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707.033
An Algebra of Quantum Processes
We introduce an algebra qCCS of pure quantum processes in which no classical data is involved, communications by moving quantum states physically are allowed, and computations is modeled by super-operators. An operational semantics of qCCS is presented in terms of (non-probabilistic) labeled transition systems. Strong bisimulation between processes modeled in qCCS is defined, and its fundamental algebraic properties are established, including uniqueness of the solutions of recursive equations. To model sequential computation in qCCS, a reduction relation between processes is defined. By combining reduction relation and strong bisimulation we introduce the notion of strong reduction-bisimulation, which is a device for observing interaction of computation and communication in quantum systems. Finally, a notion of strong approximate bisimulation (equivalently, strong bisimulation distance) and its reduction counterpart are introduced. It is proved that both approximate bisimilarity and approximate reduction-bisimilarity are preserved by various constructors of quantum processes. This provides us with a formal tool for observing robustness of quantum processes against inaccuracy in the implementation of its elementary gates.
quant-ph
we introduce an algebra qccs of pure quantum processes in which no classical data is involved communications by moving quantum states physically are allowed and computations is modeled by superoperators an operational semantics of qccs is presented in terms of nonprobabilistic labeled transition systems strong bisimulation between processes modeled in qccs is defined and its fundamental algebraic properties are established including uniqueness of the solutions of recursive equations to model sequential computation in qccs a reduction relation between processes is defined by combining reduction relation and strong bisimulation we introduce the notion of strong reductionbisimulation which is a device for observing interaction of computation and communication in quantum systems finally a notion of strong approximate bisimulation equivalently strong bisimulation distance and its reduction counterpart are introduced it is proved that both approximate bisimilarity and approximate reductionbisimilarity are preserved by various constructors of quantum processes this provides us with a formal tool for observing robustness of quantum processes against inaccuracy in the implementation of its elementary gates
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707.0331
Target mass corrections and twist-3 in the nucleon spin structure functions
The Nachtmann moment is employed to study the contribution of twist-3 operator to the nucleon spin structure functions. Target mass corrections to the Cornwall-Norton moments of the spin structure functions $g_{1,2}$ are discussed. It is found that the corrections play a sizeable role to the contribution of the twist-3 $\tilde d_2$ extracted from the Cornwall-Norton moments.
hep-ph
the nachtmann moment is employed to study the contribution of twist3 operator to the nucleon spin structure functions target mass corrections to the cornwallnorton moments of the spin structure functions g_12 are discussed it is found that the corrections play a sizeable role to the contribution of the twist3 tilde d_2 extracted from the cornwallnorton moments
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707.0332
Melting of the vortex lattice in layered superconductors
The structure function of the vortex lattice of layered superconductor is calculated to one-loop order. Based on a phenomenological melting criterion concerning the Debye-Waller factor, we calculate the melting line of the vortex lattice, and compare our results to Monte Carlo simulation and experiment. We find that our results are quantitatively in good agreement with the Monte Carlo results. Moreover, our analytic calculation of the melting line of BSCCO fits the experiment reasonably well in a temperature range not far from Tc.
cond-mat.supr-con cond-mat.stat-mech
the structure function of the vortex lattice of layered superconductor is calculated to oneloop order based on a phenomenological melting criterion concerning the debyewaller factor we calculate the melting line of the vortex lattice and compare our results to monte carlo simulation and experiment we find that our results are quantitatively in good agreement with the monte carlo results moreover our analytic calculation of the melting line of bscco fits the experiment reasonably well in a temperature range not far from tc
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707.0333
The radius and mass of the subgiant star bet Hyi from interferometry and asteroseismology
We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of beta Hydri. This star is a nearby G2 subgiant whose mean density was recently measured with high precision using asteroseismology. We determine the radius and effective temperature of the star to be 1.814+/-0.017 R_sun (0.9%) and 5872+/-44 K (0.7%) respectively. By combining this value with the mean density, as estimated from asteroseismology, we make a direct estimate of the stellar mass. We find a value of 1.07+/-0.03 M_sun (2.8%), which agrees with published estimates based on fitting in the H-R diagram, but has much higher precision. These results place valuable constraints on theoretical models of beta Hyi and its oscillation frequencies.
astro-ph
we have used the sydney university stellar interferometer susi to measure the angular diameter of beta hydri this star is a nearby g2 subgiant whose mean density was recently measured with high precision using asteroseismology we determine the radius and effective temperature of the star to be 18140017 r_sun 09 and 587244 k 07 respectively by combining this value with the mean density as estimated from asteroseismology we make a direct estimate of the stellar mass we find a value of 107003 m_sun 28 which agrees with published estimates based on fitting in the hr diagram but has much higher precision these results place valuable constraints on theoretical models of beta hyi and its oscillation frequencies
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707.0334
Implementation of three-qubit Grover search in cavity QED
Using resonant interaction of three Rydberg atoms with a single-mode microwave cavity, we consider a realization of three-qubit Grover search algorithm in the presence of weak cavity decay, based on a previous idea for three-qubit quantum gate [Phys. Rev. A 73, 064304 (2006)]. We simulate the searching process under the influence of the cavity decay and show that our scheme could be achieved efficiently to find the marked state with high fidelity. The required operations are very close to the reach with current cavity QED techniques.
quant-ph
using resonant interaction of three rydberg atoms with a singlemode microwave cavity we consider a realization of threequbit grover search algorithm in the presence of weak cavity decay based on a previous idea for threequbit quantum gate phys rev a 73 064304 2006 we simulate the searching process under the influence of the cavity decay and show that our scheme could be achieved efficiently to find the marked state with high fidelity the required operations are very close to the reach with current cavity qed techniques
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707.0335
Label-setting methods for Multimode Stochastic Shortest Path problems on graphs
Stochastic shortest path (SSP) problems arise in a variety of discrete stochastic control contexts. An optimal solutions to such a problem is typically computed using the value function, which can be found by solving the corresponding dynamic programming equations. In the deterministic case, these equations can be often solved by the highly efficient label-setting methods (such as Dijkstra's and Dial's algorithms). In this paper we define and study a class of Multimode Stochastic Shortest Path problems and develop sufficient conditions for the applicability of label-setting methods. We illustrate our approach on a number of discrete stochastic control examples. We also discuss the relationship of SSPs with discretizations of static Hamilton-Jacobi equations and provide an alternative derivation for several fast (non-iterative) numerical methods for these PDEs.
math.OC math.NA
stochastic shortest path ssp problems arise in a variety of discrete stochastic control contexts an optimal solutions to such a problem is typically computed using the value function which can be found by solving the corresponding dynamic programming equations in the deterministic case these equations can be often solved by the highly efficient labelsetting methods such as dijkstras and dials algorithms in this paper we define and study a class of multimode stochastic shortest path problems and develop sufficient conditions for the applicability of labelsetting methods we illustrate our approach on a number of discrete stochastic control examples we also discuss the relationship of ssps with discretizations of static hamiltonjacobi equations and provide an alternative derivation for several fast noniterative numerical methods for these pdes
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707.0336
Pricing Options on Defaultable Stocks
In this note, we develop stock option price approximations for a model which takes both the risk o default and the stochastic volatility into account. We also let the intensity of defaults be influenced by the volatility. We show that it might be possible to infer the risk neutral default intensity from the stock option prices. Our option price approximation has a rich implied volatility surface structure and fits the data implied volatility well. Our calibration exercise shows that an effective hazard rate from bonds issued by a company can be used to explain the implied volatility skew of the implied volatility of the option prices issued by the same company.
cs.CE
in this note we develop stock option price approximations for a model which takes both the risk o default and the stochastic volatility into account we also let the intensity of defaults be influenced by the volatility we show that it might be possible to infer the risk neutral default intensity from the stock option prices our option price approximation has a rich implied volatility surface structure and fits the data implied volatility well our calibration exercise shows that an effective hazard rate from bonds issued by a company can be used to explain the implied volatility skew of the implied volatility of the option prices issued by the same company
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707.0337
Stability, Reactivity, and Aromaticity of Compounds of a Multivalent Superatom
In this communication we analyze the stability, reactivity and possible aromatic behavior of two recently reported clusters (Reveles J. U.; Khanna S. N.; Roach P. J.; Castleman A. W. jr. Proc. Natl. Acad. Sci, 2006, 103, 18405), viz., Al7C- and Al7O- in the light of the principles of the maximum hardness and minimum electrophilicity as well as the nucleus independent chemical shift values.
physics.atm-clus physics.chem-ph
in this communication we analyze the stability reactivity and possible aromatic behavior of two recently reported clusters reveles j u khanna s n roach p j castleman a w jr proc natl acad sci 2006 103 18405 viz al7c and al7o in the light of the principles of the maximum hardness and minimum electrophilicity as well as the nucleus independent chemical shift values
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707.0338
Integral pinched 3-manifolds are space forms
In this paper we prove that, under an explicit integral pinching assumption between the $L^2$-norm of the Ricci curvature and the $L^2$-norm of the scalar curvature, a closed 3-manifold with positive scalar curvature admits an Einstein metric with positive curvature. In particular this implies that the manifold is diffeomorphic to a quotient of ${\Bbb S}^3$.
math.DG math.AP
in this paper we prove that under an explicit integral pinching assumption between the l2norm of the ricci curvature and the l2norm of the scalar curvature a closed 3manifold with positive scalar curvature admits an einstein metric with positive curvature in particular this implies that the manifold is diffeomorphic to a quotient of bbb s3
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707.0339
The BSSN formulation is a partially constrained evolution system
Relativistic simulations in 3+1 dimensions typically monitor the Hamiltonian and momentum constraints during evolution, with significant violations of these constraints indicating the presence of instabilities. In this paper we rewrite the momentum constraints as first-order evolution equations, and show that the popular BSSN formulation of the Einstein equations explicitly uses the momentum constraints as evolution equations. We conjecture that this feature is a key reason for the relative success of the BSSN formulation in numerical relativity.
gr-qc
relativistic simulations in 31 dimensions typically monitor the hamiltonian and momentum constraints during evolution with significant violations of these constraints indicating the presence of instabilities in this paper we rewrite the momentum constraints as firstorder evolution equations and show that the popular bssn formulation of the einstein equations explicitly uses the momentum constraints as evolution equations we conjecture that this feature is a key reason for the relative success of the bssn formulation in numerical relativity
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707.034
Asymptotic enumeration of sparse nonnegative integer matrices with specified row and column sums
Let \svec = (s_1,...,s_m) and \tvec = (t_1,...,t_n) be vectors of nonnegative integer-valued functions of m,n with equal sum S = sum_{i=1}^m s_i = sum_{j=1}^n t_j. Let M(\svec,\tvec) be the number of m*n matrices with nonnegative integer entries such that the i-th row has row sum s_i and the j-th column has column sum t_j for all i,j. Such matrices occur in many different settings, an important example being the contingency tables (also called frequency tables) important in statistics. Define s=max_i s_i and t=max_j t_j. Previous work has established the asymptotic value of M(\svec,\tvec) as m,n\to\infty with s and t bounded (various authors independently, 1971-1974), and when \svec,\tvec are constant vectors with m/n,n/m,s/n >= c/log n for sufficiently large (Canfield and McKay, 2007). In this paper we extend the sparse range to the case st=o(S^(2/3)). The proof in part follows a previous asymptotic enumeration of 0-1 matrices under the same conditions (Greenhill, McKay and Wang, 2006). We also generalise the enumeration to matrices over any subset of the nonnegative integers that includes 0 and 1.
math.CO math.ST stat.TH
let svec s_1s_m and tvec t_1t_n be vectors of nonnegative integervalued functions of mn with equal sum s sum_i1m s_i sum_j1n t_j let msvectvec be the number of mn matrices with nonnegative integer entries such that the ith row has row sum s_i and the jth column has column sum t_j for all ij such matrices occur in many different settings an important example being the contingency tables also called frequency tables important in statistics define smax_i s_i and tmax_j t_j previous work has established the asymptotic value of msvectvec as mntoinfty with s and t bounded various authors independently 19711974 and when svectvec are constant vectors with mnnmsn clog n for sufficiently large canfield and mckay 2007 in this paper we extend the sparse range to the case stos23 the proof in part follows a previous asymptotic enumeration of 01 matrices under the same conditions greenhill mckay and wang 2006 we also generalise the enumeration to matrices over any subset of the nonnegative integers that includes 0 and 1
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707.0341
Considering boundary conditions for black hole entropy in loop quantum gravity
We argue for black hole entropy in loop quantum gravity (LQG) by taking into account the interpretation that there is no other side of the horizon. This gives new values for the Barbero-Immirzi parameter which are fairly larger than those considered before. We also discuss its consequences.
hep-th gr-qc
we argue for black hole entropy in loop quantum gravity lqg by taking into account the interpretation that there is no other side of the horizon this gives new values for the barberoimmirzi parameter which are fairly larger than those considered before we also discuss its consequences
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707.0342
Spin-orbit-assisted electron-phonon interaction and the magnetophonon resonance in semiconductor quantum wells
We introduce a spin-orbit assisted electron-phonon (e-ph) coupling mechanism for carriers in semiconductor quantum wells and predict qualitatively the form and shape of anticrossings between the cyclotron resonance (CR) and optical (LO and TO) phonons. Since this e-ph interaction involves the electron spin it makes the predicted TO-CR anticrossing dependent on the filling factor and therefore on the polarization of the 2D electron gas in the quantum well.
cond-mat.mes-hall
we introduce a spinorbit assisted electronphonon eph coupling mechanism for carriers in semiconductor quantum wells and predict qualitatively the form and shape of anticrossings between the cyclotron resonance cr and optical lo and to phonons since this eph interaction involves the electron spin it makes the predicted tocr anticrossing dependent on the filling factor and therefore on the polarization of the 2d electron gas in the quantum well
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707.0343
Particle interference as a test of Lorentz-violating electrodynamics
In Lorentz-violating electrodynamics a steady current (and similarly a static charge) generates both static magnetic and electric fields. These induced fields, acting on interfering particles, change the interference pattern. We find that particle interference experiments are sensitive to small Lorentz violating effects, and thus they can be used to improve current bounds on some Lorentz-violating parameters.
hep-ph quant-ph
in lorentzviolating electrodynamics a steady current and similarly a static charge generates both static magnetic and electric fields these induced fields acting on interfering particles change the interference pattern we find that particle interference experiments are sensitive to small lorentz violating effects and thus they can be used to improve current bounds on some lorentzviolating parameters
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707.0344
Large deviations for symmetrised empirical measures
In this paper we prove a Large Deviation Principle for the sequence of symmetrised empirical measures $\frac{1}{n} \sum_{i=1}^{n} \delta_{(X^n_i,X^n_{\sigma_n(i)})}$ where $\sigma_n$ is a random permutation and $((X_i^n)_{1 \leq i \leq n})_{n \geq 1}$ is a triangular array of random variables with suitable properties. As an application we show how this result allows to improve the Large Deviation Principles for symmetrised initial-terminal conditions bridge processes recently established by Adams, Dorlas and K\"{o}nig.
math.PR
in this paper we prove a large deviation principle for the sequence of symmetrised empirical measures frac1n sum_i1n delta_xn_ixn_sigma_ni where sigma_n is a random permutation and x_in_1 leq i leq n_n geq 1 is a triangular array of random variables with suitable properties as an application we show how this result allows to improve the large deviation principles for symmetrised initialterminal conditions bridge processes recently established by adams dorlas and konig
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707.0345
Thermal rounding of the depinning transition
We study thermal effects at the depinning transition by numerical simulations of driven one-dimensional elastic interfaces in a disordered medium. We find that the velocity of the interface, evaluated at the critical depinning force, can be correctly described with the power law $v\sim T^\psi$, where $\psi$ is the thermal exponent. Using the sample-dependent value of the critical force, we precisely evaluate the value of $\psi$ directly from the temperature dependence of the velocity, obtaining the value $\psi = 0.15 \pm 0.01$. By measuring the structure factor of the interface we show that both the thermally-rounded and the T=0 depinning, display the same large-scale geometry, described by an identical divergence of a characteristic length with the velocity $\xi \propto v^{-\nu/\beta}$, where $\nu$ and $\beta$ are respectively the T=0 correlation and depinning exponents. We discuss the comparison of our results with previous estimates of the thermal exponent and the direct consequences for recent experiments on magnetic domain wall motion in ferromagnetic thin films.
cond-mat.stat-mech cond-mat.dis-nn
we study thermal effects at the depinning transition by numerical simulations of driven onedimensional elastic interfaces in a disordered medium we find that the velocity of the interface evaluated at the critical depinning force can be correctly described with the power law vsim tpsi where psi is the thermal exponent using the sampledependent value of the critical force we precisely evaluate the value of psi directly from the temperature dependence of the velocity obtaining the value psi 015 pm 001 by measuring the structure factor of the interface we show that both the thermallyrounded and the t0 depinning display the same largescale geometry described by an identical divergence of a characteristic length with the velocity xi propto vnubeta where nu and beta are respectively the t0 correlation and depinning exponents we discuss the comparison of our results with previous estimates of the thermal exponent and the direct consequences for recent experiments on magnetic domain wall motion in ferromagnetic thin films
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707.0346
The one-dimensional Schr\"{o}dinger-Newton equations
We prove an existence and uniqueness result for ground states of one-dimensional Schr\"{o}dinger-Newton equations.
math-ph math.MP
we prove an existence and uniqueness result for ground states of onedimensional schrodingernewton equations
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707.0347
Gauss-Bonnet Gravity with Scalar Field in Four Dimensions
We give all exact solutions of the Einstein-Gauss-Bonnet Field Equations coupled with a scalar field in four dimensions under certain assumptions.
gr-qc hep-th
we give all exact solutions of the einsteingaussbonnet field equations coupled with a scalar field in four dimensions under certain assumptions
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707.0348
Self-Organized Characteristics of the International System
Various self-organized characteristics of the international system can be identified with the help of a complexity science perspective. The perspective discussed in this article is based on various complexity science concepts and theories, and concepts related to ecology and ecosystems. It can be argued that the Great Power war dynamics of the international system in Europe during the period 1480-1945, showed self-organized critical (SOC) characteristics, resulting in a punctuated equilibrium dynamic. It seems that the SOC-characteristics of the international system and the punctuated equilibrium dynamic were - in combination with chaotic war dynamics - functional in a process of social expansion in Europe. According to a model presented in this article, population growth was a component of the driving force of the international system during this time frame. The findings of this exploratory research project contradict with generally held opinions in International Relations theory.
nlin.AO
various selforganized characteristics of the international system can be identified with the help of a complexity science perspective the perspective discussed in this article is based on various complexity science concepts and theories and concepts related to ecology and ecosystems it can be argued that the great power war dynamics of the international system in europe during the period 14801945 showed selforganized critical soc characteristics resulting in a punctuated equilibrium dynamic it seems that the soccharacteristics of the international system and the punctuated equilibrium dynamic were in combination with chaotic war dynamics functional in a process of social expansion in europe according to a model presented in this article population growth was a component of the driving force of the international system during this time frame the findings of this exploratory research project contradict with generally held opinions in international relations theory
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707.0349
Metallic Graphene Nanodisks
We explore the electronic properties of finite-length graphene nanoribbons as well as graphene nanodisks with various sizes and shapes in quest of metallic ones. For this purpose it is sufficient to search zero-energy states. We find that there exist no zero-energy states in finite-length zigzag nanoribbons though all infinite-length zigzag nanoribbons have zero-energy states. The occurrence of zero-energy states is surprisingly rare. Among typical nanodisks, only trigonal zigzag nanodisks have degenerate zero-energy states and show metallic ferromagnetism, where the degeneracy can be controlled arbitrarily by designing the size. A remarkable property is that the relaxation time is quite large in spite of its small size in trigonal zigzag nanodisks.
cond-mat.mes-hall cond-mat.mtrl-sci
we explore the electronic properties of finitelength graphene nanoribbons as well as graphene nanodisks with various sizes and shapes in quest of metallic ones for this purpose it is sufficient to search zeroenergy states we find that there exist no zeroenergy states in finitelength zigzag nanoribbons though all infinitelength zigzag nanoribbons have zeroenergy states the occurrence of zeroenergy states is surprisingly rare among typical nanodisks only trigonal zigzag nanodisks have degenerate zeroenergy states and show metallic ferromagnetism where the degeneracy can be controlled arbitrarily by designing the size a remarkable property is that the relaxation time is quite large in spite of its small size in trigonal zigzag nanodisks
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707.035
A new concept and design of ferrite-based microwave vortex devices
In microwave resonant systems with ferrite samples, one becomes faced with specific phase relations for the electromagnetic fields. Such specific phase relations may lead to appearance of nontrivial states: electromagnetic vortices. This paper provides some general ideas and design principles for microwave devices with the field vortex structures.
physics.class-ph
in microwave resonant systems with ferrite samples one becomes faced with specific phase relations for the electromagnetic fields such specific phase relations may lead to appearance of nontrivial states electromagnetic vortices this paper provides some general ideas and design principles for microwave devices with the field vortex structures
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707.0351
Dispersion representations for hard exclusive processes
Several hard exclusive scattering processes admit a description in terms of generalized parton distributions and perturbative hard-scattering kernels. Both the physical amplitude and the hard-scattering kernels fulfill dispersion relations. We give a detailed investigation of their consistency at all orders in perturbation theory. The results shed light on the information about generalized parton distributions that can be extracted from the real and imaginary parts of exclusive amplitudes. They also provide a practical consistency check for models of these distributions in which Lorentz invariance is not exactly satisfied.
hep-ph
several hard exclusive scattering processes admit a description in terms of generalized parton distributions and perturbative hardscattering kernels both the physical amplitude and the hardscattering kernels fulfill dispersion relations we give a detailed investigation of their consistency at all orders in perturbation theory the results shed light on the information about generalized parton distributions that can be extracted from the real and imaginary parts of exclusive amplitudes they also provide a practical consistency check for models of these distributions in which lorentz invariance is not exactly satisfied
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707.0352
Monte Carlo simulation of pressure-induced phase transitions in spin-crossover materials
Pressure-induced phase transitions of spin-crossover materials were simulated by a Monte Carlo simulation in the constant pressure ensemble for the first time. Here, as the origin of the cooperative interaction, we adopt elastic interaction among the distortions of the lattice due to the difference of the molecular sizes in different spin states, i.e., the high spin (HS) state and the low spin (LS) state. We studied how the temperature dependence of the ordering process changes with the pressure, and we obtained a standard sequence of temperature dependences that has been found in changing other parameters such as strength of the ligand field (S. Miyashita et al., Prog. Theor. Phys. \textbf{114}, 719 (2005)). Various effects of pressure on the spin-crossover ordering process are examined from a unified point of view.
cond-mat.mtrl-sci cond-mat.stat-mech
pressureinduced phase transitions of spincrossover materials were simulated by a monte carlo simulation in the constant pressure ensemble for the first time here as the origin of the cooperative interaction we adopt elastic interaction among the distortions of the lattice due to the difference of the molecular sizes in different spin states ie the high spin hs state and the low spin ls state we studied how the temperature dependence of the ordering process changes with the pressure and we obtained a standard sequence of temperature dependences that has been found in changing other parameters such as strength of the ligand field s miyashita et al prog theor phys textbf114 719 2005 various effects of pressure on the spincrossover ordering process are examined from a unified point of view
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707.0353
Intrinsic Zeeman Effect in Graphene
The intrinsic Zeeman energy is precisely one half of the cyclotron energy for electrons in graphene. As a result a Landau-level mixing occurs to create the energy spectrum comprised of the $4j$-fold degenerated zero-energy level and 4-fold degenerated nonzero-energy levels in the $j$-layer graphene, where $j=1,2,3$ for monolayer, bilayer and trilayer, respectively. The degeneracy manifests itself in the quantum Hall (QH) effect. We study how the degeneracy is removed by the Coulomb interactions. With respect to the zero-energy level, an excitonic gap opens by making a BCS-type condensation of electron-hole pairs at the filling factor $\nu =0$. It gives birth to the Ising QH ferromagnet at $\nu =\pm 1$ for monolayer, $\nu =\pm 1,\pm 3$ for bilayer, and $\nu =\pm 1,\pm 3,\pm 5$ for trilayer graphene from the zero-energy degeneracy. With respect to the nonzero-energy level, a remarkable consequence is derived that the effective Coulomb potential depends on spins, since a single energy level contains up-spin and down-spin electrons belonging to different Landau levels. The spin-dependent Coulomb interaction leads to the valley polarization at $\nu =\pm 4, \pm 8, \pm 12, ...$ for monolayer, $\nu =\pm 2, \pm 6, \pm 10, >...$ for bilayer, and $\nu =\pm 2,\pm 4, \pm 8, \pm 12, ...$ for trilayer graphene.
cond-mat.mes-hall cond-mat.str-el
the intrinsic zeeman energy is precisely one half of the cyclotron energy for electrons in graphene as a result a landaulevel mixing occurs to create the energy spectrum comprised of the 4jfold degenerated zeroenergy level and 4fold degenerated nonzeroenergy levels in the jlayer graphene where j123 for monolayer bilayer and trilayer respectively the degeneracy manifests itself in the quantum hall qh effect we study how the degeneracy is removed by the coulomb interactions with respect to the zeroenergy level an excitonic gap opens by making a bcstype condensation of electronhole pairs at the filling factor nu 0 it gives birth to the ising qh ferromagnet at nu pm 1 for monolayer nu pm 1pm 3 for bilayer and nu pm 1pm 3pm 5 for trilayer graphene from the zeroenergy degeneracy with respect to the nonzeroenergy level a remarkable consequence is derived that the effective coulomb potential depends on spins since a single energy level contains upspin and downspin electrons belonging to different landau levels the spindependent coulomb interaction leads to the valley polarization at nu pm 4 pm 8 pm 12 for monolayer nu pm 2 pm 6 pm 10 for bilayer and nu pm 2pm 4 pm 8 pm 12 for trilayer graphene
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707.0354
Low densities in asymmetric nuclear matter
Asymmetric nuclear matter is investigated in the low density region below the nuclear saturation density. Microscopic calculations based on the Dirac Brueckner Hartree-Fock (DBHF) approach with realistic nucleon-nucleon potentials are used to adjust a low density functional. This functional is constructed on a density expansion of the relativistic mean field theory which allows a clear interpretation of the role of the mesons to the equation of state. It is shown that a correction term should be added to the functional in order to take into account the effects beyond the mean field. Two functionals with different corrections are obtained. Those functionals converge to predict a reduction of the spinodal zone in asymmetric nuclear matter by about 15-20% and an isoscalar unstable mode closer to the constant Z/A direction than the functional without correction.
nucl-th
asymmetric nuclear matter is investigated in the low density region below the nuclear saturation density microscopic calculations based on the dirac brueckner hartreefock dbhf approach with realistic nucleonnucleon potentials are used to adjust a low density functional this functional is constructed on a density expansion of the relativistic mean field theory which allows a clear interpretation of the role of the mesons to the equation of state it is shown that a correction term should be added to the functional in order to take into account the effects beyond the mean field two functionals with different corrections are obtained those functionals converge to predict a reduction of the spinodal zone in asymmetric nuclear matter by about 1520 and an isoscalar unstable mode closer to the constant za direction than the functional without correction
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707.0355
Evolutionary Conditions in the Dissipative MHD System Revisited
The evolutionary conditions for the dissipative continuous magnetohydrodynamic (MHD) shocks are studied. We modify Hada's approach in the stability analysis of the MHD shock waves. The matching conditions between perturbed shock structure and asymptotic wave modes shows that all types of the MHD shocks, including the intermediate shocks, are evolutionary and perturbed solutions are uniquely defined. We also adopt our formalism to the MHD shocks in the system with resistivity without viscosity, which is often used in numerical simulation, and show that all types of shocks that are found in the system satisfy the evolutionary condition and perturbed solutions are uniquely defined. These results suggest that the intermediate shocks may appear in reality.
astro-ph
the evolutionary conditions for the dissipative continuous magnetohydrodynamic mhd shocks are studied we modify hadas approach in the stability analysis of the mhd shock waves the matching conditions between perturbed shock structure and asymptotic wave modes shows that all types of the mhd shocks including the intermediate shocks are evolutionary and perturbed solutions are uniquely defined we also adopt our formalism to the mhd shocks in the system with resistivity without viscosity which is often used in numerical simulation and show that all types of shocks that are found in the system satisfy the evolutionary condition and perturbed solutions are uniquely defined these results suggest that the intermediate shocks may appear in reality
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707.0356
No Higgs at the LHC ?! A case for the ILC
I discuss the question whether it is possible that the LHC will find no signal for the Higgs particle. It is argued that in this case singlet scalars should be present that could play an important role in astroparticle physics. A critical view at the existing electroweak data shows that this possibility might be favored over the simplest standard model. In this case one needs the ILC in order to study the Higgs sector.
hep-ph
i discuss the question whether it is possible that the lhc will find no signal for the higgs particle it is argued that in this case singlet scalars should be present that could play an important role in astroparticle physics a critical view at the existing electroweak data shows that this possibility might be favored over the simplest standard model in this case one needs the ilc in order to study the higgs sector
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707.0357
Relativistic Dynamics of Multi-BPS D-vortices and Straight BPS D-strings
Moduli space dynamics of multi-D-vortices from D2${\bar {\rm D}}$ (equivalently, parallel straight D-strings from D3${\bar {\rm D}}$3) is systematically studied. For the BPS D-vortices, we show through exact calculations that the classical motion of randomly-distributed $n$ D-vortices is governed by a relativistic Lagrangian of free massive point-particles. When the head-on collision of two identical BPS D-vortices of zero radius is considered, it predicts either 90${}^{\circ}$ scattering or 0${}^{\circ}$ scattering equivalent to 180${}^{\circ}$ scattering. Since the former leads to a reconnection of two identical D-strings and the latter does to a case of their passing through each other, two possibilities are consistent with the prediction of string theory. It is also shown that the force between two non-BPS vortices is repulsive. Although the obtained moduli space dynamics of multi-BPS-D-vortices is exact in classical regime, the quantum effect of an F-string pair production should be included in determining the probabilities of the reconnection and the passing through for fast-moving cosmic superstrings.
hep-th astro-ph
moduli space dynamics of multidvortices from d2bar rm d equivalently parallel straight dstrings from d3bar rm d3 is systematically studied for the bps dvortices we show through exact calculations that the classical motion of randomlydistributed n dvortices is governed by a relativistic lagrangian of free massive pointparticles when the headon collision of two identical bps dvortices of zero radius is considered it predicts either 90circ scattering or 0circ scattering equivalent to 180circ scattering since the former leads to a reconnection of two identical dstrings and the latter does to a case of their passing through each other two possibilities are consistent with the prediction of string theory it is also shown that the force between two nonbps vortices is repulsive although the obtained moduli space dynamics of multibpsdvortices is exact in classical regime the quantum effect of an fstring pair production should be included in determining the probabilities of the reconnection and the passing through for fastmoving cosmic superstrings
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707.0358
Spatial correlation of linear and nonlinear electron transport in superconducting microwave resonator: laser scanning microscopy analysis
Spatially-resolved techniques of laser scanning microscopy (LSM) have been used to image simultaneously the spatial variations of (i) rf current flow, J$_RF$(x,y), of (ii) areas of resistive dissipation and (iii) the sources of microwave nonlinearity (NL) in an operating superconducting resonator. The RF power dependent spatial evolution of these linear and NL microwave properties in the meander strip YBCO/LAO superconducting resonator have been LSM probed at different temperatures below Tc. The influence of both topologies of the twin-domain YBCO structure and of J$_RF$(x,y) peaks at the edges of superconducting strip line on its NL properties was analyzed in detail with a micron-scale spatial resolution. Result shows the resistive origin of the dominant sources of microwave NLs
cond-mat.supr-con cond-mat.mtrl-sci
spatiallyresolved techniques of laser scanning microscopy lsm have been used to image simultaneously the spatial variations of i rf current flow j_rfxy of ii areas of resistive dissipation and iii the sources of microwave nonlinearity nl in an operating superconducting resonator the rf power dependent spatial evolution of these linear and nl microwave properties in the meander strip ybcolao superconducting resonator have been lsm probed at different temperatures below tc the influence of both topologies of the twindomain ybco structure and of j_rfxy peaks at the edges of superconducting strip line on its nl properties was analyzed in detail with a micronscale spatial resolution result shows the resistive origin of the dominant sources of microwave nls
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707.0359
SM scalar and extra singlet(s)
I discuss the question whether it is possible that the LHC will find no signal for the Higgs boson. It is argued that in this case singlet scalars should be present that could play an important role in astroparticle physics. A critical view at the existing electroweak data shows that this possibility might be favored over the simplest standard model. In this case one needs the ILC in order to study the Higgs sector.
hep-ph
i discuss the question whether it is possible that the lhc will find no signal for the higgs boson it is argued that in this case singlet scalars should be present that could play an important role in astroparticle physics a critical view at the existing electroweak data shows that this possibility might be favored over the simplest standard model in this case one needs the ilc in order to study the higgs sector
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707.036
Effect of Co and Fe on the inverse magnetocaloric properties of Ni-Mn-Sn
At certain compositions Ni-Mn-$X$ Heusler alloys ($X$: group IIIA-VA elements) undergo martensitic transformations, and many of them exhibit inverse magnetocaloric effects. In alloys where $X$ is Sn, the isothermal entropy change is largest among the Heusler alloys, particularly in Ni$_{50}$Mn$_{37}$Sn$_{13}$ where it reaches a value of 20 Jkg$^{-1}$K$^{-1}$ for a field of 5T. We substitute Ni with Fe and Co in this alloy, each in amounts of 1 at% and 3 at% to perturb the electronic concentration and examine the resulting changes in the magnetocaloric properties. Increasing both Fe and Co concentrations causes the martensitic transition temperature to decrease, whereby the substitution by Co at both compositions or substituting 1 at% Fe leads to a decrease in the magnetocaloric effect. On the other hand, the magnetocaloric effect in the alloy with 3 at% Fe leads to an increase in the value of the entropy change to about 30 Jkg$^{-1}$K$^{-1}$ at 5T.
cond-mat.mtrl-sci
at certain compositions nimnx heusler alloys x group iiiava elements undergo martensitic transformations and many of them exhibit inverse magnetocaloric effects in alloys where x is sn the isothermal entropy change is largest among the heusler alloys particularly in ni_50mn_37sn_13 where it reaches a value of 20 jkg1k1 for a field of 5t we substitute ni with fe and co in this alloy each in amounts of 1 at and 3 at to perturb the electronic concentration and examine the resulting changes in the magnetocaloric properties increasing both fe and co concentrations causes the martensitic transition temperature to decrease whereby the substitution by co at both compositions or substituting 1 at fe leads to a decrease in the magnetocaloric effect on the other hand the magnetocaloric effect in the alloy with 3 at fe leads to an increase in the value of the entropy change to about 30 jkg1k1 at 5t
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707.0361
The curvature perturbation in a box
The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in a finite box. I discuss the reasons for that with reference the curvature perturbation, and explore some issues arising from it.
astro-ph gr-qc hep-ph hep-th
the stochastic properties of cosmological perturbations are best defined through the fourier expansion in a finite box i discuss the reasons for that with reference the curvature perturbation and explore some issues arising from it
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707.0362
On Fox and augmentation quotients of semidirect products
Let $G$ be a group which is the semidirect product of a normal subgroup $N$ and some subgroup $T$. Let $I^n(G)$, $n\ge 1$, denote the powers of the augmentation ideal $I(G)$ of the group ring $\Z(G)$. Using homological methods the groups $Q_n(G,H) = I^{n-1}(G)I(H)/I^{n}(G)I(H)$, $H=G,N,T$, are functorially expressed in terms of enveloping algebras of certain Lie rings associated with $N$ and $T$, in the following cases: for $n\le 4$ and arbitrary $G,N,T$ (except from one direct summand of $Q_4(G,N)$), and for all $n\ge 2$ if certain filtration quotients of $N$ and $T$ are torsionfree.
math.GR math.RA
let g be a group which is the semidirect product of a normal subgroup n and some subgroup t let ing nge 1 denote the powers of the augmentation ideal ig of the group ring zg using homological methods the groups q_ngh in1gihingih hgnt are functorially expressed in terms of enveloping algebras of certain lie rings associated with n and t in the following cases for nle 4 and arbitrary gnt except from one direct summand of q_4gn and for all nge 2 if certain filtration quotients of n and t are torsionfree
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707.0363
Detecting bubbles in exotic nuclei
The occurrence of a bubble, due to an inversion of s$_{1/2}$ state with the state usually located above, is investigated. Proton bubbles in neutron-rich Argon isotopes are optimal candidates. Pairing effects which can play against the bubble formation are evaluated. They cannot prevent bubble formation in very neutron-rich argon isotopes such as $^{68}$Ar. This pleads for a measurement of the charge density of neutron-rich argon isotopes in the forthcoming years, with the advent of electron scattering experiments in next generation exotic beam facilities such as FAIR or RIBF.
nucl-th nucl-ex
the occurrence of a bubble due to an inversion of s_12 state with the state usually located above is investigated proton bubbles in neutronrich argon isotopes are optimal candidates pairing effects which can play against the bubble formation are evaluated they cannot prevent bubble formation in very neutronrich argon isotopes such as 68ar this pleads for a measurement of the charge density of neutronrich argon isotopes in the forthcoming years with the advent of electron scattering experiments in next generation exotic beam facilities such as fair or ribf
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707.0364
Polarization types of isogenous Prym-Tyurin varieties
Let p:C-->Y be a covering of smooth, projective curves which is a composition of \pi:C-->C' of degree 2 and g:C'-->Y of degree n. Let f:X-->Y be the covering of degree 2^n, where the curve X parametrizes the liftings in C^{(n)} of the fibers of g:C'-->Y. Let P(X,\delta) be the associated Prym-Tyurin variety, known to be isogenous to the Prym variety P(C,C'). Most of the results in the paper focus on calculating the polarization type of the restriction of the canonical polarization of JX on P(X,\delta). We obtain the polarization type when n=3. When Y=P^1 we conjecture that P(X,\delta) is isomorphic to the dual of the Prym variety P(C,C'). This was known when n=2, we prove it when n=3, and for arbitrary n if \pi:C-->C' is \'{e}tale. Similar results are obtained for some other types of coverings.
math.AG
let pcy be a covering of smooth projective curves which is a composition of picc of degree 2 and gcy of degree n let fxy be the covering of degree 2n where the curve x parametrizes the liftings in cn of the fibers of gcy let pxdelta be the associated prymtyurin variety known to be isogenous to the prym variety pcc most of the results in the paper focus on calculating the polarization type of the restriction of the canonical polarization of jx on pxdelta we obtain the polarization type when n3 when yp1 we conjecture that pxdelta is isomorphic to the dual of the prym variety pcc this was known when n2 we prove it when n3 and for arbitrary n if picc is etale similar results are obtained for some other types of coverings
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707.0365
Performance Analysis of Publish/Subscribe Systems
The Desktop Grid offers solutions to overcome several challenges and to answer increasingly needs of scientific computing. Its technology consists mainly in exploiting resources, geographically dispersed, to treat complex applications needing big power of calculation and/or important storage capacity. However, as resources number increases, the need for scalability, self-organisation, dynamic reconfigurations, decentralisation and performance becomes more and more essential. Since such properties are exhibited by P2P systems, the convergence of grid computing and P2P computing seems natural. In this context, this paper evaluates the scalability and performance of P2P tools for discovering and registering services. Three protocols are used for this purpose: Bonjour, Avahi and Free-Pastry. We have studied the behaviour of theses protocols related to two criteria: the elapsed time for registrations services and the needed time to discover new services. Our aim is to analyse these results in order to choose the best protocol we can use in order to create a decentralised middleware for desktop grid.
cs.DC
the desktop grid offers solutions to overcome several challenges and to answer increasingly needs of scientific computing its technology consists mainly in exploiting resources geographically dispersed to treat complex applications needing big power of calculation andor important storage capacity however as resources number increases the need for scalability selforganisation dynamic reconfigurations decentralisation and performance becomes more and more essential since such properties are exhibited by p2p systems the convergence of grid computing and p2p computing seems natural in this context this paper evaluates the scalability and performance of p2p tools for discovering and registering services three protocols are used for this purpose bonjour avahi and freepastry we have studied the behaviour of theses protocols related to two criteria the elapsed time for registrations services and the needed time to discover new services our aim is to analyse these results in order to choose the best protocol we can use in order to create a decentralised middleware for desktop grid
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707.0366
Willmore Legendrian surfaces in pseudoconformal 5-sphere
Let $ X: M \hook S^5$ be a compact Legendrian surface in pseudoconformal(CR) 5-sphere. We introduce a pseudoconformally invariant Willmore type second order functional $ \W(X)$, and study its critical points called Willmore Legendrian surfaces. The fifth order structure equations show that Willmore dual can be defined for a class of Willmore Legendrian surfaces. Moreover when this dual is constant, Willmore Legendrian surface admits a Weierstra\ss type representation in terms of immersed meromorphic curve in $ \C^2$ satisfying an appropriate real period condition via pseudoconformal stereographic projection. We show that every compact Riemann surface admits a generally one to one, conformal, Willmore Legendrian immersion in $ S^5$ with constant Willmore dual. As a corollary, every compact Riemann surface can be conformally immersed in $ \C^2$ as an exact, algebraic Lagrangian surface.
math.DG math.AP
let x m hook s5 be a compact legendrian surface in pseudoconformalcr 5sphere we introduce a pseudoconformally invariant willmore type second order functional wx and study its critical points called willmore legendrian surfaces the fifth order structure equations show that willmore dual can be defined for a class of willmore legendrian surfaces moreover when this dual is constant willmore legendrian surface admits a weierstrass type representation in terms of immersed meromorphic curve in c2 satisfying an appropriate real period condition via pseudoconformal stereographic projection we show that every compact riemann surface admits a generally one to one conformal willmore legendrian immersion in s5 with constant willmore dual as a corollary every compact riemann surface can be conformally immersed in c2 as an exact algebraic lagrangian surface
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707.0367
Radial Dunkl Processes : Existence and uniqueness, Hitting time, Beta Processes and Random Matrices
We begin with the study of some properties of the radial Dunkl process associated to a reduced root system $R$. It is shown that this diffusion is the unique strong solution for all $t \geq 0$ of a SDE with singular drift. Then, we study $T_0$, the first hitting time of the positive Weyl chamber : we prove, via stochastic calculus, a result already obtained by Chybiryakov on the finiteness of $T_0$. The second and new part deals with the law of $T_0$ for which we compute the tail distribution, as well as some insight via stochastic calculus on how root systems are connected with eigenvalues of standard matrix-valued processes. This gives rise to the so-called $\beta$-processes. The ultraspherical $\beta$-Jacobi case still involves a reduced root system while the general case is closely connected to a non reduced one. This process lives in a convex bounded domain known as principal Weyl alcove and the strong uniqueness result remains valid. The last part deals with the first hitting time of the alcove's boundary and the semi group density which enables us to answer some open questions.
math.PR
we begin with the study of some properties of the radial dunkl process associated to a reduced root system r it is shown that this diffusion is the unique strong solution for all t geq 0 of a sde with singular drift then we study t_0 the first hitting time of the positive weyl chamber we prove via stochastic calculus a result already obtained by chybiryakov on the finiteness of t_0 the second and new part deals with the law of t_0 for which we compute the tail distribution as well as some insight via stochastic calculus on how root systems are connected with eigenvalues of standard matrixvalued processes this gives rise to the socalled betaprocesses the ultraspherical betajacobi case still involves a reduced root system while the general case is closely connected to a non reduced one this process lives in a convex bounded domain known as principal weyl alcove and the strong uniqueness result remains valid the last part deals with the first hitting time of the alcoves boundary and the semi group density which enables us to answer some open questions
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707.0368
Stochastic background of relic scalar gravitational waves from scalar-tensor gravity
A stochastic background of relic gravitational waves is achieved by the so called adiabatically-amplified zero-point fluctuations process derived from early inflation. In principle, it provides a distinctive spectrum of relic gravitational waves. In the framework of scalar-tensor gravity, we discuss the scalar modes of gravitational waves and the primordial production of this scalar component which is generated beside tensorial one. We discuss also the upper limit for such a relic scalar component with respect to the WMAP constraints.
gr-qc
a stochastic background of relic gravitational waves is achieved by the so called adiabaticallyamplified zeropoint fluctuations process derived from early inflation in principle it provides a distinctive spectrum of relic gravitational waves in the framework of scalartensor gravity we discuss the scalar modes of gravitational waves and the primordial production of this scalar component which is generated beside tensorial one we discuss also the upper limit for such a relic scalar component with respect to the wmap constraints
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707.0369
Numerical study of the influence of an applied electrical potential on the solidification of a binary metal alloy
In this work we study numerically the influence of a homogeneous electrical field on the fluid and heat transfer phenomena at macroscale and mesoscale during unidirectional solidification of a binary metal alloy. The numerical results showed that a pulse electric discharging applied perpendicularly to the solidification front leads to a much stronger Joule heating of the liquid phase in comparison to the solid phase. It was found that on the mesoscopic scale the electric current density is not homogeneous due to the complex shape of the dendrite and the difference between electrical conductivities of the solid and liquid phases. This inhomogeneity of the electrical current density in the mushy zone leads to the increase of the Joule heating of the dendrite in comparison to the interdendritic liquid and induces a pinch force (electromagnetic Lorentz force). The main features of the resulting convection in the interdendritic liquid are discussed.
cond-mat.mtrl-sci cond-mat.other
in this work we study numerically the influence of a homogeneous electrical field on the fluid and heat transfer phenomena at macroscale and mesoscale during unidirectional solidification of a binary metal alloy the numerical results showed that a pulse electric discharging applied perpendicularly to the solidification front leads to a much stronger joule heating of the liquid phase in comparison to the solid phase it was found that on the mesoscopic scale the electric current density is not homogeneous due to the complex shape of the dendrite and the difference between electrical conductivities of the solid and liquid phases this inhomogeneity of the electrical current density in the mushy zone leads to the increase of the joule heating of the dendrite in comparison to the interdendritic liquid and induces a pinch force electromagnetic lorentz force the main features of the resulting convection in the interdendritic liquid are discussed
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707.037
Efficient dynamical nuclear polarization in quantum dots: Temperature dependence
We investigate in micro-photoluminescence experiments the dynamical nuclear polarization in individual InGaAs quantum dots. Experiments carried out in an applied magnetic field of 2T show that the nuclear polarization achieved through the optical pumping of electron spins is increasing with the sample temperature between 2K and 55K, reaching a maximum of about 50%. Analysing the dependence of the Overhauser shift on the spin polarization of the optically injected electron as a function of temperature enables us to identify the main reasons for this increase.
cond-mat.other
we investigate in microphotoluminescence experiments the dynamical nuclear polarization in individual ingaas quantum dots experiments carried out in an applied magnetic field of 2t show that the nuclear polarization achieved through the optical pumping of electron spins is increasing with the sample temperature between 2k and 55k reaching a maximum of about 50 analysing the dependence of the overhauser shift on the spin polarization of the optically injected electron as a function of temperature enables us to identify the main reasons for this increase
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707.0371
Quadratic maps between groups
The notion of quadratic maps between arbitrary groups appeared at several places in the literature on quadratic algebra. Here a unified extensive treatment of their properties is given; the relation with a relative version of Passi's polynomial maps and groups of degree 2 is established and used to study the structure of the latter.
math.GR math.RA
the notion of quadratic maps between arbitrary groups appeared at several places in the literature on quadratic algebra here a unified extensive treatment of their properties is given the relation with a relative version of passis polynomial maps and groups of degree 2 is established and used to study the structure of the latter
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707.0372
Regulators of canonical extensions are torsion: the smooth divisor case
In this paper, we prove a generalization of Reznikov's theorem which says that the Chern-Simons classes and in particular the Deligne Chern classes (in degrees $>1$) are torsion, of a flat bundle on a smooth complex projective variety. We consider the case of a smooth quasi--projective variety with an irreducible smooth divisor at infinity. We define the Chern-Simons classes of Deligne's canonical extension of a flat vector bundle with unipotent monodromy at infinity, which lift the Deligne Chern classes and prove that these classes are torsion.
math.AG
in this paper we prove a generalization of reznikovs theorem which says that the chernsimons classes and in particular the deligne chern classes in degrees 1 are torsion of a flat bundle on a smooth complex projective variety we consider the case of a smooth quasiprojective variety with an irreducible smooth divisor at infinity we define the chernsimons classes of delignes canonical extension of a flat vector bundle with unipotent monodromy at infinity which lift the deligne chern classes and prove that these classes are torsion
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707.0373
Search for invisibly decaying Higgs bosons in e+e- -> Zoho production at sqrt(s) = 183 - 209 GeV
A search is performed for Higgs bosons decaying into invisible final states, produced in association with a Zo boson in e+e- collisions at energies between 183 and 209 GeV. The search is based on data samples collected by the OPAL detector at LEP corresponding to an integrated luminosity of about 660 pb-1. The analysis aims to select events containing the hadronic decay products of the Zo boson and large missing momentum, as expected from Higgs boson decay into a pair of stable weakly interacting neutral particles, such as the lightest neutralino in the Minimal Supersymmetric Standard Model. The same analysis is applied to a search for nearly invisible Higgs boson cascade decays into stable weakly interacting neutral particles. No excess over the expected background from Standard Model processes is observed. Limits on the production of invisibly decaying Higgs bosons produced in association with a Zo boson are derived. Assuming a branching ratio BR(ho->invisible)=1, a lower limit of 108.2 GeV is placed on the Higgs boson mass at the 95% confidence level. Limits on the production of nearly invisibly decaying Higgs bosons are also obtained.
hep-ex
a search is performed for higgs bosons decaying into invisible final states produced in association with a zo boson in ee collisions at energies between 183 and 209 gev the search is based on data samples collected by the opal detector at lep corresponding to an integrated luminosity of about 660 pb1 the analysis aims to select events containing the hadronic decay products of the zo boson and large missing momentum as expected from higgs boson decay into a pair of stable weakly interacting neutral particles such as the lightest neutralino in the minimal supersymmetric standard model the same analysis is applied to a search for nearly invisible higgs boson cascade decays into stable weakly interacting neutral particles no excess over the expected background from standard model processes is observed limits on the production of invisibly decaying higgs bosons produced in association with a zo boson are derived assuming a branching ratio brhoinvisible1 a lower limit of 1082 gev is placed on the higgs boson mass at the 95 confidence level limits on the production of nearly invisibly decaying higgs bosons are also obtained
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707.0374
Vibration diagnostics instrumentation for ILC
The future e-e+ 500 GeV International Linear Collider will rely on unprecedented nanometer scale particle beam size at the interaction point, in order to achieve the design luminosity. Tight tolerances on static and dynamic alignment of the accelerator cavities and optical components are demanded to transport and focus the high energy electron and positron beams with reasonable position jitter and low emittance. A brief review of techniques and devices evaluated and developed so far for the vibration diagnostics of the machine is presented in this paper.
physics.ins-det physics.acc-ph
the future ee 500 gev international linear collider will rely on unprecedented nanometer scale particle beam size at the interaction point in order to achieve the design luminosity tight tolerances on static and dynamic alignment of the accelerator cavities and optical components are demanded to transport and focus the high energy electron and positron beams with reasonable position jitter and low emittance a brief review of techniques and devices evaluated and developed so far for the vibration diagnostics of the machine is presented in this paper
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707.0375
Performance limits of graphene-ribbon-based field effect transistors
The performance of field effect transistors based on an single graphene ribbon with a constriction and a single back gate are studied with the help of atomistic models. It is shown how this scheme, unlike that of traditional carbon-nanotube-based transistors, reduces the importance of the specifics of the chemical bonding to the metallic electrodes in favor of the carbon-based part of device. The ultimate performance limits are here studied for various constriction and metal-ribbon contact models. In particular we show that, even for poorly contacting metals, properly taylored constrictions can give promising values for both the on-conductance and the subthreshold swing.
cond-mat.mes-hall cond-mat.mtrl-sci
the performance of field effect transistors based on an single graphene ribbon with a constriction and a single back gate are studied with the help of atomistic models it is shown how this scheme unlike that of traditional carbonnanotubebased transistors reduces the importance of the specifics of the chemical bonding to the metallic electrodes in favor of the carbonbased part of device the ultimate performance limits are here studied for various constriction and metalribbon contact models in particular we show that even for poorly contacting metals properly taylored constrictions can give promising values for both the onconductance and the subthreshold swing
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707.0376
Self Improving Sobolev-Poincare Inequalities, Truncation and Symmetrization
In a previous paper we developed a new method to obtain symmetrization inequalities of Sobolev type for functions in $W_{0}^{1,1}(\Omega)$. In this paper we extend our method to Sobolev functions that do not vanish at the boundary.
math.FA math.AP
in a previous paper we developed a new method to obtain symmetrization inequalities of sobolev type for functions in w_011omega in this paper we extend our method to sobolev functions that do not vanish at the boundary
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707.0377
Analysis of Emission Shapes
Shapes of relative emission sources can be accessed by expanding shapes of correlations at low relative velocities in pair center of mass in Cartesian harmonics. Coefficients of expansion for correlations are related to the respective coefficients of expansion for the sources through one dimensional integral transforms involving properties of pair relative wavefunctions. The methodology is illustrated with analyses of NA49 and PHENIX correlation data.
nucl-th
shapes of relative emission sources can be accessed by expanding shapes of correlations at low relative velocities in pair center of mass in cartesian harmonics coefficients of expansion for correlations are related to the respective coefficients of expansion for the sources through one dimensional integral transforms involving properties of pair relative wavefunctions the methodology is illustrated with analyses of na49 and phenix correlation data
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707.0378
CP violation in scatterings, three body processes and the Boltzmann equations for leptogenesis
We obtain the Boltzmann equations for leptogenesis including decay and scattering processes with two and three body initial or final states. We present an explicit computation of the CP violating scattering asymmetries. We analyze their possible impact in leptogenesis, and we discuss the validity of their approximate expressions in terms of the decay asymmetry. In scenarios in which the initial heavy neutrino density vanishes, the inclusion of CP asymmetries in scatterings can enforce a cancellation between the lepton asymmetry generated at early times and the asymmetry produced at later times. We argue that a sizeable amount of washout is crucial for spoiling this cancellation, and we show that in the regimes in which the washouts are particularly weak, the inclusion of CP violation in scatterings yields a reduction in the final value of the lepton asymmetry. In the strong washout regimes the inclusion of CP violation in scatterings still leads to a significant enhancement of the lepton asymmetry at high temperatures; however, due to the independence from the early conditions that is characteristic of these regimes, the final value of the lepton asymmetry remains approximately unchanged.
hep-ph
we obtain the boltzmann equations for leptogenesis including decay and scattering processes with two and three body initial or final states we present an explicit computation of the cp violating scattering asymmetries we analyze their possible impact in leptogenesis and we discuss the validity of their approximate expressions in terms of the decay asymmetry in scenarios in which the initial heavy neutrino density vanishes the inclusion of cp asymmetries in scatterings can enforce a cancellation between the lepton asymmetry generated at early times and the asymmetry produced at later times we argue that a sizeable amount of washout is crucial for spoiling this cancellation and we show that in the regimes in which the washouts are particularly weak the inclusion of cp violation in scatterings yields a reduction in the final value of the lepton asymmetry in the strong washout regimes the inclusion of cp violation in scatterings still leads to a significant enhancement of the lepton asymmetry at high temperatures however due to the independence from the early conditions that is characteristic of these regimes the final value of the lepton asymmetry remains approximately unchanged
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707.0379
Dependence of Resonant Absorption Linewidth on Atomic Vapour Column Thickness for D1 Line of Cs Atoms Confined in Nano-Cell
A new nano-cell with smoothly varying longitudinal thickness of the atomic vapour layer L in the range of 350 - 5100 nm allowing to study the resonant absorption of D1 and D2 lines of Cs atoms for thicknesses changing from L = Lambda/2 to L = 6 Lambda with the step of Lambda/2 (Lambda = 852 nm or 894 nm are the resonant laser wavelengths) and for different intensities is developed. It is revealed that for low laser intensities there is narrowing of the resonant absorption spectrum for the thicknesses L = (2n + 1)Lambda/2 (where n is an integer) up to L = 7Lambda /2 and broadening of the spectrum for L = n Lambda. For relatively high laser intensity (>1 mW/cm2), velocity selective optical pumping/saturated resonances of a reduced absorption (with the line-width close to the natural one), and centred on the hyperfine transitions occur when L = n Lambda. The possible application of these resonance peaks is given. The developed theoretical model describes well the experiment.
physics.atom-ph
a new nanocell with smoothly varying longitudinal thickness of the atomic vapour layer l in the range of 350 5100 nm allowing to study the resonant absorption of d1 and d2 lines of cs atoms for thicknesses changing from l lambda2 to l 6 lambda with the step of lambda2 lambda 852 nm or 894 nm are the resonant laser wavelengths and for different intensities is developed it is revealed that for low laser intensities there is narrowing of the resonant absorption spectrum for the thicknesses l 2n 1lambda2 where n is an integer up to l 7lambda 2 and broadening of the spectrum for l n lambda for relatively high laser intensity 1 mwcm2 velocity selective optical pumpingsaturated resonances of a reduced absorption with the linewidth close to the natural one and centred on the hyperfine transitions occur when l n lambda the possible application of these resonance peaks is given the developed theoretical model describes well the experiment
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707.038
Expanding Space: the Root of all Evil?
While it remains the staple of virtually all cosmological teaching, the concept of expanding space in explaining the increasing separation of galaxies has recently come under fire as a dangerous idea whose application leads to the development of confusion and the establishment of misconceptions. In this paper, we develop a notion of expanding space that is completely valid as a framework for the description of the evolution of the universe and whose application allows an intuitive understanding of the influence of universal expansion. We also demonstrate how arguments against the concept in general have failed thus far, as they imbue expanding space with physical properties not consistent with the expectations of general relativity.
astro-ph gr-qc physics.ed-ph
while it remains the staple of virtually all cosmological teaching the concept of expanding space in explaining the increasing separation of galaxies has recently come under fire as a dangerous idea whose application leads to the development of confusion and the establishment of misconceptions in this paper we develop a notion of expanding space that is completely valid as a framework for the description of the evolution of the universe and whose application allows an intuitive understanding of the influence of universal expansion we also demonstrate how arguments against the concept in general have failed thus far as they imbue expanding space with physical properties not consistent with the expectations of general relativity
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707.0381
Strong and electroweak corrections to the production of Higgs+2jets via weak interactions at the LHC
Radiative corrections of strong and electroweak interactions are presented at next-to-leading order for the production of a Higgs boson plus two hard jets via weak interactions at the LHC. The calculation includes all weak-boson fusion and quark-antiquark annihilation diagrams as well as the corresponding interferences. The electroweak corrections, which are discussed here for the first time, reduce the cross sections by 5%, and thus are of the same order of magnitude as the QCD corrections. As argued in previous papers, where s-channel diagrams and interferences were neglected, the QCD corrections connected to interference effects are small.
hep-ph
radiative corrections of strong and electroweak interactions are presented at nexttoleading order for the production of a higgs boson plus two hard jets via weak interactions at the lhc the calculation includes all weakboson fusion and quarkantiquark annihilation diagrams as well as the corresponding interferences the electroweak corrections which are discussed here for the first time reduce the cross sections by 5 and thus are of the same order of magnitude as the qcd corrections as argued in previous papers where schannel diagrams and interferences were neglected the qcd corrections connected to interference effects are small
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707.0382
Why are accreting T Tauri stars less luminous in X-rays than non-accretors?
Accreting T Tauri stars are observed to be less luminous in X-rays than non-accretors, an effect that has been detected in various star forming regions. To explain this we have combined, for the first time, a radiative transfer code with an accretion model that considers magnetic fields extrapolated from surface magnetograms obtained from Zeeman-Doppler imaging. Such fields consist of compact magnetic regions close to the stellar surface, with extended field lines interacting with the disk. We study the propagation of coronal X-rays through the magnetosphere and demonstrate that they are strongly absorbed by the dense gas in accretion columns.
astro-ph
accreting t tauri stars are observed to be less luminous in xrays than nonaccretors an effect that has been detected in various star forming regions to explain this we have combined for the first time a radiative transfer code with an accretion model that considers magnetic fields extrapolated from surface magnetograms obtained from zeemandoppler imaging such fields consist of compact magnetic regions close to the stellar surface with extended field lines interacting with the disk we study the propagation of coronal xrays through the magnetosphere and demonstrate that they are strongly absorbed by the dense gas in accretion columns
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707.0383
Pair condensation of bosonic atoms induced by optical lattices
We design a model of correlated hopping for bosonic atoms in optical lattices. Such model exhibits three kinds of phases, comprehending a Mott insulator, a charge density wave and a pair quasi-condensate. The implementation of the model relies on two-state atoms embedded in state-dependent lattices and having spin-dependent interactions. Contrary to other models of pairing, our design is not based on perturbative effects and should be observable in current experiments.
cond-mat.other quant-ph
we design a model of correlated hopping for bosonic atoms in optical lattices such model exhibits three kinds of phases comprehending a mott insulator a charge density wave and a pair quasicondensate the implementation of the model relies on twostate atoms embedded in statedependent lattices and having spindependent interactions contrary to other models of pairing our design is not based on perturbative effects and should be observable in current experiments
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707.0384
Ab-initio calculation of phonon dispersion curves: accelerating q point convergence
We present a scheme for the improved description of the long-range interatomic force constants in a more accurate way than the procedure which is commonly used within plane-wave based density-functional perturbation-theory calculations. Our scheme is based on the inclusion of a q point grid which is denser in a restricted area around the center of the Brillouin Zone than in the remaining parts, even though the method is not limited to an area around Gamma. We have tested the validity of our procedure in the case of high-pressure phases of bulk silicon considering the bct and sh structure.
cond-mat.mtrl-sci cond-mat.dis-nn cond-mat.mes-hall cond-mat.other cond-mat.soft cond-mat.stat-mech
we present a scheme for the improved description of the longrange interatomic force constants in a more accurate way than the procedure which is commonly used within planewave based densityfunctional perturbationtheory calculations our scheme is based on the inclusion of a q point grid which is denser in a restricted area around the center of the brillouin zone than in the remaining parts even though the method is not limited to an area around gamma we have tested the validity of our procedure in the case of highpressure phases of bulk silicon considering the bct and sh structure
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707.0385
Specialization of strategies and herding behavior of trading firms in a financial market
The understanding of complex social or economic systems is an important scientific challenge. Here we present a comprehensive study of the Spanish Stock Exchange showing that most financial firms trading in that market are characterized by a resulting strategy and can be classified in groups of firms with different specialization. Few large firms overally act as trending firms whereas many heterogeneous firm act as reversing firms. The herding properties of these two groups are markedly different and consistently observed over a four-year period of trading.
q-fin.ST physics.soc-ph
the understanding of complex social or economic systems is an important scientific challenge here we present a comprehensive study of the spanish stock exchange showing that most financial firms trading in that market are characterized by a resulting strategy and can be classified in groups of firms with different specialization few large firms overally act as trending firms whereas many heterogeneous firm act as reversing firms the herding properties of these two groups are markedly different and consistently observed over a fouryear period of trading
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707.0386
BRST approach to Lagrangian formulation for mixed-symmetry fermionic higher-spin fields
We construct a Lagrangian description of irreducible half-integer higher-spin representations of the Poincare group with the corresponding Young tableaux having two rows, on a basis of the BRST approach. Starting with a description of fermionic higher-spin fields in a flat space of any dimension in terms of an auxiliary Fock space, we realize a conversion of the initial operator constraint system (constructed with respect to the relations extracting irreducible Poincare-group representations) into a first-class constraint system. For this purpose, we find auxiliary representations of the constraint subsuperalgebra containing the subsystem of second-class constraints in terms of Verma modules. We propose a universal procedure of constructing gauge-invariant Lagrangians with reducible gauge symmetries describing the dynamics of both massless and massive fermionic fields of any spin. No off-shell constraints for the fields and gauge parameters are used from the very beginning. It is shown that the space of BRST cohomologies with a vanishing ghost number is determined only by the constraints corresponding to an irreducible Poincare-group representation. To illustrate the general construction, we obtain a Lagrangian description of fermionic fields with generalized spin (3/2,1/2) and (3/2,3/2) on a flat background containing the complete set of auxiliary fields and gauge symmetries.
hep-th
we construct a lagrangian description of irreducible halfinteger higherspin representations of the poincare group with the corresponding young tableaux having two rows on a basis of the brst approach starting with a description of fermionic higherspin fields in a flat space of any dimension in terms of an auxiliary fock space we realize a conversion of the initial operator constraint system constructed with respect to the relations extracting irreducible poincaregroup representations into a firstclass constraint system for this purpose we find auxiliary representations of the constraint subsuperalgebra containing the subsystem of secondclass constraints in terms of verma modules we propose a universal procedure of constructing gaugeinvariant lagrangians with reducible gauge symmetries describing the dynamics of both massless and massive fermionic fields of any spin no offshell constraints for the fields and gauge parameters are used from the very beginning it is shown that the space of brst cohomologies with a vanishing ghost number is determined only by the constraints corresponding to an irreducible poincaregroup representation to illustrate the general construction we obtain a lagrangian description of fermionic fields with generalized spin 3212 and 3232 on a flat background containing the complete set of auxiliary fields and gauge symmetries
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707.0387
Planar Homological Mirror Symmetry
In this article, we formulate a planar limited version of the B-side in homological mirror symmetry that formularizes Chern-Simons-type topological open string field theory using homotopy associative algebra ($A_{\infty}$ algebra). This formulation is based on the works by Dijkgraaf and Vafa. We show that our formularization includes gravity/gauge theory correspondence which originates in the AdS/CFT duality of Dijkgraaf-Vafa theory.
hep-th math.AG math.SG
in this article we formulate a planar limited version of the bside in homological mirror symmetry that formularizes chernsimonstype topological open string field theory using homotopy associative algebra a_infty algebra this formulation is based on the works by dijkgraaf and vafa we show that our formularization includes gravitygauge theory correspondence which originates in the adscft duality of dijkgraafvafa theory
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707.0388
From boundary to bulk in logarithmic CFT
The analogue of the charge-conjugation modular invariant for rational logarithmic conformal field theories is constructed. This is done by reconstructing the bulk spectrum from a simple boundary condition (the analogue of the Cardy `identity brane'). We apply the general method to the c_1,p triplet models and reproduce the previously known bulk theory for p=2 at c=-2. For general p we verify that the resulting partition functions are modular invariant. We also construct the complete set of 2p boundary states, and confirm that the identity brane from which we started indeed exists. As a by-product we obtain a logarithmic version of the Verlinde formula for the c_1,p triplet models.
hep-th math.QA
the analogue of the chargeconjugation modular invariant for rational logarithmic conformal field theories is constructed this is done by reconstructing the bulk spectrum from a simple boundary condition the analogue of the cardy identity brane we apply the general method to the c_1p triplet models and reproduce the previously known bulk theory for p2 at c2 for general p we verify that the resulting partition functions are modular invariant we also construct the complete set of 2p boundary states and confirm that the identity brane from which we started indeed exists as a byproduct we obtain a logarithmic version of the verlinde formula for the c_1p triplet models
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707.0389
A remark on fractional integrals on modulation spaces
In this paper, we give the necessary and sufficient conditions for the boundedness of fractional integral operators on the modulation spaces.
math.FA math.AP
in this paper we give the necessary and sufficient conditions for the boundedness of fractional integral operators on the modulation spaces
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707.039
The York Map and the Role of Non-Inertial Frames in the Geometrical View of the Gravitational Field
The role of non-inertial frames in a class of models of general relativity is clarified by means of Dirac's theory of constraints. The identification of a York canonical basis allows to give the interpretation of the gauge variables as generalized inertial effects and to identify the Dirac observables of the gravitational field with generalized tidal effects. York time is the gauge variable controlling the clock synchronization convention. Differently from special relativity, the instantaneous 3-spaces are dynamically determined.
gr-qc astro-ph hep-th
the role of noninertial frames in a class of models of general relativity is clarified by means of diracs theory of constraints the identification of a york canonical basis allows to give the interpretation of the gauge variables as generalized inertial effects and to identify the dirac observables of the gravitational field with generalized tidal effects york time is the gauge variable controlling the clock synchronization convention differently from special relativity the instantaneous 3spaces are dynamically determined
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707.0391
On the $L^2$-boundedness of pseudo-differential operators and their commutators with symbols in $\alpha$-modulation spaces
In this paper, we consider the $L^2$-boundedness of pseudo-differential operators with symbols in $\alpha$-modulation spaces.
math.FA math.AP
in this paper we consider the l2boundedness of pseudodifferential operators with symbols in alphamodulation spaces
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707.0392
Measurement of the Strong Coupling alpha_s from the Four-Jet Rate in e+e- Annihilation using JADE data
Data from e+e- annihilation into hadrons collected by the JADE experiment at centre-of-mass energies between 14 GeV and 44 GeV are used to study the four-jet event production rate as a function of the Durham jet algorithm's resolution parameter ycut. The four-jet rate is compared to QCD next-to-leading order calculations including resummation of large logarithms in the next-to-leading logarithmic approximation. The strong coupling measured from the four-jet rate is as(MZ)=0.1159+-0.0004(stat)+-0.0012(expt)+-0.0024(had)+-0.0007(theo) in agreement with the world average.
hep-ex
data from ee annihilation into hadrons collected by the jade experiment at centreofmass energies between 14 gev and 44 gev are used to study the fourjet event production rate as a function of the durham jet algorithms resolution parameter ycut the fourjet rate is compared to qcd nexttoleading order calculations including resummation of large logarithms in the nexttoleading logarithmic approximation the strong coupling measured from the fourjet rate is asmz0115900004stat00012expt00024had00007theo in agreement with the world average
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707.0393
Supernovae in the Subaru Deep Field: An Initial Sample, and Type Ia Rate, out to Redshift 1.6
Large samples of high-redshift supernovae (SNe) are potentially powerful probes of cosmic star formation, metal enrichment, and SN physics. We present initial results from a new deep SN survey, based on re-imaging in the R, i', z' bands, of the 0.25 deg2 Subaru Deep Field (SDF), with the 8.2-m Subaru telescope and Suprime-Cam. In a single new epoch consisting of two nights of observations, we have discovered 33 candidate SNe, down to a z'-band magnitude of 26.3 (AB). We have measured the photometric redshifts of the SN host galaxies, obtained Keck spectroscopic redshifts for 17 of the host galaxies, and classified the SNe using the Bayesian photometric algorithm of Poznanski et al. (2007) that relies on template matching. After correcting for biases in the classification, 55% of our sample consists of Type Ia supernovae and 45% of core-collapse SNe. The redshift distribution of the SNe Ia reaches z ~ 1.6, with a median of z ~ 1.2. The core-collapse SNe reach z ~ 1.0, with a median of z ~ 0.5. Our SN sample is comparable to the Hubble Space Telescope/GOODS sample both in size and redshift range. The redshift distributions of the SNe in the SDF and in GOODS are consistent, but there is a trend (which requires confirmation using a larger sample) for more high-z SNe Ia in the SDF. This trend is also apparent when comparing the SN Ia rates we derive to those based on GOODS data. Our results suggest a fairly constant rate at high redshift that could be tracking the star-formation rate. Additional epochs on this field, already being obtained, will enlarge our SN sample to the hundreds, and determine whether or not there is a decline in the SN Ia rate at z >~ 1.
astro-ph
large samples of highredshift supernovae sne are potentially powerful probes of cosmic star formation metal enrichment and sn physics we present initial results from a new deep sn survey based on reimaging in the r i z bands of the 025 deg2 subaru deep field sdf with the 82m subaru telescope and suprimecam in a single new epoch consisting of two nights of observations we have discovered 33 candidate sne down to a zband magnitude of 263 ab we have measured the photometric redshifts of the sn host galaxies obtained keck spectroscopic redshifts for 17 of the host galaxies and classified the sne using the bayesian photometric algorithm of poznanski et al 2007 that relies on template matching after correcting for biases in the classification 55 of our sample consists of type ia supernovae and 45 of corecollapse sne the redshift distribution of the sne ia reaches z 16 with a median of z 12 the corecollapse sne reach z 10 with a median of z 05 our sn sample is comparable to the hubble space telescopegoods sample both in size and redshift range the redshift distributions of the sne in the sdf and in goods are consistent but there is a trend which requires confirmation using a larger sample for more highz sne ia in the sdf this trend is also apparent when comparing the sn ia rates we derive to those based on goods data our results suggest a fairly constant rate at high redshift that could be tracking the starformation rate additional epochs on this field already being obtained will enlarge our sn sample to the hundreds and determine whether or not there is a decline in the sn ia rate at z 1
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707.0394
Identification of candidate regulatory sequences in mammalian 3' UTRs by statistical analysis of oligonucleotide distributions
3' untranslated regions (3' UTRs) contain binding sites for many regulatory elements, and in particular for microRNAs (miRNAs). The importance of miRNA-mediated post-transcriptional regulation has become increasingly clear in the last few years. We propose two complementary approaches to the statistical analysis of oligonucleotide frequencies in mammalian 3' UTRs aimed at the identification of candidate binding sites for regulatory elements. The first method is based on the identification of sets of genes characterized by evolutionarily conserved overrepresentation of an oligonucleotide. The second method is based on the identification of oligonucleotides showing statistically significant strand asymmetry in their distribution in 3' UTRs. Both methods are able to identify many previously known binding sites located in 3'UTRs, and in particular seed regions of known miRNAs. Many new candidates are proposed for experimental verification.
q-bio.GN
3 untranslated regions 3 utrs contain binding sites for many regulatory elements and in particular for micrornas mirnas the importance of mirnamediated posttranscriptional regulation has become increasingly clear in the last few years we propose two complementary approaches to the statistical analysis of oligonucleotide frequencies in mammalian 3 utrs aimed at the identification of candidate binding sites for regulatory elements the first method is based on the identification of sets of genes characterized by evolutionarily conserved overrepresentation of an oligonucleotide the second method is based on the identification of oligonucleotides showing statistically significant strand asymmetry in their distribution in 3 utrs both methods are able to identify many previously known binding sites located in 3utrs and in particular seed regions of known mirnas many new candidates are proposed for experimental verification
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707.0395
Warm molecular hydrogen in the Spitzer SINGS galaxy sample
(simplified) Results on the properties of warm H2 in 57 normal galaxies are derived from H2 rotational transitions, obtained as part of SINGS. This study extends previous extragalactic surveys of H2, the most abundant constituent of the molecular ISM, to more common systems (L_FIR = e7 to 6e10 L_sun) of all morphological and nuclear types. The S(1) transition is securely detected in the nuclear regions of 86% of SINGS galaxies with stellar masses above 10^9.5 M_sun. The derived column densities of warm H2 (T > ~100 K), even though averaged over kiloparsec-scale areas, are commensurate with those of resolved PDRs; the median of the sample is 3e20 cm-2. They amount to between 1% and >30% of the total H2. The power emitted in the sum of the S(0) to S(2) transitions is on average 30% of the [SiII] line power, and ~4e-4 of the total infrared power (TIR) within the same area for star-forming galaxies, which is consistent with excitation in PDRs. The fact that H2 emission scales tightly with PAH emission, even though the average radiation field intensity varies by a factor ten, can also be understood if both tracers originate predominantly in PDRs, either dense or diffuse. A large fraction of the 25 LINER/Sy targets, however, strongly depart from the rest of the sample, in having warmer H2 in the excited states, and an excess of H2 emission with respect to PAHs, TIR and [SiII]. We propose a threshold in H2 to PAH power ratios, allowing the identification of low-luminosity AGNs by an excess H2 excitation. A dominant contribution from shock heating is favored in these objects. Finally, we detect, in nearly half the star-forming targets, non-equilibrium ortho to para ratios, consistent with FUV pumping combined with incomplete ortho-para thermalization by collisions, or possibly non-equilibrium PDR fronts advancing into cold gas.
astro-ph
simplified results on the properties of warm h2 in 57 normal galaxies are derived from h2 rotational transitions obtained as part of sings this study extends previous extragalactic surveys of h2 the most abundant constituent of the molecular ism to more common systems l_fir e7 to 6e10 l_sun of all morphological and nuclear types the s1 transition is securely detected in the nuclear regions of 86 of sings galaxies with stellar masses above 1095 m_sun the derived column densities of warm h2 t 100 k even though averaged over kiloparsecscale areas are commensurate with those of resolved pdrs the median of the sample is 3e20 cm2 they amount to between 1 and 30 of the total h2 the power emitted in the sum of the s0 to s2 transitions is on average 30 of the siii line power and 4e4 of the total infrared power tir within the same area for starforming galaxies which is consistent with excitation in pdrs the fact that h2 emission scales tightly with pah emission even though the average radiation field intensity varies by a factor ten can also be understood if both tracers originate predominantly in pdrs either dense or diffuse a large fraction of the 25 linersy targets however strongly depart from the rest of the sample in having warmer h2 in the excited states and an excess of h2 emission with respect to pahs tir and siii we propose a threshold in h2 to pah power ratios allowing the identification of lowluminosity agns by an excess h2 excitation a dominant contribution from shock heating is favored in these objects finally we detect in nearly half the starforming targets nonequilibrium ortho to para ratios consistent with fuv pumping combined with incomplete orthopara thermalization by collisions or possibly nonequilibrium pdr fronts advancing into cold gas
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707.0396
Finite volume QCD at fixed topological charge
In finite volume the partition function of QCD with a given $\theta$ is a sum of different topological sectors with a weight primarily determined by the topological susceptibility. If a physical observable is evaluated only in a fixed topological sector, the result deviates from the true expectation value by an amount proportional to the inverse space-time volume 1/V. Using the saddle point expansion, we derive formulas to express the correction due to the fixed topological charge in terms of a 1/V expansion. Applying this formula, we propose a class of methods to determine the topological susceptibility in QCD from various correlation functions calculated in a fixed topological sector.
hep-lat hep-th
in finite volume the partition function of qcd with a given theta is a sum of different topological sectors with a weight primarily determined by the topological susceptibility if a physical observable is evaluated only in a fixed topological sector the result deviates from the true expectation value by an amount proportional to the inverse spacetime volume 1v using the saddle point expansion we derive formulas to express the correction due to the fixed topological charge in terms of a 1v expansion applying this formula we propose a class of methods to determine the topological susceptibility in qcd from various correlation functions calculated in a fixed topological sector
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707.0397
Robust Audio Watermarking Against the D/A and A/D conversions
Audio watermarking has played an important role in multimedia security. In many applications using audio watermarking, D/A and A/D conversions (denoted by DA/AD in this paper) are often involved. In previous works, however, the robustness issue of audio watermarking against the DA/AD conversions has not drawn sufficient attention yet. In our extensive investigation, it has been found that the degradation of a watermarked audio signal caused by the DA/AD conversions manifests itself mainly in terms of wave magnitude distortion and linear temporal scaling, making the watermark extraction failed. Accordingly, a DWT-based audio watermarking algorithm robust against the DA/AD conversions is proposed in this paper. To resist the magnitude distortion, the relative energy relationships among different groups of the DWT coefficients in the low-frequency sub-band are utilized in watermark embedding by adaptively controlling the embedding strength. Furthermore, the resynchronization is designed to cope with the linear temporal scaling. The time-frequency localization characteristics of DWT are exploited to save the computational load in the resynchronization. Consequently, the proposed audio watermarking algorithm is robust against the DA/AD conversions, other common audio processing manipulations, and the attacks in StirMark Benchmark for Audio, which has been verified by experiments.
cs.CR cs.MM
audio watermarking has played an important role in multimedia security in many applications using audio watermarking da and ad conversions denoted by daad in this paper are often involved in previous works however the robustness issue of audio watermarking against the daad conversions has not drawn sufficient attention yet in our extensive investigation it has been found that the degradation of a watermarked audio signal caused by the daad conversions manifests itself mainly in terms of wave magnitude distortion and linear temporal scaling making the watermark extraction failed accordingly a dwtbased audio watermarking algorithm robust against the daad conversions is proposed in this paper to resist the magnitude distortion the relative energy relationships among different groups of the dwt coefficients in the lowfrequency subband are utilized in watermark embedding by adaptively controlling the embedding strength furthermore the resynchronization is designed to cope with the linear temporal scaling the timefrequency localization characteristics of dwt are exploited to save the computational load in the resynchronization consequently the proposed audio watermarking algorithm is robust against the daad conversions other common audio processing manipulations and the attacks in stirmark benchmark for audio which has been verified by experiments
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707.0398
Exchange effects on electron scattering through a quantum dot embedded in a two-dimensional semiconductor structure
We have developed a theoretical method to study scattering processes of an incident electron through an N-electron quantum dot (QD) embedded in a two-dimensional (2D) semiconductor. The generalized Lippmann-Schwinger equations including the electron-electron exchange interaction in this system are solved for the continuum electron by using the method of continued fractions (MCF) combined with 2D partial-wave expansion technique. The method is applied to a one-electron QD case. Cross-sections are obtained for both the singlet and triplet couplings between the incident electron and the QD electron during the scattering. The total elastic cross-sections as well as the spin-flip scattering cross-sections resulting from the exchange potential are presented. Furthermore, inelastic scattering processes are also studied using a multichannel formalism of the MCF.
cond-mat.other
we have developed a theoretical method to study scattering processes of an incident electron through an nelectron quantum dot qd embedded in a twodimensional 2d semiconductor the generalized lippmannschwinger equations including the electronelectron exchange interaction in this system are solved for the continuum electron by using the method of continued fractions mcf combined with 2d partialwave expansion technique the method is applied to a oneelectron qd case crosssections are obtained for both the singlet and triplet couplings between the incident electron and the qd electron during the scattering the total elastic crosssections as well as the spinflip scattering crosssections resulting from the exchange potential are presented furthermore inelastic scattering processes are also studied using a multichannel formalism of the mcf
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707.0399
Low-lying ud anti-s anti-s configurations in a non-relativistic constituent quark model
The energies of the low-lying isoscalar and isovector ud anti-s anti-s configurations with spin-parity J^P=0^+, 1^+, and 2^+ are calculated in a non-relativistic constituent quark model by use of the variational method. The contributions of various parts of the quark-quark interacting potentials including the s-channel interaction are investigated, and the effect of different forms of confinement potential is examined. The model parameters are determined by the same method as in our previous work, and they still can satisfactorily describe the nucleon-nucleon scattering phase shifts and the hyperon-nucleon cross sections. The parameters of the s-channel interaction are fixed by the masses of K and K^* mesons, for which the size parameter is taken to be two possible values. When it is chosen as the same as baryons', the numerical results show that the masses of all the ud anti-s anti-s configurations are higher than the corresponding meson-meson thresholds. But when the size parameter for the K and K^* mesons is adjusted to be smaller than that for the baryons, the ud anti-s anti-s configuration with I=0 and J^P=1^+ is found to lie lower than the K^*K^* threshold, furthermore, this state has a very small KK^* component and the interaction matrix elements between this state and KK^* is comparatively small, thus its coupling to the KK^* channel will consequently be weak and it might be regarded as a possible tetraquark candidate.
nucl-th
the energies of the lowlying isoscalar and isovector ud antis antis configurations with spinparity jp0 1 and 2 are calculated in a nonrelativistic constituent quark model by use of the variational method the contributions of various parts of the quarkquark interacting potentials including the schannel interaction are investigated and the effect of different forms of confinement potential is examined the model parameters are determined by the same method as in our previous work and they still can satisfactorily describe the nucleonnucleon scattering phase shifts and the hyperonnucleon cross sections the parameters of the schannel interaction are fixed by the masses of k and k mesons for which the size parameter is taken to be two possible values when it is chosen as the same as baryons the numerical results show that the masses of all the ud antis antis configurations are higher than the corresponding mesonmeson thresholds but when the size parameter for the k and k mesons is adjusted to be smaller than that for the baryons the ud antis antis configuration with i0 and jp1 is found to lie lower than the kk threshold furthermore this state has a very small kk component and the interaction matrix elements between this state and kk is comparatively small thus its coupling to the kk channel will consequently be weak and it might be regarded as a possible tetraquark candidate
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707.04
Singular Hecke algebras, Markov traces, and HOMFLY-type invariants
We define the singular Hecke algebra ${\mathcal H} (SB_n)$ as the quotient of the singular braid monoid algebra ${\mathbb C} (q) [SB_n]$ by the Hecke relations $\sigma_k^2 = (q-1) \sigma_k +q$, $1 \le k\le n-1$, and define the Markov traces on the sequence $\{{\mathcal H}(SB_n)\}_{n=1}^{+\infty}$ in the same way as for the Markov traces on the tower of (non-singular) Hecke algebras of the symmetric groups. We prove that the Markov traces are in one-to-one correspondance with the invariants that satisfies some skein relation, and compute an explicit classification of the Markov traces. Thanks to this classification, we define some universal HOMFLY-type invariant which has the property that it distinguishes all the pairs of singular links that can be distinguished by an invariant which satisfies the required skein relation.
math.GT math.RT
we define the singular hecke algebra mathcal h sb_n as the quotient of the singular braid monoid algebra mathbb c q sb_n by the hecke relations sigma_k2 q1 sigma_k q 1 le kle n1 and define the markov traces on the sequence mathcal hsb_n_n1infty in the same way as for the markov traces on the tower of nonsingular hecke algebras of the symmetric groups we prove that the markov traces are in onetoone correspondance with the invariants that satisfies some skein relation and compute an explicit classification of the markov traces thanks to this classification we define some universal homflytype invariant which has the property that it distinguishes all the pairs of singular links that can be distinguished by an invariant which satisfies the required skein relation
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707.0401
J.S. Bell's Concept of Local Causality
John Stewart Bell's famous 1964 theorem is widely regarded as one of the most important developments in the foundations of physics. It has even been described as "the most profound discovery of science." Yet even as we approach the 50th anniversary of Bell's discovery, its meaning and implications remain controversial. Many textbooks and commentators report that Bell's theorem refutes the possibility (suggested especially by Einstein, Podolsky, and Rosen in 1935) of supplementing ordinary quantum theory with additional ("hidden") variables that might restore determinism and/or some notion of an observer-independent reality. On this view, Bell's theorem supports the orthodox Copenhagen interpretation. Bell's own view of his theorem, however, was quite different. He instead took the theorem as establishing an "essential conflict" between the now well-tested empirical predictions of quantum theory and relativistic \emph{local causality}. The goal of the present paper is, in general, to make Bell's own views more widely known and, in particular, to explain in detail Bell's little-known mathematical formulation of the concept of relativistic local causality on which his theorem rests. We thus collect and organize many of Bell's crucial statements on these topics, which are scattered throughout his writings, into a self-contained, pedagogical discussion including elaborations of the concepts "beable", "completeness", and "causality" which figure in the formulation. We also show how local causality (as formulated by Bell) can be used to derive an empirically testable Bell-type inequality, and how it can be used to recapitulate the EPR argument.
quant-ph
john stewart bells famous 1964 theorem is widely regarded as one of the most important developments in the foundations of physics it has even been described as the most profound discovery of science yet even as we approach the 50th anniversary of bells discovery its meaning and implications remain controversial many textbooks and commentators report that bells theorem refutes the possibility suggested especially by einstein podolsky and rosen in 1935 of supplementing ordinary quantum theory with additional hidden variables that might restore determinism andor some notion of an observerindependent reality on this view bells theorem supports the orthodox copenhagen interpretation bells own view of his theorem however was quite different he instead took the theorem as establishing an essential conflict between the now welltested empirical predictions of quantum theory and relativistic emphlocal causality the goal of the present paper is in general to make bells own views more widely known and in particular to explain in detail bells littleknown mathematical formulation of the concept of relativistic local causality on which his theorem rests we thus collect and organize many of bells crucial statements on these topics which are scattered throughout his writings into a selfcontained pedagogical discussion including elaborations of the concepts beable completeness and causality which figure in the formulation we also show how local causality as formulated by bell can be used to derive an empirically testable belltype inequality and how it can be used to recapitulate the epr argument
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707.0402
The maximum output p-norm of quantum channels is not multiplicative for any p>2
We prove the claim made in the title by showing that approximately randomising maps of large dimension are counterexamples to the multiplicativity conjecture.
quant-ph
we prove the claim made in the title by showing that approximately randomising maps of large dimension are counterexamples to the multiplicativity conjecture
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707.0403
Dynamical control of matter-wave tunneling in periodic potentials
We report on measurements of dynamical suppression of inter-well tunneling of a Bose-Einstein condensate (BEC) in a strongly driven optical lattice. The strong driving is a sinusoidal shaking of the lattice corresponding to a time-varying linear potential, and the tunneling is measured by letting the BEC freely expand in the lattice. The measured tunneling rate is reduced and, for certain values of the shaking parameter, completely suppressed. Our results are in excellent agreement with theoretical predictions. Furthermore, we have verified that in general the strong shaking does not destroy the phase coherence of the BEC, opening up the possibility of realizing quantum phase transitions by using the shaking strength as the control parameter.
cond-mat.other quant-ph
we report on measurements of dynamical suppression of interwell tunneling of a boseeinstein condensate bec in a strongly driven optical lattice the strong driving is a sinusoidal shaking of the lattice corresponding to a timevarying linear potential and the tunneling is measured by letting the bec freely expand in the lattice the measured tunneling rate is reduced and for certain values of the shaking parameter completely suppressed our results are in excellent agreement with theoretical predictions furthermore we have verified that in general the strong shaking does not destroy the phase coherence of the bec opening up the possibility of realizing quantum phase transitions by using the shaking strength as the control parameter
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707.0404
Search for Direc Magnetic Monopoles in e+e- Collisions with the OPAL Detector at LEP2
This letter describes a direct search for pair produced magnetic monopoles in e+e- collisions. The analysis is based on 62.7 pb^-1 of data collected with the OPAL detector at an average centre-of-mass energy of sqrt(s)= 206.3GeV. The monopole signal was assumed to be characterized by two back-to-back particles with an anomalously high ionization energy loss de/dx in the tracking chambers. No evidence for production of monopoles was observed. Upper limits were obtained on the magnetic monopole pair-production cross-section (sigma) in the mass range 45 GeV/c^2<m_M<102 GeV/c^2. The average limit is sigma < 0.05 pb and is essentially independent of the magnetic monopole mass. The cross-section limit is derived at the 95% confidence level and is valid for spin-1/2 magnetic monopoles.
hep-ex
this letter describes a direct search for pair produced magnetic monopoles in ee collisions the analysis is based on 627 pb1 of data collected with the opal detector at an average centreofmass energy of sqrts 2063gev the monopole signal was assumed to be characterized by two backtoback particles with an anomalously high ionization energy loss dedx in the tracking chambers no evidence for production of monopoles was observed upper limits were obtained on the magnetic monopole pairproduction crosssection sigma in the mass range 45 gevc2m_m102 gevc2 the average limit is sigma 005 pb and is essentially independent of the magnetic monopole mass the crosssection limit is derived at the 95 confidence level and is valid for spin12 magnetic monopoles
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707.0405
Casimir-Polder intermolecular forces in minimal length theories
Generalized uncertainty relations are known to provide a minimal length $\hbar\sqrt{\beta}$. The effect of such minimal length in the Casimir-Polder interactions between neutral atoms (molecules) is studied. The first order correction term in the minimal uncertainty parameter is derived and found to describe an attractive potential scaling as $r^{-9}$ as opposed to the well known $r^{-7}$ long range retarded potential.
hep-th hep-ph
generalized uncertainty relations are known to provide a minimal length hbarsqrtbeta the effect of such minimal length in the casimirpolder interactions between neutral atoms molecules is studied the first order correction term in the minimal uncertainty parameter is derived and found to describe an attractive potential scaling as r9 as opposed to the well known r7 long range retarded potential
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707.0406
On the onset of runaway stellar collisions in dense star clusters I. Dynamics of the first collision
We study the circumstances under which first collisions occur in young and dense star clusters. The initial conditions for our direct $N$-body simulations are chosen such that the clusters experience core collapse within a few million years, before the most massive stars have left the main-sequence. It turns out that the first collision is typically driven by the most massive stars in the cluster. Upon arrival in the cluster core, by dynamical friction, massive stars tend to form binaries. The enhanced cross section of the binary compared to a single star causes other stars to engage the binary. A collision between one of the binary components and the incoming third star is then mediated by the encounters between the binary and other cluster members. Due to the geometry of the binary-single star engagement the relative velocity at the moment of impact is substantially different than in a two-body encounter. This may have profound consequences for the further evolution of the collision product.
astro-ph
we study the circumstances under which first collisions occur in young and dense star clusters the initial conditions for our direct nbody simulations are chosen such that the clusters experience core collapse within a few million years before the most massive stars have left the mainsequence it turns out that the first collision is typically driven by the most massive stars in the cluster upon arrival in the cluster core by dynamical friction massive stars tend to form binaries the enhanced cross section of the binary compared to a single star causes other stars to engage the binary a collision between one of the binary components and the incoming third star is then mediated by the encounters between the binary and other cluster members due to the geometry of the binarysingle star engagement the relative velocity at the moment of impact is substantially different than in a twobody encounter this may have profound consequences for the further evolution of the collision product
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707.0407
Stellar Population Gradients in Bulges along the Hubble Sequence: I. The Data
This is the first paper presenting our long-term project aimed at studying the nature of bulges through the analysis of their stellar population gradients. We present deep spectroscopic observations along the minor axis and the data reduction for a sample of 32 bulges of edge-on spiral galaxies. We explain in detail our procedures to measure their dynamical parameters (rotation curves and velocity dispersion profiles) and line-strength indices, including the conversion to the Lick/IDS system. Tables giving the values of the dynamical parameters and line-strength indices at each galactocentric radius are presented (in electronic form) for each galaxy of the sample. The derived line-strength gradients from this dataset will be analyzed in a forthcoming paper to set constraints on the different scenarios for the formation of the bulges.
astro-ph
this is the first paper presenting our longterm project aimed at studying the nature of bulges through the analysis of their stellar population gradients we present deep spectroscopic observations along the minor axis and the data reduction for a sample of 32 bulges of edgeon spiral galaxies we explain in detail our procedures to measure their dynamical parameters rotation curves and velocity dispersion profiles and linestrength indices including the conversion to the lickids system tables giving the values of the dynamical parameters and linestrength indices at each galactocentric radius are presented in electronic form for each galaxy of the sample the derived linestrength gradients from this dataset will be analyzed in a forthcoming paper to set constraints on the different scenarios for the formation of the bulges
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707.0408
Disk-Evaporation Fed Corona: Structure and Evaporation Feature with Magnetic Field
The disk-corona evaporation model naturally interprets many observational phenomena in black hole X-ray binaries, such as the truncation of an accretion disk and the spectral state transitions. On the other hand, magnetic field is known to play an important role in transporting angular momentum and producing viscosity in accretion flows. In this work, we explicitly take the magnetic field in the accretion disk corona into account and numerically calculate the coronal structure on the basis of our two-temperature evaporation code. We show that the magnetic field influences the coronal structure by its contribution to the pressure, energy and radiative cooling in the corona and by decreasing the vertical heat conduction. We found that the maximal evaporation rate keeps more or less constant ($\sim 0.03$ Eddington rate) while the strength of magnetic fields changes, but that the radius corresponding to the maximal evaporation rate decreases with increasing magnetic field. This predicts that the spectral state transition always occurs at a few percent of Eddington accretion rate, while the inner edge of thin disk can be at $\sim 100 R_{\rm S} $ or even less in the hard state before the transition to the soft state. These results alleviate the problem that previous evaporation models predict too large a truncation radius, and are in better agreement with the observational results of several black hole X-ray binaries, though discrepancies remain.
astro-ph
the diskcorona evaporation model naturally interprets many observational phenomena in black hole xray binaries such as the truncation of an accretion disk and the spectral state transitions on the other hand magnetic field is known to play an important role in transporting angular momentum and producing viscosity in accretion flows in this work we explicitly take the magnetic field in the accretion disk corona into account and numerically calculate the coronal structure on the basis of our twotemperature evaporation code we show that the magnetic field influences the coronal structure by its contribution to the pressure energy and radiative cooling in the corona and by decreasing the vertical heat conduction we found that the maximal evaporation rate keeps more or less constant sim 003 eddington rate while the strength of magnetic fields changes but that the radius corresponding to the maximal evaporation rate decreases with increasing magnetic field this predicts that the spectral state transition always occurs at a few percent of eddington accretion rate while the inner edge of thin disk can be at sim 100 r_rm s or even less in the hard state before the transition to the soft state these results alleviate the problem that previous evaporation models predict too large a truncation radius and are in better agreement with the observational results of several black hole xray binaries though discrepancies remain
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707.0409
On conformal Killing-Yano tensors for Plebanski-Demianski family of solutions
We present the explicit expressions for the conformal Killing-Yano tensors for the Plebanski-Demianski family of type D solutions in four dimensions. Some physically important special cases are discussed in more detail. In particular, it is demonstrated how the conformal Killing-Yano tensor becomes the Killing-Yano tensor for the solutions without acceleration. A possible generalization into higher dimensions is studied. Whereas the transition from the nonaccelerating to accelerating solutions in four dimensions is achieved by the conformal rescaling of the metric, we show that such a procedure is not sufficiently general in higher dimensions - only the maximally symmetric spacetimes in 'accelerated' coordinates are obtained.
gr-qc hep-th
we present the explicit expressions for the conformal killingyano tensors for the plebanskidemianski family of type d solutions in four dimensions some physically important special cases are discussed in more detail in particular it is demonstrated how the conformal killingyano tensor becomes the killingyano tensor for the solutions without acceleration a possible generalization into higher dimensions is studied whereas the transition from the nonaccelerating to accelerating solutions in four dimensions is achieved by the conformal rescaling of the metric we show that such a procedure is not sufficiently general in higher dimensions only the maximally symmetric spacetimes in accelerated coordinates are obtained
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707.041
On gas drag in a circular binary system
We investigate both analytically and numerically the motion of massless particles orbiting primary star in a close circular binary system with particular focus on the gas drag effects. These are the first calculations with particles ranging in size from 1m to 10km, which account for the presence of a tidally perturbed gaseous disk. We have found numerically that the radial mass transport by the tidal waves plays a crucial role in the orbital evolution of particles. Numerical results are confirmed analytical calculations that do not assume anything about origin of the radial flow in the disk. We demonstrate that the migration rate of a particle in a disk out of radial equilibrium is enhanced due to the enhanced mass flux of gas colliding with the particle and the migration is always directed inward regardless of the sign of the radial gas velocity. Within the framework of the perturbation theory we derive general, formulae for short-term variations of the particle semi-major axis, eccentricity and inclination in such disk. The formulae account for departures from axial symmetry by introducing effective components of the gas velocity. They agree with numerical results within several percent. We have also found in numerical simulations that the tidal waves introduce coherence in periastron longitude and eccentricity for particles on neighbouring orbits. The degree of the coherence depends on the particle size and on the distance from the primary star, being most prominent for particles with 10m radius. The results are important mainly in the context of planetesimal formation and, to a lesser degree, during the early planetesimal accretion stage.
astro-ph
we investigate both analytically and numerically the motion of massless particles orbiting primary star in a close circular binary system with particular focus on the gas drag effects these are the first calculations with particles ranging in size from 1m to 10km which account for the presence of a tidally perturbed gaseous disk we have found numerically that the radial mass transport by the tidal waves plays a crucial role in the orbital evolution of particles numerical results are confirmed analytical calculations that do not assume anything about origin of the radial flow in the disk we demonstrate that the migration rate of a particle in a disk out of radial equilibrium is enhanced due to the enhanced mass flux of gas colliding with the particle and the migration is always directed inward regardless of the sign of the radial gas velocity within the framework of the perturbation theory we derive general formulae for shortterm variations of the particle semimajor axis eccentricity and inclination in such disk the formulae account for departures from axial symmetry by introducing effective components of the gas velocity they agree with numerical results within several percent we have also found in numerical simulations that the tidal waves introduce coherence in periastron longitude and eccentricity for particles on neighbouring orbits the degree of the coherence depends on the particle size and on the distance from the primary star being most prominent for particles with 10m radius the results are important mainly in the context of planetesimal formation and to a lesser degree during the early planetesimal accretion stage
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707.0411
Interference pattern of a long diffusive Josephson junction
We calculate the modulation by a magnetic field of the critical current of a long disordered Josephson junction in the diffusive limit, i.e. when the dimensions of the junction are larger that the elastic mean free path, and when the length $L$ is much larger than the width $w$. Due to the averaging of the gauge invariant phase factor over diffusive trajectories, the well-known oscillations of the Fraunhofer pattern are smoothed out and replaced by an exponential decay at large field. The predicted pattern is universal, i.e., it is independent of the disorder strength. We point out an interesting relation with the physics of speckle correlations in optics of turbid media.
cond-mat.mes-hall
we calculate the modulation by a magnetic field of the critical current of a long disordered josephson junction in the diffusive limit ie when the dimensions of the junction are larger that the elastic mean free path and when the length l is much larger than the width w due to the averaging of the gauge invariant phase factor over diffusive trajectories the wellknown oscillations of the fraunhofer pattern are smoothed out and replaced by an exponential decay at large field the predicted pattern is universal ie it is independent of the disorder strength we point out an interesting relation with the physics of speckle correlations in optics of turbid media
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707.0412
Solution of non-singlet DGLAP evolution equation in leading order and next-to-leading order at small-x by method of characteristics
The non-singlet structure functions have been obtained by solving Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) evolution equations in leading order (LO) and next-to-leading order (NLO) at the small-x limit. Here a Taylor series expansion has been used and then the method of characteristics has been applied to solve the evolution equations. Results are comopared with the Fermilab experiment E665 data and New Muon Collaboration (NMC) data.
hep-ph
the nonsinglet structure functions have been obtained by solving dokshitzergribovlipatovaltarelliparisi dglap evolution equations in leading order lo and nexttoleading order nlo at the smallx limit here a taylor series expansion has been used and then the method of characteristics has been applied to solve the evolution equations results are comopared with the fermilab experiment e665 data and new muon collaboration nmc data
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707.0413
Detuned Twin-Signal-Recycling for ultra-high precision interferometers
We propose a new interferometer technique for high precision phase measurements such as those in gravitational wave detection. The technique utilizes a pair of optically coupled resonators that provides identical resonance conditions for the upper as well the lower phase modulation signal sidebands. This symmetry significantly reduces the noise spectral density in a wide frequency band compared with single sideband recycling topologies of current and planned gravitational wave detectors. Furthermore the application of squeezed states of light becomes less demanding.
quant-ph
we propose a new interferometer technique for high precision phase measurements such as those in gravitational wave detection the technique utilizes a pair of optically coupled resonators that provides identical resonance conditions for the upper as well the lower phase modulation signal sidebands this symmetry significantly reduces the noise spectral density in a wide frequency band compared with single sideband recycling topologies of current and planned gravitational wave detectors furthermore the application of squeezed states of light becomes less demanding
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707.0414
A computation of Poisson kernels for some standard weighted biharmonic operators in the unit disc
We compute Poisson kernels for integer weight parameter standard weighted biharmonic operators in the unit disc with Dirichlet boundary conditions. The computations performed extend the supply of explicit examples of such kernels and suggest similar formulas for these Poisson kernels to hold true in more generality. Computations have been carried out using the open source computer algebra package Maxima.
math.AP math.CA
we compute poisson kernels for integer weight parameter standard weighted biharmonic operators in the unit disc with dirichlet boundary conditions the computations performed extend the supply of explicit examples of such kernels and suggest similar formulas for these poisson kernels to hold true in more generality computations have been carried out using the open source computer algebra package maxima
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707.0415
Surface Encapsulation for Low-Loss Silicon Photonics
Encapsulation layers are explored for passivating the surfaces of silicon to reduce optical absorption in the 1500-nm wavelength band. Surface-sensitive test structures consisting of microdisk resonators are fabricated for this purpose. Based on previous work in silicon photovoltaics, coatings of SiNx and SiO2 are applied under varying deposition and annealing conditions. A short dry thermal oxidation followed by a long high-temperature N2 anneal is found to be most effective at long-term encapsulation and reduction of interface absorption. Minimization of the optical loss is attributed to simultaneous reduction in sub-bandgap silicon surface states and hydrogen in the capping material.
physics.optics
encapsulation layers are explored for passivating the surfaces of silicon to reduce optical absorption in the 1500nm wavelength band surfacesensitive test structures consisting of microdisk resonators are fabricated for this purpose based on previous work in silicon photovoltaics coatings of sinx and sio2 are applied under varying deposition and annealing conditions a short dry thermal oxidation followed by a long hightemperature n2 anneal is found to be most effective at longterm encapsulation and reduction of interface absorption minimization of the optical loss is attributed to simultaneous reduction in subbandgap silicon surface states and hydrogen in the capping material
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707.0416
Relationship between non-exponentiality of relaxation and relaxation time at the glass transition
By analyzing the experimental data for various glass-forming liquids and polymers, we find that non-exponentiality $\beta$ and the relaxation time $\tau$ are uniquely related: $\log(\tau)$ is an approximately linear function of $1/\beta$, followed by a crossover to a higher linear slope. We rationalize the observed relationship using a recently developed approach, in which the problem of the glass transition is discussed as the elasticity problem.
cond-mat.dis-nn cond-mat.soft
by analyzing the experimental data for various glassforming liquids and polymers we find that nonexponentiality beta and the relaxation time tau are uniquely related logtau is an approximately linear function of 1beta followed by a crossover to a higher linear slope we rationalize the observed relationship using a recently developed approach in which the problem of the glass transition is discussed as the elasticity problem
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707.0417
Efficient identification of exoplanetary transit candidates from SuperWASP light curves
Transiting extrasolar planets constitute only a small fraction of the range of stellar systems found to display periodic, shallow dimmings in wide-field surveys employing small-aperture camera arrays. Here we present an efficient selection strategy for follow-up observations, derived from analysis of the light curves of a sample of 67 SuperWASP targets that passed the selection tests we used in earlier papers, but which have subsequently been identified either as planet hosts or as astrophysical false positives. We determine the system parameters using Markov-chain Monte Carlo analysis of the SuperWASP light curves. We use a constrained optimisation of chi-squared combined with a Bayesian prior based on the main-sequence mass and radius expected from the 2MASS J-H colour. The Bayesian nature of the analysis allows us to quantify both the departure of the host star from the main-sequence mass-radius relation and the probability that the companion radius is less than 1.5 Jupiter radii. When augmented by direct light curve analyses that detect binaries with unequal primary and secondary eclipses, and objects with aperture blends that are resolved by SuperWASP, we find that only 13 of the original 67 stars, including the three known planets in the sample, would qualify for follow-up. This suggests that planet discovery "hit rates" better than one-in-five should be achievable. In addition, the stellar binaries that qualify are likely to have astrophysically interesting stellar or sub-stellar secondaries.
astro-ph
transiting extrasolar planets constitute only a small fraction of the range of stellar systems found to display periodic shallow dimmings in widefield surveys employing smallaperture camera arrays here we present an efficient selection strategy for followup observations derived from analysis of the light curves of a sample of 67 superwasp targets that passed the selection tests we used in earlier papers but which have subsequently been identified either as planet hosts or as astrophysical false positives we determine the system parameters using markovchain monte carlo analysis of the superwasp light curves we use a constrained optimisation of chisquared combined with a bayesian prior based on the mainsequence mass and radius expected from the 2mass jh colour the bayesian nature of the analysis allows us to quantify both the departure of the host star from the mainsequence massradius relation and the probability that the companion radius is less than 15 jupiter radii when augmented by direct light curve analyses that detect binaries with unequal primary and secondary eclipses and objects with aperture blends that are resolved by superwasp we find that only 13 of the original 67 stars including the three known planets in the sample would qualify for followup this suggests that planet discovery hit rates better than oneinfive should be achievable in addition the stellar binaries that qualify are likely to have astrophysically interesting stellar or substellar secondaries
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707.0418
Random matrices beyond the Cartan classification
It is known that hermitean random matrix ensembles can be identified with symmetric coset spaces of Lie groups, or else with tangent spaces of the same. This results in a classification of random matrix ensembles as well as applications in practical calculations of physical observables. In this paper we show that a large number of non-hermitean random matrix ensembles defined by physically motivated symmetries - chiral symmetry, time reversal invariance, space rotation invariance, particle-hole symmetry, or different reality conditions - can likewise be identified with symmetric spaces. We give explicit representations of the random matrix ensembles identified with lateral algebra subspaces, and of the corresponding symmetric subalgebras spanning the group of invariance. Among the ensembles listed we identify as special cases all the hermitean ensembles identified with Cartan classes of symmetric spaces and the three Ginibre ensembles with complex eigenvalues.
math-ph cond-mat.mes-hall hep-ph hep-th math.MP
it is known that hermitean random matrix ensembles can be identified with symmetric coset spaces of lie groups or else with tangent spaces of the same this results in a classification of random matrix ensembles as well as applications in practical calculations of physical observables in this paper we show that a large number of nonhermitean random matrix ensembles defined by physically motivated symmetries chiral symmetry time reversal invariance space rotation invariance particlehole symmetry or different reality conditions can likewise be identified with symmetric spaces we give explicit representations of the random matrix ensembles identified with lateral algebra subspaces and of the corresponding symmetric subalgebras spanning the group of invariance among the ensembles listed we identify as special cases all the hermitean ensembles identified with cartan classes of symmetric spaces and the three ginibre ensembles with complex eigenvalues
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707.0419
Radiative and semileptonic decays in Chiral Perturbation Theory
I give a short overview of what has been done in radiative and semileptonic Kaon decays in Chiral Perturbation Theory. This includes for semileptonic decays the work which has been done to order $p^6$ including preliminary results of isospin breaking to that order in $K_{\ell3}$. For the radiative decays I mainly present some results from recent work concerning $K_{\ell3\gamma}$.
hep-ph
i give a short overview of what has been done in radiative and semileptonic kaon decays in chiral perturbation theory this includes for semileptonic decays the work which has been done to order p6 including preliminary results of isospin breaking to that order in k_ell3 for the radiative decays i mainly present some results from recent work concerning k_ell3gamma
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707.042
Entropy of Extremal Black Holes in Two Dimension
In this paper we apply the entropy function formalism to the two-dimensional black hole which come from the compactification of the heterotic string theory with the dilaton coupling function. We find the Bekenstein-Hawking entropy from the value of the entropy function at its saddle point. Also we consider higher derivative terms. After that we apply the entropy function formalism to the Jackiw-Teitelboim (JT) model where we consider the effect of string-loop to this model.
hep-th
in this paper we apply the entropy function formalism to the twodimensional black hole which come from the compactification of the heterotic string theory with the dilaton coupling function we find the bekensteinhawking entropy from the value of the entropy function at its saddle point also we consider higher derivative terms after that we apply the entropy function formalism to the jackiwteitelboim jt model where we consider the effect of stringloop to this model
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707.0421
The $k$-anonymity Problem is Hard
The problem of publishing personal data without giving up privacy is becoming increasingly important. An interesting formalization recently proposed is the k-anonymity. This approach requires that the rows in a table are clustered in sets of size at least k and that all the rows in a cluster become the same tuple, after the suppression of some records. The natural optimization problem, where the goal is to minimize the number of suppressed entries, is known to be NP-hard when the values are over a ternary alphabet, k = 3 and the rows length is unbounded. In this paper we give a lower bound on the approximation factor that any polynomial-time algorithm can achive on two restrictions of the problem,namely (i) when the records values are over a binary alphabet and k = 3, and (ii) when the records have length at most 8 and k = 4, showing that these restrictions of the problem are APX-hard.
cs.DB cs.CC cs.DS
the problem of publishing personal data without giving up privacy is becoming increasingly important an interesting formalization recently proposed is the kanonymity this approach requires that the rows in a table are clustered in sets of size at least k and that all the rows in a cluster become the same tuple after the suppression of some records the natural optimization problem where the goal is to minimize the number of suppressed entries is known to be nphard when the values are over a ternary alphabet k 3 and the rows length is unbounded in this paper we give a lower bound on the approximation factor that any polynomialtime algorithm can achive on two restrictions of the problemnamely i when the records values are over a binary alphabet and k 3 and ii when the records have length at most 8 and k 4 showing that these restrictions of the problem are apxhard
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707.0422
Dimerization process and elementary excitations in spin-Peierls chains coupled by frustrated interactions
We consider the ground state and the elementary excitations of an array of spin-Peierls chains coupled by elastic and magnetic interactions. It is expected that the effect of the magnetic interchain coupling will be to reduce the dimerization amplitude and that of the elastic coupling will be to confine the spin one-half solitons corresponding to each isolated chain. We show that this is the case when these interactions are not frustrated. On the other hand, in the frustrated case we show that the amplitude of dimerization in the ground state is independent of the strength of the interchain magnetic interaction in a broad range of values of this parameter. We also show that free solitons could be the elementary excitations when only nearest neighbor interactions are considered. The case of an elastic interchain coupling is analyzed on a general energetic consideration. To study the effect of the magnetic interchain interaction the problem is simplified to a two-leg ladder which is solved using DMRG calculations. We show that the deconfinement mechanism is effective even with a significantly strong antiferromagnetic interchain coupling.
cond-mat.str-el
we consider the ground state and the elementary excitations of an array of spinpeierls chains coupled by elastic and magnetic interactions it is expected that the effect of the magnetic interchain coupling will be to reduce the dimerization amplitude and that of the elastic coupling will be to confine the spin onehalf solitons corresponding to each isolated chain we show that this is the case when these interactions are not frustrated on the other hand in the frustrated case we show that the amplitude of dimerization in the ground state is independent of the strength of the interchain magnetic interaction in a broad range of values of this parameter we also show that free solitons could be the elementary excitations when only nearest neighbor interactions are considered the case of an elastic interchain coupling is analyzed on a general energetic consideration to study the effect of the magnetic interchain interaction the problem is simplified to a twoleg ladder which is solved using dmrg calculations we show that the deconfinement mechanism is effective even with a significantly strong antiferromagnetic interchain coupling
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707.0423
Inverse bremsstrahlung contributions to Drell-Yan like processes
The contribution of the sub-process $\gamma q \to q' l_1\bar{l}_2$ in hadron-hadron interactions is considered. It is a part of one-loop electroweak radiative corrections for the Drell-Yan production of lepton pairs at hadron colliders. It is shown that this contribution should be taken into account aiming at the 1% accuracy of the Drell-Yan process theoretical description. Both the neutral and charged current cases are evaluated. Numerical results are presented for typical conditions of LHC experiments.
hep-ph
the contribution of the subprocess gamma q to q l_1barl_2 in hadronhadron interactions is considered it is a part of oneloop electroweak radiative corrections for the drellyan production of lepton pairs at hadron colliders it is shown that this contribution should be taken into account aiming at the 1 accuracy of the drellyan process theoretical description both the neutral and charged current cases are evaluated numerical results are presented for typical conditions of lhc experiments
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707.0424
AdS/CFT for Four-Point Amplitudes involving Gravitino Exchange
In this paper we compute the tree-level four-point scattering amplitude of two dilatini and two axion-dilaton fields in type IIB supergravity in AdS5 x S5. A special feature of this process is that there is an "exotic" channel in which there are no singleparticle poles. Another novelty is that this process involves the exchange of a bulk gravitino. The amplitude is interpreted in terms of N = 4 supersymmetric Yang-Mills theory at large 't Hooft coupling. Properties of the Operator Product Expansion are used to analyze the various contributions from single- and double-trace operators in the weak and strongly coupled regimes, and to determine the anomalous dimensions of semi-short operators. The analysis is particularly clear in the exotic channel, given the absence of BPS states.
hep-th
in this paper we compute the treelevel fourpoint scattering amplitude of two dilatini and two axiondilaton fields in type iib supergravity in ads5 x s5 a special feature of this process is that there is an exotic channel in which there are no singleparticle poles another novelty is that this process involves the exchange of a bulk gravitino the amplitude is interpreted in terms of n 4 supersymmetric yangmills theory at large t hooft coupling properties of the operator product expansion are used to analyze the various contributions from single and doubletrace operators in the weak and strongly coupled regimes and to determine the anomalous dimensions of semishort operators the analysis is particularly clear in the exotic channel given the absence of bps states
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707.0425
Random Normal Matrices and Polynomial Curves
We show that in the large matrix limit, the eigenvalues of the normal matrix model for matrices with spectrum inside a compact domain with a special class of potentials homogeneously fill the interior of a polynomial curve uniquely defined by the area of its interior domain and its exterior harmonic moments which are all given as parameters of the potential. Then we consider the orthogonal polynomials corresponding to this matrix model and show that, under certain assumptions, the density of the zeros of the highest relevant orthogonal polynomial in the large matrix limit is (up to some constant factor) given by the discontinuity of the Schwarz function of this polynomial curve.
math.QA math.PR
we show that in the large matrix limit the eigenvalues of the normal matrix model for matrices with spectrum inside a compact domain with a special class of potentials homogeneously fill the interior of a polynomial curve uniquely defined by the area of its interior domain and its exterior harmonic moments which are all given as parameters of the potential then we consider the orthogonal polynomials corresponding to this matrix model and show that under certain assumptions the density of the zeros of the highest relevant orthogonal polynomial in the large matrix limit is up to some constant factor given by the discontinuity of the schwarz function of this polynomial curve
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707.0426
Multinucleon transfer reactions in closed-shell nuclei
Multinucleon transfer reactions in 40Ca+96Zr and 90Zr+208Pb have been measured at energies close to the Coulomb barrier in a high resolution gamma-particle coincidence experiment. The large solid angle magnetic spectrometer PRISMA coupled to the CLARA gamma-array has been employed. Trajectory reconstruction has been applied for the complete identification of transfer products. Mass and charge yields, total kinetic energy losses, gamma transitions of the binary reaction partners, and comparison of data with semiclassical calculations are reported. Specific transitions in 95Zr populated in one particle transfer channels are discussed in terms of particle-phonon couplings. The gamma decays from states in 42Ca in the excitation energy region expected from pairing vibrations are also observed.
nucl-ex
multinucleon transfer reactions in 40ca96zr and 90zr208pb have been measured at energies close to the coulomb barrier in a high resolution gammaparticle coincidence experiment the large solid angle magnetic spectrometer prisma coupled to the clara gammaarray has been employed trajectory reconstruction has been applied for the complete identification of transfer products mass and charge yields total kinetic energy losses gamma transitions of the binary reaction partners and comparison of data with semiclassical calculations are reported specific transitions in 95zr populated in one particle transfer channels are discussed in terms of particlephonon couplings the gamma decays from states in 42ca in the excitation energy region expected from pairing vibrations are also observed
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707.0427
Complete isometries between subspaces of noncommutative Lp-spaces
We prove some noncommutative analogues of a theorem by Plotkin and Rudin about isometries between subspaces of Lp-spaces. Let 0<p<\infty, p not an even integer. The main result of this paper states that in the category of unital subspaces of noncommutative probability Lp-spaces, under some boundedness condition, the unital completely isometric maps come from *-isomorphisms of the underlying von Neumann algebras. Some applications are given, including to non commutative H^p spaces.
math.OA math.FA
we prove some noncommutative analogues of a theorem by plotkin and rudin about isometries between subspaces of lpspaces let 0pinfty p not an even integer the main result of this paper states that in the category of unital subspaces of noncommutative probability lpspaces under some boundedness condition the unital completely isometric maps come from isomorphisms of the underlying von neumann algebras some applications are given including to non commutative hp spaces
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707.0428
Template-based searches for gravitational waves: efficient lattice covering of flat parameter spaces
The construction of optimal template banks for matched-filtering searches is an example of the sphere covering problem. For parameter spaces with constant-coefficient metrics a (near-) optimal template bank is achieved by the A_n* lattice, which is the best lattice-covering in dimensions n <= 5, and is close to the best covering known for dimensions n <= 16. Generally this provides a substantially more efficient covering than the simpler hyper-cubic lattice. We present an algorithm for generating lattice template banks for constant-coefficient metrics and we illustrate its implementation by generating A_n* template banks in n=2,3,4 dimensions.
gr-qc
the construction of optimal template banks for matchedfiltering searches is an example of the sphere covering problem for parameter spaces with constantcoefficient metrics a near optimal template bank is achieved by the a_n lattice which is the best latticecovering in dimensions n 5 and is close to the best covering known for dimensions n 16 generally this provides a substantially more efficient covering than the simpler hypercubic lattice we present an algorithm for generating lattice template banks for constantcoefficient metrics and we illustrate its implementation by generating a_n template banks in n234 dimensions
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707.0429
The Axion from Five-Dimensional Supergravity
We consider the axion arising from five-dimensional supergravity in the presence of boundaries. We find the approximate bosonic effective action to estimate the lower bound on the "Peccei-Quinn" energy scale with a flat bulk. With a warped bulk, one can obtain a scale within the standard window; this puts a bound on the required curvature scale relative to the proper separation between boundaries. We comment on the scalar potential that may ruin the strong-CP resolution, and the effective derivative coupling to matter in 5D hypermultiplets.
hep-ph
we consider the axion arising from fivedimensional supergravity in the presence of boundaries we find the approximate bosonic effective action to estimate the lower bound on the pecceiquinn energy scale with a flat bulk with a warped bulk one can obtain a scale within the standard window this puts a bound on the required curvature scale relative to the proper separation between boundaries we comment on the scalar potential that may ruin the strongcp resolution and the effective derivative coupling to matter in 5d hypermultiplets
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