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802.1603 | Robert Cameron | R. Cameron, L. Gizon, T.L. Duvall Jr | Helioseismology of Sunspots: Confronting Observations with
Three-Dimensional MHD Simulations of Wave Propagation | 21 pages, Accepted in Solar Physics | null | 10.1007/s11207-008-9148-1 | null | astro-ph | null | The propagation of solar waves through the sunspot of AR 9787 is observed
using temporal cross-correlations of SOHO/MDI Dopplergrams. We then use
three-dimensional MHD numerical simulations to compute the propagation of wave
packets through self-similar magneto-hydrostatic sunspot models. The
simulations are set up in such a way as to allow a comparison with observed
cross-covariances (except in the immediate vicinity of the sunspot). We find
that the simulation and the f-mode observations are in good agreement when the
model sunspot has a peak field strength of 3 kG at the photosphere, less so for
lower field strengths. Constraining the sunspot model with helioseismology is
only possible because the direct effect of the magnetic field on the waves has
been fully taken into account. Our work shows that the full-waveform modeling
of sunspots is feasible.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 10:04:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cameron",
"R.",
""
],
[
"Gizon",
"L.",
""
],
[
"Duvall",
"T. L.",
"Jr"
]
] | [
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802.1604 | Constantinos Daskalakis | Constantinos Daskalakis, Grant Schoenebeck, Gregory Valiant, Paul
Valiant | On the Complexity of Nash Equilibria of Action-Graph Games | null | null | null | null | cs.GT cs.MA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider the problem of computing Nash Equilibria of action-graph games
(AGGs). AGGs, introduced by Bhat and Leyton-Brown, is a succinct representation
of games that encapsulates both "local" dependencies as in graphical games, and
partial indifference to other agents' identities as in anonymous games, which
occur in many natural settings. This is achieved by specifying a graph on the
set of actions, so that the payoff of an agent for selecting a strategy depends
only on the number of agents playing each of the neighboring strategies in the
action graph. We present a Polynomial Time Approximation Scheme for computing
mixed Nash equilibria of AGGs with constant treewidth and a constant number of
agent types (and an arbitrary number of strategies), together with hardness
results for the cases when either the treewidth or the number of agent types is
unconstrained. In particular, we show that even if the action graph is a tree,
but the number of agent-types is unconstrained, it is NP-complete to decide the
existence of a pure-strategy Nash equilibrium and PPAD-complete to compute a
mixed Nash equilibrium (even an approximate one); similarly for symmetric AGGs
(all agents belong to a single type), if we allow arbitrary treewidth. These
hardness results suggest that, in some sense, our PTAS is as strong of a
positive result as one can expect.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 09:45:36 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Daskalakis",
"Constantinos",
""
],
[
"Schoenebeck",
"Grant",
""
],
[
"Valiant",
"Gregory",
""
],
[
"Valiant",
"Paul",
""
]
] | [
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802.1605 | Yves Colin De Verdiere | Yves Colin De Verdi\`ere (IF), Victor Guillemin | A semi-classical inverse problem I: Taylor expansions | 15 pages | null | null | null | math-ph math.AP math.MP math.SP | null | In dimension 1, we show that the Taylor expansion of a potential near a
generic non degenerate critical point can be recovered from the knowledge of
the semi-classical spectrum of the associated Schr\"odinger operator near the
corresponding critical value.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 09:46:49 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"De Verdière",
"Yves Colin",
"",
"IF"
],
[
"Guillemin",
"Victor",
""
]
] | [
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] |
802.1606 | Chang Ho Hyun | C. H. Hyun, B. Desplanques, S. Ando, C.-P. Liu | The old and the new of parity-violating two-pion-exchange $NN$ potential | 4 pages, contribution to the conference Chiral07 held in Osaka,
Japan, Nov. 13-16, 2007 | Mod.Phys.Lett.A23:2293-2296,2008 | 10.1142/S0217732308029228 | null | nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider the parity-violating two-pion-exchange potential obtained from
the covariant formalism in the past and the state-of-the-art effective field
theory approach. We discuss the behavior of the potential in coordinate space
and its application to the parity-violating asymmetry in $\vec{n} p \to d
\gamma$ at threshold.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 09:46:54 GMT"
}
] | 2009-01-30T00:00:00 | [
[
"Hyun",
"C. H.",
""
],
[
"Desplanques",
"B.",
""
],
[
"Ando",
"S.",
""
],
[
"Liu",
"C. -P.",
""
]
] | [
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] |
802.1607 | Marta Sanz-Sol\'e | Marta Sanz-Sol\'e | Properties of the density for a three dimensional stochastic wave
equation | 29 pages | null | null | null | math.PR math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider a stochastic wave equation in space dimension three driven by a
noise white in time and with an absolutely continuous correlation measure given
by the product of a smooth function and a Riesz kernel. Let $p_{t,x}(y)$ be the
density of the law of the solution $u(t,x)$ of such an equation at points
$(t,x)\in]0,T]\times \IR^3$. We prove that the mapping $(t,x)\mapsto
p_{t,x}(y)$ owns the same regularity as the sample paths of the process
$\{u(t,x), (t,x)\in]0,T]\times \mathbbR^3\}$ established Dalang and Sanz-Sol\'e
[Memoirs of the AMS, to appear]. The proof relies on Malliavin calculus and
more explicitely, Watanabe's integration by parts formula and estimates derived
form it.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 09:48:21 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Sanz-Solé",
"Marta",
""
]
] | [
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] |
802.1608 | Luis Escauriaza | L. Escauriaza, C. E. Kenig, G. Ponce, L. Vega | Hardy's Uncertainty Principle, Convexity and Schr\"odinger Evolutions | null | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove the logarithmic convexity of certain quantities, which measure the
quadratic exponential decay at infinity and within two characteristic
hyperplanes of solutions of Schr\"odinger evolutions. As a consequence we
obtain some uniqueness results that generalize (a weak form of) Hardy's version
of the uncertainty principle. We also obtain corresponding results for heat
evolutions.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 09:49:42 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Escauriaza",
"L.",
""
],
[
"Kenig",
"C. E.",
""
],
[
"Ponce",
"G.",
""
],
[
"Vega",
"L.",
""
]
] | [
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] |
802.1609 | Jun Suzuki | Jun Suzuki, Gelo Noel Macuja Tabia, Berthold-Georg Englert | Symmetric construction of reference-frame-free qudits | 5 pages, typos corrected | Phys. Rev. A 78, 052328 (2008) | 10.1103/PhysRevA.78.052328 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | By exploiting a symmetric scheme for coupling $N$ spin-1/2 constituents (the
physical qubits) to states with total angular momentum $N/2-1$, we construct
rotationally invariant logical qudits of dimension $d=N-1$. One can encode all
qudit states, and realize all qudit measurements, by this construction. The
rotational invariance of all relevant objects enables one to transmit quantum
information without having aligned reference frames between the parties that
exchange the qudits. We illustrate the method by explicit constructions of
reference-frame-free qubits and qutrits and, for the qubit case, comment on
possible experimental implementations.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 09:59:24 GMT"
},
{
"version": "v2",
"created": "Fri, 17 Oct 2008 02:14:09 GMT"
}
] | 2008-11-25T00:00:00 | [
[
"Suzuki",
"Jun",
""
],
[
"Tabia",
"Gelo Noel Macuja",
""
],
[
"Englert",
"Berthold-Georg",
""
]
] | [
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] |
802.161 | Lan Zhou | Jing Lu, Lan Zhou, Le-Man Kuang, C. P. Sun | Controlling soliton excitations in Heisenberg spin chain through magic
angle | 7 pages 4 figures | Physical Review E 79, 016606 (2009) | 10.1103/PhysRevE.79.016606 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the nonlinear dynamics of collective excitation in a $N$-site $XXZ$
quantum spin chain, which is manipulated by an oblique magnetic field. We show
that, when the tilted field is applied along the magic angle $\theta_{0}
=\pm\arccos \sqrt{1/3}$, the anisotropic Heisenberg spin chain becomes
isotropic and thus an free propagating spin wave is stimulated. And in the
regime of the tilted angle larger and smaller then the magic angle, two types
of nonlinear excitations appear, which are bright soliton and dark soliton.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 10:28:32 GMT"
},
{
"version": "v2",
"created": "Mon, 26 May 2008 05:24:34 GMT"
},
{
"version": "v3",
"created": "Thu, 19 Jun 2008 07:32:45 GMT"
},
{
"version": "v4",
"created": "Sun, 15 Feb 2009 16:22:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lu",
"Jing",
""
],
[
"Zhou",
"Lan",
""
],
[
"Kuang",
"Le-Man",
""
],
[
"Sun",
"C. P.",
""
]
] | [
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] |
802.1611 | Christian Forss\'en | C. Forss\'en and J. P. Vary and E. Caurier and P. Navr\'atil | Converging sequences in the ab initio no-core shell model | null | Phys.Rev.C77:024301,2008 | 10.1103/PhysRevC.77.024301 | null | nucl-th | null | We demonstrate the existence of multiple converging sequences in the ab
initio no-core shell model. By examining the underlying theory of effective
operators, we expose the physical foundations for the alternative pathways to
convergence. This leads us to propose a revised strategy for evaluating
effective interactions for $A$-body calculations in restricted model spaces. We
suggest that this strategy is particularly useful for applications to nuclear
processes in which states of both parities are used simultaneously, such as for
transition rates. We demonstrate the utility of our strategy with large-scale
calculations in light nuclei.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 10:35:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Forssén",
"C.",
""
],
[
"Vary",
"J. P.",
""
],
[
"Caurier",
"E.",
""
],
[
"Navrátil",
"P.",
""
]
] | [
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] |
802.1612 | Christian Mercat | Christian Mercat (I3M) | Discrete Riemann Surfaces | null | Handbook of Teichm\"uller theory. Vol. I, Eur. Math. Soc.,
Z\"urich (Ed.) (2007) 541--575 | null | null | math.CV math-ph math.DG math.MP | null | We detail the theory of Discrete Riemann Surfaces. It takes place on a
cellular decomposition of a surface, together with its Poincar\'e dual,
equipped with a discrete conformal structure. A lot of theorems of the
continuous theory follow through to the discrete case, we define the discrete
analogs of period matrices, Riemann's bilinear relations, exponential of
constant argument and series. We present the notion of criticality and its
relationship with integrability.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 10:36:56 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Mercat",
"Christian",
"",
"I3M"
]
] | [
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] |
802.1613 | Laura Tolos | Laura Tolos, Angels Ramos and Tetsuro Mizutani | Charm mesons at FAIR | 4 pages, 3 figures, contribution to the proceedings of Chiral07,
RCNP, Osaka, Japan, November 13-16, 2007 | Mod.Phys.Lett.A23:2250-2253,2008 | 10.1142/S0217732308029137 | null | nucl-th hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The in-medium properties of charm mesons ($D$ and $\bar D$) in a hot and
dense matter are studied. A self-consistent coupled-channel approach is driven
by a broken SU(4) s-wave Tomozawa-Weinberg interaction supplemented by an
attractive isoscalar-scalar term. As medium effects, we include Pauli blocking,
baryon mean-field bindings, and $\pi$ and open-charm meson self-energies. The
dynamically generated $\tilde\Lambda_c$ and $\tilde\Sigma_c$ resonances in the
$DN$ sector remain close to their free space position but acquire large widths.
The resultant $D$ meson spectral function, which shows a single pronounced
quasiparticle peak close to the free mass that broadens with increasing
density, also has a long low energy tail associated with smeared
$\tilde\Lambda_c N^{-1}$, $\tilde\Sigma_c N^{-1}$ configurations. The
low-density approximation for the $\bar D N$ is questionable already at
subsaturation densities. We touch upon the implication of our study for
$J/\Psi$ suppression at FAIR.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 10:42:28 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Tolos",
"Laura",
""
],
[
"Ramos",
"Angels",
""
],
[
"Mizutani",
"Tetsuro",
""
]
] | [
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] |
802.1614 | Raymond Burston | R. Burston, L. Gizon, T. Appourchaux, W.T. Ni, ASTROD I ESA cosmic
vision 2015-2025 team | Detecting solar g-modes with ASTROD | HELAS II international conference "Helioseismology, asteroseismology
and MHD connections", 20-24 August 2007, Goettingen, Germany | J.Phys.Conf.Ser.118:012043,2008 | 10.1088/1742-6596/118/1/012043 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present an up-to-date estimate for the prospect of using the
Astrodynamical Space Test of Relativity using Optical Devices (ASTROD) for an
unambiguous detection of solar g modes (f < 400 micro Hertz) through their
gravitational signature. There are currently two major efforts to detect
low-frequency gravitational effects, ASTROD and the Laser Interferometer Space
Antenna (LISA). Using the most recent g mode surface amplitude estimates, both
observational and theoretical, it is unclear whether LISA will be capable of
successfully detecting these modes. The ASTROD project may be better suited for
detection as its sensitivity curve is shifted towards lower frequencies with
the best sensitivity occurring in the range 100-300 micro Hertz.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 10:54:27 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Burston",
"R.",
""
],
[
"Gizon",
"L.",
""
],
[
"Appourchaux",
"T.",
""
],
[
"Ni",
"W. T.",
""
],
[
"team",
"ASTROD I ESA cosmic vision 2015-2025",
""
]
] | [
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] |
802.1615 | Jan Mandel | Jonathan D. Beezley, Soham Chakraborty, Janice L. Coen, Craig C.
Douglas, Jan Mandel, Anthony Vodacek, Zhen Wang | Real-Time Data Driven Wildland Fire Modeling | 8 pages, 4 figures. ICCS 08 | Proceedings ICCS 2008. Lecture Notes in Computer Science vol 5103
pp 46-53 2008. | 10.1007/978-3-540-69389-5_7 | null | physics.ao-ph physics.comp-ph | null | We are developing a wildland fire model based on semi-empirical relations
that estimate the rate of spread of a surface fire and post-frontal heat
release, coupled with WRF, the Weather Research and Forecasting atmospheric
model. A level set method identifies the fire front. Data are assimilated using
both amplitude and position corrections using a morphing ensemble Kalman
filter. We will use thermal images of a fire for observations that will be
compared to synthetic image based on the model state.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:08:00 GMT"
}
] | 2009-01-09T00:00:00 | [
[
"Beezley",
"Jonathan D.",
""
],
[
"Chakraborty",
"Soham",
""
],
[
"Coen",
"Janice L.",
""
],
[
"Douglas",
"Craig C.",
""
],
[
"Mandel",
"Jan",
""
],
[
"Vodacek",
"Anthony",
""
],
[
"Wang",
"Zhen",
""
]
] | [
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802.1616 | Eberhard Mayerhofer | Eberhard Mayerhofer | The wave equation on static singular space-times | 102 pages, 4 figures, PhD Thesis, concise introduction | PhD thesis, University of Vienna, 2006 | null | null | math.GM math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The first part of my thesis lays the foundations to generalized Lorentz
geometry. The basic algebraic structure of finite-dimensional modules over the
ring of generalized numbers is investigated. The motivation for this part of my
thesis evolved from the main topic, the wave equation on singular space-times.
The second and main part of my thesis is devoted to establishing a local
existence and uniqueness theorem for the wave equation on singular space-times.
The singular Lorentz metric subject to our discussion is modeled within the
special algebra on manifolds in the sense of Colombeau. Inspired by an approach
to generalized hyperbolicity of conical-space times due to Vickers and Wilson,
we succeed in establishing certain energy estimates, which by a further
elaborated equivalence of energy integrals and Sobolev norms allow us to prove
existence and uniqueness of local generalized solutions of the wave equation
with respect to a wide class of generalized metrics. The third part of my
thesis treats three different point value resp. uniqueness questions in
algebras of generalized functions
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:03:24 GMT"
}
] | 2021-01-12T00:00:00 | [
[
"Mayerhofer",
"Eberhard",
""
]
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] |
802.1617 | Christian Mercat | Christian Mercat (I3M) | Discrete Complex Structure on Surfel Surfaces | null | Dans 14th IAPR International Conference on Discrete Geometry for
Computer Imagery - 14th IAPR International Conference on Discrete Geometry
for Computer Imagery, Lyon : France (2008) | null | null | cs.CG cs.GR math.CV | null | This paper defines a theory of conformal parametrization of digital surfaces
made of surfels equipped with a normal vector. The main idea is to locally
project each surfel to the tangent plane, therefore deforming its aspect-ratio.
It is a generalization of the theory known for polyhedral surfaces. The main
difference is that the conformal ratios that appear are no longer real in
general. It yields a generalization of the standard Laplacian on weighted
graphs.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:06:38 GMT"
}
] | 2008-02-18T00:00:00 | [
[
"Mercat",
"Christian",
"",
"I3M"
]
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802.1618 | Hashem Zoubi | Hashem Zoubi and Helmut Ritsch | Coupling of Electronic and Motional Dynamics in a Cold Atom Optical
Lattice | 4 pages, 5 figures | Phys. Rev. A 79, 023411 (2009). | 10.1103/PhysRevA.79.023411 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the coupling of internal electronic excitations to vibrational modes
of the external motion of ultracold atoms in an optical lattice. For different
ground and excited state potentials the on-site coupling of excitations and
vibrations term renormalizes the effective electronic transition energy, which
appears e.g. in clock transitions. In addition in the Mott state with filling
factor one, the dipole-dipole coupling between neighbouring sites includes
emission and absorption of vibrational quanta. Such processes create a
significant mechanism for excitation of vibrations leading to motional heating
of the lattice atoms by resonant light interaction. We calculate estimates of
the corresponding parameters from a perturbation expansion in small atomic
displacements.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:21:39 GMT"
}
] | 2009-08-11T00:00:00 | [
[
"Zoubi",
"Hashem",
""
],
[
"Ritsch",
"Helmut",
""
]
] | [
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] |
802.1619 | G. Griffith Elder | G. Griffith Elder | A valuation criterion for normal basis generators in local fields of
characteristic $p$ | null | null | null | null | math.NT math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $K$ be a complete local field of characteristic $p$ with perfect residue
field. Let $L/K$ be a finite, fully ramified, Galois $p$-extension. If
$\pi_L\in L$ is a prime element, and $p'(x)$ is the derivative of $\pi_L$'s
minimal polynomial over $K$, then the relative different $\euD_{L/K}$ is
generated by $p'(\pi_L)\in L$. Let $v_L$ be the normalized valuation normalized
with $v_L(L)=\mathbb{Z}$. We show that any element $\rho\in L$ with
$v_L(\rho)\equiv -v_L(p'(\pi_L))-1\bmod[L:K]$ generates a normal basis,
$K[{Gal}(L/K)]\cdot\rho=L$. This criterion is tight: Given any integer $i$ such
that $i\not\equiv -v_L(p'(\pi_L))-1\bmod[L:K]$, there is a $\rho_i\in L$ with
$v_L(\rho_i)=i$ such that $K[{Gal}(L/K)]\cdot\rho_i\subsetneq L$.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:50:27 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Elder",
"G. Griffith",
""
]
] | [
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] |
802.162 | Andreas Schadschneider | Andreas Schadschneider, Wolfram Klingsch, Hubert Kluepfel, Tobias
Kretz, Christian Rogsch, and Armin Seyfried | Evacuation Dynamics: Empirical Results, Modeling and Applications | 57 pages, 19 figures; to appear in: ``Encyclopedia of Complexity and
System Science'', B. Meyers (Ed.) (Springer, Berlin, 2008); for more
information and a version with high quality figures, see
<http://www.ped-net.org> | Encyclopedia of Complexity and Systems Science (Editor-in-Chief:
R.A. Meyers), pages 3142-3176 (Springer 2009) | 10.1016/j.ssci.2011.12.024 | null | physics.soc-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This extensive review was written for the ``Encyclopedia of Complexity and
System Science'' (Springer, 2008) and addresses a broad audience ranging from
engineers to applied mathematicians, computer scientists and physicists. It
provides an extensive overview of various aspects of pedestrian dynamics,
focussing on evacuation processes. First the current status of empirical
results is critically reviewed as it forms the basis for the calibration of
models needed for quantitative predictions. Then various modeling approaches
are discussed, focussing on cellular automata models. Finally, some specific
applications to safety analysis in public buildings or public transport are
presented.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:32:20 GMT"
}
] | 2012-02-15T00:00:00 | [
[
"Schadschneider",
"Andreas",
""
],
[
"Klingsch",
"Wolfram",
""
],
[
"Kluepfel",
"Hubert",
""
],
[
"Kretz",
"Tobias",
""
],
[
"Rogsch",
"Christian",
""
],
[
"Seyfried",
"Armin",
""
]
] | [
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] |
802.1621 | Hong Soo Park | Myung Gyoon Lee (1), Hong Soo Park (1), Eunhyeuk Kim (1), Ho Seong
Hwang (1,2), Sang Chul Kim (3), Doug Geisler (4)((1) Seoul National
Univ.,(2)Korea Institute for Advanced Study,(3)Korea Astronomy and Space
Science Institute,(4)Univ. de Concepci) | Washington CCD Photometry of the Globular Cluster System of the Giant
Elliptical Galaxy M60 in Virgo | 32 pages, 22 figues, Accepted by ApJ | Astrophys.J.682:135-154,2008 | 10.1086/587469 | null | astro-ph | null | We present a photometric study of the globular clusters in the giant
elliptical galaxy M60 in the Virgo cluster, based on deep, relatively wide
field Washington CT_1 CCD images. The color-magnitude diagram reveals a
significant population of globular clusters in M60, and a large number of young
luminous clusters in NGC 4647, a small companion spiral galaxy north-west of
M60. The color distribution of the globular clusters in M60 is clearly bimodal,
with a blue peak at (C-T_1)=1.37, and a red peak at (C-T_1)=1.87. We derive two
new transformation relations between the (C-T_1)_0 color and [Fe/H] using the
data for the globular clusters in our Galaxy and M49. Using these relations we
derive the metallicity distribution of the globular clusters in M60, which is
also bimodal: a dominant metal-poor component with center at [Fe/H]=-1.2, and a
weaker metal-rich component with center at [Fe/H]=-0.2. The radial number
density profile of the globular clusters is more extended than that of the
stellar halo, and the radial number density profile of the blue globular
clusters is more extended than that of the red globular clusters. The number
density maps of the globular clusters show that the spatial distribution of the
blue globular clusters is roughly circular, while that of the red globular
cluster is elongated similarly to that of the stellar halo. We estimate the
total number of the globular clusters in M60 to be 3600+/-500$,and the specific
frequency to be S_N=3.8+/-0.4. The mean color of the bright blue globular
clusters gets redder as they get brighter in both the inner and outer region of
M60. This blue tilt is seen also in the outer region of M49, the brightest
Virgo galaxy. Implications of these results are discussed.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:52:23 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Lee",
"Myung Gyoon",
""
],
[
"Park",
"Hong Soo",
""
],
[
"Kim",
"Eunhyeuk",
""
],
[
"Hwang",
"Ho Seong",
""
],
[
"Kim",
"Sang Chul",
""
],
[
"Geisler",
"Doug",
""
]
] | [
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] |
802.1622 | Michele Fumagalli | Giuseppe Gavazzi (1), Riccardo Giovanelli (2), Martha P. Haynes (2),
Silvia Fabello (1), Michele Fumagalli (1), Brian R. Kent (2), Rebecca A.
Koopmann (3), Noah Brosch (4), G. Lyle Hoffman (5), John J. Salzer (6) and
Alessandro Boselli (7) ((1) Universita degli Studi di Milano-Bicocca, Italy
(2) Cornell University (3) Union College (4) The Wise Observatory, Israel (5)
Lafayette College (6) Wesleyan University (7) Laboratoire d'Astrophysique de
Marseille, France) | HI content and other structural properties of galaxies in the Virgo
cluster from the Arecibo Legacy Fast ALFA Survey | 10 pages, 10 Postscript figures, accepted for publication in
Astronomy and Astrophysics (25/01/2008) - Replaced to fit A&A vers. 6.1 | null | 10.1051/0004-6361:200809382 | null | astro-ph | null | We report the results of an HI blind survey of 80deg^2 of the Virgo cluster,
based on the 08deg < delta < 16 deg strip of ALFALFA, the Arecibo Legacy Fast
ALFA Survey. 187 HI sources of high significance are found providing a complete
census of HI sources in this region of the Virgo cluster (-1000<cz<3000 km/s)
with M_HI > 10^7.5-8 M_sun. 156/187 (83%) sources are identified with optical
galaxies from the Virgo Cluster Catalogue (Binggeli et al. 1985), all but 8
with late-type galaxies. Ten sources are not associated with optical galaxies
and were found to correspond to tidally-disrupted systems (see Kent et al. 2007
and Haynes, Giovanelli and Kent 2007). The remaining 21 (11%) are associated
with galaxies that are not listed in the Virgo Cluster Catalogue. For all
sources with an optical counterpart in the Sloan Digital Sky Survey, we
analyzed i-band SDSS plates to measure optical structural parameters. We find
that in the Virgo cluster: i) HI inhabits galaxies that are structurally
similar to ordinary late-type galaxies; ii) their HI content can be predicted
from their optical luminosity; iii) low surface brightness galaxies have low
optical luminosity and contain small quantities of neutral hydrogen; iv) low
surface brightness, massive Malin1 type galaxies are comfortably rare objects
(less than 0.5%); v) there are no "dark-galaxies" with HI masses M_HI >
10^7.5-8 M_sun; vi) less than 1% of early-type galaxies contain neutral
hydrogen with M_HI>10^7.5-8 M_sun (di Serego Alighieri et al. 2007).
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:42:07 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 11:21:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gavazzi",
"Giuseppe",
""
],
[
"Giovanelli",
"Riccardo",
""
],
[
"Haynes",
"Martha P.",
""
],
[
"Fabello",
"Silvia",
""
],
[
"Fumagalli",
"Michele",
""
],
[
"Kent",
"Brian R.",
""
],
[
"Koopmann",
"Rebecca A.",
""
],
[
"Brosch",
"Noah",
""
],
[
"Hoffman",
"G. Lyle",
""
],
[
"Salzer",
"John J.",
""
],
[
"Boselli",
"Alessandro",
""
]
] | [
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] |
802.1623 | Farhad Zolfagharour | F. Zolfagharpour | EMC effect with different oscillator-model parameters $h\omega$ for
different shells by considering difference between proton and neutron
structure functions | 10 pages 4 figures | null | null | null | nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The magnitude of binding energy used in the conventional nuclear theory to
explain the EMC experimental data, seems to be larger than the one expected. In
this paper to get sufficient depletion in the binding energy, different
oscillator-model parameters $ \textit{$h\omega$} $ for different shells and the
proton (neutron) structure function that have good agrement with experimental
data are used. The extracted results for $^4He, ^{12}C, ^{40}Ca$ and $^{56}Fe$
nuclei show that one can get improved results in medium x ranges by less
binding energy.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 11:51:19 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Mar 2008 08:03:34 GMT"
}
] | 2008-03-10T00:00:00 | [
[
"Zolfagharpour",
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""
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] |
802.1624 | Nils Carqueville | Nils Carqueville | Triangle-generation in topological D-brane categories | 34 pages | JHEP0804:031,2008 | 10.1088/1126-6708/2008/04/031 | null | hep-th | null | Tachyon condensation in topological Landau-Ginzburg models can generally be
studied using methods of commutative algebra and properties of triangulated
categories. The efficiency of this approach is demonstrated by explicitly
proving that every D-brane system in all minimal models of type ADE can be
generated from only one or two fundamental branes.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:31:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Carqueville",
"Nils",
""
]
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802.1625 | Dong-han Yeom | Dong-han Yeom, Heeseung Zoe | Constructing a counterexample to the black hole complementarity | 8 pages, 5 figures | Phys.Rev.D78:104008,2008 | 10.1103/PhysRevD.78.104008 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We propose a regular black hole whose inside generates a de Sitter space and
then is finally frustrated into a singularity. It is a modified model which was
suggested originally by Frolov, Markov, and Mukhanov. In our model, we could
adjust a regular black hole so that its period before going into the extreme
state is much longer than the information retention time. During this period an
observer could exist who observes the information of the Hawking radiation,
falls freely into the regular center of the black hole, and finally meets the
free-falling information again. The existence of such an observer implies that
the complementary view may not be consistent with a regular black hole, and
therefore, is not appropriate as a generic principle of black hole physics.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:42:16 GMT"
},
{
"version": "v2",
"created": "Fri, 19 Sep 2008 09:24:59 GMT"
},
{
"version": "v3",
"created": "Mon, 10 Nov 2008 06:19:37 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Yeom",
"Dong-han",
""
],
[
"Zoe",
"Heeseung",
""
]
] | [
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] |
802.1626 | Radu Slobodeanu Al. | Radu Slobodeanu | A special class of holomorphic mappings and the Faddeev-Hopf model | 13 pages. The proof of Proposition 3.4 has been corrected | null | null | null | math.DG math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Pseudo horizontally weakly conformal maps extend both holomorphic and
(semi)conformal maps into an almost Hermitian manifold. We find in this larger
class critical points for the (generalized) Faddeev-Hopf energy. Their
stability is also discussed in some cases.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:35:48 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 21:58:07 GMT"
},
{
"version": "v3",
"created": "Tue, 13 May 2008 21:01:08 GMT"
},
{
"version": "v4",
"created": "Tue, 4 Nov 2008 18:18:04 GMT"
},
{
"version": "v5",
"created": "Thu, 18 Jul 2013 16:12:53 GMT"
}
] | 2013-07-19T00:00:00 | [
[
"Slobodeanu",
"Radu",
""
]
] | [
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] |
802.1627 | Eliecer Hernandez-Gajate | E. Hernandez, J. Nieves, M. Valverde | Neutrino induced weak pion production off the nucleon | 4 latex pages, 2 figures. Contribution at Chiral Symmetry in Hadron
and Nuclear Physics (CHIRAL07), Osaka, November 13-16, 2007 | Mod.Phys.Lett.A23:2317-2320,2008 | 10.1142/S0217732308029289 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study neutrino induced one-pion production off the nucleon in and around
the Delta resonance region. Apart from the Delta-pole mechanism we include
background terms required by chiral symmetry. These background terms give
sizeable contributions in all channels. To better reproduce the ANL
$q^2$-differential cross section data, we make a new fit of the $C_5^A(q^2)$
axial nucleon to Delta form factor. The new result $C_5^A(0)=0.867\pm 0.075$ is
some 30% smaller than the commonly accepted value.
This correction is compatible with most quark model estimates and a recent
lattice calculation
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:20:29 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hernandez",
"E.",
""
],
[
"Nieves",
"J.",
""
],
[
"Valverde",
"M.",
""
]
] | [
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] |
802.1628 | Alexander Knebe | Alexander Knebe (AIP), Bastian Arnold (Vienna), Chris Power
(Leicester), Brad K. Gibson (UCLan) | The Dynamics of Subhalos in Warm Dark Matter Models | 10 pages, 11 figures, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.13102.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a comparison of the properties of substructure halos (subhalos)
orbiting within host halos that form in Cold Dark Matter (CDM) and Warm Dark
Matter (WDM) cosmologies. Our study focuses on selected properties of these
subhalos, namely their anisotropic spatial distribution within the hosts; the
existence of a "backsplash'' population; the age-distance relation; the degree
to which they suffer mass loss; and the distribution of relative (infall)
velocities with respect to the hosts. We find that the number density of
subhalos in our WDM model is suppressed relative to that in the CDM model, as
we would expect. Interestingly, our analysis reveals that backsplash subhalos
exist in both the WDM and CDM models. Indeed, there are no statistically
significant differences between the spatial distributions of subhalos in the
CDM and WDM models. There is evidence that subhalos in the WDM model suffer
enhanced mass loss relative to their counterparts in the CDM model, reflecting
their lower central densities. We note also a tendency for the (infall)
velocities of subhalos in the WDM model to be higher than in the CDM model.
Nevertheless, we conclude that observational tests based on either the spatial
distribution or the kinematics of the subhalo population are unlikely to help
us to differentiate between the CDM model and our adopted WDM model.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:39:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Knebe",
"Alexander",
"",
"AIP"
],
[
"Arnold",
"Bastian",
"",
"Vienna"
],
[
"Power",
"Chris",
"",
"Leicester"
],
[
"Gibson",
"Brad K.",
"",
"UCLan"
]
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802.1629 | Dmitry Knyazev A | D.A. Knyazev, O.E. Omel'yanovskii, V.M. Pudalov, I.S. Burmistrov | Metal-Insulator Transition in 2D: Experimental Test of the Two-Parameter
Scaling | 4 pages, 4 figures, 1 table | Phys. Rev. Lett. 100, 046405 (2008) | 10.1103/PhysRevLett.100.046405 | null | cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report a detailed scaling analysis of resistivity \rho(T,n) measured for
several high-mobility 2D electron systems in the vicinity of the 2D
metal-insulator transition. We analyzed the data using the two parameter
scaling approach and general scaling ideas. This enables us to determine the
critical electron density, two critical indices, and temperature dependence for
the separatrix in the self-consistent manner. In addition, we reconstruct the
empirical scaling function describing a two-parameter surface which fits well
the \rho(T,n) data.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:42:34 GMT"
}
] | 2013-03-08T00:00:00 | [
[
"Knyazev",
"D. A.",
""
],
[
"Omel'yanovskii",
"O. E.",
""
],
[
"Pudalov",
"V. M.",
""
],
[
"Burmistrov",
"I. S.",
""
]
] | [
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] |
802.163 | Ulrich Hohenester | Andreas Truegler and Ulrich Hohenester | Strong coupling between a metallic nanoparticle and a single molecule | 6 pages, 4 figures | Phys. Rev. B 77, 115403 (2008) | 10.1103/PhysRevB.77.115403 | null | cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We theoretically investigate strong coupling between a single molecule and a
single metallic nanoparticle. A theory suited for the quantum-mechanical
description of surface plasmon polaritons (SPPs) is developed. The coupling
between these SPPs and a single molecule, and the modified molecular dynamics
in presence of the nanoparticle are described within a combined Drude and
boundary-element-method approach. Our results show that strong coupling is
possible for single molecules and metallic nanoparticles, and can be observed
in fluorescence spectroscopy through the splitting of emission peaks.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:43:38 GMT"
}
] | 2013-09-10T00:00:00 | [
[
"Truegler",
"Andreas",
""
],
[
"Hohenester",
"Ulrich",
""
]
] | [
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802.1631 | Francois Sausset | Fran\c{c}ois Sausset (LPTMC), Gilles Tarjus (LPTMC) | Comment on "Correlation between Dynamic Heterogeneity and Medium-Range
Order in Two-Dimensional Glass-Forming Liquids" | Comment to appear in PRL along with reply by Kawasaki et al | Physical Review Letters 100 (2008) 099601 | 10.1103/PhysRevLett.100.099601 | null | cond-mat.stat-mech | null | In a recent letter, Kawasaki et al. (PRL 99, 215701 (2007)) study glass
formation in a 2-dimensional (2D) model of polydisperse repulsive disks. They
give numerical evidence for a direct relation between slowing down of the
relaxation, extension of some medium-range order, and development of dynamic
heterogeneities. We disagree with the authors' interpretation on two points
which we believe to be potentially important for understanding the glass
transition.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 12:46:58 GMT"
}
] | 2008-05-13T00:00:00 | [
[
"Sausset",
"François",
"",
"LPTMC"
],
[
"Tarjus",
"Gilles",
"",
"LPTMC"
]
] | [
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802.1632 | Pei-Ming Ho | Tai-Chung Cheng, Pei-Ming Ho, Tze-Kei Lee | Nonlocal Particles as Strings | 25 pages, Latex, minor changes | J.Phys.A42:055202,2009 | 10.1088/1751-8113/42/5/055202 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We find nonlocal particle theories with two dimensional conformal symmetry,
including examples equivalent to the bosonic open string and closed string.
This work provides a new approach to construct solvable consistent backgrounds
in string theory.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:07:44 GMT"
},
{
"version": "v2",
"created": "Sun, 24 Feb 2008 15:31:55 GMT"
},
{
"version": "v3",
"created": "Thu, 23 Oct 2008 04:09:41 GMT"
}
] | 2009-01-08T00:00:00 | [
[
"Cheng",
"Tai-Chung",
""
],
[
"Ho",
"Pei-Ming",
""
],
[
"Lee",
"Tze-Kei",
""
]
] | [
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802.1633 | Andrzej Grudka | Andrzej Grudka, Michal Horodecki, Pawel Horodecki, Ryszard Horodecki | Note on genuine multipartite classical correlations | null | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss the problem of coexistence of genuine quantum multipartite
correlations and classical multipartite correlations. We introduce a postulate
which any measure of genuine multipartite classical correlations should
satisfy. We show that covariance does not satisfy this postulate. Finally we
propose a definition of genuine multipartite correlations and illustrate it
with examples.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:11:16 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Grudka",
"Andrzej",
""
],
[
"Horodecki",
"Michal",
""
],
[
"Horodecki",
"Pawel",
""
],
[
"Horodecki",
"Ryszard",
""
]
] | [
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] |
802.1634 | Mario Novello | M. Novello and S.E.Perez Bergliaffa | Bouncing Cosmologies | Please send comments to [email protected] with copy to
[email protected] | Phys.Rept.463:127-213,2008 | 10.1016/j.physrep.2008.04.006 | null | astro-ph gr-qc hep-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We review the general features of nonsingular universes ({\em i.e.} those
that go from an era of accelerated collapse to an expanding era without
displaying a singularity) as well as cyclic universes. We discuss the
mechanisms behind the bounce, and analyze examples of solutions that implement
these mechanisms. Observational consequences of such regular cosmologies are
also considered, with emphasis in the behavior of the perturbations.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:11:55 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Novello",
"M.",
""
],
[
"Bergliaffa",
"S. E. Perez",
""
]
] | [
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802.1635 | Rodion Burenin | I. M. Khamitov, R. A. Burenin, I. F. Bikmaev, N. A. Sakhibullin, M. N.
Pavlinsky, R. A. Sunyaev, Z. Aslan | Observations of GRB 060526 Optical Afterglow with Russian-Turkish 1.5-m
Telescope | 6 pages, 7 figures, Astronomy Letters, 2007, 33, 797, The on-line
data tables and the original text in Russian can be found at
http://hea.iki.rssi.ru/grb/060526/indexeng.html | Astronomy Letters, 2007, 33, 797 | 10.1134/S106377370712002X | null | astro-ph | null | We present the results of the photometric multicolor observations of GRB
060526 optical afterglow obtained with Russian-Turkish 1.5-m Telescope (RTT150,
Mt. Bakirlitepe, Turkey). The detailed measurements of afterglow light curve,
starting from about 5 hours after the GRB and during 5 consecutive nights were
done. In addition, upper limits on the fast variability of the afterglow during
the first night of observations were obtained and the history of afterglow
color variations was measured in detail. In the time interval from 6 to 16
hours after the burst, there is a gradual flux decay, which can be described
approximately as a power law with an index of -1.14+-0.02. After that the
variability on the time scale \delta t < t is observed and the afterglow
started to decay faster. The color of the afterglow, V-R=~0.5, is approximately
the same during all our observations. The variability is detected on time
scales up to \delta t/t =~ 0.0055 at \Delta F_\nu/F_\nu =~ 0.3, which violates
some constraints on the variability of the observed emission from
ultrarelativistic jet obtained by Ioka et al. (2005). We suggest to explain
this variability by the fact that the motion of the emitting shell is no longer
ultrarelativistic at this time.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:27:26 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Khamitov",
"I. M.",
""
],
[
"Burenin",
"R. A.",
""
],
[
"Bikmaev",
"I. F.",
""
],
[
"Sakhibullin",
"N. A.",
""
],
[
"Pavlinsky",
"M. N.",
""
],
[
"Sunyaev",
"R. A.",
""
],
[
"Aslan",
"Z.",
""
]
] | [
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802.1636 | Rodion Burenin | R. A. Burenin | On the Variability of Gamma-Ray Burst Afterglows - A Possibility of a
Transition to Nonrelativistic Motion | 3 pages, Astronomy Letters, 33, 804, The original text in Russian can
be found at http://hea.iki.rssi.ru/grb/060526/pgrbvar.pdf | Astronomy Letters, 2007, 33, 804 | 10.1134/S1063773707120031 | null | astro-ph | null | Variability on time scales \delta t < t is observed in many gamma-ray burst
afterglows. It is well known that there should be no such variability if the
afterglow is emitted by external shock, which is produced by the interaction of
ultrarelativistic ejecta with the ambient interstellar medium, within the
framework of simple models. The corresponding constraints were established by
Ioka et al. (2005) and in some cases are inconsistent with observations. On the
other hand, if the motion is not relativistic, then the fast variability of the
afterglow can be explained much more easily.
In this connection we discuss various estimates of the time of the transition
to subrelativistic motion in GRB source. We point out, that this transition
should occur on an observed time scale of ~10 days. In the case of a higher
density of the ambient interstellar medium ~10^2-10^4 cm^{-3} or dense stellar
wind with \dot M ~ 10^{-5} - 10^{-4} M_\odot/year the transition to a
subrelativistic motion can occur on a time scale of ~1 day. These densities may
well be expected in star-forming regions and around massive Wolf-Rayet stars.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 14:09:43 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Burenin",
"R. A.",
""
]
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] |
802.1637 | Svante Janson | Svante Janson | Asymptotic equivalence and contiguity of some random graphs | 21 pages | null | null | null | math.PR math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that asymptotic equivalence, in a strong form, holds between two
random graph models with slightly differing edge probabilities under
substantially weaker conditions than what might naively be expected.
One application is a simple proof of a recent result by van den Esker, van
der Hofstad and Hooghiemstra on the equivalence between graph distances for
some random graph models.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:18:37 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Janson",
"Svante",
""
]
] | [
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] |
802.1638 | Oliver Jenkinson | Oscar F. Bandtlow, Oliver Jenkinson | Explicit eigenvalue estimates for transfer operators | 19 pages, to appear in Advances in Mathematics | null | null | null | math.DS math.FA | null | We consider transfer operators acting on spaces of holomorphic functions, and
provide explicit bounds for their eigenvalues. More precisely, if D is any open
set in C^d, and L is a suitable transfer operator acting on Bergman space
A^2(D), its eigenvalue sequence lambda_n(L) is bounded by |lambda_n(L)| \leq
A\exp(-a n^{1/d}), where a, A are explicitly given.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:27:46 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Bandtlow",
"Oscar F.",
""
],
[
"Jenkinson",
"Oliver",
""
]
] | [
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] |
802.1639 | D.-A. Deckert | Angelo Bassi, D.-A. Deckert | Noise gates for decoherent quantum circuits | 10 pages, 4 figures: journal reference added + some typos corrected | Phys. Rev. A 77, 032323 (2008) | 10.1103/PhysRevA.77.032323 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A major problem in exploiting microscopic systems for developing a new
technology based on the principles of Quantum Information is the influence of
noise which tends to work against the quantum features of such systems. It
becomes then crucial to understand how noise affects the evolution of quantum
circuits: several techniques have been proposed among which stochastic
differential equations (SDEs) can represent a very convenient tool. We show how
SDEs naturally map any Markovian noise into a linear operator, which we will
call a noise gate, acting on the wave function describing the state of the
circuit, and we will discuss some examples. We shall see that these gates can
be manipulated like any standard quantum gate, thus simplifying in certain
circumstances the task of computing the overall effect of the noise at each
stage of the protocol. This approach yields equivalent results to those derived
from the Lindblad equation; yet, as we show, it represents a handy and fast
tool for performing computations, and moreover, it allows for fast numerical
simulations and generalizations to non Markovian noise. In detail we review the
depolarizing channel and the generalized amplitude damping channel in terms of
this noise gate formalism and show how these techniques can be applied to any
quantum circuit.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 17:42:21 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Apr 2008 10:43:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bassi",
"Angelo",
""
],
[
"Deckert",
"D. -A.",
""
]
] | [
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802.164 | Aleksey Zinger | R. Pandharipande and A. Zinger | Enumerative Geometry of Calabi-Yau 5-Folds | 40 pages, 3 tables, 6 figures | null | null | null | math.AG math.SG | null | Gromov-Witten theory is used to define an enumerative geometry of curves in
Calabi-Yau 5-folds. We find recursions for meeting numbers of genus 0 curves,
and we determine the contributions of moving multiple covers of genus 0 curves
to the genus 1 Gromov-Witten invariants. The resulting invariants, conjectured
to be integral, are analogous to the previously defined BPS counts for
Calabi-Yau 3 and 4-folds. We comment on the situation in higher dimensions
where new issues arise.
Two main examples are considered: the local Calabi-Yau P^2 with balanced
normal bundle 3O(-1) and the compact Calabi-Yau hypersurface X_7 in P^6. In the
former case, a closed form for our integer invariants has been conjectured by
G. Martin. In the latter case, we recover in low degrees the classical
enumeration of elliptic curves by Ellingsrud and Stromme.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:10:06 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Pandharipande",
"R.",
""
],
[
"Zinger",
"A.",
""
]
] | [
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802.1641 | Martha Haynes P | Martha P. Haynes | ALFALFA: The Search for (Almost) Dark Galaxies and their Space
Distribution | To appear in Il Nuovo Cimento, Proceedings of the Venice conference,
"A Century of Cosmology: Past, Present and Future", August 27-31, 2007, 6
pages including 1 figure | null | null | MH-V07 | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Arecibo Legacy Fast ALFA (ALFALFA) survey is designed to explore the z=0
HI mass function (HIMF) over a cosmologically significant volume. ALFALFA will
improve on previous determinations of the HIMF by its combination of depth,
wide area and centroiding accuracy, the latter allowing, in most cases,
immediate identification of the optical counterpart to each HI signal. ALFALFA
will detect hundreds of galaxies with HI masses less than 10**7.5 solar masses
and also greater than 10**10.5 solar masses, and its final catalog will allow
investigation of the dependence of the HIMF both on local density and on galaxy
morphology. Already ALFALFA confirms previous suggestions that there is no
cosmologically significant population of HI-rich dark galaxies. Fewer than 3%
of all extragalactic HI sources and < 1% of ones with HI masses > 10**9.5 solar
masses cannot be identified with a stellar counterpart. Very preliminary
results on the presence of gas-rich dwarfs in the void in front of the
Pisces-Perseus supercluster suggest an underabundance of such objects compared
to the predictions of numerical simulations. The objects with highest HI mass
exhibit a range of morphologies and optical colors and surface brightnesses but
all appear to be massive disk systems. The latter represent the population
likely to dominate future studies of HI at higher redshift with the Square
Kilometer Array.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:33:52 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Haynes",
"Martha P.",
""
]
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802.1642 | Bruno Chilian | Bruno Chilian, Klaus Fredenhagen | The time slice axiom in perturbative quantum field theory on globally
hyperbolic spacetimes | 14 pages, 1 figure, added reference for introduction, corrected
typos, corrected a mistake in the proof in section 3 | Commun.Math.Phys.287:513-522,2009 | 10.1007/s00220-008-0670-7 | null | math-ph math.MP | null | The time slice axiom states that the observables which can be measured within
an arbitrarily small time interval suffice to predict all other observables.
While well known for free field theories where the validity of the time slice
axiom is an immediate consequence of the field equation it was not known
whether it also holds in generic interacting theories, the only exception being
certain superrenormalizable models in 2 dimensions. In this paper we prove that
the time slice axiom holds at least for scalar field theories within formal
renormalized perturbation theory.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:51:48 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 12:46:10 GMT"
},
{
"version": "v3",
"created": "Mon, 31 Mar 2008 17:18:53 GMT"
}
] | 2009-03-20T00:00:00 | [
[
"Chilian",
"Bruno",
""
],
[
"Fredenhagen",
"Klaus",
""
]
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802.1643 | Yves Colin de Verdiere | Yves Colin de Verdi\`ere (IF) | A semi-classical inverse problem II: reconstruction of the potential | 21 pages 5 Figures | null | null | null | math-ph math.AP math.MP math.SP | null | This paper is the continuation of our work with Victor Guillemin; Victor and
I proved that the Taylor expansion of the potential at a generic non degenerate
critical point is determined by the semi-classical spectrum of the associated
Schr\"odinger operator near the corresponding critical value. Here, I show
that, under some genericity assumptions, the potential of the 1D Schroedinger
operator is determined by its semi-classical spectrum. Moreover, there is an
explicit reconstruction. This paper is strongly related to a paper of David
Gurarie (J. Math. Phys. 36:1934--1944 (1995)).
| [
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802.1644 | Narges Abbasi | Narges Abbasi | On Limiting Distributions Of Estimation Of Central Moments | This paper has been withdrawn | null | null | IMS-EJS-EJS_2008_184 | math.ST stat.TH | null | This paper has been withdrawn at the author's request.
| [
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},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 12:51:11 GMT"
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802.1645 | Bruno Angles | Bruno Angles (LMNO), Filippo A. E. Nuccio (LMNO) | On Jacobi Sums in $\mathbb Q(\zeta_p)$ | null | null | null | null | math.NT | null | We study the p-adic behavior of Jacobi Sums for $\mathbb Q(\zeta_p)$ and link
this study to the p-Sylow subgroup of the ideal class group of $\mathbb
Q(\zeta_p\`a^+$
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 13:53:16 GMT"
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] | 2020-04-10T00:00:00 | [
[
"Angles",
"Bruno",
"",
"LMNO"
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[
"Nuccio",
"Filippo A. E.",
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] |
802.1646 | Charalampos Skokos | Charalampos Skokos, Tassos Bountis and Chris Antonopoulos | Detecting chaos, determining the dimensions of tori and predicting slow
diffusion in Fermi--Pasta--Ulam lattices by the Generalized Alignment Index
method | 10 pages, 5 figures, submitted for publication in European Physical
Journal - Special Topics. Revised version: Small explanatory additions to the
text and addition of some references. A small figure change | null | 10.1140/epjst/e2008-00844-2 | null | nlin.CD | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The recently introduced GALI method is used for rapidly detecting chaos,
determining the dimensionality of regular motion and predicting slow diffusion
in multi--dimensional Hamiltonian systems. We propose an efficient computation
of the GALI$_k$ indices, which represent volume elements of $k$ randomly chosen
deviation vectors from a given orbit, based on the Singular Value Decomposition
(SVD) algorithm. We obtain theoretically and verify numerically asymptotic
estimates of GALIs long--time behavior in the case of regular orbits lying on
low--dimensional tori. The GALI$_k$ indices are applied to rapidly detect
chaotic oscillations, identify low--dimensional tori of Fermi--Pasta--Ulam
(FPU) lattices at low energies and predict weak diffusion away from
quasiperiodic motion, long before it is actually observed in the oscillations.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 14:15:49 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 20:57:41 GMT"
},
{
"version": "v3",
"created": "Mon, 10 Mar 2008 17:04:29 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Skokos",
"Charalampos",
""
],
[
"Bountis",
"Tassos",
""
],
[
"Antonopoulos",
"Chris",
""
]
] | [
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] |
802.1647 | Mauricio D. Garay | Mauricio D. Garay and Duco van Straten | Classical and quantum integrability | null | null | null | null | math-ph math.MP | null | We give a sufficient condition for quantising integrable systems.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:06:56 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Garay",
"Mauricio D.",
""
],
[
"van Straten",
"Duco",
""
]
] | [
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] |
802.1648 | Dung Di Caprio | M. Holovko, D. di Caprio | On the contact conditions for the charge profile in the theory of the
electrical double layer for nonsymmetrical electrolytes | 5 pages | null | 10.1063/1.2909973 | null | cond-mat.stat-mech cond-mat.soft | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The contact value of the charge profile for nonsymmetrical electrolytes is
presented as the sum of three contributions. One of them is the normal
component of the Maxwell electrostatic stress tensor. The second one is the
surface electrostatic property defined as the integral of the product of the
gradient of the electrical potential and the density distribution function of
coions. The third term is the bulk contribution defined by the sum for anions
and for cations of the product of their charge and their partial pressure. For
noncharged surfaces only the last two are present and have the same sign in the
case of size asymmetry. In the case of charge asymmetry the contact value of
the charge profile is the result of the competitions of bulk and surface terms
in which the bulk term is dominant. Using both the contact theorems for the
density and the charge profiles, the exact expressions for the contact values
of the profiles of coions and counterions are obtained and some related
properties are discussed.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 14:35:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Holovko",
"M.",
""
],
[
"di Caprio",
"D.",
""
]
] | [
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] |
802.1649 | Yuji Shirasaki | Yuji Shirasaki, Atsumasa Yoshida, Nobuyuki Kawai, Toru Tamagawa,
Takanori Sakamoto, Motoko Suzuki, Yujin Nakagawam, Akina Kobayashi, Satoshi
Sugita, Ichiro Takahashi, Makoto Arimoto, Takashi Shimokawabe, Nicolas
Vasquez Pazmino, Takuto Ishimura, Rie Sato, Masaru Matsuoka, Edward E.
Fenimore, Mark Galassi, Donald Q. Lamb, Carlo Graziani, Timothy Q. Donaghy,
Jean-Luc Atteia, Alexandre Pelangeon, Roland Vanderspek, Geoffrey B. Crew,
John P. Doty, Joel Villasenor, Gregory Prigozhin, Nat Butler, George R.
Ricker, Kevin Hurley, Stanford E. Woosley, and Graziella Pizzichini | Multiple Component Analysis of Time Resolved Spectra of GRB041006: A
Clue to the Nature of Underlying Soft Component of GRBs | 19 pages, 10 figures, accepted for publication in PASJ, replaced with
the accepted version (minor correction) | Publ.Astron.Soc.Jap.60:919,2008 | 10.1093/pasj/60.4.919 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. This GRB
displays a soft X-ray emission, a precursor before the onset of the main event,
and also a soft X-ray tail after the end of the main peak. The light curves in
four different energy bands display different features; At higher energy bands
several peaks are seen in the light curve, while at lower energy bands a single
broader bump dominates. It is expected that these different features are the
result of a mixture of several components each of which has different
energetics and variability. To reveal the nature of each component, we analysed
the time resolved spectra and they are successfully resolved into several
components. We also found that these components can be classified into two
distinct classes; One is a component which has an exponential decay of $E_{p}$
with a characteristic timescale shorter than $\sim$ 30 sec, and its spectrum is
well represented by a broken power law function, which is frequently observed
in many prompt GRB emissions, so it should have an internal-shock origin.
Another is a component whose $E_{p}$ is almost unchanged with characteristic
timescale longer than $\sim$ 60 sec, and shows a very soft emission and slower
variability. The spectrum of the soft component is characterized by either a
broken power law or a black body spectrum. This component might originate from
a relatively wider and lower velocity jet or a photosphere of the fireball. By
assuming that the soft component is a thermal emission, the radiation radius is
initially $4.4 \times 10^{6}$ km, which is a typical radius of a blue
supergiant, and its expansion velocity is $2.4 \times 10^{5}$ km/s in the
source frame.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 14:39:01 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Apr 2008 15:18:53 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Shirasaki",
"Yuji",
""
],
[
"Yoshida",
"Atsumasa",
""
],
[
"Kawai",
"Nobuyuki",
""
],
[
"Tamagawa",
"Toru",
""
],
[
"Sakamoto",
"Takanori",
""
],
[
"Suzuki",
"Motoko",
""
],
[
"Nakagawam",
"Yujin",
""
],
[
"Kobayashi",
"Akina",
""
],
[
"Sugita",
"Satoshi",
""
],
[
"Takahashi",
"Ichiro",
""
],
[
"Arimoto",
"Makoto",
""
],
[
"Shimokawabe",
"Takashi",
""
],
[
"Pazmino",
"Nicolas Vasquez",
""
],
[
"Ishimura",
"Takuto",
""
],
[
"Sato",
"Rie",
""
],
[
"Matsuoka",
"Masaru",
""
],
[
"Fenimore",
"Edward E.",
""
],
[
"Galassi",
"Mark",
""
],
[
"Lamb",
"Donald Q.",
""
],
[
"Graziani",
"Carlo",
""
],
[
"Donaghy",
"Timothy Q.",
""
],
[
"Atteia",
"Jean-Luc",
""
],
[
"Pelangeon",
"Alexandre",
""
],
[
"Vanderspek",
"Roland",
""
],
[
"Crew",
"Geoffrey B.",
""
],
[
"Doty",
"John P.",
""
],
[
"Villasenor",
"Joel",
""
],
[
"Prigozhin",
"Gregory",
""
],
[
"Butler",
"Nat",
""
],
[
"Ricker",
"George R.",
""
],
[
"Hurley",
"Kevin",
""
],
[
"Woosley",
"Stanford E.",
""
],
[
"Pizzichini",
"Graziella",
""
]
] | [
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] |
802.165 | Roberto Aloisio | R. Aloisio, D. Boncioli, A. F. Grillo, C. Macolino, S. Petrera, P.
Privitera, V. Rizi and F. Salamida | Detection of GRB signals with Fluorescence Detectors | 16 pages 9 eps figures | Astropart.Phys.29:373-379,2008 | 10.1016/j.astropartphys.2008.04.002 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Gamma Ray Bursts are being searched in many ground based experiments
detecting the high energy component (GeV $\div$ TeV energy range) of the photon
bursts. In this paper, Fluorescence Detectors are considered as possible
candidate devices for these searches. It is shown that the GRB photons induce
fluorescence emission of UV photons on a wide range of their spectrum. The
induced fluorescence flux is dominated by GRB photons from 0.1 to about 100 MeV
and, once the extinction through the atmosphere is taken into account, it is
distributed over a wide angular region. This flux can be detected through a
monitor of the diffuse photon flux, provided that its maximum value exceeds a
threshold value, that is primarily determined by the sky brightness above the
detector. The feasibility of this search and the expected rates are discussed
on the basis of the current GRB observations and the existing fluorescence
detectors.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:03:16 GMT"
}
] | 2013-06-11T00:00:00 | [
[
"Aloisio",
"R.",
""
],
[
"Boncioli",
"D.",
""
],
[
"Grillo",
"A. F.",
""
],
[
"Macolino",
"C.",
""
],
[
"Petrera",
"S.",
""
],
[
"Privitera",
"P.",
""
],
[
"Rizi",
"V.",
""
],
[
"Salamida",
"F.",
""
]
] | [
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] |
802.1651 | Roman Travkin | Roman Travkin | Mirabolic Robinson-Schensted-Knuth correspondence | 28 pages. The list of conditions for the formulas for the action of
generators on the mirabolic bimodule over the Hecke algebra corrected; the
mirabolic RSK example modified; other minor changes. Document style reverted
to amsart | Selecta Math. (N.S.) 14 (2009), no. 3-4, 727-758 | null | null | math.AG math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The set of orbits of $GL(V)$ in $Fl(V)\times Fl(V)\times V$ is finite, and is
parametrized by the set of certain decorated permutations in a work of Solomon.
We describe a Mirabolic RSK correspondence (bijective) between this set of
decorated permutations and the set of triples: a pair of standard Young
tableaux, and an extra partition. It gives rise to a partition of the set of
orbits into combinatorial cells. We prove that the same partition is given by
the type of a general conormal vector to an orbit. We conjecture that the same
partition is given by the bimodule Kazhdan-Lusztig cells in the bimodule over
the Iwahori-Hecke algebra of $GL(V)$ arising from $Fl(V)\times Fl(V)\times V$.
We also give conjectural applications to the classification of unipotent
mirabolic character sheaves on $GL(V)\times V$.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:51:19 GMT"
},
{
"version": "v2",
"created": "Sun, 1 Feb 2009 15:21:31 GMT"
},
{
"version": "v3",
"created": "Sun, 27 Mar 2011 04:40:30 GMT"
},
{
"version": "v4",
"created": "Sat, 6 Nov 2021 18:41:54 GMT"
}
] | 2021-11-09T00:00:00 | [
[
"Travkin",
"Roman",
""
]
] | [
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802.1652 | Michael Finkelberg | Michael Finkelberg, Victor Ginzburg, Roman Travkin | Mirabolic affine Grassmannian and character sheaves | 22 pages. The final version to appear in Selecta Math | null | null | null | math.AG math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We compute the Frobenius trace functions of mirabolic character sheaves
defined over a finite field. The answer is given in terms of the character
values of general linear groups over the finite field, and the structure
constants of multiplication in the mirabolic Hall-Littlewood basis of symmetric
functions, introduced by Shoji.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:40:11 GMT"
},
{
"version": "v2",
"created": "Sun, 1 Feb 2009 15:17:30 GMT"
}
] | 2009-02-01T00:00:00 | [
[
"Finkelberg",
"Michael",
""
],
[
"Ginzburg",
"Victor",
""
],
[
"Travkin",
"Roman",
""
]
] | [
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] |
802.1653 | Panayotis Kevrekidis | D.E. Pelinovsky and P.G. Kevrekidis | Stability of discrete dark solitons in nonlinear Schrodinger lattices | 11 pages, 5 figures | null | null | null | nlin.PS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We obtain new results on the stability of discrete dark solitons bifurcating
from the anti-continuum limit of the discrete nonlinear Schrodinger equation,
following the analysis of our previous paper [Physica D 212, 1-19 (2005)]. We
derive a criterion for stability or instability of dark solitons from the
limiting configuration of the discrete dark soliton and confirm this criterion
numerically. We also develop detailed calculations of the relevant eigenvalues
for a number of prototypical configurations and obtain very good agreement of
asymptotic predictions with the numerical data.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:32:45 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Pelinovsky",
"D. E.",
""
],
[
"Kevrekidis",
"P. G.",
""
]
] | [
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] |
802.1654 | B. Svaiter F. | Regina Sandra Burachik, B. F. Svaiter | Maximal monotonicity, conjugation and the duality product | 8 pages, corrected author's names | Proceedings of the American Mathematical . Society 131 (2003),
2379-2383 | 10.1090/S0002-9939-03-07053-9 | null | math.FA math.AP | null | Recently, the authors studied the connection between each maximal monotone
operator T and a family H(T) of convex functions. Each member of this family
characterizes the operator and satisfies two particular inequalities.
The aim of this paper is to establish the converse of the latter fact.
Namely, that every convex function satisfying those two particular inequalities
is associated to a unique maximal monotone operator.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:36:37 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 11:51:06 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Burachik",
"Regina Sandra",
""
],
[
"Svaiter",
"B. F.",
""
]
] | [
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] |
802.1655 | Marko Vojinovic | Milovan Vasilic and Marko Vojinovic | Single-Pole Interaction of the Particle with the String | This is a contribution to the Proc. of the Seventh International
Conference ''Symmetry in Nonlinear Mathematical Physics'' (June 24-30, 2007,
Kyiv, Ukraine), published in SIGMA (Symmetry, Integrability and Geometry:
Methods and Applications) at http://www.emis.de/journals/SIGMA/ | SIGMA 4:019,2008 | 10.3842/SIGMA.2008.019 | null | gr-qc | http://creativecommons.org/licenses/by-nc-sa/3.0/ | Within the framework of generalized Papapetrou method, we derive the
effective equations of motion for a string with two particles attached to its
ends, along with appropriate boundary conditions. The equations of motion are
the usual Nambu-Goto-like equations, while boundary conditions turn out to be
equations of motion for the particles at the string ends. Various properties of
those equations are discussed, and a simple example is treated in detail,
exhibiting the properties of Neumann and Dirichlet boundary conditions and
giving a small correction term to the law of Regge trajectories due to the
nonzero particle mass.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:38:27 GMT"
}
] | 2008-12-19T00:00:00 | [
[
"Vasilic",
"Milovan",
""
],
[
"Vojinovic",
"Marko",
""
]
] | [
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] |
802.1656 | St\'ephane Munier | S. Munier, F. Schwennsen (Ecole Polytechnique, CPHT) | Resummation of projectile-target multiple scatterings and parton
saturation | 14 pages, 16 figures | Phys.Rev.D78:034029,2008 | 10.1103/PhysRevD.78.034029 | CPHT-RR-004-0208 | hep-ph | null | In the framework of a toy model which possesses the main features of QCD in
the high energy limit, we conduct a numerical study of scattering amplitudes
constructed from parton splittings and projectile-target multiple interactions,
in a way that unitarizes the amplitudes without however explicit saturation in
the wavefunction of the incoming states. This calculation is performed in two
different ways. One of these formulations, the closest to field theory,
involves the numerical resummation of a factorially divergent series, for which
we develop appropriate numerical tools. We accurately compare the properties of
the resulting amplitudes with what would be expected if saturation were
explicitly included in the evolution of the states. We observe that the
amplitudes have similar properties in a small but finite range of rapidity in
the beginning of the evolution, as expected. Some of the features of
reaction-diffusion processes are already present in that range, even when
saturation is left out of the model.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:44:27 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Munier",
"S.",
"",
"Ecole Polytechnique, CPHT"
],
[
"Schwennsen",
"F.",
"",
"Ecole Polytechnique, CPHT"
]
] | [
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] |
802.1657 | Natalya A. Zimbovskaya | Natalya A. Zimbovskaya and Godfrey Gumbs | On the low frequency electromagnetic waves in quasi-two-dimensional
metals | 4 pages, 2 figures, accepted in Solid State Comm | Solid State Comm. 146, 88 (2008). | 10.1016/j.ssc.2008.01.007 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Here, we theoretically analyze spectra of weakly attenuated electromagnetic
waves which may appear in a Fermi-liquid of charge carriers in
quasi-two-dimensional (Q2D) layered conductors when an external magnetic field
is applied perpendicularly to the conducting layers. We study transverse modes
propagating along the magnetic field. The frequencies of the modes are assumed
to be lower than the cyclotron frequency of the charge carriers. It is shown
that Fermi-liquid interaction of the charge carriers in Q2D conductors gives
rise to a mode which cannot appear in a gase of charged quasiparticles, as well
as it happens in conventional metals. Also, we show that the Fermi surface
plofile may cause significant changes in the waves spectra and we analyze these
changes.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:51:10 GMT"
}
] | 2008-10-23T00:00:00 | [
[
"Zimbovskaya",
"Natalya A.",
""
],
[
"Gumbs",
"Godfrey",
""
]
] | [
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] |
802.1658 | Subir Mukhopadhyay | Subir Mukhopadhyay and Koushik Ray | Branes in hearts with perverse sheaves | 21 pages, LaTeX, references added, cosmetic changes | IndianJ.Phys.A80:1109-1122,2006 | null | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Various topological properties of D-branes in the type--IIA theory are
captured by the topologically twisted B-model, treating D-branes as objects in
the bounded derived category of coherent sheaves on the compact part of the
target space. The set of basic D-branes wrapped on the homology cycles of the
compact space are taken to reside in the heart of t-structures of the derived
category of coherent sheaves on the space at any point in the K\"ahler moduli
space. The stability data entails specifying a t-structure along with a grade
for sorting the branes. Considering an example of a degenerate Calabi-Yau
space, obtained via geometric engineering, that retains but a projective curve
as the sole non-compact part, we identify the regions in the K\"ahler moduli
space of the curve that pertain to the different t-structures of the bounded
derived category of coherent sheaves on the curve corresponding to the
different phases of the topological branes.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:58:48 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 09:17:59 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mukhopadhyay",
"Subir",
""
],
[
"Ray",
"Koushik",
""
]
] | [
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802.1659 | Boris Pioline | Micha Berkooz (Weizmann) and Boris Pioline (LPTHE and LPTENS) | 5D Black Holes and Non-linear Sigma Models | 36 pages, 2 figures, uses JHEP3.cls; v3: change of convention in
quaternionic vielbein, misprints corrected | JHEP0805:045,2008 | 10.1088/1126-6708/2008/05/045 | LPTENS-08-11,WIS/05/08-FEB-DPP | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Stationary solutions of 5D supergravity with U(1) isometry can be efficiently
studied by dimensional reduction to three dimensions, where they reduce to
solutions to a locally supersymmetric non-linear sigma model. We generalize
this procedure to 5D gauged supergravity, and identify the corresponding
gauging in 3D. We pay particular attention to the case where the Killing spinor
is non constant along the fibration, which results, even for ungauged
supergravity in 5D, in an additional gauging in 3D, without introducing any
extra potential. We further study SU(2)\times U(1) symmetric solutions, which
correspond to geodesic motion on the sigma model (with potential in the gauged
case). We identify and study the algebra of BPS constraints relevant for the
Breckenridge-Myers-Peet-Vafa black hole, the Gutowski-Reall black hole and
several other BPS solutions, and obtain the corresponding radial wave functions
in the semi-classical approximation.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:01:55 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Mar 2008 17:06:16 GMT"
},
{
"version": "v3",
"created": "Thu, 19 Feb 2009 13:29:57 GMT"
}
] | 2009-02-19T00:00:00 | [
[
"Berkooz",
"Micha",
"",
"Weizmann"
],
[
"Pioline",
"Boris",
"",
"LPTHE and LPTENS"
]
] | [
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] |
802.166 | James Lindesay | Beth A. Brown, James Lindesay | Radial Photon Trajectories Near an Evaporating Black Hole | 4 figures | null | null | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The radial motion of photons emitted near the horizon of a black hole that
evaporates at a steady rate is examined. The space-time of the black hole is
generated using non-orthogonal coordinates. It is shown that some photons that
are initially drawn towards the singularity can escape falling into the
horizon. The behaviors of various outgoing and ingoing photons are clearly
demonstrated through the use of a Penrose diagram.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:10:05 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Brown",
"Beth A.",
""
],
[
"Lindesay",
"James",
""
]
] | [
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] |
802.1661 | Marie-Annick Guillemer | Dima Grigoriev (IRMAR), Vladimir Shpilrain | Zero-knowledge authentication schemes from actions on graphs, groups, or
rings | null | null | null | 08-09 | cs.CR | null | We propose a general way of constructing zero-knowledge authentication
schemes from actions of a semigroup on a set, without exploiting any specific
algebraic properties of the set acted upon. Then we give several concrete
realizations of this general idea, and in particular, we describe several
zero-knowledge authentication schemes where forgery (a.k.a. impersonation) is
NP-hard. Computationally hard problems that can be employed in these
realizations include (Sub)graph Isomorphism, Graph Colorability, Diophantine
Problem, and many others.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:10:40 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Grigoriev",
"Dima",
"",
"IRMAR"
],
[
"Shpilrain",
"Vladimir",
""
]
] | [
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] |
802.1662 | Matthew Hummon | Matthew T. Hummon, Wesley C. Campbell, Hsin-I Lu, Edem Tsikata, Yihua
Wang, John M. Doyle | Magnetic trapping of atomic nitrogen (14^N) and cotrapping of NH
(X-triplet-Sigma-) | null | null | 10.1103/PhysRevA.78.050702 | null | physics.atom-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We observe magnetic trapping of atomic nitrogen (14^N) and cotrapping of
ground state imidogen (14^NH, X-triplet-Sigma-). Both are loaded directly from
a room temperature beam via buffer gas cooling. We trap approximately 1 * 10^11
14^N atoms at a peak density of 5 * 10^11 cm^-3 at 550 mK. The 12 +5/-3 s 1/e
lifetime of atomic nitrogen in the trap is limited by elastic collisions with
the helium buffer gas. Cotrapping of 14^N and 14^NH is accomplished, with 10^8
NH trapped molecules at a peak density of 10^8 cm^-3. We observe no spin
relaxation of nitrogen in collisions with helium.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:25:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hummon",
"Matthew T.",
""
],
[
"Campbell",
"Wesley C.",
""
],
[
"Lu",
"Hsin-I",
""
],
[
"Tsikata",
"Edem",
""
],
[
"Wang",
"Yihua",
""
],
[
"Doyle",
"John M.",
""
]
] | [
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] |
802.1663 | Natalia Babkovskaia | N. Babkovskaia, A. Brandenburg and J. Poutanen | Boundary layer on the surface of a neutron star | 7 pages, 7 figures | null | 10.1111/j.1365-2966.2008.13099.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In an attempt to model the accretion onto a neutron star in low-mass X-ray
binaries, we present two-dimensional hydrodynamical models of the gas flow in
close vicinity of the stellar surface. First we consider a gas pressure
dominated case, assuming that the star is non-rotating. For the stellar mass we
take $M_{\rm star}=1.4 \times 10^{-2} \msun$ and for the gas temperature $T=5
\times 10^6$ K. Our results are qualitatively different in the case of a
realistic neutron star mass and a realistic gas temperature of $T\simeq 10^8$
K, when the radiation pressure dominates. We show that to get the stationary
solution in a latter case, the star most probably has to rotate with the
considerable velocity.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:27:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Babkovskaia",
"N.",
""
],
[
"Brandenburg",
"A.",
""
],
[
"Poutanen",
"J.",
""
]
] | [
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] |
802.1664 | Denis I. Golosov | D. I. Golosov, N. Ossi, A. Frydman, I. Felner, I. Nowik, M. I.
Tsindlekht, and Y. M. Mukovskii | Two-Fluid Behaviour at the Origin of the Resistivity Peak in Doped
Manganites | 6 pages, including 3 figures; revised version; Europhys. Lett.
(http://epljournal.edpsciences.org/), in press | Europhys. Lett. vol. 84, 47006 (2008). | 10.1209/0295-5075/84/47006 | null | cond-mat.str-el cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report a series of magnetic and transport measurements on high-quality
single crystal samples of colossal magnetoresistive manganites, La_{0.7}
Ca_{0.3} Mn O_3 and Pr_{0.7} Sr_{0.3} Mn O_3. 1 % Fe doping allows a Moessbauer
spectroscopy study, which shows (i) unusual line broadening within the
ferromagnetic phase and (ii) a coexistence of ferro- and paramagnetic
contributions in a region, T_1<T<T_2, around the Curie point T_C. In the case
of Pr_{0.7} Sr_{0.3} Mn O_3, the resistivity peak occurs at a considerably
higher temperature, T_{MI}>T_2. This shows that phase separation into metallic
(ferromagnetic) and insulating (paramagnetic) phases cannot be generally
responsible for the resistivity peak (and hence for the associated colossal
magnetoresistance). Our results can be understood phenomenologically within the
two-fluid approach, which also allows for a difference between T_C and T_{MI}.
Our data indeed imply that while magnetic and transport properties of the
manganites are closely interrelated, the two transitions at T_C and T_{MI} can
be viewed as distinct phenomena.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 20:28:56 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 15:56:57 GMT"
},
{
"version": "v3",
"created": "Tue, 4 Nov 2008 12:18:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Golosov",
"D. I.",
""
],
[
"Ossi",
"N.",
""
],
[
"Frydman",
"A.",
""
],
[
"Felner",
"I.",
""
],
[
"Nowik",
"I.",
""
],
[
"Tsindlekht",
"M. I.",
""
],
[
"Mukovskii",
"Y. M.",
""
]
] | [
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] |
802.1665 | Fritz Gesztesy | Fritz Gesztesy, Yuri Latushkin, and Kevin Zumbrun | Derivatives of (Modified) Fredholm Determinants and Stability of
Standing and Traveling Waves | 47 pp, updated Theorem 2.3 | J. Math. Pures Appl. 90, 160-200 (2008) | null | null | math.AP math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Continuing a line of investigation initiated in [11] exploring the
connections between Jost and Evans functions and (modified) Fredholm
determinants of Birman-Schwinger type integral operators, we here examine the
stability index, or sign of the first nonvanishing derivative at frequency zero
of the characteristic determinant, an object that has found considerable use in
the study by Evans function techniques of stability of standing and traveling
wave solutions of partial differential equations (PDE) in one dimension. This
leads us to the derivation of general perturbation expansions for
analytically-varying modified Fredholm determinants of abstract operators. Our
main conclusion, similarly in the analysis of the determinant itself, is that
the derivative of the characteristic Fredholm determinant may be efficiently
computed from first principles for integral operators with semi-separable
integral kernels, which include in particular the general one-dimensional case,
and for sums thereof, which latter possibility appears to offer applications in
the multi-dimensional case.
A second main result is to show that the multi-dimensional characteristic
Fredholm determinant is the renormalized limit of a sequence of Evans functions
defined in [23] on successive Galerkin subspaces, giving a natural extension of
the one-dimensional results of [11] and answering a question of [27] whether
this sequence might possibly converge (in general, no, but with
renormalization, yes). Convergence is useful in practice for numerical error
control and acceleration.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:31:08 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Nov 2016 06:53:56 GMT"
}
] | 2016-12-01T00:00:00 | [
[
"Gesztesy",
"Fritz",
""
],
[
"Latushkin",
"Yuri",
""
],
[
"Zumbrun",
"Kevin",
""
]
] | [
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] |
802.1666 | Charles Dudley | C. C. Dudley, M. Imanishi and P. R. Maloney | Ice emission and the redshifts of submillimeter sources | 37 pages, 8 figures, accepted for publication in the Astrophysical
Journal | null | 10.1086/587445 | null | astro-ph | http://creativecommons.org/licenses/publicdomain/ | Observations at submillimeter wavelengths have revealed a population of
sources thought to be at relatively large redshifts. The position of the 850
$\mu$m passband on the Rayleigh-Jeans portion of the Planck function leads to a
maximum redshift estimate of $z\sim$4.5 since sources will not retain their
redshift independent brightness close to the peak of the Planck function and
thus drop out of surveys. Here we review evidence that ice absorption is
present in the spectra of local ultraluminous infrared galaxies which are often
taken as analogs for the 850 $\mu$m source population. We consider the
implication of this absorption for ice induced spectral structure at far
infrared wavelengths and present marginal astronomical evidence that amorphous
ice may have a feature similar to crystalline ice near 150 $\mu$m. Recent
corroborative laboratory evidence is supportive of this conclusion. It is
argued that early metal enrichment by pair instability SN may lead to a high
ice content relative to refractory dust at high redshift and a fairly robust
detection of ice emission in a $z=6.42$ quasar is presented. It is further
shown that ice emission is needed to understand the 450 $\mu$m sources observed
in the GOODS-N field. We are thus encouraged to apply far infrared ice emission
models to the available observations of HDF 850.1, the brightest submillimeter
source in the {\it Hubble Deep Field}. We suggest that a redshift as large as
13 may need to be considered for this source, nearly a factor of three above
the usual top estimate. Inclusion of the possibility of far infrared ice
emission in the spectral energy distributions of model sources generally
broadens the range of redshifts to be considered for submillimeter sources
compared to models without ice emission.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:34:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dudley",
"C. C.",
""
],
[
"Imanishi",
"M.",
""
],
[
"Maloney",
"P. R.",
""
]
] | [
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] |
802.1667 | Irene Giardina Dr | Michele Ballerini, Nicola Cabibbo, Raphael Candelier, Andrea Cavagna,
Evaristo Cisbani, Irene Giardina, Alberto Orlandi, Giorgio Parisi, Andrea
Procaccini, Massimiliano Viale, Vladimir Zdravkovic | An empirical study of large, naturally occurring starling flocks: a
benchmark in collective animal behaviour | To be published in Animal Behaviour | null | null | null | q-bio.QM cond-mat.stat-mech q-bio.PE | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Bird flocking is a striking example of collective animal behaviour. A vivid
illustration of this phenomenon is provided by the aerial display of vast
flocks of starlings gathering at dusk over the roost and swirling with
extraordinary spatial coherence. Both the evolutionary justification and the
mechanistic laws of flocking are poorly understood, arguably because of a lack
of data on large flocks. Here, we report a quantitative study of aerial
display. We measured the individual three-dimensional positions in compact
flocks of up to 2700 birds. We investigated the main features of the flock as a
whole - shape, movement, density and structure - and discuss these as emergent
attributes of the grouping phenomenon. We find that flocks are relatively thin,
with variable sizes, but constant proportions. They tend to slide parallel to
the ground and, during turns, their orientation changes with respect to the
direction of motion. Individual birds keep a minimum distance from each other
that is comparable to their wingspan. The density within the aggregations is
non-homogeneous, as birds are packed more tightly at the border compared to the
centre of the flock. These results constitute the first set of large-scale data
on three-dimensional animal aggregations. Current models and theories of
collective animal behaviour can now be tested against these results.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:13:14 GMT"
}
] | 2008-02-19T00:00:00 | [
[
"Ballerini",
"Michele",
""
],
[
"Cabibbo",
"Nicola",
""
],
[
"Candelier",
"Raphael",
""
],
[
"Cavagna",
"Andrea",
""
],
[
"Cisbani",
"Evaristo",
""
],
[
"Giardina",
"Irene",
""
],
[
"Orlandi",
"Alberto",
""
],
[
"Parisi",
"Giorgio",
""
],
[
"Procaccini",
"Andrea",
""
],
[
"Viale",
"Massimiliano",
""
],
[
"Zdravkovic",
"Vladimir",
""
]
] | [
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] |
802.1668 | Andrea Cavagna | Andrea Cavagna, Irene Giardina, Alberto Orlandi, Giorgio Parisi,
Andrea Procaccini, Massimiliano Viale, Vladimir Zdravkovic | The STARFLAG handbook on collective animal behaviour: Part I, empirical
methods | To be published in Animal Behaviour | Animal Behaviour 76 (1), 217-236 (2008) | null | null | q-bio.QM cond-mat.stat-mech q-bio.PE | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The most startling examples of collective animal behaviour are provided by
very large and cohesive groups moving in three dimensions. Paradigmatic
examples are bird flocks, fish schools and insect swarms. However, because of
the sheer technical difficulty of obtaining 3D data, empirical studies
conducted to date have only considered loose groups of a few tens of animals.
Moreover, these studies were very seldom conducted in the field. Recently the
STARFLAG project achieved the 3D reconstruction of thousands of birds under
field conditions, thus opening the way to a new generation of quantitative
studies of collective animal behaviour. Here, we review the main technical
problems in 3D data collection of large animal groups and we outline some of
the methodological solutions adopted by the STARFLAG project. In particular, we
explain how to solve the stereoscopic correspondence - or matching - problem,
which was the major bottleneck of all 3D studies in the past.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 15:34:13 GMT"
}
] | 2014-10-10T00:00:00 | [
[
"Cavagna",
"Andrea",
""
],
[
"Giardina",
"Irene",
""
],
[
"Orlandi",
"Alberto",
""
],
[
"Parisi",
"Giorgio",
""
],
[
"Procaccini",
"Andrea",
""
],
[
"Viale",
"Massimiliano",
""
],
[
"Zdravkovic",
"Vladimir",
""
]
] | [
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] |
802.1669 | Nicholas Chia | Nicholas Chia and Junji Nakano | M-decomposability, elliptical unimodal densities, and applications to
clustering and kernel density estimation | 30 pages, 13 figures | null | null | null | stat.ME math.ST stat.ML stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Chia and Nakano (2009) introduced the concept of M-decomposability of
probability densities in one-dimension. In this paper, we generalize
M-decomposability to any dimension. We prove that all elliptical unimodal
densities are M-undecomposable. We also derive an inequality to show that it is
better to represent an M-decomposable density via a mixture of unimodal
densities. Finally, we demonstrate the application of M-decomposability to
clustering and kernel density estimation, using real and simulated data. Our
results show that M-decomposability can be used as a non-parametric criterion
to locate modes in probability densities.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:41:30 GMT"
},
{
"version": "v2",
"created": "Wed, 21 Apr 2010 12:40:03 GMT"
}
] | 2010-04-22T00:00:00 | [
[
"Chia",
"Nicholas",
""
],
[
"Nakano",
"Junji",
""
]
] | [
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] |
802.167 | Henri Gouin | Sergey Gavrilyuk, Henri Gouin (MSNMGP, LMMT) | Symmetric form of governing equations for capillary fluids | 6 pages | Monographs and Surveys in Pure and Applied Mathematics, France
(1999) | null | null | math-ph math.MP physics.flu-dyn | null | In classical continuum mechanics, quasi-linear systems of conservation laws
can be symmetrized if they admit an additional convex conservation law. In
particular, this implies the hyperbolicity of governing equations. For
capillary fluids, the internal energy depends not only on the density but also
on its derivatives with respect to space variables. Consequently, the governing
equations belong to the class of dispersive systems. In that case we propose a
symmetric form of governing equations which is different from the classical
Godunov -Friedrichs - Lax representation. This new symmetric form implies the
stability of constant solutions.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:44:12 GMT"
}
] | 2009-04-14T00:00:00 | [
[
"Gavrilyuk",
"Sergey",
"",
"MSNMGP, LMMT"
],
[
"Gouin",
"Henri",
"",
"MSNMGP, LMMT"
]
] | [
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] |
802.1671 | Stefano Bellucci | Stefano Bellucci and Vadim Ohanyan | Two--center quantum MICZ--Kepler system and the Zeeman effect in the
charge-dyon system | 10 pages, no figures, LaTeX file | Phys.Lett.A372:5765-5772,2008 | 10.1016/j.physleta.2008.07.023 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The quantum two-center MICZ--Kepler system is considered in the limit when
one of the interaction centers is situated at infinity, which leads to
homogeneous electric and magnetic fields appearing in the system. The emerging
system admits separation of variables in the Schr\"{o}dinger equation and is
integrable at the classical level. The first order corrections to the
unperturbed spectrum of the ordinary MICZ--Kepler system are calculated.
Particularly, the linear Zeeman--effect and effects of MICZ-terms are analyzed.
The possible realizations of the system in some quantum dots are considered.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:47:34 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 13:02:20 GMT"
},
{
"version": "v3",
"created": "Thu, 10 Jul 2008 15:05:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bellucci",
"Stefano",
""
],
[
"Ohanyan",
"Vadim",
""
]
] | [
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] |
802.1672 | Cosmas Zachos | Christopher T. Hill and Cosmas K. Zachos | Chern-Simons and WZW Anomaly Cancelations Across Dimensions | 6 pages, ReVtex 4, no figures | Annals Phys.323:3065-3073,2008 | 10.1016/j.aop.2008.08.009 | FERMILAB-Pub-08-027-T, ANL-HEP-PR-08-8 | hep-th hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The WZW functional in D=4 can be derived directly from the Chern-Simons
functional of a compactified D=5 gauge theory and the boundary fermions it
supplants. A simple pedagogical model based on U(1) gauge groups illustrates
how this works. A bulk-boundary system with the fermions eliminated manifestly
evinces anomaly cancelations between CS and WZW terms.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 17:07:47 GMT"
}
] | 2009-09-17T00:00:00 | [
[
"Hill",
"Christopher T.",
""
],
[
"Zachos",
"Cosmas K.",
""
]
] | [
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] |
802.1673 | Zhenbo Qin | Wei-Ping Li, Zhenbo Qin | Equivariant cohomology of incidence Hilbert schemes and loop algebras | 30 pages, 2 figures | null | null | null | math.AG math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $S$ be the affine plane $\C^2$ together with an appropriate $\mathbb T =
\C^*$ action. Let $\hil{m,m+1}$ be the incidence Hilbert scheme. Parallel to
\cite{LQ}, we construct an infinite dimensional Lie algebra that acts on the
direct sum $$\Wft = \bigoplus_{m=0}^{+\infty}H^{2(m+1)}_{\mathbb
T}(S^{[m,m+1]})$$ of the middle-degree equivariant cohomology group of
$\hil{m,m+1}$. The algebra is related to the loop algebra of an infinite
dimensional Heisenberg algebra. In addition, we study the transformations among
three different linear bases of $\Wft$. Our results are applied to the ring
structure of the ordinary cohomology of $\hil{m,m+1}$ and to the ring of
symmetric functions in infinitely many variables.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 17:09:41 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Li",
"Wei-Ping",
""
],
[
"Qin",
"Zhenbo",
""
]
] | [
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] |
802.1674 | Andrea Cavagna | Andrea Cavagna, Irene Giardina, Alberto Orlandi, Giorgio Parisi,
Andrea Procaccini | The STARFLAG handbook on collective animal behaviour: Part II,
three-dimensional analysis | To be published in Animal Behaviour | Animal Behaviour 76 (1), 237-248 (2008) | null | null | q-bio.QM cond-mat.stat-mech q-bio.PE | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The study of collective animal behaviour must progress through a comparison
between the theoretical predictions of numerical models and data coming from
empirical observations. To this aim it is important to develop methods of
three-dimensional (3D) analysis that are at the same time informative about the
structure of the group and suitable to empirical data. In fact, empirical data
are considerably noisier than numerical data, and they are subject to several
constraints. We review here the tools of analysis used by the STARFLAG project
to characterise the 3D structure of large flocks of starlings in the field. We
show how to avoid the most common pitfalls i the quantitative analysis of 3D
animal groups, with particular attention to the problem of the bias introduced
by the border of the group. By means of practical examples, we demonstrate that
neglecting border effects gives rise to artefacts when studying the 3D
structure of a group. Moreover, we show that mathematical rigour is essential
to distinguish important biological properties from trivial geometric features
of animal groups.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 16:38:46 GMT"
}
] | 2014-10-10T00:00:00 | [
[
"Cavagna",
"Andrea",
""
],
[
"Giardina",
"Irene",
""
],
[
"Orlandi",
"Alberto",
""
],
[
"Parisi",
"Giorgio",
""
],
[
"Procaccini",
"Andrea",
""
]
] | [
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802.1675 | Raphael Hirschi | R. Hirschi (1), C. Chiappini (2,3), G. Meynet (2), A. Maeder (2), and
S. Ekstrom (2), (1 Keele University, UK; 2 Geneva Observatory, CH; 3 Trieste
Observatory) | Stellar Evolution at Low Metallicity | 12 pages, 7 figures, "Massive Stars as Cosmic Engines" Conference
proceedings (IAU Symp 250), F. Bresolin, P.A. Crowther, J. Puls Eds | null | 10.1017/S1743921308020528 | null | astro-ph | null | Massive stars played a key role in the early evolution of the Universe. They
formed with the first halos and started the re-ionisation. It is therefore very
important to understand their evolution. In this review, we first recall the
effect of metallicity (Z) on the evolution of massive stars. We then describe
the strong impact of rotation induced mixing and mass loss at very low Z. The
strong mixing leads to a significant production of primary nitrogen 14, carbon
13 and neon 22. Mass loss during the red supergiant stage allows the production
of Wolf-Rayet stars, type Ib,c supernovae and possibly gamma-ray bursts (GRBs)
down to almost Z=0 for stars more massive than 60 solar masses. Galactic
chemical evolution models calculated with models of rotating stars better
reproduce the early evolution of N/O, C/O and C12/C13. Finally, the impact of
magnetic fields is discussed in the context of GRBs.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 17:42:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hirschi",
"R.",
""
],
[
"Chiappini",
"C.",
""
],
[
"Meynet",
"G.",
""
],
[
"Maeder",
"A.",
""
],
[
"Ekstrom",
"S.",
""
]
] | [
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] |
802.1676 | Jeremy O'Brien | Alex S. Clark, Jeremie Fulconis, John G. Rarity, William J. Wadsworth,
Jeremy L. O'Brien | An All Optical Fibre Quantum Controlled-NOT Gate | 4 pages, 4 figures, comments welcome | Phys. Rev. A 79, 030303(R) (2009) | 10.1103/PhysRevA.79.030303 | null | quant-ph | null | We report the first experimental demonstration of an optical controlled-NOT
gate constructed entirely in fibre. We operate the gate using two heralded
optical fibre single photon sources and find an average logical fidelity of 90%
and an average process fidelity of 0.83<F<0.91. On the basis of a simple model
we are able to conclude that imperfections are primarily due to the photon
sources, meaning that the gate itself works with very high fidelity.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 17:57:13 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Clark",
"Alex S.",
""
],
[
"Fulconis",
"Jeremie",
""
],
[
"Rarity",
"John G.",
""
],
[
"Wadsworth",
"William J.",
""
],
[
"O'Brien",
"Jeremy L.",
""
]
] | [
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] |
802.1677 | Chandana Sinha | S. Roy snd C. Sinha | Formation of negative hydrogen ion in Positronium - Hydrogen collisions | 16 pages, 10 figures | null | null | null | physics.atom-ph | http://creativecommons.org/licenses/by/3.0/ | The importance of the excited states of Positronium (Ps) in the formation
cross sections(both differential and total) of the negative hydrogen ion (H^-)
are investigated theoretically for the charge transfer reaction, Ps (n = 1, 2)
+ H --> e+ + H^- for a wide range of incident energies (e. g., threshold - 500
eV) . The calculations are performed in the frame work of a qualitative model,
the post collisional Coulomb Modified Eikonal Approximation (CMEA) . A
comparative study is also made between the capture from ground and excited
states of the Ps. The present CMEA model takes account of higher order effects
which is essential for a rearrangement process where the First Born type
Approximation (Coulomb Born for the ionic case) is not supposed to be adequate.
At low incident energies, the excited states of Ps (2s, 2p) are found to play a
dominant role in the H^- formation cross sections . Significant deviations are
noted between the present CMEA and the Coulomb Born (CBA) results even at very
high incident energies (e.g., Ei = 500 eV), indicating the importance of higher
order effects. At high incident energies the present CMEA differential cross
section (DCS) exhibits a double peak structure which is totally absent in the
CBA and could again be attributed to higher order effects.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 17:33:35 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Sinha",
"S. Roy snd C.",
""
]
] | [
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] |
802.1678 | Valery Kubarovsky | V. Kubarovsky, P. Stoler and I. Bedlinsky (for the CLAS Collaboration) | Deeply Virtual Pseudoscalar Meson Production with CLAS | Prepared for XII Workshop on High Energy Spin Physics DSPIN-07,
Dubna, September 3-7, 2007 | null | 10.1142/9789812796950_0020 | JLAB-PHY-08-776 | hep-ex | null | Deeply virtual meson scattering cross sections and asymmetries for the pi^0
and eta exclusive electroproduction in a very wide kinematic range of Q^2, t
and x_B have been measured with CLAS (JLab). Initial analysis is already
showing remarkable results. These data will help us to better understand the
transition from soft to hard mechanisms.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:38:04 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Kubarovsky",
"V.",
"",
"for the CLAS Collaboration"
],
[
"Stoler",
"P.",
"",
"for the CLAS Collaboration"
],
[
"Bedlinsky",
"I.",
"",
"for the CLAS Collaboration"
]
] | [
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] |
802.1679 | Feng Yuan | Feng Yuan (SHAO), Renyi Ma (SHAO), and Ramesh Narayan (CfA) | A simplified global solution for an advection-dominated accretion flow | 12 pages, 4 figures, accepted by ApJ | null | 10.1086/587484 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | When we model black hole accretion sources such as active galactic nuclei and
black hole X-ray binaries as advection-dominated accretion flows (ADAFs), it is
neccesary to use the global solution to the equations rather than the simpler
self-similar solution, since the latter is inaccurate in the region near the
black hole where most of the radiation is emitted. However, technically, it is
a difficult task to calculate the global solution because of the transonic
nature of the flow, which makes it a two-point boundary value problem. In this
paper we propose a simplified approach for calculating the global ADAF
solution. We replace the radial momentum equation by a simple algebraic
relation between the angular velocity of the gas and the Keplerian angular
velocity, while keeping all other equations unchanged. It is then easy to solve
the differential energy equations to obtain an approximate global solution. By
adjusting the free parameters, we find that for almost any accretion rate and
for $\alpha=0.1-0.3$ we can get good simplified global solutions. The predicted
spectra from the approximate solutions are very close to the spectra obtained
from the true global solutions.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:01:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Yuan",
"Feng",
"",
"SHAO"
],
[
"Ma",
"Renyi",
"",
"SHAO"
],
[
"Narayan",
"Ramesh",
"",
"CfA"
]
] | [
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] |
802.168 | Christian Angrick | Christian Angrick and Matthias Bartelmann | Statistics of gravitational potential perturbations: A novel approach to
deriving the X-ray temperature function | 10 pages, 5 figures, accepted for publication in A&A. Revision to
match the published version. Equation 8 corrected. Notable changes in section
4 including new figures | Astron.Astrophys. 494:461-470,2009 | 10.1051/0004-6361:200809562 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Context. While the halo mass function is theoretically a very sensitive
measure of cosmological models, masses of dark-matter halos are poorly defined,
global, and unobservable quantities.
Aims. We argue that local, observable quantities such as the X-ray
temperatures of galaxy clusters can be directly compared to theoretical
predictions without invoking masses. We derive the X-ray temperature function
directly from the statistics of Gaussian random fluctuations in the
gravitational potential.
Methods. We derive the abundance of potential minima constrained by the
requirement that they belong to linearly collapsed structures. We then use the
spherical-collapse model to relate linear to non-linear perturbations, and the
virial theorem to convert potential depths to temperatures. No reference is
made to mass or other global quantities in the derivation.
Results. Applying a proper high-pass filter that removes large enough modes
from the gravitational potential, we derive an X-ray temperature function that
agrees very well with the classical Press-Schechter approach on relevant
temperature scales, but avoids the necessity of measuring masses.
Conclusions. TThis first study shows that and how an X-ray temperature
function of galaxy clusters can be analytically derived, avoiding the
introduction of poorly defined global quantities such as halo masses. This
approach will be useful for reducing scatter in observed cluster distributions
and thus in cosmological conclusions drawn from them.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:05:30 GMT"
},
{
"version": "v2",
"created": "Wed, 29 Oct 2008 16:53:04 GMT"
},
{
"version": "v3",
"created": "Mon, 26 Jan 2009 10:36:04 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Angrick",
"Christian",
""
],
[
"Bartelmann",
"Matthias",
""
]
] | [
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] |
802.1681 | Lek-Heng Lim | Pierre Comon (University of Nice at Sophia-Antipolis), Gene Golub
(Stanford University), Lek-Heng Lim (Stanford University), Bernard Mourrain
(INRIA at Sophia-Antipolis) | Symmetric tensors and symmetric tensor rank | To appear in the SIAM Journal on Matrix Analysis and Applications | null | null | SCCM Technical Report 06-02 | math.NA math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A symmetric tensor is a higher order generalization of a symmetric matrix. In
this paper, we study various properties of symmetric tensors in relation to a
decomposition into a sum of symmetric outer product of vectors. A rank-1
order-k tensor is the outer product of k non-zero vectors. Any symmetric tensor
can be decomposed into a linear combination of rank-1 tensors, each of them
being symmetric or not. The rank of a symmetric tensor is the minimal number of
rank-1 tensors that is necessary to reconstruct it. The symmetric rank is
obtained when the constituting rank-1 tensors are imposed to be themselves
symmetric. It is shown that rank and symmetric rank are equal in a number of
cases, and that they always exist in an algebraically closed field. We will
discuss the notion of the generic symmetric rank, which, due to the work of
Alexander and Hirschowitz, is now known for any values of dimension and order.
We will also show that the set of symmetric tensors of symmetric rank at most r
is not closed, unless r = 1.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:17:44 GMT"
},
{
"version": "v2",
"created": "Tue, 2 Sep 2008 19:16:47 GMT"
}
] | 2008-09-02T00:00:00 | [
[
"Comon",
"Pierre",
"",
"University of Nice at Sophia-Antipolis"
],
[
"Golub",
"Gene",
"",
"Stanford University"
],
[
"Lim",
"Lek-Heng",
"",
"Stanford University"
],
[
"Mourrain",
"Bernard",
"",
"INRIA at Sophia-Antipolis"
]
] | [
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802.1682 | Matteo G. A. Paris | Roberto Gaiba, Matteo G A Paris | Squeezed vacuum as a universal quantum probe | revised version, 2 figures | Phys. Lett. A 373, 934 (2009) | 10.1016/j.physleta.2009.01.026 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We address local quantum estimation of bilinear Hamiltonians probed by
Gaussian states. We evaluate the relevant quantum Fisher information (QFI) and
derive the ultimate bound on precision. Upon maximizing the QFI we found that
single- and two-mode squeezed vacuum represent an optimal and universal class
of probe states, achieving the so-called Heisenberg limit to precision in terms
of the overall energy of the probe. We explicitly obtain the optimal observable
based on the symmetric logarithmic derivative and also found that homodyne
detection assisted by Bayesian analysis may achieve estimation of squeezing
with near-optimal sensitivity in any working regime. Besides, by comparison of
our results with those coming from global optimization of the measurement we
found that Gaussian states are effective resources, which allow to achieve the
ultimate bound on precision imposed by quantum mechanics using measurement
schemes feasible with current technology.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:18:19 GMT"
},
{
"version": "v2",
"created": "Mon, 9 Jun 2008 16:00:03 GMT"
},
{
"version": "v3",
"created": "Sun, 28 Sep 2008 14:27:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gaiba",
"Roberto",
""
],
[
"Paris",
"Matteo G A",
""
]
] | [
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802.1683 | Andrzej Drzewinski | Andrzej Drzewinski, J.M.J. van Leeuwen | Crossover from Reptation to Rouse dynamics in the Extended
Rubinstein-Duke Model | 16 Pages RevTeX and 13 PostScript figures included, accepted for
publication in Phys. Rev. E | null | 10.1103/PhysRevE.77.031802 | null | cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The competition between reptation and Rouse Dynamics is incorporated in the
Rubinstein-Duke model for polymer motion by extending it with sideways motions,
which cross barriers and create or annihilate hernias. Using the Density-Matrix
Renormalization-Group Method as solver of the Master Equation, the renewal time
and the diffusion coefficient are calculated as function of the length of the
chain and the strength of the sideways motion. These new types of moves have a
strong and delicate influence on the asymptotic behavior of long polymers. The
effects are analyzed as function of the chain length in terms of effective
exponents and crossover scaling functions.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:20:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Drzewinski",
"Andrzej",
""
],
[
"van Leeuwen",
"J. M. J.",
""
]
] | [
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] |
802.1684 | Alice Myerson | A. Myerson, D. Szwer, S. Webster, D. Allcock, M. Curtis, G. Imreh, J.
Sherman, D. Stacey, A. Steane and D. Lucas | High-fidelity readout of trapped-ion qubits | 4 pages, 3 figures; improved readout fidelity (numerical results
changed) | Phys. Rev. Lett. 100, 200502 (2008) | 10.1103/PhysRevLett.100.200502 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We demonstrate single-shot qubit readout with fidelity sufficient for
fault-tolerant quantum computation, for two types of qubit stored in single
trapped calcium ions. For an optical qubit stored in the (4S_1/2, 3D_5/2)
levels of 40Ca+ we achieve 99.991(1)% average readout fidelity in one million
trials, using time-resolved photon counting. An adaptive measurement technique
allows 99.99% fidelity to be reached in 145us average detection time. For a
hyperfine qubit stored in the long-lived 4S_1/2 (F=3, F=4) sub-levels of 43Ca+
we propose and implement a simple and robust optical pumping scheme to transfer
the hyperfine qubit to the optical qubit, capable of a theoretical fidelity
99.95% in 10us. Experimentally we achieve 99.77(3)% net readout fidelity,
inferring at least 99.87(4)% fidelity for the transfer operation.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:30:15 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Apr 2008 13:30:17 GMT"
}
] | 2013-12-24T00:00:00 | [
[
"Myerson",
"A.",
""
],
[
"Szwer",
"D.",
""
],
[
"Webster",
"S.",
""
],
[
"Allcock",
"D.",
""
],
[
"Curtis",
"M.",
""
],
[
"Imreh",
"G.",
""
],
[
"Sherman",
"J.",
""
],
[
"Stacey",
"D.",
""
],
[
"Steane",
"A.",
""
],
[
"Lucas",
"D.",
""
]
] | [
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] |
802.1685 | Christoph Durr | Marcin Bienkowski, Marek Chrobak, Christoph Durr, Mathilde Hurand,
Artur Jez, Lukasz Jez, Jakub Lopuszanski, Grzegorz Stachowiak | Generalized Whac-a-Mole | null | null | null | null | cs.DS | null | We consider online competitive algorithms for the problem of collecting
weighted items from a dynamic set S, when items are added to or deleted from S
over time. The objective is to maximize the total weight of collected items. We
study the general version, as well as variants with various restrictions,
including the following: the uniform case, when all items have the same weight,
the decremental sets, when all items are present at the beginning and only
deletion operations are allowed, and dynamic queues, where the dynamic set is
ordered and only its prefixes can be deleted (with no restriction on
insertions). The dynamic queue case is a generalization of bounded-delay packet
scheduling (also referred to as buffer management). We present several upper
and lower bounds on the competitive ratio for these variants.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:41:46 GMT"
},
{
"version": "v2",
"created": "Sun, 17 Feb 2008 00:09:51 GMT"
}
] | 2016-09-08T00:00:00 | [
[
"Bienkowski",
"Marcin",
""
],
[
"Chrobak",
"Marek",
""
],
[
"Durr",
"Christoph",
""
],
[
"Hurand",
"Mathilde",
""
],
[
"Jez",
"Artur",
""
],
[
"Jez",
"Lukasz",
""
],
[
"Lopuszanski",
"Jakub",
""
],
[
"Stachowiak",
"Grzegorz",
""
]
] | [
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] |
802.1686 | M\'arcio Jos\'e Menon | Geovanna L.P. Silva, Marcio J. Menon, Regina F. Avila | Proton Profile Function at 52.8 GeV | Published in Int. J. Mod. Phys. E | Int.J.Mod.Phys.E16:2923-2926,2007 | 10.1142/S0218301307008732 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present the results of a novel model-independent fit to elastic
proton-proton differential cross section data at $\sqrt s$ = 52.8 GeV. Taking
into account the error propagation from the fit parameters, we determine the
scattering amplitude in the impact parameter space (the proton profile
function) and its statistical uncertainty region. We show that both the real
and imaginary parts of the profile are consistent with two dynamical
contributions, one from a central dense region, up to roughly 1 fm and another
from a peripheral evanescent region from 1 to 3 fm.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 18:44:19 GMT"
}
] | 2011-03-28T00:00:00 | [
[
"Silva",
"Geovanna L. P.",
""
],
[
"Menon",
"Marcio J.",
""
],
[
"Avila",
"Regina F.",
""
]
] | [
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] |
802.1687 | Kenichi Yoshida | Kenichi Yoshida, Nguyen Van Giai | Low-lying dipole resonance in neutron-rich Ne isotopes | 8 pages, 9 figures and 5 tables | Phys.Rev.C78:014305,2008 | 10.1103/PhysRevC.78.014305 | null | nucl-th | null | Microscopic structure of the low-lying isovector dipole excitation mode in
neutron-rich $^{26,28,30}$Ne is investigated by performing deformed
quasiparticle-random-phase-approximation (QRPA) calculations. The particle-hole
residual interaction is derived from a Skyrme force through a Landau-Migdal
approximation. We have obtained the low-lying resonance in $^{26}$Ne at around
8.5 MeV. It is found that the isovector dipole strength at $E_{x}<10$ MeV
exhausts about 6.0% of the classical Thomas-Reiche-Kuhn dipole sum rule. This
excitation mode is composed of several QRPA eigenmodes, one is generated by a
$\nu(2s^{-1}_{1/2} 2p_{3/2})$ transition dominantly, and the other mostly by a
$\nu(2s^{-1}_{1/2} 2p_{1/2})$ transition. The neutron excitations take place
outside of the nuclear surface reflecting the spatially extended structure of
the $2s_{1/2}$ wave function. In $^{30}$Ne, the deformation splitting of the
giant resonance is large, and the low-lying resonance is overlapping with the
giant resonance.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 20:29:56 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Yoshida",
"Kenichi",
""
],
[
"Van Giai",
"Nguyen",
""
]
] | [
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] |
802.1688 | Fabien Bretenaker | F. Goldfarb, J. Ghosh, M. David, J. Ruggiero, T. Chaneli\`ere, J.-L.
Le Gou\"et, H. Gilles, R. Ghosh, and F. Bretenaker | Observation of Ultra-narrow Electromagnetically Induced Transparency and
Slow Light using Purely Electronic Spins in a Hot Atomic Vapor | null | Europhys. Lett. 82, 54002 (2008) | 10.1209/0295-5075/82/54002 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Electromagnetically induced transparency (EIT) is observed in gaseous 4He at
room temperature. Ultra-narrow (less than 10 kHz) EIT windows are obtained for
the first time for purely electronic spins in the presence of Doppler
broadening. The positive role of collisions is emphasized through measurements
of the power dependence of the EIT resonance. Measurement of slow light opens
up possible ways to applications.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:02:27 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Mar 2008 14:01:08 GMT"
}
] | 2008-05-19T00:00:00 | [
[
"Goldfarb",
"F.",
""
],
[
"Ghosh",
"J.",
""
],
[
"David",
"M.",
""
],
[
"Ruggiero",
"J.",
""
],
[
"Chanelière",
"T.",
""
],
[
"Gouët",
"J. -L. Le",
""
],
[
"Gilles",
"H.",
""
],
[
"Ghosh",
"R.",
""
],
[
"Bretenaker",
"F.",
""
]
] | [
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] |
802.1689 | Leonard S. Kisslinger | Leonard S Kisslinger (Department of Physics, Carnegie Mellon
University) Sandip Pakvasa (Department of Physics and Astronomy, University
of Hawaii at Manoa, Honolulu) | SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels | 2 pages, no figures | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using a recent estimate of the velocity of pulsars arising from neutrinos
emitted with modified URCA processes with electrons in Landua levels, and the
temperture of the protoneutron star created by SN1987A, derived from the energy
of the observed neutrinos, we predict the velocity of the resulting pulsar.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:03:11 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Kisslinger",
"Leonard S",
"",
"Department of Physics, Carnegie Mellon\n University"
],
[
"Pakvasa",
"Sandip",
"",
"Department of Physics and Astronomy, University\n of Hawaii at Manoa, Honolulu"
]
] | [
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802.169 | Andrzej Kwasniewski | A. Krzysztof Kwasniewski | More on the Bernoulli and Taylor Formula for Extended Umbral Calculus | 11 pages | Advances in Applied Clifford Algebras Volume 16, Number 1,(2006)
29-39 | null | null | math.CO cs.DM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | One delivers here the extended Bernoulli and Taylor formula of a new sort
with the rest term of the Cauchy type recently derived by the author in the
case of the so called $\psi$-difference calculus which constitutes the
representative for the purpose case of extended umbral calculus. The central
importance of such a type formulas is beyond any doubt. Recent publications do
confirm this historically established experience. Its links via umbrality to
combinatorics are known at least since Rota and Mullin source papers then up to
recently extended by many authors to be indicated in the sequel.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:24:00 GMT"
}
] | 2008-02-15T00:00:00 | [
[
"Kwasniewski",
"A. Krzysztof",
""
]
] | [
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802.1691 | Omar Maj | Omar Maj | Complex geometric optics for symmetric hyperbolic systems I: linear
theory | null | null | null | null | math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We obtain an asymptotic solution for $\ep \to 0$ of the Cauchy problem for
linear first-order symmetric hyperbolic systems with oscillatory initial values
written in the eikonal form of geometric optics with frequency $1/\ep$, but
with complex phases. For the most common linear wave propagation models, this
kind on Cauchy problems are well-known in the applied literature and their
asymptotic theory, referred to as complex geometric optics, is attracting
interest for applications. In this work, which is the first of a series of
papers dedicated to complex geometric optics for nonlinear symmetric hyperbolic
systems, we develop a rigorous linear theory and set the basis for the
subsequent nonlinear analysis.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:35:53 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Maj",
"Omar",
""
]
] | [
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802.1692 | Gail Schaefer | G. H. Schaefer, M. Simon, L. Prato, and T. Barman | Preliminary Orbit of the Young Binary Haro 1-14c | 28 pages, 9 figures, accepted for publication in AJ | null | 10.1088/0004-6256/135/5/1659 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using the Keck Interferometer, we spatially resolved the orbit of the
pre-main sequence binary, Haro 1-14c, for the first time. We present these
interferometric observations along with additional spectroscopic radial
velocity measurements of the components. We performed a simultaneous orbit fit
to the interferometric visibilities and the radial velocities of Haro 1-14c.
Based on a statistical analysis of the possible orbital solutions that fit the
data, we determined component masses of M_1 = 0.96 (+0.27/-0.08) Msun and M_2 =
0.33 (+0.09/-0.02) Msun for the primary and secondary, respectively, and a
distance to the system of 111 (+19/-18) pc. The distance measurement is
consistent with the close distance estimates of the Ophiuchus molecular cloud.
Comparing our results with evolutionary tracks suggests an age of 3-4 Myr for
Haro 1-14c. With additional interferometric measurements to improve the
uncertainties in the masses and distance, we expect the low-mass secondary to
provide important empirical data for calibrating the theoretical evolutionary
tracks for pre-main sequence stars.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:37:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schaefer",
"G. H.",
""
],
[
"Simon",
"M.",
""
],
[
"Prato",
"L.",
""
],
[
"Barman",
"T.",
""
]
] | [
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] |
802.1693 | Marco Picariello | F. Bazzocchi, S. Morisi, M. Picariello, E. Torrente-Lujan | Embedding A4 into SU(3)xU(1) flavor symmetry: Large neutrino mixing and
fermion mass hierarchy in SO(10) GUT | 11 pages, uses package "axodraw", "graphicx" | J.Phys.G36:015002,2009 | 10.1088/0954-3899/36/1/015002 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a common explanation of the fermion mass hierarchy and the large
lepton mixing angles in the context of a grand unified flavor and gauge theory
(GUTF). Our starting point is a SU(3)xU(1) flavor symmetry and a SO(10) GUT, a
basic ingredient of our theory which plays a major role is that two different
breaking pattern of the flavor symmetry are at work. On one side, the dynamical
breaking of SU(3)xU(1) flavor symmetry into U(2)xZ_3 explains why one family is
much heavier than the others. On the other side, an explicit symmetry breaking
of SU(3) into a discrete flavor symmetry leads to the observed tribimaximal
mixing for the leptons. We write an explicit model where this discrete symmetry
group is A4. Naturalness of the charged fermion mass hierarchy appears as a
consequence of the continuous SU(3) flavor symmetry. Moreover, the same
discrete A4-GUT invariant operators are the root of the large lepton mixing,
small Cabibbo angle, and neutrino masses.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:42:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bazzocchi",
"F.",
""
],
[
"Morisi",
"S.",
""
],
[
"Picariello",
"M.",
""
],
[
"Torrente-Lujan",
"E.",
""
]
] | [
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] |
802.1694 | Paola Rebusco Dr | Bruno Coppi | Thermo-Rotational Instability in Plasma Disks Around Compact Objects | null | Europhys.Lett.82:19001,2008 | 10.1209/0295-5075/82/19001 | null | astro-ph | null | Differentially rotating plasma disks, around compact objects, that are
imbedded in a ``seed'' magnetic field are shown to develop vertically localized
ballooning modes that are driven by the combined radial gradient of the
rotation frequency and vertical gradients of the plasma density and
temperature. When the electron mean free path is shorter than the disk height
and the relevant thermal conductivity can be neglected, the vertical particle
flows produced by of these modes have the effect to drive the density and
temperature profiles toward the ``adiabatic condition'' where
$\eta_{T}\equiv(dlnT/dz)/(dlnn/dz)=2/3$. Here $T$ is the plasma temperature and
$n$ the particle density. The faster growth rates correspond to steeper
temperature profiles $(\eta_{T}>2/3)$ such as those produced by an internal
(e.g., viscous) heating process. In the end, ballooning modes excited for
various values of $\eta_{T}$ can lead to the evolution of the disk into a
different current carrying configuration such as a sequence of plasma rings.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:49:30 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Coppi",
"Bruno",
""
]
] | [
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] |
802.1695 | Vasundhara Chetluru | B.Alver, et al (for the PHOBOS collaboration) | Identified charged antiparticle to particle ratios near midrapidity in
Cu+Cu collisions at sqrt(s) = 62.4 and 200 GeV | 5 Pages, 4 figures Made changes to the figures to include the panel
numbers. Slight changes to the text. Updated data points from other
experiments | Phys.Rev.C77:061901,2008 | 10.1103/PhysRevC.77.061901 | null | nucl-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Antiparticle to particle ratios for identified protons, kaons and pions at
sqrt(s) = 62.4 and 200 GeV in Cu+Cu collisions are presented as a function of
centrality for the midrapidity region of 0.2 < eta < 1.4. No strong dependence
on centrality is observed. For the <pbar>/<p> ratio at <p_T> ~ 0.51 GeV/c, we
observe an average value of 0.50 +/- 0.003_(stat) +/- 0.04_(syst) and 0.77 +/-
0.008_(stat) +/- 0.05_(syst) for the 10% most central collisions of 62.4 and
200 GeV Cu+Cu, respectively. The values for all three particle species measured
at sqrt(s) = 200 GeV are in agreement within systematic uncertainties with that
seen in both heavier and lighter systems measured at the same RHIC energy. This
indicates that system size does not appear to play a strong role in determining
the midrapidity chemical freeze-out properties affecting the antiparticle to
particle ratios of the three most abundant particle species produced in these
collisions.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:47:00 GMT"
},
{
"version": "v2",
"created": "Thu, 1 May 2008 14:57:35 GMT"
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] | 2019-08-13T00:00:00 | [
[
"Alver",
"B.",
""
]
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802.1696 | Andrzej Kwasniewski | A. Krzysztof Kwa\'sniewski | First Observations on Prefab Posets Whitney Numbers | 14 pages | Advances in Applied Clifford Algebras Volume 18, Number 1 /
February, 2008, 57-73 | 10.1007/s00006-007-0054-7 | null | math.CO cs.DM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce a natural partial order in structurally natural finite subsets
of the cobweb prefabs sets recently constructed by the present author. Whitney
numbers of the second kind of the corresponding subposet which constitute
Stirling like numbers triangular array are then calculated and the explicit
formula for them is provided. Next, in the second construction we endow the set
sums of prefabiants with such an another partial order that their Bell like
numbers include Fibonacci triad sequences introduced recently by the present
author in order to extend famous relation between binomial Newton coefficients
and Fibonacci numbers onto the infinity of their relatives among whom there are
also the Fibonacci triad sequences and binomial like coefficients (incidence
coefficients included). The first partial order is F sequence independent while
the second partial order is F sequence dependent where F is the so called
admissible sequence determining cobweb poset by construction. An F determined
cobweb posets Hasse diagram becomes Fibonacci tree sheathed with specific
cobweb if the sequence F is chosen to be just the Fibonacci sequence. From the
stand-point of linear algebra of formal series these are generating functions
which stay for the so called extended coherent states of quantum physics. This
information is delivered in the last section.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:47:18 GMT"
}
] | 2008-02-15T00:00:00 | [
[
"Kwaśniewski",
"A. Krzysztof",
""
]
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] |
802.1697 | Omar Maj | Omar Maj | Complex geometric optics for symmetric hyperbolic systems II: nonlinear
theory in one space dimension | null | null | null | null | math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This is the second part of a work aimed to study complex-phase oscillatory
solutions of nonlinear symmetric hyperbolic systems. We consider, in
particular, the case of one space dimension. That is a remarkable case, since
one can always satisfy the \emph{naive} coherence condition on the complex
phases, which is required in the construction of the approximate solution.
Formally the theory applies also in several space dimensions, but the
\emph{naive} coherence condition appears to be too restrictive; the
identification of the optimal coherence condition is still an open problem.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:47:55 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Maj",
"Omar",
""
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] |
802.1698 | Constantino Tsallis | Constantino Tsallis, Angel R. Plastino and Ramon F. Alvarez-Estrada | Escort mean values and the characterization of power-law-decaying
probability densities | 20 pages (2 Appendices have been added) | null | 10.1063/1.3104063 | null | cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Escort mean values (or $q$-moments) constitute useful theoretical tools for
describing basic features of some probability densities such as those which
asymptotically decay like {\it power laws}. They naturally appear in the study
of many complex dynamical systems, particularly those obeying nonextensive
statistical mechanics, a current generalization of the Boltzmann-Gibbs theory.
They recover standard mean values (or moments) for $q=1$. Here we discuss the
characterization of a (non-negative) probability density by a suitable set of
all its escort mean values together with the set of all associated normalizing
quantities, provided that all of them converge. This opens the door to a
natural extension of the well known characterization, for the $q=1$ instance,
of a distribution in terms of the standard moments, provided that {\it all} of
them have {\it finite} values. This question would be specially relevant in
connection with probability densities having {\it divergent} values for all
nonvanishing standard moments higher than a given one (e.g., probability
densities asymptotically decaying as power-laws), for which the standard
approach is not applicable. The Cauchy-Lorentz distribution, whose second and
higher even order moments diverge, constitutes a simple illustration of the
interest of this investigation. In this context, we also address some
mathematical subtleties with the aim of clarifying some aspects of an
interesting non-linear generalization of the Fourier Transform, namely, the
so-called $q$-Fourier Transform.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 19:55:23 GMT"
},
{
"version": "v2",
"created": "Sat, 18 Oct 2008 14:06:33 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Tsallis",
"Constantino",
""
],
[
"Plastino",
"Angel R.",
""
],
[
"Alvarez-Estrada",
"Ramon F.",
""
]
] | [
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] |
802.1699 | Prajakta Nimbhorkar | Nutan Limaye, Meena Mahajan, Prajakta Nimbhorkar | Longest paths in Planar DAGs in Unambiguous Logspace | null | null | null | null | cs.CC | http://creativecommons.org/licenses/by-nc-sa/3.0/ | We show via two different algorithms that finding the length of the longest
path in planar directed acyclic graph (DAG) is in unambiguous logspace UL, and
also in the complement class co-UL. The result extends to toroidal DAGs as
well.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 20:08:39 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Limaye",
"Nutan",
""
],
[
"Mahajan",
"Meena",
""
],
[
"Nimbhorkar",
"Prajakta",
""
]
] | [
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] |
802.17 | Jes\'us San Mart\'in | M. Dolores Sotelo Herrera and Jesus San Martin | An Analytical Study in Coupled Map Lattices of Synchronized States and
Travelling Waves, and of their Period-Doubling Cascades | 35 pages and 6 figures | null | null | null | nlin.PS nlin.CD | null | Several theorems are demonstrated that determine the sufficient conditions
for the existence of synchronized states (periodical and chaotic) and also of
travelling waves in a CML. Also are analytically proven the existence of
period-doubling cascades for the mentioned patterns. The temporal state of any
oscillators are completely characterized. The given results are valid for a
number of arbitrary oscillators whose individual dynamics is ruled by an
arbitrary C^{2} function.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 20:10:30 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 18:09:33 GMT"
}
] | 2008-02-14T00:00:00 | [
[
"Herrera",
"M. Dolores Sotelo",
""
],
[
"Martin",
"Jesus San",
""
]
] | [
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] |
802.1701 | Igor E. Mazets | I.E. Mazets, T. Schumm, J. Schmiedmayer | Breakdown of integrability in a quasi-one-dimensional ultracold bosonic
gas | 4 pages, 3 figures, revtex4 | Phys. Rev. Lett. 100, 210403 (2008) | 10.1103/PhysRevLett.100.210403 | null | cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We demonstrate that virtual excitations of higher radial modes in an atomic
Bose gas in a tightly confining waveguide result in effective three-body
collisions that violate integrability in this quasi-one-dimensional quantum
system and give rise to thermalization. The estimated thermalization rates are
consistent with recent experimental results in quasi-1D dynamics of ultracold
atoms.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 20:20:10 GMT"
}
] | 2008-06-14T00:00:00 | [
[
"Mazets",
"I. E.",
""
],
[
"Schumm",
"T.",
""
],
[
"Schmiedmayer",
"J.",
""
]
] | [
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802.1702 | Sidney Redner | Sanjib Sabhapandit, Satya N. Majumdar, S. Redner | Crowding at the Front of the Marathon Packs | 5 pages, 2 figures; version 2: published manuscript with various
changes in response to referee comments and some additional improvements | J. Stat. Mech. (2008) L03001 | 10.1088/1742-5468/2008/03/L03001 | null | physics.data-an physics.pop-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the crowding of near-extreme events in the time gaps between
successive finishers in major international marathons. Naively, one might
expect these gaps to become progressively larger for better-placing finishers.
While such an increase does indeed occur from the middle of the finishing pack
down to approximately 20th place, the gaps saturate for the first 10-20
finishers. We give a probabilistic account of this feature. However, the data
suggests that the gaps have a weak maximum around the 10th place, a feature
that seems to have a sociological origin.
| [
{
"version": "v1",
"created": "Tue, 12 Feb 2008 20:22:09 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Apr 2008 23:37:28 GMT"
}
] | 2008-04-23T00:00:00 | [
[
"Sabhapandit",
"Sanjib",
""
],
[
"Majumdar",
"Satya N.",
""
],
[
"Redner",
"S.",
""
]
] | [
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Subsets and Splits