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704.0801
Brice Camus
Brice Camus
Fundamental solutions for a class of non-elliptic homogeneous differential operators
15 pages, perhaps to be revised
null
null
null
math.AP math.GM
null
We compute temperate fundamental solutions of homogeneous differential operators with real-principal type symbols. Via analytic continuation of meromorphic distributions, fundamental solutions for these non-elliptic operators can be constructed in terms of radial averages and invariant distributions on the unit sphere.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 20:35:58 GMT" } ]
2007-05-23T00:00:00
[ [ "Camus", "Brice", "" ] ]
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704.0802
Caleb Lo
Caleb K. Lo, Robert W. Heath, Jr. and Sriram Vishwanath
Hybrid-ARQ in Multihop Networks with Opportunistic Relay Selection
4 pages, 5 figures, to appear in Proceedings of the 2007 International Conference on Acoustics, Speech, and Signal Processing in Honolulu, HI
null
null
null
cs.IT math.IT
null
This paper develops a contention-based opportunistic feedback technique towards relay selection in a dense wireless network. This technique enables the forwarding of additional parity information from the selected relay to the destination. For a given network, the effects of varying key parameters such as the feedback probability are presented and discussed. A primary advantage of the proposed technique is that relay selection can be performed in a distributed way. Simulation results find its performance to closely match that of centralized schemes that utilize GPS information, unlike the proposed method. The proposed relay selection method is also found to achieve throughput gains over a point-to-point transmission strategy.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 20:37:44 GMT" } ]
2012-08-27T00:00:00
[ [ "Lo", "Caleb K.", "" ], [ "Heath,", "Robert W.", "Jr." ], [ "Vishwanath", "Sriram", "" ] ]
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704.0803
Josephine Nanao
Walter A. Simmons and Sandip S. Pakvasa
Geometric Phase and Superconducting Flux Quantization
5 pages, pdf format
null
null
null
quant-ph
null
In a ring of s-wave superconducting material the magnetic flux is quantized in units of $\Phi_0 = \frac{h}{2e}$. It is well known from the theory of Josephson junctions that if the ring is interrupted with a piece of d-wave material, then the flux is quantized in one-half of those units due to a additional phase shift of $\pi$. We reinterpret this phenomenon in terms of geometric phase. We consider an idealized hetero-junction superconductor with pure s-wave and pure d-wave electron pairs. We find, for this idealized configuration, that the phase shift of $\pi$ follows from the discontinuity in the geometric phase and is thus a fundamental consequence of quantum mechanics.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 20:42:18 GMT" } ]
2019-08-19T00:00:00
[ [ "Simmons", "Walter A.", "" ], [ "Pakvasa", "Sandip S.", "" ] ]
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704.0804
Francis Alexander
Francis J. Alexander, Gregory Johnson, Gregory L. Eyink, and Ioannis G. Kevrekidis
Equation-free implementation of statistical moment closures
7 pages, 2 figures
null
10.1103/PhysRevE.77.026701
null
cond-mat.stat-mech cond-mat.other
null
We present a general numerical scheme for the practical implementation of statistical moment closures suitable for modeling complex, large-scale, nonlinear systems. Building on recently developed equation-free methods, this approach numerically integrates the closure dynamics, the equations of which may not even be available in closed form. Although closure dynamics introduce statistical assumptions of unknown validity, they can have significant computational advantages as they typically have fewer degrees of freedom and may be much less stiff than the original detailed model. The closure method can in principle be applied to a wide class of nonlinear problems, including strongly-coupled systems (either deterministic or stochastic) for which there may be no scale separation. We demonstrate the equation-free approach for implementing entropy-based Eyink-Levermore closures on a nonlinear stochastic partial differential equation.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 20:45:34 GMT" } ]
2009-11-13T00:00:00
[ [ "Alexander", "Francis J.", "" ], [ "Johnson", "Gregory", "" ], [ "Eyink", "Gregory L.", "" ], [ "Kevrekidis", "Ioannis G.", "" ] ]
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704.0805
Caleb Lo
Caleb K. Lo, Robert W. Heath, Jr. and Sriram Vishwanath
Opportunistic Relay Selection with Limited Feedback
5 pages, 6 figures, to appear in Proceedings of 2007 IEEE Vehicular Technology Conference-Spring in Dublin, Ireland
null
10.1109/VETECS.2007.40
null
cs.IT math.IT
null
It has been shown that a decentralized relay selection protocol based on opportunistic feedback from the relays yields good throughput performance in dense wireless networks. This selection strategy supports a hybrid-ARQ transmission approach where relays forward parity information to the destination in the event of a decoding error. Such an approach, however, suffers a loss compared to centralized strategies that select relays with the best channel gain to the destination. This paper closes the performance gap by adding another level of channel feedback to the decentralized relay selection problem. It is demonstrated that only one additional bit of feedback is necessary for good throughput performance. The performance impact of varying key parameters such as the number of relays and the channel feedback threshold is discussed. An accompanying bit error rate analysis demonstrates the importance of relay selection.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 20:52:26 GMT" } ]
2016-11-17T00:00:00
[ [ "Lo", "Caleb K.", "" ], [ "Heath,", "Robert W.", "Jr." ], [ "Vishwanath", "Sriram", "" ] ]
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704.0806
Daniel E. Vanden Berk
Donald P. Schneider, Patrick B. Hall, Gordon T. Richards, Michael A. Strauss, Daniel E. Vanden Berk, Scott F. Anderson, W.N. Brandt, Xiaohui Fan, Sebastian Jester, Jim Gray, James E. Gunn, Mark U. SubbaRao, Anirudda R. Thakar, Chris Stoughton, Alexander S. Szalay, Brian Yanny, Donald G. York, Neta A. Bahcall, J. Barentine, Michael R. Blanton, Howard Brewington, J. Brinkmann, Robert J. Brunner, Francisco J. Castander, Istvan Csabai, Joshua A. Frieman, Masataka Fukugita, Michael Harvanek, David W. Hogg, Zeljko Ivezic, Stephen M. Kent, S. J. Kleinman, G. R. Knapp, Richard G. Kron, Jurek Krzesinski, Daniel C. Long, Robert H. Lupton, Atsuko Nitta, Jeffrey R. Pier, David H. Saxe, Yue Shen, Stephanie A. Snedden, David H. Weinberg, and Jian Wu
The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release
37 pages, Accepted for publication in AJ
Astron.J.134:102-117,2007
10.1086/518474
null
astro-ph
null
We present the fourth edition of the Sloan Digital Sky Survey (SDSS) Quasar Catalog. The catalog contains 77,429 objects; this is an increase of over 30,000 entries since the previous edition. The catalog consists of the objects in the SDSS Fifth Data Release that have luminosities larger than M_i = -22.0 (in a cosmology with H_0 = 70 km/s/Mpc, Omega_M = 0.3, and Omega_Lambda = 0.7) have at least one emission line with FWHM larger than 1000 km/s, or have interesting/complex absorption features, are fainter than i=15.0, and have highly reliable redshifts. The area covered by the catalog is 5740 sq. deg. The quasar redshifts range from 0.08 to 5.41, with a median value of 1.48; the catalog includes 891 quasars at redshifts greater than four, of which 36 are at redshifts greater than five. Approximately half of the catalog quasars have i < 19; nearly all have i < 21. For each object the catalog presents positions accurate to better than 0.2 arcsec. rms per coordinate, five-band (ugriz) CCD-based photometry with typical accuracy of 0.03 mag, and information on the morphology and selection method. The catalog also contains basic radio, near-infrared, and X-ray emission properties of the quasars, when available, from other large-area surveys. The calibrated digital spectra cover the wavelength region 3800--9200A at a spectral resolution of ~2000. The spectra can be retrieved from the public database using the information provided in the catalog. The average SDSS colors of quasars as a function of redshift, derived from the catalog entries, are presented in tabular form. Approximately 96% of the objects in the catalog were discovered by the SDSS.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 21:00:10 GMT" } ]
2008-11-26T00:00:00
[ [ "Schneider", "Donald P.", "" ], [ "Hall", "Patrick B.", "" ], [ "Richards", "Gordon T.", "" ], [ "Strauss", "Michael A.", "" ], [ "Berk", "Daniel E. Vanden", "" ], [ "Anderson", "Scott F.", "" ], [ "Brandt", "W. N.", "" ], [ "Fan", "Xiaohui", "" ], [ "Jester", "Sebastian", "" ], [ "Gray", "Jim", "" ], [ "Gunn", "James E.", "" ], [ "SubbaRao", "Mark U.", "" ], [ "Thakar", "Anirudda R.", "" ], [ "Stoughton", "Chris", "" ], [ "Szalay", "Alexander S.", "" ], [ "Yanny", "Brian", "" ], [ "York", "Donald G.", "" ], [ "Bahcall", "Neta A.", "" ], [ "Barentine", "J.", "" ], [ "Blanton", "Michael R.", "" ], [ "Brewington", "Howard", "" ], [ "Brinkmann", "J.", "" ], [ "Brunner", "Robert J.", "" ], [ "Castander", "Francisco J.", "" ], [ "Csabai", "Istvan", "" ], [ "Frieman", "Joshua A.", "" ], [ "Fukugita", "Masataka", "" ], [ "Harvanek", "Michael", "" ], [ "Hogg", "David W.", "" ], [ "Ivezic", "Zeljko", "" ], [ "Kent", "Stephen M.", "" ], [ "Kleinman", "S. J.", "" ], [ "Knapp", "G. R.", "" ], [ "Kron", "Richard G.", "" ], [ "Krzesinski", "Jurek", "" ], [ "Long", "Daniel C.", "" ], [ "Lupton", "Robert H.", "" ], [ "Nitta", "Atsuko", "" ], [ "Pier", "Jeffrey R.", "" ], [ "Saxe", "David H.", "" ], [ "Shen", "Yue", "" ], [ "Snedden", "Stephanie A.", "" ], [ "Weinberg", "David H.", "" ], [ "Wu", "Jian", "" ] ]
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704.0807
Ruprecht Machleidt
R. Machleidt
Nuclear forces from chiral effective field theory
54 pages, 12 figures; lectures presented at the DAE-BRNS workshop on physics and astrophysics of hadrons and hadronic matter, Visva Bharati University, Santiniketan, West Begal, India, November 2006
null
null
null
nucl-th nucl-ex
null
In this lecture series, I present the recent progress in our understanding of nuclear forces in terms of chiral effective field theory.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 21:18:14 GMT" } ]
2007-05-23T00:00:00
[ [ "Machleidt", "R.", "" ] ]
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704.0808
Michael T. Lacey
Michael Lacey and Xiaochun Li
On a Conjecture of EM Stein on the Hilbert Transform on Vector Fields
92 pages, 20+ figures. Final version of the paper. To appear in Memoirs AMS
Mem. Amer. Math. Soc., vol. 205 (2010) No. 965
10.1090/S0065-9266-10-00572-7
null
math.CA
null
Let $ v$ be a smooth vector field on the plane, that is a map from the plane to the unit circle. We study sufficient conditions for the boundedness of the Hilbert transform \operatorname H_{v, \epsilon}f(x) := \text{p.v.}\int_{-\epsilon}^ \epsilon f(x-yv(x)) \frac{dy}y where $ \epsilon $ is a suitably chosen parameter, determined by the smoothness properties of the vector field. It is a conjecture, due to E.\thinspace M.\thinspace Stein, that if $ v$ is Lipschitz, there is a positive $ \epsilon $ for which the transform above is bounded on $ L ^{2}$. Our principal result gives a sufficient condition in terms of the boundedness of a maximal function associated to $ v$. This sufficient condition is that this new maximal function be bounded on some $ L ^{p}$, for some $ 1<p<2$. We show that the maximal function is bounded from $ L ^{2}$ to weak $ L ^{2}$ for all Lipschitz maximal function. The relationship between our results and other known sufficient conditions is explored.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 21:33:13 GMT" }, { "version": "v2", "created": "Tue, 18 Sep 2007 16:09:38 GMT" }, { "version": "v3", "created": "Fri, 11 Jan 2008 00:26:28 GMT" } ]
2015-09-07T00:00:00
[ [ "Lacey", "Michael", "" ], [ "Li", "Xiaochun", "" ] ]
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704.0809
Andy Lawrence
A.Lawrence
Wide Field Surveys and Astronomical Discovery Space
Review for publication in Astronomy and Geophysics, based on talk at UK National Astronomy Meeting, 2006. Fifteen pages, nine figures (figs 4,5,6 have parts a and b)
null
10.1111/j.1468-4004.2007.48327.x
null
astro-ph
null
I review the status of science with wide field surveys. For many decades surveys have been the backbone of astronomy, and the main engine of discovery, as we have mapped the sky at every possible wavelength. Surveys are an efficient use of resources. They are important as a fundamental resource; to map intrinsically large structures; to gain the necessary statistics to address some problems; and to find very rare objects. I summarise major recent wide field surveys - 2MASS, SDSS, 2dfGRS, and UKIDSS - and look at examples of the exciting science they have produced, covering the structure of the Milky Way, the measurement of cosmological parameters, the creation of a new field studying substellar objects, and the ionisation history of the Universe. I then look briefly at upcoming projects in the optical-IR survey arena - VISTA, PanSTARRS, WISE, and LSST. Finally I ask, now we have opened up essentially all wavelength windows, whether the exploration of survey discovery space is ended. I examine other possible axes of discovery space, and find them mostly to be too expensive to explore or otherwise unfruitful, with two exceptions : the first is the time axis, which we have only just begun to explore properly; and the second is the possibility of neutrino astrophysics.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 21:45:43 GMT" } ]
2009-11-13T00:00:00
[ [ "Lawrence", "A.", "" ] ]
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704.081
Carlos Alexandre Wuensche
Rodrigo Leonardi, Brian Williams, Marco Bersanelli, Ivan Ferreira, Philip M. Lubin, Peter R. Meinhold, Hugh O'Neill, Nathan C. Stebor, Fabrizio Villa, Thyrso Villela, Carlos A. Wuensche
The Cosmic Foreground Explorer (COFE): A balloon-borne microwave polarimeter to characterize polarized foregrounds
15 pages Version 2 - missing pictures now appear at the end of the text
New Astron.Rev.50:977-983,2006
10.1016/j.newar.2006.09.004
null
astro-ph
null
The COsmic Foreground Explorer (COFE) is a balloon-borne microwave polarime- ter designed to measure the low-frequency and low-l characteristics of dominant diffuse polarized foregrounds. Short duration balloon flights from the Northern and Southern Hemispheres will allow the telescope to cover up to 80% of the sky with an expected sensitivity per pixel better than 100 $\mu K / deg^2$ from 10 GHz to 20 GHz. This is an important effort toward characterizing the polarized foregrounds for future CMB experiments, in particular the ones that aim to detect primordial gravity wave signatures in the CMB polarization angular power spectrum.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 22:00:09 GMT" }, { "version": "v2", "created": "Mon, 9 Apr 2007 19:56:07 GMT" } ]
2009-06-23T00:00:00
[ [ "Leonardi", "Rodrigo", "" ], [ "Williams", "Brian", "" ], [ "Bersanelli", "Marco", "" ], [ "Ferreira", "Ivan", "" ], [ "Lubin", "Philip M.", "" ], [ "Meinhold", "Peter R.", "" ], [ "O'Neill", "Hugh", "" ], [ "Stebor", "Nathan C.", "" ], [ "Villa", "Fabrizio", "" ], [ "Villela", "Thyrso", "" ], [ "Wuensche", "Carlos A.", "" ] ]
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704.0811
Paula Benaglia
Gustavo E. Romero
Jet interactions in massive X-ray binaries
5 pages, 5 figures. Invited talk presented at the meeting: "Massive Stars: fundamental parameters and circumstellar interactions", Carilo, Dec 2006
null
null
null
astro-ph
null
Massive X-ray binaries are formed by a compact object that accretes matter from the stellar wind of an early-type donor star. In some of these systems, called microquasars, relativistic jets are launched from the surroundings of the compact object. Such jets interact with the photon field of the companion star, the stellar wind, and, at large distances, with the interstellar medium. In this paper I will review the main results of such interactions with particular emphasis on the production of high-energy photons and neutrinos. The case of some specific systems, like LS I +61 303, will be discussed in some detail. Prospects for future observations at different wavelengths of this type of objects will be presented.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 22:11:03 GMT" } ]
2007-05-23T00:00:00
[ [ "Romero", "Gustavo E.", "" ] ]
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704.0812
Rodrigo D\'iaz Mr.
Rodrigo F. D\'iaz, Carolina Cincunegui and Pablo J. D. Mauas (Instituto de Astronom\'ia y F\'isica del Espacio (IAFE). Buenos Aires, Argentina)
The Na I D resonance lines in main sequence late-type stars
12 pages, including 14 figures and 4 tables. Accepted for publication in MNRAS
Mon.Not.Roy.Astron.Soc.378:1007-1018,2007
10.1111/j.1365-2966.2007.11833.x
null
astro-ph
null
We study the sodium D lines (D1: 5895.92 \AA; D2: 5889.95 \AA) in late-type dwarf stars. The stars have spectral types between F6 and M5.5 (B-V between 0.457 and 1.807) and metallicity between [Fe/H] = -0.82 and 0.6. We obtained medium resolution echelle spectra using the 2.15-m telescope at the argentinian observatory CASLEO. The observations have been performed periodically since 1999. The spectra were calibrated in wavelength and in flux. A definition of the pseudo-continuum level is found for all our observations. We also define a continuum level for calibration purposes. The equivalent width of the D lines is computed in detail for all our spectra and related to the colour index (B-V) of the stars. When possible, we perform a careful comparison with previous studies. Finally, we construct a spectral index (R_D') as the ratio between the flux in the D lines, and the bolometric flux. We find that, once corrected for the photospheric contribution, this index can be used as a chromospheric activity indicator in stars with a high level of activity. Additionally, we find that combining some of our results, we obtain a method to calibrate in flux stars of unknown colour.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 22:49:11 GMT" } ]
2009-06-23T00:00:00
[ [ "Díaz", "Rodrigo F.", "", "Instituto de Astronomía y Física del Espacio" ], [ "Cincunegui", "Carolina", "", "Instituto de Astronomía y Física del Espacio" ], [ "Mauas", "Pablo J. D.", "", "Instituto de Astronomía y Física del Espacio" ] ]
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704.0813
Benjamin Schlein
Benjamin Schlein
Dynamics of Bose-Einstein Condensates
20 pages, 2 figures; contribution to the Proceedings of the International Congress on Mathematical Physics held at IMPA in Rio de Janeiro in August 2006
null
null
null
math-ph math.MP
null
We report on some recent results concerning the dynamics of Bose-Einstein condensates, obtained in a series of joint papers with L. Erdos and H.-T. Yau. Starting from many body quantum dynamics, we present a rigorous derivation of a cubic nonlinear Schroedinger equation known as the Gross-Pitaevskii equation for the time evolution of the condensate wave function.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 22:59:56 GMT" } ]
2007-05-23T00:00:00
[ [ "Schlein", "Benjamin", "" ] ]
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704.0814
Alexander I. Lvovsky
K.-P. Marzlin, Juergen Appel, A. I. Lvovsky
Photons as quasi-charged particles
null
Phys. Rev. A 77, 043813 (2008)
10.1103/PhysRevA.77.043813
null
quant-ph
null
The Schrodinger motion of a charged quantum particle in an electromagnetic potential can be simulated by the paraxial dynamics of photons propagating through a spatially inhomogeneous medium. The inhomogeneity induces geometric effects that generate an artificial vector potential to which signal photons are coupled. This phenomenon can be implemented with slow light propagating through an a gas of double-Lambda atoms in an electromagnetically-induced transparency setting with spatially varied control fields. It can lead to a reduced dispersion of signal photons and a topological phase shift of Aharonov-Bohm type.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 23:07:42 GMT" }, { "version": "v2", "created": "Tue, 16 Oct 2007 16:24:34 GMT" } ]
2009-12-29T00:00:00
[ [ "Marzlin", "K. -P.", "" ], [ "Appel", "Juergen", "" ], [ "Lvovsky", "A. I.", "" ] ]
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704.0815
Sergio Duarte
D. Portes Jr., H. Rodrigues, S. B. Duarte and B. Baseia
Exchange of quantum states between coupled oscillators
10 pages, no figure, Latex file
null
null
null
quant-ph
null
Exchange of quantum states between two interacting harmonic oscillator along their evolution time is discussed. It is analyzed the conditions for such exchange starting from a generic initial state and demonstrating that the effect occurs exactly only for the particular states C0|0>+Cn|N>, which includes the interesting qubits components |0>,|1>. It is also determined the relation between the coupling constant and characteristic frequencies of the oscillators to have the complete exchange.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 23:52:16 GMT" }, { "version": "v2", "created": "Sat, 7 Apr 2007 22:14:46 GMT" } ]
2007-05-23T00:00:00
[ [ "Portes", "D.", "Jr." ], [ "Rodrigues", "H.", "" ], [ "Duarte", "S. B.", "" ], [ "Baseia", "B.", "" ] ]
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704.0816
Brian Punsly
Brian Punsly
3-D Simulations of Ergospheric Disk Driven Poynting Jets
To appear in ApJ Letters. A version with high res images is at http://85.20.11.14/hosting/punsly/APJLetter4.2.07/
null
10.1086/518601
null
astro-ph
null
This Letter reports on 3-dimensional simulations of Kerr black hole magnetospheres that obey the general relativistic equations of perfect magnetohydrodynamics (MHD). In particular, we study powerful Poynting flux dominated jets that are driven from dense gas in the equatorial plane in the ergosphere. The physics of which has been previously studied in the simplified limit of an ergopsheric disk. For high spin black holes, $a/M > 0.95$, the ergospheric disk is prominent in the 3-D simulations and is responsible for greatly enhanced Poynting flux emission. Any large scale poloidal magnetic flux that is trapped in the equatorial region leads to an enormous release of electromagnetic energy that dwarfs the jet energy produced by magnetic flux threading the event horizon. The implication is that magnetic flux threading the equatorial plane of the ergosphere is a likely prerequisite for the central engine of powerful FRII quasars.
[ { "version": "v1", "created": "Thu, 5 Apr 2007 23:57:44 GMT" } ]
2009-11-13T00:00:00
[ [ "Punsly", "Brian", "" ] ]
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704.0817
Alexander Yong
Hugh Thomas, Alexander Yong
An S_3-symmetric Littlewood-Richardson rule
9 pages
Math. Res. Lett. 15 (2008), no. 5, 1027--1037
null
null
math.CO math.RT
null
The classical Littlewood-Richardson coefficients C(lambda,mu,nu) carry a natural $S_3$ symmetry via permutation of the indices. Our "carton rule" for computing these numbers transparently and uniformly explains these six symmetries; previously formulated Littlewood-Richardson rules manifest at most three of the six.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 00:25:00 GMT" } ]
2010-02-18T00:00:00
[ [ "Thomas", "Hugh", "" ], [ "Yong", "Alexander", "" ] ]
[ 0.0542151444, 0.0093157869, 0.0817133114, -0.0354924314, 0.0307010822, 0.0053609717, 0.0197643097, -0.0236963406, -0.0860359445, -0.0278887693, 0.0076817805, -0.0784322843, 0.0255321562, 0.0646311194, 0.0238655992, 0.0775469244, 0.0369246267, 0.0073953415, 0.0673392713, 0.0894211307, 0.0301282033, -0.0042900792, 0.0783281252, 0.046429202, 0.0358830281, 0.0464812815, 0.0649435967, -0.0014273139, 0.0512986705, -0.0616625659, 0.0613500848, -0.0165483784, 0.0003952781, -0.048330117, -0.1056179702, 0.0528871082, -0.0750991702, 0.0749950111, -0.0653602332, 0.063329123, -0.1065033302, -0.0079096304, -0.0321072377, -0.1440529227, -0.0046220883, 0.0197122302, -0.0279148091, -0.0540068224, -0.0937437639, 0.0260529537, -0.0125512481, 0.0401275381, 0.0885878578, -0.0038571653, -0.1094718874, 0.0022068843, -0.0130004371, 0.0854630619, 0.0489550754, -0.0777552426, -0.031065641, -0.1303038299, -0.0617146455, -0.0259618144, 0.0148037029, -0.0345810317, -0.1032743827, 0.0457261242, 0.0729638934, 0.0058557303, -0.0569753759, 0.0131696966, 0.112804994, -0.0132347969, -0.0073758112, 0.0343206339, 0.0006322822, 0.1073886901, 0.0728597343, -0.016600458, 0.012668428, 0.0318989195, 0.0247900169, -0.0246467981, -0.0532256253, -0.0453876071, -0.0060087149, 0.0537985042, -0.1297830343, -0.0083913691, 0.0190482121, -0.0881191343, -0.0614021644, -0.0176290348, 0.0717660561, -0.060100168, 0.0880670547, -0.0145433033, -0.0175769553, 0.097076878, -0.0977539122, -0.0524444282, 0.0607251264, 0.0233838614, 0.069839105, 0.0596314482, 0.095670715, -0.0064513939, -0.0621312819, -0.0150771216, -0.0328103155, 0.0639540777, -0.0314822793, 0.0551005006, 0.0551005006, 0.0408566557, -0.1119717211, 0.0275502503, -0.1020765454, 0.0122127291, -0.0793176368, -0.0477572381, 0.141553089, -0.0949416012, -0.0058166701, -0.073536776, -0.0727034956, -0.0842131451, 0.0001690561, 0.0503612347, 0.0640061572, -0.0681725442, 0.0329405181, -0.0520017482, 0.0383828618, 0.1056179702, 0.1024931818, -0.0650998354, -0.0401014984, 0.0779114813, 0.0742138103, 0.0891607329, 0.0781718791, -0.0672871917, -0.017485816, 0.0320811979, -0.1605101526, -0.0033021891, -0.0733284578, 0.0779635608, -0.040700417, -0.0610376075, 0.0183321144, 0.0113403918, -0.0745262951, -0.0581211336, -0.0131371468, 0.0236051995, 0.0601522475, 0.0236312412, 0.0042933342, 0.0732242987, -0.0434085689, 0.0092637064, 0.0586940125, -0.0374714658, -0.0594752096, -0.0316906013, -0.0266128127, -0.1205128133, 0.0432783701, -0.1390532553, -0.074005492, -0.0454917662, 0.0152854417, 0.0449709669, -0.0066662231, -0.1911331117, -0.0712452605, 0.0415597335, 0.0720264614, 0.0259227548, -0.0056474106, 0.0137751251, 0.0072586318, 0.0284095686, 0.0201288685, -0.1032223031, 0.0571836941, -0.0203502085, 0.0276283696, 0.0353101492, 0.132282868, 0.0661935136, 0.0386172235, -0.043486692, 0.0654643923, 0.0379662253, -0.0011872583, -0.0341123156, -0.0050940621, 0.0569753759, 0.068485029, -0.0265346933, -0.0451272056, 0.0258185957, -0.0484863594, -0.0631728768, -0.0517153107, 0.0229281615, -0.0163270384, -0.0221469644, 0.1007745489, 0.0965560749, -0.0991600677, 0.0689537451, -0.0866608992, 0.0063211941, -0.0312739611, 0.0897856951, -0.1011391059, -0.002547031, 0.0505174734, -0.0476270393, -0.0667143092, 0.1224918514, 0.0598397702, -0.0481478386, 0.0345810317, -0.0599439293, 0.0638499185, -0.0130720474, -0.0436689705, -0.0248030368, -0.0472885221, -0.035101831, -0.0069461525, 0.0408566557, -0.0739013329, -0.0587981716, -0.0200507492, 0.026795093, -0.0387734622, 0.1041597351, 0.000787708, 0.0167827383, -0.0228109825, -0.0173165556, 0.0195950512, -0.0964519158, -0.0124796387, 0.1680096537, 0.049007155, -0.0212876461, -0.1524898559, 0.1189504191 ]
704.0818
Michael Shay
M. A. Shay, J. F. Drake, and M. Swisdak
Two-scale structure of the electron dissipation region during collisionless magnetic reconnection
Submitted to Physical Review Letters, 4 pages, 4 figures
null
10.1103/PhysRevLett.99.155002
null
physics.plasm-ph physics.space-ph
null
Particle in cell (PIC) simulations of collisionless magnetic reconnection are presented that demonstrate that the electron dissipation region develops a distinct two-scale structure along the outflow direction. The length of the electron current layer is found to decrease with decreasing electron mass, approaching the ion inertial length for a proton-electron plasma. A surprise, however, is that the electrons form a high-velocity outflow jet that remains decoupled from the magnetic field and extends large distances downstream from the x-line. The rate of reconnection remains fast in very large systems, independent of boundary conditions and the mass of electrons.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 00:11:21 GMT" } ]
2009-11-13T00:00:00
[ [ "Shay", "M. A.", "" ], [ "Drake", "J. F.", "" ], [ "Swisdak", "M.", "" ] ]
[ 0.0563605092, 0.0093274415, 0.0062997341, 0.0014860198, -0.0299616233, 0.0910477042, -0.0730855763, -0.0061203605, -0.0105521325, 0.0465135016, -0.0848129168, 0.0659106225, -0.0232814923, 0.0633375347, 0.0554698259, 0.0479732342, -0.0255824272, 0.0144859869, 0.0622489229, 0.1218257919, -0.0887220353, -0.1469628811, 0.0865448043, 0.0669002682, -0.0690774992, -0.0053162705, -0.0186425131, 0.0396849252, 0.0528967381, -0.0566079207, 0.0931259692, -0.0726402327, -0.0520555377, -0.1011916101, -0.1000535116, 0.1438949555, -0.0497298613, 0.0068223928, -0.0313718729, 0.0393385477, 0.0434703305, -0.0171332974, -0.1431032419, 0.1328108907, 0.0019576494, -0.0898601264, -0.0358747765, -0.0232196394, 0.091097191, -0.023726834, -0.1234092265, 0.0727391988, -0.1255864501, -0.0912951156, -0.1288522929, 0.0428765416, 0.0617046133, 0.0757081509, -0.10708002, -0.0622489229, 0.0816955268, -0.070166111, -0.0114984838, 0.0519565716, -0.0070574344, 0.1087624207, 0.0519565716, 0.0238134284, 0.0532925986, -0.0136571564, -0.0328810886, -0.0667518228, -0.0179868694, -0.0774895176, 0.079815194, -0.0263494048, -0.0899590924, -0.0032689343, -0.0571522303, 0.100300923, 0.0632385686, -0.0582408421, 0.0645251125, -0.1138096303, -0.0061822133, 0.0098222662, 0.0338459946, -0.0544306934, 0.0368396826, 0.0218712427, -0.0242092889, 0.0775884837, -0.0631890893, -0.0012494319, 0.0006966201, 0.007638853, 0.0419611186, -0.0312481672, 0.019557938, 0.0568553358, 0.019607421, -0.0485917665, 0.0223660674, -0.0534410439, 0.0993112773, -0.0706114545, -0.0065687951, 0.0264236275, -0.0552718975, 0.0787760615, 0.1246957704, -0.0024107231, -0.0497793444, 0.0577955022, -0.0866437703, -0.076846242, -0.0568058528, 0.0316687673, -0.0413178466, 0.1041110754, 0.0081460485, 0.0610118583, 0.0490618497, 0.0207949989, 0.0219207257, -0.0376561433, -0.0061110826, 0.0202383213, -0.1129189506, -0.0235907584, -0.0019545567, -0.0056966669, -0.0227619261, -0.0790729523, -0.109158285, 0.0454743728, -0.0137684913, -0.040724054, 0.0111335507, -0.0853572264, 0.0353304707, 0.0398828536, 0.072343342, 0.031520322, 0.0796667412, 0.1236071587, 0.0109046949, 0.078330718, 0.0066430187, -0.0419116355, 0.0025699947, -0.0982721448, 0.0589830801, 0.0244938117, -0.0912456363, 0.0173312277, 0.0664549321, 0.0221186541, -0.0029380205, -0.0217227954, -0.0182713941, 0.036122188, -0.083724305, -0.0318419561, -0.0282049961, 0.0380272642, -0.0353057273, -0.019879574, -0.1377591342, -0.1025276333, -0.0777369291, -0.0952537134, -0.0634365007, -0.048938144, 0.0594284199, 0.0231577866, -0.0494824499, -0.0756091848, -0.0359984823, 0.0579934306, 0.0251247138, -0.0265968163, -0.0169972219, 0.0256566498, -0.0277101714, -0.0154014127, 0.0400560424, 0.0697702542, -0.0498288274, -0.1442908198, -0.0103913145, 0.0729371309, -0.1255864501, 0.042851802, -0.0084738694, -0.0716011077, 0.0927301124, 0.0178879052, -0.0066430187, 0.0296399873, 0.0281555131, 0.072343342, 0.0884746164, -0.013570562, 0.0254092384, 0.0025591704, 0.0071502137, -0.0436682627, -0.0272895712, -0.0255082026, 0.0524019152, -0.0583398081, 0.006544054, -0.0798646733, -0.0724423081, -0.109950006, -0.0155127477, 0.1203413159, 0.0006687862, 0.0189765189, -0.0659601018, 0.044410497, 0.0181353185, 0.094313547, 0.0389179476, 0.0610613413, 0.153197661, -0.0891178921, -0.0032256371, 0.0251741968, -0.0474041849, 0.0945609584, -0.0372602828, -0.0742731541, 0.0428270586, -0.0812501833, 0.0939176902, -0.0593789406, -0.0101748286, 0.0338954777, -0.064178735, 0.0646735579, 0.0097604133, 0.060319107, 0.039115876, 0.0245432947, -0.0129520316, 0.0909982249, 0.046810396, -0.1000040323, -0.0169848502, 0.0713042095, -0.0367407203, -0.0255824272, 0.0421837866, -0.0218712427 ]
704.0819
Lucero Uscanga
Lucero Uscanga, Jorge Cant\'o and Alejandro C. Raga
Position-Velocity Diagrams for the Maser Emission coming from a Keplerian Ring
13 pages, 7 figures, to appear in the 2007 July 20 issue of The Astrophysical Journal
Astrophys.J.663:857-865,2007
10.1086/518640
null
astro-ph
null
We have studied the maser emission from a thin, planar, gaseous ring in Keplerian rotation around a central mass observed edge-on. The absorption coefficient within the ring is assumed to follow a power law dependence with the distance from the central mass as, k=k0r^{-q}. We have calculated position-velocity diagrams for the most intense maser features, for different values of the exponent q. We have found that, depending on the value of q, these diagrams can be qualitatively different. The most intense maser emission at a given velocity can either come mainly from regions close to the inner or outer edges of the amplifying ring or from the line perpendicular to the line of sight and passing through the central mass (as is commonly assumed). Particularly, when q>1 the position-velocity diagram is qualitatively similar to the one observed for the water maser emission in the nucleus of the galaxy NGC 4258. In the context of this simple model, we conclude that in this object the absorption coefficient depends on the radius of the amplifying ring as a decreasing function, in order to have significant emission coming from the inner edge of the ring.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 00:15:24 GMT" } ]
2009-06-23T00:00:00
[ [ "Uscanga", "Lucero", "" ], [ "Cantó", "Jorge", "" ], [ "Raga", "Alejandro C.", "" ] ]
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704.082
Svetlana Boriskina
Svetlana V. Boriskina
Coupling of whispering-gallery modes in size-mismatched microdisk photonic molecules
3 pages with 5 figures (to appear in Opt. Lett. 2007)
Opt. Lett. 32(11) 1557-1559 (2007)
10.1364/OL.32.001557
null
physics.optics
null
Mechanisms of whispering-gallery (WG) modes coupling in microdisk photonic molecules (PMs) with slight and significant size mismatch are numerically investigated. The results reveal two different scenarios of modes interaction depending on the degree of this mismatch and offer new insight into how PM parameters can be tuned to control and modify WG-modes wavelengths and Q-factors. From a practical point of view, these findings offer a way to fabricate PM microlaser structures that exhibit low thresholds and directional emission, and at the same time are more tolerant to fabrication errors than previously explored coupled-cavity structures composed of identical microresonators.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 00:23:59 GMT" } ]
2009-11-13T00:00:00
[ [ "Boriskina", "Svetlana V.", "" ] ]
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704.0821
Karol Gregor
Karol Gregor, Olexei I. Motrunich
Spin solid phases of spin 1 and spin 3/2 antiferromagnets on a cubic lattice
15 pages, 8 figures
null
10.1103/PhysRevB.76.174404
null
cond-mat.str-el
null
We study spin S=1 and S=3/2 Heisenberg antiferromagnets on a cubic lattice focusing on spin solid states. Using Schwinger boson formulation for spins, we start in a U(1) spin liquid phase proximate to Neel phase and explore possible confining paramagnetic phases as we transition away from the spin liquid by the process of monopole condensation. Electromagnetic duality is used to rewrite the theory in terms of monopoles. For spin 1 we find several candidate phases of which the most natural one is a phase with spins organized into parallel Haldane chains. For spin 3/2 we find that the most natural phase has spins organized into parallel ladders. As a by-product, we also write a Landau theory of the ordering in two special classical frustrated XY models on the cubic lattice, one of which is the fully frustrated XY model. In a particular limit our approach maps to a dimer model with 2S dimers coming out of every site, and we find the same spin solid phases in this regime as well.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 00:25:56 GMT" } ]
2009-11-13T00:00:00
[ [ "Gregor", "Karol", "" ], [ "Motrunich", "Olexei I.", "" ] ]
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704.0822
Yuya Sasai
Yuya Sasai, Naoki Sasakura
Braided quantum field theories and their symmetries
36 pages, 18 figures, a comment added and typos corrected
Prog.Theor.Phys.118:785-814,2007
10.1143/PTP.118.785
YITP-07-14
hep-th
null
Braided quantum field theories proposed by Oeckl can provide a framework for defining quantum field theories having Hopf algebra symmetries. In quantum field theories, symmetries lead to non-perturbative relations among correlation functions. We discuss Hopf algebra symmetries and such relations in braided quantum field theories. We give the four algebraic conditions between Hopf algebra symmetries and braided quantum field theories, which are required for the relations to hold. As concrete examples, we apply our discussions to the Poincare symmetries of two examples of noncommutative field theories. One is the effective quantum field theory of three-dimensional quantum gravity coupled with spinless particles given by Freidel and Livine, and the other is noncommutative field theory on Moyal plane. We also comment on quantum field theory on kappa-Minkowski spacetime.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 00:28:12 GMT" }, { "version": "v2", "created": "Tue, 1 May 2007 06:00:46 GMT" }, { "version": "v3", "created": "Fri, 11 May 2007 05:00:57 GMT" }, { "version": "v4", "created": "Wed, 23 May 2007 07:51:41 GMT" }, { "version": "v5", "created": "Mon, 23 Jul 2007 04:46:19 GMT" }, { "version": "v6", "created": "Mon, 27 Aug 2007 05:46:56 GMT" } ]
2008-11-26T00:00:00
[ [ "Sasai", "Yuya", "" ], [ "Sasakura", "Naoki", "" ] ]
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704.0823
Hugh Hudson
Hugh S. Hudson
Chromospheric Flares
Coimbra Solar Physics Meeting on The Physics of Chromospheric Plasmas - Petr Heinzl, Ivan Dorotovic and Robert J. Rutten, eds
null
null
null
astro-ph
null
In this topical review I revisit the "chromospheric flare." This should currently be an outdated concept, because modern data seem to rule out the possiblity of a major flare happening independently in the chromosphere alone, but the chromosphere still plays a major observational role in many ways. It is the source of the bulk of a flare's radiant energy - in particular the visible/UV continuum radiation. It also provides tracers that guide us to the coronal source of the energy, even though we do not yet understand the propagation of the energy from its storage in the corona to its release in the chromosphere. The formation of chromospheric radiations during a flare presents several difficult and interesting physical problems.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 01:22:41 GMT" } ]
2007-05-23T00:00:00
[ [ "Hudson", "Hugh S.", "" ] ]
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704.0824
Eddy Pariguan
Mauricio Angel, Jaime Camacaro and Rafael Diaz
On the (3,N) Maurer-Cartan equation
21 pages
J. Nonlinear Math. Phys 14 (4) (2007) 440-461
10.1080/jnmp.2007.14.4.4
null
math.QA
null
Deformations of the 3-differential of 3-differential graded algebras are controlled by the (3,N) Maurer-Cartan equation. We find explicit formulae for the coefficients appearing in that equation, introduce new geometric examples of N-differential graded algebras, and use these results to study N Lie algebroids.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 01:04:43 GMT" }, { "version": "v2", "created": "Fri, 19 Oct 2007 22:59:40 GMT" }, { "version": "v3", "created": "Fri, 4 Jan 2008 18:19:31 GMT" } ]
2015-05-13T00:00:00
[ [ "Angel", "Mauricio", "" ], [ "Camacaro", "Jaime", "" ], [ "Diaz", "Rafael", "" ] ]
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704.0825
Shiping Feng
Yu Lan, Jihong Qin and Shiping Feng
Electronic structure of kinetic energy driven superconductors in the presence of bilayer splitting
11 pages, 4 figures, replotted figures and added references, accepted for publication in Phys. Rev. B
Phys. Rev. B 76, 014533 (2007)
10.1103/PhysRevB.76.014533
null
cond-mat.supr-con cond-mat.str-el
null
Within the framework of the kinetic energy driven superconductivity, the electronic structure of bilayer cuprate superconductors in the superconducting state is studied. It is shown that the electron spectrum of bilayer cuprate superconductors is split into the bonding and antibonding components by the bilayer splitting, then the observed peak-dip-hump structure around the $[\pi,0]$ point is mainly caused by this bilayer splitting, with the superconducting peak being related to the antibonding component, and the hump being formed by the bonding component. The spectral weight increases with increasing the doping concentration. In analogy to the normal state case, both electron antibonding peak and bonding hump have the weak dispersions around the $[\pi,0]$ point.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 01:08:40 GMT" }, { "version": "v2", "created": "Tue, 24 Jul 2007 08:10:00 GMT" } ]
2007-08-02T00:00:00
[ [ "Lan", "Yu", "" ], [ "Qin", "Jihong", "" ], [ "Feng", "Shiping", "" ] ]
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704.0826
Varsha P. Kulkarni
Varsha P. Kulkarni, Donald G. York, Giovanni Vladilo, Daniel E. Welty
9.7 micrometer Silicate Absorption in a Damped Lyman-alpha Absorber at z=0.52
4 pages, 2 figures, submitted to Astrophysical Journal Letters (revised version including referee's comments)
Astrophys.J.663:L81-L84,2007
10.1086/520048
null
astro-ph
null
We report a detection of the 9.7 micrometer silicate absorption feature in a damped Lyman-alpha (DLA) system at z_{abs} = 0.524 toward AO0235+164, using the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. The feature shows a broad shallow profile over about 8-12 micrometers in the absorber rest frame and appears to be > 15 sigma significant in equivalent width. The feature is fit reasonably well by the silicate absorption profiles for laboratory amorphous olivine or diffuse Galactic interstellar clouds. To our knowledge, this is the first indication of 9.7 micrometer silicate absorption in a DLA. We discuss potential implications of this finding for the nature of the dust in quasar absorbers. Although the feature is relatively shallow (tau_{9.7} = 0.08-0.09), it is about 2 times deeper than expected from extrapolation of the tau_{9.7} vs. E(B-V) relation known for diffuse Galactic interstellar clouds. Further studies of the 9.7 micrometer silicate feature in quasar absorbers will open a new window on the dust in distant galaxies.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 01:25:25 GMT" }, { "version": "v2", "created": "Wed, 2 May 2007 20:16:34 GMT" } ]
2009-06-23T00:00:00
[ [ "Kulkarni", "Varsha P.", "" ], [ "York", "Donald G.", "" ], [ "Vladilo", "Giovanni", "" ], [ "Welty", "Daniel E.", "" ] ]
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704.0827
Eric Sandquist
Nassissie Fekadu, Eric L. Sandquist, Michael Bolte
Photometry of the Globular Cluster NGC 5466: Red Giants and Blue Stragglers
51 pages, 21 figures, 1 electronic table, accepted to ApJ
Astrophys.J.663:277-295,2007
10.1086/518637
null
astro-ph
null
We present wide-field BVI photometry for about 11,500 stars in the low-metallicity cluster NGC 5466. We have detected the red giant branch bump for the first time, although it is at least 0.2 mag fainter than expected relative to the turnoff. The number of red giants (relative to main sequence turnoff stars) is in excellent agreement with stellar models from the Yonsei-Yale and Teramo groups, and slightly high compared to Victoria-Regina models. This adds to evidence that an abnormally large ratio of red giant to main-sequence stars is not correlated with cluster metallicity. We discuss theoretical predictions from different research groups and find that the inclusion or exclusion of helium diffusion and strong limit Coulomb interactions may be partly responsible. We also examine indicators of dynamical history: the mass function exponent and the blue straggler frequency. NGC 5466 has a very shallow mass function, consistent with large mass loss and recently-discovered tidal tails. The blue straggler sample is significantly more centrally concentrated than the HB or RGB stars. We see no evidence of an upturn in the blue straggler frequency at large distances from the center. Dynamical friction timescales indicate that the stragglers should be more concentrated if the cluster's present density structure has existed for most of its history. NGC 5466 also has an unusually low central density compared to clusters of similar luminosity. In spite of this, the specific frequency of blue stragglers that puts it right on the frequency -- cluster M_V relation observed for other clusters.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 01:27:03 GMT" } ]
2009-06-23T00:00:00
[ [ "Fekadu", "Nassissie", "" ], [ "Sandquist", "Eric L.", "" ], [ "Bolte", "Michael", "" ] ]
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704.0828
Cynthia J. Olson Reichhardt
C. Reichhardt and C. J. Olson Reichhardt
Vortex Molecular Crystal and Vortex Plastic Crystal States in Honeycomb and Kagome Pinning Arrays
19 pages, 22 postscript figures. Version to appear in Phys. Rev. B
Phys. Rev. B 76, 064523 (2007)
10.1103/PhysRevB.76.064523
null
cond-mat.supr-con cond-mat.soft
null
Using numerical simulations, we investigate vortex configurations and pinning in superconductors with honeycomb and kagome pinning arrays. We find that a variety of novel vortex crystal states can be stabilized at integer and fractional matching field densities. The honeycomb and kagome pinning arrays produce considerably more pronounced commensuration peaks in the critical depinning force than triangular pinning arrays, and also cause additional peaks at noninteger matching fields where a portion of the vortices are located in the large interstitial regions of the pinning lattices. For the honeycomb pinning array, we find matching effects of equal strength at most fillings B/B_\phi=n/2 for n>2, where n is an integer, in agreement with recent experiments. For kagome pinning arrays, pronounced matching effects generally occur at B/B_\phi=n/3 for n>3, while for triangular pinning arrays pronounced matching effects are observed only at integer fillings B/B_\phi=n. At the noninteger matching field peaks in the honeycomb and kagome pinning arrays, the interstitial vortices are arranged in dimer, trimer, and higher order n-mer states that have an overall orientational order. We call these n-mer states "vortex molecular crystals" and "vortex plastic crystals" since they are similar to the states recently observed in colloidal molecular crystal systems. We argue that the vortex molecular crystals have properties in common with certain spin systems such as Ising and n-state Potts models. We show that kagome and honeycomb pinning arrays can be useful for increasing the critical current above that of purely triangular pinning arrays.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:03:01 GMT" }, { "version": "v2", "created": "Thu, 26 Jul 2007 20:21:35 GMT" } ]
2009-11-13T00:00:00
[ [ "Reichhardt", "C.", "" ], [ "Reichhardt", "C. J. Olson", "" ] ]
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704.0829
Bang-Rong Zhou
Bang-Rong Zhou (Graduate School of Chinese Academy of Sciences)
Quark-Antiquark and Diquark Condensates in Vacuum in a 3D Two-Flavor Gross-Neveu Model
5 pages, revtex4, no figure, minor typos corrected
Commun.Theor. Phys. 47 (2007) 695
10.1088/0253-6102/47/4/027
null
hep-th
null
The effective potential analysis indicates that, in a 3D two-flavor Gross-Neveu model in vacuum, depending on less or bigger than the critical value 2/3 of $G_S/H_P$, where $G_S$ and $H_P$ are respectively the coupling constants of scalar quark-antiquark channel and pseudoscalar diquark channel, the system will have the ground state with pure diquark condensates or with pure quark-antiquark condensates, but no the one with coexistence of the two forms of condensates. The similarities and differences in the interplay between the quark-antiquark and the diquark condensates in vacuum in the 2D, 3D and 4D two-flavor four-fermion interaction models are summarized.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:22:22 GMT" }, { "version": "v2", "created": "Sat, 23 Jun 2007 16:34:04 GMT" } ]
2015-05-13T00:00:00
[ [ "Zhou", "Bang-Rong", "", "Graduate School of Chinese Academy of Sciences" ] ]
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704.083
Qin Liu
Qin Liu, Tianxing Ma, Shou-Cheng Zhang
Spin accumulation from the non-Abelian Aharonov-Bohm effect
4 pages, 4 figures
Phys. Rev. B 76, 233409 (2007)
10.1103/PhysRevB.76.233409
null
cond-mat.mes-hall
null
Recently, it has been shown that the spin-orbit coupling (SOC) of the Dresselhaus type in $[110]$ quantum wells can be mathematically removed by a non-Abelian gauge transformation. In the presence of an additional uniform magnetic field, such a non-Abelian gauge flux leads to a spin accumulation at the edges of the sample, where the relative sign of the spin accumulation between the edges can be tuned by the sign of the Dresselhaus SOC constant. Our prediction can be tested by Kerr measurements within the available experimental sensitivities.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:24:02 GMT" } ]
2009-11-13T00:00:00
[ [ "Liu", "Qin", "" ], [ "Ma", "Tianxing", "" ], [ "Zhang", "Shou-Cheng", "" ] ]
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704.0831
Brooke Shrader
Brooke Shrader and Anthony Ephremides
On packet lengths and overhead for random linear coding over the erasure channel
5 pages, 5 figures, submitted to the 2007 International Wireless Communications and Mobile Computing Conference
null
null
null
cs.IT math.IT
null
We assess the practicality of random network coding by illuminating the issue of overhead and considering it in conjunction with increasingly long packets sent over the erasure channel. We show that the transmission of increasingly long packets, consisting of either of an increasing number of symbols per packet or an increasing symbol alphabet size, results in a data rate approaching zero over the erasure channel. This result is due to an erasure probability that increases with packet length. Numerical results for a particular modulation scheme demonstrate a data rate of approximately zero for a large, but finite-length packet. Our results suggest a reduction in the performance gains offered by random network coding.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:25:40 GMT" } ]
2007-07-13T00:00:00
[ [ "Shrader", "Brooke", "" ], [ "Ephremides", "Anthony", "" ] ]
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704.0832
Nader Haghighipour
Nader Haghighipour, Steinn Sigurdsson, Jack Lissauer, Sean Raymond
Terrestrial and Habitable Planet Formation in Binary and Multi-star Systems
7 pages, White Paper Submitted to the NASA/NSF ExoPlanet Task Force
null
null
null
astro-ph
null
One of the most surprising discoveries of extrasolar planets is the detection of planets in moderately close binary star systems. The Jovian-type planets in the two binaries of Gamma Cephei and GJ 86 have brought to the forefront questions on the formation of giant planets and the possibility of the existence of smaller bodies in such dynamically complex environments. The diverse dynamical characteristics of these objects have made scientists wonder to what extent the current theories of planet formation can be applied to binaries and multiple star systems. At present, the sensitivity of the detection techniques does not allow routine discovery of Earth-sized bodies in binary systems. However, with the advancement of new techniques, and with the recent launch of CoRoT and the launch of Kepler in late 2008, the detection of more planets (possibly terrestrial-class objects) in such systems is on the horizon. Theoretical studies and numerical modeling of terrestrial and habitable planet formation are, therefore, necessary to gain fundamental insights into the prospects for life in such systems and have great strategic impact on NASA science and missions.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:34:35 GMT" } ]
2009-09-29T00:00:00
[ [ "Haghighipour", "Nader", "" ], [ "Sigurdsson", "Steinn", "" ], [ "Lissauer", "Jack", "" ], [ "Raymond", "Sean", "" ] ]
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704.0833
Kasso Okoudjou
\'Arp\'ad B\'enyi, Kasso A. Okoudjou
Local well-posedness of nonlinear dispersive equations on modulation spaces
11 pages
null
10.1112/blms/bdp027
null
math.AP math.CA
null
By using tools of time-frequency analysis, we obtain some improved local well-posedness results for the NLS, NLW and NLKG equations with Cauchy data in modulation spaces $M{p, 1}_{0,s}$.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:36:04 GMT" } ]
2014-02-26T00:00:00
[ [ "Bényi", "Árpád", "" ], [ "Okoudjou", "Kasso A.", "" ] ]
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704.0834
Anatoly Rodionov
Anatoly Rodionov, Sergey Volkov
P-adic arithmetic coding
29 pages
null
null
null
cs.DS
null
A new incremental algorithm for data compression is presented. For a sequence of input symbols algorithm incrementally constructs a p-adic integer number as an output. Decoding process starts with less significant part of a p-adic integer and incrementally reconstructs a sequence of input symbols. Algorithm is based on certain features of p-adic numbers and p-adic norm. p-adic coding algorithm may be considered as of generalization a popular compression technique - arithmetic coding algorithms. It is shown that for p = 2 the algorithm works as integer variant of arithmetic coding; for a special class of models it gives exactly the same codes as Huffman's algorithm, for another special model and a specific alphabet it gives Golomb-Rice codes.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:30:42 GMT" } ]
2007-05-23T00:00:00
[ [ "Rodionov", "Anatoly", "" ], [ "Volkov", "Sergey", "" ] ]
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704.0835
Teddy Cheung
C.C. Cheung
Compton X-ray and Gamma-ray Emission from Extended Radio Galaxies
3 pages, one 3 panel figure. Proceedings of the First GLAST Symposium. (The actual submitted version is 2 pages with references used more sparingly.)
AIP Conf.Proc.921:325-326,2007
10.1063/1.2757334
null
astro-ph
null
The extended lobes of radio galaxies are examined as sources of X-ray and gamma-ray emission via inverse Compton scattering of 3K background photons. The Compton spectra of two exemplary examples, Fornax A and Centaurus A, are estimated using available radio measurements in the ~10's MHz - 10's GHz range. For average lobe magnetic fields of >~0.3-1 micro-G, the lobe spectra are predicted to extend into the soft gamma-rays making them likely detectable with the GLAST LAT. If detected, their large angular extents (~1 deg and 8 deg) will make it possible to ``image'' the radio lobes in gamma-rays. Similarly, this process operates in more distant radio galaxies and the possibility that such systems will be detected as unresolved gamma-ray sources with GLAST is briefly considered.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:42:24 GMT" } ]
2009-06-23T00:00:00
[ [ "Cheung", "C. C.", "" ] ]
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704.0836
Kurt Luoto
Kurt W. Luoto
A matroid-friendly basis for the quasisymmetric functions
25 pages; exposition tightened, typos corrected; to appear in the Journal of Combinatorial Theory, Series A
Journal of Combinatorial Theory, Series A 115 (2008) 777-798
10.1016/j.jcta.2007.10.003
null
math.CO
null
A new Z-basis for the space of quasisymmetric functions (QSym, for short) is presented. It is shown to have nonnegative structure constants, and several interesting properties relative to the space of quasisymmetric functions associated to matroids by the Hopf algebra morphism (F) of Billera, Jia, and Reiner. In particular, for loopless matroids, this basis reflects the grading by matroid rank, as well as by the size of the ground set. It is shown that the morphism F is injective on the set of rank two matroids, and that decomposability of the quasisymmetric function of a rank two matroid mirrors the decomposability of its base polytope. An affirmative answer is given to the Hilbert basis question raised by Billera, Jia, and Reiner.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:43:59 GMT" }, { "version": "v2", "created": "Fri, 16 Nov 2007 18:35:09 GMT" } ]
2010-11-30T00:00:00
[ [ "Luoto", "Kurt W.", "" ] ]
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704.0837
Jaeweon Lee Dr.
Jae-Weon Lee, Kyungsub Kim, Chul H. Lee, Ji-ho Jang
Bremsstrahlung Radiation At a Vacuum Bubble Wall
6 pages, 2 figures, revtex, to appear in JKPS
Journal of the Korean Physical Society, 50, 1229 (2007)
10.3938/jkps.50.1229
null
hep-th
null
When charged particles collide with a vacuum bubble, they can radiate strong electromagnetic waves due to rapid deceleration. Owing to the energy loss of the particles by this bremsstrahlung radiation, there is a non-negligible damping pressure acting on the bubble wall even when thermal equilibrium is maintained. In the non-relativistic region, this pressure is proportional to the velocity of the wall and could have influenced the bubble dynamics in the early universe.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 02:55:57 GMT" } ]
2013-08-22T00:00:00
[ [ "Lee", "Jae-Weon", "" ], [ "Kim", "Kyungsub", "" ], [ "Lee", "Chul H.", "" ], [ "Jang", "Ji-ho", "" ] ]
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704.0838
Gil Shamir
Gil I. Shamir
Universal Source Coding for Monotonic and Fast Decaying Monotonic Distributions
Submitted to IEEE Transactions on Information Theory
null
null
null
cs.IT math.IT
null
We study universal compression of sequences generated by monotonic distributions. We show that for a monotonic distribution over an alphabet of size $k$, each probability parameter costs essentially $0.5 \log (n/k^3)$ bits, where $n$ is the coded sequence length, as long as $k = o(n^{1/3})$. Otherwise, for $k = O(n)$, the total average sequence redundancy is $O(n^{1/3+\epsilon})$ bits overall. We then show that there exists a sub-class of monotonic distributions over infinite alphabets for which redundancy of $O(n^{1/3+\epsilon})$ bits overall is still achievable. This class contains fast decaying distributions, including many distributions over the integers and geometric distributions. For some slower decays, including other distributions over the integers, redundancy of $o(n)$ bits overall is achievable, where a method to compute specific redundancy rates for such distributions is derived. The results are specifically true for finite entropy monotonic distributions. Finally, we study individual sequence redundancy behavior assuming a sequence is governed by a monotonic distribution. We show that for sequences whose empirical distributions are monotonic, individual redundancy bounds similar to those in the average case can be obtained. However, even if the monotonicity in the empirical distribution is violated, diminishing per symbol individual sequence redundancies with respect to the monotonic maximum likelihood description length may still be achievable.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 03:12:02 GMT" } ]
2007-07-13T00:00:00
[ [ "Shamir", "Gil I.", "" ] ]
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704.0839
Grigory Mikhalkin
Grigory Mikhalkin
Moduli spaces of rational tropical curves
For the Proceedings of the Gokova Geometry/Topology Conference
null
null
null
math.AG math.CO math.GT math.SG
null
This note is devoted to the definition of moduli spaces of rational tropical curves with n marked points. We show that this space has a structure of a smooth tropical variety of dimension n-3. We define the Deligne-Mumford compactification of this space and tropical $\psi$-class divisors.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 03:19:00 GMT" } ]
2007-05-23T00:00:00
[ [ "Mikhalkin", "Grigory", "" ] ]
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704.084
Yao-Bei Liu
Yao-Bei Liu, Jie-Fen Shen
Associated production of the charged Higgs boson and single top quark at the LHC
This paper has been withdrawn by the author(s) due to some mistakes in this paper
Mod.Phys.Lett.A24:143-150,2009
10.1142/S0217732309026711
null
hep-ph
null
The left-right twin Higgs(LRTH) model predicts the existence of the charged Higgs $\phi^{\pm}$. In this paper, we study the production of the charged Higgs boson $\phi^{-}$ with single top quark via the process $bg\to t\phi^{-}$ at the $CERN$ Large Hadron Collider(LHC). The numerical results show that the production cross section can reach the level of $10 pb$ in the reasonable parameter space of the LRTH model. We expect that, as long as it is not too heavy, the possible signatures of the heavy charged Higgs boson $\phi^{-}$ might be detected via the decay mode $\phi^{-}\to \bar{t}b$ at the LHC experiments.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 04:12:24 GMT" }, { "version": "v2", "created": "Sat, 8 Mar 2008 14:05:11 GMT" }, { "version": "v3", "created": "Thu, 13 Sep 2012 03:58:04 GMT" } ]
2012-09-14T00:00:00
[ [ "Liu", "Yao-Bei", "" ], [ "Shen", "Jie-Fen", "" ] ]
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704.0841
Bang-Rong Zhou
Bang-Rong Zhou (Graduate School of Chinese Academy of Sciences)
Difermion condensates in vacuum in 2-4D four-fermion interaction models
11 pages, 4 figures, General Poster 76 (Physical sciences) at 2007 AAAS Annual Meeting, San Francisco, Feb. 14-20, 2007, minor typos corrected,acknowledgment to financial supporter added
null
null
null
hep-th
null
Theoretical analysis of interplay between the condensates $<\bar{q}q>$ and $<qq>$ in vacuum is generally made by relativistic effective potentials in the mean field approximation in 2D, 3D and 4D models with two flavor and $N_c$ color massless fermions. It is found that in ground states of these models, interplay between the two condensates mainly depend on the ratio $G_S/H_S$ for 2D and 4D case or $G_S/H_P$ for 3D case, where $G_S$, $H_S$ and $H_P$ are respectively the coupling constants in a scalar $(\bar{q}q)$, a scalar $(qq)$ and a pseudoscalar $(qq)$ channel. In ground states of all the models, only pure $<\bar{q}q>$ condensates could exist if $G_S/H_S$ or $G_S/H_P$ is bigger than the critical value $2/N_c$, the ratio of the color numbers of the fermions entering into the condensates $<qq>$ and $<\bar{q}q>$. As $G_S/H_S$ or $G_S/H_P$ decreases to the region below $2/N_c$, differences of the models will manifest themselves. Depending on different models, and also on $N_c$ in 3D model, one will have or have no the coexistence phase of the two condensates, besides the pure $<qq>$ condensate phase. The $G_S-H_S$ (or $G_S-H_P$) phase diagrams in these models are given. The results also implicate a real constraint on two-flavor QCD-analogous NJL model.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 04:30:44 GMT" }, { "version": "v2", "created": "Sat, 23 Jun 2007 16:44:16 GMT" }, { "version": "v3", "created": "Sun, 17 Feb 2008 14:35:40 GMT" } ]
2008-02-17T00:00:00
[ [ "Zhou", "Bang-Rong", "", "Graduate School of Chinese Academy of Sciences" ] ]
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704.0842
Yanzhang He
Chengguang Bao
Oscillation bands of condensates on a ring: Beyond the mean field theory
7 pages, 8 figures
Phys. Rev. A 75 (2007) 063626
10.1103/PhysRevA.75.063626
null
cond-mat.other
null
The Hamiltonian of a N-boson system confined on a ring with zero spin and repulsive interaction is diagonalized. The excitation of a pair of p-wave-particles rotating reversely appears to be a basic mode. The fluctuation of many of these excited pairs provides a mechanism of oscillation, the states can be thereby classified into oscillation bands. The particle correlation is studied intuitively via the two-body densities. Bose-clustering originating from the symmetrization of wave functions is found, which leads to the appearance of 1-, 2-, and 3-cluster structures. The motion is divided into being collective and relative, this leads to the establishment of a relation between the very high vortex states and the low-lying states.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 05:08:44 GMT" } ]
2010-01-10T00:00:00
[ [ "Bao", "Chengguang", "" ] ]
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704.0843
Takuya Okabe
Takuya Okabe
Kadowaki-Woods Ratio of Strongly Coupled Fermi Liquids
null
Phys. Rev. B 76, 193109 (2007)
10.1103/PhysRevB.76.193109
null
cond-mat.str-el
null
On the basis of the Fermi liquid theory, the Kadowaki-Woods ratio $A/\gamma^2$ is evaluated by using a first principle band calculation for typical itinerant $d$ and $f$ electron systems. It is found as observed that the ratio for the $d$ electron systems is significantly smaller than the normal $f$ systems, even without considering their relatively weak correlation. The difference in the ratio value comes from different characters of the Fermi surfaces. By comparing Pd and USn$_3$ as typical cases, we discuss the importance of the Fermi surface dependence of the quasiparticle transport relaxation.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 06:09:57 GMT" }, { "version": "v2", "created": "Tue, 2 Oct 2007 01:11:15 GMT" } ]
2008-02-08T00:00:00
[ [ "Okabe", "Takuya", "" ] ]
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704.0844
Masayuki Matsuzaki
Masayuki Matsuzaki and Etsuchika Kobayashi (Fukuoka Univ. of Educ.)
Structure of Strange Dwarfs with Color Superconducting Core
8 pages 5 figures, J. Phys. G, accepted
J.Phys.G34:1621-1626,2007
10.1088/0954-3899/34/7/004
null
astro-ph hep-ph nucl-th
null
We study effects of two-flavor color superconductivity on the structure of strange dwarfs, which are stellar objects with similar masses and radii with ordinary white dwarfs but stabilized by the strange quark matter core. We find that unpaired quark matter is a good approximation to the core of strange dwarfs.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 05:42:41 GMT" } ]
2009-06-23T00:00:00
[ [ "Matsuzaki", "Masayuki", "", "Fukuoka Univ. of Educ." ], [ "Kobayashi", "Etsuchika", "", "Fukuoka Univ. of Educ." ] ]
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704.0845
Antti O. Niskanen
A. O. Niskanen, Y. Nakamura, J. P. Pekola
Information entropic superconducting microcooler
4 pages, 3 figures
null
10.1103/PhysRevB.76.174523
null
cond-mat.supr-con
null
We consider a design for a cyclic microrefrigerator using a superconducting flux qubit. Adiabatic modulation of the flux combined with thermalization can be used to transfer energy from a lower temperature normal metal thin film resistor to another one at higher temperature. The frequency selectivity of photonic heat conduction is achieved by including the hot resistor as part of a high frequency LC resonator and the cold one as part of a low-frequency oscillator while keeping both circuits in the underdamped regime. We discuss the performance of the device in an experimentally realistic setting. This device illustrates the complementarity of information and thermodynamic entropy as the erasure of the quantum bit directly relates to the cooling of the resistor.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:05:03 GMT" } ]
2009-11-13T00:00:00
[ [ "Niskanen", "A. O.", "" ], [ "Nakamura", "Y.", "" ], [ "Pekola", "J. P.", "" ] ]
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704.0846
Heidi Haynal
Heidi Haynal
PI degree parity in q-skew polynomial rings
43 pages; Submitted to the Journal of Algebra
null
null
null
math.RA math.QA
null
For k a field of arbitrary characteristic, and R a k-algebra, we show that the PI degree of an iterated skew polynomial ring R[x_1;\tau_1,\delta_1]...b[x_n;\tau_n,\delta_n] agrees with the PI degree of R[x_1;\tau_1]...b[x_n;\tau_n] when each (\tau_i,\delta_i) satisfies a q_i-skew relation for q_i \in k^{\times} and extends to a higher q_i-skew \tau_i-derivation. We confirm the quantum Gel'fand-Kirillov conjecture for various quantized coordinate rings, and calculate their PI degrees. We extend these results to completely prime factor algebras.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:10:19 GMT" } ]
2007-05-23T00:00:00
[ [ "Haynal", "Heidi", "" ] ]
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704.0847
Dorin Poenaru
D. N. Poenaru, R. A. Gherghescu, A. V. Solov'yov, W. Greiner
Semi-spheroidal Quantum Harmonic Oscillator
4 pages, 3 figures, 1 table
null
10.1016/j.physleta.2008.06.054
null
physics.atm-clus
null
A new single-particle shell model is derived by solving the Schr\"odinger equation for a semi-spheroidal potential well. Only the negative parity states of the $Z(z)$ component of the wave function are allowed, so that new magic numbers are obtained for oblate semi-spheroids, semi-sphere and prolate semi-spheroids. The semi-spherical magic numbers are identical with those obtained at the oblate spheroidal superdeformed shape: 2, 6, 14, 26, 44, 68, 100, 140, ... The superdeformed prolate magic numbers of the semi-spheroidal shape are identical with those obtained at the spherical shape of the spheroidal harmonic oscillator: 2, 8, 20, 40, 70, 112, 168 ...
[ { "version": "v1", "created": "Fri, 6 Apr 2007 17:51:47 GMT" } ]
2009-11-13T00:00:00
[ [ "Poenaru", "D. N.", "" ], [ "Gherghescu", "R. A.", "" ], [ "Solov'yov", "A. V.", "" ], [ "Greiner", "W.", "" ] ]
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704.0848
Hyeong-Chai Jeong
Hyeong-Chai Jeong
Growing Perfect Decagonal Quasicrystals by Local Rules
4pages, 2figures
Phys. Rev. Lett. 98, 135501 (2007)
10.1103/PhysRevLett.98.135501
null
cond-mat.dis-nn cond-mat.stat-mech math-ph math.MP
null
A local growth algorithm for a decagonal quasicrystal is presented. We show that a perfect Penrose tiling (PPT) layer can be grown on a decapod tiling layer by a three dimensional (3D) local rule growth. Once a PPT layer begins to form on the upper layer, successive 2D PPT layers can be added on top resulting in a perfect decagonal quasicrystalline structure in bulk with a point defect only on the bottom surface layer. Our growth rule shows that an ideal quasicrystal structure can be constructed by a local growth algorithm in 3D, contrary to the necessity of non-local information for a 2D PPT growth.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:07:20 GMT" } ]
2015-05-13T00:00:00
[ [ "Jeong", "Hyeong-Chai", "" ] ]
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704.0849
Dr. Anirudh Pradhan
Anirudh Pradhan, J. P. Shahi and C. V. Singh
LRS Bianchi Type-V Viscous Fluid Universe With a Time Dependent Cosmological Term $\Lambda$
13 pages, no figure
null
null
null
gr-qc
null
An LRS Bianchi type-V cosmological models representing a viscous fluid distribution with a time dependent cosmological term $\Lambda$ is investigated. To get a determinate solution, the viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density. It turns out that the cosmological term $\Lambda(t)$ is a decreasing function of time, which is consistent with recent observations of type Ia supernovae. Various physical and kinematic features of these models have also been explored.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:08:10 GMT" }, { "version": "v2", "created": "Mon, 6 Aug 2007 05:58:45 GMT" } ]
2007-08-06T00:00:00
[ [ "Pradhan", "Anirudh", "" ], [ "Shahi", "J. P.", "" ], [ "Singh", "C. V.", "" ] ]
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704.085
Jun Sato
Jun Sato, Masahiro Shiroishi
Density matrix elements and entanglement entropy for the spin-1/2 XXZ chain at $\Delta$=1/2
12 pages, 3 eps figures, 2 authors
J. Phys. A: Math. Theor. 40 8739-8749 (2007)
10.1088/1751-8113/40/30/009
null
cond-mat.stat-mech
null
We have analytically obtained all the density matrix elements up to six lattice sites for the spin-1/2 Heisenberg XXZ chain at $\Delta=1/2$. We use the multiple integral formula of the correlation function for the massless XXZ chain derived by Jimbo and Miwa. As for the spin-spin correlation functions, we have newly obtained the fourth- and fifth-neighbour transverse correlation functions. We have calculated all the eigenvalues of the density matrix and analyze the eigenvalue-distribution. Using these results the exact values of the entanglement entropy for the reduced density matrix up six lattice sites have been obtained. We observe that our exact results agree quite well with the asymptotic formula predicted by the conformal field theory.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:19:49 GMT" } ]
2009-11-13T00:00:00
[ [ "Sato", "Jun", "" ], [ "Shiroishi", "Masahiro", "" ] ]
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704.0851
Milan Janjic
Milan Janjic
Counting on rectangular areas
null
null
null
null
math.CO
null
In the first section of this paper we prove a theorem for the number of columns of a rectangular area that are identical to the given one. In the next section we apply this theorem to derive several combinatorial identities by counting specified subsets of a finite set.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:29:24 GMT" } ]
2007-05-23T00:00:00
[ [ "Janjic", "Milan", "" ] ]
[ -0.04013592, -0.0833897069, 0.1192187443, -0.0031145632, -0.0120222801, -0.0567028858, -0.0458431989, -0.0051193773, -0.1069058105, -0.0039666919, 0.0617231801, -0.0674833059, 0.046767991, 0.0330282412, 0.1378202438, 0.0763612986, 0.0433594771, 0.0380221121, 0.0375465043, 0.0656337216, -0.046952948, 0.0576540977, -0.0399773829, 0.0718166083, 0.0168708265, 0.0241766721, -0.0686987415, 0.002095642, 0.1271455139, -0.0191563796, -0.0112229967, -0.0112890527, -0.1186902896, -0.0451297909, -0.0179937854, 0.0880929232, -0.048300501, 0.0599264428, -0.0638898313, 0.088568531, -0.0247183368, 0.1275682747, -0.0514183678, 0.0522903129, 0.061511796, 0.0283514429, 0.1087553948, 0.0216665268, 0.0071208891, 0.0801133066, -0.0235293191, -0.0006168024, 0.044310689, -0.1728037596, 0.0054496601, -0.0337680727, -0.0319184922, 0.10035301, 0.0383656062, -0.0849222168, 0.0555931367, -0.1670964807, -0.0061201332, 0.0151929911, -0.1011985317, -0.0413777828, 0.0171086285, 0.0070944661, 0.0870360211, -0.0337944962, -0.1403568238, 0.0926904604, 0.1365519613, 0.0888327584, 0.0035934728, -0.04013592, 0.0626215488, 0.1019912139, -0.0229480229, 0.1380316317, 0.1473323852, -0.0513919443, 0.0200415365, 0.0481419638, -0.0097367261, 0.0335566923, 0.0168047696, -0.0243219975, -0.0403473005, -0.0198830012, -0.0251410976, -0.0321034528, -0.0504671521, 0.0641540587, 0.0777881145, -0.014439947, 0.0684345141, -0.0051391944, 0.0161045715, 0.0802189931, -0.0373087004, -0.0233179387, 0.064682506, 0.0477720499, 0.0040855934, 0.1712184101, 0.0695442632, -0.1081741005, -0.0998245552, 0.02241957, -0.0335038491, -0.1320072711, 0.0037916421, 0.0013021384, 0.0787921771, 0.0953855589, -0.0193017051, 0.0019338035, -0.0490931794, 0.0341115668, 0.0150476666, -0.0842880756, 0.122706525, -0.0350627825, 0.0690686628, -0.0954384059, 0.0119231949, -0.052871611, -0.0115863075, 0.0667434707, 0.0396338888, 0.0035967755, 0.0503086187, 0.0282457527, -0.0841295347, -0.0843937621, 0.0944343507, 0.0276908781, 0.1140399128, -0.0230140798, 0.0694385767, 0.095068492, 0.0436765477, 0.0416948535, 0.057337027, -0.070019871, -0.0683288276, 0.0561744347, 0.0381542258, 0.0119430125, 0.0074313544, -0.0053340611, 0.0592394546, -0.0276644547, -0.0774182007, -0.1104464382, 0.0998245552, 0.0302538704, 0.0690686628, -0.0776295811, 0.019420607, -0.1376088709, -0.050176505, 0.038973324, 0.0009801131, 0.072714977, -0.0743003339, -0.0192092247, -0.0796905383, -0.0208474267, 0.0444163792, -0.0432009399, 0.0280343723, 0.0244276877, -0.0342436805, -0.0076361294, -0.1031538025, 0.0275059193, -0.0127026616, -0.0957554802, 0.0081117358, 0.0306766313, 0.0760970712, -0.04483914, 0.0828084052, -0.0312579274, 0.101515606, -0.061511796, -0.0045050522, 0.0321562961, -0.0208606385, -0.0013269096, -0.0304124057, 0.140039742, 0.0286420919, -0.1417307854, 0.0058757244, -0.0803775266, -0.0570199564, -0.0242427289, 0.0078739328, -0.052818764, 0.010502981, 0.1046334729, -0.0257884506, 0.0054661739, -0.0075634676, 0.0093998378, -0.0182051677, -0.0729792044, -0.0137793822, -0.0358290374, 0.024057772, -0.0249825623, -0.0336095393, 0.0259866212, 0.0169368833, 0.0703897923, -0.0197376776, 0.1022554338, -0.0107672065, 0.0475870892, 0.0271624252, -0.0444428027, -0.0175842363, 0.07266213, 0.0356969237, -0.0523960032, 0.0104897693, 0.0029477705, 0.0895197466, -0.0557516739, -0.0168179814, 0.0135151567, 0.0173067991, -0.007424749, -0.0450505204, -0.0653166547, -0.0681702942, 0.0235161074, 0.0467151441, 0.0784751028, 0.0288270488, -0.0790035576, 0.016078148, 0.0281664841, -0.0542191602, 0.0251278859, -0.0830197856, 0.0270038899, 0.0157478657, 0.0357233472, 0.0096574575, -0.0455261283, -0.025061829, 0.0794791579 ]
704.0852
Dmitri Peressounko
D.Peressounko (for the PHENIX Collaboration)
Bose-Einstein correlations of direct photons in Au+Au collisions at $\sqrt{s_{NN}} = 200$ GeV
6 pages, 3 figures, Proceedings of Poster Session, 19th International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions (Quark Matter 2006), November 14-20, 2006, Shanghai, P.R.China
Int.J.Mod.Phys.E16:2235-2240,2007
10.1142/S021830130700774X
null
nucl-ex
null
The current status of the analysis of direct photon Bose-Einstein correlations in Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV done by the PHENIX collaboration is summarized. All possible sources of distortion of the two-photon correlation function are discussed and methods to control them in the PHENIX experiment are presented.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:32:57 GMT" } ]
2010-11-26T00:00:00
[ [ "Peressounko", "D.", "", "for the PHENIX Collaboration" ] ]
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704.0853
Hao Yin
Hao Yin
Normalized Ricci flow on nonparabolic surfaces
Some false statements corrected. Details of estimate and a discussion on Uniformization added. 14 pages
null
null
null
math.DG
null
This paper studies normalized Ricci flow on a nonparabolic surface, whose scalar curvature is asymptotically -1 in an integral sense. By a method initiated by R. Hamilton, the flow is shown to converge to a metric of constant scalar curvature -1. A relative estimate of Green's function is proved as a tool.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 07:53:53 GMT" }, { "version": "v2", "created": "Tue, 5 Jun 2007 01:44:15 GMT" } ]
2007-06-13T00:00:00
[ [ "Yin", "Hao", "" ] ]
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704.0854
Xifeng Ren
Xi-Feng Ren, Pei Zhang, Guo-Ping Guo, Yun-Feng Huang, Zhi-Wei Wang, Guang-Can Guo
Polarization properties of subwavelength hole arrays consisting of rectangular holes
8 pages, 4 figures
Appl.Phys.B 91 601(2008)
10.1007/s00340-008-3027-1
null
physics.optics
null
Influence of hole shape on extraordinary optical transmission was investigated using hole arrays consisting of rectangular holes with different aspect ratio. It was found that the transmission could be tuned continuously by rotating the hole array. Further more, a phase was generated in this process, and linear polarization states could be changed to elliptical polarization states. This phase was correlated with the aspect ratio of the holes. An intuitional model was presented to explain these results.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:09:02 GMT" }, { "version": "v2", "created": "Wed, 4 Jun 2008 01:41:36 GMT" } ]
2009-11-13T00:00:00
[ [ "Ren", "Xi-Feng", "" ], [ "Zhang", "Pei", "" ], [ "Guo", "Guo-Ping", "" ], [ "Huang", "Yun-Feng", "" ], [ "Wang", "Zhi-Wei", "" ], [ "Guo", "Guang-Can", "" ] ]
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704.0855
David Wilkowski
Thierry Chaneliere (LAC), Ling Xiang He, Robin Kaiser (INLN), David Wilkowski (INLN)
Three dimensional cooling and trapping with a narrow line
null
null
10.1140/epjd/e2007-00329-8
null
physics.atom-ph
null
The intercombination line of Strontium at 689nm is successfully used in laser cooling to reach the photon recoil limit with Doppler cooling in a magneto-optical traps (MOT). In this paper we present a systematic study of the loading efficiency of such a MOT. Comparing the experimental results to a simple model allows us to discuss the actual limitation of our apparatus. We also study in detail the final MOT regime emphasizing the role of gravity on the position, size and temperature along the vertical and horizontal directions. At large laser detuning, one finds an unusual situation where cooling and trapping occur in the presence of a high bias magnetic field.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:06:59 GMT" }, { "version": "v2", "created": "Fri, 10 Aug 2007 09:07:23 GMT" } ]
2015-05-13T00:00:00
[ [ "Chaneliere", "Thierry", "", "LAC" ], [ "He", "Ling Xiang", "", "INLN" ], [ "Kaiser", "Robin", "", "INLN" ], [ "Wilkowski", "David", "", "INLN" ] ]
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704.0856
Iosif Khriplovich
I.B. Khriplovich and D.V. Matvienko
Approximate Selection Rule for Orbital Angular Momentum in Atomic Radiative Transitions
5 pages, 1 figure
Phys. Lett. A 368 (2007) 348
10.1016/j.physleta.2007.04.031
null
physics.atom-ph physics.class-ph
null
We demonstrate that radiative transitions with \Delta l = - 1 are strongly dominating for all values of n and l, except small region where l << n.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:08:30 GMT" } ]
2009-11-13T00:00:00
[ [ "Khriplovich", "I. B.", "" ], [ "Matvienko", "D. V.", "" ] ]
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704.0857
Ivan L. Zhogin
I.L. Zhogin
Extrasolar scale change in Newton's Law from 5D `plain' R^2-gravity
Latex, 10 pages, 1 figure (poster.pdf submitted to NPPD-07 is addon)
null
null
null
astro-ph gr-qc hep-ph
null
Galactic rotation curves and lack of direct observations of Dark Matter may indicate that General Relativity is not valid (on galactic scale) and should be replaced with another theory. There is the only variant of Absolute Parallelism which solutions are free of arising singularities, if D=5 (there is no room for changes). This variant does not have a Lagrangian, nor match GR: an equation of `plain' R^2-gravity (ie without R-term) is in sight instead. Arranging an expanding O_4-symmetrical solution as the basis of 5D cosmological model, and probing a universal_function of mass distribution (along very-very long the extra dimension) to place into bi-Laplace equation (R^2 gravity), one can derive the Law of Gravitation: 1/r^2 transforms to 1/r with distance (not with acceleration).
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:47:44 GMT" } ]
2009-04-16T00:00:00
[ [ "Zhogin", "I. L.", "" ] ]
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704.0858
Mohamed Kaaniche
Eric Alata (LAAS), Vincent Nicomette (LAAS), Mohamed Ka\^aniche (LAAS), Marc Dacier (LAAS), Matthieu Herrb (LAAS)
Lessons Learned from the deployment of a high-interaction honeypot
null
Proc. 6th European Dependable Computing Conference (EDCC-6), Coimbra (Portugal), 18-20 octobre 2006 (18/10/2006) 39-44
null
null
cs.CR
null
This paper presents an experimental study and the lessons learned from the observation of the attackers when logged on a compromised machine. The results are based on a six months period during which a controlled experiment has been run with a high interaction honeypot. We correlate our findings with those obtained with a worldwide distributed system of lowinteraction honeypots.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:22:50 GMT" } ]
2016-08-14T00:00:00
[ [ "Alata", "Eric", "", "LAAS" ], [ "Nicomette", "Vincent", "", "LAAS" ], [ "Kaâniche", "Mohamed", "", "LAAS" ], [ "Dacier", "Marc", "", "LAAS" ], [ "Herrb", "Matthieu", "", "LAAS" ] ]
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704.0859
B\'alint Farkas
Balint Farkas, Bela Nagy
Transfinite diameter, Chebyshev constant and energy on locally compact spaces
null
null
null
null
math.CA
null
We study the relationship between transfinite diameter, Chebyshev constant and Wiener energy in the abstract linear potential analytic setting pioneered by Choquet, Fuglede and Ohtsuka. It turns out that, whenever the potential theoretic kernel has the maximum principle, then all these quantities are equal for all compact sets. For continuous kernels even the converse statement is true: if the Chebyshev constant of any compact set coincides with its transfinite diameter, the kernel must satisfy the maximum principle. An abundance of examples is provided to show the sharpness of the results.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:30:02 GMT" } ]
2007-05-23T00:00:00
[ [ "Farkas", "Balint", "" ], [ "Nagy", "Bela", "" ] ]
[ -0.0379307307, -0.0031614366, 0.0314223692, 0.0719043761, -0.0103417868, 0.0119363349, 0.0320732072, -0.055295039, -0.0766945332, 0.0393105038, 0.0669059604, 0.0019996942, -0.1571378857, 0.0137326429, 0.1036131158, 0.0048454753, -0.0162578877, 0.0842442364, 0.0977816284, 0.0197073184, -0.0129516395, -0.0871079117, 0.0281421561, 0.0103482949, -0.0508433208, -0.0254867449, 0.0320211388, 0.1167339757, 0.1417260766, 0.013433258, -0.062896803, -0.0282983556, -0.0518586263, -0.1163174361, -0.0616472028, 0.1719248742, -0.0252394266, 0.039779108, 0.0634174719, -0.057429783, -0.0773714036, 0.1109024808, -0.0788813457, 0.0546181723, 0.005239231, -0.0364207923, -0.0404559746, -0.0010144908, 0.0285066236, -0.0032541808, -0.1056957915, 0.0852335021, -0.0296781287, -0.0301727653, -0.0744556561, 0.1119438186, -0.0690407008, 0.0646150112, 0.0184316803, -0.0185358133, -0.0118387099, -0.0247838404, 0.07570526, 0.05732565, -0.1006973684, -0.0223366972, -0.0540975034, -0.0493333824, 0.0309537686, 0.1207951903, -0.0420700498, 0.0488647781, -0.0510776229, 0.0634695441, 0.0699258372, 0.0896071196, 0.0267623831, 0.0673224926, -0.0426688194, 0.0594083257, -0.0168826897, 0.0333748795, 0.0213734601, -0.0507652201, 0.027074784, -0.0609703325, -0.0229614992, -0.0402997769, -0.0936683416, 0.0568049811, 0.0299644973, -0.0787772089, 0.0353534222, 0.0406121761, 0.0972088873, 0.0064009735, 0.1748406291, 0.0125546297, -0.0614910014, 0.0690407008, -0.0236644037, -0.0266842823, 0.0904401913, -0.0018776624, 0.1509939879, 0.0471986383, 0.0097885756, -0.0156070516, -0.0263979156, 0.0128670307, 0.0022779265, -0.0830987617, -0.0477453396, 0.053941302, 0.0100293849, -0.0657084212, 0.0032004868, -0.055295039, -0.1127768904, -0.0264109317, 0.0285326578, 0.0183796138, 0.0995519012, 0.0202800557, 0.0074585825, -0.0804954171, -0.0340517461, -0.0233780351, -0.0832028985, -0.0751845911, 0.0814326182, -0.0471986383, 0.0007077843, -0.0072438065, -0.0581066534, -0.0508693531, -0.0172211248, 0.0170779414, 0.1002287716, -0.046625901, -0.0118712513, 0.057429783, 0.0522491261, -0.0086365957, 0.025903279, 0.0632092059, 0.0229224488, 0.0626364723, 0.08080782, -0.0169868246, 0.0126132052, -0.0204492714, 0.0389981046, -0.0254216604, -0.0395708382, -0.0653960183, 0.0765383318, 0.0972088873, 0.0416795462, -0.0646150112, 0.0419919491, 0.1048106551, -0.172237277, 0.0160235856, 0.0771110654, 0.022310663, -0.0083762612, -0.0109796058, -0.0781524032, -0.1632817835, -0.0172862075, -0.0599810593, -0.0373059288, -0.0459750667, 0.0117475931, 0.0164271053, -0.0289231595, -0.0572735816, -0.0376443639, 0.0485003106, 0.0174554251, 0.0934600756, 0.0782044753, -0.0256169122, -0.0843483657, 0.0166874398, -0.0223366972, 0.0805995539, -0.006768696, -0.0565967113, -0.047797408, 0.0537330322, 0.1077784672, 0.0574818514, -0.001890679, -0.1302713603, -0.0210350249, 0.0626885369, -0.0107387966, 0.0216207765, 0.0806516185, 0.0063196192, 0.1115272865, 0.0056590205, -0.0156200677, -0.0040579634, 0.0923666656, 0.0270487517, -0.0529520288, 0.0142402956, -0.0517284572, -0.0298343301, 0.0891385227, -0.007562716, 0.0149562154, 0.1056437269, -0.0336872786, 0.0539933667, -0.004015659, 0.1173587739, -0.0420179814, 0.0949700102, 0.0530561656, -0.0083046695, 0.0675307587, 0.0349108502, 0.0123138204, -0.0374360979, -0.0247708242, 0.062896803, 0.0704985708, -0.0962196216, -0.1142347604, -0.0612827316, 0.0770590007, -0.0087277126, 0.0879930481, 0.0511296876, -0.0544619709, -0.1530766636, -0.1242316067, 0.0084218197, 0.0061080973, 0.0720085129, -0.0457147323, 0.0263588652, -0.0621678717, 0.060085196, -0.0079662343, -0.0224668644, -0.0808598846, 0.105123058, 0.0130557735, 0.0231827833, 0.000427518, -0.0199546367 ]
704.086
Mohamed Kaaniche
Cristina Simache (LAAS), Mohamed Kaaniche (LAAS)
Availability assessment of SunOS/Solaris Unix Systems based on Syslogd and wtmpx logfiles : a case study
null
Proc. 2005 IEEE Pacific Rim International Symposium on Dependable Computing (PRDC'2005), Changsha, Hunan (Chine), 12-14 D{\'e}cembre 2005 (18/12/2005) 49-56
null
null
cs.PF
null
This paper presents a measurement-based availability assessment study using field data collected during a 4-year period from 373 SunOS/Solaris Unix workstations and servers interconnected through a local area network. We focus on the estimation of machine uptimes, downtimes and availability based on the identification of failures that caused total service loss. Data corresponds to syslogd event logs that contain a large amount of information about the normal activity of the studied systems as well as their behavior in the presence of failures. It is widely recognized that the information contained in such event logs might be incomplete or imperfect. The solution investigated in this paper to address this problem is based on the use of auxiliary sources of data obtained from wtmpx files maintained by the SunOS/Solaris Unix operating system. The results obtained suggest that the combined use of wtmpx and syslogd log files provides more complete information on the state of the target systems that is useful to provide availability estimations that better reflect reality.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:24:47 GMT" } ]
2007-05-23T00:00:00
[ [ "Simache", "Cristina", "", "LAAS" ], [ "Kaaniche", "Mohamed", "", "LAAS" ] ]
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704.0861
Mohamed Kaaniche
Mohamed Kaaniche (LAAS), Y. Deswarte (LAAS), Eric Alata (LAAS), Marc Dacier (SC), Vincent Nicomette (LAAS)
Empirical analysis and statistical modeling of attack processes based on honeypots
null
IEEE/IFIP International Conference on Dependable Systems and Networks (DSN-2006) (25/06/2006) 119-124
null
null
cs.PF cs.CR
null
Honeypots are more and more used to collect data on malicious activities on the Internet and to better understand the strategies and techniques used by attackers to compromise target systems. Analysis and modeling methodologies are needed to support the characterization of attack processes based on the data collected from the honeypots. This paper presents some empirical analyses based on the data collected from the Leurr{\'e}.com honeypot platforms deployed on the Internet and presents some preliminary modeling studies aimed at fulfilling such objectives.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:50:34 GMT" } ]
2007-05-23T00:00:00
[ [ "Kaaniche", "Mohamed", "", "LAAS" ], [ "Deswarte", "Y.", "", "LAAS" ], [ "Alata", "Eric", "", "LAAS" ], [ "Dacier", "Marc", "", "SC" ], [ "Nicomette", "Vincent", "", "LAAS" ] ]
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704.0862
Adam Leroy
Adam Leroy, John Cannon, Fabian Walter, Alberto Bolatto, Axel Weiss
The Low CO Content of the Extremely Metal Poor Galaxy I Zw 18
5 pages in emulateapj style, accepted by the Astrophysical Journal
Astrophys.J.663:990-994,2007
10.1086/518501
null
astro-ph
null
We present sensitive molecular line observations of the metal-poor blue compact dwarf I Zw 18 obtained with the IRAM Plateau de Bure interferometer. These data constrain the CO J=1-0 luminosity within our 300 pc (FWHM) beam to be L_CO < 1 \times 10^5 K km s^-1 pc^2 (I_CO < 1 K km s^-1), an order of magnitude lower than previous limits. Although I Zw 18 is starbursting, it has a CO luminosity similar to or less than nearby low-mass irregulars (e.g. NGC 1569, the SMC, and NGC 6822). There is less CO in I Zw 18 relative to its B-band luminosity, HI mass, or star formation rate than in spiral or dwarf starburst galaxies (including the nearby dwarf starburst IC 10). Comparing the star formation rate to our CO upper limit reveals that unless molecular gas forms stars much more efficiently in I Zw 18 than in our own galaxy, it must have a very low CO-to-H_2 ratio, \sim 10^-2 times the Galactic value. We detect 3mm continuum emission, presumably due to thermal dust and free-free emission, towards the radio peak.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 08:50:39 GMT" } ]
2009-06-23T00:00:00
[ [ "Leroy", "Adam", "" ], [ "Cannon", "John", "" ], [ "Walter", "Fabian", "" ], [ "Bolatto", "Alberto", "" ], [ "Weiss", "Axel", "" ] ]
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704.0863
Zhanwen Han
Z. Han, Ph. Podsiadlowski, A.E. Lynas-Gray
A binary model for the UV-upturn of elliptical galaxies (MNRAS version)
accepted for publication in MNRAS, 24 pages, 15 figures, 2 tables
null
10.1111/j.1365-2966.2007.12151.x
UVX-MN-25June2007
astro-ph
null
The discovery of a flux excess in the far-ultraviolet (UV) spectrum of elliptical galaxies was a major surprise in 1969. While it is now clear that this UV excess is caused by an old population of hot helium-burning stars without large hydrogen-rich envelopes, rather than young stars, their origin has remained a mystery. Here we show that these stars most likely lost their envelopes because of binary interactions, similar to the hot subdwarf population in our own Galaxy. We have developed an evolutionary population synthesis model for the far-UV excess of elliptical galaxies based on the binary model developed by Han et al (2002, 2003) for the formation of hot subdwarfs in our Galaxy. Despite its simplicity, it successfully reproduces most of the properties of elliptical galaxies with a UV excess: the range of observed UV excesses, both in $(1550-V)$ and $(2000-V)$, and their evolution with redshift. We also present colour-colour diagrams for use as diagnostic tools in the study of elliptical galaxies. The model has major implications for understanding the evolution of the UV excess and of elliptical galaxies in general. In particular, it implies that the UV excess is not a sign of age, as had been postulated previously, and predicts that it should not be strongly dependent on the metallicity of the population, but exists universally from dwarf ellipticals to giant ellipticals.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:55:07 GMT" }, { "version": "v2", "created": "Mon, 30 Apr 2007 03:12:38 GMT" }, { "version": "v3", "created": "Mon, 25 Jun 2007 11:49:33 GMT" } ]
2009-11-13T00:00:00
[ [ "Han", "Z.", "" ], [ "Podsiadlowski", "Ph.", "" ], [ "Lynas-Gray", "A. E.", "" ] ]
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704.0864
Istvan Horvath
Z. Bagoly, I. Csabai, A. Meszaros, P. Meszaros, I. Horvath, L.G. Balazs, R. Vavrek
Redshifts of the Long Gamma-Ray Bursts
published in Baltic Astronomy
Baltic Astron. 13 (2004) 227
null
null
astro-ph
null
The low energy spectra of some gamma-ray bursts' show excess components beside the power-law dependence. The consequences of such a feature allows to estimate the gamma photometric redshift of the long gamma-ray bursts in the BATSE Catalog. There is good correlation between the measured optical and the estimated gamma photometric redshifts. The estimated redshift values for the long bright gamma-ray bursts are up to z=4, while for the the faint long bursts - which should be up to z=20 - the redshifts cannot be determined unambiguously with this method. The redshift distribution of all the gamma-ray bursts with known optical redshift agrees quite well with the BATSE based gamma photometric redshift distribution.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 09:09:15 GMT" } ]
2007-05-23T00:00:00
[ [ "Bagoly", "Z.", "" ], [ "Csabai", "I.", "" ], [ "Meszaros", "A.", "" ], [ "Meszaros", "P.", "" ], [ "Horvath", "I.", "" ], [ "Balazs", "L. G.", "" ], [ "Vavrek", "R.", "" ] ]
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704.0865
Mohamed Kaaniche
Ana-Elena Rugina (LAAS), Karama Kanoun (LAAS), Mohamed Kaaniche (LAAS)
An architecture-based dependability modeling framework using AADL
null
Proc. 10th IASTED International Conference on Software Engineering and Applications (SEA'2006), Dallas (USA), 13-15 November2006 (13/11/2006) 222-227
null
null
cs.PF cs.SE
null
For efficiency reasons, the software system designers' will is to use an integrated set of methods and tools to describe specifications and designs, and also to perform analyses such as dependability, schedulability and performance. AADL (Architecture Analysis and Design Language) has proved to be efficient for software architecture modeling. In addition, AADL was designed to accommodate several types of analyses. This paper presents an iterative dependency-driven approach for dependability modeling using AADL. It is illustrated on a small example. This approach is part of a complete framework that allows the generation of dependability analysis and evaluation models from AADL models to support the analysis of software and system architectures, in critical application domains.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 09:33:06 GMT" } ]
2007-05-23T00:00:00
[ [ "Rugina", "Ana-Elena", "", "LAAS" ], [ "Kanoun", "Karama", "", "LAAS" ], [ "Kaaniche", "Mohamed", "", "LAAS" ] ]
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704.0866
Ahmed Zeriahi
S.Benelkourchi, V.Guedj and A.Zeriahi
A priori estimates for weak solutions of complex Monge-Amp\`ere equations
Corrected typos, added details to one proof
Ann. Scuola Norm. Sup. Pisa, Cl. Sci. (5) Vol. VII (2008), 1-16
null
null
math.CV math.DG
null
Let $X$ be a compact K\"ahler manifold and $\om$ a smooth closed form of bidegree $(1,1)$ which is nonnegative and big. We study the classes ${\mathcal E}_{\chi}(X,\om)$ of $\om$-plurisubharmonic functions of finite weighted Monge-Amp\`ere energy. When the weight $\chi$ has fast growth at infinity, the corresponding functions are close to be bounded. We show that if a positive Radon measure is suitably dominated by the Monge-Amp\`ere capacity, then it belongs to the range of the Monge-Amp\`ere operator on some class ${\mathcal E}_{\chi}(X,\om)$. This is done by establishing a priori estimates on the capacity of sublevel sets of the solutions. Our result extends U.Cegrell's and S.Kolodziej's results and puts them into a unifying frame. It also gives a simple proof of S.T.Yau's celebrated a priori ${\mathcal C}^0$-estimate.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:06:50 GMT" }, { "version": "v2", "created": "Fri, 22 Feb 2008 08:17:56 GMT" } ]
2008-02-22T00:00:00
[ [ "Benelkourchi", "S.", "" ], [ "Guedj", "V.", "" ], [ "Zeriahi", "A.", "" ] ]
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704.0867
Yanzhang He
Shuping Situ, Yanzhang He and Chengguang Bao
Density oscillation in highly flattened quantum elliptic rings and tunable strong dipole radiation
5 pages, 8 figures
null
null
null
cond-mat.other
null
A narrow elliptic ring containing an electron threaded by a magnetic field B is studied. When the ring is highly flattened, the increase of B would lead to a big energy gap between the ground and excited states, and therefore lead to a strong emission of dipole photons. The photon frequency can be tuned in a wide range by changing B and/or the shape of the ellipse. The particle density is found to oscillate from a pattern of distribution to another pattern back and forth against $B$. This is a new kind of Aharonov-Bohm oscillation originating from symmetry breaking and is different from the usual oscillation of persistent current.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:11:40 GMT" } ]
2007-05-23T00:00:00
[ [ "Situ", "Shuping", "" ], [ "He", "Yanzhang", "" ], [ "Bao", "Chengguang", "" ] ]
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704.0868
Andrea Bertoni
Juan I. Climente, Andrea Bertoni, Guido Goldoni, Massimo Rontani, Elisa Molinari
Effect of electron-electron interaction on the phonon-mediated spin relaxation in quantum dots
12 pages, 10 figures. Revised version. Changes in section V (simulation of PRL 98, 126601 experiment)
Phys. Rev. B 76, 085305 (2007)
10.1103/PhysRevB.76.085305
null
cond-mat.mes-hall
null
We estimate the spin relaxation rate due to spin-orbit coupling and acoustic phonon scattering in weakly-confined quantum dots with up to five interacting electrons. The Full Configuration Interaction approach is used to account for the inter-electron repulsion, and Rashba and Dresselhaus spin-orbit couplings are exactly diagonalized. We show that electron-electron interaction strongly affects spin-orbit admixture in the sample. Consequently, relaxation rates strongly depend on the number of carriers confined in the dot. We identify the mechanisms which may lead to improved spin stability in few electron (>2) quantum dots as compared to the usual one and two electron devices. Finally, we discuss recent experiments on triplet-singlet transitions in GaAs dots subject to external magnetic fields. Our simulations are in good agreement with the experimental findings, and support the interpretation of the observed spin relaxation as being due to spin-orbit coupling assisted by acoustic phonon emission.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:28:43 GMT" }, { "version": "v2", "created": "Mon, 11 Jun 2007 09:30:17 GMT" } ]
2009-11-13T00:00:00
[ [ "Climente", "Juan I.", "" ], [ "Bertoni", "Andrea", "" ], [ "Goldoni", "Guido", "" ], [ "Rontani", "Massimo", "" ], [ "Molinari", "Elisa", "" ] ]
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704.0869
O. Golinelli
O. Golinelli, K. Mallick (Cea Saclay, France)
Connected Operators for the Totally Asymmetric Exclusion Process
10 pages
J. Phys. A: Math. Theor. 40 (2007) 13231-13236
10.1088/1751-8113/40/44/004
null
cond-mat.stat-mech math-ph math.MP
null
We fully elucidate the structure of the hierarchy of the connected operators that commute with the Markov matrix of the Totally Asymmetric Exclusion Process (TASEP). We prove for the connected operators a combinatorial formula that was conjectured in a previous work. Our derivation is purely algebraic and relies on the algebra generated by the local jump operators involved in the TASEP. Keywords: Non-Equilibrium Statistical Mechanics, ASEP, Exact Results, Algebraic Bethe Ansatz.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:15:25 GMT" } ]
2009-11-13T00:00:00
[ [ "Golinelli", "O.", "", "Cea Saclay, France" ], [ "Mallick", "K.", "", "Cea Saclay, France" ] ]
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704.087
Evgeniy Bessonov
E.G. Bessonov, M.V. Gorbunkov (Lebedev Phys. Inst. RAS, Moscow, Russia), A.A.Mikhailichenko (Cornell University, Ithaca, NY, U.S.A.)
Proposal for an Enhanced Optical Cooling System Test in an Electron Storage Ring
21 pages, pdf. The number of electrons in the bunch in the example is decreased, the volume of the paper is increased, Misprints are corrected
Phys.Rev.STAccel.Beams11:011302,2008
10.1103/PhysRevSTAB.11.011302
null
physics.acc-ph
null
We are proposing to test experimentally the new idea of Enhanced Optical Cooling (EOC) in an electron storage ring. This experiment will confirm new fundamental processes in beam physics and will demonstrate new unique possibilities with this cooling technique. It will open important applications of EOC in nuclear physics, elementary particle physics and in Light Sources (LS) based on high brightness electron and ion beams.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:25:48 GMT" }, { "version": "v2", "created": "Wed, 16 May 2007 09:49:23 GMT" } ]
2008-11-26T00:00:00
[ [ "Bessonov", "E. G.", "", "Lebedev Phys. Inst. RAS, Moscow,\n Russia" ], [ "Gorbunkov", "M. V.", "", "Lebedev Phys. Inst. RAS, Moscow,\n Russia" ], [ "Mikhailichenko", "A. A.", "", "Cornell University, Ithaca, NY, U.S.A." ] ]
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704.0871
Krisztina Eva Gabanyi
K. E. Gabanyi (1,2), N. Marchili (1), T. P. Krichbaum (1), S. Britzen (1), L. Fuhrmann (1), A. Witzel (1), J. A. Zensus (1), P. Muller (1), X. Liu (3), H. G. Song (3), J. L. Han (4), X. H. Sun (4) ((1) Max-Planck-Institut fur Radioastronomie, (2) Hungarian Academy of Sciences, Research Group for Physical Geodesy and Geodynamics, (3) Urumqi Observatory, the National Astronomical Observatories, the Chinese Academy of Sciences, (4) National Astronomical Observatories, Chinese Academy of Sciences)
The IDV source J1128+5925, a new candidate for annual modulation?
15 pages, 9 figures Accepted for publication in Astronomy and Astrophysics
null
10.1051/0004-6361:20067033
null
astro-ph
null
Short time-scale radio variations of compact extragalactic radio sources, known as IntraDay Variability, can be explained in at least some sources by a source-extrinsic effect, in which the variations are interpreted as scintillation of radio waves caused by the turbulent ISM of the Milky Way. One of the most convincing observational arguments in favour of propagation-induced variability is the so called annual modulation of the characteristic variability time-scale, which is due to the orbital motion of the Earth. Data for the recently discovered and highly variable IDV source J1128+5925 are presented. We study the frequency and time dependence of the IDV in this compact quasar. We measure the characteristic variability time-scale of the IDV throughout the year, and analyze whether the observed changes in the variability time-scale are consistent with annual modulation. We monitored the flux density variability of J1128+5925 with dense time sampling between 2.7 and 10.45GHz with the 100m Effelsberg radio telescope of the MPIfR and with the 25m Urumqi radio telescope. From ten observing sessions, we determine the variability characteristics and time-scales. The observed pronounced changes of the variability time-scale of J1128+5925 are modelled with an anisotropic annual modulation model. The observed frequency dependence of the variation is in good agreement with the prediction from interstellar scintillation. Adopting a simple model for the annual modulation model and using also the frequency dependence of the IDV, we derive a lower limit to the distance of the scattering screen and an upper limit to the scintillating source size. The latter is found to be consistent with the measured core size from VLBI.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:54:17 GMT" } ]
2009-11-13T00:00:00
[ [ "Gabanyi", "K. E.", "" ], [ "Marchili", "N.", "" ], [ "Krichbaum", "T. P.", "" ], [ "Britzen", "S.", "" ], [ "Fuhrmann", "L.", "" ], [ "Witzel", "A.", "" ], [ "Zensus", "J. A.", "" ], [ "Muller", "P.", "" ], [ "Liu", "X.", "" ], [ "Song", "H. G.", "" ], [ "Han", "J. L.", "" ], [ "Sun", "X. H.", "" ] ]
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704.0872
Kre\v{s}imir Veseli\'c
K. Veselic
Spectral perturbation bounds for selfadjoint operators
30 pages
null
null
null
math.SP
null
We give general spectral and eigenvalue perturbation bounds for a selfadjoint operator perturbed in the sense of the pseudo-Friedrichs extension. We also give several generalisations of the aforementioned extension. The spectral bounds for finite eigenvalues are obtained by using analyticity and monotonicity properties (rather than variational principles) and they are general enough to include eigenvalues in gaps of the essential spectrum.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 10:47:51 GMT" }, { "version": "v2", "created": "Mon, 21 Jan 2008 17:24:43 GMT" } ]
2008-01-21T00:00:00
[ [ "Veselic", "K.", "" ] ]
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704.0873
Jane Greaves
J.S. Greaves, D.A. Fischer, M.C. Wyatt, C.A. Beichman and G. Bryden
Predicting the frequencies of diverse exo-planetary systems
5 pages, 2 figures; accepted by MNRAS
Mon.Not.Roy.Astron.Soc.Lett.378:L1-L5,2007
10.1111/j.1745-3933.2007.00315.x
null
astro-ph
null
Extrasolar planetary systems range from hot Jupiters out to icy comet belts more distant than Pluto. We explain this diversity in a model where the mass of solids in the primordial circumstellar disk dictates the outcome. The star retains measures of the initial heavy-element (metal) abundance that can be used to map solid masses onto outcomes, and the frequencies of all classes are correctly predicted. The differing dependences on metallicity for forming massive planets and low-mass cometary bodies are also explained. By extrapolation, around two-thirds of stars have enough solids to form Earth-like planets, and a high rate is supported by the first detections of low-mass exo-planets.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:04:07 GMT" } ]
2009-06-23T00:00:00
[ [ "Greaves", "J. S.", "" ], [ "Fischer", "D. A.", "" ], [ "Wyatt", "M. C.", "" ], [ "Beichman", "C. A.", "" ], [ "Bryden", "G.", "" ] ]
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704.0874
Gavril Farkas
Gavril Farkas
Higher ramification and varieties of secant divisors on the generic curve
25 pages. Numerous changes suggested by the referee, several proofs explained in more detail. To appear in the Journal of the London Mathematical Society
J. London Math. Soc. 78(2008) 418-440
null
null
math.AG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
For a smooth projective curve, the cycles of e-secant k-planes are among the most studied objects in classical enumerative geometry and there are well-known formulas due to Castelnuovo, Cayley and MacDonald concerning them. Despite various attempts, surprisingly little is known about the enumerative validity of such formulas. The aim of this paper is to completely clarify this problem in the case of the generic curve C of given genus. Using degeneration techniques and a few facts about the birational geometry of moduli spaces of stable pointed curves we determine precisely under which conditions the cycle of e-secant k-planes in non-empty and we compute its dimension. We also precisely determine the dimension of the variety of linear series on C carrying e-secant k-planes. In a different direction, in the last part of the paper we study the distribution of ramification points of the powers of a line bundle on C having prescribed ramification at a given point.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:07:01 GMT" }, { "version": "v2", "created": "Wed, 30 Apr 2008 17:03:55 GMT" }, { "version": "v3", "created": "Thu, 20 Nov 2014 15:03:16 GMT" } ]
2014-11-21T00:00:00
[ [ "Farkas", "Gavril", "" ] ]
[ 0.0477987044, 0.0236742403, 0.0774383992, 0.0300148837, 0.0280389041, 0.0497996956, -0.0511753783, -0.0089419344, -0.0372934937, 0.0019744167, 0.0806399882, -0.0556776114, -0.1440714449, 0.022661237, 0.0212230235, -0.0048680389, 0.0715854988, -0.0074036713, 0.0879936367, 0.0583289266, 0.069384411, -0.0095922565, 0.0951972082, 0.0368432701, 0.0210229252, -0.0375436172, 0.019184513, 0.0259878878, 0.1464726329, -0.0840416774, 0.0495745838, -0.0377187058, -0.081790559, -0.0874433666, -0.1181585938, 0.0385691263, 0.0205476899, 0.0105489809, -0.0094171697, 0.1147569045, 0.0557276346, 0.102750957, -0.1084537804, 0.0259628743, 0.0686840639, -0.0380188525, 0.0248373169, -0.033366546, 0.0150324544, 0.0207102709, -0.0064031752, 0.0689341873, 0.0311154295, -0.0652323514, -0.0989490673, 0.0537266433, -0.0995993912, 0.0321159251, -0.0105802463, -0.0195972174, 0.0715354756, -0.0604299679, -0.0904448479, -0.003873796, -0.0922457427, 0.0166707672, -0.0654824749, 0.0667330921, 0.0151700228, 0.0550272875, -0.0991991907, 0.0175837204, 0.039619647, 0.0509502664, -0.0212105177, -0.0217357781, 0.0409202911, 0.105152145, 0.0011310297, 0.0238993522, 0.1010501087, 0.0732863396, -0.0379688293, 0.0402949825, 0.0341669433, -0.0713353753, -0.001641439, -0.022773793, -0.062981233, 0.0644319504, -0.0237867963, 0.0478487276, -0.0604299679, 0.0756375119, 0.1041516513, 0.0812402889, -0.0148198493, 0.0109679392, -0.068433933, 0.0288893264, -0.0094046639, 0.030815281, 0.0204601455, -0.0507501662, 0.2141061723, 0.0684839636, -0.0389943384, 0.0608301647, -0.0972482264, -0.0258878376, -0.0475485809, -0.0361179113, -0.0248498227, -0.0099049117, 0.1224607304, 0.0144821815, -0.0602798909, -0.0121435216, -0.0867930427, 0.1024007797, -0.0588791966, -0.0604299679, 0.0051400489, -0.0735364631, 0.0715354756, 0.0334665962, -0.0646820739, -0.0090607433, -0.0600297675, -0.0006937034, 0.0708851516, -0.0509002395, 0.077538453, -0.0499747843, -0.0040551359, 0.0113431253, -0.0082290806, -0.0163330995, 0.0670832694, 0.0161079876, -0.0178088322, 0.0873433128, 0.0591293238, 0.0370933935, 0.116357699, 0.0733863935, -0.096197702, 0.121560283, 0.0126875415, 0.0258878376, -0.0495995954, 0.0119934473, 0.0682838634, -0.0324160755, 0.0063812896, -0.0288142897, -0.0076850611, 0.0564279817, 0.0078726541, 0.0634814799, 0.0437967181, 0.0816905126, -0.0113118598, -0.0168833733, 0.0412704647, 0.0049024313, -0.0900946781, 0.030865306, -0.0462229215, -0.0379688293, -0.0611303151, -0.1265627593, -0.1186588407, -0.0346671902, -0.0047242176, 0.0228988547, -0.0479988009, -0.1698842496, -0.0467731953, -0.0777385533, -0.0498497188, 0.1490739286, -0.1079535335, 0.0353675373, 0.0474485308, 0.0860926956, 0.1420704573, 0.0253000464, 0.0329913609, -0.0657325983, -0.0683338866, 0.0642318502, 0.1354671717, 0.1043517515, 0.0494995452, -0.0676835626, 0.0098924059, 0.0028779898, -0.0171960276, -0.0762878284, -0.0436216332, 0.0049118106, 0.0374185555, -0.0531763695, -0.0090857558, -0.0674834624, 0.0616805889, 0.0626810864, -0.0782388002, 0.0373435169, -0.037168432, -0.02064774, 0.014182033, 0.0550773144, -0.0012154465, 0.0688341334, 0.0391194001, -0.0170959774, 0.077388376, 0.1496742219, 0.0002346867, 0.0204351339, -0.0129939439, 0.0678336397, 0.1223606765, 0.0948970616, 0.050374981, -0.0690342337, -0.0268633217, 0.0153576154, 0.0726360232, 0.0435215831, -0.0783888698, -0.0133941425, 0.0213230737, 0.0253625773, 0.0489992984, -0.0190969706, -0.0354175642, -0.0834413767, 0.001766501, 0.0677335858, -0.0556275845, 0.0471984074, -0.0573784523, 0.0904448479, -0.0729361698, -0.0527761728, -0.0746370107, 0.0721357688, -0.0750372112, 0.0057278406, -0.0258878376, 0.0154576655, -0.0735864937, -0.0085980138 ]
704.0875
Boris Tarasov
Boris V. Tarasov
The concrete theory of numbers: initial numbers and wonderful properties of numbers repunit
8 pages ; v3: minor grammatical changes, etc
null
null
null
math.GM
null
In this work initial numbers and repunit numbers have been studied. All numbers have been considered in a decimal notation. The problem of simplicity of initial numbers has been studied. Interesting properties of numbers repunit are proved: $gcd(R_a, R_b) = R_{gcd(a,b)}$; $R_{ab}/(R_aR_b)$ is an integer only if $gcd(a,b) = 1$, where $a\geq1$, $b\geq1$ are integers. Dividers of numbers repunit, are researched by a degree of prime number.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:08:20 GMT" }, { "version": "v2", "created": "Sat, 7 Apr 2007 10:15:04 GMT" } ]
2007-05-23T00:00:00
[ [ "Tarasov", "Boris V.", "" ] ]
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704.0876
Josef Teichmann
Walter Schachermayer, Uwe Schmock, Josef Teichmann
Non-monotone convergence in the quadratic Wasserstein distance
null
null
null
null
math.PR
null
We give an easy counter-example to Problem 7.20 from C. Villani's book on mass transport: in general, the quadratic Wasserstein distance between $n$-fold normalized convolutions of two given measures fails to decrease monotonically.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:15:47 GMT" } ]
2007-05-23T00:00:00
[ [ "Schachermayer", "Walter", "" ], [ "Schmock", "Uwe", "" ], [ "Teichmann", "Josef", "" ] ]
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704.0877
Filippo Mannucci
F. Mannucci, N. Panagia, M. Della Valle
The bimodality of type Ia Supernovae
5 pages, to appear in the AIP conference proceedings of "Supernova 1987A: 20 Years after Supernovae and Gamma-Ray Bursters", Feb 19-23, 2007, Aspen, CO. Replaced figure 1
AIP Conf.Proc.937:293-297,2007
10.1063/1.2803580
null
astro-ph
null
We comment on the presence of a bimodality in the distribution of delay time between the formation of the progenitors and their explosion as type Ia SNe. Two "flavors" of such bimodality are present in the literature: a "weak" bimodality, in which type Ia SNe must explode from both young and old progenitors, and a "strong" bimodality, in which about half of the systems explode within 10^8 years from formation. The "weak" bimodality is observationally based on the dependence of the rates with the host galaxy SFR, while the "strong" one on the different rates in radio-loud and radio-quiet early-type galaxies. We review the evidence for these bimodalities. Finally, we estimate the fraction of SNe which are missed by optical and near-IR searches because of dust extinction in massive starbursts.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:28:09 GMT" }, { "version": "v2", "created": "Wed, 4 Jul 2007 13:11:02 GMT" } ]
2009-09-29T00:00:00
[ [ "Mannucci", "F.", "" ], [ "Panagia", "N.", "" ], [ "Della Valle", "M.", "" ] ]
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704.0878
Amelie Juhin
Am\'elie Juhin (IMPMC), Georges Calas (IMPMC), Delphine Cabaret (IMPMC), Laurence Galoisy (IMPMC), Jean-Louis Hazemann
Structural relaxation around substitutional Cr3+ in MgAl2O4
7 pages, 4 figures
null
10.1103/PhysRevB.76.054105
null
cond-mat.mtrl-sci
null
The structural environment of substitutional Cr3+ ion in MgAl2O4 spinel has been investigated by Cr K-edge Extended X-ray Absorption Fine Structure (EXAFS) and X-ray Absorption Near Edge Structure (XANES) spectroscopies. First-principles computations of the structural relaxation and of the XANES spectrum have been performed, with a good agreement to the experiment. The Cr-O distance is close to that in MgCr2O4, indicating a full relaxation of the first neighbors, and the second shell of Al atoms relaxes partially. These observations demonstrate that Vegard's law is not obeyed in the MgAl2O4-MgCr2O4 solid solution. Despite some angular site distortion, the local D3d symmetry of the B-site of the spinel structure is retained during the substitution of Cr for Al. Here, we show that the relaxation is accomodated by strain-induced bond buckling, with angular tilts of the Mg-centred tetrahedra around the Cr-centred octahedron. By contrast, there is no significant alteration of the angles between the edge-sharing octahedra, which build chains aligned along the three four-fold axes of the cubic structure.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:46:08 GMT" } ]
2016-08-14T00:00:00
[ [ "Juhin", "Amélie", "", "IMPMC" ], [ "Calas", "Georges", "", "IMPMC" ], [ "Cabaret", "Delphine", "", "IMPMC" ], [ "Galoisy", "Laurence", "", "IMPMC" ], [ "Hazemann", "Jean-Louis", "" ] ]
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704.0879
Mohamed Kaaniche
Mohamed Kaaniche (LAAS), Luigi Romano (UIUC), Zbigniew Kalbarczyk (UIUC), Ravishankar Iyer (UIUC), Rick Karcich (STORAGETEK)
A Hierarchical Approach for Dependability Analysis of a Commercial Cache-Based RAID Storage Architecture
null
Proc. 28th IEEE International Symposium on Fault-Tolerant Computing (FTCS-28), Munich (Germany), IEEE Computer Society, June 1998, pp.6-15 (1998) 6-15
null
null
cs.PF
null
We present a hierarchical simulation approach for the dependability analysis and evaluation of a highly available commercial cache-based RAID storage system. The archi-tecture is complex and includes several layers of overlap-ping error detection and recovery mechanisms. Three ab-straction levels have been developed to model the cache architecture, cache operations, and error detection and recovery mechanism. The impact of faults and errors oc-curring in the cache and in the disks is analyzed at each level of the hierarchy. A simulation submodel is associated with each abstraction level. The models have been devel-oped using DEPEND, a simulation-based environment for system-level dependability analysis, which provides facili-ties to inject faults into a functional behavior model, to simulate error detection and recovery mechanisms, and to evaluate quantitative measures. Several fault models are defined for each submodel to simulate cache component failures, disk failures, transmission errors, and data errors in the cache memory and in the disks. Some of the parame-ters characterizing fault injection in a given submodel cor-respond to probabilities evaluated from the simulation of the lower-level submodel. Based on the proposed method-ology, we evaluate and analyze 1) the system behavior un-der a real workload and high error rate (focusing on error bursts), 2) the coverage of the error detection mechanisms implemented in the system and the error latency distribu-tions, and 3) the accumulation of errors in the cache and in the disks.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:46:49 GMT" } ]
2007-05-23T00:00:00
[ [ "Kaaniche", "Mohamed", "", "LAAS" ], [ "Romano", "Luigi", "", "UIUC" ], [ "Kalbarczyk", "Zbigniew", "", "UIUC" ], [ "Iyer", "Ravishankar", "", "UIUC" ], [ "Karcich", "Rick", "", "STORAGETEK" ] ]
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704.088
Qiuping A. Wang
Q. A. Wang (ISMANS), F. Tsobnang (ISMANS), S. Bangoup (ISMANS), F. Dzangue (ISMANS), A. Jeatsa (ISMANS), A. Le M\'ehaut\'e (ISMANS)
Stochastic action principle and maximum entropy
This work is a further development of the idea proposed in the paper cond-mat/0407515, 15 pages
Chaos, Solitons and Fractals, 40(2009)2550-2556
10.1016/j.chaos.2007.10.047
null
cond-mat.stat-mech
null
A stochastic action principle for stochastic dynamics is revisited. We present first numerical diffusion experiments showing that the diffusion path probability depend exponentially on average Lagrangian action. This result is then used to derive an uncertainty measure defined in a way mimicking the heat or entropy in the first law of thermodynamics. It is shown that the path uncertainty (or path entropy) can be measured by the Shannon information and that the maximum entropy principle and the least action principle of classical mechanics can be unified into a concise form. It is argued that this action principle, hence the maximum entropy principle, is simply a consequence of the mechanical equilibrium condition extended to the case of stochastic dynamics.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:53:21 GMT" } ]
2020-11-25T00:00:00
[ [ "Wang", "Q. A.", "", "ISMANS" ], [ "Tsobnang", "F.", "", "ISMANS" ], [ "Bangoup", "S.", "", "ISMANS" ], [ "Dzangue", "F.", "", "ISMANS" ], [ "Jeatsa", "A.", "", "ISMANS" ], [ "Méhauté", "A. Le", "", "ISMANS" ] ]
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704.0881
Jounghun Lee
Jounghun Lee, Daeseong Park (Seoul Nat'l Univ.)
Constraining the Dark Energy Equation of State with Cosmic Voids
ApJL in press, growth factor corrected, parameter degeneracy calculated
Astrophys.J.696:L10-L12,2009
10.1088/0004-637X/696/1/L10
null
astro-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Our universe is observed to be accelerating due to the dominant dark energy with negative pressure. The dark energy equation of state (w) holds a key to understanding the ultimate fate of the universe. The cosmic voids behave like bubbles in the universe so that their shapes must be quite sensitive to the background cosmology. Assuming a flat universe and using the priors on the matter density parameter (Omega_m) and the dimensionless Hubble parameter (h), we demonstrate analytically that the ellipticity evolution of cosmic voids may be a sensitive probe of the dark energy equation of state. We also discuss the parameter degeneracy between w and Omega_m.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 11:53:57 GMT" }, { "version": "v2", "created": "Fri, 13 Mar 2009 17:47:40 GMT" } ]
2011-02-11T00:00:00
[ [ "Lee", "Jounghun", "", "Seoul Nat'l Univ." ], [ "Park", "Daeseong", "", "Seoul Nat'l Univ." ] ]
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704.0882
Matts Roos
Matts Roos
A Dark Energy model combining DGP gravity and Chaplygin gas
3 pages, 1 figure
null
null
null
astro-ph
null
The expansion of the Universe is accelerating, as testified by observations of supernovae of type Ia as a function of redshift. Explanations are of two types: modifications of Einstein gravity or new forms of energy, coined dark energy.The accelerated expansion is explained here by a combination of Dvali-Gabadadze-Porrati (DGP) model gravity and Chaplygin gas dark energy. Both models are characterized by a length scale L which may be the same. The continuity equation for the combined model is derived in flat geometry, and solved by numerical methods. The solution is shown to have the expected properties: at very small scales (a<<L) the energy density behaves as pressureless dust, at very large scales (a>>L) as a cosmological constant. The modifications to the DGP model and the Chaplygin gas model occur for values of a L. The results show an increase in the present dark energy density relative to the plain DGP model.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 12:00:14 GMT" } ]
2007-05-23T00:00:00
[ [ "Roos", "Matts", "" ] ]
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704.0883
Yutaka Hosotani
Yutaka Hosotani
Gauge-Higgs Unification and LHC/ILC
16 pages. Proceeding for SCGT2006 (Nagoya, Nov. 2006)
null
10.1142/9789812790750_0038
OU-HET 579/2007
hep-ph
null
In the gauge-Higgs unification scenario the 4D Higgs field is identified with the zero mode of the extra-dimensional component of gauge potentials. The mass of the Higgs particle in the unification in the Randall-Sundrum warped spacetime is predicted to be in the range 100 GeV - 300 GeV. The WWZ gauge couplings remains almost universal as in the standard model, but substantial deviation results for the Higgs couplings. The WWH and ZZH couplings are suppressed by a factor \cos \theta_H from the values in the standard model, where \theta_H is the Yang-Mills AB phase along the fifth dimension. These can be tested at LHC and ILC.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 12:50:53 GMT" } ]
2017-08-23T00:00:00
[ [ "Hosotani", "Yutaka", "" ] ]
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704.0884
Viet-Anh Nguyen
Peter Pflug and Viet-Anh Nguyen
Extension theorems of Sakai type for separately holomorphic and meromorphic functions
null
Ann. Polon. Math. 82 (2003), no. 2, 171--187
null
null
math.CV
null
We first exhibit counterexamples to some open questions related to a theorem of Sakai. Then we establish an extension theorem of Sakai type for separately holomorphic/meromorphic functions.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:02:19 GMT" } ]
2007-05-23T00:00:00
[ [ "Pflug", "Peter", "" ], [ "Nguyen", "Viet-Anh", "" ] ]
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704.0885
Jan Pachl
Jan Pachl
Uniform measures and countably additive measures
LaTeX; 7 pages
null
null
null
math.FA math.GN
null
Uniform measures are defined as the functionals on the space of bounded uniformly continuous functions that are continuous on bounded uniformly equicontinuous sets. If every cardinal has measure zero then every countably additive measure is a uniform measure. The functionals sequentially continuous on bounded uniformly equicontinuous sets are exactly uniform measures on the separable modification of the underlying uniform space.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:10:30 GMT" } ]
2007-05-23T00:00:00
[ [ "Pachl", "Jan", "" ] ]
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704.0886
Peter Jung
Peter Jung and Achim Rosch
Lower bounds for the conductivities of correlated quantum systems
Title changed; 9 pages, 2 figures
Phys. Rev. B 75, 245104 (2007)
10.1103/PhysRevB.75.245104
null
cond-mat.str-el
null
We show how one can obtain a lower bound for the electrical, spin or heat conductivity of correlated quantum systems described by Hamiltonians of the form H = H0 + g H1. Here H0 is an interacting Hamiltonian characterized by conservation laws which lead to an infinite conductivity for g=0. The small perturbation g H1, however, renders the conductivity finite at finite temperatures. For example, H0 could be a continuum field theory, where momentum is conserved, or an integrable one-dimensional model while H1 might describe the effects of weak disorder. In the limit g to 0, we derive lower bounds for the relevant conductivities and show how they can be improved systematically using the memory matrix formalism. Furthermore, we discuss various applications and investigate under what conditions our lower bound may become exact.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:32:51 GMT" }, { "version": "v2", "created": "Wed, 20 Jun 2007 16:04:41 GMT" } ]
2007-06-20T00:00:00
[ [ "Jung", "Peter", "" ], [ "Rosch", "Achim", "" ] ]
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704.0887
Oleg Usatenko
S. S. Apostolov, Z. A. Mayzelis, O. V. Usatenko, V. A. Yampol'skii
Non-extensive thermodynamics of 1D systems with long-range interaction
5 pages, 2 figures
null
null
null
physics.data-an physics.gen-ph
null
A new approach to non-extensive thermodynamical systems with non-additive energy and entropy is proposed. The main idea of the paper is based on the statistical matching of the thermodynamical systems with the additive multi-step Markov chains. This general approach is applied to the Ising spin chain with long-range interaction between its elements. The asymptotical expressions for the energy and entropy of the system are derived for the limiting case of weak interaction. These thermodynamical quantities are found to be non-proportional to the length of the system (number of its particle).
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:37:45 GMT" } ]
2007-05-23T00:00:00
[ [ "Apostolov", "S. S.", "" ], [ "Mayzelis", "Z. A.", "" ], [ "Usatenko", "O. V.", "" ], [ "Yampol'skii", "V. A.", "" ] ]
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704.0888
Claude Berthier
S. Kramer (LCMI), R. Stern, M. Horvatic (LCMI), C. Berthier (LCMI), T. Kimura (LANL), I.R. Fisher
NMR evidence for a strong modulation of the Bose-Einstein Condensate in BaCuSi$_2$O$_6$
null
Physical Review B 76, 10 (2007) 100406(R)
10.1103/PhysRevB.76.100406
null
cond-mat.str-el
null
We present a $^{63,65}$Cu and $^{29}$Si NMR study of the quasi-2D coupled spin 1/2 dimer compound BaCuSi$_2$O$_6$ in the magnetic field range 13-26 T and at temperatures as low as 50 mK. NMR data in the gapped phase reveal that below 90 K different intra-dimer exchange couplings and different gaps ($\Delta_{\rm{B}}/\Delta_{\rm{A}}$ = 1.16) exist in every second plane along the c-axis, in addition to a planar incommensurate (IC) modulation. $^{29}$Si spectra in the field induced magnetic ordered phase reveal that close to the quantum critical point at $H_{\rm{c1}}$ = 23.35 T the average boson density $\bar{n}$ of the Bose-Einstein condensate is strongly modulated along the c-axis with a density ratio for every second plane $\bar{n}_{\rm{A}}/\bar{n}_{\rm{B}} \simeq 5$. An IC modulation of the local density is also present in each plane. This adds new constraints for the understanding of the 2D value $\phi$ = 1 of the critical exponent describing the phase boundary.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 13:49:04 GMT" } ]
2008-02-11T00:00:00
[ [ "Kramer", "S.", "", "LCMI" ], [ "Stern", "R.", "", "LCMI" ], [ "Horvatic", "M.", "", "LCMI" ], [ "Berthier", "C.", "", "LCMI" ], [ "Kimura", "T.", "", "LANL" ], [ "Fisher", "I. R.", "" ] ]
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704.0889
Anthony van Raan
Anthony F. J. van Raan
Bibliometric statistical properties of the 100 largest European universities: prevalent scaling rules in the science system
26 pages, 33 figures, 3 tables. submitted to the Journal of the American Society for information Science and Technology
null
null
null
physics.data-an physics.soc-ph
null
For the 100 largest European universities we studied the statistical properties of bibliometric indicators related to research performance, field citation density and journal impact. We find a size-dependent cumulative advantage for the impact of universities in terms of total number of citations. In previous work a similar scaling rule was found at the level of research groups. Therefore we conjecture that this scaling rule is a prevalent property of the science system. We observe that lower performance universities have a larger size-dependent cumulative advantage for receiving citations than top-performance universities. We also find that for the lower-performance universities the fraction of not-cited publications decreases considerably with size. Generally, the higher the average journal impact of the publications of a university, the lower the number of not-cited publications. We find that the average research performance does not dilute with size. Large top-performance universities succeed in keeping a high performance over a broad range of activities. This most probably is an indication of their scientific attractive power. Next we find that particularly for the lower-performance universities the field citation density provides a strong cumulative advantage in citations per publication. The relation between number of citations and field citation density found in this study can be considered as a second basic scaling rule of the science system. Top-performance universities publish in journals with significantly higher journal impact as compared to the lower performance universities. We find a significant decrease of the fraction of self-citations with increasing research performance, average field citation density, and average journal impact.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 14:13:34 GMT" } ]
2007-05-23T00:00:00
[ [ "van Raan", "Anthony F. J.", "" ] ]
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704.089
Salvatore Orlando
S. Orlando, F. Bocchino, F. Reale, G. Peres, O. Petruk
On the Origin of Asymmetries in Bilateral Supernova Remnants
14 pages, 8 Figures; paper accepted for publication in A&A; the paper with high-resolution figures can be downloaded at http://www.astropa.unipa.it/~orlando/PAPERS/sorlando_6045.pdf
null
10.1051/0004-6361:20066045
null
astro-ph
null
AIMS: We investigate whether the morphology of bilateral supernova remnants (BSNRs) observed in the radio band is determined mainly either by a non-uniform interstellar medium (ISM) or by a non-uniform ambient magnetic field. METHODS: We perform 3-D MHD simulations of a spherical SNR shock propagating through a magnetized ISM. Two cases of shock propagation are considered: 1) through a gradient of ambient density with a uniform ambient magnetic field; 2) through a homogeneous medium with a gradient of ambient magnetic field strength. From the simulations, we synthesize the synchrotron radio emission, making different assumptions about the details of acceleration and injection of relativistic electrons. RESULTS: We find that asymmetric BSNRs are produced if the line-of-sight is not aligned with the gradient of ambient plasma density or with the gradient of ambient magnetic field strength. We derive useful parameters to quantify the degree of asymmetry of the remnants that may provide a powerful diagnostic of the microphysics of strong shock waves through the comparison between models and observations. CONCLUSIONS: BSNRs with two radio limbs of different brightness can be explained if a gradient of ambient density or, most likely, of ambient magnetic field strength is perpendicular to the radio limbs. BSNRs with converging similar radio arcs can be explained if the gradient runs between the two arcs.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 14:13:38 GMT" } ]
2009-11-13T00:00:00
[ [ "Orlando", "S.", "" ], [ "Bocchino", "F.", "" ], [ "Reale", "F.", "" ], [ "Peres", "G.", "" ], [ "Petruk", "O.", "" ] ]
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704.0891
Michel Cribier
M. Cribier (APC)
Reactor Monitoring with Neutrinos
5 pages - XXII International Conference On Neutrino Physics And Astrophysics (Neutrino 2006)
XXII International Conference On Neutrino Physics And Astrophysics (Neutrino 2006), Santa Fe, New Mexico : \'Etats-Unis (2006)
10.1016/j.nuclphysbps.2011.03.094
APC-123/conf
nucl-ex
null
The fundamental knowledge on neutrinos acquired in the recent years open the possibility of applied neutrino physics. Among it the automatic and non intrusive monitoring of nuclear reactor by its antineutrino signal could be very valuable to IAEA in charge of the control of nuclear power plants. Several efforts worldwide have already started.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 14:17:14 GMT" } ]
2012-10-09T00:00:00
[ [ "Cribier", "M.", "", "APC" ] ]
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704.0892
Xingang Wang Dr
Xingang Wang, Meng Zhan, Ghuguang Guan, and Choy Heng Lai
Nonstationary pattern in unsynchronizable complex networks
11 pages, 9 figures, preprints. Comments and suggestions are welcome
null
null
null
nlin.CD
null
Pattern formation and evolution in unsynchronizable complex networks are investigated. Due to the asymmetric topology, the synchronous patterns formed in complex networks are irregular and nonstationary. For coupling strength immediately out of the synchronizable region, the typical phenomenon is the on-off intermittency of the system dynamics. The patterns appeared in this process are signatured by the coexistence of a giant cluster, which comprises most of the nodes, and a few number of small clusters. The pattern evolution is characterized by the giant cluster irregularly absorbs or emits the small clusters. As the coupling strength leaves away from the synchronization bifurcation point, the giant cluster is gradually dissolved into a number of small clusters, and the system dynamics is characterized by the integration and separation of the small clusters. Dynamical mechanisms and statistical properties of the nonstationary pattern evolution are analyzed and conducted, and some scalings are newly revealed. Remarkably, it is found that the few active nodes, which escape from the giant cluster with a high frequency, are independent of the coupling strength while are sensitive to the bifurcation types. We hope our findings about nonstationary pattern could give additional understandings to the dynamics of complex systems and have implications to some real problems where systems maintain their normal functions only in the unsynchronizable state.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 14:19:59 GMT" } ]
2007-05-23T00:00:00
[ [ "Wang", "Xingang", "" ], [ "Zhan", "Meng", "" ], [ "Guan", "Ghuguang", "" ], [ "Lai", "Choy Heng", "" ] ]
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704.0893
Antonio Khoury
C.E.R. Souza, J.A.O. Huguenin, P. Milman, and A.Z. Khoury
Topological phase for spin-orbit transformations on a laser beam
4 pages, 4 figures
Phys. Rev. Lett. 99, 160401 (2007)
10.1103/PhysRevLett.99.160401
null
quant-ph
null
We investigate the topological phase associated with the double connectedness of the SO(3) representation in terms of maximally entangled states. An experimental demonstration is provided in the context of polarization and spatial mode transformations of a laser beam carrying orbital angular momentum. The topological phase is evidenced through interferometric measurements and a quantitative relationship between the concurrence and the fringes visibility is derived. Both the quantum and the classical regimes were investigated.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 14:27:51 GMT" } ]
2011-07-08T00:00:00
[ [ "Souza", "C. E. R.", "" ], [ "Huguenin", "J. A. O.", "" ], [ "Milman", "P.", "" ], [ "Khoury", "A. Z.", "" ] ]
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704.0894
John Subasavage Jr.
John P. Subasavage (1), Todd J. Henry (1), P. Bergeron (2), P. Dufour (2), Nigel C. Hambly (3), Thomas D. Beaulieu (1) ((1) Georgia State University, (2) University of Montreal, (3) University of Edinburgh Royal Observatory)
The Solar Neighborhood. XIX. Discovery and Characterization of 33 New Nearby White Dwarf Systems
33 pages, 10 figures, accepted for publication in the Astronomical Journal
Astron.J.134:252-261,2007
10.1086/518739
null
astro-ph
null
We present spectra for 33 previously unclassified white dwarf systems brighter than V = 17 primarily in the southern hemisphere. Of these new systems, 26 are DA, 4 are DC, 2 are DZ, and 1 is DQ. We suspect three of these systems are unresolved double degenerates. We obtained VRI photometry for these 33 objects as well as for 23 known white dwarf systems without trigonometric parallaxes, also primarily in the southern hemisphere. For the 56 objects, we converted the photometry values to fluxes and fit them to a spectral energy distribution using the spectroscopy to determine which model to use (i.e. pure hydrogen, pure helium, or metal-rich helium), resulting in estimates of effective temperature and distance. Eight of the new and 12 known systems are estimated to be within the NStars and Catalogue of Nearby Stars (CNS) horizons of 25 pc, constituting a potential 18% increase in the nearby white dwarf sample. Trigonometric parallax determinations are underway via CTIOPI for these 20 systems. One of the DCs is cool so that it displays absorption in the near infrared. Using the distance determined via trigonometric parallax, we are able to constrain the model-dependent physical parameters and find that this object is most likely a mixed H/He atmosphere white dwarf similar to other cool white dwarfs identified in recent years with significant absorption in the infrared due to collision-induced absorptions by molecular hydrogen.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 15:08:34 GMT" } ]
2009-09-29T00:00:00
[ [ "Subasavage", "John P.", "" ], [ "Henry", "Todd J.", "" ], [ "Bergeron", "P.", "" ], [ "Dufour", "P.", "" ], [ "Hambly", "Nigel C.", "" ], [ "Beaulieu", "Thomas D.", "" ] ]
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704.0895
Perrin Nicolas
Nicolas Perrin
Gorenstein locus of minuscule Schubert varieties
12 pages
null
null
null
math.AG math.CO
null
In this article, we describe explicitely the Gorenstein locus of all minuscule Schubert varieties. This proves a special case of a conjecture of A. Woo and A. Yong (see math.AG/0603273) on the Gorenstein locus of Schubert varieties.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 15:00:40 GMT" } ]
2007-05-23T00:00:00
[ [ "Perrin", "Nicolas", "" ] ]
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704.0896
Yurij Holovatch
M. Dudka, R. Folk, Yu. Holovatch, G. Moser
Model C critical dynamics of random anisotropy magnets
8 figures, style files included
J. Phys. A: Math. Gen., vol. 40 (2007) 8247-8264
10.1088/1751-8113/40/29/004
null
cond-mat.dis-nn cond-mat.stat-mech
null
We study the relaxational critical dynamics of the three-dimensional random anisotropy magnets with the non-conserved n-component order parameter coupled to a conserved scalar density. In the random anisotropy magnets the structural disorder is present in a form of local quenched anisotropy axes of random orientation. When the anisotropy axes are randomly distributed along the edges of the n-dimensional hypercube, asymptotical dynamical critical properties coincide with those of the random-site Ising model. However structural disorder gives rise to considerable effects for non-asymptotic critical dynamics. We investigate this phenomenon by a field-theoretical renormalization group analysis in the two-loop order. We study critical slowing down and obtain quantitative estimates for the effective and asymptotic critical exponents of the order parameter and scalar density. The results predict complex scenarios for the effective critical exponent approaching an asymptotic regime.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 15:08:06 GMT" } ]
2009-11-13T00:00:00
[ [ "Dudka", "M.", "" ], [ "Folk", "R.", "" ], [ "Holovatch", "Yu.", "" ], [ "Moser", "G.", "" ] ]
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704.0897
Viet-Anh Nguyen
Viet-Anh Nguyen
A unified approach to the theory of separately holomorphic mappings
54 pages, preprint of the ICTP, Trieste, Italy (2007). I have added some minor explanations, corrections and changes
null
null
null
math.CV
null
We extend the theory of separately holomorphic mappings between complex analytic spaces. Our method is based on Poletsky theory of discs, Rosay Theorem on holomorphic discs and our recent joint-work with Pflug on cross theorems in dimension 1. It also relies on our new technique of conformal mappings and a generalization of Siciak's relative extremal function. Our approach illustrates the unified character: ``From local informations to global extensions". Moreover, it avoids systematically the use of the classical method of doubly orthogonal bases of Bergman type.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 15:31:38 GMT" }, { "version": "v2", "created": "Sun, 4 Nov 2007 22:48:08 GMT" } ]
2007-11-05T00:00:00
[ [ "Nguyen", "Viet-Anh", "" ] ]
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704.0898
Xavier Bekaert
Xavier Bekaert
Higher spin algebras as higher symmetries
14 pages, expanded version of the lectures presented at the ``5th international school and workshop on QFT & Hamiltonian systems'' (Calimanesti, May 2006); v2: minor corrections performed, comments added and refs updated
null
null
null
hep-th
null
The exhaustive study of the rigid symmetries of arbitrary free field theories is motivated, along several lines, as a preliminary step in the completion of the higher-spin interaction problem in full generality. Some results for the simplest example (a scalar field) are reviewed and commented along these lines.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 15:59:02 GMT" }, { "version": "v2", "created": "Thu, 23 Aug 2007 09:56:23 GMT" } ]
2007-08-23T00:00:00
[ [ "Bekaert", "Xavier", "" ] ]
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704.0899
Van Dixon
W. V. Dixon (1), D. J. Sahnow (1), P. E. Barrett (2 and 3), T. Civeit (1 and 4), J. Dupuis (1 and 5), A. W. Fullerton (1 and 6), B. Godard (1 and 7), J. C. Hsu (2 and 8), M. E. Kaiser (1), J. W. Kruk (1), S. Lacour (1 and 9), D. J. Lindler (10), D. Massa (11), R. D. Robinson (1 and 8), M. L. Romelfanger (1), P. Sonnentrucker (1) ((1) Johns Hopkins University, (2) Space Telescope Science Institute, (3) U.S. Naval Observatory, (4) Centre National d'Etudes Spatiales, (5) Canadian Space Agency, (6) University of Victoria, (7) Institut d'Astrophysique de Paris, (8) Retired, (9) Sydney University, (10) Sigma Space Corporation, (11) SGT, Inc.)
CalFUSE v3: A Data-Reduction Pipeline for the Far Ultraviolet Spectroscopic Explorer
To appear in PASP; 29 pages, 13 figures, uses aastex, emulateapj
null
10.1086/518617
null
astro-ph
null
Since its launch in 1999, the Far Ultraviolet Spectroscopic Explorer (FUSE) has made over 4600 observations of some 2500 individual targets. The data are reduced by the Principal Investigator team at the Johns Hopkins University and archived at the Multimission Archive at Space Telescope (MAST). The data-reduction software package, called CalFUSE, has evolved considerably over the lifetime of the mission. The entire FUSE data set has recently been reprocessed with CalFUSE v3.2, the latest version of this software. This paper describes CalFUSE v3.2, the instrument calibrations upon which it is based, and the format of the resulting calibrated data files.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 15:37:01 GMT" } ]
2009-11-13T00:00:00
[ [ "Dixon", "W. V.", "", "2 and 3" ], [ "Sahnow", "D. J.", "", "2 and 3" ], [ "Barrett", "P. E.", "", "2 and 3" ], [ "Civeit", "T.", "", "1 and 4" ], [ "Dupuis", "J.", "", "1 and 5" ], [ "Fullerton", "A. W.", "", "1 and 6" ], [ "Godard", "B.", "", "1 and\n 7" ], [ "Hsu", "J. C.", "", "2 and 8" ], [ "Kaiser", "M. E.", "", "1 and\n 9" ], [ "Kruk", "J. W.", "", "1 and\n 9" ], [ "Lacour", "S.", "", "1 and\n 9" ], [ "Lindler", "D. J.", "", "1 and 8" ], [ "Massa", "D.", "", "1 and 8" ], [ "Robinson", "R. D.", "", "1 and 8" ], [ "Romelfanger", "M. L.", "" ], [ "Sonnentrucker", "P.", "" ] ]
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704.09
Benoit Doucot
Benoit Doucot and Lev B. Ioffe
Voltage-Current curves for small Josephson junction arrays
12 pages, 4 figures
null
10.1103/PhysRevB.76.214507
null
cond-mat.supr-con cond-mat.mes-hall
null
We compute the current voltage characteristic of a chain of identical Josephson circuits characterized by a large ratio of Josephson to charging energy that are envisioned as the implementation of topologically protected qubits. We show that in the limit of small coupling to the environment it exhibits a non-monotonous behavior with a maximum voltage followed by a parametrically large region where $V\propto 1/I$. We argue that its experimental measurement provides a direct probe of the amplitude of the quantum transitions in constituting Josephson circuits and thus allows their full characterization.
[ { "version": "v1", "created": "Fri, 6 Apr 2007 17:10:23 GMT" } ]
2009-11-13T00:00:00
[ [ "Doucot", "Benoit", "" ], [ "Ioffe", "Lev B.", "" ] ]
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