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711.4708
On the theory of resonances in non-relativistic QED and related models
We study the mathematical theory of quantum resonances in the standard model of non-relativistic QED and in Nelson's model. In particular, we estimate the survival probability of metastable states corresponding to quantum resonances and relate the resonances to poles of an analytic continuation of matrix elements of the resolvent of the quantum Hamiltonian.
math-ph math.MP
we study the mathematical theory of quantum resonances in the standard model of nonrelativistic qed and in nelsons model in particular we estimate the survival probability of metastable states corresponding to quantum resonances and relate the resonances to poles of an analytic continuation of matrix elements of the resolvent of the quantum hamiltonian
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711.4709
Medium Modifcations of Mesons in Elementary Reactions and Heavy-Ion Collisions
Experimental searches for modifications of vector mesons in the nuclear medium are reviewed. Data on $\rho,\omega$ and $\Phi$ mesons are presented. The results have been obtained in elementary reactions with proton and photon beams as well as in heavy-ion collisions. Compared to the free particle properties, the $\omega$ and $\Phi$ meson are found to drop in mass at normal nuclear matter density by 9-14% and 3.5% whereas their widths are reported to increase by factors of about 16 and 3.6, respectively. For the $\rho$ meson, conflicting results on in-medium mass shifts and broadening have been published. The experimental data are compared to recent model calculations.
nucl-ex
experimental searches for modifications of vector mesons in the nuclear medium are reviewed data on rhoomega and phi mesons are presented the results have been obtained in elementary reactions with proton and photon beams as well as in heavyion collisions compared to the free particle properties the omega and phi meson are found to drop in mass at normal nuclear matter density by 914 and 35 whereas their widths are reported to increase by factors of about 16 and 36 respectively for the rho meson conflicting results on inmedium mass shifts and broadening have been published the experimental data are compared to recent model calculations
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711.471
Effects of network topology on wealth distributions
We focus on the problem of how wealth is distributed among the units of a networked economic system. We first review the empirical results documenting that in many economies the wealth distribution is described by a combination of log--normal and power--law behaviours. We then focus on the Bouchaud--M\'ezard model of wealth exchange, describing an economy of interacting agents connected through an exchange network. We report analytical and numerical results showing that the system self--organises towards a stationary state whose associated wealth distribution depends crucially on the underlying interaction network. In particular we show that if the network displays a homogeneous density of links, the wealth distribution displays either the log--normal or the power--law form. This means that the first--order topological properties alone (such as the scale--free property) are not enough to explain the emergence of the empirically observed \emph{mixed} form of the wealth distribution. In order to reproduce this nontrivial pattern, the network has to be heterogeneously divided into regions with variable density of links. We show new results detailing how this effect is related to the higher--order correlation properties of the underlying network. In particular, we analyse assortativity by degree and the pairwise wealth correlations, and discuss the effects that these properties have on each other.
q-fin.GN nlin.AO physics.data-an physics.soc-ph
we focus on the problem of how wealth is distributed among the units of a networked economic system we first review the empirical results documenting that in many economies the wealth distribution is described by a combination of lognormal and powerlaw behaviours we then focus on the bouchaudmezard model of wealth exchange describing an economy of interacting agents connected through an exchange network we report analytical and numerical results showing that the system selforganises towards a stationary state whose associated wealth distribution depends crucially on the underlying interaction network in particular we show that if the network displays a homogeneous density of links the wealth distribution displays either the lognormal or the powerlaw form this means that the firstorder topological properties alone such as the scalefree property are not enough to explain the emergence of the empirically observed emphmixed form of the wealth distribution in order to reproduce this nontrivial pattern the network has to be heterogeneously divided into regions with variable density of links we show new results detailing how this effect is related to the higherorder correlation properties of the underlying network in particular we analyse assortativity by degree and the pairwise wealth correlations and discuss the effects that these properties have on each other
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711.4711
NNLO corrections to event shapes in $e^+e^-$ annihilation
We compute the next-to-next-to-leading order (NNLO) QCD corrections to the six most important event shape variables related to three-particle final states in electron-positron annihilation. The corrections are sizeable for all variables, however their magnitude is substantially different for different observables. We observe that the NNLO corrections yield a considerably better agreement between theory and experimental data both in shape and normalisation of the event shape distributions. The renormalisation scale dependence of the theoretical prediction is substantially reduced compared to the previously existing NLO results. Our results will allow a precise determination of the strong coupling constant from event shape data collected at LEP.
hep-ph
we compute the nexttonexttoleading order nnlo qcd corrections to the six most important event shape variables related to threeparticle final states in electronpositron annihilation the corrections are sizeable for all variables however their magnitude is substantially different for different observables we observe that the nnlo corrections yield a considerably better agreement between theory and experimental data both in shape and normalisation of the event shape distributions the renormalisation scale dependence of the theoretical prediction is substantially reduced compared to the previously existing nlo results our results will allow a precise determination of the strong coupling constant from event shape data collected at lep
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711.4712
Programmable discriminator of coherent states - experimental realization
The optical implementation of the recently proposed unambiguous identification of coherent states is presented. Our system works as a programmable discriminator between two, in general non-orthogonal weak coherent states. The principle of operation lies in the interference of three light beams - two program states and one unknown coherent state which can be equal to whichever of the two program states. The experiment is based on fiber optics. Its results confirm theoretical predictions and the experimental setup can be straightforwardly extended for higher numbers of program states.
quant-ph
the optical implementation of the recently proposed unambiguous identification of coherent states is presented our system works as a programmable discriminator between two in general nonorthogonal weak coherent states the principle of operation lies in the interference of three light beams two program states and one unknown coherent state which can be equal to whichever of the two program states the experiment is based on fiber optics its results confirm theoretical predictions and the experimental setup can be straightforwardly extended for higher numbers of program states
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711.4713
Six-Photon Amplitudes in Scalar QED
The analytical result for the six-photon helicity amplitudes in scalar QED is presented. To compute the loop, a recently developed method based on multiple cuts is used. The amplitudes for QED and $QED^{\caln=1}$ are also derived using the supersymmetric decomposition linking the three theories.
hep-ph
the analytical result for the sixphoton helicity amplitudes in scalar qed is presented to compute the loop a recently developed method based on multiple cuts is used the amplitudes for qed and qedcaln1 are also derived using the supersymmetric decomposition linking the three theories
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711.4714
Effects due to Resonant and Continuum States on the Neutrino-Nucleus Cross Section
Estimates of the neutrino-nucleus cross section, for the charged-current process nu+208Pb-> e+208Bi, are presented. The nuclear structure calculations have been performed by considering bound, resonant, and continuum states in the single-particle basis used to construct correlated proton-particle neutron-hole configurations. The observed features of the spectrum of 208Bi have been reproduced, as accurately as possible, by diagonalizing a phenomenological multipole-multipole interaction. Calculations of the cross section, for values of q 200 $ MeV, were performed, and the dependence of the results upon the choice of the residual proton-neutron interaction was investigated. It is found that the inclusion of resonant states in the calculation of the nuclear wave functions increases the neutrino-nucleus cross section, and that the contribution of the continuum is negligible.
nucl-th
estimates of the neutrinonucleus cross section for the chargedcurrent process nu208pb e208bi are presented the nuclear structure calculations have been performed by considering bound resonant and continuum states in the singleparticle basis used to construct correlated protonparticle neutronhole configurations the observed features of the spectrum of 208bi have been reproduced as accurately as possible by diagonalizing a phenomenological multipolemultipole interaction calculations of the cross section for values of q 200 mev were performed and the dependence of the results upon the choice of the residual protonneutron interaction was investigated it is found that the inclusion of resonant states in the calculation of the nuclear wave functions increases the neutrinonucleus cross section and that the contribution of the continuum is negligible
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711.4715
The RMS Survey: A Galaxy-wide Sample of Massive Young Stellar Objects
Here we describe the Red MSX Source (RMS) survey which is the largest, systematic, galaxy-wide search for massive young stellar objects (MYSOs) yet undertaken. Mid-IR bright point sources from the MSX satellite survey have been followed-up with ground-based radio, millimetre, and infrared observations to identify the contaminating sources and characterise the MYSOs and UCHII regions. With the initial classification now complete the distribution of sources in the galaxy will be discussed, as well as some programmes being developed to exploit our sample.
astro-ph
here we describe the red msx source rms survey which is the largest systematic galaxywide search for massive young stellar objects mysos yet undertaken midir bright point sources from the msx satellite survey have been followedup with groundbased radio millimetre and infrared observations to identify the contaminating sources and characterise the mysos and uchii regions with the initial classification now complete the distribution of sources in the galaxy will be discussed as well as some programmes being developed to exploit our sample
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711.4716
The Theory of Kairons
In relativistic quantum mechanics wave functions of particles satisfy field equations that have initial data on a space--like hypersurface. We propose a dual field theory of ``wavicles'' that have their initial data on a time--like worldline. Propagation of such fields is superluminal, even though the Hilbert space of the solutions carries a unitary representation of the Poincare group of mass zero. We call the objects described by these field equations ``Kairons''. The paper builds the field equations in a general relativistic framework, allowing for a torsion. Kairon fields are section of a vector bundle over space-time. The bundle has infinite--dimensional fibres.
math-ph gr-qc math.MP quant-ph
in relativistic quantum mechanics wave functions of particles satisfy field equations that have initial data on a spacelike hypersurface we propose a dual field theory of wavicles that have their initial data on a timelike worldline propagation of such fields is superluminal even though the hilbert space of the solutions carries a unitary representation of the poincare group of mass zero we call the objects described by these field equations kairons the paper builds the field equations in a general relativistic framework allowing for a torsion kairon fields are section of a vector bundle over spacetime the bundle has infinitedimensional fibres
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711.4717
Five Conferences on Undecidability
These five lectures on undecidability were given to students with a good level in mathematics but with no special knowledge on logic. The first conference presents the formalization of mathematics with a short historical survey, the language of first order predicates and the axioms of set theory. The second and third lectures explain the incompleteness phenomena from the Hilbert program until G\"odel's theorems with a presentation of the sequent calculus of Gentzen.The fourth talk deepens model theory reasoning in the case of the continuum hypothesis, and the last conference gives examples of effective computability results.
math.LO
these five lectures on undecidability were given to students with a good level in mathematics but with no special knowledge on logic the first conference presents the formalization of mathematics with a short historical survey the language of first order predicates and the axioms of set theory the second and third lectures explain the incompleteness phenomena from the hilbert program until godels theorems with a presentation of the sequent calculus of gentzenthe fourth talk deepens model theory reasoning in the case of the continuum hypothesis and the last conference gives examples of effective computability results
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711.4718
Increase of Thermal Resistance Between a Nanostructure and a Surface due to Phonon Multireflections
The thermal resistance between a nanostructure and a half-body is calculated in the framework of particle-phonons physics. The current models approximate the nanostructure as a thermal bath. We prove that the multireflections of heat carriers in the nanostructure significantly increase resistance in contradiction with former predictions. This increase depends on the shape of the nanostructure and the heat carriers mean free path only. We provide a general and simple expression for the contact resistance and examine the specific cases of nanowires and nanoparticles.
physics.class-ph cond-mat.mtrl-sci
the thermal resistance between a nanostructure and a halfbody is calculated in the framework of particlephonons physics the current models approximate the nanostructure as a thermal bath we prove that the multireflections of heat carriers in the nanostructure significantly increase resistance in contradiction with former predictions this increase depends on the shape of the nanostructure and the heat carriers mean free path only we provide a general and simple expression for the contact resistance and examine the specific cases of nanowires and nanoparticles
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711.4719
Young stellar populations in the Magellanic Clouds
We discuss the young population of stars and clusters in the Magellanic Clouds. We present the discovery of pre-main sequence candidates in the nebula N~11 in the Large Magellanic Clouds using HST ACS photometry. The comparison of the Colour-Magnitude diagram with pre-main sequence tracks and the presence of Spitzer objects YSO I and II suggest that the star formation has been active for a long period in the region, from a few $10^5$ yrs to several Myr ago
astro-ph
we discuss the young population of stars and clusters in the magellanic clouds we present the discovery of premain sequence candidates in the nebula n11 in the large magellanic clouds using hst acs photometry the comparison of the colourmagnitude diagram with premain sequence tracks and the presence of spitzer objects yso i and ii suggest that the star formation has been active for a long period in the region from a few 105 yrs to several myr ago
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711.472
Realization of XNOR and NAND spin-wave logic gates
We demonstrate the functionality of spin-wave logic XNOR and NAND gates based on a Mach-Zehnder type interferometer which has arms implemented as sections of ferrite film spin-wave waveguides. Logical input signals are applied to the gates by varying either the phase or the amplitude of the spin waves in the interferometer arms. This phase or amplitude variation is produced by Oersted fields of dc current pulses through conductors placed on the surface of the magnetic films.
cond-mat.other
we demonstrate the functionality of spinwave logic xnor and nand gates based on a machzehnder type interferometer which has arms implemented as sections of ferrite film spinwave waveguides logical input signals are applied to the gates by varying either the phase or the amplitude of the spin waves in the interferometer arms this phase or amplitude variation is produced by oersted fields of dc current pulses through conductors placed on the surface of the magnetic films
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711.4721
New Lump-like Structures in Scalar-field Models
In this work we investigate lump-like solutions in models described by a single real scalar field. We start considering non-topological solutions with the usual lump-like form, and then we study other models, where the bell-shape profile may have varying amplitude and width, or develop a flat plateau at its top, or even induce a lump on top of another lump. We suggest possible applications where these exotic solutions might be used in several distinct branches of physics.
hep-th hep-ph
in this work we investigate lumplike solutions in models described by a single real scalar field we start considering nontopological solutions with the usual lumplike form and then we study other models where the bellshape profile may have varying amplitude and width or develop a flat plateau at its top or even induce a lump on top of another lump we suggest possible applications where these exotic solutions might be used in several distinct branches of physics
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711.4722
The heavy-quark potential in an anisotropic plasma
We determine the hard-loop resummed propagator in an anisotropic QCD plasma in general covariant gauges and define a potential between heavy quarks from the Fourier transform of its static limit. We find that there is stronger attraction on distance scales on the order of the inverse Debye mass for quark pairs aligned along the direction of anisotropy than for transverse alignment.
hep-ph nucl-th
we determine the hardloop resummed propagator in an anisotropic qcd plasma in general covariant gauges and define a potential between heavy quarks from the fourier transform of its static limit we find that there is stronger attraction on distance scales on the order of the inverse debye mass for quark pairs aligned along the direction of anisotropy than for transverse alignment
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711.4723
The Israel Theorem: What is Nature Trying to Tell Us?
We explore the possible physical consequences derived from the fact that the only static and asymptotically-flat vacuum space-time possessing a regular horizon is the Schwarzschild solution (Israel theorem). If small deviations from the Schwarzschild metric are described by means of exact solutions to Einstein equations (as it should be), then for very compact configurations, at the time scale at which radiatable multipole moments are radiated away, important physical phenomena should occur, as illustrated by some results on different solutions beloging to the Weyl class of static axially--symmetric solutions to the Einstein equations.
gr-qc astro-ph physics.space-ph
we explore the possible physical consequences derived from the fact that the only static and asymptoticallyflat vacuum spacetime possessing a regular horizon is the schwarzschild solution israel theorem if small deviations from the schwarzschild metric are described by means of exact solutions to einstein equations as it should be then for very compact configurations at the time scale at which radiatable multipole moments are radiated away important physical phenomena should occur as illustrated by some results on different solutions beloging to the weyl class of static axiallysymmetric solutions to the einstein equations
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711.4724
A viscoelastic deadly fluid in carnivorous pitcher plants
Background : The carnivorous plants of the genus Nepenthes, widely distributed in the Asian tropics, rely mostly on nutrients derived from arthropods trapped in their pitcher-shaped leaves and digested by their enzymatic fluid. The genus exhibits a great diversity of prey and pitcher forms and its mechanism of trapping has long intrigued scientists. The slippery inner surfaces of the pitchers, which can be waxy or highly wettable, have so far been considered as the key trapping devices. However, the occurrence of species lacking such epidermal specializations but still effective at trapping insects suggests the possible implication of other mechanisms. Methodology/Principal Findings : Using a combination of insect bioassays, high-speed video and rheological measurements, we show that the digestive fluid of Nepenthes rafflesiana is highly viscoelastic and that this physical property is crucial for the retention of insects in its traps. Trapping efficiency is shown to remain strong even when the fluid is highly diluted by water, as long as the elastic relaxation time of the fluid is higher than the typical time scale of insect movements. Conclusions/Significance : This finding challenges the common classification of Nepenthes pitchers as simple passive traps and is of great adaptive significance for these tropical plants, which are often submitted to high rainfalls and variations in fluid concentration. The viscoelastic trap constitutes a cryptic but potentially widespread adaptation of Nepenthes species and could be a homologous trait shared through common ancestry with the sundew (Drosera) flypaper plants. Such large production of a highly viscoelastic biopolymer fluid in permanent pools is nevertheless unique in the plant kingdom and suggests novel applications for pest control.
q-bio.PE
background the carnivorous plants of the genus nepenthes widely distributed in the asian tropics rely mostly on nutrients derived from arthropods trapped in their pitchershaped leaves and digested by their enzymatic fluid the genus exhibits a great diversity of prey and pitcher forms and its mechanism of trapping has long intrigued scientists the slippery inner surfaces of the pitchers which can be waxy or highly wettable have so far been considered as the key trapping devices however the occurrence of species lacking such epidermal specializations but still effective at trapping insects suggests the possible implication of other mechanisms methodologyprincipal findings using a combination of insect bioassays highspeed video and rheological measurements we show that the digestive fluid of nepenthes rafflesiana is highly viscoelastic and that this physical property is crucial for the retention of insects in its traps trapping efficiency is shown to remain strong even when the fluid is highly diluted by water as long as the elastic relaxation time of the fluid is higher than the typical time scale of insect movements conclusionssignificance this finding challenges the common classification of nepenthes pitchers as simple passive traps and is of great adaptive significance for these tropical plants which are often submitted to high rainfalls and variations in fluid concentration the viscoelastic trap constitutes a cryptic but potentially widespread adaptation of nepenthes species and could be a homologous trait shared through common ancestry with the sundew drosera flypaper plants such large production of a highly viscoelastic biopolymer fluid in permanent pools is nevertheless unique in the plant kingdom and suggests novel applications for pest control
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711.4725
Asymptotically efficient estimators for nonparametric heteroscedastic regression models
This paper concerns the estimation of the regression function at a given point in nonparametric heteroscedastic models with Gaussian noise or with noise having unknown distribution. In the two cases an asymptotically efficient kernel estimator is constructed for the minimax absolute error risk.
math.ST stat.TH
this paper concerns the estimation of the regression function at a given point in nonparametric heteroscedastic models with gaussian noise or with noise having unknown distribution in the two cases an asymptotically efficient kernel estimator is constructed for the minimax absolute error risk
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711.4726
Mean-field dynamo in a turbulence with shear and kinetic helicity fluctuations
We study effects of kinetic helicity fluctuations in a turbulence with large-scale shear using two different approaches: the spectral tau-approximation and the second order correlation approximation (or first-order smoothing approximation). These two approaches demonstrate that homogeneous kinetic helicity fluctuations alone with zero mean value in a sheared homogeneous turbulence cannot cause large-scale dynamo. Mean-field dynamo can be possible when kinetic helicity fluctuations are inhomogeneous which cause a nonzero mean alpha effect in a sheared turbulence. On the other hand, shear-current effect can generate large-scale magnetic field even in a homogeneous nonhelical turbulence with large-scale shear. This effect was investigated previously for large hydrodynamic and magnetic Reynolds numbers. In this study we examine the threshold required for the shear-current dynamo versus Reynolds number. We demonstrate that there is no need for a developed inertial range in order to maintain the shear-current dynamo (e.g., the threshold in the Reynolds number is of the order of 1).
astro-ph
we study effects of kinetic helicity fluctuations in a turbulence with largescale shear using two different approaches the spectral tauapproximation and the second order correlation approximation or firstorder smoothing approximation these two approaches demonstrate that homogeneous kinetic helicity fluctuations alone with zero mean value in a sheared homogeneous turbulence cannot cause largescale dynamo meanfield dynamo can be possible when kinetic helicity fluctuations are inhomogeneous which cause a nonzero mean alpha effect in a sheared turbulence on the other hand shearcurrent effect can generate largescale magnetic field even in a homogeneous nonhelical turbulence with largescale shear this effect was investigated previously for large hydrodynamic and magnetic reynolds numbers in this study we examine the threshold required for the shearcurrent dynamo versus reynolds number we demonstrate that there is no need for a developed inertial range in order to maintain the shearcurrent dynamo eg the threshold in the reynolds number is of the order of 1
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711.4727
Third Family Corrections to Tri-bimaximal Lepton Mixing and a New Sum Rule
We investigate the theoretical stability of the predictions of tri-bimaximal neutrino mixing with respect to third family wave-function corrections. Such third family wave-function corrections can arise from either the canonical normalisation of the kinetic terms or renormalisation group running effects. At leading order both sorts of corrections can be subsumed into a single universal parameter. For hierarchical neutrinos, this leads to a new testable lepton mixing sum rule 's = r cos delta + 2/3 a' (where s, r, a describe the deviations of solar, reactor and atmospheric mixing angles from their tri-bimaximal values, and 'delta' is the observable Dirac CP phase) which is stable under all leading order third family wave-function corrections, as well as Cabibbo-like charged lepton mixing effects.
hep-ph
we investigate the theoretical stability of the predictions of tribimaximal neutrino mixing with respect to third family wavefunction corrections such third family wavefunction corrections can arise from either the canonical normalisation of the kinetic terms or renormalisation group running effects at leading order both sorts of corrections can be subsumed into a single universal parameter for hierarchical neutrinos this leads to a new testable lepton mixing sum rule s r cos delta 23 a where s r a describe the deviations of solar reactor and atmospheric mixing angles from their tribimaximal values and delta is the observable dirac cp phase which is stable under all leading order third family wavefunction corrections as well as cabibbolike charged lepton mixing effects
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711.4728
Rotation set and Entropy
In 1991 Llibre and MacKay proved that if $f$ is a 2-torus homeomorphism isotopic to identity and the rotation set of $f$ has a non empty interior then $f$ has positive topological entropy. Here, we give a converselike theorem. We show that the interior of the rotation set of a 2-torus $C^{1+ \alpha}$ diffeomorphism isotopic to identity of positive topological entropy is not empty, under the additional hypotheses that $f$ is topologically transitive and irreducible. We also give examples that show that these hypotheses are necessary.
math.DS
in 1991 llibre and mackay proved that if f is a 2torus homeomorphism isotopic to identity and the rotation set of f has a non empty interior then f has positive topological entropy here we give a converselike theorem we show that the interior of the rotation set of a 2torus c1 alpha diffeomorphism isotopic to identity of positive topological entropy is not empty under the additional hypotheses that f is topologically transitive and irreducible we also give examples that show that these hypotheses are necessary
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711.4729
Bogoliubov theory of quantum correlations in the time-dependent Bose-Hubbard model
By means of an adapted mean-field expansion for large fillings $n\gg1$, we study the evolution of quantum fluctuations in the time-dependent Bose-Hubbard model, starting in the superfluid state and approaching the Mott phase by decreasing the tunneling rate or increasing the interaction strength in time. For experimentally relevant cases, we derive analytical results for the temporal behavior of the number and phase fluctuations, respectively. This allows us to calculate the growth of the quantum depletion and the decay of off-diagonal long-range order. We estimate the conditions for the observability of the time dependence in the correlation functions in the experimental setups with external trapping present. Finally, we discuss the analogy to quantum effects in the early universe during the inflationary epoch.
cond-mat.other quant-ph
by means of an adapted meanfield expansion for large fillings ngg1 we study the evolution of quantum fluctuations in the timedependent bosehubbard model starting in the superfluid state and approaching the mott phase by decreasing the tunneling rate or increasing the interaction strength in time for experimentally relevant cases we derive analytical results for the temporal behavior of the number and phase fluctuations respectively this allows us to calculate the growth of the quantum depletion and the decay of offdiagonal longrange order we estimate the conditions for the observability of the time dependence in the correlation functions in the experimental setups with external trapping present finally we discuss the analogy to quantum effects in the early universe during the inflationary epoch
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711.473
Ueber die Tiefe von Invariantenringen unendlicher Gruppen
Let K be an algebraically closed field. For a graded K-Algebra R, we write cmdef R:=dim R -depth R. We show that for each reductive group G (over K) which is not linearly reductive, there exists a faithful G-module V such that cmdef K[\sum_i=1^k V]^G >= k-2 for all k. We will give such a V explicitly.
math.AC
let k be an algebraically closed field for a graded kalgebra r we write cmdef rdim r depth r we show that for each reductive group g over k which is not linearly reductive there exists a faithful gmodule v such that cmdef ksum_i1k vg k2 for all k we will give such a v explicitly
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711.4731
Competing Orders in One-Dimensional Half-Integer Fermionic Cold Atoms: A Conformal Field Theory Approach
The physical properties of arbitrary half-integer spins F = N - 1/2 fermionic cold atoms loaded into a one-dimensional optical lattice are investigated by means of a conformal field theory approach. We show that for attractive interactions two different superfluid phases emerge for F \ge 3/2: A BCS pairing phase, and a molecular superfluid phase which is formed from bound-states made of 2N fermions. In the low-energy approach, the competition between these instabilities and charge-density waves is described in terms of Z_N parafermionic degrees of freedom. The quantum phase transition for F=3/2,5/2 is universal and shown to belong to the Ising and three-state Potts universality classes respectively. For a filling of one atom per site, a Mott transition occurs and the nature of the possible Mott-insulating phases are determined.
cond-mat.str-el hep-th
the physical properties of arbitrary halfinteger spins f n 12 fermionic cold atoms loaded into a onedimensional optical lattice are investigated by means of a conformal field theory approach we show that for attractive interactions two different superfluid phases emerge for f ge 32 a bcs pairing phase and a molecular superfluid phase which is formed from boundstates made of 2n fermions in the lowenergy approach the competition between these instabilities and chargedensity waves is described in terms of z_n parafermionic degrees of freedom the quantum phase transition for f3252 is universal and shown to belong to the ising and threestate potts universality classes respectively for a filling of one atom per site a mott transition occurs and the nature of the possible mottinsulating phases are determined
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711.4732
Spherical symmetric charged solution with cosmological constant
A spherically symmetric charged ideal fluid solution of Einstein field equation is given in the presence of the cosmological constant and two well known example of this type of solution is presented. If the matter is confined in a region, the exterior spacetime is considered as RN-de Sitter (Reissner-Nordstrom de Sitter) and to complete solution matching conditions are examined. We show that the function which is related to the dynamics of the system will determine the fate of the system: expansion, contraction or bouncing situations may occur for different configurations. The initial conditions of the matter determine the final form of the system and therefore the nature of the singularities in the presence of the electric charge and the cosmological constant is examined to reveal their effects on the singularity formation during collapse.
gr-qc
a spherically symmetric charged ideal fluid solution of einstein field equation is given in the presence of the cosmological constant and two well known example of this type of solution is presented if the matter is confined in a region the exterior spacetime is considered as rnde sitter reissnernordstrom de sitter and to complete solution matching conditions are examined we show that the function which is related to the dynamics of the system will determine the fate of the system expansion contraction or bouncing situations may occur for different configurations the initial conditions of the matter determine the final form of the system and therefore the nature of the singularities in the presence of the electric charge and the cosmological constant is examined to reveal their effects on the singularity formation during collapse
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711.4733
A Coupled Oscillator Model for Grover's Quantum Database Search Algorithm
Grover's database search algorithm is the optimal algorithm for finding a desired object from an unsorted collection of items. Although it was discovered in the context of quantum computation, it is simple and versatile enough to be implemented using any physical system that allows superposition of states, and several proposals have been made in the literature. I study a mechanical realisation of the algorithm using coupled simple harmonic oscillators, and construct its physical model for the simplest case of four identical oscillators. The identification oracle is implemented as an elastic reflection of the desired oscillator, and the overrelaxation operation is realised as evolution of the system by half an oscillation period. I derive the equations of motion, and solve them both analytically and by computer simulation. I extend the ideal case analysis and explore the sensitivity of the algorithm to changes in the initial conditions, masses of springs and damping. The amplitude amplification provided by the algorithm enhances the energy of the desired oscillator, while running the algorithm backwards spreads out the energy of the perturbed oscillator among its partners. The former (efficient focusing of energy into a specific oscillator) can have interesting applications in processes that need crossing of an energy threshold for completion, and can be useful in nanotechnological devices and catalysis. The latter (efficient redistribution of energy) can be useful in processes requiring rapid dissipation of energy, such as shock-absorbers and vibrational shielding. I present some tentative proposals.
physics.gen-ph physics.class-ph quant-ph
grovers database search algorithm is the optimal algorithm for finding a desired object from an unsorted collection of items although it was discovered in the context of quantum computation it is simple and versatile enough to be implemented using any physical system that allows superposition of states and several proposals have been made in the literature i study a mechanical realisation of the algorithm using coupled simple harmonic oscillators and construct its physical model for the simplest case of four identical oscillators the identification oracle is implemented as an elastic reflection of the desired oscillator and the overrelaxation operation is realised as evolution of the system by half an oscillation period i derive the equations of motion and solve them both analytically and by computer simulation i extend the ideal case analysis and explore the sensitivity of the algorithm to changes in the initial conditions masses of springs and damping the amplitude amplification provided by the algorithm enhances the energy of the desired oscillator while running the algorithm backwards spreads out the energy of the perturbed oscillator among its partners the former efficient focusing of energy into a specific oscillator can have interesting applications in processes that need crossing of an energy threshold for completion and can be useful in nanotechnological devices and catalysis the latter efficient redistribution of energy can be useful in processes requiring rapid dissipation of energy such as shockabsorbers and vibrational shielding i present some tentative proposals
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711.4734
Signed Chord Length Distribution. I
In this paper is discussed an application of signed measures (charges) to description of segment and chord length distributions in nonconvex bodies. The signed distribution may naturally appears due to definition via derivatives of nonnegative autocorrelation function simply related with distances distribution between pairs of points in the body. In the work is suggested constructive geometrical interpretation of such derivatives and illustrated appearance of "positive" and "negative" elements similar with usual Hanh-Jordan decomposition in measure theory. The construction is also close related with applications of Dirac method of chords.
math-ph math.MP math.PR stat.CO
in this paper is discussed an application of signed measures charges to description of segment and chord length distributions in nonconvex bodies the signed distribution may naturally appears due to definition via derivatives of nonnegative autocorrelation function simply related with distances distribution between pairs of points in the body in the work is suggested constructive geometrical interpretation of such derivatives and illustrated appearance of positive and negative elements similar with usual hanhjordan decomposition in measure theory the construction is also close related with applications of dirac method of chords
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711.4735
Recovering the stationary phase condition for accurately obtaining scattering and tunneling times
The stationary phase method is often employed for computing tunneling {\em phase} times of analytically-continuous {\em gaussian} or infinite-bandwidth step pulses which collide with a potential barrier. The indiscriminate utilization of this method without considering the barrier boundary effects leads to some misconceptions in the interpretation of the phase times. After reexamining the above barrier diffusion problem where we notice the wave packet collision necessarily leads to the possibility of multiple reflected and transmitted wave packets, we study the phase times for tunneling/reflecting particles in a framework where an idea of multiple wave packet decomposition is recovered. To partially overcome the analytical incongruities which rise up when tunneling phase time expressions are obtained, we present a theoretical exercise involving a symmetrical collision between two identical wave packets and a one dimensional squared potential barrier where the scattered wave packets can be recomposed by summing the amplitudes of simultaneously reflected and transmitted waves.
quant-ph
the stationary phase method is often employed for computing tunneling em phase times of analyticallycontinuous em gaussian or infinitebandwidth step pulses which collide with a potential barrier the indiscriminate utilization of this method without considering the barrier boundary effects leads to some misconceptions in the interpretation of the phase times after reexamining the above barrier diffusion problem where we notice the wave packet collision necessarily leads to the possibility of multiple reflected and transmitted wave packets we study the phase times for tunnelingreflecting particles in a framework where an idea of multiple wave packet decomposition is recovered to partially overcome the analytical incongruities which rise up when tunneling phase time expressions are obtained we present a theoretical exercise involving a symmetrical collision between two identical wave packets and a one dimensional squared potential barrier where the scattered wave packets can be recomposed by summing the amplitudes of simultaneously reflected and transmitted waves
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711.4736
Beam spin asymmetry in deep and exclusive pi0 electroproduction
The beam spin asymmetry (BSA) in the exclusive reaction ep->ep pi0 was measured with the CEBAF 5.77 GeV polarized electron beam and Large Acceptance Spectrometer(CLAS). The xB, Q2, t and phi dependences of the pi0 BSA are presented in the deep inelastic regime. The asymmetries are fitted with a sin(phi) function and their amplitudes are extracted. Overall, they are of the order of 0.04 - 0.11 and roughly independent of t. This is the signature of a non-zero longitudinal-transverse interference. The implications concerning the applicability of a formalism based on generalized parton distributions, as well as the extension of a Regge formalism at high photon virtualities, are discussed.
hep-ex
the beam spin asymmetry bsa in the exclusive reaction epep pi0 was measured with the cebaf 577 gev polarized electron beam and large acceptance spectrometerclas the xb q2 t and phi dependences of the pi0 bsa are presented in the deep inelastic regime the asymmetries are fitted with a sinphi function and their amplitudes are extracted overall they are of the order of 004 011 and roughly independent of t this is the signature of a nonzero longitudinaltransverse interference the implications concerning the applicability of a formalism based on generalized parton distributions as well as the extension of a regge formalism at high photon virtualities are discussed
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711.4737
Observation of free hole gases at ambient conditions
By studying fluctuations in the electrostatic potential of a single electrode immersed in a cold plasma, we were able to perform in situ electron spectroscopy. Electron exchange processes that occur at the surface of the electrode were triggered by the surface Auger process either using metastable molecular nitrogen or triplet helium at ambient conditions. Ongoing redox reactions were decomposed into their two fundamental half reactions and the reduction and oxidation potentials were detected. We found that redox reactions near the electrode surface are the result of binary interactions of a free electron gas with a free hole gas that occur on a femtosecond time scale. The measured lifetimes of electron-hole recombination processes and the elastic scattering rate of the hole-hole process are in fair agreement with theoretical estimates. The observed asymmetry in the energy distributions of free electron and free hole ensembles suggests that at thermal equilibrium the identity of hole differs from that of an electron vacancy.
cond-mat.str-el
by studying fluctuations in the electrostatic potential of a single electrode immersed in a cold plasma we were able to perform in situ electron spectroscopy electron exchange processes that occur at the surface of the electrode were triggered by the surface auger process either using metastable molecular nitrogen or triplet helium at ambient conditions ongoing redox reactions were decomposed into their two fundamental half reactions and the reduction and oxidation potentials were detected we found that redox reactions near the electrode surface are the result of binary interactions of a free electron gas with a free hole gas that occur on a femtosecond time scale the measured lifetimes of electronhole recombination processes and the elastic scattering rate of the holehole process are in fair agreement with theoretical estimates the observed asymmetry in the energy distributions of free electron and free hole ensembles suggests that at thermal equilibrium the identity of hole differs from that of an electron vacancy
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711.4738
Interpreting the Quantum Wave Function in Terms of 'Interacting Faculties'
In this article we discuss the problem of finding an interpretation of quantum mechanics which provides an objective account of physical reality. In the first place we discuss the problem of interpretation and analyze the importance of such an objective account in physics. In this context we present the problems which arise when interpreting the quantum wave function within the orthodox formulation of quantum mechanics. In connection to this critic, we expose the concept of 'entity' as an epistemological obstruction. In the second part of this paper we discuss the relation between actuality and potentiality in classical and quantum physics, and continue to present the concept of 'ontological potentiality' which is distinguished from the generic Aristotelian notion of potentiality in terms of 'becoming actual'. In this paper our main aim is to provide an objective interpretation of quantum mechanics which allows us to discuss the meaning of physical reality according to the theory. For this specific propose we present the concept of 'faculty' in place of the concept of 'entity'. Within our theory of faculties, we continue to discuss and interpret two paradigmatic experiments of quantum mechanics such as the double-slit and Schrodinger's cat.
quant-ph
in this article we discuss the problem of finding an interpretation of quantum mechanics which provides an objective account of physical reality in the first place we discuss the problem of interpretation and analyze the importance of such an objective account in physics in this context we present the problems which arise when interpreting the quantum wave function within the orthodox formulation of quantum mechanics in connection to this critic we expose the concept of entity as an epistemological obstruction in the second part of this paper we discuss the relation between actuality and potentiality in classical and quantum physics and continue to present the concept of ontological potentiality which is distinguished from the generic aristotelian notion of potentiality in terms of becoming actual in this paper our main aim is to provide an objective interpretation of quantum mechanics which allows us to discuss the meaning of physical reality according to the theory for this specific propose we present the concept of faculty in place of the concept of entity within our theory of faculties we continue to discuss and interpret two paradigmatic experiments of quantum mechanics such as the doubleslit and schrodingers cat
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711.4739
Finite Gap Jacobi Matrices: An Announcement
We consider Jacobi matrices whose essential spectrum is a finite union of closed intervals. We focus on Szego's theorem, Jost solutions, and Szego asymptotics for this situation. This announcement describes talks the authors gave at OPSFA 2007.
math.SP math.CA
we consider jacobi matrices whose essential spectrum is a finite union of closed intervals we focus on szegos theorem jost solutions and szego asymptotics for this situation this announcement describes talks the authors gave at opsfa 2007
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711.474
On the depth of invariant rings of infinite groups
Let K be an algebraically closed field. For a finitely generated graded K algebra R, let cmdef R := dim R - depth R denote the Cohen-Macaulay-defect of R. Let G be a linear algebraic group over K that is reductive but not linearly reductive. We show that there exists a faithful rational representation V of G (which we will give explicitly) such that cmdef K[\sum_i=1^k V]^G >= k-2 for all k. We give refinements in the case G = SL2.
math.AC
let k be an algebraically closed field for a finitely generated graded k algebra r let cmdef r dim r depth r denote the cohenmacaulaydefect of r let g be a linear algebraic group over k that is reductive but not linearly reductive we show that there exists a faithful rational representation v of g which we will give explicitly such that cmdef ksum_i1k vg k2 for all k we give refinements in the case g sl2
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711.4741
The Jlab Upgrade - Studies of the Nucleon with CLAS12
An overview is presented on the program to study the nucleon structure at the 12 GeV JLab upgrade using the CLAS12 detector. The focus is on deeply virtual exclusive processes to access the generalized parton distributions, semni-inclusive processes to study transverse momentum dependent distribution functions, and inclusive spin structure functions and resonance transition form factors at high Q^2 and with high precision.
nucl-ex hep-ex hep-lat hep-ph nucl-th
an overview is presented on the program to study the nucleon structure at the 12 gev jlab upgrade using the clas12 detector the focus is on deeply virtual exclusive processes to access the generalized parton distributions semniinclusive processes to study transverse momentum dependent distribution functions and inclusive spin structure functions and resonance transition form factors at high q2 and with high precision
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711.4742
Magnetoelastic and thermal effects in the BiMn2O5 lattice: a high-resolution x-ray diffraction study
High-resolution synchrotron x-ray diffraction measurements were performed on single crystalline and powder samples of BiMn2O5. A linear temperature dependence of the unit cell volume was found between T_{N}=38$ K and 100 K, suggesting that a low-energy lattice excitation may be responsible for the lattice expansion in this temperature range. Between T* ~ 65 K and T_{N}, all lattice parameters showed incipient magnetoelastic effects, due to short-range spin correlations. An anisotropic strain along the a-direction was also observed below T*. Below T_{N}, a relatively large contraction of the a-parameter following the square of the average sublattice magnetization of Mn was found, indicating that a second-order spin hamiltonian accounts for the magnetic interactions along this direction. On the other hand, the more complex behaviors found for $b$ and $c$ suggest additional magnetic transitions below T_{N} and perhaps higher-order terms in the spin hamiltonian. Polycrystalline samples grown by distinct routes and with nearly homogeneous crystal structure above T_{N} presented structural phase coexistence below T_{N}, indicating a close competition amongst distinct magnetostructural states in this compound.
cond-mat.mtrl-sci
highresolution synchrotron xray diffraction measurements were performed on single crystalline and powder samples of bimn2o5 a linear temperature dependence of the unit cell volume was found between t_n38 k and 100 k suggesting that a lowenergy lattice excitation may be responsible for the lattice expansion in this temperature range between t 65 k and t_n all lattice parameters showed incipient magnetoelastic effects due to shortrange spin correlations an anisotropic strain along the adirection was also observed below t below t_n a relatively large contraction of the aparameter following the square of the average sublattice magnetization of mn was found indicating that a secondorder spin hamiltonian accounts for the magnetic interactions along this direction on the other hand the more complex behaviors found for b and c suggest additional magnetic transitions below t_n and perhaps higherorder terms in the spin hamiltonian polycrystalline samples grown by distinct routes and with nearly homogeneous crystal structure above t_n presented structural phase coexistence below t_n indicating a close competition amongst distinct magnetostructural states in this compound
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711.4743
Cell-permeable tumor suppressor peptides for cancer therapy: back to the future
Miniaturization is a hallmark of modern technologies. Notably, this feature has not spared molecular biology and its potential applications. Towards developing more effective therapeutics against cancer, studies began to explore more than a decade ago how natural tumor suppression could be translated into antineoplastic drugs. To this end, investigators focused on major constituents of a central pathway that protects cells against neoplastic transformation: the nuclear retinoblastoma protein (RB) pathway. As such, peptide mimetics of RB, p16 and p21 were developed. Likewise, the p53 and von Hippel-Lindau gene products which affect indirectly the RB pathway provided additional templates for the development of anti-proliferative peptides. Each of the peptides derived from these distinct tumor suppressors was made cell-permeable by its ligation to an amino acid sequence conferring cellular internalization. Details reviewed here reveal that through the application of such anti-cancer peptide therapeutics alone or in conjunction whenever synergy is to expect, the dark era of chemotherapy will likely be overcome, at last.
q-bio.BM q-bio.SC
miniaturization is a hallmark of modern technologies notably this feature has not spared molecular biology and its potential applications towards developing more effective therapeutics against cancer studies began to explore more than a decade ago how natural tumor suppression could be translated into antineoplastic drugs to this end investigators focused on major constituents of a central pathway that protects cells against neoplastic transformation the nuclear retinoblastoma protein rb pathway as such peptide mimetics of rb p16 and p21 were developed likewise the p53 and von hippellindau gene products which affect indirectly the rb pathway provided additional templates for the development of antiproliferative peptides each of the peptides derived from these distinct tumor suppressors was made cellpermeable by its ligation to an amino acid sequence conferring cellular internalization details reviewed here reveal that through the application of such anticancer peptide therapeutics alone or in conjunction whenever synergy is to expect the dark era of chemotherapy will likely be overcome at last
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711.4744
On the question of ferromagnetism in alkali metal thin films
Electronic and magnetic structure of $(100)$ films of K and Cs are calculated within the plane-wave projector augmented wave (PAW) formalism of the density functional theory (DFT) using both local spin density approximation (LSDA) and the PW91 generalized gradient approximation (GGA). Only a 6 layer Cs film is found to have a ferromagnetic (FM) state which is degenerate with a paramagnetic (PM) state within the accuracy of these calculations. This is at variance with the results obtained from a finite thickness uniform jellium model (UJM). Implications of these results for the experiments on transition metal doped alkali metal thin films and bulk hosts are discussed.
cond-mat.mtrl-sci
electronic and magnetic structure of 100 films of k and cs are calculated within the planewave projector augmented wave paw formalism of the density functional theory dft using both local spin density approximation lsda and the pw91 generalized gradient approximation gga only a 6 layer cs film is found to have a ferromagnetic fm state which is degenerate with a paramagnetic pm state within the accuracy of these calculations this is at variance with the results obtained from a finite thickness uniform jellium model ujm implications of these results for the experiments on transition metal doped alkali metal thin films and bulk hosts are discussed
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711.4745
Networking Behavior in Thin Film and Nanostructure Growth Dynamics
Thin film coatings have been essential in development of several micro and nano-scale devices. To realize thin film coatings various deposition techniques are employed, each yielding surface morphologies with different characteristics of interest. Therefore, understanding and control of the surface growth is of great interest. In this paper, we devise a novel network-based modeling of the growth dynamics of such thin films and nano-structures. We specifically map dynamic steps taking place during the growth to components (e.g., nodes, links) of a corresponding network. We present initial results showing that this network-based modeling approach to the growth dynamics can simplify our understanding of the fundamental physical dynamics such as shadowing and re-emission effects.
cond-mat.mtrl-sci cond-mat.dis-nn cond-mat.stat-mech
thin film coatings have been essential in development of several micro and nanoscale devices to realize thin film coatings various deposition techniques are employed each yielding surface morphologies with different characteristics of interest therefore understanding and control of the surface growth is of great interest in this paper we devise a novel networkbased modeling of the growth dynamics of such thin films and nanostructures we specifically map dynamic steps taking place during the growth to components eg nodes links of a corresponding network we present initial results showing that this networkbased modeling approach to the growth dynamics can simplify our understanding of the fundamental physical dynamics such as shadowing and reemission effects
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711.4746
Electron interactions in an antidot in the integer quantum Hall regime
A quantum antidot, a submicron depletion region in a two-dimensional electron system, has been actively studied in the past two decades, providing a powerful tool for understanding quantum Hall systems. In a perpendicular magnetic field, electrons form bound states around the antidot. Aharonov-Bohm resonances through such bound states have been experimentally studied, showing interesting phenomena such as Coulomb charging, h/2e oscillations, spectator modes, signatures of electron interactions in the line shape, Kondo effect, etc. None of them can be explained by a simple noninteracting electron approach. Theoretical models for the above observations have been developed recently, such as a capacitive-interaction model for explaining the h/2e oscillations and the Kondo effect, numerical prediction of a hole maximum-density-droplet antidot ground state, and spin density-functional theory for investigating the compressibility of antidot edges. In this review, we summarize such experimental and theoretical works on electron interactions in antidots.
cond-mat.mes-hall
a quantum antidot a submicron depletion region in a twodimensional electron system has been actively studied in the past two decades providing a powerful tool for understanding quantum hall systems in a perpendicular magnetic field electrons form bound states around the antidot aharonovbohm resonances through such bound states have been experimentally studied showing interesting phenomena such as coulomb charging h2e oscillations spectator modes signatures of electron interactions in the line shape kondo effect etc none of them can be explained by a simple noninteracting electron approach theoretical models for the above observations have been developed recently such as a capacitiveinteraction model for explaining the h2e oscillations and the kondo effect numerical prediction of a hole maximumdensitydroplet antidot ground state and spin densityfunctional theory for investigating the compressibility of antidot edges in this review we summarize such experimental and theoretical works on electron interactions in antidots
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711.4747
Investigating AdS/QCD duality through scalar glueball correlators
We investigate AdS/QCD duality for the two-point correlation function of the lowest dimension scalar glueball operator, in the case of the IR soft wall model. We point out the role of the boundary conditions for the bulk-to-boundary propagator in determining the gluon condensates. We show that a low energy QCD theorem can be obtained within the AdS approach, together with a gluon condensate close to the commonly accepted value and robust against perturbation of the background dilaton field.
hep-ph
we investigate adsqcd duality for the twopoint correlation function of the lowest dimension scalar glueball operator in the case of the ir soft wall model we point out the role of the boundary conditions for the bulktoboundary propagator in determining the gluon condensates we show that a low energy qcd theorem can be obtained within the ads approach together with a gluon condensate close to the commonly accepted value and robust against perturbation of the background dilaton field
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711.4748
Rho-Like Mesons from Analysis of the Pion-Pion Scattering
Considering analyticity, unitarity and an influence of coupled channels, experimental data on the isovector P-wave of pion-pion scattering was analyzed to study rho-like mesons below 1900 MeV. The analysis indicates evidently that in the energy range 1200--1800 MeV, there are three rho-like mesons: rho(1250), rho(1450) and rho(1600), unlike the PDG tables. The obtained P-wave pion-pion scattering length (a_1^1=33.9+- 2.02 [10^{-3}m_{pi^+}^{-3}]) most matches to the one calculated in the local Nambu--Jona-Lasinio model.
hep-ph
considering analyticity unitarity and an influence of coupled channels experimental data on the isovector pwave of pionpion scattering was analyzed to study rholike mesons below 1900 mev the analysis indicates evidently that in the energy range 12001800 mev there are three rholike mesons rho1250 rho1450 and rho1600 unlike the pdg tables the obtained pwave pionpion scattering length a_11339 202 103m_pi3 most matches to the one calculated in the local nambujonalasinio model
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711.4749
A Note on 3-quasi-Sasakian Geometry
3-quasi-Sasakian manifolds were recently studied by the authors as a suitable setting unifying 3-Sasakian and 3-cosymplectic geometries. In this paper some geometric properties of this class of almost 3-contact metric manifolds are briefly reviewed, with an emphasis on those more related to physical applications.
math.DG
3quasisasakian manifolds were recently studied by the authors as a suitable setting unifying 3sasakian and 3cosymplectic geometries in this paper some geometric properties of this class of almost 3contact metric manifolds are briefly reviewed with an emphasis on those more related to physical applications
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711.475
Microlensing search for extrasolar planets: observational strategy, discoveries and implications
Microlensing has proven to be a valuable tool to search for extrasolar planets of Jovian- to Super-Earth-mass planets at orbits of a few AU. Since planetary signals are of very short duration, an intense and continuous monitoring is required. This is achieved by ground-based networks of telescopes (PLANET/RoboNET, microFUN) following up targets, which are identified as microlensing events by single dedicated telescopes (OGLE, MOA). Microlensing has led to four already published detections of extrasolar planets, one of them being OGLE-2005-BLG-390Lb, a planet of only ~5.5 M_earth orbiting its M-dwarf host star at ~2.6 AU. Very recent observations (May--September 2007) provided more planetary candidates, still under study, that will double the number of detections. For non-planetary microlensing events observed from 1995 to 2006 we compute detection efficiency diagrams, which can then be used to derive an estimate of the Galactic abundance of cool planets in the mass regime from Jupiters to Sub-Neptunes.
astro-ph
microlensing has proven to be a valuable tool to search for extrasolar planets of jovian to superearthmass planets at orbits of a few au since planetary signals are of very short duration an intense and continuous monitoring is required this is achieved by groundbased networks of telescopes planetrobonet microfun following up targets which are identified as microlensing events by single dedicated telescopes ogle moa microlensing has led to four already published detections of extrasolar planets one of them being ogle2005blg390lb a planet of only 55 m_earth orbiting its mdwarf host star at 26 au very recent observations mayseptember 2007 provided more planetary candidates still under study that will double the number of detections for nonplanetary microlensing events observed from 1995 to 2006 we compute detection efficiency diagrams which can then be used to derive an estimate of the galactic abundance of cool planets in the mass regime from jupiters to subneptunes
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711.4751
Gamow-Teller strength distributions for double-beta-decaying nuclei within continuum-QRPA
A version of the pn-continuum-QRPA is outlined and applied to describe the Gamow-Teller strength distributions for $\beta\beta$-decaying open-shell nuclei. The calculation results obtained for the pairs of nuclei $^{116}$Cd-Sn and $^{130}$Te-Xe are compared with available experimental data.
nucl-th
a version of the pncontinuumqrpa is outlined and applied to describe the gamowteller strength distributions for betabetadecaying openshell nuclei the calculation results obtained for the pairs of nuclei 116cdsn and 130texe are compared with available experimental data
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711.4752
Causal Relationships between Eruptive Prominences and Coronal Mass Ejections
A close association between eruptive prominences and CMEs, both slow and fast CMEs, was reported in many studies. Sometimes it is possible to follow the material motion starting from the prominence (filament) activation to the CME in the high corona. Remnants of the prominence were found in the bright core of CMEs. However, detailed comparisons of the two phenomena reveal problems in explaining CMEs as a continuation of filament eruptions in the upper corona. For example, the heliolatitudes of the disappeared filaments and subsequent coronal ejections sometimes differ by tens of degrees. In order to clear up the problems of EP-CME association we tentatively analyse the more general question of the dynamics of a magnetic flux rope. Prominences and filaments are the best tracers of the flux ropes in the corona long before the beginning of the eruption. A twisted flux rope is held by the tension of field lines of photospheric sources until parameters of the system reach critical values and a catastrophe happens. We suggest that the associated flux rope height above the photosphere is one of these parameters and it is revealed by the height of the filament. 80 filaments were analysed and we found that eruptive prominences were near the so-called limit of stability a few days before their eruptions. We suggest that a comparison of the real heights of prominences with the calculated critical heights from magnetograms could be systematically used to predict filament eruptions and the corresponding CMEs.
astro-ph
a close association between eruptive prominences and cmes both slow and fast cmes was reported in many studies sometimes it is possible to follow the material motion starting from the prominence filament activation to the cme in the high corona remnants of the prominence were found in the bright core of cmes however detailed comparisons of the two phenomena reveal problems in explaining cmes as a continuation of filament eruptions in the upper corona for example the heliolatitudes of the disappeared filaments and subsequent coronal ejections sometimes differ by tens of degrees in order to clear up the problems of epcme association we tentatively analyse the more general question of the dynamics of a magnetic flux rope prominences and filaments are the best tracers of the flux ropes in the corona long before the beginning of the eruption a twisted flux rope is held by the tension of field lines of photospheric sources until parameters of the system reach critical values and a catastrophe happens we suggest that the associated flux rope height above the photosphere is one of these parameters and it is revealed by the height of the filament 80 filaments were analysed and we found that eruptive prominences were near the socalled limit of stability a few days before their eruptions we suggest that a comparison of the real heights of prominences with the calculated critical heights from magnetograms could be systematically used to predict filament eruptions and the corresponding cmes
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711.4753
Blowup of Jang's equation at outermost marginally trapped surfaces
The aim of this paper is to collect some facts about the blowup of Jang's equation. First, we discuss how to construct solutions that blow up at an outermost MOTS. Second, we exclude the possibility that there are extra blowup surfaces in data sets with non-positive mean curvature. Then we investigate the rate of convergence of the blowup to a cylinder near a strictly stable MOTS and show exponential convergence near a strictly stable MOTS.
gr-qc math.DG
the aim of this paper is to collect some facts about the blowup of jangs equation first we discuss how to construct solutions that blow up at an outermost mots second we exclude the possibility that there are extra blowup surfaces in data sets with nonpositive mean curvature then we investigate the rate of convergence of the blowup to a cylinder near a strictly stable mots and show exponential convergence near a strictly stable mots
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711.4754
Disentangling the Unparticles with polarized beams at e+e- colliders
Recently proposed idea of unparticles arising due to a scale invariant sector in the theory can give rise to effective operators with different Lorentz structures. We show that by using the different polarization options at the future linear e+e- colliders, the nature of these effective operators can be easily understood. The unique feature of a complex phase in the propagator of the unparticle can also be understood uniquely for the different spins by exploiting the initial beam polarizations at the International Linear Collider (ILC).
hep-ph
recently proposed idea of unparticles arising due to a scale invariant sector in the theory can give rise to effective operators with different lorentz structures we show that by using the different polarization options at the future linear ee colliders the nature of these effective operators can be easily understood the unique feature of a complex phase in the propagator of the unparticle can also be understood uniquely for the different spins by exploiting the initial beam polarizations at the international linear collider ilc
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711.4755
Band structure related wave function symmetry of amphoteric Si dopants in GaAs
Autocompensated Si-doped GaAs is studied with cross-sectional scanning tunneling spectroscopy (X-STS). The local electronic contrasts of substitutional Si(Ga) donors and Si(As) acceptors under the (110) cleavage plane are imaged with high resolution. Si(Ga) donor atoms exhibit radially symmetric contrasts. Si(As) acceptors have anisotropic features. The anisotropic acceptor contrasts are traced back to a tunnel process at the valence band edge. They reflect the probability density distribution of the localized acceptor hole state.
cond-mat.mes-hall cond-mat.dis-nn
autocompensated sidoped gaas is studied with crosssectional scanning tunneling spectroscopy xsts the local electronic contrasts of substitutional siga donors and sias acceptors under the 110 cleavage plane are imaged with high resolution siga donor atoms exhibit radially symmetric contrasts sias acceptors have anisotropic features the anisotropic acceptor contrasts are traced back to a tunnel process at the valence band edge they reflect the probability density distribution of the localized acceptor hole state
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711.4756
Recent issues in open and hidden charm spectroscopy
I present a brief review of results obtained both in open and hidden charm spectroscopy, discussing the interpretation of $D_{sJ}(2860)$, $D_{sJ}(2700)$ and X(3872).
hep-ph
i present a brief review of results obtained both in open and hidden charm spectroscopy discussing the interpretation of d_sj2860 d_sj2700 and x3872
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711.4757
The cool supergiant population of the massive young star cluster RSGC1
We present new high-resolution near-IR spectroscopy and OH maser observations to investigate the population of cool luminous stars of the young massive Galactic cluster RSGC1. Using the 2.293\micron CO-bandhead feature, we make high-precision radial velocity measurements of 16 of the 17 candidate Red Supergiants (RSGs) identified by Figer et al. We show that F16 and F17 are foreground stars, while we confirm that the rest are indeed physically-associated RSGs. We determine that Star F15, also associated with the cluster, is a Yellow Hypergiant based on its luminosity and spectroscopic similarity to $\rho$ Cas. Using the cluster's radial velocity, we have derived the kinematic distance to the cluster and revisited the stars' temperatures and luminosities. We find a larger spread of luminosities than in the discovery paper, consistent with a cluster age 30% older than previously thought (12$\pm$2Myr), and a total initial mass of $(3\pm1) \times 10^{4}$\msun. The spatial coincidence of the OH maser with F13, combined with similar radial velocities, is compelling evidence that the two are related. Combining our results with recent SiO and H$_2$O maser observations, we find that those stars with maser emission are the most luminous in the cluster. From this we suggest that the maser-active phase is associated with the end of the RSG stage, when the luminosity-mass ratios are at their highest.
astro-ph
we present new highresolution nearir spectroscopy and oh maser observations to investigate the population of cool luminous stars of the young massive galactic cluster rsgc1 using the 2293micron cobandhead feature we make highprecision radial velocity measurements of 16 of the 17 candidate red supergiants rsgs identified by figer et al we show that f16 and f17 are foreground stars while we confirm that the rest are indeed physicallyassociated rsgs we determine that star f15 also associated with the cluster is a yellow hypergiant based on its luminosity and spectroscopic similarity to rho cas using the clusters radial velocity we have derived the kinematic distance to the cluster and revisited the stars temperatures and luminosities we find a larger spread of luminosities than in the discovery paper consistent with a cluster age 30 older than previously thought 12pm2myr and a total initial mass of 3pm1 times 104msun the spatial coincidence of the oh maser with f13 combined with similar radial velocities is compelling evidence that the two are related combining our results with recent sio and h_2o maser observations we find that those stars with maser emission are the most luminous in the cluster from this we suggest that the maseractive phase is associated with the end of the rsg stage when the luminositymass ratios are at their highest
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711.4758
Generalized Galitskii approach for the vertex function of a Fermi gas with resonant interaction
We present a generalized Galitskii approach for the Bethe-Salpeter equation for the two-particle vertex function of a Fermi system with resonant interaction by accounting for the resonant state in the scattering potential and utilizing the universal form of the resonant scattering amplitude. The procedure can be carried out both for the normal as well as for the condensate state. In both cases, the vertex function in the vicinity of the resonance is shown to formally coincide with that obtained for a weakly attractive Fermi gas. Thus we justify the popular calculational framework in which results for the weakly attractive Fermi gas are formally extrapolated into the domain of strong coupling, and further to the repulsive side of the resonance, where molecular states are formed.
cond-mat.other
we present a generalized galitskii approach for the bethesalpeter equation for the twoparticle vertex function of a fermi system with resonant interaction by accounting for the resonant state in the scattering potential and utilizing the universal form of the resonant scattering amplitude the procedure can be carried out both for the normal as well as for the condensate state in both cases the vertex function in the vicinity of the resonance is shown to formally coincide with that obtained for a weakly attractive fermi gas thus we justify the popular calculational framework in which results for the weakly attractive fermi gas are formally extrapolated into the domain of strong coupling and further to the repulsive side of the resonance where molecular states are formed
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711.4759
Copeland Voting Fully Resists Constructive Control
Control and bribery are settings in which an external agent seeks to influence the outcome of an election. Faliszewski et al. [FHHR07] proved that Llull voting (which is here denoted by Copeland^1) and a variant (here denoted by Copeland^0) of Copeland voting are computationally resistant to many, yet not all, types of constructive control and that they also provide broad resistance to bribery. We study a parameterized version of Copeland voting, denoted by Copeland^alpha where the parameter alpha is a rational number between 0 and 1 that specifies how ties are valued in the pairwise comparisons of candidates in Copeland elections. We establish resistance or vulnerability results, in every previously studied control scenario, for Copeland^alpha, for each rational alpha, 0 <alpha < 1. In particular, we prove that Copeland^0.5, the system commonly referred to as ``Copeland voting,'' provides full resistance to constructive control. Among the systems with a polynomial-time winner problem, this is the first natural election system proven to have full resistance to constructive control. Results on bribery and fixed-parameter tractability of bounded-case control proven for Copeland^0 and Copeland^1 in [FHHR07] are extended to Copeland^alpha for each rational alpha, 0 < alpha < 1; we also give results in more flexible models such as microbribery and extended control.
cs.GT cs.CC cs.MA
control and bribery are settings in which an external agent seeks to influence the outcome of an election faliszewski et al fhhr07 proved that llull voting which is here denoted by copeland1 and a variant here denoted by copeland0 of copeland voting are computationally resistant to many yet not all types of constructive control and that they also provide broad resistance to bribery we study a parameterized version of copeland voting denoted by copelandalpha where the parameter alpha is a rational number between 0 and 1 that specifies how ties are valued in the pairwise comparisons of candidates in copeland elections we establish resistance or vulnerability results in every previously studied control scenario for copelandalpha for each rational alpha 0 alpha 1 in particular we prove that copeland05 the system commonly referred to as copeland voting provides full resistance to constructive control among the systems with a polynomialtime winner problem this is the first natural election system proven to have full resistance to constructive control results on bribery and fixedparameter tractability of boundedcase control proven for copeland0 and copeland1 in fhhr07 are extended to copelandalpha for each rational alpha 0 alpha 1 we also give results in more flexible models such as microbribery and extended control
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711.476
VLTI/MIDI Observations of the Massive Protostellar Candidate NGC 3603 IRS 9A
We used MIDI, the mid-infrared interferometric instrument of the VLTI, to observe the massive protostellar candidate IRS 9A, located at a distance of about 7 kpc at the periphery of the NGC 3603 star cluster. Our ongoing analysis shows that MIDI almost fully resolves the object on all observed baselines, yet below 9 $\mu$m we detect a steep rise of the visibility. This feature is modelled as a combination of a compact hot component and a resolved warm envelope which lowers the correlated flux at longer wavelengths. The extended envelope can already be seen in both MIDI's acquisition images and in complementary data from aperture masking observations at the Gemini South telescope. Its shape is asymmetric, which could indicate a circumstellar disk inclined against the line of sight. The compact component is possibly related to the inner edge of this (accretion) disk. The uncorrelated mid-infrared spectrum appears featureless and could be caused by optically thick emission without a significant contribution from the disk atmosphere.
astro-ph
we used midi the midinfrared interferometric instrument of the vlti to observe the massive protostellar candidate irs 9a located at a distance of about 7 kpc at the periphery of the ngc 3603 star cluster our ongoing analysis shows that midi almost fully resolves the object on all observed baselines yet below 9 mum we detect a steep rise of the visibility this feature is modelled as a combination of a compact hot component and a resolved warm envelope which lowers the correlated flux at longer wavelengths the extended envelope can already be seen in both midis acquisition images and in complementary data from aperture masking observations at the gemini south telescope its shape is asymmetric which could indicate a circumstellar disk inclined against the line of sight the compact component is possibly related to the inner edge of this accretion disk the uncorrelated midinfrared spectrum appears featureless and could be caused by optically thick emission without a significant contribution from the disk atmosphere
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711.4761
Path-Integral Renormalization Group Treatments for Many-Electron Systems with Long-Range Repulsive Interactions
A practical algorithm for many-electron systems based on the path-integral renormalization group (PIRG) method is proposed in the real-space finite-difference (RSFD) approach. The PIRG method, developed for investigating strongly correlated electron systems, has been successfully applied to some models such as Hubbard models. However, to apply this method to more realistic systems of electrons with long-range Coulomb interactions within the RSFD formalism, the one-body Green's function, which requires large computational resources, is to be replaced with an alternative. For the same reason, an efficient algorithm for computing the Fock matrix is needed. The newly proposed algorithm is free of the one-body Green's function and enables us to compute the Fock matrix efficiently. Our result shows a significant reduction in CPU time and the possibility of using the present algorithm as a practical numerical tool.
cond-mat.str-el cond-mat.other
a practical algorithm for manyelectron systems based on the pathintegral renormalization group pirg method is proposed in the realspace finitedifference rsfd approach the pirg method developed for investigating strongly correlated electron systems has been successfully applied to some models such as hubbard models however to apply this method to more realistic systems of electrons with longrange coulomb interactions within the rsfd formalism the onebody greens function which requires large computational resources is to be replaced with an alternative for the same reason an efficient algorithm for computing the fock matrix is needed the newly proposed algorithm is free of the onebody greens function and enables us to compute the fock matrix efficiently our result shows a significant reduction in cpu time and the possibility of using the present algorithm as a practical numerical tool
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711.4762
Power series solution of the modified KdV equation
We prove local-wellposedness of the mKdV equation in $\mathcal{F}L^{s,p}$ spaces using the new method of M. Christ.
math.AP
we prove localwellposedness of the mkdv equation in mathcalflsp spaces using the new method of m christ
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711.4763
Calculation of the Two-body T-matrix in Configuration Space
A spectral integral method (IEM) for solving the two-body Schroedinger equation in configuration space is generalized to the calculation of the corresponding T-matrix. It is found that the desirable features of the IEM, such as the economy of mesh-points for a given required accuracy, are carried over also to the solution of the T-matrix. However the algorithm is considerably more complex, because the T-matrix is a function of two variables r and r', rather than only one variable r, and has a slope discontinuity at r=r'. For a simple exponential potential an accuracy of 7 significant figures is achieved, with the number N of Chebyshev support points in each partition equal to 17. For a potential with a large repulsive core, such as the potential between two He atoms, the accuracy decreases to 4 significant figures, but is restored to 7 if N is increased to 65.
physics.comp-ph physics.atom-ph
a spectral integral method iem for solving the twobody schroedinger equation in configuration space is generalized to the calculation of the corresponding tmatrix it is found that the desirable features of the iem such as the economy of meshpoints for a given required accuracy are carried over also to the solution of the tmatrix however the algorithm is considerably more complex because the tmatrix is a function of two variables r and r rather than only one variable r and has a slope discontinuity at rr for a simple exponential potential an accuracy of 7 significant figures is achieved with the number n of chebyshev support points in each partition equal to 17 for a potential with a large repulsive core such as the potential between two he atoms the accuracy decreases to 4 significant figures but is restored to 7 if n is increased to 65
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711.4764
Description of the spin structure function g_1 at arbitrary $x$ and arbitrary Q^2
The explicit expressions describing the structure function g_1 at arbitrary x and Q^2 are obtained. In the first place, they combine the well-known DGLAP expressions for g_1 with the total resummation of leading logarithms of x, which makes possible to cover the kinematic region of arbitrary x and large Q^2. In order to cover the small-Q^2 region the shift Q^2 -> Q^2 + mu^2 in the large-Q^2 expressions for g_1 is suggested and values of mu are estimated. The expressions obtained do not require singular factors x^{-a} in the fits for initial parton densities.
hep-ph
the explicit expressions describing the structure function g_1 at arbitrary x and q2 are obtained in the first place they combine the wellknown dglap expressions for g_1 with the total resummation of leading logarithms of x which makes possible to cover the kinematic region of arbitrary x and large q2 in order to cover the smallq2 region the shift q2 q2 mu2 in the largeq2 expressions for g_1 is suggested and values of mu are estimated the expressions obtained do not require singular factors xa in the fits for initial parton densities
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711.4765
The underscreened Kondo lattice model applied to heavy fermion uranium compounds
We present theoretical results for the underscreened Kondo lattice model with localized S=1 spins coupled to a conduction band through a Kondo coupling, $J_K$, and interacting among them ferromagnetically. We use a fermionic representation for the spin operators and expand the Hamiltonian in terms of bosonic fields. For large values of $J_K$, we obtain a ferromagnetically ordered solution and a Kondo regime with a Kondo temperature, $T_K$, larger than the Curie temperature, $T_C$. This finding suggests a scenario for a coexistence of Kondo effect and ferromagnetic order. In some uranium compounds, like $UTe$ or $UCu_{0.9}Sb_{2}$, this kind of coexistence has been experimentally observed: they order ferromagnetically with a Curie temperature of order $T_C \sim 100K$ and exhibit a Kondo behavior for $T > T_C$. The proposed underscreened Kondo lattice model accounts well for the coexistence between magnetic order and Kondo behavior and yields to a new ``ferromagnetic Doniach diagram''.
cond-mat.str-el cond-mat.mtrl-sci
we present theoretical results for the underscreened kondo lattice model with localized s1 spins coupled to a conduction band through a kondo coupling j_k and interacting among them ferromagnetically we use a fermionic representation for the spin operators and expand the hamiltonian in terms of bosonic fields for large values of j_k we obtain a ferromagnetically ordered solution and a kondo regime with a kondo temperature t_k larger than the curie temperature t_c this finding suggests a scenario for a coexistence of kondo effect and ferromagnetic order in some uranium compounds like ute or ucu_09sb_2 this kind of coexistence has been experimentally observed they order ferromagnetically with a curie temperature of order t_c sim 100k and exhibit a kondo behavior for t t_c the proposed underscreened kondo lattice model accounts well for the coexistence between magnetic order and kondo behavior and yields to a new ferromagnetic doniach diagram
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711.4766
On a space related to the affine building of type E7
A locally truncated geometry with diagram of type affine E7 is studied. One considers a parapolar space, locally of type A_{7,4}, which is subject to an extra axiom. A covering of this space is constructed; it is proved that this covering space is a rank 6, residually connected, locally truncated diagram geometry which is a homomorphic image of a truncated building of affine type E7. Consequently, the initial parapolar space is also a homomorphic image of a truncated building.
math.GR
a locally truncated geometry with diagram of type affine e7 is studied one considers a parapolar space locally of type a_74 which is subject to an extra axiom a covering of this space is constructed it is proved that this covering space is a rank 6 residually connected locally truncated diagram geometry which is a homomorphic image of a truncated building of affine type e7 consequently the initial parapolar space is also a homomorphic image of a truncated building
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711.4767
Observation of negative-frequency waves in a water tank: A classical analogue to the Hawking effect?
The conversion of positive-frequency waves into negative-frequency waves at the event horizon is the mechanism at the heart of the Hawking radiation of black holes. In black-hole analogues, horizons are formed for waves propagating in a medium against the current when and where the flow exceeds the wave velocity. We report on the first direct observation of negative-frequency waves converted from positive-frequency waves in a moving medium. The measured degree of mode conversion is significantly higher than expected from theory.
gr-qc
the conversion of positivefrequency waves into negativefrequency waves at the event horizon is the mechanism at the heart of the hawking radiation of black holes in blackhole analogues horizons are formed for waves propagating in a medium against the current when and where the flow exceeds the wave velocity we report on the first direct observation of negativefrequency waves converted from positivefrequency waves in a moving medium the measured degree of mode conversion is significantly higher than expected from theory
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711.4768
Tongue Liminary Threshold Identification to Electrotactile Stimulation
Many applications use electrostimulation of the human skin to provide tactile sensation. The effect of electrotactile stimulations were studied on a 6x6 matrix of tactile electrodes placed on the anterior part of the tongue. The liminary threshold with continuous or discontinuous waveform and patterns with 2 or 4 electrodes was investigated. The result suggest that for energy saving and to improve the yield, it would probably be better to use discontinuous stimulation with two electrode patterns.
physics.med-ph q-bio.NC
many applications use electrostimulation of the human skin to provide tactile sensation the effect of electrotactile stimulations were studied on a 6x6 matrix of tactile electrodes placed on the anterior part of the tongue the liminary threshold with continuous or discontinuous waveform and patterns with 2 or 4 electrodes was investigated the result suggest that for energy saving and to improve the yield it would probably be better to use discontinuous stimulation with two electrode patterns
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711.4769
D and Ds hadronic branching fractions at B factories
Recent measurements of hadronic branching fractions of D and Ds mesons, performed by the BaBar and Belle experiments at the asymmetric e+e- B factories colliders PEP II and KEKB, are reviewed.
hep-ex
recent measurements of hadronic branching fractions of d and ds mesons performed by the babar and belle experiments at the asymmetric ee b factories colliders pep ii and kekb are reviewed
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711.477
Exponential complexity and ontological theories of quantum mechanics
Ontological theories of quantum mechanics describe a single system by means of well-defined classical variables and attribute the quantum uncertainties to our ignorance about the underlying reality represented by these variables. We consider the general class of ontological theories describing a quantum system by a set of variables with Markovian (either deterministic or stochastic) evolution. We provide the first proof that the number of continuous variables can not be smaller than 2N-2, N being the Hilbert space dimension. Thus, any ontological Markovian theory of quantum mechanics requires a number of variables which grows exponentially with the physical size. This result is relevant also in the framework of quantum Monte Carlo methods.
quant-ph
ontological theories of quantum mechanics describe a single system by means of welldefined classical variables and attribute the quantum uncertainties to our ignorance about the underlying reality represented by these variables we consider the general class of ontological theories describing a quantum system by a set of variables with markovian either deterministic or stochastic evolution we provide the first proof that the number of continuous variables can not be smaller than 2n2 n being the hilbert space dimension thus any ontological markovian theory of quantum mechanics requires a number of variables which grows exponentially with the physical size this result is relevant also in the framework of quantum monte carlo methods
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711.4771
Sequestered uplifting and the pattern of soft supersymmetry breaking terms
We examine the pattern of soft supersymmetry breaking terms in moduli stabilization, where an uplifting potential is provided by spontaneously broken supersymmetry in a generic sequestered sector. From stationary conditions, we derive the relation between moduli F-term vacuum expectation values which does not depend on the details of sequestered uplifting. This moduli F-term relation is crucial for identifying the dominant source of soft terms of visible fields.
hep-th
we examine the pattern of soft supersymmetry breaking terms in moduli stabilization where an uplifting potential is provided by spontaneously broken supersymmetry in a generic sequestered sector from stationary conditions we derive the relation between moduli fterm vacuum expectation values which does not depend on the details of sequestered uplifting this moduli fterm relation is crucial for identifying the dominant source of soft terms of visible fields
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711.4772
Modeling an accretion disc stochastical variability
Hot spots residing on the surface of an accretion disc have been considered as a model of short-term variability of active galactic nuclei. In this paper we apply the theory of random point processes to model the observed signal from an ensemble of randomly generated spots. The influence of general relativistic effects near a black hole is taken into account and it is shown that typical features of power spectral density can be reproduced. Connection among spots is also discussed in terms of Hawkes' process, which produces more power at low frequencies. We derive a semi-analytical way to approximate the resulting power-spectral density.
astro-ph
hot spots residing on the surface of an accretion disc have been considered as a model of shortterm variability of active galactic nuclei in this paper we apply the theory of random point processes to model the observed signal from an ensemble of randomly generated spots the influence of general relativistic effects near a black hole is taken into account and it is shown that typical features of power spectral density can be reproduced connection among spots is also discussed in terms of hawkes process which produces more power at low frequencies we derive a semianalytical way to approximate the resulting powerspectral density
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711.4773
The polyhedral nature of LINERs: An XMM-Newton view of LINERs in radio galaxies
Aims: We investigate the origin of X-rays and the nature of accretion flow in 4 LINERs hosted by radio galaxies, namely NGC1692, PKS0625-35, 3C88, 3C444, recently observed with XMM. Methods: We combine the results from the time-averaged spectral analysis with model-independent information from X-ray temporal and spectral variability analyses, and with additional broadband information (UV and radio). Results: The values of the Eddington ratios of our sample span 2 orders of magnitude. The 4 AGN are adequately fitted by the same continuum model that comprises at least one thermal component and a partially absorbed power law, whose relative contribution and photon index vary substantially from source to source. NGC1692 and PKS0625-35 have fairly steep power-law components, perhaps indicative of synchrotron emission from a jet. Conversely, the flat photon index derived for 3C88 may be indicative of a heavily absorbed object. Finally, the time-averaged spectral properties of 3C444 (Gamma~1.9 and an apparent line-like excess around 6.7 keV) are more in line with Seyfert galaxies. The temporal analysis reveals that PKS0625-35 and 3C88 are significantly variable in the soft energy band. PKS0625-35 also shows suggestive evidence of spectral variability on timescales of months. The main findings from the broadband analysis can be summarized as follows: 1) 3C444, PKS0625-35, and NGC1692 have alpha_OX values consistent with the well known alpha_OX -l_UV correlation. 2) No positive correlation is found between L_X and the inclination angle, suggesting that the X-ray emission is not beamed. 3) The values of the radio-loudness are inversely proportional to the Eddington ratio and locate our objects in between the ``radio-loud'' and ``radio-quiet'' branches in the R- l_UV plane.
astro-ph
aims we investigate the origin of xrays and the nature of accretion flow in 4 liners hosted by radio galaxies namely ngc1692 pks062535 3c88 3c444 recently observed with xmm methods we combine the results from the timeaveraged spectral analysis with modelindependent information from xray temporal and spectral variability analyses and with additional broadband information uv and radio results the values of the eddington ratios of our sample span 2 orders of magnitude the 4 agn are adequately fitted by the same continuum model that comprises at least one thermal component and a partially absorbed power law whose relative contribution and photon index vary substantially from source to source ngc1692 and pks062535 have fairly steep powerlaw components perhaps indicative of synchrotron emission from a jet conversely the flat photon index derived for 3c88 may be indicative of a heavily absorbed object finally the timeaveraged spectral properties of 3c444 gamma19 and an apparent linelike excess around 67 kev are more in line with seyfert galaxies the temporal analysis reveals that pks062535 and 3c88 are significantly variable in the soft energy band pks062535 also shows suggestive evidence of spectral variability on timescales of months the main findings from the broadband analysis can be summarized as follows 1 3c444 pks062535 and ngc1692 have alpha_ox values consistent with the well known alpha_ox l_uv correlation 2 no positive correlation is found between l_x and the inclination angle suggesting that the xray emission is not beamed 3 the values of the radioloudness are inversely proportional to the eddington ratio and locate our objects in between the radioloud and radioquiet branches in the r l_uv plane
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711.4774
McKay correspondence for Landau-Ginzburg models
In this paper we prove an analogue of the McKay correspondence for Landau-Ginzburg models. Our proof is based on the ideas introduced by T. Bridgeland, A. King and M. Reid, which reformulate and generalize the McKay correspondence in the language of derived categories, along with the techniques introduced by J.-C. Chen.
math.AG hep-th math-ph math.MP
in this paper we prove an analogue of the mckay correspondence for landauginzburg models our proof is based on the ideas introduced by t bridgeland a king and m reid which reformulate and generalize the mckay correspondence in the language of derived categories along with the techniques introduced by jc chen
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711.4775
The window at the edge of chaos in a simple model of gene interaction networks
As a model for gene and protein interactions we study a set for molecular catalytic reactions. The model is based on experimentally motivated interaction network topologies, and is designed to capture some key statistics of gene expression statistics. We impose a non-linearity to the system by a boundary condition which guarantees non-negative concentrations of chemical concentrations and study the system stability quantified by maximum Lyapunov exponents. We find that the non-negativity constraint leads to a drastic inflation of those regions in parameter space where the Lyapunov exponent exactly vanishes. We explain the finding as a self-organized critical phenomenon. The robustness of this finding with respect to different network topologies and the role of intrinsic molecular- and external noise is discussed. We argue that systems with inflated 'edges of chaos' could be much more easily favored by natural selection than systems where the Lyapunov exponent vanishes only on a parameter set of measure zero.
q-bio.MN
as a model for gene and protein interactions we study a set for molecular catalytic reactions the model is based on experimentally motivated interaction network topologies and is designed to capture some key statistics of gene expression statistics we impose a nonlinearity to the system by a boundary condition which guarantees nonnegative concentrations of chemical concentrations and study the system stability quantified by maximum lyapunov exponents we find that the nonnegativity constraint leads to a drastic inflation of those regions in parameter space where the lyapunov exponent exactly vanishes we explain the finding as a selforganized critical phenomenon the robustness of this finding with respect to different network topologies and the role of intrinsic molecular and external noise is discussed we argue that systems with inflated edges of chaos could be much more easily favored by natural selection than systems where the lyapunov exponent vanishes only on a parameter set of measure zero
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711.4776
Magnetoelectric Effects on Composite Nano Granular $Fe/TiO_{2-\delta}$ Films
Employing a new experimental technique to measure magnetoelectric response functions, we have measured the magnetoelectric effect in composite films of nano granular metallic iron in anatase titanium dioxide at temperatures below 50 K. A magnetoelectric resistance is defined as the ratio of a transverse voltage to bias current as a function of the magnetic field. In contrast to the anomalous Hall resistance measured above 50 K, the magnetoelectic resistance below 50 K is significantly larger and exhibits an even symmetry with respect to magnetic field reversal $H\to -H$. The measurement technique required attached electrodes in the plane of the film composite in order to measure voltage as a function of bias current and external magnetic field. To our knowledge, the composite films are unique in terms of showing magnetoelectric effects at low temperatures, $<$ 50 K, and anomalous Hall effects at high temperatures, $>$ 50 K.
cond-mat.mtrl-sci
employing a new experimental technique to measure magnetoelectric response functions we have measured the magnetoelectric effect in composite films of nano granular metallic iron in anatase titanium dioxide at temperatures below 50 k a magnetoelectric resistance is defined as the ratio of a transverse voltage to bias current as a function of the magnetic field in contrast to the anomalous hall resistance measured above 50 k the magnetoelectic resistance below 50 k is significantly larger and exhibits an even symmetry with respect to magnetic field reversal hto h the measurement technique required attached electrodes in the plane of the film composite in order to measure voltage as a function of bias current and external magnetic field to our knowledge the composite films are unique in terms of showing magnetoelectric effects at low temperatures 50 k and anomalous hall effects at high temperatures 50 k
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711.4777
A Temperley-Lieb category for 2-manifolds
Guided by consideration of problems in 2 and 3 dimensional lattice model computation, we are led to define a number of new categories, and functors between these categories and the partition category, culminating in the introduction of two categories generalising the Temperley-Lieb category. We show how to compute practically in these categories, by giving a combinatorial realisation of their (topological) construction.
math-ph math.MP
guided by consideration of problems in 2 and 3 dimensional lattice model computation we are led to define a number of new categories and functors between these categories and the partition category culminating in the introduction of two categories generalising the temperleylieb category we show how to compute practically in these categories by giving a combinatorial realisation of their topological construction
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711.4778
The WA3 data and the two $K_1(1270)$ resonances
Recent studies based on unitary chiral perturbation theory (U$\chi$PT) found that the low-lying axial vector mesons can be dynamically generated due to the interaction of the pseudoscalar octet of the pion and the vector nonet of the rho. In particular, two poles in the second Riemann sheet have been associated to the nominal $K_1(1270)$ resonance. In this talk, we present a recent analysis of the WA3 data on $K^-p\to K^-\pi^+\pi^- p$ at 63 GeV using the U$\chi$PT amplitudes, and show that it is in favor of the existence of two $K_1(1270)$'s [Phys. Rev. D 75, 014017 (2007)].
hep-ph
recent studies based on unitary chiral perturbation theory uchipt found that the lowlying axial vector mesons can be dynamically generated due to the interaction of the pseudoscalar octet of the pion and the vector nonet of the rho in particular two poles in the second riemann sheet have been associated to the nominal k_11270 resonance in this talk we present a recent analysis of the wa3 data on kpto kpipi p at 63 gev using the uchipt amplitudes and show that it is in favor of the existence of two k_11270s phys rev d 75 014017 2007
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711.4779
Dark Electric Matter Objects: History of Discovery, Modes of Interaction with Matter, Some Inferences and Prospects
Experiments with thin ZnS(Ag) scintillators provide evidence with C.L. > 99.99% for the existence of DArk Electric Matter Objects - daemons (presumably negatively charged Planckian particles with M ~ 10^-5 g) captured from the Galactic disk into near-Earth, almost circular heliocentric orbits. Their flux at V ~ 10-15 km/s was found to be as high as f > 10^-7 cm^-2 s^-1 and vary with P = 0.5 y, with maxima in March and September. A daemon flux f ~ 10^-7 - 10^-6 cm^-2 s^-1 is capable of accounting for the Troitsk anomaly in the tritium beta-spectrum and suggests its more pronounced manifestation in future KATRIN experiment. In view of the channeling effect on iodine recoil nuclei in the NaI(Tl) crystal, the DAMA/NaI experiment is also apparently detecting a flux of daemons, f ~ 6x10^-7 cm^-2 s^-1, but in this case of those falling with V = 30-50 km/s from strongly elongated, Earth-crossing heliocentric orbits oriented in the antapex direction, as a result of which the number of events detected in the 2-6-keV interval varies with P = 1 y.
astro-ph
experiments with thin znsag scintillators provide evidence with cl 9999 for the existence of dark electric matter objects daemons presumably negatively charged planckian particles with m 105 g captured from the galactic disk into nearearth almost circular heliocentric orbits their flux at v 1015 kms was found to be as high as f 107 cm2 s1 and vary with p 05 y with maxima in march and september a daemon flux f 107 106 cm2 s1 is capable of accounting for the troitsk anomaly in the tritium betaspectrum and suggests its more pronounced manifestation in future katrin experiment in view of the channeling effect on iodine recoil nuclei in the naitl crystal the damanai experiment is also apparently detecting a flux of daemons f 6x107 cm2 s1 but in this case of those falling with v 3050 kms from strongly elongated earthcrossing heliocentric orbits oriented in the antapex direction as a result of which the number of events detected in the 26kev interval varies with p 1 y
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711.478
Mosaic length and finite interaction-range effects in a one dimensional random energy model
In this paper we study finite interaction range corrections to the mosaic picture of the glass transition as emerges from the study of the Kac limit of large interaction range for disordered models. To this aim we consider point to set correlation functions, or overlaps, in a one dimensional random energy model as a function of the range of interaction. In the Kac limit, the mosaic length defines a sharp first order transition separating a high overlap phase from a low overlap one. Correspondingly we find that overlap curves as a function of the window size and different finite interaction ranges cross roughly at the mosaic lenght. Nonetheless we find very slow convergence to the Kac limit and we discuss why this could be a problem for measuring the mosaic lenght in realistic models.
cond-mat.dis-nn cond-mat.stat-mech
in this paper we study finite interaction range corrections to the mosaic picture of the glass transition as emerges from the study of the kac limit of large interaction range for disordered models to this aim we consider point to set correlation functions or overlaps in a one dimensional random energy model as a function of the range of interaction in the kac limit the mosaic length defines a sharp first order transition separating a high overlap phase from a low overlap one correspondingly we find that overlap curves as a function of the window size and different finite interaction ranges cross roughly at the mosaic lenght nonetheless we find very slow convergence to the kac limit and we discuss why this could be a problem for measuring the mosaic lenght in realistic models
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711.4781
Projective relations for m-th root metric spaces
For Finsler spaces (M,F) endowed with m-th root metrics, we provide necessary and sufficient conditions in which they are projectively flat, or projectively related to Berwald/Riemann spaces. We also give a specific characterization for m-th root metrics spaces of Landsberg and of Berwald type.
math.DG
for finsler spaces mf endowed with mth root metrics we provide necessary and sufficient conditions in which they are projectively flat or projectively related to berwaldriemann spaces we also give a specific characterization for mth root metrics spaces of landsberg and of berwald type
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711.4782
The Peculiar Type Ib Supernova 2006jc: A WCO Wolf-Rayet Star Explosion
We present a theoretical model for Type Ib supernova (SN) 2006jc. We calculate the evolution of the progenitor star, hydrodynamics and nucleosynthesis of the SN explosion, and the SN bolometric light curve (LC). The synthetic bolometric LC is compared with the observed bolometric LC constructed by integrating the UV, optical, near-infrared (NIR), and mid-infrared (MIR) fluxes. The progenitor is assumed to be as massive as $40M_\odot$ on the zero-age main-sequence. The star undergoes extensive mass loss to reduce its mass down to as small as $6.9M_\odot$, thus becoming a WCO Wolf-Rayet star. The WCO star model has a thick carbon-rich layer, in which amorphous carbon grains can be formed. This could explain the NIR brightening and the dust feature seen in the MIR spectrum. We suggest that the progenitor of SN 2006jc is a WCO Wolf-Rayet star having undergone strong mass loss and such massive stars are the important sites of dust formation. We derive the parameters of the explosion model in order to reproduce the bolometric LC of SN 2006jc by the radioactive decays: the ejecta mass $4.9M_\odot$, hypernova-like explosion energy $10^{52}$ ergs, and ejected $^{56}$Ni mass $0.22M_\odot$. We also calculate the circumstellar interaction and find that a CSM with a flat density structure is required to reproduce the X-ray LC of SN 2006jc. This suggests a drastic change of the mass-loss rate and/or the wind velocity that is consistent with the past luminous blue variable (LBV)-like event.
astro-ph
we present a theoretical model for type ib supernova sn 2006jc we calculate the evolution of the progenitor star hydrodynamics and nucleosynthesis of the sn explosion and the sn bolometric light curve lc the synthetic bolometric lc is compared with the observed bolometric lc constructed by integrating the uv optical nearinfrared nir and midinfrared mir fluxes the progenitor is assumed to be as massive as 40m_odot on the zeroage mainsequence the star undergoes extensive mass loss to reduce its mass down to as small as 69m_odot thus becoming a wco wolfrayet star the wco star model has a thick carbonrich layer in which amorphous carbon grains can be formed this could explain the nir brightening and the dust feature seen in the mir spectrum we suggest that the progenitor of sn 2006jc is a wco wolfrayet star having undergone strong mass loss and such massive stars are the important sites of dust formation we derive the parameters of the explosion model in order to reproduce the bolometric lc of sn 2006jc by the radioactive decays the ejecta mass 49m_odot hypernovalike explosion energy 1052 ergs and ejected 56ni mass 022m_odot we also calculate the circumstellar interaction and find that a csm with a flat density structure is required to reproduce the xray lc of sn 2006jc this suggests a drastic change of the massloss rate andor the wind velocity that is consistent with the past luminous blue variable lbvlike event
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711.4783
Superintegrable Systems with a Third Order Integrals of Motion
Two-dimensional superintegrable systems with one third order and one lower order integral of motion are reviewed. The fact that Hamiltonian systems with higher order integrals of motion are not the same in classical and quantum mechanics is stressed. New results on the use of classical and quantum third order integrals are presented in Section 5 and 6.
math-ph math.MP nlin.SI
twodimensional superintegrable systems with one third order and one lower order integral of motion are reviewed the fact that hamiltonian systems with higher order integrals of motion are not the same in classical and quantum mechanics is stressed new results on the use of classical and quantum third order integrals are presented in section 5 and 6
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711.4784
Transport reversal in a delayed feedback ratchet
Feedback flashing ratchets are thermal rectifiers that use information on the state of the system to operate the switching on and off of a periodic potential. They can induce directed transport even with symmetric potentials thanks to the asymmetry of the feedback protocol. We investigate here the dynamics of a feedback flashing ratchet when the asymmetry of the ratchet potential and of the feedback protocol favor transport in opposite directions. The introduction of a time delay in the control strategy allows one to nontrivially tune the relative relevance of the competing asymmetries leading to an interesting dynamics. We show that the competition between the asymmetries leads to a current reversal for large delays. For small ensembles of particles current reversal appears as the consequence of the emergence of an open-loop like dynamical regime, while for large ensembles of particles it can be understood as a consequence of the stabilization of quasiperiodic solutions. We also comment on the experimental feasibility of these feedback ratchets and their potential applications.
cond-mat.stat-mech
feedback flashing ratchets are thermal rectifiers that use information on the state of the system to operate the switching on and off of a periodic potential they can induce directed transport even with symmetric potentials thanks to the asymmetry of the feedback protocol we investigate here the dynamics of a feedback flashing ratchet when the asymmetry of the ratchet potential and of the feedback protocol favor transport in opposite directions the introduction of a time delay in the control strategy allows one to nontrivially tune the relative relevance of the competing asymmetries leading to an interesting dynamics we show that the competition between the asymmetries leads to a current reversal for large delays for small ensembles of particles current reversal appears as the consequence of the emergence of an openloop like dynamical regime while for large ensembles of particles it can be understood as a consequence of the stabilization of quasiperiodic solutions we also comment on the experimental feasibility of these feedback ratchets and their potential applications
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711.4785
Deuteron form factors in chiral effective theory: regulator-independent results and the role of two-pion exchange
We evaluate the deuteron charge, quadrupole, and magnetic form factors using wave functions obtained from chiral effective theory ($\chi$ET) when the potential includes one-pion exchange, chiral two-pion exchange, and genuine contact interactions. We study the manner in which the results for form factors behave as the regulator is removed from the $\chi$ET calculation, and compare co-ordinate- and momentum-space approaches. We show that, for both the LO and NNLO chiral potential, results obtained by imposing boundary conditions in co-ordinate space at $r=0$ are equivalent to the $\Lambda \to \infty$ limit of momentum-space calculations. The regulator-independent predictions for deuteron form factors that result from taking the $\Lambda \to \infty$ limit using the LO $\chi$ET potential are in reasonable agreement with data up to momentum transfers of order 600 MeV, provided that phenomenological information for nucleon structure is employed. In this range the use of the NNLO $\chi$ET potential results in only small changes to the LO predictions, and it improves the description of the zero of the charge form factor.
nucl-th
we evaluate the deuteron charge quadrupole and magnetic form factors using wave functions obtained from chiral effective theory chiet when the potential includes onepion exchange chiral twopion exchange and genuine contact interactions we study the manner in which the results for form factors behave as the regulator is removed from the chiet calculation and compare coordinate and momentumspace approaches we show that for both the lo and nnlo chiral potential results obtained by imposing boundary conditions in coordinate space at r0 are equivalent to the lambda to infty limit of momentumspace calculations the regulatorindependent predictions for deuteron form factors that result from taking the lambda to infty limit using the lo chiet potential are in reasonable agreement with data up to momentum transfers of order 600 mev provided that phenomenological information for nucleon structure is employed in this range the use of the nnlo chiet potential results in only small changes to the lo predictions and it improves the description of the zero of the charge form factor
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711.4786
Discovery of exceptional points in the Bose-Einstein condensation of gases with attractive 1/r-interaction
The extended Gross-Pitaevskii equation for the Bose-Einstein condensation of gases with attractive 1/r-interaction has a second solution which is born together with the ground state in a tangent bifurcation. At the bifurcation point both states coalesce, i.e., the energies and the wave functions are identical. We investigate the bifurcation point in the context of exceptional points, a phenomenon known for linear non-Hermitian Hamiltonians. We point out that the mean field energy, the chemical potential, and the wave functions show the same behavior as an exceptional point in a linear, non-symmetric system. The analysis of the analytically continued Gross-Pitaevskii equation reveals complex waves at negative scattering lengths below the tangent bifurcation. These solutions are interpreted as a decay of the condensate caused by an absorbing potential.
nlin.CD quant-ph
the extended grosspitaevskii equation for the boseeinstein condensation of gases with attractive 1rinteraction has a second solution which is born together with the ground state in a tangent bifurcation at the bifurcation point both states coalesce ie the energies and the wave functions are identical we investigate the bifurcation point in the context of exceptional points a phenomenon known for linear nonhermitian hamiltonians we point out that the mean field energy the chemical potential and the wave functions show the same behavior as an exceptional point in a linear nonsymmetric system the analysis of the analytically continued grosspitaevskii equation reveals complex waves at negative scattering lengths below the tangent bifurcation these solutions are interpreted as a decay of the condensate caused by an absorbing potential
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711.4787
Torsion and Supersymmetry Breaking
We identify the auxiliary fields in the hypermultiplets of type IIB string theory compactified on a Calabi-Yau manifold, using a combination of worldsheet and supergravity techniques. The SUSY-breaking squark and gaugino masses in type IIB models depend on these auxiliary fields, which parametrize deformations away from a pure Calabi-Yau compactification to one with NS-NS 3-form flux and SU(3) x SU(3) structure. Worldsheet arguments show that such compactifications are generically globally nongeometric. Our results, combined with earlier results for type IIA compactifications, imply that these deformations are the mirrors of NS-NS 3-form flux, in accord with work from the supergravity point of view. Using the worldsheet current algebra, we explain why mirror symmetry may continue to hold in the presence of fluxes breaking the symmetries (e.g., (2,2) SUSY) on which mirror symmetry is typically taken to depend. Finally, we give evidence that nonperturbative worldsheet effects (such as worldsheet instantons) provide important corrections to the supergravity picture in the presence of auxiliary fields for Kahler moduli.
hep-th
we identify the auxiliary fields in the hypermultiplets of type iib string theory compactified on a calabiyau manifold using a combination of worldsheet and supergravity techniques the susybreaking squark and gaugino masses in type iib models depend on these auxiliary fields which parametrize deformations away from a pure calabiyau compactification to one with nsns 3form flux and su3 x su3 structure worldsheet arguments show that such compactifications are generically globally nongeometric our results combined with earlier results for type iia compactifications imply that these deformations are the mirrors of nsns 3form flux in accord with work from the supergravity point of view using the worldsheet current algebra we explain why mirror symmetry may continue to hold in the presence of fluxes breaking the symmetries eg 22 susy on which mirror symmetry is typically taken to depend finally we give evidence that nonperturbative worldsheet effects such as worldsheet instantons provide important corrections to the supergravity picture in the presence of auxiliary fields for kahler moduli
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711.4788
Close-packed dimers on the kagome lattice: Finite lattices and the Grassmannian approach
In a recent paper [ F. Wang and F. Y. Wu, Phys. Rev. E 75 (2007) 040105(R) ] we reported exact results on the enumeration of close-packed dimers on an infinite kagome lattice. We computed the per-dimer free energy using both the Pfaffian approach and a vertex-model formulation, and found the result given by a simple expression. We also reported results on dimer-dimer correlations without giving details. In this paper we present details of the correlation function analysis. In addition, we extend the exact enumeration to finite lattices under two different boundary conditions and with asymmetric dimer weights. For symmetric dimer weights the finite-lattice results are again simple, and we show that they can be understood using a spin variable mapping. We also describe the formulation of a Grassmannian functional integral approach and apply it to the kagome lattice.
cond-mat.stat-mech math.CO
in a recent paper f wang and f y wu phys rev e 75 2007 040105r we reported exact results on the enumeration of closepacked dimers on an infinite kagome lattice we computed the perdimer free energy using both the pfaffian approach and a vertexmodel formulation and found the result given by a simple expression we also reported results on dimerdimer correlations without giving details in this paper we present details of the correlation function analysis in addition we extend the exact enumeration to finite lattices under two different boundary conditions and with asymmetric dimer weights for symmetric dimer weights the finitelattice results are again simple and we show that they can be understood using a spin variable mapping we also describe the formulation of a grassmannian functional integral approach and apply it to the kagome lattice
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711.4789
Lowest order QED radiative corrections to five-fold differential cross section of hadron leptoproduction
The contribution of exclusive radiative tail to the cross section of semi-inclusive hadron leptoproduction has been calculated exactly for the first time. Although the experience of inclusive data analyses suggests us that the contribution of radiative tail from the elastic peak is of particular importance, similar effects in the semi-inclusive process were only recently estimated in the peaking approximation. The explicit expressions for the lepton part of the lowest order QED contribution of exclusive radiative tail to the five-fold differential cross section are obtained and discussed. Numerical estimates, provided within Jefferson Lab kinematic conditions, demonstrate rather large effects of the exclusive radiative tail in the region at semi-inclusive threshold and for high energy of detected hadron.
hep-ph
the contribution of exclusive radiative tail to the cross section of semiinclusive hadron leptoproduction has been calculated exactly for the first time although the experience of inclusive data analyses suggests us that the contribution of radiative tail from the elastic peak is of particular importance similar effects in the semiinclusive process were only recently estimated in the peaking approximation the explicit expressions for the lepton part of the lowest order qed contribution of exclusive radiative tail to the fivefold differential cross section are obtained and discussed numerical estimates provided within jefferson lab kinematic conditions demonstrate rather large effects of the exclusive radiative tail in the region at semiinclusive threshold and for high energy of detected hadron
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711.479
Millihertz Oscillation Frequency Drift Predicts the Occurrence of Type I X-ray Bursts
Millihertz quasi-periodic oscillations reported in three neutron-star low mass X-ray binaries have been suggested to be a mode of marginally stable nuclear burning on the neutron star surface. In this Letter, we show that close to the transition between the island and the banana state, 4U~1636--53 shows mHz QPOs whose frequency systematically decreases with time until the oscillations disappear and a Type I X-ray burst occurs. There is a strong correlation between the QPO frequency $\nu$ and the occurrence of X-ray bursts: when $\nu\gtrsim9$ mHz no bursts occur, while $\nu\lesssim9$ mHz does allow the occurrence of bursts. The mHz QPO frequency constitutes the first identified observable that can be used to predict the occurrence of X-ray bursts. If a systematic frequency drift occurs, then a burst happens within a few kilo-seconds after $\nu$ drops below 9 mHz. This observational result confirms that the mHz QPO phenomenon is intimately related with the processes that lead to a thermonuclear burst.
astro-ph
millihertz quasiperiodic oscillations reported in three neutronstar low mass xray binaries have been suggested to be a mode of marginally stable nuclear burning on the neutron star surface in this letter we show that close to the transition between the island and the banana state 4u163653 shows mhz qpos whose frequency systematically decreases with time until the oscillations disappear and a type i xray burst occurs there is a strong correlation between the qpo frequency nu and the occurrence of xray bursts when nugtrsim9 mhz no bursts occur while nulesssim9 mhz does allow the occurrence of bursts the mhz qpo frequency constitutes the first identified observable that can be used to predict the occurrence of xray bursts if a systematic frequency drift occurs then a burst happens within a few kiloseconds after nu drops below 9 mhz this observational result confirms that the mhz qpo phenomenon is intimately related with the processes that lead to a thermonuclear burst
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711.4791
Enhanced high-energy neutrino emission from choked gamma-ray bursts due to meson and muon acceleration
It has been suggested that a potentially large fraction of supernovae could be accompanied by relativistic outflows that stall below the stellar surface. In this letter we point out that internal shocks that are believed to accelerate protons to very high energies in these flows will also accelerate secondary mesons and muons. As a result the neutrino spectrum from meson and muon decay is expected to be much harder compared to previous estimates, extending as a single power law up to ~10^3 TeV. This greatly improves the detection prospects.
astro-ph hep-ph
it has been suggested that a potentially large fraction of supernovae could be accompanied by relativistic outflows that stall below the stellar surface in this letter we point out that internal shocks that are believed to accelerate protons to very high energies in these flows will also accelerate secondary mesons and muons as a result the neutrino spectrum from meson and muon decay is expected to be much harder compared to previous estimates extending as a single power law up to 103 tev this greatly improves the detection prospects
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711.4792
On the Capacity of a Class of MIMO Cognitive Radios
Cognitive radios have been studied recently as a means to utilize spectrum in a more efficient manner. This paper focuses on the fundamental limits of operation of a MIMO cognitive radio network with a single licensed user and a single cognitive user. The channel setting is equivalent to an interference channel with degraded message sets (with the cognitive user having access to the licensed user's message). An achievable region and an outer bound is derived for such a network setting. It is shown that under certain conditions, the achievable region is optimal for a portion of the capacity region that includes sum capacity.
cs.IT math.IT
cognitive radios have been studied recently as a means to utilize spectrum in a more efficient manner this paper focuses on the fundamental limits of operation of a mimo cognitive radio network with a single licensed user and a single cognitive user the channel setting is equivalent to an interference channel with degraded message sets with the cognitive user having access to the licensed users message an achievable region and an outer bound is derived for such a network setting it is shown that under certain conditions the achievable region is optimal for a portion of the capacity region that includes sum capacity
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711.4793
Open Cavity Solutions to the rf in Magnetic Field Problem
It has been observed \cite{break} that breakdown in an 805 MHz pill-box cavi ty occurs at much lower gradients as an external axial magnetic field is inc reased. This effect was not observed with on open iris cavity. It is propose d that this effect depends on the relative angles of the magnetic and maximu m electric fields: parallel in the pill-box case; at an angle in the open ir is case. If so, using an open iris structure with solenoid coils in the iris es should perform even better. A lattice, using this principle, is presented, for use in 6D cooling for a Muon Collider. Experimental layouts to test th is principle are proposed.
physics.acc-ph
it has been observed citebreak that breakdown in an 805 mhz pillbox cavi ty occurs at much lower gradients as an external axial magnetic field is inc reased this effect was not observed with on open iris cavity it is propose d that this effect depends on the relative angles of the magnetic and maximu m electric fields parallel in the pillbox case at an angle in the open ir is case if so using an open iris structure with solenoid coils in the iris es should perform even better a lattice using this principle is presented for use in 6d cooling for a muon collider experimental layouts to test th is principle are proposed
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711.4794
Stochastic Acceleration in the Western Hotspot of Pictor A
Chandra's high resolution observations of radio galaxies require a revisit of the relevant electron acceleration processes. Although the diffusive shock particle acceleration model may explain spectra of spatially unresolved sources, it encounters difficulties in explaining the structure and spectral properties of recently discovered Chandra X-ray features in several low-power radio sources. We argue that these observations strongly suggest stochastic electron acceleration by magnetized turbulence, and show that the simplest stochastic particle acceleration model with energy independent acceleration and escape timescales can overcome most of these difficulties. We use the bright core of the western hotspot of Pictor A as an example to demonstrate the model characteristics, which may be tested with high energy observations.
astro-ph
chandras high resolution observations of radio galaxies require a revisit of the relevant electron acceleration processes although the diffusive shock particle acceleration model may explain spectra of spatially unresolved sources it encounters difficulties in explaining the structure and spectral properties of recently discovered chandra xray features in several lowpower radio sources we argue that these observations strongly suggest stochastic electron acceleration by magnetized turbulence and show that the simplest stochastic particle acceleration model with energy independent acceleration and escape timescales can overcome most of these difficulties we use the bright core of the western hotspot of pictor a as an example to demonstrate the model characteristics which may be tested with high energy observations
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711.4795
Globular Clusters and Dwarf Spheroidal Galaxies
Traditionally globular clusters and dwarf spheroidal galaxies have been distinguished by using one or more of the following criteria: (1) mass, (2) luminosity, (3) size, (4) mass-to-light ratio and (5) spread in metallicity. However, a few recently discovered objects show some overlap between the domains in parameter space that are occupied by galaxies and clusters. In the present note it is shown that ellipticity can, in some cases, be used to help distinguish between globular clusters and dwarf spheroidal galaxies.
astro-ph
traditionally globular clusters and dwarf spheroidal galaxies have been distinguished by using one or more of the following criteria 1 mass 2 luminosity 3 size 4 masstolight ratio and 5 spread in metallicity however a few recently discovered objects show some overlap between the domains in parameter space that are occupied by galaxies and clusters in the present note it is shown that ellipticity can in some cases be used to help distinguish between globular clusters and dwarf spheroidal galaxies
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711.4796
Fiber-optical analogue of the event horizon
The physics at the event horizon resembles the behavior of waves in moving media. Horizons are formed where the local speed of the medium exceeds the wave velocity. We use ultrashort pulses in microstructured optical fibers to demonstrate the formation of an artificial event horizon in optics. We observed a classical optical effect, the blue-shifting of light at a white-hole horizon. We also show by theoretical calculations that such a system is capable of probing the quantum effects of horizons, in particular Hawking radiation.
gr-qc
the physics at the event horizon resembles the behavior of waves in moving media horizons are formed where the local speed of the medium exceeds the wave velocity we use ultrashort pulses in microstructured optical fibers to demonstrate the formation of an artificial event horizon in optics we observed a classical optical effect the blueshifting of light at a whitehole horizon we also show by theoretical calculations that such a system is capable of probing the quantum effects of horizons in particular hawking radiation
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711.4797
Fiber-optical analogue of the event horizon: Appendices
We explain the theory behind our fiber-optical analogue of the event horizon and present the experiment in detail.
gr-qc
we explain the theory behind our fiberoptical analogue of the event horizon and present the experiment in detail
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711.4798
Conformal Powers of the Laplacian via Stereographic Projection
A new derivation is given of Branson's factorization formula for the conformally invariant operator on the sphere whose principal part is the k-th power of the scalar Laplacian. The derivation deduces Branson's formula from knowledge of the corresponding conformally invariant operator on Euclidean space (the k-th power of the Euclidean Laplacian) via conjugation by the stereographic projection mapping.
math.DG
a new derivation is given of bransons factorization formula for the conformally invariant operator on the sphere whose principal part is the kth power of the scalar laplacian the derivation deduces bransons formula from knowledge of the corresponding conformally invariant operator on euclidean space the kth power of the euclidean laplacian via conjugation by the stereographic projection mapping
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711.4799
Entanglement dynamics of two independent qubits in environments with and without memory
A procedure to obtain the dynamics of $N$ independent qudits ($d$-level systems) each interacting with its own reservoir, for any arbitrary initial state, is presented. This is then applied to study the dynamics of the entanglement of two qubits, initially in an extended Werner-like mixed state with each of them in a zero temperature non-Markovian environment. The dependence of the entanglement dynamics on the purity and degree of entanglement of the initial states and on the amount of non-Markovianity is also given. This extends the previous work about non-Markovian effects on the two-qubit entanglement dynamics for initial Bell-like states [B. Bellomo \textit{et al.}, Phys. Rev. Lett. \textbf{99}, 160502 (2007)]. The effect of temperature on the two-qubit entanglement dynamics in a Markovian environment is finally obtained.
quant-ph
a procedure to obtain the dynamics of n independent qudits dlevel systems each interacting with its own reservoir for any arbitrary initial state is presented this is then applied to study the dynamics of the entanglement of two qubits initially in an extended wernerlike mixed state with each of them in a zero temperature nonmarkovian environment the dependence of the entanglement dynamics on the purity and degree of entanglement of the initial states and on the amount of nonmarkovianity is also given this extends the previous work about nonmarkovian effects on the twoqubit entanglement dynamics for initial belllike states b bellomo textitet al phys rev lett textbf99 160502 2007 the effect of temperature on the twoqubit entanglement dynamics in a markovian environment is finally obtained
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711.48
Dark Energy Models With Variable Equation Of State Parameter
Two variable $\Lambda$ models, viz. $\Lambda \sim (\dot a/a)^2$ and $\Lambda \sim \rho$ have been studied under the assumption that the equation of state parameter $\omega$ is a function of time. The selected $\Lambda$ models are found to be equivalent both in four and five dimensions. The possibility of signature flip of the deceleration parameter is also shown.
gr-qc
two variable lambda models viz lambda sim dot aa2 and lambda sim rho have been studied under the assumption that the equation of state parameter omega is a function of time the selected lambda models are found to be equivalent both in four and five dimensions the possibility of signature flip of the deceleration parameter is also shown
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711.4801
Properties of newly formed dust by SN2006jc based on near-to-mid infrared observation with AKARI
We present our latest results on near- to mid- infrared observation of SN2006jc at 200 days after the discovery using the Infrared Camera (IRC) on board $AKARI$. The near-infrared (2--5$\mu$m) spectrum of SN2006jc is obtained for the first time and is found to be well interpreted in terms of the thermal emission from amorphous carbon of 800$\pm 10$K with the mass of $6.9\pm 0.5 \times 10^{-5}M_{\odot}$ that was formed in the supernova ejecta. This dust mass newly formed in the ejecta of SN 2006jc is in a range similar to those obtained for other several dust forming core collapse supernovae based on recent observations (i.e., $10^{-3}$--$10^{-5}$$M_{\odot}$). Mid-infrared photometric data with {\it{AKARI}}/IRC MIR-S/S7, S9W, and S11 bands have shown excess emission over the thermal emission by hot amorphous carbon of 800K. This mid-infrared excess emission is likely to be accounted for by the emission from warm amorphous carbon dust of 320$\pm 10$K with the mass of 2.7$^{+0.7}_{-0.5} \times 10^{-3}M_{\odot}$ rather than by the band emission of astronomical silicate and/or silica grains. This warm amorphous carbon dust is expected to have been formed in the mass loss wind associated with the Wolf-Rayet stellar activity before the SN explosion. Our result suggests that a significant amount of dust is condensed in the mass loss wind prior to the SN explosion. A possible contribution of emission bands by precursory SiO molecules in 7.5--9.5$\mu$m is also suggested.
astro-ph
we present our latest results on near to mid infrared observation of sn2006jc at 200 days after the discovery using the infrared camera irc on board akari the nearinfrared 25mum spectrum of sn2006jc is obtained for the first time and is found to be well interpreted in terms of the thermal emission from amorphous carbon of 800pm 10k with the mass of 69pm 05 times 105m_odot that was formed in the supernova ejecta this dust mass newly formed in the ejecta of sn 2006jc is in a range similar to those obtained for other several dust forming core collapse supernovae based on recent observations ie 103105m_odot midinfrared photometric data with itakariirc mirss7 s9w and s11 bands have shown excess emission over the thermal emission by hot amorphous carbon of 800k this midinfrared excess emission is likely to be accounted for by the emission from warm amorphous carbon dust of 320pm 10k with the mass of 2707_05 times 103m_odot rather than by the band emission of astronomical silicate andor silica grains this warm amorphous carbon dust is expected to have been formed in the mass loss wind associated with the wolfrayet stellar activity before the sn explosion our result suggests that a significant amount of dust is condensed in the mass loss wind prior to the sn explosion a possible contribution of emission bands by precursory sio molecules in 7595mum is also suggested
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711.4802
On the physical parametrization and magnetic analogs of the Emparan-Teo dihole solution
The Emparan-Teo non-extremal black dihole solution is reparametrized using Komar quantities and the separation distance as arbitrary parameters. We show how the potential $A_3$ can be calculated for the magnetic analogs of this solution in the Einstein-Maxwell and Einstein-Maxwell-dilaton theories. We also demonstrate that, similar to the extreme case, the external magnetic field can remove the supporting strut in the non-extremal black dihole too.
gr-qc
the emparanteo nonextremal black dihole solution is reparametrized using komar quantities and the separation distance as arbitrary parameters we show how the potential a_3 can be calculated for the magnetic analogs of this solution in the einsteinmaxwell and einsteinmaxwelldilaton theories we also demonstrate that similar to the extreme case the external magnetic field can remove the supporting strut in the nonextremal black dihole too
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711.4803
Stellar Feedback in Dwarf Galaxy Formation
Dwarf galaxies pose significant challenges for cosmological models. In particular, current models predict a dark matter density that is divergent at the center, in sharp contrast with observations which indicate an approximately constant central density core. Energy feedback, from supernova explosions and stellar winds, has been proposed as a major factor shaping the evolution of dwarf galaxies. We present detailed cosmological simulations with sufficient resolution both to model the relevant physical processes and to directly assess the impact of stellar feedback on observable properties of dwarf galaxies. We show that feedback drives large-scale, bulk motion of the interstellar gas resulting in significant gravitational potential fluctuations and a consequent reduction in the central matter density, bringing the theoretical predictions in agreement with observations.
astro-ph
dwarf galaxies pose significant challenges for cosmological models in particular current models predict a dark matter density that is divergent at the center in sharp contrast with observations which indicate an approximately constant central density core energy feedback from supernova explosions and stellar winds has been proposed as a major factor shaping the evolution of dwarf galaxies we present detailed cosmological simulations with sufficient resolution both to model the relevant physical processes and to directly assess the impact of stellar feedback on observable properties of dwarf galaxies we show that feedback drives largescale bulk motion of the interstellar gas resulting in significant gravitational potential fluctuations and a consequent reduction in the central matter density bringing the theoretical predictions in agreement with observations
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711.4804
Flow of power-law fluids in self-affine fracture channels
The two-dimensional pressure driven flow of non-Newtonian power-law fluids in self-affine fracture channels at finite Reynolds number is calculated. The channels have constant mean aperture and two values $\zeta$=0.5 and 0.8 of the Hurst exponent are considered. The calculation is based on the lattice-Boltzmann method, using a novel method to obtain a power-law variation in viscosity, and the behavior of shear-thinning, Newtonian and shear-thickening liquids is compared. Local aspects of the flow fields, such as maximum velocity and pressure fluctuations, were studied, and the non-Newtonian fluids were compared to the (previously-studied) Newtonian case. The permeability results may be collapsed into a master curve of friction factor vs. Reynolds number using a scaling similar to that employed for porous media flow, and exhibits a transition from a linear regime to a more rapid variation at Re increases.
cond-mat.soft cond-mat.mtrl-sci
the twodimensional pressure driven flow of nonnewtonian powerlaw fluids in selfaffine fracture channels at finite reynolds number is calculated the channels have constant mean aperture and two values zeta05 and 08 of the hurst exponent are considered the calculation is based on the latticeboltzmann method using a novel method to obtain a powerlaw variation in viscosity and the behavior of shearthinning newtonian and shearthickening liquids is compared local aspects of the flow fields such as maximum velocity and pressure fluctuations were studied and the nonnewtonian fluids were compared to the previouslystudied newtonian case the permeability results may be collapsed into a master curve of friction factor vs reynolds number using a scaling similar to that employed for porous media flow and exhibits a transition from a linear regime to a more rapid variation at re increases
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711.4805
Deeply Virtual Compton Scattering Beam-Spin Asymmetries
The beam spin asymmetries in the hard exclusive electroproduction of photons on the proton (ep -> epg) were measured over a wide kinematic range and with high statistical accuracy. These asymmetries result from the interference of the Bethe-Heitler process and of deeply virtual Compton scattering. Over the whole kinematic range (x_B from 0.11 to 0.58, Q^2 from 1 to 4.8 GeV^2, -t from 0.09 to 1.8 GeV^2), the azimuthal dependence of the asymmetries is compatible with expectations from leading-twist dominance, A = a*sin(phi)/[1+c*cos(phi)]. This extensive set of data can thus be used to constrain significantly the generalized parton distributions of the nucleon in the valence quark sector.
hep-ex hep-ph nucl-ex
the beam spin asymmetries in the hard exclusive electroproduction of photons on the proton ep epg were measured over a wide kinematic range and with high statistical accuracy these asymmetries result from the interference of the betheheitler process and of deeply virtual compton scattering over the whole kinematic range x_b from 011 to 058 q2 from 1 to 48 gev2 t from 009 to 18 gev2 the azimuthal dependence of the asymmetries is compatible with expectations from leadingtwist dominance a asinphi1ccosphi this extensive set of data can thus be used to constrain significantly the generalized parton distributions of the nucleon in the valence quark sector
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711.4806
Statistical Equilibrium Dynamics
The mean-field thermodynamic limit is studied for a class of isolated Newtonian N-body systems whose Hamiltonian admits several invariants of motion. It is shown that the macrostates of individual members of a statistical equilibrium ensemble are not necessarily themselves in a state of global thermal equilibrium in the strict sense. Yet they are always locally in thermodynamic equilibrium, and always global maximizers of the pertinent maximum entropy principle.
math-ph math.MP
the meanfield thermodynamic limit is studied for a class of isolated newtonian nbody systems whose hamiltonian admits several invariants of motion it is shown that the macrostates of individual members of a statistical equilibrium ensemble are not necessarily themselves in a state of global thermal equilibrium in the strict sense yet they are always locally in thermodynamic equilibrium and always global maximizers of the pertinent maximum entropy principle
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711.4807
The circumstellar medium around a rapidly rotating, chemically homogeneously evolving, possible gamma-ray burst progenitor
Rapidly rotating, chemically homogeneously evolving massive stars are considered to be progenitors of long gamma-ray bursts. We present numerical simulations of the evolution of the circumstellar medium around a rapidly rotating 20 Msol star at a metallicity of Z=0.001. Its rotation is fast enough to produce quasi-chemically homogeneous evolution. While conventionally, a star of 20 Msol would not evolve into a Wolf-Rayet stage, the considered model evolves from the main sequence directly to the helium main sequence. We use the time-dependent wind parameters, such as mass loss rate, wind velocity and rotation-induced wind anisotropy from the evolution model as input for a 2D hydrodynamical simulation. While the outer edge of the pressure-driven circumstellar bubble is spherical, the circumstellar medium close to the star shows strong non-spherical features during and after the periods of near-critical rotation. We conclude that the circumstellar medium around rapidly rotating massive stars differs considerably from the surrounding material of non-rotating stars of similar mass. Multiple blue-shifted high velocity absorption components in gamma-ray burst afterglow spectra are predicted. As a consequence of near critical rotation and short stellar evolution time scales during the last few thousand years of the star's life, we find a strong deviation of the circumstellar density profile in the polar direction from the 1/R^2 density profile normally associated with stellar winds close to the star
astro-ph
rapidly rotating chemically homogeneously evolving massive stars are considered to be progenitors of long gammaray bursts we present numerical simulations of the evolution of the circumstellar medium around a rapidly rotating 20 msol star at a metallicity of z0001 its rotation is fast enough to produce quasichemically homogeneous evolution while conventionally a star of 20 msol would not evolve into a wolfrayet stage the considered model evolves from the main sequence directly to the helium main sequence we use the timedependent wind parameters such as mass loss rate wind velocity and rotationinduced wind anisotropy from the evolution model as input for a 2d hydrodynamical simulation while the outer edge of the pressuredriven circumstellar bubble is spherical the circumstellar medium close to the star shows strong nonspherical features during and after the periods of nearcritical rotation we conclude that the circumstellar medium around rapidly rotating massive stars differs considerably from the surrounding material of nonrotating stars of similar mass multiple blueshifted high velocity absorption components in gammaray burst afterglow spectra are predicted as a consequence of near critical rotation and short stellar evolution time scales during the last few thousand years of the stars life we find a strong deviation of the circumstellar density profile in the polar direction from the 1r2 density profile normally associated with stellar winds close to the star
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