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711.4508 | Hiroshi Ishikawa | Hiroshi Ishikawa | Representation and Measure of Structural Information | Second version. Revised the Introduction and added more discussion in
the last section. The technical content is mostly unchanged. 51 pages, 4
figures | null | null | null | cs.CC cs.CV cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce a uniform representation of general objects that captures the
regularities with respect to their structure. It allows a representation of a
general class of objects including geometric patterns and images in a sparse,
modular, hierarchical, and recursive manner. The representation can exploit any
computable regularity in objects to compactly describe them, while also being
capable of representing random objects as raw data. A set of rules uniformly
dictates the interpretation of the representation into raw signal, which makes
it possible to ask what pattern a given raw signal contains. Also, it allows
simple separation of the information that we wish to ignore from that which we
measure, by using a set of maps to delineate the a priori parts of the objects,
leaving only the information in the structure.
Using the representation, we introduce a measure of information in general
objects relative to structures defined by the set of maps. We point out that
the common prescription of encoding objects by strings to use Kolmogorov
complexity is meaningless when, as often is the case, the encoding is not
specified in any way other than that it exists. Noting this, we define the
measure directly in terms of the structures of the spaces in which the objects
reside. As a result, the measure is defined relative to a set of maps that
characterize the structures. It turns out that the measure is equivalent to
Kolmogorov complexity when it is defined relative to the maps characterizing
the structure of natural numbers. Thus, the formulation gives the larger class
of objects a meaningful measure of information that generalizes Kolmogorov
complexity.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:41:30 GMT"
},
{
"version": "v2",
"created": "Thu, 12 Jun 2008 03:37:52 GMT"
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] | 2008-06-12T00:00:00 | [
[
"Ishikawa",
"Hiroshi",
""
]
] | [
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711.4509 | Rikard Olofsson | Rikard Olofsson | Large supremum norms and small Shannon entropy for Hecke eigenfunctions
of quantized cat maps | 21 pages and 4 figures | null | 10.1007/s00220-008-0627-x | null | math.NT math-ph math.MP | null | This paper concerns the behavior of eigenfunctions of quantized cat maps and
in particular their supremum norm. We observe that for composite integer values
of N, the inverse of Planck's constant, some of the desymmetrized
eigenfunctions have very small support and hence very large supremum norm. We
also prove an entropy estimate and show that our functions satisfy equality in
this estimate. In the case when N is a prime power with even exponent we
calculate the supremum norm for a large proportion of all desymmetrized
eigenfunctions and we find that for a given N there is essentially at most four
different values these assume.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:18:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Olofsson",
"Rikard",
""
]
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711.451 | Zden\v{e}k Mikul\'a\v{s}ek | Z. Mikulasek | The benefits of the orthogonal LSM models | 5 pages, 2 figures, submitted to Odessa Astronomical Publications,
vol. 20, 2007 | null | null | null | astro-ph | null | In the last few decades both the volume of high-quality observing data on
variable stars and common access to them have boomed; however the standard used
methods of data processing and interpretation have lagged behind this progress.
The most popular method of data treatment remains for many decades Linear
Regression (LR) based on the principles of Least Squares Method (LSM) or
linearized LSM. Unfortunately, we have to state that the method of linear
regression is not as a rule used accordingly namely in the evaluation of
uncertainties of the LR parameters and estimates of the uncertainty of the LR
predictions.
We present the matrix version of basic relations of LR and the true estimate
of the uncertainty of the LR predictions. We define properties of the
orthogonal LR models and show how to transform general LR models into
orthogonal ones. We give relations for orthogonal models for common polynomial
series.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:51:25 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Mikulasek",
"Z.",
""
]
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] |
711.4511 | Dmitriy Kulikov | D. A. Kulikov and R. S. Tutik | A new approach to the relativistic treatment of the fermion-boson
system, based on the extension of the SL(2,C) group | v3: revised version (to appear in Mod. Phys. Lett. A) | Mod.Phys.Lett.A23:1829-1840,2008 | 10.1142/S0217732308027205 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A new technique for constructing the relativistic wave equation for the
two-body system composed of the spin-1/2 and spin-0 particles is proposed. The
method is based on the extension of the SL(2,C) group to the Sp(4,C) one. The
obtained equation includes the interaction potentials, having both the
Lorentz-vector and Lorentz-tensor structure, exactly describes the relativistic
kinematics and possesses the correct one-particle limits. The comparison with
results of other approaches to this problem is discussed.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:36:24 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 12:21:17 GMT"
},
{
"version": "v3",
"created": "Tue, 15 Jul 2008 10:00:12 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kulikov",
"D. A.",
""
],
[
"Tutik",
"R. S.",
""
]
] | [
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711.4512 | Marco Morelli | M.J. Morelli, R.J. Allen, S. Tanase-Nicola, P.R. ten Wolde | Eliminating fast reactions in stochastic simulations of biochemical
networks: a bistable genetic switch | 46 pages, 5 figures | null | 10.1063/1.2821957 | null | q-bio.QM q-bio.MN | null | In many stochastic simulations of biochemical reaction networks, it is
desirable to ``coarse-grain'' the reaction set, removing fast reactions while
retaining the correct system dynamics. Various coarse-graining methods have
been proposed, but it remains unclear which methods are reliable and which
reactions can safely be eliminated. We address these issues for a model gene
regulatory network that is particularly sensitive to dynamical fluctuations: a
bistable genetic switch. We remove protein-DNA and/or protein-protein
association-dissociation reactions from the reaction set, using various
coarse-graining strategies. We determine the effects on the steady-state
probability distribution function and on the rate of fluctuation-driven switch
flipping transitions. We find that protein-protein interactions may be safely
eliminated from the reaction set, but protein-DNA interactions may not. We also
find that it is important to use the chemical master equation rather than
macroscopic rate equations to compute effective propensity functions for the
coarse-grained reactions.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:36:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Morelli",
"M. J.",
""
],
[
"Allen",
"R. J.",
""
],
[
"Tanase-Nicola",
"S.",
""
],
[
"Wolde",
"P. R. ten",
""
]
] | [
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] |
711.4513 | Helmut Friedrich | Helmut Friedrich | Conformal classes of asymptotically flat, static vacuum data | 23 pages | Class.Quant.Grav.25:065012,2008 | 10.1088/0264-9381/25/6/065012 | null | gr-qc | null | We show that time-reflection symmetric, asymptotically flat, static vacuum
data which admit a non-trivial conformal rescaling which leads again to such
data must be axi-symmetric and admit a conformal Killing field. Moreover, it is
shown that there exists a 3-parameter family of such data.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:40:42 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 14:30:44 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Friedrich",
"Helmut",
""
]
] | [
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] |
711.4514 | Pierre Etore | Pierre Etore (CERMICS), Benjamin Jourdain (CERMICS) | Adaptive optimal allocation in stratified sampling methods | null | null | null | null | stat.ME stat.CO | null | In this paper, we propose a stratified sampling algorithm in which the random
drawings made in the strata to compute the expectation of interest are also
used to adaptively modify the proportion of further drawings in each stratum.
These proportions converge to the optimal allocation in terms of variance
reduction. And our stratified estimator is asymptotically normal with
asymptotic variance equal to the minimal one. Numerical experiments confirm the
efficiency of our algorithm.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:52:08 GMT"
},
{
"version": "v2",
"created": "Fri, 30 Nov 2007 12:59:04 GMT"
}
] | 2007-12-04T00:00:00 | [
[
"Etore",
"Pierre",
"",
"CERMICS"
],
[
"Jourdain",
"Benjamin",
"",
"CERMICS"
]
] | [
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] |
711.4515 | Mario Silveirinha G. | Mario G. Silveirinha, Carlos A. Fernandes, Jorge R. Costa | Additional Boundary Condition for a Wire Medium Connected to a Metallic
Surface | 26 pages; under review | null | 10.1088/1367-2630/10/5/053011 | null | cond-mat.mtrl-sci | null | In this work, we demonstrate that the interaction of electromagnetic waves
with a microstructured material formed by metallic wires connected to a
metallic surface can be described using homogenization methods provided an
additional boundary condition is considered. The additional boundary condition
is derived by taking into account the specific microstructure of the wire
medium. To illustrate the application of the result, we characterize a
substrate formed by an array of tilted metallic wires connected to a ground
plane, demonstrating that in such configuration the wire medium behaves
essentially as a material with extreme optical anisotropy and that in some
circumstances the substrate can be seen as an impedance surface.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 14:55:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Silveirinha",
"Mario G.",
""
],
[
"Fernandes",
"Carlos A.",
""
],
[
"Costa",
"Jorge R.",
""
]
] | [
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711.4516 | Jocelyne Troccaz | Philippe Merloz (CHU-Grenoble ortho-traumato), Jocelyne Troccaz
(TIMC), Herv\'e Vouaillat (CHU-Grenoble ortho-traumato), Christian Vasile
(CHU-Grenoble ortho-traumato), J\'er\^ome Tonetti (CHU-Grenoble
ortho-traumato), Ahmad Eid (CHU-Grenoble ortho-traumato), St\'ephane Plaweski
(CHU-Grenoble ortho-traumato) | Fluoroscopy-based navigation system in spine surgery | null | Proceedings of the Institution of Mechanical Engineers. Part H,
Journal of Engineering in Medicine 221, 7 (2007) 813-20 | null | null | cs.OH | null | The variability in width, height, and spatial orientation of a spinal pedicle
makes pedicle screw insertion a delicate operation. The aim of the current
paper is to describe a computer-assisted surgical navigation system based on
fluoroscopic X-ray image calibration and three-dimensional optical localizers
in order to reduce radiation exposure while increasing accuracy and reliability
of the surgical procedure for pedicle screw insertion. Instrumentation using
transpedicular screw fixation was performed: in a first group, a conventional
surgical procedure was carried out with 26 patients (138 screws); in a second
group, a navigated surgical procedure (virtual fluoroscopy) was performed with
26 patients (140 screws). Evaluation of screw placement in every case was done
by using plain X-rays and post-operative computer tomography scan. A 5 per cent
cortex penetration (7 of 140 pedicle screws) occurred for the computer-assisted
group. A 13 per cent penetration (18 of 138 pedicle screws) occurred for the
non computer-assisted group. The radiation running time for each vertebra level
(two screws) reached 3.5 s on average in the computer-assisted group and 11.5 s
on average in the non computer-assisted group. The operative time for two
screws on the same vertebra level reaches 10 min on average in the non
computer-assisted group and 11.9 min on average in the computer-assisted group.
The fluoroscopy-based (two-dimensional) navigation system for pedicle screw
insertion is a safe and reliable procedure for surgery in the lower thoracic
and lumbar spine.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:19:15 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Merloz",
"Philippe",
"",
"CHU-Grenoble ortho-traumato"
],
[
"Troccaz",
"Jocelyne",
"",
"TIMC"
],
[
"Vouaillat",
"Hervé",
"",
"CHU-Grenoble ortho-traumato"
],
[
"Vasile",
"Christian",
"",
"CHU-Grenoble ortho-traumato"
],
[
"Tonetti",
"Jérôme",
"",
"CHU-Grenoble\n ortho-traumato"
],
[
"Eid",
"Ahmad",
"",
"CHU-Grenoble ortho-traumato"
],
[
"Plaweski",
"Stéphane",
"",
"CHU-Grenoble ortho-traumato"
]
] | [
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] |
711.4517 | Werner Rodejohann | Sandip Pakvasa, Werner Rodejohann, Thomas J. Weiler | Flavor Ratios of Astrophysical Neutrinos: Implications for Precision
Measurements | 32 pages, 15 figures. Minor changes, matches version in JHEP | JHEP0802:005,2008 | 10.1088/1126-6708/2008/02/005 | null | hep-ph astro-ph hep-ex | null | We discuss flavor-mixing probabilities and flavor ratios of high energy
astrophysical neutrinos. In the first part of this paper, we expand the
neutrino flavor-fluxes in terms of the small parameters U_{e3} and pi/4 -
theta_{23}, and show that there are universal first and second order
corrections. The second order term can exceed the first order term, and so
should be included in any analytic study. We also investigate the probabilities
and ratios after a further expansion around the tribimaximal value of sin^2
theta_{12} = 1/3. In the second part of the paper, we discuss implications of
deviations of initial flavor ratios from the usually assumed, idealized flavor
compositions for pion, muon-damped, and neutron beam sources, viz., (1 : 2 :
0), (0 : 1 : 0), and (1 : 0 : 0), respectively. We show that even small
deviations have significant consequences for the observed flavor ratios at
Earth. If initial flavor deviations are not taken into account in analyses,
then false inferences for the values in the PMNS matrix elements (angles and
phase) may result.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:29:22 GMT"
},
{
"version": "v2",
"created": "Fri, 8 Feb 2008 16:02:37 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Pakvasa",
"Sandip",
""
],
[
"Rodejohann",
"Werner",
""
],
[
"Weiler",
"Thomas J.",
""
]
] | [
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] |
711.4518 | Paolo Privitera | M. Ave, et al. (AIRFLY Collaboration) | Energy Dependence of Air Fluorescence Yield measured by AIRFLY | presented at the 5th Fluorescence Workshop, El Escorial - Madrid,
Spain, 16 - 20 September 2007, to appear in Nuclear Instruments and Methods A | null | null | null | astro-ph | null | In the fluorescence detection of ultra high energy (> 10**18 eV) cosmic rays,
the number of emitted fluorescence photons is assumed to be proportional to the
energy deposited in air by shower particles. We have performed measurements of
the fluorescence yield in atmospheric gases excited by electrons over energies
ranging from keV to hundreds of MeV in several accelerators. We found that
within the measured energy ranges the proportionality holds at the level of few
%.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:29:45 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Ave",
"M.",
""
]
] | [
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711.4519 | Alessio Figalli | Albert Fathi, Alessio Figalli | Optimal transportation on non-compact manifolds | null | null | null | null | math.OC math.DG | null | In this work, we show how to obtain for non-compact manifolds the results
that have already been done for Monge Transport Problem for costs coming from
Tonelli Lagrangians on compact manifolds. In particular, the already known
results for a cost of the type $d^r,r>1$, where $d$ is the Riemannian distance
of a complete Riemannian manifold, hold without any curvature restriction.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:31:43 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Fathi",
"Albert",
""
],
[
"Figalli",
"Alessio",
""
]
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] |
711.452 | Alessandro Fabbri | Roberto Balbinot, Alessandro Fabbri, Serena Fagnocchi, Alessio Recati
and Iacopo Carusotto | Non-local density correlations as signal of Hawking radiation in BEC
acoustic black holes | Strongly revised version. 5 pages, 3 eps figures | Phys.Rev.A78:021603,2008 | 10.1103/PhysRevA.78.021603 | null | cond-mat.other gr-qc hep-th | null | We have used the analogy between gravitational systems and non-homogeneous
fluid flows to calculate the density-density correlation function of an atomic
Bose-Einstein condensate in the presence of an acoustic black hole. The
emission of correlated pairs of phonons by Hawking-like process results into a
peculiar long-range density correlation. Quantitative estimations of the effect
are provided for realistic experimental configurations.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:35:41 GMT"
},
{
"version": "v2",
"created": "Mon, 12 May 2008 11:57:05 GMT"
}
] | 2009-07-20T00:00:00 | [
[
"Balbinot",
"Roberto",
""
],
[
"Fabbri",
"Alessandro",
""
],
[
"Fagnocchi",
"Serena",
""
],
[
"Recati",
"Alessio",
""
],
[
"Carusotto",
"Iacopo",
""
]
] | [
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] |
711.4521 | Paul M. Bellan | P. M. Bellan | Consideration of the relationship between Kepler and cyclotron dynamics
leading to prediction of a non-MHD gravity-driven Hamiltonian dynamo | 14 pages, 1 figure | Physics of Plasmas Vol. 14, Art. No. 122901 (2007) | 10.1063/1.2815791 | null | astro-ph | null | Conservation of canonical angular momentum shows that charged particles are
typically constrained to stay within a poloidal Larmor radius of a poloidal
magnetic flux surface. However, more detailed consideration shows that
particles with a critical charge to mass ratio can have zero canonical angular
momentum and so be both immune from centrifugal force and not constrained to
stay in the vicinity of a specific flux surface. Suitably charged dust grains
can have zero canonical angular momentum and in the presence of a gravitational
field will spiral inwards across poloidal magnetic surfaces toward the central
object and accumulate. This accumulation results in a gravitationally-driven
dynamo, i.e., a mechanism for converting gravitational potential energy into a
battery-like electric power source.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:04:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bellan",
"P. M.",
""
]
] | [
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] |
711.4522 | Harald W. Griesshammer | Harald W. Griesshammer (George Washington U.) | Estimating Consequences of 3-Body Forces | 3 pages LaTeX2e, including 1 figure as .eps file embedded with
includegraphicx. Uses FBSart (included). Contribution to the 20th European
Conference on Few-Body Problems in Physics EFB20, Pisa (Italy), 10th -- 14th
September 2007. To be published in Few-Body Systems | Few Body Syst.44:137-140,2008 | 10.1007/s00601-008-0275-x | null | nucl-th | null | Classifying the strengthes of three-body forces 3BFs with the condition that
observables must be cut-off independent, i.e. renormalised at each order, leads
to surprising results with relevance for example for thermal neutron capture on
the deuteron. Details and a better bibliography in Ref. [1].
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:51:42 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Griesshammer",
"Harald W.",
"",
"George Washington U."
]
] | [
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] |
711.4523 | Jocelyne Troccaz | Thomas Martinelli (CHU-Grenoble radio), Jean-Luc Bosson (TIMC,
CHU-Grenoble CIC), Luc Bressollette, Franck Pelissier, Eric Boidard (TIMC),
Jocelyne Troccaz (TIMC), Philippe Cinquin (TIMC) | Robot-based tele-echography: clinical evaluation of the TER system in
abdominal aortic exploration | null | Journal of ultrasound in medicine : official journal of the
American Institute of Ultrasound in Medicine 26, 11 (2007) 1611-6 | null | null | cs.OH | null | OBJECTIVE: The TER system is a robot-based tele-echography system allowing
remote ultrasound examination. The specialist moves a mock-up of the ultrasound
probe at the master site, and the robot reproduces the movements of the real
probe, which sends back ultrasound images and force feedback. This tool could
be used to perform ultrasound examinations in small health care centers or from
isolated sites. The objective of this study was to prove, under real
conditions, the feasibility and reliability of the TER system in detecting
abdominal aortic and iliac aneurysms. METHODS: Fifty-eight patients were
included in 2 centers in Brest and Grenoble, France. The remote examination was
compared with the reference standard, the bedside examination, for aorta and
iliac artery diameter measurement, detection and description of aneurysms,
detection of atheromatosis, the duration of the examination, and acceptability.
RESULTS: All aneurysms (8) were detected by both techniques as intramural
thrombosis and extension to the iliac arteries. The interobserver correlation
coefficient was 0.982 (P < .0001) for aortic diameters. The rate of concordance
between 2 operators in evaluating atheromatosis was 84% +/- 11% (95% confidence
interval). CONCLUSIONS: Our study on 58 patients suggests that the TER system
could be a reliable, acceptable, and effective robot-based system for
performing remote abdominal aortic ultrasound examinations. Research is
continuing to improve the equipment for general abdominal use.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:51:02 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Martinelli",
"Thomas",
"",
"CHU-Grenoble radio"
],
[
"Bosson",
"Jean-Luc",
"",
"TIMC,\n CHU-Grenoble CIC"
],
[
"Bressollette",
"Luc",
"",
"TIMC"
],
[
"Pelissier",
"Franck",
"",
"TIMC"
],
[
"Boidard",
"Eric",
"",
"TIMC"
],
[
"Troccaz",
"Jocelyne",
"",
"TIMC"
],
[
"Cinquin",
"Philippe",
"",
"TIMC"
]
] | [
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] |
711.4524 | Pintu Das | P. Das, M. R. Koblischka, Th. Wolf, P. Adelmann and U. Hartmann | $T_c$ Dependence of Energy Gap and Asymmetry of Coherence Peaks in
NdBa$_2$Cu$_3$O$_{7-\delta}$ | 4 pages, 1 Figure, to appear in Euro Phys. Lett | Euro Phys. Lett. 84, 47004 (2008). | 10.1209/0295-5075/84/47004 | null | cond-mat.supr-con cond-mat.str-el | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We report here the results of scanning tunneling spectroscopic experiments
performed on hole doped NdBa$_2$Cu$_3$O$_{7-\delta}$ single crystals of $T_c$
values of 76 K, 93.5 K and 95.5 K. The energy gaps are observed to be
increasing with decreasing $T_c$ values. The coherence peaks are asymmetric
with the peaks at the filled states being larger than those at the empty ones.
The asymmetry increases with decreasing $T_c$. The observed asymmetry and its
$T_c$ dependence can be explained by considering the Mott insulating nature of
the material at the undoped state.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 15:06:54 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 09:26:57 GMT"
},
{
"version": "v3",
"created": "Thu, 16 Oct 2008 20:19:35 GMT"
}
] | 2008-11-08T00:00:00 | [
[
"Das",
"P.",
""
],
[
"Koblischka",
"M. R.",
""
],
[
"Wolf",
"Th.",
""
],
[
"Adelmann",
"P.",
""
],
[
"Hartmann",
"U.",
""
]
] | [
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] |
711.4525 | Christian Huck | Christian Huck | Uniqueness in Discrete Tomography of Delone Sets with Long-Range Order | 15 pages, 2 figures; condensed and revised version | Discrete Comput. Geom. 42 (2009), 740-758 | 10.1007/s00454-009-9213-z | null | math.MG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We address the problem of determining finite subsets of Delone sets
$\varLambda\subset\R^d$ with long-range order by $X$-rays in prescribed
$\varLambda$-directions, i.e., directions parallel to non-zero interpoint
vectors of $\varLambda$. Here, an $X$-ray in direction $u$ of a finite set
gives the number of points in the set on each line parallel to $u$. For our
main result, we introduce the notion of algebraic Delone sets
$\varLambda\subset\R^2$ and derive a sufficient condition for the determination
of the convex subsets of these sets by $X$-rays in four prescribed
$\varLambda$-directions.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:06:32 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Nov 2008 15:59:17 GMT"
}
] | 2013-05-08T00:00:00 | [
[
"Huck",
"Christian",
""
]
] | [
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711.4526 | Yeong Gyun Kim | Won Sang Cho, Kiwoon Choi, Yeong Gyun Kim, Chan Beom Park | Measuring superparticle masses at hadron collider using the transverse
mass kink | Typos corrected. A few references added. Figures updated | JHEP0802:035,2008 | 10.1088/1126-6708/2008/02/035 | null | hep-ph | null | We present a detailed study of the collider observable $m_{T2}$ applied for
pair-produced superparticles decaying to visible particles and a pair of
invisible lightest supersymmetric particles (LSPs). Analytic expressions of the
maximum of $m_{T2}$ over all events ($m_{T2}^{\rm max}$) are derived. It is
noticed that if the decay product of each superparticle involves more than one
visible particles, $m_{T2}^{\rm max}$ being a function of the {\it trial} LSP
mass ${m}_\chi$ has a kink structure at ${m}_\chi=$ true LSP mass, which can be
used to determine the mother superparticle mass and the LSP mass
simultaneously. To see how well $m_{T2}^{\rm max}$ can be constructed from
collider data, a Monte-Carlo analysis of the gluino $m_{T2}$ is performed for
some superparticle spectra.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:23:33 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Dec 2007 11:33:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cho",
"Won Sang",
""
],
[
"Choi",
"Kiwoon",
""
],
[
"Kim",
"Yeong Gyun",
""
],
[
"Park",
"Chan Beom",
""
]
] | [
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] |
711.4527 | Alexandre Akimenko | A. I. Akimenko and V. A. Gudimenko | Evidence of a s-Wave Pairing in Heavily Zn-doped $YBa_2Cu_3O_{7-\delta}$
from Andreev Reflection Spectra | 4 pages, 4 figures | null | 10.1063/1.3009579 | null | cond-mat.supr-con | null | When the $d_{x^2-y^2}$-wave pairing is suppressed by Zn-doping in
$YBa_2Cu_3O_{7-\delta}$ some of the Andreev reflection spectra were found to be
similar to the s-wave spectra of conventional superconductors. The energy gap
is rather reproducible (2.3-3.0meV). It is suppressed by low magnetic field
($H_C^{PC}=120-270mT$) in great contrast to the d-wave spectra ($H_C^{PC}>3T$)
with the similar order of the gap value. We suppose that the s-wave pairing
occurs near the Zn-impurities.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:20:32 GMT"
}
] | 2010-09-21T00:00:00 | [
[
"Akimenko",
"A. I.",
""
],
[
"Gudimenko",
"V. A.",
""
]
] | [
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711.4528 | Juha Vierinen | Markku Markkanen, Juha Vierinen | Polyphase alternating codes | Submitted to Annales Geophysicae | null | 10.5194/angeo-26-2237-2008 | null | physics.data-an physics.space-ph | null | This work introduces a method for constructing polyphase alternating codes in
which the length of a code transmission cycle can be $p^m$ or $p-1$, where $p$
is a prime number and $m$ is a positive integer. The relevant properties
leading to the construction alternating codes and the algorithm for generating
alternating codes is described. Examples of all practical and some not that
practical polyphase code lengths are given.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:28:58 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Markkanen",
"Markku",
""
],
[
"Vierinen",
"Juha",
""
]
] | [
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] |
711.4529 | Hua Liang Chang | Huai-Liang Chang | Donaldson Thomas invariant of P^1 scroll | null | null | null | null | math.AG math.AC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let X be a P^1 scroll (a compactification of a line bundle L) over a complex
surafce S and assume S has a global two form with zero loci a smooth curve C.
The Donaldson Thomas invariants of X is shown to be zero if the curve class has
is component on S not a multiple of [C]. For nonzero case, when the prime field
insertion are above C, the invariant is shown to depend only on the analytic
neighborhood of L in X.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:29:11 GMT"
},
{
"version": "v2",
"created": "Tue, 24 Mar 2009 19:20:52 GMT"
},
{
"version": "v3",
"created": "Sat, 28 Mar 2009 14:02:26 GMT"
}
] | 2009-03-28T00:00:00 | [
[
"Chang",
"Huai-Liang",
""
]
] | [
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711.453 | Sebastian Volz | S. Gom\`es (CETHIL), Po Chapuis (EM2C), F. Nepveu, N. Trannoy, S. Volz
(EM2C), B. Charlot (TIMA), Gilles Tessier (LPEM), S. Dilhaire (CPMOH),
Bernard Cretin (FEMTO-ST), Pascal Vairac (FEMTO-ST) | Temperature measurement of sub-micrometric ICs by scanning thermal
microscopy | null | IEEE Transactions on Components and Packaging Technologies 30, 3
(2007) 424-431 | 10.1109/TCAPT.2007.901748 | null | physics.class-ph | null | Surface temperature measurements were performed with a Scanning Thermal
Microscope mounted with a thermoresistive wire probe of micrometrSurface
temperature measurements were performed with a Scanning Thermal Microscope
mounted with a thermoresistive wire probe of micrometric size. A CMOS device
was designed with arrays of resistive lines 0.35$\mu$m in width. The array
periods are 0.8micron and 10micron to study the spatial resolution of the SThM.
Integrated Circuits with passivation layers of micrometric and nanometric
thicknesses were tested. To enhance signal-to-noise ratio, the resistive lines
were heated with an AC current. The passivation layer of nanometric thickness
allows us to distinguish the lines when the array period is 10micron. The
results raise the difficulties of the SThM measurement due to the design and
the topography of ICs on one hand and the size of the thermal probe on the
other hand.ic size. A CMOS device was designed with arrays of resistive lines
0.35$\mu$m in width. The array periods are 0.8micron and 10micron to study the
spatial resolution of the SThM. Integrated Circuits with passivation layers of
micrometric and nanometric thicknesses were tested. To enhance signal-to-noise
ratio, the resistive lines were heated with an AC current. The passivation
layer of nanometric thickness allows us to distinguish the lines when the array
period is 10micron. The results raise the difficulties of the SThM measurement
due to the design and the topography of ICs on one hand and the size of the
thermal probe on the other hand.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:28:38 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Gomès",
"S.",
"",
"CETHIL"
],
[
"Chapuis",
"Po",
"",
"EM2C"
],
[
"Nepveu",
"F.",
"",
"EM2C"
],
[
"Trannoy",
"N.",
"",
"EM2C"
],
[
"Volz",
"S.",
"",
"EM2C"
],
[
"Charlot",
"B.",
"",
"TIMA"
],
[
"Tessier",
"Gilles",
"",
"LPEM"
],
[
"Dilhaire",
"S.",
"",
"CPMOH"
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[
"Cretin",
"Bernard",
"",
"FEMTO-ST"
],
[
"Vairac",
"Pascal",
"",
"FEMTO-ST"
]
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] |
711.4531 | Morley Bell | M.B. Bell | Evidence in Support of the Local Quasar Model from Inner Jet Structure
and Angular Motions in Radio Loud AGN | 9 pages with 5 figures, submitted to ApJL | null | null | null | astro-ph | null | Radio loud jetted sources with and without extended inner jet structure show
good agreement with the simple ballistic ejection scenario proposed in the
decreasing intrinsic redshift (DIR) model, where, because of projection
effects, those that show the most obvious extended structure and large angular
motions are assumed to have jets that lie close to the plane of the sky, and
those with little or no structure and small angular motions are assumed to have
jets that are coming almost directly towards us. This simple model also
predicts several other relations seen in the raw data that, in some cases, may
be less easily explained if the redshifts are cosmological and relativistic
ejection is required. In particular, for radio-loud sources the source number
density is found to be high for sources that are not Doppler boosted but low
for highly boosted sources. This is opposite to what is expected, suggesting
that Doppler boosting may not be involved at all, which would be in agreement
with the DIR model. If so, the reality of relativistic beaming in quasar jets,
the assumption of which has been the very foundation of the superluminal motion
explanation in the cosmological redshift (CR) model, would then be questioned.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:30:33 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 18:18:03 GMT"
}
] | 2007-12-12T00:00:00 | [
[
"Bell",
"M. B.",
""
]
] | [
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711.4532 | Yuji Tachikawa | Ofer Aharony and Yuji Tachikawa | A holographic computation of the central charges of d=4, N=2 SCFTs | 16 pages; v4: one reference added | JHEP 0801:037,2008 | 10.1088/1126-6708/2008/01/037 | WIS/20/07-NOV-DPP | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We use the AdS/CFT correspondence to compute the central charges of the d=4,
N=2 superconformal field theories arising from N D3-branes at singularities in
F-theory. These include the conformal theories with E_n global symmetries. We
compute the central charges a and c related to the conformal anomaly, and also
the central charges k associated to the global symmetry in these theories. All
of these are related to the coefficients of Chern-Simons terms in the dual
string theory on AdS_5. Our computation is exact for all values of N, enabling
several tests of the dualities recently proposed by Argyres and Seiberg for the
E_6 and E_7 theories with N=1.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:35:58 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Dec 2007 19:36:08 GMT"
},
{
"version": "v3",
"created": "Mon, 10 Mar 2008 18:03:36 GMT"
},
{
"version": "v4",
"created": "Fri, 8 Aug 2008 14:38:44 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Aharony",
"Ofer",
""
],
[
"Tachikawa",
"Yuji",
""
]
] | [
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] |
711.4533 | Stefano Piscanec | V. Scardaci, S. Piscanec, Michele Lazzeri, R. Krupke, Francesco Mauri,
A.C. Ferrari | Temperature dependent phonon renormalization in metallic nanotubes | 5 pages, 3 figures | null | null | null | cond-mat.mtrl-sci | null | We measure the temperature dependence of the Raman spectra of metallic and
semiconducting nanotubes. We show that the different trend in metallic tubes is
due to phonon re-normalization induced by the variation in electronic
temperature, which is modeled including non-adiabatic contributions to account
for the dynamic, time dependent nature
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:46:18 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Scardaci",
"V.",
""
],
[
"Piscanec",
"S.",
""
],
[
"Lazzeri",
"Michele",
""
],
[
"Krupke",
"R.",
""
],
[
"Mauri",
"Francesco",
""
],
[
"Ferrari",
"A. C.",
""
]
] | [
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] |
711.4534 | Jaromir Fiurasek | A. Cernoch, J. Soubusta, L. Bartuskova, M. Dusek, J. Fiurasek | Experimental realization of linear-optical partial SWAP gates | 4 pages, 4 figures, RevTeX4 | Phys. Rev. Lett. 100, 180501 (2008). | 10.1103/PhysRevLett.100.180501 | null | quant-ph | null | We present a linear-optical implementation of a class of two-qubit partial
SWAP gates for polarization states of photons. Different gate operations,
including the SWAP and entangling square root of SWAP, can be obtained by
changing a classical control parameter -- namely the path difference in the
interferometer. Reconstruction of output states, full process tomography and
evaluation of entanglement of formation prove very good performance of the
gates.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:38:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cernoch",
"A.",
""
],
[
"Soubusta",
"J.",
""
],
[
"Bartuskova",
"L.",
""
],
[
"Dusek",
"M.",
""
],
[
"Fiurasek",
"J.",
""
]
] | [
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] |
711.4535 | Bernhard Urbaszek | D. Lagarde, A. Balocchi, H. Carrere, P. Renucci, T. Amand, X. Marie,
S. Founta, H. Mariette | Room temperature Optical Orientation of Exciton Spin in cubic GaN/AlN
quantum dots | null | null | 10.1103/PhysRevB.77.041304 | null | cond-mat.other cond-mat.mtrl-sci | null | The optical orientation of the exciton spin in an ensemble of self-organized
cubic GaN/AlN quantum dots is studied by time-resolved photoluminescence. Under
a polarized quasi-resonant excitation, the luminescence linear polarization
exhibits no temporal decay, even at room temperature. This demonstrates the
robustness of the exciton spin polarization in these cubic nitride
nanostructures, with characteristic decay times longer than 10 ns.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 16:43:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lagarde",
"D.",
""
],
[
"Balocchi",
"A.",
""
],
[
"Carrere",
"H.",
""
],
[
"Renucci",
"P.",
""
],
[
"Amand",
"T.",
""
],
[
"Marie",
"X.",
""
],
[
"Founta",
"S.",
""
],
[
"Mariette",
"H.",
""
]
] | [
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] |
711.4536 | Mikhail Kozlov | V. V. Flambaum and M. G. Kozlov | Studying variation of fundamental constants with molecules | 14 pages, 2 figures, RevTeX4; v2: one section and 10 new references
added | Chapter in book "Cold Molecules: Theory, Experiment,
Applications", Edited by R V Krems, W C Stwalley, and B Friedrich, CRC Press,
2009 | null | null | physics.atom-ph | null | This review article is devoted to application of precision molecular
spectroscopy to studies of the possible spatial and temporal variations of the
fundamental constants. Both astrophysical observations and laboratory
experiments are discussed.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:02:36 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jan 2008 08:14:54 GMT"
}
] | 2009-07-18T00:00:00 | [
[
"Flambaum",
"V. V.",
""
],
[
"Kozlov",
"M. G.",
""
]
] | [
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711.4537 | Martin Sieber | Jack Kuipers and Martin Sieber | The semiclassical relation between open trajectories and periodic orbits
for the Wigner time delay | 21 pages, 5 figures | Phys. Rev. E 77 (2008) 046219 | 10.1103/PhysRevE.77.046219 | null | nlin.CD cond-mat.mes-hall | null | The Wigner time delay of a classically chaotic quantum system can be
expressed semiclassically either in terms of pairs of scattering trajectories
that enter and leave the system or in terms of the periodic orbits trapped
inside the system. We show how these two pictures are related on the
semiclassical level. We start from the semiclassical formula with the
scattering trajectories and derive from it all terms in the periodic orbit
formula for the time delay. The main ingredient in this calculation is a new
type of correlation between scattering trajectories which is due to
trajectories that approach the trapped periodic orbits closely. The equivalence
between the two pictures is also demonstrated by considering correlation
functions of the time delay. A corresponding calculation for the conductance
gives no periodic orbit contributions in leading order.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:03:40 GMT"
}
] | 2010-03-09T00:00:00 | [
[
"Kuipers",
"Jack",
""
],
[
"Sieber",
"Martin",
""
]
] | [
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] |
711.4538 | Angelo Bassi Dr. | A. Bassi, G.C. Ghirardi | On a recent proposal of faster than light quantum communication | 9 pages, LaTeX. Minor changes made | Int. Journ. Theor. Phys. 47, 2500 (2008). | 10.1007/s10773-008-9683-4 | null | quant-ph | null | In a recent paper, A.Y. Shiekh has discussed an experimental set-up which, in
his opinion, should make possible faster-than-light communication using the
collapse of the quantum wave function. Contrary to the many proposals which
have been presented in the past, he does not resort to an entangled state of
two systems but he works with a single particle in a superposition of two
states - corresponding to its propagation in opposite directions - one of which
goes through an appropriate interferometer. The possibility for an observer
near the interferometer to introduce or not, at his free will, a phase shifter
along one of the paths should allow to change instantaneously the probability
of finding the particle in the far-away region corresponding to the other state
of the superposition and, correspondingly, to change the intensity of a beam of
particles reaching a distant observer. In this paper we show a flaw in the
argument: once more, as it has been proved in full generality a long time ago,
the process of wave packet reduction cannot be used for superluminal
communication.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:08:06 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 18:56:43 GMT"
},
{
"version": "v3",
"created": "Thu, 20 Mar 2008 13:17:55 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bassi",
"A.",
""
],
[
"Ghirardi",
"G. C.",
""
]
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711.4539 | Alberto Saa | Roberto Venegeroles and Alberto Saa | Non-Gaussian features of chaotic Hamiltonian transport | 19 pages, 6 Figures. v2: Grammatical corrections, new references | J. Stat. Mech. (2008) P01005 | 10.1088/1742-5468/2008/01/P01005 | null | nlin.CD | null | Some non-Gaussian aspects of chaotic transport are investigated for a general
class of two-dimensional area-preserving maps. Kurtosis, in particular, is
calculated from the diffusion and the Burnett coefficients, which are obtained
analytically. A characteristic time scale delimiting the onset of the Markovian
regime for the master equation is established. Some explicit examples are
discussed.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:12:30 GMT"
},
{
"version": "v2",
"created": "Thu, 29 Nov 2007 11:22:28 GMT"
},
{
"version": "v3",
"created": "Mon, 10 Dec 2007 00:54:02 GMT"
}
] | 2008-01-03T00:00:00 | [
[
"Venegeroles",
"Roberto",
""
],
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"Saa",
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""
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711.454 | Nicola Coppola | N. Coppola (for the H1 Collaboration and ZEUS Collaboration) | High p_T jets in DIS and gamma p at HERA | 4 pages, 5 figures, submitted to proceedings ISMD2007; revised
version (few comments, typos corrected) | Acta Phys.Polon.Supp.1:475-478,2008 | null | null | hep-ex | null | Recent results on di-jet, inclusive jets, production at high p_T in Deep
Inelastic Scattering DIS and photoproduction gamma p regimes using both the H1
and ZEUS detectors at HERA are presented. Also studies of integrated jet shape
and jet radius dependencies in DIS performed by the ZEUS Collaborations are
discussed. All the measurements are found to be well described by calculations
at the next-to-leading order in perturbative QCD. A combined determination of
the value of the strong coupling constant alpha_s(M_Z) from the H1 and ZEUS
Collaborations using inclusive-jet cross-section measurements in neutral
current DIS at high Q^2 is shown.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:12:58 GMT"
},
{
"version": "v2",
"created": "Fri, 30 Nov 2007 12:31:43 GMT"
}
] | 2019-08-14T00:00:00 | [
[
"Coppola",
"N.",
"",
"for the H1 Collaboration and ZEUS Collaboration"
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711.4541 | Shahar Hod | Shahar Hod | Einstein-Yang-Mills Solitons: The Role of Gravity | 6 pages | Phys.Lett.B657:255-256,2007 | 10.1016/j.physletb.2007.10.015 | null | hep-th astro-ph gr-qc | null | The canonical Bartnik-McKinnon solitons are regular solutions of the coupled
Einstein-Yang-Mills system in which gravity may balance the repulsive nature of
the Yang-Mills field. We examine the role played by gravity in balancing the
system and determine its strength. In particular, we obtain an analytic lower
bound on the fundamental mass-to-radius ratio, max{2m(r)/r}>2/3, which is a
necessary condition for the existence of globally regular Einstein-Yang-Mills
solitons. Our analytical results are in accord with numerical calculations.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:17:08 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hod",
"Shahar",
""
]
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711.4542 | Torsten B\"oker | Torsten Boeker | Are Globular Clusters the Remnant Nuclei of Progenitor Disk Galaxies? | 5 pages, no figures. Accepted by ApJ Letters | null | 10.1086/527033 | null | astro-ph | null | The globular cluster system of a typical spheroidal galaxy makes up about
0.25% of the total galaxy mass (McLaughlin 1999). This is roughly the same mass
fraction as contained in the nuclear star clus- ter (or stellar nucleus)
present in most nearby low-mass galaxies. Motivated by this "coincidence", this
Letter discusses a scenario in which globular clusters of present-day galaxies
are the surviving nuclei of the dwarf galaxies that - according to the
hierarchical merging paradigm of galaxy forma- tion - constitute the "building
blocks" of present-day massive galaxies. This scenario, which was first
suggested by Freeman (1993), has become more attractive recently in the light
of studies that demonstrate a complex star formation history in a number of
massive globular clusters.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:31:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Boeker",
"Torsten",
""
]
] | [
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] |
711.4543 | Jan Budaj | I. Iliev, J. Budaj | Am stars in binary systems | 6 pages, 0 figures, submitted to Contrib. Astron. Obs. Skalnate Pleso
(Proceedings from the International workshop CP#Ap 2007, Vienna, Sep. 10-14,
2007, eds. J. Ziznovsky, J. Zverko, E. Pauntzen, M. Netopil) | null | null | null | astro-ph | null | It is argued that apart from the well known dependence of the Am phenomenon
on the mass, age (effective temperature, gravity) and rotation there is also a
complex dependence on the orbital parameters in binary systems. This is why the
generally accepted scenario in which the Am star rotation plays a unique role
needs to be revisited, the strong correlations between the rotation, orbital
period and eccentricity need to be properly addressed and tidal effects taken
into account. Recent observations of Am stars in binary systems are reviewed.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:37:19 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Iliev",
"I.",
""
],
[
"Budaj",
"J.",
""
]
] | [
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] |
711.4544 | Yogiro Hama | Yogiro Hama, Rone Peterson G. Andrade, Fr\'ed\'erique Grassi,
Wei-Liang Qian, Takeshi Osada, Carlos Eduardo Aguiar, Takeshi Kodama | NeXSPheRIO Results on Elliptic-Flow Fluctuations at RHIC | 12 pages, 6 figures, prepared for the Workshop "Relativistic Nuclear
Physics: from Nuclotron to LHC Energies", June 18-22, 2007 (BITP, Kiev,
Ukraine) | Phys.Atom.Nucl.71:1558-1564,2008 | 10.1134/S106377880809010X | null | hep-ph | null | By using the NexSPheRIO code, we study the elliptic-flow fluctuations in
Au+Au collisions at 200A GeV. It is shown that, by fixing the parameters of the
model to correctly reproduce the charged pseudo-rapidity and the
transverse-momentum distributions, reasonable agreement of <v_2> with data is
obtained, both as function of pseudo-rapidity as well as of transverse
momentum, for charged particles. Our results on elliptic-flow fluctuations are
in good agreement with the recently measured data in experiments.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:38:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hama",
"Yogiro",
""
],
[
"Andrade",
"Rone Peterson G.",
""
],
[
"Grassi",
"Frédérique",
""
],
[
"Qian",
"Wei-Liang",
""
],
[
"Osada",
"Takeshi",
""
],
[
"Aguiar",
"Carlos Eduardo",
""
],
[
"Kodama",
"Takeshi",
""
]
] | [
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] |
711.4545 | Sylvain Brochard | Sylvain Brochard | Foncteur de Picard d'un champ alg\'ebrique | null | Math. Ann. Volume 343, Number 3 / mars 2009, pages 541-602. | 10.1007/s00208-008-0282-8 | null | math.AG | null | In this article we study the Picard functor and the Picard stack of an
algebraic stack. We give a new and direct proof of the representability of the
Picard stack. We prove that it is quasi-separated, and that the connected
component of the identity is proper when the fibers of the stack are
geometrically normal. We study some examples of Picard functors of classical
stacks. In an appendix, we review the lisse-etale cohomology of abelian sheaves
on an algebraic stack.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:58:12 GMT"
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] | 2009-09-18T00:00:00 | [
[
"Brochard",
"Sylvain",
""
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] |
711.4546 | A. Tureanu | M. Chaichian, M. R. Setare, A. Tureanu, G. Zet | On Black Holes and Cosmological Constant in Noncommutative Gauge Theory
of Gravity | Based on a talk given at the International Conference on Fundamental
and Applied Research in Physics "Farphys 2007", 25-28 October 2007, Iasi,
Romania | JHEP0804:064,2008 | 10.1088/1126-6708/2008/04/064 | null | hep-th gr-qc | null | Deformed Reissner-Nordstr\"om, as well as Reissner-Nordstr\"om de Sitter,
solutions are obtained in a noncommutative gauge theory of gravitation. The
gauge potentials (tetrad fields) and the components of deformed metric are
calculated to second order in the noncommutativity parameter. The solutions
reduce to the deformed Schwarzschild ones when the electric charge of the
gravitational source and the cosmological constant vanish. Corrections to the
thermodynamical quantities of the corresponding black holes and to the radii of
different horizons have been determined. All the independent invariants, such
as the Ricci scalar and the so-called Kretschmann scalar, have the same
singularity structure as the ones of the usual undeformed case and no smearing
of singularities occurs. The possibility of such a smearing is discussed. In
the noncommutative case we have a local disturbance of the geometry around the
source, although asymptotically at large distances it becomes flat.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:48:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Chaichian",
"M.",
""
],
[
"Setare",
"M. R.",
""
],
[
"Tureanu",
"A.",
""
],
[
"Zet",
"G.",
""
]
] | [
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] |
711.4547 | Alessio Marrani | S. Bellucci, S. Ferrara, R. Kallosh, A. Marrani | Extremal Black Hole and Flux Vacua Attractors | 1+74 pages, 2 Tables. Contribution to the Proceedings of the Winter
School on Attractor Mechanism 2006 (SAM2006), 20-24 March 2006, INFN-LNF,
Frascati, Italy | Lect.NotesPhys.755:115-191,2008 | null | CERN-PH-TH/182; UCLA/07/TEP/22; SU-ITP-2007-21 | hep-th | null | These lectures provide a pedagogical, introductory review of the so-called
Attractor Mechanism (AM) at work in two different 4-dimensional frameworks:
extremal black holes in N=2 supergravity and N=1 flux compactifications. In the
first case, AM determines the stabilization of scalars at the black hole event
horizon purely in terms of the electric and magnetic charges, whereas in the
second context the AM is responsible for the stabilization of the universal
axion-dilaton and of the (complex structure) moduli purely in terms of the RR
and NSNS fluxes. Two equivalent approaches to AM, namely the so-called
``criticality conditions'' and ``New Attractor'' ones, are analyzed in detail
in both frameworks, whose analogies and differences are discussed. Also a
stringy analysis of both frameworks (relying on Hodge-decomposition techniques)
is performed, respectively considering Type IIB compactified on $CY_{3}$ and
its orientifolded version, associated with $\frac{CY_{3}\times
T^{2}}{\mathbb{Z}_{2}}$. Finally, recent results on the U-duality orbits and
moduli spaces of non-BPS extremal black hole attractors in $3\leqslant
N\leqslant 8$, d=4 supergravities are reported.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 17:49:18 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Bellucci",
"S.",
""
],
[
"Ferrara",
"S.",
""
],
[
"Kallosh",
"R.",
""
],
[
"Marrani",
"A.",
""
]
] | [
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] |
711.4548 | Stefan Taubenberger | S. Taubenberger, S. Hachinger, G. Pignata, P. A. Mazzali, C.
Contreras, S. Valenti, A. Pastorello, N. Elias-Rosa, O. B\"arnbantner, H.
Barwig, S. Benetti, M. Dolci, J. Fliri, G. Folatelli, W. L. Freedman, S.
Gonzalez, M. Hamuy, W. Krzeminski, N. Morrell, H. Navasardyan, S. E. Persson,
M. M. Phillips, C. Ries, M. Roth, N. B. Suntzeff, M. Turatto and W.
Hillebrandt | The underluminous Type Ia Supernova 2005bl and the class of objects
similar to SN 1991bg | 24 pages, 24 figures, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12843.x | null | astro-ph | null | Optical observations of the Type Ia supernova (SN Ia) 2005bl in NGC 4070,
obtained from -6 to +66 d with respect to the B-band maximum, are presented.
The photometric evolution is characterised by rapidly-declining light curves
and red colours at peak and soon thereafter. With M_B,max = -17.24 the SN is an
underluminous SN Ia, similar to the peculiar SNe 1991bg and 1999by. This
similarity also holds for the spectroscopic appearance, the only remarkable
difference being the likely presence of carbon in pre-maximum spectra of SN
2005bl. A comparison study among underluminous SNe Ia is performed, based on a
number of spectrophotometric parameters. Previously reported correlations of
the light-curve decline rate with peak luminosity and R(Si) are confirmed, and
a large range of post-maximum Si II lambda6355 velocity gradients is
encountered. 1D synthetic spectra for SN 2005bl are presented, which confirm
the presence of carbon and suggest an overall low burning efficiency with a
significant amount of leftover unburned material. Also, the Fe content in
pre-maximum spectra is very low, which may point to a low metallicity of the
precursor. Implications for possible progenitor scenarios of underluminous SNe
Ia are briefly discussed.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:32:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Taubenberger",
"S.",
""
],
[
"Hachinger",
"S.",
""
],
[
"Pignata",
"G.",
""
],
[
"Mazzali",
"P. A.",
""
],
[
"Contreras",
"C.",
""
],
[
"Valenti",
"S.",
""
],
[
"Pastorello",
"A.",
""
],
[
"Elias-Rosa",
"N.",
""
],
[
"Bärnbantner",
"O.",
""
],
[
"Barwig",
"H.",
""
],
[
"Benetti",
"S.",
""
],
[
"Dolci",
"M.",
""
],
[
"Fliri",
"J.",
""
],
[
"Folatelli",
"G.",
""
],
[
"Freedman",
"W. L.",
""
],
[
"Gonzalez",
"S.",
""
],
[
"Hamuy",
"M.",
""
],
[
"Krzeminski",
"W.",
""
],
[
"Morrell",
"N.",
""
],
[
"Navasardyan",
"H.",
""
],
[
"Persson",
"S. E.",
""
],
[
"Phillips",
"M. M.",
""
],
[
"Ries",
"C.",
""
],
[
"Roth",
"M.",
""
],
[
"Suntzeff",
"N. B.",
""
],
[
"Turatto",
"M.",
""
],
[
"Hillebrandt",
"W.",
""
]
] | [
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] |
711.4549 | Dariusz Lis | D.C. Lis, D. Bockelee-Morvan, J. Boissier, J. Crovisier, N. Biver, and
S.B. Charnley | Hydrogen Isocyanide in Comet 73P/Schwassmann-Wachmann (Fragment B) | 6 pages, 5 figures, 2 tables | null | 10.1086/527345 | null | astro-ph | null | We present a sensitive 3-sigma upper limit of 1.1% for the HNC/HCN abundance
ratio in comet 73P/Schwassmann-Wachmann (Fragment B), obtained on May 10-11,
2006 using Caltech Submillimeter Observatory (CSO). This limit is a factor of
~7 lower than the values measured previously in moderately active comets at 1
AU from the Sun. Comet 73P/Schwassmann-Wachmann was depleted in most volatile
species, except of HCN. The low HNC/HCN ratio thus argues against HNC
production from polymers produced from HCN. However, thermal degradation of
macromolecules, or polymers, produced from ammonia and carbon compounds, such
as acetylene, methane, or ethane appears a plausible explanation for the
observed variations of the HNC/HCN ratio in moderately active comets, including
the very low ratio in comet 73P/Schwassmann-Wachmann reported here. Similar
polymers have been invoked previously to explain anomalous 14N/15N ratios
measured in cometary CN.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:04:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Lis",
"D. C.",
""
],
[
"Bockelee-Morvan",
"D.",
""
],
[
"Boissier",
"J.",
""
],
[
"Crovisier",
"J.",
""
],
[
"Biver",
"N.",
""
],
[
"Charnley",
"S. B.",
""
]
] | [
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] |
711.455 | George Svetlichny | George Svetlichny | Equivariance, Variational Principles, and the Feynman Integral | This is a contribution to the Proc. of the Seventh International
Conference ''Symmetry in Nonlinear Mathematical Physics'' (June 24-30, 2007,
Kyiv, Ukraine), published in SIGMA (Symmetry, Integrability and Geometry:
Methods and Applications) at http://www.emis.de/journals/SIGMA/ | SIGMA 4 (2008), 032, 13 pages | 10.3842/SIGMA.2008.032 | null | math-ph math.MP | null | We argue that the variational calculus leading to Euler's equations and
Noether's theorem can be replaced by equivariance and invariance conditions
avoiding the action integral. We also speculate about the origin of Lagrangian
theories in physics and their connection to Feynman's integral.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:02:30 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Mar 2008 07:54:13 GMT"
}
] | 2008-04-25T00:00:00 | [
[
"Svetlichny",
"George",
""
]
] | [
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] |
711.4551 | Rajamani Narayanan | R. Narayanan, H. Neuberger | Universality of large N phase transitions in Wilson loop operators in
two and three dimensions | 43 pages, 1 table, 18 figures, uses JHEP3.cls, one reference added,
replaced Figure 3 and a small change to eqn (4.8) | JHEP 0712:066,2007 | 10.1088/1126-6708/2007/12/066 | null | hep-th hep-lat | null | The eigenvalue distribution of a Wilson loop operator of fixed shape
undergoes a transition under scaling at infinite N. We derive a large N scaling
function in a double scaling limit of the average characteristic polynomial
associated with the Wilson loop operator in two dimensional QCD. We hypothesize
that the transition in three and four dimensional large N QCD are also in the
same universality class and provide a numerical test for our hypothesis in
three dimensions.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:10:10 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Dec 2007 19:34:51 GMT"
},
{
"version": "v3",
"created": "Sun, 9 Dec 2007 10:14:23 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Narayanan",
"R.",
""
],
[
"Neuberger",
"H.",
""
]
] | [
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] |
711.4552 | Oren Zarchin | O. Zarchin, M. Zaffalon, M. Heiblum, D. Mahalu, and V. Umansky | Two-electron bunching in transport through a QD induced by Kondo
correlations | null | null | 10.1103/PhysRevB.77.241303 | null | cond-mat.mes-hall | null | We report on noise measurements in a quantum dot in the presence of Kondo
correlations. Close to the unitary limit, with the conductance reaching
1.8e2/h, we observed an average backscattered charge of e*~5e/3, while weakly
biasing the quantum dot. This result held to bias voltages up to half the Kondo
temperature. Away from the unitary limit, the charge was measured to be e as
expected. These results confirm and extend the prediction by E. Sela et al.
[1], that suggested that two-electron backscattering processes dominate over
single-electron backscattering processes near the unitary limit, with an
average backscattered charge e*~5e/3.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:14:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zarchin",
"O.",
""
],
[
"Zaffalon",
"M.",
""
],
[
"Heiblum",
"M.",
""
],
[
"Mahalu",
"D.",
""
],
[
"Umansky",
"V.",
""
]
] | [
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] |
711.4553 | Markus Schmidt | Markus A. Schmidt, Luis N. Prill Sempere, Hemant K. Tyagi, Chris G.
Poulton, and Philip St.J. Russell | Waveguiding and Plasmon Resonances in Two-Dimensional Photonic Lattices
of Gold and Silver Nanowires | 4 pages, 4 figures | null | 10.1103/PhysRevB.77.033417 | null | physics.optics | null | We report the fabrication of triangular lattices of parallel gold and silver
nanowires of high optical quality, with diameters down to 500 nm and
length-to-diameter ratios as high as 100,000. The nanowires are supported by a
silica glass matrix and are disposed around a central solid glass core, i.e., a
missing nanowire. These cm-long structures make it possible to trap light
within an array of nanowires and characterize the plasmon resonances that form
at specific optical frequencies. Such nanowire arrays have many potential
applications, e.g., to imaging on the sub-wavelength scale.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:15:10 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schmidt",
"Markus A.",
""
],
[
"Sempere",
"Luis N. Prill",
""
],
[
"Tyagi",
"Hemant K.",
""
],
[
"Poulton",
"Chris G.",
""
],
[
"Russell",
"Philip St. J.",
""
]
] | [
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] |
711.4554 | Diana Lopez Nacir | Diana L\'opez Nacir and Francisco D. Mazzitelli | New counterterms induced by trans-Planckian physics in semiclassical
gravity | null | Phys.Rev.D78:044001,2008 | 10.1103/PhysRevD.78.044001 | null | gr-qc hep-th | null | We consider free and self-interacting quantum scalar fields satisfying
modified dispersion relations in the framework of Einstein-Aether theory. Using
adiabatic regularization, we study the renormalization of the equation for the
mean value of the field in the self-interacting case, and the renormalization
of the semiclassical Einstein-Aether equations for free fields. In both cases
we consider Bianchi type I background spacetimes. Contrary to what happens for
{\it free} fields in {\it flat} Robertson-Walker spacetimes, the
self-interaction and/or the anisotropy produce non-purely geometric terms in
the adiabatic expansion, i.e terms that involve both the metric $g_{\mu\nu}$
and the aether field $u_{\mu}$. We argue that, in a general spacetime, the
renormalization of the theory would involve new counterterms constructed with
$g_{\mu\nu}$ and $u_{\mu}$, generating a fine-tuning problem for the
Einstein-Aether theory.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:16:56 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Nacir",
"Diana López",
""
],
[
"Mazzitelli",
"Francisco D.",
""
]
] | [
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] |
711.4555 | John Lafferty | Pradeep Ravikumar, John Lafferty, Han Liu, Larry Wasserman | Sparse Additive Models | null | null | null | null | math.ST stat.TH | null | We present a new class of methods for high-dimensional nonparametric
regression and classification called sparse additive models (SpAM). Our methods
combine ideas from sparse linear modeling and additive nonparametric
regression. We derive an algorithm for fitting the models that is practical and
effective even when the number of covariates is larger than the sample size.
SpAM is closely related to the COSSO model of Lin and Zhang (2006), but
decouples smoothing and sparsity, enabling the use of arbitrary nonparametric
smoothers. An analysis of the theoretical properties of SpAM is given. We also
study a greedy estimator that is a nonparametric version of forward stepwise
regression. Empirical results on synthetic and real data are presented, showing
that SpAM can be effective in fitting sparse nonparametric models in high
dimensional data.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:28:59 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Apr 2008 03:58:42 GMT"
}
] | 2008-04-09T00:00:00 | [
[
"Ravikumar",
"Pradeep",
""
],
[
"Lafferty",
"John",
""
],
[
"Liu",
"Han",
""
],
[
"Wasserman",
"Larry",
""
]
] | [
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] |
711.4556 | Mikhail Voloshin | M.B. Voloshin | Charmonium | 67 pages, 10 figures, To be published in Prog. Part. Nucl. Phys | Prog.Part.Nucl.Phys.61:455-511,2008 | 10.1016/j.ppnp.2008.02.001 | FTPI-MINN-07/34, UMN-TH-2625/07 | hep-ph | null | Topics in the description of the properties of charmonium states are reviewed
with an emphasis on specific theoretical ideas and methods of relating those
properties to the underlying theory of Quantum Chromodynamics.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:33:44 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Dec 2007 20:34:14 GMT"
},
{
"version": "v3",
"created": "Wed, 30 Jan 2008 19:51:08 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Voloshin",
"M. B.",
""
]
] | [
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] |
711.4557 | Wenyi Zhang | Wenyi Zhang and Urbashi Mitra | On Outage Behavior of Wideband Slow-Fading Channels | Submitted to IEEE Transactions on Information Theory | null | null | USC CSI Technical Report CSI 07-08-01 | cs.IT math.IT | null | This paper investigates point-to-point information transmission over a
wideband slow-fading channel, modeled as an (asymptotically) large number of
independent identically distributed parallel channels, with the random channel
fading realizations remaining constant over the entire coding block. On the one
hand, in the wideband limit the minimum achievable energy per nat required for
reliable transmission, as a random variable, converges in probability to
certain deterministic quantity. On the other hand, the exponential decay rate
of the outage probability, termed as the wideband outage exponent,
characterizes how the number of parallel channels, {\it i.e.}, the
``bandwidth'', should asymptotically scale in order to achieve a target outage
probability at a target energy per nat. We examine two scenarios: when the
transmitter has no channel state information and adopts uniform transmit power
allocation among parallel channels; and when the transmitter is endowed with an
one-bit channel state feedback for each parallel channel and accordingly
allocates its transmit power. For both scenarios, we evaluate the wideband
minimum energy per nat and the wideband outage exponent, and discuss their
implication for system performance.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:38:13 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Zhang",
"Wenyi",
""
],
[
"Mitra",
"Urbashi",
""
]
] | [
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711.4558 | Enrico Barausse | E. Barausse (SISSA, Italy) and L. Rezzolla (AEI, Germany) | The influence of the hydrodynamic drag from an accretion torus on
extreme mass-ratio inspirals | 21 pages, 8 figures. Phys. Rev. D, in press. Typos fixed and minor
changes; added discussion on the gravitational pull exerted by the torus | Phys.Rev.D77:104027,2008 | 10.1103/PhysRevD.77.104027 | null | gr-qc astro-ph | null | We have studied extreme mass-ratio inspirals (EMRIs) in spacetimes containing
a rotating black hole and a non self-gravitating torus with constant specific
angular momentum. We have found that the effect of the hydrodynamic drag
exerted by the torus on the satellite is much smaller than the corresponding
one due to radiation reaction, for systems such as those generically expected
in AGNs and at distances from the SMBH which can be probed with LISA. However,
given the uncertainty on the parameters of these systems, there exist
configurations in which the effect of the hydrodynamic drag can be comparable
to the radiation-reaction one in phases of the inspiral which are detectable by
LISA. This is the case, for instance, for a 10^6 M_sun SMBH surrounded by a
corotating torus of comparable mass and with radius of 10^3-10^4 gravitational
radii, or for a 10^5 M_sun SMBH surrounded by a corotating 10^4 M_sun torus
with radius of 10^5 gravitational radii. Should these conditions be met in
astrophysical systems, EMRI-gravitational waves could provide a characteristic
signature of the presence of the torus. In fact, while radiation reaction
always increases the inclination of the orbit with respect to the equatorial
plane, the hydrodynamic drag from a torus corotating with the SMBH always
decreases it. However, even when initially dominating over radiation reaction,
the influence of the hydrodynamic drag decays very rapidly as the satellite
moves into the very strong-field region of the SMBH (i.e., p <~ 5M). Although
our results have been obtained for a specific class of tori, we argue that they
will be qualitatively valid also for more generic distributions of the specific
angular momentum.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 18:55:08 GMT"
},
{
"version": "v2",
"created": "Wed, 28 Nov 2007 22:07:50 GMT"
},
{
"version": "v3",
"created": "Fri, 16 May 2008 12:21:39 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Barausse",
"E.",
"",
"SISSA, Italy"
],
[
"Rezzolla",
"L.",
"",
"AEI, Germany"
]
] | [
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] |
711.4559 | Kurasov Victor | Victor Kurasov | Theoretical description of nucleation in multicomponent system | LATEX, 91 p | null | null | null | cond-mat.stat-mech | null | The full theoretical analysis of the kinetics of multicomponent nucleation is
presented. The relief of the free energy with surface excesses was analyzed,
the valleys and ridges were described, their mutual interaction was studied.
The new possibility to change the valley of nucleation is shown. The
possibility to have one common valley instead of several neighbor ones which
leads to the radical change in the height of the effective activation barrier
and to the new value for the nucleation rate.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:10:25 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Kurasov",
"Victor",
""
]
] | [
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] |
711.456 | Christian Heiliger | Christian Heiliger and M. D. Stiles | Ab initio studies of the spin-transfer torque in tunnel junctions | 5 pages, 4 figures | null | 10.1103/PhysRevLett.100.186805 | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | We calculate the spin-transfer torque in Fe/MgO/Fe tunnel junctions and
compare the results to those for all-metallic junctions. We show that the
spin-transfer torque is interfacial in the ferromagnetic layer to a greater
degree than in all-metallic junctions. This result originates in the half
metallic behavior of Fe for the $\Delta_1$ states at the Brillouin zone center;
in contrast to all-metallic structures, dephasing does not play an important
role. We further show that it is possible to get a component of the torque that
is out of the plane of the magnetizations and that is linear in the bias.
However, observation of such a torque requires highly ideal samples. In samples
with typical interfacial roughness, the torque is similar to that in
all-metallic multilayers, although for different reasons.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:14:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Heiliger",
"Christian",
""
],
[
"Stiles",
"M. D.",
""
]
] | [
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711.4561 | Aki Roberge | Aki Roberge and Alycia J. Weinberger | Debris Disks Around Nearby Stars with Circumstellar Gas | 10 pages including 4 figures. Accepted for publication in ApJ | Astrophys.J.676:509-517,2008 | 10.1086/527314 | null | astro-ph | null | We conducted a survey for infrared excess emission from 16 nearby main
sequence shell stars using the Multiband Imaging Photometer for Spitzer (MIPS)
on the Spitzer Space Telescope. Shell stars are early-type stars with narrow
absorption lines in their spectra that appear to arise from circumstellar (CS)
gas. Four of the 16 stars in our survey showed excess emission at 24 microns
and 70 microns characteristic of cool CS dust and are likely to be edge-on
debris disks. Including previously known disks, it appears that the fraction of
protoplanetary and debris disks among the main sequence shell stars is at least
48% +/- 14%. While dust in debris disks has been extensively studied,
relatively little is known about their gas content. In the case of Beta
Pictoris, extensive observations of gaseous species have provided insights into
the dynamics of the CS material and surprises about the composition of the CS
gas coming from young planetesimals (e.g. Roberge et al. 2006). To understand
the co-evolution of gas and dust through the terrestrial planet formation
phase, we need to study the gas in additional debris disks. The new debris disk
candidates from this Spitzer survey double the number of systems in which the
gas can be observed right now with sensitive line of sight absorption
spectroscopy.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:26:16 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Roberge",
"Aki",
""
],
[
"Weinberger",
"Alycia J.",
""
]
] | [
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] |
711.4562 | Ehud Weinsberg | Yuval Shavitt, Eran Shir, Udi Weinsberg | Near-Deterministic Inference of AS Relationships | null | null | null | null | cs.NI | null | The discovery of Autonomous Systems (ASes) interconnections and the inference
of their commercial Type-of-Relationships (ToR) has been extensively studied
during the last few years. The main motivation is to accurately calculate
AS-level paths and to provide better topological view of the Internet. An
inherent problem in current algorithms is their extensive use of heuristics.
Such heuristics incur unbounded errors which are spread over all inferred
relationships. We propose a near-deterministic algorithm for solving the ToR
inference problem. Our algorithm uses as input the Internet core, which is a
dense sub-graph of top-level ASes. We test several methods for creating such a
core and demonstrate the robustness of the algorithm to the core's size and
density, the inference period, and errors in the core.
We evaluate our algorithm using AS-level paths collected from RouteViews BGP
paths and DIMES traceroute measurements. Our proposed algorithm
deterministically infers over 95% of the approximately 58,000 AS topology
links. The inference becomes stable when using a week worth of data and as
little as 20 ASes in the core. The algorithm infers 2-3 times more peer-to-peer
relationships in edges discovered only by DIMES than in RouteViews edges,
validating the DIMES promise to discover periphery AS edges.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:20:08 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Shavitt",
"Yuval",
""
],
[
"Shir",
"Eran",
""
],
[
"Weinsberg",
"Udi",
""
]
] | [
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] |
711.4563 | Paul Hodge | O. K. Krienke and Paul W. Hodge | An HST Survey of the Disk Cluster Population of M31. II. ACS Pointings | 15 pages, 5 figures, 4 tables | null | null | null | astro-ph | null | This paper reports on a survey of star clusters in M31 based on archival
images from the Hubble Space Telescope. Paper I (Krienke and Hodge 2007)
reported results from images obtained with the Wide Field/Planetary Camera 2
(WFPC2) and this paper reports results from the Advanced Camera for Surveys
(ACS). The ACS survey has yielded a total of 339 star clusters. The color-
integrated magnitude diagram of clusters shows three significant features: (1)
a group of very red, luminous objects: the globular clusters, (2) a wide range
in color for the fainter clusters, representing a considerable range in age and
reddening, and (3) a maximum density of intermediate-age, intermediate-mass
clusters with ages close to 500 million years and masses of about 2000 solar
masses. We give a brief qualitative interpretation of the distribution of
clusters in the CMDs in terms of their formation and destruction rates.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:19:03 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Krienke",
"O. K.",
""
],
[
"Hodge",
"Paul W.",
""
]
] | [
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] |
711.4564 | Carlos A. R. Herdeiro | Carlos A. R. Herdeiro, Raquel H. Ribeiro, Marco Sampaio | Scalar Casimir Effect on a D-dimensional Einstein Static Universe | 37 pages, 15 figures, v2: minor changes in sections 1, 2.5, 3 and 4;
version published in CQG | Class.Quant.Grav.25:165010,2008 | 10.1088/0264-9381/25/16/165010 | null | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We compute the renormalised energy momentum tensor of a free scalar field
coupled to gravity on an (n+1)-dimensional Einstein Static Universe (ESU),
RxS^n, with arbitrary low energy effective operators (up to mass dimension
n+1). A generic class of regulators is used, together with the Abel-Plana
formula, leading to a manifestly regulator independent result. The general
structure of the divergences is analysed to show that all the gravitational
couplings (not just the cosmological constant) are renormalised for an
arbitrary regulator. Various commonly used methods (damping function,
point-splitting, momentum cut-off and zeta function) are shown to, effectively,
belong to the given class. The final results depend strongly on the parity of
n. A detailed analytical and numerical analysis is performed for the behaviours
of the renormalised energy density and a quantity `sigma' which determines if
the strong energy condition holds for the `quantum fluid'. We briefly discuss
the quantum fluid back-reaction problem, via the higher dimensional Friedmann
and Raychaudhuri equations, observe that equilibrium radii exist and unveil the
possibility of a `Casimir stabilisation of Einstein Static Universes'.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:26:07 GMT"
},
{
"version": "v2",
"created": "Fri, 29 Aug 2008 10:32:26 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Herdeiro",
"Carlos A. R.",
""
],
[
"Ribeiro",
"Raquel H.",
""
],
[
"Sampaio",
"Marco",
""
]
] | [
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] |
711.4565 | Marcelo Miguel Miller Bertolami | Marcelo M. Miller Bertolami, Leandro G. Althaus | The importance of the remnant's mass for VLTP born again times.
Implications for V4334 Sgr and V605 Aql | 4 Pages, 2 Figures, 1 Table. Presented at the Third Conference in
Hydrogen Deficient Stars, Tubingen, September, 2007 | Hydrogen-Deficient Stars ASP Conference Series, Vol. 391,
proceedings of the conference held 17-21 September, 2007, p.203 | null | null | astro-ph | null | We present numerical simulations of the very late thermal pulse (VLTP)
scenario for a wide range of remnant masses. We show that, by taking into
account the different possible remnant masses, the fast outburst evolution of
V4334 Sgr (a.k.a. Sakurai's Object) and V605 Aql can be reproduced within
standard 1D stellar evolution models. A dichotomy in the born again timescales
is found, with lower mass remnants evolving in a few years and higher mass
remnants (M $\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$}}}\hbox{$>$}}$ 0.6
M$_{\odot}$) failing to expand due to the H-flash and, as a consequence,
evolving in timescales typical of He-shell flash driven born agains ($\sim 100$
yr).
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:31:08 GMT"
}
] | 2008-08-27T00:00:00 | [
[
"Bertolami",
"Marcelo M. Miller",
""
],
[
"Althaus",
"Leandro G.",
""
]
] | [
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] |
711.4566 | Xiaoli Han | Xiaoli Han, Jiayu Li | The second type singularity of symplectic and Lagrangian mean curvature
flows | null | null | null | null | math.DG math.AP | null | In this paper we mainly study the type II singularities of the mean curvature
flow from a symplectic surface or from an almost calibrated Lagrangian surface
in a K \"ahler-Einstein surface. We show the relation between the maximum of
the K\"ahler angle and the maximum of $|H|^2$ on the limit flow.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:32:57 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Feb 2008 14:28:14 GMT"
}
] | 2008-02-05T00:00:00 | [
[
"Han",
"Xiaoli",
""
],
[
"Li",
"Jiayu",
""
]
] | [
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] |
711.4567 | Savely G. Karshenboim | Savely G. Karshenboim | Guide for atomic and particle physicists to CODATA's recommended values
of the fundamental physical constants | presented at PSAS'2006; to be pubslished in Lect. Not. Phys | Lect.Notes Phys.745:35-53,2008 | 10.1007/978-3-540-75479-4_15 | null | physics.atom-ph | null | The CODATA recommended values of the fundamental constants are widely applied
in particle, nuclear and atomic physics. They are a result of a complicated
evaluation (adjustment) of numerous correlated data of different nature. Their
application is often rather mechanical and as a result is not free of various
confusions which are discussed in this note.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:35:28 GMT"
}
] | 2009-01-09T00:00:00 | [
[
"Karshenboim",
"Savely G.",
""
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] |
711.4568 | Daniel Snowman | Daniel P. Snowman | Quantifying Student Effort and Class Involvement in the Introductory
Higher Education Science Classroom | null | null | null | null | physics.ed-ph | null | This note details a minimal effort program, Cash Participation, that
quantifies class participation while increasing class energy, decreasing
student apathy and removing student embraced anonymity.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:38:39 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Snowman",
"Daniel P.",
""
]
] | [
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711.4569 | Savely G. Karshenboim | Savely G. Karshenboim | Conceptual problems in phenomenological interpretation in searches for
variation of constants & violation of various invariances | null | Adv.Quant.Chem.53:237-252,2008 | 10.1016/S0065-3276(07)53012-1 | null | physics.atom-ph | null | At present a number of current or proposed experiments are directed towards a
search for a `new physics' by detecting variations of fundamental physical
constants or violations of certain basic symmetries. Various problems related
to the phenomenology of such experiments are considered here.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:43:01 GMT"
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] | 2015-05-13T00:00:00 | [
[
"Karshenboim",
"Savely G.",
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-0.0315776877,
-0.0636152402,
-0.0767470673,
-0.0237343609,
-0.0055343984
] |
711.457 | Lev I. Shekhtman | V. M. Aulchenko, P. A. Papushev, M. R. Sharafutdinov, L. I. Shekhtman,
V. M. Titov, B. P. Tolochko, V. V. Zhulanov | Development of one-coordinate gaseous detector for wide angle
diffraction studies | null | JINST3:P04008,2008 | 10.1088/1748-0221/3/04/P04008 | null | physics.ins-det | null | A one-coordinate gaseous detector of soft X-ray photons for wide-angle X-ray
scattering (WAXS) studies is being developed. The detector operates in counting
mode and is based on multi-stage Gas Electron Multiplier(GEM). Full size
detector is assembled and has 67 degrees aperture with 350mm distance to the
source, readout multi-strip structure with 2048 strips at 0.2mm pitch and is
partially equipped with readout electronics in the central part. Main
parameters of the detector have been measured with 8keV X-ray beam at VEPP-3
synchrotron ring. Spatial resolution of 470 um (FWHM) has been demonstrated
that will allow to distinguish diffraction spots at 0.1 degrees.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:43:45 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Aulchenko",
"V. M.",
""
],
[
"Papushev",
"P. A.",
""
],
[
"Sharafutdinov",
"M. R.",
""
],
[
"Shekhtman",
"L. I.",
""
],
[
"Titov",
"V. M.",
""
],
[
"Tolochko",
"B. P.",
""
],
[
"Zhulanov",
"V. V.",
""
]
] | [
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] |
711.4571 | Alexander V. Milovanov Dr. | A. V. Milovanov (Department of Physics and Technology, University of
Tromso, Tromso, Norway) K. Rypdal (Department of Physics and Technology,
University of Tromso, Tromso, Norway) J. J. Rasmussen (Optics and Plasma
Research Department, Technical University of Denmark, Riso National
Laboratory, Roskilde, Denmark) | E-pile model of self-organized criticality | 4 pages, 2 figures | null | null | null | cond-mat.stat-mech | null | The concept of percolation is combined with a self-consistent treatment of
the interaction between the dynamics on a lattice and the external drive. Such
a treatment can provide a mechanism by which the system evolves to criticality
without fine tuning, thus offering a route to self-organized criticality (SOC)
which in many cases is more natural than the weak random drive combined with
boundary loss/dissipation as used in standard sand-pile formulations. We
introduce a new metaphor, the e-pile model, and a formalism for electric
conduction in random media to compute critical exponents for such a system.
Variations of the model apply to a number of other physical problems, such as
electric plasma discharges, dielectric relaxation, and the dynamics of the
Earth's magnetotail.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 19:58:18 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Milovanov",
"A. V.",
"",
"Department of Physics and Technology, University of\n Tromso, Tromso, Norway"
],
[
"Rypdal",
"K.",
"",
"Department of Physics and Technology,\n University of Tromso, Tromso, Norway"
],
[
"Rasmussen",
"J. J.",
"",
"Optics and Plasma\n Research Department, Technical University of Denmark, Riso National\n Laboratory, Roskilde, Denmark"
]
] | [
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] |
711.4572 | Shane P. O'Sullivan | D. C. Gabuzda, V. M. Vitrishchak, M. Mahmud, S. P. O'Sullivan | Radio Circular Polarization Produced in Helical Magnetic Fields in Eight
Active Galactic Nuclei | 24 pages, 6 figures, accepted for publication in Monthly Notices of
the Royal Astronomical Society (MNRAS) | null | 10.1111/j.1365-2966.2007.12773.x | null | astro-ph | null | Homan & Lister (2006) have recently published circular-polarization (CP)
detections for 34 objects in the MOJAVE sample - a set of bright, compact AGN
being monitored by the Very Long Baseline Array at 15 GHz. We report the
detection of 15-GHz parsec-scale CP in two more AGN (3C345 and 2231+114), and
confirm the MOJAVE detection of CP in 1633+382. It is generally believed that
the most likely mechanism for the generation of this CP is Faraday conversion
of linear polarization to CP. A helical jet magnetic-field (B-field) geometry
can facilitate this process - linearly polarized emission from the far side of
the jet is converted to CP as it passes through the magnetised plasma at the
front side of the jet on its way toward the observer. In this case, the sign of
the generated CP is essentially determined by the pitch angle and helicity of
the helical B field. We have determined the pitch-angle regimes and helicities
of the helical jet B fields in 8 AGN for which parsec-scale CP has been
detected, and used them to predict the expected CP signs for these AGN if the
CP is generated via conversion in these helical fields. We have obtained the
intriguing result that our predictions agree with the observed signs in all
eight cases, provided that the longitudinal B-field components in the jets
correspond to South magnetic poles. This clearly non-random pattern
demonstrates that the observed CP in AGN is directly associated with the
presence of helical jet B fields. These results suggest that helical B fields
are ubiquitous in AGN jets.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:04:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gabuzda",
"D. C.",
""
],
[
"Vitrishchak",
"V. M.",
""
],
[
"Mahmud",
"M.",
""
],
[
"O'Sullivan",
"S. P.",
""
]
] | [
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] |
711.4573 | Mathieu Raffinot | Pierre Charbit (LIAFA), Michel Habib (LIAFA), Vincent Limouzy (LIAFA),
Fabien De Montgolfier (LIAFA), Mathieu Raffinot (LIAFA), Micha\"el Rao
(LIRMM) | A Note On Computing Set Overlap Classes | null | null | null | null | cs.DS | null | Let ${\cal V}$ be a finite set of $n$ elements and ${\cal F}=\{X_1,X_2, >...,
X_m\}$ a family of $m$ subsets of ${\cal V}.$ Two sets $X_i$ and $X_j$ of
${\cal F}$ overlap if $X_i \cap X_j \neq \emptyset,$ $X_j \setminus X_i \neq
\emptyset,$ and $X_i \setminus X_j \neq \emptyset.$ Two sets $X,Y\in {\cal F}$
are in the same overlap class if there is a series $X=X_1,X_2, ..., X_k=Y$ of
sets of ${\cal F}$ in which each $X_iX_{i+1}$ overlaps. In this note, we focus
on efficiently identifying all overlap classes in $O(n+\sum_{i=1}^m |X_i|)$
time. We thus revisit the clever algorithm of Dahlhaus of which we give a clear
presentation and that we simplify to make it practical and implementable in its
real worst case complexity. An useful variant of Dahlhaus's approach is also
explained.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:07:46 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Charbit",
"Pierre",
"",
"LIAFA"
],
[
"Habib",
"Michel",
"",
"LIAFA"
],
[
"Limouzy",
"Vincent",
"",
"LIAFA"
],
[
"De Montgolfier",
"Fabien",
"",
"LIAFA"
],
[
"Raffinot",
"Mathieu",
"",
"LIAFA"
],
[
"Rao",
"Michaël",
"",
"LIRMM"
]
] | [
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] |
711.4574 | Anthony Randriamampianina | Anthony Randriamampianina (IRPHE), Pierre Maubert (IRPHE), Wolf-Gerrit
Fruh (SEPS), Peter L. Read (AOPP) | Direct Numerical Simulation of structural vacillation in the transition
to geostrophic turbulence | 6 pages | Dans Stratified and Rotating Flows Symposium, Congres Francais de
Mecanique - Congres Francais de Mecanique, Grenoble : France (2007) | null | null | physics.geo-ph nlin.CD | null | The onset of small-scale fluctuations around a steady convection pattern in a
rotating baroclinic annulus filled with air is investigated using Direct
Numerical Simulation. In previous laboratory experiments of baroclinic waves,
such fluctuations have been associated with a flow regime termed Structural
Vacillation which is regarded as the first step in the transition to
fully-developed geostrophic turbulence.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:08:49 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Randriamampianina",
"Anthony",
"",
"IRPHE"
],
[
"Maubert",
"Pierre",
"",
"IRPHE"
],
[
"Fruh",
"Wolf-Gerrit",
"",
"SEPS"
],
[
"Read",
"Peter L.",
"",
"AOPP"
]
] | [
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] |
711.4575 | G. Bourda | G. Bourda (SYRTE), N. Capitaine (SYRTE) | Precession, nutation, and space geodetic determination of the Earth's
variable gravity field | null | Astron.Astrophys.428:691-702,2004 | 10.1051/0004-6361:20041533 | null | astro-ph physics.space-ph | null | Precession and nutation of the Earth depend on the Earth's dynamical
flattening, H, which is closely related to the second degree zonal coefficient,
J2 of the geopotential. A small secular decrease as well as seasonal variations
of this coefficient have been detected by precise measurements of artificial
satellites (Nerem et al. 1993; Cazenave et al. 1995) which have to be taken
into account for modelling precession and nutation at a microarcsecond accuracy
in order to be in agreement with the accuracy of current VLBI determinations of
the Earth orientation parameters. However, the large uncertainties in the
theoretical models for these J2 variations (for example a recent change in the
observed secular trend) is one of the most important causes of why the accuracy
of the precession-nutation models is limited (Williams 1994; Capitaine et al.
2003). We have investigated in this paper how the use of the variations of J2
observed by space geodetic techniques can influence the theoretical expressions
for precession and nutation. We have used time series of J2 obtained by the
"Groupe de Recherches en G\'eod\'esie spatiale" (GRGS) from the precise orbit
determination of several artificial satellites from 1985 to 2002 to evaluate
the effect of the corresponding constant, secular and periodic parts of H and
we have discussed the best way of taking the observed variations into account.
We have concluded that, although a realistic estimation of the J2 rate must
rely not only on space geodetic observations over a limited period but also on
other kinds of observations, the monitoring of periodic variations in J2 could
be used for predicting the effects on the periodic part of the
precession-nutation motion.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:09:39 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Bourda",
"G.",
"",
"SYRTE"
],
[
"Capitaine",
"N.",
"",
"SYRTE"
]
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] |
711.4576 | Michel Destrade | Michel Destrade (LMM) | Seismic Rayleigh waves on an exponentially graded, orthotropic
half-space | 8 pages | Proceedings of the Royal Society of London A463 (2007) 495-502 | 10.1098/rspa.2006.1774 | null | physics.geo-ph | null | Efforts at modelling the propagation of seismic waves in half-spaces with
continuously varying properties have been mostly focused on shear-horizontal
waves. Here a sagittaly polarized (Rayleigh type) wave travels along a symmetry
axis (and is attenuated along another) of an orthotropic material with
stiffnesses and mass density varying in the same exponential manner with depth.
Contrary to what could be expected at first sight, the analysis is very similar
to that of the homogeneous half-space, with the main and capital difference
that the Rayleigh wave is now dispersive. The results are illustrated
numerically for (i) an orthotropic half-space typical of horizontally layered
and vertically fractured shales and (ii) for an isotropic half-space made of
silica. In both examples, the wave travels at a slower speed and penetrates
deeper than in the homogeneous case; in the second example, the inhomogeneity
can force the wave amplitude to oscillate as well as decay with depth, in
marked contrast with the homogeneous isotropic general case.
| [
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711.4577 | G. Bourda | G. Bourda (SYRTE) | Gravitational potential, inertia and Earth rotation | null | Dans Journ\'ees 2002 - syst\`emes de r\'ef\'erence
spatio-temporels. - Astrometry from ground and from space, Bucarest :
Roumanie (2002) | null | null | astro-ph physics.space-ph | null | Several satellite missions, devoted to the study of the Earth gravity field,
have been launched (like CHAMP, recently). This year, GRACE (Gravity Recovery
and Climate Experiment) will allow us to obtain a more precise geoid. But the
most important is that they will supply the temporal variations of the
geopotential coefficients (called Stokes coefficients). In the poster we show
how the Earth gravitational potential is linked to the Earth rotation
parameters. Indeed, through the Earth inertia coefficients, we can connect the
variation of LOD and Polar Motion with the temporal variations of the Stokes
coefficients. We also consider the nutations, that are related to the
gravitational geopotential coefficients. We discuss the possibility of using
the Stokes coefficients in order to improve our knowledge of the Earth
rotation.
| [
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"version": "v1",
"created": "Wed, 28 Nov 2007 20:10:33 GMT"
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711.4578 | Cristinel Diaconu | H1 Collaboration | Measurement of Isolated Photon Production in Deep-Inelastic Scattering
at HERA | 32 pages, 10 figures | Eur.Phys.J.C54:371-387,2008 | 10.1140/epjc/s10052-008-0541-6 | DESY 07-147 | hep-ex | null | The production of isolated photons in deep-inelastic scattering $ep\to e
\gamma X$ is measured with the H1 detector at HERA. The measurement is
performed in the kinematic range of negative four-momentum transfer squared
$4<Q^2<150 $~GeV$^2$ and a mass of the hadronic system $W_X>50$ GeV. The
analysis is based on a total integrated luminosity of 227~pb$^{-1}$. The
production cross section of isolatedphotons with a transverse energy in the
range $3 < E_T^\gamma < 10$ GeV and pseudorapidity range $-1.2 < \eta^\gamma <
1.8$ is measured as a function of $E_T^\gamma$, $\eta^\gamma$ and $Q^2$.
Isolated photon cross sections are also measured for events with no jets or at
least one hadronic jet. The measurements are compared with predictions from
Monte Carlo generators modelling the photon radiation from the quark and the
electron lines, as well as with calculations at leading and next to leading
order in the strong coupling. The predictions significantly underestimate the
measured cross sections.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:31:59 GMT"
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] | 2012-08-27T00:00:00 | [
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] |
711.4579 | G. Bourda | G. Bourda (SYRTE), N. Capitaine (SYRTE) | Temporal variations of the gravity field and Earth precession-nutation | null | Dans Journ\'ees 2003 - Syst\`emes de r\'ef\'erence
spatio-temporels. - Astrometry, geodynamics and solar system dynamics: from
milliarseconds to microarcseconds, St. Petersburg : Russie (2003) | null | null | astro-ph physics.space-ph | null | Due to the accuracy now reached by space geodetic techniques, and also
considering some modelisations, the temporal variations of some Earth Gravity
Field coefficients can be determined. They are due to Earth oceanic and solid
tides, as well as geophysical reservoirs masses displacements. They can be
related to the variations in the Earth's orientation parameters (through the
inertia tensor). Then, we can try to improve our knowledge of the Earth
Rotation with those space measurements of the Gravity variations. We have
undertaken such a study, using data obtained with the combination of space
geodetic techniques. In particular, we use CHAMP data that are more sensitive
to such variations and that complete the ones already accumulated (for example
with Starlette and LAGEOS I). In this first approach, we focus on the Earth
precession nutation, trying to refine it by taking into account the temporal
variations of the Earth dynamical flattening. The goal is mainly to understand
how Geodesy can influence this field of science. Like this, we will be able to
compare our computation with up to date determinations of precession nutation.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:11:46 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Bourda",
"G.",
"",
"SYRTE"
],
[
"Capitaine",
"N.",
"",
"SYRTE"
]
] | [
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] |
711.458 | Sebastian Volz | Guillaume Galli\'ero (TEFC, Trefle), S. Volz (EM2C) | Thermodiffusion in model nanofluids by molecular dynamics simulations | null | null | 10.1063/1.2834545 | null | cond-mat.stat-mech | null | In this work, a new algorithm is proposed to compute single particle
(infinite dilution) thermodiffusion using Non-Equilibrium Molecular Dynamics
simulations through the estimation of the thermophoretic force that applies on
a solute particle. This scheme is shown to provide consistent results for
simple Lennard-Jones fluids and for model nanofluids (spherical non-metallic
nanoparticles + Lennard-Jones fluid) where it appears that thermodiffusion
amplitude, as well as thermal conductivity, decrease with nanoparticles
concentration. Then, in nanofluids in the liquid state, by changing the nature
of the nanoparticle (size, mass and internal stiffness) and of the solvent
(quality and viscosity) various trends are exhibited. In all cases the single
particle thermodiffusion is positive, i.e. the nanoparticle tends to migrate
toward the cold area. The single particle thermal diffusion 2 coefficient is
shown to be independent of the size of the nanoparticle (diameter of 0.8 to 4
nm), whereas it increases with the quality of the solvent and is inversely
proportional to the viscosity of the fluid. In addition, this coefficient is
shown to be independent of the mass of the nanoparticle and to increase with
the stiffness of the nanoparticle internal bonds. Besides, for these
configurations, the mass diffusion coefficient behavior appears to be
consistent with a Stokes-Einstein like law.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:12:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Galliéro",
"Guillaume",
"",
"TEFC, Trefle"
],
[
"Volz",
"S.",
"",
"EM2C"
]
] | [
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-0.0235214084,
0.0270509068,
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] |
711.4581 | G. Bourda | G. Bourda (SYRTE, Igg) | Length of day and polar motion, with respect to temporal variations of
the Earth gravity field | null | Dans SF2A-2005: Semaine de l'Astrophysique Francaise - SF2A-2005:
Semaine de l'Astrophysique Francaise, Strasbourg : France (2005) | null | null | astro-ph physics.space-ph | null | The masses distribution inside the Earth governs the behaviour of the
rotation axis in the Earth (polar motion), as well as the Earth rotation rate
(or equivalently, length of day). This masses distribution can be measured from
space owing to artificial satellites, the orbitography of which provides the
Earth gravity field determination. Then, the temporal variations of the Earth
gravity field can be related to the variations of the Earth Orientation
Parameters (EOP) (with the Inertia Tensor). Nowadays, owing to the satellite
laser ranging (SLR) technique and to the new gravimetric satellite missions
(such as CHAMP or GRACE), the temporal variations of the low degree
coefficients of the Earth gravity field (i.e. Stokes coefficients) can be
determined. This paper is one of the first study using gravity variations data
in the equations already established (e.g. Lambeck 1988) and linking the
variations of the length of day and of the C20 Stokes coefficient (or, linking
the polar motion and the C21 and S21 coefficients). This paper combines the
Earth rotation data (mainly obtained from VLBI and GPS measurements) and the
Earth gravity field variations ones (e.g. Lageos I and II data, or GRACE data),
in order to complete and constrain the models of the Earth rotation. The final
goal is a better Earth global dynamics understanding, which possible
application can be the constraint on the couplings into the Earth system (e.g.
core-mantle couplings).
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:17:50 GMT"
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] | 2007-11-29T00:00:00 | [
[
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711.4582 | G. Bourda | G. Bourda (SYRTE) | Earth rotation and variations of the gravity field, in the framework of
the "Descartes-nutation" project | null | Dans Journ\'ees 2004 - syst\`emes de r\'ef\'erence
spatio-temporels. - Fundamental astronomy: new concepts and models for high
accuracy observations, Paris : France (2004) | null | null | astro-ph physics.space-ph | null | The "Descartes-Nutation" Project is devoted to the "understanding of the next
decimal of precession-nutation, from the theoretical point of view as well as
from the observational point of view". In this framework, we made a proposal in
order to contribute to the study of (i) the dynamical flattening of the Earth,
(ii) the coupling effects of the lunisolar forcing, (iii) the effect of the
geophysical fluids on the EOP and (iv) the Nutation observations. We
investigate further the links between Earth Orientation and Gravity Field
Variations. Indeed, the masses distributions inside the Earth govern the
behaviour of the rotation axis in space (precession-nutation) and in the Earth
(polar motion), as well as the Earth rotation rate (or equivalently, length of
the day). These distributions of masses can be measured by space owing to
artificial satellites, the orbitography of which provides the Earth gravity
field determination. Then, the temporal variations of the Earth gravity field
can be related to the variations of the Earth Orientation Parameters (EOP)
(with the Inertia Tensor). Nowadays, the Earth orientation measurements in
space, obtained with Very Long Baseline Interferometry (VLBI), have a precision
better than the milliarcsecond level. It is then necessary to consider all the
geophysical sources that can improve the models precision. The goal of my PhD
Thesis was to use the Earth gravity field measurements, as well as its
variations, as a tool to improve the Earth orientation modelisation. We present
here the results obtained as well as various proposals to extend these
investigations (numerical studies, the use of J2 geophysical series,
integration of GRACE data ...).
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:20:00 GMT"
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711.4583 | Paolo Privitera | M. Ave, et al. (for the AIRFLY Collaboration) | Temperature and Humidity Dependence of Air Fluorescence Yield measured
by AIRFLY | presented at the 5th Fluorescence Workshop, El Escorial - Madrid,
Spain, 16 - 20 September 2007, to appear in Nuclear Instruments and Methods A | Nucl.Instrum.Meth.A597:50-54,2008 | 10.1016/j.nima.2008.08.050 | null | astro-ph | null | The fluorescence detection of ultra high energy cosmic rays requires a
detailed knowledge of the fluorescence light emission from nitrogen molecules
over a wide range of atmospheric parameters, corresponding to altitudes typical
of the cosmic ray shower development in the atmosphere. We have studied the
temperature and humidity dependence of the fluorescence light spectrum excited
by MeV electrons in air. Results for the 313.6 nm, 337.1 nm, 353.7 nm and 391.4
nm bands are reported in this paper. We found that the temperature and humidity
dependence of the quenching process changes the fluorescence yield by a
sizeable amount (up to 20%) and its effect must be included for a precise
estimation of the energy of ultra high energy cosmic rays.
| [
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] |
711.4584 | G. Bourda | G. Bourda (SYRTE) | Earth Orientation and Temporal Variations of the Gravity Field | null | Dans SF2A-2004: Semaine de l'Astrophysique Francaise - SF2A-2004:
Semaine de l'Astrophysique Francaise, Paris : France (2004) | null | null | astro-ph physics.space-ph | null | The high accuracy now reached in the VLBI Earth Orientation Parameters (EOP)
determination requires looking further at the various geophysical contributions
to variations in EOP. The determination of the Earth gravity field from space
geodetic techniques now allows us to obtain the temporal variations of the low
degree coefficients of the geopotential, combining the treatment of different
satellites (e.g. Lageos1, Lageos2, Starlette ...). We present a new computation
of the degree 2 coefficients of the variable Earth gravity field. This study is
based upon the using of (i) new orbit standards, (ii) the GRACE mean gravity
field and (iii) Lageos1 data from 1985 until 2004 (merged with Lageos2 data
from 1993). These temporal variations of the Earth gravity field can be related
to the Earth Orientation Parameters through the inertia tensor. This paper
shows these relations and discusses how such geodetic data can contribute to
the understanding of the variations in EOP. This paper also studies if these
refined 20-yr of Lageos data can give us refined value of the 18.6-yr tidal
term, as well as of the secular drift of the C20 geopotential coefficient.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:21:10 GMT"
}
] | 2007-11-29T00:00:00 | [
[
"Bourda",
"G.",
"",
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711.4585 | Eduardo G. Altmann | E. G. Altmann, T. Friedrich, A. E. Motter, H. Kantz, and A. Richter | Prevalence of marginally unstable periodic orbits in chaotic billiards | 6 pages, 5 figures | Phys. Rev. E 77, 016205 (2008) | 10.1103/PhysRevE.77.016205 | null | nlin.CD quant-ph | null | The dynamics of chaotic billiards is significantly influenced by coexisting
regions of regular motion. Here we investigate the prevalence of a different
fundamental structure, which is formed by marginally unstable periodic orbits
and stands apart from the regular regions. We show that these structures both
{\it exist} and {\it strongly influence} the dynamics of locally perturbed
billiards, which include a large class of widely studied systems. We
demonstrate the impact of these structures in the quantum regime using
microwave experiments in annular billiards.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 20:32:50 GMT"
}
] | 2008-01-24T00:00:00 | [
[
"Altmann",
"E. G.",
""
],
[
"Friedrich",
"T.",
""
],
[
"Motter",
"A. E.",
""
],
[
"Kantz",
"H.",
""
],
[
"Richter",
"A.",
""
]
] | [
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] |
711.4586 | Nicholas Ingle | N.J.C. Ingle and I.S. Elfimov | Epitaxial influence on the ferromagnetic semiconducotor EuO | null | Physical Review B, 77, 121202R (2008) | 10.1103/PhysRevB.77.121202 | null | cond-mat.str-el cond-mat.mtrl-sci | null | From first principles calculations we investigate the electronic structure
and the magnetic properties of EuO under hydrostatic and epitaxial forces.
There is a complex interdependence of the O 2p and Eu 4f and 5d bands on the
magnetism in EuO, and decreasing lattice parameters is an ideal method to
increase the Curie temperature, T_c. Compared to hydrostatic pressure, the
out-of-plane compensation that is available to epitaxial films influences this
increase in T_c, although it is minimized by the small value of poisson's ratio
for EuO. We find the semiconducting gap closes at a 6% in-plane lattice
compression for epitaxy, at which point a significant conceptual change must
occur in the active exchange mechanisms.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:39:33 GMT"
}
] | 2008-03-08T00:00:00 | [
[
"Ingle",
"N. J. C.",
""
],
[
"Elfimov",
"I. S.",
""
]
] | [
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] |
711.4587 | Priya Natarajan | Priyamvada Natarajan, Jean-Paul Kneib, Ian Smail, Tommaso Treu,
Richard Ellis, Sean Moran, Marceau Limousin and Oliver Czoske | The survival of dark matter halos in the cluster Cl0024+16 | 35 pages, 7 figures, revised version, accepted by ApJ | Astrophys.J.693:970-983,2009 | 10.1088/0004-637X/693/1/970 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Theories of structure formation in a cold dark matter dominated
Universe predict that massive clusters of galaxies assemble from the
hierarchical merging of lower mass subhalos. Exploiting strong and weak
gravitational lensing signals inferred from panoramic HST imaging data, we
present a high resolution reconstruction of the mass distribution in the
massive, lensing cluster Cl0024+16. Applying galaxy-galaxy lensing techniques
we track the fate of dark matter subhalos as a function of projected
cluster-centric radius out to 5 Mpc, well beyond the virial radius. We report
the first detection of the statistical lensing signal of dark matter subhalos
associated with late-type galaxies in clusters. The mass of a typical dark
matter subhalo that hosts an L* galaxy increases with projected cluster-centric
radius in line with expectations from the tidal stripping hypothesis.
Early-type galaxies appear to be hosted on average in more massive dark matter
subhalos compared to late-type galaxies. We interpret our findings as evidence
for the active assembly of mass via tidal stripping in galaxy clusters. The
mass function of dark matter subhalos as a function of projected
cluster-centric radius, is compared with an equivalent mass function derived
from clusters in the Millenium Run simulation populated with galaxies using
semi-analytic models. The shape of the lensing determined mass functions are in
very good agreement with the subhalo mass functions derived from the Millenium
Run simulation. However, simulated subhalos appear to be more efficiently
stripped than lensing observations suggest. (Abridged)
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:03:15 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Nov 2008 15:05:55 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Natarajan",
"Priyamvada",
""
],
[
"Kneib",
"Jean-Paul",
""
],
[
"Smail",
"Ian",
""
],
[
"Treu",
"Tommaso",
""
],
[
"Ellis",
"Richard",
""
],
[
"Moran",
"Sean",
""
],
[
"Limousin",
"Marceau",
""
],
[
"Czoske",
"Oliver",
""
]
] | [
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] |
711.4588 | Andreas Koch | A. Koch, R.M. Rich, D.B. Reitzel, N.F. Martin, R.A. Ibata, S.C.
Chapman, S.R. Majewski, M. Mori, Y.-S. Loh, J.C. Ostheimer, M. Tanaka | Kinematic and Chemical constraints on the formation of M31's inner and
outer halo | 35 pages, 20 figures, accpted to the Astrophysical Journal, revised
after referee's comments | null | null | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The halo of M31 shows a wealth of substructures that are consistent with
satellite accretion. Here we report on kinematic and abundance results from
Keck/DEIMOS spectroscopy in the calcium triplet region of over 3500 red giant
star candidates along the minor axis and in off-axis spheroid fields of M31.
Our data reach out to large radial distances of 160 kpc. The derived velocity
distributions show a kinematically cold substructure at 17 kpc that has been
reported before. We devise an improved method to measure accurate metallicities
from the calcium triplet in low signal-to-noise spectra using a coaddition of
the individual lines. The resulting distribution leads us to note an even
stronger gradient in the abundance distribution along M31's minor axis than
previously detected. The mean metallicity in the outer halo reaches below -2
dex, with individual values as low as -2.6 dex. In the inner spheroid, at 17-19
kpc, we find a sharp decline of ~0.5 dex in metallicity, which roughly
coincides with the edge of an extended disk, previously detected from star
count maps. A large fraction of red giants in the most distant fields are
likely members of M33's overlapping halo. A comparison of our velocities with
those predicted by new N-body simulations argues that the event responsible for
the giant Stream is most likely not responsible for the full population of the
inner halo; we show further that the abundance distribution of the Stream is
different from that of the inner halo, from which it becomes evident that the
merger event that formed the outer halo cannot have contributed any significant
material to the inner spheroid. All this evidence of severe structure changes
in the halo suggests a high degree of infall and stochastic abundance accretion
governing the build-up of M31's halo. (Abridged)
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:01:07 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Aug 2008 17:23:49 GMT"
}
] | 2008-08-05T00:00:00 | [
[
"Koch",
"A.",
""
],
[
"Rich",
"R. M.",
""
],
[
"Reitzel",
"D. B.",
""
],
[
"Martin",
"N. F.",
""
],
[
"Ibata",
"R. A.",
""
],
[
"Chapman",
"S. C.",
""
],
[
"Majewski",
"S. R.",
""
],
[
"Mori",
"M.",
""
],
[
"Loh",
"Y. -S.",
""
],
[
"Ostheimer",
"J. C.",
""
],
[
"Tanaka",
"M.",
""
]
] | [
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711.4589 | Andreas Koch | Masao Mori (Senshu University), R. Michael Rich (UCLA) | The Once and Future Andromeda Stream | 5 pages, 4 figures, accepted for publication in ApJL; see
http://www.isc.senshu-u.ac.jp/~thj0613/M31/M31.html for high-resolution
figures and movie | null | 10.1086/529140 | null | astro-ph | null | The interaction between an accreting satellite and the Andromeda galaxy (M31)
has been studied analytically and numerically, using a high-resolution N-body
simulation with $4\times10^7$ particles. For the first time, we show the
self-gravitating response of the disk, the bulge, and the dark matter halo of
M31 to an accreting satellite. We reproduce the Stream and the shells at the
East and West side of M31, by following the evolution of the collision 4 Gyr
into the future, and show that recently discovered diffuse arcs on the south
side of the minor axis are the remnants of a similar collision that occurred
3-4 Gyr earlier than the Stream event. The present day integrity of the M31
disk constrains the satellite mass to be $M \leq 5\times10^9 M_\odot$. The
stars that were originally in the center of the satellite are now in the east
shell. Therefore, observations in this region might reveal additional clues
about the nature of satellite, such as the central core and any metallicity
gradient.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:08:10 GMT"
},
{
"version": "v2",
"created": "Sat, 1 Dec 2007 16:17:30 GMT"
},
{
"version": "v3",
"created": "Sat, 12 Jan 2008 09:26:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mori",
"Masao",
"",
"Senshu University"
],
[
"Rich",
"R. Michael",
"",
"UCLA"
]
] | [
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711.459 | Sarbani Basu | Sarbani Basu (Yale University), H.M. Antia (Tata Institute, Mumbai) | Helioseismology and Solar Abundances | To appear in Physics Reports. Large file (1.6M PDF, 3.4M PS), 27
figures | Phys.Rept.457:217-283,2008 | 10.1016/j.physrep.2007.12.002 | null | astro-ph | null | Helioseismology has allowed us to study the structure of the Sun in
unprecedented detail. One of the triumphs of the theory of stellar evolution
was that helioseismic studies had shown that the structure of solar models is
very similar to that of the Sun. However, this agreement has been spoiled by
recent revisions of the solar heavy-element abundances. Heavy element
abundances determine the opacity of the stellar material and hence, are an
important input to stellar model calculations. The models with the new, low
abundances do not satisfy helioseismic constraints. We review here how
heavy-element abundances affect solar models, how these models are tested with
helioseismology, and the impact of the new abundances on standard solar models.
We also discuss the attempts made to improve the agreement of the low-abundance
models with the Sun and discuss how helioseismology is being used to determine
the solar heavy-element abundance. A review of current literature shows that
attempts to improve agreement between solar models with low heavy-element
abundances and seismic inference have been unsuccessful so far. The
low-metallicity models that have the least disagreement with seismic data
require changing all input physics to stellar models beyond their acceptable
ranges. Seismic determinations of the solar heavy-element abundance yield
results that are consistent with the older, higher values of the solar
abundance, and hence, no major changes to the inputs to solar models are
required to make higher-metallicity solar models consistent with helioseismic
data.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:02:54 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Basu",
"Sarbani",
"",
"Yale University"
],
[
"Antia",
"H. M.",
"",
"Tata Institute, Mumbai"
]
] | [
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] |
711.4591 | Pran Nath | Daniel Feldman, Zuowei Liu and Pran Nath | Light Higgses at the Tevatron and at the LHC and Observable Dark Matter
in SUGRA and D Branes | Refs. added in V2, Published in Physics Letters B | Phys.Lett.B662:190-198,2008 | 10.1016/j.physletb.2008.02.063 | null | hep-ph astro-ph | null | Sparticle landscapes in mSUGRA, in SUGRA models with nonuniversalities
(NUSUGRA), and in D brane models are analyzed. The analysis exhibits the
existence of Higgs Mass Patterns (HPs) (for $\mu>0$) where the CP odd Higgs
could be the next heavier particle beyond the LSP and sometimes even lighter
than the LSP. It is shown that the Higgs production cross sections from the HPs
are typically the largest enhancing the prospects for their detection at the
LHC. Indeed it is seen that the recent Higgs production limits from CDF/D\O\
are beginning to put constraints on the HPs. It is also seen that the $B_s\to
\mu^+\mu^-$ limits constrain the HPs more stringently. Predictions of the Higgs
production cross sections for these patterns at the LHC are made. We compute
the neutralino-proton cross sections $\sigma (\chi p)$ for dark matter
experiments and show that the largest $\sigma (\chi p)$ also arise from the HPs
and further that the HPs and some of the other patterns are beginning to be
constrained by the most recent data from CDMS and from Xenon10 experiments.
Finally, it is shown that the prospects are bright for the discovery of dark
matter with $\sigma(\chi p)$ in the range $10^{-44\pm .5}$cm$^2$ due to a
"Wall" consisting of a copious number of parameter points in the Chargino
Patterns (CPs) where the chargino is the NLSP. The Wall, which appears in all
models considered (mSUGRA, NUSUGRA and D branes) and runs up to about a TeV in
LSP mass, significantly enhances the chances for the observation of dark matter
by SuperCDMS, ZEPLIN-MAX, or LUX experiments which are expected to achieve a
sensitivity of $10^{-45}$ cm$^2$ or more.
| [
{
"version": "v1",
"created": "Thu, 29 Nov 2007 19:32:13 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 20:29:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Feldman",
"Daniel",
""
],
[
"Liu",
"Zuowei",
""
],
[
"Nath",
"Pran",
""
]
] | [
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] |
711.4592 | Xiaodong Wang | Xiaodong Wang | Harmonic Functions, Entropy, and a Characterization of the Hyperbolic
Space | to appear in J. Geom. Anal | null | null | null | math.DG | null | Let $(M^{n},g)$ be a compact Riemannian manifold with $Ric\geq-(n-1) $. It is
well known that the bottom of spectrum $\lambda_{0}$ of its unverversal
covering satisfies $\lambda_{0}\leq(n-1) ^{2}/4 $. We prove that equality holds
iff $M$ is hyperbolic. This follows from a sharp estimate for the Kaimanovich
entropy.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:07:09 GMT"
}
] | 2007-11-30T00:00:00 | [
[
"Wang",
"Xiaodong",
""
]
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] |
711.4593 | T. L. Trueman | T.L. Trueman | Spin asymmetries for elastic proton scattering and the spin dependent
couplings of the Pomeron | final reference modifed | Phys.Rev.D77:054005,2008 | 10.1103/PhysRevD.77.054005 | BNL-HET-07/14 | hep-ph nucl-ex | null | This paper serves as a report on the large amount of analysis done in
conjunction with the polarized proton program at RHIC. This comprises elastic
scattering data of protons on protons in colliding beam or fixed target mode
and proton beams on carbon targets. In addition to providing a model for the
energy dependence of the analyzing power of elastic scattering needed for
proton polarimetry, it also provides some significant information about the
spin dependence of dominant Regge poles. Most notably, the data indicates that
the Pomeron has a significant spin-flip coupling. This allows the exploration
of the double spin flip asymmetry A_{NN} for which some data over a wide energy
range is now available, along with a concrete realization of a proposed Odderon
search.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:07:45 GMT"
},
{
"version": "v2",
"created": "Mon, 10 Dec 2007 17:02:11 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Trueman",
"T. L.",
""
]
] | [
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] |
711.4594 | Khandker Quader | R. Liao, F. Popescu, K. Quader | P-wave Pairing in Two-Component Fermi Systems with Unequal Population
near Feshbach Resonance | 5 pages, 3 figures | Phys. Rev. B 88, 134507 (2013) | 10.1103/PhysRevB.88.134507 | null | cond-mat.supr-con cond-mat.other | null | We explore p-wave pairing in a single-channel two-component Fermi system with
unequal population near Feshbach resonance. Our analytical and numerical study
reveal a rich superfluid (SF) ground state structure as a function of
imbalance. In addition to the state $\Delta_{\pm 1} \propto Y_{1\pm 1}$, a
multitude of ``mixed'' SF states formed of linear combinations of $Y_{1m}$'s
give global energy minimum under a phase stability condition; these states
exhibit variation in energy with the relative phase between the constituent gap
amplitudes. States with local energy minimum are also obtained. We provide a
geometric representation of the states. A $T$=0 polarization vs. p-wave
coupling phase diagram is constructed across the BEC-BCS regimes. With
increased polarization, the global minimum SF state may undergo a quantum phase
transition to the local minimum SF state.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:08:20 GMT"
}
] | 2015-09-01T00:00:00 | [
[
"Liao",
"R.",
""
],
[
"Popescu",
"F.",
""
],
[
"Quader",
"K.",
""
]
] | [
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] |
711.4595 | Xiaodong Wang | Fengbo Hang, Xiaodong Wang | A Rigidity Theorem for the Hemisphere | The extrinsic boundary condition is relaxed | null | null | null | math.DG | null | We prove the following rigidity theorem: For an n-dimensional compact
Riemannian manifold with boundary whose Ricci curvature is bounded by n-1 from
below, if its boundary is isometric to the standard sphere of dimension n-1 and
totally geodesic, then the manifold is isometric to the standard hemisphere.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:18:09 GMT"
},
{
"version": "v2",
"created": "Mon, 3 Dec 2007 18:33:16 GMT"
}
] | 2007-12-03T00:00:00 | [
[
"Hang",
"Fengbo",
""
],
[
"Wang",
"Xiaodong",
""
]
] | [
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] |
711.4596 | Gabriele La Spada | Gabriele La Spada, J. Doyne Farmer and Fabrizio Lillo | The non-random walk of stock prices: The long-term correlation between
signs and sizes | 9 pages, 5 figures, StatPhys23 | null | 10.1140/epjb/e2008-00244-4 | null | q-fin.ST physics.soc-ph | null | We investigate the random walk of prices by developing a simple model
relating the properties of the signs and absolute values of individual price
changes to the diffusion rate (volatility) of prices at longer time scales. We
show that this benchmark model is unable to reproduce the diffusion properties
of real prices. Specifically, we find that for one hour intervals this model
consistently over-predicts the volatility of real price series by about 70%,
and that this effect becomes stronger as the length of the intervals increases.
By selectively shuffling some components of the data while preserving others we
are able to show that this discrepancy is caused by a subtle but long-range
non-contemporaneous correlation between the signs and sizes of individual
returns. We conjecture that this is related to the long-memory of transaction
signs and the need to enforce market efficiency.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:58:46 GMT"
},
{
"version": "v2",
"created": "Mon, 5 May 2008 14:45:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"La Spada",
"Gabriele",
""
],
[
"Farmer",
"J. Doyne",
""
],
[
"Lillo",
"Fabrizio",
""
]
] | [
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] |
711.4597 | Derrick Hart | Derrick Hart, Alex Iosevich | Pinned distance sets, Wolff's exponent in finite fields and improved
sum-product estimates | null | null | null | null | math.CA math.CO | null | An analog of the Falconer distance problem in vector spaces over finite
fields asks for the threshold $\alpha>0$ such that $|\Delta(E)| \gtrsim q$
whenever $|E| \gtrsim q^{\alpha}$, where $E \subset {\Bbb F}_q^d$, the
$d$-dimensional vector space over a finite field with $q$ elements (not
necessarily prime). Here $\Delta(E)=\{{(x_1-y_1)}^2+...+{(x_d-y_d)}^2: x,y \in
E\}$. The second listed author and Misha Rudnev established the threshold
$\frac{d+1}{2}$, and the authors of this paper, Doowon Koh and Misha Rudnev
proved that this exponent is sharp in even dimensions. In this paper we improve
the threshold to $\frac{d^2}{2d-1}$ under the additional assumption that $E$
has product structure. In particular, we obtain the exponent 4/3, consistent
with the corresponding exponent in Euclidean space obtained by Wolff.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:24:05 GMT"
}
] | 2007-11-30T00:00:00 | [
[
"Hart",
"Derrick",
""
],
[
"Iosevich",
"Alex",
""
]
] | [
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] |
711.4598 | Oleg Y. Gnedin | Oleg Y. Gnedin, Jose L. Prieto | Dynamical Evolution of Globular Clusters in Hierarchical Cosmology | 5 pages, proceedings of IAU 246 "Dynamical Evolution of Dense Stellar
Systems", eds. Vesperini, Giersz, Sills | null | 10.1017/S1743921308016049 | null | astro-ph | null | We probe the evolution of globular clusters that could form in giant
molecular clouds within high-redshift galaxies. Numerical simulations
demonstrate that the large and dense enough gas clouds assemble naturally in
current hierarchical models of galaxy formation. These clouds are enriched with
heavy elements from earlier stars and could produce star clusters in a similar
way to nearby molecular clouds. The masses and sizes of the model clusters are
in excellent agreement with the observations of young massive clusters. Do
these model clusters evolve into globular clusters that we see in our and
external galaxies? In order to study their dynamical evolution, we calculate
the orbits of model clusters using the outputs of the cosmological simulation
of a Milky Way-sized galaxy. We find that at present the orbits are isotropic
in the inner 50 kpc of the Galaxy and preferentially radial at larger
distances. All clusters located outside 10 kpc from the center formed in the
now-disrupted satellite galaxies. The spatial distribution of model clusters is
spheroidal, with a power-law density profile consistent with observations. The
combination of two-body scattering, tidal shocks, and stellar evolution results
in the evolution of the cluster mass function from an initial power law to the
observed log-normal distribution.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:27:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gnedin",
"Oleg Y.",
""
],
[
"Prieto",
"Jose L.",
""
]
] | [
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711.4599 | Dvira Segal | Lian-Ao Wu and Dvira Segal | How can we derive Fourier's Law from quantum mechanics? Exact master
equation analysis | null | Phys. Rev. E 77, 060101R (2008) | 10.1103/PhysRevE.77.060101 | null | cond-mat.mes-hall cond-mat.stat-mech | null | We derive the macroscopic Fourier's Law of heat conduction from the exact
gain-loss time convolutionless quantum master equation under three assumptions
for the interaction kernel. To second order in the interaction, we show that
the first two assumptions are natural results of the long time limit. The third
assumption can be satisfied by a family of interactions consisting an exchange
effect. The pure exchange model directly leads to energy diffusion in a weakly
coupled spin-1/2 chain.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:30:37 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Wu",
"Lian-Ao",
""
],
[
"Segal",
"Dvira",
""
]
] | [
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] |
711.46 | Bert Schroer | Bert Schroer | Localization and the interface between quantum mechanics, quantum field
theory and quantum gravity | 70 pages, actualization, addition of references | null | null | null | hep-th gr-qc nucl-th quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show that there are significant conceptual differences between QM and QFT
which make it difficult to view the latter as just a relativistic extension of
the principles of QM. At the root of this is a fundamental distinction between
Born-localization in QM (which in the relativistic context changes its name to
Newton-Wigner localization) and modular localization which is the localization
underlying QFT, after one liberates it from its standard presentation in terms
of field coordinates. The first comes with a probability notion and projection
operators, whereas the latter describes causal propagation in QFT and leads to
thermal aspects of locally reduced finite energy states. The Born-Newton-Wigner
localization in QFT is only applicable asymptotically and the covariant
correlation between asymptotic in and out localization projectors is the basis
of the existence of an invariant scattering matrix. Taking these significant
differences serious has not only repercussions for the philosophy of science,
but also leads to a new structural properties as a consequence of vacuum
polarization: the area law for localization entropy near the the causal
localization horizon and a more realistic cutoff independent setting for the
cosmological vacuum energy density which is compatible with local covariance.
The article presents some observations about the interface between QFT in CST
and QG.
| [
{
"version": "v1",
"created": "Thu, 29 Nov 2007 19:28:19 GMT"
},
{
"version": "v2",
"created": "Tue, 4 Dec 2007 19:48:29 GMT"
},
{
"version": "v3",
"created": "Thu, 26 Feb 2009 19:42:46 GMT"
},
{
"version": "v4",
"created": "Tue, 26 May 2009 18:23:15 GMT"
}
] | 2009-05-26T00:00:00 | [
[
"Schroer",
"Bert",
""
]
] | [
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] |
711.4601 | Mladen Georgiev | Mladen Georgiev | Colossal Van der Waals small-polaron superlattice: a hint to
understanding the colossal magnetoresistance and electroresistance in
manganites | 9 pages including 3(5) figuresq all pdf format | null | null | null | physics.chem-ph | null | A mechanism is proposed to explain the formation of a small-polaron
superlattice above the Curie temperature in manganites. The order-disorder
transition initiated by the external field at a lattice is known responsible
for the colossal resistance effect. We attribute the lattice formation to the
occurrence of strong Van der Waals pairing of vibronic small polarons arising
from the phonon coupling of highly polarizable two-level orbital systems. The
latter having inherent electric and magnetic dipoles associated with them, they
couple to the external field leading to the observed colossal effects. We find
numerical estimates of the critical field compatible.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:39:30 GMT"
}
] | 2007-11-30T00:00:00 | [
[
"Georgiev",
"Mladen",
""
]
] | [
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711.4602 | Robert Brandenberger | Andrew Stewart and Robert Brandenberger (McGill University) | Observational Constraints on Theories with a Blue Spectrum of Tensor
Modes | 12 pages, 1 figure, 2 references added, relationship of this work
with Ref. 20 added | JCAP 0808:012,2008 | 10.1088/1475-7516/2008/08/012 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Motivated by the string gas cosmological model, which predicts a blue tilt of
the primordial gravitational wave spectrum, we examine the constraints imposed
by current and planned observations on a blue tilted tensor spectrum. Starting
from an expression for the primordial gravitational wave spectrum normalized
using cosmic microwave background observations, pulsar timing, direct detection
and nucleosynthesis bounds are examined. If we assume a tensor to scalar ratio
on scales of the CMB which equals the current observational upper bound, we
obtain from these current observations constraints on the tensor spectral index
of $n_{T} \lesssim 0.79$, $n_{T} \lesssim 0.53$, and $n_{T} \lesssim 0.15$
respectively.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 21:58:45 GMT"
},
{
"version": "v2",
"created": "Thu, 26 Jun 2008 14:44:27 GMT"
},
{
"version": "v3",
"created": "Sun, 13 Jul 2008 01:34:46 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Stewart",
"Andrew",
"",
"McGill University"
],
[
"Brandenberger",
"Robert",
"",
"McGill University"
]
] | [
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] |
711.4603 | Salah Aly A | Salah A. Aly | A Note on Quantum Hamming Bound | null | null | null | null | quant-ph cs.IT math.IT | null | Proving the quantum Hamming bound for degenerate nonbinary stabilizer codes
has been an open problem for a decade. In this note, I prove this bound for
double error-correcting degenerate stabilizer codes. Also, I compute the
maximum length of single and double error-correcting MDS stabilizer codes over
finite fields.
| [
{
"version": "v1",
"created": "Thu, 29 Nov 2007 19:12:24 GMT"
}
] | 2011-11-10T00:00:00 | [
[
"Aly",
"Salah A.",
""
]
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] |
711.4604 | James Mullaney | James R. Mullaney and Martin J. Ward | Optical emission line properties of Narrow Line Seyfert 1s and
comparison AGN | 24 pages, 13 figures, 5 tables, Accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2007.12777.x | null | astro-ph | null | Based on a new spectroscopic sample observed using the WHT, we examine the
kinematic properties of the various emission line regions in narrow line
Seyfert 1 galaxies (NLS1s) by modelling their profiles using multiple component
fits. We interpret these results by comparison with velocity components
observed for different lines species covered in the same spectrum, and
equivalent components measured in the spectra of some broad line Seyfert 1s and
a representative Seyfert 2 galaxy. We find that the fits to the Halpha and
Hbeta line profiles in NLS1s require an additional broad (~3000km/s) component
that might correspond to a suppressed broad line region with similar kinematics
to those of typical broad line Seyfert 1s. From the profiles of the forbidden
high ionisation lines (FHILs) in NLS1s, we find evidence that they appear to
trace an `intermediate' velocity region with kinematics between the standard
broad and narrow line regions. Weaker evidence of this region is also present
in the profiles of the permitted Balmer lines. Finally, we note that despite
having similar ionisation potentials, the relative intensities of the highly
ionised lines of [Fe X]6374 and [FeXI]7892 show considerable dispersion from
one galaxy to another. The interpretation of this requires further modelling,
but suggests the possibility of using the ratio as a diagnostic to constrain
the physical conditions of the FHIL emitting region and possibly the shape of
the spectral energy distribution in the vicinity of 200eV. This spectral region
is very difficult to observe directly due to photoelectric absorption both in
our Galaxy and intrinsic to the source.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 22:14:05 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mullaney",
"James R.",
""
],
[
"Ward",
"Martin J.",
""
]
] | [
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] |
711.4605 | Yancy L. Shirley | Yancy L. Shirley (Bok Fellow, Univ. of Arizona), Jingwen Wu (CfA), R.
Shane Bussmann (Univ. of Arizona), and Al Wootten (NRAO) | The Properties of Dense Molecular Gas in the Milky Way and Galaxies | 7 pages. To appear in Massive Star Formation: Observations Confront
Theory, ed. H. Beuther, ASP Conference Series | null | null | null | astro-ph | null | We review the evidence for a constant star formation rate per unit mass in
dense molecular gas in the Milky Way and the extragalactic correlations of L_IR
with L' from observations of dense molecular gas. We discuss the connection
between the constant SFR/M interpretation in dense gas and the global
Schmidt-Kennicutt star formation law.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 22:06:25 GMT"
}
] | 2007-11-30T00:00:00 | [
[
"Shirley",
"Yancy L.",
"",
"Bok Fellow, Univ. of Arizona"
],
[
"Wu",
"Jingwen",
"",
"CfA"
],
[
"Bussmann",
"R. Shane",
"",
"Univ. of Arizona"
],
[
"Wootten",
"Al",
"",
"NRAO"
]
] | [
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] |
711.4606 | Amelia Sparavigna | Amelia Sparavigna | Physics in Carnacki's investigations | 8 pages, added references | International Journal of Literature and Arts. Vol. 1, No. 1, 2013,
pp. 11-15 | 10.11648/j.ijla.20130101.13 | null | physics.pop-ph | null | In the stories of Carnacki, created by the English writer William H. Hodgson
and written between 1910 and 1912, we find an interesting mixture of science
and fantasy. In spite of the fact that Carnacki is a ghost finder, who
investigates in an environment where supernatural is acting, we see the
character using technology and sometimes discussing of physics phenomena such
as X-rays. The Carnacki's stories can be seen as mirrors of the physics and
technology knowledge at the beginning of Twentieth Century, in the society
outside scientific circles.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 22:06:31 GMT"
},
{
"version": "v2",
"created": "Sat, 1 Dec 2007 09:00:01 GMT"
},
{
"version": "v3",
"created": "Fri, 18 Jan 2008 09:54:28 GMT"
}
] | 2014-01-03T00:00:00 | [
[
"Sparavigna",
"Amelia",
""
]
] | [
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] |
711.4607 | Yury Kozhedub Sergeevich | Y. S. Kozhedub, O. V. Andreev, V. M. Shabaev, I. I. Tupitsyn, C.
Brandau, C. Kozhuharov, G. Plunien, T. Stohlker | Nuclear deformation effect on the binding energies in heavy ions | 19 pages, 5 tables | Phys. Rev. A 77, 032501 (2008) | 10.1103/PhysRevA.77.032501 | null | physics.atom-ph | null | Nuclear deformation effects on the binding energies in heavy ions are
investigated. Approximate formulas for the nuclear-size correction and the
isotope shift for deformed nuclei are derived. Combined with direct numerical
evaluations, these formulas are employed to reanalyse experimental data on the
nuclear-charge-distribution parameters in $^{238}\textrm{U}$ and to revise the
nuclear-size corrections to the binding energies in H- and Li-like
$^{238}\textrm{U}$. As a result, the theoretical uncertainties for the
ground-state Lamb shift in $^{238}\textrm{U}^{91+}$ and for the $2p_{1/2}-2s$
transition energy in $^{238}\textrm{U}^{89+}$ are significantly reduced. The
isotope shift of the $2p_{j}-2s$ transition energies for
$^{142}\textrm{Nd}^{57+}$ and $^{150}\textrm{Nd}^{57+}$ is also evaluated
including nuclear size and nuclear recoil effects within a full QED treatment.
| [
{
"version": "v1",
"created": "Wed, 28 Nov 2007 22:08:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kozhedub",
"Y. S.",
""
],
[
"Andreev",
"O. V.",
""
],
[
"Shabaev",
"V. M.",
""
],
[
"Tupitsyn",
"I. I.",
""
],
[
"Brandau",
"C.",
""
],
[
"Kozhuharov",
"C.",
""
],
[
"Plunien",
"G.",
""
],
[
"Stohlker",
"T.",
""
]
] | [
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