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712.3779 | Jean-Luc Lehners | Jean-Luc Lehners, Paul J. Steinhardt | Non-Gaussian Density Fluctuations from Entropically Generated Curvature
Perturbations in Ekpyrotic Models | 5 pages, 2 figures. Sign error corrected and results generalized | Phys.Rev.D77:063533,2008; Erratum-ibid.D79:129903,2009 | 10.1103/PhysRevD.77.063533 10.1103/PhysRevD.79.129903 | null | hep-th astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We analyze the non-gaussian density perturbations generated in
ekpyrotic/cyclic models based on heterotic M-theory. In this picture, two
scalar fields produce nearly scale-invariant entropic perturbations during an
ekpyrotic phase that are converted into curvature modes {\it after the
ekpyrotic phase is complete} and just before the big bang. Both intrinsic
non-linearity in the entropy perturbation and the conversion process contribute
to non-gaussianity. The range of the non-gaussianity parameter $f_{NL}$ depends
on how gradual the conversion process is and the steepness of the scalar field
potential during the ekpyrotic phase. Although a wider range is possible, in
principle, natural values of the ekpyrotic parameters combined with a gradual
conversion process lead to values of $-60 \lesssim f_{NL} \lesssim +80$,
typically much greater than slow-roll inflation but within the current
observational bounds.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 19:27:00 GMT"
},
{
"version": "v2",
"created": "Sun, 24 Feb 2008 16:06:05 GMT"
},
{
"version": "v3",
"created": "Tue, 2 Jun 2009 15:14:49 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Lehners",
"Jean-Luc",
""
],
[
"Steinhardt",
"Paul J.",
""
]
] | [
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712.378 | Arik Yochelis | A. Yochelis, Y. Tintut, L.L. Demer, and A. Garfinkel | The formation of labyrinths, spots and stripe patterns in a biochemical
approach to cardiovascular calcification | null | New J. Phys 10, 055002 (2008) | 10.1088/1367-2630/10/5/055002 | null | nlin.PS | null | Calcification and mineralization are fundamental physiological processes, yet
the mechanisms of calcification, in trabecular bone and in calcified lesions in
atherosclerotic calcification, are unclear. Recently, it was shown in in vitro
experiments that vascular-derived mesenchymal stem cells can display
self-organized calcified patterns. These patterns were attributed to
activator/inhibitor dynamics in the style of Turing, with bone morphogenetic
protein 2 acting as an activator, and matrix GLA protein acting as an
inhibitor. Motivated by this qualitative activator-inhibitor dynamics, we
employ a prototype Gierer-Meinhardt model used in the context of
activator-inhibitor based biological pattern formation. Through a detailed
analysis in one and two spatial dimensions, we explore the pattern formation
mechanisms of steady state patterns, including their dependence on initial
conditions. These patterns range from localized holes to labyrinths and
localized peaks, or in other words, from dense to sparse activator
distributions (respectively). We believe that an understanding of the wide
spectrum of activator-inhibitor patterns discussed here is prerequisite to
their biochemical control. The mechanisms of pattern formation suggest
therapeutic strategies applicable to bone formation in atherosclerotic lesions
in arteries (where it is pathological) and to the regeneration of trabecular
bone (recapitulating normal physiological development).
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 19:39:59 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Dec 2007 21:43:51 GMT"
},
{
"version": "v3",
"created": "Wed, 23 Jan 2008 22:27:10 GMT"
},
{
"version": "v4",
"created": "Thu, 24 Apr 2008 18:35:22 GMT"
}
] | 2012-02-08T00:00:00 | [
[
"Yochelis",
"A.",
""
],
[
"Tintut",
"Y.",
""
],
[
"Demer",
"L. L.",
""
],
[
"Garfinkel",
"A.",
""
]
] | [
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712.3781 | Hans De Raedt | H. De Raedt, K. De Raedt, K. Michielsen, K. Keimpema, and S. Miyashita | Event-by-event simulation of quantum phenomena: Application to
Einstein-Podolosky-Rosen-Bohm experiments | Published paper with minor corrections | J. Comp. Theor. Nanosci. 4, 957 - 991, (2007) | null | null | quant-ph | null | We review the data gathering and analysis procedure used in real
Einstein-Podolsky-Rosen-Bohm experiments with photons and we illustrate the
procedure by analyzing experimental data. Based on this analysis, we construct
event-based computer simulation models in which every essential element in the
experiment has a counterpart. The data is analyzed by counting single-particle
events and two-particle coincidences, using the same procedure as in
experiments. The simulation models strictly satisfy Einstein's criteria of
local causality, do not rely on any concept of quantum theory or probability
theory, and reproduce all results of quantum theory for a quantum system of two
$S=1/2$ particles. We present a rigorous analytical treatment of these models
and show that they may yield results that are in exact agreement with quantum
theory. The apparent conflict with the folklore on Bell's theorem, stating that
such models are not supposed to exist, is resolved. Finally, starting from the
principles of probable inference, we derive the probability distributions of
quantum theory of the Einstein-Podolsky-Rosen-Bohm experiment without invoking
concepts of quantum theory.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:40:31 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Dec 2007 17:54:16 GMT"
}
] | 2007-12-26T00:00:00 | [
[
"De Raedt",
"H.",
""
],
[
"De Raedt",
"K.",
""
],
[
"Michielsen",
"K.",
""
],
[
"Keimpema",
"K.",
""
],
[
"Miyashita",
"S.",
""
]
] | [
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] |
712.3782 | Ricardo Gaitan | J. L. Diaz-Cruz, R. Gaitan-Lozano, G. Lopez-Castro and C. E.
Pagliarone | CKM-suppressed top quark decays t -> q + W in the SM and beyond | 11 pages | Phys.Rev.D77:094010,2008 | 10.1103/PhysRevD.77.094010 | null | hep-ph | null | Top quark decays are of particular interest as a mean to test the standard
model (SM) predictions, both for dominant (t -> b + W) and rare decays (t -> q
+ W, cV, cVV, c phi^{0}, bWZ). As the latter are highly suppressed, they become
an excellent window to probe the predictions of thories beyond the SM. In
particular, we evaluate the corrections from new physics to the CKM-suppressed
SM top quark decay t -> q + W (q = d, s), both within the an effective model
with right-handed currents and the MSSM. We also discuss the perspectives to
probe those predictions at the ILC.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 19:44:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Diaz-Cruz",
"J. L.",
""
],
[
"Gaitan-Lozano",
"R.",
""
],
[
"Lopez-Castro",
"G.",
""
],
[
"Pagliarone",
"C. E.",
""
]
] | [
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] |
712.3783 | Johannes Hirn | J. Hirn, A. Martin (Yale) and V. Sanz (BU) | Benchmarks for new strong interactions at the LHC | null | JHEP 0805:084,2008 | 10.1088/1126-6708/2008/05/084 | null | hep-ph | null | New strong interactions at the LHC may exhibit a richer structure than
expected from simply rescaling QCD to the electroweak scale. In fact, a
departure from rescaled QCD is required for compatibility with electroweak
constraints. To navigate the space of possible scenarios, we use a simple
framework, based on a 5D model with modifications of AdS geometry in the
infrared. In the parameter space, we select two points with particularly
interesting phenomenology. For these benchmark points, we explore the discovery
of triplets of vector and axial resonances at the LHC.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 19:44:59 GMT"
},
{
"version": "v2",
"created": "Mon, 24 Dec 2007 16:07:24 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Hirn",
"J.",
"",
"Yale"
],
[
"Martin",
"A.",
"",
"Yale"
],
[
"Sanz",
"V.",
"",
"BU"
]
] | [
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] |
712.3784 | Mamouni Ismail My | Mohamed Rachid Hilali and My Ismail Mamouni | The conjecture H: A lower bound of cohomologic dimension for an elliptic
space | 18 pages; Work exposed by the second author in the Algebraic topology
conference of Angers, France, October 2007 | null | null | null | math.AT | null | The goal of this paper is to ameliorate the sufficients conditions, already
established by the first author so that the sum of the numbers of Betti, of
1-connected rational finite CW-complex, is higher than the dimension of his
$\mathbb Q$-vectorial space of homotopy, we will present it in two aspects, one
algebraic and another geometrical.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 19:45:42 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Dec 2007 09:24:05 GMT"
}
] | 2007-12-26T00:00:00 | [
[
"Hilali",
"Mohamed Rachid",
""
],
[
"Mamouni",
"My Ismail",
""
]
] | [
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] |
712.3785 | Steven R. White | Steven R. White and Ian Affleck | Spectral Function for the S=1 Heisenberg Antiferromagetic Chain | 12 pages, 19 figs | null | 10.1103/PhysRevB.77.134437 | null | cond-mat.str-el | null | We study the spectral function, $S(k,\omega)$ for the spin-1, one dimensional
antiferromagnetic chain using a time-dependent density matrix renormalizaton
group (DMRG) numerical method. We develop methods for extrapolating the time
dependent correlation functions to larger times in order to enhance the
frequency resolution. The resulting spectral functions are impressively precise
and accurate. Our results confirm many qualitative expectations from non-linear
$\sigma$ model methods and test them quantitatively. The critical wave-vector
at which the single particle excitation emerges from the 2-particle continuum
is estimated to be $0.23\pi-0.24\pi$.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:46:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"White",
"Steven R.",
""
],
[
"Affleck",
"Ian",
""
]
] | [
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] |
712.3786 | Michael Hagan | Michael F. Hagan | Controlling Viral Capsid Assembly with Templating | submitted to Phys. Rev. E | null | 10.1103/PhysRevE.77.051904 | null | q-bio.BM | null | We develop coarse-grained models that describe the dynamic encapsidation of
functionalized nanoparticles by viral capsid proteins. We find that some forms
of cooperative interactions between protein subunits and nanoparticles can
dramatically enhance rates and robustness of assembly, as compared to the
spontaneous assembly of subunits into empty capsids. For large core-subunit
interactions, subunits adsorb onto core surfaces en masse in a disordered
manner, and then undergo a cooperative rearrangement into an ordered capsid
structure. These assembly pathways are unlike any identified for empty capsid
formation. Our models can be directly applied to recent experiments in which
viral capsid proteins assemble around the functionalized inorganic
nanoparticles [Sun et al., Proc. Natl. Acad. Sci (2007) 104, 1354]. In
addition, we discuss broader implications for understanding the dynamic
encapsidation of single-stranded genomic molecules during viral replication and
for developing multicomponent nanostructured materials.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 19:56:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hagan",
"Michael F.",
""
]
] | [
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] |
712.3787 | Mark Hannam | Mark Hannam, Sascha Husa, Bernd Br\"ugmann, Achamveedu Gopakumar | Comparison between numerical-relativity and post-Newtonian waveforms
from spinning binaries: the orbital hang-up case | 10 pages, 6 figures. Matches version published in PRD | Phys.Rev.D78:104007,2008 | 10.1103/PhysRevD.78.104007 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We compare results from numerical simulations of spinning binaries in the
"orbital hangup" case, where the binary completes at least nine orbits before
merger, with post-Newtonian results using the approximants TaylorT1, T4 and Et.
We find that, over the ten cycles before the gravitational-wave frequency
reaches $M\omega = 0.1$, the accumulated phase disagreement between NR and
2.5PN results is less than three radians, and is less than 2.5 radians when
using 3.5PN results. The amplitude disagreement between NR and restricted PN
results increases with the black holes' spin, from about 6% in the equal-mass
case to 12% when the black holes' spins are $S_i/M_i^2 = 0.85$. Finally, our
results suggest that the merger waveform will play an important role in
estimating the spin from such inspiral waveforms.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:03:04 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Dec 2007 19:25:32 GMT"
},
{
"version": "v3",
"created": "Wed, 26 Nov 2008 09:59:23 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hannam",
"Mark",
""
],
[
"Husa",
"Sascha",
""
],
[
"Brügmann",
"Bernd",
""
],
[
"Gopakumar",
"Achamveedu",
""
]
] | [
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712.3788 | Cristian LaRocca | C. E. La Rocca, L. A. Braunstein and P. A. Macri | Evolution equation for a model of surface relaxation in complex networks | 9 pages, 2 figures | Phys Rev E 77, 046120 (2008) | 10.1103/PhysRevE.77.046120 | null | cond-mat.stat-mech cond-mat.dis-nn | null | In this paper we derive analytically the evolution equation of the interface
for a model of surface growth with relaxation to the minimum (SRM) in complex
networks. We were inspired by the disagreement between the scaling results of
the steady state of the fluctuations between the discrete SRM model and the
Edward-Wilkinson process found in scale-free networks with degree distribution
$ P(k) \sim k^{-\lambda}$ for $\lambda <3$ [Pastore y Piontti {\it et al.},
Phys. Rev. E {\bf 76}, 046117 (2007)]. Even though for Euclidean lattices the
evolution equation is linear, we find that in complex heterogeneous networks
non-linear terms appear due to the heterogeneity and the lack of symmetry of
the network; they produce a logarithmic divergency of the saturation roughness
with the system size as found by Pastore y Piontti {\it et al.} for $\lambda
<3$.
| [
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},
{
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] | 2009-11-13T00:00:00 | [
[
"La Rocca",
"C. E.",
""
],
[
"Braunstein",
"L. A.",
""
],
[
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"P. A.",
""
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712.3789 | Richard J. van Kooten | D0 Collaboration: V. Abazov, et al | Measurement of the B0_s semileptonic branching ratio to an orbitally
excited D_s** state, Br(B0_s -> Ds1(2536) mu nu) | 7 pages, 2 figures, LaTeX, version with minor changes as accepted by
Phys. Rev. Lett | Phys.Rev.Lett.102:051801,2009 | 10.1103/PhysRevLett.102.051801 | Fermilab-Pub-07/659-E | hep-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In a data sample of approximately 1.3 fb-1 collected with the D0 detector
between 2002 and 2006, the orbitally excited charm state D_s1(2536) has been
observed with a measured mass of 2535.7 +/- 0.6 (stat) +/- 0.5 (syst) MeV via
the decay mode B0_s -> D_s1(2536) mu nu X. A first measurement is made of the
branching ratio product Br(b(bar) -> D_s1(2536) mu nu X).Br(D_s1(2536)->D*
K0_S). Assuming that D_s1(2536) production in semileptonic decay is entirely
from B0_s, an extraction of the semileptonic branching ratio Br(B0_s ->
D_s1(2536) mu nu X) is made.
| [
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},
{
"version": "v2",
"created": "Wed, 4 Feb 2009 17:01:28 GMT"
}
] | 2009-02-27T00:00:00 | [
[
"D0 Collaboration",
"",
""
],
[
"Abazov",
"V.",
""
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712.379 | Arik Yochelis | Arik Yochelis and Alan Garfinkel | Front motion and localized states in an asymmetric bistable
activator-inhibitor system with saturation | 4 pages, 3 figures | Phys. Rev. E 77, R035204 (2008) | 10.1103/PhysRevE.77.035204 | null | nlin.PS | null | We study the spatiotemporal properties of coherent states (peaks, holes, and
fronts) in a bistable activator-inhibitor system that exhibits biochemical
saturated autocatalysis, and in which fronts do not preserve spatial parity
symmetry. Using the Gierer-Meinhardt prototype model, we find the conditions in
which two distinct pinning regions are formed. The first pinning type is known
in the context of variational systems while the second is structurally
different due to the presence of a heteroclinic bifurcation between two uniform
states. The bifurcation also separates the parameter regions of
counterpropagating fronts, leading in turn to the growth or contraction of
activator domains. These phenomena expand the range of pattern formation theory
and its biomedical applications: activator domain retraction suggests potential
therapeutic strategies for patterned pathologies, such as cardiovascular
calcification.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:18:59 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Mar 2008 20:23:13 GMT"
}
] | 2008-03-20T00:00:00 | [
[
"Yochelis",
"Arik",
""
],
[
"Garfinkel",
"Alan",
""
]
] | [
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] |
712.3791 | Johannes Berg | Johannes Berg | Dynamics of gene expression and the regulatory inference problem | revised version to appear in Europhys. Lett., new title | null | 10.1209/0295-5075/82/28010 | null | q-bio.MN | null | From the response to external stimuli to cell division and death, the
dynamics of living cells is based on the expression of specific genes at
specific times. The decision when to express a gene is implemented by the
binding and unbinding of transcription factor molecules to regulatory DNA.
Here, we construct stochastic models of gene expression dynamics and test them
on experimental time-series data of messenger-RNA concentrations. The models
are used to infer biophysical parameters of gene transcription, including the
statistics of transcription factor-DNA binding and the target genes controlled
by a given transcription factor.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:21:44 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Mar 2008 16:17:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Berg",
"Johannes",
""
]
] | [
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] |
712.3792 | Christian Degen | C. L. Degen, M. Poggio, H. J. Mamin, and D. Rugar | Nuclear spin relaxation induced by a mechanical resonator | 4 pages, 4 figures | Phys. Rev. Lett. 100, 137601 (2008) | 10.1103/PhysRevLett.100.137601 | null | cond-mat.mes-hall | null | We report on measurements of the spin lifetime of nuclear spins strongly
coupled to a micromechanical cantilever as used in magnetic resonance force
microscopy. We find that the rotating-frame correlation time of the statistical
nuclear polarization is set by the magneto-mechanical noise originating from
the thermal motion of the cantilever. Evidence is based on the effect of three
parameters: (1) the magnetic field gradient (the coupling strength), (2) the
Rabi frequency of the spins (the transition energy), and (3) the temperature of
the low-frequency mechanical modes. Experimental results are compared to
relaxation rates calculated from the spectral density of the magneto-mechanical
noise.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:32:36 GMT"
}
] | 2008-04-04T00:00:00 | [
[
"Degen",
"C. L.",
""
],
[
"Poggio",
"M.",
""
],
[
"Mamin",
"H. J.",
""
],
[
"Rugar",
"D.",
""
]
] | [
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] |
712.3793 | Pablo Moya S | C. A. Far\'ias, P. S. Moya and V. A. Pinto | On the Relationship between Thermodynamics and Special Relativity | 8 pages, no figures | null | null | null | physics.class-ph | null | Starting from a formulation for the $dS$ element that includes movement, and
considering the variation of the entropy Lorentz invariant, we found the
relativistic transformations for thermodynamic systems that satisfy the three
laws of thermodynamics. Particularly, we found the temperature and pressure
transformations, given by $T'=\gamma T$ and $p'=\gamma^2p$ respectively.
Furthermore, we show that this transformations keeps the form of the state
equation for an ideal gas in agreement with the relativity principle.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:34:54 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Mar 2008 16:43:16 GMT"
}
] | 2008-03-20T00:00:00 | [
[
"Farías",
"C. A.",
""
],
[
"Moya",
"P. S.",
""
],
[
"Pinto",
"V. A.",
""
]
] | [
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] |
712.3794 | Jason Bell | Jason P. Bell | Simple algebras of Gelfand-Kirillov dimension two | 6 pages; fixed reference and corrected a misquoted statement from the
literature | null | null | null | math.RA | null | Let $k$ be a field. We show that a finitely generated simple Goldie
$k$-algebra of quadratic growth is noetherian and has Krull dimension 1. Thus a
simple algebra of quadratic growth is left noetherian if and only if it is
right noetherian. As a special case, we see that if A is a finitely generated
simple domain of quadratic growth then A is noetherian and by a result of
Stafford every right and left ideal is generated by at most two elements. We
conclude by posing questions and giving examples in which we consider what
happens when the hypotheses are relaxed.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:35:08 GMT"
},
{
"version": "v2",
"created": "Mon, 31 Dec 2007 21:14:43 GMT"
}
] | 2007-12-31T00:00:00 | [
[
"Bell",
"Jason P.",
""
]
] | [
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] |
712.3795 | Irina Zhuravleva Vladimirovna | B. V. Komberg, D. I. Nagirner, I. V. Zhuravleva | The Sunyaev-Zel'dovich Effect On Elliptical Galaxies | 10 pages, 4 figures, submitted to Astronomichesky Zhurnal | null | null | null | astro-ph | null | The history of discovering of hot gas in galaxies is traced briefly, its main
properties are described and the desirability to make them more precise, in
particular to obtain additional data on the mass of such gas is pointed out.
For this purpose observations of the Sunyaev-Zel'dovich effect on hot gas of
coronas of elliptic galaxies are proposed. The absolute and relative
disturbances of the cosmic microwave radiation spectrum due to scattering of
relic photons by Maxwellian electrons are calculated according the formula of
the article. With the example of three elliptic galaxies it is shown that
observation of the SZ effect on such galaxies is quite possible. Kinematic SZ
effect arising due to peculiar movement and rotation of galaxies is available
for observation as well. Such observations combined with X-ray data would make
it possible to get more about properties of galactic gas, to obtain additional
information on rotation of galaxies, on possible accreting gas flows and on hot
galactic wind.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:14:00 GMT"
},
{
"version": "v2",
"created": "Fri, 8 Feb 2008 14:40:01 GMT"
}
] | 2008-02-08T00:00:00 | [
[
"Komberg",
"B. V.",
""
],
[
"Nagirner",
"D. I.",
""
],
[
"Zhuravleva",
"I. V.",
""
]
] | [
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] |
712.3796 | Olaf Maron Dr. | Napoleon Maron, Olaf Maron | Criteria for mixing rules application for inhomogeneous astrophysical
grains | 36 pages, 21 figures, accepted for MNRAS | null | 10.1111/j.1365-2966.2008.13908.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The analysis presented in this paper verifies which of the mixing rules are
best for real components of interstellar dust in possible wide range of
wavelengths.The DDA method with elements of different components with various
volume fractions has been used. We have considered 6 materials: ice, amorphous
carbon, graphite, SiC, silicates and iron, and the following mixing rules:
Maxwell-Garnett, Bruggeman, Looyenga, Hanay and Lichtenecker which must satisfy
rigorous bounds. The porous materials have also been considered. We have
assumed simplified spatial distribution, shape and size of inclusions. The
criteria given by \citet{draine1988} have been used to determine the range of
wavelengths for the considered mixtures in order to calculate the ${\rm
Q_{ext}}$ using the DDA. From all chosen mixing rules for the examined
materials in majority of cases (13 out of 20) the best results have been
obtained using the Lichtenecker mixing rule. In 5 cases this rule is better for
some volume fraction of inclusions.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:33:30 GMT"
},
{
"version": "v2",
"created": "Thu, 3 Jan 2008 23:04:48 GMT"
},
{
"version": "v3",
"created": "Sat, 6 Sep 2008 09:36:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
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""
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712.3797 | Eyer Laurent | Laurent Eyer, Nami Mowlavi | Variable stars across the observational HR diagram | 21 pages, 9 figures | J.Phys.Conf.Ser.118:012010,2008 | 10.1088/1742-6596/118/1/012010 | null | astro-ph | null | An overview of pulsating variable stars across the observational
Hertzprung-Russel (HR) diagram is presented, together with a summary of their
global properties. The HR diagram is presented with a third colour-coded
dimension, visualizing the fraction of variable, the amplitude of variability
or the period of variability. The distribution of variable stars in the other
observational diagrams, such as the Period-Amplitude diagram, is also
presented. Some of the progresses performed in the field of variable stars
during the last decade are briefly summarized, and future projects that will
improve our knowledge of variable stars are mentioned.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:08:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Eyer",
"Laurent",
""
],
[
"Mowlavi",
"Nami",
""
]
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712.3798 | Basudeb Dasgupta | Basudeb Dasgupta and Amol Dighe | Collective three-flavor oscillations of supernova neutrinos | 44 pages, 24 figures. Typo corrected in Eqs. (52, 68, 85 and 91) of
the version published in PRD. Results unchanged | Phys.Rev.D77:113002,2008 | 10.1103/PhysRevD.77.113002 | TIFR/TH/07-36 | hep-ph astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Neutrinos and antineutrinos emitted from a core collapse supernova interact
among themselves, giving rise to collective flavor conversion effects that are
significant near the neutrinosphere. We develop a formalism to analyze these
collective effects in the complete three-flavor framework. It naturally
generalizes the spin-precession analogy to three flavors and is capable of
analytically describing phenomena like vacuum/MSW oscillations, synchronized
oscillations, bipolar oscillations and spectral split. Using the formalism, we
demonstrate that the flavor conversions may be "factorized" into two-flavor
oscillations with hierarchical frequencies. We explicitly show how the
three-flavor solution may be constructed by combining two-flavor solutions. For
a typical supernova density profile, we identify an approximate separation of
regions where distinctly different flavor conversion mechanisms operate, and
demonstrate the interplay between collective and MSW effects. We pictorialize
our results in terms of the "e_3 - e_8 triangle" diagram, which is a tool that
can be used to visualize three-neutrino flavor conversions in general, and
offers insights into the analysis of the collective effects in particular.
| [
{
"version": "v1",
"created": "Sun, 23 Dec 2007 20:39:10 GMT"
},
{
"version": "v2",
"created": "Sat, 5 Apr 2008 18:56:51 GMT"
},
{
"version": "v3",
"created": "Thu, 21 Jan 2010 17:14:50 GMT"
}
] | 2010-01-21T00:00:00 | [
[
"Dasgupta",
"Basudeb",
""
],
[
"Dighe",
"Amol",
""
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712.3799 | Norihiro Tanahashi | Norihiro Tanahashi, Takahiro Tanaka | Time-symmetric initial data of large brane-localized black hole in RS-II
model | 14 pages, 9 figures. Typo corrected | JHEP0803:041,2008 | 10.1088/1126-6708/2008/03/041 | KUNS-2117 | gr-qc | null | In the aim of shedding a new light on the classical black hole evaporation
conjecture stating that a static brane-localized black hole (BH) larger than
the bulk curvature scale does not exist in Randall-Sundrum II (RS-II) model, we
investigate time-symmetric initial data with a brane-localized apparent horizon
(AH) and analyzed its properties. We find that a three-parameter family of such
initial data can be constructed by simply placing a brane on a constant time
surface of Schwarzschild anti-de Sitter space. By this method, we unambiguously
confirm that initial data with an arbitrarily large AH area do exist. We
compare the ADM mass and the horizon area of our initial data with that of the
black string (BS) solution, and find that any initial data constructed by this
method do not have a smaller mass than the BS solution when the horizon area is
larger than the size determined by the bulk curvature scale. We further
investigate what kind of configuration realizes the minimum mass for the same
AH area. The configuration that realizes the smallest mass turns out to be the
one close to the BS truncated by a cap. We also demonstrate that the same
method applies to construct initial data in (3+1)-dimensional RS-II brane
world. In this case an exact solution of a brane-localized BH exists but BS
solution does not. Nevertheless, the behavior of the initial data is quite
similar in both cases. We find that the known exact solution always has a
smaller mass than our initial data with the same horizon area. This result
enforces the standard belief that the exact BH solution is the most stable
black object in the four-dimensional RS-II model. These results are all
consistent with the classical BH evaporation conjecture, but unfortunately it
turns out that they do not provide a strong support of it.
| [
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] | 2008-11-26T00:00:00 | [
[
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""
],
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""
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712.38 | Jorge Moreno | Jorge Moreno, Carlo Giocoli, and Ravi K. Sheth | Merger history trees of dark matter haloes in moving barrier models | MNRAS accepted, 15 pages, 12 figures | Mon.Not.Roy.Astron.Soc.391:1729-1740,2008 | 10.1111/j.1365-2966.2008.13766.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present an algorithm for generating merger histories of dark matter
haloes. The algorithm is based on the excursion set approach with moving
barriers whose shape is motivated by the ellipsoidal collapse model of halo
formation. In contrast to most other merger-tree algorithms, ours takes
discrete steps in mass rather than time. This allows us to quantify effects
which arise from the fact that outputs from numerical simulations are usually
in discrete time bins. In addition, it suggests a natural set of scaling
variables for describing the abundance of halo progenitors; this scaling is not
as general as that associated with a spherical collapse. We test our algorithm
by comparing its predictions with measurements in numerical simulations. The
progenitor mass fractions and mass functions are in good agreement, as is the
predicted scaling law. We also test the formation-redshift distribution, the
mass distribution at formation, and the redshift distribution of the most
recent major merger; all are in reasonable agreement with N-body simulation
data, over a broad range of masses and redshifts. Finally, we study the effects
of sampling in discrete time snapshots. In all cases, the improvement over
algorithms based on the spherical collapse assumption is significant.
| [
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"created": "Sat, 3 Jan 2009 00:52:26 GMT"
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] | 2009-01-03T00:00:00 | [
[
"Moreno",
"Jorge",
""
],
[
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"Carlo",
""
],
[
"Sheth",
"Ravi K.",
""
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712.3801 | Jose La Luz | David Allen and Jose La Luz | A Counterexample to a conjecture of Bosio and Meersseman | null | null | null | null | math.SG | null | In a paper of Bosio and Meersseman (Real quadrics in Cn, complex manifolds
and convex polytopes) the following is conjectured: If P is dual neighborly,
then Zp is diffeomorphic to the connected sum of products of spheres. In this
paper a counterexample is provided.
| [
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},
{
"version": "v2",
"created": "Sat, 15 Mar 2008 12:55:48 GMT"
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] | 2008-03-15T00:00:00 | [
[
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"David",
""
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[
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""
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712.3802 | Marco Lenci | Luca Bussolari, Marco Lenci | Hyperbolic billiards with nearly flat focusing boundaries. I | 21 pages, 9 figures | Physica D 237 (2008), no. 18, 2272-2281 | 10.1016/j.physd.2008.02.006 | null | math.DS math-ph math.MP | null | The standard Wojtkowski-Markarian-Donnay-Bunimovich technique for the
hyperbolicity of focusing or mixed billiards in the plane requires the diameter
of a billiard table to be of the same order as the largest ray of curvature
along the focusing boundary. This is due to the physical principle that is used
in the proofs, the so-called defocusing mechanism of geometrical optics. In
this paper we construct examples of hyperbolic billiards with a focusing
boundary component of arbitrarily small curvature whose diameter is bounded by
a constant independent of that curvature. Our proof employs a nonstardard cone
bundle that does not solely use the familiar dispersing and defocusing
mechanisms.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:23:41 GMT"
}
] | 2008-10-15T00:00:00 | [
[
"Bussolari",
"Luca",
""
],
[
"Lenci",
"Marco",
""
]
] | [
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712.3803 | Mladen Georgiev | Mladen Georgiev | Vibronic polarons: comments on a model for the colossal field-resistance
effects in manganites | 8 pages with 4 figures, all pdf format | null | null | null | cond-mat.mtrl-sci cond-mat.str-el | null | In addition to mechanisms already proposed to account for the formation in
manganites of a small-polaron superlattice above the Curie temperature Tc and
to a metallic-like sea of large polarons below Tc, we now consider other
observed colossal-resistance inducing fields, such as magnetic, electric,
photon, or strain fields. We attribute the charge-ordered phase formation to
the occurrence of strong dipolar binding of vibronic small polarons arising
from the phonon coupling of highly polarizable two-level orbital systems. These
species having associated inherent electric and magnetic off-center dipoles,
they couple to the external fields leading to the observed colossal effects.
The random phase appears due to polaron band widening in the external field.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:38:15 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Georgiev",
"Mladen",
""
]
] | [
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712.3804 | A. Lobel | A. Lobel, R. Blomme (Royal Observatory of Belgium) | Modeling Ultraviolet Wind Line Variability in Massive Hot Stars | 58 pages, 16 figures, 1 animation. Accepted for publication in The
Astrophysical Journal, Main Journal. More information and animations are
available at http://alobel.freeshell.org/hotstars.html | null | 10.1086/529129 | null | astro-ph | null | We model the detailed time-evolution of Discrete Absorption Components (DACs)
observed in P Cygni profiles of the Si IV lam1400 resonance doublet lines of
the fast-rotating supergiant HD 64760 (B0.5 Ib). We adopt the common assumption
that the DACs are caused by Co-rotating Interaction Regions (CIRs) in the
stellar wind. We perform 3D radiative transfer calculations with hydrodynamic
models of the stellar wind that incorporate these large-scale density- and
velocity-structures. We develop the 3D transfer code Wind3D to investigate the
physical properties of CIRs with detailed fits to the DAC shape and morphology.
The CIRs are caused by irregularities on the stellar surface that change the
radiative force in the stellar wind. In our hydrodynamic model we approximate
these irregularities by circular symmetric spots on the stellar surface. We use
the Zeus3D code to model the stellar wind and the CIRs, limited to the
equatorial plane. We constrain the properties of large-scale wind structures
with detailed fits to DACs observed in HD 64760. A model with two spots of
unequal brightness and size on opposite sides of the equator, with opening
angles of 20 +/- 5 degr and 30 +/- 5 degr diameter, and that are 20 +/- 5 % and
8 +/- 5 % brighter than the stellar surface, respectively, provides the best
fit to the observed DACs. The recurrence time of the DACs compared to the
estimated rotational period corresponds to spot velocities that are 5 times
slower than the rotational velocity. The mass-loss rate of the structured wind
model for HD 64760 does not exceed the rate of the spherically symmetric smooth
wind model by more than 1 %. The fact that DACs are observed in a large number
of hot stars constrains the clumping that can be present in their winds, as
substantial amounts of clumping would tend to destroy the CIRs.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:40:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lobel",
"A.",
"",
"Royal Observatory of Belgium"
],
[
"Blomme",
"R.",
"",
"Royal Observatory of Belgium"
]
] | [
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] |
712.3805 | Patrice Verdier | D0 Collaboration: V. Abazov, et al | Search for squarks and gluinos in events with jets and missing
transverse energy using 2.1 fb-1 of ppbar collision data at sqrt(s)=1.96 TeV | null | Phys.Lett.B660:449-457,2008 | 10.1016/j.physletb.2008.01.042 | FERMILAB-PUB-07-668-E | hep-ex | null | A data sample corresponding to an integrated luminosity of 2.1 fb-1 collected
by the D0 detector at the Fermilab Tevatron Collider was analyzed to search for
squarks and gluinos produced in ppbar collisions at a center-of-mass energy of
1.96 TeV. No evidence for the production of such particles was observed in
topologies involving jets and missing transverse energy, and 95% C.L. lower
limits of 379 GeV and 308 GeV were set on the squark and gluino masses,
respectively, within the framework of minimal supergravity with tan(beta)=3,
A0=0, and mu<0. The corresponding previous limits are improved by 54 GeV and 67
GeV.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 21:53:50 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 09:18:35 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"D0 Collaboration",
"",
""
],
[
"Abazov",
"V.",
""
]
] | [
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712.3806 | Emmanuil Saridakis | E. N. Saridakis | Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in
the Bulk. Interacting Behavior and the w =-1 Crossing | 16 pages, version published in Phys. Lett. B | Phys.Lett.B661:335-341,2008 | 10.1016/j.physletb.2008.02.032 | null | gr-qc hep-th | null | We apply bulk holographic dark energy in general braneworld models with a
Gauss-Bonnet term in the bulk and an induced gravity term and a perfect fluid
on the brane. Without making any additional assumptions we extract the
Friedmann equation on the physical brane and we show that a
$\rho$-$\rho_\Lambda$ coupling arises naturally by the full 5D dynamics. The
low-energy (late-time) evolution reveals that the effective 4D holographic dark
energy behaves as ``quintom'', that is it crosses the phantom divide $w=-1$
during the evolution. In particular, the Gauss-Bonnet contribution decreases
the present value of $w_\Lambda$, while it increases the growing rate of
$w_\Lambda(z)$ with $z$, in comparison with the case where such a term is
absent.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:04:30 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 20:01:46 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Saridakis",
"E. N.",
""
]
] | [
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0.0218994524,
0.103107892,
-0.0006592089,
0.0047402075,
-0.0154978875,
0.0666738376
] |
712.3807 | Jianguo Liu | Jian-Guo Liu, Bing-Hong Wang, Qiang Guo | Improved Collaborative Filtering Algorithm via Information
Transformation | 5 pages, 4 figures | Int. J. Mod. Phys. C 20(2), 285-293 (2009) | 10.1142/S0129183109013613 | null | cs.LG cs.CY | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, we propose a spreading activation approach for collaborative
filtering (SA-CF). By using the opinion spreading process, the similarity
between any users can be obtained. The algorithm has remarkably higher accuracy
than the standard collaborative filtering (CF) using Pearson correlation.
Furthermore, we introduce a free parameter $\beta$ to regulate the
contributions of objects to user-user correlations. The numerical results
indicate that decreasing the influence of popular objects can further improve
the algorithmic accuracy and personality. We argue that a better algorithm
should simultaneously require less computation and generate higher accuracy.
Accordingly, we further propose an algorithm involving only the top-$N$ similar
neighbors for each target user, which has both less computational complexity
and higher algorithmic accuracy.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 14:25:18 GMT"
},
{
"version": "v2",
"created": "Fri, 12 Dec 2008 16:31:13 GMT"
},
{
"version": "v3",
"created": "Wed, 14 Oct 2009 15:30:56 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Liu",
"Jian-Guo",
""
],
[
"Wang",
"Bing-Hong",
""
],
[
"Guo",
"Qiang",
""
]
] | [
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] |
712.3808 | Karl-Heinz Schmidt | C. Boeckstiegel, S. Steinhaeuser, K.-H. Schmidt, H.-G. Clerc, A.
Grewe, A. Heinz, M. de Jong, A. R. Junghans, J. Mueller, B. Voss | Nuclear-fission studies with relativistic secondary beams: analysis of
fission channels | 16 pages, 3 figures, background information on
http://www.gsi.de/charms | Nucl.Phys.A802:12-25,2008 | 10.1016/j.nuclphysa.2008.01.012 | null | nucl-ex | null | Nuclear fission of several neutron-deficient actinides and pre-actinides from
excitation energies around 11 MeV was studied at GSI Darmstadt by use of
relativistic secondary beams. The characteristics of multimodal fission of
nuclei around 226Th are systematically investigated and interpreted as the
superposition of three fission channels. Properties of these fission channels
have been determined for 15 systems. A global view on the properties of fission
channels including previous results is presented. The positions of the
asymmetric fission channels are found to be constant in element number over the
whole range of systems investigated.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:25:38 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Boeckstiegel",
"C.",
""
],
[
"Steinhaeuser",
"S.",
""
],
[
"Schmidt",
"K. -H.",
""
],
[
"Clerc",
"H. -G.",
""
],
[
"Grewe",
"A.",
""
],
[
"Heinz",
"A.",
""
],
[
"de Jong",
"M.",
""
],
[
"Junghans",
"A. R.",
""
],
[
"Mueller",
"J.",
""
],
[
"Voss",
"B.",
""
]
] | [
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712.3809 | Ramses van Zon | Ramses van Zon, Jeremy Schofield | Event-Driven Dynamics of Rigid Bodies Interacting via Discretized
Potentials | 9 pages, 5 figures | J. Chem. Phys. 128, 154119 (2008) | 10.1063/1.2901173 | null | cond-mat.soft | null | A framework for performing event-driven, adaptive time step simulations of
systems of rigid bodies interacting under stepped or terraced potentials in
which the potential energy is only allowed to have discrete values is outlined.
The scheme is based on a discretization of an underlying continuous potential
that effectively determines the times at which interaction energies change. As
in most event-driven approaches, the method consists of specifying a means of
computing the free motion, evaluating the times at which interactions occur,
and determining the consequences of interactions on subsequent motion for the
terraced-potential. The latter two aspects are shown to be simply expressible
in terms of the underlying smooth potential. Within this context, algorithms
for computing the times of interaction events and carrying out efficient
event-driven simulations are discussed. The method is illustrated on system
composed of rigid rods in which the constituents interact via a terraced
potential that depends on the relative orientations of the rods.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:32:03 GMT"
}
] | 2008-08-11T00:00:00 | [
[
"van Zon",
"Ramses",
""
],
[
"Schofield",
"Jeremy",
""
]
] | [
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] |
712.381 | Philippe G. LeFloch | Philippe G. LeFloch and Majid Mohammadian | Why many theories of shock waves are necessary. Kinetic functions,
equivalent equations, and fourth-order models | 35 pages | null | 10.1016/j.jcp.2007.12.026 | null | math.NA math.AP physics.flu-dyn | null | We consider several systems of nonlinear hyperbolic conservation laws
describing the dynamics of nonlinear waves in presence of phase transition
phenomena. These models admit under-compressive shock waves which are not
uniquely determined by a standard entropy criterion but must be characterized
by a kinetic relation. Building on earlier work by LeFloch and collaborators,
we investigate the numerical approximation of these models by {\sl high-order}
finite difference schemes, and uncover several new features of the kinetic
function associated with with physically motivated second and third-order
regularization terms, especially viscosity and capillarity terms. On one hand,
the role of the equivalent equation associated with a finite difference scheme
is discussed. We conjecture here and demonstrate numerically that the
(numerical) kinetic function associated with a scheme approaches the (analytic)
kinetic function associated with the given model --especially since its
equivalent equation approaches the regularized model at a higher order. On the
other hand, we demonstrate numerically that a kinetic function can be
associated with the thin liquid film model and the generalized Camassa-Holm
model. Finally, we investigate to what extent a kinetic function can be
associated with the equations of van der Waals fluids, whose flux-function
admits two inflection points.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:33:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"LeFloch",
"Philippe G.",
""
],
[
"Mohammadian",
"Majid",
""
]
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] |
712.3811 | Kimball A. Milton | Kimball A. Milton and Jef Wagner | Multiple Scattering Methods in Casimir Calculations | 21 pages, 7 figures, ReVTEX. Introduction shortened, Appendix A
expanded, references added | J.Phys.A41:155402,2008 | 10.1088/1751-8113/41/15/155402 | null | hep-th quant-ph | null | Multiple scattering formulations have been employed for more than 30 years as
a method of studying the quantum vacuum or Casimir interactions between
distinct bodies. Here we review the method in the simple context of
$\delta$-function potentials, so-called semitransparent bodies. (In the limit
of strong coupling, a semitransparent boundary becomes a Dirichlet one.) After
applying the method to rederive the Casimir force between two semitransparent
plates and the Casimir self-stress on a semitransparent sphere, we obtain
expressions for the Casimir energies between disjoint parallel semitransparent
cylinders and between disjoint semitransparent spheres. Simplifications occur
for weak and strong coupling. In particular, after performing a power series
expansion in the ratio of the radii of the objects to the separation between
them, we are able to sum the weak-coupling expansions exactly to obtain
explicit closed forms for the Casimir interaction energy. The same can be done
for the interaction of a weak-coupling sphere or cylinder with a Dirichlet
plane. We show that the proximity force approximation (PFA), which becomes the
proximity force theorem when the objects are almost touching, is very poor for
finite separations.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:34:28 GMT"
},
{
"version": "v2",
"created": "Tue, 26 Feb 2008 00:45:57 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Milton",
"Kimball A.",
""
],
[
"Wagner",
"Jef",
""
]
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712.3812 | Lucas Platter | Lucas Platter | Universality in Few-Body Systems | Plenary talk at 20th European Conference on Few-Body Problems in
Physics (EFB 20), Pisa, Italy, 10-14 Sep 2007, FBS style, 2 figues | Few Body Syst.43:155-160,2008 | 10.1007/s00601-008-0225-7 | null | nucl-th | null | Low-energy universality in atomic few-body systems as a result of a large
two-body scattering length has gained a lot of attention recently. Here, I
discuss recent progress in describing the three-body recombination of cold
atoms in terms of a finite set of universal scaling functions and review
results for the recombination length of cesium-133 atoms obtained with these
functions. Furthermore, I will consider the inclusion of effective range
corrections and the relevance for further calculations in atomic and nuclear
physics.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:34:56 GMT"
}
] | 2009-01-08T00:00:00 | [
[
"Platter",
"Lucas",
""
]
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] |
712.3813 | Seunghoon Han | Seunghoon Han, Yi Xiong, Dentcho Genov, Zhaowei Liu, Guy Bartal and
Xiang Zhang | Molding the flow of light at deep sub-wavelength scale | 4 figures and supplementary information | null | null | null | physics.optics | null | The diffractive nature of light has limited optics and photonics to operate
at scales much larger than the wavelength of light. The major challenge in
scaling-down integrated photonics is how to mold the light flow below
diffraction-limit in all three dimensions. A high index solid immersion lens
can improve the spatial resolution by increasing the medium refractive index,
but only to few times higher than in air. Photonic crystals can guide light in
three dimensions, however, the guided beam width is around a wavelength.
Surface plasmons has a potential to reach the sub-wavelength scales;
nevertheless, it is confined in the two-dimensional interface between metals
and dielectrics. Here, we present a new approach for molding the light flow at
the deep sub-wavelength scale, using metamaterials with uniquely designed
dispersion. We develop a design methodology for realizing sub-wavelength ray
optics, and demonstrate lambda/10 width light beams flow through
three-dimensional space.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:42:42 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Han",
"Seunghoon",
""
],
[
"Xiong",
"Yi",
""
],
[
"Genov",
"Dentcho",
""
],
[
"Liu",
"Zhaowei",
""
],
[
"Bartal",
"Guy",
""
],
[
"Zhang",
"Xiang",
""
]
] | [
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] |
712.3814 | Korkut Okan Ozansoy | O. Cakir and K. O. Ozansoy | Unparticle Searches Through Gamma Gamma Scattering | 15 pages, 5 figures, 2 tables | Eur.Phys.J.C56:279-285,2008 | 10.1140/epjc/s10052-008-0658-7 | null | hep-ph | null | We investigate the effects of unparticles on gamma gamma--> gamma gamma
scattering for photon collider mode of the future multi-TeV e^+e^- linear
collider. We show the effects of unparticles on the differential, and total
scattering cross sections for different polarization configurations.
Considering 1-loop Standard Model background contributions from the charged
fermions, and W^{+-} bosons to the cross section, we calculate the upper limits
on the unparticle couplings lambda_0 to the photons for various values of the
scaling dimension d(1<d<2) at sqrt{s}=0.5-5 TeV.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 12:17:32 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Jan 2008 22:25:00 GMT"
},
{
"version": "v3",
"created": "Mon, 10 Mar 2008 18:31:14 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cakir",
"O.",
""
],
[
"Ozansoy",
"K. O.",
""
]
] | [
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] |
712.3815 | Sylvie Ruette | Sylvie Ruette | Rotation set for maps of degree 1 on the graph sigma | Changes in new version: numbers of theorems cited from [2]
(consequence of editing process of [2]), modification of definition 2.8 (to
avoid a possible ambiguity), reference [2] (now published), some typos | Israel Journal of Mathematics, 184, 275-299, 2011 | null | null | math.DS | null | For a continuous map on a topological graph containing a unique loop S it is
possible to define the degree and, for a map of degree 1, rotation numbers. It
is known that the set of rotation numbers of points in S is a compact interval
and for every rational r in this interval there exists a periodic point of
rotation number r. The whole rotation set (i.e. the set of all rotation
numbers) may not be connected and it is not known in general whether it is
closed.
The graph sigma is the space consisting in an interval attached by one of its
endpoints to a circle. We show that, for a map of degree 1 on the graph sigma,
the rotation set is closed and has finitely many connected components.
Moreover, for all rational numbers r in the rotation set, there exists a
periodic point of rotation number r.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:48:45 GMT"
},
{
"version": "v2",
"created": "Thu, 22 May 2008 16:17:49 GMT"
}
] | 2014-07-08T00:00:00 | [
[
"Ruette",
"Sylvie",
""
]
] | [
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] |
712.3816 | Matthias Keller | Matthias Keller | The essential spectrum of the Laplacian on rapidly branching
tessellations | null | null | null | null | math-ph math.MP math.SP | null | In this paper we characterize emptiness of the essential spectrum of the
Laplacian under a hyperbolicity assumption for general graphs. Moreover we
present a characterization for emptiness of the essential spectrum for planar
tessellations in terms of curvature.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 22:59:14 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Jan 2008 19:36:47 GMT"
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] | 2008-01-17T00:00:00 | [
[
"Keller",
"Matthias",
""
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] |
712.3817 | Richard Hill | Richard J. Hill | Update on semileptonic charm decays | 4 pages. To be published in the proceedings of CHARM07, Ithaca, NY,
August 2007, eConf C070805 | ECONF C070805:22,2007 | 10.2172/922051 | FERMILAB-CONF-07-669-T | hep-ph | null | A brief update is given on recent developments in the theory of exclusive
semileptonic charm decays. A check on analyticity arguments from the kaon
system is reviewed. Recent results on form factor shape measurements are
discussed.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 19:30:46 GMT"
}
] | 2011-03-18T00:00:00 | [
[
"Hill",
"Richard J.",
""
]
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712.3818 | Marie A. Vitulli | Marie A. Vitulli | Serre's Condition R_l for Affine Semigroup Rings | 13 pages | null | null | null | math.AC math.AG | null | In this note we characterize the affine semigroup rings K[S] over an
arbitrary field K that satisfy condition R_l of Serre. Our characterization is
in terms of the face lattice of the positive cone pos(S) of S. We start by
reviewing some basic facts about the faces of pos(S) and consequences for the
monomial primes of K[S]. After proving our characterization we turn our
attention to the Rees algebras of a special class of monomial ideals in a
polynomial ring over a field. In this special case, some of the characterizing
criteria are always satisfied. We give examples of nonnormal affine semigroup
rings that satisfy R_2.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 23:28:08 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Vitulli",
"Marie A.",
""
]
] | [
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] |
712.3819 | Jeremy Coe | J. P. Coe, A. Sudbery, and I. D'Amico | Entanglement and density-functional theory: testing approximations on
Hooke's atom | 14 pages with 18 figures; corrected typos, corrected expression for
first-order energy in section VI and consequently Fig.13, conclusions and
other results unaffected | Phys. Rev. B 77, 205122 (2008) | 10.1103/PhysRevB.77.205122 | null | quant-ph cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present two methods of calculating the spatial entanglement of an
interacting electron system within the framework of density-functional theory.
These methods are tested on the model system of Hooke's atom for which the
spatial entanglement can be calculated exactly. We analyse how the strength of
the confining potential affects the spatial entanglement and how accurately the
methods that we introduced reproduce the exact trends. We also compare the
results with the outcomes of standard first-order perturbation methods. The
accuracies of energies and densities when using these methods are also
considered.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 23:41:09 GMT"
},
{
"version": "v2",
"created": "Mon, 31 Mar 2008 10:53:52 GMT"
},
{
"version": "v3",
"created": "Tue, 3 Aug 2010 10:02:23 GMT"
}
] | 2015-03-13T00:00:00 | [
[
"Coe",
"J. P.",
""
],
[
"Sudbery",
"A.",
""
],
[
"D'Amico",
"I.",
""
]
] | [
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712.382 | Bruno Nachtergaele | Bruno Nachtergaele, Hillel Raz, Benjamin Schlein, Robert Sims | Lieb-Robinson Bounds for Harmonic and Anharmonic Lattice Systems | null | Commun. Math. Phys. 286 (2009) 1073--1098 | 10.1007/s00220-008-0630-2 | null | math-ph cond-mat.stat-mech math.MP quant-ph | null | We prove Lieb-Robinson bounds for the dynamics of systems with an infinite
dimensional Hilbert space and generated by unbounded Hamiltonians. In
particular, we consider quantum harmonic and certain anharmonic lattice
systems.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 18:19:37 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 17:40:01 GMT"
}
] | 2009-02-03T00:00:00 | [
[
"Nachtergaele",
"Bruno",
""
],
[
"Raz",
"Hillel",
""
],
[
"Schlein",
"Benjamin",
""
],
[
"Sims",
"Robert",
""
]
] | [
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712.3821 | Hongbao Zhang | Song He and Hongbao Zhang | Covariant entropy conjecture and concordance cosmological models | 10 pages, 1 figure, JHEP style, references added, published version | JCAP0810:020,2008 | 10.1088/1475-7516/2008/10/020 | null | hep-th astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Recently a covariant entropy conjecture has been proposed for dynamical
horizons. We apply this conjecture to concordance cosmological models, namely,
those cosmological models filled with perfect fluids, in the presence of a
positive cosmological constant. As a result, we find this conjecture has a
severe constraint power. Not only does this conjecture rule out those
cosmological models disfavored by the anthropic principle, but also it imposes
an upper bound $10^{-60}$ on the cosmological constant for our own universe,
which thus provides an alternative macroscopic perspective for understanding
the long-standing cosmological constant problem.
| [
{
"version": "v1",
"created": "Mon, 24 Dec 2007 03:18:27 GMT"
},
{
"version": "v2",
"created": "Mon, 13 Oct 2008 14:57:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"He",
"Song",
""
],
[
"Zhang",
"Hongbao",
""
]
] | [
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] |
712.3822 | Kaspar von Braun | Kaspar von Braun (1), Gerard T. van Belle (1,2), David R. Ciardi (1),
Mercedes Lopez-Morales (3), D. W. Hoard (4), and Stefanie Wachter (4) ((1)
Michelson Science Center / Caltech, (2) ESO, (3) Carnegie Inst. of Washington
/ Dept. of Terrestrial Magnetism, (4) Spitzer Science Center / Caltech) | Spitzer 24-micron Time-Series Observations of the Eclipsing M-dwarf
Binary GU Bootis | ApJ accepted. 10 pages, 12 figures | null | 10.1086/529037 | null | astro-ph | null | We present a set of {\it Spitzer} 24$\mu$m MIPS time series observations of
the M-dwarf eclipsing binary star GU Bo\"otis. Our data cover three secondary
eclipses of the system: two consecutive events and an additional eclipse six
weeks later. The study's main purpose is the long wavelength (and thus limb
darkening-independent) characterization of GU Boo's light curve, allowing for
independent verification of the results of previous optical studies. Our
results confirm previously obtained system parameters. We further compare GU
Boo's measured 24$\mu$m flux density to the value predicted by spectral fitting
and find no evidence for circumstellar dust. In addition to GU Boo, we
characterize (and show examples of) light curves of other objects in the field
of view. Analysis of these light curves serves to characterize the photometric
stability and repeatability of {\it Spitzer's} MIPS 24\micron array over short
(days) and long (weeks) timescales at flux densities between approximately
300--2,000$\mu$Jy. We find that the light curve root mean square about the
median level falls into the 1--4% range for flux densities higher than 1mJy.
Finally, we comment on the fluctuations of the 24\micron background on short
and long timescales.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 00:12:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"von Braun",
"Kaspar",
""
],
[
"van Belle",
"Gerard T.",
""
],
[
"Ciardi",
"David R.",
""
],
[
"Lopez-Morales",
"Mercedes",
""
],
[
"Hoard",
"D. W.",
""
],
[
"Wachter",
"Stefanie",
""
]
] | [
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] |
712.3823 | Anthony Leverrier | Anthony Leverrier, Romain All\'eaume, Joseph Boutros, Gilles Z\'emor,
Philippe Grangier | Multidimensional reconciliation for continuous-variable quantum key
distribution | 8 pages, 3 figures | Phys. Rev. A 77, 042325 (2008) | 10.1103/PhysRevA.77.042325 | null | quant-ph cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We propose a method for extracting an errorless secret key in a
continuous-variable quantum key distribution protocol, which is based on
Gaussian modulation of coherent states and homodyne detection. The crucial
feature is an eight-dimensional reconciliation method, based on the algebraic
properties of octonions. Since the protocol does not use any postselection, it
can be proven secure against arbitrary collective attacks, by using
well-established theorems on the optimality of Gaussian attacks. By using this
new coding scheme with an appropriate signal to noise ratio, the distance for
secure continuous-variable quantum key distribution can be significantly
extended.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 00:41:54 GMT"
},
{
"version": "v2",
"created": "Thu, 3 Jul 2008 10:37:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Leverrier",
"Anthony",
""
],
[
"Alléaume",
"Romain",
""
],
[
"Boutros",
"Joseph",
""
],
[
"Zémor",
"Gilles",
""
],
[
"Grangier",
"Philippe",
""
]
] | [
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712.3824 | Diego Tonelli | Diego Tonelli (for the CDF and D0 Collaborations) | Prospects in CP violation measurements at the Tevatron Collider | This is an OLD conference proceeding prepared for the 18th Rencontres
de Physique de la Vallee d'Aoste - La Thuile in 2004. Already published and
posted to arxiv just for the record and to make it searchable with SPIRES. 20
pages, 12 figures | null | null | null | hep-ex | null | The Fermilab Tevatron Collider is currently the most copious source of
b-hadrons, thanks to the large b-bbar production cross-section in
1.96 TeV ppbar collisions. Recent detector upgrades allow for a wide range of
CP violation and flavor-mixing measurements that are fully competitive
(asymmetries in self-tagging modes) or complementary (asymmetries of B_s and
b-baryons decays) with B-factories. In this paper we review some recent CP
violation results from the DO and CDF Collaborations and we discuss the
prospects for future measurements.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 00:46:05 GMT"
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] | 2019-08-14T00:00:00 | [
[
"Tonelli",
"Diego",
"",
"for the CDF and D0 Collaborations"
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712.3825 | Marcus Hutter | Shane Legg and Marcus Hutter | Tests of Machine Intelligence | 12 pages; 1 table. Turing test and derivatives; Compression tests;
Linguistic complexity; Multiple cognitive abilities; Competitive games;
Psychometric tests; Smith's test; C-test; Universal intelligence | 50 Years of Artificial Intelligence (2007) pages 232-242 | null | IDSIA-11-07 | cs.AI | null | Although the definition and measurement of intelligence is clearly of
fundamental importance to the field of artificial intelligence, no general
survey of definitions and tests of machine intelligence exists. Indeed few
researchers are even aware of alternatives to the Turing test and its many
derivatives. In this paper we fill this gap by providing a short survey of the
many tests of machine intelligence that have been proposed.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 01:17:24 GMT"
}
] | 2008-06-26T00:00:00 | [
[
"Legg",
"Shane",
""
],
[
"Hutter",
"Marcus",
""
]
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712.3826 | Paulo C. Freire | Paulo C. C. Freire, Alex Wolszczan, Maureen van den Berg and Jason W.
T. Hessels | A Massive Neutron Star in the Globular Cluster M5 | 10 pages in ApJ emulate format, 2 tables, 6 figures. Added February
2008 data, slightly revised mass limits. Accepted for publication in ApJ | null | 10.1086/587832 | null | astro-ph | null | We report the results of 19 years of Arecibo timing for two pulsars in the
globular cluster NGC 5904 (M5), PSR B1516+02A (M5A) and PSR B1516+02B (M5B).
This has resulted in the measurement of the proper motions of these pulsars
and, by extension, that of the cluster itself. M5B is a 7.95-ms pulsar in a
binary system with a > 0.13 solar mass companion and an orbital period of 6.86
days. In deep HST images, no optical counterpart is detected within ~2.5 sigma
of the position of the pulsar, implying that the companion is either a white
dwarf or a low-mass main-sequence star. The eccentricity of the orbit (e =
0.14) has allowed a measurement of the rate of advance of periastron: (0.0142
+/-0.0007) degrees per year. We argue that it is very likely that this
periastron advance is due to the effects of general relativity, the total mass
of the binary system then being 2.29 +/-0.17 solar masses. The small measured
mass function implies, in a statistical sense, that a very large fraction of
this total mass is contained in the pulsar: 2.08 +/- 0.19 solar masses (1
sigma); there is a 5% probability that the mass of this object is < 1.72 solar
masses and a 0.77% probability that is is between 1.2 and 1.44 solar masses.
Confirmation of the median mass for this neutron star would exclude most
``soft'' equations of state for dense neutron matter. Millisecond pulsars
(MSPs) appear to have a much wider mass distribution than is found in double
neutron star systems; about half of these objects are significantly more
massive than 1.44 solar masses. A possible cause is the much longer episode of
mass accretion necessary to recycle a MSP, which in some cases corresponds to a
much larger mass transfer.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 14:31:25 GMT"
},
{
"version": "v2",
"created": "Sun, 24 Feb 2008 20:48:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Freire",
"Paulo C. C.",
""
],
[
"Wolszczan",
"Alex",
""
],
[
"Berg",
"Maureen van den",
""
],
[
"Hessels",
"Jason W. T.",
""
]
] | [
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] |
712.3827 | Manu Punnen John | Manu. P. John and V. M. Nandakumaran | Chaos in an intermittently driven damped oscillator | 13 pages LaTex, added references, corrected typos | null | null | null | nlin.CD | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We observe chaotic dynamics in a damped linear oscillator, which is driven
only at certain regions of phase space. Both deterministic and random drives
are studied. The dynamics is characterized using standard techniques of
nonlinear dynamics. Interchanging roles of determinism and stochasticity is
also considered.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 04:03:22 GMT"
},
{
"version": "v2",
"created": "Fri, 5 Sep 2008 14:23:16 GMT"
}
] | 2008-09-05T00:00:00 | [
[
"John",
"Manu. P.",
""
],
[
"Nandakumaran",
"V. M.",
""
]
] | [
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] |
712.3828 | Mikhail Olshanetsky | A.Levin, M.Olshanetsky | Lie Algebroids and generalized projective structures on Riemann surfaces | 36 pages,AMS-LaTeX 1.2, Essentially revised and elaborated version of
hep-th/0010043 | null | null | ITEP-TH-07/80; ESI-1989 | math.QA | null | The space of generalized projective structures on a Riemann surface $\Sigma$
of genus g with n marked points is the affine space over the cotangent bundle
to the space of SL(N)-opers. It is a phase space of $W_N$-gravity on
$\Sigma\times\mathbb{R}$.
This space is a generalization of the space of projective structures on the
Riemann surface. We define the moduli space of $W_N$-gravity as a symplectic
quotient with respect to the canonical action of a special class of Lie
algebroids. This moduli space describes in particular the moduli space of
deformations of complex structures on the Riemann surface by differential
operators of finite order, or equivalently, by a quotient space of Volterra
operators. We call these algebroids the Adler-Gelfand-Dikii (AGD) algebroids,
because they are constructed by means of AGD bivector on the space of opers
restricted on a circle. The AGD-algebroids are particular case of Lie
algebroids related to a Poisson sigma-model. The moduli space of the
generalized projective structure can be described by cohomology of a
BRST-complex.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 15:23:38 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Levin",
"A.",
""
],
[
"Olshanetsky",
"M.",
""
]
] | [
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] |
712.3829 | Francois Le Gall | Yoshifumi Inui and Francois Le Gall | Quantum Property Testing of Group Solvability | 11 pages; supersedes arXiv:quant-ph/0610013 | Algorithmica 59(1): 35-47 (2011) | 10.1007/s00453-009-9338-8 | null | quant-ph cs.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Testing efficiently whether a finite set with a binary operation over it,
given as an oracle, is a group is a well-known open problem in the field of
property testing. Recently, Friedl, Ivanyos and Santha have made a significant
step in the direction of solving this problem by showing that it it possible to
test efficiently whether the input is an Abelian group or is far, with respect
to some distance, from any Abelian group. In this paper, we make a step further
and construct an efficient quantum algorithm that tests whether the input is a
solvable group, or is far from any solvable group. More precisely, the number
of queries used by our algorithm is polylogarithmic in the size of the set.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 04:47:03 GMT"
},
{
"version": "v2",
"created": "Sun, 3 Jan 2010 08:29:30 GMT"
}
] | 2021-10-05T00:00:00 | [
[
"Inui",
"Yoshifumi",
""
],
[
"Gall",
"Francois Le",
""
]
] | [
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] |
712.383 | Tom Schrijvers | Tom Schrijvers, Bart Demoen, David S. Warren | TCHR: a framework for tabled CLP | Accepted for publication in Theory and Practice of Logic Programming | null | null | null | cs.PL | null | Tabled Constraint Logic Programming is a powerful execution mechanism for
dealing with Constraint Logic Programming without worrying about fixpoint
computation. Various applications, e.g in the fields of program analysis and
model checking, have been proposed. Unfortunately, a high-level system for
developing new applications is lacking, and programmers are forced to resort to
complicated ad hoc solutions.
This papers presents TCHR, a high-level framework for tabled Constraint Logic
Programming. It integrates in a light-weight manner Constraint Handling Rules
(CHR), a high-level language for constraint solvers, with tabled Logic
Programming. The framework is easily instantiated with new application-specific
constraint domains. Various high-level operations can be instantiated to
control performance. In particular, we propose a novel, generalized technique
for compacting answer sets.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 15:28:16 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Schrijvers",
"Tom",
""
],
[
"Demoen",
"Bart",
""
],
[
"Warren",
"David S.",
""
]
] | [
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] |
712.3831 | Dawei Ding | Dawei Ding, Jie Zhu, Xiaoshu Luo, Yuliang Liu | Hopf bifurcation analysis in a dual model of Internet congestion control
algorithm with communication delay | 18 pages, 6 figures | null | null | null | cs.NI | null | This paper focuses on the delay induced Hopf bifurcation in a dual model of
Internet congestion control algorithms which can be modeled as a time-delay
system described by a one-order delay differential equation (DDE). By choosing
communication delay as the bifurcation parameter, we demonstrate that the
system loses its stability and a Hopf bifurcation occurs when communication
delay passes through a critical value. Moreover, the bifurcating periodic
solution of system is calculated by means of perturbation methods. Discussion
of stability of the periodic solutions involves the computation of Floquet
exponents by considering the corresponding Poincare -Lindstedt series
expansion. Finally, numerical simulations for verify the theoretical analysis
are provided.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 06:16:26 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Ding",
"Dawei",
""
],
[
"Zhu",
"Jie",
""
],
[
"Luo",
"Xiaoshu",
""
],
[
"Liu",
"Yuliang",
""
]
] | [
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] |
712.3832 | Yang Zhao | S. R. Dunsiger, Y. Zhao, B. D. Gaulin, Y. Qiu, P. Bourges, Y. Sidis,
J. R. D. Copley, A. B. Kallin, E. M. Mazurek, and H.A. Dabkowska | Diagonal and Collinear Incommensurate Spin Structures in underdoped
La$_{2-x}$Ba$_{x}$CuO$_{4}$ | 5 pages, 4 figures, submitted to PRL | null | 10.1103/PhysRevB.78.092507 | null | cond-mat.str-el cond-mat.supr-con | null | We have studied incommensurate spin ordering in single crystal underdoped
La_{2-x}Ba_{x}CuO_{4} with x~0.08, 0.05 and 0.025 using neutron scattering
techniques. Static incommensurate magnetic order is observed in the
La_{2-x}Ba_{x}CuO_{4} (x=0.05 and 0.025) compounds with ordering wavevectors
which are rotated by 45 degree about the commensurate (0.5,0.5,0) position,
with respect to that in the superconducting x=0.08 material. These spin
modulations are one dimensional in the x=0.05 and 0.025 samples, with ordering
wavevectors lying along the orthorhombic b* direction. Such a rotation in the
orientation of the static spin ordering as a function of increasing Ba doping,
from diagonal to collinear, is roughly coincident with the transition from an
insulating to a superconducting ground state and is similar to that observed in
the related La_{2-x}Sr_{x}CuO_{4} system. This phenomenon is therefore a
generic property of underdoped La-214 cuprates.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 07:19:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dunsiger",
"S. R.",
""
],
[
"Zhao",
"Y.",
""
],
[
"Gaulin",
"B. D.",
""
],
[
"Qiu",
"Y.",
""
],
[
"Bourges",
"P.",
""
],
[
"Sidis",
"Y.",
""
],
[
"Copley",
"J. R. D.",
""
],
[
"Kallin",
"A. B.",
""
],
[
"Mazurek",
"E. M.",
""
],
[
"Dabkowska",
"H. A.",
""
]
] | [
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] |
712.3833 | John Hartnett | John G. Hartnett | Unknown selection effect simulates redshift periodicity in quasar number
counts from Sloan Digital Sky Survey | 5 pages, 6 figures, major revision | Astrophys.Space Sci.324:13-16, 2009 | 10.1007/s10509-008-9906-4 | null | astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Discrete Fourier analysis on the quasar number count, as a function of
redshift, $z$, calculated from the Sloan Digital Sky Survey DR6 release appears
to indicate that quasars have preferred periodic redshifts with redshift
intervals of 0.258, 0.312, 0.44, 0.63, and 1.1. However the same periods are
found in the mean of the $zConf$ parameter used to flag the reliability of the
spectroscopic measurements. It follows that these redshift periods must result
from some selection effect, as yet undetermined. It does not signal any
intrinsic (quantized) redshifts in the quasars.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 07:17:03 GMT"
},
{
"version": "v2",
"created": "Fri, 8 Feb 2008 00:52:42 GMT"
},
{
"version": "v3",
"created": "Fri, 10 Jul 2009 06:52:29 GMT"
}
] | 2010-04-14T00:00:00 | [
[
"Hartnett",
"John G.",
""
]
] | [
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712.3834 | Olivier Fruchart | Fabien Cheynis (NEEL), Aur\'elien Masseboeuf (SP2M), Olivier Fruchart
(NEEL), Nicolas Rougemaille (NEEL), Jean-Christophe Toussaint (NEEL,
SPINTEC), Rachid Belkhou, Pascale Bayle-Guillemaud (SP2M, INAC), Alain Marty
(SP2M, INAC, NM) | Controlled switching of N\'eel caps in flux-closure magnetic dots | 4 pages, 3 figures | Physical Review Letters 102, 10 (2009) 107201 | 10.1103/PhysRevLett.102.107201 | null | cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | While magnetic hysteresis usually considers magnetic domains, the switching
of the core of magnetic vortices has recently become an active topic. We
considered Bloch domain walls, which are known to display at the surface of
thin films flux-closure features called N\'eel caps. We demonstrated the
controlled switching of these caps under a magnetic field, occurring via the
propagation of a surface vortex. For this we considered flux-closure states in
elongated micron-sized dots, so that only the central domain wall can be
addressed, while domains remain unaffected.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 07:36:27 GMT"
},
{
"version": "v2",
"created": "Thu, 29 May 2008 06:48:12 GMT"
},
{
"version": "v3",
"created": "Fri, 6 Mar 2009 07:54:31 GMT"
}
] | 2009-03-12T00:00:00 | [
[
"Cheynis",
"Fabien",
"",
"NEEL"
],
[
"Masseboeuf",
"Aurélien",
"",
"SP2M"
],
[
"Fruchart",
"Olivier",
"",
"NEEL"
],
[
"Rougemaille",
"Nicolas",
"",
"NEEL"
],
[
"Toussaint",
"Jean-Christophe",
"",
"NEEL,\n SPINTEC"
],
[
"Belkhou",
"Rachid",
"",
"SP2M, INAC"
],
[
"Bayle-Guillemaud",
"Pascale",
"",
"SP2M, INAC"
],
[
"Marty",
"Alain",
"",
"SP2M, INAC, NM"
]
] | [
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712.3835 | Noam Soker | Noam Soker (Technion, Israel) | Defining the Termination of the Asymptotic Giant Branch | Submitted to ApJ Letters | null | 10.1086/528987 | null | astro-ph | null | I suggest a theoretical quantitative definition for the termination of the
asymptotic giant branch (AGB) phase and the beginning of the post-AGB phase. I
suggest that the transition will be taken to occur when the ratio of the
dynamical time scale to the the envelope thermal time scale, Q, reaches its
maximum value. Time average values are used for the different quantities, as
the criterion does not refer to the short time-scale variations occurring on
the AGB and post-AGB, e.g., thermal pulses (helium shell flashes) and magnetic
activity. Along the entire AGB the value of Q increases, even when the star
starts to contract. Only when a rapid contraction starts does the value of Q
start to decrease. This criterion captures the essence of the transition from
the AGB to the post AGB phase, because Q is connected to the stellar effective
temperature, reaching its maximum value at T~4000-6000 K, it is related to the
mass loss properties, and it reaches its maximum value when rapid contraction
starts and envelope mass is very low.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 07:41:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Soker",
"Noam",
"",
"Technion, Israel"
]
] | [
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712.3836 | Jean Fromentin | Jean Fromentin (LMNO) | The well-ordering of dual braid monoids | null | null | null | null | math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We describe the restriction of the Dehornoy ordering of braids to the dual
braid monoids introduced by Birman, Ko and Lee: we give an inductive
characterization of the ordering of the dual braid monoids and compute the
corresponding ordinal type. The proof consists in introducing a new ordering on
the dual braid monoid using the rotating normal form of arXiv:0811.3902
[math.GR], and then proving that this new ordering coincides with the standard
ordering of braids.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 07:42:20 GMT"
},
{
"version": "v2",
"created": "Wed, 10 Dec 2008 09:19:57 GMT"
}
] | 2008-12-10T00:00:00 | [
[
"Fromentin",
"Jean",
"",
"LMNO"
]
] | [
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] |
712.3837 | Ciprian Tudor | Xavier Bardina, Maria Jolis, Ciprian Tudor (CES, SAMOS) | On the convergence to the multiple Wiener-Ito integral | null | null | null | null | math.PR | null | We study the convergence to the multiple Wiener-It\^{o} integral from
processes with absolutely continuous paths. More precisely, consider a family
of processes, with paths in the Cameron-Martin space, that converges weakly to
a standard Brownian motion in $\mathcal C_0([0,T])$. Using these processes, we
construct a family that converges weakly, in the sense of the finite
dimensional distributions, to the multiple Wiener-It\^{o} integral process of a
function $f\in L^2([0,T]^n)$. We prove also the weak convergence in the space
$\mathcal C_0([0,T])$ to the second order integral for two important families
of processes that converge to a standard Brownian motion.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 07:52:19 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Bardina",
"Xavier",
"",
"CES, SAMOS"
],
[
"Jolis",
"Maria",
"",
"CES, SAMOS"
],
[
"Tudor",
"Ciprian",
"",
"CES, SAMOS"
]
] | [
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] |
712.3838 | Peter Collas | David Klein and Peter Collas | General Transformation Formulas for Fermi-Walker Coordinates | 23 pages. Corrected typos in the last two equations. Accepted for
publication in Classical and Quantum Gravity | Class.Quant.Grav.25:145019,2008 | 10.1088/0264-9381/25/14/145019 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We calculate the transformation and inverse transformation, in the form of
Taylor expansions, from arbitrary coordinates to Fermi-Walker coordinates in
tubular neighborhoods of arbitrary timelike paths for general spacetimes.
Explicit formulas for coefficients and the Jacobian matrix are given.
| [
{
"version": "v1",
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},
{
"version": "v2",
"created": "Mon, 3 Mar 2008 05:10:23 GMT"
},
{
"version": "v3",
"created": "Sat, 31 May 2008 23:35:56 GMT"
},
{
"version": "v4",
"created": "Fri, 27 Jun 2008 07:40:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Klein",
"David",
""
],
[
"Collas",
"Peter",
""
]
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712.3839 | Koji Miwa | K. Miwa, S. Dairaku, D. Nakajima (for the KEK-PS E559 Collaboration) | Search for Theta+ via K+p -> pi+X reaction with a 1.2 GeV/c K+ beam | 11pages, 13figures | Phys.Rev.C77:045203,2008 | 10.1103/PhysRevC.77.045203 | null | nucl-ex | null | The Theta+ was searched for via the K+p -> pi+X reaction using the 1.2 GeV/c
K+ beam at the K6 beam line of the KEK-PS 12 GeV Proton Synchrotron. In the
missing mass spectrum of the K+p -> pi+X reaction, no clear peak structure was
observed. Therefore a 90 % C.L. upper limit of 3.5 ub/sr was derived for the
differential cross section averaged over 2degree to 22degree in the laboratory
frame of the K+p -> pi+Theta+ reaction. This upper limit is much smaller than
the theoretical calculation for the t-channel process where a K0* is exchanged.
From the present result, either the t-channel process is excluded or the
coupling constant of g_{K*N\Theta} is quite small.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 08:46:35 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 02:19:11 GMT"
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{
"version": "v3",
"created": "Sun, 17 Feb 2008 03:50:12 GMT"
},
{
"version": "v4",
"created": "Sun, 9 Mar 2008 04:51:03 GMT"
}
] | 2019-08-14T00:00:00 | [
[
"Miwa",
"K.",
"",
"for the KEK-PS E559 Collaboration"
],
[
"Dairaku",
"S.",
"",
"for the KEK-PS E559 Collaboration"
],
[
"Nakajima",
"D.",
"",
"for the KEK-PS E559 Collaboration"
]
] | [
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712.384 | Giovanni Alessandrini | Giovanni Alessandrini, Vincenzo Nesi | Invertible harmonic mappings, beyond Kneser | One section added. 15 pages | Ann. Scuola Norm. Sup. Pisa, Cl. Sci. (5) VIII (2009), 451-468 | 10.2422/2036-2145.2009.3.03 | null | math.AP | null | We prove necessary and sufficient criteria of invertibility for planar
harmonic mappings which generalize a classical result of H. Kneser, also known
as the Rad\'{o}-Kneser-Choquet theorem.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 08:39:15 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 08:03:09 GMT"
}
] | 2010-11-09T00:00:00 | [
[
"Alessandrini",
"Giovanni",
""
],
[
"Nesi",
"Vincenzo",
""
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] |
712.3841 | Barbara Sciascia | KLOE Collaboration | Measurement of the absolute branching ratios for semileptonic K+/-
decays with the KLOE detector | 13 pages, 3 figures, submitted to JHEP. v2: minor revisions required
by JHEP, v3: final version published by JHEP (replacement of 2 incorrect
affiliations)link: http://www.iop.org/EJ/abstract/1029-8479/2008/02/098 | JHEP 0802:098,2008 | 10.1088/1126-6708/2008/02/098 | null | hep-ex | null | Using a sample of over 600 million phi->K+K- decays collected at the Dafne
e+e- collider, we have measured with the KLOE detector the absolute branching
ratios for the charged kaon semileptonic decays, K+/- -> p0 e nu (gamma) (Ke3)
and K+/- -> p0 mu nu (gamma) (Kmu3). The results, BR(Ke3) = 0.04965 +/-
0.00038_{stat} +/- 0.00037_{syst} and BR(Kmu3) = 0.03233 +/- 0.00029_{stat} +/-
0.00026_{syst}, are inclusive of radiation. Accounting for correlations, we
derive the ratio Kmu3/Ke3 = 0.6511+/-0.0064. Using the semileptonic form
factors measured in the same experiment, we obtain V_{us}f_{+}(0) = 0.2141 +/-
0.0013.
| [
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"created": "Sat, 22 Dec 2007 08:48:22 GMT"
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"version": "v2",
"created": "Fri, 15 Feb 2008 11:46:14 GMT"
},
{
"version": "v3",
"created": "Thu, 28 Feb 2008 13:26:10 GMT"
}
] | 2012-08-27T00:00:00 | [
[
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"",
""
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712.3842 | Murilo Baptista S. | D. M. Maranh\~ao, M. S. Baptista, J. C. Sartorelli, I. L. Caldas | Experimental observation of a complex periodic window | 4.2 pages, 4 figures | Phys. Rev. E (2008) | 10.1103/PhysRevE.77.037202 | null | nlin.CD | null | The existence of a special periodic window in the two-dimensional parameter
space of an experimental Chua's circuit is reported. One of the main reasons
that makes such a window special is that the observation of one implies that
other similar periodic windows must exist for other parameter values. However,
such a window has never been experimentally observed, since its size in
parameter space decreases exponentially with the period of the periodic
attractor. This property imposes clear limitations for its experimental
detection.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 09:01:29 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Mar 2008 08:47:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Maranhão",
"D. M.",
""
],
[
"Baptista",
"M. S.",
""
],
[
"Sartorelli",
"J. C.",
""
],
[
"Caldas",
"I. L.",
""
]
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712.3843 | Zakaria Giunashvili | Zakaria Giunashvili | Cyclic Evolution on Grassmann Manifold and Berry Phase | 4 pages | null | null | null | quant-ph | null | For a given $k$-dimensional subspace $V_0$ in a Hilbert space $\hilb$ and a
unitary transformation $g_0:V_0\To V_0$, we find a path in the Grassmann
manifold the monodromy of which coincides with $g_0$.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 09:05:54 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Giunashvili",
"Zakaria",
""
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] |
712.3844 | Chushun Tian | Chushun Tian | Supersymmetric field theory of local light diffusion in semi-infinite
media | 14 pages, 1 figure. accepted for publication in Phys. Rev. B | null | 10.1103/PhysRevB.77.064205 | null | cond-mat.dis-nn cond-mat.mes-hall | null | A supersymmetric field theory of light diffusion in semi-infinite disordered
media is presented. With the help of this technique we justify--at the
perturbative level--the local light diffusion proposed by Tiggelen, Lagendijk,
and Wiersma [Phys. Rev. Lett. \textbf{84}, 4333 (2000)], and show that the
coherent backscattering line shape of medium bar displays a crossover from
two-dimensional weak to quasi-one-dimensional strong localization.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 09:15:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tian",
"Chushun",
""
]
] | [
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712.3845 | Yuri Shchekinov A. | V. Prudskikh, Yu. A. Shchekinov | Acceleration of dust particles by low-frequency Alfv\'en waves | 8 pages, no figs, accepted in Phys. Lett. A | null | 10.1016/j.physleta.2007.12.061 | null | physics.plasm-ph astro-ph | null | We investigate the efficiency of acceleration of charged dust particles by
low-frequency Alfv\'en waves in nonlinear approximation. We show that the
longitudinal acceleration of dust particles is proportional to the square of
the soliton amplitude $O(|b_m|^2)$, while the transversal acceleration is of
$O(|b_m|)$. In the conditions of the interstellar medium the resulting velocity
of dust particles can reach 0.3 to 1 km s$^{-1}$.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 10:03:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Prudskikh",
"V.",
""
],
[
"Shchekinov",
"Yu. A.",
""
]
] | [
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] |
712.3846 | Piotr T. Chru\'sciel | Piotr T. Chru\'sciel and Paul Tod | On Mason's rigidity theorem | minor typos corrected | Commun.Math.Phys.285:1-29,2009 | 10.1007/s00220-008-0643-x | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Following an argument proposed by Mason, we prove that there are no
algebraically special asymptotically simple vacuum space-times with a smooth,
shear-free, geodesic congruence of principal null directions extending
transversally to a cross-section of Scri. Our analysis leaves the door open for
escaping this conclusion if the congruence is not smooth, or not transverse to
Scri. One of the elements of the proof is a new rigidity theorem for the
Trautman-Bondi mass.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 10:43:39 GMT"
},
{
"version": "v2",
"created": "Sat, 4 Oct 2008 08:36:00 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Chruściel",
"Piotr T.",
""
],
[
"Tod",
"Paul",
""
]
] | [
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] |
712.3847 | Pierre van Moerbeke | Pierre van Moerbeke | Random and Integrable Models in Mathematics and Physics | Lectures (163 pages) at Montreal, CRM Short Program on Random
Matrices, Random Processes and Integrable Systems, June 20 - July 8, 2005 | null | null | null | math.PR math-ph math.MP | null | This set of Montreal lectures is an elementary and sketchy introduction to
the general field of random matrices. The first half is devoted to
combinatorial models, whereas the second half deals with random matrix
questions(GUE, etc...).
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 10:47:57 GMT"
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] | 2007-12-27T00:00:00 | [
[
"van Moerbeke",
"Pierre",
""
]
] | [
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] |
712.3848 | Emil Johansson Bergholtz | E.J. Bergholtz, T.H. Hansson, M. Hermanns, A. Karlhede, and S. Viefers | Hierarchy wave functions--from conformal correlators to Tao-Thouless
states | 9 pages | Phys. Rev. B 77, 165325 (2008) | 10.1103/PhysRevB.77.165325 | null | cond-mat.mes-hall cond-mat.str-el | null | Laughlin's wave functions, describing the fractional quantum Hall effect at
filling factors $\nu=1/(2k+1)$, can be obtained as correlation functions in
conformal field theory, and recently this construction was extended to Jain's
composite fermion wave functions at filling factors $\nu=n/(2kn+1)$. Here we
generalize this latter construction and present ground state wave functions for
all quantum Hall hierarchy states that are obtained by successive condensation
of quasielectrons (as opposed to quasiholes) in the original hierarchy
construction. By considering these wave functions on a cylinder, we show that
they approach the exact ground states, the Tao-Thouless states, when the
cylinder becomes thin. We also present wave functions for the multi-hole
states, make the connection to Wen's general classification of abelian quantum
Hall fluids, and discuss whether the fractional statistics of the
quasiparticles can be analytically determined. Finally we discuss to what
extent our wave functions can be described in the language of composite
fermions.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 11:11:00 GMT"
}
] | 2008-12-22T00:00:00 | [
[
"Bergholtz",
"E. J.",
""
],
[
"Hansson",
"T. H.",
""
],
[
"Hermanns",
"M.",
""
],
[
"Karlhede",
"A.",
""
],
[
"Viefers",
"S.",
""
]
] | [
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712.3849 | Sandor Varro | Sandor Varro | Entangled Photon-Electron States and the Number-Phase Minimum
Uncertainty States of the Photon Field | 31 pages, 6 figures | New Journal of Physics, Vol. 10, 053028 (35pp) (2008) | 10.1088/1367-2630/10/5/053028 | null | quant-ph | null | The exact analytic solutions of the energy eigenvalue equation of the system
consisting of a free electron and one mode of the quantized radiation field are
used for studying the physical meaning of a class of number-phase minimum
uncertainty states. The states of the mode which minimize the uncertainty
product of the photon number and the Susskind and Glogower (1964) cosine
operator have been obtained by Jackiw (1968). However, these states have so far
been remained mere mathematical constructions without any physical
significance. It is proved that the most fundamental interaction in quantum
electrodynamics - namely the interaction of a free electron with a mode of the
quantized radiation field - leads quite naturally to the generation of the
mentioned minimum uncertainty states. It is shown that from the entangled
photon-electron states developing from a highly excited number state, due to
the interaction with a Gaussian electronic wave packet, the minimum uncertainty
states of Jackiw's type can be constructed. In the electron's coordinate
representation the physical meaning of the expansion coefficients of these
states are the joint probability amplitudes of simultaneous detection of an
electron and of a definite number of photons. The joint occupation
probabilities in these states preserve their functional form as time elapses,
but they vary from point to point in space-time, depending on the location of
the detected electron. An analysis of the entanglement entropies derived from
the photon number distribution and from the electron's density operator is
given.
| [
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"version": "v1",
"created": "Sat, 22 Dec 2007 11:36:04 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Apr 2008 13:45:28 GMT"
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] | 2009-03-02T00:00:00 | [
[
"Varro",
"Sandor",
""
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] |
712.385 | Alfred J van der Poorten AM | Alf van der Poorten | Fermat's Four Squares Theorem | 3 pqges | null | null | ALF'S PREPRINTS 183 | math.NT math.HO | null | It is easy to find a right-angled triangle with integer sides whose area is
6. There is no such triangle with area 5, but there is one with rational sides
(a `\emph{Pythagorean triangle}').
For historical reasons, integers such as 6 or 5 that are (the squarefree part
of) the area of some Pythagorean triangle are called `\emph{congruent
numbers}'. These numbers actually are interesting for the following reason:
Notice the sequence $\frac14$, $6\frac14$, $12\frac14$. It is an arithmetic
progression with common difference 6, consisting of squares $(\frac12)^2$,
$(\frac52)^2$, $(\frac72)^2$ of rational numbers. Indeed the common difference
of three rational squares in AP is a congruent number and every congruent
number is the common difference of three rational squares in arithmetic
progression.
The triangle given by $9^{2}+40^{2}=41^{2}$ has area $180=5\cdot6^{2}$ and
the numbers $x-5$, $x$ and $x+5$ all are rational squares if $x=11{97/144}$.
Recall one obtains all Pythagorean triangles with relatively prime integer
sides by taking $x=4uv$, $y=\pm(4u^{2}-v^{2})$, $z=4u^{2}+v^{2}$ where $u$ and
$v$ are integers with $2u$ and $v$ relatively prime.
Fermat proved that there is no AP of more than three squares of rationals.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 11:39:43 GMT"
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] | 2007-12-27T00:00:00 | [
[
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"Alf",
""
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712.3851 | Emil Lundh | A. Cetoli, E. Lundh | Nonlinear behavior of bosons in anisotropic optical lattices | 5 pages, 4 figures, discussion revised after referee comments | null | null | null | cond-mat.other | null | We investigate the behavior of an array of Bose-Einstein condensate tubes
described by means of a Bose-Hubbard Hamiltonian. Using an anisotropic
non-polynomial Schrodinger equation we link the macroscopic parameters in the
Bose-Hubbard Hamiltonian to the ones that are tunable in experiments. Using a
mean field approach we predict that increasing the optical lattice strength
along the direction of the tubes, the condensate can experience a reentrant
transition between a Mott insulating phase and the superfluid one.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 11:58:59 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Feb 2008 12:17:13 GMT"
}
] | 2008-02-29T00:00:00 | [
[
"Cetoli",
"A.",
""
],
[
"Lundh",
"E.",
""
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712.3852 | Bernd Berg | Bernd A. Berg and Robert C. Harris | From Data to Probability Densities without Histograms | 9 pages, 9 figures | Comp. Phys. Commun. 179 (2008) 443-448 | 10.1016/j.cpc.2008.03.010 | null | physics.data-an cond-mat.stat-mech hep-lat physics.comp-ph | null | When one deals with data drawn from continuous variables, a histogram is
often inadequate to display their probability density. It deals inefficiently
with statistical noise, and binsizes are free parameters. In contrast to that,
the empirical cumulative distribution function (obtained after sorting the
data) is parameter free. But it is a step function, so that its differentiation
does not give a smooth probability density. Based on Fourier series expansion
and Kolmogorov tests, we introduce a simple method, which overcomes this
problem. Error bars on the estimated probability density are calculated using a
jackknife method. We give several examples and provide computer code
reproducing them. You may want to look at the corresponding figures 4 to 9
first.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 12:17:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Berg",
"Bernd A.",
""
],
[
"Harris",
"Robert C.",
""
]
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] |
712.3853 | Mattias Marklund | Vitaly Bychkov, Mattias Marklund and Mikhail Modestov | The Rayleigh-Taylor instability and internal waves in quantum plasmas | 9 pages, 2 figures | null | 10.1016/j.physleta.2007.12.065 | null | physics.flu-dyn | null | Influence of quantum effects on the internal waves and the Rayleigh-Taylor
instability in plasma is investigated. It is shown that quantum pressure always
stabilizes the RT instability. The problem is solved both in the limit of
short-wavelength perturbations and exactly for density profiles with layers of
exponential stratification. In the case of stable stratification, quantum
pressure modifies the dispersion relation of the inertial waves. Because of the
quantum effects, the internal waves may propagate in the transverse direction,
which was impossible in the classical case. A specific form of pure quantum
internal waves is obtained, which do not require any external gravitational
field.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 12:21:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bychkov",
"Vitaly",
""
],
[
"Marklund",
"Mattias",
""
],
[
"Modestov",
"Mikhail",
""
]
] | [
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] |
712.3854 | Juan Mart\'inez-Sykora | Juan Mart\'inez-Sykora, Viggo Hansteen, Mats Carlsson (Institute of
Theoretical Astrophysics, University of Oslo) | Twisted flux tube emergence from the convection zone to the corona | 53 pages,79 figures, Submitted to ApJ | null | 10.1086/587028 | null | astro-ph | null | 3D numerical simulations of a horizontal magnetic flux tube emergence with
different twist are carried out in a computational domain spanning the upper
layers of the convection zone to the lower corona. We use the Oslo Staggered
Code to solve the full MHD equations with non-grey and non-LTE radiative
transfer and thermal conduction along the magnetic field lines. The emergence
of the magnetic flux tube input at the bottom boundary into a weakly magnetized
atmosphere is presented. The photospheric and chromospheric response is
described with magnetograms, synthetic images and velocity field distributions.
The emergence of a magnetic flux tube into such an atmosphere results in varied
atmospheric responses. In the photosphere the granular size increases when the
flux tube approaches from below. In the convective overshoot region some 200km
above the photosphere adiabatic expansion produces cooling, darker regions with
the structure of granulation cells. We also find collapsed granulation in the
boundaries of the rising flux tube. Once the flux tube has crossed the
photosphere, bright points related with concentrated magnetic field, vorticity,
high vertical velocities and heating by compressed material are found at
heights up to 500km above the photosphere. At greater heights in the magnetized
chromosphere, the rising flux tube produces a cool, magnetized bubble that
tends to expel the usual chromospheric oscillations. In addition the rising
flux tube dramatically increases the chromospheric scale height, pushing the
transition region and corona aside such that the chromosphere extends up to 6Mm
above the photosphere. The emergence of magnetic flux tubes through the
photosphere to the lower corona is a relatively slow process, taking of order 1
hour.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 12:25:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Martínez-Sykora",
"Juan",
"",
"Institute of\n Theoretical Astrophysics, University of Oslo"
],
[
"Hansteen",
"Viggo",
"",
"Institute of\n Theoretical Astrophysics, University of Oslo"
],
[
"Carlsson",
"Mats",
"",
"Institute of\n Theoretical Astrophysics, University of Oslo"
]
] | [
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] |
712.3855 | Elisa Di Carlo | E. Di Carlo (1), C. Corsi (2), A. A. Arkharov (3), F. Massi (4), V. M.
Larionov (3 and 5), N. V. Efimova (3), M. Dolci (1), N. Napoleone (2) and A.
Di Paola (2) ((1) INAF - Osservatorio Astronomico Collurania di Teramo -
Italy, (2) INAF - Osservatorio Astronomico di Roma - Italy, (3) Central
Astronomical Observatory at Pulkovo - Russia, (4) INAF - Osservatorio
Astrofisico di Arcetri - Italy, (5) Astronomical Institute of St. Petersburg
University - Russia) | Near-Infrared observations of the type Ib Supernova SN2006jc: evidence
of interactions with dust | 22 pages, 5 figures, submitted to ApJ | null | 10.1086/590051 | null | astro-ph | null | In the framework of a program for the monitoring of Supernovae in the
Near-Infrared (NIR) carried out by the Teramo, Rome and Pulkovo observatories
with the AZT-24 telescope, we observed the Supernova SN2006jc in the J,H,K
photometric bands during a period of 7 months, starting ~36 days after its
discovery. Our observations evidence a NIR re-brightening, peaking ~70 days
after discovery, along with a reddening of H-K and J-H colors until 120 days
from discovery. After that date, J-H seems to evolve towards bluer colors. Our
data, complemented by IR, optical, UV and X-ray observations found in the
literature, show that the re-brightening is produced by hot dust surrounding
the supernova, formed in the interaction of the ejecta with dense circumstellar
matter.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 12:36:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Di Carlo",
"E.",
"",
"3 and 5"
],
[
"Corsi",
"C.",
"",
"3 and 5"
],
[
"Arkharov",
"A. A.",
"",
"3 and 5"
],
[
"Massi",
"F.",
"",
"3 and 5"
],
[
"Larionov",
"V. M.",
"",
"3 and 5"
],
[
"Efimova",
"N. V.",
""
],
[
"Dolci",
"M.",
""
],
[
"Napoleone",
"N.",
""
],
[
"Di Paola",
"A.",
""
]
] | [
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] |
712.3856 | Matti Vuorinen | G. D. Anderson, M. K. Vamanamurthy, and M. Vuorinen | Topics in Special Functions | 22 pages | null | null | Report 83, Univ. Jyv\"askyl\"a (2001), 5-26, ISBN 951-39-1120-9 | math.CA math.CV | null | The authors survey recent results in special functions, particularly the
gamma function and the Gaussian hypergeometric function.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 13:08:28 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Anderson",
"G. D.",
""
],
[
"Vamanamurthy",
"M. K.",
""
],
[
"Vuorinen",
"M.",
""
]
] | [
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] |
712.3857 | Gr\'egory Ginot | Kai Behrend, Gr\'egory Ginot, Behrang Noohi, Ping Xu | String topology for stacks | extended version, 152 pages | null | null | null | math.AT hep-th math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We establish the general machinery of string topology for differentiable
stacks. This machinery allows us to treat on an equal footing free loops in
stacks and hidden loops. In particular, we give a good notion of a free loop
stack, and of a mapping stack $\map(Y,\XX)$, where $Y$ is a compact space and
$\XX$ a topological stack, which is functorial both in $\XX$ and $Y$ and
behaves well enough with respect to pushouts. We also construct a bivariant (in
the sense of Fulton and MacPherson) theory for topological stacks: it gives us
a flexible theory of Gysin maps which are automatically compatible with
pullback, pushforward and products. Further we prove an excess formula in this
context. We introduce oriented stacks, generalizing oriented manifolds, which
are stacks on which we can do string topology. We prove that the homology of
the free loop stack of an oriented stack and the homology of hidden loops
(sometimes called ghost loops) are a Frobenius algebra which are related by a
natural morphism of Frobenius algebras. We also prove that the homology of free
loop stack has a natural structure of a BV-algebra, which together with the
Frobenius structure fits into an homological conformal field theories with
closed positive boundaries. Using our general machinery, we construct an
intersection pairing for (non necessarily compact) almost complex orbifolds
which is in the same relation to the intersection pairing for manifolds as
Chen-Ruan orbifold cup-product is to ordinary cup-product of manifolds. We show
that the hidden loop product of almost complex is isomorphic to the orbifold
intersection pairing twisted by a canonical class. Finally we gave some
examples including the case of the classifying stacks $[*/G]$ of a compact Lie
group.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 13:34:16 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Jan 2011 13:51:09 GMT"
}
] | 2011-01-05T00:00:00 | [
[
"Behrend",
"Kai",
""
],
[
"Ginot",
"Grégory",
""
],
[
"Noohi",
"Behrang",
""
],
[
"Xu",
"Ping",
""
]
] | [
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] |
712.3858 | Abraham Punnen | Abraham P. Punnen and Ruonan Zhang | Bottleneck flows in networks | null | null | null | null | cs.DS | null | The bottleneck network flow problem (BNFP) is a generalization of several
well-studied bottleneck problems such as the bottleneck transportation problem
(BTP), bottleneck assignment problem (BAP), bottleneck path problem (BPP), and
so on. In this paper we provide a review of important results on this topic and
its various special cases. We observe that the BNFP can be solved as a sequence
of $O(\log n)$ maximum flow problems. However, special augmenting path based
algorithms for the maximum flow problem can be modified to obtain algorithms
for the BNFP with the property that these variations and the corresponding
maximum flow algorithms have identical worst case time complexity. On unit
capacity network we show that BNFP can be solved in $O(\min \{{m(n\log
n)}^{{2/3}}, m^{{3/2}}\sqrt{\log n}\})$. This improves the best available
algorithm by a factor of $\sqrt{\log n}$. On unit capacity simple graphs, we
show that BNFP can be solved in $O(m \sqrt {n \log n})$ time. As a consequence
we have an $O(m \sqrt {n \log n})$ algorithm for the BTP with unit arc
capacities.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 13:49:45 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Punnen",
"Abraham P.",
""
],
[
"Zhang",
"Ruonan",
""
]
] | [
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] |
712.3859 | Vadim Meshkov | Andrey Bogdanov, Vadim Meshkov, Alexander Omelchenko, Michael Petrov | Classification of $k$-tangle projections using cascade representation | 15 pages, 15 figures and 3 tables | null | null | null | math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The paper addresses the $k$-tangle enumeration problem. We introduce a notion
of cascade diagram for $k$-tangle projections. An effective enumeration
algorithm for projections is proposed based on cascade representation. Tangles
projections with up to 12 crossings are tabulated. We provide also pictures of
alternating $k$-tangles with 5 crossing or less.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 14:10:25 GMT"
},
{
"version": "v2",
"created": "Sun, 18 Jul 2010 08:42:30 GMT"
}
] | 2010-07-20T00:00:00 | [
[
"Bogdanov",
"Andrey",
""
],
[
"Meshkov",
"Vadim",
""
],
[
"Omelchenko",
"Alexander",
""
],
[
"Petrov",
"Michael",
""
]
] | [
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] |
712.386 | Drahos Venos | D. Venos, J. Jakubek, O. Dragoun, S. Pospisil | Distribution of the 83Rb/83mKr activity on vacuum evaporated samples
examined with the Timepix position sensitive detector | 8 pages, 3 figures, 2 tables | null | null | EXP-01/2007 | nucl-ex | null | Properties of vacuum evaporated 83Rb/83mKr sources of low-energy conversion
electrons, which are under development for monitoring the energy scale
stability of the Karlsruhe Tritium Neutrino experiment KATRIN, were examined by
the Timepix pixel detector exhibiting the position resolution of at least 55
microm. No distinct local inhomogeneities in the surface distribution of
83Rb/83mKr were observed. The source diameter derived from the recorded image
agrees within 5 % with that expected from evaporation geometry. More precise
determination of the actual source diameter is complicated by Compton scattered
electrons caused by 83Rb gamma-rays.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 15:47:17 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Venos",
"D.",
""
],
[
"Jakubek",
"J.",
""
],
[
"Dragoun",
"O.",
""
],
[
"Pospisil",
"S.",
""
]
] | [
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712.3861 | Yan Elensky | Ya. S. Elensky | Effect of Multiple Scattering on the Critical Electric Field for Runaway
Electrons in the Atmosphere | 3 pages, 2 figures | BULLETIN OF THE RUSSIAN ACADEMY OF SCIENCES: PHYSICS Vol. 71 No. 7
2007 | 10.3103/S1062873807070428 | null | physics.ao-ph physics.geo-ph | null | A simple method for taking into account the multiple Coulomb scattering in
construction of a separatrix (the line separating the regions of runaway and
decelerating electrons in an electric field) is described. The desired line is
obtained by solving a simple transcendental equation.
| [
{
"version": "v1",
"created": "Wed, 26 Dec 2007 15:33:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Elensky",
"Ya. S.",
""
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712.3862 | Roman Baluev | Roman V. Baluev | Accounting for velocity jitter in planet search surveys | 10 pages, 1 figure, 1 table; accepted to MNRAS; 4th version due to a
few extra minor corrections in Sect.11 and Tab.1 | Mon. Not. R. Astron. Soc., 2009, Vol. 393, Issue 3, pp. 969-978 | 10.1111/j.1365-2966.2008.14217.x | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The role of radial velocity (RV) jitter in extrasolar planet search surveys
is discussed. Based on the maximum likelihood principle, improved statistical
algorithms for RV fitting and period search are developed. These algorithms
incorporate a built-in jitter determination, so that resulting estimations of
planetary parameters account for this jitter automatically. This approach is
applied to RV data for several extrasolar planetary systems. It is shown that
many RV planet search surveys suffer from periodic systematic errors which
increase effective RV jitter and can lead to erroneous conclusions. For
instance, the planet candidate HD74156 d may be a false detection made due to
annual systematic errors.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 14:08:09 GMT"
},
{
"version": "v2",
"created": "Tue, 6 May 2008 09:58:45 GMT"
},
{
"version": "v3",
"created": "Fri, 7 Nov 2008 10:15:06 GMT"
},
{
"version": "v4",
"created": "Sat, 8 Nov 2008 11:21:50 GMT"
}
] | 2009-02-14T00:00:00 | [
[
"Baluev",
"Roman V.",
""
]
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712.3863 | Misha Verbitsky | Maria Laura Barberis, Isabel G. Dotti and Misha Verbitsky | Canonical bundles of complex nilmanifolds, with applications to
hypercomplex geometry | 19 pages, v. 4, added reference to arXiv:0803.2048 by S. Rollenske | Math. Res. Lett. 16 (2009), no. 2, 331--347. | null | null | math.DG math.AG math.CV | null | A nilmanifold is a quotient of a nilpotent group $G$ by a co-compact discrete
subgroup. A complex nilmanifold is one which is equipped with a $G$-invariant
complex structure. We prove that a complex nilmanifold has trivial canonical
bundle. This is used to study hypercomplex nilmanifolds (nilmanifolds with a
triple of $G$-invariant complex structures which satisfy quaternionic
relations). We prove that a hypercomplex nilmanifold admits an HKT (hyperkahler
with torsion) metric if and only if the underlying hypercomplex structure is
abelian. Moreover, any $G$-invariant HKT-metric on a nilmanifold is balanced
with respect to all associated complex structures.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 14:19:32 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Jan 2008 17:53:04 GMT"
},
{
"version": "v3",
"created": "Fri, 11 Jan 2008 04:03:49 GMT"
},
{
"version": "v4",
"created": "Wed, 30 Apr 2008 12:54:08 GMT"
}
] | 2009-07-14T00:00:00 | [
[
"Barberis",
"Maria Laura",
""
],
[
"Dotti",
"Isabel G.",
""
],
[
"Verbitsky",
"Misha",
""
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] |
712.3864 | Pengbo Li | Pengbo Li, Qihuang Gong, Guangcan Guo | Effective generation of Ising interaction and cluster states in coupled
microcavities | 11pages, 2 figures, Revtex4 | null | 10.1140/epjd/e2009-00188-3 | null | quant-ph | null | We propose a scheme for realizing the Ising spin-spin interaction and atomic
cluster states utilizing trapped atoms in coupled microcavities. It is shown
that the atoms can interact with each other via the exchange of virtual photons
of the cavities. Through suitably tuning the parameters, an effective Ising
spin-spin interaction can be generated in this optical system, which is used to
produce the cluster states. This scheme does not need the preparation of
initial states of atoms and cavity modes, and is insensitive to cavity decay.
| [
{
"version": "v1",
"created": "Sun, 23 Dec 2007 08:50:10 GMT"
}
] | 2009-07-01T00:00:00 | [
[
"Li",
"Pengbo",
""
],
[
"Gong",
"Qihuang",
""
],
[
"Guo",
"Guangcan",
""
]
] | [
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] |
712.3865 | Ingrid Beltita | Ingrid Beltita, Anders Melin | Local smoothing for the backscattering transform | 22 pages | null | null | null | math.AP math-ph math.MP | null | An analysis of the backscattering data for the Schr\"odinger operator in odd
dimensions $n\ge 3$ motivates the introduction of the backscattering transform
$B: C_0^\infty ({\mathbb R}^n;{\mathbb C})\to C^\infty ({\mathbb R}^n; {\mathbb
C})$. This is an entire analytic mapping and we write $ Bv = \sum_1^\infty B_Nv
$ where $B_Nv$ is the $N$:th order term in the power series expansion at $v=0$.
In this paper we study estimates for $B_Nv$ in $H_{(s)}$ spaces, and prove that
$Bv$ is entire analytic in $v \in H_{(s)}\cap \Cal E'$ when $s\ge (n-3)/2$.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 15:55:35 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Beltita",
"Ingrid",
""
],
[
"Melin",
"Anders",
""
]
] | [
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] |
712.3866 | Sandro Wimberger | Alessandro Zenesini, Carlo Sias, Hans Lignier, Yeshpal Singh,
Donatella Ciampini, Oliver Morsch, Riccardo Mannella, Ennio Arimondo, Andrea
Tomadin, and Sandro Wimberger | Resonant tunneling of Bose-Einstein condensates in optical lattices | New J. Phys., in press | New J. Phys. 10, 053038 (2008) | 10.1088/1367-2630/10/5/053038 | null | cond-mat.other | null | In this article, we present theoretical as well as experimental results on
resonantly enhanced tunneling of Bose-Einstein condensates in optical lattices
both in the linear case and for small nonlinearities. Our results demonstrate
the usefulness of condensates in optical lattices for simulating Hamiltonians
originally used for describing solid state phenomena.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 16:19:43 GMT"
},
{
"version": "v2",
"created": "Mon, 5 May 2008 07:30:02 GMT"
}
] | 2008-06-01T00:00:00 | [
[
"Zenesini",
"Alessandro",
""
],
[
"Sias",
"Carlo",
""
],
[
"Lignier",
"Hans",
""
],
[
"Singh",
"Yeshpal",
""
],
[
"Ciampini",
"Donatella",
""
],
[
"Morsch",
"Oliver",
""
],
[
"Mannella",
"Riccardo",
""
],
[
"Arimondo",
"Ennio",
""
],
[
"Tomadin",
"Andrea",
""
],
[
"Wimberger",
"Sandro",
""
]
] | [
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] |
712.3867 | Rahul Jain | Rahul Jain (U. Waterloo) and Ashwin Nayak (U. Waterloo and Perimeter)
and Yi Su (U. Waterloo) | A Separation between Divergence and Holevo Information for Ensembles | 15 pages, 1 figure, version 1 | null | null | null | quant-ph | null | The notion of divergence information of an ensemble of probability
distributions was introduced by Jain, Radhakrishnan, and Sen in the context of
the ``substate theorem''. Since then, divergence has been recognized as a more
natural measure of information in several situations in quantum and classical
communication. We construct ensembles of probability distributions for which
divergence information may be significantly smaller than the more standard
Holevo information. As a result, we establish that lower bounds previously
shown for Holevo information are weaker than similar ones shown for divergence
information.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 16:24:38 GMT"
},
{
"version": "v2",
"created": "Sat, 29 Dec 2007 13:08:35 GMT"
}
] | 2008-01-02T00:00:00 | [
[
"Jain",
"Rahul",
"",
"U. Waterloo"
],
[
"Nayak",
"Ashwin",
"",
"U. Waterloo and Perimeter"
],
[
"Su",
"Yi",
"",
"U. Waterloo"
]
] | [
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] |
712.3868 | Pierluigi Contucci | Pierluigi Contucci, Francesco Unguendoli | Correlation Inequalities for Spin Glass in one Dimension | typos corrected | null | null | null | math-ph cond-mat.dis-nn cond-mat.stat-mech math.MP | null | We prove two inequalities for the direct and truncated correlation for the
nearest-neighboor one-dimensional Edwards-Anderson model with symmetric
quenched disorder. The second inequality has the opposite sign of the GKS
inequality of type II. In the non symmetric case with positive average we show
that while the direct correlation keeps its sign the truncated one changes sign
when crossing a suitable line in the parameter space. That line separates the
regions satisfying the GKS second inequality and the one proved here.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 16:40:45 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 18:23:00 GMT"
}
] | 2008-01-07T00:00:00 | [
[
"Contucci",
"Pierluigi",
""
],
[
"Unguendoli",
"Francesco",
""
]
] | [
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] |
712.3869 | Pakovich Fedor | M. Muzychuk, F. Pakovich | Jordan-Holder theorem for imprimitivity systems and maximal
decompositions of rational functions | In the current version the approach was considerably simplified and a
lot of new material was added (see e.g. Section 2.2, Section 2.3 and Section
3.2). On the other hand, some results of rather calculating character were
removed | null | 10.1112/plms/pdq009 | null | math.CV math.AG math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we prove several results about the lattice of imprimitivity
systems of a permutation group containing a cyclic subgroup with at most two
orbits. As an application we generalize the first Ritt theorem about functional
decompositions of polynomials, and some other related results. Besides, we
discuss examples of rational functions, related to finite subgroups of the
automorphism group of the sphere for which the first Ritt theorem fails to be
true.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 16:47:50 GMT"
},
{
"version": "v2",
"created": "Wed, 7 Jan 2009 16:34:49 GMT"
}
] | 2014-02-26T00:00:00 | [
[
"Muzychuk",
"M.",
""
],
[
"Pakovich",
"F.",
""
]
] | [
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] |
712.387 | Bruce Hajek | Bruce Hajek | Substitute Valuations: Generation and Structure | Revision includes more background and explanations | null | 10.1016/j.peva.2008.07.001 | null | cs.GT cs.PF | null | Substitute valuations (in some contexts called gross substitute valuations)
are prominent in combinatorial auction theory. An algorithm is given in this
paper for generating a substitute valuation through Monte Carlo simulation. In
addition, the geometry of the set of all substitute valuations for a fixed
number of goods K is investigated. The set consists of a union of polyhedrons,
and the maximal polyhedrons are identified for K=4. It is shown that the
maximum dimension of the maximal polyhedrons increases with K nearly as fast as
two to the power K. Consequently, under broad conditions, if a combinatorial
algorithm can present an arbitrary substitute valuation given a list of input
numbers, the list must grow nearly as fast as two to the power K.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 16:52:39 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Mar 2008 16:14:03 GMT"
},
{
"version": "v3",
"created": "Mon, 19 May 2008 14:50:58 GMT"
}
] | 2014-08-15T00:00:00 | [
[
"Hajek",
"Bruce",
""
]
] | [
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712.3871 | Denis Dalmazi | D. Dalmazi, A. de Souza Dutra | Multiflavor Soldering | 14 pages, no figures | Phys.Lett.B656:158-163,2007 | 10.1016/j.physletb.2007.09.007 | null | hep-th | null | In two dimensions the simple addition of two chiral bosons of opposite
chiralities does not lead to a full massless scalar field. Similarly, in three
dimensions the addition of two Maxwell-Chern-Simons fields of opposite
helicities $\pm 1$ will not produce a parity invariant Maxwell-Proca theory. An
interference term between the opposite chiralities (helicities) states is
required in order to obtain the expected result. The so called soldering
procedure provides the missing interference Lagrangian in both 2D and 3D cases.
In two dimensions such interference term allows to fuse two chiral fermionic
determinants into a nonchiral one. In a recent work we have generalized this
procedure by allowing the appearance of an extra parameter which takes two
possible values and leads to two different soldered Lagrangians. Here we apply
this generalized soldering in a bosonic theory which has appeared in a partial
bosonization of the 3D gauged Thirring with $N$ flavors. The multiplicity of
flavors allow new types of solderings and help us to understand the connection
between different perturbative approaches to bosonization in 3D. In particular,
we obtain an interference term which takes us from a multiflavor
Maxwell-Chern-Simons theory to a pair of self-dual and anti-self-dual theories
when we combine together both fermionic determinants of +1/2 and -1/2 helicity
fermions. An important role is played by a set of pure non-interacting
Chern-Simons fields which amount to a normalization factor in the fermionic
determinants and act like spectators in the original theory but play an active
role in the soldering procedure. Our results suggest that the generalized
soldering could be used to provide dual theories in both 2D and 3D cases.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 16:57:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Dalmazi",
"D.",
""
],
[
"Dutra",
"A. de Souza",
""
]
] | [
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-0.1291379482,
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] |
712.3872 | Denis Dalmazi | D. Dalmazi and A. de Souza Dutra | Restrictions over two-dimensional gauge models with Thirring-like
interaction | 9 pages, no figures | J.Phys.A40:13479-13484,2007 | 10.1088/1751-8113/40/44/024 | null | hep-th | null | Some years ago, it was shown how fermion self-interacting terms of the
Thirring-type impact the usual structure of massless two-dimensional gauge
theories [1]. In that work only the cases of pure vector and pure chiral gauge
couplings have been considered and the corresponding Thirring term was also
pure vector and pure chiral respectively, such that the vector (or chiral)
Schwinger model should not lose its chirality structure due to the addition of
the quartic interaction term. Here we extend this analysis to a generalized
vector and axial coupling both for the gauge interaction and the quartic
fermionic interactions. The idea is to perform quantization without losing the
original structure of the gauge coupling. In order to do that we make use of an
arbitrariness in the definition of the Thirring-like interaction.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 17:12:25 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Dalmazi",
"D.",
""
],
[
"Dutra",
"A. de Souza",
""
]
] | [
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] |
712.3873 | Matthias Sch\"utt | Matthias Schuett, Andreas Schweizer | On the uniqueness of elliptic K3 surfaces with maximal singular fibre | 20 pages; v2: refereed version with some corrections and additions;
author addresses and bibliography updated | Annales de l'institut Fourier, 63 no. 2 (2013), p. 689-713 | null | null | math.AG math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We explicitly determine the elliptic K3 surfaces with a maximal singular
fibre. If the characteristic of the ground field is different from 2, for each
of the two possible maximal fibre types, $I_{19}$ and $I^*_{14}$, the surface
is unique. In characteristic 2 the maximal fibre types are $I_{18}$ and
$I^*_{13}$, and there exist two (resp. one) one-parameter families of such
surfaces.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 17:33:40 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Jan 2011 07:46:38 GMT"
}
] | 2013-07-02T00:00:00 | [
[
"Schuett",
"Matthias",
""
],
[
"Schweizer",
"Andreas",
""
]
] | [
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] |
712.3874 | Thomas Thompson | Thomas W. J. Thompson, Duncan K. Galloway, Richard E. Rothschild, and
Lee Homer | Deviations from the Flux-Recurrence Time Relationship in GS 1826-238:
Potential Transient Spectral Changes | 10 pages, 9 figures, Accepted by ApJ | null | 10.1086/588723 | null | astro-ph | null | The low-mass X-ray binary GS 1826-238 is presently unique for its
consistently regular bursting behavior. In previous Rossi X-Ray Timing Explorer
(RXTE) measurements between 1997 November and 2002 July, this source exhibited
(nearly) limit-cycle bursts with recurrence times that decreased
proportionately as the persistent flux increased. Here we report additional
measurements of the burst recurrence time by RXTE, Chandra, and XMM-Newton, as
well as observations of optical bursts. On a few occasions we measured burst
recurrence times which deviated significantly from the earlier flux-recurrence
time relationship, and most of these bursts occurred earlier than would be
predicted based on the X-ray flux level. The epochs with early bursts were also
accompanied by unusual broadband timing signatures, with the entire power
spectrum shifting to higher frequencies. Concurrent XMM-Newton observations
during one of these occasions, in 2003 April, indicate that an additional soft
component may be present in the spectrum containing enough flux (30% of the
total) to account for the burst recurrence time discrepancy. A self-consistent
interpretation for the increase in soft flux and accompanying timing changes
during 2003 April is that accretion disk extends down to smaller radial
distances from the source than during the other observing epochs. The RXTE
observations since 2003 April show that the spectral and timing properties have
nearly returned to the previously established level.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 18:05:49 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 18:33:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Thompson",
"Thomas W. J.",
""
],
[
"Galloway",
"Duncan K.",
""
],
[
"Rothschild",
"Richard E.",
""
],
[
"Homer",
"Lee",
""
]
] | [
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712.3875 | Massoud Tousi | Mohsen Asgharzadeh and Massoud Tousi | A Unified Approach to Local Cohomology Modules Using Serre Classes | 10 pages | Can. Math. Bull. 53 (2010) 577-586 | 10.4153/CMB-2010-064-0 | null | math.AC | null | This paper discusses the connection between the local cohomology modules and
the Serre classes of $R$-modules. Such connection provided a common language
for expressing some results about the local cohomology $R$-modules, that has
appeared in different papers.
| [
{
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},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 09:11:03 GMT"
}
] | 2019-08-15T00:00:00 | [
[
"Asgharzadeh",
"Mohsen",
""
],
[
"Tousi",
"Massoud",
""
]
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712.3876 | Amir Rothschild | Ely Porat and Amir Rothschild | Explicit Non-Adaptive Combinatorial Group Testing Schemes | 15 pages, accepted to ICALP 2008 | null | null | null | cs.DS | null | Group testing is a long studied problem in combinatorics: A small set of $r$
ill people should be identified out of the whole ($n$ people) by using only
queries (tests) of the form "Does set X contain an ill human?". In this paper
we provide an explicit construction of a testing scheme which is better
(smaller) than any known explicit construction. This scheme has $\bigT{\min[r^2
\ln n,n]}$ tests which is as many as the best non-explicit schemes have. In our
construction we use a fact that may have a value by its own right: Linear
error-correction codes with parameters $[m,k,\delta m]_q$ meeting the
Gilbert-Varshamov bound may be constructed quite efficiently, in $\bigT{q^km}$
time.
| [
{
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{
"version": "v2",
"created": "Wed, 23 Jan 2008 22:30:43 GMT"
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{
"version": "v3",
"created": "Sun, 27 Apr 2008 20:32:13 GMT"
},
{
"version": "v4",
"created": "Tue, 29 Apr 2008 19:55:32 GMT"
},
{
"version": "v5",
"created": "Tue, 29 Apr 2008 20:02:41 GMT"
}
] | 2008-04-29T00:00:00 | [
[
"Porat",
"Ely",
""
],
[
"Rothschild",
"Amir",
""
]
] | [
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712.3877 | Tim Riley | Will Dison, Murray Elder, Tim Riley and Robert Young | The Dehn function of Stallings' group | 19 pages, 2 figures | Geometric and Functional Analysis, 19(2), pages 406-422, 2009 | 10.1007/s00039-009-0011-9 | null | math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that the Dehn function of a group of Stallings that is finitely
presented but not of type F_3 is quadratic. To appear in Geometric and
Functional Analysis.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 20:17:52 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Nov 2008 19:38:22 GMT"
}
] | 2012-05-16T00:00:00 | [
[
"Dison",
"Will",
""
],
[
"Elder",
"Murray",
""
],
[
"Riley",
"Tim",
""
],
[
"Young",
"Robert",
""
]
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712.3878 | Jeremy Yirmeyahu Kaminski | J.Y. Kaminski, A. Kanel-Belov and M. Teicher | Trisecant Lemma for Non Equidimensional Varieties | null | J. Math. Sci., 149:2 (2008), 1087--1097 | 10.1007/s10958-008-0047-7 | null | math.AG | null | The classic trisecant lemma states that if $X$ is an integral curve of
$\PP^3$ then the variety of trisecants has dimension one, unless the curve is
planar and has degree at least 3, in which case the variety of trisecants has
dimension 2. In this paper, our purpose is first to present another derivation
of this result and then to introduce a generalization to non-equidimensional
varities. For the sake of clarity, we shall reformulate our first problem as
follows. Let $Z$ be an equidimensional variety (maybe singular and/or
reducible) of dimension $n$, other than a linear space, embedded into $\PP^r$,
$r \geq n+1$. The variety of trisecant lines of $Z$, say $V_{1,3}(Z)$, has
dimension strictly less than $2n$, unless $Z$ is included in a
$(n+1)-$dimensional linear space and has degree at least 3, in which case
$\dim(V_{1,3}(Z)) = 2n$. Then we inquire the more general case, where $Z$ is
not required to be equidimensional. In that case, let $Z$ be a possibly
singular variety of dimension $n$, that may be neither irreducible nor
equidimensional, embedded into $\PP^r$, where $r \geq n+1$, and $Y$ a proper
subvariety of dimension $k \geq 1$. Consider now $S$ being a component of
maximal dimension of the closure of $\{l \in \G(1,r) \vtl \exists p \in Y, q_1,
q_2 \in Z \backslash Y, q_1,q_2,p \in l\}$. We show that $S$ has dimension
strictly less than $n+k$, unless the union of lines in $S$ has dimension $n+1$,
in which case $dim(S) = n+k$. In the latter case, if the dimension of the space
is stricly greater then $n+1$, the union of lines in $S$ cannot cover the whole
space. This is the main result of our work. We also introduce some examples
showing than our bound is strict.
| [
{
"version": "v1",
"created": "Sat, 22 Dec 2007 20:27:10 GMT"
}
] | 2017-12-05T00:00:00 | [
[
"Kaminski",
"J. Y.",
""
],
[
"Kanel-Belov",
"A.",
""
],
[
"Teicher",
"M.",
""
]
] | [
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