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712.1279 | Salvatore Caporaso | Salvatore Caporaso and Nicola Corriero | Kleene, Rogers and Rice Theorems Revisited in C and in Bash | 10 pages | null | null | null | cs.LO | null | The recursion theorem in the weak form {e}(z)=x(e,z) (universal function not
needed) and in Rogers form {n}(z)={{x}(n)}(z) and Rice theorem are proved a
first time using programs in C, and a second time with scripts in Bash.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 12:05:40 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Caporaso",
"Salvatore",
""
],
[
"Corriero",
"Nicola",
""
]
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712.128 | Sacha E. Kopp | Sacha E. Kopp (for the MINOS Collaboration) | Neutrino Spectra and Uncertainties for MINOS | contribution to the proceedings of NuFact07 (Okayama, Japan) | AIPConf.Proc.981:142-144,2008 | 10.1063/1.2898912 | null | hep-ex | null | The MINOS experiment at Fermilab has released an updated result on muon
disappearance based upon 2.5 x 10^20 protons on target. The experiment utilizes
the intense source of muon neutrinos provided by the NuMI beam line. This note
summarizes the systematic uncertainties in the experiment's knowledge of the
flux and energy spectrum of the neutrinos from NuMI.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 12:11:48 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Kopp",
"Sacha E.",
"",
"for the MINOS Collaboration"
]
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712.1281 | David Singh | D. J. Singh, Chul-Hong Park | Polar Behavior in a Magnetic Perovskite Via A-Site Disorder | 4 pages | null | null | null | cond-mat.mtrl-sci cond-mat.str-el | null | We elucidate a mechanism for obtaining polar behavior in magnetic perovskites
based on A-site disorder and demonstrate this mechanism by density functional
calculations for the double perovskite (La,Lu)MnNiO$_6$ with Lu concentrations
at and below 50%. We show that this material combines polar behavior and
ferromagnetism. The mechanism is quite general and may be applicable to a wide
range of magnetic perovskites.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 12:12:22 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Singh",
"D. J.",
""
],
[
"Park",
"Chul-Hong",
""
]
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-0.1020859107,
0.0110211791,
-0.0283095371,
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] |
712.1282 | Liang Gang Liu | Bao-quan Ai, Hui-zhang Xie and Liang-gang Liu | Thermal noise can facilitate energy transformation in the presence of
entropic barriers | 14 pages, 7 figures | Phys. Rev. E 75(2007)061126 | 10.1103/PhysRevE.75.061126 | null | cond-mat.stat-mech cond-mat.soft | null | Efficiency of a Brownian particle moving along the axis of a
three-dimensional asymmetric periodic channel is investigated in the presence
of a symmetric unbiased force and a load. Reduction of the spatial
dimensionality from two or three physical dimensions to an effective
one-dimensional system entails the appearance of entropic barriers and an
effective diffusion coefficient. The energetics in the presence of entropic
barriers exhibits peculiar behavior which is different from that occurring
through energy barriers. We found that even on the quasistatic limit there is a
regime where the efficiency can be a peaked function of temperature, which
indicates that thermal noise can facilitate energy transformation, contrary to
the case of energy barriers. The appearance of entropic barriers may induce
optimized efficiency at a finite temperature.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 12:29:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ai",
"Bao-quan",
""
],
[
"Xie",
"Hui-zhang",
""
],
[
"Liu",
"Liang-gang",
""
]
] | [
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] |
712.1283 | Tsuyoshi Sawada | Tsuyoshi Sawada, Norio Ikeda, Kazuyoshi Sunada, Nario Kuno, Takeshi
Kamazaki, Koh-Ichiro Morita, Yasutaka Kurono, Norikazu Koura, Katsumi Abe,
Sachiko Kawase, Jun Maekawa, Osamu Horigome, Kiyohiko Yanagisawa | On-The-Fly Observing System of the Nobeyama 45-m and ASTE 10-m
Telescopes | 11 pages, 13 figures, accepted for publication in PASJ | null | 10.1093/pasj/60.3.445 | null | astro-ph | null | We have developed spectral line On-The-Fly (OTF) observing mode for the
Nobeyama Radio Observatory 45-m and the Atacama Submillimeter Telescope
Experiment 10-m telescopes. Sets of digital autocorrelation spectrometers are
available for OTF with heterodyne receivers mounted on the telescopes,
including the focal-plane 5 x 5 array receiver, BEARS, on the 45-m. During OTF
observations, the antenna is continuously driven to cover the mapped region
rapidly, resulting in high observing efficiency and accuracy. Pointing of the
antenna and readouts from the spectrometer are recorded as fast as 0.1 second.
In this paper we report improvements made on software and instruments,
requirements and optimization of observing parameters, data reduction process,
and verification of the system. It is confirmed that, using optimal parameters,
the OTF is about twice as efficient as conventional position-switch observing
method.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 14:15:39 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Sawada",
"Tsuyoshi",
""
],
[
"Ikeda",
"Norio",
""
],
[
"Sunada",
"Kazuyoshi",
""
],
[
"Kuno",
"Nario",
""
],
[
"Kamazaki",
"Takeshi",
""
],
[
"Morita",
"Koh-Ichiro",
""
],
[
"Kurono",
"Yasutaka",
""
],
[
"Koura",
"Norikazu",
""
],
[
"Abe",
"Katsumi",
""
],
[
"Kawase",
"Sachiko",
""
],
[
"Maekawa",
"Jun",
""
],
[
"Horigome",
"Osamu",
""
],
[
"Yanagisawa",
"Kiyohiko",
""
]
] | [
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] |
712.1284 | Gennady Chuev N. | Gennady N. Chuev and Pascal Quemerais | Nature of metal-nonmetal transition in metal-ammonia solutions. II. From
uniform metallic state to inhomogeneous electronic microstructure | 22 pages, 10 figures | null | 10.1063/1.2883695 | null | cond-mat.stat-mech cond-mat.str-el | null | Applying semi-analytical models of nonideal plasma, we evaluate the behavior
of the metallic phase in metal-ammonia solutions (MAS). This behavior is mainly
controlled by the degenerate electron gas, which remains stable down to 5 MPM
due to high solvent polarizability and strong dielectric screening of solvated
ions. Comparing the behavior of the metallic state with those of localized
solvated electrons, we have estimated the miscibility gap $\Delta n$ for
various alkali metals and found $\Delta n$(Na)$> \Delta n($K$)$. It is rather
narrow in Rb-NH$_3$ and does not occur in Cs-NH$_3$ solutions, which is in full
agreement with the experiments. The case of Li is discussed separately. The
difference calculated in the excess free energies of the metallic and
nonmetallic phases is in the order of $k_BT$, yielding a thermally fluctuating
mixed state at intermediate metal concentrations. It results in a continuous
metal-nonmetal (MNM) transition above the consolute point $T_c$ and a phase
separation below $T_c$. We propose a criterion for the MNM transition which may
be attributed to the line of the maximum of compressibility above $T_c$. This
line crosses the spinodal one at the critical temperature. Finally, we assert
that a new electronic phase similar to microemulsion should also arise between
the spinodal and the binodal lines.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 14:09:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chuev",
"Gennady N.",
""
],
[
"Quemerais",
"Pascal",
""
]
] | [
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712.1285 | Paride Paradisi | J. Hisano, M. Nagai and P. Paradisi | "Flavored" Electric Dipole Moments in Supersymmetric Theories | 4 pages, 1 figure | Phys.Rev.D78:075019,2008 | 10.1103/PhysRevD.78.075019 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Standard Model (SM) predictions for the hadronic electric dipole moments
(EDMs) are well far from the present experimental resolutions, thus, the EDMs
represent very clean probes of New Physics (NP) effects. Especially, within an
MSSM framework with flavor-changing (but not necessarily CP violating) soft
terms, large and potentially visible effects to the EDMs are typically
expected. In this Letter we point out that, beyond-leading-order (BLO) effects,
so far neglected in the literature, dominate over the leading-order (LO)
effects in large regions of the parameter space, hence, their inclusion in the
evaluation of the hadronic EDMs is unavoidable.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 13:58:55 GMT"
},
{
"version": "v2",
"created": "Tue, 30 Sep 2008 17:49:05 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hisano",
"J.",
""
],
[
"Nagai",
"M.",
""
],
[
"Paradisi",
"P.",
""
]
] | [
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712.1286 | Bernhard Heim | Bernhard Heim | Miyawaki's $F_{12}$ Spinor L-function Conjecture | 13 pages | Kyoto J. Math. 52, no. 4 (2012), 817-828 | 10.1215/21562261-1728875 | null | math.NT math.RT | null | In this paper we prove the Miyawaki conjecture related to the spinor
$L$--function of a Siegel cusp form of weight 12 and degree 3 as a special
example of results related to Miyawaki lifts of odd degree.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 14:16:03 GMT"
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] | 2015-01-14T00:00:00 | [
[
"Heim",
"Bernhard",
""
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712.1287 | Fatemeh Ebrahimi | Fatemeh Ebrahimi | The shape of invasion perclation clusters in random and correlated media | null | null | 10.1088/1742-5468/2008/04/P04005 | null | cond-mat.stat-mech | null | The shape of two-dimensional invasion percolation clusters are studied
numerically for both non-trapping (NTIP) and trapping (TIP) invasion
percolation processes. Two different anisotropy quantifiers, the anisotropy
parameter and the asphericity are used for probing the degree of anisotropy of
clusters. We observe that in spite of the difference in scaling properties of
NTIP and TIP, there is no difference in the values of anisotropy quantifiers of
these processes. Furthermore, we find that in completely random media, the
invasion percolation clusters are on average slightly less isotropic than
standard percolation clusters. Introducing isotropic long-range correlations
into the media reduces the isotropy of the invasion percolation clusters. The
effect is more pronounced for the case of persisting long-range correlations.
The implication of boundary conditions on the shape of clusters is another
subject of interest. Compared to the case of free boundary conditions, IP
clusters of conventional rectangular geometry turn out to be more isotropic.
Moreover, we see that in conventional rectangular geometry the NTIP clusters
are more isotropic than TIP clusters.
| [
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"created": "Sat, 8 Dec 2007 14:21:04 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Mar 2008 12:07:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ebrahimi",
"Fatemeh",
""
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] |
712.1288 | Takayuki Matsuki | Takayuki Matsuki, Toshiyuki Morii, and Kazutaka Sudoh | Study of Structure of the Mass Gap between Two Spin Multiplets | 8 pages, 2 figures, Invited talk given at the XII International
Conference on Hadron Spectroscopy (Hadron 07), Frascati, October 8-13, 2007 | null | null | null | hep-ph hep-ex | null | Studying our semirelativistic potential model and the numerical results,
which succeeds in predicting and reproducing recently discovered higher
resonances of $D$, $D_s$, $B$, and $B_s$, we find a simple expression for the
mass gap between two spin multiplets of heavy-light mesons, $(0^-,1^-)$ and
$(0^+,1^+)$. The mass gap between chiral partners defined by $\Delta
M=M(0^+)-M(0^-)$ and/or $M(1^+)-M(1^-)$ is given by $\Delta
M=M(0^+)-M(0^-)=M(1^+)-M(1^-)\approx \Lambda_{\rm Q}-m_q$ in the limit of heavy
quark symmetry. We also study the case including $1/m_Q$ corrections.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 15:45:51 GMT"
}
] | 2008-03-29T00:00:00 | [
[
"Matsuki",
"Takayuki",
""
],
[
"Morii",
"Toshiyuki",
""
],
[
"Sudoh",
"Kazutaka",
""
]
] | [
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] |
712.1289 | Dimitri Vvedensky | A. Zangwill and D. D. Vvedensky | Regimes of Precursor-Mediated Epitaxial Growth | 10 pages, 2 figures | null | null | null | cond-mat.mtrl-sci | null | A discussion of epitaxial growth is presented for those situations (OMVPE,
CBE, ALE, MOMBE, GSMBE, etc.) when the kinetics of surface processes associated
with molecular precursors may be rate limiting. Emphasis is placed on the
identification of various {\it characteristic length scales} associated with
the surface processes. Study of the relative magnitudes of these lengths
permits one to identify regimes of qualitatively different growth kinetics as a
function of temperature and deposition flux. The approach is illustrated with a
simple model which takes account of deposition, diffusion, desorption,
dissociation, and step incorporation of a single precursor species, as well as
the usual processes of atomic diffusion and step incorporation. Experimental
implications are discussed in some detail.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 15:51:31 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Zangwill",
"A.",
""
],
[
"Vvedensky",
"D. D.",
""
]
] | [
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] |
712.129 | Nils Bluemer | N. Bl\"umer | Numerically exact Green functions from Hirsch-Fye quantum Monte Carlo
simulations | 4 pages, 6 figures | null | null | null | cond-mat.str-el | null | We present a new method for extracting numerically exact imaginary-time Green
functions from standard Hirsch-Fye quantum Monte Carlo (HF-QMC) simulations
within dynamical mean-field theory. By analytic continuation, angular resolved
spectra are obtained without the discretization bias previously associated with
HF-QMC results. The method is shown to be accurate even at very low
temperatures (T=W/800 for bandwidth W) in the strongly correlated regime.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 16:07:11 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Blümer",
"N.",
""
]
] | [
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] |
712.1291 | Kaiki Taro Inoue | Kenji Tomita and Kaiki Taro Inoue | Second Order Gravitational Effects on CMB Temperature Anisotropy in
Lambda dominated flat universes | 16 pages, 8 figures, No major change. Eqs (5.6) and (5.7) are
modified to include uncompensating cases | Phys.Rev.D77:103522,2008 | 10.1103/PhysRevD.77.103522 | KU-TP-18 | astro-ph gr-qc | null | We study second order gravitational effects of local inhomogeneities on the
cosmic microwave background radiation in flat universes with matter and a
cosmological constant $\Lambda$. We find that the general relativistic
correction to the Newtonian approximation is negligible at second order
provided that the size of the inhomogeneous region is sufficiently smaller than
the horizon scale. For a spherically symmetric top-hat type quasi-linear
perturbation, the first order temperature fluctuation corresponding to the
linear integrated Sachs-Wolfe (ISW) effect is enhanced(suppressed) by the
second order one for a compensated void(lump). As a function of redshift of the
local inhomogeneity, the second order temperature fluctuations due to evolution
of the gravitational potential have a peak before the matter-$\Lambda$ equality
epoch for a fixed comoving size and a density contrast. The second order
gravitational effects from local quasi-linear inhomogeneities at a redshift z~1
may significantly affect the cosmic microwave background.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 16:53:40 GMT"
},
{
"version": "v2",
"created": "Thu, 15 May 2008 07:27:31 GMT"
}
] | 2014-09-08T00:00:00 | [
[
"Tomita",
"Kenji",
""
],
[
"Inoue",
"Kaiki Taro",
""
]
] | [
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] |
712.1292 | Manuela Rodriguez-Gallardo | M. Rodriguez-Gallardo, A. Deltuva, E. Cravo, R. Crespo, and A. C.
Fonseca | Two-body scattering without angular-momentum decomposition | null | Phys.Rev.C78:034602,2008 | 10.1103/PhysRevC.78.034602 | null | nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Two-body scattering is studied by solving the Lippmann-Schwinger equation in
momentum space without angular-momentum decomposition for a local spin
dependent short range interaction plus Coulomb. The screening and
renormalization approach is employed to treat the Coulomb interaction.
Benchmark calculations are performed by comparing our procedure with
partial-wave calculations in configuration space for p-10Be, p-16O and 12C-10Be
elastic scattering, using a simple optical potential model.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 15:48:25 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Jul 2008 14:03:16 GMT"
},
{
"version": "v3",
"created": "Fri, 5 Sep 2008 15:10:02 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Rodriguez-Gallardo",
"M.",
""
],
[
"Deltuva",
"A.",
""
],
[
"Cravo",
"E.",
""
],
[
"Crespo",
"R.",
""
],
[
"Fonseca",
"A. C.",
""
]
] | [
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] |
712.1293 | Tomasz Dietl | Tomasz Dietl | Interplay between carrier localization and magnetism in diluted magnetic
and ferromagnetic semiconductors | 8 figures, special issue of Journal of the Physical Society of Japan
on "Advances in Spintronics"; in v2, typo in Eq. 1 corrected | J. Phys. Soc. Jpn. 77 (2008) 031005 | 10.1143/JPSJ.77.031005 | null | cond-mat.dis-nn cond-mat.mtrl-sci | null | The presence of localized spins exerts a strong influence on quantum
localization in doped semiconductors. At the same time carrier-mediated
interactions between the localized spins are modified or even halted by
carriers' localization. The interplay of these effects is discussed for II-VI
and III-V diluted magnetic semiconductors. This insight is exploited to
interpret the complex dependence of resistance on temperature, magnetic field,
and concentration of valence-band holes in (Ga,Mn)As. In particular, high field
negative magnetoresistance results from the orbital weak localization effect.
The resistance maximum and the associated negative magnetoresistance near the
Curie temperature are assigned to the destructive influence of preformed
ferromagnetic bubbles on the "antilocalization" effect driven by
disorder-modified carrier-carrier interactions. These interactions account also
for the low-temperature increase of resistance. Furthermore, the sensitivity of
conductance to spin splitting and to scattering by spin disorder may explain
resistance anomalies at coercive fields, where relative directions of external
and molecular fields change.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 08:56:15 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Dec 2007 13:20:12 GMT"
}
] | 2008-10-20T00:00:00 | [
[
"Dietl",
"Tomasz",
""
]
] | [
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] |
712.1294 | Antonio Pineda | David Nevado and Antonio Pineda | Forward virtual Compton scattering and the Lamb shift in chiral
perturbation theory | 13 pages, 1 figure. Minor changes, misprints corrected, two
referenced added | Phys.Rev.C77:035202,2008 | 10.1103/PhysRevC.77.035202 | null | hep-ph nucl-th physics.atom-ph | null | We compute the spin-independent structure functions of the forward
virtual-photon Compton tensor of the proton at one loop using heavy baryon
chiral perturbation theory and dispersion relations. We study the relation
between both approaches. We use these results to generalize some sum rules to
virtual photon transfer momentum and relate them with sum rules in deep
inelastic scattering. We then compute the leading chiral term of the
polarizability correction to the Lamb shift of the hydrogen and muonic
hydrogen. We obtain -87.05/n^3 Hz and -0.148/n^3 meV for the correction to the
hydrogen and muonic hydrogen Lamb shift respectively.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 17:38:24 GMT"
},
{
"version": "v2",
"created": "Sat, 8 Mar 2008 14:38:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Nevado",
"David",
""
],
[
"Pineda",
"Antonio",
""
]
] | [
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712.1295 | Ciprian Demeter | Ciprian Demeter, Michael Lacey, Terence Tao, Christoph Thiele | The Walsh model for $M_2^{*}$ Carleson | 20 pages, 0 figures | null | null | null | math.CA | null | We study the Walsh model of a certain maximal truncation of Carleson's
operator, related to the Return Times Theorem from Ergodic Theory.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 18:01:20 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Demeter",
"Ciprian",
""
],
[
"Lacey",
"Michael",
""
],
[
"Tao",
"Terence",
""
],
[
"Thiele",
"Christoph",
""
]
] | [
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712.1296 | Venkateswaran Krishnan | Venkateswaran P. Krishnan | A generalization of inversion formulas of Pestov and Uhlmann | 6 pages | null | null | null | math.DG math.CA | null | In this note, we give a generalization of the inversion formulas of
Pestov-Uhlmann for the geodesic ray transform of functions and vector fields on
simple 2-dimensional manifolds of constant curvature. The inversion formulas
given here hold for 2-dimensional simple manifolds whose curvatures close to a
constant.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 18:02:48 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Krishnan",
"Venkateswaran P.",
""
]
] | [
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] |
712.1297 | Olga Melnyk | O. V. Melnyk, A. A. Elyiv, I. B. Vavilova | The Structure of the Local Supercluster of Galaxies Revealed by the
Three-Dimensional Voronoi's Tessellation Method | 14 pages | KinematikaFiz.NebesnykhTel22:283-296,2006 | null | null | astro-ph | null | 3D Voronoi's tessellation method was first applied to identify groups of
galaxies in the structure of a supercluster. The sample under consideration
consists of more than 7000 galaxies of the Local Supercluster (LS) with radial
velocities up to 3100 km/s. Because of an essential non-homogeneity of the LS
catalogue, it was proposed to overscale distances in such an ''artificial'' way
that the concentration of galaxies was varying as with increase of the distance
a power-behaved function with the same exponent beta as for the full
homogeneous catalogue. Various parameters of clustering were taking into
account: alpha (0.01, 0.1, 1%) as the part of galaxies, which have the relative
volume of a Voronoi's cell smaller than the critical one for the random
distribution; beta = 0, which fits to the random galaxy distribution; beta =
0.7, which is close to the pancake galaxy distribution. It is revealed that
Voronoi's tessellation method depends weakly on beta-parameter, and the number
of galaxies in rich structures is growing rather than in poor ones with
increase of alpha-parameter. The comparison of the groups derived with the
groups obtained by Karachentsev's dynamical method shows that the number of
groups, which coincides by all the components, is 22%. As a whole, the
dynamical method is more preferred for identifying sparsely populated galaxy
groups, whereas 3D Voronoi's tessellation method is preferred for more
populated ones.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 18:40:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Melnyk",
"O. V.",
""
],
[
"Elyiv",
"A. A.",
""
],
[
"Vavilova",
"I. B.",
""
]
] | [
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] |
712.1298 | William Wylie | Peter Petersen and William Wylie | On the classification of gradient Ricci solitons | 14 pages. case. v.4--Added formula for the f-laplacian of the
curvature operator and applications | Geom. Topol. 14 (2010) 2277-2300 | 10.2140/gt.2010.14.2277 | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that the only complete shrinking gradient Ricci solitons with
vanishing Weyl tensor are quotients of the standard ones. This gives a new
proof of the Hamilton-Ivey-Perel'man classification of 3-dimensional shrinking
gradient solitons. We also prove a classification for expanding gradient Ricci
solitons with constant scalar curvature and suitably decaying Weyl tensor.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 19:10:42 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Jan 2008 18:56:28 GMT"
},
{
"version": "v3",
"created": "Sat, 10 May 2008 01:42:21 GMT"
},
{
"version": "v4",
"created": "Thu, 26 Jun 2008 05:07:36 GMT"
},
{
"version": "v5",
"created": "Wed, 24 Sep 2008 16:02:06 GMT"
}
] | 2014-11-11T00:00:00 | [
[
"Petersen",
"Peter",
""
],
[
"Wylie",
"William",
""
]
] | [
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-0.0144522553,
0.0546692349,
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-0.0060487073,
0.0519450083,
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0.0046375347,
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] |
712.1299 | Kevin Zumbrun | Jeffrey Humpherys, Gregory Lyng, and Kevin Zumbrun | Stability of strong ideal-gas shock layers | null | null | 10.1007/s00205-008-0195-4 | null | math-ph math.MP | null | Extending recent results in the isentropic case, we use a combination of
asymptotic ODE estimates and numerical Evans-function computations to examine
the spectral stability of shock-wave solutions of the compressible
Navier--Stokes equations with ideal gas equation of state. Our main results are
that, in appropriately rescaled coordinates, the Evans function associated with
the linearized operator about the wave (i) converges in the large-amplitude
limit to the Evans function for a limiting shock profile of the same equations,
for which internal energy vanishes at one endstate; and (ii) has no unstable
(positive real part) zeros outside a uniform ball $|\lambda|\le \Lambda$. Thus,
the rescaled eigenvalue ODE for the set of all shock waves, augmented with the
(nonphysical) limiting case, form a compact family of boundary-value problems
that can be conveniently investigated numerically. An extensive numerical
Evans-function study yields one-dimensional spectral stability, independent of
amplitude, for gas constant $\gamma$ in $[1.2, 3]$ and ratio $\nu/\mu$ of heat
conduction to viscosity coefficient within $[0.2,5]$ ($\gamma\approx 1.4$,
$\nu/\mu\approx 1.47$ for air). Other values may be treated similarly but were
not considered. The method of analysis extends also to the multi-dimensional
case, a direction that we shall pursue in a future work.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 19:25:50 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 19:34:52 GMT"
}
] | 2017-06-09T00:00:00 | [
[
"Humpherys",
"Jeffrey",
""
],
[
"Lyng",
"Gregory",
""
],
[
"Zumbrun",
"Kevin",
""
]
] | [
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712.13 | Robyn Miller | John H. Hubbard, Robyn L. Miller | Equidistribution of Horocyclic Flows on Complete Hyperbolic Surfaces of
Finite Area | 29 pages, 10 figures | null | null | null | math.DS math.PR | null | We provide a self-contained, accessible introduction to Ratner's
Equidistribution Theorem in the special case of horocyclic flow on a complete
hyperbolic surface of finite area. This equidistribution result was first
obtained in the early 1980s by Dani and Smillie and later reappeared as an
illustrative special case of Ratner's work on the equidistribution of unipotent
flows in homogeneous spaces. We also prove an interesting probabilistic result
due to Breuillard: on the modular surface an arbitrary uncentered random walk
on the horocycle through almost any point will fail to equidistribute, even
though the horocycles are themselves equidistributed. In many aspects of this
exposition we are indebted to Bekka and Mayer's more ambitious survey, "Ergodic
Theory and Topological Dynamics for Group Actions on Homogeneous Spaces."
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 22:13:16 GMT"
},
{
"version": "v2",
"created": "Sun, 2 Mar 2008 23:38:06 GMT"
}
] | 2008-03-03T00:00:00 | [
[
"Hubbard",
"John H.",
""
],
[
"Miller",
"Robyn L.",
""
]
] | [
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] |
712.1301 | Vladimir Nikiforov | Vladimir Nikiforov | The maximum spectral radius of C_4-free graphs of given order and size | null | null | null | null | math.CO | null | Let G be a graph of n vertices and m edges, and let G has no cycles of length
4. We give upper bounds on the adjacency spectral radius of G in terms of n and
m.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 19:39:32 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Nikiforov",
"Vladimir",
""
]
] | [
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-0.129671067,
-0.0543729737,
-0.0431832895,
0.043062102,
0.1091499105,
0.0434660614,
-0.0388205275,
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-0.0150071029,
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] |
712.1302 | Jean-Francois Bony | Bernard Bercu, Jean-Francois Bony, Vincent Bruneau | Spectrum of the product of Toeplitz matrices with application in
probability | 16 pages | null | null | null | math.FA math.PR | null | We study the spectrum of the product of two Toeplitz operators. Assume that
the symbols of these operators are continuous and real-valued and that one of
them is non-negative. We prove that the spectrum of the product of finite
section Toeplitz matrices converges to the spectrum of the product of the
semi-infinite Toeplitz operators. We give an example showing that the supremum
of this set is not always the supremum of the product of the two symbols.
Finally, we provide an application in probability which is the first motivation
of this study. More precisely, we obtain a large deviation principle for
Gaussian quadratic forms.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 14:09:03 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Bercu",
"Bernard",
""
],
[
"Bony",
"Jean-Francois",
""
],
[
"Bruneau",
"Vincent",
""
]
] | [
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712.1303 | Ilya Zaliapin | Ilya Zaliapin, Andrei Gabrielov, Vladimir Keilis-Borok, and Henry Wong | Aftershock identification | 4 pages, 5 figures | Phys. Rev. Lett., 101, 018501, 2008 | 10.1103/PhysRevLett.101.018501 | SCEC publication 1137 | physics.geo-ph physics.data-an | null | Earthquake aftershock identification is closely related to the question "Are
aftershocks different from the rest of earthquakes?" We give a positive answer
to this question and introduce a general statistical procedure for clustering
analysis of seismicity that can be used, in particular, for aftershock
detection. The proposed approach expands the analysis of Baiesi and Paczuski
[PRE, 69, 066106 (2004)] based on the space-time-magnitude nearest-neighbor
distance $\eta$ between earthquakes. We show that for a homogeneous Poisson
marked point field with exponential marks, the distance $\eta$ has Weibull
distribution, which bridges our results with classical correlation analysis for
unmarked point fields. We introduce a 2D distribution of spatial and temporal
components of $\eta$, which allows us to identify the clustered part of a point
field. The proposed technique is applied to several synthetic seismicity models
and to the observed seismicity of Southern California.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 19:50:14 GMT"
}
] | 2010-03-01T00:00:00 | [
[
"Zaliapin",
"Ilya",
""
],
[
"Gabrielov",
"Andrei",
""
],
[
"Keilis-Borok",
"Vladimir",
""
],
[
"Wong",
"Henry",
""
]
] | [
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] |
712.1304 | Hamad Alyahyaei | R. A. Jishi and H. M. Alyahyaei | Electronic structure of copper intercalated transition metal
dichalcogenides: First-principles calculations | 8 pages, 6 figures | R. A. Jishi and H. M. Alyahyaei, Phys. Rev. B 78, 144516 (2008) | 10.1103/PhysRevB.78.144516 | null | cond-mat.supr-con cond-mat.str-el | null | We report first principles calculations, within density functional theory, of
copper intercalated titanium diselenides, CuxTiSe2, for values of x ranging
from 0 to 0.11. The effect of intercalation on the energy bands and densities
of states of the host material is studied in order to better understand the
cause of the superconductivity that was recently observed in these structures.
We find that charge transfer from the copper atoms to the metal dichalcogenide
host layers causes a gradual reduction in the number of holes in the otherwise
semi-metallic pristine TiSe2, thus suppressing the charge density wave
transition at low temperatures, and a corresponding increase in the density of
states at the Fermi level. These effects are probably what drive the
superconducting transition in the intercalated systems.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 19:55:33 GMT"
},
{
"version": "v2",
"created": "Tue, 20 May 2008 20:39:39 GMT"
}
] | 2009-01-12T00:00:00 | [
[
"Jishi",
"R. A.",
""
],
[
"Alyahyaei",
"H. M.",
""
]
] | [
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-0.0417662859,
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0.0302421041,
0.0054722116,
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0.0176648907,
0.0509241074,
-0.0608154982,
-0.0487943813,
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] |
712.1305 | Hamid Kachkachi | P.-M. Dejardin, H. Kachkachi, and Yu. P. Kalmykov | Thermal and surface anisotropy effects on the magnetization reversal of
a nanocluster | 8 pages, 3 eps figures (Oral communication at ICFPM, Rome 9-12/10/07,
by H. Kachkachi) | null | 10.1088/0022-3727/41/13/134004 | 0712.1302v2 | cond-mat.mtrl-sci cond-mat.stat-mech | null | The relaxation rate and temperature-dependent switching field curve of a
spherical magnetic nanocluster are calculated by taking into account the effect
of surface anisotropy via an effective anisotropy model. In particular, it is
shown that surface anisotropy may change the thermally activated magnetization
reversal by more than an order of magnitude, and that temperature-dependent
switching field curves noticeably deviate from the Stoner-Wohlfarth astroid.
With recent and future $\mu$-SQUID measurements in mind, we indicate how
comparison of our results with experimental data on isolated clusters may allow
one to obtain valuable information on surface anisotropy.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 19:58:08 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 10:18:59 GMT"
},
{
"version": "v3",
"created": "Wed, 16 Jan 2008 22:08:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dejardin",
"P. -M.",
""
],
[
"Kachkachi",
"H.",
""
],
[
"Kalmykov",
"Yu. P.",
""
]
] | [
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] |
712.1306 | Tapan Nath | P. Dey, T. K. Nath, P. K. Manna and S. M. Yusuf | Enhanced grain surface effect on magnetic properties of nanometric
La0.7Ca0.3MnO3 manganite : Evidence of surface spin freezing of manganite
nanoparticles | 41 pages, 10 figures | null | 10.1063/1.3020524 | null | cond-mat.mtrl-sci | null | We have investigated the effect of nanometric grain size on magnetic
properties of single phase, nanocrystalline, granular La0.7Ca0.3MnO3 (LCMO)
sample. We have considered core-shell structure of our LCMO nanoparticles,
which can explain its magnetic properties. From the temperature dependence of
field cooled (FC) and zero-field cooled (ZFC) dc magnetization (DCM), the
magnetic properties could be distinguished into two regimes: a relatively high
temperature regime T > 40 K where the broad maximum of ZFC curve (at T = Tmax)
is associated with the blocking of core particle moments, whereas the sharp
maximum (at T = TS) is related to the freezing of surface (shell) spins. The
unusual shape of M (H) loop at T = 1.5 K, temperature dependent feature of
coercive field and remanent magnetization give a strong support of surface spin
freezing that are occurring at lower temperature regime (T < 40 K) in this LCMO
nanoparticles. Additionally, waiting time (tw) dependence of ZFC relaxation
measurements at T = 50 K show weak dependence of relaxation rate [S(t)] on tw
and dM/dln(t) following a logarithmic variation on time. Both of these features
strongly support the high temperature regime to be associated with the blocking
of core moments. At T = 20 K, ZFC relaxation measurements indicates the
existence of two different types of relaxation processes in the sample with
S(t) attaining a maximum at the elapsed time very close to the wait time tw =
1000 sec, which is an unequivocal sign of glassy behavior. This age-dependent
effect convincingly establish the surface spin freezing of our LCMO
nanoparticles associated with a background of superparamagnetic (SPM) phase of
core moments.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 20:19:53 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dey",
"P.",
""
],
[
"Nath",
"T. K.",
""
],
[
"Manna",
"P. K.",
""
],
[
"Yusuf",
"S. M.",
""
]
] | [
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] |
712.1307 | Alejandro Fernandez-Martinez | Alejandro Fernandez-Martinez (ILL, LGIT), Gabriel J. Cuello (ILL),
Gabriela Roman-Ross (LGIT), Mark R. Johnson (ILL), Fabrizio Bardelli (GILDA,
ESRF), Xavier Turrillas (ICC), Laurent Charlet (LGIT) | Arsenic uptake by gypsum and calcite: Modeling and probing by neutron
and x-ray scattering | Proceedings of the Eighth International Conference on Neutron
Scattering | Physica B: Condensed Matter 385-386, 2 (2006) 935-937 | 10.1016/j.physb.2006.05.276 | null | physics.chem-ph | null | Here we report on two structural studies performed on As-doped gypsum (CaSO4
2H2O) and calcite (CaCO3), using neutron (D20-ILL) and x-ray (ID11-ESRF)
diffraction data and EXAFS (BM8-ESRF). The aim of this study is to determine
whether As gets into the bulk of gypsum and calcite structures or is simply
adsorbed on the surface. Different mechanisms of substitution are used as
hypotheses. The combined Rietveld analysis of neutron and x-ray diffraction
data shows an expansion of the unit cell volume proportional to the As
concentration within the samples. DFT-based simulations confirm the increase of
the unit cell volume proportional to the amount of carbonate or sulphate groups
substituted. Interpolation of the experimental Rietveld data allows us to
distinguish As substituted within the structure from that adsorbed on the
surface of both minerals.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 21:23:51 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Fernandez-Martinez",
"Alejandro",
"",
"ILL, LGIT"
],
[
"Cuello",
"Gabriel J.",
"",
"ILL"
],
[
"Roman-Ross",
"Gabriela",
"",
"LGIT"
],
[
"Johnson",
"Mark R.",
"",
"ILL"
],
[
"Bardelli",
"Fabrizio",
"",
"GILDA,\n ESRF"
],
[
"Turrillas",
"Xavier",
"",
"ICC"
],
[
"Charlet",
"Laurent",
"",
"LGIT"
]
] | [
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] |
712.1308 | J. M. Wrobel | J.M. Wrobel, Y. Terashima, L.C. Ho | Outflow-Dominated Emission from the Quiescent Massive Black Holes in NGC
4621 and NGC 4697 | 11 pages; 4 figures: emulateapj; to appear in ApJ | null | 10.1086/527542 | null | astro-ph | null | The nearby elliptical galaxies NGC 4621 and NGC 4697 each host a supermassive
black hole with a mass more than 1e8 Solar masses. Analysis of archival Chandra
data and new NRAO Very Large Array data shows that each galaxy contains a
low-luminosity active galactic nucleus (LLAGN), identified as a faint, hard
X-ray source that is astrometrically coincident with a faint 8.5-GHz source.
The latter has a diameter less than 0.3 arcsec (26 pc for NGC 4621, 17 pc for
NGC 4697). The black holes energizing these LLAGNs have Eddington ratios L(2-10
keV) / L(Edd) ~ 1e-9, placing them in the so-called quiescent regime. The
emission from these quiescent black holes is radio-loud, with log Rx = log
nuLnu(8.5 GHz) / L(2-10 keV) ~ -2, suggesting the presence of a radio outflow.
Also, application of the radio-X-ray-mass relation from Yuan & Cui for
quiescent black holes predicts the observed radio luminosities nuLnu(8.5 GHz)
to within a factor of a few. Significantly, that relation invokes X-ray
emission from the outflow rather than from an accretion flow. The faint, but
detectable, emission from these two massive black holes is therefore consistent
with being outflow-dominated. Observational tests of this finding are
suggested.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 21:37:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wrobel",
"J. M.",
""
],
[
"Terashima",
"Y.",
""
],
[
"Ho",
"L. C.",
""
]
] | [
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712.1309 | Jarek Duda | Jarek Duda | Complex base numeral systems | 19 pages, 7 figures | null | null | null | math.DS cs.DM | null | In this paper will be introduced large, probably complete family of complex
base systems, which are 'proper' - for each point of the space there is a
representation which is unique for all but some zero measure set. The condition
defining this family is the periodicity - we get periodic covering of the plane
by fractals in hexagonal-type structure, what can be used for example in image
compression. There will be introduced full methodology of analyzing and using
this approach - both for the integer part: periodic lattice and the fractional:
attractor of some IFS, for which the convex hull or properties like dimension
of the boundary can be found analytically. There will be also shown how to
generalize this approach to higher dimensions and found some proper systems in
dimension 3.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 09:51:48 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Dec 2007 21:49:02 GMT"
},
{
"version": "v3",
"created": "Sun, 24 Feb 2008 20:41:34 GMT"
}
] | 2008-02-24T00:00:00 | [
[
"Duda",
"Jarek",
""
]
] | [
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] |
712.131 | Lev Cherbanski Dr. | Lev Cherbanski | About Algorithm for Transformation of Logic Functions (ATLF) | 25 pages, in English, German and Russian | null | null | null | cs.LO cs.AI | null | In this article the algorithm for transformation of logic functions which are
given by truth tables is considered. The suggested algorithm allows the
transformation of many-valued logic functions with the required number of
variables and can be looked in this sense as universal.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 22:36:44 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Cherbanski",
"Lev",
""
]
] | [
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712.1311 | Bruce Knuteson | CDF Collaboration | Model-Independent and Quasi-Model-Independent Search for New Physics at
CDF | 40 pages. Version published in Physical Review D | Phys.Rev.D78:012002,2008 | 10.1103/PhysRevD.78.012002 | null | hep-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Data collected in Run II of the Fermilab Tevatron are searched for
indications of new electroweak scale physics. Rather than focusing on
particular new physics scenarios, CDF data are analyzed for discrepancies with
respect to the standard model prediction. A model-independent approach (Vista)
considers the gross features of the data, and is sensitive to new large cross
section physics. A quasi-model-independent approach (Sleuth) searches for a
significant excess of events with large summed transverse momentum, and is
particularly sensitive to new electroweak scale physics that appears
predominantly in one final state. This global search for new physics in over
three hundred exclusive final states in 927 pb^-1 of ppbar collisions at
sqrt(s)=1.96 TeV reveals no such significant indication of physics beyond the
standard model.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 14:41:35 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jul 2008 19:31:46 GMT"
}
] | 2015-03-13T00:00:00 | [
[
"CDF Collaboration",
"",
""
]
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712.1312 | Ilya Zaliapin | Michael Ghil, Ilya Zaliapin, Sylvester Thompson | A delay differential model of ENSO variability: Parametric instability
and the distribution of extremes | 22 pages, 9 figures | Nonlin. Proc. Geophys., 15, 417-433, 2008 | 10.5194/npg-15-417-2008 | null | physics.ao-ph | null | We consider a delay differential equation (DDE) model for El-Nino Southern
Oscillation (ENSO) variability. The model combines two key mechanisms that
participate in ENSO dynamics: delayed negative feedback and seasonal forcing.
We perform stability analyses of the model in the three-dimensional space of
its physically relevant parameters. Our results illustrate the role of these
three parameters: strength of seasonal forcing $b$, atmosphere-ocean coupling
$\kappa$, and propagation period $\tau$ of oceanic waves across the Tropical
Pacific. Two regimes of variability, stable and unstable, are separated by a
sharp neutral curve in the $(b,\tau)$ plane at constant $\kappa$. The detailed
structure of the neutral curve becomes very irregular and possibly fractal,
while individual trajectories within the unstable region become highly complex
and possibly chaotic, as the atmosphere-ocean coupling $\kappa$ increases. In
the unstable regime, spontaneous transitions occur in the mean ``temperature''
({\it i.e.}, thermocline depth), period, and extreme annual values, for purely
periodic, seasonal forcing. The model reproduces the Devil's bleachers
characterizing other ENSO models, such as nonlinear, coupled systems of partial
differential equations; some of the features of this behavior have been
documented in general circulation models, as well as in observations. We
expect, therefore, similar behavior in much more detailed and realistic models,
where it is harder to describe its causes as completely.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 23:01:45 GMT"
}
] | 2020-01-29T00:00:00 | [
[
"Ghil",
"Michael",
""
],
[
"Zaliapin",
"Ilya",
""
],
[
"Thompson",
"Sylvester",
""
]
] | [
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] |
712.1313 | Hongbao Zhang | Song He and Hongbao Zhang | The black hole dynamical horizon and generalized second law of
thermodynamics | JHEP style, 8 pages, 2 figures, version to appear in JHEP with typos
corrected | JHEP0712:052,2007 | 10.1088/1126-6708/2007/12/052 | null | gr-qc astro-ph hep-th | null | The generalized second law of thermodynamics for a system containing a black
hole dynamical horizon is proposed in a covariant way. Its validity is also
tested in case of adiabatically collapsing thick light shells.
| [
{
"version": "v1",
"created": "Sat, 8 Dec 2007 23:16:33 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 16:47:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"He",
"Song",
""
],
[
"Zhang",
"Hongbao",
""
]
] | [
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712.1314 | Zden\v{e}k Dole\v{z}al | N.S. Borisov (1), N.A. Bazhanov (1), A.A. Belyaev (4), J. Broz (2), J.
Cerny (2), Z. Dolezal (2), A.N. Fedorov (1), G.M. Gurevich (3), M.P. Ivanov
(1), P. Kodys (2), P. Kubik (2), E.S. Kuzmin (1), A.B. Lazarev (1), F. Lehar
(5,6), O.O. Lukhanin (4), V.N. Matafonov (1), A.B. Neganov (1), I.L. Pisarev
(1), J. Svejda (2), S.N. Shilov (1), Yu.A. Usov (1) and I.Wilhelm (2) ((1)
Joint Institute for Nuclear Research, Dubna, Russia; (2) Institute of
Particle and Nuclear Physics, Faculty of Mathematics and Physics, Charles
University in Prague; (3) Institute for Nuclear Research, Russian Academy of
Sciences, Moscow, Russia; (4) NSC KIPT, Kharkov, Ukraine (5) SPP DAPNIA CEA
Saclay, France (6) IEAP CTU, Prague, Czech Republic) | Deuteron frozen spin polarized target for nd experiements at the VdG
accelerator of Charles University | null | Nucl.Instrum.Meth.A593:177-182,2008 | 10.1016/j.nima.2008.05.026 | null | nucl-ex | null | A frozen spin polarized deuteron target cooled by the 3He/4He dilution
refrigerator is described. Fully deuterated 1,2-propanediol was used as a
target material. Deuteron vector polarization about 40% was obtained for the
target in the shape of a cylinder of 2 cm diameter and 6 cm length. The target
is intended for a study of 3N interactions at the polarized neutron beam
generated by the Van de Graaff accelerator at the Charles University in Prague.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 00:01:31 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Borisov",
"N. S.",
""
],
[
"Bazhanov",
"N. A.",
""
],
[
"Belyaev",
"A. A.",
""
],
[
"Broz",
"J.",
""
],
[
"Cerny",
"J.",
""
],
[
"Dolezal",
"Z.",
""
],
[
"Fedorov",
"A. N.",
""
],
[
"Gurevich",
"G. M.",
""
],
[
"Ivanov",
"M. P.",
""
],
[
"Kodys",
"P.",
""
],
[
"Kubik",
"P.",
""
],
[
"Kuzmin",
"E. S.",
""
],
[
"Lazarev",
"A. B.",
""
],
[
"Lehar",
"F.",
""
],
[
"Lukhanin",
"O. O.",
""
],
[
"Matafonov",
"V. N.",
""
],
[
"Neganov",
"A. B.",
""
],
[
"Pisarev",
"I. L.",
""
],
[
"Svejda",
"J.",
""
],
[
"Shilov",
"S. N.",
""
],
[
"Usov",
"Yu. A.",
""
],
[
"Wilhelm",
"I.",
""
]
] | [
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712.1315 | Paul Wesson | Paul S. Wesson | The Meaning of Dimensions | null | Wesson P.S. (2008), The Meaning of Dimensions in Relativity and
the Dimensionality of the World, Series: Fundamental Theories of Physics, Vol
153 Petkov, Vesselin (Ed.), 276 p | 10.1007/978-1-4020-6318-3_1 | null | gr-qc | null | We review the current status of dimensions, as the result of a long and
controversial history that includes input from philosophy and physics. Our
conclusion is that they are subjective but essential concepts which provide a
kind of book-keeping device, their number increasing as required by advances in
physics. The world almost certainly has more than the four dimensions of space
and time, but the introduction of the fifth and higher dimensions requires a
careful approach wherein known results are embedded and new ones are couched in
the most productive manner.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 00:13:53 GMT"
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] | 2015-05-13T00:00:00 | [
[
"Wesson",
"Paul S.",
""
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712.1316 | Christopher J. Conselice | Nicola Atkinson, Christopher J. Conselice, Nicole Fox (Nottingham) | Hierarchical Disk Galaxy Assembly as the Origin of Scatter in the z~1
Stellar Mass Tully-Fisher Relation | 12 pages, MNRAS, submitted | null | null | null | astro-ph | null | Recent observations of distant disk galaxies show that there is little to no
evolution in the relation between maximum rotation speed and stellar mass at z
< 1.2. There is however a significant scatter between these two quantities
whose origin is uncertain. We show in this paper that this scatter is at least
partially the result of galaxy merging, revealing that disk galaxy growth at z
< 1 is fundamentally hierarchical. We carry this out by calculating CAS
(concentration, asymmetry, clumpiness) structural parameters using archival
Hubble Space Telescope imaging of 91 high-redshift disk galaxies at 0.4 < z <
1.0 with robustly measured stellar masses and rotational maximum velocities
taken from Conselice et al. (2005). We separate our sample into two redshift
bins divided at z = 0.7, and investigate deviations from the stellar-mass
Tully-Fisher relation in both the M_* and V_max directions, and how these
correlate with structural asymmetries. We find a significant (> 3 sigma)
correlation between the residuals from the stellar-mass Tully-Fisher relation
in both the M_* and V_max directions, and high asymmetries. This result holds
after we remove contributions from star formation and edge-on galaxies which
can produce higher asymmetries unrelated to merging. While there are a few
cases in which our disk galaxies have very large asymmetries, and are
potentially involved in major mergers, in general these asymmetries are smaller
than the major merger limit. It is therefore likely that these galaxies are
forming hierarchically through minor galaxy mergers, which is also suggested by
the constant slope and zero point of the stellar mass Tully-Fisher relation
during the same epoch.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 00:21:59 GMT"
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] | 2007-12-11T00:00:00 | [
[
"Atkinson",
"Nicola",
"",
"Nottingham"
],
[
"Conselice",
"Christopher J.",
"",
"Nottingham"
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[
"Fox",
"Nicole",
"",
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712.1317 | Luis Dieulefait | Luis Dieulefait | How to facet a gemstone: from potential modularity to the proof of
Serre's modularity conjecture | Survey based on two talks I gave last summer, at the Segundas
Jornadas de Teoria de Numeros (Madrid) and at the Summer School on Serre's
Modularity Conjecture (Luminy) | null | null | null | math.NT | null | In this survey paper we present recent results obtained by Khare,
Wintenberger and the author that have led to a proof of Serre's conjecture,
such as existence of compatible families, modular upper bounds for universal
deformation rings and existence of minimal lifts, prime switching and
modularity propagation, weight reduction (via existence of conjugates) and
(iterated) killing ramification.
The main tools used in the proof of these results are modularity lifting
theorems a la Wiles and a result of potential modularity due to R. Taylor.
| [
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"created": "Sun, 9 Dec 2007 00:28:41 GMT"
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"Luis",
""
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712.1318 | Laszlo E. Szabo | Laszlo E. Szabo | The Einstein-Podolsky-Rosen Argument and the Bell Inequalities | (Review, forthcoming in The Internet Encyclopedia of Philosophy) 28
pages, LaTeX, 11 figures | null | null | null | quant-ph | null | In 1935 Einstein, Podolsky, and Rosen (EPR) published an important paper in
which they claimed that the whole formalism of quantum mechanics together with
what they called "Reality Criterion" imply that quantum mechanics cannot be
complete. That is, there must exist some elements of reality that are not
described by quantum mechanics. There must be, they concluded, a more complete
description of physical reality behind quantum mechanics. There must be a
state, a hidden variable, characterizing the state of affairs in the world in
more details than the quantum mechanical state, something that also reflects
the missing elements of reality.
Under some further but quite plausible assumptions, this conclusion implies
that in some spin-correlation experiments the measured quantum mechanical
probabilities should satisfy particular inequalities (Bell-type inequalities).
The paradox consists in the fact that quantum probabilities do not satisfy
these inequalities. And this paradoxical fact has been confirmed by several
laboratory experiments in the last three decades. The problem is still open and
hotly debated among both physicists and philosophers. It has motivated a wide
range of research from the most fundamental quantum mechanical experiments
through foundations of probability theory to the theory of stochastic causality
as well as the metaphysics of free will.
| [
{
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712.1319 | Alexandru E. Stanculescu | Alexandru E. Stanculescu | A homotopy theory for enrichment in simplicial modules | 6 pages, comments are welcome | null | null | null | math.CT | null | We put a Quillen model structure on the category of small categories enriched
in simplicial $k$-modules and non-negatively graded chain complexes of
$k$-modules, where $k$ is a commutative ring. The model structure is obtained
by transfer from the model structure on simplicial categories due to J.
Bergner.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 01:42:29 GMT"
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] | 2007-12-11T00:00:00 | [
[
"Stanculescu",
"Alexandru E.",
""
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] |
712.132 | Timothy Y. Chow | Timothy Y. Chow | A beginner's guide to forcing | Accepted version (Contemp. Math.); bugs fixed, exposition improved,
new references | null | null | null | math.LO math.HO | null | This expository paper, aimed at the reader without much background in set
theory or logic, gives an overview of Cohen's proof (via forcing) of the
independence of the continuum hypothesis. It emphasizes the broad outlines and
the intuitive motivation while omitting most of the proofs. The reader must of
course consult standard textbooks for the missing details, but this article
provides a map of the forest so that the beginner will not get lost while
forging through the trees.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:47:29 GMT"
},
{
"version": "v2",
"created": "Thu, 8 May 2008 14:40:05 GMT"
}
] | 2008-05-08T00:00:00 | [
[
"Chow",
"Timothy Y.",
""
]
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712.1321 | Jeffrey Case | Jeffrey S. Case | Singularity theorems and the Lorentzian splitting theorem for the
Bakry-Emery-Ricci tensor | Correction to one of the examples | J. Geom. Phys., Volume 60, Issue 3, March 2010, 477-490 | 10.1016/j.geomphys.2009.11.001 | null | math.DG | null | We consider the Hawking-Penrose singularity theorems and the Lorentzian
splitting theorem under the weaker curvature condition of nonnegative
Bakry-Emery-Ricci curvature $Ric_f^m$ in timelike directions. We prove that
they still hold when $m$ is finite, and when $m$ is infinite, they hold under
the additional assumption that $f$ is bounded from above.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:40:58 GMT"
},
{
"version": "v2",
"created": "Tue, 3 Jun 2008 05:51:34 GMT"
}
] | 2010-12-15T00:00:00 | [
[
"Case",
"Jeffrey S.",
""
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] |
712.1322 | Paul SanGiorgio | P. SanGiorgio, S. Reymond, M. R. Beasley, J.H. Kwon, K. Char | Anomalous double peak structure in Nb/Ni superconductor/ferromagnet
tunneling DOS | 4 pages, 3 figures | null | 10.1103/PhysRevLett.100.237002 | null | cond-mat.supr-con | null | We have experimentally investigated the density of states (DOS) in Nb/Ni
(S/F) bilayers as a function of Ni thickness, $d_F$. Our thinnest samples show
the usual DOS peak at $\pm\Delta_0$, whereas intermediate-thickness samples
have an anomalous ``double-peak'' structure. For thicker samples ($d_F \geq
3.5$ nm), we see an ``inverted'' DOS which has previously only been reported in
superconductor/weak-ferromagnet structures. We analyze the data using the
self-consistent non-linear Usadel equation and find that we are able to
quantitatively fit the features at $\pm\Delta_0$ if we include a large amount
of spin-orbit scattering in the model. Interestingly, we are unable to
reproduce the sub-gap structure through the addition of any parameter(s).
Therefore, the observed anomalous sub-gap structure represents new physics
beyond that contained in the present Usadel theory.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 01:56:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"SanGiorgio",
"P.",
""
],
[
"Reymond",
"S.",
""
],
[
"Beasley",
"M. R.",
""
],
[
"Kwon",
"J. H.",
""
],
[
"Char",
"K.",
""
]
] | [
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] |
712.1323 | Daniel H. Lenz | Daniel Lenz | Aperiodic order via dynamical systems: Diffraction for sets of finite
local complexity | 22 pages | null | null | null | math.DS math-ph math.MP | null | We give an introduction into diffraction theory for aperiodic order. We focus
on an approach via dynamical systems and the phenomenon of pure point
diffraction. We review recent results and sketch proofs. We then present a new
uniform Wiener/Wintner type result generalizing various earlier results of this
type.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 03:30:09 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Lenz",
"Daniel",
""
]
] | [
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] |
712.1324 | Ji Wei He | J.-W. He and Q.-S. Wu | Koszul differential graded algebras and BGG correspondence | 29 pages | null | null | null | math.RA math.KT | null | The concept of Koszul differential graded algebra (Koszul DG algebra) is
introduced. Koszul DG algebras exist extensively, and have nice properties
similar to the classic Koszul algebras. A DG version of the Koszul duality is
proved. When the Koszul DG algebra $A$ is AS-regular, the Ext-algebra $E$ of
$A$ is Frobenius. In this case, similar to the classical BGG correspondence,
there is an equivalence between the stable category of finitely generated left
$E$-modules, and the quotient triangulated category of the full triangulated
subcategory of the derived category of right DG $A$-modules consisting of all
compact DG modules modulo the full triangulated subcategory consisting of all
the right DG modules with finite dimensional cohomology. The classical BGG
correspondence can derived from the DG version.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 03:34:43 GMT"
},
{
"version": "v2",
"created": "Thu, 13 Dec 2007 11:55:27 GMT"
},
{
"version": "v3",
"created": "Fri, 1 Feb 2008 12:40:00 GMT"
}
] | 2008-02-01T00:00:00 | [
[
"He",
"J. -W.",
""
],
[
"Wu",
"Q. -S.",
""
]
] | [
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712.1325 | Giacomo Mauro D'Ariano | Giulio Chiribella, Giacomo Mauro D'Ariano, and Paolo Perinotti | Quantum Circuits Architecture | 10 eps figures + Qcircuit.tex | Phys. Rev. Lett. 101, 060401 (2008) | 10.1103/PhysRevLett.101.060401 | null | quant-ph | null | We present a method for optimizing quantum circuits architecture. The method
is based on the notion of "quantum comb", which describes a circuit board in
which one can insert variable subcircuits. The method allows one to efficiently
address novel kinds of quantum information processing tasks, such as
storing-retrieving, and cloning of channels.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 03:55:02 GMT"
}
] | 2008-09-08T00:00:00 | [
[
"Chiribella",
"Giulio",
""
],
[
"D'Ariano",
"Giacomo Mauro",
""
],
[
"Perinotti",
"Paolo",
""
]
] | [
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712.1326 | Chitta Ranjan Das | C.R. Das and L.V. Laperashvili | Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology | 31 pages, 7 figures | Int.J.Mod.Phys.A23:1863-1890,2008 | 10.1142/S0217751X08039712 | CHEP-PKU/2/12-2007 | hep-ph astro-ph | null | In the present paper we have developed a concept of parallel ordinary (O) and
mirror (M) worlds. We have shown that in the case of a broken mirror parity
(MP), the evolutions of fine structure constants in the O- and M-worlds are not
identical. It is assumed that E_6-unification inspired by superstring theory
restores the broken MP at the scale \sim 10^{18} GeV, what unavoidably leads to
the different E_6-breakdowns at this scale: E_6 \to SO(10)\times U(1)_Z - in
the O-world, and E'_6 \to SU(6)'\times SU(2)'_Z - in the M-world. Considering
only asymptotically free theories, we have presented the running of all the
inverse gauge constants \alpha_i^{-1} in the one-loop approximation. Then a
`quintessence' scenario is discussed for our model of accelerating universe.
Such a scenario is related with an axion (`acceleron') of a new gauge group
SU(2)'_Z which has a coupling constant g_Z extremely growing at the scale
\Lambda_Z\sim 10^{-3} eV.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 03:56:29 GMT"
},
{
"version": "v2",
"created": "Sun, 27 Jan 2008 02:27:53 GMT"
}
] | 2008-06-22T00:00:00 | [
[
"Das",
"C. R.",
""
],
[
"Laperashvili",
"L. V.",
""
]
] | [
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712.1327 | Corey Hoelscher | Corey A. Hoelscher | Classification of Cohomogeneity One Manifolds in Low Dimensions | null | null | null | null | math.DG | null | A cohomogeneity one manifold is a manifold with the action of a compact Lie
group, whose quotient is one dimensional. Such manifolds are of interest in
Riemannian geometry, in the context of nonnegative sectional curvature, as well
as in other areas of geometry and in physics. In this paper we classify compact
simply connected cohomogeneity one manifolds in dimensions 5, 6 and 7. We also
show that all such manifolds admit metrics of nonnegative sectional curvature,
with the possible exception of two families of manifolds.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 04:35:22 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Hoelscher",
"Corey A.",
""
]
] | [
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] |
712.1328 | Zhaoyong Huang | Rong Luo and Zhaoyong Huang | When Are Torsionless Modules Projective? | 10 pages | null | null | null | math.RA math.RT | null | In this paper, we study the problem when a finitely generated torsionless
module is projective. Let $\Lambda$ be an Artinian local algebra with radical
square zero. Then a finitely generated torsionless $\Lambda$-module $M$ is
projective if ${\rm Ext^1_\Lambda}(M,M)=0$. For a commutative Artinian ring
$\Lambda$, a finitely generated torsionless $\Lambda$-module $M$ is projective
if the following conditions are satisfied: (1) ${\rm
Ext}^i_{\Lambda}(M,\Lambda)=0$ for $i=1,2,3$; and (2) ${\rm
Ext}^i_{\Lambda}(M,M)=0$ for $i=1,2$. As a consequence of this result, we have
that for a commutative Artinian ring $\Lambda$, a finitely generated Gorenstein
projective $\Lambda$-module is projective if and only if it is selforthogonal.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 06:10:17 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Luo",
"Rong",
""
],
[
"Huang",
"Zhaoyong",
""
]
] | [
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] |
712.1329 | Qi Zhang S. | Qi S. Zhang | Strong non-collapsing and uniform Sobolev inequalities for Ricci flow
with surgeries | null | null | null | null | math.DG math.AP | null | We prove a uniform Sobolev inequality for Ricci flow, which is independent of
the number of surgeries. As an application, under less assumptions, a
non-collapsing result stronger than Perelman's $\kappa$ non-collapsing with
surgery is derived. The proof is shorter and seems more accessible. The result
also improves some earlier ones where the Sobolev inequality depended on the
number of surgeries.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 06:22:27 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Zhang",
"Qi S.",
""
]
] | [
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712.133 | Manuel Guedel | M. Guedel, S. L. Skinner, M. Audard, K. R. Briggs, S. Cabrit | Discovery of a bipolar X-ray jet from the T Tauri star DG Tau | accepted by Astronomy & Astrophysics, 11 pages, 6 figures | null | 10.1051/0004-6361:20078141 | null | astro-ph | null | We have obtained and analyzed Chandra ACIS-S observations of the strongly
accreting classical T Tauri star DG Tau. Our principal goals are to map the
immediate environment of the star to characterize possible extended X-rays
formed in the jet, and to re-visit the anomalous, doubly absorbed X-ray
spectrum of DG Tau itself. We combine our new ACIS-S data with a data set
previously obtained. The data are superimposed to obtain flux and hardness
images. Separate X-ray spectra are extracted for DG Tau and areas outside its
point spread function. We detect a prominent X-ray jet at a position angle of
PA ~225 deg (tentatively suggested by Guedel et al. 2005), coincident with the
optical jet axis. We also identify a counter jet at PA = 45 deg. The X-ray jets
are detected out to a distance of ~5" from the star, their sources being
extended at the ACIS-S resolution. The jet spectra are soft, with a best-fit
electron temperature of 3.4 MK. We find evidence for excess absorption of the
counter jet. The spectrum of the DG Tau point source shows two components with
largely different temperatures and absorption column densities. The similar
temperatures and small absorbing gas columns of the jet sources and the soft
component of the "stellar" source suggest that these sources are related,
produced either by shocks or by magnetic heating in the jets. Cooling estimates
suggest that the pressure in the hot gas contributes to jet expansion. The hard
"stellar" component, on the other hand, is associated with a stellar corona or
magnetosphere. The excessive photoelectric absorption of this component
suggests the presence of dust-depleted accretion streams above coronal magnetic
fields.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 08:10:50 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Guedel",
"M.",
""
],
[
"Skinner",
"S. L.",
""
],
[
"Audard",
"M.",
""
],
[
"Briggs",
"K. R.",
""
],
[
"Cabrit",
"S.",
""
]
] | [
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] |
712.1331 | Maria J. Esteban | Maria J. Esteban (CEREMADE), Patricio Felmer (CMM), Alexander Quaas | Super-linear elliptic equation for the Pucci operator without growth
restrictions for the data | null | null | null | null | math.AP | null | In this paper we deal with existence and uniqueness of solution to
super-linear problems for the Pucci operator: $$ -\M^+(D^2u)+|u|^{s-1}u=f(x)
\quad {in} \RR^n, $$ where $s>1$ and $f$ satisfies only local integrability
conditions. This result is well known when, instead of the Pucci operator, the
Laplacian or a divergence form operator is considered. Our existence results
use the Alexandroff-Bakelman-Pucci inequality since we cannot use any
variational formulation. For radially symmetric $f$ we can prove our results
under less local integrability assumptions, taking advantage of an appropriate
variational formulation. We also obtain an existence result with boundary
explosion in smooth domains.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 08:28:26 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Esteban",
"Maria J.",
"",
"CEREMADE"
],
[
"Felmer",
"Patricio",
"",
"CMM"
],
[
"Quaas",
"Alexander",
""
]
] | [
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] |
712.1332 | Wadim Zudilin | Wadim Zudilin | Ramanujan-type formulae for $1/\pi$: A second wind? | 13 pages; v2: two typos corrected, references updated, numeration of
formulae changed to agree with the published version | Modular Forms and String Duality, N. Yui, H. Verrill, and C.F.
Doran (eds.), Fields Inst. Commun. Ser. 54 (2008), Amer. Math. Soc. & Fields
Inst., 179--188 | null | null | math.NT math.CA | null | In 1914 S. Ramanujan recorded a list of 17 series for $1/\pi$. We survey the
methods of proofs of Ramanujan's formulae and indicate recently discovered
generalizations, some of which are not yet proven.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 10:12:48 GMT"
},
{
"version": "v2",
"created": "Mon, 19 May 2008 05:12:25 GMT"
}
] | 2009-02-24T00:00:00 | [
[
"Zudilin",
"Wadim",
""
]
] | [
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-0.0659610182,
-0.1124749929,
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] |
712.1333 | Andrei Martinez-Finkelshtein | A.B.J. Kuijlaars, A. Martinez-Finkelshtein, and F. Wielonsky | Non-intersecting squared Bessel paths and multiple orthogonal
polynomials for modified Bessel weights | 59 pages, 11 figures | null | 10.1007/s00220-008-0652-9 | null | math.CA math-ph math.MP math.PR | null | We study a model of $n$ non-intersecting squared Bessel processes in the
confluent case: all paths start at time $t = 0$ at the same positive value $x =
a$, remain positive, and are conditioned to end at time $t = T$ at $x = 0$. In
the limit $n \to \infty$, after appropriate rescaling, the paths fill out a
region in the $tx$-plane that we describe explicitly. In particular, the paths
initially stay away from the hard edge at $x = 0$, but at a certain critical
time $t^*$ the smallest paths hit the hard edge and from then on are stuck to
it. For $t \neq t^*$ we obtain the usual scaling limits from random matrix
theory, namely the sine, Airy, and Bessel kernels. A key fact is that the
positions of the paths at any time $t$ constitute a multiple orthogonal
polynomial ensemble, corresponding to a system of two modified Bessel-type
weights. As a consequence, there is a $3 \times 3$ matrix valued
Riemann-Hilbert problem characterizing this model, that we analyze in the large
$n$ limit using the Deift-Zhou steepest descent method. There are some novel
ingredients in the Riemann-Hilbert analysis that are of independent interest.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 10:26:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kuijlaars",
"A. B. J.",
""
],
[
"Martinez-Finkelshtein",
"A.",
""
],
[
"Wielonsky",
"F.",
""
]
] | [
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712.1334 | Hisaki Hatanaka | Hisaki Hatanaka | Radiatively Induced Spontaneous Symmetry Breaking by Wilson Line in a
Warped Extra Dimension | 32 pages, 11 figures | null | null | null | hep-th hep-ph | null | We investigate the dynamical gauge-Higgs unification in the Randall-Sundrum
(RS) space-time. We study the dynamical gauge-Higgs unification in the SU(2)
gauge theory with a bulk fermion in the RS space-time. We evaluate the
contribution from fermion loop to the one-loop effective potential with respect
to the Wilson-line phase, and study the dynamical gauge symmetry breaking. We
also apply this mechanism of the gauge symmetry breaking to the electroweak
gauge-Higgs unification in the RS space-time. Especially we numerically studied
a SU(3)_w gauge model as a toy model of electroweak gauge-Higgs unification in
the RS space-time. We introduce an adjoint fermion into the model to break the
gauge symmetry and to obtain the U(1)_em electromagnetic symmetry. We found
that in this model the ratio of Z-boson mass to W-boson varies with respect to
the Wilson-line phase even at the tree level. We also propose a dynamical
mechanism of tuning the ratio m_Z/m_W to the experimental value
91.2GeV/80.4GeV=1.13 by introducing bulk scalars or bulk fermions with twisted
boundary conditions. In these models the Higgs can vary in mass between zero
and 290GeV.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 18:54:58 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Hatanaka",
"Hisaki",
""
]
] | [
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] |
712.1335 | Yuri A. Rylov | Yuri A. Rylov | Discrimination of particle masses in multivariant space-time geometry | 16 pages, 0 figures, removal of extra root | null | null | null | physics.gen-ph | null | Multivariance of geometry means that at the point $P_{0}$ there exist many
vectors $P_{0}P_{1}$, $\P_{0}P_{2}$,... which are equivalent (equal) to the
vector $\Q_{0}Q_{1}$ at the point $Q_{0}$, but they are not equivalent between
themselves. The discrimination capacity (zero-variance) of geometry appears,
when at the point $P_{0}$ there are no vectors, which are equivalent to the
vector $Q_{0}Q_{1}$ at the point $Q_{0}$. It is shown, that in some
multivariant space-time geometries some particles of small mass may be
discriminated (i.e. either they do not exist, or their evolution is
impossible). The possibility of some particle discrimination may appear to be
important for explanation of the discrete character of mass spectrum of
elementary particles.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 12:15:05 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 03:44:06 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Rylov",
"Yuri A.",
""
]
] | [
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] |
712.1336 | Daiji Kimura | T. Inagaki, D. Kimura, A. Kvinikhidze | $\pi$ and $\sigma$ mesons at finite temperature and density in the NJL
model with dimensional regularization | 28 pages, 9 figures, v2: a few points corrected and references added | Phys.Rev.D77:116004,2008 | 10.1103/PhysRevD.77.116004 | HUPD-0704 | hep-ph | null | Dynamical Symmetry breaking and meson masses are studied in the
Nambu-Jona-Lasinio (NJL) model at finite temperature and chemical potential
using the dimensional regularization. Since the model is not renormalizable in
four space-time dimensions, physical results and parameters depend on the
regularization method. Following the imaginary time formalism, we introduce the
temperature, $T$ and the chemical potential, $\mu$. The parameters in the model
are fixed by calculating the pion mass and decay constant in the dimensional
regularization at $T=\mu=0$.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 12:22:26 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Jan 2008 10:18:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Inagaki",
"T.",
""
],
[
"Kimura",
"D.",
""
],
[
"Kvinikhidze",
"A.",
""
]
] | [
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] |
712.1337 | Zoltan Esik | S. L. Bloom, Z. Esik | Axiomatizing rational power series | null | null | null | null | cs.LO cs.DM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Iteration semirings are Conway semirings satisfying Conway's group
identities. We show that the semirings $\N^{\rat}\llangle \Sigma^* \rrangle$ of
rational power series with coefficients in the semiring $\N$ of natural numbers
are the free partial iteration semirings. Moreover, we characterize the
semirings $\N_\infty^{\rat}\llangle \Sigma^* \rrangle$ as the free semirings in
the variety of iteration semirings defined by three additional simple
identities, where $\N_\infty$ is the completion of $\N$ obtained by adding a
point of infinity. We also show that this latter variety coincides with the
variety generated by the complete, or continuous semirings. As a consequence of
these results, we obtain that the semirings $\N_\infty^{\rat}\llangle \Sigma^*
\rrangle$, equipped with the sum order, are free in the class of symmetric
inductive $^*$-semirings. This characterization corresponds to Kozen's
axiomatization of regular languages.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 12:45:00 GMT"
},
{
"version": "v2",
"created": "Tue, 9 Dec 2008 14:11:09 GMT"
}
] | 2008-12-09T00:00:00 | [
[
"Bloom",
"S. L.",
""
],
[
"Esik",
"Z.",
""
]
] | [
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] |
712.1338 | Dipanjan Mitra | Dipanjan Mitra, Joanna M Rankin | On the Subpulse Modulation, Polarization and Subbeam Carousel
Configuration of Pulsar B1857--26 | Accepted for publication in MNRAS | AIPConf.Proc.983:109-111,2008 | 10.1063/1.2900116 | null | astro-ph | null | New GMRT observations of the five-component pulsar B1857--26 provide detailed
insight into its pulse-sequence modulation phenomena for the first time. The
outer conal components exhibit a 7.4-rotation-period, longitude-stationary
modulation. Several lines of evidence indicate a carousel circulation time
$\P3hat$ of about 147 stellar rotations, characteristic of a pattern with 20
beamlets. The pulsar nulls some 20% of the time, usually for only a single
pulse, and these nulls show no discernible order or periodicity. Finally, the
pulsar's polarization-angle traverse raises interesting issues: if most of its
emission is comprised of a single polarization mode, the full traverse exceeds
180\degr; or if both polarization modes are present, then the leading and the
trailing halves of the profiles exhibit two different modes. In either case the
rotating vector model fails to fit the polarization-angle traverse of the core
component.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 06:00:24 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mitra",
"Dipanjan",
""
],
[
"Rankin",
"Joanna M",
""
]
] | [
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] |
712.1339 | Stefano Buzzi | Stefano Buzzi and H. Vincent Poor | Joint Receiver and Transmitter Optimization for Energy-Efficient CDMA
Communications | To appear in the IEEE Journal on Selected Areas in Communications -
Special Issue on Multiuser Detection for Advanced Communication Systems and
Networks | null | null | null | cs.IT cs.GT math.IT | null | This paper focuses on the cross-layer issue of joint multiuser detection and
resource allocation for energy efficiency in wireless CDMA networks. In
particular, assuming that a linear multiuser detector is adopted in the uplink
receiver, the case considered is that in which each terminal is allowed to vary
its transmit power, spreading code, and uplink receiver in order to maximize
its own utility, which is defined as the ratio of data throughput to transmit
power. Resorting to a game-theoretic formulation, a non-cooperative game for
utility maximization is formulated, and it is proved that a unique Nash
equilibrium exists, which, under certain conditions, is also Pareto-optimal.
Theoretical results concerning the relationship between the problems of SINR
maximization and MSE minimization are given, and, resorting to the tools of
large system analysis, a new distributed power control algorithm is
implemented, based on very little prior information about the user of interest.
The utility profile achieved by the active users in a large CDMA system is also
computed, and, moreover, the centralized socially optimum solution is analyzed.
Considerations on the extension of the proposed framework to a multi-cell
scenario are also briefly detailed. Simulation results confirm that the
proposed non-cooperative game largely outperforms competing alternatives, and
that it exhibits a quite small performance loss with respect to the socially
optimum solution, and only in the case in which the users number exceeds the
processing gain. Finally, results also show an excellent agreement between the
theoretical closed-form formulas based on large system analysis and the outcome
of numerical experiments.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 17:26:24 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Buzzi",
"Stefano",
""
],
[
"Poor",
"H. Vincent",
""
]
] | [
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] |
712.134 | Oleg Kochukhov | M. Sachkov, O. Kochukhov, T. Ryabchikova, F. Leone, S. Bagnulo, W.W.
Weiss | Spectroscopic study of pulsations in the atmosphere of roAp star 10 Aql | submitted to Contrib. Astron. Obs. Skalnate Pleso (Proceedings of the
CP#Ap Workshop, Vienna, 2007, eds. J. Ziznovsky, J. Zverko, E. Pauntzen, M.
Netopil) | Contrib.Astron.Obs.Skalnate Pleso 38:323-328,2008 | null | null | astro-ph | null | We present the analysis of spectroscopic time-series observations of the roAp
star 10 Aql. Observations were carried out in July 2006 with the UVES and SARG
spectrographs simultaneously with the MOST mini-satellite photometry. All these
data were analysed for radial velocity (RV) variations. About 150 lines out of
the 1000 measured reveal clear pulsation signal. Frequency analysis of the
spectroscopic data gives four frequencies. Three highest amplitude frequencies
in spectroscopy coincide with the photometric ones. Phase-amplitude diagrams
created for the lines of different elements/ions show that atmospheric
pulsations may be represented by a superposition of the standing and running
wave components, similar to other roAp stars. The highest RV amplitudes,
300-400 m/s, were measured for Ce II, Dy III, Tb III, and two unidentified
lines at lambda 5471, 5556 A. We discovered ~0.4 period phase jump in the RV
measurements across the Nd III line profiles. It indicates the presence of the
pulsation node in stellar atmosphere. The phase jump occurs at nearly the same
atmospheric layers for the two main frequencies. There is no rotational
modulation in the average spectra for the 6 different nights we analysed.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 14:38:16 GMT"
}
] | 2010-11-26T00:00:00 | [
[
"Sachkov",
"M.",
""
],
[
"Kochukhov",
"O.",
""
],
[
"Ryabchikova",
"T.",
""
],
[
"Leone",
"F.",
""
],
[
"Bagnulo",
"S.",
""
],
[
"Weiss",
"W. W.",
""
]
] | [
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712.1341 | Lisa L. Everett | Durmus A. Demir, Lisa L. Everett, and Paul Langacker | Dirac Neutrino Masses from Generalized Supersymmetry Breaking | 5 pages, 1 figure, references added, note added on effective
superpotential mass terms generated upon U(1)' breaking | Phys.Rev.Lett.100:091804, 2008 | 10.1103/PhysRevLett.100.091804 | MADPH-07-1500, IZTECH-P-07/05, DESY-07-213 | hep-ph hep-th | null | We demonstrate that Dirac neutrino masses in the experimentally preferred
range are generated within supersymmetric gauge extensions of the Standard
Model with a generalized supersymmetry breaking sector. If the usual
superpotential Yukawa couplings are forbidden by the additional gauge symmetry
(such as a U(1)'), effective Dirac mass terms involving the "wrong Higgs" field
can arise either at tree level due to hard supersymmetry breaking fermion
Yukawa couplings, or at one-loop due to nonanalytic or "nonholomorphic" soft
supersymmetry breaking trilinear scalar couplings. As both of these operators
are naturally suppressed in generic models of supersymmetry breaking, the
resulting neutrino masses are naturally in the sub-eV range. The neutrino
magnetic and electric dipole moments resulting from the radiative mechanism
also vanish at one-loop order.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 15:06:44 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 22:47:16 GMT"
}
] | 2011-01-28T00:00:00 | [
[
"Demir",
"Durmus A.",
""
],
[
"Everett",
"Lisa L.",
""
],
[
"Langacker",
"Paul",
""
]
] | [
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] |
712.1342 | Heng Lian | Heng Lian | Stochastic adaptation of importance sampler | 11 pages, minor changes | null | null | null | stat.ME | null | Improving efficiency of importance sampler is at the center of research in
Monte Carlo methods. While adaptive approach is usually difficult within the
Markov Chain Monte Carlo framework, the counterpart in importance sampling can
be justified and validated easily. We propose an iterative adaptation method
for learning the proposal distribution of an importance sampler based on
stochastic approximation. The stochastic approximation method can recruit
general iterative optimization techniques like the minorization-maximization
algorithm. The effectiveness of the approach in optimizing the Kullback
divergence between the proposal distribution and the target is demonstrated
using several simple examples.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 05:24:26 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Lian",
"Heng",
""
]
] | [
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] |
712.1343 | Giorgio Fabbri | A. Brace, G. Fabbri, B. Goldys | An Hilbert space approach for a class of arbitrage free implied
volatilities models | 21 pages | null | null | null | q-fin.CP math.PR | null | We present an Hilbert space formulation for a set of implied volatility
models introduced in \cite{BraceGoldys01} in which the authors studied
conditions for a family of European call options, varying the maturing time and
the strike price $T$ an $K$, to be arbitrage free. The arbitrage free
conditions give a system of stochastic PDEs for the evolution of the implied
volatility surface ${\hat\sigma}_t(T,K)$. We will focus on the family obtained
fixing a strike $K$ and varying $T$. In order to give conditions to prove an
existence-and-uniqueness result for the solution of the system it is here
expressed in terms of the square root of the forward implied volatility and
rewritten in an Hilbert space setting. The existence and the uniqueness for the
(arbitrage free) evolution of the forward implied volatility, and then of the
the implied volatility, among a class of models, are proved. Specific examples
are also given.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 15:36:46 GMT"
},
{
"version": "v2",
"created": "Sat, 15 Dec 2007 10:30:59 GMT"
}
] | 2008-12-10T00:00:00 | [
[
"Brace",
"A.",
""
],
[
"Fabbri",
"G.",
""
],
[
"Goldys",
"B.",
""
]
] | [
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] |
712.1344 | Adriano Barra Dr. | Adriano Barra | The mean field Ising model trough interpolating techniques | 35 pages, no figure | null | 10.1007/s10955-008-9567-2 | null | cond-mat.dis-nn | null | Aim of this work is not trying to explore a macroscopic behavior of some
recent model in statistical mechanics but showing how some recent techniques
developed within the framework of spin glasses do work on simpler model,
focusing on the method and not on the analyzed system. To fulfil our will the
candidate model turns out to be the paradigmatic mean field Ising model. The
model is introduced and investigated with the interpolation techniques. We show
the existence of the thermodynamic limit, bounds for the free energy density,
the explicit expression for the free energy with its suitable expansion via the
order parameter, the self-consistency relation, the phase transition, the
critical behavior and the self-averaging properties. At the end a bridge to a
Parisi-like theory is tried and discussed.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 16:19:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Barra",
"Adriano",
""
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712.1345 | Giorgi Japaridze | Giorgi Japaridze | Sequential operators in computability logic | To appear in "Information and Computation" | Information and Computation 206 (2008), pp. 1443-1475 | 10.1016/j.ic.2008.10.001 | null | cs.LO cs.AI math.LO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Computability logic (CL) (see http://www.cis.upenn.edu/~giorgi/cl.html) is a
semantical platform and research program for redeveloping logic as a formal
theory of computability, as opposed to the formal theory of truth which it has
more traditionally been. Formulas in CL stand for (interactive) computational
problems, understood as games between a machine and its environment; logical
operators represent operations on such entities; and "truth" is understood as
existence of an effective solution, i.e., of an algorithmic winning strategy.
The formalism of CL is open-ended, and may undergo series of extensions as
the study of the subject advances. The main groups of operators on which CL has
been focused so far are the parallel, choice, branching, and blind operators.
The present paper introduces a new important group of operators, called
sequential. The latter come in the form of sequential conjunction and
disjunction, sequential quantifiers, and sequential recurrences. As the name
may suggest, the algorithmic intuitions associated with this group are those of
sequential computations, as opposed to the intuitions of parallel computations
associated with the parallel group of operations: playing a sequential
combination of games means playing its components in a sequential fashion, one
after one.
The main technical result of the present paper is a sound and complete
axiomatization of the propositional fragment of computability logic whose
vocabulary, together with negation, includes all three -- parallel, choice and
sequential -- sorts of conjunction and disjunction. An extension of this result
to the first-order level is also outlined.
| [
{
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},
{
"version": "v2",
"created": "Wed, 15 Oct 2008 07:44:55 GMT"
}
] | 2011-04-15T00:00:00 | [
[
"Japaridze",
"Giorgi",
""
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712.1346 | Emilio Elizalde | Emilio Elizalde | Zeta Function Methods and Quantum Fluctuations | 17 pages, Talk given at the Conference ``Quantum Theory and
Symmetries - 5'', Valladolid (Spain), July 22 - 28, 2007 | J.Phys.A41:304040,2008 | 10.1088/1751-8113/41/30/304040 | null | hep-th gr-qc math-ph math.MP quant-ph | null | A review of some recent advances in zeta function techniques is given, in
problems of pure mathematical nature but also as applied to the computation of
quantum vacuum fluctuations in different field theories, and specially with a
view to cosmological applications.
| [
{
"version": "v1",
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[
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] |
712.1347 | Emilio Elizalde | Emilio Elizalde | Dynamical Casimir Effect with Semi-Transparent Mirrors, and Cosmology | 11 pages, Talk given in the Workshop ``Quantum Field Theory under the
Influence of External Conditions (QFEXT07)'', Leipzig (Germany), September 17
- 21, 2007 | J.Phys.A41:164061,2008 | 10.1088/1751-8113/41/16/164061 | null | hep-th astro-ph gr-qc quant-ph | null | After reviewing some essential features of the Casimir effect and,
specifically, of its regularization by zeta function and Hadamard methods, we
consider the dynamical Casimir effect (or Fulling-Davis theory), where related
regularization problems appear, with a view to an experimental verification of
this theory. We finish with a discussion of the possible contribution of vacuum
fluctuations to dark energy, in a Casimir like fashion, that might involve the
dynamical version.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 17:09:20 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Elizalde",
"Emilio",
""
]
] | [
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712.1348 | Patrick Wils | Patrick Wils, Ioannis Rozakis, Stelios Kleidis, Franz-Josef Hambsch,
Klaus Bernhard | Photometry of GSC 762-110, a new triple-mode radially pulsating star | Accepted for publication in Astronomy & Astrophysics | null | 10.1051/0004-6361:20078992 | null | astro-ph | null | Stars pulsating in three radial modes are very rare; only three examples are
known in the Galaxy. These stars are very useful since their periods may be
measured very precisely, and this will constrain the global stellar parameters
and the models of the star's interior. The purpose of this paper is to present
a new example of the class of triple-mode radial pulsators. A search for
candidate multi-mode pulsators was carried out in public survey data.
Time-series photometry of one of the candidates, GSC 762-110, was performed.
GSC 762-110 was found to be a triple-mode radial pulsator, with a fundamental
period of 0.1945d and period ratios of 0.7641 and 0.8012. In addition two
non-radial modes were found, for which the amplitude has diminished
considerably over the last few years.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 17:11:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wils",
"Patrick",
""
],
[
"Rozakis",
"Ioannis",
""
],
[
"Kleidis",
"Stelios",
""
],
[
"Hambsch",
"Franz-Josef",
""
],
[
"Bernhard",
"Klaus",
""
]
] | [
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712.1349 | Petr Nicolaevich Bibikov | P. N. Bibikov | Low- and high-field induced uniform and staggered magnetizations of a
spin ladder with DM term | 7 pages | null | null | null | cond-mat.str-el | null | Analytic expressions for uniform and staggered magnetizations of a spin
ladder with a staggered Dzyaloshinskii-Moriya interaction along rungs are
obtained in the lowest perturbative orders. The obtained formulas describe
magnetic behavior in two marginal regions related to low ($h\ll h_c$) and high
($h\gg h_s$) magnetic fields.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 17:13:50 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Bibikov",
"P. N.",
""
]
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] |
712.135 | Mark Slater | M. Slater, C. Adolphsen, R. Arnold, S. Boogert, G. Boorman, F.
Gournaris, M. Hildreth, C. Hlaing, F. Jackson, O. Khainovski, Yu. G.
Kolomensky, A. Lyapin, B. Maiheu, D. McCormick, D. J. Miller, T. J. Orimoto,
Z. Szalata, M. Thomson, D. Ward, M. Wing, M. Woods | Cavity BPM System Tests for the ILC Spectrometer | Paper submitted to Nuclear Instruments and Methods. 35 pages, 23
figures | null | 10.1016/j.nima.2008.04.033 | null | physics.ins-det | null | The main physics programme of the International Linear Collider (ILC)
requires a measurement of the beam energy at the interaction point with an
accuracy of $10^{-4}$ or better. To achieve this goal a magnetic spectrometer
using high resolution beam position monitors (BPMs) has been proposed. This
paper reports on the cavity BPM system that was deployed to test this proposal.
We demonstrate sub-micron resolution and micron level stability over 20 hours
for a $1\m$ long BPM triplet. We find micron-level stability over 1 hour for 3
BPM stations distributed over a $30\m$ long baseline. The understanding of the
behaviour and response of the BPMs gained from this work has allowed full
spectrometer tests to be carried out.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 17:50:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Slater",
"M.",
""
],
[
"Adolphsen",
"C.",
""
],
[
"Arnold",
"R.",
""
],
[
"Boogert",
"S.",
""
],
[
"Boorman",
"G.",
""
],
[
"Gournaris",
"F.",
""
],
[
"Hildreth",
"M.",
""
],
[
"Hlaing",
"C.",
""
],
[
"Jackson",
"F.",
""
],
[
"Khainovski",
"O.",
""
],
[
"Kolomensky",
"Yu. G.",
""
],
[
"Lyapin",
"A.",
""
],
[
"Maiheu",
"B.",
""
],
[
"McCormick",
"D.",
""
],
[
"Miller",
"D. J.",
""
],
[
"Orimoto",
"T. J.",
""
],
[
"Szalata",
"Z.",
""
],
[
"Thomson",
"M.",
""
],
[
"Ward",
"D.",
""
],
[
"Wing",
"M.",
""
],
[
"Woods",
"M.",
""
]
] | [
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] |
712.1351 | V\'ictor M. Egu\'iluz | V\'ictor M. Egu\'iluz (1), Mart\'in G. Zimmermann (2), Camilo J.
Cela-Conde (3), Maxi San Miguel (1) ((1) IMEDEA (CSIC-UIB), Spain, (2)
Universidad de Buenos Aires, Argentina, (3) Universidad de las Islas
Baleares, Spain) | Cooperation and the Emergence of Role Differentiation in the Dynamics of
Social Networks | (15 pages, 7 figures) | American Journal of Sociology 110, 977-1008 (2005) | 10.1086/428716 | null | physics.soc-ph | null | By means of extensive computer simulations, the authors consider the
entangled coevolution of actions and social structure in a new version of a
spatial Prisoner's Dilemma model that naturally gives way to a process of
social differentiation. Diverse social roles emerge from the dynamics of the
system: leaders are individuals getting a large payoff who are imitated by a
considerable fraction of the population, conformists are unsatisfied
cooperative agents that keep cooperating, and exploiters are defectors with a
payoff larger than the average one obtained by cooperators. The dynamics
generate a social network that can have the topology of a small world network.
The network has a strong hierarchical structure in which the leaders play an
essential role in sustaining a highly cooperative stable regime. But
disruptions affecting leaders produce social crises described as dynamical
cascades that propagate through the network.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 19:46:01 GMT"
}
] | 2011-06-16T00:00:00 | [
[
"Eguíluz",
"Víctor M.",
""
],
[
"Zimmermann",
"Martín G.",
""
],
[
"Cela-Conde",
"Camilo J.",
""
],
[
"Miguel",
"Maxi San",
""
]
] | [
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] |
712.1352 | Yaroslav Zolotaryuk | Yaroslav Zolotaryuk | Resonant fluxon transmission through impurities | 8 figures | null | 10.1140/epjb/e2008-00152-7 | null | nlin.PS | null | Fluxon transmission through several impurities of different strength and type
(i.e., microshorts and microresistors), placed in a long Josephson junction is
investigated. Threshold pinning current on the impurities is computed as a
function of the distance between them, their amplitudes and the dissipation
parameter. It is shown that in the case of consequently placed microshorts or
microresistors, the threshold pinning current exhibits a clear minimum as a
function of the distance between the impurities. In the case of a
microresistor, followed by a microshort, an opposite phenomenon is observed,
namely the threshold pinning current exhibits maximum as a function of the
distance between the impurities.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 18:19:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zolotaryuk",
"Yaroslav",
""
]
] | [
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] |
712.1353 | Deborah Nancy Aguilera | Deborah N. Aguilera, Jos\'e A. Pons and Juan A. Miralles | The impact of magnetic field on the thermal evolution of neutron stars | 4 pages, 3 figures, 1 table. Accepted for publication in APJ Letters | Astrophys.J.673:L167-L170,2008 | 10.1086/527547 | null | astro-ph hep-ph nucl-th | null | The impact of strong magnetic fields B>10e13 G on the thermal evolution of
neutron stars is investigated, including crustal heating by magnetic field
decay. For this purpose, we perform 2D cooling simulations with anisotropic
thermal conductivity considering all relevant neutrino emission processes for
realistic neutron stars. The standard cooling models of neutron stars are
called into question by showing that the magnetic field has relevant (and in
many cases dominant) effects on the thermal evolution. The presence of the
magnetic field significantly affects the thermal surface distribution and the
cooling history of these objects during both, the early neutrino cooling era
and the late photon cooling era. The minimal cooling scenario is thus more
complex than generally assumed. A consistent magneto-thermal evolution of
magnetized neutron stars is needed to explain the observations.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 18:40:58 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Aguilera",
"Deborah N.",
""
],
[
"Pons",
"José A.",
""
],
[
"Miralles",
"Juan A.",
""
]
] | [
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] |
712.1354 | Holger Fehske | H. Fehske, G. Wellein, J. Loos, and A. R. Bishop | Localized polarons and doorway vibrons in finite quantum structures | corrected Figs 5 and 6, updated references | Physical Review B 77, 085117 (2008) | 10.1103/PhysRevB.77.085117 | null | cond-mat.str-el | null | We consider transport through finite quantum systems such as quantum
barriers, wells, dots or junctions, coupled to local vibrational modes in the
quantal regime. As a generic model we study the Holstein-Hubbard Hamiltonian
with site-dependent potentials and interactions. Depending on the barrier
height to electron-phonon coupling strength ratio and the phonon frequency we
find distinct opposed behaviors: Vibration-mediated tunneling or intrinsic
localization of (bi)polarons. These regimes are strongly manifested in the
density correlations, mobility, and optical response calculated by exact
numerical techniques.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 18:37:15 GMT"
},
{
"version": "v2",
"created": "Sat, 23 Feb 2008 17:01:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Fehske",
"H.",
""
],
[
"Wellein",
"G.",
""
],
[
"Loos",
"J.",
""
],
[
"Bishop",
"A. R.",
""
]
] | [
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] |
712.1355 | Michael Dine | Michael Dine and John Mason | Dynamical Supersymmetry Breaking and Low Energy Gauge Mediation | 20 pages (minor change in referencing) | Phys.Rev.D78:055013,2008 | 10.1103/PhysRevD.78.055013 | SCIPP-07/18 | hep-ph | null | Dynamical breaking of supersymmetry was long thought to be an exceptional
phenomenon, but recent developments have altered this view. A question of great
interest in the current framework is the value of the underlying scale of
supersymmetry breaking. The "little hierarchy" problem suggests that
supersymmetry should be broken at low energies. Within one class of models, low
energy breaking be achieved as a consequence of symmetries, without requiring
odd coincidences. The low energy theories are distinguished by the presence or
absence of $R$ symmetries; in either case, and especially the latter one often
finds modifications of the minimal gauge-mediated spectrum which can further
ameliorate problems of fine tuning. Various natural mechanisms exist to solve
the $\mu$ problem in this framework.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 19:28:13 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Dec 2007 19:17:26 GMT"
}
] | 2009-01-09T00:00:00 | [
[
"Dine",
"Michael",
""
],
[
"Mason",
"John",
""
]
] | [
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] |
712.1356 | Ilian Iliev | Ilian T. Iliev (1), Garrelt Mellema (2), Ue-Li Pen (3), Paul R.
Shapiro (4) ((1) ITP, University of Zurich, (2) Stockholm University, (3)
CITA, University of Toronto, (4) University of Texas) | Character and detectability of the dark ages and the epoch of
reionization: the view from the simulations | 5 pages, 5 figures (most in color). In Proceedings of "From planets
to dark energy: the modern radio universe", October 1-5 2007, University of
Manchester, Manchester, UK. To appear in Proceedings of Science online
journal | PoSMRU:01118,2007 | null | null | astro-ph | null | Direct detection of the Dark Ages and the Epoch of Reionization
(EOR) is among the main scientific objectives of all current and future
low-frequency radio facilities. In this paper we summarize and discuss recent
results, based on state-of-the-art numerical simulations, regarding the
fundamental EOR properties and its observability with current and future radio
arrays, like the Giant Metrewave Radio Telescope (GMRT), the Low Frequency
Array (LOFAR), the 21-CM Array (21CMA), the Murchison Widefield Array (MWA) and
the Square Kilometre Array (SKA). Results show that the optimal observational
frequencies for statistical detection are 140-160 MHz. The signals are strongly
non-Gaussian at late times. The correlation widths between 21-cm maps at
neighbouring frequencies are short, of order 300-800 kHz, which should help
with the cleaning of the strong foregrounds. Direct comparison of the
resolutions and expected sensitivities of GMRT and MWA indicate that their
optimal sensitivity ranges are similar, at scales k~0.2-0.4 h/Mpc, however, all
else being equal the former should require shorter integration times due to its
significantly larger collecting area.
| [
{
"version": "v1",
"created": "Mon, 10 Dec 2007 20:51:39 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Iliev",
"Ilian T.",
""
],
[
"Mellema",
"Garrelt",
""
],
[
"Pen",
"Ue-Li",
""
],
[
"Shapiro",
"Paul R.",
""
]
] | [
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712.1357 | Shelly Garion | Shelly Garion | Connectivity of the Product Replacement Algorithm Graph of PSL(2,q) | 12 pages. This article was submitted to the Journal of Group Theory
on July 2007 and accepted on December 2007 | J. Group Theory 11 (2008), 765-777 | 10.1515/JGT.2008.048 | null | math.GR | null | The product replacement algorithm is a practical algorithm to construct
random elements of a finite group G. It can be described as a random walk on a
graph whose vertices are the generating k-tuples of G (for a fixed k). We show
that if G is PSL(2,q) or PGL(2,q), where q is a prime power, then this graph is
connected for any k>=4. This generalizes former results obtained by Gilman and
Evans.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 19:41:14 GMT"
},
{
"version": "v2",
"created": "Sun, 30 Dec 2007 18:36:16 GMT"
}
] | 2010-03-17T00:00:00 | [
[
"Garion",
"Shelly",
""
]
] | [
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712.1358 | Mariusz Dabrowski P. | Mariusz P. Dabrowski and Janusz Garecki | Energy, angular momentum, superenergy and angular supermomentum in
conformal frames | REVTEX 4, 21 pages, no figures, minor changes, references added | null | null | null | hep-th astro-ph gr-qc | null | We find the rules of the conformal transformation for the energetic
quantities such as the Einstein energy-momentum complex, the Bergmann-Thomson
angular momentum complex, the superenergy tensor, and the angular supermomentum
tensor of gravitation and matter. We show that the conformal transformation
rules for the matter parts of both the Einstein complex and the
Bergmann-Thomson complex are fairly simple, while the transformation rules for
their gravitational parts are more complicated. We also find that the
transformational rules of the superenergy tensor of matter and the superenergy
tensor of gravity are quite complicated except for the case of a pure gravity.
In such a special case the superenergy density as well as the sum of the
superenergy density and the matter energy density are invariants of the
conformal transformation. Besides, in that case, a conformal invariant is also
the Bel-Robinson tensor which is a part of the superenergy tensor. As for the
angular supermomentum tensor of gravity - it emerges that its transformational
rule even for a pure gravity is quite complicated but this is not the case for
the angular supermomentum tensor of matter. Having investigated some
technicalities of the conformal transformations, we also find the conformal
transformation rule for the curvature invariants and, in particular, for the
Gauss-Bonnet invariant in a spacetime of arbitrary dimension.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 19:43:26 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Dec 2007 20:02:34 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Dabrowski",
"Mariusz P.",
""
],
[
"Garecki",
"Janusz",
""
]
] | [
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712.1359 | Olivier Finkel | Olivier Finkel (ELM) | Borel Ranks and Wadge Degrees of Context Free Omega Languages | null | Mathematical Structures in Computer Science 16 (5) (2006) 813-840 | null | null | cs.LO cs.GT math.LO | null | We show that, from a topological point of view, considering the Borel and the
Wadge hierarchies, 1-counter B\"uchi automata have the same accepting power
than Turing machines equipped with a B\"uchi acceptance condition. In
particular, for every non null recursive ordinal alpha, there exist some
Sigma^0_alpha-complete and some Pi^0_alpha-complete omega context free
languages accepted by 1-counter B\"uchi automata, and the supremum of the set
of Borel ranks of context free omega languages is the ordinal gamma^1_2 which
is strictly greater than the first non recursive ordinal. This very surprising
result gives answers to questions of H. Lescow and W. Thomas [Logical
Specifications of Infinite Computations, In:"A Decade of Concurrency", LNCS
803, Springer, 1994, p. 583-621].
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:01:02 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Finkel",
"Olivier",
"",
"ELM"
]
] | [
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712.136 | Deanna Needell | Deanna Needell and Roman Vershynin | Signal Recovery from Incomplete and Inaccurate Measurements via
Regularized Orthogonal Matching Pursuit | null | null | null | null | math.NA | null | We demonstrate a simple greedy algorithm that can reliably recover a
d-dimensional vector v from incomplete and inaccurate measurements x. Here our
measurement matrix is an N by d matrix with N much smaller than d. Our
algorithm, Regularized Orthogonal Matching Pursuit (ROMP), seeks to close the
gap between two major approaches to sparse recovery. It combines the speed and
ease of implementation of the greedy methods with the strong guarantees of the
convex programming methods. For any measurement matrix that satisfies a Uniform
Uncertainty Principle, ROMP recovers a signal with O(n) nonzeros from its
inaccurate measurements x in at most n iterations, where each iteration amounts
to solving a Least Squares Problem. The noise level of the recovery is
proportional to the norm of the error, up to a log factor. In particular, if
the error vanishes the reconstruction is exact. This stability result extends
naturally to the very accurate recovery of approximately sparse signals.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:05:19 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Needell",
"Deanna",
""
],
[
"Vershynin",
"Roman",
""
]
] | [
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] |
712.1361 | Heng-Yu Chen HYC | Heng-Yu Chen, Diego H. Correa | Comments on the Boundary Scattering Phase | 14 pages, 2 figures; v2: affiliation corrected | JHEP0802:028,2008 | 10.1088/1126-6708/2008/02/028 | DAMTP-07-114, MAD-TH-07-12 | hep-th | null | We present a simple solution to the crossing equation for an open string
worldsheet reflection matrix, with boundaries preserving a SU(1|2)^2 residual
symmetry, which constrains the boundary dressing factor. In addition, we also
propose an analogous crossing equation for the dressing factor where extra
boundary degrees of freedom preserve a SU(2|2)^2 residual symmetry.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:16:37 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Mar 2008 10:07:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chen",
"Heng-Yu",
""
],
[
"Correa",
"Diego H.",
""
]
] | [
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712.1362 | Stuart Parkin | Hyunsoo Yang, See-Hun Yang and Stuart Parkin | Crossover from Kondo assisted suppression to co-tunneling enhancement of
tunneling magnetoresistance via ferromagnetic nanodots in MgO tunnel barriers | Nano Letters (in press) | null | 10.1021/nl072930n | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | Recently, it has been shown that magnetic tunnel junctions with thin MgO
tunnel barriers exhibit extraordinarily high tunneling magnetoresistance (TMR)
values at room temperature1, 2. However, the physics of spin dependent
tunneling through MgO barriers is only beginning to be unravelled. Using planar
magnetic tunnel junctions in which ultra-thin layers of magnetic metals are
deposited in the middle of a MgO tunnel barrier here we demonstrate that the
TMR is strongly modified when these layers are discontinuous and composed of
small pancake shaped nanodots. At low temperatures, in the Coulomb blockade
regime, for layers less than ~1 nm thick, the conductance of the junction is
increased at low bias consistent with Kondo assisted tunneling. In the same
regime we observe a suppression of the TMR. For slightly thicker layers, and
correspondingly larger nanodots, the TMR is enhanced at low bias, consistent
with co-tunneling.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:11:29 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Yang",
"Hyunsoo",
""
],
[
"Yang",
"See-Hun",
""
],
[
"Parkin",
"Stuart",
""
]
] | [
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712.1363 | Olivier Finkel | Olivier Finkel (ELM) | Undecidable Problems About Timed Automata | null | Dans Proceedings of the 4th International Conference on Formal
Modelling and Analysis of Timed Systems - FORMATS'06, France (2006) | null | null | cs.LO cs.CC math.LO | null | We solve some decision problems for timed automata which were recently raised
by S. Tripakis in [ Folk Theorems on the Determinization and Minimization of
Timed Automata, in the Proceedings of the International Workshop FORMATS'2003,
LNCS, Volume 2791, p. 182-188, 2004 ] and by E. Asarin in [ Challenges in Timed
Languages, From Applied Theory to Basic Theory, Bulletin of the EATCS, Volume
83, p. 106-120, 2004 ]. In particular, we show that one cannot decide whether a
given timed automaton is determinizable or whether the complement of a timed
regular language is timed regular. We show that the problem of the minimization
of the number of clocks of a timed automaton is undecidable. It is also
undecidable whether the shuffle of two timed regular languages is timed
regular. We show that in the case of timed B\"uchi automata accepting infinite
timed words some of these problems are Pi^1_1-hard, hence highly undecidable
(located beyond the arithmetical hierarchy).
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:11:42 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Finkel",
"Olivier",
"",
"ELM"
]
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712.1364 | Stefano Gandolfi | Stefano Gandolfi | The Auxiliary Field Diffusion Monte Carlo Method for Nuclear Physics and
Nuclear Astrophysics | Ph.D. thesis at University of Trento, Italy. 121 pages | null | null | null | nucl-th astro-ph cond-mat.other | null | In this thesis, I discuss the use of the Auxiliary Field Diffusion Monte
Carlo method to compute the ground state of nuclear Hamiltonians, and I show
several applications to interesting problems both in nuclear physics and in
nuclear astrophysics.
In particular, the AFDMC algorithm is applied to the study of several nuclear
systems, finite, and infinite matter. Results about the ground state of nuclei
($^4$He, $^8$He, $^{16}$O and $^{40}$Ca), neutron drops (with 8 and 20
neutrons) and neutron rich-nuclei (isotopes of oxygen and calcium) are
discussed, and the equation of state of nuclear and neutron matter are
calculated and compared with other many-body calculations. The $^1S_0$
superfluid phase of neutron matter in the low-density regime was also studied.
| [
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712.1365 | Alexei Vazquez | Alexei Vazquez | Population stratification using a statistical model on hypergraphs | 7 pages, 6 figures | Phys. Rev. E 77, 066106 (2008) | 10.1103/PhysRevE.77.066106 | null | q-bio.PE cs.AI physics.data-an | null | Population stratification is a problem encountered in several areas of
biology and public health. We tackle this problem by mapping a population and
its elements attributes into a hypergraph, a natural extension of the concept
of graph or network to encode associations among any number of elements. On
this hypergraph, we construct a statistical model reflecting our intuition
about how the elements attributes can emerge from a postulated population
structure. Finally, we introduce the concept of stratification
representativeness as a mean to identify the simplest stratification already
containing most of the information about the population structure. We
demonstrate the power of this framework stratifying an animal and a human
population based on phenotypic and genotypic properties, respectively.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 20:53:45 GMT"
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[
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""
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712.1366 | Erwin Mi\~na-D\'iaz | Erwin Mi\~na-D\'iaz | An expansion for polynomials orthogonal over an analytic Jordan curve | 15 pages, 1 figure | Communications in Mathematical Physics. Vol. 285, 3:1109-1128
(2009) | 10.1007/s00220-008-0541-2 | null | math.CA math.CV | null | We consider polynomials that are orthogonal over an analytic Jordan curve L
with respect to a positive analytic weight, and show that each such polynomial
of sufficiently large degree can be expanded in a series of certain integral
transforms that converges uniformly in the whole complex plane. This expansion
yields, in particular and simultaneously, Szego's classical strong asymptotic
formula and a new integral representation for the polynomials inside L. We
further exploit such a representation to derive finer asymptotic results for
weights having finitely many singularities (all of algebraic type) on a thin
neighborhood of the orthogonality curve. Our results are a generalization of
those previously obtained in [7] for the case of L being the unit circle.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:02:03 GMT"
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] | 2009-03-19T00:00:00 | [
[
"Miña-Díaz",
"Erwin",
""
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] |
712.1367 | Anatoly Svidzinsky | Daniel M. Greenberger, Noam Erez, Marlan O. Scully, Anatoly A.
Svidzinsky, M. Suhail Zubairy | Planck, Photon Statistics, and Bose-Einstein Condensation | Review paper, 58 pages, 10 figures | Progress in Optics, vol. 50, edited by E. Wolf, Elsevier,
Amsterdam, 275-330 (2007) | null | null | physics.optics physics.hist-ph | null | The interplay between optical and statistical physics is a rich and exciting
field of study. Black body radiation was the first application of photon
statistics, although it was initially treated as a problem of the cavity
oscillators in equilibrium with the photon field. However Planck surprisingly
resisted the idea that anything physical would be quantized for a long time
after he had solved the problem. We trace this development.
Then, after the invention of the laser itself, it proved difficult to develop
a theory of laser action that could account for photon statistics, i.e.
fluctuations near threshold. This was accomplished in 1965. After Bose-Einstein
condensation was successfully achieved, the same problem arose in this case.
The fluctuation problem had not been treated adequately even for the ideal Bose
gas. However this problem has now been solved using the same techniques as in
the theory of laser action.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:08:45 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Greenberger",
"Daniel M.",
""
],
[
"Erez",
"Noam",
""
],
[
"Scully",
"Marlan O.",
""
],
[
"Svidzinsky",
"Anatoly A.",
""
],
[
"Zubairy",
"M. Suhail",
""
]
] | [
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] |
712.1368 | Benoit Mosser | B. Mosser, F. Bouchy, M. Martic, et al | Asteroseismology of Procyon with SOPHIE | 7 pages, 7 figures | null | 10.1051/0004-6361:20078337 | null | astro-ph | null | This paper reports a 9-night asteroseismic observation program conducted in
January 2007 with the new spectrometer Sophie at the OHP 193-cm telescope, on
the F5 IV-V target Procyon A. This first asteroseismic program with Sophie was
intended to test the performance of the instrument with a bright but demanding
asteroseismic target and was part of a multisite network. The Sophie spectra
have been reduced with the data reduction software provided by OHP. The Procyon
asteroseismic data were then analyzed with statistical tools. The asymptotic
analysis has been conducted considering possible curvature in the echelle
diagram analysis. These observations have proven the efficient performance of
Sophie used as an asteroseismometer, and succeed in a clear detection of the
large spacing. An \'echelle diagram based on the 54-$\mu$Hz spacing shows clear
ridges. Identification of the peaks exhibits large spacings varying from about
52 $\mu$Hz to 56 $\mu$Hz.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:16:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mosser",
"B.",
""
],
[
"Bouchy",
"F.",
""
],
[
"Martic",
"M.",
""
]
] | [
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] |
712.1369 | Ivan Rungger | Ivan Rungger and Stefano Sanvito (School of Physics and CRANN, Trinity
College, Dublin, Ireland) | Accurate self-energy algorithm for quasi-1D systems | null | null | null | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | We present a complete prescription for the numerical calculation of surface
Green's functions and self-energies of semi-infinite quasi-onedimensional
systems. Our work extends the results of Sanvito et al. [1] generating a robust
algorithm to be used in conjunction with ab initio electronic structure
methods. We perform a detailed error analysis of the scheme and find that the
highest accuracy is found if no inversion of the usually ill conditioned
hopping matrix is involved. Even in this case however a transformation of the
hopping matrix that decreases its condition number is needed in order to limit
the size of the imaginary part of the wave-vectors. This is done in two
different ways, either by applying a singular value decomposition and setting a
lowest bound for the smallest singular value, or by adding a random matrix of
small amplitude. By using the first scheme the size of the Hamiltonian matrix
is reduced, making the computation considerably faster for large systems. For
most energies the method gives high accuracy, however in the presence of
surface states the error diverges due to the singularity in the self-energy. A
surface state is found at a particular energy if the set of solution
eigenvectors of the infinite system is linearly dependent. This is then used as
a criterion to detect surface states, and the error is limited by adding a
small imaginary part to the energy.
[1] S. Sanvito, C. J. Lambert, J. H. Jefferson, and A. M. Bratkovsky, Phys.
Rev. B 59, 11936 (1999).
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:43:13 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Rungger",
"Ivan",
"",
"School of Physics and CRANN, Trinity\n College, Dublin, Ireland"
],
[
"Sanvito",
"Stefano",
"",
"School of Physics and CRANN, Trinity\n College, Dublin, Ireland"
]
] | [
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] |
712.137 | Caroline Soubiran | C. Soubiran (1), O. Bienayme (2), T.V. Mishenina (3), V.V. Kovtyukh
(3) ((1) Laboratoire d'Astrophysique de Bordeaux, (2) Observatoire de
Strasbourg, (3) Odessa Observatory) | Vertical distribution of Galactic disk stars IV - AMR and AVR from clump
giants | 13 pages, 14 figures, accepted in A&A | null | 10.1051/0004-6361:20078788 | null | astro-ph | null | We present the parameters of 891 stars, mostly clump giants, including
atmospheric parameters, distances, absolute magnitudes, spatial velocities,
galactic orbits and ages. One part of this sample consists of local giants,
within 100 pc, with atmospheric parameters either estimated from our
spectroscopic observations at high resolution and high signal-to-noise ratio,
or retrieved from the literature. The other part of the sample includes 523
distant stars, which we have estimated atmospheric parameters from high
resolution but low signal-to-noise Echelle spectra. This new sample is
kinematically unbiased, with well-defined boundaries in magnitude and colours.
We revisit the basic properties of the Galactic thin disk as traced by clump
giants. We find the metallicity distribution to be different from that of
dwarfs, with less metal-rich stars. We find evidence for a vertical metallicity
gradient of -0.31 dex/kpc and for a transition at 4-5 Gyr in both the
metallicity and velocities. The age - metallicity relation (AMR), which
exhibits a very low dispersion, increases smoothly from 10 to 4 Gyr, with a
steeper increase for younger stars. The age-velocity relation (AVR) is
characterized by the saturation of the V and W dispersions at 5 Gyr, and
continuous heating in U.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:36:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Soubiran",
"C.",
""
],
[
"Bienayme",
"O.",
""
],
[
"Mishenina",
"T. V.",
""
],
[
"Kovtyukh",
"V. V.",
""
]
] | [
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] |
712.1371 | Constantin Loizides | Constantin Loizides (for the PHOBOS collaboration) | Recent Results from PHOBOS | 6 pages, 4 figures, talk given at SQM 2007 | J.Phys.G35:044006,2008 | 10.1088/0954-3899/35/4/044006 | null | nucl-ex | null | In this manuscript we give a short summary of recent physics results from
PHOBOS. Particular emphasis is put on elliptic flow, fluctuations in the
initial geometry and the recent measurements of elliptic flow fluctuations.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:42:57 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Loizides",
"Constantin",
"",
"for the PHOBOS collaboration"
]
] | [
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712.1372 | Kshitij Khare | Kshitij Khare | Dynkin's Isomorphism with Sign Structure | null | null | null | null | math.ST stat.TH | null | The Dynkin isomorphism associates a Gaussian field to a Markov chain. These
Gaussian fields can be used as priors for prediction and time series analysis.
Dynkin's construction gives Gaussian fields with all non-negative covariances.
We extend Dynkin's construction (by introducing a sign structure on the Markov
chain) to allow general covariance sign patterns.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 21:51:19 GMT"
}
] | 2007-12-11T00:00:00 | [
[
"Khare",
"Kshitij",
""
]
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] |
712.1373 | Andrey Ivanov B. | A.B.Ivanov | Behavior of bounded solutions of quasilinear elliptic equations on
Riemannian manifolds | null | null | 10.1007/s11503-008-1016-7 | null | math.AP | null | This paper deals with bounded solutions of quasilinear elliptic equations on
Riemannian manifolds satisfying special condition.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 22:17:04 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 17:18:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ivanov",
"A. B.",
""
]
] | [
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712.1374 | Fr\'ed\'eric Pont | F. Pont, H. Knutson, R. L. Gilliland, C. Moutou, D. Charbonneau | Detection of atmospheric haze on an extrasolar planet: The 0.55 - 1.05
micron transmission spectrum of HD189733b with the Hubble Space Telescope | 11 pages, MNRAS, accepted, minor corrections | null | 10.1111/j.1365-2966.2008.12852.x | null | astro-ph | null | The nearby transiting planet HD 189733b was observed during three transits
with the ACS camera of the Hubble Space Telescope in spectroscopic mode. The
resulting time series of 675 spectra covers the 550-1050 nm range, with a
resolution element of ~8 nm, at extremely high accuracy (signal-to-noise ratio
up to 10,000 in 50 nm intervals in each individual spectrum). Using these data,
we disentangle the effects of limb darkening, measurement systematics, and
spots on the surface of the host star, to calculate the wavelength dependence
of the effective transit radius to an accuracy of ~50 km. This constitutes the
``transmission spectrum'' of the planetary atmosphere. It indicates at each
wavelength at what height the planetary atmosphere becomes opaque to the
grazing stellar light during the transit. In this wavelength range, strong
features due to sodium, potassium and water are predicted by atmosphere models
for a planet like HD 189733b, but they can be hidden by broad absorption from
clouds or hazes higher up in the atmosphere.
We observed an almost featureless transmission spectrum between 550 and 1050
nm, with no indication of the expected sodium or potassium atomic absorption
features. Comparison of our results with the transit radius observed in the
near and mid-infrared (2-8 microns), and the slope of the spectrum, suggest the
presence of a haze of sub-micron particles in the upper atmosphere of the
planet.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 22:31:24 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Dec 2007 08:28:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Pont",
"F.",
""
],
[
"Knutson",
"H.",
""
],
[
"Gilliland",
"R. L.",
""
],
[
"Moutou",
"C.",
""
],
[
"Charbonneau",
"D.",
""
]
] | [
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] |
712.1375 | Jason Fulman | Jason Fulman | Commutation relations and Markov chains | 37 pages; referee suggestions implemented, discuss up-down chains as
well, slightly better bounds in Props. 5.6, 7.6 | null | null | null | math.PR math.CO | null | It is shown that the combinatorics of commutation relations is well suited
for analyzing the convergence rate of certain Markov chains. Examples studied
include random walk on irreducible representations, a local random walk on
partitions whose stationary distribution is the Ewens distribution, and some
birth-death chains.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 23:17:44 GMT"
},
{
"version": "v2",
"created": "Sun, 20 Jan 2008 22:44:39 GMT"
}
] | 2008-01-21T00:00:00 | [
[
"Fulman",
"Jason",
""
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] |
712.1376 | Toshiro Sakakibara | K. Yano, T. Sakakibara, T. Tayama, M. Yokoyama, H. Amitsuka, Y. Homma,
P. Miranovic, M. Ichioka, Y. Tsutsumi, and K. Machida | Field-angle-dependent specific heat measurements and gap determination
of a heavy fermion superconductor URu2Si2 | 4 pages, 5 figures, to appear in Phys. Rev. Lett | Phys. Rev. Lett. 100, 017004 (2008) | 10.1103/PhysRevLett.100.017004 | null | cond-mat.str-el cond-mat.supr-con | null | To identify the superconducting gap structure in URu2Si2 we perform
field-angle-dependent specific heat measurements for the two principal
orientations in addition to field rotations, and theoretical analysis based on
microscopic calculations. The Sommerfeld coefficient \gamma(H)'s in the mixed
state exhibit distinctively different field-dependence. This comes from point
nodes and substantial Pauli paramagnetic effect of URu2Si2. These two features
combined give rise to a consistent picture of superconducting properties,
including a possible first order transition of Hc2 at low temperatures.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 23:19:08 GMT"
}
] | 2010-03-31T00:00:00 | [
[
"Yano",
"K.",
""
],
[
"Sakakibara",
"T.",
""
],
[
"Tayama",
"T.",
""
],
[
"Yokoyama",
"M.",
""
],
[
"Amitsuka",
"H.",
""
],
[
"Homma",
"Y.",
""
],
[
"Miranovic",
"P.",
""
],
[
"Ichioka",
"M.",
""
],
[
"Tsutsumi",
"Y.",
""
],
[
"Machida",
"K.",
""
]
] | [
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] |
712.1377 | Zhenghan Wang | Eric Rowell, Richard Stong, Zhenghan Wang | On classification of modular tensor categories | Several references added. Minor revisions of the abstract,
introduction and Section 2. Error in one R-matrix eigenvalue for (A_1,2) in
the published version corrected | Comm. Math. Phys. 292 (2009) no. 2, 343--389 | null | null | math.QA cond-mat.mes-hall math.GT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We classify all unitary modular tensor categories (UMTCs) of rank $\leq 4$.
There are a total of 70 UMTCs of rank $\leq 4$ (Note that some authors would
have counted as 35 MTCs.) In our convention there are two trivial unitary MTCs
distinguished by the modular $S$ matrix $S=(\pm1)$. Each such UMTC can be
obtained from 10 non-trivial prime UMTCs by direct product, and some symmetry
operations.
UMTCs encode topological properties of anyonic quantum systems and can be
used to build fault-tolerant quantum computers. We conjecture that there are
only finitely many equivalence classes of MTCs for any given rank, and a UMTC
is universal for anyonic quantum computation if and only if its global quantum
dimension $D^2$ is \emph{not} an integer.
Discovery of non-abelain anyons in Nature will be a landmark in condensed
matter physics. The non-abelian anyons in UMTCs of rank $\leq 4$ are the
simplest, and, therefore, are most likely to be found. G. Moore and N. Read
proposed that non-abelian statistics could occur in fractional quantum Hall
(FQH) liquids. The Read-Rezayi conjecture predicts the existence of anyons
related to $SU(2)_k$ in FQH liquids at filling fractions $\nu=2+\frac{k}{k+2}$
for $k=1,2,3$. For $\nu={5/2}$ and $SU(2)_2$, there is a numerical proof and
experimental evidence for this conjecture. The Ising anyons might exist in
chiral superconductors (strontium ruthenate). There are theoretical designs for
the toric code MTC using Josephson junction array, for the $Fib\times Fib$ MTC
using optical lattice, and for the $SU(2)_k$ using cold trapped bosonic atoms.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 23:35:50 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 03:38:54 GMT"
},
{
"version": "v3",
"created": "Mon, 17 Dec 2007 03:22:04 GMT"
},
{
"version": "v4",
"created": "Mon, 9 Nov 2009 18:04:18 GMT"
}
] | 2009-11-09T00:00:00 | [
[
"Rowell",
"Eric",
""
],
[
"Stong",
"Richard",
""
],
[
"Wang",
"Zhenghan",
""
]
] | [
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712.1378 | Vladislav Kargin | Vladislav Kargin | Lyapunov Exponents of Free Operators | 16 pages | Journal of Functional Analysis, 2008, 255, 1874-1888 | null | null | math.PR math.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Lyapunov exponents of a dynamical system are a useful tool to gauge the
stability and complexity of the system. This paper offers a definition of
Lyapunov exponents for a sequence of free linear operators. The definition is
based on the concept of the extended Fuglede-Kadison determinant. We establish
the existence of Lyapunov exponents, derive formulas for their calculation, and
show that Lyapunov exponents of free variables are additive with respect to
operator product. We illustrate these results using an example of free
operators whose singular values are distributed by the Marchenko-Pastur law,
and relate this example to C. M. Newman's "triangle" law for the distribution
of Lyapunov exponents of large random matrices with independent Gaussian
entries. As an interesting by-product of our results, we derive a relation
between the extended Fuglede-Kadison determinant and Voiculescu's S-transform.
| [
{
"version": "v1",
"created": "Sun, 9 Dec 2007 23:46:25 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Nov 2008 23:15:29 GMT"
}
] | 2008-11-29T00:00:00 | [
[
"Kargin",
"Vladislav",
""
]
] | [
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