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712.2979 | Dinh-V.-Trung | Jeremy Lim, YiPing Ao, Dinh-V-Trung | Radially-Inflowing Molecular Gas in NGC 1275 Deposited by a X-ray
Cooling Flow in the Perseus Cluster | 40 pages, 10 figures, accepted for publication in ApJ | null | 10.1086/523664 | null | astro-ph | null | We have imaged in CO(2-1) the molecular gas in NGC 1275 (Perseus A), the cD
galaxy at the center of the Perseus Cluster, at a spatial resolution of $\sim$1
kpc over a central region of radius $\sim$ 10 kpc. Per A is known to contain
$\sim$1.3x10$^{10}$ M$_\odot$ of molecular gas, which has been proposed to be
captured from mergers with or ram-pressure stripping of gas-rich galaxies, or
accreted from a X-ray cooling flow. The molecular gas detected in our image has
a total mass of $\sim$4x10$^9$ M$_\odot$, and for the first time can be seen to
be concentrated in three radial filaments with lengths ranging from at least
1.1-2.4 kpc all lying in the east-west directions spanning the center of the
galaxy to radii of $\sim$8 kpc. The eastern and outer western filaments exhibit
larger blueshifted velocities with decreasing radii, whereas the inner western
filament spans the systemic velocity of the galaxy. The molecular gas shows no
signature of orbital motion, and is therefore unlikely to have been captured
from gas-rich galaxies. Instead, we are able to reproduce the observed
kinematics of the two outer filaments as free-fall in the gravitational
potential of Per A, as would be expected if they originate from a X-ray cooling
flow. Indeed, all three filaments lie between two prominent X-ray cavities
carved out by radio jets from Per A, and closely resembles the spatial
distribution of the coolest X-ray gas in the cluster core. The inferred
mass-deposition rate into the two outermost filaments alone is roughly 75
M$_odot$ yr$^{-1}$. This cooling flow can provide a nearly continuous supply of
molecular gas to fuel the active nucleus in Per A.
| [
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"version": "v1",
"created": "Tue, 18 Dec 2007 15:03:34 GMT"
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] | 2009-11-13T00:00:00 | [
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"Jeremy",
""
],
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"Ao",
"YiPing",
""
],
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"",
""
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712.298 | Salvatore Capozziello | S. Capozziello, M. De Laurentis, M. Francaviglia | Higher-order gravity and the cosmological background of gravitational
waves | 6 pages, 8 figures | Astropart.Phys.29:125-129,2008 | 10.1016/j.astropartphys.2007.12.001 | null | gr-qc | null | The cosmological background of gravitational waves can be tuned by the
higher-order corrections to the gravitational Lagrangian. In particular, it can
be shown that assuming $R^{1+\epsilon}$, where $\epsilon$ indicates a generic
(eventually small) correction to the Hilbert-Einstein action in the Ricci
scalar $R$, gives a parametric approach to control the evolution and the
production mechanism of gravitational waves in the early Universe.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:08:32 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Capozziello",
"S.",
""
],
[
"De Laurentis",
"M.",
""
],
[
"Francaviglia",
"M.",
""
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712.2981 | Razvan Radulescu M.D. | Razvan Tudor Radulescu | Oncoprotein metastasis disjoined | 6 pages | null | null | null | q-bio.SC q-bio.BM | null | As the past decade barely dawned, a fundamentally novel view of cancer
relating to signal transduction through intracellular hormones/growth factors
and their subunits began to unfold. Further along, it gained additional
substance with the advent of the interdisciplinary fields of particle biology
and peptide strings which explain (onco)protein dynamics in spacetime, for
instance insulin-driven sub- and trans-cellular carcinogenesis, by physical
principles. Here, this new understanding is expanded to introduce the concept
of "oncoprotein metastasis" preceding cancer cell spread and, thereby, a
particular emphasis is placed on its potential role in the emergence of the
pre-metastatic niche. Consistent with this perception, yet unlike currently
advocated treatments that target cancer cells only, future antineoplastic
strategies should aim to mimic natural tumor suppressors as well as involve
both (morphologically) normal and malignant cells. If validated in human
patients with advanced cancer disease, its otherwise frequently lethal course
may be halted and reversed just in time.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:14:30 GMT"
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"Radulescu",
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""
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] |
712.2982 | Carsten Deibel | C. Deibel, V. Dyakonov, J. Parisi | Spectroscopy of electronic defect states in Cu(In, Ga)(S, Se)$_2$-based
heterojunctions and Schottky diodes under damp-heat exposure | 4 pages, 5 figures | Europhysics Letters, 66 (2004) 399-404 | 10.1209/epl/i2003-10211-3 | deibel2004 | cond-mat.mtrl-sci | null | The changes of defect characteristics induced by accelerated lifetime tests
on the heterostructure n-ZnO/i-ZnO/CdS/Cu(In, Ga)(S, Se)$_2$/Mo relevant for
photovoltaic energy conversion are investigated. We subject heterojunction and
Schottky devices to extended damp heat exposure at 85$^{\circ}$C ambient
temperature and 85% relative humidity for various time periods. In order to
understand the origin of the pronounced changes of the devices, we apply
current--voltage and capacitance--voltage measurements, admittance
spectroscopy, and deep-level transient spectroscopy. The fill factor and
open-circuit voltage of test devices are reduced after prolonged damp heat
treatment, leading to a reduced energy conversion efficiency. We observe the
presence of defect states in the vicinity of the CdS/chalcopyrite interface.
Their activation energy increases due to damp heat exposure, indicating a
reduced band bending at the Cu(In, Ga)(S, Se)$_2$ surface. The Fermi-level
pinning at the buffer/chalcopyrite interface, maintaining a high band bending
in as-grown cells, is lifted due to the damp-heat exposure. We also observe
changes in the bulk defect spectra due to the damp-heat treatment.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:16:23 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Deibel",
"C.",
""
],
[
"Dyakonov",
"V.",
""
],
[
"Parisi",
"J.",
""
]
] | [
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] |
712.2983 | Alberto Sainz Dalda | A. Sainz Dalda and L. R. Bellot Rubio | Detection of sea-serpent field lines in sunspot penumbrae | 4 pages, 3 figures, 1 movie. Letter accepted by Astronomy &
Astrophysics | null | 10.1051/0004-6361:20079115 | null | astro-ph | null | We investigate the spatial distribution of magnetic polarities in the
penumbra of a spot observed very close to disk center. High-spatial resolution,
high-cadence magnetograms taken with the Narrowband Filter Imager aboard Hinode
are used in this study. They provide continuous and stable measurements in the
photospheric Fe I 630.25 line for long periods of time. We discover
small-scale, elongated, bipolar magnetic structures that appear in the mid
penumbra and move radially outward across the penumbra. They occur in between
the more vertical fields of the penumbra, and can be associated with the
horizontal fields that harbor the Evershed flow. Many of them cross the outer
penumbral boundary, becoming moving magnetic features in the sunspot moat. We
determine the properties of these structures, including their sizes, proper
motions, footpoint separation, and lifetimes. The bipolar patches can be
interpreted as being produced by sea-serpent field lines that originate in the
mid-penumbra and eventually leave the spot in the form moving magnetic
features. The existence of such field lines has been inferred from Stokes
inversions of spectropolarimetric measurements at lower angular resolution, but
this is the first time they are imaged directly. Our observations add another
piece of evidence in favor of the uncombed structure of penumbral magnetic
fields.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 12:10:03 GMT"
},
{
"version": "v2",
"created": "Sun, 20 Jan 2008 17:11:15 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dalda",
"A. Sainz",
""
],
[
"Rubio",
"L. R. Bellot",
""
]
] | [
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] |
712.2984 | Mohammad Ali Rajabpour | A. A. Saberi, M. A. Rajabpour, S. Rouhani | Conformal Curves on $WO_3$ Surface | 4 pages, 6 figures. accepted in PRL | Phys. Rev. Lett. 100, 044504 (2008) | 10.1103/PhysRevLett.100.044504 | null | cond-mat.stat-mech | null | We have studied the iso-height lines on the $\mathrm{WO_3}$ surface as a
physical candidate for conformally invariant curves. We have shown that these
lines are conformally invariant with the same statistics of domain walls in the
critical Ising model. They belong to the family of conformal invariant curves
called Schramm-Loewner evolution (or $SLE_{\kappa}$), with diffusivity of
$\kappa \sim 3$. This can be regarded as the first experimental observation of
SLE curves. We have also argued that Ballistic Deposition (BD) can serve as a
growth model giving rise to contours with similar statistics at large scales.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:32:45 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Saberi",
"A. A.",
""
],
[
"Rajabpour",
"M. A.",
""
],
[
"Rouhani",
"S.",
""
]
] | [
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] |
712.2985 | Mattias Marklund | G. Brodin, M. Marklund, R. Bingham, J. Collier, R. G. Evans | Laboratory soft x-ray emission due to the Hawking-Unruh effect? | 11 pages, 3 figures, 1 table | Class.Quant.Grav.25:145005,2008 | 10.1088/0264-9381/25/14/145005 | null | hep-ph gr-qc | null | The structure of spacetime, quantum field theory, and thermodynamics are all
connected through the concepts of the Hawking and Unruh temperatures. The
possible detection of the related radiation constitutes a fundamental test of
such subtle connections. Here a scheme is presented for the detection of Unruh
radiation based on currently available laser systems. By separating the
classical radiation from the Unruh-response in frequency space, it is found
that the detection of Unruh radiation is possible in terms of soft x-ray
photons using current laser-electron beam technology. The experimental
constraints are discussed and a proposal for an experimental design is given.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:36:50 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Brodin",
"G.",
""
],
[
"Marklund",
"M.",
""
],
[
"Bingham",
"R.",
""
],
[
"Collier",
"J.",
""
],
[
"Evans",
"R. G.",
""
]
] | [
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] |
712.2986 | Auguste Aman | Auguste Aman (LMAI), Modeste N'Zi (LMAI) | Homogenization of reflected semilinear PDE with nonlinear Neumann
boundary condition | Ce papier a 19 pages et est soumis pour publication dans Stochastic
Analysis and Applications | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the homogenization problem of semi linear reflected partial
differential equations (reflected PDEs for short) with nonlinear Neumann
conditions. The non-linear term is a function of the solution but not of its
gradient. The proof are fully probabilistic and uses weak convergence of
associated reflected generalized backward differential stochastic equations
(reflected GBSDEs in short).
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:48:05 GMT"
},
{
"version": "v2",
"created": "Sat, 10 Jan 2009 11:22:51 GMT"
},
{
"version": "v3",
"created": "Thu, 15 Jan 2009 15:45:16 GMT"
}
] | 2009-01-15T00:00:00 | [
[
"Aman",
"Auguste",
"",
"LMAI"
],
[
"N'Zi",
"Modeste",
"",
"LMAI"
]
] | [
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] |
712.2987 | Wouter Bos | Wouter J.T. Bos (LMFA), Jean-Pierre Bertoglio (LMFA) | Inertial range scaling of scalar flux spectra in uniformly sheared
turbulence | null | Physics of Fluids 19 (2007) 025104 | 10.1063/1.2565563 | null | physics.class-ph | null | A model based on two-point closure theory of turbulence is proposed and
applied to study the Reynolds number dependency of the scalar flux spectra in
homogeneous shear flow with a cross-stream uniform scalar gradient. For the
cross-stream scalar flux, in the inertial range the spectral behavior agrees
with classical predictions and measurements. The streamwise scalar flux is
found to be in good agreement with the results of atmospheric measurements.
However, both the model results and the atmospheric measurements disagree with
classical predictions. A detailed analysis of the different terms in the
evolution equation for the streamwise scalar flux spectrum shows that nonlinear
contributions are governing the inertial subrange of this spectrum and that
these contributions are relatively more important than for the cross-stream
flux. A new expression for the scalar flux spectra is proposed. It allows us to
unify the description of the components in one single expression, leading to a
classical K^-7/3 inertial range for the cross-stream component and to a new
K^-23/9 scaling for the streamwise component that agrees better with
atmospheric measurements than the K^-3 prediction of J. C. Wyngaard and O. R.
Cot\'e [Quart. J. R. Met. Soc. 98, 590 (1972)].
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 15:54:26 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Bos",
"Wouter J. T.",
"",
"LMFA"
],
[
"Bertoglio",
"Jean-Pierre",
"",
"LMFA"
]
] | [
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] |
712.2988 | Jerome Bouvier | Jerome Bouvier (LAOG) | The rotational evolution of young low mass stars | 10 pages | Dans Star-Disk Interaction in Young Stars - Star-Disk Interaction
in Young Stars, Grenoble : France (2007) | 10.1017/S1743921307009593 | null | astro-ph | null | Star-disk interaction is thought to drive the angular momentum evolution of
young stars. In this review, I present the latest results obtained on the
rotational properties of low mass and very low mass pre-main sequence stars. I
discuss the evidence for extremely efficient angular momentum removal over the
first few Myr of pre-main sequence evolution and describe recent results that
support an accretion-driven braking mechanism. Angular momentum evolution
models are presented and their implication for accretion disk lifetimes
discussed.
| [
{
"version": "v1",
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] | 2009-11-13T00:00:00 | [
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712.2989 | Recai Erdem | Recai Erdem | A way to get rid of cosmological constant and zero point energy problems
of quantum fields through metric reversal symmetry | Presentation and content are improved, references are added. I would
like to thank the anonymous referee for his valuable comments and suggestions
to improve the paper | J.Phys.A41:235401,2008 | 10.1088/1751-8113/41/23/235401 | IZTECH-P-07-06 | hep-th astro-ph gr-qc hep-ph | null | In this paper a framework is introduced to remove the huge discrepancy
between the empirical value of the cosmological constant and the contribution
to the cosmological constant predicted from the vacuum energy of quantum
fields. An extra dimensional space with metric reversal symmetry and $R^2$
gravity is considered to this end. The resulting 4-dimensional energy-momentum
tensor (obtained after integration over extra dimensions) consists of terms
that contain off-diagonally coupled pair of Kaluza-Klein modes. This, in turn,
generically results in vanishing of the vacuum expectation value of the
energy-momentum tensor for quantum fields, and offers a way to solve the
problem of huge contribution of quantum fields to the vacuum energy density.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:16:52 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Apr 2008 15:50:36 GMT"
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] | 2008-11-26T00:00:00 | [
[
"Erdem",
"Recai",
""
]
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712.299 | Dean Lee J | Bugra Borasoy, Evgeny Epelbaum, Hermann Krebs, Dean Lee, Ulf-G.
Mei{\ss}ner | Chiral effective field theory on the lattice at next-to-leading order | 30 pages, 10 figures, published version | Eur.Phys.J.A35:343-355,2008 | 10.1140/epja/i2008-10544-3 | null | nucl-th hep-lat | null | We study nucleon-nucleon scattering on the lattice at next-to-leading order
in chiral effective field theory. We determine phase shifts and mixing angles
from the properties of two-nucleon standing waves induced by a hard spherical
wall in the center-of-mass frame. At fixed lattice spacing we test model
independence of the low-energy effective theory by computing
next-to-leading-order corrections for two different leading-order lattice
actions. The first leading-order action includes instantaneous one-pion
exchange and same-site contact interactions. The second leading-order action
includes instantaneous one-pion exchange and Gaussian-smeared interactions. We
find that in each case the results at next-to-leading order are accurate up to
corrections expected at higher order.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:17:17 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Apr 2008 14:53:11 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Borasoy",
"Bugra",
""
],
[
"Epelbaum",
"Evgeny",
""
],
[
"Krebs",
"Hermann",
""
],
[
"Lee",
"Dean",
""
],
[
"Meißner",
"Ulf-G.",
""
]
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712.2991 | Richard Easther | Richard Easther, John T. Giblin Jr, and Eugene A. Lim | Gravitational Waves From the End of Inflation: Computational Strategies | 15 pages, 13 figures | Phys.Rev.D77:103519,2008 | 10.1103/PhysRevD.77.103519 | null | astro-ph | null | Parametric resonance or preheating is a plausible mechanism for bringing
about the transition between the inflationary phase and a hot, radiation
dominated universe. This epoch results in the rapid production of heavy
particles far from thermal equilibrium and could source a significant
stochastic background of gravitational radiation. Here, we present a numerical
algorithm for computing the contemporary power spectrum of gravity waves
generated in this post-inflationary phase transition for a large class of
scalar-field driven inflationary models. We explicitly calculate this spectrum
for both quartic and quadratic models of chaotic inflation, and low-scale
hybrid models. In particular, we consider hybrid models with an ``inverted''
potential. These models have a very short and intense period of resonance which
is qualitatively different from previous examples studied in this context, but
we find that they lead to a similar spectrum of gravitational radiation.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:23:00 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Easther",
"Richard",
""
],
[
"Giblin",
"John T.",
"Jr"
],
[
"Lim",
"Eugene A.",
""
]
] | [
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712.2992 | Elio Conte | Elio Conte | A Proof Of Kochen - Specker Theorem of Quantum Mechanics Using a Quantum
Like Algebraic Formulation | null | null | null | null | physics.gen-ph | null | Using a quantum like algebraic formulation we give proof of Kochen-Specker
theorem. We introduce new criteria in order to account for the contextual
nature of measurements in quantum mechanics.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:22:11 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Conte",
"Elio",
""
]
] | [
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712.2993 | Dean Lee J | Bugra Borasoy, Evgeny Epelbaum, Hermann Krebs, Dean Lee, Ulf-G.
Mei{\ss}ner | Dilute neutron matter on the lattice at next-to-leading order in chiral
effective field theory | 25 pages, 7 figures, published version | Eur.Phys.J.A35:357-367,2008 | 10.1140/epja/i2008-10545-2 | null | nucl-th astro-ph hep-lat | null | We discuss lattice simulations of the ground state of dilute neutron matter
at next-to-leading order in chiral effective field theory. In a previous paper
the coefficients of the next-to-leading-order lattice action were determined by
matching nucleon-nucleon scattering data for momenta up to the pion mass. Here
the same lattice action is used to simulate the ground state of up to 12
neutrons in a periodic cube using Monte Carlo. We explore the density range
from 2% to 8% of normal nuclear density and analyze the ground state energy as
an expansion about the unitarity limit with corrections due to finite
scattering length, effective range, and P-wave interactions.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:24:49 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Apr 2008 14:57:51 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Borasoy",
"Bugra",
""
],
[
"Epelbaum",
"Evgeny",
""
],
[
"Krebs",
"Hermann",
""
],
[
"Lee",
"Dean",
""
],
[
"Meißner",
"Ulf-G.",
""
]
] | [
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] |
712.2994 | Wouter Bos | Guillevic Lamaison (LMFA), Wouter Bos (LMFA), L. Shao (LMFA),
Jean-Pierre Bertoglio (LMFA) | Decay of scalar variance in isotropic turbulence in a bounded domain | null | Journal of turbulence 8, 4 (2007) 1 | 10.1080/14685240601091676 | null | physics.class-ph | null | The decay of scalar variance in isotropic turbulence in a bounded domain is
investigated. Extending the study of Touil, Bertoglio and Shao (2002; Journal
of Turbulence, 03, 49) to the case of a passive scalar, the effect of the
finite size of the domain on the lengthscales of turbulent eddies and scalar
structures is studied by truncating the infrared range of the wavenumber
spectra. Analytical arguments based on a simple model for the spectral
distributions show that the decay exponent for the variance of scalar
fluctuations is proportional to the ratio of the Kolmogorov constant to the
Corrsin-Obukhov constant. This result is verified by closure calculations in
which the Corrsin-Obukhov constant is artificially varied. Large-eddy
simulations provide support to the results and give an estimation of the value
of the decay exponent and of the scalar to velocity time scale ratio.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:27:14 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Lamaison",
"Guillevic",
"",
"LMFA"
],
[
"Bos",
"Wouter",
"",
"LMFA"
],
[
"Shao",
"L.",
"",
"LMFA"
],
[
"Bertoglio",
"Jean-Pierre",
"",
"LMFA"
]
] | [
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] |
712.2995 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB) | Note sur la conjecture de Leopoldt | null | null | null | null | math.NT | null | We prove that number fields with arbitrary degree but weak ramification
satisfy the Leopoldt conjecture on the l-adic rank of the group of units
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:30:18 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
]
] | [
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] |
712.2996 | Giovanni Panti | Giovanni Panti | A general Lagrange Theorem | 5 pages, 2 figures | null | null | null | math.NT math.DS | null | The ordinary continued fractions expansion of a real number is based on the
Euclidean division. Variants of the latter yield variants of the former, all
encompassed by a more general Dynamical Systems framework. For all these
variants the Lagrange Theorem holds: a number has an eventually periodic
expansion if and only if it is a quadratic irrational. This fact is surely
known for specific expansions, but the only proof for the general case that I
could trace in the literature follows as an implicit corollary from much deeper
results by Boshernitzan and Carroll on interval exchange transformations. It
may then be useful to have at hand a simple and virtually computation-free
proof of a general Lagrange Theorem.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:30:59 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Panti",
"Giovanni",
""
]
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712.2997 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB) | Plongements l-adiques et l-nombres de Weil | null | null | null | null | math.NT | null | We define l-adic analogs of classical Weil numbers in connexion both with
complex or l-adic imbeddings of number fields and real or l-adic absolute
values. As an application we give some consequences related to the Iwasawa
theory of cyclotomic towers.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:31:33 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
]
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712.2998 | Jean-Francois Jaulent | Jean-Fran\c{c}ois Jaulent (IMB) | Compactification l-adique de R | null | null | null | null | math.NT | null | We construct a compact topological group Rl which contains both the real
additive group R and the l-adic one Ql (for a given prime number l) as dense
subgroups; thus we study some of its properties. This construction gives an
arithmetic description of the so-called l-adic solenoid classically defined in
terms of foliations.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:32:35 GMT"
},
{
"version": "v2",
"created": "Sun, 6 Jan 2008 17:29:51 GMT"
}
] | 2008-01-06T00:00:00 | [
[
"Jaulent",
"Jean-François",
"",
"IMB"
]
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] |
712.2999 | Alexander Khodjamirian | K.G. Chetyrkin, A. Khodjamirian, A.A. Pivovarov | Towards NNLO Accuracy in the QCD Sum Rule for the Kaon Distribution
Amplitude | 14 pages, 2 figures | Phys.Lett.B661:250-258,2008 | 10.1016/j.physletb.2008.02.031 | SI-HEP-2007-19, TTP-07-36, SFB/CPP-07-83 | hep-ph | null | We calculate the $O(\alpha_s)$ and $O(\alpha_s^2)$ gluon radiative
corrections to the QCD sum rule for the first Gegenbauer moment $a_1^K$ of the
kaon light-cone distribution amplitude. The NNL0 accuracy is achieved for the
perturbative term and quark-condensate contributions to the sum rule. A
complete factorization is implemented, removing logarithms of $s$-quark mass
from the coefficients in the operator-product expansion. The sum rule with
radiative corrections yields $a_1^K(1 \GeV)=0.10\pm 0.04$.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:45:21 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chetyrkin",
"K. G.",
""
],
[
"Khodjamirian",
"A.",
""
],
[
"Pivovarov",
"A. A.",
""
]
] | [
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712.3 | Hans-Thomas Janka | C. Lunardini (1,2), B. Mueller (3), and H.-Th. Janka (3) ((1) Arizona
State University, Tempe (2) RIKEN BNL Research Center, Upton (3) MPI for
Astrophysics, Garching) | Neutrino oscillation signatures of oxygen-neon-magnesium supernovae | 14 pages, 10 figures (16 figure files). Text and graphics added for
illustration and clarification; Results unchanged. Version accepted for
publication in Physical Review D | Phys.Rev.D78:023016,2008 | 10.1103/PhysRevD.78.023016 | RBRC 712 | astro-ph hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss the flavor conversion of neutrinos from core collapse supernovae
that have oxygen-neon-magnesium (ONeMg) cores. Using the numerically calculated
evolution of the star up to 650 ms post bounce, we find that, for the normal
mass hierarchy, the electron neutrino flux in a detector shows signatures of
two typical features of an ONeMg-core supernova: a sharp step in the density
profile at the base of the He shell and a faster shock wave propagation
compared to iron core supernovae. Before the shock hits the density step (t ~
150 ms), the survival probability of electron neutrinos is about 0.68, in
contrast to values of 0.32 or less for an iron core supernova. The passage of
the shock through the step and its subsequent propagation cause a decrease of
the survival probability and a decrease of the amplitude of oscillations in the
Earth, reflecting the transition to a more adiabatic propagation inside the
star. These changes affect the lower energy neutrinos first; they are faster
and more sizable for larger theta_13. They are unique of ONeMg-core supernovae,
and give the possibility to test the speed of the shock wave. The time
modulation of the Earth effect and its negative sign at the neutronization peak
are the most robust signatures in a detector.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:43:21 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Dec 2007 21:07:31 GMT"
},
{
"version": "v3",
"created": "Mon, 16 Jun 2008 21:45:11 GMT"
}
] | 2009-12-06T00:00:00 | [
[
"Lunardini",
"C.",
""
],
[
"Mueller",
"B.",
""
],
[
"Janka",
"H. -Th.",
""
]
] | [
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] |
712.3001 | Marek Gazdzicki | Marek Gazdzicki | Onset of Deconfinement in Nucleus-Nucleus Collisions - Past, Present and
Future - | Dedicated to 60th birthday of Mark I. Gorenstein, Presented at "New
Trends in High Energy Physics", Yalta, Crimea, September 15-22, 2007 | null | null | null | nucl-th | null | In 2007 Mark I. Gorenstein celebrated his 60th birthday. This report is
dedicated to Mark and it sketches the results obtained during the past ten
years of our collaboration and friendship. They concern search for and study of
the onset of deconfinement in high energy nucleus-nucleus collisions.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 16:51:00 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Gazdzicki",
"Marek",
""
]
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] |
712.3002 | Nicholas Parker | N. G. Parker, A. M. Martin, S. L. Cornish and C. S. Adams | Collisions of bright solitary matter waves | 9 pages, 4 colour figures | J. Phys. B: At. Mol. Opt. Phys. 41 No 4 (28 February 2008) 045303 | 10.1088/0953-4075/41/4/045303 | null | cond-mat.other | null | The collisions of three-dimensional bright solitary matter waves formed from
atomic Bose-Einstein condensates are shown to exhibit rich behaviour.
Collisions range from being elastic to completely destructive due to the onset
of collapse during the interaction. Through a detailed quantitative analysis we
map out the role of relative phase, impact speed and interaction strength. In
particular, we identify the importance of the collapse time in the onset of
unstable collisions and show how the relative phase controls a population
transfer between the waves. Our analysis enables us to interpret recent
experimental observations of bright solitary matter waves.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:20:49 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Parker",
"N. G.",
""
],
[
"Martin",
"A. M.",
""
],
[
"Cornish",
"S. L.",
""
],
[
"Adams",
"C. S.",
""
]
] | [
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] |
712.3003 | Alessandro Nagar | Thibault Damour, Alessandro Nagar, Ernst Nils Dorband, Denis Pollney,
Luciano Rezzolla | Faithful Effective-One-Body waveforms of equal-mass coalescing
black-hole binaries | 13 pages, 3 figures. Small changes. Version published in Phys. Rev. D | Phys.Rev.D77:084017,2008 | 10.1103/PhysRevD.77.084017 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We continue the program of constructing, within the Effective-One-Body (EOB)
approach, high-accuracy analytic waveforms describing the signal emitted by
inspiralling and coalescing black hole binaries. Here, we compare a recently
derived, resummed 3 PN-accurate EOB quadrupolar waveform to the results of a
numerical simulation of the inspiral and merger of an equal-mass black hole
binary. We find a remarkable agreement, both in phase and in amplitude, with a
maximal dephasing which can be reduced below $\pm 0.005$ gravitational-wave
(GW) cycles over 12 GW cycles corresponding to the end of the inspiral, the
plunge, the merger and the beginning of the ringdown. This level of agreement
is shown for two different values of the effective 4 PN parameter a_5, and for
corresponding, appropriately "flexed" values of the radiation-reaction
resummation parameter v_pole. In addition, our resummed EOB amplitude agrees to
better than the 1% level with the numerical-relativity one up to the late
inspiral. These results, together with other recent work on the
EOB-numerical-relativity comparison, confirm the ability of the EOB formalism
to faithfully capture the general relativistic waveforms.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:33:05 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Aug 2008 09:04:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Damour",
"Thibault",
""
],
[
"Nagar",
"Alessandro",
""
],
[
"Dorband",
"Ernst Nils",
""
],
[
"Pollney",
"Denis",
""
],
[
"Rezzolla",
"Luciano",
""
]
] | [
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] |
712.3004 | Francesco Shankar | Francesco Shankar (1), Alfonso Cavaliere (2), Michele Cirasuolo (3)
and Laura Maraschi (4) ((1) OSU, USA; (2) Tor Vergata, Italy; (3) SUPA,
Scotland (4)-INAF-Oss. Astr. Brera, Italy) | The Optical-Radio Mapping: the kinetic efficiency of Radio-Loud AGNs | ApJ, accepted, 7 pages, 6 figures | null | 10.1086/528836 | null | astro-ph | null | We constrain the mean kinetic efficiency of radio-loud active galactic nuclei
by using an optically selected sample for which both the optical and the radio
luminosity functions (LFs) have been determined; the former traces the
bolometric luminosity L, while the latter traces the kinetic power L_k,
empirically correlated to the radio emission. Thus in terms of the ratio
g_k=L_k/L, we can convert the optical LF of the sample into a radio one. This
computed LF is shown to match the directly observed LF for the same sample if
g_k=0.10^{+0.05}_{-0.01} holds, with a scatter \sigma=0.38^{+0.04}_{-0.09} dex;
with these values we also match a number of independent correlations between
L_k, L and radio emission, that we derive through Monte Carlo simulations. We
proceed to translate the value of g_k into a constraint on the kinetic
efficiency for the production of radio jets or winds, namely,
\epsilon_k=L_k/(Mdot*c^2)~0.01 in terms of the rate Mdot of mass accretion onto
the central black hole. Then, on assuming that on average the radio sources
share the same kinetic efficiency, we compute a solid lower limit of about 25%
on the contribution of radio sources to the local black hole mass density.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:49:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shankar",
"Francesco",
""
],
[
"Cavaliere",
"Alfonso",
""
],
[
"Cirasuolo",
"Michele",
""
],
[
"Maraschi",
"Laura",
""
]
] | [
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] |
712.3005 | Scott J. Wolk | Scott J. Wolk, Bradley D. Spitzbart, Tyler L. Bourke, Robert A.
Gutermuth, Miquela Vigil, Fernando Comer\'on | X-ray and IR Point Source Identification and Characteristics in the
Embedded, Massive Star-Forming Region RCW 108 | 63 pages including 18 figures, and 15 tables. Tables 1,2,5,7,10,and
11 have been stubbed in the text and included as ancillary files. Accepted by
the Astronomical Journal | null | 10.1088/0004-6256/135/2/693 | null | astro-ph | null | We report on the results of an approximately 90 ks Chandra observation of a
complex region that hosts multiple sites of recent and active star formation in
ARA OB1a. The field is centered on the embedded cluster RCW 108-IR and includes
and a large portion of the open cluster NGC 6193. We detect over 420 X-ray
sources in the field and combined these data with deep near-IR, Spitzer/IRAC
and MSX mid-IR data. We find about 360 of the X-ray sources have near--IR
counterparts. We divide the region into 5 parts based on the X-ray point source
characteristics and extended 8 micron emission. The most clearly defined
regions are the central region - identified by embedded sources with high
luminosities in the both the near-IR and X-ray as well as high X-ray
temperatures (about 3 keV) and the eastern region - identified by low
extinction and 1 keV X-ray temperatures. Other regions, identified by their
directional relationship to RCW 108-IR are less uniform - representing
combinations of the first two regions, independent star formation epochs, or
both. Over 18% percent of the cluster members with over 100 counts exhibit
flares. Overall about 50% of the stars appear to have optically thick disks
when IRAC data are employed. The largest fraction of X-ray sources are best
described as possessing some disk material via a more detailed extinction
fitting. We estimate that the total number of pre--main sequence stars in the
field is about 1600. Approximately 800 are confined to (1.1 pc) central region.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:37:39 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wolk",
"Scott J.",
""
],
[
"Spitzbart",
"Bradley D.",
""
],
[
"Bourke",
"Tyler L.",
""
],
[
"Gutermuth",
"Robert A.",
""
],
[
"Vigil",
"Miquela",
""
],
[
"Comerón",
"Fernando",
""
]
] | [
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] |
712.3006 | Silvia Pedicelli | S. Pedicelli, J. Lub, J.W. Pel, B. Lemasle, G. Bono, P. Francois, D.
Laney, A. Piersimoni, F. Primas, M. Romaniello, R. Buonanno, F. Caputo, S.
Cassisi, F. Castelli, A. Pietrinferni, J. Pritchard | Metallicity estimates of Galactic Cepheids based on Walraven photometry | 6 pages, 5 figures; to appear in Mem. Soc. Astr. Italiana, Vol. 79/2
(proceeding Cefalu' Workshop "XXI Century Challenges for Stellar Evolution",
ed. S. Cassisi & M. Salaris) | null | null | null | astro-ph | null | We present new empirical and theoretical calibrations of two photometric
metallicity indices based on Walraven photometry. The empirical calibration
relies on a sample of 48 Cepheids for which iron abundances based on high
resolution spectra are available in the literature. They cover a broad range in
metal abundance (-0.5 < [Fe/H] < +0.5) and the intrinsic accuracy of the
Metallicity Index Color (MIC) relations is better than 0.2 dex. The theoretical
calibration relies on a homogeneous set of scaled-solar evolutionary tracks for
intermediate-mass stars and on pulsation predictions concerning the topology of
the instability strip. The metal content of the adopted evolutionary tracks
ranges from Z=0.001 to Z=0.03 and the intrinsic accuracy of the MIC relations
is better than 0.1 dex.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:40:16 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Pedicelli",
"S.",
""
],
[
"Lub",
"J.",
""
],
[
"Pel",
"J. W.",
""
],
[
"Lemasle",
"B.",
""
],
[
"Bono",
"G.",
""
],
[
"Francois",
"P.",
""
],
[
"Laney",
"D.",
""
],
[
"Piersimoni",
"A.",
""
],
[
"Primas",
"F.",
""
],
[
"Romaniello",
"M.",
""
],
[
"Buonanno",
"R.",
""
],
[
"Caputo",
"F.",
""
],
[
"Cassisi",
"S.",
""
],
[
"Castelli",
"F.",
""
],
[
"Pietrinferni",
"A.",
""
],
[
"Pritchard",
"J.",
""
]
] | [
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] |
712.3007 | Elena Rubei | Elena Rubei | On tropical and Kapranov ranks of tropical matrices | 12 pages, third version equal to the second, I added only a note with
a reference | null | null | null | math.AG math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that, for any g greater or equal than 3, a matrix g x 5 with
tropical rank 3 has Kapranov rank 3.
| [
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"version": "v2",
"created": "Sun, 13 Dec 2009 10:30:25 GMT"
},
{
"version": "v3",
"created": "Tue, 10 May 2011 14:37:34 GMT"
}
] | 2011-05-11T00:00:00 | [
[
"Rubei",
"Elena",
""
]
] | [
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712.3008 | Giovanni Montani | Giovanni Montani, Marco Valerio Battisti, Riccardo Benini, Giovanni
Imponente | Classical and Quantum Features of the Mixmaster Singularity | 170 pages, 14 figures, ~500 references. Invited review paper to
appear on Int. J. Mod. Phys. A. v2: minor changes, references added. v3:
Conclusions added | Int.J.Mod.Phys.A23:2353-2503,2008 | 10.1142/S0217751X08040275 | null | gr-qc astro-ph hep-th quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This review article is devoted to analyze the main properties characterizing
the cosmological singularity associated to the homogeneous and inhomogeneous
Mixmaster model. After the introduction of the main tools required to treat the
cosmological issue, we review in details the main results got along the last
forty years on the Mixmaster topic. We firstly assess the classical picture of
the homogeneous chaotic cosmologies and, after a presentation of the canonical
method for the quantization, we develop the quantum Mixmaster behavior.
Finally, we extend both the classical and quantum features to the fully
inhomogeneous case. Our survey analyzes the fundamental framework of the
Mixmaster picture and completes it by accounting for recent and peculiar
outstanding results.
| [
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"version": "v1",
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},
{
"version": "v3",
"created": "Fri, 12 Sep 2008 13:24:57 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Montani",
"Giovanni",
""
],
[
"Battisti",
"Marco Valerio",
""
],
[
"Benini",
"Riccardo",
""
],
[
"Imponente",
"Giovanni",
""
]
] | [
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712.3009 | Tobias Hurth | Tobias Huber (Zurich U., Aachen Tech. Hochsch), Tobias Hurth (CERN,
SLAC), and Enrico Lunghi (Fermilab) | Logarithmically Enhanced Corrections to the Decay Rate and Forward
Backward Asymmetry in anti-B --> X(s) l+ l- | 26 pages, 3 figures, minor changes, published version | Nucl.Phys.B802:40-62,2008 | 10.1016/j.nuclphysb.2008.04.028 | CERN CERN-PH-TH/2007-177, SLAC-PUB-12859, ZU-TH 30/07,
FERMILAB-PUB-07-639-T, PITHA 07/21 | hep-ph hep-ex | null | We study logarithmically enhanced electromagnetic corrections to the decay
rate in the high dilepton invariant mass region as well as corrections to the
forward backward asymmetry (FBA) of the inclusive rare decay $\bar{B} \to X_s
\ell^+ \ell^-$. As expected, the relative effect of these corrections in the
high dilepton mass region is around -8% for the muonic final state and
therefore much larger than in the low dilepton mass region.
We also present a complete phenomenological analysis, to improved NNLO
accuracy, of the dilepton mass spectrum and the FBA integrated in the low
dilepton mass region, including a new approach to the zero of the FBA. The
latter represents one of the most precise predictions in flavour physics with a
theoretical uncertainty of order 5%. We find $(q_0^2)_{\mu\mu} = (3.50 \pm
0.12) \gev^2$. For the high dilepton invariant mass region, we have ${\cal
B}(\bar B\to X_s\mu\mu)_{\rm high} = (2.40^{+0.69}_{-0.62}) \times 10^{-7}$.
The dominant uncertainty is due to the $1/m_b$ corrections and can be
significantly reduced in the future. For the low dilepton invariant mass
region, we confirm previous results up to small corrections.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:50:57 GMT"
},
{
"version": "v2",
"created": "Mon, 19 May 2008 10:39:17 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Huber",
"Tobias",
"",
"Zurich U., Aachen Tech. Hochsch"
],
[
"Hurth",
"Tobias",
"",
"CERN,\n SLAC"
],
[
"Lunghi",
"Enrico",
"",
"Fermilab"
]
] | [
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] |
712.301 | Vladimir Pomerantsev | T.S. Jensen, V.P. Popov and V.N. Pomerantsev | Atomic Cascade in Muonic and Hadronic Hydrogen Atoms | 9 pages, 11 figures | null | null | null | nucl-th | null | The atomic cascade in $\mu^- p$ and $\pi^- p$ atoms has been studied with the
improved version of the extended cascade model in which new quantum mechanical
calculations of the differential and integral cross sections of the elastic
scattering, Stark transitions and Coulomb de-excitation have been included for
the principal quantum number values $n\le 8$ and the relative energies $E \ge
0.01$ eV. The $X$-ray yields and kinetic energy distributions are compared with
the experimental data.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 17:53:46 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Jensen",
"T. S.",
""
],
[
"Popov",
"V. P.",
""
],
[
"Pomerantsev",
"V. N.",
""
]
] | [
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] |
712.3011 | Denjoe O'Connor | Rodrigo Delgadillo-Blando, Denjoe O'Connor and Badis Ydri | Geometry in transition: A model of emergent geometry | 6 pages, 4 figures | Phys.Rev.Lett.100:201601,2008 | 10.1103/PhysRevLett.100.201601 | DIAS-preprint 07-22 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study a three matrix model with global SO(3) symmetry containing at most
quartic powers of the matrices. We find an exotic line of discontinuous
transitions with a jump in the entropy, characteristic of a 1st order
transition, yet with divergent critical fluctuations and a divergent specific
heat with critical exponent $\alpha=1/2$. The low temperature phase is a
geometrical one with gauge fields fluctuating on a round sphere. As the
temperature increased the sphere evaporates in a transition to a pure matrix
phase with no background geometrical structure. Both the geometry and gauge
fields are determined dynamically. It is not difficult to invent higher
dimensional models with essentially similar phenomenology. The model presents
an appealing picture of a geometrical phase emerging as the system cools and
suggests a scenario for the emergence of geometry in the early universe.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:52:47 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Jul 2008 19:38:05 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Delgadillo-Blando",
"Rodrigo",
""
],
[
"O'Connor",
"Denjoe",
""
],
[
"Ydri",
"Badis",
""
]
] | [
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712.3012 | Nicholas Rattenbury | Nicholas J. Rattenbury, Shude Mao | OGLE-II High Proper Motion Stars towards the Galactic centre | 7 figures and 4 tables, MNRAS, accepted | null | 10.1111/j.1365-2966.2008.12878.x | null | astro-ph | null | The photometry data base of the second phase of the OGLE microlensing
experiment, OGLE-II, is a rich source of information about the kinematics and
structure of the Galaxy. In this work we use the OGLE-II proper motion
catalogue to identify candidate stars which have high proper motions. 521 stars
with proper motion mu > 50 mas/yr in the OGLE-II proper motion catalogue (Sumi
2004) were cross-identified with stars in the MACHO high proper motion
catalogue, and the DENIS and 2MASS infra-red photometry catalogues. Photometric
distances were computed for stars with colours consistent with G/K and M type
stars. 6 stars were newly identified as possible nearby (< 50 pc) M dwarfs.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:02:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rattenbury",
"Nicholas J.",
""
],
[
"Mao",
"Shude",
""
]
] | [
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] |
712.3013 | Eulogio Oset | E. Oset, L. S. Geng, D. Gamermann, M.J. Vicente Vacas, D. Strottman,
K. P. Khemchandani, A. Martinez Torres, J. A. Oller and L. Roca | Recent Developments in Chiral Unitary Dynamics of Resonances | Talk at the International Conference on Hadron Physics, Troia07,
Canakkale, Turkey, Sep. 2007 and at the Chiral Symmetry in Hadron and Nuclear
Physics Workshop, Chiral07, Osaka, November 2007 | Mod.Phys.Lett.A23:2201-2208,2008 | 10.1142/S0217732308029046 | FTUV-07-1218, IFIC-07-1218 | nucl-th | null | In this talk I summarize recent findings made on the description of axial
vector mesons as dynamically generated states from the interaction of
peseudoscalar mesons and vector mesons, dedicating some attention to the two
$K_1(1270)$ states. Then I review the generation of open and hidden charm
scalar and axial states. Finally, I present recent results showing that the low
lying $1/2^+$ baryon resonances for S=-1 can be obtained as bound states or
resonances of two mesons and one baryon in coupled channels dynamics.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:07:36 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Oset",
"E.",
""
],
[
"Geng",
"L. S.",
""
],
[
"Gamermann",
"D.",
""
],
[
"Vacas",
"M. J. Vicente",
""
],
[
"Strottman",
"D.",
""
],
[
"Khemchandani",
"K. P.",
""
],
[
"Torres",
"A. Martinez",
""
],
[
"Oller",
"J. A.",
""
],
[
"Roca",
"L.",
""
]
] | [
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] |
712.3014 | Gavin Salam | Mrinal Dasgupta, Lorenzo Magnea and Gavin P. Salam | Non-perturbative QCD effects in jets at hadron colliders | 33 pages, 7 figures | JHEP 0802:055,2008 | 10.1088/1126-6708/2008/02/055 | null | hep-ph | null | We discuss non-perturbative QCD contributions to jet observables, computing
their dependence on the jet radius R, and on the colour and transverse momentum
of the parton initiating the jet. We show, using analytic QCD models of power
corrections as well as Monte Carlo simulations, that hadronisation corrections
grow at small values of R, behaving as 1/R, while underlying event
contributions grow with the jet area as R^2. We highlight the connection
between hadronisation corrections to jets and those for event shapes in e^+e^-
and DIS; we note the limited dependence of our results on the choice of jet
algorithm; finally, we propose several measurements in the context of which to
test or implement our predictions. The results presented here reinforce the
motivation for the use of a range of R values, as well as a plurality of
infrared-safe jet algorithms, in precision jet studies at hadron colliders.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:32:17 GMT"
}
] | 2009-04-30T00:00:00 | [
[
"Dasgupta",
"Mrinal",
""
],
[
"Magnea",
"Lorenzo",
""
],
[
"Salam",
"Gavin P.",
""
]
] | [
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] |
712.3015 | Bobby Ramsey Jr | Bobby W. Ramsey | A Spectral sequence for polynomially bounded cohomology | 20 pages, no figures | null | 10.1016/j.jpaa.2012.10.001 | null | math.KT math.GR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We construct an analogue of the Lyndon-Hochschild-Serre spectral sequence in
the context of polynomial cohomology, for group extensions. If G is an
extension of Q by H, then the spectral sequence converges to the polynomial
cohomology of G. For the polynomial extensions of Noskov with normal subgroup
isocohomological, the E_2 term is the polynomial cohomology of Q with
coefficients in the polynomial cohomology of H. When both Q and H are
isocohomological G must be as well. By referencing results of Connes-Moscovici
and Noskov, if Q and H are both isocohomological and have the Rapid Decay
property of Jolissaint, then G satisfies the Novikov Conjecture.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:10:08 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Sep 2012 17:02:11 GMT"
}
] | 2012-12-12T00:00:00 | [
[
"Ramsey",
"Bobby W.",
""
]
] | [
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] |
712.3016 | Stefan Legel | Stefan Legel, J\"urgen K\"onig, Gerd Sch\"on | Generation and detection of a spin entanglement in nonequilibrium
quantum dots | 6 pages, 3 figures | New. J. Phys. 10 (2008) 045016 | 10.1088/1367-2630/10/4/045016 | null | cond-mat.mes-hall | null | Spin entanglement between two spatially separated electrons can be generated
in nonequilibrium interacting quantum dots, coherently coupled to a common
lead. In this system entangled two-electron states develop which are Werner
states with an imbalance between singlet and triplet probabilities. We propose
a multi-terminal, multiply-connected setup for the generation and detection of
this imbalance. In particular, we identify a regime in which the formation of
spin entanglement leads to a cancellation of Aharonov-Bohm oscillations.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:16:51 GMT"
},
{
"version": "v2",
"created": "Fri, 2 May 2008 14:21:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Legel",
"Stefan",
""
],
[
"König",
"Jürgen",
""
],
[
"Schön",
"Gerd",
""
]
] | [
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712.3017 | Marco Miceli | M. Miceli, F. Bocchino, F. Reale | Physical and chemical inhomogeneities inside the Vela SNR shell.
Indications of ejecta shrapnels | Accepted for publication in The Astrophysical Journal. For the
version of the paper with high resolution images, please see
http://www.astropa.unipa.it/Library/preprint.html | null | 10.1086/528737 | null | astro-ph | null | We present the results of the combined analysis of three XMM-Newton EPIC
observations of the northern rim of the Vela SNR. The three pointings cover an
area of ~10 pc^2 (at 250 pc) behind the main shock front and we aim at studying
with high resolution the spatial distribution of the physical and chemical
properties of the X-ray emitting plasma on this large scale. We produce
count-rate images and equivalent width maps of the Ne IX and Mg XI emission
blends. We also perform a spatially resolved spectral analysis of a set of
physically homogeneous regions. We reveal physical and chemical inhomogeneities
in the X-ray emitting plasma. In particular, we find large variations of the O,
Ne, Mg, and Fe abundances. In some bright knots we also find unexpectedly
enhanced Ne and Mg abundances, with values significantly larger than solar. Our
results support a possible association of a few X-ray emitting knots with
previously undetected residuals of stellar fragments (i. e. shrapnels)
observed, in projection, inside the Vela shell.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:21:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Miceli",
"M.",
""
],
[
"Bocchino",
"F.",
""
],
[
"Reale",
"F.",
""
]
] | [
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] |
712.3018 | Julien Dub\'edat | Julien Dubedat | SLE and the free field: Partition functions and couplings | 55 pages, 4 figures. v2: additional material | null | null | null | math.PR | null | Schramm-Loewner Evolutions ($\SLE$) are random curves in planar simply
connected domains; the massless (Euclidean) free field in such a domain is a
random distribution. Both have conformal invariance properties in law. In the
present article, some relations between the two objects are studied. We
establish identities of partition functions between different versions of
$\SLE$ and the free field with appropriate boundary conditions; this involves
$\zeta$-regularization and the Polyakov-Alvarez conformal anomaly formula. We
proceed with a construction of couplings of $\SLE$ with the free field, showing
that, in a precise sense, chordal $\SLE$ is the solution of a stochastic
"differential" equation driven by the free field. Existence, uniqueness in law,
and pathwise uniqueness for these SDEs are proved for general $\kappa>0$.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:30:12 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Jan 2008 17:53:45 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Dubedat",
"Julien",
""
]
] | [
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712.3019 | Ariel Yadin | Ariel Yadin | When Do Random Subsets Decompose a Finite Group? | null | null | null | null | math.PR math.GR | null | Let A,B be two random subsets of a finite group G. We consider the event that
the products of elements from A and B span the whole group; i.e. (AB union BA)
= G. The study of this event gives rise to a group invariant we call \Theta(G).
\Theta(G) is between 1/2 and 1, and is 1 if and only if the group is abelian.
We show that a phase transition occurs as the size of A and B passes
\sqrt{\Theta(G)|G|\log|G|}; i.e. for any c>0, if the size of A and B is less
than (1-c)\sqrt{\Theta(G)|G|\log|G|}, then with high probability (AB union BA)
does not equal G. If A and B are larger than (1+c)\sqrt{\Theta(G)|G|\log|G|}
then (AB union BA) equals G with high probability.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:41:36 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Yadin",
"Ariel",
""
]
] | [
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] |
712.302 | Leonid Mirny | Carlos Gomez-Uribe, George C. Verghese, and Leonid A. Mirny | Operating Regimes of Signaling Cycles: Statics, Dynamics, and Noise
Filtering | to appear in PLoS Computational Biology | null | 10.1371/journal.pcbi.0030246 | null | q-bio.MN q-bio.BM q-bio.QM q-bio.SC | null | A ubiquitous building block of signaling pathways is a cycle of covalent
modification (e.g., phosphorylation and dephosphorylation in MAPK cascades).
Our paper explores the kind of information processing and filtering that can be
accomplished by this simple biochemical circuit.
Signaling cycles are particularly known for exhibiting a highly sigmoidal
(ultrasensitive) input-output characteristic in a certain steady-state regime.
Here we systematically study the cycle's steady-state behavior and its response
to time-varying stimuli. We demonstrate that the cycle can actually operate in
four different regimes, each with its specific input-output characteristics.
These results are obtained using the total quasi-steady-state approximation,
which is more generally valid than the typically used Michaelis-Menten
approximation for enzymatic reactions. We invoke experimental data that
suggests the possibility of signaling cycles operating in one of the new
regimes.
We then consider the cycle's dynamic behavior, which has so far been
relatively neglected. We demonstrate that the intrinsic architecture of the
cycles makes them act - in all four regimes - as tunable low-pass filters,
filtering out high-frequency fluctuations or noise in signals and environmental
cues. Moreover, the cutoff frequency can be adjusted by the cell. Numerical
simulations show that our analytical results hold well even for noise of large
amplitude. We suggest that noise filtering and tunability make signaling cycles
versatile components of more elaborate cell signaling pathways.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:43:43 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Gomez-Uribe",
"Carlos",
""
],
[
"Verghese",
"George C.",
""
],
[
"Mirny",
"Leonid A.",
""
]
] | [
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712.3021 | Camille Laurent-Gengoux | Yvette Kosmann-Schwarzbach, Camille Laurent-Gengoux, Alan Weinstein | Modular classes of Lie algebroid morphisms | 33 pages. Dedicated to Bertram Kostant for his eightieth birthday.
Minor changes in version 2: Proposition 3.11 added, typos corected | null | null | null | math.DG math.SG | null | We study the behavior of the modular class of a Lie algebroid under general
Lie algebroid morphisms by introducing the relative modular class. We
investigate the modular classes of pull-back morphisms and of base-preserving
morphisms associated to Lie algebroid extensions. We also define generalized
morphisms, including Morita equivalences, that act on the 1-cohomology, and
observe that the relative modular class is a coboundary on the category of Lie
algebroids and generalized morphisms with values in the 1-cohomology.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:50:04 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Apr 2008 15:15:32 GMT"
}
] | 2008-04-18T00:00:00 | [
[
"Kosmann-Schwarzbach",
"Yvette",
""
],
[
"Laurent-Gengoux",
"Camille",
""
],
[
"Weinstein",
"Alan",
""
]
] | [
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712.3022 | Mike McCulloch | M.E. McCulloch | Can the flyby anomalies be explained by a modification of inertia? | Presented at a BIS symposium on 15/11/2007, and submitted to JBIS. 13
pages, 4 figures | J.Br.Interplanet.Soc. 61: 373-378, 2008 | null | null | astro-ph physics.gen-ph | null | The flyby anomalies are unexplained velocity increases of 3.9, 13.5, 0.1 and
1.8 mm/s observed near closest approach during the Earth flybys of the Galileo,
NEAR, Cassini and Rosetta spacecraft. Here, these flybys are modelled using a
theory that assumes that inertia is caused by a form of Unruh radiation,
modified by a Hubble-scale Casimir effect. This theory predicts that when the
craft's accelerations relative to the galactic centre approached zero near
closest approach, their inertial masses reduced for about 10^-7 s causing
Earthward jumps of 2.6, 1.2, 1.4 and 1.9 mm/s respectively, and, to conserve
angular momentum, increases in orbital velocity of a few mm/s that, except
NEAR's, were quite close to those observed. However, these results were
extremely sensitive to the Hubble constant used. As an experimental test of
these ideas, it is proposed that metamaterials could be used to bend Unruh
radiation around objects, possibly reducing their inertial mass.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 18:54:30 GMT"
}
] | 2011-09-15T00:00:00 | [
[
"McCulloch",
"M. E.",
""
]
] | [
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712.3023 | Neil Dobbs | Neil Dobbs | Renormalisation-induced phase transitions for unimodal maps | 14 pages, 2 figures. Revised following comments of referees. First
page is blank | Commun. Math. Phys. 286, 377\^a?"387 (2009) | 10.1007/s00220-008-0656-5 | null | math.DS | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The thermodynamical formalism is studied for renormalisable maps of the
interval and the natural potential $-t \log|Df|$. Multiple and indeed
infinitely many phase transitions at positive $t$ can occur for some quadratic
maps. All unimodal quadratic maps with positive topological entropy exhibit a
phase transition in the negative spectrum.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:02:42 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jul 2008 14:22:27 GMT"
}
] | 2009-02-18T00:00:00 | [
[
"Dobbs",
"Neil",
""
]
] | [
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] |
712.3024 | K. C. Steenbrugge | K. C. Steenbrugge, K. M. Blundell, P. Duffy | Detection of a relic X-ray jet in Cygnus A | 4 pages. Proceedings of "High Energy Phenomena in Relativistic
Outflows", held in Dublin, Ireland, September 24-28, 2007 | Int.J.Mod.Phys.D17:1561-1567,2008 | 10.1142/S0218271808013157 | null | astro-ph | null | We present a 200 ks Chandra ACIS-I image of Cygnus A, and discuss a long
linear feature seen in its counterlobe. This feature has a non-thermal spectrum
and lies on the line connecting the brighter hotspot on the approaching side
and the nucleus. We therefore conclude that this feature is (or was) a jet.
However, the outer part of this X-ray jet does not trace the current counterjet
observed in radio. No X-ray counterpart is observed on the jet side. Using
light-travel time effects we conclude that this X-ray 50 kpc linear feature is
a relic jet that contains enough low-energy plasma (gamma ~ 10^3) to
inverse-Compton scatter cosmic microwave background photons, producing emission
in the X-rays.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:33:55 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Steenbrugge",
"K. C.",
""
],
[
"Blundell",
"K. M.",
""
],
[
"Duffy",
"P.",
""
]
] | [
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712.3025 | Mihail Chizhov | Mihail V. Chizhov | Can we use hadronic tau decay for V_us determination | 17 pages, 5 figures | null | null | null | hep-ph hep-ex hep-lat | null | It is known that the discrepancy in pion spectral functions extracted from
positron-electron annihilation and tau decay leads to different predictions for
the muon anomalous magnetic moment. We will show that this discrepancy effects
also the extraction of the Cabibbo angle from the hadronic tau decays. The
corrections to the tau branching fractions, corresponding to the presence of
new centi-weak tensor interactions, allow us to extract the Cabibbo angle from
tau decays in agreement with its other precision determinations. Thus a more
precise value of |V_us|=0.2246 +/- 0.0012 is obtained and as a consequence
f(0)=0.9645 +/- 0.0055 and F_K/F_pi=1.196 +/- 0.007.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:12:54 GMT"
}
] | 2008-01-30T00:00:00 | [
[
"Chizhov",
"Mihail V.",
""
]
] | [
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712.3026 | Elena Rubei | Elena Rubei | Sets of double and triple weights of trees | 11 pages, to appear in Annals of Combinatorics | null | null | null | math.AG math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let T be a weighted tree with n leaves. Let D_{i,j} be the distance between
the leaves i and j. Let D_{i,j,k}= (D_{i,j} + D_{j,k} +D_{i,k})/2. We will call
such numbers "triple weights" of the tree. In this paper, we give a
characterization, different from the previous ones, for sets indexed by
2-subsets of a $n$-set to be double weights of a tree. By using the same
ideas,we find also necessary and sufficient conditions for a set of real
numbers indexed by 3-subsets of an $n$-set to be the set of the triple weights
of a tree with $n$ leaves. Besides we propose a slight modification of
Saitou-Nei's Neighbour-Joining algorithm to reconstruct trees from the data
D_{i,j}.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:18:36 GMT"
},
{
"version": "v2",
"created": "Tue, 9 Jun 2009 17:42:44 GMT"
},
{
"version": "v3",
"created": "Fri, 22 Apr 2011 11:54:03 GMT"
}
] | 2011-04-25T00:00:00 | [
[
"Rubei",
"Elena",
""
]
] | [
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] |
712.3027 | Pawel Sobkowicz | Pawel Sobkowicz | Simple queueing approach to segregation dynamics in Schelling model | null | null | null | null | cond-mat.dis-nn physics.soc-ph | null | A simple queueing approach for segregation of agents in modified one
dimensional Schelling segregation model is presented. The goal is to arrive at
simple formula for the number of unhappy agents remaining after the
segregation.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:20:26 GMT"
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] | 2007-12-19T00:00:00 | [
[
"Sobkowicz",
"Pawel",
""
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712.3028 | Licia Verde | Licia Verde (ICREA and Institute of Space Sciences, IEEC-CSIC) | A practical guide to Basic Statistical Techniques for Data Analysis in
Cosmology | To appear in the proceedings of the XIX Canary Island Winter School
"The Cosmic Microwave Background: from Quantum fluctuations to the present
Universe", comments welcome. (fixed entry of table1) | null | null | null | astro-ph | null | This is the summary of 4 Lectures given at the XIX Canary islands winter
school of Astrophysics ''The Cosmic Microwave Background, from Quantum
Fluctuations to the present Universe''. Lectures were intended for
master/beginning PhD students in cosmology.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:30:58 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 11:00:58 GMT"
}
] | 2008-01-07T00:00:00 | [
[
"Verde",
"Licia",
"",
"ICREA and Institute of Space Sciences, IEEC-CSIC"
]
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712.3029 | Marcin Bilski | Marcin Bilski | Approximation of sets defined by polynomials with holomorphic
coefficients | 10 pages | null | null | null | math.CV | null | Let X be an analytic set defined by polynomials whose coefficients
a_1,...,a_s are holomorphic functions. We formulate conditions such that for
all sequences {a_(1,n)},...,{a_(s,n)} of holomorphic functions converging
locally uniformly to a_1,...,a_s respectively the following holds true. If
a_(1,n),...,a_(s,n) satisfy the conditions then the sequence of the sets {X_n}
obtained by replacing a_j by a_(j,n) in the polynomials, converge to X.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:24:20 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Bilski",
"Marcin",
""
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] |
712.303 | Janusz Skalski | J. Skalski | Nuclear fission with mean-field instantons | null | Phys.Rev.C77:064610,2008 | 10.1103/PhysRevC.77.064610 | null | nucl-th | null | We present a description of nuclear spontaneous fission, and generally of
quantum tunneling, in terms of instantons - periodic imaginary-time solutions
to time-dependent mean-field equations - that allows for a comparison with more
familiar and used generator coordinate (GCM) and adiabatic time-dependent
Hartree-Fock (ATDHF) methods. It is shown that the action functional whose
value for the instanton is the quasiclassical estimate of the decay exponent
fulfils the minimum principle when additional constraints are imposed on trial
fission paths. In analogy with mechanics, these are conditions of energy
conservation and the velocity-momentum relations. In the adiabatic limit the
instanton method reduces to the time-odd ATDHF equation, with collective mass
including the time-odd Thouless-Valatin term, while the GCM mass completely
ignores velocity-momentum relations. This implies that GCM inertia generally
overestimates instanton-related decay rate.
The very existence of the minimum principle offers a hope for a variational
search for instantons. After the inclusion of pairing, the instanton equations
and the variational principle can be expressed in terms of the
imaginary-time-dependent Hartree-Fock- Bogolyubov (TDHFB) theory. The adiabatic
limit of this theory reproduces ATDHFB inertia.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:30:31 GMT"
},
{
"version": "v2",
"created": "Fri, 16 May 2008 15:41:01 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Skalski",
"J.",
""
]
] | [
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712.3031 | Elena Rubei | Elena Rubei | Stability of homogeneous bundles on P^3 | to appear in Geometriae Dedicata
http://www.springer.com/mathematics/geometry/journal/10711 | null | 10.1007/s10711-011-9617-9 | null | math.AG math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the stability of some homogeneous bundles on P^3 by using their
representations of the quiver associated to the homgeneous bundles on P^3. In
particular we show that homogeneous bundles on P^3 whose support of the quiver
representation is a parallelepiped are stable, for instance the bundles E whose
minimal free resolution is of the kind 0 --> S^{l_1, l_2, l_3} V (t) --> S^{l_1
+s, l_2, l_3} V (t+s) --> E --> 0 are stable.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:36:00 GMT"
},
{
"version": "v2",
"created": "Mon, 2 May 2011 14:23:31 GMT"
}
] | 2011-05-03T00:00:00 | [
[
"Rubei",
"Elena",
""
]
] | [
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] |
712.3032 | Mauricio Bellini | Federico Agustin Membiela (Mar del Plata University & CONICET),
Mauricio Bellini (Mar del Plata University & CONICET) | Power spectrum of large-scale magnetic fields from
Gravitoelectromagnetic inflation with a decaying cosmological parameter | 7 pages, no figures | null | null | null | hep-th | null | Introducing a variable cosmological parameter $\Lambda (t)$ in a geometrical
manner from a 5D Riemann-flat metric, we investigate the origin and evolution
of primordial magnetic fields in the early universe, when the expansion is
governed by a cosmological parameter $\Lambda (t)$ that decreases with time.
Using the gravitoelectromagnetic inflationary formalism, but without the
Feynman gauge, we obtain the power of spectrums for large-scale magnetic fields
and the inflaton field fluctuations during inflation. A very important fact is
that our formalism is {\em naturally non-conformally invariant}.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:42:55 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Membiela",
"Federico Agustin",
"",
"Mar del Plata University & CONICET"
],
[
"Bellini",
"Mauricio",
"",
"Mar del Plata University & CONICET"
]
] | [
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] |
712.3033 | Brant M. Johnson | PHENIX Collaboration, S. Afanasiev, et al | Particle-species dependent modification of jet-induced correlations in
Au+Au collisions at sqrt(s_NN) = 200 GeV | 344 authors, 4 pages text, RevTeX, 4 figures. Submitted to Physical
Review Letters. Plain text data tables for the points plotted in figures for
this and previous PHENIX publications are (or will be) publicly available at
http://www.phenix.bnl.gov/papers.html | Phys.Rev.Lett.101:082301,2008 | 10.1103/PhysRevLett.101.082301 | null | nucl-ex | null | We report PHENIX measurements of the correlation of a trigger hadron at
intermediate transverse momentum (2.5<p_{T,trig}<4 GeV/c), with associated
mesons or baryons at lower p_{T,assoc}, in Au+Au collisions at sqrt(s_NN) = 200
GeV. The jet correlations for both baryons and mesons show similar shape
alterations as a function of centrality, characteristic of strong modification
of the away-side jet. The ratio of jet-associated baryons to mesons for this
jet increases with centrality and p_{T,assoc} and, in the most central
collisions, reaches a value similar to that for inclusive measurements. This
trend is incompatible with in-vacuum fragmentation, but could be due to
jet-like contributions from correlated soft partons which recombine upon
hadronization.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:39:34 GMT"
}
] | 2008-11-26T00:00:00 | [
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"",
""
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"Afanasiev",
"S.",
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712.3034 | Noah Graham | E. Farhi, N. Graham, A. H. Guth, N. Iqbal, R. R. Rosales, N.
Stamatopoulos | Emergence of Oscillons in an Expanding Background | 13 pages, 4 .eps figures, uses RevTeX4; v2: clarified details of
expansion, added references | Phys.Rev.D77:085019,2008 | 10.1103/PhysRevD.77.085019 | MIT-CTP 3924 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider a (1+1) dimensional scalar field theory that supports oscillons,
which are localized, oscillatory, stable solutions to nonlinear equations of
motion. We study this theory in an expanding background and show that oscillons
now lose energy, but at a rate that is exponentially small when the expansion
rate is slow. We also show numerically that a universe that starts with
(almost) thermal initial conditions will cool to a final state where a
significant fraction of the energy of the universe -- on the order of 50% -- is
stored in oscillons. If this phenomenon persists in realistic models, oscillons
may have cosmological consequences.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:48:31 GMT"
},
{
"version": "v2",
"created": "Wed, 11 Jun 2008 23:33:52 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Farhi",
"E.",
""
],
[
"Graham",
"N.",
""
],
[
"Guth",
"A. H.",
""
],
[
"Iqbal",
"N.",
""
],
[
"Rosales",
"R. R.",
""
],
[
"Stamatopoulos",
"N.",
""
]
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712.3035 | Russell Lyons | Russell Lyons | Identities and Inequalities for Tree Entropy | 12 pages; revision contains more background | Combin. Probab. Comput. 19, no. 2 (2010), 303-313. | null | null | math.CO math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The notion of tree entropy was introduced by the author as a normalized limit
of the number of spanning trees in finite graphs, but is defined on random
infinite rooted graphs. We give some new expressions for tree entropy; one uses
Fuglede-Kadison determinants, while another uses effective resistance. We use
the latter to prove that tree entropy respects stochastic domination. We also
prove that tree entropy is non-negative in the unweighted case, a special case
of which establishes Lueck's Determinant Conjecture for Cayley-graph
Laplacians. We use techniques from the theory of operators affiliated to von
Neumann algebras.
| [
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{
"version": "v2",
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] |
712.3036 | Biagio Lucini | Luigi Del Debbio, Biagio Lucini, Agostino Patella and Claudio Pica | Quenched mesonic spectrum at large N | Reference added; typos corrected; version to appear on JHEP | JHEP 0803:062,2008 | 10.1088/1126-6708/2008/03/062 | BNL-NT-07/56, IFUP-TH/2007-36, NI07089 | hep-th hep-lat hep-ph | null | We compute the masses of the $\pi$ and of the $\rho$ mesons in the quenched
approximation on a lattice with fixed lattice spacing $a \simeq 0.145 \
\mathrm{fm}$ for SU($N$) gauge theory with $N = 2,3,4,6$. We find that a simple
linear expression in $1/N^2$ correctly captures the features of the
lowest-lying meson states at those values of $N$. This enables us to
extrapolate to $N = \infty$ the behaviour of $m_{\pi}$ as a function of the
quark mass and of $m_{\rho}$ as a function of $m_{\pi}$. Our results for the
latter agree within 5% with recent predictions obtained in the AdS/CFT
framework.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:06:19 GMT"
},
{
"version": "v2",
"created": "Sun, 16 Mar 2008 23:07:40 GMT"
}
] | 2009-12-10T00:00:00 | [
[
"Del Debbio",
"Luigi",
""
],
[
"Lucini",
"Biagio",
""
],
[
"Patella",
"Agostino",
""
],
[
"Pica",
"Claudio",
""
]
] | [
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] |
712.3037 | Manik Lal Das | Manik Lal Das | Comments on "Improved Efficient Remote User Authentication Schemes" | null | International Journal of Network Security, Vol. 6, No. 3, pp.
282-284, 2008 | null | null | cs.CR | null | Recently, Tian et al presented an article, in which they discussed some
security weaknesses of Yoon et al's scheme and subsequently proposed two
``improved'' schemes. In this paper, we show that the Tian et al's schemes are
insecure and vulnerable than the Yoon et al's scheme.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:26:39 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Das",
"Manik Lal",
""
]
] | [
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712.3038 | Matthew Johnson | Anthony Aguirre, Matthew C Johnson | Towards observable signatures of other bubble universes II: Exact
solutions for thin-wall bubble collisions | 18 PRD-style pages, 12 figures. Added appendix on the expected number
of collisions, added references, minor correction to Appendix C, conclusions
unchanged. Replaced to match published version | Phys.Rev.D77:123536,2008 | 10.1103/PhysRevD.77.123536 | null | hep-th astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We assess the effects of a collision between two vacuum bubbles in the
thin-wall limit. After describing the outcome of a generic collision possessing
the expected hyperbolic symmetry, we focus on collisions experienced by a
bubble containing positive vacuum energy, which could in principle contain our
observable universe. We provide criteria governing whether the post-collision
domain wall accelerates towards or away from this "observation" bubble, and
discuss the implications for observers located at various positions inside of
the bubble. Then, we identify the class of solutions which have minimal impact
on the interior of the observation bubble, and derive a simple formula for the
energy density of a shell of radiation emitted from such a collision. In the
context of a universe undergoing false vacuum eternal inflation, these
solutions are perhaps the most promising candidates for collisions that could
exist within our past light cone, and therefore in principle be observable.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:47:15 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Jan 2008 19:02:54 GMT"
},
{
"version": "v3",
"created": "Mon, 28 Jan 2008 20:03:34 GMT"
},
{
"version": "v4",
"created": "Tue, 22 Jul 2008 21:06:26 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Aguirre",
"Anthony",
""
],
[
"Johnson",
"Matthew C",
""
]
] | [
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] |
712.3039 | Peter Wong | Marek Golasinski, Daciberg Goncalves, Peter Wong | A note on generalized equivariant homotopy groups | 9 pages, submitted to Proceedings for Postnikov Memorial Conference | Algebraic topology--old and new, 179--185, Banach Center Publ.,
85, Polish Acad. Sci. Inst. Math., Warsaw, 2009 | null | null | math.AT | null | In this paper, we generalize the equivariant homotopy groups or equivalently
the Rhodes groups. We establish a short exact sequence relating the generalized
Rhodes groups and the generalized Fox homotopy groups and we introduce
$\Gamma$-Rhodes groups, where $\Gamma$ admits a certain co-grouplike structure.
Evaluation subgroups of $\Gamma$-Rhodes groups are discussed.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:31:57 GMT"
}
] | 2011-05-11T00:00:00 | [
[
"Golasinski",
"Marek",
""
],
[
"Goncalves",
"Daciberg",
""
],
[
"Wong",
"Peter",
""
]
] | [
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] |
712.304 | Kristian McDonald | Robert Foot, Archil Kobakhidze, Kristian L. McDonald, Raymond R.
Volkas | Renormalization-scale independence of the physical cosmological constant | 3 pages; V2 to appear in PLB | Phys.Lett.B664:199-200,2008 | 10.1016/j.physletb.2008.05.029 | null | hep-th gr-qc hep-ph | null | Treating the metric as a classical background field, we show that the
cosmological constant does not run with the renormalization scale -- contrary
to some claims in the literature.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:32:10 GMT"
},
{
"version": "v2",
"created": "Tue, 13 May 2008 21:15:18 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Foot",
"Robert",
""
],
[
"Kobakhidze",
"Archil",
""
],
[
"McDonald",
"Kristian L.",
""
],
[
"Volkas",
"Raymond R.",
""
]
] | [
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] |
712.3041 | Yi-Kai Liu | Yi-Kai Liu | The Complexity of the Consistency and N-representability Problems for
Quantum States | PhD thesis. Yay, no more grad school!! (Finished in August, but did
not get around to posting it until now.) 91 pages, a few figures, some boring
sections. Has detailed proofs of results in quant-ph/0604166 and
quant-ph/0609125. Ch.4 is a preliminary sketch of 0712.1388. Ch.5 is
quant-ph/0603012 | null | null | null | quant-ph | null | QMA (Quantum Merlin-Arthur) is the quantum analogue of the class NP. There
are a few QMA-complete problems, most notably the ``Local Hamiltonian'' problem
introduced by Kitaev. In this dissertation we show some new QMA-complete
problems.
The first one is ``Consistency of Local Density Matrices'': given several
density matrices describing different (constant-size) subsets of an n-qubit
system, decide whether these are consistent with a single global state. This
problem was first suggested by Aharonov. We show that it is QMA-complete, via
an oracle reduction from Local Hamiltonian. This uses algorithms for convex
optimization with a membership oracle, due to Yudin and Nemirovskii.
Next we show that two problems from quantum chemistry, ``Fermionic Local
Hamiltonian'' and ``N-representability,'' are QMA-complete. These problems
arise in calculating the ground state energies of molecular systems.
N-representability is a key component in recently developed numerical methods
using the contracted Schrodinger equation. Although these problems have been
studied since the 1960's, it is only recently that the theory of quantum
computation has allowed us to properly characterize their complexity.
Finally, we study some special cases of the Consistency problem, pertaining
to 1-dimensional and ``stoquastic'' systems. We also give an alternative proof
of a result due to Jaynes: whenever local density matrices are consistent, they
are consistent with a Gibbs state.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:37:22 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Liu",
"Yi-Kai",
""
]
] | [
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712.3042 | Ulrich S. Schwarz | T. Erdmann, S. Pierrat, P. Nassoy and U. S. Schwarz | Dynamic force spectroscopy on multiple bonds: experiments and model | to appear in Europhysics Letters | Europhys. Lett., 81:48001, 2008 | 10.1209/0295-5075/81/48001 | null | q-bio.BM cond-mat.soft physics.bio-ph | null | We probe the dynamic strength of multiple biotin-streptavidin adhesion bonds
under linear loading using the biomembrane force probe setup for dynamic force
spectroscopy. Measured rupture force histograms are compared to results from a
master equation model for the stochastic dynamics of bond rupture under load.
This allows us to extract the distribution of the number of initially closed
bonds. We also extract the molecular parameters of the adhesion bonds, in good
agreement with earlier results from single bond experiments. Our analysis shows
that the peaks in the measured histograms are not simple multiples of the
single bond values, but follow from a superposition procedure which generates
different peak positions.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:37:48 GMT"
}
] | 2010-02-24T00:00:00 | [
[
"Erdmann",
"T.",
""
],
[
"Pierrat",
"S.",
""
],
[
"Nassoy",
"P.",
""
],
[
"Schwarz",
"U. S.",
""
]
] | [
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] |
712.3043 | Mark Everitt | M.J. Everitt | On the correspondence principle: implications from a study of the
chaotic dynamics of a macroscopic quantum device | 16 pages, 5 figures. significantly expanded - to be published in New
Journal of Physics | New J. Phys. 11 (2009) 013014 | 10.1088/1367-2630/11/1/013014 | null | quant-ph cond-mat.mes-hall cond-mat.other cond-mat.supr-con | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The recovery of classical chaotic dynamics from quantum systems has long been
a subject of interest. Furthermore, recent work indicates that quantum chaos
may well be significant in quantum information processing. In this paper we
discuss the quantum to classical crossover of a superconducting quantum
inference device (SQUID) ring. Such devices comprise of thick superconducting
loop enclosing a Josephson weak link. These devices are currently strong
candidates for many applications in quantum technologies. The weak link brings
with it a non-linearity such that semi-classical models of this system can
exhibit chaotic dynamics. For many similar systems an application of the
correspondence principle together with the inclusion of environmental degrees
of freedom through a quantum trajectories approach can be used to effectively
recover classical dynamics. Here we show (i) that the standard expression of
the correspondence principle is incompatible with the ring Hamiltonian and we
present a more pragmatic and general expression which finds application here
and (ii) that practical limitations to circuit parameters of the SQUID ring
prevent arbitrarily accurate recovery of classical chaotic dynamics.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:52:44 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 10:37:49 GMT"
},
{
"version": "v3",
"created": "Sat, 8 Nov 2008 18:31:56 GMT"
}
] | 2009-01-08T00:00:00 | [
[
"Everitt",
"M. J.",
""
]
] | [
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0.0288173854,
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0.0450563133,
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0.1105208248,
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] |
712.3044 | Maximilien Cazayous | M. Cazayous, Y. Gallais, A. Sacuto, R. De Sousa, D. Lebeugle, D.
Colson | Observation of electromagnon excitations in the BiFe0$_3$ spiral magnet | null | Phys. Rev. Lett. 101, 037601 (2008) | 10.1103/PhysRevLett.101.037601 | null | cond-mat.str-el | null | Recently, oxide multiferroics have attracted much attention due to their
large magnetoelectric effect which allows the tuning of magnetic properties
with electric field and vice versa and open new venues for future spintronic
applications such as multiple-state memory devices with dual magnetic and
electric control. BiFeO$_3$ (BFO) belongs to this new class of materials and
shows both ferroelectric and antiferromagnetic orders at room temperature with
a large electric polarizationassociated with a cycloidal spiral magnetic
ordering. The incommensurate magnetic order induces magnon zone folding and
allows investigations by optical probes of unusual spin waves which couples to
optical phonons, the so called "`electromagnons"'. Here, we unravel for the
first time the electromagnon spectra of BFO by means low energy inelastic light
scattering technique. We show the existence of two species of electromagnons
corresponding to spin wave excitations in and out of the cycloidal plane. The
present observations present an unique opportunity to study the interplay
between ferroelectric and magnetic orders.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:57:13 GMT"
}
] | 2010-10-12T00:00:00 | [
[
"Cazayous",
"M.",
""
],
[
"Gallais",
"Y.",
""
],
[
"Sacuto",
"A.",
""
],
[
"De Sousa",
"R.",
""
],
[
"Lebeugle",
"D.",
""
],
[
"Colson",
"D.",
""
]
] | [
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712.3045 | Rathindra Nath Sen (Retd) | R. N. Sen | Physics and the measurement of continuous variables | 20 pages | null | 10.1007/s10701-007-9203-z | null | quant-ph | null | Wigner had expressed the opinion that the impossibility of exact measurements
of single operators like position operators rendered the notion of geometrical
points somewhat dubious in physics. Using Sewell's recent resolution of the
measurement problem (collapse of the wave packet) in quantum mechanics and
extending it to the measurement of operators with continuous spectra, we are
able to compare the situation in quantum mechanics with that in quantum
mechanics. Our conclusion is that the notion of a geometrical point is as
meaningful in quantum mechanics as it is in classical mechanics.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:58:26 GMT"
}
] | 2007-12-19T00:00:00 | [
[
"Sen",
"R. N.",
""
]
] | [
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712.3046 | Ari Pakman | Gaston Giribet, Ari Pakman and Leonardo Rastelli | Spectral Flow in AdS(3)/CFT(2) | 50 pages, 2 figures | JHEP 0806:013,2008 | 10.1088/1126-6708/2008/06/013 | YITP-SB-07-38 | hep-th | null | We study the spectral flowed sectors of the H3 WZW model in the context of
the holographic duality between type IIB string theory in AdS(3)x S^3 x T^4
with NSNS flux and the symmetric product orbifold of T^4. We construct
explicitly the physical vertex operators in the flowed sectors that belong to
short representations of the superalgebra, thus completing the bulk-to-boundary
dictionary for 1/2 BPS states. We perform a partial calculation of the string
three-point functions of these operators. A complete calculation would require
the three-point couplings of non-extremal flowed operators in the H3 WZW model,
which are at present unavailable. In the unflowed sector, perfect agreement has
recently been found between the bulk and boundary three-point functions of 1/2
BPS operators. Assuming that this agreement persists in the flowed sectors, we
determine certain unknown three-point couplings in the H3 WZW model in terms of
three-point couplings of affine descendants in the SU(2) WZW model.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 20:58:51 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 01:39:25 GMT"
}
] | 2009-12-10T00:00:00 | [
[
"Giribet",
"Gaston",
""
],
[
"Pakman",
"Ari",
""
],
[
"Rastelli",
"Leonardo",
""
]
] | [
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] |
712.3047 | Rob Ivison | A. D. Biggs and R. J. Ivison (Edinburgh) | High-resolution radio observations of submillimetre galaxies | In press at MNRAS. 12 pages. High-resolution PDF version available at
http://www.roe.ac.uk/~rji/merlin.pdf | null | 10.1111/j.1365-2966.2008.12869.x | null | astro-ph | null | We have produced sensitive, high-resolution radio maps of 12 SMGs in the
Lockman Hole using combined MERLIN and VLA data at a frequency of 1.4 GHz.
Integrating for 350hr yielded an r.m.s. noise of 6.0 uJy/beam and a resolution
of 0.2-0.5". For the first time, wide-field data from the two arrays have been
combined in the (u,v) plane and the bandwidth smearing response of the VLA data
has been removed. All of the SMGs are detected in our maps as well as sources
comprising a non-submm luminous control sample. We find evidence that SMGs are
more extended than the general uJy radio population and that therefore, unlike
in local ULIRGs, the starburst component of the radio emission is extended and
not confined to the galactic nucleus. For the eight sources with redshifts we
measure linear sizes between 1 and 8 kpc with a median of 5 kpc. Therefore,
they are in general larger than local ULIRGs which may support an early-stage
merger scenario for the starburst trigger. X-rays betray AGN in six of the 33
sources in the combined sample. All but one of these are in the control sample,
suggesting a lower incidence of AGN amongst the submm-luminous galaxies which
is, in turn, consistent with increased X-ray absorption in these dust-obscured
starbursts. Only one of our sources is resolved into multiple, distinct
components with our high-resolution data. Finally, compared to a previous study
of faint radio sources in the GOODS-N field we find systematically smaller
source sizes and no evidence for a tail extending to ~4". Possible reasons for
this are discussed.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:00:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Biggs",
"A. D.",
"",
"Edinburgh"
],
[
"Ivison",
"R. J.",
"",
"Edinburgh"
]
] | [
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712.3048 | Ian Parrish | Ian J. Parrish, Eliot Quataert | Nonlinear Simulations of the Heat Flux Driven Buoyancy Instability and
its Implications for Galaxy Clusters | 4 pages, 4 figures, submitted to ApJ Letters | ApJ Letters 677 (2008), 9-12 | 10.1086/587937 | null | astro-ph | null | In low collisionality plasmas heat flows almost exclusively along magnetic
field lines, and the condition for stability to convection is modified from the
standard Schwarzschild criterion. We present local two and three-dimensional
simulations of a new heat flux driven buoyancy instability (the HBI) that
occurs when the temperature in a plasma decreases in the direction of gravity.
We find that the HBI drives a convective dynamo that amplifies an initially
weak magnetic field by a factor of ~20. In simulations that begin with the
magnetic field aligned with the temperature gradient, the HBI saturates by
rearranging the magnetic field lines to be almost purely perpendicular to the
initial temperature gradient. This magnetic field reorientation results in a
net heat flux through the plasma that is less than 1% of the field-free
(Spitzer) value. We show that the HBI is likely to be present in the cool cores
of clusters of galaxies between ~0.1-100 kpc, where the temperature increases
outwards. The saturated state of the HBI suggests that inward thermal
conduction from large radii in clusters is unlikely to solve the cooling flow
problem. Finally, we also suggest that the HBI may contribute to suppressing
conduction across cold fronts in galaxy clusters.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:21:22 GMT"
}
] | 2008-06-09T00:00:00 | [
[
"Parrish",
"Ian J.",
""
],
[
"Quataert",
"Eliot",
""
]
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712.3049 | Mark C. Neyrinck | Mark C. Neyrinck (IfA, Hawaii) | ZOBOV: a parameter-free void-finding algorithm | 10 pages, 8 figures, MNRAS, accepted. Added explanatory figures, and
better edge-detection methods. ZOBOV code available at
http://www.ifa.hawaii.edu/~neyrinck/voboz | Mon.Not.Roy.Astron.Soc. 386 (2008) 2101-2109 | 10.1111/j.1365-2966.2008.13180.x | null | astro-ph | null | ZOBOV (ZOnes Bordering On Voidness) is an algorithm that finds density
depressions in a set of points, without any free parameters, or assumptions
about shape. It uses the Voronoi tessellation to estimate densities, which it
uses to find both voids and subvoids. It also measures probabilities that each
void or subvoid arises from Poisson fluctuations. This paper describes the
ZOBOV algorithm, and the results from its application to the dark-matter
particles in a region of the Millennium Simulation. Additionally, the paper
points out an interesting high-density peak in the probability distribution of
dark-matter particle densities.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:25:12 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Feb 2008 20:56:59 GMT"
}
] | 2008-05-15T00:00:00 | [
[
"Neyrinck",
"Mark C.",
"",
"IfA, Hawaii"
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] |
712.305 | Alexei Kolezhuk | I. P. McCulloch, R. Kube, M. Kurz, A. Kleine, U. Schollwock, A. K.
Kolezhuk | Vector chiral order in frustrated spin chains | 8 pages, 9 figures | Phys. Rev. B 77, 094404 (2008) | 10.1103/PhysRevB.77.094404 | null | cond-mat.str-el cond-mat.other | null | By means of a numerical analysis using a non-Abelian symmetry realization of
the density matrix renormalization group, we study the behavior of vector
chirality correlations in isotropic frustrated chains of spin S=1 and S=1/2,
subject to a strong external magnetic field. It is shown that the field induces
a phase with spontaneously broken chiral symmetry, in line with earlier
theoretical predictions. We present results on the field dependence of the
order parameter and the critical exponents.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:01:12 GMT"
}
] | 2008-04-22T00:00:00 | [
[
"McCulloch",
"I. P.",
""
],
[
"Kube",
"R.",
""
],
[
"Kurz",
"M.",
""
],
[
"Kleine",
"A.",
""
],
[
"Schollwock",
"U.",
""
],
[
"Kolezhuk",
"A. K.",
""
]
] | [
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] |
712.3051 | Benjamin Johnson | Benjamin D. Johnson, David Schiminovich, Mark Seibert, Marie Treyer,
D. Christopher Martin, Tom A. Barlow, Karl Forster, Peter G. Friedman,
Patrick Morrissey, Susan G. Neff, Todd Small, Ted K. Wyder, Luciana Bianchi,
Jose Donas, Timothy M. Heckman, Young-Wook Lee, Barry F. Madore, Bruno
Milliard, R. Michael Rich, Alex S. Szalay, Barry Y. Welsh, Sukyoung K. Yi | Ultraviolet, Optical, and Infrared Constraints on Models of Stellar
Populations and Dust Attenuation | 16 pages, 11 figures, 2 tables. Appearing in the GALEX special issue
of ApJ Supp. (29 papers) | Astrophys.J.Suppl.173:377-391,2007 | 10.1086/522932 | null | astro-ph | null | The color of galaxies is a fundamental property, easily measured, that
constrains models of galaxies and their evolution. Dust attenuation and star
formation history (SFH) are the dominant factors affecting the color of
galaxies. Here we explore the empirical relation between SFH, attenuation, and
color for a wide range of galaxies, including early types. These galaxies have
been observed by GALEX, SDSS, and Spitzer, allowing the construction of
measures of dust attenuation from the ratio of infrared (IR) to ultraviolet
(UV) flux and measures of SFH from the strength of the 4000A break. The
empirical relation between these three quantities is compared to models that
separately predict the effects of dust and SFH on color. This comparison
demonstrates the quantitative consistency of these simple models with the data
and hints at the power of multiwavelength data for constraining these models.
The UV color is a strong constraint; we find that a Milky Way extinction curve
is disfavored, and that the UV emission of galaxies with large 4000A break
strengths is likely to arise from evolved populations. We perform fits to the
relation between SFH, attenuation, and color. This relation links the
production of starlight and its absorption by dust to the subsequent reemission
of the absorbed light in the IR. Galaxy models that self-consistently treat
dust absorption and emission as well as stellar populations will need to
reproduce these fitted relations in the low-redshift universe.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:03:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Johnson",
"Benjamin D.",
""
],
[
"Schiminovich",
"David",
""
],
[
"Seibert",
"Mark",
""
],
[
"Treyer",
"Marie",
""
],
[
"Martin",
"D. Christopher",
""
],
[
"Barlow",
"Tom A.",
""
],
[
"Forster",
"Karl",
""
],
[
"Friedman",
"Peter G.",
""
],
[
"Morrissey",
"Patrick",
""
],
[
"Neff",
"Susan G.",
""
],
[
"Small",
"Todd",
""
],
[
"Wyder",
"Ted K.",
""
],
[
"Bianchi",
"Luciana",
""
],
[
"Donas",
"Jose",
""
],
[
"Heckman",
"Timothy M.",
""
],
[
"Lee",
"Young-Wook",
""
],
[
"Madore",
"Barry F.",
""
],
[
"Milliard",
"Bruno",
""
],
[
"Rich",
"R. Michael",
""
],
[
"Szalay",
"Alex S.",
""
],
[
"Welsh",
"Barry Y.",
""
],
[
"Yi",
"Sukyoung K.",
""
]
] | [
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] |
712.3052 | Gregory Sivakoff | Gregory R. Sivakoff (1), Andr\'es Jord\'an (2), Adrienne M. Juett (3),
Craig L. Sarazin (4), Jimmy A. Irwin (5) ((1) The Ohio State University, (2)
Harvard-Smithsonian Center for Astrophysics, (3) NASA Goddard Space Flight
Center, (4) University of Virginia, (5) University of Michigan) | Variable Low-Mass X-ray Binaries in Early-Type Galaxies | Conference proceedings from 'A Population Explosion: The Nature and
Evolution of X-ray Binaries in Diverse Environments', 28 Oct - 2 Nov, St.
Petersburg Beach, FL. 5 pages, 2 B & W figures, 3 Color figures | AIP Conf.Proc.1010:308-312,2008 | 10.1063/1.2945063 | null | astro-ph | null | As the Chandra X-ray Observatory mission matures, increasing numbers of
nearby galaxies are being observed multiple times, sampling the variability of
extragalactic X-ray binaries on timescales extending from seconds to years. We
present results on luminous low-mass X-ray binaries from several early-type
galaxies. We show that instantaneous LMXB luminosity functions of early-type
galaxies do not significantly change between observations; a relatively low
fraction of sources are strongly variable on <~ 5 yr timescales. We discuss the
implications that a relatively small number of transient LMXBs are being
discovered in early-type galaxies.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:03:40 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Sivakoff",
"Gregory R.",
""
],
[
"Jordán",
"Andrés",
""
],
[
"Juett",
"Adrienne M.",
""
],
[
"Sarazin",
"Craig L.",
""
],
[
"Irwin",
"Jimmy A.",
""
]
] | [
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] |
712.3053 | Stella Offner | S. S. R. Offner (1), M. R. Krumholz (2), R. I. Klein (1 and 3), C. F.
McKee (1) ((1) University of California-Berkeley, (2) Princeton University,
(3) Lawrence Livermore National Laboratory) | The Kinematics of Molecular Cloud Cores in the Presence of Driven and
Decaying Turbulence: Comparisons with Observations | 18 pages, 12 figures, accepted to AJ | null | 10.1088/0004-6256/136/1/404 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this study we investigate the formation and properties of prestellar and
protostellar cores using hydrodynamic, self-gravitating Adaptive Mesh
Refinement simulations, comparing the cases where turbulence is continually
driven and where it is allowed to decay. We model observations of these cores
in the C$^{18}$O$(2\to 1)$, NH$_3(1,1)$, and N$_2$H$^+(1\to 0)$ lines, and from
the simulated observations we measure the linewidths of individual cores, the
linewidths of the surrounding gas, and the motions of the cores relative to one
another. Some of these distributions are significantly different in the driven
and decaying runs, making them potential diagnostics for determining whether
the turbulence in observed star-forming clouds is driven or decaying. Comparing
our simulations with observed cores in the Perseus and $\rho$ Ophiuchus clouds
shows reasonably good agreement between the observed and simulated core-to-core
velocity dispersions for both the driven and decaying cases. However, we find
that the linewidths through protostellar cores in both simulations are too
large compared to the observations. The disagreement is noticably worse for the
decaying simulation, in which cores show highly supersonic infall signatures in
their centers that decrease toward their edges, a pattern not seen in the
observed regions. This result gives some support to the use of driven
turbulence for modeling regions of star formation, but reaching a firm
conclusion on the relative merits of driven or decaying turbulence will require
more complete data on a larger sample of clouds as well as simulations that
include magnetic fields, outflows, and thermal feedback from the protostars.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:11:16 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Jul 2008 05:02:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Offner",
"S. S. R.",
"",
"1 and 3"
],
[
"Krumholz",
"M. R.",
"",
"1 and 3"
],
[
"Klein",
"R. I.",
"",
"1 and 3"
],
[
"McKee",
"C. F.",
""
]
] | [
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] |
712.3054 | Beth Willman | S. M. Walsh (ANU), B. Willman (CfA), D. Sand (Steward, U Arizona), J.
Harris (Steward, U Arizona), A. Seth (CfA), D. Zaritsky (Steward, U Arizona),
H. Jerjen (ANU) | Bootes II ReBooted: An MMT/MegaCam Study of An Ultra-Faint Milky Way
Satellite | 10 pages, 8 figures. ApJ accepted. Conclusions are unchanged, but
content and figures have changed substantively in this accepted version | null | 10.1086/592076 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | [abridged] We present MMT/Megacam imaging in Sloan $g$ and $r$ of the
extremely low luminosity Bo\"otes II Milky Way companion. We use a bootstrap
approach to perform robust measurements of, and uncertainties on, Bo\"otes II's
distance, luminosity, size, and morphology. We show that Bo\"otes II's stellar
population is old and metal-poor ([Fe/H] $\lta$ -2). Assuming a stellar
population like that of M92, Bo\"otes II is at a distance of 42 $\pm$ 2 kpc,
closer than the initial published estimate of 60 $\pm$ 10 kpc. This distance
revision, combined with a more robust measurement of Bo\"otes II's structure
with a Plummer model (exponential model) results in a more compact half-light
size of $r_h\simeq 36 (33) \pm 9 (10)$ pc and lower luminosity of
$M_V\simeq-2.4 (-2.2) \pm 0.7 (0.7)$ mag. This revised size and luminosity move
Bo\"otes II into a region of size-luminosity space not previously known to be
occupied by old stellar populations, but also occupied by the recently
discovered Milky Way satellites Willman 1 and SEGUE 1. We show that the
apparently distorted morphology of Bo\"otes II is not statistically significant
given the present data. We use a tidal argument to support a scenario where
Bo\"otes II is a dwarf galaxy (dark matter dominated) rather than a globular
cluster (not dark matter dominated). However, we can not rule out that Bo\"otes
II is a star cluster on the verge of disruption, such as Palomar 5.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:20:09 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jul 2008 16:36:47 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Walsh",
"S. M.",
"",
"ANU"
],
[
"Willman",
"B.",
"",
"CfA"
],
[
"Sand",
"D.",
"",
"Steward, U Arizona"
],
[
"Harris",
"J.",
"",
"Steward, U Arizona"
],
[
"Seth",
"A.",
"",
"CfA"
],
[
"Zaritsky",
"D.",
"",
"Steward, U Arizona"
],
[
"Jerjen",
"H.",
"",
"ANU"
]
] | [
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] |
712.3055 | Lech Longa | David Allender and Lech Longa | Landau-deGennes Theory of Biaxial Nematics Re-examined | 12 pages, 14 figures | Phys. Rev. E78, 011704 (2008) | 10.1103/PhysRevE.78.011704 | null | cond-mat.soft cond-mat.stat-mech | null | Recent experiments report that the long looked for thermotropic biaxial
nematic phase has been finally detected in some thermotropic liquid crystalline
systems. Inspired by these experimental observations we concentrate on some
elementary theoretical issues concerned with the classical sixth-order
Landau-deGennes free energy expansion in terms of the symmetric and traceless
tensor order parameter $Q_{\alpha\beta}$. In particular, we fully explore the
stability of the biaxial nematic phase giving analytical solutions for all
distinct classes of the phase diagrams that theory allows. This includes
diagrams with triple- and (tri-)critical points and with multiple (reentrant)
biaxial- and uniaxial phase transitions. A brief comparison with predictions of
existing molecular theories is also given.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 19:45:41 GMT"
}
] | 2008-09-24T00:00:00 | [
[
"Allender",
"David",
""
],
[
"Longa",
"Lech",
""
]
] | [
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] |
712.3056 | Alicia Johnson | Alicia A. Johnson and Galin L. Jones | Gibbs Sampling for a Bayesian Hierarchical General Linear Model | 20 pages, 1 figure, submitted to Electronic Journal of Statistics | null | null | null | stat.CO math.ST stat.TH | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider a Bayesian hierarchical version of the normal theory general
linear model which is practically relevant in the sense that it is general
enough to have many applications and it is not straightforward to sample
directly from the corresponding posterior distribution. Thus we study a block
Gibbs sampler that has the posterior as its invariant distribution. In
particular, we establish that the Gibbs sampler converges at a geometric rate.
This allows us to establish conditions for a central limit theorem for the
ergodic averages used to estimate features of the posterior. Geometric
ergodicity is also a key component for using batch means methods to
consistently estimate the variance of the asymptotic normal distribution.
Together, our results give practitioners the tools to be as confident in
inferences based on the observations from the Gibbs sampler as they would be
with inferences based on random samples from the posterior. Our theoretical
results are illustrated with an application to data on the cost of health plans
issued by health maintenance organizations.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:12:02 GMT"
},
{
"version": "v2",
"created": "Thu, 15 May 2008 15:10:31 GMT"
},
{
"version": "v3",
"created": "Mon, 27 Oct 2008 16:37:29 GMT"
},
{
"version": "v4",
"created": "Sat, 17 Oct 2009 19:53:46 GMT"
},
{
"version": "v5",
"created": "Thu, 21 Jan 2010 23:04:50 GMT"
}
] | 2010-01-22T00:00:00 | [
[
"Johnson",
"Alicia A.",
""
],
[
"Jones",
"Galin L.",
""
]
] | [
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712.3057 | Jing Shu | Ben Lillie, Jing Shu, Tim M.P. Tait | Top Compositeness at the Tevatron and LHC | 9 pages, 4 figures | JHEP 0804:087,2008 | 10.1088/1126-6708/2008/04/087 | ANL-HEP-PR-07-96, EFI/07-31, NUHEP-TH/07-11 | hep-ph | null | We explore the possibility that the right-handed top quark is composite. We
examine the consequences that compositeness would have on $t \bar{t}$
production at the Tevatron, and derive a weak constraint on the scale of
compositeness of order a few hundred GeV from the $t \bar{t}$ inclusive cross
section. More detailed studies of differential properties of $t \bar{t}$
production could potentially improve this limit. We find that a composite top
can result in an enhancement of the $t \bar{t} t \bar{t}$ production rate at
the LHC (of as much as $10^3$ compared to the Standatd Model four top rate). We
explore observables which allow us to extract the four top rate from the
backgrounds, and show that the LHC can either discover or constrain top
compositeness for wide ranges of parameter space.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:18:37 GMT"
}
] | 2009-02-18T00:00:00 | [
[
"Lillie",
"Ben",
""
],
[
"Shu",
"Jing",
""
],
[
"Tait",
"Tim M. P.",
""
]
] | [
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] |
712.3058 | Stephan Haas | Kazumi Maki, Aditya Raghavan, Stephan Haas | Chiral d-wave superconductivity in the heavy-fermion compound CeIrIn_5 | null | null | null | null | cond-mat.supr-con | null | Recent thermal conductivity measurements in the heavy-fermion compound
CeIrIn_5 indicate that its superconducting order parameter is very different
from CeCoIn_5. Here we show that these experiments are consistent with chiral
d-wave symmetry.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:19:30 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Maki",
"Kazumi",
""
],
[
"Raghavan",
"Aditya",
""
],
[
"Haas",
"Stephan",
""
]
] | [
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] |
712.3059 | Alex Hamilton | Alex Hamilton, Jeff Murugan, Andrea Prinsloo | A note on the universality of the Hagedorn behavior of pp-wave strings | 25 pages; fixed minor typo; added references | JHEP 0802:108,2008 | 10.1088/1126-6708/2008/02/108 | null | hep-th | null | Following on from recent studies of string theory on a one-parameter family
of integrable deformations of $AdS_{5}\times S^{5}$ proposed by Lunin and
Maldacena, we carry out a systematic analysis of the high temperature
properties of type IIB strings on the associated pp-wave geometries. In
particular, through the computation of the thermal partition function and free
energy we find that not only does the theory exhibit a Hagedorn transition in
both the $(J,0,0)$ and $(J,J,J)$ class of pp-waves, but that the Hagedorn
temperature is insensitive to the deformation suggesting an interesting
universality in the high temperature behaviour of the pp-wave string theory. We
comment also on the implications of this universality on the
confinement/deconfinement transition in the dual $\mathcal{N}=1$
Leigh-Strassler deformation of ${\cal N}=4$ Yang-Mills theory.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:20:22 GMT"
},
{
"version": "v2",
"created": "Thu, 21 Feb 2008 08:55:34 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Hamilton",
"Alex",
""
],
[
"Murugan",
"Jeff",
""
],
[
"Prinsloo",
"Andrea",
""
]
] | [
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] |
712.306 | Greg Martin | Greg Martin and Erick B. Wong | Almost all integer matrices have no integer eigenvalues | 9 pages, 1 figure | null | null | null | math.NT | null | For a fixed $n\ge2$, consider an $n\times n$ matrix $M$ whose entries are
random integers bounded by $k$ in absolute value. In this paper, we examine the
probability that $M$ is singular (hence has eigenvalue 0), and the probability
that $M$ has at least one rational eigenvalue. We show that both of these
probabilities tend to 0 as $k$ increases. More precisely, we establish an upper
bound of size $k^{-2+\epsilon}$ for the probability that $M$ is singular, and
size $k^{-1+\epsilon}$ for the probability that $M$ has a rational eigenvalue.
These results generalize earlier work by Kowalsky for the case $n=2$ and answer
a question posed by Hetzel, Liew, and Morrison.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:27:26 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Martin",
"Greg",
""
],
[
"Wong",
"Erick B.",
""
]
] | [
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] |
712.3061 | Surajit Saha | Surjeet Singh, Surajit Saha, S. K. Dhar, R. Suryanarayanan, A. K.
Sood, and A. Revcolevschi | Manifestation of geometric frustration on magnetic and thermodynamic
properties of pyrochlores $Sm_2X_2O_7$ (X=Ti, Zr) | 24 pages, 6 figures, Accepted for publication in Phys. Rev. B | null | 10.1103/PhysRevB.77.054408 | null | cond-mat.mtrl-sci | null | We present here magnetization, specific heat and Raman studies on
single-crystalline specimens of the first pyrochlore member $Sm_2Ti_2O_7$ of
the rare-earth titanate series. Its analogous compound $Sm_2Zr_2O_7$ in the
rare-earth zirconate series is also investigated in the polycrystalline form.
The Sm spins in $Sm_2Ti_2O_7$ remain unordered down to at least T = 0.5 K. The
absence of magnetic ordering is attributed to very small values of exchange
($\theta_{cw} ~ -0.26 K$) and dipolar interaction ($\mu_{eff} ~ 0.15 \mu_B$)
between the $Sm^{3+}$ spins in this pyrochlore. In contrast, the pyrochlore
$Sm_2Zr_2O_7$ is characterized by a relatively large value of Sm-Sm spin
exchange ($\theta_{cw} ~ - 10 K$); however, long-range ordering of the
$Sm^{3+}$ spins is not established at least down to T = 0.67 K, due to
frustration of the $Sm^{3+}$ spins on the pyrochlore lattice. The ground state
of $Sm^{3+}$ ions in both pyrochlores is a well-isolated Kramer's doublet. The
higher-lying crystal field excitations are observed in the low-frequency region
of the Raman spectra of the two compounds recorded at T = 10 K. At higher
temperatures, the magnetic susceptibility of $Sm_2Ti_2O_7$ shows a broad
maximum at T = 140 K while that of $Sm_2Zr_2O_7$ changes monotonically. Whereas
$Sm_2Ti_2O_7$ is a promising candidate for investigating spin-fluctuations on a
frustrated lattice as indicated by our data, the properties of $Sm_2Zr_2O_7$
seem to conform to a conventional scenario where geometrical frustration of the
spin exclude their long-range ordering.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:34:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Singh",
"Surjeet",
""
],
[
"Saha",
"Surajit",
""
],
[
"Dhar",
"S. K.",
""
],
[
"Suryanarayanan",
"R.",
""
],
[
"Sood",
"A. K.",
""
],
[
"Revcolevschi",
"A.",
""
]
] | [
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] |
712.3062 | C\'assius de Melo | R. R. Cuzinatto, C. A. M. de Melo, L. G. Medeiros and P. J. Pompeia | Cosmic acceleration from second order gauge gravity | RevTex4 15 pages, 1 figure. Accepted for publication in Astrophysics
& Space Science | Astrophys.Space Sci.332:201-208,2011 | 10.1007/s10509-010-0483-y | IFT-P.020/2007 | gr-qc astro-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We construct a phenomenological theory of gravitation based on a second order
gauge formulation for the Lorentz group. The model presents a long-range
modification for the gravitational field leading to a cosmological model
provided with an accelerated expansion at recent times. We estimate the model
parameters using observational data and verify that our estimative for the age
of the Universe is of the same magnitude than the one predicted by the standard
model. The transition from the decelerated expansion regime to the accelerated
one occurs recently (at $\sim9.3\;Gyr$).
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 21:49:40 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Aug 2008 23:05:34 GMT"
},
{
"version": "v3",
"created": "Tue, 7 Sep 2010 22:20:26 GMT"
}
] | 2011-02-09T00:00:00 | [
[
"Cuzinatto",
"R. R.",
""
],
[
"de Melo",
"C. A. M.",
""
],
[
"Medeiros",
"L. G.",
""
],
[
"Pompeia",
"P. J.",
""
]
] | [
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712.3063 | Jeffrey Kubo | Jeffrey M. Kubo, Ian P. Dell'Antonio | A method to search for strong galaxy-galaxy lenses in optical imaging
surveys | Accepted for publication in MNRAS, 12 pages | Mon.Not.Roy.Astron.Soc.385:918,2008 | 10.1111/j.1365-2966.2008.12880.x | FERMILAB-PUB-07-662-A-CD | astro-ph | null | We present a semi-automated method to search for strong galaxy-galaxy lenses
in optical imaging surveys. Our search technique constrains the shape of
strongly lensed galaxies (or arcs) in a multi-parameter space, which includes
the third order (octopole) moments of objects. This method is applied to the
Deep Lens Survey (DLS), a deep ground based weak lensing survey imaging to
$R\sim26$. The parameter space of arcs in the DLS is simulated using real
galaxies extracted from deep HST fields in order to more accurately reproduce
the properties of arcs. Arcs are detected in the DLS using a pixel thresholding
method and candidate arcs are selected within this multi-parameter space.
Examples of strong galaxy-galaxy lens candidates discovered in the DLS F2 field
(4 square degrees) are presented.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 22:17:31 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 21:15:53 GMT"
}
] | 2008-11-07T00:00:00 | [
[
"Kubo",
"Jeffrey M.",
""
],
[
"Dell'Antonio",
"Ian P.",
""
]
] | [
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] |
712.3064 | Lance Dixon | Lance J. Dixon | Hard QCD Processes at Colliders | 14 pages, 17 figures, talk presented at Lepton-Photon 2007; v2,
references updated | null | null | SLAC-PUB-13054 | hep-ph hep-ex | null | Recent developments in the study of hard QCD processes at colliders are
reviewed, in the context of the imminent startup of the LHC.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 22:01:34 GMT"
},
{
"version": "v2",
"created": "Mon, 24 Dec 2007 18:01:14 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Dixon",
"Lance J.",
""
]
] | [
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] |
712.3065 | Wayne Witzel | W. M. Witzel and S. Das Sarma | Wavefunction considerations for the central spin decoherence problem in
a nuclear spin bath | null | Phys. Rev. B 77, 165319 (2008) | 10.1103/PhysRevB.77.165319 | null | cond-mat.mes-hall | null | Decoherence of a localized electron spin in a solid state material (the
``central spin'' problem) at low temperature is believed to be dominated by
interactions with nuclear spins in the lattice. This decoherence is partially
suppressed through the application of a large magnetic field that splits the
energy levels of the electron spin and prevents depolarization. However,
dephasing decoherence resulting from a dynamical nuclear spin bath cannot be
removed in this way. Fluctuations of the nuclear field lead to uncertainty of
the electron's precessional frequency in a process known as spectral diffusion.
This article considers the effect of the electron's wavefunction shape upon
spectral diffusion and provides wavefunction dependent decoherence time
formulas for free induction decay as well as spin echoes and concatenated
dynamical decoupling schemes for enhancing coherence. We also discuss dephasing
of a qubit encoded in singlet-triplet states of a double quantum dot. A central
theoretical result of this work is the development of a continuum approximation
for the spectral diffusion problem which we have applied to GaAs and InAs
materials specifically.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 00:24:20 GMT"
},
{
"version": "v2",
"created": "Fri, 11 Apr 2008 20:13:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Witzel",
"W. M.",
""
],
[
"Sarma",
"S. Das",
""
]
] | [
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] |
712.3066 | Michal Bajdich | Michal Bajdich | Generalized Pairing Wave Functions and Nodal Properties for Electronic
Structure Quantum Monte Carlo | Phd Thesis under advisory of Prof. Lubos Mitas, NCSU, Raleigh, 2007 | null | null | null | cond-mat.other | null | The quantum Monte Carlo (QMC) is one of the most promising many-body
electronic structure approaches. It employs stochastic techniques for solving
the stationary Schr\" odinger equation and for evaluation of expectation
values. The key advantage of QMC is its capability to use the explicitly
correlated wave functions, which allow the study of many-body effects beyond
the reach of mean-field methods. The most important limit on QMC accuracy is
the fixed-node approximation, which comes from necessity to circumvent the
fermion sign problem. The size of resulting fixed-node errors depends on the
quality of the nodes (the subset of position space where the wave function
vanishes) of a used wave function. In this dissertation, we analyze the nodal
properties of the existing fermionic wave functions and offer new types of
variational wave functions with improved nodal structure.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 22:12:38 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Bajdich",
"Michal",
""
]
] | [
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-0.0286993161,
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-0.0663070604,
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] |
712.3067 | Waldyr A. Rodrigues Jr. | Waldyr A. Rodrigues Jr | Differential Forms on Riemannian (Lorentzian) and Riemann-Cartan
Structures and Some Applications to Physics | Some few important misprints appearing in the version of the paper
published in AFLB (in a special issue dedicated to torsion) are corrected | Ann. Fond. L. de Broglie 32 (4), 425-478 (2007) | null | null | math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper after recalling some essential tools concerning the theory of
differential forms in the Cartan, Hodge and Clifford bundles over a Riemannian
or Riemann-Cartan space or a Lorentzian or Riemann-Cartan spacetime we solve
with details several exercises involving different grades of difficult. One of
the problems is to show that a recent formula appearing in the literature for
the exterior covariant derivative of the Hodge dual of the torsion 2-forms is
simply wrong. We believe that the paper will be useful for students (and
eventually for some experts) on applications of differential geometry on
physical problems. A detailed account of the issues discussed in the paper
appears in the table of contents.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:32:42 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Jan 2008 10:08:09 GMT"
},
{
"version": "v3",
"created": "Mon, 7 Jan 2008 16:04:03 GMT"
},
{
"version": "v4",
"created": "Mon, 12 May 2008 14:36:40 GMT"
},
{
"version": "v5",
"created": "Tue, 20 May 2008 12:28:27 GMT"
},
{
"version": "v6",
"created": "Thu, 4 Dec 2008 19:14:04 GMT"
}
] | 2008-12-04T00:00:00 | [
[
"Rodrigues",
"Waldyr A.",
"Jr"
]
] | [
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] |
712.3068 | Dipanjan Basu | D. Basu, M. J. Gilbert, L. F. Register, A. H. MacDonald and S. K.
Banerjee | Effect of Edge Roughness on Electronic Transport in Graphene Nanoribbon
Channel Metal Oxide Semiconductor Field-Effect Transistors | 8 pages, 5 figures | Applied Physics Letters 92, 042114 (2008) | 10.1063/1.2839330 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | Results of quantum mechanical simulations of the influence of edge disorder
on transport in graphene nanoribbon metal oxide semiconductor field-effect
transistors (MOSFETs) are reported. The addition of edge disorder significantly
reduces ON-state currents and increases OFF-state currents, and introduces wide
variability across devices. These effects decrease as ribbon widths increase
and as edges become smoother. However the bandgap decreases with increasing
width, thereby increasing the band-to-band tunneling mediated subthreshold
leakage current even with perfect nanoribbons. These results suggest that
without atomically precise edge control during fabrication, MOSFET performance
gains through use of graphene will be difficult to achieve.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 22:22:38 GMT"
}
] | 2008-04-10T00:00:00 | [
[
"Basu",
"D.",
""
],
[
"Gilbert",
"M. J.",
""
],
[
"Register",
"L. F.",
""
],
[
"MacDonald",
"A. H.",
""
],
[
"Banerjee",
"S. K.",
""
]
] | [
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] |
712.3069 | John Franks | John Franks and Michael Handel | Complete semi-conjugacies for psuedo-Anosov homeomorphisms | null | null | null | null | math.DS math.GT | null | Suppose $S$ is a surface of genus $\ge 2 $, $f: S \to S$ is a surface
homeomorphism isotopic to a pseudo-Anosov map $\alpha$ and suppose $\ti S$ is
the universal cover of $S$ and $F$ and $A$ are lifts of $f$ and $\alpha$
respectively. We show there is a semiconjugacy $\Theta : \ti S \to \bar \L^s
\times \bar \L^u$ from $F$ to $\bar A$, where $\bar \L^s$ ($\bar \L^u$) is the
completion of the $R$-tree of leaves of the stable (resp. unstable) foliation
for $A$ and $\bar A$ is the map induced by $A$.
We also generalize a result of Markovich and show that for any $g \in
Homeo(S)$ which commutes with $f$ and has identity lift $G : \ti S \to \ti S$
and for any $(c,w)$ in the image of $\Theta$ each component of
$\Theta^{-1}(c,w)$ is $G$-invariant.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:02:10 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Dec 2007 14:31:24 GMT"
}
] | 2007-12-26T00:00:00 | [
[
"Franks",
"John",
""
],
[
"Handel",
"Michael",
""
]
] | [
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] |
712.307 | Hans-Thomas Janka | H.-Th. Janka, A. Marek, B. Mueller, and L. Scheck (MPI for
Astrophysics, Garching) | Supernova explosions and the birth of neutron stars | 10 pages, 8 figures, 19 ps files; to be published in Proc. of Conf.
"40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August
12-17, 2007, McGill Univ., Montreal, Canada; high-resolution images can be
obtained upon request; incorrect panel in fig.8 replaced | AIP Conf.Proc.983:369-378,2008 | 10.1063/1.2900257 | null | astro-ph | null | We report here on recent progress in understanding the birth conditions of
neutron stars and the way how supernovae explode. More sophisticated numerical
models have led to the discovery of new phenomena in the supernova core, for
example a generic hydrodynamic instability of the stagnant supernova shock
against low-mode nonradial deformation and the excitation of gravity-wave
activity in the surface and core of the nascent neutron star. Both can have
supportive or decisive influence on the inauguration of the explosion, the
former by improving the conditions for energy deposition by neutrino heating in
the postshock gas, the latter by supplying the developing blast with a flux of
acoustic power that adds to the energy transfer by neutrinos. While recent
two-dimensional models suggest that the neutrino-driven mechanism may be viable
for stars from about 8 solar masses to at least 15 solar masses, acoustic
energy input has been advocated as an alternative if neutrino heating fails.
Magnetohydrodynamic effects constitute another way to trigger explosions in
connection with the collapse of sufficiently rapidly rotating stellar cores,
perhaps linked to the birth of magnetars. The global explosion asymmetries seen
in the recent simulations offer an explanation of even the highest measured
kick velocities of young neutron stars.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:14:15 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 08:05:31 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Janka",
"H. -Th.",
"",
"MPI for\n Astrophysics, Garching"
],
[
"Marek",
"A.",
"",
"MPI for\n Astrophysics, Garching"
],
[
"Mueller",
"B.",
"",
"MPI for\n Astrophysics, Garching"
],
[
"Scheck",
"L.",
"",
"MPI for\n Astrophysics, Garching"
]
] | [
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] |
712.3071 | Yujin Guo | Nassif Ghoussoub and Yujin Guo | Estimates for the quenching time of a parabolic equation modeling
electrostatic MEMS | 17 pages, 5 figures. Updated version -- if any -- of this paper can
be downloaded from the website: http://www.birs.ca/~nassif | null | null | null | math.AP | null | The singular parabolic problem $u_t=\Delta u -\frac{\lambda f(x)}{(1+u)^2}$
on a bounded domain $\Omega$ of $R^N$ with Dirichlet boundary conditions,
models the dynamic deflection of an elastic membrane in a simple electrostatic
Micro-Electromechanical System (MEMS) device. In this paper, we analyze and
estimate the quenching time of the elastic membrane in terms of the applied
voltage --represented here by $\lambda$. As a byproduct, we prove that for
sufficiently large $\lambda$, finite-time quenching must occur near the maximum
point of the varying dielectric permittivity profile $f(x)$.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:06:05 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Ghoussoub",
"Nassif",
""
],
[
"Guo",
"Yujin",
""
]
] | [
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] |
712.3072 | Manolis Plionis Dr. | M. Plionis, M. Rovilos, S. Basilakos, I. Georgantopoulos, F. Bauer | Luminosity Dependent X-ray AGN Clustering ? | ApJ Letters accepted | null | 10.1086/528845 | null | astro-ph | null | We have analysed the angular clustering of X-ray selected active galactic
nuclei (AGN) in different flux-limited sub-samples of the Chandra Deep Field
North (CDF-N) and South (CDF-S) surveys. We find a strong dependence of the
clustering strength on the sub-sample flux-limit, a fact which explains most of
the disparate clustering results of different XMM and Chandra surveys. Using
Limber's equation, we find that the inverted CDF-N and CDF-S spatial clustering
lengths are consistent with direct spatial clustering measures found in the
literature, while at higher flux-limits the clustering length increases
considerably; for example, at $fx,limit ~ 10^{-15} erg/s/cm^{-2} we obtain r_0~
17 +- 5 and 18+- 3 h^{-1} Mpc, for the CDF-N and CDF-S, respectively. We show
that the observed flux-limit clustering trend hints towards an X-ray luminosity
dependent clustering of X-ray selected, $z\sim 1$, AGNs.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:17:06 GMT"
}
] | 2017-03-22T00:00:00 | [
[
"Plionis",
"M.",
""
],
[
"Rovilos",
"M.",
""
],
[
"Basilakos",
"S.",
""
],
[
"Georgantopoulos",
"I.",
""
],
[
"Bauer",
"F.",
""
]
] | [
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712.3073 | Aidan Sims | Aidan Sims and Trent Yeend | C*-algebras associated to product systems of Hilbert bimodules | 24 pages. v2: material has been rearranged so that the algebra NO_X
is defined only under hypotheses which ensure that the universal
representation is injective. The substance of the results is unchanged. v3:
minor revisions; this version to appear in J. Operator Theory | null | null | null | math.OA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let (G,P) be a quasi-lattice ordered group and let X be a compactly aligned
product system over P of Hilbert bimodules. Under mild hypotheses we associate
to X a C*-algebra which we call the Cuntz-Nica-Pimsner algebra of X. Our
construction generalises a number of others: a sub-class of Fowler's
Cuntz-Pimsner algebras for product systems of Hilbert bimodules; Katsura's
formulation of Cuntz-Pimsner algebras of Hilbert bimodules; the C*-algebras of
finitely aligned higher-rank graphs; and Crisp and Laca's boundary quotients of
Toeplitz algebras. We show that for a large class of product systems X, the
universal representation of X in its Cuntz-Nica-Pimsner algebra is isometric.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:20:16 GMT"
},
{
"version": "v2",
"created": "Wed, 13 Aug 2008 11:13:40 GMT"
},
{
"version": "v3",
"created": "Wed, 7 Jan 2009 23:24:12 GMT"
}
] | 2009-01-08T00:00:00 | [
[
"Sims",
"Aidan",
""
],
[
"Yeend",
"Trent",
""
]
] | [
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] |
712.3074 | Anosh Joseph | Simon Catterall, Anosh Joseph | Lattice Actions for Yang-Mills Quantum Mechanics with Exact
Supersymmetry | 24 pages, minor corrections, published version | Phys.Rev.D77:094504,2008 | 10.1103/PhysRevD.77.094504 | SU-4252-871 | hep-lat hep-th | null | We derive lattice actions for Yang-Mills quantum mechanics for models with
$\cQ=4, 8$ and 16 supercharges which possess an exact supersymmetry at non-zero
lattice spacing. These are obtained by dimensional reduction of twisted
versions of the corresponding super Yang-Mills theories in $D=2, 3$ and 4
dimensions.
| [
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"created": "Tue, 18 Dec 2007 23:28:40 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 20:37:57 GMT"
},
{
"version": "v3",
"created": "Thu, 15 May 2008 16:24:58 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Catterall",
"Simon",
""
],
[
"Joseph",
"Anosh",
""
]
] | [
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712.3075 | Jean-Philippe Lenain | J.-P. Lenain, C. Boisson, H. Sol | SSC scenario for TeV emission from non-blazar AGNs | 4 pages, 5 figures, HEPRO Workshop Proceedings, revised manuscript | Int.J.Mod.Phys.D17:1577-1584,2008 | 10.1142/S0218271808013170 | null | astro-ph | null | M87 is the first extragalactic source detected in the TeV gamma-ray domain
that is not a blazar, its large scale jet not being aligned to the line of
sight. We present here a multi-blob synchrotron self-Compton model accounting
explicitly for large viewing angles and moderate Lorentz factors as inferred
from magnetohydrodynamic simulations of jet formation, motivated by the
detection of M87 at very high energies (VHE; E > 100GeV). Predictions are
presented for the very high-energy emission of active galactic nuclei with
extended optical or X-ray jet, which could be misaligned blazars but still show
some moderate beaming. We include predictions for 3C273, Cen A and PKS 0521-36.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:37:46 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Mar 2008 14:39:49 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Lenain",
"J. -P.",
""
],
[
"Boisson",
"C.",
""
],
[
"Sol",
"H.",
""
]
] | [
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] |
712.3076 | Guido Boffetta | G. Boffetta, A. Celani, D. Dezzani, A. Seminara | How winding is the coast of Britain ? Conformal invariance of rocky
shorelines | null | null | 10.1029/2007GL033093 | null | nlin.CD | null | We show that rocky shorelines with fractal dimension 4/3 are conformally
invariant curves by measuring the statistics of their winding angles from
global high-resolution data. Such coastlines are thus statistically equivalent
to the outer boundary of the random walk and of percolation clusters. A simple
model of coastal erosion gives an explanation for these results. Conformal
invariance allows also to predict the highly intermittent spatial distribution
of the flux of pollutant diffusing ashore.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:37:47 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Boffetta",
"G.",
""
],
[
"Celani",
"A.",
""
],
[
"Dezzani",
"D.",
""
],
[
"Seminara",
"A.",
""
]
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-0.0964774787,
-0.0258677043,
-0.0424194634,
0.0185680855,
-0.0523734875,
0.0328738056,
-0.0045909751,
-0.0668706298,
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0.0122574894,
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0.0100369761
] |
712.3077 | Young-Heon Kim | Young-Heon Kim and Robert J. McCann | Continuity, curvature, and the general covariance of optimal
transportation | 43 pages, 1 figure | null | null | null | math.DG math.AP | null | Let M and \bar M be n-dimensional manifolds equipped with suitable Borel
probability measures \rho and \bar\rho. Ma, Trudinger & Wang gave sufficient
conditions on a transportation cost c \in C^4(M \times \bar M) to guarantee
smoothness of the optimal map pushing \rho forward to \bar\rho; the necessity
of these conditions was deduced by Loeper. The present manuscript shows the
form of these conditions to be largely dictated by the covariance of the
question; it expresses them via non-negativity of the sectional curvature of
certain null-planes in a novel but natural pseudo-Riemannian geometry which the
cost c induces on the product space M \times \bar M.
H\"older continuity of optimal maps was established for rougher mass
distributions by Loeper, still relying on a key result of Trudinger & Wang
which required certain structure on the domains and the cost. We go on to
develop this theory for mass distributions on differentiable manifolds --
recovering Loeper's Riemannian examples such as the round sphere as particular
cases -- give a direct proof of the key result mentioned above, and revise
Loeper's H\"older continuity argument to make it logically independent of all
earlier works, while extending it to less restricted geometries and cost
functions even for subdomains M and \bar M of R^n. We also give new examples of
geometries satisfying the hypotheses -- obtained using submersions and tensor
products -- and some connections to spacelike Lagrangian submanifolds in
symplectic geometry.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 00:33:49 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Kim",
"Young-Heon",
""
],
[
"McCann",
"Robert J.",
""
]
] | [
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712.3078 | Guido Boffetta | S. Berti, A. Bistagnino, G. Boffetta, A. Celani and S. Musacchio | Two-dimensional elastic turbulence | null | null | 10.1103/PhysRevE.77.055306 | null | nlin.CD physics.flu-dyn | null | We investigate the effect of polymer additives on a two-dimensional
Kolmogorov flow at very low Reynolds numbers by direct numerical simulations of
the Oldroyd-B viscoelastic model. We find that above the elastic instability
threshold the flow develops the elastic turbulence regime recently observed in
experiments. We observe that both the turbulent drag and the Lyapunov exponent
increase with Weissenberg, indicating the presence of a disordered,
turbulent-like mixing flow. The energy spectrum develops a power-law scaling
range with an exponent close to the experimental and theoretical expectations.
| [
{
"version": "v1",
"created": "Tue, 18 Dec 2007 23:42:32 GMT"
}
] | 2010-06-23T00:00:00 | [
[
"Berti",
"S.",
""
],
[
"Bistagnino",
"A.",
""
],
[
"Boffetta",
"G.",
""
],
[
"Celani",
"A.",
""
],
[
"Musacchio",
"S.",
""
]
] | [
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