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710.0653
Study of the critical point in lattice QCD at high temperature and density
We propose a method to probe the nature of phase transitions in lattice QCD at finite temperature and density, which is based on the investigation of an effective potential as a function of the average plaquette. We analyze data obtained in a simulation of two-flavor QCD using p4-improved staggered quarks with bare quark mass $m/T = 0.4$, and find that a first order phase transition line appears in the high density regime for $\mu_q/T \sim 2.5$. The effective potential as a function of the quark number density is also studied. We calculate the chemical potential as a function of the density from the canonical partition function and discuss the existence of the first order phase transition line.
hep-lat
we propose a method to probe the nature of phase transitions in lattice qcd at finite temperature and density which is based on the investigation of an effective potential as a function of the average plaquette we analyze data obtained in a simulation of twoflavor qcd using p4improved staggered quarks with bare quark mass mt 04 and find that a first order phase transition line appears in the high density regime for mu_qt sim 25 the effective potential as a function of the quark number density is also studied we calculate the chemical potential as a function of the density from the canonical partition function and discuss the existence of the first order phase transition line
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710.0654
Steady-state analysis of a multi-server queue in the Halfin-Whitt regime
We consider a multi-server queue in the Halfin-Whitt regime: as the number of servers $n$ grows without a bound, the utilization approaches 1 from below at the rate $\Theta(1/\sqrt{n})$. Assuming that the service time distribution is lattice-valued with a finite support, we characterize the limiting stationary queue length distribution in terms of the stationary distribution of an explicitly constructed Markov chain. Furthermore, we obtain an explicit expression for the critical exponent for the moment generating function of a limiting (scaled) steady-state queue length. This exponent has a compact representation in terms of three parameters: the amount of spare capacity and the coefficients of variation of interarrival and service times. Interestingly, it matches an analogous exponent corresponding to a single-server queue in the conventional heavy-traffic regime.
math.PR
we consider a multiserver queue in the halfinwhitt regime as the number of servers n grows without a bound the utilization approaches 1 from below at the rate theta1sqrtn assuming that the service time distribution is latticevalued with a finite support we characterize the limiting stationary queue length distribution in terms of the stationary distribution of an explicitly constructed markov chain furthermore we obtain an explicit expression for the critical exponent for the moment generating function of a limiting scaled steadystate queue length this exponent has a compact representation in terms of three parameters the amount of spare capacity and the coefficients of variation of interarrival and service times interestingly it matches an analogous exponent corresponding to a singleserver queue in the conventional heavytraffic regime
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710.0655
Unique Games with Entangled Provers are Easy
We consider one-round games between a classical verifier and two provers who share entanglement. We show that when the constraints enforced by the verifier are `unique' constraints (i.e., permutations), the value of the game can be well approximated by a semidefinite program. Essentially the only algorithm known previously was for the special case of binary answers, as follows from the work of Tsirelson in 1980. Among other things, our result implies that the variant of the unique games conjecture where we allow the provers to share entanglement is false. Our proof is based on a novel `quantum rounding technique', showing how to take a solution to an SDP and transform it to a strategy for entangled provers. Using our approximation by a semidefinite program we also show a parallel repetition theorem for unique entangled games.
quant-ph
we consider oneround games between a classical verifier and two provers who share entanglement we show that when the constraints enforced by the verifier are unique constraints ie permutations the value of the game can be well approximated by a semidefinite program essentially the only algorithm known previously was for the special case of binary answers as follows from the work of tsirelson in 1980 among other things our result implies that the variant of the unique games conjecture where we allow the provers to share entanglement is false our proof is based on a novel quantum rounding technique showing how to take a solution to an sdp and transform it to a strategy for entangled provers using our approximation by a semidefinite program we also show a parallel repetition theorem for unique entangled games
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710.0656
Measurement of b-Baryons with the CDF II detector
We report the observation of new bottom baryon states. The most recent result is the observation of the baryon \Xi_b^- through the decay \Xi_b^- to J/\psi \Xi^-. The significance of the signal corresponds to 7.7 sigma and the \Xi_b^- mass is measured to be 5792.9 \pm 2.5(stat.) \pm 1.7(syst.) MeV/c^2. In addition we observe four resonances in the \Lambda_b^0 \pi^{\pm} spectra, consistent with the bottom baryons \Sigma_b^{(*)\pm}. All observations are in agreement with theoretical expectations.
hep-ex
we report the observation of new bottom baryon states the most recent result is the observation of the baryon xi_b through the decay xi_b to jpsi xi the significance of the signal corresponds to 77 sigma and the xi_b mass is measured to be 57929 pm 25stat pm 17syst mevc2 in addition we observe four resonances in the lambda_b0 pipm spectra consistent with the bottom baryons sigma_bpm all observations are in agreement with theoretical expectations
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710.0657
A Multiresolution Census Algorithm for Calculating Vortex Statistics in Turbulent Flows
The fundamental equations that model turbulent flow do not provide much insight into the size and shape of observed turbulent structures. We investigate the efficient and accurate representation of structures in two-dimensional turbulence by applying statistical models directly to the simulated vorticity field. Rather than extract the coherent portion of the image from the background variation, as in the classical signal-plus-noise model, we present a model for individual vortices using the non-decimated discrete wavelet transform. A template image, supplied by the user, provides the features to be extracted from the vorticity field. By transforming the vortex template into the wavelet domain, specific characteristics present in the template, such as size and symmetry, are broken down into components associated with spatial frequencies. Multivariate multiple linear regression is used to fit the vortex template to the vorticity field in the wavelet domain. Since all levels of the template decomposition may be used to model each level in the field decomposition, the resulting model need not be identical to the template. Application to a vortex census algorithm that records quantities of interest (such as size, peak amplitude, circulation, etc.) as the vorticity field evolves is given. The multiresolution census algorithm extracts coherent structures of all shapes and sizes in simulated vorticity fields and is able to reproduce known physical scaling laws when processing a set of voriticity fields that evolve over time.
stat.AP physics.ao-ph
the fundamental equations that model turbulent flow do not provide much insight into the size and shape of observed turbulent structures we investigate the efficient and accurate representation of structures in twodimensional turbulence by applying statistical models directly to the simulated vorticity field rather than extract the coherent portion of the image from the background variation as in the classical signalplusnoise model we present a model for individual vortices using the nondecimated discrete wavelet transform a template image supplied by the user provides the features to be extracted from the vorticity field by transforming the vortex template into the wavelet domain specific characteristics present in the template such as size and symmetry are broken down into components associated with spatial frequencies multivariate multiple linear regression is used to fit the vortex template to the vorticity field in the wavelet domain since all levels of the template decomposition may be used to model each level in the field decomposition the resulting model need not be identical to the template application to a vortex census algorithm that records quantities of interest such as size peak amplitude circulation etc as the vorticity field evolves is given the multiresolution census algorithm extracts coherent structures of all shapes and sizes in simulated vorticity fields and is able to reproduce known physical scaling laws when processing a set of voriticity fields that evolve over time
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710.0658
Detailed Network Measurements Using Sparse Graph Counters: The Theory
Measuring network flow sizes is important for tasks like accounting/billing, network forensics and security. Per-flow accounting is considered hard because it requires that many counters be updated at a very high speed; however, the large fast memories needed for storing the counters are prohibitively expensive. Therefore, current approaches aim to obtain approximate flow counts; that is, to detect large elephant flows and then measure their sizes. Recently the authors and their collaborators have developed [1] a novel method for per-flow traffic measurement that is fast, highly memory efficient and accurate. At the core of this method is a novel counter architecture called "counter braids.'' In this paper, we analyze the performance of the counter braid architecture under a Maximum Likelihood (ML) flow size estimation algorithm and show that it is optimal; that is, the number of bits needed to store the size of a flow matches the entropy lower bound. While the ML algorithm is optimal, it is too complex to implement. In [1] we have developed an easy-to-implement and efficient message passing algorithm for estimating flow sizes.
cs.NI cs.IT math.IT
measuring network flow sizes is important for tasks like accountingbilling network forensics and security perflow accounting is considered hard because it requires that many counters be updated at a very high speed however the large fast memories needed for storing the counters are prohibitively expensive therefore current approaches aim to obtain approximate flow counts that is to detect large elephant flows and then measure their sizes recently the authors and their collaborators have developed 1 a novel method for perflow traffic measurement that is fast highly memory efficient and accurate at the core of this method is a novel counter architecture called counter braids in this paper we analyze the performance of the counter braid architecture under a maximum likelihood ml flow size estimation algorithm and show that it is optimal that is the number of bits needed to store the size of a flow matches the entropy lower bound while the ml algorithm is optimal it is too complex to implement in 1 we have developed an easytoimplement and efficient message passing algorithm for estimating flow sizes
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710.0659
The TrICE Prototype MAMPT Imaging Camera
The Track Imaging Cerenov Experiment (TrICE) is an air Cerenkov prototype telescope designed to use multi-anode photomultiplier to acheive a high angular resolution for measuring cosmic-ray composition at TeV-PeV energies. The TrICE camera, composed of 16 Hamamatsu R8900 16-channel multi-anode photomultiplier tubes, achieves 0.086 degree angular width per pixel over 1.5 degree wide field of view. We present a description of the TrICE camera design, calibration and performance.
astro-ph
the track imaging cerenov experiment trice is an air cerenkov prototype telescope designed to use multianode photomultiplier to acheive a high angular resolution for measuring cosmicray composition at tevpev energies the trice camera composed of 16 hamamatsu r8900 16channel multianode photomultiplier tubes achieves 0086 degree angular width per pixel over 15 degree wide field of view we present a description of the trice camera design calibration and performance
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710.066
Effective Dynamics of Solitons in the Presence of Rough Nonlinear Perturbations
The effective long-time dynamics of solitary wave solutions of the nonlinear Schr\"odinger equation in the presence of rough nonlinear perturbations is rigorously studied. It is shown that, if the initial state is close to a slowly travelling soliton of the unperturbed NLS equation (in $H^1$ norm), then, over a long time scale, the true solution of the initial value problem will be close to a soliton whose center of mass dynamics is approximately determined by an effective potential that corresponds to the restriction of the nonlinear perturbation to the soliton manifold.
math-ph math.MP
the effective longtime dynamics of solitary wave solutions of the nonlinear schrodinger equation in the presence of rough nonlinear perturbations is rigorously studied it is shown that if the initial state is close to a slowly travelling soliton of the unperturbed nls equation in h1 norm then over a long time scale the true solution of the initial value problem will be close to a soliton whose center of mass dynamics is approximately determined by an effective potential that corresponds to the restriction of the nonlinear perturbation to the soliton manifold
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710.0661
Self-consistent theory of phonon renormalization and electron-phonon coupling near a 2D Kohn singularity
We show that the usual expression for evaluating electron-phonon coupling and the phonon linewidth in 2D metals with a cylindrical Fermi surface cannot be applied near the wave vector corresponding to the Kohn singularity. Instead, the Dyson equation for phonons has to be solved self-consistently. If a self-consistent procedure is properly followed, there is no divergency in either the coupling constant or the phonon linewidth near the offending wave vectors, in contrast to the standard expression.
cond-mat.supr-con cond-mat.str-el
we show that the usual expression for evaluating electronphonon coupling and the phonon linewidth in 2d metals with a cylindrical fermi surface cannot be applied near the wave vector corresponding to the kohn singularity instead the dyson equation for phonons has to be solved selfconsistently if a selfconsistent procedure is properly followed there is no divergency in either the coupling constant or the phonon linewidth near the offending wave vectors in contrast to the standard expression
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710.0662
Modeling the line variations from the wind-wind shock emissions of WR 30a
The study of Wolf-Rayet stars plays an important role in evolutionary theories of massive stars. Among these objects, ~ 20% are known to be in binary systems and can therefore be used for the mass determination of these stars. Most of these systems are not spatially resolved and spectral lines can be used to constrain the orbital parameters. However, part of the emission may originate in the interaction zone between the stellar winds, modifying the line profiles and thus challenging us to use different models to interpret them. In this work, we analyzed the HeII4686\AA + CIV4658\AA blended lines of WR30a (WO4+O5) assuming that part of the emission originate in the wind-wind interaction zone. In fact, this line presents a quiescent base profile, attributed to the WO wind, and a superposed excess, which varies with the orbital phase along the 4.6 day period. Under these assumptions, we were able to fit the excess spectral line profile and central velocity for all phases, except for the longest wavelengths, where a spectral line with constant velocity seems to be present. The fit parameters provide the eccentricity and inclination of the binary orbit, from which it is possible to constrain the stellar masses.
astro-ph
the study of wolfrayet stars plays an important role in evolutionary theories of massive stars among these objects 20 are known to be in binary systems and can therefore be used for the mass determination of these stars most of these systems are not spatially resolved and spectral lines can be used to constrain the orbital parameters however part of the emission may originate in the interaction zone between the stellar winds modifying the line profiles and thus challenging us to use different models to interpret them in this work we analyzed the heii4686aa civ4658aa blended lines of wr30a wo4o5 assuming that part of the emission originate in the windwind interaction zone in fact this line presents a quiescent base profile attributed to the wo wind and a superposed excess which varies with the orbital phase along the 46 day period under these assumptions we were able to fit the excess spectral line profile and central velocity for all phases except for the longest wavelengths where a spectral line with constant velocity seems to be present the fit parameters provide the eccentricity and inclination of the binary orbit from which it is possible to constrain the stellar masses
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710.0663
SAURON's Challenge for the Major Merger Scenario of Elliptical Galaxy Formation
The intrinsic anisotropy delta and flattening epsilon of simulated merger remnants is compared with elliptical galaxies that have been observed by the SAURON collaboration, and that were analysed using axisymmetric Schwarzschild models. Collisionless binary mergers of stellar disks and disk mergers with an additional isothermal gas component, neglecting star formation cannot reproduce the observed trend delta = 0.55 epsilon (SAURON relationship). An excellent fit of the SAURON relationship for flattened ellipticals with epsilon >= 0.25 is however found for merger simulations of disks with gas fractions >= 20%, including star formation and stellar energy feedback. Massive black hole feedback does not strongly affect this result. Subsequent dry merging of merger remnants however does not generate the slowly-rotating SAURON ellipticals which are characterized by low ellipticities epsilon < 0.25 and low anisotropies. This indicates that at least some ellipticals on the red galaxy sequence did not form by binary mergers of disks or early-type galaxies. We show that stellar spheroids resulting from multiple, hierarchical mergers of star-bursting subunits in a cosmological context are in excellent agreement with the low ellipticities and anisotropies of the slowly rotating SAURON ellipticals and their observed trend of delta with epsilon. The numerical simulations indicate that the SAURON relation might be a result of strong violent relaxation and phase mixing of multiple, kinematically cold stellar subunits with the angular momentum of the system determining its location on the relation.
astro-ph
the intrinsic anisotropy delta and flattening epsilon of simulated merger remnants is compared with elliptical galaxies that have been observed by the sauron collaboration and that were analysed using axisymmetric schwarzschild models collisionless binary mergers of stellar disks and disk mergers with an additional isothermal gas component neglecting star formation cannot reproduce the observed trend delta 055 epsilon sauron relationship an excellent fit of the sauron relationship for flattened ellipticals with epsilon 025 is however found for merger simulations of disks with gas fractions 20 including star formation and stellar energy feedback massive black hole feedback does not strongly affect this result subsequent dry merging of merger remnants however does not generate the slowlyrotating sauron ellipticals which are characterized by low ellipticities epsilon 025 and low anisotropies this indicates that at least some ellipticals on the red galaxy sequence did not form by binary mergers of disks or earlytype galaxies we show that stellar spheroids resulting from multiple hierarchical mergers of starbursting subunits in a cosmological context are in excellent agreement with the low ellipticities and anisotropies of the slowly rotating sauron ellipticals and their observed trend of delta with epsilon the numerical simulations indicate that the sauron relation might be a result of strong violent relaxation and phase mixing of multiple kinematically cold stellar subunits with the angular momentum of the system determining its location on the relation
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710.0664
Synthesis and Optimization of Reversible Circuits for Homogeneous Boolean Functions
Homogenous Boolean function is an essential part of any cryptographic system. The ability to construct an optimized reversible circuits for homogeneous Boolean functions might arise the possibility of building cryptographic system on novel computing paradigms such as quantum computers. This paper shows a factorization algorithm to synthesize such circuits.
quant-ph
homogenous boolean function is an essential part of any cryptographic system the ability to construct an optimized reversible circuits for homogeneous boolean functions might arise the possibility of building cryptographic system on novel computing paradigms such as quantum computers this paper shows a factorization algorithm to synthesize such circuits
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710.0665
Infrared exponents of gluon and ghost propagators from Lattice QCD
The compatibility of the pure power law infrared solution of QCD Dyson-Schwinger equations (DSE) and lattice data for the gluon and ghost propagators in Landau gauge is discussed. For the gluon propagator, the lattice data is compatible with the DSE infrared solution with an exponent $\kappa\sim0.53$, measured using a technique that suppresses finite volume effects and allows to model these corrections to the lattice data. For the ghost propagator, the lattice data does not seem to follow the infrared DSE power law solution.
hep-lat
the compatibility of the pure power law infrared solution of qcd dysonschwinger equations dse and lattice data for the gluon and ghost propagators in landau gauge is discussed for the gluon propagator the lattice data is compatible with the dse infrared solution with an exponent kappasim053 measured using a technique that suppresses finite volume effects and allows to model these corrections to the lattice data for the ghost propagator the lattice data does not seem to follow the infrared dse power law solution
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710.0666
Thiol density dependent classical potential for methyl-thiol on a Au(111) surface
A new classical potential for methyl-thiol on a Au(111) surface has been developed using density functional theory electronic structure calculations. Energy surfaces between methyl-thiol and a gold surface were investigated in terms of symmetry sites and thiol density. Geometrical optimization was employed over all the configurations while minimum energy and thiol height were determined. Finally, a new interatomic potential has been generated as a function of thiol density, and applications to coarse-grained simulations are presented.
cond-mat.mtrl-sci cond-mat.soft
a new classical potential for methylthiol on a au111 surface has been developed using density functional theory electronic structure calculations energy surfaces between methylthiol and a gold surface were investigated in terms of symmetry sites and thiol density geometrical optimization was employed over all the configurations while minimum energy and thiol height were determined finally a new interatomic potential has been generated as a function of thiol density and applications to coarsegrained simulations are presented
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710.0667
Chaotic Period Doubling
The period doubling renormalization operator was introduced by M. Feigenbaum and by P. Coullet and C. Tresser in the nineteen-seventieth to study the asymptotic small scale geometry of the attractor of one-dimensional systems which are at the transition from simple to chaotic dynamics. This geometry turns out to not depend on the choice of the map under rather mild smoothness conditions. The existence of a unique renormalization fixed point which is also hyperbolic among generic smooth enough maps plays a crucial role in the corresponding renormalization theory. The uniqueness and hyperbolicity of the renormalization fixed point were first shown in the holomorphic context, by means that generalize to other renormalization operators. It was then proved that in the space of $C^{2+\alpha}$ unimodal maps, for $\alpha$ close to one, the period doubling renormalization fixed point is hyperbolic as well. In this paper we study what happens when one approaches from below the minimal smoothness thresholds for the uniqueness and for the hyperbolicity of the period doubling renormalization generic fixed point. Indeed, our main results states that in the space of $C^2$ unimodal maps the analytic fixed point is not hyperbolic and that the same remains true when adding enough smoothness to get a priori bounds. In this smoother class, called $C^{2+|\cdot|}$ the failure of hyperbolicity is tamer than in $C^2$. Things get much worse with just a bit less of smoothness than $C^2$ as then even the uniqueness is lost and other asymptotic behavior become possible. We show that the period doubling renormalization operator acting on the space of $C^{1+Lip}$ unimodal maps has infinite topological entropy.
math.DS
the period doubling renormalization operator was introduced by m feigenbaum and by p coullet and c tresser in the nineteenseventieth to study the asymptotic small scale geometry of the attractor of onedimensional systems which are at the transition from simple to chaotic dynamics this geometry turns out to not depend on the choice of the map under rather mild smoothness conditions the existence of a unique renormalization fixed point which is also hyperbolic among generic smooth enough maps plays a crucial role in the corresponding renormalization theory the uniqueness and hyperbolicity of the renormalization fixed point were first shown in the holomorphic context by means that generalize to other renormalization operators it was then proved that in the space of c2alpha unimodal maps for alpha close to one the period doubling renormalization fixed point is hyperbolic as well in this paper we study what happens when one approaches from below the minimal smoothness thresholds for the uniqueness and for the hyperbolicity of the period doubling renormalization generic fixed point indeed our main results states that in the space of c2 unimodal maps the analytic fixed point is not hyperbolic and that the same remains true when adding enough smoothness to get a priori bounds in this smoother class called c2cdot the failure of hyperbolicity is tamer than in c2 things get much worse with just a bit less of smoothness than c2 as then even the uniqueness is lost and other asymptotic behavior become possible we show that the period doubling renormalization operator acting on the space of c1lip unimodal maps has infinite topological entropy
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710.0668
Visible and invisible molecular gas in collisional debris of galaxies
Molecular gas has been searched for and found in unexpectedly large quantities in some collisional debris of interacting galaxies: HI-rich tidal tails, bridges and collisional rings. It was so far observed through millimeter observations of the CO line and detected towards or near regions of star-formation associated to dense condensations of the atomic hydrogen. The discovery of cool H2 at distances greater than 50 kpc from the parent (colliding) galaxies, whereas the external disk of spirals is generally considered to be CO-poor, raised question on its origin and favored the hypothesis of a local production out of collapsed HI clouds. However recent observations of a diffuse CO component along tidal debris have challenged this idea. Another recent puzzle is the measurement in the collisional debris of two interacting systems and four recycled objects of a missing mass, whereas no dark matter is expected there. One debated interpretation is that this unseen component is cold, "invisible" molecular gas initially present in the disk of spirals.
astro-ph
molecular gas has been searched for and found in unexpectedly large quantities in some collisional debris of interacting galaxies hirich tidal tails bridges and collisional rings it was so far observed through millimeter observations of the co line and detected towards or near regions of starformation associated to dense condensations of the atomic hydrogen the discovery of cool h2 at distances greater than 50 kpc from the parent colliding galaxies whereas the external disk of spirals is generally considered to be copoor raised question on its origin and favored the hypothesis of a local production out of collapsed hi clouds however recent observations of a diffuse co component along tidal debris have challenged this idea another recent puzzle is the measurement in the collisional debris of two interacting systems and four recycled objects of a missing mass whereas no dark matter is expected there one debated interpretation is that this unseen component is cold invisible molecular gas initially present in the disk of spirals
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710.0669
Gauge fixing methods and Gribov copies effects in lattice QCD
We compare two Landau gauge fixing methods, aiming to find the global maximum of the gauge fixing functional. Moreover, a systematic effect of Gribov copies in the gluon and ghost propagators computed in Landau gauge is presented and discussed.
hep-lat
we compare two landau gauge fixing methods aiming to find the global maximum of the gauge fixing functional moreover a systematic effect of gribov copies in the gluon and ghost propagators computed in landau gauge is presented and discussed
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710.067
Evolution of Schrodinger Uncertainty Relation in Quantum Mechanics
In the present article, we discuss one of the basic relations of Quantum Mechanics - the Uncertainty Relation (UR). In 1930, few years after Heisenberg, Erwin Schrodinger generalized the famous Uncertainty Relation in Quantum Mechanics, making it more precise than the original. The present study discusses recent generalizations of Schrodinger's work and explains why his paper remains almost forgotten in the last century.
quant-ph
in the present article we discuss one of the basic relations of quantum mechanics the uncertainty relation ur in 1930 few years after heisenberg erwin schrodinger generalized the famous uncertainty relation in quantum mechanics making it more precise than the original the present study discusses recent generalizations of schrodingers work and explains why his paper remains almost forgotten in the last century
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710.0671
The Cosmos in Your Pocket: How Cosmological Science Became Earth Technology. I
Astronomy provides a laboratory for extreme physics, a window into environments at extremes of distance, temperature and density that often can't be reproduced in Earth laboratories, or at least not right away. A surprising amount of the science we understand today started out as solutions to problems in astronomy. Some of this science was key in the development of many technologies which we enjoy today. This paper describes some of these connections between astronomy and technology and their history.
physics.pop-ph astro-ph
astronomy provides a laboratory for extreme physics a window into environments at extremes of distance temperature and density that often cant be reproduced in earth laboratories or at least not right away a surprising amount of the science we understand today started out as solutions to problems in astronomy some of this science was key in the development of many technologies which we enjoy today this paper describes some of these connections between astronomy and technology and their history
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710.0672
Optimization of supply diversity for the self-assembly of simple objects in two and three dimensions
The field of algorithmic self-assembly is concerned with the design and analysis of self-assembly systems from a computational perspective, that is, from the perspective of mathematical problems whose study may give insight into the natural processes through which elementary objects self-assemble into more complex ones. One of the main problems of algorithmic self-assembly is the minimum tile set problem (MTSP), which asks for a collection of types of elementary objects (called tiles) to be found for the self-assembly of an object having a pre-established shape. Such a collection is to be as concise as possible, thus minimizing supply diversity, while satisfying a set of stringent constraints having to do with the termination and other properties of the self-assembly process from its tile types. We present a study of what we think is the first practical approach to MTSP. Our study starts with the introduction of an evolutionary heuristic to tackle MTSP and includes results from extensive experimentation with the heuristic on the self-assembly of simple objects in two and three dimensions. The heuristic we introduce combines classic elements from the field of evolutionary computation with a problem-specific variant of Pareto dominance into a multi-objective approach to MTSP.
cs.NE
the field of algorithmic selfassembly is concerned with the design and analysis of selfassembly systems from a computational perspective that is from the perspective of mathematical problems whose study may give insight into the natural processes through which elementary objects selfassemble into more complex ones one of the main problems of algorithmic selfassembly is the minimum tile set problem mtsp which asks for a collection of types of elementary objects called tiles to be found for the selfassembly of an object having a preestablished shape such a collection is to be as concise as possible thus minimizing supply diversity while satisfying a set of stringent constraints having to do with the termination and other properties of the selfassembly process from its tile types we present a study of what we think is the first practical approach to mtsp our study starts with the introduction of an evolutionary heuristic to tackle mtsp and includes results from extensive experimentation with the heuristic on the selfassembly of simple objects in two and three dimensions the heuristic we introduce combines classic elements from the field of evolutionary computation with a problemspecific variant of pareto dominance into a multiobjective approach to mtsp
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710.0673
Phase diagram of the one-dimensional half-filled extended Hubbard model
We study the ground state of the one-dimensional half-filled Hubbard model with on-site (nearest-neighbor) repulsive interaction $U$ ($V$) and nearest-neighbor hopping $t$. In order to obtain an accurate phase diagram, we consider various physical quantities such as the charge gap, spin gap, Luttinger-liquid exponents, and bond-order-wave (BOW) order parameter using the density-matrix renormalization group technique. We confirm that the BOW phase appears in a substantial region between the charge-density-wave (CDW) and spin-density-wave phases. Each phase boundary is determined by multiple means and it allows us to do a cross-check to demonstrate the validity of our estimations. Thus, our results agree quantitatively with the renormalization group results in the weak-coupling regime ($U \lesssim 2t$), with the perturbation results in the strong-coupling regime ($U \gtrsim 6t$), and with the quantum Monte Carlo results in the intermediate-coupling regime. We also find that the BOW-CDW transition changes from continuous to first order at the tricritical point $(U_{\rm t}, V_{\rm t}) \approx (5.89t, 3.10t)$ and the BOW phase vanishes at the critical end point $(U_{\rm c}, V_{\rm c}) \approx (9.25t, 4.76t)$.
cond-mat.str-el
we study the ground state of the onedimensional halffilled hubbard model with onsite nearestneighbor repulsive interaction u v and nearestneighbor hopping t in order to obtain an accurate phase diagram we consider various physical quantities such as the charge gap spin gap luttingerliquid exponents and bondorderwave bow order parameter using the densitymatrix renormalization group technique we confirm that the bow phase appears in a substantial region between the chargedensitywave cdw and spindensitywave phases each phase boundary is determined by multiple means and it allows us to do a crosscheck to demonstrate the validity of our estimations thus our results agree quantitatively with the renormalization group results in the weakcoupling regime u lesssim 2t with the perturbation results in the strongcoupling regime u gtrsim 6t and with the quantum monte carlo results in the intermediatecoupling regime we also find that the bowcdw transition changes from continuous to first order at the tricritical point u_rm t v_rm t approx 589t 310t and the bow phase vanishes at the critical end point u_rm c v_rm c approx 925t 476t
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710.0674
New phases of finite temperature gauge theory from an extended action
We study the behavior of the order parameter, the phase diagram, and the thermodynamics of exotic phases of finite temperature gauge theory. Lattice simulations were performed in SU(3) and SU(4) with an adjoint Polyakov loop term added to the standard Wilson action. In SU(3), the pattern of Z(3) symmetry breaking in the new phase is distinct from the pattern observed in the deconfined phase. In SU(4), the Z(4) symmetry is spontaneously broken down to Z(2), representing a partially-confined phase. The existence of the new phases is confirmed in analytical calculations of the free energy based on high-temperature perturbation theory.
hep-lat
we study the behavior of the order parameter the phase diagram and the thermodynamics of exotic phases of finite temperature gauge theory lattice simulations were performed in su3 and su4 with an adjoint polyakov loop term added to the standard wilson action in su3 the pattern of z3 symmetry breaking in the new phase is distinct from the pattern observed in the deconfined phase in su4 the z4 symmetry is spontaneously broken down to z2 representing a partiallyconfined phase the existence of the new phases is confirmed in analytical calculations of the free energy based on hightemperature perturbation theory
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710.0675
Finding pulsars with LOFAR
We investigate the number and type of pulsars that will be discovered with the low-frequency radio telescope LOFAR. We consider different search strategies for the Galaxy, for globular clusters and for galaxies other than our own. We show an all-sky Galactic survey can be optimally carried out by incoherently combining the LOFAR stations. In a 60-day all-sky Galactic survey LOFAR can find over a thousand pulsars, probing the local pulsar population to a very deep luminosity limit. For targets of smaller angular size, globular clusters and galaxies, the LOFAR stations can be combined coherently, making use of the full sensitivity. Searches of nearby northern-sky globular clusters can find large numbers of low luminosity millisecond pulsars (eg. over 10 new millisecond pulsars in a 10-hour observation of M15). If the pulsar population in nearby galaxies is similar to that of the Milky Way, a 10-hour observation could find the 10 brightest pulsars in M33, or pulsars in other galaxies out to a distance of 1.2Mpc.
astro-ph
we investigate the number and type of pulsars that will be discovered with the lowfrequency radio telescope lofar we consider different search strategies for the galaxy for globular clusters and for galaxies other than our own we show an allsky galactic survey can be optimally carried out by incoherently combining the lofar stations in a 60day allsky galactic survey lofar can find over a thousand pulsars probing the local pulsar population to a very deep luminosity limit for targets of smaller angular size globular clusters and galaxies the lofar stations can be combined coherently making use of the full sensitivity searches of nearby northernsky globular clusters can find large numbers of low luminosity millisecond pulsars eg over 10 new millisecond pulsars in a 10hour observation of m15 if the pulsar population in nearby galaxies is similar to that of the milky way a 10hour observation could find the 10 brightest pulsars in m33 or pulsars in other galaxies out to a distance of 12mpc
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710.0676
Remarks on the symmetric powers of cusp forms on GL(2)
In this paper we prove the following conditional result: Let F be a number field, and pi a cusp form on GL(2)/F which is not solvable polyhedral. Assume that all the symmetric powers sym^m(pi) are modular, i.e., define automorphic forms on GL(m+1)/F. If sym^6(pi) is cuspidal, then all the symmetric powers are cuspidal, for all m. Moreover, sym^6(pi) is Eisenteinian iff sym^5(pi) is an abelian twist of the functorial product of pi with the symmetric square of a cusp form pi' on GL(2)/F.
math.NT math.RT
in this paper we prove the following conditional result let f be a number field and pi a cusp form on gl2f which is not solvable polyhedral assume that all the symmetric powers symmpi are modular ie define automorphic forms on glm1f if sym6pi is cuspidal then all the symmetric powers are cuspidal for all m moreover sym6pi is eisenteinian iff sym5pi is an abelian twist of the functorial product of pi with the symmetric square of a cusp form pi on gl2f
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710.0677
The divided cell algorithm and the inhomogeneous Lagrange and Markoff spectra
The divided cell algorithm was introduced by Delone in 1947 to calculate the inhomogeneous minima of binary quadratic forms and developed further by E. S. Barnes and H. P. F. Swinnerton-Dyer in the 1950s. We show how advances of the past fifty years in both symbolic computation and our understanding of homogeneous spectra can be combined to make divided cells more useful for organizing information about inhomogeneous approximation problems. A crucial part of our analysis relies on work of Jane Pitman, who related the divided cell algorithm to the regular continued fraction algorithm. In particular, the relation to continued fractions allows two divided cells for the same problem to be compared without stepping through the chain of divided cells connecting them.
math.NT
the divided cell algorithm was introduced by delone in 1947 to calculate the inhomogeneous minima of binary quadratic forms and developed further by e s barnes and h p f swinnertondyer in the 1950s we show how advances of the past fifty years in both symbolic computation and our understanding of homogeneous spectra can be combined to make divided cells more useful for organizing information about inhomogeneous approximation problems a crucial part of our analysis relies on work of jane pitman who related the divided cell algorithm to the regular continued fraction algorithm in particular the relation to continued fractions allows two divided cells for the same problem to be compared without stepping through the chain of divided cells connecting them
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710.0678
Calculated Momentum Dependence of Zhang-Rice States in Transition Metal Oxides
Using a combination of local density functional theory and cluster exact diagonalization based dynamical mean field theory, we calculate many body electronic structures of several Mott insulating oxides including undoped high T_{c} materials. The dispersions of the lowest occupied electronic states are associated with the Zhang-Rice singlets in cuprates and with doublets, triplets, quadruplets and quintets in more general cases. Our results agree with angle resolved photoemission experiments including the decrease of the spectral weight of the Zhang--Rice band as it approaches k=0.
cond-mat.str-el
using a combination of local density functional theory and cluster exact diagonalization based dynamical mean field theory we calculate many body electronic structures of several mott insulating oxides including undoped high t_c materials the dispersions of the lowest occupied electronic states are associated with the zhangrice singlets in cuprates and with doublets triplets quadruplets and quintets in more general cases our results agree with angle resolved photoemission experiments including the decrease of the spectral weight of the zhangrice band as it approaches k0
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710.0679
Antisymmetric tensor matter fields in a curved space-time
An analysis about the antisymmetric tensor matter fields Avdeev-Chizhov theory in a curved space-time is performed. We show, in a curved spacetime, that the Avdeev-Chizhov theory can be seen as a kind of a $\lambda\phi^{4}$ theory for a "complex self-dual" field. This relationship between Avdeev-Chizhov theory and $\lambda\phi^{4}$ theory simplify the study of tensor matter fields in a curved space-time. The energy-momentum tensor for matter fields is computed.
hep-th
an analysis about the antisymmetric tensor matter fields avdeevchizhov theory in a curved spacetime is performed we show in a curved spacetime that the avdeevchizhov theory can be seen as a kind of a lambdaphi4 theory for a complex selfdual field this relationship between avdeevchizhov theory and lambdaphi4 theory simplify the study of tensor matter fields in a curved spacetime the energymomentum tensor for matter fields is computed
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710.068
Dynamical Threshold Enhancement and Resummation in Drell-Yan Production
Partonic cross sections for the production of massive objects in hadronic collisions receive large corrections when the invariant mass of the initial-state partons is just above the production threshold. Since typically the center-of-mass energy of the hadronic collision is much higher than the mass of the heavy objects, it is not obvious that these contributions translate into large corrections to the hadronic cross section. Using a recent approach to threshold resummation based on effective field theory, we quantify to which extent the fall-off of the parton densities at high x leads to a dynamical enhancement of the partonic threshold region. With the example of Drell-Yan production, we study the emergence of an effective physical scale characterizing the soft emissions in the process. We derive compact analytical expressions for the resummed Drell-Yan cross section and rapidity distribution directly in momentum space. They are free of Landau-pole singularities and are trivially matched onto fixed-order perturbative calculations. Evaluating the resummed cross sections at NNNLL order and matching onto NNLO fixed-order calculations, we perform a detailed numerical analysis of the cross section and rapidity distribution in proton-proton collisions.
hep-ph
partonic cross sections for the production of massive objects in hadronic collisions receive large corrections when the invariant mass of the initialstate partons is just above the production threshold since typically the centerofmass energy of the hadronic collision is much higher than the mass of the heavy objects it is not obvious that these contributions translate into large corrections to the hadronic cross section using a recent approach to threshold resummation based on effective field theory we quantify to which extent the falloff of the parton densities at high x leads to a dynamical enhancement of the partonic threshold region with the example of drellyan production we study the emergence of an effective physical scale characterizing the soft emissions in the process we derive compact analytical expressions for the resummed drellyan cross section and rapidity distribution directly in momentum space they are free of landaupole singularities and are trivially matched onto fixedorder perturbative calculations evaluating the resummed cross sections at nnnll order and matching onto nnlo fixedorder calculations we perform a detailed numerical analysis of the cross section and rapidity distribution in protonproton collisions
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710.0681
Yang-Mills theory over surfaces and the Atiyah-Segal theorem
In this paper we explain how Morse theory for the Yang-Mills functional can be used to prove an analogue, for surface groups, of the Atiyah-Segal theorem. Classically, the Atiyah-Segal theorem relates the representation ring R(\Gamma) of a compact Lie group $\Gamma$ to the complex K-theory of the classifying space $B\Gamma$. For infinite discrete groups, it is necessary to take into account deformations of representations, and with this in mind we replace the representation ring by Carlsson's deformation $K$--theory spectrum $\K (\Gamma)$ (the homotopy-theoretical analogue of $R(\Gamma)$). Our main theorem provides an isomorphism in homotopy $\K_*(\pi_1 \Sigma)\isom K^{-*}(\Sigma)$ for all compact, aspherical surfaces $\Sigma$ and all $*>0$. Combining this result with work of Tyler Lawson, we obtain homotopy theoretical information about the stable moduli space of flat unitary connections over surfaces.
math.AT math.DG math.KT
in this paper we explain how morse theory for the yangmills functional can be used to prove an analogue for surface groups of the atiyahsegal theorem classically the atiyahsegal theorem relates the representation ring rgamma of a compact lie group gamma to the complex ktheory of the classifying space bgamma for infinite discrete groups it is necessary to take into account deformations of representations and with this in mind we replace the representation ring by carlssons deformation ktheory spectrum k gamma the homotopytheoretical analogue of rgamma our main theorem provides an isomorphism in homotopy k_pi_1 sigmaisom ksigma for all compact aspherical surfaces sigma and all 0 combining this result with work of tyler lawson we obtain homotopy theoretical information about the stable moduli space of flat unitary connections over surfaces
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710.0682
Demonstration of a New Transport Regime of Photon in Two-dimensional Photonic Crystal
A new transport regime of photon in two-dimensional photonic crystal near the Dirac point has been demonstrated by exact numerical simulation. In this regime, the conductance of photon is inversely proportional to the thickness of sample, which can be described by Dirac equation very well. Both of bulk and surface disorders always reduce the transmission, which is in contrast to the previous theoretical prediction that they increase the conductance of electron at the Dirac point of grephene. However, regular tuning of interface structures can cause the improvement of photon conductance. Furthermore, large conductance fluctuations of photon have also been observed, which is similar to the case of electron in graphene.
cond-mat.mtrl-sci cond-mat.dis-nn
a new transport regime of photon in twodimensional photonic crystal near the dirac point has been demonstrated by exact numerical simulation in this regime the conductance of photon is inversely proportional to the thickness of sample which can be described by dirac equation very well both of bulk and surface disorders always reduce the transmission which is in contrast to the previous theoretical prediction that they increase the conductance of electron at the dirac point of grephene however regular tuning of interface structures can cause the improvement of photon conductance furthermore large conductance fluctuations of photon have also been observed which is similar to the case of electron in graphene
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710.0683
The One-Dimensional Wigner Crystal in Carbon Nanotubes
Electron-electron interactions strongly affect the behavior of low-dimensional systems. In one dimension (1D), arbitrarily weak interactions qualitatively alter the ground state producing a Luttinger liquid (LL) which has now been observed in a number of experimental systems. Interactions are even more important at low carrier density, and in the limit when the long-ranged Coulomb potential is the dominant energy scale, the electron liquid is expected to become a periodically ordered solid known as the Wigner crystal. In 1D, the Wigner crystal has been predicted to exhibit novel spin and magnetic properties not present in an ordinary LL. However, despite recent progress in coupled quantum wires, unambiguous experimental demonstration of this state has not been possible due to the role of disorder. Here, we demonstrate using low-temperature single-electron transport spectroscopy that a hole gas in low-disorder carbon nanotubes with a band gap is a realization of the 1D Wigner crystal. Our observation can lead to unprecedented control over the behavior of the spatially separated system of carriers, and could be used to realize solid state quantum computing with long coherence times.
cond-mat.str-el cond-mat.mes-hall
electronelectron interactions strongly affect the behavior of lowdimensional systems in one dimension 1d arbitrarily weak interactions qualitatively alter the ground state producing a luttinger liquid ll which has now been observed in a number of experimental systems interactions are even more important at low carrier density and in the limit when the longranged coulomb potential is the dominant energy scale the electron liquid is expected to become a periodically ordered solid known as the wigner crystal in 1d the wigner crystal has been predicted to exhibit novel spin and magnetic properties not present in an ordinary ll however despite recent progress in coupled quantum wires unambiguous experimental demonstration of this state has not been possible due to the role of disorder here we demonstrate using lowtemperature singleelectron transport spectroscopy that a hole gas in lowdisorder carbon nanotubes with a band gap is a realization of the 1d wigner crystal our observation can lead to unprecedented control over the behavior of the spatially separated system of carriers and could be used to realize solid state quantum computing with long coherence times
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710.0684
Quantum Control Landscapes
Numerous lines of experimental, numerical and analytical evidence indicate that it is surprisingly easy to locate optimal controls steering quantum dynamical systems to desired objectives. This has enabled the control of complex quantum systems despite the expense of solving the Schrodinger equation in simulations and the complicating effects of environmental decoherence in the laboratory. Recent work indicates that this simplicity originates in universal properties of the solution sets to quantum control problems that are fundamentally different from their classical counterparts. Here, we review studies that aim to systematically characterize these properties, enabling the classification of quantum control mechanisms and the design of globally efficient quantum control algorithms.
quant-ph
numerous lines of experimental numerical and analytical evidence indicate that it is surprisingly easy to locate optimal controls steering quantum dynamical systems to desired objectives this has enabled the control of complex quantum systems despite the expense of solving the schrodinger equation in simulations and the complicating effects of environmental decoherence in the laboratory recent work indicates that this simplicity originates in universal properties of the solution sets to quantum control problems that are fundamentally different from their classical counterparts here we review studies that aim to systematically characterize these properties enabling the classification of quantum control mechanisms and the design of globally efficient quantum control algorithms
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710.0685
Uniformly Balanced Repeated Measurements Designs in the Presence of Subject Dropout
Low, Lewis and Prescott (1999) showed that a crossover design based on a Williams Latin square of order 4 can suffer substantial loss of efficiency if some observations in the final period are unavailable. Indeed, if all observations are missing, the design becomes disconnected. We derive the information matrix for the direct effects of a Uniformly Balanced Repeated Measurements Design (UBRMD) in t periods when subjects may drop out before the end of the study and examine the maximum loss of information. The special case of loss of observations in the final period only is examined in detail. In particular we show that a UBRMD in t>= 5 periods remains connected when some or all observations in the final period are unavailable.
math.ST stat.TH
low lewis and prescott 1999 showed that a crossover design based on a williams latin square of order 4 can suffer substantial loss of efficiency if some observations in the final period are unavailable indeed if all observations are missing the design becomes disconnected we derive the information matrix for the direct effects of a uniformly balanced repeated measurements design ubrmd in t periods when subjects may drop out before the end of the study and examine the maximum loss of information the special case of loss of observations in the final period only is examined in detail in particular we show that a ubrmd in t 5 periods remains connected when some or all observations in the final period are unavailable
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710.0686
Habitability of Planets in Binaries
A survey of currently known extrasolar planets indicates that close to 20% of their hosting stars are members of binary systems. While the majority of these binaries are wide (i.e., with separations between 250 and 6500 AU), the detection of Jovian-type planets in the three binaries of Gamma Cephei (separation of 18.5 AU), GL 86 (separation of 21 AU), and HD 41004 (separation of 23 AU) have brought to the forefront questions on the formation of giant planets and the possibility of the existence of smaller bodies in moderately close binary star systems. This paper discusses the late stage of the formation of habitable planets in binary systems that host Jovian-type bodies, and reviews the effects of the binary companion on the formation of Earth-like planets in the system's habitable zone. The results of a large survey of the parameter-space of binary-planetary systems in search of regions where habitable planets can form and have long-term stable orbits are also presented.
astro-ph
a survey of currently known extrasolar planets indicates that close to 20 of their hosting stars are members of binary systems while the majority of these binaries are wide ie with separations between 250 and 6500 au the detection of joviantype planets in the three binaries of gamma cephei separation of 185 au gl 86 separation of 21 au and hd 41004 separation of 23 au have brought to the forefront questions on the formation of giant planets and the possibility of the existence of smaller bodies in moderately close binary star systems this paper discusses the late stage of the formation of habitable planets in binary systems that host joviantype bodies and reviews the effects of the binary companion on the formation of earthlike planets in the systems habitable zone the results of a large survey of the parameterspace of binaryplanetary systems in search of regions where habitable planets can form and have longterm stable orbits are also presented
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710.0687
Entanglement of a Laguerre-Gaussian cavity mode with a rotating mirror
It has previously been shown theoretically that the exchange of linear momentum between the light field in an optical cavity and a vibrating end mirror can entangle the electromagnetic field with the vibrational motion of that mirror. In this paper we consider the rotational analog of this situation and show that radiation torque can similarly entangle a Laguerre-Gaussian cavity mode with a rotating end mirror. We examine the mirror-field entanglement as a function of ambient temperature, radiation detuning and orbital angular momentum carried by the cavity mode.
quant-ph
it has previously been shown theoretically that the exchange of linear momentum between the light field in an optical cavity and a vibrating end mirror can entangle the electromagnetic field with the vibrational motion of that mirror in this paper we consider the rotational analog of this situation and show that radiation torque can similarly entangle a laguerregaussian cavity mode with a rotating end mirror we examine the mirrorfield entanglement as a function of ambient temperature radiation detuning and orbital angular momentum carried by the cavity mode
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710.0688
The type N Karlhede bound is sharp
We present a family of four-dimensional Lorentzian manifolds whose invariant classification requires the seventh covariant derivative of the curvature tensor. The spacetimes in questions are null radiation, type N solutions on an anti-de Sitter background. The large order of the bound is due to the fact that these spacetimes are properly $CH_2$, i.e., curvature homogeneous of order 2 but non-homogeneous. This means that tetrad components of $R, \nabla R, \nabla^{(2)}R$ are constant, and that essential coordinates first appear as components of $\nabla^{(3)}R$. Covariant derivatives of orders 4,5,6 yield one additional invariant each, and $\nabla^{(7)}R$ is needed for invariant classification. Thus, our class proves that the bound of 7 on the order of the covariant derivative, first established by Karlhede, is sharp. Our finding corrects an outstanding assertion that invariant classification of four-dimensional Lorentzian manifolds requires at most $\nabla^{(6)}R$.
gr-qc math.DG
we present a family of fourdimensional lorentzian manifolds whose invariant classification requires the seventh covariant derivative of the curvature tensor the spacetimes in questions are null radiation type n solutions on an antide sitter background the large order of the bound is due to the fact that these spacetimes are properly ch_2 ie curvature homogeneous of order 2 but nonhomogeneous this means that tetrad components of r nabla r nabla2r are constant and that essential coordinates first appear as components of nabla3r covariant derivatives of orders 456 yield one additional invariant each and nabla7r is needed for invariant classification thus our class proves that the bound of 7 on the order of the covariant derivative first established by karlhede is sharp our finding corrects an outstanding assertion that invariant classification of fourdimensional lorentzian manifolds requires at most nabla6r
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710.0689
Convexity and Cone-Vexing
The idea of convexity feeds generation, separation, calculus, and approximation. Generation appears as duality; separation, as optimality; calculus, as representation; and approximation, as stability. This is an overview of the origin, evolution, and trends of convexity. Study of convexity in the Sobolev Institute was initiated by Leonid Kantorovich (1912--1986) and Alexandr Alexandrov (1912--1999). This talk is a part of their memory.
math.FA math.HO
the idea of convexity feeds generation separation calculus and approximation generation appears as duality separation as optimality calculus as representation and approximation as stability this is an overview of the origin evolution and trends of convexity study of convexity in the sobolev institute was initiated by leonid kantorovich 19121986 and alexandr alexandrov 19121999 this talk is a part of their memory
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710.069
Deblurring of Motionally Averaged Images with Applications to Single-Particle Cryo-Electron Microscopy
This paper addresses the deconvolution of an image that has been obtained by superimposing many copies of an underlying unknown image of interest. The superposition is assumed to not be exact due to noise, and is described using an error distribution in position, orientation, or both. We assume that a good estimate of the error distribution is known. The most natural approach to take for the purely translational case is to apply the Fourier transform and use the classical convolution theorem together with a Weiner filter to invert. In the case of purely rotational deblurring, the similar Fourier analysis is applied. That is, for an blurred image function defined on polar coordinates, the Fourier series and the convolution theorem for the series can be applied. In the case of combinations of translational and rotational errors, the motion-group Fourier transform is used. In addition, for the three cases we present the alternative method using Hermite and Laguerre-Fourier expansion, which has a special property in Fourier transform. The problem that is solved here is motivated by one of the steps in the cryo-electron-tomographic reconstruction of biomolecular complexes such as viruses and ion channels.
math.NA
this paper addresses the deconvolution of an image that has been obtained by superimposing many copies of an underlying unknown image of interest the superposition is assumed to not be exact due to noise and is described using an error distribution in position orientation or both we assume that a good estimate of the error distribution is known the most natural approach to take for the purely translational case is to apply the fourier transform and use the classical convolution theorem together with a weiner filter to invert in the case of purely rotational deblurring the similar fourier analysis is applied that is for an blurred image function defined on polar coordinates the fourier series and the convolution theorem for the series can be applied in the case of combinations of translational and rotational errors the motiongroup fourier transform is used in addition for the three cases we present the alternative method using hermite and laguerrefourier expansion which has a special property in fourier transform the problem that is solved here is motivated by one of the steps in the cryoelectrontomographic reconstruction of biomolecular complexes such as viruses and ion channels
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710.0691
Pion mass difference from vacuum polarization
We calculate the electromagnetic contribution to the pion mass difference, $\Delta m^2_\pi=m^2_{\pi^+}-m^2_{\pi^0}$, in the chiral limit through the $VV-AA$ type vacuum polarization using Das-Guralnik-Mathur-Low-Young (DGMLY) sum rule. The calculation is made with two-flavors of dynamical overlap fermions on a $16^3\times 32$ lattice at $a\sim$0.12 fm. The exact chiral symmetry of the overlap fermion is essential to control the systematic error in the difference $VV-AA$. We obtain $\Delta m_\pi^2 = 1024(100) {\rm MeV^2}$ combining the lattice data with the perturbative contribution in the high momentum region evaluated by the operator product expansion. By analyzing the momentum dependence of the vacuum polarization, we also obtain pion decay constant $f_\pi$ and the low-energy constants $L_{10}^r$ in the chiral limit.
hep-lat hep-ph
we calculate the electromagnetic contribution to the pion mass difference delta m2_pim2_pim2_pi0 in the chiral limit through the vvaa type vacuum polarization using dasguralnikmathurlowyoung dgmly sum rule the calculation is made with twoflavors of dynamical overlap fermions on a 163times 32 lattice at asim012 fm the exact chiral symmetry of the overlap fermion is essential to control the systematic error in the difference vvaa we obtain delta m_pi2 1024100 rm mev2 combining the lattice data with the perturbative contribution in the high momentum region evaluated by the operator product expansion by analyzing the momentum dependence of the vacuum polarization we also obtain pion decay constant f_pi and the lowenergy constants l_10r in the chiral limit
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710.0692
Entanglement renormalization in fermionic systems
We demonstrate, in the context of quadratic fermion lattice models in one and two spatial dimensions, the potential of entanglement renormalization (ER) to define a proper real-space renormalization group transformation. Our results show, for the first time, the validity of the multi-scale entanglement renormalization ansatz (MERA) to describe ground states in two dimensions, even at a quantum critical point. They also unveil a connection between the performance of ER and the logarithmic violations of the boundary law for entanglement in systems with a one-dimensional Fermi surface. ER is recast in the language of creation/annihilation operators and correlation matrices.
quant-ph
we demonstrate in the context of quadratic fermion lattice models in one and two spatial dimensions the potential of entanglement renormalization er to define a proper realspace renormalization group transformation our results show for the first time the validity of the multiscale entanglement renormalization ansatz mera to describe ground states in two dimensions even at a quantum critical point they also unveil a connection between the performance of er and the logarithmic violations of the boundary law for entanglement in systems with a onedimensional fermi surface er is recast in the language of creationannihilation operators and correlation matrices
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710.0693
Scaling analysis of normal state properties of high-temperature superconductors
We propose a model-independent scaling method to study the physical properties of high-temperature superconductors in the normal state. We have analyze the experimental data of the c-axis resistivity, the in-plane resistivity, the Hall coefficient, the magnetic susceptibility, the spin-lattice relaxation rate, and the thermoelectric power using this method. It is shown that all these physical quantities exhibit good scaling behaviors, controlled purely by the pseudogap energy scale in the normal state. The doping dependence of the pseudogap obtained from this scaling analysis agrees with the experimental results of angle-resolved photoemission and other measurements. It sheds light on the understanding of the basic electronic structure of high-Tc oxides.
cond-mat.supr-con cond-mat.str-el
we propose a modelindependent scaling method to study the physical properties of hightemperature superconductors in the normal state we have analyze the experimental data of the caxis resistivity the inplane resistivity the hall coefficient the magnetic susceptibility the spinlattice relaxation rate and the thermoelectric power using this method it is shown that all these physical quantities exhibit good scaling behaviors controlled purely by the pseudogap energy scale in the normal state the doping dependence of the pseudogap obtained from this scaling analysis agrees with the experimental results of angleresolved photoemission and other measurements it sheds light on the understanding of the basic electronic structure of hightc oxides
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710.0694
Gain Stabilization of a Submillimeter SIS Heterodyne Receiver
We have designed a system to stabilize the gain of a submillimeter heterodyne receiver against thermal fluctuations of the mixing element. In the most sensitive heterodyne receivers, the mixer is usually cooled to 4 K using a closed-cycle cryocooler, which can introduce ~1% fluctuations in the physical temperature of the receiver components. We compensate for the resulting mixer conversion gain fluctuations by monitoring the physical temperature of the mixer and adjusting the gain of the intermediate frequency (IF) amplifier that immediately follows the mixer. This IF power stabilization scheme, developed for use at the Submillimeter Array (SMA), a submillimeter interferometer telescope on Mauna Kea in Hawaii, routinely achieves a receiver gain stability of 1 part in 6,000 (rms to mean). This is an order of magnitude improvement over the typical uncorrected stability of 1 part in a few hundred. Our gain stabilization scheme is a useful addition to SIS heterodyne receivers that are cooled using closed-cycle cryocoolers in which the 4 K temperature fluctuations tend to be the leading cause of IF power fluctuations.
astro-ph
we have designed a system to stabilize the gain of a submillimeter heterodyne receiver against thermal fluctuations of the mixing element in the most sensitive heterodyne receivers the mixer is usually cooled to 4 k using a closedcycle cryocooler which can introduce 1 fluctuations in the physical temperature of the receiver components we compensate for the resulting mixer conversion gain fluctuations by monitoring the physical temperature of the mixer and adjusting the gain of the intermediate frequency if amplifier that immediately follows the mixer this if power stabilization scheme developed for use at the submillimeter array sma a submillimeter interferometer telescope on mauna kea in hawaii routinely achieves a receiver gain stability of 1 part in 6000 rms to mean this is an order of magnitude improvement over the typical uncorrected stability of 1 part in a few hundred our gain stabilization scheme is a useful addition to sis heterodyne receivers that are cooled using closedcycle cryocoolers in which the 4 k temperature fluctuations tend to be the leading cause of if power fluctuations
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710.0695
Exciton spectroscopy of hexagonal boron nitride using non-resonant x-ray Raman scattering
We report non-resonant x-ray Raman scattering (XRS) measurements from hexagonal boron nitride for transferred momentum from 2 to 9 $\mathrm{\AA}^{-1}$ along directions both in and out of the basal plane. A symmetry-based argument, together with real-space full multiple scattering calculations of the projected density of states in the spherical harmonics basis, reveals that a strong pre-edge feature is a dominantly $Y_{10}$-type Frenkel exciton with no other \textit{s}-, \textit{p}-, or \textit{d}- components. This conclusion is supported by a second, independent calculation of the \textbf{q}-dependent XRS cross-section based on the Bethe-Salpeter equation.
cond-mat.mtrl-sci
we report nonresonant xray raman scattering xrs measurements from hexagonal boron nitride for transferred momentum from 2 to 9 mathrmaa1 along directions both in and out of the basal plane a symmetrybased argument together with realspace full multiple scattering calculations of the projected density of states in the spherical harmonics basis reveals that a strong preedge feature is a dominantly y_10type frenkel exciton with no other textits textitp or textitd components this conclusion is supported by a second independent calculation of the textbfqdependent xrs crosssection based on the bethesalpeter equation
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710.0696
The lowest modes around Gaussian solutions of tensor models and the general relativity
In the previous paper, the number distribution of the low-lying spectra around Gaussian solutions representing various dimensional fuzzy tori of a tensor model was numerically shown to be in accordance with the general relativity on tori. In this paper, I perform more detailed numerical analysis of the properties of the modes for two-dimensional fuzzy tori, and obtain conclusive evidences for the agreement. Under a proposed correspondence between the rank-three tensor in tensor models and the metric tensor in the general relativity, conclusive agreement is obtained between the profiles of the low-lying modes in a tensor model and the metric modes transverse to the general coordinate transformation. Moreover, the low-lying modes are shown to be well on a massless trajectory with quartic momentum dependence in the tensor model. This is in agreement with that the lowest momentum dependence of metric fluctuations in the general relativity will come from the R^2-term, since the R-term is topological in two dimensions. These evidences support the idea that the low-lying low-momentum dynamics around the Gaussian solutions of tensor models is described by the general relativity. I also propose a renormalization procedure for tensor models. A classical application of the procedure makes the patterns of the low-lying spectra drastically clearer, and suggests also the existence of massive trajectories.
hep-th gr-qc
in the previous paper the number distribution of the lowlying spectra around gaussian solutions representing various dimensional fuzzy tori of a tensor model was numerically shown to be in accordance with the general relativity on tori in this paper i perform more detailed numerical analysis of the properties of the modes for twodimensional fuzzy tori and obtain conclusive evidences for the agreement under a proposed correspondence between the rankthree tensor in tensor models and the metric tensor in the general relativity conclusive agreement is obtained between the profiles of the lowlying modes in a tensor model and the metric modes transverse to the general coordinate transformation moreover the lowlying modes are shown to be well on a massless trajectory with quartic momentum dependence in the tensor model this is in agreement with that the lowest momentum dependence of metric fluctuations in the general relativity will come from the r2term since the rterm is topological in two dimensions these evidences support the idea that the lowlying lowmomentum dynamics around the gaussian solutions of tensor models is described by the general relativity i also propose a renormalization procedure for tensor models a classical application of the procedure makes the patterns of the lowlying spectra drastically clearer and suggests also the existence of massive trajectories
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710.0697
Toroidalization of generating sequences in dimension two function fields of positive characteristic
We give a characteristic free proof of the main result of our previous paper (math.AC/0509697) concerning toroidalization of generating sequences of valuations in dimension two function fields. We show that when an extension of two dimensional algebraic regular local rings $R\subset S$ satisfies the conclusions of the Strong Monomialization theorem of Cutkosky and Piltant, the map between generating sequences in $R$ and $S$ has a toroidal structure.
math.AC math.AG
we give a characteristic free proof of the main result of our previous paper mathac0509697 concerning toroidalization of generating sequences of valuations in dimension two function fields we show that when an extension of two dimensional algebraic regular local rings rsubset s satisfies the conclusions of the strong monomialization theorem of cutkosky and piltant the map between generating sequences in r and s has a toroidal structure
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710.0698
Theoretical progress on V_us on lattice
Recent lattice studies on (semi-)leptonic kaon decays towards a precise determination of V_us are reviewed. Attention is given to recent unquenched calculations and consistency of their results with chiral perturbation theory.
hep-ph
recent lattice studies on semileptonic kaon decays towards a precise determination of v_us are reviewed attention is given to recent unquenched calculations and consistency of their results with chiral perturbation theory
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710.0699
Inevitability of Plate Tectonics on Super-Earths
The recent discovery of super-Earths (masses less or equal to 10 earth-masses) has initiated a discussion about conditions for habitable worlds. Among these is the mode of convection, which influences a planet's thermal evolution and surface conditions. On Earth, plate tectonics has been proposed as a necessary condition for life. Here we show, that super-Earths will also have plate tectonics. We demonstrate that as planetary mass increases, the shear stress available to overcome resistance to plate motion increases while the plate thickness decreases, thereby enhancing plate weakness. These effects contribute favorably to the subduction of the lithosphere, an essential component of plate tectonics. Moreover, uncertainties in achieving plate tectonics in the one earth-mass regime disappear as mass increases: super-Earths, even if dry, will exhibit plate tectonic behaviour.
astro-ph
the recent discovery of superearths masses less or equal to 10 earthmasses has initiated a discussion about conditions for habitable worlds among these is the mode of convection which influences a planets thermal evolution and surface conditions on earth plate tectonics has been proposed as a necessary condition for life here we show that superearths will also have plate tectonics we demonstrate that as planetary mass increases the shear stress available to overcome resistance to plate motion increases while the plate thickness decreases thereby enhancing plate weakness these effects contribute favorably to the subduction of the lithosphere an essential component of plate tectonics moreover uncertainties in achieving plate tectonics in the one earthmass regime disappear as mass increases superearths even if dry will exhibit plate tectonic behaviour
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710.07
Directional-dependent thermally activated motion of vortex bundles and theory of anomalous Hall effect in type-II conventional and high-Tc superconductors
The anomalous Hall effect for type-II conventional and high-Tc superconductors is studied based upon the theory of thermally activated motion of vortex bundles jumping over the directional-dependent energy barrier. It is shown that the Hall anomaly is universal for type-II conventional and high-Tc superconductors as well as for superconducting bulk materials and thin films, provided certain conditions are satisfied. We find that the directional-dependent potential barrier of the vortex bundles renormalizes the Hall and longitudinal resistivities, and Hall anomaly for superconductors is induced by the competition between the Magnus force and the random collective pinning force of the vortex bundle. We also find that the domain of anomalous Hall effect includes two regions: the region of thermally activated motion of the small vortex bundles and that of the large vortex bundles separated by the contour of the quasiorder-disorder first-order phase transition, or the peak effect of the vortex system. The Hall and longitudinal resistivities as functions of temperature as well as applied magnetic field have been calculated for type-II superconducting films and bulk materials. The conditions for occurring the double sign reversal or reentry phenomenon is also investigated. All the results are in agreement with the experiments.
cond-mat.supr-con
the anomalous hall effect for typeii conventional and hightc superconductors is studied based upon the theory of thermally activated motion of vortex bundles jumping over the directionaldependent energy barrier it is shown that the hall anomaly is universal for typeii conventional and hightc superconductors as well as for superconducting bulk materials and thin films provided certain conditions are satisfied we find that the directionaldependent potential barrier of the vortex bundles renormalizes the hall and longitudinal resistivities and hall anomaly for superconductors is induced by the competition between the magnus force and the random collective pinning force of the vortex bundle we also find that the domain of anomalous hall effect includes two regions the region of thermally activated motion of the small vortex bundles and that of the large vortex bundles separated by the contour of the quasiorderdisorder firstorder phase transition or the peak effect of the vortex system the hall and longitudinal resistivities as functions of temperature as well as applied magnetic field have been calculated for typeii superconducting films and bulk materials the conditions for occurring the double sign reversal or reentry phenomenon is also investigated all the results are in agreement with the experiments
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710.0701
The First Lunar Ranging Constraints on Gravity Sector SME Parameters
We present the first constraints on pure-gravity sector Standard-Model Extension (SME) parameters using Lunar Laser Ranging (LLR). LLR measures the round trip travel time of light between the Earth and the Moon. With 34+ years of LLR data, we have constrained six independent linear combinations of SME parameters at the level of $10^{-6}$ to $10^{-11}$. There is no evidence for Lorentz violation in the LLR dataset.
gr-qc astro-ph
we present the first constraints on puregravity sector standardmodel extension sme parameters using lunar laser ranging llr llr measures the round trip travel time of light between the earth and the moon with 34 years of llr data we have constrained six independent linear combinations of sme parameters at the level of 106 to 1011 there is no evidence for lorentz violation in the llr dataset
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710.0702
Testing for Lorentz Violation: Constraints on Standard-Model Extension Parameters via Lunar Laser Ranging
We present constraints on violations of Lorentz Invariance based on Lunar Laser Ranging (LLR) data. LLR measures the Earth-Moon separation by timing the round-trip travel of light between the two bodies, and is currently accurate to a few centimeters (parts in $10^{11}$ of the total distance). By analyzing archival LLR data under the Standard-Model Extension (SME) framework, we derived six observational constraints on dimensionless SME parameters that describe potential Lorentz-violation. We found no evidence for Lorentz violation at the $10^{-6}$ to $10^{-11}$ level in these parameters.
gr-qc astro-ph
we present constraints on violations of lorentz invariance based on lunar laser ranging llr data llr measures the earthmoon separation by timing the roundtrip travel of light between the two bodies and is currently accurate to a few centimeters parts in 1011 of the total distance by analyzing archival llr data under the standardmodel extension sme framework we derived six observational constraints on dimensionless sme parameters that describe potential lorentzviolation we found no evidence for lorentz violation at the 106 to 1011 level in these parameters
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710.0703
pQCD vs. AdS/CFT Tested by Heavy Quark Energy Loss
We predict the charm and bottom quark nuclear modification factors using weakly coupled pQCD and strongly coupled AdS/CFT drag methods. The log(pT/M_Q)/pT dependence of pQCD loss and the momentum independence of drag loss lead to different momentum dependencies for the R_{AA} predictions. This difference is enhanced by examining a new experimental observable, the double ratio of charm to bottom nuclear modification factors, R^{cb}=R^c_{AA}/R^b_{AA}. At LHC the weakly coupled theory predicts R^{cb} goes to 1; whereas the strongly coupled theory predicts R^{cb} .2 independent of pT. At RHIC the differences are less dramatic, as the production spectra are harder, but the drag formula is applicable to higher momenta, due to the lower temperature.
nucl-th
we predict the charm and bottom quark nuclear modification factors using weakly coupled pqcd and strongly coupled adscft drag methods the logptm_qpt dependence of pqcd loss and the momentum independence of drag loss lead to different momentum dependencies for the r_aa predictions this difference is enhanced by examining a new experimental observable the double ratio of charm to bottom nuclear modification factors rcbrc_aarb_aa at lhc the weakly coupled theory predicts rcb goes to 1 whereas the strongly coupled theory predicts rcb 2 independent of pt at rhic the differences are less dramatic as the production spectra are harder but the drag formula is applicable to higher momenta due to the lower temperature
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710.0704
Triage of the Sign Problem
We discuss the sign problem in QCD at nonzero chemical potential and its relation with chiral symmetry breaking and the spectrum of the Dirac operator using the framework of chiral random matrix theory. We show that the Banks-Casher formula is not valid for theories with a sign problem and has to be replaced by an alternative mechanism that is worked out in detail for QCD in one dimension at nonzero chemical potential.
hep-th
we discuss the sign problem in qcd at nonzero chemical potential and its relation with chiral symmetry breaking and the spectrum of the dirac operator using the framework of chiral random matrix theory we show that the bankscasher formula is not valid for theories with a sign problem and has to be replaced by an alternative mechanism that is worked out in detail for qcd in one dimension at nonzero chemical potential
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710.0705
Hopf Algebras and Congruence Subgroups
We prove that the kernel of the natural action of the modular group on the center of the Drinfel'd double of a semisimple Hopf algebra is a congruence subgroup. To do this, we introduce a class of generalized Frobenius-Schur indicators and endow it with an action of the modular group that is compatible with the original one.
math.RA hep-th math-ph math.MP math.QA math.RT
we prove that the kernel of the natural action of the modular group on the center of the drinfeld double of a semisimple hopf algebra is a congruence subgroup to do this we introduce a class of generalized frobeniusschur indicators and endow it with an action of the modular group that is compatible with the original one
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710.0706
Area-Preserving Surface Dynamics and S. Saito's Fixed Point Formula
We show that S. Saito's fixed point formula serves as a powerful tool for counting the number of isolated periodic points of an area-preserving surface map admitting periodic curves. His notion of periodic curves of types I and II plays a central role in our discussion. We establish a Shub-Sullivan type result on the stability of local indices under iterations of the map, the finiteness of the number of periodic curves of type II, and the absence of periodic curves of type I. Combined with these results, Saito's formula implies the existence of infinitely many isolated periodic points whose cardinality grows exponentially as period tends to infinity.
math.DS math.AG
we show that s saitos fixed point formula serves as a powerful tool for counting the number of isolated periodic points of an areapreserving surface map admitting periodic curves his notion of periodic curves of types i and ii plays a central role in our discussion we establish a shubsullivan type result on the stability of local indices under iterations of the map the finiteness of the number of periodic curves of type ii and the absence of periodic curves of type i combined with these results saitos formula implies the existence of infinitely many isolated periodic points whose cardinality grows exponentially as period tends to infinity
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710.0707
New branch of Kaluza-Klein compactification
We found a new branch of solutions in Freund-Rubin type flux compactifications. The geometry of these solutions is described as the external space which has a de Sitter symmetry and the internal space which is topologically spherical. However, it is not a simple form of dS_p x S^q but a warped product of de Sitter space and a deformed sphere. We explicitly constructed numerical solutions for a specific case with p=4 and q=4. We show that the new branch of solutions emanates from the marginally stable solution in the branch of dS_4 x S^4 solutions.
hep-th gr-qc
we found a new branch of solutions in freundrubin type flux compactifications the geometry of these solutions is described as the external space which has a de sitter symmetry and the internal space which is topologically spherical however it is not a simple form of ds_p x sq but a warped product of de sitter space and a deformed sphere we explicitly constructed numerical solutions for a specific case with p4 and q4 we show that the new branch of solutions emanates from the marginally stable solution in the branch of ds_4 x s4 solutions
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710.0708
A characterization of all equilateral triangles in \Bbb Z^3
This paper is a continuation of previous work of the authors. We extend one of the theorems that gave a way to construct equilateral triangles whose vertices have integer coordinates to the general situation. An approximate extrapolation formula for the sequence ET(n) of all equilateral triangles with vertices in $\{0,1,2,...,n\}^3$ (A 102698) is given and the asymptotic behavior of this sequence is analyzed.
math.NT
this paper is a continuation of previous work of the authors we extend one of the theorems that gave a way to construct equilateral triangles whose vertices have integer coordinates to the general situation an approximate extrapolation formula for the sequence etn of all equilateral triangles with vertices in 012n3 a 102698 is given and the asymptotic behavior of this sequence is analyzed
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710.0709
Superstring vertex operators in type IIB matrix model
We clarify the relation between the vertex operators in type IIB matrix model and superstring. Green-Schwarz light-cone closed superstring theory is obtained from IIB matrix model on two dimensional noncommutative backgrounds. Superstring vertex operators should be reproduced from those of IIB matrix model through this connection. Indeed, we confirm that supergravity vertex operators in IIB matrix model on the two dimensional backgrounds reduce to those in superstring theory. Noncommutativity plays an important role in our identification. Through this correspondence, we can reproduce superstring scattering amplitudes from IIB matrix model.
hep-th
we clarify the relation between the vertex operators in type iib matrix model and superstring greenschwarz lightcone closed superstring theory is obtained from iib matrix model on two dimensional noncommutative backgrounds superstring vertex operators should be reproduced from those of iib matrix model through this connection indeed we confirm that supergravity vertex operators in iib matrix model on the two dimensional backgrounds reduce to those in superstring theory noncommutativity plays an important role in our identification through this correspondence we can reproduce superstring scattering amplitudes from iib matrix model
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710.071
Non-perturbative renormalization of four-quark operators and B_K with Schroedinger functional scheme in quenched domain-wall QCD
We present non-perturbative renormalization factors for $\Delta S=2$ four-quark operators in quenched domain-wall QCD using the Schroedinger functional method. Non-perturbative renormalization factor for $B_K$ is evaluated at hadronic scale. Combined with the non-perturbative RG running obtained by the Alpha collaboration, our result yields renormalization factor which converts lattice bare $B_K$ to the renormalization group invariant one. We apply the renormalization factor to bare $B_K$ previously obtained by the CP-PACS collaboration with the quenched domain-wall QCD(DWQCD). We compare our result with previous ones obtained by perturbative renormalization factors, different renormalization schemes or different quark actions. We also show that chiral symmetry breaking effects in the renormalization factor are numerically small.
hep-lat
we present nonperturbative renormalization factors for delta s2 fourquark operators in quenched domainwall qcd using the schroedinger functional method nonperturbative renormalization factor for b_k is evaluated at hadronic scale combined with the nonperturbative rg running obtained by the alpha collaboration our result yields renormalization factor which converts lattice bare b_k to the renormalization group invariant one we apply the renormalization factor to bare b_k previously obtained by the cppacs collaboration with the quenched domainwall qcddwqcd we compare our result with previous ones obtained by perturbative renormalization factors different renormalization schemes or different quark actions we also show that chiral symmetry breaking effects in the renormalization factor are numerically small
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710.0711
Canes Venatici I cloud of galaxies seen in the H-alpha line
We present results of H-alpha imaging for 42 galaxies in the nearby low-density cloud Canes Venatici I populated mainly by late-type objects. Estimates of the H-alpha flux and integrated star formation rate (SFR) are now available for all 78 known members of this scattered system, spanning a large range in luminosity, surface brightness, HI content and SFR. Distributions of the CVnI galaxies versus their SFR, blue absolute magnitude and total hydrogen mass are given in comparison with those for a population of the nearby virialized group around M81. We found no essential correlation between star formation activity in a galaxy and its density environment. A bulk of CVnI galaxies had enough time to generate their baryon mass with the observed SFR. Most of them possess also a supply of gas sufficient to maintain their observed SFR's during the next Hubble time.
astro-ph
we present results of halpha imaging for 42 galaxies in the nearby lowdensity cloud canes venatici i populated mainly by latetype objects estimates of the halpha flux and integrated star formation rate sfr are now available for all 78 known members of this scattered system spanning a large range in luminosity surface brightness hi content and sfr distributions of the cvni galaxies versus their sfr blue absolute magnitude and total hydrogen mass are given in comparison with those for a population of the nearby virialized group around m81 we found no essential correlation between star formation activity in a galaxy and its density environment a bulk of cvni galaxies had enough time to generate their baryon mass with the observed sfr most of them possess also a supply of gas sufficient to maintain their observed sfrs during the next hubble time
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710.0712
Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores
We investigate molecular evolution in a star-forming core that is initially a hydrostatic starless core and collapses to form a low-mass protostar. The results of a one-dimensional radiation-hydrodynamics calculation are adopted as a physical model of the core. We first derive radii at which CO and large organic species sublimate. CO sublimation in the central region starts shortly before the formation of the first hydrostatic core. When the protostar is born, the CO sublimation radius extends to 100 AU, and the region inside $\lesssim 10$ AU is hotter than 100 K, at which some large organic species evaporate. We calculate the temporal variation of physical parameters in infalling shells, in which the molecular evolution is solved using an updated gas-grain chemical model to derive the spatial distribution of molecules in a protostellar core. The shells pass through the warm region of $10 -100$ K in several $\times$ $10^4$ yr, and fall into the central star $\sim 100$ yr after they enter the region where $T \gtrsim 100$ K. We find that large organic species are formed mainly via grain-surface reactions at temperatures of $20 -40$ K and then desorbed into the gas-phase at their sublimation temperatures. Carbon-chain species can be formed by a combination of gas-phase reactions and grain-surface reactions following the sublimation of CH$_4$. Our model also predicts that CO$_2$ is more abundant in isolated cores, while gas-phase large organic species are more abundant in cores embedded in ambient clouds.
astro-ph
we investigate molecular evolution in a starforming core that is initially a hydrostatic starless core and collapses to form a lowmass protostar the results of a onedimensional radiationhydrodynamics calculation are adopted as a physical model of the core we first derive radii at which co and large organic species sublimate co sublimation in the central region starts shortly before the formation of the first hydrostatic core when the protostar is born the co sublimation radius extends to 100 au and the region inside lesssim 10 au is hotter than 100 k at which some large organic species evaporate we calculate the temporal variation of physical parameters in infalling shells in which the molecular evolution is solved using an updated gasgrain chemical model to derive the spatial distribution of molecules in a protostellar core the shells pass through the warm region of 10 100 k in several times 104 yr and fall into the central star sim 100 yr after they enter the region where t gtrsim 100 k we find that large organic species are formed mainly via grainsurface reactions at temperatures of 20 40 k and then desorbed into the gasphase at their sublimation temperatures carbonchain species can be formed by a combination of gasphase reactions and grainsurface reactions following the sublimation of ch_4 our model also predicts that co_2 is more abundant in isolated cores while gasphase large organic species are more abundant in cores embedded in ambient clouds
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710.0713
Corrections to the running of gauge couplings due to quantum gravity
Concerning the gravitational corrections to the running of gauge couplings two different results were reported. Some authors claim that gravitational correction at the one-loop level indicates an interesting effect of universal gravitational decreasing of gauge couplings, that is, gravitational correction works universally in the direction of asymptotic freedom no matter how the gauge coupling behaves without gravity, while others reject the presence of gravitational correction at the one-loop level at all. Being these calculations done in the framework of an effective field theory approach to general relativity, we wanted to draw attention to a recently discovered profound quantum-gravitational effect of space-time dimension running that inevitably affects the running of gauge couplings. The running of space-time dimension indicating gradual reduction of dimension as one gets into smaller scales acts on the coupling constants in the direction of asymptotic freedom and therefore in any case manifests the plausibility of this quantum-gravitational effect. Curiously enough, the results are also in perfect quantitative agreement with those of Robinson and Wilczek.
hep-th gr-qc hep-ph
concerning the gravitational corrections to the running of gauge couplings two different results were reported some authors claim that gravitational correction at the oneloop level indicates an interesting effect of universal gravitational decreasing of gauge couplings that is gravitational correction works universally in the direction of asymptotic freedom no matter how the gauge coupling behaves without gravity while others reject the presence of gravitational correction at the oneloop level at all being these calculations done in the framework of an effective field theory approach to general relativity we wanted to draw attention to a recently discovered profound quantumgravitational effect of spacetime dimension running that inevitably affects the running of gauge couplings the running of spacetime dimension indicating gradual reduction of dimension as one gets into smaller scales acts on the coupling constants in the direction of asymptotic freedom and therefore in any case manifests the plausibility of this quantumgravitational effect curiously enough the results are also in perfect quantitative agreement with those of robinson and wilczek
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710.0714
Light-front quark model analysis of heavy meson radiative decays
We present the magnetic dipole($M1$) transitions $V\to P\gamma$ of various heavy-flavored mesons such as $(D,D^*,D_s,D^{*}_s,\eta_c, J/\psi)$ and $(B,B^*,B_s,B^*_s,\eta_b,\Upsilon)$ using the light-front quark model constrained by the variational principle for the QCD-motivated effective Hamiltonian. The weak decay constants of heavy mesons and the decay widths for $V\to P\gamma$ are calculated. The radiative decay for $\Upsilon\to\eta_{b}\gamma$ process is found to be very helpful to determine the unmeasured mass of $\eta_b$. Our numerical results are overall in good agreement with the available experimental data as well as other theoretical model calculations.
hep-ph
we present the magnetic dipolem1 transitions vto pgamma of various heavyflavored mesons such as ddd_sd_seta_c jpsi and bbb_sb_seta_bupsilon using the lightfront quark model constrained by the variational principle for the qcdmotivated effective hamiltonian the weak decay constants of heavy mesons and the decay widths for vto pgamma are calculated the radiative decay for upsilontoeta_bgamma process is found to be very helpful to determine the unmeasured mass of eta_b our numerical results are overall in good agreement with the available experimental data as well as other theoretical model calculations
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710.0715
Effect of Ti4+ substitution on structural, transport and magnetic properties of La0.67Sr0.33Mn1-xTixO3
La$_{0.67}$Sr$_{0.33}$Mn$_{1-x}$Ti$_x$O$_{3}$ ($0 \le x \le 0.20$) polycrystalline materials are prepared by employing lower annealing temperature compared to the temperatures reported for the materials of the same composition. The transport and magnetic properties of these materials are significantly different from those compounds prepared at higher annealing temperature. Samples with $x < 0.10$, show metal-insulator transition and those with $x \ge 0.10$ exhibit insulating behavior over the entire temperature range investigated. A gradual transition occurs from ferromagnetic-metallic state to ferromagnetic-insulator state with increasing Ti substitution. Lattice parameters and bond lengths of Mn and its near neighbours however do not change appreciably with the dopant content $x$ in these materials. It is shown that Ti$^{4+}$ doping in the low temperature annealed samples is inhomogeneous resulting in isolated Mn rich regions that are connected by a variable range hopping polaron.
cond-mat.str-el cond-mat.mtrl-sci
la_067sr_033mn_1xti_xo_3 0 le x le 020 polycrystalline materials are prepared by employing lower annealing temperature compared to the temperatures reported for the materials of the same composition the transport and magnetic properties of these materials are significantly different from those compounds prepared at higher annealing temperature samples with x 010 show metalinsulator transition and those with x ge 010 exhibit insulating behavior over the entire temperature range investigated a gradual transition occurs from ferromagneticmetallic state to ferromagneticinsulator state with increasing ti substitution lattice parameters and bond lengths of mn and its near neighbours however do not change appreciably with the dopant content x in these materials it is shown that ti4 doping in the low temperature annealed samples is inhomogeneous resulting in isolated mn rich regions that are connected by a variable range hopping polaron
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710.0716
The Boltzmann-Grad limit of the periodic Lorentz gas in two space dimensions
The periodic Lorentz gas is the dynamical system corresponding to the free motion of a point particle in a periodic system of fixed spherical obstacles of radius $r$ centered at the integer points, assuming all collisions of the particle with the obstacles to be elastic. In this Note, we study this motion on time intervals of order $1/r$ and in the limit as $r\to 0^+$, in the case of two space dimensions.
math.DS math-ph math.MP
the periodic lorentz gas is the dynamical system corresponding to the free motion of a point particle in a periodic system of fixed spherical obstacles of radius r centered at the integer points assuming all collisions of the particle with the obstacles to be elastic in this note we study this motion on time intervals of order 1r and in the limit as rto 0 in the case of two space dimensions
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710.0717
Ultrafast coelectrophoretic fluorescent staining of proteins with carbocyanines
Protein detection on SDS gels or on 2-D gels must combine several features, such as sensitivity, homogeneity from one protein to another, speed, low cost, and user-friendliness. For some applications, it is also interesting to have a nonfixing stain, so that proteins can be mobilized from the gel for further use (electroelution, blotting). We show here that coelectrophoretic staining by fluorophores of the oxacarbocyanine family, and especially diheptyloxacarbocyanine, offers several positive features. The sensitivity is intermediate between the one of colloidal CBB and the one of fluroescent ruthenium complexes. Detection is achieved within 1 h after the end of the electrophoretic process and does not use any fixing or toxic agent. The fluorescent SDS-carbocyanine-protein complexes can be detected either with a laser scanner with an excitation wavelength of 488 nm or with a UV table operating at 302 nm. Excellent sequence coverage in subsequent MS analysis of proteolytic peptides is also achieved with this detection method.
q-bio.GN
protein detection on sds gels or on 2d gels must combine several features such as sensitivity homogeneity from one protein to another speed low cost and userfriendliness for some applications it is also interesting to have a nonfixing stain so that proteins can be mobilized from the gel for further use electroelution blotting we show here that coelectrophoretic staining by fluorophores of the oxacarbocyanine family and especially diheptyloxacarbocyanine offers several positive features the sensitivity is intermediate between the one of colloidal cbb and the one of fluroescent ruthenium complexes detection is achieved within 1 h after the end of the electrophoretic process and does not use any fixing or toxic agent the fluorescent sdscarbocyanineprotein complexes can be detected either with a laser scanner with an excitation wavelength of 488 nm or with a uv table operating at 302 nm excellent sequence coverage in subsequent ms analysis of proteolytic peptides is also achieved with this detection method
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710.0718
Exchange-energy functionals for finite two-dimensional systems
Implicit and explicit density functionals for the exchange energy in finite two-dimensional systems are developed following the approach of Becke and Roussel [Phys. Rev. A 39, 3761 (1989)]. Excellent agreement for the exchange-hole potentials and exchange energies is found when compared with the exact-exchange reference data for the two-dimensional uniform electron gas and few-electron quantum dots, respectively. Thereby, this work significantly improves the availability of approximate density functionals for dealing with electrons in quasi-two-dimensional structures, which have various applications in semiconductor nanotechnology.
cond-mat.str-el
implicit and explicit density functionals for the exchange energy in finite twodimensional systems are developed following the approach of becke and roussel phys rev a 39 3761 1989 excellent agreement for the exchangehole potentials and exchange energies is found when compared with the exactexchange reference data for the twodimensional uniform electron gas and fewelectron quantum dots respectively thereby this work significantly improves the availability of approximate density functionals for dealing with electrons in quasitwodimensional structures which have various applications in semiconductor nanotechnology
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710.0719
Nuclear Structure Relevant to Neutrinoless Double Beta Decay: 76Ge and 76Se
The possibility of observing neutrinoless double beta decay offers the opportunity of determining the neutrino mass IF the nuclear matrix element were known. Theoretical calculations are uncertain and measurements of the occupations of valence orbits by nucleons active in the decay can be important. The occupation of valence neutron orbits in the ground states of 76Ge and 76Se were determined by precisely measuring cross sections for both neutron-adding and removing transfer reactions. Our results indicate that the Fermi surface is much more diffuse than in theoretical (QRPA) calculations. We find that the populations of at least three orbits change significantly between these two ground states while in the calculations the changes are confined primarily to one orbit.
nucl-ex
the possibility of observing neutrinoless double beta decay offers the opportunity of determining the neutrino mass if the nuclear matrix element were known theoretical calculations are uncertain and measurements of the occupations of valence orbits by nucleons active in the decay can be important the occupation of valence neutron orbits in the ground states of 76ge and 76se were determined by precisely measuring cross sections for both neutronadding and removing transfer reactions our results indicate that the fermi surface is much more diffuse than in theoretical qrpa calculations we find that the populations of at least three orbits change significantly between these two ground states while in the calculations the changes are confined primarily to one orbit
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710.072
The tensor of interaction of a two-level system with an arbitrary strain field
The interaction between two-level systems (TLS) and strain fields in a solid is contained in the diagonal matrix element of the interaction hamiltonian, $\delta$, which, in general, has the expression $\delta=2[\gamma]:[S]$, with the tensor $[\gamma]$ describing the TLS ``deformability'' and $[S]$ being the symmetric strain tensor. We construct $[\gamma]$ on very general grounds, by associating to the TLS two objects: a direction, $\hat\bt$, and a forth rank tensor of coupling constants, $[[R]]$. Based on the method of construction and on the invariance of the expression of $\delta$ with respect to the symmetry transformation of the solid, we conclude that $[[R]]$ has the same structure as the tensor of stiffness constants, $[[c]]$, from elasticity theory. In particular, if the solid is isotropic, $[[R]]$ has only two independent parameters, which are the equivalent of the Lam\'e constants. Employing this model we calculate the absorption and emission rates of phonons on TLSs and show that in isotropic solids, on average, the longitudinal phonons interact stronger with the TLSs than the transversal ones, as it is observed in experiments. We also show that in isotropic solids, a transversal wave leaves unperturbed all the TLSs with the direction contained in one of the two planes that are perpendicular either to the wave propagation direction or to the polarization direction and that a longitudinal strain applied to the solid polarises the TLS ensemble.
cond-mat.dis-nn cond-mat.mtrl-sci
the interaction between twolevel systems tls and strain fields in a solid is contained in the diagonal matrix element of the interaction hamiltonian delta which in general has the expression delta2gammas with the tensor gamma describing the tls deformability and s being the symmetric strain tensor we construct gamma on very general grounds by associating to the tls two objects a direction hatbt and a forth rank tensor of coupling constants r based on the method of construction and on the invariance of the expression of delta with respect to the symmetry transformation of the solid we conclude that r has the same structure as the tensor of stiffness constants c from elasticity theory in particular if the solid is isotropic r has only two independent parameters which are the equivalent of the lame constants employing this model we calculate the absorption and emission rates of phonons on tlss and show that in isotropic solids on average the longitudinal phonons interact stronger with the tlss than the transversal ones as it is observed in experiments we also show that in isotropic solids a transversal wave leaves unperturbed all the tlss with the direction contained in one of the two planes that are perpendicular either to the wave propagation direction or to the polarization direction and that a longitudinal strain applied to the solid polarises the tls ensemble
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710.0721
Noncommutative families of instantons
We construct $\theta$-deformations of the classical groups SL(2,H) and Sp(2). Coacting on the basic instanton on a noncommutative four-sphere $S^4_\theta$, we construct a noncommutative family of instantons of charge 1. The family is parametrized by the quantum quotient of $SL_\theta(2,H)$ by $Sp_\theta(2)$.
math.QA hep-th math-ph math.MP
we construct thetadeformations of the classical groups sl2h and sp2 coacting on the basic instanton on a noncommutative foursphere s4_theta we construct a noncommutative family of instantons of charge 1 the family is parametrized by the quantum quotient of sl_theta2h by sp_theta2
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710.0722
Boost symmetry in the Quantum Gravity sector
We perform a canonical quantization of gravity in a second-order formulation, taking as configuration variables those describing a 4-bein, not adapted to the space-time splitting. We outline how, neither if we fix the Lorentz frame before quantizing, nor if we perform no gauge fixing at all, is invariance under boost transformations affected by the quantization.
gr-qc
we perform a canonical quantization of gravity in a secondorder formulation taking as configuration variables those describing a 4bein not adapted to the spacetime splitting we outline how neither if we fix the lorentz frame before quantizing nor if we perform no gauge fixing at all is invariance under boost transformations affected by the quantization
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710.0723
Uncertainty Relation for the Discrete Fourier Transform
We derive an uncertainty relation for two unitary operators which obey a commutation relation of the form UV=exp[i phi] VU. Its most important application is to constrain how much a quantum state can be localised simultaneously in two mutually unbiased bases related by a Discrete Fourier Transform. It provides an uncertainty relation which smoothly interpolates between the well known cases of the Pauli operators in 2 dimensions and the continuous variables position and momentum. This work also provides an uncertainty relation for modular variables, and could find applications in signal processing. In the finite dimensional case the minimum uncertainty states, discrete analogues of coherent and squeezed states, are minimum energy solutions of Harper's equation, a discrete version of the Harmonic oscillator equation.
quant-ph
we derive an uncertainty relation for two unitary operators which obey a commutation relation of the form uvexpi phi vu its most important application is to constrain how much a quantum state can be localised simultaneously in two mutually unbiased bases related by a discrete fourier transform it provides an uncertainty relation which smoothly interpolates between the well known cases of the pauli operators in 2 dimensions and the continuous variables position and momentum this work also provides an uncertainty relation for modular variables and could find applications in signal processing in the finite dimensional case the minimum uncertainty states discrete analogues of coherent and squeezed states are minimum energy solutions of harpers equation a discrete version of the harmonic oscillator equation
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710.0724
The thermodynamic limit for fractional exclusion statistics
I discuss Haldane's concept of generalised exclusion statistics (Phys. Rev. Lett. {\bf 67}, 937, 1991) and I show that it leads to inconsistencies in the calculation of the particle distribution that maximizes the partition function. These inconsistencies appear when mutual exclusion statistics is manifested between different subspecies of particles in the system. In order to eliminate these inconsistencies, I introduce new mutual exclusion statistics parameters, which are proportional to the dimension of the Hilbert sub-space on which they act. These new definitions lead to properly defined particle distributions and thermodynamic properties. In another paper (arXiv:0710.0728) I show that fractional exclusion statistics manifested in general systems with interaction have these, physically consistent, statistics parameters.
cond-mat.stat-mech cond-mat.mes-hall
i discuss haldanes concept of generalised exclusion statistics phys rev lett bf 67 937 1991 and i show that it leads to inconsistencies in the calculation of the particle distribution that maximizes the partition function these inconsistencies appear when mutual exclusion statistics is manifested between different subspecies of particles in the system in order to eliminate these inconsistencies i introduce new mutual exclusion statistics parameters which are proportional to the dimension of the hilbert subspace on which they act these new definitions lead to properly defined particle distributions and thermodynamic properties in another paper arxiv07100728 i show that fractional exclusion statistics manifested in general systems with interaction have these physically consistent statistics parameters
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710.0725
Near-Constant Mean Curvature Solutions of the Einstein Constraint Equations with Non-Negative Yamabe Metrics
We show that sets of conformal data on closed manifolds with the metric in the positive or zero Yamabe class, and with the gradient of the mean curvature function sufficiently small, are mapped to solutions of the Einstein constraint equations. This result extends previous work which required the conformal metric to be in the negative Yamabe class, and required the mean curvature function to be nonzero.
gr-qc
we show that sets of conformal data on closed manifolds with the metric in the positive or zero yamabe class and with the gradient of the mean curvature function sufficiently small are mapped to solutions of the einstein constraint equations this result extends previous work which required the conformal metric to be in the negative yamabe class and required the mean curvature function to be nonzero
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710.0726
Distinguishing SUSY scenarios using \tau polarisation and \tilde\chi^0_1 Dark Matter
We discuss first a method of measuring $\tau$ polarisation at the ILC using the 1--prong hadronic decays of the $\tau$. We then show in this contribution how a study of the $\tilde \tau$ sector and particularly use of decay $\tau$ polarisation can offer a very good handle for distinguishing between mSUGRA and a SUSY-GUT scenario, both of which can give rise to appropriate Dark Matter.
hep-ph
we discuss first a method of measuring tau polarisation at the ilc using the 1prong hadronic decays of the tau we then show in this contribution how a study of the tilde tau sector and particularly use of decay tau polarisation can offer a very good handle for distinguishing between msugra and a susygut scenario both of which can give rise to appropriate dark matter
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710.0727
The afterglow onset for GRB060418 and GRB060607A
Gamma-ray burst are thought to be produced by highly relativistic outflows. Although upper and lower limits for the outflow initial Lorentz factor $\Gamma_0$ are available, observational efforts to derive a direct determination of $\Gamma_0$ have so far failed or provided ambiguous results. As a matter of fact, the shape of the early-time afterglow light curve is strongly sensitive on $\Gamma_0$ which determines the time of the afterglow peak, i.e. when the outflow and the shocked circumburst material share a comparable amount of energy. We now comment early-time observations of the near-infrared afterglows of GRB 060418 and GRB 060607A performed by the REM robotic telescope. For both events, the afterglow peak was singled out and allowed us to determine the initial fireball Lorentz, $\Gamma_0\sim 400$.
astro-ph
gammaray burst are thought to be produced by highly relativistic outflows although upper and lower limits for the outflow initial lorentz factor gamma_0 are available observational efforts to derive a direct determination of gamma_0 have so far failed or provided ambiguous results as a matter of fact the shape of the earlytime afterglow light curve is strongly sensitive on gamma_0 which determines the time of the afterglow peak ie when the outflow and the shocked circumburst material share a comparable amount of energy we now comment earlytime observations of the nearinfrared afterglows of grb 060418 and grb 060607a performed by the rem robotic telescope for both events the afterglow peak was singled out and allowed us to determine the initial fireball lorentz gamma_0sim 400
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710.0728
Fractional exclusion statistics in general systems with interaction
I show that fractional exclusion statistics (FES) is manifested in general interacting systems and I calculate the exclusion statistics parameters. Most importantly, I show that the mutual exclusion statistics parameters--when the presence of particles in one Hilbert space influences the dimension of another Hilbert space--are proportional to the dimension of the Hilbert space on which they act. This result, although surprising and different from the usual way of understanding the FES, renders this statistics consistent and valid in the thermodynamic limit, in accordance with the conjucture introduced in J. Phys. A: Math. Theor. 40, F1013 (2007).
cond-mat.stat-mech cond-mat.mes-hall
i show that fractional exclusion statistics fes is manifested in general interacting systems and i calculate the exclusion statistics parameters most importantly i show that the mutual exclusion statistics parameterswhen the presence of particles in one hilbert space influences the dimension of another hilbert spaceare proportional to the dimension of the hilbert space on which they act this result although surprising and different from the usual way of understanding the fes renders this statistics consistent and valid in the thermodynamic limit in accordance with the conjucture introduced in j phys a math theor 40 f1013 2007
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710.0729
Semileptonic decays of heavy-light pseudoscalar mesons
I discuss the results of a recent quenched lattice calculation of the two independent form factors parametrizing the semileptonic decays between heavy-light pseudoscalar mesons. The differential decay rate of the process B --> D l nu has been calculated at non vanishing momentum transfer both in the case of the light leptons, l=e,mu, and in the case of a non vanishing lepton mass, l=tau.
hep-lat
i discuss the results of a recent quenched lattice calculation of the two independent form factors parametrizing the semileptonic decays between heavylight pseudoscalar mesons the differential decay rate of the process b d l nu has been calculated at non vanishing momentum transfer both in the case of the light leptons lemu and in the case of a non vanishing lepton mass ltau
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710.073
Fractional Charge and Quantized Current in the Quantum Spin Hall State
A profound manifestation of topologically non-trivial states of matter is the occurrence of fractionally charged elementary excitations. The quantum spin Hall insulator state is a fundamentally novel quantum state of matter that exists at zero external magnetic field. In this work, we show that a magnetic domain wall at the edge of the quantum spin Hall insulator carries one half of the unit of electron charge, and we propose an experiment to directly measure this fractional charge on an individual basis. We also show that as an additional consequence, a rotating magnetic field can induce a quantized dc electric current, and vice versa.
cond-mat.mes-hall
a profound manifestation of topologically nontrivial states of matter is the occurrence of fractionally charged elementary excitations the quantum spin hall insulator state is a fundamentally novel quantum state of matter that exists at zero external magnetic field in this work we show that a magnetic domain wall at the edge of the quantum spin hall insulator carries one half of the unit of electron charge and we propose an experiment to directly measure this fractional charge on an individual basis we also show that as an additional consequence a rotating magnetic field can induce a quantized dc electric current and vice versa
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710.0731
Symplectic resolutions, Lefschetz property and formality
We introduce a method to resolve a symplectic orbifold into a smooth symplectic manifold. Then we study how the formality and the Lefschetz property of the symplectic resolution are compared with that of the symplectic orbifold. We also study the formality of the symplectic blow-up of a symplectic orbifold along symplectic submanifolds disjoint from the orbifold singularities. This allows us to construct the first example of a simply connected compact symplectic manifold of dimension 8 which satisfies the Lefschetz property but is not formal, therefore giving a counter-example to a conjecture of Babenko and Taimanov.
math.SG math.AT math.DG
we introduce a method to resolve a symplectic orbifold into a smooth symplectic manifold then we study how the formality and the lefschetz property of the symplectic resolution are compared with that of the symplectic orbifold we also study the formality of the symplectic blowup of a symplectic orbifold along symplectic submanifolds disjoint from the orbifold singularities this allows us to construct the first example of a simply connected compact symplectic manifold of dimension 8 which satisfies the lefschetz property but is not formal therefore giving a counterexample to a conjecture of babenko and taimanov
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710.0732
Comment on ``Coherent Control of a V-Type Three-Level System in a Single Quantum Dot''
This is a Comment on Phys. Rev. Lett., {\bf 95}, 187404 (2005)
cond-mat.mtrl-sci
this is a comment on phys rev lett bf 95 187404 2005
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710.0733
Total control over ultracold interactions via electric and magnetic fields
The scattering length is commonly used to characterize the strength of ultracold atomic interactions, since it is the leading parameter in the low-energy expansion of the scattering phase shift. Its value can be modified via a magnetic field, by using a Feshbach resonance. However, the effective range term, which is the second parameter in the phase shift expansion, determines the width of the resonance and gives rise to important properties of ultracold gases. Independent control over this parameter is not possible by using a magnetic field only. We demonstrate that a combination of magnetic and electric fields can be used to get independent control over both parameters, which leads to full control over elastic ultracold interactions.
physics.atom-ph cond-mat.other
the scattering length is commonly used to characterize the strength of ultracold atomic interactions since it is the leading parameter in the lowenergy expansion of the scattering phase shift its value can be modified via a magnetic field by using a feshbach resonance however the effective range term which is the second parameter in the phase shift expansion determines the width of the resonance and gives rise to important properties of ultracold gases independent control over this parameter is not possible by using a magnetic field only we demonstrate that a combination of magnetic and electric fields can be used to get independent control over both parameters which leads to full control over elastic ultracold interactions
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710.0734
Obstruction theory on 8-manifolds
This note gives a uniform, self-contained, and fairly direct approach to a variety of obstruction-theoretic problems on 8-manifolds. We give necessary and sufficient cohomological critera for the existence of almost complex and almost quaternionic structures on the tangent bundle and for the reduction of the structure group to U(3) by the homomorphism U(3) --> O(8) given by the Lie algebra representation of PU(3).
math.AT math.GT
this note gives a uniform selfcontained and fairly direct approach to a variety of obstructiontheoretic problems on 8manifolds we give necessary and sufficient cohomological critera for the existence of almost complex and almost quaternionic structures on the tangent bundle and for the reduction of the structure group to u3 by the homomorphism u3 o8 given by the lie algebra representation of pu3
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710.0735
Critical points of quadratic renormalizations of random variables and phase transitions of disordered polymer models on diamond lattices
We study the wetting transition and the directed polymer delocalization transition on diamond hierarchical lattices.These two phase transitions with frozen disorder correspond to the critical points of quadratic renormalizations of the partition function.(These exact renormalizations on diamond lattices can also be considered as approximate Migdal-Kadanoff renormalizations for hypercubic lattices). In terms of the rescaled partition function $z=Z/Z_{typ}$,we find that the critical point corresponds to a fixed point distribution with a power-law tail $P_c(z) \sim \Phi(\ln z)/z^{1+\mu}$ as $z \to +\infty$ (up to some sub-leading logarithmic correction $\Phi(\ln z)$), so that all moments $z^{n}$ with $n>\mu$ diverge. For the wetting transition, the first moment diverges $\bar{z}=+\infty$ (case $0<\mu<1$), and the critical temperature is strictly below the annealed temperature $T_c<T_{ann}$. For the directed polymer case, the second moment diverges $\bar{z^2}=+\infty$ (case $1<\mu<2$), and the critical temperature is strictly below the exactly known transition temperature $T_2$ of the second moment.We then consider the correlation length exponent $\nu$ :the linearized renormalization around the fixed point distribution coincides with the transfer matrix describing a directed polymer on the Cayley tree, but the random weights determined by the fixed point distribution $P_c(z)$ are broadly distributed. This induces some changes in the travelling wave solutions with respect to the usual case of more narrow distributions.
cond-mat.dis-nn
we study the wetting transition and the directed polymer delocalization transition on diamond hierarchical latticesthese two phase transitions with frozen disorder correspond to the critical points of quadratic renormalizations of the partition functionthese exact renormalizations on diamond lattices can also be considered as approximate migdalkadanoff renormalizations for hypercubic lattices in terms of the rescaled partition function zzz_typwe find that the critical point corresponds to a fixed point distribution with a powerlaw tail p_cz sim philn zz1mu as z to infty up to some subleading logarithmic correction philn z so that all moments zn with nmu diverge for the wetting transition the first moment diverges barzinfty case 0mu1 and the critical temperature is strictly below the annealed temperature t_ct_ann for the directed polymer case the second moment diverges barz2infty case 1mu2 and the critical temperature is strictly below the exactly known transition temperature t_2 of the second momentwe then consider the correlation length exponent nu the linearized renormalization around the fixed point distribution coincides with the transfer matrix describing a directed polymer on the cayley tree but the random weights determined by the fixed point distribution p_cz are broadly distributed this induces some changes in the travelling wave solutions with respect to the usual case of more narrow distributions
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710.0736
Colour image segmentation by the vector-valued Allen-Cahn phase-field model: a multigrid solution
We propose a new method for the numerical solution of a PDE-driven model for colour image segmentation and give numerical examples of the results. The method combines the vector-valued Allen-Cahn phase field equation with initial data fitting terms. This method is known to be closely related to the Mumford-Shah problem and the level set segmentation by Chan and Vese. Our numerical solution is performed using a multigrid splitting of a finite element space, thereby producing an efficient and robust method for the segmentation of large images.
cs.CV cs.NA
we propose a new method for the numerical solution of a pdedriven model for colour image segmentation and give numerical examples of the results the method combines the vectorvalued allencahn phase field equation with initial data fitting terms this method is known to be closely related to the mumfordshah problem and the level set segmentation by chan and vese our numerical solution is performed using a multigrid splitting of a finite element space thereby producing an efficient and robust method for the segmentation of large images
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710.0737
Dynamical Simulations with Highly Improved Staggered Quarks
It is well established that lattice artifacts can be suppressed substantially by the use of SU(3)-projected smeared links in the fermion action. An example is the Highly Improved Staggered Quark action where the ASQ-like effective links are constructed from reunitarized Fat7 links. A general procedure is presented for computing the derivative of the fermion action with respect to the base links (fermion force) - a key component in dynamical simulations using molecular dynamics evolution. The method is iterative and can be applied to actions with arbitrary levels of smearing and reunitarization. The cost of calculating the fermion force is determined for the ASQ action and the HISQ action. Test results show that calculating the HISQ force is about two times more expensive than the ASQ force.
hep-lat
it is well established that lattice artifacts can be suppressed substantially by the use of su3projected smeared links in the fermion action an example is the highly improved staggered quark action where the asqlike effective links are constructed from reunitarized fat7 links a general procedure is presented for computing the derivative of the fermion action with respect to the base links fermion force a key component in dynamical simulations using molecular dynamics evolution the method is iterative and can be applied to actions with arbitrary levels of smearing and reunitarization the cost of calculating the fermion force is determined for the asq action and the hisq action test results show that calculating the hisq force is about two times more expensive than the asq force
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710.0738
Superconductivity in novel Ge-based skutterudites: {Sr,Ba}Pt_4Ge_{12}
Combining experiments and ab initio models we report on $\rm SrPt_4Ge_{12}$ and $\rm BaPt_4Ge_{12}$ as members of a novel class of superconducting skutterudites, where Sr or Ba atoms stabilize a framework entirely formed by Ge-atoms. Below $T_c=5.35$ K, and 5.10 K for $\rm BaPt_4Ge_{12}$ and $\rm SrPt_4Ge_{12}$, respectively, electron-phonon coupled superconductivity emerges, ascribed to intrinsic features of the Pt-Ge framework, where Ge-$p$ states dominate the electronic structure at the Fermi energy.
cond-mat.supr-con cond-mat.mtrl-sci
combining experiments and ab initio models we report on rm srpt_4ge_12 and rm bapt_4ge_12 as members of a novel class of superconducting skutterudites where sr or ba atoms stabilize a framework entirely formed by geatoms below t_c535 k and 510 k for rm bapt_4ge_12 and rm srpt_4ge_12 respectively electronphonon coupled superconductivity emerges ascribed to intrinsic features of the ptge framework where gep states dominate the electronic structure at the fermi energy
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710.0739
Transport and spectral functions in high-temperature QCD
The current status of transport coefficients in relativistic field theories at high temperature is reviewed. I contrast weak coupling results obtained using kinetic theory/diagrammatic techniques with strong coupling results obtained using gauge/gravity duality, and describe the recent developments in extracting transport coefficients and spectral functions from lattice QCD simulations. The fate of quarkonium at high temperature as seen from the lattice is briefly mentioned as well.
hep-lat hep-ph nucl-th
the current status of transport coefficients in relativistic field theories at high temperature is reviewed i contrast weak coupling results obtained using kinetic theorydiagrammatic techniques with strong coupling results obtained using gaugegravity duality and describe the recent developments in extracting transport coefficients and spectral functions from lattice qcd simulations the fate of quarkonium at high temperature as seen from the lattice is briefly mentioned as well
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710.074
On 3-dimensional Asymptotically Harmonic Manifolds
Let (M,g) be a complete, simply connected Riemannian manifold of dimension 3 without conjugate points. We show that M is a hyperbolic manifold of constant sectional curvature, provided M is asymptotically harmonic of constant h > 0.
math.DG
let mg be a complete simply connected riemannian manifold of dimension 3 without conjugate points we show that m is a hyperbolic manifold of constant sectional curvature provided m is asymptotically harmonic of constant h 0
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710.0741
B Semileptonic Decays at High Recoil Momentum
We explore the possibility of studying $B\to\pi l\nu$ semileptonic decays at large recoil momentum. Our methods include the use of a random-wall source for the pion to reduce statistical errors, and different smearing functions are used for the B meson to improve the overlap with the ground state. We observe, in general, a factor of 3-4 improvement in the signal-to-noise ratio in correlation functions if random-wall propagators are used.
hep-lat
we explore the possibility of studying btopi lnu semileptonic decays at large recoil momentum our methods include the use of a randomwall source for the pion to reduce statistical errors and different smearing functions are used for the b meson to improve the overlap with the ground state we observe in general a factor of 34 improvement in the signaltonoise ratio in correlation functions if randomwall propagators are used
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710.0742
Principle of Minimum Distance in Space of States as New Principle in Quantum Physics
The mathematician Leonhard Euler (1707-1783) appears to have been a philosophical optimist having written: "Since the fabric of universe is the most perfect and is the work of the most wise Creator, nothing whatsoever take place in this universe in which some relation of maximum or minimum does not appear. Wherefore, there is absolutely no doubt that every effect in universe can be explained as satisfactory from final causes themselves the aid of the method of Maxima and Minima, as can from the effective causes". Having in mind this kind of optimism, in the papers [1-16] we introduced and investigated the possibility to construct a predictive analytic theory of the elementary particle interaction based on the principle of minimum distance in the space of quantum states (PMD-SQS). So, choosing the partial transition amplitudes as the system variational variables and the distance in the space of the quantum states as a measure of the system effectiveness, we obtained the results [1-16]. These results proved that the principle of minimum distance in space of quantum states (PMD-SQS) can be chosen as variational principle by which we can find the analytic expressions of the partial transition amplitudes. In this paper we present a description of hadron-hadron scattering via principle of minimum distance PMD-SQS when the distance in space of states is minimized with two directional constraints. Then by using the available experimental (pion-nucleon and kaon-nucleon) phase shifts we obtained not only consistent experimental tests of the PMD-SQS optimality, but also strong experimental evidences for new principles in hadronic physics such as: Principle of nonextensivity conjugation via the Riesz-Thorin relation (1/2p+1/2q=1) and a new Principle of limited uncertainty in nonextensive quantum physics.
physics.gen-ph
the mathematician leonhard euler 17071783 appears to have been a philosophical optimist having written since the fabric of universe is the most perfect and is the work of the most wise creator nothing whatsoever take place in this universe in which some relation of maximum or minimum does not appear wherefore there is absolutely no doubt that every effect in universe can be explained as satisfactory from final causes themselves the aid of the method of maxima and minima as can from the effective causes having in mind this kind of optimism in the papers 116 we introduced and investigated the possibility to construct a predictive analytic theory of the elementary particle interaction based on the principle of minimum distance in the space of quantum states pmdsqs so choosing the partial transition amplitudes as the system variational variables and the distance in the space of the quantum states as a measure of the system effectiveness we obtained the results 116 these results proved that the principle of minimum distance in space of quantum states pmdsqs can be chosen as variational principle by which we can find the analytic expressions of the partial transition amplitudes in this paper we present a description of hadronhadron scattering via principle of minimum distance pmdsqs when the distance in space of states is minimized with two directional constraints then by using the available experimental pionnucleon and kaonnucleon phase shifts we obtained not only consistent experimental tests of the pmdsqs optimality but also strong experimental evidences for new principles in hadronic physics such as principle of nonextensivity conjugation via the rieszthorin relation 12p12q1 and a new principle of limited uncertainty in nonextensive quantum physics
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710.0743
Generalized Super-Cerenkov Radiations in Nuclear and Hadronic Media
Generalized Super-Cerenkov Radiations (SCR), as well as their SCR-signatures are investigated and classified. Two general SCR- coherence conditions are found as two natural extremes of the same spontaneous particles decay in (dielectric, nuclear or hadronic) media The main results on the quantum theory of the SCR-phenomena as well as the results of the first experimental test of the super-coherence conditions, obtained by using the experimental data from BNL are presented. The new concepts such as: SCR-gluons, SCR-W-bosons and SCR-Z-bosons, all three suggested by elementary particle classification, are introduced. The gluonic Super-Cerenkov-like radiation, first introduced here, is schematically described. The interpretation of some recent RHIC results as signature of the SCR-gluons is suggested.
hep-ph
generalized supercerenkov radiations scr as well as their scrsignatures are investigated and classified two general scr coherence conditions are found as two natural extremes of the same spontaneous particles decay in dielectric nuclear or hadronic media the main results on the quantum theory of the scrphenomena as well as the results of the first experimental test of the supercoherence conditions obtained by using the experimental data from bnl are presented the new concepts such as scrgluons scrwbosons and scrzbosons all three suggested by elementary particle classification are introduced the gluonic supercerenkovlike radiation first introduced here is schematically described the interpretation of some recent rhic results as signature of the scrgluons is suggested
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710.0744
New Nuclear And Subnuclear Exotic Decays
In this paper new nuclear and subnuclear exotic decays are investigated. Some theoretical problems of the pionic radioactivity, such as fission-like models, applicable to all kind of exotic nuclear and subnuclear decays are presented. The induced nuclear and subnuclear decays are discussed. Moreover, using the recent results on the spontaneous fission half lives T of the heavy nuclei with Z new predictions on the pionic yields in the region of superheavy elements are presented.
nucl-th
in this paper new nuclear and subnuclear exotic decays are investigated some theoretical problems of the pionic radioactivity such as fissionlike models applicable to all kind of exotic nuclear and subnuclear decays are presented the induced nuclear and subnuclear decays are discussed moreover using the recent results on the spontaneous fission half lives t of the heavy nuclei with z new predictions on the pionic yields in the region of superheavy elements are presented
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710.0745
Mixing Kohonen Algorithm, Markov Switching Model and Detection of Multiple Change-Points: An Application to Monetary History
The present paper aims at locating the breakings of the integration process of an international system observed during about 50 years in the 19th century. A historical study could link them to special events, which operated as exogenous shocks on this process. The indicator of integration used is the spread between the highest and the lowest among the London, Hamburg and Paris gold-silver prices. Three algorithms are combined to study this integration: a periodization obtained with the SOM algorithm is confronted to the estimation of a two-regime Markov switching model, in order to give an interpretation of the changes of regime; in the same time change-points are identified over the whole period providing a more precise interpretation of the various types of regulation.
q-fin.GN stat.AP
the present paper aims at locating the breakings of the integration process of an international system observed during about 50 years in the 19th century a historical study could link them to special events which operated as exogenous shocks on this process the indicator of integration used is the spread between the highest and the lowest among the london hamburg and paris goldsilver prices three algorithms are combined to study this integration a periodization obtained with the som algorithm is confronted to the estimation of a tworegime markov switching model in order to give an interpretation of the changes of regime in the same time changepoints are identified over the whole period providing a more precise interpretation of the various types of regulation
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710.0746
Universality and Scaling at the chiral transition in two-flavor QCD at finite temperature
The order of the phase transition in finite-temperature QCD with two degenerate light quarks is still an open problem and corresponds to the last question mark in the zero-density phase diagram of QCD. We argue that establishing the nature of the transition in this case is also a crucial test for numerical simulations of lattice QCD, allowing precise estimates of possible systematic errors related e.g. to the choice of fermion-simulation algorithm or of discretized formulation for fermions.
hep-lat
the order of the phase transition in finitetemperature qcd with two degenerate light quarks is still an open problem and corresponds to the last question mark in the zerodensity phase diagram of qcd we argue that establishing the nature of the transition in this case is also a crucial test for numerical simulations of lattice qcd allowing precise estimates of possible systematic errors related eg to the choice of fermionsimulation algorithm or of discretized formulation for fermions
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710.0747
Calibration of the mirror system in the HERA-B RICH
The mirror system of the HERA-B RICH consists of two spherical and two planar mirrors, composed of altogether 116 mirror segments. Analysis of displacements of the \v{C}erenkov ring center relative to the charged particle track, for given spherical-planar segment pairs, leads to accurate information regarding the orientation of individual mirror segments. The method is described and the effect of applying the required corrections on the \v{C}erenkov angle resolution of the HERA-B RICH is discussed.
physics.ins-det
the mirror system of the herab rich consists of two spherical and two planar mirrors composed of altogether 116 mirror segments analysis of displacements of the vcerenkov ring center relative to the charged particle track for given sphericalplanar segment pairs leads to accurate information regarding the orientation of individual mirror segments the method is described and the effect of applying the required corrections on the vcerenkov angle resolution of the herab rich is discussed
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710.0748
A Fast Heuristic Algorithm Based on Verification and Elimination Methods for Maximum Clique Problem
A clique in an undirected graph G= (V, E) is a subset V' V of vertices, each pair of which is connected by an edge in E. The clique problem is an optimization problem of finding a clique of maximum size in graph. The clique problem is NP-Complete. We have succeeded in developing a fast algorithm for maximum clique problem by employing the method of verification and elimination. For a graph of size N there are 2N sub graphs, which may be cliques and hence verifying all of them, will take a long time. Idea is to eliminate a major number of sub graphs, which cannot be cliques and verifying only the remaining sub graphs. This heuristic algorithm runs in polynomial time and executes successfully for several examples when applied to random graphs and DIMACS benchmark graphs.
cs.DM cs.CC
a clique in an undirected graph g v e is a subset v v of vertices each pair of which is connected by an edge in e the clique problem is an optimization problem of finding a clique of maximum size in graph the clique problem is npcomplete we have succeeded in developing a fast algorithm for maximum clique problem by employing the method of verification and elimination for a graph of size n there are 2n sub graphs which may be cliques and hence verifying all of them will take a long time idea is to eliminate a major number of sub graphs which cannot be cliques and verifying only the remaining sub graphs this heuristic algorithm runs in polynomial time and executes successfully for several examples when applied to random graphs and dimacs benchmark graphs
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710.0749
Observations of V838 Mon in the CO rotational lines
We investigate the structure of a field around the position of V838 Mon as seen in the lowest CO rotational transitions. We also measure and analyse emission in the same lines at the position of V838 Mon.Observations have primarily been done in the CO J = 2-1 and J = 3-2 lines using the KOSMA telescope. A field of 3.4 squared degrees has been mapped in the on-the-fly mode in these transitions. Longer integration spectra in the on-off mode have been obtained to study the emission at the position of V838 Mon. Selected positions in the field have also been observed in the CO J = 1-0 transition using the Delingha telescope.In the observed field we have identified many molecular clouds. They can be divided into two groups from the point of view of their observed radial velocities. One, having V(LSR) in the range 18-32 km/s, can be identified with the Perseus Galactic arm. The other one, having V(LSR) between 44-57 km/s, probably belongs to the Norma-Cygnus arm. The radial velocity of V838 Mon is within the second range but the object does not seem to be related to any of the observed clouds. We did not find any molecular buble of a 1 degree dimension around the position of V838 Mon claimed in van Loon et al. An emission has been detected at the position of the object in the CO J = 2-1 and J = 3-2 transitions. The emission is very narrow (FWHM ~ 1.2 km/s) and at V(LSR) = 53.3 km/s. Our analysis of the data suggests that the emission is probably extended.
astro-ph
we investigate the structure of a field around the position of v838 mon as seen in the lowest co rotational transitions we also measure and analyse emission in the same lines at the position of v838 monobservations have primarily been done in the co j 21 and j 32 lines using the kosma telescope a field of 34 squared degrees has been mapped in the onthefly mode in these transitions longer integration spectra in the onoff mode have been obtained to study the emission at the position of v838 mon selected positions in the field have also been observed in the co j 10 transition using the delingha telescopein the observed field we have identified many molecular clouds they can be divided into two groups from the point of view of their observed radial velocities one having vlsr in the range 1832 kms can be identified with the perseus galactic arm the other one having vlsr between 4457 kms probably belongs to the normacygnus arm the radial velocity of v838 mon is within the second range but the object does not seem to be related to any of the observed clouds we did not find any molecular buble of a 1 degree dimension around the position of v838 mon claimed in van loon et al an emission has been detected at the position of the object in the co j 21 and j 32 transitions the emission is very narrow fwhm 12 kms and at vlsr 533 kms our analysis of the data suggests that the emission is probably extended
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710.075
Nuclear Tuning and Detuning of the Electron Spin Resonance in a Quantum Dot
We study nuclear spin dynamics in a quantum dot close to the conditions of electron spin resonance. We show that at small frequency mismatch the nuclear field detunes the resonance. Remarkably, at larger frequency mismatch its effect is opposite: The nuclear system is bistable, and in one of the stable states the field accurately tunes the electron spin splitting to resonance. In this state the nuclear field fluctuations are strongly suppressed and nuclear spin relaxation is accelerated.
cond-mat.mes-hall
we study nuclear spin dynamics in a quantum dot close to the conditions of electron spin resonance we show that at small frequency mismatch the nuclear field detunes the resonance remarkably at larger frequency mismatch its effect is opposite the nuclear system is bistable and in one of the stable states the field accurately tunes the electron spin splitting to resonance in this state the nuclear field fluctuations are strongly suppressed and nuclear spin relaxation is accelerated
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710.0751
Leptonic secondary emission in a hadronic microquasar model
Context: It has been proposed that the origin of the very high-energy photons emitted from high-mass X-ray binaries with jet-like features, so-called microquasars (MQs), is related to hadronic interactions between relativistic protons in the jet and cold protons of the stellar wind. Leptonic secondary emission should be calculated in a complete hadronic model that include the effects of pairs from charged pion decays inside the jets and the emission from pairs generated by gamma-ray absorption in the photosphere of the system. Aims: We aim at predicting the broadband spectrum from a general hadronic microquasar model, taking into account the emission from secondaries created by charged pion decay inside the jet. Methods: The particle energy distribution for secondary leptons injected along the jets is consistently derived taking the energy losses into account. We also compute the spectral energy distribution resulting from these leptons is calculated after assuming different values of the magnetic field inside the jets. The spectrum of the gamma-rays produced by neutral pion-decay and processed by electromagnetic cascades under the stellar photon field. Results: We show that the secondary emission can dominate the spectral energy distribution at low energies (~1 MeV). At high energies, the production spectrum can be significantly distorted by the effect of electromagnetic cascades. These effects are phase-dependent, and some variability modulated by the orbital period is predicted.
astro-ph
context it has been proposed that the origin of the very highenergy photons emitted from highmass xray binaries with jetlike features socalled microquasars mqs is related to hadronic interactions between relativistic protons in the jet and cold protons of the stellar wind leptonic secondary emission should be calculated in a complete hadronic model that include the effects of pairs from charged pion decays inside the jets and the emission from pairs generated by gammaray absorption in the photosphere of the system aims we aim at predicting the broadband spectrum from a general hadronic microquasar model taking into account the emission from secondaries created by charged pion decay inside the jet methods the particle energy distribution for secondary leptons injected along the jets is consistently derived taking the energy losses into account we also compute the spectral energy distribution resulting from these leptons is calculated after assuming different values of the magnetic field inside the jets the spectrum of the gammarays produced by neutral piondecay and processed by electromagnetic cascades under the stellar photon field results we show that the secondary emission can dominate the spectral energy distribution at low energies 1 mev at high energies the production spectrum can be significantly distorted by the effect of electromagnetic cascades these effects are phasedependent and some variability modulated by the orbital period is predicted
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710.0752
The Einstein-Yang-Mills equations from Bianchi identities
We suggest a novel extension to the Kaluza-Klein scheme that allows us to obtain consistently all SU(n) Einstein-Yang-Mills theories. This construction is based on allowing the five-dimensional spacetime to carry some non-vanishing torsion; however, the four-dimensional spacetime remains intrinsically torsion-free.
gr-qc hep-th
we suggest a novel extension to the kaluzaklein scheme that allows us to obtain consistently all sun einsteinyangmills theories this construction is based on allowing the fivedimensional spacetime to carry some nonvanishing torsion however the fourdimensional spacetime remains intrinsically torsionfree
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