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801.4773
Lenny Fukshansky
Lenny Fukshansky
Effective structure theorems for symplectic spaces via height
null
in "Quadratic forms -- algebra, arithmetic, and geometry" (R. Baeza, W.K. Chan, D.W. Hoffmann, and R. Schulze-Pillot, eds.), Contemporary Mathematics 493 (2009), pg. 117--130
null
null
math.NT
null
Given a $2k$-dimensional symplectic space $(Z,F)$ in $N$ variables, $1 < 2k \leq N$, over a global field $K$, we prove the existence of a symplectic basis for $(Z,F)$ of bounded height. This can be viewed as a version of Siegel's lemma for a symplectic space. As corollaries of our main result, we prove the existence of a small-height decomposition of $(Z,F)$ into hyperbolic planes, as well as the existence of two generating flags of totally isotropic subspaces. These present analogues of known results for quadratic spaces. A distinctive feature of our argument is that it works simultaneously for essentially any field with a product formula, algebraically closed or not. In fact, we prove an even more general version of these statements, where canonical height is replaced with twisted height. All bounds on height are explicit.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 21:32:13 GMT" } ]
2009-08-25T00:00:00
[ [ "Fukshansky", "Lenny", "" ] ]
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801.4774
Grenville Croll
Thomas A. Grossman
Source Code Protection for Applications Written in Microsoft Excel and Google Spreadsheet
11 pages
Proc. European Spreadsheet Risks Int. Grp. 2007 81-91 ISBN 978-905617-58-6
null
null
cs.SE
null
Spreadsheets are used to develop application software that is distributed to users. Unfortunately, the users often have the ability to change the programming statements ("source code") of the spreadsheet application. This causes a host of problems. By critically examining the suitability of spreadsheet computer programming languages for application development, six "application development features" are identified, with source code protection being the most important. We investigate the status of these features and discuss how they might be implemented in the dominant Microsoft Excel spreadsheet and in the new Google Spreadsheet. Although Google Spreadsheet currently provides no source code control, its web-centric delivery model offers technical advantages for future provision of a rich set of features. Excel has a number of tools that can be combined to provide "pretty good protection" of source code, but weak passwords reduce its robustness. User access to Excel source code must be considered a programmer choice rather than an attribute of the spreadsheet.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 21:35:17 GMT" } ]
2008-03-10T00:00:00
[ [ "Grossman", "Thomas A.", "" ] ]
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801.4775
Grenville Croll
Harmen Ettema, Paul Janssen, Jacques de Swart
Spreadsheet Assurance by "Control Around" is a Viable Alternative to the Traditional Approach
9 pages, one colour diagram and a client case study
Proc. European Spreadsheet Risks Int. Grp. 2001 107-116 ISBN:1 86166 179 7
null
null
cs.SE
null
The traditional approach to spreadsheet auditing generally consists of auditing every distinct formula within a spreadsheet. Although tools are developed to support auditors during this process, the approach is still very time consuming and therefore relatively expensive. As an alternative to the traditional "control through" approach, this paper discusses a "control around" approach. Within the proposed approach not all distinct formulas are audited separately, but the relationship between input data and output data of a spreadsheet is audited through comparison with a shadow model developed in a modelling language. Differences between the two models then imply possible errors in the spreadsheet. This paper describes relevant issues regarding the "control around" approach and the circumstances in which this approach is preferred above a traditional spreadsheet audit approach.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 21:53:43 GMT" } ]
2008-03-10T00:00:00
[ [ "Ettema", "Harmen", "" ], [ "Janssen", "Paul", "" ], [ "de Swart", "Jacques", "" ] ]
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801.4776
N. A. Levenson
M. M. Sirocky, N. A. Levenson, M. Elitzur, H. W. W. Spoon, and L. Armus
Silicates in Ultra-Luminous Infrared Galaxies
38 pages, 11 figures; to appear in ApJ v679 (May 20)
null
10.1086/586727
null
astro-ph
null
We analyze the mid-infrared (MIR) spectra of ultraluminous infrared galaxies (ULIRGs) observed with the Spitzer Space Telescope's Infrared Spectrograph. Dust emission dominates the MIR spectra of ULIRGs, and the reprocessed radiation that emerges is independent of the underlying heating spectrum. Instead, the resulting emission depends sensitively on the geometric distribution of the dust, which we diagnose with comparisons of numerical simulations of radiative transfer. Quantifying the silicate emission and absorption features that appear near 10 and 18um requires a reliable determination of the continuum, and we demonstrate that including a measurement of the continuum at intermediate wavelength (between the features) produces accurate results at all optical depths. With high-quality spectra, we successfully use the silicate features to constrain the dust chemistry. The observations of the ULIRGs and local sightlines require dust that has a relatively high 18/10um absorption ratio of the silicate features (around 0.5). Specifically, the cold dust of Ossenkopf et al. (1992) is consistent with the observations, while other dust models are not. We use the silicate feature strengths to identify two families of ULIRGs, in which the dust distributions are fundamentally different. Optical spectral classifications are related to these families. In ULIRGs that harbor an active galactic nucleus, the spectrally broad lines are detected only when the nuclear surroundings are clumpy. In contrast, the sources of lower ionization optical spectra are deeply embedded in smooth distributions of optically thick dust.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 21:53:46 GMT" } ]
2009-11-13T00:00:00
[ [ "Sirocky", "M. M.", "" ], [ "Levenson", "N. A.", "" ], [ "Elitzur", "M.", "" ], [ "Spoon", "H. W. W.", "" ], [ "Armus", "L.", "" ] ]
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801.4777
Anil Ada
Anil Ada
Non-Deterministic Communication Complexity of Regular Languages
Master's thesis, 93 pages
null
null
null
cs.CC
null
In this thesis, we study the place of regular languages within the communication complexity setting. In particular, we are interested in the non-deterministic communication complexity of regular languages. We show that a regular language has either O(1) or Omega(log n) non-deterministic complexity. We obtain several linear lower bound results which cover a wide range of regular languages having linear non-deterministic complexity. These lower bound results also imply a result in semigroup theory: we obtain sufficient conditions for not being in the positive variety Pol(Com). To obtain our results, we use algebraic techniques. In the study of regular languages, the algebraic point of view pioneered by Eilenberg (\cite{Eil74}) has led to many interesting results. Viewing a semigroup as a computational device that recognizes languages has proven to be prolific from both semigroup theory and formal languages perspectives. In this thesis, we provide further instances of such mutualism.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 21:55:13 GMT" } ]
2008-02-01T00:00:00
[ [ "Ada", "Anil", "" ] ]
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801.4778
Mladen Georgiev
Mladen Georgiev
Off-center impurities in alkali halides: reorientation, electric polarization and binding to F center. V. Temperature-dependent electrostatic polarizabilities
6 pages including 1 figure, all pdf format
null
null
null
cond-mat.mtrl-sci cond-mat.other
null
We derive and discuss expressions for the temperature-dependent electrostatic polarizabilities of off-center ions holding good under various experimental conditions. At low temperatures and electric-field strengths, all of them reasonably reduce to values characteristic of phonon-coupled two-level systems. Prospects for further studies of the dispersive coupling are also considered.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 21:58:43 GMT" } ]
2008-02-01T00:00:00
[ [ "Georgiev", "Mladen", "" ] ]
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801.4779
David Henley
D.B. Henley, M.F. Corcoran, J.M. Pittard, I.R. Stevens, K. Hamaguchi, T.R. Gull
Chandra X-ray Grating Spectrometry of Eta Carinae near X-ray Minimum: I. Variability of the Sulfur and Silicon Emission Lines
23 pages, 24 figures. Accepted for publication in the Astrophysical Journal. New layout for Figure 21; corrected typo in Table 7; corrected x-axis label in Figure 23
Astrophys.J. 680:705,2008
10.1086/587472
null
astro-ph
null
We report on variations in important X-ray emission lines in a series of Chandra grating spectra of the supermassive colliding wind binary star Eta Carinae, including key phases around the X-ray minimum/periastron passage in 2003.5. The X-rays arise from the collision of the slow, dense wind of Eta Car with the fast, low-density wind of an otherwise hidden companion star. The X-ray emission lines provide the only direct measure of the flow dynamics of the companion's wind along the wind-wind collision zone. We concentrate here on the silicon and sulfur lines, which are the strongest and best resolved lines in the X-ray spectra. Most of the line profiles can be adequately fit with symmetric Gaussians with little significant skewness. Both the silicon and sulfur lines show significant velocity shifts and correlated increases in line widths through the observations. The R = forbidden-to-intercombination ratio from the Si XIII and S XV triplets is near or above the low-density limit in all observations, suggesting that the line-forming region is >1.6 stellar radii from the companion star. We show that simple geometrical models cannot simultaneously fit both the observed centroid variations and changes in line width as a function of phase. We show that the observed profiles can be fitted with synthetic profiles with a reasonable model of the emissivity along the wind-wind collision boundary. We use this analysis to help constrain the line formation region as a function of orbital phase, and the orbital geometry.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:14:44 GMT" }, { "version": "v2", "created": "Sat, 15 Mar 2008 16:35:14 GMT" } ]
2014-11-18T00:00:00
[ [ "Henley", "D. B.", "" ], [ "Corcoran", "M. F.", "" ], [ "Pittard", "J. M.", "" ], [ "Stevens", "I. R.", "" ], [ "Hamaguchi", "K.", "" ], [ "Gull", "T. R.", "" ] ]
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801.478
David H. Cohen
David H. Cohen (Swarthmore College)
X-rays from magnetically channeled winds of OB stars
2 pages; 1 figure (color, but looks fine in b/w). To appear as part of an article on the specialist session on magnetic massive stars held prior to IAU Symposium 250, "Massive Stars as Cosmic Engines," Kauai, HI, December 2007; eds. Bresolin, Crowther, & Puls, Cambridge University Press, 2008
null
null
null
astro-ph
null
OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong and hard X-ray emission via the Magnetically Channeled Wind Shock (MCWS) mechanism. In this brief paper, I describe four separate X-ray diagnostics of the MCWS mechanism in OB stars, with applications to the prototype young O star, theta-1 Ori C.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:06:07 GMT" } ]
2008-02-01T00:00:00
[ [ "Cohen", "David H.", "", "Swarthmore College" ] ]
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801.4781
Richard Henry
R.B.C. Henry (Univ. of Oklahoma), K.B. Kwitter (Williams College), R.J. Dufour (Rice Univ.), J.N. Skinner (Dartmouth College)
A Multiwavelength Analysis of the Halo Planetary Nebula DdDm-1
39 pages, including 7 figures. Submitted to ApJ. Comments welcome
null
10.1086/588460
null
astro-ph
null
We present new HST optical imagery as well as new UV and IR spectroscopic data obtained with the Hubble and Spitzer Space Telescopes, respectively, of the halo planetary nebula DdDm-1. For the first time we present a resolved image of this object which indicates that the morphology of DdDm-1 can be described as two orthogonal elliptical components in the central part surrounded by an extended halo. The extent of the emission is somewhat larger than was previously reported in the literature. We combine the spectral data with our own previously published optical measurements to derive nebular abundances of He, C, N, O, Ne, Si, S, Cl, Ar, and Fe. Our abundance determinations include the use of the newly developed program ELSA for obtaining abundances directly from emission line strengths along with detailed photoionization models to render a robust set of abundances for this object. The metallicity, as gauged by oxygen, is found to be 0.46 dex below the solar value, confirming DdDm-1's status as a halo PN. In addition, we find that Si and Fe are markedly underabundant, suggesting their depletion onto dust. The very low (but uncertain) C/O ratio suggests that the chemistry of the nebula should be consistent with an oxygen-rich environment. We find that the sulfur abundance of DdDm-1 is only slightly below the value expected based upon the normal lockstep behavior between S and O observed in H II regions and blue compact galaxies. The central star effective temperature and luminosity are estimated to be 55,000 K and 1000 solar luminosities, respectively, implying an initial progenitor mass of <1 solar masses. Finally, we report on a new radial velocity determination from echelle observations.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:08:52 GMT" } ]
2009-11-13T00:00:00
[ [ "Henry", "R. B. C.", "", "Univ. of Oklahoma" ], [ "Kwitter", "K. B.", "", "Williams College" ], [ "Dufour", "R. J.", "", "Rice Univ." ], [ "Skinner", "J. N.", "", "Dartmouth College" ] ]
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801.4782
Junya Yagi
Meng-Chwan Tan, Junya Yagi
Chiral Algebras of (0,2) Sigma Models: Beyond Perturbation Theory
38 pages. Minor changes to Section 2.3 and corrections to Section 4.2. Final results unchanged. Typos corrected
Lett.Math.Phys.84:257-273,2008
10.1007/s11005-008-0249-4
RUNHETC-2008-01
hep-th math.DG math.QA
null
We explore the nonperturbative aspects of the chiral algebras of N = (0,2) sigma models, which perturbatively are intimately related to the theory of chiral differential operators (CDOs). The grading by charge and scaling dimension is anomalous if the first Chern class of the target space is nonzero. This has some nontrivial consequences for the chiral algebra. As an example, we study the case where the target space is CP^1, and show that worldsheet instantons trivialize the chiral algebra entirely. Consequently, supersymmetry is spontaneously broken in this model. We then turn to a closer look at the supersymmetry breaking from the viewpoint of Morse theory on loop space. We find that instantons interpolate between pairs of perturbative supersymmetric states with different fermionic numbers, hence lifting them out of the supersymmetric spectrum. Our results reveal that a "quantum" deformation of the geometry of the target space leads to a trivialization of the kernels of certain twisted Dirac operators on CP^1.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 20:33:35 GMT" }, { "version": "v2", "created": "Mon, 3 Mar 2008 07:50:56 GMT" }, { "version": "v3", "created": "Sat, 19 Apr 2008 02:59:43 GMT" } ]
2008-11-26T00:00:00
[ [ "Tan", "Meng-Chwan", "" ], [ "Yagi", "Junya", "" ] ]
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801.4783
Ferenc Simon
S. Toth, D. Quintavalle, B. Nafradi, L. Korecz, L. Forro, and F. Simon
Enhanced thermal stability and spin-lattice relaxation rate of N@C60 inside carbon nanotubes
5 pages, 4 figures, 1 table
Phys. Rev. B 77, 214409 (2008)
10.1103/PhysRevB.77.214409
null
cond-mat.mtrl-sci
null
We studied the temperature stability of the endohedral fullerene molecule, N@C60, inside single-wall carbon nanotubes using electron spin resonance spectroscopy. We found that the nitrogen escapes at higher temperatures in the encapsulated material as compared to its pristine, crystalline form. The temperature dependent spin-lattice relaxation time, T_1, of the encapsulated molecule is significantly shorter than that of the crystalline material, which is explained by the interaction of the nitrogen spin with the conduction electrons of the nanotubes.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:15:40 GMT" } ]
2010-07-14T00:00:00
[ [ "Toth", "S.", "" ], [ "Quintavalle", "D.", "" ], [ "Nafradi", "B.", "" ], [ "Korecz", "L.", "" ], [ "Forro", "L.", "" ], [ "Simon", "F.", "" ] ]
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801.4784
Rubens Luis Pinto Gurgel do Amaral
R. L. P. G. Amaral, L. V. Belvedere and K. D. Rothe
Two-Dimensional Thermofield Bosonization II: Massive Fermions
21 pages, to be published in Annals of Physics
Annals Phys.323:2662-2684,2008
10.1016/j.aop.2008.01.005
null
hep-th
null
We consider the perturbative computation of the N-point function of chiral densities of massive free fermions at finite temperature within the thermofield dynamics approach. The infinite series in the mass parameter for the N-point functions are computed in the fermionic formulation and compared with the corresponding perturbative series in the interaction parameter in the bosonized thermofield formulation. Thereby we establish in thermofield dynamics the formal equivalence of the massive free fermion theory with the sine-Gordon thermofield model for a particular value of the sine-Gordon parameter. We extend the thermofield bosonization to include the massive Thirring model.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:23:12 GMT" } ]
2014-11-18T00:00:00
[ [ "Amaral", "R. L. P. G.", "" ], [ "Belvedere", "L. V.", "" ], [ "Rothe", "K. D.", "" ] ]
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801.4785
Tatsuhiro Misumi
Tatsuhiro Misumi
The zero-energy Landau levels in graphene as BPS-saturated states
This paper has been withdrawn
null
null
null
cond-mat.mes-hall
null
This paper has been withdrawn by the author, due to the crucial mistake of the discussion in Sec IV.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:29:19 GMT" }, { "version": "v2", "created": "Tue, 12 Feb 2008 08:07:20 GMT" } ]
2008-02-12T00:00:00
[ [ "Misumi", "Tatsuhiro", "" ] ]
[ 0.0562306084, 0.0290459488, 0.0504018255, 0.0661248416, -0.0498385392, 0.0200823601, -0.037544217, 0.0154413749, -0.0199476611, -0.0569163449, 0.0214293469, -0.0706801116, 0.0260091051, 0.0196537729, 0.1329354197, 0.1010975391, -0.0322297364, 0.1167715713, 0.0206211545, 0.0090186941, -0.0251764208, -0.0621573515, 0.0265478995, 0.0860112756, -0.0642635524, 0.0067533054, 0.1462583542, -0.039723888, 0.0149882976, 0.0299521051, 0.0574551411, -0.0044756723, -0.0372258388, -0.1145184338, -0.0248090606, 0.1381274462, -0.0152821857, 0.0673983544, -0.0947789401, -0.0334542729, -0.0366380624, -0.0393075459, -0.1936723143, 0.1022730917, 0.015845472, 0.0907624662, -0.0048552779, 0.0434709601, 0.0873827562, -0.0383279175, -0.067447342, 0.025715217, 0.005366521, 0.0277724341, -0.0252254028, -0.0561816245, -0.003991981, 0.017804727, -0.0635288283, 0.0223844834, 0.0265234094, 0.0008020698, -0.0004725936, -0.0019516012, -0.0292418748, -0.0357319042, -0.110306032, -0.0092268642, -0.001579649, 0.0342379734, -0.0356829241, 0.0254948009, 0.0033521622, 0.0032052181, -0.0090493076, 0.1046241969, 0.1010975391, -0.0386218056, -0.045332253, 0.0362951905, 0.0518712662, 0.065194197, -0.0173883848, -0.0482711345, -0.008981958, -0.0957095847, -0.0371768549, -0.0264009554, -0.1057997495, -0.0252254028, 0.0599531904, -0.0316664539, -0.0545652397, 0.0073533272, 0.0696514994, -0.0538794994, 0.0699943677, 0.0212089308, -0.0199476611, -0.0467282236, -0.001536025, 0.0535856113, 0.0228375606, -0.0509896018, 0.0567694008, 0.0326215886, -0.0569163449, -0.0097534144, -0.0046226163, 0.0442301705, 0.0213068929, 0.035658434, -0.0931135714, 0.0407280065, -0.0543693155, -0.0828274861, -0.0468016937, -0.035658434, 0.0622553155, 0.1717286706, -0.0306623336, 0.1116775125, 0.0575531051, -0.0167761166, 0.0422954075, 0.0690637231, 0.1177512035, -0.0531447791, -0.0496915951, 0.0174006298, 0.0865500718, 0.0174618568, 0.0048950752, -0.0179149341, -0.0185272004, 0.0419035591, -0.0477078483, 0.0769007429, 0.0541733876, -0.1173593476, 0.0076900744, 0.0416586511, 0.0939462557, 0.0242335293, -0.0135311019, 0.0373972729, 0.0375931971, 0.1517442614, 0.0889991373, 0.0429076739, 0.1030567884, 0.0060032783, 0.080770269, 0.021649763, 0.0042583174, -0.1395968944, 0.1111876965, 0.0206823815, 0.0439362824, 0.0366135687, 0.0248947777, 0.0284336824, 0.1322496831, -0.0365156084, 0.0621083714, 0.0142535772, -0.1047221571, -0.122257486, -0.0225681644, -0.195827499, -0.0220538601, -0.0346298255, -0.0146944094, -0.0741577893, -0.0433974899, 0.023609018, -0.0353400558, -0.0263274834, 0.0102983322, -0.0007622725, 0.1429276168, -0.053242743, -0.0083268322, 0.0580918975, -0.067447342, -0.092721723, 0.0760190785, 0.0154658658, 0.0028975538, 0.0298786331, -0.0932605192, 0.1182410121, 0.0326460786, -0.0400177762, -0.0123310583, -0.0897338614, 0.0323032103, 0.1349926442, 0.0074329223, 0.0684269667, -0.0555448681, -0.037666671, 0.0544672757, 0.0104146628, -0.029682707, 0.0419035591, -0.0340420492, -0.033723671, -0.0129555706, -0.0512345061, 0.0195435639, 0.0242457762, -0.0388177298, -0.0220905952, -0.0427607298, -0.0066920789, -0.0729332492, 0.0012735155, 0.0098391315, 0.0233886018, -0.096297361, 0.0387197696, 0.0244539455, 0.1040364206, 0.0558877364, -0.0146331824, -0.0250784587, 0.0632839203, -0.017816972, 0.1377355903, -0.0150372786, 0.0477323383, 0.0101881241, -0.0203517564, 0.0249560047, 0.0324011743, 0.0790069401, -0.0047726217, -0.1214737818, -0.0915461704, -0.0376176871, 0.0451363288, -0.0393075459, 0.079202868, -0.0339440852, -0.0231559407, -0.0489078909, -0.0166291725, 0.0547611639, -0.0241478123, -0.0630390197, 0.1918110251, -0.021698745, -0.0185516924, -0.154291302, -0.0209762696 ]
801.4786
Alexander Ushakov
Alex D. Myasnikov, Alexander Ushakov
Cryptanalysis of Anshel-Anshel-Goldfeld-Lemieux key agreement protocol
null
null
null
null
math.GR
null
The Anshel-Anshel-Goldfeld-Lemieux (abbreviated AAGL) key agreement protocol is proposed to be used on low-cost platforms which constraint the use of computational resources. The core of the protocol is the concept of an Algebraic Eraser (abbreviated AE) which is claimed to be a suitable primitive for use within lightweight cryptography. The AE primitive is based on a new and ingenious idea of using an action of a semidirect product on a (semi)group to obscure involved algebraic structures. The underlying motivation for AAGL protocol is the need to secure networks which deploy Radio Frequency Identification (RFID) tags used for identification, authentication, tracing and point-of-sale applications. In this paper we revisit the computational problem on which AE relies and heuristically analyze its hardness. We show that for proposed parameter values it is impossible to instantiate the secure protocol. To be more precise, in 100% of randomly generated instances of the protocol we were able to find a secret conjugator z generated by TTP algorithm (part of AAGL protocol).
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:35:11 GMT" } ]
2008-02-01T00:00:00
[ [ "Myasnikov", "Alex D.", "" ], [ "Ushakov", "Alexander", "" ] ]
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801.4787
Volker Eyert
Volker Eyert, Raymond Fresard, Antoine Maignan
Long-range magnetic order and spin-lattice coupling in the delafossite CuFeO2
5 pages, 5 figures, more information at http:www.physik.uni-augsburg.de/~eyert/
Phys. Rev. B 78, 052402 (2008)
10.1103/PhysRevB.78.052402
null
cond-mat.str-el
null
The electronic and magnetic properties of the delafossite CuFeO2 are investigated by means of electronic structure calculations. They are performed using density functional theory in the generalized gradient approximation as well as the new full-potential augmented spherical wave method. The calculations reveal three different spin states at the iron sites. Taking into account the correct crystal structure, we find long-range antiferromagnetic ordering in agreement with experiment. Contrasting previous work, our calculations show that non-local exchange interactions lead to a semiconducting ground state.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:38:43 GMT" } ]
2008-08-24T00:00:00
[ [ "Eyert", "Volker", "" ], [ "Fresard", "Raymond", "" ], [ "Maignan", "Antoine", "" ] ]
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801.4788
Benito Al\'en
Benito Alen, David Fuster, Guillermo Munoz-Matutano, Juan Martinez-Pastor, Yolanda Gonzalez, Luisa Gonzalez
Exciton Gas Compression and Metallic Condensation in a Single Semiconductor Quantum Wire
4 pages, 5 figures
Phys. Rev. Lett. 101, 067405 (2008)
10.1103/PhysRevLett.101.067405
null
cond-mat.str-el cond-mat.mes-hall
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the metal-insulator transition in individual self-assembled quantum wires and report optical evidences of metallic liquid condensation at low temperatures. Firstly, we observe that the temperature and power dependence of the single nanowire photoluminescence follow the evolution expected for an electron-hole liquid in one dimension. Secondly, we find novel spectral features that suggest that in this situation the expanding liquid condensate compresses the exciton gas in real space. Finally, we estimate the critical density and critical temperature of the phase transition diagram at $n_c\sim1\times10^5$ cm$^{-1}$ and $T_c\sim35$ K, respectively.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:45:36 GMT" }, { "version": "v2", "created": "Tue, 12 Aug 2008 11:19:32 GMT" } ]
2008-08-12T00:00:00
[ [ "Alen", "Benito", "" ], [ "Fuster", "David", "" ], [ "Munoz-Matutano", "Guillermo", "" ], [ "Martinez-Pastor", "Juan", "" ], [ "Gonzalez", "Yolanda", "" ], [ "Gonzalez", "Luisa", "" ] ]
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801.4789
Minho Son
Minho Son, Raman Sundrum
Anomaly-Mediation and Sequestering from a Higher-Dimensional viewpoint
33 pages, typos corrected, added references, version appearing in JHEP
JHEP 0808:004,2008
10.1088/1126-6708/2008/08/004
null
hep-th hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study a five-dimensional supergravity model with boundary-localized visible sector exhibiting anomaly-mediated supersymmetry breaking, in which the central requirements of sequestering and radius stabilization are achieved perturbatively. This makes it possible to understand these various mechanisms in a more integrated and transparent fashion, mostly from the higher-dimensional viewpoint. Local supersymmetry, in the presence of visible sector quantum effects, is enforced by the formalism of the five-dimensional superconformal tensor calculus. The construction results in only mild warping, which allows a natural supersymmetry-breaking mediation mechanism of (finite) boundary-to-boundary gravity loops to co-dominate with anomaly-mediation, thereby solving the latter's tachyonic slepton problem. We make the non-trivial check that this can occur while dangerous loops of stabilizing fields remain highly suppressed. Our discussion is a well-controlled starting point for considering other generalizations of anomaly-mediation, or for string theory realizations.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:47:52 GMT" }, { "version": "v2", "created": "Tue, 5 Aug 2008 17:55:27 GMT" } ]
2009-09-15T00:00:00
[ [ "Son", "Minho", "" ], [ "Sundrum", "Raman", "" ] ]
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801.479
Joel Ratsaby
Joel Ratsaby
Information Width
Typo error in eq. (13)
null
null
null
cs.DM cs.IT cs.LG math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Kolmogorov argued that the concept of information exists also in problems with no underlying stochastic model (as Shannon's information representation) for instance, the information contained in an algorithm or in the genome. He introduced a combinatorial notion of entropy and information $I(x:\sy)$ conveyed by a binary string $x$ about the unknown value of a variable $\sy$. The current paper poses the following questions: what is the relationship between the information conveyed by $x$ about $\sy$ to the description complexity of $x$ ? is there a notion of cost of information ? are there limits on how efficient $x$ conveys information ? To answer these questions Kolmogorov's definition is extended and a new concept termed {\em information width} which is similar to $n$-widths in approximation theory is introduced. Information of any input source, e.g., sample-based, general side-information or a hybrid of both can be evaluated by a single common formula. An application to the space of binary functions is considered.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 22:49:57 GMT" }, { "version": "v2", "created": "Tue, 1 Jul 2008 09:46:33 GMT" } ]
2008-07-01T00:00:00
[ [ "Ratsaby", "Joel", "" ] ]
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801.4791
Wally Melnitchouk
T. Hobbs, W. Melnitchouk
Finite-Q^2 corrections to parity-violating DIS
26 pages, 10 figures; figures 8 and 9 corrected; Eqs. (13) corrected
Phys.Rev.D77:114023,2008
10.1103/PhysRevD.77.114023
JLAB-THY-08-766
hep-ph hep-ex nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Parity-violating deep inelastic scattering (PVDIS) has been proposed as an important new tool to extract the flavor and isospin dependence of parton distributions in the nucleon. We discuss finite-Q^2 effects in PVDIS asymmetries arising from subleading kinematical corrections and longitudinal contributions to the photon-Z interference. For the proton, these need to be accounted for in order to accurately extract the d/u ratio at large x; for the deuteron they are important to consider when searching for evidence of charge symmetry violation in parton distributions or signals for physics beyond the standard model. We further explore the dependence of PVDIS asymmetries for polarized targets on the u and d helicity distributions at large x.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:02:18 GMT" }, { "version": "v2", "created": "Thu, 19 Jun 2008 19:37:58 GMT" }, { "version": "v3", "created": "Sat, 26 Jul 2008 13:52:41 GMT" }, { "version": "v4", "created": "Thu, 2 Oct 2014 15:34:46 GMT" } ]
2014-10-03T00:00:00
[ [ "Hobbs", "T.", "" ], [ "Melnitchouk", "W.", "" ] ]
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801.4792
Fabrizio Canfora
Marco Astorino, Fabrizio Canfora, Cristian Martinez, Luca Parisi
Minimal duality breaking in the Kallen-Lehman approach to 3D Ising model: a numerical test
15 pages, 3 figures; accepted for publication on PHYSICS LETTERS B; typos corrected in Eqs. (21) and (28); numerical results improved; references and clarifying comments added including the discussion of the behavior near the critical point; v6: acknowledgements added
Phys.Lett.B664:139-144,2008
10.1016/j.physletb.2008.05.016
null
cond-mat.stat-mech gr-qc hep-lat hep-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A Kallen-Lehman approach to 3D Ising model is analyzed numerically both at low and high temperature. It is shown that, even assuming a minimal duality breaking, one can fix three parameters of the model to get a very good agreement with the MonteCarlo results at high temperatures. With the same parameters the agreement is satisfactory both at low and near critical temperatures. How to improve the agreement with MonteCarlo results by introducing a more general duality breaking is shortly discussed.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 17:06:36 GMT" }, { "version": "v2", "created": "Thu, 7 Feb 2008 21:42:46 GMT" }, { "version": "v3", "created": "Wed, 20 Feb 2008 23:10:09 GMT" }, { "version": "v4", "created": "Thu, 28 Feb 2008 06:04:40 GMT" }, { "version": "v5", "created": "Thu, 8 May 2008 20:19:57 GMT" }, { "version": "v6", "created": "Fri, 20 Feb 2009 20:46:36 GMT" } ]
2009-02-20T00:00:00
[ [ "Astorino", "Marco", "" ], [ "Canfora", "Fabrizio", "" ], [ "Martinez", "Cristian", "" ], [ "Parisi", "Luca", "" ] ]
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801.4793
Francesco Nitti
F. Nitti
Holography and Emergent 4D Gravity
14 pages, 1 figure. Invited review for Modern Physics Letters A. Journal version; minor typos corrected
Mod.Phys.Lett.A23:289-303,2008
10.1142/S021773230802642X
null
hep-th hep-ph
null
I review recent work toward constructing, via five-dimensional holographic duals, four-dimensional theories in which spin-2 states (gravitons) are emergent. The basic idea is to extend to gravity model-building the applications of holographic duality to phenomenology construction.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 01:11:45 GMT" }, { "version": "v2", "created": "Mon, 25 Feb 2008 11:30:12 GMT" } ]
2008-11-26T00:00:00
[ [ "Nitti", "F.", "" ] ]
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801.4794
Joel Ratsaby
Joel Ratsaby
On the Complexity of Binary Samples
null
null
null
null
cs.DM cs.AI cs.LG
null
Consider a class $\mH$ of binary functions $h: X\to\{-1, +1\}$ on a finite interval $X=[0, B]\subset \Real$. Define the {\em sample width} of $h$ on a finite subset (a sample) $S\subset X$ as $\w_S(h) \equiv \min_{x\in S} |\w_h(x)|$, where $\w_h(x) = h(x) \max\{a\geq 0: h(z)=h(x), x-a\leq z\leq x+a\}$. Let $\mathbb{S}_\ell$ be the space of all samples in $X$ of cardinality $\ell$ and consider sets of wide samples, i.e., {\em hypersets} which are defined as $A_{\beta, h} = \{S\in \mathbb{S}_\ell: \w_{S}(h) \geq \beta\}$. Through an application of the Sauer-Shelah result on the density of sets an upper estimate is obtained on the growth function (or trace) of the class $\{A_{\beta, h}: h\in\mH\}$, $\beta>0$, i.e., on the number of possible dichotomies obtained by intersecting all hypersets with a fixed collection of samples $S\in\mathbb{S}_\ell$ of cardinality $m$. The estimate is $2\sum_{i=0}^{2\lfloor B/(2\beta)\rfloor}{m-\ell\choose i}$.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:14:19 GMT" } ]
2008-02-01T00:00:00
[ [ "Ratsaby", "Joel", "" ] ]
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801.4795
Christian Moni Bidin
C. Moni Bidin, M. Catelan, M. Altmann
Is a binary fraction-age relation responsible for the lack of EHB binaries in globular clusters?
Accepted for publication in A&A Lettersto the Editor
null
10.1051/0004-6361:20078782
null
astro-ph
null
The recently-discovered lack of close binaries, among extreme horizontal branch (EHB) stars in Galactic globular clusters, has thus far constituted a major puzzle, in view of the fact that blue subdwarf stars - the field counterparts of cluster EHB stars - are well-known to present a high binary fraction. In this Letter, we provide new results that confirm the lack of close EHB binaries in globular clusters, and present a first scenario to explain the difference between field and cluster EHB stars. First, in order to confirm that the lack of EHB binaries in globular clusters is a statistically robust result, we undertook a new analysis of 145 horizontal branch stars in NGC6752, out of which forty-one belong to the EHB. To search for radial-velocity variations as a function of time, we repeated high-resolution (R=18500) spectroscopy of all stars, four times during a single night of observations. We detected a single, hot (25000 K), radial-velocity variable star as a close-binary candidate. From these results, we estimate an upper-limit for the close (period P < 5 day) binary fraction f among NGC6752 EHB stars of 16% (95% confidence level), with the most probable value being f=4%. Thus our results clearly confirm the lack of close binaries among the hot HB stars in this cluster. We suggest that the confirmed discrepancy between the binary fractions for field and cluster EHB stars is the consequence of an f-age relation, with close binaries being more likely in the case of younger systems. We analyze theoretical and observational results available in the literature, which support this scenario. If so, an age difference between the EHB progenitors in the field and in clusters, the former being younger (on average) by up to several Gyr, would naturally account for the startling differences in binary fraction between the two populations.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:17:36 GMT" } ]
2009-11-13T00:00:00
[ [ "Bidin", "C. Moni", "" ], [ "Catelan", "M.", "" ], [ "Altmann", "M.", "" ] ]
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801.4796
Matthew Stowe
Matthew C. Stowe, Avi Pe'er, and Jun Ye
Control of Four-Level Quantum Coherence via Discrete Spectral Shaping of an Optical Frequency Comb
5 pages, 4 figures Submitted to Physical Review Letters
Phys. Rev. Lett. 100, 203001 (2008)
10.1103/PhysRevLett.100.203001
null
quant-ph physics.atom-ph
null
We present an experiment demonstrating high-resolution coherent control of a four-level atomic system in a closed (diamond) type configuration. A femtosecond frequency comb is used to establish phase coherence between a pair of two-photon transitions in cold Rb atoms. By controlling the spectral phase of the frequency comb we demonstrate the optical phase sensitive response of the diamond system. The high-resolution state selectivity of the comb is used to demonstrate the importance of the signs of dipole moment matrix elements in this type of closed-loop excitation. Finally, the pulse shape is optimized resulting in a 256% increase in the two-photon transition rate by forcing constructive interference between the mode pairs detuned from an intermediate resonance.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:25:34 GMT" } ]
2009-11-13T00:00:00
[ [ "Stowe", "Matthew C.", "" ], [ "Pe'er", "Avi", "" ], [ "Ye", "Jun", "" ] ]
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801.4797
Nikodem Poplawski
Nikodem J. Poplawski
Geometrization of electromagnetism in tetrad-spin-connection gravity
8 pages; published version
Mod. Phys. Lett.A24:431-442, 2009; Erratum-ibid.A26:1243,2011
10.1142/S0217732309030151 10.1142/S0217732311036024
null
gr-qc hep-th math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The metric-affine Lagrangian of Ponomarev and Obukhov for the unified gravitational and electromagnetic field is linear in the Ricci scalar and quadratic in the tensor of homothetic curvature. We apply to this Lagrangian the variational principle with the tetrad and spin connection as dynamical variables and show that, in this approach, the field equations are the Einstein-Maxwell equations if we relate the electromagnetic potential to the trace of the spin connection. We also show that, as in the Ponomarev-Obukhov formulation, the generally covariant Dirac Lagrangian gives rise to the standard spinor source for the Einstein-Maxwell equations, while the spinor field obeys the nonlinear Heisenberg-Ivanenko equation with the electromagnetic coupling. We generalize that formulation to spinors with arbitrary electric charges.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:30:00 GMT" }, { "version": "v2", "created": "Mon, 6 Apr 2009 15:49:23 GMT" }, { "version": "v3", "created": "Sat, 13 Nov 2010 20:06:16 GMT" } ]
2011-06-15T00:00:00
[ [ "Poplawski", "Nikodem J.", "" ] ]
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801.4798
Oscar Barraza
Oscar A. Barraza and Laura B. Langoni
Asymptotic behavior of global solutions of the $u_t=\Delta u + u^{p}$
15
null
null
null
math.AP
null
We study the asymptotic behavior of nonnegative solutions of the semilinear parabolic problem {u_t=\Delta u + u^{p}, x\in\mathbb{R}^{N}, t>0 u(0)=u_{0}, x\in\mathbb{R}^{N}, t=0. It is known that the nonnegative solution $u(t)$ of this problem blows up in finite time for $1<p\leq 1+ 2/N$. Moreover, if $p> 1+ 2/N$ and the norm of $u_{0}$ is small enough, the problem admits global solution. In this work, we use the entropy method to obtain the decay rate of the global solution $u(t)$.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:31:11 GMT" } ]
2008-02-01T00:00:00
[ [ "Barraza", "Oscar A.", "" ], [ "Langoni", "Laura B.", "" ] ]
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801.4799
Thomas Gregoire
Thomas Gregoire and Emanuel Katz
A composite gluino at the LHC
14 pages, 9 figures
JHEP 0812:084,2008
10.1088/1126-6708/2008/12/084
EDINBURGH-2008/05
hep-ph
null
We investigate the decay of particles with the quantum numbers of the gluino. Besides SUSY, such particles may be present in models where the Higgs and top are composite. We find that such 'composite' gluinos have decay signatures similar to those of gluinos in 'more minimal' SUSY type models. Though it is in principle possible to distinguish the two scenarios, we find that it will be a challenging task at the LHC. This puts into question the common lore that a gluino is an obvious 'smoking-gun' signature of SUSY.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:54:29 GMT" } ]
2008-12-25T00:00:00
[ [ "Gregoire", "Thomas", "" ], [ "Katz", "Emanuel", "" ] ]
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801.48
Joan Licata
Joan E. Licata
Constructing Seifert surfaces from n-bridge link projections
19 pages, 15 figures
null
null
null
math.GT math.GN
null
This paper presents a new algorithm "A" for constructing Seifert surfaces from n-bridge projections of links. The algorithm produces minimal complexity surfaces for large classes of braids and alternating links. In addition, we consider a family of knots for which the canonical genus is strictly greater than the genus, (g_c(K) > g(K)), and show that A builds surfaces realizing the knot genus g(K). We also present a generalization of Seifert's algorithm which may be used to construct surfaces representing arbitrary relative second homology classes in a link complement.
[ { "version": "v1", "created": "Wed, 30 Jan 2008 23:42:35 GMT" } ]
2008-02-01T00:00:00
[ [ "Licata", "Joan E.", "" ] ]
[ -0.0578475222, -0.025878448, 0.0745363757, 0.0660577938, -0.0308287591, 0.0229941215, -0.0514885895, -0.0064528431, -0.1002404168, -0.0193316974, -0.0088206744, -0.0859663561, -0.0569352694, -0.0211830325, 0.0374023393, -0.0346119218, 0.0294067189, -0.0437076129, 0.0258382019, 0.1312569976, 0.0986842215, -0.0701361001, 0.1370524764, 0.0081297774, 0.0539570339, 0.0267638694, 0.1276079863, -0.020109795, 0.0894007161, -0.0093036313, 0.0560766794, -0.042983178, -0.0327874161, 0.0163802933, -0.0666480735, 0.11236801, -0.0552180894, 0.003977688, 0.0119062327, 0.1684983522, 0.1088263243, 0.0826929808, -0.0124227284, -0.0139923394, 0.0158973355, 0.0810294598, 0.0124696828, 0.0036926093, 0.0029849429, 0.0357656516, -0.0469273254, 0.0904739574, 0.0176547635, -0.0601013228, -0.1181634963, 0.0496372543, -0.0517837293, 0.0113830296, -0.0948205665, -0.0041286121, 0.0907959267, -0.0997038037, -0.0223099329, 0.0082035623, -0.0940693021, 0.0519178845, -0.0665944144, 0.0998647884, -0.0115976771, -0.0025925403, -0.0845711455, -0.0124696828, 0.0051850807, 0.0355241746, -0.0422587432, -0.0367583968, -0.0325459391, 0.1042113975, 0.004967079, 0.0290579163, 0.0004921802, 0.0427685305, 0.0261065122, -0.0081163617, -0.0199488103, -0.0659504682, 0.0653065294, -0.0056043142, -0.1431699395, -0.0323312916, 0.031365376, 0.0399512798, 0.0180303976, 0.0921911374, 0.0958938077, 0.0491274633, 0.0588671006, 0.0550571047, 0.015629027, -0.0159241669, 0.0711556748, -0.0521861911, 0.0885957852, -0.0794732645, 0.1351206452, 0.0239734519, 0.0722289085, 0.0227928907, -0.1573366821, 0.0693311691, -0.0230209529, -0.0257174633, 0.0037563327, 0.0173730385, 0.2078861743, 0.0180840585, -0.0535545722, -0.0071102013, 0.0309360828, 0.0664334297, -0.045317471, -0.0378048047, 0.0592963956, -0.0034980848, 0.0068754302, -0.0368925519, 0.0182047971, 0.0051448341, 0.0279846787, -0.0460150763, 0.101689294, -0.0173327923, 0.1234223619, 0.0086194417, -0.0590280853, -0.0039877496, 0.0346924141, -0.0123288203, 0.0486176759, 0.06176484, 0.0389048755, 0.0129526397, 0.0093975393, 0.0302653089, 0.0455052853, 0.0547351316, -0.0280383397, 0.1376964301, 0.0771658048, 0.0946059227, -0.0626234338, 0.0024835395, 0.0426075459, 0.0799025595, -0.0814587548, -0.1470335871, -0.0246442258, 0.0333508663, 0.0425807126, 0.0400586054, 0.0877371952, 0.0728728548, 0.0478395782, 0.0534740798, -0.0833905861, 0.0558083691, -0.0276090447, 0.0137642762, -0.0043700906, 0.0152265625, 0.0746436939, -0.1320082545, -0.0313385464, 0.0536618941, -0.016729096, 0.0827466398, -0.1306130588, -0.1767622828, 0.0015679335, -0.0035450389, -0.0147301899, 0.1217051744, -0.005302466, -0.0739997551, -0.0468200035, 0.0147570213, 0.0102628376, -0.0179230738, 0.1094702631, 0.0667553991, -0.1003477424, 0.0392000154, 0.0248320419, 0.0568816103, -0.0505495034, -0.0148777608, 0.0171047281, 0.0194658525, 0.10979224, -0.0810294598, 0.0336460099, -0.109845899, 0.0770048201, -0.0180438124, 0.0202171188, -0.0570962578, 0.0650382191, -0.0090755681, -0.0301848166, -0.0087267654, 0.0219745468, -0.0396293104, -0.0002134947, 0.0537423864, 0.0532594323, 0.0230477843, 0.0302116461, -0.0052119116, 0.0010430531, 0.0954108462, -0.0865566358, 0.0049603716, 0.0299969986, 0.0691165179, 0.0918155015, 0.0236514807, 0.0137911066, -0.0517837293, -0.0442174003, -0.0350412168, -0.0072309403, 0.0675066635, -0.1122606844, -0.0116178002, -0.0673456788, 0.0544936545, -0.0664334297, -0.039119523, -0.0309360828, -0.0512202792, 0.0435466282, 0.0170778986, -0.0014153324, 0.11150942, 0.0134288892, 0.0265358072, -0.1086116731, -0.0251003522, 0.0129861785, 0.0644479394, 0.035497345, 0.1208465844, 0.0109067801, 0.0189560652, -0.0604232922, 0.0319824889 ]
801.4801
Jochen Greiner
J. Greiner, W. Bornemann, C. Clemens, M. Deuter, G. Hasinger, M. Honsberg, H. Huber, S. Huber, M. Krauss, T. Kr\"uhler, A. K\"upc\"u Yolda\c{s}, H. Mayer-Hasselwander, B. Mican, N. Primak, F. Schrey, I. Steiner, G. Szokoly, C.C. Th\"one, A. Yolda\c{s}, S. Klose, U. Laux, J. Winkler
GROND - a 7-channel imager
25 pages, 21 figs, PASP (subm); version with full-resolution figures at http://www.mpe.mpg.de/~jcg/GROND/grond_pasp.pdf
null
10.1086/587032
null
astro-ph
null
We describe the construction of GROND, a 7-channel imager, primarily designed for rapid observations of gamma-ray burst afterglows. It allows simultaneous imaging in the Sloan g'r'i'z' and near-infrared $JHK$ bands. GROND was commissioned at the MPI/ESO 2.2m telescope at La Silla (Chile) in April 2007, and first results of its performance and calibration are presented.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 00:33:51 GMT" } ]
2009-11-13T00:00:00
[ [ "Greiner", "J.", "" ], [ "Bornemann", "W.", "" ], [ "Clemens", "C.", "" ], [ "Deuter", "M.", "" ], [ "Hasinger", "G.", "" ], [ "Honsberg", "M.", "" ], [ "Huber", "H.", "" ], [ "Huber", "S.", "" ], [ "Krauss", "M.", "" ], [ "Krühler", "T.", "" ], [ "Yoldaş", "A. Küpcü", "" ], [ "Mayer-Hasselwander", "H.", "" ], [ "Mican", "B.", "" ], [ "Primak", "N.", "" ], [ "Schrey", "F.", "" ], [ "Steiner", "I.", "" ], [ "Szokoly", "G.", "" ], [ "Thöne", "C. C.", "" ], [ "Yoldaş", "A.", "" ], [ "Klose", "S.", "" ], [ "Laux", "U.", "" ], [ "Winkler", "J.", "" ] ]
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801.4802
Grenville Croll
Alan Rust, Brian Bishop, Kevin McDaid
Investigating the Potential of Test-Driven Development for Spreadsheet Engineering
11 pages, 5 colour figures, 2 case studies
Proc. European Spreadsheet Risks Int. Grp. 2006 95-105 ISBN:1-905617-08-9
null
null
cs.SE
null
It is widely documented that the absence of a structured approach to spreadsheet engineering is a key factor in the high level of spreadsheet errors. In this paper we propose and investigate the application of Test-Driven Development to the creation of spreadsheets. Test-Driven Development is an emerging development technique in software engineering that has been shown to result in better quality software code. It has also been shown that this code requires less testing and is easier to maintain. Through a pair of case studies we demonstrate that Test-Driven Development can be applied to the development of spreadsheets. We present the detail of these studies preceded by a clear explanation of the technique and its application to spreadsheet engineering. A supporting tool under development by the authors is also documented along with proposed research to determine the effectiveness of the methodology and the associated tool.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 00:39:38 GMT" } ]
2008-03-10T00:00:00
[ [ "Rust", "Alan", "" ], [ "Bishop", "Brian", "" ], [ "McDaid", "Kevin", "" ] ]
[ -0.0480630808, 0.0138837937, 0.0462382138, -0.0388647579, -0.0319598541, -0.0679640099, -0.0108505674, 0.0500112511, 0.0194077194, 0.0504304767, 0.0671748742, -0.0335874371, 0.0438708179, 0.0301349852, 0.0837959722, 0.0726988018, 0.0888266936, -0.0618975535, -0.0752634779, 0.026707191, 0.0776802003, -0.0092414776, 0.0002591267, 0.1134377494, -0.0040997881, -0.0290992483, 0.010647119, 0.0612070635, 0.0353876464, -0.1514147371, 0.0143770017, -0.0548940077, 0.001511219, 0.0674708039, 0.0827602372, 0.1450030357, 0.0472986102, 0.1001704633, 0.0326750055, -0.0443393625, 0.0302089658, 0.0014395497, 0.0200488884, 0.1937319487, -0.0050492128, 0.0127617465, -0.0541541949, -0.0238342583, 0.0757566914, -0.0453257784, -0.0371385328, 0.0307268333, 0.0343519114, -0.0558804236, -0.0077741849, 0.0219847299, -0.1311932206, -0.0417007022, -0.0172252748, -0.0798996314, 0.0273483619, 0.0125829587, -0.0480630808, 0.087149784, -0.0631798953, -0.004633069, -0.0470520072, -0.0056780525, 0.008310548, -0.0282607954, -0.0180390682, 0.0113622705, 0.0884321257, 0.0608124994, 0.045745004, -0.1268529892, -0.04209527, 0.1106757894, -0.0474712327, 0.0599740446, 0.071071215, -0.0585930645, -0.0689504221, -0.0091613317, -0.0752634779, -0.0846837461, -0.0352150239, -0.0776308775, -0.0550912879, -0.1082097515, -0.1041654497, 0.068999745, 0.0217504557, 0.0552392527, 0.0887773708, 0.0137358317, -0.0132179642, 0.0578532517, 0.052921176, -0.0567188747, -0.0097901709, 0.0305542108, -0.0125829587, 0.0087421052, 0.1503296793, -0.0241548419, -0.0091798268, -0.0061650951, -0.0053451373, 0.0320091732, -0.1253733784, -0.017903436, -0.0261400025, -0.0704793707, 0.0531184599, -0.0104375063, 0.0298143998, -0.1385913342, -0.0244507678, -0.090947479, -0.0984935611, 0.0880868807, 0.0219847299, -0.0231314376, 0.0971125811, -0.0485809483, 0.0108505674, -0.1071246937, -0.0064301942, 0.0500852317, -0.0122932, 0.0298637208, 0.0743263885, 0.0182240214, -0.0661884621, 0.0078420006, -0.1597992629, 0.125176087, 0.0193090774, 0.0337354019, 0.0413307957, -0.0244014468, -0.0046947198, 0.0872484222, 0.009543567, -0.1163969934, 0.041306138, 0.065004766, 0.0246850401, 0.0792584643, -0.1212304309, 0.0294691548, -0.0557817817, 0.0039795688, 0.0394319482, -0.085768804, 0.0136495205, 0.0935614854, -0.0277675875, -0.1158051491, 0.0196173321, 0.0377797037, 0.0062976447, 0.1219209209, -0.0499865897, 0.0313186832, -0.0063808733, -0.0524279699, -0.1534862071, 0.0321817957, -0.0281868149, -0.1273462027, -0.008705114, 0.0587903485, 0.0179157667, -0.0270031169, -0.0609604605, -0.0513922311, 0.0476438552, -0.0430323631, -0.1082097515, -0.0678160489, -0.072452195, -0.0437228531, -0.0577546097, -0.0943012908, 0.0163868219, 0.0284827389, 0.0822177082, -0.0032829132, -0.0438708179, -0.0196789838, -0.0083290432, 0.0654486492, 0.0044635287, -0.0769403875, 0.0086434633, 0.1123526916, -0.0099258032, 0.0483096838, 0.0309980977, -0.0380509682, 0.0198516063, -0.0700848028, 0.0144756436, -0.0105793029, -0.0628346503, 0.049616687, -0.0584450997, -0.1354348063, 0.0292965323, 0.0010318828, -0.0179650877, 0.1246828809, 0.0565709136, -0.0678653643, 0.0322557762, -0.0000379779, 0.0532171018, 0.0470520072, -0.0385441743, -0.0209366623, -0.054647401, -0.021836767, 0.0014819347, 0.070380725, 0.0179157667, -0.0321078151, 0.1053491458, -0.1249788105, -0.0389387421, -0.0772856325, -0.0688517839, 0.0164977945, 0.0944985747, -0.0098518217, -0.0521813631, -0.1182711869, 0.0058537577, 0.0102587184, 0.0177308135, 0.0751155168, -0.0116027091, -0.0833027661, -0.0571627617, 0.0374097973, -0.0523293279, -0.0675694421, -0.010597798, 0.0278908908, 0.0193953887, -0.1082097515, 0.0679640099, -0.0393333063, -0.0463861749, -0.0572614037 ]
801.4803
Li Xiao
L. Xiao, E. F\"urst, W. Reich and J. L. Han
Radio spectral properties and the magnetic field of the SNR S147
11 pages, 17 figures, accepted for publication in Astronomy & Astrophysics, the resolution of some figures have been reduced. For high resolution version, see ftp://ftp.mpifr-bonn.mpg.de/outgoing/p098wre/xiao-etal.pdf,revised following the language editor
null
10.1051/0004-6361:20078461
null
astro-ph
null
(Abridged) S147 is a large faint shell-type supernova remnant (SNR). Its remarkable spectral break at cm-wavelengths is an important physical property to characterize the SNR evolution. However, the spectral break is based on radio observations with limited precision. We made new radio continuum and polarization observations of S147 at 11cm and at 6cm with the Effelsberg 100-m telescope and the Urumqi 25-m telescope, respectively. These new data were combined with published lower frequency data from the Effelsberg 100-m telescope and very high frequency data from WMAP to investigate the spectral turnover and polarization properties of S147. S147 consists of numerous filaments embedded in diffuse emission. We found that the integrated flux densities of S147 are 34.8+/-4.0 Jy at 11cm and 15.4+/-3.0Jy at 6cm. These new measurements confirm the known spectral turnover at ~1.5GHz, which can be entirely attributed to the diffuse emission component. The spectral index above the turnover is -1.35+/-0.20. The filamentary emission component has a constant spectral index over the entire wavelength range up to 40.7GHz of -0.35+/-0.15. The weak polarized emission of S147 is at the same level as the ambient diffuse Galactic polarization. The rotation measure of the eastern filamentary shell is about -70 rad/m2. The filamentary and diffuse emission components of S147 have different physical properties, which make S147 outstanding among shell type SNRs.The weak polarization of S147 at 11cm and at 6cm can be attributed to a section of the S147 shell showing a tangential magnetic field direction.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 00:50:34 GMT" }, { "version": "v2", "created": "Tue, 26 Feb 2008 03:45:47 GMT" } ]
2009-11-13T00:00:00
[ [ "Xiao", "L.", "" ], [ "Fürst", "E.", "" ], [ "Reich", "W.", "" ], [ "Han", "J. L.", "" ] ]
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801.4804
Eric Hudson
Eric R. Hudson, Nathan B. Gilfoy, Svetlana Kotochigova, Jeremy M. Sage, and David DeMille
Inelastic collisions of ultra-cold heteronuclear molecules in an optical trap
null
null
10.1103/PhysRevLett.100.203201
null
physics.atom-ph physics.chem-ph
null
Ultra-cold RbCs molecules in high-lying vibrational levels of the a$^3\Sigma^+$ ground electronic state are confined in an optical trap. Inelastic collision rates of these molecules with both Rb and Cs atoms are determined for individual vibrational levels, across an order of magnitude of binding energies. A simple model for the collision process is shown to accurately reproduce the observed scattering rates.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 01:10:42 GMT" } ]
2009-11-13T00:00:00
[ [ "Hudson", "Eric R.", "" ], [ "Gilfoy", "Nathan B.", "" ], [ "Kotochigova", "Svetlana", "" ], [ "Sage", "Jeremy M.", "" ], [ "DeMille", "David", "" ] ]
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801.4805
Makoto Uemura
M. Uemura, A. Arai, M. Sasada, P. Schmeer, I. Miller, T. Ohsugi, T. Yamashita, K. S. Kawabata, M. Isogai, S. Sato, and M. Kino
Outburst of a WZ Sge-type dwarf nova, AL Com in 2007
4 pages, 2 figures, accepted for publication in IBVS
null
null
null
astro-ph
null
We report photometric observations of AL Com during its rare outburst in 2007. The light curve is reminiscent of its past superoutbursts in 1995 and 2001, except for the rebrightening phase after the main superoutburst. During the rebrightening phase in 2007, we found clear modulations between V=16.2-15.2. In conjunction with the lack of prominent superhumps in our time-series observations, the modulations can most naturally be interpreted as repetitive short rebrightenings with a cycle of 1-2 days. The rebrightening characteristics in 2007 are different from those in 1995 and 2001. This indicates that the type of rebrightenings in WZ Sge stars depends not on binary parameters of objects, but on the mass-accretion process for each outburst.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 01:23:09 GMT" } ]
2008-02-01T00:00:00
[ [ "Uemura", "M.", "" ], [ "Arai", "A.", "" ], [ "Sasada", "M.", "" ], [ "Schmeer", "P.", "" ], [ "Miller", "I.", "" ], [ "Ohsugi", "T.", "" ], [ "Yamashita", "T.", "" ], [ "Kawabata", "K. S.", "" ], [ "Isogai", "M.", "" ], [ "Sato", "S.", "" ], [ "Kino", "M.", "" ] ]
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801.4806
Mark Neubauer
CDF Collaboration: T. Aaltonen, et al
First Measurement of ZZ Production in ppbar Collisions at sqrt(s)=1.96 TeV
7 pages, 1 figure. Submitted to Phys. Rev. Lett
Phys.Rev.Lett.100:201801,2008
10.1103/PhysRevLett.100.201801
FERMILAB-PUB-08-022-E
hep-ex
null
We report the first measurement of the cross section for Z boson pair production at a hadron collider. This result is based on a data sample corresponding to 1.9 fb-1 of integrated luminosity from ppbar collisions at sqrt{s} = 1.96 TeV collected with the CDF II detector at the Fermilab Tevatron. In the llll channel, we observe three ZZ candidates with an expected background of 0.096^{+0.092}_{-0.063} events. In the llnunu channel, we use a leading-order calculation of the relative ZZ and WW event probabilities to discriminate between signal and background. In the combination of llll and llnunu channels, we observe an excess of events with a probability of $5.1\times 10^{-6}$ to be due to the expected background. This corresponds to a significance of 4.4 standard deviations. The measured cross section is sigma(ppbar -> ZZ) = 1.4^{+0.7}_{-0.6} (stat.+syst.) pb, consistent with the standard model expectation.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 01:28:10 GMT" } ]
2010-05-12T00:00:00
[ [ "CDF Collaboration", "", "" ], [ "Aaltonen", "T.", "" ] ]
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801.4807
Syed Ali Jafri
Syed Ali Raza Jafri, Mireille Boutin, and Edward J. Delp
Automatic Text Area Segmentation in Natural Images
null
null
null
null
cs.CV
null
We present a hierarchical method for segmenting text areas in natural images. The method assumes that the text is written with a contrasting color on a more or less uniform background. But no assumption is made regarding the language or character set used to write the text. In particular, the text can contain simple graphics or symbols. The key feature of our approach is that we first concentrate on finding the background of the text, before testing whether there is actually text on the background. Since uniform areas are easy to find in natural images, and since text backgrounds define areas which contain "holes" (where the text is written) we thus look for uniform areas containing "holes" and label them as text backgrounds candidates. Each candidate area is then further tested for the presence of text within its convex hull. We tested our method on a database of 65 images including English and Urdu text. The method correctly segmented all the text areas in 63 of these images, and in only 4 of these were areas that do not contain text also segmented.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 01:46:32 GMT" } ]
2008-02-01T00:00:00
[ [ "Jafri", "Syed Ali Raza", "" ], [ "Boutin", "Mireille", "" ], [ "Delp", "Edward J.", "" ] ]
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801.4808
Murray Gerstenhaber
Murray Gerstenhaber, Anthony Giaquinto
The Principal Element of a Frobenius Lie Algebra
10 pages
Letters in Mathematical Physics, Vol. 88, 2009, 333-341
10.1007/s11005-009-0321-8
null
math.RT math.QA math.RA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We introduce the notion of the \textit{principal element} of a Frobenius Lie algebra $\f$. The principal element corresponds to a choice of $F\in \f^*$ such that $F[-,-]$ non-degenerate. In many natural instances, the principal element is shown to be semisimple, and when associated to $\sl_n$, its eigenvalues are integers and are independent of $F$. For certain ``small'' functionals $F$, a simple construction is given which readily yields the principal element. When applied to the first maximal parabolic subalgebra of $\sl_n$, the principal element coincides with semisimple element of the principal three-dimensional subalgebra. We also show that Frobenius algebras are stable under deformation.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 02:40:36 GMT" }, { "version": "v2", "created": "Wed, 21 Oct 2009 13:10:31 GMT" } ]
2015-05-13T00:00:00
[ [ "Gerstenhaber", "Murray", "" ], [ "Giaquinto", "Anthony", "" ] ]
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801.4809
Masataka Mizushima
Masataka Mizushima
Creation of Spiral Galaxies
null
null
null
null
physics.gen-ph
null
The spiral galaxies, including our galaxy, are created by the gravito-radiative forces generated by colliding black holes at the center of quasars. The gravito-radiative force is predicted by Einstein's general relativity. A quasar is assumed to have a circular disk of highly compressed neutrons (ylem) orbiting around black holes. The collision of two black holes at the center generates the gravito-radiative force, exerted on the ylem disk, producing a pair of bars with 180 degree rotational symmetry. This pair of bars develop into a pair of spiral arms, keeping the 180 degree rotational symmetry. Therefore, the number of spiral arms must be even. Our Milky Way galaxy has two pairs of arms, and has the 180 degree rotational symmetry, indicating that we have had two galactic nuclear explosions. The theory proposed by Gamow and others on the making of chemical elements fits into this theory. Thus, the age of the Milky Way must be equal to or greater than the age of the earth, 4.5 billion yr. The spirality of the Milky Way galaxy is examined under this assumption, and it is found that our galaxy was once about 10 times larger than it is now, and has been shrinking during the last half of its life.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 02:42:57 GMT" } ]
2008-02-01T00:00:00
[ [ "Mizushima", "Masataka", "" ] ]
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801.481
Ignacio General
Ping Wang, Stephen R. Cotanch and Ignacio J. General
Meson and tetra-quark mixing
7 pages, 6 figures
Eur.Phys.J.C55:409-415,2008
10.1140/epjc/s10052-008-0605-7
null
hep-ph
null
The mixing between q-qbar meson and qqbar-qqbar tetra-quark states is examined within an effective QCD Coulomb gauge Hamiltonian model. Mixing matrix elements of the Hamiltonian are computed and then diagonalized yielding an improved prediction for the low-lying J^{PC} = 0^{+/- +}, 1^{--} isoscalar spectra. Mixing effects were found significant for the scalar hadrons but not for the 1^{--} states, which is consistent with the ideal mixing of vector mesons. A perturbative assessment of the exact QCD kernel is also reported.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 02:52:35 GMT" } ]
2008-11-26T00:00:00
[ [ "Wang", "Ping", "" ], [ "Cotanch", "Stephen R.", "" ], [ "General", "Ignacio J.", "" ] ]
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801.4811
Xander Faber
X.W.C. Faber
Equidistribution of Dynamically Small Subvarieties over the Function Field of a Curve
v2: Various typos fixed; statement and proof of auxiliary Prop. 6.1 corrected. During the process of preparing this manuscript for submission, it came to the author's attention that Walter Gubler has recently proved many of the same results. See arXiv:0801.4508v3. v3: References updated and a few more typos corrected. To appear in Acta Arithmetica
null
10.4064/aa137-4-4
null
math.NT math.DS
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
For a projective variety X defined over a field K, there is a special class of self-morphisms of X called algebraic dynamical systems. In this paper we take K to be the function field of a smooth curve and prove that at each place of K, subvarieties of X of dynamically small height are equidistributed on the associated Berkovich analytic space. We carefully develop all of the arithmetic intersection theory needed to state and prove this theorem, and we present several applications on the non-Zariski density of preperiodic points and of points of small height in field extensions of bounded degree.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:16:39 GMT" }, { "version": "v2", "created": "Wed, 13 Feb 2008 17:21:38 GMT" }, { "version": "v3", "created": "Wed, 3 Dec 2008 14:17:18 GMT" } ]
2015-05-13T00:00:00
[ [ "Faber", "X. W. C.", "" ] ]
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801.4812
Christopher Wylie
C. Scott Wylie, Cheol-Min Ghim, David A. Kessler, Herbert Levine
The fixation probability of rare mutators in finite asexual populations
46 pages, 8 figures
null
null
null
q-bio.PE
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A mutator is an allele that increases the mutation rate throughout the genome by disrupting some aspect of DNA replication or repair. Mutators that increase the mutation rate by the order of 100 fold have been observed to spontaneously emerge and achieve high frequencies in natural populations and in long-term laboratory evolution experiments with \textit{E. coli}. In principle, the fixation of mutator alleles is limited by (i) competition with mutations in wild-type backgrounds, (ii) additional deleterious mutational load, and (iii) random genetic drift. Using a multiple locus model and employing both simulation and analytic methods, we investigate the effects of these three factors on the fixation probability $P_{fix}$ of an initially rare mutator as a function of population size $N$, beneficial and deleterious mutation rates, and the strength of mutations $s$. Our diffusion based approximation for $P_{fix}$ successfully captures effects (ii) and (iii) when selection is fast compared to mutation ($\mu/s \ll 1$). This enables us to predict the conditions under which mutators will be evolutionarily favored. Surprisingly, our simulations show that effect (i) is typically small for strong-effect mutators. Our results agree semi-quantitatively with existing laboratory evolution experiments and suggest future experimental directions.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:08:43 GMT" }, { "version": "v2", "created": "Tue, 5 Feb 2008 02:14:07 GMT" }, { "version": "v3", "created": "Wed, 31 Dec 2008 04:10:57 GMT" } ]
2008-12-31T00:00:00
[ [ "Wylie", "C. Scott", "" ], [ "Ghim", "Cheol-Min", "" ], [ "Kessler", "David A.", "" ], [ "Levine", "Herbert", "" ] ]
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801.4813
David Broadhurst
David Broadhurst
Elliptic integral evaluation of a Bessel moment by contour integration of a lattice Green function
13 pages, now includes staircase polygons and complex separatrices
null
null
null
hep-th
null
A proof is found for the elliptic integral evaluation of the Bessel moment $$M:=\int_0^\infty t I_0^2(t)K_0^2(t)K_0(2t) {\rm d}t ={1/12} {\bf K}(\sin(\pi/12)){\bf K}(\cos(\pi/12)) =\frac{\Gamma^6(\frac13)}{64\pi^22^{2/3}}$$ resulting from an angular average of a 2-loop 4-point massive Feynman diagram, with one internal mass doubled. This evaluation follows from contour integration of the Green function for a hexagonal lattice, thereby relating $M$ to a linear combination of two more tractable moments, one given by the Green function for a diamond lattice and both evaluated by using W.N. Bailey's reduction of an Appell double series to a product of elliptic integrals. Cubic and sesquiplicate modular transformations of an elliptic integral from the equal-mass Dalitz plot are proven and used extensively. Derivations are given of the sum rules $$\int_0^\infty(I_0(a t)K_0(a t)-\frac{2}{\pi} K_0(4a t) K_0(t))K_0(t) {\rm d}t=0$$ with $a>0$, proven by analytic continuation of an identity from Bailey's work, and $$\int_0^\infty t I_0(a t)(I_0^3(a t)K_0(8t)- \frac{1}{4\pi^2} I_0(t)K_0^3(t)) {\rm d}t=0$$ with $2\ge a\ge0$, proven by showing that a Feynman diagram in two spacetime dimensions generates the enumeration of staircase polygons in four dimensions.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:14:13 GMT" }, { "version": "v2", "created": "Fri, 1 Feb 2008 10:48:33 GMT" }, { "version": "v3", "created": "Wed, 6 Feb 2008 05:17:25 GMT" } ]
2008-02-06T00:00:00
[ [ "Broadhurst", "David", "" ] ]
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801.4814
Patrick Morris
P. Morris and the Spitzer WRRINGS Team
Infrared Tracers of Mass-Loss Histories and Wind-ISM Interactions in Hot Star Nebulae
6 pages, 6 figs, to be published in proceedings of IAU Symposium 250: Massive Stars as Cosmic Engines by CUP, eds. F. Bresolin, P.A. Crowther, J. Puls Eds
null
10.1017/S174392130802070X
null
astro-ph
null
Infrared observations of hot massive stars and their environments provide a detailed picture of mass loss histories, dust formation, and dynamical interactions with the local stellar medium that can be unique to the thermal regime. We have acquired new infrared spectroscopy and imaging with the sensitive instruments onboard the Spitzer Space Telescope in guaranteed and open time programs comprised of some of the best known examples of hot stars with circumstellar nebulae, supplementing with unpublished Infrared Space Observatory spectroscopy. Here we present highlights of our work on the environment around the extreme P Cygni-type star HDE316285, revealing collisionally excited H2 for the first time in a hot star nebula, and providing some defining characteristics of the star's evolution and interactions with the ISM at unprecented detail in the infrared.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:24:04 GMT" } ]
2009-11-13T00:00:00
[ [ "Morris", "P.", "" ], [ "Team", "the Spitzer WRRINGS", "" ] ]
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801.4815
Craig Hodgson
Oliver Goodman, Damian Heard and Craig Hodgson
Commensurators of cusped hyperbolic manifolds
32 pages, 46 figures; to appear in "Experimental Mathematics"
null
null
null
math.GT
null
This paper describes a general algorithm for finding the commensurator of a non-arithmetic cusped hyperbolic manifold, and for deciding when two such manifolds are commensurable. The method is based on some elementary observations regarding horosphere packings and canonical cell decompositions. For example, we use this to find the commensurators of all non-arithmetic hyperbolic once-punctured torus bundles over the circle. For hyperbolic 3-manifolds, the algorithm has been implemented using Goodman's computer program Snap. We use this to determine the commensurability classes of all cusped hyperbolic 3-manifolds triangulated using at most 7 ideal tetrahedra, and for the complements of hyperbolic knots and links with up to 12 crossings.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:40:46 GMT" } ]
2008-02-01T00:00:00
[ [ "Goodman", "Oliver", "" ], [ "Heard", "Damian", "" ], [ "Hodgson", "Craig", "" ] ]
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801.4816
Albert Seaver
Albert E. Seaver
The Criteria for Interfacial Electro-Thermal Equilibrium
PDF, 17 pages, Paper was presented at the 2005 Electrostatics Society of America Annual Meeting, University of Alberta, Edmonton, Alberta, Canada, 6/22-24/05
null
null
null
physics.class-ph physics.gen-ph
null
When the surface of a first material is brought into contact with the surface of a second material the contact region is called an interface. Since the time of James Clerk Maxwell it has been customary to treat a material electrically as having well-defined bulk properties and having surfaces of zero-thickness. In order to obtain a better understanding of the interface this paper reviews Maxwell's original argument to justify a zero-thickness-surface and reexamines the interface problem assuming electrical charges are actually particles having a finite thickness. Thermodynamics requires that in thermal equilibrium any movement of free charge cannot produce a net electrical current anywhere in the materials or across their interface. For materials in contact and in thermal equilibrium this reexamination gives a set of equations that can be called the interfacial electro-thermal equilibrium (IETE) criteria. A well-defined interfacial potential results from this criteria.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:42:36 GMT" } ]
2008-02-01T00:00:00
[ [ "Seaver", "Albert E.", "" ] ]
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801.4817
Shenghui Su
Shenghui Su and Shuwang Lv
The REESSE2+ Public-key Encryption Scheme
11 pages, 2 tables
null
null
null
cs.CR cs.CC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper gives the definitions of an anomalous super-increasing sequence and an anomalous subset sum separately, proves the two properties of an anomalous super-increasing sequence, and proposes the REESSE2+ public-key encryption scheme which includes the three algorithms for key generation, encryption and decryption. The paper discusses the necessity and sufficiency of the lever function for preventing the Shamir extremum attack, analyzes the security of REESSE2+ against extracting a private key from a public key through the exhaustive search, recovering a plaintext from a ciphertext plus a knapsack of high density through the L3 lattice basis reduction method, and heuristically obtaining a plaintext through the meet-in-the-middle attack or the adaptive-chosen-ciphertext attack. The authors evaluate the time complexity of REESSE2+ encryption and decryption algorithms, compare REESSE2+ with ECC and NTRU, and find that the encryption speed of REESSE2+ is ten thousand times faster than ECC and NTRU bearing the equivalent security, and the decryption speed of REESSE2+ is roughly equivalent to ECC and NTRU respectively.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 03:50:39 GMT" }, { "version": "v2", "created": "Tue, 5 Feb 2008 17:56:47 GMT" }, { "version": "v3", "created": "Sat, 1 Nov 2014 15:57:54 GMT" } ]
2014-11-04T00:00:00
[ [ "Su", "Shenghui", "" ], [ "Lv", "Shuwang", "" ] ]
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801.4818
Stefan Mashkevich
Stefan Mashkevich (New York / Kiev), St\'ephane Ouvry (Orsay)
Random Aharonov-Bohm vortices and some exact families of integrals: Part II
9 pages, LaTeX 2e. A few sentences rephrased more exactly, misprints corrected
J. Stat. Mech. (2008) P03018
10.1088/1742-5468/2008/03/P03018
null
cond-mat.mes-hall cond-mat.stat-mech hep-th
null
At 6th order in perturbation theory, the random magnetic impurity problem at second order in impurity density narrows down to the evaluation of a single Feynman diagram with maximal impurity line crossing. This diagram can be rewritten as a sum of ordinary integrals and nested double integrals of products of the modified Bessel functions $K_{\nu}$ and $I_{\nu}$, with $\nu=0,1$. That sum, in turn, is shown to be a linear combination with rational coefficients of $(2^5-1)\zeta(5)$, $\int_0^{\infty} u K_0(u)^6 du$ and $\int_0^{\infty} u^3 K_0(u)^6 du$. Unlike what happens at lower orders, these two integrals are not linear combinations with rational coefficients of Euler sums, even though they appear in combination with $\zeta(5)$. On the other hand, any integral $\int_0^{\infty} u^{n+1} K_0(u)^p (uK_1(u))^q du$ with weight $p+q=6$ and an even $n$ is shown to be a linear combination with rational coefficients of the above two integrals and 1, a result that can be easily generalized to any weight $p+q=k$. A matrix recurrence relation in $n$ is built for such integrals. The initial conditions are such that the asymptotic behavior is determined by the smallest eigenvalue of the transition matrix.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 14:46:24 GMT" }, { "version": "v2", "created": "Fri, 22 Feb 2008 04:01:59 GMT" } ]
2009-11-13T00:00:00
[ [ "Mashkevich", "Stefan", "", "New York / Kiev" ], [ "Ouvry", "Stéphane", "", "Orsay" ] ]
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801.4819
Michael R. Peterson
Michael R. Peterson, Th. Jolicoeur, and S. Das Sarma
Orbital Landau level dependence of the fractional quantum Hall effect in quasi-two dimensional electron layers: finite-thickness effects
27 pages, 20 figures, revised version (with additional author) as accepted for publication in Physical Review B
Phys. Rev. B 78, 155308 (2008)
10.1103/PhysRevB.78.155308
null
cond-mat.mes-hall cond-mat.str-el
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The fractional quantum Hall effect (FQHE) in the second orbital Landau level at filling factor 5/2 remains enigmatic and motivates our work. We consider the effect of the quasi-2D nature of the experimental FQH system on a number of FQH states (fillings 1/3, 1/5, 1/2) in the lowest, second, and third Landau levels (LLL, SLL, TLL,) by calculating the overlap, as a function of quasi-2D layer thickness, between the exact ground state of a model Hamiltonian and the consensus variational wavefunctions (Laughlin wavefunction for 1/3 and 1/5 and the Moore-Read Pfaffian wavefunction for 1/2). Using large overlap as a stability, or FQHE robustness, criterion we find the FQHE does not occur in the TLL (for any thickness), is the most robust for zero thickness in the LLL for 1/3 and 1/5 and for 11/5 in the SLL, and is most robust at finite-thickness (4-5 magnetic lengths) in the SLL for the mysterious 5/2 state and the 7/3 state. No FQHE is found at 1/2 in the LLL for any thickness. We examine the orbital effects of an in-plane (parallel) magnetic field finding its application effectively reduces the thickness and could destroy the FQHE at 5/2 and 7/3, while enhancing it at 11/5 as well as for LLL FQHE states. The in-plane field effects could thus be qualitatively different in the LLL and the SLL by virtue of magneto-orbital coupling through the finite thickness effect. In the torus geometry, we show the appearance of the threefold topological degeneracy expected for the Pfaffian state which is enhanced by thickness corroborating our findings from overlap calculations. Our results have ramifications for wavefunction engineering--the possibility of creating an optimal experimental system where the 5/2 FQHE state is more likely described by the Pfaffian state with applications to topological quantum computing.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 04:33:05 GMT" }, { "version": "v2", "created": "Wed, 10 Sep 2008 18:28:47 GMT" } ]
2009-11-13T00:00:00
[ [ "Peterson", "Michael R.", "" ], [ "Jolicoeur", "Th.", "" ], [ "Sarma", "S. Das", "" ] ]
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801.482
Alexander Bolonkin
Alexander Bolonkin
Cheap Artificial AB-Mountains, Extraction of Water and Energy from Atmosphere and Change of Regional Climate
28 pages, 20 figures, 4 tables. Version 1 is submitted on 31 January 2008, the small corrected version 2 is submitted on 10 May 2008
null
null
null
physics.gen-ph physics.ao-ph physics.soc-ph
null
Author suggests and researches a new revolutionary method for changing the climates of entire countries or portions thereof, obtaining huge amounts of cheap water and energy from the atmosphere. In this paper is presented the idea of cheap artificial inflatable mountains, which may cardinally change the climate of a large region or country. Additional benefits: The potential of tapping large amounts of fresh water and energy. The mountains are inflatable semi-cylindrical constructions from thin film (gas bags) having heights of up to 3 - 5 km. They are located perpendicular to the main wind direction. Encountering these artificial mountains, humid air (wind) rises to crest altitude, is cooled and produces rain (or rain clouds). Many natural mountains are sources of rivers, and other forms of water and power production - and artificial mountains may provide these services for entire nations in the future. The film of these gasbags is supported at altitude by small additional atmospheric overpressure and may be connected to the ground by thin cables. The author has shown (in previous works about the AB-Dome) that this closed AB-Dome allows full control of the weather inside the Dome (the day is always fine, the rain is only at night, no strong winds) and influence to given region. This is a realistic and cheap method of economical irrigation, getting energy and virtual weather control on Earth at the current time.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 04:09:19 GMT" }, { "version": "v2", "created": "Sun, 11 May 2008 00:31:42 GMT" } ]
2008-05-11T00:00:00
[ [ "Bolonkin", "Alexander", "" ] ]
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801.4821
De-Min Li
De-Min Li, Bing Ma
$X(1835)$ and $\eta(1760)$ observed by the BES Collaboration
14 pages, 2 figures, version to appear in Physical Review D
Phys.Rev.D77:074004,2008
10.1103/PhysRevD.77.074004
null
hep-ph
null
With the assumption that the $X(1835)$ and $\eta(1760)$ recently observed by the BES Collaboration are the $3\,^1S_0$ meson states, the strong decays of these two states are investigated in the $^3P_0$ decay model. We find that the predicted total widths of the $X(1835)$ and $\eta(1760)$ can be reasonably reproduced with the $X(18350)-\eta(1760)$ mixing angle lying on the range from $-0.26$ to $+0.55$ radians. Further, the mixing angle of the $X(1835)$ and $\eta(1760)$ is phenomenologically determined to be about $-0.24$ radians in the presence of the $\pi(1800)$, $K(1830)$, $\eta(1760)$ and $X(1835)$ belonging to the $3\,^1S_0$ meson nonet. Our estimated mixing angle can naturally account for the widths of the $X(1835)$ and $\eta(1760)$, which shows that the assignment of the $X(1835)$ and $\eta(1760)$, together the $\pi(1800)$ and $K(1830)$ as the $3\,^1S_0$ $q\bar{q}$ members seems reasonable.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 04:11:41 GMT" }, { "version": "v2", "created": "Thu, 28 Feb 2008 01:12:42 GMT" }, { "version": "v3", "created": "Thu, 3 Apr 2008 02:38:41 GMT" } ]
2008-11-26T00:00:00
[ [ "Li", "De-Min", "" ], [ "Ma", "Bing", "" ] ]
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801.4822
Kelli Talaska
Kelli Talaska
A formula for Pl\"ucker coordinates associated with a planar network
15 pages, 6 figures. Extensive additions, including a generalization for arbitrarily oriented planar graphs and a formula for some Pluecker coordinates of non-planar perfectly oriented graphs
Int Math Res Notices (2008) Vol. 2008, article ID rnn081, 19 pages, published on July 24, 2008.
10.1093/imrn/rnn081
null
math.CO math.RA
null
For a planar directed graph G, Postnikov's boundary measurement map sends positive weight functions on the edges of G onto the appropriate totally nonnegative Grassmann cell. We establish an explicit formula for Postnikov's map by expressing each Pluecker coordinate as a ratio of two combinatorially defined polynomials in the edge weights, with positive integer coefficients. In the non-planar setting, we show that a similar formula holds for special choices of Pluecker coordinates.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 05:07:42 GMT" }, { "version": "v2", "created": "Tue, 15 Apr 2008 00:47:59 GMT" } ]
2008-09-18T00:00:00
[ [ "Talaska", "Kelli", "" ] ]
[ -0.0625336617, -0.0268041007, 0.0949646831, -0.0373095348, -0.0188210793, -0.1215193123, 0.0267625209, -0.0582095236, -0.1249564439, 0.021343492, 0.0373926908, 0.0419940129, 0.0990116298, -0.0363948122, -0.0056546396, -0.039443884, 0.0572670847, -0.0030906484, -0.0216345396, 0.0869262218, -0.0040919911, -0.0020598548, 0.0247806255, 0.0390558206, -0.0078513557, 0.0331517085, 0.0725124329, -0.0375035666, 0.0735103115, -0.0410792939, -0.018987393, -0.0307956096, -0.0287444182, -0.0616466589, -0.0675784871, -0.011413225, -0.0773355141, 0.084431529, -0.0798302069, 0.1547818929, -0.0883676037, 0.0869816616, -0.1154211685, 0.0457914919, 0.0227848701, 0.073011376, -0.025889378, 0.068631798, 0.0022989297, -0.0345930904, -0.0545783602, 0.1592169106, 0.043379955, 0.0217731334, -0.0913612321, -0.0092788758, 0.0443223938, -0.0002492528, 0.017476717, 0.0259863939, 0.0789986402, -0.0592074022, 0.0625891015, 0.0211078823, -0.0560474582, 0.0131179318, -0.117084302, 0.0568235852, 0.0649174824, 0.0199852698, -0.0811607093, 0.1205214337, -0.0341218673, -0.0315717384, -0.0322647095, 0.0360344686, -0.0108449887, 0.1295023263, -0.0225631204, -0.0261388477, 0.0037316463, 0.0302689523, 0.0671904236, -0.0793867037, -0.0572670847, -0.1137580425, -0.0125704855, -0.0431582034, -0.1333829612, 0.0011893107, -0.0143306302, -0.0378916301, -0.0134436283, 0.0687426776, 0.0158135872, 0.0807726458, 0.0658599213, 0.0304907039, -0.0436294228, 0.0545506403, -0.0122932969, -0.090751417, 0.0095560635, -0.0956853703, 0.1283935755, 0.1234041899, 0.063753292, 0.1373744756, -0.021274196, -0.0434631109, -0.0607042201, 0.0350088701, -0.041827701, 0.060149841, 0.0779453218, -0.0506422855, -0.0877023488, -0.1024487615, -0.0578214601, -0.0103945583, -0.0762821957, -0.002681796, 0.1363766044, -0.0908068568, 0.0452925526, 0.0029988301, -0.0369214714, -0.133937344, 0.044987645, -0.0582095236, 0.042603828, -0.0737320632, -0.0055818777, -0.0697405562, -0.0905851051, 0.023616435, 0.0619238466, 0.0342881829, 0.0679111108, 0.0022764083, 0.0172133874, 0.1856052279, -0.0017947936, -0.0105678001, -0.0373095348, 0.049561251, -0.0451262407, -0.0194031745, -0.0199852698, 0.0658599213, -0.0037732245, 0.0383351296, 0.0659153536, 0.0398596637, -0.0555485189, -0.0351751857, 0.0755060688, 0.0513629764, 0.041827701, 0.0326250531, 0.0350643098, 0.0660262331, 0.0547723919, 0.1390376091, 0.0149958823, 0.0218147114, -0.0668577999, -0.0792758316, -0.0079275826, -0.0163679644, -0.0112815602, -0.1303893328, -0.1016726345, -0.0012767982, -0.0114617329, 0.0337892435, -0.0975702479, -0.0338446796, -0.0460963994, -0.0424929522, -0.0305461418, 0.0191398468, 0.0391112566, 0.0108727077, -0.0348702781, 0.1464662552, 0.0488959998, 0.0665251687, -0.0119676013, 0.0123140858, -0.0658599213, 0.0339832753, 0.0441283621, 0.0696296766, -0.0183498599, -0.0561583303, 0.0700731799, -0.0653055459, 0.0346762463, 0.0142890522, -0.0671904236, -0.0195279103, 0.0423266403, 0.0094867665, -0.0777235776, -0.0828792751, 0.101007387, -0.0306570157, -0.0511412248, 0.0068257595, 0.0056373151, -0.0323478654, 0.0384460054, -0.0385291614, -0.0697405562, 0.0131317917, -0.1030031368, 0.0391389765, -0.0356464051, 0.1174169257, -0.1227389425, 0.079164952, -0.0458746478, -0.0254181586, 0.0178232025, 0.0520005077, 0.1545601487, -0.0721798092, -0.0504205339, -0.0042894874, -0.0743973181, -0.0337060876, 0.0172688253, -0.0671349838, 0.0063857236, -0.075450629, -0.0559920184, -0.0218840092, -0.0454865843, -0.0362007804, -0.0490345955, -0.0650283545, -0.0097639551, 0.0092650158, -0.0176014509, 0.000154619, -0.0467616506, -0.047870405, -0.0421603285, -0.0368660316, -0.044072926, 0.0903633535, -0.0018069206, 0.0394161642, -0.0551604554, 0.117860429 ]
801.4823
Yang Sun
Yang Sun, Jing-ye Zhang, Gui-Lu Long, Cheng-Li Wu
Coexistence of normal, super-, and hyper-deformation in nuclei: A study with angular momentum projection
12 pages, 5 figures
null
null
null
nucl-th nucl-ex physics.atm-clus
null
Angular-momentum-projected energy surface calculations for A~110 nuclei indicate three distinct energy minima occurring at different angular-momenta. These correspond to normal, super-, and hyper-deformed shapes coexisting in one nucleus. 110Pd is studied in detail, with a quantitative prediction on super- and hyper-deformed spectra by the Projected Shell Model calculation. It is suggested that several other neighboring nuclei in the A-110 mass region, with the neutron number around 64, also exhibit clear super- and hyper-deformation minima.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 05:15:35 GMT" } ]
2008-02-01T00:00:00
[ [ "Sun", "Yang", "" ], [ "Zhang", "Jing-ye", "" ], [ "Long", "Gui-Lu", "" ], [ "Wu", "Cheng-Li", "" ] ]
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801.4824
Iasson Karafyllis
Iasson Karafyllis and Costas Kravaris
From Continuous-Time Design to Sampled-Data Design of Nonlinear Observers
Submitted for possible publication to IEEE Transactions on Automatic Control
null
null
null
math.OC
null
In this work, a sampled-data nonlinear observer is designed using a continuous-time design coupled with an inter-sample output predictor. The proposed sampled-data observer is a hybrid system. It is shown that under certain conditions, the robustness properties of the continuous-time design are inherited by the sampled-data design, as long as the sampling period is not too large. The approach is applied to linear systems and to triangular globally Lipschitz systems.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 06:06:50 GMT" } ]
2008-02-01T00:00:00
[ [ "Karafyllis", "Iasson", "" ], [ "Kravaris", "Costas", "" ] ]
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801.4825
Cheongho Han
Byeong-Gon Park (KASI) and Cheongho Han (CBNU)
Color-Shift Measurement in Microlensing-Induced Stellar Variation from Future Space-Based Surveys
5 pages and 3 figures
null
10.1086/586880
null
astro-ph
null
If a microlensing event is caused by a star, the event can exhibit change in color due to the light from the lens. In the previous and current lensing surveys, the color shift could not be used to constrain the lens population because the blended light responsible for the color shift is mostly attributed to nearby background stars rather than the lens. However, events to be observed in future space-based surveys do not suffer from blending and thus the color information can be used to constrain lenses. In this paper, we demonstrate the usefulness of future surveys in measuring color shifts. By conducting simulation of galactic lensing events based on the specification of a proposed space-based lensing survey, we estimate that the shift in the color of $R-H$ will be measured at 5$\sigma$ level for $\sim 12%$ of events that occur on source stars with apparent magnitudes brighter than $J=22.5$. Color-shifted events tend to have high magnifications and the lenses will have brightnesses equivalent to those of source stars. The time scales of the color-shifted events tend to be longer than those without color shifts. From the mass distribution of lenses, we find that most of the color-shifted events will be produced by stellar lenses with spectral types down to mid M-type main sequence stars.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 06:56:44 GMT" } ]
2009-11-13T00:00:00
[ [ "Park", "Byeong-Gon", "", "KASI" ], [ "Han", "Cheongho", "", "CBNU" ] ]
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801.4826
Licia Verde
Sabino Matarrese, Licia Verde
The effect of primordial non-Gaussianity on halo bias
4 pages, 3 figures, submitted. Typos fixed, reference added, minor clarifications in the text
Astrophys.J.677:L77-L80,2008
10.1086/587840
null
astro-ph hep-ph
null
It has long been known how to analytically relate the clustering properties of the collapsed structures (halos) to those of the underlying dark matter distribution for Gaussian initial conditions. Here we apply the same approach to physically motivated non-Gaussian models. The techniques we use were developed in the 1980s to deal with the clustering of peaks of non-Gaussian density fields. The description of the clustering of halos for non-Gaussian initial conditions has recently received renewed interest, motivated by the forthcoming large galaxy and cluster surveys. For inflationary-motivated non-Gaussianites, we find an analytic expression for the halo bias as a function of scale, mass and redshift, employing only the approximations of high-peaks and large separations.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 18:34:36 GMT" }, { "version": "v2", "created": "Fri, 15 Feb 2008 17:37:01 GMT" } ]
2010-11-11T00:00:00
[ [ "Matarrese", "Sabino", "" ], [ "Verde", "Licia", "" ] ]
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801.4827
Makiko Yoshida
Makiko Yoshida, Kazuhiro Shimasaku, Masami Ouchi, Kazuhiro Sekiguchi, Hisanori Furusawa, and Sadanori Okamura
The Subaru/XMM-Newton Deep Survey (SXDS) -VII. Clustering Segregation with Ultraviolet and Optical Luminosities of Lyman-Break Galaxies at z~3
16 pages, 15 figures, accepted for publication in ApJ
null
10.1086/586726
null
astro-ph
null
We investigate clustering properties of Lyman-break galaxies (LBGs) at z~3 based on deep multi-waveband imaging data from optical to near-infrared wavelengths in the Subaru/XMM-Newton Deep Field. The LBGs are selected by U-V and V-z' colors in one contiguous area of 561 arcmin^2 down to z'=25.5. We study the dependence of the clustering strength on rest-frame UV and optical magnitudes, which can be indicators of star formation rate and stellar mass, respectively. The correlation length is found to be a strong function of both UV and optical magnitudes with brighter galaxies being more clustered than faint ones in both cases. Furthermore, the correlation length is dependent on a combination of UV and optical magnitudes in the sense that galaxies bright in optical magnitude have large correlation lengths irrespective of UV magnitude, while galaxies faint in optical magnitude have correlation lengths decreasing with decreasing UV brightness. These results suggest that galaxies with large stellar masses always belong to massive halos in which they can have various star formation rates, while galaxies with small stellar masses reside in less massive halos only if they have low star formation rates. There appears to be an upper limit to the stellar mass and the star formation rate which is determined by the mass of hosting dark halos.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 07:04:41 GMT" } ]
2009-11-13T00:00:00
[ [ "Yoshida", "Makiko", "" ], [ "Shimasaku", "Kazuhiro", "" ], [ "Ouchi", "Masami", "" ], [ "Sekiguchi", "Kazuhiro", "" ], [ "Furusawa", "Hisanori", "" ], [ "Okamura", "Sadanori", "" ] ]
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801.4828
Cheongho Han
Cheongho Han
Microlensing Search for Planets with Two Simultaneously Rising Suns
4 pages, 4 figures
null
10.1086/586896
null
astro-ph
null
Among more than 200 extrasolar planet candidates discovered to date, there is no known planet orbiting around normal binary stars. In this paper, we demonstrate that microlensing is a technique that can detect such planets. Microlensing discoveries of these planets are possible because the planet and host binary stars produce perturbations at a common region around center of mass of the binary stars and thus the signatures of both planet and binary can be detected in the light curves of high-magnification microlensing events. The ranges of the planetary and binary separations of systems for optimal detection vary depending on the planet mass. For a Jupiter-mass planet, we find that high detection efficiency is expected for planets located in the range of $\sim$ 1 AU -- 5 AU from the binary stars which are separated by $\sim$ 0.15 AU -- 0.5 AU
[ { "version": "v1", "created": "Thu, 31 Jan 2008 07:06:17 GMT" } ]
2009-11-13T00:00:00
[ [ "Han", "Cheongho", "" ] ]
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801.4829
Francois Limousin
Dorota Gondek-Rosinska (LUTH), Francois Limousin (LUTH)
The final phase of inspiral of strange quark star binaries
null
null
null
null
gr-qc
null
We present calculations of the final phase of inspiral of irrotational strange star binaries. Two types of equation of state at zero temperature are used - the MIT bag model and the Dey et al. 1998 model of strange quark matter. We study the precoalescence stage within the Isenberg-Wilson-Mathews approximation of General Relativity using a multidomain spectral method. The gravitational-radiation driven evolution of the binary system is approximated by a sequence of quasi-equilibrium configurations at a fixed baryon number and with decreasing separation. We find that the innermost stable circular orbit (ISCO) is determined always by an orbital instability for binaries consisting of two stars built predominantly of strange quark matter independently on the total mass of a binary system and compactness parameter of each star. In contrast, for neutron stars described by baryonic equation of state without exotic phases the ISCO is given by the mass-shedding limit. The gravitational wave frequency at the ISCO, which marks the end of the inspiral phase, is always higher than 1.1kHz for equal masses irrotational strange quark stars with the total mass-energy of a binary system greater than $2 M_\odot$. We find that the dependence of the frequency of gravitational waves at the ISCO on the compactness parameter for the equal mass binaries can be described by the same simple analytical formulae for broad ranges of masses independently on a strange star model. Detailed comparisons with binary neutrons star models, as well as with the third order Post-Newtonian point-mass binaries are given. The difference in the phase, for two $1.35 M_\odot$ strange stars, between our numerical results and 3PN is $\sim 40 %$ for the last two orbits of inspiral.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 07:12:14 GMT" } ]
2008-02-01T00:00:00
[ [ "Gondek-Rosinska", "Dorota", "", "LUTH" ], [ "Limousin", "Francois", "", "LUTH" ] ]
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801.483
Philippe-Emmanuel P.-E. Roche
Fr\'ed\'eric Gauthier (NEEL), Philippe-Emmanuel P.-E. Roche (NEEL)
Evidence of a boundary layer instability at very high Rayleigh number
Submitted for publication
Europhysics Letters : Gauthier and Roche, EPL 83:24005 (2008)
10.1209/0295-5075/83/24005
null
cond-mat.other physics.class-ph physics.flu-dyn
null
In 1997, a Rayleigh-B\'enard experiment evidenced a significant increase of the heat transport efficiency for Rayleigh numbers larger than $Ra \sim 10^{12}$ and interpreted this observation as the signature of the Kraichnan's ``Ultime Regime'' of convection. According to Kraichnan's 1962 prediction, the flow boundary layers above the cold and hot plates -in which most of the fluid temperature drop is localized- become unstable for large enough $Ra$ and this instability boosts the heat transport compared to the other turbulent regimes. Using the same convection cell as in the 1997 experiment, we show that the reported heat transport increase is accompanied with enhanced temperature fluctuations of the bottom plate, which was heated at constant power levels. Indeed, for $Ra < 10^{12}$, the bottom plate fluctuations can simply be accounted from those in the bulk of the flow. In particular, they share the same spectral density at low frequencies, as if the bottom plate was following the slow temperature fluctuations of the bulk, modulo a constant temperature drop across the bottom boundary layer. Conversely, to account for the plate's temperature fluctuations at higher $Ra$, we no-longuer can ignore the fluctuations of the temperature drop across the boundary layer. The negative skewness of fluctuations at high $Ra$ supports the picture of a boundary layer instability. These observations provide new evidence that the transition reported in 1997 corresponds to the triggering of the Ultimate Regime of convection.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 07:20:35 GMT" } ]
2012-02-07T00:00:00
[ [ "Gauthier", "Frédéric", "", "NEEL" ], [ "Roche", "Philippe-Emmanuel P. -E.", "", "NEEL" ] ]
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801.4831
Yuriy Kolesnichenko
Ye.S. Avotina, Yu.A. Kolesnichenko, and J.M. van Ruitenbeek
The signature of subsurface Kondo impurities in the local tunnel current
13 pages, 4 figures. To be published in J. Phys.: Cond. Mat
J.Phys.: Cond. Mat., 20, No.11, 115208 (2008)
10.1088/0953-8984/20/11/115208
null
cond-mat.mes-hall cond-mat.str-el
null
The conductance of a tunnel point-contact in an STM-like geometry having a single defect placed below the surface is investigated theoretically. The effect of multiple electron scattering by the defect after reflections by the metal surface is taken into account. In the approximation of s-wave scattering the dependence of the conductance on the applied voltage and the position of the defect is obtained. The results are illustrated for a model s-wave phase shift describing Kondo-resonance scattering. We demonstrate that multiple electron scattering by the magnetic impurity plays a decisive role in the point-contact conductance at voltages near the Kondo resonance. We find that the sign and shape of the Kondo anomaly depends on the position of the defect.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 07:58:14 GMT" } ]
2009-11-13T00:00:00
[ [ "Avotina", "Ye. S.", "" ], [ "Kolesnichenko", "Yu. A.", "" ], [ "van Ruitenbeek", "J. M.", "" ] ]
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801.4832
Daisuke Nakajo
Daisuke Nakajo
A representation formula for indefinite improper affine spheres
null
null
null
null
math.DG
null
We construct a new representation formula for indefinite improper affine spheres in terms of two para-holomorphic functions and study singularities which appear in this representation formula. As a result, it follows that cuspidal cross caps never appear as the singularities on indefinite improper affine spheres and so on. Comparison with other representation formulae are also studied.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 07:47:39 GMT" } ]
2008-02-01T00:00:00
[ [ "Nakajo", "Daisuke", "" ] ]
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801.4833
Joseph Geraci
Joseph Geraci
A BQP-complete problem related to the Ising model partition function via a new connection between quantum circuits and graphs
12 pages, 2 figures
null
10.1007/s11128-008-0084-7
null
quant-ph
null
We present a simple construction that maps quantum circuits to graphs and vice-versa. Inspired by the results of D.A. Lidar linking the Ising partition function with quadratically signed weight enumerators (QWGTs), we also present a BQP-complete problem for the additive approximation of a function over hypergraphs related to the generating function of Eulerian subgraphs for ordinary graphs. We discuss connections with the Ising partition function.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 08:14:57 GMT" }, { "version": "v2", "created": "Fri, 1 Feb 2008 07:08:21 GMT" }, { "version": "v3", "created": "Wed, 2 Apr 2008 18:40:18 GMT" } ]
2009-03-02T00:00:00
[ [ "Geraci", "Joseph", "" ] ]
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801.4834
Daisuke Jido
D. Jido (YITP Kyoto), E.E. Kolomeitsev (Univ. of Minnesota, YITP Kyoto, GSI), H. Nagahiro (RCNP Osaka), S. Hirenzaki (Nara Women's Univ.)
Level crossing of particle-hole and mesonic modes in eta mesic nuclei
22 pages, 12 figures
Nucl.Phys.A811:158-178,2008
10.1016/j.nuclphysa.2008.07.012
YITP-08-4
nucl-th
null
We study eta meson properties in the infinite nuclear matter and in atomic nuclei with an emphasis on effects of the eta coupling to N*(1535)--nucleon-hole modes. The N*(1535) resonance, which dominates the low-energy eta-nucleon scattering, can be seen as a chiral partner of the nucleon. The change of the chiral mass gap between the N* and the nucleon in a nuclear medium has an impact on the properties of the eta-nucleus system. If the N*-nucleon mass gap decreases with a density increase (chiral symmetry restoration) the calculations show the existence of the resonance state at the energy about 60 MeV and two bound eta-nucleus states with the binding energies about -80 MeV. These states can have strong effect on predicted cross sections of the ^12C (gamma,p) ^11B reaction with eta-meson production.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 08:24:12 GMT" } ]
2008-11-26T00:00:00
[ [ "Jido", "D.", "", "YITP Kyoto" ], [ "Kolomeitsev", "E. E.", "", "Univ. of Minnesota, YITP\n Kyoto, GSI" ], [ "Nagahiro", "H.", "", "RCNP Osaka" ], [ "Hirenzaki", "S.", "", "Nara Women's Univ." ] ]
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801.4835
Michael Joswig
Michael Joswig and Katja Kulas
Tropical and Ordinary Convexity Combined
revised proof of Theorem 7; a few more results and references added
null
null
null
math.CO math.AC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A polytrope is a tropical polytope which at the same time is convex in the ordinary sense. A $d$-dimensional polytrope turns out to be a tropical simplex, that is, it is the tropical convex hull of $d+1$ points. This statement is equivalent to the known fact that the Segre product of two full polynomial rings (over some field $K$) has the Gorenstein property if and only if the factors are generated by the same number of indeterminates. The combinatorial types of polytropes up to dimension three are classified.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 08:57:28 GMT" }, { "version": "v2", "created": "Thu, 31 Jan 2008 21:51:41 GMT" }, { "version": "v3", "created": "Tue, 23 Mar 2010 09:07:45 GMT" } ]
2010-03-24T00:00:00
[ [ "Joswig", "Michael", "" ], [ "Kulas", "Katja", "" ] ]
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801.4836
X. L. Lei
X. L. Lei
Low temperature electron-phonon resonance in dc-current-biased two-dimensional electron systems
7 pages, 5 figures, published version
Phys. Rev. B 77, 205309 (2008)
10.1103/PhysRevB.77.205309
null
cond-mat.mes-hall
null
Effects of resonant acoustic phonon scattering on magnetoresistivity are examined in two-dimensional electron systems at low temperatures by using a balance-equation magnetotransport scheme direct controlled by the current. The experimentally observed resonances in linear resistivity are shown to result from the conventional bulk phonon modes in a GaAs-based system, without invoking leaky interface phonons. Due to quick heating of electrons, phonon resonances can be dramatically enhanced by a finite bias current. When the electron drift velocity increases to the speed of sound, additional and prominent phonon resonance peaks begin to emerge. As a result, remarkable resistance oscillation and negative differential resistivity can appear in nonlinear transport in a modest mobility sample at low temperatures, which is in agreement with recent experiments.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:09:53 GMT" }, { "version": "v2", "created": "Tue, 13 May 2008 02:55:57 GMT" } ]
2008-05-13T00:00:00
[ [ "Lei", "X. L.", "" ] ]
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801.4837
Elizaveta Levina
Adam J. Rothman, Peter J. Bickel, Elizaveta Levina, Ji Zhu
Sparse permutation invariant covariance estimation
Published in at http://dx.doi.org/10.1214/08-EJS176 the Electronic Journal of Statistics (http://www.i-journals.org/ejs/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Electronic Journal of Statistics 2008, Vol. 2, 494-515
10.1214/08-EJS176
IMS-EJS-EJS_2008_176
math.ST stat.TH
null
The paper proposes a method for constructing a sparse estimator for the inverse covariance (concentration) matrix in high-dimensional settings. The estimator uses a penalized normal likelihood approach and forces sparsity by using a lasso-type penalty. We establish a rate of convergence in the Frobenius norm as both data dimension $p$ and sample size $n$ are allowed to grow, and show that the rate depends explicitly on how sparse the true concentration matrix is. We also show that a correlation-based version of the method exhibits better rates in the operator norm. We also derive a fast iterative algorithm for computing the estimator, which relies on the popular Cholesky decomposition of the inverse but produces a permutation-invariant estimator. The method is compared to other estimators on simulated data and on a real data example of tumor tissue classification using gene expression data.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:20:06 GMT" }, { "version": "v2", "created": "Thu, 26 Jun 2008 08:35:25 GMT" } ]
2008-06-26T00:00:00
[ [ "Rothman", "Adam J.", "" ], [ "Bickel", "Peter J.", "" ], [ "Levina", "Elizaveta", "" ], [ "Zhu", "Ji", "" ] ]
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801.4838
Alessandro Fiasconaro
Alessandro Fiasconaro, Werner Ebeling, Ewa Gudowska-Nowak
Active Brownian Motion Models and Applications to Ratchets
12 pages, 17 figures
null
10.1140/epjb/e2008-00267-9
null
physics.data-an cond-mat.soft cond-mat.stat-mech
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We give an overview over recent studies on the model of Active Brownian Motion (ABM) coupled to reservoirs providing free energy which may be converted into kinetic energy of motion. First, we present an introduction to a general concept of active Brownian particles which are capable to take up energy from the source and transform part of it in order to perform various activities. In the second part of our presentation we consider applications of ABM to ratchet systems with different forms of differentiable potentials. Both analytical and numerical evaluations are discussed for three cases of sinusoidal, staircase-like and Mateos ratchet potentials, also with the additional loads modeled by tilted potential structure. In addition, stochastic character of the kinetics is investigated by considering perturbation by Gaussian white noise which is shown to be responsible for driving the directionality of the asymptotic flux in the ratchet. This \textit{stochastically driven directionality} effect is visualized as a strong nonmonotonic dependence of the statistics of the right versus left trajectories of motion leading to a net current of particles. Possible applications of the ratchet systems to molecular motors are also briefly discussed
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:30:30 GMT" }, { "version": "v2", "created": "Sun, 29 Jun 2008 14:36:43 GMT" } ]
2009-11-13T00:00:00
[ [ "Fiasconaro", "Alessandro", "" ], [ "Ebeling", "Werner", "" ], [ "Gudowska-Nowak", "Ewa", "" ] ]
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801.4839
Philipp Schmidt-Wellenburg
O. Zimmer, P. Schmidt-Wellenburg, M. Assmann, M. Fertl, J. Klenke, S. Mironov, H.-F. Wirth, B. van den Brandt
Accumulation and extraction of ultracold neutrons from a superfluid helium converter coated with fluorinated grease
11 pages, 6 figures
null
null
null
nucl-ex
null
We report experiments on the production of ultracold neutrons (UCN) in a converter of superfluid helium coated with fluorinated grease. We employed our technique of window-free extraction of accumulated UCN from the helium, in which they were produced by downscattering neutrons of a cold beam from the Munich research reactor. The time constant for UCN passage through the same extraction aperture as in a previous experiment was a factor two shorter, despite a lower mean velocity of the accumulated UCN in the present experiments. A time-of-flight measurement of the cold neutron spectrum incident on the converter allowed us to estimate the multi-phonon contribution to the UCN production. The UCN production rate inferred from two methods agrees with the theoretical expectation.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:34:25 GMT" } ]
2008-02-01T00:00:00
[ [ "Zimmer", "O.", "" ], [ "Schmidt-Wellenburg", "P.", "" ], [ "Assmann", "M.", "" ], [ "Fertl", "M.", "" ], [ "Klenke", "J.", "" ], [ "Mironov", "S.", "" ], [ "Wirth", "H. -F.", "" ], [ "Brandt", "B. van den", "" ] ]
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801.484
Peter Thomas
P. A. Thomas, M. J. Drinkwater, E. Evstigneeva
Formation of ultra-compact dwarf galaxies: tests of the galaxy threshing scenario in Fornax
18 pages, accepted for publication by MNRAS Changes in response to referee's comments: Amended Figure 6 to allow for missing UCDs at large radii Modified discussion
null
10.1111/j.1365-2966.2008.13543.x
null
astro-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper investigates the possibility that UCD galaxies in the Fornax cluster are formed by the threshing of nucleated, early-type dwarf galaxies (hereafter dwarf galaxies). Similar to the results of Cote et al. (2006) for the Virgo cluster, we show that the Fornax Cluster observations are consistent with a single population in which all dwarfs are nucleated, with a ratio of nuclear to total magnitude that varies slowly with magnitude. Importantly, the magnitude distribution of the UCD population is similar to that of the dwarf nuclei in the Fornax cluster. The joint population of UCDs and the dwarfs from which they may originate is modelled and shown to be consistent with an NFW profile with a characteristic radius of 5 kpc. Furthermore, a steady-state dynamical model reproduces the known mass profile of Fornax. However, there are a number of peculiarities in the velocity dispersion data that remain unexplained. The simplest possible threshing model is tested, in which dwarf galaxies move on orbits in a static cluster potential and are threshed if they pass within a radius at which the tidal force from the cluster exceeds the internal gravity at the core of their dark matter halo. This fails to reproduce the observed fraction of UCDs at radii greater than 30 kpc from the core of Fornax.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:42:20 GMT" }, { "version": "v2", "created": "Thu, 12 Jun 2008 16:03:20 GMT" } ]
2009-11-13T00:00:00
[ [ "Thomas", "P. A.", "" ], [ "Drinkwater", "M. J.", "" ], [ "Evstigneeva", "E.", "" ] ]
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801.4841
Mattias Marklund
Vitaly Bychkov, Mikhail Modestov, Mattias Marklund
The Darrieus-Landau instability in fast deflagration and laser ablation
24 pages, 3 figures, version to appear in Physics of Plasmas
null
10.1063/1.2898402
null
physics.plasm-ph
null
The problem of the Darrieus-Landau instability at a discontinuous deflagration front in a compressible flow is solved. Numerous previous attempts to solve this problem suffered from the deficit of boundary conditions. Here, the required additional boundary condition is derived rigorously taking into account the internal structure of the front. The derived condition implies a constant mass flux at the front; it reduces to the classical Darrieus-Landau condition in the limit of an incompressible flow. It is demonstrated that in general the solution to the problem depends on the type of energy source present in the system. In the common case of a strongly localized source, compression effects make the Darrieus-Landau instability considerably weaker. In particular, the Darrieus-Landau instability growth rate is reduced for laser ablation in comparison with the classical incompressible case. The instability disappears completely in the Chapman-Jouguet regime of ultimately fast deflagration.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:38:57 GMT" }, { "version": "v2", "created": "Thu, 6 Mar 2008 14:44:18 GMT" } ]
2009-11-13T00:00:00
[ [ "Bychkov", "Vitaly", "" ], [ "Modestov", "Mikhail", "" ], [ "Marklund", "Mattias", "" ] ]
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801.4842
Nils Manuel Bezares-Roder
Nils M. Bezares-Roder and Heinz Dehnen
Higgs Scalar-Tensor Theory for Gravity and the Flat Rotation Curves of Spiral Galaxies
17 pages, 12 figures
Gen.Rel.Grav.39:1259-1277,2007
10.1007/s10714-007-0449-8
null
gr-qc astro-ph hep-ph
null
The scalar-tensor theory of gravity with the Higgs field as scalar field is presented. For central symmetry it reproduces the empirically measured flat rotation curves of galaxies. We approximate the galaxy by a polytropic gas sphere with the polytropic index $\gamma=2$ and a massive core.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 09:44:31 GMT" } ]
2008-11-26T00:00:00
[ [ "Bezares-Roder", "Nils M.", "" ], [ "Dehnen", "Heinz", "" ] ]
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801.4843
Shin'ichi Nojiri
Shin'ichi Nojiri and Sergei D. Odintsov
Can F(R)-gravity be a viable model: the universal unification scenario for inflation, dark energy and dark matter
LaTeX 17 pages, based on the lectures given at JGRG17 (Nagoya, Japan) and at VI Winter School on Theor.Phys. (Dubna, Russia)
null
null
null
astro-ph gr-qc hep-ph hep-th
null
We review on the viability of $F(R)$-gravity. We show that recent cosmic acceleration, radiation/matter-dominated epoch and inflation could be realized in the framework of $F(R)$-gravity in the unified way. For some classes of $F(R)$-gravity, the correction to the Newton law is extremely small and there is no so-called matter instability (the very heavy positive mass for additional scalar degree of freedom is generated). The reconstruction program in modified gravity is also reviewed and it is demonstrated that {\it any} time-evolution of the universe expansion could be realized in $F(R)$-gravity. Special attention is paid to modified gravity which unifies inflation with cosmic acceleration and passes local tests. It turns out that such a theory may describe also dark matter.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 10:06:30 GMT" } ]
2008-02-01T00:00:00
[ [ "Nojiri", "Shin'ichi", "" ], [ "Odintsov", "Sergei D.", "" ] ]
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801.4844
Gilbert Levitt
Gilbert Levitt
Counting growth types of automorphisms of free groups
final version, to appear in GAFA; proof of 3.1 simplified thanks to the referee
Geom. Funct. Anal. 19 (2009), no. 4, 1119--1146
null
null
math.GR math.GT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Given an automorphism of a free group $F_n$, we consider the following invariants: $e$ is the number of exponential strata (an upper bound for the number of different exponential growth rates of conjugacy classes); $d$ is the maximal degree of polynomial growth of conjugacy classes; $R$ is the rank of the fixed subgroup. We determine precisely which triples $(e,d,R)$ may be realized by an automorphism of $F_n$. In particular, the inequality $e\le (3n-2)/4}$ (due to Levitt-Lustig) always holds. In an appendix, we show that any conjugacy class grows like a polynomial times an exponential under iteration of the automorphism.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 10:13:00 GMT" }, { "version": "v2", "created": "Mon, 6 Oct 2008 12:15:50 GMT" } ]
2019-06-07T00:00:00
[ [ "Levitt", "Gilbert", "" ] ]
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801.4845
Shailesh Vaya
Carlos Brito and Shailesh Vaya
Improved lower bound for deterministic broadcasting in radio networks
13 pages
null
null
null
cs.DM cs.DC
null
We consider the problem of deterministic broadcasting in radio networks when the nodes have limited knowledge about the topology of the network. We show that for every deterministic broadcasting protocol there exists a network, of radius 2, for which the protocol takes at least $\Omega(\sqrt{n}) rounds for completing the broadcast. Our argument can be extended to prove a lower bound of Omega(\sqrt{nD}) rounds for broadcasting in radio networks of radius D. This resolves one of the open problems posed in [29], where in the authors proved a lower bound of $\Omega(n^{1/4}) rounds for broadcasting in constant diameter networks. We prove the new lower $\Omega(\sqrt{n})$ bound for a special family of radius 2 networks. Each network of this family consists of O(\sqrt{n}) components which are connected to each other via only the source node. At the heart of the proof is a novel simulation argument, which essentially says that any arbitrarily complicated strategy of the source node can be simulated by the nodes of the networks, if the source node just transmits partial topological knowledge about some component instead of arbitrary complicated messages. To the best of our knowledge this type of simulation argument is novel and may be useful in further improving the lower bound or may find use in other applications. Keywords: radio networks, deterministic broadcast, lower bound, advice string, simulation, selective families, limited topological knowledge.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 10:27:10 GMT" } ]
2008-02-01T00:00:00
[ [ "Brito", "Carlos", "" ], [ "Vaya", "Shailesh", "" ] ]
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801.4846
Leslie Woodcock PhD
Leslie V. Woodcock
Virial Equation-of-State for Hard Spheres
Hard-sphere fluid: 4 pages 2 tables 2 figures
null
null
null
cond-mat.stat-mech
null
Recent values for virial coefficients up to B12, when expressed in powers of density relative to maximum close packing,lead to a closed equation-of-state for the equilibrium fluid. The series obtained converges for all densities;it becomes negative and diverges to a negative pole at maximum packing. MD data for 64000 spheres in the metastable region shows the virial pressure begins to deviate at the fluid freezing density.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 10:27:14 GMT" }, { "version": "v2", "created": "Fri, 1 Feb 2008 02:23:26 GMT" }, { "version": "v3", "created": "Sat, 2 Feb 2008 03:30:23 GMT" } ]
2008-02-02T00:00:00
[ [ "Woodcock", "Leslie V.", "" ] ]
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801.4847
Daniela Anca Macinic
Anca Daniela Macinic
Cohomology rings and formality properties of nilpotent groups
18 pages
Journal of Pure and Applied Algebra 214 (2010), pp. 1818-1826
null
null
math.AT
null
We introduce partial formality and relate resonance with partial formality properties. For instance, we show that for finitely generated nilpotent groups that are k-formal, the resonance varieties are trivial up to degree k. We also show that the cohomology ring of a nilpotent k-formal group is generated in degree 1, up to degree k+1; this criterion is necessary and sufficient for 2-step nilpotent groups to be k-formal. We compute resonance varieties for Heisenberg-type groups and deduce the degree of partial formality for this class of groups.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 10:56:58 GMT" } ]
2010-04-09T00:00:00
[ [ "Macinic", "Anca Daniela", "" ] ]
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801.4848
Piotr Gawron
P. Gawron, J.A. Miszczak, J. Sladkowski
Noise Effects in Quantum Magic Squares Game
5 figures
Int. J. Quant. Inf, Vol. 6, No. 1 (2008), pp. 667 - 673
10.1142/S0219749908003931
null
quant-ph
null
In the article we analyse how noisiness of quantum channels can influence the magic squares quantum pseudo-telepathy game. We show that the probability of success can be used to determine characteristics of quantum channels. Therefore the game deserves more careful study aiming at its implementation.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 11:26:02 GMT" } ]
2008-09-09T00:00:00
[ [ "Gawron", "P.", "" ], [ "Miszczak", "J. A.", "" ], [ "Sladkowski", "J.", "" ] ]
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801.4849
Adam Gilbertson
A. M. Gilbertson, M. Fearn, J. H. Jefferson, B. N. Murdin, P. D. Buckle, L. F. Cohen
Zero-field spin-splitting and spin lifetime in n-InSb/In1-xAlxSb asymmetric quantum well heterostructures
18 pages 12 figures
null
10.1103/PhysRevB.77.165335
null
cond-mat.mes-hall
null
The spin-orbit (SO) coupling parameters for lowest conduction subband due to structural (SIA) and bulk (BIA) inversion asymmetry are calculated for a range of carrier densities in [001]-grown delta-doped n-type InSb/In1-xAlxSb asymmetric quantum wells using the established 8 band k.p formalism [PRB 59,8 R5312 (1999)]. We present calculations for conditions of zero bias at 10 K. It is shown that both the SIA and BIA parameters scale approximately linearly with carrier density, and exhibit a marked dependence on well width when alloy composition is adjusted to allow maximum upper barrier height for a given well width. In contrast to other material systems the BIA contribution to spin splitting is found to be of significant and comparable value to the SIA mechanism in these structures. We calculate the spin lifetime for spins oriented along [11-0] based on D'yakonov-Perel mechanism using both the theory of Averkiev et al. [J. Phys.:Condens. Matter 14 (2002)] and also the rate of precession of spins about the effective magnetic field, taking into account all three SO couplings, showing good agreement.Spin lifeime for this direction is largest in the narrow wells over the range of moderate carrier densities considered, which is attributed to the reduced magnitude of the k-cubic BIA parameter in narrow wells. The inherently large BIA induced SO coupling in these systems is shown to have considerable effect on the spin lifetime, which exhibits significant reduction in the maximum spin lifetime compared to previous studies which consider systems with relatively weak BIA induced SO coupling. The relaxation rate of spins oriented in the [001] direction is dominated by the k-linear SIA and BIA coupling parameters and at least an order of magnitude greater than in the [11-0] direction.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 11:41:44 GMT" }, { "version": "v2", "created": "Tue, 5 Feb 2008 15:50:53 GMT" } ]
2009-11-13T00:00:00
[ [ "Gilbertson", "A. M.", "" ], [ "Fearn", "M.", "" ], [ "Jefferson", "J. H.", "" ], [ "Murdin", "B. N.", "" ], [ "Buckle", "P. D.", "" ], [ "Cohen", "L. F.", "" ] ]
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801.485
Felipe Barbedo Rizzato
G.I. de Oliveira and F.B. Rizzato
Coherence and incoherence in extended broad band triplet interaction
6 pages, 2 figures
Phys. Rev. E 77, 016607 (2008)
10.1103/PhysRevE.77.016607
null
physics.plasm-ph physics.class-ph
null
In the present analysis we study the transition from coherent to incoherent dynamics in a nonlinear triplet of broad band combs of waves. Expanding the analysis of previous works, this paper investigates what happens when the band of available modes is much larger than that of the initial narrower combs within which the nonlinear interaction is not subjected to selection rules involving wave momenta. Here selection rules are present and active, and we examine how and when coherence can be defined.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 11:52:31 GMT" } ]
2008-02-01T00:00:00
[ [ "de Oliveira", "G. I.", "" ], [ "Rizzato", "F. B.", "" ] ]
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801.4851
Rajgopal Kannan
Costas Busch and Rajgopal Kannan
Bicretieria Optimization in Routing Games
15 pages, submitted to SPAA
null
null
null
cs.GT cs.DS
null
Two important metrics for measuring the quality of routing paths are the maximum edge congestion $C$ and maximum path length $D$. Here, we study bicriteria in routing games where each player $i$ selfishly selects a path that simultaneously minimizes its maximum edge congestion $C_i$ and path length $D_i$. We study the stability and price of anarchy of two bicriteria games: - {\em Max games}, where the social cost is $\max(C,D)$ and the player cost is $\max(C_i, D_i)$. We prove that max games are stable and convergent under best-response dynamics, and that the price of anarchy is bounded above by the maximum path length in the players' strategy sets. We also show that this bound is tight in worst-case scenarios. - {\em Sum games}, where the social cost is $C+D$ and the player cost is $C_i+D_i$. For sum games, we first show the negative result that there are game instances that have no Nash-equilibria. Therefore, we examine an approximate game called the {\em sum-bucket game} that is always convergent (and therefore stable). We show that the price of anarchy in sum-bucket games is bounded above by $C^* \cdot D^* / (C^* + D^*)$ (with a poly-log factor), where $C^*$ and $D^*$ are the optimal coordinated congestion and path length. Thus, the sum-bucket game has typically superior price of anarchy bounds than the max game. In fact, when either $C^*$ or $D^*$ is small (e.g. constant) the social cost of the Nash-equilibria is very close to the coordinated optimal $C^* + D^*$ (within a poly-log factor). We also show that the price of anarchy bound is tight for cases where both $C^*$ and $D^*$ are large.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 19:29:13 GMT" } ]
2008-02-01T00:00:00
[ [ "Busch", "Costas", "" ], [ "Kannan", "Rajgopal", "" ] ]
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801.4852
Enrico Barausse
Enrico Barausse, Thomas P. Sotiriou and John C. Miller
Polytropic spheres in Palatini f(R) gravity
Talk given by EB at the 30th Spanish Relativity Meeting, 10 - 14 September 2007, Tenerife (Spain). Based on arXiv:gr-qc/0703132 and arXiv:0712.1141 [gr-qc]
EAS Publ.Ser.30:189-192,2008
10.1051/eas:0830023
null
gr-qc
null
We examine static spherically symmetric polytropic spheres in Palatini f(R) gravity and show that no regular solutions to the field equations exist for physically relevant cases such as a monatomic isentropic gas or a degenerate electron gas, thus casting doubt on the validity of Palatini f(R) gravity as an alternative to General Relativity.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:00:17 GMT" } ]
2011-08-31T00:00:00
[ [ "Barausse", "Enrico", "" ], [ "Sotiriou", "Thomas P.", "" ], [ "Miller", "John C.", "" ] ]
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801.4853
Vasudevarao Allu
S. Ponnusamy (IIT Madras, India), A. Vasudevarao (IIT Madras, India), and M. Vuorinen (University of Turku, Finland)
Region of Variability for Spirallike Functions with Respect to a Boundary Point
15 pages, 6 figures. To appear in Colloquium Mathematicum
null
null
null
math.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper we determine the region of variability for spirallike funcions with respect to a boundary point. In the final section we graphically illustrate the region of variability for several sets of parameters.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:11:11 GMT" }, { "version": "v2", "created": "Fri, 5 Dec 2008 16:22:39 GMT" }, { "version": "v3", "created": "Sat, 8 Aug 2009 15:56:22 GMT" } ]
2009-08-08T00:00:00
[ [ "Ponnusamy", "S.", "", "IIT Madras, India" ], [ "Vasudevarao", "A.", "", "IIT Madras, India" ], [ "Vuorinen", "M.", "", "University of Turku, Finland" ] ]
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801.4854
Tatyana P. Shestakova
T. P. Shestakova
The Wheeler - DeWitt Quantum Geometrodynamics: its fundamental problems and tendencies of their resolution
8 pages, no figures
Proceedings of Russian summer school-seminar on Gravitation and Cosmology "GRACOS-2007", Kazan (2007) P. 179 - 183
null
null
gr-qc
null
The paper is devoted to fundamental problems of the Wheeler - DeWitt quantum geometrodynamics, which was the first attempt to apply quantum principles to the Universe as a whole. Our purpose is to find out the origin of these problems and follow up their consequences. We start from Dirac generalized Hamiltonian dynamics as a cornerstone on which the Wheeler - DeWitt theory is based. We remind the main statements of the famous DeWitt's paper of 1967 and discuss the flaws of the theory: the well-known problem of time, the problem of Hilbert space and others. In the concluding part of the paper we consider new tendencies and approaches to quantum geometrodynamics appeared in the last decade.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:11:18 GMT" } ]
2008-02-01T00:00:00
[ [ "Shestakova", "T. P.", "" ] ]
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801.4855
Luca Leuzzi
L. Leuzzi, G. Parisi, F. Ricci-Tersenghi and J.J. Ruiz-Lorenzo
Diluted one-dimensional spin glasses with power law decaying interactions
4 pages, 6 figures, 2 tables
Phys. Rev. Lett. 101, 107203 (2008)
10.1103/PhysRevLett.101.107203
null
cond-mat.dis-nn cond-mat.stat-mech
null
We introduce a diluted version of the one dimensional spin-glass model with interactions decaying in probability as an inverse power of the distance. In this model varying the power corresponds to change the dimension in short-range models. The spin-glass phase is studied in and out of the range of validity of the mean-field approximation in order to discriminate between different theories. Since each variable interacts only with a finite number of others the cost for simulating the model is drastically reduced with respect to the fully connected version and larger sizes can be studied. We find both static and dynamic evidence in favor of the so-called replica symmetry breaking theory.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:26:21 GMT" } ]
2009-11-13T00:00:00
[ [ "Leuzzi", "L.", "" ], [ "Parisi", "G.", "" ], [ "Ricci-Tersenghi", "F.", "" ], [ "Ruiz-Lorenzo", "J. J.", "" ] ]
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801.4856
Susanne Viefers
Susanne Viefers
Quantum Hall physics in rotating Bose-Einstein condensates
Topical review; to appear in Journal of Physics: Condensed Matter. 28 pages, 6 figures
J. Phys. - Cond. Mat. 20, 123202 (2008)
10.1088/0953-8984/20/12/123202
OSLO-TP 1-08
cond-mat.mes-hall
null
The close theoretical analogy between the physics of rapidly rotating atomic Bose condensates and the quantum Hall effect (i.e., a two dimensional electron gas in a strong magnetic field) was first pointed out ten years ago. As a consequence of this analogy, a large number of strongly correlated quantum Hall-type states have been predicted to occur in rotating Bose systems, and suggestions have been made how to manipulate and observe their fractional quasiparticle excitations. Due to a very rapid development in experimental techniques over the past years, experiments on BEC now appear to be close to reaching the quantum Hall regime. This paper reviews the theoretical and experimental work done to date in exploring quantum Hall physics in cold bosonic gases. Future perspectives are discussed briefly, in particular the idea of exploiting some of these strongly correlated states in the context of topological quantum computing.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:38:13 GMT" } ]
2009-11-13T00:00:00
[ [ "Viefers", "Susanne", "" ] ]
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801.4857
Ramazan Sever
Sameer M. Ikhdair and Ramazan Sever
Solution of the D-dimensional Klein-Gordon equation with equal scalar and vector ring-shaped pseudoharmonic potential
25 pages
Int. J. Mod. Phys. C 19, 1425(2008)
10.1142/S0129183108012923
null
quant-ph
null
We present the exact solution of the Klein-Gordon equation in D-dimensions in the presence of the noncentral equal scalar and vector pseudoharmonic potential plus the new ring-shaped potential using the Nikiforov-Uvarov method. We obtain the exact bound-state energy levels and the corresponding eigen functions for a spin-zero particles. We also find that the solution for this noncentral ring-shaped pseudoharmonic potential can be reduced to the three-dimensional pseudoharmonic solution once the coupling constant of the noncentral part of the potential becomes zero.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:39:50 GMT" }, { "version": "v2", "created": "Fri, 8 Feb 2008 13:19:34 GMT" }, { "version": "v3", "created": "Thu, 14 Feb 2008 07:16:50 GMT" } ]
2009-11-13T00:00:00
[ [ "Ikhdair", "Sameer M.", "" ], [ "Sever", "Ramazan", "" ] ]
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801.4858
Peter Henseler
P. Henseler and B. Shapiro
Density Correlations in Cold Atomic Gases: Atomic Speckles in the Presence of Disorder
8 pages, 2 figures
Phys. Rev. A 77, 033624 (2008)
10.1103/PhysRevA.77.033624
null
cond-mat.dis-nn cond-mat.mes-hall
null
The phenomenon of random intensity patterns, for waves propagating in the presence of disorder, is well known in optics and in mesoscopic physics. We study this phenomenon for cold atomic gases expanding, by a diffusion process, in a weak random potential. We show that the density-density correlation function of the expanding gas is strongly affected by disorder and we estimate the typical size of a speckle spot, i.e., a region of enhanced or depleted density. Both a Fermi gas and a Bose-Einstein condensate (in a mean field approach) are considered.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 12:43:50 GMT" }, { "version": "v2", "created": "Tue, 25 Mar 2008 09:51:38 GMT" } ]
2009-11-13T00:00:00
[ [ "Henseler", "P.", "" ], [ "Shapiro", "B.", "" ] ]
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801.4859
Naomichi Hatano
Hiroyuki Nishiuchi, Naomichi Hatano and Kenn Kubo
Vortex generation in the RSP game on the triangular lattice
null
Physica A 387 (2008) 1319-1337
10.1016/j.physa.2007.10.032
null
cond-mat.stat-mech
null
A new model of population dynamics on lattices is proposed. The model consists of players on lattice points, each of which plays the RSP game with neighboring players. Each player copies the next hand from the hand of the neighbouring player with the maximum point. The model exhibits a steady pattern with pairs of vortices and sinks on the triangular lattice. It is shown that the stationary vortex is due to the frustrations on the triangular lattice. A frustration is the three-sided situation where each of the three players around a triangle chooses the rock, the scissors and the paper, respectively.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 04:29:26 GMT" } ]
2008-02-01T00:00:00
[ [ "Nishiuchi", "Hiroyuki", "" ], [ "Hatano", "Naomichi", "" ], [ "Kubo", "Kenn", "" ] ]
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801.486
Bal\'azs Kozma
Balazs Kozma and Alain Barrat
Consensus formation on coevolving networks: groups' formation and structure
10 pages, 3 figures,to appear in a special proceedings issue of J. Phys. A covering the "Complex Networks: from Biology to Information Technology" conference (Pula, Italy, 2007)
J. Phys. A: Math. Theor. 41 (2008) 224020.
10.1088/1751-8113/41/22/224020
null
physics.soc-ph
null
We study the effect of adaptivity on a social model of opinion dynamics and consensus formation. We analyze how the adaptivity of the network of contacts between agents to the underlying social dynamics affects the size and topological properties of groups and the convergence time to the stable final state. We find that, while on static networks these properties are determined by percolation phenomena, on adaptive networks the rewiring process leads to different behaviors: Adaptive rewiring fosters group formation by enhancing communication between agents of similar opinion, though it also makes possible the division of clusters. We show how the convergence time is determined by the characteristic time of link rearrangement. We finally investigate how the adaptivity yields nontrivial correlations between the internal topology and the size of the groups of agreeing agents.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:01:57 GMT" } ]
2008-05-23T00:00:00
[ [ "Kozma", "Balazs", "" ], [ "Barrat", "Alain", "" ] ]
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801.4861
Barkov Maxim
Maxim V. Barkov, Serguei S. Komissarov
Magnetic acceleration of ultra-relativistic GRB and AGN jets
4 pages, 3 figures, HEPRO-2007 Dublin
null
10.1142/S0218271808013285
null
astro-ph
null
We present numerical simulations of cold, axisymmetric, magnetically driven relativistic outflows. The outflows are initially sub-Alfv\'enic and Poynting flux-dominated, with total--to--rest-mass energy flux ratio up to $\mu \sim 620$. To study the magnetic acceleration of jets we simulate flows confined within a funnel with rigid wall of prescribed shape, which we take to be $z\propto r^a$ (in cylindrical coordinates, with $a$ ranging from 1 to 2). This allows us to eliminate the numerical dissipative effects induced by a free boundary with an ambient medium. We find that in all cases they converge to a steady state characterized by a spatially extended acceleration region. For the jet solutions the acceleration process is very efficient - on the outermost scale of the simulation more than half of the Poynting flux has been converted into kinetic energy flux, and the terminal Lorentz factor approached its maximum possible value ($\Gamma_\infty \simeq \mu$). The acceleration is accompanied by the collimation of magnetic field lines in excess of that dictated by the funnel shape. The numerical solutions are generally consistent with the semi-analytic self-similar jets solutions and the spatially extended acceleration observed in some astrophysical relativistic jets. In agreement with previous studies we also find that the acceleration is significantly less effective for wind solutions suggesting that pulsar winds may remain Poynting dominated when they reach the termination shock.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 14:48:33 GMT" }, { "version": "v2", "created": "Tue, 15 Apr 2008 11:09:57 GMT" }, { "version": "v3", "created": "Wed, 16 Apr 2008 13:37:52 GMT" } ]
2009-11-13T00:00:00
[ [ "Barkov", "Maxim V.", "" ], [ "Komissarov", "Serguei S.", "" ] ]
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801.4862
Tatiana Shulman
Tatiana Shulman, Victor Shulman
On algebras generated by inner derivations
null
null
null
null
math.OA math.FA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We look for an effective description of the algebra D_{Lie}(X,B) of operators on a bimodule X over an algebra B, generated by inner derivations. It is shown that in some important examples D_{Lie}(X,B) consists of all elementary operators x\to \sum_i a_ixb_i satisfying the conditions $\sum_i a_ib_i = \sum_i b_ia_i = 0. The Banach algebraic versions of these results are also obtained and applied to the description of closed Lie ideals in some Banach algebras, and to the proof of a density theorem for Lie algebras of operators on Hilbert space.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:13:12 GMT" }, { "version": "v2", "created": "Thu, 17 Jul 2008 17:40:37 GMT" } ]
2008-07-17T00:00:00
[ [ "Shulman", "Tatiana", "" ], [ "Shulman", "Victor", "" ] ]
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801.4863
Sandor Frey
S. Frey, K.E. Gabanyi
Potential Targets for ASTRO-G In-Beam Phase-Referencing
3 pages; proceedings of the symposium "Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technology" (ISAS/JAXA, Sagamihara, Japan, 3-7 Dec 2007). Astronomical Society of the Pacific Conference Series, eds. Hagiwara Y., Fomalont E.B., Tsuboi M., Murata Y., in press
null
null
null
astro-ph
null
We show that as many as ~50 quasars with at least mJy-level expected flux density can be pre-selected as potential in-beam phase-reference targets for ASTRO-G. Most of them have never been imaged with VLBI. These sources are located around strong, compact calibrator sources that have correlated flux density >100 mJy on the longest VLBA baselines at 8.4 GHz. All the targets lie within 12' from the respective reference source. The basis of this selection is an efficient method to identify potential weak VLBI target quasars simply using optical and low-resolution radio catalogue data. The sample of these dominantly weak sources offers a good opportunity for a statistical study of their radio structure with unprecedented angular resolution at 8.4 GHz.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:14:37 GMT" } ]
2008-02-01T00:00:00
[ [ "Frey", "S.", "" ], [ "Gabanyi", "K. E.", "" ] ]
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801.4864
Sandor Frey
S. Frey, L.I. Gurvits, A.P. Lobanov, R.T. Schilizzi, Z. Paragi
High-Redshift Quasars at the Highest Resolution: VSOP Results
3 pages; proceedings of the symposium "Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technology" (ISAS/JAXA, Sagamihara, Japan, 3-7 Dec 2007). Astronomical Society of the Pacific Conference Series, eds. Hagiwara Y., Fomalont E.B., Tsuboi M., Murata Y., in press
null
null
null
astro-ph
null
We studied the radio structure of high-redshift (z>3) quasars with VSOP at 1.6 and 5 GHz. These sources are the most distant objects ever observed with Space VLBI, at rest-frame frequencies up to ~25 GHz. Here we give an account of the observations and briefly highlight the most interesting cases and results. These observations allowed us, among other things, to estimate the mass of the central black holes powering these quasars, to identify large misalignments between the milli-arcsecond (mas) and sub-mas scale radio structures, and to detect apparent superluminal motion at sub-mas scale.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:22:01 GMT" } ]
2008-02-01T00:00:00
[ [ "Frey", "S.", "" ], [ "Gurvits", "L. I.", "" ], [ "Lobanov", "A. P.", "" ], [ "Schilizzi", "R. T.", "" ], [ "Paragi", "Z.", "" ] ]
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801.4865
Lawrence M. Widrow
Lawrence M. Widrow
Dynamical Models for Disk Galaxies with Triaxial Halos
23 pages including 9 figures
null
10.1086/587130
null
astro-ph
null
We construct self-consistent dynamical models for disk galaxies with triaxial, cuspy halos. We begin with an equilibrium, axisymmetric, disk-bulge-halo system and apply an artificial acceleration to the halo particles. By design, this acceleration conserves energy and thereby preserving the system's differential energy distribution even as its phase space distribution function is altered. The halo becomes triaxial but its spherically-averaged density profile remains largely unchanged. The final system is in equilibrium, to a very good approximation, so long as the halo's shape changes adiabatically. The disk and bulge are ``live'' while the halo is being deformed; they respond to the changing gravitational potential but also influence the deformation of the halo. We test the hypothesis that halo triaxiality can explain the rotation curves of low surface brightness galaxies by modelling the galaxy F568-3.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 19:28:58 GMT" } ]
2009-11-13T00:00:00
[ [ "Widrow", "Lawrence M.", "" ] ]
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801.4866
Jugal K. Verma
J. K. Verma
Hilbert Coefficients and Depth of the Associated Graded Ring of an Ideal
24 pages, expository paper to appear in Mathematics Student
null
null
null
math.AC math.AG
null
In this expository paper we survey results that relate Hilbert coefficients of an m-primary ideal I in a Cohen-Macaulay local ring (R, m) with depth of the associated graded ring G(I). Several results in this area follow from two theorems of S. Huckaba and T. Marley. These were proved using homological techniques. We provide simple proofs using superficial sequences.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:27:30 GMT" } ]
2008-02-01T00:00:00
[ [ "Verma", "J. K.", "" ] ]
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801.4867
Jonathan Allcock
Jonathan Allcock and Noah Linden
Quantum communication beyond the localization length in disordered spin chains
5 pages, 2 figures
null
10.1103/PhysRevLett.102.110501
null
quant-ph
null
We study the effects of localization on quantum state transfer in spin chains. We show how to use quantum error correction and multiple parallel spin chains to send a qubit with high fidelity over arbitrary distances; in particular distances much greater than the localization length of the chain.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:31:12 GMT" } ]
2009-11-13T00:00:00
[ [ "Allcock", "Jonathan", "" ], [ "Linden", "Noah", "" ] ]
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801.4868
Richard Kerner
Richard Kerner and Salvatore Vitale
Approximate solutions in General Relativity via deformation of embeddings
null
null
null
null
gr-qc
null
A systematic study of deformations of four-dimensional Einsteinian space-times embedded in a pseudo-Euclidean space $E^N$ of higher dimension is presented. Infinitesimal deformations, seen as vector fields in $E^N$, can be divided in two parts, tangent to the embedded hypersurface and orthogonal to it; only the second ones are relevant, the tangent ones being equivalent to coordinate transformations in the embedded manifold. The geometrical quantities can be then expressed in terms of embedding functions $z^A$ and their infinitesimal deformations $v^A z^A \to {\tilde{z}}^A = z^A + \epsilon v^A$. The deformations are called Einsteinian if they keep Einstein equations satisfied up to a given order in $\epsilon$. The system so obtained is then analyzed in particular in the case of the Schwarzschild metric taken as the starting point, and some solutions of the first-order deformation of Einstein's equations are found. We discuss also second and third order deformations leading to wave-like solutions and to the departure from spherical symmetry towards an axial one (the approximate Kerr solution)
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:48:21 GMT" } ]
2008-02-01T00:00:00
[ [ "Kerner", "Richard", "" ], [ "Vitale", "Salvatore", "" ] ]
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801.4869
Kyrill Bugaev
K. A. Bugaev, V. K. Petrov and G. M. Zinovjev
Why Don't We See the Hagedorn Mass Spectrum in the Experiments?
7 pages, 1 figure added, one chaper added, more references included
null
null
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The influence of medium dependent finite width of the QGP bags on their equation of state is analyzed on a basis of an exactly solvable model with the general mass-volume spectrum of these bags. It is arguing that the consistent statistical description of the QGP bags is achieved for the width proportional to the square root of their volume. The model allows us to estimate the minimal value of the QGP bags' width from the new lattice QCD data. The large width of the QGP bags not only explains the observed deficit in the number of hadronic resonances compared to the Hagedorn mass spectrum, but also clarifies the reason why the heavy/ large QGP bags cannot be directly observed in experiments as metastable states in a hadronic phase.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:52:49 GMT" }, { "version": "v2", "created": "Thu, 11 Dec 2008 16:30:47 GMT" } ]
2008-12-11T00:00:00
[ [ "Bugaev", "K. A.", "" ], [ "Petrov", "V. K.", "" ], [ "Zinovjev", "G. M.", "" ] ]
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801.487
Gergely Sz\'ekely
H. Andreka, J. X. Madarasz, I. Nemeti and G. Szekely
Axiomatizing relativistic dynamics without conservation postulates
21 pages, 7 figures
Studia Logica Volume 89, Number 2 (2008), 163-186
10.1007/s11225-008-9125-6
null
math-ph gr-qc math.LO math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A part of relativistic dynamics (or mechanics) is axiomatized by simple and purely geometrical axioms formulated within first-order logic. A geometrical proof of the formula connecting relativistic and rest masses of bodies is presented, leading up to a geometric explanation of Einstein's famous $E=mc^2$. The connection of our geometrical axioms and the usual axioms on the conservation of mass, momentum and four-momentum is also investigated.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 13:57:31 GMT" }, { "version": "v2", "created": "Fri, 25 Jul 2008 10:50:51 GMT" } ]
2012-11-20T00:00:00
[ [ "Andreka", "H.", "" ], [ "Madarasz", "J. X.", "" ], [ "Nemeti", "I.", "" ], [ "Szekely", "G.", "" ] ]
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801.4871
Joachim Kupsch
Joachim Kupsch
Towards the saturation of the Froissart bound
37 pages, minor corrections, added references
null
null
null
math-ph hep-th math.MP
null
It is the aim of this paper to summarize results about the construction of amplitudes, which rigorously satisfy Mandelstam analyticity, crossing symmetry, and (at least partly) the constraints imposed by elastic and inelastic unitarity. The results are discussed under particular emphasis of a strong increase of the absorptive part of the forward amplitude and the saturation of the Froissart bound.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 14:04:24 GMT" }, { "version": "v2", "created": "Fri, 8 Feb 2008 12:19:56 GMT" }, { "version": "v3", "created": "Wed, 27 Feb 2008 19:54:46 GMT" } ]
2008-02-27T00:00:00
[ [ "Kupsch", "Joachim", "" ] ]
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801.4872
Eugen Paal
Eugen Paal and Jyri Virkepu
Note on 2d binary operadic harmonic oscillator
5 pages, LaTex2e, presented at the International Conference "Algebra, Geometry, and Mathematical Physics", Gotheburg, Sweden, October 11-13, 2007
J. Gen Lie Theory Appl. Vol. 2 (2008), 221-225
null
null
math-ph math.MP
null
It is explained how the time evolution of the operadic variables may be introduced. As an example, a 2-dimensional binary operadic Lax representation of the harmonic oscillator is found.
[ { "version": "v1", "created": "Thu, 31 Jan 2008 14:18:16 GMT" } ]
2009-02-01T00:00:00
[ [ "Paal", "Eugen", "" ], [ "Virkepu", "Jyri", "" ] ]
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