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709.1735
CGRaBS: An All-Sky Survey of Gamma-Ray Blazar Candidates
We describe a uniform all-sky survey of bright blazars, selected primarily by their flat radio spectra, that is designed to provide a large catalog of likely gamma-ray AGN. The defined sample has 1625 targets with radio and X-ray properties similar to those of the EGRET blazars, spread uniformly across the |b| > 10 deg sky. We also report progress toward optical characterization of the sample; of objects with known R < 23, 85% have been classified and 81% have measured redshifts. One goal of this program is to focus attention on the most interesting (e.g., high redshift, high luminosity, ...) sources for intensive multiwavelength study during the observations by the Large Area Telescope (LAT) on GLAST.
astro-ph
we describe a uniform allsky survey of bright blazars selected primarily by their flat radio spectra that is designed to provide a large catalog of likely gammaray agn the defined sample has 1625 targets with radio and xray properties similar to those of the egret blazars spread uniformly across the b 10 deg sky we also report progress toward optical characterization of the sample of objects with known r 23 85 have been classified and 81 have measured redshifts one goal of this program is to focus attention on the most interesting eg high redshift high luminosity sources for intensive multiwavelength study during the observations by the large area telescope lat on glast
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709.1736
LAQGSM03.03 Upgrade and its Validation
This paper presents part of an internal LANL Progress Report on LAQGSM03.03, an upgrade of the Los Alamos version of the Quark-Gluon String Model event generator for MCNPX/6 and MARS15 transport codes and on its validation and testing against a large variety of recent measurements. We present here an analysis with LAQGSM03.03 of the recent PHENIX mid-rapidity spectra of pi+, pi-, K+, K-, p, and p-bar produced in ultra-relativistic p + p interactions at sqrt(s) = 200 GeV; GSI cross sections for the fragmentation of Pb208 at 1 GeV/nucleon on Be9; fragmentation cross sections of Si28 on H, C, Al, Cu, Sn, and Pb at energies from 290 to 1200 MeV/nucleon measred recently at HIMAC and BNL; recent HIMAC data on B, Be, Li, and He production cross sections from fragmentation of C12 on H, C, Al, Cu, Sn, and Pb at 290 and 400 MeV/nucleon; BNL data on fragmentation cross sections of Fe56 on H, C, Al, Cu, and Pb targets at 1.05 GeV/nucleon; recent pi+ and pi- spectra from 6.4, 12.3, and 17.5 GeV/c p + Be9 from the E910 BNL measurements; and fragmentation cross sections of Ca40, Ca48, Ni58, and Ni64 on Be9 and Ta181 at 140 MeV/nucleon, and of Kr86 at 64 MeV/nucleon on the same targets measured recently at NSCL-MSU and RARF-RIKEN, respectively.
nucl-th astro-ph hep-ph nucl-ex
this paper presents part of an internal lanl progress report on laqgsm0303 an upgrade of the los alamos version of the quarkgluon string model event generator for mcnpx6 and mars15 transport codes and on its validation and testing against a large variety of recent measurements we present here an analysis with laqgsm0303 of the recent phenix midrapidity spectra of pi pi k k p and pbar produced in ultrarelativistic p p interactions at sqrts 200 gev gsi cross sections for the fragmentation of pb208 at 1 gevnucleon on be9 fragmentation cross sections of si28 on h c al cu sn and pb at energies from 290 to 1200 mevnucleon measred recently at himac and bnl recent himac data on b be li and he production cross sections from fragmentation of c12 on h c al cu sn and pb at 290 and 400 mevnucleon bnl data on fragmentation cross sections of fe56 on h c al cu and pb targets at 105 gevnucleon recent pi and pi spectra from 64 123 and 175 gevc p be9 from the e910 bnl measurements and fragmentation cross sections of ca40 ca48 ni58 and ni64 on be9 and ta181 at 140 mevnucleon and of kr86 at 64 mevnucleon on the same targets measured recently at nsclmsu and rarfriken respectively
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709.1737
The Fundamental Plane of Bulges at Intermediate Redshift
We report on a new study aimed at understanding the diversity and evolutionary properties of distant galactic bulges in the context of well-established trends for pure spheroidal galaxies. Bulges have been isolated for a sample of 137 spiral galaxies in the GOODS fields within the redshift range 0.1 < z < 1.2. Using proven photometric techniques we determine for each galaxy the characteristic parameters (size, surface brightness, profile shape) in the 4 GOODS-ACS imaging bands of both the disk and bulge components. Using the DEIMOS spectrograph on Keck, precision stellar velocity dispersions were secured for a sizeable fraction of the bulges. This has enabled us to compare the Fundamental Plane of our distant bulges with that of field spheroidal galaxies in a similar redshift range. Bulges in spiral galaxies with a bulge-to-total luminosity ratio (B/T) > 0.2 show very similar patterns of evolution to those seen for low luminosity spheroidals. To first order, their recent mass assembly histories are equivalent.
astro-ph
we report on a new study aimed at understanding the diversity and evolutionary properties of distant galactic bulges in the context of wellestablished trends for pure spheroidal galaxies bulges have been isolated for a sample of 137 spiral galaxies in the goods fields within the redshift range 01 z 12 using proven photometric techniques we determine for each galaxy the characteristic parameters size surface brightness profile shape in the 4 goodsacs imaging bands of both the disk and bulge components using the deimos spectrograph on keck precision stellar velocity dispersions were secured for a sizeable fraction of the bulges this has enabled us to compare the fundamental plane of our distant bulges with that of field spheroidal galaxies in a similar redshift range bulges in spiral galaxies with a bulgetototal luminosity ratio bt 02 show very similar patterns of evolution to those seen for low luminosity spheroidals to first order their recent mass assembly histories are equivalent
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709.1738
Symmetrized cut-join equation of Marino-Vafa formula
In this note, we symmetrized the cut-join equation from the proof of Marino-Vafa formula by applying a transcendental changing of variable. One can derive more recursion formulas of Hodge integrals out of this polynomial equations. We also give some applications.
math-ph math.CO math.MP
in this note we symmetrized the cutjoin equation from the proof of marinovafa formula by applying a transcendental changing of variable one can derive more recursion formulas of hodge integrals out of this polynomial equations we also give some applications
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709.1739
Undecidability in function fields of positive characteristic
We prove that the first-order theory of any function field K of characteristic p>2 is undecidable in the language of rings without parameters. When K is a function field in one variable whose constant field is algebraic over a finite field, we can also prove undecidability in characteristic 2. The proof uses a result by Moret-Bailly about ranks of elliptic curves over function fields.
math.NT math.LO
we prove that the firstorder theory of any function field k of characteristic p2 is undecidable in the language of rings without parameters when k is a function field in one variable whose constant field is algebraic over a finite field we can also prove undecidability in characteristic 2 the proof uses a result by moretbailly about ranks of elliptic curves over function fields
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709.174
Addendum to the paper "Two-Dimensional Infinite Prandtl Number Convection: Structure of Bifurcated Solutions, J. Nonlinear Sci., 17(3), 199-220, 2007"
The main objective of this addendum to the mentioned article by Park is to provide some remarks on bifurcation theories for nonlinear partial differential equations (PDE) and their applications to fluid dynamics problems. We only wish to comment and list some related literatures, without any intention to provide a complete survey.
math-ph math.MP
the main objective of this addendum to the mentioned article by park is to provide some remarks on bifurcation theories for nonlinear partial differential equations pde and their applications to fluid dynamics problems we only wish to comment and list some related literatures without any intention to provide a complete survey
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709.1741
How do black holes move, as quantum objects or as classical objects?
Results of a recent study of the transition between quantum and classical behavior are applied to black holes. The study led to a criterion separating quantum from classical behavior on the basis of mass or size, dependent on local effects of cosmic expansion. Application of this criterion to black holes indicates that the motion of smaller black holes will be characteristically quantum mechanical, while the motion of larger black holes must be classical, with a threshold distinguishing these behaviors at a Schwartzschild radius of roughly the size of a nucleon.
physics.gen-ph
results of a recent study of the transition between quantum and classical behavior are applied to black holes the study led to a criterion separating quantum from classical behavior on the basis of mass or size dependent on local effects of cosmic expansion application of this criterion to black holes indicates that the motion of smaller black holes will be characteristically quantum mechanical while the motion of larger black holes must be classical with a threshold distinguishing these behaviors at a schwartzschild radius of roughly the size of a nucleon
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709.1742
Non-semisimple Macdonald polynomials
The paper is mainly devoted to the irreducibility of the polynomial representation of the double affine Hecke algebra for an arbitrary reduced root systems and generic "central charge" q. The technique of intertwiners in the non-semisimple variant is the main tool. We introduce Macdonald's non-semisimple polynomials and use them to analyze the reducibility of the polynomial representation in terms of the affine exponents, counterparts of the classical Coxeter exponents. The focus is on the principal aspects of the technique of intertwiners, including related problems in the theory of reduced decompositions on affine Weyl groups.
math.QA math.RT
the paper is mainly devoted to the irreducibility of the polynomial representation of the double affine hecke algebra for an arbitrary reduced root systems and generic central charge q the technique of intertwiners in the nonsemisimple variant is the main tool we introduce macdonalds nonsemisimple polynomials and use them to analyze the reducibility of the polynomial representation in terms of the affine exponents counterparts of the classical coxeter exponents the focus is on the principal aspects of the technique of intertwiners including related problems in the theory of reduced decompositions on affine weyl groups
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709.1743
Experimental evidence of a natural parity state in $^{26}$Mg and its impact to the production of neutrons for the s process
We have studied natural parity states in $^{26}$Mg via the $^{22}$Ne($^{6}$Li,d)$^{26}$Mg reaction. Our method significantly improves the energy resolution of previous experiments and, as a result, we report the observation of a natural parity state in $^{26}$Mg. Possible spin-parity assignments are suggested on the basis of published $\gamma$-ray decay experiments. The stellar rate of the $^{22}$Ne($\alpha$,$\gamma$)$^{26}$Mg reaction is reduced and may give rise to an increase in the production of s-process neutrons via the $^{22}$Ne($\alpha$,n)$^{25}$Mg reaction.
nucl-ex
we have studied natural parity states in 26mg via the 22ne6lid26mg reaction our method significantly improves the energy resolution of previous experiments and as a result we report the observation of a natural parity state in 26mg possible spinparity assignments are suggested on the basis of published gammaray decay experiments the stellar rate of the 22nealphagamma26mg reaction is reduced and may give rise to an increase in the production of sprocess neutrons via the 22nealphan25mg reaction
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709.1744
Experiments with small helicopter automated landings at unusual attitudes
This paper describes a set of experiments involving small helicopters landing automated landing at unusual attitudes. By leveraging the increased agility of small air vehicles, we show that it is possible to automatically land a small helicopter on surfaces pitched at angles up to 60 degrees. Such maneuvers require considerable agility from the vehicle and its avionics system, and they pose significant technical and safety challenges. Our work builds upon previous activities in human-inspired, high-agility flight for small rotorcraft. However, it was not possible to leverage manual flight test data to extract landing maneuvers due to stringent attitude and position control requirements. Availability of low-cost, local navigation systems requiring no on-board instrumentation has proven particularly important for these experiments to be successful.
cs.RO
this paper describes a set of experiments involving small helicopters landing automated landing at unusual attitudes by leveraging the increased agility of small air vehicles we show that it is possible to automatically land a small helicopter on surfaces pitched at angles up to 60 degrees such maneuvers require considerable agility from the vehicle and its avionics system and they pose significant technical and safety challenges our work builds upon previous activities in humaninspired highagility flight for small rotorcraft however it was not possible to leverage manual flight test data to extract landing maneuvers due to stringent attitude and position control requirements availability of lowcost local navigation systems requiring no onboard instrumentation has proven particularly important for these experiments to be successful
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709.1745
Electromagnetic form factors of the pion and kaon from the instanton vacuum
We investigate the pion and kaon (pi^+, K^+, K^0) electromagnetic form factors in the space-like region: Q^2 ~< 1 GeV, based on the gauged low-energy effective chiral action from the instanton vacuum in the large N_c limit. Explicit flavor SU(3) symmetry breaking is taken into account. The nonlocal contributions turn out to be crucial to reproduce the experimental data. While the pion electromagnetic form factor is in good agreement with the data, the kaon one seems underestimated. We also calculate the electromagnetic charge radii for the pion and kaon: <r^2>_{pi^+}=0.455 fm^2, <r^2>_{K^+}=0.486 fm^2 and <r^2>_{K^0}=-0.055 fm^2 without any adjustable free parameter except for the average instanton size and inter-instanton distance, and they are compatible with the experimental data. The low-energy constant L_9 in the large N_c limit is estimated to be 8.42*10^{-3} from the pion charge radius.
hep-ph
we investigate the pion and kaon pi k k0 electromagnetic form factors in the spacelike region q2 1 gev based on the gauged lowenergy effective chiral action from the instanton vacuum in the large n_c limit explicit flavor su3 symmetry breaking is taken into account the nonlocal contributions turn out to be crucial to reproduce the experimental data while the pion electromagnetic form factor is in good agreement with the data the kaon one seems underestimated we also calculate the electromagnetic charge radii for the pion and kaon r2_pi0455 fm2 r2_k0486 fm2 and r2_k00055 fm2 without any adjustable free parameter except for the average instanton size and interinstanton distance and they are compatible with the experimental data the lowenergy constant l_9 in the large n_c limit is estimated to be 842103 from the pion charge radius
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709.1746
On exit times of Levy-driven Ornstein--Uhlenbeck processes
We prove two martingale identities which involve exit times of Levy-driven Ornstein--Uhlenbeck processes. Using these identities we find an explicit formula for the Laplace transform of the exit time under the assumption that positive jumps of the Levy process are exponentially distributed.
math.PR
we prove two martingale identities which involve exit times of levydriven ornsteinuhlenbeck processes using these identities we find an explicit formula for the laplace transform of the exit time under the assumption that positive jumps of the levy process are exponentially distributed
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709.1747
Bounds on the mixing enhancement for a stirred binary fluid
The Cahn-Hilliard equation describes phase separation in binary liquids. Here we study this equation with spatially-varying sources and stirring, or advection. We specialize to symmetric mixtures and time-independent sources and discuss stirring strategies that homogenize the binary fluid. By measuring fluctuations of the composition away from its mean value, we quantify the amount of homogenization achievable. We find upper and lower bounds on our measure of homogenization using only the Cahn-Hilliard equation and the incompressibility of the advecting flow. We compare these theoretical bounds with numerical simulations for two model flows: the constant flow, and the random-phase sine flow. Using the sine flow as an example, we show how our bounds on composition fluctuations provide a measure of the effectiveness of a given stirring protocol in homogenizing a phase-separating binary fluid.
physics.flu-dyn
the cahnhilliard equation describes phase separation in binary liquids here we study this equation with spatiallyvarying sources and stirring or advection we specialize to symmetric mixtures and timeindependent sources and discuss stirring strategies that homogenize the binary fluid by measuring fluctuations of the composition away from its mean value we quantify the amount of homogenization achievable we find upper and lower bounds on our measure of homogenization using only the cahnhilliard equation and the incompressibility of the advecting flow we compare these theoretical bounds with numerical simulations for two model flows the constant flow and the randomphase sine flow using the sine flow as an example we show how our bounds on composition fluctuations provide a measure of the effectiveness of a given stirring protocol in homogenizing a phaseseparating binary fluid
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709.1748
Heat Transfer in Underground Rail Tunnels
The transfer of heat between the air and surrounding soil in underground tunnels ins investigated, as part of the analysis of environmental conditions in underground rail systems. Using standard turbulent modelling assumptions, flow profiles are obtained in both open tunnels and in the annulus between a tunnel wall and a moving train, from which the heat transfer coefficient between the air and tunnel wall is computed. The radial conduction of heat through the surrounding soil resulting from changes in the temperature of air in the tunnel are determined. An impulse change and an oscillating tunnel air temperature are considered separately. The correlations between fluctuations in heat transfer coefficient and air temperature are found to increase the mean soil temperature. Finally, a model for the coupled evolution of the air and surrounding soil temperature along a tunnel of finite length is given.
physics.flu-dyn
the transfer of heat between the air and surrounding soil in underground tunnels ins investigated as part of the analysis of environmental conditions in underground rail systems using standard turbulent modelling assumptions flow profiles are obtained in both open tunnels and in the annulus between a tunnel wall and a moving train from which the heat transfer coefficient between the air and tunnel wall is computed the radial conduction of heat through the surrounding soil resulting from changes in the temperature of air in the tunnel are determined an impulse change and an oscillating tunnel air temperature are considered separately the correlations between fluctuations in heat transfer coefficient and air temperature are found to increase the mean soil temperature finally a model for the coupled evolution of the air and surrounding soil temperature along a tunnel of finite length is given
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709.1749
General Non-extremal Rotating Charged Godel Black Holes in Minimal Five-Dimensional Gauged Supergravity
We present the general exact solutions for non-extremal rotating charged black holes in the Godel universe of five-dimensional minimal supergravity theory. They are uniquely characterized by four non-trivial parameters, namely the mass $m$, the charge $q$, the Kerr equal rotation parameter $a$, and the Godel parameter $j$. We calculate the conserved energy, angular momenta and charge for the solutions and show that they completely satisfy the first law of black hole thermodynamics. We also study the symmetry and separability of the Hamilton-Jacobi and the massive Klein-Gordon equations in these Einstein-Maxwell-Chern-Simons-Godel black hole backgrounds.
hep-th astro-ph gr-qc hep-ph math-ph math.MP quant-ph
we present the general exact solutions for nonextremal rotating charged black holes in the godel universe of fivedimensional minimal supergravity theory they are uniquely characterized by four nontrivial parameters namely the mass m the charge q the kerr equal rotation parameter a and the godel parameter j we calculate the conserved energy angular momenta and charge for the solutions and show that they completely satisfy the first law of black hole thermodynamics we also study the symmetry and separability of the hamiltonjacobi and the massive kleingordon equations in these einsteinmaxwellchernsimonsgodel black hole backgrounds
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709.175
Mutation-selection balance with recombination: convergence to equilibrium for polynomial selection costs
We study a continuous-time dynamical system that models the evolving distribution of genotypes in an infinite population where genomes may have infinitely many or even a continuum of loci, mutations accumulate along lineages without back-mutation, added mutations reduce fitness, and recombination occurs on a faster time scale than mutation and selection. Some features of the model, such as existence and uniqueness of solutions and convergence to the dynamical system of an approximating sequence of discrete time models, were presented in earlier work by Evans, Steinsaltz, and Wachter for quite general selective costs. Here we study a special case where the selective cost of a genotype with a given accumulation of ancestral mutations from a wild type ancestor is a sum of costs attributable to each individual mutation plus successive interaction contributions from each $k$-tuple of mutations for $k$ up to some finite ``degree''. Using ideas from complex chemical reaction networks and a novel Lyapunov function, we establish that the phenomenon of mutation-selection balance occurs for such selection costs under mild conditions. That is, we show that the dynamical system has a unique equilibrium and that it converges to this equilibrium from all initial conditions.
q-bio.PE math.DS math.PR
we study a continuoustime dynamical system that models the evolving distribution of genotypes in an infinite population where genomes may have infinitely many or even a continuum of loci mutations accumulate along lineages without backmutation added mutations reduce fitness and recombination occurs on a faster time scale than mutation and selection some features of the model such as existence and uniqueness of solutions and convergence to the dynamical system of an approximating sequence of discrete time models were presented in earlier work by evans steinsaltz and wachter for quite general selective costs here we study a special case where the selective cost of a genotype with a given accumulation of ancestral mutations from a wild type ancestor is a sum of costs attributable to each individual mutation plus successive interaction contributions from each ktuple of mutations for k up to some finite degree using ideas from complex chemical reaction networks and a novel lyapunov function we establish that the phenomenon of mutationselection balance occurs for such selection costs under mild conditions that is we show that the dynamical system has a unique equilibrium and that it converges to this equilibrium from all initial conditions
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709.1751
Asymptotics for the Wiener sausage among Poissonian obstacles
We consider the Wiener sausage among Poissonian obstacles. The obstacle is called hard if Brownian motion entering the obstacle is immediately killed, and is called soft if it is killed at certain rate. It is known that Brownian motion conditioned to survive among obstacles is confined in a ball near its starting point. We show the weak law of large numbers, large deviation principle in special cases and the moment asymptotics for the volume of the corresponding Wiener sausage. One of the consequence of our results is that the trajectory of Brownian motion almost fills the confinement ball.
math.PR math-ph math.MP
we consider the wiener sausage among poissonian obstacles the obstacle is called hard if brownian motion entering the obstacle is immediately killed and is called soft if it is killed at certain rate it is known that brownian motion conditioned to survive among obstacles is confined in a ball near its starting point we show the weak law of large numbers large deviation principle in special cases and the moment asymptotics for the volume of the corresponding wiener sausage one of the consequence of our results is that the trajectory of brownian motion almost fills the confinement ball
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709.1752
Transversely Polarized Drell-Yan Process and Soft Gluon Resummation in QCD
We calculate the transverse-momentum $Q_T$ spectrum of the dilepton in the transversely polarized Drell-Yan process on the basis of the factorization theorem in QCD. We take into account universal logarithmically enhanced corrections in edge region of phase space by resumming multiple soft-gluon emissions to all orders in the small $Q_T$ region.
hep-ph
we calculate the transversemomentum q_t spectrum of the dilepton in the transversely polarized drellyan process on the basis of the factorization theorem in qcd we take into account universal logarithmically enhanced corrections in edge region of phase space by resumming multiple softgluon emissions to all orders in the small q_t region
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709.1753
Spectrum and polarization of coherent and incoherent radiation and the LPM effect in oriented single crystal
The spectrum and the circular polarization of radiation from longitudinally polarized high-energy electrons in oriented single crystal are considered using the method which permits inseparable consideration of both the coherent and the incoherent mechanisms of photon emission. The spectral and polarization properties of radiation are obtained and analyzed. It is found that in some part of spectral distribution the influence of multiple scattering (the Landau-Pomeranchuk-Migdal (LPM) effect) attains the order of 7 percent. The same is true for the influence of multiple scattering on the polarization part of the radiation intensity. The degree of circular polarization of total intensity of radiation is found. It is shown that the influence of multiple scattering on the photon polarization is similar to the influence of the LPM effect on the total intensity of radiation: it appears only for relatively low energies of radiating electron and has the order of 1 percent, while at higher energies the crystal field action excludes the LPM effect.
hep-ph
the spectrum and the circular polarization of radiation from longitudinally polarized highenergy electrons in oriented single crystal are considered using the method which permits inseparable consideration of both the coherent and the incoherent mechanisms of photon emission the spectral and polarization properties of radiation are obtained and analyzed it is found that in some part of spectral distribution the influence of multiple scattering the landaupomeranchukmigdal lpm effect attains the order of 7 percent the same is true for the influence of multiple scattering on the polarization part of the radiation intensity the degree of circular polarization of total intensity of radiation is found it is shown that the influence of multiple scattering on the photon polarization is similar to the influence of the lpm effect on the total intensity of radiation it appears only for relatively low energies of radiating electron and has the order of 1 percent while at higher energies the crystal field action excludes the lpm effect
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709.1754
Greybody Factor and Hawking Radiation of Charged Dilatonic Black Holes
The greybody factor and the Hawking temperature for a class of asymptotically flat charged dilatonic black holes are computed by using the low-energy dynamics of scalar fields in the black hole background. In the semi-classical approximation, the Hawking temperature has a good agreement with the one computed from the surface gravity, which is independent of the magnetic (or electric) charges of dilatonic black holes.
hep-th gr-qc
the greybody factor and the hawking temperature for a class of asymptotically flat charged dilatonic black holes are computed by using the lowenergy dynamics of scalar fields in the black hole background in the semiclassical approximation the hawking temperature has a good agreement with the one computed from the surface gravity which is independent of the magnetic or electric charges of dilatonic black holes
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709.1755
Dynamical tunneling in molecules: Quantum routes to energy flow
Dynamical tunneling, introduced in the molecular context, is more than two decades old and refers to phenomena that are classically forbidden but allowed by quantum mechanics. On the other hand the phenomenon of intramolecular vibrational energy redistribution (IVR) has occupied a central place in the field of chemical physics for a much longer period of time. Although the two phenomena seem to be unrelated several studies indicate that dynamical tunneling, in terms of its mechanism and timescales, can have important implications for IVR. Examples include the observation of local mode doublets, clustering of rotational energy levels, and extremely narrow vibrational features in high resolution molecular spectra. Both the phenomena are strongly influenced by the nature of the underlying classical phase space. This work reviews the current state of understanding of dynamical tunneling from the phase space perspective and the consequences for intramolecular vibrational energy flow in polyatomic molecules.
physics.chem-ph nlin.CD
dynamical tunneling introduced in the molecular context is more than two decades old and refers to phenomena that are classically forbidden but allowed by quantum mechanics on the other hand the phenomenon of intramolecular vibrational energy redistribution ivr has occupied a central place in the field of chemical physics for a much longer period of time although the two phenomena seem to be unrelated several studies indicate that dynamical tunneling in terms of its mechanism and timescales can have important implications for ivr examples include the observation of local mode doublets clustering of rotational energy levels and extremely narrow vibrational features in high resolution molecular spectra both the phenomena are strongly influenced by the nature of the underlying classical phase space this work reviews the current state of understanding of dynamical tunneling from the phase space perspective and the consequences for intramolecular vibrational energy flow in polyatomic molecules
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709.1756
Physical Meaning of Hermiticity and Shortcomings of the Composite (Hermitian + non-Hermitian) Quantum Theory of Gunther and Samsonov
In arXiv:0709.0483 Gunther and Samsonov outline a ``generalization'' of quantum mechanics that involves simultaneous consideration of Hermitian and non-Hermitian operators and promises to be ``capable to produce effects beyond those of standard Hermitian quantum mechanics.'' We give a simple physical interpretation of Hermiticity and discuss in detail the shortcomings of the above-mentioned composite quantum theory. In particular, we show that the corresponding ``generalization of measurement theory'' suffers from a dynamical inconsistency and that it is by no means adequate to replace the standard measurement theory.
quant-ph
in arxiv07090483 gunther and samsonov outline a generalization of quantum mechanics that involves simultaneous consideration of hermitian and nonhermitian operators and promises to be capable to produce effects beyond those of standard hermitian quantum mechanics we give a simple physical interpretation of hermiticity and discuss in detail the shortcomings of the abovementioned composite quantum theory in particular we show that the corresponding generalization of measurement theory suffers from a dynamical inconsistency and that it is by no means adequate to replace the standard measurement theory
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709.1757
On the Four Vertex Theorem on planes with radial density $e^{\phi(r)}$
It is showed that on a plane with a radial density the Four Vertex Theorem holds for the class of all simple closed curves if and only if the density is constant. But for the class of simple closed curves that are invariant under a rotation about the origin, the Four Vertex Theorem holds for every radial density.
math.DG
it is showed that on a plane with a radial density the four vertex theorem holds for the class of all simple closed curves if and only if the density is constant but for the class of simple closed curves that are invariant under a rotation about the origin the four vertex theorem holds for every radial density
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709.1758
Difference sets and Polynomials of prime variables
Let \psi(x) be a polynomial with rational coefficients. Suppose that \psi has the positive leading coefficient and zero constant term. Let A be a set of positive integers with the positive upper density. Then there exist x,y\in A and a prime p such that x-y=\psi(p-1). Furthermore, if P be a set of primes with the positive relative upper density, then there exist x,y\in P and a prime p such that x-y=\psi(p-1).
math.NT math.CO
let psix be a polynomial with rational coefficients suppose that psi has the positive leading coefficient and zero constant term let a be a set of positive integers with the positive upper density then there exist xyin a and a prime p such that xypsip1 furthermore if p be a set of primes with the positive relative upper density then there exist xyin p and a prime p such that xypsip1
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709.1759
Two Ferromagnetic Phases in Spin-Fermion Systems
We consider spin-fermion systems which get their magnetic properties from a system of localized magnetic moments being coupled to conducting electrons. The dynamical degrees of freedom are spin-$s$ operators of localized spins and spin-1/2 fermi operators of itinerant electrons. We develop modified spin-wave theory and obtain that system has two ferromagnetic phases. At the characteristic temperature T* the magnetization of itinerant electrons becomes zero, and high temperature ferromagnetic phase (T*<T<T_C) is a phase where only localized electrons give contribution to the magnetization of the system. An anomalous increasing of magnetization below T* is obtained in a good agrement with experimental measurements of the ferromagnetic phase of UGe2.
cond-mat.str-el
we consider spinfermion systems which get their magnetic properties from a system of localized magnetic moments being coupled to conducting electrons the dynamical degrees of freedom are spins operators of localized spins and spin12 fermi operators of itinerant electrons we develop modified spinwave theory and obtain that system has two ferromagnetic phases at the characteristic temperature t the magnetization of itinerant electrons becomes zero and high temperature ferromagnetic phase ttt_c is a phase where only localized electrons give contribution to the magnetization of the system an anomalous increasing of magnetization below t is obtained in a good agrement with experimental measurements of the ferromagnetic phase of uge2
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709.176
Thermal Waves in Irradiated Protoplanetary Disks
Protoplanetary disks are mainly heated by radiation from the central star. Since the incident stellar flux at any radius is sensitive to the disk structure near that location, an unstable feedback may be present. Previous investigations show that the disk would be stable to finite-amplitude temperature perturbations if the vertical height of optical surface is everywhere directly proportional to the gas scale height and if the intercepted fraction of stellar radiation is determined from the local grazing angle. We show that these assumptions may not be generally applicable. Instead, we calculate the quasi-static thermal evolution of irradiated disks by directly integrating the global optical depths to determine the optical surface and the total emitting area-filling factor of surface dust. We show that, in disks with modest mass accretion rates, thermal waves are spontaneously and continually excited in the outer disk, propagate inward through the planet-forming domains, and dissipated at small radii where viscous dissipation is dominant. This state is quasi-periodic over several thermal timescales and its pattern does not depend on the details of the opacity law. The viscous dissipation resulting from higher mass accretion stabilizes this instability such that an approximately steady state is realized throughout the disk. In passive protostellar disks, especially transitional disks, these waves induce significant episodic changes in SEDs, on the time scales of years to decades, because the midplane temperatures can vary by a factor of two between the exposed and shadowed regions. The transitory peaks and troughs in the potential vorticity distribution may also lead to baroclinic instability and excite turbulence in theplanet-forming regions.
astro-ph
protoplanetary disks are mainly heated by radiation from the central star since the incident stellar flux at any radius is sensitive to the disk structure near that location an unstable feedback may be present previous investigations show that the disk would be stable to finiteamplitude temperature perturbations if the vertical height of optical surface is everywhere directly proportional to the gas scale height and if the intercepted fraction of stellar radiation is determined from the local grazing angle we show that these assumptions may not be generally applicable instead we calculate the quasistatic thermal evolution of irradiated disks by directly integrating the global optical depths to determine the optical surface and the total emitting areafilling factor of surface dust we show that in disks with modest mass accretion rates thermal waves are spontaneously and continually excited in the outer disk propagate inward through the planetforming domains and dissipated at small radii where viscous dissipation is dominant this state is quasiperiodic over several thermal timescales and its pattern does not depend on the details of the opacity law the viscous dissipation resulting from higher mass accretion stabilizes this instability such that an approximately steady state is realized throughout the disk in passive protostellar disks especially transitional disks these waves induce significant episodic changes in seds on the time scales of years to decades because the midplane temperatures can vary by a factor of two between the exposed and shadowed regions the transitory peaks and troughs in the potential vorticity distribution may also lead to baroclinic instability and excite turbulence in theplanetforming regions
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709.1761
ZEN2: A narrow J-band search for z~9 Lya emitting galaxies directed towards three lensing clusters
We present the results of a continuing survey to detect Lya emitting galaxies at redshifts z~9: the ZEN ("z equals nine'') survey. We have obtained deep VLT/ISAAC observations in the narrow J-band filter NB119 directed towards three massive lensing clusters: Abell clusters 1689, 1835, and 114. The foreground clusters provide a magnified view of the distant universe and permit a sensitive test for the presence of very high-redshift galaxies. We search for z~9 Lya emitting galaxies displaying a significant narrow-band excess relative to accompanying J-band observations that remain undetected in HST/ACS optical images of each field. No sources consistent with this criterion are detected above the unlensed 90% point-source flux limit of the narrow-band image, F_NB=3.7e-18 ergs/s/cm2. To date, the total coverage of the ZEN survey has sampled a volume at z~9 of approximately 1700 co-moving Mpc3 to a Lya emission luminosity of 1e43 erg/s. We conclude by considering the prospects for detecting z~9 Lya emitting galaxies in light of both observed galaxy properties at z<7 and simulated populations at z>7.
astro-ph
we present the results of a continuing survey to detect lya emitting galaxies at redshifts z9 the zen z equals nine survey we have obtained deep vltisaac observations in the narrow jband filter nb119 directed towards three massive lensing clusters abell clusters 1689 1835 and 114 the foreground clusters provide a magnified view of the distant universe and permit a sensitive test for the presence of very highredshift galaxies we search for z9 lya emitting galaxies displaying a significant narrowband excess relative to accompanying jband observations that remain undetected in hstacs optical images of each field no sources consistent with this criterion are detected above the unlensed 90 pointsource flux limit of the narrowband image f_nb37e18 ergsscm2 to date the total coverage of the zen survey has sampled a volume at z9 of approximately 1700 comoving mpc3 to a lya emission luminosity of 1e43 ergs we conclude by considering the prospects for detecting z9 lya emitting galaxies in light of both observed galaxy properties at z7 and simulated populations at z7
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709.1762
Relative Singularity Categories and Gorenstein-Projective Modules
We introduce the notion of relative singularity category with respect to any self-orthogonal subcategory $\omega$ of an abelian category. We introduce the Frobenius category of $\omega$-Cohen-Macaulay objects, and under some reasonable conditions, we show that the stable category of $\omega$-Cohen-Macaulay objects is triangle-equivalent to the relative singularity category. As applications, we relate the stable category of (unnecessarily finitely-generated) Gorenstein-projective modules with singularity categories of rings. We prove that for a Gorenstein ring, the stable category of Gorenstein-projective modules is compactly generated and its compact objects coincide with finitely-generated Gorenstein-projective modules up to direct summands.
math.RA math.RT
we introduce the notion of relative singularity category with respect to any selforthogonal subcategory omega of an abelian category we introduce the frobenius category of omegacohenmacaulay objects and under some reasonable conditions we show that the stable category of omegacohenmacaulay objects is triangleequivalent to the relative singularity category as applications we relate the stable category of unnecessarily finitelygenerated gorensteinprojective modules with singularity categories of rings we prove that for a gorenstein ring the stable category of gorensteinprojective modules is compactly generated and its compact objects coincide with finitelygenerated gorensteinprojective modules up to direct summands
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709.1763
Magnetic Phase Transitions in One-dimensional Strongly Attractive Three-Component Ultracold Fermions
We investigate the nature of trions, pairing and quantum phase transitions in one-dimensional strongly attractive three-component ultracold fermions in external fields. Exact results for the groundstate energy, critical fields, magnetization and phase diagrams are obtained analytically from the Bethe ansatz solutions. Driven by Zeeman splitting, the system shows exotic phases of trions, bound pairs, a normal Fermi liquid and four mixtures of these states. Particularly, a smooth phase transition from a trionic phase into a pairing phase occurs as the highest hyperfine level separates from the two lower energy levels. In contrast, there is a smooth phase transition from the trionic phase into a normal Fermi liquid as the lowest level separates from the two higher levels.
cond-mat.stat-mech cond-mat.str-el
we investigate the nature of trions pairing and quantum phase transitions in onedimensional strongly attractive threecomponent ultracold fermions in external fields exact results for the groundstate energy critical fields magnetization and phase diagrams are obtained analytically from the bethe ansatz solutions driven by zeeman splitting the system shows exotic phases of trions bound pairs a normal fermi liquid and four mixtures of these states particularly a smooth phase transition from a trionic phase into a pairing phase occurs as the highest hyperfine level separates from the two lower energy levels in contrast there is a smooth phase transition from the trionic phase into a normal fermi liquid as the lowest level separates from the two higher levels
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709.1764
"Slow Light" and "Slow Current"
It is shown that the effect of hole-burning under conditions of coherent population oscillations as well as the light pulse delay in a saturable absorber (a modification of the "slow light" effect) can be interpreted, in a comprehensive way, in terms of {\it intensity spectrum} of the light and {\it intensity-related susceptibility} of the non-linear medium. The physical content of these effects is illustrated by a simple electric circuit with a non-linear resistor which realizes a full analog of the saturable absorber. In this case the effect of hole-burning in the absorption spectrum of the medium is converted in to the effect of hole-burning in the frequency dependence of resistance of the non-linear resistor and the effect of "slow light" -- in to the effect of "slow current".
physics.optics
it is shown that the effect of holeburning under conditions of coherent population oscillations as well as the light pulse delay in a saturable absorber a modification of the slow light effect can be interpreted in a comprehensive way in terms of it intensity spectrum of the light and it intensityrelated susceptibility of the nonlinear medium the physical content of these effects is illustrated by a simple electric circuit with a nonlinear resistor which realizes a full analog of the saturable absorber in this case the effect of holeburning in the absorption spectrum of the medium is converted in to the effect of holeburning in the frequency dependence of resistance of the nonlinear resistor and the effect of slow light in to the effect of slow current
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709.1765
Covariant Calculus for Effective String Theories
A covariant calculus for the construction of effective string theories is developed. Effective string theory, describing quantum string-like excitations in arbitrary dimension, has in the past been constructed using the principles of conformal field theory, but not in a systematic way. Using the freedom of choice of field definition, a particular field definition is made in a systematic way to allow an explicit construction of effective string theories with manifest exact conformal symmetry. The impossibility of a manifestly invariant description of the Polchinski-Strominger Lagrangian is demonstrated and its meaning is explained.
hep-th hep-lat
a covariant calculus for the construction of effective string theories is developed effective string theory describing quantum stringlike excitations in arbitrary dimension has in the past been constructed using the principles of conformal field theory but not in a systematic way using the freedom of choice of field definition a particular field definition is made in a systematic way to allow an explicit construction of effective string theories with manifest exact conformal symmetry the impossibility of a manifestly invariant description of the polchinskistrominger lagrangian is demonstrated and its meaning is explained
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709.1766
Magnetohydrodynamics of Neutrino-Cooled Accretion Tori around a Rotating Black Hole in General Relativity
We present our first numerical results of axisymmetric magnetohydrodynamic simulations for neutrino-cooled accretion tori around rotating black holes in general relativity. We consider tori of mass $\sim 0.1$--0.4$M_{\odot}$ around a black hole of mass $M=4M_{\odot}$ and spin $a=0$--$0.9M$; such systems are candidates for the central engines of gamma-ray bursts (GRBs) formed after the collapse of massive rotating stellar cores and the merger of a black hole and a neutron star. In this paper, we consider the short-term evolution of a torus for a duration of $\approx 60$ ms, focusing on short-hard GRBs. Simulations were performed with a plausible microphysical equation of state that takes into account neutronization, the nuclear statistical equilibrium of a gas of free nucleons and $\alpha$-particles, black body radiation, and a relativistic Fermi gas (neutrinos, electrons, and positrons). Neutrino-emission processes, such as $e^{\pm}$ capture onto free nucleons, $e^{\pm}$ pair annihilation, plasmon decay, and nucleon-nucleon bremsstrahlung are taken into account as cooling processes. Magnetic braking and the magnetorotational instability in the accretion tori play a role in angular momentum redistribution, which causes turbulent motion, resultant shock heating, and mass accretion onto the black hole. The mass accretion rate is found to be $\dot M_* \sim 1$--$10 M_{\odot}$/s, and the shock heating increases the temperature to $\sim 10^{11}$ K. This results in a maximum neutrino emission rate of $L_{\nu}=$ several $\times 10^{53}$ ergs/s and a conversion efficiency $L_{\nu}/\dot M_* c^2$ on the order of a few percent for tori with mass $M_{\rm t} \approx 0.1$--0.4$M_{\odot}$ and for moderately high black hole spins.
astro-ph
we present our first numerical results of axisymmetric magnetohydrodynamic simulations for neutrinocooled accretion tori around rotating black holes in general relativity we consider tori of mass sim 0104m_odot around a black hole of mass m4m_odot and spin a009m such systems are candidates for the central engines of gammaray bursts grbs formed after the collapse of massive rotating stellar cores and the merger of a black hole and a neutron star in this paper we consider the shortterm evolution of a torus for a duration of approx 60 ms focusing on shorthard grbs simulations were performed with a plausible microphysical equation of state that takes into account neutronization the nuclear statistical equilibrium of a gas of free nucleons and alphaparticles black body radiation and a relativistic fermi gas neutrinos electrons and positrons neutrinoemission processes such as epm capture onto free nucleons epm pair annihilation plasmon decay and nucleonnucleon bremsstrahlung are taken into account as cooling processes magnetic braking and the magnetorotational instability in the accretion tori play a role in angular momentum redistribution which causes turbulent motion resultant shock heating and mass accretion onto the black hole the mass accretion rate is found to be dot m_ sim 110 m_odots and the shock heating increases the temperature to sim 1011 k this results in a maximum neutrino emission rate of l_nu several times 1053 ergss and a conversion efficiency l_nudot m_ c2 on the order of a few percent for tori with mass m_rm t approx 0104m_odot and for moderately high black hole spins
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709.1767
K-theory of quiver varieties, q-Fock space and nonsymmetric Macdonald polynomials
We have two constructions of the level-$(0,1)$ irreducible representation of the quantum toroidal algebra of type $A$. One is due to Nakajima and Varagnolo-Vasserot. They constructed the representation on the direct sum of the equivariant K-groups of the quiver varieties of type $\hat{A}$. The other is due to Saito-Takemura-Uglov and Varagnolo-Vasserot. They constructed the representation on the q-deformed Fock space introduced by Kashiwara-Miwa-Stern. In this paper we give an explicit isomorphism between these two constructions. For this purpose we construct simultaneous eigenvectors on the q-Fock space using nonsymmetric Macdonald polynomials. Then the isomorphism is given by corresponding these vectors to the torus fixed points on the quiver varieties.
math.QA math.RT
we have two constructions of the level01 irreducible representation of the quantum toroidal algebra of type a one is due to nakajima and varagnolovasserot they constructed the representation on the direct sum of the equivariant kgroups of the quiver varieties of type hata the other is due to saitotakemurauglov and varagnolovasserot they constructed the representation on the qdeformed fock space introduced by kashiwaramiwastern in this paper we give an explicit isomorphism between these two constructions for this purpose we construct simultaneous eigenvectors on the qfock space using nonsymmetric macdonald polynomials then the isomorphism is given by corresponding these vectors to the torus fixed points on the quiver varieties
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709.1768
Cohomology of $\mathfrak {osp}(1|2)$ acting on linear differential operators on the supercircle $S^{1|1}
We compute the first cohomology spaces $H^1(\mathfrak{osp}(1|2);\mathfrak{D}_{\lambda,\mu})$ ($\lambda, \mu\in\mathbb{R}$) of the Lie superalgebra $\mathfrak{osp}(1|2)$ with coefficients in the superspace $\mathfrak{D}_{\lambda,\mu}$ of linear differential operators acting on weighted densities on the supercircle $S^{1|1}$. The structure of these spaces was conjectured in \cite{gmo}. In fact, we prove here that the situation is a little bit more complicated. (To appear in LMP.)
math.RT
we compute the first cohomology spaces h1mathfrakosp12mathfrakd_lambdamu lambda muinmathbbr of the lie superalgebra mathfrakosp12 with coefficients in the superspace mathfrakd_lambdamu of linear differential operators acting on weighted densities on the supercircle s11 the structure of these spaces was conjectured in citegmo in fact we prove here that the situation is a little bit more complicated to appear in lmp
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709.1769
Feynman integrals and difference equations
We report on the calculation of multi-loop Feynman integrals for single-scale problems by means of difference equations in Mellin space. The solution to these difference equations in terms of harmonic sums can be constructed algorithmically over difference fields, the so-called Pi-Sigma-fields. We test the implementaion of the Mathematica package Sigma on examples from recent higher order perturbative calculations in Quantum Chromodynamics.
math-ph math.MP
we report on the calculation of multiloop feynman integrals for singlescale problems by means of difference equations in mellin space the solution to these difference equations in terms of harmonic sums can be constructed algorithmically over difference fields the socalled pisigmafields we test the implementaion of the mathematica package sigma on examples from recent higher order perturbative calculations in quantum chromodynamics
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709.177
Combining directional light output and ultralow loss in deformed microdisks
A drawback of high-quality modes in optical microdisks is their isotropic light emission characteristics. Here we report a novel, robust, and general mechanism that results in highly directional light emission from those modes. This surprising finding is explained by a combination of wave phenomena (wave localization along unstable periodic ray trajectories) and chaotic ray dynamics in open systems (escape along unstable manifolds). The emission properties originating in the chaotic ray dynamics permit directional light output even from microlasers operating in the common multi-mode regime. We demonstrate our novel mechanism for the limacon billiard family and find directional emission with narrow angular divergence for a significant range of geometries and material parameters.
cond-mat.other nlin.CD physics.optics
a drawback of highquality modes in optical microdisks is their isotropic light emission characteristics here we report a novel robust and general mechanism that results in highly directional light emission from those modes this surprising finding is explained by a combination of wave phenomena wave localization along unstable periodic ray trajectories and chaotic ray dynamics in open systems escape along unstable manifolds the emission properties originating in the chaotic ray dynamics permit directional light output even from microlasers operating in the common multimode regime we demonstrate our novel mechanism for the limacon billiard family and find directional emission with narrow angular divergence for a significant range of geometries and material parameters
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709.1771
Variational local structure estimation for image super-resolution
Super-resolution is an important but difficult problem in image/video processing. If a video sequence or some training set other than the given low-resolution image is available, this kind of extra information can greatly aid in the reconstruction of the high-resolution image. The problem is substantially more difficult with only a single low-resolution image on hand. The image reconstruction methods designed primarily for denoising is insufficient for super-resolution problem in the sense that it tends to oversmooth images with essentially no noise. We propose a new adaptive linear interpolation method based on variational method and inspired by local linear embedding (LLE). The experimental result shows that our method avoids the problem of oversmoothing and preserves image structures well.
cs.CV
superresolution is an important but difficult problem in imagevideo processing if a video sequence or some training set other than the given lowresolution image is available this kind of extra information can greatly aid in the reconstruction of the highresolution image the problem is substantially more difficult with only a single lowresolution image on hand the image reconstruction methods designed primarily for denoising is insufficient for superresolution problem in the sense that it tends to oversmooth images with essentially no noise we propose a new adaptive linear interpolation method based on variational method and inspired by local linear embedding lle the experimental result shows that our method avoids the problem of oversmoothing and preserves image structures well
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709.1772
Isospin Matter in AdS/QCD
We study strange and isospin asymmetric matter in a bottom-up AdS/QCD model. We first consider isospin matter, which has served as a good testing ground for nonperturbative QCD. We calculate the isospin chemical potential dependence of hadronic observables such as the masses and the decay constants of the pseudo-scalar, vector, and axial-vector mesons. We discuss a possibility of the charged pion condensation in the matter within the bottom-up AdS/QCD model. Then, we study the properties of the hadronic observables in strange matter. We calculate the deconfinement temperature in strange and isospin asymmetric matter. One of the interesting results of our study is that the critical temperature at a fixed baryon number density increases when the strangeness chemical potential is introduced. This suggests that if matter undergoes a first-order transition to strange matter, the critical temperature shows a sudden jump at the transition point.
hep-ph hep-th
we study strange and isospin asymmetric matter in a bottomup adsqcd model we first consider isospin matter which has served as a good testing ground for nonperturbative qcd we calculate the isospin chemical potential dependence of hadronic observables such as the masses and the decay constants of the pseudoscalar vector and axialvector mesons we discuss a possibility of the charged pion condensation in the matter within the bottomup adsqcd model then we study the properties of the hadronic observables in strange matter we calculate the deconfinement temperature in strange and isospin asymmetric matter one of the interesting results of our study is that the critical temperature at a fixed baryon number density increases when the strangeness chemical potential is introduced this suggests that if matter undergoes a firstorder transition to strange matter the critical temperature shows a sudden jump at the transition point
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709.1773
Deformation potential dominated phonons in ZnS quantum dots
Strong deformation potential (DP) dominated Raman spectra are reported for quantum confined cubic ZnS nanoclusters under off-resonance conditions allowed only in quantum dots. A flurry of zone boundary phonons is demonstrated in the scattering process. Transverse optic (TO) mode in the multi-phonon process shows only even order overtones suggesting the dominance of a two-phonon process (having large DP value in ZnS) and its integral multiples. Two-phonon TO modes corresponding to A1 and B2 symmetries are also demonstrated under off-resonance conditions which are allowed only in quantum dots.
physics.optics physics.gen-ph
strong deformation potential dp dominated raman spectra are reported for quantum confined cubic zns nanoclusters under offresonance conditions allowed only in quantum dots a flurry of zone boundary phonons is demonstrated in the scattering process transverse optic to mode in the multiphonon process shows only even order overtones suggesting the dominance of a twophonon process having large dp value in zns and its integral multiples twophonon to modes corresponding to a1 and b2 symmetries are also demonstrated under offresonance conditions which are allowed only in quantum dots
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709.1774
A parametrized version of the Borsuk Ulam theorem
The main result of this note is a parametrized version of the Borsuk-Ulam theorem. We show that for a continuous family of Borsuk-Ulam situations, parameterized by points of a compact manifold W, its solution set also depends continuously on the parameter space W. Continuity here means that the solution set supports a homology class which maps onto the fundamental class of W. When W is a subset of Euclidean space, we also show how to construct such a continuous family starting from a family depending in the same way continuously on the points of the boundary of W. This solves a problem related to a conjecture which is relevant for the construction of equilibrium strategies in repeated two-player games with incomplete information. A new method (of independent interest) used in this context is a canonical symmetric squaring construction in Cech homology with coefficients in Z/2Z.
math.AT math.KT
the main result of this note is a parametrized version of the borsukulam theorem we show that for a continuous family of borsukulam situations parameterized by points of a compact manifold w its solution set also depends continuously on the parameter space w continuity here means that the solution set supports a homology class which maps onto the fundamental class of w when w is a subset of euclidean space we also show how to construct such a continuous family starting from a family depending in the same way continuously on the points of the boundary of w this solves a problem related to a conjecture which is relevant for the construction of equilibrium strategies in repeated twoplayer games with incomplete information a new method of independent interest used in this context is a canonical symmetric squaring construction in cech homology with coefficients in z2z
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709.1775
A Review of Target Mass Corrections
With recent advances in the precision of inclusive lepton--nuclear scattering experiments, it has become apparent that comparable improvements are needed in the accuracy of the theoretical analysis tools. In particular, when extracting parton distribution functions in the large-x region, it is crucial to correct the data for effects associated with the nonzero mass of the target. We present here a comprehensive review of these target mass corrections (TMC) to structure functions data, summarizing the relevant formulas for TMCs in electromagnetic and weak processes. We include a full analysis of both hadronic and partonic masses, and trace how these effects appear in the operator product expansion and the factorized parton model formalism, as well as their limitations when applied to data in the x->1 limit. We evaluate the numerical effects of TMCs on various structure functions, and compare fits to data with and without these corrections.
hep-ph
with recent advances in the precision of inclusive leptonnuclear scattering experiments it has become apparent that comparable improvements are needed in the accuracy of the theoretical analysis tools in particular when extracting parton distribution functions in the largex region it is crucial to correct the data for effects associated with the nonzero mass of the target we present here a comprehensive review of these target mass corrections tmc to structure functions data summarizing the relevant formulas for tmcs in electromagnetic and weak processes we include a full analysis of both hadronic and partonic masses and trace how these effects appear in the operator product expansion and the factorized parton model formalism as well as their limitations when applied to data in the x1 limit we evaluate the numerical effects of tmcs on various structure functions and compare fits to data with and without these corrections
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709.1776
Regularity of C^{1} smooth surfaces with prescribed p-mean curvature in the Heisenberg group
We consider a $C^{1}$ smooth surface with prescribed $p$(or $H$)-mean curvature in the 3-dimensional Heisenberg group. Assuming only the prescribed $p$-mean curvature $H\in C^{0},$ we show that any characteristic curve is $C^{2}$ smooth and its (line) curvature equals $-H$ in the nonsingular domain$.$ By introducing characteristic coordinates and invoking the jump formulas along characteristic curves, we can prove that the Legendrian (or horizontal) normal gains one more derivative. Therefore the seed curves are $C^{2}$ smooth. We also obtain the uniqueness of characteristic and seed curves passing through a common point under some mild conditions, respectively. These results can be applied to more general situations.
math.DG math.AP
we consider a c1 smooth surface with prescribed por hmean curvature in the 3dimensional heisenberg group assuming only the prescribed pmean curvature hin c0 we show that any characteristic curve is c2 smooth and its line curvature equals h in the nonsingular domain by introducing characteristic coordinates and invoking the jump formulas along characteristic curves we can prove that the legendrian or horizontal normal gains one more derivative therefore the seed curves are c2 smooth we also obtain the uniqueness of characteristic and seed curves passing through a common point under some mild conditions respectively these results can be applied to more general situations
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709.1777
Compact broadband planar orthomode transducer
We present the design and test results of a compact C-band orthomode transducer which comprises four rectangular probes orthogonally arranged in a circular waveguide, designed to work in the WG13 band. Measurements of the system in the frequency range 4.64 GHz to 7.05 GHz agree very well with simulation results and show a cross-polarisation level below -58 dB, a return loss of about -20 dB, and an insertion loss difference of less than 0.18 dB between the orthogonal polarisation modes across the full waveguide band.
astro-ph
we present the design and test results of a compact cband orthomode transducer which comprises four rectangular probes orthogonally arranged in a circular waveguide designed to work in the wg13 band measurements of the system in the frequency range 464 ghz to 705 ghz agree very well with simulation results and show a crosspolarisation level below 58 db a return loss of about 20 db and an insertion loss difference of less than 018 db between the orthogonal polarisation modes across the full waveguide band
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709.1778
A local homology theory for linearly compact modules
We introduce a local homology theory for linearly compact modules which is in some sense dual to the local cohomology theory of A. Grothendieck. Some basic properties such as the noetherianness, the vanishing and non-vanishing of local homology modules of linearly compact modules are proved. A duality theory between local homology and local cohomology modules of linearly compact modules is developed by using Matlis duality and Macdonald duality. As consequences of the duality theorem we obtain some generalizations of well-known results in the theory of local cohomology for semi-discrete linearly compact modules.
math.AC math.RA
we introduce a local homology theory for linearly compact modules which is in some sense dual to the local cohomology theory of a grothendieck some basic properties such as the noetherianness the vanishing and nonvanishing of local homology modules of linearly compact modules are proved a duality theory between local homology and local cohomology modules of linearly compact modules is developed by using matlis duality and macdonald duality as consequences of the duality theorem we obtain some generalizations of wellknown results in the theory of local cohomology for semidiscrete linearly compact modules
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709.1779
Magnetic properties of the Haldane-gap material NENB
Results of magnetization and high-field ESR studies of the new spin-1 Haldane-chain material [Ni(C2H8N2)2NO2](BF4) (NENB) are reported. A definite signature of the Haldane state in NENB was obtained. From the analysis of the frequency-field dependence of magnetic excitations in NENB, the spin-Hamiltonian parameters were calculated, yielding Delta = 17.4 K, g_parallel = 2.14, D = 7.5 K, and |E| = 0.7 K for the Haldane gap, g factor and the crystal-field anisotropy constants, respectively. The presence of fractional S = 1/2 chain-end states, revealed by ESR and magnetization measurements, is found to be responsible for spin-glass freezing effects. In addition, extra states in the excitation spectrum of NENB have been observed in the vicinity of the Haldane gap, which origin is discussed.
cond-mat.other
results of magnetization and highfield esr studies of the new spin1 haldanechain material nic2h8n22no2bf4 nenb are reported a definite signature of the haldane state in nenb was obtained from the analysis of the frequencyfield dependence of magnetic excitations in nenb the spinhamiltonian parameters were calculated yielding delta 174 k g_parallel 214 d 75 k and e 07 k for the haldane gap g factor and the crystalfield anisotropy constants respectively the presence of fractional s 12 chainend states revealed by esr and magnetization measurements is found to be responsible for spinglass freezing effects in addition extra states in the excitation spectrum of nenb have been observed in the vicinity of the haldane gap which origin is discussed
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709.178
Graphical Quantum Error-Correcting Codes
We introduce a purely graph-theoretical object, namely the coding clique, to construct quantum errorcorrecting codes. Almost all quantum codes constructed so far are stabilizer (additive) codes and the construction of nonadditive codes, which are potentially more efficient, is not as well understood as that of stabilizer codes. Our graphical approach provides a unified and classical way to construct both stabilizer and nonadditive codes. In particular we have explicitly constructed the optimal ((10,24,3)) code and a family of 1-error detecting nonadditive codes with the highest encoding rate so far. In the case of stabilizer codes a thorough search becomes tangible and we have classified all the extremal stabilizer codes up to 8 qubits.
quant-ph
we introduce a purely graphtheoretical object namely the coding clique to construct quantum errorcorrecting codes almost all quantum codes constructed so far are stabilizer additive codes and the construction of nonadditive codes which are potentially more efficient is not as well understood as that of stabilizer codes our graphical approach provides a unified and classical way to construct both stabilizer and nonadditive codes in particular we have explicitly constructed the optimal 10243 code and a family of 1error detecting nonadditive codes with the highest encoding rate so far in the case of stabilizer codes a thorough search becomes tangible and we have classified all the extremal stabilizer codes up to 8 qubits
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709.1781
On scattering of Giant Pulses from the Crab Pulsar: a Scattering Function
Simultaneous dual-frequency observations of giant pulses from the Crab pulsar were performed at the frequencies of 61 and 111 MHz. It is shown that scattering of giant pulses from the Crab pulsar occurs at thick, and not at thin screen.
astro-ph
simultaneous dualfrequency observations of giant pulses from the crab pulsar were performed at the frequencies of 61 and 111 mhz it is shown that scattering of giant pulses from the crab pulsar occurs at thick and not at thin screen
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709.1782
Supersonic dislocations observed in a plasma crystal
Experimental results on the dislocation dynamics in a two-dimensional plasma crystal are presented. Edge dislocations were created in pairs in lattice locations where the internal shear stress exceeded a threshold and then moved apart in the glide plane at a speed higher than the sound speed of shear waves, $C_T$. The experimental system, a plasma crystal, allowed observation of this process at an atomistic (kinetic) level. The early stage of this process is identified as a stacking fault. At a later stage, supersonically moving dislocations generated shear-wave Mach cones.
cond-mat.soft cond-mat.mtrl-sci
experimental results on the dislocation dynamics in a twodimensional plasma crystal are presented edge dislocations were created in pairs in lattice locations where the internal shear stress exceeded a threshold and then moved apart in the glide plane at a speed higher than the sound speed of shear waves c_t the experimental system a plasma crystal allowed observation of this process at an atomistic kinetic level the early stage of this process is identified as a stacking fault at a later stage supersonically moving dislocations generated shearwave mach cones
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709.1783
Wakefield Acceleration by Radiation Pressure in Relativistic Shock Waves
A particle acceleration mechanism by radiation pressure of precursor waves in a relativistic shock is studied. For a relativistic, perpendicular shock with the upstream bulk Lorentz factor of $\gamma_1 \gg 1$, large amplitude electromagnetic (light) waves are known to be excited in the shock front due to the synchrotron maser instability, and those waves can propagate towards upstream as precursor waves. We find that non-thermal, high energy electrons and ions can be quickly produced by an action of electrostatic wakefields generated by the ponderomotive force of the precursor waves. The particles can be quickly accelerated up to $\epsilon_{\rm max}/\gamma_1 m_e c^2 \sim \gamma_1$ in the upstream coherent wakefield region, and they can be further accelerated during the nonlinear stage of the wakefield evolution. The maximum attainable energy is estimated by $\epsilon_{\rm max}/\gamma_1 m_e c^2 \sim L_{\rm sys}/(c/\omega_{pe})$, where $L_{\rm sys}$ and $c/\omega_{pe}$ are the size of an astrophysical object and the electron inertial length, respectively.
astro-ph
a particle acceleration mechanism by radiation pressure of precursor waves in a relativistic shock is studied for a relativistic perpendicular shock with the upstream bulk lorentz factor of gamma_1 gg 1 large amplitude electromagnetic light waves are known to be excited in the shock front due to the synchrotron maser instability and those waves can propagate towards upstream as precursor waves we find that nonthermal high energy electrons and ions can be quickly produced by an action of electrostatic wakefields generated by the ponderomotive force of the precursor waves the particles can be quickly accelerated up to epsilon_rm maxgamma_1 m_e c2 sim gamma_1 in the upstream coherent wakefield region and they can be further accelerated during the nonlinear stage of the wakefield evolution the maximum attainable energy is estimated by epsilon_rm maxgamma_1 m_e c2 sim l_rm syscomega_pe where l_rm sys and comega_pe are the size of an astrophysical object and the electron inertial length respectively
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709.1784
A numerical simulation of the evolution and fate of a FRI jet. The case of 3C 31
The evolution of FRI jets has been long studied in the framework of the FRI-FRII dichotomy. In this paper, we test the present theoretical and observational models via a relativistic numerical simulation of the jets in the radio galaxy 3C 31. We use the parameters derived from the modelling presented by \cite{lb02a,lb02b} as input parameters for the simulation of the evolution of the source, thus assuming that they have not varied over the lifetime of the source. We simulate about 10 % of the total lifetime of the jets in 3C 31. Realistic density and pressure gradients for the atmosphere are used. The simulation includes an equation of state for a two-component relativistic gas that allows a separate treatment of leptonic and baryonic matter. We compare our results with the modelling of the observational data of the source. Our results show that the bow shock evolves self-similarly at a quasi-constant speed, with slight deceleration by the end of the simulation, in agreement with recent X-ray observations that show the presence of bow shocks in FRI sources. The jet expands until it becomes underpressured with respect to the ambient medium, and then recollimates. Subsequent oscillations around pressure equilibrium and generation of standing shocks lead to the mass loading and disruption of the jet flow. We derive an estimate for the minimum age of the source of $t>1. 10^8 \rm{yrs}$, which may imply continuous activity of 3C 31 since the triggering of its activity. The simulation shows that weak CSS sources may be the young counterparts of FRIs. We conclude that the observed properties of the jets in 3C 31 are basically recovered by the standing shock scenario.
astro-ph
the evolution of fri jets has been long studied in the framework of the frifrii dichotomy in this paper we test the present theoretical and observational models via a relativistic numerical simulation of the jets in the radio galaxy 3c 31 we use the parameters derived from the modelling presented by citelb02alb02b as input parameters for the simulation of the evolution of the source thus assuming that they have not varied over the lifetime of the source we simulate about 10 of the total lifetime of the jets in 3c 31 realistic density and pressure gradients for the atmosphere are used the simulation includes an equation of state for a twocomponent relativistic gas that allows a separate treatment of leptonic and baryonic matter we compare our results with the modelling of the observational data of the source our results show that the bow shock evolves selfsimilarly at a quasiconstant speed with slight deceleration by the end of the simulation in agreement with recent xray observations that show the presence of bow shocks in fri sources the jet expands until it becomes underpressured with respect to the ambient medium and then recollimates subsequent oscillations around pressure equilibrium and generation of standing shocks lead to the mass loading and disruption of the jet flow we derive an estimate for the minimum age of the source of t1 108 rmyrs which may imply continuous activity of 3c 31 since the triggering of its activity the simulation shows that weak css sources may be the young counterparts of fris we conclude that the observed properties of the jets in 3c 31 are basically recovered by the standing shock scenario
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709.1785
Storage and Retrieval of a Squeezed Vacuum
Storage and retrieval of a squeezed vacuum was successfully demonstrated using electromagnetically induced transparency. 930ns of the squeezed vacuum pulse was incident on the laser cooled 87Rb atoms with an intense control light in a coherent state. When the squeezed vacuum pulse was slowed and spatially compressed in the cold atoms, the control light was switched off. After 3us of storage, the control light was switched on again and the squeezed vacuum was retrieved, as was confirmed using the time-domain homodyne method.
quant-ph
storage and retrieval of a squeezed vacuum was successfully demonstrated using electromagnetically induced transparency 930ns of the squeezed vacuum pulse was incident on the laser cooled 87rb atoms with an intense control light in a coherent state when the squeezed vacuum pulse was slowed and spatially compressed in the cold atoms the control light was switched off after 3us of storage the control light was switched on again and the squeezed vacuum was retrieved as was confirmed using the timedomain homodyne method
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709.1786
Inflaton Decay in Supergravity and Gravitino Problem
We have recently shown that, if the inflaton has a nonzero vacuum expectation value, it generically couples to any matter fields that appear in the superpotential at the tree level, and to any gauge sectors through anomalies in the supergravity. Through these processes, the inflaton decays into the supersymmetry breaking sector, producing many gravitinos. The inflaton also directly decays into a pair of the gravitinos. Taking account of these processes, we derive constraints on both inflation models and supersymmetry breaking scenarios for avoiding overproduction of the gravitinos.
hep-ph
we have recently shown that if the inflaton has a nonzero vacuum expectation value it generically couples to any matter fields that appear in the superpotential at the tree level and to any gauge sectors through anomalies in the supergravity through these processes the inflaton decays into the supersymmetry breaking sector producing many gravitinos the inflaton also directly decays into a pair of the gravitinos taking account of these processes we derive constraints on both inflation models and supersymmetry breaking scenarios for avoiding overproduction of the gravitinos
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709.1787
Dismantling sparse random graphs
We consider the number of vertices that must be removed from a graph G in order that the remaining subgraph has no component with more than k vertices. Our principal observation is that, if G is a sparse random graph or a random regular graph on n vertices with n tending to infinity, then the number in question is essentially the same for all values of k such that k tends to infinity but k=o(n).
math.CO
we consider the number of vertices that must be removed from a graph g in order that the remaining subgraph has no component with more than k vertices our principal observation is that if g is a sparse random graph or a random regular graph on n vertices with n tending to infinity then the number in question is essentially the same for all values of k such that k tends to infinity but kon
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709.1788
Leonhard Euler and a q-analogue of the logarithm
We study a q-logarithm which was introduced by Euler and give some of its properties. This q-logarithm did not get much attention in the recent literature. We derive basic properties, some of which were already given by Euler in a 1751-paper and 1734-letter to Daniel Bernoulli. The corresponding q-analogue of the dilogarithm is introduced. The relation to the values at 1 and 2 of a q-analogue of the zeta function is given. We briefly describe some other q-logarithms that have appeared in the recent literature.
math.CA math.HO
we study a qlogarithm which was introduced by euler and give some of its properties this qlogarithm did not get much attention in the recent literature we derive basic properties some of which were already given by euler in a 1751paper and 1734letter to daniel bernoulli the corresponding qanalogue of the dilogarithm is introduced the relation to the values at 1 and 2 of a qanalogue of the zeta function is given we briefly describe some other qlogarithms that have appeared in the recent literature
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709.1789
Remarkable virtual SUSY effects in $W^{\pm}$ production at high energy hadron colliders
We present a complete 1-loop study of the electroweak corrections to the process $ug\to dW^+$ in MSSM and SM. The occurrence of a number of remarkable properties in the behavior of the helicity amplitudes at high energies is stressed, and the crucial role of the virtual SUSY contributions in establishing them, is emphasized. The approach to asymptopia of these amplitudes is discussed, comparing the effects of the logarithmic and constant contributions to the mass suppressed ones, which are relevant at lower energies. Applying crossing to $ug\to d W^+$, we obtain all subprocesses needed for the 1-loop electroweak corrections to $W^\pm$-production at LHC. The SUSY model dependence of such a production is then studied, and illustrations are given for the transverse $W^{\pm}$ momentum distribution, as well as the angular distribution in the subprocess center of mass.
hep-ph
we present a complete 1loop study of the electroweak corrections to the process ugto dw in mssm and sm the occurrence of a number of remarkable properties in the behavior of the helicity amplitudes at high energies is stressed and the crucial role of the virtual susy contributions in establishing them is emphasized the approach to asymptopia of these amplitudes is discussed comparing the effects of the logarithmic and constant contributions to the mass suppressed ones which are relevant at lower energies applying crossing to ugto d w we obtain all subprocesses needed for the 1loop electroweak corrections to wpmproduction at lhc the susy model dependence of such a production is then studied and illustrations are given for the transverse wpm momentum distribution as well as the angular distribution in the subprocess center of mass
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709.179
Morphology of flows and buoyant bubbles in the Virgo cluster
There is growing evidence that the active galactic nuclei (AGN) associated with the central elliptical galaxy in clusters of galaxies are playing an important role in the evolution of the intracluster medium (ICM) and clusters themselves. We use high resolution three-dimensional simulations to study the interaction of the cavities created by AGN outflows (bubbles) with the ambient ICM. The gravitational potential of the cluster is modelled using the observed temperature and density profiles of the Virgo cluster. We demonstrate the importance of the hydrodynamical Kutta-Zhukovsky forces associated with the vortex ring structure of the bubbles, and discuss possible effects of diffusive processes on their evolution.
astro-ph
there is growing evidence that the active galactic nuclei agn associated with the central elliptical galaxy in clusters of galaxies are playing an important role in the evolution of the intracluster medium icm and clusters themselves we use high resolution threedimensional simulations to study the interaction of the cavities created by agn outflows bubbles with the ambient icm the gravitational potential of the cluster is modelled using the observed temperature and density profiles of the virgo cluster we demonstrate the importance of the hydrodynamical kuttazhukovsky forces associated with the vortex ring structure of the bubbles and discuss possible effects of diffusive processes on their evolution
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709.1791
Ferroelectricity in artificial bicolor oxide superlattices
We report on the growth and properties of high quality bicolor oxide superlattices, composed of two perovskites out of BaTiO3, CaTiO3, and SrTiO3. The artificially grown superlattices are structurally unique and have a macroscopically homogeneous phase, which is not feasible to recreate in bulk form. By artificial structuring, it is found that the polarization of such superlattices can be highly increased as compared to pseudo-binary ceramics with the same overall composition. Such strong enhancement in superlattice is attributed to newly-developed ionic motions of A-site cations at the hetero-interfaces due to the interfacial coupling of electrostatic and elastic interactions, which cannot be found in single phase materials.
cond-mat.mtrl-sci
we report on the growth and properties of high quality bicolor oxide superlattices composed of two perovskites out of batio3 catio3 and srtio3 the artificially grown superlattices are structurally unique and have a macroscopically homogeneous phase which is not feasible to recreate in bulk form by artificial structuring it is found that the polarization of such superlattices can be highly increased as compared to pseudobinary ceramics with the same overall composition such strong enhancement in superlattice is attributed to newlydeveloped ionic motions of asite cations at the heterointerfaces due to the interfacial coupling of electrostatic and elastic interactions which cannot be found in single phase materials
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709.1792
On the influence of time and space correlations on the next earthquake magnitude
A crucial point in the debate on feasibility of earthquake prediction is the dependence of an earthquake magnitude from past seismicity. Indeed, whilst clustering in time and space is widely accepted, much more questionable is the existence of magnitude correlations. The standard approach generally assumes that magnitudes are independent and therefore in principle unpredictable. Here we show the existence of clustering in magnitude: earthquakes occur with higher probability close in time, space and magnitude to previous events. More precisely, the next earthquake tends to have a magnitude similar but smaller than the previous one. A dynamical scaling relation between magnitude, time and space distances reproduces the complex pattern of magnitude, spatial and temporal correlations observed in experimental seismic catalogs.
physics.geo-ph physics.ins-det
a crucial point in the debate on feasibility of earthquake prediction is the dependence of an earthquake magnitude from past seismicity indeed whilst clustering in time and space is widely accepted much more questionable is the existence of magnitude correlations the standard approach generally assumes that magnitudes are independent and therefore in principle unpredictable here we show the existence of clustering in magnitude earthquakes occur with higher probability close in time space and magnitude to previous events more precisely the next earthquake tends to have a magnitude similar but smaller than the previous one a dynamical scaling relation between magnitude time and space distances reproduces the complex pattern of magnitude spatial and temporal correlations observed in experimental seismic catalogs
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709.1793
Effective dislocation lines in continuously dislocated crystals. I. Material anholonomity
A continuous geometric description of Bravais monocrystals with many dislocations and secondary point defects created by the distribution of these dislocations is proposed. Namely, it is distinguished, basing oneself on Kondo and Kroners Gedanken Experiments for dislocated bodies, an anholonomic triad of linearly independent vector fields. The triad defines local crystallographic directions of the defective crystal as well as a continuous counterpart of the Burgers vector for single dislocations. Next, the influence of secondary point defects on the distribution of many dislocations is modeled by treating these local crystallographic directions as well as Burgers circuits as those located in such a Riemannian material space that becomes an Euclidean 3-manifold when dislocations are absent. Some consequences of this approach are discussed.
math-ph math.MP
a continuous geometric description of bravais monocrystals with many dislocations and secondary point defects created by the distribution of these dislocations is proposed namely it is distinguished basing oneself on kondo and kroners gedanken experiments for dislocated bodies an anholonomic triad of linearly independent vector fields the triad defines local crystallographic directions of the defective crystal as well as a continuous counterpart of the burgers vector for single dislocations next the influence of secondary point defects on the distribution of many dislocations is modeled by treating these local crystallographic directions as well as burgers circuits as those located in such a riemannian material space that becomes an euclidean 3manifold when dislocations are absent some consequences of this approach are discussed
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709.1794
Overlap-free words and spectra of matrices
Overlap-free words are words over the binary alphabet $A=\{a, b\}$ that do not contain factors of the form $xvxvx$, where $x \in A$ and $v \in A^*$. We analyze the asymptotic growth of the number $u_n$ of overlap-free words of length $n$ as $ n \to \infty$. We obtain explicit formulas for the minimal and maximal rates of growth of $u_n$ in terms of spectral characteristics (the lower spectral radius and the joint spectral radius) of certain sets of matrices of dimension $20 \times 20$. Using these descriptions we provide new estimates of the rates of growth that are within 0.4% and $0.03 %$ of their exact values. The best previously known bounds were within 11% and 3% respectively. We then prove that the value of $u_n$ actually has the same rate of growth for ``almost all'' natural numbers $n$. This ``average'' growth is distinct from the maximal and minimal rates and can also be expressed in terms of a spectral quantity (the Lyapunov exponent). We use this expression to estimate it. In order to obtain our estimates, we introduce new algorithms to compute spectral characteristics of sets of matrices. These algorithms can be used in other contexts and are of independent interest.
cs.DM
overlapfree words are words over the binary alphabet aa b that do not contain factors of the form xvxvx where x in a and v in a we analyze the asymptotic growth of the number u_n of overlapfree words of length n as n to infty we obtain explicit formulas for the minimal and maximal rates of growth of u_n in terms of spectral characteristics the lower spectral radius and the joint spectral radius of certain sets of matrices of dimension 20 times 20 using these descriptions we provide new estimates of the rates of growth that are within 04 and 003 of their exact values the best previously known bounds were within 11 and 3 respectively we then prove that the value of u_n actually has the same rate of growth for almost all natural numbers n this average growth is distinct from the maximal and minimal rates and can also be expressed in terms of a spectral quantity the lyapunov exponent we use this expression to estimate it in order to obtain our estimates we introduce new algorithms to compute spectral characteristics of sets of matrices these algorithms can be used in other contexts and are of independent interest
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709.1795
Numerical Simulations of Equatorially-Asymmetric Magnetized Supernovae: Formation of Magnetars and Their Kicks
A series of numerical simulations on magnetorotational core-collapse supernovae are carried out. Dipole-like configurations which are offset northward are assumed for the initially strong magnetic fields together with rapid differential rotations. Aims of our study are to investigate effects of the offset magnetic field on magnetar kicks and on supernova dynamics. Note that we study a regime where the proto-neutron star formed after collapse has a large magnetic field strength approaching that of a ``magnetar'', a highly magnetized slowly rotating neutron star. As a result, equatorially-asymmetric explosions occur with a formation of the bipolar jets. Resultant magnetar's kick velocities are $\sim 300-1000$ km s$^{-1}$. We find that the acceleration is mainly due to the magnetic pressure while the somewhat weaker magnetic tension works toward the opposite direction, which is due to stronger magnetic field in the northern hemisphere. Noted that observations of magnetar's proper motions are very scarce, our results supply a prediction for future observations. Namely, magnetars possibly have large kick velocities, several hundred km s$^{-1}$, as ordinary neutron stars do, and in an extreme case they could have those up to 1000 km s$^{-1}$.
astro-ph
a series of numerical simulations on magnetorotational corecollapse supernovae are carried out dipolelike configurations which are offset northward are assumed for the initially strong magnetic fields together with rapid differential rotations aims of our study are to investigate effects of the offset magnetic field on magnetar kicks and on supernova dynamics note that we study a regime where the protoneutron star formed after collapse has a large magnetic field strength approaching that of a magnetar a highly magnetized slowly rotating neutron star as a result equatoriallyasymmetric explosions occur with a formation of the bipolar jets resultant magnetars kick velocities are sim 3001000 km s1 we find that the acceleration is mainly due to the magnetic pressure while the somewhat weaker magnetic tension works toward the opposite direction which is due to stronger magnetic field in the northern hemisphere noted that observations of magnetars proper motions are very scarce our results supply a prediction for future observations namely magnetars possibly have large kick velocities several hundred km s1 as ordinary neutron stars do and in an extreme case they could have those up to 1000 km s1
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709.1796
Dynamics of buoyant bubbles in clusters of galaxies
We present a phenomenological model of the dynamics of buoyant bubbles in the atmosphere of a cluster of galaxies. The derived equations describe velocity, size, mass, temperature and density of the buoyant bubbles as functions of time based on several simple approximations. The constructed model is then used to interpret results of a numerical experiment of heating of the cluster core with buoyant bubbles in a hydrodynamical approximation (i.e. in the absence of magnetic fields, viscosity, and thermal diffusion). Based on the model parameters we discuss possible limitations of the numerical treatment of the problem, and highlight the main physical processes that govern the dynamics of bubbles in the intracluster medium.
astro-ph
we present a phenomenological model of the dynamics of buoyant bubbles in the atmosphere of a cluster of galaxies the derived equations describe velocity size mass temperature and density of the buoyant bubbles as functions of time based on several simple approximations the constructed model is then used to interpret results of a numerical experiment of heating of the cluster core with buoyant bubbles in a hydrodynamical approximation ie in the absence of magnetic fields viscosity and thermal diffusion based on the model parameters we discuss possible limitations of the numerical treatment of the problem and highlight the main physical processes that govern the dynamics of bubbles in the intracluster medium
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709.1797
Stellar molecular jets traced by maser emission
Highly collimated jets found in AGB and post-AGB stars are expected to play an important role for shaping planetary nebulae. Recent VLBI observations of H2O maser sources have revealed that some of the spatio-kinematical structures of H2O maser sources exhibit stellar jets with extremely spatially and kinematically high collimation. Such stellar H2O maser jets, so-called "water fountain" sources, have been identified in about 10 sources to date. Here we review recent VLBI observations and relevant observational results of the water fountain sources. They have revealed a typical dynamical age and the detailed kinematical structures of the water fountains, possibility of the existence of "equatorial flows", and the evolutionary status of the host stars. The location and kinematics of one of the water fountain sources in the Galaxy is also revealed and shown here.
astro-ph
highly collimated jets found in agb and postagb stars are expected to play an important role for shaping planetary nebulae recent vlbi observations of h2o maser sources have revealed that some of the spatiokinematical structures of h2o maser sources exhibit stellar jets with extremely spatially and kinematically high collimation such stellar h2o maser jets socalled water fountain sources have been identified in about 10 sources to date here we review recent vlbi observations and relevant observational results of the water fountain sources they have revealed a typical dynamical age and the detailed kinematical structures of the water fountains possibility of the existence of equatorial flows and the evolutionary status of the host stars the location and kinematics of one of the water fountain sources in the galaxy is also revealed and shown here
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709.1798
Effective dislocation lines in continuously dislocated crystals. II. Congruences of effective dislocations
The notion of a congruence of effective dislocation lines endowed with the nonvanishing local Burgers vector is introduced. Particularly, the class of congruences of principal Volterra-type effective dislocation lines associated with the dislocation densities (tensorial as well as scalar) is distinguished in order to investigate the geometry of continuized defective crystals in terms of these densities. It is shown that effective dislocation lines can be endowed with the dislocation line tension and with a finite self-energy.
math-ph math.MP
the notion of a congruence of effective dislocation lines endowed with the nonvanishing local burgers vector is introduced particularly the class of congruences of principal volterratype effective dislocation lines associated with the dislocation densities tensorial as well as scalar is distinguished in order to investigate the geometry of continuized defective crystals in terms of these densities it is shown that effective dislocation lines can be endowed with the dislocation line tension and with a finite selfenergy
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709.1799
Symplectically aspherical manifolds
This is a survey article on symplectically aspherical manifolds. The paper contains a discussion on constructions of symplectically aspherical manifolds, their topological properties and the role of this class in symplectic topology. Research perspectives are discussed.
math.SG math.DG
this is a survey article on symplectically aspherical manifolds the paper contains a discussion on constructions of symplectically aspherical manifolds their topological properties and the role of this class in symplectic topology research perspectives are discussed
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709.18
Molecular motors: design, mechanism and control
Biological functions in each animal cell depend on coordinated operations of a wide variety of molecular motors. Some of the these motors transport cargo to their respective destinations whereas some others are mobile workshops which synthesize macromolecules while moving on their tracks. Some other motors are designed to function as packers and movers. All these motors require input energy for performing their mechanical works and operate under conditions far from thermodynamic equilibrium. The typical size of these motors and the forces they generate are of the order of nano-meters and pico-Newtons, respectively. They are subjected to random bombardments by the molecules of the surrounding aqueous medium and, therefore, follow noisy trajectories. Because of their small inertia, their movements in the viscous intracellular space exhibits features that are characteristics of hydrodynamics at low Reynold's number. In this article we discuss how theoretical modeling and computer simulations of these machines by physicists are providing insight into their mechanisms which engineers can exploit to design and control artificial nano-motors.
physics.bio-ph cond-mat.stat-mech physics.pop-ph q-bio.SC
biological functions in each animal cell depend on coordinated operations of a wide variety of molecular motors some of the these motors transport cargo to their respective destinations whereas some others are mobile workshops which synthesize macromolecules while moving on their tracks some other motors are designed to function as packers and movers all these motors require input energy for performing their mechanical works and operate under conditions far from thermodynamic equilibrium the typical size of these motors and the forces they generate are of the order of nanometers and piconewtons respectively they are subjected to random bombardments by the molecules of the surrounding aqueous medium and therefore follow noisy trajectories because of their small inertia their movements in the viscous intracellular space exhibits features that are characteristics of hydrodynamics at low reynolds number in this article we discuss how theoretical modeling and computer simulations of these machines by physicists are providing insight into their mechanisms which engineers can exploit to design and control artificial nanomotors
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709.1801
Campbell equilibrium equation and pseudo-likelihood estimation for non-hereditary Gibbs point processes
In this paper, we study Gibbs point processes involving a hardcore interaction which is not necessarily hereditary. We first extend the famous Campbell equilibrium equation, initially proposed by Nguyen and Zessin [Math. Nachr. 88 (1979) 105--115], to the non-hereditary setting and consequently introduce the new concept of removable points. A modified version of the pseudo-likelihood estimator is then proposed, which involves these removable points. We consider the following two-step estimation procedure: first estimate the hardcore parameter, then estimate the smooth interaction parameter by pseudo-likelihood, where the hardcore parameter estimator is plugged in. We prove the consistency of this procedure in both the hereditary and non-hereditary settings.
math.ST stat.TH
in this paper we study gibbs point processes involving a hardcore interaction which is not necessarily hereditary we first extend the famous campbell equilibrium equation initially proposed by nguyen and zessin math nachr 88 1979 105115 to the nonhereditary setting and consequently introduce the new concept of removable points a modified version of the pseudolikelihood estimator is then proposed which involves these removable points we consider the following twostep estimation procedure first estimate the hardcore parameter then estimate the smooth interaction parameter by pseudolikelihood where the hardcore parameter estimator is plugged in we prove the consistency of this procedure in both the hereditary and nonhereditary settings
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709.1802
Effective dislocation lines in continuously dislocated crystals. III. Kinematics
A class of congruences of principal Volterra-type effective dislocation lines associated with a dislocation density tensor is distinguished in order to investigate the kinematics of continuized defective crystals in terms of their dislocation densities (tensorial as well as scalar). Moreover, it shown, basing oneself on a formula defining the mean curvature of glide surfaces for principal edge effective dislocation lines, that the considered kinematics of continuized defective crystals is consistent with some relations appearing in the physical theory of plasticity (e.g. with the Orowan-type kinematic relations and with the treatment of shear stresses as driving stresses of moving dislocations).
math-ph math.MP
a class of congruences of principal volterratype effective dislocation lines associated with a dislocation density tensor is distinguished in order to investigate the kinematics of continuized defective crystals in terms of their dislocation densities tensorial as well as scalar moreover it shown basing oneself on a formula defining the mean curvature of glide surfaces for principal edge effective dislocation lines that the considered kinematics of continuized defective crystals is consistent with some relations appearing in the physical theory of plasticity eg with the orowantype kinematic relations and with the treatment of shear stresses as driving stresses of moving dislocations
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709.1803
Electron energy spectrum and the Berry phase in graphite bilayer
We emphasize that there exist four Dirac-type points in the electron-energy spectrum of a graphite bilayer near the point K of its Brillouin zone. One of the Dirac points is at the point K, and three Dirac points lie nearby. Each of these three points generates the Berry phase $\pi$, while the Dirac point at K gives the phase $-\pi$. It is these four points that determine the Berry phase in the bilayer. If an electron orbit surrounds all these points, the Berry phase is equal to $2\pi$.
cond-mat.mtrl-sci
we emphasize that there exist four diractype points in the electronenergy spectrum of a graphite bilayer near the point k of its brillouin zone one of the dirac points is at the point k and three dirac points lie nearby each of these three points generates the berry phase pi while the dirac point at k gives the phase pi it is these four points that determine the berry phase in the bilayer if an electron orbit surrounds all these points the berry phase is equal to 2pi
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709.1804
Reproducing the assembly of massive galaxies within the hierarchical cosmogony
In order to gain insight into the physical mechanisms leading to the formation of stars and their assembly in galaxies, we compare the predictions of the MOdel for the Rise of GAlaxies aNd Active nuclei (MORGANA) to the properties of K- and 850 micron-selected galaxies (such as number counts, redshift distributions and luminosity functions) by combining MORGANA with the spectrophotometric model GRASIL. We find that it is possible to reproduce the K- and 850 micron-band datasets at the same time and with a standard Salpeter IMF, and ascribe this success to our improved modeling of cooling in DM halos. We then predict that massively star-forming discs are common at z~2 and dominate the star-formation rate, but most of them merge with other galaxies within ~100 Myr. Our preferred model produces an overabundance of bright galaxies at z<1; this overabundance might be connected to the build-up of the diffuse stellar component in galaxy clusters, as suggested by Monaco et al. (2006), but a naive implementation of the mechanism suggested in that paper does not produce a sufficient slow-down of the evolution of these objects. Moreover, our model over-predicts the number of 10^{10}-10^{11} M_sun galaxies at z~1; this is a common behavior of theoretical models as shown by Fontana et al. (2006). These findings show that, while the overall build-up of the stellar mass is correctly reproduced by galaxy formation models, the ``downsizing'' trend of galaxies is not fully reproduced yet. This hints to some missing feedback mechanism in order to reproduce at the same time the formation of both the massive and the small galaxies.
astro-ph
in order to gain insight into the physical mechanisms leading to the formation of stars and their assembly in galaxies we compare the predictions of the model for the rise of galaxies and active nuclei morgana to the properties of k and 850 micronselected galaxies such as number counts redshift distributions and luminosity functions by combining morgana with the spectrophotometric model grasil we find that it is possible to reproduce the k and 850 micronband datasets at the same time and with a standard salpeter imf and ascribe this success to our improved modeling of cooling in dm halos we then predict that massively starforming discs are common at z2 and dominate the starformation rate but most of them merge with other galaxies within 100 myr our preferred model produces an overabundance of bright galaxies at z1 this overabundance might be connected to the buildup of the diffuse stellar component in galaxy clusters as suggested by monaco et al 2006 but a naive implementation of the mechanism suggested in that paper does not produce a sufficient slowdown of the evolution of these objects moreover our model overpredicts the number of 10101011 m_sun galaxies at z1 this is a common behavior of theoretical models as shown by fontana et al 2006 these findings show that while the overall buildup of the stellar mass is correctly reproduced by galaxy formation models the downsizing trend of galaxies is not fully reproduced yet this hints to some missing feedback mechanism in order to reproduce at the same time the formation of both the massive and the small galaxies
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709.1805
New twist field couplings from the partition function for multiply wrapped D-branes
We consider toroidal compactifications of bosonic string theory with particular regard to the phases (cocycles) necessary for a consistent definition of the vertex operators, the boundary states and the T-duality rules. We use these ingredients to compute the planar multi-loop partition function describing the interaction among magnetized or intersecting D-branes, also in presence of open string moduli. It turns out that unitarity in the open string channel crucially depends on the presence of the cocycles. We then focus on the 2-loop case and study the degeneration limit where this partition function is directly related to the tree-level 3-point correlators between twist fields. These correlators represent the main ingredient in the computation of Yukawa couplings and other terms in the effective action for D-brane phenomenological models. By factorizing the 2-loop partition function we are able to compute the 3-point couplings for abelian twist fields on generic non-factorized tori, thus generalizing previous expressions valid for the 2-torus.
hep-th
we consider toroidal compactifications of bosonic string theory with particular regard to the phases cocycles necessary for a consistent definition of the vertex operators the boundary states and the tduality rules we use these ingredients to compute the planar multiloop partition function describing the interaction among magnetized or intersecting dbranes also in presence of open string moduli it turns out that unitarity in the open string channel crucially depends on the presence of the cocycles we then focus on the 2loop case and study the degeneration limit where this partition function is directly related to the treelevel 3point correlators between twist fields these correlators represent the main ingredient in the computation of yukawa couplings and other terms in the effective action for dbrane phenomenological models by factorizing the 2loop partition function we are able to compute the 3point couplings for abelian twist fields on generic nonfactorized tori thus generalizing previous expressions valid for the 2torus
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709.1806
Initial Helioseismic Observations by Hinode/SOT
Results from initial helioseismic observations by Solar Optical Telescope onboard Hinode are reported. It has been demonstrated that intensity oscillation data from Broadband Filter Imager can be used for various helioseismic analyses. The k-omega power spectra, as well as corresponding time-distance cross-correlation function that promises high-resolution time-distance analysis below 6-Mm travelling distance, were obtained for G-band and CaII-H data. Subsurface supergranular patterns have been observed from our first time-distance analysis. The results show that the solar oscillation spectrum is extended to much higher frequencies and wavenumbers, and the time-distance diagram is extended to much shorter travel distances and times than they were observed before, thus revealing great potential for high-resolution helioseismic observations from Hinode.
astro-ph
results from initial helioseismic observations by solar optical telescope onboard hinode are reported it has been demonstrated that intensity oscillation data from broadband filter imager can be used for various helioseismic analyses the komega power spectra as well as corresponding timedistance crosscorrelation function that promises highresolution timedistance analysis below 6mm travelling distance were obtained for gband and caiih data subsurface supergranular patterns have been observed from our first timedistance analysis the results show that the solar oscillation spectrum is extended to much higher frequencies and wavenumbers and the timedistance diagram is extended to much shorter travel distances and times than they were observed before thus revealing great potential for highresolution helioseismic observations from hinode
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709.1807
Pion-Nucleon Distribution Amplitudes
This is a short presentation of the results for the pion-nucleon distribution amplitudes which are expressed in terms of the nucleon distribution amplitudes with the help of current algebra. Everything is considered to be at threshold.
hep-ph
this is a short presentation of the results for the pionnucleon distribution amplitudes which are expressed in terms of the nucleon distribution amplitudes with the help of current algebra everything is considered to be at threshold
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709.1808
SiPM Development for Astroparticle Physics Applications
The SiPM is a novel solid state photodetector which can be operated in the single photon counting mode. It has excellent features, such as high quantum efficiency, good charge resolution, fast response, very compact size, high gain of 106, very low power consumption, immunity to the magnetic field and low bias voltage (30-70V). Drawbacks of this device currently are a large dark current, crosstalk between micropixels and relatively low sensitivity to UV and blue light. In the last few years, we have developed large size SiPMs (9 mm^2 and 25 mm^2) for applications in the imaging atmospheric Cherenkov telescopes, MAGIC and CTA, and in the space-borne fluorescence telescope EUSO. The current status of the SiPM development by MPI and MEPhI will be presented.
astro-ph
the sipm is a novel solid state photodetector which can be operated in the single photon counting mode it has excellent features such as high quantum efficiency good charge resolution fast response very compact size high gain of 106 very low power consumption immunity to the magnetic field and low bias voltage 3070v drawbacks of this device currently are a large dark current crosstalk between micropixels and relatively low sensitivity to uv and blue light in the last few years we have developed large size sipms 9 mm2 and 25 mm2 for applications in the imaging atmospheric cherenkov telescopes magic and cta and in the spaceborne fluorescence telescope euso the current status of the sipm development by mpi and mephi will be presented
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709.1809
Dynamical response functions in the quantum Ising chain with a boundary
We determine dynamical response functions $<{\cal O}^\dagger(t,x_1){\cal O}(0,x_2)>$ in the scaling limit of the quantum Ising chain on the half line in the presence of a boundary magnetic field. Using a spectral representation in terms of infinite volume form factors and a boundary state, we derive an expansion for the correlator that is found to be rapidly convergent as long as $|\frac{x_1+x_2}{\xi}|\agt 0.2$ where $\xi$ is the correlation length. At sufficiently late times we observe oscillatory behaviour of the correlations arbitrarily far away from the boundary. We investigate the effects of the boundary bound state that is present for a range of boundary magnetic fields.
cond-mat.str-el hep-th
we determine dynamical response functions cal odaggertx_1cal o0x_2 in the scaling limit of the quantum ising chain on the half line in the presence of a boundary magnetic field using a spectral representation in terms of infinite volume form factors and a boundary state we derive an expansion for the correlator that is found to be rapidly convergent as long as fracx_1x_2xiagt 02 where xi is the correlation length at sufficiently late times we observe oscillatory behaviour of the correlations arbitrarily far away from the boundary we investigate the effects of the boundary bound state that is present for a range of boundary magnetic fields
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709.181
Shaping the waveform of entangled photons
We demonstrate experimentally the tunable control of the joint spectrum, i.e. waveform and degree of frequency correlations, of paired photons generated in spontaneous parametric downconversion. This control is mediated by the spatial shape of the pump beam in a type-I noncollinear configuration. We discuss the applicability of this technique to other sources of frequency entangled photons, such as electromagnetically induced Raman transitions.
quant-ph
we demonstrate experimentally the tunable control of the joint spectrum ie waveform and degree of frequency correlations of paired photons generated in spontaneous parametric downconversion this control is mediated by the spatial shape of the pump beam in a typei noncollinear configuration we discuss the applicability of this technique to other sources of frequency entangled photons such as electromagnetically induced raman transitions
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709.1811
Discovery of a galactic wind in the central region of M100
We report the discovery of a galactic wind in the central region of the galaxy M100. This result is based on a careful 2D spectroscopic study performed on observations made with the fibre system INTEGRAL on the WHT. The primary evidence of the wind is the presence of blueshifted interstellar NaD absorption lines. The velocity field of the absorbers show a clear rotation pattern but globally blueshifted ($\sim$ -115 km/s) with respect to the systemic velocity of the galaxy. The emission lines also present a blueward component arising from the ionized gas phase of the galactic wind. The velocity field of the ionized gas wind component shows no evidences of rotation but exhibits a pattern that can be interpreted in terms of the projection of an outflowing cone or shell. The wind component has [NII]/H$\alpha$ ratios of about 1.8, typical of shock ionization. The ionized component of the wind can be identified with an expanding shell of shocked gas, and the neutral component with disk gas entrained in the wind at the interface of the expanding shell with the galactic ISM. The galactic wind seems to be driven uniquely by the nuclear starburst. Our analysis indicates that a non negligible fraction of the wind material might escape to the IGM. In this case, if the wind detected in M100 were representative of similar phenomena in other galaxies with low to moderate activity, the current estimates of metal and dust content of the IGM might be drastically underestimated.
astro-ph
we report the discovery of a galactic wind in the central region of the galaxy m100 this result is based on a careful 2d spectroscopic study performed on observations made with the fibre system integral on the wht the primary evidence of the wind is the presence of blueshifted interstellar nad absorption lines the velocity field of the absorbers show a clear rotation pattern but globally blueshifted sim 115 kms with respect to the systemic velocity of the galaxy the emission lines also present a blueward component arising from the ionized gas phase of the galactic wind the velocity field of the ionized gas wind component shows no evidences of rotation but exhibits a pattern that can be interpreted in terms of the projection of an outflowing cone or shell the wind component has niihalpha ratios of about 18 typical of shock ionization the ionized component of the wind can be identified with an expanding shell of shocked gas and the neutral component with disk gas entrained in the wind at the interface of the expanding shell with the galactic ism the galactic wind seems to be driven uniquely by the nuclear starburst our analysis indicates that a non negligible fraction of the wind material might escape to the igm in this case if the wind detected in m100 were representative of similar phenomena in other galaxies with low to moderate activity the current estimates of metal and dust content of the igm might be drastically underestimated
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709.1812
A Bohr's Semiclassical Model of the Black Hole Thermodynamics
We propose a simple procedure for evaluating the main thermodynamical attributes of a Schwarzschild's black hole: Bekenstein-Hawking entropy, Hawking's temperature and Bekenstein's quantization of the surface area. We make use of the condition that the circumference of a great circle on the black hole horizon contains finite number of the corresponding reduced Compton's wavelength. It is essentially analogous to Bohr's quantization postulate in Bohr's atomic model interpreted by de Broglie's relation. We present black hole radiation in the form conceptually analogous to Bohr's postulate on the photon emission by discrete quantum jump of the electron within the Old quantum theory. It enables us, in accordance with Heisenberg's uncertainty relation and Bohr's correspondence principle, to make a rough estimate of the time interval for black hole evaporation, which turns out very close to time interval predicted by the standard Hawking's theory. Our calculations confirm Bekenstein's semiclassical result for the energy quantization, in variance with Frasca's (2005) calculations. Finally we speculate about the possible source-energy distribution within the black hole horizon.
gr-qc
we propose a simple procedure for evaluating the main thermodynamical attributes of a schwarzschilds black hole bekensteinhawking entropy hawkings temperature and bekensteins quantization of the surface area we make use of the condition that the circumference of a great circle on the black hole horizon contains finite number of the corresponding reduced comptons wavelength it is essentially analogous to bohrs quantization postulate in bohrs atomic model interpreted by de broglies relation we present black hole radiation in the form conceptually analogous to bohrs postulate on the photon emission by discrete quantum jump of the electron within the old quantum theory it enables us in accordance with heisenbergs uncertainty relation and bohrs correspondence principle to make a rough estimate of the time interval for black hole evaporation which turns out very close to time interval predicted by the standard hawkings theory our calculations confirm bekensteins semiclassical result for the energy quantization in variance with frascas 2005 calculations finally we speculate about the possible sourceenergy distribution within the black hole horizon
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709.1813
Enabling electronic prognostics using thermal data
Prognostics is a process of assessing the extent of deviation or degradation of a product from its expected normal operating condition, and then, based on continuous monitoring, predicting the future reliability of the product. By being able to determine when a product will fail, procedures can be developed to provide advanced warning of failures, optimize maintenance, reduce life cycle costs, and improve the design, qualification and logistical support of fielded and future systems. In the case of electronics, the reliability is often influenced by thermal loads, in the form of steady-state temperatures, power cycles, temperature gradients, ramp rates, and dwell times. If one can continuously monitor the thermal loads, in-situ, this data can be used in conjunction with precursor reasoning algorithms and stress-and-damage models to enable prognostics. This paper discusses approaches to enable electronic prognostics and provides a case study of prognostics using thermal data.
cond-mat.mtrl-sci
prognostics is a process of assessing the extent of deviation or degradation of a product from its expected normal operating condition and then based on continuous monitoring predicting the future reliability of the product by being able to determine when a product will fail procedures can be developed to provide advanced warning of failures optimize maintenance reduce life cycle costs and improve the design qualification and logistical support of fielded and future systems in the case of electronics the reliability is often influenced by thermal loads in the form of steadystate temperatures power cycles temperature gradients ramp rates and dwell times if one can continuously monitor the thermal loads insitu this data can be used in conjunction with precursor reasoning algorithms and stressanddamage models to enable prognostics this paper discusses approaches to enable electronic prognostics and provides a case study of prognostics using thermal data
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709.1814
Thermal measurement and modeling of multi-die packages
Thermal measurement and modeling of multi-die packages became a hot topic recently in different fields like RAM chip packaging or LEDs / LED assemblies, resulting in vertical (stacked) and lateral arrangement. In our present study we show results for a mixed arrangement: an opto-coupler device has been investigated with 4 chips in lateral as well as vertical arrangement. In this paper we give an overview of measurement and modeling techniques and results for stacked and MCM structures, describe our present measurement results together with our structure function based methodology of validating the detailed model of the package being studied. Also, we show how to derive junction-to-pin thermal resistances with a technique using structure functions.
cond-mat.mtrl-sci
thermal measurement and modeling of multidie packages became a hot topic recently in different fields like ram chip packaging or leds led assemblies resulting in vertical stacked and lateral arrangement in our present study we show results for a mixed arrangement an optocoupler device has been investigated with 4 chips in lateral as well as vertical arrangement in this paper we give an overview of measurement and modeling techniques and results for stacked and mcm structures describe our present measurement results together with our structure function based methodology of validating the detailed model of the package being studied also we show how to derive junctiontopin thermal resistances with a technique using structure functions
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709.1815
Electrical, thermal and optical characterization of power LED assemblies
Besides their electrical properties the optical parameters of LEDs also depend on junction temperature. For this reason thermal characterization and thermal management play important role in case of power LEDs, necessitating both physical measurements and simulation tools. The focus of this paper is a combined electrical, thermal and optical characterization of power LED assemblies. In terms of simulation a method for board-level electro-thermal simulation is presented, for measurements a combined thermal and radiometric characterization system of power LEDs and LED assemblies is discussed. Comparison of measurement and simulation results is presented in a case study.
cond-mat.mtrl-sci
besides their electrical properties the optical parameters of leds also depend on junction temperature for this reason thermal characterization and thermal management play important role in case of power leds necessitating both physical measurements and simulation tools the focus of this paper is a combined electrical thermal and optical characterization of power led assemblies in terms of simulation a method for boardlevel electrothermal simulation is presented for measurements a combined thermal and radiometric characterization system of power leds and led assemblies is discussed comparison of measurement and simulation results is presented in a case study
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709.1816
Dynamics of hadron strong production and decay
We generalize results of lattice QCD to determine the spin-dependent symmetries and factorization properties of meson production in OZI allowed processes. This explains some conjectures previously made in the literature about axial meson decays and gives predictions for exclusive decays of vector charmonia, including ways of establishing the structure of Y(4260) and Y(4325) from their S-wave decays. Factorization gives a selection rule which forbids $e^+e^- \to D^* D_2$ near threshold with the tensor meson in helicity 2. The relations among amplitudes for double charmonia production $\e^+e^-\to \psi\chi_{0,1,2}$ are expected to differ from the analagous relations among light flavour production such as $\e^+e^-\to \omega f_{0,1,2}$.
hep-ph
we generalize results of lattice qcd to determine the spindependent symmetries and factorization properties of meson production in ozi allowed processes this explains some conjectures previously made in the literature about axial meson decays and gives predictions for exclusive decays of vector charmonia including ways of establishing the structure of y4260 and y4325 from their swave decays factorization gives a selection rule which forbids ee to d d_2 near threshold with the tensor meson in helicity 2 the relations among amplitudes for double charmonia production eeto psichi_012 are expected to differ from the analagous relations among light flavour production such as eeto omega f_012
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709.1817
Thermal Transient Characterization of Packaged Thin Film Microcoolers
A network identification by deconvolution (NID) method is applied to the thermal transient response of packaged and unpackaged microcoolers. A thin film resistor on top of the device is used as the heat source and the temperature sensor. The package and the bonding thermal resistances can be easily identified by comparing structure functions. High-speed coplanar probes are used to achieve a short time resolution of roughly 100ns in the transient temperature response. This is used to separate the thermal properties of the thin film from the substrate. The obtained thermal resistances of the buffer layer and Silicon substrate are consistent with the theoretical calculations. In order to estimate the superlattice thermal resistance and separate it from the thin SiNx layer deposited underneath the thin film resistive sensor, an order of magnitude faster thermal transient response is needed.
cond-mat.mtrl-sci
a network identification by deconvolution nid method is applied to the thermal transient response of packaged and unpackaged microcoolers a thin film resistor on top of the device is used as the heat source and the temperature sensor the package and the bonding thermal resistances can be easily identified by comparing structure functions highspeed coplanar probes are used to achieve a short time resolution of roughly 100ns in the transient temperature response this is used to separate the thermal properties of the thin film from the substrate the obtained thermal resistances of the buffer layer and silicon substrate are consistent with the theoretical calculations in order to estimate the superlattice thermal resistance and separate it from the thin sinx layer deposited underneath the thin film resistive sensor an order of magnitude faster thermal transient response is needed
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709.1818
Dynamic Thermal Analysis of a Power Amplifier
This paper presents dynamic thermal analyses of a power amplifier. All the investigations are based on the transient junction temperature measurements performed during the circuit cooling process. The presented results include the cooling curves, the structure functions, the thermal time constant distribution and the Nyquist plot of the thermal impedance. The experiments carried out demonstrated the influence of the contact resistance and the position of the entire cooling assembly on the obtained results.
cond-mat.mtrl-sci
this paper presents dynamic thermal analyses of a power amplifier all the investigations are based on the transient junction temperature measurements performed during the circuit cooling process the presented results include the cooling curves the structure functions the thermal time constant distribution and the nyquist plot of the thermal impedance the experiments carried out demonstrated the influence of the contact resistance and the position of the entire cooling assembly on the obtained results
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709.1819
Thermal Properties of High Power Laser Bars Investigated by Spatially Resolved Thermoreflectance Spectroscopy
In this work we present results of the analysis of thermal properties of high-power laser bars obtained by spatially resolved thermoreflectance (TR) spectroscopy. Thermoreflectance is a modulation technique relying on periodic facet temperature modulation induced by pulsed current supply of the laser. The periodic temperature change of the laser induces variation of the refractive index and consequently modulates probe beam reflectivity. The technique has a spatial resolution of about ~1 $\mu$m and can be used for temperature mapping over 300 $\mu$m x 300 $\mu$m area. Information obtained in these experiments provide an insight into thermal processes occurring at devices' facets and consequently lead to increased reliability and substantially longer lifetimes of such structures.
cond-mat.mtrl-sci
in this work we present results of the analysis of thermal properties of highpower laser bars obtained by spatially resolved thermoreflectance tr spectroscopy thermoreflectance is a modulation technique relying on periodic facet temperature modulation induced by pulsed current supply of the laser the periodic temperature change of the laser induces variation of the refractive index and consequently modulates probe beam reflectivity the technique has a spatial resolution of about 1 mum and can be used for temperature mapping over 300 mum x 300 mum area information obtained in these experiments provide an insight into thermal processes occurring at devices facets and consequently lead to increased reliability and substantially longer lifetimes of such structures
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709.182
Quantum phase slips in a confined geometry
We consider tunneling of vortices across a superconducting film that is both narrow and short (and connected to bulk superconducting leads at the ends). We find that in the superconducting state the resistance, at low values of the temperature (T) and current, does not follow the power-law dependence on T characteristic of longer samples but is exponential in 1/T. The coefficient of 1/T in the exponent depends on the length or, equivalently, the total normal-state resistance of the sample. These conclusions persist in the one-dimensional limit, which is similar to the problem of quantum phase slips in an ultra-narrow short wire.
cond-mat.supr-con cond-mat.mes-hall
we consider tunneling of vortices across a superconducting film that is both narrow and short and connected to bulk superconducting leads at the ends we find that in the superconducting state the resistance at low values of the temperature t and current does not follow the powerlaw dependence on t characteristic of longer samples but is exponential in 1t the coefficient of 1t in the exponent depends on the length or equivalently the total normalstate resistance of the sample these conclusions persist in the onedimensional limit which is similar to the problem of quantum phase slips in an ultranarrow short wire
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709.1821
Contactless Thermal Characterization Method of PCB-s Using Different IR Sensor Arrays
In this paper the methodology and the results of a quasi real-time thermal characterization tool and method for the temperature mapping of circuits and boards based on sensing the infrared radiation will be introduced. With the proposed method the IR radiation-distribution of boards from the close proximity of the sensor card is monitored in quasi real-time. The proposed method is enabling in situ IR measurement among operating cards of a system e.g. in a rack, enabling the immediate detection of potential hot spots in the system. . The elevated temperature encountered in different packaged electronic devices, like digital processors, high power amplifier, high power switches, etc., demands the application of careful temperature-aware design methodologies and the electro-thermal simulations of PCBs. The results of different electro-thermal simulations and modeling in most of the cases give good approximating results and consider the coupled effects of the real surroundings of these cards and other dissipation elements in an operating system. However the simulation time may take hours, and different systems, different surroundings should be simulated again and again. In our expectation, by using contactless temperature measurement procedure the heat distribution and the places of high dissipation elements on an operating PCB board (PCI or AGP cards in a rack-house of a PC) can be measured and localized in a dense rack system, where only a thin measuring board can be inserted between the cards during operation.
cond-mat.mtrl-sci
in this paper the methodology and the results of a quasi realtime thermal characterization tool and method for the temperature mapping of circuits and boards based on sensing the infrared radiation will be introduced with the proposed method the ir radiationdistribution of boards from the close proximity of the sensor card is monitored in quasi realtime the proposed method is enabling in situ ir measurement among operating cards of a system eg in a rack enabling the immediate detection of potential hot spots in the system the elevated temperature encountered in different packaged electronic devices like digital processors high power amplifier high power switches etc demands the application of careful temperatureaware design methodologies and the electrothermal simulations of pcbs the results of different electrothermal simulations and modeling in most of the cases give good approximating results and consider the coupled effects of the real surroundings of these cards and other dissipation elements in an operating system however the simulation time may take hours and different systems different surroundings should be simulated again and again in our expectation by using contactless temperature measurement procedure the heat distribution and the places of high dissipation elements on an operating pcb board pci or agp cards in a rackhouse of a pc can be measured and localized in a dense rack system where only a thin measuring board can be inserted between the cards during operation
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709.1822
TherMos3, a tool for 3D electrothermal simulation of Smart Power Mosfets
In this paper we report on a novel simulation tool designed for the 3D coupled electro-thermal simulation of Smart Power Mosfets, that is a tool capable of taking into account not only the electrical (and thermal) behaviour of the power device but also the different driving strategies as they are imposed by a control logic circuit which usually resides on the same chip. The simulator is fully developed under Matlab and solves, self consistently, the 3D heat equation with proper boundary conditions and heat sources. An adaptive meshing algorithm based on temperature gradients and an optimized time stepping strategy have also been developed to reduce computational load and speed up simulation time without loosing accuracy. To validate this approach, simulator results are finally compared to experimental data obtained on a commercial Smart Power device used in automotive applications.
cond-mat.mtrl-sci
in this paper we report on a novel simulation tool designed for the 3d coupled electrothermal simulation of smart power mosfets that is a tool capable of taking into account not only the electrical and thermal behaviour of the power device but also the different driving strategies as they are imposed by a control logic circuit which usually resides on the same chip the simulator is fully developed under matlab and solves self consistently the 3d heat equation with proper boundary conditions and heat sources an adaptive meshing algorithm based on temperature gradients and an optimized time stepping strategy have also been developed to reduce computational load and speed up simulation time without loosing accuracy to validate this approach simulator results are finally compared to experimental data obtained on a commercial smart power device used in automotive applications
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709.1823
Performance of the Pierre Auger Observatory Surface Detector
The Surface Detector of the Pierre Auger Observatory will consist of 1600 water Cherenkov tanks sampling ground particles of air showers produced by energetic cosmic rays. The arrival times are obtained from GPS and power is provided by solar panels. The construction of the array is nearly completed and a large number of detectors has been operational for more than three years. In this paper the performance of different components of the detectors are discussed. The accuracy of the signal measurement and the trigger stability are presented. The performance of the solar power system and other hardware, as well as the water purity and its long-term stability are discussed.
astro-ph
the surface detector of the pierre auger observatory will consist of 1600 water cherenkov tanks sampling ground particles of air showers produced by energetic cosmic rays the arrival times are obtained from gps and power is provided by solar panels the construction of the array is nearly completed and a large number of detectors has been operational for more than three years in this paper the performance of different components of the detectors are discussed the accuracy of the signal measurement and the trigger stability are presented the performance of the solar power system and other hardware as well as the water purity and its longterm stability are discussed
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709.1824
Monte Carlo Simulations for NLO Chargino Production at the ILC
We present an extension of the Monte Carlo Event Generator Whizard which includes chargino production at the ILC at NLO. We include photons using both a fixed order and a resummation approach. In the latter, leading higher order corrections are automatically included. We present results for cross sections and event generation for both methods.
hep-ph
we present an extension of the monte carlo event generator whizard which includes chargino production at the ilc at nlo we include photons using both a fixed order and a resummation approach in the latter leading higher order corrections are automatically included we present results for cross sections and event generation for both methods
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709.1825
Cold Atoms and Molecules in Self-Assembled Dipolar Lattices
We study the realization of lattice models, where cold atoms and molecules move as extra particles in a dipolar crystal of trapped polar molecules. The crystal is a self-assembled floating mesoscopic lattice structure with quantum dynamics given by phonons. We show that within an experimentally accessible parameter regime extended Hubbard models with tunable long-range phonon-mediated interactions describe the effective dynamics of dressed particles.
cond-mat.other
we study the realization of lattice models where cold atoms and molecules move as extra particles in a dipolar crystal of trapped polar molecules the crystal is a selfassembled floating mesoscopic lattice structure with quantum dynamics given by phonons we show that within an experimentally accessible parameter regime extended hubbard models with tunable longrange phononmediated interactions describe the effective dynamics of dressed particles
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709.1826
Tropical analysis of plurisubharmonic singularities
Some results on singularities of plurisubharmonic functions are put into the context of tropical mathematics.
math.CV
some results on singularities of plurisubharmonic functions are put into the context of tropical mathematics
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709.1827
On detecting CP violation in a single neutrino oscillation channel at very long baselines
We propose a way of detecting CP violation in a single neutrino oscillation channel at very long baselines (on the order of several thousands of kilometers), given precise knowledge of the smallest mass-squared difference. It is shown that CP violation can be characterized by a shift in $L/E$ of the peak oscillation in the $\nu_e$--$\nu_\mu$ appearance channel, both in vacuum and in matter. In fact, matter effects enhance the shift at a fixed energy. We consider the case in which sub-GeV neutrinos are measured with varying baseline and also the case of a fixed baseline. For the varied baseline, accurate knowledge of the absolute neutrino flux would not be necessary; however, neutrinos must be distinguishable from antineutrinos. For the fixed baseline, it is shown that CP violation can be distinguished if the mixing angle $\theta_{13}$ were known.
hep-ph
we propose a way of detecting cp violation in a single neutrino oscillation channel at very long baselines on the order of several thousands of kilometers given precise knowledge of the smallest masssquared difference it is shown that cp violation can be characterized by a shift in le of the peak oscillation in the nu_enu_mu appearance channel both in vacuum and in matter in fact matter effects enhance the shift at a fixed energy we consider the case in which subgev neutrinos are measured with varying baseline and also the case of a fixed baseline for the varied baseline accurate knowledge of the absolute neutrino flux would not be necessary however neutrinos must be distinguishable from antineutrinos for the fixed baseline it is shown that cp violation can be distinguished if the mixing angle theta_13 were known
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709.1828
One-loop energy-momentum tensor in QED with electric-like background
We have obtained nonperturbative one-loop expressions for the mean energy-momentum tensor and current density of Dirac's field on a constant electric-like background. One of the goals of this calculation is to give a consistent description of back-reaction in such a theory. Two cases of initial states are considered: the vacuum state and the thermal equilibrium state. First, we perform calculations for the vacuum initial state. In the obtained expressions, we separate the contributions due to particle creation and vacuum polarization. The latter contributions are related to the Heisenberg-Euler Lagrangian. Then, we study the case of the thermal initial state. Here, we separate the contributions due to particle creation, vacuum polarization, and the contributions due to the work of the external field on the particles at the initial state. All these contributions are studied in detail, in different regimes of weak and strong fields and low and high temperatures. The obtained results allow us to establish restrictions on the electric field and its duration under which QED with a strong constant electric field is consistent. Under such restrictions, one can neglect the back-reaction of particles created by the electric field. Some of the obtained results generalize the calculations of Heisenberg-Euler for energy density to the case of arbitrary strong electric fields.
hep-th
we have obtained nonperturbative oneloop expressions for the mean energymomentum tensor and current density of diracs field on a constant electriclike background one of the goals of this calculation is to give a consistent description of backreaction in such a theory two cases of initial states are considered the vacuum state and the thermal equilibrium state first we perform calculations for the vacuum initial state in the obtained expressions we separate the contributions due to particle creation and vacuum polarization the latter contributions are related to the heisenbergeuler lagrangian then we study the case of the thermal initial state here we separate the contributions due to particle creation vacuum polarization and the contributions due to the work of the external field on the particles at the initial state all these contributions are studied in detail in different regimes of weak and strong fields and low and high temperatures the obtained results allow us to establish restrictions on the electric field and its duration under which qed with a strong constant electric field is consistent under such restrictions one can neglect the backreaction of particles created by the electric field some of the obtained results generalize the calculations of heisenbergeuler for energy density to the case of arbitrary strong electric fields
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709.1829
Nonlinear mean field Fokker-Planck equations. Application to the chemotaxis of biological populations
We study a general class of nonlinear mean field Fokker-Planck equations in relation with an effective generalized thermodynamical formalism. We show that these equations describe several physical systems such as: chemotaxis of bacterial populations, Bose-Einstein condensation in the canonical ensemble, porous media, generalized Cahn-Hilliard equations, Kuramoto model, BMF model, Burgers equation, Smoluchowski-Poisson system for self-gravitating Brownian particles, Debye-Huckel theory of electrolytes, two-dimensional turbulence... In particular, we show that nonlinear mean field Fokker-Planck equations can provide generalized Keller-Segel models describing the chemotaxis of biological populations. As an example, we introduce a new model of chemotaxis incorporating both effects of anomalous diffusion and exclusion principle (volume filling). Therefore, the notion of generalized thermodynamics can have applications for concrete physical systems. We also consider nonlinear mean field Fokker-Planck equations in phase space and show the passage from the generalized Kramers equation to the generalized Smoluchowski equation in a strong friction limit. Our formalism is simple and illustrated by several explicit examples corresponding to Boltzmann, Tsallis and Fermi-Dirac entropies among others.
cond-mat.stat-mech q-bio.QM
we study a general class of nonlinear mean field fokkerplanck equations in relation with an effective generalized thermodynamical formalism we show that these equations describe several physical systems such as chemotaxis of bacterial populations boseeinstein condensation in the canonical ensemble porous media generalized cahnhilliard equations kuramoto model bmf model burgers equation smoluchowskipoisson system for selfgravitating brownian particles debyehuckel theory of electrolytes twodimensional turbulence in particular we show that nonlinear mean field fokkerplanck equations can provide generalized kellersegel models describing the chemotaxis of biological populations as an example we introduce a new model of chemotaxis incorporating both effects of anomalous diffusion and exclusion principle volume filling therefore the notion of generalized thermodynamics can have applications for concrete physical systems we also consider nonlinear mean field fokkerplanck equations in phase space and show the passage from the generalized kramers equation to the generalized smoluchowski equation in a strong friction limit our formalism is simple and illustrated by several explicit examples corresponding to boltzmann tsallis and fermidirac entropies among others
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709.183
Advanced Compact Thermal Modeling by using VHDL-AMS
This paper presents an improved methodology to generate Compact Thermal Models "CTMs" by using (VHDL-AMS) modeling language. This methodology makes it possible to have Boundary Conditions Independent "BCI" CTMs for multi chip components and systems while taking into account the nonlinear thermal conductivity of semiconductors and other materials.
cond-mat.mtrl-sci
this paper presents an improved methodology to generate compact thermal models ctms by using vhdlams modeling language this methodology makes it possible to have boundary conditions independent bci ctms for multi chip components and systems while taking into account the nonlinear thermal conductivity of semiconductors and other materials
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709.1831
The Hot-Spot Phenomenon and its Countermeasures in Bipolar Power Transistors by Analytical Electro-Thermal Simulation
This communication deals with a theoretical study of the hot spot onset (HSO) in cellular bipolar power transistors. This well-known phenomenon consists of a current crowding within few cells occurring for high power conditions, which significantly decreases the forward safe operating area (FSOA) of the device. The study was performed on a virtual sample by means of a fast, fully analytical electro-thermal simulator operating in the steady state regime and under the condition of imposed input base current. The purpose was to study the dependence of the phenomenon on several thermal and geometrical factors and to test suitable countermeasures able to impinge this phenomenon at higher biases or to completely eliminate it. The power threshold of HSO and its localization within the silicon die were observed as a function of the electrical bias conditions as for instance the collector voltage, the equivalent thermal resistance of the assembling structure underlying the silicon die, the value of the ballasting resistances purposely added in the emitter metal interconnections and the thickness of the copper heat spreader placed on the die top just to the aim of making more uniform the temperature of the silicon surface.
cond-mat.mtrl-sci
this communication deals with a theoretical study of the hot spot onset hso in cellular bipolar power transistors this wellknown phenomenon consists of a current crowding within few cells occurring for high power conditions which significantly decreases the forward safe operating area fsoa of the device the study was performed on a virtual sample by means of a fast fully analytical electrothermal simulator operating in the steady state regime and under the condition of imposed input base current the purpose was to study the dependence of the phenomenon on several thermal and geometrical factors and to test suitable countermeasures able to impinge this phenomenon at higher biases or to completely eliminate it the power threshold of hso and its localization within the silicon die were observed as a function of the electrical bias conditions as for instance the collector voltage the equivalent thermal resistance of the assembling structure underlying the silicon die the value of the ballasting resistances purposely added in the emitter metal interconnections and the thickness of the copper heat spreader placed on the die top just to the aim of making more uniform the temperature of the silicon surface
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709.1832
Ground-state structure of the hydrogen double vacancy on Pd(111)
We determine the ground-state structure of a double vacancy in a hydrogen monolayer on the Pd(111) surface. We represent the double vacancy as a triple vacancy containing one additional hydrogen atom. The potential-energy surface for a hydrogen atom moving in the triple vacancy is obtained by density-functional theory, and the wave function of the fully quantum hydrogen atom is obtained by solving the Schr\"odinger equation. We find that an H atom in a divacancy defect experiences significant quantum effects, and that the ground-state wave function is centered at the hcp site rather than the fcc site normally occupied by H atoms on Pd(111). Our results agree well with scanning tunneling microscopy images.
cond-mat.mtrl-sci
we determine the groundstate structure of a double vacancy in a hydrogen monolayer on the pd111 surface we represent the double vacancy as a triple vacancy containing one additional hydrogen atom the potentialenergy surface for a hydrogen atom moving in the triple vacancy is obtained by densityfunctional theory and the wave function of the fully quantum hydrogen atom is obtained by solving the schrodinger equation we find that an h atom in a divacancy defect experiences significant quantum effects and that the groundstate wave function is centered at the hcp site rather than the fcc site normally occupied by h atoms on pd111 our results agree well with scanning tunneling microscopy images
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709.1833
Dynamical Instability of Laminar Axisymmetric Flow of Perfect Fluid with Stratification
The instability of non-homoentropic axisymmetric flow of perfect fluid with respect to non-axisymmetric infinitesimal perturbations was investigated by numerical integration of hydrodynamical differential equations in two-dimensional approximation. The non-trivial influence of entropy gradient on unstable sound and surface gravity waves was revealed. In particular, both decrease and growth of entropy against the direction of effective gravitational acceleration $g_{eff}$ give rise to growing surface gravity modes which are stable with the same parameters in the case of homoentropic flow. At the same time increment of sound modes either grows monotonically while the rate of entropy decrease against $g_{eff}$ gets higher or vanishes at some values of positive and negative entropy gradient in the basic flow. The calculations have showed also that growing internal gravity modes appear only in the flow unstable to axisymmetric perturbations. At last, the analysis of boundary problem with free boundaries uncovered that's incorrect to set the entropy distribution according to polytropic law with polytropic index different from adiabatic value, since in this case perturbations don't satisfy the free boundary conditions.
astro-ph
the instability of nonhomoentropic axisymmetric flow of perfect fluid with respect to nonaxisymmetric infinitesimal perturbations was investigated by numerical integration of hydrodynamical differential equations in twodimensional approximation the nontrivial influence of entropy gradient on unstable sound and surface gravity waves was revealed in particular both decrease and growth of entropy against the direction of effective gravitational acceleration g_eff give rise to growing surface gravity modes which are stable with the same parameters in the case of homoentropic flow at the same time increment of sound modes either grows monotonically while the rate of entropy decrease against g_eff gets higher or vanishes at some values of positive and negative entropy gradient in the basic flow the calculations have showed also that growing internal gravity modes appear only in the flow unstable to axisymmetric perturbations at last the analysis of boundary problem with free boundaries uncovered thats incorrect to set the entropy distribution according to polytropic law with polytropic index different from adiabatic value since in this case perturbations dont satisfy the free boundary conditions
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709.1834
Thermal Benchmark and Power Benchmark Software
Power consumption and heat dissipation become key elements in the field of high-end integrated circuits, especially those used in mobile and high-speed applications, due to their increase of transistor count and clock frequencies. Dynamic thermal management strategies have been proposed and implemented in order to mitigate heat dissipation. However, there is a lack of a tool that can be used to evaluate DTM strategies and thermal response of real life systems. Therefore, in this paper we introduce and define the concepts of thermal benchmark software and power benchmark software as a software application for run-time system level thermal and power characterization
cond-mat.mtrl-sci
power consumption and heat dissipation become key elements in the field of highend integrated circuits especially those used in mobile and highspeed applications due to their increase of transistor count and clock frequencies dynamic thermal management strategies have been proposed and implemented in order to mitigate heat dissipation however there is a lack of a tool that can be used to evaluate dtm strategies and thermal response of real life systems therefore in this paper we introduce and define the concepts of thermal benchmark software and power benchmark software as a software application for runtime system level thermal and power characterization
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