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708.2249
The spin structure of the pion
We present the first calculation of the transverse spin structure of the pion in lattice QCD. Our simulations are based on two flavors of non-perturbatively improved Wilson fermions, with pion masses as low as 400 MeV in volumes up to (2.1 fm)^3 and lattice spacings below 0.1 fm. We find a characteristic asymmetry in the spatial distribution of transversely polarized quarks. This asymmetry is very similar in magnitude to the analogous asymmetry we previously obtained for quarks in the nucleon. Our results support the hypothesis that all Boer-Mulders functions are alike.
hep-lat hep-ph
we present the first calculation of the transverse spin structure of the pion in lattice qcd our simulations are based on two flavors of nonperturbatively improved wilson fermions with pion masses as low as 400 mev in volumes up to 21 fm3 and lattice spacings below 01 fm we find a characteristic asymmetry in the spatial distribution of transversely polarized quarks this asymmetry is very similar in magnitude to the analogous asymmetry we previously obtained for quarks in the nucleon our results support the hypothesis that all boermulders functions are alike
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708.225
Lorentz Invariance Violation from String Theory
In this brief, and by no means complete, review I discuss situations in string theory, in which Lorentz Invariance Violation may occur in a way consistent with world-sheet conformal invariance, thereby leading to acceptable, in principle, string backgrounds. In particular, I first discuss spontaneous Lorentz violation in (non supersymmetric) open string field theory. Then, I move onto a discussion of gravity-induced modified dispersion relations in non-critical (Liouville) strings, in the sense of an induced Finsler-like geometry depending on both coordinates and momenta, for string propagation in non-trivial space times (such as D-particle ``foamy situations''). I pay attention to explaining the appearance of bi-metric models from such string theories, which could serve as examples of alternative scenaria to dark matter. Finally, I make some comparisons with similar developments in other contexts, such as critical strings in non-commutative space times, as well as deformed special relativities and theories with reduced Lorentz symmetry, advocated recently, where again Finsler geometry seems to come into play. In this latter respect, I put the emphasis on phenomenology and attempt to answer the question as to whether there is the possibility of experimental disentanglement of the various approaches.
hep-th gr-qc hep-ph
in this brief and by no means complete review i discuss situations in string theory in which lorentz invariance violation may occur in a way consistent with worldsheet conformal invariance thereby leading to acceptable in principle string backgrounds in particular i first discuss spontaneous lorentz violation in non supersymmetric open string field theory then i move onto a discussion of gravityinduced modified dispersion relations in noncritical liouville strings in the sense of an induced finslerlike geometry depending on both coordinates and momenta for string propagation in nontrivial space times such as dparticle foamy situations i pay attention to explaining the appearance of bimetric models from such string theories which could serve as examples of alternative scenaria to dark matter finally i make some comparisons with similar developments in other contexts such as critical strings in noncommutative space times as well as deformed special relativities and theories with reduced lorentz symmetry advocated recently where again finsler geometry seems to come into play in this latter respect i put the emphasis on phenomenology and attempt to answer the question as to whether there is the possibility of experimental disentanglement of the various approaches
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708.2251
First real time detection of Be7 solar neutrinos by Borexino
This paper reports a direct measurement of the Be7 solar neutrino signal rate performed with the Borexino low background liquid scintillator detector. This is the first real-time spectral measurement of sub-MeV solar neutrinos. The result for 0.862 MeV Be7 is 47 +- 7 (stat} +- 12 (sys} counts/(day x 100 ton), consistent with predictions of Standard Solar Models and neutrino oscillations with LMA-MSW parameters.
astro-ph hep-ph nucl-ex
this paper reports a direct measurement of the be7 solar neutrino signal rate performed with the borexino low background liquid scintillator detector this is the first realtime spectral measurement of submev solar neutrinos the result for 0862 mev be7 is 47 7 stat 12 sys countsday x 100 ton consistent with predictions of standard solar models and neutrino oscillations with lmamsw parameters
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708.2252
Focusing and Polarization in Intuitionistic Logic
A focused proof system provides a normal form to cut-free proofs that structures the application of invertible and non-invertible inference rules. The focused proof system of Andreoli for linear logic has been applied to both the proof search and the proof normalization approaches to computation. Various proof systems in literature exhibit characteristics of focusing to one degree or another. We present a new, focused proof system for intuitionistic logic, called LJF, and show how other proof systems can be mapped into the new system by inserting logical connectives that prematurely stop focusing. We also use LJF to design a focused proof system for classical logic. Our approach to the design and analysis of these systems is based on the completeness of focusing in linear logic and on the notion of polarity that appears in Girard's LC and LU proof systems.
cs.LO
a focused proof system provides a normal form to cutfree proofs that structures the application of invertible and noninvertible inference rules the focused proof system of andreoli for linear logic has been applied to both the proof search and the proof normalization approaches to computation various proof systems in literature exhibit characteristics of focusing to one degree or another we present a new focused proof system for intuitionistic logic called ljf and show how other proof systems can be mapped into the new system by inserting logical connectives that prematurely stop focusing we also use ljf to design a focused proof system for classical logic our approach to the design and analysis of these systems is based on the completeness of focusing in linear logic and on the notion of polarity that appears in girards lc and lu proof systems
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708.2253
The Concept of Entropy and its Concavity for a Finite Protein in its Environment: An exact study on a Square Lattice
We consider a general lattice model of a finite protein in its environment and calculate its Boltzmann entropy SB(E) as a function of its energy E in a microcanonical ensemble, and Gibbs entropy SG(E) as a function of its average energy E in a canonical ensemble by exact enumeration on a square lattice. We find that because of the finite size of the protein, (i) the two are very different and SG(E)>SB(E), (ii) SB(E) need not be concave while SG(E) is, and (iii) SG(E) is relevant for experiments but not SB(E), even though SB(E) is conceptually more useful. We discuss the consequences of these differences. The results are general and applicable to all finite systems.
cond-mat.soft cond-mat.other
we consider a general lattice model of a finite protein in its environment and calculate its boltzmann entropy sbe as a function of its energy e in a microcanonical ensemble and gibbs entropy sge as a function of its average energy e in a canonical ensemble by exact enumeration on a square lattice we find that because of the finite size of the protein i the two are very different and sgesbe ii sbe need not be concave while sge is and iii sge is relevant for experiments but not sbe even though sbe is conceptually more useful we discuss the consequences of these differences the results are general and applicable to all finite systems
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708.2254
Effective Field Theory for the Anisotropic Wilson Lattice Action
We construct the effective field theory appropriate for describing the low energy behavior of anisotropic Wilson lattice actions and the O(a) improved variant thereof. We then apply this effective field theory to the hadron spectrum and dispersion relations, focussing on the corrections due to the anisotropy. We point out an important feature of anisotropic lattices regarding the Aoki-regime; for a given set of fermion masses and spatial lattice spacing, if an isotropic action is in the QCD-phase, this does not guarantee that the anisotropic action is outside the Aoki-regime. This may be important in the tuning of bare parameters for anisotropic lattices using domain-wall and overlap fermions as well as Wilson and O(a)-improved Wilson fermions.
hep-lat
we construct the effective field theory appropriate for describing the low energy behavior of anisotropic wilson lattice actions and the oa improved variant thereof we then apply this effective field theory to the hadron spectrum and dispersion relations focussing on the corrections due to the anisotropy we point out an important feature of anisotropic lattices regarding the aokiregime for a given set of fermion masses and spatial lattice spacing if an isotropic action is in the qcdphase this does not guarantee that the anisotropic action is outside the aokiregime this may be important in the tuning of bare parameters for anisotropic lattices using domainwall and overlap fermions as well as wilson and oaimproved wilson fermions
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708.2255
A Language for Generic Programming in the Large
Generic programming is an effective methodology for developing reusable software libraries. Many programming languages provide generics and have features for describing interfaces, but none completely support the idioms used in generic programming. To address this need we developed the language G. The central feature of G is the concept, a mechanism for organizing constraints on generics that is inspired by the needs of modern C++ libraries. G provides modular type checking and separate compilation (even of generics). These characteristics support modular software development, especially the smooth integration of independently developed components. In this article we present the rationale for the design of G and demonstrate the expressiveness of G with two case studies: porting the Standard Template Library and the Boost Graph Library from C++ to G. The design of G shares much in common with the concept extension proposed for the next C++ Standard (the authors participated in its design) but there are important differences described in this article.
cs.PL cs.SE
generic programming is an effective methodology for developing reusable software libraries many programming languages provide generics and have features for describing interfaces but none completely support the idioms used in generic programming to address this need we developed the language g the central feature of g is the concept a mechanism for organizing constraints on generics that is inspired by the needs of modern c libraries g provides modular type checking and separate compilation even of generics these characteristics support modular software development especially the smooth integration of independently developed components in this article we present the rationale for the design of g and demonstrate the expressiveness of g with two case studies porting the standard template library and the boost graph library from c to g the design of g shares much in common with the concept extension proposed for the next c standard the authors participated in its design but there are important differences described in this article
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708.2256
Automorphisms and isomorphisms of Chevalley groups and algebras
An adjoint Chevalley group of rank at least 2 over a rational algebra (or a similar ring), its elementary subgroup, and the corresponding Lie ring have the same automorphism group. These automorphisms are explicitly described.
math.GR math.RA math.RT
an adjoint chevalley group of rank at least 2 over a rational algebra or a similar ring its elementary subgroup and the corresponding lie ring have the same automorphism group these automorphisms are explicitly described
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708.2257
Dynamics of Atom-Field Entanglement from Exact Solutions: Towards Strong Coupling and Non-Markovian Regimes
We examine the dynamics of bipartite entanglement between a two-level atom and the electromagnetic field. We treat the Jaynes-Cummings model with a single field mode and examine in detail the exact time evolution of entanglement, including cases where the atomic state is initially mixed and the atomic transition is detuned from resonance. We then explore the effects of other nearby modes by calculating the exact time evolution of entanglement in more complex systems with two, three, and five field modes. For these cases we can obtain exact solutions which include the strong coupling regimes. Finally, we consider the entanglement of a two-level atom with the infinite collection of modes present in the intracavity field of a Fabre-Perot cavity. In contrast to the usual treatment of atom-field interactions with a continuum of modes using the Born-Markov approximation, our treatment in all cases describes the full non-Markovian dynamics of the atomic subsystem. Only when an analytic expression for the infinite mode case is desired do we need to make a weak coupling assumption which at long times approximates Markovian dynamics.
quant-ph
we examine the dynamics of bipartite entanglement between a twolevel atom and the electromagnetic field we treat the jaynescummings model with a single field mode and examine in detail the exact time evolution of entanglement including cases where the atomic state is initially mixed and the atomic transition is detuned from resonance we then explore the effects of other nearby modes by calculating the exact time evolution of entanglement in more complex systems with two three and five field modes for these cases we can obtain exact solutions which include the strong coupling regimes finally we consider the entanglement of a twolevel atom with the infinite collection of modes present in the intracavity field of a fabreperot cavity in contrast to the usual treatment of atomfield interactions with a continuum of modes using the bornmarkov approximation our treatment in all cases describes the full nonmarkovian dynamics of the atomic subsystem only when an analytic expression for the infinite mode case is desired do we need to make a weak coupling assumption which at long times approximates markovian dynamics
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708.2258
The evolution of cosmological gravitational waves in f(R) gravity
We give a rigorous and mathematically clear presentation of the Covariant and Gauge Invariant theory of gravitational waves in a perturbed Friedmann-Lemaitre-Robertson-Walker universe for Fourth Order Gravity, where the matter is described by a perfect fluid with a barotropic equation of state. As an example of a consistent analysis of tensor perturbations in Fourth Order Gravity, we apply the formalism to a simple background solution of R^n gravity. We obtain the exact solutions of the perturbation equations for scales much bigger than and smaller than the Hubble radius. It is shown that the evolution of tensor modes is highly sensitive to the choice of n and an interesting new feature arises. During the radiation dominated era, their exist a growing tensor perturbation for nearly all choices of n. This occurs even when the background model is undergoing accelerated expansion as opposed to the case of General Relativity. Consequently, cosmological gravitational wave modes can in principle provide a strong constraint on the theory of gravity independent of other cosmological data sets.
gr-qc astro-ph
we give a rigorous and mathematically clear presentation of the covariant and gauge invariant theory of gravitational waves in a perturbed friedmannlemaitrerobertsonwalker universe for fourth order gravity where the matter is described by a perfect fluid with a barotropic equation of state as an example of a consistent analysis of tensor perturbations in fourth order gravity we apply the formalism to a simple background solution of rn gravity we obtain the exact solutions of the perturbation equations for scales much bigger than and smaller than the hubble radius it is shown that the evolution of tensor modes is highly sensitive to the choice of n and an interesting new feature arises during the radiation dominated era their exist a growing tensor perturbation for nearly all choices of n this occurs even when the background model is undergoing accelerated expansion as opposed to the case of general relativity consequently cosmological gravitational wave modes can in principle provide a strong constraint on the theory of gravity independent of other cosmological data sets
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708.2259
Photometric Calibration of the Swift Ultraviolet/Optical Telescope
We present the photometric calibration of the Swift UltraViolet/Optical Telescope (UVOT) which includes: optimum photometric and background apertures, effective area curves, colour transformations, conversion factors for count rates to flux, and the photometric zero points (which are accurate to better than 4 per cent) for each of the seven UVOT broadband filters. The calibration was performed with observations of standard stars and standard star fields that represent a wide range of spectral star types. The calibration results include the position dependent uniformity, and instrument response over the 1600-8000A operational range. Because the UVOT is a photon counting instrument, we also discuss the effect of coincidence loss on the calibration results. We provide practical guidelines for using the calibration in UVOT data analysis. The results presented here supersede previous calibration results.
astro-ph
we present the photometric calibration of the swift ultravioletoptical telescope uvot which includes optimum photometric and background apertures effective area curves colour transformations conversion factors for count rates to flux and the photometric zero points which are accurate to better than 4 per cent for each of the seven uvot broadband filters the calibration was performed with observations of standard stars and standard star fields that represent a wide range of spectral star types the calibration results include the position dependent uniformity and instrument response over the 16008000a operational range because the uvot is a photon counting instrument we also discuss the effect of coincidence loss on the calibration results we provide practical guidelines for using the calibration in uvot data analysis the results presented here supersede previous calibration results
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708.226
A search for B+ --> tau+ nu with Hadronic B tags
We present a search for the decay B^+ --> tau^+ nu using $383 \times 10^{6}}$ BBbar pairs collected at the Upsilon(4S) resonance with the BABAR detector at the SLAC PEP-II B Factory. We select a sample of events with one completely reconstructed tag B in a hadronic decay mode ($B^- \to D^{(*)0} X^-$), and examine the rest of the event to search for a B^+ --> tau^+ nu decay. We identify the tau lepton in the following modes: tau^+ --> e^+ nu nu,tau^+ --> mu^+ nu nu, tau^+ --> pi^+ nu and tau^+ --> pi^+ pi^0 nu. We find a 2.2 sigma excess in data and measure a branching fraction of B(B+ --> tau^+ nu) = (1.8^{+0.9}_{-0.8}(stat.) \pm 0.4(bkg. syst.) \pm 0.2 (other syst.)) \times 10^{4}. We calculate the product of the B meson decay constant f_{B} and |V_{ub}| to be f_{B} |V_{ub}| = (10.1^{+2.3}_{-2.5}(stat.)^{+1.2}_{-1.5}(syst.))\times10^{-4} GeV
hep-ex
we present a search for the decay b tau nu using 383 times 106 bbbar pairs collected at the upsilon4s resonance with the babar detector at the slac pepii b factory we select a sample of events with one completely reconstructed tag b in a hadronic decay mode b to d0 x and examine the rest of the event to search for a b tau nu decay we identify the tau lepton in the following modes tau e nu nutau mu nu nu tau pi nu and tau pi pi0 nu we find a 22 sigma excess in data and measure a branching fraction of bb tau nu 1809_08stat pm 04bkg syst pm 02 other syst times 104 we calculate the product of the b meson decay constant f_b and v_ub to be f_b v_ub 10123_25stat12_15systtimes104 gev
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708.2261
Association of mid-infrared solar plages with Calcium K line emissions and magnetic structures
Solar mid-IR observations in the 8-15 micrometer band continuum with moderate angular resolution (18 arcseconds) reveal the presence of bright structures surrounding sunspots. These plage-like features present good association with calcium CaII K1v plages and active region magnetograms. We describe a new optical setup with reflecting mirrors to produce solar images on the focal plane array of uncooled bolometers of a commercial camera preceded by germanium optics. First observations of a sunspot on September 11, 2006 show a mid-IR continuum plage exhibiting spatial distribution closely associated with CaII K1v line plage and magnetogram structures. The mid-IR continuum bright plage is about 140 K hotter than the neighboring photospheric regions, consistent with hot plasma confined by the magnetic spatial structures in and above the active region
astro-ph
solar midir observations in the 815 micrometer band continuum with moderate angular resolution 18 arcseconds reveal the presence of bright structures surrounding sunspots these plagelike features present good association with calcium caii k1v plages and active region magnetograms we describe a new optical setup with reflecting mirrors to produce solar images on the focal plane array of uncooled bolometers of a commercial camera preceded by germanium optics first observations of a sunspot on september 11 2006 show a midir continuum plage exhibiting spatial distribution closely associated with caii k1v line plage and magnetogram structures the midir continuum bright plage is about 140 k hotter than the neighboring photospheric regions consistent with hot plasma confined by the magnetic spatial structures in and above the active region
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708.2262
Gauge invariance in fractional field theories
The principle of local gauge invariance is applied to fractional wave equations and the interaction term is determined up to order $o(\bar{g})$ in the coupling constant $\bar{g}$. As a first application, based on the Riemann-Liouville fractional derivative definition, the fractional Zeeman effect is used to reproduce the baryon spectrum accurately. The transformation properties of the non relativistic fractional Schr\"odinger-equation under spatial rotations are investigated and an internal fractional spin is deduced.
math-ph math.MP
the principle of local gauge invariance is applied to fractional wave equations and the interaction term is determined up to order obarg in the coupling constant barg as a first application based on the riemannliouville fractional derivative definition the fractional zeeman effect is used to reproduce the baryon spectrum accurately the transformation properties of the non relativistic fractional schrodingerequation under spatial rotations are investigated and an internal fractional spin is deduced
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708.2263
The SN 1987A Link to Others and Gamma-Ray Bursts
Early measurements of SN 1987A can be interpreted in light of a beam/jet (BJ), with a collimation factor >10,000, which impacted polar ejecta (PE) to produce the "Mystery Spot" (MS), ~24 lt-d away. Other details of SN 1987A suggest that it came from a merger of 2 stellar cores of a common envelope (CE) binary, i.e. a "double degenerate" (DD) SN. Even having to penetrate the CE, the BJ may have caused a long-soft (l)GRB upon hitting the PE, thus DD can produce lGRBs. Because DD must be the dominant merger/SN mechanism in elliptical galaxies (EGs), where only short, hard GRBs (sGRBs) have been observed, DD without CE or PE must also produce sGRBs, and thus NS-NS mergers may not make GRBs as we know them, and/or be as common as previously thought. Millisecond pulsars (MSPs) in the non-core-collapsed globular clusters are also 99% DD-formed from WD-WD merger, consistent with their 2.10 ms minimum spin period, the 2.14 ms signal seen from SN 1987A, and sGRBs offset from the centers of EGs. The details of Ia's suggest that these are also DD, and the total thermonuclear disruption paradigm is now in serious doubt as well, a cause for concern in Ia Cosmology, because Ia's will appear to be Ic's when viewed from their DD merger poles, given sufficient matter above that lost to core-collapse. As a DD SN, 1987A appears to be the Rosetta Stone for 99% of SNe, GRBs and MSPs, including all recent nearby SNe except SN 1986J, and the more distant SN 2006gy. There is no need to invent exotica, such as "collapsars," to account for GRBs.
astro-ph
early measurements of sn 1987a can be interpreted in light of a beamjet bj with a collimation factor 10000 which impacted polar ejecta pe to produce the mystery spot ms 24 ltd away other details of sn 1987a suggest that it came from a merger of 2 stellar cores of a common envelope ce binary ie a double degenerate dd sn even having to penetrate the ce the bj may have caused a longsoft lgrb upon hitting the pe thus dd can produce lgrbs because dd must be the dominant mergersn mechanism in elliptical galaxies egs where only short hard grbs sgrbs have been observed dd without ce or pe must also produce sgrbs and thus nsns mergers may not make grbs as we know them andor be as common as previously thought millisecond pulsars msps in the noncorecollapsed globular clusters are also 99 ddformed from wdwd merger consistent with their 210 ms minimum spin period the 214 ms signal seen from sn 1987a and sgrbs offset from the centers of egs the details of ias suggest that these are also dd and the total thermonuclear disruption paradigm is now in serious doubt as well a cause for concern in ia cosmology because ias will appear to be ics when viewed from their dd merger poles given sufficient matter above that lost to corecollapse as a dd sn 1987a appears to be the rosetta stone for 99 of sne grbs and msps including all recent nearby sne except sn 1986j and the more distant sn 2006gy there is no need to invent exotica such as collapsars to account for grbs
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708.2264
Influence of random roughness on the adhesion between metal surfaces due to capillary condensation
The capillary force was measured by atomic force microscopy between a gold coated sphere mounted on a cantilever and gold surfaces with different roughness. For smooth surfaces the capillary adhesive force surpasses in magnitude any dispersion, e.g. van der Waals/Casimir, and/or electrostatic forces. A substantial decrease in the capillary force was observed by increasing the roughness ampltitude a few nanometers between 1-10 nm. From these measurements two limits can be defined: a smooth limit where a closely macroscopic size contact surface interacts through the capillary force, and the rough limit where only a few asperities give a capillary contribution.
cond-mat.mtrl-sci
the capillary force was measured by atomic force microscopy between a gold coated sphere mounted on a cantilever and gold surfaces with different roughness for smooth surfaces the capillary adhesive force surpasses in magnitude any dispersion eg van der waalscasimir andor electrostatic forces a substantial decrease in the capillary force was observed by increasing the roughness ampltitude a few nanometers between 110 nm from these measurements two limits can be defined a smooth limit where a closely macroscopic size contact surface interacts through the capillary force and the rough limit where only a few asperities give a capillary contribution
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708.2265
Solutions of fractional reaction-diffusion equations in terms of Mittag-Leffler functions
This paper deals with the solution of unified fractional reaction-diffusion systems. The results are obtained in compact and elegant forms in terms of Mittag-Leffler functions and generalized Mittag-Leffler functions, which are suitable for numerical computation. On account of the most general character of the derived results, numerous results on fractional reaction, fractional diffusion, and fractional reaction-diffusion problems scattered in the literature, including the recently derived results by the authors for reaction-diffusion models, follow as special cases.
math.CA math-ph math.MP
this paper deals with the solution of unified fractional reactiondiffusion systems the results are obtained in compact and elegant forms in terms of mittagleffler functions and generalized mittagleffler functions which are suitable for numerical computation on account of the most general character of the derived results numerous results on fractional reaction fractional diffusion and fractional reactiondiffusion problems scattered in the literature including the recently derived results by the authors for reactiondiffusion models follow as special cases
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708.2266
The study of a new gerrymandering methodology
This paper is to obtain a simple dividing-diagram of the congressional districts, where the only limit is that each district should contain the same population if possibly. In order to solve this problem, we introduce three different standards of the "simple" shape. The first standard is that the final shape of the congressional districts should be of a simplest figure and we apply a modified "shortest split line algorithm" where the factor of the same population is considered only. The second standard is that the gerrymandering should ensure the integrity of the current administrative area as the convenience for management. Thus we combine the factor of the administrative area with the first standard, and generate an improved model resulting in the new diagram in which the perimeters of the districts are along the boundaries of some current counties. Moreover, the gerrymandering should consider the geographic features.The third standard is introduced to describe this situation. Finally, it can be proved that the difference between the supporting ratio of a certain party in each district and the average supporting ratio of that particular party in the whole state obeys the Chi-square distribution approximately. Consequently, we can obtain an archetypal formula to check whether the gerrymandering we propose is fair.
cs.CY
this paper is to obtain a simple dividingdiagram of the congressional districts where the only limit is that each district should contain the same population if possibly in order to solve this problem we introduce three different standards of the simple shape the first standard is that the final shape of the congressional districts should be of a simplest figure and we apply a modified shortest split line algorithm where the factor of the same population is considered only the second standard is that the gerrymandering should ensure the integrity of the current administrative area as the convenience for management thus we combine the factor of the administrative area with the first standard and generate an improved model resulting in the new diagram in which the perimeters of the districts are along the boundaries of some current counties moreover the gerrymandering should consider the geographic featuresthe third standard is introduced to describe this situation finally it can be proved that the difference between the supporting ratio of a certain party in each district and the average supporting ratio of that particular party in the whole state obeys the chisquare distribution approximately consequently we can obtain an archetypal formula to check whether the gerrymandering we propose is fair
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708.2267
Background Field Equations for the Duality Symmetric String
This paper describes the background field equations for strings in T-duality symmetric formalisms in which the dimension of target space is doubled and the sigma model supplemented with constraints. These are calculated by demanding the vanishing of the beta-functional of the sigma model couplings in the doubled target space. We demonstrate the equivalence with the background field equations of the standard string sigma model.
hep-th
this paper describes the background field equations for strings in tduality symmetric formalisms in which the dimension of target space is doubled and the sigma model supplemented with constraints these are calculated by demanding the vanishing of the betafunctional of the sigma model couplings in the doubled target space we demonstrate the equivalence with the background field equations of the standard string sigma model
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708.2268
Tropical fans and the moduli spaces of tropical curves
We give a rigorous definition of tropical fans (the "local building blocks for tropical varieties") and their morphisms. For such a morphism of tropical fans of the same dimension we show that the number of inverse images (counted with suitable tropical multiplicities) of a point in the target does not depend on the chosen point - a statement that can be viewed as the beginning of a tropical intersection theory. As an application we consider the moduli spaces of rational tropical curves (both abstract and in some R^r) together with the evaluation and forgetful morphisms. Using our results this gives new, easy, and unified proofs of various tropical independence statements, e.g. of the fact that the numbers of rational tropical curves (in any R^r) through given points are independent of the points.
math.AG
we give a rigorous definition of tropical fans the local building blocks for tropical varieties and their morphisms for such a morphism of tropical fans of the same dimension we show that the number of inverse images counted with suitable tropical multiplicities of a point in the target does not depend on the chosen point a statement that can be viewed as the beginning of a tropical intersection theory as an application we consider the moduli spaces of rational tropical curves both abstract and in some rr together with the evaluation and forgetful morphisms using our results this gives new easy and unified proofs of various tropical independence statements eg of the fact that the numbers of rational tropical curves in any rr through given points are independent of the points
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708.2269
Quasi-periodic stability of normally resonant tori
We study quasi-periodic tori under a normal-internal resonance, possibly with multiple eigenvalues. Two non-degeneracy conditions play a role. The first of these generalizes invertibility of the Floquet matrix and prevents drift of the lower dimensional torus. The second condition involves a Kolmogorov-like variation of the internal frequencies and simultaneously versality of the Floquet matrix unfolding. We focus on the reversible setting, but our results carry over to the Hamiltonian and dissipative contexts.
math.DS
we study quasiperiodic tori under a normalinternal resonance possibly with multiple eigenvalues two nondegeneracy conditions play a role the first of these generalizes invertibility of the floquet matrix and prevents drift of the lower dimensional torus the second condition involves a kolmogorovlike variation of the internal frequencies and simultaneously versality of the floquet matrix unfolding we focus on the reversible setting but our results carry over to the hamiltonian and dissipative contexts
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708.227
Capacity of the Degraded Half-Duplex Relay Channel
A discrete memoryless half-duplex relay channel is constructed from a broadcast channel from the source to the relay and destination and a multiple access channel from the source and relay to the destination. When the relay listens, the channel operates in the broadcast mode. The channel switches to the multiple access mode when the relay transmits. If the broadcast component channel is physically degraded, the half-duplex relay channel will also be referred to as physically degraded. The capacity of this degraded half-duplex relay channel is examined. It is shown that the block Markov coding suggested in the seminal paper by Cover and El Gamal can be modified to achieve capacity for the degraded half-duplex relay channel. In the code construction, the listen-transmit schedule of the relay is made to depend on the message to be sent and hence the schedule carries information itself. If the schedule is restricted to be deterministic, it is shown that the capacity can be achieved by a simple management of information flows across the broadcast and multiple access component channels.
cs.IT math.IT
a discrete memoryless halfduplex relay channel is constructed from a broadcast channel from the source to the relay and destination and a multiple access channel from the source and relay to the destination when the relay listens the channel operates in the broadcast mode the channel switches to the multiple access mode when the relay transmits if the broadcast component channel is physically degraded the halfduplex relay channel will also be referred to as physically degraded the capacity of this degraded halfduplex relay channel is examined it is shown that the block markov coding suggested in the seminal paper by cover and el gamal can be modified to achieve capacity for the degraded halfduplex relay channel in the code construction the listentransmit schedule of the relay is made to depend on the message to be sent and hence the schedule carries information itself if the schedule is restricted to be deterministic it is shown that the capacity can be achieved by a simple management of information flows across the broadcast and multiple access component channels
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708.2271
Solution of the equation d/dx(pdu/dx)+qu=cu by a solution of the equation d/dx(pdu/dx)+qu=0
We give a simple solution of the equation d/dx(pdu/dx)+qu=cu whenever a nontrivial solution of d/dx(pdu/dx)+qu=0 is known. The method developed for obtaining this result is based on the theory of pseudoanalytic functions and their relationship with solutions of the stationary two-dimensional Schrodinger equation. The final result, that is the formula for the general solution of the equation d/dx(pdu/dx)+qu=cu has a simple and easily verifiable form.
math-ph math.MP
we give a simple solution of the equation ddxpdudxqucu whenever a nontrivial solution of ddxpdudxqu0 is known the method developed for obtaining this result is based on the theory of pseudoanalytic functions and their relationship with solutions of the stationary twodimensional schrodinger equation the final result that is the formula for the general solution of the equation ddxpdudxqucu has a simple and easily verifiable form
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708.2272
Reflecting magnons
We study the worldsheet reflection matrix of a string attached to a D-brane in $AdS_5 \times S^5$. The D-brane corresponds to a maximal giant graviton and it wraps an $S^3$ inside $S^5$. In the gauge theory, the open string is described by a spin chain with boundaries. We study an open string with a large SO(6) charge, which allows us to focus on one boundary at a time and to define an asymptotic boundary reflection matrix. We consider two cases corresponding to two possible relative orientations for the charges of the giant graviton and the open string. Using the symmetries of the problem we compute the boundary reflection matrix up to a phase. These matrices obey the boundary Yang Baxter equation. A crossing equation is derived for the overall phase. We perform weak coupling computations up to two loops and obtain results that are consistent with integrability. Finally, we determine the phase factor at strong coupling using classical solutions.
hep-th
we study the worldsheet reflection matrix of a string attached to a dbrane in ads_5 times s5 the dbrane corresponds to a maximal giant graviton and it wraps an s3 inside s5 in the gauge theory the open string is described by a spin chain with boundaries we study an open string with a large so6 charge which allows us to focus on one boundary at a time and to define an asymptotic boundary reflection matrix we consider two cases corresponding to two possible relative orientations for the charges of the giant graviton and the open string using the symmetries of the problem we compute the boundary reflection matrix up to a phase these matrices obey the boundary yang baxter equation a crossing equation is derived for the overall phase we perform weak coupling computations up to two loops and obtain results that are consistent with integrability finally we determine the phase factor at strong coupling using classical solutions
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708.2273
Opportunism in Multiuser Relay Channels: Scheduling, Routing and Spectrum Reuse
In order to understand the key merits of multiuser diversity techniques in relay-assisted cellular multihop networks, this paper analyzes the spectral efficiency of opportunistic (i.e., channel-aware) scheduling algorithms over a fading multiuser relay channel with $K$ users in the asymptotic regime of large (but finite) number of users. Using tools from extreme-value theory, we characterize the limiting distribution of spectral efficiency focusing on Type I convergence and utilize it in investigating the large system behavior of the multiuser relay channel as a function of the number of users and physical channel signal-to-noise ratios (SNRs). Our analysis results in very accurate formulas in the large (but finite) $K$ regime, provides insights on the potential performance enhancements from multihop routing and spectrum reuse policies in the presence of multiuser diversity gains from opportunistic scheduling and helps to identify the regimes and conditions in which relay-assisted multiuser communication provides a clear advantage over direct multiuser communication.
cs.IT math.IT
in order to understand the key merits of multiuser diversity techniques in relayassisted cellular multihop networks this paper analyzes the spectral efficiency of opportunistic ie channelaware scheduling algorithms over a fading multiuser relay channel with k users in the asymptotic regime of large but finite number of users using tools from extremevalue theory we characterize the limiting distribution of spectral efficiency focusing on type i convergence and utilize it in investigating the large system behavior of the multiuser relay channel as a function of the number of users and physical channel signaltonoise ratios snrs our analysis results in very accurate formulas in the large but finite k regime provides insights on the potential performance enhancements from multihop routing and spectrum reuse policies in the presence of multiuser diversity gains from opportunistic scheduling and helps to identify the regimes and conditions in which relayassisted multiuser communication provides a clear advantage over direct multiuser communication
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708.2274
The first rotation periods in Praesepe
The cluster Praesepe (age 650 Myr) is an ideal laboratory to study stellar evolution. Specifically, it allows us to trace the long-term decline of rotation and activity on the main-sequence. Here we present rotation periods measured for five stars in Praesepe with masses of 0.1-0.5Ms -- the first rotation periods for members of this cluster. Photometric periodicities were found from two extensive monitoring campaigns, and are confirmed by multiple independent test procedures. We attribute these variations to magnetic spots co-rotating with the objects, thus indicating the rotation period. The five periods, ranging from 5 to 84h, show a clear positive correlation with object mass, a trend which has been reported previously in younger clusters. When comparing with data for F-K stars in the coeval Hyades, we find a dramatic drop in the periods at spectral type K8-M2 (corresponding to 0.4-0.6Ms). A comparison with periods of VLM stars in younger clusters provides a constraint on the spin-down timescale: We find that the exponential rotational braking timescale is clearly longer than 200 Myr, most likely 400-800 Myr. These results are not affected by the small sample size in the rotation periods. Both findings, the steep drop in the period-mass relation and the long spin-down timescale, indicate a substantial change in the angular momentum loss mechanism for very low mass objects, possibly the breakdown of the solar-type (Skumanich) rotational braking. While the physical origin for this behaviour is unclear, we argue that parts of it might be explained by the disappearance of the radiative core and the resulting breakdown of an interface-type dynamo in the VLM regime. Rotational studies in this mass range hold great potential to probe magnetic properties and interior structure of main-sequence stars.
astro-ph
the cluster praesepe age 650 myr is an ideal laboratory to study stellar evolution specifically it allows us to trace the longterm decline of rotation and activity on the mainsequence here we present rotation periods measured for five stars in praesepe with masses of 0105ms the first rotation periods for members of this cluster photometric periodicities were found from two extensive monitoring campaigns and are confirmed by multiple independent test procedures we attribute these variations to magnetic spots corotating with the objects thus indicating the rotation period the five periods ranging from 5 to 84h show a clear positive correlation with object mass a trend which has been reported previously in younger clusters when comparing with data for fk stars in the coeval hyades we find a dramatic drop in the periods at spectral type k8m2 corresponding to 0406ms a comparison with periods of vlm stars in younger clusters provides a constraint on the spindown timescale we find that the exponential rotational braking timescale is clearly longer than 200 myr most likely 400800 myr these results are not affected by the small sample size in the rotation periods both findings the steep drop in the periodmass relation and the long spindown timescale indicate a substantial change in the angular momentum loss mechanism for very low mass objects possibly the breakdown of the solartype skumanich rotational braking while the physical origin for this behaviour is unclear we argue that parts of it might be explained by the disappearance of the radiative core and the resulting breakdown of an interfacetype dynamo in the vlm regime rotational studies in this mass range hold great potential to probe magnetic properties and interior structure of mainsequence stars
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708.2275
Completeness of the classical 2D Ising model and universal quantum computation
We prove that the 2D Ising model is complete in the sense that the partition function of any classical q-state spin model (on an arbitrary graph) can be expressed as a special instance of the partition function of a 2D Ising model with complex inhomogeneous couplings and external fields. In the case where the original model is an Ising or Potts-type model, we find that the corresponding 2D square lattice requires only polynomially more spins w.r.t the original one, and we give a constructive method to map such models to the 2D Ising model. For more general models the overhead in system size may be exponential. The results are established by connecting classical spin models with measurement-based quantum computation and invoking the universality of the 2D cluster states.
quant-ph cond-mat.stat-mech
we prove that the 2d ising model is complete in the sense that the partition function of any classical qstate spin model on an arbitrary graph can be expressed as a special instance of the partition function of a 2d ising model with complex inhomogeneous couplings and external fields in the case where the original model is an ising or pottstype model we find that the corresponding 2d square lattice requires only polynomially more spins wrt the original one and we give a constructive method to map such models to the 2d ising model for more general models the overhead in system size may be exponential the results are established by connecting classical spin models with measurementbased quantum computation and invoking the universality of the 2d cluster states
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708.2276
Heterotic twistor-string theory
We reformulate twistor-string theory as a heterotic string based on a twisted (0,2) model. The path integral localizes on holomorphic maps, while the (0,2) moduli naturally correspond to the states of N=4 super Yang-Mills and conformal supergravity under the Penrose transform. We show how the standard twistor-string formulae of scattering amplitudes as integrals over the space of curves in supertwistor space may be obtained from our model. The corresponding string field theory gives rise to a twistor action for N=4 conformal supergravity coupled to super Yang-Mills. The model helps to explain how the twistor-strings of Witten and Berkovits are related and clarifies various aspects of each of these models.
hep-th
we reformulate twistorstring theory as a heterotic string based on a twisted 02 model the path integral localizes on holomorphic maps while the 02 moduli naturally correspond to the states of n4 super yangmills and conformal supergravity under the penrose transform we show how the standard twistorstring formulae of scattering amplitudes as integrals over the space of curves in supertwistor space may be obtained from our model the corresponding string field theory gives rise to a twistor action for n4 conformal supergravity coupled to super yangmills the model helps to explain how the twistorstrings of witten and berkovits are related and clarifies various aspects of each of these models
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708.2277
A Chandra Observation of Abell 13: Investigating the Origin of the Radio Relic
We present results from the Chandra X-ray observation of Abell 13, a galaxy cluster that contains an unusual noncentral radio source, also known as a radio relic. This is the first pointed X-ray observation of Abell 13, providing a more sensitive study of the properties of the X-ray gas. The X-ray emission from Abell 13 is extended to the northwest of the X-ray peak and shows substructure indicative of a recent merger event. The cluster X-ray emission is centered on the bright galaxy H of Slee et al. 2001. We find no evidence for a cooling flow in the cluster. A knot of excess X-ray emission is coincident with the other bright elliptical galaxy F. This knot of emission has properties similar to the enhanced emission associated with the large galaxies in the Coma cluster. With these Chandra data we are able to compare the properties of the hot X-ray gas with those of the radio relic from VLA data, to study the interaction of the X-ray gas with the radio emitting electrons. Our results suggest that the radio relic is associated with cooler gas in the cluster. We suggest two explanations for the coincidence of the cooler gas and radio source. First, the gas may have been uplifted by the radio relic from the cluster core. Alternatively, the relic and cool gas may have been displaced from the central galaxy during the cluster merger event.
astro-ph
we present results from the chandra xray observation of abell 13 a galaxy cluster that contains an unusual noncentral radio source also known as a radio relic this is the first pointed xray observation of abell 13 providing a more sensitive study of the properties of the xray gas the xray emission from abell 13 is extended to the northwest of the xray peak and shows substructure indicative of a recent merger event the cluster xray emission is centered on the bright galaxy h of slee et al 2001 we find no evidence for a cooling flow in the cluster a knot of excess xray emission is coincident with the other bright elliptical galaxy f this knot of emission has properties similar to the enhanced emission associated with the large galaxies in the coma cluster with these chandra data we are able to compare the properties of the hot xray gas with those of the radio relic from vla data to study the interaction of the xray gas with the radio emitting electrons our results suggest that the radio relic is associated with cooler gas in the cluster we suggest two explanations for the coincidence of the cooler gas and radio source first the gas may have been uplifted by the radio relic from the cluster core alternatively the relic and cool gas may have been displaced from the central galaxy during the cluster merger event
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708.2278
Weighted hyperprojective spaces and homotopy invariance in orbifold cohomology
We show that Chen-Ruan cohomology is a homotopy invariant in certain cases. We introduce the notion of a T-representation homotopy, which is a stringent form of homotopy under which Chen-Ruan cohomology is invariant. We show that while hyperkahler quotients of the cotangent bundle to a complex vector space by a circle S^1 (here termed weighted hyperprojective spaces) are homotopy equivalent to weighted projective spaces, they are not S^1-representation homotopic. Indeed, we show that their Chen-Ruan cohomology rings (over the rationals) are distinct.
math.SG math.DG
we show that chenruan cohomology is a homotopy invariant in certain cases we introduce the notion of a trepresentation homotopy which is a stringent form of homotopy under which chenruan cohomology is invariant we show that while hyperkahler quotients of the cotangent bundle to a complex vector space by a circle s1 here termed weighted hyperprojective spaces are homotopy equivalent to weighted projective spaces they are not s1representation homotopic indeed we show that their chenruan cohomology rings over the rationals are distinct
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708.2279
Relating gravitational wave constraints from primordial nucleosynthesis, pulsar timing, laser interferometers, and the CMB: implications for the early universe
We derive a general master equation relating the gravitational-wave observables r and Omega_gw(f). Here r is the tensor-to-scalar ratio, constrained by cosmic-microwave-background (CMB) experiments; and Omega_gw(f) is the energy spectrum of primordial gravitational-waves, constrained e.g. by pulsar-timing measurements, laser-interferometer experiments, and Big Bang Nucleosynthesis (BBN). Differentiating the master equation yields a new expression for the tilt d(ln Omega_gw(f))/d(ln f). The relationship between r and Omega_gw(f) depends sensitively on the uncertain physics of the early universe, and we show that this uncertainty may be encapsulated (in a model-independent way) by two quantities: w_hat(f) and nt_hat(f), where nt_hat(f) is a certain logarithmic average over nt(k) (the primordial tensor spectral index); and w_hat(f) is a certain logarithmic average over w_tilde(a) (the effective equation-of-state in the early universe, after horizon re-entry). Here the effective equation-of-state parameter w_tilde(a) is a combination of the ordinary equation-of-state parameter w(a) and the bulk viscosity zeta(a). Thus, by comparing constraints on r and Omega_gw(f), one can obtain (remarkably tight) constraints in the [w_hat(f), nt_hat(f)] plane. In particular, this is the best way to constrain (or detect) the presence of a ``stiff'' energy component (with w > 1/3) in the early universe, prior to BBN. Finally, although most of our analysis does not assume inflation, we point out that if CMB experiments detect a non-zero value for r, then we will immediately obtain (as a free by-product) a new upper bound w_hat < 0.55 on the logarithmically averaged effective equation-of-state parameter during the ``primordial dark age'' between the end of inflation and the start of BBN.
astro-ph gr-qc hep-ph hep-th
we derive a general master equation relating the gravitationalwave observables r and omega_gwf here r is the tensortoscalar ratio constrained by cosmicmicrowavebackground cmb experiments and omega_gwf is the energy spectrum of primordial gravitationalwaves constrained eg by pulsartiming measurements laserinterferometer experiments and big bang nucleosynthesis bbn differentiating the master equation yields a new expression for the tilt dln omega_gwfdln f the relationship between r and omega_gwf depends sensitively on the uncertain physics of the early universe and we show that this uncertainty may be encapsulated in a modelindependent way by two quantities w_hatf and nt_hatf where nt_hatf is a certain logarithmic average over ntk the primordial tensor spectral index and w_hatf is a certain logarithmic average over w_tildea the effective equationofstate in the early universe after horizon reentry here the effective equationofstate parameter w_tildea is a combination of the ordinary equationofstate parameter wa and the bulk viscosity zetaa thus by comparing constraints on r and omega_gwf one can obtain remarkably tight constraints in the w_hatf nt_hatf plane in particular this is the best way to constrain or detect the presence of a stiff energy component with w 13 in the early universe prior to bbn finally although most of our analysis does not assume inflation we point out that if cmb experiments detect a nonzero value for r then we will immediately obtain as a free byproduct a new upper bound w_hat 055 on the logarithmically averaged effective equationofstate parameter during the primordial dark age between the end of inflation and the start of bbn
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708.228
Minimal Number of Generators and Minimum Order of a Non-Abelian Group whose Elements Commute with Their Endomorphic Images
A group in which every element commutes with its endomorphic images is called an $E$-group. If $p$ is a prime number, a $p$-group $G$ which is an $E$-group is called a $pE$-group. Every abelian group is obviously an $E$-group. We prove that every 2-generator $E$-group is abelian and that all 3-generator $E$-groups are nilpotent of class at most 2. It is also proved that every infinite 3-generator $E$-group is abelian. We conjecture that every finite 3-generator $E$-group should be abelian. Moreover we show that the minimum order of a non-abelian $pE$-group is $p^8$ for any odd prime number $p$ and this order is $2^7$ for $p=2$. Some of these results are proved for a class wider than the class of $E$-groups.
math.GR
a group in which every element commutes with its endomorphic images is called an egroup if p is a prime number a pgroup g which is an egroup is called a pegroup every abelian group is obviously an egroup we prove that every 2generator egroup is abelian and that all 3generator egroups are nilpotent of class at most 2 it is also proved that every infinite 3generator egroup is abelian we conjecture that every finite 3generator egroup should be abelian moreover we show that the minimum order of a nonabelian pegroup is p8 for any odd prime number p and this order is 27 for p2 some of these results are proved for a class wider than the class of egroups
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708.2281
A lower bound for the number of conjugacy classes of finite groups
In 2000, L. H\'{e}thelyi and B. K\"{u}lshammer proved that if $p$ is a prime number dividing the order of a finite solvable group $G$, then $G$ has at least $2\sqrt{p-1}$ conjugacy classes. In this paper we show that if $p$ is large, the result remains true for arbitrary finite groups.
math.GR
in 2000 l hethelyi and b kulshammer proved that if p is a prime number dividing the order of a finite solvable group g then g has at least 2sqrtp1 conjugacy classes in this paper we show that if p is large the result remains true for arbitrary finite groups
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708.2282
Minimal blocking sets in PG(n,2) and covering groups by subgroups
In this paper we prove that a set of points $B$ of PG(n,2) is a minimal blocking set if and only if $<B>=PG(d,2)$ with $d$ odd and $B$ is a set of $d+2$ points of $PG(d,2)$ no $d+1$ of them in the same hyperplane. As a corollary to the latter result we show that if $G$ is a finite 2-group and $n$ is a positive integer, then $G$ admits a $\mathfrak{C}_{n+1}$-cover if and only if $n$ is even and $G\cong (C_2)^{n}$, where by a $\mathfrak{C}_m$-cover for a group $H$ we mean a set $\mathcal{C}$ of size $m$ of maximal subgroups of $H$ whose set-theoretic union is the whole $H$ and no proper subset of $\mathcal{C}$ has the latter property and the intersection of the maximal subgroups is core-free. Also for all $n<10$ we find all pairs $(m,p)$ ($m>0$ an integer and $p$ a prime number) for which there is a blocking set $B$ of size $n$ in $PG(m,p)$ such that $<B>=PG(m,p)$.
math.GR math.CO
in this paper we prove that a set of points b of pgn2 is a minimal blocking set if and only if bpgd2 with d odd and b is a set of d2 points of pgd2 no d1 of them in the same hyperplane as a corollary to the latter result we show that if g is a finite 2group and n is a positive integer then g admits a mathfrakc_n1cover if and only if n is even and gcong c_2n where by a mathfrakc_mcover for a group h we mean a set mathcalc of size m of maximal subgroups of h whose settheoretic union is the whole h and no proper subset of mathcalc has the latter property and the intersection of the maximal subgroups is corefree also for all n10 we find all pairs mp m0 an integer and p a prime number for which there is a blocking set b of size n in pgmp such that bpgmp
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708.2283
On quasi-Baer rings of Ore extensions
Let $R$ be a ring and $S=R[x;\sigma,\delta]$ its Ore extension. We prove under some conditions that $R$ is a quasi-Baer ring if and only if the Ore extension $R[x;\sigma,\delta]$ is a quasi-Baer ring. Examples are provided to illustrate and delimit our results.
math.RA
let r be a ring and srxsigmadelta its ore extension we prove under some conditions that r is a quasibaer ring if and only if the ore extension rxsigmadelta is a quasibaer ring examples are provided to illustrate and delimit our results
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708.2284
The Role of MHD in the ICM and its Interactions with AGN Outflows
Magnetic fields probably play a central role in the dynamics and thermodynamics of ICMs and their interactions with AGNs, despite the fact that the fields usually contribute relatively little pressure; i.e., the ICM is a ``high-$\beta$'' plasma. More typically, the roles of magnetic fields come through ``microscopic'' influences on charged particle behaviors, and through magnetic tension, which can still be significant in subsonic, high-$\beta$ flows. I briefly review these issues, while exploring the underlying question of using the commonly-applied magnetohydrodynamics model in the ICM when Coulomb scattering mean free paths can sometimes exceed tens of kiloparsecs.
astro-ph
magnetic fields probably play a central role in the dynamics and thermodynamics of icms and their interactions with agns despite the fact that the fields usually contribute relatively little pressure ie the icm is a highbeta plasma more typically the roles of magnetic fields come through microscopic influences on charged particle behaviors and through magnetic tension which can still be significant in subsonic highbeta flows i briefly review these issues while exploring the underlying question of using the commonlyapplied magnetohydrodynamics model in the icm when coulomb scattering mean free paths can sometimes exceed tens of kiloparsecs
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708.2285
Mapping an Island in the Landscape
We provide a complete classification and statistical analysis of all type IIA orientifold compactifications with intersecting D6-branes on the orbifold T^6/Z'_6. The total number of four dimensional N=1 supersymmetric models is found to be O(10^23). After a statistical analysis of the gauge sector properties of all possible solutions, we study three subsets of configurations which contain the chiral matter sector of the standard model, a Pati-Salam or SU(5) GUT model, respectively. We find O(10^15) compactifications with an MSSM and O(10^11) models with a Pati-Salam sector. Along the way we derive an explicit algebraic formulation for the computation of the non-chiral matter spectrum for all Z_N orbifolds.
hep-th hep-ph
we provide a complete classification and statistical analysis of all type iia orientifold compactifications with intersecting d6branes on the orbifold t6z_6 the total number of four dimensional n1 supersymmetric models is found to be o1023 after a statistical analysis of the gauge sector properties of all possible solutions we study three subsets of configurations which contain the chiral matter sector of the standard model a patisalam or su5 gut model respectively we find o1015 compactifications with an mssm and o1011 models with a patisalam sector along the way we derive an explicit algebraic formulation for the computation of the nonchiral matter spectrum for all z_n orbifolds
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708.2286
Effective Spin-1/2 Description of Transverse-Field-Induced Random Fields in Dipolar Spin Glasses with Strong Single-Ion Anisotropy
We present analytical and numerical evidence for the validity of an effective S=1/2 approach to the description of random field generation in S>=1, and especially in an S=1, dipolar spin glass models with strong uniaxial Ising anisotropy and subject to weak external magnetic field Bx transverse to the Ising direction. Explicitely Bx-dependent random fields are shown to naturally emerge in the effective low-energy description of a microscopic S=1 toy model. We discuss our results in relation to recent theoretical studies pertaining to the topic of Bx-induced random fields in the LiHo$_x$Y$_{1-x}$F$_4$ magnetic materials with the Ho$^{3+}$ Ising moments subject to a transverse field. We show that the S_{eff}=1/2 approach is able to capture both the qualitative and quantitative aspects of the physics at small Bx, giving results that agree with those obtained using conventional second order perturbation theory.
cond-mat.dis-nn cond-mat.stat-mech
we present analytical and numerical evidence for the validity of an effective s12 approach to the description of random field generation in s1 and especially in an s1 dipolar spin glass models with strong uniaxial ising anisotropy and subject to weak external magnetic field bx transverse to the ising direction explicitely bxdependent random fields are shown to naturally emerge in the effective lowenergy description of a microscopic s1 toy model we discuss our results in relation to recent theoretical studies pertaining to the topic of bxinduced random fields in the liho_xy_1xf_4 magnetic materials with the ho3 ising moments subject to a transverse field we show that the s_eff12 approach is able to capture both the qualitative and quantitative aspects of the physics at small bx giving results that agree with those obtained using conventional second order perturbation theory
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708.2287
Q7-branes and their coupling to IIB supergravity
We show how, by making use of a new basis of the IIB supergravity axion-dilaton coset, SL(2,R)/SO(2), 7-branes that belong to different conjugacy classes of the duality group SL(2,R) naturally couple to IIB supergravity with appropriate source terms characterized by an SL(2,R) charge matrix Q. The conjugacy classes are determined by the value of the determinant of Q. The (p,q) 7-branes are the branes in the conjugacy class detQ = 0. The 7-branes in the conjugacy class detQ > 0 are labelled by three numbers (p,q,r) which parameterize the matrix Q and will be called Q7-branes. We construct the full bosonic Wess--Zumino term for the Q7-branes. In order to realize a gauge invariant coupling of the Q7-brane to the gauge fields of IIB supergravity it is necessary to introduce an SL(2,R) doublet of two distinct Born--Infeld fields on the Q7-brane world-volume.
hep-th
we show how by making use of a new basis of the iib supergravity axiondilaton coset sl2rso2 7branes that belong to different conjugacy classes of the duality group sl2r naturally couple to iib supergravity with appropriate source terms characterized by an sl2r charge matrix q the conjugacy classes are determined by the value of the determinant of q the pq 7branes are the branes in the conjugacy class detq 0 the 7branes in the conjugacy class detq 0 are labelled by three numbers pqr which parameterize the matrix q and will be called q7branes we construct the full bosonic wesszumino term for the q7branes in order to realize a gauge invariant coupling of the q7brane to the gauge fields of iib supergravity it is necessary to introduce an sl2r doublet of two distinct borninfeld fields on the q7brane worldvolume
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708.2288
Scalar Trefoils
The knot model is extended by assuming that the trefoils are realized as either chiral fermions or as scalar bosons. There are then four scalar trefoils with electric charges (0, -1,2/3,-1/3) that may be classified in the same way as the chiral fermions: as two isotopic doublets where the two doublets have different hypercharge and the two members of the doublets have different t_3. Only the neutral scalar plays the role of the standard Higgs in fixing the mass ratios of the vector bosons, wile the charged scalars, in addition to having the usual electromagnetic interactions of scalar particles, fix the mass spectrum of the fermions. The extended model would suggest a search for the charged scalars.
hep-th
the knot model is extended by assuming that the trefoils are realized as either chiral fermions or as scalar bosons there are then four scalar trefoils with electric charges 0 12313 that may be classified in the same way as the chiral fermions as two isotopic doublets where the two doublets have different hypercharge and the two members of the doublets have different t_3 only the neutral scalar plays the role of the standard higgs in fixing the mass ratios of the vector bosons wile the charged scalars in addition to having the usual electromagnetic interactions of scalar particles fix the mass spectrum of the fermions the extended model would suggest a search for the charged scalars
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708.2289
Definitive Evidence of Interlayer Coupling Between (Ga,Mn)As Layers Separated by a Nonmagnetic Spacer
We have used polarized neutron reflectometry to study the structural and magnetic properties of the individual layers in a series of (Al,Be,Ga)As/(Ga,Mn)As/GaAs/(Ga,Mn)As multilayer samples. Structurally, we observe that the samples are virtually identical except for the GaAs spacer thickness (which varies from 3-12 nm), and confirm that the spacers contain little or no Mn. Magnetically, we observe that for the sample with the thickest spacer layer, modulation doping by the(Al,Be,Ga)As results in (Ga,Mn)As layers with very different temperature dependent magnetizations. However, as the spacer layer thickness is reduced, the temperature dependent magnetizations of the top an bottom (Ga,Mn)As layers become progressively more similar - a trend we find to be independent of the crystallographic direction along which spins are magnetized. These results definitively show that (Ga,Mn)As layers can couple across a non-magnetic spacer, and that such coupling depends on spacer thickness.
cond-mat.mtrl-sci
we have used polarized neutron reflectometry to study the structural and magnetic properties of the individual layers in a series of albegaasgamnasgaasgamnas multilayer samples structurally we observe that the samples are virtually identical except for the gaas spacer thickness which varies from 312 nm and confirm that the spacers contain little or no mn magnetically we observe that for the sample with the thickest spacer layer modulation doping by thealbegaas results in gamnas layers with very different temperature dependent magnetizations however as the spacer layer thickness is reduced the temperature dependent magnetizations of the top an bottom gamnas layers become progressively more similar a trend we find to be independent of the crystallographic direction along which spins are magnetized these results definitively show that gamnas layers can couple across a nonmagnetic spacer and that such coupling depends on spacer thickness
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708.229
MASA's and certain type I closed faces of C*-algebras
A result of Akemann, Anderson, and Pedersen states that if a sequence of pure states of a C*-algebra A approaches infinity in a certain sense, then there is a MASA B such that each of the states has the unique extension property with respect to B. We generalize this in two ways: We prove that B can be required to contain an approximate identity of A, and we show that the discrete space which underlies the result cited can be replaced with a totally disconnected space. We consider two special kinds of type I closed faces, both related to the above, atomic closed faces and closed faces with nearly closed extreme boundary. One specific question is whether an atomic closed face always has an "isolated point". We give a counterexample for this and also show that the answer is yes if the the atomic face has nearly closed extreme boundary. We prove a complement to Glimm's theorem on type I C*-algebras which arises from the theory of type I closed faces. One of our examples is a type I closed face which is isomorphic to a closed face of every non-type I separable C*-algebra and which is not isomorphic to a closed face of any type I C*-algebra.
math.OA
a result of akemann anderson and pedersen states that if a sequence of pure states of a calgebra a approaches infinity in a certain sense then there is a masa b such that each of the states has the unique extension property with respect to b we generalize this in two ways we prove that b can be required to contain an approximate identity of a and we show that the discrete space which underlies the result cited can be replaced with a totally disconnected space we consider two special kinds of type i closed faces both related to the above atomic closed faces and closed faces with nearly closed extreme boundary one specific question is whether an atomic closed face always has an isolated point we give a counterexample for this and also show that the answer is yes if the the atomic face has nearly closed extreme boundary we prove a complement to glimms theorem on type i calgebras which arises from the theory of type i closed faces one of our examples is a type i closed face which is isomorphic to a closed face of every nontype i separable calgebra and which is not isomorphic to a closed face of any type i calgebra
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708.2291
The WEBT Campaign on the Blazar 3C279 in 2006
The quasar 3C279 was the target of an extensive multiwavelength monitoring campaign from January through April 2006, including an optical-IR-radio monitoring campaign by the Whole Earth Blazar Telescope (WEBT) collaboration. In this paper we focus on the results of the WEBT campaign. The source exhibited substantial variability of optical flux and spectral shape, with a characteristic time scale of a few days. The variability patterns throughout the optical BVRI bands were very closely correlated with each other. In intriguing contrast to other (in particular, BL Lac type) blazars, we find a lag of shorter- behind longer-wavelength variability throughout the RVB ranges, with a time delay increasing with increasing frequency. Spectral hardening during flares appears delayed with respect to a rising optical flux. This, in combination with the very steep IR-optical continuum spectral index of ~ 1.5 - 2.0, may indicate a highly oblique magnetic field configuration near the base of the jet. An alternative explanation through a slow (time scale of several days) acceleration mechanism would require an unusually low magnetic field of < 0.2 G, about an order of magnitude lower than inferred from previous analyses of simultaneous SEDs of 3C279 and other FSRQs with similar properties.
astro-ph
the quasar 3c279 was the target of an extensive multiwavelength monitoring campaign from january through april 2006 including an opticalirradio monitoring campaign by the whole earth blazar telescope webt collaboration in this paper we focus on the results of the webt campaign the source exhibited substantial variability of optical flux and spectral shape with a characteristic time scale of a few days the variability patterns throughout the optical bvri bands were very closely correlated with each other in intriguing contrast to other in particular bl lac type blazars we find a lag of shorter behind longerwavelength variability throughout the rvb ranges with a time delay increasing with increasing frequency spectral hardening during flares appears delayed with respect to a rising optical flux this in combination with the very steep iroptical continuum spectral index of 15 20 may indicate a highly oblique magnetic field configuration near the base of the jet an alternative explanation through a slow time scale of several days acceleration mechanism would require an unusually low magnetic field of 02 g about an order of magnitude lower than inferred from previous analyses of simultaneous seds of 3c279 and other fsrqs with similar properties
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708.2292
Multiscale Analysis and Localization of Random Operators
A discussion of the method of multiscale analysis in the study of localization of random operators based on lectures given at \emph{Random Schr\"odinger operators: methods, results, and perspectives}, \'Etats de la recherche, Universit\'e Paris 13, June 2002
math-ph math.MP
a discussion of the method of multiscale analysis in the study of localization of random operators based on lectures given at emphrandom schrodinger operators methods results and perspectives etats de la recherche universite paris 13 june 2002
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708.2293
Localization for a continuum Cantor-Anderson Hamiltonian
We prove localization at the bottom of the spectrum for a random Schr\"odinger operator in the continuum with a single-site potential probability distribution supported by a Cantor set of zero Lebesgue measure. This distribution is too singular to be treated by the usual methods. In particular, an "a priori" Wegner estimate is not available. To prove the result we perform a multiscale analysis following the work of Bourgain and Kenig for the Bernoulli-Anderson Hamiltonian, and obtain the required Wegner estimate scale by scale. To do so, we generalize their argument based on Sperner's Lemma by resorting to the LYM inequality for multisets, and combine it with the concept of scale dependent equivalent classes of configurations introduced by Germinet, Hislop and Klein for the study of Poisson Hamiltonians.
math-ph math.MP
we prove localization at the bottom of the spectrum for a random schrodinger operator in the continuum with a singlesite potential probability distribution supported by a cantor set of zero lebesgue measure this distribution is too singular to be treated by the usual methods in particular an a priori wegner estimate is not available to prove the result we perform a multiscale analysis following the work of bourgain and kenig for the bernoullianderson hamiltonian and obtain the required wegner estimate scale by scale to do so we generalize their argument based on sperners lemma by resorting to the lym inequality for multisets and combine it with the concept of scale dependent equivalent classes of configurations introduced by germinet hislop and klein for the study of poisson hamiltonians
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708.2294
A probabilistic regulatory network for the human immune system
In this paper we made a review of some papers about probabilistic regulatory networks (PRN), in particular we introduce our concept of homomorphisms of PRN with an example of projection of a regulatory network to a smaller one. We apply the model PRN (or Probabilistic Boolean Network) to the immune system, the PRN works with two functions. The model called ""The B/T-cells interaction"" is Boolean, so we are really working with a Probabilistic Boolean Network. Using Markov Chains we determine the state of equilibrium of the immune response.
q-bio.CB q-bio.BM
in this paper we made a review of some papers about probabilistic regulatory networks prn in particular we introduce our concept of homomorphisms of prn with an example of projection of a regulatory network to a smaller one we apply the model prn or probabilistic boolean network to the immune system the prn works with two functions the model called the btcells interaction is boolean so we are really working with a probabilistic boolean network using markov chains we determine the state of equilibrium of the immune response
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708.2295
Product-free subsets of groups, then and now
A subset of a group is product-free if it does not contain elements a, b, c such that ab = c. We review progress on the problem of determining the size of the largest product-free subset of an arbitrary finite group, including a lower bound due to the author, and a recent upper bound due to Gowers. The bound of Gowers is more general; it allows three different sets A, B, C such that one cannot solve ab = c with a in A, b in B, c in C. We exhibit a refinement of the lower bound construction which shows that for this broader question, the bound of Gowers is essentially optimal.
math.GR math.CO
a subset of a group is productfree if it does not contain elements a b c such that ab c we review progress on the problem of determining the size of the largest productfree subset of an arbitrary finite group including a lower bound due to the author and a recent upper bound due to gowers the bound of gowers is more general it allows three different sets a b c such that one cannot solve ab c with a in a b in b c in c we exhibit a refinement of the lower bound construction which shows that for this broader question the bound of gowers is essentially optimal
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708.2296
Linking Jet Emission, X-ray States and Hard X-ray Tails in the Neutron Star X-ray Binary GX 17+2
We present the results from simultaneous radio (Very Large Array) and X-ray (Rossi-X-ray Timing Explorer) observations of the Z-type neutron star X-ray binary GX~17+2. The aim is to assess the coupling between X-ray and radio properties throughout its three rapidly variable X-ray states and during the time-resolved transitions. These observations allow us, for the first time, to investigate quantitatively the possible relations between the radio emission and the presence of the hard X-ray tails and the X-ray state of the source. The observations show: 1) a coupling between the radio jet emission and the X-ray state of the source, i.e. the position in the X-ray hardness-intensity diagram (HID); 2) a coupling between the presence of a hard X-ray tail and the position in the HID, qualitatively similar to that found for the radio emission; 3) an indication for a quantitative positive correlation between the radio flux density and the X-ray flux in the hard-tail power law component; 4) evidence for the formation of a radio jet associated with the Flaring Branch-to-Normal Branch X-ray state transition; 5) that the radio flux density of the newly-formed jet stabilizes when also the normal-branch oscillation (NBO) in the X-ray power spectrum stabilizes its characteristic frequency, suggesting a possible relation between X-ray variability associated to the NBO and the jet formation. We discuss our results in the context of jet models.
astro-ph
we present the results from simultaneous radio very large array and xray rossixray timing explorer observations of the ztype neutron star xray binary gx172 the aim is to assess the coupling between xray and radio properties throughout its three rapidly variable xray states and during the timeresolved transitions these observations allow us for the first time to investigate quantitatively the possible relations between the radio emission and the presence of the hard xray tails and the xray state of the source the observations show 1 a coupling between the radio jet emission and the xray state of the source ie the position in the xray hardnessintensity diagram hid 2 a coupling between the presence of a hard xray tail and the position in the hid qualitatively similar to that found for the radio emission 3 an indication for a quantitative positive correlation between the radio flux density and the xray flux in the hardtail power law component 4 evidence for the formation of a radio jet associated with the flaring branchtonormal branch xray state transition 5 that the radio flux density of the newlyformed jet stabilizes when also the normalbranch oscillation nbo in the xray power spectrum stabilizes its characteristic frequency suggesting a possible relation between xray variability associated to the nbo and the jet formation we discuss our results in the context of jet models
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708.2297
Densities, Parton Distributions, and Measuring the Non-Spherical Shape of the Nucleon
Spin-dependent quark densities, matrix elements of specific density operators in proton states of definite spin-polarization, indicate that the nucleon may harbor an infinite variety of non-spherical shapes. We show that these matrix elements are closely related to specific transverse momentum dependent parton distributions accessible in the angular dependence of the semi-inclusive processes electron plus proton goes to electron plus pion plus anything, and the Drell-Yan reaction proton plus proton goes to a lepton anti-lepton pair plus anything. New measurements or analyses would allow the direct exhibition of the non-spherical nature of the proton.
nucl-th hep-ex hep-ph nucl-ex
spindependent quark densities matrix elements of specific density operators in proton states of definite spinpolarization indicate that the nucleon may harbor an infinite variety of nonspherical shapes we show that these matrix elements are closely related to specific transverse momentum dependent parton distributions accessible in the angular dependence of the semiinclusive processes electron plus proton goes to electron plus pion plus anything and the drellyan reaction proton plus proton goes to a lepton antilepton pair plus anything new measurements or analyses would allow the direct exhibition of the nonspherical nature of the proton
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708.2298
The Number of Different Binary Functions Generated by NK-Kauffman Networks and the Emergence of Genetic Robustness
We determine the average number $ \vartheta (N, K) $, of \textit{NK}-Kauffman networks that give rise to the same binary function. We show that, for $ N \gg 1 $, there exists a connectivity critical value $ K_c $ such that $ \vartheta(N,K) \approx e^{\phi N} $ ($ \phi > 0 $) for $ K < K_c $ and $\vartheta(N,K) \approx 1 $ for $ K > K_c $. We find that $ K_c $ is not a constant, but scales very slowly with $ N $, as $ K_c \approx \log_2 \log_2 (2N / \ln 2) $. The problem of genetic robustness emerges as a statistical property of the ensemble of \textit{NK}-Kauffman networks and impose tight constraints in the average number of epistatic interactions that the genotype-phenotype map can have.
nlin.AO nlin.CD
we determine the average number vartheta n k of textitnkkauffman networks that give rise to the same binary function we show that for n gg 1 there exists a connectivity critical value k_c such that varthetank approx ephi n phi 0 for k k_c and varthetank approx 1 for k k_c we find that k_c is not a constant but scales very slowly with n as k_c approx log_2 log_2 2n ln 2 the problem of genetic robustness emerges as a statistical property of the ensemble of textitnkkauffman networks and impose tight constraints in the average number of epistatic interactions that the genotypephenotype map can have
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708.2299
Global well-posedness for the radial defocusing cubic wave equation on $\mathbb{R}^{3}$ and for rough data
We prove global well-posedness for the $3D$ radial defocusing cubic wave equation with data in $H^{s} \times H^{s-1}$, $1>s>{7/10}$.
math.AP math-ph math.MP
we prove global wellposedness for the 3d radial defocusing cubic wave equation with data in hs times hs1 1s710
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708.23
Observation of Ferromagnetic Clusters in Bi0.125Ca0.875MnO3
The electron doped manganite system, Bi0.125Ca0.875MnO3, exhibits large bulk magnetization of unknown origin. To select amongst possible magnetic ordering models, we have conducted temperature and magnetic field dependent small-angle neutron scattering measurements. Nontrivial spin structure has been revealed. Ferromagnetic spin clusters form in the antiferromagnetic background when temperature is decreased to Tc~108K. With a further reduction in temperature or the application of external magnetic field, the clusters begin to form in larger numbers, which gives an overall enhancement of magnetization below Tc.
cond-mat.mtrl-sci
the electron doped manganite system bi0125ca0875mno3 exhibits large bulk magnetization of unknown origin to select amongst possible magnetic ordering models we have conducted temperature and magnetic field dependent smallangle neutron scattering measurements nontrivial spin structure has been revealed ferromagnetic spin clusters form in the antiferromagnetic background when temperature is decreased to tc108k with a further reduction in temperature or the application of external magnetic field the clusters begin to form in larger numbers which gives an overall enhancement of magnetization below tc
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708.2301
Ti-rich and Cu-poor grain-boundary layers of CaCu$_3$Ti$_4$O$_{12}$ detected by x-ray photoelectron spectroscopy
Cleaved and polished surfaces of CaCu$_3$Ti$_4$O$_{12}$ ceramics have been investigated by x-ray photoelectron spectroscopy (XPS) and energy dispersive x-ray spectroscopy (EDX), respectively. While EDX technique shows the identical CaCu$_3$Ti$_4$O$_{12}$ stoichiometry for the two surfaces, XPS indicates that the cleaved surface with grain-boundary layers is remarkably Ti-rich and Cu-poor. The core-level spectrum of Cu 2$p$ unambiguously shows the existence of monovalent copper only for the cleaved surface. Possible grain-boundary structure and its formation are discussed.
cond-mat.mtrl-sci cond-mat.other
cleaved and polished surfaces of cacu_3ti_4o_12 ceramics have been investigated by xray photoelectron spectroscopy xps and energy dispersive xray spectroscopy edx respectively while edx technique shows the identical cacu_3ti_4o_12 stoichiometry for the two surfaces xps indicates that the cleaved surface with grainboundary layers is remarkably tirich and cupoor the corelevel spectrum of cu 2p unambiguously shows the existence of monovalent copper only for the cleaved surface possible grainboundary structure and its formation are discussed
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708.2302
Nondestructive interaction-free atom-photon controlled-NOT gate
We present a probabilistic (ideally 50%) nondestructive interaction-free atom-photon controlled-NOT gate, where nondestructive means that all four outgoing target photon modes of the gate are available and feed-forwardable. Individual atoms are controlled by a stimulated Raman adiabatic passage transition and photons by a ring resonator with two outgoing ports. Realistic estimates we obtain for ions confined in a Paul trap around which the resonator is mounted show that a strong atom-photon coupling can be achieved. It is also shown how the resonator can be used for controlling superposition of atom states.
quant-ph
we present a probabilistic ideally 50 nondestructive interactionfree atomphoton controllednot gate where nondestructive means that all four outgoing target photon modes of the gate are available and feedforwardable individual atoms are controlled by a stimulated raman adiabatic passage transition and photons by a ring resonator with two outgoing ports realistic estimates we obtain for ions confined in a paul trap around which the resonator is mounted show that a strong atomphoton coupling can be achieved it is also shown how the resonator can be used for controlling superposition of atom states
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708.2303
Compositional Semantics Grounded in Commonsense Metaphysics
We argue for a compositional semantics grounded in a strongly typed ontology that reflects our commonsense view of the world and the way we talk about it in ordinary language. Assuming the existence of such a structure, we show that the semantics of various natural language phenomena may become nearly trivial.
cs.AI cs.CL
we argue for a compositional semantics grounded in a strongly typed ontology that reflects our commonsense view of the world and the way we talk about it in ordinary language assuming the existence of such a structure we show that the semantics of various natural language phenomena may become nearly trivial
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708.2304
Inverse problems for linear forms over finite sets of integers
Let f(x_1,x_2,...,x_m) = u_1x_1+u_2 x_2+... + u_mx_m be a linear form with positive integer coefficients, and let N_f(k) = min{|f(A)| : A \subseteq Z and |A|=k}. A minimizing k-set for f is a set A such that |A|=k and |f(A)| = N_f(k). A finite sequence (u_1, u_2,...,u_m) of positive integers is called complete if {\sum_{j\in J} u_j : J \subseteq {1,2,..,m}} = {0,1,2,..., U}, where $U = \sum_{j=1}^m u_j.$ It is proved that if f is an m-ary linear form whose coefficient sequence (u_1,...,u_m) is complete, then N_f(k) = Uk-U+1 and the minimizing k-sets are precisely the arithmetic progressions of length k. Other extremal results on linear forms over finite sets of integers are obtained.
math.NT math.CO
let fx_1x_2x_m u_1x_1u_2 x_2 u_mx_m be a linear form with positive integer coefficients and let n_fk minfa a subseteq z and ak a minimizing kset for f is a set a such that ak and fa n_fk a finite sequence u_1 u_2u_m of positive integers is called complete if sum_jin j u_j j subseteq 12m 012 u where u sum_j1m u_j it is proved that if f is an mary linear form whose coefficient sequence u_1u_m is complete then n_fk uku1 and the minimizing ksets are precisely the arithmetic progressions of length k other extremal results on linear forms over finite sets of integers are obtained
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708.2305
Abnormal Electronic Transport in Disordered Graphene Nanoribbon
We investigate the conductivity $\sigma$ of graphene nanoribbons with zigzag edges as a function of Fermi energy $E_F$ in the presence of the impurities with different potential range. The dependence of $\sigma(E_F)$ displays four different types of behavior, classified to different regimes of length scales decided by the impurity potential range and its density. Particularly, low density of long range impurities results in an extremely low conductance compared to the ballistic value, a linear dependence of $\sigma(E_F)$ and a wide dip near the Dirac point, due to the special properties of long range potential and edge states. These behaviors agree well with the results from a recent experiment by Miao \emph{et al.} (to appear in Science).
cond-mat.mes-hall cond-mat.dis-nn
we investigate the conductivity sigma of graphene nanoribbons with zigzag edges as a function of fermi energy e_f in the presence of the impurities with different potential range the dependence of sigmae_f displays four different types of behavior classified to different regimes of length scales decided by the impurity potential range and its density particularly low density of long range impurities results in an extremely low conductance compared to the ballistic value a linear dependence of sigmae_f and a wide dip near the dirac point due to the special properties of long range potential and edge states these behaviors agree well with the results from a recent experiment by miao emphet al to appear in science
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708.2306
Effects of impurities on Tamm-like lanthanide-metal surface states
The effects of isolated residual-gas adsorbates on the local electronic structure of the Dy(0001) surface were spatially mapped by scanning tunneling microscopy and spectroscopy at 12 K. Less than 15 A away from an adsorbate, a strong reduction of the intensity and a significant increase of the width of the majority component of the surface state due to impurity scattering were observed, with essentially no change of the minority component; this reflects a high lateral localization of the Tamm-like surface state. Furthermore, an adsorbate-induced state was found that behaves metastable.
cond-mat.mtrl-sci
the effects of isolated residualgas adsorbates on the local electronic structure of the dy0001 surface were spatially mapped by scanning tunneling microscopy and spectroscopy at 12 k less than 15 a away from an adsorbate a strong reduction of the intensity and a significant increase of the width of the majority component of the surface state due to impurity scattering were observed with essentially no change of the minority component this reflects a high lateral localization of the tammlike surface state furthermore an adsorbateinduced state was found that behaves metastable
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708.2307
Small value estimates for the additive group
We generalize Gel'fond's criterion of algebraic independence to the context of a sequence of polynomials whose first derivatives take small values on large subsets of a fixed subgroup of the additive group of complex numbers, instead of just one point. We also provide one extension dealing with a subgroup of the multiplicative group of non-zero complex numbers.
math.NT
we generalize gelfonds criterion of algebraic independence to the context of a sequence of polynomials whose first derivatives take small values on large subsets of a fixed subgroup of the additive group of complex numbers instead of just one point we also provide one extension dealing with a subgroup of the multiplicative group of nonzero complex numbers
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708.2308
Intermittent dynamics and 1/f^beta noise in single cardiac muscle cells
Fluctuations in the spontaneous beating activity of isolated cardiac cells were studied over a timescale of six decades. The beat dynamics of single cardiac cells were heterogeneous and intermittent. The interbeat intervals (IBIs) were power-law distributed in a long-time regime. Furthermore, for long timescales up to the experimental window, the autocorrelation of IBIs exhibits a scaling behavior of 1/f^beta-noise type. These observations suggest that 1/f^beta noise is an intrinsic characteristic of spontaneous activity of single cardiac cells.
q-bio.CB
fluctuations in the spontaneous beating activity of isolated cardiac cells were studied over a timescale of six decades the beat dynamics of single cardiac cells were heterogeneous and intermittent the interbeat intervals ibis were powerlaw distributed in a longtime regime furthermore for long timescales up to the experimental window the autocorrelation of ibis exhibits a scaling behavior of 1fbetanoise type these observations suggest that 1fbeta noise is an intrinsic characteristic of spontaneous activity of single cardiac cells
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708.2309
On Compact Routing for the Internet
While there exist compact routing schemes designed for grids, trees, and Internet-like topologies that offer routing tables of sizes that scale logarithmically with the network size, we demonstrate in this paper that in view of recent results in compact routing research, such logarithmic scaling on Internet-like topologies is fundamentally impossible in the presence of topology dynamics or topology-independent (flat) addressing. We use analytic arguments to show that the number of routing control messages per topology change cannot scale better than linearly on Internet-like topologies. We also employ simulations to confirm that logarithmic routing table size scaling gets broken by topology-independent addressing, a cornerstone of popular locator-identifier split proposals aiming at improving routing scaling in the presence of network topology dynamics or host mobility. These pessimistic findings lead us to the conclusion that a fundamental re-examination of assumptions behind routing models and abstractions is needed in order to find a routing architecture that would be able to scale ``indefinitely.''
cs.NI
while there exist compact routing schemes designed for grids trees and internetlike topologies that offer routing tables of sizes that scale logarithmically with the network size we demonstrate in this paper that in view of recent results in compact routing research such logarithmic scaling on internetlike topologies is fundamentally impossible in the presence of topology dynamics or topologyindependent flat addressing we use analytic arguments to show that the number of routing control messages per topology change cannot scale better than linearly on internetlike topologies we also employ simulations to confirm that logarithmic routing table size scaling gets broken by topologyindependent addressing a cornerstone of popular locatoridentifier split proposals aiming at improving routing scaling in the presence of network topology dynamics or host mobility these pessimistic findings lead us to the conclusion that a fundamental reexamination of assumptions behind routing models and abstractions is needed in order to find a routing architecture that would be able to scale indefinitely
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708.231
Benefiting from Disorder: Source Coding for Unordered Data
The order of letters is not always relevant in a communication task. This paper discusses the implications of order irrelevance on source coding, presenting results in several major branches of source coding theory: lossless coding, universal lossless coding, rate-distortion, high-rate quantization, and universal lossy coding. The main conclusions demonstrate that there is a significant rate savings when order is irrelevant. In particular, lossless coding of n letters from a finite alphabet requires Theta(log n) bits and universal lossless coding requires n + o(n) bits for many countable alphabet sources. However, there are no universal schemes that can drive a strong redundancy measure to zero. Results for lossy coding include distribution-free expressions for the rate savings from order irrelevance in various high-rate quantization schemes. Rate-distortion bounds are given, and it is shown that the analogue of the Shannon lower bound is loose at all finite rates.
cs.IT math.IT
the order of letters is not always relevant in a communication task this paper discusses the implications of order irrelevance on source coding presenting results in several major branches of source coding theory lossless coding universal lossless coding ratedistortion highrate quantization and universal lossy coding the main conclusions demonstrate that there is a significant rate savings when order is irrelevant in particular lossless coding of n letters from a finite alphabet requires thetalog n bits and universal lossless coding requires n on bits for many countable alphabet sources however there are no universal schemes that can drive a strong redundancy measure to zero results for lossy coding include distributionfree expressions for the rate savings from order irrelevance in various highrate quantization schemes ratedistortion bounds are given and it is shown that the analogue of the shannon lower bound is loose at all finite rates
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708.2311
Phase Transition Dynamics and Its Alpha' Corrections
We study the dynamics of the first order phase transition in the holographic hard wall model, namely, Polchinski-Strassler's model and come to the conclusion that the phase transition is incomplete in large N limit with the natural boundary condition. We also consider the string length corrections to both hard wall model and Witten's model, and find that the interesting transition configuration is preserved under the alpha' corrections.
hep-th hep-ph
we study the dynamics of the first order phase transition in the holographic hard wall model namely polchinskistrasslers model and come to the conclusion that the phase transition is incomplete in large n limit with the natural boundary condition we also consider the string length corrections to both hard wall model and wittens model and find that the interesting transition configuration is preserved under the alpha corrections
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708.2312
Markov bases for two-way subtable sum problems
It has been well-known that for two-way contingency tables with fixed row sums and column sums the set of square-free moves of degree two forms a Markov basis. However when we impose an additional constraint that the sum of a subtable is also fixed, then these moves do not necessarily form a Markov basis. Thus, in this paper, we show a necessary and sufficient condition on a subtable so that the set of square-free moves of degree two forms a Markov basis.
math.CO math.AC
it has been wellknown that for twoway contingency tables with fixed row sums and column sums the set of squarefree moves of degree two forms a markov basis however when we impose an additional constraint that the sum of a subtable is also fixed then these moves do not necessarily form a markov basis thus in this paper we show a necessary and sufficient condition on a subtable so that the set of squarefree moves of degree two forms a markov basis
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708.2313
Comparative study of electron and hole doped High-Tc compounds in pseudogap regime: LDA+DMFT+Sk approach
Pseudogap regime for the prototype high-Tc compounds hole doped Bi2Sr2CaCu2O8-x (Bi2212) and electron doped Nd2-xCexCuO4 (NCCO) is described by means of novel generalized LDA+DMFT+Sk approach. Here conventional dynamical mean-field theory (DMFT) equations are supplied with additional (momentum dependent) self-energy Sk. In the present case Sk describes non-local dynamical correlations induced by short-ranged collective Heisenberg-like antiferromagnetic spin fluctuations. Material specific model parameters of two neighboring CuO2 layers of Bi2212 and single CuO2 layer of NCCO were obtained within local density approximation (LDA) and constrained LDA method. We show that Fermi surface in presence of the pseudogap fluctuations have perfectly visible "hot-spots" for NCCO while in Bi2212 there is just rather broad region with strong antiferromagnetic scattering. Results obtained are in good agreement with recent ARPES and optical experiments.
cond-mat.str-el cond-mat.supr-con
pseudogap regime for the prototype hightc compounds hole doped bi2sr2cacu2o8x bi2212 and electron doped nd2xcexcuo4 ncco is described by means of novel generalized ldadmftsk approach here conventional dynamical meanfield theory dmft equations are supplied with additional momentum dependent selfenergy sk in the present case sk describes nonlocal dynamical correlations induced by shortranged collective heisenberglike antiferromagnetic spin fluctuations material specific model parameters of two neighboring cuo2 layers of bi2212 and single cuo2 layer of ncco were obtained within local density approximation lda and constrained lda method we show that fermi surface in presence of the pseudogap fluctuations have perfectly visible hotspots for ncco while in bi2212 there is just rather broad region with strong antiferromagnetic scattering results obtained are in good agreement with recent arpes and optical experiments
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708.2314
Spectacular Trailing Streamers near LMC X-1: The First Evidence of a Jet?
We report VIMOS integral field spectroscopy of the N159F nebula surrounding LMC X-1. Our observations reveal a rich, extended system of emission line filaments lining the boundary of a large conical cavity identified in Spitzer mid-IR imaging. We find that X-ray photoionization cannot be solely responsible for the observed ionization structure of N159F. We propose that the extended filamentary emission is produced primarily by ionization from a shock driven by a presently unobserved jet from LMC X-1. We infer a shock velocity of v_s ~ 90 km/s and conclude that the jet responsible for the bow shock is presently undetected because it has switched off, rather than because it has a low surface brightness. This interpretation is consistent with the present soft X-ray spectral state of LMC X-1 and suggests the jet is intermittent.
astro-ph
we report vimos integral field spectroscopy of the n159f nebula surrounding lmc x1 our observations reveal a rich extended system of emission line filaments lining the boundary of a large conical cavity identified in spitzer midir imaging we find that xray photoionization cannot be solely responsible for the observed ionization structure of n159f we propose that the extended filamentary emission is produced primarily by ionization from a shock driven by a presently unobserved jet from lmc x1 we infer a shock velocity of v_s 90 kms and conclude that the jet responsible for the bow shock is presently undetected because it has switched off rather than because it has a low surface brightness this interpretation is consistent with the present soft xray spectral state of lmc x1 and suggests the jet is intermittent
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708.2315
Conformal representations of Leibniz algebras
In this note we present a more detailed and explicit exposition of the definition of a conformal representation of a Leibniz algebra. Recall (arXiv:math/0611501v3) that Leibniz algebras are exactly Lie dialgebras. The idea is based on the general fact that every dialgebra that belongs to a variety $\Var $ can be embedded into a conformal algebra of the same variety. In particular, we prove that an arbitrary (finite dimensional) Leibniz algebra has a (finite) faithful conformal representation. As a corollary, we deduce the analogue of the PBW-theorem for Leibniz algebras.
math.RA math.QA
in this note we present a more detailed and explicit exposition of the definition of a conformal representation of a leibniz algebra recall arxivmath0611501v3 that leibniz algebras are exactly lie dialgebras the idea is based on the general fact that every dialgebra that belongs to a variety var can be embedded into a conformal algebra of the same variety in particular we prove that an arbitrary finite dimensional leibniz algebra has a finite faithful conformal representation as a corollary we deduce the analogue of the pbwtheorem for leibniz algebras
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708.2316
Generalized rational blow-down, torus knots, and Euclidean algorithm
We construct a Kirby diagram of the rational homology ball used in "generalized rational blow-down" developed by Jongil Park. The diagram consists of a dotted circle and a torus knot. The link is simpler, but the parameters are a little complicate. Euclidean Algorithm is used three times in the construction and the proof.
math.GT
we construct a kirby diagram of the rational homology ball used in generalized rational blowdown developed by jongil park the diagram consists of a dotted circle and a torus knot the link is simpler but the parameters are a little complicate euclidean algorithm is used three times in the construction and the proof
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708.2317
Effects of nuclear molecular configurations on the astrophysical S-factor for $^{16}$O + $^{16}$O
The impact of nuclear molecular configurations on the astrophysical S-factor for $^{16}$O + $^{16}$O is investigated within the realistic two-center shell model based on Woods-Saxon potentials. These molecular effects refer to the formation of a neck between the interacting nuclei and the radial dependent collective mass parameter. It is demonstrated that the former is crucial to explain the current experimental data with high accuracy and without any free parameter, whilst in addition the latter predicts a pronounced maximum in the S-factor. In contrast to very recent results by Jiang et al., the S-factor does not decline towards extremely low values as energy decreases.
nucl-th
the impact of nuclear molecular configurations on the astrophysical sfactor for 16o 16o is investigated within the realistic twocenter shell model based on woodssaxon potentials these molecular effects refer to the formation of a neck between the interacting nuclei and the radial dependent collective mass parameter it is demonstrated that the former is crucial to explain the current experimental data with high accuracy and without any free parameter whilst in addition the latter predicts a pronounced maximum in the sfactor in contrast to very recent results by jiang et al the sfactor does not decline towards extremely low values as energy decreases
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708.2318
Electronic structures of hexagonal RMnO3 (R = Gd, Tb, Dy, and Ho) thin films
We investigated the electronic structure of multiferroic hexagonal RMnO3 (R = Gd, Tb, Dy, and Ho) thin films using both optical spectroscopy and first-principles calculations. Using artificially stabilized hexagonal RMnO3, we extended the optical spectroscopic studies on the hexagonal multiferroic manganite system. We observed two optical transitions located near 1.7 eV and 2.3 eV, in addition to the predominant absorption above 5 eV. With the help of first-principles calculations, we attribute the low-lying optical absorption peaks to inter-site transitions from the oxygen states hybridized strongly with different Mn orbital symmetries to the Mn 3d3z2-r2 state. As the ionic radius of the rare earth ion increased, the lowest peak showed a systematic increase in its peak position. We explained this systematic change in terms of a flattening of the MnO5 triangular bipyramid.
cond-mat.str-el
we investigated the electronic structure of multiferroic hexagonal rmno3 r gd tb dy and ho thin films using both optical spectroscopy and firstprinciples calculations using artificially stabilized hexagonal rmno3 we extended the optical spectroscopic studies on the hexagonal multiferroic manganite system we observed two optical transitions located near 17 ev and 23 ev in addition to the predominant absorption above 5 ev with the help of firstprinciples calculations we attribute the lowlying optical absorption peaks to intersite transitions from the oxygen states hybridized strongly with different mn orbital symmetries to the mn 3d3z2r2 state as the ionic radius of the rare earth ion increased the lowest peak showed a systematic increase in its peak position we explained this systematic change in terms of a flattening of the mno5 triangular bipyramid
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708.2319
On Semimeasures Predicting Martin-Loef Random Sequences
Solomonoff's central result on induction is that the posterior of a universal semimeasure M converges rapidly and with probability 1 to the true sequence generating posterior mu, if the latter is computable. Hence, M is eligible as a universal sequence predictor in case of unknown mu. Despite some nearby results and proofs in the literature, the stronger result of convergence for all (Martin-Loef) random sequences remained open. Such a convergence result would be particularly interesting and natural, since randomness can be defined in terms of M itself. We show that there are universal semimeasures M which do not converge for all random sequences, i.e. we give a partial negative answer to the open problem. We also provide a positive answer for some non-universal semimeasures. We define the incomputable measure D as a mixture over all computable measures and the enumerable semimeasure W as a mixture over all enumerable nearly-measures. We show that W converges to D and D to mu on all random sequences. The Hellinger distance measuring closeness of two distributions plays a central role.
cs.IT cs.LG math.IT math.PR
solomonoffs central result on induction is that the posterior of a universal semimeasure m converges rapidly and with probability 1 to the true sequence generating posterior mu if the latter is computable hence m is eligible as a universal sequence predictor in case of unknown mu despite some nearby results and proofs in the literature the stronger result of convergence for all martinloef random sequences remained open such a convergence result would be particularly interesting and natural since randomness can be defined in terms of m itself we show that there are universal semimeasures m which do not converge for all random sequences ie we give a partial negative answer to the open problem we also provide a positive answer for some nonuniversal semimeasures we define the incomputable measure d as a mixture over all computable measures and the enumerable semimeasure w as a mixture over all enumerable nearlymeasures we show that w converges to d and d to mu on all random sequences the hellinger distance measuring closeness of two distributions plays a central role
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708.232
The non-viscous Burgers equation associated with random positions in coordinate space: a threshold for blow up behaviour
It is well known that the solutions to the non-viscous Burgers equation develop a gradient catastrophe at a critical time provided the initial data have a negative derivative in certain points. We consider this equation assuming that the particle paths in the medium are governed by a random process with a variance which depends in a polynomial way on the velocity. Given an initial distribution of the particles which is uniform in space and with the initial velocity linearly depending on the position we show both analytically and numerically that there exists a threshold effect: if the power in the above variance is less than 1, then the noise does not influence the solution behavior, in the following sense: the mean of the velocity when we keep the value of position fixed goes to infinity outside the origin. If however the power is larger or equal 1, then this mean decays to zero as the time tends to a critical value.
math.AP math.PR
it is well known that the solutions to the nonviscous burgers equation develop a gradient catastrophe at a critical time provided the initial data have a negative derivative in certain points we consider this equation assuming that the particle paths in the medium are governed by a random process with a variance which depends in a polynomial way on the velocity given an initial distribution of the particles which is uniform in space and with the initial velocity linearly depending on the position we show both analytically and numerically that there exists a threshold effect if the power in the above variance is less than 1 then the noise does not influence the solution behavior in the following sense the mean of the velocity when we keep the value of position fixed goes to infinity outside the origin if however the power is larger or equal 1 then this mean decays to zero as the time tends to a critical value
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708.2321
Fast learning rates for plug-in classifiers
It has been recently shown that, under the margin (or low noise) assumption, there exist classifiers attaining fast rates of convergence of the excess Bayes risk, that is, rates faster than $n^{-1/2}$. The work on this subject has suggested the following two conjectures: (i) the best achievable fast rate is of the order $n^{-1}$, and (ii) the plug-in classifiers generally converge more slowly than the classifiers based on empirical risk minimization. We show that both conjectures are not correct. In particular, we construct plug-in classifiers that can achieve not only fast, but also super-fast rates, that is, rates faster than $n^{-1}$. We establish minimax lower bounds showing that the obtained rates cannot be improved.
math.ST stat.TH
it has been recently shown that under the margin or low noise assumption there exist classifiers attaining fast rates of convergence of the excess bayes risk that is rates faster than n12 the work on this subject has suggested the following two conjectures i the best achievable fast rate is of the order n1 and ii the plugin classifiers generally converge more slowly than the classifiers based on empirical risk minimization we show that both conjectures are not correct in particular we construct plugin classifiers that can achieve not only fast but also superfast rates that is rates faster than n1 we establish minimax lower bounds showing that the obtained rates cannot be improved
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708.2322
Zero
You shall not find any new physics, because all physical events are interpreted well-known particles (leptons, quarks, photons, gluons, W-bosons, Z-boson) and forces which have long known (electroweak, gravity, strong interactions). Contents: 1. Pointlike events and probability. 2. Leptons' moving equations and masses. 3. Fermion-antifermion asommetry. 4. Electroweak equations. 5. Chromatic states and gluons. 6. Asimptotic freedom, confinement, Newton's gravity. 7. Dark energy and dark matter. 8. Events and particles. 9. Conclusion.
physics.gen-ph
you shall not find any new physics because all physical events are interpreted wellknown particles leptons quarks photons gluons wbosons zboson and forces which have long known electroweak gravity strong interactions contents 1 pointlike events and probability 2 leptons moving equations and masses 3 fermionantifermion asommetry 4 electroweak equations 5 chromatic states and gluons 6 asimptotic freedom confinement newtons gravity 7 dark energy and dark matter 8 events and particles 9 conclusion
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708.2323
Optimal Unambiguous Discrimination of Quantum States
Unambiguously distinguishing between nonorthogonal but linearly independent quantum states is a challenging problem in quantum information processing. In this work, an exact analytic solution to an optimum measurement problem involving an arbitrary number of pure linearly independent quantum states is presented. To this end, the relevant semi-definite programming task is reduced to a linear programming one with a feasible region of polygon type which can be solved via simplex method. The strength of the method is illustrated through some explicit examples. Also using the close connection between the Lewenstein-Sanpera decomposition(LSD) and semi-definite programming approach, the optimal positive operator valued measure for some of the well-known examples is obtain via Lewenstein-Sanpera decomposition method. {\bf Keywords:} Optimal Unambiguous State Discrimination, Linear Programming, Lewenstein-Sanpera decomposition. {\bf PACs Index: 03.67.Hk, 03.65.Ta, 42.50.-p
quant-ph
unambiguously distinguishing between nonorthogonal but linearly independent quantum states is a challenging problem in quantum information processing in this work an exact analytic solution to an optimum measurement problem involving an arbitrary number of pure linearly independent quantum states is presented to this end the relevant semidefinite programming task is reduced to a linear programming one with a feasible region of polygon type which can be solved via simplex method the strength of the method is illustrated through some explicit examples also using the close connection between the lewensteinsanpera decompositionlsd and semidefinite programming approach the optimal positive operator valued measure for some of the wellknown examples is obtain via lewensteinsanpera decomposition method bf keywords optimal unambiguous state discrimination linear programming lewensteinsanpera decomposition bf pacs index 0367hk 0365ta 4250p
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708.2324
A twist in the geometry of rotating black holes: seeking the cause of acausality
We investigate Kerr-Newman black holes in which a rotating charged ring-shaped singularity induces a region which contains closed timelike curves (CTCs). Contrary to popular belief, it turns out that the time orientation of the CTC is opposite to the direction in which the singularity or the ergosphere rotates. In this sense, CTCs "counter-rotate" against the rotating black hole. We have similar results for all spacetimes sufficiently familiar to us in which rotation induces CTCs. This motivates our conjecture that perhaps this counter-rotation is not an accidental oddity particular to Kerr-Newman spacetimes, but instead there may be a general and intuitively comprehensible reason for this.
gr-qc physics.hist-ph
we investigate kerrnewman black holes in which a rotating charged ringshaped singularity induces a region which contains closed timelike curves ctcs contrary to popular belief it turns out that the time orientation of the ctc is opposite to the direction in which the singularity or the ergosphere rotates in this sense ctcs counterrotate against the rotating black hole we have similar results for all spacetimes sufficiently familiar to us in which rotation induces ctcs this motivates our conjecture that perhaps this counterrotation is not an accidental oddity particular to kerrnewman spacetimes but instead there may be a general and intuitively comprehensible reason for this
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708.2325
A two-parameter generalization of the complete elliptic integral of second kind
A two-parameter generalization of the complete elliptic integral of second kind is expressed in terms of the Appell function $F_{4}$. This function is further reduced to a quite simple bilinear form in the complete elliptic integrals $K$ and $E$. The physical applications are briefly mentioned.
math-ph math.MP
a twoparameter generalization of the complete elliptic integral of second kind is expressed in terms of the appell function f_4 this function is further reduced to a quite simple bilinear form in the complete elliptic integrals k and e the physical applications are briefly mentioned
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708.2326
Quantum spin correlations through the superconducting-normal phase transition in electron-doped superconducting Pr0.88LaCe0.12CuO4-d
The quantum spin fluctuations of the S = 1/2 Cu ions are important in determining the physical properties of the high-transition temperature (high-Tc) copper oxide superconductors, but their possible role in the electron pairing for superconductivity remains an open question. The principal feature of the spin fluctuations in optimally doped high-Tc superconductors is a well defined magnetic resonance whose energy (Er) tracks Tc (as the composition is varied) and whose intensity develops like an order parameter in the superconducting state. We show that the suppression of superconductivity and its associated condensation energy by a magnetic field in the electron-doped high-Tc superconductor, Pr0.88LaCe0.12CuO4-d (Tc = 24 K), is accompanied by the complete suppression of the resonance and the concomitant emergence of static antiferromagnetic (AF) order. Our results demonstrate that the resonance is intimately related to the superconducting condensation energy, and thus suggest that it plays a role in the electron pairing and superconductivity.
cond-mat.supr-con cond-mat.str-el
the quantum spin fluctuations of the s 12 cu ions are important in determining the physical properties of the hightransition temperature hightc copper oxide superconductors but their possible role in the electron pairing for superconductivity remains an open question the principal feature of the spin fluctuations in optimally doped hightc superconductors is a well defined magnetic resonance whose energy er tracks tc as the composition is varied and whose intensity develops like an order parameter in the superconducting state we show that the suppression of superconductivity and its associated condensation energy by a magnetic field in the electrondoped hightc superconductor pr088lace012cuo4d tc 24 k is accompanied by the complete suppression of the resonance and the concomitant emergence of static antiferromagnetic af order our results demonstrate that the resonance is intimately related to the superconducting condensation energy and thus suggest that it plays a role in the electron pairing and superconductivity
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708.2327
Non-cyclic graph of a group
We associate a graph $\Gamma_G$ to a non locally cyclic group $G$ (called the non-cyclic graph of $G$) as follows: take $G\backslash Cyc(G)$ as vertex set, where $Cyc(G)=\{x\in G | \left<x,y\right> \text{is cyclic for all} y\in G\}$, and join two vertices if they do not generate a cyclic subgroup. We study the properties of this graph and we establish some graph theoretical properties (such as regularity) of this graph in terms of the group ones. We prove that the clique number of $\Gamma_G$ is finite if and only if $\Gamma_G$ has no infinite clique. We prove that if $G$ is a finite nilpotent group and $H$ is a group with $\Gamma_G\cong\Gamma_H$ and $|Cyc(G)|=|Cyc(H)|=1$, then $H$ is a finite nilpotent group. We give some examples of groups $G$ whose non-cyclic graphs are ``unique'', i.e., if $\Gamma_G\cong \Gamma_H$ for some group $H$, then $G\cong H$. In view of these examples, we conjecture that every finite non-abelian simple group has a unique non-cyclic graph. Also we give some examples of finite non-cyclic groups $G$ with the property that if $\Gamma_G \cong \Gamma_H$ for some group $H$, then $|G|=|H|$. These suggest the question whether the latter property holds for all finite non-cyclic groups.
math.GR math.CO
we associate a graph gamma_g to a non locally cyclic group g called the noncyclic graph of g as follows take gbackslash cycg as vertex set where cycgxin g leftxyright textis cyclic for all yin g and join two vertices if they do not generate a cyclic subgroup we study the properties of this graph and we establish some graph theoretical properties such as regularity of this graph in terms of the group ones we prove that the clique number of gamma_g is finite if and only if gamma_g has no infinite clique we prove that if g is a finite nilpotent group and h is a group with gamma_gconggamma_h and cycgcych1 then h is a finite nilpotent group we give some examples of groups g whose noncyclic graphs are unique ie if gamma_gcong gamma_h for some group h then gcong h in view of these examples we conjecture that every finite nonabelian simple group has a unique noncyclic graph also we give some examples of finite noncyclic groups g with the property that if gamma_g cong gamma_h for some group h then gh these suggest the question whether the latter property holds for all finite noncyclic groups
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708.2328
Neutrino oscillations in matter and in twisting magnetic fields
We find the solution to the Dirac equation for a massive neutrino with a magnetic moment propagating in background matter and interacting with the twisting magnetic field. In frames of the relativistic quantum mechanics approach to the description of neutrino evolution we use the obtained solution to derive neutrino wave functions satisfying the given initial condition. We apply the results to the analysis of neutrino spin oscillations in matter under the influence of the twisting magnetic field. Then on the basis of the yielded results we describe spin-flavor oscillations of Dirac neutrinos that mix and have non-vanishing matrix of magnetic moments. We again formulate the initial condition problem, derive neutrinos wave functions and calculate the transition probabilities for different magnetic moments matrices. The consistency of the obtained results with the quantum mechanical treatment of spin-flavor oscillations is discussed. We also consider several applications to astrophysical and cosmological neutrinos.
hep-ph hep-th
we find the solution to the dirac equation for a massive neutrino with a magnetic moment propagating in background matter and interacting with the twisting magnetic field in frames of the relativistic quantum mechanics approach to the description of neutrino evolution we use the obtained solution to derive neutrino wave functions satisfying the given initial condition we apply the results to the analysis of neutrino spin oscillations in matter under the influence of the twisting magnetic field then on the basis of the yielded results we describe spinflavor oscillations of dirac neutrinos that mix and have nonvanishing matrix of magnetic moments we again formulate the initial condition problem derive neutrinos wave functions and calculate the transition probabilities for different magnetic moments matrices the consistency of the obtained results with the quantum mechanical treatment of spinflavor oscillations is discussed we also consider several applications to astrophysical and cosmological neutrinos
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708.2329
Feshbach Molecules in a One-dimensional Optical Lattice
We present the theory of a pair of atoms in a one-dimensional optical lattice interacting via a narrow Feshbach resonance. Using a two-channel description of the resonance, we derive analytic results for the scattering states inside the continuum band and the discrete bound states outside the band. We identify a Fano resonance profile, and the survival probability of a molecule when swept through the Bloch band of scattering states by varying an applied magnetic field. We discuss how these results may be used to investigate the importance of the structured nature of the continuum in experiments.
cond-mat.other quant-ph
we present the theory of a pair of atoms in a onedimensional optical lattice interacting via a narrow feshbach resonance using a twochannel description of the resonance we derive analytic results for the scattering states inside the continuum band and the discrete bound states outside the band we identify a fano resonance profile and the survival probability of a molecule when swept through the bloch band of scattering states by varying an applied magnetic field we discuss how these results may be used to investigate the importance of the structured nature of the continuum in experiments
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708.233
Light dressed-excitons in an incoherent-electron sea: Evidence for Mollow-triplet and Autler-Townes doublet
We demonstrate that the interaction between excitons and a sea of incoherent electrons does not preclude excitons dressing by light. We investigate the role of exciton-electron scattering in the light dressing by measuring the dynamical absorption spectrum of a modulation-doped CdTe quantum well, which shows a clear evidence for significant electron scattering of the excitonic states. We show the occurrence of dressed and correlated excitons by detecting quantum coherent interferences through excitonic Autler-Townes doublet and ac Stark splitting, which evolves to Mollow triplet with gain. We also evidence the partial inhibition of the electron-exciton scattering by exciton-light coupling.
cond-mat.mtrl-sci
we demonstrate that the interaction between excitons and a sea of incoherent electrons does not preclude excitons dressing by light we investigate the role of excitonelectron scattering in the light dressing by measuring the dynamical absorption spectrum of a modulationdoped cdte quantum well which shows a clear evidence for significant electron scattering of the excitonic states we show the occurrence of dressed and correlated excitons by detecting quantum coherent interferences through excitonic autlertownes doublet and ac stark splitting which evolves to mollow triplet with gain we also evidence the partial inhibition of the electronexciton scattering by excitonlight coupling
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708.2331
The Boron Buckyball has an Unexpected Th Symmetry
The boron buckyball avoids the high symmetry icosahedral cage structure. The previously reported Ih symmetric structure is not an energy minimum in the potential energy surface and exhibits a spontaneous symmetry breaking to yield a puckered cage with a rare Th symmetry. The HOMO-LUMO gap is twice as large as the reported value and amounts to 1.94 eV at B3LYP/6-31G(d) level. The valence orbital structure of boron buckyball is identical to the one in the carbon analogue.
cond-mat.other
the boron buckyball avoids the high symmetry icosahedral cage structure the previously reported ih symmetric structure is not an energy minimum in the potential energy surface and exhibits a spontaneous symmetry breaking to yield a puckered cage with a rare th symmetry the homolumo gap is twice as large as the reported value and amounts to 194 ev at b3lyp631gd level the valence orbital structure of boron buckyball is identical to the one in the carbon analogue
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708.2332
Metastable state involved resonant tunneling through single InAs/GaAs quantum dot
A scheme of resonant tunneling through the metastable state of semiconductor quantum dot is presented and implemented in the transport study of freestanding InAs quantum dots grown on GaAs(001) under illumination using conductive atomic force microscopy. The metastable state is achieved by capturing one photoexcited Fermi hole in the valence energy level of InAs quantum dot. Resonant tunneling through single quantum dot can be observed at room temperature due to the existence of metastable state. The amplitude of tunneling current depends on the barrier arrangement and the concentration of photoexcited holes around the quantum dot, but is found steady when the height of dot varies from 1.8 to 9.9 nm, which are in good agreement with the proposed model. The experiment demonstrates a solution of room temperature operated single electron device to amplify the photocurrent by the singularity of resonant tunneling in epitaxial quantum dot.
quant-ph
a scheme of resonant tunneling through the metastable state of semiconductor quantum dot is presented and implemented in the transport study of freestanding inas quantum dots grown on gaas001 under illumination using conductive atomic force microscopy the metastable state is achieved by capturing one photoexcited fermi hole in the valence energy level of inas quantum dot resonant tunneling through single quantum dot can be observed at room temperature due to the existence of metastable state the amplitude of tunneling current depends on the barrier arrangement and the concentration of photoexcited holes around the quantum dot but is found steady when the height of dot varies from 18 to 99 nm which are in good agreement with the proposed model the experiment demonstrates a solution of room temperature operated single electron device to amplify the photocurrent by the singularity of resonant tunneling in epitaxial quantum dot
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708.2333
The coherent {\it d}-wave superconducting gap in underdoped La$_{2-x}$Sr$_{x}$CuO$_4$ as studied by angle-resolved photoemission
We present angle-resolved photoemission spectroscopy (ARPES) data on moderately underdoped La$_{1.855}$Sr$_{0.145}$CuO$_4$ at temperatures below and above the superconducting transition temperature. Unlike previous studies of this material, we observe sharp spectral peaks along the entire underlying Fermi surface in the superconducting state. These peaks trace out an energy gap that follows a simple {\it d}-wave form, with a maximum superconducting gap of 14 meV. Our results are consistent with a single gap picture for the cuprates. Furthermore our data on the even more underdoped sample La$_{1.895}$Sr$_{0.105}$CuO$_4$ also show sharp spectral peaks, even at the antinode, with a maximum superconducting gap of 26 meV.
cond-mat.supr-con cond-mat.str-el
we present angleresolved photoemission spectroscopy arpes data on moderately underdoped la_1855sr_0145cuo_4 at temperatures below and above the superconducting transition temperature unlike previous studies of this material we observe sharp spectral peaks along the entire underlying fermi surface in the superconducting state these peaks trace out an energy gap that follows a simple it dwave form with a maximum superconducting gap of 14 mev our results are consistent with a single gap picture for the cuprates furthermore our data on the even more underdoped sample la_1895sr_0105cuo_4 also show sharp spectral peaks even at the antinode with a maximum superconducting gap of 26 mev
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708.2334
Collective transport in the insulating state of Josephson junction arrays
We investigate collective Cooper-pair transport of one- and two-dimensional Josephson junction arrays in the insulating state. We derive an analytical expression for the current-voltage characteristic revealing thermally activated conductivity at small voltages and threshold voltage depinning. The activation energy and the related depinning voltage represent a dynamic Coulomb barrier for collective charge transfer over the whole system and scale with the system size. We show that both quantities are non-monotonic functions of magnetic field. We propose that formation of the dynamic Coulomb barrier as well as the size scaling of the activation energy and the depinning threshold voltage, are consequences of the mutual phase synchronization. We apply the results for interpretation of experimental data in disordered films near the superconductor-insulator transition.
cond-mat.supr-con cond-mat.mes-hall
we investigate collective cooperpair transport of one and twodimensional josephson junction arrays in the insulating state we derive an analytical expression for the currentvoltage characteristic revealing thermally activated conductivity at small voltages and threshold voltage depinning the activation energy and the related depinning voltage represent a dynamic coulomb barrier for collective charge transfer over the whole system and scale with the system size we show that both quantities are nonmonotonic functions of magnetic field we propose that formation of the dynamic coulomb barrier as well as the size scaling of the activation energy and the depinning threshold voltage are consequences of the mutual phase synchronization we apply the results for interpretation of experimental data in disordered films near the superconductorinsulator transition
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708.2335
2D shift of the centre of gravity of the light beam carrying orbital angular momentum, which accompanies reflection from a lossy medium
It is shown that after reflection from a lossy medium the $s$- or $p$-polarized paraxial light beam carrying the orbital angular momentum suffers the 2D shift of the beam's centre of gravity relative the geometric optic axis. The mutually orthogonal components of this shift are expressed through the real and imaginary parts of the common complex quantity. The features of the 2D vector, which describes the shift, are analyzed.
physics.optics
it is shown that after reflection from a lossy medium the s or ppolarized paraxial light beam carrying the orbital angular momentum suffers the 2d shift of the beams centre of gravity relative the geometric optic axis the mutually orthogonal components of this shift are expressed through the real and imaginary parts of the common complex quantity the features of the 2d vector which describes the shift are analyzed
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708.2336
Unsatisfiable Linear k-CNFs Exist, for every k
We call a CNF formula linear if any two clauses have at most one variable in common. Let Linear k-SAT be the problem of deciding whether a given linear k-CNF formula is satisfiable. Here, a k-CNF formula is a CNF formula in which every clause has size exactly k. It was known that for k >= 3, Linear k-SAT is NP-complete if and only if an unsatisfiable linear k-CNF formula exists, and that they do exist for k >= 4. We prove that unsatisfiable linear k-CNF formulas exist for every k. Let f(k) be the minimum number of clauses in an unsatisfiable linear k-CNF formula. We show that f(k) is Omega(k2^k) and O(4^k*k^4), i.e., minimum size unsatisfiable linear k-CNF formulas are significantly larger than minimum size unsatisfiable k-CNF formulas. Finally, we prove that, surprisingly, linear k-CNF formulas do not allow for a larger fraction of clauses to be satisfied than general k-CNF formulas.
cs.DM cs.CC cs.LO
we call a cnf formula linear if any two clauses have at most one variable in common let linear ksat be the problem of deciding whether a given linear kcnf formula is satisfiable here a kcnf formula is a cnf formula in which every clause has size exactly k it was known that for k 3 linear ksat is npcomplete if and only if an unsatisfiable linear kcnf formula exists and that they do exist for k 4 we prove that unsatisfiable linear kcnf formulas exist for every k let fk be the minimum number of clauses in an unsatisfiable linear kcnf formula we show that fk is omegak2k and o4kk4 ie minimum size unsatisfiable linear kcnf formulas are significantly larger than minimum size unsatisfiable kcnf formulas finally we prove that surprisingly linear kcnf formulas do not allow for a larger fraction of clauses to be satisfied than general kcnf formulas
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708.2337
Evolution of the bursting-layer wave during a Type 1 X-ray burst
In a popular scenario due to Heyl, quasi periodic oscillations (QPOs) which are seen during type 1 X-ray bursts are produced by giant travelling waves in neutron-star oceans. Piro and Bildsten have proposed that during the burst cooling the wave in the bursting layer may convert into a deep crustal interface wave, which would cut off the visible QPOs. This cut-off would help explain the magnitude of the QPO frequency drift, which is otherwise overpredicted by a factor of several in Heyl's scenario. In this paper, we study the coupling between the bursting layer and the deep ocean. The coupling turns out to be weak and only a small fraction of the surface-wave energy gets transferred to that of the crustal-interface wave during the burst. Thus the crustal-interface wave plays no dynamical role during the burst, and no early QPO cut-off should occur.
astro-ph
in a popular scenario due to heyl quasi periodic oscillations qpos which are seen during type 1 xray bursts are produced by giant travelling waves in neutronstar oceans piro and bildsten have proposed that during the burst cooling the wave in the bursting layer may convert into a deep crustal interface wave which would cut off the visible qpos this cutoff would help explain the magnitude of the qpo frequency drift which is otherwise overpredicted by a factor of several in heyls scenario in this paper we study the coupling between the bursting layer and the deep ocean the coupling turns out to be weak and only a small fraction of the surfacewave energy gets transferred to that of the crustalinterface wave during the burst thus the crustalinterface wave plays no dynamical role during the burst and no early qpo cutoff should occur
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708.2338
Magnetic Phase Diagram of Spin-1/2 Two-Leg Ladder with Four-Spin Ring Exchange
We study the spin-1/2 two-leg Heisenberg ladder with four-spin ring exchanges under a magnetic field. We introduce an exact duality transformation which is an extension of the spin-chirality duality developed previously and yields a new self-dual surface in the parameter space. We then determine the magnetic phase diagram using the numerical approaches of the density-matrix renormalization-group and exact diagonalization methods. We demonstrate the appearance of a magnetization plateau and the Tomonaga-Luttinger liquid with dominant vector-chirality quasi-long-range order for a wide parameter regime of strong ring exchange. A "nematic" phase, in which magnons form bound pairs and the magnon-pairing correlation functions dominate, is also identified.
cond-mat.str-el
we study the spin12 twoleg heisenberg ladder with fourspin ring exchanges under a magnetic field we introduce an exact duality transformation which is an extension of the spinchirality duality developed previously and yields a new selfdual surface in the parameter space we then determine the magnetic phase diagram using the numerical approaches of the densitymatrix renormalizationgroup and exact diagonalization methods we demonstrate the appearance of a magnetization plateau and the tomonagaluttinger liquid with dominant vectorchirality quasilongrange order for a wide parameter regime of strong ring exchange a nematic phase in which magnons form bound pairs and the magnonpairing correlation functions dominate is also identified
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708.2339
A pentaquark picture of Lambda(1405)
We test a pentaquark model of the negative parity hyperon Lambda(1405). We use a model where valence four quarks and one antiquark move in a potential relativistically and interact with each other and themselves through gluon and NG boson. Fall-apart decay rate of the system is studied and strong model dependence is pointed out.
hep-ph
we test a pentaquark model of the negative parity hyperon lambda1405 we use a model where valence four quarks and one antiquark move in a potential relativistically and interact with each other and themselves through gluon and ng boson fallapart decay rate of the system is studied and strong model dependence is pointed out
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708.234
Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm
The principles of measuring the shapes of galaxies by a model-fitting approach are discussed in the context of shape-measurement for surveys of weak gravitational lensing. It is argued that such an approach should be optimal, allowing measurement with maximal signal-to-noise, coupled with estimation of measurement errors. The distinction between likelihood-based and Bayesian methods is discussed. Systematic biases in the Bayesian method may be evaluated as part of the fitting process, and overall such an approach should yield unbiased shear estimation without requiring external calibration from simulations. The principal disadvantage of model-fitting for large surveys is the computational time required, but here an algorithm is presented that enables large surveys to be analysed in feasible computation times. The method and algorithm is tested on simulated galaxies from the Shear TEsting Program (STEP).
astro-ph
the principles of measuring the shapes of galaxies by a modelfitting approach are discussed in the context of shapemeasurement for surveys of weak gravitational lensing it is argued that such an approach should be optimal allowing measurement with maximal signaltonoise coupled with estimation of measurement errors the distinction between likelihoodbased and bayesian methods is discussed systematic biases in the bayesian method may be evaluated as part of the fitting process and overall such an approach should yield unbiased shear estimation without requiring external calibration from simulations the principal disadvantage of modelfitting for large surveys is the computational time required but here an algorithm is presented that enables large surveys to be analysed in feasible computation times the method and algorithm is tested on simulated galaxies from the shear testing program step
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708.2341
Unimodality of ordinary multinomials and maximal probabilities of convolution powers of discrete uniform distribution
We establish the unimodality and the asymptotic strong unimodality of the ordinary multinomials and give their smallest mode leading to the expression of the maximal probability of convolution powers of the discrete uniform distribution. We conclude giving the generating functions of the sequence of generalized ordinary multinomials and for an extension of the sequence of maximal probabilities for convolution power of discrete uniform distribution.
math.PR math.CO
we establish the unimodality and the asymptotic strong unimodality of the ordinary multinomials and give their smallest mode leading to the expression of the maximal probability of convolution powers of the discrete uniform distribution we conclude giving the generating functions of the sequence of generalized ordinary multinomials and for an extension of the sequence of maximal probabilities for convolution power of discrete uniform distribution
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708.2342
Complex dynamics in a nerve fiber model with periodic coefficients
We deal with the periodic boundary value problem for a second-order nonlinear ODE which includes the case of the Nagumo type equation $v_{xx} - g v + n(x) F(v) = 0,$ previously considered by Grindrod and Sleeman and by Chen and Bell in the study of nerve fiber models. In some recent works we discussed the case of nonexistence of nontrivial solutions as well as the case in which many positive periodic solutions may arise, the different situations depending by threshold parameters related to the weight function $n(x).$ Here we show that for a step function $n(x)$ (or for small perturbations of it) it is possible to obtain infinitely many periodic solutions and chaotic dynamics, due to the presence of a topological horseshoe (according to Kennedy and Yorke).
math.DS
we deal with the periodic boundary value problem for a secondorder nonlinear ode which includes the case of the nagumo type equation v_xx g v nx fv 0 previously considered by grindrod and sleeman and by chen and bell in the study of nerve fiber models in some recent works we discussed the case of nonexistence of nontrivial solutions as well as the case in which many positive periodic solutions may arise the different situations depending by threshold parameters related to the weight function nx here we show that for a step function nx or for small perturbations of it it is possible to obtain infinitely many periodic solutions and chaotic dynamics due to the presence of a topological horseshoe according to kennedy and yorke
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708.2343
The quantum Chernoff bound as a measure of distinguishability between density matrices: application to qubit and Gaussian states
Hypothesis testing is a fundamental issue in statistical inference and has been a crucial element in the development of information sciences. The Chernoff bound gives the minimal Bayesian error probability when discriminating two hypotheses given a large number of observations. Recently the combined work of Audenaert et al. [Phys. Rev. Lett. 98, 160501] and Nussbaum and Szkola [quant-ph/0607216] has proved the quantum analog of this bound, which applies when the hypotheses correspond to two quantum states. Based on the quantum Chernoff bound, we define a physically meaningful distinguishability measure and its corresponding metric in the space of states; the latter is shown to coincide with the Wigner-Yanase metric. Along the same lines, we define a second, more easily implementable, distinguishability measure based on the error probability of discrimination when the same local measurement is performed on every copy. We study some general properties of these measures, including the probability distribution of density matrices, defined via the volume element induced by the metric, and illustrate their use in the paradigmatic cases of qubits and Gaussian infinite-dimensional states.
quant-ph
hypothesis testing is a fundamental issue in statistical inference and has been a crucial element in the development of information sciences the chernoff bound gives the minimal bayesian error probability when discriminating two hypotheses given a large number of observations recently the combined work of audenaert et al phys rev lett 98 160501 and nussbaum and szkola quantph0607216 has proved the quantum analog of this bound which applies when the hypotheses correspond to two quantum states based on the quantum chernoff bound we define a physically meaningful distinguishability measure and its corresponding metric in the space of states the latter is shown to coincide with the wigneryanase metric along the same lines we define a second more easily implementable distinguishability measure based on the error probability of discrimination when the same local measurement is performed on every copy we study some general properties of these measures including the probability distribution of density matrices defined via the volume element induced by the metric and illustrate their use in the paradigmatic cases of qubits and gaussian infinitedimensional states
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708.2344
Developments and the preliminary tests of Resistive GEMs manufactured by a screen printing technology
We report promising initial results obtained with new resistive-electrode GEM (RETGEM) detectors manufactured, for the first time, using screen printing technology. These new detectors allow one to reach gas gains nearly as high as with ordinary GEM-like detectors with metallic electrodes; however, due to the high resistivity of its electrodes the RETGEM, in contrast to ordinary hole-type detectors, has the advantage of being fully spark protected. We discovered that RETGEMs can operate stably and at high gains in noble gases and in other badly quenched gases, such as mixtures of noble gases with air and in pure air; therefore, a wide range of practical applications, including dosimetry and detection of dangerous gases, is foreseeable. To promote a better understanding of RETGEM technology some comparative studies were completed with metallic-electrode thick GEMs. A primary benefit of these new RETGEMs is that the screen printing technology is easily accessible to many research laboratories. This accessibility encourages the possibility to manufacture these GEM-like detectors with the electrode resistivity easily optimized for particular experimental or practical applications.
physics.ins-det
we report promising initial results obtained with new resistiveelectrode gem retgem detectors manufactured for the first time using screen printing technology these new detectors allow one to reach gas gains nearly as high as with ordinary gemlike detectors with metallic electrodes however due to the high resistivity of its electrodes the retgem in contrast to ordinary holetype detectors has the advantage of being fully spark protected we discovered that retgems can operate stably and at high gains in noble gases and in other badly quenched gases such as mixtures of noble gases with air and in pure air therefore a wide range of practical applications including dosimetry and detection of dangerous gases is foreseeable to promote a better understanding of retgem technology some comparative studies were completed with metallicelectrode thick gems a primary benefit of these new retgems is that the screen printing technology is easily accessible to many research laboratories this accessibility encourages the possibility to manufacture these gemlike detectors with the electrode resistivity easily optimized for particular experimental or practical applications
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708.2345
Onsager-Machlup theory and work fluctuation theorem for a harmonically driven Brownian particle
We extend Tooru-Cohen analysis for nonequilirium steady state(NSS) of a Brownian particle to nonequilibrium oscillatory state (NOS) of Brownian particle by considering time dependent external drive protocol. We consider an unbounded charged Brownian particle in the presence of an oscillating electric field and prove work fluctuation theorem, which is valid for any initial distribution and at all times. For harmonically bounded and constantly dragged Brownian particle considered by Tooru and Cohen, work fluctuation theorem is valid for any initial condition(also NSS), but only in large time limit. We use Onsager-Machlup Lagrangian with a constraint to obtain frequency dependent work distribution function, and describe entropy production rate and properties of dissipation functions for the present system using Onsager-Machlup functional.
cond-mat.stat-mech
we extend toorucohen analysis for nonequilirium steady statenss of a brownian particle to nonequilibrium oscillatory state nos of brownian particle by considering time dependent external drive protocol we consider an unbounded charged brownian particle in the presence of an oscillating electric field and prove work fluctuation theorem which is valid for any initial distribution and at all times for harmonically bounded and constantly dragged brownian particle considered by tooru and cohen work fluctuation theorem is valid for any initial conditionalso nss but only in large time limit we use onsagermachlup lagrangian with a constraint to obtain frequency dependent work distribution function and describe entropy production rate and properties of dissipation functions for the present system using onsagermachlup functional
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708.2346
Apparent density fluctuations in N-constant ensemble simulations
In computer simulations performed in constant number of particles ensembles, although the total number of particles N contained in the simulation box does not fluctuate, hence giving a zero apparent compressibility, there are still local fluctuations in the number of particles. It is shown herein that these apparent fluctuations produce a compressibility that can be computed from the calculated radial distribution function, and which matches to a great accuracy the compressibility of the fluid for the open system. This statement implies that the radial distribution function evaluated in simulation of constant number of particles is identical to that evaluated in the grand canonical ensemble, for the entire distance range within half-box width. This is illustrated for the hard sphere and Lennard-Jones fluids and for molecular models of water. The origin of this apparent fluctuation is that the bulk of the remaining particles, outside the range over which the distribution function is calculated, act as a reservoir of particles for those within this range, thanks to the periodic boundary conditions. The implications on the calculation of the Kirkwood-Buff integrals are discussed.
physics.chem-ph physics.comp-ph
in computer simulations performed in constant number of particles ensembles although the total number of particles n contained in the simulation box does not fluctuate hence giving a zero apparent compressibility there are still local fluctuations in the number of particles it is shown herein that these apparent fluctuations produce a compressibility that can be computed from the calculated radial distribution function and which matches to a great accuracy the compressibility of the fluid for the open system this statement implies that the radial distribution function evaluated in simulation of constant number of particles is identical to that evaluated in the grand canonical ensemble for the entire distance range within halfbox width this is illustrated for the hard sphere and lennardjones fluids and for molecular models of water the origin of this apparent fluctuation is that the bulk of the remaining particles outside the range over which the distribution function is calculated act as a reservoir of particles for those within this range thanks to the periodic boundary conditions the implications on the calculation of the kirkwoodbuff integrals are discussed
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708.2347
Sums of products of generalized Fibonacci and Lucas numbers
In this paper, we establish several formulae for sums and alternating sums of products of generalized Fibonacci and Lucas numbers. In particular, we recover and extend all results of Z. Cerin and Z. Cerin & G. M. Gianella, more easily.
math.NT math.CO
in this paper we establish several formulae for sums and alternating sums of products of generalized fibonacci and lucas numbers in particular we recover and extend all results of z cerin and z cerin g m gianella more easily
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708.2348
Properties of voids in the Local Volume
Current explanation of the overabundance of dark matter subhalos in the Local Group (LG) indicates that there maybe a limit on mass of a halo, which can host a galaxy. This idea can be tested using voids in the distribution of galaxies: at some level small voids should not contain any (even dwarf) galaxies. We use observational samples complete to M_B=-12 with distances less than 8 Mpc to construct the void function (VF): the distribution of sizes of voids empty of any galaxies. There are ~ 30 voids with sizes ranging from 1 to 5 Mpc. We also study the distribution of dark matter halos in very high resolution simulations of the LCDM model. The theoretical VF matches the observations remarkably well only if we use halos with circular velocities larger than 45 +/- 10 km/s. This agrees with the Local Group predictions. Small voids look quite similar to heir giant cousins: the density has a minimum at the center of a void and it increases as we get closer to the border. Thus, both the Local Group data and the nearby voids indicate that isolated halos below 45 +/- 10 km/s must not host galaxies and that small (few Mpc) voids are truly dark.
astro-ph
current explanation of the overabundance of dark matter subhalos in the local group lg indicates that there maybe a limit on mass of a halo which can host a galaxy this idea can be tested using voids in the distribution of galaxies at some level small voids should not contain any even dwarf galaxies we use observational samples complete to m_b12 with distances less than 8 mpc to construct the void function vf the distribution of sizes of voids empty of any galaxies there are 30 voids with sizes ranging from 1 to 5 mpc we also study the distribution of dark matter halos in very high resolution simulations of the lcdm model the theoretical vf matches the observations remarkably well only if we use halos with circular velocities larger than 45 10 kms this agrees with the local group predictions small voids look quite similar to heir giant cousins the density has a minimum at the center of a void and it increases as we get closer to the border thus both the local group data and the nearby voids indicate that isolated halos below 45 10 kms must not host galaxies and that small few mpc voids are truly dark
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