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710.4953
Different canonical formulations of Einstein's theory of gravity
We describe the four most famous versions of the classical canonical formalism in the Einstein theory of gravity: the Arnovitt-Deser-Misner formalism, the Faddeev-Popov formalism, the tetrad formalism in the usual form, and the tetrad formalism in the form best suited for constructing the loop theory of gravity, which is now being developed. We present the canonical transformations relating these formalisms. The paper is written mainly for pedagogical purposes.
gr-qc
we describe the four most famous versions of the classical canonical formalism in the einstein theory of gravity the arnovittdesermisner formalism the faddeevpopov formalism the tetrad formalism in the usual form and the tetrad formalism in the form best suited for constructing the loop theory of gravity which is now being developed we present the canonical transformations relating these formalisms the paper is written mainly for pedagogical purposes
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710.4954
Cosmogenic neutrinos and quasi-stable supersymmetric particle production
We study the signal for the detection of quasi-stable supersymmetric particles produced in interactions of cosmogenic neutrinos. We consider energy loss of high energy staus due to photonuclear and weak interactions. We show that there are optimal nadir angles for which the stau signal is a factor of several hundred larager than muons. We discuss how one could potentially eliminate the muon background by considering the energy loss of muons in the detector. We also show results for the showers produced by weak interactions of staus that reach the detector.
hep-ph astro-ph
we study the signal for the detection of quasistable supersymmetric particles produced in interactions of cosmogenic neutrinos we consider energy loss of high energy staus due to photonuclear and weak interactions we show that there are optimal nadir angles for which the stau signal is a factor of several hundred larager than muons we discuss how one could potentially eliminate the muon background by considering the energy loss of muons in the detector we also show results for the showers produced by weak interactions of staus that reach the detector
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710.4955
The MSSM Higgs sector and B-Bbar mixing for large tan(beta)
A systematic analysis of Higgs-mediated contributions to the Bd and Bs mass differences is presented in the MSSM with large values of tan(beta). In particular, supersymmetric corrections to Higgs self-interactions are seen to modify the correlation between Delta Mq and BR(Bq --> mu+ mu-) for light Higgses. The present experimental upper bound on BR(Bs --> mu+ mu-) is nevertheless still sufficient to exclude noticeable Higgs-mediated effects on the mass differences in most of the parameter space.
hep-ph
a systematic analysis of higgsmediated contributions to the bd and bs mass differences is presented in the mssm with large values of tanbeta in particular supersymmetric corrections to higgs selfinteractions are seen to modify the correlation between delta mq and brbq mu mu for light higgses the present experimental upper bound on brbs mu mu is nevertheless still sufficient to exclude noticeable higgsmediated effects on the mass differences in most of the parameter space
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710.4956
SMA High Angular Resolution Imaging of the Lensed Quasar APM08279+5255
We present Submillimeter Array observations of the z=3.91 gravitationally lensed broad absorption line quasar APM08279+5255 which spatially resolve the 1.0mm (0.2mm rest-frame) dust continuum emission. At 0.4" resolution, the emission is separated into two components, a stronger, extended one to the northeast (46+/-5mJy) and a weaker, compact one to the southwest (15+/-2mJy). We have carried out simulations of the gravitational lensing effect responsible for the two submm components in order to constrain the intrinsic size of the submm continuum emission. Using an elliptical lens potential, the best fit lensing model yields an intrinsic (projected) diameter of ~80pc, which is not as compact as the optical/near-infrared (NIR) emission and agrees with previous size estimates of the gas and dust emission in APM08279+5255. Based on our estimate, we favor a scenario in which the 0.2mm (rest-frame) emission originates from a warm dust component (T_d=150-220K) that is mainly heated by the AGN rather than by a starburst (SB). The flux is boosted by a factor of ~90 in our model, consistent with recent estimates for APM08279+5255.
astro-ph
we present submillimeter array observations of the z391 gravitationally lensed broad absorption line quasar apm082795255 which spatially resolve the 10mm 02mm restframe dust continuum emission at 04 resolution the emission is separated into two components a stronger extended one to the northeast 465mjy and a weaker compact one to the southwest 152mjy we have carried out simulations of the gravitational lensing effect responsible for the two submm components in order to constrain the intrinsic size of the submm continuum emission using an elliptical lens potential the best fit lensing model yields an intrinsic projected diameter of 80pc which is not as compact as the opticalnearinfrared nir emission and agrees with previous size estimates of the gas and dust emission in apm082795255 based on our estimate we favor a scenario in which the 02mm restframe emission originates from a warm dust component t_d150220k that is mainly heated by the agn rather than by a starburst sb the flux is boosted by a factor of 90 in our model consistent with recent estimates for apm082795255
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710.4957
Fixing the fixed-point system - Applying Dynamic Renormalization Group to systems with long-range interactions
In this paper a mode of using the Dynamic Renormalization Group (DRG) method is suggested in order to cope with inconsistent results obtained when applying it to a continuous family of one-dimensional nonlocal models. The key observation is that the correct fixed-point dynamical system has to be identified during the analysis in order to account for all the relevant terms that are generated under renormalization. This is well established for static problems, however poorly implemented in dynamical ones. An application of this approach to a nonlocal extension of the Kardar-Parisi-Zhang equation resolves certain problems in one-dimension. Namely, obviously problematic predictions are eliminated and the existing exact analytic results are recovered.
cond-mat.stat-mech cond-mat.dis-nn math-ph math.MP
in this paper a mode of using the dynamic renormalization group drg method is suggested in order to cope with inconsistent results obtained when applying it to a continuous family of onedimensional nonlocal models the key observation is that the correct fixedpoint dynamical system has to be identified during the analysis in order to account for all the relevant terms that are generated under renormalization this is well established for static problems however poorly implemented in dynamical ones an application of this approach to a nonlocal extension of the kardarparisizhang equation resolves certain problems in onedimension namely obviously problematic predictions are eliminated and the existing exact analytic results are recovered
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710.4958
Thermodynamics of Protein Folding from Coarse-Grained Models' Perspectives
Folding and aggregation of proteins, the interaction between proteins and membranes, as well as the adsorption of organic soft matter to inorganic solid substrates belong to the most interesting challenges in understanding structure and function of complex macromolecules. This is reasoned by the interdisciplinary character of the associated questions ranging from the molecular origin of the loss of biological functionality as, for example, in Alzheimer's disease to the development of organic circuits for biosensory applications. In this lecture, we focus on the analysis of mesoscopic models for protein folding, aggregation, and hybrid systems of soft and solid condensed matter. The simplicity of the coarse-grained models allows for a more universal description of the notoriously difficult problem of protein folding. In this approach, classifications of structure formation processes with respect to the conformational pseudophases are possible. This is similar in aggregation and adsorption processes, where the individual folding propensity is influenced by external forces. The main problem in studies of conformational transitions is that the sequences of amino acids proteins are built up of are necessarily of finite length and, therefore, a thermodynamic limit does not exist. Thus, structural transitions are not phase transitions in the strict thermodynamic sense and the analysis of pseudouniversal aspects is intricate, as apparently small-system effects accompany all conformational transitions and cannot be neglected.
cond-mat.soft
folding and aggregation of proteins the interaction between proteins and membranes as well as the adsorption of organic soft matter to inorganic solid substrates belong to the most interesting challenges in understanding structure and function of complex macromolecules this is reasoned by the interdisciplinary character of the associated questions ranging from the molecular origin of the loss of biological functionality as for example in alzheimers disease to the development of organic circuits for biosensory applications in this lecture we focus on the analysis of mesoscopic models for protein folding aggregation and hybrid systems of soft and solid condensed matter the simplicity of the coarsegrained models allows for a more universal description of the notoriously difficult problem of protein folding in this approach classifications of structure formation processes with respect to the conformational pseudophases are possible this is similar in aggregation and adsorption processes where the individual folding propensity is influenced by external forces the main problem in studies of conformational transitions is that the sequences of amino acids proteins are built up of are necessarily of finite length and therefore a thermodynamic limit does not exist thus structural transitions are not phase transitions in the strict thermodynamic sense and the analysis of pseudouniversal aspects is intricate as apparently smallsystem effects accompany all conformational transitions and cannot be neglected
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710.4959
Outlook from SUSY07
Make-or-break time is near for the Higgs boson and supersymmetry. The LHC will soon put to the sword many theoretical ideas, and define the future for collider physics.
hep-ph
makeorbreak time is near for the higgs boson and supersymmetry the lhc will soon put to the sword many theoretical ideas and define the future for collider physics
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710.496
Freezing and Collapse of Flexible Polymers on Regular Lattices in Three Dimensions
We analyze the crystallization and collapse transition of a simple model for flexible polymer chains on simple cubic and face-centered cubic lattices by means of sophisticated chain-growth methods. In contrast to bond-fluctuation polymer models in certain parameter ranges, where these two conformational transitions were found to merge in the thermodynamic limit, we conclude from our results that the two transitions remain well-separated in the limit of infinite chain lengths. The reason for this qualitatively distinct behavior is presumably due to the ultrashort attractive interaction range in the lattice models considered here.
cond-mat.soft
we analyze the crystallization and collapse transition of a simple model for flexible polymer chains on simple cubic and facecentered cubic lattices by means of sophisticated chaingrowth methods in contrast to bondfluctuation polymer models in certain parameter ranges where these two conformational transitions were found to merge in the thermodynamic limit we conclude from our results that the two transitions remain wellseparated in the limit of infinite chain lengths the reason for this qualitatively distinct behavior is presumably due to the ultrashort attractive interaction range in the lattice models considered here
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710.4961
A Note on Graviton Amplitudes for New Twistor String Theories
A new class of twistor string theories were recently constructed by Abou-Zeid, Hull and Mason. The most interesting one of these theories has the particle content of N=8 supergravity. Arguments are given for the vanishing of the (+ - -)-helicity amplitude for gravitons which suggest that this theory describes a chiral N=8 supergravity rather than Einstein supergravity.
hep-th
a new class of twistor string theories were recently constructed by abouzeid hull and mason the most interesting one of these theories has the particle content of n8 supergravity arguments are given for the vanishing of the helicity amplitude for gravitons which suggest that this theory describes a chiral n8 supergravity rather than einstein supergravity
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710.4962
Connecting Galaxy Disk and Extended Halo Gas Kinematics
We have explored the galaxy disk/extended halo gas kinematic relationship using rotation curves (Keck/ESI) of ten intermediate redshift galaxies which were selected by MgII halo gas absorption observed in quasar spectra. Previous results of six edge-on galaxies, probed along their major axis, suggest that observed halo gas velocities are consistent with extended disk-like halo rotation at galactocentric distances of 25-72 kpc. Using our new sample, we demonstrate that the gas velocities are by and large not consistent with being directly coupled to the galaxy kinematics. Thus, mechanisms other than co-rotation dynamics (i.e., gas inflow, feedback, galaxy-galaxy interactions, etc.) must be invoked to account for the overall observed kinematics of the halo gas. In order to better understand the dynamic interaction of the galaxy/halo/cosmic web environment, we performed similar mock observations of galaxies and gaseous halos in Lambda-CDM cosmological simulations. We discuss an example case of a z=0.92 galaxy with various orientations probing halo gas at a range of positions. The gas dynamics inferred using simulated quasar absorption lines are consistent with observational data.
astro-ph
we have explored the galaxy diskextended halo gas kinematic relationship using rotation curves keckesi of ten intermediate redshift galaxies which were selected by mgii halo gas absorption observed in quasar spectra previous results of six edgeon galaxies probed along their major axis suggest that observed halo gas velocities are consistent with extended disklike halo rotation at galactocentric distances of 2572 kpc using our new sample we demonstrate that the gas velocities are by and large not consistent with being directly coupled to the galaxy kinematics thus mechanisms other than corotation dynamics ie gas inflow feedback galaxygalaxy interactions etc must be invoked to account for the overall observed kinematics of the halo gas in order to better understand the dynamic interaction of the galaxyhalocosmic web environment we performed similar mock observations of galaxies and gaseous halos in lambdacdm cosmological simulations we discuss an example case of a z092 galaxy with various orientations probing halo gas at a range of positions the gas dynamics inferred using simulated quasar absorption lines are consistent with observational data
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710.4963
Non Extensivity in Meteor Showers
A meteor shower is a luminous phenomenon that takes place by the entry into the Earths atmosphere of a cascade of particles coming from a stream intersected by our planet in its orbit. Here we investigate the possibility of a description of the mass distribution of meteoroids in meteor showers int terms of a non extensive formulation, which could shed light and give some insight into the origin of such particles.
cond-mat.stat-mech
a meteor shower is a luminous phenomenon that takes place by the entry into the earths atmosphere of a cascade of particles coming from a stream intersected by our planet in its orbit here we investigate the possibility of a description of the mass distribution of meteoroids in meteor showers int terms of a non extensive formulation which could shed light and give some insight into the origin of such particles
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710.4964
Cosmological Backreaction from Perturbations
We reformulate the averaged Einstein equations in a form suitable for use with Newtonian gauge linear perturbation theory and track the size of the modifications to standard Robertson-Walker evolution on the largest scales as a function of redshift for both Einstein de-Sitter and Lambda CDM cosmologies. In both cases the effective energy density arising from linear perturbations is of the order of 10^-5 the matter density, as would be expected, with an effective equation of state w ~ -1/19. Employing a modified Halofit code to extend our results to quasilinear scales, we find that, while larger, the deviations from Robertson-Walker behaviour remain of the order of 10^-5.
astro-ph gr-qc
we reformulate the averaged einstein equations in a form suitable for use with newtonian gauge linear perturbation theory and track the size of the modifications to standard robertsonwalker evolution on the largest scales as a function of redshift for both einstein desitter and lambda cdm cosmologies in both cases the effective energy density arising from linear perturbations is of the order of 105 the matter density as would be expected with an effective equation of state w 119 employing a modified halofit code to extend our results to quasilinear scales we find that while larger the deviations from robertsonwalker behaviour remain of the order of 105
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710.4965
On compositions of numbers and graphs
The main purpose of this note is to pose a couple of problems which are easily formulated thought some seem to be not yet solved. These problems are of general interest for discrete mathematics including a new twig of a bough of theory of graphs i.e. a given graph compositions. The problems result from and are served in the entourage of series of exercises with hints based predominantly on the second reference and other related recent papers.
math.CO cs.DM
the main purpose of this note is to pose a couple of problems which are easily formulated thought some seem to be not yet solved these problems are of general interest for discrete mathematics including a new twig of a bough of theory of graphs ie a given graph compositions the problems result from and are served in the entourage of series of exercises with hints based predominantly on the second reference and other related recent papers
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710.4966
Uncertainties of the antiproton flux from Dark Matter annihilation in comparison to the EGRET excess of diffuse gamma rays
The EGRET excess of diffuse Galactic gamma rays shows all the features expected from dark matter annihilation (DMA): a spectral shape given by the fragmentation of mono-energetic quarks, which is the same in all sky directions and an intensity distribution of the excess expected from a standard dark matter halo, predicted by the rotation curve. From the EGRET excess one can predict the flux of antiprotons from DMA. However, how many antiprotons arrive at the detector strongly depends on the propagation model. The conventional isotropic propagation models trap the antiprotons in the Galaxy leading to a local antiproton flux far above the observed flux. According to Bergstrom et. al. this excludes the DMA interpretation of the EGRET excess. Here it is shown that more realistic anisotropic propagation models, in which most antiprotons escape by fast transport in the z-direction, are consistent with the B/C ratio, the antiproton flux and the EGRET excess from DMA.
astro-ph
the egret excess of diffuse galactic gamma rays shows all the features expected from dark matter annihilation dma a spectral shape given by the fragmentation of monoenergetic quarks which is the same in all sky directions and an intensity distribution of the excess expected from a standard dark matter halo predicted by the rotation curve from the egret excess one can predict the flux of antiprotons from dma however how many antiprotons arrive at the detector strongly depends on the propagation model the conventional isotropic propagation models trap the antiprotons in the galaxy leading to a local antiproton flux far above the observed flux according to bergstrom et al this excludes the dma interpretation of the egret excess here it is shown that more realistic anisotropic propagation models in which most antiprotons escape by fast transport in the zdirection are consistent with the bc ratio the antiproton flux and the egret excess from dma
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710.4967
Black Holes in Supergravity: the non-BPS Branch
We construct extremal, spherically symmetric black hole solutions to 4D supergravity with charge assignments that preclude BPS-saturation. In particular, we determine the ground state energy as a function of charges and moduli. We find that the mass of the non-BPS black hole remains that of a marginal bound state of four basic constituents throughout the entire moduli space and that there is always a non-zero gap above the BPS bound.
hep-th
we construct extremal spherically symmetric black hole solutions to 4d supergravity with charge assignments that preclude bpssaturation in particular we determine the ground state energy as a function of charges and moduli we find that the mass of the nonbps black hole remains that of a marginal bound state of four basic constituents throughout the entire moduli space and that there is always a nonzero gap above the bps bound
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710.4968
Inversion of perturbation series
We investigate the inversion of perturbation series and its resummation, and prove that it is related to a recently developed parametric perturbation theory. Results for some illustrative examples show that in some cases series reversion may improve the accuracy of the results.
math-ph math.MP
we investigate the inversion of perturbation series and its resummation and prove that it is related to a recently developed parametric perturbation theory results for some illustrative examples show that in some cases series reversion may improve the accuracy of the results
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710.4969
A Near-Infrared Spectroscopic Study of the Accreting Magnetic White Dwarf SDSS J121209.31+013627.7 and its Substellar Companion
The nature of the excess near-infrared emission associated with the magnetic white dwarf commonly known as SDSS 1212 is investigated primarily through spectroscopy, and also via photometry. The inferred low mass secondary in this system has been previously detected by the emission and variation of H$\alpha$, and the $1-2.5$ $\mu$m spectral data presented here are consistent with the presence of a late L or early T dwarf. The excess flux seen beyond 1.5 $\mu$m in the phase-averaged spectrum is adequately modeled with an L8 dwarf substellar companion and cyclotron emission in a 7 MG magnetic field. This interesting system manifests several observational properties typical of polars, and is most likely an old interacting binary with a magnetic white dwarf and a substellar donor in an extended low state.
astro-ph
the nature of the excess nearinfrared emission associated with the magnetic white dwarf commonly known as sdss 1212 is investigated primarily through spectroscopy and also via photometry the inferred low mass secondary in this system has been previously detected by the emission and variation of halpha and the 125 mum spectral data presented here are consistent with the presence of a late l or early t dwarf the excess flux seen beyond 15 mum in the phaseaveraged spectrum is adequately modeled with an l8 dwarf substellar companion and cyclotron emission in a 7 mg magnetic field this interesting system manifests several observational properties typical of polars and is most likely an old interacting binary with a magnetic white dwarf and a substellar donor in an extended low state
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710.497
Explorando Sistemas Hamiltonianos II: A Natureza de Pontos de Equilibrio Degenerados
Neste segundo artigo sobre sistemas Hamiltonianos, apresentamos o metodo da explosao para a determinacao da natureza de pontos fixos (pontos de equilibrio degenerados. Aplicamos o metodo a dois modelos hamiltonianos com um e dois graus de liberdade, respectivamente. Primeiramente, analisamos um sistema formado por um pendulo simples submetido a um torque externo constante T. Em seguida, consideramos um sistema formado por um pendulo duplo com segmentos de comprimentos e massas iguais, tambem submetidos a torques externos constantes e nao nulos. A presenca de pontos de equilibrio degenerados nos casos dos pendulos simples e duplo ocorre para certos valores dos torques externos. In this second article on Hamiltonian systems, we present the blow-up method for the determination of the nature of degenerate fixed points (equilibrium points). We apply the method to two hamiltonian models with one and two degrees of freedom, respectively. Firstly we study a system formed by a simple pendulum submitted to a constant external torque T. Then we consider a system formed by a double pendulum of segments with equal lengths and masses, also submitted to non-vanishing constant external torques. The presence of degenerate equilibrium points in both cases of simple and double pendulums occurs for some values of the external torques.
math-ph math.MP
neste segundo artigo sobre sistemas hamiltonianos apresentamos o metodo da explosao para a determinacao da natureza de pontos fixos pontos de equilibrio degenerados aplicamos o metodo a dois modelos hamiltonianos com um e dois graus de liberdade respectivamente primeiramente analisamos um sistema formado por um pendulo simples submetido a um torque externo constante t em seguida consideramos um sistema formado por um pendulo duplo com segmentos de comprimentos e massas iguais tambem submetidos a torques externos constantes e nao nulos a presenca de pontos de equilibrio degenerados nos casos dos pendulos simples e duplo ocorre para certos valores dos torques externos in this second article on hamiltonian systems we present the blowup method for the determination of the nature of degenerate fixed points equilibrium points we apply the method to two hamiltonian models with one and two degrees of freedom respectively firstly we study a system formed by a simple pendulum submitted to a constant external torque t then we consider a system formed by a double pendulum of segments with equal lengths and masses also submitted to nonvanishing constant external torques the presence of degenerate equilibrium points in both cases of simple and double pendulums occurs for some values of the external torques
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710.4971
Limits of Gaudin algebras, quantization of bending flows, Jucys--Murphy elements and Gelfand--Tsetlin bases
Gaudin algebras form a family of maximal commutative subalgebras in the tensor product of $n$ copies of the universal enveloping algebra $U(\g)$ of a semisimple Lie algebra $\g$. This family is parameterized by collections of pairwise distinct complex numbers $z_1,...,z_n$. We obtain some new commutative subalgebras in $U(\g)^{\otimes n}$ as limit cases of Gaudin subalgebras. These commutative subalgebras turn to be related to the hamiltonians of bending flows and to the Gelfand--Tsetlin bases. We use this to prove the simplicity of spectrum in the Gaudin model for some new cases.
math.QA hep-th nlin.SI
gaudin algebras form a family of maximal commutative subalgebras in the tensor product of n copies of the universal enveloping algebra ug of a semisimple lie algebra g this family is parameterized by collections of pairwise distinct complex numbers z_1z_n we obtain some new commutative subalgebras in ugotimes n as limit cases of gaudin subalgebras these commutative subalgebras turn to be related to the hamiltonians of bending flows and to the gelfandtsetlin bases we use this to prove the simplicity of spectrum in the gaudin model for some new cases
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710.4972
Nonlinear polarisation and dissipative correspondence between low frequency fluid and gyrofluid equations
The correspondence between gyrofluid and low frequency fluid equations is examined. The lowest order conservative effects in ExB advection, parallel dynamics, and curvature match trivially. The principal concerns are polarisation fluxes, and dissipative parallel viscosity and parallel heat fluxes. The emergence of the polarisation heat flux in the fluid model and its contribution to the energy theorem is reviewed. It is shown that gyroviscosity and the polarisation fluxes are matched by the finite gyroradius corrections to advection in the long wavelength limit, provided that the differences between gyrocenter and particle representations is taken into account. The dissipative parallel viscosity is matched by the residual thermal anisotropy in the gyrofluid model in the collision dominated limit. The dissipative parallel heat flux is matched by the gyrofluid parallel heat flux variables in the collision dominated limit. Hence, the gyrofluid equations are a complete superset of the low frequency fluid equations.
physics.plasm-ph
the correspondence between gyrofluid and low frequency fluid equations is examined the lowest order conservative effects in exb advection parallel dynamics and curvature match trivially the principal concerns are polarisation fluxes and dissipative parallel viscosity and parallel heat fluxes the emergence of the polarisation heat flux in the fluid model and its contribution to the energy theorem is reviewed it is shown that gyroviscosity and the polarisation fluxes are matched by the finite gyroradius corrections to advection in the long wavelength limit provided that the differences between gyrocenter and particle representations is taken into account the dissipative parallel viscosity is matched by the residual thermal anisotropy in the gyrofluid model in the collision dominated limit the dissipative parallel heat flux is matched by the gyrofluid parallel heat flux variables in the collision dominated limit hence the gyrofluid equations are a complete superset of the low frequency fluid equations
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710.4973
Liquid crystal anchoring transitions on aligning substrates processed by plasma beam
We observe a sequence of the anchoring transitions in nematic liquid crystals (NLC) sandwiched between the hydrophobic polyimide substrates treated with the plasma beam. There is a pronounced continuous transition from homeotropic to low tilted (nearly planar) alignment with the easy axis parallel to the incidence plane of the plasma beam (the zenithal transition) that takes place as the exposure dose increases. In NLC with positive dielectric anisotropy, a further increase in the exposure dose results in in-plane reorientation of the easy axis by 90 degrees (the azimuthal transition). This transition occurs through the two-fold degenerated alignment characteristic for the second order anchoring transitions. In contrast to critical behavior of anchoring, the contact angle of NLC and water on the treated substrates monotonically declines with the exposure dose. It follows that the surface concentration of hydrophobic chains decreases continuously. The anchoring transitions under consideration are qualitatively interpreted by using a simple phenomenological model of competing easy axes which is studied by analyzing anchoring diagrams of the generalized polar and non-polar anchoring models.
cond-mat.mtrl-sci cond-mat.soft
we observe a sequence of the anchoring transitions in nematic liquid crystals nlc sandwiched between the hydrophobic polyimide substrates treated with the plasma beam there is a pronounced continuous transition from homeotropic to low tilted nearly planar alignment with the easy axis parallel to the incidence plane of the plasma beam the zenithal transition that takes place as the exposure dose increases in nlc with positive dielectric anisotropy a further increase in the exposure dose results in inplane reorientation of the easy axis by 90 degrees the azimuthal transition this transition occurs through the twofold degenerated alignment characteristic for the second order anchoring transitions in contrast to critical behavior of anchoring the contact angle of nlc and water on the treated substrates monotonically declines with the exposure dose it follows that the surface concentration of hydrophobic chains decreases continuously the anchoring transitions under consideration are qualitatively interpreted by using a simple phenomenological model of competing easy axes which is studied by analyzing anchoring diagrams of the generalized polar and nonpolar anchoring models
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710.4974
Measurement of CP Asymmetries and Branching Fractions in a Time-Dependent Dalitz Analysis of B^0-->(rho pi)^0 and a Constraint on the Quark Mixing Angle phi_2
We present the results of a time-dependent Dalitz plot analysis of B0 --> pi+ pi- pi0 decays based on a 414/fb data sample that contains 449 x 10^6 BB pairs. The data was collected on the Upsilon(4S) resonance with the Belle detector at the KEKB asymmetric energy e+e- collider. Combining our analysis with information on charged B decay modes, we perform a full Dalitz and isospin analysis and obtain a constraint on the quark mixing angle phi_2, 68deg. < phi_2 < 95deg. at the 68.3% confidence level for the phi_2 solution consistent with the standard model (SM). A large SM-disfavored region also remains. The branching fractions for the decay processes of B0 --> rho+-(770) pi-+ and B0 --> rho0(770) pi0 are measured to be (22.6 +- 1.1[stat.] +- 4.4 [syst.]) x 10^{-6} and (3.0 +- 0.5 [stat.] +- 0.7 [syst.]) x 10^{-6}, respectively. These are the first branching fraction measurements of the process B0 --> rho(770)pi with the lowest resonance rho(770) explicitly separated from the radial excitations.
hep-ex
we present the results of a timedependent dalitz plot analysis of b0 pi pi pi0 decays based on a 414fb data sample that contains 449 x 106 bb pairs the data was collected on the upsilon4s resonance with the belle detector at the kekb asymmetric energy ee collider combining our analysis with information on charged b decay modes we perform a full dalitz and isospin analysis and obtain a constraint on the quark mixing angle phi_2 68deg phi_2 95deg at the 683 confidence level for the phi_2 solution consistent with the standard model sm a large smdisfavored region also remains the branching fractions for the decay processes of b0 rho770 pi and b0 rho0770 pi0 are measured to be 226 11stat 44 syst x 106 and 30 05 stat 07 syst x 106 respectively these are the first branching fraction measurements of the process b0 rho770pi with the lowest resonance rho770 explicitly separated from the radial excitations
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710.4975
Node discovery problem for a social network
Methods to solve a node discovery problem for a social network are presented. Covert nodes refer to the nodes which are not observable directly. They transmit the influence and affect the resulting collaborative activities among the persons in a social network, but do not appear in the surveillance logs which record the participants of the collaborative activities. Discovering the covert nodes is identifying the suspicious logs where the covert nodes would appear if the covert nodes became overt. The performance of the methods is demonstrated with a test dataset generated from computationally synthesized networks and a real organization.
cs.AI
methods to solve a node discovery problem for a social network are presented covert nodes refer to the nodes which are not observable directly they transmit the influence and affect the resulting collaborative activities among the persons in a social network but do not appear in the surveillance logs which record the participants of the collaborative activities discovering the covert nodes is identifying the suspicious logs where the covert nodes would appear if the covert nodes became overt the performance of the methods is demonstrated with a test dataset generated from computationally synthesized networks and a real organization
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710.4976
q-Bernoulli numbers and Stirling numbers(2)
In this paper we study q-Bernoulli numbers and polynomials related to q-Stirling numbers. From thsese studying we investigate some interesting q-stirling numbers' identities related to q-Bernoulli numbers.
math.NT
in this paper we study qbernoulli numbers and polynomials related to qstirling numbers from thsese studying we investigate some interesting qstirling numbers identities related to qbernoulli numbers
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710.4977
An ab initio full potential fully relativistic study of atomic carbon, nitrogen, and oxygen chemisorption on the (111) surface of delta-plutonium
Adsorption of carbon, nitrogen, and oxygen on the (111) surface of delta-Plutonium has been studied within the framework of density functional theory using the full-potential linear augmented plane wave plus local basis (FP-LAPW+lo) method. All adatoms prefer to bind at the higher coordinated hollow sites, with the chemisorption energies for C, N, and O being 6.539 eV, 6.714 eV, and 8.2 eV respectively. The work function and the surface Pu magnetic moments respectively increased and decreased in all cases upon chemisorption. The partial charges inside the muffin tins spheres, difference charge density distributions, and the local density of states have been used to analyze the Pu-adatom bond interactions.
cond-mat.str-el cond-mat.mtrl-sci
adsorption of carbon nitrogen and oxygen on the 111 surface of deltaplutonium has been studied within the framework of density functional theory using the fullpotential linear augmented plane wave plus local basis fplapwlo method all adatoms prefer to bind at the higher coordinated hollow sites with the chemisorption energies for c n and o being 6539 ev 6714 ev and 82 ev respectively the work function and the surface pu magnetic moments respectively increased and decreased in all cases upon chemisorption the partial charges inside the muffin tins spheres difference charge density distributions and the local density of states have been used to analyze the puadatom bond interactions
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710.4978
Limits of log canonical thresholds
Let T_n denote the set of log canonical thresholds of pairs (X,Y), with X a nonsingular variety of dimension n, and Y a nonempty closed subscheme of X. Using non-standard methods, we show that every limit of a decreasing sequence in T_n lies in T_{n-1}, proving in this setting a conjecture of Koll\'{a}r. We also show that T_n is a closed subset in the set of real numbers; in particular, every limit of log canonical thresholds on smooth varieties of fixed dimension is a rational number. As a consequence of this property, we see that in order to check Shokurov's ACC Conjecture for all T_n, it is enough to show that 1 is not a point of accumulation from below of any T_n. In a different direction, we interpret the ACC Conjecture as a semi-continuity property for log canonical thresholds of formal power series.
math.AG
let t_n denote the set of log canonical thresholds of pairs xy with x a nonsingular variety of dimension n and y a nonempty closed subscheme of x using nonstandard methods we show that every limit of a decreasing sequence in t_n lies in t_n1 proving in this setting a conjecture of kollar we also show that t_n is a closed subset in the set of real numbers in particular every limit of log canonical thresholds on smooth varieties of fixed dimension is a rational number as a consequence of this property we see that in order to check shokurovs acc conjecture for all t_n it is enough to show that 1 is not a point of accumulation from below of any t_n in a different direction we interpret the acc conjecture as a semicontinuity property for log canonical thresholds of formal power series
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710.4979
High power radially polarized light generated from photonic crystal segmented half-wave-plate
We have generated more than 100 watts of radial polarized beam from a Yb fiber laser using a photonics crystal segmented half-wave-plate. We demonstrated the high power handling capability of such a photonics crystal segmented half-wave-plate and show that it is a promising external radial polarization converter for high power Yb fiber laser used in laser cutting industry.
physics.optics
we have generated more than 100 watts of radial polarized beam from a yb fiber laser using a photonics crystal segmented halfwaveplate we demonstrated the high power handling capability of such a photonics crystal segmented halfwaveplate and show that it is a promising external radial polarization converter for high power yb fiber laser used in laser cutting industry
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710.498
Entangling the optical frequency comb: simultaneous generation of multiple 2x2 and 2x3 continuous-variable cluster states in a single optical parametric oscillator
We report on our research effort to generate large-scale multipartite optical-mode entanglement using as few physical resources as possible. We have previously shown that cluster- and GHZ-type N-partite continuous-variable entanglement can be obtained in an optical resonator that contains a suitably designed second-order nonlinear optical medium, pumped by at most O(N^2) fields. In this paper, we show that the frequency comb of such a resonator can be entangled into an arbitrary number of independent 2x2 and 2x3 continuous-variable cluster states by a single optical parametric oscillator pumped by just a few optical modes.
quant-ph
we report on our research effort to generate largescale multipartite opticalmode entanglement using as few physical resources as possible we have previously shown that cluster and ghztype npartite continuousvariable entanglement can be obtained in an optical resonator that contains a suitably designed secondorder nonlinear optical medium pumped by at most on2 fields in this paper we show that the frequency comb of such a resonator can be entangled into an arbitrary number of independent 2x2 and 2x3 continuousvariable cluster states by a single optical parametric oscillator pumped by just a few optical modes
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710.4981
A note on the p-adic log-gamma functions
In this paper we prove that q-Euler numbers are occured in the coefficients of some stirling type seies for p-adic analytic q-log gamma function
math.NT
in this paper we prove that qeuler numbers are occured in the coefficients of some stirling type seies for padic analytic qlog gamma function
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710.4982
First to Market is not Everything: an Analysis of Preferential Attachment with Fitness
In this paper, we provide a rigorous analysis of preferential attachment with fitness, a random graph model introduced by Bianconi and Barabasi. Depending on the shape of the fitness distribution, we observe three distinct phases: a first-mover-advantage phase, a fit-get-richer phase and an innovation-pays-off phase.
math.PR cs.SI
in this paper we provide a rigorous analysis of preferential attachment with fitness a random graph model introduced by bianconi and barabasi depending on the shape of the fitness distribution we observe three distinct phases a firstmoveradvantage phase a fitgetricher phase and an innovationpaysoff phase
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710.4983
Electroweak and Top Physics at the Tevatron and Indirect Higgs Limits
We report a selection of the most recent CDF and D0 results on top quark and W and Z boson properties, based on Tevatron Run 2 data. The large datasets of W and Z bosons allow a very precise measurement of the W mass and detailed studies of vector boson production and asymmetries. Associated production of vector boson pairs has been observed and cross sections have been measured. The top quark is being studied in great detail, and a precision of 1.1 % in the measurement of its mass has been achieved. The precise knowledge of top and W masses are constraining the allowed mass range of a standard model Higgs in an unprecedented way.
hep-ex
we report a selection of the most recent cdf and d0 results on top quark and w and z boson properties based on tevatron run 2 data the large datasets of w and z bosons allow a very precise measurement of the w mass and detailed studies of vector boson production and asymmetries associated production of vector boson pairs has been observed and cross sections have been measured the top quark is being studied in great detail and a precision of 11 in the measurement of its mass has been achieved the precise knowledge of top and w masses are constraining the allowed mass range of a standard model higgs in an unprecedented way
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710.4984
Josephson Current and Multiple Andreev Reflections in Graphene SNS Junctions
The Josephson Effect and Superconducting Proximity Effect were observed in Superconductor -Graphene-Superconductor (SGS) Josephson junctions with coherence lengths comparable to the distance between the superconducting leads. By comparing the measured temperature and doping dependence of the supercurrent and the proximity induced sub-gap features (multiple Andreev reflections) to theoretical predictions we find that, contrary to expectations, the ballistic transport model fails to describe the SGS junctions. In contrast, the diffusive junction model yields close quantitative agreement with the results. This conclusion is consistent with transport measurements in the normal state, which yield mean free paths in the graphene link that are much shorter than the junction length. We show that all devices fabricated on SiO2 substrates so far (our own as well as those reported by other groups) fall in the diffusive junction category.
cond-mat.mes-hall cond-mat.supr-con
the josephson effect and superconducting proximity effect were observed in superconductor graphenesuperconductor sgs josephson junctions with coherence lengths comparable to the distance between the superconducting leads by comparing the measured temperature and doping dependence of the supercurrent and the proximity induced subgap features multiple andreev reflections to theoretical predictions we find that contrary to expectations the ballistic transport model fails to describe the sgs junctions in contrast the diffusive junction model yields close quantitative agreement with the results this conclusion is consistent with transport measurements in the normal state which yield mean free paths in the graphene link that are much shorter than the junction length we show that all devices fabricated on sio2 substrates so far our own as well as those reported by other groups fall in the diffusive junction category
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710.4985
A new multi-component CKP hierarchy
We construct a new multi-component CKP hierarchy based on the eigenfunction symmetry reduction. It contains two types of CKP equation with self-consistent sources which Lax representations are presented. Also it admits reductions to $k$-constrained CKP hierarchy and to a (1+1)-dimensional soliton hierarchy with self-consistent source, which include two types of Kaup-Kuperschmidt equation with self-consistent sources and of bi-directional Kaup-Kuperschmidt equation with self-consistent sources.
nlin.SI
we construct a new multicomponent ckp hierarchy based on the eigenfunction symmetry reduction it contains two types of ckp equation with selfconsistent sources which lax representations are presented also it admits reductions to kconstrained ckp hierarchy and to a 11dimensional soliton hierarchy with selfconsistent source which include two types of kaupkuperschmidt equation with selfconsistent sources and of bidirectional kaupkuperschmidt equation with selfconsistent sources
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710.4986
Axisymmetric toroidal modes of magnetized neutron stars
We calculate axisymmetric toroidal modes of magnetized neutron stars with a solid crust. We assume the interior of the star is threaded by a poloidal magnetic field that is continuous at the surface with the outside dipole field whose strength $B_p$ at the magnetic pole is $B_p\sim 10^{16}$G. Since separation of variables is not possible for oscillations of magnetized stars, we employ finite series expansions of the perturbations using spherical harmonic functions to represent the angular dependence of the oscillation modes. For $B_p\sim 10^{16}$G, we find distinct mode sequences, in each of which the oscillation frequency of the toroidal mode slowly increases as the number of radial nodes of the eigenfunction increases. The frequency spectrum of the toroidal modes for $B_p\sim 10^{16}$G is largely different from that of the crustal toroidal modes of the non-magnetized model, although the frequency ranges are overlapped each other. This suggests that an interpretation of the observed QPOs based on the magnetic toroidal modes may be possible if the field strength of the star is as strong as $B_p\sim 10^{16}$G.
astro-ph
we calculate axisymmetric toroidal modes of magnetized neutron stars with a solid crust we assume the interior of the star is threaded by a poloidal magnetic field that is continuous at the surface with the outside dipole field whose strength b_p at the magnetic pole is b_psim 1016g since separation of variables is not possible for oscillations of magnetized stars we employ finite series expansions of the perturbations using spherical harmonic functions to represent the angular dependence of the oscillation modes for b_psim 1016g we find distinct mode sequences in each of which the oscillation frequency of the toroidal mode slowly increases as the number of radial nodes of the eigenfunction increases the frequency spectrum of the toroidal modes for b_psim 1016g is largely different from that of the crustal toroidal modes of the nonmagnetized model although the frequency ranges are overlapped each other this suggests that an interpretation of the observed qpos based on the magnetic toroidal modes may be possible if the field strength of the star is as strong as b_psim 1016g
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710.4987
Universal source coding over generalized complementary delivery networks
This paper deals with a universal coding problem for a certain kind of multiterminal source coding network called a generalized complementary delivery network. In this network, messages from multiple correlated sources are jointly encoded, and each decoder has access to some of the messages to enable it to reproduce the other messages. Both fixed-to-fixed length and fixed-to-variable length lossless coding schemes are considered. Explicit constructions of universal codes and the bounds of the error probabilities are clarified by using methods of types and graph-theoretical analysis.
cs.IT math.IT
this paper deals with a universal coding problem for a certain kind of multiterminal source coding network called a generalized complementary delivery network in this network messages from multiple correlated sources are jointly encoded and each decoder has access to some of the messages to enable it to reproduce the other messages both fixedtofixed length and fixedtovariable length lossless coding schemes are considered explicit constructions of universal codes and the bounds of the error probabilities are clarified by using methods of types and graphtheoretical analysis
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710.4988
Inter-vehicle gap statistics on signal-controlled crossroads
We investigate a microscopical structure in a chain of cars waiting at a red signal on signal-controlled crossroads. Presented is an one-dimensional space-continuous thermodynamical model leading to an excellent agreement with the data measured.Moreover, we demonstrate that an inter-vehicle spacing distribution disclosed in relevant traffic data agrees with the thermal-balance distribution of particles in the thermodynamical traffic gas (discussed in [1]) with a high inverse temperature (corresponding to a strong traffic congestion). Therefore, as we affirm, such a system of stationary cars can be understood as a specific state of the traffic sample operating inside a congested traffic stream.
nlin.AO
we investigate a microscopical structure in a chain of cars waiting at a red signal on signalcontrolled crossroads presented is an onedimensional spacecontinuous thermodynamical model leading to an excellent agreement with the data measuredmoreover we demonstrate that an intervehicle spacing distribution disclosed in relevant traffic data agrees with the thermalbalance distribution of particles in the thermodynamical traffic gas discussed in 1 with a high inverse temperature corresponding to a strong traffic congestion therefore as we affirm such a system of stationary cars can be understood as a specific state of the traffic sample operating inside a congested traffic stream
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710.4989
Exact minimum and maximum of yield with a finite number of decoy light intensities
In this paper, for the decoy state method using a finite number of decoy light intensities, we present an improved upper and lower bounds for the asymptotic yield y_n for n-photon states. In particular if all the light intensities are less than or equal to one, they are not only a lower or upper bound, but in fact are the exact minimum or maximum.
quant-ph
in this paper for the decoy state method using a finite number of decoy light intensities we present an improved upper and lower bounds for the asymptotic yield y_n for nphoton states in particular if all the light intensities are less than or equal to one they are not only a lower or upper bound but in fact are the exact minimum or maximum
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710.499
Exploring the High-Energy Cosmic Ray Spectrum with a Toy Model of Cosmic Ray Diffusion
We introduce a static toy model of the cosmic ray (CR) universe in which cosmic ray propagation is taken to be diffusive and cosmic ray sources are distributed randomly with a density the same as that of local L* galaxies, $5 \times 10^{-3}$ Mpc$^{-3}$. These sources "fire" at random times through the history of the universe but with a set expectation time for the period between bursts. Our toy model model captures much of the essential CR physics despite its simplicity and, moreover, broadly reproduces CR phenomenology for reasonable parameter values and without extreme fine-tuning. Using this model we investigate -- and find tenable -- the idea that the Milky Way may itself be a typical high-energy cosmic ray source. We also consider the possible phenomenological implications of the magnetic CR horizon for the overall cosmic ray spectrum observed at Earth. Finally, we show that anisotropy studies should most profitably focus on cosmic rays detected at energies above the so-called GZK cut-off, $\sim 6 \times 10^{19}$ eV.
astro-ph
we introduce a static toy model of the cosmic ray cr universe in which cosmic ray propagation is taken to be diffusive and cosmic ray sources are distributed randomly with a density the same as that of local l galaxies 5 times 103 mpc3 these sources fire at random times through the history of the universe but with a set expectation time for the period between bursts our toy model model captures much of the essential cr physics despite its simplicity and moreover broadly reproduces cr phenomenology for reasonable parameter values and without extreme finetuning using this model we investigate and find tenable the idea that the milky way may itself be a typical highenergy cosmic ray source we also consider the possible phenomenological implications of the magnetic cr horizon for the overall cosmic ray spectrum observed at earth finally we show that anisotropy studies should most profitably focus on cosmic rays detected at energies above the socalled gzk cutoff sim 6 times 1019 ev
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710.4991
The Fifteen Theorem for Universal Hermitian Lattices over Imaginary Quadratic Fields
We will introduce a method to get all universal Hermitian lattices over imaginary quadratic fields over $\mathbb{Q}(\sqrt{-m})$ for all m. For each imaginary quadratic field $\mathbb{Q}(\sqrt{-m})$, we obtain a criterion on universality of Hermitian lattices: if a Hermitian lattice L represents 1, 2, 3, 5, 6, 7, 10, 13,14 and 15, then L is universal. We call this the fifteen theorem for universal Hermitian lattices. Note that the difference between Conway-Schneeberger's fifteen theorem and ours is the number 13.
math.NT
we will introduce a method to get all universal hermitian lattices over imaginary quadratic fields over mathbbqsqrtm for all m for each imaginary quadratic field mathbbqsqrtm we obtain a criterion on universality of hermitian lattices if a hermitian lattice l represents 1 2 3 5 6 7 10 1314 and 15 then l is universal we call this the fifteen theorem for universal hermitian lattices note that the difference between conwayschneebergers fifteen theorem and ours is the number 13
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710.4992
Nonminimal isotropic cosmological model with Yang-Mills and Higgs fields
We establish a nonminimal Einstein-Yang-Mills-Higgs model, which contains six coupling parameters. First three parameters relate to the nonminimal coupling of non-Abelian gauge field and gravity field, two parameters describe the so-called derivative nonminimal coupling of scalar multiplet with gravity field, and the sixth parameter introduces the standard coupling of scalar field with Ricci scalar. The formulated six-parameter nonminimal Einstein-Yang-Mills-Higgs model is applied to cosmology. We show that there exists a unique exact cosmological solution of the de Sitter type for a special choice of the coupling parameters. The nonminimally extended Yang-Mills and Higgs equations are satisfied for arbitrary gauge and scalar fields, when the coupling parameters are specifically related to the curvature constant of the isotropic spacetime. Basing on this special exact solution we discuss the problem of a hidden anisotropy of the Yang-Mills field, and give an explicit example, when the nonminimal coupling effectively screens the anisotropy induced by the Yang-Mills field and thus restores the isotropy of the model.
gr-qc astro-ph hep-th
we establish a nonminimal einsteinyangmillshiggs model which contains six coupling parameters first three parameters relate to the nonminimal coupling of nonabelian gauge field and gravity field two parameters describe the socalled derivative nonminimal coupling of scalar multiplet with gravity field and the sixth parameter introduces the standard coupling of scalar field with ricci scalar the formulated sixparameter nonminimal einsteinyangmillshiggs model is applied to cosmology we show that there exists a unique exact cosmological solution of the de sitter type for a special choice of the coupling parameters the nonminimally extended yangmills and higgs equations are satisfied for arbitrary gauge and scalar fields when the coupling parameters are specifically related to the curvature constant of the isotropic spacetime basing on this special exact solution we discuss the problem of a hidden anisotropy of the yangmills field and give an explicit example when the nonminimal coupling effectively screens the anisotropy induced by the yangmills field and thus restores the isotropy of the model
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710.4993
Dark Energy may link the numbers of Rees
There is increasing evidence that the universe is dominated by dark energy of the type given by an invariant cosmological constant. Latest data also indicates that fundamental interaction couplings and particle masses have remained remarkably constant from the earliest epochs. It is natural to connect these two steady state features of the evolving universe, suggesting a role for the cosmic vacuum energy in fixing these interaction constants. Advances in high precision cosmology have revealed that dark matter of an unknown type constitutes about one-fourth of cosmic matter while baryons account for just four percent. These various cosmic parameters are enumerated by the six numbers of Rees. With the dark energy as a unifying link these
astro-ph
there is increasing evidence that the universe is dominated by dark energy of the type given by an invariant cosmological constant latest data also indicates that fundamental interaction couplings and particle masses have remained remarkably constant from the earliest epochs it is natural to connect these two steady state features of the evolving universe suggesting a role for the cosmic vacuum energy in fixing these interaction constants advances in high precision cosmology have revealed that dark matter of an unknown type constitutes about onefourth of cosmic matter while baryons account for just four percent these various cosmic parameters are enumerated by the six numbers of rees with the dark energy as a unifying link these
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710.4994
Tau polarization in SUSY cascade decays at LHC
We explore how the polarization of the tau leptons in the cascade decay $\tilde{q}\to q\tilde\chi^0_2\to q\tau\tilde\tau\to q\tau\tau\tilde\chi^0_1$ can be exploited to study mixing properties of neutralinos and staus. We present details of the analysis including experimental effects such as transverse momentum cuts for the $\tau\to\pi\nu$ decay mode, and show that the di-pion invariant mass distribution provides valuable information on their properties.
hep-ph
we explore how the polarization of the tau leptons in the cascade decay tildeqto qtildechi0_2to qtautildetauto qtautautildechi0_1 can be exploited to study mixing properties of neutralinos and staus we present details of the analysis including experimental effects such as transverse momentum cuts for the tautopinu decay mode and show that the dipion invariant mass distribution provides valuable information on their properties
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710.4995
Toeplitz Operators, K\"ahler Manifolds, and Line Bundles
This is a survey paper. We discuss Toeplitz operators in K\"ahler geometry, with applications to geometric quantization, and review some recent developments.
math.SG math.CV
this is a survey paper we discuss toeplitz operators in kahler geometry with applications to geometric quantization and review some recent developments
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710.4996
Large scale dynamics of the Persistent Turning Walker model of fish behavior
This paper considers a new model of individual displacement, based on fish motion, the so-called Persistent Turning Walker (PTW) model, which involves an Ornstein-Uhlenbeck process on the curvature of the particle trajectory. The goal is to show that its large time and space scale dynamics is of diffusive type, and to provide an analytic expression of the diffusion coefficient. Two methods are investigated. In the first one, we compute the large time asymptotics of the variance of the individual stochastic trajectories. The second method is based on a diffusion approximation of the kinetic formulation of these stochastic trajectories. The kinetic model is a Fokker-Planck type equation posed in an extended phase-space involving the curvature among the kinetic variables. We show that both methods lead to the same value of the diffusion constant. We present some numerical simulations to illustrate the theoretical results.
math-ph math.MP
this paper considers a new model of individual displacement based on fish motion the socalled persistent turning walker ptw model which involves an ornsteinuhlenbeck process on the curvature of the particle trajectory the goal is to show that its large time and space scale dynamics is of diffusive type and to provide an analytic expression of the diffusion coefficient two methods are investigated in the first one we compute the large time asymptotics of the variance of the individual stochastic trajectories the second method is based on a diffusion approximation of the kinetic formulation of these stochastic trajectories the kinetic model is a fokkerplanck type equation posed in an extended phasespace involving the curvature among the kinetic variables we show that both methods lead to the same value of the diffusion constant we present some numerical simulations to illustrate the theoretical results
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710.4997
Age-structured Trait Substitution Sequence Process and Canonical Equation
We are interested in a stochastic model of trait and age-structured population undergoing mutation and selection. We start with a continuous time, discrete individual-centered population process. Taking the large population and rare mutations limits under a well-chosen time-scale separation condition, we obtain a jump process that generalizes the Trait Substitution Sequence process describing Adaptive Dynamics for populations without age structure. Under the additional assumption of small mutations, we derive an age-dependent ordinary differential equation that extends the Canonical Equation. These evolutionary approximations have never been introduced to our knowledge. They are based on ecological phenomena represented by PDEs that generalize the Gurtin-McCamy equation in Demography. Another particularity is that they involve a fitness function, describing the probability of invasion of the resident population by the mutant one, that can not always be computed explicitly. Examples illustrate how adding an age-structure enrich the modelling of structured population by including life history features such as senescence. In the cases considered, we establish the evolutionary approximations and study their long time behavior and the nature of their evolutionary singularities when computation is tractable. Numerical procedures and simulations are carried.
math.PR q-bio.PE
we are interested in a stochastic model of trait and agestructured population undergoing mutation and selection we start with a continuous time discrete individualcentered population process taking the large population and rare mutations limits under a wellchosen timescale separation condition we obtain a jump process that generalizes the trait substitution sequence process describing adaptive dynamics for populations without age structure under the additional assumption of small mutations we derive an agedependent ordinary differential equation that extends the canonical equation these evolutionary approximations have never been introduced to our knowledge they are based on ecological phenomena represented by pdes that generalize the gurtinmccamy equation in demography another particularity is that they involve a fitness function describing the probability of invasion of the resident population by the mutant one that can not always be computed explicitly examples illustrate how adding an agestructure enrich the modelling of structured population by including life history features such as senescence in the cases considered we establish the evolutionary approximations and study their long time behavior and the nature of their evolutionary singularities when computation is tractable numerical procedures and simulations are carried
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710.4998
Binary normal regular Hermitian lattices over imaginary quadratic fields
We call a positive definite Hermitian lattice regular if it represents all integers which can be represented locally by the lattice. We investigate binary regular Hermitian lattices over imaginary quadratic fields $\mathbb{Q}(\sqrt{-m})$ and provide a complete list of the (normal) Hermitian lattices.
math.NT
we call a positive definite hermitian lattice regular if it represents all integers which can be represented locally by the lattice we investigate binary regular hermitian lattices over imaginary quadratic fields mathbbqsqrtm and provide a complete list of the normal hermitian lattices
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710.4999
L'analyse de l'expertise du point de vue de l'ergonomie cognitive
This paper presents a review of methods for collecting and analysing data on complex activities. Starting with methods developed for design, we examine the possibility to transpose them to other complex activities, especially activities referring to sensorial expertise. R\'esum\'e Ce texte pr\'esente une revue de m\'ethodes pour recueillir et analyser des donn\'ees sur des actvit\'es complexes. A partir de m\'ethodes d\'evelopp\'ees pour des actvit\'es de conception, nous examinons la possibilit\'e de les transposer \`a d'autres actvit\'es complexes, notamment des actvit\'es faisant \`a appel \`a des expertises sensorielles.
cs.HC
this paper presents a review of methods for collecting and analysing data on complex activities starting with methods developed for design we examine the possibility to transpose them to other complex activities especially activities referring to sensorial expertise resume ce texte presente une revue de methodes pour recueillir et analyser des donnees sur des actvites complexes a partir de methodes developpees pour des actvites de conception nous examinons la possibilite de les transposer a dautres actvites complexes notamment des actvites faisant a appel a des expertises sensorielles
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710.5
Diagrammatic quantum field formalism for localized electrons
We introduce a diagrammatic quantum field formalism for the evaluation of normalized expectation values of operators, and suitable for systems with localized electrons. It is used to develop a convergent series expansion for the energy in powers of overlap integrals of single-particle orbitals. This method gives intuitive and practical rules for writing down the expansion to arbitrary order of overlap, and can be applied to any spin configuration and to any dimension. Its applicability for systems with well localized electrons has been illustrated with examples, including the two-dimensional Wigner crystal and spin-singlets in the low-density electron gas.
cond-mat.other
we introduce a diagrammatic quantum field formalism for the evaluation of normalized expectation values of operators and suitable for systems with localized electrons it is used to develop a convergent series expansion for the energy in powers of overlap integrals of singleparticle orbitals this method gives intuitive and practical rules for writing down the expansion to arbitrary order of overlap and can be applied to any spin configuration and to any dimension its applicability for systems with well localized electrons has been illustrated with examples including the twodimensional wigner crystal and spinsinglets in the lowdensity electron gas
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710.5001
Anisotropic inharmonic Higgs oscillator and related (MICZ-)Kepler-like systems
We propose the integrable (pseudo)spherical generalization of the four-dimensional anisotropic oscillator with additional nonlinear potential. Performing its Kustaanheimo-Stiefel transformation we then obtain the pseudospherical generalization of the MICZ-Kepler system with linear and $\cos\theta$ potential terms. We also present the generalization of the parabolic coordinates, in which this system admits the separation of variables. Finally, we get the spherical analog of the presented MICZ-Kepler-like system.
math-ph hep-th math.MP quant-ph
we propose the integrable pseudospherical generalization of the fourdimensional anisotropic oscillator with additional nonlinear potential performing its kustaanheimostiefel transformation we then obtain the pseudospherical generalization of the miczkepler system with linear and costheta potential terms we also present the generalization of the parabolic coordinates in which this system admits the separation of variables finally we get the spherical analog of the presented miczkeplerlike system
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710.5002
The entropy of keys derived from laser speckle
Laser speckle has been proposed in a number of papers as a high-entropy source of unpredictable bits for use in security applications. Bit strings derived from speckle can be used for a variety of security purposes such as identification, authentication, anti-counterfeiting, secure key storage, random number generation and tamper protection. The choice of laser speckle as a source of random keys is quite natural, given the chaotic properties of speckle. However, this same chaotic behaviour also causes reproducibility problems. Cryptographic protocols require either zero noise or very low noise in their inputs; hence the issue of error rates is critical to applications of laser speckle in cryptography. Most of the literature uses an error reduction method based on Gabor filtering. Though the method is successful, it has not been thoroughly analysed. In this paper we present a statistical analysis of Gabor-filtered speckle patterns. We introduce a model in which perturbations are described as random phase changes in the source plane. Using this model we compute the second and fourth order statistics of Gabor coefficients. We determine the mutual information between perturbed and unperturbed Gabor coefficients and the bit error rate in the derived bit string. The mutual information provides an absolute upper bound on the number of secure bits that can be reproducibly extracted from noisy measurements.
cs.CR cs.CV
laser speckle has been proposed in a number of papers as a highentropy source of unpredictable bits for use in security applications bit strings derived from speckle can be used for a variety of security purposes such as identification authentication anticounterfeiting secure key storage random number generation and tamper protection the choice of laser speckle as a source of random keys is quite natural given the chaotic properties of speckle however this same chaotic behaviour also causes reproducibility problems cryptographic protocols require either zero noise or very low noise in their inputs hence the issue of error rates is critical to applications of laser speckle in cryptography most of the literature uses an error reduction method based on gabor filtering though the method is successful it has not been thoroughly analysed in this paper we present a statistical analysis of gaborfiltered speckle patterns we introduce a model in which perturbations are described as random phase changes in the source plane using this model we compute the second and fourth order statistics of gabor coefficients we determine the mutual information between perturbed and unperturbed gabor coefficients and the bit error rate in the derived bit string the mutual information provides an absolute upper bound on the number of secure bits that can be reproducibly extracted from noisy measurements
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710.5003
Tracer density discontinuities in turbulent flows: simple model and scaling laws
Mixing in fully developed incompressible turbulent flows is known to lead to a cascade of discontinuity fronts of passive scalar fields. A one-dimensional (1D) variant of Baker's map is developed, capturing the main mechanism responsible for the emergence of these discontinuities. For this 1D model, expressions for the height-distribution function of the discontinuity fronts and structure function scaling exponents $\zeta_p$ are derived [for Kolmogorov turbulence, $\zeta_p=\frac 23\log_3(p+1)$]. These analytic findings are in a good agreement with both our 1D simulations, and the results of earlier numerical and experimental studies.
physics.flu-dyn physics.ao-ph
mixing in fully developed incompressible turbulent flows is known to lead to a cascade of discontinuity fronts of passive scalar fields a onedimensional 1d variant of bakers map is developed capturing the main mechanism responsible for the emergence of these discontinuities for this 1d model expressions for the heightdistribution function of the discontinuity fronts and structure function scaling exponents zeta_p are derived for kolmogorov turbulence zeta_pfrac 23log_3p1 these analytic findings are in a good agreement with both our 1d simulations and the results of earlier numerical and experimental studies
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710.5004
Computer-intensive rate estimation, diverging statistics and scanning
A general rate estimation method is proposed that is based on studying the in-sample evolution of appropriately chosen diverging/converging statistics. The proposed rate estimators are based on simple least squares arguments, and are shown to be accurate in a very general setting without requiring the choice of a tuning parameter. The notion of scanning is introduced with the purpose of extracting useful subsamples of the data series; the proposed rate estimation method is applied to different scans, and the resulting estimators are then combined to improve accuracy. Applications to heavy tail index estimation as well as to the problem of estimating the long memory parameter are discussed; a small simulation study complements our theoretical results.
math.ST stat.TH
a general rate estimation method is proposed that is based on studying the insample evolution of appropriately chosen divergingconverging statistics the proposed rate estimators are based on simple least squares arguments and are shown to be accurate in a very general setting without requiring the choice of a tuning parameter the notion of scanning is introduced with the purpose of extracting useful subsamples of the data series the proposed rate estimation method is applied to different scans and the resulting estimators are then combined to improve accuracy applications to heavy tail index estimation as well as to the problem of estimating the long memory parameter are discussed a small simulation study complements our theoretical results
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710.5005
Struggles with Survey Weighting and Regression Modeling
The general principles of Bayesian data analysis imply that models for survey responses should be constructed conditional on all variables that affect the probability of inclusion and nonresponse, which are also the variables used in survey weighting and clustering. However, such models can quickly become very complicated, with potentially thousands of poststratification cells. It is then a challenge to develop general families of multilevel probability models that yield reasonable Bayesian inferences. We discuss in the context of several ongoing public health and social surveys. This work is currently open-ended, and we conclude with thoughts on how research could proceed to solve these problems.
stat.ME
the general principles of bayesian data analysis imply that models for survey responses should be constructed conditional on all variables that affect the probability of inclusion and nonresponse which are also the variables used in survey weighting and clustering however such models can quickly become very complicated with potentially thousands of poststratification cells it is then a challenge to develop general families of multilevel probability models that yield reasonable bayesian inferences we discuss in the context of several ongoing public health and social surveys this work is currently openended and we conclude with thoughts on how research could proceed to solve these problems
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710.5006
CANE: The Content Addressed Network Environment
The fragmented nature and asymmetry of local and remote file access and network access, combined with the current lack of robust authenticity and privacy, hamstrings the current internet. The collection of disjoint and often ad-hoc technologies currently in use are at least partially responsible for the magnitude and potency of the plagues besetting the information economy, of which spam and email borne virii are canonical examples. The proposed replacement for the internet, Internet Protocol Version 6 (IPv6), does little to tackle these underlying issues, instead concentrating on addressing the technical issues of a decade ago. This paper introduces CANE, a Content Addressed Network Environment, and compares it against current internet and related technologies. Specifically, CANE presents a simple computing environment in which location is abstracted away in favour of identity, and trust is explicitly defined. Identity is cryptographically verified and yet remains pervasively open in nature. It is argued that this approach is capable of being generalised such that file storage and network access can be unified and subsequently combined with human interfaces to result in a Unified Theory of Access, which addresses many of the significant problems besetting the internet community of the early 21st century.
cs.NI cs.CR cs.DC
the fragmented nature and asymmetry of local and remote file access and network access combined with the current lack of robust authenticity and privacy hamstrings the current internet the collection of disjoint and often adhoc technologies currently in use are at least partially responsible for the magnitude and potency of the plagues besetting the information economy of which spam and email borne virii are canonical examples the proposed replacement for the internet internet protocol version 6 ipv6 does little to tackle these underlying issues instead concentrating on addressing the technical issues of a decade ago this paper introduces cane a content addressed network environment and compares it against current internet and related technologies specifically cane presents a simple computing environment in which location is abstracted away in favour of identity and trust is explicitly defined identity is cryptographically verified and yet remains pervasively open in nature it is argued that this approach is capable of being generalised such that file storage and network access can be unified and subsequently combined with human interfaces to result in a unified theory of access which addresses many of the significant problems besetting the internet community of the early 21st century
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710.5007
Sub-threshold production of $\Sigma$(1385) baryons in Al+Al collisions at 1.9$A$ GeV
First measurement of sub-threshold $\Sigma$(1385) production is presented. Experimental data are presented for Al+Al reactions at 1.9$A$ GeV measured with the FOPI detector at SIS/GSI. The $\Sigma$(1385)/$\Lambda$ ratio is found to be in good agreement with the transport and statistical model predictions. The results allow for a better understanding of sub-threshold strangeness production and strangeness exchange reaction which is the dominant process for $K^-$ production below and close-to threshold.
nucl-ex
first measurement of subthreshold sigma1385 production is presented experimental data are presented for alal reactions at 19a gev measured with the fopi detector at sisgsi the sigma1385lambda ratio is found to be in good agreement with the transport and statistical model predictions the results allow for a better understanding of subthreshold strangeness production and strangeness exchange reaction which is the dominant process for k production below and closeto threshold
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710.5008
Transport and magnetic properties in YBaCo2O5.45: Focus on the high-temperature transition
The electronic transport properties and the magnetic susceptibility were measured in detail in $YBaCo_2O_{5.45}$. Close to the so-called metal-insulator transition, strong effects of resistance relaxation, a clear thermal hysteresis and a sudden increase of the resistance noise are observed. This is likely due to the first order character of the transition and to the underlying phases coexistence. Despite these out of equilibrium features, a positive and linear magneto-resistance is also observed, possibly linked to the heterogeneity of the state. From a magnetic point of view, the paramagnetic to ordered magnetic state transition is observed using non linear susceptibilty. This transition shows the characteristics of a continuous transition, and time dependent effects can be linked with the dynamics of magnetic domains in presence of disorder. Thus, when focusing on the order of the transitions, the electronic one and the magnetic one can not be directly associated.
cond-mat.mtrl-sci
the electronic transport properties and the magnetic susceptibility were measured in detail in ybaco_2o_545 close to the socalled metalinsulator transition strong effects of resistance relaxation a clear thermal hysteresis and a sudden increase of the resistance noise are observed this is likely due to the first order character of the transition and to the underlying phases coexistence despite these out of equilibrium features a positive and linear magnetoresistance is also observed possibly linked to the heterogeneity of the state from a magnetic point of view the paramagnetic to ordered magnetic state transition is observed using non linear susceptibilty this transition shows the characteristics of a continuous transition and time dependent effects can be linked with the dynamics of magnetic domains in presence of disorder thus when focusing on the order of the transitions the electronic one and the magnetic one can not be directly associated
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710.5009
Comment: Struggles with Survey Weighting and Regression Modeling
Comment: Struggles with Survey Weighting and Regression Modeling [arXiv:0710.5005]
stat.ME
comment struggles with survey weighting and regression modeling arxiv07105005
[['comment', 'struggles', 'with', 'survey', 'weighting', 'and', 'regression', 'modeling', 'arxiv07105005']]
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710.501
EOS of dense matter and fast rotation of neutron stars
Recent observations of XTE J1739-285 suggest that it contains a neutron star rotating at 1122 Hz. Such rotational frequency would be the first for which the effects of rotation are significant. We study the consequences of very fast rotating neutron stars for the potentially observable quantities as stellar mass and pulsar period.
astro-ph
recent observations of xte j1739285 suggest that it contains a neutron star rotating at 1122 hz such rotational frequency would be the first for which the effects of rotation are significant we study the consequences of very fast rotating neutron stars for the potentially observable quantities as stellar mass and pulsar period
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710.5011
A precursor state to unconventional superconductivity in CeIrIn${_5}$
We present sensitive measurements of the Hall effect and magnetoresistance in CeIrIn${_5}$ down to temperatures of 50 mK and magnetic fields up to 15 T. The presence of a low temperature coherent Kondo state is established. Deviations from Kohler's rule and a quadratic temperature dependence of the cotangent of the Hall angle are reminiscent of properties observed in the high temperature superconducting cuprates. The most striking observation pertains to the presence of a \textit{precursor} state--characterized by a change in the Hall mobility--that appears to precede the superconductivity in this material, in similarity to the pseudogap in the cuprate high $T_c$ superconductors.
cond-mat.str-el cond-mat.supr-con
we present sensitive measurements of the hall effect and magnetoresistance in ceirin_5 down to temperatures of 50 mk and magnetic fields up to 15 t the presence of a low temperature coherent kondo state is established deviations from kohlers rule and a quadratic temperature dependence of the cotangent of the hall angle are reminiscent of properties observed in the high temperature superconducting cuprates the most striking observation pertains to the presence of a textitprecursor statecharacterized by a change in the hall mobilitythat appears to precede the superconductivity in this material in similarity to the pseudogap in the cuprate high t_c superconductors
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710.5012
Comment: Struggles with Survey Weighting and Regression Modeling
Comment: Struggles with Survey Weighting and Regression Modeling [arXiv:0710.5005]
stat.ME
comment struggles with survey weighting and regression modeling arxiv07105005
[['comment', 'struggles', 'with', 'survey', 'weighting', 'and', 'regression', 'modeling', 'arxiv07105005']]
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710.5013
Comment: Struggles with Survey Weighting and Regression Modeling
Comment: Struggles with Survey Weighting and Regression Modeling [arXiv:0710.5005]
stat.ME
comment struggles with survey weighting and regression modeling arxiv07105005
[['comment', 'struggles', 'with', 'survey', 'weighting', 'and', 'regression', 'modeling', 'arxiv07105005']]
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710.5014
On $k$-noncrossing partitions
In this paper we prove a duality between $k$-noncrossing partitions over $[n]=\{1,...,n\}$ and $k$-noncrossing braids over $[n-1]$. This duality is derived directly via (generalized) vacillating tableaux which are in correspondence to tangled-diagrams \cite{Reidys:07vac}. We give a combinatorial interpretation of the bijection in terms of the contraction of arcs of tangled-diagrams. Furthermore it induces by restriction a bijection between $k$-noncrossing, 2-regular partitions over $[n]$ and $k$-noncrossing braids without isolated points over $[n-1]$. Since braids without isolated points correspond to enhanced partitions this allows, using the results of \cite{MIRXIN}, to enumerate 2-regular, 3-noncrossing partitions.
math.CO math.RT
in this paper we prove a duality between knoncrossing partitions over n1n and knoncrossing braids over n1 this duality is derived directly via generalized vacillating tableaux which are in correspondence to tangleddiagrams citereidys07vac we give a combinatorial interpretation of the bijection in terms of the contraction of arcs of tangleddiagrams furthermore it induces by restriction a bijection between knoncrossing 2regular partitions over n and knoncrossing braids without isolated points over n1 since braids without isolated points correspond to enhanced partitions this allows using the results of citemirxin to enumerate 2regular 3noncrossing partitions
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710.5015
Comment: Struggles with Survey Weighting and Regression Modeling
Comment: Struggles with Survey Weighting and Regression Modeling [arXiv:0710.5005]
stat.ME
comment struggles with survey weighting and regression modeling arxiv07105005
[['comment', 'struggles', 'with', 'survey', 'weighting', 'and', 'regression', 'modeling', 'arxiv07105005']]
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710.5016
Comment: Struggles with Survey Weighting and Regression Modeling
Comment: Struggles with Survey Weighting and Regression Modeling [arXiv:0710.5005]
stat.ME
comment struggles with survey weighting and regression modeling arxiv07105005
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710.5017
Coherent states, constraint classes, and area operators in the new spin-foam models
Recently, two new spin-foam models have appeared in the literature, both motivated by a desire to modify the Barrett-Crane model in such a way that the imposition of certain second class constraints, called cross-simplicity constraints, are weakened. We refer to these two models as the FKLS model, and the flipped model. Both of these models are based on a reformulation of the cross-simplicity constraints. This paper has two main parts. First, we clarify the structure of the reformulated cross-simplicity constraints and the nature of their quantum imposition in the new models. In particular we show that in the FKLS model, quantum cross-simplicity implies no restriction on states. The deeper reason for this is that, with the symplectic structure relevant for FKLS, the reformulated cross-simplicity constraints, in a certain relevant sense, are now \emph{first class}, and this causes the coherent state method of imposing the constraints, key in the FKLS model, to fail to give any restriction on states. Nevertheless, the cross-simplicity can still be seen as implemented via suppression of intertwiner degrees of freedom in the dynamical propagation. In the second part of the paper, we investigate area spectra in the models. The results of these two investigations will highlight how, in the flipped model, the Hilbert space of states, as well as the spectra of area operators exactly match those of loop quantum gravity, whereas in the FKLS (and Barrett-Crane) models, the boundary Hilbert spaces and area spectra are different.
gr-qc
recently two new spinfoam models have appeared in the literature both motivated by a desire to modify the barrettcrane model in such a way that the imposition of certain second class constraints called crosssimplicity constraints are weakened we refer to these two models as the fkls model and the flipped model both of these models are based on a reformulation of the crosssimplicity constraints this paper has two main parts first we clarify the structure of the reformulated crosssimplicity constraints and the nature of their quantum imposition in the new models in particular we show that in the fkls model quantum crosssimplicity implies no restriction on states the deeper reason for this is that with the symplectic structure relevant for fkls the reformulated crosssimplicity constraints in a certain relevant sense are now emphfirst class and this causes the coherent state method of imposing the constraints key in the fkls model to fail to give any restriction on states nevertheless the crosssimplicity can still be seen as implemented via suppression of intertwiner degrees of freedom in the dynamical propagation in the second part of the paper we investigate area spectra in the models the results of these two investigations will highlight how in the flipped model the hilbert space of states as well as the spectra of area operators exactly match those of loop quantum gravity whereas in the fkls and barrettcrane models the boundary hilbert spaces and area spectra are different
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710.5018
Some remarks on Pr\"{u}fer $\star $--multiplication domains and class groups
Let $D$ be an integral domain with quotient field $K$ and let $X$ be an indeterminate over $D$. Also, let $\boldsymbol{\mathcal{T}}:=\{T_{\lambda}\mid \lambda \in \Lambda \}$ be a defining family of quotient rings of $D$ and suppose that $\ast $ is a finite type star operation on $D$ induced by $\boldsymbol{\mathcal{T}}$. We show that $D$ is a P$ \ast $MD (resp., P$v$MD) if and only if $(\co_D(fg))^{\ast}=(\co_D(f)\co_D(g))^{\ast}$ (resp., $(\co_D(fg))^{w}=(\co_D(f)\co_D(g))^{w}$) for all $0 \ne f,g \in K[X]$. A more general version of this result is given in the semistar operation setting. We give a method for recognizing P$v$MD's which are not P$\ast $MD's for a certain finite type star operation $\ast $. We study domains $D$ for which the $\ast $--class group $\Cl^{\ast}(D)$ equals the $t$--class group $\Cl^{t}(D)$ for any finite type star operation $\ast $, and we indicate examples of P$v$MD's $D$ such that $\Cl^{\ast}(D)\subsetneq \Cl^{t}(D)$. We also compute $\Cl^v(D)$ for certain valuation domains $D$.
math.AC math.AG
let d be an integral domain with quotient field k and let x be an indeterminate over d also let boldsymbolmathcaltt_lambdamid lambda in lambda be a defining family of quotient rings of d and suppose that ast is a finite type star operation on d induced by boldsymbolmathcalt we show that d is a p ast md resp pvmd if and only if co_dfgastco_dfco_dgast resp co_dfgwco_dfco_dgw for all 0 ne fg in kx a more general version of this result is given in the semistar operation setting we give a method for recognizing pvmds which are not past mds for a certain finite type star operation ast we study domains d for which the ast class group clastd equals the tclass group cltd for any finite type star operation ast and we indicate examples of pvmds d such that clastdsubsetneq cltd we also compute clvd for certain valuation domains d
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710.5019
Rejoinder: Struggles with Survey Weighting and Regression Modeling
Rejoinder: Struggles with Survey Weighting and Regression Modeling [arXiv:0710.5005]
stat.ME
rejoinder struggles with survey weighting and regression modeling arxiv07105005
[['rejoinder', 'struggles', 'with', 'survey', 'weighting', 'and', 'regression', 'modeling', 'arxiv07105005']]
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710.502
On the weight and the density of the space of order-preserving functionals
In the present paper it is proved that the functors $O_\tau$ of $\tau$-smooth order preserving functionals and $O_R$ of Radon order preserving functionals preserve the weight of infinite Tychonoff spaces. Moreover, it is established that the density and the weak density of infinite Tychonoff spaces do not increase under these functors.
math.GN math.FA
in the present paper it is proved that the functors o_tau of tausmooth order preserving functionals and o_r of radon order preserving functionals preserve the weight of infinite tychonoff spaces moreover it is established that the density and the weak density of infinite tychonoff spaces do not increase under these functors
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710.5021
On the first integral conjecture of Rene Thom
More that half a century ago R. Thom asserted in an unpublished manuscript that, generically, vector fields on compact connected smooth manifolds without boundary can admit only trivial continuous first integrals. Though somehow unprecise for what concerns the interpretation of the word \textquotedblleft generically\textquotedblright, this statement is ostensibly true and is nowadays commonly accepted. On the other hand, the (few) known formal proofs of Thom's conjecture are all relying to the classical Sard theorem and are thus requiring the technical assumption that first integrals should be of class $C^{k}$ with $k\geq d,$ where $d$ is the dimension of the manifold. In this work, using a recent nonsmooth extension of Sard theorem we establish the validity of Thom's conjecture for locally Lipschitz first integrals, interpreting genericity in the $C^{1}$ sense.
math.DS
more that half a century ago r thom asserted in an unpublished manuscript that generically vector fields on compact connected smooth manifolds without boundary can admit only trivial continuous first integrals though somehow unprecise for what concerns the interpretation of the word textquotedblleft genericallytextquotedblright this statement is ostensibly true and is nowadays commonly accepted on the other hand the few known formal proofs of thoms conjecture are all relying to the classical sard theorem and are thus requiring the technical assumption that first integrals should be of class ck with kgeq d where d is the dimension of the manifold in this work using a recent nonsmooth extension of sard theorem we establish the validity of thoms conjecture for locally lipschitz first integrals interpreting genericity in the c1 sense
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710.5022
Star Formation History in the Galactic Thin Disk
The behavior of the relative magnesium abundances in the thin-disk stars versus their orbital radii suggests that the star formation rate in the thin disk decreases with increasing Galactocentric distance, and there was no star formation for some time outside the solar circle while this process was continuous within the solar circle. The decrease in the star formation rate with increasing Galactocentric distance is responsible for the existence of a negative radial metallicity gradient in the thin disk. At the same time the relative magnesium abundance exhibits no radial gradient. It is in detail considered the influence of selective effects on the form of both age - metallicity and age - relative magnesium abundance diagrams. It is shown that the first several billion years of the formation of the thin disk interstellar medium in it was on the average sufficiently rich in heavy elements (<[Fe/H]> = -0.22), badly mixed (\sigma_[Fe/H] = 0.21), and the average relative magnesium abundance was comparatively high (<[Mg/Fe]> = 0.10). Approximately 5 billion years ago average metallicity began to systematically increase, and its dispersion and the average relative magnesium abundance - to decrease. These properties may be explained by an increase in star formation rate with the simultaneous intensification of the processes of mixing the interstellar medium in the thin disk, provoke possible by interaction the Galaxy with the completely massive by satellite galaxy.
astro-ph
the behavior of the relative magnesium abundances in the thindisk stars versus their orbital radii suggests that the star formation rate in the thin disk decreases with increasing galactocentric distance and there was no star formation for some time outside the solar circle while this process was continuous within the solar circle the decrease in the star formation rate with increasing galactocentric distance is responsible for the existence of a negative radial metallicity gradient in the thin disk at the same time the relative magnesium abundance exhibits no radial gradient it is in detail considered the influence of selective effects on the form of both age metallicity and age relative magnesium abundance diagrams it is shown that the first several billion years of the formation of the thin disk interstellar medium in it was on the average sufficiently rich in heavy elements feh 022 badly mixed sigma_feh 021 and the average relative magnesium abundance was comparatively high mgfe 010 approximately 5 billion years ago average metallicity began to systematically increase and its dispersion and the average relative magnesium abundance to decrease these properties may be explained by an increase in star formation rate with the simultaneous intensification of the processes of mixing the interstellar medium in the thin disk provoke possible by interaction the galaxy with the completely massive by satellite galaxy
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710.5023
Observations and asteroseismic analysis of the rapidly pulsating hot B subdwarf PG 0911+456
The principal aim of this project is to determine the structural parameters of the rapidly pulsating subdwarf B star PG 0911+456 from asteroseismology. Our work forms part of an ongoing programme to constrain the internal characteristics of hot B subdwarfs with the long-term goal of differentiating between the various formation scenarios proposed for these objects. First comparisons of asteroseismic values with evolutionary theory look promising, however it is clear that more targets are needed for meaningful statistics to be derived. The observational pulsation periods of PG 0911+456 were extracted from rapid time-series photometry using standard Fourier analysis techniques. Supplemented by spectroscopic estimates of the star's mean atmospheric parameters, they were used as a basis for the "forward modelling" approach in asteroseismology. The latter culminates in the identification of one or more "optimal" models that can accurately reproduce the observed period spectrum. This naturally leads to an identification of the oscillations detected in terms of degree l and radial order k, and infers the structural parameters of the target. From the photometry it was possible to extract 7 independent pulsation periods in the 150-200 s range with amplitudes between 0.05 and 0.8 % of the star's mean brightness. An asteroseismic search of parameter space identified several models that matched the observed properties of PG 0911+456 well, one of which was isolated as the "optimal" model on the basis of spectroscopic and mode identification considerations. All the observed pulsations are identified with low-order acoustic modes with degree indices l=0,1,2 and 4, and match the computed periods with a dispersion of only ~0.26 %.
astro-ph
the principal aim of this project is to determine the structural parameters of the rapidly pulsating subdwarf b star pg 0911456 from asteroseismology our work forms part of an ongoing programme to constrain the internal characteristics of hot b subdwarfs with the longterm goal of differentiating between the various formation scenarios proposed for these objects first comparisons of asteroseismic values with evolutionary theory look promising however it is clear that more targets are needed for meaningful statistics to be derived the observational pulsation periods of pg 0911456 were extracted from rapid timeseries photometry using standard fourier analysis techniques supplemented by spectroscopic estimates of the stars mean atmospheric parameters they were used as a basis for the forward modelling approach in asteroseismology the latter culminates in the identification of one or more optimal models that can accurately reproduce the observed period spectrum this naturally leads to an identification of the oscillations detected in terms of degree l and radial order k and infers the structural parameters of the target from the photometry it was possible to extract 7 independent pulsation periods in the 150200 s range with amplitudes between 005 and 08 of the stars mean brightness an asteroseismic search of parameter space identified several models that matched the observed properties of pg 0911456 well one of which was isolated as the optimal model on the basis of spectroscopic and mode identification considerations all the observed pulsations are identified with loworder acoustic modes with degree indices l012 and 4 and match the computed periods with a dispersion of only 026
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710.5024
On fractional Ornstein-Uhlenbeck processes
In this paper we study Doob's transform of fractional Brownian motion (FBM). It is well known that Doob's transform of standard Brownian motion is identical in law with the Ornstein-Uhlenbeck diffusion defined as the solution of the (stochastic) Langevin equation where the driving process is a Brownian motion. It is also known that Doob's transform of FBM and the process obtained from the Langevin equation with FBM as the driving process are different. However, also the first one of these can be described as a solution of a Langevin equation but now with some other driving process than FBM. We are mainly interested in the properties of this new driving process denoted Y^{(1)}. We also study the solution of the Langevin equation with Y^{(1)} as the driving process. Moreover, we show that the covariance of Y^{(1)} grows linearly; hence, in this respect Y^{(1)} is more like a standard Brownian motion than a FBM. In fact, it is proved that a properly scaled version of Y^{(1)} converges weakly to Brownian motion.
math.PR
in this paper we study doobs transform of fractional brownian motion fbm it is well known that doobs transform of standard brownian motion is identical in law with the ornsteinuhlenbeck diffusion defined as the solution of the stochastic langevin equation where the driving process is a brownian motion it is also known that doobs transform of fbm and the process obtained from the langevin equation with fbm as the driving process are different however also the first one of these can be described as a solution of a langevin equation but now with some other driving process than fbm we are mainly interested in the properties of this new driving process denoted y1 we also study the solution of the langevin equation with y1 as the driving process moreover we show that the covariance of y1 grows linearly hence in this respect y1 is more like a standard brownian motion than a fbm in fact it is proved that a properly scaled version of y1 converges weakly to brownian motion
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710.5025
From the Pr\'ekopa-Leindler inequality to modified logarithmic Sobolev inequality
We develop in this paper an improvement of the method given by S. Bobkov and M. Ledoux. Using the Pr\'ekopa-Leindler inequality, we prove a modified logarithmic Sobolev inequality adapted for all measures on $\dR^n$, with a strictly convex and super-linear potential. This inequality implies modified logarithmic Sobolev inequality for all uniform strictly convex potential as well as the Euclidean logarithmic Sobolev inequality.
math.PR
we develop in this paper an improvement of the method given by s bobkov and m ledoux using the prekopaleindler inequality we prove a modified logarithmic sobolev inequality adapted for all measures on drn with a strictly convex and superlinear potential this inequality implies modified logarithmic sobolev inequality for all uniform strictly convex potential as well as the euclidean logarithmic sobolev inequality
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710.5026
The Parkes Pulsar Timing Array
Detection and study of gravitational waves from astrophysical sources is a major goal of current astrophysics. Ground-based laser-interferometer systems such as LIGO and VIRGO are sensitive to gravitational waves with frequencies of order 100 Hz, whereas space-based systems such as LISA are sensitive in the millihertz regime. Precise timing observations of a sample of millisecond pulsars widely distributed on the sky have the potential to detect gravitational waves at nanohertz frequencies. Potential sources of such waves include binary super-massive black holes in the cores of galaxies, relic radiation from the inflationary era and oscillations of cosmic strings. The Parkes Pulsar Timing Array (PPTA) is an implementation of such a system in which 20 millisecond pulsars have been observed using the Parkes radio telescope at three frequencies at intervals of two -- three weeks for more than two years. Analysis of these data has been used to limit the gravitational wave background in our Galaxy and to constrain some models for its generation. The data have also been used to investigate fluctuations in the interstellar and Solar-wind electron density and have the potential to investigate the stability of terrestrial time standards and the accuracy of solar-system ephemerides.
astro-ph
detection and study of gravitational waves from astrophysical sources is a major goal of current astrophysics groundbased laserinterferometer systems such as ligo and virgo are sensitive to gravitational waves with frequencies of order 100 hz whereas spacebased systems such as lisa are sensitive in the millihertz regime precise timing observations of a sample of millisecond pulsars widely distributed on the sky have the potential to detect gravitational waves at nanohertz frequencies potential sources of such waves include binary supermassive black holes in the cores of galaxies relic radiation from the inflationary era and oscillations of cosmic strings the parkes pulsar timing array ppta is an implementation of such a system in which 20 millisecond pulsars have been observed using the parkes radio telescope at three frequencies at intervals of two three weeks for more than two years analysis of these data has been used to limit the gravitational wave background in our galaxy and to constrain some models for its generation the data have also been used to investigate fluctuations in the interstellar and solarwind electron density and have the potential to investigate the stability of terrestrial time standards and the accuracy of solarsystem ephemerides
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710.5027
Neutrino oscillations: present status and outlook
I summarize the status of three-flavour neutrino oscillations with date of Oct. 2007, and provide an outlook for the developments to be expected in the near future. Furthermore, I discuss the status of sterile neutrino oscillation interpretations of the LSND anomaly in the light of recent MiniBooNE results, and comment on implications for the future neutrino oscillation program.
hep-ph
i summarize the status of threeflavour neutrino oscillations with date of oct 2007 and provide an outlook for the developments to be expected in the near future furthermore i discuss the status of sterile neutrino oscillation interpretations of the lsnd anomaly in the light of recent miniboone results and comment on implications for the future neutrino oscillation program
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710.5028
The CORALIE survey for southern extra-solar planets XV. Discovery of two eccentric planets orbiting HD4113 and HD156846
We report the detection of two very eccentric planets orbiting HD4113 and HD156846 with the CORALIE Echelle spectrograph mounted on the 1.2-m Euler Swiss telescope at La Silla. The first planet, HD4113b, has minimum mass of $m\sin{i}=1.6\pm0.2 M_{\rm Jup}$, a period of $P=526.59\pm0.21$ days and an eccentricity of $e=0.903\pm0.02$. It orbits a metal rich G5V star at $a=1.28$ AU which displays an additional radial velocity drift of 28 m s$^{-1}$/yr observed during 8 years. The combination of the radial-velocity data and the non-detection of any main sequence stellar companion in our high contrast images taken at the VLT with NACO/SDI, characterizes the companion as a probable brown dwarf or as a faint white dwarf. The second planet, \object{HD 156846 b}, has minimum mass of $m\sin{i}=10.45\pm0.05$ M$_{\rm Jup}$, a period of $P=359.51\pm0.09 $ days, an eccentricity of $e=0.847\pm0.002$ and is located at $a=1.0$ AU from its parent star. HD156846 is a metal rich G0 dwarf and is also the primary of a wide binary system ($a>250$ AU, $P>4000$ years). Its stellar companion, \object{IDS 17147-1914 B}, is a M4 dwarf. The very high eccentricities of both planets can be explained by Kozai oscillations induced by the presence of a third object.
astro-ph
we report the detection of two very eccentric planets orbiting hd4113 and hd156846 with the coralie echelle spectrograph mounted on the 12m euler swiss telescope at la silla the first planet hd4113b has minimum mass of msini16pm02 m_rm jup a period of p52659pm021 days and an eccentricity of e0903pm002 it orbits a metal rich g5v star at a128 au which displays an additional radial velocity drift of 28 m s1yr observed during 8 years the combination of the radialvelocity data and the nondetection of any main sequence stellar companion in our high contrast images taken at the vlt with nacosdi characterizes the companion as a probable brown dwarf or as a faint white dwarf the second planet objecthd 156846 b has minimum mass of msini1045pm005 m_rm jup a period of p35951pm009 days an eccentricity of e0847pm0002 and is located at a10 au from its parent star hd156846 is a metal rich g0 dwarf and is also the primary of a wide binary system a250 au p4000 years its stellar companion objectids 171471914 b is a m4 dwarf the very high eccentricities of both planets can be explained by kozai oscillations induced by the presence of a third object
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710.5029
Magnetic ground state of coupled edge-sharing CuO_2 spin-chains
By means of density functional theory, we investigate the magnetic ground state of edge-sharing CuO_2 spin-chains, as found in the (La,Ca,Sr)_14Cu_24O_41system, for instance. Our data rely on spin-polarized electronic structure calculations including onsite interaction (LDA+U) and an effective model for the interchain coupling. Strong doping dependence of the magnetic order is characteristic for edge-sharing CuO_2 spin-chains. We determine the ground state magnetic structure as function of the spin-chain filling and quantify the competing exchange interactions.
cond-mat.str-el
by means of density functional theory we investigate the magnetic ground state of edgesharing cuo_2 spinchains as found in the lacasr_14cu_24o_41system for instance our data rely on spinpolarized electronic structure calculations including onsite interaction ldau and an effective model for the interchain coupling strong doping dependence of the magnetic order is characteristic for edgesharing cuo_2 spinchains we determine the ground state magnetic structure as function of the spinchain filling and quantify the competing exchange interactions
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710.503
High-resolution spectroscopy of the R Coronae Borealis Star V Coronae Australis
Optical high-resolution spectra of the R Coronae Borealis star V CrA at light maximum and during minimum light arediscussed. Abundance analysis confirms previous results showing that V CrA has the composition of the small subclass of R Coronae Borealis (RCB) stars know as `minority' RCBs, i.e., the Si/Fe and S/Fe ratios are 100 times their solar values. A notable novel result for RCBs is the detection of the 1-0 Swan system $^{12}$C$^{13}$C bandhead indicating that $^{13}$C is abundant: spectrum synthesis shows that $^{12}$C/$^{13}$C is about 3 to 4. Absorption line profiles are variable at maximum light with some lines showing evidence of splitting by about 10 km s$^{-1}$. A spectrum obtained as the star was recovering from a deep minimum shows the presence of cool C$_2$ molecules with a rotational temperature of about 1200K, a temperature suggestive of gas in which carbon is condensing into soot. The presence of rapidly outflowing gas is shown by blue-shifted absorption components of the Na {\sc i} D and K {\sc i} 7698 \AA resonance lines.
astro-ph
optical highresolution spectra of the r coronae borealis star v cra at light maximum and during minimum light arediscussed abundance analysis confirms previous results showing that v cra has the composition of the small subclass of r coronae borealis rcb stars know as minority rcbs ie the sife and sfe ratios are 100 times their solar values a notable novel result for rcbs is the detection of the 10 swan system 12c13c bandhead indicating that 13c is abundant spectrum synthesis shows that 12c13c is about 3 to 4 absorption line profiles are variable at maximum light with some lines showing evidence of splitting by about 10 km s1 a spectrum obtained as the star was recovering from a deep minimum shows the presence of cool c_2 molecules with a rotational temperature of about 1200k a temperature suggestive of gas in which carbon is condensing into soot the presence of rapidly outflowing gas is shown by blueshifted absorption components of the na sc i d and k sc i 7698 aa resonance lines
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710.5031
Elementary Pseudoconcavity and fields of CR meromorphic functions
Let M be a smooth CR manifold of CR dimension n and CR codimension k, which is not compact, but has the local extension property E. We introduce the notion of "elementary pseudoconcavity" for M, which extends to CR manifolds the concept of a "pseudoconcave" complex manifold. This notion is then used to obtain generalizations, to the noncompact case, of the results of our previous paper about algebraic dependence, transcendence degree and related matters for the field K(M) of CR meromorphic functions on M.
math.CV math.AG math.AP
let m be a smooth cr manifold of cr dimension n and cr codimension k which is not compact but has the local extension property e we introduce the notion of elementary pseudoconcavity for m which extends to cr manifolds the concept of a pseudoconcave complex manifold this notion is then used to obtain generalizations to the noncompact case of the results of our previous paper about algebraic dependence transcendence degree and related matters for the field km of cr meromorphic functions on m
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710.5032
The s-s(bar) asymmetry in nucleon and "NuTeV anomaly"
The $s$-$\bar{s}$ asymmetry in nucleon sea is an important observable for understanding nucleon structure and strong interaction. There have been many theoretical attempts on this subject and recently on its relation to the "NuTeV anomaly". Calculations with different theoretical frameworks lead to different conclusions. Here assuming a newly proposed penta-quark configuration for the $s$-$\bar{s}$ asymmetry in nucleon, we examine its contribution to the "NuTeV anomaly", with a result of about $10-20%$.
hep-ph
the sbars asymmetry in nucleon sea is an important observable for understanding nucleon structure and strong interaction there have been many theoretical attempts on this subject and recently on its relation to the nutev anomaly calculations with different theoretical frameworks lead to different conclusions here assuming a newly proposed pentaquark configuration for the sbars asymmetry in nucleon we examine its contribution to the nutev anomaly with a result of about 1020
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710.5033
Efficient spatially-resolved multimode quantum memory
We propose a method that enables efficient storage and retrieval of a photonic excitation stored in an ensemble quantum memory consisting of Lambda-type absorbers with non-zero Stokes shift. We show that this can be used to implement a multimode quantum memory storing multiple frequency-encoded qubits in a single ensemble, and allowing their selective retrieval. The read-out scheme applies to memory setups based on both electromagnetically-induced transparency and stimulated Raman scattering, and spatially separates the output signal field from the control fields.
quant-ph
we propose a method that enables efficient storage and retrieval of a photonic excitation stored in an ensemble quantum memory consisting of lambdatype absorbers with nonzero stokes shift we show that this can be used to implement a multimode quantum memory storing multiple frequencyencoded qubits in a single ensemble and allowing their selective retrieval the readout scheme applies to memory setups based on both electromagneticallyinduced transparency and stimulated raman scattering and spatially separates the output signal field from the control fields
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710.5034
Numerical indications on the semiclassical limit of the flipped vertex
We introduce a technique for testing the semiclassical limit of a quantum gravity vertex amplitude. The technique is based on the propagation of a semiclassical wave packet. We apply this technique to the newly introduced "flipped" vertex in loop quantum gravity, in order to test the intertwiner dependence of the vertex. Under some drastic simplifications, we find very preliminary, but surprisingly good numerical evidence for the correct classical limit.
gr-qc
we introduce a technique for testing the semiclassical limit of a quantum gravity vertex amplitude the technique is based on the propagation of a semiclassical wave packet we apply this technique to the newly introduced flipped vertex in loop quantum gravity in order to test the intertwiner dependence of the vertex under some drastic simplifications we find very preliminary but surprisingly good numerical evidence for the correct classical limit
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710.5035
The NIR to UV continuum of radio loud vs. radio quiet quasars
Starting from a sample of SDSS quasars appearing also in the 2MASS survey, we study the continuum properties of about 1000 objects observed in 8 bands, from NIR to UV. We construct the mean spectral energy distribution (SED) and compare and contrast the continua of radio loud (RLQ) and radio quiet (RQQ) objects. The SEDs of the two populations are significantly different in the sense that RLQs are redder, with power law spectral indices <alpha(RLQ)>=-0.55+/-0.04 and <alpha(RQQ)>=-0.31+/-0.01 in the spectral range between 10^14.5 and 10^15.35 Hz. This difference is discussed in terms of different extinctions, different disc temperatures, or slopes of the non-thermal component.
astro-ph
starting from a sample of sdss quasars appearing also in the 2mass survey we study the continuum properties of about 1000 objects observed in 8 bands from nir to uv we construct the mean spectral energy distribution sed and compare and contrast the continua of radio loud rlq and radio quiet rqq objects the seds of the two populations are significantly different in the sense that rlqs are redder with power law spectral indices alpharlq055004 and alpharqq031001 in the spectral range between 10145 and 101535 hz this difference is discussed in terms of different extinctions different disc temperatures or slopes of the nonthermal component
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710.5036
Accretion indicators for the 37 brightest radio sources in the Subaru/XMM-Newton Deep Field
We study the 37 brightest radio sources in the Subaru/XMM-Newton Deep Field (SXDF). Using mid-IR (Spitzer MIPS 24 micron) data we expect to trace nuclear accretion activity, even if it is obscured at optical wavelengths, unless the obscuring column is extreme. Our results suggest that above the `FRI/FRII' radio luminosity break most of the radio sources are associated with objects that have excess mid-IR emission, only some of which are broad-line objects, although there is one clear low-accretion-rate FRI. The fraction of objects with mid-IR excess drops dramatically below the FRI/FRII break, although there exists at least one high-accretion-rate QSO. Investigation of mid-IR and blue excesses shows that they are correlated as predicted by a model in which a torus of dust absorbs ~30% of the light, and the dust above and below the torus scatters >~1% of the light.
astro-ph
we study the 37 brightest radio sources in the subaruxmmnewton deep field sxdf using midir spitzer mips 24 micron data we expect to trace nuclear accretion activity even if it is obscured at optical wavelengths unless the obscuring column is extreme our results suggest that above the frifrii radio luminosity break most of the radio sources are associated with objects that have excess midir emission only some of which are broadline objects although there is one clear lowaccretionrate fri the fraction of objects with midir excess drops dramatically below the frifrii break although there exists at least one highaccretionrate qso investigation of midir and blue excesses shows that they are correlated as predicted by a model in which a torus of dust absorbs 30 of the light and the dust above and below the torus scatters 1 of the light
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710.5037
Entanglement measures as physical observables
We discuss why regular observables can not be proper entanglement measures, and how observables in a generalized setting can be used to make an entanglement monotone a directly observable quantity for the case of pure states. For the case of mixed states, these generalized observables can be used to find valid lower bounds on entanglement monotones that can be measured in laboratory experiments in the same fashion as it can also be done for pure states.
quant-ph
we discuss why regular observables can not be proper entanglement measures and how observables in a generalized setting can be used to make an entanglement monotone a directly observable quantity for the case of pure states for the case of mixed states these generalized observables can be used to find valid lower bounds on entanglement monotones that can be measured in laboratory experiments in the same fashion as it can also be done for pure states
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710.5038
Higgs boson productions at LHC as a probe of different littlest Higgs models with T-parity
Higgs boson productions at the LHC will serve as a sensitive probe of various little Higgs models. In this work we comparatively study two littlest Higgs models with different T-parity constructions through examining their effects in three production processes of the Higgs boson at the LHC, namely the productions of a single Higgs, a Higgs-pair, as well as a Higgs boson associated with a pair of top and anti-top quarks. The two models are characterized by predicting a top partner canceling the Higgs mass quadratic divergence contributed by the top quark with even and odd T-parity, respectively. We find that both models can alter the SM cross sections sizably and their corrections also differ significantly. Therefore, the Higgs boson productions at the LHC may shed some light on these two models or even distinguish them.
hep-ph
higgs boson productions at the lhc will serve as a sensitive probe of various little higgs models in this work we comparatively study two littlest higgs models with different tparity constructions through examining their effects in three production processes of the higgs boson at the lhc namely the productions of a single higgs a higgspair as well as a higgs boson associated with a pair of top and antitop quarks the two models are characterized by predicting a top partner canceling the higgs mass quadratic divergence contributed by the top quark with even and odd tparity respectively we find that both models can alter the sm cross sections sizably and their corrections also differ significantly therefore the higgs boson productions at the lhc may shed some light on these two models or even distinguish them
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710.5039
On the separability criterion for continuous variable systems
We present an elementary and explicit proof of the separability criterion for continuous variable two-party Gaussian systems. Our proof is based on an elementary formulation of uncertainty relations and an explicit determination of squeezing parameters for which the P-representation condition saturates the $Sp(2,R)\otimes Sp(2,R)$ invariant separability condition. We thus give the explicit formulas of squeezing parameters, which establish the equivalence of the separability condition with the P-representation condition, in terms of the parameters of the standard form of the correlation matrix. Our proof is compared to the past proofs, and it is pointed out that the original proof of the P-representation by Duan, Giedke, Cirac and Zoller(DGCZ) is incomplete. A way to complete their proof is then shown. It is noted that both of the corrected proof of DGCZ and the proof of R. Simon are closely related to our explicit construction despite their quite different appearances.
quant-ph
we present an elementary and explicit proof of the separability criterion for continuous variable twoparty gaussian systems our proof is based on an elementary formulation of uncertainty relations and an explicit determination of squeezing parameters for which the prepresentation condition saturates the sp2rotimes sp2r invariant separability condition we thus give the explicit formulas of squeezing parameters which establish the equivalence of the separability condition with the prepresentation condition in terms of the parameters of the standard form of the correlation matrix our proof is compared to the past proofs and it is pointed out that the original proof of the prepresentation by duan giedke cirac and zollerdgcz is incomplete a way to complete their proof is then shown it is noted that both of the corrected proof of dgcz and the proof of r simon are closely related to our explicit construction despite their quite different appearances
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710.504
Verification of new identity for the Green functions in N=1 supersymmetric non-Abelian Yang--Mills theory with the matter fields
We investigate a new identity for Green functions using the higher covariant derivative regularization. It relates some coefficients in the vertex function of the matter superfield, in which one of external matter lines is not chiral. The calculation in the first nontrivial order (for the two-loop vertex function) reveals that the new identity is also valid for the non-Abelian Yang--Mills theory with matter fields. The new identity is shown to appear because three-loop integrals, defining the Gell-Mann--Low function are factorized into integrals of total derivatives.
hep-th
we investigate a new identity for green functions using the higher covariant derivative regularization it relates some coefficients in the vertex function of the matter superfield in which one of external matter lines is not chiral the calculation in the first nontrivial order for the twoloop vertex function reveals that the new identity is also valid for the nonabelian yangmills theory with matter fields the new identity is shown to appear because threeloop integrals defining the gellmannlow function are factorized into integrals of total derivatives
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710.5041
A Remark on Almost Umbilical Hypersurfaces
In this article, we prove new stability results for almost-Einstein hypersurfaces of the Euclidean space, based on previous eigenvalue pinching results. Then, we deduce some comparable results for almost umbilical hypersurfaces.
math.DG
in this article we prove new stability results for almosteinstein hypersurfaces of the euclidean space based on previous eigenvalue pinching results then we deduce some comparable results for almost umbilical hypersurfaces
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710.5042
Highly Accurate Analytic Presentation of Solution of the Schr\"{o}dinger Equation
High-precision approximate analytic expressions for energies and wave functions are found for arbitrary physical potentials. The Schr\"{o}dinger equation is cast into nonlinear Riccati equation, which is solved analytically in first iteration of the quasi-linearization method (QLM). The zeroth iteration is based on general features of the exact solution near the boundaries. The approach is illustrated on the Yukawa potential. The results enable accurate analytical estimates of effects of parameter variations on physical systems.
math-ph hep-ph math.MP
highprecision approximate analytic expressions for energies and wave functions are found for arbitrary physical potentials the schrodinger equation is cast into nonlinear riccati equation which is solved analytically in first iteration of the quasilinearization method qlm the zeroth iteration is based on general features of the exact solution near the boundaries the approach is illustrated on the yukawa potential the results enable accurate analytical estimates of effects of parameter variations on physical systems
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710.5043
Lorentzian LQG vertex amplitude
We generalize a model recently proposed for Euclidean quantum gravity to the case of Lorentzian signature. The main features of the Euclidean model are preserved in the Lorentzian one. In particular, the boundary Hilbert space matches the one of SU(2) loop quantum gravity. As in the Euclidean case, the model can be obtained from the Lorentzian Barrett-Crane model from a flipping of the Poisson structure, or alternatively, by adding a topological term to the action and taking the small Barbero-Immirzi parameter limit.
gr-qc
we generalize a model recently proposed for euclidean quantum gravity to the case of lorentzian signature the main features of the euclidean model are preserved in the lorentzian one in particular the boundary hilbert space matches the one of su2 loop quantum gravity as in the euclidean case the model can be obtained from the lorentzian barrettcrane model from a flipping of the poisson structure or alternatively by adding a topological term to the action and taking the small barberoimmirzi parameter limit
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710.5044
On the extendability of free multiarrangements
A free multiarrangement of rank $k$ is defined to be extendable if it is obtained from a simple rank $(k+1)$ free arrangement by the natural restriction to a hyperplane (in the sense of Ziegler). Not all free multiarrangements are extendable. We will discuss extendability of free multiarrangements for a special class. We also give two applications. The first is to produce totally non-free arrangements. The second is to give interpolating free arrangements between extended Shi and Catalan arrangements.
math.CO math.AC
a free multiarrangement of rank k is defined to be extendable if it is obtained from a simple rank k1 free arrangement by the natural restriction to a hyperplane in the sense of ziegler not all free multiarrangements are extendable we will discuss extendability of free multiarrangements for a special class we also give two applications the first is to produce totally nonfree arrangements the second is to give interpolating free arrangements between extended shi and catalan arrangements
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710.5045
Statistical approach to dislocation dynamics: From dislocation correlations to a multiple-slip continuum plasticity theory
Due to recent successes of a statistical-based nonlocal continuum crystal plasticity theory for single-glide in explaining various aspects such as dislocation patterning and size-dependent plasticity, several attempts have been made to extend the theory to describe crystals with multiple slip systems using ad-hoc assumptions. We present here a mesoscale continuum theory of plasticity for multiple slip systems of parallel edge dislocations. We begin by constructing the Bogolyubov-Born-Green-Yvon-Kirkwood (BBGYK) integral equations relating different orders of dislocation correlation functions in a grand canonical ensemble. Approximate pair correlation functions are obtained for single-slip systems with two types of dislocations and, subsequently, for general multiple-slip systems of both charges. The effect of the correlations manifests itself in the form of an entropic force in addition to the external stress and the self-consistent internal stress. Comparisons with a previous multiple-slip theory based on phenomenological considerations shall be discussed.
cond-mat.stat-mech cond-mat.mtrl-sci
due to recent successes of a statisticalbased nonlocal continuum crystal plasticity theory for singleglide in explaining various aspects such as dislocation patterning and sizedependent plasticity several attempts have been made to extend the theory to describe crystals with multiple slip systems using adhoc assumptions we present here a mesoscale continuum theory of plasticity for multiple slip systems of parallel edge dislocations we begin by constructing the bogolyubovborngreenyvonkirkwood bbgyk integral equations relating different orders of dislocation correlation functions in a grand canonical ensemble approximate pair correlation functions are obtained for singleslip systems with two types of dislocations and subsequently for general multipleslip systems of both charges the effect of the correlations manifests itself in the form of an entropic force in addition to the external stress and the selfconsistent internal stress comparisons with a previous multipleslip theory based on phenomenological considerations shall be discussed
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710.5046
Comparative Quantum Cosmology: Causality, Singularity, and Boundary Conditions
In this review article we compare the recent work of Peter Lynds, "On a finite universe with no beginning or end", with that of Stephen Hawking, primarily "Quantum Cosmology, M-Theory, and the Anthropic Principle", and two foundational works by Sean M. Carroll and Jennifer Chen, "Does Inflation Provide Natural Conditions for the Universe" and "Spontaneous Inflation and the Origin of the Arrow of Time", in order to evaluate their comparative treatments of the nature and role of causality, time ordering, thermodynamic reversibility, singularities and boundary conditions in the formation of the early universe. We briefly reference Smolin and Kauffman's recent arguments with respect to possible processes of "evolutionary selection" in early universe formation as an alternative explanation to key elements of Hawking's earlier "M-Theory", and its attendant anthropic principle. We also briefly excerpt a short section of Smolin's recent work on topology in quantum loop gravity, simply as an illustrative example of the type of complex quantum topological transformation which he offers as a theoretical alternative to string theory in quantum cosmology.
gr-qc
in this review article we compare the recent work of peter lynds on a finite universe with no beginning or end with that of stephen hawking primarily quantum cosmology mtheory and the anthropic principle and two foundational works by sean m carroll and jennifer chen does inflation provide natural conditions for the universe and spontaneous inflation and the origin of the arrow of time in order to evaluate their comparative treatments of the nature and role of causality time ordering thermodynamic reversibility singularities and boundary conditions in the formation of the early universe we briefly reference smolin and kauffmans recent arguments with respect to possible processes of evolutionary selection in early universe formation as an alternative explanation to key elements of hawkings earlier mtheory and its attendant anthropic principle we also briefly excerpt a short section of smolins recent work on topology in quantum loop gravity simply as an illustrative example of the type of complex quantum topological transformation which he offers as a theoretical alternative to string theory in quantum cosmology
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710.5047
Kinematic structure of the atmosphere and envelope of the post-AGB star HD56126
We present results of an analysis of the optical spectrum of the post-AGB star HD56126 (IRAS 07134+1005) based on observations made with the echelle spectrographs of the 6-m telescope with spectral resolutions of R=25000 and 60000 at 4012-8790 AA. The profiles of strongest lines (HI; FeII, YII, BaII absorptions, etc.) formed in the expanding atmosphere at the base of the stellar wind have complex and variable shapes. To study the kinematics of the atmosphere, the velocities of individual features in these profiles must be measured. Differential line shifts of up to Vr=15-30 km/s have been detected from the lines of metals and molecular features. The star's atmosphere simultaneously contains both expanding layers and layers falling onto the star. A comparison of the data for different times demonstrates that both the radial velocity and the velocity pattern in whole are variable. The position of the molecular spectrum is stable, implying stability of the expansion velocity of the circumstellar envelope around HD56126 detected in observations in the C_2 and NaI lines.
astro-ph
we present results of an analysis of the optical spectrum of the postagb star hd56126 iras 071341005 based on observations made with the echelle spectrographs of the 6m telescope with spectral resolutions of r25000 and 60000 at 40128790 aa the profiles of strongest lines hi feii yii baii absorptions etc formed in the expanding atmosphere at the base of the stellar wind have complex and variable shapes to study the kinematics of the atmosphere the velocities of individual features in these profiles must be measured differential line shifts of up to vr1530 kms have been detected from the lines of metals and molecular features the stars atmosphere simultaneously contains both expanding layers and layers falling onto the star a comparison of the data for different times demonstrates that both the radial velocity and the velocity pattern in whole are variable the position of the molecular spectrum is stable implying stability of the expansion velocity of the circumstellar envelope around hd56126 detected in observations in the c_2 and nai lines
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710.5048
Vacuum - induced stationary entanglement in radiatively coupled three - level atoms
We consider a pair of three - level atoms interacting with a common vacuum and analyze the process of entanglement production due to spontaneous emission. We show that in the case of closely separated atoms, collective damping can generate robust entanglement of the asymptotic states.
quant-ph
we consider a pair of three level atoms interacting with a common vacuum and analyze the process of entanglement production due to spontaneous emission we show that in the case of closely separated atoms collective damping can generate robust entanglement of the asymptotic states
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710.5049
Search for Supersymmetric Neutral Higgs Bosons at the Tevatron
Recent preliminary results obtained by the CDF and DO Collaborations on searches for Higgs bosons beyond the Standard Model at Run II of the Tevatron are discussed. The data, corresponding to integrated luminosities of up to 1 fb-1, are compared to theoretical expectations. No significant excess of signal above the expected background is observed in any of the various final states examined, and so limits at 95% Confidence Level (CL) are presented.
hep-ex
recent preliminary results obtained by the cdf and do collaborations on searches for higgs bosons beyond the standard model at run ii of the tevatron are discussed the data corresponding to integrated luminosities of up to 1 fb1 are compared to theoretical expectations no significant excess of signal above the expected background is observed in any of the various final states examined and so limits at 95 confidence level cl are presented
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710.505
Solution of the wave equation in a tridiagonal representation space
We use variable transformation from the real line to finite or semi-infinite spaces where we expand the regular solution of the 1D time-independent Schrodinger equation in terms of square integrable bases. We also require that the basis support an infinite tridiagonal matrix representation of the wave operator. By this requirement, we deduce a class of solvable potentials along with their corresponding bound states and stationary wavefunctions expressed as infinite series in terms of these bases. This approach allows for simultaneous treatment of the discrete (bound states) as well as the continuous (scattering states) spectrum on the same footing. The problem translates into finding solutions of the resulting three-term recursion relation for the expansion coefficients of the wavefunction. These are written in terms of orthogonal polynomials, some of which are modified versions of known polynomials. The examples given, which are not exhaustive, illustrate the power of this approach in dealing with 1D quantum problems.
quant-ph
we use variable transformation from the real line to finite or semiinfinite spaces where we expand the regular solution of the 1d timeindependent schrodinger equation in terms of square integrable bases we also require that the basis support an infinite tridiagonal matrix representation of the wave operator by this requirement we deduce a class of solvable potentials along with their corresponding bound states and stationary wavefunctions expressed as infinite series in terms of these bases this approach allows for simultaneous treatment of the discrete bound states as well as the continuous scattering states spectrum on the same footing the problem translates into finding solutions of the resulting threeterm recursion relation for the expansion coefficients of the wavefunction these are written in terms of orthogonal polynomials some of which are modified versions of known polynomials the examples given which are not exhaustive illustrate the power of this approach in dealing with 1d quantum problems
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710.5051
Localization of Gauge Fields and Monopole Tunnelling
We study the dynamical localization of a massless gauge field on a lower-dimensional surface (2-brane). In flat space, the necessary and sufficient condition for this phenomenon is the existence of confinement in the bulk. The resulting configuration is equivalent to a dual Josephson junction. This duality leads to an interesting puzzle, as it implies that a localized massless theory, even in the Abelian case, must become confining at exponentially large distances. Through the use of topological arguments we clarify the physics behind this large-distance confinement and identify the instantons of the brane world-volume theory that are responsible for its appearance. We show that they correspond to the (condensed) bulk magnetic charges (monopoles), that occasionally tunnel through the brane and induce weak confinement of the brane theory. We consider the possible generalization of this effect to higher dimensions and discuss phenomenological bounds on the confinement of electric charges at exponentially large distances within our Universe.
hep-th hep-ph
we study the dynamical localization of a massless gauge field on a lowerdimensional surface 2brane in flat space the necessary and sufficient condition for this phenomenon is the existence of confinement in the bulk the resulting configuration is equivalent to a dual josephson junction this duality leads to an interesting puzzle as it implies that a localized massless theory even in the abelian case must become confining at exponentially large distances through the use of topological arguments we clarify the physics behind this largedistance confinement and identify the instantons of the brane worldvolume theory that are responsible for its appearance we show that they correspond to the condensed bulk magnetic charges monopoles that occasionally tunnel through the brane and induce weak confinement of the brane theory we consider the possible generalization of this effect to higher dimensions and discuss phenomenological bounds on the confinement of electric charges at exponentially large distances within our universe
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710.5052
Magnetic fluctuations and formation of large-scale inhomogeneous magnetic structures in a turbulent convection
Magnetic fluctuations generated by a tangling of the mean magnetic field by velocity fluctuations are studied in a developed turbulent convection with large magnetic Reynolds numbers. We show that the energy of magnetic fluctuations depends on magnetic Reynolds number only when the mean magnetic field is smaller than $B_{eq} / 4 Rm^{1/4}$, where $B_{eq}$ is the equipartition mean magnetic field determined by the turbulent kinetic energy and Rm is magnetic Reynolds number. Generation of magnetic fluctuations in a turbulent convection with a nonzero mean magnetic field results in a decrease of the total turbulent pressure and may cause formation of the large-scale inhomogeneous magnetic structures even in an originally uniform mean magnetic field. This effect is caused by a negative contribution of the turbulent convection to the effective mean Lorentz force. The inhomogeneous large-scale magnetic fields are formed due to the excitation of the large-scale instability. The energy for this instability is supplied by the small-scale turbulent convection. The discussed effects might be useful for understanding the origin of the solar nonuniform magnetic fields, e.g., sunspots.
astro-ph
magnetic fluctuations generated by a tangling of the mean magnetic field by velocity fluctuations are studied in a developed turbulent convection with large magnetic reynolds numbers we show that the energy of magnetic fluctuations depends on magnetic reynolds number only when the mean magnetic field is smaller than b_eq 4 rm14 where b_eq is the equipartition mean magnetic field determined by the turbulent kinetic energy and rm is magnetic reynolds number generation of magnetic fluctuations in a turbulent convection with a nonzero mean magnetic field results in a decrease of the total turbulent pressure and may cause formation of the largescale inhomogeneous magnetic structures even in an originally uniform mean magnetic field this effect is caused by a negative contribution of the turbulent convection to the effective mean lorentz force the inhomogeneous largescale magnetic fields are formed due to the excitation of the largescale instability the energy for this instability is supplied by the smallscale turbulent convection the discussed effects might be useful for understanding the origin of the solar nonuniform magnetic fields eg sunspots
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