homogeneous and isotropic torsion in a model of de Sitter gauge theory of
gravity are presented, which may explain the observation data for SN Ia when
parameters are suitably chosen and supply a natural transit from decelerating
expansion to accelerating expansion without the help of the introduction of
other strange fields in the theory.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 05:34:48 GMT"
}
] | 2011-07-19T00:00:00 | [
[
"Huang",
"Chao-Guang",
""
],
[
"Zhang",
"Hai-Qing",
""
],
[
"Guo",
"Han-Ying",
""
]
] | [
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] |
801.0906 | Kin Hung Fung | Yu-Rong Zhen, Kin Hung Fung, C. T. Chan | Collective plasmonic modes of metal nano-particles in two-dimensional
periodic regular arrays | 26 pages, 8 figures | Phys. Rev. B 78, 035419 (2008) | 10.1103/PhysRevB.78.035419 | null | physics.optics cond-mat.mes-hall | null | We investigate the collective plasmonic modes of metal nano-particles in
periodic two-dimensional (2D) arrays within a point-dipole description. As an
open system, the full-dynamic dispersion relations of the 2D arrays are
obtained through an efficient method which gives an effective polarizability
describing the collective response of a system. Both the dispersion relations
and mode qualities are simultaneously related to the imaginary part of the
effective polarizability, which has contributions from the single-particle
response as well as the inter-particle coupling. The transversal long-range
dipolar interaction is dominated by a wave term together with a purely
geometrical constant representing the static geometrical contribution to
resonant frequencies. As concrete examples, we considered small Ag spheres
arranged in a square lattice. We find that inside the light-cone, the
transverse quasi-mode has a reasonably high mode quality while the two in-plane
modes show significant radiation damping. Near the light-line, we observe
strong coupling with free photons for the bands of the transverse mode and the
transversal in-plane mode, and the longitudinal in-plane mode exhibits a
negative group-velocity inside the light-cone. Vanishing group velocities in
the light-cone for all the quasi-modes are found to be intrinsic properties of
the 2D metal nano-sphere dense arrays.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:07:34 GMT"
}
] | 2016-07-29T00:00:00 | [
[
"Zhen",
"Yu-Rong",
""
],
[
"Fung",
"Kin Hung",
""
],
[
"Chan",
"C. T.",
""
]
] | [
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] |
801.0907 | Taku Takeuchi | Taku Takeuchi and Oliver Krauss | Photophoretic Structuring of Circumstellar Dust Disks | 15 pages, 9 figures, Accepted by ApJ; corrected a typo in the author
name | null | 10.1086/527426 | null | astro-ph | null | We study dust accumulation by photophoresis in optically thin gas disks.
Using formulae of the photophoretic force that are applicable for the free
molecular regime and for the slip-flow regime, we calculate dust accumulation
distances as a function of the particle size. It is found that photophoresis
pushes particles (smaller than 10 cm) outward. For a Sun-like star, these
particles are transported to 0.1-100 AU, depending on the particle size, and
forms an inner disk. Radiation pressure pushes out small particles (< 1 mm)
further and forms an extended outer disk. Consequently, an inner hole opens
inside ~0.1 AU. The radius of the inner hole is determined by the condition
that the mean free path of the gas molecules equals the maximum size of the
particles that photophoresis effectively works on (100 micron - 10 cm,
depending on the dust property). The dust disk structure formed by
photophoresis can be distinguished from the structure of gas-free dust disk
models, because the particle sizes of the outer disks are larger, and the inner
hole radius depends on the gas density.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 06:28:48 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 00:46:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Takeuchi",
"Taku",
""
],
[
"Krauss",
"Oliver",
""
]
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] |
801.0908 | Ming-Yong Ye | Ming-Yong Ye and Xiu-Min Lin | A genuine four-partite entangled state | submitted | Physics Letters A 372 (2008) 4157-4159 | 10.1016/j.physleta.2008.03.035 | null | quant-ph | null | In a recent paper, a genuine four-partite entangled state is proposed [Y. Yeo
and W. K. Chua, Phys. Rev. Lett. 96, 060502 (2006)], which has been found to
have many interesting entanglement properties. We show this state is locally
equivalent to some graph states.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:54:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ye",
"Ming-Yong",
""
],
[
"Lin",
"Xiu-Min",
""
]
] | [
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] |
801.0909 | Yi Chou | Y. Chou, Y. Chung, C. P. Hu and T. C. Yang (National Central
University) | Precise Orbital Parameters and Anomalous Phase Variations of the
Accretion-powered Millisecond Pulsar XTE J1807-294 | 26 pages, 8 figures, accepted by ApJ | null | 10.1086/529126 | null | astro-ph | null | This study reports pulse variation analysis results for the forth discovered
accretion-powered millisecond pulsar XTE J1807-294 during its 2003 outburst
observed by {\it Rossi X-ray Timing Explorer}. The pulsation is significantly
detected only in the first $\sim$90d out of $\sim$150d observations. The pulse
phase variation is too complex to be described as an orbital motion plus a
simple polynomial model. The precise orbital parameters with
$P_{orb}=40.073601(8)$ min and ${\it a_x}\sin {\it i}=4.823(5)$ lt-ms were
obtained after applying the trend removal to the daily observed 150s segments
pulse phases folded with a constant spin frequency without Keplerian orbit
included. The binary barycenter corrected pulse phases show smooth evolution
and clear negative phase shifts coincident with the flares seen on the light
curve and the enhancements of fractional pulse amplitude. The non-flare pulse
phases for the first $\sim$60d data are well described as a fourth order
polynomial implying that the neutron star was spun-up during the first
$\sim$60d with a rate $\dot \nu=(1.7\pm0.3) \times 10^{-13}$ Hz/s at the
beginning of the outburst. Significant soft phase lags up to $\sim$500 $\mu s$
($\sim$10% cycle) between 2 to 20 keV were detected for the nonflare pulse
phases. We conclude that the anomalous phase shifts are unlikely due to the
accretion torque but could result from the ``hot spot'' moving on the surface
of neutron star.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 06:43:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chou",
"Y.",
"",
"National Central\n University"
],
[
"Chung",
"Y.",
"",
"National Central\n University"
],
[
"Hu",
"C. P.",
"",
"National Central\n University"
],
[
"Yang",
"T. C.",
"",
"National Central\n University"
]
] | [
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801.091 | Boddapati Anandarao G. | V. Venkata Raman and B.G. Anandarao | Infrared Spectroscopic Study of a Selection of AGB and Post-AGB Stars | 14 pages; accepted in MNRAS, 2008 | null | 10.1111/j.1365-2966.2008.12915.x | null | astro-ph | null | We present here near-infrared spectroscopy in the H and K bands of a
selection of nearly 80 stars that belong to various AGB types, namely S type, M
type and SR type. This sample also includes 16 Post-AGB (PAGB) stars. From
these spectra, we seek correlations between the equivalent widths of some
important spectral signatures and the infrared colors that are indicative of
mass loss. Repeated spectroscopic observations were made on some PAGB stars to
look for spectral variations. We also analyse archival SPITZER mid-infrared
spectra on a few PAGB stars to identify spectral features due to PAH molecules
providing confirmation of the advanced stage of their evolution. Further, we
model the SEDs of the stars (compiled from archival data) and compare
circumstellar dust parameters and mass loss rates in different types.
Our near-infrared spectra show that in the case of M and S type stars, the
equivalent widths of the CO(3-0) band are moderately correlated with infrared
colors, suggesting a possible relationship with mass loss processes. A few PAGB
stars revealed short term variability in their spectra, indicating episodic
mass loss: the cooler stars showed in CO first overtone bands and the hotter
ones showed in HI Brackett lines. Our spectra on IRAS 19399+2312 suggest that
it is a transition object. From the SPITZER spectra, there seems to be a
dependence between the spectral type of the PAGB stars and the strength of the
PAH features. Modelling of SEDs showed among the M and PAGB stars that the
higher the mass loss rates, the higher the [K-12] colour in our sample.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:19:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Raman",
"V. Venkata",
""
],
[
"Anandarao",
"B. G.",
""
]
] | [
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] |
801.0911 | Nikolay Prokof'ev | Nikolay Prokof'ev and Boris Svistunov | Bold diagrammatic Monte Carlo: A generic technique for polaron (and
many-body?) problems | 15 pages, 15 figures, revtex4 | null | null | null | cond-mat.str-el | null | We develop a Monte Carlo scheme for sampling series of Feynman diagrams for
the proper self-energy which are self-consistently expressed in terms of
renormalized particle propagators. This approach is used to solve the problem
of a single spin-down fermion resonantly interacting with the Fermi gas of
spin-up particles. Though the original series based on bare propagators are
sign-alternating and divergent one can still determine the answer behind them
by using two strategies (separately or together): (i) using proper series
re-summation techniques, and (ii) introducing renormalized propagators which
are defined in terms of the simulated proper self-energy, i.e. making the
entire scheme self-consistent. Our solution is important for understanding the
phase diagram and properties of the BCS-BEC crossover in the strongly
imbalanced regime. On the technical side, we develop a generic sign-problem
tolerant method for exact numerical solution of polaron-type models, and,
possibly, of the interacting many-body Hamiltonians.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:25:39 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Prokof'ev",
"Nikolay",
""
],
[
"Svistunov",
"Boris",
""
]
] | [
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] |
801.0912 | Shuzo Izumi | Hirotada Ito, Shuzo Izumi | Diophantine inequality for equicharacteristic excellent Henselian local
domains | A correction in the final part of the proof. Accepted to Comptes
rendus mathematiques (Mathematical Reports) | C. R. Rep. Acad. Sci. Canada vol. 30 (2) 2008, pp. 48-55 | null | null | math.AC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | G. Rond has proved a Diophantine type inequality for the field of quotients
of the convergent or formal power series ring in multivariables. We generalize
his theorem to the field of the quotients of an excellent Henselian local
domain in equicharacteristic case.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:35:36 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 10:25:24 GMT"
},
{
"version": "v3",
"created": "Sun, 24 Feb 2008 07:22:57 GMT"
},
{
"version": "v4",
"created": "Sun, 20 Apr 2008 15:45:03 GMT"
},
{
"version": "v5",
"created": "Mon, 27 Oct 2008 13:07:48 GMT"
}
] | 2011-02-15T00:00:00 | [
[
"Ito",
"Hirotada",
""
],
[
"Izumi",
"Shuzo",
""
]
] | [
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] |
801.0913 | Sandra Ninet | Sandra Ninet (IMPMC), Fr\'ed\'eric Datchi (IMPMC) | High pressure-high temperature phase diagram of ammonia | null | null | 10.1063/1.2903491 | null | cond-mat.mtrl-sci | null | The high pressure(P)-high temperature(T) phase diagram of solid ammonia has
been investigated using diamond anvil cell and resistive heating techniques.
The III-IV transition line has been determined up to 20 GPa and 500 K both on
compression and decompression paths. No discontinuity is observed at the
expected location for the III-IV-V triple point. The melting line has been
determined by visual observations of the fluid-solid equilibrium up to 9 GPa
and 900 K. The experimental data is well fitted by a Simon-Glatzel equation in
the covered P-T range. These transition lines and their extrapolations are
compared with reported calculations.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:47:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ninet",
"Sandra",
"",
"IMPMC"
],
[
"Datchi",
"Frédéric",
"",
"IMPMC"
]
] | [
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] |
801.0914 | Ngau Lam | Shun-Jen Cheng, Jae-Hoon Kwon, Ngau Lam | A BGG-type resolution for tensor modules over general linear
superalgebra | 11pages, LaTeX format | null | 10.1007/s11005-008-0231-1 | null | math.RT | null | We construct a Bernstein-Gelfand-Gelfand type resolution in terms of direct
sums of Kac modules for the finite-dimensional irreducible tensor
representations of the general linear superalgebra. As a consequence it follows
that the unique maximal submodule of a corresponding reducible Kac module is
generated by its proper singular vector.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:47:38 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Mar 2008 05:21:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cheng",
"Shun-Jen",
""
],
[
"Kwon",
"Jae-Hoon",
""
],
[
"Lam",
"Ngau",
""
]
] | [
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] |
801.0915 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB), Sebastian Pauli (DMS), Michael Pohst,
Florence Soriano-Gafiuk (LMAM) | Computation of 2-groups of narrow logarithmic divisor classes of number
fields | null | null | null | null | math.NT | null | We present an algorithm for computing the 2-group of narrow logarithmic
divisor classes of degree 0 for number fields F. As an application, we compute
in some cases the 2-rank of the wild kernel WK2(F).
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:48:44 GMT"
}
] | 2009-03-06T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
],
[
"Pauli",
"Sebastian",
"",
"DMS"
],
[
"Pohst",
"Michael",
"",
"LMAM"
],
[
"Soriano-Gafiuk",
"Florence",
"",
"LMAM"
]
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] |
801.0916 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB), Florence Soriano-Gafiuk (LMAM) | Sur le sous-groupe des \'el\'ements de hauteur infinie du K2 d'un corps
de nombres | null | Acta Arithmetica 122 (2006) 235-244 | null | null | math.NT | null | By using the logarithmic approach of the classical kernels for the K2 of
number fields, we compute the 2-rank of the wild kernel WK2(F) and the 2-rank
of the subgroup of infinite heigh elements in K2(F) in terms of positive class
groups for any number field F.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 07:50:34 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
],
[
"Soriano-Gafiuk",
"Florence",
"",
"LMAM"
]
] | [
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] |
801.0917 | Syedafsar Abbas | Syed Afsar Abbas | Whither Nuclear Physics ? | Invited Talk at "International Conference on Recent Trends in
Theoretical Physics, ISI, Kolkata, India, Dec 4-7 2007; 16 pages, 3 figures | "Recent Developments in Theoretical Ohysics", Ed S Ghosh and G
Kar, World Scientific, Singapore, 2009 | null | null | nucl-th | null | Nuclear Physics has had its ups and downs. However in recent years, bucked up
by some new and often puzzling data, it has become a potentially very rich
field. We review some of these exciting developments in a few important sectors
of nuclear physics. Emphasis shall be on the study of exotic nuclei and the new
physics that these nuclei are teaching us.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:01:16 GMT"
}
] | 2010-01-27T00:00:00 | [
[
"Abbas",
"Syed Afsar",
""
]
] | [
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] |
801.0918 | FengLan Shao | Jun Song, Feng-lan Shao, Qu-bing Xie, Yun-fei Wang, De-ming Wei | The influence of net-quarks on the yields and rapidity spectra of
identified hadrons | 8 pages, 7 figures | Int.J.Mod.Phys.A24:1161-1174,2009 | 10.1142/S0217751X0904302X | null | hep-ph | null | Within a quark combination model, we study systematically the yields and
rapidity spectra of various hadrons in central Au+Au collisions at
$\sqrt{s_{NN}}= 200$ GeV. We find that considering the difference in rapidity
between net-quarks and newborn quarks, the data of multiplicities, rapidity
distributions for $\pi^{\pm}$, $K^{\pm}$, $p(\bar{p})$ and, in particular the
ratios of charged antihadron to hadron as a function of rapidity, can be well
described. The effect of net-quarks on various hadrons is analysed, and the
rapidity distributions for $K^{0}_{s}$, $\Lambda(\bar{\Lambda})$,
$\Sigma^{+}(\bar{\Sigma}^{_-})$, $\mathrm{\Xi^{-}}$ ($\mathrm{\bar{\Xi}^{_+}}$)
and $\mathrm{\Omega^{-}}(\mathrm{\bar{\Omega}}^{_+})$ are predicted. We discuss
the rapidity distribution of net-baryon, and find that it reflects exactly the
energy loss of colliding nuclei.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:08:51 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 05:08:16 GMT"
}
] | 2009-04-30T00:00:00 | [
[
"Song",
"Jun",
""
],
[
"Shao",
"Feng-lan",
""
],
[
"Xie",
"Qu-bing",
""
],
[
"Wang",
"Yun-fei",
""
],
[
"Wei",
"De-ming",
""
]
] | [
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] |
801.0919 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB), Alexis Michel (IMB) | Approche logarithmique des noyaux \'etales sauvages des corps de nombres | null | Journal of Number Theory 120 (2006) 72--91 | null | null | math.NT | null | We study the l-part of the the wild \'etale kernels WK2i(F) of an arbitary
number field F for a given prime l in connection with the logarithmic l-class
groups. From the logarithmic arithmetic we deduce rank formulas, periodicity
and reflection theorems, triviality characterizations and various consequences.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:11:43 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
],
[
"Michel",
"Alexis",
"",
"IMB"
]
] | [
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] |
801.092 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB) | G\'en\'eralisation d'un Th\'eor\`eme d'Iwasawa | null | Journal de Th\'eorie des Nombres de Bordeaux 17 (2005) 527--553 | null | null | math.NT | null | We extend to convenient finite quotients of a noetherian Lambda-module the
classical result of K. Iwasawa giving the asymptotic expression of the l-part
of the number of ideal class groups in Zl-extensions of number fields. Then, in
the arithmetic context, we compute the three characters associated by this way
to the l-groups of T-infinitesimal S-classes in the cyclotomic tower and relate
them to the classical invariants and the decomposition characters associated to
the finite sets of places S and T. A main tool in this study is the so-called
Spiegelungssatz of Georges Gras, which exchanges (wild or tame) ramification
and decomposition. The main results of this arithmetical part extend those we
obtained with Christian Maire in a previous article. The most intricate study
of the wild contribution of the sets S and T involves a generalization of a
classical result of R. Greenberg on the genus theory of cyclotomic towers.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:17:29 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Mar 2008 08:29:40 GMT"
}
] | 2008-03-10T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
]
] | [
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] |
801.0921 | Jean-Francois Jaulent | Francisco Diaz Y Diaz (IMB), Jean-Fran\c{c}ois Jaulent (IMB),
Sebastian Pauli (DMS), Michael Pohst, Florence Soriano-Gafiuk (LMAM) | A new Algorithm for the Computation of logarithmic l-Class Groups of
Number Fields | null | Experimental Mathematics (Project Euclid) 14 (2005) 67--76 | null | null | math.NT | null | We present an algorithm for the computation of logarithmic l-class groups of
number fields. Our principal motivation is the effective determination of the
l-rank of the wild kernel in the K-theory of number fields.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:25:12 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Diaz",
"Francisco Diaz Y",
"",
"IMB"
],
[
"Jaulent",
"Jean-François",
"",
"IMB"
],
[
"Pauli",
"Sebastian",
"",
"DMS"
],
[
"Pohst",
"Michael",
"",
"LMAM"
],
[
"Soriano-Gafiuk",
"Florence",
"",
"LMAM"
]
] | [
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] |
801.0922 | A. M. Abd Elfattah | A. M. Abd Elfattah, O. Mohamed Marwa | Estimating of $P(Y<X)$ in the Exponential case Based on Censored Samples | Submitted to the Electronic Journal of Statistics
(http://www.i-journals.org/ejs/) by the Institute of Mathematical Statistics
(http://www.imstat.org) | null | null | IMS-EJS-EJS_2008_166 | stat.ME | null | In this article, the estimation of reliability of a system is discussed
$p(y<x)$ when strength, $X$, and stress, $Y$, are two independent exponential
distribution with different scale parameters when the available data are type
II Censored sample. Different methods for estimating the reliability are
applied. The point estimators obtained are maximum likelihood estimator,
uniformly minimum variance unbiased estimator, and Bayesian estimators based on
conjugate and non informative prior distributions. A comparison of the
estimates obtained is performed. Interval estimators of the reliability are
also discussed.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:30:01 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Elfattah",
"A. M. Abd",
""
],
[
"Marwa",
"O. Mohamed",
""
]
] | [
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] |
801.0923 | J. S. Kaastra | V. Petrosian, A. Bykov | Particle acceleration mechanisms | 22 pages, 5 figures, accepted for publication in Space Science
Reviews, special issue "Clusters of galaxies: beyond the thermal view",
Editor J.S. Kaastra, Chapter 11; work done by an international team at the
International Space Science Institute (ISSI), Bern, organised by J.S.
Kaastra, A.M. Bykov, S. Schindler & J.A.M. Bleeker | null | 10.1007/s11214-008-9315-6 | null | astro-ph | null | We review the possible mechanisms for production of non-thermal electrons
which are responsible for non-thermal radiation in clusters of galaxies. Our
primary focus is on non-thermal Bremsstrahlung and inverse Compton scattering,
that produce hard X-ray emission. We briefly review acceleration mechanisms and
point out that in most astrophysical situations, and in particular for the
intracluster medium, shocks, turbulence and plasma waves play a crucial role.
We consider two scenarios for production of non-thermal radiation. The first is
hard X-ray emission due to non-thermal Bremsstrahlung by nonrelativistic
particles. Non-thermal tails are produced by accelerating electrons from the
background plasma with an initial Maxwellian distribution. However, these tails
are accompanied by significant heating and they are present for a short time of
<10^6 yr, which is also the time that the tail will be thermalised. Such
non-thermal tails, even if possible, can only explain the hard X-ray but not
the radio emission which needs GeV or higher energy electrons. For these and
for production of hard X-rays by the inverse Compton model, we need the second
scenario where there is injection and subsequent acceleration of relativistic
electrons. It is shown that a steady state situation, for example arising from
secondary electrons produced from cosmic ray proton scattering by background
protons, will most likely lead to flatter than required electron spectra or it
requires a short escape time of the electrons from the cluster. An episodic
injection of relativistic electrons, presumably from galaxies or AGN, and/or
episodic generation of turbulence and shocks by mergers can result in an
electron spectrum consistent with observations but for only a short period of
less than one billion years.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 15:25:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Petrosian",
"V.",
""
],
[
"Bykov",
"A.",
""
]
] | [
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] |
801.0924 | Wojciech Satula | M. Zalewski (Univ. of Warsaw), J. Dobaczewski (Univ. of Warsaw and
Univ. of Jyvaskyla), W. Satula (Univ. of Warsaw), and T.R. Werner (Univ. of
Warsaw) | Spin-orbit and tensor mean-field effects on spin-orbit splitting
including self-consistent core polarizations | 15 pages, 7 figures, submitted to Physical Review C | Phys.Rev.C77:024316,2008 | 10.1103/PhysRevC.77.024316 | null | nucl-th | null | A new strategy of fitting the coupling constants of the nuclear energy
density functional is proposed, which shifts attention from ground-state bulk
to single-particle properties. The latter are analyzed in terms of the bare
single-particle energies and mass, shape, and spin core-polarization effects.
Fit of the isoscalar spin-orbit and both isoscalar and isovector tensor
coupling constants directly to the f5/2-f7/2 spin-orbit splittings in 40Ca,
56Ni, and 48Ca is proposed as a practical realization of this new programme. It
is shown that this fit requires drastic changes in the isoscalar spin-orbit
strength and the tensor coupling constants as compared to the commonly accepted
values but it considerably and systematically improves basic single-particle
properties including spin-orbit splittings and magic-gap energies. Impact of
these changes on nuclear binding energies is also discussed.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:32:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Zalewski",
"M.",
"",
"Univ. of Warsaw"
],
[
"Dobaczewski",
"J.",
"",
"Univ. of Warsaw and\n Univ. of Jyvaskyla"
],
[
"Satula",
"W.",
"",
"Univ. of Warsaw"
],
[
"Werner",
"T. R.",
"",
"Univ. of\n Warsaw"
]
] | [
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] |
801.0925 | Jacques Moret-Bailly | Jacques Moret-Bailly | Light emission of very low density hydrogen excited by an extremely hot
light source; applications in astrophysics | 16 pages,3 figures | null | null | null | physics.gen-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Stromgren studied the action of an extremely hot source on a diluted pure
hydrogen cloud; a very ionized, spherical hydrogen plasma surrounded by neutral
atomic hydrogen is formed. A relatively thin intermediate, partially ionized,
hydrogen shell, is cooled by the radiation of the atoms.
Stromgren was unaware of that this plasma, similar to the plasma of a gas
laser, can be superradiant at several eigen frequencies of atomic hydrogen; the
superradiant rays emitted tangentially with the sphere appear resulting from a
discontinuous ring because of the competition of optical modes. The
superradiance intensely depopulates the excited levels, including the continuum
of proton-electron collisions, by cascades of transitions combined into
resonant multiphotonic transitions so that the gas is cooled brutally beyond
the radius of the Stromgren sphere.
The extreme brightness of the rays emitted by the source allows a
multiphotonic non-resonant absorption leading in stationary states or the
ionization continuum. This absorption combines with the superradiant emissions
in a multiphotonic diffusion induced by the superradiant rays. Although its
brightness remains higher than that of the superradiant rays, the source
becomes invisible if it is observed through a small solid angle.
The lines emitted inside the sphere are all the more weak as they arrive of
an internal area, lower in atoms, and more reddened also by a parametric
transfer of energy towards the thermal radiation catalyzed by excited atomic
hydrogen present in the sphere only.
The Stromgren sphere appears to help to simply explain the appearance and the
spectrum of supernova 1987A.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:32:36 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jul 2008 07:44:07 GMT"
}
] | 2008-07-19T00:00:00 | [
[
"Moret-Bailly",
"Jacques",
""
]
] | [
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] |
801.0926 | Oren Raz | E. Putterman, O. Raz | The Square Cat | 13 pages, 5 figures | Am. J. Phys. 76 1040 (2008) | 10.1119/1.2952448 | null | physics.class-ph | null | We present a simple, two dimensional example of a "cat" -- a body with zero
angular momentum that can rotate itself with no external forces. This model is
used to explain why this problem is known to be a gauge theory and to
illustrate the importance of non-commutative operators. We will also show a
comparison between the free-space "cat" in Newtonian mechanics and the same
problem in Aristotelian mechanics at low Reynolds number; this simple example
shows the analogy between (angular) momentum in Newtonian mechanics and
(torque) force in Aristotelian mechanics. We will end by pointing out a
topological invariant common to our model in free space and at low Reynolds
number.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 08:53:43 GMT"
}
] | 2010-07-28T00:00:00 | [
[
"Putterman",
"E.",
""
],
[
"Raz",
"O.",
""
]
] | [
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] |
801.0927 | Stefano Andreon | S. Andreon, E. Puddu, R. De Propris, J.-C. Cuillandre | Galaxy evolution in the high redshift, colour-selected cluster RzCS 052
at z=1.02 | MNRAS, in press | null | 10.1111/j.1365-2966.2008.12890.x | null | astro-ph | null | We present deep I and z' imaging of the colour-selected cluster RzCS 052 and
study the color-magnitude relation of this cluster, its scatter, the
morphological distribution on the red sequence, the luminosity and stellar mass
functions of red galaxies and the cluster blue fraction. We find that the
stellar populations of early type galaxies in this cluster are uniformly old
and that their luminosity function does not show any sign of evolution other
than the passive evolution of their stellar populations. We rule out a
significant contribution from mergers in the buildup of the red sequence of
RzCS 052. The cluster has a large (~30%) blue fraction and and we infer that
the evolution of the blue galaxies is faster than an exponentially declining
star formation model and that these objects have probably experienced starburst
episodes. Mergers are unlikely to be the driver of the observed colour
evolution, because of the measured constancy of the mass function, as derived
from near-infrared photometry of 32 clusters, including RzCS 052, presented in
a related paper. Mechanisms with clustercentric radial dependent efficiencies
are disfavored as well, because of the observed constant blue fraction with
clustercentric distance.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:03:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Andreon",
"S.",
""
],
[
"Puddu",
"E.",
""
],
[
"De Propris",
"R.",
""
],
[
"Cuillandre",
"J. -C.",
""
]
] | [
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] |
801.0928 | Yveline Lebreton | Yveline Lebreton, Josefina Montalban, Joergen Christensen-Dalsgaard,
Ian W. Roxburgh, Achim Weiss | CoRoT/ESTA-TASK 1 and TASK 3 comparison of the internal structure and
seismic properties of representative stellar models: Comparisons between the
ASTEC, CESAM, CLES, GARSTEC and STAROX codes | 26 pages, 21 figures, accepted for publication in Astrophysics and
Space Science, CoRoT/ESTA Volume | Astrophys.Space Sci.316:187-213,2008 | 10.1007/s10509-008-9740-8 | null | astro-ph | null | We compare stellar models produced by different stellar evolution codes for
the CoRoT/ESTA project, comparing their global quantities, their physical
structure, and their oscillation properties. We discuss the differences between
models and identify the underlying reasons for these differences. The stellar
models are representative of potential CoRoT targets. Overall we find very good
agreement between the five different codes, but with some significant
deviations. We find noticeable discrepancies (though still at the per cent
level) that result from the handling of the equation of state, of the opacities
and of the convective boundaries. The results of our work will be helpful in
interpreting future asteroseismology results from CoRoT.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:05:01 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Lebreton",
"Yveline",
""
],
[
"Montalban",
"Josefina",
""
],
[
"Christensen-Dalsgaard",
"Joergen",
""
],
[
"Roxburgh",
"Ian W.",
""
],
[
"Weiss",
"Achim",
""
]
] | [
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0.0285275877,
0.078822799
] |
801.0929 | Hidefumi Ohsugi | Satoshi Aoki, Takayuki Hibi, Hidefumi Ohsugi, Akimichi Takemura | Groebner bases of nested configurations | 11 pages | Journal of Algebra 320 (2008), pp. 2583-2593 | 10.1016/j.jalgebra.2008.05.023 | null | math.AC | null | In this paper we introduce a new and large family of configurations whose
toric ideals possess quadratic Groebner bases. As an application, a
generalization of algebras of Segre-Veronese type will be studied.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:14:56 GMT"
}
] | 2008-09-23T00:00:00 | [
[
"Aoki",
"Satoshi",
""
],
[
"Hibi",
"Takayuki",
""
],
[
"Ohsugi",
"Hidefumi",
""
],
[
"Takemura",
"Akimichi",
""
]
] | [
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] |
801.093 | Sylvain Schwartz | Sylvain Schwartz (TRT), Fran\c{c}ois Gutty, Gilles Feugnet (TRT),
Philippe Bouyer (LCFIO), Jean-Paul Pocholle (TRT) | Suppression of Nonlinear Interactions in Resonant Macroscopic Quantum
Devices : the Example of the Solid-State Ring Laser Gyroscope | null | Physical Review Letters 100, 18 (2008) 183901 | 10.1103/PhysRevLett.100.183901 | null | physics.optics | null | We study the suppression of nonlinear interactions in resonant macroscopic
quantum devices in the case of the solid-state ring laser gyroscope. These
nonlinear interactions are tuned by vibrating the gain medium along the cavity
axis. Beat note occurrence under rotation provides a precise measurement of the
strength of nonlinear interactions, which turn out to vanish for some discrete
values of the amplitude of vibration. Our theoretical description, in very good
agreement with the measured data, suggests the use of a higher vibration
frequency to achieve quasi-ideal rotation sensing over a broad range of
rotation speeds. We finally underline the analogy between this device and some
other macroscopic quantum rotation sensors, such as ring-shaped superfluid
configurations, where nonlinear interactions could be tuned for example by the
use of magnetically-induced Feschbach resonance.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:16:44 GMT"
}
] | 2011-09-26T00:00:00 | [
[
"Schwartz",
"Sylvain",
"",
"TRT"
],
[
"Gutty",
"François",
"",
"TRT"
],
[
"Feugnet",
"Gilles",
"",
"TRT"
],
[
"Bouyer",
"Philippe",
"",
"LCFIO"
],
[
"Pocholle",
"Jean-Paul",
"",
"TRT"
]
] | [
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] |
801.0931 | Ryuhei Mori | Ryuhei Mori, Kenta Kasai, Tomoharu Shibuya, and Kohichi Sakaniwa | The Asymptotic Bit Error Probability of LDPC Codes for the Binary
Erasure Channel with Finite Iteration Number | 5 pages, 6 figures, correcting errors in Theorem 1 and poor English | null | null | null | cs.IT math.IT | null | We consider communication over the binary erasure channel (BEC) using
low-density parity-check (LDPC) code and belief propagation (BP) decoding. The
bit error probability for infinite block length is known by density evolution
and it is well known that a difference between the bit error probability at
finite iteration number for finite block length $n$ and for infinite block
length is asymptotically $\alpha/n$, where $\alpha$ is a specific constant
depending on the degree distribution, the iteration number and the erasure
probability. Our main result is to derive an efficient algorithm for
calculating $\alpha$ for regular ensembles. The approximation using $\alpha$ is
accurate for $(2,r)$-regular ensembles even in small block length.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:40:41 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 12:37:13 GMT"
}
] | 2008-01-23T00:00:00 | [
[
"Mori",
"Ryuhei",
""
],
[
"Kasai",
"Kenta",
""
],
[
"Shibuya",
"Tomoharu",
""
],
[
"Sakaniwa",
"Kohichi",
""
]
] | [
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] |
801.0932 | Alice Sinatra | Yun Li (LKB - Lhomond, ECNU), Yvan Castin (LKB - Lhomond), Alice
Sinatra (LKB - Lhomond) | Optimum spin-squeezing in Bose-Einstein condensates with particle losses | 4 pages | Physical Review Letters 100, 21 (2008) 210401 | 10.1103/PhysRevLett.100.210401 | null | quant-ph | null | The problem of spin squeezing with a bimodal condensate in presence of
particle losses is solved analytically by the Monte Carlo wavefunction method.
We find the largest obtainable spin squeezing as a function of the one-body
loss rate, the two-body and three-body rate constants, and the s-wave
scattering length.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:22:52 GMT"
},
{
"version": "v2",
"created": "Tue, 6 May 2008 07:29:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Li",
"Yun",
"",
"LKB - Lhomond, ECNU"
],
[
"Castin",
"Yvan",
"",
"LKB - Lhomond"
],
[
"Sinatra",
"Alice",
"",
"LKB - Lhomond"
]
] | [
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] |
801.0933 | Abhijit Pal | Abhijit Pal | Relative Hyperbolic Extensions of Groups and Cannon-Thurston Maps | 16 pages, No figures | null | null | null | math.GR math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $1\to (K,K_1)\to (G,N_G(K_1))\to(Q,Q_1)\to 1$ be a short exact sequence
of pairs of finitely generated groups with $K$ strongly hyperbolic relative to
proper subgroup $K_1$. Assuming that for all $g\in G$ there exists $k\in K$
such that $gK_1g^{-1}=kK_1k^{-1}$, we prove that there exists a quasi-isometric
section $s\colon Q \to G$. Further we prove that if $G$ is strongly hyperbolic
relative to the normalizer subgroup $N_G(K_1)$ and weakly hyperbolic relative
to $K_1$, then there exists a Cannon-Thurston map for the inclusion
$i\colon\Gamma_K\to \Gamma_G$.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:19:20 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jul 2008 13:08:56 GMT"
}
] | 2008-07-22T00:00:00 | [
[
"Pal",
"Abhijit",
""
]
] | [
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] |
801.0934 | Haijun Zhou | Jie Zhou, Zhong-Can Ou-Yang, and Haijun Zhou | Simulating the collapse transition of a two-dimensional semiflexible
lattice polymer | 16 pages | null | 10.1063/1.2842064 | null | cond-mat.soft | null | It has been revealed by mean-field theories and computer simulations that the
nature of the collapse transition of a polymer is influenced by its bending
stiffness $\epsilon_{\rm b}$. In two dimensions, a recent analytical work
demonstrated that the collapse transition of a partially directed lattice
polymer is always first-order as long as $\epsilon_{\rm b}$ is positive
[H. Zhou {\em et al.}, Phys. Rev. Lett. {\bf 97}, 158302 (2006)]. Here we
employ Monte Carlo simulation to investigate systematically the effect of
bending stiffness on the static properties of a 2D lattice polymer. The
system's phase-diagram at zero force is obtained. Depending on $\epsilon_{\rm
b}$ and the temperature $T$, the polymer can be in one of three phases:
crystal, disordered globule, or swollen coil. The crystal-globule transition is
discontinuous, the globule-coil transition is continuous. At moderate or high
values of $\epsilon_{\rm b}$ the intermediate globular phase disappears and the
polymer has only a discontinuous crystal-coil transition. When an external
force is applied, the force-induced collapse transition will either be
continuous or discontinuous, depending on whether the polymer is originally in
the globular or the crystal phase at zero force. The simulation results also
demonstrate an interesting scaling behavior of the polymer at the force-induced
globule-coil transition.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 09:36:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zhou",
"Jie",
""
],
[
"Ou-Yang",
"Zhong-Can",
""
],
[
"Zhou",
"Haijun",
""
]
] | [
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] |
801.0935 | Michael Lashkevich | Michael Lashkevich (Landau Institute) | Boundary form factors in the Smirnov--Fateev model with a diagonal
boundary $S$ matrix | 15 pages, 2 figures included in the LaTeX file | null | null | null | hep-th | null | The boundary conditions with diagonal boundary $S$ matrix and the boundary
form factors for the Smirnov--Fateev model on a half line has been considered
in the framework of the free field representation. In contrast to the case of
the sine-Gordon model, in this case the free field representation is shown to
impose severe restrictions on the boundary $S$ matrix, so that a finite number
of solutions is only consistent with the free field realization.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:25:21 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Lashkevich",
"Michael",
"",
"Landau Institute"
]
] | [
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] |
801.0936 | Robert Alicki | Robert Alicki | Pure decoherence in quantum systems | 11 pages | Open Sys.& Information Dyn. 11: 53-61 (2004) | null | null | quant-ph | null | A popular model of decoherence based on the linear coupling to harmonic
oscillator heat baths is analized and shown to be inappropriate in the regime
where decoherence dominates over energy dissipation, called pure decoherence
regime. The similar mechanism essentially related to the energy conservation
implies that, on the contrary to the recent conjectures, chaotic environments
can be less efficient decoherers than regular ones. Finally, the elastic
scattering mechanism is advocated as the simplest source of pure decoherence.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:12:31 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Alicki",
"Robert",
""
]
] | [
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] |
801.0937 | Tsuneo Uematsu | Yoshio Kitadono, Ken Sasaki, Takahiro Ueda and Tsuneo Uematsu | Target Mass Corrections for the Virtual Photon Structure Functions to
the Next-to-next-to-leading Order in QCD | 24 pages, LaTeX, 7 eps figures, REVTeX 4 | Phys.Rev.D77:054019,2008 | 10.1103/PhysRevD.77.054019 | YNU-HEPTh-07-102,KUNS-2119 | hep-ph | null | We investigate target mass effects in the unpolarized virtual photon
structure functions $F_2^\gamma(x,Q^2,P^2)$ and $F_L^\gamma(x,Q^2,P^2)$ in
perturbative QCD for the kinematical region $\Lambda^2 \ll P^2 \ll Q^2$, where
$-Q^2(-P^2)$ is the mass squared of the probe (target) photon and $\Lambda$ is
the QCD scale parameter. We obtain the Nachtmann moments for the structure
functions and then, by inverting the moments, we get the expressions in closed
form for $F_2^\gamma(x,Q^2,P^2)$ up to the next-to-next-to-leading order and
for $F_L^\gamma(x,Q^2,P^2)$ up to the next-to-leading order, both of which
include the target mass corrections. Numerical analysis exhibits that target
mass effects appear at large $x$ and become sizable near $x_{\rm
max}(=1/(1+\frac{P^2}{Q^2}))$, the maximal value of $x$, as the ratio $P^2/Q^2$
increases.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:16:10 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kitadono",
"Yoshio",
""
],
[
"Sasaki",
"Ken",
""
],
[
"Ueda",
"Takahiro",
""
],
[
"Uematsu",
"Tsuneo",
""
]
] | [
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] |
801.0938 | Sang-Woon Jeon | Sang-Woon Jeon, Natasha Devroye, Mai Vu, Sae-Young Chung, Vahid Tarokh | Cognitive Networks Achieve Throughput Scaling of a Homogeneous Network | 28 pages, 12 figures, submitted to IEEE Trans. on Information Theory | IEEE Transactions on Information Theory, vol. 57, no. 8, pp.
5103-5115, Aug. 2011 | 10.1109/TIT.2011.2158874 | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study two distinct, but overlapping, networks that operate at the same
time, space, and frequency. The first network consists of $n$ randomly
distributed \emph{primary users}, which form either an ad hoc network, or an
infrastructure-supported ad hoc network with $l$ additional base stations. The
second network consists of $m$ randomly distributed, ad hoc secondary users or
cognitive users. The primary users have priority access to the spectrum and do
not need to change their communication protocol in the presence of secondary
users. The secondary users, however, need to adjust their protocol based on
knowledge about the locations of the primary nodes to bring little loss to the
primary network's throughput. By introducing preservation regions around
primary receivers and avoidance regions around primary base stations, we
propose two modified multihop routing protocols for the cognitive users. Base
on percolation theory, we show that when the secondary network is denser than
the primary network, both networks can simultaneously achieve the same
throughput scaling law as a stand-alone network. Furthermore, the primary
network throughput is subject to only a vanishingly fractional loss.
Specifically, for the ad hoc and the infrastructure-supported primary models,
the primary network achieves sum throughputs of order $n^{1/2}$ and
$\max\{n^{1/2},l\}$, respectively. For both primary network models, for any
$\delta>0$, the secondary network can achieve sum throughput of order
$m^{1/2-\delta}$ with an arbitrarily small fraction of outage. Thus, almost all
secondary source-destination pairs can communicate at a rate of order
$m^{-1/2-\delta}$.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:52:39 GMT"
},
{
"version": "v2",
"created": "Thu, 16 Jul 2009 05:24:13 GMT"
}
] | 2016-11-17T00:00:00 | [
[
"Jeon",
"Sang-Woon",
""
],
[
"Devroye",
"Natasha",
""
],
[
"Vu",
"Mai",
""
],
[
"Chung",
"Sae-Young",
""
],
[
"Tarokh",
"Vahid",
""
]
] | [
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801.0939 | Christos Athanasiadis | Christos A. Athanasiadis | On the graph-connectivity of skeleta of convex polytopes | Added Remark 1.2 and reference to the article [Incidence graphs of
convex polytopes, J. Combin. Theory 2 (1967), 466-506] by G.T. Sallee | null | null | null | math.CO | null | Given a $d$-dimensional convex polytope $P$ and nonnegative integer $k$ not
exceeding $d-1$, let $G_k (P)$ denote the simple graph on the node set of
$k$-dimensional faces of $P$ in which two such faces are adjacent if there
exists a $(k+1)$-dimensional face of $P$ which contains them both. The graph
$G_k (P)$ is isomorphic to the dual graph of the $(d-k)$-dimensional skeleton
of the normal fan of $P$. For fixed values of $k$ and $d$, the largest integer
$m$ such that $G_k (P)$ is $m$-vertex-connected for all $d$-dimensional
polytopes $P$ is determined. This result generalizes Balinski's theorem on the
one-dimensional skeleton of a $d$-dimensional convex polytope.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:24:43 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 07:50:04 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Athanasiadis",
"Christos A.",
""
]
] | [
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801.094 | Herve Mohrbach | Pierre Gosselin (IF), Herve Mohrbach (FCN, LPMC - EA 3468) | Diagonal Representation for a Generic Matrix Valued Quantum Hamiltonian | Significant revision, typos corrected and references added | Eur.Phys.J.C64:495-527,2009 | 10.1140/epjc/s10052-009-1155-3 | null | math-ph cond-mat.other hep-th math.MP quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A general method to derive the diagonal representation for a generic matrix
valued quantum Hamiltonian is proposed. In this approach new mathematical
objects like non-commuting operators evolving with the Planck constant promoted
as a running variable are introduced. This method leads to a formal compact
expression for the diagonal Hamiltonian which can be expanded in a power series
of the Planck constant. In particular, we provide an explicit expression for
the diagonal representation of a generic Hamiltonian to the second order in the
Planck constant. This last result is applied, as a physical illustration, to
Dirac electrons and neutrinos in external fields.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:32:54 GMT"
},
{
"version": "v2",
"created": "Fri, 6 Jun 2008 08:24:54 GMT"
},
{
"version": "v3",
"created": "Fri, 18 Jul 2008 12:24:28 GMT"
},
{
"version": "v4",
"created": "Tue, 3 Feb 2009 14:50:33 GMT"
},
{
"version": "v5",
"created": "Mon, 25 May 2009 04:47:27 GMT"
}
] | 2009-11-10T00:00:00 | [
[
"Gosselin",
"Pierre",
"",
"IF"
],
[
"Mohrbach",
"Herve",
"",
"FCN, LPMC - EA 3468"
]
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] |
801.0941 | Philippe Jaming | Philippe Jaming (MAPMO), Mat\'e Matolcsi, Szilard Gy. R\'evesz | On the extremal rays of the cone of positive, positive definite
functions | null | Journal of fourier analysis and applications 15 (2009) 561-582 | 10.1007/s00041-008-9057-6 | null | math.CA math.FA math.PR | null | The aim of this paper is to investigate the cone of non-negative, radial,
positive-definite functions in the set of continuous functions on $\R^d$.
Elements of this cone admit a Choquet integral representation in terms of the
extremals. The main feature of this article is to characterize some large
classes of such extremals. In particular, we show that there many other
extremals than the gaussians, thus disproving a conjecture of G. Choquet and
that no reasonable conjecture can be made on the full set of extremals. The
last feature of this article is to show that many characterizations of positive
definite functions available in the literature are actually particular cases of
the Choquet integral representations we obtain.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:36:37 GMT"
}
] | 2009-10-08T00:00:00 | [
[
"Jaming",
"Philippe",
"",
"MAPMO"
],
[
"Matolcsi",
"Maté",
""
],
[
"Révesz",
"Szilard Gy.",
""
]
] | [
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] |
801.0942 | Almut Beige | Jonathan Busch, Elica S. Kyoseva, Michael Trupke, and Almut Beige | Entangling distant quantum dots using classical interference | 5 pages, 5 figures, revised version, new title | Phys. Rev. A 78, 040301(R) (2008) | 10.1103/PhysRevA.78.040301 | null | cond-mat.mes-hall quant-ph | null | We show that it is possible to employ reservoir engineering to turn two
distant and relatively bad cavities into one good cavity with a tunable
spontaneous decay rate. As a result, quantum computing schemes, that would
otherwise require the shuttling of atomic qubits in and out of an optical
resonator, can now be applied to distant quantum dots. To illustrate this we
transform a recent proposal to entangle two qubits via the observation of
macroscopic fluorescence signals [Metz et al., Phys. Rev. Lett. 97, 040503
(2006)] to the electron-spin states of two semiconductor quantum dots. Our
scheme requires neither the coherent control of qubit-qubit interactions nor
the detection of single photons. Moreover, the scheme is relatively robust
against spin-bath couplings, parameter fluctuations, and the spontaneous
emission of photons.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 10:48:10 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Apr 2008 18:52:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Busch",
"Jonathan",
""
],
[
"Kyoseva",
"Elica S.",
""
],
[
"Trupke",
"Michael",
""
],
[
"Beige",
"Almut",
""
]
] | [
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] |
801.0943 | Kirtiman Ghosh | Kirtiman Ghosh, Anindya Datta | Phenomenology of spinless adjoints in two Universal Extra Dimensions | 20 pages, 10 figures | Nucl.Phys.B800:109-126,2008 | 10.1016/j.nuclphysb.2008.03.012 | null | hep-ph | null | We discuss the phenomenology of $(1,1)$-mode adjoint scalars in the framework
of two Universal Extra Dimensions. The Kaluza-Klein (KK) towers of these
adjoint scalars arise in the 4-dimensional effective theory from the 6th
component of the gauge fields after compactification. Adjoint scalars can have
KK-number conserving as well as KK-number violating interactions. We calculate
the KK-number violating operators involving these scalars and two Standard
Model fields. Decay widths of these scalars into different channels have been
estimated. We have also briefly discussed pair-production and single production
of such scalars at the Large Hadron Collider.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:04:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Ghosh",
"Kirtiman",
""
],
[
"Datta",
"Anindya",
""
]
] | [
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] |
801.0944 | Choon-Lin Ho | Choon-Lin Ho | Prepotential approach to exact and quasi-exact solvabilities of
Hermitian and non-Hermitian Hamiltonians | 12 pages, no figures. Based on talk presented at "Conference in Honor
of CN Yang's 85th Birthday", 31 oct - 3 Nov 2007, Singapore | null | null | null | hep-th math-ph math.MP math.SP quant-ph | null | In this talk I present a simple and unified approach to both exact and
quasi-exact solvabilities of the one-dimensional Schr\"odinger equation. It is
based on the prepotential together with Bethe ansatz equations. This approach
gives the potential as well as the eigenfunctions and eigenvalues
simultaneously. In this approach the system is completely defined by the choice
of the change of variables, and the so-called zero-th order prepotential. We
illustrate the approach by several examples of Hermitian and non-Hermitian
Hamiltonians with real energies. The method can be easily extended to the
constructions of exactly and quasi-exactly solvable Dirac, Pauli, and
Fokker-Planck equations, and to quasinormal modes.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:14:02 GMT"
}
] | 2019-12-06T00:00:00 | [
[
"Ho",
"Choon-Lin",
""
]
] | [
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] |
801.0945 | Soumen Karmakar | Naveen V. Kulkarni, Soumen Karmakar, Indrani Banerjee, R. Pasricha, S.
N. Sahasrabudhe, A. K. Das and S. V. Bhoraskar | DC transferred arc thermal plasma assisted growth of nanoparticles with
different crystalline phases | 30 pages, 9 figures, 1 table | null | null | null | cond-mat.mtrl-sci | null | The control of the crystalline phases of the nanoparticles grown in a
direct-current transferred-arc plasma-assisted reactor is reported. The
crystalline phases of the as synthesized nanoparticles are shown to critically
depend on the operating gas pressure. The paper reports about the change in the
crystalline phases of three distinct compounds namely aluminium oxide (Al2O3),
aluminium nitride (AlN) and iron oxide (FexOy). The major outcome of the
present work is that the phases having higher defect densities are more
probable to form at the sub-atmospheric operating pressure. The variations in
the crystalline structures are discussed on the basis of the equilibrium defect
density formed during the homogeneous nucleation. The as synthesized
nanoparticles were examined by X-ray diffraction analysis and transmission
electron microscopy. In addition, the confirmatory analysis for the crystalline
phases of the as synthesized iron oxides was carried out with the help of
Mossbauer spectroscopy.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:22:33 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Kulkarni",
"Naveen V.",
""
],
[
"Karmakar",
"Soumen",
""
],
[
"Banerjee",
"Indrani",
""
],
[
"Pasricha",
"R.",
""
],
[
"Sahasrabudhe",
"S. N.",
""
],
[
"Das",
"A. K.",
""
],
[
"Bhoraskar",
"S. V.",
""
]
] | [
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] |
801.0946 | Jean-Christophe Pain | Jean-Christophe Pain | Benford's law and complex atomic spectra | 7 pages, 2 figures. submitted to Physical Review E | null | 10.1103/PhysRevE.77.012102 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We found that in transition arrays of complex atomic spectra, the strengths
of electric-dipolar lines obey Benford's law, which means that their
significant digits follow a logarithmic distribution favoring the smallest
values. This indicates that atomic processes result from the superposition of
uncorrelated probability laws and that the occurrence of digits reflects the
constraints induced by the selection rules. Furthermore, Benford's law can be a
useful test of theoretical spectroscopic models. Its applicability to the
statistics of electric-dipolar lines can be understood in the framework of
random matrix theory and is consistent with the Porter-Thomas law.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:23:30 GMT"
},
{
"version": "v2",
"created": "Sat, 10 Dec 2022 17:06:36 GMT"
}
] | 2022-12-13T00:00:00 | [
[
"Pain",
"Jean-Christophe",
""
]
] | [
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] |
801.0947 | Gongwei Lin | Gong-Wei Lin, Xu-Bo Zou, Ming-Yong Ye, Xiu-Min Lin, and Guang-Can Guo | A scheme for tunable quantum phase gate and effective preparation of
graph-state entanglement | 7 pages, 5 figures | Phys. Rev. A 77, 032308 (2008) | 10.1103/PhysRevA.77.032308 | null | quant-ph | null | A scheme is presented for realizing a quantum phase gate with three-level
atoms, solid-state qubits--often called artificial atoms, or ions that share a
quantum data bus such as a single mode field in cavity QED system or a
collective vibrational state of trapped ions. In this scheme, the conditional
phase shift is tunable and controllable via the total effective interaction
time. Furthermore, we show that the method can be used for effective
preparation of graph-state entanglement, which are important resources for
quantum computation, quantum error correction, studies of multiparticle
entanglement, fundamental tests of non-locality and decoherence.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:39:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lin",
"Gong-Wei",
""
],
[
"Zou",
"Xu-Bo",
""
],
[
"Ye",
"Ming-Yong",
""
],
[
"Lin",
"Xiu-Min",
""
],
[
"Guo",
"Guang-Can",
""
]
] | [
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] |
801.0948 | Bin Xu | Zhi Chen, Yiqian Shi and Bin Xu | The Riemannian manifolds with boundary and large symmetry | The former paper has been replaced by a substantially revised
version. Title also changed | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Sixty years ago, S. B. Myers and N. E. Steenrod ({\it Ann. of Math.} {\bf 40}
(1939), 400-416) showed that the isometry group of a Riemannian manifold
without boundary has a structure of Lie group. Recently A. V. Bagaev and N. I.
Zhukova ({\it Siberian Math. J.} {\bf 48} (2007), 579-592) proved the same
result for a Riemannian orbifold. In this paper, we firstly show that the
isometry group of a Riemannian manifold $M$ with boundary has dimension at most
${1/2} \dim M (\dim M-1)$. Then we completely classify such Riemannian
manifolds with boundary that their isometry groups attain the preceding maximal
dimension.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:45:06 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 08:14:45 GMT"
},
{
"version": "v3",
"created": "Sat, 9 May 2009 02:43:33 GMT"
}
] | 2009-05-11T00:00:00 | [
[
"Chen",
"Zhi",
""
],
[
"Shi",
"Yiqian",
""
],
[
"Xu",
"Bin",
""
]
] | [
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] |
801.0949 | Jad Saklawi | Paul C. Attie | On the Refinement of Liveness Properties of Distributed Systems | 54 pages, 12 figures | null | null | null | cs.LO | null | We present a new approach for reasoning about liveness properties of
distributed systems, represented as automata. Our approach is based on
simulation relations, and requires reasoning only over finite execution
fragments. Current simulation-relation based methods for reasoning about
liveness properties of automata require reasoning over entire executions, since
they involve a proof obligation of the form: if a concrete and abstract
execution ``correspond'' via the simulation, and the concrete execution is
live, then so is the abstract execution.
Our contribution consists of (1) a formalism for defining liveness
properties, (2) a proof method for liveness properties based on that formalism,
and (3) two expressive completeness results: firstly, our formalism can express
any liveness property which satisfies a natural ``robustness'' condition, and
secondly, our formalism can express any liveness property at all, provided that
history variables can be used
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:55:03 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Attie",
"Paul C.",
""
]
] | [
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] |
801.095 | Franz X. Bronold | F. X. Bronold, H. Fehske, H. Kersten, and H. Deutsch | Surface states and the charge of a dust particle in a plasma | 4 pages, 3 figures, slightly revised manuscript including radius
dependence of the particle charge | Phys. Rev. Lett. 101, 175002 (2008) | 10.1103/PhysRevLett.101.175002 | null | physics.plasm-ph physics.space-ph | null | We investigate electron and ion surface states of a negatively charged dust
particle in a gas discharge and identify the charge of the particle with the
electron surface density bound in the polarization-induced short-range part of
the particle potential. On that scale, ions do not affect the charge. They are
trapped in the shallow states of the Coulomb tail of the potential and act only
as screening charges. Using orbital-motion limited electron charging fluxes and
the particle temperature as an adjustable parameter, we obtain excellent
agreement with experimental data.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:55:27 GMT"
},
{
"version": "v2",
"created": "Thu, 15 May 2008 13:25:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bronold",
"F. X.",
""
],
[
"Fehske",
"H.",
""
],
[
"Kersten",
"H.",
""
],
[
"Deutsch",
"H.",
""
]
] | [
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] |
801.0951 | Jesper Pedersen Mr. | Jesper Pedersen, Christian Flindt, Niels Asger Mortensen, Antti-Pekka
Jauho | Designed defects in 2D antidot lattices for quantum information
processing | 3 pages, 3 figures | Physica E 40, 1075 (2008). | 10.1016/j.physe.2007.08.016 | null | cond-mat.mes-hall | null | We propose a new physical implementation of spin qubits for quantum
information processing, namely defect states in antidot lattices defined in the
two-dimensional electron gas at a semiconductor heterostructure. Calculations
of the band structure of a periodic antidot lattice are presented. A point
defect is created by removing a single antidot, and calculations show that
localized states form within the defect, with an energy structure which is
robust against thermal dephasing. The exchange coupling between two electrons
residing in two tunnel-coupled defect states is calculated numerically. We find
results reminiscent of double quantum dot structures, indicating that the
suggested structure is a feasible physical implementation of spin qubits.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:06:40 GMT"
}
] | 2008-02-15T00:00:00 | [
[
"Pedersen",
"Jesper",
""
],
[
"Flindt",
"Christian",
""
],
[
"Mortensen",
"Niels Asger",
""
],
[
"Jauho",
"Antti-Pekka",
""
]
] | [
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] |
801.0952 | Becca Federico | Manuela Capello, Federico Becca, Michele Fabrizio, and Sandro Sorella | Mott transition in bosonic systems: Insights from the variational
approach | 12 pages and 19 figures. Related to arXiv:0705.2684 | Physical Review B 77, 144517 (2008) | 10.1103/PhysRevB.77.144517 | null | cond-mat.str-el | null | We study the Mott transition occurring for bosonic Hubbard models in one,
two, and three spatial dimensions, by means of a variational wave function
benchmarked by Green's function Monte Carlo calculations. We show that a very
accurate variational wave function, constructed by applying a long-range
Jastrow factor to the non-interacting boson ground state, can describe the
superfluid-insulator transition in any dimensionality. Moreover, by mapping the
quantum averages over such a wave function into the the partition function of a
classical model, important insights into the insulating phase are uncovered.
Finally, the evidence in favor of anomalous scenarios for the Mott transition
in two dimensions are reported whenever additional long-range repulsive
interactions are added to the Hamiltonian.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 11:59:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Capello",
"Manuela",
""
],
[
"Becca",
"Federico",
""
],
[
"Fabrizio",
"Michele",
""
],
[
"Sorella",
"Sandro",
""
]
] | [
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] |
801.0953 | Rudy Wijnands | Rudy Wijnands | Enigmatic sub-luminous accreting neutron stars in our Galaxy | Conference proceedings from 'A Population Explosion: The Nature and
Evolution of X-ray Binaries in Diverse Environments', 28 Oct - 2 Nov, St.
Petersburg Beach, FL | AIP Conf.Proc.1010:382-386,2008 | 10.1063/1.2945081 | null | astro-ph | null | During the last few years a class of enigmatic sub-luminous accreting neutron
stars has been found in our Galaxy. They have peak X-ray luminosities (2-10
keV) of a few times 1E34 erg/s to a few times 1E35 erg/s, and both persistent
and transient sources have been found. I present a short overview of our
knowledge of these systems and what we can learn from them.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:02:38 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Wijnands",
"Rudy",
""
]
] | [
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801.0954 | Kazuharu Bamba | Kazuharu Bamba and Sergei D. Odintsov | Inflation and late-time cosmic acceleration in non-minimal
Maxwell-$F(R)$ gravity and the generation of large-scale magnetic fields | 20 pages, no figure, JCAP version | JCAP 0804:024,2008 | 10.1088/1475-7516/2008/04/024 | KU-TP 019 | astro-ph gr-qc hep-ph hep-th | null | We study inflation and late-time acceleration in the expansion of the
universe in non-minimal electromagnetism, in which the electromagnetic field
couples to the scalar curvature function. It is shown that power-law inflation
can be realized due to the non-minimal gravitational coupling of the
electromagnetic field, and that large-scale magnetic fields can be generated
due to the breaking of the conformal invariance of the electromagnetic field
through its non-minimal gravitational coupling. Furthermore, it is demonstrated
that both inflation and the late-time acceleration of the universe can be
realized in a modified Maxwell-$F(R)$ gravity which is consistent with solar
system tests and cosmological bounds and free of instabilities. At small
curvature typical for current universe the standard Maxwell theory is
recovered. We also consider classically equivalent form of non-minimal
Maxwell-$F(R)$ gravity, and propose the origin of the non-minimal gravitational
coupling function based on renormalization-group considerations.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:04:05 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Mar 2008 18:43:48 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Bamba",
"Kazuharu",
""
],
[
"Odintsov",
"Sergei D.",
""
]
] | [
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] |
801.0955 | Jose Lorenzana | C. Ortix, J. Lorenzana and C. Di Castro | Phase diagram for Coulomb-frustrated phase separation in systems with
negative short-range compressibility | 4 pages, 3 figures. Improved figures and presentation | Phys. Rev. Lett. 100, 246402 (2008) | 10.1103/PhysRevLett.100.246402 | null | cond-mat.str-el cond-mat.mtrl-sci cond-mat.soft | null | Using numerical techniques and asymptotic expansions we obtain the phase
diagram of a paradigmatic model of Coulomb frustrated phase separation in
systems with negative short-range compressibility. The transition from the
homogeneous phase to the inhomogeneous phase is generically first order in
isotropic three-dimensional systems except for a critical point. Close to the
critical point, inhomogeneities are predicted to form a BCC lattice with
subsequent transitions to a triangular lattice of rods and a layered structure.
Inclusion of a strong anisotropy allows for second- and first-order transition
lines joined by a tricritical point.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:06:58 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Apr 2008 15:02:24 GMT"
}
] | 2008-07-10T00:00:00 | [
[
"Ortix",
"C.",
""
],
[
"Lorenzana",
"J.",
""
],
[
"Di Castro",
"C.",
""
]
] | [
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] |
801.0956 | Markus H. Thoma | Markus H. Thoma | Field Theoretic Description of Ultrarelativistic Electron-Positron
Plasmas | 13 pages, 7 figures, 1 table, published version | Rev.Mod.Phys.81:959-968,2009 | 10.1103/RevModPhys.81.959 | null | physics.plasm-ph astro-ph hep-ph nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Ultrarelativistic electron-positron plasmas can be produced in high-intensity
laser fields and play a role in various astrophysical situations. Their
properties can be calculated using QED at finite temperature. Here we will use
perturbative QED at finite temperature for calculating various important
properties, such as the equation of state, dispersion relations of collective
plasma modes of photons and electrons, Debye screening, damping rates, mean
free paths, collision times, transport coefficients, and particle production
rates, of ultrarelativistic electron-positron plasmas. In particular, we will
focus on electron-positron plasmas produced with ultra-strong lasers.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:07:12 GMT"
},
{
"version": "v2",
"created": "Mon, 6 Jul 2009 13:52:44 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Thoma",
"Markus H.",
""
]
] | [
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] |
801.0957 | Yury Zinoviev | Yury M. Zinoviev | Relativistic Newton and Coulomb Laws | null | null | null | null | math-ph math.MP | null | The relativistic equations for the electromagnetic and gravitation
interactions are similar: The only Lagrangian equation is the equation with
Lorentz force. The potential satisfies the wave equation with the right - hand
side proprtional to the velocity of another particle multiplied by the delta -
function concentrated at the position of another particle. If the interaction
propagates at the speed of light, then the wave equation has the unique
solution: the Lienard - Wiechert potential. The Maxwell equations are
completely defined by the obtained relativistic Coulomb law. The Coulomb law
and the Newton gravity law differ from each other only in the choice of the
constants. If we choose in Coulomb law the electric charges equal to the masses
and choose the interaction constant of another sign, then we get Newton gravity
law. If we choose in the relativistic Coulomb law the electric charges equal to
the masses and choose the interaction constant of another sign, then we get the
relativistic Newton gravity law.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:14:28 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Zinoviev",
"Yury M.",
""
]
] | [
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] |
801.0958 | Kazem Azizi | T. M. Aliev, K. Azizi, A. Ozpineci | QCD sum rules analysis of the $B_{s}\to D_{sJ}(2460)l\nu $ decay | Talk at the International Conference on Hadron Physics TROIA'07, 30
Aug. - 3 Sept. 2007, Canakkale, Turkey | null | null | null | hep-ph | null | Using three point QCD sum rules method, the form factors relevant to the
semileptonic
$B_{s}\to D_{sJ}(2460)\ell\nu$ decay are calculated. The $q^2$ dependencies
of these form factors are evaluated. The dependence of the asymmetry parameter
$\alpha$, characterizing the polarization of $D_{sJ}$ meson, on $q^2$ is
studied. This study gives useful information about the structure of the
$D_{sJ}$ meson. Finally the branching ratio of this decay is also estimated and
is shown that it can be easily detected at LHC.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:30:24 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Aliev",
"T. M.",
""
],
[
"Azizi",
"K.",
""
],
[
"Ozpineci",
"A.",
""
]
] | [
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] |
801.0959 | Hans Behringer | Hans Behringer, Andreas Degenhard, Friederike Schmid | Coarse-grained lattice model for investigating the role of cooperativity
in molecular recognition | 12 pages, 7 figures | Phys. Rev. E 76, 031914 (2007) | 10.1103/PhysRevE.76.031914 | null | physics.bio-ph | null | Equilibrium aspects of molecular recognition of rigid biomolecules are
investigated using coarse-grained lattice models. The analysis is carried out
in two stages. First an ensemble of probe molecules is designed with respect to
the target biomolecule. The recognition ability of the probe ensemble is then
investigated by calculating the free energy of association. The influence of
cooperative and anti-cooperative effects accompanying the association of the
target and probe molecules is studied. Numerical findings are presented and
compared to analytical results which can be obtained in the limit of dominating
cooperativity and in the mean-field formulation of the models.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:34:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Behringer",
"Hans",
""
],
[
"Degenhard",
"Andreas",
""
],
[
"Schmid",
"Friederike",
""
]
] | [
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] |
801.096 | Lorenzo Natalucci Dr. | L. Natalucci, M. Feroci, E. Quadrini, P. Ubertini, L. Piro, J.W. den
Herder, D. Barret, L. Amati, C. Budtz-Jorgensen, E. Caroli, S. Di Cosimo, M.
Frutti, C. Labanti, F. Monzani, J.M. Poulsen, L. Nicolini, A. Stevoli | Design of a CZT Gamma-Camera for GRB and Fast Transient Follow-up: a
Wide-Field-Monitor for the EDGE Mission | 9 pages, 7 figures, SPIE Conference on UV, X-ray, and Gamma-Ray
Instrumentation for Astronomy, San Diego 26-30 August 2007 | Proc.SPIE Int.Soc.Opt.Eng.6686:66860T,2007 | 10.1117/12.734522 | null | astro-ph | null | The success of the SWIFT/BAT and INTEGRAL missions has definitely opened a
new window for follow-up and deep study of the transient gamma-ray sky. This
now appears as the access key to important progresses in the area of
cosmological research and deep understanding of the physics of compact objects.
To detect in near real-time explosive events like Gamma-Ray bursts,
thermonuclear flashes from Neutron Stars and other types of X-ray outbursts we
have developed a concept for a wide-field gamma-ray coded mask instrument
working in the range 8-200 keV, having a sensitivity of 0.4 ph cm-2 s-1 in 1s
(15-150 keV) and arcmin location accuracy over a sky region as wide as 3sr.
This scientific requirement can be achieved by means of two large area, high
spatial resolution CZT detection planes made of arrays of relatively large
(~1cm2) crystals, which are in turn read out as matrices of smaller pixels. To
achieve such a wide Field-Of-View the two units can be placed at the sides of a
S/C platform serving a payload with a complex of powerful X-ray instruments, as
designed for the EDGE mission. The two units will be equipped with powerful
signal read out system and data handling electronics, providing accurate
on-board reconstruction of the source positions for fast, autonomous target
acquisition by the X-ray telescopes.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:34:59 GMT"
}
] | 2009-06-25T00:00:00 | [
[
"Natalucci",
"L.",
""
],
[
"Feroci",
"M.",
""
],
[
"Quadrini",
"E.",
""
],
[
"Ubertini",
"P.",
""
],
[
"Piro",
"L.",
""
],
[
"Herder",
"J. W. den",
""
],
[
"Barret",
"D.",
""
],
[
"Amati",
"L.",
""
],
[
"Budtz-Jorgensen",
"C.",
""
],
[
"Caroli",
"E.",
""
],
[
"Di Cosimo",
"S.",
""
],
[
"Frutti",
"M.",
""
],
[
"Labanti",
"C.",
""
],
[
"Monzani",
"F.",
""
],
[
"Poulsen",
"J. M.",
""
],
[
"Nicolini",
"L.",
""
],
[
"Stevoli",
"A.",
""
]
] | [
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801.0961 | Jerome Rodriguez | Jerome Rodriguez, Arash Bodaghee | The Galactic population of HMXBs as seen with INTEGRAL during its four
first years of activity | 5 pages, 3 figures proceedings of "A population explosion: the nature
and evolution of X-ray binaries in diverse environments", conference held in
St.Petersburg Beach, Florida; R.M.Bandyopadhyay, S.Wachter, D.Gelino,
C.R.Gelino, eds | null | 10.1063/1.2945046 | null | astro-ph | null | We collected the parameters (position, absorption, spin, orbital period,
etc..), when known, of all Galactic sources detected by INTEGRAL during its
four first years of activity. We use these parameters to test theoretical
predictions. For example, it is clear that HMXBs tend to be found mostly in the
tangential direction of the Galactic arms, while LMXBs tend to be clustered in
the Galactic bulge. We then focus on HMXBs and present two possible new tools,
in addition to the well-known ``Corbet-diagram'', to distinguish between
Be-HMXBs and Sg-HMXBs
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:41:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rodriguez",
"Jerome",
""
],
[
"Bodaghee",
"Arash",
""
]
] | [
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] |
801.0962 | Gabor Takacs | G. Takacs | Form factors of boundary exponential operators in the sinh-Gordon model | 22 pages, LaTeX2e file | null | 10.1016/j.nuclphysb.2008.01.025 | ITP-Budapest Report No. 637 | hep-th cond-mat.other | null | Using the recently introduced boundary form factor bootstrap equations, the
form factors of boundary exponential operators in the sinh-Gordon model are
constructed. The ultraviolet scaling dimension and the normalization of these
operators are checked against previously known results. The construction
presented in this paper can be applied to determine form factors of relevant
primary boundary operators in general integrable boundary quantum field
theories.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:53:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Takacs",
"G.",
""
]
] | [
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] |
801.0963 | Robert Brignall | Robert Brignall | A Survey of Simple Permutations | 21 pages, 6 figures | null | null | null | math.CO | null | We survey the known results about simple permutations. In particular, we
present a number of recent enumerative and structural results pertaining to
simple permutations, and show how simple permutations play an important role in
the study of permutation classes. We demonstrate how classes containing only
finitely many simple permutations satisfy a number of special properties
relating to enumeration, partial well-order and the property of being finitely
based.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:48:34 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Apr 2008 18:45:06 GMT"
}
] | 2008-04-18T00:00:00 | [
[
"Brignall",
"Robert",
""
]
] | [
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801.0964 | J. S. Kaastra | J.S. Kaastra, A.M. Bykov, S. Schindler, J.A.M. Bleeker, S. Borgani, A.
Diaferio, K. Dolag, F. Durret, J. Nevalainen, T. Ohashi, F.B.S. Paerels, V.
Petrosian, Y. Rephaeli, P. Richter, J. Schaye, N. Werner | Clusters of galaxies: beyond the thermal view | 6 pages, 1 figure, accepted for publication in Space Science Reviews,
special issue "Clusters of galaxies: beyond the thermal view", Editor J.S.
Kaastra, Chapter 1; work done by an international team at the International
Space Science Institute (ISSI), Bern, organised by J.S. Kaastra, A.M. Bykov,
S. Schindler & J.A.M. Bleeker | null | 10.1007/s11214-008-9326-3 | null | astro-ph | null | We present the work of an international team at the International Space
Science Institute (ISSI) in Bern that worked together to review the current
observational and theoretical status of the non-virialised X-ray emission
components in clusters of galaxies. The subject is important for the study of
large-scale hierarchical structure formation and to shed light on the "missing
baryon" problem. The topics of the team work include thermal emission and
absorption from the warm-hot intergalactic medium, non-thermal X-ray emission
in clusters of galaxies, physical processes and chemical enrichment of this
medium and clusters of galaxies, and the relationship between all these
processes. One of the main goals of the team is to write and discuss a series
of review papers on this subject. These reviews are intended as introductory
text and reference for scientists wishing to work actively in this field. The
team consists of sixteen experts in observations, theory and numerical
simulations.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:51:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kaastra",
"J. S.",
""
],
[
"Bykov",
"A. M.",
""
],
[
"Schindler",
"S.",
""
],
[
"Bleeker",
"J. A. M.",
""
],
[
"Borgani",
"S.",
""
],
[
"Diaferio",
"A.",
""
],
[
"Dolag",
"K.",
""
],
[
"Durret",
"F.",
""
],
[
"Nevalainen",
"J.",
""
],
[
"Ohashi",
"T.",
""
],
[
"Paerels",
"F. B. S.",
""
],
[
"Petrosian",
"V.",
""
],
[
"Rephaeli",
"Y.",
""
],
[
"Richter",
"P.",
""
],
[
"Schaye",
"J.",
""
],
[
"Werner",
"N.",
""
]
] | [
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] |
801.0965 | Rodolfo Smiljanic | R. Smiljanic (1,2), L. Pasquini (2), F. Primas (2), P. Mazzali (3,4),
D. Galli (5), G. Valle (6) ((1) Universidade de Sao Paulo - Brazil, (2) ESO -
Germany, (3) Max-Planck Institut fur Astrophysik - Germany, (4) Osservatorio
Astronomico de Trieste - Italy, (5) Osservatorio Astrofisico di Arcetri -
Italy, (6) Universita di Pisa - Italy) | Possible signature of hypernova nucleosynthesis in a beryllium rich halo
dwarf | Accepted for publication in the MNRAS letters | null | 10.1111/j.1745-3933.2008.00440.x | null | astro-ph | null | As part of a large survey of halo and thick disc stars, we found one halo
star, HD 106038, exceptionally overabundant in beryllium. In spite of its low
metallicity, [Fe/H] = -1.26, the star has log(Be/H) = -10.60, which is similar
to the solar meteoritic abundance, log(Be/H) = -10.58. This abundance is more
than ten times higher the abundance of stars with similar metallicity and
cannot be explained by models of chemical evolution of the Galaxy that include
the standard theory of cosmic-ray spallation. No other halo star exhibiting
such a beryllium overabundance is known. In addition, overabundances of Li, Si,
Ni, Y, and Ba are also observed. We suggest that all these chemical
peculiarities, but the Ba abundance, can be simultaneously explained if the
star was formed in the vicinity of a hypernova.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:52:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Smiljanic",
"R.",
""
],
[
"Pasquini",
"L.",
""
],
[
"Primas",
"F.",
""
],
[
"Mazzali",
"P.",
""
],
[
"Galli",
"D.",
""
],
[
"Valle",
"G.",
""
]
] | [
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] |
801.0966 | Magnus Borgh | M. Borgh, M. Koskinen, J. Christensson, M. Manninen, S. M. Reimann | Universality of Many-Body States in Rotating Bose and Fermi Systems | 9 pages, 9 figures | null | 10.1103/PhysRevA.77.033615 | null | cond-mat.mes-hall cond-mat.other | null | We propose a universal transformation from a many-boson state to a
corresponding many-fermion state in the lowest Landau level approximation of
rotating many-body systems, inspired by the Laughlin wave function and by the
Jain composite-fermion construction. We employ the exact-diagonalization
technique for finding the many-body states. The overlap between the transformed
boson ground state and the true fermion ground state is calculated in order to
measure the quality of the transformation. For very small and high angular
momenta, the overlap is typically above 90%. For intermediate angular momenta,
mixing between states complicates the picture and leads to small ground-state
overlaps at some angular momenta.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 12:55:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Borgh",
"M.",
""
],
[
"Koskinen",
"M.",
""
],
[
"Christensson",
"J.",
""
],
[
"Manninen",
"M.",
""
],
[
"Reimann",
"S. M.",
""
]
] | [
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] |
801.0967 | Marie Th\'eret | Rapha\"el Rossignol and Marie Th\'eret | Lower large deviations and laws of large numbers for maximal flows
through a box in first passage percolation | 39 pages, 4 figures; improvement of the moment conditions and
introduction of new results in the revised version | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider the standard first passage percolation model in $\mathbb{Z}^d$
for $d\geq 2$. We are interested in two quantities, the maximal flow $\tau$
between the lower half and the upper half of the box, and the maximal flow
$\phi$ between the top and the bottom of the box. A standard subadditive
argument yields the law of large numbers for $\tau$ in rational directions.
Kesten and Zhang have proved the law of large numbers for $\tau$ and $\phi$
when the sides of the box are parallel to the coordinate hyperplanes: the two
variables grow linearly with the surface $s$ of the basis of the box, with the
same deterministic speed. We study the probabilities that the rescaled
variables $\tau /s$ and $\phi /s$ are abnormally small. For $\tau$, the box can
have any orientation, whereas for $\phi$, we require either that the box is
sufficiently flat, or that its sides are parallel to the coordinate
hyperplanes. We show that these probabilities decay exponentially fast with
$s$, when $s$ grows to infinity. Moreover, we prove an associated large
deviation principle of speed $s$ for $\tau /s$ and $\phi /s$, and we improve
the conditions required to obtain the law of large numbers for these variables.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:28:08 GMT"
},
{
"version": "v2",
"created": "Fri, 3 Jul 2009 13:36:56 GMT"
}
] | 2009-07-03T00:00:00 | [
[
"Rossignol",
"Raphaël",
""
],
[
"Théret",
"Marie",
""
]
] | [
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] |
801.0968 | J. S. Kaastra | A. Diaferio, S. Schindler, K. Dolag | Clusters of galaxies: setting the stage | 20 pages, 8 figures, accepted for publication in Space Science
Reviews, special issue "Clusters of galaxies: beyond the thermal view",
Editor J.S. Kaastra, Chapter 2; work done by an international team at the
International Space Science Institute (ISSI), Bern, organised by J.S.
Kaastra, A.M. Bykov, S. Schindler & J.A.M. Bleeker | null | 10.1007/s11214-008-9324-5 | null | astro-ph | null | Clusters of galaxies are self-gravitating systems of mass ~10^14-10^15 Msun.
They consist of dark matter (~80 %), hot diffuse intracluster plasma (< 20 %)
and a small fraction of stars, dust, and cold gas, mostly locked in galaxies.
In most clusters, scaling relations between their properties testify that the
cluster components are in approximate dynamical equilibrium within the cluster
gravitational potential well. However, spatially inhomogeneous thermal and
non-thermal emission of the intracluster medium (ICM), observed in some
clusters in the X-ray and radio bands, and the kinematic and morphological
segregation of galaxies are a signature of non-gravitational processes, ongoing
cluster merging and interactions. In the current bottom-up scenario for the
formation of cosmic structure, clusters are the most massive nodes of the
filamentary large-scale structure of the cosmic web and form by anisotropic and
episodic accretion of mass. In this model of the universe dominated by cold
dark matter, at the present time most baryons are expected to be in a diffuse
component rather than in stars and galaxies; moreover, ~50 % of this diffuse
component has temperature ~0.01-1 keV and permeates the filamentary
distribution of the dark matter. The temperature of this Warm-Hot Intergalactic
Medium (WHIM) increases with the local density and its search in the outer
regions of clusters and lower density regions has been the quest of much recent
observational effort. Over the last thirty years, an impressive coherent
picture of the formation and evolution of cosmic structures has emerged from
the intense interplay between observations, theory and numerical experiments.
Future efforts will continue to test whether this picture keeps being valid,
needs corrections or suffers dramatic failures in its predictive power.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:35:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Diaferio",
"A.",
""
],
[
"Schindler",
"S.",
""
],
[
"Dolag",
"K.",
""
]
] | [
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] |
801.0969 | Javier Gonz\'alez Est\'evez | J. Gonzalez-Estevez, M. G. Cosenza, R. Lopez-Ruiz, and J. R. Sanchez | Pareto and Boltzmann-Gibbs behaviors in a deterministic multi-agent
system | 9 pages, 9 color .eps figures, submitted to Physica A | null | 10.1016/j.physa.2008.03.013 | null | q-fin.GN cond-mat.stat-mech cs.MA nlin.AO nlin.CD physics.comp-ph physics.soc-ph | null | A deterministic system of interacting agents is considered as a model for
economic dynamics. The dynamics of the system is described by a coupled map
lattice with near neighbor interactions. The evolution of each agent results
from the competition between two factors: the agent's own tendency to grow and
the environmental influence that moderates this growth. Depending on the values
of the parameters that control these factors, the system can display Pareto or
Boltzmann-Gibbs statistical behaviors in its asymptotic dynamical regime. The
regions where these behaviors appear are calculated on the space of parameters
of the system. Other statistical properties, such as the mean wealth, the
standard deviation, and the Gini coefficient characterizing the degree of
equity in the wealth distribution are also calculated on the space of
parameters of the system.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:15:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gonzalez-Estevez",
"J.",
""
],
[
"Cosenza",
"M. G.",
""
],
[
"Lopez-Ruiz",
"R.",
""
],
[
"Sanchez",
"J. R.",
""
]
] | [
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] |
801.097 | Nathalie Akakpo | Nathalie Akakpo | Detecting change-points in a discrete distribution via model selection | Submitted to the Electronic Journal of Statistics
(http://www.i-journals.org/ejs/) by the Institute of Mathematical Statistics
(http://www.imstat.org) | null | null | IMS-EJS-EJS_2008_170 | math.ST stat.TH | null | This paper is concerned with the detection of multiple change-points in the
joint distribution of independent categorical variables. The procedures
introduced rely on model selection and are based on a penalized least-squares
criterion. Their performance is assessed from a nonasymptotic point of view.
Using a special collection of models, a preliminary estimator is built.
According to an existing model selection theorem, it satisfies an oracle-type
inequality. Moreover, thanks to an approximation result demonstrated in this
paper, it is also proved to be adaptive in the minimax sense. In order to
eliminate some irrelevant change-points selected by that first estimator, a
two-stage procedure is proposed, that also enjoys some adaptivity property.
Besides, the first estimator can be computed with a complexity only linear in
the size of the data. A heuristic method allows to implement the second
procedure quite satisfactorily with the same computational complexity.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:17:05 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Akakpo",
"Nathalie",
""
]
] | [
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] |
801.0971 | Matthias Maercker | Matthias Maercker, Fredrik L. Schoeier, Hans Olofsson, Per Bergman,
Sofia Ramstedt | Circumstellar water vapour in M-type AGB stars: Radiative transfer
models, abundances and predictions for HIFI | Accepted by A&A, Dec 12 2007, 13 pages, 8 figures, correct
affiliation address | null | 10.1051/0004-6361:20078680 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Aims: By performing a detailed radiative transfer analysis, we determine
fractional abundances of circumstellar H2O in the envelopes around six M-type
asymptotic giant branch stars. The models are also used to predict H2O spectral
line emission for the upcoming Herschel/HIFI mission.
Methods: We use Infrared space observatory long wavelength spectrometer
spectra to constrain the circumstellar fractional abundance distribution of
ortho-H2O, using a non-local thermal equilibrium, and non-local, radiative
transfer code based on the accelerated lambda iteration formalism. The
mass-loss rates and kinetic temperature structures for the sample stars are
determined through radiative transfer modelling of CO line emission based on
the Monte-Carlo method. The density and temperature profiles of the
circumstellar dust grains are determined through spectral energy distribution
modelling using the publicly available code Dusty.
Results: The determined ortho-H2O abundances lie between 1e-4 and 1.5e-3
relative to H2, with the exception of WX Psc, which has a much lower estimated
ortho-H2O abundance of only 2e-6, possibly indicating H_2O adsorption onto dust
grains or recent mass-loss-rate modulations. The estimated abundances are
uncertain by, at best, a factor of a few.
Conclusions: The high water abundance found for the majority of the sources
suggests that either the `normal' chemical processes are very effective in
producing H2O, or else non-local thermal equilibrium atmospheric chemistry,
grain surface reactions, or a release of H_2O (e.g. from icy bodies like Kuiper
belt objects) play a role. We provide predictions for ortho-H2O lines in the
spectral window of Herschel/HIFI.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:48:25 GMT"
},
{
"version": "v2",
"created": "Sat, 10 Jan 2009 14:20:31 GMT"
},
{
"version": "v3",
"created": "Wed, 14 Apr 2010 11:58:37 GMT"
}
] | 2010-04-15T00:00:00 | [
[
"Maercker",
"Matthias",
""
],
[
"Schoeier",
"Fredrik L.",
""
],
[
"Olofsson",
"Hans",
""
],
[
"Bergman",
"Per",
""
],
[
"Ramstedt",
"Sofia",
""
]
] | [
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] |
801.0972 | Philippe Lebacque | Philippe Lebacque | On Tsfasman--Vl\u{a}du\c{t} Invariants of Infinite Global Fields | null | null | null | null | math.NT | null | In this article we study certain asymptotic properties of global fields. We
consider the set of Tsfasman-Vladuts invariants of infinite global fields and
answer some natural questions arising from their work. In particular, we prove
the existence of infinite global fields having finitely many strictly positive
invariants at given places, and the existence of infinite number fields with
certain prescribed invariants being zero. We also give precisions on the
deficiency of infinite global fields and on the primes decomposition in those
fields.
| [
{
"version": "v1",
"created": "Mon, 7 Jan 2008 13:38:15 GMT"
}
] | 2008-01-08T00:00:00 | [
[
"Lebacque",
"Philippe",
""
]
] | [
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