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712.2979
Dinh-V.-Trung
Jeremy Lim, YiPing Ao, Dinh-V-Trung
Radially-Inflowing Molecular Gas in NGC 1275 Deposited by a X-ray Cooling Flow in the Perseus Cluster
40 pages, 10 figures, accepted for publication in ApJ
null
10.1086/523664
null
astro-ph
null
We have imaged in CO(2-1) the molecular gas in NGC 1275 (Perseus A), the cD galaxy at the center of the Perseus Cluster, at a spatial resolution of $\sim$1 kpc over a central region of radius $\sim$ 10 kpc. Per A is known to contain $\sim$1.3x10$^{10}$ M$_\odot$ of molecular gas, which has been proposed to be captured from mergers with or ram-pressure stripping of gas-rich galaxies, or accreted from a X-ray cooling flow. The molecular gas detected in our image has a total mass of $\sim$4x10$^9$ M$_\odot$, and for the first time can be seen to be concentrated in three radial filaments with lengths ranging from at least 1.1-2.4 kpc all lying in the east-west directions spanning the center of the galaxy to radii of $\sim$8 kpc. The eastern and outer western filaments exhibit larger blueshifted velocities with decreasing radii, whereas the inner western filament spans the systemic velocity of the galaxy. The molecular gas shows no signature of orbital motion, and is therefore unlikely to have been captured from gas-rich galaxies. Instead, we are able to reproduce the observed kinematics of the two outer filaments as free-fall in the gravitational potential of Per A, as would be expected if they originate from a X-ray cooling flow. Indeed, all three filaments lie between two prominent X-ray cavities carved out by radio jets from Per A, and closely resembles the spatial distribution of the coolest X-ray gas in the cluster core. The inferred mass-deposition rate into the two outermost filaments alone is roughly 75 M$_odot$ yr$^{-1}$. This cooling flow can provide a nearly continuous supply of molecular gas to fuel the active nucleus in Per A.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:03:34 GMT" } ]
2009-11-13T00:00:00
[ [ "Lim", "Jeremy", "" ], [ "Ao", "YiPing", "" ], [ "Dinh-V-Trung", "", "" ] ]
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712.298
Salvatore Capozziello
S. Capozziello, M. De Laurentis, M. Francaviglia
Higher-order gravity and the cosmological background of gravitational waves
6 pages, 8 figures
Astropart.Phys.29:125-129,2008
10.1016/j.astropartphys.2007.12.001
null
gr-qc
null
The cosmological background of gravitational waves can be tuned by the higher-order corrections to the gravitational Lagrangian. In particular, it can be shown that assuming $R^{1+\epsilon}$, where $\epsilon$ indicates a generic (eventually small) correction to the Hilbert-Einstein action in the Ricci scalar $R$, gives a parametric approach to control the evolution and the production mechanism of gravitational waves in the early Universe.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:08:32 GMT" } ]
2008-11-26T00:00:00
[ [ "Capozziello", "S.", "" ], [ "De Laurentis", "M.", "" ], [ "Francaviglia", "M.", "" ] ]
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712.2981
Razvan Radulescu M.D.
Razvan Tudor Radulescu
Oncoprotein metastasis disjoined
6 pages
null
null
null
q-bio.SC q-bio.BM
null
As the past decade barely dawned, a fundamentally novel view of cancer relating to signal transduction through intracellular hormones/growth factors and their subunits began to unfold. Further along, it gained additional substance with the advent of the interdisciplinary fields of particle biology and peptide strings which explain (onco)protein dynamics in spacetime, for instance insulin-driven sub- and trans-cellular carcinogenesis, by physical principles. Here, this new understanding is expanded to introduce the concept of "oncoprotein metastasis" preceding cancer cell spread and, thereby, a particular emphasis is placed on its potential role in the emergence of the pre-metastatic niche. Consistent with this perception, yet unlike currently advocated treatments that target cancer cells only, future antineoplastic strategies should aim to mimic natural tumor suppressors as well as involve both (morphologically) normal and malignant cells. If validated in human patients with advanced cancer disease, its otherwise frequently lethal course may be halted and reversed just in time.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:14:30 GMT" } ]
2007-12-19T00:00:00
[ [ "Radulescu", "Razvan Tudor", "" ] ]
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712.2982
Carsten Deibel
C. Deibel, V. Dyakonov, J. Parisi
Spectroscopy of electronic defect states in Cu(In, Ga)(S, Se)$_2$-based heterojunctions and Schottky diodes under damp-heat exposure
4 pages, 5 figures
Europhysics Letters, 66 (2004) 399-404
10.1209/epl/i2003-10211-3
deibel2004
cond-mat.mtrl-sci
null
The changes of defect characteristics induced by accelerated lifetime tests on the heterostructure n-ZnO/i-ZnO/CdS/Cu(In, Ga)(S, Se)$_2$/Mo relevant for photovoltaic energy conversion are investigated. We subject heterojunction and Schottky devices to extended damp heat exposure at 85$^{\circ}$C ambient temperature and 85% relative humidity for various time periods. In order to understand the origin of the pronounced changes of the devices, we apply current--voltage and capacitance--voltage measurements, admittance spectroscopy, and deep-level transient spectroscopy. The fill factor and open-circuit voltage of test devices are reduced after prolonged damp heat treatment, leading to a reduced energy conversion efficiency. We observe the presence of defect states in the vicinity of the CdS/chalcopyrite interface. Their activation energy increases due to damp heat exposure, indicating a reduced band bending at the Cu(In, Ga)(S, Se)$_2$ surface. The Fermi-level pinning at the buffer/chalcopyrite interface, maintaining a high band bending in as-grown cells, is lifted due to the damp-heat exposure. We also observe changes in the bulk defect spectra due to the damp-heat treatment.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:16:23 GMT" } ]
2007-12-19T00:00:00
[ [ "Deibel", "C.", "" ], [ "Dyakonov", "V.", "" ], [ "Parisi", "J.", "" ] ]
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712.2983
Alberto Sainz Dalda
A. Sainz Dalda and L. R. Bellot Rubio
Detection of sea-serpent field lines in sunspot penumbrae
4 pages, 3 figures, 1 movie. Letter accepted by Astronomy & Astrophysics
null
10.1051/0004-6361:20079115
null
astro-ph
null
We investigate the spatial distribution of magnetic polarities in the penumbra of a spot observed very close to disk center. High-spatial resolution, high-cadence magnetograms taken with the Narrowband Filter Imager aboard Hinode are used in this study. They provide continuous and stable measurements in the photospheric Fe I 630.25 line for long periods of time. We discover small-scale, elongated, bipolar magnetic structures that appear in the mid penumbra and move radially outward across the penumbra. They occur in between the more vertical fields of the penumbra, and can be associated with the horizontal fields that harbor the Evershed flow. Many of them cross the outer penumbral boundary, becoming moving magnetic features in the sunspot moat. We determine the properties of these structures, including their sizes, proper motions, footpoint separation, and lifetimes. The bipolar patches can be interpreted as being produced by sea-serpent field lines that originate in the mid-penumbra and eventually leave the spot in the form moving magnetic features. The existence of such field lines has been inferred from Stokes inversions of spectropolarimetric measurements at lower angular resolution, but this is the first time they are imaged directly. Our observations add another piece of evidence in favor of the uncombed structure of penumbral magnetic fields.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 12:10:03 GMT" }, { "version": "v2", "created": "Sun, 20 Jan 2008 17:11:15 GMT" } ]
2009-11-13T00:00:00
[ [ "Dalda", "A. Sainz", "" ], [ "Rubio", "L. R. Bellot", "" ] ]
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712.2984
Mohammad Ali Rajabpour
A. A. Saberi, M. A. Rajabpour, S. Rouhani
Conformal Curves on $WO_3$ Surface
4 pages, 6 figures. accepted in PRL
Phys. Rev. Lett. 100, 044504 (2008)
10.1103/PhysRevLett.100.044504
null
cond-mat.stat-mech
null
We have studied the iso-height lines on the $\mathrm{WO_3}$ surface as a physical candidate for conformally invariant curves. We have shown that these lines are conformally invariant with the same statistics of domain walls in the critical Ising model. They belong to the family of conformal invariant curves called Schramm-Loewner evolution (or $SLE_{\kappa}$), with diffusivity of $\kappa \sim 3$. This can be regarded as the first experimental observation of SLE curves. We have also argued that Ballistic Deposition (BD) can serve as a growth model giving rise to contours with similar statistics at large scales.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:32:45 GMT" } ]
2009-11-13T00:00:00
[ [ "Saberi", "A. A.", "" ], [ "Rajabpour", "M. A.", "" ], [ "Rouhani", "S.", "" ] ]
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712.2985
Mattias Marklund
G. Brodin, M. Marklund, R. Bingham, J. Collier, R. G. Evans
Laboratory soft x-ray emission due to the Hawking-Unruh effect?
11 pages, 3 figures, 1 table
Class.Quant.Grav.25:145005,2008
10.1088/0264-9381/25/14/145005
null
hep-ph gr-qc
null
The structure of spacetime, quantum field theory, and thermodynamics are all connected through the concepts of the Hawking and Unruh temperatures. The possible detection of the related radiation constitutes a fundamental test of such subtle connections. Here a scheme is presented for the detection of Unruh radiation based on currently available laser systems. By separating the classical radiation from the Unruh-response in frequency space, it is found that the detection of Unruh radiation is possible in terms of soft x-ray photons using current laser-electron beam technology. The experimental constraints are discussed and a proposal for an experimental design is given.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:36:50 GMT" } ]
2008-11-26T00:00:00
[ [ "Brodin", "G.", "" ], [ "Marklund", "M.", "" ], [ "Bingham", "R.", "" ], [ "Collier", "J.", "" ], [ "Evans", "R. G.", "" ] ]
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712.2986
Auguste Aman
Auguste Aman (LMAI), Modeste N'Zi (LMAI)
Homogenization of reflected semilinear PDE with nonlinear Neumann boundary condition
Ce papier a 19 pages et est soumis pour publication dans Stochastic Analysis and Applications
null
null
null
math.PR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the homogenization problem of semi linear reflected partial differential equations (reflected PDEs for short) with nonlinear Neumann conditions. The non-linear term is a function of the solution but not of its gradient. The proof are fully probabilistic and uses weak convergence of associated reflected generalized backward differential stochastic equations (reflected GBSDEs in short).
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:48:05 GMT" }, { "version": "v2", "created": "Sat, 10 Jan 2009 11:22:51 GMT" }, { "version": "v3", "created": "Thu, 15 Jan 2009 15:45:16 GMT" } ]
2009-01-15T00:00:00
[ [ "Aman", "Auguste", "", "LMAI" ], [ "N'Zi", "Modeste", "", "LMAI" ] ]
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712.2987
Wouter Bos
Wouter J.T. Bos (LMFA), Jean-Pierre Bertoglio (LMFA)
Inertial range scaling of scalar flux spectra in uniformly sheared turbulence
null
Physics of Fluids 19 (2007) 025104
10.1063/1.2565563
null
physics.class-ph
null
A model based on two-point closure theory of turbulence is proposed and applied to study the Reynolds number dependency of the scalar flux spectra in homogeneous shear flow with a cross-stream uniform scalar gradient. For the cross-stream scalar flux, in the inertial range the spectral behavior agrees with classical predictions and measurements. The streamwise scalar flux is found to be in good agreement with the results of atmospheric measurements. However, both the model results and the atmospheric measurements disagree with classical predictions. A detailed analysis of the different terms in the evolution equation for the streamwise scalar flux spectrum shows that nonlinear contributions are governing the inertial subrange of this spectrum and that these contributions are relatively more important than for the cross-stream flux. A new expression for the scalar flux spectra is proposed. It allows us to unify the description of the components in one single expression, leading to a classical K^-7/3 inertial range for the cross-stream component and to a new K^-23/9 scaling for the streamwise component that agrees better with atmospheric measurements than the K^-3 prediction of J. C. Wyngaard and O. R. Cot\'e [Quart. J. R. Met. Soc. 98, 590 (1972)].
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:54:26 GMT" } ]
2007-12-19T00:00:00
[ [ "Bos", "Wouter J. T.", "", "LMFA" ], [ "Bertoglio", "Jean-Pierre", "", "LMFA" ] ]
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712.2988
Jerome Bouvier
Jerome Bouvier (LAOG)
The rotational evolution of young low mass stars
10 pages
Dans Star-Disk Interaction in Young Stars - Star-Disk Interaction in Young Stars, Grenoble : France (2007)
10.1017/S1743921307009593
null
astro-ph
null
Star-disk interaction is thought to drive the angular momentum evolution of young stars. In this review, I present the latest results obtained on the rotational properties of low mass and very low mass pre-main sequence stars. I discuss the evidence for extremely efficient angular momentum removal over the first few Myr of pre-main sequence evolution and describe recent results that support an accretion-driven braking mechanism. Angular momentum evolution models are presented and their implication for accretion disk lifetimes discussed.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 15:56:36 GMT" } ]
2009-11-13T00:00:00
[ [ "Bouvier", "Jerome", "", "LAOG" ] ]
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712.2989
Recai Erdem
Recai Erdem
A way to get rid of cosmological constant and zero point energy problems of quantum fields through metric reversal symmetry
Presentation and content are improved, references are added. I would like to thank the anonymous referee for his valuable comments and suggestions to improve the paper
J.Phys.A41:235401,2008
10.1088/1751-8113/41/23/235401
IZTECH-P-07-06
hep-th astro-ph gr-qc hep-ph
null
In this paper a framework is introduced to remove the huge discrepancy between the empirical value of the cosmological constant and the contribution to the cosmological constant predicted from the vacuum energy of quantum fields. An extra dimensional space with metric reversal symmetry and $R^2$ gravity is considered to this end. The resulting 4-dimensional energy-momentum tensor (obtained after integration over extra dimensions) consists of terms that contain off-diagonally coupled pair of Kaluza-Klein modes. This, in turn, generically results in vanishing of the vacuum expectation value of the energy-momentum tensor for quantum fields, and offers a way to solve the problem of huge contribution of quantum fields to the vacuum energy density.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:16:52 GMT" }, { "version": "v2", "created": "Tue, 29 Apr 2008 15:50:36 GMT" } ]
2008-11-26T00:00:00
[ [ "Erdem", "Recai", "" ] ]
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712.299
Dean Lee J
Bugra Borasoy, Evgeny Epelbaum, Hermann Krebs, Dean Lee, Ulf-G. Mei{\ss}ner
Chiral effective field theory on the lattice at next-to-leading order
30 pages, 10 figures, published version
Eur.Phys.J.A35:343-355,2008
10.1140/epja/i2008-10544-3
null
nucl-th hep-lat
null
We study nucleon-nucleon scattering on the lattice at next-to-leading order in chiral effective field theory. We determine phase shifts and mixing angles from the properties of two-nucleon standing waves induced by a hard spherical wall in the center-of-mass frame. At fixed lattice spacing we test model independence of the low-energy effective theory by computing next-to-leading-order corrections for two different leading-order lattice actions. The first leading-order action includes instantaneous one-pion exchange and same-site contact interactions. The second leading-order action includes instantaneous one-pion exchange and Gaussian-smeared interactions. We find that in each case the results at next-to-leading order are accurate up to corrections expected at higher order.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:17:17 GMT" }, { "version": "v2", "created": "Thu, 17 Apr 2008 14:53:11 GMT" } ]
2008-11-26T00:00:00
[ [ "Borasoy", "Bugra", "" ], [ "Epelbaum", "Evgeny", "" ], [ "Krebs", "Hermann", "" ], [ "Lee", "Dean", "" ], [ "Meißner", "Ulf-G.", "" ] ]
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712.2991
Richard Easther
Richard Easther, John T. Giblin Jr, and Eugene A. Lim
Gravitational Waves From the End of Inflation: Computational Strategies
15 pages, 13 figures
Phys.Rev.D77:103519,2008
10.1103/PhysRevD.77.103519
null
astro-ph
null
Parametric resonance or preheating is a plausible mechanism for bringing about the transition between the inflationary phase and a hot, radiation dominated universe. This epoch results in the rapid production of heavy particles far from thermal equilibrium and could source a significant stochastic background of gravitational radiation. Here, we present a numerical algorithm for computing the contemporary power spectrum of gravity waves generated in this post-inflationary phase transition for a large class of scalar-field driven inflationary models. We explicitly calculate this spectrum for both quartic and quadratic models of chaotic inflation, and low-scale hybrid models. In particular, we consider hybrid models with an ``inverted'' potential. These models have a very short and intense period of resonance which is qualitatively different from previous examples studied in this context, but we find that they lead to a similar spectrum of gravitational radiation.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:23:00 GMT" } ]
2008-11-26T00:00:00
[ [ "Easther", "Richard", "" ], [ "Giblin", "John T.", "Jr" ], [ "Lim", "Eugene A.", "" ] ]
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712.2992
Elio Conte
Elio Conte
A Proof Of Kochen - Specker Theorem of Quantum Mechanics Using a Quantum Like Algebraic Formulation
null
null
null
null
physics.gen-ph
null
Using a quantum like algebraic formulation we give proof of Kochen-Specker theorem. We introduce new criteria in order to account for the contextual nature of measurements in quantum mechanics.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:22:11 GMT" } ]
2007-12-19T00:00:00
[ [ "Conte", "Elio", "" ] ]
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712.2993
Dean Lee J
Bugra Borasoy, Evgeny Epelbaum, Hermann Krebs, Dean Lee, Ulf-G. Mei{\ss}ner
Dilute neutron matter on the lattice at next-to-leading order in chiral effective field theory
25 pages, 7 figures, published version
Eur.Phys.J.A35:357-367,2008
10.1140/epja/i2008-10545-2
null
nucl-th astro-ph hep-lat
null
We discuss lattice simulations of the ground state of dilute neutron matter at next-to-leading order in chiral effective field theory. In a previous paper the coefficients of the next-to-leading-order lattice action were determined by matching nucleon-nucleon scattering data for momenta up to the pion mass. Here the same lattice action is used to simulate the ground state of up to 12 neutrons in a periodic cube using Monte Carlo. We explore the density range from 2% to 8% of normal nuclear density and analyze the ground state energy as an expansion about the unitarity limit with corrections due to finite scattering length, effective range, and P-wave interactions.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:24:49 GMT" }, { "version": "v2", "created": "Thu, 17 Apr 2008 14:57:51 GMT" } ]
2008-11-26T00:00:00
[ [ "Borasoy", "Bugra", "" ], [ "Epelbaum", "Evgeny", "" ], [ "Krebs", "Hermann", "" ], [ "Lee", "Dean", "" ], [ "Meißner", "Ulf-G.", "" ] ]
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712.2994
Wouter Bos
Guillevic Lamaison (LMFA), Wouter Bos (LMFA), L. Shao (LMFA), Jean-Pierre Bertoglio (LMFA)
Decay of scalar variance in isotropic turbulence in a bounded domain
null
Journal of turbulence 8, 4 (2007) 1
10.1080/14685240601091676
null
physics.class-ph
null
The decay of scalar variance in isotropic turbulence in a bounded domain is investigated. Extending the study of Touil, Bertoglio and Shao (2002; Journal of Turbulence, 03, 49) to the case of a passive scalar, the effect of the finite size of the domain on the lengthscales of turbulent eddies and scalar structures is studied by truncating the infrared range of the wavenumber spectra. Analytical arguments based on a simple model for the spectral distributions show that the decay exponent for the variance of scalar fluctuations is proportional to the ratio of the Kolmogorov constant to the Corrsin-Obukhov constant. This result is verified by closure calculations in which the Corrsin-Obukhov constant is artificially varied. Large-eddy simulations provide support to the results and give an estimation of the value of the decay exponent and of the scalar to velocity time scale ratio.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:27:14 GMT" } ]
2007-12-19T00:00:00
[ [ "Lamaison", "Guillevic", "", "LMFA" ], [ "Bos", "Wouter", "", "LMFA" ], [ "Shao", "L.", "", "LMFA" ], [ "Bertoglio", "Jean-Pierre", "", "LMFA" ] ]
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712.2995
Jean-Francois Jaulent
Jean-Fran\c{c}ois Jaulent (IMB)
Note sur la conjecture de Leopoldt
null
null
null
null
math.NT
null
We prove that number fields with arbitrary degree but weak ramification satisfy the Leopoldt conjecture on the l-adic rank of the group of units
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:30:18 GMT" } ]
2007-12-19T00:00:00
[ [ "Jaulent", "Jean-François", "", "IMB" ] ]
[ -0.0149828615, -0.0379550196, -0.0549644902, -0.0057342537, 0.0366898514, -0.017208619, -0.0536524653, -0.014947718, -0.0633520856, -0.0631646514, 0.1011196673, -0.0157091618, -0.1789977401, -0.0495758168, -0.0248113368, 0.0540741868, 0.0596971549, -0.0166111775, 0.0020192889, 0.0820484459, 0.0165994633, -0.0676630214, 0.1211749166, -0.0595565811, 0.0511689894, -0.0708962306, -0.0136708356, -0.032074336, 0.1675643772, -0.0505129769, 0.0731922686, -0.0305045899, 0.0003144614, 0.0141511308, -0.1224869415, 0.0058045406, 0.0777375028, 0.0146431401, -0.059790872, -0.000223857, -0.0000454624, 0.0756288916, -0.0975584611, 0.0448431522, 0.0621806309, 0.106648922, 0.113958776, 0.0525747314, -0.0439059921, 0.0178060587, -0.0113396477, 0.1512577832, 0.078159228, 0.0259125009, -0.0755820349, 0.0337612256, -0.0011626653, 0.0357761197, 0.1075860783, -0.0733328462, 0.0725362599, -0.1244549751, -0.0305748768, -0.0911389068, -0.1048683152, 0.0400636308, -0.1079609469, 0.0329177789, 0.1127404645, 0.1133027598, -0.1691575497, 0.0009400896, 0.107867226, 0.0827981755, -0.1168639734, -0.0410476513, 0.0295908581, -0.0003280063, -0.035494972, 0.0271308105, 0.016189456, 0.087155968, 0.0408133604, 0.0007493627, 0.0550582074, -0.0657887012, -0.005450177, 0.0417036638, -0.1171451211, 0.0356121175, 0.0687407553, 0.0066186995, -0.0364087038, 0.0446557216, -0.0026269793, 0.0268496629, 0.086312525, 0.0221755709, 0.0069994209, -0.0372287184, 0.0002665051, 0.0305280183, 0.0650858283, -0.1615665555, 0.0747854486, 0.1446976513, 0.0566045232, -0.0657887012, -0.1549127102, 0.0828450322, -0.0043460838, -0.0212149825, -0.0021891494, -0.007198568, 0.0503724031, -0.018286353, -0.1149896532, 0.0266388003, -0.0537930392, 0.001515565, 0.0902017429, -0.0058631133, -0.0339486562, -0.0021906139, 0.0886085704, 0.0526684485, -0.0471391976, -0.0609154627, -0.0422425307, -0.0234641675, 0.051684428, 0.0247644782, 0.0301765837, 0.0454991646, -0.097277306, -0.0262405071, 0.1137713417, -0.0391264707, 0.0999950767, -0.0774563551, 0.0707556531, 0.0048468793, 0.0365961343, 0.0576822571, -0.0593222901, 0.0946532562, -0.0335035063, -0.015334296, 0.1323271245, 0.0093013225, -0.0192352291, -0.0224801488, 0.0373224355, -0.027950827, -0.0074211434, -0.0808769912, 0.0067241299, 0.0481700748, 0.0945126861, 0.0182394963, 0.0641018078, 0.0892645866, 0.0889834315, -0.0142682763, 0.0881868452, 0.0335035063, -0.0328943506, 0.0000122179, 0.0405087844, -0.0138348388, -0.0202075336, -0.0362915583, -0.0863593817, -0.0759568959, -0.017044615, 0.0132608274, -0.111147292, -0.0858908072, 0.0104434872, -0.0221169982, 0.0192235149, 0.0604000241, -0.0842976272, 0.0411413684, -0.0758163258, -0.0282085445, 0.0721613988, 0.0137059791, 0.0018992153, -0.0085984515, -0.0183097832, 0.0535587482, 0.0289114155, 0.1418861747, 0.1688764095, -0.0730985552, 0.0042025815, 0.0799866915, -0.0441168547, -0.0087038828, -0.0023765818, -0.0002092139, -0.0353778265, 0.0422659591, -0.0288411286, -0.024905052, 0.0184386428, 0.0207581148, -0.0390327536, -0.0021291126, -0.0036666424, -0.0491540916, 0.0727236941, 0.0065425551, 0.0146431401, 0.0034938534, 0.0088151703, -0.0335269347, -0.0333629325, 0.03408923, 0.0221638568, -0.0370178595, -0.0133311152, 0.0706619397, 0.0501381122, 0.0840633363, -0.0016707823, 0.0063668373, 0.0325429142, -0.0094536114, 0.0428985432, -0.0181574933, -0.046319183, -0.0908577591, 0.0192118008, -0.0052656732, 0.0596971549, -0.0071927104, -0.0336909369, -0.0989641994, 0.0888428614, 0.0540273301, 0.011679369, 0.0305045899, -0.0824701637, 0.0203129649, -0.0192118008, 0.0337143652, 0.0557610765, -0.0064078383, -0.055339355, 0.0348389596, -0.0433905534, -0.056417089, -0.1058054715, 0.0724894032 ]
712.2996
Giovanni Panti
Giovanni Panti
A general Lagrange Theorem
5 pages, 2 figures
null
null
null
math.NT math.DS
null
The ordinary continued fractions expansion of a real number is based on the Euclidean division. Variants of the latter yield variants of the former, all encompassed by a more general Dynamical Systems framework. For all these variants the Lagrange Theorem holds: a number has an eventually periodic expansion if and only if it is a quadratic irrational. This fact is surely known for specific expansions, but the only proof for the general case that I could trace in the literature follows as an implicit corollary from much deeper results by Boshernitzan and Carroll on interval exchange transformations. It may then be useful to have at hand a simple and virtually computation-free proof of a general Lagrange Theorem.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:30:59 GMT" } ]
2007-12-19T00:00:00
[ [ "Panti", "Giovanni", "" ] ]
[ -0.0398274884, -0.0673924387, 0.1233467162, 0.0369421877, 0.0132028386, 0.0034037563, -0.0419657044, 0.0435114019, 0.0092226658, 0.0181748345, 0.0208154023, -0.0466028005, -0.1246863157, -0.0160752609, 0.1405554861, 0.114690803, 0.0132672423, 0.005104024, 0.0044664238, 0.077748619, 0.036426954, -0.0198235791, -0.0247440524, -0.0075417189, 0.0915053338, -0.1248924136, -0.0180202648, 0.0211760644, 0.0008151143, -0.0460360423, 0.0676500574, -0.0492820106, -0.0569847375, 0.0259806104, -0.0834161788, 0.1357122958, -0.0196947716, -0.0085721845, -0.0042281286, 0.0364011936, -0.0663104504, -0.008256604, -0.1056227088, 0.0657436922, 0.0588910989, 0.0928449333, 0.0721841082, -0.0207509976, -0.0533265881, 0.0681137666, 0.017414866, -0.042558223, 0.0698140338, -0.0362981446, -0.063631244, -0.0116184978, -0.048431877, 0.0716688707, 0.0077349311, -0.1130420566, 0.0871773735, -0.0527083091, 0.0380499363, 0.046551276, -0.1056227088, 0.0831585601, -0.0922266543, 0.052682545, 0.0670832992, 0.0417596139, -0.0912992358, 0.01101954, 0.0290848874, 0.0511368476, 0.1149999425, 0.0294713117, 0.1158243194, 0.1162365004, 0.0233271625, 0.0473756492, 0.0624462068, -0.0325369462, 0.0284408461, 0.0449282937, 0.0823857114, 0.0653315112, -0.0214852039, 0.056778647, -0.1379793286, 0.024254581, -0.016345758, -0.0264571998, -0.0072841025, 0.0188703984, 0.0415535197, -0.0562634133, 0.0745541751, 0.0349585414, 0.0518066511, -0.0181233119, -0.0080633918, -0.0553875193, 0.0716688707, -0.0192697048, 0.2034138739, 0.0849103555, 0.0181877147, 0.0197720565, -0.1250985116, -0.0198622216, -0.0589426234, 0.0438978299, 0.0084562572, -0.0655891225, -0.0246796478, 0.0354737714, 0.0131577561, -0.015547147, -0.0831585601, 0.0132930046, 0.0216784161, -0.1259228736, 0.0187287088, -0.0053584203, 0.1009856164, -0.0758422539, -0.0028305599, -0.0440266356, 0.128499046, -0.0246667676, 0.0457784273, 0.0073485067, -0.0877441317, 0.0223095771, -0.0894443989, -0.0284923688, 0.0220004376, -0.0746572241, 0.0768727213, 0.0616733581, -0.0137180714, 0.0078508584, -0.0438205451, -0.0154312197, 0.0735237077, 0.0114768092, -0.0446191542, -0.0083145685, 0.0550783798, -0.047787834, -0.079500407, -0.0407806709, 0.0509565175, -0.015019034, 0.0383075513, -0.0100599192, -0.008089154, 0.0484576374, -0.0048721693, -0.0576030202, 0.0194113925, 0.1329300404, -0.0606944151, 0.0728023872, 0.0325884707, 0.05827282, -0.0604368001, -0.1073744968, -0.0916599035, -0.1252015531, -0.0158176441, -0.0934116915, -0.1244802251, -0.0605913699, 0.0091453809, 0.0408064313, -0.0328203253, -0.0570877865, -0.0172216538, -0.0378180817, -0.0036903543, 0.1248924136, -0.0751724541, -0.0753785446, 0.0310427714, 0.0191924181, -0.0703292638, 0.0613126941, 0.0817674324, -0.0067881909, -0.0072068176, 0.0948028192, 0.0958332866, 0.127880767, 0.0631160066, -0.0618794486, 0.0729054287, -0.0308882017, -0.0362466238, 0.0510080382, -0.0204547383, -0.0309912488, 0.0682683364, 0.0658467412, -0.0585304387, 0.0167321824, 0.0607974604, 0.0272300504, -0.0700716525, -0.0472468399, 0.0245637204, -0.0685259551, 0.045675382, 0.0164616853, -0.0492562503, 0.0651769415, 0.0380499363, 0.0763574913, 0.0210730191, 0.0773879588, -0.0196046047, -0.0094609605, -0.0504155234, 0.1453986764, 0.0341341682, -0.00361951, 0.1423072815, 0.0359374844, 0.0256585889, 0.0654860809, 0.0592002384, 0.0225027893, -0.0634766743, -0.1052620485, 0.0905779153, -0.0038706858, 0.0026550586, -0.0406003371, -0.0363496691, -0.0788306072, 0.0001182419, 0.1144847125, -0.0105429497, -0.0525279753, -0.0208025221, 0.0489213467, -0.036684569, 0.0104270224, 0.0737298056, 0.0433310717, -0.1137633845, -0.0332582742, 0.0061087278, 0.0086108269, -0.0624462068, -0.0516263172 ]
712.2997
Jean-Francois Jaulent
Jean-Fran\c{c}ois Jaulent (IMB)
Plongements l-adiques et l-nombres de Weil
null
null
null
null
math.NT
null
We define l-adic analogs of classical Weil numbers in connexion both with complex or l-adic imbeddings of number fields and real or l-adic absolute values. As an application we give some consequences related to the Iwasawa theory of cyclotomic towers.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:31:33 GMT" } ]
2007-12-19T00:00:00
[ [ "Jaulent", "Jean-François", "", "IMB" ] ]
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712.2998
Jean-Francois Jaulent
Jean-Fran\c{c}ois Jaulent (IMB)
Compactification l-adique de R
null
null
null
null
math.NT
null
We construct a compact topological group Rl which contains both the real additive group R and the l-adic one Ql (for a given prime number l) as dense subgroups; thus we study some of its properties. This construction gives an arithmetic description of the so-called l-adic solenoid classically defined in terms of foliations.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:32:35 GMT" }, { "version": "v2", "created": "Sun, 6 Jan 2008 17:29:51 GMT" } ]
2008-01-06T00:00:00
[ [ "Jaulent", "Jean-François", "", "IMB" ] ]
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712.2999
Alexander Khodjamirian
K.G. Chetyrkin, A. Khodjamirian, A.A. Pivovarov
Towards NNLO Accuracy in the QCD Sum Rule for the Kaon Distribution Amplitude
14 pages, 2 figures
Phys.Lett.B661:250-258,2008
10.1016/j.physletb.2008.02.031
SI-HEP-2007-19, TTP-07-36, SFB/CPP-07-83
hep-ph
null
We calculate the $O(\alpha_s)$ and $O(\alpha_s^2)$ gluon radiative corrections to the QCD sum rule for the first Gegenbauer moment $a_1^K$ of the kaon light-cone distribution amplitude. The NNL0 accuracy is achieved for the perturbative term and quark-condensate contributions to the sum rule. A complete factorization is implemented, removing logarithms of $s$-quark mass from the coefficients in the operator-product expansion. The sum rule with radiative corrections yields $a_1^K(1 \GeV)=0.10\pm 0.04$.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:45:21 GMT" } ]
2008-11-26T00:00:00
[ [ "Chetyrkin", "K. G.", "" ], [ "Khodjamirian", "A.", "" ], [ "Pivovarov", "A. A.", "" ] ]
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712.3
Hans-Thomas Janka
C. Lunardini (1,2), B. Mueller (3), and H.-Th. Janka (3) ((1) Arizona State University, Tempe (2) RIKEN BNL Research Center, Upton (3) MPI for Astrophysics, Garching)
Neutrino oscillation signatures of oxygen-neon-magnesium supernovae
14 pages, 10 figures (16 figure files). Text and graphics added for illustration and clarification; Results unchanged. Version accepted for publication in Physical Review D
Phys.Rev.D78:023016,2008
10.1103/PhysRevD.78.023016
RBRC 712
astro-ph hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We discuss the flavor conversion of neutrinos from core collapse supernovae that have oxygen-neon-magnesium (ONeMg) cores. Using the numerically calculated evolution of the star up to 650 ms post bounce, we find that, for the normal mass hierarchy, the electron neutrino flux in a detector shows signatures of two typical features of an ONeMg-core supernova: a sharp step in the density profile at the base of the He shell and a faster shock wave propagation compared to iron core supernovae. Before the shock hits the density step (t ~ 150 ms), the survival probability of electron neutrinos is about 0.68, in contrast to values of 0.32 or less for an iron core supernova. The passage of the shock through the step and its subsequent propagation cause a decrease of the survival probability and a decrease of the amplitude of oscillations in the Earth, reflecting the transition to a more adiabatic propagation inside the star. These changes affect the lower energy neutrinos first; they are faster and more sizable for larger theta_13. They are unique of ONeMg-core supernovae, and give the possibility to test the speed of the shock wave. The time modulation of the Earth effect and its negative sign at the neutronization peak are the most robust signatures in a detector.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:43:21 GMT" }, { "version": "v2", "created": "Tue, 18 Dec 2007 21:07:31 GMT" }, { "version": "v3", "created": "Mon, 16 Jun 2008 21:45:11 GMT" } ]
2009-12-06T00:00:00
[ [ "Lunardini", "C.", "" ], [ "Mueller", "B.", "" ], [ "Janka", "H. -Th.", "" ] ]
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712.3001
Marek Gazdzicki
Marek Gazdzicki
Onset of Deconfinement in Nucleus-Nucleus Collisions - Past, Present and Future -
Dedicated to 60th birthday of Mark I. Gorenstein, Presented at "New Trends in High Energy Physics", Yalta, Crimea, September 15-22, 2007
null
null
null
nucl-th
null
In 2007 Mark I. Gorenstein celebrated his 60th birthday. This report is dedicated to Mark and it sketches the results obtained during the past ten years of our collaboration and friendship. They concern search for and study of the onset of deconfinement in high energy nucleus-nucleus collisions.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 16:51:00 GMT" } ]
2007-12-19T00:00:00
[ [ "Gazdzicki", "Marek", "" ] ]
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712.3002
Nicholas Parker
N. G. Parker, A. M. Martin, S. L. Cornish and C. S. Adams
Collisions of bright solitary matter waves
9 pages, 4 colour figures
J. Phys. B: At. Mol. Opt. Phys. 41 No 4 (28 February 2008) 045303
10.1088/0953-4075/41/4/045303
null
cond-mat.other
null
The collisions of three-dimensional bright solitary matter waves formed from atomic Bose-Einstein condensates are shown to exhibit rich behaviour. Collisions range from being elastic to completely destructive due to the onset of collapse during the interaction. Through a detailed quantitative analysis we map out the role of relative phase, impact speed and interaction strength. In particular, we identify the importance of the collapse time in the onset of unstable collisions and show how the relative phase controls a population transfer between the waves. Our analysis enables us to interpret recent experimental observations of bright solitary matter waves.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:20:49 GMT" } ]
2009-11-13T00:00:00
[ [ "Parker", "N. G.", "" ], [ "Martin", "A. M.", "" ], [ "Cornish", "S. L.", "" ], [ "Adams", "C. S.", "" ] ]
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712.3003
Alessandro Nagar
Thibault Damour, Alessandro Nagar, Ernst Nils Dorband, Denis Pollney, Luciano Rezzolla
Faithful Effective-One-Body waveforms of equal-mass coalescing black-hole binaries
13 pages, 3 figures. Small changes. Version published in Phys. Rev. D
Phys.Rev.D77:084017,2008
10.1103/PhysRevD.77.084017
null
gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We continue the program of constructing, within the Effective-One-Body (EOB) approach, high-accuracy analytic waveforms describing the signal emitted by inspiralling and coalescing black hole binaries. Here, we compare a recently derived, resummed 3 PN-accurate EOB quadrupolar waveform to the results of a numerical simulation of the inspiral and merger of an equal-mass black hole binary. We find a remarkable agreement, both in phase and in amplitude, with a maximal dephasing which can be reduced below $\pm 0.005$ gravitational-wave (GW) cycles over 12 GW cycles corresponding to the end of the inspiral, the plunge, the merger and the beginning of the ringdown. This level of agreement is shown for two different values of the effective 4 PN parameter a_5, and for corresponding, appropriately "flexed" values of the radiation-reaction resummation parameter v_pole. In addition, our resummed EOB amplitude agrees to better than the 1% level with the numerical-relativity one up to the late inspiral. These results, together with other recent work on the EOB-numerical-relativity comparison, confirm the ability of the EOB formalism to faithfully capture the general relativistic waveforms.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:33:05 GMT" }, { "version": "v2", "created": "Fri, 29 Aug 2008 09:04:01 GMT" } ]
2008-11-26T00:00:00
[ [ "Damour", "Thibault", "" ], [ "Nagar", "Alessandro", "" ], [ "Dorband", "Ernst Nils", "" ], [ "Pollney", "Denis", "" ], [ "Rezzolla", "Luciano", "" ] ]
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712.3004
Francesco Shankar
Francesco Shankar (1), Alfonso Cavaliere (2), Michele Cirasuolo (3) and Laura Maraschi (4) ((1) OSU, USA; (2) Tor Vergata, Italy; (3) SUPA, Scotland (4)-INAF-Oss. Astr. Brera, Italy)
The Optical-Radio Mapping: the kinetic efficiency of Radio-Loud AGNs
ApJ, accepted, 7 pages, 6 figures
null
10.1086/528836
null
astro-ph
null
We constrain the mean kinetic efficiency of radio-loud active galactic nuclei by using an optically selected sample for which both the optical and the radio luminosity functions (LFs) have been determined; the former traces the bolometric luminosity L, while the latter traces the kinetic power L_k, empirically correlated to the radio emission. Thus in terms of the ratio g_k=L_k/L, we can convert the optical LF of the sample into a radio one. This computed LF is shown to match the directly observed LF for the same sample if g_k=0.10^{+0.05}_{-0.01} holds, with a scatter \sigma=0.38^{+0.04}_{-0.09} dex; with these values we also match a number of independent correlations between L_k, L and radio emission, that we derive through Monte Carlo simulations. We proceed to translate the value of g_k into a constraint on the kinetic efficiency for the production of radio jets or winds, namely, \epsilon_k=L_k/(Mdot*c^2)~0.01 in terms of the rate Mdot of mass accretion onto the central black hole. Then, on assuming that on average the radio sources share the same kinetic efficiency, we compute a solid lower limit of about 25% on the contribution of radio sources to the local black hole mass density.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:49:09 GMT" } ]
2009-11-13T00:00:00
[ [ "Shankar", "Francesco", "" ], [ "Cavaliere", "Alfonso", "" ], [ "Cirasuolo", "Michele", "" ], [ "Maraschi", "Laura", "" ] ]
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712.3005
Scott J. Wolk
Scott J. Wolk, Bradley D. Spitzbart, Tyler L. Bourke, Robert A. Gutermuth, Miquela Vigil, Fernando Comer\'on
X-ray and IR Point Source Identification and Characteristics in the Embedded, Massive Star-Forming Region RCW 108
63 pages including 18 figures, and 15 tables. Tables 1,2,5,7,10,and 11 have been stubbed in the text and included as ancillary files. Accepted by the Astronomical Journal
null
10.1088/0004-6256/135/2/693
null
astro-ph
null
We report on the results of an approximately 90 ks Chandra observation of a complex region that hosts multiple sites of recent and active star formation in ARA OB1a. The field is centered on the embedded cluster RCW 108-IR and includes and a large portion of the open cluster NGC 6193. We detect over 420 X-ray sources in the field and combined these data with deep near-IR, Spitzer/IRAC and MSX mid-IR data. We find about 360 of the X-ray sources have near--IR counterparts. We divide the region into 5 parts based on the X-ray point source characteristics and extended 8 micron emission. The most clearly defined regions are the central region - identified by embedded sources with high luminosities in the both the near-IR and X-ray as well as high X-ray temperatures (about 3 keV) and the eastern region - identified by low extinction and 1 keV X-ray temperatures. Other regions, identified by their directional relationship to RCW 108-IR are less uniform - representing combinations of the first two regions, independent star formation epochs, or both. Over 18% percent of the cluster members with over 100 counts exhibit flares. Overall about 50% of the stars appear to have optically thick disks when IRAC data are employed. The largest fraction of X-ray sources are best described as possessing some disk material via a more detailed extinction fitting. We estimate that the total number of pre--main sequence stars in the field is about 1600. Approximately 800 are confined to (1.1 pc) central region.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:37:39 GMT" } ]
2009-11-13T00:00:00
[ [ "Wolk", "Scott J.", "" ], [ "Spitzbart", "Bradley D.", "" ], [ "Bourke", "Tyler L.", "" ], [ "Gutermuth", "Robert A.", "" ], [ "Vigil", "Miquela", "" ], [ "Comerón", "Fernando", "" ] ]
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712.3006
Silvia Pedicelli
S. Pedicelli, J. Lub, J.W. Pel, B. Lemasle, G. Bono, P. Francois, D. Laney, A. Piersimoni, F. Primas, M. Romaniello, R. Buonanno, F. Caputo, S. Cassisi, F. Castelli, A. Pietrinferni, J. Pritchard
Metallicity estimates of Galactic Cepheids based on Walraven photometry
6 pages, 5 figures; to appear in Mem. Soc. Astr. Italiana, Vol. 79/2 (proceeding Cefalu' Workshop "XXI Century Challenges for Stellar Evolution", ed. S. Cassisi & M. Salaris)
null
null
null
astro-ph
null
We present new empirical and theoretical calibrations of two photometric metallicity indices based on Walraven photometry. The empirical calibration relies on a sample of 48 Cepheids for which iron abundances based on high resolution spectra are available in the literature. They cover a broad range in metal abundance (-0.5 < [Fe/H] < +0.5) and the intrinsic accuracy of the Metallicity Index Color (MIC) relations is better than 0.2 dex. The theoretical calibration relies on a homogeneous set of scaled-solar evolutionary tracks for intermediate-mass stars and on pulsation predictions concerning the topology of the instability strip. The metal content of the adopted evolutionary tracks ranges from Z=0.001 to Z=0.03 and the intrinsic accuracy of the MIC relations is better than 0.1 dex.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:40:16 GMT" } ]
2007-12-19T00:00:00
[ [ "Pedicelli", "S.", "" ], [ "Lub", "J.", "" ], [ "Pel", "J. W.", "" ], [ "Lemasle", "B.", "" ], [ "Bono", "G.", "" ], [ "Francois", "P.", "" ], [ "Laney", "D.", "" ], [ "Piersimoni", "A.", "" ], [ "Primas", "F.", "" ], [ "Romaniello", "M.", "" ], [ "Buonanno", "R.", "" ], [ "Caputo", "F.", "" ], [ "Cassisi", "S.", "" ], [ "Castelli", "F.", "" ], [ "Pietrinferni", "A.", "" ], [ "Pritchard", "J.", "" ] ]
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712.3007
Elena Rubei
Elena Rubei
On tropical and Kapranov ranks of tropical matrices
12 pages, third version equal to the second, I added only a note with a reference
null
null
null
math.AG math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We prove that, for any g greater or equal than 3, a matrix g x 5 with tropical rank 3 has Kapranov rank 3.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:40:45 GMT" }, { "version": "v2", "created": "Sun, 13 Dec 2009 10:30:25 GMT" }, { "version": "v3", "created": "Tue, 10 May 2011 14:37:34 GMT" } ]
2011-05-11T00:00:00
[ [ "Rubei", "Elena", "" ] ]
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712.3008
Giovanni Montani
Giovanni Montani, Marco Valerio Battisti, Riccardo Benini, Giovanni Imponente
Classical and Quantum Features of the Mixmaster Singularity
170 pages, 14 figures, ~500 references. Invited review paper to appear on Int. J. Mod. Phys. A. v2: minor changes, references added. v3: Conclusions added
Int.J.Mod.Phys.A23:2353-2503,2008
10.1142/S0217751X08040275
null
gr-qc astro-ph hep-th quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This review article is devoted to analyze the main properties characterizing the cosmological singularity associated to the homogeneous and inhomogeneous Mixmaster model. After the introduction of the main tools required to treat the cosmological issue, we review in details the main results got along the last forty years on the Mixmaster topic. We firstly assess the classical picture of the homogeneous chaotic cosmologies and, after a presentation of the canonical method for the quantization, we develop the quantum Mixmaster behavior. Finally, we extend both the classical and quantum features to the fully inhomogeneous case. Our survey analyzes the fundamental framework of the Mixmaster picture and completes it by accounting for recent and peculiar outstanding results.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:45:03 GMT" }, { "version": "v2", "created": "Wed, 19 Mar 2008 16:15:11 GMT" }, { "version": "v3", "created": "Fri, 12 Sep 2008 13:24:57 GMT" } ]
2008-11-26T00:00:00
[ [ "Montani", "Giovanni", "" ], [ "Battisti", "Marco Valerio", "" ], [ "Benini", "Riccardo", "" ], [ "Imponente", "Giovanni", "" ] ]
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712.3009
Tobias Hurth
Tobias Huber (Zurich U., Aachen Tech. Hochsch), Tobias Hurth (CERN, SLAC), and Enrico Lunghi (Fermilab)
Logarithmically Enhanced Corrections to the Decay Rate and Forward Backward Asymmetry in anti-B --> X(s) l+ l-
26 pages, 3 figures, minor changes, published version
Nucl.Phys.B802:40-62,2008
10.1016/j.nuclphysb.2008.04.028
CERN CERN-PH-TH/2007-177, SLAC-PUB-12859, ZU-TH 30/07, FERMILAB-PUB-07-639-T, PITHA 07/21
hep-ph hep-ex
null
We study logarithmically enhanced electromagnetic corrections to the decay rate in the high dilepton invariant mass region as well as corrections to the forward backward asymmetry (FBA) of the inclusive rare decay $\bar{B} \to X_s \ell^+ \ell^-$. As expected, the relative effect of these corrections in the high dilepton mass region is around -8% for the muonic final state and therefore much larger than in the low dilepton mass region. We also present a complete phenomenological analysis, to improved NNLO accuracy, of the dilepton mass spectrum and the FBA integrated in the low dilepton mass region, including a new approach to the zero of the FBA. The latter represents one of the most precise predictions in flavour physics with a theoretical uncertainty of order 5%. We find $(q_0^2)_{\mu\mu} = (3.50 \pm 0.12) \gev^2$. For the high dilepton invariant mass region, we have ${\cal B}(\bar B\to X_s\mu\mu)_{\rm high} = (2.40^{+0.69}_{-0.62}) \times 10^{-7}$. The dominant uncertainty is due to the $1/m_b$ corrections and can be significantly reduced in the future. For the low dilepton invariant mass region, we confirm previous results up to small corrections.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:50:57 GMT" }, { "version": "v2", "created": "Mon, 19 May 2008 10:39:17 GMT" } ]
2008-11-26T00:00:00
[ [ "Huber", "Tobias", "", "Zurich U., Aachen Tech. Hochsch" ], [ "Hurth", "Tobias", "", "CERN,\n SLAC" ], [ "Lunghi", "Enrico", "", "Fermilab" ] ]
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712.301
Vladimir Pomerantsev
T.S. Jensen, V.P. Popov and V.N. Pomerantsev
Atomic Cascade in Muonic and Hadronic Hydrogen Atoms
9 pages, 11 figures
null
null
null
nucl-th
null
The atomic cascade in $\mu^- p$ and $\pi^- p$ atoms has been studied with the improved version of the extended cascade model in which new quantum mechanical calculations of the differential and integral cross sections of the elastic scattering, Stark transitions and Coulomb de-excitation have been included for the principal quantum number values $n\le 8$ and the relative energies $E \ge 0.01$ eV. The $X$-ray yields and kinetic energy distributions are compared with the experimental data.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 17:53:46 GMT" } ]
2007-12-19T00:00:00
[ [ "Jensen", "T. S.", "" ], [ "Popov", "V. P.", "" ], [ "Pomerantsev", "V. N.", "" ] ]
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712.3011
Denjoe O'Connor
Rodrigo Delgadillo-Blando, Denjoe O'Connor and Badis Ydri
Geometry in transition: A model of emergent geometry
6 pages, 4 figures
Phys.Rev.Lett.100:201601,2008
10.1103/PhysRevLett.100.201601
DIAS-preprint 07-22
hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study a three matrix model with global SO(3) symmetry containing at most quartic powers of the matrices. We find an exotic line of discontinuous transitions with a jump in the entropy, characteristic of a 1st order transition, yet with divergent critical fluctuations and a divergent specific heat with critical exponent $\alpha=1/2$. The low temperature phase is a geometrical one with gauge fields fluctuating on a round sphere. As the temperature increased the sphere evaporates in a transition to a pure matrix phase with no background geometrical structure. Both the geometry and gauge fields are determined dynamically. It is not difficult to invent higher dimensional models with essentially similar phenomenology. The model presents an appealing picture of a geometrical phase emerging as the system cools and suggests a scenario for the emergence of geometry in the early universe.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:52:47 GMT" }, { "version": "v2", "created": "Wed, 2 Jul 2008 19:38:05 GMT" } ]
2008-11-26T00:00:00
[ [ "Delgadillo-Blando", "Rodrigo", "" ], [ "O'Connor", "Denjoe", "" ], [ "Ydri", "Badis", "" ] ]
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712.3012
Nicholas Rattenbury
Nicholas J. Rattenbury, Shude Mao
OGLE-II High Proper Motion Stars towards the Galactic centre
7 figures and 4 tables, MNRAS, accepted
null
10.1111/j.1365-2966.2008.12878.x
null
astro-ph
null
The photometry data base of the second phase of the OGLE microlensing experiment, OGLE-II, is a rich source of information about the kinematics and structure of the Galaxy. In this work we use the OGLE-II proper motion catalogue to identify candidate stars which have high proper motions. 521 stars with proper motion mu > 50 mas/yr in the OGLE-II proper motion catalogue (Sumi 2004) were cross-identified with stars in the MACHO high proper motion catalogue, and the DENIS and 2MASS infra-red photometry catalogues. Photometric distances were computed for stars with colours consistent with G/K and M type stars. 6 stars were newly identified as possible nearby (< 50 pc) M dwarfs.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:02:06 GMT" } ]
2009-11-13T00:00:00
[ [ "Rattenbury", "Nicholas J.", "" ], [ "Mao", "Shude", "" ] ]
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712.3013
Eulogio Oset
E. Oset, L. S. Geng, D. Gamermann, M.J. Vicente Vacas, D. Strottman, K. P. Khemchandani, A. Martinez Torres, J. A. Oller and L. Roca
Recent Developments in Chiral Unitary Dynamics of Resonances
Talk at the International Conference on Hadron Physics, Troia07, Canakkale, Turkey, Sep. 2007 and at the Chiral Symmetry in Hadron and Nuclear Physics Workshop, Chiral07, Osaka, November 2007
Mod.Phys.Lett.A23:2201-2208,2008
10.1142/S0217732308029046
FTUV-07-1218, IFIC-07-1218
nucl-th
null
In this talk I summarize recent findings made on the description of axial vector mesons as dynamically generated states from the interaction of peseudoscalar mesons and vector mesons, dedicating some attention to the two $K_1(1270)$ states. Then I review the generation of open and hidden charm scalar and axial states. Finally, I present recent results showing that the low lying $1/2^+$ baryon resonances for S=-1 can be obtained as bound states or resonances of two mesons and one baryon in coupled channels dynamics.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:07:36 GMT" } ]
2008-11-26T00:00:00
[ [ "Oset", "E.", "" ], [ "Geng", "L. S.", "" ], [ "Gamermann", "D.", "" ], [ "Vacas", "M. J. Vicente", "" ], [ "Strottman", "D.", "" ], [ "Khemchandani", "K. P.", "" ], [ "Torres", "A. Martinez", "" ], [ "Oller", "J. A.", "" ], [ "Roca", "L.", "" ] ]
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712.3014
Gavin Salam
Mrinal Dasgupta, Lorenzo Magnea and Gavin P. Salam
Non-perturbative QCD effects in jets at hadron colliders
33 pages, 7 figures
JHEP 0802:055,2008
10.1088/1126-6708/2008/02/055
null
hep-ph
null
We discuss non-perturbative QCD contributions to jet observables, computing their dependence on the jet radius R, and on the colour and transverse momentum of the parton initiating the jet. We show, using analytic QCD models of power corrections as well as Monte Carlo simulations, that hadronisation corrections grow at small values of R, behaving as 1/R, while underlying event contributions grow with the jet area as R^2. We highlight the connection between hadronisation corrections to jets and those for event shapes in e^+e^- and DIS; we note the limited dependence of our results on the choice of jet algorithm; finally, we propose several measurements in the context of which to test or implement our predictions. The results presented here reinforce the motivation for the use of a range of R values, as well as a plurality of infrared-safe jet algorithms, in precision jet studies at hadron colliders.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:32:17 GMT" } ]
2009-04-30T00:00:00
[ [ "Dasgupta", "Mrinal", "" ], [ "Magnea", "Lorenzo", "" ], [ "Salam", "Gavin P.", "" ] ]
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712.3015
Bobby Ramsey Jr
Bobby W. Ramsey
A Spectral sequence for polynomially bounded cohomology
20 pages, no figures
null
10.1016/j.jpaa.2012.10.001
null
math.KT math.GR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We construct an analogue of the Lyndon-Hochschild-Serre spectral sequence in the context of polynomial cohomology, for group extensions. If G is an extension of Q by H, then the spectral sequence converges to the polynomial cohomology of G. For the polynomial extensions of Noskov with normal subgroup isocohomological, the E_2 term is the polynomial cohomology of Q with coefficients in the polynomial cohomology of H. When both Q and H are isocohomological G must be as well. By referencing results of Connes-Moscovici and Noskov, if Q and H are both isocohomological and have the Rapid Decay property of Jolissaint, then G satisfies the Novikov Conjecture.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:10:08 GMT" }, { "version": "v2", "created": "Wed, 26 Sep 2012 17:02:11 GMT" } ]
2012-12-12T00:00:00
[ [ "Ramsey", "Bobby W.", "" ] ]
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712.3016
Stefan Legel
Stefan Legel, J\"urgen K\"onig, Gerd Sch\"on
Generation and detection of a spin entanglement in nonequilibrium quantum dots
6 pages, 3 figures
New. J. Phys. 10 (2008) 045016
10.1088/1367-2630/10/4/045016
null
cond-mat.mes-hall
null
Spin entanglement between two spatially separated electrons can be generated in nonequilibrium interacting quantum dots, coherently coupled to a common lead. In this system entangled two-electron states develop which are Werner states with an imbalance between singlet and triplet probabilities. We propose a multi-terminal, multiply-connected setup for the generation and detection of this imbalance. In particular, we identify a regime in which the formation of spin entanglement leads to a cancellation of Aharonov-Bohm oscillations.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:16:51 GMT" }, { "version": "v2", "created": "Fri, 2 May 2008 14:21:17 GMT" } ]
2009-11-13T00:00:00
[ [ "Legel", "Stefan", "" ], [ "König", "Jürgen", "" ], [ "Schön", "Gerd", "" ] ]
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712.3017
Marco Miceli
M. Miceli, F. Bocchino, F. Reale
Physical and chemical inhomogeneities inside the Vela SNR shell. Indications of ejecta shrapnels
Accepted for publication in The Astrophysical Journal. For the version of the paper with high resolution images, please see http://www.astropa.unipa.it/Library/preprint.html
null
10.1086/528737
null
astro-ph
null
We present the results of the combined analysis of three XMM-Newton EPIC observations of the northern rim of the Vela SNR. The three pointings cover an area of ~10 pc^2 (at 250 pc) behind the main shock front and we aim at studying with high resolution the spatial distribution of the physical and chemical properties of the X-ray emitting plasma on this large scale. We produce count-rate images and equivalent width maps of the Ne IX and Mg XI emission blends. We also perform a spatially resolved spectral analysis of a set of physically homogeneous regions. We reveal physical and chemical inhomogeneities in the X-ray emitting plasma. In particular, we find large variations of the O, Ne, Mg, and Fe abundances. In some bright knots we also find unexpectedly enhanced Ne and Mg abundances, with values significantly larger than solar. Our results support a possible association of a few X-ray emitting knots with previously undetected residuals of stellar fragments (i. e. shrapnels) observed, in projection, inside the Vela shell.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:21:23 GMT" } ]
2009-11-13T00:00:00
[ [ "Miceli", "M.", "" ], [ "Bocchino", "F.", "" ], [ "Reale", "F.", "" ] ]
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712.3018
Julien Dub\'edat
Julien Dubedat
SLE and the free field: Partition functions and couplings
55 pages, 4 figures. v2: additional material
null
null
null
math.PR
null
Schramm-Loewner Evolutions ($\SLE$) are random curves in planar simply connected domains; the massless (Euclidean) free field in such a domain is a random distribution. Both have conformal invariance properties in law. In the present article, some relations between the two objects are studied. We establish identities of partition functions between different versions of $\SLE$ and the free field with appropriate boundary conditions; this involves $\zeta$-regularization and the Polyakov-Alvarez conformal anomaly formula. We proceed with a construction of couplings of $\SLE$ with the free field, showing that, in a precise sense, chordal $\SLE$ is the solution of a stochastic "differential" equation driven by the free field. Existence, uniqueness in law, and pathwise uniqueness for these SDEs are proved for general $\kappa>0$.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:30:12 GMT" }, { "version": "v2", "created": "Fri, 25 Jan 2008 17:53:45 GMT" } ]
2011-11-10T00:00:00
[ [ "Dubedat", "Julien", "" ] ]
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712.3019
Ariel Yadin
Ariel Yadin
When Do Random Subsets Decompose a Finite Group?
null
null
null
null
math.PR math.GR
null
Let A,B be two random subsets of a finite group G. We consider the event that the products of elements from A and B span the whole group; i.e. (AB union BA) = G. The study of this event gives rise to a group invariant we call \Theta(G). \Theta(G) is between 1/2 and 1, and is 1 if and only if the group is abelian. We show that a phase transition occurs as the size of A and B passes \sqrt{\Theta(G)|G|\log|G|}; i.e. for any c>0, if the size of A and B is less than (1-c)\sqrt{\Theta(G)|G|\log|G|}, then with high probability (AB union BA) does not equal G. If A and B are larger than (1+c)\sqrt{\Theta(G)|G|\log|G|} then (AB union BA) equals G with high probability.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:41:36 GMT" } ]
2007-12-19T00:00:00
[ [ "Yadin", "Ariel", "" ] ]
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712.302
Leonid Mirny
Carlos Gomez-Uribe, George C. Verghese, and Leonid A. Mirny
Operating Regimes of Signaling Cycles: Statics, Dynamics, and Noise Filtering
to appear in PLoS Computational Biology
null
10.1371/journal.pcbi.0030246
null
q-bio.MN q-bio.BM q-bio.QM q-bio.SC
null
A ubiquitous building block of signaling pathways is a cycle of covalent modification (e.g., phosphorylation and dephosphorylation in MAPK cascades). Our paper explores the kind of information processing and filtering that can be accomplished by this simple biochemical circuit. Signaling cycles are particularly known for exhibiting a highly sigmoidal (ultrasensitive) input-output characteristic in a certain steady-state regime. Here we systematically study the cycle's steady-state behavior and its response to time-varying stimuli. We demonstrate that the cycle can actually operate in four different regimes, each with its specific input-output characteristics. These results are obtained using the total quasi-steady-state approximation, which is more generally valid than the typically used Michaelis-Menten approximation for enzymatic reactions. We invoke experimental data that suggests the possibility of signaling cycles operating in one of the new regimes. We then consider the cycle's dynamic behavior, which has so far been relatively neglected. We demonstrate that the intrinsic architecture of the cycles makes them act - in all four regimes - as tunable low-pass filters, filtering out high-frequency fluctuations or noise in signals and environmental cues. Moreover, the cutoff frequency can be adjusted by the cell. Numerical simulations show that our analytical results hold well even for noise of large amplitude. We suggest that noise filtering and tunability make signaling cycles versatile components of more elaborate cell signaling pathways.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:43:43 GMT" } ]
2015-05-13T00:00:00
[ [ "Gomez-Uribe", "Carlos", "" ], [ "Verghese", "George C.", "" ], [ "Mirny", "Leonid A.", "" ] ]
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712.3021
Camille Laurent-Gengoux
Yvette Kosmann-Schwarzbach, Camille Laurent-Gengoux, Alan Weinstein
Modular classes of Lie algebroid morphisms
33 pages. Dedicated to Bertram Kostant for his eightieth birthday. Minor changes in version 2: Proposition 3.11 added, typos corected
null
null
null
math.DG math.SG
null
We study the behavior of the modular class of a Lie algebroid under general Lie algebroid morphisms by introducing the relative modular class. We investigate the modular classes of pull-back morphisms and of base-preserving morphisms associated to Lie algebroid extensions. We also define generalized morphisms, including Morita equivalences, that act on the 1-cohomology, and observe that the relative modular class is a coboundary on the category of Lie algebroids and generalized morphisms with values in the 1-cohomology.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:50:04 GMT" }, { "version": "v2", "created": "Fri, 18 Apr 2008 15:15:32 GMT" } ]
2008-04-18T00:00:00
[ [ "Kosmann-Schwarzbach", "Yvette", "" ], [ "Laurent-Gengoux", "Camille", "" ], [ "Weinstein", "Alan", "" ] ]
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712.3022
Mike McCulloch
M.E. McCulloch
Can the flyby anomalies be explained by a modification of inertia?
Presented at a BIS symposium on 15/11/2007, and submitted to JBIS. 13 pages, 4 figures
J.Br.Interplanet.Soc. 61: 373-378, 2008
null
null
astro-ph physics.gen-ph
null
The flyby anomalies are unexplained velocity increases of 3.9, 13.5, 0.1 and 1.8 mm/s observed near closest approach during the Earth flybys of the Galileo, NEAR, Cassini and Rosetta spacecraft. Here, these flybys are modelled using a theory that assumes that inertia is caused by a form of Unruh radiation, modified by a Hubble-scale Casimir effect. This theory predicts that when the craft's accelerations relative to the galactic centre approached zero near closest approach, their inertial masses reduced for about 10^-7 s causing Earthward jumps of 2.6, 1.2, 1.4 and 1.9 mm/s respectively, and, to conserve angular momentum, increases in orbital velocity of a few mm/s that, except NEAR's, were quite close to those observed. However, these results were extremely sensitive to the Hubble constant used. As an experimental test of these ideas, it is proposed that metamaterials could be used to bend Unruh radiation around objects, possibly reducing their inertial mass.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 18:54:30 GMT" } ]
2011-09-15T00:00:00
[ [ "McCulloch", "M. E.", "" ] ]
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712.3023
Neil Dobbs
Neil Dobbs
Renormalisation-induced phase transitions for unimodal maps
14 pages, 2 figures. Revised following comments of referees. First page is blank
Commun. Math. Phys. 286, 377\^a?"387 (2009)
10.1007/s00220-008-0656-5
null
math.DS
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The thermodynamical formalism is studied for renormalisable maps of the interval and the natural potential $-t \log|Df|$. Multiple and indeed infinitely many phase transitions at positive $t$ can occur for some quadratic maps. All unimodal quadratic maps with positive topological entropy exhibit a phase transition in the negative spectrum.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:02:42 GMT" }, { "version": "v2", "created": "Thu, 10 Jul 2008 14:22:27 GMT" } ]
2009-02-18T00:00:00
[ [ "Dobbs", "Neil", "" ] ]
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712.3024
K. C. Steenbrugge
K. C. Steenbrugge, K. M. Blundell, P. Duffy
Detection of a relic X-ray jet in Cygnus A
4 pages. Proceedings of "High Energy Phenomena in Relativistic Outflows", held in Dublin, Ireland, September 24-28, 2007
Int.J.Mod.Phys.D17:1561-1567,2008
10.1142/S0218271808013157
null
astro-ph
null
We present a 200 ks Chandra ACIS-I image of Cygnus A, and discuss a long linear feature seen in its counterlobe. This feature has a non-thermal spectrum and lies on the line connecting the brighter hotspot on the approaching side and the nucleus. We therefore conclude that this feature is (or was) a jet. However, the outer part of this X-ray jet does not trace the current counterjet observed in radio. No X-ray counterpart is observed on the jet side. Using light-travel time effects we conclude that this X-ray 50 kpc linear feature is a relic jet that contains enough low-energy plasma (gamma ~ 10^3) to inverse-Compton scatter cosmic microwave background photons, producing emission in the X-rays.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:33:55 GMT" } ]
2009-06-23T00:00:00
[ [ "Steenbrugge", "K. C.", "" ], [ "Blundell", "K. M.", "" ], [ "Duffy", "P.", "" ] ]
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712.3025
Mihail Chizhov
Mihail V. Chizhov
Can we use hadronic tau decay for V_us determination
17 pages, 5 figures
null
null
null
hep-ph hep-ex hep-lat
null
It is known that the discrepancy in pion spectral functions extracted from positron-electron annihilation and tau decay leads to different predictions for the muon anomalous magnetic moment. We will show that this discrepancy effects also the extraction of the Cabibbo angle from the hadronic tau decays. The corrections to the tau branching fractions, corresponding to the presence of new centi-weak tensor interactions, allow us to extract the Cabibbo angle from tau decays in agreement with its other precision determinations. Thus a more precise value of |V_us|=0.2246 +/- 0.0012 is obtained and as a consequence f(0)=0.9645 +/- 0.0055 and F_K/F_pi=1.196 +/- 0.007.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:12:54 GMT" } ]
2008-01-30T00:00:00
[ [ "Chizhov", "Mihail V.", "" ] ]
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712.3026
Elena Rubei
Elena Rubei
Sets of double and triple weights of trees
11 pages, to appear in Annals of Combinatorics
null
null
null
math.AG math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let T be a weighted tree with n leaves. Let D_{i,j} be the distance between the leaves i and j. Let D_{i,j,k}= (D_{i,j} + D_{j,k} +D_{i,k})/2. We will call such numbers "triple weights" of the tree. In this paper, we give a characterization, different from the previous ones, for sets indexed by 2-subsets of a $n$-set to be double weights of a tree. By using the same ideas,we find also necessary and sufficient conditions for a set of real numbers indexed by 3-subsets of an $n$-set to be the set of the triple weights of a tree with $n$ leaves. Besides we propose a slight modification of Saitou-Nei's Neighbour-Joining algorithm to reconstruct trees from the data D_{i,j}.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:18:36 GMT" }, { "version": "v2", "created": "Tue, 9 Jun 2009 17:42:44 GMT" }, { "version": "v3", "created": "Fri, 22 Apr 2011 11:54:03 GMT" } ]
2011-04-25T00:00:00
[ [ "Rubei", "Elena", "" ] ]
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712.3027
Pawel Sobkowicz
Pawel Sobkowicz
Simple queueing approach to segregation dynamics in Schelling model
null
null
null
null
cond-mat.dis-nn physics.soc-ph
null
A simple queueing approach for segregation of agents in modified one dimensional Schelling segregation model is presented. The goal is to arrive at simple formula for the number of unhappy agents remaining after the segregation.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:20:26 GMT" } ]
2007-12-19T00:00:00
[ [ "Sobkowicz", "Pawel", "" ] ]
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712.3028
Licia Verde
Licia Verde (ICREA and Institute of Space Sciences, IEEC-CSIC)
A practical guide to Basic Statistical Techniques for Data Analysis in Cosmology
To appear in the proceedings of the XIX Canary Island Winter School "The Cosmic Microwave Background: from Quantum fluctuations to the present Universe", comments welcome. (fixed entry of table1)
null
null
null
astro-ph
null
This is the summary of 4 Lectures given at the XIX Canary islands winter school of Astrophysics ''The Cosmic Microwave Background, from Quantum Fluctuations to the present Universe''. Lectures were intended for master/beginning PhD students in cosmology.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:30:58 GMT" }, { "version": "v2", "created": "Mon, 7 Jan 2008 11:00:58 GMT" } ]
2008-01-07T00:00:00
[ [ "Verde", "Licia", "", "ICREA and Institute of Space Sciences, IEEC-CSIC" ] ]
[ 0.028422948, 0.0363803804, -0.0691799149, -0.097975865, -0.1108072251, -0.0844979659, 0.0142363412, 0.0149450498, -0.0242577307, 0.0040533165, -0.007248722, 0.0581887141, -0.1231412441, -0.0248172376, 0.1318944097, 0.129507184, -0.0871836022, 0.1179689094, 0.0664942786, 0.0826080814, 0.0291689578, -0.0752474591, 0.0572437681, 0.040582899, -0.0344158895, -0.1347789913, 0.0579897761, 0.0625155643, 0.0709703341, -0.0575421713, 0.0913115218, -0.0385935381, -0.0746009126, -0.03406775, -0.0181528889, 0.0736062378, 0.0020204415, 0.0167852063, -0.0207514875, -0.0636097118, 0.0025317685, -0.1083205268, 0.0042491439, 0.0362063088, -0.0109352507, -0.0980753377, 0.0290446226, -0.0058965804, 0.0099592218, -0.0367533825, -0.0437410027, -0.0224300083, 0.060725145, -0.0365047157, -0.0329984725, -0.0660466775, -0.0674889609, 0.0393395498, -0.0061701173, -0.0759437308, -0.0065337969, 0.0351370312, 0.0397871546, 0.0436166674, -0.0741533116, 0.0738549083, 0.0595315285, 0.0352862328, 0.0044915965, 0.0646541268, 0.00272915, 0.0296414308, -0.0856418461, 0.0388173424, 0.0430695936, 0.0316805206, -0.0620182268, -0.0343412869, -0.0529666506, -0.0396130867, 0.0074290079, 0.1133933887, 0.035584636, -0.0358084403, -0.0174068809, -0.0522206388, 0.0306609757, 0.0456060246, -0.0427214578, 0.0428955257, 0.0033259573, -0.0810663253, -0.0620182268, 0.0105062956, 0.1796389967, -0.0732083619, 0.0713184774, -0.0430695936, 0.063908115, -0.0729596913, 0.0264335908, 0.061570622, 0.0509772897, -0.0126448553, 0.1172726378, -0.0611230172, -0.041229438, -0.1335853636, -0.0969811901, 0.0451335534, -0.0842493027, 0.0317799896, 0.0805689842, 0.0603770055, -0.0438404717, 0.0204530843, -0.0641567856, -0.0928532705, -0.0709703341, -0.0487392657, -0.1015069783, -0.0067016487, 0.064753592, 0.0139752375, 0.0281494111, -0.1429353505, 0.1040434092, -0.0509275571, 0.0145347444, -0.0139255039, 0.0790769681, -0.0213980284, 0.0219451021, -0.0679863021, 0.0292932931, 0.0114698904, 0.0352116302, 0.0359079055, 0.0508280881, -0.0071927714, 0.1421396136, 0.0392898135, 0.081812337, -0.000149299, 0.0410305038, -0.0428706594, -0.0725618228, 0.0743025094, 0.0708708689, -0.0441388749, -0.019483272, -0.0481921919, -0.0778833553, -0.0351867639, -0.0120666977, -0.0969811901, 0.0039600651, -0.0152061526, 0.0012985221, -0.1264236867, 0.0243944991, -0.0467499048, -0.0303874388, -0.0146342125, -0.0199806113, -0.0177425835, -0.0704730004, -0.013080027, -0.1090168059, 0.0104068276, -0.0392649472, -0.0419505797, 0.0986224115, -0.0606256761, -0.0402844921, 0.0317799896, -0.0311831813, -0.1067290381, 0.0008361519, -0.0173447132, -0.0380713344, 0.0436166674, -0.0166733041, -0.0930024758, 0.0601283386, 0.0179663859, -0.0040937252, 0.0299647003, 0.044511877, -0.0034658341, -0.0807181895, -0.0413786396, -0.0326751992, 0.1576565951, -0.0063908119, 0.0006562549, 0.005508034, -0.042174384, -0.0124832196, 0.0732083619, -0.0280002095, 0.031630788, 0.0173820127, -0.0368031189, 0.052817449, -0.0956881046, 0.07773415, 0.0163997672, -0.126523152, -0.0485900603, 0.0298652332, -0.0355349034, 0.0115569253, 0.0094556659, -0.1803352833, 0.0300144348, -0.0938976854, 0.0489879325, 0.0316805206, 0.258218646, -0.0460536294, 0.0557020158, 0.0785298944, 0.0416273102, 0.0467747748, -0.0204903837, 0.1035460681, -0.0806684569, 0.0520714372, -0.0495598726, 0.0259113833, 0.0331725404, -0.0602278039, 0.1074253172, -0.0123091508, -0.0707714036, -0.0628139675, 0.0304620396, -0.0922067314, -0.0000873258, -0.0248048045, 0.0499328785, 0.0226289444, -0.0272790678, -0.0654996037, -0.0231387168, -0.0257621817, -0.028049944, -0.0223927069, 0.0513254292, 0.0887750909, 0.0093251141, 0.029268425, -0.0365793146, 0.0253021438, -0.0051661134 ]
712.3029
Marcin Bilski
Marcin Bilski
Approximation of sets defined by polynomials with holomorphic coefficients
10 pages
null
null
null
math.CV
null
Let X be an analytic set defined by polynomials whose coefficients a_1,...,a_s are holomorphic functions. We formulate conditions such that for all sequences {a_(1,n)},...,{a_(s,n)} of holomorphic functions converging locally uniformly to a_1,...,a_s respectively the following holds true. If a_(1,n),...,a_(s,n) satisfy the conditions then the sequence of the sets {X_n} obtained by replacing a_j by a_(j,n) in the polynomials, converge to X.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:24:20 GMT" } ]
2007-12-19T00:00:00
[ [ "Bilski", "Marcin", "" ] ]
[ -0.026501473, 0.0031399454, -0.0629437864, -0.0234033205, -0.0542957038, -0.0618739203, 0.0215533432, -0.0689172074, 0.0850543529, 0.0604920089, 0.0827363059, -0.0901807919, -0.0445108861, -0.0562125444, -0.002566007, 0.1059167385, -0.0391615555, 0.0313827358, 0.0588426329, 0.011980271, 0.0370218232, -0.009088289, -0.0242057201, -0.0068761185, 0.0719039142, -0.1064516753, 0.0263677407, 0.0774315521, 0.1150997579, -0.0012823069, -0.0175079126, -0.0024893889, -0.000635233, -0.0980710536, -0.1400633007, 0.1236586869, -0.0612944104, 0.1079673171, 0.0349266678, 0.0549643673, -0.0775207132, 0.0270364061, -0.0727508888, 0.0354393125, 0.1233020648, 0.019770233, 0.0711906701, -0.0588426329, -0.0281062722, 0.0815327093, -0.0729292035, 0.11545638, -0.010743238, -0.0433072858, 0.0569703653, 0.05193308, -0.0418585092, 0.0437753536, 0.0648160502, -0.0594667196, 0.0665100068, -0.1211623326, 0.0039534895, 0.0179425459, -0.0628100559, 0.0451572612, 0.0269026738, -0.0550089478, 0.0268358067, 0.0921867937, -0.116169624, 0.0399193764, 0.0107933879, 0.0627208948, -0.0644148514, 0.071591869, 0.0758267567, 0.0243617408, 0.0069095516, 0.0221105646, 0.0349935368, -0.0097012334, 0.0714135617, 0.030156849, 0.0307363607, -0.0785014182, -0.0029198427, 0.103955321, -0.1307911277, 0.0859013274, -0.0181431454, 0.0292875823, 0.0046945945, 0.0079905624, 0.1736749262, -0.0559896566, 0.0854109749, 0.031694781, 0.0149781248, 0.007851257, 0.0355061777, -0.0012412118, 0.1176852658, -0.0943265259, 0.1920409501, 0.1175069511, -0.0645931661, 0.04319584, -0.0588872097, 0.0014863894, 0.0354838893, -0.0359742455, -0.047698196, -0.0713244006, 0.0258996747, 0.0093000336, -0.06597507, 0.019357888, -0.076361686, 0.0776098669, 0.0539836586, 0.0601353869, 0.0704774261, -0.0213304535, 0.0501053929, -0.0396742001, 0.0207620878, 0.0540728122, -0.017886823, -0.0668666288, 0.0538499244, -0.0750689358, -0.0072215958, -0.0162708797, -0.0493029952, -0.0177976675, -0.0092554558, 0.0223111641, 0.0937915891, 0.0527354814, 0.0467620604, 0.0623196959, 0.0959313214, 0.0212970208, -0.0244063195, 0.0084140506, -0.0262785852, -0.0079961345, -0.0231804308, 0.0060291411, 0.0505957492, -0.0185443442, 0.0633449852, 0.0850989297, -0.0089378394, -0.0768966228, -0.063166678, -0.0084697725, -0.0278833844, 0.0391838439, -0.0621859655, 0.1062733606, 0.0207397994, 0.0208066665, 0.1339115649, 0.0149781248, 0.0377573557, 0.0035996535, -0.0047280276, -0.2013131231, -0.045625329, -0.0495704599, 0.0186112113, 0.0004193095, 0.0212301537, -0.0163711794, -0.0499716587, -0.124371931, -0.1085022464, 0.0704774261, 0.0176527891, 0.0885314122, -0.0375344679, -0.045625329, 0.0871940851, 0.0054552024, -0.0185332, 0.0258105192, 0.0900916383, -0.0548752137, -0.0448675081, -0.0629883632, 0.0405211784, 0.1593208909, 0.0337007791, -0.149781242, 0.0199039672, 0.0336784907, 0.0349712446, 0.0566583239, 0.0165049136, -0.0601799637, -0.0071825902, 0.0852326602, -0.065350987, 0.0380694009, 0.0167278014, -0.0052016666, -0.0895121247, 0.0287749395, -0.0521559715, -0.0606257431, 0.0304911826, 0.0141757252, 0.0418362208, 0.065618448, -0.0606257431, 0.0845639929, 0.0308923814, 0.1685038954, -0.0052295276, 0.0724388435, 0.014933547, 0.0395404659, 0.0050289277, 0.0008713558, 0.0791700855, 0.0320514031, 0.048812639, -0.0190904215, 0.0458259284, 0.0415018871, -0.0275713392, -0.0429952405, 0.0322520025, -0.0347929336, -0.0273484513, -0.0425494649, -0.0773869753, -0.0898687467, -0.0356622003, 0.1013698056, -0.0594667196, -0.0259442516, 0.028685784, -0.0105537828, -0.0410338193, 0.0239605419, -0.0992300734, -0.0600908101, -0.0756484419, -0.0204054657, 0.0124929147, 0.076005064, -0.0152790248, -0.0303574484 ]
712.303
Janusz Skalski
J. Skalski
Nuclear fission with mean-field instantons
null
Phys.Rev.C77:064610,2008
10.1103/PhysRevC.77.064610
null
nucl-th
null
We present a description of nuclear spontaneous fission, and generally of quantum tunneling, in terms of instantons - periodic imaginary-time solutions to time-dependent mean-field equations - that allows for a comparison with more familiar and used generator coordinate (GCM) and adiabatic time-dependent Hartree-Fock (ATDHF) methods. It is shown that the action functional whose value for the instanton is the quasiclassical estimate of the decay exponent fulfils the minimum principle when additional constraints are imposed on trial fission paths. In analogy with mechanics, these are conditions of energy conservation and the velocity-momentum relations. In the adiabatic limit the instanton method reduces to the time-odd ATDHF equation, with collective mass including the time-odd Thouless-Valatin term, while the GCM mass completely ignores velocity-momentum relations. This implies that GCM inertia generally overestimates instanton-related decay rate. The very existence of the minimum principle offers a hope for a variational search for instantons. After the inclusion of pairing, the instanton equations and the variational principle can be expressed in terms of the imaginary-time-dependent Hartree-Fock- Bogolyubov (TDHFB) theory. The adiabatic limit of this theory reproduces ATDHFB inertia.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:30:31 GMT" }, { "version": "v2", "created": "Fri, 16 May 2008 15:41:01 GMT" } ]
2008-11-26T00:00:00
[ [ "Skalski", "J.", "" ] ]
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712.3031
Elena Rubei
Elena Rubei
Stability of homogeneous bundles on P^3
to appear in Geometriae Dedicata http://www.springer.com/mathematics/geometry/journal/10711
null
10.1007/s10711-011-9617-9
null
math.AG math.RT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the stability of some homogeneous bundles on P^3 by using their representations of the quiver associated to the homgeneous bundles on P^3. In particular we show that homogeneous bundles on P^3 whose support of the quiver representation is a parallelepiped are stable, for instance the bundles E whose minimal free resolution is of the kind 0 --> S^{l_1, l_2, l_3} V (t) --> S^{l_1 +s, l_2, l_3} V (t+s) --> E --> 0 are stable.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:36:00 GMT" }, { "version": "v2", "created": "Mon, 2 May 2011 14:23:31 GMT" } ]
2011-05-03T00:00:00
[ [ "Rubei", "Elena", "" ] ]
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712.3032
Mauricio Bellini
Federico Agustin Membiela (Mar del Plata University & CONICET), Mauricio Bellini (Mar del Plata University & CONICET)
Power spectrum of large-scale magnetic fields from Gravitoelectromagnetic inflation with a decaying cosmological parameter
7 pages, no figures
null
null
null
hep-th
null
Introducing a variable cosmological parameter $\Lambda (t)$ in a geometrical manner from a 5D Riemann-flat metric, we investigate the origin and evolution of primordial magnetic fields in the early universe, when the expansion is governed by a cosmological parameter $\Lambda (t)$ that decreases with time. Using the gravitoelectromagnetic inflationary formalism, but without the Feynman gauge, we obtain the power of spectrums for large-scale magnetic fields and the inflaton field fluctuations during inflation. A very important fact is that our formalism is {\em naturally non-conformally invariant}.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:42:55 GMT" } ]
2007-12-19T00:00:00
[ [ "Membiela", "Federico Agustin", "", "Mar del Plata University & CONICET" ], [ "Bellini", "Mauricio", "", "Mar del Plata University & CONICET" ] ]
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712.3033
Brant M. Johnson
PHENIX Collaboration, S. Afanasiev, et al
Particle-species dependent modification of jet-induced correlations in Au+Au collisions at sqrt(s_NN) = 200 GeV
344 authors, 4 pages text, RevTeX, 4 figures. Submitted to Physical Review Letters. Plain text data tables for the points plotted in figures for this and previous PHENIX publications are (or will be) publicly available at http://www.phenix.bnl.gov/papers.html
Phys.Rev.Lett.101:082301,2008
10.1103/PhysRevLett.101.082301
null
nucl-ex
null
We report PHENIX measurements of the correlation of a trigger hadron at intermediate transverse momentum (2.5<p_{T,trig}<4 GeV/c), with associated mesons or baryons at lower p_{T,assoc}, in Au+Au collisions at sqrt(s_NN) = 200 GeV. The jet correlations for both baryons and mesons show similar shape alterations as a function of centrality, characteristic of strong modification of the away-side jet. The ratio of jet-associated baryons to mesons for this jet increases with centrality and p_{T,assoc} and, in the most central collisions, reaches a value similar to that for inclusive measurements. This trend is incompatible with in-vacuum fragmentation, but could be due to jet-like contributions from correlated soft partons which recombine upon hadronization.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:39:34 GMT" } ]
2008-11-26T00:00:00
[ [ "PHENIX Collaboration", "", "" ], [ "Afanasiev", "S.", "" ] ]
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712.3034
Noah Graham
E. Farhi, N. Graham, A. H. Guth, N. Iqbal, R. R. Rosales, N. Stamatopoulos
Emergence of Oscillons in an Expanding Background
13 pages, 4 .eps figures, uses RevTeX4; v2: clarified details of expansion, added references
Phys.Rev.D77:085019,2008
10.1103/PhysRevD.77.085019
MIT-CTP 3924
hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider a (1+1) dimensional scalar field theory that supports oscillons, which are localized, oscillatory, stable solutions to nonlinear equations of motion. We study this theory in an expanding background and show that oscillons now lose energy, but at a rate that is exponentially small when the expansion rate is slow. We also show numerically that a universe that starts with (almost) thermal initial conditions will cool to a final state where a significant fraction of the energy of the universe -- on the order of 50% -- is stored in oscillons. If this phenomenon persists in realistic models, oscillons may have cosmological consequences.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:48:31 GMT" }, { "version": "v2", "created": "Wed, 11 Jun 2008 23:33:52 GMT" } ]
2008-11-26T00:00:00
[ [ "Farhi", "E.", "" ], [ "Graham", "N.", "" ], [ "Guth", "A. H.", "" ], [ "Iqbal", "N.", "" ], [ "Rosales", "R. R.", "" ], [ "Stamatopoulos", "N.", "" ] ]
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712.3035
Russell Lyons
Russell Lyons
Identities and Inequalities for Tree Entropy
12 pages; revision contains more background
Combin. Probab. Comput. 19, no. 2 (2010), 303-313.
null
null
math.CO math.PR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The notion of tree entropy was introduced by the author as a normalized limit of the number of spanning trees in finite graphs, but is defined on random infinite rooted graphs. We give some new expressions for tree entropy; one uses Fuglede-Kadison determinants, while another uses effective resistance. We use the latter to prove that tree entropy respects stochastic domination. We also prove that tree entropy is non-negative in the unweighted case, a special case of which establishes Lueck's Determinant Conjecture for Cayley-graph Laplacians. We use techniques from the theory of operators affiliated to von Neumann algebras.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:00:21 GMT" }, { "version": "v2", "created": "Sun, 9 Aug 2009 19:08:12 GMT" } ]
2010-04-27T00:00:00
[ [ "Lyons", "Russell", "" ] ]
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712.3036
Biagio Lucini
Luigi Del Debbio, Biagio Lucini, Agostino Patella and Claudio Pica
Quenched mesonic spectrum at large N
Reference added; typos corrected; version to appear on JHEP
JHEP 0803:062,2008
10.1088/1126-6708/2008/03/062
BNL-NT-07/56, IFUP-TH/2007-36, NI07089
hep-th hep-lat hep-ph
null
We compute the masses of the $\pi$ and of the $\rho$ mesons in the quenched approximation on a lattice with fixed lattice spacing $a \simeq 0.145 \ \mathrm{fm}$ for SU($N$) gauge theory with $N = 2,3,4,6$. We find that a simple linear expression in $1/N^2$ correctly captures the features of the lowest-lying meson states at those values of $N$. This enables us to extrapolate to $N = \infty$ the behaviour of $m_{\pi}$ as a function of the quark mass and of $m_{\rho}$ as a function of $m_{\pi}$. Our results for the latter agree within 5% with recent predictions obtained in the AdS/CFT framework.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:06:19 GMT" }, { "version": "v2", "created": "Sun, 16 Mar 2008 23:07:40 GMT" } ]
2009-12-10T00:00:00
[ [ "Del Debbio", "Luigi", "" ], [ "Lucini", "Biagio", "" ], [ "Patella", "Agostino", "" ], [ "Pica", "Claudio", "" ] ]
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712.3037
Manik Lal Das
Manik Lal Das
Comments on "Improved Efficient Remote User Authentication Schemes"
null
International Journal of Network Security, Vol. 6, No. 3, pp. 282-284, 2008
null
null
cs.CR
null
Recently, Tian et al presented an article, in which they discussed some security weaknesses of Yoon et al's scheme and subsequently proposed two ``improved'' schemes. In this paper, we show that the Tian et al's schemes are insecure and vulnerable than the Yoon et al's scheme.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:26:39 GMT" } ]
2007-12-19T00:00:00
[ [ "Das", "Manik Lal", "" ] ]
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712.3038
Matthew Johnson
Anthony Aguirre, Matthew C Johnson
Towards observable signatures of other bubble universes II: Exact solutions for thin-wall bubble collisions
18 PRD-style pages, 12 figures. Added appendix on the expected number of collisions, added references, minor correction to Appendix C, conclusions unchanged. Replaced to match published version
Phys.Rev.D77:123536,2008
10.1103/PhysRevD.77.123536
null
hep-th astro-ph gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We assess the effects of a collision between two vacuum bubbles in the thin-wall limit. After describing the outcome of a generic collision possessing the expected hyperbolic symmetry, we focus on collisions experienced by a bubble containing positive vacuum energy, which could in principle contain our observable universe. We provide criteria governing whether the post-collision domain wall accelerates towards or away from this "observation" bubble, and discuss the implications for observers located at various positions inside of the bubble. Then, we identify the class of solutions which have minimal impact on the interior of the observation bubble, and derive a simple formula for the energy density of a shell of radiation emitted from such a collision. In the context of a universe undergoing false vacuum eternal inflation, these solutions are perhaps the most promising candidates for collisions that could exist within our past light cone, and therefore in principle be observable.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:47:15 GMT" }, { "version": "v2", "created": "Fri, 25 Jan 2008 19:02:54 GMT" }, { "version": "v3", "created": "Mon, 28 Jan 2008 20:03:34 GMT" }, { "version": "v4", "created": "Tue, 22 Jul 2008 21:06:26 GMT" } ]
2008-11-26T00:00:00
[ [ "Aguirre", "Anthony", "" ], [ "Johnson", "Matthew C", "" ] ]
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712.3039
Peter Wong
Marek Golasinski, Daciberg Goncalves, Peter Wong
A note on generalized equivariant homotopy groups
9 pages, submitted to Proceedings for Postnikov Memorial Conference
Algebraic topology--old and new, 179--185, Banach Center Publ., 85, Polish Acad. Sci. Inst. Math., Warsaw, 2009
null
null
math.AT
null
In this paper, we generalize the equivariant homotopy groups or equivalently the Rhodes groups. We establish a short exact sequence relating the generalized Rhodes groups and the generalized Fox homotopy groups and we introduce $\Gamma$-Rhodes groups, where $\Gamma$ admits a certain co-grouplike structure. Evaluation subgroups of $\Gamma$-Rhodes groups are discussed.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:31:57 GMT" } ]
2011-05-11T00:00:00
[ [ "Golasinski", "Marek", "" ], [ "Goncalves", "Daciberg", "" ], [ "Wong", "Peter", "" ] ]
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712.304
Kristian McDonald
Robert Foot, Archil Kobakhidze, Kristian L. McDonald, Raymond R. Volkas
Renormalization-scale independence of the physical cosmological constant
3 pages; V2 to appear in PLB
Phys.Lett.B664:199-200,2008
10.1016/j.physletb.2008.05.029
null
hep-th gr-qc hep-ph
null
Treating the metric as a classical background field, we show that the cosmological constant does not run with the renormalization scale -- contrary to some claims in the literature.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:32:10 GMT" }, { "version": "v2", "created": "Tue, 13 May 2008 21:15:18 GMT" } ]
2008-11-26T00:00:00
[ [ "Foot", "Robert", "" ], [ "Kobakhidze", "Archil", "" ], [ "McDonald", "Kristian L.", "" ], [ "Volkas", "Raymond R.", "" ] ]
[ 0.0732286274, 0.0835818052, -0.0092540374, 0.0362597518, 0.0252683666, 0.0320522971, 0.0137687782, -0.1005061716, -0.0433746055, 0.0098863374, -0.0838654488, 0.0570606552, -0.0686902478, 0.0748832449, 0.1178087369, 0.0557842366, -0.0974805877, 0.0091890348, 0.0113223083, 0.0375125334, -0.0594243929, -0.0252683666, 0.0519549772, -0.0125396345, -0.010684099, -0.0951168463, 0.0210254565, -0.0108731985, 0.1643271148, -0.083439976, 0.0312722623, -0.0582897998, -0.0854727924, -0.0114345867, 0.0062343609, 0.1165795997, 0.0429727696, -0.0910984948, -0.0165343527, -0.0134260366, -0.1049500033, -0.0722831339, -0.0730395317, 0.084385477, 0.0489293933, -0.003004903, 0.0868910402, 0.0210609119, 0.0617881306, 0.0064116414, -0.1235762611, -0.0303976797, 0.0053568231, -0.102208063, -0.034274213, 0.0084267287, 0.0610317364, 0.0040331292, -0.0314613618, -0.0371579751, 0.0085803717, -0.098898828, -0.0716212839, 0.0709594414, -0.1093938276, 0.0767269582, -0.0571552031, -0.0107136462, -0.0119014243, 0.0687375218, -0.0536568686, -0.0028054623, -0.05602061, 0.0586207211, 0.0058798003, -0.016215248, -0.0044586021, 0.0671301782, -0.0471329503, 0.0510094836, -0.0439655408, -0.0308940653, -0.0235073827, -0.0222546011, -0.0015792729, -0.0065711937, 0.0454546958, -0.0359761044, 0.01474973, 0.0404435694, 0.0703921393, -0.0159197804, 0.0052622734, 0.0506312847, -0.0118068755, -0.0312722623, 0.1067464426, 0.0527113751, 0.1123248637, -0.0112513965, 0.0050318087, 0.0609371848, 0.0211672802, -0.0727086067, 0.1104338765, 0.0603698865, 0.0229637213, -0.0013473311, -0.0982369855, 0.095920518, -0.057533402, 0.0108259236, -0.0466129296, -0.0429491326, -0.1079755872, -0.0002291719, -0.1086374372, 0.0282466784, -0.0955895931, -0.0001474567, -0.0428545848, 0.011139119, 0.0620717816, -0.0818799138, -0.0137924161, -0.0724722296, -0.0439419039, 0.0174325742, -0.1250890493, -0.0240155868, 0.1401224285, -0.0507258326, -0.021592753, -0.0164279845, -0.1002225205, -0.0097031472, 0.0531368479, -0.0518131554, 0.0390016884, 0.0028704652, -0.0132014807, 0.1086374372, -0.0643409714, 0.059046194, 0.0020062232, 0.1203615814, 0.027277546, 0.0439419039, 0.1370968521, 0.0073275901, -0.031343177, 0.1165795997, -0.0107254647, -0.0012476109, 0.0129178325, -0.0288612507, 0.0880729035, 0.0660901368, 0.12527816, -0.0298540201, 0.0001751567, 0.0844800249, -0.0563042574, 0.0546969138, 0.0107195554, 0.0198672246, -0.0169834625, -0.0401362851, -0.0857091695, -0.1839934289, 0.0119073344, 0.0561151579, -0.0580061488, -0.1383259892, 0.016794363, 0.2053616196, 0.0335414521, -0.0499694385, 0.0676029325, 0.0569188297, 0.0637736693, 0.0602280647, 0.0370870605, 0.0330450684, -0.0252683666, 0.049449414, -0.0725667775, 0.0241101347, 0.1087319851, -0.0224082433, -0.1011680216, 0.0536095947, 0.0092422189, 0.1243326589, 0.0272539072, -0.0884983763, 0.0506785586, 0.0362124778, 0.0027552331, 0.0719049349, -0.0095199579, -0.0006980416, 0.096251443, -0.1407842785, -0.0338487402, -0.0302085821, -0.0261429511, 0.0683120489, -0.0734177232, 0.0592352934, -0.0360233784, 0.0121377986, -0.0244883336, 0.0419327244, -0.0691629946, -0.0176098533, -0.0920439884, -0.0028763746, 0.0030669509, 0.0890184045, -0.0093722241, 0.0852836967, 0.0882620066, 0.0346760489, 0.0580061488, -0.0055872877, 0.0285303276, -0.0296176467, -0.0268284343, 0.0441782773, 0.0377016328, 0.0674611032, -0.020103598, 0.038387116, 0.0185671672, -0.0424054749, -0.0282939523, 0.0536095947, -0.1231980622, -0.0635372996, -0.0894438773, -0.0092363097, -0.0661374107, 0.0476293378, -0.0759705678, 0.0508203842, -0.0020638395, -0.0595189407, -0.0073571368, -0.0170543753, 0.023259189, 0.0570133775, -0.0697775707, -0.0865128413, -0.0338251032, 0.0341323875 ]
712.3041
Yi-Kai Liu
Yi-Kai Liu
The Complexity of the Consistency and N-representability Problems for Quantum States
PhD thesis. Yay, no more grad school!! (Finished in August, but did not get around to posting it until now.) 91 pages, a few figures, some boring sections. Has detailed proofs of results in quant-ph/0604166 and quant-ph/0609125. Ch.4 is a preliminary sketch of 0712.1388. Ch.5 is quant-ph/0603012
null
null
null
quant-ph
null
QMA (Quantum Merlin-Arthur) is the quantum analogue of the class NP. There are a few QMA-complete problems, most notably the ``Local Hamiltonian'' problem introduced by Kitaev. In this dissertation we show some new QMA-complete problems. The first one is ``Consistency of Local Density Matrices'': given several density matrices describing different (constant-size) subsets of an n-qubit system, decide whether these are consistent with a single global state. This problem was first suggested by Aharonov. We show that it is QMA-complete, via an oracle reduction from Local Hamiltonian. This uses algorithms for convex optimization with a membership oracle, due to Yudin and Nemirovskii. Next we show that two problems from quantum chemistry, ``Fermionic Local Hamiltonian'' and ``N-representability,'' are QMA-complete. These problems arise in calculating the ground state energies of molecular systems. N-representability is a key component in recently developed numerical methods using the contracted Schrodinger equation. Although these problems have been studied since the 1960's, it is only recently that the theory of quantum computation has allowed us to properly characterize their complexity. Finally, we study some special cases of the Consistency problem, pertaining to 1-dimensional and ``stoquastic'' systems. We also give an alternative proof of a result due to Jaynes: whenever local density matrices are consistent, they are consistent with a Gibbs state.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:37:22 GMT" } ]
2007-12-19T00:00:00
[ [ "Liu", "Yi-Kai", "" ] ]
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712.3042
Ulrich S. Schwarz
T. Erdmann, S. Pierrat, P. Nassoy and U. S. Schwarz
Dynamic force spectroscopy on multiple bonds: experiments and model
to appear in Europhysics Letters
Europhys. Lett., 81:48001, 2008
10.1209/0295-5075/81/48001
null
q-bio.BM cond-mat.soft physics.bio-ph
null
We probe the dynamic strength of multiple biotin-streptavidin adhesion bonds under linear loading using the biomembrane force probe setup for dynamic force spectroscopy. Measured rupture force histograms are compared to results from a master equation model for the stochastic dynamics of bond rupture under load. This allows us to extract the distribution of the number of initially closed bonds. We also extract the molecular parameters of the adhesion bonds, in good agreement with earlier results from single bond experiments. Our analysis shows that the peaks in the measured histograms are not simple multiples of the single bond values, but follow from a superposition procedure which generates different peak positions.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:37:48 GMT" } ]
2010-02-24T00:00:00
[ [ "Erdmann", "T.", "" ], [ "Pierrat", "S.", "" ], [ "Nassoy", "P.", "" ], [ "Schwarz", "U. S.", "" ] ]
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712.3043
Mark Everitt
M.J. Everitt
On the correspondence principle: implications from a study of the chaotic dynamics of a macroscopic quantum device
16 pages, 5 figures. significantly expanded - to be published in New Journal of Physics
New J. Phys. 11 (2009) 013014
10.1088/1367-2630/11/1/013014
null
quant-ph cond-mat.mes-hall cond-mat.other cond-mat.supr-con
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The recovery of classical chaotic dynamics from quantum systems has long been a subject of interest. Furthermore, recent work indicates that quantum chaos may well be significant in quantum information processing. In this paper we discuss the quantum to classical crossover of a superconducting quantum inference device (SQUID) ring. Such devices comprise of thick superconducting loop enclosing a Josephson weak link. These devices are currently strong candidates for many applications in quantum technologies. The weak link brings with it a non-linearity such that semi-classical models of this system can exhibit chaotic dynamics. For many similar systems an application of the correspondence principle together with the inclusion of environmental degrees of freedom through a quantum trajectories approach can be used to effectively recover classical dynamics. Here we show (i) that the standard expression of the correspondence principle is incompatible with the ring Hamiltonian and we present a more pragmatic and general expression which finds application here and (ii) that practical limitations to circuit parameters of the SQUID ring prevent arbitrarily accurate recovery of classical chaotic dynamics.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:52:44 GMT" }, { "version": "v2", "created": "Thu, 10 Jan 2008 10:37:49 GMT" }, { "version": "v3", "created": "Sat, 8 Nov 2008 18:31:56 GMT" } ]
2009-01-08T00:00:00
[ [ "Everitt", "M. J.", "" ] ]
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712.3044
Maximilien Cazayous
M. Cazayous, Y. Gallais, A. Sacuto, R. De Sousa, D. Lebeugle, D. Colson
Observation of electromagnon excitations in the BiFe0$_3$ spiral magnet
null
Phys. Rev. Lett. 101, 037601 (2008)
10.1103/PhysRevLett.101.037601
null
cond-mat.str-el
null
Recently, oxide multiferroics have attracted much attention due to their large magnetoelectric effect which allows the tuning of magnetic properties with electric field and vice versa and open new venues for future spintronic applications such as multiple-state memory devices with dual magnetic and electric control. BiFeO$_3$ (BFO) belongs to this new class of materials and shows both ferroelectric and antiferromagnetic orders at room temperature with a large electric polarizationassociated with a cycloidal spiral magnetic ordering. The incommensurate magnetic order induces magnon zone folding and allows investigations by optical probes of unusual spin waves which couples to optical phonons, the so called "`electromagnons"'. Here, we unravel for the first time the electromagnon spectra of BFO by means low energy inelastic light scattering technique. We show the existence of two species of electromagnons corresponding to spin wave excitations in and out of the cycloidal plane. The present observations present an unique opportunity to study the interplay between ferroelectric and magnetic orders.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:57:13 GMT" } ]
2010-10-12T00:00:00
[ [ "Cazayous", "M.", "" ], [ "Gallais", "Y.", "" ], [ "Sacuto", "A.", "" ], [ "De Sousa", "R.", "" ], [ "Lebeugle", "D.", "" ], [ "Colson", "D.", "" ] ]
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712.3045
Rathindra Nath Sen (Retd)
R. N. Sen
Physics and the measurement of continuous variables
20 pages
null
10.1007/s10701-007-9203-z
null
quant-ph
null
Wigner had expressed the opinion that the impossibility of exact measurements of single operators like position operators rendered the notion of geometrical points somewhat dubious in physics. Using Sewell's recent resolution of the measurement problem (collapse of the wave packet) in quantum mechanics and extending it to the measurement of operators with continuous spectra, we are able to compare the situation in quantum mechanics with that in quantum mechanics. Our conclusion is that the notion of a geometrical point is as meaningful in quantum mechanics as it is in classical mechanics.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:58:26 GMT" } ]
2007-12-19T00:00:00
[ [ "Sen", "R. N.", "" ] ]
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712.3046
Ari Pakman
Gaston Giribet, Ari Pakman and Leonardo Rastelli
Spectral Flow in AdS(3)/CFT(2)
50 pages, 2 figures
JHEP 0806:013,2008
10.1088/1126-6708/2008/06/013
YITP-SB-07-38
hep-th
null
We study the spectral flowed sectors of the H3 WZW model in the context of the holographic duality between type IIB string theory in AdS(3)x S^3 x T^4 with NSNS flux and the symmetric product orbifold of T^4. We construct explicitly the physical vertex operators in the flowed sectors that belong to short representations of the superalgebra, thus completing the bulk-to-boundary dictionary for 1/2 BPS states. We perform a partial calculation of the string three-point functions of these operators. A complete calculation would require the three-point couplings of non-extremal flowed operators in the H3 WZW model, which are at present unavailable. In the unflowed sector, perfect agreement has recently been found between the bulk and boundary three-point functions of 1/2 BPS operators. Assuming that this agreement persists in the flowed sectors, we determine certain unknown three-point couplings in the H3 WZW model in terms of three-point couplings of affine descendants in the SU(2) WZW model.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 20:58:51 GMT" }, { "version": "v2", "created": "Wed, 19 Dec 2007 01:39:25 GMT" } ]
2009-12-10T00:00:00
[ [ "Giribet", "Gaston", "" ], [ "Pakman", "Ari", "" ], [ "Rastelli", "Leonardo", "" ] ]
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712.3047
Rob Ivison
A. D. Biggs and R. J. Ivison (Edinburgh)
High-resolution radio observations of submillimetre galaxies
In press at MNRAS. 12 pages. High-resolution PDF version available at http://www.roe.ac.uk/~rji/merlin.pdf
null
10.1111/j.1365-2966.2008.12869.x
null
astro-ph
null
We have produced sensitive, high-resolution radio maps of 12 SMGs in the Lockman Hole using combined MERLIN and VLA data at a frequency of 1.4 GHz. Integrating for 350hr yielded an r.m.s. noise of 6.0 uJy/beam and a resolution of 0.2-0.5". For the first time, wide-field data from the two arrays have been combined in the (u,v) plane and the bandwidth smearing response of the VLA data has been removed. All of the SMGs are detected in our maps as well as sources comprising a non-submm luminous control sample. We find evidence that SMGs are more extended than the general uJy radio population and that therefore, unlike in local ULIRGs, the starburst component of the radio emission is extended and not confined to the galactic nucleus. For the eight sources with redshifts we measure linear sizes between 1 and 8 kpc with a median of 5 kpc. Therefore, they are in general larger than local ULIRGs which may support an early-stage merger scenario for the starburst trigger. X-rays betray AGN in six of the 33 sources in the combined sample. All but one of these are in the control sample, suggesting a lower incidence of AGN amongst the submm-luminous galaxies which is, in turn, consistent with increased X-ray absorption in these dust-obscured starbursts. Only one of our sources is resolved into multiple, distinct components with our high-resolution data. Finally, compared to a previous study of faint radio sources in the GOODS-N field we find systematically smaller source sizes and no evidence for a tail extending to ~4". Possible reasons for this are discussed.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:00:16 GMT" } ]
2009-11-13T00:00:00
[ [ "Biggs", "A. D.", "", "Edinburgh" ], [ "Ivison", "R. J.", "", "Edinburgh" ] ]
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712.3048
Ian Parrish
Ian J. Parrish, Eliot Quataert
Nonlinear Simulations of the Heat Flux Driven Buoyancy Instability and its Implications for Galaxy Clusters
4 pages, 4 figures, submitted to ApJ Letters
ApJ Letters 677 (2008), 9-12
10.1086/587937
null
astro-ph
null
In low collisionality plasmas heat flows almost exclusively along magnetic field lines, and the condition for stability to convection is modified from the standard Schwarzschild criterion. We present local two and three-dimensional simulations of a new heat flux driven buoyancy instability (the HBI) that occurs when the temperature in a plasma decreases in the direction of gravity. We find that the HBI drives a convective dynamo that amplifies an initially weak magnetic field by a factor of ~20. In simulations that begin with the magnetic field aligned with the temperature gradient, the HBI saturates by rearranging the magnetic field lines to be almost purely perpendicular to the initial temperature gradient. This magnetic field reorientation results in a net heat flux through the plasma that is less than 1% of the field-free (Spitzer) value. We show that the HBI is likely to be present in the cool cores of clusters of galaxies between ~0.1-100 kpc, where the temperature increases outwards. The saturated state of the HBI suggests that inward thermal conduction from large radii in clusters is unlikely to solve the cooling flow problem. Finally, we also suggest that the HBI may contribute to suppressing conduction across cold fronts in galaxy clusters.
[ { "version": "v1", "created": "Wed, 19 Dec 2007 17:21:22 GMT" } ]
2008-06-09T00:00:00
[ [ "Parrish", "Ian J.", "" ], [ "Quataert", "Eliot", "" ] ]
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712.3049
Mark C. Neyrinck
Mark C. Neyrinck (IfA, Hawaii)
ZOBOV: a parameter-free void-finding algorithm
10 pages, 8 figures, MNRAS, accepted. Added explanatory figures, and better edge-detection methods. ZOBOV code available at http://www.ifa.hawaii.edu/~neyrinck/voboz
Mon.Not.Roy.Astron.Soc. 386 (2008) 2101-2109
10.1111/j.1365-2966.2008.13180.x
null
astro-ph
null
ZOBOV (ZOnes Bordering On Voidness) is an algorithm that finds density depressions in a set of points, without any free parameters, or assumptions about shape. It uses the Voronoi tessellation to estimate densities, which it uses to find both voids and subvoids. It also measures probabilities that each void or subvoid arises from Poisson fluctuations. This paper describes the ZOBOV algorithm, and the results from its application to the dark-matter particles in a region of the Millennium Simulation. Additionally, the paper points out an interesting high-density peak in the probability distribution of dark-matter particle densities.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:25:12 GMT" }, { "version": "v2", "created": "Fri, 29 Feb 2008 20:56:59 GMT" } ]
2008-05-15T00:00:00
[ [ "Neyrinck", "Mark C.", "", "IfA, Hawaii" ] ]
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712.305
Alexei Kolezhuk
I. P. McCulloch, R. Kube, M. Kurz, A. Kleine, U. Schollwock, A. K. Kolezhuk
Vector chiral order in frustrated spin chains
8 pages, 9 figures
Phys. Rev. B 77, 094404 (2008)
10.1103/PhysRevB.77.094404
null
cond-mat.str-el cond-mat.other
null
By means of a numerical analysis using a non-Abelian symmetry realization of the density matrix renormalization group, we study the behavior of vector chirality correlations in isotropic frustrated chains of spin S=1 and S=1/2, subject to a strong external magnetic field. It is shown that the field induces a phase with spontaneously broken chiral symmetry, in line with earlier theoretical predictions. We present results on the field dependence of the order parameter and the critical exponents.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:01:12 GMT" } ]
2008-04-22T00:00:00
[ [ "McCulloch", "I. P.", "" ], [ "Kube", "R.", "" ], [ "Kurz", "M.", "" ], [ "Kleine", "A.", "" ], [ "Schollwock", "U.", "" ], [ "Kolezhuk", "A. K.", "" ] ]
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712.3051
Benjamin Johnson
Benjamin D. Johnson, David Schiminovich, Mark Seibert, Marie Treyer, D. Christopher Martin, Tom A. Barlow, Karl Forster, Peter G. Friedman, Patrick Morrissey, Susan G. Neff, Todd Small, Ted K. Wyder, Luciana Bianchi, Jose Donas, Timothy M. Heckman, Young-Wook Lee, Barry F. Madore, Bruno Milliard, R. Michael Rich, Alex S. Szalay, Barry Y. Welsh, Sukyoung K. Yi
Ultraviolet, Optical, and Infrared Constraints on Models of Stellar Populations and Dust Attenuation
16 pages, 11 figures, 2 tables. Appearing in the GALEX special issue of ApJ Supp. (29 papers)
Astrophys.J.Suppl.173:377-391,2007
10.1086/522932
null
astro-ph
null
The color of galaxies is a fundamental property, easily measured, that constrains models of galaxies and their evolution. Dust attenuation and star formation history (SFH) are the dominant factors affecting the color of galaxies. Here we explore the empirical relation between SFH, attenuation, and color for a wide range of galaxies, including early types. These galaxies have been observed by GALEX, SDSS, and Spitzer, allowing the construction of measures of dust attenuation from the ratio of infrared (IR) to ultraviolet (UV) flux and measures of SFH from the strength of the 4000A break. The empirical relation between these three quantities is compared to models that separately predict the effects of dust and SFH on color. This comparison demonstrates the quantitative consistency of these simple models with the data and hints at the power of multiwavelength data for constraining these models. The UV color is a strong constraint; we find that a Milky Way extinction curve is disfavored, and that the UV emission of galaxies with large 4000A break strengths is likely to arise from evolved populations. We perform fits to the relation between SFH, attenuation, and color. This relation links the production of starlight and its absorption by dust to the subsequent reemission of the absorbed light in the IR. Galaxy models that self-consistently treat dust absorption and emission as well as stellar populations will need to reproduce these fitted relations in the low-redshift universe.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:03:09 GMT" } ]
2009-11-13T00:00:00
[ [ "Johnson", "Benjamin D.", "" ], [ "Schiminovich", "David", "" ], [ "Seibert", "Mark", "" ], [ "Treyer", "Marie", "" ], [ "Martin", "D. Christopher", "" ], [ "Barlow", "Tom A.", "" ], [ "Forster", "Karl", "" ], [ "Friedman", "Peter G.", "" ], [ "Morrissey", "Patrick", "" ], [ "Neff", "Susan G.", "" ], [ "Small", "Todd", "" ], [ "Wyder", "Ted K.", "" ], [ "Bianchi", "Luciana", "" ], [ "Donas", "Jose", "" ], [ "Heckman", "Timothy M.", "" ], [ "Lee", "Young-Wook", "" ], [ "Madore", "Barry F.", "" ], [ "Milliard", "Bruno", "" ], [ "Rich", "R. Michael", "" ], [ "Szalay", "Alex S.", "" ], [ "Welsh", "Barry Y.", "" ], [ "Yi", "Sukyoung K.", "" ] ]
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712.3052
Gregory Sivakoff
Gregory R. Sivakoff (1), Andr\'es Jord\'an (2), Adrienne M. Juett (3), Craig L. Sarazin (4), Jimmy A. Irwin (5) ((1) The Ohio State University, (2) Harvard-Smithsonian Center for Astrophysics, (3) NASA Goddard Space Flight Center, (4) University of Virginia, (5) University of Michigan)
Variable Low-Mass X-ray Binaries in Early-Type Galaxies
Conference proceedings from 'A Population Explosion: The Nature and Evolution of X-ray Binaries in Diverse Environments', 28 Oct - 2 Nov, St. Petersburg Beach, FL. 5 pages, 2 B & W figures, 3 Color figures
AIP Conf.Proc.1010:308-312,2008
10.1063/1.2945063
null
astro-ph
null
As the Chandra X-ray Observatory mission matures, increasing numbers of nearby galaxies are being observed multiple times, sampling the variability of extragalactic X-ray binaries on timescales extending from seconds to years. We present results on luminous low-mass X-ray binaries from several early-type galaxies. We show that instantaneous LMXB luminosity functions of early-type galaxies do not significantly change between observations; a relatively low fraction of sources are strongly variable on <~ 5 yr timescales. We discuss the implications that a relatively small number of transient LMXBs are being discovered in early-type galaxies.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:03:40 GMT" } ]
2009-06-23T00:00:00
[ [ "Sivakoff", "Gregory R.", "" ], [ "Jordán", "Andrés", "" ], [ "Juett", "Adrienne M.", "" ], [ "Sarazin", "Craig L.", "" ], [ "Irwin", "Jimmy A.", "" ] ]
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712.3053
Stella Offner
S. S. R. Offner (1), M. R. Krumholz (2), R. I. Klein (1 and 3), C. F. McKee (1) ((1) University of California-Berkeley, (2) Princeton University, (3) Lawrence Livermore National Laboratory)
The Kinematics of Molecular Cloud Cores in the Presence of Driven and Decaying Turbulence: Comparisons with Observations
18 pages, 12 figures, accepted to AJ
null
10.1088/0004-6256/136/1/404
null
astro-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this study we investigate the formation and properties of prestellar and protostellar cores using hydrodynamic, self-gravitating Adaptive Mesh Refinement simulations, comparing the cases where turbulence is continually driven and where it is allowed to decay. We model observations of these cores in the C$^{18}$O$(2\to 1)$, NH$_3(1,1)$, and N$_2$H$^+(1\to 0)$ lines, and from the simulated observations we measure the linewidths of individual cores, the linewidths of the surrounding gas, and the motions of the cores relative to one another. Some of these distributions are significantly different in the driven and decaying runs, making them potential diagnostics for determining whether the turbulence in observed star-forming clouds is driven or decaying. Comparing our simulations with observed cores in the Perseus and $\rho$ Ophiuchus clouds shows reasonably good agreement between the observed and simulated core-to-core velocity dispersions for both the driven and decaying cases. However, we find that the linewidths through protostellar cores in both simulations are too large compared to the observations. The disagreement is noticably worse for the decaying simulation, in which cores show highly supersonic infall signatures in their centers that decrease toward their edges, a pattern not seen in the observed regions. This result gives some support to the use of driven turbulence for modeling regions of star formation, but reaching a firm conclusion on the relative merits of driven or decaying turbulence will require more complete data on a larger sample of clouds as well as simulations that include magnetic fields, outflows, and thermal feedback from the protostars.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:11:16 GMT" }, { "version": "v2", "created": "Tue, 1 Jul 2008 05:02:52 GMT" } ]
2009-11-13T00:00:00
[ [ "Offner", "S. S. R.", "", "1 and 3" ], [ "Krumholz", "M. R.", "", "1 and 3" ], [ "Klein", "R. I.", "", "1 and 3" ], [ "McKee", "C. F.", "" ] ]
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712.3054
Beth Willman
S. M. Walsh (ANU), B. Willman (CfA), D. Sand (Steward, U Arizona), J. Harris (Steward, U Arizona), A. Seth (CfA), D. Zaritsky (Steward, U Arizona), H. Jerjen (ANU)
Bootes II ReBooted: An MMT/MegaCam Study of An Ultra-Faint Milky Way Satellite
10 pages, 8 figures. ApJ accepted. Conclusions are unchanged, but content and figures have changed substantively in this accepted version
null
10.1086/592076
null
astro-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
[abridged] We present MMT/Megacam imaging in Sloan $g$ and $r$ of the extremely low luminosity Bo\"otes II Milky Way companion. We use a bootstrap approach to perform robust measurements of, and uncertainties on, Bo\"otes II's distance, luminosity, size, and morphology. We show that Bo\"otes II's stellar population is old and metal-poor ([Fe/H] $\lta$ -2). Assuming a stellar population like that of M92, Bo\"otes II is at a distance of 42 $\pm$ 2 kpc, closer than the initial published estimate of 60 $\pm$ 10 kpc. This distance revision, combined with a more robust measurement of Bo\"otes II's structure with a Plummer model (exponential model) results in a more compact half-light size of $r_h\simeq 36 (33) \pm 9 (10)$ pc and lower luminosity of $M_V\simeq-2.4 (-2.2) \pm 0.7 (0.7)$ mag. This revised size and luminosity move Bo\"otes II into a region of size-luminosity space not previously known to be occupied by old stellar populations, but also occupied by the recently discovered Milky Way satellites Willman 1 and SEGUE 1. We show that the apparently distorted morphology of Bo\"otes II is not statistically significant given the present data. We use a tidal argument to support a scenario where Bo\"otes II is a dwarf galaxy (dark matter dominated) rather than a globular cluster (not dark matter dominated). However, we can not rule out that Bo\"otes II is a star cluster on the verge of disruption, such as Palomar 5.
[ { "version": "v1", "created": "Wed, 19 Dec 2007 15:20:09 GMT" }, { "version": "v2", "created": "Wed, 23 Jul 2008 16:36:47 GMT" } ]
2009-11-13T00:00:00
[ [ "Walsh", "S. M.", "", "ANU" ], [ "Willman", "B.", "", "CfA" ], [ "Sand", "D.", "", "Steward, U Arizona" ], [ "Harris", "J.", "", "Steward, U Arizona" ], [ "Seth", "A.", "", "CfA" ], [ "Zaritsky", "D.", "", "Steward, U Arizona" ], [ "Jerjen", "H.", "", "ANU" ] ]
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712.3055
Lech Longa
David Allender and Lech Longa
Landau-deGennes Theory of Biaxial Nematics Re-examined
12 pages, 14 figures
Phys. Rev. E78, 011704 (2008)
10.1103/PhysRevE.78.011704
null
cond-mat.soft cond-mat.stat-mech
null
Recent experiments report that the long looked for thermotropic biaxial nematic phase has been finally detected in some thermotropic liquid crystalline systems. Inspired by these experimental observations we concentrate on some elementary theoretical issues concerned with the classical sixth-order Landau-deGennes free energy expansion in terms of the symmetric and traceless tensor order parameter $Q_{\alpha\beta}$. In particular, we fully explore the stability of the biaxial nematic phase giving analytical solutions for all distinct classes of the phase diagrams that theory allows. This includes diagrams with triple- and (tri-)critical points and with multiple (reentrant) biaxial- and uniaxial phase transitions. A brief comparison with predictions of existing molecular theories is also given.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 19:45:41 GMT" } ]
2008-09-24T00:00:00
[ [ "Allender", "David", "" ], [ "Longa", "Lech", "" ] ]
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712.3056
Alicia Johnson
Alicia A. Johnson and Galin L. Jones
Gibbs Sampling for a Bayesian Hierarchical General Linear Model
20 pages, 1 figure, submitted to Electronic Journal of Statistics
null
null
null
stat.CO math.ST stat.TH
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider a Bayesian hierarchical version of the normal theory general linear model which is practically relevant in the sense that it is general enough to have many applications and it is not straightforward to sample directly from the corresponding posterior distribution. Thus we study a block Gibbs sampler that has the posterior as its invariant distribution. In particular, we establish that the Gibbs sampler converges at a geometric rate. This allows us to establish conditions for a central limit theorem for the ergodic averages used to estimate features of the posterior. Geometric ergodicity is also a key component for using batch means methods to consistently estimate the variance of the asymptotic normal distribution. Together, our results give practitioners the tools to be as confident in inferences based on the observations from the Gibbs sampler as they would be with inferences based on random samples from the posterior. Our theoretical results are illustrated with an application to data on the cost of health plans issued by health maintenance organizations.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:12:02 GMT" }, { "version": "v2", "created": "Thu, 15 May 2008 15:10:31 GMT" }, { "version": "v3", "created": "Mon, 27 Oct 2008 16:37:29 GMT" }, { "version": "v4", "created": "Sat, 17 Oct 2009 19:53:46 GMT" }, { "version": "v5", "created": "Thu, 21 Jan 2010 23:04:50 GMT" } ]
2010-01-22T00:00:00
[ [ "Johnson", "Alicia A.", "" ], [ "Jones", "Galin L.", "" ] ]
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712.3057
Jing Shu
Ben Lillie, Jing Shu, Tim M.P. Tait
Top Compositeness at the Tevatron and LHC
9 pages, 4 figures
JHEP 0804:087,2008
10.1088/1126-6708/2008/04/087
ANL-HEP-PR-07-96, EFI/07-31, NUHEP-TH/07-11
hep-ph
null
We explore the possibility that the right-handed top quark is composite. We examine the consequences that compositeness would have on $t \bar{t}$ production at the Tevatron, and derive a weak constraint on the scale of compositeness of order a few hundred GeV from the $t \bar{t}$ inclusive cross section. More detailed studies of differential properties of $t \bar{t}$ production could potentially improve this limit. We find that a composite top can result in an enhancement of the $t \bar{t} t \bar{t}$ production rate at the LHC (of as much as $10^3$ compared to the Standatd Model four top rate). We explore observables which allow us to extract the four top rate from the backgrounds, and show that the LHC can either discover or constrain top compositeness for wide ranges of parameter space.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:18:37 GMT" } ]
2009-02-18T00:00:00
[ [ "Lillie", "Ben", "" ], [ "Shu", "Jing", "" ], [ "Tait", "Tim M. P.", "" ] ]
[ 0.0800376832, -0.0718416646, -0.064606905, -0.0160252433, -0.0357184596, 0.0464947112, 0.0076521491, 0.1187917069, -0.0508456826, -0.0490749404, 0.0221849084, 0.0676424652, -0.0161137823, 0.0158481691, 0.0667823926, -0.0318734124, 0.0066023502, 0.0859064385, 0.0796329454, 0.0403982885, -0.0937989056, -0.0969356522, 0.0648598671, 0.0625831932, -0.0674906895, -0.0506180152, -0.0334417894, -0.1035633013, 0.0608124509, 0.0395129137, 0.0283319242, -0.062077269, -0.0957720205, -0.0692108423, -0.0278512929, 0.0884360746, 0.0230955761, 0.0310639311, -0.0320504867, -0.0076458249, 0.0552472509, 0.1016913652, -0.0301532615, -0.0121865217, 0.0160505399, -0.0727523342, -0.0064284373, -0.0173153579, -0.0979980975, -0.0102134058, 0.057776887, 0.0492520146, -0.0172015242, -0.0667317957, -0.07290411, -0.0185169354, -0.078924641, -0.0091509586, -0.042143736, -0.0528693944, -0.0949625373, -0.0573721454, -0.0330370478, 0.0385516547, -0.1056376025, -0.0161517262, -0.0287113693, 0.0108268419, -0.0950637236, -0.0388299115, -0.0063746828, 0.0134576634, 0.0499856062, 0.120916605, 0.0397911742, -0.0012569129, -0.0619254895, 0.0489484556, 0.0415366217, -0.0564108826, 0.0255872682, -0.037843354, -0.0477342308, -0.0388299115, -0.0071209255, -0.0399682485, -0.0140647767, 0.0199208837, -0.1428738385, -0.0720946267, 0.0053565041, 0.0019193613, -0.0457105227, 0.0098402845, 0.1055364162, -0.1215237156, 0.0903080031, -0.0511745363, -0.053476505, 0.0165185239, -0.0447998531, 0.0199841242, 0.0794811621, -0.0205659401, 0.1402430236, 0.0356425717, -0.0081517519, -0.020945387, -0.0843380615, -0.0215651467, 0.0588899255, -0.0689578801, -0.1794017851, 0.0604077093, -0.0871206671, -0.0861594006, -0.0053596664, 0.0438385904, -0.047278896, 0.0443192236, -0.0212362949, 0.0062482008, 0.0515286848, 0.0365532413, 0.0037881299, -0.1174762994, 0.0158481691, -0.1588611454, -0.059041705, -0.0339477137, 0.0884866714, -0.0288631469, -0.0314939693, 0.0702732876, -0.0007509857, 0.0380457267, -0.0053438563, -0.0117754554, -0.0592440739, -0.0774574578, 0.0148869082, -0.0074118334, 0.0109027317, 0.0269912165, 0.0357690528, 0.0019667919, -0.030254446, 0.031949304, 0.0412836596, 0.0067351558, -0.0591934845, -0.1517781615, -0.0430038124, -0.0037343751, 0.0236647446, -0.218358174, 0.022336686, 0.0877277777, -0.0493279025, -0.1130241379, 0.0520599075, -0.0015826036, -0.012559643, 0.0771033093, 0.1362967938, 0.0758890808, -0.0971380249, 0.1266841739, -0.1176786646, -0.0482401587, 0.0090497732, 0.0013367545, -0.0672377273, 0.0233232435, 0.0896503031, -0.0282054413, -0.114238359, -0.0390575789, -0.066175282, 0.0390575789, -0.0131288106, 0.0784187168, -0.0138118127, 0.0570685901, -0.1443916261, -0.0957214236, 0.0105485823, 0.0556013994, -0.0196932163, -0.054235395, -0.0289137401, 0.0314939693, 0.049176123, 0.0535776913, 0.0172900613, -0.0413089544, 0.0704756603, 0.1357908547, 0.0876771808, -0.0220331289, 0.0109280273, 0.0354654975, 0.0639997944, -0.035946127, -0.1033103317, -0.0324046388, 0.1403442025, -0.0429785177, -0.0197185129, -0.0471271202, -0.0240694862, 0.0327334888, 0.0382228009, 0.0680978, 0.0018071088, -0.0205026995, -0.041384846, 0.0294449627, -0.0074434541, 0.1270889193, -0.1263806224, 0.0623808242, 0.0849451795, 0.0115920566, -0.0075130188, 0.028534295, 0.114541918, 0.0266876593, 0.0562085137, 0.0690590665, 0.0015328013, -0.086260587, -0.0945072025, -0.0715887025, 0.0456346348, -0.013824461, -0.0225517042, -0.0200220682, 0.0414860323, -0.077659823, -0.0097074779, -0.0417642891, 0.0229058545, 0.0518069454, 0.0187193062, 0.0406259559, -0.0641515702, 0.0047146091, 0.0477595292, 0.0340741985, 0.0742701143, 0.0135841453, -0.0276236255, 0.0006007886, 0.0067983968, -0.0302291512 ]
712.3058
Stephan Haas
Kazumi Maki, Aditya Raghavan, Stephan Haas
Chiral d-wave superconductivity in the heavy-fermion compound CeIrIn_5
null
null
null
null
cond-mat.supr-con
null
Recent thermal conductivity measurements in the heavy-fermion compound CeIrIn_5 indicate that its superconducting order parameter is very different from CeCoIn_5. Here we show that these experiments are consistent with chiral d-wave symmetry.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:19:30 GMT" } ]
2007-12-20T00:00:00
[ [ "Maki", "Kazumi", "" ], [ "Raghavan", "Aditya", "" ], [ "Haas", "Stephan", "" ] ]
[ 0.0812367871, -0.0322326608, -0.0771749467, 0.0142710321, 0.1093639284, 0.0801448971, 0.0255502798, 0.0020404737, -0.0347221754, -0.1042975485, -0.0418631509, -0.034875039, 0.0028607578, 0.0471697487, 0.0154502755, 0.0351370946, -0.0777864084, 0.0400506109, -0.0221763328, 0.0838136524, -0.0741613209, -0.1183611229, 0.0946015492, 0.0492225029, 0.0208879001, -0.0076323273, 0.0485236943, 0.0286075771, 0.0758209974, -0.0162691958, 0.0399414189, -0.0494845584, 0.0038844068, -0.1288432926, -0.1919983476, 0.0262709279, -0.0561669394, 0.0373208784, -0.0756462961, -0.0062838402, -0.0457284488, 0.1198460981, -0.0770875961, 0.0658629462, -0.039089743, 0.007948976, -0.0342417434, 0.093116574, 0.0865652189, 0.0466456376, -0.0550750457, 0.04409061, 0.0544635877, -0.0744233802, -0.0046241637, 0.0026150821, 0.0601414256, 0.0997552797, -0.0130481133, -0.1019390672, 0.0459905043, -0.0957371145, 0.0900592729, -0.0742923543, -0.0531533174, -0.0937280357, -0.0359887704, 0.094426848, 0.0840757042, 0.0126222745, -0.0531533174, 0.0252882261, -0.0143693024, -0.0302235782, 0.0333682299, -0.0099635171, -0.0007568179, -0.0520177484, 0.010176436, 0.0393517986, -0.0790529996, 0.0553371012, 0.050838504, 0.0100890845, -0.0435009897, -0.1084030643, 0.012829734, -0.003354839, -0.0270134155, -0.0253974143, 0.0702305138, 0.0120872473, -0.0461215302, 0.0274064969, -0.030900551, -0.007441246, 0.0149916811, -0.0477812067, -0.0719775409, 0.0246767662, -0.0254629273, -0.0162255187, -0.0559048839, 0.0900592729, 0.1874560714, 0.0850802436, 0.0301362276, -0.0391770937, -0.1637838483, -0.0467766672, 0.1246504262, 0.0073375162, -0.0085113002, 0.0368622839, -0.077218622, -0.0647710487, 0.0131245451, -0.0559048839, -0.123165451, 0.1409851313, 0.0473007746, 0.1136441529, 0.0332372002, 0.0081072999, 0.0761267319, -0.0130481133, -0.0004115069, -0.16911228, -0.0637665093, 0.0058034076, 0.0939900875, -0.0164766554, -0.0114976261, 0.039089743, 0.0580013171, 0.0045886775, 0.0404000133, -0.0968726873, -0.0092647057, 0.0373208784, 0.0140198972, 0.0162801147, 0.180293262, -0.0340670384, 0.0883995965, 0.0714971051, 0.0050527314, 0.08346425, 0.137753129, -0.006141894, 0.0006786793, -0.0369277969, 0.0543762371, 0.0353336334, -0.038063366, -0.0872640312, 0.0315775238, 0.0518430471, 0.0375392586, -0.0457721241, 0.0904086828, 0.0038680285, -0.0708856508, -0.0348968767, 0.1098006889, 0.000681409, -0.0549440198, 0.0313591473, -0.053240668, 0.0309442282, -0.0219579544, -0.0165312495, -0.0487420708, -0.0359669328, 0.0372990407, -0.0086914627, 0.0315775238, -0.0845998153, -0.0750348419, 0.0434354767, 0.0325383916, 0.0364473648, -0.0436756909, -0.0023980686, -0.0531533174, 0.0116286529, 0.0355738513, 0.016869735, -0.0589185096, 0.0190426018, -0.0373208784, 0.0771312714, 0.0716718063, 0.0769128948, -0.0353554711, -0.0804506242, 0.0734625161, 0.1267468631, 0.0514499657, 0.0133647621, -0.0327786058, -0.0007691016, -0.0424964465, 0.0042501907, -0.0473444499, -0.0703615397, 0.0274283346, -0.0278432537, -0.0846434906, 0.0013068586, -0.0039117043, -0.0167496279, 0.1032493338, -0.0131573025, -0.0392207727, 0.017099034, -0.0648583993, -0.0711913779, 0.0763451084, 0.0842940882, 0.0441124476, 0.0153738437, 0.0322326608, 0.0801885724, 0.010029031, 0.1784588695, -0.0222527646, -0.031861417, -0.0497902893, 0.0477812067, -0.0144457351, -0.0246549286, 0.1048216596, 0.0463399105, -0.0876134411, 0.0184420608, 0.0813241377, -0.0408586077, 0.0695753768, -0.0042556501, -0.0499649905, -0.0313373096, 0.0416010953, 0.0456410982, -0.0855170041, 0.0755152702, 0.0069389753, -0.0574772097, 0.0450733155, 0.0568220764, 0.022340117, 0.0797518119, -0.0488731004, -0.0580886714, -0.0664307252, 0.0169134121 ]
712.3059
Alex Hamilton
Alex Hamilton, Jeff Murugan, Andrea Prinsloo
A note on the universality of the Hagedorn behavior of pp-wave strings
25 pages; fixed minor typo; added references
JHEP 0802:108,2008
10.1088/1126-6708/2008/02/108
null
hep-th
null
Following on from recent studies of string theory on a one-parameter family of integrable deformations of $AdS_{5}\times S^{5}$ proposed by Lunin and Maldacena, we carry out a systematic analysis of the high temperature properties of type IIB strings on the associated pp-wave geometries. In particular, through the computation of the thermal partition function and free energy we find that not only does the theory exhibit a Hagedorn transition in both the $(J,0,0)$ and $(J,J,J)$ class of pp-waves, but that the Hagedorn temperature is insensitive to the deformation suggesting an interesting universality in the high temperature behaviour of the pp-wave string theory. We comment also on the implications of this universality on the confinement/deconfinement transition in the dual $\mathcal{N}=1$ Leigh-Strassler deformation of ${\cal N}=4$ Yang-Mills theory.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:20:22 GMT" }, { "version": "v2", "created": "Thu, 21 Feb 2008 08:55:34 GMT" } ]
2014-11-18T00:00:00
[ [ "Hamilton", "Alex", "" ], [ "Murugan", "Jeff", "" ], [ "Prinsloo", "Andrea", "" ] ]
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712.306
Greg Martin
Greg Martin and Erick B. Wong
Almost all integer matrices have no integer eigenvalues
9 pages, 1 figure
null
null
null
math.NT
null
For a fixed $n\ge2$, consider an $n\times n$ matrix $M$ whose entries are random integers bounded by $k$ in absolute value. In this paper, we examine the probability that $M$ is singular (hence has eigenvalue 0), and the probability that $M$ has at least one rational eigenvalue. We show that both of these probabilities tend to 0 as $k$ increases. More precisely, we establish an upper bound of size $k^{-2+\epsilon}$ for the probability that $M$ is singular, and size $k^{-1+\epsilon}$ for the probability that $M$ has a rational eigenvalue. These results generalize earlier work by Kowalsky for the case $n=2$ and answer a question posed by Hetzel, Liew, and Morrison.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:27:26 GMT" } ]
2007-12-20T00:00:00
[ [ "Martin", "Greg", "" ], [ "Wong", "Erick B.", "" ] ]
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712.3061
Surajit Saha
Surjeet Singh, Surajit Saha, S. K. Dhar, R. Suryanarayanan, A. K. Sood, and A. Revcolevschi
Manifestation of geometric frustration on magnetic and thermodynamic properties of pyrochlores $Sm_2X_2O_7$ (X=Ti, Zr)
24 pages, 6 figures, Accepted for publication in Phys. Rev. B
null
10.1103/PhysRevB.77.054408
null
cond-mat.mtrl-sci
null
We present here magnetization, specific heat and Raman studies on single-crystalline specimens of the first pyrochlore member $Sm_2Ti_2O_7$ of the rare-earth titanate series. Its analogous compound $Sm_2Zr_2O_7$ in the rare-earth zirconate series is also investigated in the polycrystalline form. The Sm spins in $Sm_2Ti_2O_7$ remain unordered down to at least T = 0.5 K. The absence of magnetic ordering is attributed to very small values of exchange ($\theta_{cw} ~ -0.26 K$) and dipolar interaction ($\mu_{eff} ~ 0.15 \mu_B$) between the $Sm^{3+}$ spins in this pyrochlore. In contrast, the pyrochlore $Sm_2Zr_2O_7$ is characterized by a relatively large value of Sm-Sm spin exchange ($\theta_{cw} ~ - 10 K$); however, long-range ordering of the $Sm^{3+}$ spins is not established at least down to T = 0.67 K, due to frustration of the $Sm^{3+}$ spins on the pyrochlore lattice. The ground state of $Sm^{3+}$ ions in both pyrochlores is a well-isolated Kramer's doublet. The higher-lying crystal field excitations are observed in the low-frequency region of the Raman spectra of the two compounds recorded at T = 10 K. At higher temperatures, the magnetic susceptibility of $Sm_2Ti_2O_7$ shows a broad maximum at T = 140 K while that of $Sm_2Zr_2O_7$ changes monotonically. Whereas $Sm_2Ti_2O_7$ is a promising candidate for investigating spin-fluctuations on a frustrated lattice as indicated by our data, the properties of $Sm_2Zr_2O_7$ seem to conform to a conventional scenario where geometrical frustration of the spin exclude their long-range ordering.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:34:27 GMT" } ]
2009-11-13T00:00:00
[ [ "Singh", "Surjeet", "" ], [ "Saha", "Surajit", "" ], [ "Dhar", "S. K.", "" ], [ "Suryanarayanan", "R.", "" ], [ "Sood", "A. K.", "" ], [ "Revcolevschi", "A.", "" ] ]
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712.3062
C\'assius de Melo
R. R. Cuzinatto, C. A. M. de Melo, L. G. Medeiros and P. J. Pompeia
Cosmic acceleration from second order gauge gravity
RevTex4 15 pages, 1 figure. Accepted for publication in Astrophysics & Space Science
Astrophys.Space Sci.332:201-208,2011
10.1007/s10509-010-0483-y
IFT-P.020/2007
gr-qc astro-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We construct a phenomenological theory of gravitation based on a second order gauge formulation for the Lorentz group. The model presents a long-range modification for the gravitational field leading to a cosmological model provided with an accelerated expansion at recent times. We estimate the model parameters using observational data and verify that our estimative for the age of the Universe is of the same magnitude than the one predicted by the standard model. The transition from the decelerated expansion regime to the accelerated one occurs recently (at $\sim9.3\;Gyr$).
[ { "version": "v1", "created": "Tue, 18 Dec 2007 21:49:40 GMT" }, { "version": "v2", "created": "Wed, 27 Aug 2008 23:05:34 GMT" }, { "version": "v3", "created": "Tue, 7 Sep 2010 22:20:26 GMT" } ]
2011-02-09T00:00:00
[ [ "Cuzinatto", "R. R.", "" ], [ "de Melo", "C. A. M.", "" ], [ "Medeiros", "L. G.", "" ], [ "Pompeia", "P. J.", "" ] ]
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712.3063
Jeffrey Kubo
Jeffrey M. Kubo, Ian P. Dell'Antonio
A method to search for strong galaxy-galaxy lenses in optical imaging surveys
Accepted for publication in MNRAS, 12 pages
Mon.Not.Roy.Astron.Soc.385:918,2008
10.1111/j.1365-2966.2008.12880.x
FERMILAB-PUB-07-662-A-CD
astro-ph
null
We present a semi-automated method to search for strong galaxy-galaxy lenses in optical imaging surveys. Our search technique constrains the shape of strongly lensed galaxies (or arcs) in a multi-parameter space, which includes the third order (octopole) moments of objects. This method is applied to the Deep Lens Survey (DLS), a deep ground based weak lensing survey imaging to $R\sim26$. The parameter space of arcs in the DLS is simulated using real galaxies extracted from deep HST fields in order to more accurately reproduce the properties of arcs. Arcs are detected in the DLS using a pixel thresholding method and candidate arcs are selected within this multi-parameter space. Examples of strong galaxy-galaxy lens candidates discovered in the DLS F2 field (4 square degrees) are presented.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 22:17:31 GMT" }, { "version": "v2", "created": "Wed, 19 Dec 2007 21:15:53 GMT" } ]
2008-11-07T00:00:00
[ [ "Kubo", "Jeffrey M.", "" ], [ "Dell'Antonio", "Ian P.", "" ] ]
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712.3064
Lance Dixon
Lance J. Dixon
Hard QCD Processes at Colliders
14 pages, 17 figures, talk presented at Lepton-Photon 2007; v2, references updated
null
null
SLAC-PUB-13054
hep-ph hep-ex
null
Recent developments in the study of hard QCD processes at colliders are reviewed, in the context of the imminent startup of the LHC.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 22:01:34 GMT" }, { "version": "v2", "created": "Mon, 24 Dec 2007 18:01:14 GMT" } ]
2007-12-24T00:00:00
[ [ "Dixon", "Lance J.", "" ] ]
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712.3065
Wayne Witzel
W. M. Witzel and S. Das Sarma
Wavefunction considerations for the central spin decoherence problem in a nuclear spin bath
null
Phys. Rev. B 77, 165319 (2008)
10.1103/PhysRevB.77.165319
null
cond-mat.mes-hall
null
Decoherence of a localized electron spin in a solid state material (the ``central spin'' problem) at low temperature is believed to be dominated by interactions with nuclear spins in the lattice. This decoherence is partially suppressed through the application of a large magnetic field that splits the energy levels of the electron spin and prevents depolarization. However, dephasing decoherence resulting from a dynamical nuclear spin bath cannot be removed in this way. Fluctuations of the nuclear field lead to uncertainty of the electron's precessional frequency in a process known as spectral diffusion. This article considers the effect of the electron's wavefunction shape upon spectral diffusion and provides wavefunction dependent decoherence time formulas for free induction decay as well as spin echoes and concatenated dynamical decoupling schemes for enhancing coherence. We also discuss dephasing of a qubit encoded in singlet-triplet states of a double quantum dot. A central theoretical result of this work is the development of a continuum approximation for the spectral diffusion problem which we have applied to GaAs and InAs materials specifically.
[ { "version": "v1", "created": "Wed, 19 Dec 2007 00:24:20 GMT" }, { "version": "v2", "created": "Fri, 11 Apr 2008 20:13:23 GMT" } ]
2009-11-13T00:00:00
[ [ "Witzel", "W. M.", "" ], [ "Sarma", "S. Das", "" ] ]
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712.3066
Michal Bajdich
Michal Bajdich
Generalized Pairing Wave Functions and Nodal Properties for Electronic Structure Quantum Monte Carlo
Phd Thesis under advisory of Prof. Lubos Mitas, NCSU, Raleigh, 2007
null
null
null
cond-mat.other
null
The quantum Monte Carlo (QMC) is one of the most promising many-body electronic structure approaches. It employs stochastic techniques for solving the stationary Schr\" odinger equation and for evaluation of expectation values. The key advantage of QMC is its capability to use the explicitly correlated wave functions, which allow the study of many-body effects beyond the reach of mean-field methods. The most important limit on QMC accuracy is the fixed-node approximation, which comes from necessity to circumvent the fermion sign problem. The size of resulting fixed-node errors depends on the quality of the nodes (the subset of position space where the wave function vanishes) of a used wave function. In this dissertation, we analyze the nodal properties of the existing fermionic wave functions and offer new types of variational wave functions with improved nodal structure.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 22:12:38 GMT" } ]
2007-12-20T00:00:00
[ [ "Bajdich", "Michal", "" ] ]
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712.3067
Waldyr A. Rodrigues Jr.
Waldyr A. Rodrigues Jr
Differential Forms on Riemannian (Lorentzian) and Riemann-Cartan Structures and Some Applications to Physics
Some few important misprints appearing in the version of the paper published in AFLB (in a special issue dedicated to torsion) are corrected
Ann. Fond. L. de Broglie 32 (4), 425-478 (2007)
null
null
math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper after recalling some essential tools concerning the theory of differential forms in the Cartan, Hodge and Clifford bundles over a Riemannian or Riemann-Cartan space or a Lorentzian or Riemann-Cartan spacetime we solve with details several exercises involving different grades of difficult. One of the problems is to show that a recent formula appearing in the literature for the exterior covariant derivative of the Hodge dual of the torsion 2-forms is simply wrong. We believe that the paper will be useful for students (and eventually for some experts) on applications of differential geometry on physical problems. A detailed account of the issues discussed in the paper appears in the table of contents.
[ { "version": "v1", "created": "Wed, 19 Dec 2007 16:32:42 GMT" }, { "version": "v2", "created": "Wed, 2 Jan 2008 10:08:09 GMT" }, { "version": "v3", "created": "Mon, 7 Jan 2008 16:04:03 GMT" }, { "version": "v4", "created": "Mon, 12 May 2008 14:36:40 GMT" }, { "version": "v5", "created": "Tue, 20 May 2008 12:28:27 GMT" }, { "version": "v6", "created": "Thu, 4 Dec 2008 19:14:04 GMT" } ]
2008-12-04T00:00:00
[ [ "Rodrigues", "Waldyr A.", "Jr" ] ]
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712.3068
Dipanjan Basu
D. Basu, M. J. Gilbert, L. F. Register, A. H. MacDonald and S. K. Banerjee
Effect of Edge Roughness on Electronic Transport in Graphene Nanoribbon Channel Metal Oxide Semiconductor Field-Effect Transistors
8 pages, 5 figures
Applied Physics Letters 92, 042114 (2008)
10.1063/1.2839330
null
cond-mat.mes-hall cond-mat.mtrl-sci
null
Results of quantum mechanical simulations of the influence of edge disorder on transport in graphene nanoribbon metal oxide semiconductor field-effect transistors (MOSFETs) are reported. The addition of edge disorder significantly reduces ON-state currents and increases OFF-state currents, and introduces wide variability across devices. These effects decrease as ribbon widths increase and as edges become smoother. However the bandgap decreases with increasing width, thereby increasing the band-to-band tunneling mediated subthreshold leakage current even with perfect nanoribbons. These results suggest that without atomically precise edge control during fabrication, MOSFET performance gains through use of graphene will be difficult to achieve.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 22:22:38 GMT" } ]
2008-04-10T00:00:00
[ [ "Basu", "D.", "" ], [ "Gilbert", "M. J.", "" ], [ "Register", "L. F.", "" ], [ "MacDonald", "A. H.", "" ], [ "Banerjee", "S. K.", "" ] ]
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712.3069
John Franks
John Franks and Michael Handel
Complete semi-conjugacies for psuedo-Anosov homeomorphisms
null
null
null
null
math.DS math.GT
null
Suppose $S$ is a surface of genus $\ge 2 $, $f: S \to S$ is a surface homeomorphism isotopic to a pseudo-Anosov map $\alpha$ and suppose $\ti S$ is the universal cover of $S$ and $F$ and $A$ are lifts of $f$ and $\alpha$ respectively. We show there is a semiconjugacy $\Theta : \ti S \to \bar \L^s \times \bar \L^u$ from $F$ to $\bar A$, where $\bar \L^s$ ($\bar \L^u$) is the completion of the $R$-tree of leaves of the stable (resp. unstable) foliation for $A$ and $\bar A$ is the map induced by $A$. We also generalize a result of Markovich and show that for any $g \in Homeo(S)$ which commutes with $f$ and has identity lift $G : \ti S \to \ti S$ and for any $(c,w)$ in the image of $\Theta$ each component of $\Theta^{-1}(c,w)$ is $G$-invariant.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:02:10 GMT" }, { "version": "v2", "created": "Wed, 26 Dec 2007 14:31:24 GMT" } ]
2007-12-26T00:00:00
[ [ "Franks", "John", "" ], [ "Handel", "Michael", "" ] ]
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712.307
Hans-Thomas Janka
H.-Th. Janka, A. Marek, B. Mueller, and L. Scheck (MPI for Astrophysics, Garching)
Supernova explosions and the birth of neutron stars
10 pages, 8 figures, 19 ps files; to be published in Proc. of Conf. "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007, McGill Univ., Montreal, Canada; high-resolution images can be obtained upon request; incorrect panel in fig.8 replaced
AIP Conf.Proc.983:369-378,2008
10.1063/1.2900257
null
astro-ph
null
We report here on recent progress in understanding the birth conditions of neutron stars and the way how supernovae explode. More sophisticated numerical models have led to the discovery of new phenomena in the supernova core, for example a generic hydrodynamic instability of the stagnant supernova shock against low-mode nonradial deformation and the excitation of gravity-wave activity in the surface and core of the nascent neutron star. Both can have supportive or decisive influence on the inauguration of the explosion, the former by improving the conditions for energy deposition by neutrino heating in the postshock gas, the latter by supplying the developing blast with a flux of acoustic power that adds to the energy transfer by neutrinos. While recent two-dimensional models suggest that the neutrino-driven mechanism may be viable for stars from about 8 solar masses to at least 15 solar masses, acoustic energy input has been advocated as an alternative if neutrino heating fails. Magnetohydrodynamic effects constitute another way to trigger explosions in connection with the collapse of sufficiently rapidly rotating stellar cores, perhaps linked to the birth of magnetars. The global explosion asymmetries seen in the recent simulations offer an explanation of even the highest measured kick velocities of young neutron stars.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:14:15 GMT" }, { "version": "v2", "created": "Thu, 20 Dec 2007 08:05:31 GMT" } ]
2009-06-23T00:00:00
[ [ "Janka", "H. -Th.", "", "MPI for\n Astrophysics, Garching" ], [ "Marek", "A.", "", "MPI for\n Astrophysics, Garching" ], [ "Mueller", "B.", "", "MPI for\n Astrophysics, Garching" ], [ "Scheck", "L.", "", "MPI for\n Astrophysics, Garching" ] ]
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712.3071
Yujin Guo
Nassif Ghoussoub and Yujin Guo
Estimates for the quenching time of a parabolic equation modeling electrostatic MEMS
17 pages, 5 figures. Updated version -- if any -- of this paper can be downloaded from the website: http://www.birs.ca/~nassif
null
null
null
math.AP
null
The singular parabolic problem $u_t=\Delta u -\frac{\lambda f(x)}{(1+u)^2}$ on a bounded domain $\Omega$ of $R^N$ with Dirichlet boundary conditions, models the dynamic deflection of an elastic membrane in a simple electrostatic Micro-Electromechanical System (MEMS) device. In this paper, we analyze and estimate the quenching time of the elastic membrane in terms of the applied voltage --represented here by $\lambda$. As a byproduct, we prove that for sufficiently large $\lambda$, finite-time quenching must occur near the maximum point of the varying dielectric permittivity profile $f(x)$.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:06:05 GMT" } ]
2007-12-20T00:00:00
[ [ "Ghoussoub", "Nassif", "" ], [ "Guo", "Yujin", "" ] ]
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712.3072
Manolis Plionis Dr.
M. Plionis, M. Rovilos, S. Basilakos, I. Georgantopoulos, F. Bauer
Luminosity Dependent X-ray AGN Clustering ?
ApJ Letters accepted
null
10.1086/528845
null
astro-ph
null
We have analysed the angular clustering of X-ray selected active galactic nuclei (AGN) in different flux-limited sub-samples of the Chandra Deep Field North (CDF-N) and South (CDF-S) surveys. We find a strong dependence of the clustering strength on the sub-sample flux-limit, a fact which explains most of the disparate clustering results of different XMM and Chandra surveys. Using Limber's equation, we find that the inverted CDF-N and CDF-S spatial clustering lengths are consistent with direct spatial clustering measures found in the literature, while at higher flux-limits the clustering length increases considerably; for example, at $fx,limit ~ 10^{-15} erg/s/cm^{-2} we obtain r_0~ 17 +- 5 and 18+- 3 h^{-1} Mpc, for the CDF-N and CDF-S, respectively. We show that the observed flux-limit clustering trend hints towards an X-ray luminosity dependent clustering of X-ray selected, $z\sim 1$, AGNs.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:17:06 GMT" } ]
2017-03-22T00:00:00
[ [ "Plionis", "M.", "" ], [ "Rovilos", "M.", "" ], [ "Basilakos", "S.", "" ], [ "Georgantopoulos", "I.", "" ], [ "Bauer", "F.", "" ] ]
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712.3073
Aidan Sims
Aidan Sims and Trent Yeend
C*-algebras associated to product systems of Hilbert bimodules
24 pages. v2: material has been rearranged so that the algebra NO_X is defined only under hypotheses which ensure that the universal representation is injective. The substance of the results is unchanged. v3: minor revisions; this version to appear in J. Operator Theory
null
null
null
math.OA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let (G,P) be a quasi-lattice ordered group and let X be a compactly aligned product system over P of Hilbert bimodules. Under mild hypotheses we associate to X a C*-algebra which we call the Cuntz-Nica-Pimsner algebra of X. Our construction generalises a number of others: a sub-class of Fowler's Cuntz-Pimsner algebras for product systems of Hilbert bimodules; Katsura's formulation of Cuntz-Pimsner algebras of Hilbert bimodules; the C*-algebras of finitely aligned higher-rank graphs; and Crisp and Laca's boundary quotients of Toeplitz algebras. We show that for a large class of product systems X, the universal representation of X in its Cuntz-Nica-Pimsner algebra is isometric.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:20:16 GMT" }, { "version": "v2", "created": "Wed, 13 Aug 2008 11:13:40 GMT" }, { "version": "v3", "created": "Wed, 7 Jan 2009 23:24:12 GMT" } ]
2009-01-08T00:00:00
[ [ "Sims", "Aidan", "" ], [ "Yeend", "Trent", "" ] ]
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712.3074
Anosh Joseph
Simon Catterall, Anosh Joseph
Lattice Actions for Yang-Mills Quantum Mechanics with Exact Supersymmetry
24 pages, minor corrections, published version
Phys.Rev.D77:094504,2008
10.1103/PhysRevD.77.094504
SU-4252-871
hep-lat hep-th
null
We derive lattice actions for Yang-Mills quantum mechanics for models with $\cQ=4, 8$ and 16 supercharges which possess an exact supersymmetry at non-zero lattice spacing. These are obtained by dimensional reduction of twisted versions of the corresponding super Yang-Mills theories in $D=2, 3$ and 4 dimensions.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:28:40 GMT" }, { "version": "v2", "created": "Wed, 9 Jan 2008 20:37:57 GMT" }, { "version": "v3", "created": "Thu, 15 May 2008 16:24:58 GMT" } ]
2008-11-26T00:00:00
[ [ "Catterall", "Simon", "" ], [ "Joseph", "Anosh", "" ] ]
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712.3075
Jean-Philippe Lenain
J.-P. Lenain, C. Boisson, H. Sol
SSC scenario for TeV emission from non-blazar AGNs
4 pages, 5 figures, HEPRO Workshop Proceedings, revised manuscript
Int.J.Mod.Phys.D17:1577-1584,2008
10.1142/S0218271808013170
null
astro-ph
null
M87 is the first extragalactic source detected in the TeV gamma-ray domain that is not a blazar, its large scale jet not being aligned to the line of sight. We present here a multi-blob synchrotron self-Compton model accounting explicitly for large viewing angles and moderate Lorentz factors as inferred from magnetohydrodynamic simulations of jet formation, motivated by the detection of M87 at very high energies (VHE; E > 100GeV). Predictions are presented for the very high-energy emission of active galactic nuclei with extended optical or X-ray jet, which could be misaligned blazars but still show some moderate beaming. We include predictions for 3C273, Cen A and PKS 0521-36.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:37:46 GMT" }, { "version": "v2", "created": "Mon, 10 Mar 2008 14:39:49 GMT" } ]
2009-06-23T00:00:00
[ [ "Lenain", "J. -P.", "" ], [ "Boisson", "C.", "" ], [ "Sol", "H.", "" ] ]
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712.3076
Guido Boffetta
G. Boffetta, A. Celani, D. Dezzani, A. Seminara
How winding is the coast of Britain ? Conformal invariance of rocky shorelines
null
null
10.1029/2007GL033093
null
nlin.CD
null
We show that rocky shorelines with fractal dimension 4/3 are conformally invariant curves by measuring the statistics of their winding angles from global high-resolution data. Such coastlines are thus statistically equivalent to the outer boundary of the random walk and of percolation clusters. A simple model of coastal erosion gives an explanation for these results. Conformal invariance allows also to predict the highly intermittent spatial distribution of the flux of pollutant diffusing ashore.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:37:47 GMT" } ]
2015-05-13T00:00:00
[ [ "Boffetta", "G.", "" ], [ "Celani", "A.", "" ], [ "Dezzani", "D.", "" ], [ "Seminara", "A.", "" ] ]
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712.3077
Young-Heon Kim
Young-Heon Kim and Robert J. McCann
Continuity, curvature, and the general covariance of optimal transportation
43 pages, 1 figure
null
null
null
math.DG math.AP
null
Let M and \bar M be n-dimensional manifolds equipped with suitable Borel probability measures \rho and \bar\rho. Ma, Trudinger & Wang gave sufficient conditions on a transportation cost c \in C^4(M \times \bar M) to guarantee smoothness of the optimal map pushing \rho forward to \bar\rho; the necessity of these conditions was deduced by Loeper. The present manuscript shows the form of these conditions to be largely dictated by the covariance of the question; it expresses them via non-negativity of the sectional curvature of certain null-planes in a novel but natural pseudo-Riemannian geometry which the cost c induces on the product space M \times \bar M. H\"older continuity of optimal maps was established for rougher mass distributions by Loeper, still relying on a key result of Trudinger & Wang which required certain structure on the domains and the cost. We go on to develop this theory for mass distributions on differentiable manifolds -- recovering Loeper's Riemannian examples such as the round sphere as particular cases -- give a direct proof of the key result mentioned above, and revise Loeper's H\"older continuity argument to make it logically independent of all earlier works, while extending it to less restricted geometries and cost functions even for subdomains M and \bar M of R^n. We also give new examples of geometries satisfying the hypotheses -- obtained using submersions and tensor products -- and some connections to spacelike Lagrangian submanifolds in symplectic geometry.
[ { "version": "v1", "created": "Wed, 19 Dec 2007 00:33:49 GMT" } ]
2007-12-20T00:00:00
[ [ "Kim", "Young-Heon", "" ], [ "McCann", "Robert J.", "" ] ]
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712.3078
Guido Boffetta
S. Berti, A. Bistagnino, G. Boffetta, A. Celani and S. Musacchio
Two-dimensional elastic turbulence
null
null
10.1103/PhysRevE.77.055306
null
nlin.CD physics.flu-dyn
null
We investigate the effect of polymer additives on a two-dimensional Kolmogorov flow at very low Reynolds numbers by direct numerical simulations of the Oldroyd-B viscoelastic model. We find that above the elastic instability threshold the flow develops the elastic turbulence regime recently observed in experiments. We observe that both the turbulent drag and the Lyapunov exponent increase with Weissenberg, indicating the presence of a disordered, turbulent-like mixing flow. The energy spectrum develops a power-law scaling range with an exponent close to the experimental and theoretical expectations.
[ { "version": "v1", "created": "Tue, 18 Dec 2007 23:42:32 GMT" } ]
2010-06-23T00:00:00
[ [ "Berti", "S.", "" ], [ "Bistagnino", "A.", "" ], [ "Boffetta", "G.", "" ], [ "Celani", "A.", "" ], [ "Musacchio", "S.", "" ] ]
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