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712.1079 | Dr Anthony Henderson | Pramod N. Achar and Anthony Henderson | Orbit closures in the enhanced nilpotent cone | 32 pages. Update (August 2010): There is an error in the proof of
Theorem 4.7, in this version and the almost-identical published version. See
the corrigendum arXiv:1008.1117 for independent proofs of later results that
depend on that statement | Adv. Math. 219 (2008), no. 1, pp. 27-62 | 10.1016/j.aim.2008.04.008 | null | math.RT math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the orbits of $G=\mathrm{GL}(V)$ in the enhanced nilpotent cone
$V\times\mathcal{N}$, where $\mathcal{N}$ is the variety of nilpotent
endomorphisms of $V$. These orbits are parametrized by bipartitions of $n=\dim
V$, and we prove that the closure ordering corresponds to a natural partial
order on bipartitions. Moreover, we prove that the local intersection
cohomology of the orbit closures is given by certain bipartition analogues of
Kostka polynomials, defined by Shoji. Finally, we make a connection with Kato's
exotic nilpotent cone in type C, proving that the closure ordering is the same,
and conjecturing that the intersection cohomology is the same but with degrees
doubled.
| [
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] | 2010-08-10T00:00:00 | [
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"Achar",
"Pramod N.",
""
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712.108 | Igor Shparlinski | Sergei V. Konyagin, Carl Pomerance and Igor E. Shparlinski | On the Distribution of Pseudopowers | null | Can. J. Math.-J. Can. Math. 62 (2010) 582-594 | 10.4153/CJM-2010-020-4 | null | math.NT | null | An $x$-pseudopower to base $g$ is a positive integer which is not a power of
$g$ yet is so modulo $p$ for all primes $p\le x$. We improve an upper bound for
the least such number due to E. Bach, R. Lukes, J. Shallit, and H. C. Williams.
The method is based on a combination of some bounds of exponential sums with
new results about the average behaviour of the multiplicative order of $g$
modulo prime numbers.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 04:56:58 GMT"
}
] | 2019-08-15T00:00:00 | [
[
"Konyagin",
"Sergei V.",
""
],
[
"Pomerance",
"Carl",
""
],
[
"Shparlinski",
"Igor E.",
""
]
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712.1081 | Igor Shparlinski | Carl Pomerance and Igor E. Shparlinski | On Pseudosquares and Pseudopowers | null | null | null | null | math.NT | null | Introduced by Kraitchik and Lehmer, an $x$-pseudosquare is a positive integer
$n\equiv1\pmod 8$ that is a quadratic residue for each odd prime $p\le x$, yet
is not a square. We use bounds of character sums to prove that pseudosquares
are equidistributed in fairly short intervals. An $x$-pseudopower to base $g$
is a positive integer which is not a power of $g$ yet is so modulo $p$ for all
primes $p\le x$. It is conjectured by Bach, Lukes, Shallit, and Williams that
the least such number is at most $\exp(a_g x/\log x)$ for a suitable constant
$a_g$. A bound of $\exp(a_g x\log\log x/\log x)$ is proved conditionally on the
Riemann Hypothesis for Dedekind zeta functions, thus improving on a recent
conditional exponential bound of Konyagin and the present authors. We also give
a GRH-conditional equidistribution result for pseudopowers that is analogous to
our unconditional result for pseudosquares.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 05:04:58 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 21:29:07 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Pomerance",
"Carl",
""
],
[
"Shparlinski",
"Igor E.",
""
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] |
712.1082 | Ioan Bucataru | Ioan Bucataru, Michael A. Slawinski | Invariant properties for finding distance in space of elasticity tensors | null | Journal of Elasticity, 94 (2009), no. 2, 97--114 | 10.1007/s10659-008-9186-9 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using orthogonal projections, we investigate distance of a given elasticity
tensor to classes of elasticity tensors exhibiting particular material
symmetries. These projections depend on the orientation of the elasticity
tensor, hence the distance is obtained as the minimization of corresponding
expressions with respect to the action of the orthogonal group. These
expressions are stated in terms of the eigenvalues of both the given tensor and
the projected one. The process of minimization is facilitated by the fact that,
as we prove, the traces of the corresponding Voigt and dilatation tensors are
invariant under these orthogonal projections. For isotropy, cubic symmetry and
transverse isotropy, we formulate algorithms to find both the orientation and
the eigenvalues of the elasticity tensor that is endowed with a particular
symmetry and is closest to the given elasticity tensor.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 06:44:14 GMT"
},
{
"version": "v2",
"created": "Thu, 11 Sep 2008 09:53:17 GMT"
}
] | 2009-08-12T00:00:00 | [
[
"Bucataru",
"Ioan",
""
],
[
"Slawinski",
"Michael A.",
""
]
] | [
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712.1083 | Arend Bayer | Arend Bayer | Polynomial Bridgeland stability conditions and the large volume limit | v3: minor revisions; v2: Acknowledgment added; 31 pages, 6 figures | Geom. Topol. 13 (2009) 2389-2425 | 10.2140/gt.2009.13.2389 | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce the notion of a polynomial stability condition, generalizing
Bridgeland stability conditions on triangulated categories. We construct and
study a family of polynomial stability conditions for any normal projective
variety. This family includes both Simpson-stability, and large volume limits
of Bridgeland stability conditions.
We show that the PT/DT-correspondence relating stable pairs to
Donaldson-Thomas invariants (conjectured by Pandharipande and Thomas) can be
understood as a wall-crossing in our family of polynomial stability conditions.
Similarly, we show that the relation between stable pairs and invariants of
one-dimensional torsion sheaves (proven recently by the same authors) is a
wall-crossing formula.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 07:02:25 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 20:19:08 GMT"
},
{
"version": "v3",
"created": "Wed, 25 Mar 2009 19:28:59 GMT"
}
] | 2014-11-11T00:00:00 | [
[
"Bayer",
"Arend",
""
]
] | [
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712.1084 | Keigo Fukumura | Keigo Fukumura, Demosthenes Kazanas | Light Echoes in Kerr Geometry: A Source of High Frequency QPOs from
Random X-ray Bursts | accepted to ApJ (v4); 19 pages, 22 black/white figures | null | 10.1086/587159 | null | astro-ph | null | We propose that high frequency quasi-periodic oscillations (HFQPOs) can be
produced from randomly-formed X-ray bursts (flashes) by plasma interior to the
ergosphere of a rapidly-rotating black hole. We show by direct computation of
their orbits that the photons comprising the observed X-ray light curves, if
due to a multitude of such flashes, are affected significantly by the black
hole's dragging of inertial frames; the photons of each such burst arrive to an
observer at infinity in multiple (double or triple), distinct "bunches"
separated by a roughly constant time lag of t/M~14, regardless of the bursts'
azimuthal position. We argue that every other such "bunch" represents photons
that follow trajectories with an additional orbit around the black hole at the
photon circular orbit radius (a photon "echo"). The presence of this constant
lag in the response function of the system leads to a QPO feature in its power
density spectra, even though the corresponding light curve consists of a
totally stochastic signal. This effect is by and large due to the black hole
spin and is shown to gradually diminish as the spin parameter a decreases or
the radial position of the burst moves outside the static limit surface
(ergosphere). Our calculations indicate that for a black hole with Kerr
parameter of a/M=0.99 and mass of M=10*Msun the QPO is expected at a frequency
of ~ 1.3-1.4 kHz. We discuss the plausibility and observational implications of
our model/results as well as its limitations.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 06:53:02 GMT"
},
{
"version": "v2",
"created": "Mon, 4 Feb 2008 20:24:04 GMT"
},
{
"version": "v3",
"created": "Tue, 5 Feb 2008 16:56:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fukumura",
"Keigo",
""
],
[
"Kazanas",
"Demosthenes",
""
]
] | [
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] |
712.1085 | Yihong Hu | Yihong Hu, Daoli Zhu, Yang Li, Bing Su, Bingxin Zhu | Cost-driven weighted networks evolution | 5 pages, 3 figures | null | null | null | physics.soc-ph physics.data-an | null | Inspired by studies on airline networks we propose a general model for
weighted networks in which topological growth and weight dynamics are both
determined by cost adversarial mechanism. Since transportation networks are
designed and operated with objectives to reduce cost, the theory of cost in
micro-economics plays a critical role in the evolution. We assume vertices and
edges are given cost functions according to economics of scale and diseconomics
of scale (congestion effect). With different cost functions the model produces
broad distribution of networks. The model reproduces key properties of real
airline networks: truncated degree distributions, nonlinear strength degree
correlations, hierarchy structures, and particulary the disassortative and
assortative behavior observed in different airline networks. The result
suggests that the interplay between economics of scale and diseconomics of
scale is a key ingredient in order to understand the underlying driving factor
of the real-world weighted networks.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 07:01:46 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Hu",
"Yihong",
""
],
[
"Zhu",
"Daoli",
""
],
[
"Li",
"Yang",
""
],
[
"Su",
"Bing",
""
],
[
"Zhu",
"Bingxin",
""
]
] | [
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] |
712.1086 | P\'ech\'e Sandrine | A. Borodin, S. Peche | Airy kernel with two sets of parameters in directed percolation and
random matrix theory | figures improved; references and comments added | null | 10.1007/s10955-008-9553-8 | null | math-ph math.MP math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce a generalization of the extended Airy kernel with two sets of
real parameters. We show that this kernel arises in the edge scaling limit of
correlation kernels of determinantal processes related to a directed
percolation model and to an ensemble of random matrices.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 07:02:52 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Jan 2008 07:03:11 GMT"
},
{
"version": "v3",
"created": "Fri, 27 Jun 2008 11:02:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Borodin",
"A.",
""
],
[
"Peche",
"S.",
""
]
] | [
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] |
712.1087 | Shizeng Lin | Shizeng Lin and Bo Zheng | Short-time critical dynamics at perfect and non-perfect surface | 11figures | Phys. Rev. E 78, 011127 (2008) | 10.1103/PhysRevE.78.011127 | null | physics.comp-ph physics.gen-ph | null | We report Monte Carlo simulations of critical dynamics far from equilibrium
on a perfect and non-perfect surface in the 3d Ising model. For an ordered
initial state, the dynamic relaxation of the surface magnetization, the line
magnetization of the defect line, and the corresponding susceptibilities and
appropriate cumulant is carefully examined at the ordinary, special and surface
phase transitions. The universal dynamic scaling behavior including a dynamic
crossover scaling form is identified. The exponent $\beta_1$ of the surface
magnetization and $\beta_2$ of the line magnetization are extracted. The impact
of the defect line on the surface universality classes is investigated.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:19:21 GMT"
}
] | 2008-07-31T00:00:00 | [
[
"Lin",
"Shizeng",
""
],
[
"Zheng",
"Bo",
""
]
] | [
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] |
712.1088 | Valerij Gurin S | Valerij Gurin | Asymmetry of Endofullerenes with Silver Atoms | 7 pages, 2 figures | null | null | null | cond-mat.other | null | A series of endofullerenes Ag@C60 with different symmetry are calculated at
ab initio level. The lowest energy structure is completely asymmetrical one
(C1), in which the endo-atom has noticeably off-centre position. The
symmetrical structures are less stable. Silver atom in the Ag@C60 (C1)
endofullerene has the low negative charge and high spin density.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 07:48:05 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Gurin",
"Valerij",
""
]
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712.1089 | Ibrar Hussain | Ibrar Hussain, Fazal M. Mahomed and Asghar Qadir | Second-Order Approximate Symmetries of the Geodesic Equations for the
Reissner-Nordstr\"om Metric and Re-Scaling of Energy of a Test Particle | 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 3:115,2007 | 10.3842/SIGMA.2007.115 | null | gr-qc nlin.SI | null | Following the use of approximate symmetries for the Schwarzschild spacetime
by A.H. Kara, F.M. Mahomed and A. Qadir (Nonlinear Dynam., to appear), we have
investigated the exact and approximate symmetries of the system of geodesic
equations for the Reissner-Nordstr\"om spacetime (RN). For this purpose we are
forced to use second order approximate symmetries. It is shown that in the
second-order approximation, energy must be rescaled for the RN metric. The
implications of this rescaling are discussed.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 08:16:34 GMT"
}
] | 2008-12-19T00:00:00 | [
[
"Hussain",
"Ibrar",
""
],
[
"Mahomed",
"Fazal M.",
""
],
[
"Qadir",
"Asghar",
""
]
] | [
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712.109 | Francisco Gancedo | Diego Cordoba and Francisco Gancedo | A maximum principle for the Muskat problem for fluids with different
densities | 16 pages | null | 10.1007/s00220-008-0587-1 | null | math.AP | null | We consider the fluid interface problem given by two incompressible fluids
with different densities evolving by Darcy's law. This scenario is known as the
Muskat problem for fluids with the same viscosities, being in two dimensions
mathematically analogous to the two-phase Hele-Shaw cell. We prove in the
stable case (the denser fluid is below) a maximum principle for the $L^\infty$
norm of the free boundary.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 17:21:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cordoba",
"Diego",
""
],
[
"Gancedo",
"Francisco",
""
]
] | [
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] |
712.1091 | Gian Salis | L. Meier, G. Salis, E. Gini, I. Shorubalko, K. Ensslin | Two-dimensional imaging of the spin-orbit effective magnetic field | 6 pages, 4 figures | Physical Review B 77, 035305 (2008) | 10.1103/PhysRevB.77.035305 | null | cond-mat.mes-hall | null | We report on spatially resolved measurements of the spin-orbit effective
magnetic field in a GaAs/InGaAs quantum-well. Biased gate electrodes lead to an
electric-field distribution in which the quantum-well electrons move according
to the local orientation and magnitude of the electric field. This motion
induces Rashba and Dresselhaus effective magnetic fields. The projection of the
sum of these fields onto an external magnetic field is monitored locally by
measuring the electron spin-precession frequency using time-resolved Faraday
rotation. A comparison with simulations shows good agreement with the
experimental data.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 08:27:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Meier",
"L.",
""
],
[
"Salis",
"G.",
""
],
[
"Gini",
"E.",
""
],
[
"Shorubalko",
"I.",
""
],
[
"Ensslin",
"K.",
""
]
] | [
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] |
712.1092 | Ranjith Nair | Ranjith Nair and Horace P. Yuen | Comment on "Exposed-Key Weakness of Alpha-Eta" [Phys. Lett. A 370 (2007)
131] | Published version | Phys. Lett. A 372 (2008) 7091-7096 | 10.1016/j.physleta.2008.10.037 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that the insecurity claim of the AlphaEta cryptosystem made by C. Ahn
and K. Birnbaum in Phys. Lett. A 370 (2007) 131-135 under heterodyne attack is
based on invalid extrapolations of Shannon's random cipher analysis and on an
invalid statistical independence assumption. We show, both for standard ciphers
and AlphaEta, that expressions of the kind given by Ahn and Birnbaum can at
best be interpreted as security lower bounds.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 08:39:23 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Jan 2008 04:53:25 GMT"
},
{
"version": "v3",
"created": "Fri, 8 Feb 2008 22:22:13 GMT"
},
{
"version": "v4",
"created": "Sat, 2 Aug 2008 03:49:26 GMT"
},
{
"version": "v5",
"created": "Fri, 26 Sep 2008 04:19:34 GMT"
},
{
"version": "v6",
"created": "Wed, 19 Nov 2008 00:26:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nair",
"Ranjith",
""
],
[
"Yuen",
"Horace P.",
""
]
] | [
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] |
712.1093 | Kyounghee Kim | Jungmin Choi and Kyounghee Kim | The derivatives of Asian call option prices | null | null | null | null | q-fin.PR math.PR | null | The distribution of a time integral of geometric Brownian motion is not well
understood. To price an Asian option and to obtain measures of its dependence
on the parameters of time, strike price, and underlying market price, it is
essential to have the distribution of time integral of geometric Brownian
motion and it is also required to have a way to manipulate its distribution. We
present integral forms for key quantities in the price of Asian option and its
derivatives ({\it{delta, gamma,theta, and vega}}). For example for any $a>0$
$\mathbb{E} [ (A_t -a)^+] = t -a + a^{2} \mathbb{E} [ (a+A_t)^{-1} \exp
(\frac{2M_t}{a+ A_t} - \frac{2}{a}) ]$, where $A_t = \int^t_0 \exp (B_s -s/2)
ds$ and $M_t =\exp (B_t -t/2).$
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 08:40:48 GMT"
}
] | 2008-12-02T00:00:00 | [
[
"Choi",
"Jungmin",
""
],
[
"Kim",
"Kyounghee",
""
]
] | [
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] |
712.1094 | Beata Ziaja | B. Ziaja, H. Wabnitz, E. Weckert and T. M\"oller | Atomic clusters of various sizes irradiated with short intense pulses of
VUV radiation | 6 pages, 5 figures | null | 10.1209/0295-5075/82/24002 | null | physics.plasm-ph | null | Non-equilibrium processes following the irradiation of atomic clusters with
short pulses of vacuum ultraviolet radiation are modelled using kinetic
Boltzmann equations. The dependence of the ionization dynamics on the cluster
size is investigated. The predictions on: (i) the maximal and average ion
charge created, (ii) ion charge state distribution, (iii) average energy
absorbed per atom, (iv) spatial charge distribution, and (v) thermalization
scales are obtained for spherical xenon clusters containing: 20, 70, 2500 and
90000 atoms. These clusters were exposed to single rectangular pulses of vacuum
ultraviolet radiation of various pulse intensities, I ~ 10^{12}-10^{14} W/cm^2
and durations < 50 fs, at a fixed integrated radiation flux of F=0.4 J/cm^2.
The results obtained are found to be in good agreement with the available
experimental data, especially the dependence on the cluster size, if it is
assumed that the ions from the positively charged outer layer of the cluster
constitute the dominant contribution to the experimentally measured ion charge
state distribution.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:02:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ziaja",
"B.",
""
],
[
"Wabnitz",
"H.",
""
],
[
"Weckert",
"E.",
""
],
[
"Möller",
"T.",
""
]
] | [
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] |
712.1095 | S. K. Malik | R. Nirmala, Darshan C. Kundaliya, A. V. Morozkin, S. K. Malik | Magnetocaloric effect in R2Ti3Ge4 (R = Gd, Tb and Er) Compounds | 12 pages incl 3 figures, submitted to Journal of Applied Physics | null | 10.1063/1.2841720 | null | cond-mat.mtrl-sci | null | Heat capacity of polycrystalline R2Ti3Ge4 (R = Gd, Tb and Er) compounds
(Orthorhombic, Sm5Ge4-type, Space group Pnma) has been studied in the
temperature range of 1.8 K to 300 K in various applied magnetic fields. The
compounds with magnetic lanthanide elements show interesting low field
magnetism intrigued by possible presence of competing antiferromagnetic and
ferromagnetic interactions. The magnetocaloric effect in these compounds is
estimated from the field dependent heat capacity data. The magnetic entropy
change and the adiabatic temperature change in the vicinity of the magnetic
transition are found to be significant.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 08:52:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nirmala",
"R.",
""
],
[
"Kundaliya",
"Darshan C.",
""
],
[
"Morozkin",
"A. V.",
""
],
[
"Malik",
"S. K.",
""
]
] | [
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] |
712.1096 | Bongsoo Kim | Bongsoo Kim and Kyozi Kawasaki | A FDR-preserving field theory for interacting Brownian particles:
one-loop theory and MCT | 66 pages, 8 figures, submitted to J. Stat. Mech | J. Stat. Mech. (2008) P02004 | 10.1063/1.2897790 | null | cond-mat.dis-nn cond-mat.stat-mech | null | We develop a field theoretical treatment of a model of interacting Brownian
particles. We pay particular attention to the requirement of the time reversal
invariance and the fluctuation-dissipation relationship (FDR). The method used
is a modified version of the auxiliary field method due originally to
Andreanov, Biroli and Lefevre [J. Stat. Mech. P07008 (2006)]. We recover the
correct diffusion law when the interaction is dropped as well as the standard
mode coupling equation in the one-loop order calculation for interacting
Brownian particle systems.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:21:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kim",
"Bongsoo",
""
],
[
"Kawasaki",
"Kyozi",
""
]
] | [
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712.1097 | Joao Marques-Silva | Joao Marques-Silva, Jordi Planes | On Using Unsatisfiability for Solving Maximum Satisfiability | null | null | null | null | cs.AI cs.DS | null | Maximum Satisfiability (MaxSAT) is a well-known optimization pro- blem, with
several practical applications. The most widely known MAXS AT algorithms are
ineffective at solving hard problems instances from practical application
domains. Recent work proposed using efficient Boolean Satisfiability (SAT)
solvers for solving the MaxSAT problem, based on identifying and eliminating
unsatisfiable subformulas. However, these algorithms do not scale in practice.
This paper analyzes existing MaxSAT algorithms based on unsatisfiable
subformula identification. Moreover, the paper proposes a number of key
optimizations to these MaxSAT algorithms and a new alternative algorithm. The
proposed optimizations and the new algorithm provide significant performance
improvements on MaxSAT instances from practical applications. Moreover, the
efficiency of the new generation of unsatisfiability-based MaxSAT solvers
becomes effectively indexed to the ability of modern SAT solvers to proving
unsatisfiability and identifying unsatisfiable subformulas.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:21:58 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Marques-Silva",
"Joao",
""
],
[
"Planes",
"Jordi",
""
]
] | [
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712.1098 | Steven Duplij | Steven Duplij (Kharkov National University) and Illia Shapoval (NSC
Kharkov Institute of Physics and Technology) | Quantum Computations: Fundamentals And Algorithms | 6 pages, presented at "Quantum Electrodynamics and Statistical
Physics", 2nd Int. Conf., Sept. 19-23, 2006 Kharkov, Ukraine. For extended
28pp. (10pt,wide) version in Russian "Topological Methods In Quantum
Computations" (J.KNU,2007) see
http://www.math.rutgers.edu/~duplij/publications/Duplij-Shapoval_TOPOLOGICAL-QUANTUM-COMPUTERS.pdf | Problems Of Atomic Science And Technology
(PAST-VANT).-2007.-No.3(1).-p.230-235 | null | null | quant-ph | null | Basic concepts of quantum theory of information, principles of quantum
calculations and the possibility of creation on this basis unique on
calculation power and functioning principle device, named quantum computer, are
briefly reviewed. The main blocks of quantum logic, schemes of implementation
of quantum calculations, as well as some known today effective quantum
algorithms, called to realize advantages of quantum calculations upon
classical, are concerned. Among them special place is taken by Shor's algorithm
of number factorization, Grover's algorithm of unsorted database search and,
finally, the most promising in application methods of quantum phenomena
simulation, particularly quantum chaos. The most perspective methods of
experimental realization of quantum computer, namely nuclear-magnetic resonance
and trapped ions realizations, are discussed. Phenomena of decoherence, its
influence on quantum computer stability and methods of quantum error correction
are described.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:10:17 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Duplij",
"Steven",
"",
"Kharkov National University"
],
[
"Shapoval",
"Illia",
"",
"NSC\n Kharkov Institute of Physics and Technology"
]
] | [
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712.1099 | Bruce S. Weir | Bruce S. Weir | The rarity of DNA profiles | Published in at http://dx.doi.org/10.1214/07-AOAS128 the Annals of
Applied Statistics (http://www.imstat.org/aoas/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Statistics 2007, Vol. 1, No. 2, 358-370 | 10.1214/07-AOAS128 | IMS-AOAS-AOAS128 | stat.AP | null | It is now widely accepted that forensic DNA profiles are rare, so it was a
surprise to some people that different people represented in offender databases
are being found to have the same profile. In the first place this is just an
illustration of the birthday problem, but a deeper analysis must take into
account dependencies among profiles caused by family or population membership.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:42:10 GMT"
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] | 2007-12-18T00:00:00 | [
[
"Weir",
"Bruce S.",
""
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712.11 | Gary Steigman | Gary Steigman | Primordial Nucleosynthesis in the Precision Cosmology Era | Recently published article in the 2007 volume of the Annual Reviews
of Nuclear and Particle Science (Vol. 57, p. 463-491). 13 Figures. Note that
there are typos in eq.6 (2.68 should be 2.67) and in eq.26 (there should be a
+ sign in front of 106...) | Ann.Rev.Nucl.Part.Sci.57:463-491,2007 | 10.1146/annurev.nucl.56.080805.140437 | null | astro-ph gr-qc hep-ph nucl-th | null | Primordial nucleosynthesis provides a probe of the Universe during its early
evolution. Given the progress exploring the constituents, structure, and recent
evolution of the Universe, it is timely to review the status of Big Bang
Nucleosynthesis (BBN) and to confront its predictions, along with the
constraints which emerge from them, with those derived from independent
observations of the Universe at much later epochs in its evolution. Following
an overview of the key physics controlling element synthesis in the early
Universe, the predictions of BBN in the standard models of cosmology and
particle physics are presented, along with those from some non-standard models.
The observational data used to infer the primordial abundances are described,
with an emphasis on the distinction between precision and accuracy. The
observationally inferred relic abundances are compared with the predicted
abundances, testing the internal consistency of BBN and enabling a comparison
of the BBN-inferred constraints with those derived from the Cosmic Background
Radiation and Large Scale Structure data. Emerging from these comparisons is
confirmation of a successful standard model along with constraints on (or hints
of) physics beyond the standard models of particle physics and of cosmology.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 20:57:06 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Steigman",
"Gary",
""
]
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712.1101 | Imam Fachruddin | I. Fachruddin and I. Abdulrahman | Scattering of Spin-Zero and Spin-Half Particles in Momentum-Helicity
Basis | 3 pages, 2 columns, 2 figures, Contribution to The Second Asian
Physics Symposium, November 29-30, 2007, Bandung, Indonesia | null | null | null | nucl-th | null | Scattering of 2 particles of spin 0 and 1/2 is evaluated based on a basis
constructed from the momentum and the helicity states (the momentum-helicity
basis). This shortly called three-dimensional (3D) technique is a good
alternative to the standard partial wave (PW) technique especially for higher
energies, where PW calculations may become not feasible. Taking as input a
simple spin-orbit potential model we calculate as an example the spin averaged
differential cross section and polarization.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:01:22 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Fachruddin",
"I.",
""
],
[
"Abdulrahman",
"I.",
""
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] |
712.1102 | Gregoire Misguich | Gregoire Misguich (IPhT [ex-SPhT], CEA Saclay), and Frederic Mila
(EPFL) | Quantum Dimer Model on the triangular lattice: Semiclassical and
variational approaches to vison dispersion and condensation | 12 pages, 10 figures. v2: minor changes, to appear in Phys. Rev. B | Phys. Rev. B 77, 134421 (2008) | 10.1103/PhysRevB.77.134421 | IPhT t07/159 | cond-mat.str-el | null | After reviewing the concept of vison excitations in Z_2 dimer liquids, we
study the liquid-crystal transition of the Quantum Dimer Model on the
triangular lattice by means of a semiclassical spin-wave approximation to the
dispersion of visons in the context of a "soft-dimer" version of the model.
This approach captures some important qualitative features of the transition:
continuous nature of the transition, linear dispersion at the critical point,
and \sqrt{12}x\sqrt{12} symmetry-breaking pattern. In a second part, we present
a variational calculation of the vison dispersion relation at the RK point
which reproduces the qualitative shape of the dispersion relation and the order
of magnitude of the gap. This approach provides a simple but reliable
approximation of the vison wave functions at the RK point.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:06:51 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 10:58:26 GMT"
}
] | 2008-05-27T00:00:00 | [
[
"Misguich",
"Gregoire",
"",
"IPhT [ex-SPhT], CEA Saclay"
],
[
"Mila",
"Frederic",
"",
"EPFL"
]
] | [
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] |
712.1103 | Claudio Bonanno | J. Bellazzini, V. Benci, C. Bonanno, A.M. Micheletti | Solitons for the nonlinear Klein-Gordon equation | 20 pages | null | null | null | math.AP math-ph math.MP | null | In this paper we study existence and orbital stability for solitary waves of
the nonlinear Klein-Gordon equation. The energy of these solutions travels as a
localized packet, hence they are a particular type of solitons. In particular
we are interested in sufficient conditions on the potential for the existence
of solitons. Our proof is based on the study of the ratio energy/charge of a
function, which turns out to be a useful approach for many field equations.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:58:30 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Bellazzini",
"J.",
""
],
[
"Benci",
"V.",
""
],
[
"Bonanno",
"C.",
""
],
[
"Micheletti",
"A. M.",
""
]
] | [
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] |
712.1104 | Dmitry Anchishkin | Dmitry Anchishkin (Bogolyubov Institute for Theoretical Physics, Kiev)
and Ulrich Heinz (The Ohio State University, Columbus) | Two-Particle Correlations in the Wave Function and Covariant Current
Approaches | 27 pages, 3 figures; Extended version of the talk given at the
International Workshop on Relativistic Nuclear Physics (WRNP 2007), June
2007, Kiev, Ukraine; typos added | Phys.Atom.Nucl.71:1632-1646,2008 | 10.1134/S1063778808090202 | null | hep-ph | null | We consider two-particle correlations, which appear in relativistic nuclear
collisions due to the quantum statistics of identical particles, in the frame
of two formalisms: wave-function and current. The first one is based on
solution of the Cauchy problem, whereas the second one is a so-called current
parametrization of the source of secondary particles. We argue that these two
parameterizations of the source coincide when the wave function at freeze-out
times is put in a specific correspondence with a current. Then, the
single-particle Wigner density evaluated in both approaches gives the same
result.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 09:58:49 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 14:22:24 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Anchishkin",
"Dmitry",
"",
"Bogolyubov Institute for Theoretical Physics, Kiev"
],
[
"Heinz",
"Ulrich",
"",
"The Ohio State University, Columbus"
]
] | [
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] |
712.1105 | Richard Lyon | Richard G. Lyon, Sally Heap, Amy Lo, Webster Cash, Glenn D. Starkman,
Robert J. Vanderbei, N. Jeremy Kasdin, Craig J. Copi | Externally Occulted Terrestrial Planet Finder Coronagraph: Simulations
and Sensitivities | null | Proc.SPIE Int.Soc.Opt.Eng.6687:668719,2007 | 10.1117/12.731755 | null | astro-ph | null | A multitude of coronagraphic techniques for the space-based direct detection
and characterization of exo-solar terrestrial planets are actively being
pursued by the astronomical community. Typical coronagraphs have internal
shaped focal plane and/or pupil plane occulting masks which block and/or
diffract starlight thereby increasing the planet's contrast with respect to its
parent star. Past studies have shown that any internal technique is limited by
the ability to sense and control amplitude, phase (wavefront) and polarization
to exquisite levels - necessitating stressing optical requirements. An
alternative and promising technique is to place a starshade, i.e. external
occulter, at some distance in front of the telescope. This starshade suppresses
most of the starlight before entering the telescope - relaxing optical
requirements to that of a more conventional telescope. While an old technique
it has been recently been advanced by the recognition that circularly symmetric
graded apodizers can be well approximated by shaped binary occulting masks.
Indeed optimal shapes have been designed that can achieve smaller inner working
angles than conventional coronagraphs and yet have high effective throughput
allowing smaller aperture telescopes to achieve the same coronagraphic
resolution and similar sensitivity as larger ones.
Herein we report on our ongoing modeling, simulation and optimization of
external occulters and show sensitivity results with respect to number and
shape errors of petals, spectral passband, accuracy of Fresnel propagation, and
show results for both filled and segmented aperture telescopes and discuss
acquisition and sensing of the occulter's location relative to the telescope.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:11:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lyon",
"Richard G.",
""
],
[
"Heap",
"Sally",
""
],
[
"Lo",
"Amy",
""
],
[
"Cash",
"Webster",
""
],
[
"Starkman",
"Glenn D.",
""
],
[
"Vanderbei",
"Robert J.",
""
],
[
"Kasdin",
"N. Jeremy",
""
],
[
"Copi",
"Craig J.",
""
]
] | [
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] |
712.1106 | Amy Berrington de Gonz\'{a}lez | Amy Berrington de Gonz\'alez, D. R. Cox | Interpretation of interaction: A review | Published in at http://dx.doi.org/10.1214/07-AOAS124 the Annals of
Applied Statistics (http://www.imstat.org/aoas/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Statistics 2007, Vol. 1, No. 2, 371-385 | 10.1214/07-AOAS124 | IMS-AOAS-AOAS124 | stat.AP | null | Several different types of statistical interaction are defined and
distinguished, primarily on the basis of the nature of the factors defining the
interaction. Illustrative examples, mostly epidemiological, are given. The
emphasis is primarily on interpretation rather than on methods for detecting
interactions.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:16:48 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"de González",
"Amy Berrington",
""
],
[
"Cox",
"D. R.",
""
]
] | [
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] |
712.1107 | Ilya D. Feranchuk | Ilya D. Feranchuk and Sergey I. Feranchuk | Self-Localized Quasi-Particle Excitation in Quantum Electrodynamics and
Its Physical Interpretation | 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 3:117,2007 | 10.3842/SIGMA.2007.117 | null | math-ph hep-ph math.MP | null | The self-localized quasi-particle excitation of the electron-positron field
(EPF) is found for the first time in the framework of a standard form of the
quantum electrodynamics. This state is interpreted as the ``physical'' electron
(positron) and it allows one to solve the following problems: i) to express the
``primary'' charge $e_0$ and the mass $m_0$ of the ``bare'' electron in terms
of the observed values of $e$ and $m$ of the ``physical'' electron without any
infinite parameters and by essentially nonperturbative way; ii) to consider
$\mu$-meson as another self-localized EPF state and to estimate the ratio
$m_{\mu}/m$; iii) to prove that the self-localized state is Lorentz-invariant
and its energy spectrum corresponds to the relativistic free particle with the
observed mass $m$; iv) to show that the expansion in a power of the observed
charge $e \ll 1$ corresponds to the strong coupling expansion in a power of the
``primary'' charge $e^{-1}_0 \sim e $ when the interaction between the
``physical'' electron and the transverse electromagnetic field is considered by
means of the perturbation theory and all terms of this series are free from the
ultraviolet divergence.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:18:14 GMT"
}
] | 2008-12-19T00:00:00 | [
[
"Feranchuk",
"Ilya D.",
""
],
[
"Feranchuk",
"Sergey I.",
""
]
] | [
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712.1108 | Giovanni Vladilo | Giovanni Vladilo, Jason X. Prochaska, Arthur M. Wolfe | The color excess of quasars with intervening DLA systems- Analysis of
the SDSS data release five | Accepted for publication on Astronomy & Astrophysics, 17 pages, 10
figures | null | 10.1051/0004-6361:20078480 | null | astro-ph | null | We analyzed the spectroscopic and photometric database of the 5th data
release of the Sloan Digital Sky Survey (SDSS) to search for evidence of the
quasar reddening produced by dust embedded in intervening damped Ly alpha (DLA)
systems. From a list of 5164 quasars in the interval of emission redshift 2.25
</= z_e </= 3.5 and SDSS spectra with signal-to-noise ratio SNR >/= 4, we built
up an "absorption sample" of 248 QSOs with a single DLA system in the interval
of absorption redshift 2.2 < z_a </= 3.5 and a "pool" of 1959 control QSOs
without DLA systems or strong metal systems. For each QSO of the absorption
sample we extracted from the pool a subset of control QSOs that are closest in
redshift and magnitude. The mean color of this subset was used as a zero point
to measure the "deviation from the mean color" of individual DLA-QSOs, Delta_i.
The colors were measured using "BEST" ugriz SDSS imaging data. The mean color
excess of the absorption sample, <E>, was estimated by averaging the individual
color deviations Delta_i. We find <E(r-z)> = 27 +/- 9 x 10**(-3) mag and
<E(g-z)> = 54 +/- 12 x 10**(-3) mag. These values are representative of the
reddening of DLA systems at z_a ~ 2.7 in SDSS QSOs with limiting magnitude r
=/~ 20.2. The detection of the mean reddening is confirmed by several
statistical tests. Analysis of the results suggests an origin of the reddening
in dust embedded in the DLA systems, with an SMC-type extinction curve. By
converting the reddening into rest-frame extinction, we derive a mean
dust-to-gas ratio <A_V/N(HI)> ~ 2 to 4 x 10**(-23) mag cm^2. This value is ~
-1.25 dex lower than the mean dust-to-gas ratio of the Milky Way, in line with
the lower level of metallicity in the present DLA sample.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:37:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vladilo",
"Giovanni",
""
],
[
"Prochaska",
"Jason X.",
""
],
[
"Wolfe",
"Arthur M.",
""
]
] | [
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712.1109 | Henrik Beuther | Henrik Beuther | Massive Star Formation: The Power of Interferometry | 26 pages, 10 figures, review on the occasion of the Ludwig Biermann
prize of the German Astronomical Society, a high-resolution version can be
found at http://www.mpia.de/homes/beuther/papers.html | null | null | null | astro-ph | null | This article presents recent work to constrain the physical and chemical
properties in high-mass star formation based largely on interferometric
high-spatial-resolution continuum and spectral line studies at (sub)mm
wavelengths. After outlining the concepts, potential observational tests, a
proposed evolutionary sequence and different possible definitions for massive
protostars, four particular topics are highlighted: (a) What are the physical
conditions at the onset of massive star formation? (b) What are the
characteristics of potential massive accretion disks and what do they tell us
about massive star formation in general? (c) How do massive clumps fragment,
and what does it imply to high-mass star formation? (d) What do we learn from
imaging spectral line surveys with respect to the chemistry itself as well as
for utilizing molecules as tools for astrophysical investigations?
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:41:19 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Beuther",
"Henrik",
""
]
] | [
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0.0531111732,
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] |
712.111 | Rudi Van Nieuwenhove | Rudi Van Nieuwenhove | Vacuum Modified Gravity as an explanation for flat galaxy rotation
curves | aacelerated expansion of the universe explained by vacuum modified
gravity | Concepts Phys.6:43,2009 | 10.2478/v10005-009-0003-4 | null | physics.gen-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A theory is proposed which allows explaining the observed flat galaxy
rotation curves, without needing to invoke dark matter. Whereas other theories
have been proposed in the past which realize the same, the present theory rests
on basic physical principles, in contrast to for instance the MOND theory. The
key to arrive at this new theory is to consider from the start the energy
density of the vacuum. The way to calculate the effect of the corresponding
vacuum pressure on a mass has previously been laid down by Van Nieuwenhove
(1992). We obtain a modification of Newton's law of gravitation with some
peculiar properties such as the occurrence of regions of repulsive gravity.
Based on a newly derived equation of state of the vacuum, the Tully-Fisher
relation is derived. The theory can make detailed predictions about galaxy
rotation curves and is also able to explain to the Pioneer anomaly, the foamy
distribution of galaxies and the observed accelerated expansion of the
universe. A relativistic extension of the theory is included as well.
| [
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{
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"created": "Thu, 10 Jan 2008 11:22:49 GMT"
},
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"version": "v4",
"created": "Mon, 23 Jun 2008 07:53:19 GMT"
},
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"created": "Tue, 24 Jun 2008 05:56:26 GMT"
},
{
"version": "v6",
"created": "Wed, 25 Jun 2008 08:02:12 GMT"
},
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"version": "v7",
"created": "Tue, 25 Nov 2008 07:13:00 GMT"
},
{
"version": "v8",
"created": "Fri, 23 Jan 2009 07:16:53 GMT"
},
{
"version": "v9",
"created": "Wed, 4 Aug 2010 06:38:14 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Van Nieuwenhove",
"Rudi",
""
]
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712.1111 | Art B. Owen | Art B. Owen | The pigeonhole bootstrap | Published in at http://dx.doi.org/10.1214/07-AOAS122 the Annals of
Applied Statistics (http://www.imstat.org/aoas/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Statistics 2007, Vol. 1, No. 2, 386-411 | 10.1214/07-AOAS122 | IMS-AOAS-AOAS122 | stat.AP | null | Recently there has been much interest in data that, in statistical language,
may be described as having a large crossed and severely unbalanced random
effects structure. Such data sets arise for recommender engines and information
retrieval problems. Many large bipartite weighted graphs have this structure
too. We would like to assess the stability of algorithms fit to such data. Even
for linear statistics, a naive form of bootstrap sampling can be seriously
misleading and McCullagh [Bernoulli 6 (2000) 285--301] has shown that no
bootstrap method is exact. We show that an alternative bootstrap separately
resampling rows and columns of the data matrix satisfies a mean consistency
property even in heteroscedastic crossed unbalanced random effects models. This
alternative does not require the user to fit a crossed random effects model to
the data.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:45:24 GMT"
}
] | 2007-12-18T00:00:00 | [
[
"Owen",
"Art B.",
""
]
] | [
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712.1112 | Paolo Massarotti | F. Ambrosino, A. Antonelli, M. Antonelli, F. Archilli, C. Bacci, P.
Beltrame, G. Bencivenni, S. Bertolucci, C. Bini, C. Bloise, S. Bocchetta, F.
Bossi, P. Branchini, R. Caloi, P. Campana, G. Capon, T. Capussela, F.
Ceradini, S. Chi, G. Chiefari, P. Ciambrone, E. De Lucia, A. De Santis, P. De
Simone, G. De Zorzi, A. Denig, A. Di Domenico, C. Di Donato, B. Di Micco, A.
Doria, M. Dreucci, G. Felici, A. Ferrari, M. L. Ferrer, S. Fiore, C. Forti,
P. Franzini, C. Gatti, P. Gauzzi, S. Giovannella, E. Gorini, E. Graziani, W.
Kluge, V. Kulikov, F. Lacava, G. Lanfranchi, J. Lee-Franzini, D. Leone, M.
Martini, P. Massarotti, W. Mei, S. Meola, S. Miscetti, M. Moulson, S.
M\"uller, F. Murtas, M. Napolitano, F. Nguyen, M. Palutan, E. Pasqualucci, A.
Passeri, V. Patera, F. Perfetto, M. Primavera, P. Santangelo, G. Saracino, B.
Sciascia, A. Sciubba, A. Sibidanov, T. Spadaro, M. Testa, L. Tortora, P.
Valente, G. Venanzoni, R. Versaci, G. Xu | Measurement of the charged kaon lifetime with the KLOE detector | 13 pages, 14 figures | JHEP 0801:073,2008 | 10.1088/1126-6708/2008/01/073 | null | hep-ex | null | We have measured the charged kaon lifetime using a sample of 15 \times 10^6
tagged kaon decays. Charged kaons were produced in pairs at the DA\PhiNE
\phi-factory, e^+e^- \to \phi \to K^+ K^-. The decay of a K^+ was tagged by the
production of a K^- and viceversa. The lifetime was obtained, for both charges,
from independent measurements of the decay time and decay lenght distributions.
From fits to the four distributions we find \tau = (12.347\pm0.030) ns.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 10:59:00 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 17:46:21 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Ambrosino",
"F.",
""
],
[
"Antonelli",
"A.",
""
],
[
"Antonelli",
"M.",
""
],
[
"Archilli",
"F.",
""
],
[
"Bacci",
"C.",
""
],
[
"Beltrame",
"P.",
""
],
[
"Bencivenni",
"G.",
""
],
[
"Bertolucci",
"S.",
""
],
[
"Bini",
"C.",
""
],
[
"Bloise",
"C.",
""
],
[
"Bocchetta",
"S.",
""
],
[
"Bossi",
"F.",
""
],
[
"Branchini",
"P.",
""
],
[
"Caloi",
"R.",
""
],
[
"Campana",
"P.",
""
],
[
"Capon",
"G.",
""
],
[
"Capussela",
"T.",
""
],
[
"Ceradini",
"F.",
""
],
[
"Chi",
"S.",
""
],
[
"Chiefari",
"G.",
""
],
[
"Ciambrone",
"P.",
""
],
[
"De Lucia",
"E.",
""
],
[
"De Santis",
"A.",
""
],
[
"De Simone",
"P.",
""
],
[
"De Zorzi",
"G.",
""
],
[
"Denig",
"A.",
""
],
[
"Di Domenico",
"A.",
""
],
[
"Di Donato",
"C.",
""
],
[
"Di Micco",
"B.",
""
],
[
"Doria",
"A.",
""
],
[
"Dreucci",
"M.",
""
],
[
"Felici",
"G.",
""
],
[
"Ferrari",
"A.",
""
],
[
"Ferrer",
"M. L.",
""
],
[
"Fiore",
"S.",
""
],
[
"Forti",
"C.",
""
],
[
"Franzini",
"P.",
""
],
[
"Gatti",
"C.",
""
],
[
"Gauzzi",
"P.",
""
],
[
"Giovannella",
"S.",
""
],
[
"Gorini",
"E.",
""
],
[
"Graziani",
"E.",
""
],
[
"Kluge",
"W.",
""
],
[
"Kulikov",
"V.",
""
],
[
"Lacava",
"F.",
""
],
[
"Lanfranchi",
"G.",
""
],
[
"Lee-Franzini",
"J.",
""
],
[
"Leone",
"D.",
""
],
[
"Martini",
"M.",
""
],
[
"Massarotti",
"P.",
""
],
[
"Mei",
"W.",
""
],
[
"Meola",
"S.",
""
],
[
"Miscetti",
"S.",
""
],
[
"Moulson",
"M.",
""
],
[
"Müller",
"S.",
""
],
[
"Murtas",
"F.",
""
],
[
"Napolitano",
"M.",
""
],
[
"Nguyen",
"F.",
""
],
[
"Palutan",
"M.",
""
],
[
"Pasqualucci",
"E.",
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"A.",
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"V.",
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"F.",
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"M.",
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"P.",
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"G.",
""
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"B.",
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"A.",
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"A.",
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"T.",
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"M.",
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"L.",
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"P.",
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"G.",
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"R.",
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"G.",
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712.1113 | Laura Elisa Marcucci | L. E. Marcucci, L. Girlanda, A. Kievsky, S. Rosati, M. Viviani | Structure of A=3 Nuclear Systems Using Realistic Hamiltonians | 3 pages, 1 table, Proceedings of the 20th European Conference on
Few-Body Problems in Physics (EFB20), Pisa, September 2007 | Few Body Syst.44:207-209,2008 | 10.1007/s00601-008-0292-9 | null | nucl-th | null | The structure of A=3 low-energy scattering states is described using the
hyperspherical harmonics method with realistic Hamiltonian models, consisting
of two- and three-nucleon interactions. Both coordinate and momentum space
two-nucleon potential models are considered.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:19:47 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Marcucci",
"L. E.",
""
],
[
"Girlanda",
"L.",
""
],
[
"Kievsky",
"A.",
""
],
[
"Rosati",
"S.",
""
],
[
"Viviani",
"M.",
""
]
] | [
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712.1114 | Dariusz Chru\'sci\'nski | Dariusz Chruscinski and Andrzej Kossakowski | How to construct entanglement witnesses | 10 pages | J. Phys. A: Math. Theor. 41 (2008) 145301 | 10.1088/1751-8113/41/14/145301 | null | quant-ph | null | We present very simple method for constructing indecomposable entanglement
witnesses out of a given pair -- an entanglement witness W and the
corresponding state detected by W. This method may be used to produce new
classes of atomic witnesses which are able to detect the `weakest' quantum
entanglement. Actually, it works perfectly in the multipartite case, too.
Moreover, this method provides a powerful tool for constructing new examples of
bound entangled states.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:21:22 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Chruscinski",
"Dariusz",
""
],
[
"Kossakowski",
"Andrzej",
""
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] |
712.1115 | Pierre Patie | P. Patie | Law of the exponential functional of a new family of one-sided Levy
processes via self-similar continuous state branching processes with
immigration and the Wright hypergeometric functions | null | null | null | null | math.PR | null | We first introduce and derive some basic properties of a two-parameters
family of one-sided Levy processes. Their Laplace exponents are given in terms
of the Pochhammer symbol. This family includes, in a limit case, the family of
Brownian motion with drifts. Then, we proceed by computing the density of the
law of the exponential functional associated to some elements of this family
(and their dual) and some transformations of these elements. These densities
are expressed in terms of the Wright hypergeometric functions. By means of
probabilistic arguments, we derive some interesting properties enjoyed by these
functions. On the way we also characterize explicitly the density of the
semi-groups of the family of self-similar continuous state branching processes
with immigration.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:23:24 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Patie",
"P.",
""
]
] | [
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] |
712.1116 | Liuba Mazzanti | Liuba Mazzanti | Topics in noncommutative integrable theories and holographic brane-world
cosmology | Ph.D. Thesis, 256 pages, 6 figures, references added | null | null | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This thesis follows two main lines of research, both related to relevant
aspects of string theory and its phenomenological/cosmological applications. We
study two different generalizations of the integrable SG model to NC geometry,
after discussing general properties and issues of integrable theories and NC
field theories, mentioning their role in string theory. The question is whether
we can obtain an integrable NC SG with factorized S matrix. Of the two models
we study, the second NC SG -- derived by dimensional reduction from the stringy
NC self-dual YM in (2+2) dimensions -- exhibits the good properties of S matrix
required by integrability in 2D, while the first one does not. As a second
topic, a particular brane-world model is analyzed both from the cosmological
point of view and in the spirit of holography, after introducing conventional
cosmology, brane-worlds and AdS/CFT. The 7D RS set-up with brane-bulk energy
exchange we propose leads to a non conventional cosmological evolution where
all fixed points have positive acceleration and are found to be stable for a
wide range of choices for the parameters. We construct the holographic dual
theory, represented by a renormalized 6D CFT coupled to 6D gravity. The
matching of parameters on the two sides of the duality is then achieved in
specific approximations.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:27:00 GMT"
},
{
"version": "v2",
"created": "Wed, 6 Aug 2008 17:51:12 GMT"
}
] | 2008-08-06T00:00:00 | [
[
"Mazzanti",
"Liuba",
""
]
] | [
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] |
712.1117 | Christian Holm Christensen | Christian Holm Christensen, Jens Jorgen Gaardhoje, Kristjan
Gulbrandsen, Borge Svane Nielsen, Carsten Sogaard | The ALICE Forward Multiplicity Detector | Quark Matter 2006 poster proceeding, will be published in Int. J.
Mod. Phys. E | Int.J.Mod.Phys.E16:2432-2437,2007 | 10.1142/S0218301307008057 | null | nucl-ex | null | The ALICE Forward Multiplicity Detector (FMD) is a silicon strip detector
with 51,200 strips arranged in 5 rings, covering the range $-3.4 < \eta < 5.1$.
It is placed around the beam pipe at small angles to extend the charged
particle acceptance of ALICE into the forward regions, not covered by the
central barrel detectors.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:41:18 GMT"
}
] | 2010-11-26T00:00:00 | [
[
"Christensen",
"Christian Holm",
""
],
[
"Gaardhoje",
"Jens Jorgen",
""
],
[
"Gulbrandsen",
"Kristjan",
""
],
[
"Nielsen",
"Borge Svane",
""
],
[
"Sogaard",
"Carsten",
""
]
] | [
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] |
712.1118 | Oleg Verkhodanov | Pavel D. Naselsky (1), Per Rex Christensen (1), Peter Coles (2), Oleg
Verkhodanov (3), Dmitry Novikov (4,5), Jaiseung Kim (1) ((1) Niels Bohr
Institute, Copenhagen, Denmark, (2) School of Physics and Astronomy, Cardiff
University, Wales, United Kingdom, (3) Special astrophysical observatory,
Nizhnij Arkhyz, Russia, (4) Imperial College, London, United Kingdom, (5)
AstroSpace Center of Lebedev Physical Institute, Moscow, Russia) | Understanding the WMAP Cold Spot mystery | 35 pages, 17 figures | Astrophys. Bull. 65: 101-120,2010 | 10.1134/S199034131002001X | null | astro-ph astro-ph.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The first and third year data releases from the WMAP provide evidence of an
anomalous Cold Spot (CS) at galactic latitude b=-57deg and longitude l=209deg.
We have examined the properties of the CS in some detail in order to assess its
cosmological significance. We have performed a cluster analysis of the local
extrema in the CMB signal to show that the CS is actually associated with a
large group of extrema rather than just one. In the light of this we have
re-examined the properties of the WMAP ILC and co-added "cleaned" WCM maps,
which have previously been used for the analysis of the properties of the
signal in the vicinity of the CS. These two maps have remarkably similar
properties on equal latitude rings for |b|>30deg, as well as in the vicinity of
the CS. We have also checked the idea that the CMB signal has a non-Gaussian
tail, localized in the low multipole components of the signal. For each ring we
apply a linear filter with characteristic scale R, dividing the CMB signal in
two parts: the filtered part, with characteristic scale above that of the
filter R, and the difference between the initial and filtered signal. Using the
filter scale as a variable, we can maximize the skewness and kurtosis of the
smoothed signal and minimize these statistics for the difference between
initial and filtered signal. We have discovered that the shape of the CS is
formed primarily by the components of the CMB signal represented by multipoles
between 10<=L<=20, with a corresponding angular scale about 5-10 degs. This
signal leads to modulation of the whole CMB sky, clearly seen at |b|>30deg in
both the ILC and WCM maps, rather than a single localized feature. After
subtraction of this modulation, the remaining part of the CMB signal appears to
be consistent with statistical homogeneity and Gaussianity.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:41:24 GMT"
},
{
"version": "v2",
"created": "Sat, 29 Jan 2011 10:37:10 GMT"
}
] | 2011-02-02T00:00:00 | [
[
"Naselsky",
"Pavel D.",
""
],
[
"Christensen",
"Per Rex",
""
],
[
"Coles",
"Peter",
""
],
[
"Verkhodanov",
"Oleg",
""
],
[
"Novikov",
"Dmitry",
""
],
[
"Kim",
"Jaiseung",
""
]
] | [
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] |
712.1119 | Ignacio Gallo | Pierluigi Contucci, Ignacio Gallo, Stefano Ghirlanda | Equilibria of culture contact derived from ingroup and outgroup
attitudes | null | null | null | null | physics.soc-ph cond-mat.stat-mech math-ph math.MP | null | Modern societies feature an increasing contact between cultures, yet we have
a poor understanding of what the outcomes might be. Here we consider a
mathematical model of contact between social groups, grounded in social
psychology and analyzed using tools from statistical physics. We use the model
to study how a culture might be affected by immigration. We find that in some
cases residents' culture is relatively unchanged, but in other cases residents
may adopt the opinions and beliefs of immigrants. The decisive factors are each
group's cultural legacy and its attitudes towards in- and out-groups. The model
can also predict how social policies may influence the outcome of culture
contact.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 12:11:58 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Apr 2008 15:17:08 GMT"
}
] | 2008-04-29T00:00:00 | [
[
"Contucci",
"Pierluigi",
""
],
[
"Gallo",
"Ignacio",
""
],
[
"Ghirlanda",
"Stefano",
""
]
] | [
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] |
712.112 | Gert Aarts | Gert Aarts (Swansea University) and Anders Tranberg (University of
Oulu) | Thermal effects on slow-roll dynamics | 25 pages, 11 eps figures. v2: paper reorganized, title changed,
conclusions unchanged, to appear in PRD | Phys.Rev.D77:123521,2008 | 10.1103/PhysRevD.77.123521 | null | hep-ph astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A description of the transition from the inflationary epoch to radiation
domination requires the understanding of quantum fields out of thermal
equilibrium, particle creation and thermalisation. This can be studied from
first principles by solving a set of truncated real-time Schwinger-Dyson
equations, written in terms of the mean field (inflaton) and the field
propagators, derived from the two-particle irreducible effective action. We
investigate some aspects of this problem by considering the dynamics of a
slow-rolling mean field coupled to a second quantum field, using a \phi^2\chi^2
interaction. We focus on thermal effects. It is found that interactions lead to
an earlier end of slow-roll and that the evolution afterwards depends on
details of the heatbath.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:49:39 GMT"
},
{
"version": "v2",
"created": "Fri, 13 Jun 2008 08:42:09 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Aarts",
"Gert",
"",
"Swansea University"
],
[
"Tranberg",
"Anders",
"",
"University of\n Oulu"
]
] | [
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] |
712.1121 | D. S. Berman | David S. Berman and Daniel C. Thompson | Duality Symmetric Strings, Dilatons and O(d,d) Effective Actions | 15 pages, latex; v2 reference added, typos fixed | Phys.Lett.B662:279-284,2008 | 10.1016/j.physletb.2008.03.012 | QMUL-PH-07-25 | hep-th | null | We calculate the background field equations for the T-duality symmetric
string building on previous work by including the effect of the Dilaton up to
two-loops. Inclusion of the Dilaton allows us to obtain the full beta
functionals of the duality symmetric sigma model. We are able to interpret the
result in terms of a dimensionally reduced O(d,d) invariant target space
effective action.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:51:07 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Dec 2007 12:47:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Berman",
"David S.",
""
],
[
"Thompson",
"Daniel C.",
""
]
] | [
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712.1122 | Michal Dovciak | M. Dovciak, V. Karas, G. Matt, R. W. Goosmann | Variation in the primary and reprocessed radiation from an orbiting spot
around a black hole | 10 pages, 9 figures, accepted by MNRAS | MNRAS, 384, 2008, p. 361-369 | 10.1111/j.1365-2966.2007.12713.x | null | astro-ph | null | We study light curves and spectra (equivalent widths of the iron line and
some other spectral characteristics) which arise by reflection on the surface
of an accretion disc, following its illumination by a primary off-axis source -
an X-ray 'flare', assumed to be a point-like source just above the accretion
disc resulting in a spot with radius dr/r<1. We consider General Relativity
effects (energy shifts, light bending, time delays) near a rotating black hole,
and we find them all important, including the light bending and delay
amplification due to the spot motion. For some sets of parameters the reflected
flux exceeds the flux from the primary component. We show that the
orbit-induced variations of the equivalent width with respect to its mean value
can be as high as 30% for the observer's inclination of 30 degrees, and much
more at higher inclinations. We calculate the ratio of the reflected flux to
the primary flux and the hardness ratio which we find to vary significantly
with the spot phase mainly for small orbital radii. This offers the chance to
estimate the lower limit of the black hole spin if the flare arises close to
the black hole.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 11:56:26 GMT"
}
] | 2008-02-29T00:00:00 | [
[
"Dovciak",
"M.",
""
],
[
"Karas",
"V.",
""
],
[
"Matt",
"G.",
""
],
[
"Goosmann",
"R. W.",
""
]
] | [
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] |
712.1123 | Daniel Wilczak | Daniel Wilczak, Piotr Zgliczynski | Period doubling in the Rossler system - a computer assisted proof | 39 pages, 3 figures | null | null | null | math.DS math.NA | null | The goal of this paper is to show how to produce a piece of rigorous
bifurcation diagram of periodic orbits for an ODE. We study the Rossler system,
one of the textbook examples of ODEs generating nontrivial dynamics, for the
parameter range containing two period doubling bifurcations.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 12:00:12 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Wilczak",
"Daniel",
""
],
[
"Zgliczynski",
"Piotr",
""
]
] | [
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] |
712.1124 | Haiyan Wu | Haiyan Wu, Ming Yuan, Susan M. Kaech, M. Elizabeth Halloran | A statistical analysis of memory CD8 T cell differentiation: An
application of a hierarchical state space model to a short time course
microarray experiment | Published in at http://dx.doi.org/10.1214/07-AOAS118 the Annals of
Applied Statistics (http://www.imstat.org/aoas/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Statistics 2007, Vol. 1, No. 2, 442-458 | 10.1214/07-AOAS118 | IMS-AOAS-AOAS118 | stat.AP | null | CD8 T cells are specialized immune cells that play an important role in the
regulation of antiviral immune response and the generation of protective
immunity. In this paper we investigate the differentiation of memory CD8 T
cells in the immune response using a short time course microarray experiment.
Structurally, this experiment is similar to many in that it involves
measurements taken on independent samples, in one biological group, at a small
number of irregularly spaced time points, and exhibiting patterns of temporal
nonstationarity. To analyze this CD8 T-cell experiment, we develop a
hierarchical state space model so that we can: (1) detect temporally
differentially expressed genes, (2) identify the direction of successive
changes over time, and (3) assess the magnitude of successive changes over
time. We incorporate hidden Markov models into our model to utilize the
information embedded in the time series and set up the proposed hierarchical
state space model in an empirical Bayes framework to utilize the population
information from the large-scale data. Analysis of the CD8 T-cell experiment
using the proposed model results in biologically meaningful findings. Temporal
patterns involved in the differentiation of memory CD8 T cells are summarized
separately and performance of the proposed model is illustrated in a simulation
study.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 12:25:08 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Wu",
"Haiyan",
""
],
[
"Yuan",
"Ming",
""
],
[
"Kaech",
"Susan M.",
""
],
[
"Halloran",
"M. Elizabeth",
""
]
] | [
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] |
712.1125 | Michal Dovciak | M. Dovciak, V. Karas, G. Matt, R. W. Goosmann | Variation of the primary and reprocessed radiation in the flare-spot
model | 15 pages, 10 figures, accepted to the Proceedings of RAGtime 8/9:
Workshops on black holes and neutron stars, Opava, 15-19/19-21 September,
2006/2007, Eds.: S. Hledik, Z. Stuchlik, Silesian University in Opava, Czech
republic, 2007 | Proceedings of RAGtime 8/9: Workshops on black holes and neutron
stars, Eds.: S. Hledik & Z. Stuchlik, Opava: Silesian University, 2007, ISBN
978-80-7248-419-5, p. 45-59 | null | null | astro-ph | null | We study light curves and spectra (equivalent widths of the iron line and
some other spectral characteristics) which arise by reprocessing on the surface
of an accretion disc, following its illumination by a primary off-axis source -
an X-ray 'flare', assumed to be a point-like source just above the accretion
disc. We consider all general relativity effects (energy shifts, light bending,
time delays, delay amplification due to the spot motion) near a rotating black
hole. For some sets of parameters the reflected flux exceeds the flux from the
primary component. We show that the orbit-induced variations of the equivalent
width with respect to its mean value can be as high as 30% for an observer's
inclination of 30 degrees, and much more at higher inclinations. We calculate
the ratio of the reflected flux to the primary flux and the hardness ratio
which we find to vary significantly with the spot phase mainly for small
orbital radii. This offers the chance to estimate the lower limit of the black
hole spin if the flare arises close to the black hole. We show the results for
different values of the flare orbital radius.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 12:33:29 GMT"
}
] | 2008-02-29T00:00:00 | [
[
"Dovciak",
"M.",
""
],
[
"Karas",
"V.",
""
],
[
"Matt",
"G.",
""
],
[
"Goosmann",
"R. W.",
""
]
] | [
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] |
712.1126 | Ricard Sole | Ricard V. Sole | Consciousness, brains and the replica problem | 4 pages, 1 figure, preprint | null | null | null | nlin.AO q-bio.NC | null | Although the conscious state is considered an emergent property of the
underlying brain activity and thus somehow resides on brain hardware, there is
a non-univocal mapping between both. Given a neural hardware, multiple
conscious patterns are consistent with it. Here we show, by means of a simple
{\em gedankenexperiment} that this has an important logic consequence: any
scenario involving the transient shutdown of brain activity leads to the
irreversible death of the conscious experience. In a fundamental way, unless
the continuous stream of consciousness is guaranteed, the previous self
vanishes and is replaced by a new one.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 12:27:38 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Sole",
"Ricard V.",
""
]
] | [
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712.1127 | Filipe Veloso | J. Carvalho, N. Castro, L. Chikovani, T. Djobava, J. Dodd, S. McGrath,
A. Onofre, J. Parsons, F. Veloso | Study of ATLAS sensitivity to FCNC top decays | null | Eur.Phys.J.C52:999-1019,2007 | 10.1140/epjc/s10052-007-0434-0 | SN-ATLAS-2007-059 | hep-ex | null | The ATLAS experiment sensitivity to top quark Flavour Changing Neutral
Current (FCNC) decays was studied at LHC using ttbar events. While one of the
top quarks is expected to follow the dominant Standard Model decay t->bW, the
other decays through a FCNC channel, i.e. t-> Z u(c), t-> gamma u(c) or t-> g
u(c). Different types of analyses, applied to each FCNC decay mode, were
compared. The FCNC branching ratio sensitivity (assuming a 5sigma signal
significance) and 95% confidence level limits on the branching ratios (in the
hypothesis of signal absence) were obtained.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:19:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Carvalho",
"J.",
""
],
[
"Castro",
"N.",
""
],
[
"Chikovani",
"L.",
""
],
[
"Djobava",
"T.",
""
],
[
"Dodd",
"J.",
""
],
[
"McGrath",
"S.",
""
],
[
"Onofre",
"A.",
""
],
[
"Parsons",
"J.",
""
],
[
"Veloso",
"F.",
""
]
] | [
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712.1128 | Helge Maakestad Dr. | Helge {\O}ystein Maakestad | On operations and characteristic classes | 21 pages | null | null | null | math.KT math.RT | http://creativecommons.org/licenses/by-nc-sa/4.0/ | In this paper exterior products are used to define operations and
characteristic classes with values in the K-theory of an abelian category with
tensor and exterior products. We apply the general construction to define Chern
and Segre classes with values in algebraic K-theory and the K-theory of
connections.
| [
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] | 2020-11-13T00:00:00 | [
[
"Maakestad",
"Helge Øystein",
""
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] |
712.1129 | D. N. Basu | D.N. Basu and Tapan Mukhopadhyay | Relativistic kinematics for reactions involving massless particles | 3 pages; http://physics.unipune.ernet.in/~phyed/26.3.html | Phys.Educ.26:199-203,2009 | null | null | nucl-th nucl-ex | null | Some useful kinematical relations for the absorption of a photon by a nucleus
and its recoil are derived for the relativistic incident energies. These
expressions provided for the relativistic kinematics of photoabsorption
reactions, though simple, will be immensely useful for experimentalists as well
as theoreticians.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:40:09 GMT"
}
] | 2009-10-19T00:00:00 | [
[
"Basu",
"D. N.",
""
],
[
"Mukhopadhyay",
"Tapan",
""
]
] | [
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] |
712.113 | Stefano Liberati | Carlos Barcelo, Stefano Liberati, Sebastiano Sonego, Matt Visser | Fate of gravitational collapse in semiclassical gravity | revtex4, 14 pages, 2 figures | Phys.Rev.D77:044032,2008 | 10.1103/PhysRevD.77.044032 | null | gr-qc hep-th | null | While the outcome of gravitational collapse in classical general relativity
is unquestionably a black hole, up to now no full and complete semiclassical
description of black hole formation has been thoroughly investigated. Here we
revisit the standard scenario for this process. By analyzing how semiclassical
collapse proceeds we show that the very formation of a trapping horizon can be
seriously questioned for a large set of, possibly realistic, scenarios. We
emphasise that in principle the theoretical framework of semiclassical gravity
certainly allows the formation of trapping horizons. What we are questioning
here is the more subtle point of whether or not the standard black hole picture
is appropriate for describing the end point of realistic collapse. Indeed if
semiclassical physics were in some cases to prevent formation of the trapping
horizon, then this suggests the possibility of new collapsed objects which can
be much less problematic, making it unnecessary to confront the information
paradox or the run-away end point problem.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:00:28 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Barcelo",
"Carlos",
""
],
[
"Liberati",
"Stefano",
""
],
[
"Sonego",
"Sebastiano",
""
],
[
"Visser",
"Matt",
""
]
] | [
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] |
712.1131 | Jakub J{\ke}drak | Jakub J\c{e}drak | On some mathematical identities resulting from evaluation of the
partition function for an electron moving in a periodic lattice | 27 pages | null | null | null | math-ph math.MP | null | We consider a simple model of the dynamics of a single electron in a crystal
lattice. Although this is a standard problem in condensed matter physics,
alternative ways of evaluating a partition function for such a system lead to
equalities, that may be interesting from the point of view of mathematical
analysis, combinatorics and graph theory.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:08:55 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Jȩdrak",
"Jakub",
""
]
] | [
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] |
712.1132 | Filippo Frontera | F. Frontera, G. Loffredo, A. Pisa, L. Milani, F. Nobili, N. Auricchio,
V. Carassiti, F. Evangelisti, L. Landi, S. Squerzanti, K.H. Andersen, P.
Courtois, L. Amati, E. Caroli, G. Landini, S. Silvestri, J.B. Stephen, J. M.
Poulsen, B. Negri, G. Pareschi | Development status of a Laue lens project for gamma-ray astronomy | 11 pages, 11 figures, 2007 SPIE Conference on Optics for EUV, X-Ray,
and Gamma-Ray Astronomy III | Proc.SPIE Int.Soc.Opt.Eng.6688:66880N,2007 | 10.1117/12.736038 | null | astro-ph | null | We report the status of the HAXTEL project, devoted to perform a design study
and the development of a Laue lens prototype. After a summary of the major
results of the design study, the approach adopted to develop a Demonstration
Model of a Laue lens is discussed, the set up described, and some results
presented.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:10:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Frontera",
"F.",
""
],
[
"Loffredo",
"G.",
""
],
[
"Pisa",
"A.",
""
],
[
"Milani",
"L.",
""
],
[
"Nobili",
"F.",
""
],
[
"Auricchio",
"N.",
""
],
[
"Carassiti",
"V.",
""
],
[
"Evangelisti",
"F.",
""
],
[
"Landi",
"L.",
""
],
[
"Squerzanti",
"S.",
""
],
[
"Andersen",
"K. H.",
""
],
[
"Courtois",
"P.",
""
],
[
"Amati",
"L.",
""
],
[
"Caroli",
"E.",
""
],
[
"Landini",
"G.",
""
],
[
"Silvestri",
"S.",
""
],
[
"Stephen",
"J. B.",
""
],
[
"Poulsen",
"J. M.",
""
],
[
"Negri",
"B.",
""
],
[
"Pareschi",
"G.",
""
]
] | [
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] |
712.1133 | Gabi Ben Simon | Gabi Ben Simon, Dietmar A. Salamon | Homogeneous quasimorphisms on the symplectic linear group | null | null | null | null | math.SG | null | In this note, we show a uniqueness result of homogeneous quasimorphisms
defined on the universal cover of the symplectic linear group.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:15:49 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 23:01:57 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Simon",
"Gabi Ben",
""
],
[
"Salamon",
"Dietmar A.",
""
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] | [
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] |
712.1134 | Achille A. Nucita | A.A.Nucita, F. De Paolis, G. Ingrosso, S. Carpano, and M. Guainazzi | The globular cluster NGC 6388: $XMM$-Newton and $Chandra$ observations | accepted on A&A, some references modified | null | null | null | astro-ph | null | By studying the optical brightness surface density of the globular cluster
NGC 6388, it has been recently proposed that it harbors a central
intermediate-mass black hole with mass $\simeq 5.7\times 10^3$ M$_{\odot}$. We
expect that the compact object in the center of NGC 6388 emits radiation in the
$X$-ray band as a consequence of the accretion from the surrounding matter. We
searched for $XMM$-Newton and $Chandra$ observations towards NGC 6388 to test
this hypothesis. The $Chandra$ satellite disentangles several point-like
$X$-ray sources, probably low mass $X$-ray binaries, well within the core
radius of the globular cluster. However, three of them, coinciding with the
cluster center of gravity, remain unresolved. Their total luminosity is
$L_X^{Obs}\simeq 2.7\times 10^{33}$ erg s$^{-1}$. If one of these sources is
the $X$-ray counterpart of the intermediate-mass black hole in NGC 6388, the
corresponding upper limit on the accretion efficiency, with respect to the
Eddington luminosity, is $3\times 10^{-9}$. This measurement could be tightened
if moderately deep radio observations of the field were performed.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:21:10 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Dec 2007 09:49:58 GMT"
}
] | 2007-12-17T00:00:00 | [
[
"Nucita",
"A. A.",
""
],
[
"De Paolis",
"F.",
""
],
[
"Ingrosso",
"G.",
""
],
[
"Carpano",
"S.",
""
],
[
"Guainazzi",
"M.",
""
]
] | [
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] |
712.1135 | Murach Aleksandr | Vladimir A. Mikhailets, Alexandr A. Murach | Interpolation with a function parameter and refined scale of spaces | null | Methods Funct. Anal. Topology, 14 (2008), no. 1, 81--100. | null | null | math.AP | null | The interpolation of couples of separable Hilbert spaces with a function
parameter is studied. The main properties of the classic interpolation are
proved. Some applications to the interpolation of isotropic H\"ormander spaces
over a closed manifold are given.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:27:36 GMT"
}
] | 2009-03-30T00:00:00 | [
[
"Mikhailets",
"Vladimir A.",
""
],
[
"Murach",
"Alexandr A.",
""
]
] | [
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] |
712.1136 | Peter Koroteev | Peter Koroteev, Maxim Libanov | On Existence of Self-Tuning Solutions in Static Braneworlds without
Singularities | 11 pages, JHEP style, minor corrections, metric with Lifshitz scaling
added | JHEP 0802:104,2008 | 10.1088/1126-6708/2008/02/104 | ITEP-TH-60/07, ULB-TH/07-34 | hep-th gr-qc hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A static self-tuning SO(3)xZ_2 symmetric and translation invariant braneworld
setup with flat brane is considered. We discuss the null energy conditions
(NEC) for matter on the brane and in the bulk and prove that for the static
regular background with broken Lorentz invariance the NEC and positiveness of
the total energy density on the brane and NEC in the bulk cannot be satisfied
simultaneously. Then we give some examples and elaborate some special cases.
For instance, we provide a macroscopic solution for a background with Lifshitz
scaling.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:56:57 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jul 2008 14:13:33 GMT"
},
{
"version": "v3",
"created": "Mon, 14 Dec 2009 16:32:45 GMT"
}
] | 2009-12-17T00:00:00 | [
[
"Koroteev",
"Peter",
""
],
[
"Libanov",
"Maxim",
""
]
] | [
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] |
712.1137 | Sergio Pastor | Andreu Esteban-Pretel, Sergio Pastor, Ricard Tomas, Georg G. Raffelt,
Gunter Sigl | Mu-tau neutrino refraction and collective three-flavor transformations
in supernovae | 9 pages, 7 figures. New presentation of results, version to be
published in PRD | Phys.Rev.D77:065024,2008 | 10.1103/PhysRevD.77.065024 | MPP-2007-178, IFIC/07-69 | astro-ph hep-ph | null | We study three-flavor collective neutrino transformations in the
dense-neutrino region above the neutrino sphere of a supernova core. We find
that two-flavor conversions driven by the atmospheric mass difference and the
13-mixing angle capture the full effect if one neglects the second-order
difference between the muon and tau neutrino refractive index. Including this
"mu-tau matter term" provides a resonance at a density of approximately 3 x
10^7 g cm^-3 that typically causes significant modifications of the overall
electron neutrino and antineutrino survival probabilities. This effect is
surprisingly sensitive to deviations from maximal 23-mixing, being different
for each octant.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:38:27 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Mar 2008 16:37:09 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Esteban-Pretel",
"Andreu",
""
],
[
"Pastor",
"Sergio",
""
],
[
"Tomas",
"Ricard",
""
],
[
"Raffelt",
"Georg G.",
""
],
[
"Sigl",
"Gunter",
""
]
] | [
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] |
712.1138 | Mathieu Puech | M. Puech, F. Hammer, H. Flores, Y. Yang, and B. Neichel | IMAGES: a unique view of the galaxy mass assembly since z=1 | 5 pages, 2 figures, proceeding of the meeting "Science with the VLT
in the ELT era", held in garching, 8-12 Oct 2007 | null | null | null | astro-ph | null | The Large Program IMAGES is near 2/3 of its completion. It provides us with
kinematics (GIRAFFE deployable IFUs), gas chemistry (FORS2), detailed
morphologies (HST/ACS) and IR photometry (Spitzer) for a set of 70 galaxies
representative of intermediate mass galaxies (MJ<=-20.3 or 1.5e10 Mo) at
z=0.4-0.75. We discover that, 6 Gyr ago, a significant fraction of galaxies
(>40%) had anomalous kinematics, i.e. kinematics significantly discrepant from
those of rotational or dispersion supported galaxies. The anomalous kinematics
cause the observed large dispersion of the Tully-Fisher relation at large
distances. IMAGES will soon allow us to study distant galaxies at a level of
detail almost comparable to that of nearby galaxies.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:42:56 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Puech",
"M.",
""
],
[
"Hammer",
"F.",
""
],
[
"Flores",
"H.",
""
],
[
"Yang",
"Y.",
""
],
[
"Neichel",
"B.",
""
]
] | [
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] |
712.1139 | Anthony Coolen | A. Mozeika and A. C. C. Coolen | Dynamical replica analysis of processes on finitely connected random
graphs I: vertex covering | 26 pages LaTeX, 5 figures | null | 10.1088/1751-8113/41/11/115003 | null | cond-mat.dis-nn | null | We study the stochastic dynamics of Ising spin models with random bonds,
interacting on finitely connected Poissonnian random graphs. We use the
dynamical replica method to derive closed dynamical equations for the joint
spin-field probability distribution, and solve these within the replica
symmetry ansatz. Although the theory is developed in a general setting, with a
view to future applications in various other fields, in this paper we apply it
mainly to the dynamics of the Glauber algorithm (extended with cooling
schedules) when running on the so-called vertex cover optimization problem. Our
theoretical predictions are tested against both Monte Carlo simulations and
known results from equilibrium studies. In contrast to previous dynamical
analyses based on deriving closed equations for only a small numbers of scalar
order parameters, the agreement between theory and experiment in the present
study is nearly perfect.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:44:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mozeika",
"A.",
""
],
[
"Coolen",
"A. C. C.",
""
]
] | [
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] |
712.114 | Timoteo Carletti | Gani Aldashev and Timoteo Carletti | Benefits of Diversity, Communication Costs, and Public Opinion Dynamics | 23 pages, 11 figures, 2 tables | null | null | null | physics.soc-ph | null | We study the dynamics of public opinion in a model in which agents change
their opinions as a result of random binary encounters if the opinion
difference is below their individual thresholds that evolve over time. We
ground these thresholds in a simple individual cost-benefit analysis with
linear benefits of diversity and quadratic communication costs. We clarify and
deepen the results of earlier continuous-opinion dynamics models (Deffuant et
al., Adv Complex Systems 2000; Weisbuch et al., Complexity 2002) and establish
several new results regarding the patterns of opinions in the asymptotic state
and the cluster formation time.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:46:35 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Aldashev",
"Gani",
""
],
[
"Carletti",
"Timoteo",
""
]
] | [
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712.1141 | Enrico Barausse | E. Barausse, T. P. Sotiriou and J. C. Miller | Curvature singularities, tidal forces and the viability of Palatini f(R)
gravity | 15 pages. CQG in press. Part of the material moved to an appendix,
discussion on the meV scale predictions of Palatini f(R) gravity added | Class.Quant.Grav.25:105008,2008 | 10.1088/0264-9381/25/10/105008 | null | gr-qc astro-ph hep-ph | null | In a previous paper we showed that static spherically symmetric objects
which, in the vicinity of their surface, are well-described by a polytropic
equation of state with 3/2<Gamma<2 exhibit a curvature singularity in Palatini
f(R) gravity. We argued that this casts serious doubt on the validity of
Palatini f(R) gravity as a viable alternative to General Relativity. In the
present paper we further investigate this characteristic of Palatini f(R)
gravity in order to clarify its physical interpretation and consequences.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 19:55:14 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Apr 2008 08:20:23 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Barausse",
"E.",
""
],
[
"Sotiriou",
"T. P.",
""
],
[
"Miller",
"J. C.",
""
]
] | [
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] |
712.1142 | Lars Hellstr\"om | Lars Hellstr\"om | A Generic Framework for Diamond Lemmas | 74 pages. Includes index | null | null | null | math.RA | null | This paper gives a generic form of the diamond lemma, which includes support
for additive and topological structures of the base set, and which does not
require any further structure (e.g. an associative multiplication operation) to
be present. This result is intended to be used as the core of diamond lemmas
for particular algebraic structures, taking care of all the common
technicalities. With this generic diamond lemma, the main steps needed to prove
a specialised diamond lemma is to define the reduction maps and analyse the
structure of critical ambiguities.
The abstract machinery is backed up with concrete suggestions for how one
should set things up in order to reproduce traditional results in the general
setting. Several instances of the fundamental theorem of Groebner basis theory
are derived as corollaries of the main result.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:51:34 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Hellström",
"Lars",
""
]
] | [
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-0.0209779609,
-0.0103631373,
-0.031863343,
-0.0308062658,
-0.1248358488
] |
712.1143 | Xia Wan | BES Collaboration: M. Ablikim, et al | Observation of Y(2175) in $J/\psi\to \eta\phi f_0(980)$ | 5 pages, 4 figures, accepted by Phys. Rev. Lett | Phys.Rev.Lett.100:102003,2008 | 10.1103/PhysRevLett.100.102003 | null | hep-ex | null | The decays of $J/\psi\to \eta\phi f_0(980) (\eta\to \gamma\gamma, \phi \to
K^+K^-, f_0(980)\to\pi^+\pi^-)$ are analyzed using a sample of $5.8 \times
10^{7}$ $J/\psi$ events collected with the BESII detector at the Beijing
Electron-Positron Collider (BEPC). A structure at around $2.18 $GeV/$c^2$ with
about $5\sigma$ significance is observed in the $\phi f_0(980)$ invariant mass
spectrum. A fit with a Breit-Wigner function gives the peak mass and width of
$m=2.186\pm 0.010 (stat)\pm 0.006 (syst) $GeV/$c^2$ and $\Gamma=0.065\pm 0.023
(stat)\pm 0.017 (syst) $GeV/$c^2$, respectively, that are consistent with those
of Y(2175), observed by the BABAR collaboration in the initial-state radiation
(ISR) process $e^+e^-\to\gamma_{ISR}\phi f_0(980)$. The production branching
ratio is determined to be $Br(J/\psi\to\eta Y(2175))\cdot Br(Y(2175)\to\phi
f_0(980))\cdot Br(f_0(980)\to\pi^+\pi^-)=(3.23\pm 0.75 (stat)\pm0.73
(syst))\times 10^{-4}$, assuming that the Y(2175) is a $1^{--}$ state.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 13:57:08 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Jan 2008 09:04:23 GMT"
},
{
"version": "v3",
"created": "Fri, 4 Jan 2008 21:41:54 GMT"
},
{
"version": "v4",
"created": "Tue, 5 Feb 2008 20:05:14 GMT"
},
{
"version": "v5",
"created": "Tue, 11 Mar 2008 09:18:07 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"BES Collaboration",
"",
""
],
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"Ablikim",
"M.",
""
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] | [
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712.1144 | Bence Kocsis | Bence Kocsis (Harvard), Zoltan Haiman (Columbia), Kristen Menou
(Columbia) | Pre-Merger Localization of Gravitational-Wave Standard Sirens With LISA:
Triggered Search for an Electromagnetic Counterpart | 17 pages, 9 figures, submitted to ApJ | Astrophys.J. 684 (2008) 870-888 | 10.1086/590230 | null | astro-ph gr-qc | null | Electromagnetic (EM) counterparts to supermassive black hole binary mergers
observed by LISA can be localized to within the field of view of astronomical
instruments ~10 deg^2 hours to weeks prior to coalescence. The temporal
coincidence of any prompt EM counterpart with a gravitationally-timed merger
may offer the best chance of identifying a unique host galaxy. We discuss the
challenges posed by searches for prompt EM counterparts and propose novel
observational strategies to address them. In particular, we discuss the size
and shape evolution of the LISA localization error ellipses on the sky, and
quantify the requirements for dedicated EM surveys of the area prior to
coalescence. A triggered EM counterpart search campaign will require monitoring
a several-square degree area. It could aim for variability at the 24-27 mag
level in optical bands, for example, which corresponds to 1-10% of the
Eddington luminosity of the prime LISA sources of 10^6-10^7 Msun BHs at z=1-2,
on time-scales of minutes to hours, the orbital time-scale of the binary in the
last 2-4 weeks. A cross-correlation of the period of any variable EM signal
with the quasi-periodic gravitational waveform over 10-1000 cycles may aid the
detection. Alternatively, EM searches can detect a transient signal
accompanying the coalescence. We highlight the measurement of differences in
the arrival times of photons and gravitons from the same cosmological source as
a valuable independent test of the massive character of gravity, and of
possible violations of Lorentz invariance in the gravity sector.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 20:59:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kocsis",
"Bence",
"",
"Harvard"
],
[
"Haiman",
"Zoltan",
"",
"Columbia"
],
[
"Menou",
"Kristen",
"",
"Columbia"
]
] | [
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712.1145 | Anupreeta More | A. More, J. P. McKean, T. W. B. Muxlow, R. W. Porcas, C. D. Fassnacht
and L. V. E. Koopmans | Probing a massive radio galaxy with gravitational lensing | 11 pages, 7 figures, 4 tables, MNRAS accepted | null | 10.1111/j.1365-2966.2007.12831.x | null | astro-ph | null | The gravitational lens system CLASS B2108+213 has two lensed images separated
by 4.56 arcsec. Such a wide image separation suggests that the lens is either a
massive galaxy, or is composed of a group of galaxies. To investigate the
structure of the lensing potential we have carried out new high resolution
imaging of the two lensed images at 1.7 GHz with the VLBA and at 5 GHz with
global VLBI. Compact and extended emission is detected from the two lensed
images, which provides additional constraints to the lensing mass model. We
find that the data are consistent with either a single lensing galaxy, or a two
galaxy lens model that takes account of a nearby companion to the main lensing
galaxy within the Einstein radius of the system. However, for an ensemble of
global power-law mass models, those with density profiles steeper than
isothermal are a better fit. The best-fitting profile for a single spherical
mass model has a slope of $\gamma=$~2.45$_{-0.18}^{+0.19}$. The system also has
a third radio component which is coincident with the main lensing galaxy. This
component is detected at milli-arcsecond scales for the first time by the 1.7
GHz VLBA and 5 GHz global VLBI imaging. However, the third radio component is
found not to be consistent with a core lensed image because the radio spectrum
differs from the two lensed images, and its flux-density is too high when
compared to what is expected from simple mass models with a variable power-law
density profile and/or a reasonable core radius. Furthermore, 1.4 GHz imaging
of the system with the MERLIN finds extended lobe emission on either side of
the main lensing galaxy. Therefore, the radio emission from the third radio
component is almost certainly from an AGN within the main lensing galaxy, which
is classified as an FR I type radio source.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:01:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"More",
"A.",
""
],
[
"McKean",
"J. P.",
""
],
[
"Muxlow",
"T. W. B.",
""
],
[
"Porcas",
"R. W.",
""
],
[
"Fassnacht",
"C. D.",
""
],
[
"Koopmans",
"L. V. E.",
""
]
] | [
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712.1146 | Jon Urrestilla | Jon Urrestilla and Alexander Vilenkin | Evolution of cosmic superstring networks: a numerical simulation | 16 pages, 13 figures; Minor changes; Matches published version | JHEP0802:037,2008 | 10.1088/1126-6708/2008/02/037 | null | hep-th astro-ph | null | We study the formation and evolution of an interconnected string network in
large-scale field-theory numerical simulations, both in flat spacetime and in
expanding universe. The network consists of gauge U(1) strings of two different
kinds and their bound states, arising due to an attractive interaction
potential. We find that the network shows no tendency to ``freeze'' and appears
to approach a scaling regime, with all characteristic lengths growing linearly
with time. Bound strings constitute only a small fraction of the total string
length in the network.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:10:41 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Feb 2008 13:57:05 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Urrestilla",
"Jon",
""
],
[
"Vilenkin",
"Alexander",
""
]
] | [
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] |
712.1147 | Markus Risse | The Pierre Auger Collaboration | Upper limit on the cosmic-ray photon flux above 10^19 eV using the
surface detector of the Pierre Auger Observatory | 28 pages, 9 figures; v2: minor modifications; accepted by Astropart.
Phys | Astropart.Phys.29:243-256,2008 | 10.1016/j.astropartphys.2008.01.003 | null | astro-ph hep-ph | null | A method is developed to search for air showers initiated by photons using
data recorded by the surface detector of the Auger Observatory. The approach is
based on observables sensitive to the longitudinal shower development, the
signal risetime and the curvature of the shower front. Applying this method to
the data, upper limits on the flux of photons of 3.8*10^-3, 2.5*10^-3, and
2.2*10^-3 km^-2 sr^-1 yr^-1 above 10^19 eV, 2*10^19 eV, and 4*10^19 eV are
derived, with corresponding limits on the fraction of photons being 2.0%, 5.1%,
and 31% (all limits at 95% c.l.). These photon limits disfavor certain exotic
models of sources of cosmic rays. The results also show that the approach
adopted by the Auger Observatory to calibrate the shower energy is not strongly
biased by a contamination from photons.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:10:42 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Jan 2008 11:27:04 GMT"
}
] | 2012-08-27T00:00:00 | [
[
"The Pierre Auger Collaboration",
"",
""
]
] | [
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712.1148 | Amit Pratap Yadav | Amit P. S. Yadav and Benjamin D. Wandelt | Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at
above 99.5% confidence | 4 pages, 2 figures, 1 tables, submitted to PRL, references added. New
version has several additional tests and systematic error estimates. Results
largely unchanged | Phys.Rev.Lett.100:181301,2008 | 10.1103/PhysRevLett.100.181301 | null | astro-ph | null | We present evidence for the detection of primordial non-Gaussianity of the
local type (fNL), using the temperature information of the Cosmic Microwave
Background (CMB) from the WMAP 3-year data. We employ the bispectrum estimator
of non-Gaussianity described in (Yadav et al. 2007) which allows us to analyze
the entirety of the WMAP data without an arbitrary cut-off in angular scale.
Using the combined information from WMAP's two main science channels up to
lmax=750 and the conservative Kp0 foreground mask we find 27 < fNL < 147 at 95%
C.L., with a central value of fNL=87. This corresponds to a rejection of fNL=0
at more than 99.5% significance. We find that this detection is robust to
variations in lmax, frequency and masks, and that no known foreground,
instrument systematic, or secondary anisotropy explains our signal while
passing our suite of tests. We explore the impact of several analysis choices
on the stated significance and find 2.5 sigma for the most conservative view.
We conclude that the WMAP 3-year data disfavors canonical single field
slow-roll inflation.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:51:14 GMT"
},
{
"version": "v2",
"created": "Sun, 9 Dec 2007 20:57:19 GMT"
},
{
"version": "v3",
"created": "Wed, 5 Mar 2008 20:46:53 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Yadav",
"Amit P. S.",
""
],
[
"Wandelt",
"Benjamin D.",
""
]
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] |
712.1149 | Anatoly Zasov V. | A. V. Zasov, O. V. Abramova | Midplane Gas Density and the Schmidt Law | 2 pages, 2 figures, proceeding of the poster presented at the Vatican
Conf. "Formation and evolution of galaxy disks" held in Rome, 1-5 Oct. 2007 | null | null | null | astro-ph | null | The thickness of isothermal gaseous layers and their midplane volume
densities \rho_{gas}(R) were calculated for several spiral and LSB galaxies by
solving the self-consistent equilibrium equations for gaseous discs embedded
into a stellar one. The self-gravity of the gas and influence of dark halo on
the disk thickness were taken into account. The resulting midplane volume
densities of spiral galaxies were compared with the azimuthally averaged star
formation rate SFR to verify the feasibility and universality of the Schmidt
law SFR ~ \rho_{gas}^n.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:16:19 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Zasov",
"A. V.",
""
],
[
"Abramova",
"O. V.",
""
]
] | [
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] |
712.115 | Nazirah Jetha | Nazirah N. Jetha (1 and 2), Martin J. Hardcastle (3), Arif Babul (4),
Ewan O'Sullivan (5), Trevor J. Ponman (2), Somak Raychaudhury (2), and Jan
Vrtilek (5) ((1) CEA-Saclay France, (2) University of Birmingham UK, (3)
University of Hertfordshire UK, (4) University of Victoria Canada, (5)
Harvard-Smithsonian Center for Astrophysics USA) | The nature of the ghost cavity in the NGC 741 group | 11 pages, 6 figures, accepted 7/12/07 MNRAS | null | 10.1111/j.1365-2966.2007.12829.x | null | astro-ph | null | We discuss the effects of energy injection into the intra-group medium of the
group of galaxies associated with NGC 741. The X-ray emission reveals a large
bubble, which in the absence of a currently bright central radio source, may
have been inflated by a previous cycle of nuclear activity . If the bubble is
filled with a light, relativistic fluid we calculate that in expanding, it has
done more than sufficient work to counteract the energy lost from the
intra-group medium via radiative cooling; the bubble can provide this energy as
it expands and rises. Using upper limits on the flux density of the plasma
filling the bubble at 330 MHz and 1.4 GHz, we derive constraints on its
electron energy distribution and magnetic field strength. We show that the data
require the high-energy cut-off of the electron spectrum to be very low
compared to the cut-offs seen in more typical radio sources if the fluid
filling the bubble is a conventional relativistic plasma. This suggests that
the fluid filling the bubble may not have evolved by expansion or synchrotron
losses consistent with a dead radio source, leaving a puzzle as to what the
origin of the bubble may be.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:21:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jetha",
"Nazirah N.",
"",
"1 and 2"
],
[
"Hardcastle",
"Martin J.",
""
],
[
"Babul",
"Arif",
""
],
[
"O'Sullivan",
"Ewan",
""
],
[
"Ponman",
"Trevor J.",
""
],
[
"Raychaudhury",
"Somak",
""
],
[
"Vrtilek",
"Jan",
""
]
] | [
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] |
712.1151 | Alexander Kobushkin | A.P.Kobushkin and Ya.D.Krivenko-Emetov | Effect of the Coulomb interaction in A(d,p) fragmentation | 6 pages, 3 figures | null | null | null | nucl-th | null | In the framework of Glauber-Sitenko model we calculate contribution of
Coulomb interaction in cross-section of A(d,p) reaction at high energy and zero
angle. It is demonstrated that such effect significantly increases the
differential cross section only at peak, where the proton momentum $p$ is near
half of the deuteron momentum $p_d$ in lab. frame, $p \sim \frac12 p_d$. The
Coulomb interaction do not change the results in the high momentum region,
where quark effects should be taken into account.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:53:25 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Kobushkin",
"A. P.",
""
],
[
"Krivenko-Emetov",
"Ya. D.",
""
]
] | [
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712.1152 | Roman Taranets | Roman Taranets, Yuliya Namlyeyeva | Euler equation for incompressible non-Newtonian fluids: finite speed of
propagations and asymptotic behavior of weak solutions | null | null | null | null | math.AP | null | We investigate multidimensional model for incompressible non-Newtonian
fluids. Using method of energy estimates we prove the property of finite speed
of propagations of the solution support for this problem. We find sharp bounds
of the propagations by $L^2$--norm and $L^1$--norm of initial data.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:41:36 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Taranets",
"Roman",
""
],
[
"Namlyeyeva",
"Yuliya",
""
]
] | [
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] |
712.1153 | Keiya Shirahama | Keiya Shirahama, Keiichi Yamamoto, Yoshiyuki Shibayama | Superfluidity of $^4$He Confined in Nano-Porous Media | 6 Pages, 6 Figures, Submitted to "Helium: 100 years", Special Issue
of Low Temperature Physics | null | 10.1063/1.2908885 | null | cond-mat.mes-hall cond-mat.str-el | null | We have examined superfluid properties of $^4$He confined to a nano-porous
Gelsil glass that has nanopores 2.5 nm in diameter. The pressure-temperature
phase diagram was determined by torsional oscillator, heat capacity and
pressure studies. The superfluid transition temperature $T_{\mathrm c}$
approaches zero at 3.4 MPa, indicating a novel "quantum" superfluid transition.
By heat capacity measurements, the nonsuperfluid phase adjacent to the
superfluid and solid phases is identified to be a nanometer-scale, localized
Bose condensation state, in which global phase coherence is destroyed. At high
pressures, the superfluid density has a $T$-linear term, and $T_{\mathrm c}$ is
proportional to the zero-temperature superfluid density. These results strongly
suggest that phase fluctuations in the superfluid order parameter play a
dominant role on the phase diagram and superfluid properties.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 14:52:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shirahama",
"Keiya",
""
],
[
"Yamamoto",
"Keiichi",
""
],
[
"Shibayama",
"Yoshiyuki",
""
]
] | [
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0.0124879023,
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] |
712.1154 | Denis Ullmo | Denis Ullmo | Many-Body Physics and Quantum Chaos | To appear in Rep. Prog. Phys | Rep. Prog. Phys. 71 (2008) 026001 | 10.1088/0034-4885/71/2/026001 | null | cond-mat.mes-hall | null | Experimental progresses in the miniaturisation of electronic devices have
made routinely available in the laboratory small electronic systems, on the
micron or sub-micron scale, which at low temperature are sufficiently well
isolated from their environment to be considered as fully coherent. Some of
their most important properties are dominated by the interaction between
electrons. Understanding their behaviour therefore requires a description of
the interplay between interference effects and interactions.
The goal of this review is to address this relatively broad issue, and more
specifically to address it from the perspective of the quantum chaos community.
I will therefore present some of the concepts developed in the field of quantum
chaos which have some application to study many-body effects in mesoscopic and
nanoscopic systems. Their implementation is illustrated on a few examples of
experimental relevance such as persistent currents, mesoscopic fluctuations of
Kondo properties or Coulomb blockade. I will furthermore try to bring out, from
the various physical illustrations, some of the specific advantages on more
general grounds of the quantum chaos based approach.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:09:38 GMT"
}
] | 2008-02-06T00:00:00 | [
[
"Ullmo",
"Denis",
""
]
] | [
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] |
712.1155 | Ariel Goobar | Serena Nobili, Ariel Goobar | The colour-lightcurve shape relation of Type Ia supernovae and the
reddening law | Major revision of the text. Accepted for publication in A&A | null | 10.1051/0004-6361:20079292 | null | astro-ph | null | A study of the time sequence of optical colours of a large sample of nearby
Type Ia supernovae (SNe Ia) is presented. We study the dependence of the colour
time evolution with respect to the lightcurve shape, parametrized by the
stretch factor. We fit the spectral template that minimizes the colour
dispersion in SNe Ia, as measured through UBVRI photometry of near-by
supernovae. A clear colour dependence upon lightcurve shape is found, with the
narrower lightcurves being redder up to about one month past lightcurve
maximum. We also derive an average reddening law, after correcting for
lightcurve shape differences in intrinsic colour, that is well described by a
Cardelli, Clayton & Mathis law with R_V=1.75 \pm 0.27 for 80 Type Ia supernovae
with E(B-V) < 0.7 mag. A subset sample including 69 SNe with modest reddening,
E(B-V)<0.25 mag, yields a significantly smaller value, R_V ~ 1, suggesting that
the observed reddening of Type Ia supernovae may have a more complex origin,
perhaps involving other processes beside extinction by interstellar dust in the
host galaxy.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:13:24 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Apr 2008 11:11:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nobili",
"Serena",
""
],
[
"Goobar",
"Ariel",
""
]
] | [
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] |
712.1156 | Adri\'an Rodr\'iguez | Sylvio Ferraz-Mello (1), Adri\'an Rodr\'iguez (1), Hauke Hussmann (2)
((1) Instituto de Astronomia Geof\'isica e Ci\^encias Atmosf\'ericas.
Universidade de S\~ao Paulo, Brasil, (2) Institut f\"ur Planetenforschung,
DLR, Berlin-Adlershof, Germany) | Tidal friction in close-in satellites and exoplanets. The Darwin theory
re-visited | 30 pages, 7 figures, corrected typos | Celest.Mech.Dyn.Astron.101:171-197,2008 | 10.1007/s10569-008-9133-x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This report is a review of Darwin's classical theory of bodily tides in which
we present the analytical expressions for the orbital and rotational evolution
of the bodies and for the energy dissipation rates due to their tidal
interaction. General formulas are given which do not depend on any assumption
linking the tidal lags to the frequencies of the corresponding tidal waves
(except that equal frequency harmonics are assumed to span equal lags).
Emphasis is given to the cases of companions having reached one of the two
possible final states: (1) the super-synchronous stationary rotation resulting
from the vanishing of the average tidal torque; (2) the capture into a 1:1
spin-orbit resonance (true synchronization). In these cases, the energy
dissipation is controlled by the tidal harmonic with period equal to the
orbital period (instead of the semi-diurnal tide) and the singularity due to
the vanishing of the geometric phase lag does not exist. It is also shown that
the true synchronization with non-zero eccentricity is only possible if an
extra torque exists opposite to the tidal torque. The theory is developed
assuming that this additional torque is produced by an equatorial permanent
asymmetry in the companion. The results are model-dependent and the theory is
developed only to the second degree in eccentricity and inclination
(obliquity). It can easily be extended to higher orders, but formal accuracy
will not be a real improvement as long as the physics of the processes leading
to tidal lags is not better known.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:12:39 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 18:56:52 GMT"
},
{
"version": "v3",
"created": "Mon, 27 Apr 2009 12:55:05 GMT"
}
] | 2009-06-19T00:00:00 | [
[
"Ferraz-Mello",
"Sylvio",
""
],
[
"Rodríguez",
"Adrián",
""
],
[
"Hussmann",
"Hauke",
""
]
] | [
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] |
712.1157 | Jean-Marc Bardet | Jean-Marc Bardet (CES, Matisse, Samos), Imen Kammoun (CES, Matisse,
Samos) | Detecting changes in the fluctuations of a Gaussian process and an
application to heartbeat time series | null | null | null | null | math.ST stat.TH | null | The aim of this paper is first the detection of multiple abrupt changes of
the long-range dependence (respectively self-similarity, local fractality)
parameters from a sample of a Gaussian stationary times series (respectively
time series, continuous-time process having stationary increments). The
estimator of the $m$ change instants (the number $m$ is supposed to be known)
is proved to satisfied a limit theorem with an explicit convergence rate.
Moreover, a central limit theorem is established for an estimator of each
long-range dependence (respectively self-similarity, local fractality)
parameter. Finally, a goodness-of-fit test is also built in each time domain
without change and proved to asymptotically follow a Khi-square distribution.
Such statistics are applied to heart rate data of marathon's runners and lead
to interesting conclusions.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:19:36 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Bardet",
"Jean-Marc",
"",
"CES, Matisse, Samos"
],
[
"Kammoun",
"Imen",
"",
"CES, Matisse,\n Samos"
]
] | [
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] |
712.1158 | Ruslan Sepkhanov | R. A. Sepkhanov and C. W. J. Beenakker | Numerical test of the theory of pseudo-diffusive transmission at the
Dirac point of a photonic band structure | 4 pages, 7 figures. Figure added | Opt. Commun. 281, 5267 (2008) | 10.1016/j.optcom.2008.07.017 | null | physics.optics cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | It has recently been predicted that a conical singularity (= Dirac point) in
the band structure of a photonic crystal produces an unusual 1/L scaling of the
photon flux transmitted through a slab of thickness L. This inverse-linear
scaling is unusual, because it is characteristic of radiative transport via
diffusion modes through a disordered medium -- while here it appears for
propagation of Bloch modes in an ideal crystal without any disorder. We present
a quantitative numerical test of the predicted scaling, by calculating the
scattering of transverse-electric (TE) modes by a two-dimensional triangular
lattice of dielectric rods in air. We verify the 1/L scaling and show that the
slope differs by less than 10% from the value predicted for maximal coupling of
the Bloch modes in the photonic crystal to the plane waves in free space.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:23:03 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Dec 2007 21:49:13 GMT"
},
{
"version": "v3",
"created": "Fri, 11 Jul 2008 12:39:26 GMT"
}
] | 2008-09-04T00:00:00 | [
[
"Sepkhanov",
"R. A.",
""
],
[
"Beenakker",
"C. W. J.",
""
]
] | [
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] |
712.1159 | Marco Pierleoni | M. Pierleoni, A. Maselli, B. Ciardi | CRASH_alpha: coupling continuum and line radiative transfer | 13 pages, 8 figures. Submitted to MNRAS | null | null | null | astro-ph | null | In this paper we present CRASH_alpha, the first radiative transfer code for
cosmological application that follows the parallel propagation of Ly_alpha and
ionizing photons. CRASH_alpha is a version of the continuum radiative transfer
code CRASH with a new algorithm to follow the propagation of Ly_alpha photons
through a gas configuration whose ionization structure is evolving. The
implementation introduces the time evolution for Ly_alpha photons (a feature
commonly neglected in line radiative transfer codes) and, to reduce the
computational time needed to follow each scattering, adopts a statistical
approach to the Ly_alpha treatment by making extensive use of pre-compiled
tables. With this statistical approach we experience a drastic increase of the
computational speed and, at the same time, an excellent agreement with the full
Ly_alpha radiative transfer computations of the code MCLy_alpha. We find that
the emerging spectra keep memory of the ionization history which generates a
given ionization configuration of the gas and, to properly account for this
effect, a self-consistent joint evolution of line and ionizing continuum
radiation as implemented in CRASH_alpha is necessary. A comparison between the
results from our code and from Ly_alpha scattering alone on a fixed HI density
field shows that the extent of the difference between the emerging spectra
depends on the particular configuration considered, but it can be substantial
and can thus affect the physical interpretation of the problem at hand. These
differences should furthermore be taken into account when computing the impact
of the Ly_alpha radiation on e.g. the observability of the 21 cm line from
neutral hydrogen at epochs preceeding complete reionization.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:43:24 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Pierleoni",
"M.",
""
],
[
"Maselli",
"A.",
""
],
[
"Ciardi",
"B.",
""
]
] | [
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] |
712.116 | Ho Bun Lau | H.B. Lau, R.J. Stancliffe and C.A. Tout | An Explosive End to Intermediate-Mass Zero-Metallicity Stars and Early
Universe Nucleosynthesis | 18 pages, 6 figures, 2 tables, accepted for MNRAS | null | 10.1111/j.1365-2966.2007.12816.x | null | astro-ph | null | We use the Cambridge stellar evolution code STARS to model the evolution of
5-7 solar mass zero-metallicity stars. With enhanced resolution at the hydrogen
and helium burning shell in the AGB phases, we are able to model the entire
thermally pulsing asymptotic giant branch (TP-AGB) phase. The helium
luminosities of the thermal pulses are significantly lower than in higher
metallicity stars so there is no third dredge-up. The envelope is enriched in
nitrogen by hot-bottom burning of carbon that was previously mixed in during
second dredge-up. There is no s-process enrichment owing to the lack of third
dredge up. The thermal pulses grow weaker as the core mass increases and they
eventually cease. From then on the star enters a quiescent burning phase which
lasts until carbon ignites at the centre of the star when the CO core mass is
1.36 solar mass. With such a high degeneracy and a core mass so close to the
Chandrasekhar mass, we expect these stars to explode as type 1.5 supernovae,
very similar to Type Ia supernovae but inside a hydrogen rich envelope.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:43:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lau",
"H. B.",
""
],
[
"Stancliffe",
"R. J.",
""
],
[
"Tout",
"C. A.",
""
]
] | [
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712.1161 | Gennady Lykasov I | Alexander P. Ierusalimov (1), Gennady I. Lykasov (1) and Michele
Viviani (2) ((1) JINR, Dubna, (2) INFN, Sezione di Pisa) | Spin effects in elastic backward P-D scattering | 4 pages, 4 figures. Talk given at XII International Workshop on High
Energy Spin Physics, Dubna, September 3-7, 2007. Talk given at the 20th
European Conference on Few-Body Problems in Physics, Pisa, Italy, September
10-14, 2007 | null | null | null | nucl-th | null | The elastic backward proton-deuteron scattering is analyzed including both
relativistic effects in the deuteron and the reaction mechanism. It is shown
that inclusion of the graphs corresponding to the emission, rescattering and
absorption of the virtual pion by a deuteron nucleon in addition to the
one-nucleon exchange graph allows a rather satisfactory description of all the
experimental data on the differential cross section, tensor analyzing power of
the deuteron and transfer polarization in this reaction.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 17:59:42 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Dec 2007 08:58:44 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Ierusalimov",
"Alexander P.",
"",
"JINR, Dubna"
],
[
"Lykasov",
"Gennady I.",
"",
"JINR, Dubna"
],
[
"Viviani",
"Michele",
"",
"INFN, Sezione di Pisa"
]
] | [
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] |
712.1162 | Lam Hui | Lam Hui and Kyle P. Parfrey (Columbia University) | The Evolution of Bias - Generalized | 8 pages, 2 figures. References added. Accepted for publication in
Physical Review D | Phys.Rev.D77:043527,2008 | 10.1103/PhysRevD.77.043527 | null | astro-ph | null | Fry (1996) showed that galaxy bias has the tendency to evolve towards unity,
i.e. in the long run, the galaxy distribution tends to trace that of matter.
Generalizing slightly Fry's reasoning, we show that his conclusion remains
valid in theories of modified gravity (or equivalently, complex clustered dark
energy). This is not surprising: as long as both galaxies and matter are
subject to the same force, dynamics would drive them towards tracing each
other. This holds, for instance, in theories where both galaxies and matter
move on geodesics. This relaxation of bias towards unity is tempered by cosmic
acceleration, however: the bias tends towards unity but does not quite make it,
unless the formation bias were close to unity. Our argument is extended in a
straightforward manner to the case of a stochastic or nonlinear bias. An
important corollary is that dynamical evolution could imprint a scale
dependence on the large scale galaxy bias. This is especially pronounced if
non-standard gravity introduces new scales to the problem: the bias at
different scales relaxes at different rates, the larger scales generally more
slowly and retaining a longer memory of the initial bias. A consistency test of
the current (general relativity + uniform dark energy) paradigm is therefore to
look for departure from a scale independent bias on large scales. A simple way
is to measure the relative bias of different populations of galaxies which are
at different stages of bias relaxation. Lastly, we comment on the possibility
of directly testing the Poisson equation on cosmological scales, as opposed to
indirectly through the growth factor.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:47:26 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 18:58:16 GMT"
},
{
"version": "v3",
"created": "Fri, 25 Jan 2008 22:22:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hui",
"Lam",
"",
"Columbia University"
],
[
"Parfrey",
"Kyle P.",
"",
"Columbia University"
]
] | [
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] |
712.1163 | Philipp Schuetz | Philipp Schuetz and Amedeo Caflisch | Efficient modularity optimization by multistep greedy algorithm and
vertex mover refinement | 7 pages, parts of text rewritten, illustrations and pseudocode
representation of algorithms added | Phys. Rev. E 77,046112 (2008) | 10.1103/PhysRevE.77.046112 | null | cs.DS cond-mat.dis-nn cs.DM physics.soc-ph | null | Identifying strongly connected substructures in large networks provides
insight into their coarse-grained organization. Several approaches based on the
optimization of a quality function, e.g., the modularity, have been proposed.
We present here a multistep extension of the greedy algorithm (MSG) that allows
the merging of more than one pair of communities at each iteration step. The
essential idea is to prevent the premature condensation into few large
communities. Upon convergence of the MSG a simple refinement procedure called
"vertex mover" (VM) is used for reassigning vertices to neighboring communities
to improve the final modularity value. With an appropriate choice of the step
width, the combined MSG-VM algorithm is able to find solutions of higher
modularity than those reported previously. The multistep extension does not
alter the scaling of computational cost of the greedy algorithm.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:48:31 GMT"
},
{
"version": "v2",
"created": "Fri, 2 May 2008 10:16:35 GMT"
}
] | 2008-05-02T00:00:00 | [
[
"Schuetz",
"Philipp",
""
],
[
"Caflisch",
"Amedeo",
""
]
] | [
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] |
712.1164 | Ville Lahtinen Mr. | Ville Lahtinen, Graham Kells, Angelo Carollo, Tim Stitt, Jiri Vala,
Jiannis K. Pachos | Spectrum of the non-abelian phase in Kitaev's honeycomb lattice model | 32 pages, 13 figures; corrected typos and changed SU(2)_2 to Ising | Ann. Phys. 323, 2286 (2008) | 10.1016/j.aop.2007.12.009 | null | cond-mat.mes-hall cond-mat.str-el quant-ph | null | The spectral properties of Kitaev's honeycomb lattice model are investigated
both analytically and numerically with the focus on the non-abelian phase of
the model. After summarizing the fermionization technique which maps spins into
free Majorana fermions, we evaluate the spectrum of sparse vortex
configurations and derive the interaction between two vortices as a function of
their separation. We consider the effect vortices can have on the fermionic
spectrum as well as on the phase transition between the abelian and non-abelian
phases. We explicitly demonstrate the $2^n$-fold ground state degeneracy in the
presence of $2n$ well separated vortices and the lifting of the degeneracy due
to their short-range interactions. The calculations are performed on an
infinite lattice. In addition to the analytic treatment, a numerical study of
finite size systems is performed which is in exact agreement with the
theoretical considerations. The general spectral properties of the non-abelian
phase are considered for various finite toroidal systems.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:58:34 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Dec 2007 16:07:48 GMT"
},
{
"version": "v3",
"created": "Mon, 14 Apr 2008 19:41:34 GMT"
}
] | 2010-07-02T00:00:00 | [
[
"Lahtinen",
"Ville",
""
],
[
"Kells",
"Graham",
""
],
[
"Carollo",
"Angelo",
""
],
[
"Stitt",
"Tim",
""
],
[
"Vala",
"Jiri",
""
],
[
"Pachos",
"Jiannis K.",
""
]
] | [
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0.1213165298,
0.011209175,
0.0408679023,
0.0137097873,
0.0047464692,
-0.0667723566,
0.018838387,
0.0548927784,
0.0269636977,
-0.0454802886,
-0.0057688369,
-0.1277524233,
-0.0487250499,
-0.0353973955,
-0.0619454421,
-0.028103387,
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] |
712.1165 | Martin Weigt | Michele Leone, Sumedha, Martin Weigt | Unsupervised and semi-supervised clustering by message passing:
Soft-constraint affinity propagation | 11 pages, 13 pdf figures, to app. in EPJB | Eur. Phys. J. B (2008), published online 8 Oct. 2008 | 10.1140/epjb/e2008-00381-8 | null | physics.data-an cond-mat.stat-mech q-bio.QM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Soft-constraint affinity propagation (SCAP) is a new statistical-physics
based clustering technique. First we give the derivation of a simplified
version of the algorithm and discuss possibilities of time- and
memory-efficient implementations. Later we give a detailed analysis of the
performance of SCAP on artificial data, showing that the algorithm efficiently
unveils clustered and hierarchical data structures. We generalize the algorithm
to the problem of semi-supervised clustering, where data are already partially
labeled, and clustering assigns labels to previously unlabeled points. SCAP
uses both the geometrical organization of the data and the available labels
assigned to few points in a computationally efficient way, as is shown on
artificial and biological benchmark data.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:54:55 GMT"
},
{
"version": "v2",
"created": "Mon, 15 Sep 2008 14:50:02 GMT"
}
] | 2008-10-20T00:00:00 | [
[
"Leone",
"Michele",
""
],
[
"Sumedha",
"",
""
],
[
"Weigt",
"Martin",
""
]
] | [
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712.1166 | Michael Galperin | Michael Galperin and Sergei Tretiak | Linear optical response of current-carrying molecular junction: A
NEGF-TDDFT approach | 10 pages | J. Chem. Phys. 128, 124705 (2008) | 10.1063/1.2876011 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | We propose a scheme for calculation of linear optical response of
current-carrying molecular junctions for the case when electronic tunneling
through the junction is much faster than characteristic time of external laser
field. We discuss relationships between nonequilibrium Green function (NEGF)
and time-dependent density functional theory (TDDFT) approaches, and derive
expressions for optical response and linear polarizability within NEGF-TDDFT
scheme. Corresponding results for isolated molecule, derived within TDDFT
approach previously, are reproduced when coupling to contacts is neglected.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:56:09 GMT"
}
] | 2008-04-07T00:00:00 | [
[
"Galperin",
"Michael",
""
],
[
"Tretiak",
"Sergei",
""
]
] | [
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] |
712.1167 | Felipe Fran\c{c}a | Leandro A. J. Marzulo, Felipe M. G. Fran\c{c}a and V\'itor Santos
Costa | Transactional WaveCache: Towards Speculative and Out-of-Order DataFlow
Execution of Memory Operations | Submitted to ACM International Conference on Computing Frontiers
2008, http://www.computingfrontiers.org/, 20 pages | null | null | null | cs.AR cs.DC | null | The WaveScalar is the first DataFlow Architecture that can efficiently
provide the sequential memory semantics required by imperative languages. This
work presents an alternative memory ordering mechanism for this architecture,
the Transaction WaveCache. Our mechanism maintains the execution order of
memory operations within blocks of code, called Waves, but adds the ability to
speculatively execute, out-of-order, operations from different waves. This
ordering mechanism is inspired by progress in supporting Transactional
Memories. Waves are considered as atomic regions and executed as nested
transactions. If a wave has finished the execution of all its memory
operations, as soon as the previous waves are committed, it can be committed.
If a hazard is detected in a speculative Wave, all the following Waves
(children) are aborted and re-executed. We evaluate the WaveCache on a set
artificial benchmarks. If the benchmark does not access memory often, we could
achieve speedups of around 90%. Speedups of 33.1% and 24% were observed on more
memory intensive applications, and slowdowns up to 16% arise if memory
bandwidth is a bottleneck. For an application full of WAW, WAR and RAW hazards,
a speedup of 139.7% was verified.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 15:59:37 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Marzulo",
"Leandro A. J.",
""
],
[
"França",
"Felipe M. G.",
""
],
[
"Costa",
"Vítor Santos",
""
]
] | [
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] |
712.1168 | Aram Mekjian | Aram Z. Mekjian | Properties of baryonic, electric and strangeness chemical potentials and
some of their consequences in relativistic heavy ion collisions | null | Phys.Lett.B651:33-38,2007 | 10.1016/j.physletb.2007.05.061 | null | nucl-th | null | Analytic expressions are given for the baryonic, electric and strangeness
chemical potentials which explicitly show the importance of various terms.
Simple scaling relations connecting these chemical potentials are found.
Applications to particle ratios and to fluctuations and related thermal
properties such as the isothermal compressibility kappaT are illustrated. A
possible divergence of kappaT is discussed.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:02:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mekjian",
"Aram Z.",
""
]
] | [
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] |
712.1169 | Shengshan Cui | Shengshan Cui, Alexander M. Haimovich, Oren Somekh and H. Vincent Poor | Opportunistic Relaying in Wireless Networks | 17 pages, 8 figures, To appear in IEEE Transactions on Information
Theory | null | 10.1109/TIT.2009.2030435 | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Relay networks having $n$ source-to-destination pairs and $m$ half-duplex
relays, all operating in the same frequency band in the presence of block
fading, are analyzed. This setup has attracted significant attention and
several relaying protocols have been reported in the literature. However, most
of the proposed solutions require either centrally coordinated scheduling or
detailed channel state information (CSI) at the transmitter side. Here, an
opportunistic relaying scheme is proposed, which alleviates these limitations.
The scheme entails a two-hop communication protocol, in which sources
communicate with destinations only through half-duplex relays. The key idea is
to schedule at each hop only a subset of nodes that can benefit from
\emph{multiuser diversity}. To select the source and destination nodes for each
hop, it requires only CSI at receivers (relays for the first hop, and
destination nodes for the second hop) and an integer-value CSI feedback to the
transmitters. For the case when $n$ is large and $m$ is fixed, it is shown that
the proposed scheme achieves a system throughput of $m/2$ bits/s/Hz. In
contrast, the information-theoretic upper bound of $(m/2)\log \log n$ bits/s/Hz
is achievable only with more demanding CSI assumptions and cooperation between
the relays. Furthermore, it is shown that, under the condition that the product
of block duration and system bandwidth scales faster than $\log n$, the
achievable throughput of the proposed scheme scales as $\Theta ({\log n})$.
Notably, this is proven to be the optimal throughput scaling even if
centralized scheduling is allowed, thus proving the optimality of the proposed
scheme in the scaling law sense.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:19:52 GMT"
},
{
"version": "v2",
"created": "Wed, 7 Jan 2009 07:17:19 GMT"
},
{
"version": "v3",
"created": "Fri, 24 Jul 2009 06:06:23 GMT"
}
] | 2016-11-15T00:00:00 | [
[
"Cui",
"Shengshan",
""
],
[
"Haimovich",
"Alexander M.",
""
],
[
"Somekh",
"Oren",
""
],
[
"Poor",
"H. Vincent",
""
]
] | [
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] |
712.117 | Nicolas Ruty | Nicolas Ruty (GIPSA-lab), Annemie Van Hirtum (GIPSA-lab), Xavier
Pelorson (GIPSA-lab), Avraham Hirschberg, Ines Lopez-Arteaga | A preliminary study of asymmetric vocal fold vibrations: modeling and
"in-vitro" validation | null | Dans Proceeding of the International Seminar on Speech Production
- 7TH International Seminar on Speech Production, Ubatuba : Br\'esil (2006) | null | null | physics.class-ph | null | This paper deals with some of aspects of the influence of asymmetry on vocal
folds vibrations. A theoretical model of vocal fold asymmetry is presented. The
influence of asymmetry is quantitatively examined in terms of oscillation
frequency and pressure threshold. The theoretical model is compared to
"in-vitro" experiment on a deformable replica of vocal folds. It is found that
asymmetry strongly influences the oscillation subglottal pressure threshold.
Moreover, the vocal fold with the highest mechanical resonance frequency
imposes the oscillation fundamental frequency. The influence of geometrical
asymmetry instead of purely mechanical asymmetry is shown
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:02:38 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Ruty",
"Nicolas",
"",
"GIPSA-lab"
],
[
"Van Hirtum",
"Annemie",
"",
"GIPSA-lab"
],
[
"Pelorson",
"Xavier",
"",
"GIPSA-lab"
],
[
"Hirschberg",
"Avraham",
""
],
[
"Lopez-Arteaga",
"Ines",
""
]
] | [
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] |
712.1171 | Arnaud Le Ny | Arnaud Le Ny | Introduction to (generalized) Gibbs measures | 95 pages | null | null | null | math.PR | null | These notes have been written to complete a mini-course "Introduction to
(generalized) Gibbs measures" given at the universities UFMG (Universidade
Federal de Minas Gerais, Belo Horizonte, Brasil) and UFRGS (Universidade
Federal do Rio Grande do Sul, Porto Alegre, Brasil) during the first semester
2007. The main goal of the lectures was to describe Gibbs and generalized Gibbs
measures on lattices at a rigorous mathematical level, as equilibirum states of
systems of a huge number of particles in interaction. In particular, our main
message is that although the historical approach based on potentials has been
rather successful from a physical point of view, one has to insist on (almost
sure) continuity properties of conditional probabilities to get a proper
mathematical framework.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:03:26 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Ny",
"Arnaud Le",
""
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712.1172 | Jean-Philippe Chancelier | Jean-Philippe Chancelier (CERMICS) | Iterative schemes for computing fixed points of nonexpansive mappings in
Banach spaces | null | null | null | null | math.OC | null | Let $X$ be a real Banach space with a normalized duality mapping uniformly
norm-to-weak$^\star$ continuous on bounded sets or a reflexive Banach space
which admits a weakly continuous duality mapping $J_{\Phi}$ with gauge $\phi$.
Let $f$ be an {\em $\alpha$-contraction} and $\{T_n\}$ a sequence of
nonexpansive mapping, we study the strong convergence of explicit iterative
schemes
x_{n+1} = \alpha_n f(x_n) + (1-\alpha_n) T_n x_n
with a general theorem and then recover and improve some specific cases
studied in the literature
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:04:33 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Chancelier",
"Jean-Philippe",
"",
"CERMICS"
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712.1173 | Karl Kosack | HESS Collaboration: F. Aharonian, et al | HESS VHE Gamma-Ray Sources Without Identified Counterparts | null | null | 10.1051/0004-6361:20078516 | null | astro-ph | null | The detection of gamma rays in the very-high-energy (VHE) energy range (100
GeV--100 TeV) provides a direct view of the parent population of
ultra-relativistic particles found in astrophysical sources. For this reason,
VHE gamma rays are useful for understanding the underlying astrophysical
processes in non-thermal sources. We investigate unidentified VHE gamma-ray
sources that have been discovered with HESS in the most sensitive blind survey
of the Galactic plane at VHE energies conducted so far. The HESS array of
imaging atmospheric Cherenkov telescopes (IACTs) has a high sensitivity
compared with previous instruments(~ 0.01 Crab) in 25 hours observation time
for a 5 sigma point-source detection), and with its large field of view, is
well suited for scan-based observations. The on-going HESS survey of the inner
Galaxy has revealed a large number of new VHE sources, and for each we attempt
to associate the VHE emission with multi-wavelength data in the radio through
X-ray wavebands. For each of the eight unidentified VHE sources considered
here, we present the energy spectra and sky maps of the sources and their
environment. The VHE morphology is compared with available multi-wavelength
data (mainly radio and X-rays). No plausible counterparts are found.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:14:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"HESS Collaboration",
"",
""
],
[
"Aharonian",
"F.",
""
]
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] |
712.1174 | Marcelino Agundez | M. Agundez, J. Cernicharo, M. Guelin, M. Gerin, M. C. McCarthy and P.
Thaddeus | Search for anions in molecular sources: C4H- detection in L1527 | 4 pages, 1 figure; accepted for A&A Letters | null | 10.1051/0004-6361:20078985 | null | astro-ph | null | We present the results of a search for the negative ion C4H- in various dark
clouds, low mass star-forming regions and photon-dominated regions (PDRs). We
have also searched for C6H-, C2H- and CN- in some of the sources. The
millimeter-wave observations were carried out with the IRAM-30m telescope. We
detect C4H-, through the J = 9-8 and J = 10-9 rotational transitions, in the
low mass star-forming region L1527. We thus confirm the tentative detection of
the J = 9-8 line recently reported toward this source. The [C4H-]/[C4H] ratio
found is 0.011 %, which is slightly lower than the value observed in IRC
+10216, 0.024 %, but above the 3 sigma upper limit we derive in TMC-1, < 0.0052
%. We have also derived an upper limit for the [C6H-]/[C6H] ratio in the
Horsehead Nebula, and for various anion-to-neutral ratios in the observed
sources. These results are compared with recent chemical models.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:16:59 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 11:30:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Agundez",
"M.",
""
],
[
"Cernicharo",
"J.",
""
],
[
"Guelin",
"M.",
""
],
[
"Gerin",
"M.",
""
],
[
"McCarthy",
"M. C.",
""
],
[
"Thaddeus",
"P.",
""
]
] | [
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] |
712.1175 | Pamela Morehouse | CLEO Collaboration: K. M. Ecklund, et al | Measurement of the Absolute Branching Fraction of D_s^+ --> tau^+ nu_tau
Decay | 9 pages, postscript also available through
http://www.lns.cornell.edu/public/CLNS/2007/, revised | Phys.Rev.Lett.100:161801,2008 | 10.1103/PhysRevLett.100.161801 | CLNS 07/2011, CLEO 07-15 | hep-ex | null | Using a sample of tagged D_s decays collected near the D^*_s D_s peak
production energy in e+e- collisions with the CLEO-c detector, we study the
leptonic decay D^+_s to tau^+ nu_tau via the decay channel tau^+ to e^+ nu_e
bar{nu}_tau. We measure B(D^+_s to tau^+ nu_tau) = (6.17 +- 0.71 +- 0.34) %,
where the first error is statistical and the second systematic. Combining this
result with our measurements of D^+_s to mu^+ nu_mu and D^+_s to tau^+ nu_tau
(via tau^+ to pi^+ bar{nu}_tau), we determine f_{D_s} = (274 +- 10 +- 5) MeV.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 18:15:20 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Apr 2008 20:53:26 GMT"
}
] | 2010-04-08T00:00:00 | [
[
"CLEO Collaboration",
"",
""
],
[
"Ecklund",
"K. M.",
""
]
] | [
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] |
712.1176 | Eduardo Esteves | Eduardo Esteves | Compactified Jacobians of curves with spine decompositions | null | null | null | null | math.AG | null | A curve, that is, a connected, reduced, projective scheme of dimension 1 over
an algebraically closed field, admits two types of compactifications of its
(generalized) Jacobian: the moduli schemes of P-quasistable torsion-free,
rank-1 sheaves and Seshadri's moduli schemes of S-equivalence classes of
semistable torsion-free, rank-1 sheaves. Both are constructed with respect to a
choice of polarization. The former are fine moduli spaces which were shown to
be complete; here we show that they are actually projective. The latter are
just coarse moduli spaces. Here we give a sufficient condition for when these
two types of moduli spaces are equal.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:21:23 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Esteves",
"Eduardo",
""
]
] | [
0.0242686514,
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] |
712.1177 | Grigoris Panotopoulos | Grigoris Panotopoulos | Statefinder parameters in two dark energy models | 16 pages, 2 tables, 7 figures | Nucl.Phys.B796:66-76,2008 | 10.1016/j.nuclphysb.2007.12.001 | null | astro-ph | null | The statefinder parameters ($r,s$) in two dark energy models are studied. In
the first, we discuss in four-dimensional General Relativity a two fluid model,
in which dark energy and dark matter are allowed to interact with each other.
In the second model, we consider the DGP brane model generalized by taking a
possible energy exchange between the brane and the bulk into account. We
determine the values of the statefinder parameters that correspond to the
unique attractor of the system at hand. Furthermore, we produce plots in which
we show $s,r$ as functions of red-shift, and the ($s-r$) plane for each model.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:22:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Panotopoulos",
"Grigoris",
""
]
] | [
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] |
712.1178 | Qiang Li | Qiang Li (1), Alfred III Garson (1), Ira Jung (1), Michael Groza (2),
Paul Dowkontt (1), Richard Bose (1), Garry Simburger (1), Arnold Burger (2),
Henric Krawczynski (1) ((1): Dept. of Physics, Washington University in St.
Louis,(2): Dept. of Physics, Fisk University) | Test of CZT Detectors with Different Pixel Pitches and Thicknesses | 5 pages, 14 figures,Proceedings of NSS/MIC 2007 conference, October
2007, Hawaii | null | null | null | astro-ph | null | The Modified Horizontal Bridgman (MHB) process produces Cadmium Zinc
Telluride (CZT) crystals with high yield and excellent homogeneity. Various
groups,including our own, previously reported on the test of 2x2x0.5 cm3 MHB
CZT detectors grown by the company Orbotech and read out with 8x8 pixels. In
this contribution, we describe the optimization of the photolithographic
process used for contacting the CZT detector with pixel contacts. The optimized
process gives a high yield of good pixels down to pixel diameters/pitches of 50
microns. Furthermore, we discuss the performance of 0.5 cm and 0.75 cm thick
detectors contacted with 64 and 225 pixel read out with the RENA-3 ASICs from
the company NOVA R&D.
| [
{
"version": "v1",
"created": "Fri, 7 Dec 2007 16:28:22 GMT"
},
{
"version": "v2",
"created": "Sat, 8 Dec 2007 03:07:51 GMT"
}
] | 2007-12-10T00:00:00 | [
[
"Li",
"Qiang",
""
],
[
"Garson",
"Alfred III",
""
],
[
"Jung",
"Ira",
""
],
[
"Groza",
"Michael",
""
],
[
"Dowkontt",
"Paul",
""
],
[
"Bose",
"Richard",
""
],
[
"Simburger",
"Garry",
""
],
[
"Burger",
"Arnold",
""
],
[
"Krawczynski",
"Henric",
""
]
] | [
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-0.0724918321,
0.0579265654,
-0.0303620342,
-0.009259128,
-0.0097988639,
0.020722812,
-0.0223344173,
-0.1368344128,
0.0674441606,
-0.0747419968,
-0.0396515727,
-0.0538519435,
-0.0630046427,
-0.0537911281,
0.0487130508,
0.0717620477
] |
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