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801.1773 | Hans Christian Krahl | H. C. Krahl, J. A. M\"uller, C. Wetterich | Generation of d-wave coupling in the two-dimensional Hubbard model from
functional renormalization | 11 pages, 13 figures, equivalent to published version | Phys. Rev. B 79, 094526 (2009) | 10.1103/PhysRevB.79.094526 | null | cond-mat.str-el hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Within the two-dimensional repulsive t-t'-Hubbard model, an attractive
coupling in the d-wave pairing channel is induced by antiferromagnetic
fluctuations. We investigate this coupling using functional renormalization
group equations. The momentum dependent d-wave coupling can be bosonized by the
use of scale dependent field transformations. We propose an effective coarse
grained model for the Hubbard model which is based on the exchange of
antiferromagnetic and d-wave collective bosons.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:55:01 GMT"
},
{
"version": "v2",
"created": "Mon, 13 Apr 2009 13:14:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Krahl",
"H. C.",
""
],
[
"Müller",
"J. A.",
""
],
[
"Wetterich",
"C.",
""
]
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801.1774 | Dirk Lorenz | Dirk A. Lorenz | Convergence rates and source conditions for Tikhonov regularization with
sparsity constraints | null | Journal of Inverse and Ill-Posed Problems, 16(5):463-478, 2008 | 10.1515/JIIP.2008.025 | null | math.FA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper addresses the regularization by sparsity constraints by means of
weighted $\ell^p$ penalties for $0\leq p\leq 2$. For $1\leq p\leq 2$ special
attention is payed to convergence rates in norm and to source conditions. As
main result it is proven that one gets a convergence rate in norm of
$\sqrt{\delta}$ for $1\leq p\leq 2$ as soon as the unknown solution is sparse.
The case $p=1$ needs a special technique where not only Bregman distances but
also a so-called Bregman-Taylor distance has to be employed.
For $p<1$ only preliminary results are shown. These results indicate that,
different from $p\geq 1$, the regularizing properties depend on the interplay
of the operator and the basis of sparsity. A counterexample for $p=0$ shows
that regularization need not to happen.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:01:22 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jul 2008 11:07:38 GMT"
}
] | 2011-03-16T00:00:00 | [
[
"Lorenz",
"Dirk A.",
""
]
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801.1775 | X.R. Wang | X. R. Wang | Giant dynamical Zeeman split in inverse spin valves | null | null | null | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | The inversion of a spin valve device is proposed. Opposite to a conventional
spin valve of a non-magnetic spacer sandwiched between two ferromagnetic
metals, an inverse spin valve is a ferromagnet sandwiched between two
non-magnetic metals. It is predicted that, under a bias, the chemical
potentials of spin-up and spin-down electrons in the metals split at
metal-ferromagnet interfaces, a dynamical Zeeman effect. This split is of the
order of an applied bias. Thus, there should be no problem of generating an
$eV$ split that is not possible to be realized on the earth by the usual Zeeman
effect.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:05:30 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Wang",
"X. R.",
""
]
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] |
801.1776 | Peter Morgan | Peter Morgan | Violation of Bell inequalities through the coincidence-time loophole | 4 pages | null | null | null | quant-ph | null | The coincidence-time loophole was identified by Larsson & Gill (Europhys.
Lett. 67, 707 (2004)); a concrete model that exploits this loophole has
recently been described by De Raedt et al. (Found. Phys., to appear). It is
emphasized here that De Raedt et al.'s model is experimentally testable. De
Raedt et al.'s model also introduces contextuality in a novel and classically
more natural way than the use of contextual particle properties, by introducing
a probabilistic model of a limited set of degrees of freedom of the measurement
apparatus, so that it can also be seen as a random field model. Even though De
Raedt et al.'s model may well contradict detailed Physics, it nonetheless
provides a way to simulate the logical operation of elements of a quantum
computer, and may provide a way forward for more detailed random field models.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:11:03 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Morgan",
"Peter",
""
]
] | [
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801.1777 | Vincent Tatischeff | V. Tatischeff, J.-P. Thibaud and I. Ribas | Nucleosynthesis in stellar flares | 12 pages, 3 figures, contribution to the Proceedings of the XIXemes
Rencontres de Blois, Matter and energy in the Universe, Blois, France, May
2007 | null | null | null | astro-ph | null | Nuclear interactions of ions accelerated at the surface of flaring stars can
produce fresh isotopes in stellar atmospheres. Although this nucleosynthesis is
not significant for the chemical evolution of the Galaxy, it can be important
for a number of measurements of "anomalously" high 6-Li and 7-Li abundances. We
discuss the possible role of stellar flares to explain the recent report of
high 6-Li abundances in metal-poor halo stars and the well-established
correlation between Li abundance and stellar activity in young open clusters.
We then study the possibility of observing directly Li production during flares
of nearby and active dwarfs of spectral type M.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:28:46 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Tatischeff",
"V.",
""
],
[
"Thibaud",
"J. -P.",
""
],
[
"Ribas",
"I.",
""
]
] | [
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] |
801.1778 | Henrik Beuther | H. Beuther, A.J. Walsh, S. Thorwirth, Q. Zhang, T.R. Hunter, S.T.
Megeath, K.M. Menten | ATCA 3mm observations of NGC6334I and I(N): dense cores, outflows and an
UCHII region | 14 pages, 14 figures, accepted for A&A | null | 10.1051/0004-6361:20079014 | null | astro-ph | null | Aims: Investigation of the dense gas, the outflows and the continuum emission
from the massive twin cores NGC6334I and I(N) at high spatial resolution.
Methods: We imaged the region with the Australia Telescope Compact Array (ATCA)
at 3.4mm wavelength in continuum as well as CH3CN(5_K-4_K) and HCN(1-0)
spectral line emission. Results: While the continuum emission in NGC6334I
mainly traces the UCHII region, toward NGC6334I(N) we detect line emission from
four of the previously identified dust continuum condensations that are of
protostellar or pre-stellar nature. The CH3CN(5_K-4_K) lines are detected in
all K-components up to energies of 128K above ground toward two protostellar
condensations in both regions. We find line-width increasing with increasing K
for all sources, which indicates a higher degree of internal motions closer to
the central protostars. Toward the main mm and CH3CN source in NGC6334I we
identify a velocity gradient approximately perpendicular to the large-scale
molecular outflow. This may be interpreted as a signature of an accretion disk,
although other scenarios, e.g., an unresolved double source, could produce a
similar signature as well. No comparable signature is found toward any of the
other sources. HCN does not trace the dense gas well but it is dominated by the
molecular outflows. While the outflow in NGC6334I exhibits a normal Hubble-law
like velocity structure, the data indicate a precessing outflow close to the
plane of the sky for NGC6334I(N). Furthermore, we observe a wide (~15.4km/s)
HCN absorption line, much broader than the previously observed CH3OH and NH3
absorption lines. Several explanations for the difference are discussed.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:25:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Beuther",
"H.",
""
],
[
"Walsh",
"A. J.",
""
],
[
"Thorwirth",
"S.",
""
],
[
"Zhang",
"Q.",
""
],
[
"Hunter",
"T. R.",
""
],
[
"Megeath",
"S. T.",
""
],
[
"Menten",
"K. M.",
""
]
] | [
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] |
801.1779 | Jiang Xiao | Jiang Xiao, Gerrit E. W. Bauer, Arne Brataas | Charge pumping in magnetic tunnel junctions: Scattering theory | 4 pages, 3 figures. to be published on Physical Review B Rapid
Communication | Physical Review B 77, 180407(R) (2008) | 10.1103/PhysRevB.77.180407 | null | cond-mat.mtrl-sci | null | We study theoretically the charge transport pumped by magnetization dynamics
through epitaxial FIF and FNIF magnetic tunnel junctions (F: Ferromagnet, I:
Insulator, N: Normal metal). We predict a small but measurable DC pumping
voltage under ferromagnetic resonance conditions for collinear magnetization
configurations, which may change sign as function of barrier parameters. A much
larger AC pumping voltage is expected when the magnetizations are at right
angles. Quantum size effects are predicted for an FNIF structure as a function
of the normal layer thickness.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:26:01 GMT"
},
{
"version": "v2",
"created": "Sat, 12 Jan 2008 15:55:57 GMT"
},
{
"version": "v3",
"created": "Wed, 21 May 2008 09:53:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Xiao",
"Jiang",
""
],
[
"Bauer",
"Gerrit E. W.",
""
],
[
"Brataas",
"Arne",
""
]
] | [
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] |
801.178 | J\'er\^ome Bolte | Hedy Attouch, Jerome Bolte, Patrick Redont, Antoine Soubeyran | Proximal alternating minimization and projection methods for nonconvex
problems. An approach based on the Kurdyka-Lojasiewicz inequality | null | null | null | null | math.OC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the convergence properties of an alternating proximal minimization
algorithm for nonconvex structured functions of the type:
$L(x,y)=f(x)+Q(x,y)+g(y)$, where $f:\R^n\rightarrow\R\cup{+\infty}$ and
$g:\R^m\rightarrow\R\cup{+\infty}$ are proper lower semicontinuous functions,
and $Q:\R^n\times\R^m\rightarrow \R$ is a smooth $C^1$ function which couples
the variables $x$ and $y$. The algorithm can be viewed as a proximal
regularization of the usual Gauss-Seidel method to minimize $L$. We work in a
nonconvex setting, just assuming that the function $L$ satisfies the Kurdyka-\L
ojasiewicz inequality. An entire section illustrates the relevancy of such an
assumption by giving examples ranging from semialgebraic geometry to
"metrically regular" problems. Our main result can be stated as follows: If L
has the Kurdyka-\L ojasiewicz property, then each bounded sequence generated by
the algorithm converges to a critical point of $L$. This result is completed by
the study of the convergence rate of the algorithm, which depends on the
geometrical properties of the function $L$ around its critical points. When
specialized to $Q(x,y)=|x-y|^2$ and to $f$, $g$ indicator functions, the
algorithm is an alternating projection mehod (a variant of Von Neumann's) that
converges for a wide class of sets including semialgebraic and tame sets,
transverse smooth manifolds or sets with "regular" intersection. In order to
illustrate our results with concrete problems, we provide a convergent proximal
reweighted $\ell^1$ algorithm for compressive sensing and an application to
rank reduction problems.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:54:05 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Jan 2008 09:34:35 GMT"
},
{
"version": "v3",
"created": "Tue, 22 Jan 2013 20:19:54 GMT"
}
] | 2013-01-23T00:00:00 | [
[
"Attouch",
"Hedy",
""
],
[
"Bolte",
"Jerome",
""
],
[
"Redont",
"Patrick",
""
],
[
"Soubeyran",
"Antoine",
""
]
] | [
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] |
801.1781 | Erhu Zhang | Shengli Zhang, Qi Wang, Erhu Zhang | The Geometrical Effects on Electronic Spectrum and Persistent Currents
in Mesoscopic Polygon | 10 pages, 6 figures | Modern Physics Letters B, Vol. 23, No. 2 (2009) 191-201 | 10.1142/S0217984909017959 | null | cond-mat.mes-hall | null | In this paper, a new mesoscopic polygon which possesses smooth transition at
its corners is proposed. Because of the particularity of structure, this kind
of mesoscopic polygon can also be a geometrical supperlattice. The geometrical
effects on the electron states and persistent current are investigated
comprehensively in the presence of magnetic flux. We find that the particular
geometric structure of the polygon induces an effective periodic potential
which results in gaps in the energy spectrum. The changes of gaps show the
consistency with the geometrical twoness of this new polygon. This electronic
structure and the corresponding physical properties are found to be periodic
with period $\phi_{0}$ in the magnetic flux $\phi $ and can be controlled by
the geometric method. We also consider the Rahsba spin-orbit interaction which
make the energy levels splitting newly to double and leads to an additional
small zigzag in one period of the persistent current. These new phenomena may
be useful for the applications in quantum device design in the future.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 13:44:25 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Apr 2008 05:06:04 GMT"
}
] | 2009-03-03T00:00:00 | [
[
"Zhang",
"Shengli",
""
],
[
"Wang",
"Qi",
""
],
[
"Zhang",
"Erhu",
""
]
] | [
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] |
801.1782 | Xavier Artru | X. Artru (IPNL), J.-M. Richard (LPSC), J. Soffer | Positivity domains for pairs of triples of spin observables | Talk given by Xavier Artru at "DSPIN-07", XII Workshop on High-Energy
Spin Physics, Dubna, Sept. 3-7, 2007, to appear in the Proceedings | Dans High-Energy Spin Physics - Proceeding of the XII Workshop on
High-Energy Spin Physics, Dubna (2007) | null | null | nucl-th hep-ph | null | Positivity restrains the allowed domains for pairs or triples of spin
observables in polarised reactions. Various domain shapes in
${1\over2}+{1\over2}\to{1\over2}+{1\over2}$ reactions are displayed. Some
methods to determine these domains are mentioned and a new one based on the
anticommutation between two observables is presented.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:03:50 GMT"
}
] | 2008-01-17T00:00:00 | [
[
"Artru",
"X.",
"",
"IPNL"
],
[
"Richard",
"J. -M.",
"",
"LPSC"
],
[
"Soffer",
"J.",
""
]
] | [
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] |
801.1783 | Olivier Finkel | Jacques Duparc (UNIL), Olivier Finkel (LIP) | An omega-power of a context-free language which is Borel above
Delta^0_omega | To appear in the Proceedings of the International Conference
Foundations of the Formal Sciences V : Infinite Games, November 26th to 29th,
2004, Bonn, Germany, Stefan Bold, Benedikt L\"owe, Thoralf R\"asch, Johan van
Benthem (eds.), College Publications at King's College (Studies in Logic),
2007 | Dans Proceedings of the International Conference on Foundations of
the Formal Sciences V : Infinite Games - Foundations of the Formal Sciences V
: Infinite Games, November 26-29, 2004, Bonn : Allemagne | null | null | cs.CC cs.GT cs.LO math.LO | null | We use erasers-like basic operations on words to construct a set that is both
Borel and above Delta^0_omega, built as a set V^\omega where V is a language of
finite words accepted by a pushdown automaton. In particular, this gives a
first example of an omega-power of a context free language which is a Borel set
of infinite rank.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:20:30 GMT"
}
] | 2008-09-10T00:00:00 | [
[
"Duparc",
"Jacques",
"",
"UNIL"
],
[
"Finkel",
"Olivier",
"",
"LIP"
]
] | [
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] |
801.1784 | Sergei Vyshenski | S. V. Vyshenski, P. V. Grigoriev, Yu. Yu. Dubenskaya | Ideal synchronizer for marked pairs in fork-join network | 18 pages, 3 figures, in Russian, typos fixed | null | null | null | cs.DM | null | We introduce a new functional element (synchronizer for marked pairs) meant
to join results of parallel processing in two-branch fork-join queueing
network. Approximations for distribution of sojourn time at the synchronizer
are derived along with a validity domain. Calculations are performed assuming
that: arrivals to the network form a Poisson process, each branch operates like
an M/M/N queueing system. It is shown that mean sojourn time at a real
synchronizer node is bounded below by the value, defined by parameters of the
network (which contains the synchronizer) and does not depend upon performance
and particular properties of the synchronizer.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:00:59 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 20:57:32 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Vyshenski",
"S. V.",
""
],
[
"Grigoriev",
"P. V.",
""
],
[
"Dubenskaya",
"Yu. Yu.",
""
]
] | [
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801.1785 | Troost Jan | Raphael Benichou, Giuseppe Policastro, Jan Troost | T-duality in Ramond-Ramond backgrounds | 7 pages, accepted for publication in PLB | Phys.Lett.B661:192-195,2008 | 10.1016/j.physletb.2008.01.059 | LPTENS-08/03 | hep-th | null | Using the pure spinor formalism on the world-sheet, we derive the T-duality
rules for all target space couplings in an efficient manner. The world-sheet
path integral derivation is a proof of the equivalence of the T-dual
Ramond-Ramond backgrounds which is valid non-perturbatively in the string
length over the curvature radius and to all orders in perturbation theory in
the string coupling.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:34:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Benichou",
"Raphael",
""
],
[
"Policastro",
"Giuseppe",
""
],
[
"Troost",
"Jan",
""
]
] | [
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] |
801.1786 | Roberto Raimondi | M. Milletari', R. Raimondi and P. Schwab | Magneto-spin Hall conductivity of a two-dimensional electron gas | 5 pages, 1 figure | null | 10.1209/0295-5075/82/67005 | null | cond-mat.mes-hall cond-mat.dis-nn | null | It is shown that the interplay of long-range disorder and in-plane magnetic
field gives rise to an out-of-plane spin polarization and a finite spin Hall
conductivity of the two-dimensional electron gas in the presence of Rashba
spin-orbit coupling. A key aspect is provided by the electric-field induced
in-plane spin polarization. Our results are obtained first in the
\textit{clean} limit where the spin-orbit splitting is much larger than the
disorder broadening of the energy levels via the diagrammatic evaluation of the
Kubo-formula. Then the results are shown to hold in the full range of the
disorder parameter $\alpha p_F \tau$ by means of the quasiclassical Green
function technique.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:37:36 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Milletari'",
"M.",
""
],
[
"Raimondi",
"R.",
""
],
[
"Schwab",
"P.",
""
]
] | [
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] |
801.1787 | Daniel Senff | D. Senff, O. Schumann, M. Benomar, M. Kriener, T. Lorenz, Y. Sidis, K.
Habicht, P. Link, and M. Braden | Melting of magnetic correlations in charge-orbital ordered
La(0.5)Sr(1.5)MnO(4) : competition of ferro and antiferromagnetic states | 14 pages, 11 figures | null | 10.1103/PhysRevB.77.184413 | null | cond-mat.str-el | null | The magnetic correlations in the charge- and orbital-ordered manganite
La(0.5)Sr(1.5)MnO(4) have been studied by elastic and inelastic neutron
scattering techniques. Out of the well-defined CE-type magnetic structure with
the corresponding magnons a competition between CE-type and ferromagnetic
fluctuations develops. Whereas ferromagnetic correlations are fully suppressed
by the static CE-type order at low temperature, elastic and inelastic CE-type
correlations disappear with the melting of the charge-orbital order at high
temperature. In its charge-orbital disordered phase, La(0.5)Sr(1.5)MnO(4)
exhibits a dispersion of ferromagnetic correlations which remarkably resembles
the magnon dispersion in ferromagnetically ordered metallic perovskite
manganites.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:50:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Senff",
"D.",
""
],
[
"Schumann",
"O.",
""
],
[
"Benomar",
"M.",
""
],
[
"Kriener",
"M.",
""
],
[
"Lorenz",
"T.",
""
],
[
"Sidis",
"Y.",
""
],
[
"Habicht",
"K.",
""
],
[
"Link",
"P.",
""
],
[
"Braden",
"M.",
""
]
] | [
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] |
801.1788 | Dong Ye | Dong Ye and Heping Zhang | Extremal fullerene graphs with the maximum Clar number | 35 pages, 43 figures | Discrete Appl. Math. 157 (2009) 3152-3173 | 10.1016/j.dam.2009.06.007 | null | math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A fullerene graph is a cubic 3-connected plane graph with (exactly 12)
pentagonal faces and hexagonal faces. Let $F_n$ be a fullerene graph with $n$
vertices. A set $\mathcal H$ of mutually disjoint hexagons of $F_n$ is a sextet
pattern if $F_n$ has a perfect matching which alternates on and off each
hexagon in $\mathcal H$. The maximum cardinality of sextet patterns of $F_n$ is
the Clar number of $F_n$. It was shown that the Clar number is no more than
$\lfloor\frac {n-12} 6\rfloor$. Many fullerenes with experimental evidence
attain the upper bound, for instance, $\text{C}_{60}$ and $\text{C}_{70}$. In
this paper, we characterize extremal fullerene graphs whose Clar numbers equal
$\frac{n-12} 6$. By the characterization, we show that there are precisely 18
fullerene graphs with 60 vertices, including $\text{C}_{60}$, achieving the
maximum Clar number 8 and we construct all these extremal fullerene graphs.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:30:43 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Aug 2009 12:19:53 GMT"
}
] | 2009-08-11T00:00:00 | [
[
"Ye",
"Dong",
""
],
[
"Zhang",
"Heping",
""
]
] | [
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] |
801.1789 | Ekaterina Christova | Ekaterina Christova and Elliot Leader | About S-\bar s, \Delta S-\Delta\bar s and D_d^{K+ - K-} in K^\pm
Production in Sidis | this is a talk given at the XII Workshop On High Energy Spin Physics
(DSPIN-07), September 3--7, 2007 at JINR, Dubna, Russia, 4 pages. to appear
in the proceedings of the workshop | null | null | null | hep-ph | null | We consider semi-inclusive unpolarized DIS for the production of charged
Kaons and the different possibilities, both in LO and NLO, to test the
conventionally used assumptions s-\bar s=0, \Delta s-\Delta \bar s=0 and
D_d^{K+ - K-}=0. The considered tests have the advantage that they do not
require any knowledge of the fragmentation functions.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:54:27 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Christova",
"Ekaterina",
""
],
[
"Leader",
"Elliot",
""
]
] | [
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] |
801.179 | Ian Appelbaum | Biqin Huang and Ian Appelbaum | Spin Dephasing in Drift-Dominated Semiconductor Spintronics Devices | null | Phys. Rev. B 77, 165331 (2008) | 10.1103/PhysRevB.77.165331 | null | cond-mat.mtrl-sci cond-mat.other | null | A spin transport model is employed to study the effects of spin dephasing
induced by diffusion-driven transit-time uncertainty through semiconductor
spintronic devices where drift is the dominant transport mechanism. It is found
that in the ohmic regime, dephasing is independent of transit length, and
determined primarily by voltage drop across the spin transport region. The
effects of voltage and temperature predicted by the model are compared to
experimental results from a 350-micron-thick silicon spin-transport device
using derived mathematical expressions of spin dephasing.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:40:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Huang",
"Biqin",
""
],
[
"Appelbaum",
"Ian",
""
]
] | [
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801.1791 | Christos Efthymiopoulos | Christos Efthymiopoulos, Tassos Bountis and Thanos Manos | Explicit Construction of First Integrals with Quasi-monomial Terms from
the Painlev\'{e} Series | 16 pages, 0 figures | null | 10.1070/RD2004v009n03ABEH000286 | null | nlin.SI | null | The Painlev\'{e} and weak Painlev\'{e} conjectures have been used widely to
identify new integrable nonlinear dynamical systems. For a system which passes
the Painlev\'{e} test, the calculation of the integrals relies on a variety of
methods which are independent from Painlev\'{e} analysis. The present paper
proposes an explicit algorithm to build first integrals of a dynamical system,
expressed as `quasi-polynomial' functions, from the information provided solely
by the Painlev\'{e} - Laurent series solutions of a system of ODEs.
Restrictions on the number and form of quasi-monomial terms appearing in a
quasi-polynomial integral are obtained by an application of a theorem by
Yoshida (1983). The integrals are obtained by a proper balancing of the
coefficients in a quasi-polynomial function selected as initial ansatz for the
integral, so that all dependence on powers of the time $\tau=t-t_0$ is
eliminated. Both right and left Painlev\'{e} series are useful in the method.
Alternatively, the method can be used to show the non-existence of a
quasi-polynomial first integral. Examples from specific dynamical systems are
given.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:36:57 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Efthymiopoulos",
"Christos",
""
],
[
"Bountis",
"Tassos",
""
],
[
"Manos",
"Thanos",
""
]
] | [
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] |
801.1792 | Dmitry Beliaev | D. Beliaev and S. Smirnov | Harmonic measure and SLE | null | null | 10.1007/s00220-009-0864-7 | null | math.CV math.PR | null | In this paper we rigorously compute the average multifractal spectrum of
harmonic measure on the boundary of SLE clusters.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:50:33 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Beliaev",
"D.",
""
],
[
"Smirnov",
"S.",
""
]
] | [
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] |
801.1793 | Giuseppe Falzetta doc | Giuseppe Falzetta | Realizzazione di un esperimento innovativo con doppia fenditura
utilizzando coppie correlate di fotoni | My master thesis in italian | null | null | null | quant-ph | null | In this Thesis I present a double slit experiment where two undistinguishable
photons produced by type I PDC are sent each to a well defined slit. Data about
the diffraction and interference patterns for coincidences are presented and
discussed. An analysis of these data allows a first test of standard quantum
mechanics against de Broglie-Bohm theory.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:43:20 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Falzetta",
"Giuseppe",
""
]
] | [
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] |
801.1794 | Partha Konar | Kaoru Hagiwara, Partha Konar, Qiang Li, Kentarou Mawatari, Dieter
Zeppenfeld | Graviton production with 2 jets at the LHC in large extra dimensions | 8 pages, 10 figures, 1 table; Version to be printed in JHEP | JHEP 0804:019,2008 | 10.1088/1126-6708/2008/04/019 | KA-TP-01-2008, KEK-TH-1217, KIAS-P08006, SFB/CPP-08-01,
UFIFT-HEP-08-01 | hep-ph | null | We study Kaluza-Klein (KK) graviton production in the large extra dimensions
model via 2 jets plus missing transverse momentum signatures at the LHC. We
make predictions for both the signal and the dominant Zjj and Wjj backgrounds,
where we introduce missing P_T-dependent jet selection cuts that ensure the
smallness of the 2-jet rate over the 1-jet rate. With the same jet selection
cuts, the distributions of the two jets and their correlation with the missing
transverse momentum provide additional evidence for the production of an
invisible massive object.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:44:27 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Mar 2008 20:00:37 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Hagiwara",
"Kaoru",
""
],
[
"Konar",
"Partha",
""
],
[
"Li",
"Qiang",
""
],
[
"Mawatari",
"Kentarou",
""
],
[
"Zeppenfeld",
"Dieter",
""
]
] | [
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] |
801.1795 | Aleksi Halkola | A. Halkola, H. Hildebrandt, T. Schrabback, M. Lombardi, M. Bradac, T.
Erben, P. Schneider, D. Wuttke | The mass distribution of RX J1347-1145 from strong lensing | Accepted for publication in the A&A | null | 10.1051/0004-6361:20078877 | null | astro-ph | null | High resolution HST/ACS images of the galaxy cluster RX J1347-1145 have
enabled us to identify several new multiple image candidates in the cluster,
including a 5 image system with a central image. The multiple images allow us
to construct an accurate 2-dimensional mass map of the central part of the
cluster. The modelling of the cluster mass includes the most prominent cluster
galaxies modelled as truncated isothermal spheres and a smooth halo component
that is described with 2 parametric profiles. The mass reconstruction is done
using a Markov chain Monte Carlo method that provides us with a total projected
mass density as well as estimates for the parameters of interest and their
respective errors. The mass profile is in reasonable agreement with previous
mass estimates based on the X-ray emission from the hot intra-cluster gas,
however the X-ray mass estimates are systematically lower than what we obtain
with gravitational lensing.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:54:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Halkola",
"A.",
""
],
[
"Hildebrandt",
"H.",
""
],
[
"Schrabback",
"T.",
""
],
[
"Lombardi",
"M.",
""
],
[
"Bradac",
"M.",
""
],
[
"Erben",
"T.",
""
],
[
"Schneider",
"P.",
""
],
[
"Wuttke",
"D.",
""
]
] | [
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] |
801.1796 | Alexander Khodjamirian | G.Duplancic, A.Khodjamirian, Th.Mannel, B.Melic, N.Offen | Light-cone sum rules for $B \to \pi$ form factors revisited | 33 pages, 7 figures, one figure and a few comments added, version to
appear in JHEP | JHEP 0804:014,2008 | 10.1088/1126-6708/2008/04/014 | SI-HEP-2007-15 | hep-ph | null | We reconsider and update the QCD light-cone sum rules for $B\to \pi$ form
factors. The gluon radiative corrections to the twist-2 and twist-3 terms in
the correlation functions are calculated. The $\bar{MS}$ $b$-quark mass is
employed, instead of the one-loop pole mass used in the previous analyses. The
light-cone sum rule for $f^+_{B\pi}(q^2)$ is fitted to the measured
$q^2$-distribution in $B\to \pi l \nu_l$, fixing the input parameters with the
largest uncertainty: the Gegenbauer moments of the pion distribution amplitude.
For the $B\to \pi$ vector form factor at zero momentum transfer we predict
$f^+_{B\pi}(0)= 0.26^{+0.04}_{-0.03}$. Combining it with the value of the
product $|V_{ub}f^+_{B\pi}(0)|$ extracted from experiment, we obtain
$|V_{ub}|=(3.5\pm 0.4\pm 0.2\pm 0.1) \times 10^{-3}$. In addition, the scalar
and penguin $B\to \pi$ form factors $f^0_{B\pi}(q^2)$ and $f^T_{B\pi}(q^2)$ are
calculated.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:59:02 GMT"
},
{
"version": "v2",
"created": "Thu, 3 Apr 2008 12:47:31 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Duplancic",
"G.",
""
],
[
"Khodjamirian",
"A.",
""
],
[
"Mannel",
"Th.",
""
],
[
"Melic",
"B.",
""
],
[
"Offen",
"N.",
""
]
] | [
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] |
801.1797 | Makoto Natsuume | Makoto Natsuume and Takashi Okamura | A note on causal hydrodynamics for M-theory branes | 6 pages, ReVTeX4 | Prog.Theor.Phys.120:1217-1222,2008 | 10.1143/PTP.120.1217 | KEK-TH-1221 | hep-th hep-ph nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We obtain new transport coefficients of causal hydrodynamics for the M2 and
the M5-brane using a Kubo-like formula proposed by Baier, Romatschke, Son,
Starinets, and Stephanov (arXiv:0712.2451 [hep-th]). The relaxation times agree
with the ones obtained from the "sound mode" in our paper (arXiv:0712.2916
[hep-th]).
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:40:11 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 19:46:28 GMT"
},
{
"version": "v3",
"created": "Wed, 10 Dec 2008 09:12:52 GMT"
}
] | 2008-12-25T00:00:00 | [
[
"Natsuume",
"Makoto",
""
],
[
"Okamura",
"Takashi",
""
]
] | [
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] |
801.1798 | Tobias Reichenbach | Tobias Reichenbach, Mauro Mobilia, and Erwin Frey | Self-Organization of Mobile Populations in Cyclic Competition | 21 pages, 10 figures. To appear in J. Theor. Biol | J. Theor. Biol. 254, 368-383 (2008) | 10.1016/j.jtbi.2008.05.014 | LMU-ASC 04/08 | q-bio.PE cond-mat.stat-mech nlin.AO physics.bio-ph | null | The formation of out-of-equilibrium patterns is a characteristic feature of
spatially-extended, biodiverse, ecological systems. Intriguing examples are
provided by cyclic competition of species, as metaphorically described by the
`rock-paper-scissors' game. Both experimentally and theoretically, such
non-transitive interactions have been found to induce self-organization of
static individuals into noisy, irregular clusters. However, a profound
understanding and characterization of such patterns is still lacking. Here, we
theoretically investigate the influence of individuals' mobility on the spatial
structures emerging in rock-paper-scissors games. We devise a quantitative
approach to analyze the spatial patterns self-forming in the course of the
stochastic time evolution. For a paradigmatic model originally introduced by
May and Leonard, within an interacting particle approach, we demonstrate that
the system's behavior - in the proper continuum limit - is aptly captured by a
set of stochastic partial differential equations. The system's stochastic
dynamics is shown to lead to the emergence of entangled rotating spiral waves.
While the spirals' wavelength and spreading velocity is demonstrated to be
accurately predicted by a (deterministic) complex Ginzburg-Landau equation,
their entanglement results from the inherent stochastic nature of the
system.These findings and our methods have important applications for
understanding the formation of noisy patterns, e.g., in ecological and
evolutionary contexts, and are also of relevance for the kinetics of
(bio)-chemical reactions.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:08:56 GMT"
},
{
"version": "v2",
"created": "Wed, 28 May 2008 11:23:18 GMT"
}
] | 2008-08-31T00:00:00 | [
[
"Reichenbach",
"Tobias",
""
],
[
"Mobilia",
"Mauro",
""
],
[
"Frey",
"Erwin",
""
]
] | [
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] |
801.1799 | Ivana Petkovi\'c | R. Latempa, M. Aprili and I. Petkovic | Quasiparticle Trapping In Three Terminal Ferromagnetic Tunneling Devices | null | null | 10.1063/1.3260237 | null | cond-mat.supr-con cond-mat.mes-hall | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Hybrid Superconductor/Ferromagnet structures have been investigated recently
to address the interplay between ferromagnetism and superconductivity. They
also open up new routes for the investigation of out of equilibrium
superconductivity. Here, we show how it is possible for out of equilibrium
excitations produced in a superconducting thin film (S) to be localized in a
ferromagnetic trap (F). Specifically, a ferromagnetic nano-volume in good
contact with S represents a potential well for the quasiparticles (QPs) at the
gap edge. As the superconducting proximity effect is highly suppressed in F,
QPs get efficiently trapped and they share their energy with the free electrons
in the trap. The electronic temperature Te in the trap can be increased by up
to 60% from the bath temperature at 320 mK as measured by tunneling
spectroscopy using a second junction.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:07:36 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 12:27:28 GMT"
},
{
"version": "v3",
"created": "Tue, 13 Jan 2009 13:30:35 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Latempa",
"R.",
""
],
[
"Aprili",
"M.",
""
],
[
"Petkovic",
"I.",
""
]
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801.18 | Michelangelo Mangano | T. Lari, L. Pape, W. Porod, J.A. Aguilar-Saavedra, F. del Aguila, B.C.
Allanach, J. Alwall, Yu. Andreev, D. Aristizabal Sierra, A. Bartl, M.
Beccaria, S. Bejar, L. Benucci, S. Bityukov, I. Borjanovic, G. Bozzi, G.
Burdman, J. Carvalho, N. Castro, B. Clerbaux, F. de Campos, A. de Gouvea, C.
Dennis, A. Djouadi, O.J.P. Eboli, U. Ellwanger, D. Fassouliotis, P.M.
Ferreira, R. Frederix, B. Fuks, J.-M. Gerard, A. Giammanco, S. Gopalakrishna,
T. Goto, B. Grzadkowski, J. Guasch, T. Hahn, S. Heinemeyer, A. Hektor, M.
Herquet, B. Herrmann, K. Hidaka, M. K. Hirsch, K. Hohenwarter-Sodek, W.
Hollik, G. W. S. Hou, T. Hurth, A. Ibarra, J. Illana, M. Kadastik, S.
Kalinin, C. Karafasoulis, M. Karagoz Unel, T. Kernreiter, M. M. Kirsanov, M.
Klasen, E. Kou, C. Kourkoumelis, S. Kraml, N. Krasnikov, F. Krauss, A.
Kyriakis, V. Lemaitre, G. Macorini, M.B. Magro, W. Majerotto, F. Maltoni, R.
Mehdiyev, M. Misiak, F. Moortgat, G. Moreau, M. M\"uhlleitner, M. Muntel, A.
Onofre, E. Ozcan, F. Palla, L. Panizzi, L. Pape, S. Penaranda, R. Pittau, G.
Polesello, A. Pukhov, M. Raidal, A.R. Raklev, L. Rebane, F. M. Renard, D.
Restrepo, Z. Roupas, R. Santos, S. Schumann, G. Servant, F. Siegert, P.
Skands, P. Slavich, J. Sola, M. Spira, S. Sultansoy, A. Toropin, A. Tricomi,
J. Tseng, G. Unel, J.W.F. Valle, F. Veloso, A. Ventura, G. Vermisoglou, C.
Verzegnassi, A. Villanova del Moral, G. Weiglein, M. Yilmaz | Collider aspects of flavour physics at high Q | Report of Working Group 1 of the CERN Workshop ``Flavour in the era
of the LHC'', Geneva, Switzerland, November 2005 -- March 2007 | Eur.Phys.J.C57:183-308,2008 | 10.1140/epjc/s10052-008-0713-4 | null | hep-ph hep-ex | null | This review presents flavour related issues in the production and decays of
heavy states at LHC, both from the experimental side and from the theoretical
side. We review top quark physics and discuss flavour aspects of several
extensions of the Standard Model, such as supersymmetry, little Higgs model or
models with extra dimensions. This includes discovery aspects as well as
measurement of several properties of these heavy states. We also present public
available computational tools related to this topic.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:34:00 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Lari",
"T.",
""
],
[
"Pape",
"L.",
""
],
[
"Porod",
"W.",
""
],
[
"Aguilar-Saavedra",
"J. A.",
""
],
[
"del Aguila",
"F.",
""
],
[
"Allanach",
"B. C.",
""
],
[
"Alwall",
"J.",
""
],
[
"Andreev",
"Yu.",
""
],
[
"Sierra",
"D. Aristizabal",
""
],
[
"Bartl",
"A.",
""
],
[
"Beccaria",
"M.",
""
],
[
"Bejar",
"S.",
""
],
[
"Benucci",
"L.",
""
],
[
"Bityukov",
"S.",
""
],
[
"Borjanovic",
"I.",
""
],
[
"Bozzi",
"G.",
""
],
[
"Burdman",
"G.",
""
],
[
"Carvalho",
"J.",
""
],
[
"Castro",
"N.",
""
],
[
"Clerbaux",
"B.",
""
],
[
"de Campos",
"F.",
""
],
[
"de Gouvea",
"A.",
""
],
[
"Dennis",
"C.",
""
],
[
"Djouadi",
"A.",
""
],
[
"Eboli",
"O. J. P.",
""
],
[
"Ellwanger",
"U.",
""
],
[
"Fassouliotis",
"D.",
""
],
[
"Ferreira",
"P. M.",
""
],
[
"Frederix",
"R.",
""
],
[
"Fuks",
"B.",
""
],
[
"Gerard",
"J. -M.",
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],
[
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"A.",
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],
[
"Gopalakrishna",
"S.",
""
],
[
"Goto",
"T.",
""
],
[
"Grzadkowski",
"B.",
""
],
[
"Guasch",
"J.",
""
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[
"Hahn",
"T.",
""
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[
"Heinemeyer",
"S.",
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[
"Hektor",
"A.",
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[
"Herquet",
"M.",
""
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[
"Herrmann",
"B.",
""
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[
"Hidaka",
"K.",
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[
"Hirsch",
"M. K.",
""
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"Hohenwarter-Sodek",
"K.",
""
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"Hollik",
"W.",
""
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[
"Hou",
"G. W. S.",
""
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"T.",
""
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[
"Ibarra",
"A.",
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[
"Illana",
"J.",
""
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"M.",
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"S.",
""
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[
"Karafasoulis",
"C.",
""
],
[
"Unel",
"M. Karagoz",
""
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[
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"T.",
""
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[
"Kirsanov",
"M. M.",
""
],
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"Klasen",
"M.",
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[
"Kou",
"E.",
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"C.",
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"V.",
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"G.",
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[
"Magro",
"M. B.",
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"Majerotto",
"W.",
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"F.",
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[
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"R.",
""
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"M.",
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"F.",
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"G.",
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"M.",
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"Sultansoy",
"S.",
""
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"A.",
""
],
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"A.",
""
],
[
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"J.",
""
],
[
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"G.",
""
],
[
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"J. W. F.",
""
],
[
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"F.",
""
],
[
"Ventura",
"A.",
""
],
[
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"G.",
""
],
[
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"C.",
""
],
[
"del Moral",
"A. Villanova",
""
],
[
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"G.",
""
],
[
"Yilmaz",
"M.",
""
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] | [
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801.1801 | Henri Gouin | Henri Gouin (LMMT, MSNMGP) | The wetting problem of fluids on solid surfaces. Part 1: the dynamics of
contact lines | Fichier preprint 28 pages | Continuum Mechanics and Thermodynamics 15, 6 (2003) 581-596 | 10.1007/s00161-003-0136-2 | null | physics.class-ph | null | The understanding of the spreading of liquids on solid surfaces is an
important challenge for contemporary physics. Today, the motion of the contact
line formed at the intersection of two immiscible fluids and a solid is still
subject to dispute. In this paper, a new picture of the dynamics of wetting is
offered through an example of non-Newtonian slow liquid movements. The
kinematics of liquids at the contact line and equations of motion are
revisited. Adherence conditions are required except at the contact line.
Consequently, for each fluid, the velocity field is multivalued at the contact
line and generates an equivalent concept of line friction but stresses and
viscous dissipation remain bounded. A Young-Dupr\'e equation for the apparent
dynamic contact angle between the interface and solid surface depending on the
movements of the fluid near the contact line is proposed.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:22:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gouin",
"Henri",
"",
"LMMT, MSNMGP"
]
] | [
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] |
801.1802 | Thorsten Feldmann | Thorsten Feldmann (TU Munich and Univ. Siegen), Thomas Mannel (Univ.
Siegen) | Large Top Mass and Non-Linear Representation of Flavour Symmetry | 4 pages, no figures, uses revtex4 | Phys.Rev.Lett.100:171601,2008 | 10.1103/PhysRevLett.100.171601 | SI-HEP-2008-01, TUM-HEP-680/08 | hep-ph hep-th | null | We consider an effective theory (ET) approach to flavour-violating processes
beyond the Standard Model (SM), where the breaking of flavour symmetry is
described by spurion fields whose low-energy vacuum expectation values are
identified with the SM Yukawa couplings. Insisting on canonical mass dimensions
for the spurion fields, the large top-quark Yukawa coupling also implies a
large expectation value for the associated spurion, which breaks part of the
flavour symmetry already at the UV scale Lambda of the ET. Below that scale,
flavour symmetry in the ET is represented in a non-linear way by introducing
Goldstone modes for the partly broken flavour symmetry and spurion fields
transforming under the residual symmetry. As a result, the dominance of certain
flavour structures in rare quark decays can be understood in terms of the
1/Lambda expansion in the ET. We also discuss the generalization to
2-Higgs-doublet models with large tan(beta).
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:30:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Feldmann",
"Thorsten",
"",
"TU Munich and Univ. Siegen"
],
[
"Mannel",
"Thomas",
"",
"Univ.\n Siegen"
]
] | [
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] |
801.1803 | Huang Jing | M. Amenomori, et al (for the Tibet ASgamma Collaboration) | The all-particle spectrum of primary cosmic rays in the wide energy
range from 10^14 eV to 10^17 eV observed with the Tibet-III air-shower array | 19 pages, 20 figures, accepted by ApJ | Astrophys.J.678:1165-1179,2008 | 10.1086/529514 | null | hep-ex astro-ph | null | We present an updated all-particle energy spectrum of primary cosmic rays in
a wide range from 10^14 eV to 10^17 eV using 5.5 times 10^7 events collected in
the period from 2000 November through 2004 October by the Tibet-III air-shower
array located at 4300 m above sea level (atmospheric depth of 606 g/cm^2). The
size spectrum exhibits a sharp knee at a corresponding primary energy around 4
PeV. This work uses increased statistics and new simulation calculations for
the analysis. We performed extensive Monte Carlo calculations and discuss the
model dependences involved in the final result assuming interaction models of
QGSJET01c and SIBYLL2.1 and primary composition models of heavy dominant (HD)
and proton dominant (PD) ones. Pure proton and pure iron primary models are
also examined as extreme cases. The detector simulation was also made to
improve the accuracy of determining the size of the air showers and the energy
of the primary particle. We confirmed that the all-particle energy spectra
obtained under various plausible model parameters are not significantly
different from each other as expected from the characteristics of the
experiment at the high altitude, where the air showers of the primary energy
around the knee reaches near maximum development and their features are
dominated by electromagnetic components leading to the weak dependence on the
interaction model or the primary mass. This is the highest-statistical and the
best systematics-controlled measurement covering the widest energy range around
the knee energy region.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:40:39 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Jan 2008 12:14:46 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Amenomori",
"M.",
""
]
] | [
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801.1804 | Bernhard Heim | Bernhard Heim | On the Spezialschar of Maass | null | null | null | null | math.NT math.CV | null | Let $M_k^{(n)}$ be the space of Siegel modular forms of degree $n$ and even
weight $k$. In this paper firstly a certain subspace
$\mathsf{Spez}(M_k^{(2n)})$ the Spezialschar of $M_k^{(2n)}$ is introduced. In
the setting of the Siegel three-fold it is proven that this Spezialschar is the
Maass Spezialschar. Secondly an embedding of $M_k^{(2)}$ into a direct sum
$\oplus_{\nu = 0}^{\lfloor \frac{k}{10} \rfloor} \text{Sym}^2 M_{k + 2 \nu}$ is
given. This leads to a basic characterization of the Spezialschar property. The
results of this paper are directly related to the non-vanishing of certain
special values of L-functions related to the Gross-Prasad conjecture. This is
illustrated by a significant example in the paper.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:55:34 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Heim",
"Bernhard",
""
]
] | [
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] |
801.1805 | Leonardo Vanni | R. Laura, L. Vanni | Conditional probabilities and collapse in quantum measurements | 15 pages | International Journal of Theoretical Physics, Volume 47, Issue 9,
(2008), pp. 2382-2392 | 10.1007/s10773-008-9672-7 | null | quant-ph | null | We show that including both the system and the apparatus in the quantum
description of the measurement process, and using the concept of conditional
probabilities, it is possible to deduce the statistical operator of the system
after a measurement with a given result, which gives the probability
distribution for all possible consecutive measurements on the system. This
statistical operator, representing the state of the system after the first
measurement, is in general not the same that would be obtained using the
postulate of collapse.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:07:36 GMT"
}
] | 2008-11-29T00:00:00 | [
[
"Laura",
"R.",
""
],
[
"Vanni",
"L.",
""
]
] | [
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] |
801.1806 | Philip Massey | Philip Massey, Emily M. Levesque, Bertrand Plez, K. A. G. Olsen | The Physical Properties of Red Supergiants: Comparing Theory and
Observations | Invited review; to appear in Massive Stars as Cosmic Engines, IAU
Symp. 250, ed. F. Bresolin, P. A. Crowther, and J. Puls (Cambridge University
Press) | null | 10.1017/S1743921308020383 | null | astro-ph | null | Red supergiants (RSGs) are an evolved stage in the life of intermediate
massive stars (than than 25 solar masses). For many years, their location in
the H-R diagram was at variance with the evolutionary models. Using the MARCS
stellar atmospheres, we have determined new effective temperatures and
bolometric luminosities for RSGs in the Milky Way, LMC, and SMC, and our work
has resulted in much better agreement with the evolutionary models. We have
also found evidence of significant visual extinction due to circumstellar dust.
Although in the Milky Way the RSGs contribute only a small fraction (than than
1 percent) of the dust to the interstellar medium (ISM), in starburst galaxies
or galaxies at large look-back times, we expect that RSGs may be the main dust
source. We are in the process of extending this work now to RSGs of higher and
lower metallicities using the galaxies M31 and WLM.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:30:41 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 23:28:22 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Massey",
"Philip",
""
],
[
"Levesque",
"Emily M.",
""
],
[
"Plez",
"Bertrand",
""
],
[
"Olsen",
"K. A. G.",
""
]
] | [
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] |
801.1807 | Sergei Urazhdin | Weng L. Lim, Nicholas Anthony, Andrew Higgins, Sergei Urazhdin | Thermal Dynamics in Symmetric Magnetic Nanopillars Driven by Spin
Transfer | 3 pages, 3 figures | null | 10.1063/1.2918012 | null | cond-mat.mtrl-sci | null | We study the effects of spin transfer on thermally activated dynamics of
magnetic nanopillars with identical thicknesses of the magnetic layers. The
symmetric nanopillars exhibit anomalous dependencies of switching statistics on
magnetic field and current. We interpret our data in terms of simultaneous
current-induced excitation of both layers. We also find evidence for coupling
between the fluctuations of the layers due to the spin transfer.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:19:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lim",
"Weng L.",
""
],
[
"Anthony",
"Nicholas",
""
],
[
"Higgins",
"Andrew",
""
],
[
"Urazhdin",
"Sergei",
""
]
] | [
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] |
801.1808 | Pablo I. Tamborenea | C. L. Romano, P. I. Tamborenea, and S. E. Ulloa | Spin-orbit effects on two-electron states in nanowhisker double quantum
dots | 5 pages, 6 figures | null | 10.1016/j.physe.2009.04.039 | null | cond-mat.mes-hall | null | We investigate theoretically the combined effects of the electron-electron
and the Rashba spin-orbit interactions on two electrons confined in
quasi-one-dimensional AlInSb-based double quantum dots. We calculate the
two-electron wave functions and explore the interplay between these two
interactions on the energy levels and the spin of the states. The energy
spectrum as a function of an applied magnetic field shows crossings and
anticrossings between triplet and singlet states, associated with level mixing
induced by the spin-orbit coupling. We find that the fields at which these
crossings occur can be naturally controlled by the interdot barrier width,
which controls the exchange integral in the structure.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:26:35 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Romano",
"C. L.",
""
],
[
"Tamborenea",
"P. I.",
""
],
[
"Ulloa",
"S. E.",
""
]
] | [
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] |
801.1809 | Reinhard Laubenbacher | Reinhard Laubenbacher and David Pengelley | "Voici ce que j'ai trouve": Sophie Germain's grand plan to prove
Fermat's Last Theorem | to appear in Historia Mathematica | Historia Mathematica 37 (2010) 641-692 | 10.1016/j.hm.2009.12.002 | null | math.HO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A study of Sophie Germain's extensive manuscripts on Fermat's Last Theorem
calls for a reassessment of her work in number theory. There is much in these
manuscripts beyond the single theorem for Case 1 for which she is known from a
published footnote by Legendre. Germain had a fully-fledged, highly developed,
sophisticated plan of attack on Fermat's Last Theorem. The supporting
algorithms she invented for this plan are based on ideas and results discovered
independently only much later by others, and her methods are quite different
from any of Legendre's. In addition to her program for proving Fermat's Last
Theorem in its entirety, Germain also made major efforts at proofs for
particular families of exponents. The isolation Germain worked in, due in
substantial part to her difficult position as a woman, was perhaps sufficient
that much of this extensive and impressive work may never have been studied and
understood by anyone.
| [
{
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{
"version": "v2",
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},
{
"version": "v3",
"created": "Fri, 9 Jul 2010 06:47:35 GMT"
}
] | 2019-12-20T00:00:00 | [
[
"Laubenbacher",
"Reinhard",
""
],
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801.181 | Bernhard Heim | Bernhard Heim | A Strong Symmetry Property Of Eisenstein Series | To appear in the conference volume "Modular forms" Schiermonnikoog
2006, by B. Edixhoven, G.van der Geer, and B. Moonen | null | null | null | math.NT | null | In this paper we present a new method to study Fourier coefficients of
holomorphic and non-holomorphic Eisenstein series simultaneously.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:34:02 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Heim",
"Bernhard",
""
]
] | [
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] |
801.1811 | Abhay Ashtekar | Abhay Ashtekar, Victor Taveras, Madhavan Varadarajan | Information is Not Lost in the Evaporation of 2-dimensional Black Holes | 4 pages, 2 figures | Phys.Rev.Lett.100:211302,2008 | 10.1103/PhysRevLett.100.211302 | IGC-08/01-02 | gr-qc hep-th | null | We analyze Hawking evaporation of the Callen-Giddings-Harvey-Strominger
(CGHS) black holes from a quantum geometry perspective and show that
information is not lost, primarily because the quantum space-time is
sufficiently larger than the classical. Using suitable approximations to
extract physics from quantum space-times we establish that: i)future null
infinity of the quantum space-time is sufficiently long for the the past vacuum
to evolve to a pure state in the future; ii) this state has a finite norm in
the future Fock space; and iii) all the information comes out at future
infinity; there are no remnants.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:36:26 GMT"
},
{
"version": "v2",
"created": "Thu, 22 May 2008 13:39:24 GMT"
}
] | 2015-01-30T00:00:00 | [
[
"Ashtekar",
"Abhay",
""
],
[
"Taveras",
"Victor",
""
],
[
"Varadarajan",
"Madhavan",
""
]
] | [
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] |
801.1812 | Daniel M. Pellegrino | G. Botelho, M. C. Matos and D. Pellegrino | Lineability of summing sets of homogeneous polynomials | 15 pages | null | null | null | math.FA | null | Given a continuous $n$-homogeneous polynomial $P\colon E\longrightarrow F$
between Banach spaces and $1\leq q\leq p<\infty$, in this paper we investigate
some properties concerning lineability and spaceability of the $(p;q)$-summing
set of $P$, defined by $S_{p;q}(P)=\{a\in E:P\mathrm{is}% (p;q)\mathrm{summing
at}a\}$.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:24:22 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Botelho",
"G.",
""
],
[
"Matos",
"M. C.",
""
],
[
"Pellegrino",
"D.",
""
]
] | [
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] |
801.1813 | David Tong | Chris Pedder, Julian Sonner and David Tong | The Berry Phase of D0-Branes | 14 pages, 1 figure. v3: references added | JHEP 0803:065,2008 | 10.1088/1126-6708/2008/03/065 | null | hep-th | null | We study SU(2) Yang-Mills quantum mechanics with N=2,4,8 and 16 supercharges.
This describes the non-relativistic dynamics of a pair of D0-branes moving in
d=3,4,6 and 10 spacetime dimensions respectively. We show that as the D0-branes
orbit, states undergo a Berry holonomy described by the four Hopf maps. For the
N=2 theory, the associated Hopf map is the Mobius bundle and its effect is to
turn the D0-branes into anyons with exchange statistics +i and -i. For the
N=4,8 and 16 theories, the Hopf maps give rise to Berry connections that are
familiar to physicists: the U(1) Dirac monopole; the SU(2) Yang monopole; and
the SO(8) octonionic monopole.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:43:21 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jan 2008 12:42:44 GMT"
},
{
"version": "v3",
"created": "Mon, 4 Feb 2008 17:18:09 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Pedder",
"Chris",
""
],
[
"Sonner",
"Julian",
""
],
[
"Tong",
"David",
""
]
] | [
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] |
801.1814 | Antonio Di Lorenzo | Antonio Di Lorenzo and J. Carlos Egues | Weak measurement: Effect of the detector dynamics | 5 pages, 3 figures. References added. Minor revisions | Phys. Rev. A 77, 042108 (2008) (5 pages) | 10.1103/PhysRevA.77.042108 | null | quant-ph cond-mat.other | null | A general approach to the measurement of an observable with pre- and
post-selection is presented. The limit of weak measurement is studied in
detail, and it is shown that the phase of the probe, including a Hamiltonian
contribution to it, gives rise to observable effects, since the coherence of
the probe is essential for the concept of complex weak value to be meaningful.
As a particular example, the measurement of a spin component is considered. We
find that the contribution of the imaginary part of the weak value is sizeable
in this case.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 17:59:45 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Apr 2008 21:22:35 GMT"
}
] | 2008-04-19T00:00:00 | [
[
"Di Lorenzo",
"Antonio",
""
],
[
"Egues",
"J. Carlos",
""
]
] | [
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] |
801.1815 | M. A. Baranov | M.A. Baranov, C. Lobo, and G.V. Shlyapnikov | Superfluid pairing between fermions with unequal masses | 21 pages, 9 figures, 1 table, discussions added | Phys.Rev.A78:033620,2008 | 10.1103/PhysRevA.78.033620 | null | cond-mat.other cond-mat.supr-con | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider a superfluid state in a two-component gas of fermionic atoms with
equal densities and unequal masses in the BCS limit. We develop a perturbation
theory along the lines proposed by Gorkov and Melik-Barkhudarov and find that
for a large difference in the masses of heavy ($M$) and light ($m$) atoms one
has to take into account both the second-order and third-order contributions.
The result for the critical temperature and order parameter is then quite
different from the prediction of the simple BCS approach. Moreover, the small
parameter of the theory turns out to be $(p_{F}|a|)/\hbar)\sqrt{M/m}\ll1$,
where $p_{F}$ is the Fermi momentum, and $a$ the scattering length. Thus, for a
large mass ratio $M/m$ the conventional perturbation theory requires
significantly smaller Fermi momenta (densities) or scattering lengths than in
the case of $M\sim m$, where the small parameter is $(p_{F}|a|)/\hbar)\ll1$. We
show that 3-body scattering resonances appearing at a large mass ratio due to
the presence of 3-body bound Efimov states do not influence the result, which
in this sense becomes universal.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:06:13 GMT"
},
{
"version": "v2",
"created": "Wed, 11 Jun 2008 13:18:49 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Baranov",
"M. A.",
""
],
[
"Lobo",
"C.",
""
],
[
"Shlyapnikov",
"G. V.",
""
]
] | [
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801.1816 | Georgios Mountrichas | G. Mountrichas, T. Shanks, S. M. Croom, U. Sawangwit, D. P. Schneider,
A. D. Myers, K. Pimbblet | QSO-LRG 2-Point Cross-Correlation Function and Redshift-Space Distorions | 22 pages, 25 figures, 8 tables | null | 10.1111/j.1365-2966.2009.14456.x | null | astro-ph | null | We have measured the bias of QSOs as a function of QSO luminosity at fixed
redshift (z<1) by cross-correlating them with LRGs in the same spatial volume,
hence breaking the degeneracy between QSO luminosity and redshift. We use three
QSO samples from 2SLAQ, 2QZ and SDSS covering a QSO absolute magnitude range,
-24.5<M_{b_J}<-21.5, and cross-correlate them with 2SLAQ (z~0.5) and AAOmega
(z~0.7) photometric and spectroscopic LRGs in the same redshift ranges. The 2-D
and 3-D cross-clustering measurements are generally in good agreement. Our
(2SLAQ) QSO-LRG clustering amplitude (r_0=6.8_{-0.3}^{+0.1}h^{-1}Mpc) as
measured from the semi-projected cross-correlation function appears similar to
the (2SLAQ) LRG-LRG auto-correlation amplitude (r_0=7.45\pm0.35h^{-1}Mpc) and
both are higher than the (2QZ+2SLAQ) QSO-QSO amplitude (r_0\simeq5.0h^{-1}Mpc).
Our measurements show remarkably little QSO-LRG cross-clustering dependence on
QSO luminosity. If anything, the results imply that brighter QSOs may be less
highly biased than faint QSOs, the opposite direction expected from simple high
peaks biasing models. Assuming a standard LCDM model and values for b_{LRG}
measured from LRG autocorrelation analyses, we find b_Q=1.45\pm0.11 at
M_{b_J}\approx-24 and b_Q=1.90\pm0.16 at M_{b_J}~-22. We also find consistent
results for the QSO bias from a z-space distortion analysis of the QSO-LRG
cross-clustering at z~0.55. The dynamical infall results give \beta
_Q=0.55\pm0.10, implying b_Q=1.4\pm0.2. Thus both the z-space distortion and
the amplitude analyses yield b_Q~1.5 at M_{b_J}~-23. The implied DM halo mass
inhabited by QSOs at z~0.55 is \sim10^{13}h^{-1}M_{\sun}, again approximately
independent of QSO luminosity.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:16:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mountrichas",
"G.",
""
],
[
"Shanks",
"T.",
""
],
[
"Croom",
"S. M.",
""
],
[
"Sawangwit",
"U.",
""
],
[
"Schneider",
"D. P.",
""
],
[
"Myers",
"A. D.",
""
],
[
"Pimbblet",
"K.",
""
]
] | [
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0.047613468,
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] |
801.1817 | Federico Mescia DR | FlaviaNet Working Group on Kaon Decays, M. Antonelli, V. Cirigliano,
P. Franzini, S. Glazov, R. Hill, G. Isidori, F. Mescia, M. Moulson, M.
Palutan, E. Passemar, M. Piccini, M. Veltri, O. Yushchenko, R.Wanke | Precision tests of the Standard Model with leptonic and semileptonic
kaon decays | null | Nucl.Phys.Proc.Suppl.181-182:83-88,2008 | 10.1016/j.nuclphysbps.2008.09.008 | null | hep-ph | null | We present a global analysis of leptonic and semileptonic kaon decays data,
including all recent results by BNL-E865, KLOE, KTeV, ISTRA+, and NA48.
Experimental results are critically reviewed and combined, taking into account
theoretical (both analytical and numerical) constraints on the semileptonic
kaon form factors. This analysis leads to a very accurate determination of Vus
and allows us to perform several stringent tests of the Standard Model.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:57:43 GMT"
}
] | 2012-08-27T00:00:00 | [
[
"FlaviaNet Working Group",
"",
""
],
[
"Antonelli",
"M.",
""
],
[
"Cirigliano",
"V.",
""
],
[
"Franzini",
"P.",
""
],
[
"Glazov",
"S.",
""
],
[
"Hill",
"R.",
""
],
[
"Isidori",
"G.",
""
],
[
"Mescia",
"F.",
""
],
[
"Moulson",
"M.",
""
],
[
"Palutan",
"M.",
""
],
[
"Passemar",
"E.",
""
],
[
"Piccini",
"M.",
""
],
[
"Veltri",
"M.",
""
],
[
"Yushchenko",
"O.",
""
],
[
"Wanke",
"R.",
""
]
] | [
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801.1818 | Antonio De Nicola | Beniamino Cappelletti Montano, Antonio De Nicola, Giulia Dileo | The geometry of 3-quasi-Sasakian manifolds | 22 pages, LaTeX, to appear in Internat. J. Math | Internat. J. Math. 20 (2009), 1081-1105. | 10.1142/S0129167X09005662 | DMUC 07-38 | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | 3-quasi-Sasakian manifolds were studied systematically by the authors in a
recent paper as a suitable setting unifying 3-Sasakian and 3-cosymplectic
geometries. This paper throws new light on their geometric structure which
reveals to be generally richer compared to the 3-Sasakian subclass. In fact, it
turns out that they are multiply foliated by four distinct fundamental
foliations. The study of the transversal geometries with respect to these
foliations allows us to link the 3-quasi-Sasakian manifolds to the more famous
hyper-Kaehler and quaternionic-Kaehler geometries. Furthermore, we strongly
improve the splitting results previously found; we prove that any
3-quasi-Sasakian manifold of rank 4l+1 is 3-cosymplectic and any
3-quasi-Sasakian manifold of maximal rank is 3-alpha-Sasakian.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:43:29 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jul 2008 19:04:55 GMT"
}
] | 2009-10-27T00:00:00 | [
[
"Montano",
"Beniamino Cappelletti",
""
],
[
"De Nicola",
"Antonio",
""
],
[
"Dileo",
"Giulia",
""
]
] | [
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] |
801.1819 | Abraham Jalbout | Abraham F. Jalbout and Thomas H. Seligman | Electron Localization on Molecular Surfaces by Metal Adsorption | This manuscript was accepted for publication on January 3, 2008 to
the Journal of Computational and Theoretical Nanoscience (JCTN) | null | null | null | cond-mat.mtrl-sci | null | The ability of metal adsorption to transfer charge to the surface of single
molecular carbon sheets is explored in this paper. Though other metals are
considered we basically will deal with Lithium We concentrate on fairly small
sheets and examined the minimum threshold size of a molecular surface needed to
separate metals. From our quantum chemical calculations we deduce that a
molecular surface of six benzene rings is needed for Lithium dimers to be
separated. We further observe symmetry breaking, when two lithium atoms are
adsorbed right opposite to each other on the two sides of the sheet.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:45:36 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Jalbout",
"Abraham F.",
""
],
[
"Seligman",
"Thomas H.",
""
]
] | [
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] |
801.182 | I. V. Zozoulenko | I. V. Zozoulenko, S. Ihnatsenko | Magnetoconductance of interacting electrons in quantum wires: Spin
density functional theory study | null | Physical Review B 78, 78, 035340 (2008) | 10.1103/PhysRevB.78.035340 | null | cond-mat.mes-hall | null | We present systematic quantitative description of the magnetoconductance of
the split-gate quantum wires. Accounting for the exchange and correlation
interactions within the spin density function theory (DFT) leads to the lifting
of the spin degeneracy and formation of the spin-resolved plateaus at odd
values of $e^{2}/h$. We show that the width of the odd conductance steps in the
spin DFT calculations is equal to the width of the transition intervals between
the conductance steps for the spinless electrons in the Hartree approximation.
A detailed analysis of the structure of compressible/incompressible strips and
the evolution of the Hartree and the spin-DFT subband structure provides an
explanation of this finding. Our spin-DFT calculations reproduce not only
qualitatively, but rather quantitatively all the features in the
magnetoconductance observed in the recent experiment (I. P. Radu, J. B. Miller,
S. Amasha, E. Levenson-Falk, D. M. Zumbuhl, M. A. Kastner, C. M. Marcus, L. N.
Pfeiffer, and K. W. West, to be published) including the unexpected effect of
the collapse of the odd conductance plateaus at lower fields.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:49:56 GMT"
}
] | 2009-05-26T00:00:00 | [
[
"Zozoulenko",
"I. V.",
""
],
[
"Ihnatsenko",
"S.",
""
]
] | [
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801.1821 | Konstantin Chetyrkin G. | P.A. Baikov, K.G. Chetyrkin and J.H. K\"uhn | Hadronic Z- and tau-Decays in Order alpha_s^4 | few citations added, final published version | Phys.Rev.Lett.101:012002,2008 | 10.1103/PhysRevLett.101.012002 | SFB/CPP-08-04, TTP08-01 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Using recently developed methods for the evaluation of five-loop amplitudes
in perturbative QCD, corrections of order alpha_s^4 for the cross section of
electron-positron annihilation into hadrons and for the decay rates of the
Z-boson and the tau-lepton into hadrons are evaluated. The new terms lead to a
significant stabilization of the perturbative series, to a reduction of the
theory uncertainly in the strong coupling constant alpha_s, as extracted from
these measurements, and to a small shift of the central value, moving two
central values closer together. The agreement between two values of alpha_s
measured at vastly different energies constitutes a striking test of asymptotic
freedom. Combining the results from Z and tau decays we find
alpha_s(M_Z)=0.1198 \pm 0.0015 as one of the most precise and presently only
result for the strong coupling constant in order alpha_s^4.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:11:37 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Jul 2008 15:09:36 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Baikov",
"P. A.",
""
],
[
"Chetyrkin",
"K. G.",
""
],
[
"Kühn",
"J. H.",
""
]
] | [
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801.1822 | Gerald Hoehn | Gerald Hoehn | Self-Dual Vertex Operator Superalgebras of Large Minimal Weight | 18 pages with 1 table, LaTeX | null | null | null | math.QA math-ph math.MP | null | The new general upper bound mu <= [c/24] + 1 for the minimal weight mu of a
self-dual vertex operator superalgebra of central charge c different from 47/2
is proven. For central charges c <= 48, further improved estimates are given
and examples of with large minimal weight are discussed. We also study the case
of vertex operator superalgebras with N=1 supersymmetry which was first
considered by Witten in connection with three-dimensional quantum gravity. The
upper bound mu^* <= (1/2)[c/12]+1/2 for the minimal superconformal weight is
obtained for c different from 47/2.
In addition, we show that it is impossible that the monster sporadic group
acts on an extremal self-dual N=1 supersymmetric vertex operator superalgebra
of central charge 48 in a way proposed by Witten if certain standard
assumptions about orbifold constructions hold. The same statement holds for
extremal self-dual vertex operator algebras of central charge 48.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:17:38 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Hoehn",
"Gerald",
""
]
] | [
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] |
801.1823 | Manuel Tiglio | Oleg Korobkin, Burak Aksoylu, Michael Holst, Enrique Pazos, Manuel
Tiglio | Solving the Einstein constraint equations on multi-block triangulations
using finite element methods | Changes made to match the version to appear in Classical and Quantum
Gravity | Class. Quantum Grav. 26, 145007 (2009) | 10.1088/0264-9381/26/14/145007 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In order to generate initial data for nonlinear relativistic simulations, one
needs to solve the Einstein constraints, which can be cast into a coupled set
of nonlinear elliptic equations. Here we present an approach for solving these
equations on three-dimensional multi-block domains using finite element
methods. We illustrate our approach on a simple example of Brill wave initial
data, with the constraints reducing to a single linear elliptic equation for
the conformal factor $\psi$. We use quadratic Lagrange elements on
semi-structured simplicial meshes, obtained by triangulation of multi-block
grids. In the case of uniform refinement the scheme is superconvergent at most
mesh vertices, due to local symmetry of the finite element basis with respect
to local spatial inversions. We show that in the superconvergent case
subsequent unstructured mesh refinements do not improve the quality of our
initial data. As proof of concept that this approach is feasible for generating
multi-block initial data in three dimensions, after constructing the initial
data we evolve them in time using a high order finite-differencing multi-block
approach and extract the gravitational waves from the numerical solution.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:20:08 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 21:33:19 GMT"
},
{
"version": "v3",
"created": "Wed, 3 Jun 2009 07:05:21 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Korobkin",
"Oleg",
""
],
[
"Aksoylu",
"Burak",
""
],
[
"Holst",
"Michael",
""
],
[
"Pazos",
"Enrique",
""
],
[
"Tiglio",
"Manuel",
""
]
] | [
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] |
801.1824 | Jaime Julve | J. Julve and F. J. de Urries | Tunnelling of plane waves through a square barrier | 16 pages | null | 10.1088/1751-8113/41/30/304010 | null | quant-ph | null | The time evolution of plane waves in the presence of a 1-dimensional square
quantum barrier is considered. Comparison is made between the cases of an
infinite and a cut-off (shutter) initial plane wave. The difference is relevant
when the results are applied to the analysis of the tunnelling regime. This
work is focused on the analytical calculation of the time-evolved solution and
highlights the contribution of the resonant (Gamow) states.
PACS numbers: 11.10.Ef, 11.10.Lm, 04.60
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:27:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Julve",
"J.",
""
],
[
"de Urries",
"F. J.",
""
]
] | [
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] |
801.1825 | Steven Diehl | Steven Diehl (T-6, LANL), Hui Li (T-6, LANL), Chris Fryer (CCS-2,
LANL), David Rafferty (Penn State) | Constraining the Nature of X-ray Cavities in Clusters and Galaxies | 21 pages, 12 figures, emulateapj, accepted for publication in ApJ,
responded to referee's comments and added a new model, conclusions unchanged | null | 10.1086/591310 | LA-UR-07-7698 | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present results from an extensive survey of 64 cavities in the X-ray halos
of clusters, groups and normal elliptical galaxies. We show that the evolution
of the size of the cavities as they rise in the X-ray atmosphere is
inconsistent with the standard model of adiabatic expansion of purely
hydrodynamic models. We also note that the majority of the observed bubbles
should have already been shredded apart by Rayleigh-Taylor and
Richtmyer-Meshkov instabilities if they were of purely hydrodynamic nature.
Instead we find that the data agrees much better with a model where the
cavities are magnetically dominated and inflated by a current-dominated
magneto-hydrodynamic jet model, recently developed by Li et al. (2006) and
Nakamura et al. (2006). We conduct complex Monte-Carlo simulations of the
cavity detection process including incompleteness effects to reproduce the
cavity sample's characteristics. We find that the current-dominated model
agrees within 1sigma, whereas the other models can be excluded at >5sigma
confidence. To bring hydrodynamic models into better agreement, cavities would
have to be continuously inflated. However, these assessments are dependent on
our correct understanding of the detectability of cavities in X-ray
atmospheres, and will await confirmation when automated cavity detection tools
become available in the future. Our results have considerable impact on the
energy budget associated with active galactic nucleus feedback.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:34:46 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Jul 2008 17:56:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Diehl",
"Steven",
"",
"T-6, LANL"
],
[
"Li",
"Hui",
"",
"T-6, LANL"
],
[
"Fryer",
"Chris",
"",
"CCS-2,\n LANL"
],
[
"Rafferty",
"David",
"",
"Penn State"
]
] | [
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] |
801.1826 | Michelangelo Mangano | M. Raidal, A. van der Schaaf, I. Bigi, M.L. Mangano, Y. Semertzidis,
S. Abel, S. Albino, S. Antusch, E. Arganda, B. Bajc, S. Banerjee, C. Biggio,
M. Blanke, W. Bonivento, G.C. Branco, D. Bryman, A.J. Buras, L. Calibbi, A.
Ceccucci, P.H. Chankowski, S. Davidson, A. Deandrea, D.P. DeMille, F.
Deppisch, M. Diaz, B. Duling, M. Felcini, W. Fetscher, D.K. Ghosh, M.
Giffels, G. Giudice, E. Goudzovskij, T. Han, P.G. Harris, M.J. Herrero, J.
Hisano, R.J. Holt, K. Huitu, A. Ibarra, O. Igonkina, A. Ilakovac, J. Imazato,
G. Isidori, F.R. Joaquim, M. Kadastik, Y. Kajiyama, S.F. King, K. Kirch, M.G.
Kozlov, M. Krawczyk, T. Kress, O. Lebedev, A. Lusiani, E. Ma, G. Marchiori,
I. Masina, G. Moreau, T. Mori, M. Muntel, F. Nesti, C.J.G. Onderwater, P.
Paradisi, S.T. Petcov, M. Picariello, V. Porretti, A. Poschenrieder, M.
Pospelov, L. Rebane, M.N. Rebelo, A. Ritz, L. Roberts, A. Romanino, A. Rossi,
R. Rueckl, G. Senjanovic, N. Serra, T. Shindou, Y. Takanishi, C. Tarantino,
A.M. Teixeira, E. Torrente-Lujan, K.J. Turzynski, T.E.J. Underwood, S.K.
Vempati, O. Vives | Flavour physics of leptons and dipole moments | Report of Working Group 3 of the CERN Workshop ``Flavour in the era
of the LHC'', Geneva, Switzerland, November 2005 -- March 2007 | Eur.Phys.J.C57:13-182,2008 | 10.1140/epjc/s10052-008-0715-2 | null | hep-ph hep-ex | null | This chapter of the report of the ``Flavour in the era of the LHC'' Workshop
discusses the theoretical, phenomenological and experimental issues related to
flavour phenomena in the charged lepton sector and in flavour-conserving
CP-violating processes. We review the current experimental limits and the main
theoretical models for the flavour structure of fundamental particles. We
analyze the phenomenological consequences of the available data, setting
constraints on explicit models beyond the Standard Model, presenting benchmarks
for the discovery potential of forthcoming measurements both at the LHC and at
low energy, and exploring options for possible future experiments.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:25:25 GMT"
}
] | 2008-12-18T00:00:00 | [
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"G. C.",
""
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"D.",
""
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[
"Buras",
"A. J.",
""
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[
"Calibbi",
"L.",
""
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"A.",
""
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[
"Chankowski",
"P. H.",
""
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"S.",
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[
"Deandrea",
"A.",
""
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[
"DeMille",
"D. P.",
""
],
[
"Deppisch",
"F.",
""
],
[
"Diaz",
"M.",
""
],
[
"Duling",
"B.",
""
],
[
"Felcini",
"M.",
""
],
[
"Fetscher",
"W.",
""
],
[
"Ghosh",
"D. K.",
""
],
[
"Giffels",
"M.",
""
],
[
"Giudice",
"G.",
""
],
[
"Goudzovskij",
"E.",
""
],
[
"Han",
"T.",
""
],
[
"Harris",
"P. G.",
""
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[
"Herrero",
"M. J.",
""
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[
"Hisano",
"J.",
""
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"Holt",
"R. J.",
""
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"Huitu",
"K.",
""
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"Ibarra",
"A.",
""
],
[
"Igonkina",
"O.",
""
],
[
"Ilakovac",
"A.",
""
],
[
"Imazato",
"J.",
""
],
[
"Isidori",
"G.",
""
],
[
"Joaquim",
"F. R.",
""
],
[
"Kadastik",
"M.",
""
],
[
"Kajiyama",
"Y.",
""
],
[
"King",
"S. F.",
""
],
[
"Kirch",
"K.",
""
],
[
"Kozlov",
"M. G.",
""
],
[
"Krawczyk",
"M.",
""
],
[
"Kress",
"T.",
""
],
[
"Lebedev",
"O.",
""
],
[
"Lusiani",
"A.",
""
],
[
"Ma",
"E.",
""
],
[
"Marchiori",
"G.",
""
],
[
"Masina",
"I.",
""
],
[
"Moreau",
"G.",
""
],
[
"Mori",
"T.",
""
],
[
"Muntel",
"M.",
""
],
[
"Nesti",
"F.",
""
],
[
"Onderwater",
"C. J. G.",
""
],
[
"Paradisi",
"P.",
""
],
[
"Petcov",
"S. T.",
""
],
[
"Picariello",
"M.",
""
],
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"Porretti",
"V.",
""
],
[
"Poschenrieder",
"A.",
""
],
[
"Pospelov",
"M.",
""
],
[
"Rebane",
"L.",
""
],
[
"Rebelo",
"M. N.",
""
],
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"Ritz",
"A.",
""
],
[
"Roberts",
"L.",
""
],
[
"Romanino",
"A.",
""
],
[
"Rossi",
"A.",
""
],
[
"Rueckl",
"R.",
""
],
[
"Senjanovic",
"G.",
""
],
[
"Serra",
"N.",
""
],
[
"Shindou",
"T.",
""
],
[
"Takanishi",
"Y.",
""
],
[
"Tarantino",
"C.",
""
],
[
"Teixeira",
"A. M.",
""
],
[
"Torrente-Lujan",
"E.",
""
],
[
"Turzynski",
"K. J.",
""
],
[
"Underwood",
"T. E. J.",
""
],
[
"Vempati",
"S. K.",
""
],
[
"Vives",
"O.",
""
]
] | [
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801.1827 | Cindy Regal | C. A. Regal, J. D. Teufel, and K. W. Lehnert | Measuring nanomechanical motion with a microwave cavity interferometer | Minor changes and corrections to text and figures; 7 pages, 6 figures | Nature Physics 4, 555 (2008) | null | null | quant-ph cond-mat.other | null | In recent years microfabricated microwave cavities have been extremely
successful in a wide variety of detector applications. In this article we focus
this technology on the challenge of quantum-limited displacement detection of a
macroscopic object. We measure the displacement of a nanomechanical beam by
capacitively coupling its position to the resonant frequency of a
superconducting transmission-line microwave cavity. With our device we realize
near state-of-the-art mechanical force sensitivity (3 $\rm{aN/\sqrt{Hz}}$) and
thus add to only a handful of techniques able to measure thermomechanical
motion at 10's of milliKelvin temperatures. Our measurement imprecision reaches
a promising 30 times the expected imprecision at the standard quantum limit,
and we quantify our ability to extract measurement backaction from our results
as well as elucidate the important steps that will be required to progress
towards the full quantum limit with this new detector.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:40:13 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Apr 2008 17:37:41 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Regal",
"C. A.",
""
],
[
"Teufel",
"J. D.",
""
],
[
"Lehnert",
"K. W.",
""
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] |
801.1828 | Jacob Lund Fisker | R.D. Hoffman, J.L. Fisker, J. Pruet, S.E. Woosley, H.-T. Janka, R.
Buras | Nucleosynthesis in Early Neutrino Driven Winds | 4 pages, 4 figures, proceedings for CNR 2007 Compound-Nuclear
Reactions and Related Topics Workshop | AIP Conf.Proc.1005:225-228,2008 | 10.1063/1.2920736 | null | astro-ph | null | Nucleosynthesis in early neutrino winds is investigated. Presented is a brief
overview of two recent problems of supernova nucleosynthesis. In the first part
we investigate the effect of nuclear parameters on the synthesis of Mo92 and
Mo94. Based on recent experimental results, we find that the proton rich winds
of the model investigated here can not be the source of solar Mo92 and Mo94. In
the second part we investigate the nucleosynthesis from neutron rich bubbles
and show that they do not contribute to the overall nucleosynthesis.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:32:25 GMT"
}
] | 2010-12-13T00:00:00 | [
[
"Hoffman",
"R. D.",
""
],
[
"Fisker",
"J. L.",
""
],
[
"Pruet",
"J.",
""
],
[
"Woosley",
"S. E.",
""
],
[
"Janka",
"H. -T.",
""
],
[
"Buras",
"R.",
""
]
] | [
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] |
801.1829 | Thomas Creutzig | Thomas Creutzig, Alexander Klauer, Nils R. Scheithauer | Natural constructions of some generalized Kac-Moody algebras as bosonic
strings | 22 pages; published in Comm. Number Theory Phys. 1 (2007), 453-477 | Commun.Num.Theor.Phys.1:453-477,2007 | null | null | math.NT math-ph math.MP | null | There are 10 generalized Kac-Moody algebras whose denominator identities are
completely reflective automorphic products of singular weight on lattices of
squarefree level. Under the assumption that the meromorphic vertex operator
algebra of central charge 24 and spin-1 algebra $\hat{A}_{p-1,p}^r$ exists we
show that four of them can be constructed in a uniform way from bosonic strings
moving on suitable target spaces.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:44:13 GMT"
}
] | 2009-03-24T00:00:00 | [
[
"Creutzig",
"Thomas",
""
],
[
"Klauer",
"Alexander",
""
],
[
"Scheithauer",
"Nils R.",
""
]
] | [
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] |
801.183 | Xicheng Zhang | Jiagang Ren, Xicheng Zhang | Freidlin-Wentzell's Large Deviations for Stochastic Evolution Equations | 17Pages | null | null | null | math.PR math.DS | null | We prove a Freidlin-Wentzell large deviation principle for general stochastic
evolution equations with small perturbation multiplicative noises. In
particular, our general result can be used to deal with a large class of quasi
linear stochastic partial differential equations, such as stochastic porous
medium equations and stochastic reaction diffusion equations with polynomial
growth zero order term and $p$-Laplacian second order term.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 19:50:12 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Ren",
"Jiagang",
""
],
[
"Zhang",
"Xicheng",
""
]
] | [
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] |
801.1831 | Howard Baer | Howard Baer, Sabine Kraml, Sezen Sekmen and Heaya Summy | Dark matter allowed scenarios for Yukawa-unified SO(10) SUSY GUTs | 35 pages with 21 eps figures | JHEP0803:056,2008 | 10.1088/1126-6708/2008/03/056 | FSU-HEP-071225, LPSC 07-195 | hep-ph | null | Simple supersymmetric grand unified models based on the gauge group SO(10)
require --in addition to gauge and matter unification-- the unification of
t-b-\tau Yukawa couplings. Yukawa unification, however, only occurs for very
special values of the soft SUSY breaking parameters. We perform a search using
a Markov Chain Monte Carlo (MCMC) technique to investigate model parameters and
sparticle mass spectra which occur in Yukawa-unified SUSY models, where we also
require the relic density of neutralino dark matter to saturate the
WMAP-measured abundance. We find the spectrum is characterizd by three mass
scales: first/second generation scalars in the multi-TeV range, third
generation scalars in the TeV range, and gauginos in the \sim 100 GeV range.
Most solutions give far too high a relic abundance of neutralino dark matter.
The dark matter discrepancy can be rectified by 1. allowing for neutralino
decay to axino plus photon, 2. imposing gaugino mass non-universality or 3.
imposing generational non-universality. In addition, the MCMC approach finds 4.
a compromise solution where scalar masses are not too heavy, and where
neutralino annihilation occurs via the light Higgs h resonance. By imposing
weak scale Higgs soft term boundary conditions, we are also able to generate 5.
low \mu, m_A solutions with neutralino annihilation via a light A resonance,
though these solutions seem to be excluded by CDF/D0 measurements of the B_s\to
\mu^+\mu^- branching fraction. Based on the dual requirements of Yukawa
coupling unification and dark matter relic density, we predict new physics
signals at the LHC from pair production of 350--450 GeV gluinos. The events are
characterized by very high b-jet multiplicity and a dilepton mass edge around
mz2-mz1 \sim 50-75 GeV.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 18:15:02 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Mar 2008 20:23:50 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Baer",
"Howard",
""
],
[
"Kraml",
"Sabine",
""
],
[
"Sekmen",
"Sezen",
""
],
[
"Summy",
"Heaya",
""
]
] | [
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] |
801.1832 | Greg Bell | Gregory C. Bell and Alexander Dranishnikov | Mapping class groups have finite asymptotic dimension | Withdrawn due to a critical error in Theorem 3 of [5] on which the
main result relied | null | null | null | math.GR math.GT | null | By recognizing them as fundamental groups of developable complexes of groups
we prove that mapping class groups of compact orientable surfaces have finite
asymptotic dimension.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:10:10 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 19:13:53 GMT"
}
] | 2008-01-22T00:00:00 | [
[
"Bell",
"Gregory C.",
""
],
[
"Dranishnikov",
"Alexander",
""
]
] | [
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801.1833 | Michelangelo Mangano | G. Buchalla, T.K. Komatsubara, F. Muheim, L. Silvestrini, M. Artuso,
D.M. Asner, P. Ball, E. Baracchini, G. Bell, M. Beneke, J. Berryhill, A.
Bevan, I.I. Bigi, M. Blanke, Ch. Bobeth, M. Bona, F. Borzumati, T. Browder,
T. Buanes, O. Buchmuller, A.J. Buras, S. Burdin, D.G. Cassel, R. Cavanaugh,
M. Ciuchini, P. Colangelo, G. Crosetti, A. Dedes, F. De Fazio, S.
Descotes-Genon, J. Dickens, Z. Dolezal, S. Durr, U. Egede, C. Eggel, G.
Eigen, S. Fajfer, Th. Feldmann, R. Ferrandes, P. Gambino, T. Gershon, V.
Gibson, M. Giorgi, V.V. Gligorov, B. Golob, A. Golutvin, Y. Grossman, D.
Guadagnoli, U. Haisch, M. Hazumi, S. Heinemeyer, G. Hiller, D. Hitlin, T.
Huber, T. Hurth, T. Iijima, A. Ishikawa, G. Isidori, S. Jager, A.
Khodjamirian, P. Koppenburg, T. Lagouri, U. Langenegger, C. Lazzeroni, A.
Lenz, V. Lubicz, W. Lucha, H. Mahlke, D. Melikhov, F. Mescia, M. Misiak, M.
Nakao, J. Napolitano, N. Nikitin, U. Nierste, K. Oide, Y. Okada, P. Paradisi,
F. Parodi, M. Patel, A.A. Petrov, T.N. Pham, M. Pierini, S. Playfer, G.
Polesello, A. Policicchio, A. Poschenrieder, P. Raimondi, S. Recksiegel, P.
Reznicek, A. Robert, S. Robertson, J.L. Rosner, G. Ruggiero, A. Sarti, O.
Schneider, F. Schwab, S. Simula, S. Sivoklokov, P. Slavich, C. Smith, M.
Smizanska, A. Soni, T. Speer, P. Spradlin, M. Spranger, A. Starodumov, B.
Stech, A. Stocchi, S. Stone, C. Tarantino, F. Teubert, S. T'Jampens, K. Toms,
K. Trabelsi, S. Trine, S. Uhlig, V. Vagnoni, J.J. van Hunen, G. Weiglein, A.
Weiler, G. Wilkinson, Y. Xie, M. Yamauchi, G. Zhu, J. Zupan, R. Zwicky | B, D and K decays | Report of Working Group 2 of the CERN Workshop ``Flavour in the era
of the LHC'', Geneva, Switzerland, November 2005 -- March 2007 | Eur.Phys.J.C57:309-492,2008 | 10.1140/epjc/s10052-008-0716-1 | null | hep-ph hep-ex | null | With the advent of the LHC, we will be able to probe New Physics (NP) up to
energy scales almost one order of magnitude larger than it has been possible
with present accelerator facilities. While direct detection of new particles
will be the main avenue to establish the presence of NP at the LHC, indirect
searches will provide precious complementary information, since most probably
it will not be possible to measure the full spectrum of new particles and their
couplings through direct production. In particular, precision measurements and
computations in the realm of flavour physics are expected to play a key role in
constraining the unknown parameters of the Lagrangian of any NP model emerging
from direct searches at the LHC. The aim of Working Group 2 was twofold: on one
hand, to provide a coherent, up-to-date picture of the status of flavour
physics before the start of the LHC; on the other hand, to initiate activities
on the path towards integrating information on NP from high-pT and flavour
data.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:14:51 GMT"
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801.1834 | Shaun Mosley | Shaun N. Mosley | Non-dispersive wavepacket solutions of the Schrodinger equation | 12 pages, parameters amended to yield correct dimension and new
section added on relativistic extension | null | 10.1088/1751-8113/41/26/265305 | null | quant-ph | null | The free Schrodinger equation has constant velocity wavepacket solutions
\psi_{\bf v} of the form \psi= f({\bf r} - {\bf v}t) e^{- i m c^2 t / 2}. These
solutions are eigenvectors of a momentum operator {\bf \tilde p} which is
symmetric in a positive definite scalar product space. We discuss whether these
\psi_{\bf v} can act as basis states rather than the usual plane wave
solutions.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:30:48 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 20:42:15 GMT"
},
{
"version": "v3",
"created": "Mon, 21 Jan 2008 19:49:58 GMT"
},
{
"version": "v4",
"created": "Wed, 23 Jan 2008 20:52:08 GMT"
},
{
"version": "v5",
"created": "Fri, 1 Feb 2008 20:43:37 GMT"
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] | 2009-11-13T00:00:00 | [
[
"Mosley",
"Shaun N.",
""
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] |
801.1835 | Ricardo Paszko | Ricardo Paszko | Semiclassical and Effective Theories of Gravitation | 58 pages, 3 figures, Ph.D. Thesis (Advisor: Antonio Accioly), in
portuguese, uses axodraw | null | null | IFT-T.003/06 | gr-qc | null | First and second order corrections for the scattering of different types of
particles by a weak gravitational field, treated as an external field, are
calculated. These computations indicate a violation of the Equivalence
Principle: to first order, the cross-sections are spin dependent; if the
calculations are pushed to the next order, they become dependent upon energy as
well. Interesting enough, the aforementioned results are equivalent to those
obtained by means of the so-called Effective Theory of Gravitation, in the
limit in which one of the masses is much greater than all the other energies
involved. We discuss also some applications of our research, such as the
determination of an upper bound for the photon mass, and the possible
detection, in the foreseeable future, of these violations of the Equivalence
Principle.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:47:28 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Jan 2008 19:21:10 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Paszko",
"Ricardo",
""
]
] | [
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] |
801.1836 | Elisabeth Nicol | E.J. Nicol and J.P. Carbotte | Optical conductivity of bilayer graphene with and without an asymmetry
gap | final accepted version for PRB, added discussion and typos fixed | Phys. Rev. B vol. 77, 155409 (2008) | 10.1103/PhysRevB.77.155409 | null | cond-mat.mes-hall cond-mat.str-el | null | When a bilayer of graphene is placed in a suitably configured field effect
device, an asymmetry gap can be generated and the carrier concentration made
different in each layer. This provides a tunable semiconducting gap, and the
valence and the conductance band no longer meet at the two Dirac points of the
graphene Brillouin zone. We calculate the optical conductivity of such a
semiconductor with particular emphasis on the optical spectral weight
redistribution brought about by changes in gap and chemical potential due to
charging. We derive an algebraic formula for arbitrary value of the chemical
potential for the case of the bilayer conductivity without a gap.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:52:48 GMT"
},
{
"version": "v2",
"created": "Mon, 17 Mar 2008 18:58:29 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nicol",
"E. J.",
""
],
[
"Carbotte",
"J. P.",
""
]
] | [
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] |
801.1837 | Andrey Chubukov | Andrey V. Chubukov, Dmitrii L. Maslov, and Fabian H.L. Essler | A test of the g-ology model for one-dimensional interacting Fermi
systems | 4 pp, 1 fig, submitted to PRB RC | null | 10.1103/PhysRevB.77.161102 | null | cond-mat.str-el | null | Bosonization predicts that the specific heat, C(T), of a one-dimensional
interacting Fermi system is a sum of the specific heats of free collective
charge and spin excitations, plus the term with the running backscattering
amplitude which flows to zero logarithmically with decreasing T. We verify
whether this result is reproduced in the g-ology model. Of specific interest
are the anomalous terms in C(T) that depend on the bare backscattering
amplitude. We show that these terms can be incorporated into a renormalized
spin velocity. We do this by proving the equivalence of the results for C(T)
obtained within the g-ology model and by bosonization with velocities obtained
by the numerical solution of the Bethe-ansatz equations for the Hubbard model.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:53:44 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chubukov",
"Andrey V.",
""
],
[
"Maslov",
"Dmitrii L.",
""
],
[
"Essler",
"Fabian H. L.",
""
]
] | [
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] |
801.1838 | Inanc Sahin | I. Sahin | Rare decay Z \to \nu\bar{\nu}\gamma\gamma via tensor unparticle
mediation | 10 pages, 2 figures | Chinese Jour. of Phys. 47, 20-26 (2009) | null | null | hep-ph | null | The decay width of the rare decay Z \to \nu\bar{\nu}\gamma\gamma is strictly
constrained from the LEP data. Tensor unparticles provide a tree-level
contribution to this rare decay. We have calculated the tensor unparticle
contribution to the rare decay Z\to \nu\bar{\nu}\gamma\gamma. The current
experimental limit have been used to constrain unparticle couplings
\nu\bar{\nu}Z {U}^{\mu\nu} and \gamma\gamma {U}^{\mu\nu}.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:55:52 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 21:40:14 GMT"
}
] | 2012-12-19T00:00:00 | [
[
"Sahin",
"I.",
""
]
] | [
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] |
801.1839 | Shabnam Safaei | Shabnam Safaei, Simone Montangero, Fabio Taddei and Rosario Fazio | Optimized Cooper pair pumps | 9 pages, 10 figures | Phys. Rev. B 77, 144522 (2008) | 10.1103/PhysRevB.77.144522 | null | cond-mat.mes-hall cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In adiabatic Cooper pair pumps, operated by means of gate voltage modulation
only, the quantization of the pumped charge during a cycle is limited due to
the quantum coherence of the macroscopic superconducting wave function. In this
work we show that it is possible to obtain very accurate pumps in the
non-adiabatic regime by a suitable choice of the shape of the gate voltage
pulses. We determine the shape of these pulses by applying quantum optimal
control theory to this problem. In the optimal case the error, with respect to
the quantized value, can be as small as of the order of (10E-6)e: the error is
reduced by up to five orders of magnitude with respect to the adiabatic
pumping. In order to test the experimental feasibility of this approach we
consider the effect of charge noise and the deformations of the optimal pulse
shapes on the accuracy of the pump. Charge noise is assumed to be induced by
random background charges in the substrate, responsible for the observed 1/f
noise. Inaccuracies in the pulse shaping are described by assuming a finite
bandwidth for the pulse generator. In realistic cases the error increases at
most of one order of magnitude as compared to the optimal case. Our results are
promising for the realization of accurate and fast superconducting pumps.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:59:12 GMT"
},
{
"version": "v2",
"created": "Mon, 24 Nov 2008 14:35:33 GMT"
}
] | 2010-09-08T00:00:00 | [
[
"Safaei",
"Shabnam",
""
],
[
"Montangero",
"Simone",
""
],
[
"Taddei",
"Fabio",
""
],
[
"Fazio",
"Rosario",
""
]
] | [
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] |
801.184 | Louis-Francois Arsenault | Louis-Francois Arsenault, B. Movaghar, P. Desjardins and A. Yelon | Transport in the metallic regime of Mn doped III-V Semiconductors | submitted to Phys. Rev. B | Phys. Rev. B 77, 115211 (2008) | 10.1103/PhysRevB.77.115211 | null | cond-mat.mtrl-sci | null | The standard model of Mn doping in GaAs is subjected to a coherent potential
approximation (CPA) treatment. Transport coefficients are evaluated within the
linear response Kubo formalism. Both normal (NHE) and anomalous contributions
(AHE) to the Hall effect are examined. We use a simple model density of states
to describe the undoped valence band. The CPA bandstructure evolves into a spin
split band caused by the $p-d$ exchange scattering with Mn dopants. This gives
rise to a strong magnetoresistance, which decreases sharply with temperature.
The temperature ($T$) dependence of the resistance is due to spin disorder
scattering (increasing with $T$), CPA bandstructure renormalization and charged
impurity scattering (decreasing with $T$). The calculated transport
coefficients are discussed in relation to experiment, with a view of assessing
the overall trends and deciding whether the model describes the right physics.
This does indeed appear to be case, bearing in mind that the hopping limit
needs to be treated separately, as it cannot be described within the band CPA.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 20:59:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Arsenault",
"Louis-Francois",
""
],
[
"Movaghar",
"B.",
""
],
[
"Desjardins",
"P.",
""
],
[
"Yelon",
"A.",
""
]
] | [
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] |
801.1841 | Guillermo Torres | G. Torres (CfA), J. N. Winn (MIT), M. J. Holman (CfA) | Improved parameters for extrasolar transiting planets | To appear in The Astrophysical Journal. 23 pages in emulateapj
format, including figures and tables. Figures 7, 8, and 9 are low resolution;
higher resolution versions will be available from the journal when published.
Acknowledgement added, and minor changes made to TrES-3 and TrES-4 in the
Appendix | null | 10.1086/529429 | null | astro-ph | null | We present refined values for the physical parameters of transiting
exoplanets, based on a self-consistent and uniform analysis of transit light
curves and the observable properties of the host stars. Previously it has been
difficult to interpret the ensemble properties of transiting exoplanets,
because of the widely different methodologies that have been applied in
individual cases. Furthermore, previous studies often ignored an important
constraint on the mean stellar density that can be derived directly from the
light curve. The main contributions of this work are 1) a critical compilation
and error assessment of all reported values for the effective temperature and
metallicity of the host stars; 2) the application of a consistent methodology
and treatment of errors in modeling the transit light curves; and 3) more
accurate estimates of the stellar mass and radius based on stellar evolution
models, incorporating the photometric constraint on the stellar density. We use
our results to revisit some previously proposed patterns and correlations
within the ensemble. We confirm the mass-period correlation, and we find
evidence for a new pattern within the scatter about this correlation: planets
around metal-poor stars are more massive than those around metal-rich stars at
a given orbital period. Likewise, we confirm the proposed dichotomy of planets
according to their Safronov number, and we find evidence that the systems with
small Safronov numbers are more metal-rich on average. Finally, we confirm the
trend that led to the suggestion that higher-metallicity stars harbor planets
with a greater heavy-element content.
| [
{
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"created": "Fri, 11 Jan 2008 20:59:55 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 21:06:38 GMT"
},
{
"version": "v3",
"created": "Wed, 16 Jan 2008 18:20:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Torres",
"G.",
"",
"CfA"
],
[
"Winn",
"J. N.",
"",
"MIT"
],
[
"Holman",
"M. J.",
"",
"CfA"
]
] | [
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] |
801.1842 | Duncan Farrah | D. Farrah (Cornell), C. Lonsdale (Virginia), D. Weedman (Cornell), H.
Spoon (Cornell), M. Rowan-Robinson (Imperial College), M. Polletta (Institut
d'Astrophysique de Paris), S. Oliver (Sussex), J. R. Houck (Cornell), H. E.
Smith (UCSD) | The nature of star formation in distant ultraluminous infrared galaxies
selected in a remarkably narrow redshift range | ApJ accepted. Higher quality figures available on request | null | 10.1086/529485 | null | astro-ph | null | We present mid-infrared spectra of thirty two high redshift ultraluminous
infrared galaxies, selected via the stellar photospheric feature at rest-frame
1.6um, and an observed-frame 24um flux of >500muJy. Nearly all the sample
reside in a redshift range of <z>=1.71+/-0.15, and have rest-frame 1-1000um
luminosities of 10^12.9 - 10^13.8 Lsun. Most of the spectra exhibit prominent
polycyclic aromatic hydrocarbon emission features, and weak silicate
absorption, consistent with a starburst origin for the IR emission. Our
selection method appears to be a straightforward and efficient way of finding
distant, IR-luminous, star-forming galaxies in narrow redshift ranges. There is
however evidence that the mid-IR spectra of our sample differ systematically
from those of local ULIRGs; our sample have comparable PAH equivalent widths
but weaker apparent silicate absorption, and (possibly) enhanced PAH
6.2um/7.7um and 6.2um/11.2um flux ratios. Furthermore, the composite mid-IR
spectrum of our sample is almost identical to that of local starbursts with IR
luminosities of 10^10-10^11 Lsun rather than that of local ULIRGs. These
differences are consistent with a reduced dust column, which can plausibly be
obtained via some combination of (1) star formation that is extended over
spatial scales of 1-4Kpc, and (2) star formation in unusually gas-rich regions.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:00:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Farrah",
"D.",
"",
"Cornell"
],
[
"Lonsdale",
"C.",
"",
"Virginia"
],
[
"Weedman",
"D.",
"",
"Cornell"
],
[
"Spoon",
"H.",
"",
"Cornell"
],
[
"Rowan-Robinson",
"M.",
"",
"Imperial College"
],
[
"Polletta",
"M.",
"",
"Institut\n d'Astrophysique de Paris"
],
[
"Oliver",
"S.",
"",
"Sussex"
],
[
"Houck",
"J. R.",
"",
"Cornell"
],
[
"Smith",
"H. E.",
"",
"UCSD"
]
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] |
801.1843 | Xi Kang | X. Kang, Frank C. van den Bosch | New Constraints on the Efficiencies of Ram-Pressure Stripping and the
Tidal Disruption of Satellite Galaxies | A few discussions added, updated to match the accepted version to ApJ
Letters | Astrophys.J.676:L101-L104,2008 | 10.1086/587620 | null | astro-ph | null | Using data from the Sloan Digital Sky Survey (SDSS) it has recently been
shown that the red fraction of satellite galaxies increases with stellar mass.
Semi-analytical models, however, predict red satellite fractions that are
independent of stellar mass, and much higher than observed. It has been argued
that this discrepancy owes to the fact that the models assume that satellite
galaxies are instantaneously stripped of their hot gas reservoirs at the moment
they are accreted into a bigger halo. In this letter we show that the fraction
of red satellites can be brought in better agreement with the data by simply
decreasing this stripping efficiency. However, this also results in a red
fraction of massive centrals that is much too low. This owes to the fact that
the massive centrals now accrete satellite galaxies that are bluer and more
gas-rich. However, if a significant fraction of low mass satellite galaxies is
tidally disrupted before being accreted by their central host galaxy, as
suggested by recent studies, the red fractions of both centrals and satellites
can be reproduced reasonably well. A problem remains with the red fraction of
centrals of intermediate mass, which is likely to reflect an oversimplified
treatment of AGN feedback.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:10:16 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 18:44:13 GMT"
}
] | 2010-05-25T00:00:00 | [
[
"Kang",
"X.",
""
],
[
"Bosch",
"Frank C. van den",
""
]
] | [
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801.1844 | Paul Bourdon | Paul S. Bourdon and Joel H. Shapiro | Adjoints of rationally induced composition operators | 21 pages, Published Version | J. Functional Analysis 255 (2008), 1995-2012 | null | null | math.FA math.CV | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give an elementary proof of a formula recently obtained by Hammond,
Moorhouse, and Robbins for the adjoint of a rationally induced composition
operator on the Hardy space H^2. We discuss some variants and implications of
this formula, and use it to provide a sufficient condition for a rationally
induced composition operator adjoint to be a compact perturbation of a weighted
composition operator.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:01:01 GMT"
},
{
"version": "v2",
"created": "Fri, 20 Mar 2009 19:47:42 GMT"
}
] | 2009-03-20T00:00:00 | [
[
"Bourdon",
"Paul S.",
""
],
[
"Shapiro",
"Joel H.",
""
]
] | [
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801.1845 | Martin Snoager Sloth | Antonio Riotto and Martin S. Sloth | On Resumming Inflationary Perturbations beyond One-loop | 17 pages, v2: minor corrections, to appear in jcap | JCAP0804:030,2008 | 10.1088/1475-7516/2008/04/030 | CERN-PH-TH/2008-006 | hep-ph astro-ph hep-th | null | It is well known that the correlation functions of a scalar field in a
quasi-de Sitter space exhibit at the loop level cumulative infra-red effects
proportional to the total number of e-foldings of inflation. Using the in-in
formalism, we explore the behavior of these infra-red effects in the large N
limit of an O(N) invariant scalar field theory with quartic self-interactions.
By resumming all higher-order loop diagrams non-perturbatively, we show that
the connected four-point correlation function, which is a signal of
non-Gaussianity, is non-perturbatively enhanced with respect to its tree-level
value.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:19:58 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 11:13:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Riotto",
"Antonio",
""
],
[
"Sloth",
"Martin S.",
""
]
] | [
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] |
801.1846 | Alain Barrat | Aurelien Gautreau (LPT), Alain Barrat (LPT), Marc Barthelemy (CEA
DIF/DPTA) | Global disease spread: statistics and estimation of arrival times | J. Theor. Biol., in press | Journal of Theoretical Biology 251 (2008) 509-522 | 10.1016/j.jtbi.2007.12.001 | null | q-bio.PE cond-mat.stat-mech | null | We study metapopulation models for the spread of epidemics in which different
subpopulations (cities) are connected by fluxes of individuals (travelers).
This framework allows to describe the spread of a disease on a large scale and
we focus here on the computation of the arrival time of a disease as a function
of the properties of the seed of the epidemics and of the characteristics of
the network connecting the various subpopulations. Using analytical and
numerical arguments, we introduce an easily computable quantity which
approximates this average arrival time. We show on the example of a disease
spread on the world-wide airport network that this quantity predicts with a
good accuracy the order of arrival of the disease in the various subpopulations
in each realization of epidemic scenario, and not only for an average over
realizations. Finally, this quantity might be useful in the identification of
the dominant paths of the disease spread.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:05:18 GMT"
}
] | 2008-03-20T00:00:00 | [
[
"Gautreau",
"Aurelien",
"",
"LPT"
],
[
"Barrat",
"Alain",
"",
"LPT"
],
[
"Barthelemy",
"Marc",
"",
"CEA\n DIF/DPTA"
]
] | [
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] |
801.1847 | Stephen D. H. Hsu | Paul Frampton, Stephen D.H. Hsu, Thomas W. Kephart, David Reeb | What is the entropy of the universe? | 5 pages, 3 figures, 1 table, revtex; v3: revised and expanded
version, to appear in Class. Quant. Grav | Class.Quant.Grav.26:145005,2009 | 10.1088/0264-9381/26/14/145005 | null | hep-th astro-ph gr-qc hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Standard calculations suggest that the entropy of our universe is dominated
by black holes, whose entropy is of order their area in Planck units, although
they comprise only a tiny fraction of its total energy. Statistical entropy is
the logarithm of the number of microstates consistent with the observed
macroscopic properties of a system, hence a measure of uncertainty about its
precise state. Therefore, assuming unitarity in black hole evaporation, the
standard results suggest that the largest uncertainty in the future quantum
state of the universe is due to the Hawking radiation from evaporating black
holes. However, the entropy of the matter precursors to astrophysical black
holes is enormously less than that given by area entropy. If unitarity relates
the future radiation states to the black hole precursor states, then the
standard results are highly misleading, at least for an observer that can
differentiate the individual states of the Hawking radiation.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:43:43 GMT"
},
{
"version": "v2",
"created": "Thu, 15 May 2008 20:24:47 GMT"
},
{
"version": "v3",
"created": "Fri, 29 May 2009 20:02:41 GMT"
}
] | 2009-09-17T00:00:00 | [
[
"Frampton",
"Paul",
""
],
[
"Hsu",
"Stephen D. H.",
""
],
[
"Kephart",
"Thomas W.",
""
],
[
"Reeb",
"David",
""
]
] | [
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] |
801.1848 | Gerald Seidler | T. T. Fister, G. T. Seidler, E. L. Shirley, F. D. Vila, J. J. Rehr, K.
P. Nagle, J. C. Linehan, J. O. Cross | The local electronic structure of alpha-Li3N | 34 pages, 7 figures, 1 table | null | 10.1063/1.2949550 | null | cond-mat.mtrl-sci | null | New theoretical and experimental investigation of the occupied and unoccupied
local electronic density of states (DOS) are reported for alpha-Li3N. Band
structure and density functional theory calculations confirm the absence of
covalent bonding character. However, real-space full-multiple-scattering
(RSFMS) calculations of the occupied local DOS finds less extreme nominal
valences than have previously been proposed. Nonresonant inelastic x-ray
scattering (NRIXS), RSFMS calculations, and calculations based on the
Bethe-Salpeter equation are used to characterize the unoccupied electronic
final states local to both the Li and N sites. There is good agreement between
experiment and theory. Throughout the Li 1s near-edge region, both experiment
and theory find strong similarities in the s- and p-type components of the
unoccupied local final density of states projected onto an orbital angular
momentum basis (l-DOS). An unexpected, significant correspondence exists
between the near-edge spectra for the Li 1s and N 1s initial states. We argue
that both spectra are sampling essentially the same final density of states due
to the combination of long core-hole lifetimes, long photoelectron lifetimes,
and the fact that orbital angular momentum is the same for all relevant initial
states. Such considerations may be generically applicable for low atomic number
compounds.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:07:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fister",
"T. T.",
""
],
[
"Seidler",
"G. T.",
""
],
[
"Shirley",
"E. L.",
""
],
[
"Vila",
"F. D.",
""
],
[
"Rehr",
"J. J.",
""
],
[
"Nagle",
"K. P.",
""
],
[
"Linehan",
"J. C.",
""
],
[
"Cross",
"J. O.",
""
]
] | [
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801.1849 | Lisa J. Kewley | Lisa J. Kewley (1), Sara L. Ellison (2) ((1) University of Hawaii, (2)
University of Victoria) | Metallicity Calibrations and the Mass-Metallicity Relation for
Star-Forming Galaxies | 26 pages, 5 tables, 11 figures (reduced resolution); accepted for
publication in the Astrophysical Journal. . A full resolution version can be
downloaded in pdf form (1 Mb) from
http://www.ifa.hawaii.edu/~kewley/Metallicity/ms.pdf | Astrophys.J.681:1183-1204,2008 | 10.1086/587500 | null | astro-ph | null | (Abridged) We investigate the effect of metallicity calibrations, AGN
classification, and aperture covering fraction on the local mass-metallicity
(MZ) relation using 27,730 star-forming galaxies from the Sloan Digital Sky
Survey (SDSS) Data Release 4. We analyse the SDSS MZ relation with 10
metallicity calibrations, including theoretical and empirical methods. We show
that the choice of metallicity calibration has a significant effect on the
shape and y-intercept(12+log(O/H)) of the MZ relation. The absolute metallicity
scale (y-int) varies up to 0.7 dex, depending on the calibration used, and the
change in shape is substantial. These results indicate that it is critical to
use the same metallicity calibration when comparing different
luminosity-metallicity or mass-metallicity relations. We present new
metallicity conversions that allow metallicities that have been derived using
different strong-line calibrations to be converted to the same base
calibration. These conversions facilitate comparisons between different
samples, particularly comparisons between galaxies at different redshifts for
which different suites of emission-lines are available.Our new conversions
successfully remove the large 0.7 dex discrepancies between the metallicity
calibrations, and we reach agreement in the MZ relation to within 0.03 dex on
average. We find that different AGN classification methods have negligible
effect on the SDSS MZ relation. We compare the SDSS MZ relation with nuclear
and global relations from the Nearby Field Galaxy Survey (NFGS). The turn over
of the MZ relation depends on aperture covering fraction. We find that a lower
redshift limit of z<0.04 is insufficient for avoiding aperture effects in fiber
spectra of the highest stellar mass galaxies.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:07:04 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Kewley",
"Lisa J.",
""
],
[
"Ellison",
"Sara L.",
""
]
] | [
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] |
801.185 | Voisin Christophe | Christophe Voisin (LGIT), Jean-Robert Grasso (LGIT), Eric Larose
(LGIT), Fran\c{c}ois Renard (LGIT) | Evolution of seismic signals and slip patterns along subduction zones:
insights from a friction lab scale experiment | null | null | 10.1029/2008GL033356 | null | physics.geo-ph | null | Continuous GPS and broadband seismic monitoring have revealed a variety of
disparate slip patterns especially in shallow dipping subduction zones, among
which regular earthquakes, slow slip events and silent quakes1,2. Slow slip
events are sometimes accompanied by Non Volcanic Tremors (NVT), which origin
remains unclear3, either related to fluid migration or to friction. The present
understanding of the whole menagerie of slip patterns is based upon numerical
simulations imposing ad hoc values of the rate and state parameters a and b4-6
derived from the temperature dependence of a and b of a wet granite gouge7.
Here we investigate the influence of the cumulative slip on the frictional and
acoustic patterns of a lab scale subduction zone. Shallow loud earthquakes
(stick-slip events), medium depth slow, deeper silent quakes (smooth sliding
oscillations) and deepest steady-state creep (continuous sliding) are
reproduced by the ageing of contact interface with cumulative displacement8.
The Acoustic Emission evolves with cumulative displacement and interface
ageing, following a trend from strong impulsive events, similar to earthquake
seismic signals, to a collection of smaller amplitude and longer duration
signals, similar to Non Volcanic Tremors. NVT emerge as the recollection of the
local unstable behaviour of the contact interface globally evolving towards the
stable sliding regime.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:08:14 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Voisin",
"Christophe",
"",
"LGIT"
],
[
"Grasso",
"Jean-Robert",
"",
"LGIT"
],
[
"Larose",
"Eric",
"",
"LGIT"
],
[
"Renard",
"François",
"",
"LGIT"
]
] | [
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801.1851 | Steffen Knollmann | Steffen R. Knollmann, Chris Power and Alexander Knebe | Dark Matter Halo Profiles in Scale-Free Cosmologies | 9 pages, 4 figures. Accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12857.x | null | astro-ph | null | We explore the dependence of the central logarithmic slope of dark matter
halo density profiles $\alpha$ on the spectral index $n$ of the linear matter
power spectrum $P(k)$ using cosmological $N$-body simulations of scale-free
models (i.e. $P(k) \propto k^n$). For each of our simulations we identify
samples of well resolved haloes in dynamical equilibrium and we analyse their
mass profiles. By parameterising the mass profile using a ``generalised''
Navarro, Frenk & White profile in which the central logarithmic slope $\alpha$
is allowed to vary while preserving the $r^{-3}$ asymptotic form at large
radii, we obtain preferred central slopes for haloes in each of our models.
There is a strong correlation between $\alpha$ and $n$, such that $\alpha$
becomes shallower as $n$ becomes steeper. However, if we normalise our mass
profiles by $r_{-2}$, the radius at which the logarithmic slope of the density
profile is -2, we find that these differences are no longer present. We
conclude that there is no evidence for convergence to a unique central
asymptotic slope, at least on the scales that we can resolve.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:09:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Knollmann",
"Steffen R.",
""
],
[
"Power",
"Chris",
""
],
[
"Knebe",
"Alexander",
""
]
] | [
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] |
801.1852 | Darren Williams | D.M. Williams, E. Gaidos | Detecting the Glint of Starlight on the Oceans of Distant Planets | 41 pages, 7 figures. Icarus in press | null | 10.1016/j.icarus.2008.01.002 | null | astro-ph | null | We propose that astronomers will be eventually be able to discriminate
between extrasolar Earth-like planets with surface oceans and those without
using the shape of phase light curves in the visible and near-IR spectrum. We
model the visible light curves of planets having Earth-like surfaces, seasons,
and optically-thin atmospheres with idealized diffuse-scattering clouds. We
show that planets partially covered by water will appear measurably brighter
near crescent phase (relative to Lambertian planets) because of the efficient
specular reflection (i.e., glint) of starlight incident on their surfaces at a
highly oblique angle. Planets on orbits within 30 degrees of edge-on
orientation (half of all planets) will show pronounced glint over a sizeable
range of orbital longitudes, from quadrature to crescent, all outside the glare
of their parent stars. Also, water-covered planets will appear darker than a
Lambertian disk near full illumination. Finally, we show that planets with a
mixed land/water surface will polarize the reflected signal by as much as 30-70
percent. These results suggest several new ways of directly identifying water
on distant planets.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:10:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Williams",
"D. M.",
""
],
[
"Gaidos",
"E.",
""
]
] | [
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] |
801.1853 | Gerald Seidler | T.T. Fister, K.P. Nagle, F.D. Vila, G.T. Seidler, C. Hamner, J.O.
Cross, J.J. Rehr | Intermediate-Range Order in Water Ices | 20 page, 4 figure. Submitted PRB | null | null | null | cond-mat.mtrl-sci | null | We report measurements of the non-resonant inelastic x-ray scattering (NRIXS)
from the O 1s orbitals in ice Ih, and also report calculations of the
corresponding spectra for ice Ih and several other phases of water ice. We find
that the intermediate-energy fine structure may be calculated well using an ab
initio real-space full multiple scattering approach, and that it provides a
strong fingerprint of the intermediate-range order for some ice phases. These
results have important consequences for future NRIXS measurements of
high-pressure phases of ice and also may call into question the assumption that
the wavefunctions for final states within a few eV of the absorption edge are
strongly localized.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:12:26 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Fister",
"T. T.",
""
],
[
"Nagle",
"K. P.",
""
],
[
"Vila",
"F. D.",
""
],
[
"Seidler",
"G. T.",
""
],
[
"Hamner",
"C.",
""
],
[
"Cross",
"J. O.",
""
],
[
"Rehr",
"J. J.",
""
]
] | [
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] |
801.1854 | Andrew Tolley | Andrew J. Tolley, Mark Wyman | Stochastic Inflation Revisited: Non-Slow Roll Statistics and DBI
Inflation | 38 pages, 2 figures. v3: minor revisions; version accepted into JCAP | JCAP0804:028,2008 | 10.1088/1475-7516/2008/04/028 | PI-COSMO-58 | hep-th astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Stochastic inflation describes the global structure of the inflationary
universe by modeling the super-Hubble dynamics as a system of matter fields
coupled to gravity where the sub-Hubble field fluctuations induce a stochastic
force into the equations of motion. The super-Hubble dynamics are ultralocal,
allowing us to neglect spatial derivatives and treat each Hubble patch as a
separate universe. This provides a natural framework in which to discuss
probabilities on the space of solutions and initial conditions. In this article
we derive an evolution equation for this probability for an arbitrary class of
matter systems, including DBI and k-inflationary models, and discover
equilibrium solutions that satisfy detailed balance. Our results are more
general than those derived assuming slow roll or a quasi-de Sitter geometry,
and so are directly applicable to models that do not satisfy the usual slow
roll conditions. We discuss in general terms the conditions for eternal
inflation to set in, and we give explicit numerical solutions of highly
stochastic, quasi-stationary trajectories in the relativistic DBI regime.
Finally, we show that the probability for stochastic/thermal tunneling can be
significantly enhanced relative to the Hawking-Moss instanton result due to
relativistic DBI effects.
| [
{
"version": "v1",
"created": "Mon, 14 Jan 2008 20:16:52 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jan 2008 00:18:11 GMT"
},
{
"version": "v3",
"created": "Thu, 19 Jun 2008 14:52:43 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Tolley",
"Andrew J.",
""
],
[
"Wyman",
"Mark",
""
]
] | [
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] |
801.1855 | Alexander Volberg L | V. Eiderman, F. Nazarov, A. Volberg | Vector-valued Riesz potentials: Cartan type estimates and related
capacities | 33 pages | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | There are many interesting problems about the electrostatic potential of
finitely many charges. We consider one of them concerning the intensity of the
field, in other words, about the magnitude of the gradient of this potential.
We want to give a sharp estimate of the size of the set of points where this
gradient is large. Of course we want the estimate to be sharp in number $N$ of
charges. The size will be measured by the Hausdorff content with various gauge
functions. Such a setting allows us to consider a wide class of measures (not
necessarily with finitely many charges). The main technique will be
Calder\'on-Zygmund capacities and nonhomogeneous Calder\'on-Zygmund operators.
Here we establish a relationship between various types of capacities with
singular kernels (e. g. analytic capacity, lipschitz harmonic capacity, etc)
and non-linear capacity from the theory of potential \'a la Adams, Hedberg,
Havin, Maz'ya, Wolff. "Capacitary" part of the paper extends the theorem of
Mateu, Prat and Verdera [J. reine und angew. Math., 578 (2005), 201--223].
"Size estimates" part of the paper extends the theorem of M. Anderson and V.
Eiderman [Annals of Math., 163 (2005), 1057--1076]. The difficulty lies in the
fact that we cannot use Menger's curvature anymore because we are working in
spaces of dimension bigger than two.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:20:49 GMT"
},
{
"version": "v2",
"created": "Sat, 1 Nov 2008 17:29:37 GMT"
}
] | 2008-11-01T00:00:00 | [
[
"Eiderman",
"V.",
""
],
[
"Nazarov",
"F.",
""
],
[
"Volberg",
"A.",
""
]
] | [
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] |
801.1856 | Grenville Croll | David A. Banks, Ann Monday | Interpretation as a factor in understanding flawed spreadsheets | 9 pages incuding references | Proc. European Spreadsheet Risks Int. Grp. 2002 13 21 ISBN 1 86166
182 7 | null | null | cs.CY cs.HC | null | The spreadsheet has been used by the business community for many years and
yet still raises a number of significant concerns. As educators our concern is
to try to develop the students skills in both the development of spreadsheets
and in taking a critical view of their potential defects. In this paper we
consider both the problems of mechanical production and the problems of
translation of problem to spreadsheet representation.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:47:01 GMT"
}
] | 2008-03-10T00:00:00 | [
[
"Banks",
"David A.",
""
],
[
"Monday",
"Ann",
""
]
] | [
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] |
801.1857 | Shailesh Chandrasekharan | D. J. Cecile and Shailesh Chandrasekharan | Absence of vortex condensation in a two dimensional fermionic XY model | 5 pages, 5 figures | Phys.Rev.D77:054502,2008 | 10.1103/PhysRevD.77.054502 | null | hep-lat | null | Motivated by a puzzle in the study of two dimensional lattice Quantum
Electrodynamics with staggered fermions, we construct a two dimensional
fermionic model with a global U(1) symmetry. Our model can be mapped into a
model of closed packed dimers and plaquettes. Although the model has the same
symmetries as the XY model, we show numerically that the model lacks the well
known Kosterlitz-Thouless phase transition. The model is always in the gapless
phase showing the absence of a phase with vortex condensation. In other words
the low energy physics is described by a non-compact U(1) field theory. We show
that by introducing an even number of layers one can introduce vortex
condensation within the model and thus also induce a KT transition.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:50:21 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cecile",
"D. J.",
""
],
[
"Chandrasekharan",
"Shailesh",
""
]
] | [
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] |
801.1858 | Pavel Bleher | Pavel M. Bleher | Lectures on random matrix models. The Riemann-Hilbert approach | 84 pages, 23 figures, to appear in the CRM volume on "Random
Matrices", Springer, 2008 | null | null | null | math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This is a review of the Riemann-Hilbert approach to the large $N$ asymptotics
in random matrix models and its applications. We discuss the following topics:
random matrix models and orthogonal polynomials, the Riemann-Hilbert approach
to the large $N$ asymptotics of orthogonal polynomials and its applications to
the problem of universality in random matrix models, the double scaling limits,
the large $N$ asymptotics of the partition function, and random matrix models
with external source.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 21:56:55 GMT"
},
{
"version": "v2",
"created": "Thu, 26 Jun 2008 15:52:29 GMT"
}
] | 2008-06-26T00:00:00 | [
[
"Bleher",
"Pavel M.",
""
]
] | [
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] |
801.1859 | Maciej Nowak A. | Jean-Paul Blaizot and Maciej A. Nowak | Large N_c confinement and turbulence | 4 pages, no figures- Some rewriting - Typos corrected - References
completed and some corrected | Phys.Rev.Lett.101:102001,2008 | 10.1103/PhysRevLett.101.102001 | null | hep-th hep-lat hep-ph | null | We suggest that the transition that occurs at large $N_c$ in the eigenvalue
distribution of a Wilson loop may have a turbulent origin. We arrived at this
conclusion by studying the complex-valued inviscid Burgers-Hopf equation that
corresponds to the Makeenko-Migdal loop equation, and we demonstrate the
appearance of a shock in the spectral flow of the Wilson loop eigenvalues. This
picture supplements that of the Durhuus-Olesen transition with a particular
realization of disorder. The critical behavior at the formation of the shock
allows us to infer exponents that have been measured recently in lattice
simulations by Narayanan and Neuberger in $d=2$ and $d=3$. Our analysis leads
us to speculate that the universal behavior observed in these lattice
simulations might be a generic feature of confinement, also in $d=4$ Yang-Mills
theory.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:00:39 GMT"
},
{
"version": "v2",
"created": "Sun, 24 Feb 2008 20:51:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Blaizot",
"Jean-Paul",
""
],
[
"Nowak",
"Maciej A.",
""
]
] | [
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] |
801.186 | Arjun Dey | Arjun Dey (1), B. T. Soifer (2), Vandana Desai (2), Kate Brand (3),
Emeric LeFloc'h (4), Michael J. Brown (5), Buell T. Jannuzi (1), Lee Armus
(2), Shane Bussmann (6), Mark Brodwin (1), Chao Bian (2), Peter Eisenhardt
(7), Sarah Higdon (8), Daniel Weedman (9), Steve Willner (10) ((1) NOAO, (2)
Caltech, (3) STScI, (4) U of Hawaii, (5) Monash, (6) U of Arizona, (7) JPL,
(8) Georgia Southern U, (9) Cornell, (10) Harvard/CfA) | A Significant Population of Very Luminous Dust-Obscured Galaxies at
Redshift z ~ 2 | Accepted for publication in the Astrophysical Journal | null | 10.1086/529516 | null | astro-ph | null | Observations with Spitzer Space Telescope have recently revealed a
significant population of high-redshift z~2 dust-obscured galaxies (DOGs) with
large mid-IR to UV luminosity ratios. These galaxies have been missed in
traditional optical studies of the distant universe. We present a simple method
for selecting this high-z population based solely on the ratio of the observed
mid-IR 24um to optical R-band flux density. In the 8.6 sq.deg Bootes NDWFS
Field, we uncover ~2,600 DOG candidates (= 0.089/sq.arcmin) with 24um flux
densities F24>0.3mJy and (R-[24])>14 (i.e., F[24]/F[R] > 1000). These galaxies
have no counterparts in the local universe, and become a larger fraction of the
population at fainter F24, representing 13% of the sources at 0.3~mJy. DOGs
exhibit evidence of both star-formation and AGN activity, with the brighter
24um sources being more AGN- dominated. We have measured spectroscopic
redshifts for 86 DOGs, and find a broad z distribution centered at <z>~2.0.
Their space density is 2.82E-5 per cubic Mpc, similar to that of bright
sub-mm-selected galaxies at z~2. These redshifts imply very large luminosities
LIR>~1E12-14 Lsun. DOGs contribute ~45-100% of the IR luminosity density
contributed by all z~2 ULIRGs, suggesting that our simple selection criterion
identifies the bulk of z~2 ULIRGs. DOGs may be the progenitors of ~4L*
present-day galaxies seen undergoing a luminous,short- lived phase of bulge and
black hole growth. They may represent a brief evolution phase between SMGs and
less obscured quasars or galaxies. [Abridged]
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:05:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dey",
"Arjun",
""
],
[
"Soifer",
"B. T.",
""
],
[
"Desai",
"Vandana",
""
],
[
"Brand",
"Kate",
""
],
[
"LeFloc'h",
"Emeric",
""
],
[
"Brown",
"Michael J.",
""
],
[
"Jannuzi",
"Buell T.",
""
],
[
"Armus",
"Lee",
""
],
[
"Bussmann",
"Shane",
""
],
[
"Brodwin",
"Mark",
""
],
[
"Bian",
"Chao",
""
],
[
"Eisenhardt",
"Peter",
""
],
[
"Higdon",
"Sarah",
""
],
[
"Weedman",
"Daniel",
""
],
[
"Willner",
"Steve",
""
]
] | [
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] |
801.1861 | Erik Henriksen | E.A. Henriksen, Z. Jiang, L.-C. Tung, M.E. Schwartz, M. Takita, Y.-J.
Wang, P. Kim, H.L. Stormer | Cyclotron resonance in bilayer graphene | to appear in Phys. Rev. Lett. Updated version with two added
references and minor text editing | Phys. Rev. Lett. 100, 087403 (2008) | 10.1103/PhysRevLett.100.087403 | null | cond-mat.mes-hall | null | We present the first measurements of cyclotron resonance of electrons and
holes in bilayer graphene. In magnetic fields up to B = 18 T we observe four
distinct intraband transitions in both the conduction and valence bands. The
transition energies are roughly linear in B between the lowest Landau levels,
whereas they follow \sqrt{B} for the higher transitions. This highly unusual
behavior represents a change from a parabolic to a linear energy dispersion.
The density of states derived from our data generally agrees with the existing
lowest order tight binding calculation for bilayer graphene. However in
comparing data to theory, a single set of fitting parameters fails to describe
the experimental results.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:18:37 GMT"
},
{
"version": "v2",
"created": "Sat, 23 Feb 2008 23:32:46 GMT"
}
] | 2008-05-21T00:00:00 | [
[
"Henriksen",
"E. A.",
""
],
[
"Jiang",
"Z.",
""
],
[
"Tung",
"L. -C.",
""
],
[
"Schwartz",
"M. E.",
""
],
[
"Takita",
"M.",
""
],
[
"Wang",
"Y. -J.",
""
],
[
"Kim",
"P.",
""
],
[
"Stormer",
"H. L.",
""
]
] | [
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0.0593264848,
-0.0008506463,
0.0188605841
] |
801.1862 | Matthew Horak | Matthew Horak, Melanie Stein, Jennifer Taback | Convexity properties of Thompson's group F | 11 pages, 3 figures | J. Group Theory 15 (2012): 37-45 | 10.1515/JGT.2010.093 | null | math.GR | null | We prove that Thompson's group F is not minimally almost convex with respect
to any generating set which is a subset of the standard infinite generating set
for F and which contains x_1. We use this to show that F is not almost convex
with respect to any generating set which is a subset of the standard infinite
generating set.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:24:19 GMT"
}
] | 2021-09-24T00:00:00 | [
[
"Horak",
"Matthew",
""
],
[
"Stein",
"Melanie",
""
],
[
"Taback",
"Jennifer",
""
]
] | [
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] |
801.1863 | Joshua Davis | Alejandra Castro, Joshua L. Davis, Per Kraus, Finn Larsen | String Theory Effects on Five-Dimensional Black Hole Physics | 85 pages; uses ws-ijmpa-mod.cls article class; Invited review for
IJMPA | null | 10.1142/S0217751X08039724 | null | hep-th | null | We review recent developments in understanding quantum/string corrections to
BPS black holes and strings in five-dimensional supergravity. These objects are
solutions to the effective action obtained from M-theory compactified on a
Calabi-Yau threefold, including the one-loop corrections determined by anomaly
cancellation and supersymmetry. We introduce the off-shell formulation of this
theory obtained through the conformal supergravity method and review the
methods for investigating supersymmetric solutions. This leads to
quantum/string corrected attractor geometries, as well as asymptotically flat
black strings and spinning black holes. With these solutions in hand, we
compare our results with analogous studies in four-dimensional string-corrected
supergravity, emphasizing the distinctions between the four and five
dimensional theories.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 23:00:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Castro",
"Alejandra",
""
],
[
"Davis",
"Joshua L.",
""
],
[
"Kraus",
"Per",
""
],
[
"Larsen",
"Finn",
""
]
] | [
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] |
801.1864 | Robert Kohn | P. Giordani and R. Kohn | Adaptive Independent Metropolis-Hastings by Fast Estimation of Mixtures
of Normals | 35 pages and 6 figures | null | null | null | stat.CO stat.AP stat.ME | null | We construct an adaptive independent Metropolis-Hastings sampler that uses a
mixture of normals as a proposal distribution. To take full advantage of the
potential of adaptive sampling our algorithm updates the mixture of normals
frequently, starting early in the chain. The algorithm is built for speed and
reliability and its sampling performance is evaluated with real and simulated
examples. Our article outlines conditions for adaptive sampling to hold and
gives a readily accessible proof that under these conditions the sampling
scheme generates iterates that converge to the target distribution.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 22:53:12 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Giordani",
"P.",
""
],
[
"Kohn",
"R.",
""
]
] | [
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] |
801.1865 | Delfim F. M. Torres | Moulay Rchid Sidi Ammi, Delfim F. M. Torres | Combined dynamic Gruss inequalities on time scales | 9 pages | Journal of Mathematical Sciences, Vol. 161, No. 6, 2009, 792--802 | 10.1007/s10958-009-9600-2 | null | math.CA | null | We prove a more general version of the Gruss inequality by using the recent
theory of combined dynamic derivatives on time scales and the more general
notions of diamond-alpha derivative and integral. For the particular case when
alpha = 1, one gets a delta-integral Gruss inequality on time scales; for alpha
= 0 a nabla-integral Gruss inequality. If we further restrict ourselves by
fixing the time scale to the real (or integer) numbers, then the standard
continuous (discrete) inequalities are obtained.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 23:39:13 GMT"
}
] | 2009-09-18T00:00:00 | [
[
"Ammi",
"Moulay Rchid Sidi",
""
],
[
"Torres",
"Delfim F. M.",
""
]
] | [
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] |
801.1866 | William Krekelberg | William P. Krekelberg, Jeetain Mittal, Venkat Ganesan, Thomas M.
Truskett | Structural anomalies of fluids: Origins in second and higher
coordination shells | Submitted to The Journal of Chemical Physics | Phys. Rev. E 77, 041201 (2008) | 10.1103/PhysRevE.77.041201 | null | cond-mat.soft | null | Compressing or cooling a fluid typically enhances its static interparticle
correlations. However, there are notable exceptions. Isothermal compression can
reduce the translational order of fluids that exhibit anomalous waterlike
trends in their thermodynamic and transport properties, while isochoric cooling
(or strengthening of attractive interactions) can have a similar effect on
fluids of particles with short-range attractions. Recent simulation studies by
Yan et al. [Phys. Rev. E 76, 051201 (2007)] on the former type of system and
Krekelberg et al. [J. Chem. Phys. 127, 044502 (2007)] on the latter provide
examples where such structural anomalies can be related to specific changes in
second and more distant coordination shells of the radial distribution
function. Here, we confirm the generality of this microscopic picture through
analysis, via molecular simulation and integral equation theory, of
coordination shell contributions to the two-body excess entropy for several
related model fluids which incorporate different levels of molecular
resolution. The results suggest that integral equation theory can be an
effective and computationally inexpensive first-pass tool for assessing, based
on the pair potential alone, whether new model systems are good candidates for
exhibiting structural (and hence thermodynamic and transport) anomalies.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 23:59:26 GMT"
}
] | 2008-04-11T00:00:00 | [
[
"Krekelberg",
"William P.",
""
],
[
"Mittal",
"Jeetain",
""
],
[
"Ganesan",
"Venkat",
""
],
[
"Truskett",
"Thomas M.",
""
]
] | [
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] |
801.1867 | Artour Mouftakhov V | A. M. Akhtymov, A. V. Mouftakhov, M. Teicher | Identification of Boundary Conditions Using Natural Frequencies in Case
of a Ring Membrane | null | null | null | null | math.SP | null | The problem of finding boundary conditions for fastening of a ring membrane,
which are inaccessible for direct observation from the natural frequencies of
its flexural oscillations, is considered. Two theorems on the uniqueness of
this problem are proved, and a method for establishing the unknown conditions
for fastening of the membrane to the walls is indicated. An approximate formula
for determining the unknown conditions is obtained, using first three natural
frequencies. The method of approximate calculation of unknown boundary
conditions, is explained with the help of an example. Keywords: Boundary
conditions, inverse spectral problem, membrane, natural frequencies, Plucker
coordinates, Plucker relation.
| [
{
"version": "v1",
"created": "Sat, 12 Jan 2008 00:03:37 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Akhtymov",
"A. M.",
""
],
[
"Mouftakhov",
"A. V.",
""
],
[
"Teicher",
"M.",
""
]
] | [
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] |
801.1868 | Luis Dorado | Luis A. Dorado and Ricardo A. Depine | Optical response of a self-standing monolayer of dielectric spheres | 22 pages, 7 figures | null | null | null | physics.optics physics.class-ph | null | An analysis of the optical response of periodically arrayed monolayers
composed of dielectric spheres with low refractive index is herein presented.
The reflectance spectra of two-dimensional square and triangular lattices are
obtained by means of the vector Korringa-Kohn-Rostoker method, both spectra
showing very similar qualitative features for photon energies below the onset
of diffraction spots. In this energy region, the same number of peaks of
unitary amplitude in the reflectance spectra are predicted for both kinds of
monolayers, suggesting that this must be a universal feature independent of the
particular geometry of the lattice. The origin of these high reflectance peaks
is investigated. It is found that the resonances of TM and TE modes due to
dipolar, quadrupolar and octupolar interaction inside the monolayer are largely
responsible for the peak structure observed in the reflectance spectra.
| [
{
"version": "v1",
"created": "Sat, 12 Jan 2008 00:03:49 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Dorado",
"Luis A.",
""
],
[
"Depine",
"Ricardo A.",
""
]
] | [
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] |
801.1869 | Yuki Kaneko | Y. Kaneko, M.M. Gonzalez, R. Preece, B.L. Dingus, M.S. Briggs | Broadband Spectral Properties of Bright High-Energy Gamma-Ray Bursts
Observed with BATSE and EGRET | 18 pages (emulateapj) including 7 figures & 2 tables. Accepted for
publication in ApJ | null | 10.1086/529486 | null | astro-ph | null | We present the spectral analysis of duration-integrated broadband spectra (in
$\sim30 $keV$-200 $MeV) of 15 bright BATSE gamma-ray bursts (GRBs). Some GRB
spectra are very hard, with their spectral peak energies being above the BATSE
LAD passband limit of $\sim$2 MeV. In such cases, their high-energy spectral
parameters (peak energy and high-energy power-law indices) cannot be adequately
constrained by BATSE LAD data alone. A few dozen bright BATSE GRBs were also
observed with EGRET's calorimeter, TASC, in multi-MeV energy band, with a large
effective area and fine energy resolution. Combining the BATSE and TASC data,
therefore, affords spectra that span four decades of energy ($30 $keV$-200
$MeV), allowing for a broadband spectral analysis with good statistics.
Studying such broadband high-energy spectra of GRB prompt emission is crucial,
as they provide key clues to understanding its gamma-ray emission mechanism.
Among the 15 GRB spectra, we found two cases with a significant high-energy
excess, and another case with a extremely high peak energy (\epeak $\gtrsim$
170 MeV). There have been very limited number of GRBs observed at MeV energies
and above, and only a few instruments have been capable of observing GRBs in
this energy band with such high sensitivity. Thus, our analysis results
presented here should also help predict GRB observations with current and
future high-energy instruments such as AGILE and GLAST, as well as with
ground-based very-high-energy telescopes.
| [
{
"version": "v1",
"created": "Sat, 12 Jan 2008 00:12:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kaneko",
"Y.",
""
],
[
"Gonzalez",
"M. M.",
""
],
[
"Preece",
"R.",
""
],
[
"Dingus",
"B. L.",
""
],
[
"Briggs",
"M. S.",
""
]
] | [
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] |
801.187 | Gerhard Kramm | Gerhard Kramm | Comment to "Recent Climate Observations Compared to Projections" by
Rahmstorf et al | 5 pages, 4 figures. Submitted for publication to Science | null | null | null | physics.ao-ph physics.ed-ph | null | It is shown in this comment that considering the Mauna Loa observation of the
atmospheric carbon dioxide concentration and the mean near surface temperature
anomalies for the period from the beginning of the seventies to recent years
only is, clearly, a source of misinterpretation. If we consider the whole
period of available data (1958 - 2004), we obtain results which differ from
those presented by Rahmstorf et al. It is also shown that in 1988 when the
Intergovernmental Panel of Climate Change (IPCC) of the United Nations and the
World Meteorological Organization (WMO) was established there was certainly no
correlation between the atmospheric carbon dioxide concentration and the mean
near surface temperature anomalies, neither on the annual time scale nor on the
monthly time scale.
| [
{
"version": "v1",
"created": "Sat, 12 Jan 2008 00:43:45 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Kramm",
"Gerhard",
""
]
] | [
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] |
801.1871 | Toshihide Takagahara | Toshihide Takagahara and Ozgur Cakir | Theoretical aspects of quantum state transfer, correlation measurement
and electron-nuclei coupled dynamics in quantum dots | null | J. Nanophotonics Vol. 1, 011593 (2007) | null | null | cond-mat.mes-hall | null | Photons and electrons are the key quantum media for the quantum information
processing based on solid state devices. The essential ingredients to
accomplish the quantum repeater were investigated and their underlying physics
were revealed. The relevant elementary processes of the quantum state transfer
between a single photon and a single electron were analyzed, to clarify the
conditions to be satisfied to achieve the high fidelity of the quantum state
transfer. An optical method based on the Faraday rotation was proposed to carry
out the Bell measurement of two electrons which is a key operation in the
entanglement swapping for the quantum repeater and its feasibility was
confirmed. Also investigated was the quantum dynamics in the electron-nuclei
coupled spin system in quantum dots and a couple of new phenomena were
predicted related to the correlations induced by the hyperfine interaction,
namely, bunching and revival in the electron spin measurements. These findings
will pave the way to accomplish the efficient and robust quantum repeater and
nuclear spin quantum memory.
| [
{
"version": "v1",
"created": "Sat, 12 Jan 2008 00:37:26 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Takagahara",
"Toshihide",
""
],
[
"Cakir",
"Ozgur",
""
]
] | [
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] |
801.1872 | Artour Mouftakhov V | A. M. Akhtyamov, A. V. Mouftakhov, M. Teicher, L. S. Yamilova | Can One Hear Fastening of a Rod? | null | null | null | null | math.SP | null | Rods are parts of various devices. If it is impossible to observe the rod
directly, the only source of information about possible defects of its
fastening can be the natural frequencies of its flexural vibrations. The
question arises whether one would be able to detect damage in rod fastening by
the natural frequencies of its flexural vibrations. This paper gives and
substantiates a positive answer to this question.
| [
{
"version": "v1",
"created": "Sat, 12 Jan 2008 00:38:38 GMT"
}
] | 2008-01-15T00:00:00 | [
[
"Akhtyamov",
"A. M.",
""
],
[
"Mouftakhov",
"A. V.",
""
],
[
"Teicher",
"M.",
""
],
[
"Yamilova",
"L. S.",
""
]
] | [
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