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711.3708 | Gennady Makanin | G.S.Makanin | Equations in a free group. Elementary theory | null | null | null | null | math.GM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove the decidability of the elementary theory of a free group.
| [
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},
{
"version": "v2",
"created": "Thu, 14 Sep 2017 14:05:46 GMT"
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"G. S.",
""
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711.3709 | Yuri Litvinov | Yu.A. Litvinov, F. Bosch, H. Geissel, J. Kurcewicz, Z. Patyk, N.
Winckler, L. Batist, K. Beckert, D. Boutin, C. Brandau, L. Chen, C.
Dimopoulou, B. Fabian, T. Faestermann, A. Fragner, L. Grigorenko, E.
Haettner, S. Hess, P. Kienle, R. Kn\"obel, C. Kozhuharov, S.A. Litvinov, L.
Maier, M. Mazzocco, F. Montes, G. M\"unzenberg, A. Musumarra, C. Nociforo, F.
Nolden, M. Pf\"utzner, W.R. Plass, A. Prochazka, R. Reda, R. Reuschl, C.
Scheidenberger, M. Steck, T. St\"ohlker, S. Torilov, M. Trassinelli, B. Sun,
H. Weick, M. Winkler | Measurement of the $\beta^+$ and orbital electron-capture decay rates in
fully-ionized, hydrogen-like, and helium-like $^{140}$Pr ions | 4 pages, 3 figures | Phys.Rev.Lett.99:262501,2007 | 10.1103/PhysRevLett.99.262501 | null | nucl-ex | null | We report on the first measurement of the $\beta^+$- and orbital electron
capture decay rates of $^{140}$Pr nuclei with the most simple electron
configurations: bare nuclei, hydrogen-like and helium-like ions. The measured
electron capture decay constant of hydrogen-like $^{140}$Pr$^{58+}$ ions is
about 50% larger than that of helium-like $^{140}$Pr$^{57+}$ ions. Moreover,
$^{140}$Pr ions with one bound electron decay faster than neutral
$^{140}$Pr$^{0+}$ atoms with 59 electrons. To explain this peculiar observation
one has to take into account the conservation of the total angular momentum,
since only particular spin orientations of the nucleus and of the captured
electron can contribute to the allowed decay.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 11:17:20 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Litvinov",
"Yu. A.",
""
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[
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"F.",
""
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"Geissel",
"H.",
""
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"Kurcewicz",
"J.",
""
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"Z.",
""
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"N.",
""
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"Batist",
"L.",
""
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"K.",
""
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[
"Boutin",
"D.",
""
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[
"Brandau",
"C.",
""
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[
"Chen",
"L.",
""
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[
"Dimopoulou",
"C.",
""
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[
"Fabian",
"B.",
""
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"Faestermann",
"T.",
""
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"Fragner",
"A.",
""
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"Grigorenko",
"L.",
""
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"Haettner",
"E.",
""
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"Hess",
"S.",
""
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"Kienle",
"P.",
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"M.",
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"T.",
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"S.",
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"M.",
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711.371 | Bernat Corominas-Murtra BCM | Ricard V. Sol\'e, Mart\'i Rosas-Casals, Bernat Corominas-Murtra and
Sergi Valverde | Robustness of the European power grids under intentional attack | 7 pages, 4 figures | null | 10.1103/PhysRevE.77.026102 | null | physics.soc-ph | null | The power grid defines one of the most important technological networks of
our times and sustains our complex society. It has evolved for more than a
century into an extremely huge and seemingly robust and well understood system.
But it becomes extremely fragile as well, when unexpected, usually minimal,
failures turn into unknown dynamical behaviours leading, for example, to sudden
and massive blackouts. Here we explore the fragility of the European power grid
under the effect of selective node removal. A mean field analysis of fragility
against attacks is presented together with the observed patterns. Deviations
from the theoretical conditions for network percolation (and fragmentation)
under attacks are analysed and correlated with non topological reliability
measures.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 11:17:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Solé",
"Ricard V.",
""
],
[
"Rosas-Casals",
"Martí",
""
],
[
"Corominas-Murtra",
"Bernat",
""
],
[
"Valverde",
"Sergi",
""
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] |
711.3711 | Lutz Hille | Simon M. Goodwin, Lutz Hille, Gerhard R\"ohrle, | Orbits of parabolic subgroups on metabelian ideals | 10 pages, 6 eps figures | null | null | null | math.RT | null | We consider the action of a parabolic subgroup of the General Linear Group on
a metabelian ideal. For those actions, we classify actions with finitely many
orbits using methods from representation theory.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 11:20:30 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Goodwin",
"Simon M.",
""
],
[
"Hille",
"Lutz",
""
],
[
"Röhrle",
"Gerhard",
""
]
] | [
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] |
711.3712 | Paolo Castorina | P. Castorina | Thermal Hadronization, Hawking-Unruh Radiation and Event Horizon in QCD | Invited talk, 8 pages, 6 figures | null | 10.1142/9789812797049_0040 | null | hep-ph | null | Because of colour confinement, the physical vacuum forms an event horizon for
quarks and gluons; this can be crossed only by quantum tunneling, i.e., through
the QCD counterpart of Hawking radiation by black holes. Since such radiation
cannot transmit information to the outside, it must be thermal, of a
temperature determined by the strong force at the confinement surface, and it
must maintain colour neutrality. The resulting process provides a common
mechanism for thermal hadron production in high energy interactions, from
$e^+e^-$ annihilation to heavy ion collisions. The analogy with black-hole
event horizon suggests a dependence of the hadronization temperature on the
baryon density.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 11:28:40 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Castorina",
"P.",
""
]
] | [
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] |
711.3713 | Ian D. Lawrie | Javier Moreno Almeida and Ian D. Lawrie | Dissipation due to fermions in inflaton equations of motion | 9 pages, 4 figures | null | null | null | hep-ph | null | According to quantum field theory, the inflaton equation of motion does not
have the local form that is generally assumed for cosmological purposes. In
particular, earlier investigations of the nonequilibrium dynamics of an
inflaton that decays into scalar particles suggest that the loss of inflaton
energy is not well approximated by the local friction term derived from linear
response theory. We extend this analysis to the case of an inflaton that decays
into fermions, and reach broadly the same conclusion.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 11:37:16 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Almeida",
"Javier Moreno",
""
],
[
"Lawrie",
"Ian D.",
""
]
] | [
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] |
711.3714 | Gui-Fang Dang | Gui-Fang Dang and Heng Fan | Remote controlled-NOT gate of d-dimension | 5 pages, 2 figures; corrected typos, added references | null | null | null | quant-ph | null | Single qubit rotation gate and the controlled-NOT (CNOT) gate constitute a
complete set of gates for universal quantum computation. In general the CNOT
gate are only for two nearby qubits. For two qubits which are remote from each
other, we need a series of swap gates to transfer these two qubits to the
nearest neighboring sites, and then after the CNOT gate we should transfer them
to their original sites again. However, a series of swap gates are resource for
quantum information processing. One economy way which does not consume so much
resource is to implement CNOT gate remotely. The remote CNOT gate is to
implement the CNOT gate for two remotely separated qubits with the help of one
additional maximally entangled state. The original remote CNOT gate is for two
qubits, here we will present the d-dimensional remote CNOT gate. The role of
quantum teleportation is identified in the process of the remote CNOT gate.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 12:54:01 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 10:28:59 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Dang",
"Gui-Fang",
""
],
[
"Fan",
"Heng",
""
]
] | [
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] |
711.3715 | Julia Kempe | Julia Kempe, Hirotada Kobayashi, Keiji Matsumoto and Thomas Vidick | Using Entanglement in Quantum Multi-Prover Interactive Proofs | 19 pages | null | null | null | quant-ph | null | The central question in quantum multi-prover interactive proof systems is
whether or not entanglement shared between provers affects the verification
power of the proof system. We study for the first time positive aspects of
prior entanglement and show that entanglement is useful even for honest
provers. We show how to use shared entanglement to parallelize any multi-prover
quantum interactive proof system to a one-round system with perfect
completeness, with one extra prover. Alternatively, we can also parallelize to
a three-turn system with the same number of provers, where the verifier only
broadcasts the outcome of a coin flip. This "public-coin" property is somewhat
surprising, since in the classical case public-coin multi-prover interactive
proofs are equivalent to single prover ones.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 11:44:45 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Kempe",
"Julia",
""
],
[
"Kobayashi",
"Hirotada",
""
],
[
"Matsumoto",
"Keiji",
""
],
[
"Vidick",
"Thomas",
""
]
] | [
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] |
711.3716 | Francesco Sorrentino Ing | Francesco Sorrentino and Edward Ott | Network synchronization of groups | null | Phys. Rev. E, 76, 056114, 2007 | 10.1103/PhysRevE.76.056114 | null | cond-mat.dis-nn | null | In this paper we study synchronized motions in complex networks in which
there are distinct groups of nodes where the dynamical systems on each node
within a group are the same but are different for nodes in different groups.
Both continuous time and discrete time systems are considered. We initially
focus on the case where two groups are present and the network has bipartite
topology (i.e., links exist between nodes in different groups but not between
nodes in the same group). We also show that group synchronous motions are
compatible with more general network topologies, where there are also
connections within the groups.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 12:22:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sorrentino",
"Francesco",
""
],
[
"Ott",
"Edward",
""
]
] | [
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] |
711.3717 | Mario Martinez Dr. | T. Aaltonen, et al (for the CDF Collaboration) | Measurement of Inclusive Jet Cross Sections in Z/g* (-> ee)+jets
Production in ppbar Collisions at sqrt(s)=1.96 TeV | Submitted to Phys. Rev. Letters | Phys.Rev.Lett.100:102001,2008 | 10.1103/PhysRevLett.100.102001 | null | hep-ex | null | Inclusive jet cross sections in Z/gamma^* events, with Z/gamma^* decaying
into an electron-positron pair, are measured as a function of jet transverse
momentum and jet multiplicity in ppbar collisions at sqrt{s} = 1.96 TeV with
the upgraded Collider Detector at Fermilab in Run II, based on an integrated
luminosity of 1.7 fb^-1. The measurements cover the rapidity region | yjet | <
2.1 and the transverse momentum range ptjet > 30 GeV/c. Next-to-leading order
perturbative QCD predictions are in good agreement with the measured cross
sections.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:38:51 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Aaltonen",
"T.",
""
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] |
711.3718 | Pascal Brault | Thu Huong Vo Thi (MAPMO), Jean-Louis Rouet (MAPMO, ISTO), Pascal
Brault (GREMI), Jean-Marc Bauchire (GREMI), St\'ephane Cordier (MAPMO),
Christophe Josserand (LMM) | A continuous non-linear shadowing model of columnar growth | Fast Track Communication | Journal of Physics D: Applied Physics 41 (2008) 022003 (3pp) | 10.1088/0022-3727/41/2/022003 | null | cond-mat.stat-mech | null | We propose the first continuous model with long range screening (shadowing)
that described columnar growth in one space dimension, as observed in plasma
sputter deposition. It is based on a new continuous partial derivative equation
with non-linear diffusion and where the shadowing effects apply on all the
different processes.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 12:50:27 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 14:35:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Thi",
"Thu Huong Vo",
"",
"MAPMO"
],
[
"Rouet",
"Jean-Louis",
"",
"MAPMO, ISTO"
],
[
"Brault",
"Pascal",
"",
"GREMI"
],
[
"Bauchire",
"Jean-Marc",
"",
"GREMI"
],
[
"Cordier",
"Stéphane",
"",
"MAPMO"
],
[
"Josserand",
"Christophe",
"",
"LMM"
]
] | [
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] |
711.3719 | Mauricio Porto Pato | O. Bohigas, J. X. de Carvalho and M. P. Pato | Disordered ensembles of random matrices | 8 pages, 4 figures | null | 10.1103/PhysRevE.77.011122 | null | cond-mat.stat-mech | null | It is shown that the families of generalized matrix ensembles recently
considered which give rise to an orthogonal invariant stable L\'{e}vy ensemble
can be generated by the simple procedure of dividing Gaussian matrices by a
random variable. The nonergodicity of this kind of disordered ensembles is
investigated. It is shown that the same procedure applied to random graphs
gives rise to a family that interpolates between the Erd\"{o}s-Renyi and the
scale free models.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 12:52:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bohigas",
"O.",
""
],
[
"de Carvalho",
"J. X.",
""
],
[
"Pato",
"M. P.",
""
]
] | [
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711.372 | Geert Jan van Oldenborgh | G. J. van Oldenborgh | How unusual was autumn 2006 in Europe? | null | Clim. Past, 3, 659-668, 2007 | 10.5194/cp-3-659-2007 | null | physics.ao-ph | null | The temperatures in large parts of Europe have been record high during the
meteorological autumn of 2006. Compared to 1961-1990, the 2m temperature was
more than three degrees Celsius above normal from the North side of the Alps to
southern Norway. This made it by far the warmest autumn on record in the United
Kingdom, Belgium, the Netherlands, Denmark, Germany and Switzerland, with the
records in Central England going back to 1659, in the Netherlands to 1706 and
in Denmark to 1768.
Assuming that the mean of the temperature distribution changes proportional
to the global mean temperature, but the shape remains the same includes to
first order the effects of global warming. Even under this assumption the
autumn temperatures were very unusual, with estimates of the return time of 200
to 2000 years in this region. The lower bound of the 95% confidence interval is
more than 100 to 300 years.
Climate models that simulate the current atmospheric circulation well
underestimate the observed mean rise in autumn temperatures. They do not
simulate a change in the shape of the distribution that would increase the
probability of warm events under global warming. This implies that the warm
autumn 2006 either was a very rare coincidence, or the local temperature rise
is much stronger than modelled, or non-linear physics that is missing from
these models increases the probability of warm extremes.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:59:46 GMT"
}
] | 2020-11-04T00:00:00 | [
[
"van Oldenborgh",
"G. J.",
""
]
] | [
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711.3721 | Zhaoqing Feng | Zhao-Qing Feng, Gen-Ming Jin, Feng-Shou Zhang | Dynamical analysis on heavy-ion fusion reactions near Coulomb barrier | 20 pages, 12 figures | Nucl.Phys.A802:91-106,2008 | 10.1016/j.nuclphysa.2008.01.022 | null | nucl-th | null | The shell correction is proposed in the improved isospin dependent quantum
molecular dynamics (ImIQMD) model, which plays an important role in heavy-ion
fusion reactions near Coulomb barrier. By using the ImIQMD model, the static
and dynamical fusion barriers, dynamical barrier distribution in the fusion
reactions are analyzed systematically. The fusion and capture excitation
functions for a series of reaction systems are calculated and compared with
experimental data. It is found that the fusion cross sections for neutron-rich
systems increase obviously, and the strong shell effects of two colliding
nuclei result in a decrease of the fusion cross sections at the sub-barrier
energies. The lowering of the dynamical fusion barriers favors the enhancement
of the sub-barrier fusion cross sections, which is related to the nucleon
transfer and the neck formation in the fusion reactions.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:14:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Feng",
"Zhao-Qing",
""
],
[
"Jin",
"Gen-Ming",
""
],
[
"Zhang",
"Feng-Shou",
""
]
] | [
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711.3722 | Andrew Stacey | Andrew Stacey and Sarah Whitehouse | The Hunting of the Hopf Ring | 61 pages, no figures; uses xy, pxfonts | null | null | null | math.AT math.KT math.RA | null | We provide a new algebraic description of the structure on the set of all
unstable cohomology operations for a suitable generalised cohomology theory,
E^*. Our description is as a graded and completed version of a Tall-Wraith
monoid. The E^*-cohomology of a space X is a module for this Tall-Wraith
monoid. We also show that the corresponding Hopf ring of unstable co-operations
is a module for the Tall-Wraith monoid of unstable operations. Further examples
are provided by considering operations from one theory to another.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:14:18 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Stacey",
"Andrew",
""
],
[
"Whitehouse",
"Sarah",
""
]
] | [
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] |
711.3723 | Philippe Jetzer | Philippe Jetzer and Mauro Sereno | Solar system tests of the cosmological constant | 10 pages, to appear in the proceedings of the I Italian-Pakistan
Workshop on Relativistic Astrophysics, which will be published in the Journal
Nuovo Cimento | null | 10.1393/ncb/i2007-10384-8 | null | astro-ph | null | We discuss the influence of the cosmological constant $\Lambda$ on the
gravitational equations of motion of bodies with arbitrary masses and
eventually solve the two-body problem. Observational constraints are derived
from measurements of the periastron advance in stellar systems, in particular
binary pulsars and the solar system. For the latter we consider also the change
in the mean motion due to $\Lambda$. Up to now, Earth and Mars data give the
best constraint, $\Lambda \sim 10^{-36} \mathrm{km}^{-2}$. If properly
accounting for the gravito-magnetic effect, this upper limit on $\Lambda$ could
greatly improve in the near future thanks to new data from planned or already
operating space-missions. Dark matter or modifications of the Newtonian
inverse-square law in the solar system are discussed as well. Variations in the
$1/r^2$ behavior are considered in the form of either a possible Yukawa-like
interaction or a modification of gravity of MOND type.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:35:23 GMT"
},
{
"version": "v2",
"created": "Tue, 27 Nov 2007 10:02:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jetzer",
"Philippe",
""
],
[
"Sereno",
"Mauro",
""
]
] | [
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] |
711.3724 | Constantin Loizides | B.Alver, B.B.Back, M.D.Baker, M.Ballintijn, D.S.Barton, R.R.Betts,
R.Bindel, W.Busza, V.Chetluru, E.Garc\'ia, T.Gburek, J.Hamblen, U.Heinz,
D.J.Hofman, R.S.Hollis, A.Iordanova, W.Li, C.Loizides, S.Manly, A.C.Mignerey,
R.Nouicer, A.Olszewski, C.Reed, C.Roland, G.Roland, J.Sagerer, P.Steinberg,
G.S.F.Stephans, M.B.Tonjes, A.Trzupek, G.J.van Nieuwenhuizen,
S.S.Vaurynovich, R.Verdier, G.I.Veres, P.Walters, E.Wenger, B.Wosiek,
K.Wo\'zniak, B.Wys{\l}ouch | The Importance of Correlations and Fluctuations on the Initial Source
Eccentricity in High-Energy Nucleus-Nucleus Collisions | 18 pages, 10 figures, submitted to PRC | Phys.Rev.C77:014906,2008 | 10.1103/PhysRevC.77.014906 | null | nucl-ex nucl-th | null | In this paper, we investigate various ways of defining the initial source
eccentricity using the Monte Carlo Glauber (MCG) approach. In particular, we
examine the participant eccentricity, which quantifies the eccentricity of the
initial source shape by the major axes of the ellipse formed by the interaction
points of the participating nucleons. We show that reasonable variation of the
density parameters in the Glauber calculation, as well as variations in how
matter production is modeled, do not significantly modify the already
established behavior of the participant eccentricity as a function of collision
centrality. Focusing on event-by-event fluctuations and correlations of the
distributions of participating nucleons we demonstrate that, depending on the
achieved event-plane resolution, fluctuations in the elliptic flow magnitude
$v_2$ lead to most measurements being sensitive to the root-mean-square, rather
than the mean of the $v_2$ distribution. Neglecting correlations among
participants, we derive analytical expressions for the participant eccentricity
cumulants as a function of the number of participating nucleons,
$\Npart$,keeping non-negligible contributions up to $\ordof{1/\Npart^3}$. We
find that the derived expressions yield the same results as obtained from
mixed-event MCG calculations which remove the correlations stemming from the
nuclear collision process. Most importantly, we conclude from the comparison
with MCG calculations that the fourth order participant eccentricity cumulant
does not approach the spatial anisotropy obtained assuming a smooth nuclear
matter distribution. In particular, for the Cu+Cu system, these quantities
deviate from each other by almost a factor of two over a wide range in
centrality.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:35:55 GMT"
}
] | 2016-03-28T00:00:00 | [
[
"Alver",
"B.",
""
],
[
"Back",
"B. B.",
""
],
[
"Baker",
"M. D.",
""
],
[
"Ballintijn",
"M.",
""
],
[
"Barton",
"D. S.",
""
],
[
"Betts",
"R. R.",
""
],
[
"Bindel",
"R.",
""
],
[
"Busza",
"W.",
""
],
[
"Chetluru",
"V.",
""
],
[
"García",
"E.",
""
],
[
"Gburek",
"T.",
""
],
[
"Hamblen",
"J.",
""
],
[
"Heinz",
"U.",
""
],
[
"Hofman",
"D. J.",
""
],
[
"Hollis",
"R. S.",
""
],
[
"Iordanova",
"A.",
""
],
[
"Li",
"W.",
""
],
[
"Loizides",
"C.",
""
],
[
"Manly",
"S.",
""
],
[
"Mignerey",
"A. C.",
""
],
[
"Nouicer",
"R.",
""
],
[
"Olszewski",
"A.",
""
],
[
"Reed",
"C.",
""
],
[
"Roland",
"C.",
""
],
[
"Roland",
"G.",
""
],
[
"Sagerer",
"J.",
""
],
[
"Steinberg",
"P.",
""
],
[
"Stephans",
"G. S. F.",
""
],
[
"Tonjes",
"M. B.",
""
],
[
"Trzupek",
"A.",
""
],
[
"van Nieuwenhuizen",
"G. J.",
""
],
[
"Vaurynovich",
"S. S.",
""
],
[
"Verdier",
"R.",
""
],
[
"Veres",
"G. I.",
""
],
[
"Walters",
"P.",
""
],
[
"Wenger",
"E.",
""
],
[
"Wosiek",
"B.",
""
],
[
"Woźniak",
"K.",
""
],
[
"Wysłouch",
"B.",
""
]
] | [
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] |
711.3725 | Beata Ziaja | B. Ziaja, H. Wabnitz, E. Weckert, T. Moeller | Femtosecond non-equilibrium dynamics of clusters irradiated with short
intense VUV pulses | 32 pages, 17 figures | null | 10.1088/1367-2630/10/4/043003 | null | physics.plasm-ph hep-ph | null | The kinetic Boltzmann equation is used to model the non-equilibrium
ionization phase that initiates the evolution of atomic clusters irradiated
with single pulses of intense vacuum ultraviolet radiation. The duration of the
pulses is < 50 fs and their intensity in the focus is < 10^{14} W/cm^2. This
statistical model includes various processes contributing to the sample
dynamics at this particular radiation wavelength, and is computationally
efficient also for large samples. Two effects are investigated in detail: the
impact of the electron heating rate and the effect of the plasma environment on
the overall ionization dynamics. Results on the maximal ion charge, the average
ion charge and the average energy absorbed per atom estimated with this model
are compared to the experimental data obtained at the free-electron-laser
facility FLASH at DESY. Our analysis confirms that the dynamics within the
irradiated samples is complex, and the total ionization rate is the resultant
of various processes. In particular, within the theoretical framework defined
in this model the high charge states as observed in experiment cannot be
obtained with the standard heating rates derived with Coulomb atomic
potentials. Such high charge states can be created with the enhanced heating
rates derived with the effective atomic potentials. The modification of
ionization potentials by plasma environment is found to have less effect on the
ionization dynamics than the electron heating rate. We believe that our results
are a step towards better understanding the dynamics within the samples
irradiated with intense VUV radiation.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:10:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ziaja",
"B.",
""
],
[
"Wabnitz",
"H.",
""
],
[
"Weckert",
"E.",
""
],
[
"Moeller",
"T.",
""
]
] | [
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] |
711.3726 | Stergos Afantenos | Michael Zock and Stergos D. Afantenos | Let's get the student into the driver's seat | 6 pages | The Seventh International Symposium on Natural Language Processing
(SNLP 2007). Chonburi, Thailand | null | null | cs.CL | null | Speaking a language and achieving proficiency in another one is a highly
complex process which requires the acquisition of various kinds of knowledge
and skills, like the learning of words, rules and patterns and their connection
to communicative goals (intentions), the usual starting point. To help the
learner to acquire these skills we propose an enhanced, electronic version of
an age old method: pattern drills (henceforth PDs). While being highly regarded
in the fifties, PDs have become unpopular since then, partially because of
their lack of grounding (natural context) and rigidity. Despite these
shortcomings we do believe in the virtues of this approach, at least with
regard to the acquisition of basic linguistic reflexes or skills (automatisms),
necessary to survive in the new language. Of course, the method needs
improvement, and we will show here how this can be achieved. Unlike tapes or
books, computers are open media, allowing for dynamic changes, taking users'
performances and preferences into account. Building an electronic version of
PDs amounts to building an open resource, accomodatable to the users' ever
changing needs.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:44:55 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Zock",
"Michael",
""
],
[
"Afantenos",
"Stergos D.",
""
]
] | [
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] |
711.3727 | Demetrio Stojanoff | Jorge Antezana, Enrique R. Pujals and Demetrio Stojanoff | The iterated Aluthge transforms of a matrix converge | 23 pages | null | null | null | math.FA math.DS | null | Given an $r\times r$ complex matrix $T$, if $T=U|T|$ is the polar
decomposition of $T$, then, the Aluthge transform is defined by $$ \Delta(T)=
|T|^{1/2} U |T |^{1/2}. $$ Let $\Delta^{n}(T)$ denote the n-times iterated
Aluthge transform of $T$, i.e. $\Delta^{0}(T)=T$ and
$\Delta^{n}(T)=\Delta(\Delta^{n-1}(T))$, $n\in\mathbb{N}$. We prove that the
sequence $\{\Delta^{n}(T)\}_{n\in\mathbb{N}}$ converges for every $r\times r$
matrix $T$. This result was conjecturated by Jung, Ko and Pearcy in 2003. We
also analyze the regularity of the limit function.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:49:21 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Antezana",
"Jorge",
""
],
[
"Pujals",
"Enrique R.",
""
],
[
"Stojanoff",
"Demetrio",
""
]
] | [
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] |
711.3728 | Sascha Orlik | Sascha Orlik | The fundamental group of period domains over finite fields | 13 pages | null | null | null | math.AG | null | We determine the fundamental group of period domains over finite fields.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 13:59:26 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Orlik",
"Sascha",
""
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711.3729 | S. Chaturvedi | S. Chaturvedi, G. Marmo, N. Mukunda, R. Simon | Schwinger Representation for the Symmetric Group: Two explicit
constructions for the Carrier Space | Latex, 6 pages | Phys.Lett.A372:3763-3767,2008 | 10.1016/j.physleta.2008.02.071 | null | quant-ph | null | We give two explicit construction for the carrier space for the Schwinger
representation of the group $S_n$. While the first relies on a class of
functions consisting of monomials in antisymmetric variables, the second is
based on the Fock space associated with the Greenberg algebra.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:14:37 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chaturvedi",
"S.",
""
],
[
"Marmo",
"G.",
""
],
[
"Mukunda",
"N.",
""
],
[
"Simon",
"R.",
""
]
] | [
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711.373 | Christiane Helling | Christiane Helling | Cloud formation in giant planets | 4 pages, Proceeding to "Extreme solar systems", eds. Fischer, Rasio,
Thorsett, Wolszczan | null | null | null | astro-ph | null | We calculate the formation of dust clouds in atmospheres of giant
gas-planets. The chemical structure and the evolution of the grain size
distribution in the dust cloud layer is discussed based on a consistent
treatment of seed formation, growth/evaporation and gravitational settling.
Future developments are shortly addressed.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:16:55 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Helling",
"Christiane",
""
]
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] |
711.3731 | Dr. Georgios M. Nikolopoulos | G. M. Nikolopoulos, C. Lazarou, and P. Lambropoulos | Effects of relative phase and interactions on atom-laser outcoupling
from a double-well Bose-Einstein condensate: Markovian and non-Markovian
dynamics | to appear in J. Phys. B | J. Phys. B: At. Mol. Opt. Phys. 41 (2008) 025301. | 10.1088/0953-4075/41/2/025301 | null | quant-ph cond-mat.other | null | We investigate aspects of the dynamics of a continuous atom-laser scheme
based on the merging of independently formed atomic condensates. Our
theoretical analysis covers the Markovian as well as the non-Markovian
operational regimes, and is based on a semiclassical (mean-field) two-mode
model. The role of the relative phase between the two condensates and the
effect of interatomic interactions on the evolution of the trapped populations
and the distribution of outcoupled atoms are discussed.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:17:39 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Nikolopoulos",
"G. M.",
""
],
[
"Lazarou",
"C.",
""
],
[
"Lambropoulos",
"P.",
""
]
] | [
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] |
711.3732 | Gustavo Murgida | D.A. Wisniacki, G.E. Murgida, P.I. Tamborenea | Quantum control using diabatic and adiabatic transitions | 3 pages, 3 figures | null | 10.1063/1.2836223 | null | cond-mat.mes-hall cond-mat.str-el | null | We exploit the concept of Landau-Zener transitions at avoided energy
crossings as a quantum-control tool. In an avoided crossing the two quantum
states interchange their characteristics as an external parameter is varied.
Depending on the rate of change of the parameter it is possible to control the
final state. We use this simple idea to travel along the energy spectrum of a
realistic system: two interacting electrons confined in a quasi-one-dimensional
semiconductor system.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:19:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wisniacki",
"D. A.",
""
],
[
"Murgida",
"G. E.",
""
],
[
"Tamborenea",
"P. I.",
""
]
] | [
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] |
711.3733 | Craig Sooman Mr | C. R. Gilson, J. J. C. Nimmo and C. M. Sooman | On a direct approach to quasideterminant solutions of a noncommutative
modified KP equation | null | J. Phys. A: Math. Theor. 41 (2008) 085202 | 10.1088/1751-8113/40/14/007 | null | nlin.SI | null | A noncommutative version of the modified KP equation and a family of its
solutions expressed as quasideterminants are discussed. The origin of these
solutions is explained by means of Darboux transformations and the solutions
are verified directly. We also verify directly an explicit connection between
quasideterminant solutions of the noncommutative mKP equation and the
noncommutative KP equation arising from the Miura transformation.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:24:29 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 11:40:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gilson",
"C. R.",
""
],
[
"Nimmo",
"J. J. C.",
""
],
[
"Sooman",
"C. M.",
""
]
] | [
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] |
711.3734 | Hannes Horst | Hannes Horst, Poshak Gandhi, Alain Smette, Wolfgang J. Duschl | The mid IR -- hard X-ray correlation in AGN and its implications for
dusty torus models | accepted for publication in Astronomy & Astrophysics, 13 pages, 4
figures | null | 10.1051/0004-6361:20078548 | null | astro-ph | null | Context: We investigate mid-infrared and X-ray properties of the dusty torus
invoked in the unification scenario for active galactic nuclei.
Aims: We use the relation between mid IR and hard X-ray luminosities to
constrain the geometry and physical state of the dusty torus.
Methods: We present new VISIR observations of 17 nearby AGN and combine these
with our earlier VISIR sample of 8 Seyfert galaxies. Combining these
observations with X-ray data from the literature we study the correlation
between their mid IR and hard X-ray luminosities.
Results: A statistically highly significant correlation between the rest
frame 12.3 mircon (L_MIR) and 2-10 keV (L_X) luminosities is found.
Furthermore, with a probability of 97%, we find that Sy 1 and Sy 2 have the
same distribution of L_MIR over L_X.
Conclusions: The high resolution of our MIR imaging allows us to exclude any
significant non-torus contribution to the AGN mid IR continuum,thereby implying
that the similarity in the L_MIR / L_X ratio between Sy 1s and Sy 2s is
intrinsic to AGN. We argue that this is best explained by clumpy torus models.
The slope of the correlation is in good agreement with the expectations from
the unified scenario and indicates little to no change of the torus geometry
with luminosity. In addition, we demonstrate that the high angular resolution
is crucial for AGN studies in the IR regime.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:03:01 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 08:18:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Horst",
"Hannes",
""
],
[
"Gandhi",
"Poshak",
""
],
[
"Smette",
"Alain",
""
],
[
"Duschl",
"Wolfgang J.",
""
]
] | [
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] |
711.3735 | Ho-Chih Lin | H.-C. Lin, A. J. Fisher | Local entanglement of multidimensional continuous-variable systems | RevTex, 11 pages, 3 figures (13 files) | Phys. Rev. A 78, 012349 (2008) | 10.1103/PhysRevA.78.012349 | null | quant-ph | null | We study the `local entanglement' remaining after filtering operations
corresponding to imperfect measurements performed by one or both parties, such
that the parties can only determine whether or not the system is located in
some region of space. The local entanglement in pure states of general
bipartite multidimensional continuous-variable systems can be completely
determined through simple expressions. We apply our approach to semiclassical
WKB systems, multi-dimensional harmonic oscillators, and a hydrogen atom as
three examples.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:37:42 GMT"
}
] | 2008-08-01T00:00:00 | [
[
"Lin",
"H. -C.",
""
],
[
"Fisher",
"A. J.",
""
]
] | [
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-0.0085867587,
0.0827582479,
0.0259898696,
-0.0849098563,
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0.1136679575,
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] |
711.3736 | Pierre de la Harpe | Martin R. Bridson, Pierre de la Harpe, and Victor Kleptsyn | The Chabauty space of closed subgroups of the three-dimensional
Heisenberg group | Minor edits. Final version. To appear in the Pacific Journal. 41
pages, no figures | null | null | null | math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | When equipped with the natural topology first defined by Chabauty, the closed
subgroups of a locally compact group $G$ form a compact space $\Cal C(G)$. We
analyse the structure of $\Cal C(G)$ for some low-dimensional Lie groups,
concentrating mostly on the 3-dimensional Heisenberg group $H$. We prove that
$\Cal C(H)$ is a 6-dimensional space that is path--connected but not locally
connected. The lattices in $H$ form a dense open subset $\Cal L(H) \subset \Cal
C(H)$ that is the disjoint union of an infinite sequence of
pairwise--homeomorphic aspherical manifolds of dimension six, each a torus
bundle over $(\bold S^3 \smallsetminus T) \times \bold R$, where $T$ denotes a
trefoil knot. The complement of $\Cal L(H)$ in $\Cal C(H)$ is also described
explicitly. The subspace of $\Cal C(H)$ consisting of subgroups that contain
the centre $Z(H)$ is homeomorphic to the 4--sphere, and we prove that this is a
weak retract of $\Cal C(H)$.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:26:54 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Nov 2008 11:28:45 GMT"
}
] | 2008-11-18T00:00:00 | [
[
"Bridson",
"Martin R.",
""
],
[
"de la Harpe",
"Pierre",
""
],
[
"Kleptsyn",
"Victor",
""
]
] | [
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] |
711.3737 | Heinrichs Jean | J. Heinrichs | Anomalous scaling of conductance cumulants in one-dimensional Anderson
localization | null | J. Phys.: Condens. Matter 16 (2004) 7995-8005 | 10.1088/0953-8984/16/45/021 | null | cond-mat.mes-hall cond-mat.dis-nn | null | The mean and the variance of the logarithm of the conductance ($ln g$) in the
localized regime in the one-dimensional Anderson model are calculated
analytically for weak disorder, starting from the recursion relations for the
complex reflection- and transmission amplitudes. The exact recursion relation
for the reflection amplitudes is approximated by improved Born approximation
forms which ensure that averaged reflection coefficients tend asymptotically to
unity in the localized regime, for chain lengths $L=Na\to\infty$. In contrast
the familiar Born approximation of perturbation theory would not be adapted for
the localized regime since it constrains the reflection coefficient to be less
than one. The proper behaviour of the reflection coefficient (and of other
related reflection parameters) is responsible for various anomalies in the
cumulants of $\ln g$, in particular for the well-known band center anomaly of
the localization length. While a simple improved Born approximation is
sufficient for studying cumulants at a generic band energy, we find that a
generalized improved Born approximation is necessary to account satisfactorily
for numerical results for the band center anomaly in the mean of $\ln g$. For
the variance of $\ln g$ at the band center, we reveal the existence of a weak
anomalous quadratic term proportional to $L^2$, besides the previously found
anomaly in the linear term. At a generic band energy the variance of $\ln g$ is
found to be linear in $L$ and is given by twice the mean, up to higher order
corrections which are calculated. We also exhibit the $L=$independent offset
terms in the variance, which strongly depend on reflection anomalies.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:33:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Heinrichs",
"J.",
""
]
] | [
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] |
711.3738 | Lars Kadison | Lars Kadison | Simplicial Hochschild cochains as an Amitsur complex | 5 pages formatted for AGMF proceedings | null | null | null | math.RA math.KT | null | It is shown that the cochain complex of relative Hochschild A-valued cochains
of a depth two extension A | B under cup product is isomorphic as a
differential graded algebra with the Amitsur complex of the coring S = End
{}_BA_B over the centralizer R = A^B with grouplike element 1_S, which itself
is isomorphic to the Cartier complex of S with coefficients in the
(S,S)-bicomodule R^e. This specializes to finite dimensional algebras,
H-separable extensions and Hopf-Galois extensions.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:38:39 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Kadison",
"Lars",
""
]
] | [
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] |
711.3739 | Alberto Moretti | A. Moretti (1), R. Margutti (1,2), F. Pasotti (1,2), A.P. Beardmore
(3), S. Campana (1), G. Chincarini (2,1), S. Covino (1), O. Godet (3), C.
Guidorzi (2,1) J.P. Osborne (3), P. Romano (2,1), G. Tagliaferri (1) ((1)
INAF-OAB; (2) U. Bicocca; (3) U. Leicester) | When GRB afterglows get softer, hard components come into play | 10 pages, accepted for publication in A&A | AIP Conf.Proc.1000:216-219,2008 | 10.1063/1.2943448 | null | astro-ph | null | We aim to investigate the ability of simple spectral models to describe the
GRB early afterglow emission. We performed a time resolved spectral analysis of
a bright GRB sample detected by the Swift Burst Alert Telescope and promptly
observed by the Swift X-ray Telescope,with spectroscopically measured redshift
in the period April 2005 -- January 2007. The sample consists of 22 GRBs and a
total of 214 spectra. We restricted our analysis to the softest spectra
sub--sample which consists of 13 spectra with photon index > 3. In this sample
we found that four spectra, belonging to GRB060502A, GRB060729, GRB060904B,
GRB061110A prompt--afterglow transition phase, cannot be modeled neither by a
single power law nor by the Band model. Instead we find that the data present
high energy (> 3 keV, in the observer frame) excesses with respect to these
models. We estimated the joint statistical significance of these excesses at
the level of 4.3 sigma. In all four cases, the deviations can be modeled well
by adding either a second power law or a blackbody component to the usual
synchrotron power law spectrum. The additional power law would be explained by
the emerging of the afterglow, while the blackbody could be interpreted as the
photospheric emission from X-ray flares or as the shock breakout emission. In
one case these models leave a 2.2 sigma excess which can be fit by a Gaussian
line at the energy the highly ionized Nickel recombination. Although the data
do not allow an unequivocal interpretation, the importance of this analysis
consists in the fact that we show that a simple power law model or a Band model
are insufficient to describe the X-ray spectra of a small homogeneous sample of
GRBs at the end of their prompt phase.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:40:04 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Moretti",
"A.",
""
],
[
"Margutti",
"R.",
""
],
[
"Pasotti",
"F.",
""
],
[
"Beardmore",
"A. P.",
""
],
[
"Campana",
"S.",
""
],
[
"Chincarini",
"G.",
""
],
[
"Covino",
"S.",
""
],
[
"Godet",
"O.",
""
],
[
"Guidorzi",
"C.",
""
],
[
"Osborne",
"J. P.",
""
],
[
"Romano",
"P.",
""
],
[
"Tagliaferri",
"G.",
""
]
] | [
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] |
711.374 | Surachate Limkumnerd | Surachate Limkumnerd, Erik Van der Giessen | Study of size effects in thin films by means of a crystal plasticity
theory based on DiFT | 20 pages, 11 figures | null | 10.1016/j.jmps.2008.06.004 | null | cond-mat.mtrl-sci | null | In a recent publication, we derived the mesoscale continuum theory of
plasticity for multiple-slip systems of parallel edge dislocations, motivated
by the statistical-based nonlocal continuum crystal plasticity theory for
single-glide due to Yefimov et al. (2004b). In this dislocation field theory
(DiFT) the transport equations for both the total dislocation densities and
geometrically necessary dislocation densities on each slip system were obtained
from the Peach-Koehler interactions through both single and pair dislocation
correlations. The effect of pair correlation interactions manifested itself in
the form of a back stress in addition to the external shear and the
self-consistent internal stress. We here present the study of size effects in
single crystalline thin films with symmetric double slip using the novel
continuum theory. Two boundary value problems are analyzed: (1) stress
relaxation in thin films on substrates subject to thermal loading, and (2)
simple shear in constrained films. In these problems, earlier discrete
dislocation simulations had shown that size effects are born out of layers of
dislocations developing near constrained interfaces. These boundary layers
depend on slip orientations and applied loading but are insensitive to the film
thickness. We investigate stress response to changes in controlled parameters
in both problems. Comparisons with previous discrete dislocation simulations
are discussed.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:40:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Limkumnerd",
"Surachate",
""
],
[
"Van der Giessen",
"Erik",
""
]
] | [
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] |
711.3741 | Alberto Carrassi A. | Alberto Carrassi, Michael Ghil, Anna Trevisan and Francesco Uboldi | Data assimilation as a nonlinear dynamical systems problem: Stability
and convergence of the prediction-assimilation system | null | null | 10.1063/1.2909862 | null | nlin.CD | null | We study prediction-assimilation systems, which have become routine in
meteorology and oceanography and are rapidly spreading to other areas of the
geosciences and of continuum physics. The long-term, nonlinear stability of
such a system leads to the uniqueness of its sequentially estimated solutions
and is required for the convergence of these solutions to the system's true,
chaotic evolution. The key ideas of our approach are illustrated for a
linearized Lorenz system. Stability of two nonlinear prediction-assimilation
systems from dynamic meteorology is studied next via the complete spectrum of
their Lyapunov exponents; these two systems are governed by a large set of
ordinary and of partial differential equations, respectively. The degree of
data-induced stabilization is crucial for the performance of such a system.
This degree, in turn, depends on two key ingredients: (i) the observational
network, either fixed or data-adaptive; and (ii) the assimilation method.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:41:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Carrassi",
"Alberto",
""
],
[
"Ghil",
"Michael",
""
],
[
"Trevisan",
"Anna",
""
],
[
"Uboldi",
"Francesco",
""
]
] | [
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] |
711.3742 | Brian Moore | Brian Moore, Josef Schicho, Clement M. Gosselin | Dynamic balancing of planar mechanisms using toric geometry | null | null | null | null | math.AG math.CV | null | In this paper, a new method to determine the complete set of dynamically
balanced planar four-bar mechanims is presented. Using complex variables to
model the kinematics of the mechanism, the dynamic balancing constraints are
written as algebraic equations over complex variables and joint angular
velocities. After elimination of the joint angular velocity variables, the
problem is formulated as a problem of factorization of Laurent polynomials.
Using toric polynomial division, necessary and sufficient conditions for
dynamic balancing of planar four-bar mechanisms are derived.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:42:24 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Moore",
"Brian",
""
],
[
"Schicho",
"Josef",
""
],
[
"Gosselin",
"Clement M.",
""
]
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] |
711.3743 | Guidal | M. Guidal, S. Morrow | Exclusive rho^0 electroproduction on the proton : GPDs or not GPDs ? | 11 pages, 4 figures, proceedings of the workshop on "Exclusive
Reactions at High Momentum Transfer", Jefferson Lab, May07 | null | 10.1142/9789812796950_0021 | null | hep-ph | null | We discuss the interpretation of the $ep\to ep\rho^0$ process in terms of, on
the one hand, Generalized Parton Distributions and, on the other hand, an
effective hadronic model based on Regge theory.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:23:55 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Guidal",
"M.",
""
],
[
"Morrow",
"S.",
""
]
] | [
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711.3744 | Luis Bonilla L. | I. Plans, A. Carpio, L.L. Bonilla | Homogeneous nucleation of dislocations as bifurcations in a periodized
discrete elasticity model | 6 pages, 4 figures, to appear in Europhys. Lett | Europhys. Lett. 81, 36001 (2008) | 10.1209/0295-5075/81/36001 | null | cond-mat.mtrl-sci | null | A novel analysis of homogeneous nucleation of dislocations in sheared
two-dimensional crystals described by periodized discrete elasticity models is
presented. When the crystal is sheared beyond a critical strain $F=F_{c}$, the
strained dislocation-free state becomes unstable via a subcritical pitchfork
bifurcation. Selecting a fixed final applied strain $F_{f}>F_{c}$, different
simultaneously stable stationary configurations containing two or four edge
dislocations may be reached by setting $F=F_{f}t/t_{r}$ during different time
intervals $t_{r}$. At a characteristic time after $t_{r}$, one or two dipoles
are nucleated, split, and the resulting two edge dislocations move in opposite
directions to the sample boundary. Numerical continuation shows how
configurations with different numbers of edge dislocation pairs emerge as
bifurcations from the dislocation-free state.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:45:31 GMT"
}
] | 2008-05-09T00:00:00 | [
[
"Plans",
"I.",
""
],
[
"Carpio",
"A.",
""
],
[
"Bonilla",
"L. L.",
""
]
] | [
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] |
711.3745 | Sannino Francesco | Thomas A. Ryttov (CERN and NBI) and Francesco Sannino (University of
Southern Denmark and NBI) | Supersymmetry Inspired QCD Beta Function | 17 pages and 3 figures. References Added | Phys.Rev.D78:065001,2008 | 10.1103/PhysRevD.78.065001 | CERN-PH-TH/2007-231 | hep-th hep-lat hep-ph | null | We propose an all orders beta function for ordinary Yang-Mills theories with
or without fermions inspired by the Novikov-Shifman-Vainshtein-Zakharov beta
function of N=1 supersymmetric gauge theories. The beta function allows us to
bound the conformal window. When restricting to one adjoint Weyl fermion we
show how the proposed beta function matches the one of supersymmetric
Yang-Mills theory. The running of the pure Yang-Mills coupling is computed and
the deviation from the two loop result is presented. We then compare the
deviation with the one obtained from lattice data also with respect to the two
loop running.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 14:46:29 GMT"
},
{
"version": "v2",
"created": "Sun, 25 Nov 2007 16:45:10 GMT"
},
{
"version": "v3",
"created": "Thu, 13 Dec 2007 16:00:51 GMT"
}
] | 2008-11-07T00:00:00 | [
[
"Ryttov",
"Thomas A.",
"",
"CERN and NBI"
],
[
"Sannino",
"Francesco",
"",
"University of\n Southern Denmark and NBI"
]
] | [
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711.3746 | Michael G. Eastwood | Michael G. Eastwood | Symmetries and Invariant Differential Pairings | 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 (2007), 113, 10 pages | 10.3842/SIGMA.2007.113 | null | math.DG | null | The purpose of this article is to motivate the study of invariant, and
especially conformally invariant, differential pairings. Since a general theory
is lacking, this work merely presents some interesting examples of these
pairings, explains how they naturally arise, and formulates various associated
problems.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:00:36 GMT"
}
] | 2008-04-25T00:00:00 | [
[
"Eastwood",
"Michael G.",
""
]
] | [
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] |
711.3747 | Matti Ropo | M. Ropo, K. Kokko and L. Vitos | Proving the Perdew-Burke-Ernzerhof density functional designed for
metallic bulk and surface systems | 12 pages, 1 figure | null | 10.1103/PhysRevB.77.195445 | null | cond-mat.mtrl-sci | null | We test the accuracy of the revised Perdew-Burke-Ernzerhof
exchange-correlation density functional (PBEsol) for metallic bulk and surface
systems. It is shown that, on average, PBEsol yields equilibrium volumes and
bulk moduli in close agreement with the former generalized gradient
approximation (PBE) and two gradient level functionals derived from model
system approach (LAG and AM05). On the other hand, for close-packed metal
surfaces, PBEsol has the same performance as AM05, giving significantly larger
surface energies than PBE and LAG.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:01:27 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Mar 2008 09:02:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ropo",
"M.",
""
],
[
"Kokko",
"K.",
""
],
[
"Vitos",
"L.",
""
]
] | [
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711.3748 | Balazs Dora | B. D\'ora, K. Ziegler, P. Thalmeier | On the effect of weak disorder on the density of states in graphene | 7 pages, 5 figures | Phys. Rev. B 77, 115422 (2008) | 10.1103/PhysRevB.77.115422 | null | cond-mat.mes-hall cond-mat.str-el | null | The effect of weak potential and bond disorder on the density of states of
graphene is studied. By comparing the self-consistent non-crossing
approximation on the honeycomb lattice with perturbation theory on the Dirac
fermions, we conclude, that the linear density of states of pure graphene
changes to a non-universal power-law, whose exponent depends on the strength of
disorder like 1-4g/sqrt{3}t^2\pi, with g the variance of the Gaussian disorder,
t the hopping integral. This can result in a significant suppression of the
exponent of the density of states in the weak-disorder limit. We argue, that
even a non-linear density of states can result in a conductivity being
proportional to the number of charge carriers, in accordance with experimental
findings.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:08:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dóra",
"B.",
""
],
[
"Ziegler",
"K.",
""
],
[
"Thalmeier",
"P.",
""
]
] | [
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] |
711.3749 | Gunter Scharf | G. Scharf | From massive gravity to dark matter density | 10 pages, further clarification, better numerical results | null | null | null | hep-th | null | Massive gravity previously constructed as the spin-2 quantum gauge theory is
studied in the classical limit. The vector-graviton field v which does not
decouple in the limit of vanishing graviton mass gives rise to a modification
of general relativity. The modified Schwarzschild solution contains a
contribution which can be interpreted as the dark mass density. We calculate
the density profile in the simplest spherically symmetric geometry.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:10:25 GMT"
},
{
"version": "v2",
"created": "Mon, 26 Nov 2007 13:57:23 GMT"
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"version": "v3",
"created": "Thu, 6 Dec 2007 15:29:15 GMT"
},
{
"version": "v4",
"created": "Mon, 24 Dec 2007 08:37:12 GMT"
},
{
"version": "v5",
"created": "Sat, 1 Mar 2008 14:32:41 GMT"
},
{
"version": "v6",
"created": "Mon, 28 Apr 2008 11:24:36 GMT"
}
] | 2008-04-28T00:00:00 | [
[
"Scharf",
"G.",
""
]
] | [
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] |
711.375 | Yurij Holovatch | V. Blavats'ka, C. von Ferber, Yu. Holovatch | Star polymers in correlated disorder | Submitted to the Proceedings of the International Conference "Path
Integrals - New Trends and Perspectives", September 23-28, 2007, Dresden,
Germany | null | 10.1142/9789812837271_0081 | null | cond-mat.soft cond-mat.dis-nn | null | We analyze the impact of a porous medium (structural disorder) on the scaling
of the partition function of a star polymer immersed in a good solvent. We show
that corresponding scaling exponents change if the disorder is
long-range-correlated and calculate the exponents in the new universality
class. A notable finding is that star and chain polymers react in qualitatively
different manner on the presence of disorder: the corresponding scaling
exponents increase for chains and decrease for stars. We discuss the physical
consequences of this difference.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:10:31 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Blavats'ka",
"V.",
""
],
[
"von Ferber",
"C.",
""
],
[
"Holovatch",
"Yu.",
""
]
] | [
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] |
711.3751 | Frank Simon | Frank Simon, James Kelsey, Michael Kohl, Richard Majka, Miroslav
Plesko, David Underwood, Tai Sakuma, Nikolai Smirnov, Harold Spinka and Bernd
Surrow | Triple GEM Detectors for the Forward Tracker in STAR | 5 pages, 8 figures, presented at the IEEE Nuclear Science Symposium
in Honolulu, HI, USA, October 27 - November 3, 2007 | null | 10.1109/NSSMIC.2007.4436321 | null | physics.ins-det | null | Future measurements of the flavor-separated spin structure of the proton via
parity-violating W boson production at RHIC require an upgrade of the forward
tracking system of the STAR detector. This upgrade will allow the
reconstruction of the charge sign of electrons and positrons produced from
decaying W bosons. A design based on six large area triple GEM disks using GEM
foils produced by Tech-Etch Inc. has emerged as a cost-effective solution to
provide the necessary tracking precision. We report first results from a beam
test of three test detectors using Tech-Etch produced GEM foils and a laser
etched two dimensional strip readout. The detectors show good operational
stability, high efficiency and a spacial resolution of around 70 um or better,
exceeding the requirements for the forward tracking upgrade. The influence of
the angle of incidence of the particles on the spatial resolution of the
detectors has also been studied in detail.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:16:14 GMT"
}
] | 2016-11-17T00:00:00 | [
[
"Simon",
"Frank",
""
],
[
"Kelsey",
"James",
""
],
[
"Kohl",
"Michael",
""
],
[
"Majka",
"Richard",
""
],
[
"Plesko",
"Miroslav",
""
],
[
"Underwood",
"David",
""
],
[
"Sakuma",
"Tai",
""
],
[
"Smirnov",
"Nikolai",
""
],
[
"Spinka",
"Harold",
""
],
[
"Surrow",
"Bernd",
""
]
] | [
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] |
711.3752 | Vakhtang Rostiashvili | Swati Bhattacharya, Hsiao-Ping Hsu, Andrey Milchev, Vakhtang G.
Rostiashvili, Thomas A. Vilgis | Adsorption of Multi-block and Random Copolymer on a Solid Surface:
Critical Behavior and Phase Diagram | 27 pages, 12 figures | Macromolecules 41, 2920-2930 (2008) | 10.1021/ma702608j | null | cond-mat.soft cond-mat.stat-mech | null | The adsorption of a single multi-block $AB$-copolymer on a solid planar
substrate is investigated by means of computer simulations and scaling
analysis. It is shown that the problem can be mapped onto an effective
homopolymer adsorption problem. In particular we discuss how the critical
adsorption energy and the fraction of adsorbed monomers depend on the block
length $M$ of sticking monomers $A$, and on the total length $N$ of the polymer
chains. Also the adsorption of the random copolymers is considered and found to
be well described within the framework of the annealed approximation. For a
better test of our theoretical prediction, two different Monte Carlo (MC)
simulation methods were employed: a) off-lattice dynamic bead-spring model,
based on the standard Metropolis algorithm (MA), and b) coarse-grained lattice
model using the Pruned-enriched Rosenbluth method (PERM) which enables tests
for very long chains. The findings of both methods are fully consistent and in
good agreement with theoretical predictions.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 15:40:38 GMT"
}
] | 2008-06-27T00:00:00 | [
[
"Bhattacharya",
"Swati",
""
],
[
"Hsu",
"Hsiao-Ping",
""
],
[
"Milchev",
"Andrey",
""
],
[
"Rostiashvili",
"Vakhtang G.",
""
],
[
"Vilgis",
"Thomas A.",
""
]
] | [
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] |
711.3753 | Rhaana L. C. Starling | R.L.C. Starling (1), P.T. O'Brien, R. Willingale, K.L. Page, J.P.
Osborne, M. De Pasquale, Y.E. Nakagawa, N.P.M. Kuin, K. Onda, J.P. Norris,
T.N. Ukwatta, N. Kodaka, D.N. Burrows, J.A. Kennea, M.J. Page, M. Perri and
C.B. Markwardt ((1) University of Leicester, UK) | Swift captures the spectrally evolving prompt emission of GRB 070616 | 13 pages, 11 figures (2 in colour), MNRAS accepted | null | 10.1111/j.1365-2966.2007.12763.x | null | astro-ph | null | The origins of Gamma-ray Burst prompt emission are currently not well
understood and in this context long, well-observed events are particularly
important to study. We present the case of GRB 070616, analysing the
exceptionally long-duration multipeaked prompt emission, and later afterglow,
captured by all the instruments on-board Swift and by Suzaku WAM. The high
energy light curve remained generally flat for several hundred seconds before
going into a steep decline. Spectral evolution from hard to soft is clearly
taking place throughout the prompt emission, beginning at 285 s after the
trigger and extending to 1200 s. We track the movement of the spectral peak
energy, whilst observing a softening of the low energy spectral slope. The
steep decline in flux may be caused by a combination of this strong spectral
evolution and the curvature effect. We investigate origins for the spectral
evolution, ruling out a superposition of two power laws and considering instead
an additional component dominant during the late prompt emission. We also
discuss origins for the early optical emission and the physics of the
afterglow. The case of GRB 070616 clearly demonstrates that both broadband
coverage and good time resolution are crucial to pin down the origins of the
complex prompt emission in GRBs.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:07:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Starling",
"R. L. C.",
"",
"University of Leicester, UK"
],
[
"O'Brien",
"P. T.",
""
],
[
"Willingale",
"R.",
""
],
[
"Page",
"K. L.",
""
],
[
"Osborne",
"J. P.",
""
],
[
"De Pasquale",
"M.",
""
],
[
"Nakagawa",
"Y. E.",
""
],
[
"Kuin",
"N. P. M.",
""
],
[
"Onda",
"K.",
""
],
[
"Norris",
"J. P.",
""
],
[
"Ukwatta",
"T. N.",
""
],
[
"Kodaka",
"N.",
""
],
[
"Burrows",
"D. N.",
""
],
[
"Kennea",
"J. A.",
""
],
[
"Page",
"M. J.",
""
],
[
"Perri",
"M.",
""
],
[
"Markwardt",
"C. B.",
""
]
] | [
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] |
711.3754 | St\'ephane Schanne | S. Schanne, B. Cordier, D. Gotz, A. Gros, P. Kestener, H. Le Provost,
B. L'Huillier, M. Mur | The trigger function of the space borne gamma-ray burst telescope
ECLAIRs | 4 pages, proceedings of the "30^th International Cosmic Ray
Conference (ICRC)", 3-12 July 2007, Merida, Yucatan, Mexico | null | null | null | astro-ph | null | Gamma-ray bursts (GRB) sign energetic explosions in the Universe, occurring
at cosmological distances. Multi-wavelength observations of GRB allow to study
their properties and to use them as cosmological tools. In 2012 the space borne
gamma-ray telescope ECLAIRs is expected to provide accurate GRB localizations
on the sky in near real-time, necessary for ground-based follow-up
observations. Led by CEA Saclay, France, the project is currently in its
technical design phase. ECLAIRs is optimized to detect highly red-shifted GRB
thanks to a 4 keV low energy threshold. A coded mask telescope with a 1024 cm^2
detection plane of 80x80 CdTe pixels permanently observes a 2 sr sky field. The
on-board trigger detects GRB using count-rate increase monitors on multiple
time-scales and cyclic images. It computes sky images in the 4-50 keV energy
range by de-convolving detector plane images with the mask pattern and
localizes newly detected sources with <10 arcmin accuracy. While individual GRB
photons are available hours later, GRB alerts are transmitted over a VHF
network within seconds to ground, in particular to robotic follow-up
telescopes, which refine GRB localizations to the level needed by large
spectroscopic telescopes. This paper describes the ECLAIRs concept, with
emphasis on the GRB triggering scheme.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:08:34 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Schanne",
"S.",
""
],
[
"Cordier",
"B.",
""
],
[
"Gotz",
"D.",
""
],
[
"Gros",
"A.",
""
],
[
"Kestener",
"P.",
""
],
[
"Provost",
"H. Le",
""
],
[
"L'Huillier",
"B.",
""
],
[
"Mur",
"M.",
""
]
] | [
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] |
711.3755 | Frank Close Prof | T.J.Burns and F.E.Close | Hadron production in $\psi$, $\eta_c$ and $\chi$ decays | null | null | null | null | hep-ph | null | We derive relations among branching fractions in the exclusive decay of
charmonia to light flavour meson pairs assuming factorization between the quark
spin and spatial degrees of freedom. With the further assumption that these
amplitudes can be described by flux-tube models, we assess prospects for
production of hybrid mesons in charmonium decays.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:10:51 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Burns",
"T. J.",
""
],
[
"Close",
"F. E.",
""
]
] | [
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] |
711.3756 | Erhard Seiler | Max Niedermaier, Erhard Seiler | On the large N expansion in hyperbolic sigma-models | 15 pages. Some changes in introduction and discussion; to appear in
J. Math. Phys | J.Math.Phys.49:073301,2008 | 10.1063/1.2951886 | ESI preprint 1979 | math-ph hep-lat hep-th math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Invariant correlation functions for ${\rm SO}(1,N)$ hyperbolic sigma-models
are investigated. The existence of a large $N$ asymptotic expansion is proven
on finite lattices of dimension $d \geq 2$. The unique saddle point
configuration is characterized by a negative gap vanishing at least like 1/V
with the volume. Technical difficulties compared to the compact case are
bypassed using horospherical coordinates and the matrix-tree theorem.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:15:38 GMT"
},
{
"version": "v2",
"created": "Fri, 27 Jun 2008 11:48:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Niedermaier",
"Max",
""
],
[
"Seiler",
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""
]
] | [
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] |
711.3757 | Rob Heylen | D. Boll\'e, R. Heylen | Small-world hypergraphs on a bond-disordered Bethe lattice | 9 pages, 4 figures | null | 10.1103/PhysRevE.77.046104 | null | cond-mat.stat-mech cond-mat.dis-nn | null | We study the thermodynamic properties of spin systems with bond-disorder on
small-world hypergraphs, obtained by superimposing a one-dimensional Ising
chain onto a random Bethe graph with p-spin interactions. Using transfer-matrix
techniques, we derive fixed-point equations describing the relevant order
parameters and the free energy, both in the replica symmetric and one step
replica symmetry breaking approximation. We determine the static and dynamic
ferromagnetic transition and the spinglass transition within replica symmetry
for all temperatures, and demonstrate corrections to these results when one
step replica symmetry breaking is taken into account. The results obtained are
in agreement with Monte-Carlo simulations.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:16:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bollé",
"D.",
""
],
[
"Heylen",
"R.",
""
]
] | [
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711.3758 | Sebastiano Calchi Novati | S. Calchi Novati (1,2), F. De Luca (3), Ph. Jetzer (3), L. Mancini
(1,2) G. Scarpetta (1,2) ((1) University of Salerno, (2) INFN, Napoli, (3)
University of Zurich) | Microlensing constraints on the Galactic Bulge Initial Mass Function | A&A in press - Minor changes to match the published version | Astron.Astrophys.480:723-733,2008 | 10.1051/0004-6361:20078439 | null | astro-ph | null | Aims. We seek to probe the Galactic bulge IMF starting from microlensing
observations. Methods. We analyse the recent results of the microlensing
campaigns carried out towards the Galactic bulge presented by the EROS, MACHO
and OGLE collaborations. In particular, we study the duration distribution of
the events. We assume a power law initial mass function, $\xi(\mu)\propto
\mu^{-\alpha}$, and we study the slope $\alpha$ both in the brown dwarf and in
the main sequence ranges. Moreover, we compare the observed and expected
optical depth profiles. Results. The values of the mass function slopes are
strongly driven by the observed timescales of the microlensing events. The
analysis of the MACHO data set gives, for the main sequence stars, $\alpha=1.7
\pm 0.5$, compatible with the result we obtain with the EROS and OGLE data
sets, and a similar, though less constrained slope for brown dwarfs. The lack
of short duration events in both EROS and OGLE data sets, on the other hand,
only allows the determination of an \emph{upper} limit in this range of masses,
making the overall result less robust. The optical depth analysis gives a very
good agreement between the observed and the expected values, and we show that
the available data do not allow one to discriminate between different bulge
models.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:23:20 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Mar 2008 08:17:56 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Novati",
"S. Calchi",
""
],
[
"De Luca",
"F.",
""
],
[
"Jetzer",
"Ph.",
""
],
[
"Mancini",
"L.",
""
],
[
"Scarpetta",
"G.",
""
]
] | [
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] |
711.3759 | Raquel Mallavibarrena | Antonio Lanteri and Raquel Mallavibarrena | Osculating properties of decomposable scrolls | 18 pages, to appear in Math. Nachr | null | null | null | math.AG math.DG | null | Osculating spaces of decomposable scrolls (of any genus and not necessarily
normal)are studied and their inflectional loci are related to those of their
generating curves by using systematically an idea introduced by Piene and
Sacchiero in the setting of rational normal scrolls. In this broader setting
the extra components of the second discriminant locus - deriving from flexes -
are investigated and a new class of uninflected surface scrolls is presented
and characterized. Further properties related to osculation are discussed for
(not necessarily decomposable) scrolls.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:25:25 GMT"
}
] | 2015-03-13T00:00:00 | [
[
"Lanteri",
"Antonio",
""
],
[
"Mallavibarrena",
"Raquel",
""
]
] | [
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711.376 | Markos Maniatis | M. Maniatis, A. von Manteuffel, O. Nachtmann | A new type of CP symmetry, family replication and fermion mass
hierarchies | 24 pages. Version published in EPJC. Minor changes as suggested by
the referee | Eur.Phys.J.C57:739-762,2008 | 10.1140/epjc/s10052-008-0726-z | HD-THEP-07-30 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study a two-Higgs-doublet model with four generalised CP symmetries in the
scalar sector. Electroweak symmetry breaking leads automatically to spontaneous
breaking of two of them. We require that these four CP symmetries can be
extended from the scalar sector to the full Lagrangian and call this
requirement the principle of maximal CP invariance. The Yukawa interactions of
the fermions are severely restricted by this requirement. In particular, a
single fermion family cannot be coupled to the Higgs fields. For two fermion
families, however, this is possible. Enforcing the absence of flavour-changing
neutral currents, we find degenerate masses in both families or one family
massless and one massive. In the latter case the Lagrangian is highly
symmetric, with the mass hierarchy being generated by electroweak symmetry
breaking. Adding a third family uncoupled to the Higgs fields and thus keeping
it massless we get a model which gives a rough approximation of some features
of the fermions observed in Nature. We discuss a number of predictions of the
model which may be checked in future experiments at the LHC.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 20:23:40 GMT"
},
{
"version": "v2",
"created": "Mon, 27 Oct 2008 14:16:37 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Maniatis",
"M.",
""
],
[
"von Manteuffel",
"A.",
""
],
[
"Nachtmann",
"O.",
""
]
] | [
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-0.0447587892,
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] |
711.3761 | Massimo Di Toro | J. Rizzo, M. Colonna, V. Baran, M. Di Toro, H.H. Wolter, M.
Zielinska-Pfabe | Isospin Dynamics in Peripheral Heavy Ion Collisions at Fermi Energies | 34 pages, 15 figures, Nucl.Phys. A, in press | null | 10.1016/j.nuclphysa.2008.02.307 | null | nucl-th | null | We present a detailed study of isospin dynamics in peripheral collisions at
Fermi energies. We consider symmetric and mixed collisions of (124,112)Sn
isotopes at 35 and 50 AMeV to study the isospin transport between the different
reaction components (residues, gas and possibly intermediate mass fragments)
and, in particular, the charge equilibration in the mixed system. We evaluate
the effects of drift terms due to asymmetry and density gradients, which are
directly related to the poorly known value and slope of the symmetry energy
below saturation density. We verify the importance of an isoscalar momentum
dependence of the mean field, which is found to influence the isospin transport
since it changes the reaction times. We finally suggest two observables
particularly sensitive to the isovector part of the nuclear equation-of-state:
the correlation between isospin equilibration and kinetic energy loss for
binary events, and the isospin content of the produced mid-rapidity fragments
for neck fragmentation events.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:33:17 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 16:12:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rizzo",
"J.",
""
],
[
"Colonna",
"M.",
""
],
[
"Baran",
"V.",
""
],
[
"Di Toro",
"M.",
""
],
[
"Wolter",
"H. H.",
""
],
[
"Zielinska-Pfabe",
"M.",
""
]
] | [
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711.3762 | Oliver Muelken | Oliver Muelken, Volker Pernice, Alexander Blumen | Universal Behavior of Quantum Walks with Long-Range Steps | 4 pages, 3 figures | Phys. Rev. E 77, 021117 (2008) | 10.1103/PhysRevE.77.021117 | null | quant-ph cond-mat.stat-mech | null | Quantum walks with long-range steps $R^{-\gamma}$ ($R$ being the distance
between sites) on a discrete line behave in similar ways for all $\gamma\geq2$.
This is in contrast to classical random walks, which for $\gamma >3$ belong to
a different universality class than for $\gamma \leq 3$. We show that the
average probabilities to be at the initial site after time $t$ as well as the
mean square displacements are of the same functional form for quantum walks
with $\gamma=2$, 4, and with nearest neighbor steps. We interpolate this result
to arbitrary $\gamma\geq2$.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:33:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Muelken",
"Oliver",
""
],
[
"Pernice",
"Volker",
""
],
[
"Blumen",
"Alexander",
""
]
] | [
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] |
711.3763 | Johannes Schmude | Johannes Schmude | The quark-gluon plasma and D6-branes on the conifold | 41 pages, 9 figures; minor corrections; discussion of
Bekenstein-Hawking entropy | null | null | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the possibility of constructing a supergravity background dual
to the quark-gluon plasma using D6-branes wrapping a three-cycle in the
deformed conifold. The UV-completion of this setup is given by M-theory on a G2
holonomy manifold. For the class of metrics considered we find that there are
only non-extremal D-brane solutions in the limit of the singular conifold with
the singularity being resolved by the D-brane horizon. The thermodynamic
properties of the system show some puzzling features, such as negative specific
heat at an unusual behavior of the entropy. Among the properties of the plasma
studied using this holographic dual are the quark-antiquark potential, the
shear viscosity and parton energy loss. While one finds the expected behavior
for the potential and the viscosity -- deconfinement and the universal
shear-viscosity to entropy ratio -- both the jet quenching parameter and the
calculation of the drag force lead us to the conclusion that there is no parton
energy loss in the dual plasma. Our results indicate that the background
constructed is not dual to a realistic QGP, yet we argue that this should
improve upon inclusion of the three-form gauge potential in the
eleven-dimensional background.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:38:33 GMT"
},
{
"version": "v2",
"created": "Thu, 31 Jul 2008 22:58:54 GMT"
},
{
"version": "v3",
"created": "Fri, 28 Nov 2008 15:24:10 GMT"
}
] | 2008-11-28T00:00:00 | [
[
"Schmude",
"Johannes",
""
]
] | [
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] |
711.3764 | Christof Kuelske | C. Kuelske, A. A. Opoku | The Posterior metric and the Goodness of Gibbsianness for transforms of
Gibbs measures | 32 pages | null | null | null | math.PR math-ph math.MP | null | We present a general method to derive continuity estimates for conditional
probabilities of general (possibly continuous) spin models sub jected to local
transformations. Such systems arise in the study of a stochastic time-evolution
of Gibbs measures or as noisy observations. We exhibit the minimal necessary
structure for such double-layer systems. Assuming no a priori metric on the
local state spaces, we define the posterior metric on the local image space. We
show that it allows in a natural way to divide the local part of the continuity
estimates from the spatial part (which is treated by Dobrushin uniqueness
here). We show in the concrete example of the time evolution of rotators on the
q-1 dimensional sphere how this method can be used to obtain estimates in terms
of the familiar Euclidean metric.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:49:17 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Kuelske",
"C.",
""
],
[
"Opoku",
"A. A.",
""
]
] | [
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] |
711.3765 | Artin Armagan | Russell Zaretzki and Michael A. Gilchrist and William M. Briggs and
Artin Armagan | MCMC Inference for a Model with Sampling Bias: An Illustration using
SAGE data | null | null | null | null | stat.AP | null | This paper explores Bayesian inference for a biased sampling model in
situations where the population of interest cannot be sampled directly, but
rather through an indirect and inherently biased method. Observations are
viewed as being the result of a multinomial sampling process from a tagged
population which is, in turn, a biased sample from the original population of
interest. This paper presents several Gibbs Sampling techniques to estimate the
joint posterior distribution of the original population based on the observed
counts of the tagged population. These algorithms efficiently sample from the
joint posterior distribution of a very large multinomial parameter vector.
Samples from this method can be used to generate both joint and marginal
posterior inferences. We also present an iterative optimization procedure based
upon the conditional distributions of the Gibbs Sampler which directly computes
the mode of the posterior distribution. To illustrate our approach, we apply it
to a tagged population of messanger RNAs (mRNA) generated using a common
high-throughput technique, Serial Analysis of Gene Expression (SAGE).
Inferences for the mRNA expression levels in the yeast Saccharomyces cerevisiae
are reported.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:48:11 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Zaretzki",
"Russell",
""
],
[
"Gilchrist",
"Michael A.",
""
],
[
"Briggs",
"William M.",
""
],
[
"Armagan",
"Artin",
""
]
] | [
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] |
711.3766 | Panayiotis Varotsos | P.A. Varotsos, N.V. Sarlis, E.S. Skordas | Seismic Electric Signals and 1/f "noise" in natural time | 15 pages | null | null | null | cond-mat.stat-mech | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | By making use of the concept of natural time, a simple model is proposed
which exhibits the $1/f^a$ behavior with $a$ close to unity. The properties of
the model are compared to those of the Seismic Electric Signals (SES)
activities that have been found to obey the ubiquitous $1/f^a$ behavior with $a
\approx 1$. This comparison, which is made by using the most recent SES data,
reveals certain similarities, but the following important difference is found:
The model suggests that the entropy $S_-$ under time reversal becomes larger
compared to the entropy $S$ in forward time, thus disagreeing with the
experimental SES results which show that $S$ may be either smaller or larger
than $S_-$. This might be due to the fact that SES activities exhibit {\em
critical} dynamics, while the model cannot capture all the characteristics of
such dynamics.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:52:38 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 17:28:30 GMT"
},
{
"version": "v3",
"created": "Fri, 1 Feb 2008 08:14:29 GMT"
},
{
"version": "v4",
"created": "Fri, 24 Oct 2008 13:22:07 GMT"
},
{
"version": "v5",
"created": "Sun, 7 Dec 2008 17:02:25 GMT"
}
] | 2008-12-07T00:00:00 | [
[
"Varotsos",
"P. A.",
""
],
[
"Sarlis",
"N. V.",
""
],
[
"Skordas",
"E. S.",
""
]
] | [
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] |
711.3767 | Rafael Pepino | Evgueny Kochetov, Alvaro Ferraz and Rafael T. Pepino | Low-energy effective representation of the Gutzwiller-projected BCS
Hamiltonian close to half filling | null | null | 10.1142/9789812837271_0066 | null | cond-mat.str-el | null | We investigate analytically a connection between the t-J model and the
strongly correlated Bardeen-Cooper-Schrieffer (BCS) Hamiltonian, with the
effect of strong electron correlations accounted by the Gutzwiller projection.
We show that in the immediate vicinity of half filling the projected 2D BCS
Hamiltonian with strong pairing develops an antiferromagnetically (AF) ordered
ground state. This result explicitly demonstrates that antiferromagnetism in
this model appears as a natural consequence of the strong Coulomb repulsion in
a low doped regime. At moderate doping the ground state of the
Gutzwiller-projected BCS Hamiltonian becomes qualitatively similar to
Anderson's resonating valence bond state which is known to fit nicely the
properties of the t-J model in this regime. These two properties taken together
indicate that the projected BCS Hamiltonian captures the essential low-energy
physics of the t-J model in the whole underdoped region.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 16:55:04 GMT"
}
] | 2017-08-23T00:00:00 | [
[
"Kochetov",
"Evgueny",
""
],
[
"Ferraz",
"Alvaro",
""
],
[
"Pepino",
"Rafael T.",
""
]
] | [
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] |
711.3768 | Jarno Talponen | Jarno Talponen | Convex-transitivity and function spaces | Corrected version | null | null | null | math.FA | null | If X is a convex-transitive Banach space and 1\leq p\leq \infty then the
closed linear span of the simple functions in the Bochner space L^{p}([0,1],X)
is convex-transitive. If H is an infinite-dimensional Hilbert space and
C_{0}(L) is convex-transitive, then C_{0}(L,H) is convex-transitive. Some new
fairly concrete examples of convex-transitive spaces are provided.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:03:13 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Jan 2008 14:04:00 GMT"
}
] | 2008-01-28T00:00:00 | [
[
"Talponen",
"Jarno",
""
]
] | [
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] |
711.3769 | Alexander N. Poddubny | A.N. Poddubny, L. Pilozzi, M.M. Voronov, and E.L. Ivchenko | Resonant Fibonacci Quantum Well Structures | 5 pages, 3 figures, submitted to Phys. Rev. B | null | 10.1103/PhysRevB.77.113306 | null | cond-mat.mes-hall | null | We propose a resonant one-dimensional quasicrystal, namely, a multiple
quantum well (MQW) structure satisfying the Fibonacci-chain rule with the
golden ratio between the long and short inter-well distances. The resonant
Bragg condition is generalized from the periodic to Fibonacci MQWs. A
dispersion equation for exciton-polaritons is derived in the two-wave
approximation, the effective allowed and forbidden bands are found. The
reflection spectra from the proposed structures are calculated as a function of
the well number and detuning from the Bragg condition.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:16:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Poddubny",
"A. N.",
""
],
[
"Pilozzi",
"L.",
""
],
[
"Voronov",
"M. M.",
""
],
[
"Ivchenko",
"E. L.",
""
]
] | [
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] |
711.377 | Vladimir Ivashchuk | J.-M. Alimi, V.D. Ivashchuk and V.N. Melnikov | An S-brane solution with acceleration and small enough variation of G | 5 pages, Latex, journal version | Grav.Cosmol.13:137-141,2007 | null | IGC-PFUR/07-05/01 | gr-qc astro-ph hep-th | null | An S-brane solution with two non-composite electric branes and a set of l
scalar fields is considered. The intersection rule for branes corresponds to
the Lie algebra A_2. The solution contains five factor spaces with the fifth
one interpreted as ``our'' 3-dimensional space. It is shown that there exists a
time interval where accelerating expansion of ``our'' 3-dimensional space is
compatible with small enough value of effective gravitational ``constant''
variation.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:24:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Alimi",
"J. -M.",
""
],
[
"Ivashchuk",
"V. D.",
""
],
[
"Melnikov",
"V. N.",
""
]
] | [
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711.3771 | Frederic P. Schuller | Raffaele Punzi, Frederic P. Schuller, Mattias N. R. Wohlfarth | Propagation of light in area metric backgrounds | 18pp, no figures, Journal version | Class.Quant.Grav.26:035024,2009 | 10.1088/0264-9381/26/3/035024 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The propagation of light in area metric spacetimes, which naturally emerge as
refined backgrounds in quantum electrodynamics and quantum gravity, is studied
from first principles. In the geometric-optical limit, light rays are found to
follow geodesics in a Finslerian geometry, with the Finsler norm being
determined by the area metric tensor. Based on this result, and an
understanding of the non-linear relation between ray vectors and wave covectors
in such refined backgrounds, we study light deflection in spherically symmetric
situations, and obtain experimental bounds on the non-metricity of spacetime in
the solar system.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:30:26 GMT"
},
{
"version": "v2",
"created": "Tue, 20 Jan 2009 22:59:21 GMT"
}
] | 2009-01-28T00:00:00 | [
[
"Punzi",
"Raffaele",
""
],
[
"Schuller",
"Frederic P.",
""
],
[
"Wohlfarth",
"Mattias N. R.",
""
]
] | [
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] |
711.3772 | Ramin Golestanian | Ramin Golestanian | Three-Sphere Low Reynolds Number Swimmer with a Cargo Container | 4 pages, 1 figure | Euro. Phys. J. E 25, 1 (2008) | 10.1140/epje/i2007-10276-2 | null | cond-mat.soft cond-mat.stat-mech | null | A recently introduced model for an autonomous swimmer at low Reynolds number
that is comprised of three spheres connected by two arms is considered when one
of the spheres has a large radius. The Stokes hydrodynamic flow associated with
the swimming strokes and net motion of this system can be studied analytically
using the Stokes Green's function of a point force in front of a sphere of
arbitrary radius $R$ provided by Oseen. The swimming velocity is calculated,
and shown to scale as $1/R^3$ with the radius of the sphere.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:32:39 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Mar 2008 09:42:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Golestanian",
"Ramin",
""
]
] | [
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711.3773 | T. P. Singh | T. P. Singh (Tata Institute of Fundamental Research, Mumbai) | Quantum measurement and quantum gravity : many-worlds or collapse of the
wave-function? | 23 pages. Based on talks given at: [FTAGVI, HRI, Allahabad, 13-18
Nov. 2007]; [Himalayan Relativity Dialog, Mirik, April, 2007]; [Workshop
Session on Quantum Gravity, IAGRG, Delhi, Feb. 2007]; [Parmenides Workshop:
The present - perspectives from physics and philosophy, Wildbad Kreuth,
Germany, October, 2006]; [ICGC,Pune, Dec.2007] | J.Phys.Conf.Ser.174:012024,2009 | 10.1088/1742-6596/174/1/012024 | null | gr-qc hep-th quant-ph | null | At present, there are two possible, and equally plausible, explanations for
the physics of quantum measurement. The first explanation, known as the
many-worlds interpretation, does not require any modification of quantum
mechanics, and asserts that at the time of measurement the Universe splits into
many branches, one branch for every possible alternative. The various branches
do not interfere with each other because of decoherence, thus providing a
picture broadly consistent with the observed Universe. The second explanation,
which requires quantum mechanics to be modified from its presently known form,
is that at the time of measurement the wave-function collapses into one of the
possible alternatives. The two explanations are mutually exclusive, and up
until now, no theoretical reasoning has been put forward to choose one
explanation over the other. In this article, we provide an argument which
implies that the collapse interpretation is favored over the many-worlds
interpretation. Our starting point is the assertion (which we justify) that
there ought to exist a reformulation of quantum mechanics which does not refer
to a classical spacetime manifold. The need for such a reformulation implies
that quantum theory becomes non-linear on the Planck mass/energy scale.
Standard linear quantum mechanics is an approximation to this non-linear
theory, valid at energy scales much smaller than the Planck scale. Using ideas
based on noncommutative differential geometry, we develop such a reformulation
and derive a non-linear Schr\"{o}dinger equation, which can explain collapse of
the wave-function. We also obtain an expression for the lifetime of a quantum
superposition. We suggest ideas for an experimental test of this model.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:44:08 GMT"
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] | 2009-07-24T00:00:00 | [
[
"Singh",
"T. P.",
"",
"Tata Institute of Fundamental Research, Mumbai"
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711.3774 | Tom Fisher | Tom Fisher | Finding rational points on elliptic curves using 6-descent and
12-descent | 33 pages | null | null | null | math.NT | null | We explain how recent work on 3-descent and 4-descent for elliptic curves
over Q can be combined to search for generators of the Mordell-Weil group of
large height. As an application we show that every elliptic curve of prime
conductor in the Stein-Watkins database has rank at least as large as predicted
by the conjecture of Birch and Swinnerton-Dyer.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:45:03 GMT"
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[
"Fisher",
"Tom",
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711.3775 | Gabriele Migliorini | G. Migliorini | The Critical Properties of Two-dimensional Oscillator Arrays | Contribution to the conference "Viewing the World through Spin
Glasses" in honour of Professor David Sherrington on the occasion of his 65th
birthday | null | 10.1088/1751-8113/41/32/324021 | null | cond-mat.stat-mech | null | We present a renormalization group study of two dimensional arrays of
oscillators, with dissipative, short range interactions. We consider the case
of non-identical oscillators, with distributed intrinsic frequencies within the
array and study the steady-state properties of the system. In two dimensions no
macroscopic mutual entrainment is found but, for identical oscillators,
critical behavior of the Berezinskii-Kosterlitz-Thouless type is shown to be
present. We then discuss the stability of (BKT) order in the physical case of
distributed quenched random frequencies. In order to do that, we show how the
steady-state dynamical properties of the two dimensional array of non-identical
oscillators are related to the equilibrium properties of the XY model with
quenched randomness, that has been already studied in the past. We propose a
novel set of recursion relations to study this system within the Migdal
Kadanoff renormalization group scheme, by mean of the discrete clock-state
formulation. We compute the phase diagram in the presence of random dissipative
coupling, at finite values of the clock state parameter. Possible experimental
applications in two dimensional arrays of microelectromechanical oscillators
are briefly suggested.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:46:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Migliorini",
"G.",
""
]
] | [
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] |
711.3776 | Guillaume Bossard | Laurent Baulieu (LPTHE), Guillaume Bossard (AEI) | Superconformal invariance from N=2 supersymmetry Ward identities | 17 pages | JHEP0802:075,2008 | 10.1088/1126-6708/2008/02/075 | null | hep-th | null | We algebraically prove the cancellation of the beta function at all order of
perturbation theory of N=2 supersymmetric gauge theories with a vanishing
one-loop beta function. The proof generalises that recently given for the N=4
case. It uses the consistent Slavnov-Taylor identities of the shadow dependent
formulation. We also demonstrate the cancellation at all orders of the
anomalous dimensions of vector and hypermultiplet one half BPS operators.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 17:59:05 GMT"
},
{
"version": "v2",
"created": "Mon, 4 Feb 2008 13:52:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Baulieu",
"Laurent",
"",
"LPTHE"
],
[
"Bossard",
"Guillaume",
"",
"AEI"
]
] | [
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] |
711.3777 | Mikhail Zverev | V.A. Khodel, V.M. Yakovenko, M.V. Zverev | Flattening of Single-Particle Spectra in Strongly Correlated Electron
Systems and the Violation of the Wiedemann-Franz Law | 6 pages, 5 figures, added references | JETP Letters 86, 772 (2007) | 10.1134/S0021364007240058 | null | cond-mat.str-el | null | The renormalization of the Wiedemann-Franz (WF) ratio in strongly correlated
electron systems is analyzed within the Landau quasiparticle picture. We
demonstrate that the WF law is violated: (i) at the quantum critical point,
where the effective mass diverges, and (ii) beyond a point of fermion
condensation, where the single-particle spectrum $\epsilon(p)$ becomes flat.
Results of the analysis are compared with available experimental data.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 18:04:07 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Dec 2007 21:13:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Khodel",
"V. A.",
""
],
[
"Yakovenko",
"V. M.",
""
],
[
"Zverev",
"M. V.",
""
]
] | [
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] |
711.3778 | Zhi L\"u | Zhi L\"u | Graphs of 2-torus actions | 12 pages with 3 figures. To appear in Contemporary Mathematics of AMS
(Proceedings of the International Conference on Toric Topology) | Contemp. Math. 460 (2008), 261-272. | null | null | math.CO math.AT | null | It has been known that an effective smooth $({\Bbb Z}_2)^k$-action on a
smooth connected closed manifold $M^n$ fixing a finite set can be associated to
a $({\Bbb Z}_2)^k$-colored regular graph. In this paper, we consider abstract
graphs $(\Gamma,\alpha)$ of $({\Bbb Z}_2)^k$-actions, called abstract
1-skeletons. We study when an abstract 1-skeleton is a colored graph of some
$({\Bbb Z}_2)^k$-action. We also study the existence of faces of an abstract
1-skeleton (note that faces often have certain geometric meanings if an
abstract 1-skeleton is a colored graph of some $({\Bbb Z}_2)^k$-action).
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 18:19:10 GMT"
},
{
"version": "v2",
"created": "Sun, 25 Nov 2007 04:07:03 GMT"
}
] | 2009-02-06T00:00:00 | [
[
"Lü",
"Zhi",
""
]
] | [
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711.3779 | Francesco Mainardi | Francesco Mainardi and Gianni Pagnini | The role of the Fox-Wright functions in fractional sub-diffusion of
distributed order | 18 pages. Conference "Special Functions: Asymptotic Analysis and
Computation", Santander (Spain) on 4-6 July, 2005 | Journal of Computational and Applied Mathematics: Vol 207, No 2,
pp.245-257 (2007) | null | null | math-ph cond-mat.stat-mech math.CV math.MP | null | The fundamental solution of the fractional diffusion equation of distributed
order in time (usually adopted for modelling sub-diffusion processes) is
obtained based on its Mellin-Barnes integral representation. Such solution is
proved to be related via a Laplace-type integral to the Fox-Wright functions. A
series expansion is also provided in order to point out the distribution of
time-scales related to the distribution of the fractional orders. The results
of the time fractional diffusion equation of a single order are also recalled
and then re-obtained from the general theory.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 18:16:59 GMT"
}
] | 2008-05-18T00:00:00 | [
[
"Mainardi",
"Francesco",
""
],
[
"Pagnini",
"Gianni",
""
]
] | [
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711.378 | Jules P. Halpern | J.P. Halpern, E.V. Gotthelf, J. Reynolds, S.M. Ransom, F. Camilo | Outburst of the 2 s Anomalous X-ray Pulsar 1E 1547.0-5408 | 7 pages, 5 figures, to appear in The Astrophysical Journal | null | 10.1086/527293 | null | astro-ph | null | Following our discovery of radio pulsations from the newly recognized
Anomalous X-ray Pulsar (AXP) 1E 1547.0-5408, we initiated X-ray monitoring with
the Swift X-ray Telescope, and obtained a single target-of-opportunity
observation with the Newton X-ray Multi-Mirror Mission (XMM-Newton). In
comparison with its historic minimum flux of 3e-13 ergs cm^-2 s^-1, the source
was found to be in a record high state, f_X(1-8 keV) = 5e-12 ergs cm^-2 s^-1,
or L_X = 1.7e35(d/9 kpc)^2 ergs s^-1, and declining by 25% in 1 month.
Extrapolating the decay, we bound the total energy in this outburst to 1e42 < E
< 1e43 ergs. The spectra (fitted with a Comptonized blackbody) show that an
increase in the temperature and area of a hot region, to 0.5 keV and ~16% of
the surface area of the neutron star, respectively, are primarily responsible
for its increase in luminosity. The energy, spectrum, and timescale of decay
are consistent with a deep crustal heating event, similar to an interpretation
of the X-ray turn-on of the transient AXP XTE J1810-197. Simultaneous with the
4.6 hour XMM-Newton observation, we observed at 6.4 GHz with the Parkes
telescope, measuring the phase relationship of the radio and X-ray pulse. The
X-ray pulsed fraction of 1E 1547.0-5408 is only ~7%, while its radio pulse is
relatively broad for such a slow pulsar, which may indicate a nearly aligned
rotator. As also inferred from the transient behavior of XTE J1810-197, the
only other AXP known to emit in the radio, the magnetic field rearrangement
responsible for this X-ray outburst of 1E 1547.0-5408 is probably the cause of
its radio turn-on.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 18:41:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Halpern",
"J. P.",
""
],
[
"Gotthelf",
"E. V.",
""
],
[
"Reynolds",
"J.",
""
],
[
"Ransom",
"S. M.",
""
],
[
"Camilo",
"F.",
""
]
] | [
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] |
711.3781 | Giuseppe De Risi | G. De Risi | Bouncing cosmology from Kalb-Ramond Braneworld | 14 pages, 3 figures. references added. Matches the published version | Phys.Rev.D77:044030,2008 | 10.1103/PhysRevD.77.044030 | null | hep-th gr-qc | null | We consider a 3-brane embedded in a warped 5-dimensional background with a
dilaton and a Kalb-Ramond 2-form. We show that it is possible to find static
solutions of the form of charged dS/AdS-like black hole with horizon which
could have a negative mass parameter. The motion of the 3-brane in this bulk
generates an effective 4-dimensional bouncing cosmology induced by the negative
dark radiation term. This model avoids the instability that arises for bouncing
brane in a Reissner-Nordstr{\o}m-AdS bulk.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 18:54:44 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Mar 2008 11:45:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"De Risi",
"G.",
""
]
] | [
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] |
711.3782 | Gabriel Vigny | Gabriel Vigny | Lelong-Skoda transform for compact Kaehler manifolds and
self-intersection inequalities | 15 pages | null | null | null | math.CV | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $X$ be a compact Kaehler manifold of dimension $k$ and $T$ be a positive
closed current on $X$ of bidimension $(p,p)$ ($1\leq p < k-1$). We construct a
continuous linear transform $\mathcal{L}_p(T)$ of $T$ which is a positive
closed current on $X$ of bidimension $(k-1,k-1)$ which has the same Lelong
numbers as $T$. We deduce from that construction self-intersection inequalities
for positive closed currents of any bidegree.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 19:25:19 GMT"
},
{
"version": "v2",
"created": "Tue, 17 Dec 2019 10:20:20 GMT"
}
] | 2019-12-18T00:00:00 | [
[
"Vigny",
"Gabriel",
""
]
] | [
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711.3783 | Maria Fernanda Nieva Dr. | M.F. Nieva and N. Przybilla | Carbon abundances of early B-type stars in the solar vicinity. Non-LTE
line-formation for C II/III/IV and self-consistent atmospheric parameters | 25 pages, 22 figures. Accepted for publication in A&A | null | 10.1051/0004-6361:20078203 | null | astro-ph | null | Precise determinations of the chemical composition in early B-type stars
consitute fundamental observational constraints on stellar and galactochemical
evolution. Carbon is one of the most abundant metals in the Universe but
analyses in early-type stars show inconclusive results, like large
discrepancies between analyses of different lines in C II, a failure to
establish the C II/III ionization balance and the derivation of systematically
lower abundances than from other objects. We present a comprehensive and robust
C II/III/IV model for non-LTE line-formation calculations based on carefully
selected atomic data. The model is calibrated with high-S/N spectra of six
apparently slow-rotating early B-type dwarfs and giants, which cover a wide
parameter range and are randomly distributed in the solar neighbourhood. A
self-consistent quantitative spectrum analysis is performed using an extensive
iteration scheme to determine stellar atmospheric parameters and to select the
appropriate atomic data used for the derivation of chemical abundances. We
establish the carbon ionization balance for all sample stars based on a unique
set of input atomic data, achieving consistency for all modelled lines. Highly
accurate atmospheric parameters and a homogeneous carbon abundance with reduced
systematic errors are derived. This results in a present-day stellar carbon
abundance in the solar neighbourhood, which is in good agreement with recent
determinations of the solar value and with the gas-phase abundance of the Orion
H II region. The homogeneous present-day carbon abundance also conforms with
predictions of chemical-evolution models for the Galaxy. The present approach
allows us to constrain the effects of systematic errors on fundamental
parameters and abundances. (abridged)
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 20:17:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nieva",
"M. F.",
""
],
[
"Przybilla",
"N.",
""
]
] | [
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] |
711.3784 | Masumi Nakajima | Masumi Nakajima | The Lindelof Hypothesis for almost all Hurwitz's Zeta-Functions holds
True | 16 pages. | null | null | null | math.GM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | By Probability theory, that is, by a kind of quasi-law of the iterated
logarithm, we prove the title claim.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 19:48:11 GMT"
},
{
"version": "v2",
"created": "Sat, 20 Mar 2010 02:29:12 GMT"
}
] | 2010-03-23T00:00:00 | [
[
"Nakajima",
"Masumi",
""
]
] | [
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711.3785 | Patrick Dehornoy | Lorenzo Carlucci, Patrick Dehornoy (LMNO), Andreas Weiermann | Unprovability results involving braids | 32 pages | null | 10.1112/plms/pdq016 | null | math.LO | null | We construct long sequences of braids that are descending with respect to the
standard order of braids (``Dehornoy order''), and we deduce that, contrary to
all usual algebraic properties of braids, certain simple combinatorial
statements involving the braid order are true, but not provable in the
subsystems ISigma1 or ISigma2 of the standard Peano system.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 19:49:03 GMT"
}
] | 2014-02-26T00:00:00 | [
[
"Carlucci",
"Lorenzo",
"",
"LMNO"
],
[
"Dehornoy",
"Patrick",
"",
"LMNO"
],
[
"Weiermann",
"Andreas",
""
]
] | [
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] |
711.3786 | Yohan Payan | Olivier Chenu (TIMC), Nicolas Vuillerme (TIMC), Alexandre
Moreau-Gaudry (TIMC), Anthony Fleury (TIMC), Jacques Demongeot (TIMC), Yohan
Payan (TIMC) | Suppl\'eance perceptive par \'electro-stimulation linguale embarqu\'ee :
perspectives pour la pr\'evention des escarres chez le bless\'e m\'edullaire | null | Dans Actes de la 1\`ere Conf\'erence Internationale Sur
l'accessibilit\'e et les syst\`emes de suppl\'eance aux personnes en
situations de handicap - ASSISTH'2007, Toulouse : France (2007) | null | null | physics.med-ph q-bio.NC | null | We introduce the innovative technologies, based on the concept of "sensory
substitution", we are developing in the fields of biomedical engineering and
human disability. Precisely, our goal is to design, develop and validate
practical assistive biomedical and/or technical devices and/or rehabilitating
procedures for persons with disabilities, using artificial tongue-placed
tactile biofeedback systems. This paper proposes an application for pressure
sores prevention in case of spinal cord injuries (persons with paraplegia, or
tetraplegia).
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 19:51:07 GMT"
}
] | 2007-11-27T00:00:00 | [
[
"Chenu",
"Olivier",
"",
"TIMC"
],
[
"Vuillerme",
"Nicolas",
"",
"TIMC"
],
[
"Moreau-Gaudry",
"Alexandre",
"",
"TIMC"
],
[
"Fleury",
"Anthony",
"",
"TIMC"
],
[
"Demongeot",
"Jacques",
"",
"TIMC"
],
[
"Payan",
"Yohan",
"",
"TIMC"
]
] | [
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] |
711.3787 | Alexandru Nica | Serban T. Belinschi, Alexandru Nica | Free Brownian motion and evolution towards boxplus-infinite divisibility
for k-tuples | null | null | null | null | math.OA math.PR | null | Let D be the space of non-commutative distributions of k-tuples of
selfadjoints in a C*-probability space (for a fixed k). We introduce a
semigroup of transformations B_t of D, such that every distribution in D
evolves under the B_t towards infinite divisibility with respect to free
additive convolution. The very good properties of B_t come from some special
connections that we put into evidence between free additive convolution and the
operation of Boolean convolution.
On the other hand we put into evidence a relation between the transformations
B_t and free Brownian motion. More precisely, we introduce a transformation Phi
of D which converts the free Brownian motion started at an arbitrary
distribution m in D into the process B_t (Phi(m)), t>0.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 20:29:07 GMT"
}
] | 2007-11-26T00:00:00 | [
[
"Belinschi",
"Serban T.",
""
],
[
"Nica",
"Alexandru",
""
]
] | [
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711.3788 | Laura Baudis | Laura Baudis | Direct Detection of Cold Dark Matter | 10 pages, 11 figures; submitted for the SUSY07 proceedings | null | null | null | astro-ph | null | We know from cosmological and astrophysical observations that more than 80%
of the matter density in the Universe is non-luminous, or dark. This
non-baryonic dark matter could be composed of neutral, heavy particles, which
were non-relativistic, or 'cold', when they decoupled from ordinary matter. I
will review the direct detection methods of these hypothetical particles via
their interactions with nuclei in ultra-low background, deep underground
experiments. The emphasis is on most recent results and on the status of near
future projects.
| [
{
"version": "v1",
"created": "Sun, 25 Nov 2007 21:58:51 GMT"
}
] | 2007-11-27T00:00:00 | [
[
"Baudis",
"Laura",
""
]
] | [
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] |
711.3789 | Sharanya Sur Mr. | Sharanya Sur (1), Axel Brandenburg (2), Kandaswamy Subramanian (1)
((1) IUCAA, (2) NORDITA) | Kinematic alpha effect in isotropic turbulence simulations | Accepted for publication in MNRAS Letters | Monthly Notices Roy. Astron. Soc. 385, L15-L19 (2008) | 10.1111/j.1745-3933.2008.00423.x | NORDITA-2007-35 | astro-ph | null | Using numerical simulations at moderate magnetic Reynolds numbers up to 220
it is shown that in the kinematic regime, isotropic helical turbulence leads to
an alpha effect and a turbulent diffusivity whose values are independent of the
magnetic Reynolds number, $\Rm$, provided $\Rm$ exceeds unity. These turbulent
coefficients are also consistent with expectations from the first order
smoothing approximation. For small values of $\Rm$, alpha and turbulent
diffusivity are proportional to $\Rm$. Over finite time intervals meaningful
values of alpha and turbulent diffusivity can be obtained even when there is
small-scale dynamo action that produces strong magnetic fluctuations. This
suggests that small-scale dynamo-generated fields do not make a correlated
contribution to the mean electromotive force.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 21:00:18 GMT"
}
] | 2008-03-10T00:00:00 | [
[
"Sur",
"Sharanya",
"",
"IUCAA"
],
[
"Brandenburg",
"Axel",
"",
"NORDITA"
],
[
"Subramanian",
"Kandaswamy",
"",
"IUCAA"
]
] | [
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] |
711.379 | Vladimir Juricic | Vladimir Juricic, Igor F. Herbut, and Zlatko Tesanovic | Restoration of the magnetic hc/e-periodicity in unconventional
superconductors | 4 RevTex pages, 2 figures, published version | Phys. Rev. Lett. 100, 187006 (2008) | 10.1103/PhysRevLett.100.187006 | null | cond-mat.supr-con cond-mat.str-el | null | We consider the energy of the filled quasiparticle's Fermi sea of a
macroscopic superconducting ring threaded by an hc/2e-vortex, when the material
of the ring is of an unconventional pairing symmetry. The energy relative to
the one for the hc/e-vortex configuration is finite, positive, and inversely
proportional to ring's inner radius. We argue that the existence of this energy
in unconventional superconductors removes the commonly assumed degeneracy
between the odd and the even vortices, with the loss of the concomitant hc/2e
periodicity in external magnetic field as a consequence. This macroscopic
quantum effect should be observable in nanosized unconventional superconductors
with a small phase stiffness, such as deeply underdoped YBCO with Tc < 5K.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 21:00:23 GMT"
},
{
"version": "v2",
"created": "Fri, 9 May 2008 23:19:01 GMT"
}
] | 2008-05-10T00:00:00 | [
[
"Juricic",
"Vladimir",
""
],
[
"Herbut",
"Igor F.",
""
],
[
"Tesanovic",
"Zlatko",
""
]
] | [
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] |
711.3791 | Isaac Shlosman | Amir Zait (Racah Inst., Hebrew U., Jerusalem, Israel), Yehuda Hoffman
(Racah Inst., Hebrew U., Jerusalem, Israel) and Isaac Shlosman (UK Lexington) | Dark Matter Halos: Velocity Anisotropy -- Density Slope Relation | 7 pages, 5 figures, submitted to the Astrophysical Journal | null | 10.1086/589431 | null | astro-ph | null | Dark matter (DM) halos formed in CDM cosmologies seem to be characterized by
a power law phase-space density profile. The density of the DM halos is often
fitted by the NFW profile but a better fit is provided by the Sersic fitting
formula. These relations are empirically derived from cosmological simulations
of structure formation but have not yet been explained on a first principle
basis. Here we solve the Jeans equation under the assumption of a spherical DM
halo in dynamical equilibrium, that obeys a power law phase space density and
either the NFW-like or the Sersic density profile. We then calculate the
velocity anisotropy, beta(r), analytically. Our main result is that for the
NFW-like profile the beta - gamma relation is not a linear one (where gamma is
the logarithmic derivative of the density rho[r]). The shape of beta(r) depends
mostly on the ratio of the gravitational to kinetic energy within the NFW scale
radius R_s. For the Sersic profile a linear beta - gamma relation is recovered,
and in particular for the Sersic index of n = 6.0 case the linear fit of Hansen
& Moore is reproduced. Our main result is that the phase-space density power
law, the Sersic density form and the linear beta - gamma dependence constitute
a consistent set of relations which obey the spherical Jeans equation and as
such provide the framework for the dynamical modeling of DM halos.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 21:00:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zait",
"Amir",
"",
"Racah Inst., Hebrew U., Jerusalem, Israel"
],
[
"Hoffman",
"Yehuda",
"",
"Racah Inst., Hebrew U., Jerusalem, Israel"
],
[
"Shlosman",
"Isaac",
"",
"UK Lexington"
]
] | [
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] |
711.3792 | Cheng Li | Cheng Li, Guinevere Kauffmann, Timothy Heckman, Y. P. Jing, Simon D.
M. White | Interaction-induced star formation in a complete sample of 10^5 nearby
star-forming galaxies | v1: 13 pages, 12 figures, submitted for publication in Monthly
Notices; v2: 15 pages, 14 figures, accepted for publication, a new analysis
(sec. 6 and figs 13 and 14) is done in order to address the effect of rich
environments | Mon.Not.Roy.Astron.Soc.385:1903-1914,2008 | 10.1111/j.1365-2966.2008.13000.x | null | astro-ph | null | We investigate the clustering properties of a complete sample of 10^5
star-forming galaxies drawn from the SDSS DR4. On scales less than 100 kpc, the
amplitude of the correlation function exhibits a strong dependence on the
specific star formation rate of the galaxy. We interpret this as the signature
of enhanced star formation induced by tidal interactions. We then explore how
the average star formation rate in a galaxy is enhanced as the projected
separation r_p between the galaxy and its companions decreases. We find that
the enhancement depends strongly on r_p, but very weakly on the relative
luminosity of the companions. The enhancement is also stronger in low mass
galaxies than in high mass galaxies. In order to explore whether a tidal
interaction is not only sufficient, but also necessary to trigger enhanced star
formation in a galaxy, we compute background subtracted neighbour counts for
the galaxies in our sample. The average number of close neighbours around
galaxies with low to average values of SFR/M* is close to zero. At the highest
specific star formation rates, however, more than 40% of the galaxies in our
sample have a companion within a projected radius of 100 kpc. Visual inspection
of the highest SFR/M* galaxies without companions reveals that more than 50% of
these are clear interacting or merging systems. We conclude that tidal
interactions are the dominant trigger of enhanced star formation in the most
strongly star-forming systems. Finally, we find clear evidence that tidal
interactions not only lead to enhanced star formation in galaxies, but also
cause structural changes such as an increase in concentration.
| [
{
"version": "v1",
"created": "Sun, 25 Nov 2007 17:27:31 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 13:23:38 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Li",
"Cheng",
""
],
[
"Kauffmann",
"Guinevere",
""
],
[
"Heckman",
"Timothy",
""
],
[
"Jing",
"Y. P.",
""
],
[
"White",
"Simon D. M.",
""
]
] | [
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] |
711.3793 | Sudeep Das | Sudeep Das and Paul Bode | A Large Sky Simulation of the Gravitational Lensing of the Cosmic
Microwave Background | 14 pages, 12 figures, replaced with version accepted for publication
by the APJ | Astrophys. J. 682 (2008) 1 | 10.1086/589638 | null | astro-ph | null | Large scale structure deflects cosmic microwave background (CMB) photons.
Since large angular scales in the large scale structure contribute
significantly to the gravitational lensing effect, a realistic simulation of
CMB lensing requires a sufficiently large sky area. We describe simulations
that include these effects, and present both effective and multiple plane
ray-tracing versions of the algorithm, which employs spherical harmonic space
and does not use the flat sky approximation. We simulate lensed CMB maps with
an angular resolution of ~0.9 arcmin. The angular power spectrum of the
simulated sky agrees well with analytical predictions. Maps generated in this
manner are a useful tool for the analysis and interpretation of upcoming CMB
experiments such as PLANCK and ACT.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 21:05:25 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 20:28:24 GMT"
},
{
"version": "v3",
"created": "Fri, 25 Apr 2008 19:02:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Das",
"Sudeep",
""
],
[
"Bode",
"Paul",
""
]
] | [
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] |
711.3794 | Mircea Mustata | Mircea Mustata | Bernstein-Sato polynomials in positive characteristic | 26 pages; v.2: new section added, treating the decomposition of an
arbitrary D-module under the Euler operators; v.3: final version, to appear
in Journal of Algebra | null | null | null | math.AG math.AC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In characteristic zero, the Bernstein-Sato polynomial of a hypersurface can
be described as the minimal polynomial of the action of an Euler operator on a
suitable D-module. We consider the analogous D-module in positive
characteristic, and use it to define a sequence of Bernstein-Sato polynomials
(corresponding to the fact that we need to consider also divided powers Euler
operators). We show that the information contained in these polynomials is
equivalent to that given by the F-jumping exponents of the hypersurface, in the
sense of Hara and Yoshida.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 21:16:58 GMT"
},
{
"version": "v2",
"created": "Thu, 12 Jun 2008 07:23:47 GMT"
},
{
"version": "v3",
"created": "Sun, 17 Aug 2008 20:05:43 GMT"
}
] | 2008-08-17T00:00:00 | [
[
"Mustata",
"Mircea",
""
]
] | [
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711.3795 | Chi-Sing Lam | C.S. Lam | Horizontal Symmetry | Based on a talk given at the International Conference on Flavor
Physics, Beijing, China, September, 2007. To appear in the conference
proceedings | Int.J.Mod.Phys.A23:3371-3375,2008 | 10.1142/S0217751X08042146 | null | hep-ph | null | The relation between fermion mixing and horizontal symmetry is discussed.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 22:04:02 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Lam",
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""
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711.3796 | Belen Paredes | Belen Paredes and Immanuel Bloch | Minimum instances of topological matter in an optical plaquette | 8 pages, 11 figures | null | 10.1103/PhysRevA.77.023603 | null | cond-mat.other | null | We propose experimental schemes to create and probe minimum forms of
different topologically ordered states in a plaquette of an optical lattice:
Resonating Valence Bond, Laughlin and string-net condensed states. We show how
to create anyonic excitations on top of these liquids and detect their
fractional statistics. In addition, we propose a way to design a plaquette
ring-exchange interaction, the building block Hamiltonian of a lattice
topological theory. Our preparation and detection schemes combine different
techniques already demonstrated in experiments with atoms in optical
superlattices.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 22:35:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Paredes",
"Belen",
""
],
[
"Bloch",
"Immanuel",
""
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711.3797 | Dong Wang | Dong Wang | A PDE for the multi-time joint probability of the Airy process | 21 pages | null | null | null | math.PR math-ph math.MP | null | This paper gives a PDE for multi-time joint probability of the Airy process,
which generalizes Adler and van Moerbeke's result on the 2-time case. As an
intermediate step, the PDE for the multi-time joint probability of the Dyson
Brownian motion is also given.
| [
{
"version": "v1",
"created": "Mon, 26 Nov 2007 20:39:13 GMT"
}
] | 2007-11-27T00:00:00 | [
[
"Wang",
"Dong",
""
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] |
711.3798 | Eric Cavalcanti | E. G. Cavalcanti, P. D. Drummond, H. A. Bachor and M. D. Reid | Spin entanglement, decoherence and Bohm's EPR paradox | 4 pages 3 figures | Optics Express, Vol. 17, Issue 21, pp. 18693-18702 (2009) | 10.1364/OE.17.018693 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We obtain criteria for entanglement and the EPR paradox for spin-entangled
particles and analyse the effects of decoherence caused by absorption and state
purity errors. For a two qubit photonic state, entanglement can occur for all
transmission efficiencies. In this case, the state preparation purity must be
above a threshold value. However, Bohm's spin EPR paradox can be achieved only
above a critical level of loss. We calculate a required efficiency of 58%,
which appears achievable with current quantum optical technologies. For a
macroscopic number of particles prepared in a correlated state, spin
entanglement and the EPR paradox can be demonstrated using our criteria for
efficiencies {\eta} > 1/3 and {\eta} > 2/3 respectively. This indicates a
surprising insensitivity to loss decoherence, in a macroscopic system of
ultra-cold atoms or photons.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 23:26:42 GMT"
},
{
"version": "v2",
"created": "Mon, 6 Sep 2010 06:30:08 GMT"
}
] | 2010-09-17T00:00:00 | [
[
"Cavalcanti",
"E. G.",
""
],
[
"Drummond",
"P. D.",
""
],
[
"Bachor",
"H. A.",
""
],
[
"Reid",
"M. D.",
""
]
] | [
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711.3799 | Jie Sun | Arturo Pianzola, Daniel Prelat and Jie Sun | Descent constructions for central extensions of infinite dimensional Lie
algebras | 13 pages, minor corrections | manuscripta mathematica 122 (2007), 137-148 | null | null | math.AG math.RA | null | We use Galois descent to construct central extensions of twisted forms of
split simple Lie algebras over rings. These types of algebras arise naturally
in the construction of Extended Affine Lie Algebras. The construction also
gives information about the structure of the group of automorphisms of such
algebras.
| [
{
"version": "v1",
"created": "Fri, 23 Nov 2007 23:59:23 GMT"
}
] | 2007-11-27T00:00:00 | [
[
"Pianzola",
"Arturo",
""
],
[
"Prelat",
"Daniel",
""
],
[
"Sun",
"Jie",
""
]
] | [
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] |
711.38 | Lang Shao | L. Shao (1 and 2), Z. G. Dai (1) and N. Mirabal (3) ((1)Nanjing
University, China, (2)University of Colorado, USA, (3)Columbia University,
USA) | Echo Emission From Dust Scattering and X-Ray Afterglows of Gamma-Ray
Bursts | 25 pages, 3 figures, 2 tables. Accepted for publication in ApJ | Astrophys.J.675:507-518,2008 | 10.1086/527047 | null | astro-ph | null | We investigate the effect of X-ray echo emission in gamma-ray bursts (GRBs).
We find that the echo emission can provide an alternative way of understanding
X-ray shallow decays and jet breaks. In particular, a shallow decay followed by
a "normal" decay and a further rapid decay of X-ray afterglows can be together
explained as being due to the echo from prompt X-ray emission scattered by dust
grains in a massive wind bubble around a GRB progenitor. We also introduce an
extra temporal break in the X-ray echo emission. By fitting the afterglow light
curves, we can measure the locations of the massive wind bubbles, which will
bring us closer to finding the mass loss rate, wind velocity, and the age of
the progenitors prior to the GRB explosions.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 00:13:31 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Shao",
"L.",
"",
"1 and 2"
],
[
"Dai",
"Z. G.",
""
],
[
"Mirabal",
"N.",
""
]
] | [
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] |
711.3801 | Viacheslav Titov | V. S. Titov, Z. Mikic, J. A. Linker, and R. Lionello | May 12 1997 Cme Event: I. a Simplified Model of the Pre-Eruptive
Magnetic Structure | 25 pages, 11 figures, to appear in ApJ 2008 | 2008, Astrophys. J., vol. 675, No. 2, pp. 1614-1628 | 10.1086/527280 | null | astro-ph | null | A simple model of the coronal magnetic field prior to the CME eruption on May
12 1997 is developed. First, the magnetic field is constructed by superimposing
a large-scale background field and a localized bipolar field to model the
active region (AR) in the current-free approximation. Second, this potential
configuration is quasi-statically sheared by photospheric vortex motions
applied to two flux concentrations of the AR. Third, the resulting force-free
field is then evolved by canceling the photospheric magnetic flux with the help
of an appropriate tangential electric field applied to the central part of the
AR.
To understand the structure of the modeled configuration, we use the field
line mapping technique by generalizing it to spherical geometry. It is
demonstrated that the initial potential configuration contains a hyperbolic
flux tube (HFT) which is a union of two intersecting quasi-separatrix layers.
This HFT provides a partition of the closed magnetic flux between the AR and
the global solar magnetic field. The vortex motions applied to the AR interlock
the field lines in the coronal volume to form additionally two new HFTs pinched
into thin current layers. Reconnection in these current layers helps to
redistribute the magnetic flux and current within the AR in the
flux-cancellation phase. In this phase, a magnetic flux rope is formed together
with a bald patch separatrix surface wrapping around the rope. Other important
implications of the identified structural features of the modeled configuration
are also discussed.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 00:39:30 GMT"
}
] | 2008-03-11T00:00:00 | [
[
"Titov",
"V. S.",
""
],
[
"Mikic",
"Z.",
""
],
[
"Linker",
"J. A.",
""
],
[
"Lionello",
"R.",
""
]
] | [
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] |
711.3802 | Dongwoo Cha | Guanghao Jin, Jin-Hee Yoon, and Dongwoo Cha | N_pN_n dependence of empirical formula for the lowest excitation energy
of the 2^+ states in even-even nuclei | 14 pages, 5 figures | J. Phys. G: Nucl. Part. Phys. 35 (2008) 035105 | 10.1088/0954-3899/35/3/035105 | null | nucl-th | null | We examine the effects of the additional term of the type $\sim e^{- \lambda'
N_pN_n}$ on the recently proposed empirical formula for the lowest excitation
energy of the $2^+$ states in even-even nuclei. This study is motivated by the
fact that this term carries the favorable dependence of the valence nucleon
numbers dictated by the $N_pN_n$ scheme. We show explicitly that there is not
any improvement in reproducing $E_x(2_1^+)$ by including the extra $N_pN_n$
term. However, our study also reveals that the excitation energies
$E_x(2_1^+)$, when calculated by the $N_pN_n$ term alone (with the mass number
$A$ dependent term), are quite comparable to those calculated by the original
empirical formula.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 00:33:38 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Feb 2008 15:54:58 GMT"
}
] | 2008-02-13T00:00:00 | [
[
"Jin",
"Guanghao",
""
],
[
"Yoon",
"Jin-Hee",
""
],
[
"Cha",
"Dongwoo",
""
]
] | [
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] |
711.3803 | Sven Bjarke Gudnason | Stefano Bolognesi, Sven Bjarke Gudnason | A Note on Chern-Simons Solitons - a type III vortex from the wall vortex | 27 pages, 17 figures; v2.: references added, subsection 3.2 added,
explanation added in section 2.3 | Nucl.Phys.B805:104-123,2008 | 10.1016/j.nuclphysb.2008.07.018 | FTPI-MINN-07/32; UMN-TH-2623/07; IFUP-TH/2007-32 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study some properties of topological Chern-Simons vortices in 2 + 1
dimensions. As has already been understood in the past, in the large magnetic
flux limit, they are well described by a Chern-Simons domain wall, which has
been compactified on a circle with the symmetric phase inside and the
asymmetric phase on the outside. Our goal is two-fold. First we want to explore
how the tension depends on the magnetic flux discretized by the integer n. The
BPS case is already known, but not much has been explored about the non-BPS
potentials. A generic renormalizable potential has two dimensionless parameters
that can be varied. Variation of only one of them lead to a type I and type II
vortex, very similar to the Abrikosov-Nielsen-Olesen (ANO) case. Variation of
both the parameters leads to a much richer structure. In particular we have
found a new type of vortex, which is type I-like for small flux and then turns
type II-like for larger flux. We could tentatively denote it a type III vortex.
This results in a stable vortex with number of fluxes which can be greater than
one. Our second objective is to study the Maxwell-Chern-Simons theory and and
understand how the large n limit of the CS vortex is smoothly connected with
the large n limit of the ANO vortex.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 01:00:51 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jul 2008 11:28:25 GMT"
}
] | 2010-05-27T00:00:00 | [
[
"Bolognesi",
"Stefano",
""
],
[
"Gudnason",
"Sven Bjarke",
""
]
] | [
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] |
711.3804 | Michael Courtney | Michael Courtney, Amy Courtney | Sheep Collisions: the Good, the Bad, and the TBI | null | null | null | null | physics.ed-ph | null | The title page of Chapter 9 in Fundamentals of Physics (Halliday, Resnick,
and Walker, 8th Edition, p. 201) shows a dramatic photograph of two Big Horn
sheep butting heads and promises to explain how sheep survive such violent
clashes without serious injury. However, the answer presented in sample problem
9-4 (p. 213) errs in presuming an interaction time of 0.27 s which results in
an unrealistically long stopping distance of 0.62 m. Furthermore, the assertion
that the horns provide necessary cushioning of the blow is inconsistent with
the absence of concussions in domestic breeds of hornless sheep. Results from
traumatic brain injury (TBI) research allow acceleration tolerance of sheep to
be estimated as 450 g facilitating an analysis of sheep collisions that is more
consistent with available observations (stopping distance less than 1 cm,
impact time of roughly 2 ms).
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 01:03:35 GMT"
}
] | 2007-11-27T00:00:00 | [
[
"Courtney",
"Michael",
""
],
[
"Courtney",
"Amy",
""
]
] | [
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] |
711.3805 | Jan-Uwe Ness | J.-U. Ness and C. Jordan | The corona and upper transition region of epsilon Eridani | accepted by MNRAS; 19 pages, five figures, 10 tables | null | 10.1111/j.1365-2966.2007.12757.x | null | astro-ph | null | We present analyses of observations of epsilon Eridani (K2 V) made with the
Low Energy Transmission Grating Spectrometer on Chandra and the Extreme
Ultraviolet Explorer, supplemented by observations made with the Space
Telescope Imaging Spectrograph, the Far Ultraviolet Spectroscopic Explorer and
the Reflection Grating Spectrometer on XMM-Newton. The observed emission lines
are used to find relative element abundances, to place limits on the electron
densities and pressures and to determine the mean apparent emission measure
distribution. As in the previous paper by Sim & Jordan (2003a), the mean
emitting area as a function of the electron temperature is derived by
comparisons with a theoretical emission measure distribution found from energy
balance arguments. The final model has a coronal temperature of 3.4 x 10^6 K,
an electron pressure of 1.3 x 10^16 cm^-3 K at T_e = 2 x 10^5 K and an area
filling factor of 0.14 at 3.2 x 10^5 K. We discuss a number of issues
concerning the atomic data currently available. Our analyses are based mainly
on the latest version of CHIANTI (v5.2). We conclude that the Ne/O relative
abundance is 0.30, larger than that recommended from solar studies, and that
there is no convincing evidence for enhanced coronal abundances of elements
with low first ionization potentials.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 01:38:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ness",
"J. -U.",
""
],
[
"Jordan",
"C.",
""
]
] | [
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711.3806 | Ilya Kapovich | Ilya Kapovich and Martin Lustig | Geometric Intersection Number and analogues of the Curve Complex for
free groups | Revised version, to appear in Geometry & Topology | Geom. Topol. 13 (2009) 1805-1833 | 10.2140/gt.2009.13.1805 | null | math.GR math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For the free group $F_{N}$ of finite rank $N \geq 2$ we construct a canonical
Bonahon-type continuous and $Out(F_N)$-invariant \emph{geometric intersection
form} \[ <, >: \bar{cv}(F_N)\times Curr(F_N)\to \mathbb R_{\ge 0}. \]
Here $\bar{cv}(F_N)$ is the closure of unprojectivized Culler-Vogtmann's
Outer space $cv(F_N)$ in the equivariant Gromov-Hausdorff convergence topology
(or, equivalently, in the length function topology). It is known that
$\bar{cv}(F_N)$ consists of all \emph{very small} minimal isometric actions of
$F_N$ on $\mathbb R$-trees. The projectivization of $\bar{cv}(F_N)$ provides a
free group analogue of Thurston's compactification of the Teichm\"uller space.
As an application, using the \emph{intersection graph} determined by the
intersection form, we show that several natural analogues of the curve complex
in the free group context have infinite diameter.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 01:43:24 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 13:38:10 GMT"
},
{
"version": "v3",
"created": "Wed, 5 Dec 2007 23:52:25 GMT"
},
{
"version": "v4",
"created": "Sat, 21 Feb 2009 19:47:37 GMT"
}
] | 2014-11-11T00:00:00 | [
[
"Kapovich",
"Ilya",
""
],
[
"Lustig",
"Martin",
""
]
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711.3807 | Serguei Mechkov | S. Mechkov, M. Rauscher, S. Dietrich | Stability of liquid ridges on chemical micro- and nanostripes | 10 pages, 6 figures | null | 10.1103/PhysRevE.77.061605 | null | cond-mat.soft | null | We analyze the stability of sessile filaments (ridges) of nonvolatile liquids
versus pearling in the case of externally driven flow along a chemical stripe
within the framework of the thin film approximation. The ridges can be stable
with respect to pearling even if the contact line is not completely pinned. A
generalized stability criterion for moving contact lines is provided. For large
wavelengths and no drive, within perturbation theory, an analytical expression
of the growth rate of pearling instabilities is derived. A numerical analysis
shows that drive further stabilizes the ridge by reducing the growth rate of
unstable perturbations, even though there is no complete stabilization. Hence
the stability criteria established without drive ensure overall stability.
| [
{
"version": "v1",
"created": "Sat, 24 Nov 2007 01:43:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mechkov",
"S.",
""
],
[
"Rauscher",
"M.",
""
],
[
"Dietrich",
"S.",
""
]
] | [
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